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		<title>偏微分方程</title>
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		<summary type="html">&lt;p&gt;Ruili：&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;此词条暂由Yuling翻译，未经人工整理和审校，带来阅读不便，请见谅。&lt;br /&gt;
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[[File:Heat.gif|thumb|right|A visualisation of a solution to the two-dimensional [[heat equation]] with temperature represented by the third dimension]]&lt;br /&gt;
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A visualisation of a solution to the two-dimensional [[heat equation with temperature represented by the third dimension]]&lt;br /&gt;
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以三维表示温度的二维热方程解的可视化&lt;br /&gt;
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In [[mathematics]], a '''partial differential equation''' ('''PDE''') is a [[differential equation]] that contains unknown [[Multivariable calculus|multivariable functions]] and their [[partial derivative]]s. PDEs are used to formulate problems involving functions of several variables, and are either solved by hand, or used to create a [[computer model]]. A special case is [[ordinary differential equation]]s (ODEs), which deal with functions of a single variable and their derivatives.&lt;br /&gt;
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In mathematics, a partial differential equation (PDE) is a differential equation that contains unknown multivariable functions and their partial derivatives. PDEs are used to formulate problems involving functions of several variables, and are either solved by hand, or used to create a computer model. A special case is ordinary differential equations (ODEs), which deal with functions of a single variable and their derivatives.&lt;br /&gt;
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在数学中，'''&amp;lt;font color = &amp;quot;#ff8000&amp;quot;&amp;gt; 偏微分方程函数 Partial Differential Equation&amp;lt;/font&amp;gt;'''是包含未知多元函数及其偏导数的微分方程。偏微分方程用于描述涉及多元函数的问题，可以通过人为求解，也可以通过建立计算机模型来求解。常微分方程是偏微分方程一种特殊情况，它处理的是一元函数及其导数。&lt;br /&gt;
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PDEs can be used to describe a wide variety of phenomena such as sound, heat, [[diffusion]], [[electrostatics]], [[Electromagnetism|electrodynamics]], [[fluid dynamics]], [[Elasticity (physics)|elasticity]], [[gravitation]] and [[quantum mechanics]]. These seemingly distinct physical phenomena can be formalised similarly in terms of PDEs. Just as ordinary differential equations often model one-dimensional [[dynamical system]]s, partial differential equations often model [[multidimensional system]]s. PDEs find their generalisation in [[stochastic partial differential equation]]s.&lt;br /&gt;
&lt;br /&gt;
PDEs can be used to describe a wide variety of phenomena such as sound, heat, diffusion, electrostatics, electrodynamics, fluid dynamics, elasticity, gravitation and quantum mechanics. These seemingly distinct physical phenomena can be formalised similarly in terms of PDEs. Just as ordinary differential equations often model one-dimensional dynamical systems, partial differential equations often model multidimensional systems. PDEs find their generalisation in stochastic partial differential equations.&lt;br /&gt;
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偏微分方程可以用来描述各种各样的物理现象，如声音，热量，扩散，静电，电动力学，流体力学，弹性力学，重力和量子力学。这些看起来截然不同的物理现象却可以用类似的偏微分方程来描述。正如常微分方程经常对一维动力系统进行建模一样，偏微分方程经常对多维系统进行建模。随机偏微分方程是偏微分方程的一种推广。&lt;br /&gt;
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== Introduction ==&lt;br /&gt;
引言&lt;br /&gt;
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Partial differential equations (PDEs) are equations that involve rates of change with respect to [[continuous variables]]. For example, the position of a [[rigid body]] is specified by six parameters,&amp;lt;ref&amp;gt;{{Cite book|url=https://books.google.com/books?id=v9PLbcYd9aUC&amp;amp;pg=PA32|title=Modelling and Control of Robot Manipulators|last=Sciavicco|first=Lorenzo|last2=Siciliano|first2=Bruno|date=2001-02-19|publisher=Springer Science &amp;amp; Business Media|isbn=9781852332211|language=en}}&amp;lt;/ref&amp;gt; but the configuration of a [[fluid]] is given by the [[continuous distribution]] of several parameters, such as the [[temperature]], [[pressure]], and so forth. The dynamics for the rigid body take place in a finite-dimensional [[Configuration space (physics)|configuration space]]; the dynamics for the fluid occur in an infinite-dimensional configuration space. This distinction usually makes PDEs much harder to solve than ordinary differential equations (ODEs), but here again, there will be simple solutions for linear problems. Classic domains where PDEs are used include [[acoustics]], [[fluid dynamics]], [[electrodynamics]], and [[heat transfer]].&lt;br /&gt;
&lt;br /&gt;
Partial differential equations (PDEs) are equations that involve rates of change with respect to continuous variables. For example, the position of a rigid body is specified by six parameters, but the configuration of a fluid is given by the continuous distribution of several parameters, such as the temperature, pressure, and so forth. The dynamics for the rigid body take place in a finite-dimensional configuration space; the dynamics for the fluid occur in an infinite-dimensional configuration space. This distinction usually makes PDEs much harder to solve than ordinary differential equations (ODEs), but here again, there will be simple solutions for linear problems. Classic domains where PDEs are used include acoustics, fluid dynamics, electrodynamics, and heat transfer.&lt;br /&gt;
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偏微分方程(简称为PDEs)涉及到方程相对于连续变量的变化率。例如，刚体的位置是由六个参数确定的，而流体的状态是由几个参数的连续分布给出的，如温度、压力等。刚体的动力学过程发生在有限维状态空间中，流体的动力学过程发生在无限维状态空间中。这种区别通常使偏微分方程比常微分方程更难求解，但是线性问题仍然有简单的求解方式。使用偏微分方程的经典领域包括声学、流体力学、电动力学和传热学。&lt;br /&gt;
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A partial differential equation (PDE) for the function {{math|''u''(''x''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;,… ''x&amp;lt;sub&amp;gt;n&amp;lt;/sub&amp;gt;'')}} is an equation of the form&lt;br /&gt;
&lt;br /&gt;
A partial differential equation (PDE) for the function  is an equation of the form&lt;br /&gt;
&lt;br /&gt;
函数 {{math|''u''(''x''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;,… ''x&amp;lt;sub&amp;gt;n&amp;lt;/sub&amp;gt;'')}} 的偏微分方程形式是：&lt;br /&gt;
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: &amp;lt;math&amp;gt;f \left (x_1, \ldots x_n; u, \frac{\partial u}{\partial x_1}, \ldots \frac{\partial u}{\partial x_n}; \frac{\partial^2 u}{\partial x_1 \partial x_1}, \ldots \frac{\partial^2 u}{\partial x_1 \partial x_n}; \ldots \right) = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;f \left (x_1, \ldots x_n; u, \frac{\partial u}{\partial x_1}, \ldots \frac{\partial u}{\partial x_n}; \frac{\partial^2 u}{\partial x_1 \partial x_1}, \ldots \frac{\partial^2 u}{\partial x_1 \partial x_n}; \ldots \right) = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
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If {{mvar|f}} is a [[linear function]] of {{mvar|u}} and its derivatives, then the PDE is called linear. Common examples of linear PDEs include the [[heat equation]], the [[wave equation]], [[Laplace's equation]], [[Helmholtz equation]], [[Klein–Gordon equation]], and [[Poisson's equation]].&lt;br /&gt;
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If  is a linear function of  and its derivatives, then the PDE is called linear. Common examples of linear PDEs include the heat equation, the wave equation, Laplace's equation, Helmholtz equation, Klein–Gordon equation, and Poisson's equation.&lt;br /&gt;
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如果 {{mvar|f}} 是函数 {{math|''u''}} 及其导数的线性函数，则偏微分方程称为线性函数。线性偏微分方程的常见例子包括热方程、波动方程、拉普拉斯方程、亥姆霍兹方程方程、克莱因-高登方程和泊松方程。&lt;br /&gt;
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A relatively simple PDE is&lt;br /&gt;
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A relatively simple PDE is&lt;br /&gt;
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一个相对简单的偏微分方程：&lt;br /&gt;
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: &amp;lt;math&amp;gt;\frac{\partial u}{\partial x}(x,y) = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;\frac{\partial u}{\partial x}(x,y) = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
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This relation [[Logical implication|implies]] that the function {{math|''u''(''x'',''y'')}} is independent of {{mvar|x}}. However, the equation gives no information on the function's dependence on the variable {{mvar|y}}. Hence the general solution of this equation is&lt;br /&gt;
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This relation implies that the function  is independent of . However, the equation gives no information on the function's dependence on the variable . Hence the general solution of this equation is&lt;br /&gt;
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这意味着函数 {{math|''u''(''x'',''y'')}} 独立于 {{mvar|x}} 的。然而，这个方程没有给出关于函数和自变量的相关性的信息。因此，这个方程的通解是&lt;br /&gt;
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: &amp;lt;math&amp;gt;u(x,y) = f(y),&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;u(x,y) = f(y),&amp;lt;/math&amp;gt;&lt;br /&gt;
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where {{mvar|f}} is an arbitrary function of {{mvar|y}}. The analogous ordinary differential equation is&lt;br /&gt;
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where  is an arbitrary function of . The analogous ordinary differential equation is&lt;br /&gt;
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其中， {{mvar|f}} 是 {{mvar|y}} 的任意函数。&lt;br /&gt;
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类似的常微分方程是：&lt;br /&gt;
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: &amp;lt;math&amp;gt;\frac{\mathrm{d} u}{\mathrm{d} x}(x) = 0,&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;\frac{\mathrm{d} u}{\mathrm{d} x}(x) = 0,&amp;lt;/math&amp;gt;&lt;br /&gt;
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which has the solution&lt;br /&gt;
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which has the solution&lt;br /&gt;
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它的解为&lt;br /&gt;
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: &amp;lt;math&amp;gt;u(x) = c,&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;u(x) = c,&amp;lt;/math&amp;gt;&lt;br /&gt;
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where {{mvar|c}} is any [[Constant (mathematics)|constant]] value. These two examples illustrate that general solutions of ordinary differential equations (ODEs) involve arbitrary constants, but solutions of PDEs involve arbitrary functions.&lt;br /&gt;
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where  is any constant value. These two examples illustrate that general solutions of ordinary differential equations (ODEs) involve arbitrary constants, but solutions of PDEs involve arbitrary functions.&lt;br /&gt;
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这里，{{mvar|c}} 是一个任意常量。&lt;br /&gt;
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这两个例子说明常微分方程的一般解包含任意常数，但偏微分方程的解包含任意函数。&lt;br /&gt;
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A solution of a PDE is generally not [[Uniqueness quantification|unique]]; additional conditions must generally be specified on the [[Boundary (topology)|boundary]] of the region where the solution is defined. For instance, in the simple example above, the function {{math|''f''(''y'')}} can be determined if {{mvar|u}} is specified on the line {{math|''x'' {{=}} 0}}.&lt;br /&gt;
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A solution of a PDE is generally not unique; additional conditions must generally be specified on the boundary of the region where the solution is defined. For instance, in the simple example above, the function  can be determined if  is specified on the line  0}}.&lt;br /&gt;
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偏微分方程的解一般不是唯一的; 一般必须在定义解的区域边界上定义附加条件。 例如，在上面的简单示例中，如果在 {{math|''x'' {{=}} 0}} 时确定了 {{mvar|u}} 的值，则可以确定该函数 {{math|''f''(''y'')}}。&lt;br /&gt;
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== Existence and uniqueness ==&lt;br /&gt;
存在性和唯一性&lt;br /&gt;
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Although the issue of existence and uniqueness of solutions of ordinary differential equations has a very satisfactory answer with the [[Picard–Lindelöf theorem]], that is far from the case for partial differential equations. The [[Cauchy–Kowalevski theorem]] states that the [[Cauchy problem]] for any partial differential equation whose coefficients are [[Analytic function|analytic]] in the unknown function and its derivatives, has a locally unique analytic solution. Although this result might appear to settle the existence and uniqueness of solutions, there are examples of linear partial differential equations whose coefficients have derivatives of all orders (which are nevertheless not analytic) but which have no solutions at all: see [[Lewy's example|Lewy (1957)]]. Even if the solution of a partial differential equation exists and is unique, it may nevertheless have undesirable properties.  The mathematical study of these questions is usually in the more powerful context of [[weak solution]]s.&lt;br /&gt;
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Although the issue of existence and uniqueness of solutions of ordinary differential equations has a very satisfactory answer with the Picard–Lindelöf theorem, that is far from the case for partial differential equations. The Cauchy–Kowalevski theorem states that the Cauchy problem for any partial differential equation whose coefficients are analytic in the unknown function and its derivatives, has a locally unique analytic solution. Although this result might appear to settle the existence and uniqueness of solutions, there are examples of linear partial differential equations whose coefficients have derivatives of all orders (which are nevertheless not analytic) but which have no solutions at all: see Lewy (1957). Even if the solution of a partial differential equation exists and is unique, it may nevertheless have undesirable properties.  The mathematical study of these questions is usually in the more powerful context of weak solutions.&lt;br /&gt;
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尽管常微分方程解的存在性和唯一性用'''&amp;lt;font color=&amp;quot;#ff8000&amp;quot;&amp;gt;弗罗贝尼乌斯定理 Picard–Lindelöf Theorem&amp;lt;/font&amp;gt;得到了令人满意的结果，但偏微分方程解的存在性和唯一性却远没有得到解决。'''&amp;lt;font color=&amp;quot;#ff8000&amp;quot;&amp;gt;柯西-科瓦列夫斯基定理 Cauchy–Kowalevski theorem&amp;lt;/font&amp;gt;指出：对于任意系数在未知函数及其导数中解析的偏微分方程，柯西问题存在一个局部唯一的解析解。虽然这个结果似乎解决了解的存在性和唯一性问题，但是存在一些线性偏微分方程-其系数具有所有级数的导数(尽管这些导数不是解析的) ，但是根本没有解: 见 Lewy (1957)。即使偏微分方程的解存在且唯一，它仍然可能具有不可预料的性质。这些问题的数学研究通常是在更有力的弱解的背景下进行的。&lt;br /&gt;
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An example of pathological behavior is the sequence (depending upon {{mvar|n}}) of [[Cauchy problem]]s for the [[Laplace equation]]&lt;br /&gt;
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An example of pathological behavior is the sequence (depending upon ) of Cauchy problems for the Laplace equation&lt;br /&gt;
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反常特征的一个例子是拉普拉斯方程的柯西问题的序列(取决于{{mvar|n}})&lt;br /&gt;
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: &amp;lt;math&amp;gt;\frac{\partial^2 u}{\partial x^2} + \frac{\partial^2 u}{\partial y^2}=0,&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;\frac{\partial^2 u}{\partial x^2} + \frac{\partial^2 u}{\partial y^2}=0,&amp;lt;/math&amp;gt;&lt;br /&gt;
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with [[boundary condition]]s&lt;br /&gt;
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with boundary conditions&lt;br /&gt;
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具有边界条件&lt;br /&gt;
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: &amp;lt;math&amp;gt;\begin{align} u(x,0) &amp;amp;= 0, \\ \frac{\partial u}{\partial y}(x,0) &amp;amp;= \frac{\sin nx}{n}, \end{align}&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;\begin{align} u(x,0) &amp;amp;= 0, \\ \frac{\partial u}{\partial y}(x,0) &amp;amp;= \frac{\sin nx}{n}, \end{align}&amp;lt;/math&amp;gt;&lt;br /&gt;
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where {{mvar|n}} is an integer. The derivative of {{mvar|u}} with respect to {{mvar|y}} approaches zero [[uniform convergence|uniformly]] in {{mvar|x}} as {{mvar|n}} increases, but the solution is&lt;br /&gt;
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where  is an integer. The derivative of  with respect to  approaches zero uniformly in  as  increases, but the solution is&lt;br /&gt;
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其中 {{mvar|n}} 是整数。{{mvar|u}} 关于 {{mvar|y}} 的导数，一致地随着 {{mvar|n}} 的增加而趋于零，但解是&lt;br /&gt;
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: &amp;lt;math&amp;gt;u(x,y) = \frac{\sinh ny \sin nx}{n^2}.&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;u(x,y) = \frac{\sinh ny \sin nx}{n^2}.&amp;lt;/math&amp;gt;&lt;br /&gt;
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This solution approaches infinity if {{mvar|nx}} is not an integer multiple of {{pi}} for any non-zero value of {{mvar|y}}. The Cauchy problem for the Laplace equation is called ''ill-posed'' or ''not [[Well-posed problem|well-posed]]'', since the solution does not continuously depend on the data of the problem. Such ill-posed problems are not usually satisfactory for physical applications.&lt;br /&gt;
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This solution approaches infinity if  is not an integer multiple of  for any non-zero value of . The Cauchy problem for the Laplace equation is called ill-posed or not well-posed, since the solution does not continuously depend on the data of the problem. Such ill-posed problems are not usually satisfactory for physical applications.&lt;br /&gt;
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对于任何非零的 {{mvar|y}}，如果 {{mvar|nx}} 不是模板 {{pi}} 的整数倍，这个解会接近于无穷大。拉普拉斯方程的柯西问题被称为不适定的（可以译为ill-posed或not well-posed），因为解不是连续地依赖于问题的数据。这种不适定问题通常不能满足物理应用。&lt;br /&gt;
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The [[Navier–Stokes existence and smoothness|existence of solutions for the Navier–Stokes equations]], a partial differential equation, is part of one of the [[Millennium Prize Problems]].&lt;br /&gt;
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The existence of solutions for the Navier–Stokes equations, a partial differential equation, is part of one of the Millennium Prize Problems.&lt;br /&gt;
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偏微分方程”纳维-斯托克斯方程“的解的存在性就是千禧年大奖难题之一的一部分。&lt;br /&gt;
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== Notation ==&lt;br /&gt;
符号&lt;br /&gt;
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In PDEs, it is common to denote partial derivatives using subscripts. That is:&lt;br /&gt;
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In PDEs, it is common to denote partial derivatives using subscripts. That is:&lt;br /&gt;
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在偏微分方程中，通常用下标表示偏导数。例如:&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt;u_x = \frac{\partial u}{\partial x}&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;u_x = \frac{\partial u}{\partial x}&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt;u_{xx} = \frac{\partial^2 u}{\partial x^2} &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;u_{xx} = \frac{\partial^2 u}{\partial x^2} &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
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: &amp;lt;math&amp;gt;u_{xy} = \frac{\partial^2 u}{\partial y\, \partial x} = \frac{\partial}{\partial y } \left(\frac{\partial u}{\partial x}\right). &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;u_{xy} = \frac{\partial^2 u}{\partial y\, \partial x} = \frac{\partial}{\partial y } \left(\frac{\partial u}{\partial x}\right). &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Especially in physics, [[del]] or nabla ({{math|∇}}) is often used to denote spatial derivatives, and {{math|''&amp;amp;#x307;u'', ''ü''}} for time derivatives. For example, the [[wave equation]] (mentioned below) can be written as&lt;br /&gt;
&lt;br /&gt;
Especially in physics, del or nabla () is often used to denote spatial derivatives, and  for time derivatives. For example, the wave equation (mentioned below) can be written as&lt;br /&gt;
&lt;br /&gt;
特别是在物理学中，[[del]] 或 nabla ({{math|∇}}) 经常用来表示空间导数和时间导数。例如，波动方程(在下文中提到)可以写成：&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt;\ddot u=c^2\nabla^2u&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt;\ddot u=c^2\nabla^2u&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
or&lt;br /&gt;
&lt;br /&gt;
or&lt;br /&gt;
&lt;br /&gt;
或&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt;\ddot u=c^2\Delta u&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt;\ddot u=c^2\Delta u&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
where {{math|Δ}} is the [[Laplace operator]].&lt;br /&gt;
&lt;br /&gt;
where  is the Laplace operator.&lt;br /&gt;
&lt;br /&gt;
其中，{{math|Δ}} 代表拉普拉斯算子。&lt;br /&gt;
&lt;br /&gt;
== Classification ==&lt;br /&gt;
分类&lt;br /&gt;
&lt;br /&gt;
Some linear, second-order partial differential equations can be classified as [[parabolic partial differential equation|parabolic]], [[hyperbolic partial differential equation|hyperbolic]] and [[elliptic partial differential equation|elliptic]]. Others, such as the [[Euler–Tricomi equation]], have different types in different regions. The classification provides a guide to appropriate initial and boundary conditions and to the smoothness of the solutions.&lt;br /&gt;
&lt;br /&gt;
Some linear, second-order partial differential equations can be classified as parabolic, hyperbolic and elliptic. Others, such as the Euler–Tricomi equation, have different types in different regions. The classification provides a guide to appropriate initial and boundary conditions and to the smoothness of the solutions.&lt;br /&gt;
&lt;br /&gt;
一些线性二阶偏微分方程可分为抛物型方程、双曲型方程和椭圆型方程。其他的方程，如欧拉-特里科米方程，在不同的领域有不同的类型。这种分类有助于选择适当的初始和边界条件以及提高解的平滑性。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
=== Equations of first order ===&lt;br /&gt;
一阶方程&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{{main|First-order partial differential equation}}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
=== Linear equations of second order ===&lt;br /&gt;
二阶线性方程&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Assuming {{math|''u&amp;lt;sub&amp;gt;xy&amp;lt;/sub&amp;gt;'' {{=}} ''u&amp;lt;sub&amp;gt;yx&amp;lt;/sub&amp;gt;''}}, the general linear second-order PDE in two independent variables has the form&lt;br /&gt;
&lt;br /&gt;
Assuming  u&amp;lt;sub&amp;gt;yx&amp;lt;/sub&amp;gt;}}, the general linear second-order PDE in two independent variables has the form&lt;br /&gt;
&lt;br /&gt;
假设 {{math|''u&amp;lt;sub&amp;gt;xy&amp;lt;/sub&amp;gt;'' {{=}} ''u&amp;lt;sub&amp;gt;yx&amp;lt;/sub&amp;gt;''}}，含有两个独立变量的一般线性二阶偏微分方程具有如下形式：&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt;Au_{xx} + 2Bu_{xy} + Cu_{yy} + \cdots \mbox{(lower order terms)} = 0,&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;Au_{xx} + 2Bu_{xy} + Cu_{yy} + \cdots \mbox{(lower order terms)} = 0,&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
where the coefficients {{mvar|A}}, {{mvar|B}}, {{mvar|C}}... may depend upon {{mvar|x}} and {{mvar|y}}. If {{math|''A''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; + ''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; + ''C''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; &amp;gt; 0}} over a region of the {{mvar|xy}}-plane, the PDE is second-order in that region. This form is analogous to the equation for a conic section:&lt;br /&gt;
&lt;br /&gt;
where the coefficients , , ... may depend upon  and . If  over a region of the -plane, the PDE is second-order in that region. This form is analogous to the equation for a conic section:&lt;br /&gt;
&lt;br /&gt;
其中的系数 {{mvar|A}}, {{mvar|B}}, {{mvar|C}}... 一般取决于 {{mvar|x}} 和 {{mvar|y}} 。如果在 {{mvar|xy}}-平面的一个区域上 {{math|''A''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; + ''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; + ''C''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; &amp;gt; 0}}，偏微分方程是二阶的，这种形式类似于圆锥截面的方程:&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt;Ax^2 + 2Bxy + Cy^2 + \cdots = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;Ax^2 + 2Bxy + Cy^2 + \cdots = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
More precisely, replacing {{math|∂&amp;lt;sub&amp;gt;''x''&amp;lt;/sub&amp;gt;}} by {{mvar|X}}, and likewise for other variables (formally this is done by a [[Fourier transform]]), converts a constant-coefficient PDE into a polynomial of the same degree, with the terms of the highest degree (a [[homogeneous polynomial]], here a [[quadratic form]]) being most significant for the classification.&lt;br /&gt;
&lt;br /&gt;
More precisely, replacing  by , and likewise for other variables (formally this is done by a Fourier transform), converts a constant-coefficient PDE into a polynomial of the same degree, with the terms of the highest degree (a homogeneous polynomial, here a quadratic form) being most significant for the classification.&lt;br /&gt;
&lt;br /&gt;
更准确地说，用 {{mvar|X}} 替换 {{math|∂&amp;lt;sub&amp;gt;''x''&amp;lt;/sub&amp;gt;}}，并同样替换其它变量(通常由傅里叶变换完成)，将一个常系数偏微分方程转换成一个相同次数的多项式，最高次数的项(齐次多项式，这里是一个二次形式)对于偏微分方程的分类最为重要。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Just as one classifies [[conic section]]s and quadratic forms into parabolic, hyperbolic, and elliptic based on the [[discriminant]] {{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − 4''AC''}}, the same can be done for a second-order PDE at a given point.  However, the [[discriminant]] in a PDE is given by {{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC''}} due to the convention of the {{mvar|xy}} term being {{math|2''B''}} rather than {{mvar|B}}; formally, the discriminant (of the associated quadratic form) is {{math|(2''B'')&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − 4''AC'' {{=}} 4(''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC'')}}, with the factor of 4 dropped for simplicity.&lt;br /&gt;
&lt;br /&gt;
Just as one classifies conic sections and quadratic forms into parabolic, hyperbolic, and elliptic based on the discriminant , the same can be done for a second-order PDE at a given point.  However, the discriminant in a PDE is given by  due to the convention of the  term being  rather than ; formally, the discriminant (of the associated quadratic form) is  4(B&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − AC)}}, with the factor of 4 dropped for simplicity.&lt;br /&gt;
&lt;br /&gt;
正如人们可以根据判别式 {{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − 4''AC''}} 将圆锥截面和二次型分为抛物型、双曲型和椭圆型一样，对于给定点的二阶偏微分方程也可以这样做。然而，偏微分方程中的判别式 {{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − 4''AC''}} 是根据交叉项的系数{{math|2''B''}} 而不是 {{mvar|B}} 给出的，形式上，判别式(关联二次型)是 {{math|(2''B'')&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − 4''AC'' {{=}} 4(''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC'')}}，为简单起见，去掉了因子4。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
# {{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC'' &amp;lt; 0}} (''[[elliptic partial differential equation]]''): Solutions of [[elliptic partial differential equation|elliptic PDEs]] are as smooth as the coefficients allow, within the interior of the region where the equation and solutions are defined. For example, solutions of [[Laplace's equation]] are analytic within the domain where they are defined, but solutions may assume boundary values that are not smooth. The motion of a fluid at subsonic speeds can be approximated with elliptic PDEs, and the Euler–Tricomi equation is elliptic where {{math|''x'' &amp;lt; 0}}.&lt;br /&gt;
&lt;br /&gt;
  (elliptic partial differential equation): Solutions of elliptic PDEs are as smooth as the coefficients allow, within the interior of the region where the equation and solutions are defined. For example, solutions of Laplace's equation are analytic within the domain where they are defined, but solutions may assume boundary values that are not smooth. The motion of a fluid at subsonic speeds can be approximated with elliptic PDEs, and the Euler–Tricomi equation is elliptic where .&lt;br /&gt;
&lt;br /&gt;
{{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC'' &amp;lt; 0}} (椭圆型微分方程)：在定义方程和解的区域内部，椭圆型偏微分方程的解在系数允许的程度内光滑。例如，拉普拉斯方程的解在它们被定义的区域内是解析的，但可能假设边界值是不光滑的。亚音速流体的运动可以用椭圆型偏微分方程近似，欧拉-特里科米方程在 {{math|''x'' &amp;lt; 0}} 时是椭圆型偏微分方程。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
# {{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC'' {{=}} 0}} (''[[parabolic partial differential equation]]''): Equations that are [[parabolic partial differential equation|parabolic]] at every point can be transformed into a form analogous to the [[heat equation]] by a change of independent variables. Solutions smooth out as the transformed time variable increases. The Euler–Tricomi equation has parabolic type on the line where {{math|''x'' {{=}} 0}}.&lt;br /&gt;
&lt;br /&gt;
  0}} (parabolic partial differential equation): Equations that are parabolic at every point can be transformed into a form analogous to the heat equation by a change of independent variables. Solutions smooth out as the transformed time variable increases. The Euler–Tricomi equation has parabolic type on the line where  0}}.&lt;br /&gt;
&lt;br /&gt;
{{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC'' {{=}} 0}}（抛物型偏微分方程）：在每一点上都是抛物线型的方程可以通过改变自变量从而转化成类似于热方程的形式。随着转换后的时间变量的增加，方程的解变得平滑。欧拉-特里科米方程在特征线 {{math|''x'' {{=}} 0}} 上是抛物线型的。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
# {{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC'' &amp;gt; 0}} (''[[hyperbolic partial differential equation]]''): [[hyperbolic partial differential equation|hyperbolic]] equations retain any discontinuities of functions or derivatives in the initial data. An example is the [[wave equation]]. The motion of a fluid at supersonic speeds can be approximated with hyperbolic PDEs, and the Euler–Tricomi equation is hyperbolic where {{math|''x'' &amp;gt; 0}}.&lt;br /&gt;
&lt;br /&gt;
  (hyperbolic partial differential equation): hyperbolic equations retain any discontinuities of functions or derivatives in the initial data. An example is the wave equation. The motion of a fluid at supersonic speeds can be approximated with hyperbolic PDEs, and the Euler–Tricomi equation is hyperbolic where .&lt;br /&gt;
&lt;br /&gt;
{{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC'' &amp;gt; 0}} (双曲型偏微分方程)：双曲型方程在初始数据中保留了函数或导数的任何不连续性。波动方程就是其中的一个例子。超音速流体的运动可以用双曲型偏微分方程近似，欧拉-特里科米方程在 {{math|''x'' &amp;gt; 0}} 时是双曲型的。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
If there are {{mvar|n}} independent variables {{math|''x''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;, ''x''&amp;lt;sub&amp;gt;2 &amp;lt;/sub&amp;gt;,… ''x''&amp;lt;sub&amp;gt;''n''&amp;lt;/sub&amp;gt;}}, a general linear partial differential equation of second order has the form&lt;br /&gt;
&lt;br /&gt;
If there are  independent variables , a general linear partial differential equation of second order has the form&lt;br /&gt;
&lt;br /&gt;
如果存在 {{mvar|n}} 个自变量 {{math|''x''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;, ''x''&amp;lt;sub&amp;gt;2 &amp;lt;/sub&amp;gt;,… ''x''&amp;lt;sub&amp;gt;''n''&amp;lt;/sub&amp;gt;}}，一般二阶线性偏微分方程的形式是：&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt;L u =\sum_{i=1}^n\sum_{j=1}^n a_{i,j} \frac{\partial^2 u}{\partial x_i \partial x_j} \quad \text{ plus lower-order terms} =0.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;L u =\sum_{i=1}^n\sum_{j=1}^n a_{i,j} \frac{\partial^2 u}{\partial x_i \partial x_j} \quad \text{ plus lower-order terms} =0.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The classification depends upon the signature of the eigenvalues of the coefficient matrix {{math|''a''&amp;lt;sub&amp;gt;''i'',''j''&amp;lt;/sub&amp;gt;}}.&lt;br /&gt;
&lt;br /&gt;
The classification depends upon the signature of the eigenvalues of the coefficient matrix .&lt;br /&gt;
&lt;br /&gt;
这种分类取决于系数矩阵特征值的符号（正负性）。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
# Elliptic: the eigenvalues are all positive or all negative.&lt;br /&gt;
&lt;br /&gt;
 Elliptic: the eigenvalues are all positive or all negative.&lt;br /&gt;
&lt;br /&gt;
椭圆形方程: 特征值全部为正或全部为负。&lt;br /&gt;
&lt;br /&gt;
# Parabolic: the eigenvalues are all positive or all negative, save one that is zero.&lt;br /&gt;
&lt;br /&gt;
 Parabolic: the eigenvalues are all positive or all negative, save one that is zero.&lt;br /&gt;
&lt;br /&gt;
抛物线形方程:除了一个为零值，特征值全部为正或全部为负。&lt;br /&gt;
&lt;br /&gt;
# Hyperbolic: there is only one negative eigenvalue and all the rest are positive, or there is only one positive eigenvalue and all the rest are negative.&lt;br /&gt;
&lt;br /&gt;
 Hyperbolic: there is only one negative eigenvalue and all the rest are positive, or there is only one positive eigenvalue and all the rest are negative.&lt;br /&gt;
&lt;br /&gt;
双曲形方程: 只有一个负特征值，其余的都是正特征值，或者只有一个正特征值，其余的都是负特征值。&lt;br /&gt;
&lt;br /&gt;
# Ultrahyperbolic: there is more than one positive eigenvalue and more than one negative eigenvalue, and there are no zero eigenvalues. There is only a limited theory for ultrahyperbolic equations (Courant and Hilbert, 1962).&lt;br /&gt;
&lt;br /&gt;
 Ultrahyperbolic: there is more than one positive eigenvalue and more than one negative eigenvalue, and there are no zero eigenvalues. There is only a limited theory for ultrahyperbolic equations (Courant and Hilbert, 1962).&lt;br /&gt;
&lt;br /&gt;
超双形方程: 存在多于一个正特征值和多于一个的负特征值，且不存在零特征值。对于超双曲方程，只存在有限的理论(Courant 和 Hilbert，1962)。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
=== Systems of first-order equations and characteristic surfaces ===&lt;br /&gt;
一阶方程组和特征曲面&lt;br /&gt;
&lt;br /&gt;
The classification of partial differential equations can be extended to systems of first-order equations, where the unknown {{mvar|u}} is now a [[Euclidean vector|vector]] with {{mvar|m}} components, and the coefficient matrices {{mvar|A&amp;lt;sub&amp;gt;ν&amp;lt;/sub&amp;gt;}} are {{mvar|m}} by {{mvar|m}} matrices for {{math|''ν'' {{=}} 1, 2,… ''n''}}. The partial differential equation takes the form&lt;br /&gt;
&lt;br /&gt;
The classification of partial differential equations can be extended to systems of first-order equations, where the unknown  is now a vector with  components, and the coefficient matrices  are  by  matrices for  1, 2,… n}}. The partial differential equation takes the form&lt;br /&gt;
&lt;br /&gt;
偏微分方程的分类可以推广到一阶方程组，其中未知量 {{mvar|u}} 是有 {{mvar|m}} 个分量的向量。对于 {{math|''ν'' {{=}} 1, 2,… ''n''}}，系数矩阵 {{mvar|A&amp;lt;sub&amp;gt;ν&amp;lt;/sub&amp;gt;}} 是 {{mvar|m}} × {{mvar|m}} 的矩阵。偏微分方程形式如下：&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt;Lu = \sum_{\nu=1}^{n} A_\nu \frac{\partial u}{\partial x_\nu} + B=0,&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;Lu = \sum_{\nu=1}^{n} A_\nu \frac{\partial u}{\partial x_\nu} + B=0,&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
where the coefficient matrices {{mvar|A&amp;lt;sub&amp;gt;ν&amp;lt;/sub&amp;gt;}} and the vector {{mvar|B}} may depend upon {{mvar|x}} and {{mvar|u}}. If a [[hypersurface]] {{mvar|S}} is given in the implicit form&lt;br /&gt;
&lt;br /&gt;
where the coefficient matrices  and the vector  may depend upon  and . If a hypersurface  is given in the implicit form&lt;br /&gt;
&lt;br /&gt;
其中，系数矩阵 {{mvar|A&amp;lt;sub&amp;gt;ν&amp;lt;/sub&amp;gt;}} 和向量 {{mvar|B}} 可能依赖于 {{mvar|x}} 和 {{mvar|u}}。如果超曲面是以以下隐式形式给出的，&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt;\varphi(x_1, x_2, \ldots x_n)=0,&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;\varphi(x_1, x_2, \ldots x_n)=0,&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
where {{mvar|φ}} has a non-zero gradient, then {{mvar|S}} is a '''characteristic surface''' for the operator {{mvar|L}} at a given point if the characteristic form vanishes:&lt;br /&gt;
&lt;br /&gt;
where  has a non-zero gradient, then  is a characteristic surface for the operator  at a given point if the characteristic form vanishes:&lt;br /&gt;
&lt;br /&gt;
其中，存在一个非零的梯度 {{mvar|φ}}，对于在给定点上特征形式消失的算子，特征曲面 {{mvar|S}} 形式如下:&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt;Q\left(\frac{\partial\varphi}{\partial x_1}, \ldots\frac{\partial\varphi}{\partial x_n}\right) =\det\left[\sum_{\nu=1}^nA_\nu \frac{\partial \varphi}{\partial x_\nu}\right]=0.\,&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;Q\left(\frac{\partial\varphi}{\partial x_1}, \ldots\frac{\partial\varphi}{\partial x_n}\right) =\det\left[\sum_{\nu=1}^nA_\nu \frac{\partial \varphi}{\partial x_\nu}\right]=0.\,&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The geometric interpretation of this condition is as follows: if data for {{mvar|u}} are prescribed on the surface {{mvar|S}}, then it may be possible to determine the normal derivative of {{mvar|u}} on {{mvar|S}} from the differential equation. If the data on {{mvar|S}} and the differential equation determine the normal derivative of {{mvar|u}} on {{mvar|S}}, then {{mvar|S}} is non-characteristic. If the data on {{mvar|S}} and the differential equation ''do not'' determine the normal derivative of {{mvar|u}} on {{mvar|S}}, then the surface is '''characteristic''', and the differential equation restricts the data on {{mvar|S}}: the differential equation is ''internal'' to {{mvar|S}}.&lt;br /&gt;
&lt;br /&gt;
The geometric interpretation of this condition is as follows: if data for  are prescribed on the surface , then it may be possible to determine the normal derivative of  on  from the differential equation. If the data on  and the differential equation determine the normal derivative of  on , then  is non-characteristic. If the data on  and the differential equation do not determine the normal derivative of  on , then the surface is characteristic, and the differential equation restricts the data on : the differential equation is internal to .&lt;br /&gt;
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这个条件的几何解释如下: 如果关于 {{mvar|u}} 的数据是在曲面 {{mvar|S}} 上规定的，那么就有可能依据微分方程确定曲面 {{mvar|S}} 上 {{mvar|u}} 的法向导数。如果曲面 {{mvar|S}} 上的数据和上面的微分方程能确定曲面 {{mvar|S}} 上 {{mvar|u}} 的法向导数，那么它就是非特征的。如果曲面 {{mvar|S}} 上的数据和上面的微分方程不能确定曲面 {{mvar|S}} 上 {{mvar|u}} 的法向导数，那么曲面是特征的，并且微分方程将数据限制在曲面 {{mvar|S}} 上：微分方程是在曲面 {{mvar|S}} 内部。&lt;br /&gt;
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# A first-order system {{math|''Lu'' {{=}} 0}} is ''elliptic'' if no surface is characteristic for {{mvar|L}}: the values of {{mvar|u}} on {{mvar|S}} and the differential equation always determine the normal derivative of {{mvar|u}} on {{mvar|S}}.&lt;br /&gt;
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 A first-order system  0}} is elliptic if no surface is characteristic for : the values of  on  and the differential equation always determine the normal derivative of  on .&lt;br /&gt;
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如果对于 {{mvar|L}} 没有曲面是特征的，则一阶系统 {{math|''Lu'' {{=}} 0}} 是椭圆形的：{{mvar|u}}在 {{mvar|S}} 的值和微分方程总能够决定 {{mvar|S}} 上 {{mvar|u}} 的法向导数。&lt;br /&gt;
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# A first-order system is ''hyperbolic'' at a point if there is a '''spacelike''' surface {{mvar|S}} with normal {{mvar|ξ}} at that point. This means that, given any non-trivial vector {{mvar|η}} orthogonal to {{mvar|ξ}}, and a scalar multiplier {{mvar|λ}}, the equation {{math|''Q''(''λξ'' + ''η'') {{=}} 0}} has {{mvar|m}} real roots {{math|''λ''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;, ''λ''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;,… ''λ''&amp;lt;sub&amp;gt;''m''&amp;lt;/sub&amp;gt;}}. The system is '''strictly hyperbolic''' if these roots are always distinct. The geometrical interpretation of this condition is as follows: the characteristic form {{math|''Q''(''ζ'') {{=}} 0}} defines a cone (the normal cone) with homogeneous coordinates ζ. In the hyperbolic case, this cone has {{mvar|m}} sheets, and the axis {{math|''ζ'' {{=}} ''λξ''}} runs inside these sheets: it does not intersect any of them. But when displaced from the origin by η, this axis intersects every sheet. In the elliptic case, the normal cone has no real sheets.&lt;br /&gt;
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 A first-order system is hyperbolic at a point if there is a spacelike surface  with normal  at that point. This means that, given any non-trivial vector  orthogonal to , and a scalar multiplier , the equation  0}} has  real roots . The system is strictly hyperbolic if these roots are always distinct. The geometrical interpretation of this condition is as follows: the characteristic form  0}} defines a cone (the normal cone) with homogeneous coordinates ζ. In the hyperbolic case, this cone has  sheets, and the axis  λξ}} runs inside these sheets: it does not intersect any of them. But when displaced from the origin by η, this axis intersects every sheet. In the elliptic case, the normal cone has no real sheets.&lt;br /&gt;
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如果在该点存在一个法向量为 {{mvar|ξ}}的 '''&amp;lt;font color=&amp;quot;#ff8000&amp;quot;&amp;gt;类空曲面 Spacclike Surface&amp;lt;/font&amp;gt; {{mvar|S}} ，则一阶系统在那一点是双曲的。这意味着，给定任意正交于 {{mvar|ξ}} 的非平凡向量 {{mvar|η}} 和一个标量乘子 {{mvar|λ}}，方程 {{math|''Q''(''λξ'' + ''η'') {{=}} 0}} 有 {{mvar|m}} 个实根 {{math|''λ''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;, ''λ''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;,… ''λ''&amp;lt;sub&amp;gt;''m''&amp;lt;/sub&amp;gt;}}。如果这些根始终不同，则该系统是严格双曲形的。这个条件的几何解释如下: 特征形式 {{math|''Q''(''ζ'') {{=}} 0}} 定义了一个具有齐次坐标 ζ的圆锥(法线圆锥)。在双曲形的情况下，这个圆锥体有 {{mvar|m}} 层，并且轴 {{math|''ζ'' {{=}} ''λξ''}} 在这些层中运动: 它不与任何一层相交。但是当从原点偏离η时，这条轴线与每一层都相交。在椭圆形的情况下，法向圆锥没有实层。&lt;br /&gt;
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==[[用户:Yuling|Yuling]]（[[用户讨论:Yuling|讨论]]） sheet 这个单词也不很理解，我直译为了“层”&lt;br /&gt;
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=== Equations of mixed type ===&lt;br /&gt;
混合型方程&lt;br /&gt;
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If a PDE has coefficients that are not constant, it is possible that it will not belong to any of these categories but rather be of '''mixed type'''. A simple but important example is the [[Euler–Tricomi equation]]&lt;br /&gt;
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If a PDE has coefficients that are not constant, it is possible that it will not belong to any of these categories but rather be of mixed type. A simple but important example is the Euler–Tricomi equation&lt;br /&gt;
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如果偏微分方程有非常数的系数，那么它可能不属于这些类别中的任何一个，而是属于混合型。一个简单但重要的例子是欧拉-特里科米方程：&lt;br /&gt;
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: &amp;lt;math&amp;gt;u_{xx} = xu_{yy},&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;u_{xx} = xu_{yy},&amp;lt;/math&amp;gt;&lt;br /&gt;
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which is called '''elliptic-hyperbolic''' because it is elliptic in the region {{math|''x'' &amp;lt; 0}}, hyperbolic in the region {{math|''x'' &amp;gt; 0}}, and degenerate parabolic on the line {{math|''x'' {{=}} 0}}.&lt;br /&gt;
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which is called elliptic-hyperbolic because it is elliptic in the region , hyperbolic in the region , and degenerate parabolic on the line  0}}.&lt;br /&gt;
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它在 {{math|''x'' &amp;lt; 0}} 的区域上是椭圆形，在 {{math|''x'' &amp;gt; 0}} 区域上是双曲形，在 {{math|''x'' {{=}} 0}}这条线上是退化为抛物线形，因此称之为椭圆-双曲型。&lt;br /&gt;
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''fill in: Dirichlet and Neumann boundaries, hyperbolic/parabolic/elliptic separation of variables, [[Fourier analysis]], [[Green's function]]s ...--&amp;gt;&lt;br /&gt;
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fill in: Dirichlet and Neumann boundaries, hyperbolic/parabolic/elliptic separation of variables, Fourier analysis, Green's functions ...--&amp;gt;&lt;br /&gt;
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填写: Dirichlet 和 Neumann 边界，双曲 / 抛物线 / 椭圆分离变量法，傅立叶分析，Green 函数... --&lt;br /&gt;
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=== Infinite-order PDEs in quantum mechanics ===&lt;br /&gt;
量子力学中的无限阶偏微分方程&lt;br /&gt;
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In the [[phase space formulation]] of quantum mechanics,  one may consider the [[Method of quantum characteristics|quantum Hamilton's equations]] for trajectories of quantum particles. These equations are infinite-order PDEs. However, in the semiclassical expansion, one has a finite system of ODEs at any fixed order of [[Dirac constant|{{mvar|ħ}}]].  The evolution equation of the [[Wigner quasi-probability distribution|c]] is also an infinite-order PDE. The quantum trajectories are [[Method of quantum characteristics|quantum characteristics]], with the use of which one could calculate the evolution of the Wigner function.&lt;br /&gt;
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In the phase space formulation of quantum mechanics,  one may consider the quantum Hamilton's equations for trajectories of quantum particles. These equations are infinite-order PDEs. However, in the semiclassical expansion, one has a finite system of ODEs at any fixed order of Dirac constant|.  The evolution equation of the Wigner function is also an infinite-order PDE. The quantum trajectories are quantum characteristics, with the use of which one could calculate the evolution of the Wigner function.&lt;br /&gt;
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在量子力学中的相空间表述中，我们可以考虑求解量子粒子的轨迹的量子哈密顿的方程。这些方程是无限阶偏微分方程。然而，在半经典展开中，我们在给定[[Dirac constant|{{mvar|ħ}}]]阶数下有一个有限的常微分方程组。'''&amp;lt;font color=&amp;quot;#ff8000&amp;quot;&amp;gt;维格纳函数  Wigner Function&amp;lt;/font&amp;gt;的演化方程也是一个无限阶偏微分方程。量子轨道具有量子特性，通常可以用来计算维格纳函数的演化。&lt;br /&gt;
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== Analytical solutions ==&lt;br /&gt;
解析解&lt;br /&gt;
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===Separation of variables===&lt;br /&gt;
分离变量法&lt;br /&gt;
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{{main|Separable partial differential equation}}&lt;br /&gt;
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Linear PDEs can be reduced to systems of ordinary differential equations by the important technique of separation of variables. This technique rests on a characteristic of solutions to differential equations: if one can find any solution that solves the equation and satisfies the boundary conditions, then it is ''the'' solution (this also applies to ODEs). We assume as an [[ansatz]] that the dependence of a solution on the parameters space and time can be written as a product of terms that each depend on a single parameter, and then see if this can be made to solve the problem.&amp;lt;ref&amp;gt;{{cite book|last1=Gershenfeld|first1=Neil|title=The nature of mathematical modeling|date=2000|publisher=Cambridge Univ. Press|location=Cambridge|isbn=0521570956|page=27|edition=Reprinted (with corr.)}}&amp;lt;/ref&amp;gt;&lt;br /&gt;
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Linear PDEs can be reduced to systems of ordinary differential equations by the important technique of separation of variables. This technique rests on a characteristic of solutions to differential equations: if one can find any solution that solves the equation and satisfies the boundary conditions, then it is the solution (this also applies to ODEs). We assume as an ansatz that the dependence of a solution on the parameters space and time can be written as a product of terms that each depend on a single parameter, and then see if this can be made to solve the problem.&lt;br /&gt;
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线性偏微分方程组可以通过分离变量法简化为常微分方程组。这种方法依赖于微分方程解的一个特性: 如果能找到任何一个满足方程和边界条件的解，那么这个解就是方程的解(这也适用于常微分方程)。我们假设解对空间和时间的依赖可以写成对它们每一项的依赖的乘积，然后再看否可以用来解决问题。&lt;br /&gt;
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In the method of separation of variables, one reduces a PDE to a PDE in fewer variables, which is an ordinary differential equation if in one variable – these are in turn easier to solve.&lt;br /&gt;
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In the method of separation of variables, one reduces a PDE to a PDE in fewer variables, which is an ordinary differential equation if in one variable – these are in turn easier to solve.&lt;br /&gt;
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在分离变量法方法中，可以将偏微分方程简化为含有更少变量的偏微分方程，如果只有一个变量，那么就变成了一个'''&amp;lt;font color = &amp;quot;#ff8000&amp;quot;&amp;gt;常微分方程 Ordinary Differential Equation&amp;lt;/font&amp;gt;'''--，这些方程也更容易求解。&lt;br /&gt;
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This is possible for simple PDEs, which are called [[separable partial differential equation]]s, and the domain is generally a rectangle (a product of intervals). Separable PDEs correspond to [[diagonal matrices]] – thinking of &amp;quot;the value for fixed {{mvar|x}}&amp;quot; as a coordinate, each coordinate can be understood separately.&lt;br /&gt;
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This is possible for simple PDEs, which are called separable partial differential equations, and the domain is generally a rectangle (a product of intervals). Separable PDEs correspond to diagonal matrices – thinking of &amp;quot;the value for fixed &amp;quot; as a coordinate, each coordinate can be understood separately.&lt;br /&gt;
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对于简单的偏微分方程(称为可分离偏微分方程)来说，这是可能的，而且方程通常定义在一个矩形区域(区间的积)上。可分离偏微分方程对应于对角线矩阵——以“固定值”为坐标，每个坐标可分开理解。&lt;br /&gt;
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This generalizes to the [[method of characteristics]], and is also used in [[integral transform]]s.&lt;br /&gt;
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This generalizes to the method of characteristics, and is also used in integral transforms.&lt;br /&gt;
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这种方法可以推广到特征曲线法，也可以用于积分变换。&lt;br /&gt;
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===Method of characteristics===&lt;br /&gt;
特征曲线法&lt;br /&gt;
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{{main|Method of characteristics}}&lt;br /&gt;
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In special cases, one can find characteristic curves on which the equation reduces to an ODE – changing coordinates in the domain to straighten these curves allows separation of variables, and is called the [[method of characteristics]].&lt;br /&gt;
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In special cases, one can find characteristic curves on which the equation reduces to an ODE – changing coordinates in the domain to straighten these curves allows separation of variables, and is called the method of characteristics.&lt;br /&gt;
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在特殊情况下，可以找到一些特征曲线，在这些曲线上方程可以变成一个常微分方程——意味着改变坐标从而使这些曲线变直从而达到分离变量的目的，这就是所谓的特征曲线法。&lt;br /&gt;
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More generally, one may find characteristic surfaces.&lt;br /&gt;
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More generally, one may find characteristic surfaces.&lt;br /&gt;
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更一般地说，人们可能会找到特征表面。&lt;br /&gt;
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===Integral transform===&lt;br /&gt;
积分变换&lt;br /&gt;
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An [[integral transform]] may transform the PDE to a simpler one, in particular, a separable PDE. This corresponds to diagonalizing an operator.&lt;br /&gt;
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An integral transform may transform the PDE to a simpler one, in particular, a separable PDE. This corresponds to diagonalizing an operator.&lt;br /&gt;
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积分变换可以将偏微分方程转换为更简单的偏微分方程，特别是可分离的偏微分方程。这对应于对角化算符。&lt;br /&gt;
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An important example of this is [[Fourier analysis]], which diagonalizes the heat equation using the [[eigenbasis]] of sinusoidal waves.&lt;br /&gt;
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An important example of this is Fourier analysis, which diagonalizes the heat equation using the eigenbasis of sinusoidal waves.&lt;br /&gt;
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这方面的一个重要例子是'''&amp;lt;font color = &amp;quot;#ff8000&amp;quot;&amp;gt;傅里叶分析  Fourier Analysis&amp;lt;/font&amp;gt;'''，它使用正弦波的特征基来对角化热方程。&lt;br /&gt;
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If the domain is finite or periodic, an infinite sum of solutions such as a [[Fourier series]] is appropriate, but an integral of solutions such as a [[Fourier integral]] is generally required for infinite domains. The solution for a point source for the heat equation given above is an example of the use of a Fourier integral.&lt;br /&gt;
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If the domain is finite or periodic, an infinite sum of solutions such as a Fourier series is appropriate, but an integral of solutions such as a Fourier integral is generally required for infinite domains. The solution for a point source for the heat equation given above is an example of the use of a Fourier integral.&lt;br /&gt;
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如果区域是有限的或周期性的，那么解为无限和的形式是恰当的，例如傅里叶级数，但是一个解的积分，例如傅立叶积分，一般是在无限区域上的。上面给出的热传导方程的点源解法就是使用傅里叶积分的一个例子。&lt;br /&gt;
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===Change of variables===&lt;br /&gt;
变量代换&lt;br /&gt;
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Often a PDE can be reduced to a simpler form with a known solution by a suitable [[Change of variables (PDE)|change of variables]].  For example, the [[Black–Scholes equation#Derivation|Black–Scholes]] PDE&lt;br /&gt;
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Often a PDE can be reduced to a simpler form with a known solution by a suitable change of variables.  For example, the Black–Scholes PDE&lt;br /&gt;
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偏微分方程通常可以通过变量的适当变化，用已知的解简化为更简单的形式。例如，布莱克-舒尔斯偏微分方程&lt;br /&gt;
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:&amp;lt;math&amp;gt; \frac{\partial V}{\partial t} + \tfrac{1}{2}\sigma^2 S^2\frac{\partial^2 V}{\partial S^2} + rS\frac{\partial V}{\partial S} - rV = 0 &amp;lt;/math&amp;gt;&lt;br /&gt;
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&amp;lt;math&amp;gt; \frac{\partial V}{\partial t} + \tfrac{1}{2}\sigma^2 S^2\frac{\partial^2 V}{\partial S^2} + rS\frac{\partial V}{\partial S} - rV = 0 &amp;lt;/math&amp;gt;&lt;br /&gt;
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is reducible to the [[heat equation]]&lt;br /&gt;
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is reducible to the heat equation&lt;br /&gt;
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可以简化为热传导方程&lt;br /&gt;
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:&amp;lt;math&amp;gt; \frac{\partial u}{\partial \tau} = \frac{\partial^2 u}{\partial x^2}&amp;lt;/math&amp;gt;&lt;br /&gt;
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&amp;lt;math&amp;gt; \frac{\partial u}{\partial \tau} = \frac{\partial^2 u}{\partial x^2}&amp;lt;/math&amp;gt;&lt;br /&gt;
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by the change of variables (for complete details see {{webarchive |url=https://web.archive.org/web/20080411030405/http://www.math.unl.edu/~sdunbar1/Teaching/MathematicalFinance/Lessons/BlackScholes/Solution/solution.shtml |date=April 11, 2008 |title=Solution of the Black Scholes Equation }})&lt;br /&gt;
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by the change of variables (for complete details see )&lt;br /&gt;
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通过变量替换(完整的细节见)&lt;br /&gt;
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:&amp;lt;math&amp;gt;\begin{align}&lt;br /&gt;
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V(S,t) &amp;amp;= K v(x,\tau),\\[5px]&lt;br /&gt;
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x &amp;amp;= \ln\left(\tfrac{S}{K} \right),\\[5px]&lt;br /&gt;
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\tau &amp;amp;= \tfrac{1}{2} \sigma^2 (T - t),\\[5px]&lt;br /&gt;
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v(x,\tau)&amp;amp;=e^{-\alpha x-\beta\tau} u(x,\tau).&lt;br /&gt;
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\end{align}&amp;lt;/math&amp;gt;&lt;br /&gt;
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===Fundamental solution===&lt;br /&gt;
基本解&lt;br /&gt;
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{{main|Fundamental solution}}&lt;br /&gt;
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Inhomogeneous equations can often be solved (for constant coefficient PDEs, always be solved) by finding the [[fundamental solution]] (the solution for a point source), then taking the [[convolution]] with the boundary conditions to get the solution.&lt;br /&gt;
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Inhomogeneous equations can often be solved (for constant coefficient PDEs, always be solved) by finding the fundamental solution (the solution for a point source), then taking the convolution with the boundary conditions to get the solution.&lt;br /&gt;
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非齐次方程(常系数偏微分方程)一般是通过先求出基本解(点源的解) ，然后利用带边界条件的卷积来求解。&lt;br /&gt;
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This is analogous in [[signal processing]] to understanding a filter by its [[impulse response]].&lt;br /&gt;
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This is analogous in signal processing to understanding a filter by its impulse response.&lt;br /&gt;
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这类似于在信号处理中通过滤波器的脉冲响应来理解滤波器。&lt;br /&gt;
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===Superposition principle===&lt;br /&gt;
叠加原理&lt;br /&gt;
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{{further| Superposition principle }}&lt;br /&gt;
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The superposition principle applies to any linear system, including linear systems of PDEs. A common visualization of this concept is the interaction of two waves in phase being combined to result in a greater amplitude, for example {{math|sin ''x'' + sin ''x'' {{=}} 2 sin ''x''}}. The same principle can be observed in PDEs where the solutions may be real or complex and additive. [[Superposition principle|superposition]]&lt;br /&gt;
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The superposition principle applies to any linear system, including linear systems of PDEs. A common visualization of this concept is the interaction of two waves in phase being combined to result in a greater amplitude, for example  2 sin x}}. The same principle can be observed in PDEs where the solutions may be real or complex and additive. superposition&lt;br /&gt;
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'''&amp;lt;font color = &amp;quot;#ff8000&amp;quot;&amp;gt;叠加原理 Superposition Principle&amp;lt;/font&amp;gt;适用于任何线性系统，包括偏微分方程的线性系统。这个概念的一个常见的可视化是两个同相位的波相互作用结合在一起会产生更大的振幅，例如 {{math|sin ''x'' + sin ''x'' {{=}} 2 sin ''x''}}。在偏微分方程中也可以观察到同样的原理，其中的解可能是真实的或复杂的和可加的。叠加&lt;br /&gt;
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If {{math|''u''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;}} and {{math|''u''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;}} are solutions of linear PDE in some function space {{mvar|R}}, then {{math|''u'' {{=}} ''c''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;''u''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; + ''c''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;''u''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;}} with any constants {{math|''c''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;}} and {{math|''c''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;}} are also a solution of that PDE in the same function space.&lt;br /&gt;
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If  and  are solutions of linear PDE in some function space , then  c&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;u&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; + c&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;u&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;}} with any constants  and  are also a solution of that PDE in the same function space.&lt;br /&gt;
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若线性偏微分方程在某个函数空间{{mvar|R}}中有解{{math|''u''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;}} 和 {{math|''u''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;}}，则{{math|''u'' {{=}} ''c''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;''u''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; + ''c''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;''u''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;}}也是该偏微分方程在同一函数空间中的解，其中{{math|''c''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;}} 和 {{math|''c''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;}} 是任意常数。&lt;br /&gt;
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===Methods for non-linear equations===&lt;br /&gt;
非线性方程的求解方法&lt;br /&gt;
{{see also|nonlinear partial differential equation}}&lt;br /&gt;
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There are no generally applicable methods to solve nonlinear PDEs. Still, existence and uniqueness results (such as the [[Cauchy–Kowalevski theorem]]) are often possible, as are proofs of important qualitative and quantitative properties of solutions (getting these results is a major part of [[mathematical analysis|analysis]]). Computational solution to the nonlinear PDEs, the [[split-step method]], exist for specific equations like [[nonlinear Schrödinger equation]].&lt;br /&gt;
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There are no generally applicable methods to solve nonlinear PDEs. Still, existence and uniqueness results (such as the Cauchy–Kowalevski theorem) are often possible, as are proofs of important qualitative and quantitative properties of solutions (getting these results is a major part of analysis). Computational solution to the nonlinear PDEs, the split-step method, exist for specific equations like nonlinear Schrödinger equation.&lt;br /&gt;
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对于非线性偏微分方程，目前还没有普遍适用的求解方法。然而，通常是可能知道解的存在性和唯一性(如柯西-科瓦列夫斯基定理)，也是可能得到解的重要定性和定量性质的证明(得到这些结果是分析的主要部分)。非线性偏微分方程的计算解，即分步法，对一些特定的方程适用，比如非线性'''&amp;lt;font color=&amp;quot;#ff8000&amp;quot;&amp;gt;薛定谔方程 Schrödinger equation&amp;lt;/font&amp;gt;'''。&lt;br /&gt;
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Nevertheless, some techniques can be used for several types of equations. The [[h-principle|{{mvar|h}}-principle]] is the most powerful method to solve [[Underdetermined system|underdetermined]] equations. The [[Riquier–Janet theory]] is an effective method for obtaining information about many analytic [[Overdetermined system|overdetermined]] systems.&lt;br /&gt;
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Nevertheless, some techniques can be used for several types of equations. The -principle is the most powerful method to solve underdetermined equations. The Riquier–Janet theory is an effective method for obtaining information about many analytic overdetermined systems.&lt;br /&gt;
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然而，一些技巧可以用于几种类型的方程。h-原理是求解欠定方程最有效的方法。里基尔-珍妮特理论是一种可以获得许多解析超定系统信息的有效方法。&lt;br /&gt;
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The [[method of characteristics]] can be used in some very special cases to solve partial differential equations.&lt;br /&gt;
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The method of characteristics can be used in some very special cases to solve partial differential equations.&lt;br /&gt;
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特征线法可用于求解某些特殊情况下的偏微分方程。&lt;br /&gt;
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In some cases, a PDE can be solved via [[perturbation analysis]] in which the solution is considered to be a correction to an equation with a known solution. Alternatives are [[numerical analysis]] techniques from simple [[finite difference]] schemes to the more mature [[multigrid]] and [[finite element method]]s. Many interesting problems in science and engineering are solved in this way using [[computer]]s, sometimes high performance [[supercomputer]]s.&lt;br /&gt;
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In some cases, a PDE can be solved via perturbation analysis in which the solution is considered to be a correction to an equation with a known solution. Alternatives are numerical analysis techniques from simple finite difference schemes to the more mature multigrid and finite element methods. Many interesting problems in science and engineering are solved in this way using computers, sometimes high performance supercomputers.&lt;br /&gt;
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在某些情况下，偏微分方程可以通过扰动分析来求解。在扰动分析中，通常是求解将具有已知解的方程修正后的新得到方程。可供选择的数值分析技术从简单的差分格式到更成熟的多重网格和有限元方法。许多有趣的科学和工程问题都是在计算机上用这种方法解决的，有时是高性能超级计算机。&lt;br /&gt;
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===Lie group method===&lt;br /&gt;
李群方法&lt;br /&gt;
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From 1870 [[Sophus Lie]]'s work put the theory of differential equations on a more satisfactory foundation. He showed that the integration theories of the older mathematicians can, by the introduction of what are now called [[Lie group]]s, be referred, to a common source; and that ordinary differential equations which admit the same [[infinitesimal transformation]]s present comparable difficulties of integration. He also emphasized the subject of [[contact transformation|transformations of contact]].&lt;br /&gt;
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From 1870 Sophus Lie's work put the theory of differential equations on a more satisfactory foundation. He showed that the integration theories of the older mathematicians can, by the introduction of what are now called Lie groups, be referred, to a common source; and that ordinary differential equations which admit the same infinitesimal transformations present comparable difficulties of integration. He also emphasized the subject of transformations of contact.&lt;br /&gt;
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从1870年起，索弗斯·李的工作为微分方程理论奠定了一个较为令人满意的基础。他指出，通过引入现在所谓的李群，老一辈数学家的积分理论可以引用到一个共同的来源; 承认相同的无穷小变换的常微分方程在积分方面存在相当的困难。他还强调了接触的转变这一主题。&lt;br /&gt;
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==[[用户:Yuling|Yuling]]（[[用户讨论:Yuling|讨论]]）这句话“He also emphasized the subject of transformations of contact.”中的transformations of contact翻译的不太好。&lt;br /&gt;
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A general approach to solving PDEs uses the symmetry property of differential equations, the continuous [[infinitesimal transformation]]s of solutions to solutions ([[Lie theory]]). Continuous [[group theory]], [[Lie algebras]] and [[differential geometry]] are used to understand the structure of linear and nonlinear partial differential equations for generating integrable equations, to find its [[Lax pair]]s, recursion operators, [[Bäcklund transform]] and finally finding exact analytic solutions to the PDE.&lt;br /&gt;
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A general approach to solving PDEs uses the symmetry property of differential equations, the continuous infinitesimal transformations of solutions to solutions (Lie theory). Continuous group theory, Lie algebras and differential geometry are used to understand the structure of linear and nonlinear partial differential equations for generating integrable equations, to find its Lax pairs, recursion operators, Bäcklund transform and finally finding exact analytic solutions to the PDE.&lt;br /&gt;
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求解偏微分方程的一般方法是利用微分方程的对称性，即解到解的连续无穷小变换(李理论)。连续群论、李代数和微分几何理论被用来理解生成可积方程的线性和非线性偏微分方程的结构，找到它的Lax对、递归算子、 贝克伦德变换，最后找到偏微分方程的精确解析解。&lt;br /&gt;
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Symmetry methods have been recognized to study differential equations arising in mathematics, physics, engineering, and many other disciplines.&lt;br /&gt;
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Symmetry methods have been recognized to study differential equations arising in mathematics, physics, engineering, and many other disciplines.&lt;br /&gt;
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对称方法已被公认可以用于研究出现在数学，物理，工程和许多其他学科的微分方程。&lt;br /&gt;
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===Semianalytical methods===&lt;br /&gt;
半解析方法&lt;br /&gt;
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The [[Adomian decomposition method]], the [[Aleksandr Lyapunov|Lyapunov]] artificial small parameter method, and He's [[homotopy perturbation method]] are all special cases of the more general [[homotopy analysis method]]. These are series expansion methods, and except for the Lyapunov method, are independent of small physical parameters as compared to the well known [[perturbation theory]], thus giving these methods greater flexibility and solution generality.&lt;br /&gt;
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The Adomian decomposition method, the Lyapunov artificial small parameter method, and He's homotopy perturbation method are all special cases of the more general homotopy analysis method. These are series expansion methods, and except for the Lyapunov method, are independent of small physical parameters as compared to the well known perturbation theory, thus giving these methods greater flexibility and solution generality.&lt;br /&gt;
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阿多米安分解法、李雅普诺夫人工小参数方法和何同伦摄动方法都是更一般的同伦分析方法的特殊情况。除了李雅普诺夫方法之外，这些都是级数展开方法，与为人熟知的摄动理论方法相比，它们与小的物理参数无关，因此这些方法具有更大的灵活性和解的通用性。&lt;br /&gt;
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== Numerical solutions ==&lt;br /&gt;
数值解&lt;br /&gt;
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The three most widely used [[Numerical partial differential equations|numerical methods to solve PDEs]] are the [[finite element analysis|finite element method]] (FEM), [[finite volume method]]s (FVM) and [[finite difference method]]s (FDM), as well other kind of methods called [[Meshfree methods]], which were made to solve problems where the before mentioned methods are limited. The FEM has a prominent position among these methods and especially its exceptionally efficient higher-order version [[hp-FEM]]. Other hybrid versions of FEM and Meshfree methods include the generalized finite element method (GFEM), [[extended finite element method]] (XFEM), [[Spectral element method|spectral finite element method]] (SFEM), [[Meshfree methods|meshfree finite element method]], [[Discontinuous Galerkin Method|discontinuous Galerkin finite element method]] (DGFEM), [[Element-Free Galerkin Method]] (EFGM), [[Interpolating Element-Free Galerkin Method]] (IEFGM), etc.&lt;br /&gt;
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The three most widely used numerical methods to solve PDEs are the finite element method (FEM), finite volume methods (FVM) and finite difference methods (FDM), as well other kind of methods called Meshfree methods, which were made to solve problems where the before mentioned methods are limited. The FEM has a prominent position among these methods and especially its exceptionally efficient higher-order version hp-FEM. Other hybrid versions of FEM and Meshfree methods include the generalized finite element method (GFEM), extended finite element method (XFEM), spectral finite element method (SFEM), meshfree finite element method, discontinuous Galerkin finite element method (DGFEM), Element-Free Galerkin Method (EFGM), Interpolating Element-Free Galerkin Method (IEFGM), etc.&lt;br /&gt;
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求解偏微分方程最常用的三种数值方法是有限元分析法、有限体积法和有限差分法，以及其他一些称为无网格法的方法，用于解决前面用提到的方法求解受到限制的问题。在这些方法中，有限元方法，尤其是高效的高阶有限元方法（hp-FEM），占有重要地位。其他有限元法和无网格法的混合形式包括广义有限元分析法(GFEM)、扩展有限元分析法(XFEM)、谱有限元分析法(SFEM)、无网格有限元分析法(DGFEM)、间断伽辽金有限元分析法(DGFEM)、无单元伽辽金法(EFGM)、插值无单元伽辽金法(IEFGM)等。&lt;br /&gt;
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=== Finite element method ===&lt;br /&gt;
有限元分析法&lt;br /&gt;
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{{main|Finite element method}}&lt;br /&gt;
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The finite element method (FEM) (its practical application often known as finite element analysis (FEA)) is a numerical technique for finding approximate solutions of partial differential equations (PDE) as well as of integral equations. The solution approach is based either on eliminating the differential equation completely (steady state problems), or rendering the PDE into an approximating system of ordinary differential equations, which are then numerically integrated using standard techniques such as Euler's method, Runge–Kutta, etc.&lt;br /&gt;
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The finite element method (FEM) (its practical application often known as finite element analysis (FEA)) is a numerical technique for finding approximate solutions of partial differential equations (PDE) as well as of integral equations. The solution approach is based either on eliminating the differential equation completely (steady state problems), or rendering the PDE into an approximating system of ordinary differential equations, which are then numerically integrated using standard techniques such as Euler's method, Runge–Kutta, etc.&lt;br /&gt;
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'''&amp;lt;font color = &amp;quot;#ff8000&amp;quot;&amp;gt;有限元分析法 Finite Element Method&amp;lt;/font&amp;gt;''' ((其实际应用通常被称为有限元分析(FEA))是一种寻找偏微分方程(PDE)和积分方程近似解的数值技术。这种求解方法要么基于完全消除微分方程(稳态问题) ，要么将偏微分方程转化为常微分方程的近似系统，然后使用标准技术进行数值积分，如欧拉方法、 Runge-Kutta 等。&lt;br /&gt;
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===Finite difference method===&lt;br /&gt;
有限差分法&lt;br /&gt;
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{{main|Finite difference method}}&lt;br /&gt;
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Finite-difference methods are numerical methods for approximating the solutions to differential equations using [[finite difference]] equations to approximate derivatives.&lt;br /&gt;
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Finite-difference methods are numerical methods for approximating the solutions to differential equations using finite difference equations to approximate derivatives.&lt;br /&gt;
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有限差分法是一种数值方法，用差分方程近似倒数来近似微分方程的解。&lt;br /&gt;
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=== Finite volume method ===&lt;br /&gt;
有限体积法&lt;br /&gt;
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{{main|Finite volume method}}&lt;br /&gt;
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Similar to the finite difference method or finite element method, values are calculated at discrete places on a meshed geometry. &amp;quot;Finite volume&amp;quot; refers to the small volume surrounding each node point on a mesh. In the finite volume method, surface integrals in a partial differential equation that contain a divergence term are converted to volume integrals, using the [[divergence theorem]]. These terms are then evaluated as fluxes at the surfaces of each finite volume. Because the flux entering a given volume is identical to that leaving the adjacent volume, these methods conserve mass by design.&lt;br /&gt;
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Similar to the finite difference method or finite element method, values are calculated at discrete places on a meshed geometry. &amp;quot;Finite volume&amp;quot; refers to the small volume surrounding each node point on a mesh. In the finite volume method, surface integrals in a partial differential equation that contain a divergence term are converted to volume integrals, using the divergence theorem. These terms are then evaluated as fluxes at the surfaces of each finite volume. Because the flux entering a given volume is identical to that leaving the adjacent volume, these methods conserve mass by design.&lt;br /&gt;
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类似于有限差分法或有限元分析，函数值是在网格化的几何体上的离散位置进行计算的。“有限体积”是指网格上每个节点周围的小体积。在有限体积法中，偏微分方程中含有散度项的面积分用散度定理积分转换成体积分。然后将这些项用于估算每个有限体积表面上的通量。由于进入给定体积元的通量与转移出相邻体积元的通量相同，所以这些方法通过设计保证了质量守恒。&lt;br /&gt;
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==See also==&lt;br /&gt;
请参阅&lt;br /&gt;
* [[Dirichlet boundary condition]]&lt;br /&gt;
狄利克雷边界条件&lt;br /&gt;
* [[Jet bundle]]&lt;br /&gt;
射流丛&lt;br /&gt;
* [[Laplace transform applied to differential equations]]&lt;br /&gt;
微分方程中的拉普拉斯变换&lt;br /&gt;
* [[List of dynamical systems and differential equations topics]]&lt;br /&gt;
动力学系统列表和微分方程主题&lt;br /&gt;
* [[Matrix differential equation]]&lt;br /&gt;
矩阵微分方程&lt;br /&gt;
* [[Neumann boundary condition]]&lt;br /&gt;
诺伊曼边界条件&lt;br /&gt;
* [[Numerical partial differential equations]]&lt;br /&gt;
数值偏微分方程&lt;br /&gt;
* [[Partial differential algebraic equation]]&lt;br /&gt;
偏微分代数方程&lt;br /&gt;
* [[Recurrence relation]]&lt;br /&gt;
递推关系&lt;br /&gt;
* [[Robin boundary condition]]&lt;br /&gt;
罗宾边界条件&lt;br /&gt;
* [[Stochastic processes and boundary value problems]]&lt;br /&gt;
随机过程和边值问题&lt;br /&gt;
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== The energy method ==&lt;br /&gt;
能量法&lt;br /&gt;
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The energy method is a mathematical procedure that can be used to verify well-posedness of initial-boundary-value-problems.&amp;lt;ref&amp;gt;{{cite book |title=High Order Difference Methods for Time Dependent PDE&lt;br /&gt;
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The energy method is a mathematical procedure that can be used to verify well-posedness of initial-boundary-value-problems.&amp;lt;ref&amp;gt;{{cite book |title=High Order Difference Methods for Time Dependent PDE&lt;br /&gt;
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能量法是一种数学过程，可用于验证初始边界值问题的适定性。&lt;br /&gt;
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In the following example the energy method is used to decide where and which boundary conditions should be imposed such that the resulting IBVP is well-posed. Consider the one-dimensional hyperbolic PDE given by&lt;br /&gt;
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In the following example the energy method is used to decide where and which boundary conditions should be imposed such that the resulting IBVP is well-posed. Consider the one-dimensional hyperbolic PDE given by&lt;br /&gt;
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在下面的示例中，将使用能量法决定应在何处施加哪些边界条件，以使得到的IBVP处于适当位置。考虑下式给出的一维双曲PDE&lt;br /&gt;
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: &amp;lt;math&amp;gt;\frac{\partial u}{\partial t} + \alpha \frac{\partial u}{\partial x} = 0, \quad x \in [a,b], \operatorname t &amp;gt; 0,&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;\frac{\partial u}{\partial t} + \alpha \frac{\partial u}{\partial x} = 0, \quad x \in [a,b], \operatorname t &amp;gt; 0,&amp;lt;/math&amp;gt;&lt;br /&gt;
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where &amp;lt;math&amp;gt;\alpha \neq 0&amp;lt;/math&amp;gt; is a constant and &amp;lt;math&amp;gt;u(x,t)&amp;lt;/math&amp;gt; is an unknown function with initial condition &amp;lt;math&amp;gt;u(x,0) = f(x)&amp;lt;/math&amp;gt;. Multiplying with &amp;lt;math&amp;gt;u&amp;lt;/math&amp;gt; and integrating over the domain gives&lt;br /&gt;
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where &amp;lt;math&amp;gt;\alpha \neq 0&amp;lt;/math&amp;gt; is a constant and &amp;lt;math&amp;gt;u(x,t)&amp;lt;/math&amp;gt; is an unknown function with initial condition &amp;lt;math&amp;gt;u(x,0) = f(x)&amp;lt;/math&amp;gt;. Multiplying with &amp;lt;math&amp;gt;u&amp;lt;/math&amp;gt; and integrating over the domain gives&lt;br /&gt;
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其中 &amp;lt;math&amp;gt;\alpha \neq 0&amp;lt;/math&amp;gt; 是常数，并且 &amp;lt;math&amp;gt;u(x,t)&amp;lt;/math&amp;gt; 是初始条件是 &amp;lt;math&amp;gt;u(x,0) = f(x)&amp;lt;/math&amp;gt;的未知函数，乘以 &amp;lt;math&amp;gt;u&amp;lt;/math&amp;gt; 并在域上进行积分。&lt;br /&gt;
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: &amp;lt;math&amp;gt;\int_a^b u \frac{\partial u}{\partial t} \operatorname dx + \alpha \int _a ^b u \frac{\partial u}{\partial x} \operatorname dx = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;\int_a^b u \frac{\partial u}{\partial t} \operatorname dx + \alpha \int _a ^b u \frac{\partial u}{\partial x} \operatorname dx = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
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Using that&lt;br /&gt;
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Using that&lt;br /&gt;
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利用这一点&lt;br /&gt;
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: &amp;lt;math&amp;gt;\int _a ^b u \frac{\partial u}{\partial t} \operatorname dx = \frac{1}{2} \frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 \quad \text{and} \quad \int _a ^b u \frac{\partial u}{\partial x} \operatorname dx = \frac{1}{2} u(b,t)^2 - \frac{1}{2} u(a,t)^2,.&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;\int _a ^b u \frac{\partial u}{\partial t} \operatorname dx = \frac{1}{2} \frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 \quad \text{and} \quad \int _a ^b u \frac{\partial u}{\partial x} \operatorname dx = \frac{1}{2} u(b,t)^2 - \frac{1}{2} u(a,t)^2,.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
where integration by parts has been used for the second relationship, we get&lt;br /&gt;
&lt;br /&gt;
where integration by parts has been used for the second relationship, we get&lt;br /&gt;
&lt;br /&gt;
第二个关系中采用了分部积分法，我们可以得到&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt;\frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 + \alpha u(b,t)^2 - \alpha u(a,t)^2 = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;\frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 + \alpha u(b,t)^2 - \alpha u(a,t)^2 = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Here &amp;lt;math&amp;gt;\vert \vert \cdot \vert \vert&amp;lt;/math&amp;gt; denotes the standard L2-norm.&lt;br /&gt;
&lt;br /&gt;
Here &amp;lt;math&amp;gt;\vert \vert \cdot \vert \vert&amp;lt;/math&amp;gt; denotes the standard L2-norm.&lt;br /&gt;
&lt;br /&gt;
在这里，&amp;lt;math&amp;gt;\vert \vert \cdot \vert \vert&amp;lt;/math&amp;gt; 表示标准的L2-正则。&lt;br /&gt;
&lt;br /&gt;
For well-posedness we require that the energy of the solution is non-increasing, i.e. that &amp;lt;math&amp;gt;\frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 \leq 0&amp;lt;/math&amp;gt;, which is achieved by specifying &amp;lt;math&amp;gt;u&amp;lt;/math&amp;gt; at &amp;lt;math&amp;gt;x = a&amp;lt;/math&amp;gt; if &amp;lt;math&amp;gt;\alpha &amp;gt; 0&amp;lt;/math&amp;gt; and at &amp;lt;math&amp;gt;x = b&amp;lt;/math&amp;gt; if &amp;lt;math&amp;gt;\alpha &amp;lt; 0&amp;lt;/math&amp;gt;. This corresponds to only imposing boundary conditions at the inflow. Note that well-posedness allows for growth in terms of data (initial and boundary) and thus it is sufficient to show that &amp;lt;math&amp;gt;\frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 \leq 0&amp;lt;/math&amp;gt; holds when all data is set to zero.&lt;br /&gt;
&lt;br /&gt;
For well-posedness we require that the energy of the solution is non-increasing, i.e. that &amp;lt;math&amp;gt;\frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 \leq 0&amp;lt;/math&amp;gt;, which is achieved by specifying &amp;lt;math&amp;gt;u&amp;lt;/math&amp;gt; at &amp;lt;math&amp;gt;x = a&amp;lt;/math&amp;gt; if &amp;lt;math&amp;gt;\alpha &amp;gt; 0&amp;lt;/math&amp;gt; and at &amp;lt;math&amp;gt;x = b&amp;lt;/math&amp;gt; if &amp;lt;math&amp;gt;\alpha &amp;lt; 0&amp;lt;/math&amp;gt;. This corresponds to only imposing boundary conditions at the inflow. Note that well-posedness allows for growth in terms of data (initial and boundary) and thus it is sufficient to show that &amp;lt;math&amp;gt;\frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 \leq 0&amp;lt;/math&amp;gt; holds when all data is set to zero.&lt;br /&gt;
&lt;br /&gt;
对于适定性，我们要求解的能量是不增加的，即 &amp;lt;math&amp;gt;\frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 \leq 0&amp;lt;/math&amp;gt; ，这种关系可以通过在&amp;lt;math&amp;gt;x = a&amp;lt;/math&amp;gt;处 （如果 &amp;lt;math&amp;gt;\alpha &amp;gt; 0&amp;lt;/math&amp;gt;） 以及 &amp;lt;math&amp;gt;x = b&amp;lt;/math&amp;gt;处 （如果 &amp;lt;math&amp;gt;\alpha &amp;lt; 0&amp;lt;/math&amp;gt;）指定&amp;lt;math&amp;gt;u&amp;lt;/math&amp;gt;的值来实现。这相当于只在流入处附加边界条件。注意，适定性允许在数据项(初始和边界)上的增长，因此它足以表明当所有数据设置为零时应有 &amp;lt;math&amp;gt;\frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 \leq 0&amp;lt;/math&amp;gt;。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==Notes==&lt;br /&gt;
&lt;br /&gt;
{{Reflist}}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
== References ==&lt;br /&gt;
&lt;br /&gt;
{{refbegin|2}}&lt;br /&gt;
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|first=G.|last=Adomian|publisher=Kluwer Academic Publishers|year=1994|isbn=|page=|url=https://books.google.com/books?id=UKPqCAAAQBAJ&amp;amp;printsec=frontcover#v=onepage&amp;amp;q=%22partial%20differential%22&amp;amp;f=false}}&lt;br /&gt;
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&lt;br /&gt;
* {{Citation |first=A. D. |last=Polyanin |first2=V. F. |last2=Zaitsev |lastauthoramp=yes |first3=A. |last3=Moussiaux |title=Handbook of First Order Partial Differential Equations |publisher=Taylor &amp;amp; Francis |location=London |year=2002 |isbn=0-415-27267-X }}.&lt;br /&gt;
&lt;br /&gt;
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&lt;br /&gt;
* {{Citation |first=P. |last=Solin |title=Partial Differential Equations and the Finite Element Method |publisher=J. Wiley &amp;amp; Sons |location=Hoboken, NJ |year=2005 |isbn=0-471-72070-4 }}.&lt;br /&gt;
&lt;br /&gt;
* {{Citation |first=P. |last=Solin |first2=K. |last2=Segeth |lastauthoramp=yes |first3=I. |last3=Dolezel |title=Higher-Order Finite Element Methods |publisher=Chapman &amp;amp; Hall/CRC Press |location=Boca Raton |year=2003 |isbn=1-58488-438-X }}.&lt;br /&gt;
&lt;br /&gt;
* {{Citation |first=H. |last=Stephani |year=1989 |title=Differential Equations: Their Solution Using Symmetries. Edited by M. MacCallum |publisher=Cambridge University Press }}.&lt;br /&gt;
&lt;br /&gt;
* {{cite book |title=Partial Differential Equations and Solitary Waves Theory&lt;br /&gt;
&lt;br /&gt;
|first=Abdul-Majid|last=Wazwaz|publisher=Higher Education Press|year=2009|isbn=978-3-642-00251-9|page=}}&lt;br /&gt;
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| first Abdul-Majid | last Wazwaz | publisher Higher Education Press | year 2009 | isbn 978-3-642-00251-9 | page }&lt;br /&gt;
&lt;br /&gt;
* {{cite book |title=Partial Differential Equations Methods and Applications&lt;br /&gt;
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&lt;br /&gt;
| first Abdul-Majid | last Wazwaz | publisher a.a.Balkema | year 2002 | isbn 90-5809-369-7 | page }&lt;br /&gt;
&lt;br /&gt;
* {{Citation |first=D. |last=Zwillinger |title=Handbook of Differential Equations |publisher=Academic Press |location=Boston |year=1997 |edition=3rd |isbn=0-12-784395-7 }}.&lt;br /&gt;
&lt;br /&gt;
* {{Citation |authorlink=Neil Gershenfeld |first=N. |last=Gershenfeld |title=The Nature of Mathematical Modeling |location=New York |publisher=Cambridge University Press, New York, NY, USA |year=1999 |edition=1st |isbn=0-521-57095-6 }}.&lt;br /&gt;
&lt;br /&gt;
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&lt;br /&gt;
* {{Citation |first=I.S. |last=Krasil'shchik |first2=V.V. |last2=Lychagin|lastauthoramp=yes |first3=A.M. |last3=Vinogradov |title=Geometry of Jet Spaces and Nonlinear Partial Differential Equations |publisher=Gordon and Breach Science Publishers, New York, London, Paris, Montreux, Tokyo |year=1986 |isbn=2-88124-051-8 }}.&lt;br /&gt;
&lt;br /&gt;
* {{Citation |first=A.M. |last=Vinogradov |title=Cohomological Analysis of Partial Differential Equations and Secondary Calculus |publisher=American Mathematical Society, Providence, Rhode Island, USA |year=2001 |isbn=0-8218-2922-X }}.&lt;br /&gt;
&lt;br /&gt;
* {{cite book |title=High Order Difference Methods for Time Dependent PDE&lt;br /&gt;
&lt;br /&gt;
|first=Bertil|last=Gustafsson|publisher=Springer|year=2008|isbn=978-3-540-74992-9|doi=10.1007/978-3-540-74993-6}}&lt;br /&gt;
&lt;br /&gt;
|first=Bertil|last=Gustafsson|publisher=Springer|year=2008|isbn=978-3-540-74992-9|doi=10.1007/978-3-540-74993-6}}&lt;br /&gt;
&lt;br /&gt;
| first Bertil | last Gustafsson | Springer | year 2008 | isbn 978-3-540-74992-9 | doi 10.1007 / 978-3-540-74993-6}&lt;br /&gt;
&lt;br /&gt;
{{refend}}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
== Further reading ==&lt;br /&gt;
&lt;br /&gt;
* {{Cite journal|last=Cajori|first=Florian|authorlink=Florian Cajori|year=1928|title=The Early History of Partial Differential Equations and of Partial Differentiation and Integration|url=http://www.math.harvard.edu/archive/21a_fall_14/exhibits/cajori/cajori.pdf|journal=The American Mathematical Monthly|volume=35|issue=9|pages=459–467|doi=10.2307/2298771|access-date=2016-05-15|archive-url=https://web.archive.org/web/20181123102253/http://www.math.harvard.edu/archive/21a_fall_14/exhibits/cajori/cajori.pdf|archive-date=2018-11-23|url-status=dead}}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
== External links ==&lt;br /&gt;
&lt;br /&gt;
{{Sister project links| wikt=no | commons=Category:Solutions of PDE | b=Partial Differential Equations | n=no | q=Partial differential equation | s=no | v=no | voy=no | species=no | d=no}}&lt;br /&gt;
&lt;br /&gt;
* {{springer|title=Differential equation, partial|id=p/d031920}}&lt;br /&gt;
&lt;br /&gt;
* [http://eqworld.ipmnet.ru/en/pde-en.htm Partial Differential Equations: Exact Solutions] at EqWorld: The World of Mathematical Equations.&lt;br /&gt;
&lt;br /&gt;
* [http://eqworld.ipmnet.ru/en/solutions/eqindex/eqindex-pde.htm Partial Differential Equations: Index] at EqWorld: The World of Mathematical Equations.&lt;br /&gt;
&lt;br /&gt;
* [http://eqworld.ipmnet.ru/en/methods/meth-pde.htm Partial Differential Equations: Methods] at EqWorld: The World of Mathematical Equations.&lt;br /&gt;
&lt;br /&gt;
* [https://web.archive.org/web/20170701144823/http://www.exampleproblems.com/wiki/index.php?title=Partial_Differential_Equations Example problems with solutions] at exampleproblems.com&lt;br /&gt;
&lt;br /&gt;
* [http://mathworld.wolfram.com/PartialDifferentialEquation.html Partial Differential Equations] at mathworld.wolfram.com&lt;br /&gt;
&lt;br /&gt;
* [https://reference.wolfram.com/language/FEMDocumentation/tutorial/SolvingPDEwithFEM.html Partial Differential Equations] with Mathematica&lt;br /&gt;
&lt;br /&gt;
* [http://www.mathworks.com/moler/pdes.pdf Partial Differential Equations] in Cleve Moler: Numerical Computing with MATLAB&lt;br /&gt;
&lt;br /&gt;
* [http://www.nag.com/numeric/fl/nagdoc_fl24/html/D03/d03intro.html Partial Differential Equations] at nag.com&lt;br /&gt;
&lt;br /&gt;
* {{cite web |first=Grant |last=Sanderson |title=But what is a partial differential equation? |work=3Blue1Brown |date=April 21, 2019 |url=https://www.youtube.com/watch?v=ly4S0oi3Yz8&amp;amp;list=PLZHQObOWTQDNPOjrT6KVlfJuKtYTftqH6 |via=[[YouTube]] }}&lt;br /&gt;
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&lt;br /&gt;
&lt;br /&gt;
{{Differential equations topics}}&lt;br /&gt;
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{{Authority control}}&lt;br /&gt;
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&lt;br /&gt;
[[Category:Partial differential equations| ]]&lt;br /&gt;
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[[Category:Multivariable calculus]]&lt;br /&gt;
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Category:Multivariable calculus&lt;br /&gt;
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类别: 多元微积分&lt;br /&gt;
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[[Category:Differential equations]]&lt;br /&gt;
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Category:Differential equations&lt;br /&gt;
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类别: 微分方程&lt;br /&gt;
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[[Category:Concepts in physics]]&lt;br /&gt;
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Category:Concepts in physics&lt;br /&gt;
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分类: 物理概念&lt;br /&gt;
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&amp;lt;noinclude&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;small&amp;gt;This page was moved from [[wikipedia:en:Partial differential equation]]. Its edit history can be viewed at [[偏微分方程/edithistory]]&amp;lt;/small&amp;gt;&amp;lt;/noinclude&amp;gt;&lt;br /&gt;
&lt;br /&gt;
[[Category:待整理页面]]&lt;/div&gt;</summary>
		<author><name>Ruili</name></author>
	</entry>
	<entry>
		<id>https://wiki.swarma.org/index.php?title=%E5%81%8F%E5%BE%AE%E5%88%86%E6%96%B9%E7%A8%8B&amp;diff=20107</id>
		<title>偏微分方程</title>
		<link rel="alternate" type="text/html" href="https://wiki.swarma.org/index.php?title=%E5%81%8F%E5%BE%AE%E5%88%86%E6%96%B9%E7%A8%8B&amp;diff=20107"/>
		<updated>2020-12-15T13:42:13Z</updated>

		<summary type="html">&lt;p&gt;Ruili：&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;此词条暂由Yuling翻译，未经人工整理和审校，带来阅读不便，请见谅。&lt;br /&gt;
&lt;br /&gt;
[[File:Heat.gif|thumb|right|A visualisation of a solution to the two-dimensional [[heat equation]] with temperature represented by the third dimension]]&lt;br /&gt;
&lt;br /&gt;
A visualisation of a solution to the two-dimensional [[heat equation with temperature represented by the third dimension]]&lt;br /&gt;
&lt;br /&gt;
以三维表示温度的二维热方程解的可视化&lt;br /&gt;
&lt;br /&gt;
In [[mathematics]], a '''partial differential equation''' ('''PDE''') is a [[differential equation]] that contains unknown [[Multivariable calculus|multivariable functions]] and their [[partial derivative]]s. PDEs are used to formulate problems involving functions of several variables, and are either solved by hand, or used to create a [[computer model]]. A special case is [[ordinary differential equation]]s (ODEs), which deal with functions of a single variable and their derivatives.&lt;br /&gt;
&lt;br /&gt;
In mathematics, a partial differential equation (PDE) is a differential equation that contains unknown multivariable functions and their partial derivatives. PDEs are used to formulate problems involving functions of several variables, and are either solved by hand, or used to create a computer model. A special case is ordinary differential equations (ODEs), which deal with functions of a single variable and their derivatives.&lt;br /&gt;
&lt;br /&gt;
在数学中，'''&amp;lt;font color = &amp;quot;#ff8000&amp;quot;&amp;gt; 偏微分方程函数 Partial Differential Equation&amp;lt;/font&amp;gt;'''是包含未知多元函数及其偏导数的微分方程。偏微分方程用于描述涉及多元函数的问题，可以通过人为求解，也可以通过建立计算机模型来求解。常微分方程是偏微分方程一种特殊情况，它处理的是一元函数及其导数。&lt;br /&gt;
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PDEs can be used to describe a wide variety of phenomena such as sound, heat, [[diffusion]], [[electrostatics]], [[Electromagnetism|electrodynamics]], [[fluid dynamics]], [[Elasticity (physics)|elasticity]], [[gravitation]] and [[quantum mechanics]]. These seemingly distinct physical phenomena can be formalised similarly in terms of PDEs. Just as ordinary differential equations often model one-dimensional [[dynamical system]]s, partial differential equations often model [[multidimensional system]]s. PDEs find their generalisation in [[stochastic partial differential equation]]s.&lt;br /&gt;
&lt;br /&gt;
PDEs can be used to describe a wide variety of phenomena such as sound, heat, diffusion, electrostatics, electrodynamics, fluid dynamics, elasticity, gravitation and quantum mechanics. These seemingly distinct physical phenomena can be formalised similarly in terms of PDEs. Just as ordinary differential equations often model one-dimensional dynamical systems, partial differential equations often model multidimensional systems. PDEs find their generalisation in stochastic partial differential equations.&lt;br /&gt;
&lt;br /&gt;
偏微分方程可以用来描述各种各样的物理现象，如声音，热量，扩散，静电，电动力学，流体力学，弹性力学，重力和量子力学。这些看起来截然不同的物理现象却可以用类似的偏微分方程来描述。正如常微分方程经常对一维动力系统进行建模一样，偏微分方程经常对多维系统进行建模。随机偏微分方程是偏微分方程的一种推广。&lt;br /&gt;
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&lt;br /&gt;
== Introduction ==&lt;br /&gt;
引言&lt;br /&gt;
&lt;br /&gt;
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Partial differential equations (PDEs) are equations that involve rates of change with respect to [[continuous variables]]. For example, the position of a [[rigid body]] is specified by six parameters,&amp;lt;ref&amp;gt;{{Cite book|url=https://books.google.com/books?id=v9PLbcYd9aUC&amp;amp;pg=PA32|title=Modelling and Control of Robot Manipulators|last=Sciavicco|first=Lorenzo|last2=Siciliano|first2=Bruno|date=2001-02-19|publisher=Springer Science &amp;amp; Business Media|isbn=9781852332211|language=en}}&amp;lt;/ref&amp;gt; but the configuration of a [[fluid]] is given by the [[continuous distribution]] of several parameters, such as the [[temperature]], [[pressure]], and so forth. The dynamics for the rigid body take place in a finite-dimensional [[Configuration space (physics)|configuration space]]; the dynamics for the fluid occur in an infinite-dimensional configuration space. This distinction usually makes PDEs much harder to solve than ordinary differential equations (ODEs), but here again, there will be simple solutions for linear problems. Classic domains where PDEs are used include [[acoustics]], [[fluid dynamics]], [[electrodynamics]], and [[heat transfer]].&lt;br /&gt;
&lt;br /&gt;
Partial differential equations (PDEs) are equations that involve rates of change with respect to continuous variables. For example, the position of a rigid body is specified by six parameters, but the configuration of a fluid is given by the continuous distribution of several parameters, such as the temperature, pressure, and so forth. The dynamics for the rigid body take place in a finite-dimensional configuration space; the dynamics for the fluid occur in an infinite-dimensional configuration space. This distinction usually makes PDEs much harder to solve than ordinary differential equations (ODEs), but here again, there will be simple solutions for linear problems. Classic domains where PDEs are used include acoustics, fluid dynamics, electrodynamics, and heat transfer.&lt;br /&gt;
&lt;br /&gt;
偏微分方程(简称为PDEs)涉及到方程相对于连续变量的变化率。例如，刚体的位置是由六个参数确定的，而流体的状态是由几个参数的连续分布给出的，如温度、压力等。刚体的动力学过程发生在有限维状态空间中，流体的动力学过程发生在无限维状态空间中。这种区别通常使偏微分方程比常微分方程更难求解，但是线性问题仍然有简单的求解方式。使用偏微分方程的经典领域包括声学、流体力学、电动力学和传热学。&lt;br /&gt;
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&lt;br /&gt;
A partial differential equation (PDE) for the function {{math|''u''(''x''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;,… ''x&amp;lt;sub&amp;gt;n&amp;lt;/sub&amp;gt;'')}} is an equation of the form&lt;br /&gt;
&lt;br /&gt;
A partial differential equation (PDE) for the function  is an equation of the form&lt;br /&gt;
&lt;br /&gt;
函数 {{math|''u''(''x''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;,… ''x&amp;lt;sub&amp;gt;n&amp;lt;/sub&amp;gt;'')}} 的偏微分方程形式是：&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt;f \left (x_1, \ldots x_n; u, \frac{\partial u}{\partial x_1}, \ldots \frac{\partial u}{\partial x_n}; \frac{\partial^2 u}{\partial x_1 \partial x_1}, \ldots \frac{\partial^2 u}{\partial x_1 \partial x_n}; \ldots \right) = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;f \left (x_1, \ldots x_n; u, \frac{\partial u}{\partial x_1}, \ldots \frac{\partial u}{\partial x_n}; \frac{\partial^2 u}{\partial x_1 \partial x_1}, \ldots \frac{\partial^2 u}{\partial x_1 \partial x_n}; \ldots \right) = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
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If {{mvar|f}} is a [[linear function]] of {{mvar|u}} and its derivatives, then the PDE is called linear. Common examples of linear PDEs include the [[heat equation]], the [[wave equation]], [[Laplace's equation]], [[Helmholtz equation]], [[Klein–Gordon equation]], and [[Poisson's equation]].&lt;br /&gt;
&lt;br /&gt;
If  is a linear function of  and its derivatives, then the PDE is called linear. Common examples of linear PDEs include the heat equation, the wave equation, Laplace's equation, Helmholtz equation, Klein–Gordon equation, and Poisson's equation.&lt;br /&gt;
&lt;br /&gt;
如果 {{mvar|f}} 是函数 {{math|''u''}} 及其导数的线性函数，则偏微分方程称为线性函数。线性偏微分方程的常见例子包括热方程、波动方程、拉普拉斯方程、亥姆霍兹方程方程、克莱因-高登方程和泊松方程。&lt;br /&gt;
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A relatively simple PDE is&lt;br /&gt;
&lt;br /&gt;
A relatively simple PDE is&lt;br /&gt;
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一个相对简单的偏微分方程：&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
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: &amp;lt;math&amp;gt;\frac{\partial u}{\partial x}(x,y) = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;\frac{\partial u}{\partial x}(x,y) = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
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This relation [[Logical implication|implies]] that the function {{math|''u''(''x'',''y'')}} is independent of {{mvar|x}}. However, the equation gives no information on the function's dependence on the variable {{mvar|y}}. Hence the general solution of this equation is&lt;br /&gt;
&lt;br /&gt;
This relation implies that the function  is independent of . However, the equation gives no information on the function's dependence on the variable . Hence the general solution of this equation is&lt;br /&gt;
&lt;br /&gt;
这意味着函数 {{math|''u''(''x'',''y'')}} 独立于 {{mvar|x}} 的。然而，这个方程没有给出关于函数和自变量的相关性的信息。因此，这个方程的通解是&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
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: &amp;lt;math&amp;gt;u(x,y) = f(y),&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;u(x,y) = f(y),&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
where {{mvar|f}} is an arbitrary function of {{mvar|y}}. The analogous ordinary differential equation is&lt;br /&gt;
&lt;br /&gt;
where  is an arbitrary function of . The analogous ordinary differential equation is&lt;br /&gt;
&lt;br /&gt;
其中， {{mvar|f}} 是 {{mvar|y}} 的任意函数。&lt;br /&gt;
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类似的常微分方程是：&lt;br /&gt;
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&lt;br /&gt;
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: &amp;lt;math&amp;gt;\frac{\mathrm{d} u}{\mathrm{d} x}(x) = 0,&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;\frac{\mathrm{d} u}{\mathrm{d} x}(x) = 0,&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
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which has the solution&lt;br /&gt;
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which has the solution&lt;br /&gt;
&lt;br /&gt;
它的解为&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt;u(x) = c,&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;u(x) = c,&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
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&lt;br /&gt;
&lt;br /&gt;
where {{mvar|c}} is any [[Constant (mathematics)|constant]] value. These two examples illustrate that general solutions of ordinary differential equations (ODEs) involve arbitrary constants, but solutions of PDEs involve arbitrary functions.&lt;br /&gt;
&lt;br /&gt;
where  is any constant value. These two examples illustrate that general solutions of ordinary differential equations (ODEs) involve arbitrary constants, but solutions of PDEs involve arbitrary functions.&lt;br /&gt;
&lt;br /&gt;
这里，{{mvar|c}} 是一个任意常量。&lt;br /&gt;
&lt;br /&gt;
这两个例子说明常微分方程的一般解包含任意常数，但偏微分方程的解包含任意函数。&lt;br /&gt;
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A solution of a PDE is generally not [[Uniqueness quantification|unique]]; additional conditions must generally be specified on the [[Boundary (topology)|boundary]] of the region where the solution is defined. For instance, in the simple example above, the function {{math|''f''(''y'')}} can be determined if {{mvar|u}} is specified on the line {{math|''x'' {{=}} 0}}.&lt;br /&gt;
&lt;br /&gt;
A solution of a PDE is generally not unique; additional conditions must generally be specified on the boundary of the region where the solution is defined. For instance, in the simple example above, the function  can be determined if  is specified on the line  0}}.&lt;br /&gt;
&lt;br /&gt;
偏微分方程的解一般不是唯一的; 一般必须在定义解的区域边界上定义附加条件。 例如，在上面的简单示例中，如果在 {{math|''x'' {{=}} 0}} 时确定了 {{mvar|u}} 的值，则可以确定该函数 {{math|''f''(''y'')}}。&lt;br /&gt;
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== Existence and uniqueness ==&lt;br /&gt;
存在性和唯一性&lt;br /&gt;
&lt;br /&gt;
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Although the issue of existence and uniqueness of solutions of ordinary differential equations has a very satisfactory answer with the [[Picard–Lindelöf theorem]], that is far from the case for partial differential equations. The [[Cauchy–Kowalevski theorem]] states that the [[Cauchy problem]] for any partial differential equation whose coefficients are [[Analytic function|analytic]] in the unknown function and its derivatives, has a locally unique analytic solution. Although this result might appear to settle the existence and uniqueness of solutions, there are examples of linear partial differential equations whose coefficients have derivatives of all orders (which are nevertheless not analytic) but which have no solutions at all: see [[Lewy's example|Lewy (1957)]]. Even if the solution of a partial differential equation exists and is unique, it may nevertheless have undesirable properties.  The mathematical study of these questions is usually in the more powerful context of [[weak solution]]s.&lt;br /&gt;
&lt;br /&gt;
Although the issue of existence and uniqueness of solutions of ordinary differential equations has a very satisfactory answer with the Picard–Lindelöf theorem, that is far from the case for partial differential equations. The Cauchy–Kowalevski theorem states that the Cauchy problem for any partial differential equation whose coefficients are analytic in the unknown function and its derivatives, has a locally unique analytic solution. Although this result might appear to settle the existence and uniqueness of solutions, there are examples of linear partial differential equations whose coefficients have derivatives of all orders (which are nevertheless not analytic) but which have no solutions at all: see Lewy (1957). Even if the solution of a partial differential equation exists and is unique, it may nevertheless have undesirable properties.  The mathematical study of these questions is usually in the more powerful context of weak solutions.&lt;br /&gt;
&lt;br /&gt;
尽管常微分方程解的存在性和唯一性用'''&amp;lt;font color=&amp;quot;#ff8000&amp;quot;&amp;gt;弗罗贝尼乌斯定理 Picard–Lindelöf Theorem&amp;lt;/font&amp;gt;得到了令人满意的结果，但偏微分方程解的存在性和唯一性却远没有得到解决。'''&amp;lt;font color=&amp;quot;#ff8000&amp;quot;&amp;gt;柯西-科瓦列夫斯基定理 Cauchy–Kowalevski theorem&amp;lt;/font&amp;gt;指出：对于任意系数在未知函数及其导数中解析的偏微分方程，柯西问题存在一个局部唯一的解析解。虽然这个结果似乎解决了解的存在性和唯一性问题，但是存在一些线性偏微分方程-其系数具有所有级数的导数(尽管这些导数不是解析的) ，但是根本没有解: 见 Lewy (1957)。即使偏微分方程的解存在且唯一，它仍然可能具有不可预料的性质。这些问题的数学研究通常是在更有力的弱解的背景下进行的。&lt;br /&gt;
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An example of pathological behavior is the sequence (depending upon {{mvar|n}}) of [[Cauchy problem]]s for the [[Laplace equation]]&lt;br /&gt;
&lt;br /&gt;
An example of pathological behavior is the sequence (depending upon ) of Cauchy problems for the Laplace equation&lt;br /&gt;
&lt;br /&gt;
反常特征的一个例子是拉普拉斯方程的柯西问题的序列(取决于{{mvar|n}})&lt;br /&gt;
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: &amp;lt;math&amp;gt;\frac{\partial^2 u}{\partial x^2} + \frac{\partial^2 u}{\partial y^2}=0,&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;\frac{\partial^2 u}{\partial x^2} + \frac{\partial^2 u}{\partial y^2}=0,&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
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with [[boundary condition]]s&lt;br /&gt;
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with boundary conditions&lt;br /&gt;
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具有边界条件&lt;br /&gt;
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: &amp;lt;math&amp;gt;\begin{align} u(x,0) &amp;amp;= 0, \\ \frac{\partial u}{\partial y}(x,0) &amp;amp;= \frac{\sin nx}{n}, \end{align}&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;\begin{align} u(x,0) &amp;amp;= 0, \\ \frac{\partial u}{\partial y}(x,0) &amp;amp;= \frac{\sin nx}{n}, \end{align}&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
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where {{mvar|n}} is an integer. The derivative of {{mvar|u}} with respect to {{mvar|y}} approaches zero [[uniform convergence|uniformly]] in {{mvar|x}} as {{mvar|n}} increases, but the solution is&lt;br /&gt;
&lt;br /&gt;
where  is an integer. The derivative of  with respect to  approaches zero uniformly in  as  increases, but the solution is&lt;br /&gt;
&lt;br /&gt;
其中 {{mvar|n}} 是整数。{{mvar|u}} 关于 {{mvar|y}} 的导数，一致地随着 {{mvar|n}} 的增加而趋于零，但解是&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt;u(x,y) = \frac{\sinh ny \sin nx}{n^2}.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;u(x,y) = \frac{\sinh ny \sin nx}{n^2}.&amp;lt;/math&amp;gt;&lt;br /&gt;
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This solution approaches infinity if {{mvar|nx}} is not an integer multiple of {{pi}} for any non-zero value of {{mvar|y}}. The Cauchy problem for the Laplace equation is called ''ill-posed'' or ''not [[Well-posed problem|well-posed]]'', since the solution does not continuously depend on the data of the problem. Such ill-posed problems are not usually satisfactory for physical applications.&lt;br /&gt;
&lt;br /&gt;
This solution approaches infinity if  is not an integer multiple of  for any non-zero value of . The Cauchy problem for the Laplace equation is called ill-posed or not well-posed, since the solution does not continuously depend on the data of the problem. Such ill-posed problems are not usually satisfactory for physical applications.&lt;br /&gt;
&lt;br /&gt;
对于任何非零的 {{mvar|y}}，如果 {{mvar|nx}} 不是模板 {{pi}} 的整数倍，这个解会接近于无穷大。拉普拉斯方程的柯西问题被称为不适定的（可以译为ill-posed或not well-posed），因为解不是连续地依赖于问题的数据。这种不适定问题通常不能满足物理应用。&lt;br /&gt;
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The [[Navier–Stokes existence and smoothness|existence of solutions for the Navier–Stokes equations]], a partial differential equation, is part of one of the [[Millennium Prize Problems]].&lt;br /&gt;
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The existence of solutions for the Navier–Stokes equations, a partial differential equation, is part of one of the Millennium Prize Problems.&lt;br /&gt;
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偏微分方程”纳维-斯托克斯方程“的解的存在性就是千禧年大奖难题之一的一部分。&lt;br /&gt;
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== Notation ==&lt;br /&gt;
符号&lt;br /&gt;
&lt;br /&gt;
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In PDEs, it is common to denote partial derivatives using subscripts. That is:&lt;br /&gt;
&lt;br /&gt;
In PDEs, it is common to denote partial derivatives using subscripts. That is:&lt;br /&gt;
&lt;br /&gt;
在偏微分方程中，通常用下标表示偏导数。例如:&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt;u_x = \frac{\partial u}{\partial x}&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;u_x = \frac{\partial u}{\partial x}&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt;u_{xx} = \frac{\partial^2 u}{\partial x^2} &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;u_{xx} = \frac{\partial^2 u}{\partial x^2} &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt;u_{xy} = \frac{\partial^2 u}{\partial y\, \partial x} = \frac{\partial}{\partial y } \left(\frac{\partial u}{\partial x}\right). &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;u_{xy} = \frac{\partial^2 u}{\partial y\, \partial x} = \frac{\partial}{\partial y } \left(\frac{\partial u}{\partial x}\right). &amp;lt;/math&amp;gt;&lt;br /&gt;
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Especially in physics, [[del]] or nabla ({{math|∇}}) is often used to denote spatial derivatives, and {{math|''&amp;amp;#x307;u'', ''ü''}} for time derivatives. For example, the [[wave equation]] (mentioned below) can be written as&lt;br /&gt;
&lt;br /&gt;
Especially in physics, del or nabla () is often used to denote spatial derivatives, and  for time derivatives. For example, the wave equation (mentioned below) can be written as&lt;br /&gt;
&lt;br /&gt;
特别是在物理学中，[[del]] 或 nabla ({{math|∇}}) 经常用来表示空间导数和时间导数。例如，波动方程(在下文中提到)可以写成：&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt;\ddot u=c^2\nabla^2u&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt;\ddot u=c^2\nabla^2u&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
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&lt;br /&gt;
&lt;br /&gt;
or&lt;br /&gt;
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or&lt;br /&gt;
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或&lt;br /&gt;
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&lt;br /&gt;
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:&amp;lt;math&amp;gt;\ddot u=c^2\Delta u&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt;\ddot u=c^2\Delta u&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
where {{math|Δ}} is the [[Laplace operator]].&lt;br /&gt;
&lt;br /&gt;
where  is the Laplace operator.&lt;br /&gt;
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其中，{{math|Δ}} 代表拉普拉斯算子。&lt;br /&gt;
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== Classification ==&lt;br /&gt;
分类&lt;br /&gt;
&lt;br /&gt;
Some linear, second-order partial differential equations can be classified as [[parabolic partial differential equation|parabolic]], [[hyperbolic partial differential equation|hyperbolic]] and [[elliptic partial differential equation|elliptic]]. Others, such as the [[Euler–Tricomi equation]], have different types in different regions. The classification provides a guide to appropriate initial and boundary conditions and to the smoothness of the solutions.&lt;br /&gt;
&lt;br /&gt;
Some linear, second-order partial differential equations can be classified as parabolic, hyperbolic and elliptic. Others, such as the Euler–Tricomi equation, have different types in different regions. The classification provides a guide to appropriate initial and boundary conditions and to the smoothness of the solutions.&lt;br /&gt;
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一些线性二阶偏微分方程可分为抛物型方程、双曲型方程和椭圆型方程。其他的方程，如欧拉-特里科米方程，在不同的领域有不同的类型。这种分类有助于选择适当的初始和边界条件以及提高解的平滑性。&lt;br /&gt;
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&lt;br /&gt;
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=== Equations of first order ===&lt;br /&gt;
一阶方程&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{{main|First-order partial differential equation}}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
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=== Linear equations of second order ===&lt;br /&gt;
二阶线性方程&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Assuming {{math|''u&amp;lt;sub&amp;gt;xy&amp;lt;/sub&amp;gt;'' {{=}} ''u&amp;lt;sub&amp;gt;yx&amp;lt;/sub&amp;gt;''}}, the general linear second-order PDE in two independent variables has the form&lt;br /&gt;
&lt;br /&gt;
Assuming  u&amp;lt;sub&amp;gt;yx&amp;lt;/sub&amp;gt;}}, the general linear second-order PDE in two independent variables has the form&lt;br /&gt;
&lt;br /&gt;
假设 {{math|''u&amp;lt;sub&amp;gt;xy&amp;lt;/sub&amp;gt;'' {{=}} ''u&amp;lt;sub&amp;gt;yx&amp;lt;/sub&amp;gt;''}}，含有两个独立变量的一般线性二阶偏微分方程具有如下形式：&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt;Au_{xx} + 2Bu_{xy} + Cu_{yy} + \cdots \mbox{(lower order terms)} = 0,&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;Au_{xx} + 2Bu_{xy} + Cu_{yy} + \cdots \mbox{(lower order terms)} = 0,&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
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where the coefficients {{mvar|A}}, {{mvar|B}}, {{mvar|C}}... may depend upon {{mvar|x}} and {{mvar|y}}. If {{math|''A''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; + ''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; + ''C''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; &amp;gt; 0}} over a region of the {{mvar|xy}}-plane, the PDE is second-order in that region. This form is analogous to the equation for a conic section:&lt;br /&gt;
&lt;br /&gt;
where the coefficients , , ... may depend upon  and . If  over a region of the -plane, the PDE is second-order in that region. This form is analogous to the equation for a conic section:&lt;br /&gt;
&lt;br /&gt;
其中的系数 {{mvar|A}}, {{mvar|B}}, {{mvar|C}}... 一般取决于 {{mvar|x}} 和 {{mvar|y}} 。如果在 {{mvar|xy}}-平面的一个区域上 {{math|''A''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; + ''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; + ''C''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; &amp;gt; 0}}，偏微分方程是二阶的，这种形式类似于圆锥截面的方程:&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt;Ax^2 + 2Bxy + Cy^2 + \cdots = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;Ax^2 + 2Bxy + Cy^2 + \cdots = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
More precisely, replacing {{math|∂&amp;lt;sub&amp;gt;''x''&amp;lt;/sub&amp;gt;}} by {{mvar|X}}, and likewise for other variables (formally this is done by a [[Fourier transform]]), converts a constant-coefficient PDE into a polynomial of the same degree, with the terms of the highest degree (a [[homogeneous polynomial]], here a [[quadratic form]]) being most significant for the classification.&lt;br /&gt;
&lt;br /&gt;
More precisely, replacing  by , and likewise for other variables (formally this is done by a Fourier transform), converts a constant-coefficient PDE into a polynomial of the same degree, with the terms of the highest degree (a homogeneous polynomial, here a quadratic form) being most significant for the classification.&lt;br /&gt;
&lt;br /&gt;
更准确地说，用 {{mvar|X}} 替换 {{math|∂&amp;lt;sub&amp;gt;''x''&amp;lt;/sub&amp;gt;}}，并同样替换其它变量(通常由傅里叶变换完成)，将一个常系数偏微分方程转换成一个相同次数的多项式，最高次数的项(齐次多项式，这里是一个二次形式)对于偏微分方程的分类最为重要。&lt;br /&gt;
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Just as one classifies [[conic section]]s and quadratic forms into parabolic, hyperbolic, and elliptic based on the [[discriminant]] {{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − 4''AC''}}, the same can be done for a second-order PDE at a given point.  However, the [[discriminant]] in a PDE is given by {{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC''}} due to the convention of the {{mvar|xy}} term being {{math|2''B''}} rather than {{mvar|B}}; formally, the discriminant (of the associated quadratic form) is {{math|(2''B'')&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − 4''AC'' {{=}} 4(''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC'')}}, with the factor of 4 dropped for simplicity.&lt;br /&gt;
&lt;br /&gt;
Just as one classifies conic sections and quadratic forms into parabolic, hyperbolic, and elliptic based on the discriminant , the same can be done for a second-order PDE at a given point.  However, the discriminant in a PDE is given by  due to the convention of the  term being  rather than ; formally, the discriminant (of the associated quadratic form) is  4(B&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − AC)}}, with the factor of 4 dropped for simplicity.&lt;br /&gt;
&lt;br /&gt;
正如人们可以根据判别式 {{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − 4''AC''}} 将圆锥截面和二次型分为抛物型、双曲型和椭圆型一样，对于给定点的二阶偏微分方程也可以这样做。然而，偏微分方程中的判别式 {{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − 4''AC''}} 是根据交叉项的系数{{math|2''B''}} 而不是 {{mvar|B}} 给出的，形式上，判别式(关联二次型)是 {{math|(2''B'')&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − 4''AC'' {{=}} 4(''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC'')}}，为简单起见，去掉了因子4。&lt;br /&gt;
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# {{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC'' &amp;lt; 0}} (''[[elliptic partial differential equation]]''): Solutions of [[elliptic partial differential equation|elliptic PDEs]] are as smooth as the coefficients allow, within the interior of the region where the equation and solutions are defined. For example, solutions of [[Laplace's equation]] are analytic within the domain where they are defined, but solutions may assume boundary values that are not smooth. The motion of a fluid at subsonic speeds can be approximated with elliptic PDEs, and the Euler–Tricomi equation is elliptic where {{math|''x'' &amp;lt; 0}}.&lt;br /&gt;
&lt;br /&gt;
  (elliptic partial differential equation): Solutions of elliptic PDEs are as smooth as the coefficients allow, within the interior of the region where the equation and solutions are defined. For example, solutions of Laplace's equation are analytic within the domain where they are defined, but solutions may assume boundary values that are not smooth. The motion of a fluid at subsonic speeds can be approximated with elliptic PDEs, and the Euler–Tricomi equation is elliptic where .&lt;br /&gt;
&lt;br /&gt;
{{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC'' &amp;lt; 0}} (椭圆型微分方程)：在定义方程和解的区域内部，椭圆型偏微分方程的解在系数允许的程度内光滑。例如，拉普拉斯方程的解在它们被定义的区域内是解析的，但可能假设边界值是不光滑的。亚音速流体的运动可以用椭圆型偏微分方程近似，欧拉-特里科米方程在 {{math|''x'' &amp;lt; 0}} 时是椭圆型偏微分方程。&lt;br /&gt;
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# {{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC'' {{=}} 0}} (''[[parabolic partial differential equation]]''): Equations that are [[parabolic partial differential equation|parabolic]] at every point can be transformed into a form analogous to the [[heat equation]] by a change of independent variables. Solutions smooth out as the transformed time variable increases. The Euler–Tricomi equation has parabolic type on the line where {{math|''x'' {{=}} 0}}.&lt;br /&gt;
&lt;br /&gt;
  0}} (parabolic partial differential equation): Equations that are parabolic at every point can be transformed into a form analogous to the heat equation by a change of independent variables. Solutions smooth out as the transformed time variable increases. The Euler–Tricomi equation has parabolic type on the line where  0}}.&lt;br /&gt;
&lt;br /&gt;
{{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC'' {{=}} 0}}（抛物型偏微分方程）：在每一点上都是抛物线型的方程可以通过改变自变量从而转化成类似于热方程的形式。随着转换后的时间变量的增加，方程的解变得平滑。欧拉-特里科米方程在特征线 {{math|''x'' {{=}} 0}} 上是抛物线型的。&lt;br /&gt;
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&lt;br /&gt;
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# {{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC'' &amp;gt; 0}} (''[[hyperbolic partial differential equation]]''): [[hyperbolic partial differential equation|hyperbolic]] equations retain any discontinuities of functions or derivatives in the initial data. An example is the [[wave equation]]. The motion of a fluid at supersonic speeds can be approximated with hyperbolic PDEs, and the Euler–Tricomi equation is hyperbolic where {{math|''x'' &amp;gt; 0}}.&lt;br /&gt;
&lt;br /&gt;
  (hyperbolic partial differential equation): hyperbolic equations retain any discontinuities of functions or derivatives in the initial data. An example is the wave equation. The motion of a fluid at supersonic speeds can be approximated with hyperbolic PDEs, and the Euler–Tricomi equation is hyperbolic where .&lt;br /&gt;
&lt;br /&gt;
{{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC'' &amp;gt; 0}} (双曲型偏微分方程)：双曲型方程在初始数据中保留了函数或导数的任何不连续性。波动方程就是其中的一个例子。超音速流体的运动可以用双曲型偏微分方程近似，欧拉-特里科米方程在 {{math|''x'' &amp;gt; 0}} 时是双曲型的。&lt;br /&gt;
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If there are {{mvar|n}} independent variables {{math|''x''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;, ''x''&amp;lt;sub&amp;gt;2 &amp;lt;/sub&amp;gt;,… ''x''&amp;lt;sub&amp;gt;''n''&amp;lt;/sub&amp;gt;}}, a general linear partial differential equation of second order has the form&lt;br /&gt;
&lt;br /&gt;
If there are  independent variables , a general linear partial differential equation of second order has the form&lt;br /&gt;
&lt;br /&gt;
如果存在 {{mvar|n}} 个自变量 {{math|''x''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;, ''x''&amp;lt;sub&amp;gt;2 &amp;lt;/sub&amp;gt;,… ''x''&amp;lt;sub&amp;gt;''n''&amp;lt;/sub&amp;gt;}}，一般二阶线性偏微分方程的形式是：&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt;L u =\sum_{i=1}^n\sum_{j=1}^n a_{i,j} \frac{\partial^2 u}{\partial x_i \partial x_j} \quad \text{ plus lower-order terms} =0.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;L u =\sum_{i=1}^n\sum_{j=1}^n a_{i,j} \frac{\partial^2 u}{\partial x_i \partial x_j} \quad \text{ plus lower-order terms} =0.&amp;lt;/math&amp;gt;&lt;br /&gt;
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The classification depends upon the signature of the eigenvalues of the coefficient matrix {{math|''a''&amp;lt;sub&amp;gt;''i'',''j''&amp;lt;/sub&amp;gt;}}.&lt;br /&gt;
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The classification depends upon the signature of the eigenvalues of the coefficient matrix .&lt;br /&gt;
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这种分类取决于系数矩阵特征值的符号（正负性）。&lt;br /&gt;
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# Elliptic: the eigenvalues are all positive or all negative.&lt;br /&gt;
&lt;br /&gt;
 Elliptic: the eigenvalues are all positive or all negative.&lt;br /&gt;
&lt;br /&gt;
椭圆形方程: 特征值全部为正或全部为负。&lt;br /&gt;
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# Parabolic: the eigenvalues are all positive or all negative, save one that is zero.&lt;br /&gt;
&lt;br /&gt;
 Parabolic: the eigenvalues are all positive or all negative, save one that is zero.&lt;br /&gt;
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抛物线形方程:除了一个为零值，特征值全部为正或全部为负。&lt;br /&gt;
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# Hyperbolic: there is only one negative eigenvalue and all the rest are positive, or there is only one positive eigenvalue and all the rest are negative.&lt;br /&gt;
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 Hyperbolic: there is only one negative eigenvalue and all the rest are positive, or there is only one positive eigenvalue and all the rest are negative.&lt;br /&gt;
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双曲形方程: 只有一个负特征值，其余的都是正特征值，或者只有一个正特征值，其余的都是负特征值。&lt;br /&gt;
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# Ultrahyperbolic: there is more than one positive eigenvalue and more than one negative eigenvalue, and there are no zero eigenvalues. There is only a limited theory for ultrahyperbolic equations (Courant and Hilbert, 1962).&lt;br /&gt;
&lt;br /&gt;
 Ultrahyperbolic: there is more than one positive eigenvalue and more than one negative eigenvalue, and there are no zero eigenvalues. There is only a limited theory for ultrahyperbolic equations (Courant and Hilbert, 1962).&lt;br /&gt;
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超双形方程: 存在多于一个正特征值和多于一个的负特征值，且不存在零特征值。对于超双曲方程，只存在有限的理论(Courant 和 Hilbert，1962)。&lt;br /&gt;
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=== Systems of first-order equations and characteristic surfaces ===&lt;br /&gt;
一阶方程组和特征曲面&lt;br /&gt;
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The classification of partial differential equations can be extended to systems of first-order equations, where the unknown {{mvar|u}} is now a [[Euclidean vector|vector]] with {{mvar|m}} components, and the coefficient matrices {{mvar|A&amp;lt;sub&amp;gt;ν&amp;lt;/sub&amp;gt;}} are {{mvar|m}} by {{mvar|m}} matrices for {{math|''ν'' {{=}} 1, 2,… ''n''}}. The partial differential equation takes the form&lt;br /&gt;
&lt;br /&gt;
The classification of partial differential equations can be extended to systems of first-order equations, where the unknown  is now a vector with  components, and the coefficient matrices  are  by  matrices for  1, 2,… n}}. The partial differential equation takes the form&lt;br /&gt;
&lt;br /&gt;
偏微分方程的分类可以推广到一阶方程组，其中未知量 {{mvar|u}} 是有 {{mvar|m}} 个分量的向量。对于 {{math|''ν'' {{=}} 1, 2,… ''n''}}，系数矩阵 {{mvar|A&amp;lt;sub&amp;gt;ν&amp;lt;/sub&amp;gt;}} 是 {{mvar|m}} × {{mvar|m}} 的矩阵。偏微分方程形式如下：&lt;br /&gt;
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: &amp;lt;math&amp;gt;Lu = \sum_{\nu=1}^{n} A_\nu \frac{\partial u}{\partial x_\nu} + B=0,&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;Lu = \sum_{\nu=1}^{n} A_\nu \frac{\partial u}{\partial x_\nu} + B=0,&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
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where the coefficient matrices {{mvar|A&amp;lt;sub&amp;gt;ν&amp;lt;/sub&amp;gt;}} and the vector {{mvar|B}} may depend upon {{mvar|x}} and {{mvar|u}}. If a [[hypersurface]] {{mvar|S}} is given in the implicit form&lt;br /&gt;
&lt;br /&gt;
where the coefficient matrices  and the vector  may depend upon  and . If a hypersurface  is given in the implicit form&lt;br /&gt;
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其中，系数矩阵 {{mvar|A&amp;lt;sub&amp;gt;ν&amp;lt;/sub&amp;gt;}} 和向量 {{mvar|B}} 可能依赖于 {{mvar|x}} 和 {{mvar|u}}。如果超曲面是以以下隐式形式给出的，&lt;br /&gt;
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: &amp;lt;math&amp;gt;\varphi(x_1, x_2, \ldots x_n)=0,&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;\varphi(x_1, x_2, \ldots x_n)=0,&amp;lt;/math&amp;gt;&lt;br /&gt;
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where {{mvar|φ}} has a non-zero gradient, then {{mvar|S}} is a '''characteristic surface''' for the operator {{mvar|L}} at a given point if the characteristic form vanishes:&lt;br /&gt;
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where  has a non-zero gradient, then  is a characteristic surface for the operator  at a given point if the characteristic form vanishes:&lt;br /&gt;
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其中，存在一个非零的梯度 {{mvar|φ}}，对于在给定点上特征形式消失的算子，特征曲面 {{mvar|S}} 形式如下:&lt;br /&gt;
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: &amp;lt;math&amp;gt;Q\left(\frac{\partial\varphi}{\partial x_1}, \ldots\frac{\partial\varphi}{\partial x_n}\right) =\det\left[\sum_{\nu=1}^nA_\nu \frac{\partial \varphi}{\partial x_\nu}\right]=0.\,&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;Q\left(\frac{\partial\varphi}{\partial x_1}, \ldots\frac{\partial\varphi}{\partial x_n}\right) =\det\left[\sum_{\nu=1}^nA_\nu \frac{\partial \varphi}{\partial x_\nu}\right]=0.\,&amp;lt;/math&amp;gt;&lt;br /&gt;
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The geometric interpretation of this condition is as follows: if data for {{mvar|u}} are prescribed on the surface {{mvar|S}}, then it may be possible to determine the normal derivative of {{mvar|u}} on {{mvar|S}} from the differential equation. If the data on {{mvar|S}} and the differential equation determine the normal derivative of {{mvar|u}} on {{mvar|S}}, then {{mvar|S}} is non-characteristic. If the data on {{mvar|S}} and the differential equation ''do not'' determine the normal derivative of {{mvar|u}} on {{mvar|S}}, then the surface is '''characteristic''', and the differential equation restricts the data on {{mvar|S}}: the differential equation is ''internal'' to {{mvar|S}}.&lt;br /&gt;
&lt;br /&gt;
The geometric interpretation of this condition is as follows: if data for  are prescribed on the surface , then it may be possible to determine the normal derivative of  on  from the differential equation. If the data on  and the differential equation determine the normal derivative of  on , then  is non-characteristic. If the data on  and the differential equation do not determine the normal derivative of  on , then the surface is characteristic, and the differential equation restricts the data on : the differential equation is internal to .&lt;br /&gt;
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这个条件的几何解释如下: 如果关于 {{mvar|u}} 的数据是在曲面 {{mvar|S}} 上规定的，那么就有可能依据微分方程确定曲面 {{mvar|S}} 上 {{mvar|u}} 的法向导数。如果曲面 {{mvar|S}} 上的数据和上面的微分方程能确定曲面 {{mvar|S}} 上 {{mvar|u}} 的法向导数，那么它就是非特征的。如果曲面 {{mvar|S}} 上的数据和上面的微分方程不能确定曲面 {{mvar|S}} 上 {{mvar|u}} 的法向导数，那么曲面是特征的，并且微分方程将数据限制在曲面 {{mvar|S}} 上：微分方程是在曲面 {{mvar|S}} 内部。&lt;br /&gt;
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# A first-order system {{math|''Lu'' {{=}} 0}} is ''elliptic'' if no surface is characteristic for {{mvar|L}}: the values of {{mvar|u}} on {{mvar|S}} and the differential equation always determine the normal derivative of {{mvar|u}} on {{mvar|S}}.&lt;br /&gt;
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 A first-order system  0}} is elliptic if no surface is characteristic for : the values of  on  and the differential equation always determine the normal derivative of  on .&lt;br /&gt;
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如果对于 {{mvar|L}} 没有曲面是特征的，则一阶系统 {{math|''Lu'' {{=}} 0}} 是椭圆形的：{{mvar|u}}在 {{mvar|S}} 的值和微分方程总能够决定 {{mvar|S}} 上 {{mvar|u}} 的法向导数。&lt;br /&gt;
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# A first-order system is ''hyperbolic'' at a point if there is a '''spacelike''' surface {{mvar|S}} with normal {{mvar|ξ}} at that point. This means that, given any non-trivial vector {{mvar|η}} orthogonal to {{mvar|ξ}}, and a scalar multiplier {{mvar|λ}}, the equation {{math|''Q''(''λξ'' + ''η'') {{=}} 0}} has {{mvar|m}} real roots {{math|''λ''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;, ''λ''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;,… ''λ''&amp;lt;sub&amp;gt;''m''&amp;lt;/sub&amp;gt;}}. The system is '''strictly hyperbolic''' if these roots are always distinct. The geometrical interpretation of this condition is as follows: the characteristic form {{math|''Q''(''ζ'') {{=}} 0}} defines a cone (the normal cone) with homogeneous coordinates ζ. In the hyperbolic case, this cone has {{mvar|m}} sheets, and the axis {{math|''ζ'' {{=}} ''λξ''}} runs inside these sheets: it does not intersect any of them. But when displaced from the origin by η, this axis intersects every sheet. In the elliptic case, the normal cone has no real sheets.&lt;br /&gt;
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 A first-order system is hyperbolic at a point if there is a spacelike surface  with normal  at that point. This means that, given any non-trivial vector  orthogonal to , and a scalar multiplier , the equation  0}} has  real roots . The system is strictly hyperbolic if these roots are always distinct. The geometrical interpretation of this condition is as follows: the characteristic form  0}} defines a cone (the normal cone) with homogeneous coordinates ζ. In the hyperbolic case, this cone has  sheets, and the axis  λξ}} runs inside these sheets: it does not intersect any of them. But when displaced from the origin by η, this axis intersects every sheet. In the elliptic case, the normal cone has no real sheets.&lt;br /&gt;
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如果在该点存在一个法向量为 {{mvar|ξ}}的 '''&amp;lt;font color=&amp;quot;#ff8000&amp;quot;&amp;gt;类空曲面 Spacclike Surface&amp;lt;/font&amp;gt; {{mvar|S}} ，则一阶系统在那一点是双曲的。这意味着，给定任意正交于 {{mvar|ξ}} 的非平凡向量 {{mvar|η}} 和一个标量乘子 {{mvar|λ}}，方程 {{math|''Q''(''λξ'' + ''η'') {{=}} 0}} 有 {{mvar|m}} 个实根 {{math|''λ''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;, ''λ''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;,… ''λ''&amp;lt;sub&amp;gt;''m''&amp;lt;/sub&amp;gt;}}。如果这些根始终不同，则该系统是严格双曲形的。这个条件的几何解释如下: 特征形式 {{math|''Q''(''ζ'') {{=}} 0}} 定义了一个具有齐次坐标 ζ的圆锥(法线圆锥)。在双曲形的情况下，这个圆锥体有 {{mvar|m}} 层，并且轴 {{math|''ζ'' {{=}} ''λξ''}} 在这些层中运动: 它不与任何一层相交。但是当从原点偏离η时，这条轴线与每一层都相交。在椭圆形的情况下，法向圆锥没有实层。&lt;br /&gt;
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==[[用户:Yuling|Yuling]]（[[用户讨论:Yuling|讨论]]） sheet 这个单词也不很理解，我直译为了“层”&lt;br /&gt;
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=== Equations of mixed type ===&lt;br /&gt;
混合型方程&lt;br /&gt;
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If a PDE has coefficients that are not constant, it is possible that it will not belong to any of these categories but rather be of '''mixed type'''. A simple but important example is the [[Euler–Tricomi equation]]&lt;br /&gt;
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If a PDE has coefficients that are not constant, it is possible that it will not belong to any of these categories but rather be of mixed type. A simple but important example is the Euler–Tricomi equation&lt;br /&gt;
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如果偏微分方程的系数不是常数，那么它可能不属于这些类别中的任何一个，而是属于混合类型。一个简单但重要的例子是欧拉-特里科米方程&lt;br /&gt;
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: &amp;lt;math&amp;gt;u_{xx} = xu_{yy},&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;u_{xx} = xu_{yy},&amp;lt;/math&amp;gt;&lt;br /&gt;
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which is called '''elliptic-hyperbolic''' because it is elliptic in the region {{math|''x'' &amp;lt; 0}}, hyperbolic in the region {{math|''x'' &amp;gt; 0}}, and degenerate parabolic on the line {{math|''x'' {{=}} 0}}.&lt;br /&gt;
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which is called elliptic-hyperbolic because it is elliptic in the region , hyperbolic in the region , and degenerate parabolic on the line  0}}.&lt;br /&gt;
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它在 {{math|''x'' &amp;lt; 0}} 的区域上是椭圆形，在 {{math|''x'' &amp;gt; 0}} 区域上是双曲形，在 {{math|''x'' {{=}} 0}}这条线上是退化为抛物线形，因此称之为椭圆-双曲型。&lt;br /&gt;
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&amp;lt;!--&lt;br /&gt;
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&amp;lt;!--&lt;br /&gt;
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&amp;lt;!--&lt;br /&gt;
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''fill in: Dirichlet and Neumann boundaries, hyperbolic/parabolic/elliptic separation of variables, [[Fourier analysis]], [[Green's function]]s ...--&amp;gt;&lt;br /&gt;
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fill in: Dirichlet and Neumann boundaries, hyperbolic/parabolic/elliptic separation of variables, Fourier analysis, Green's functions ...--&amp;gt;&lt;br /&gt;
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填写: Dirichlet 和 Neumann 边界，双曲 / 抛物线 / 椭圆分离变量法，傅立叶分析，Green 函数... --&lt;br /&gt;
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=== Infinite-order PDEs in quantum mechanics ===&lt;br /&gt;
量子力学中的无限阶偏微分方程&lt;br /&gt;
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In the [[phase space formulation]] of quantum mechanics,  one may consider the [[Method of quantum characteristics|quantum Hamilton's equations]] for trajectories of quantum particles. These equations are infinite-order PDEs. However, in the semiclassical expansion, one has a finite system of ODEs at any fixed order of [[Dirac constant|{{mvar|ħ}}]].  The evolution equation of the [[Wigner quasi-probability distribution|c]] is also an infinite-order PDE. The quantum trajectories are [[Method of quantum characteristics|quantum characteristics]], with the use of which one could calculate the evolution of the Wigner function.&lt;br /&gt;
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In the phase space formulation of quantum mechanics,  one may consider the quantum Hamilton's equations for trajectories of quantum particles. These equations are infinite-order PDEs. However, in the semiclassical expansion, one has a finite system of ODEs at any fixed order of Dirac constant|.  The evolution equation of the Wigner function is also an infinite-order PDE. The quantum trajectories are quantum characteristics, with the use of which one could calculate the evolution of the Wigner function.&lt;br /&gt;
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在量子力学中的相空间表述中，我们可以考虑用于求解量子粒子的轨迹的量子哈密顿的方程。这些方程是无限阶偏微分方程。然而，在半经典展开中，我们在给定[[Dirac constant|{{mvar|ħ}}]]阶数下有一个有限的的常微分方程组。'''&amp;lt;font color=&amp;quot;#ff8000&amp;quot;&amp;gt;维格纳函数  Wigner Function&amp;lt;/font&amp;gt;的演化方程也是一个无限阶偏微分方程。由于量子轨道的量子特性，所以它通常可以用来计算维格纳函数的演化。&lt;br /&gt;
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== Analytical solutions ==&lt;br /&gt;
解析解&lt;br /&gt;
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===Separation of variables===&lt;br /&gt;
分离变量法&lt;br /&gt;
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{{main|Separable partial differential equation}}&lt;br /&gt;
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Linear PDEs can be reduced to systems of ordinary differential equations by the important technique of separation of variables. This technique rests on a characteristic of solutions to differential equations: if one can find any solution that solves the equation and satisfies the boundary conditions, then it is ''the'' solution (this also applies to ODEs). We assume as an [[ansatz]] that the dependence of a solution on the parameters space and time can be written as a product of terms that each depend on a single parameter, and then see if this can be made to solve the problem.&amp;lt;ref&amp;gt;{{cite book|last1=Gershenfeld|first1=Neil|title=The nature of mathematical modeling|date=2000|publisher=Cambridge Univ. Press|location=Cambridge|isbn=0521570956|page=27|edition=Reprinted (with corr.)}}&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
Linear PDEs can be reduced to systems of ordinary differential equations by the important technique of separation of variables. This technique rests on a characteristic of solutions to differential equations: if one can find any solution that solves the equation and satisfies the boundary conditions, then it is the solution (this also applies to ODEs). We assume as an ansatz that the dependence of a solution on the parameters space and time can be written as a product of terms that each depend on a single parameter, and then see if this can be made to solve the problem.&lt;br /&gt;
&lt;br /&gt;
线性偏微分方程组可以通过分离变量法这一重要方法来简化为常微分方程组。这种方法依赖于微分方程解的一个特征: 如果能找到任何一个满足方程和边界条件的解，那么这个解就是方程的解(这也适用于常微分方程)。我们假设解对参数空间和时间的依赖可以写成对它们每一项的依赖以及一个参数的乘积，然后再看看这是否可以用来解决这个问题。&lt;br /&gt;
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In the method of separation of variables, one reduces a PDE to a PDE in fewer variables, which is an ordinary differential equation if in one variable – these are in turn easier to solve.&lt;br /&gt;
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In the method of separation of variables, one reduces a PDE to a PDE in fewer variables, which is an ordinary differential equation if in one variable – these are in turn easier to solve.&lt;br /&gt;
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在分离变量法方法中，可以将偏微分方程简化为含有更少变量的偏微分方程，如果只有一个变量，那么就变成了一个'''&amp;lt;font color = &amp;quot;#ff8000&amp;quot;&amp;gt;常微分方程 Ordinary Differential Equation&amp;lt;/font&amp;gt;'''-- 反过来，这些方程也更容易求解。&lt;br /&gt;
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This is possible for simple PDEs, which are called [[separable partial differential equation]]s, and the domain is generally a rectangle (a product of intervals). Separable PDEs correspond to [[diagonal matrices]] – thinking of &amp;quot;the value for fixed {{mvar|x}}&amp;quot; as a coordinate, each coordinate can be understood separately.&lt;br /&gt;
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This is possible for simple PDEs, which are called separable partial differential equations, and the domain is generally a rectangle (a product of intervals). Separable PDEs correspond to diagonal matrices – thinking of &amp;quot;the value for fixed &amp;quot; as a coordinate, each coordinate can be understood separately.&lt;br /&gt;
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对于简单的偏微分方程(称为可分离偏微分方程)来说，这是可能的，而且方程通常定义在一个矩形区域(区间的乘积)上。可分离偏微分方程对应于对角线矩阵——以“固定值”为坐标，每个坐标可分开理解。&lt;br /&gt;
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This generalizes to the [[method of characteristics]], and is also used in [[integral transform]]s.&lt;br /&gt;
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This generalizes to the method of characteristics, and is also used in integral transforms.&lt;br /&gt;
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这种方法可以推广到特征曲线法，也可以用于积分变换。&lt;br /&gt;
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===Method of characteristics===&lt;br /&gt;
特征曲线法&lt;br /&gt;
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{{main|Method of characteristics}}&lt;br /&gt;
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In special cases, one can find characteristic curves on which the equation reduces to an ODE – changing coordinates in the domain to straighten these curves allows separation of variables, and is called the [[method of characteristics]].&lt;br /&gt;
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In special cases, one can find characteristic curves on which the equation reduces to an ODE – changing coordinates in the domain to straighten these curves allows separation of variables, and is called the method of characteristics.&lt;br /&gt;
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在特殊情况下，可以找到一些特征曲线，在这些曲线上方程可以变成一个常微分方程——意味着改变坐标从而使这些曲线变直从而达到分离变量的目的，这就是所谓的特征曲线法。&lt;br /&gt;
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More generally, one may find characteristic surfaces.&lt;br /&gt;
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More generally, one may find characteristic surfaces.&lt;br /&gt;
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更一般地说，人们可能会找到特征表面。&lt;br /&gt;
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===Integral transform===&lt;br /&gt;
积分变换&lt;br /&gt;
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An [[integral transform]] may transform the PDE to a simpler one, in particular, a separable PDE. This corresponds to diagonalizing an operator.&lt;br /&gt;
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An integral transform may transform the PDE to a simpler one, in particular, a separable PDE. This corresponds to diagonalizing an operator.&lt;br /&gt;
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积分变换可以将偏微分方程转换为更简单的偏微分方程，特别是可分离的偏微分方程。这对应于对角化算符。&lt;br /&gt;
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An important example of this is [[Fourier analysis]], which diagonalizes the heat equation using the [[eigenbasis]] of sinusoidal waves.&lt;br /&gt;
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An important example of this is Fourier analysis, which diagonalizes the heat equation using the eigenbasis of sinusoidal waves.&lt;br /&gt;
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这方面的一个重要例子是'''&amp;lt;font color = &amp;quot;#ff8000&amp;quot;&amp;gt;傅里叶分析  Fourier Analysis&amp;lt;/font&amp;gt;'''，它使用正弦波的特征基来对角化热方程。&lt;br /&gt;
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If the domain is finite or periodic, an infinite sum of solutions such as a [[Fourier series]] is appropriate, but an integral of solutions such as a [[Fourier integral]] is generally required for infinite domains. The solution for a point source for the heat equation given above is an example of the use of a Fourier integral.&lt;br /&gt;
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If the domain is finite or periodic, an infinite sum of solutions such as a Fourier series is appropriate, but an integral of solutions such as a Fourier integral is generally required for infinite domains. The solution for a point source for the heat equation given above is an example of the use of a Fourier integral.&lt;br /&gt;
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如果区域是有限的或周期性的，那么解为无限和的形式是恰当的，例如傅里叶级数，但是一个解的积分，例如傅立叶积分，一般是在无限区域上的。上面给出的热传导方程的点源解法就是使用傅里叶积分的一个例子。&lt;br /&gt;
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===Change of variables===&lt;br /&gt;
变量代换&lt;br /&gt;
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Often a PDE can be reduced to a simpler form with a known solution by a suitable [[Change of variables (PDE)|change of variables]].  For example, the [[Black–Scholes equation#Derivation|Black–Scholes]] PDE&lt;br /&gt;
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Often a PDE can be reduced to a simpler form with a known solution by a suitable change of variables.  For example, the Black–Scholes PDE&lt;br /&gt;
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偏微分方程通常可以通过变量的适当变化，用已知的解简化为更简单的形式。例如，布莱克-舒尔斯偏微分方程&lt;br /&gt;
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:&amp;lt;math&amp;gt; \frac{\partial V}{\partial t} + \tfrac{1}{2}\sigma^2 S^2\frac{\partial^2 V}{\partial S^2} + rS\frac{\partial V}{\partial S} - rV = 0 &amp;lt;/math&amp;gt;&lt;br /&gt;
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&amp;lt;math&amp;gt; \frac{\partial V}{\partial t} + \tfrac{1}{2}\sigma^2 S^2\frac{\partial^2 V}{\partial S^2} + rS\frac{\partial V}{\partial S} - rV = 0 &amp;lt;/math&amp;gt;&lt;br /&gt;
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is reducible to the [[heat equation]]&lt;br /&gt;
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is reducible to the heat equation&lt;br /&gt;
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可以简化为热传导方程&lt;br /&gt;
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:&amp;lt;math&amp;gt; \frac{\partial u}{\partial \tau} = \frac{\partial^2 u}{\partial x^2}&amp;lt;/math&amp;gt;&lt;br /&gt;
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&amp;lt;math&amp;gt; \frac{\partial u}{\partial \tau} = \frac{\partial^2 u}{\partial x^2}&amp;lt;/math&amp;gt;&lt;br /&gt;
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by the change of variables (for complete details see {{webarchive |url=https://web.archive.org/web/20080411030405/http://www.math.unl.edu/~sdunbar1/Teaching/MathematicalFinance/Lessons/BlackScholes/Solution/solution.shtml |date=April 11, 2008 |title=Solution of the Black Scholes Equation }})&lt;br /&gt;
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by the change of variables (for complete details see )&lt;br /&gt;
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通过变量替换(完整的细节见)&lt;br /&gt;
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:&amp;lt;math&amp;gt;\begin{align}&lt;br /&gt;
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V(S,t) &amp;amp;= K v(x,\tau),\\[5px]&lt;br /&gt;
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x &amp;amp;= \ln\left(\tfrac{S}{K} \right),\\[5px]&lt;br /&gt;
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\tau &amp;amp;= \tfrac{1}{2} \sigma^2 (T - t),\\[5px]&lt;br /&gt;
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v(x,\tau)&amp;amp;=e^{-\alpha x-\beta\tau} u(x,\tau).&lt;br /&gt;
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\end{align}&amp;lt;/math&amp;gt;&lt;br /&gt;
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===Fundamental solution===&lt;br /&gt;
基本解&lt;br /&gt;
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{{main|Fundamental solution}}&lt;br /&gt;
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Inhomogeneous equations can often be solved (for constant coefficient PDEs, always be solved) by finding the [[fundamental solution]] (the solution for a point source), then taking the [[convolution]] with the boundary conditions to get the solution.&lt;br /&gt;
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Inhomogeneous equations can often be solved (for constant coefficient PDEs, always be solved) by finding the fundamental solution (the solution for a point source), then taking the convolution with the boundary conditions to get the solution.&lt;br /&gt;
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非齐次方程(常系数偏微分方程)一般是通过先求出基本解(点源的解) ，然后利用带边界条件的卷积来求解。&lt;br /&gt;
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This is analogous in [[signal processing]] to understanding a filter by its [[impulse response]].&lt;br /&gt;
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This is analogous in signal processing to understanding a filter by its impulse response.&lt;br /&gt;
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这类似于在信号处理中通过滤波器的脉冲响应来理解滤波器。&lt;br /&gt;
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===Superposition principle===&lt;br /&gt;
叠加原理&lt;br /&gt;
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{{further| Superposition principle }}&lt;br /&gt;
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The superposition principle applies to any linear system, including linear systems of PDEs. A common visualization of this concept is the interaction of two waves in phase being combined to result in a greater amplitude, for example {{math|sin ''x'' + sin ''x'' {{=}} 2 sin ''x''}}. The same principle can be observed in PDEs where the solutions may be real or complex and additive. [[Superposition principle|superposition]]&lt;br /&gt;
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The superposition principle applies to any linear system, including linear systems of PDEs. A common visualization of this concept is the interaction of two waves in phase being combined to result in a greater amplitude, for example  2 sin x}}. The same principle can be observed in PDEs where the solutions may be real or complex and additive. superposition&lt;br /&gt;
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'''&amp;lt;font color = &amp;quot;#ff8000&amp;quot;&amp;gt;叠加原理 Superposition Principle&amp;lt;/font&amp;gt;适用于任何线性系统，包括偏微分方程的线性系统。这个概念的一个常见的可视化是两个同相位的波相互作用结合在一起会产生更大的振幅，例如 {{math|sin ''x'' + sin ''x'' {{=}} 2 sin ''x''}}。在偏微分方程中也可以观察到同样的原理，其中的解可能是真实的或复杂的和可加的。叠加&lt;br /&gt;
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If {{math|''u''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;}} and {{math|''u''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;}} are solutions of linear PDE in some function space {{mvar|R}}, then {{math|''u'' {{=}} ''c''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;''u''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; + ''c''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;''u''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;}} with any constants {{math|''c''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;}} and {{math|''c''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;}} are also a solution of that PDE in the same function space.&lt;br /&gt;
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If  and  are solutions of linear PDE in some function space , then  c&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;u&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; + c&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;u&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;}} with any constants  and  are also a solution of that PDE in the same function space.&lt;br /&gt;
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若线性偏微分方程在某个函数空间{{mvar|R}}中有解{{math|''u''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;}} 和 {{math|''u''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;}}，则{{math|''u'' {{=}} ''c''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;''u''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; + ''c''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;''u''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;}}也是该偏微分方程在同一函数空间中的解，其中{{math|''c''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;}} 和 {{math|''c''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;}} 是任意常数。&lt;br /&gt;
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===Methods for non-linear equations===&lt;br /&gt;
非线性方程的求解方法&lt;br /&gt;
{{see also|nonlinear partial differential equation}}&lt;br /&gt;
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There are no generally applicable methods to solve nonlinear PDEs. Still, existence and uniqueness results (such as the [[Cauchy–Kowalevski theorem]]) are often possible, as are proofs of important qualitative and quantitative properties of solutions (getting these results is a major part of [[mathematical analysis|analysis]]). Computational solution to the nonlinear PDEs, the [[split-step method]], exist for specific equations like [[nonlinear Schrödinger equation]].&lt;br /&gt;
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There are no generally applicable methods to solve nonlinear PDEs. Still, existence and uniqueness results (such as the Cauchy–Kowalevski theorem) are often possible, as are proofs of important qualitative and quantitative properties of solutions (getting these results is a major part of analysis). Computational solution to the nonlinear PDEs, the split-step method, exist for specific equations like nonlinear Schrödinger equation.&lt;br /&gt;
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对于非线性偏微分方程，目前还没有普遍适用的求解方法。然而，通常是可能知道解的存在性和唯一性(如柯西-科瓦列夫斯基定理)，也是可能得到解的重要定性和定量性质的证明(得到这些结果是分析的主要部分)。非线性偏微分方程的计算解，即分步法，对一些特定的方程适用，比如非线性'''&amp;lt;font color=&amp;quot;#ff8000&amp;quot;&amp;gt;薛定谔方程 Schrödinger equation&amp;lt;/font&amp;gt;'''。&lt;br /&gt;
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Nevertheless, some techniques can be used for several types of equations. The [[h-principle|{{mvar|h}}-principle]] is the most powerful method to solve [[Underdetermined system|underdetermined]] equations. The [[Riquier–Janet theory]] is an effective method for obtaining information about many analytic [[Overdetermined system|overdetermined]] systems.&lt;br /&gt;
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Nevertheless, some techniques can be used for several types of equations. The -principle is the most powerful method to solve underdetermined equations. The Riquier–Janet theory is an effective method for obtaining information about many analytic overdetermined systems.&lt;br /&gt;
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然而，一些技巧可以用于几种类型的方程。h-原理是求解欠定方程最有效的方法。里基尔-珍妮特理论是一种可以获得许多解析超定系统信息的有效方法。&lt;br /&gt;
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The [[method of characteristics]] can be used in some very special cases to solve partial differential equations.&lt;br /&gt;
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The method of characteristics can be used in some very special cases to solve partial differential equations.&lt;br /&gt;
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特征线法可用于求解某些特殊情况下的偏微分方程。&lt;br /&gt;
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In some cases, a PDE can be solved via [[perturbation analysis]] in which the solution is considered to be a correction to an equation with a known solution. Alternatives are [[numerical analysis]] techniques from simple [[finite difference]] schemes to the more mature [[multigrid]] and [[finite element method]]s. Many interesting problems in science and engineering are solved in this way using [[computer]]s, sometimes high performance [[supercomputer]]s.&lt;br /&gt;
&lt;br /&gt;
In some cases, a PDE can be solved via perturbation analysis in which the solution is considered to be a correction to an equation with a known solution. Alternatives are numerical analysis techniques from simple finite difference schemes to the more mature multigrid and finite element methods. Many interesting problems in science and engineering are solved in this way using computers, sometimes high performance supercomputers.&lt;br /&gt;
&lt;br /&gt;
在某些情况下，偏微分方程可以通过扰动分析来求解。在扰动分析中，通常是求解将具有已知解的方程修正后的新得到方程。可供选择的数值分析技术从简单的差分格式到更成熟的多重网格和有限元方法。许多有趣的科学和工程问题都是在计算机上用这种方法解决的，有时是高性能超级计算机。&lt;br /&gt;
&lt;br /&gt;
===Lie group method===&lt;br /&gt;
李群方法&lt;br /&gt;
&lt;br /&gt;
From 1870 [[Sophus Lie]]'s work put the theory of differential equations on a more satisfactory foundation. He showed that the integration theories of the older mathematicians can, by the introduction of what are now called [[Lie group]]s, be referred, to a common source; and that ordinary differential equations which admit the same [[infinitesimal transformation]]s present comparable difficulties of integration. He also emphasized the subject of [[contact transformation|transformations of contact]].&lt;br /&gt;
&lt;br /&gt;
From 1870 Sophus Lie's work put the theory of differential equations on a more satisfactory foundation. He showed that the integration theories of the older mathematicians can, by the introduction of what are now called Lie groups, be referred, to a common source; and that ordinary differential equations which admit the same infinitesimal transformations present comparable difficulties of integration. He also emphasized the subject of transformations of contact.&lt;br /&gt;
&lt;br /&gt;
从1870年起，索弗斯·李的工作为微分方程理论奠定了一个较为令人满意的基础。他指出，通过引入现在所谓的李群，老一辈数学家的积分理论可以引用到一个共同的来源; 承认相同的无穷小变换的常微分方程在积分方面存在相当的困难。他还强调了接触的转变这一主题。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==[[用户:Yuling|Yuling]]（[[用户讨论:Yuling|讨论]]）这句话“He also emphasized the subject of transformations of contact.”中的transformations of contact翻译的不太好。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
A general approach to solving PDEs uses the symmetry property of differential equations, the continuous [[infinitesimal transformation]]s of solutions to solutions ([[Lie theory]]). Continuous [[group theory]], [[Lie algebras]] and [[differential geometry]] are used to understand the structure of linear and nonlinear partial differential equations for generating integrable equations, to find its [[Lax pair]]s, recursion operators, [[Bäcklund transform]] and finally finding exact analytic solutions to the PDE.&lt;br /&gt;
&lt;br /&gt;
A general approach to solving PDEs uses the symmetry property of differential equations, the continuous infinitesimal transformations of solutions to solutions (Lie theory). Continuous group theory, Lie algebras and differential geometry are used to understand the structure of linear and nonlinear partial differential equations for generating integrable equations, to find its Lax pairs, recursion operators, Bäcklund transform and finally finding exact analytic solutions to the PDE.&lt;br /&gt;
&lt;br /&gt;
求解偏微分方程的一般方法是利用微分方程的对称性，即解到解的连续无穷小变换(李理论)。连续群论、李代数和微分几何理论被用来理解生成可积方程的线性和非线性偏微分方程的结构，找到它的Lax对、递归算子、 贝克伦德变换，最后找到偏微分方程的精确解析解。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Symmetry methods have been recognized to study differential equations arising in mathematics, physics, engineering, and many other disciplines.&lt;br /&gt;
&lt;br /&gt;
Symmetry methods have been recognized to study differential equations arising in mathematics, physics, engineering, and many other disciplines.&lt;br /&gt;
&lt;br /&gt;
对称方法已被公认可以用于研究出现在数学，物理，工程和许多其他学科的微分方程。&lt;br /&gt;
&lt;br /&gt;
===Semianalytical methods===&lt;br /&gt;
半解析方法&lt;br /&gt;
&lt;br /&gt;
The [[Adomian decomposition method]], the [[Aleksandr Lyapunov|Lyapunov]] artificial small parameter method, and He's [[homotopy perturbation method]] are all special cases of the more general [[homotopy analysis method]]. These are series expansion methods, and except for the Lyapunov method, are independent of small physical parameters as compared to the well known [[perturbation theory]], thus giving these methods greater flexibility and solution generality.&lt;br /&gt;
&lt;br /&gt;
The Adomian decomposition method, the Lyapunov artificial small parameter method, and He's homotopy perturbation method are all special cases of the more general homotopy analysis method. These are series expansion methods, and except for the Lyapunov method, are independent of small physical parameters as compared to the well known perturbation theory, thus giving these methods greater flexibility and solution generality.&lt;br /&gt;
&lt;br /&gt;
阿多米安分解法、李雅普诺夫人工小参数方法和何同伦摄动方法都是更一般的同伦分析方法的特殊情况。除了李雅普诺夫方法之外，这些都是级数展开方法，与为人熟知的摄动理论方法相比，它们与小的物理参数无关，因此这些方法具有更大的灵活性和解的通用性。&lt;br /&gt;
&lt;br /&gt;
== Numerical solutions ==&lt;br /&gt;
数值解&lt;br /&gt;
&lt;br /&gt;
The three most widely used [[Numerical partial differential equations|numerical methods to solve PDEs]] are the [[finite element analysis|finite element method]] (FEM), [[finite volume method]]s (FVM) and [[finite difference method]]s (FDM), as well other kind of methods called [[Meshfree methods]], which were made to solve problems where the before mentioned methods are limited. The FEM has a prominent position among these methods and especially its exceptionally efficient higher-order version [[hp-FEM]]. Other hybrid versions of FEM and Meshfree methods include the generalized finite element method (GFEM), [[extended finite element method]] (XFEM), [[Spectral element method|spectral finite element method]] (SFEM), [[Meshfree methods|meshfree finite element method]], [[Discontinuous Galerkin Method|discontinuous Galerkin finite element method]] (DGFEM), [[Element-Free Galerkin Method]] (EFGM), [[Interpolating Element-Free Galerkin Method]] (IEFGM), etc.&lt;br /&gt;
&lt;br /&gt;
The three most widely used numerical methods to solve PDEs are the finite element method (FEM), finite volume methods (FVM) and finite difference methods (FDM), as well other kind of methods called Meshfree methods, which were made to solve problems where the before mentioned methods are limited. The FEM has a prominent position among these methods and especially its exceptionally efficient higher-order version hp-FEM. Other hybrid versions of FEM and Meshfree methods include the generalized finite element method (GFEM), extended finite element method (XFEM), spectral finite element method (SFEM), meshfree finite element method, discontinuous Galerkin finite element method (DGFEM), Element-Free Galerkin Method (EFGM), Interpolating Element-Free Galerkin Method (IEFGM), etc.&lt;br /&gt;
&lt;br /&gt;
求解偏微分方程最常用的三种数值方法是有限元分析法、有限体积法和有限差分法，以及其他一些称为无网格法的方法，用于解决前面用提到的方法求解受到限制的问题。在这些方法中，有限元方法，尤其是高效的高阶有限元方法（hp-FEM），占有重要地位。其他有限元法和无网格法的混合形式包括广义有限元分析法(GFEM)、扩展有限元分析法(XFEM)、谱有限元分析法(SFEM)、无网格有限元分析法(DGFEM)、间断伽辽金有限元分析法(DGFEM)、无单元伽辽金法(EFGM)、插值无单元伽辽金法(IEFGM)等。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
=== Finite element method ===&lt;br /&gt;
有限元分析法&lt;br /&gt;
&lt;br /&gt;
{{main|Finite element method}}&lt;br /&gt;
&lt;br /&gt;
The finite element method (FEM) (its practical application often known as finite element analysis (FEA)) is a numerical technique for finding approximate solutions of partial differential equations (PDE) as well as of integral equations. The solution approach is based either on eliminating the differential equation completely (steady state problems), or rendering the PDE into an approximating system of ordinary differential equations, which are then numerically integrated using standard techniques such as Euler's method, Runge–Kutta, etc.&lt;br /&gt;
&lt;br /&gt;
The finite element method (FEM) (its practical application often known as finite element analysis (FEA)) is a numerical technique for finding approximate solutions of partial differential equations (PDE) as well as of integral equations. The solution approach is based either on eliminating the differential equation completely (steady state problems), or rendering the PDE into an approximating system of ordinary differential equations, which are then numerically integrated using standard techniques such as Euler's method, Runge–Kutta, etc.&lt;br /&gt;
&lt;br /&gt;
'''&amp;lt;font color = &amp;quot;#ff8000&amp;quot;&amp;gt;有限元分析法 Finite Element Method&amp;lt;/font&amp;gt;''' ((其实际应用通常被称为有限元分析(FEA))是一种寻找偏微分方程(PDE)和积分方程近似解的数值技术。这种求解方法要么基于完全消除微分方程(稳态问题) ，要么将偏微分方程转化为常微分方程的近似系统，然后使用标准技术进行数值积分，如欧拉方法、 Runge-Kutta 等。&lt;br /&gt;
&lt;br /&gt;
===Finite difference method===&lt;br /&gt;
有限差分法&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{{main|Finite difference method}}&lt;br /&gt;
&lt;br /&gt;
Finite-difference methods are numerical methods for approximating the solutions to differential equations using [[finite difference]] equations to approximate derivatives.&lt;br /&gt;
&lt;br /&gt;
Finite-difference methods are numerical methods for approximating the solutions to differential equations using finite difference equations to approximate derivatives.&lt;br /&gt;
&lt;br /&gt;
有限差分法是一种数值方法，用差分方程近似倒数来近似微分方程的解。&lt;br /&gt;
&lt;br /&gt;
=== Finite volume method ===&lt;br /&gt;
有限体积法&lt;br /&gt;
&lt;br /&gt;
{{main|Finite volume method}}&lt;br /&gt;
&lt;br /&gt;
Similar to the finite difference method or finite element method, values are calculated at discrete places on a meshed geometry. &amp;quot;Finite volume&amp;quot; refers to the small volume surrounding each node point on a mesh. In the finite volume method, surface integrals in a partial differential equation that contain a divergence term are converted to volume integrals, using the [[divergence theorem]]. These terms are then evaluated as fluxes at the surfaces of each finite volume. Because the flux entering a given volume is identical to that leaving the adjacent volume, these methods conserve mass by design.&lt;br /&gt;
&lt;br /&gt;
Similar to the finite difference method or finite element method, values are calculated at discrete places on a meshed geometry. &amp;quot;Finite volume&amp;quot; refers to the small volume surrounding each node point on a mesh. In the finite volume method, surface integrals in a partial differential equation that contain a divergence term are converted to volume integrals, using the divergence theorem. These terms are then evaluated as fluxes at the surfaces of each finite volume. Because the flux entering a given volume is identical to that leaving the adjacent volume, these methods conserve mass by design.&lt;br /&gt;
&lt;br /&gt;
类似于有限差分法或有限元分析，函数值是在网格化的几何体上的离散位置进行计算的。“有限体积”是指网格上每个节点周围的小体积。在有限体积法中，偏微分方程中含有散度项的面积分用散度定理积分转换成体积分。然后将这些项用于估算每个有限体积表面上的通量。由于进入给定体积元的通量与转移出相邻体积元的通量相同，所以这些方法通过设计保证了质量守恒。&lt;br /&gt;
&lt;br /&gt;
==See also==&lt;br /&gt;
请参阅&lt;br /&gt;
* [[Dirichlet boundary condition]]&lt;br /&gt;
狄利克雷边界条件&lt;br /&gt;
* [[Jet bundle]]&lt;br /&gt;
射流丛&lt;br /&gt;
* [[Laplace transform applied to differential equations]]&lt;br /&gt;
微分方程中的拉普拉斯变换&lt;br /&gt;
* [[List of dynamical systems and differential equations topics]]&lt;br /&gt;
动力学系统列表和微分方程主题&lt;br /&gt;
* [[Matrix differential equation]]&lt;br /&gt;
矩阵微分方程&lt;br /&gt;
* [[Neumann boundary condition]]&lt;br /&gt;
诺伊曼边界条件&lt;br /&gt;
* [[Numerical partial differential equations]]&lt;br /&gt;
数值偏微分方程&lt;br /&gt;
* [[Partial differential algebraic equation]]&lt;br /&gt;
偏微分代数方程&lt;br /&gt;
* [[Recurrence relation]]&lt;br /&gt;
递推关系&lt;br /&gt;
* [[Robin boundary condition]]&lt;br /&gt;
罗宾边界条件&lt;br /&gt;
* [[Stochastic processes and boundary value problems]]&lt;br /&gt;
随机过程和边值问题&lt;br /&gt;
&lt;br /&gt;
== The energy method ==&lt;br /&gt;
能量法&lt;br /&gt;
&lt;br /&gt;
The energy method is a mathematical procedure that can be used to verify well-posedness of initial-boundary-value-problems.&amp;lt;ref&amp;gt;{{cite book |title=High Order Difference Methods for Time Dependent PDE&lt;br /&gt;
&lt;br /&gt;
The energy method is a mathematical procedure that can be used to verify well-posedness of initial-boundary-value-problems.&amp;lt;ref&amp;gt;{{cite book |title=High Order Difference Methods for Time Dependent PDE&lt;br /&gt;
&lt;br /&gt;
能量法是一种数学过程，可用于验证初始边界值问题的适定性。&lt;br /&gt;
&lt;br /&gt;
In the following example the energy method is used to decide where and which boundary conditions should be imposed such that the resulting IBVP is well-posed. Consider the one-dimensional hyperbolic PDE given by&lt;br /&gt;
&lt;br /&gt;
In the following example the energy method is used to decide where and which boundary conditions should be imposed such that the resulting IBVP is well-posed. Consider the one-dimensional hyperbolic PDE given by&lt;br /&gt;
&lt;br /&gt;
在下面的示例中，将使用能量法决定应在何处施加哪些边界条件，以使得到的IBVP处于适当位置。考虑下式给出的一维双曲PDE&lt;br /&gt;
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: &amp;lt;math&amp;gt;\frac{\partial u}{\partial t} + \alpha \frac{\partial u}{\partial x} = 0, \quad x \in [a,b], \operatorname t &amp;gt; 0,&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;\frac{\partial u}{\partial t} + \alpha \frac{\partial u}{\partial x} = 0, \quad x \in [a,b], \operatorname t &amp;gt; 0,&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
where &amp;lt;math&amp;gt;\alpha \neq 0&amp;lt;/math&amp;gt; is a constant and &amp;lt;math&amp;gt;u(x,t)&amp;lt;/math&amp;gt; is an unknown function with initial condition &amp;lt;math&amp;gt;u(x,0) = f(x)&amp;lt;/math&amp;gt;. Multiplying with &amp;lt;math&amp;gt;u&amp;lt;/math&amp;gt; and integrating over the domain gives&lt;br /&gt;
&lt;br /&gt;
where &amp;lt;math&amp;gt;\alpha \neq 0&amp;lt;/math&amp;gt; is a constant and &amp;lt;math&amp;gt;u(x,t)&amp;lt;/math&amp;gt; is an unknown function with initial condition &amp;lt;math&amp;gt;u(x,0) = f(x)&amp;lt;/math&amp;gt;. Multiplying with &amp;lt;math&amp;gt;u&amp;lt;/math&amp;gt; and integrating over the domain gives&lt;br /&gt;
&lt;br /&gt;
其中 &amp;lt;math&amp;gt;\alpha \neq 0&amp;lt;/math&amp;gt; 是常数，并且 &amp;lt;math&amp;gt;u(x,t)&amp;lt;/math&amp;gt; 是初始条件是 &amp;lt;math&amp;gt;u(x,0) = f(x)&amp;lt;/math&amp;gt;的未知函数，乘以 &amp;lt;math&amp;gt;u&amp;lt;/math&amp;gt; 并在域上进行积分。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt;\int_a^b u \frac{\partial u}{\partial t} \operatorname dx + \alpha \int _a ^b u \frac{\partial u}{\partial x} \operatorname dx = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;\int_a^b u \frac{\partial u}{\partial t} \operatorname dx + \alpha \int _a ^b u \frac{\partial u}{\partial x} \operatorname dx = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Using that&lt;br /&gt;
&lt;br /&gt;
Using that&lt;br /&gt;
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利用这一点&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt;\int _a ^b u \frac{\partial u}{\partial t} \operatorname dx = \frac{1}{2} \frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 \quad \text{and} \quad \int _a ^b u \frac{\partial u}{\partial x} \operatorname dx = \frac{1}{2} u(b,t)^2 - \frac{1}{2} u(a,t)^2,.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;\int _a ^b u \frac{\partial u}{\partial t} \operatorname dx = \frac{1}{2} \frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 \quad \text{and} \quad \int _a ^b u \frac{\partial u}{\partial x} \operatorname dx = \frac{1}{2} u(b,t)^2 - \frac{1}{2} u(a,t)^2,.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
where integration by parts has been used for the second relationship, we get&lt;br /&gt;
&lt;br /&gt;
where integration by parts has been used for the second relationship, we get&lt;br /&gt;
&lt;br /&gt;
第二个关系中采用了分部积分法，我们可以得到&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt;\frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 + \alpha u(b,t)^2 - \alpha u(a,t)^2 = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;\frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 + \alpha u(b,t)^2 - \alpha u(a,t)^2 = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Here &amp;lt;math&amp;gt;\vert \vert \cdot \vert \vert&amp;lt;/math&amp;gt; denotes the standard L2-norm.&lt;br /&gt;
&lt;br /&gt;
Here &amp;lt;math&amp;gt;\vert \vert \cdot \vert \vert&amp;lt;/math&amp;gt; denotes the standard L2-norm.&lt;br /&gt;
&lt;br /&gt;
在这里，&amp;lt;math&amp;gt;\vert \vert \cdot \vert \vert&amp;lt;/math&amp;gt; 表示标准的L2-正则。&lt;br /&gt;
&lt;br /&gt;
For well-posedness we require that the energy of the solution is non-increasing, i.e. that &amp;lt;math&amp;gt;\frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 \leq 0&amp;lt;/math&amp;gt;, which is achieved by specifying &amp;lt;math&amp;gt;u&amp;lt;/math&amp;gt; at &amp;lt;math&amp;gt;x = a&amp;lt;/math&amp;gt; if &amp;lt;math&amp;gt;\alpha &amp;gt; 0&amp;lt;/math&amp;gt; and at &amp;lt;math&amp;gt;x = b&amp;lt;/math&amp;gt; if &amp;lt;math&amp;gt;\alpha &amp;lt; 0&amp;lt;/math&amp;gt;. This corresponds to only imposing boundary conditions at the inflow. Note that well-posedness allows for growth in terms of data (initial and boundary) and thus it is sufficient to show that &amp;lt;math&amp;gt;\frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 \leq 0&amp;lt;/math&amp;gt; holds when all data is set to zero.&lt;br /&gt;
&lt;br /&gt;
For well-posedness we require that the energy of the solution is non-increasing, i.e. that &amp;lt;math&amp;gt;\frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 \leq 0&amp;lt;/math&amp;gt;, which is achieved by specifying &amp;lt;math&amp;gt;u&amp;lt;/math&amp;gt; at &amp;lt;math&amp;gt;x = a&amp;lt;/math&amp;gt; if &amp;lt;math&amp;gt;\alpha &amp;gt; 0&amp;lt;/math&amp;gt; and at &amp;lt;math&amp;gt;x = b&amp;lt;/math&amp;gt; if &amp;lt;math&amp;gt;\alpha &amp;lt; 0&amp;lt;/math&amp;gt;. This corresponds to only imposing boundary conditions at the inflow. Note that well-posedness allows for growth in terms of data (initial and boundary) and thus it is sufficient to show that &amp;lt;math&amp;gt;\frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 \leq 0&amp;lt;/math&amp;gt; holds when all data is set to zero.&lt;br /&gt;
&lt;br /&gt;
对于适定性，我们要求解的能量是不增加的，即 &amp;lt;math&amp;gt;\frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 \leq 0&amp;lt;/math&amp;gt; ，这种关系可以通过在&amp;lt;math&amp;gt;x = a&amp;lt;/math&amp;gt;处 （如果 &amp;lt;math&amp;gt;\alpha &amp;gt; 0&amp;lt;/math&amp;gt;） 以及 &amp;lt;math&amp;gt;x = b&amp;lt;/math&amp;gt;处 （如果 &amp;lt;math&amp;gt;\alpha &amp;lt; 0&amp;lt;/math&amp;gt;）指定&amp;lt;math&amp;gt;u&amp;lt;/math&amp;gt;的值来实现。这相当于只在流入处附加边界条件。注意，适定性允许在数据项(初始和边界)上的增长，因此它足以表明当所有数据设置为零时应有 &amp;lt;math&amp;gt;\frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 \leq 0&amp;lt;/math&amp;gt;。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==Notes==&lt;br /&gt;
&lt;br /&gt;
{{Reflist}}&lt;br /&gt;
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&lt;br /&gt;
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== References ==&lt;br /&gt;
&lt;br /&gt;
{{refbegin|2}}&lt;br /&gt;
&lt;br /&gt;
* {{cite book |title=Solving Frontier problems of Physics: The decomposition method&lt;br /&gt;
&lt;br /&gt;
|first=G.|last=Adomian|publisher=Kluwer Academic Publishers|year=1994|isbn=|page=|url=https://books.google.com/books?id=UKPqCAAAQBAJ&amp;amp;printsec=frontcover#v=onepage&amp;amp;q=%22partial%20differential%22&amp;amp;f=false}}&lt;br /&gt;
&lt;br /&gt;
|first=G.|last=Adomian|publisher=Kluwer Academic Publishers|year=1994|isbn=|page=|url=https://books.google.com/books?id=UKPqCAAAQBAJ&amp;amp;printsec=frontcover#v=onepage&amp;amp;q=%22partial%20differential%22&amp;amp;f=false}}&lt;br /&gt;
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1994年 | isbn | 页面 | 网址: 施普林格科学+商业媒体 https://books.google.com/books?id=ukpqcaaaqbaj&amp;amp;printsec=frontcover#v=onepage&amp;amp;q=%22partial%20differential%22&amp;amp;f=false&lt;br /&gt;
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* {{Citation |first=A. D. |last=Polyanin |first2=V. F. |last2=Zaitsev |lastauthoramp=yes |first3=A. |last3=Moussiaux |title=Handbook of First Order Partial Differential Equations |publisher=Taylor &amp;amp; Francis |location=London |year=2002 |isbn=0-415-27267-X }}.&lt;br /&gt;
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* {{Citation |first=P. |last=Solin |first2=K. |last2=Segeth |lastauthoramp=yes |first3=I. |last3=Dolezel |title=Higher-Order Finite Element Methods |publisher=Chapman &amp;amp; Hall/CRC Press |location=Boca Raton |year=2003 |isbn=1-58488-438-X }}.&lt;br /&gt;
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* {{Citation |first=H. |last=Stephani |year=1989 |title=Differential Equations: Their Solution Using Symmetries. Edited by M. MacCallum |publisher=Cambridge University Press }}.&lt;br /&gt;
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* {{cite book |title=Partial Differential Equations and Solitary Waves Theory&lt;br /&gt;
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|first=Abdul-Majid|last=Wazwaz|publisher=Higher Education Press|year=2009|isbn=978-3-642-00251-9|page=}}&lt;br /&gt;
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|first=Abdul-Majid|last=Wazwaz|publisher=Higher Education Press|year=2009|isbn=978-3-642-00251-9|page=}}&lt;br /&gt;
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| first Abdul-Majid | last Wazwaz | publisher Higher Education Press | year 2009 | isbn 978-3-642-00251-9 | page }&lt;br /&gt;
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* {{cite book |title=Partial Differential Equations Methods and Applications&lt;br /&gt;
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|first=Abdul-Majid|last=Wazwaz|publisher=A.A. Balkema|year=2002|isbn=90-5809-369-7|page=}}&lt;br /&gt;
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|first=Abdul-Majid|last=Wazwaz|publisher=A.A. Balkema|year=2002|isbn=90-5809-369-7|page=}}&lt;br /&gt;
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| first Abdul-Majid | last Wazwaz | publisher a.a.Balkema | year 2002 | isbn 90-5809-369-7 | page }&lt;br /&gt;
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* {{Citation |first=D. |last=Zwillinger |title=Handbook of Differential Equations |publisher=Academic Press |location=Boston |year=1997 |edition=3rd |isbn=0-12-784395-7 }}.&lt;br /&gt;
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* {{Citation |authorlink=Neil Gershenfeld |first=N. |last=Gershenfeld |title=The Nature of Mathematical Modeling |location=New York |publisher=Cambridge University Press, New York, NY, USA |year=1999 |edition=1st |isbn=0-521-57095-6 }}.&lt;br /&gt;
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* {{Citation |first=I.S. |last=Krasil'shchik |lastauthoramp=yes |first2=A.M., Eds. |last2=Vinogradov |title=Symmetries and Conserwation Laws for Differential Equations of Mathematical Physics |publisher=American Mathematical Society, Providence, Rhode Island, USA |year=1999 |isbn=0-8218-0958-X }}.&lt;br /&gt;
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* {{Citation |first=I.S. |last=Krasil'shchik |first2=V.V. |last2=Lychagin|lastauthoramp=yes |first3=A.M. |last3=Vinogradov |title=Geometry of Jet Spaces and Nonlinear Partial Differential Equations |publisher=Gordon and Breach Science Publishers, New York, London, Paris, Montreux, Tokyo |year=1986 |isbn=2-88124-051-8 }}.&lt;br /&gt;
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* {{Citation |first=A.M. |last=Vinogradov |title=Cohomological Analysis of Partial Differential Equations and Secondary Calculus |publisher=American Mathematical Society, Providence, Rhode Island, USA |year=2001 |isbn=0-8218-2922-X }}.&lt;br /&gt;
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* {{cite book |title=High Order Difference Methods for Time Dependent PDE&lt;br /&gt;
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|first=Bertil|last=Gustafsson|publisher=Springer|year=2008|isbn=978-3-540-74992-9|doi=10.1007/978-3-540-74993-6}}&lt;br /&gt;
&lt;br /&gt;
|first=Bertil|last=Gustafsson|publisher=Springer|year=2008|isbn=978-3-540-74992-9|doi=10.1007/978-3-540-74993-6}}&lt;br /&gt;
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| first Bertil | last Gustafsson | Springer | year 2008 | isbn 978-3-540-74992-9 | doi 10.1007 / 978-3-540-74993-6}&lt;br /&gt;
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{{refend}}&lt;br /&gt;
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== Further reading ==&lt;br /&gt;
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* {{Cite journal|last=Cajori|first=Florian|authorlink=Florian Cajori|year=1928|title=The Early History of Partial Differential Equations and of Partial Differentiation and Integration|url=http://www.math.harvard.edu/archive/21a_fall_14/exhibits/cajori/cajori.pdf|journal=The American Mathematical Monthly|volume=35|issue=9|pages=459–467|doi=10.2307/2298771|access-date=2016-05-15|archive-url=https://web.archive.org/web/20181123102253/http://www.math.harvard.edu/archive/21a_fall_14/exhibits/cajori/cajori.pdf|archive-date=2018-11-23|url-status=dead}}&lt;br /&gt;
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== External links ==&lt;br /&gt;
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{{Sister project links| wikt=no | commons=Category:Solutions of PDE | b=Partial Differential Equations | n=no | q=Partial differential equation | s=no | v=no | voy=no | species=no | d=no}}&lt;br /&gt;
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* {{springer|title=Differential equation, partial|id=p/d031920}}&lt;br /&gt;
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* [http://eqworld.ipmnet.ru/en/pde-en.htm Partial Differential Equations: Exact Solutions] at EqWorld: The World of Mathematical Equations.&lt;br /&gt;
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* [http://eqworld.ipmnet.ru/en/solutions/eqindex/eqindex-pde.htm Partial Differential Equations: Index] at EqWorld: The World of Mathematical Equations.&lt;br /&gt;
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* [http://eqworld.ipmnet.ru/en/methods/meth-pde.htm Partial Differential Equations: Methods] at EqWorld: The World of Mathematical Equations.&lt;br /&gt;
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* [https://web.archive.org/web/20170701144823/http://www.exampleproblems.com/wiki/index.php?title=Partial_Differential_Equations Example problems with solutions] at exampleproblems.com&lt;br /&gt;
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* [http://mathworld.wolfram.com/PartialDifferentialEquation.html Partial Differential Equations] at mathworld.wolfram.com&lt;br /&gt;
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* [https://reference.wolfram.com/language/FEMDocumentation/tutorial/SolvingPDEwithFEM.html Partial Differential Equations] with Mathematica&lt;br /&gt;
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* [http://www.mathworks.com/moler/pdes.pdf Partial Differential Equations] in Cleve Moler: Numerical Computing with MATLAB&lt;br /&gt;
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* [http://www.nag.com/numeric/fl/nagdoc_fl24/html/D03/d03intro.html Partial Differential Equations] at nag.com&lt;br /&gt;
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* {{cite web |first=Grant |last=Sanderson |title=But what is a partial differential equation? |work=3Blue1Brown |date=April 21, 2019 |url=https://www.youtube.com/watch?v=ly4S0oi3Yz8&amp;amp;list=PLZHQObOWTQDNPOjrT6KVlfJuKtYTftqH6 |via=[[YouTube]] }}&lt;br /&gt;
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{{Differential equations topics}}&lt;br /&gt;
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[[Category:Partial differential equations| ]]&lt;br /&gt;
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[[Category:Multivariable calculus]]&lt;br /&gt;
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Category:Multivariable calculus&lt;br /&gt;
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类别: 多元微积分&lt;br /&gt;
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[[Category:Differential equations]]&lt;br /&gt;
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Category:Differential equations&lt;br /&gt;
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类别: 微分方程&lt;br /&gt;
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[[Category:Concepts in physics]]&lt;br /&gt;
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Category:Concepts in physics&lt;br /&gt;
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分类: 物理概念&lt;br /&gt;
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&amp;lt;small&amp;gt;This page was moved from [[wikipedia:en:Partial differential equation]]. Its edit history can be viewed at [[偏微分方程/edithistory]]&amp;lt;/small&amp;gt;&amp;lt;/noinclude&amp;gt;&lt;br /&gt;
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[[Category:待整理页面]]&lt;/div&gt;</summary>
		<author><name>Ruili</name></author>
	</entry>
	<entry>
		<id>https://wiki.swarma.org/index.php?title=%E5%81%8F%E5%BE%AE%E5%88%86%E6%96%B9%E7%A8%8B&amp;diff=20106</id>
		<title>偏微分方程</title>
		<link rel="alternate" type="text/html" href="https://wiki.swarma.org/index.php?title=%E5%81%8F%E5%BE%AE%E5%88%86%E6%96%B9%E7%A8%8B&amp;diff=20106"/>
		<updated>2020-12-15T13:24:05Z</updated>

		<summary type="html">&lt;p&gt;Ruili：&lt;/p&gt;
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&lt;div&gt;此词条暂由Yuling翻译，未经人工整理和审校，带来阅读不便，请见谅。&lt;br /&gt;
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[[File:Heat.gif|thumb|right|A visualisation of a solution to the two-dimensional [[heat equation]] with temperature represented by the third dimension]]&lt;br /&gt;
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A visualisation of a solution to the two-dimensional [[heat equation with temperature represented by the third dimension]]&lt;br /&gt;
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以三维表示温度的二维热方程解的可视化&lt;br /&gt;
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In [[mathematics]], a '''partial differential equation''' ('''PDE''') is a [[differential equation]] that contains unknown [[Multivariable calculus|multivariable functions]] and their [[partial derivative]]s. PDEs are used to formulate problems involving functions of several variables, and are either solved by hand, or used to create a [[computer model]]. A special case is [[ordinary differential equation]]s (ODEs), which deal with functions of a single variable and their derivatives.&lt;br /&gt;
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In mathematics, a partial differential equation (PDE) is a differential equation that contains unknown multivariable functions and their partial derivatives. PDEs are used to formulate problems involving functions of several variables, and are either solved by hand, or used to create a computer model. A special case is ordinary differential equations (ODEs), which deal with functions of a single variable and their derivatives.&lt;br /&gt;
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在数学中，'''&amp;lt;font color = &amp;quot;#ff8000&amp;quot;&amp;gt; 偏微分方程函数 Partial Differential Equation&amp;lt;/font&amp;gt;'''是包含未知多元函数及其偏导数的微分方程。偏微分方程用于描述涉及多元函数的问题，可以通过人为求解，也可以通过建立计算机模型来求解。常微分方程是偏微分方程一种特殊情况，它处理的是一元函数及其导数。&lt;br /&gt;
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PDEs can be used to describe a wide variety of phenomena such as sound, heat, [[diffusion]], [[electrostatics]], [[Electromagnetism|electrodynamics]], [[fluid dynamics]], [[Elasticity (physics)|elasticity]], [[gravitation]] and [[quantum mechanics]]. These seemingly distinct physical phenomena can be formalised similarly in terms of PDEs. Just as ordinary differential equations often model one-dimensional [[dynamical system]]s, partial differential equations often model [[multidimensional system]]s. PDEs find their generalisation in [[stochastic partial differential equation]]s.&lt;br /&gt;
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PDEs can be used to describe a wide variety of phenomena such as sound, heat, diffusion, electrostatics, electrodynamics, fluid dynamics, elasticity, gravitation and quantum mechanics. These seemingly distinct physical phenomena can be formalised similarly in terms of PDEs. Just as ordinary differential equations often model one-dimensional dynamical systems, partial differential equations often model multidimensional systems. PDEs find their generalisation in stochastic partial differential equations.&lt;br /&gt;
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偏微分方程可以用来描述各种各样的物理现象，如声音，热量，扩散，静电，电动力学，流体力学，弹性力学，重力和量子力学。这些看起来截然不同的物理现象却可以用类似的偏微分方程来描述。正如常微分方程经常对一维动力系统进行建模一样，偏微分方程经常对多维系统进行建模。随机偏微分方程是偏微分方程的一种推广。&lt;br /&gt;
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== Introduction ==&lt;br /&gt;
引言&lt;br /&gt;
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Partial differential equations (PDEs) are equations that involve rates of change with respect to [[continuous variables]]. For example, the position of a [[rigid body]] is specified by six parameters,&amp;lt;ref&amp;gt;{{Cite book|url=https://books.google.com/books?id=v9PLbcYd9aUC&amp;amp;pg=PA32|title=Modelling and Control of Robot Manipulators|last=Sciavicco|first=Lorenzo|last2=Siciliano|first2=Bruno|date=2001-02-19|publisher=Springer Science &amp;amp; Business Media|isbn=9781852332211|language=en}}&amp;lt;/ref&amp;gt; but the configuration of a [[fluid]] is given by the [[continuous distribution]] of several parameters, such as the [[temperature]], [[pressure]], and so forth. The dynamics for the rigid body take place in a finite-dimensional [[Configuration space (physics)|configuration space]]; the dynamics for the fluid occur in an infinite-dimensional configuration space. This distinction usually makes PDEs much harder to solve than ordinary differential equations (ODEs), but here again, there will be simple solutions for linear problems. Classic domains where PDEs are used include [[acoustics]], [[fluid dynamics]], [[electrodynamics]], and [[heat transfer]].&lt;br /&gt;
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Partial differential equations (PDEs) are equations that involve rates of change with respect to continuous variables. For example, the position of a rigid body is specified by six parameters, but the configuration of a fluid is given by the continuous distribution of several parameters, such as the temperature, pressure, and so forth. The dynamics for the rigid body take place in a finite-dimensional configuration space; the dynamics for the fluid occur in an infinite-dimensional configuration space. This distinction usually makes PDEs much harder to solve than ordinary differential equations (ODEs), but here again, there will be simple solutions for linear problems. Classic domains where PDEs are used include acoustics, fluid dynamics, electrodynamics, and heat transfer.&lt;br /&gt;
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偏微分方程(简称为PDEs)涉及到方程相对于连续变量的变化率。例如，刚体的位置是由六个参数确定的，而流体的状态是由几个参数的连续分布给出的，如温度、压力等。刚体的动力学过程发生在有限维状态空间中，流体的动力学过程发生在无限维状态空间中。这种区别通常使偏微分方程比常微分方程更难求解，但是线性问题仍然有简单的求解方式。使用偏微分方程的经典领域包括声学、流体力学、电动力学和传热学。&lt;br /&gt;
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A partial differential equation (PDE) for the function {{math|''u''(''x''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;,… ''x&amp;lt;sub&amp;gt;n&amp;lt;/sub&amp;gt;'')}} is an equation of the form&lt;br /&gt;
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A partial differential equation (PDE) for the function  is an equation of the form&lt;br /&gt;
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函数 {{math|''u''(''x''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;,… ''x&amp;lt;sub&amp;gt;n&amp;lt;/sub&amp;gt;'')}} 的偏微分方程形式是：&lt;br /&gt;
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: &amp;lt;math&amp;gt;f \left (x_1, \ldots x_n; u, \frac{\partial u}{\partial x_1}, \ldots \frac{\partial u}{\partial x_n}; \frac{\partial^2 u}{\partial x_1 \partial x_1}, \ldots \frac{\partial^2 u}{\partial x_1 \partial x_n}; \ldots \right) = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;f \left (x_1, \ldots x_n; u, \frac{\partial u}{\partial x_1}, \ldots \frac{\partial u}{\partial x_n}; \frac{\partial^2 u}{\partial x_1 \partial x_1}, \ldots \frac{\partial^2 u}{\partial x_1 \partial x_n}; \ldots \right) = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
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If {{mvar|f}} is a [[linear function]] of {{mvar|u}} and its derivatives, then the PDE is called linear. Common examples of linear PDEs include the [[heat equation]], the [[wave equation]], [[Laplace's equation]], [[Helmholtz equation]], [[Klein–Gordon equation]], and [[Poisson's equation]].&lt;br /&gt;
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If  is a linear function of  and its derivatives, then the PDE is called linear. Common examples of linear PDEs include the heat equation, the wave equation, Laplace's equation, Helmholtz equation, Klein–Gordon equation, and Poisson's equation.&lt;br /&gt;
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如果 {{mvar|f}} 是函数 {{math|''u''}} 及其导数的线性函数，则偏微分方程称为线性函数。线性偏微分方程的常见例子包括热方程、波动方程、拉普拉斯方程、亥姆霍兹方程方程、克莱因-高登方程和泊松方程。&lt;br /&gt;
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A relatively simple PDE is&lt;br /&gt;
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A relatively simple PDE is&lt;br /&gt;
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一个相对简单的偏微分方程：&lt;br /&gt;
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: &amp;lt;math&amp;gt;\frac{\partial u}{\partial x}(x,y) = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;\frac{\partial u}{\partial x}(x,y) = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
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This relation [[Logical implication|implies]] that the function {{math|''u''(''x'',''y'')}} is independent of {{mvar|x}}. However, the equation gives no information on the function's dependence on the variable {{mvar|y}}. Hence the general solution of this equation is&lt;br /&gt;
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This relation implies that the function  is independent of . However, the equation gives no information on the function's dependence on the variable . Hence the general solution of this equation is&lt;br /&gt;
&lt;br /&gt;
这意味着函数 {{math|''u''(''x'',''y'')}} 独立于 {{mvar|x}} 的。然而，这个方程没有给出关于函数和自变量的相关性的信息。因此，这个方程的通解是&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt;u(x,y) = f(y),&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;u(x,y) = f(y),&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
where {{mvar|f}} is an arbitrary function of {{mvar|y}}. The analogous ordinary differential equation is&lt;br /&gt;
&lt;br /&gt;
where  is an arbitrary function of . The analogous ordinary differential equation is&lt;br /&gt;
&lt;br /&gt;
其中， {{mvar|f}} 是 {{mvar|y}} 的任意函数。&lt;br /&gt;
&lt;br /&gt;
类似的常微分方程是：&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt;\frac{\mathrm{d} u}{\mathrm{d} x}(x) = 0,&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;\frac{\mathrm{d} u}{\mathrm{d} x}(x) = 0,&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
which has the solution&lt;br /&gt;
&lt;br /&gt;
which has the solution&lt;br /&gt;
&lt;br /&gt;
它的解为&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt;u(x) = c,&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;u(x) = c,&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
where {{mvar|c}} is any [[Constant (mathematics)|constant]] value. These two examples illustrate that general solutions of ordinary differential equations (ODEs) involve arbitrary constants, but solutions of PDEs involve arbitrary functions.&lt;br /&gt;
&lt;br /&gt;
where  is any constant value. These two examples illustrate that general solutions of ordinary differential equations (ODEs) involve arbitrary constants, but solutions of PDEs involve arbitrary functions.&lt;br /&gt;
&lt;br /&gt;
这里，{{mvar|c}} 是一个任意常量。&lt;br /&gt;
&lt;br /&gt;
这两个例子说明常微分方程的一般解包含任意常数，但偏微分方程的解包含任意函数。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
A solution of a PDE is generally not [[Uniqueness quantification|unique]]; additional conditions must generally be specified on the [[Boundary (topology)|boundary]] of the region where the solution is defined. For instance, in the simple example above, the function {{math|''f''(''y'')}} can be determined if {{mvar|u}} is specified on the line {{math|''x'' {{=}} 0}}.&lt;br /&gt;
&lt;br /&gt;
A solution of a PDE is generally not unique; additional conditions must generally be specified on the boundary of the region where the solution is defined. For instance, in the simple example above, the function  can be determined if  is specified on the line  0}}.&lt;br /&gt;
&lt;br /&gt;
偏微分方程的解一般不是唯一的; 一般必须在定义解的区域边界上定义附加条件。 例如，在上面的简单示例中，如果在 {{math|''x'' {{=}} 0}} 时确定了 {{mvar|u}} 的值，则可以确定该函数 {{math|''f''(''y'')}}。&lt;br /&gt;
&lt;br /&gt;
== Existence and uniqueness ==&lt;br /&gt;
存在性和唯一性&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Although the issue of existence and uniqueness of solutions of ordinary differential equations has a very satisfactory answer with the [[Picard–Lindelöf theorem]], that is far from the case for partial differential equations. The [[Cauchy–Kowalevski theorem]] states that the [[Cauchy problem]] for any partial differential equation whose coefficients are [[Analytic function|analytic]] in the unknown function and its derivatives, has a locally unique analytic solution. Although this result might appear to settle the existence and uniqueness of solutions, there are examples of linear partial differential equations whose coefficients have derivatives of all orders (which are nevertheless not analytic) but which have no solutions at all: see [[Lewy's example|Lewy (1957)]]. Even if the solution of a partial differential equation exists and is unique, it may nevertheless have undesirable properties.  The mathematical study of these questions is usually in the more powerful context of [[weak solution]]s.&lt;br /&gt;
&lt;br /&gt;
Although the issue of existence and uniqueness of solutions of ordinary differential equations has a very satisfactory answer with the Picard–Lindelöf theorem, that is far from the case for partial differential equations. The Cauchy–Kowalevski theorem states that the Cauchy problem for any partial differential equation whose coefficients are analytic in the unknown function and its derivatives, has a locally unique analytic solution. Although this result might appear to settle the existence and uniqueness of solutions, there are examples of linear partial differential equations whose coefficients have derivatives of all orders (which are nevertheless not analytic) but which have no solutions at all: see Lewy (1957). Even if the solution of a partial differential equation exists and is unique, it may nevertheless have undesirable properties.  The mathematical study of these questions is usually in the more powerful context of weak solutions.&lt;br /&gt;
&lt;br /&gt;
尽管常微分方程解的存在性和唯一性用'''&amp;lt;font color=&amp;quot;#ff8000&amp;quot;&amp;gt;弗罗贝尼乌斯定理 Picard–Lindelöf Theorem&amp;lt;/font&amp;gt;得到了令人满意的结果，但偏微分方程解的存在性和唯一性却远没有得到解决。'''&amp;lt;font color=&amp;quot;#ff8000&amp;quot;&amp;gt;柯西-科瓦列夫斯基定理 Cauchy–Kowalevski theorem&amp;lt;/font&amp;gt;指出：对于任意系数在未知函数及其导数中解析的偏微分方程，柯西问题存在一个局部唯一的解析解。虽然这个结果似乎解决了解的存在性和唯一性问题，但是存在一些线性偏微分方程-其系数具有所有级数的导数(尽管这些导数不是解析的) ，但是根本没有解: 见 Lewy (1957)。即使偏微分方程的解存在且唯一，它仍然可能具有不可预料的性质。这些问题的数学研究通常是在更有力的弱解的背景下进行的。&lt;br /&gt;
&lt;br /&gt;
An example of pathological behavior is the sequence (depending upon {{mvar|n}}) of [[Cauchy problem]]s for the [[Laplace equation]]&lt;br /&gt;
&lt;br /&gt;
An example of pathological behavior is the sequence (depending upon ) of Cauchy problems for the Laplace equation&lt;br /&gt;
&lt;br /&gt;
反常特征的一个例子是拉普拉斯方程的柯西问题的序列(取决于{{mvar|n}})&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt;\frac{\partial^2 u}{\partial x^2} + \frac{\partial^2 u}{\partial y^2}=0,&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;\frac{\partial^2 u}{\partial x^2} + \frac{\partial^2 u}{\partial y^2}=0,&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
with [[boundary condition]]s&lt;br /&gt;
&lt;br /&gt;
with boundary conditions&lt;br /&gt;
&lt;br /&gt;
具有边界条件&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt;\begin{align} u(x,0) &amp;amp;= 0, \\ \frac{\partial u}{\partial y}(x,0) &amp;amp;= \frac{\sin nx}{n}, \end{align}&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;\begin{align} u(x,0) &amp;amp;= 0, \\ \frac{\partial u}{\partial y}(x,0) &amp;amp;= \frac{\sin nx}{n}, \end{align}&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
where {{mvar|n}} is an integer. The derivative of {{mvar|u}} with respect to {{mvar|y}} approaches zero [[uniform convergence|uniformly]] in {{mvar|x}} as {{mvar|n}} increases, but the solution is&lt;br /&gt;
&lt;br /&gt;
where  is an integer. The derivative of  with respect to  approaches zero uniformly in  as  increases, but the solution is&lt;br /&gt;
&lt;br /&gt;
其中 {{mvar|n}} 是整数。{{mvar|u}} 关于 {{mvar|y}} 的导数，一致地随着 {{mvar|n}} 的增加而趋于零，但解是&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt;u(x,y) = \frac{\sinh ny \sin nx}{n^2}.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;u(x,y) = \frac{\sinh ny \sin nx}{n^2}.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
This solution approaches infinity if {{mvar|nx}} is not an integer multiple of {{pi}} for any non-zero value of {{mvar|y}}. The Cauchy problem for the Laplace equation is called ''ill-posed'' or ''not [[Well-posed problem|well-posed]]'', since the solution does not continuously depend on the data of the problem. Such ill-posed problems are not usually satisfactory for physical applications.&lt;br /&gt;
&lt;br /&gt;
This solution approaches infinity if  is not an integer multiple of  for any non-zero value of . The Cauchy problem for the Laplace equation is called ill-posed or not well-posed, since the solution does not continuously depend on the data of the problem. Such ill-posed problems are not usually satisfactory for physical applications.&lt;br /&gt;
&lt;br /&gt;
对于任何非零的 {{mvar|y}}，如果 {{mvar|nx}} 不是模板 {{pi}} 的整数倍，这个解会接近于无穷大。拉普拉斯方程的柯西问题被称为不适定的（可以译为ill-posed或not well-posed），因为解不是连续地依赖于问题的数据。这种不适定问题通常不能满足物理应用。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The [[Navier–Stokes existence and smoothness|existence of solutions for the Navier–Stokes equations]], a partial differential equation, is part of one of the [[Millennium Prize Problems]].&lt;br /&gt;
&lt;br /&gt;
The existence of solutions for the Navier–Stokes equations, a partial differential equation, is part of one of the Millennium Prize Problems.&lt;br /&gt;
&lt;br /&gt;
偏微分方程”纳维-斯托克斯方程“的解的存在性就是千禧年大奖难题之一的一部分。&lt;br /&gt;
&lt;br /&gt;
== Notation ==&lt;br /&gt;
符号&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
In PDEs, it is common to denote partial derivatives using subscripts. That is:&lt;br /&gt;
&lt;br /&gt;
In PDEs, it is common to denote partial derivatives using subscripts. That is:&lt;br /&gt;
&lt;br /&gt;
在偏微分方程中，通常用下标表示偏导数。例如:&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt;u_x = \frac{\partial u}{\partial x}&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;u_x = \frac{\partial u}{\partial x}&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt;u_{xx} = \frac{\partial^2 u}{\partial x^2} &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;u_{xx} = \frac{\partial^2 u}{\partial x^2} &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt;u_{xy} = \frac{\partial^2 u}{\partial y\, \partial x} = \frac{\partial}{\partial y } \left(\frac{\partial u}{\partial x}\right). &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;u_{xy} = \frac{\partial^2 u}{\partial y\, \partial x} = \frac{\partial}{\partial y } \left(\frac{\partial u}{\partial x}\right). &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Especially in physics, [[del]] or nabla ({{math|∇}}) is often used to denote spatial derivatives, and {{math|''&amp;amp;#x307;u'', ''ü''}} for time derivatives. For example, the [[wave equation]] (mentioned below) can be written as&lt;br /&gt;
&lt;br /&gt;
Especially in physics, del or nabla () is often used to denote spatial derivatives, and  for time derivatives. For example, the wave equation (mentioned below) can be written as&lt;br /&gt;
&lt;br /&gt;
特别是在物理学中，[[del]] 或 nabla ({{math|∇}}) 经常用来表示空间导数和时间导数。例如，波动方程(在下文中提到)可以写成：&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt;\ddot u=c^2\nabla^2u&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt;\ddot u=c^2\nabla^2u&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
or&lt;br /&gt;
&lt;br /&gt;
or&lt;br /&gt;
&lt;br /&gt;
或&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt;\ddot u=c^2\Delta u&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt;\ddot u=c^2\Delta u&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
where {{math|Δ}} is the [[Laplace operator]].&lt;br /&gt;
&lt;br /&gt;
where  is the Laplace operator.&lt;br /&gt;
&lt;br /&gt;
其中，{{math|Δ}} 代表拉普拉斯算子。&lt;br /&gt;
&lt;br /&gt;
== Classification ==&lt;br /&gt;
分类&lt;br /&gt;
&lt;br /&gt;
Some linear, second-order partial differential equations can be classified as [[parabolic partial differential equation|parabolic]], [[hyperbolic partial differential equation|hyperbolic]] and [[elliptic partial differential equation|elliptic]]. Others, such as the [[Euler–Tricomi equation]], have different types in different regions. The classification provides a guide to appropriate initial and boundary conditions and to the smoothness of the solutions.&lt;br /&gt;
&lt;br /&gt;
Some linear, second-order partial differential equations can be classified as parabolic, hyperbolic and elliptic. Others, such as the Euler–Tricomi equation, have different types in different regions. The classification provides a guide to appropriate initial and boundary conditions and to the smoothness of the solutions.&lt;br /&gt;
&lt;br /&gt;
一些线性二阶偏微分方程可分为抛物型方程、双曲型方程和椭圆型方程。其他的方程，如欧拉-特里科米方程，在不同的领域有不同的类型。这种分类有助于选择适当的初始和边界条件以及提高解的平滑性。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
=== Equations of first order ===&lt;br /&gt;
一阶方程&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{{main|First-order partial differential equation}}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
=== Linear equations of second order ===&lt;br /&gt;
二阶线性方程&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Assuming {{math|''u&amp;lt;sub&amp;gt;xy&amp;lt;/sub&amp;gt;'' {{=}} ''u&amp;lt;sub&amp;gt;yx&amp;lt;/sub&amp;gt;''}}, the general linear second-order PDE in two independent variables has the form&lt;br /&gt;
&lt;br /&gt;
Assuming  u&amp;lt;sub&amp;gt;yx&amp;lt;/sub&amp;gt;}}, the general linear second-order PDE in two independent variables has the form&lt;br /&gt;
&lt;br /&gt;
假设 {{math|''u&amp;lt;sub&amp;gt;xy&amp;lt;/sub&amp;gt;'' {{=}} ''u&amp;lt;sub&amp;gt;yx&amp;lt;/sub&amp;gt;''}}，含有两个独立变量的一般线性二阶偏微分方程具有如下形式：&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt;Au_{xx} + 2Bu_{xy} + Cu_{yy} + \cdots \mbox{(lower order terms)} = 0,&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;Au_{xx} + 2Bu_{xy} + Cu_{yy} + \cdots \mbox{(lower order terms)} = 0,&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
where the coefficients {{mvar|A}}, {{mvar|B}}, {{mvar|C}}... may depend upon {{mvar|x}} and {{mvar|y}}. If {{math|''A''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; + ''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; + ''C''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; &amp;gt; 0}} over a region of the {{mvar|xy}}-plane, the PDE is second-order in that region. This form is analogous to the equation for a conic section:&lt;br /&gt;
&lt;br /&gt;
where the coefficients , , ... may depend upon  and . If  over a region of the -plane, the PDE is second-order in that region. This form is analogous to the equation for a conic section:&lt;br /&gt;
&lt;br /&gt;
其中的系数 {{mvar|A}}, {{mvar|B}}, {{mvar|C}}... 一般取决于 {{mvar|x}} 和 {{mvar|y}} 。如果在 {{mvar|xy}}-平面的一个区域上 {{math|''A''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; + ''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; + ''C''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; &amp;gt; 0}}，偏微分方程是二阶的，这种形式类似于圆锥截面的方程:&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt;Ax^2 + 2Bxy + Cy^2 + \cdots = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;Ax^2 + 2Bxy + Cy^2 + \cdots = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
More precisely, replacing {{math|∂&amp;lt;sub&amp;gt;''x''&amp;lt;/sub&amp;gt;}} by {{mvar|X}}, and likewise for other variables (formally this is done by a [[Fourier transform]]), converts a constant-coefficient PDE into a polynomial of the same degree, with the terms of the highest degree (a [[homogeneous polynomial]], here a [[quadratic form]]) being most significant for the classification.&lt;br /&gt;
&lt;br /&gt;
More precisely, replacing  by , and likewise for other variables (formally this is done by a Fourier transform), converts a constant-coefficient PDE into a polynomial of the same degree, with the terms of the highest degree (a homogeneous polynomial, here a quadratic form) being most significant for the classification.&lt;br /&gt;
&lt;br /&gt;
更准确地说，用 {{mvar|X}} 替换 {{math|∂&amp;lt;sub&amp;gt;''x''&amp;lt;/sub&amp;gt;}}，并同样替换其它变量(通常由傅里叶变换完成)，将一个常系数偏微分方程转换成一个相同次数的多项式，最高次数的项(齐次多项式，这里是一个二次形式)对于偏微分方程的分类最为重要。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Just as one classifies [[conic section]]s and quadratic forms into parabolic, hyperbolic, and elliptic based on the [[discriminant]] {{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − 4''AC''}}, the same can be done for a second-order PDE at a given point.  However, the [[discriminant]] in a PDE is given by {{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC''}} due to the convention of the {{mvar|xy}} term being {{math|2''B''}} rather than {{mvar|B}}; formally, the discriminant (of the associated quadratic form) is {{math|(2''B'')&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − 4''AC'' {{=}} 4(''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC'')}}, with the factor of 4 dropped for simplicity.&lt;br /&gt;
&lt;br /&gt;
Just as one classifies conic sections and quadratic forms into parabolic, hyperbolic, and elliptic based on the discriminant , the same can be done for a second-order PDE at a given point.  However, the discriminant in a PDE is given by  due to the convention of the  term being  rather than ; formally, the discriminant (of the associated quadratic form) is  4(B&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − AC)}}, with the factor of 4 dropped for simplicity.&lt;br /&gt;
&lt;br /&gt;
正如人们可以根据判别式 {{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − 4''AC''}} 将圆锥截面和二次型分为抛物型、双曲型和椭圆型一样，对于给定点的二阶偏微分方程也可以这样做。然而，偏微分方程中的判别式 {{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − 4''AC''}} 是根据交叉项的系数{{math|2''B''}} 而不是 {{mvar|B}} 给出的，形式上，判别式(关联二次型)是 {{math|(2''B'')&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − 4''AC'' {{=}} 4(''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC'')}}，为简单起见，去掉了因子4。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
# {{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC'' &amp;lt; 0}} (''[[elliptic partial differential equation]]''): Solutions of [[elliptic partial differential equation|elliptic PDEs]] are as smooth as the coefficients allow, within the interior of the region where the equation and solutions are defined. For example, solutions of [[Laplace's equation]] are analytic within the domain where they are defined, but solutions may assume boundary values that are not smooth. The motion of a fluid at subsonic speeds can be approximated with elliptic PDEs, and the Euler–Tricomi equation is elliptic where {{math|''x'' &amp;lt; 0}}.&lt;br /&gt;
&lt;br /&gt;
  (elliptic partial differential equation): Solutions of elliptic PDEs are as smooth as the coefficients allow, within the interior of the region where the equation and solutions are defined. For example, solutions of Laplace's equation are analytic within the domain where they are defined, but solutions may assume boundary values that are not smooth. The motion of a fluid at subsonic speeds can be approximated with elliptic PDEs, and the Euler–Tricomi equation is elliptic where .&lt;br /&gt;
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{{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC'' &amp;lt; 0}} (椭圆型微分方程)：在定义方程和解的区域内部，椭圆型偏微分方程的解在系数允许的程度内光滑。例如，拉普拉斯方程的解在它们被定义的区域内是解析的，但可能假设边界值是不光滑的。亚音速流体的运动可以用椭圆型偏微分方程近似，欧拉-特里科米方程在 {{math|''x'' &amp;lt; 0}} 时是椭圆型偏微分方程。&lt;br /&gt;
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# {{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC'' {{=}} 0}} (''[[parabolic partial differential equation]]''): Equations that are [[parabolic partial differential equation|parabolic]] at every point can be transformed into a form analogous to the [[heat equation]] by a change of independent variables. Solutions smooth out as the transformed time variable increases. The Euler–Tricomi equation has parabolic type on the line where {{math|''x'' {{=}} 0}}.&lt;br /&gt;
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  0}} (parabolic partial differential equation): Equations that are parabolic at every point can be transformed into a form analogous to the heat equation by a change of independent variables. Solutions smooth out as the transformed time variable increases. The Euler–Tricomi equation has parabolic type on the line where  0}}.&lt;br /&gt;
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{{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC'' {{=}} 0}}（抛物型偏微分方程）：在每一点上都是抛物线型的方程可以通过改变自变量从而转化成类似于热方程的形式。随着转换后的时间变量的增加，方程的解变得平滑。欧拉-特里科米方程在特征线 {{math|''x'' {{=}} 0}} 上是抛物线型的。&lt;br /&gt;
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# {{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC'' &amp;gt; 0}} (''[[hyperbolic partial differential equation]]''): [[hyperbolic partial differential equation|hyperbolic]] equations retain any discontinuities of functions or derivatives in the initial data. An example is the [[wave equation]]. The motion of a fluid at supersonic speeds can be approximated with hyperbolic PDEs, and the Euler–Tricomi equation is hyperbolic where {{math|''x'' &amp;gt; 0}}.&lt;br /&gt;
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  (hyperbolic partial differential equation): hyperbolic equations retain any discontinuities of functions or derivatives in the initial data. An example is the wave equation. The motion of a fluid at supersonic speeds can be approximated with hyperbolic PDEs, and the Euler–Tricomi equation is hyperbolic where .&lt;br /&gt;
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{{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC'' &amp;gt; 0}} (双曲型偏微分方程)：双曲型方程在初始数据中保留了函数或导数的任何不连续性。波动方程就是其中的一个例子。超音速流体的运动可以用双曲型偏微分方程近似，欧拉-特里科米方程在 {{math|''x'' &amp;gt; 0}} 时是双曲型的。&lt;br /&gt;
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If there are {{mvar|n}} independent variables {{math|''x''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;, ''x''&amp;lt;sub&amp;gt;2 &amp;lt;/sub&amp;gt;,… ''x''&amp;lt;sub&amp;gt;''n''&amp;lt;/sub&amp;gt;}}, a general linear partial differential equation of second order has the form&lt;br /&gt;
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If there are  independent variables , a general linear partial differential equation of second order has the form&lt;br /&gt;
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如果存在 {{mvar|n}} 个自变量 {{math|''x''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;, ''x''&amp;lt;sub&amp;gt;2 &amp;lt;/sub&amp;gt;,… ''x''&amp;lt;sub&amp;gt;''n''&amp;lt;/sub&amp;gt;}}，一般二阶线性偏微分方程的形式是：&lt;br /&gt;
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: &amp;lt;math&amp;gt;L u =\sum_{i=1}^n\sum_{j=1}^n a_{i,j} \frac{\partial^2 u}{\partial x_i \partial x_j} \quad \text{ plus lower-order terms} =0.&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;L u =\sum_{i=1}^n\sum_{j=1}^n a_{i,j} \frac{\partial^2 u}{\partial x_i \partial x_j} \quad \text{ plus lower-order terms} =0.&amp;lt;/math&amp;gt;&lt;br /&gt;
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The classification depends upon the signature of the eigenvalues of the coefficient matrix {{math|''a''&amp;lt;sub&amp;gt;''i'',''j''&amp;lt;/sub&amp;gt;}}.&lt;br /&gt;
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The classification depends upon the signature of the eigenvalues of the coefficient matrix .&lt;br /&gt;
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这种分类取决于系数矩阵特征值的符号（正负性）。&lt;br /&gt;
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# Elliptic: the eigenvalues are all positive or all negative.&lt;br /&gt;
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 Elliptic: the eigenvalues are all positive or all negative.&lt;br /&gt;
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椭圆形方程: 特征值全部为正或全部为负。&lt;br /&gt;
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# Parabolic: the eigenvalues are all positive or all negative, save one that is zero.&lt;br /&gt;
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 Parabolic: the eigenvalues are all positive or all negative, save one that is zero.&lt;br /&gt;
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抛物线形方程:除了一个为零值，特征值全部为正或全部为负。&lt;br /&gt;
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# Hyperbolic: there is only one negative eigenvalue and all the rest are positive, or there is only one positive eigenvalue and all the rest are negative.&lt;br /&gt;
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 Hyperbolic: there is only one negative eigenvalue and all the rest are positive, or there is only one positive eigenvalue and all the rest are negative.&lt;br /&gt;
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双曲形方程: 只有一个负特征值，其余的都是正特征值，或者只有一个正特征值，其余的都是负特征值。&lt;br /&gt;
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# Ultrahyperbolic: there is more than one positive eigenvalue and more than one negative eigenvalue, and there are no zero eigenvalues. There is only a limited theory for ultrahyperbolic equations (Courant and Hilbert, 1962).&lt;br /&gt;
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 Ultrahyperbolic: there is more than one positive eigenvalue and more than one negative eigenvalue, and there are no zero eigenvalues. There is only a limited theory for ultrahyperbolic equations (Courant and Hilbert, 1962).&lt;br /&gt;
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超双形方程: 存在多于一个正特征值和多于一个的负特征值，且不存在零特征值。对于超双曲方程，只存在有限的理论(Courant 和 Hilbert，1962)。&lt;br /&gt;
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=== Systems of first-order equations and characteristic surfaces ===&lt;br /&gt;
一阶方程组和特征曲面&lt;br /&gt;
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The classification of partial differential equations can be extended to systems of first-order equations, where the unknown {{mvar|u}} is now a [[Euclidean vector|vector]] with {{mvar|m}} components, and the coefficient matrices {{mvar|A&amp;lt;sub&amp;gt;ν&amp;lt;/sub&amp;gt;}} are {{mvar|m}} by {{mvar|m}} matrices for {{math|''ν'' {{=}} 1, 2,… ''n''}}. The partial differential equation takes the form&lt;br /&gt;
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The classification of partial differential equations can be extended to systems of first-order equations, where the unknown  is now a vector with  components, and the coefficient matrices  are  by  matrices for  1, 2,… n}}. The partial differential equation takes the form&lt;br /&gt;
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偏微分方程的分类可以推广到一阶方程组，其中未知量 {{mvar|u}} 是有 {{mvar|m}} 个分量的向量。对于 {{math|''ν'' {{=}} 1, 2,… ''n''}}，系数矩阵 {{mvar|A&amp;lt;sub&amp;gt;ν&amp;lt;/sub&amp;gt;}} 是 {{mvar|m}} × {{mvar|m}} 的矩阵。偏微分方程形式如下：&lt;br /&gt;
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: &amp;lt;math&amp;gt;Lu = \sum_{\nu=1}^{n} A_\nu \frac{\partial u}{\partial x_\nu} + B=0,&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;Lu = \sum_{\nu=1}^{n} A_\nu \frac{\partial u}{\partial x_\nu} + B=0,&amp;lt;/math&amp;gt;&lt;br /&gt;
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where the coefficient matrices {{mvar|A&amp;lt;sub&amp;gt;ν&amp;lt;/sub&amp;gt;}} and the vector {{mvar|B}} may depend upon {{mvar|x}} and {{mvar|u}}. If a [[hypersurface]] {{mvar|S}} is given in the implicit form&lt;br /&gt;
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where the coefficient matrices  and the vector  may depend upon  and . If a hypersurface  is given in the implicit form&lt;br /&gt;
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其中，系数矩阵 {{mvar|A&amp;lt;sub&amp;gt;ν&amp;lt;/sub&amp;gt;}} 和向量 {{mvar|B}} 可能依赖于 {{mvar|x}} 和 {{mvar|u}}。如果超曲面是以以下隐式形式给出的，&lt;br /&gt;
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: &amp;lt;math&amp;gt;\varphi(x_1, x_2, \ldots x_n)=0,&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;\varphi(x_1, x_2, \ldots x_n)=0,&amp;lt;/math&amp;gt;&lt;br /&gt;
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where {{mvar|φ}} has a non-zero gradient, then {{mvar|S}} is a '''characteristic surface''' for the operator {{mvar|L}} at a given point if the characteristic form vanishes:&lt;br /&gt;
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where  has a non-zero gradient, then  is a characteristic surface for the operator  at a given point if the characteristic form vanishes:&lt;br /&gt;
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其中，存在一个非零的梯度 {{mvar|φ}}，对于在给定点上特征形式消失的算子，特征曲面 {{mvar|S}} 形式如下:&lt;br /&gt;
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: &amp;lt;math&amp;gt;Q\left(\frac{\partial\varphi}{\partial x_1}, \ldots\frac{\partial\varphi}{\partial x_n}\right) =\det\left[\sum_{\nu=1}^nA_\nu \frac{\partial \varphi}{\partial x_\nu}\right]=0.\,&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;Q\left(\frac{\partial\varphi}{\partial x_1}, \ldots\frac{\partial\varphi}{\partial x_n}\right) =\det\left[\sum_{\nu=1}^nA_\nu \frac{\partial \varphi}{\partial x_\nu}\right]=0.\,&amp;lt;/math&amp;gt;&lt;br /&gt;
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The geometric interpretation of this condition is as follows: if data for {{mvar|u}} are prescribed on the surface {{mvar|S}}, then it may be possible to determine the normal derivative of {{mvar|u}} on {{mvar|S}} from the differential equation. If the data on {{mvar|S}} and the differential equation determine the normal derivative of {{mvar|u}} on {{mvar|S}}, then {{mvar|S}} is non-characteristic. If the data on {{mvar|S}} and the differential equation ''do not'' determine the normal derivative of {{mvar|u}} on {{mvar|S}}, then the surface is '''characteristic''', and the differential equation restricts the data on {{mvar|S}}: the differential equation is ''internal'' to {{mvar|S}}.&lt;br /&gt;
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The geometric interpretation of this condition is as follows: if data for  are prescribed on the surface , then it may be possible to determine the normal derivative of  on  from the differential equation. If the data on  and the differential equation determine the normal derivative of  on , then  is non-characteristic. If the data on  and the differential equation do not determine the normal derivative of  on , then the surface is characteristic, and the differential equation restricts the data on : the differential equation is internal to .&lt;br /&gt;
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这个条件的几何解释如下: 如果关于 {{mvar|u}} 的数据是在曲面 {{mvar|S}} 上规定的，那么就有可能依据微分方程确定曲面 {{mvar|S}} 上 {{mvar|u}} 的法向导数。如果曲面 {{mvar|S}} 上的数据和上面的微分方程能确定曲面 {{mvar|S}} 上 {{mvar|u}} 的法向导数，那么它就是非特征的。如果曲面 {{mvar|S}} 上的数据和上面的微分方程不能确定曲面 {{mvar|S}} 上 {{mvar|u}} 的法向导数，那么曲面是特征的，并且微分方程将数据限制在曲面 {{mvar|S}} 上：微分方程是在曲面 {{mvar|S}} 内部。&lt;br /&gt;
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# A first-order system {{math|''Lu'' {{=}} 0}} is ''elliptic'' if no surface is characteristic for {{mvar|L}}: the values of {{mvar|u}} on {{mvar|S}} and the differential equation always determine the normal derivative of {{mvar|u}} on {{mvar|S}}.&lt;br /&gt;
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 A first-order system  0}} is elliptic if no surface is characteristic for : the values of  on  and the differential equation always determine the normal derivative of  on .&lt;br /&gt;
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如果对于 {{mvar|L}} 没有曲面是特征的，则一阶系统 {{math|''Lu'' {{=}} 0}} 是椭圆形的：{{mvar|u}}在 {{mvar|S}} 的值和微分方程总能够决定 {{mvar|S}} 上 {{mvar|u}} 的法向导数。&lt;br /&gt;
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# A first-order system is ''hyperbolic'' at a point if there is a '''spacelike''' surface {{mvar|S}} with normal {{mvar|ξ}} at that point. This means that, given any non-trivial vector {{mvar|η}} orthogonal to {{mvar|ξ}}, and a scalar multiplier {{mvar|λ}}, the equation {{math|''Q''(''λξ'' + ''η'') {{=}} 0}} has {{mvar|m}} real roots {{math|''λ''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;, ''λ''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;,… ''λ''&amp;lt;sub&amp;gt;''m''&amp;lt;/sub&amp;gt;}}. The system is '''strictly hyperbolic''' if these roots are always distinct. The geometrical interpretation of this condition is as follows: the characteristic form {{math|''Q''(''ζ'') {{=}} 0}} defines a cone (the normal cone) with homogeneous coordinates ζ. In the hyperbolic case, this cone has {{mvar|m}} sheets, and the axis {{math|''ζ'' {{=}} ''λξ''}} runs inside these sheets: it does not intersect any of them. But when displaced from the origin by η, this axis intersects every sheet. In the elliptic case, the normal cone has no real sheets.&lt;br /&gt;
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 A first-order system is hyperbolic at a point if there is a spacelike surface  with normal  at that point. This means that, given any non-trivial vector  orthogonal to , and a scalar multiplier , the equation  0}} has  real roots . The system is strictly hyperbolic if these roots are always distinct. The geometrical interpretation of this condition is as follows: the characteristic form  0}} defines a cone (the normal cone) with homogeneous coordinates ζ. In the hyperbolic case, this cone has  sheets, and the axis  λξ}} runs inside these sheets: it does not intersect any of them. But when displaced from the origin by η, this axis intersects every sheet. In the elliptic case, the normal cone has no real sheets.&lt;br /&gt;
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如果在该点存在一个法向量为 {{mvar|ξ}}的 '''&amp;lt;font color=&amp;quot;#ff8000&amp;quot;&amp;gt;类空曲面 Spacclike Surface&amp;lt;/font&amp;gt; {{mvar|S}} ，则一阶系统在那一点是双曲的。这意味着，给定任意正交于 {{mvar|ξ}} 的非平凡向量 {{mvar|η}} 和一个标量乘子 {{mvar|λ}}，方程 {{math|''Q''(''λξ'' + ''η'') {{=}} 0}} 有 {{mvar|m}} 个实根 {{math|''λ''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;, ''λ''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;,… ''λ''&amp;lt;sub&amp;gt;''m''&amp;lt;/sub&amp;gt;}}。如果这些根始终不同，则该系统是严格双曲形的。这个条件的几何解释如下: 特征形式 {{math|''Q''(''ζ'') {{=}} 0}} 定义了一个具有齐次坐标 ζ的圆锥(法线圆锥)。在双曲形的情况下，这个圆锥体有 {{mvar|m}} 层，并且轴 {{math|''ζ'' {{=}} ''λξ''}} 在这些层中运动: 它不与任何一层相交。但是当从原点偏离η时，这条轴线与每一层都相交。在椭圆形的情况下，法向圆锥没有实层。&lt;br /&gt;
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==[[用户:Yuling|Yuling]]（[[用户讨论:Yuling|讨论]]） sheet 这个单词也不很理解，我直译为了“层”&lt;br /&gt;
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=== Equations of mixed type ===&lt;br /&gt;
混合型方程&lt;br /&gt;
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If a PDE has coefficients that are not constant, it is possible that it will not belong to any of these categories but rather be of '''mixed type'''. A simple but important example is the [[Euler–Tricomi equation]]&lt;br /&gt;
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If a PDE has coefficients that are not constant, it is possible that it will not belong to any of these categories but rather be of mixed type. A simple but important example is the Euler–Tricomi equation&lt;br /&gt;
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如果偏微分方程的系数不是常数，那么它可能不属于这些类别中的任何一个，而是属于混合类型。一个简单但重要的例子是欧拉-特里科米方程&lt;br /&gt;
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: &amp;lt;math&amp;gt;u_{xx} = xu_{yy},&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;u_{xx} = xu_{yy},&amp;lt;/math&amp;gt;&lt;br /&gt;
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which is called '''elliptic-hyperbolic''' because it is elliptic in the region {{math|''x'' &amp;lt; 0}}, hyperbolic in the region {{math|''x'' &amp;gt; 0}}, and degenerate parabolic on the line {{math|''x'' {{=}} 0}}.&lt;br /&gt;
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which is called elliptic-hyperbolic because it is elliptic in the region , hyperbolic in the region , and degenerate parabolic on the line  0}}.&lt;br /&gt;
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它在 {{math|''x'' &amp;lt; 0}} 的区域上是椭圆形，在 {{math|''x'' &amp;gt; 0}} 区域上是双曲形，在 {{math|''x'' {{=}} 0}}这条线上是退化为抛物线形，因此称之为椭圆-双曲型。&lt;br /&gt;
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''fill in: Dirichlet and Neumann boundaries, hyperbolic/parabolic/elliptic separation of variables, [[Fourier analysis]], [[Green's function]]s ...--&amp;gt;&lt;br /&gt;
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fill in: Dirichlet and Neumann boundaries, hyperbolic/parabolic/elliptic separation of variables, Fourier analysis, Green's functions ...--&amp;gt;&lt;br /&gt;
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填写: Dirichlet 和 Neumann 边界，双曲 / 抛物线 / 椭圆分离变量法，傅立叶分析，Green 函数... --&lt;br /&gt;
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=== Infinite-order PDEs in quantum mechanics ===&lt;br /&gt;
量子力学中的无限阶偏微分方程&lt;br /&gt;
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In the [[phase space formulation]] of quantum mechanics,  one may consider the [[Method of quantum characteristics|quantum Hamilton's equations]] for trajectories of quantum particles. These equations are infinite-order PDEs. However, in the semiclassical expansion, one has a finite system of ODEs at any fixed order of [[Dirac constant|{{mvar|ħ}}]].  The evolution equation of the [[Wigner quasi-probability distribution|c]] is also an infinite-order PDE. The quantum trajectories are [[Method of quantum characteristics|quantum characteristics]], with the use of which one could calculate the evolution of the Wigner function.&lt;br /&gt;
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In the phase space formulation of quantum mechanics,  one may consider the quantum Hamilton's equations for trajectories of quantum particles. These equations are infinite-order PDEs. However, in the semiclassical expansion, one has a finite system of ODEs at any fixed order of Dirac constant|.  The evolution equation of the Wigner function is also an infinite-order PDE. The quantum trajectories are quantum characteristics, with the use of which one could calculate the evolution of the Wigner function.&lt;br /&gt;
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在量子力学中的相空间表述中，我们可以考虑用于求解量子粒子的轨迹的量子哈密顿的方程。这些方程是无限阶偏微分方程。然而，在半经典展开中，我们在给定[[Dirac constant|{{mvar|ħ}}]]阶数下有一个有限的的常微分方程组。'''&amp;lt;font color=&amp;quot;#ff8000&amp;quot;&amp;gt;维格纳函数  Wigner Function&amp;lt;/font&amp;gt;的演化方程也是一个无限阶偏微分方程。由于量子轨道的量子特性，所以它通常可以用来计算维格纳函数的演化。&lt;br /&gt;
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== Analytical solutions ==&lt;br /&gt;
解析解&lt;br /&gt;
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===Separation of variables===&lt;br /&gt;
分离变量法&lt;br /&gt;
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{{main|Separable partial differential equation}}&lt;br /&gt;
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Linear PDEs can be reduced to systems of ordinary differential equations by the important technique of separation of variables. This technique rests on a characteristic of solutions to differential equations: if one can find any solution that solves the equation and satisfies the boundary conditions, then it is ''the'' solution (this also applies to ODEs). We assume as an [[ansatz]] that the dependence of a solution on the parameters space and time can be written as a product of terms that each depend on a single parameter, and then see if this can be made to solve the problem.&amp;lt;ref&amp;gt;{{cite book|last1=Gershenfeld|first1=Neil|title=The nature of mathematical modeling|date=2000|publisher=Cambridge Univ. Press|location=Cambridge|isbn=0521570956|page=27|edition=Reprinted (with corr.)}}&amp;lt;/ref&amp;gt;&lt;br /&gt;
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Linear PDEs can be reduced to systems of ordinary differential equations by the important technique of separation of variables. This technique rests on a characteristic of solutions to differential equations: if one can find any solution that solves the equation and satisfies the boundary conditions, then it is the solution (this also applies to ODEs). We assume as an ansatz that the dependence of a solution on the parameters space and time can be written as a product of terms that each depend on a single parameter, and then see if this can be made to solve the problem.&lt;br /&gt;
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线性偏微分方程组可以通过分离变量法这一重要方法来简化为常微分方程组。这种方法依赖于微分方程解的一个特征: 如果能找到任何一个满足方程和边界条件的解，那么这个解就是方程的解(这也适用于常微分方程)。我们假设解对参数空间和时间的依赖可以写成对它们每一项的依赖以及一个参数的乘积，然后再看看这是否可以用来解决这个问题。&lt;br /&gt;
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In the method of separation of variables, one reduces a PDE to a PDE in fewer variables, which is an ordinary differential equation if in one variable – these are in turn easier to solve.&lt;br /&gt;
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In the method of separation of variables, one reduces a PDE to a PDE in fewer variables, which is an ordinary differential equation if in one variable – these are in turn easier to solve.&lt;br /&gt;
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在分离变量法方法中，可以将偏微分方程简化为含有更少变量的偏微分方程，如果只有一个变量，那么就变成了一个'''&amp;lt;font color = &amp;quot;#ff8000&amp;quot;&amp;gt;常微分方程 Ordinary Differential Equation&amp;lt;/font&amp;gt;'''-- 反过来，这些方程也更容易求解。&lt;br /&gt;
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This is possible for simple PDEs, which are called [[separable partial differential equation]]s, and the domain is generally a rectangle (a product of intervals). Separable PDEs correspond to [[diagonal matrices]] – thinking of &amp;quot;the value for fixed {{mvar|x}}&amp;quot; as a coordinate, each coordinate can be understood separately.&lt;br /&gt;
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This is possible for simple PDEs, which are called separable partial differential equations, and the domain is generally a rectangle (a product of intervals). Separable PDEs correspond to diagonal matrices – thinking of &amp;quot;the value for fixed &amp;quot; as a coordinate, each coordinate can be understood separately.&lt;br /&gt;
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对于简单的偏微分方程(称为可分离偏微分方程)来说，这是可能的，而且方程通常定义在一个矩形区域(区间的乘积)上。可分离偏微分方程对应于对角线矩阵——以“固定值”为坐标，每个坐标可分开理解。&lt;br /&gt;
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This generalizes to the [[method of characteristics]], and is also used in [[integral transform]]s.&lt;br /&gt;
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This generalizes to the method of characteristics, and is also used in integral transforms.&lt;br /&gt;
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这种方法可以推广到特征曲线法，也可以用于积分变换。&lt;br /&gt;
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===Method of characteristics===&lt;br /&gt;
特征曲线法&lt;br /&gt;
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{{main|Method of characteristics}}&lt;br /&gt;
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In special cases, one can find characteristic curves on which the equation reduces to an ODE – changing coordinates in the domain to straighten these curves allows separation of variables, and is called the [[method of characteristics]].&lt;br /&gt;
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In special cases, one can find characteristic curves on which the equation reduces to an ODE – changing coordinates in the domain to straighten these curves allows separation of variables, and is called the method of characteristics.&lt;br /&gt;
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在特殊情况下，可以找到一些特征曲线，在这些曲线上方程可以变成一个常微分方程——意味着改变坐标从而使这些曲线变直从而达到分离变量的目的，这就是所谓的特征曲线法。&lt;br /&gt;
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More generally, one may find characteristic surfaces.&lt;br /&gt;
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More generally, one may find characteristic surfaces.&lt;br /&gt;
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更一般地说，人们可能会找到特征表面。&lt;br /&gt;
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===Integral transform===&lt;br /&gt;
积分变换&lt;br /&gt;
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An [[integral transform]] may transform the PDE to a simpler one, in particular, a separable PDE. This corresponds to diagonalizing an operator.&lt;br /&gt;
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An integral transform may transform the PDE to a simpler one, in particular, a separable PDE. This corresponds to diagonalizing an operator.&lt;br /&gt;
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积分变换可以将偏微分方程转换为更简单的偏微分方程，特别是可分离的偏微分方程。这对应于对角化算符。&lt;br /&gt;
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An important example of this is [[Fourier analysis]], which diagonalizes the heat equation using the [[eigenbasis]] of sinusoidal waves.&lt;br /&gt;
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An important example of this is Fourier analysis, which diagonalizes the heat equation using the eigenbasis of sinusoidal waves.&lt;br /&gt;
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这方面的一个重要例子是'''&amp;lt;font color = &amp;quot;#ff8000&amp;quot;&amp;gt;傅里叶分析  Fourier Analysis&amp;lt;/font&amp;gt;'''，它使用正弦波的特征基来对角化热方程。&lt;br /&gt;
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If the domain is finite or periodic, an infinite sum of solutions such as a [[Fourier series]] is appropriate, but an integral of solutions such as a [[Fourier integral]] is generally required for infinite domains. The solution for a point source for the heat equation given above is an example of the use of a Fourier integral.&lt;br /&gt;
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If the domain is finite or periodic, an infinite sum of solutions such as a Fourier series is appropriate, but an integral of solutions such as a Fourier integral is generally required for infinite domains. The solution for a point source for the heat equation given above is an example of the use of a Fourier integral.&lt;br /&gt;
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如果区域是有限的或周期性的，那么解为无限和的形式是恰当的，例如傅里叶级数，但是一个解的积分，例如傅立叶积分，一般是在无限区域上的。上面给出的热传导方程的点源解法就是使用傅里叶积分的一个例子。&lt;br /&gt;
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===Change of variables===&lt;br /&gt;
变量代换&lt;br /&gt;
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Often a PDE can be reduced to a simpler form with a known solution by a suitable [[Change of variables (PDE)|change of variables]].  For example, the [[Black–Scholes equation#Derivation|Black–Scholes]] PDE&lt;br /&gt;
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Often a PDE can be reduced to a simpler form with a known solution by a suitable change of variables.  For example, the Black–Scholes PDE&lt;br /&gt;
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偏微分方程通常可以通过变量的适当变化，用已知的解简化为更简单的形式。例如，布莱克-舒尔斯偏微分方程&lt;br /&gt;
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:&amp;lt;math&amp;gt; \frac{\partial V}{\partial t} + \tfrac{1}{2}\sigma^2 S^2\frac{\partial^2 V}{\partial S^2} + rS\frac{\partial V}{\partial S} - rV = 0 &amp;lt;/math&amp;gt;&lt;br /&gt;
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&amp;lt;math&amp;gt; \frac{\partial V}{\partial t} + \tfrac{1}{2}\sigma^2 S^2\frac{\partial^2 V}{\partial S^2} + rS\frac{\partial V}{\partial S} - rV = 0 &amp;lt;/math&amp;gt;&lt;br /&gt;
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is reducible to the [[heat equation]]&lt;br /&gt;
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is reducible to the heat equation&lt;br /&gt;
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可以简化为热传导方程&lt;br /&gt;
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:&amp;lt;math&amp;gt; \frac{\partial u}{\partial \tau} = \frac{\partial^2 u}{\partial x^2}&amp;lt;/math&amp;gt;&lt;br /&gt;
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&amp;lt;math&amp;gt; \frac{\partial u}{\partial \tau} = \frac{\partial^2 u}{\partial x^2}&amp;lt;/math&amp;gt;&lt;br /&gt;
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by the change of variables (for complete details see {{webarchive |url=https://web.archive.org/web/20080411030405/http://www.math.unl.edu/~sdunbar1/Teaching/MathematicalFinance/Lessons/BlackScholes/Solution/solution.shtml |date=April 11, 2008 |title=Solution of the Black Scholes Equation }})&lt;br /&gt;
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by the change of variables (for complete details see )&lt;br /&gt;
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通过变量替换(完整的细节见)&lt;br /&gt;
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:&amp;lt;math&amp;gt;\begin{align}&lt;br /&gt;
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V(S,t) &amp;amp;= K v(x,\tau),\\[5px]&lt;br /&gt;
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x &amp;amp;= \ln\left(\tfrac{S}{K} \right),\\[5px]&lt;br /&gt;
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\tau &amp;amp;= \tfrac{1}{2} \sigma^2 (T - t),\\[5px]&lt;br /&gt;
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v(x,\tau)&amp;amp;=e^{-\alpha x-\beta\tau} u(x,\tau).&lt;br /&gt;
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\end{align}&amp;lt;/math&amp;gt;&lt;br /&gt;
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===Fundamental solution===&lt;br /&gt;
基本解&lt;br /&gt;
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{{main|Fundamental solution}}&lt;br /&gt;
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Inhomogeneous equations can often be solved (for constant coefficient PDEs, always be solved) by finding the [[fundamental solution]] (the solution for a point source), then taking the [[convolution]] with the boundary conditions to get the solution.&lt;br /&gt;
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Inhomogeneous equations can often be solved (for constant coefficient PDEs, always be solved) by finding the fundamental solution (the solution for a point source), then taking the convolution with the boundary conditions to get the solution.&lt;br /&gt;
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非齐次方程(常系数偏微分方程)一般是通过先求出基本解(点源的解) ，然后利用带边界条件的卷积来求解。&lt;br /&gt;
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This is analogous in [[signal processing]] to understanding a filter by its [[impulse response]].&lt;br /&gt;
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This is analogous in signal processing to understanding a filter by its impulse response.&lt;br /&gt;
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这类似于在信号处理中通过滤波器的脉冲响应来理解滤波器。&lt;br /&gt;
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===Superposition principle===&lt;br /&gt;
叠加原理&lt;br /&gt;
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{{further| Superposition principle }}&lt;br /&gt;
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The superposition principle applies to any linear system, including linear systems of PDEs. A common visualization of this concept is the interaction of two waves in phase being combined to result in a greater amplitude, for example {{math|sin ''x'' + sin ''x'' {{=}} 2 sin ''x''}}. The same principle can be observed in PDEs where the solutions may be real or complex and additive. [[Superposition principle|superposition]]&lt;br /&gt;
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The superposition principle applies to any linear system, including linear systems of PDEs. A common visualization of this concept is the interaction of two waves in phase being combined to result in a greater amplitude, for example  2 sin x}}. The same principle can be observed in PDEs where the solutions may be real or complex and additive. superposition&lt;br /&gt;
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'''&amp;lt;font color = &amp;quot;#ff8000&amp;quot;&amp;gt;叠加原理 Superposition Principle&amp;lt;/font&amp;gt;适用于任何线性系统，包括偏微分方程的线性系统。这个概念的一个常见的可视化是两个同相位的波相互作用结合在一起会产生更大的振幅，例如 {{math|sin ''x'' + sin ''x'' {{=}} 2 sin ''x''}}。在偏微分方程中也可以观察到同样的原理，其中的解可能是真实的或复杂的和可加的。叠加&lt;br /&gt;
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If {{math|''u''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;}} and {{math|''u''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;}} are solutions of linear PDE in some function space {{mvar|R}}, then {{math|''u'' {{=}} ''c''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;''u''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; + ''c''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;''u''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;}} with any constants {{math|''c''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;}} and {{math|''c''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;}} are also a solution of that PDE in the same function space.&lt;br /&gt;
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If  and  are solutions of linear PDE in some function space , then  c&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;u&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; + c&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;u&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;}} with any constants  and  are also a solution of that PDE in the same function space.&lt;br /&gt;
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若线性偏微分方程在某个函数空间{{mvar|R}}中有解{{math|''u''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;}} 和 {{math|''u''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;}}，则{{math|''u'' {{=}} ''c''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;''u''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; + ''c''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;''u''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;}}也是该偏微分方程在同一函数空间中的解，其中{{math|''c''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;}} 和 {{math|''c''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;}} 是任意常数。&lt;br /&gt;
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===Methods for non-linear equations===&lt;br /&gt;
非线性方程的求解方法&lt;br /&gt;
{{see also|nonlinear partial differential equation}}&lt;br /&gt;
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There are no generally applicable methods to solve nonlinear PDEs. Still, existence and uniqueness results (such as the [[Cauchy–Kowalevski theorem]]) are often possible, as are proofs of important qualitative and quantitative properties of solutions (getting these results is a major part of [[mathematical analysis|analysis]]). Computational solution to the nonlinear PDEs, the [[split-step method]], exist for specific equations like [[nonlinear Schrödinger equation]].&lt;br /&gt;
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There are no generally applicable methods to solve nonlinear PDEs. Still, existence and uniqueness results (such as the Cauchy–Kowalevski theorem) are often possible, as are proofs of important qualitative and quantitative properties of solutions (getting these results is a major part of analysis). Computational solution to the nonlinear PDEs, the split-step method, exist for specific equations like nonlinear Schrödinger equation.&lt;br /&gt;
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对于非线性偏微分方程，目前还没有普遍适用的求解方法。然而，通常是可能知道解的存在性和唯一性(如柯西-科瓦列夫斯基定理)，也是可能得到解的重要定性和定量性质的证明(得到这些结果是分析的主要部分)。非线性偏微分方程的计算解，即分步法，对一些特定的方程适用，比如非线性'''&amp;lt;font color=&amp;quot;#ff8000&amp;quot;&amp;gt;薛定谔方程 Schrödinger equation&amp;lt;/font&amp;gt;'''。&lt;br /&gt;
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Nevertheless, some techniques can be used for several types of equations. The [[h-principle|{{mvar|h}}-principle]] is the most powerful method to solve [[Underdetermined system|underdetermined]] equations. The [[Riquier–Janet theory]] is an effective method for obtaining information about many analytic [[Overdetermined system|overdetermined]] systems.&lt;br /&gt;
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Nevertheless, some techniques can be used for several types of equations. The -principle is the most powerful method to solve underdetermined equations. The Riquier–Janet theory is an effective method for obtaining information about many analytic overdetermined systems.&lt;br /&gt;
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然而，一些技巧可以用于几种类型的方程。h-原理是求解欠定方程最有效的方法。里基尔-珍妮特理论是一种可以获得许多解析超定系统信息的有效方法。&lt;br /&gt;
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The [[method of characteristics]] can be used in some very special cases to solve partial differential equations.&lt;br /&gt;
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The method of characteristics can be used in some very special cases to solve partial differential equations.&lt;br /&gt;
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特征线法可用于求解某些特殊情况下的偏微分方程。&lt;br /&gt;
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In some cases, a PDE can be solved via [[perturbation analysis]] in which the solution is considered to be a correction to an equation with a known solution. Alternatives are [[numerical analysis]] techniques from simple [[finite difference]] schemes to the more mature [[multigrid]] and [[finite element method]]s. Many interesting problems in science and engineering are solved in this way using [[computer]]s, sometimes high performance [[supercomputer]]s.&lt;br /&gt;
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In some cases, a PDE can be solved via perturbation analysis in which the solution is considered to be a correction to an equation with a known solution. Alternatives are numerical analysis techniques from simple finite difference schemes to the more mature multigrid and finite element methods. Many interesting problems in science and engineering are solved in this way using computers, sometimes high performance supercomputers.&lt;br /&gt;
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在某些情况下，偏微分方程可以通过扰动分析来求解。在扰动分析中，通常是求解将具有已知解的方程修正后的新得到方程。可供选择的数值分析技术从简单的差分格式到更成熟的多重网格和有限元方法。许多有趣的科学和工程问题都是在计算机上用这种方法解决的，有时是高性能超级计算机。&lt;br /&gt;
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===Lie group method===&lt;br /&gt;
李群方法&lt;br /&gt;
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From 1870 [[Sophus Lie]]'s work put the theory of differential equations on a more satisfactory foundation. He showed that the integration theories of the older mathematicians can, by the introduction of what are now called [[Lie group]]s, be referred, to a common source; and that ordinary differential equations which admit the same [[infinitesimal transformation]]s present comparable difficulties of integration. He also emphasized the subject of [[contact transformation|transformations of contact]].&lt;br /&gt;
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From 1870 Sophus Lie's work put the theory of differential equations on a more satisfactory foundation. He showed that the integration theories of the older mathematicians can, by the introduction of what are now called Lie groups, be referred, to a common source; and that ordinary differential equations which admit the same infinitesimal transformations present comparable difficulties of integration. He also emphasized the subject of transformations of contact.&lt;br /&gt;
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从1870年起，索弗斯·李的工作为微分方程理论奠定了一个较为令人满意的基础。他指出，通过引入现在所谓的李群，老一辈数学家的积分理论可以引用到一个共同的来源; 承认相同的无穷小变换的常微分方程在积分方面存在相当的困难。他还强调了接触的转变这一主题。&lt;br /&gt;
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==[[用户:Yuling|Yuling]]（[[用户讨论:Yuling|讨论]]）这句话“He also emphasized the subject of transformations of contact.”中的transformations of contact翻译的不太好。&lt;br /&gt;
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A general approach to solving PDEs uses the symmetry property of differential equations, the continuous [[infinitesimal transformation]]s of solutions to solutions ([[Lie theory]]). Continuous [[group theory]], [[Lie algebras]] and [[differential geometry]] are used to understand the structure of linear and nonlinear partial differential equations for generating integrable equations, to find its [[Lax pair]]s, recursion operators, [[Bäcklund transform]] and finally finding exact analytic solutions to the PDE.&lt;br /&gt;
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A general approach to solving PDEs uses the symmetry property of differential equations, the continuous infinitesimal transformations of solutions to solutions (Lie theory). Continuous group theory, Lie algebras and differential geometry are used to understand the structure of linear and nonlinear partial differential equations for generating integrable equations, to find its Lax pairs, recursion operators, Bäcklund transform and finally finding exact analytic solutions to the PDE.&lt;br /&gt;
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求解偏微分方程的一般方法是利用微分方程的对称性，即解到解的连续无穷小变换(李理论)。连续群论、李代数和微分几何理论被用来理解生成可积方程的线性和非线性偏微分方程的结构，找到它的Lax对、递归算子、 贝克伦德变换，最后找到偏微分方程的精确解析解。&lt;br /&gt;
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Symmetry methods have been recognized to study differential equations arising in mathematics, physics, engineering, and many other disciplines.&lt;br /&gt;
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Symmetry methods have been recognized to study differential equations arising in mathematics, physics, engineering, and many other disciplines.&lt;br /&gt;
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对称方法已被公认可以用于研究出现在数学，物理，工程和许多其他学科的微分方程。&lt;br /&gt;
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===Semianalytical methods===&lt;br /&gt;
半解析方法&lt;br /&gt;
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The [[Adomian decomposition method]], the [[Aleksandr Lyapunov|Lyapunov]] artificial small parameter method, and He's [[homotopy perturbation method]] are all special cases of the more general [[homotopy analysis method]]. These are series expansion methods, and except for the Lyapunov method, are independent of small physical parameters as compared to the well known [[perturbation theory]], thus giving these methods greater flexibility and solution generality.&lt;br /&gt;
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The Adomian decomposition method, the Lyapunov artificial small parameter method, and He's homotopy perturbation method are all special cases of the more general homotopy analysis method. These are series expansion methods, and except for the Lyapunov method, are independent of small physical parameters as compared to the well known perturbation theory, thus giving these methods greater flexibility and solution generality.&lt;br /&gt;
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阿多米安分解法、李雅普诺夫人工小参数方法和何同伦摄动方法都是更一般的同伦分析方法的特殊情况。除了李雅普诺夫方法之外，这些都是级数展开方法，与为人熟知的摄动理论方法相比，它们与小的物理参数无关，因此这些方法具有更大的灵活性和解的通用性。&lt;br /&gt;
&lt;br /&gt;
== Numerical solutions ==&lt;br /&gt;
数值解&lt;br /&gt;
&lt;br /&gt;
The three most widely used [[Numerical partial differential equations|numerical methods to solve PDEs]] are the [[finite element analysis|finite element method]] (FEM), [[finite volume method]]s (FVM) and [[finite difference method]]s (FDM), as well other kind of methods called [[Meshfree methods]], which were made to solve problems where the before mentioned methods are limited. The FEM has a prominent position among these methods and especially its exceptionally efficient higher-order version [[hp-FEM]]. Other hybrid versions of FEM and Meshfree methods include the generalized finite element method (GFEM), [[extended finite element method]] (XFEM), [[Spectral element method|spectral finite element method]] (SFEM), [[Meshfree methods|meshfree finite element method]], [[Discontinuous Galerkin Method|discontinuous Galerkin finite element method]] (DGFEM), [[Element-Free Galerkin Method]] (EFGM), [[Interpolating Element-Free Galerkin Method]] (IEFGM), etc.&lt;br /&gt;
&lt;br /&gt;
The three most widely used numerical methods to solve PDEs are the finite element method (FEM), finite volume methods (FVM) and finite difference methods (FDM), as well other kind of methods called Meshfree methods, which were made to solve problems where the before mentioned methods are limited. The FEM has a prominent position among these methods and especially its exceptionally efficient higher-order version hp-FEM. Other hybrid versions of FEM and Meshfree methods include the generalized finite element method (GFEM), extended finite element method (XFEM), spectral finite element method (SFEM), meshfree finite element method, discontinuous Galerkin finite element method (DGFEM), Element-Free Galerkin Method (EFGM), Interpolating Element-Free Galerkin Method (IEFGM), etc.&lt;br /&gt;
&lt;br /&gt;
求解偏微分方程最常用的三种数值方法是有限元分析法、有限体积法和有限差分法，以及其他一些称为无网格法的方法，用于解决前面用提到的方法求解受到限制的问题。在这些方法中，有限元方法，尤其是高效的高阶有限元方法（hp-FEM），占有重要地位。其他有限元法和无网格法的混合形式包括广义有限元分析法(GFEM)、扩展有限元分析法(XFEM)、谱有限元分析法(SFEM)、无网格有限元分析法(DGFEM)、间断伽辽金有限元分析法(DGFEM)、无单元伽辽金法(EFGM)、插值无单元伽辽金法(IEFGM)等。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
=== Finite element method ===&lt;br /&gt;
有限元分析法&lt;br /&gt;
&lt;br /&gt;
{{main|Finite element method}}&lt;br /&gt;
&lt;br /&gt;
The finite element method (FEM) (its practical application often known as finite element analysis (FEA)) is a numerical technique for finding approximate solutions of partial differential equations (PDE) as well as of integral equations. The solution approach is based either on eliminating the differential equation completely (steady state problems), or rendering the PDE into an approximating system of ordinary differential equations, which are then numerically integrated using standard techniques such as Euler's method, Runge–Kutta, etc.&lt;br /&gt;
&lt;br /&gt;
The finite element method (FEM) (its practical application often known as finite element analysis (FEA)) is a numerical technique for finding approximate solutions of partial differential equations (PDE) as well as of integral equations. The solution approach is based either on eliminating the differential equation completely (steady state problems), or rendering the PDE into an approximating system of ordinary differential equations, which are then numerically integrated using standard techniques such as Euler's method, Runge–Kutta, etc.&lt;br /&gt;
&lt;br /&gt;
'''&amp;lt;font color = &amp;quot;#ff8000&amp;quot;&amp;gt;有限元分析法 Finite Element Method&amp;lt;/font&amp;gt;''' ((其实际应用通常被称为有限元分析(FEA))是一种寻找偏微分方程(PDE)和积分方程近似解的数值技术。这种求解方法要么基于完全消除微分方程(稳态问题) ，要么将偏微分方程转化为常微分方程的近似系统，然后使用标准技术进行数值积分，如欧拉方法、 Runge-Kutta 等。&lt;br /&gt;
&lt;br /&gt;
===Finite difference method===&lt;br /&gt;
有限差分法&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{{main|Finite difference method}}&lt;br /&gt;
&lt;br /&gt;
Finite-difference methods are numerical methods for approximating the solutions to differential equations using [[finite difference]] equations to approximate derivatives.&lt;br /&gt;
&lt;br /&gt;
Finite-difference methods are numerical methods for approximating the solutions to differential equations using finite difference equations to approximate derivatives.&lt;br /&gt;
&lt;br /&gt;
有限差分法是一种数值方法，用差分方程近似微分方程的解。&lt;br /&gt;
&lt;br /&gt;
=== Finite volume method ===&lt;br /&gt;
有限体积法&lt;br /&gt;
&lt;br /&gt;
{{main|Finite volume method}}&lt;br /&gt;
&lt;br /&gt;
Similar to the finite difference method or finite element method, values are calculated at discrete places on a meshed geometry. &amp;quot;Finite volume&amp;quot; refers to the small volume surrounding each node point on a mesh. In the finite volume method, surface integrals in a partial differential equation that contain a divergence term are converted to volume integrals, using the [[divergence theorem]]. These terms are then evaluated as fluxes at the surfaces of each finite volume. Because the flux entering a given volume is identical to that leaving the adjacent volume, these methods conserve mass by design.&lt;br /&gt;
&lt;br /&gt;
Similar to the finite difference method or finite element method, values are calculated at discrete places on a meshed geometry. &amp;quot;Finite volume&amp;quot; refers to the small volume surrounding each node point on a mesh. In the finite volume method, surface integrals in a partial differential equation that contain a divergence term are converted to volume integrals, using the divergence theorem. These terms are then evaluated as fluxes at the surfaces of each finite volume. Because the flux entering a given volume is identical to that leaving the adjacent volume, these methods conserve mass by design.&lt;br /&gt;
&lt;br /&gt;
类似于有限差分法或有限元分析，函数值是在网状几何体上的离散位置进行计算的。“有限体积”是指网格上每个节点周围的小体积。在有限体积法中，偏微分方程中含有散度项的面积分用散度定理积分转换成体积分。然后将这些项用于估算每个有限体积表面上的通量。由于进入给定体积的通量与转移到相邻体积元的通量相同，所以这些方法在设计上保证了质量守恒。&lt;br /&gt;
&lt;br /&gt;
==See also==&lt;br /&gt;
请参阅&lt;br /&gt;
* [[Dirichlet boundary condition]]&lt;br /&gt;
狄利克雷边界条件&lt;br /&gt;
* [[Jet bundle]]&lt;br /&gt;
射流丛&lt;br /&gt;
* [[Laplace transform applied to differential equations]]&lt;br /&gt;
微分方程中的拉普拉斯变换&lt;br /&gt;
* [[List of dynamical systems and differential equations topics]]&lt;br /&gt;
动力学系统列表和微分方程主题&lt;br /&gt;
* [[Matrix differential equation]]&lt;br /&gt;
矩阵微分方程&lt;br /&gt;
* [[Neumann boundary condition]]&lt;br /&gt;
诺伊曼边界条件&lt;br /&gt;
* [[Numerical partial differential equations]]&lt;br /&gt;
数值偏微分方程&lt;br /&gt;
* [[Partial differential algebraic equation]]&lt;br /&gt;
偏微分代数方程&lt;br /&gt;
* [[Recurrence relation]]&lt;br /&gt;
递推关系&lt;br /&gt;
* [[Robin boundary condition]]&lt;br /&gt;
罗宾边界条件&lt;br /&gt;
* [[Stochastic processes and boundary value problems]]&lt;br /&gt;
随机过程和边值问题&lt;br /&gt;
&lt;br /&gt;
== The energy method ==&lt;br /&gt;
能量法&lt;br /&gt;
&lt;br /&gt;
The energy method is a mathematical procedure that can be used to verify well-posedness of initial-boundary-value-problems.&amp;lt;ref&amp;gt;{{cite book |title=High Order Difference Methods for Time Dependent PDE&lt;br /&gt;
&lt;br /&gt;
The energy method is a mathematical procedure that can be used to verify well-posedness of initial-boundary-value-problems.&amp;lt;ref&amp;gt;{{cite book |title=High Order Difference Methods for Time Dependent PDE&lt;br /&gt;
&lt;br /&gt;
能量法是一种数学过程，可用于验证初始边界值问题的适定性。&lt;br /&gt;
&lt;br /&gt;
In the following example the energy method is used to decide where and which boundary conditions should be imposed such that the resulting IBVP is well-posed. Consider the one-dimensional hyperbolic PDE given by&lt;br /&gt;
&lt;br /&gt;
In the following example the energy method is used to decide where and which boundary conditions should be imposed such that the resulting IBVP is well-posed. Consider the one-dimensional hyperbolic PDE given by&lt;br /&gt;
&lt;br /&gt;
在下面的示例中，将使用能量法决定应在何处施加哪些边界条件，以使得到的IBVP处于适当位置。考虑下式给出的一维双曲PDE&lt;br /&gt;
&lt;br /&gt;
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: &amp;lt;math&amp;gt;\frac{\partial u}{\partial t} + \alpha \frac{\partial u}{\partial x} = 0, \quad x \in [a,b], \operatorname t &amp;gt; 0,&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;\frac{\partial u}{\partial t} + \alpha \frac{\partial u}{\partial x} = 0, \quad x \in [a,b], \operatorname t &amp;gt; 0,&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
where &amp;lt;math&amp;gt;\alpha \neq 0&amp;lt;/math&amp;gt; is a constant and &amp;lt;math&amp;gt;u(x,t)&amp;lt;/math&amp;gt; is an unknown function with initial condition &amp;lt;math&amp;gt;u(x,0) = f(x)&amp;lt;/math&amp;gt;. Multiplying with &amp;lt;math&amp;gt;u&amp;lt;/math&amp;gt; and integrating over the domain gives&lt;br /&gt;
&lt;br /&gt;
where &amp;lt;math&amp;gt;\alpha \neq 0&amp;lt;/math&amp;gt; is a constant and &amp;lt;math&amp;gt;u(x,t)&amp;lt;/math&amp;gt; is an unknown function with initial condition &amp;lt;math&amp;gt;u(x,0) = f(x)&amp;lt;/math&amp;gt;. Multiplying with &amp;lt;math&amp;gt;u&amp;lt;/math&amp;gt; and integrating over the domain gives&lt;br /&gt;
&lt;br /&gt;
其中 &amp;lt;math&amp;gt;\alpha \neq 0&amp;lt;/math&amp;gt; 是常数，并且 &amp;lt;math&amp;gt;u(x,t)&amp;lt;/math&amp;gt; 是初始条件是 &amp;lt;math&amp;gt;u(x,0) = f(x)&amp;lt;/math&amp;gt;的未知函数，乘以 &amp;lt;math&amp;gt;u&amp;lt;/math&amp;gt; 并在域上进行积分。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt;\int_a^b u \frac{\partial u}{\partial t} \operatorname dx + \alpha \int _a ^b u \frac{\partial u}{\partial x} \operatorname dx = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;\int_a^b u \frac{\partial u}{\partial t} \operatorname dx + \alpha \int _a ^b u \frac{\partial u}{\partial x} \operatorname dx = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Using that&lt;br /&gt;
&lt;br /&gt;
Using that&lt;br /&gt;
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利用这一点&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt;\int _a ^b u \frac{\partial u}{\partial t} \operatorname dx = \frac{1}{2} \frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 \quad \text{and} \quad \int _a ^b u \frac{\partial u}{\partial x} \operatorname dx = \frac{1}{2} u(b,t)^2 - \frac{1}{2} u(a,t)^2,.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;\int _a ^b u \frac{\partial u}{\partial t} \operatorname dx = \frac{1}{2} \frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 \quad \text{and} \quad \int _a ^b u \frac{\partial u}{\partial x} \operatorname dx = \frac{1}{2} u(b,t)^2 - \frac{1}{2} u(a,t)^2,.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
where integration by parts has been used for the second relationship, we get&lt;br /&gt;
&lt;br /&gt;
where integration by parts has been used for the second relationship, we get&lt;br /&gt;
&lt;br /&gt;
第二个关系中采用了分部积分法，我们可以得到&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt;\frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 + \alpha u(b,t)^2 - \alpha u(a,t)^2 = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;\frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 + \alpha u(b,t)^2 - \alpha u(a,t)^2 = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Here &amp;lt;math&amp;gt;\vert \vert \cdot \vert \vert&amp;lt;/math&amp;gt; denotes the standard L2-norm.&lt;br /&gt;
&lt;br /&gt;
Here &amp;lt;math&amp;gt;\vert \vert \cdot \vert \vert&amp;lt;/math&amp;gt; denotes the standard L2-norm.&lt;br /&gt;
&lt;br /&gt;
在这里，&amp;lt;math&amp;gt;\vert \vert \cdot \vert \vert&amp;lt;/math&amp;gt; 表示标准的L2-正则。&lt;br /&gt;
&lt;br /&gt;
For well-posedness we require that the energy of the solution is non-increasing, i.e. that &amp;lt;math&amp;gt;\frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 \leq 0&amp;lt;/math&amp;gt;, which is achieved by specifying &amp;lt;math&amp;gt;u&amp;lt;/math&amp;gt; at &amp;lt;math&amp;gt;x = a&amp;lt;/math&amp;gt; if &amp;lt;math&amp;gt;\alpha &amp;gt; 0&amp;lt;/math&amp;gt; and at &amp;lt;math&amp;gt;x = b&amp;lt;/math&amp;gt; if &amp;lt;math&amp;gt;\alpha &amp;lt; 0&amp;lt;/math&amp;gt;. This corresponds to only imposing boundary conditions at the inflow. Note that well-posedness allows for growth in terms of data (initial and boundary) and thus it is sufficient to show that &amp;lt;math&amp;gt;\frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 \leq 0&amp;lt;/math&amp;gt; holds when all data is set to zero.&lt;br /&gt;
&lt;br /&gt;
For well-posedness we require that the energy of the solution is non-increasing, i.e. that &amp;lt;math&amp;gt;\frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 \leq 0&amp;lt;/math&amp;gt;, which is achieved by specifying &amp;lt;math&amp;gt;u&amp;lt;/math&amp;gt; at &amp;lt;math&amp;gt;x = a&amp;lt;/math&amp;gt; if &amp;lt;math&amp;gt;\alpha &amp;gt; 0&amp;lt;/math&amp;gt; and at &amp;lt;math&amp;gt;x = b&amp;lt;/math&amp;gt; if &amp;lt;math&amp;gt;\alpha &amp;lt; 0&amp;lt;/math&amp;gt;. This corresponds to only imposing boundary conditions at the inflow. Note that well-posedness allows for growth in terms of data (initial and boundary) and thus it is sufficient to show that &amp;lt;math&amp;gt;\frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 \leq 0&amp;lt;/math&amp;gt; holds when all data is set to zero.&lt;br /&gt;
&lt;br /&gt;
对于适定性，我们要求解的能量是不增加的，即 &amp;lt;math&amp;gt;\frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 \leq 0&amp;lt;/math&amp;gt; ，这种关系可以通过在&amp;lt;math&amp;gt;x = a&amp;lt;/math&amp;gt;处 （如果 &amp;lt;math&amp;gt;\alpha &amp;gt; 0&amp;lt;/math&amp;gt;） 以及 &amp;lt;math&amp;gt;x = b&amp;lt;/math&amp;gt;处 （如果 &amp;lt;math&amp;gt;\alpha &amp;lt; 0&amp;lt;/math&amp;gt;）指定&amp;lt;math&amp;gt;u&amp;lt;/math&amp;gt;的值来实现。这相当于只在流入处附加边界条件。注意，适定性允许在数据项(初始和边界)上的增长，因此它足以表明当所有数据设置为零时应有 &amp;lt;math&amp;gt;\frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 \leq 0&amp;lt;/math&amp;gt;。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==Notes==&lt;br /&gt;
&lt;br /&gt;
{{Reflist}}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
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&lt;br /&gt;
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* {{Citation |first=P. |last=Solin |title=Partial Differential Equations and the Finite Element Method |publisher=J. Wiley &amp;amp; Sons |location=Hoboken, NJ |year=2005 |isbn=0-471-72070-4 }}.&lt;br /&gt;
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* {{Citation |first=P. |last=Solin |first2=K. |last2=Segeth |lastauthoramp=yes |first3=I. |last3=Dolezel |title=Higher-Order Finite Element Methods |publisher=Chapman &amp;amp; Hall/CRC Press |location=Boca Raton |year=2003 |isbn=1-58488-438-X }}.&lt;br /&gt;
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* {{Citation |first=H. |last=Stephani |year=1989 |title=Differential Equations: Their Solution Using Symmetries. Edited by M. MacCallum |publisher=Cambridge University Press }}.&lt;br /&gt;
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* {{cite book |title=Partial Differential Equations and Solitary Waves Theory&lt;br /&gt;
&lt;br /&gt;
|first=Abdul-Majid|last=Wazwaz|publisher=Higher Education Press|year=2009|isbn=978-3-642-00251-9|page=}}&lt;br /&gt;
&lt;br /&gt;
|first=Abdul-Majid|last=Wazwaz|publisher=Higher Education Press|year=2009|isbn=978-3-642-00251-9|page=}}&lt;br /&gt;
&lt;br /&gt;
| first Abdul-Majid | last Wazwaz | publisher Higher Education Press | year 2009 | isbn 978-3-642-00251-9 | page }&lt;br /&gt;
&lt;br /&gt;
* {{cite book |title=Partial Differential Equations Methods and Applications&lt;br /&gt;
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|first=Abdul-Majid|last=Wazwaz|publisher=A.A. Balkema|year=2002|isbn=90-5809-369-7|page=}}&lt;br /&gt;
&lt;br /&gt;
|first=Abdul-Majid|last=Wazwaz|publisher=A.A. Balkema|year=2002|isbn=90-5809-369-7|page=}}&lt;br /&gt;
&lt;br /&gt;
| first Abdul-Majid | last Wazwaz | publisher a.a.Balkema | year 2002 | isbn 90-5809-369-7 | page }&lt;br /&gt;
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* {{Citation |first=D. |last=Zwillinger |title=Handbook of Differential Equations |publisher=Academic Press |location=Boston |year=1997 |edition=3rd |isbn=0-12-784395-7 }}.&lt;br /&gt;
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* {{Citation |authorlink=Neil Gershenfeld |first=N. |last=Gershenfeld |title=The Nature of Mathematical Modeling |location=New York |publisher=Cambridge University Press, New York, NY, USA |year=1999 |edition=1st |isbn=0-521-57095-6 }}.&lt;br /&gt;
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* {{Citation |first=I.S. |last=Krasil'shchik |lastauthoramp=yes |first2=A.M., Eds. |last2=Vinogradov |title=Symmetries and Conserwation Laws for Differential Equations of Mathematical Physics |publisher=American Mathematical Society, Providence, Rhode Island, USA |year=1999 |isbn=0-8218-0958-X }}.&lt;br /&gt;
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* {{Citation |first=I.S. |last=Krasil'shchik |first2=V.V. |last2=Lychagin|lastauthoramp=yes |first3=A.M. |last3=Vinogradov |title=Geometry of Jet Spaces and Nonlinear Partial Differential Equations |publisher=Gordon and Breach Science Publishers, New York, London, Paris, Montreux, Tokyo |year=1986 |isbn=2-88124-051-8 }}.&lt;br /&gt;
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* {{Citation |first=A.M. |last=Vinogradov |title=Cohomological Analysis of Partial Differential Equations and Secondary Calculus |publisher=American Mathematical Society, Providence, Rhode Island, USA |year=2001 |isbn=0-8218-2922-X }}.&lt;br /&gt;
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* {{cite book |title=High Order Difference Methods for Time Dependent PDE&lt;br /&gt;
&lt;br /&gt;
|first=Bertil|last=Gustafsson|publisher=Springer|year=2008|isbn=978-3-540-74992-9|doi=10.1007/978-3-540-74993-6}}&lt;br /&gt;
&lt;br /&gt;
|first=Bertil|last=Gustafsson|publisher=Springer|year=2008|isbn=978-3-540-74992-9|doi=10.1007/978-3-540-74993-6}}&lt;br /&gt;
&lt;br /&gt;
| first Bertil | last Gustafsson | Springer | year 2008 | isbn 978-3-540-74992-9 | doi 10.1007 / 978-3-540-74993-6}&lt;br /&gt;
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{{refend}}&lt;br /&gt;
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== Further reading ==&lt;br /&gt;
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* {{Cite journal|last=Cajori|first=Florian|authorlink=Florian Cajori|year=1928|title=The Early History of Partial Differential Equations and of Partial Differentiation and Integration|url=http://www.math.harvard.edu/archive/21a_fall_14/exhibits/cajori/cajori.pdf|journal=The American Mathematical Monthly|volume=35|issue=9|pages=459–467|doi=10.2307/2298771|access-date=2016-05-15|archive-url=https://web.archive.org/web/20181123102253/http://www.math.harvard.edu/archive/21a_fall_14/exhibits/cajori/cajori.pdf|archive-date=2018-11-23|url-status=dead}}&lt;br /&gt;
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== External links ==&lt;br /&gt;
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{{Sister project links| wikt=no | commons=Category:Solutions of PDE | b=Partial Differential Equations | n=no | q=Partial differential equation | s=no | v=no | voy=no | species=no | d=no}}&lt;br /&gt;
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* {{springer|title=Differential equation, partial|id=p/d031920}}&lt;br /&gt;
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* [http://eqworld.ipmnet.ru/en/pde-en.htm Partial Differential Equations: Exact Solutions] at EqWorld: The World of Mathematical Equations.&lt;br /&gt;
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* [http://eqworld.ipmnet.ru/en/solutions/eqindex/eqindex-pde.htm Partial Differential Equations: Index] at EqWorld: The World of Mathematical Equations.&lt;br /&gt;
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* [http://eqworld.ipmnet.ru/en/methods/meth-pde.htm Partial Differential Equations: Methods] at EqWorld: The World of Mathematical Equations.&lt;br /&gt;
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* [https://web.archive.org/web/20170701144823/http://www.exampleproblems.com/wiki/index.php?title=Partial_Differential_Equations Example problems with solutions] at exampleproblems.com&lt;br /&gt;
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* [http://mathworld.wolfram.com/PartialDifferentialEquation.html Partial Differential Equations] at mathworld.wolfram.com&lt;br /&gt;
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* [https://reference.wolfram.com/language/FEMDocumentation/tutorial/SolvingPDEwithFEM.html Partial Differential Equations] with Mathematica&lt;br /&gt;
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* [http://www.mathworks.com/moler/pdes.pdf Partial Differential Equations] in Cleve Moler: Numerical Computing with MATLAB&lt;br /&gt;
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* [http://www.nag.com/numeric/fl/nagdoc_fl24/html/D03/d03intro.html Partial Differential Equations] at nag.com&lt;br /&gt;
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* {{cite web |first=Grant |last=Sanderson |title=But what is a partial differential equation? |work=3Blue1Brown |date=April 21, 2019 |url=https://www.youtube.com/watch?v=ly4S0oi3Yz8&amp;amp;list=PLZHQObOWTQDNPOjrT6KVlfJuKtYTftqH6 |via=[[YouTube]] }}&lt;br /&gt;
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{{Differential equations topics}}&lt;br /&gt;
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[[Category:Partial differential equations| ]]&lt;br /&gt;
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[[Category:Multivariable calculus]]&lt;br /&gt;
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Category:Multivariable calculus&lt;br /&gt;
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类别: 多元微积分&lt;br /&gt;
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[[Category:Differential equations]]&lt;br /&gt;
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Category:Differential equations&lt;br /&gt;
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类别: 微分方程&lt;br /&gt;
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Category:Concepts in physics&lt;br /&gt;
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&amp;lt;small&amp;gt;This page was moved from [[wikipedia:en:Partial differential equation]]. Its edit history can be viewed at [[偏微分方程/edithistory]]&amp;lt;/small&amp;gt;&amp;lt;/noinclude&amp;gt;&lt;br /&gt;
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[[Category:待整理页面]]&lt;/div&gt;</summary>
		<author><name>Ruili</name></author>
	</entry>
	<entry>
		<id>https://wiki.swarma.org/index.php?title=%E5%81%8F%E5%BE%AE%E5%88%86%E6%96%B9%E7%A8%8B&amp;diff=20105</id>
		<title>偏微分方程</title>
		<link rel="alternate" type="text/html" href="https://wiki.swarma.org/index.php?title=%E5%81%8F%E5%BE%AE%E5%88%86%E6%96%B9%E7%A8%8B&amp;diff=20105"/>
		<updated>2020-12-15T13:06:35Z</updated>

		<summary type="html">&lt;p&gt;Ruili：&lt;/p&gt;
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&lt;div&gt;此词条暂由Yuling翻译，未经人工整理和审校，带来阅读不便，请见谅。&lt;br /&gt;
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[[File:Heat.gif|thumb|right|A visualisation of a solution to the two-dimensional [[heat equation]] with temperature represented by the third dimension]]&lt;br /&gt;
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A visualisation of a solution to the two-dimensional [[heat equation with temperature represented by the third dimension]]&lt;br /&gt;
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以三维表示温度的二维热方程解的可视化&lt;br /&gt;
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In [[mathematics]], a '''partial differential equation''' ('''PDE''') is a [[differential equation]] that contains unknown [[Multivariable calculus|multivariable functions]] and their [[partial derivative]]s. PDEs are used to formulate problems involving functions of several variables, and are either solved by hand, or used to create a [[computer model]]. A special case is [[ordinary differential equation]]s (ODEs), which deal with functions of a single variable and their derivatives.&lt;br /&gt;
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In mathematics, a partial differential equation (PDE) is a differential equation that contains unknown multivariable functions and their partial derivatives. PDEs are used to formulate problems involving functions of several variables, and are either solved by hand, or used to create a computer model. A special case is ordinary differential equations (ODEs), which deal with functions of a single variable and their derivatives.&lt;br /&gt;
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在数学中，'''&amp;lt;font color = &amp;quot;#ff8000&amp;quot;&amp;gt; 偏微分方程函数 Partial Differential Equation&amp;lt;/font&amp;gt;'''是包含未知多元函数及其偏导数的微分方程。偏微分方程用于描述涉及多元函数的问题，可以通过人为求解，也可以通过建立计算机模型来求解。常微分方程是偏微分方程一种特殊情况，它处理的是一元函数及其导数。&lt;br /&gt;
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PDEs can be used to describe a wide variety of phenomena such as sound, heat, [[diffusion]], [[electrostatics]], [[Electromagnetism|electrodynamics]], [[fluid dynamics]], [[Elasticity (physics)|elasticity]], [[gravitation]] and [[quantum mechanics]]. These seemingly distinct physical phenomena can be formalised similarly in terms of PDEs. Just as ordinary differential equations often model one-dimensional [[dynamical system]]s, partial differential equations often model [[multidimensional system]]s. PDEs find their generalisation in [[stochastic partial differential equation]]s.&lt;br /&gt;
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PDEs can be used to describe a wide variety of phenomena such as sound, heat, diffusion, electrostatics, electrodynamics, fluid dynamics, elasticity, gravitation and quantum mechanics. These seemingly distinct physical phenomena can be formalised similarly in terms of PDEs. Just as ordinary differential equations often model one-dimensional dynamical systems, partial differential equations often model multidimensional systems. PDEs find their generalisation in stochastic partial differential equations.&lt;br /&gt;
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偏微分方程可以用来描述各种各样的物理现象，如声音，热量，扩散，静电，电动力学，流体力学，弹性力学，重力和量子力学。这些看起来截然不同的物理现象却可以用类似的偏微分方程来描述。正如常微分方程经常对一维动力系统进行建模一样，偏微分方程经常对多维系统进行建模。随机偏微分方程是偏微分方程的一种推广。&lt;br /&gt;
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== Introduction ==&lt;br /&gt;
引言&lt;br /&gt;
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Partial differential equations (PDEs) are equations that involve rates of change with respect to [[continuous variables]]. For example, the position of a [[rigid body]] is specified by six parameters,&amp;lt;ref&amp;gt;{{Cite book|url=https://books.google.com/books?id=v9PLbcYd9aUC&amp;amp;pg=PA32|title=Modelling and Control of Robot Manipulators|last=Sciavicco|first=Lorenzo|last2=Siciliano|first2=Bruno|date=2001-02-19|publisher=Springer Science &amp;amp; Business Media|isbn=9781852332211|language=en}}&amp;lt;/ref&amp;gt; but the configuration of a [[fluid]] is given by the [[continuous distribution]] of several parameters, such as the [[temperature]], [[pressure]], and so forth. The dynamics for the rigid body take place in a finite-dimensional [[Configuration space (physics)|configuration space]]; the dynamics for the fluid occur in an infinite-dimensional configuration space. This distinction usually makes PDEs much harder to solve than ordinary differential equations (ODEs), but here again, there will be simple solutions for linear problems. Classic domains where PDEs are used include [[acoustics]], [[fluid dynamics]], [[electrodynamics]], and [[heat transfer]].&lt;br /&gt;
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Partial differential equations (PDEs) are equations that involve rates of change with respect to continuous variables. For example, the position of a rigid body is specified by six parameters, but the configuration of a fluid is given by the continuous distribution of several parameters, such as the temperature, pressure, and so forth. The dynamics for the rigid body take place in a finite-dimensional configuration space; the dynamics for the fluid occur in an infinite-dimensional configuration space. This distinction usually makes PDEs much harder to solve than ordinary differential equations (ODEs), but here again, there will be simple solutions for linear problems. Classic domains where PDEs are used include acoustics, fluid dynamics, electrodynamics, and heat transfer.&lt;br /&gt;
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偏微分方程(简称为PDEs)涉及到方程相对于连续变量的变化率。例如，刚体的位置是由六个参数确定的，而流体的状态是由几个参数的连续分布给出的，如温度、压力等。刚体的动力学过程发生在有限维状态空间中，流体的动力学过程发生在无限维状态空间中。这种区别通常使偏微分方程比常微分方程更难求解，但是线性问题仍然有简单的求解方式。使用偏微分方程的经典领域包括声学、流体力学、电动力学和传热学。&lt;br /&gt;
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A partial differential equation (PDE) for the function {{math|''u''(''x''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;,… ''x&amp;lt;sub&amp;gt;n&amp;lt;/sub&amp;gt;'')}} is an equation of the form&lt;br /&gt;
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A partial differential equation (PDE) for the function  is an equation of the form&lt;br /&gt;
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函数 {{math|''u''(''x''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;,… ''x&amp;lt;sub&amp;gt;n&amp;lt;/sub&amp;gt;'')}} 的偏微分方程形式是：&lt;br /&gt;
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: &amp;lt;math&amp;gt;f \left (x_1, \ldots x_n; u, \frac{\partial u}{\partial x_1}, \ldots \frac{\partial u}{\partial x_n}; \frac{\partial^2 u}{\partial x_1 \partial x_1}, \ldots \frac{\partial^2 u}{\partial x_1 \partial x_n}; \ldots \right) = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;f \left (x_1, \ldots x_n; u, \frac{\partial u}{\partial x_1}, \ldots \frac{\partial u}{\partial x_n}; \frac{\partial^2 u}{\partial x_1 \partial x_1}, \ldots \frac{\partial^2 u}{\partial x_1 \partial x_n}; \ldots \right) = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
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If {{mvar|f}} is a [[linear function]] of {{mvar|u}} and its derivatives, then the PDE is called linear. Common examples of linear PDEs include the [[heat equation]], the [[wave equation]], [[Laplace's equation]], [[Helmholtz equation]], [[Klein–Gordon equation]], and [[Poisson's equation]].&lt;br /&gt;
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If  is a linear function of  and its derivatives, then the PDE is called linear. Common examples of linear PDEs include the heat equation, the wave equation, Laplace's equation, Helmholtz equation, Klein–Gordon equation, and Poisson's equation.&lt;br /&gt;
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如果 {{mvar|f}} 是函数 {{math|''u''}} 及其导数的线性函数，则偏微分方程称为线性函数。线性偏微分方程的常见例子包括热方程、波动方程、拉普拉斯方程、亥姆霍兹方程方程、克莱因-高登方程和泊松方程。&lt;br /&gt;
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A relatively simple PDE is&lt;br /&gt;
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A relatively simple PDE is&lt;br /&gt;
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一个相对简单的偏微分方程：&lt;br /&gt;
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: &amp;lt;math&amp;gt;\frac{\partial u}{\partial x}(x,y) = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;\frac{\partial u}{\partial x}(x,y) = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
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This relation [[Logical implication|implies]] that the function {{math|''u''(''x'',''y'')}} is independent of {{mvar|x}}. However, the equation gives no information on the function's dependence on the variable {{mvar|y}}. Hence the general solution of this equation is&lt;br /&gt;
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This relation implies that the function  is independent of . However, the equation gives no information on the function's dependence on the variable . Hence the general solution of this equation is&lt;br /&gt;
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这意味着函数 {{math|''u''(''x'',''y'')}} 独立于 {{mvar|x}} 的。然而，这个方程没有给出关于函数和自变量的相关性的信息。因此，这个方程的通解是&lt;br /&gt;
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: &amp;lt;math&amp;gt;u(x,y) = f(y),&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;u(x,y) = f(y),&amp;lt;/math&amp;gt;&lt;br /&gt;
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where {{mvar|f}} is an arbitrary function of {{mvar|y}}. The analogous ordinary differential equation is&lt;br /&gt;
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where  is an arbitrary function of . The analogous ordinary differential equation is&lt;br /&gt;
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其中， {{mvar|f}} 是 {{mvar|y}} 的任意函数。&lt;br /&gt;
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类似的常微分方程是：&lt;br /&gt;
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: &amp;lt;math&amp;gt;\frac{\mathrm{d} u}{\mathrm{d} x}(x) = 0,&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;\frac{\mathrm{d} u}{\mathrm{d} x}(x) = 0,&amp;lt;/math&amp;gt;&lt;br /&gt;
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which has the solution&lt;br /&gt;
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which has the solution&lt;br /&gt;
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它的解为&lt;br /&gt;
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: &amp;lt;math&amp;gt;u(x) = c,&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;u(x) = c,&amp;lt;/math&amp;gt;&lt;br /&gt;
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where {{mvar|c}} is any [[Constant (mathematics)|constant]] value. These two examples illustrate that general solutions of ordinary differential equations (ODEs) involve arbitrary constants, but solutions of PDEs involve arbitrary functions.&lt;br /&gt;
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where  is any constant value. These two examples illustrate that general solutions of ordinary differential equations (ODEs) involve arbitrary constants, but solutions of PDEs involve arbitrary functions.&lt;br /&gt;
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这里，{{mvar|c}} 是一个任意常量。&lt;br /&gt;
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这两个例子说明常微分方程的一般解包含任意常数，但偏微分方程的解包含任意函数。&lt;br /&gt;
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A solution of a PDE is generally not [[Uniqueness quantification|unique]]; additional conditions must generally be specified on the [[Boundary (topology)|boundary]] of the region where the solution is defined. For instance, in the simple example above, the function {{math|''f''(''y'')}} can be determined if {{mvar|u}} is specified on the line {{math|''x'' {{=}} 0}}.&lt;br /&gt;
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A solution of a PDE is generally not unique; additional conditions must generally be specified on the boundary of the region where the solution is defined. For instance, in the simple example above, the function  can be determined if  is specified on the line  0}}.&lt;br /&gt;
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偏微分方程的解一般不是唯一的; 一般必须在定义解的区域边界上定义附加条件。 例如，在上面的简单示例中，如果在 {{math|''x'' {{=}} 0}} 时确定了 {{mvar|u}} 的值，则可以确定该函数 {{math|''f''(''y'')}}。&lt;br /&gt;
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== Existence and uniqueness ==&lt;br /&gt;
存在性和唯一性&lt;br /&gt;
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Although the issue of existence and uniqueness of solutions of ordinary differential equations has a very satisfactory answer with the [[Picard–Lindelöf theorem]], that is far from the case for partial differential equations. The [[Cauchy–Kowalevski theorem]] states that the [[Cauchy problem]] for any partial differential equation whose coefficients are [[Analytic function|analytic]] in the unknown function and its derivatives, has a locally unique analytic solution. Although this result might appear to settle the existence and uniqueness of solutions, there are examples of linear partial differential equations whose coefficients have derivatives of all orders (which are nevertheless not analytic) but which have no solutions at all: see [[Lewy's example|Lewy (1957)]]. Even if the solution of a partial differential equation exists and is unique, it may nevertheless have undesirable properties.  The mathematical study of these questions is usually in the more powerful context of [[weak solution]]s.&lt;br /&gt;
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Although the issue of existence and uniqueness of solutions of ordinary differential equations has a very satisfactory answer with the Picard–Lindelöf theorem, that is far from the case for partial differential equations. The Cauchy–Kowalevski theorem states that the Cauchy problem for any partial differential equation whose coefficients are analytic in the unknown function and its derivatives, has a locally unique analytic solution. Although this result might appear to settle the existence and uniqueness of solutions, there are examples of linear partial differential equations whose coefficients have derivatives of all orders (which are nevertheless not analytic) but which have no solutions at all: see Lewy (1957). Even if the solution of a partial differential equation exists and is unique, it may nevertheless have undesirable properties.  The mathematical study of these questions is usually in the more powerful context of weak solutions.&lt;br /&gt;
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尽管常微分方程解的存在性和唯一性用'''&amp;lt;font color=&amp;quot;#ff8000&amp;quot;&amp;gt;弗罗贝尼乌斯定理 Picard–Lindelöf Theorem&amp;lt;/font&amp;gt;得到了令人满意的结果，但偏微分方程解的存在性和唯一性却远没有得到解决。'''&amp;lt;font color=&amp;quot;#ff8000&amp;quot;&amp;gt;柯西-科瓦列夫斯基定理 Cauchy–Kowalevski theorem&amp;lt;/font&amp;gt;指出：对于任意系数在未知函数及其导数中解析的偏微分方程，柯西问题存在一个局部唯一的解析解。虽然这个结果似乎解决了解的存在性和唯一性问题，但是存在一些线性偏微分方程-其系数具有所有级数的导数(尽管这些导数不是解析的) ，但是根本没有解: 见 Lewy (1957)。即使偏微分方程的解存在且唯一，它仍然可能具有不可预料的性质。这些问题的数学研究通常是在更有力的弱解的背景下进行的。&lt;br /&gt;
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An example of pathological behavior is the sequence (depending upon {{mvar|n}}) of [[Cauchy problem]]s for the [[Laplace equation]]&lt;br /&gt;
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An example of pathological behavior is the sequence (depending upon ) of Cauchy problems for the Laplace equation&lt;br /&gt;
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反常特征的一个例子是拉普拉斯方程的柯西问题的序列(取决于{{mvar|n}})&lt;br /&gt;
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: &amp;lt;math&amp;gt;\frac{\partial^2 u}{\partial x^2} + \frac{\partial^2 u}{\partial y^2}=0,&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;\frac{\partial^2 u}{\partial x^2} + \frac{\partial^2 u}{\partial y^2}=0,&amp;lt;/math&amp;gt;&lt;br /&gt;
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with [[boundary condition]]s&lt;br /&gt;
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with boundary conditions&lt;br /&gt;
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具有边界条件&lt;br /&gt;
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: &amp;lt;math&amp;gt;\begin{align} u(x,0) &amp;amp;= 0, \\ \frac{\partial u}{\partial y}(x,0) &amp;amp;= \frac{\sin nx}{n}, \end{align}&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;\begin{align} u(x,0) &amp;amp;= 0, \\ \frac{\partial u}{\partial y}(x,0) &amp;amp;= \frac{\sin nx}{n}, \end{align}&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
where {{mvar|n}} is an integer. The derivative of {{mvar|u}} with respect to {{mvar|y}} approaches zero [[uniform convergence|uniformly]] in {{mvar|x}} as {{mvar|n}} increases, but the solution is&lt;br /&gt;
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where  is an integer. The derivative of  with respect to  approaches zero uniformly in  as  increases, but the solution is&lt;br /&gt;
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其中 {{mvar|n}} 是整数。{{mvar|u}} 关于 {{mvar|y}} 的导数，一致地随着 {{mvar|n}} 的增加而趋于零，但解是&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
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: &amp;lt;math&amp;gt;u(x,y) = \frac{\sinh ny \sin nx}{n^2}.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;u(x,y) = \frac{\sinh ny \sin nx}{n^2}.&amp;lt;/math&amp;gt;&lt;br /&gt;
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This solution approaches infinity if {{mvar|nx}} is not an integer multiple of {{pi}} for any non-zero value of {{mvar|y}}. The Cauchy problem for the Laplace equation is called ''ill-posed'' or ''not [[Well-posed problem|well-posed]]'', since the solution does not continuously depend on the data of the problem. Such ill-posed problems are not usually satisfactory for physical applications.&lt;br /&gt;
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This solution approaches infinity if  is not an integer multiple of  for any non-zero value of . The Cauchy problem for the Laplace equation is called ill-posed or not well-posed, since the solution does not continuously depend on the data of the problem. Such ill-posed problems are not usually satisfactory for physical applications.&lt;br /&gt;
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对于任何非零的 {{mvar|y}}，如果 {{mvar|nx}} 不是模板 {{pi}} 的整数倍，这个解会接近于无穷大。拉普拉斯方程的柯西问题被称为不适定的（可以译为ill-posed或not well-posed），因为解不是连续地依赖于问题的数据。这种不适定问题通常不能满足物理应用。&lt;br /&gt;
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The [[Navier–Stokes existence and smoothness|existence of solutions for the Navier–Stokes equations]], a partial differential equation, is part of one of the [[Millennium Prize Problems]].&lt;br /&gt;
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The existence of solutions for the Navier–Stokes equations, a partial differential equation, is part of one of the Millennium Prize Problems.&lt;br /&gt;
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偏微分方程”纳维-斯托克斯方程“的解的存在性就是千禧年大奖难题之一的一部分。&lt;br /&gt;
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== Notation ==&lt;br /&gt;
符号&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
In PDEs, it is common to denote partial derivatives using subscripts. That is:&lt;br /&gt;
&lt;br /&gt;
In PDEs, it is common to denote partial derivatives using subscripts. That is:&lt;br /&gt;
&lt;br /&gt;
在偏微分方程中，通常用下标表示偏导数。例如:&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt;u_x = \frac{\partial u}{\partial x}&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;u_x = \frac{\partial u}{\partial x}&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt;u_{xx} = \frac{\partial^2 u}{\partial x^2} &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;u_{xx} = \frac{\partial^2 u}{\partial x^2} &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt;u_{xy} = \frac{\partial^2 u}{\partial y\, \partial x} = \frac{\partial}{\partial y } \left(\frac{\partial u}{\partial x}\right). &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;u_{xy} = \frac{\partial^2 u}{\partial y\, \partial x} = \frac{\partial}{\partial y } \left(\frac{\partial u}{\partial x}\right). &amp;lt;/math&amp;gt;&lt;br /&gt;
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Especially in physics, [[del]] or nabla ({{math|∇}}) is often used to denote spatial derivatives, and {{math|''&amp;amp;#x307;u'', ''ü''}} for time derivatives. For example, the [[wave equation]] (mentioned below) can be written as&lt;br /&gt;
&lt;br /&gt;
Especially in physics, del or nabla () is often used to denote spatial derivatives, and  for time derivatives. For example, the wave equation (mentioned below) can be written as&lt;br /&gt;
&lt;br /&gt;
特别是在物理学中，[[del]] 或 nabla ({{math|∇}}) 经常用来表示空间导数和时间导数。例如，波动方程(在下文中提到)可以写成：&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
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:&amp;lt;math&amp;gt;\ddot u=c^2\nabla^2u&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt;\ddot u=c^2\nabla^2u&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
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or&lt;br /&gt;
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or&lt;br /&gt;
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或&lt;br /&gt;
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:&amp;lt;math&amp;gt;\ddot u=c^2\Delta u&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt;\ddot u=c^2\Delta u&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
where {{math|Δ}} is the [[Laplace operator]].&lt;br /&gt;
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where  is the Laplace operator.&lt;br /&gt;
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其中，{{math|Δ}} 代表拉普拉斯算子。&lt;br /&gt;
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== Classification ==&lt;br /&gt;
分类&lt;br /&gt;
&lt;br /&gt;
Some linear, second-order partial differential equations can be classified as [[parabolic partial differential equation|parabolic]], [[hyperbolic partial differential equation|hyperbolic]] and [[elliptic partial differential equation|elliptic]]. Others, such as the [[Euler–Tricomi equation]], have different types in different regions. The classification provides a guide to appropriate initial and boundary conditions and to the smoothness of the solutions.&lt;br /&gt;
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Some linear, second-order partial differential equations can be classified as parabolic, hyperbolic and elliptic. Others, such as the Euler–Tricomi equation, have different types in different regions. The classification provides a guide to appropriate initial and boundary conditions and to the smoothness of the solutions.&lt;br /&gt;
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一些线性二阶偏微分方程可分为抛物型方程、双曲型方程和椭圆型方程。其他的方程，如欧拉-特里科米方程，在不同的领域有不同的类型。这种分类有助于选择适当的初始和边界条件以及提高解的平滑性。&lt;br /&gt;
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=== Equations of first order ===&lt;br /&gt;
一阶方程&lt;br /&gt;
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{{main|First-order partial differential equation}}&lt;br /&gt;
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=== Linear equations of second order ===&lt;br /&gt;
二阶线性方程&lt;br /&gt;
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&lt;br /&gt;
Assuming {{math|''u&amp;lt;sub&amp;gt;xy&amp;lt;/sub&amp;gt;'' {{=}} ''u&amp;lt;sub&amp;gt;yx&amp;lt;/sub&amp;gt;''}}, the general linear second-order PDE in two independent variables has the form&lt;br /&gt;
&lt;br /&gt;
Assuming  u&amp;lt;sub&amp;gt;yx&amp;lt;/sub&amp;gt;}}, the general linear second-order PDE in two independent variables has the form&lt;br /&gt;
&lt;br /&gt;
假设 {{math|''u&amp;lt;sub&amp;gt;xy&amp;lt;/sub&amp;gt;'' {{=}} ''u&amp;lt;sub&amp;gt;yx&amp;lt;/sub&amp;gt;''}}，含有两个独立变量的一般线性二阶偏微分方程具有如下形式：&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt;Au_{xx} + 2Bu_{xy} + Cu_{yy} + \cdots \mbox{(lower order terms)} = 0,&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;Au_{xx} + 2Bu_{xy} + Cu_{yy} + \cdots \mbox{(lower order terms)} = 0,&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
where the coefficients {{mvar|A}}, {{mvar|B}}, {{mvar|C}}... may depend upon {{mvar|x}} and {{mvar|y}}. If {{math|''A''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; + ''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; + ''C''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; &amp;gt; 0}} over a region of the {{mvar|xy}}-plane, the PDE is second-order in that region. This form is analogous to the equation for a conic section:&lt;br /&gt;
&lt;br /&gt;
where the coefficients , , ... may depend upon  and . If  over a region of the -plane, the PDE is second-order in that region. This form is analogous to the equation for a conic section:&lt;br /&gt;
&lt;br /&gt;
其中的系数 {{mvar|A}}, {{mvar|B}}, {{mvar|C}}... 一般取决于 {{mvar|x}} 和 {{mvar|y}} 。如果在 {{mvar|xy}}-平面的一个区域上 {{math|''A''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; + ''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; + ''C''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; &amp;gt; 0}}，偏微分方程是二阶的，这种形式类似于圆锥截面的方程:&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
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: &amp;lt;math&amp;gt;Ax^2 + 2Bxy + Cy^2 + \cdots = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;Ax^2 + 2Bxy + Cy^2 + \cdots = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
More precisely, replacing {{math|∂&amp;lt;sub&amp;gt;''x''&amp;lt;/sub&amp;gt;}} by {{mvar|X}}, and likewise for other variables (formally this is done by a [[Fourier transform]]), converts a constant-coefficient PDE into a polynomial of the same degree, with the terms of the highest degree (a [[homogeneous polynomial]], here a [[quadratic form]]) being most significant for the classification.&lt;br /&gt;
&lt;br /&gt;
More precisely, replacing  by , and likewise for other variables (formally this is done by a Fourier transform), converts a constant-coefficient PDE into a polynomial of the same degree, with the terms of the highest degree (a homogeneous polynomial, here a quadratic form) being most significant for the classification.&lt;br /&gt;
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更准确地说，用 {{mvar|X}} 替换 {{math|∂&amp;lt;sub&amp;gt;''x''&amp;lt;/sub&amp;gt;}}，并同样替换其它变量(通常由傅里叶变换完成)，将一个常系数偏微分方程转换成一个相同次数的多项式，最高次数的项(齐次多项式，这里是一个二次形式)对于偏微分方程的分类最为重要。&lt;br /&gt;
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Just as one classifies [[conic section]]s and quadratic forms into parabolic, hyperbolic, and elliptic based on the [[discriminant]] {{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − 4''AC''}}, the same can be done for a second-order PDE at a given point.  However, the [[discriminant]] in a PDE is given by {{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC''}} due to the convention of the {{mvar|xy}} term being {{math|2''B''}} rather than {{mvar|B}}; formally, the discriminant (of the associated quadratic form) is {{math|(2''B'')&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − 4''AC'' {{=}} 4(''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC'')}}, with the factor of 4 dropped for simplicity.&lt;br /&gt;
&lt;br /&gt;
Just as one classifies conic sections and quadratic forms into parabolic, hyperbolic, and elliptic based on the discriminant , the same can be done for a second-order PDE at a given point.  However, the discriminant in a PDE is given by  due to the convention of the  term being  rather than ; formally, the discriminant (of the associated quadratic form) is  4(B&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − AC)}}, with the factor of 4 dropped for simplicity.&lt;br /&gt;
&lt;br /&gt;
正如人们可以根据判别式 {{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − 4''AC''}} 将圆锥截面和二次型分为抛物型、双曲型和椭圆型一样，对于给定点的二阶偏微分方程也可以这样做。然而，偏微分方程中的判别式 {{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − 4''AC''}} 是根据交叉项的系数{{math|2''B''}} 而不是 {{mvar|B}} 给出的，形式上，判别式(关联二次型)是 {{math|(2''B'')&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − 4''AC'' {{=}} 4(''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC'')}}，为简单起见，去掉了因子4。&lt;br /&gt;
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# {{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC'' &amp;lt; 0}} (''[[elliptic partial differential equation]]''): Solutions of [[elliptic partial differential equation|elliptic PDEs]] are as smooth as the coefficients allow, within the interior of the region where the equation and solutions are defined. For example, solutions of [[Laplace's equation]] are analytic within the domain where they are defined, but solutions may assume boundary values that are not smooth. The motion of a fluid at subsonic speeds can be approximated with elliptic PDEs, and the Euler–Tricomi equation is elliptic where {{math|''x'' &amp;lt; 0}}.&lt;br /&gt;
&lt;br /&gt;
  (elliptic partial differential equation): Solutions of elliptic PDEs are as smooth as the coefficients allow, within the interior of the region where the equation and solutions are defined. For example, solutions of Laplace's equation are analytic within the domain where they are defined, but solutions may assume boundary values that are not smooth. The motion of a fluid at subsonic speeds can be approximated with elliptic PDEs, and the Euler–Tricomi equation is elliptic where .&lt;br /&gt;
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{{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC'' &amp;lt; 0}} (椭圆型微分方程)：在定义方程和解的区域内部，椭圆型偏微分方程的解在系数允许的程度内光滑。例如，拉普拉斯方程的解在它们被定义的区域内是解析的，但可能假设边界值是不光滑的。亚音速流体的运动可以用椭圆型偏微分方程近似，欧拉-特里科米方程在 {{math|''x'' &amp;lt; 0}} 时是椭圆型偏微分方程。&lt;br /&gt;
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# {{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC'' {{=}} 0}} (''[[parabolic partial differential equation]]''): Equations that are [[parabolic partial differential equation|parabolic]] at every point can be transformed into a form analogous to the [[heat equation]] by a change of independent variables. Solutions smooth out as the transformed time variable increases. The Euler–Tricomi equation has parabolic type on the line where {{math|''x'' {{=}} 0}}.&lt;br /&gt;
&lt;br /&gt;
  0}} (parabolic partial differential equation): Equations that are parabolic at every point can be transformed into a form analogous to the heat equation by a change of independent variables. Solutions smooth out as the transformed time variable increases. The Euler–Tricomi equation has parabolic type on the line where  0}}.&lt;br /&gt;
&lt;br /&gt;
{{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC'' {{=}} 0}}（抛物型偏微分方程）：在每一点上都是抛物线型的方程可以通过改变自变量从而转化成类似于热方程的形式。随着转换后的时间变量的增加，方程的解变得平滑。欧拉-特里科米方程在特征线 {{math|''x'' {{=}} 0}} 上是抛物线型的。&lt;br /&gt;
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# {{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC'' &amp;gt; 0}} (''[[hyperbolic partial differential equation]]''): [[hyperbolic partial differential equation|hyperbolic]] equations retain any discontinuities of functions or derivatives in the initial data. An example is the [[wave equation]]. The motion of a fluid at supersonic speeds can be approximated with hyperbolic PDEs, and the Euler–Tricomi equation is hyperbolic where {{math|''x'' &amp;gt; 0}}.&lt;br /&gt;
&lt;br /&gt;
  (hyperbolic partial differential equation): hyperbolic equations retain any discontinuities of functions or derivatives in the initial data. An example is the wave equation. The motion of a fluid at supersonic speeds can be approximated with hyperbolic PDEs, and the Euler–Tricomi equation is hyperbolic where .&lt;br /&gt;
&lt;br /&gt;
{{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC'' &amp;gt; 0}} (双曲型偏微分方程)：双曲型方程在初始数据中保留了函数或导数的任何不连续性。波动方程就是其中的一个例子。超音速流体的运动可以用双曲型偏微分方程近似，欧拉-特里科米方程在 {{math|''x'' &amp;gt; 0}} 时是双曲型的。&lt;br /&gt;
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If there are {{mvar|n}} independent variables {{math|''x''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;, ''x''&amp;lt;sub&amp;gt;2 &amp;lt;/sub&amp;gt;,… ''x''&amp;lt;sub&amp;gt;''n''&amp;lt;/sub&amp;gt;}}, a general linear partial differential equation of second order has the form&lt;br /&gt;
&lt;br /&gt;
If there are  independent variables , a general linear partial differential equation of second order has the form&lt;br /&gt;
&lt;br /&gt;
如果存在 {{mvar|n}} 个自变量 {{math|''x''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;, ''x''&amp;lt;sub&amp;gt;2 &amp;lt;/sub&amp;gt;,… ''x''&amp;lt;sub&amp;gt;''n''&amp;lt;/sub&amp;gt;}}，一般二阶线性偏微分方程的形式是：&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt;L u =\sum_{i=1}^n\sum_{j=1}^n a_{i,j} \frac{\partial^2 u}{\partial x_i \partial x_j} \quad \text{ plus lower-order terms} =0.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;L u =\sum_{i=1}^n\sum_{j=1}^n a_{i,j} \frac{\partial^2 u}{\partial x_i \partial x_j} \quad \text{ plus lower-order terms} =0.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
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The classification depends upon the signature of the eigenvalues of the coefficient matrix {{math|''a''&amp;lt;sub&amp;gt;''i'',''j''&amp;lt;/sub&amp;gt;}}.&lt;br /&gt;
&lt;br /&gt;
The classification depends upon the signature of the eigenvalues of the coefficient matrix .&lt;br /&gt;
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这种分类取决于系数矩阵特征值的符号（正负性）。&lt;br /&gt;
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# Elliptic: the eigenvalues are all positive or all negative.&lt;br /&gt;
&lt;br /&gt;
 Elliptic: the eigenvalues are all positive or all negative.&lt;br /&gt;
&lt;br /&gt;
椭圆形方程: 特征值全部为正或全部为负。&lt;br /&gt;
&lt;br /&gt;
# Parabolic: the eigenvalues are all positive or all negative, save one that is zero.&lt;br /&gt;
&lt;br /&gt;
 Parabolic: the eigenvalues are all positive or all negative, save one that is zero.&lt;br /&gt;
&lt;br /&gt;
抛物线形方程:除了一个为零值，特征值全部为正或全部为负。&lt;br /&gt;
&lt;br /&gt;
# Hyperbolic: there is only one negative eigenvalue and all the rest are positive, or there is only one positive eigenvalue and all the rest are negative.&lt;br /&gt;
&lt;br /&gt;
 Hyperbolic: there is only one negative eigenvalue and all the rest are positive, or there is only one positive eigenvalue and all the rest are negative.&lt;br /&gt;
&lt;br /&gt;
双曲形方程: 只有一个负特征值，其余的都是正特征值，或者只有一个正特征值，其余的都是负特征值。&lt;br /&gt;
&lt;br /&gt;
# Ultrahyperbolic: there is more than one positive eigenvalue and more than one negative eigenvalue, and there are no zero eigenvalues. There is only a limited theory for ultrahyperbolic equations (Courant and Hilbert, 1962).&lt;br /&gt;
&lt;br /&gt;
 Ultrahyperbolic: there is more than one positive eigenvalue and more than one negative eigenvalue, and there are no zero eigenvalues. There is only a limited theory for ultrahyperbolic equations (Courant and Hilbert, 1962).&lt;br /&gt;
&lt;br /&gt;
超双形方程: 存在多于一个正特征值和多于一个的负特征值，且不存在零特征值。对于超双曲方程，只存在有限的理论(Courant 和 Hilbert，1962)。&lt;br /&gt;
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=== Systems of first-order equations and characteristic surfaces ===&lt;br /&gt;
一阶方程组和特征曲面&lt;br /&gt;
&lt;br /&gt;
The classification of partial differential equations can be extended to systems of first-order equations, where the unknown {{mvar|u}} is now a [[Euclidean vector|vector]] with {{mvar|m}} components, and the coefficient matrices {{mvar|A&amp;lt;sub&amp;gt;ν&amp;lt;/sub&amp;gt;}} are {{mvar|m}} by {{mvar|m}} matrices for {{math|''ν'' {{=}} 1, 2,… ''n''}}. The partial differential equation takes the form&lt;br /&gt;
&lt;br /&gt;
The classification of partial differential equations can be extended to systems of first-order equations, where the unknown  is now a vector with  components, and the coefficient matrices  are  by  matrices for  1, 2,… n}}. The partial differential equation takes the form&lt;br /&gt;
&lt;br /&gt;
偏微分方程的分类可以推广到一阶方程组，其中未知量 {{mvar|u}} 是有 {{mvar|m}} 个分量的向量。对于 {{math|''ν'' {{=}} 1, 2,… ''n''}}，系数矩阵 {{mvar|A&amp;lt;sub&amp;gt;ν&amp;lt;/sub&amp;gt;}} 是 {{mvar|m}} × {{mvar|m}} 的矩阵。偏微分方程形式如下：&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt;Lu = \sum_{\nu=1}^{n} A_\nu \frac{\partial u}{\partial x_\nu} + B=0,&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;Lu = \sum_{\nu=1}^{n} A_\nu \frac{\partial u}{\partial x_\nu} + B=0,&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
where the coefficient matrices {{mvar|A&amp;lt;sub&amp;gt;ν&amp;lt;/sub&amp;gt;}} and the vector {{mvar|B}} may depend upon {{mvar|x}} and {{mvar|u}}. If a [[hypersurface]] {{mvar|S}} is given in the implicit form&lt;br /&gt;
&lt;br /&gt;
where the coefficient matrices  and the vector  may depend upon  and . If a hypersurface  is given in the implicit form&lt;br /&gt;
&lt;br /&gt;
其中，系数矩阵 {{mvar|A&amp;lt;sub&amp;gt;ν&amp;lt;/sub&amp;gt;}} 和向量 {{mvar|B}} 可能依赖于 {{mvar|x}} 和 {{mvar|u}}。如果超曲面是以以下隐式形式给出的，&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt;\varphi(x_1, x_2, \ldots x_n)=0,&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;\varphi(x_1, x_2, \ldots x_n)=0,&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
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where {{mvar|φ}} has a non-zero gradient, then {{mvar|S}} is a '''characteristic surface''' for the operator {{mvar|L}} at a given point if the characteristic form vanishes:&lt;br /&gt;
&lt;br /&gt;
where  has a non-zero gradient, then  is a characteristic surface for the operator  at a given point if the characteristic form vanishes:&lt;br /&gt;
&lt;br /&gt;
其中，存在一个非零的梯度 {{mvar|φ}}，对于在给定点上特征形式消失的算子，特征曲面 {{mvar|S}} 形式如下:&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
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: &amp;lt;math&amp;gt;Q\left(\frac{\partial\varphi}{\partial x_1}, \ldots\frac{\partial\varphi}{\partial x_n}\right) =\det\left[\sum_{\nu=1}^nA_\nu \frac{\partial \varphi}{\partial x_\nu}\right]=0.\,&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;Q\left(\frac{\partial\varphi}{\partial x_1}, \ldots\frac{\partial\varphi}{\partial x_n}\right) =\det\left[\sum_{\nu=1}^nA_\nu \frac{\partial \varphi}{\partial x_\nu}\right]=0.\,&amp;lt;/math&amp;gt;&lt;br /&gt;
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The geometric interpretation of this condition is as follows: if data for {{mvar|u}} are prescribed on the surface {{mvar|S}}, then it may be possible to determine the normal derivative of {{mvar|u}} on {{mvar|S}} from the differential equation. If the data on {{mvar|S}} and the differential equation determine the normal derivative of {{mvar|u}} on {{mvar|S}}, then {{mvar|S}} is non-characteristic. If the data on {{mvar|S}} and the differential equation ''do not'' determine the normal derivative of {{mvar|u}} on {{mvar|S}}, then the surface is '''characteristic''', and the differential equation restricts the data on {{mvar|S}}: the differential equation is ''internal'' to {{mvar|S}}.&lt;br /&gt;
&lt;br /&gt;
The geometric interpretation of this condition is as follows: if data for  are prescribed on the surface , then it may be possible to determine the normal derivative of  on  from the differential equation. If the data on  and the differential equation determine the normal derivative of  on , then  is non-characteristic. If the data on  and the differential equation do not determine the normal derivative of  on , then the surface is characteristic, and the differential equation restricts the data on : the differential equation is internal to .&lt;br /&gt;
&lt;br /&gt;
这个条件的几何解释如下: 如果关于 {{mvar|u}} 的数据是在曲面 {{mvar|S}} 上规定的，那么就有可能依据微分方程确定曲面 {{mvar|S}} 上 {{mvar|u}} 的法向导数。如果曲面 {{mvar|S}} 上的数据和上面的微分方程能确定曲面 {{mvar|S}} 上 {{mvar|u}} 的法向导数，那么它就是非特征的。如果曲面 {{mvar|S}} 上的数据和上面的微分方程不能确定曲面 {{mvar|S}} 上 {{mvar|u}} 的法向导数，那么曲面是特征的，并且微分方程将数据限制在曲面 {{mvar|S}} 上：微分方程是在曲面 {{mvar|S}} 内部。&lt;br /&gt;
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# A first-order system {{math|''Lu'' {{=}} 0}} is ''elliptic'' if no surface is characteristic for {{mvar|L}}: the values of {{mvar|u}} on {{mvar|S}} and the differential equation always determine the normal derivative of {{mvar|u}} on {{mvar|S}}.&lt;br /&gt;
&lt;br /&gt;
 A first-order system  0}} is elliptic if no surface is characteristic for : the values of  on  and the differential equation always determine the normal derivative of  on .&lt;br /&gt;
&lt;br /&gt;
如果对于 {{mvar|L}} 没有曲面是特征的，则一阶系统 {{math|''Lu'' {{=}} 0}} 是椭圆形的：{{mvar|u}}在 {{mvar|S}} 的值和微分方程总能够决定 {{mvar|S}} 上 {{mvar|u}} 的法向导数。&lt;br /&gt;
&lt;br /&gt;
# A first-order system is ''hyperbolic'' at a point if there is a '''spacelike''' surface {{mvar|S}} with normal {{mvar|ξ}} at that point. This means that, given any non-trivial vector {{mvar|η}} orthogonal to {{mvar|ξ}}, and a scalar multiplier {{mvar|λ}}, the equation {{math|''Q''(''λξ'' + ''η'') {{=}} 0}} has {{mvar|m}} real roots {{math|''λ''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;, ''λ''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;,… ''λ''&amp;lt;sub&amp;gt;''m''&amp;lt;/sub&amp;gt;}}. The system is '''strictly hyperbolic''' if these roots are always distinct. The geometrical interpretation of this condition is as follows: the characteristic form {{math|''Q''(''ζ'') {{=}} 0}} defines a cone (the normal cone) with homogeneous coordinates ζ. In the hyperbolic case, this cone has {{mvar|m}} sheets, and the axis {{math|''ζ'' {{=}} ''λξ''}} runs inside these sheets: it does not intersect any of them. But when displaced from the origin by η, this axis intersects every sheet. In the elliptic case, the normal cone has no real sheets.&lt;br /&gt;
&lt;br /&gt;
 A first-order system is hyperbolic at a point if there is a spacelike surface  with normal  at that point. This means that, given any non-trivial vector  orthogonal to , and a scalar multiplier , the equation  0}} has  real roots . The system is strictly hyperbolic if these roots are always distinct. The geometrical interpretation of this condition is as follows: the characteristic form  0}} defines a cone (the normal cone) with homogeneous coordinates ζ. In the hyperbolic case, this cone has  sheets, and the axis  λξ}} runs inside these sheets: it does not intersect any of them. But when displaced from the origin by η, this axis intersects every sheet. In the elliptic case, the normal cone has no real sheets.&lt;br /&gt;
&lt;br /&gt;
如果在该点存在一个法向量为 {{mvar|ξ}}的 '''&amp;lt;font color=&amp;quot;#ff8000&amp;quot;&amp;gt;类空曲面 Spacclike Surface&amp;lt;/font&amp;gt; {{mvar|S}} ，则一阶系统在那一点是双曲的。这意味着，给定任意正交于 {{mvar|ξ}} 的非平凡向量 {{mvar|η}} 和一个标量乘子 {{mvar|λ}}，方程 {{math|''Q''(''λξ'' + ''η'') {{=}} 0}} 有 {{mvar|m}} 个实根 {{math|''λ''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;, ''λ''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;,… ''λ''&amp;lt;sub&amp;gt;''m''&amp;lt;/sub&amp;gt;}}。如果这些根始终不同，则该系统是严格双曲形的。这个条件的几何解释如下: 特征形式 {{math|''Q''(''ζ'') {{=}} 0}} 定义了一个具有齐次坐标 ζ的圆锥(法线圆锥)。在双曲形的情况下，这个圆锥体有 {{mvar|m}} 层，并且轴 {{math|''ζ'' {{=}} ''λξ''}} 在这些层中运动: 它不与任何一层相交。但是当从原点偏离η时，这条轴线与每一层都相交。在椭圆形的情况下，法向圆锥没有实层。&lt;br /&gt;
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==[[用户:Yuling|Yuling]]（[[用户讨论:Yuling|讨论]]） sheet 这个单词也不很理解，我直译为了“层”&lt;br /&gt;
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=== Equations of mixed type ===&lt;br /&gt;
混合型方程&lt;br /&gt;
&lt;br /&gt;
If a PDE has coefficients that are not constant, it is possible that it will not belong to any of these categories but rather be of '''mixed type'''. A simple but important example is the [[Euler–Tricomi equation]]&lt;br /&gt;
&lt;br /&gt;
If a PDE has coefficients that are not constant, it is possible that it will not belong to any of these categories but rather be of mixed type. A simple but important example is the Euler–Tricomi equation&lt;br /&gt;
&lt;br /&gt;
如果偏微分方程的系数不是常数，那么它可能不属于这些类别中的任何一个，而是属于混合类型。一个简单但重要的例子是欧拉-特里科米方程&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
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: &amp;lt;math&amp;gt;u_{xx} = xu_{yy},&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;u_{xx} = xu_{yy},&amp;lt;/math&amp;gt;&lt;br /&gt;
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&lt;br /&gt;
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which is called '''elliptic-hyperbolic''' because it is elliptic in the region {{math|''x'' &amp;lt; 0}}, hyperbolic in the region {{math|''x'' &amp;gt; 0}}, and degenerate parabolic on the line {{math|''x'' {{=}} 0}}.&lt;br /&gt;
&lt;br /&gt;
which is called elliptic-hyperbolic because it is elliptic in the region , hyperbolic in the region , and degenerate parabolic on the line  0}}.&lt;br /&gt;
&lt;br /&gt;
它在 {{math|''x'' &amp;lt; 0}} 的区域上是椭圆形，在 {{math|''x'' &amp;gt; 0}} 区域上是双曲形，在 {{math|''x'' {{=}} 0}}这条线上是退化为抛物线形，因此称之为椭圆-双曲型。&lt;br /&gt;
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&amp;lt;!--&lt;br /&gt;
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&amp;lt;!--&lt;br /&gt;
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&amp;lt;!--&lt;br /&gt;
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''fill in: Dirichlet and Neumann boundaries, hyperbolic/parabolic/elliptic separation of variables, [[Fourier analysis]], [[Green's function]]s ...--&amp;gt;&lt;br /&gt;
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fill in: Dirichlet and Neumann boundaries, hyperbolic/parabolic/elliptic separation of variables, Fourier analysis, Green's functions ...--&amp;gt;&lt;br /&gt;
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填写: Dirichlet 和 Neumann 边界，双曲 / 抛物线 / 椭圆分离变量法，傅立叶分析，Green 函数... --&lt;br /&gt;
&lt;br /&gt;
=== Infinite-order PDEs in quantum mechanics ===&lt;br /&gt;
量子力学中的无限阶偏微分方程&lt;br /&gt;
&lt;br /&gt;
In the [[phase space formulation]] of quantum mechanics,  one may consider the [[Method of quantum characteristics|quantum Hamilton's equations]] for trajectories of quantum particles. These equations are infinite-order PDEs. However, in the semiclassical expansion, one has a finite system of ODEs at any fixed order of [[Dirac constant|{{mvar|ħ}}]].  The evolution equation of the [[Wigner quasi-probability distribution|c]] is also an infinite-order PDE. The quantum trajectories are [[Method of quantum characteristics|quantum characteristics]], with the use of which one could calculate the evolution of the Wigner function.&lt;br /&gt;
&lt;br /&gt;
In the phase space formulation of quantum mechanics,  one may consider the quantum Hamilton's equations for trajectories of quantum particles. These equations are infinite-order PDEs. However, in the semiclassical expansion, one has a finite system of ODEs at any fixed order of Dirac constant|.  The evolution equation of the Wigner function is also an infinite-order PDE. The quantum trajectories are quantum characteristics, with the use of which one could calculate the evolution of the Wigner function.&lt;br /&gt;
&lt;br /&gt;
在量子力学中的相空间表述中，我们可以考虑用于求解量子粒子的轨迹的量子哈密顿的方程。这些方程是无限阶偏微分方程。然而，在半经典展开中，我们在给定[[Dirac constant|{{mvar|ħ}}]]阶数下有一个有限的的常微分方程组。'''&amp;lt;font color=&amp;quot;#ff8000&amp;quot;&amp;gt;维格纳函数  Wigner Function&amp;lt;/font&amp;gt;的演化方程也是一个无限阶偏微分方程。由于量子轨道的量子特性，所以它通常可以用来计算维格纳函数的演化。&lt;br /&gt;
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== Analytical solutions ==&lt;br /&gt;
解析解&lt;br /&gt;
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===Separation of variables===&lt;br /&gt;
分离变量法&lt;br /&gt;
&lt;br /&gt;
{{main|Separable partial differential equation}}&lt;br /&gt;
&lt;br /&gt;
Linear PDEs can be reduced to systems of ordinary differential equations by the important technique of separation of variables. This technique rests on a characteristic of solutions to differential equations: if one can find any solution that solves the equation and satisfies the boundary conditions, then it is ''the'' solution (this also applies to ODEs). We assume as an [[ansatz]] that the dependence of a solution on the parameters space and time can be written as a product of terms that each depend on a single parameter, and then see if this can be made to solve the problem.&amp;lt;ref&amp;gt;{{cite book|last1=Gershenfeld|first1=Neil|title=The nature of mathematical modeling|date=2000|publisher=Cambridge Univ. Press|location=Cambridge|isbn=0521570956|page=27|edition=Reprinted (with corr.)}}&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
Linear PDEs can be reduced to systems of ordinary differential equations by the important technique of separation of variables. This technique rests on a characteristic of solutions to differential equations: if one can find any solution that solves the equation and satisfies the boundary conditions, then it is the solution (this also applies to ODEs). We assume as an ansatz that the dependence of a solution on the parameters space and time can be written as a product of terms that each depend on a single parameter, and then see if this can be made to solve the problem.&lt;br /&gt;
&lt;br /&gt;
线性偏微分方程组可以通过分离变量法这一重要方法来简化为常微分方程组。这种方法依赖于微分方程解的一个特征: 如果能找到任何一个满足方程和边界条件的解，那么这个解就是方程的解(这也适用于常微分方程)。我们假设解对参数空间和时间的依赖可以写成对它们每一项的依赖以及一个参数的乘积，然后再看看这是否可以用来解决这个问题。&lt;br /&gt;
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In the method of separation of variables, one reduces a PDE to a PDE in fewer variables, which is an ordinary differential equation if in one variable – these are in turn easier to solve.&lt;br /&gt;
&lt;br /&gt;
In the method of separation of variables, one reduces a PDE to a PDE in fewer variables, which is an ordinary differential equation if in one variable – these are in turn easier to solve.&lt;br /&gt;
&lt;br /&gt;
在分离变量法方法中，可以将偏微分方程简化为含有更少变量的偏微分方程，如果只有一个变量，那么就变成了一个'''&amp;lt;font color = &amp;quot;#ff8000&amp;quot;&amp;gt;常微分方程 Ordinary Differential Equation&amp;lt;/font&amp;gt;'''-- 反过来，这些方程也更容易求解。&lt;br /&gt;
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This is possible for simple PDEs, which are called [[separable partial differential equation]]s, and the domain is generally a rectangle (a product of intervals). Separable PDEs correspond to [[diagonal matrices]] – thinking of &amp;quot;the value for fixed {{mvar|x}}&amp;quot; as a coordinate, each coordinate can be understood separately.&lt;br /&gt;
&lt;br /&gt;
This is possible for simple PDEs, which are called separable partial differential equations, and the domain is generally a rectangle (a product of intervals). Separable PDEs correspond to diagonal matrices – thinking of &amp;quot;the value for fixed &amp;quot; as a coordinate, each coordinate can be understood separately.&lt;br /&gt;
&lt;br /&gt;
对于简单的偏微分方程(称为可分离偏微分方程)来说，这是可能的，而且方程通常定义在一个矩形区域(区间的乘积)上。可分离偏微分方程对应于对角线矩阵——以“固定值”为坐标，每个坐标可分开理解。&lt;br /&gt;
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This generalizes to the [[method of characteristics]], and is also used in [[integral transform]]s.&lt;br /&gt;
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This generalizes to the method of characteristics, and is also used in integral transforms.&lt;br /&gt;
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这种方法可以推广到特征曲线法，也可以用于积分变换。&lt;br /&gt;
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===Method of characteristics===&lt;br /&gt;
特征曲线法&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{{main|Method of characteristics}}&lt;br /&gt;
&lt;br /&gt;
In special cases, one can find characteristic curves on which the equation reduces to an ODE – changing coordinates in the domain to straighten these curves allows separation of variables, and is called the [[method of characteristics]].&lt;br /&gt;
&lt;br /&gt;
In special cases, one can find characteristic curves on which the equation reduces to an ODE – changing coordinates in the domain to straighten these curves allows separation of variables, and is called the method of characteristics.&lt;br /&gt;
&lt;br /&gt;
在特殊情况下，可以找到一些特征曲线，在这些曲线上方程可以变成一个常微分方程——意味着改变坐标从而使这些曲线变直从而达到分离变量的目的，这就是所谓的特征曲线法。&lt;br /&gt;
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More generally, one may find characteristic surfaces.&lt;br /&gt;
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More generally, one may find characteristic surfaces.&lt;br /&gt;
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更一般地说，人们可能会找到特征表面。&lt;br /&gt;
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===Integral transform===&lt;br /&gt;
积分变换&lt;br /&gt;
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An [[integral transform]] may transform the PDE to a simpler one, in particular, a separable PDE. This corresponds to diagonalizing an operator.&lt;br /&gt;
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An integral transform may transform the PDE to a simpler one, in particular, a separable PDE. This corresponds to diagonalizing an operator.&lt;br /&gt;
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积分变换可以将偏微分方程转换为更简单的偏微分方程，特别是可分离的偏微分方程。这对应于对角化算符。&lt;br /&gt;
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An important example of this is [[Fourier analysis]], which diagonalizes the heat equation using the [[eigenbasis]] of sinusoidal waves.&lt;br /&gt;
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An important example of this is Fourier analysis, which diagonalizes the heat equation using the eigenbasis of sinusoidal waves.&lt;br /&gt;
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这方面的一个重要例子是'''&amp;lt;font color = &amp;quot;#ff8000&amp;quot;&amp;gt;傅里叶分析  Fourier Analysis&amp;lt;/font&amp;gt;'''，它使用正弦波的特征基来对角化热方程。&lt;br /&gt;
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If the domain is finite or periodic, an infinite sum of solutions such as a [[Fourier series]] is appropriate, but an integral of solutions such as a [[Fourier integral]] is generally required for infinite domains. The solution for a point source for the heat equation given above is an example of the use of a Fourier integral.&lt;br /&gt;
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If the domain is finite or periodic, an infinite sum of solutions such as a Fourier series is appropriate, but an integral of solutions such as a Fourier integral is generally required for infinite domains. The solution for a point source for the heat equation given above is an example of the use of a Fourier integral.&lt;br /&gt;
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如果区域是有限的或周期性的，那么解为无限和的形式是恰当的，例如傅里叶级数，但是一个解的积分，例如傅立叶积分，一般是在无限区域上的。上面给出的热传导方程的点源解法就是使用傅里叶积分的一个例子。&lt;br /&gt;
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===Change of variables===&lt;br /&gt;
变量代换&lt;br /&gt;
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Often a PDE can be reduced to a simpler form with a known solution by a suitable [[Change of variables (PDE)|change of variables]].  For example, the [[Black–Scholes equation#Derivation|Black–Scholes]] PDE&lt;br /&gt;
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Often a PDE can be reduced to a simpler form with a known solution by a suitable change of variables.  For example, the Black–Scholes PDE&lt;br /&gt;
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偏微分方程通常可以通过变量的适当变化，用已知的解简化为更简单的形式。例如，布莱克-舒尔斯偏微分方程&lt;br /&gt;
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:&amp;lt;math&amp;gt; \frac{\partial V}{\partial t} + \tfrac{1}{2}\sigma^2 S^2\frac{\partial^2 V}{\partial S^2} + rS\frac{\partial V}{\partial S} - rV = 0 &amp;lt;/math&amp;gt;&lt;br /&gt;
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&amp;lt;math&amp;gt; \frac{\partial V}{\partial t} + \tfrac{1}{2}\sigma^2 S^2\frac{\partial^2 V}{\partial S^2} + rS\frac{\partial V}{\partial S} - rV = 0 &amp;lt;/math&amp;gt;&lt;br /&gt;
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is reducible to the [[heat equation]]&lt;br /&gt;
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is reducible to the heat equation&lt;br /&gt;
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可以简化为热传导方程&lt;br /&gt;
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:&amp;lt;math&amp;gt; \frac{\partial u}{\partial \tau} = \frac{\partial^2 u}{\partial x^2}&amp;lt;/math&amp;gt;&lt;br /&gt;
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&amp;lt;math&amp;gt; \frac{\partial u}{\partial \tau} = \frac{\partial^2 u}{\partial x^2}&amp;lt;/math&amp;gt;&lt;br /&gt;
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by the change of variables (for complete details see {{webarchive |url=https://web.archive.org/web/20080411030405/http://www.math.unl.edu/~sdunbar1/Teaching/MathematicalFinance/Lessons/BlackScholes/Solution/solution.shtml |date=April 11, 2008 |title=Solution of the Black Scholes Equation }})&lt;br /&gt;
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by the change of variables (for complete details see )&lt;br /&gt;
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通过变量替换(完整的细节见)&lt;br /&gt;
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:&amp;lt;math&amp;gt;\begin{align}&lt;br /&gt;
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V(S,t) &amp;amp;= K v(x,\tau),\\[5px]&lt;br /&gt;
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x &amp;amp;= \ln\left(\tfrac{S}{K} \right),\\[5px]&lt;br /&gt;
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\tau &amp;amp;= \tfrac{1}{2} \sigma^2 (T - t),\\[5px]&lt;br /&gt;
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v(x,\tau)&amp;amp;=e^{-\alpha x-\beta\tau} u(x,\tau).&lt;br /&gt;
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\end{align}&amp;lt;/math&amp;gt;&lt;br /&gt;
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===Fundamental solution===&lt;br /&gt;
基本解&lt;br /&gt;
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{{main|Fundamental solution}}&lt;br /&gt;
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Inhomogeneous equations can often be solved (for constant coefficient PDEs, always be solved) by finding the [[fundamental solution]] (the solution for a point source), then taking the [[convolution]] with the boundary conditions to get the solution.&lt;br /&gt;
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Inhomogeneous equations can often be solved (for constant coefficient PDEs, always be solved) by finding the fundamental solution (the solution for a point source), then taking the convolution with the boundary conditions to get the solution.&lt;br /&gt;
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非齐次方程(常系数偏微分方程)一般是通过先求出基本解(点源的解) ，然后利用带边界条件的卷积来求解。&lt;br /&gt;
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This is analogous in [[signal processing]] to understanding a filter by its [[impulse response]].&lt;br /&gt;
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This is analogous in signal processing to understanding a filter by its impulse response.&lt;br /&gt;
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这类似于在信号处理中通过滤波器的脉冲响应来理解滤波器。&lt;br /&gt;
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===Superposition principle===&lt;br /&gt;
叠加原理&lt;br /&gt;
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{{further| Superposition principle }}&lt;br /&gt;
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The superposition principle applies to any linear system, including linear systems of PDEs. A common visualization of this concept is the interaction of two waves in phase being combined to result in a greater amplitude, for example {{math|sin ''x'' + sin ''x'' {{=}} 2 sin ''x''}}. The same principle can be observed in PDEs where the solutions may be real or complex and additive. [[Superposition principle|superposition]]&lt;br /&gt;
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The superposition principle applies to any linear system, including linear systems of PDEs. A common visualization of this concept is the interaction of two waves in phase being combined to result in a greater amplitude, for example  2 sin x}}. The same principle can be observed in PDEs where the solutions may be real or complex and additive. superposition&lt;br /&gt;
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'''&amp;lt;font color = &amp;quot;#ff8000&amp;quot;&amp;gt;叠加原理 Superposition Principle&amp;lt;/font&amp;gt;适用于任何线性系统，包括偏微分方程的线性系统。这个概念的一个常见的可视化是两个同相位的波相互作用结合在一起会产生更大的振幅，例如 {{math|sin ''x'' + sin ''x'' {{=}} 2 sin ''x''}}。在偏微分方程中也可以观察到同样的原理，其中的解可能是真实的或复杂的和可加的。叠加&lt;br /&gt;
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If {{math|''u''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;}} and {{math|''u''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;}} are solutions of linear PDE in some function space {{mvar|R}}, then {{math|''u'' {{=}} ''c''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;''u''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; + ''c''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;''u''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;}} with any constants {{math|''c''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;}} and {{math|''c''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;}} are also a solution of that PDE in the same function space.&lt;br /&gt;
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If  and  are solutions of linear PDE in some function space , then  c&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;u&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; + c&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;u&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;}} with any constants  and  are also a solution of that PDE in the same function space.&lt;br /&gt;
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若线性偏微分方程在某个函数空间{{mvar|R}}中有解{{math|''u''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;}} 和 {{math|''u''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;}}，则{{math|''u'' {{=}} ''c''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;''u''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; + ''c''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;''u''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;}}也是该偏微分方程在同一函数空间中的解，其中{{math|''c''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;}} 和 {{math|''c''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;}} 是任意常数。&lt;br /&gt;
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===Methods for non-linear equations===&lt;br /&gt;
非线性方程的求解方法&lt;br /&gt;
{{see also|nonlinear partial differential equation}}&lt;br /&gt;
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There are no generally applicable methods to solve nonlinear PDEs. Still, existence and uniqueness results (such as the [[Cauchy–Kowalevski theorem]]) are often possible, as are proofs of important qualitative and quantitative properties of solutions (getting these results is a major part of [[mathematical analysis|analysis]]). Computational solution to the nonlinear PDEs, the [[split-step method]], exist for specific equations like [[nonlinear Schrödinger equation]].&lt;br /&gt;
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There are no generally applicable methods to solve nonlinear PDEs. Still, existence and uniqueness results (such as the Cauchy–Kowalevski theorem) are often possible, as are proofs of important qualitative and quantitative properties of solutions (getting these results is a major part of analysis). Computational solution to the nonlinear PDEs, the split-step method, exist for specific equations like nonlinear Schrödinger equation.&lt;br /&gt;
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对于非线性偏微分方程，目前还没有普遍适用的求解方法。然而，通常是可能知道解的存在性和唯一性(如柯西-科瓦列夫斯基定理)，也是可能得到解的重要定性和定量性质的证明(得到这些结果是分析的主要部分)。非线性偏微分方程的计算解，即分步法，对一些特定的方程适用，比如非线性'''&amp;lt;font color=&amp;quot;#ff8000&amp;quot;&amp;gt;薛定谔方程 Schrödinger equation&amp;lt;/font&amp;gt;'''。&lt;br /&gt;
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Nevertheless, some techniques can be used for several types of equations. The [[h-principle|{{mvar|h}}-principle]] is the most powerful method to solve [[Underdetermined system|underdetermined]] equations. The [[Riquier–Janet theory]] is an effective method for obtaining information about many analytic [[Overdetermined system|overdetermined]] systems.&lt;br /&gt;
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Nevertheless, some techniques can be used for several types of equations. The -principle is the most powerful method to solve underdetermined equations. The Riquier–Janet theory is an effective method for obtaining information about many analytic overdetermined systems.&lt;br /&gt;
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然而，一些技巧可以用于几种类型的方程。h-原理是求解欠定方程最有效的方法。里基尔-珍妮特理论是一种可以获得许多解析超定系统信息的有效方法。&lt;br /&gt;
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The [[method of characteristics]] can be used in some very special cases to solve partial differential equations.&lt;br /&gt;
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The method of characteristics can be used in some very special cases to solve partial differential equations.&lt;br /&gt;
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特征线法可用于求解某些特殊情况下的偏微分方程。&lt;br /&gt;
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In some cases, a PDE can be solved via [[perturbation analysis]] in which the solution is considered to be a correction to an equation with a known solution. Alternatives are [[numerical analysis]] techniques from simple [[finite difference]] schemes to the more mature [[multigrid]] and [[finite element method]]s. Many interesting problems in science and engineering are solved in this way using [[computer]]s, sometimes high performance [[supercomputer]]s.&lt;br /&gt;
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In some cases, a PDE can be solved via perturbation analysis in which the solution is considered to be a correction to an equation with a known solution. Alternatives are numerical analysis techniques from simple finite difference schemes to the more mature multigrid and finite element methods. Many interesting problems in science and engineering are solved in this way using computers, sometimes high performance supercomputers.&lt;br /&gt;
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在某些情况下，偏微分方程可以通过扰动分析来求解。在扰动分析中，通常是求解将具有已知解的方程修正后的新得到方程。可供选择的数值分析技术从简单的差分格式到更成熟的多重网格和有限元方法。许多有趣的科学和工程问题都是在计算机上用这种方法解决的，有时是高性能超级计算机。&lt;br /&gt;
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===Lie group method===&lt;br /&gt;
李群方法&lt;br /&gt;
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From 1870 [[Sophus Lie]]'s work put the theory of differential equations on a more satisfactory foundation. He showed that the integration theories of the older mathematicians can, by the introduction of what are now called [[Lie group]]s, be referred, to a common source; and that ordinary differential equations which admit the same [[infinitesimal transformation]]s present comparable difficulties of integration. He also emphasized the subject of [[contact transformation|transformations of contact]].&lt;br /&gt;
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From 1870 Sophus Lie's work put the theory of differential equations on a more satisfactory foundation. He showed that the integration theories of the older mathematicians can, by the introduction of what are now called Lie groups, be referred, to a common source; and that ordinary differential equations which admit the same infinitesimal transformations present comparable difficulties of integration. He also emphasized the subject of transformations of contact.&lt;br /&gt;
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从1870年起，索弗斯·李的工作为微分方程理论奠定了一个较为令人满意的基础。他指出，通过引入现在所谓的李群，老一辈数学家的积分理论可以引用到一个共同的来源; 承认相同的无穷小变换的常微分方程在积分方面存在相当的困难。他还强调了接触的转变这一主题。&lt;br /&gt;
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==[[用户:Yuling|Yuling]]（[[用户讨论:Yuling|讨论]]）这句话“He also emphasized the subject of transformations of contact.”中的transformations of contact翻译的不太好。&lt;br /&gt;
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A general approach to solving PDEs uses the symmetry property of differential equations, the continuous [[infinitesimal transformation]]s of solutions to solutions ([[Lie theory]]). Continuous [[group theory]], [[Lie algebras]] and [[differential geometry]] are used to understand the structure of linear and nonlinear partial differential equations for generating integrable equations, to find its [[Lax pair]]s, recursion operators, [[Bäcklund transform]] and finally finding exact analytic solutions to the PDE.&lt;br /&gt;
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A general approach to solving PDEs uses the symmetry property of differential equations, the continuous infinitesimal transformations of solutions to solutions (Lie theory). Continuous group theory, Lie algebras and differential geometry are used to understand the structure of linear and nonlinear partial differential equations for generating integrable equations, to find its Lax pairs, recursion operators, Bäcklund transform and finally finding exact analytic solutions to the PDE.&lt;br /&gt;
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求解偏微分方程的一般方法是利用微分方程的对称性，即解到解的连续无穷小变换(李理论)。连续群论、李代数和微分几何理论被用来理解生成可积方程的线性和非线性偏微分方程的结构，找到它的Lax对、递归算子、 贝克伦德变换，最后找到偏微分方程的精确解析解。&lt;br /&gt;
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Symmetry methods have been recognized to study differential equations arising in mathematics, physics, engineering, and many other disciplines.&lt;br /&gt;
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Symmetry methods have been recognized to study differential equations arising in mathematics, physics, engineering, and many other disciplines.&lt;br /&gt;
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对称方法已被公认可以用于研究出现在数学，物理，工程和许多其他学科的微分方程。&lt;br /&gt;
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===Semianalytical methods===&lt;br /&gt;
半解析方法&lt;br /&gt;
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The [[Adomian decomposition method]], the [[Aleksandr Lyapunov|Lyapunov]] artificial small parameter method, and He's [[homotopy perturbation method]] are all special cases of the more general [[homotopy analysis method]]. These are series expansion methods, and except for the Lyapunov method, are independent of small physical parameters as compared to the well known [[perturbation theory]], thus giving these methods greater flexibility and solution generality.&lt;br /&gt;
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The Adomian decomposition method, the Lyapunov artificial small parameter method, and He's homotopy perturbation method are all special cases of the more general homotopy analysis method. These are series expansion methods, and except for the Lyapunov method, are independent of small physical parameters as compared to the well known perturbation theory, thus giving these methods greater flexibility and solution generality.&lt;br /&gt;
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阿多米安分解法、李雅普诺夫人工小参数方法和何同伦摄动方法都是更一般的同伦分析方法的特殊情况。除了李雅普诺夫方法之外，这些都是级数展开方法，与为人熟知的摄动理论方法相比，它们与小的物理参数无关，因此这些方法具有更大的灵活性和解的通用性。&lt;br /&gt;
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== Numerical solutions ==&lt;br /&gt;
数值解&lt;br /&gt;
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The three most widely used [[Numerical partial differential equations|numerical methods to solve PDEs]] are the [[finite element analysis|finite element method]] (FEM), [[finite volume method]]s (FVM) and [[finite difference method]]s (FDM), as well other kind of methods called [[Meshfree methods]], which were made to solve problems where the before mentioned methods are limited. The FEM has a prominent position among these methods and especially its exceptionally efficient higher-order version [[hp-FEM]]. Other hybrid versions of FEM and Meshfree methods include the generalized finite element method (GFEM), [[extended finite element method]] (XFEM), [[Spectral element method|spectral finite element method]] (SFEM), [[Meshfree methods|meshfree finite element method]], [[Discontinuous Galerkin Method|discontinuous Galerkin finite element method]] (DGFEM), [[Element-Free Galerkin Method]] (EFGM), [[Interpolating Element-Free Galerkin Method]] (IEFGM), etc.&lt;br /&gt;
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The three most widely used numerical methods to solve PDEs are the finite element method (FEM), finite volume methods (FVM) and finite difference methods (FDM), as well other kind of methods called Meshfree methods, which were made to solve problems where the before mentioned methods are limited. The FEM has a prominent position among these methods and especially its exceptionally efficient higher-order version hp-FEM. Other hybrid versions of FEM and Meshfree methods include the generalized finite element method (GFEM), extended finite element method (XFEM), spectral finite element method (SFEM), meshfree finite element method, discontinuous Galerkin finite element method (DGFEM), Element-Free Galerkin Method (EFGM), Interpolating Element-Free Galerkin Method (IEFGM), etc.&lt;br /&gt;
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求解偏微分方程最常用的三种数值方法是有限元分析法、有限体积法和有限差分法，以及其他一些称为无网格法的方法。这些方法用于解决前面提到的方法受到的限制。在这些方法中，有限元方法，尤其是高效的高阶有限元方法，占有重要地位。其他有限元法和无网格法的混合形式包括广义有限元分析法(GFEM)、扩展有限元分析法(XFEM)、谱有限元分析法(SFEM)、无网格有限元分析法(DGFEM)、间断伽辽金有限元分析法(DGFEM)、无网格伽辽金法(EFGM)、插值无网格伽辽金法(IEFGM)等。&lt;br /&gt;
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=== Finite element method ===&lt;br /&gt;
有限元分析法&lt;br /&gt;
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{{main|Finite element method}}&lt;br /&gt;
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The finite element method (FEM) (its practical application often known as finite element analysis (FEA)) is a numerical technique for finding approximate solutions of partial differential equations (PDE) as well as of integral equations. The solution approach is based either on eliminating the differential equation completely (steady state problems), or rendering the PDE into an approximating system of ordinary differential equations, which are then numerically integrated using standard techniques such as Euler's method, Runge–Kutta, etc.&lt;br /&gt;
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The finite element method (FEM) (its practical application often known as finite element analysis (FEA)) is a numerical technique for finding approximate solutions of partial differential equations (PDE) as well as of integral equations. The solution approach is based either on eliminating the differential equation completely (steady state problems), or rendering the PDE into an approximating system of ordinary differential equations, which are then numerically integrated using standard techniques such as Euler's method, Runge–Kutta, etc.&lt;br /&gt;
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'''&amp;lt;font color = &amp;quot;#ff8000&amp;quot;&amp;gt;有限元分析法 Finite Element Method&amp;lt;/font&amp;gt;''' ((其实际应用通常被称为有限元分析(FEA))是一种寻找偏微分方程(PDE)和积分方程近似解的数值技术。这种求解方法要么基于完全消除微分方程(稳态问题) ，要么将偏微分方程转化为常微分方程的近似系统，然后使用标准技术进行数值积分，如欧拉方法、 Runge-Kutta 等。&lt;br /&gt;
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===Finite difference method===&lt;br /&gt;
有限差分法&lt;br /&gt;
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{{main|Finite difference method}}&lt;br /&gt;
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Finite-difference methods are numerical methods for approximating the solutions to differential equations using [[finite difference]] equations to approximate derivatives.&lt;br /&gt;
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Finite-difference methods are numerical methods for approximating the solutions to differential equations using finite difference equations to approximate derivatives.&lt;br /&gt;
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有限差分法是一种数值方法，用差分方程近似微分方程的解。&lt;br /&gt;
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=== Finite volume method ===&lt;br /&gt;
有限体积法&lt;br /&gt;
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{{main|Finite volume method}}&lt;br /&gt;
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Similar to the finite difference method or finite element method, values are calculated at discrete places on a meshed geometry. &amp;quot;Finite volume&amp;quot; refers to the small volume surrounding each node point on a mesh. In the finite volume method, surface integrals in a partial differential equation that contain a divergence term are converted to volume integrals, using the [[divergence theorem]]. These terms are then evaluated as fluxes at the surfaces of each finite volume. Because the flux entering a given volume is identical to that leaving the adjacent volume, these methods conserve mass by design.&lt;br /&gt;
&lt;br /&gt;
Similar to the finite difference method or finite element method, values are calculated at discrete places on a meshed geometry. &amp;quot;Finite volume&amp;quot; refers to the small volume surrounding each node point on a mesh. In the finite volume method, surface integrals in a partial differential equation that contain a divergence term are converted to volume integrals, using the divergence theorem. These terms are then evaluated as fluxes at the surfaces of each finite volume. Because the flux entering a given volume is identical to that leaving the adjacent volume, these methods conserve mass by design.&lt;br /&gt;
&lt;br /&gt;
类似于有限差分法或有限元分析，函数值是在网状几何体上的离散位置进行计算的。“有限体积”是指网格上每个节点周围的小体积。在有限体积法中，偏微分方程中含有散度项的面积分用散度定理积分转换成体积分。然后将这些项用于估算每个有限体积表面上的通量。由于进入给定体积的通量与转移到相邻体积元的通量相同，所以这些方法在设计上保证了质量守恒。&lt;br /&gt;
&lt;br /&gt;
==See also==&lt;br /&gt;
请参阅&lt;br /&gt;
* [[Dirichlet boundary condition]]&lt;br /&gt;
狄利克雷边界条件&lt;br /&gt;
* [[Jet bundle]]&lt;br /&gt;
射流丛&lt;br /&gt;
* [[Laplace transform applied to differential equations]]&lt;br /&gt;
微分方程中的拉普拉斯变换&lt;br /&gt;
* [[List of dynamical systems and differential equations topics]]&lt;br /&gt;
动力学系统列表和微分方程主题&lt;br /&gt;
* [[Matrix differential equation]]&lt;br /&gt;
矩阵微分方程&lt;br /&gt;
* [[Neumann boundary condition]]&lt;br /&gt;
诺伊曼边界条件&lt;br /&gt;
* [[Numerical partial differential equations]]&lt;br /&gt;
数值偏微分方程&lt;br /&gt;
* [[Partial differential algebraic equation]]&lt;br /&gt;
偏微分代数方程&lt;br /&gt;
* [[Recurrence relation]]&lt;br /&gt;
递推关系&lt;br /&gt;
* [[Robin boundary condition]]&lt;br /&gt;
罗宾边界条件&lt;br /&gt;
* [[Stochastic processes and boundary value problems]]&lt;br /&gt;
随机过程和边值问题&lt;br /&gt;
&lt;br /&gt;
== The energy method ==&lt;br /&gt;
能量法&lt;br /&gt;
&lt;br /&gt;
The energy method is a mathematical procedure that can be used to verify well-posedness of initial-boundary-value-problems.&amp;lt;ref&amp;gt;{{cite book |title=High Order Difference Methods for Time Dependent PDE&lt;br /&gt;
&lt;br /&gt;
The energy method is a mathematical procedure that can be used to verify well-posedness of initial-boundary-value-problems.&amp;lt;ref&amp;gt;{{cite book |title=High Order Difference Methods for Time Dependent PDE&lt;br /&gt;
&lt;br /&gt;
能量法是一种数学过程，可用于验证初始边界值问题的适定性。&lt;br /&gt;
&lt;br /&gt;
In the following example the energy method is used to decide where and which boundary conditions should be imposed such that the resulting IBVP is well-posed. Consider the one-dimensional hyperbolic PDE given by&lt;br /&gt;
&lt;br /&gt;
In the following example the energy method is used to decide where and which boundary conditions should be imposed such that the resulting IBVP is well-posed. Consider the one-dimensional hyperbolic PDE given by&lt;br /&gt;
&lt;br /&gt;
在下面的示例中，将使用能量法决定应在何处施加哪些边界条件，以使得到的IBVP处于适当位置。考虑下式给出的一维双曲PDE&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt;\frac{\partial u}{\partial t} + \alpha \frac{\partial u}{\partial x} = 0, \quad x \in [a,b], \operatorname t &amp;gt; 0,&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;\frac{\partial u}{\partial t} + \alpha \frac{\partial u}{\partial x} = 0, \quad x \in [a,b], \operatorname t &amp;gt; 0,&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
where &amp;lt;math&amp;gt;\alpha \neq 0&amp;lt;/math&amp;gt; is a constant and &amp;lt;math&amp;gt;u(x,t)&amp;lt;/math&amp;gt; is an unknown function with initial condition &amp;lt;math&amp;gt;u(x,0) = f(x)&amp;lt;/math&amp;gt;. Multiplying with &amp;lt;math&amp;gt;u&amp;lt;/math&amp;gt; and integrating over the domain gives&lt;br /&gt;
&lt;br /&gt;
where &amp;lt;math&amp;gt;\alpha \neq 0&amp;lt;/math&amp;gt; is a constant and &amp;lt;math&amp;gt;u(x,t)&amp;lt;/math&amp;gt; is an unknown function with initial condition &amp;lt;math&amp;gt;u(x,0) = f(x)&amp;lt;/math&amp;gt;. Multiplying with &amp;lt;math&amp;gt;u&amp;lt;/math&amp;gt; and integrating over the domain gives&lt;br /&gt;
&lt;br /&gt;
其中 &amp;lt;math&amp;gt;\alpha \neq 0&amp;lt;/math&amp;gt; 是常数，并且 &amp;lt;math&amp;gt;u(x,t)&amp;lt;/math&amp;gt; 是初始条件是 &amp;lt;math&amp;gt;u(x,0) = f(x)&amp;lt;/math&amp;gt;的未知函数，乘以 &amp;lt;math&amp;gt;u&amp;lt;/math&amp;gt; 并在域上进行积分。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt;\int_a^b u \frac{\partial u}{\partial t} \operatorname dx + \alpha \int _a ^b u \frac{\partial u}{\partial x} \operatorname dx = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;\int_a^b u \frac{\partial u}{\partial t} \operatorname dx + \alpha \int _a ^b u \frac{\partial u}{\partial x} \operatorname dx = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Using that&lt;br /&gt;
&lt;br /&gt;
Using that&lt;br /&gt;
&lt;br /&gt;
利用这一点&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt;\int _a ^b u \frac{\partial u}{\partial t} \operatorname dx = \frac{1}{2} \frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 \quad \text{and} \quad \int _a ^b u \frac{\partial u}{\partial x} \operatorname dx = \frac{1}{2} u(b,t)^2 - \frac{1}{2} u(a,t)^2,.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;\int _a ^b u \frac{\partial u}{\partial t} \operatorname dx = \frac{1}{2} \frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 \quad \text{and} \quad \int _a ^b u \frac{\partial u}{\partial x} \operatorname dx = \frac{1}{2} u(b,t)^2 - \frac{1}{2} u(a,t)^2,.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
where integration by parts has been used for the second relationship, we get&lt;br /&gt;
&lt;br /&gt;
where integration by parts has been used for the second relationship, we get&lt;br /&gt;
&lt;br /&gt;
第二个关系中采用了分部积分法，我们可以得到&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt;\frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 + \alpha u(b,t)^2 - \alpha u(a,t)^2 = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;\frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 + \alpha u(b,t)^2 - \alpha u(a,t)^2 = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Here &amp;lt;math&amp;gt;\vert \vert \cdot \vert \vert&amp;lt;/math&amp;gt; denotes the standard L2-norm.&lt;br /&gt;
&lt;br /&gt;
Here &amp;lt;math&amp;gt;\vert \vert \cdot \vert \vert&amp;lt;/math&amp;gt; denotes the standard L2-norm.&lt;br /&gt;
&lt;br /&gt;
在这里，&amp;lt;math&amp;gt;\vert \vert \cdot \vert \vert&amp;lt;/math&amp;gt; 表示标准的L2-正则。&lt;br /&gt;
&lt;br /&gt;
For well-posedness we require that the energy of the solution is non-increasing, i.e. that &amp;lt;math&amp;gt;\frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 \leq 0&amp;lt;/math&amp;gt;, which is achieved by specifying &amp;lt;math&amp;gt;u&amp;lt;/math&amp;gt; at &amp;lt;math&amp;gt;x = a&amp;lt;/math&amp;gt; if &amp;lt;math&amp;gt;\alpha &amp;gt; 0&amp;lt;/math&amp;gt; and at &amp;lt;math&amp;gt;x = b&amp;lt;/math&amp;gt; if &amp;lt;math&amp;gt;\alpha &amp;lt; 0&amp;lt;/math&amp;gt;. This corresponds to only imposing boundary conditions at the inflow. Note that well-posedness allows for growth in terms of data (initial and boundary) and thus it is sufficient to show that &amp;lt;math&amp;gt;\frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 \leq 0&amp;lt;/math&amp;gt; holds when all data is set to zero.&lt;br /&gt;
&lt;br /&gt;
For well-posedness we require that the energy of the solution is non-increasing, i.e. that &amp;lt;math&amp;gt;\frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 \leq 0&amp;lt;/math&amp;gt;, which is achieved by specifying &amp;lt;math&amp;gt;u&amp;lt;/math&amp;gt; at &amp;lt;math&amp;gt;x = a&amp;lt;/math&amp;gt; if &amp;lt;math&amp;gt;\alpha &amp;gt; 0&amp;lt;/math&amp;gt; and at &amp;lt;math&amp;gt;x = b&amp;lt;/math&amp;gt; if &amp;lt;math&amp;gt;\alpha &amp;lt; 0&amp;lt;/math&amp;gt;. This corresponds to only imposing boundary conditions at the inflow. Note that well-posedness allows for growth in terms of data (initial and boundary) and thus it is sufficient to show that &amp;lt;math&amp;gt;\frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 \leq 0&amp;lt;/math&amp;gt; holds when all data is set to zero.&lt;br /&gt;
&lt;br /&gt;
对于适定性，我们要求解的能量是不增加的，即 &amp;lt;math&amp;gt;\frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 \leq 0&amp;lt;/math&amp;gt; ，这种关系可以通过在&amp;lt;math&amp;gt;x = a&amp;lt;/math&amp;gt;处 （如果 &amp;lt;math&amp;gt;\alpha &amp;gt; 0&amp;lt;/math&amp;gt;） 以及 &amp;lt;math&amp;gt;x = b&amp;lt;/math&amp;gt;处 （如果 &amp;lt;math&amp;gt;\alpha &amp;lt; 0&amp;lt;/math&amp;gt;）指定&amp;lt;math&amp;gt;u&amp;lt;/math&amp;gt;的值来实现。这相当于只在流入处附加边界条件。注意，适定性允许在数据项(初始和边界)上的增长，因此它足以表明当所有数据设置为零时应有 &amp;lt;math&amp;gt;\frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 \leq 0&amp;lt;/math&amp;gt;。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==Notes==&lt;br /&gt;
&lt;br /&gt;
{{Reflist}}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
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&lt;br /&gt;
{{refend}}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
== Further reading ==&lt;br /&gt;
&lt;br /&gt;
* {{Cite journal|last=Cajori|first=Florian|authorlink=Florian Cajori|year=1928|title=The Early History of Partial Differential Equations and of Partial Differentiation and Integration|url=http://www.math.harvard.edu/archive/21a_fall_14/exhibits/cajori/cajori.pdf|journal=The American Mathematical Monthly|volume=35|issue=9|pages=459–467|doi=10.2307/2298771|access-date=2016-05-15|archive-url=https://web.archive.org/web/20181123102253/http://www.math.harvard.edu/archive/21a_fall_14/exhibits/cajori/cajori.pdf|archive-date=2018-11-23|url-status=dead}}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
== External links ==&lt;br /&gt;
&lt;br /&gt;
{{Sister project links| wikt=no | commons=Category:Solutions of PDE | b=Partial Differential Equations | n=no | q=Partial differential equation | s=no | v=no | voy=no | species=no | d=no}}&lt;br /&gt;
&lt;br /&gt;
* {{springer|title=Differential equation, partial|id=p/d031920}}&lt;br /&gt;
&lt;br /&gt;
* [http://eqworld.ipmnet.ru/en/pde-en.htm Partial Differential Equations: Exact Solutions] at EqWorld: The World of Mathematical Equations.&lt;br /&gt;
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* [http://eqworld.ipmnet.ru/en/solutions/eqindex/eqindex-pde.htm Partial Differential Equations: Index] at EqWorld: The World of Mathematical Equations.&lt;br /&gt;
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* [http://eqworld.ipmnet.ru/en/methods/meth-pde.htm Partial Differential Equations: Methods] at EqWorld: The World of Mathematical Equations.&lt;br /&gt;
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* [https://web.archive.org/web/20170701144823/http://www.exampleproblems.com/wiki/index.php?title=Partial_Differential_Equations Example problems with solutions] at exampleproblems.com&lt;br /&gt;
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* [http://mathworld.wolfram.com/PartialDifferentialEquation.html Partial Differential Equations] at mathworld.wolfram.com&lt;br /&gt;
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* [https://reference.wolfram.com/language/FEMDocumentation/tutorial/SolvingPDEwithFEM.html Partial Differential Equations] with Mathematica&lt;br /&gt;
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* [http://www.mathworks.com/moler/pdes.pdf Partial Differential Equations] in Cleve Moler: Numerical Computing with MATLAB&lt;br /&gt;
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* [http://www.nag.com/numeric/fl/nagdoc_fl24/html/D03/d03intro.html Partial Differential Equations] at nag.com&lt;br /&gt;
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* {{cite web |first=Grant |last=Sanderson |title=But what is a partial differential equation? |work=3Blue1Brown |date=April 21, 2019 |url=https://www.youtube.com/watch?v=ly4S0oi3Yz8&amp;amp;list=PLZHQObOWTQDNPOjrT6KVlfJuKtYTftqH6 |via=[[YouTube]] }}&lt;br /&gt;
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{{Differential equations topics}}&lt;br /&gt;
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[[Category:Partial differential equations| ]]&lt;br /&gt;
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[[Category:Multivariable calculus]]&lt;br /&gt;
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[[Category:Differential equations]]&lt;br /&gt;
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Category:Differential equations&lt;br /&gt;
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类别: 微分方程&lt;br /&gt;
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Category:Concepts in physics&lt;br /&gt;
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&amp;lt;small&amp;gt;This page was moved from [[wikipedia:en:Partial differential equation]]. Its edit history can be viewed at [[偏微分方程/edithistory]]&amp;lt;/small&amp;gt;&amp;lt;/noinclude&amp;gt;&lt;br /&gt;
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[[Category:待整理页面]]&lt;/div&gt;</summary>
		<author><name>Ruili</name></author>
	</entry>
	<entry>
		<id>https://wiki.swarma.org/index.php?title=%E5%81%8F%E5%BE%AE%E5%88%86%E6%96%B9%E7%A8%8B&amp;diff=20104</id>
		<title>偏微分方程</title>
		<link rel="alternate" type="text/html" href="https://wiki.swarma.org/index.php?title=%E5%81%8F%E5%BE%AE%E5%88%86%E6%96%B9%E7%A8%8B&amp;diff=20104"/>
		<updated>2020-12-15T12:56:59Z</updated>

		<summary type="html">&lt;p&gt;Ruili：&lt;/p&gt;
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&lt;div&gt;此词条暂由Yuling翻译，未经人工整理和审校，带来阅读不便，请见谅。&lt;br /&gt;
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[[File:Heat.gif|thumb|right|A visualisation of a solution to the two-dimensional [[heat equation]] with temperature represented by the third dimension]]&lt;br /&gt;
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A visualisation of a solution to the two-dimensional [[heat equation with temperature represented by the third dimension]]&lt;br /&gt;
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以三维表示温度的二维热方程解的可视化&lt;br /&gt;
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In [[mathematics]], a '''partial differential equation''' ('''PDE''') is a [[differential equation]] that contains unknown [[Multivariable calculus|multivariable functions]] and their [[partial derivative]]s. PDEs are used to formulate problems involving functions of several variables, and are either solved by hand, or used to create a [[computer model]]. A special case is [[ordinary differential equation]]s (ODEs), which deal with functions of a single variable and their derivatives.&lt;br /&gt;
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In mathematics, a partial differential equation (PDE) is a differential equation that contains unknown multivariable functions and their partial derivatives. PDEs are used to formulate problems involving functions of several variables, and are either solved by hand, or used to create a computer model. A special case is ordinary differential equations (ODEs), which deal with functions of a single variable and their derivatives.&lt;br /&gt;
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在数学中，'''&amp;lt;font color = &amp;quot;#ff8000&amp;quot;&amp;gt; 偏微分方程函数 Partial Differential Equation&amp;lt;/font&amp;gt;'''是包含未知多元函数及其偏导数的微分方程。偏微分方程用于描述涉及多元函数的问题，可以通过人为求解，也可以通过建立计算机模型来求解。常微分方程是偏微分方程一种特殊情况，它处理的是一元函数及其导数。&lt;br /&gt;
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PDEs can be used to describe a wide variety of phenomena such as sound, heat, [[diffusion]], [[electrostatics]], [[Electromagnetism|electrodynamics]], [[fluid dynamics]], [[Elasticity (physics)|elasticity]], [[gravitation]] and [[quantum mechanics]]. These seemingly distinct physical phenomena can be formalised similarly in terms of PDEs. Just as ordinary differential equations often model one-dimensional [[dynamical system]]s, partial differential equations often model [[multidimensional system]]s. PDEs find their generalisation in [[stochastic partial differential equation]]s.&lt;br /&gt;
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PDEs can be used to describe a wide variety of phenomena such as sound, heat, diffusion, electrostatics, electrodynamics, fluid dynamics, elasticity, gravitation and quantum mechanics. These seemingly distinct physical phenomena can be formalised similarly in terms of PDEs. Just as ordinary differential equations often model one-dimensional dynamical systems, partial differential equations often model multidimensional systems. PDEs find their generalisation in stochastic partial differential equations.&lt;br /&gt;
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偏微分方程可以用来描述各种各样的物理现象，如声音，热量，扩散，静电，电动力学，流体力学，弹性力学，重力和量子力学。这些看起来截然不同的物理现象却可以用类似的偏微分方程来描述。正如常微分方程经常对一维动力系统进行建模一样，偏微分方程经常对多维系统进行建模。随机偏微分方程是偏微分方程的一种推广。&lt;br /&gt;
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== Introduction ==&lt;br /&gt;
引言&lt;br /&gt;
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Partial differential equations (PDEs) are equations that involve rates of change with respect to [[continuous variables]]. For example, the position of a [[rigid body]] is specified by six parameters,&amp;lt;ref&amp;gt;{{Cite book|url=https://books.google.com/books?id=v9PLbcYd9aUC&amp;amp;pg=PA32|title=Modelling and Control of Robot Manipulators|last=Sciavicco|first=Lorenzo|last2=Siciliano|first2=Bruno|date=2001-02-19|publisher=Springer Science &amp;amp; Business Media|isbn=9781852332211|language=en}}&amp;lt;/ref&amp;gt; but the configuration of a [[fluid]] is given by the [[continuous distribution]] of several parameters, such as the [[temperature]], [[pressure]], and so forth. The dynamics for the rigid body take place in a finite-dimensional [[Configuration space (physics)|configuration space]]; the dynamics for the fluid occur in an infinite-dimensional configuration space. This distinction usually makes PDEs much harder to solve than ordinary differential equations (ODEs), but here again, there will be simple solutions for linear problems. Classic domains where PDEs are used include [[acoustics]], [[fluid dynamics]], [[electrodynamics]], and [[heat transfer]].&lt;br /&gt;
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Partial differential equations (PDEs) are equations that involve rates of change with respect to continuous variables. For example, the position of a rigid body is specified by six parameters, but the configuration of a fluid is given by the continuous distribution of several parameters, such as the temperature, pressure, and so forth. The dynamics for the rigid body take place in a finite-dimensional configuration space; the dynamics for the fluid occur in an infinite-dimensional configuration space. This distinction usually makes PDEs much harder to solve than ordinary differential equations (ODEs), but here again, there will be simple solutions for linear problems. Classic domains where PDEs are used include acoustics, fluid dynamics, electrodynamics, and heat transfer.&lt;br /&gt;
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偏微分方程(简称为PDEs)涉及到方程相对于连续变量的变化率。例如，刚体的位置是由六个参数确定的，而流体的状态是由几个参数的连续分布给出的，如温度、压力等。刚体的动力学过程发生在有限维状态空间中，流体的动力学过程发生在无限维状态空间中。这种区别通常使偏微分方程比常微分方程更难求解，但是线性问题仍然有简单的求解方式。使用偏微分方程的经典领域包括声学、流体力学、电动力学和传热学。&lt;br /&gt;
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A partial differential equation (PDE) for the function {{math|''u''(''x''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;,… ''x&amp;lt;sub&amp;gt;n&amp;lt;/sub&amp;gt;'')}} is an equation of the form&lt;br /&gt;
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A partial differential equation (PDE) for the function  is an equation of the form&lt;br /&gt;
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函数 {{math|''u''(''x''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;,… ''x&amp;lt;sub&amp;gt;n&amp;lt;/sub&amp;gt;'')}} 的偏微分方程形式是：&lt;br /&gt;
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: &amp;lt;math&amp;gt;f \left (x_1, \ldots x_n; u, \frac{\partial u}{\partial x_1}, \ldots \frac{\partial u}{\partial x_n}; \frac{\partial^2 u}{\partial x_1 \partial x_1}, \ldots \frac{\partial^2 u}{\partial x_1 \partial x_n}; \ldots \right) = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;f \left (x_1, \ldots x_n; u, \frac{\partial u}{\partial x_1}, \ldots \frac{\partial u}{\partial x_n}; \frac{\partial^2 u}{\partial x_1 \partial x_1}, \ldots \frac{\partial^2 u}{\partial x_1 \partial x_n}; \ldots \right) = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
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If {{mvar|f}} is a [[linear function]] of {{mvar|u}} and its derivatives, then the PDE is called linear. Common examples of linear PDEs include the [[heat equation]], the [[wave equation]], [[Laplace's equation]], [[Helmholtz equation]], [[Klein–Gordon equation]], and [[Poisson's equation]].&lt;br /&gt;
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If  is a linear function of  and its derivatives, then the PDE is called linear. Common examples of linear PDEs include the heat equation, the wave equation, Laplace's equation, Helmholtz equation, Klein–Gordon equation, and Poisson's equation.&lt;br /&gt;
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如果 {{mvar|f}} 是函数 {{math|''u''}} 及其导数的线性函数，则偏微分方程称为线性函数。线性偏微分方程的常见例子包括热方程、波动方程、拉普拉斯方程、亥姆霍兹方程方程、克莱因-高登方程和泊松方程。&lt;br /&gt;
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A relatively simple PDE is&lt;br /&gt;
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A relatively simple PDE is&lt;br /&gt;
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一个相对简单的偏微分方程：&lt;br /&gt;
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: &amp;lt;math&amp;gt;\frac{\partial u}{\partial x}(x,y) = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;\frac{\partial u}{\partial x}(x,y) = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
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This relation [[Logical implication|implies]] that the function {{math|''u''(''x'',''y'')}} is independent of {{mvar|x}}. However, the equation gives no information on the function's dependence on the variable {{mvar|y}}. Hence the general solution of this equation is&lt;br /&gt;
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This relation implies that the function  is independent of . However, the equation gives no information on the function's dependence on the variable . Hence the general solution of this equation is&lt;br /&gt;
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这意味着函数 {{math|''u''(''x'',''y'')}} 独立于 {{mvar|x}} 的。然而，这个方程没有给出关于函数和自变量的相关性的信息。因此，这个方程的通解是&lt;br /&gt;
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: &amp;lt;math&amp;gt;u(x,y) = f(y),&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;u(x,y) = f(y),&amp;lt;/math&amp;gt;&lt;br /&gt;
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where {{mvar|f}} is an arbitrary function of {{mvar|y}}. The analogous ordinary differential equation is&lt;br /&gt;
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where  is an arbitrary function of . The analogous ordinary differential equation is&lt;br /&gt;
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其中， {{mvar|f}} 是 {{mvar|y}} 的任意函数。&lt;br /&gt;
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类似的常微分方程是：&lt;br /&gt;
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: &amp;lt;math&amp;gt;\frac{\mathrm{d} u}{\mathrm{d} x}(x) = 0,&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;\frac{\mathrm{d} u}{\mathrm{d} x}(x) = 0,&amp;lt;/math&amp;gt;&lt;br /&gt;
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which has the solution&lt;br /&gt;
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which has the solution&lt;br /&gt;
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它的解为&lt;br /&gt;
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: &amp;lt;math&amp;gt;u(x) = c,&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;u(x) = c,&amp;lt;/math&amp;gt;&lt;br /&gt;
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where {{mvar|c}} is any [[Constant (mathematics)|constant]] value. These two examples illustrate that general solutions of ordinary differential equations (ODEs) involve arbitrary constants, but solutions of PDEs involve arbitrary functions.&lt;br /&gt;
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where  is any constant value. These two examples illustrate that general solutions of ordinary differential equations (ODEs) involve arbitrary constants, but solutions of PDEs involve arbitrary functions.&lt;br /&gt;
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这里，{{mvar|c}} 是一个任意常量。&lt;br /&gt;
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这两个例子说明常微分方程的一般解包含任意常数，但偏微分方程的解包含任意函数。&lt;br /&gt;
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A solution of a PDE is generally not [[Uniqueness quantification|unique]]; additional conditions must generally be specified on the [[Boundary (topology)|boundary]] of the region where the solution is defined. For instance, in the simple example above, the function {{math|''f''(''y'')}} can be determined if {{mvar|u}} is specified on the line {{math|''x'' {{=}} 0}}.&lt;br /&gt;
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A solution of a PDE is generally not unique; additional conditions must generally be specified on the boundary of the region where the solution is defined. For instance, in the simple example above, the function  can be determined if  is specified on the line  0}}.&lt;br /&gt;
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偏微分方程的解一般不是唯一的; 一般必须在定义解的区域边界上定义附加条件。 例如，在上面的简单示例中，如果在 {{math|''x'' {{=}} 0}} 时确定了 {{mvar|u}} 的值，则可以确定该函数 {{math|''f''(''y'')}}。&lt;br /&gt;
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== Existence and uniqueness ==&lt;br /&gt;
存在性和唯一性&lt;br /&gt;
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Although the issue of existence and uniqueness of solutions of ordinary differential equations has a very satisfactory answer with the [[Picard–Lindelöf theorem]], that is far from the case for partial differential equations. The [[Cauchy–Kowalevski theorem]] states that the [[Cauchy problem]] for any partial differential equation whose coefficients are [[Analytic function|analytic]] in the unknown function and its derivatives, has a locally unique analytic solution. Although this result might appear to settle the existence and uniqueness of solutions, there are examples of linear partial differential equations whose coefficients have derivatives of all orders (which are nevertheless not analytic) but which have no solutions at all: see [[Lewy's example|Lewy (1957)]]. Even if the solution of a partial differential equation exists and is unique, it may nevertheless have undesirable properties.  The mathematical study of these questions is usually in the more powerful context of [[weak solution]]s.&lt;br /&gt;
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Although the issue of existence and uniqueness of solutions of ordinary differential equations has a very satisfactory answer with the Picard–Lindelöf theorem, that is far from the case for partial differential equations. The Cauchy–Kowalevski theorem states that the Cauchy problem for any partial differential equation whose coefficients are analytic in the unknown function and its derivatives, has a locally unique analytic solution. Although this result might appear to settle the existence and uniqueness of solutions, there are examples of linear partial differential equations whose coefficients have derivatives of all orders (which are nevertheless not analytic) but which have no solutions at all: see Lewy (1957). Even if the solution of a partial differential equation exists and is unique, it may nevertheless have undesirable properties.  The mathematical study of these questions is usually in the more powerful context of weak solutions.&lt;br /&gt;
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尽管常微分方程解的存在性和唯一性用'''&amp;lt;font color=&amp;quot;#ff8000&amp;quot;&amp;gt;弗罗贝尼乌斯定理 Picard–Lindelöf Theorem&amp;lt;/font&amp;gt;得到了令人满意的结果，但偏微分方程解的存在性和唯一性却远没有得到解决。'''&amp;lt;font color=&amp;quot;#ff8000&amp;quot;&amp;gt;柯西-科瓦列夫斯基定理 Cauchy–Kowalevski theorem&amp;lt;/font&amp;gt;指出：对于任意系数在未知函数及其导数中解析的偏微分方程，柯西问题存在一个局部唯一的解析解。虽然这个结果似乎解决了解的存在性和唯一性问题，但是存在一些线性偏微分方程-其系数具有所有级数的导数(尽管这些导数不是解析的) ，但是根本没有解: 见 Lewy (1957)。即使偏微分方程的解存在且唯一，它仍然可能具有不可预料的性质。这些问题的数学研究通常是在更有力的弱解的背景下进行的。&lt;br /&gt;
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An example of pathological behavior is the sequence (depending upon {{mvar|n}}) of [[Cauchy problem]]s for the [[Laplace equation]]&lt;br /&gt;
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An example of pathological behavior is the sequence (depending upon ) of Cauchy problems for the Laplace equation&lt;br /&gt;
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反常特征的一个例子是拉普拉斯方程的柯西问题的序列(取决于{{mvar|n}})&lt;br /&gt;
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: &amp;lt;math&amp;gt;\frac{\partial^2 u}{\partial x^2} + \frac{\partial^2 u}{\partial y^2}=0,&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;\frac{\partial^2 u}{\partial x^2} + \frac{\partial^2 u}{\partial y^2}=0,&amp;lt;/math&amp;gt;&lt;br /&gt;
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with [[boundary condition]]s&lt;br /&gt;
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with boundary conditions&lt;br /&gt;
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具有边界条件&lt;br /&gt;
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: &amp;lt;math&amp;gt;\begin{align} u(x,0) &amp;amp;= 0, \\ \frac{\partial u}{\partial y}(x,0) &amp;amp;= \frac{\sin nx}{n}, \end{align}&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;\begin{align} u(x,0) &amp;amp;= 0, \\ \frac{\partial u}{\partial y}(x,0) &amp;amp;= \frac{\sin nx}{n}, \end{align}&amp;lt;/math&amp;gt;&lt;br /&gt;
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where {{mvar|n}} is an integer. The derivative of {{mvar|u}} with respect to {{mvar|y}} approaches zero [[uniform convergence|uniformly]] in {{mvar|x}} as {{mvar|n}} increases, but the solution is&lt;br /&gt;
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where  is an integer. The derivative of  with respect to  approaches zero uniformly in  as  increases, but the solution is&lt;br /&gt;
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其中 {{mvar|n}} 是整数。{{mvar|u}} 关于 {{mvar|y}} 的导数，一致地随着 {{mvar|n}} 的增加而趋于零，但解是&lt;br /&gt;
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: &amp;lt;math&amp;gt;u(x,y) = \frac{\sinh ny \sin nx}{n^2}.&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;u(x,y) = \frac{\sinh ny \sin nx}{n^2}.&amp;lt;/math&amp;gt;&lt;br /&gt;
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This solution approaches infinity if {{mvar|nx}} is not an integer multiple of {{pi}} for any non-zero value of {{mvar|y}}. The Cauchy problem for the Laplace equation is called ''ill-posed'' or ''not [[Well-posed problem|well-posed]]'', since the solution does not continuously depend on the data of the problem. Such ill-posed problems are not usually satisfactory for physical applications.&lt;br /&gt;
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This solution approaches infinity if  is not an integer multiple of  for any non-zero value of . The Cauchy problem for the Laplace equation is called ill-posed or not well-posed, since the solution does not continuously depend on the data of the problem. Such ill-posed problems are not usually satisfactory for physical applications.&lt;br /&gt;
&lt;br /&gt;
对于任何非零的 {{mvar|y}}，如果 {{mvar|nx}} 不是模板 {{pi}} 的整数倍，这个解会接近于无穷大。拉普拉斯方程的柯西问题被称为不适定的（可以译为ill-posed或not well-posed），因为解不是连续地依赖于问题的数据。这种不适定问题通常不能满足物理应用。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The [[Navier–Stokes existence and smoothness|existence of solutions for the Navier–Stokes equations]], a partial differential equation, is part of one of the [[Millennium Prize Problems]].&lt;br /&gt;
&lt;br /&gt;
The existence of solutions for the Navier–Stokes equations, a partial differential equation, is part of one of the Millennium Prize Problems.&lt;br /&gt;
&lt;br /&gt;
偏微分方程”纳维-斯托克斯方程“的解的存在性就是千禧年大奖难题之一的一部分。&lt;br /&gt;
&lt;br /&gt;
== Notation ==&lt;br /&gt;
符号&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
In PDEs, it is common to denote partial derivatives using subscripts. That is:&lt;br /&gt;
&lt;br /&gt;
In PDEs, it is common to denote partial derivatives using subscripts. That is:&lt;br /&gt;
&lt;br /&gt;
在偏微分方程中，通常用下标表示偏导数。例如:&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt;u_x = \frac{\partial u}{\partial x}&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;u_x = \frac{\partial u}{\partial x}&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt;u_{xx} = \frac{\partial^2 u}{\partial x^2} &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;u_{xx} = \frac{\partial^2 u}{\partial x^2} &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt;u_{xy} = \frac{\partial^2 u}{\partial y\, \partial x} = \frac{\partial}{\partial y } \left(\frac{\partial u}{\partial x}\right). &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;u_{xy} = \frac{\partial^2 u}{\partial y\, \partial x} = \frac{\partial}{\partial y } \left(\frac{\partial u}{\partial x}\right). &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Especially in physics, [[del]] or nabla ({{math|∇}}) is often used to denote spatial derivatives, and {{math|''&amp;amp;#x307;u'', ''ü''}} for time derivatives. For example, the [[wave equation]] (mentioned below) can be written as&lt;br /&gt;
&lt;br /&gt;
Especially in physics, del or nabla () is often used to denote spatial derivatives, and  for time derivatives. For example, the wave equation (mentioned below) can be written as&lt;br /&gt;
&lt;br /&gt;
特别是在物理学中，[[del]] 或 nabla ({{math|∇}}) 经常用来表示空间导数和时间导数。例如，波动方程(在下文中提到)可以写成：&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt;\ddot u=c^2\nabla^2u&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt;\ddot u=c^2\nabla^2u&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
or&lt;br /&gt;
&lt;br /&gt;
or&lt;br /&gt;
&lt;br /&gt;
或&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt;\ddot u=c^2\Delta u&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt;\ddot u=c^2\Delta u&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
where {{math|Δ}} is the [[Laplace operator]].&lt;br /&gt;
&lt;br /&gt;
where  is the Laplace operator.&lt;br /&gt;
&lt;br /&gt;
其中，{{math|Δ}} 代表拉普拉斯算子。&lt;br /&gt;
&lt;br /&gt;
== Classification ==&lt;br /&gt;
分类&lt;br /&gt;
&lt;br /&gt;
Some linear, second-order partial differential equations can be classified as [[parabolic partial differential equation|parabolic]], [[hyperbolic partial differential equation|hyperbolic]] and [[elliptic partial differential equation|elliptic]]. Others, such as the [[Euler–Tricomi equation]], have different types in different regions. The classification provides a guide to appropriate initial and boundary conditions and to the smoothness of the solutions.&lt;br /&gt;
&lt;br /&gt;
Some linear, second-order partial differential equations can be classified as parabolic, hyperbolic and elliptic. Others, such as the Euler–Tricomi equation, have different types in different regions. The classification provides a guide to appropriate initial and boundary conditions and to the smoothness of the solutions.&lt;br /&gt;
&lt;br /&gt;
一些线性二阶偏微分方程可分为抛物型方程、双曲型方程和椭圆型方程。其他的方程，如欧拉-特里科米方程，在不同的领域有不同的类型。这种分类有助于选择适当的初始和边界条件以及提高解的平滑性。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
=== Equations of first order ===&lt;br /&gt;
一阶方程&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{{main|First-order partial differential equation}}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
=== Linear equations of second order ===&lt;br /&gt;
二阶线性方程&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Assuming {{math|''u&amp;lt;sub&amp;gt;xy&amp;lt;/sub&amp;gt;'' {{=}} ''u&amp;lt;sub&amp;gt;yx&amp;lt;/sub&amp;gt;''}}, the general linear second-order PDE in two independent variables has the form&lt;br /&gt;
&lt;br /&gt;
Assuming  u&amp;lt;sub&amp;gt;yx&amp;lt;/sub&amp;gt;}}, the general linear second-order PDE in two independent variables has the form&lt;br /&gt;
&lt;br /&gt;
假设 {{math|''u&amp;lt;sub&amp;gt;xy&amp;lt;/sub&amp;gt;'' {{=}} ''u&amp;lt;sub&amp;gt;yx&amp;lt;/sub&amp;gt;''}}，含有两个独立变量的一般线性二阶偏微分方程具有如下形式：&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt;Au_{xx} + 2Bu_{xy} + Cu_{yy} + \cdots \mbox{(lower order terms)} = 0,&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;Au_{xx} + 2Bu_{xy} + Cu_{yy} + \cdots \mbox{(lower order terms)} = 0,&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
where the coefficients {{mvar|A}}, {{mvar|B}}, {{mvar|C}}... may depend upon {{mvar|x}} and {{mvar|y}}. If {{math|''A''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; + ''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; + ''C''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; &amp;gt; 0}} over a region of the {{mvar|xy}}-plane, the PDE is second-order in that region. This form is analogous to the equation for a conic section:&lt;br /&gt;
&lt;br /&gt;
where the coefficients , , ... may depend upon  and . If  over a region of the -plane, the PDE is second-order in that region. This form is analogous to the equation for a conic section:&lt;br /&gt;
&lt;br /&gt;
其中的系数 {{mvar|A}}, {{mvar|B}}, {{mvar|C}}... 一般取决于 {{mvar|x}} 和 {{mvar|y}} 。如果在 {{mvar|xy}}-平面的一个区域上 {{math|''A''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; + ''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; + ''C''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; &amp;gt; 0}}，偏微分方程是二阶的，这种形式类似于圆锥截面的方程:&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt;Ax^2 + 2Bxy + Cy^2 + \cdots = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;Ax^2 + 2Bxy + Cy^2 + \cdots = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
More precisely, replacing {{math|∂&amp;lt;sub&amp;gt;''x''&amp;lt;/sub&amp;gt;}} by {{mvar|X}}, and likewise for other variables (formally this is done by a [[Fourier transform]]), converts a constant-coefficient PDE into a polynomial of the same degree, with the terms of the highest degree (a [[homogeneous polynomial]], here a [[quadratic form]]) being most significant for the classification.&lt;br /&gt;
&lt;br /&gt;
More precisely, replacing  by , and likewise for other variables (formally this is done by a Fourier transform), converts a constant-coefficient PDE into a polynomial of the same degree, with the terms of the highest degree (a homogeneous polynomial, here a quadratic form) being most significant for the classification.&lt;br /&gt;
&lt;br /&gt;
更准确地说，用 {{mvar|X}} 替换 {{math|∂&amp;lt;sub&amp;gt;''x''&amp;lt;/sub&amp;gt;}}，并同样替换其它变量(通常由傅里叶变换完成)，将一个常系数偏微分方程转换成一个相同次数的多项式，最高次数的项(齐次多项式，这里是一个二次形式)对于偏微分方程的分类最为重要。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Just as one classifies [[conic section]]s and quadratic forms into parabolic, hyperbolic, and elliptic based on the [[discriminant]] {{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − 4''AC''}}, the same can be done for a second-order PDE at a given point.  However, the [[discriminant]] in a PDE is given by {{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC''}} due to the convention of the {{mvar|xy}} term being {{math|2''B''}} rather than {{mvar|B}}; formally, the discriminant (of the associated quadratic form) is {{math|(2''B'')&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − 4''AC'' {{=}} 4(''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC'')}}, with the factor of 4 dropped for simplicity.&lt;br /&gt;
&lt;br /&gt;
Just as one classifies conic sections and quadratic forms into parabolic, hyperbolic, and elliptic based on the discriminant , the same can be done for a second-order PDE at a given point.  However, the discriminant in a PDE is given by  due to the convention of the  term being  rather than ; formally, the discriminant (of the associated quadratic form) is  4(B&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − AC)}}, with the factor of 4 dropped for simplicity.&lt;br /&gt;
&lt;br /&gt;
正如人们可以根据判别式 {{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − 4''AC''}} 将圆锥截面和二次型分为抛物型、双曲型和椭圆型一样，对于给定点的二阶偏微分方程也可以这样做。然而，偏微分方程中的判别式 {{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − 4''AC''}} 是根据交叉项的系数{{math|2''B''}} 而不是 {{mvar|B}} 给出的，形式上，判别式(关联二次型)是 {{math|(2''B'')&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − 4''AC'' {{=}} 4(''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC'')}}，为简单起见，去掉了因子4。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
# {{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC'' &amp;lt; 0}} (''[[elliptic partial differential equation]]''): Solutions of [[elliptic partial differential equation|elliptic PDEs]] are as smooth as the coefficients allow, within the interior of the region where the equation and solutions are defined. For example, solutions of [[Laplace's equation]] are analytic within the domain where they are defined, but solutions may assume boundary values that are not smooth. The motion of a fluid at subsonic speeds can be approximated with elliptic PDEs, and the Euler–Tricomi equation is elliptic where {{math|''x'' &amp;lt; 0}}.&lt;br /&gt;
&lt;br /&gt;
  (elliptic partial differential equation): Solutions of elliptic PDEs are as smooth as the coefficients allow, within the interior of the region where the equation and solutions are defined. For example, solutions of Laplace's equation are analytic within the domain where they are defined, but solutions may assume boundary values that are not smooth. The motion of a fluid at subsonic speeds can be approximated with elliptic PDEs, and the Euler–Tricomi equation is elliptic where .&lt;br /&gt;
&lt;br /&gt;
{{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC'' &amp;lt; 0}} (椭圆型微分方程)：在定义方程和解的区域内部，椭圆型偏微分方程的解在系数允许的程度内光滑。例如，拉普拉斯方程的解在它们被定义的区域内是解析的，但可能假设边界值是不光滑的。亚音速流体的运动可以用椭圆型偏微分方程近似，欧拉-特里科米方程在 {{math|''x'' &amp;lt; 0}} 时是椭圆型偏微分方程。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
# {{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC'' {{=}} 0}} (''[[parabolic partial differential equation]]''): Equations that are [[parabolic partial differential equation|parabolic]] at every point can be transformed into a form analogous to the [[heat equation]] by a change of independent variables. Solutions smooth out as the transformed time variable increases. The Euler–Tricomi equation has parabolic type on the line where {{math|''x'' {{=}} 0}}.&lt;br /&gt;
&lt;br /&gt;
  0}} (parabolic partial differential equation): Equations that are parabolic at every point can be transformed into a form analogous to the heat equation by a change of independent variables. Solutions smooth out as the transformed time variable increases. The Euler–Tricomi equation has parabolic type on the line where  0}}.&lt;br /&gt;
&lt;br /&gt;
{{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC'' {{=}} 0}}（抛物型偏微分方程）：在每一点上都是抛物线型的方程可以通过改变自变量从而转化成类似于热方程的形式。随着转换后的时间变量的增加，方程的解变得平滑。欧拉-特里科米方程在特征线 {{math|''x'' {{=}} 0}} 上是抛物线型的。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
# {{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC'' &amp;gt; 0}} (''[[hyperbolic partial differential equation]]''): [[hyperbolic partial differential equation|hyperbolic]] equations retain any discontinuities of functions or derivatives in the initial data. An example is the [[wave equation]]. The motion of a fluid at supersonic speeds can be approximated with hyperbolic PDEs, and the Euler–Tricomi equation is hyperbolic where {{math|''x'' &amp;gt; 0}}.&lt;br /&gt;
&lt;br /&gt;
  (hyperbolic partial differential equation): hyperbolic equations retain any discontinuities of functions or derivatives in the initial data. An example is the wave equation. The motion of a fluid at supersonic speeds can be approximated with hyperbolic PDEs, and the Euler–Tricomi equation is hyperbolic where .&lt;br /&gt;
&lt;br /&gt;
{{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC'' &amp;gt; 0}} (双曲型偏微分方程)：双曲型方程在初始数据中保留了函数或导数的任何不连续性。波动方程就是其中的一个例子。超音速流体的运动可以用双曲型偏微分方程近似，欧拉-特里科米方程在 {{math|''x'' &amp;gt; 0}} 时是双曲型的。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
If there are {{mvar|n}} independent variables {{math|''x''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;, ''x''&amp;lt;sub&amp;gt;2 &amp;lt;/sub&amp;gt;,… ''x''&amp;lt;sub&amp;gt;''n''&amp;lt;/sub&amp;gt;}}, a general linear partial differential equation of second order has the form&lt;br /&gt;
&lt;br /&gt;
If there are  independent variables , a general linear partial differential equation of second order has the form&lt;br /&gt;
&lt;br /&gt;
如果存在 {{mvar|n}} 个自变量 {{math|''x''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;, ''x''&amp;lt;sub&amp;gt;2 &amp;lt;/sub&amp;gt;,… ''x''&amp;lt;sub&amp;gt;''n''&amp;lt;/sub&amp;gt;}}，一般二阶线性偏微分方程的形式是：&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt;L u =\sum_{i=1}^n\sum_{j=1}^n a_{i,j} \frac{\partial^2 u}{\partial x_i \partial x_j} \quad \text{ plus lower-order terms} =0.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;L u =\sum_{i=1}^n\sum_{j=1}^n a_{i,j} \frac{\partial^2 u}{\partial x_i \partial x_j} \quad \text{ plus lower-order terms} =0.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The classification depends upon the signature of the eigenvalues of the coefficient matrix {{math|''a''&amp;lt;sub&amp;gt;''i'',''j''&amp;lt;/sub&amp;gt;}}.&lt;br /&gt;
&lt;br /&gt;
The classification depends upon the signature of the eigenvalues of the coefficient matrix .&lt;br /&gt;
&lt;br /&gt;
这种分类取决于系数矩阵特征值的符号（正负性）。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
# Elliptic: the eigenvalues are all positive or all negative.&lt;br /&gt;
&lt;br /&gt;
 Elliptic: the eigenvalues are all positive or all negative.&lt;br /&gt;
&lt;br /&gt;
椭圆形方程: 特征值全部为正或全部为负。&lt;br /&gt;
&lt;br /&gt;
# Parabolic: the eigenvalues are all positive or all negative, save one that is zero.&lt;br /&gt;
&lt;br /&gt;
 Parabolic: the eigenvalues are all positive or all negative, save one that is zero.&lt;br /&gt;
&lt;br /&gt;
抛物线形方程:除了一个为零值，特征值全部为正或全部为负。&lt;br /&gt;
&lt;br /&gt;
# Hyperbolic: there is only one negative eigenvalue and all the rest are positive, or there is only one positive eigenvalue and all the rest are negative.&lt;br /&gt;
&lt;br /&gt;
 Hyperbolic: there is only one negative eigenvalue and all the rest are positive, or there is only one positive eigenvalue and all the rest are negative.&lt;br /&gt;
&lt;br /&gt;
双曲形方程: 只有一个负特征值，其余的都是正特征值，或者只有一个正特征值，其余的都是负特征值。&lt;br /&gt;
&lt;br /&gt;
# Ultrahyperbolic: there is more than one positive eigenvalue and more than one negative eigenvalue, and there are no zero eigenvalues. There is only a limited theory for ultrahyperbolic equations (Courant and Hilbert, 1962).&lt;br /&gt;
&lt;br /&gt;
 Ultrahyperbolic: there is more than one positive eigenvalue and more than one negative eigenvalue, and there are no zero eigenvalues. There is only a limited theory for ultrahyperbolic equations (Courant and Hilbert, 1962).&lt;br /&gt;
&lt;br /&gt;
超双形方程: 存在多于一个正特征值和多于一个的负特征值，且不存在零特征值。对于超双曲方程，只存在有限的理论(Courant 和 Hilbert，1962)。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
=== Systems of first-order equations and characteristic surfaces ===&lt;br /&gt;
一阶方程组和特征曲面&lt;br /&gt;
&lt;br /&gt;
The classification of partial differential equations can be extended to systems of first-order equations, where the unknown {{mvar|u}} is now a [[Euclidean vector|vector]] with {{mvar|m}} components, and the coefficient matrices {{mvar|A&amp;lt;sub&amp;gt;ν&amp;lt;/sub&amp;gt;}} are {{mvar|m}} by {{mvar|m}} matrices for {{math|''ν'' {{=}} 1, 2,… ''n''}}. The partial differential equation takes the form&lt;br /&gt;
&lt;br /&gt;
The classification of partial differential equations can be extended to systems of first-order equations, where the unknown  is now a vector with  components, and the coefficient matrices  are  by  matrices for  1, 2,… n}}. The partial differential equation takes the form&lt;br /&gt;
&lt;br /&gt;
偏微分方程的分类可以推广到一阶方程组，其中未知量 {{mvar|u}} 是有 {{mvar|m}} 个分量的向量。对于 {{math|''ν'' {{=}} 1, 2,… ''n''}}，系数矩阵 {{mvar|A&amp;lt;sub&amp;gt;ν&amp;lt;/sub&amp;gt;}} 是 {{mvar|m}} × {{mvar|m}} 的矩阵。偏微分方程形式如下：&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt;Lu = \sum_{\nu=1}^{n} A_\nu \frac{\partial u}{\partial x_\nu} + B=0,&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;Lu = \sum_{\nu=1}^{n} A_\nu \frac{\partial u}{\partial x_\nu} + B=0,&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
where the coefficient matrices {{mvar|A&amp;lt;sub&amp;gt;ν&amp;lt;/sub&amp;gt;}} and the vector {{mvar|B}} may depend upon {{mvar|x}} and {{mvar|u}}. If a [[hypersurface]] {{mvar|S}} is given in the implicit form&lt;br /&gt;
&lt;br /&gt;
where the coefficient matrices  and the vector  may depend upon  and . If a hypersurface  is given in the implicit form&lt;br /&gt;
&lt;br /&gt;
其中，系数矩阵 {{mvar|A&amp;lt;sub&amp;gt;ν&amp;lt;/sub&amp;gt;}} 和向量 {{mvar|B}} 可能依赖于 {{mvar|x}} 和 {{mvar|u}}。如果超曲面是以以下隐式形式给出的，&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt;\varphi(x_1, x_2, \ldots x_n)=0,&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;\varphi(x_1, x_2, \ldots x_n)=0,&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
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where {{mvar|φ}} has a non-zero gradient, then {{mvar|S}} is a '''characteristic surface''' for the operator {{mvar|L}} at a given point if the characteristic form vanishes:&lt;br /&gt;
&lt;br /&gt;
where  has a non-zero gradient, then  is a characteristic surface for the operator  at a given point if the characteristic form vanishes:&lt;br /&gt;
&lt;br /&gt;
其中，存在一个非零的梯度 {{mvar|φ}}，对于在给定点上特征形式消失的算子，特征曲面 {{mvar|S}} 形式如下:&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt;Q\left(\frac{\partial\varphi}{\partial x_1}, \ldots\frac{\partial\varphi}{\partial x_n}\right) =\det\left[\sum_{\nu=1}^nA_\nu \frac{\partial \varphi}{\partial x_\nu}\right]=0.\,&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;Q\left(\frac{\partial\varphi}{\partial x_1}, \ldots\frac{\partial\varphi}{\partial x_n}\right) =\det\left[\sum_{\nu=1}^nA_\nu \frac{\partial \varphi}{\partial x_\nu}\right]=0.\,&amp;lt;/math&amp;gt;&lt;br /&gt;
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The geometric interpretation of this condition is as follows: if data for {{mvar|u}} are prescribed on the surface {{mvar|S}}, then it may be possible to determine the normal derivative of {{mvar|u}} on {{mvar|S}} from the differential equation. If the data on {{mvar|S}} and the differential equation determine the normal derivative of {{mvar|u}} on {{mvar|S}}, then {{mvar|S}} is non-characteristic. If the data on {{mvar|S}} and the differential equation ''do not'' determine the normal derivative of {{mvar|u}} on {{mvar|S}}, then the surface is '''characteristic''', and the differential equation restricts the data on {{mvar|S}}: the differential equation is ''internal'' to {{mvar|S}}.&lt;br /&gt;
&lt;br /&gt;
The geometric interpretation of this condition is as follows: if data for  are prescribed on the surface , then it may be possible to determine the normal derivative of  on  from the differential equation. If the data on  and the differential equation determine the normal derivative of  on , then  is non-characteristic. If the data on  and the differential equation do not determine the normal derivative of  on , then the surface is characteristic, and the differential equation restricts the data on : the differential equation is internal to .&lt;br /&gt;
&lt;br /&gt;
这个条件的几何解释如下: 如果关于 {{mvar|u}} 的数据是在曲面 {{mvar|S}} 上规定的，那么就有可能依据微分方程确定曲面 {{mvar|S}} 上 {{mvar|u}} 的法向导数。如果曲面 {{mvar|S}} 上的数据和上面的微分方程能确定曲面 {{mvar|S}} 上 {{mvar|u}} 的法向导数，那么它就是非特征的。如果曲面 {{mvar|S}} 上的数据和上面的微分方程不能确定曲面 {{mvar|S}} 上 {{mvar|u}} 的法向导数，那么曲面是特征的，并且微分方程将数据限制在曲面 {{mvar|S}} 上：微分方程是在曲面 {{mvar|S}} 内部。&lt;br /&gt;
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# A first-order system {{math|''Lu'' {{=}} 0}} is ''elliptic'' if no surface is characteristic for {{mvar|L}}: the values of {{mvar|u}} on {{mvar|S}} and the differential equation always determine the normal derivative of {{mvar|u}} on {{mvar|S}}.&lt;br /&gt;
&lt;br /&gt;
 A first-order system  0}} is elliptic if no surface is characteristic for : the values of  on  and the differential equation always determine the normal derivative of  on .&lt;br /&gt;
&lt;br /&gt;
如果对于 {{mvar|L}} 没有曲面是特征的，则一阶系统 {{math|''Lu'' {{=}} 0}} 是椭圆形的：{{mvar|u}}在 {{mvar|S}} 的值和微分方程总能够决定 {{mvar|S}} 上 {{mvar|u}} 的法向导数。&lt;br /&gt;
&lt;br /&gt;
# A first-order system is ''hyperbolic'' at a point if there is a '''spacelike''' surface {{mvar|S}} with normal {{mvar|ξ}} at that point. This means that, given any non-trivial vector {{mvar|η}} orthogonal to {{mvar|ξ}}, and a scalar multiplier {{mvar|λ}}, the equation {{math|''Q''(''λξ'' + ''η'') {{=}} 0}} has {{mvar|m}} real roots {{math|''λ''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;, ''λ''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;,… ''λ''&amp;lt;sub&amp;gt;''m''&amp;lt;/sub&amp;gt;}}. The system is '''strictly hyperbolic''' if these roots are always distinct. The geometrical interpretation of this condition is as follows: the characteristic form {{math|''Q''(''ζ'') {{=}} 0}} defines a cone (the normal cone) with homogeneous coordinates ζ. In the hyperbolic case, this cone has {{mvar|m}} sheets, and the axis {{math|''ζ'' {{=}} ''λξ''}} runs inside these sheets: it does not intersect any of them. But when displaced from the origin by η, this axis intersects every sheet. In the elliptic case, the normal cone has no real sheets.&lt;br /&gt;
&lt;br /&gt;
 A first-order system is hyperbolic at a point if there is a spacelike surface  with normal  at that point. This means that, given any non-trivial vector  orthogonal to , and a scalar multiplier , the equation  0}} has  real roots . The system is strictly hyperbolic if these roots are always distinct. The geometrical interpretation of this condition is as follows: the characteristic form  0}} defines a cone (the normal cone) with homogeneous coordinates ζ. In the hyperbolic case, this cone has  sheets, and the axis  λξ}} runs inside these sheets: it does not intersect any of them. But when displaced from the origin by η, this axis intersects every sheet. In the elliptic case, the normal cone has no real sheets.&lt;br /&gt;
&lt;br /&gt;
如果在该点存在一个法向量为 {{mvar|ξ}}的 '''&amp;lt;font color=&amp;quot;#ff8000&amp;quot;&amp;gt;类空曲面 Spacclike Surface&amp;lt;/font&amp;gt; {{mvar|S}} ，则一阶系统在那一点是双曲的。这意味着，给定任意正交于 {{mvar|ξ}} 的非平凡向量 {{mvar|η}} 和一个标量乘子 {{mvar|λ}}，方程 {{math|''Q''(''λξ'' + ''η'') {{=}} 0}} 有 {{mvar|m}} 个实根 {{math|''λ''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;, ''λ''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;,… ''λ''&amp;lt;sub&amp;gt;''m''&amp;lt;/sub&amp;gt;}}。如果这些根始终不同，则该系统是严格双曲形的。这个条件的几何解释如下: 特征形式 {{math|''Q''(''ζ'') {{=}} 0}} 定义了一个具有齐次坐标 ζ的圆锥(法线圆锥)。在双曲形的情况下，这个圆锥体有 {{mvar|m}} 层，并且轴 {{math|''ζ'' {{=}} ''λξ''}} 在这些层中运动: 它不与任何一层相交。但是当从原点偏离η时，这条轴线与每一层都相交。在椭圆形的情况下，法向圆锥没有实层。&lt;br /&gt;
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==[[用户:Yuling|Yuling]]（[[用户讨论:Yuling|讨论]]） sheet 这个单词也不很理解，我直译为了“层”&lt;br /&gt;
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=== Equations of mixed type ===&lt;br /&gt;
混合型方程&lt;br /&gt;
&lt;br /&gt;
If a PDE has coefficients that are not constant, it is possible that it will not belong to any of these categories but rather be of '''mixed type'''. A simple but important example is the [[Euler–Tricomi equation]]&lt;br /&gt;
&lt;br /&gt;
If a PDE has coefficients that are not constant, it is possible that it will not belong to any of these categories but rather be of mixed type. A simple but important example is the Euler–Tricomi equation&lt;br /&gt;
&lt;br /&gt;
如果偏微分方程的系数不是常数，那么它可能不属于这些类别中的任何一个，而是属于混合类型。一个简单但重要的例子是欧拉-特里科米方程&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt;u_{xx} = xu_{yy},&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;u_{xx} = xu_{yy},&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
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which is called '''elliptic-hyperbolic''' because it is elliptic in the region {{math|''x'' &amp;lt; 0}}, hyperbolic in the region {{math|''x'' &amp;gt; 0}}, and degenerate parabolic on the line {{math|''x'' {{=}} 0}}.&lt;br /&gt;
&lt;br /&gt;
which is called elliptic-hyperbolic because it is elliptic in the region , hyperbolic in the region , and degenerate parabolic on the line  0}}.&lt;br /&gt;
&lt;br /&gt;
它在 {{math|''x'' &amp;lt; 0}} 的区域上是椭圆形，在 {{math|''x'' &amp;gt; 0}} 区域上是双曲形，在 {{math|''x'' {{=}} 0}}这条线上是退化为抛物线形，因此称之为椭圆-双曲型。&lt;br /&gt;
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&amp;lt;!--&lt;br /&gt;
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&amp;lt;!--&lt;br /&gt;
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&amp;lt;!--&lt;br /&gt;
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''fill in: Dirichlet and Neumann boundaries, hyperbolic/parabolic/elliptic separation of variables, [[Fourier analysis]], [[Green's function]]s ...--&amp;gt;&lt;br /&gt;
&lt;br /&gt;
fill in: Dirichlet and Neumann boundaries, hyperbolic/parabolic/elliptic separation of variables, Fourier analysis, Green's functions ...--&amp;gt;&lt;br /&gt;
&lt;br /&gt;
填写: Dirichlet 和 Neumann 边界，双曲 / 抛物线 / 椭圆分离变量法，傅立叶分析，Green 函数... --&lt;br /&gt;
&lt;br /&gt;
=== Infinite-order PDEs in quantum mechanics ===&lt;br /&gt;
量子力学中的无限阶偏微分方程&lt;br /&gt;
&lt;br /&gt;
In the [[phase space formulation]] of quantum mechanics,  one may consider the [[Method of quantum characteristics|quantum Hamilton's equations]] for trajectories of quantum particles. These equations are infinite-order PDEs. However, in the semiclassical expansion, one has a finite system of ODEs at any fixed order of [[Dirac constant|{{mvar|ħ}}]].  The evolution equation of the [[Wigner quasi-probability distribution|c]] is also an infinite-order PDE. The quantum trajectories are [[Method of quantum characteristics|quantum characteristics]], with the use of which one could calculate the evolution of the Wigner function.&lt;br /&gt;
&lt;br /&gt;
In the phase space formulation of quantum mechanics,  one may consider the quantum Hamilton's equations for trajectories of quantum particles. These equations are infinite-order PDEs. However, in the semiclassical expansion, one has a finite system of ODEs at any fixed order of Dirac constant|.  The evolution equation of the Wigner function is also an infinite-order PDE. The quantum trajectories are quantum characteristics, with the use of which one could calculate the evolution of the Wigner function.&lt;br /&gt;
&lt;br /&gt;
在量子力学中的相空间表述中，我们可以考虑用于求解量子粒子的轨迹的量子哈密顿的方程。这些方程是无限阶偏微分方程。然而，在半经典展开中，我们在给定[[Dirac constant|{{mvar|ħ}}]]阶数下有一个有限的的常微分方程组。'''&amp;lt;font color=&amp;quot;#ff8000&amp;quot;&amp;gt;维格纳函数  Wigner Function&amp;lt;/font&amp;gt;的演化方程也是一个无限阶偏微分方程。由于量子轨道的量子特性，所以它通常可以用来计算维格纳函数的演化。&lt;br /&gt;
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== Analytical solutions ==&lt;br /&gt;
解析解&lt;br /&gt;
&lt;br /&gt;
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===Separation of variables===&lt;br /&gt;
分离变量法&lt;br /&gt;
&lt;br /&gt;
{{main|Separable partial differential equation}}&lt;br /&gt;
&lt;br /&gt;
Linear PDEs can be reduced to systems of ordinary differential equations by the important technique of separation of variables. This technique rests on a characteristic of solutions to differential equations: if one can find any solution that solves the equation and satisfies the boundary conditions, then it is ''the'' solution (this also applies to ODEs). We assume as an [[ansatz]] that the dependence of a solution on the parameters space and time can be written as a product of terms that each depend on a single parameter, and then see if this can be made to solve the problem.&amp;lt;ref&amp;gt;{{cite book|last1=Gershenfeld|first1=Neil|title=The nature of mathematical modeling|date=2000|publisher=Cambridge Univ. Press|location=Cambridge|isbn=0521570956|page=27|edition=Reprinted (with corr.)}}&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
Linear PDEs can be reduced to systems of ordinary differential equations by the important technique of separation of variables. This technique rests on a characteristic of solutions to differential equations: if one can find any solution that solves the equation and satisfies the boundary conditions, then it is the solution (this also applies to ODEs). We assume as an ansatz that the dependence of a solution on the parameters space and time can be written as a product of terms that each depend on a single parameter, and then see if this can be made to solve the problem.&lt;br /&gt;
&lt;br /&gt;
线性偏微分方程组可以通过分离变量法这一重要方法来简化为常微分方程组。这种方法依赖于微分方程解的一个特征: 如果能找到任何一个满足方程和边界条件的解，那么这个解就是方程的解(这也适用于常微分方程)。我们假设解对参数空间和时间的依赖可以写成对它们每一项的依赖以及一个参数的乘积，然后再看看这是否可以用来解决这个问题。&lt;br /&gt;
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In the method of separation of variables, one reduces a PDE to a PDE in fewer variables, which is an ordinary differential equation if in one variable – these are in turn easier to solve.&lt;br /&gt;
&lt;br /&gt;
In the method of separation of variables, one reduces a PDE to a PDE in fewer variables, which is an ordinary differential equation if in one variable – these are in turn easier to solve.&lt;br /&gt;
&lt;br /&gt;
在分离变量法方法中，可以将偏微分方程简化为含有更少变量的偏微分方程，如果只有一个变量，那么就变成了一个'''&amp;lt;font color = &amp;quot;#ff8000&amp;quot;&amp;gt;常微分方程 Ordinary Differential Equation&amp;lt;/font&amp;gt;'''-- 反过来，这些方程也更容易求解。&lt;br /&gt;
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This is possible for simple PDEs, which are called [[separable partial differential equation]]s, and the domain is generally a rectangle (a product of intervals). Separable PDEs correspond to [[diagonal matrices]] – thinking of &amp;quot;the value for fixed {{mvar|x}}&amp;quot; as a coordinate, each coordinate can be understood separately.&lt;br /&gt;
&lt;br /&gt;
This is possible for simple PDEs, which are called separable partial differential equations, and the domain is generally a rectangle (a product of intervals). Separable PDEs correspond to diagonal matrices – thinking of &amp;quot;the value for fixed &amp;quot; as a coordinate, each coordinate can be understood separately.&lt;br /&gt;
&lt;br /&gt;
对于简单的偏微分方程(称为可分离偏微分方程)来说，这是可能的，而且方程通常定义在一个矩形区域(区间的乘积)上。可分离偏微分方程对应于对角线矩阵——以“固定值”为坐标，每个坐标可分开理解。&lt;br /&gt;
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This generalizes to the [[method of characteristics]], and is also used in [[integral transform]]s.&lt;br /&gt;
&lt;br /&gt;
This generalizes to the method of characteristics, and is also used in integral transforms.&lt;br /&gt;
&lt;br /&gt;
这种方法可以推广到特征曲线法，也可以用于积分变换。&lt;br /&gt;
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===Method of characteristics===&lt;br /&gt;
特征曲线法&lt;br /&gt;
&lt;br /&gt;
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{{main|Method of characteristics}}&lt;br /&gt;
&lt;br /&gt;
In special cases, one can find characteristic curves on which the equation reduces to an ODE – changing coordinates in the domain to straighten these curves allows separation of variables, and is called the [[method of characteristics]].&lt;br /&gt;
&lt;br /&gt;
In special cases, one can find characteristic curves on which the equation reduces to an ODE – changing coordinates in the domain to straighten these curves allows separation of variables, and is called the method of characteristics.&lt;br /&gt;
&lt;br /&gt;
在特殊情况下，可以找到一些特征曲线，在这些曲线上方程可以变成一个常微分方程——意味着改变坐标从而使这些曲线变直从而达到分离变量的目的，这就是所谓的特征曲线法。&lt;br /&gt;
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More generally, one may find characteristic surfaces.&lt;br /&gt;
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More generally, one may find characteristic surfaces.&lt;br /&gt;
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更一般地说，人们可能会找到特征表面。&lt;br /&gt;
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===Integral transform===&lt;br /&gt;
积分变换&lt;br /&gt;
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An [[integral transform]] may transform the PDE to a simpler one, in particular, a separable PDE. This corresponds to diagonalizing an operator.&lt;br /&gt;
&lt;br /&gt;
An integral transform may transform the PDE to a simpler one, in particular, a separable PDE. This corresponds to diagonalizing an operator.&lt;br /&gt;
&lt;br /&gt;
积分变换可以将偏微分方程转换为更简单的偏微分方程，特别是可分离的偏微分方程。这对应于对角化算符。&lt;br /&gt;
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An important example of this is [[Fourier analysis]], which diagonalizes the heat equation using the [[eigenbasis]] of sinusoidal waves.&lt;br /&gt;
&lt;br /&gt;
An important example of this is Fourier analysis, which diagonalizes the heat equation using the eigenbasis of sinusoidal waves.&lt;br /&gt;
&lt;br /&gt;
这方面的一个重要例子是'''&amp;lt;font color = &amp;quot;#ff8000&amp;quot;&amp;gt;傅里叶分析  Fourier Analysis&amp;lt;/font&amp;gt;'''，它使用正弦波的特征基来对角化热方程。&lt;br /&gt;
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If the domain is finite or periodic, an infinite sum of solutions such as a [[Fourier series]] is appropriate, but an integral of solutions such as a [[Fourier integral]] is generally required for infinite domains. The solution for a point source for the heat equation given above is an example of the use of a Fourier integral.&lt;br /&gt;
&lt;br /&gt;
If the domain is finite or periodic, an infinite sum of solutions such as a Fourier series is appropriate, but an integral of solutions such as a Fourier integral is generally required for infinite domains. The solution for a point source for the heat equation given above is an example of the use of a Fourier integral.&lt;br /&gt;
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如果区域是有限的或周期性的，那么解为无限和的形式是恰当的，例如傅里叶级数，但是一个解的积分，例如傅立叶积分，一般是在无限区域上的。上面给出的热传导方程的点源解法就是使用傅里叶积分的一个例子。&lt;br /&gt;
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===Change of variables===&lt;br /&gt;
变量代换&lt;br /&gt;
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Often a PDE can be reduced to a simpler form with a known solution by a suitable [[Change of variables (PDE)|change of variables]].  For example, the [[Black–Scholes equation#Derivation|Black–Scholes]] PDE&lt;br /&gt;
&lt;br /&gt;
Often a PDE can be reduced to a simpler form with a known solution by a suitable change of variables.  For example, the Black–Scholes PDE&lt;br /&gt;
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偏微分方程通常可以通过变量的适当变化，用已知的解简化为更简单的形式。例如，布莱克-舒尔斯偏微分方程&lt;br /&gt;
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:&amp;lt;math&amp;gt; \frac{\partial V}{\partial t} + \tfrac{1}{2}\sigma^2 S^2\frac{\partial^2 V}{\partial S^2} + rS\frac{\partial V}{\partial S} - rV = 0 &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \frac{\partial V}{\partial t} + \tfrac{1}{2}\sigma^2 S^2\frac{\partial^2 V}{\partial S^2} + rS\frac{\partial V}{\partial S} - rV = 0 &amp;lt;/math&amp;gt;&lt;br /&gt;
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is reducible to the [[heat equation]]&lt;br /&gt;
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is reducible to the heat equation&lt;br /&gt;
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可以简化为热传导方程&lt;br /&gt;
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:&amp;lt;math&amp;gt; \frac{\partial u}{\partial \tau} = \frac{\partial^2 u}{\partial x^2}&amp;lt;/math&amp;gt;&lt;br /&gt;
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&amp;lt;math&amp;gt; \frac{\partial u}{\partial \tau} = \frac{\partial^2 u}{\partial x^2}&amp;lt;/math&amp;gt;&lt;br /&gt;
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by the change of variables (for complete details see {{webarchive |url=https://web.archive.org/web/20080411030405/http://www.math.unl.edu/~sdunbar1/Teaching/MathematicalFinance/Lessons/BlackScholes/Solution/solution.shtml |date=April 11, 2008 |title=Solution of the Black Scholes Equation }})&lt;br /&gt;
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by the change of variables (for complete details see )&lt;br /&gt;
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通过变量替换(完整的细节见)&lt;br /&gt;
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:&amp;lt;math&amp;gt;\begin{align}&lt;br /&gt;
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V(S,t) &amp;amp;= K v(x,\tau),\\[5px]&lt;br /&gt;
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x &amp;amp;= \ln\left(\tfrac{S}{K} \right),\\[5px]&lt;br /&gt;
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\tau &amp;amp;= \tfrac{1}{2} \sigma^2 (T - t),\\[5px]&lt;br /&gt;
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v(x,\tau)&amp;amp;=e^{-\alpha x-\beta\tau} u(x,\tau).&lt;br /&gt;
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\end{align}&amp;lt;/math&amp;gt;&lt;br /&gt;
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===Fundamental solution===&lt;br /&gt;
基本解&lt;br /&gt;
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{{main|Fundamental solution}}&lt;br /&gt;
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Inhomogeneous equations can often be solved (for constant coefficient PDEs, always be solved) by finding the [[fundamental solution]] (the solution for a point source), then taking the [[convolution]] with the boundary conditions to get the solution.&lt;br /&gt;
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Inhomogeneous equations can often be solved (for constant coefficient PDEs, always be solved) by finding the fundamental solution (the solution for a point source), then taking the convolution with the boundary conditions to get the solution.&lt;br /&gt;
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非齐次方程(常系数偏微分方程)一般是通过先求出基本解(点源的解) ，然后利用带边界条件的卷积来求解。&lt;br /&gt;
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This is analogous in [[signal processing]] to understanding a filter by its [[impulse response]].&lt;br /&gt;
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This is analogous in signal processing to understanding a filter by its impulse response.&lt;br /&gt;
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这类似于在信号处理中通过滤波器的脉冲响应来理解滤波器。&lt;br /&gt;
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===Superposition principle===&lt;br /&gt;
叠加原理&lt;br /&gt;
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{{further| Superposition principle }}&lt;br /&gt;
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The superposition principle applies to any linear system, including linear systems of PDEs. A common visualization of this concept is the interaction of two waves in phase being combined to result in a greater amplitude, for example {{math|sin ''x'' + sin ''x'' {{=}} 2 sin ''x''}}. The same principle can be observed in PDEs where the solutions may be real or complex and additive. [[Superposition principle|superposition]]&lt;br /&gt;
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The superposition principle applies to any linear system, including linear systems of PDEs. A common visualization of this concept is the interaction of two waves in phase being combined to result in a greater amplitude, for example  2 sin x}}. The same principle can be observed in PDEs where the solutions may be real or complex and additive. superposition&lt;br /&gt;
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'''&amp;lt;font color = &amp;quot;#ff8000&amp;quot;&amp;gt;叠加原理 Superposition Principle&amp;lt;/font&amp;gt;适用于任何线性系统，包括偏微分方程的线性系统。这个概念的一个常见的可视化是两个同相位的波相互作用结合在一起会产生更大的振幅，例如 {{math|sin ''x'' + sin ''x'' {{=}} 2 sin ''x''}}。在偏微分方程中也可以观察到同样的原理，其中的解可能是真实的或复杂的和可加的。叠加&lt;br /&gt;
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If {{math|''u''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;}} and {{math|''u''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;}} are solutions of linear PDE in some function space {{mvar|R}}, then {{math|''u'' {{=}} ''c''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;''u''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; + ''c''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;''u''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;}} with any constants {{math|''c''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;}} and {{math|''c''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;}} are also a solution of that PDE in the same function space.&lt;br /&gt;
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If  and  are solutions of linear PDE in some function space , then  c&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;u&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; + c&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;u&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;}} with any constants  and  are also a solution of that PDE in the same function space.&lt;br /&gt;
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若线性偏微分方程在某个函数空间{{mvar|R}}中有解{{math|''u''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;}} 和 {{math|''u''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;}}，则{{math|''u'' {{=}} ''c''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;''u''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; + ''c''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;''u''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;}}也是该偏微分方程在同一函数空间中的解，其中{{math|''c''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;}} 和 {{math|''c''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;}} 是任意常数。&lt;br /&gt;
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===Methods for non-linear equations===&lt;br /&gt;
非线性方程的求解方法&lt;br /&gt;
{{see also|nonlinear partial differential equation}}&lt;br /&gt;
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There are no generally applicable methods to solve nonlinear PDEs. Still, existence and uniqueness results (such as the [[Cauchy–Kowalevski theorem]]) are often possible, as are proofs of important qualitative and quantitative properties of solutions (getting these results is a major part of [[mathematical analysis|analysis]]). Computational solution to the nonlinear PDEs, the [[split-step method]], exist for specific equations like [[nonlinear Schrödinger equation]].&lt;br /&gt;
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There are no generally applicable methods to solve nonlinear PDEs. Still, existence and uniqueness results (such as the Cauchy–Kowalevski theorem) are often possible, as are proofs of important qualitative and quantitative properties of solutions (getting these results is a major part of analysis). Computational solution to the nonlinear PDEs, the split-step method, exist for specific equations like nonlinear Schrödinger equation.&lt;br /&gt;
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对于非线性偏微分方程，目前还没有普遍适用的求解方法。然而，通常是可能知道解的存在性和唯一性(如柯西-科瓦列夫斯基定理)，也是可能得到解的重要定性和定量性质的证明(得到这些结果是分析的主要部分)。非线性偏微分方程的计算解，即分步法，对一些特定的方程适用，比如非线性'''&amp;lt;font color=&amp;quot;#ff8000&amp;quot;&amp;gt;薛定谔方程 Schrödinger equation&amp;lt;/font&amp;gt;'''。&lt;br /&gt;
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Nevertheless, some techniques can be used for several types of equations. The [[h-principle|{{mvar|h}}-principle]] is the most powerful method to solve [[Underdetermined system|underdetermined]] equations. The [[Riquier–Janet theory]] is an effective method for obtaining information about many analytic [[Overdetermined system|overdetermined]] systems.&lt;br /&gt;
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Nevertheless, some techniques can be used for several types of equations. The -principle is the most powerful method to solve underdetermined equations. The Riquier–Janet theory is an effective method for obtaining information about many analytic overdetermined systems.&lt;br /&gt;
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然而，一些技巧可以用于几种类型的方程。h-原理是求解欠定方程最有效的方法。里基尔-珍妮特理论是一种可以获得许多解析超定系统信息的有效方法。&lt;br /&gt;
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The [[method of characteristics]] can be used in some very special cases to solve partial differential equations.&lt;br /&gt;
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The method of characteristics can be used in some very special cases to solve partial differential equations.&lt;br /&gt;
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特征线法可用于求解某些特殊情况下的偏微分方程。&lt;br /&gt;
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In some cases, a PDE can be solved via [[perturbation analysis]] in which the solution is considered to be a correction to an equation with a known solution. Alternatives are [[numerical analysis]] techniques from simple [[finite difference]] schemes to the more mature [[multigrid]] and [[finite element method]]s. Many interesting problems in science and engineering are solved in this way using [[computer]]s, sometimes high performance [[supercomputer]]s.&lt;br /&gt;
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In some cases, a PDE can be solved via perturbation analysis in which the solution is considered to be a correction to an equation with a known solution. Alternatives are numerical analysis techniques from simple finite difference schemes to the more mature multigrid and finite element methods. Many interesting problems in science and engineering are solved in this way using computers, sometimes high performance supercomputers.&lt;br /&gt;
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在某些情况下，偏微分方程可以通过扰动分析来求解。在扰动分析中，通常是求解将具有已知解的方程修正后的新得到方程。可供选择的数值分析技术从简单的差分格式到更成熟的多重网格和有限元方法。许多有趣的科学和工程问题都是在计算机上用这种方法解决的，有时是高性能超级计算机。&lt;br /&gt;
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===Lie group method===&lt;br /&gt;
李群方法&lt;br /&gt;
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From 1870 [[Sophus Lie]]'s work put the theory of differential equations on a more satisfactory foundation. He showed that the integration theories of the older mathematicians can, by the introduction of what are now called [[Lie group]]s, be referred, to a common source; and that ordinary differential equations which admit the same [[infinitesimal transformation]]s present comparable difficulties of integration. He also emphasized the subject of [[contact transformation|transformations of contact]].&lt;br /&gt;
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From 1870 Sophus Lie's work put the theory of differential equations on a more satisfactory foundation. He showed that the integration theories of the older mathematicians can, by the introduction of what are now called Lie groups, be referred, to a common source; and that ordinary differential equations which admit the same infinitesimal transformations present comparable difficulties of integration. He also emphasized the subject of transformations of contact.&lt;br /&gt;
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从1870年起，索弗斯·李的工作为微分方程理论奠定了一个较为令人满意的基础。他指出，通过引入现在所谓的李群，老一辈数学家的积分理论可以引用到一个共同的来源; 承认相同的无穷小变换的常微分方程在积分方面存在相当的困难。他还强调了接触的转变这一主题。&lt;br /&gt;
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==[[用户:Yuling|Yuling]]（[[用户讨论:Yuling|讨论]]）这句话“He also emphasized the subject of transformations of contact.”中的transformations of contact翻译的不太好。&lt;br /&gt;
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A general approach to solving PDEs uses the symmetry property of differential equations, the continuous [[infinitesimal transformation]]s of solutions to solutions ([[Lie theory]]). Continuous [[group theory]], [[Lie algebras]] and [[differential geometry]] are used to understand the structure of linear and nonlinear partial differential equations for generating integrable equations, to find its [[Lax pair]]s, recursion operators, [[Bäcklund transform]] and finally finding exact analytic solutions to the PDE.&lt;br /&gt;
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A general approach to solving PDEs uses the symmetry property of differential equations, the continuous infinitesimal transformations of solutions to solutions (Lie theory). Continuous group theory, Lie algebras and differential geometry are used to understand the structure of linear and nonlinear partial differential equations for generating integrable equations, to find its Lax pairs, recursion operators, Bäcklund transform and finally finding exact analytic solutions to the PDE.&lt;br /&gt;
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求解偏微分方程的一般方法是利用微分方程的对称性，即解到解的连续无穷小变换(李理论)。连续群论、李代数和微分几何理论被用来理解生成可积方程的线性和非线性偏微分方程的结构，找到它的Lax对、递归算子、 贝克伦德变换，最后找到偏微分方程的精确解析解。&lt;br /&gt;
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Symmetry methods have been recognized to study differential equations arising in mathematics, physics, engineering, and many other disciplines.&lt;br /&gt;
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Symmetry methods have been recognized to study differential equations arising in mathematics, physics, engineering, and many other disciplines.&lt;br /&gt;
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对称方法已被公认可以用于研究出现在数学，物理，工程和许多其他学科的微分方程。&lt;br /&gt;
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===Semianalytical methods===&lt;br /&gt;
半解析方法&lt;br /&gt;
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The [[Adomian decomposition method]], the [[Aleksandr Lyapunov|Lyapunov]] artificial small parameter method, and He's [[homotopy perturbation method]] are all special cases of the more general [[homotopy analysis method]]. These are series expansion methods, and except for the Lyapunov method, are independent of small physical parameters as compared to the well known [[perturbation theory]], thus giving these methods greater flexibility and solution generality.&lt;br /&gt;
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The Adomian decomposition method, the Lyapunov artificial small parameter method, and He's homotopy perturbation method are all special cases of the more general homotopy analysis method. These are series expansion methods, and except for the Lyapunov method, are independent of small physical parameters as compared to the well known perturbation theory, thus giving these methods greater flexibility and solution generality.&lt;br /&gt;
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阿多米安分解法、李雅普诺夫人工小参数方法和何同伦摄动方法都是更一般的同伦分析方法的特殊情况。除了李雅普诺夫方法之外，这些都是级数展开方法，与为人熟知的摄动理论方法相比，它们与小的物理参数无关，因此这些方法具有更大的灵活性和解的通用性。&lt;br /&gt;
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== Numerical solutions ==&lt;br /&gt;
数值解&lt;br /&gt;
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The three most widely used [[Numerical partial differential equations|numerical methods to solve PDEs]] are the [[finite element analysis|finite element method]] (FEM), [[finite volume method]]s (FVM) and [[finite difference method]]s (FDM), as well other kind of methods called [[Meshfree methods]], which were made to solve problems where the before mentioned methods are limited. The FEM has a prominent position among these methods and especially its exceptionally efficient higher-order version [[hp-FEM]]. Other hybrid versions of FEM and Meshfree methods include the generalized finite element method (GFEM), [[extended finite element method]] (XFEM), [[Spectral element method|spectral finite element method]] (SFEM), [[Meshfree methods|meshfree finite element method]], [[Discontinuous Galerkin Method|discontinuous Galerkin finite element method]] (DGFEM), [[Element-Free Galerkin Method]] (EFGM), [[Interpolating Element-Free Galerkin Method]] (IEFGM), etc.&lt;br /&gt;
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The three most widely used numerical methods to solve PDEs are the finite element method (FEM), finite volume methods (FVM) and finite difference methods (FDM), as well other kind of methods called Meshfree methods, which were made to solve problems where the before mentioned methods are limited. The FEM has a prominent position among these methods and especially its exceptionally efficient higher-order version hp-FEM. Other hybrid versions of FEM and Meshfree methods include the generalized finite element method (GFEM), extended finite element method (XFEM), spectral finite element method (SFEM), meshfree finite element method, discontinuous Galerkin finite element method (DGFEM), Element-Free Galerkin Method (EFGM), Interpolating Element-Free Galerkin Method (IEFGM), etc.&lt;br /&gt;
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求解偏微分方程最常用的三种数值方法是有限元分析法、有限体积法和有限差分法，以及其他一些称为无网格法的方法。这些方法用于解决前面提到的方法受到的限制。在这些方法中，有限元方法，尤其是高效的高阶有限元方法，占有重要地位。其他有限元法和无网格法的混合形式包括广义有限元分析法(GFEM)、扩展有限元分析法(XFEM)、谱有限元分析法(SFEM)、无网格有限元分析法(DGFEM)、间断伽辽金有限元分析法(DGFEM)、无网格伽辽金法(EFGM)、插值无网格伽辽金法(IEFGM)等。&lt;br /&gt;
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=== Finite element method ===&lt;br /&gt;
有限元分析法&lt;br /&gt;
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{{main|Finite element method}}&lt;br /&gt;
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The finite element method (FEM) (its practical application often known as finite element analysis (FEA)) is a numerical technique for finding approximate solutions of partial differential equations (PDE) as well as of integral equations. The solution approach is based either on eliminating the differential equation completely (steady state problems), or rendering the PDE into an approximating system of ordinary differential equations, which are then numerically integrated using standard techniques such as Euler's method, Runge–Kutta, etc.&lt;br /&gt;
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The finite element method (FEM) (its practical application often known as finite element analysis (FEA)) is a numerical technique for finding approximate solutions of partial differential equations (PDE) as well as of integral equations. The solution approach is based either on eliminating the differential equation completely (steady state problems), or rendering the PDE into an approximating system of ordinary differential equations, which are then numerically integrated using standard techniques such as Euler's method, Runge–Kutta, etc.&lt;br /&gt;
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'''&amp;lt;font color = &amp;quot;#ff8000&amp;quot;&amp;gt;有限元分析法 Finite Element Method&amp;lt;/font&amp;gt;''' ((其实际应用通常被称为有限元分析(FEA))是一种寻找偏微分方程(PDE)和积分方程近似解的数值技术。这种求解方法要么基于完全消除微分方程(稳态问题) ，要么将偏微分方程转化为常微分方程的近似系统，然后使用标准技术进行数值积分，如欧拉方法、 Runge-Kutta 等。&lt;br /&gt;
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===Finite difference method===&lt;br /&gt;
有限差分法&lt;br /&gt;
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{{main|Finite difference method}}&lt;br /&gt;
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Finite-difference methods are numerical methods for approximating the solutions to differential equations using [[finite difference]] equations to approximate derivatives.&lt;br /&gt;
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Finite-difference methods are numerical methods for approximating the solutions to differential equations using finite difference equations to approximate derivatives.&lt;br /&gt;
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有限差分法是一种数值方法，用差分方程近似微分方程的解。&lt;br /&gt;
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=== Finite volume method ===&lt;br /&gt;
有限体积法&lt;br /&gt;
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{{main|Finite volume method}}&lt;br /&gt;
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Similar to the finite difference method or finite element method, values are calculated at discrete places on a meshed geometry. &amp;quot;Finite volume&amp;quot; refers to the small volume surrounding each node point on a mesh. In the finite volume method, surface integrals in a partial differential equation that contain a divergence term are converted to volume integrals, using the [[divergence theorem]]. These terms are then evaluated as fluxes at the surfaces of each finite volume. Because the flux entering a given volume is identical to that leaving the adjacent volume, these methods conserve mass by design.&lt;br /&gt;
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Similar to the finite difference method or finite element method, values are calculated at discrete places on a meshed geometry. &amp;quot;Finite volume&amp;quot; refers to the small volume surrounding each node point on a mesh. In the finite volume method, surface integrals in a partial differential equation that contain a divergence term are converted to volume integrals, using the divergence theorem. These terms are then evaluated as fluxes at the surfaces of each finite volume. Because the flux entering a given volume is identical to that leaving the adjacent volume, these methods conserve mass by design.&lt;br /&gt;
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类似于有限差分法或有限元分析，函数值是在网状几何体上的离散位置进行计算的。“有限体积”是指网格上每个节点周围的小体积。在有限体积法中，偏微分方程中含有散度项的面积分用散度定理积分转换成体积分。然后将这些项用于估算每个有限体积表面上的通量。由于进入给定体积的通量与转移到相邻体积元的通量相同，所以这些方法在设计上保证了质量守恒。&lt;br /&gt;
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==See also==&lt;br /&gt;
请参阅&lt;br /&gt;
* [[Dirichlet boundary condition]]&lt;br /&gt;
狄利克雷边界条件&lt;br /&gt;
* [[Jet bundle]]&lt;br /&gt;
射流丛&lt;br /&gt;
* [[Laplace transform applied to differential equations]]&lt;br /&gt;
微分方程中的拉普拉斯变换&lt;br /&gt;
* [[List of dynamical systems and differential equations topics]]&lt;br /&gt;
动力学系统列表和微分方程主题&lt;br /&gt;
* [[Matrix differential equation]]&lt;br /&gt;
矩阵微分方程&lt;br /&gt;
* [[Neumann boundary condition]]&lt;br /&gt;
诺伊曼边界条件&lt;br /&gt;
* [[Numerical partial differential equations]]&lt;br /&gt;
数值偏微分方程&lt;br /&gt;
* [[Partial differential algebraic equation]]&lt;br /&gt;
偏微分代数方程&lt;br /&gt;
* [[Recurrence relation]]&lt;br /&gt;
递推关系&lt;br /&gt;
* [[Robin boundary condition]]&lt;br /&gt;
罗宾边界条件&lt;br /&gt;
* [[Stochastic processes and boundary value problems]]&lt;br /&gt;
随机过程和边值问题&lt;br /&gt;
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== The energy method ==&lt;br /&gt;
能量法&lt;br /&gt;
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The energy method is a mathematical procedure that can be used to verify well-posedness of initial-boundary-value-problems.&amp;lt;ref&amp;gt;{{cite book |title=High Order Difference Methods for Time Dependent PDE&lt;br /&gt;
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The energy method is a mathematical procedure that can be used to verify well-posedness of initial-boundary-value-problems.&amp;lt;ref&amp;gt;{{cite book |title=High Order Difference Methods for Time Dependent PDE&lt;br /&gt;
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能量法是一种数学过程，可用于验证初始边界值问题的适定性。&lt;br /&gt;
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In the following example the energy method is used to decide where and which boundary conditions should be imposed such that the resulting IBVP is well-posed. Consider the one-dimensional hyperbolic PDE given by&lt;br /&gt;
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In the following example the energy method is used to decide where and which boundary conditions should be imposed such that the resulting IBVP is well-posed. Consider the one-dimensional hyperbolic PDE given by&lt;br /&gt;
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在下面的示例中，将使用能量法决定应在何处施加哪些边界条件，以使得到的IBVP处于适当位置。考虑下式给出的一维双曲PDE&lt;br /&gt;
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: &amp;lt;math&amp;gt;\frac{\partial u}{\partial t} + \alpha \frac{\partial u}{\partial x} = 0, \quad x \in [a,b], \operatorname t &amp;gt; 0,&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;\frac{\partial u}{\partial t} + \alpha \frac{\partial u}{\partial x} = 0, \quad x \in [a,b], \operatorname t &amp;gt; 0,&amp;lt;/math&amp;gt;&lt;br /&gt;
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where &amp;lt;math&amp;gt;\alpha \neq 0&amp;lt;/math&amp;gt; is a constant and &amp;lt;math&amp;gt;u(x,t)&amp;lt;/math&amp;gt; is an unknown function with initial condition &amp;lt;math&amp;gt;u(x,0) = f(x)&amp;lt;/math&amp;gt;. Multiplying with &amp;lt;math&amp;gt;u&amp;lt;/math&amp;gt; and integrating over the domain gives&lt;br /&gt;
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where &amp;lt;math&amp;gt;\alpha \neq 0&amp;lt;/math&amp;gt; is a constant and &amp;lt;math&amp;gt;u(x,t)&amp;lt;/math&amp;gt; is an unknown function with initial condition &amp;lt;math&amp;gt;u(x,0) = f(x)&amp;lt;/math&amp;gt;. Multiplying with &amp;lt;math&amp;gt;u&amp;lt;/math&amp;gt; and integrating over the domain gives&lt;br /&gt;
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其中 &amp;lt;math&amp;gt;\alpha \neq 0&amp;lt;/math&amp;gt; 是常数，并且 &amp;lt;math&amp;gt;u(x,t)&amp;lt;/math&amp;gt; 是初始条件是 &amp;lt;math&amp;gt;u(x,0) = f(x)&amp;lt;/math&amp;gt;的未知函数，乘以 &amp;lt;math&amp;gt;u&amp;lt;/math&amp;gt; 并在域上进行积分。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt;\int_a^b u \frac{\partial u}{\partial t} \operatorname dx + \alpha \int _a ^b u \frac{\partial u}{\partial x} \operatorname dx = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;\int_a^b u \frac{\partial u}{\partial t} \operatorname dx + \alpha \int _a ^b u \frac{\partial u}{\partial x} \operatorname dx = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Using that&lt;br /&gt;
&lt;br /&gt;
Using that&lt;br /&gt;
&lt;br /&gt;
利用这一点&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt;\int _a ^b u \frac{\partial u}{\partial t} \operatorname dx = \frac{1}{2} \frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 \quad \text{and} \quad \int _a ^b u \frac{\partial u}{\partial x} \operatorname dx = \frac{1}{2} u(b,t)^2 - \frac{1}{2} u(a,t)^2,.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;\int _a ^b u \frac{\partial u}{\partial t} \operatorname dx = \frac{1}{2} \frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 \quad \text{and} \quad \int _a ^b u \frac{\partial u}{\partial x} \operatorname dx = \frac{1}{2} u(b,t)^2 - \frac{1}{2} u(a,t)^2,.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
where integration by parts has been used for the second relationship, we get&lt;br /&gt;
&lt;br /&gt;
where integration by parts has been used for the second relationship, we get&lt;br /&gt;
&lt;br /&gt;
第二个关系中采用了分部积分法，我们可以得到&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt;\frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 + \alpha u(b,t)^2 - \alpha u(a,t)^2 = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;\frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 + \alpha u(b,t)^2 - \alpha u(a,t)^2 = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Here &amp;lt;math&amp;gt;\vert \vert \cdot \vert \vert&amp;lt;/math&amp;gt; denotes the standard L2-norm.&lt;br /&gt;
&lt;br /&gt;
Here &amp;lt;math&amp;gt;\vert \vert \cdot \vert \vert&amp;lt;/math&amp;gt; denotes the standard L2-norm.&lt;br /&gt;
&lt;br /&gt;
在这里，&amp;lt;math&amp;gt;\vert \vert \cdot \vert \vert&amp;lt;/math&amp;gt; 表示标准的L2-正则。&lt;br /&gt;
&lt;br /&gt;
For well-posedness we require that the energy of the solution is non-increasing, i.e. that &amp;lt;math&amp;gt;\frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 \leq 0&amp;lt;/math&amp;gt;, which is achieved by specifying &amp;lt;math&amp;gt;u&amp;lt;/math&amp;gt; at &amp;lt;math&amp;gt;x = a&amp;lt;/math&amp;gt; if &amp;lt;math&amp;gt;\alpha &amp;gt; 0&amp;lt;/math&amp;gt; and at &amp;lt;math&amp;gt;x = b&amp;lt;/math&amp;gt; if &amp;lt;math&amp;gt;\alpha &amp;lt; 0&amp;lt;/math&amp;gt;. This corresponds to only imposing boundary conditions at the inflow. Note that well-posedness allows for growth in terms of data (initial and boundary) and thus it is sufficient to show that &amp;lt;math&amp;gt;\frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 \leq 0&amp;lt;/math&amp;gt; holds when all data is set to zero.&lt;br /&gt;
&lt;br /&gt;
For well-posedness we require that the energy of the solution is non-increasing, i.e. that &amp;lt;math&amp;gt;\frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 \leq 0&amp;lt;/math&amp;gt;, which is achieved by specifying &amp;lt;math&amp;gt;u&amp;lt;/math&amp;gt; at &amp;lt;math&amp;gt;x = a&amp;lt;/math&amp;gt; if &amp;lt;math&amp;gt;\alpha &amp;gt; 0&amp;lt;/math&amp;gt; and at &amp;lt;math&amp;gt;x = b&amp;lt;/math&amp;gt; if &amp;lt;math&amp;gt;\alpha &amp;lt; 0&amp;lt;/math&amp;gt;. This corresponds to only imposing boundary conditions at the inflow. Note that well-posedness allows for growth in terms of data (initial and boundary) and thus it is sufficient to show that &amp;lt;math&amp;gt;\frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 \leq 0&amp;lt;/math&amp;gt; holds when all data is set to zero.&lt;br /&gt;
&lt;br /&gt;
对于适定性，我们要求解的能量是不增加的，即 &amp;lt;math&amp;gt;\frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 \leq 0&amp;lt;/math&amp;gt; ，这种关系可以通过在&amp;lt;math&amp;gt;x = a&amp;lt;/math&amp;gt;处 （如果 &amp;lt;math&amp;gt;\alpha &amp;gt; 0&amp;lt;/math&amp;gt;） 以及 &amp;lt;math&amp;gt;x = b&amp;lt;/math&amp;gt;处 （如果 &amp;lt;math&amp;gt;\alpha &amp;lt; 0&amp;lt;/math&amp;gt;）指定&amp;lt;math&amp;gt;u&amp;lt;/math&amp;gt;的值来实现。这只相当于在流入处附加边界条件。注意，适定性允许在数据项(初始和边界)上的增长，因此它足以表明当所有数据设置为零时应有 &amp;lt;math&amp;gt;\frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 \leq 0&amp;lt;/math&amp;gt;。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==Notes==&lt;br /&gt;
&lt;br /&gt;
{{Reflist}}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
== References ==&lt;br /&gt;
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{{refbegin|2}}&lt;br /&gt;
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&lt;br /&gt;
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&lt;br /&gt;
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&lt;br /&gt;
* {{Citation |first=H. |last=Stephani |year=1989 |title=Differential Equations: Their Solution Using Symmetries. Edited by M. MacCallum |publisher=Cambridge University Press }}.&lt;br /&gt;
&lt;br /&gt;
* {{cite book |title=Partial Differential Equations and Solitary Waves Theory&lt;br /&gt;
&lt;br /&gt;
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| first Abdul-Majid | last Wazwaz | publisher Higher Education Press | year 2009 | isbn 978-3-642-00251-9 | page }&lt;br /&gt;
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| first Abdul-Majid | last Wazwaz | publisher a.a.Balkema | year 2002 | isbn 90-5809-369-7 | page }&lt;br /&gt;
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&lt;br /&gt;
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&lt;br /&gt;
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&lt;br /&gt;
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&lt;br /&gt;
* {{cite book |title=High Order Difference Methods for Time Dependent PDE&lt;br /&gt;
&lt;br /&gt;
|first=Bertil|last=Gustafsson|publisher=Springer|year=2008|isbn=978-3-540-74992-9|doi=10.1007/978-3-540-74993-6}}&lt;br /&gt;
&lt;br /&gt;
|first=Bertil|last=Gustafsson|publisher=Springer|year=2008|isbn=978-3-540-74992-9|doi=10.1007/978-3-540-74993-6}}&lt;br /&gt;
&lt;br /&gt;
| first Bertil | last Gustafsson | Springer | year 2008 | isbn 978-3-540-74992-9 | doi 10.1007 / 978-3-540-74993-6}&lt;br /&gt;
&lt;br /&gt;
{{refend}}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
== Further reading ==&lt;br /&gt;
&lt;br /&gt;
* {{Cite journal|last=Cajori|first=Florian|authorlink=Florian Cajori|year=1928|title=The Early History of Partial Differential Equations and of Partial Differentiation and Integration|url=http://www.math.harvard.edu/archive/21a_fall_14/exhibits/cajori/cajori.pdf|journal=The American Mathematical Monthly|volume=35|issue=9|pages=459–467|doi=10.2307/2298771|access-date=2016-05-15|archive-url=https://web.archive.org/web/20181123102253/http://www.math.harvard.edu/archive/21a_fall_14/exhibits/cajori/cajori.pdf|archive-date=2018-11-23|url-status=dead}}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
== External links ==&lt;br /&gt;
&lt;br /&gt;
{{Sister project links| wikt=no | commons=Category:Solutions of PDE | b=Partial Differential Equations | n=no | q=Partial differential equation | s=no | v=no | voy=no | species=no | d=no}}&lt;br /&gt;
&lt;br /&gt;
* {{springer|title=Differential equation, partial|id=p/d031920}}&lt;br /&gt;
&lt;br /&gt;
* [http://eqworld.ipmnet.ru/en/pde-en.htm Partial Differential Equations: Exact Solutions] at EqWorld: The World of Mathematical Equations.&lt;br /&gt;
&lt;br /&gt;
* [http://eqworld.ipmnet.ru/en/solutions/eqindex/eqindex-pde.htm Partial Differential Equations: Index] at EqWorld: The World of Mathematical Equations.&lt;br /&gt;
&lt;br /&gt;
* [http://eqworld.ipmnet.ru/en/methods/meth-pde.htm Partial Differential Equations: Methods] at EqWorld: The World of Mathematical Equations.&lt;br /&gt;
&lt;br /&gt;
* [https://web.archive.org/web/20170701144823/http://www.exampleproblems.com/wiki/index.php?title=Partial_Differential_Equations Example problems with solutions] at exampleproblems.com&lt;br /&gt;
&lt;br /&gt;
* [http://mathworld.wolfram.com/PartialDifferentialEquation.html Partial Differential Equations] at mathworld.wolfram.com&lt;br /&gt;
&lt;br /&gt;
* [https://reference.wolfram.com/language/FEMDocumentation/tutorial/SolvingPDEwithFEM.html Partial Differential Equations] with Mathematica&lt;br /&gt;
&lt;br /&gt;
* [http://www.mathworks.com/moler/pdes.pdf Partial Differential Equations] in Cleve Moler: Numerical Computing with MATLAB&lt;br /&gt;
&lt;br /&gt;
* [http://www.nag.com/numeric/fl/nagdoc_fl24/html/D03/d03intro.html Partial Differential Equations] at nag.com&lt;br /&gt;
&lt;br /&gt;
* {{cite web |first=Grant |last=Sanderson |title=But what is a partial differential equation? |work=3Blue1Brown |date=April 21, 2019 |url=https://www.youtube.com/watch?v=ly4S0oi3Yz8&amp;amp;list=PLZHQObOWTQDNPOjrT6KVlfJuKtYTftqH6 |via=[[YouTube]] }}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{{Differential equations topics}}&lt;br /&gt;
&lt;br /&gt;
{{Authority control}}&lt;br /&gt;
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&lt;br /&gt;
[[Category:Partial differential equations| ]]&lt;br /&gt;
&lt;br /&gt;
[[Category:Multivariable calculus]]&lt;br /&gt;
&lt;br /&gt;
Category:Multivariable calculus&lt;br /&gt;
&lt;br /&gt;
类别: 多元微积分&lt;br /&gt;
&lt;br /&gt;
[[Category:Differential equations]]&lt;br /&gt;
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Category:Differential equations&lt;br /&gt;
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类别: 微分方程&lt;br /&gt;
&lt;br /&gt;
[[Category:Concepts in physics]]&lt;br /&gt;
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Category:Concepts in physics&lt;br /&gt;
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分类: 物理概念&lt;br /&gt;
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&amp;lt;noinclude&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;small&amp;gt;This page was moved from [[wikipedia:en:Partial differential equation]]. Its edit history can be viewed at [[偏微分方程/edithistory]]&amp;lt;/small&amp;gt;&amp;lt;/noinclude&amp;gt;&lt;br /&gt;
&lt;br /&gt;
[[Category:待整理页面]]&lt;/div&gt;</summary>
		<author><name>Ruili</name></author>
	</entry>
	<entry>
		<id>https://wiki.swarma.org/index.php?title=%E5%81%8F%E5%BE%AE%E5%88%86%E6%96%B9%E7%A8%8B&amp;diff=20103</id>
		<title>偏微分方程</title>
		<link rel="alternate" type="text/html" href="https://wiki.swarma.org/index.php?title=%E5%81%8F%E5%BE%AE%E5%88%86%E6%96%B9%E7%A8%8B&amp;diff=20103"/>
		<updated>2020-12-15T12:48:24Z</updated>

		<summary type="html">&lt;p&gt;Ruili：&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;此词条暂由Yuling翻译，未经人工整理和审校，带来阅读不便，请见谅。&lt;br /&gt;
&lt;br /&gt;
[[File:Heat.gif|thumb|right|A visualisation of a solution to the two-dimensional [[heat equation]] with temperature represented by the third dimension]]&lt;br /&gt;
&lt;br /&gt;
A visualisation of a solution to the two-dimensional [[heat equation with temperature represented by the third dimension]]&lt;br /&gt;
&lt;br /&gt;
以三维表示温度的二维热方程解的可视化&lt;br /&gt;
&lt;br /&gt;
In [[mathematics]], a '''partial differential equation''' ('''PDE''') is a [[differential equation]] that contains unknown [[Multivariable calculus|multivariable functions]] and their [[partial derivative]]s. PDEs are used to formulate problems involving functions of several variables, and are either solved by hand, or used to create a [[computer model]]. A special case is [[ordinary differential equation]]s (ODEs), which deal with functions of a single variable and their derivatives.&lt;br /&gt;
&lt;br /&gt;
In mathematics, a partial differential equation (PDE) is a differential equation that contains unknown multivariable functions and their partial derivatives. PDEs are used to formulate problems involving functions of several variables, and are either solved by hand, or used to create a computer model. A special case is ordinary differential equations (ODEs), which deal with functions of a single variable and their derivatives.&lt;br /&gt;
&lt;br /&gt;
在数学中，'''&amp;lt;font color = &amp;quot;#ff8000&amp;quot;&amp;gt; 偏微分方程函数 Partial Differential Equation&amp;lt;/font&amp;gt;'''是包含未知多元函数及其偏导数的微分方程。偏微分方程用于描述涉及多元函数的问题，可以通过人为求解，也可以通过建立计算机模型来求解。常微分方程是偏微分方程一种特殊情况，它处理的是一元函数及其导数。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
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PDEs can be used to describe a wide variety of phenomena such as sound, heat, [[diffusion]], [[electrostatics]], [[Electromagnetism|electrodynamics]], [[fluid dynamics]], [[Elasticity (physics)|elasticity]], [[gravitation]] and [[quantum mechanics]]. These seemingly distinct physical phenomena can be formalised similarly in terms of PDEs. Just as ordinary differential equations often model one-dimensional [[dynamical system]]s, partial differential equations often model [[multidimensional system]]s. PDEs find their generalisation in [[stochastic partial differential equation]]s.&lt;br /&gt;
&lt;br /&gt;
PDEs can be used to describe a wide variety of phenomena such as sound, heat, diffusion, electrostatics, electrodynamics, fluid dynamics, elasticity, gravitation and quantum mechanics. These seemingly distinct physical phenomena can be formalised similarly in terms of PDEs. Just as ordinary differential equations often model one-dimensional dynamical systems, partial differential equations often model multidimensional systems. PDEs find their generalisation in stochastic partial differential equations.&lt;br /&gt;
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偏微分方程可以用来描述各种各样的物理现象，如声音，热量，扩散，静电，电动力学，流体力学，弹性力学，重力和量子力学。这些看起来截然不同的物理现象却可以用类似的偏微分方程来描述。正如常微分方程经常对一维动力系统进行建模一样，偏微分方程经常对多维系统进行建模。随机偏微分方程是偏微分方程的一种推广。&lt;br /&gt;
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== Introduction ==&lt;br /&gt;
引言&lt;br /&gt;
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Partial differential equations (PDEs) are equations that involve rates of change with respect to [[continuous variables]]. For example, the position of a [[rigid body]] is specified by six parameters,&amp;lt;ref&amp;gt;{{Cite book|url=https://books.google.com/books?id=v9PLbcYd9aUC&amp;amp;pg=PA32|title=Modelling and Control of Robot Manipulators|last=Sciavicco|first=Lorenzo|last2=Siciliano|first2=Bruno|date=2001-02-19|publisher=Springer Science &amp;amp; Business Media|isbn=9781852332211|language=en}}&amp;lt;/ref&amp;gt; but the configuration of a [[fluid]] is given by the [[continuous distribution]] of several parameters, such as the [[temperature]], [[pressure]], and so forth. The dynamics for the rigid body take place in a finite-dimensional [[Configuration space (physics)|configuration space]]; the dynamics for the fluid occur in an infinite-dimensional configuration space. This distinction usually makes PDEs much harder to solve than ordinary differential equations (ODEs), but here again, there will be simple solutions for linear problems. Classic domains where PDEs are used include [[acoustics]], [[fluid dynamics]], [[electrodynamics]], and [[heat transfer]].&lt;br /&gt;
&lt;br /&gt;
Partial differential equations (PDEs) are equations that involve rates of change with respect to continuous variables. For example, the position of a rigid body is specified by six parameters, but the configuration of a fluid is given by the continuous distribution of several parameters, such as the temperature, pressure, and so forth. The dynamics for the rigid body take place in a finite-dimensional configuration space; the dynamics for the fluid occur in an infinite-dimensional configuration space. This distinction usually makes PDEs much harder to solve than ordinary differential equations (ODEs), but here again, there will be simple solutions for linear problems. Classic domains where PDEs are used include acoustics, fluid dynamics, electrodynamics, and heat transfer.&lt;br /&gt;
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偏微分方程(简称为PDEs)涉及到方程相对于连续变量的变化率。例如，刚体的位置是由六个参数确定的，而流体的状态是由几个参数的连续分布给出的，如温度、压力等。刚体的动力学过程发生在有限维状态空间中，流体的动力学过程发生在无限维状态空间中。这种区别通常使偏微分方程比常微分方程更难求解，但是线性问题仍然有简单的求解方式。使用偏微分方程的经典领域包括声学、流体力学、电动力学和传热学。&lt;br /&gt;
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A partial differential equation (PDE) for the function {{math|''u''(''x''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;,… ''x&amp;lt;sub&amp;gt;n&amp;lt;/sub&amp;gt;'')}} is an equation of the form&lt;br /&gt;
&lt;br /&gt;
A partial differential equation (PDE) for the function  is an equation of the form&lt;br /&gt;
&lt;br /&gt;
函数 {{math|''u''(''x''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;,… ''x&amp;lt;sub&amp;gt;n&amp;lt;/sub&amp;gt;'')}} 的偏微分方程形式是：&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt;f \left (x_1, \ldots x_n; u, \frac{\partial u}{\partial x_1}, \ldots \frac{\partial u}{\partial x_n}; \frac{\partial^2 u}{\partial x_1 \partial x_1}, \ldots \frac{\partial^2 u}{\partial x_1 \partial x_n}; \ldots \right) = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;f \left (x_1, \ldots x_n; u, \frac{\partial u}{\partial x_1}, \ldots \frac{\partial u}{\partial x_n}; \frac{\partial^2 u}{\partial x_1 \partial x_1}, \ldots \frac{\partial^2 u}{\partial x_1 \partial x_n}; \ldots \right) = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
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If {{mvar|f}} is a [[linear function]] of {{mvar|u}} and its derivatives, then the PDE is called linear. Common examples of linear PDEs include the [[heat equation]], the [[wave equation]], [[Laplace's equation]], [[Helmholtz equation]], [[Klein–Gordon equation]], and [[Poisson's equation]].&lt;br /&gt;
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If  is a linear function of  and its derivatives, then the PDE is called linear. Common examples of linear PDEs include the heat equation, the wave equation, Laplace's equation, Helmholtz equation, Klein–Gordon equation, and Poisson's equation.&lt;br /&gt;
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如果 {{mvar|f}} 是函数 {{math|''u''}} 及其导数的线性函数，则偏微分方程称为线性函数。线性偏微分方程的常见例子包括热方程、波动方程、拉普拉斯方程、亥姆霍兹方程方程、克莱因-高登方程和泊松方程。&lt;br /&gt;
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A relatively simple PDE is&lt;br /&gt;
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A relatively simple PDE is&lt;br /&gt;
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一个相对简单的偏微分方程：&lt;br /&gt;
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: &amp;lt;math&amp;gt;\frac{\partial u}{\partial x}(x,y) = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;\frac{\partial u}{\partial x}(x,y) = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
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This relation [[Logical implication|implies]] that the function {{math|''u''(''x'',''y'')}} is independent of {{mvar|x}}. However, the equation gives no information on the function's dependence on the variable {{mvar|y}}. Hence the general solution of this equation is&lt;br /&gt;
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This relation implies that the function  is independent of . However, the equation gives no information on the function's dependence on the variable . Hence the general solution of this equation is&lt;br /&gt;
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这意味着函数 {{math|''u''(''x'',''y'')}} 独立于 {{mvar|x}} 的。然而，这个方程没有给出关于函数和自变量的相关性的信息。因此，这个方程的通解是&lt;br /&gt;
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: &amp;lt;math&amp;gt;u(x,y) = f(y),&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;u(x,y) = f(y),&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
where {{mvar|f}} is an arbitrary function of {{mvar|y}}. The analogous ordinary differential equation is&lt;br /&gt;
&lt;br /&gt;
where  is an arbitrary function of . The analogous ordinary differential equation is&lt;br /&gt;
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其中， {{mvar|f}} 是 {{mvar|y}} 的任意函数。&lt;br /&gt;
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类似的常微分方程是：&lt;br /&gt;
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: &amp;lt;math&amp;gt;\frac{\mathrm{d} u}{\mathrm{d} x}(x) = 0,&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;\frac{\mathrm{d} u}{\mathrm{d} x}(x) = 0,&amp;lt;/math&amp;gt;&lt;br /&gt;
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which has the solution&lt;br /&gt;
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which has the solution&lt;br /&gt;
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它的解为&lt;br /&gt;
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: &amp;lt;math&amp;gt;u(x) = c,&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;u(x) = c,&amp;lt;/math&amp;gt;&lt;br /&gt;
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where {{mvar|c}} is any [[Constant (mathematics)|constant]] value. These two examples illustrate that general solutions of ordinary differential equations (ODEs) involve arbitrary constants, but solutions of PDEs involve arbitrary functions.&lt;br /&gt;
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where  is any constant value. These two examples illustrate that general solutions of ordinary differential equations (ODEs) involve arbitrary constants, but solutions of PDEs involve arbitrary functions.&lt;br /&gt;
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这里，{{mvar|c}} 是一个任意常量。&lt;br /&gt;
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这两个例子说明常微分方程的一般解包含任意常数，但偏微分方程的解包含任意函数。&lt;br /&gt;
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A solution of a PDE is generally not [[Uniqueness quantification|unique]]; additional conditions must generally be specified on the [[Boundary (topology)|boundary]] of the region where the solution is defined. For instance, in the simple example above, the function {{math|''f''(''y'')}} can be determined if {{mvar|u}} is specified on the line {{math|''x'' {{=}} 0}}.&lt;br /&gt;
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A solution of a PDE is generally not unique; additional conditions must generally be specified on the boundary of the region where the solution is defined. For instance, in the simple example above, the function  can be determined if  is specified on the line  0}}.&lt;br /&gt;
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偏微分方程的解一般不是唯一的; 一般必须在定义解的区域边界上定义附加条件。 例如，在上面的简单示例中，如果在 {{math|''x'' {{=}} 0}} 时确定了 {{mvar|u}} 的值，则可以确定该函数 {{math|''f''(''y'')}}。&lt;br /&gt;
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== Existence and uniqueness ==&lt;br /&gt;
存在性和唯一性&lt;br /&gt;
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Although the issue of existence and uniqueness of solutions of ordinary differential equations has a very satisfactory answer with the [[Picard–Lindelöf theorem]], that is far from the case for partial differential equations. The [[Cauchy–Kowalevski theorem]] states that the [[Cauchy problem]] for any partial differential equation whose coefficients are [[Analytic function|analytic]] in the unknown function and its derivatives, has a locally unique analytic solution. Although this result might appear to settle the existence and uniqueness of solutions, there are examples of linear partial differential equations whose coefficients have derivatives of all orders (which are nevertheless not analytic) but which have no solutions at all: see [[Lewy's example|Lewy (1957)]]. Even if the solution of a partial differential equation exists and is unique, it may nevertheless have undesirable properties.  The mathematical study of these questions is usually in the more powerful context of [[weak solution]]s.&lt;br /&gt;
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Although the issue of existence and uniqueness of solutions of ordinary differential equations has a very satisfactory answer with the Picard–Lindelöf theorem, that is far from the case for partial differential equations. The Cauchy–Kowalevski theorem states that the Cauchy problem for any partial differential equation whose coefficients are analytic in the unknown function and its derivatives, has a locally unique analytic solution. Although this result might appear to settle the existence and uniqueness of solutions, there are examples of linear partial differential equations whose coefficients have derivatives of all orders (which are nevertheless not analytic) but which have no solutions at all: see Lewy (1957). Even if the solution of a partial differential equation exists and is unique, it may nevertheless have undesirable properties.  The mathematical study of these questions is usually in the more powerful context of weak solutions.&lt;br /&gt;
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尽管常微分方程解的存在性和唯一性用'''&amp;lt;font color=&amp;quot;#ff8000&amp;quot;&amp;gt;弗罗贝尼乌斯定理 Picard–Lindelöf Theorem&amp;lt;/font&amp;gt;得到了令人满意的结果，但偏微分方程解的存在性和唯一性却远没有得到解决。'''&amp;lt;font color=&amp;quot;#ff8000&amp;quot;&amp;gt;柯西-科瓦列夫斯基定理 Cauchy–Kowalevski theorem&amp;lt;/font&amp;gt;指出：对于任意系数在未知函数及其导数中解析的偏微分方程，柯西问题存在一个局部唯一的解析解。虽然这个结果似乎解决了解的存在性和唯一性问题，但是存在一些线性偏微分方程-其系数具有所有级数的导数(尽管这些导数不是解析的) ，但是根本没有解: 见 Lewy (1957)。即使偏微分方程的解存在且唯一，它仍然可能具有不可预料的性质。这些问题的数学研究通常是在更有力的弱解的背景下进行的。&lt;br /&gt;
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An example of pathological behavior is the sequence (depending upon {{mvar|n}}) of [[Cauchy problem]]s for the [[Laplace equation]]&lt;br /&gt;
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An example of pathological behavior is the sequence (depending upon ) of Cauchy problems for the Laplace equation&lt;br /&gt;
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反常特征的一个例子是拉普拉斯方程的柯西问题的序列(取决于{{mvar|n}})&lt;br /&gt;
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: &amp;lt;math&amp;gt;\frac{\partial^2 u}{\partial x^2} + \frac{\partial^2 u}{\partial y^2}=0,&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;\frac{\partial^2 u}{\partial x^2} + \frac{\partial^2 u}{\partial y^2}=0,&amp;lt;/math&amp;gt;&lt;br /&gt;
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with [[boundary condition]]s&lt;br /&gt;
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with boundary conditions&lt;br /&gt;
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具有边界条件&lt;br /&gt;
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: &amp;lt;math&amp;gt;\begin{align} u(x,0) &amp;amp;= 0, \\ \frac{\partial u}{\partial y}(x,0) &amp;amp;= \frac{\sin nx}{n}, \end{align}&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;\begin{align} u(x,0) &amp;amp;= 0, \\ \frac{\partial u}{\partial y}(x,0) &amp;amp;= \frac{\sin nx}{n}, \end{align}&amp;lt;/math&amp;gt;&lt;br /&gt;
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where {{mvar|n}} is an integer. The derivative of {{mvar|u}} with respect to {{mvar|y}} approaches zero [[uniform convergence|uniformly]] in {{mvar|x}} as {{mvar|n}} increases, but the solution is&lt;br /&gt;
&lt;br /&gt;
where  is an integer. The derivative of  with respect to  approaches zero uniformly in  as  increases, but the solution is&lt;br /&gt;
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其中 {{mvar|n}} 是整数。{{mvar|u}} 关于 {{mvar|y}} 的导数，一致地随着 {{mvar|n}} 的增加而趋于零，但解是&lt;br /&gt;
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: &amp;lt;math&amp;gt;u(x,y) = \frac{\sinh ny \sin nx}{n^2}.&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;u(x,y) = \frac{\sinh ny \sin nx}{n^2}.&amp;lt;/math&amp;gt;&lt;br /&gt;
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This solution approaches infinity if {{mvar|nx}} is not an integer multiple of {{pi}} for any non-zero value of {{mvar|y}}. The Cauchy problem for the Laplace equation is called ''ill-posed'' or ''not [[Well-posed problem|well-posed]]'', since the solution does not continuously depend on the data of the problem. Such ill-posed problems are not usually satisfactory for physical applications.&lt;br /&gt;
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This solution approaches infinity if  is not an integer multiple of  for any non-zero value of . The Cauchy problem for the Laplace equation is called ill-posed or not well-posed, since the solution does not continuously depend on the data of the problem. Such ill-posed problems are not usually satisfactory for physical applications.&lt;br /&gt;
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对于任何非零的 {{mvar|y}}，如果 {{mvar|nx}} 不是模板 {{pi}} 的整数倍，这个解会接近于无穷大。拉普拉斯方程的柯西问题被称为不适定的（可以译为ill-posed或not well-posed），因为解不是连续地依赖于问题的数据。这种不适定问题通常不能满足物理应用。&lt;br /&gt;
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The [[Navier–Stokes existence and smoothness|existence of solutions for the Navier–Stokes equations]], a partial differential equation, is part of one of the [[Millennium Prize Problems]].&lt;br /&gt;
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The existence of solutions for the Navier–Stokes equations, a partial differential equation, is part of one of the Millennium Prize Problems.&lt;br /&gt;
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偏微分方程”纳维-斯托克斯方程“的解的存在性就是千禧年大奖难题之一的一部分。&lt;br /&gt;
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== Notation ==&lt;br /&gt;
符号&lt;br /&gt;
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In PDEs, it is common to denote partial derivatives using subscripts. That is:&lt;br /&gt;
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In PDEs, it is common to denote partial derivatives using subscripts. That is:&lt;br /&gt;
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在偏微分方程中，通常用下标表示偏导数。例如:&lt;br /&gt;
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: &amp;lt;math&amp;gt;u_x = \frac{\partial u}{\partial x}&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;u_x = \frac{\partial u}{\partial x}&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt;u_{xx} = \frac{\partial^2 u}{\partial x^2} &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;u_{xx} = \frac{\partial^2 u}{\partial x^2} &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
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: &amp;lt;math&amp;gt;u_{xy} = \frac{\partial^2 u}{\partial y\, \partial x} = \frac{\partial}{\partial y } \left(\frac{\partial u}{\partial x}\right). &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;u_{xy} = \frac{\partial^2 u}{\partial y\, \partial x} = \frac{\partial}{\partial y } \left(\frac{\partial u}{\partial x}\right). &amp;lt;/math&amp;gt;&lt;br /&gt;
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Especially in physics, [[del]] or nabla ({{math|∇}}) is often used to denote spatial derivatives, and {{math|''&amp;amp;#x307;u'', ''ü''}} for time derivatives. For example, the [[wave equation]] (mentioned below) can be written as&lt;br /&gt;
&lt;br /&gt;
Especially in physics, del or nabla () is often used to denote spatial derivatives, and  for time derivatives. For example, the wave equation (mentioned below) can be written as&lt;br /&gt;
&lt;br /&gt;
特别是在物理学中，[[del]] 或 nabla ({{math|∇}}) 经常用来表示空间导数和时间导数。例如，波动方程(在下文中提到)可以写成：&lt;br /&gt;
&lt;br /&gt;
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:&amp;lt;math&amp;gt;\ddot u=c^2\nabla^2u&amp;lt;/math&amp;gt;&lt;br /&gt;
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&amp;lt;math&amp;gt;\ddot u=c^2\nabla^2u&amp;lt;/math&amp;gt;&lt;br /&gt;
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or&lt;br /&gt;
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or&lt;br /&gt;
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或&lt;br /&gt;
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:&amp;lt;math&amp;gt;\ddot u=c^2\Delta u&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt;\ddot u=c^2\Delta u&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
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&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
where {{math|Δ}} is the [[Laplace operator]].&lt;br /&gt;
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where  is the Laplace operator.&lt;br /&gt;
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其中，{{math|Δ}} 代表拉普拉斯算子。&lt;br /&gt;
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== Classification ==&lt;br /&gt;
分类&lt;br /&gt;
&lt;br /&gt;
Some linear, second-order partial differential equations can be classified as [[parabolic partial differential equation|parabolic]], [[hyperbolic partial differential equation|hyperbolic]] and [[elliptic partial differential equation|elliptic]]. Others, such as the [[Euler–Tricomi equation]], have different types in different regions. The classification provides a guide to appropriate initial and boundary conditions and to the smoothness of the solutions.&lt;br /&gt;
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Some linear, second-order partial differential equations can be classified as parabolic, hyperbolic and elliptic. Others, such as the Euler–Tricomi equation, have different types in different regions. The classification provides a guide to appropriate initial and boundary conditions and to the smoothness of the solutions.&lt;br /&gt;
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一些线性二阶偏微分方程可分为抛物型方程、双曲型方程和椭圆型方程。其他的方程，如欧拉-特里科米方程，在不同的领域有不同的类型。这种分类有助于选择适当的初始和边界条件以及提高解的平滑性。&lt;br /&gt;
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=== Equations of first order ===&lt;br /&gt;
一阶方程&lt;br /&gt;
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{{main|First-order partial differential equation}}&lt;br /&gt;
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=== Linear equations of second order ===&lt;br /&gt;
二阶线性方程&lt;br /&gt;
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Assuming {{math|''u&amp;lt;sub&amp;gt;xy&amp;lt;/sub&amp;gt;'' {{=}} ''u&amp;lt;sub&amp;gt;yx&amp;lt;/sub&amp;gt;''}}, the general linear second-order PDE in two independent variables has the form&lt;br /&gt;
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Assuming  u&amp;lt;sub&amp;gt;yx&amp;lt;/sub&amp;gt;}}, the general linear second-order PDE in two independent variables has the form&lt;br /&gt;
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假设 {{math|''u&amp;lt;sub&amp;gt;xy&amp;lt;/sub&amp;gt;'' {{=}} ''u&amp;lt;sub&amp;gt;yx&amp;lt;/sub&amp;gt;''}}，含有两个独立变量的一般线性二阶偏微分方程具有如下形式：&lt;br /&gt;
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: &amp;lt;math&amp;gt;Au_{xx} + 2Bu_{xy} + Cu_{yy} + \cdots \mbox{(lower order terms)} = 0,&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;Au_{xx} + 2Bu_{xy} + Cu_{yy} + \cdots \mbox{(lower order terms)} = 0,&amp;lt;/math&amp;gt;&lt;br /&gt;
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where the coefficients {{mvar|A}}, {{mvar|B}}, {{mvar|C}}... may depend upon {{mvar|x}} and {{mvar|y}}. If {{math|''A''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; + ''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; + ''C''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; &amp;gt; 0}} over a region of the {{mvar|xy}}-plane, the PDE is second-order in that region. This form is analogous to the equation for a conic section:&lt;br /&gt;
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where the coefficients , , ... may depend upon  and . If  over a region of the -plane, the PDE is second-order in that region. This form is analogous to the equation for a conic section:&lt;br /&gt;
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其中的系数 {{mvar|A}}, {{mvar|B}}, {{mvar|C}}... 一般取决于 {{mvar|x}} 和 {{mvar|y}} 。如果在 {{mvar|xy}}-平面的一个区域上 {{math|''A''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; + ''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; + ''C''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; &amp;gt; 0}}，偏微分方程是二阶的，这种形式类似于圆锥截面的方程:&lt;br /&gt;
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: &amp;lt;math&amp;gt;Ax^2 + 2Bxy + Cy^2 + \cdots = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;Ax^2 + 2Bxy + Cy^2 + \cdots = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
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More precisely, replacing {{math|∂&amp;lt;sub&amp;gt;''x''&amp;lt;/sub&amp;gt;}} by {{mvar|X}}, and likewise for other variables (formally this is done by a [[Fourier transform]]), converts a constant-coefficient PDE into a polynomial of the same degree, with the terms of the highest degree (a [[homogeneous polynomial]], here a [[quadratic form]]) being most significant for the classification.&lt;br /&gt;
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More precisely, replacing  by , and likewise for other variables (formally this is done by a Fourier transform), converts a constant-coefficient PDE into a polynomial of the same degree, with the terms of the highest degree (a homogeneous polynomial, here a quadratic form) being most significant for the classification.&lt;br /&gt;
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更准确地说，用 {{mvar|X}} 替换 {{math|∂&amp;lt;sub&amp;gt;''x''&amp;lt;/sub&amp;gt;}}，并同样替换其它变量(通常由傅里叶变换完成)，将一个常系数偏微分方程转换成一个相同次数的多项式，最高次数的项(齐次多项式，这里是一个二次形式)对于偏微分方程的分类最为重要。&lt;br /&gt;
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Just as one classifies [[conic section]]s and quadratic forms into parabolic, hyperbolic, and elliptic based on the [[discriminant]] {{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − 4''AC''}}, the same can be done for a second-order PDE at a given point.  However, the [[discriminant]] in a PDE is given by {{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC''}} due to the convention of the {{mvar|xy}} term being {{math|2''B''}} rather than {{mvar|B}}; formally, the discriminant (of the associated quadratic form) is {{math|(2''B'')&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − 4''AC'' {{=}} 4(''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC'')}}, with the factor of 4 dropped for simplicity.&lt;br /&gt;
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Just as one classifies conic sections and quadratic forms into parabolic, hyperbolic, and elliptic based on the discriminant , the same can be done for a second-order PDE at a given point.  However, the discriminant in a PDE is given by  due to the convention of the  term being  rather than ; formally, the discriminant (of the associated quadratic form) is  4(B&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − AC)}}, with the factor of 4 dropped for simplicity.&lt;br /&gt;
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正如人们可以根据判别式 {{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − 4''AC''}} 将圆锥截面和二次型分为抛物型、双曲型和椭圆型一样，对于给定点的二阶偏微分方程也可以这样做。然而，偏微分方程中的判别式 {{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − 4''AC''}} 是根据交叉项的系数{{math|2''B''}} 而不是 {{mvar|B}} 给出的，形式上，判别式(关联二次型)是 {{math|(2''B'')&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − 4''AC'' {{=}} 4(''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC'')}}，为简单起见，去掉了因子4。&lt;br /&gt;
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# {{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC'' &amp;lt; 0}} (''[[elliptic partial differential equation]]''): Solutions of [[elliptic partial differential equation|elliptic PDEs]] are as smooth as the coefficients allow, within the interior of the region where the equation and solutions are defined. For example, solutions of [[Laplace's equation]] are analytic within the domain where they are defined, but solutions may assume boundary values that are not smooth. The motion of a fluid at subsonic speeds can be approximated with elliptic PDEs, and the Euler–Tricomi equation is elliptic where {{math|''x'' &amp;lt; 0}}.&lt;br /&gt;
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  (elliptic partial differential equation): Solutions of elliptic PDEs are as smooth as the coefficients allow, within the interior of the region where the equation and solutions are defined. For example, solutions of Laplace's equation are analytic within the domain where they are defined, but solutions may assume boundary values that are not smooth. The motion of a fluid at subsonic speeds can be approximated with elliptic PDEs, and the Euler–Tricomi equation is elliptic where .&lt;br /&gt;
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{{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC'' &amp;lt; 0}} (椭圆型微分方程)：在定义方程和解的区域内部，椭圆型偏微分方程的解在系数允许的程度内光滑。例如，拉普拉斯方程的解在它们被定义的区域内是解析的，但可能假设边界值是不光滑的。亚音速流体的运动可以用椭圆型偏微分方程近似，欧拉-特里科米方程在 {{math|''x'' &amp;lt; 0}} 时是椭圆型偏微分方程。&lt;br /&gt;
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# {{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC'' {{=}} 0}} (''[[parabolic partial differential equation]]''): Equations that are [[parabolic partial differential equation|parabolic]] at every point can be transformed into a form analogous to the [[heat equation]] by a change of independent variables. Solutions smooth out as the transformed time variable increases. The Euler–Tricomi equation has parabolic type on the line where {{math|''x'' {{=}} 0}}.&lt;br /&gt;
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  0}} (parabolic partial differential equation): Equations that are parabolic at every point can be transformed into a form analogous to the heat equation by a change of independent variables. Solutions smooth out as the transformed time variable increases. The Euler–Tricomi equation has parabolic type on the line where  0}}.&lt;br /&gt;
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{{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC'' {{=}} 0}}（抛物型偏微分方程）：在每一点上都是抛物线型的方程可以通过改变自变量从而转化成类似于热方程的形式。随着转换后的时间变量的增加，方程的解变得平滑。欧拉-特里科米方程在特征线 {{math|''x'' {{=}} 0}} 上是抛物线型的。&lt;br /&gt;
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# {{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC'' &amp;gt; 0}} (''[[hyperbolic partial differential equation]]''): [[hyperbolic partial differential equation|hyperbolic]] equations retain any discontinuities of functions or derivatives in the initial data. An example is the [[wave equation]]. The motion of a fluid at supersonic speeds can be approximated with hyperbolic PDEs, and the Euler–Tricomi equation is hyperbolic where {{math|''x'' &amp;gt; 0}}.&lt;br /&gt;
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  (hyperbolic partial differential equation): hyperbolic equations retain any discontinuities of functions or derivatives in the initial data. An example is the wave equation. The motion of a fluid at supersonic speeds can be approximated with hyperbolic PDEs, and the Euler–Tricomi equation is hyperbolic where .&lt;br /&gt;
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{{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC'' &amp;gt; 0}} (双曲型偏微分方程)：双曲型方程在初始数据中保留了函数或导数的任何不连续性。波动方程就是其中的一个例子。超音速流体的运动可以用双曲型偏微分方程近似，欧拉-特里科米方程在 {{math|''x'' &amp;gt; 0}} 时是双曲型的。&lt;br /&gt;
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If there are {{mvar|n}} independent variables {{math|''x''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;, ''x''&amp;lt;sub&amp;gt;2 &amp;lt;/sub&amp;gt;,… ''x''&amp;lt;sub&amp;gt;''n''&amp;lt;/sub&amp;gt;}}, a general linear partial differential equation of second order has the form&lt;br /&gt;
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If there are  independent variables , a general linear partial differential equation of second order has the form&lt;br /&gt;
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如果存在 {{mvar|n}} 个自变量 {{math|''x''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;, ''x''&amp;lt;sub&amp;gt;2 &amp;lt;/sub&amp;gt;,… ''x''&amp;lt;sub&amp;gt;''n''&amp;lt;/sub&amp;gt;}}，一般二阶线性偏微分方程的形式是：&lt;br /&gt;
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: &amp;lt;math&amp;gt;L u =\sum_{i=1}^n\sum_{j=1}^n a_{i,j} \frac{\partial^2 u}{\partial x_i \partial x_j} \quad \text{ plus lower-order terms} =0.&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;L u =\sum_{i=1}^n\sum_{j=1}^n a_{i,j} \frac{\partial^2 u}{\partial x_i \partial x_j} \quad \text{ plus lower-order terms} =0.&amp;lt;/math&amp;gt;&lt;br /&gt;
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The classification depends upon the signature of the eigenvalues of the coefficient matrix {{math|''a''&amp;lt;sub&amp;gt;''i'',''j''&amp;lt;/sub&amp;gt;}}.&lt;br /&gt;
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The classification depends upon the signature of the eigenvalues of the coefficient matrix .&lt;br /&gt;
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这种分类取决于系数矩阵特征值的符号（正负性）。&lt;br /&gt;
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# Elliptic: the eigenvalues are all positive or all negative.&lt;br /&gt;
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 Elliptic: the eigenvalues are all positive or all negative.&lt;br /&gt;
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椭圆形方程: 特征值全部为正或全部为负。&lt;br /&gt;
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# Parabolic: the eigenvalues are all positive or all negative, save one that is zero.&lt;br /&gt;
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 Parabolic: the eigenvalues are all positive or all negative, save one that is zero.&lt;br /&gt;
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抛物线形方程:除了一个为零值，特征值全部为正或全部为负。&lt;br /&gt;
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# Hyperbolic: there is only one negative eigenvalue and all the rest are positive, or there is only one positive eigenvalue and all the rest are negative.&lt;br /&gt;
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 Hyperbolic: there is only one negative eigenvalue and all the rest are positive, or there is only one positive eigenvalue and all the rest are negative.&lt;br /&gt;
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双曲形方程: 只有一个负特征值，其余的都是正特征值，或者只有一个正特征值，其余的都是负特征值。&lt;br /&gt;
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# Ultrahyperbolic: there is more than one positive eigenvalue and more than one negative eigenvalue, and there are no zero eigenvalues. There is only a limited theory for ultrahyperbolic equations (Courant and Hilbert, 1962).&lt;br /&gt;
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 Ultrahyperbolic: there is more than one positive eigenvalue and more than one negative eigenvalue, and there are no zero eigenvalues. There is only a limited theory for ultrahyperbolic equations (Courant and Hilbert, 1962).&lt;br /&gt;
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超双形方程: 存在多于一个正特征值和多于一个的负特征值，且不存在零特征值。对于超双曲方程，只存在有限的理论(Courant 和 Hilbert，1962)。&lt;br /&gt;
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=== Systems of first-order equations and characteristic surfaces ===&lt;br /&gt;
一阶方程组和特征曲面&lt;br /&gt;
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The classification of partial differential equations can be extended to systems of first-order equations, where the unknown {{mvar|u}} is now a [[Euclidean vector|vector]] with {{mvar|m}} components, and the coefficient matrices {{mvar|A&amp;lt;sub&amp;gt;ν&amp;lt;/sub&amp;gt;}} are {{mvar|m}} by {{mvar|m}} matrices for {{math|''ν'' {{=}} 1, 2,… ''n''}}. The partial differential equation takes the form&lt;br /&gt;
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The classification of partial differential equations can be extended to systems of first-order equations, where the unknown  is now a vector with  components, and the coefficient matrices  are  by  matrices for  1, 2,… n}}. The partial differential equation takes the form&lt;br /&gt;
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偏微分方程的分类可以推广到一阶方程组，其中未知量 {{mvar|u}} 是有 {{mvar|m}} 个分量的向量。对于 {{math|''ν'' {{=}} 1, 2,… ''n''}}，系数矩阵 {{mvar|A&amp;lt;sub&amp;gt;ν&amp;lt;/sub&amp;gt;}} 是 {{mvar|m}} × {{mvar|m}} 的矩阵。偏微分方程形式如下：&lt;br /&gt;
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: &amp;lt;math&amp;gt;Lu = \sum_{\nu=1}^{n} A_\nu \frac{\partial u}{\partial x_\nu} + B=0,&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;Lu = \sum_{\nu=1}^{n} A_\nu \frac{\partial u}{\partial x_\nu} + B=0,&amp;lt;/math&amp;gt;&lt;br /&gt;
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where the coefficient matrices {{mvar|A&amp;lt;sub&amp;gt;ν&amp;lt;/sub&amp;gt;}} and the vector {{mvar|B}} may depend upon {{mvar|x}} and {{mvar|u}}. If a [[hypersurface]] {{mvar|S}} is given in the implicit form&lt;br /&gt;
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where the coefficient matrices  and the vector  may depend upon  and . If a hypersurface  is given in the implicit form&lt;br /&gt;
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其中，系数矩阵 {{mvar|A&amp;lt;sub&amp;gt;ν&amp;lt;/sub&amp;gt;}} 和向量 {{mvar|B}} 可能依赖于 {{mvar|x}} 和 {{mvar|u}}。如果超曲面是以以下隐式形式给出的，&lt;br /&gt;
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: &amp;lt;math&amp;gt;\varphi(x_1, x_2, \ldots x_n)=0,&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;\varphi(x_1, x_2, \ldots x_n)=0,&amp;lt;/math&amp;gt;&lt;br /&gt;
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where {{mvar|φ}} has a non-zero gradient, then {{mvar|S}} is a '''characteristic surface''' for the operator {{mvar|L}} at a given point if the characteristic form vanishes:&lt;br /&gt;
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where  has a non-zero gradient, then  is a characteristic surface for the operator  at a given point if the characteristic form vanishes:&lt;br /&gt;
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其中，存在一个非零的梯度 {{mvar|φ}}，对于在给定点上特征形式消失的算子，特征曲面 {{mvar|S}} 形式如下:&lt;br /&gt;
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: &amp;lt;math&amp;gt;Q\left(\frac{\partial\varphi}{\partial x_1}, \ldots\frac{\partial\varphi}{\partial x_n}\right) =\det\left[\sum_{\nu=1}^nA_\nu \frac{\partial \varphi}{\partial x_\nu}\right]=0.\,&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;Q\left(\frac{\partial\varphi}{\partial x_1}, \ldots\frac{\partial\varphi}{\partial x_n}\right) =\det\left[\sum_{\nu=1}^nA_\nu \frac{\partial \varphi}{\partial x_\nu}\right]=0.\,&amp;lt;/math&amp;gt;&lt;br /&gt;
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The geometric interpretation of this condition is as follows: if data for {{mvar|u}} are prescribed on the surface {{mvar|S}}, then it may be possible to determine the normal derivative of {{mvar|u}} on {{mvar|S}} from the differential equation. If the data on {{mvar|S}} and the differential equation determine the normal derivative of {{mvar|u}} on {{mvar|S}}, then {{mvar|S}} is non-characteristic. If the data on {{mvar|S}} and the differential equation ''do not'' determine the normal derivative of {{mvar|u}} on {{mvar|S}}, then the surface is '''characteristic''', and the differential equation restricts the data on {{mvar|S}}: the differential equation is ''internal'' to {{mvar|S}}.&lt;br /&gt;
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The geometric interpretation of this condition is as follows: if data for  are prescribed on the surface , then it may be possible to determine the normal derivative of  on  from the differential equation. If the data on  and the differential equation determine the normal derivative of  on , then  is non-characteristic. If the data on  and the differential equation do not determine the normal derivative of  on , then the surface is characteristic, and the differential equation restricts the data on : the differential equation is internal to .&lt;br /&gt;
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这个条件的几何解释如下: 如果关于 {{mvar|u}} 的数据是在曲面 {{mvar|S}} 上规定的，那么就有可能依据微分方程确定曲面 {{mvar|S}} 上 {{mvar|u}} 的法向导数。如果曲面 {{mvar|S}} 上的数据和上面的微分方程能确定曲面 {{mvar|S}} 上 {{mvar|u}} 的法向导数，那么它就是非特征的。如果曲面 {{mvar|S}} 上的数据和上面的微分方程不能确定曲面 {{mvar|S}} 上 {{mvar|u}} 的法向导数，那么曲面是特征的，并且微分方程将数据限制在曲面 {{mvar|S}} 上：微分方程是在曲面 {{mvar|S}} 内部。&lt;br /&gt;
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# A first-order system {{math|''Lu'' {{=}} 0}} is ''elliptic'' if no surface is characteristic for {{mvar|L}}: the values of {{mvar|u}} on {{mvar|S}} and the differential equation always determine the normal derivative of {{mvar|u}} on {{mvar|S}}.&lt;br /&gt;
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 A first-order system  0}} is elliptic if no surface is characteristic for : the values of  on  and the differential equation always determine the normal derivative of  on .&lt;br /&gt;
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如果对于 {{mvar|L}} 没有曲面是特征的，则一阶系统 {{math|''Lu'' {{=}} 0}} 是椭圆形的：{{mvar|u}}在 {{mvar|S}} 的值和微分方程总能够决定 {{mvar|S}} 上 {{mvar|u}} 的法向导数。&lt;br /&gt;
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# A first-order system is ''hyperbolic'' at a point if there is a '''spacelike''' surface {{mvar|S}} with normal {{mvar|ξ}} at that point. This means that, given any non-trivial vector {{mvar|η}} orthogonal to {{mvar|ξ}}, and a scalar multiplier {{mvar|λ}}, the equation {{math|''Q''(''λξ'' + ''η'') {{=}} 0}} has {{mvar|m}} real roots {{math|''λ''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;, ''λ''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;,… ''λ''&amp;lt;sub&amp;gt;''m''&amp;lt;/sub&amp;gt;}}. The system is '''strictly hyperbolic''' if these roots are always distinct. The geometrical interpretation of this condition is as follows: the characteristic form {{math|''Q''(''ζ'') {{=}} 0}} defines a cone (the normal cone) with homogeneous coordinates ζ. In the hyperbolic case, this cone has {{mvar|m}} sheets, and the axis {{math|''ζ'' {{=}} ''λξ''}} runs inside these sheets: it does not intersect any of them. But when displaced from the origin by η, this axis intersects every sheet. In the elliptic case, the normal cone has no real sheets.&lt;br /&gt;
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 A first-order system is hyperbolic at a point if there is a spacelike surface  with normal  at that point. This means that, given any non-trivial vector  orthogonal to , and a scalar multiplier , the equation  0}} has  real roots . The system is strictly hyperbolic if these roots are always distinct. The geometrical interpretation of this condition is as follows: the characteristic form  0}} defines a cone (the normal cone) with homogeneous coordinates ζ. In the hyperbolic case, this cone has  sheets, and the axis  λξ}} runs inside these sheets: it does not intersect any of them. But when displaced from the origin by η, this axis intersects every sheet. In the elliptic case, the normal cone has no real sheets.&lt;br /&gt;
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如果在该点存在一个法向量为 {{mvar|ξ}}的 '''&amp;lt;font color=&amp;quot;#ff8000&amp;quot;&amp;gt;类空曲面 Spacclike Surface&amp;lt;/font&amp;gt; {{mvar|S}} ，则一阶系统在那一点是双曲的。这意味着，给定任意正交于 {{mvar|ξ}} 的非平凡向量 {{mvar|η}} 和一个标量乘子 {{mvar|λ}}，方程 {{math|''Q''(''λξ'' + ''η'') {{=}} 0}} 有 {{mvar|m}} 个实根 {{math|''λ''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;, ''λ''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;,… ''λ''&amp;lt;sub&amp;gt;''m''&amp;lt;/sub&amp;gt;}}。如果这些根始终不同，则该系统是严格双曲形的。这个条件的几何解释如下: 特征形式 {{math|''Q''(''ζ'') {{=}} 0}} 定义了一个具有齐次坐标 ζ的圆锥(法线圆锥)。在双曲形的情况下，这个圆锥体有 {{mvar|m}} 层，并且轴 {{math|''ζ'' {{=}} ''λξ''}} 在这些层中运动: 它不与任何一层相交。但是当从原点偏离η时，这条轴线与每一层都相交。在椭圆形的情况下，法向圆锥没有实层。&lt;br /&gt;
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==[[用户:Yuling|Yuling]]（[[用户讨论:Yuling|讨论]]） sheet 这个单词也不很理解，我直译为了“层”&lt;br /&gt;
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=== Equations of mixed type ===&lt;br /&gt;
混合型方程&lt;br /&gt;
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If a PDE has coefficients that are not constant, it is possible that it will not belong to any of these categories but rather be of '''mixed type'''. A simple but important example is the [[Euler–Tricomi equation]]&lt;br /&gt;
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If a PDE has coefficients that are not constant, it is possible that it will not belong to any of these categories but rather be of mixed type. A simple but important example is the Euler–Tricomi equation&lt;br /&gt;
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如果偏微分方程的系数不是常数，那么它可能不属于这些类别中的任何一个，而是属于混合类型。一个简单但重要的例子是欧拉-特里科米方程&lt;br /&gt;
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: &amp;lt;math&amp;gt;u_{xx} = xu_{yy},&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;u_{xx} = xu_{yy},&amp;lt;/math&amp;gt;&lt;br /&gt;
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which is called '''elliptic-hyperbolic''' because it is elliptic in the region {{math|''x'' &amp;lt; 0}}, hyperbolic in the region {{math|''x'' &amp;gt; 0}}, and degenerate parabolic on the line {{math|''x'' {{=}} 0}}.&lt;br /&gt;
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which is called elliptic-hyperbolic because it is elliptic in the region , hyperbolic in the region , and degenerate parabolic on the line  0}}.&lt;br /&gt;
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它在 {{math|''x'' &amp;lt; 0}} 的区域上是椭圆形，在 {{math|''x'' &amp;gt; 0}} 区域上是双曲形，在 {{math|''x'' {{=}} 0}}这条线上是退化为抛物线形，因此称之为椭圆-双曲型。&lt;br /&gt;
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''fill in: Dirichlet and Neumann boundaries, hyperbolic/parabolic/elliptic separation of variables, [[Fourier analysis]], [[Green's function]]s ...--&amp;gt;&lt;br /&gt;
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fill in: Dirichlet and Neumann boundaries, hyperbolic/parabolic/elliptic separation of variables, Fourier analysis, Green's functions ...--&amp;gt;&lt;br /&gt;
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填写: Dirichlet 和 Neumann 边界，双曲 / 抛物线 / 椭圆分离变量法，傅立叶分析，Green 函数... --&lt;br /&gt;
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=== Infinite-order PDEs in quantum mechanics ===&lt;br /&gt;
量子力学中的无限阶偏微分方程&lt;br /&gt;
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In the [[phase space formulation]] of quantum mechanics,  one may consider the [[Method of quantum characteristics|quantum Hamilton's equations]] for trajectories of quantum particles. These equations are infinite-order PDEs. However, in the semiclassical expansion, one has a finite system of ODEs at any fixed order of [[Dirac constant|{{mvar|ħ}}]].  The evolution equation of the [[Wigner quasi-probability distribution|c]] is also an infinite-order PDE. The quantum trajectories are [[Method of quantum characteristics|quantum characteristics]], with the use of which one could calculate the evolution of the Wigner function.&lt;br /&gt;
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In the phase space formulation of quantum mechanics,  one may consider the quantum Hamilton's equations for trajectories of quantum particles. These equations are infinite-order PDEs. However, in the semiclassical expansion, one has a finite system of ODEs at any fixed order of Dirac constant|.  The evolution equation of the Wigner function is also an infinite-order PDE. The quantum trajectories are quantum characteristics, with the use of which one could calculate the evolution of the Wigner function.&lt;br /&gt;
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在量子力学中的相空间表述中，我们可以考虑用于求解量子粒子的轨迹的量子哈密顿的方程。这些方程是无限阶偏微分方程。然而，在半经典展开中，我们在给定[[Dirac constant|{{mvar|ħ}}]]阶数下有一个有限的的常微分方程组。'''&amp;lt;font color=&amp;quot;#ff8000&amp;quot;&amp;gt;维格纳函数  Wigner Function&amp;lt;/font&amp;gt;的演化方程也是一个无限阶偏微分方程。由于量子轨道的量子特性，所以它通常可以用来计算维格纳函数的演化。&lt;br /&gt;
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== Analytical solutions ==&lt;br /&gt;
解析解&lt;br /&gt;
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===Separation of variables===&lt;br /&gt;
分离变量法&lt;br /&gt;
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{{main|Separable partial differential equation}}&lt;br /&gt;
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Linear PDEs can be reduced to systems of ordinary differential equations by the important technique of separation of variables. This technique rests on a characteristic of solutions to differential equations: if one can find any solution that solves the equation and satisfies the boundary conditions, then it is ''the'' solution (this also applies to ODEs). We assume as an [[ansatz]] that the dependence of a solution on the parameters space and time can be written as a product of terms that each depend on a single parameter, and then see if this can be made to solve the problem.&amp;lt;ref&amp;gt;{{cite book|last1=Gershenfeld|first1=Neil|title=The nature of mathematical modeling|date=2000|publisher=Cambridge Univ. Press|location=Cambridge|isbn=0521570956|page=27|edition=Reprinted (with corr.)}}&amp;lt;/ref&amp;gt;&lt;br /&gt;
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Linear PDEs can be reduced to systems of ordinary differential equations by the important technique of separation of variables. This technique rests on a characteristic of solutions to differential equations: if one can find any solution that solves the equation and satisfies the boundary conditions, then it is the solution (this also applies to ODEs). We assume as an ansatz that the dependence of a solution on the parameters space and time can be written as a product of terms that each depend on a single parameter, and then see if this can be made to solve the problem.&lt;br /&gt;
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线性偏微分方程组可以通过分离变量法这一重要方法来简化为常微分方程组。这种方法依赖于微分方程解的一个特征: 如果能找到任何一个满足方程和边界条件的解，那么这个解就是方程的解(这也适用于常微分方程)。我们假设解对参数空间和时间的依赖可以写成对它们每一项的依赖以及一个参数的乘积，然后再看看这是否可以用来解决这个问题。&lt;br /&gt;
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In the method of separation of variables, one reduces a PDE to a PDE in fewer variables, which is an ordinary differential equation if in one variable – these are in turn easier to solve.&lt;br /&gt;
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In the method of separation of variables, one reduces a PDE to a PDE in fewer variables, which is an ordinary differential equation if in one variable – these are in turn easier to solve.&lt;br /&gt;
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在分离变量法方法中，可以将偏微分方程简化为含有更少变量的偏微分方程，如果只有一个变量，那么就变成了一个'''&amp;lt;font color = &amp;quot;#ff8000&amp;quot;&amp;gt;常微分方程 Ordinary Differential Equation&amp;lt;/font&amp;gt;'''-- 反过来，这些方程也更容易求解。&lt;br /&gt;
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This is possible for simple PDEs, which are called [[separable partial differential equation]]s, and the domain is generally a rectangle (a product of intervals). Separable PDEs correspond to [[diagonal matrices]] – thinking of &amp;quot;the value for fixed {{mvar|x}}&amp;quot; as a coordinate, each coordinate can be understood separately.&lt;br /&gt;
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This is possible for simple PDEs, which are called separable partial differential equations, and the domain is generally a rectangle (a product of intervals). Separable PDEs correspond to diagonal matrices – thinking of &amp;quot;the value for fixed &amp;quot; as a coordinate, each coordinate can be understood separately.&lt;br /&gt;
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对于简单的偏微分方程(称为可分离偏微分方程)来说，这是可能的，而且方程通常定义在一个矩形区域(区间的乘积)上。可分离偏微分方程对应于对角线矩阵——以“固定值”为坐标，每个坐标可分开理解。&lt;br /&gt;
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This generalizes to the [[method of characteristics]], and is also used in [[integral transform]]s.&lt;br /&gt;
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This generalizes to the method of characteristics, and is also used in integral transforms.&lt;br /&gt;
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这种方法可以推广到特征曲线法，也可以用于积分变换。&lt;br /&gt;
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===Method of characteristics===&lt;br /&gt;
特征曲线法&lt;br /&gt;
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{{main|Method of characteristics}}&lt;br /&gt;
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In special cases, one can find characteristic curves on which the equation reduces to an ODE – changing coordinates in the domain to straighten these curves allows separation of variables, and is called the [[method of characteristics]].&lt;br /&gt;
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In special cases, one can find characteristic curves on which the equation reduces to an ODE – changing coordinates in the domain to straighten these curves allows separation of variables, and is called the method of characteristics.&lt;br /&gt;
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在特殊情况下，可以找到一些特征曲线，在这些曲线上方程可以变成一个常微分方程——意味着改变坐标从而使这些曲线变直从而达到分离变量的目的，这就是所谓的特征曲线法。&lt;br /&gt;
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More generally, one may find characteristic surfaces.&lt;br /&gt;
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More generally, one may find characteristic surfaces.&lt;br /&gt;
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更一般地说，人们可能会找到特征表面。&lt;br /&gt;
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===Integral transform===&lt;br /&gt;
积分变换&lt;br /&gt;
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An [[integral transform]] may transform the PDE to a simpler one, in particular, a separable PDE. This corresponds to diagonalizing an operator.&lt;br /&gt;
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An integral transform may transform the PDE to a simpler one, in particular, a separable PDE. This corresponds to diagonalizing an operator.&lt;br /&gt;
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积分变换可以将偏微分方程转换为更简单的偏微分方程，特别是可分离的偏微分方程。这对应于对角化算符。&lt;br /&gt;
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An important example of this is [[Fourier analysis]], which diagonalizes the heat equation using the [[eigenbasis]] of sinusoidal waves.&lt;br /&gt;
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An important example of this is Fourier analysis, which diagonalizes the heat equation using the eigenbasis of sinusoidal waves.&lt;br /&gt;
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这方面的一个重要例子是'''&amp;lt;font color = &amp;quot;#ff8000&amp;quot;&amp;gt;傅里叶分析  Fourier Analysis&amp;lt;/font&amp;gt;'''，它使用正弦波的特征基来对角化热方程。&lt;br /&gt;
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If the domain is finite or periodic, an infinite sum of solutions such as a [[Fourier series]] is appropriate, but an integral of solutions such as a [[Fourier integral]] is generally required for infinite domains. The solution for a point source for the heat equation given above is an example of the use of a Fourier integral.&lt;br /&gt;
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If the domain is finite or periodic, an infinite sum of solutions such as a Fourier series is appropriate, but an integral of solutions such as a Fourier integral is generally required for infinite domains. The solution for a point source for the heat equation given above is an example of the use of a Fourier integral.&lt;br /&gt;
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如果区域是有限的或周期性的，那么解为无限和的形式是恰当的，例如傅里叶级数，但是一个解的积分，例如傅立叶积分，一般是在无限区域上的。上面给出的热传导方程的点源解法就是使用傅里叶积分的一个例子。&lt;br /&gt;
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===Change of variables===&lt;br /&gt;
变量代换&lt;br /&gt;
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Often a PDE can be reduced to a simpler form with a known solution by a suitable [[Change of variables (PDE)|change of variables]].  For example, the [[Black–Scholes equation#Derivation|Black–Scholes]] PDE&lt;br /&gt;
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Often a PDE can be reduced to a simpler form with a known solution by a suitable change of variables.  For example, the Black–Scholes PDE&lt;br /&gt;
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偏微分方程通常可以通过变量的适当变化，用已知的解简化为更简单的形式。例如，布莱克-舒尔斯偏微分方程&lt;br /&gt;
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:&amp;lt;math&amp;gt; \frac{\partial V}{\partial t} + \tfrac{1}{2}\sigma^2 S^2\frac{\partial^2 V}{\partial S^2} + rS\frac{\partial V}{\partial S} - rV = 0 &amp;lt;/math&amp;gt;&lt;br /&gt;
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&amp;lt;math&amp;gt; \frac{\partial V}{\partial t} + \tfrac{1}{2}\sigma^2 S^2\frac{\partial^2 V}{\partial S^2} + rS\frac{\partial V}{\partial S} - rV = 0 &amp;lt;/math&amp;gt;&lt;br /&gt;
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is reducible to the [[heat equation]]&lt;br /&gt;
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is reducible to the heat equation&lt;br /&gt;
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可以简化为热传导方程&lt;br /&gt;
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:&amp;lt;math&amp;gt; \frac{\partial u}{\partial \tau} = \frac{\partial^2 u}{\partial x^2}&amp;lt;/math&amp;gt;&lt;br /&gt;
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&amp;lt;math&amp;gt; \frac{\partial u}{\partial \tau} = \frac{\partial^2 u}{\partial x^2}&amp;lt;/math&amp;gt;&lt;br /&gt;
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by the change of variables (for complete details see {{webarchive |url=https://web.archive.org/web/20080411030405/http://www.math.unl.edu/~sdunbar1/Teaching/MathematicalFinance/Lessons/BlackScholes/Solution/solution.shtml |date=April 11, 2008 |title=Solution of the Black Scholes Equation }})&lt;br /&gt;
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by the change of variables (for complete details see )&lt;br /&gt;
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通过变量替换(完整的细节见)&lt;br /&gt;
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:&amp;lt;math&amp;gt;\begin{align}&lt;br /&gt;
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V(S,t) &amp;amp;= K v(x,\tau),\\[5px]&lt;br /&gt;
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x &amp;amp;= \ln\left(\tfrac{S}{K} \right),\\[5px]&lt;br /&gt;
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\tau &amp;amp;= \tfrac{1}{2} \sigma^2 (T - t),\\[5px]&lt;br /&gt;
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v(x,\tau)&amp;amp;=e^{-\alpha x-\beta\tau} u(x,\tau).&lt;br /&gt;
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\end{align}&amp;lt;/math&amp;gt;&lt;br /&gt;
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===Fundamental solution===&lt;br /&gt;
基本解&lt;br /&gt;
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{{main|Fundamental solution}}&lt;br /&gt;
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Inhomogeneous equations can often be solved (for constant coefficient PDEs, always be solved) by finding the [[fundamental solution]] (the solution for a point source), then taking the [[convolution]] with the boundary conditions to get the solution.&lt;br /&gt;
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Inhomogeneous equations can often be solved (for constant coefficient PDEs, always be solved) by finding the fundamental solution (the solution for a point source), then taking the convolution with the boundary conditions to get the solution.&lt;br /&gt;
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非齐次方程(常系数偏微分方程)一般是通过先求出基本解(点源的解) ，然后利用带边界条件的卷积来求解。&lt;br /&gt;
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This is analogous in [[signal processing]] to understanding a filter by its [[impulse response]].&lt;br /&gt;
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This is analogous in signal processing to understanding a filter by its impulse response.&lt;br /&gt;
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这类似于在信号处理中通过滤波器的脉冲响应来理解滤波器。&lt;br /&gt;
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===Superposition principle===&lt;br /&gt;
叠加原理&lt;br /&gt;
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{{further| Superposition principle }}&lt;br /&gt;
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The superposition principle applies to any linear system, including linear systems of PDEs. A common visualization of this concept is the interaction of two waves in phase being combined to result in a greater amplitude, for example {{math|sin ''x'' + sin ''x'' {{=}} 2 sin ''x''}}. The same principle can be observed in PDEs where the solutions may be real or complex and additive. [[Superposition principle|superposition]]&lt;br /&gt;
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The superposition principle applies to any linear system, including linear systems of PDEs. A common visualization of this concept is the interaction of two waves in phase being combined to result in a greater amplitude, for example  2 sin x}}. The same principle can be observed in PDEs where the solutions may be real or complex and additive. superposition&lt;br /&gt;
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'''&amp;lt;font color = &amp;quot;#ff8000&amp;quot;&amp;gt;叠加原理 Superposition Principle&amp;lt;/font&amp;gt;适用于任何线性系统，包括偏微分方程的线性系统。这个概念的一个常见的可视化是两个同相位的波相互作用结合在一起会产生更大的振幅，例如 {{math|sin ''x'' + sin ''x'' {{=}} 2 sin ''x''}}。在偏微分方程中也可以观察到同样的原理，其中的解可能是真实的或复杂的和可加的。叠加&lt;br /&gt;
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If {{math|''u''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;}} and {{math|''u''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;}} are solutions of linear PDE in some function space {{mvar|R}}, then {{math|''u'' {{=}} ''c''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;''u''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; + ''c''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;''u''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;}} with any constants {{math|''c''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;}} and {{math|''c''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;}} are also a solution of that PDE in the same function space.&lt;br /&gt;
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If  and  are solutions of linear PDE in some function space , then  c&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;u&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; + c&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;u&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;}} with any constants  and  are also a solution of that PDE in the same function space.&lt;br /&gt;
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若线性偏微分方程在某个函数空间{{mvar|R}}中有解{{math|''u''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;}} 和 {{math|''u''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;}}，则{{math|''u'' {{=}} ''c''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;''u''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; + ''c''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;''u''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;}}也是该偏微分方程在同一函数空间中的解，其中{{math|''c''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;}} 和 {{math|''c''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;}} 是任意常数。&lt;br /&gt;
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===Methods for non-linear equations===&lt;br /&gt;
非线性方程的求解方法&lt;br /&gt;
{{see also|nonlinear partial differential equation}}&lt;br /&gt;
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There are no generally applicable methods to solve nonlinear PDEs. Still, existence and uniqueness results (such as the [[Cauchy–Kowalevski theorem]]) are often possible, as are proofs of important qualitative and quantitative properties of solutions (getting these results is a major part of [[mathematical analysis|analysis]]). Computational solution to the nonlinear PDEs, the [[split-step method]], exist for specific equations like [[nonlinear Schrödinger equation]].&lt;br /&gt;
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There are no generally applicable methods to solve nonlinear PDEs. Still, existence and uniqueness results (such as the Cauchy–Kowalevski theorem) are often possible, as are proofs of important qualitative and quantitative properties of solutions (getting these results is a major part of analysis). Computational solution to the nonlinear PDEs, the split-step method, exist for specific equations like nonlinear Schrödinger equation.&lt;br /&gt;
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对于非线性偏微分方程，目前还没有普遍适用的求解方法。然而，通常是可能知道解的存在性和唯一性(如柯西-科瓦列夫斯基定理)，也是可能得到解的重要定性和定量性质的证明(得到这些结果是分析的主要部分)。非线性偏微分方程的计算解，即分步法，对一些特定的方程适用，比如非线性'''&amp;lt;font color=&amp;quot;#ff8000&amp;quot;&amp;gt;薛定谔方程 Schrödinger equation&amp;lt;/font&amp;gt;'''。&lt;br /&gt;
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Nevertheless, some techniques can be used for several types of equations. The [[h-principle|{{mvar|h}}-principle]] is the most powerful method to solve [[Underdetermined system|underdetermined]] equations. The [[Riquier–Janet theory]] is an effective method for obtaining information about many analytic [[Overdetermined system|overdetermined]] systems.&lt;br /&gt;
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Nevertheless, some techniques can be used for several types of equations. The -principle is the most powerful method to solve underdetermined equations. The Riquier–Janet theory is an effective method for obtaining information about many analytic overdetermined systems.&lt;br /&gt;
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然而，一些技巧可以用于几种类型的方程。h-原理是求解欠定方程最有效的方法。里基尔-珍妮特理论是一种可以获得许多解析超定系统信息的有效方法。&lt;br /&gt;
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The [[method of characteristics]] can be used in some very special cases to solve partial differential equations.&lt;br /&gt;
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The method of characteristics can be used in some very special cases to solve partial differential equations.&lt;br /&gt;
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特征线法可用于求解某些特殊情况下的偏微分方程。&lt;br /&gt;
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In some cases, a PDE can be solved via [[perturbation analysis]] in which the solution is considered to be a correction to an equation with a known solution. Alternatives are [[numerical analysis]] techniques from simple [[finite difference]] schemes to the more mature [[multigrid]] and [[finite element method]]s. Many interesting problems in science and engineering are solved in this way using [[computer]]s, sometimes high performance [[supercomputer]]s.&lt;br /&gt;
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In some cases, a PDE can be solved via perturbation analysis in which the solution is considered to be a correction to an equation with a known solution. Alternatives are numerical analysis techniques from simple finite difference schemes to the more mature multigrid and finite element methods. Many interesting problems in science and engineering are solved in this way using computers, sometimes high performance supercomputers.&lt;br /&gt;
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在某些情况下，偏微分方程可以通过扰动分析来求解。在扰动分析中，通常是求解将具有已知解的方程修正后的新得到方程。可供选择的数值分析技术从简单的差分格式到更成熟的多重网格和有限元方法。许多有趣的科学和工程问题都是在计算机上用这种方法解决的，有时是高性能超级计算机。&lt;br /&gt;
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===Lie group method===&lt;br /&gt;
李群方法&lt;br /&gt;
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From 1870 [[Sophus Lie]]'s work put the theory of differential equations on a more satisfactory foundation. He showed that the integration theories of the older mathematicians can, by the introduction of what are now called [[Lie group]]s, be referred, to a common source; and that ordinary differential equations which admit the same [[infinitesimal transformation]]s present comparable difficulties of integration. He also emphasized the subject of [[contact transformation|transformations of contact]].&lt;br /&gt;
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From 1870 Sophus Lie's work put the theory of differential equations on a more satisfactory foundation. He showed that the integration theories of the older mathematicians can, by the introduction of what are now called Lie groups, be referred, to a common source; and that ordinary differential equations which admit the same infinitesimal transformations present comparable difficulties of integration. He also emphasized the subject of transformations of contact.&lt;br /&gt;
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从1870年起，索弗斯·李的工作为微分方程理论奠定了一个较为令人满意的基础。他指出，通过引入现在所谓的李群，老一辈数学家的积分理论可以引用到一个共同的来源; 承认相同的无穷小变换的常微分方程在积分方面存在相当的困难。他还强调了接触的转变这一主题。&lt;br /&gt;
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==[[用户:Yuling|Yuling]]（[[用户讨论:Yuling|讨论]]）这句话“He also emphasized the subject of transformations of contact.”中的transformations of contact翻译的不太好。&lt;br /&gt;
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A general approach to solving PDEs uses the symmetry property of differential equations, the continuous [[infinitesimal transformation]]s of solutions to solutions ([[Lie theory]]). Continuous [[group theory]], [[Lie algebras]] and [[differential geometry]] are used to understand the structure of linear and nonlinear partial differential equations for generating integrable equations, to find its [[Lax pair]]s, recursion operators, [[Bäcklund transform]] and finally finding exact analytic solutions to the PDE.&lt;br /&gt;
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A general approach to solving PDEs uses the symmetry property of differential equations, the continuous infinitesimal transformations of solutions to solutions (Lie theory). Continuous group theory, Lie algebras and differential geometry are used to understand the structure of linear and nonlinear partial differential equations for generating integrable equations, to find its Lax pairs, recursion operators, Bäcklund transform and finally finding exact analytic solutions to the PDE.&lt;br /&gt;
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求解偏微分方程的一般方法是利用微分方程的对称性，即解到解的连续无穷小变换(李理论)。连续群论、李代数和微分几何理论被用来理解生成可积方程的线性和非线性偏微分方程的结构，找到它的Lax对、递归算子、 贝克伦德变换，最后找到偏微分方程的精确解析解。&lt;br /&gt;
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Symmetry methods have been recognized to study differential equations arising in mathematics, physics, engineering, and many other disciplines.&lt;br /&gt;
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Symmetry methods have been recognized to study differential equations arising in mathematics, physics, engineering, and many other disciplines.&lt;br /&gt;
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对称方法已被公认可以用于研究出现在数学，物理，工程和许多其他学科的微分方程。&lt;br /&gt;
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===Semianalytical methods===&lt;br /&gt;
半解析方法&lt;br /&gt;
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The [[Adomian decomposition method]], the [[Aleksandr Lyapunov|Lyapunov]] artificial small parameter method, and He's [[homotopy perturbation method]] are all special cases of the more general [[homotopy analysis method]]. These are series expansion methods, and except for the Lyapunov method, are independent of small physical parameters as compared to the well known [[perturbation theory]], thus giving these methods greater flexibility and solution generality.&lt;br /&gt;
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The Adomian decomposition method, the Lyapunov artificial small parameter method, and He's homotopy perturbation method are all special cases of the more general homotopy analysis method. These are series expansion methods, and except for the Lyapunov method, are independent of small physical parameters as compared to the well known perturbation theory, thus giving these methods greater flexibility and solution generality.&lt;br /&gt;
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阿多米安分解法、李雅普诺夫人工小参数方法和何同伦摄动方法都是更一般的同伦分析方法的特殊情况。除了李雅普诺夫方法之外，这些都是级数展开方法，与为人熟知的摄动理论方法相比，它们与小的物理参数无关，因此这些方法具有更大的灵活性和解的通用性。&lt;br /&gt;
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== Numerical solutions ==&lt;br /&gt;
数值解&lt;br /&gt;
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The three most widely used [[Numerical partial differential equations|numerical methods to solve PDEs]] are the [[finite element analysis|finite element method]] (FEM), [[finite volume method]]s (FVM) and [[finite difference method]]s (FDM), as well other kind of methods called [[Meshfree methods]], which were made to solve problems where the before mentioned methods are limited. The FEM has a prominent position among these methods and especially its exceptionally efficient higher-order version [[hp-FEM]]. Other hybrid versions of FEM and Meshfree methods include the generalized finite element method (GFEM), [[extended finite element method]] (XFEM), [[Spectral element method|spectral finite element method]] (SFEM), [[Meshfree methods|meshfree finite element method]], [[Discontinuous Galerkin Method|discontinuous Galerkin finite element method]] (DGFEM), [[Element-Free Galerkin Method]] (EFGM), [[Interpolating Element-Free Galerkin Method]] (IEFGM), etc.&lt;br /&gt;
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The three most widely used numerical methods to solve PDEs are the finite element method (FEM), finite volume methods (FVM) and finite difference methods (FDM), as well other kind of methods called Meshfree methods, which were made to solve problems where the before mentioned methods are limited. The FEM has a prominent position among these methods and especially its exceptionally efficient higher-order version hp-FEM. Other hybrid versions of FEM and Meshfree methods include the generalized finite element method (GFEM), extended finite element method (XFEM), spectral finite element method (SFEM), meshfree finite element method, discontinuous Galerkin finite element method (DGFEM), Element-Free Galerkin Method (EFGM), Interpolating Element-Free Galerkin Method (IEFGM), etc.&lt;br /&gt;
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求解偏微分方程最常用的三种数值方法是有限元分析法、有限体积法和有限差分法，以及其他一些称为无网格法的方法。这些方法用于解决前面提到的方法受到的限制。在这些方法中，有限元方法，尤其是高效的高阶有限元方法，占有重要地位。其他有限元法和无网格法的混合形式包括广义有限元分析法(GFEM)、扩展有限元分析法(XFEM)、谱有限元分析法(SFEM)、无网格有限元分析法(DGFEM)、间断伽辽金有限元分析法(DGFEM)、无网格伽辽金法(EFGM)、插值无网格伽辽金法(IEFGM)等。&lt;br /&gt;
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=== Finite element method ===&lt;br /&gt;
有限元分析法&lt;br /&gt;
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{{main|Finite element method}}&lt;br /&gt;
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The finite element method (FEM) (its practical application often known as finite element analysis (FEA)) is a numerical technique for finding approximate solutions of partial differential equations (PDE) as well as of integral equations. The solution approach is based either on eliminating the differential equation completely (steady state problems), or rendering the PDE into an approximating system of ordinary differential equations, which are then numerically integrated using standard techniques such as Euler's method, Runge–Kutta, etc.&lt;br /&gt;
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The finite element method (FEM) (its practical application often known as finite element analysis (FEA)) is a numerical technique for finding approximate solutions of partial differential equations (PDE) as well as of integral equations. The solution approach is based either on eliminating the differential equation completely (steady state problems), or rendering the PDE into an approximating system of ordinary differential equations, which are then numerically integrated using standard techniques such as Euler's method, Runge–Kutta, etc.&lt;br /&gt;
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'''&amp;lt;font color = &amp;quot;#ff8000&amp;quot;&amp;gt;有限元分析法 Finite Element Method&amp;lt;/font&amp;gt;''' ((其实际应用通常被称为有限元分析(FEA))是一种寻找偏微分方程(PDE)和积分方程近似解的数值技术。这种求解方法要么基于完全消除微分方程(稳态问题) ，要么将偏微分方程转化为常微分方程的近似系统，然后使用标准技术进行数值积分，如欧拉方法、 Runge-Kutta 等。&lt;br /&gt;
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===Finite difference method===&lt;br /&gt;
有限差分法&lt;br /&gt;
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{{main|Finite difference method}}&lt;br /&gt;
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Finite-difference methods are numerical methods for approximating the solutions to differential equations using [[finite difference]] equations to approximate derivatives.&lt;br /&gt;
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Finite-difference methods are numerical methods for approximating the solutions to differential equations using finite difference equations to approximate derivatives.&lt;br /&gt;
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有限差分法是一种数值方法，用差分方程近似微分方程的解。&lt;br /&gt;
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=== Finite volume method ===&lt;br /&gt;
有限体积法&lt;br /&gt;
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{{main|Finite volume method}}&lt;br /&gt;
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Similar to the finite difference method or finite element method, values are calculated at discrete places on a meshed geometry. &amp;quot;Finite volume&amp;quot; refers to the small volume surrounding each node point on a mesh. In the finite volume method, surface integrals in a partial differential equation that contain a divergence term are converted to volume integrals, using the [[divergence theorem]]. These terms are then evaluated as fluxes at the surfaces of each finite volume. Because the flux entering a given volume is identical to that leaving the adjacent volume, these methods conserve mass by design.&lt;br /&gt;
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Similar to the finite difference method or finite element method, values are calculated at discrete places on a meshed geometry. &amp;quot;Finite volume&amp;quot; refers to the small volume surrounding each node point on a mesh. In the finite volume method, surface integrals in a partial differential equation that contain a divergence term are converted to volume integrals, using the divergence theorem. These terms are then evaluated as fluxes at the surfaces of each finite volume. Because the flux entering a given volume is identical to that leaving the adjacent volume, these methods conserve mass by design.&lt;br /&gt;
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类似于有限差分法或有限元分析，函数值是在网状几何体上的离散位置进行计算的。“有限体积”是指网格上每个节点周围的小体积。在有限体积法中，偏微分方程中含有散度项的面积分用散度定理积分转换成体积分。然后将这些项用于估算每个有限体积表面上的通量。由于进入给定体积的通量与转移到相邻体积元的通量相同，所以这些方法在设计上保证了质量守恒。&lt;br /&gt;
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==See also==&lt;br /&gt;
请参阅&lt;br /&gt;
* [[Dirichlet boundary condition]]&lt;br /&gt;
狄利克雷边界条件&lt;br /&gt;
* [[Jet bundle]]&lt;br /&gt;
射流丛&lt;br /&gt;
* [[Laplace transform applied to differential equations]]&lt;br /&gt;
微分方程中的拉普拉斯变换&lt;br /&gt;
* [[List of dynamical systems and differential equations topics]]&lt;br /&gt;
动力学系统列表和微分方程主题&lt;br /&gt;
* [[Matrix differential equation]]&lt;br /&gt;
矩阵微分方程&lt;br /&gt;
* [[Neumann boundary condition]]&lt;br /&gt;
诺伊曼边界条件&lt;br /&gt;
* [[Numerical partial differential equations]]&lt;br /&gt;
数值偏微分方程&lt;br /&gt;
* [[Partial differential algebraic equation]]&lt;br /&gt;
偏微分代数方程&lt;br /&gt;
* [[Recurrence relation]]&lt;br /&gt;
递推关系&lt;br /&gt;
* [[Robin boundary condition]]&lt;br /&gt;
罗宾边界条件&lt;br /&gt;
* [[Stochastic processes and boundary value problems]]&lt;br /&gt;
随机过程和边值问题&lt;br /&gt;
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== The energy method ==&lt;br /&gt;
能量法&lt;br /&gt;
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The energy method is a mathematical procedure that can be used to verify well-posedness of initial-boundary-value-problems.&amp;lt;ref&amp;gt;{{cite book |title=High Order Difference Methods for Time Dependent PDE&lt;br /&gt;
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The energy method is a mathematical procedure that can be used to verify well-posedness of initial-boundary-value-problems.&amp;lt;ref&amp;gt;{{cite book |title=High Order Difference Methods for Time Dependent PDE&lt;br /&gt;
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能量法是一种数学过程，可用于验证初始边界值问题的适定性。&lt;br /&gt;
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In the following example the energy method is used to decide where and which boundary conditions should be imposed such that the resulting IBVP is well-posed. Consider the one-dimensional hyperbolic PDE given by&lt;br /&gt;
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In the following example the energy method is used to decide where and which boundary conditions should be imposed such that the resulting IBVP is well-posed. Consider the one-dimensional hyperbolic PDE given by&lt;br /&gt;
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在下面的示例中，将使用能量法决定应在何处施加哪些边界条件，以使得到的IBVP处于适当位置。考虑下式给出的一维双曲PDE&lt;br /&gt;
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: &amp;lt;math&amp;gt;\frac{\partial u}{\partial t} + \alpha \frac{\partial u}{\partial x} = 0, \quad x \in [a,b], \operatorname t &amp;gt; 0,&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;\frac{\partial u}{\partial t} + \alpha \frac{\partial u}{\partial x} = 0, \quad x \in [a,b], \operatorname t &amp;gt; 0,&amp;lt;/math&amp;gt;&lt;br /&gt;
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where &amp;lt;math&amp;gt;\alpha \neq 0&amp;lt;/math&amp;gt; is a constant and &amp;lt;math&amp;gt;u(x,t)&amp;lt;/math&amp;gt; is an unknown function with initial condition &amp;lt;math&amp;gt;u(x,0) = f(x)&amp;lt;/math&amp;gt;. Multiplying with &amp;lt;math&amp;gt;u&amp;lt;/math&amp;gt; and integrating over the domain gives&lt;br /&gt;
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where &amp;lt;math&amp;gt;\alpha \neq 0&amp;lt;/math&amp;gt; is a constant and &amp;lt;math&amp;gt;u(x,t)&amp;lt;/math&amp;gt; is an unknown function with initial condition &amp;lt;math&amp;gt;u(x,0) = f(x)&amp;lt;/math&amp;gt;. Multiplying with &amp;lt;math&amp;gt;u&amp;lt;/math&amp;gt; and integrating over the domain gives&lt;br /&gt;
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其中 &amp;lt;math&amp;gt;\alpha \neq 0&amp;lt;/math&amp;gt; 是常数，并且 &amp;lt;math&amp;gt;u(x,t)&amp;lt;/math&amp;gt; 是初始条件是 &amp;lt;math&amp;gt;u(x,0) = f(x)&amp;lt;/math&amp;gt;的未知函数，乘以 &amp;lt;math&amp;gt;u&amp;lt;/math&amp;gt; 并在域上进行积分。&lt;br /&gt;
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: &amp;lt;math&amp;gt;\int_a^b u \frac{\partial u}{\partial t} \operatorname dx + \alpha \int _a ^b u \frac{\partial u}{\partial x} \operatorname dx = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;\int_a^b u \frac{\partial u}{\partial t} \operatorname dx + \alpha \int _a ^b u \frac{\partial u}{\partial x} \operatorname dx = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
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Using that&lt;br /&gt;
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Using that&lt;br /&gt;
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利用这一点&lt;br /&gt;
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: &amp;lt;math&amp;gt;\int _a ^b u \frac{\partial u}{\partial t} \operatorname dx = \frac{1}{2} \frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 \quad \text{and} \quad \int _a ^b u \frac{\partial u}{\partial x} \operatorname dx = \frac{1}{2} u(b,t)^2 - \frac{1}{2} u(a,t)^2,.&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;\int _a ^b u \frac{\partial u}{\partial t} \operatorname dx = \frac{1}{2} \frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 \quad \text{and} \quad \int _a ^b u \frac{\partial u}{\partial x} \operatorname dx = \frac{1}{2} u(b,t)^2 - \frac{1}{2} u(a,t)^2,.&amp;lt;/math&amp;gt;&lt;br /&gt;
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where integration by parts has been used for the second relationship, we get&lt;br /&gt;
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where integration by parts has been used for the second relationship, we get&lt;br /&gt;
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第二个关系中采用了分部积分法，我们可以得到&lt;br /&gt;
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: &amp;lt;math&amp;gt;\frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 + \alpha u(b,t)^2 - \alpha u(a,t)^2 = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;\frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 + \alpha u(b,t)^2 - \alpha u(a,t)^2 = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
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Here &amp;lt;math&amp;gt;\vert \vert \cdot \vert \vert&amp;lt;/math&amp;gt; denotes the standard L2-norm.&lt;br /&gt;
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Here &amp;lt;math&amp;gt;\vert \vert \cdot \vert \vert&amp;lt;/math&amp;gt; denotes the standard L2-norm.&lt;br /&gt;
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在这里，&amp;lt;math&amp;gt;\vert \vert \cdot \vert \vert&amp;lt;/math&amp;gt; 表示标准的L2-正则。&lt;br /&gt;
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For well-posedness we require that the energy of the solution is non-increasing, i.e. that &amp;lt;math&amp;gt;\frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 \leq 0&amp;lt;/math&amp;gt;, which is achieved by specifying &amp;lt;math&amp;gt;u&amp;lt;/math&amp;gt; at &amp;lt;math&amp;gt;x = a&amp;lt;/math&amp;gt; if &amp;lt;math&amp;gt;\alpha &amp;gt; 0&amp;lt;/math&amp;gt; and at &amp;lt;math&amp;gt;x = b&amp;lt;/math&amp;gt; if &amp;lt;math&amp;gt;\alpha &amp;lt; 0&amp;lt;/math&amp;gt;. This corresponds to only imposing boundary conditions at the inflow. Note that well-posedness allows for growth in terms of data (initial and boundary) and thus it is sufficient to show that &amp;lt;math&amp;gt;\frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 \leq 0&amp;lt;/math&amp;gt; holds when all data is set to zero.&lt;br /&gt;
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For well-posedness we require that the energy of the solution is non-increasing, i.e. that &amp;lt;math&amp;gt;\frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 \leq 0&amp;lt;/math&amp;gt;, which is achieved by specifying &amp;lt;math&amp;gt;u&amp;lt;/math&amp;gt; at &amp;lt;math&amp;gt;x = a&amp;lt;/math&amp;gt; if &amp;lt;math&amp;gt;\alpha &amp;gt; 0&amp;lt;/math&amp;gt; and at &amp;lt;math&amp;gt;x = b&amp;lt;/math&amp;gt; if &amp;lt;math&amp;gt;\alpha &amp;lt; 0&amp;lt;/math&amp;gt;. This corresponds to only imposing boundary conditions at the inflow. Note that well-posedness allows for growth in terms of data (initial and boundary) and thus it is sufficient to show that &amp;lt;math&amp;gt;\frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 \leq 0&amp;lt;/math&amp;gt; holds when all data is set to zero.&lt;br /&gt;
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对于适定性，我们要解的能量是不增加的，即 &amp;lt;math&amp;gt;\frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 \leq 0&amp;lt;/math&amp;gt; ，这种关系可以通过在&amp;lt;math&amp;gt;x = a&amp;lt;/math&amp;gt;处 （如果 &amp;lt;math&amp;gt;\alpha &amp;gt; 0&amp;lt;/math&amp;gt;） 以及 &amp;lt;math&amp;gt;x = b&amp;lt;/math&amp;gt;处 （如果 &amp;lt;math&amp;gt;\alpha &amp;lt; 0&amp;lt;/math&amp;gt;）指定&amp;lt;math&amp;gt;u&amp;lt;/math&amp;gt;的值来实现。这只相当于在入流处附加边界条件。注意，适定性允许在数据(初始和边界)上的增长，因此它足以表明当所有数据设置为零时应有 &amp;lt;math&amp;gt;\frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 \leq 0&amp;lt;/math&amp;gt;。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==[[用户:Yuling|Yuling]]（[[用户讨论:Yuling|讨论]]）“This corresponds to only imposing boundary conditions at the inflow.” 这句话中的inflow不是很理解&lt;br /&gt;
&lt;br /&gt;
==Notes==&lt;br /&gt;
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{{Reflist}}&lt;br /&gt;
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== References ==&lt;br /&gt;
&lt;br /&gt;
{{refbegin|2}}&lt;br /&gt;
&lt;br /&gt;
* {{cite book |title=Solving Frontier problems of Physics: The decomposition method&lt;br /&gt;
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|first=G.|last=Adomian|publisher=Kluwer Academic Publishers|year=1994|isbn=|page=|url=https://books.google.com/books?id=UKPqCAAAQBAJ&amp;amp;printsec=frontcover#v=onepage&amp;amp;q=%22partial%20differential%22&amp;amp;f=false}}&lt;br /&gt;
&lt;br /&gt;
|first=G.|last=Adomian|publisher=Kluwer Academic Publishers|year=1994|isbn=|page=|url=https://books.google.com/books?id=UKPqCAAAQBAJ&amp;amp;printsec=frontcover#v=onepage&amp;amp;q=%22partial%20differential%22&amp;amp;f=false}}&lt;br /&gt;
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&lt;br /&gt;
* {{Citation |first=A. D. |last=Polyanin |first2=V. F. |last2=Zaitsev |lastauthoramp=yes |first3=A. |last3=Moussiaux |title=Handbook of First Order Partial Differential Equations |publisher=Taylor &amp;amp; Francis |location=London |year=2002 |isbn=0-415-27267-X }}.&lt;br /&gt;
&lt;br /&gt;
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&lt;br /&gt;
* {{Citation |first=P. |last=Solin |title=Partial Differential Equations and the Finite Element Method |publisher=J. Wiley &amp;amp; Sons |location=Hoboken, NJ |year=2005 |isbn=0-471-72070-4 }}.&lt;br /&gt;
&lt;br /&gt;
* {{Citation |first=P. |last=Solin |first2=K. |last2=Segeth |lastauthoramp=yes |first3=I. |last3=Dolezel |title=Higher-Order Finite Element Methods |publisher=Chapman &amp;amp; Hall/CRC Press |location=Boca Raton |year=2003 |isbn=1-58488-438-X }}.&lt;br /&gt;
&lt;br /&gt;
* {{Citation |first=H. |last=Stephani |year=1989 |title=Differential Equations: Their Solution Using Symmetries. Edited by M. MacCallum |publisher=Cambridge University Press }}.&lt;br /&gt;
&lt;br /&gt;
* {{cite book |title=Partial Differential Equations and Solitary Waves Theory&lt;br /&gt;
&lt;br /&gt;
|first=Abdul-Majid|last=Wazwaz|publisher=Higher Education Press|year=2009|isbn=978-3-642-00251-9|page=}}&lt;br /&gt;
&lt;br /&gt;
|first=Abdul-Majid|last=Wazwaz|publisher=Higher Education Press|year=2009|isbn=978-3-642-00251-9|page=}}&lt;br /&gt;
&lt;br /&gt;
| first Abdul-Majid | last Wazwaz | publisher Higher Education Press | year 2009 | isbn 978-3-642-00251-9 | page }&lt;br /&gt;
&lt;br /&gt;
* {{cite book |title=Partial Differential Equations Methods and Applications&lt;br /&gt;
&lt;br /&gt;
|first=Abdul-Majid|last=Wazwaz|publisher=A.A. Balkema|year=2002|isbn=90-5809-369-7|page=}}&lt;br /&gt;
&lt;br /&gt;
|first=Abdul-Majid|last=Wazwaz|publisher=A.A. Balkema|year=2002|isbn=90-5809-369-7|page=}}&lt;br /&gt;
&lt;br /&gt;
| first Abdul-Majid | last Wazwaz | publisher a.a.Balkema | year 2002 | isbn 90-5809-369-7 | page }&lt;br /&gt;
&lt;br /&gt;
* {{Citation |first=D. |last=Zwillinger |title=Handbook of Differential Equations |publisher=Academic Press |location=Boston |year=1997 |edition=3rd |isbn=0-12-784395-7 }}.&lt;br /&gt;
&lt;br /&gt;
* {{Citation |authorlink=Neil Gershenfeld |first=N. |last=Gershenfeld |title=The Nature of Mathematical Modeling |location=New York |publisher=Cambridge University Press, New York, NY, USA |year=1999 |edition=1st |isbn=0-521-57095-6 }}.&lt;br /&gt;
&lt;br /&gt;
* {{Citation |first=I.S. |last=Krasil'shchik |lastauthoramp=yes |first2=A.M., Eds. |last2=Vinogradov |title=Symmetries and Conserwation Laws for Differential Equations of Mathematical Physics |publisher=American Mathematical Society, Providence, Rhode Island, USA |year=1999 |isbn=0-8218-0958-X }}.&lt;br /&gt;
&lt;br /&gt;
* {{Citation |first=I.S. |last=Krasil'shchik |first2=V.V. |last2=Lychagin|lastauthoramp=yes |first3=A.M. |last3=Vinogradov |title=Geometry of Jet Spaces and Nonlinear Partial Differential Equations |publisher=Gordon and Breach Science Publishers, New York, London, Paris, Montreux, Tokyo |year=1986 |isbn=2-88124-051-8 }}.&lt;br /&gt;
&lt;br /&gt;
* {{Citation |first=A.M. |last=Vinogradov |title=Cohomological Analysis of Partial Differential Equations and Secondary Calculus |publisher=American Mathematical Society, Providence, Rhode Island, USA |year=2001 |isbn=0-8218-2922-X }}.&lt;br /&gt;
&lt;br /&gt;
* {{cite book |title=High Order Difference Methods for Time Dependent PDE&lt;br /&gt;
&lt;br /&gt;
|first=Bertil|last=Gustafsson|publisher=Springer|year=2008|isbn=978-3-540-74992-9|doi=10.1007/978-3-540-74993-6}}&lt;br /&gt;
&lt;br /&gt;
|first=Bertil|last=Gustafsson|publisher=Springer|year=2008|isbn=978-3-540-74992-9|doi=10.1007/978-3-540-74993-6}}&lt;br /&gt;
&lt;br /&gt;
| first Bertil | last Gustafsson | Springer | year 2008 | isbn 978-3-540-74992-9 | doi 10.1007 / 978-3-540-74993-6}&lt;br /&gt;
&lt;br /&gt;
{{refend}}&lt;br /&gt;
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== Further reading ==&lt;br /&gt;
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* {{Cite journal|last=Cajori|first=Florian|authorlink=Florian Cajori|year=1928|title=The Early History of Partial Differential Equations and of Partial Differentiation and Integration|url=http://www.math.harvard.edu/archive/21a_fall_14/exhibits/cajori/cajori.pdf|journal=The American Mathematical Monthly|volume=35|issue=9|pages=459–467|doi=10.2307/2298771|access-date=2016-05-15|archive-url=https://web.archive.org/web/20181123102253/http://www.math.harvard.edu/archive/21a_fall_14/exhibits/cajori/cajori.pdf|archive-date=2018-11-23|url-status=dead}}&lt;br /&gt;
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== External links ==&lt;br /&gt;
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{{Sister project links| wikt=no | commons=Category:Solutions of PDE | b=Partial Differential Equations | n=no | q=Partial differential equation | s=no | v=no | voy=no | species=no | d=no}}&lt;br /&gt;
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* {{springer|title=Differential equation, partial|id=p/d031920}}&lt;br /&gt;
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* [http://eqworld.ipmnet.ru/en/pde-en.htm Partial Differential Equations: Exact Solutions] at EqWorld: The World of Mathematical Equations.&lt;br /&gt;
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* [http://eqworld.ipmnet.ru/en/solutions/eqindex/eqindex-pde.htm Partial Differential Equations: Index] at EqWorld: The World of Mathematical Equations.&lt;br /&gt;
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* [http://eqworld.ipmnet.ru/en/methods/meth-pde.htm Partial Differential Equations: Methods] at EqWorld: The World of Mathematical Equations.&lt;br /&gt;
&lt;br /&gt;
* [https://web.archive.org/web/20170701144823/http://www.exampleproblems.com/wiki/index.php?title=Partial_Differential_Equations Example problems with solutions] at exampleproblems.com&lt;br /&gt;
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* [http://mathworld.wolfram.com/PartialDifferentialEquation.html Partial Differential Equations] at mathworld.wolfram.com&lt;br /&gt;
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* [https://reference.wolfram.com/language/FEMDocumentation/tutorial/SolvingPDEwithFEM.html Partial Differential Equations] with Mathematica&lt;br /&gt;
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* [http://www.mathworks.com/moler/pdes.pdf Partial Differential Equations] in Cleve Moler: Numerical Computing with MATLAB&lt;br /&gt;
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* [http://www.nag.com/numeric/fl/nagdoc_fl24/html/D03/d03intro.html Partial Differential Equations] at nag.com&lt;br /&gt;
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* {{cite web |first=Grant |last=Sanderson |title=But what is a partial differential equation? |work=3Blue1Brown |date=April 21, 2019 |url=https://www.youtube.com/watch?v=ly4S0oi3Yz8&amp;amp;list=PLZHQObOWTQDNPOjrT6KVlfJuKtYTftqH6 |via=[[YouTube]] }}&lt;br /&gt;
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{{Differential equations topics}}&lt;br /&gt;
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{{Authority control}}&lt;br /&gt;
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[[Category:Partial differential equations| ]]&lt;br /&gt;
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[[Category:Multivariable calculus]]&lt;br /&gt;
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Category:Multivariable calculus&lt;br /&gt;
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类别: 多元微积分&lt;br /&gt;
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[[Category:Differential equations]]&lt;br /&gt;
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Category:Differential equations&lt;br /&gt;
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类别: 微分方程&lt;br /&gt;
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[[Category:Concepts in physics]]&lt;br /&gt;
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Category:Concepts in physics&lt;br /&gt;
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分类: 物理概念&lt;br /&gt;
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&amp;lt;small&amp;gt;This page was moved from [[wikipedia:en:Partial differential equation]]. Its edit history can be viewed at [[偏微分方程/edithistory]]&amp;lt;/small&amp;gt;&amp;lt;/noinclude&amp;gt;&lt;br /&gt;
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[[Category:待整理页面]]&lt;/div&gt;</summary>
		<author><name>Ruili</name></author>
	</entry>
	<entry>
		<id>https://wiki.swarma.org/index.php?title=%E5%81%8F%E5%BE%AE%E5%88%86%E6%96%B9%E7%A8%8B&amp;diff=20102</id>
		<title>偏微分方程</title>
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		<updated>2020-12-15T12:34:52Z</updated>

		<summary type="html">&lt;p&gt;Ruili：&lt;/p&gt;
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&lt;div&gt;此词条暂由Yuling翻译，未经人工整理和审校，带来阅读不便，请见谅。&lt;br /&gt;
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[[File:Heat.gif|thumb|right|A visualisation of a solution to the two-dimensional [[heat equation]] with temperature represented by the third dimension]]&lt;br /&gt;
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A visualisation of a solution to the two-dimensional [[heat equation with temperature represented by the third dimension]]&lt;br /&gt;
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以三维表示温度的二维热方程解的可视化&lt;br /&gt;
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In [[mathematics]], a '''partial differential equation''' ('''PDE''') is a [[differential equation]] that contains unknown [[Multivariable calculus|multivariable functions]] and their [[partial derivative]]s. PDEs are used to formulate problems involving functions of several variables, and are either solved by hand, or used to create a [[computer model]]. A special case is [[ordinary differential equation]]s (ODEs), which deal with functions of a single variable and their derivatives.&lt;br /&gt;
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In mathematics, a partial differential equation (PDE) is a differential equation that contains unknown multivariable functions and their partial derivatives. PDEs are used to formulate problems involving functions of several variables, and are either solved by hand, or used to create a computer model. A special case is ordinary differential equations (ODEs), which deal with functions of a single variable and their derivatives.&lt;br /&gt;
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在数学中，'''&amp;lt;font color = &amp;quot;#ff8000&amp;quot;&amp;gt; 偏微分方程函数 Partial Differential Equation&amp;lt;/font&amp;gt;'''是包含未知多元函数及其偏导数的微分方程。偏微分方程用于描述涉及多元函数的问题，可以通过人为求解，也可以通过建立计算机模型来求解。常微分方程是偏微分方程一种特殊情况，它处理的是一元函数及其导数。&lt;br /&gt;
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PDEs can be used to describe a wide variety of phenomena such as sound, heat, [[diffusion]], [[electrostatics]], [[Electromagnetism|electrodynamics]], [[fluid dynamics]], [[Elasticity (physics)|elasticity]], [[gravitation]] and [[quantum mechanics]]. These seemingly distinct physical phenomena can be formalised similarly in terms of PDEs. Just as ordinary differential equations often model one-dimensional [[dynamical system]]s, partial differential equations often model [[multidimensional system]]s. PDEs find their generalisation in [[stochastic partial differential equation]]s.&lt;br /&gt;
&lt;br /&gt;
PDEs can be used to describe a wide variety of phenomena such as sound, heat, diffusion, electrostatics, electrodynamics, fluid dynamics, elasticity, gravitation and quantum mechanics. These seemingly distinct physical phenomena can be formalised similarly in terms of PDEs. Just as ordinary differential equations often model one-dimensional dynamical systems, partial differential equations often model multidimensional systems. PDEs find their generalisation in stochastic partial differential equations.&lt;br /&gt;
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偏微分方程可以用来描述各种各样的物理现象，如声音，热量，扩散，静电，电动力学，流体力学，弹性力学，重力和量子力学。这些看起来截然不同的物理现象却可以用类似的偏微分方程来描述。正如常微分方程经常对一维动力系统进行建模一样，偏微分方程经常对多维系统进行建模。随机偏微分方程是偏微分方程的一种推广。&lt;br /&gt;
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== Introduction ==&lt;br /&gt;
引言&lt;br /&gt;
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Partial differential equations (PDEs) are equations that involve rates of change with respect to [[continuous variables]]. For example, the position of a [[rigid body]] is specified by six parameters,&amp;lt;ref&amp;gt;{{Cite book|url=https://books.google.com/books?id=v9PLbcYd9aUC&amp;amp;pg=PA32|title=Modelling and Control of Robot Manipulators|last=Sciavicco|first=Lorenzo|last2=Siciliano|first2=Bruno|date=2001-02-19|publisher=Springer Science &amp;amp; Business Media|isbn=9781852332211|language=en}}&amp;lt;/ref&amp;gt; but the configuration of a [[fluid]] is given by the [[continuous distribution]] of several parameters, such as the [[temperature]], [[pressure]], and so forth. The dynamics for the rigid body take place in a finite-dimensional [[Configuration space (physics)|configuration space]]; the dynamics for the fluid occur in an infinite-dimensional configuration space. This distinction usually makes PDEs much harder to solve than ordinary differential equations (ODEs), but here again, there will be simple solutions for linear problems. Classic domains where PDEs are used include [[acoustics]], [[fluid dynamics]], [[electrodynamics]], and [[heat transfer]].&lt;br /&gt;
&lt;br /&gt;
Partial differential equations (PDEs) are equations that involve rates of change with respect to continuous variables. For example, the position of a rigid body is specified by six parameters, but the configuration of a fluid is given by the continuous distribution of several parameters, such as the temperature, pressure, and so forth. The dynamics for the rigid body take place in a finite-dimensional configuration space; the dynamics for the fluid occur in an infinite-dimensional configuration space. This distinction usually makes PDEs much harder to solve than ordinary differential equations (ODEs), but here again, there will be simple solutions for linear problems. Classic domains where PDEs are used include acoustics, fluid dynamics, electrodynamics, and heat transfer.&lt;br /&gt;
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偏微分方程(简称为PDEs)涉及到方程相对于连续变量的变化率。例如，刚体的位置是由六个参数确定的，而流体的状态是由几个参数的连续分布给出的，如温度、压力等。刚体的动力学过程发生在有限维状态空间中，流体的动力学过程发生在无限维状态空间中。这种区别通常使偏微分方程比常微分方程更难求解，但是线性问题仍然有简单的求解方式。使用偏微分方程的经典领域包括声学、流体力学、电动力学和传热学。&lt;br /&gt;
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A partial differential equation (PDE) for the function {{math|''u''(''x''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;,… ''x&amp;lt;sub&amp;gt;n&amp;lt;/sub&amp;gt;'')}} is an equation of the form&lt;br /&gt;
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A partial differential equation (PDE) for the function  is an equation of the form&lt;br /&gt;
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函数 {{math|''u''(''x''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;,… ''x&amp;lt;sub&amp;gt;n&amp;lt;/sub&amp;gt;'')}} 的偏微分方程形式是：&lt;br /&gt;
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&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt;f \left (x_1, \ldots x_n; u, \frac{\partial u}{\partial x_1}, \ldots \frac{\partial u}{\partial x_n}; \frac{\partial^2 u}{\partial x_1 \partial x_1}, \ldots \frac{\partial^2 u}{\partial x_1 \partial x_n}; \ldots \right) = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;f \left (x_1, \ldots x_n; u, \frac{\partial u}{\partial x_1}, \ldots \frac{\partial u}{\partial x_n}; \frac{\partial^2 u}{\partial x_1 \partial x_1}, \ldots \frac{\partial^2 u}{\partial x_1 \partial x_n}; \ldots \right) = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
If {{mvar|f}} is a [[linear function]] of {{mvar|u}} and its derivatives, then the PDE is called linear. Common examples of linear PDEs include the [[heat equation]], the [[wave equation]], [[Laplace's equation]], [[Helmholtz equation]], [[Klein–Gordon equation]], and [[Poisson's equation]].&lt;br /&gt;
&lt;br /&gt;
If  is a linear function of  and its derivatives, then the PDE is called linear. Common examples of linear PDEs include the heat equation, the wave equation, Laplace's equation, Helmholtz equation, Klein–Gordon equation, and Poisson's equation.&lt;br /&gt;
&lt;br /&gt;
如果 {{mvar|f}} 是函数 {{math|''u''}} 及其导数的线性函数，则偏微分方程称为线性函数。线性偏微分方程的常见例子包括热方程、波动方程、拉普拉斯方程、亥姆霍兹方程方程、克莱因-高登方程和泊松方程。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
A relatively simple PDE is&lt;br /&gt;
&lt;br /&gt;
A relatively simple PDE is&lt;br /&gt;
&lt;br /&gt;
一个相对简单的偏微分方程：&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt;\frac{\partial u}{\partial x}(x,y) = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;\frac{\partial u}{\partial x}(x,y) = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
This relation [[Logical implication|implies]] that the function {{math|''u''(''x'',''y'')}} is independent of {{mvar|x}}. However, the equation gives no information on the function's dependence on the variable {{mvar|y}}. Hence the general solution of this equation is&lt;br /&gt;
&lt;br /&gt;
This relation implies that the function  is independent of . However, the equation gives no information on the function's dependence on the variable . Hence the general solution of this equation is&lt;br /&gt;
&lt;br /&gt;
这意味着函数 {{math|''u''(''x'',''y'')}} 独立于 {{mvar|x}} 的。然而，这个方程没有给出关于函数和自变量的相关性的信息。因此，这个方程的通解是&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt;u(x,y) = f(y),&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;u(x,y) = f(y),&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
where {{mvar|f}} is an arbitrary function of {{mvar|y}}. The analogous ordinary differential equation is&lt;br /&gt;
&lt;br /&gt;
where  is an arbitrary function of . The analogous ordinary differential equation is&lt;br /&gt;
&lt;br /&gt;
其中， {{mvar|f}} 是 {{mvar|y}} 的任意函数。&lt;br /&gt;
&lt;br /&gt;
类似的常微分方程是：&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt;\frac{\mathrm{d} u}{\mathrm{d} x}(x) = 0,&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;\frac{\mathrm{d} u}{\mathrm{d} x}(x) = 0,&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
which has the solution&lt;br /&gt;
&lt;br /&gt;
which has the solution&lt;br /&gt;
&lt;br /&gt;
它的解为&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt;u(x) = c,&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;u(x) = c,&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
where {{mvar|c}} is any [[Constant (mathematics)|constant]] value. These two examples illustrate that general solutions of ordinary differential equations (ODEs) involve arbitrary constants, but solutions of PDEs involve arbitrary functions.&lt;br /&gt;
&lt;br /&gt;
where  is any constant value. These two examples illustrate that general solutions of ordinary differential equations (ODEs) involve arbitrary constants, but solutions of PDEs involve arbitrary functions.&lt;br /&gt;
&lt;br /&gt;
这里，{{mvar|c}} 是一个任意常量。&lt;br /&gt;
&lt;br /&gt;
这两个例子说明常微分方程的一般解包含任意常数，但偏微分方程的解包含任意函数。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
A solution of a PDE is generally not [[Uniqueness quantification|unique]]; additional conditions must generally be specified on the [[Boundary (topology)|boundary]] of the region where the solution is defined. For instance, in the simple example above, the function {{math|''f''(''y'')}} can be determined if {{mvar|u}} is specified on the line {{math|''x'' {{=}} 0}}.&lt;br /&gt;
&lt;br /&gt;
A solution of a PDE is generally not unique; additional conditions must generally be specified on the boundary of the region where the solution is defined. For instance, in the simple example above, the function  can be determined if  is specified on the line  0}}.&lt;br /&gt;
&lt;br /&gt;
偏微分方程的解一般不是唯一的; 一般必须在定义解的区域边界上定义附加条件。 例如，在上面的简单示例中，如果在 {{math|''x'' {{=}} 0}} 时确定了 {{mvar|u}} 的值，则可以确定该函数 {{math|''f''(''y'')}}。&lt;br /&gt;
&lt;br /&gt;
== Existence and uniqueness ==&lt;br /&gt;
存在性和唯一性&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Although the issue of existence and uniqueness of solutions of ordinary differential equations has a very satisfactory answer with the [[Picard–Lindelöf theorem]], that is far from the case for partial differential equations. The [[Cauchy–Kowalevski theorem]] states that the [[Cauchy problem]] for any partial differential equation whose coefficients are [[Analytic function|analytic]] in the unknown function and its derivatives, has a locally unique analytic solution. Although this result might appear to settle the existence and uniqueness of solutions, there are examples of linear partial differential equations whose coefficients have derivatives of all orders (which are nevertheless not analytic) but which have no solutions at all: see [[Lewy's example|Lewy (1957)]]. Even if the solution of a partial differential equation exists and is unique, it may nevertheless have undesirable properties.  The mathematical study of these questions is usually in the more powerful context of [[weak solution]]s.&lt;br /&gt;
&lt;br /&gt;
Although the issue of existence and uniqueness of solutions of ordinary differential equations has a very satisfactory answer with the Picard–Lindelöf theorem, that is far from the case for partial differential equations. The Cauchy–Kowalevski theorem states that the Cauchy problem for any partial differential equation whose coefficients are analytic in the unknown function and its derivatives, has a locally unique analytic solution. Although this result might appear to settle the existence and uniqueness of solutions, there are examples of linear partial differential equations whose coefficients have derivatives of all orders (which are nevertheless not analytic) but which have no solutions at all: see Lewy (1957). Even if the solution of a partial differential equation exists and is unique, it may nevertheless have undesirable properties.  The mathematical study of these questions is usually in the more powerful context of weak solutions.&lt;br /&gt;
&lt;br /&gt;
尽管常微分方程解的存在性和唯一性用'''&amp;lt;font color=&amp;quot;#ff8000&amp;quot;&amp;gt;弗罗贝尼乌斯定理 Picard–Lindelöf Theorem&amp;lt;/font&amp;gt;得到了令人满意的结果，但偏微分方程解的存在性和唯一性却远没有得到解决。'''&amp;lt;font color=&amp;quot;#ff8000&amp;quot;&amp;gt;柯西-科瓦列夫斯基定理 Cauchy–Kowalevski theorem&amp;lt;/font&amp;gt;指出：对于任意系数在未知函数及其导数中解析的偏微分方程，柯西问题存在一个局部唯一的解析解。虽然这个结果似乎解决了解的存在性和唯一性问题，但是存在一些线性偏微分方程-其系数具有所有级数的导数(尽管这些导数不是解析的) ，但是根本没有解: 见 Lewy (1957)。即使偏微分方程的解存在且唯一，它仍然可能具有不可预料的性质。这些问题的数学研究通常是在更有力的弱解的背景下进行的。&lt;br /&gt;
&lt;br /&gt;
An example of pathological behavior is the sequence (depending upon {{mvar|n}}) of [[Cauchy problem]]s for the [[Laplace equation]]&lt;br /&gt;
&lt;br /&gt;
An example of pathological behavior is the sequence (depending upon ) of Cauchy problems for the Laplace equation&lt;br /&gt;
&lt;br /&gt;
反常特征的一个例子是拉普拉斯方程的柯西问题的序列(取决于{{mvar|n}})&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt;\frac{\partial^2 u}{\partial x^2} + \frac{\partial^2 u}{\partial y^2}=0,&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;\frac{\partial^2 u}{\partial x^2} + \frac{\partial^2 u}{\partial y^2}=0,&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
with [[boundary condition]]s&lt;br /&gt;
&lt;br /&gt;
with boundary conditions&lt;br /&gt;
&lt;br /&gt;
具有边界条件&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt;\begin{align} u(x,0) &amp;amp;= 0, \\ \frac{\partial u}{\partial y}(x,0) &amp;amp;= \frac{\sin nx}{n}, \end{align}&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;\begin{align} u(x,0) &amp;amp;= 0, \\ \frac{\partial u}{\partial y}(x,0) &amp;amp;= \frac{\sin nx}{n}, \end{align}&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
where {{mvar|n}} is an integer. The derivative of {{mvar|u}} with respect to {{mvar|y}} approaches zero [[uniform convergence|uniformly]] in {{mvar|x}} as {{mvar|n}} increases, but the solution is&lt;br /&gt;
&lt;br /&gt;
where  is an integer. The derivative of  with respect to  approaches zero uniformly in  as  increases, but the solution is&lt;br /&gt;
&lt;br /&gt;
其中 {{mvar|n}} 是整数。{{mvar|u}} 关于 {{mvar|y}} 的导数，一致地随着 {{mvar|n}} 的增加而趋于零，但解是&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt;u(x,y) = \frac{\sinh ny \sin nx}{n^2}.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;u(x,y) = \frac{\sinh ny \sin nx}{n^2}.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
This solution approaches infinity if {{mvar|nx}} is not an integer multiple of {{pi}} for any non-zero value of {{mvar|y}}. The Cauchy problem for the Laplace equation is called ''ill-posed'' or ''not [[Well-posed problem|well-posed]]'', since the solution does not continuously depend on the data of the problem. Such ill-posed problems are not usually satisfactory for physical applications.&lt;br /&gt;
&lt;br /&gt;
This solution approaches infinity if  is not an integer multiple of  for any non-zero value of . The Cauchy problem for the Laplace equation is called ill-posed or not well-posed, since the solution does not continuously depend on the data of the problem. Such ill-posed problems are not usually satisfactory for physical applications.&lt;br /&gt;
&lt;br /&gt;
对于任何非零的 {{mvar|y}}，如果 {{mvar|nx}} 不是模板 {{pi}} 的整数倍，这个解会接近于无穷大。拉普拉斯方程的柯西问题被称为不适定的（可以译为ill-posed或not well-posed），因为解不是连续地依赖于问题的数据。这种不适定问题通常不能满足物理应用。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The [[Navier–Stokes existence and smoothness|existence of solutions for the Navier–Stokes equations]], a partial differential equation, is part of one of the [[Millennium Prize Problems]].&lt;br /&gt;
&lt;br /&gt;
The existence of solutions for the Navier–Stokes equations, a partial differential equation, is part of one of the Millennium Prize Problems.&lt;br /&gt;
&lt;br /&gt;
偏微分方程”纳维-斯托克斯方程“的解的存在性就是千禧年大奖难题之一的一部分。&lt;br /&gt;
&lt;br /&gt;
== Notation ==&lt;br /&gt;
符号&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
In PDEs, it is common to denote partial derivatives using subscripts. That is:&lt;br /&gt;
&lt;br /&gt;
In PDEs, it is common to denote partial derivatives using subscripts. That is:&lt;br /&gt;
&lt;br /&gt;
在偏微分方程中，通常用下标表示偏导数。例如:&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt;u_x = \frac{\partial u}{\partial x}&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;u_x = \frac{\partial u}{\partial x}&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt;u_{xx} = \frac{\partial^2 u}{\partial x^2} &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;u_{xx} = \frac{\partial^2 u}{\partial x^2} &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt;u_{xy} = \frac{\partial^2 u}{\partial y\, \partial x} = \frac{\partial}{\partial y } \left(\frac{\partial u}{\partial x}\right). &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;u_{xy} = \frac{\partial^2 u}{\partial y\, \partial x} = \frac{\partial}{\partial y } \left(\frac{\partial u}{\partial x}\right). &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Especially in physics, [[del]] or nabla ({{math|∇}}) is often used to denote spatial derivatives, and {{math|''&amp;amp;#x307;u'', ''ü''}} for time derivatives. For example, the [[wave equation]] (mentioned below) can be written as&lt;br /&gt;
&lt;br /&gt;
Especially in physics, del or nabla () is often used to denote spatial derivatives, and  for time derivatives. For example, the wave equation (mentioned below) can be written as&lt;br /&gt;
&lt;br /&gt;
特别是在物理学中，[[del]] 或 nabla ({{math|∇}}) 经常用来表示空间导数和时间导数。例如，波动方程(在下文中提到)可以写成：&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt;\ddot u=c^2\nabla^2u&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt;\ddot u=c^2\nabla^2u&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
or&lt;br /&gt;
&lt;br /&gt;
or&lt;br /&gt;
&lt;br /&gt;
或&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt;\ddot u=c^2\Delta u&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt;\ddot u=c^2\Delta u&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
where {{math|Δ}} is the [[Laplace operator]].&lt;br /&gt;
&lt;br /&gt;
where  is the Laplace operator.&lt;br /&gt;
&lt;br /&gt;
其中，{{math|Δ}} 代表拉普拉斯算子。&lt;br /&gt;
&lt;br /&gt;
== Classification ==&lt;br /&gt;
分类&lt;br /&gt;
&lt;br /&gt;
Some linear, second-order partial differential equations can be classified as [[parabolic partial differential equation|parabolic]], [[hyperbolic partial differential equation|hyperbolic]] and [[elliptic partial differential equation|elliptic]]. Others, such as the [[Euler–Tricomi equation]], have different types in different regions. The classification provides a guide to appropriate initial and boundary conditions and to the smoothness of the solutions.&lt;br /&gt;
&lt;br /&gt;
Some linear, second-order partial differential equations can be classified as parabolic, hyperbolic and elliptic. Others, such as the Euler–Tricomi equation, have different types in different regions. The classification provides a guide to appropriate initial and boundary conditions and to the smoothness of the solutions.&lt;br /&gt;
&lt;br /&gt;
一些线性二阶偏微分方程可分为抛物型方程、双曲型方程和椭圆型方程。其他的方程，如欧拉-特里科米方程，在不同的领域有不同的类型。这种分类有助于选择适当的初始和边界条件以及提高解的平滑性。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
=== Equations of first order ===&lt;br /&gt;
一阶方程&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{{main|First-order partial differential equation}}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
=== Linear equations of second order ===&lt;br /&gt;
二阶线性方程&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Assuming {{math|''u&amp;lt;sub&amp;gt;xy&amp;lt;/sub&amp;gt;'' {{=}} ''u&amp;lt;sub&amp;gt;yx&amp;lt;/sub&amp;gt;''}}, the general linear second-order PDE in two independent variables has the form&lt;br /&gt;
&lt;br /&gt;
Assuming  u&amp;lt;sub&amp;gt;yx&amp;lt;/sub&amp;gt;}}, the general linear second-order PDE in two independent variables has the form&lt;br /&gt;
&lt;br /&gt;
假设 {{math|''u&amp;lt;sub&amp;gt;xy&amp;lt;/sub&amp;gt;'' {{=}} ''u&amp;lt;sub&amp;gt;yx&amp;lt;/sub&amp;gt;''}}，含有两个独立变量的一般线性二阶偏微分方程具有如下形式：&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt;Au_{xx} + 2Bu_{xy} + Cu_{yy} + \cdots \mbox{(lower order terms)} = 0,&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;Au_{xx} + 2Bu_{xy} + Cu_{yy} + \cdots \mbox{(lower order terms)} = 0,&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
where the coefficients {{mvar|A}}, {{mvar|B}}, {{mvar|C}}... may depend upon {{mvar|x}} and {{mvar|y}}. If {{math|''A''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; + ''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; + ''C''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; &amp;gt; 0}} over a region of the {{mvar|xy}}-plane, the PDE is second-order in that region. This form is analogous to the equation for a conic section:&lt;br /&gt;
&lt;br /&gt;
where the coefficients , , ... may depend upon  and . If  over a region of the -plane, the PDE is second-order in that region. This form is analogous to the equation for a conic section:&lt;br /&gt;
&lt;br /&gt;
其中的系数 {{mvar|A}}, {{mvar|B}}, {{mvar|C}}... 一般取决于 {{mvar|x}} 和 {{mvar|y}} 。如果在 {{mvar|xy}}-平面的一个区域上 {{math|''A''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; + ''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; + ''C''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; &amp;gt; 0}}，偏微分方程是二阶的，这种形式类似于圆锥截面的方程:&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt;Ax^2 + 2Bxy + Cy^2 + \cdots = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;Ax^2 + 2Bxy + Cy^2 + \cdots = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
More precisely, replacing {{math|∂&amp;lt;sub&amp;gt;''x''&amp;lt;/sub&amp;gt;}} by {{mvar|X}}, and likewise for other variables (formally this is done by a [[Fourier transform]]), converts a constant-coefficient PDE into a polynomial of the same degree, with the terms of the highest degree (a [[homogeneous polynomial]], here a [[quadratic form]]) being most significant for the classification.&lt;br /&gt;
&lt;br /&gt;
More precisely, replacing  by , and likewise for other variables (formally this is done by a Fourier transform), converts a constant-coefficient PDE into a polynomial of the same degree, with the terms of the highest degree (a homogeneous polynomial, here a quadratic form) being most significant for the classification.&lt;br /&gt;
&lt;br /&gt;
更准确地说，用 {{mvar|X}} 替换 {{math|∂&amp;lt;sub&amp;gt;''x''&amp;lt;/sub&amp;gt;}}，并同样替换其它变量(通常由傅里叶变换完成)，将一个常系数偏微分方程转换成一个相同次数的多项式，最高次数的项(齐次多项式，这里是一个二次形式)对于偏微分方程的分类最为重要。&lt;br /&gt;
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Just as one classifies [[conic section]]s and quadratic forms into parabolic, hyperbolic, and elliptic based on the [[discriminant]] {{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − 4''AC''}}, the same can be done for a second-order PDE at a given point.  However, the [[discriminant]] in a PDE is given by {{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC''}} due to the convention of the {{mvar|xy}} term being {{math|2''B''}} rather than {{mvar|B}}; formally, the discriminant (of the associated quadratic form) is {{math|(2''B'')&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − 4''AC'' {{=}} 4(''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC'')}}, with the factor of 4 dropped for simplicity.&lt;br /&gt;
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Just as one classifies conic sections and quadratic forms into parabolic, hyperbolic, and elliptic based on the discriminant , the same can be done for a second-order PDE at a given point.  However, the discriminant in a PDE is given by  due to the convention of the  term being  rather than ; formally, the discriminant (of the associated quadratic form) is  4(B&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − AC)}}, with the factor of 4 dropped for simplicity.&lt;br /&gt;
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正如人们可以根据判别式 {{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − 4''AC''}} 将圆锥截面和二次型分为抛物型、双曲型和椭圆型一样，对于给定点的二阶偏微分方程也可以这样做。然而，偏微分方程中的判别式 {{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − 4''AC''}} 是根据交叉项的系数{{math|2''B''}} 而不是 {{mvar|B}} 给出的，形式上，判别式(关联二次型)是 {{math|(2''B'')&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − 4''AC'' {{=}} 4(''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC'')}}，为简单起见，去掉了因子4。&lt;br /&gt;
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# {{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC'' &amp;lt; 0}} (''[[elliptic partial differential equation]]''): Solutions of [[elliptic partial differential equation|elliptic PDEs]] are as smooth as the coefficients allow, within the interior of the region where the equation and solutions are defined. For example, solutions of [[Laplace's equation]] are analytic within the domain where they are defined, but solutions may assume boundary values that are not smooth. The motion of a fluid at subsonic speeds can be approximated with elliptic PDEs, and the Euler–Tricomi equation is elliptic where {{math|''x'' &amp;lt; 0}}.&lt;br /&gt;
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  (elliptic partial differential equation): Solutions of elliptic PDEs are as smooth as the coefficients allow, within the interior of the region where the equation and solutions are defined. For example, solutions of Laplace's equation are analytic within the domain where they are defined, but solutions may assume boundary values that are not smooth. The motion of a fluid at subsonic speeds can be approximated with elliptic PDEs, and the Euler–Tricomi equation is elliptic where .&lt;br /&gt;
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{{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC'' &amp;lt; 0}} (椭圆型微分方程)：在定义方程和解的区域内部，椭圆型偏微分方程的解在系数允许的程度内光滑。例如，拉普拉斯方程的解在它们被定义的区域内是解析的，但可能假设边界值是不光滑的。亚音速流体的运动可以用椭圆型偏微分方程近似，欧拉-特里科米方程在 {{math|''x'' &amp;lt; 0}} 时是椭圆型偏微分方程。&lt;br /&gt;
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# {{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC'' {{=}} 0}} (''[[parabolic partial differential equation]]''): Equations that are [[parabolic partial differential equation|parabolic]] at every point can be transformed into a form analogous to the [[heat equation]] by a change of independent variables. Solutions smooth out as the transformed time variable increases. The Euler–Tricomi equation has parabolic type on the line where {{math|''x'' {{=}} 0}}.&lt;br /&gt;
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  0}} (parabolic partial differential equation): Equations that are parabolic at every point can be transformed into a form analogous to the heat equation by a change of independent variables. Solutions smooth out as the transformed time variable increases. The Euler–Tricomi equation has parabolic type on the line where  0}}.&lt;br /&gt;
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{{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC'' {{=}} 0}}（抛物型偏微分方程）：在每一点上都是抛物线型的方程可以通过改变自变量从而转化成类似于热方程的形式。随着转换后的时间变量的增加，方程的解变得平滑。欧拉-特里科米方程在特征线 {{math|''x'' {{=}} 0}} 上是抛物线型的。&lt;br /&gt;
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# {{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC'' &amp;gt; 0}} (''[[hyperbolic partial differential equation]]''): [[hyperbolic partial differential equation|hyperbolic]] equations retain any discontinuities of functions or derivatives in the initial data. An example is the [[wave equation]]. The motion of a fluid at supersonic speeds can be approximated with hyperbolic PDEs, and the Euler–Tricomi equation is hyperbolic where {{math|''x'' &amp;gt; 0}}.&lt;br /&gt;
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  (hyperbolic partial differential equation): hyperbolic equations retain any discontinuities of functions or derivatives in the initial data. An example is the wave equation. The motion of a fluid at supersonic speeds can be approximated with hyperbolic PDEs, and the Euler–Tricomi equation is hyperbolic where .&lt;br /&gt;
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{{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC'' &amp;gt; 0}} (双曲型偏微分方程)：双曲型方程在初始数据中保留了函数或导数的任何不连续性。波动方程就是其中的一个例子。超音速流体的运动可以用双曲型偏微分方程近似，欧拉-特里科米方程在 {{math|''x'' &amp;gt; 0}} 时是双曲型的。&lt;br /&gt;
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If there are {{mvar|n}} independent variables {{math|''x''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;, ''x''&amp;lt;sub&amp;gt;2 &amp;lt;/sub&amp;gt;,… ''x''&amp;lt;sub&amp;gt;''n''&amp;lt;/sub&amp;gt;}}, a general linear partial differential equation of second order has the form&lt;br /&gt;
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If there are  independent variables , a general linear partial differential equation of second order has the form&lt;br /&gt;
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如果存在 {{mvar|n}} 个自变量 {{math|''x''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;, ''x''&amp;lt;sub&amp;gt;2 &amp;lt;/sub&amp;gt;,… ''x''&amp;lt;sub&amp;gt;''n''&amp;lt;/sub&amp;gt;}}，一般二阶线性偏微分方程的形式是：&lt;br /&gt;
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: &amp;lt;math&amp;gt;L u =\sum_{i=1}^n\sum_{j=1}^n a_{i,j} \frac{\partial^2 u}{\partial x_i \partial x_j} \quad \text{ plus lower-order terms} =0.&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;L u =\sum_{i=1}^n\sum_{j=1}^n a_{i,j} \frac{\partial^2 u}{\partial x_i \partial x_j} \quad \text{ plus lower-order terms} =0.&amp;lt;/math&amp;gt;&lt;br /&gt;
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The classification depends upon the signature of the eigenvalues of the coefficient matrix {{math|''a''&amp;lt;sub&amp;gt;''i'',''j''&amp;lt;/sub&amp;gt;}}.&lt;br /&gt;
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The classification depends upon the signature of the eigenvalues of the coefficient matrix .&lt;br /&gt;
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这种分类取决于系数矩阵特征值的符号（正负性）。&lt;br /&gt;
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# Elliptic: the eigenvalues are all positive or all negative.&lt;br /&gt;
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 Elliptic: the eigenvalues are all positive or all negative.&lt;br /&gt;
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椭圆形方程: 特征值全部为正或全部为负。&lt;br /&gt;
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# Parabolic: the eigenvalues are all positive or all negative, save one that is zero.&lt;br /&gt;
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 Parabolic: the eigenvalues are all positive or all negative, save one that is zero.&lt;br /&gt;
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抛物线形方程:除了一个为零值，特征值全部为正或全部为负。&lt;br /&gt;
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# Hyperbolic: there is only one negative eigenvalue and all the rest are positive, or there is only one positive eigenvalue and all the rest are negative.&lt;br /&gt;
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 Hyperbolic: there is only one negative eigenvalue and all the rest are positive, or there is only one positive eigenvalue and all the rest are negative.&lt;br /&gt;
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双曲形方程: 只有一个负特征值，其余的都是正特征值，或者只有一个正特征值，其余的都是负特征值。&lt;br /&gt;
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# Ultrahyperbolic: there is more than one positive eigenvalue and more than one negative eigenvalue, and there are no zero eigenvalues. There is only a limited theory for ultrahyperbolic equations (Courant and Hilbert, 1962).&lt;br /&gt;
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 Ultrahyperbolic: there is more than one positive eigenvalue and more than one negative eigenvalue, and there are no zero eigenvalues. There is only a limited theory for ultrahyperbolic equations (Courant and Hilbert, 1962).&lt;br /&gt;
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超双形方程: 存在多于一个正特征值和多于一个的负特征值，且不存在零特征值。对于超双曲方程，只存在有限的理论(Courant 和 Hilbert，1962)。&lt;br /&gt;
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=== Systems of first-order equations and characteristic surfaces ===&lt;br /&gt;
一阶方程组和特征曲面&lt;br /&gt;
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The classification of partial differential equations can be extended to systems of first-order equations, where the unknown {{mvar|u}} is now a [[Euclidean vector|vector]] with {{mvar|m}} components, and the coefficient matrices {{mvar|A&amp;lt;sub&amp;gt;ν&amp;lt;/sub&amp;gt;}} are {{mvar|m}} by {{mvar|m}} matrices for {{math|''ν'' {{=}} 1, 2,… ''n''}}. The partial differential equation takes the form&lt;br /&gt;
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The classification of partial differential equations can be extended to systems of first-order equations, where the unknown  is now a vector with  components, and the coefficient matrices  are  by  matrices for  1, 2,… n}}. The partial differential equation takes the form&lt;br /&gt;
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偏微分方程的分类可以推广到一阶方程组，其中未知量 {{mvar|u}} 是有 {{mvar|m}} 个分量的向量。对于 {{math|''ν'' {{=}} 1, 2,… ''n''}}，系数矩阵 {{mvar|A&amp;lt;sub&amp;gt;ν&amp;lt;/sub&amp;gt;}} 是 {{mvar|m}} × {{mvar|m}} 的矩阵。偏微分方程形式如下：&lt;br /&gt;
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: &amp;lt;math&amp;gt;Lu = \sum_{\nu=1}^{n} A_\nu \frac{\partial u}{\partial x_\nu} + B=0,&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;Lu = \sum_{\nu=1}^{n} A_\nu \frac{\partial u}{\partial x_\nu} + B=0,&amp;lt;/math&amp;gt;&lt;br /&gt;
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where the coefficient matrices {{mvar|A&amp;lt;sub&amp;gt;ν&amp;lt;/sub&amp;gt;}} and the vector {{mvar|B}} may depend upon {{mvar|x}} and {{mvar|u}}. If a [[hypersurface]] {{mvar|S}} is given in the implicit form&lt;br /&gt;
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where the coefficient matrices  and the vector  may depend upon  and . If a hypersurface  is given in the implicit form&lt;br /&gt;
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其中，系数矩阵 {{mvar|A&amp;lt;sub&amp;gt;ν&amp;lt;/sub&amp;gt;}} 和向量 {{mvar|B}} 可能依赖于 {{mvar|x}} 和 {{mvar|u}}。如果超曲面是以以下隐式形式给出的，&lt;br /&gt;
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: &amp;lt;math&amp;gt;\varphi(x_1, x_2, \ldots x_n)=0,&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;\varphi(x_1, x_2, \ldots x_n)=0,&amp;lt;/math&amp;gt;&lt;br /&gt;
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where {{mvar|φ}} has a non-zero gradient, then {{mvar|S}} is a '''characteristic surface''' for the operator {{mvar|L}} at a given point if the characteristic form vanishes:&lt;br /&gt;
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where  has a non-zero gradient, then  is a characteristic surface for the operator  at a given point if the characteristic form vanishes:&lt;br /&gt;
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其中，存在一个非零的梯度 {{mvar|φ}}，对于在给定点上特征形式消失的算子，特征曲面 {{mvar|S}} 形式如下:&lt;br /&gt;
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: &amp;lt;math&amp;gt;Q\left(\frac{\partial\varphi}{\partial x_1}, \ldots\frac{\partial\varphi}{\partial x_n}\right) =\det\left[\sum_{\nu=1}^nA_\nu \frac{\partial \varphi}{\partial x_\nu}\right]=0.\,&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;Q\left(\frac{\partial\varphi}{\partial x_1}, \ldots\frac{\partial\varphi}{\partial x_n}\right) =\det\left[\sum_{\nu=1}^nA_\nu \frac{\partial \varphi}{\partial x_\nu}\right]=0.\,&amp;lt;/math&amp;gt;&lt;br /&gt;
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The geometric interpretation of this condition is as follows: if data for {{mvar|u}} are prescribed on the surface {{mvar|S}}, then it may be possible to determine the normal derivative of {{mvar|u}} on {{mvar|S}} from the differential equation. If the data on {{mvar|S}} and the differential equation determine the normal derivative of {{mvar|u}} on {{mvar|S}}, then {{mvar|S}} is non-characteristic. If the data on {{mvar|S}} and the differential equation ''do not'' determine the normal derivative of {{mvar|u}} on {{mvar|S}}, then the surface is '''characteristic''', and the differential equation restricts the data on {{mvar|S}}: the differential equation is ''internal'' to {{mvar|S}}.&lt;br /&gt;
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The geometric interpretation of this condition is as follows: if data for  are prescribed on the surface , then it may be possible to determine the normal derivative of  on  from the differential equation. If the data on  and the differential equation determine the normal derivative of  on , then  is non-characteristic. If the data on  and the differential equation do not determine the normal derivative of  on , then the surface is characteristic, and the differential equation restricts the data on : the differential equation is internal to .&lt;br /&gt;
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这个条件的几何解释如下: 如果关于 {{mvar|u}} 的数据是在曲面 {{mvar|S}} 上规定的，那么就有可能依据微分方程确定曲面 {{mvar|S}} 上 {{mvar|u}} 的法向导数。如果曲面 {{mvar|S}} 上的数据和上面的微分方程能确定曲面 {{mvar|S}} 上 {{mvar|u}} 的法向导数，那么它就是非特征的。如果曲面 {{mvar|S}} 上的数据和上面的微分方程不能确定曲面 {{mvar|S}} 上 {{mvar|u}} 的法向导数，那么曲面是特征的，并且微分方程将数据限制在曲面 {{mvar|S}} 上：微分方程是在曲面 {{mvar|S}} 内部。&lt;br /&gt;
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# A first-order system {{math|''Lu'' {{=}} 0}} is ''elliptic'' if no surface is characteristic for {{mvar|L}}: the values of {{mvar|u}} on {{mvar|S}} and the differential equation always determine the normal derivative of {{mvar|u}} on {{mvar|S}}.&lt;br /&gt;
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 A first-order system  0}} is elliptic if no surface is characteristic for : the values of  on  and the differential equation always determine the normal derivative of  on .&lt;br /&gt;
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如果对于 {{mvar|L}} 没有曲面是特征的，则一阶系统 {{math|''Lu'' {{=}} 0}} 是椭圆形的：{{mvar|u}}在 {{mvar|S}} 的值和微分方程总能够决定 {{mvar|S}} 上 {{mvar|u}} 的法向导数。&lt;br /&gt;
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# A first-order system is ''hyperbolic'' at a point if there is a '''spacelike''' surface {{mvar|S}} with normal {{mvar|ξ}} at that point. This means that, given any non-trivial vector {{mvar|η}} orthogonal to {{mvar|ξ}}, and a scalar multiplier {{mvar|λ}}, the equation {{math|''Q''(''λξ'' + ''η'') {{=}} 0}} has {{mvar|m}} real roots {{math|''λ''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;, ''λ''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;,… ''λ''&amp;lt;sub&amp;gt;''m''&amp;lt;/sub&amp;gt;}}. The system is '''strictly hyperbolic''' if these roots are always distinct. The geometrical interpretation of this condition is as follows: the characteristic form {{math|''Q''(''ζ'') {{=}} 0}} defines a cone (the normal cone) with homogeneous coordinates ζ. In the hyperbolic case, this cone has {{mvar|m}} sheets, and the axis {{math|''ζ'' {{=}} ''λξ''}} runs inside these sheets: it does not intersect any of them. But when displaced from the origin by η, this axis intersects every sheet. In the elliptic case, the normal cone has no real sheets.&lt;br /&gt;
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 A first-order system is hyperbolic at a point if there is a spacelike surface  with normal  at that point. This means that, given any non-trivial vector  orthogonal to , and a scalar multiplier , the equation  0}} has  real roots . The system is strictly hyperbolic if these roots are always distinct. The geometrical interpretation of this condition is as follows: the characteristic form  0}} defines a cone (the normal cone) with homogeneous coordinates ζ. In the hyperbolic case, this cone has  sheets, and the axis  λξ}} runs inside these sheets: it does not intersect any of them. But when displaced from the origin by η, this axis intersects every sheet. In the elliptic case, the normal cone has no real sheets.&lt;br /&gt;
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如果在该点存在一个法向量为 {{mvar|ξ}}的 '''&amp;lt;font color=&amp;quot;#ff8000&amp;quot;&amp;gt;类空曲面 Spacclike Surface&amp;lt;/font&amp;gt; {{mvar|S}} ，则一阶系统在那一点是双曲的。这意味着，给定任意正交于 {{mvar|ξ}} 的非平凡向量 {{mvar|η}} 和一个标量乘子 {{mvar|λ}}，方程 {{math|''Q''(''λξ'' + ''η'') {{=}} 0}} 有 {{mvar|m}} 个实根 {{math|''λ''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;, ''λ''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;,… ''λ''&amp;lt;sub&amp;gt;''m''&amp;lt;/sub&amp;gt;}}。如果这些根始终不同，则该系统是严格双曲形的。这个条件的几何解释如下: 特征形式 {{math|''Q''(''ζ'') {{=}} 0}} 定义了一个具有齐次坐标 ζ的圆锥(法线圆锥)。在双曲形的情况下，这个圆锥体有 {{mvar|m}} 层，并且轴 {{math|''ζ'' {{=}} ''λξ''}} 在这些层中运动: 它不与任何一层相交。但是当从原点偏离η时，这条轴线与每一层都相交。在椭圆形的情况下，法向圆锥没有实层。&lt;br /&gt;
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==[[用户:Yuling|Yuling]]（[[用户讨论:Yuling|讨论]]） sheet 这个单词也不很理解，我直译为了“层”&lt;br /&gt;
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=== Equations of mixed type ===&lt;br /&gt;
混合型方程&lt;br /&gt;
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If a PDE has coefficients that are not constant, it is possible that it will not belong to any of these categories but rather be of '''mixed type'''. A simple but important example is the [[Euler–Tricomi equation]]&lt;br /&gt;
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If a PDE has coefficients that are not constant, it is possible that it will not belong to any of these categories but rather be of mixed type. A simple but important example is the Euler–Tricomi equation&lt;br /&gt;
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如果偏微分方程的系数不是常数，那么它可能不属于这些类别中的任何一个，而是属于混合类型。一个简单但重要的例子是欧拉-特里科米方程&lt;br /&gt;
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: &amp;lt;math&amp;gt;u_{xx} = xu_{yy},&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;u_{xx} = xu_{yy},&amp;lt;/math&amp;gt;&lt;br /&gt;
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which is called '''elliptic-hyperbolic''' because it is elliptic in the region {{math|''x'' &amp;lt; 0}}, hyperbolic in the region {{math|''x'' &amp;gt; 0}}, and degenerate parabolic on the line {{math|''x'' {{=}} 0}}.&lt;br /&gt;
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which is called elliptic-hyperbolic because it is elliptic in the region , hyperbolic in the region , and degenerate parabolic on the line  0}}.&lt;br /&gt;
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它在 {{math|''x'' &amp;lt; 0}} 的区域上是椭圆形，在 {{math|''x'' &amp;gt; 0}} 区域上是双曲形，在 {{math|''x'' {{=}} 0}}这条线上是退化为抛物线形，因此称之为椭圆-双曲型。&lt;br /&gt;
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''fill in: Dirichlet and Neumann boundaries, hyperbolic/parabolic/elliptic separation of variables, [[Fourier analysis]], [[Green's function]]s ...--&amp;gt;&lt;br /&gt;
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fill in: Dirichlet and Neumann boundaries, hyperbolic/parabolic/elliptic separation of variables, Fourier analysis, Green's functions ...--&amp;gt;&lt;br /&gt;
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填写: Dirichlet 和 Neumann 边界，双曲 / 抛物线 / 椭圆分离变量法，傅立叶分析，Green 函数... --&lt;br /&gt;
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=== Infinite-order PDEs in quantum mechanics ===&lt;br /&gt;
量子力学中的无限阶偏微分方程&lt;br /&gt;
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In the [[phase space formulation]] of quantum mechanics,  one may consider the [[Method of quantum characteristics|quantum Hamilton's equations]] for trajectories of quantum particles. These equations are infinite-order PDEs. However, in the semiclassical expansion, one has a finite system of ODEs at any fixed order of [[Dirac constant|{{mvar|ħ}}]].  The evolution equation of the [[Wigner quasi-probability distribution|c]] is also an infinite-order PDE. The quantum trajectories are [[Method of quantum characteristics|quantum characteristics]], with the use of which one could calculate the evolution of the Wigner function.&lt;br /&gt;
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In the phase space formulation of quantum mechanics,  one may consider the quantum Hamilton's equations for trajectories of quantum particles. These equations are infinite-order PDEs. However, in the semiclassical expansion, one has a finite system of ODEs at any fixed order of Dirac constant|.  The evolution equation of the Wigner function is also an infinite-order PDE. The quantum trajectories are quantum characteristics, with the use of which one could calculate the evolution of the Wigner function.&lt;br /&gt;
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在量子力学中的相空间表述中，我们可以考虑用于求解量子粒子的轨迹的量子哈密顿的方程。这些方程是无限阶偏微分方程。然而，在半经典展开中，我们在给定[[Dirac constant|{{mvar|ħ}}]]阶数下有一个有限的的常微分方程组。'''&amp;lt;font color=&amp;quot;#ff8000&amp;quot;&amp;gt;维格纳函数  Wigner Function&amp;lt;/font&amp;gt;的演化方程也是一个无限阶偏微分方程。由于量子轨道的量子特性，所以它通常可以用来计算维格纳函数的演化。&lt;br /&gt;
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== Analytical solutions ==&lt;br /&gt;
解析解&lt;br /&gt;
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===Separation of variables===&lt;br /&gt;
分离变量法&lt;br /&gt;
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{{main|Separable partial differential equation}}&lt;br /&gt;
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Linear PDEs can be reduced to systems of ordinary differential equations by the important technique of separation of variables. This technique rests on a characteristic of solutions to differential equations: if one can find any solution that solves the equation and satisfies the boundary conditions, then it is ''the'' solution (this also applies to ODEs). We assume as an [[ansatz]] that the dependence of a solution on the parameters space and time can be written as a product of terms that each depend on a single parameter, and then see if this can be made to solve the problem.&amp;lt;ref&amp;gt;{{cite book|last1=Gershenfeld|first1=Neil|title=The nature of mathematical modeling|date=2000|publisher=Cambridge Univ. Press|location=Cambridge|isbn=0521570956|page=27|edition=Reprinted (with corr.)}}&amp;lt;/ref&amp;gt;&lt;br /&gt;
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Linear PDEs can be reduced to systems of ordinary differential equations by the important technique of separation of variables. This technique rests on a characteristic of solutions to differential equations: if one can find any solution that solves the equation and satisfies the boundary conditions, then it is the solution (this also applies to ODEs). We assume as an ansatz that the dependence of a solution on the parameters space and time can be written as a product of terms that each depend on a single parameter, and then see if this can be made to solve the problem.&lt;br /&gt;
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线性偏微分方程组可以通过分离变量法这一重要方法来简化为常微分方程组。这种方法依赖于微分方程解的一个特征: 如果能找到任何一个满足方程和边界条件的解，那么这个解就是方程的解(这也适用于常微分方程)。我们假设解对参数空间和时间的依赖可以写成对它们每一项的依赖以及一个参数的乘积，然后再看看这是否可以用来解决这个问题。&lt;br /&gt;
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In the method of separation of variables, one reduces a PDE to a PDE in fewer variables, which is an ordinary differential equation if in one variable – these are in turn easier to solve.&lt;br /&gt;
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In the method of separation of variables, one reduces a PDE to a PDE in fewer variables, which is an ordinary differential equation if in one variable – these are in turn easier to solve.&lt;br /&gt;
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在分离变量法方法中，可以将偏微分方程简化为含有更少变量的偏微分方程，如果只有一个变量，那么就变成了一个'''&amp;lt;font color = &amp;quot;#ff8000&amp;quot;&amp;gt;常微分方程 Ordinary Differential Equation&amp;lt;/font&amp;gt;'''-- 反过来，这些方程也更容易求解。&lt;br /&gt;
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This is possible for simple PDEs, which are called [[separable partial differential equation]]s, and the domain is generally a rectangle (a product of intervals). Separable PDEs correspond to [[diagonal matrices]] – thinking of &amp;quot;the value for fixed {{mvar|x}}&amp;quot; as a coordinate, each coordinate can be understood separately.&lt;br /&gt;
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This is possible for simple PDEs, which are called separable partial differential equations, and the domain is generally a rectangle (a product of intervals). Separable PDEs correspond to diagonal matrices – thinking of &amp;quot;the value for fixed &amp;quot; as a coordinate, each coordinate can be understood separately.&lt;br /&gt;
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对于简单的偏微分方程(称为可分离偏微分方程)来说，这是可能的，而且方程通常定义在一个矩形区域(区间的乘积)上。可分离偏微分方程对应于对角线矩阵——以“固定值”为坐标，每个坐标可分开理解。&lt;br /&gt;
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This generalizes to the [[method of characteristics]], and is also used in [[integral transform]]s.&lt;br /&gt;
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This generalizes to the method of characteristics, and is also used in integral transforms.&lt;br /&gt;
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这种方法可以推广到特征曲线法，也可以用于积分变换。&lt;br /&gt;
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===Method of characteristics===&lt;br /&gt;
特征曲线法&lt;br /&gt;
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{{main|Method of characteristics}}&lt;br /&gt;
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In special cases, one can find characteristic curves on which the equation reduces to an ODE – changing coordinates in the domain to straighten these curves allows separation of variables, and is called the [[method of characteristics]].&lt;br /&gt;
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In special cases, one can find characteristic curves on which the equation reduces to an ODE – changing coordinates in the domain to straighten these curves allows separation of variables, and is called the method of characteristics.&lt;br /&gt;
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在特殊情况下，可以找到一些特征曲线，在这些曲线上方程可以变成一个常微分方程——意味着改变坐标从而使这些曲线变直从而达到分离变量的目的，这就是所谓的特征曲线法。&lt;br /&gt;
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More generally, one may find characteristic surfaces.&lt;br /&gt;
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More generally, one may find characteristic surfaces.&lt;br /&gt;
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更一般地说，人们可能会找到特征表面。&lt;br /&gt;
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===Integral transform===&lt;br /&gt;
积分变换&lt;br /&gt;
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An [[integral transform]] may transform the PDE to a simpler one, in particular, a separable PDE. This corresponds to diagonalizing an operator.&lt;br /&gt;
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An integral transform may transform the PDE to a simpler one, in particular, a separable PDE. This corresponds to diagonalizing an operator.&lt;br /&gt;
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积分变换可以将偏微分方程转换为更简单的偏微分方程，特别是可分离的偏微分方程。这对应于对角化算符。&lt;br /&gt;
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An important example of this is [[Fourier analysis]], which diagonalizes the heat equation using the [[eigenbasis]] of sinusoidal waves.&lt;br /&gt;
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An important example of this is Fourier analysis, which diagonalizes the heat equation using the eigenbasis of sinusoidal waves.&lt;br /&gt;
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这方面的一个重要例子是'''&amp;lt;font color = &amp;quot;#ff8000&amp;quot;&amp;gt;傅里叶分析  Fourier Analysis&amp;lt;/font&amp;gt;'''，它使用正弦波的特征基来对角化热方程。&lt;br /&gt;
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If the domain is finite or periodic, an infinite sum of solutions such as a [[Fourier series]] is appropriate, but an integral of solutions such as a [[Fourier integral]] is generally required for infinite domains. The solution for a point source for the heat equation given above is an example of the use of a Fourier integral.&lt;br /&gt;
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If the domain is finite or periodic, an infinite sum of solutions such as a Fourier series is appropriate, but an integral of solutions such as a Fourier integral is generally required for infinite domains. The solution for a point source for the heat equation given above is an example of the use of a Fourier integral.&lt;br /&gt;
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如果区域是有限的或周期性的，那么解为无限和的形式是恰当的，例如傅里叶级数，但是一个解的积分，例如傅立叶积分，一般是在无限区域上的。上面给出的热传导方程的点源解法就是使用傅里叶积分的一个例子。&lt;br /&gt;
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===Change of variables===&lt;br /&gt;
变量代换&lt;br /&gt;
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Often a PDE can be reduced to a simpler form with a known solution by a suitable [[Change of variables (PDE)|change of variables]].  For example, the [[Black–Scholes equation#Derivation|Black–Scholes]] PDE&lt;br /&gt;
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Often a PDE can be reduced to a simpler form with a known solution by a suitable change of variables.  For example, the Black–Scholes PDE&lt;br /&gt;
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偏微分方程通常可以通过变量的适当变化，用已知的解简化为更简单的形式。例如，布莱克-舒尔斯偏微分方程&lt;br /&gt;
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:&amp;lt;math&amp;gt; \frac{\partial V}{\partial t} + \tfrac{1}{2}\sigma^2 S^2\frac{\partial^2 V}{\partial S^2} + rS\frac{\partial V}{\partial S} - rV = 0 &amp;lt;/math&amp;gt;&lt;br /&gt;
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&amp;lt;math&amp;gt; \frac{\partial V}{\partial t} + \tfrac{1}{2}\sigma^2 S^2\frac{\partial^2 V}{\partial S^2} + rS\frac{\partial V}{\partial S} - rV = 0 &amp;lt;/math&amp;gt;&lt;br /&gt;
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is reducible to the [[heat equation]]&lt;br /&gt;
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is reducible to the heat equation&lt;br /&gt;
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可以简化为热传导方程&lt;br /&gt;
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:&amp;lt;math&amp;gt; \frac{\partial u}{\partial \tau} = \frac{\partial^2 u}{\partial x^2}&amp;lt;/math&amp;gt;&lt;br /&gt;
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&amp;lt;math&amp;gt; \frac{\partial u}{\partial \tau} = \frac{\partial^2 u}{\partial x^2}&amp;lt;/math&amp;gt;&lt;br /&gt;
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by the change of variables (for complete details see {{webarchive |url=https://web.archive.org/web/20080411030405/http://www.math.unl.edu/~sdunbar1/Teaching/MathematicalFinance/Lessons/BlackScholes/Solution/solution.shtml |date=April 11, 2008 |title=Solution of the Black Scholes Equation }})&lt;br /&gt;
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by the change of variables (for complete details see )&lt;br /&gt;
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通过变量替换(完整的细节见)&lt;br /&gt;
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:&amp;lt;math&amp;gt;\begin{align}&lt;br /&gt;
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V(S,t) &amp;amp;= K v(x,\tau),\\[5px]&lt;br /&gt;
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x &amp;amp;= \ln\left(\tfrac{S}{K} \right),\\[5px]&lt;br /&gt;
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\tau &amp;amp;= \tfrac{1}{2} \sigma^2 (T - t),\\[5px]&lt;br /&gt;
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v(x,\tau)&amp;amp;=e^{-\alpha x-\beta\tau} u(x,\tau).&lt;br /&gt;
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\end{align}&amp;lt;/math&amp;gt;&lt;br /&gt;
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===Fundamental solution===&lt;br /&gt;
基本解&lt;br /&gt;
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{{main|Fundamental solution}}&lt;br /&gt;
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Inhomogeneous equations can often be solved (for constant coefficient PDEs, always be solved) by finding the [[fundamental solution]] (the solution for a point source), then taking the [[convolution]] with the boundary conditions to get the solution.&lt;br /&gt;
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Inhomogeneous equations can often be solved (for constant coefficient PDEs, always be solved) by finding the fundamental solution (the solution for a point source), then taking the convolution with the boundary conditions to get the solution.&lt;br /&gt;
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非齐次方程(常系数偏微分方程)一般是通过先求出基本解(点源的解) ，然后利用带边界条件的卷积来求解。&lt;br /&gt;
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This is analogous in [[signal processing]] to understanding a filter by its [[impulse response]].&lt;br /&gt;
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This is analogous in signal processing to understanding a filter by its impulse response.&lt;br /&gt;
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这类似于在信号处理中通过滤波器的脉冲响应来理解滤波器。&lt;br /&gt;
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===Superposition principle===&lt;br /&gt;
叠加原理&lt;br /&gt;
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{{further| Superposition principle }}&lt;br /&gt;
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The superposition principle applies to any linear system, including linear systems of PDEs. A common visualization of this concept is the interaction of two waves in phase being combined to result in a greater amplitude, for example {{math|sin ''x'' + sin ''x'' {{=}} 2 sin ''x''}}. The same principle can be observed in PDEs where the solutions may be real or complex and additive. [[Superposition principle|superposition]]&lt;br /&gt;
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The superposition principle applies to any linear system, including linear systems of PDEs. A common visualization of this concept is the interaction of two waves in phase being combined to result in a greater amplitude, for example  2 sin x}}. The same principle can be observed in PDEs where the solutions may be real or complex and additive. superposition&lt;br /&gt;
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'''&amp;lt;font color = &amp;quot;#ff8000&amp;quot;&amp;gt;叠加原理 Superposition Principle&amp;lt;/font&amp;gt;适用于任何线性系统，包括偏微分方程的线性系统。这个概念的一个常见的可视化是两个同相位的波相互作用结合在一起会产生更大的振幅，例如 {{math|sin ''x'' + sin ''x'' {{=}} 2 sin ''x''}}。在偏微分方程中也可以观察到同样的原理，其中的解可能是真实的或复杂的和可加的。叠加&lt;br /&gt;
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If {{math|''u''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;}} and {{math|''u''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;}} are solutions of linear PDE in some function space {{mvar|R}}, then {{math|''u'' {{=}} ''c''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;''u''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; + ''c''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;''u''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;}} with any constants {{math|''c''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;}} and {{math|''c''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;}} are also a solution of that PDE in the same function space.&lt;br /&gt;
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If  and  are solutions of linear PDE in some function space , then  c&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;u&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; + c&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;u&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;}} with any constants  and  are also a solution of that PDE in the same function space.&lt;br /&gt;
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若线性偏微分方程在某个函数空间{{mvar|R}}中有解{{math|''u''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;}} 和 {{math|''u''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;}}，则{{math|''u'' {{=}} ''c''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;''u''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; + ''c''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;''u''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;}}也是该偏微分方程在同一函数空间中的解，其中{{math|''c''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;}} 和 {{math|''c''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;}} 是任意常数。&lt;br /&gt;
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===Methods for non-linear equations===&lt;br /&gt;
非线性方程的求解方法&lt;br /&gt;
{{see also|nonlinear partial differential equation}}&lt;br /&gt;
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There are no generally applicable methods to solve nonlinear PDEs. Still, existence and uniqueness results (such as the [[Cauchy–Kowalevski theorem]]) are often possible, as are proofs of important qualitative and quantitative properties of solutions (getting these results is a major part of [[mathematical analysis|analysis]]). Computational solution to the nonlinear PDEs, the [[split-step method]], exist for specific equations like [[nonlinear Schrödinger equation]].&lt;br /&gt;
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There are no generally applicable methods to solve nonlinear PDEs. Still, existence and uniqueness results (such as the Cauchy–Kowalevski theorem) are often possible, as are proofs of important qualitative and quantitative properties of solutions (getting these results is a major part of analysis). Computational solution to the nonlinear PDEs, the split-step method, exist for specific equations like nonlinear Schrödinger equation.&lt;br /&gt;
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对于非线性偏微分方程，目前还没有普遍适用的求解方法。然而，通常是可能知道解的存在性和唯一性(如柯西-科瓦列夫斯基定理)，也是可能得到解的重要定性和定量性质的证明(得到这些结果是分析的主要部分)。非线性偏微分方程的计算解，即分步法，对一些特定的方程适用，比如非线性'''&amp;lt;font color=&amp;quot;#ff8000&amp;quot;&amp;gt;薛定谔方程 Schrödinger equation&amp;lt;/font&amp;gt;'''。&lt;br /&gt;
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Nevertheless, some techniques can be used for several types of equations. The [[h-principle|{{mvar|h}}-principle]] is the most powerful method to solve [[Underdetermined system|underdetermined]] equations. The [[Riquier–Janet theory]] is an effective method for obtaining information about many analytic [[Overdetermined system|overdetermined]] systems.&lt;br /&gt;
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Nevertheless, some techniques can be used for several types of equations. The -principle is the most powerful method to solve underdetermined equations. The Riquier–Janet theory is an effective method for obtaining information about many analytic overdetermined systems.&lt;br /&gt;
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然而，一些技巧可以用于几种类型的方程。h-原理是求解欠定方程最有效的方法。里基尔-珍妮特理论是一种可以获得许多解析超定系统信息的有效方法。&lt;br /&gt;
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The [[method of characteristics]] can be used in some very special cases to solve partial differential equations.&lt;br /&gt;
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The method of characteristics can be used in some very special cases to solve partial differential equations.&lt;br /&gt;
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特征线法可用于求解某些特殊情况下的偏微分方程。&lt;br /&gt;
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In some cases, a PDE can be solved via [[perturbation analysis]] in which the solution is considered to be a correction to an equation with a known solution. Alternatives are [[numerical analysis]] techniques from simple [[finite difference]] schemes to the more mature [[multigrid]] and [[finite element method]]s. Many interesting problems in science and engineering are solved in this way using [[computer]]s, sometimes high performance [[supercomputer]]s.&lt;br /&gt;
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In some cases, a PDE can be solved via perturbation analysis in which the solution is considered to be a correction to an equation with a known solution. Alternatives are numerical analysis techniques from simple finite difference schemes to the more mature multigrid and finite element methods. Many interesting problems in science and engineering are solved in this way using computers, sometimes high performance supercomputers.&lt;br /&gt;
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在某些情况下，偏微分方程可以通过扰动分析来求解。在扰动分析中，通常是求解将具有已知解的方程修正后的新得到方程。可供选择的数值分析技术从简单的差分格式到更成熟的多重网格和有限元方法。许多有趣的科学和工程问题都是在计算机上用这种方法解决的，有时是高性能超级计算机。&lt;br /&gt;
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===Lie group method===&lt;br /&gt;
李群方法&lt;br /&gt;
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From 1870 [[Sophus Lie]]'s work put the theory of differential equations on a more satisfactory foundation. He showed that the integration theories of the older mathematicians can, by the introduction of what are now called [[Lie group]]s, be referred, to a common source; and that ordinary differential equations which admit the same [[infinitesimal transformation]]s present comparable difficulties of integration. He also emphasized the subject of [[contact transformation|transformations of contact]].&lt;br /&gt;
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From 1870 Sophus Lie's work put the theory of differential equations on a more satisfactory foundation. He showed that the integration theories of the older mathematicians can, by the introduction of what are now called Lie groups, be referred, to a common source; and that ordinary differential equations which admit the same infinitesimal transformations present comparable difficulties of integration. He also emphasized the subject of transformations of contact.&lt;br /&gt;
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从1870年起，索弗斯·李的工作为微分方程理论奠定了一个较为令人满意的基础。他指出，通过引入现在所谓的李群，老一辈数学家的积分理论可以引用到一个共同的来源; 承认相同的无穷小变换的常微分方程在积分方面存在相当的困难。他还强调了接触的转变这一主题。&lt;br /&gt;
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==[[用户:Yuling|Yuling]]（[[用户讨论:Yuling|讨论]]）这句话“He also emphasized the subject of transformations of contact.”中的transformations of contact翻译的不太好。&lt;br /&gt;
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A general approach to solving PDEs uses the symmetry property of differential equations, the continuous [[infinitesimal transformation]]s of solutions to solutions ([[Lie theory]]). Continuous [[group theory]], [[Lie algebras]] and [[differential geometry]] are used to understand the structure of linear and nonlinear partial differential equations for generating integrable equations, to find its [[Lax pair]]s, recursion operators, [[Bäcklund transform]] and finally finding exact analytic solutions to the PDE.&lt;br /&gt;
&lt;br /&gt;
A general approach to solving PDEs uses the symmetry property of differential equations, the continuous infinitesimal transformations of solutions to solutions (Lie theory). Continuous group theory, Lie algebras and differential geometry are used to understand the structure of linear and nonlinear partial differential equations for generating integrable equations, to find its Lax pairs, recursion operators, Bäcklund transform and finally finding exact analytic solutions to the PDE.&lt;br /&gt;
&lt;br /&gt;
求解偏微分方程的一般方法是利用微分方程的对称性，即解到解的连续无穷小变换(李理论)。连续群论、李代数和微分几何理论被用来理解生成可积方程的线性和非线性偏微分方程的结构，找到它的Lax对、递归算子、 贝克伦德变换，最后找到偏微分方程的精确解析解。&lt;br /&gt;
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Symmetry methods have been recognized to study differential equations arising in mathematics, physics, engineering, and many other disciplines.&lt;br /&gt;
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Symmetry methods have been recognized to study differential equations arising in mathematics, physics, engineering, and many other disciplines.&lt;br /&gt;
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对称方法已被公认可以用于研究出现在数学，物理，工程和许多其他学科的微分方程。&lt;br /&gt;
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===Semianalytical methods===&lt;br /&gt;
半解析方法&lt;br /&gt;
&lt;br /&gt;
The [[Adomian decomposition method]], the [[Aleksandr Lyapunov|Lyapunov]] artificial small parameter method, and He's [[homotopy perturbation method]] are all special cases of the more general [[homotopy analysis method]]. These are series expansion methods, and except for the Lyapunov method, are independent of small physical parameters as compared to the well known [[perturbation theory]], thus giving these methods greater flexibility and solution generality.&lt;br /&gt;
&lt;br /&gt;
The Adomian decomposition method, the Lyapunov artificial small parameter method, and He's homotopy perturbation method are all special cases of the more general homotopy analysis method. These are series expansion methods, and except for the Lyapunov method, are independent of small physical parameters as compared to the well known perturbation theory, thus giving these methods greater flexibility and solution generality.&lt;br /&gt;
&lt;br /&gt;
阿多米安分解法、李雅普诺夫人工小参数方法和何同伦摄动方法都是更一般的同伦分析方法的特殊情况。除了李雅普诺夫方法之外，这些都是级数展开方法，与为人熟知的摄动理论方法相比，它们与小的物理参数无关，因此这些方法具有更大的灵活性和解的通用性。&lt;br /&gt;
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== Numerical solutions ==&lt;br /&gt;
数值解&lt;br /&gt;
&lt;br /&gt;
The three most widely used [[Numerical partial differential equations|numerical methods to solve PDEs]] are the [[finite element analysis|finite element method]] (FEM), [[finite volume method]]s (FVM) and [[finite difference method]]s (FDM), as well other kind of methods called [[Meshfree methods]], which were made to solve problems where the before mentioned methods are limited. The FEM has a prominent position among these methods and especially its exceptionally efficient higher-order version [[hp-FEM]]. Other hybrid versions of FEM and Meshfree methods include the generalized finite element method (GFEM), [[extended finite element method]] (XFEM), [[Spectral element method|spectral finite element method]] (SFEM), [[Meshfree methods|meshfree finite element method]], [[Discontinuous Galerkin Method|discontinuous Galerkin finite element method]] (DGFEM), [[Element-Free Galerkin Method]] (EFGM), [[Interpolating Element-Free Galerkin Method]] (IEFGM), etc.&lt;br /&gt;
&lt;br /&gt;
The three most widely used numerical methods to solve PDEs are the finite element method (FEM), finite volume methods (FVM) and finite difference methods (FDM), as well other kind of methods called Meshfree methods, which were made to solve problems where the before mentioned methods are limited. The FEM has a prominent position among these methods and especially its exceptionally efficient higher-order version hp-FEM. Other hybrid versions of FEM and Meshfree methods include the generalized finite element method (GFEM), extended finite element method (XFEM), spectral finite element method (SFEM), meshfree finite element method, discontinuous Galerkin finite element method (DGFEM), Element-Free Galerkin Method (EFGM), Interpolating Element-Free Galerkin Method (IEFGM), etc.&lt;br /&gt;
&lt;br /&gt;
求解偏微分方程最常用的三种数值方法是有限元分析法、有限体积法和有限差分法，以及其他一些称为无网格法的方法。这些方法用于解决前面提到的方法受到的限制。在这些方法中，有限元方法，尤其是高效的高阶有限元方法，占有重要地位。其他有限元法和无网格法的混合形式包括广义有限元分析法(GFEM)、扩展有限元分析法(XFEM)、谱有限元分析法(SFEM)、无网格有限元分析法(DGFEM)、间断伽辽金有限元分析法(DGFEM)、无网格伽辽金法(EFGM)、插值无网格伽辽金法(IEFGM)等。&lt;br /&gt;
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=== Finite element method ===&lt;br /&gt;
有限元分析法&lt;br /&gt;
&lt;br /&gt;
{{main|Finite element method}}&lt;br /&gt;
&lt;br /&gt;
The finite element method (FEM) (its practical application often known as finite element analysis (FEA)) is a numerical technique for finding approximate solutions of partial differential equations (PDE) as well as of integral equations. The solution approach is based either on eliminating the differential equation completely (steady state problems), or rendering the PDE into an approximating system of ordinary differential equations, which are then numerically integrated using standard techniques such as Euler's method, Runge–Kutta, etc.&lt;br /&gt;
&lt;br /&gt;
The finite element method (FEM) (its practical application often known as finite element analysis (FEA)) is a numerical technique for finding approximate solutions of partial differential equations (PDE) as well as of integral equations. The solution approach is based either on eliminating the differential equation completely (steady state problems), or rendering the PDE into an approximating system of ordinary differential equations, which are then numerically integrated using standard techniques such as Euler's method, Runge–Kutta, etc.&lt;br /&gt;
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'''&amp;lt;font color = &amp;quot;#ff8000&amp;quot;&amp;gt;有限元分析法 Finite Element Method&amp;lt;/font&amp;gt;''' ((其实际应用通常被称为有限元分析(FEA))是一种寻找偏微分方程(PDE)和积分方程近似解的数值技术。这种求解方法要么基于完全消除微分方程(稳态问题) ，要么将偏微分方程转化为常微分方程的近似系统，然后使用标准技术进行数值积分，如欧拉方法、 Runge-Kutta 等。&lt;br /&gt;
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===Finite difference method===&lt;br /&gt;
有限差分法&lt;br /&gt;
&lt;br /&gt;
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{{main|Finite difference method}}&lt;br /&gt;
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Finite-difference methods are numerical methods for approximating the solutions to differential equations using [[finite difference]] equations to approximate derivatives.&lt;br /&gt;
&lt;br /&gt;
Finite-difference methods are numerical methods for approximating the solutions to differential equations using finite difference equations to approximate derivatives.&lt;br /&gt;
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有限差分法是一种数值方法，用差分方程近似微分方程的解。&lt;br /&gt;
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=== Finite volume method ===&lt;br /&gt;
有限体积法&lt;br /&gt;
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{{main|Finite volume method}}&lt;br /&gt;
&lt;br /&gt;
Similar to the finite difference method or finite element method, values are calculated at discrete places on a meshed geometry. &amp;quot;Finite volume&amp;quot; refers to the small volume surrounding each node point on a mesh. In the finite volume method, surface integrals in a partial differential equation that contain a divergence term are converted to volume integrals, using the [[divergence theorem]]. These terms are then evaluated as fluxes at the surfaces of each finite volume. Because the flux entering a given volume is identical to that leaving the adjacent volume, these methods conserve mass by design.&lt;br /&gt;
&lt;br /&gt;
Similar to the finite difference method or finite element method, values are calculated at discrete places on a meshed geometry. &amp;quot;Finite volume&amp;quot; refers to the small volume surrounding each node point on a mesh. In the finite volume method, surface integrals in a partial differential equation that contain a divergence term are converted to volume integrals, using the divergence theorem. These terms are then evaluated as fluxes at the surfaces of each finite volume. Because the flux entering a given volume is identical to that leaving the adjacent volume, these methods conserve mass by design.&lt;br /&gt;
&lt;br /&gt;
类似于有限差分法或有限元分析，函数值是在网状几何体上的离散位置进行计算的。“有限体积”是指网格上每个节点周围的小体积。在有限体积法中，偏微分方程中含有散度项的面积分用散度定理积分转换成体积分。然后将这些项用于估算每个有限体积表面上的通量。由于进入给定体积的通量与转移到相邻体积元的通量相同，所以这些方法在设计上保证了质量守恒。&lt;br /&gt;
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==See also==&lt;br /&gt;
请参阅&lt;br /&gt;
* [[Dirichlet boundary condition]]&lt;br /&gt;
狄利克雷边界条件&lt;br /&gt;
* [[Jet bundle]]&lt;br /&gt;
射流丛&lt;br /&gt;
* [[Laplace transform applied to differential equations]]&lt;br /&gt;
微分方程中的拉普拉斯变换&lt;br /&gt;
* [[List of dynamical systems and differential equations topics]]&lt;br /&gt;
动力学系统和微分方程的列表&lt;br /&gt;
* [[Matrix differential equation]]&lt;br /&gt;
矩阵微分方程&lt;br /&gt;
* [[Neumann boundary condition]]&lt;br /&gt;
诺伊曼边界条件&lt;br /&gt;
* [[Numerical partial differential equations]]&lt;br /&gt;
数值偏微分方程&lt;br /&gt;
* [[Partial differential algebraic equation]]&lt;br /&gt;
偏微分代数方程&lt;br /&gt;
* [[Recurrence relation]]&lt;br /&gt;
递推关系&lt;br /&gt;
* [[Robin boundary condition]]&lt;br /&gt;
罗宾边界条件&lt;br /&gt;
* [[Stochastic processes and boundary value problems]]&lt;br /&gt;
随机过程和边值问题&lt;br /&gt;
&lt;br /&gt;
== The energy method ==&lt;br /&gt;
能量法&lt;br /&gt;
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The energy method is a mathematical procedure that can be used to verify well-posedness of initial-boundary-value-problems.&amp;lt;ref&amp;gt;{{cite book |title=High Order Difference Methods for Time Dependent PDE&lt;br /&gt;
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The energy method is a mathematical procedure that can be used to verify well-posedness of initial-boundary-value-problems.&amp;lt;ref&amp;gt;{{cite book |title=High Order Difference Methods for Time Dependent PDE&lt;br /&gt;
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能量法是验证初边值问题适定性的一种数学方法。 时变偏微分方程的高阶差分方法&lt;br /&gt;
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能量法是一种数学过程，可用于验证初始边界值问题的适定性。在下面的示例中，将使用能量法决定应在何处施加哪些边界条件，以使得到的IBVP处于适当位置。考虑下式给出的一维双曲PDE&lt;br /&gt;
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|first=Bertil|last=Gustafsson|publisher=Springer|year=2008|isbn=978-3-540-74992-9|doi=10.1007/978-3-540-74993-6}}&amp;lt;/ref&amp;gt; In the following example the energy method is used to decide where and which boundary conditions should be imposed such that the resulting IBVP is well-posed. Consider the one-dimensional hyperbolic PDE given by&lt;br /&gt;
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|first=Bertil|last=Gustafsson|publisher=Springer|year=2008|isbn=978-3-540-74992-9|doi=10.1007/978-3-540-74993-6}}&amp;lt;/ref&amp;gt; In the following example the energy method is used to decide where and which boundary conditions should be imposed such that the resulting IBVP is well-posed. Consider the one-dimensional hyperbolic PDE given by&lt;br /&gt;
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| first Bertil | last Gustafsson | publisher | Springer | year 2008 | isbn 978-3-540-74992-9 | doi 10.1007 / 978-3-540-74993-6} / ref 在下面的例子中，使用能量方法来决定应该施加哪些边界条件，使得得到的 IBVP适定。考虑一维双曲偏微分方程&lt;br /&gt;
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: &amp;lt;math&amp;gt;\frac{\partial u}{\partial t} + \alpha \frac{\partial u}{\partial x} = 0, \quad x \in [a,b], \operatorname t &amp;gt; 0,&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;\frac{\partial u}{\partial t} + \alpha \frac{\partial u}{\partial x} = 0, \quad x \in [a,b], \operatorname t &amp;gt; 0,&amp;lt;/math&amp;gt;&lt;br /&gt;
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where &amp;lt;math&amp;gt;\alpha \neq 0&amp;lt;/math&amp;gt; is a constant and &amp;lt;math&amp;gt;u(x,t)&amp;lt;/math&amp;gt; is an unknown function with initial condition &amp;lt;math&amp;gt;u(x,0) = f(x)&amp;lt;/math&amp;gt;. Multiplying with &amp;lt;math&amp;gt;u&amp;lt;/math&amp;gt; and integrating over the domain gives&lt;br /&gt;
&lt;br /&gt;
where &amp;lt;math&amp;gt;\alpha \neq 0&amp;lt;/math&amp;gt; is a constant and &amp;lt;math&amp;gt;u(x,t)&amp;lt;/math&amp;gt; is an unknown function with initial condition &amp;lt;math&amp;gt;u(x,0) = f(x)&amp;lt;/math&amp;gt;. Multiplying with &amp;lt;math&amp;gt;u&amp;lt;/math&amp;gt; and integrating over the domain gives&lt;br /&gt;
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其中 &amp;lt;math&amp;gt;\alpha \neq 0&amp;lt;/math&amp;gt; 是常数，并且 &amp;lt;math&amp;gt;u(x,t)&amp;lt;/math&amp;gt; 是未知函数，初始条件是 &amp;lt;math&amp;gt;u(x,0) = f(x)&amp;lt;/math&amp;gt;。乘以 &amp;lt;math&amp;gt;u&amp;lt;/math&amp;gt; 并在域上进行积分。&lt;br /&gt;
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: &amp;lt;math&amp;gt;\int_a^b u \frac{\partial u}{\partial t} \operatorname dx + \alpha \int _a ^b u \frac{\partial u}{\partial x} \operatorname dx = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;\int_a^b u \frac{\partial u}{\partial t} \operatorname dx + \alpha \int _a ^b u \frac{\partial u}{\partial x} \operatorname dx = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
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Using that&lt;br /&gt;
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Using that&lt;br /&gt;
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利用这一点&lt;br /&gt;
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: &amp;lt;math&amp;gt;\int _a ^b u \frac{\partial u}{\partial t} \operatorname dx = \frac{1}{2} \frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 \quad \text{and} \quad \int _a ^b u \frac{\partial u}{\partial x} \operatorname dx = \frac{1}{2} u(b,t)^2 - \frac{1}{2} u(a,t)^2,.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;\int _a ^b u \frac{\partial u}{\partial t} \operatorname dx = \frac{1}{2} \frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 \quad \text{and} \quad \int _a ^b u \frac{\partial u}{\partial x} \operatorname dx = \frac{1}{2} u(b,t)^2 - \frac{1}{2} u(a,t)^2,.&amp;lt;/math&amp;gt;&lt;br /&gt;
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where integration by parts has been used for the second relationship, we get&lt;br /&gt;
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where integration by parts has been used for the second relationship, we get&lt;br /&gt;
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第二个关系中采用了分部积分法，我们可以得到&lt;br /&gt;
&lt;br /&gt;
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: &amp;lt;math&amp;gt;\frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 + \alpha u(b,t)^2 - \alpha u(a,t)^2 = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;\frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 + \alpha u(b,t)^2 - \alpha u(a,t)^2 = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
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Here &amp;lt;math&amp;gt;\vert \vert \cdot \vert \vert&amp;lt;/math&amp;gt; denotes the standard L2-norm.&lt;br /&gt;
&lt;br /&gt;
Here &amp;lt;math&amp;gt;\vert \vert \cdot \vert \vert&amp;lt;/math&amp;gt; denotes the standard L2-norm.&lt;br /&gt;
&lt;br /&gt;
在这里，&amp;lt;math&amp;gt;\vert \vert \cdot \vert \vert&amp;lt;/math&amp;gt; 表示标准的 L2-正则。&lt;br /&gt;
&lt;br /&gt;
For well-posedness we require that the energy of the solution is non-increasing, i.e. that &amp;lt;math&amp;gt;\frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 \leq 0&amp;lt;/math&amp;gt;, which is achieved by specifying &amp;lt;math&amp;gt;u&amp;lt;/math&amp;gt; at &amp;lt;math&amp;gt;x = a&amp;lt;/math&amp;gt; if &amp;lt;math&amp;gt;\alpha &amp;gt; 0&amp;lt;/math&amp;gt; and at &amp;lt;math&amp;gt;x = b&amp;lt;/math&amp;gt; if &amp;lt;math&amp;gt;\alpha &amp;lt; 0&amp;lt;/math&amp;gt;. This corresponds to only imposing boundary conditions at the inflow. Note that well-posedness allows for growth in terms of data (initial and boundary) and thus it is sufficient to show that &amp;lt;math&amp;gt;\frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 \leq 0&amp;lt;/math&amp;gt; holds when all data is set to zero.&lt;br /&gt;
&lt;br /&gt;
For well-posedness we require that the energy of the solution is non-increasing, i.e. that &amp;lt;math&amp;gt;\frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 \leq 0&amp;lt;/math&amp;gt;, which is achieved by specifying &amp;lt;math&amp;gt;u&amp;lt;/math&amp;gt; at &amp;lt;math&amp;gt;x = a&amp;lt;/math&amp;gt; if &amp;lt;math&amp;gt;\alpha &amp;gt; 0&amp;lt;/math&amp;gt; and at &amp;lt;math&amp;gt;x = b&amp;lt;/math&amp;gt; if &amp;lt;math&amp;gt;\alpha &amp;lt; 0&amp;lt;/math&amp;gt;. This corresponds to only imposing boundary conditions at the inflow. Note that well-posedness allows for growth in terms of data (initial and boundary) and thus it is sufficient to show that &amp;lt;math&amp;gt;\frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 \leq 0&amp;lt;/math&amp;gt; holds when all data is set to zero.&lt;br /&gt;
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对于适定性，我们要解的能量是不增加的，即 &amp;lt;math&amp;gt;\frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 \leq 0&amp;lt;/math&amp;gt; ，这种关系可以通过在&amp;lt;math&amp;gt;x = a&amp;lt;/math&amp;gt;处 （如果 &amp;lt;math&amp;gt;\alpha &amp;gt; 0&amp;lt;/math&amp;gt;） 以及 &amp;lt;math&amp;gt;x = b&amp;lt;/math&amp;gt;处 （如果 &amp;lt;math&amp;gt;\alpha &amp;lt; 0&amp;lt;/math&amp;gt;）指定&amp;lt;math&amp;gt;u&amp;lt;/math&amp;gt;的值来实现。这只相当于在入流处附加边界条件。注意，适定性允许在数据(初始和边界)上的增长，因此它足以表明当所有数据设置为零时应有 &amp;lt;math&amp;gt;\frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 \leq 0&amp;lt;/math&amp;gt;。&lt;br /&gt;
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==[[用户:Yuling|Yuling]]（[[用户讨论:Yuling|讨论]]）“This corresponds to only imposing boundary conditions at the inflow.” 这句话中的inflow不是很理解&lt;br /&gt;
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==Notes==&lt;br /&gt;
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{{Reflist}}&lt;br /&gt;
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== References ==&lt;br /&gt;
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{{refbegin|2}}&lt;br /&gt;
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* {{cite book |title=Solving Frontier problems of Physics: The decomposition method&lt;br /&gt;
&lt;br /&gt;
|first=G.|last=Adomian|publisher=Kluwer Academic Publishers|year=1994|isbn=|page=|url=https://books.google.com/books?id=UKPqCAAAQBAJ&amp;amp;printsec=frontcover#v=onepage&amp;amp;q=%22partial%20differential%22&amp;amp;f=false}}&lt;br /&gt;
&lt;br /&gt;
|first=G.|last=Adomian|publisher=Kluwer Academic Publishers|year=1994|isbn=|page=|url=https://books.google.com/books?id=UKPqCAAAQBAJ&amp;amp;printsec=frontcover#v=onepage&amp;amp;q=%22partial%20differential%22&amp;amp;f=false}}&lt;br /&gt;
&lt;br /&gt;
1994年 | isbn | 页面 | 网址: 施普林格科学+商业媒体 https://books.google.com/books?id=ukpqcaaaqbaj&amp;amp;printsec=frontcover#v=onepage&amp;amp;q=%22partial%20differential%22&amp;amp;f=false&lt;br /&gt;
&lt;br /&gt;
* {{Citation |first=R. |last=Courant |lastauthoramp=yes |first2=D. |last2=Hilbert |title=Methods of Mathematical Physics |volume=II |publisher=Wiley-Interscience |location=New York |year=1962 |url=https://books.google.com/books?id=fcZV4ohrerwC&amp;amp;printsec=frontcover#v=onepage&amp;amp;q&amp;amp;f=false}}.&lt;br /&gt;
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* {{Citation |authorlink=Lawrence C. Evans |first=L. C. |last=Evans |title=Partial Differential Equations |publisher=American Mathematical Society |location=Providence |year=1998 |isbn=0-8218-0772-2 }}.&lt;br /&gt;
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* {{cite book|last1=Holubová|first1=Pavel Drábek ; Gabriela|title=Elements of partial differential equations|date=2007|publisher=de Gruyter|location=Berlin|isbn=9783110191240|edition=[Online-Ausg.].}}&lt;br /&gt;
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* {{Citation |first=Nail H |last=Ibragimov |title=CRC Handbook of Lie Group Analysis of Differential Equations Vol. 1-3 |publisher=CRC-Press |location=Providence |year=1993 |isbn=0-8493-4488-3 }}.&lt;br /&gt;
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* {{Citation |first=A. D. |last=Polyanin |first2=V. F. |last2=Zaitsev |lastauthoramp=yes |first3=A. |last3=Moussiaux |title=Handbook of First Order Partial Differential Equations |publisher=Taylor &amp;amp; Francis |location=London |year=2002 |isbn=0-415-27267-X }}.&lt;br /&gt;
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* {{Citation |first=P. |last=Solin |title=Partial Differential Equations and the Finite Element Method |publisher=J. Wiley &amp;amp; Sons |location=Hoboken, NJ |year=2005 |isbn=0-471-72070-4 }}.&lt;br /&gt;
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* {{Citation |first=P. |last=Solin |first2=K. |last2=Segeth |lastauthoramp=yes |first3=I. |last3=Dolezel |title=Higher-Order Finite Element Methods |publisher=Chapman &amp;amp; Hall/CRC Press |location=Boca Raton |year=2003 |isbn=1-58488-438-X }}.&lt;br /&gt;
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* {{Citation |first=H. |last=Stephani |year=1989 |title=Differential Equations: Their Solution Using Symmetries. Edited by M. MacCallum |publisher=Cambridge University Press }}.&lt;br /&gt;
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* {{cite book |title=Partial Differential Equations and Solitary Waves Theory&lt;br /&gt;
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|first=Abdul-Majid|last=Wazwaz|publisher=Higher Education Press|year=2009|isbn=978-3-642-00251-9|page=}}&lt;br /&gt;
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| first Abdul-Majid | last Wazwaz | publisher Higher Education Press | year 2009 | isbn 978-3-642-00251-9 | page }&lt;br /&gt;
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* {{cite book |title=Partial Differential Equations Methods and Applications&lt;br /&gt;
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|first=Abdul-Majid|last=Wazwaz|publisher=A.A. Balkema|year=2002|isbn=90-5809-369-7|page=}}&lt;br /&gt;
&lt;br /&gt;
| first Abdul-Majid | last Wazwaz | publisher a.a.Balkema | year 2002 | isbn 90-5809-369-7 | page }&lt;br /&gt;
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* {{Citation |first=D. |last=Zwillinger |title=Handbook of Differential Equations |publisher=Academic Press |location=Boston |year=1997 |edition=3rd |isbn=0-12-784395-7 }}.&lt;br /&gt;
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* {{Citation |authorlink=Neil Gershenfeld |first=N. |last=Gershenfeld |title=The Nature of Mathematical Modeling |location=New York |publisher=Cambridge University Press, New York, NY, USA |year=1999 |edition=1st |isbn=0-521-57095-6 }}.&lt;br /&gt;
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* {{Citation |first=I.S. |last=Krasil'shchik |lastauthoramp=yes |first2=A.M., Eds. |last2=Vinogradov |title=Symmetries and Conserwation Laws for Differential Equations of Mathematical Physics |publisher=American Mathematical Society, Providence, Rhode Island, USA |year=1999 |isbn=0-8218-0958-X }}.&lt;br /&gt;
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* {{Citation |first=I.S. |last=Krasil'shchik |first2=V.V. |last2=Lychagin|lastauthoramp=yes |first3=A.M. |last3=Vinogradov |title=Geometry of Jet Spaces and Nonlinear Partial Differential Equations |publisher=Gordon and Breach Science Publishers, New York, London, Paris, Montreux, Tokyo |year=1986 |isbn=2-88124-051-8 }}.&lt;br /&gt;
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* {{Citation |first=A.M. |last=Vinogradov |title=Cohomological Analysis of Partial Differential Equations and Secondary Calculus |publisher=American Mathematical Society, Providence, Rhode Island, USA |year=2001 |isbn=0-8218-2922-X }}.&lt;br /&gt;
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* {{cite book |title=High Order Difference Methods for Time Dependent PDE&lt;br /&gt;
&lt;br /&gt;
|first=Bertil|last=Gustafsson|publisher=Springer|year=2008|isbn=978-3-540-74992-9|doi=10.1007/978-3-540-74993-6}}&lt;br /&gt;
&lt;br /&gt;
|first=Bertil|last=Gustafsson|publisher=Springer|year=2008|isbn=978-3-540-74992-9|doi=10.1007/978-3-540-74993-6}}&lt;br /&gt;
&lt;br /&gt;
| first Bertil | last Gustafsson | Springer | year 2008 | isbn 978-3-540-74992-9 | doi 10.1007 / 978-3-540-74993-6}&lt;br /&gt;
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{{refend}}&lt;br /&gt;
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== Further reading ==&lt;br /&gt;
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* {{Cite journal|last=Cajori|first=Florian|authorlink=Florian Cajori|year=1928|title=The Early History of Partial Differential Equations and of Partial Differentiation and Integration|url=http://www.math.harvard.edu/archive/21a_fall_14/exhibits/cajori/cajori.pdf|journal=The American Mathematical Monthly|volume=35|issue=9|pages=459–467|doi=10.2307/2298771|access-date=2016-05-15|archive-url=https://web.archive.org/web/20181123102253/http://www.math.harvard.edu/archive/21a_fall_14/exhibits/cajori/cajori.pdf|archive-date=2018-11-23|url-status=dead}}&lt;br /&gt;
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== External links ==&lt;br /&gt;
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{{Sister project links| wikt=no | commons=Category:Solutions of PDE | b=Partial Differential Equations | n=no | q=Partial differential equation | s=no | v=no | voy=no | species=no | d=no}}&lt;br /&gt;
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* {{springer|title=Differential equation, partial|id=p/d031920}}&lt;br /&gt;
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* [http://eqworld.ipmnet.ru/en/pde-en.htm Partial Differential Equations: Exact Solutions] at EqWorld: The World of Mathematical Equations.&lt;br /&gt;
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* [http://eqworld.ipmnet.ru/en/solutions/eqindex/eqindex-pde.htm Partial Differential Equations: Index] at EqWorld: The World of Mathematical Equations.&lt;br /&gt;
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* [http://eqworld.ipmnet.ru/en/methods/meth-pde.htm Partial Differential Equations: Methods] at EqWorld: The World of Mathematical Equations.&lt;br /&gt;
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* [https://web.archive.org/web/20170701144823/http://www.exampleproblems.com/wiki/index.php?title=Partial_Differential_Equations Example problems with solutions] at exampleproblems.com&lt;br /&gt;
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* [http://mathworld.wolfram.com/PartialDifferentialEquation.html Partial Differential Equations] at mathworld.wolfram.com&lt;br /&gt;
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* [https://reference.wolfram.com/language/FEMDocumentation/tutorial/SolvingPDEwithFEM.html Partial Differential Equations] with Mathematica&lt;br /&gt;
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* [http://www.mathworks.com/moler/pdes.pdf Partial Differential Equations] in Cleve Moler: Numerical Computing with MATLAB&lt;br /&gt;
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* [http://www.nag.com/numeric/fl/nagdoc_fl24/html/D03/d03intro.html Partial Differential Equations] at nag.com&lt;br /&gt;
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* {{cite web |first=Grant |last=Sanderson |title=But what is a partial differential equation? |work=3Blue1Brown |date=April 21, 2019 |url=https://www.youtube.com/watch?v=ly4S0oi3Yz8&amp;amp;list=PLZHQObOWTQDNPOjrT6KVlfJuKtYTftqH6 |via=[[YouTube]] }}&lt;br /&gt;
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{{Differential equations topics}}&lt;br /&gt;
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[[Category:Partial differential equations| ]]&lt;br /&gt;
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[[Category:Multivariable calculus]]&lt;br /&gt;
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Category:Multivariable calculus&lt;br /&gt;
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类别: 多元微积分&lt;br /&gt;
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[[Category:Differential equations]]&lt;br /&gt;
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Category:Differential equations&lt;br /&gt;
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类别: 微分方程&lt;br /&gt;
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[[Category:Concepts in physics]]&lt;br /&gt;
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Category:Concepts in physics&lt;br /&gt;
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&amp;lt;small&amp;gt;This page was moved from [[wikipedia:en:Partial differential equation]]. Its edit history can be viewed at [[偏微分方程/edithistory]]&amp;lt;/small&amp;gt;&amp;lt;/noinclude&amp;gt;&lt;br /&gt;
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[[Category:待整理页面]]&lt;/div&gt;</summary>
		<author><name>Ruili</name></author>
	</entry>
	<entry>
		<id>https://wiki.swarma.org/index.php?title=%E5%81%8F%E5%BE%AE%E5%88%86%E6%96%B9%E7%A8%8B&amp;diff=20101</id>
		<title>偏微分方程</title>
		<link rel="alternate" type="text/html" href="https://wiki.swarma.org/index.php?title=%E5%81%8F%E5%BE%AE%E5%88%86%E6%96%B9%E7%A8%8B&amp;diff=20101"/>
		<updated>2020-12-15T12:16:15Z</updated>

		<summary type="html">&lt;p&gt;Ruili：&lt;/p&gt;
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&lt;div&gt;此词条暂由Yuling翻译，未经人工整理和审校，带来阅读不便，请见谅。&lt;br /&gt;
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[[File:Heat.gif|thumb|right|A visualisation of a solution to the two-dimensional [[heat equation]] with temperature represented by the third dimension]]&lt;br /&gt;
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A visualisation of a solution to the two-dimensional [[heat equation with temperature represented by the third dimension]]&lt;br /&gt;
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以三维表示温度的二维热方程解的可视化&lt;br /&gt;
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In [[mathematics]], a '''partial differential equation''' ('''PDE''') is a [[differential equation]] that contains unknown [[Multivariable calculus|multivariable functions]] and their [[partial derivative]]s. PDEs are used to formulate problems involving functions of several variables, and are either solved by hand, or used to create a [[computer model]]. A special case is [[ordinary differential equation]]s (ODEs), which deal with functions of a single variable and their derivatives.&lt;br /&gt;
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In mathematics, a partial differential equation (PDE) is a differential equation that contains unknown multivariable functions and their partial derivatives. PDEs are used to formulate problems involving functions of several variables, and are either solved by hand, or used to create a computer model. A special case is ordinary differential equations (ODEs), which deal with functions of a single variable and their derivatives.&lt;br /&gt;
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在数学中，'''&amp;lt;font color = &amp;quot;#ff8000&amp;quot;&amp;gt; 偏微分方程函数 Partial Differential Equation&amp;lt;/font&amp;gt;'''是包含未知多元函数及其偏导数的微分方程。偏微分方程用于描述涉及多元函数的问题，可以通过人为求解，也可以通过建立计算机模型来求解。常微分方程是偏微分方程一种特殊情况，它处理的是一元函数及其导数。&lt;br /&gt;
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PDEs can be used to describe a wide variety of phenomena such as sound, heat, [[diffusion]], [[electrostatics]], [[Electromagnetism|electrodynamics]], [[fluid dynamics]], [[Elasticity (physics)|elasticity]], [[gravitation]] and [[quantum mechanics]]. These seemingly distinct physical phenomena can be formalised similarly in terms of PDEs. Just as ordinary differential equations often model one-dimensional [[dynamical system]]s, partial differential equations often model [[multidimensional system]]s. PDEs find their generalisation in [[stochastic partial differential equation]]s.&lt;br /&gt;
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PDEs can be used to describe a wide variety of phenomena such as sound, heat, diffusion, electrostatics, electrodynamics, fluid dynamics, elasticity, gravitation and quantum mechanics. These seemingly distinct physical phenomena can be formalised similarly in terms of PDEs. Just as ordinary differential equations often model one-dimensional dynamical systems, partial differential equations often model multidimensional systems. PDEs find their generalisation in stochastic partial differential equations.&lt;br /&gt;
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偏微分方程可以用来描述各种各样的物理现象，如声音，热量，扩散，静电，电动力学，流体力学，弹性力学，重力和量子力学。这些看起来截然不同的物理现象却可以用类似的偏微分方程来描述。正如常微分方程经常对一维动力系统进行建模一样，偏微分方程经常对多维系统进行建模。随机偏微分方程是偏微分方程的一种推广。&lt;br /&gt;
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== Introduction ==&lt;br /&gt;
引言&lt;br /&gt;
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Partial differential equations (PDEs) are equations that involve rates of change with respect to [[continuous variables]]. For example, the position of a [[rigid body]] is specified by six parameters,&amp;lt;ref&amp;gt;{{Cite book|url=https://books.google.com/books?id=v9PLbcYd9aUC&amp;amp;pg=PA32|title=Modelling and Control of Robot Manipulators|last=Sciavicco|first=Lorenzo|last2=Siciliano|first2=Bruno|date=2001-02-19|publisher=Springer Science &amp;amp; Business Media|isbn=9781852332211|language=en}}&amp;lt;/ref&amp;gt; but the configuration of a [[fluid]] is given by the [[continuous distribution]] of several parameters, such as the [[temperature]], [[pressure]], and so forth. The dynamics for the rigid body take place in a finite-dimensional [[Configuration space (physics)|configuration space]]; the dynamics for the fluid occur in an infinite-dimensional configuration space. This distinction usually makes PDEs much harder to solve than ordinary differential equations (ODEs), but here again, there will be simple solutions for linear problems. Classic domains where PDEs are used include [[acoustics]], [[fluid dynamics]], [[electrodynamics]], and [[heat transfer]].&lt;br /&gt;
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Partial differential equations (PDEs) are equations that involve rates of change with respect to continuous variables. For example, the position of a rigid body is specified by six parameters, but the configuration of a fluid is given by the continuous distribution of several parameters, such as the temperature, pressure, and so forth. The dynamics for the rigid body take place in a finite-dimensional configuration space; the dynamics for the fluid occur in an infinite-dimensional configuration space. This distinction usually makes PDEs much harder to solve than ordinary differential equations (ODEs), but here again, there will be simple solutions for linear problems. Classic domains where PDEs are used include acoustics, fluid dynamics, electrodynamics, and heat transfer.&lt;br /&gt;
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偏微分方程(简称为PDEs)涉及到方程相对于连续变量的变化率。例如，刚体的位置是由六个参数确定的，而流体的状态是由几个参数的连续分布给出的，如温度、压力等。刚体的动力学过程发生在有限维状态空间中，流体的动力学过程发生在无限维状态空间中。这种区别通常使偏微分方程比常微分方程更难求解，但是线性问题仍然有简单的求解方式。使用偏微分方程的经典领域包括声学、流体力学、电动力学和传热学。&lt;br /&gt;
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A partial differential equation (PDE) for the function {{math|''u''(''x''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;,… ''x&amp;lt;sub&amp;gt;n&amp;lt;/sub&amp;gt;'')}} is an equation of the form&lt;br /&gt;
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A partial differential equation (PDE) for the function  is an equation of the form&lt;br /&gt;
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函数 {{math|''u''(''x''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;,… ''x&amp;lt;sub&amp;gt;n&amp;lt;/sub&amp;gt;'')}} 的偏微分方程形式是：&lt;br /&gt;
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: &amp;lt;math&amp;gt;f \left (x_1, \ldots x_n; u, \frac{\partial u}{\partial x_1}, \ldots \frac{\partial u}{\partial x_n}; \frac{\partial^2 u}{\partial x_1 \partial x_1}, \ldots \frac{\partial^2 u}{\partial x_1 \partial x_n}; \ldots \right) = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;f \left (x_1, \ldots x_n; u, \frac{\partial u}{\partial x_1}, \ldots \frac{\partial u}{\partial x_n}; \frac{\partial^2 u}{\partial x_1 \partial x_1}, \ldots \frac{\partial^2 u}{\partial x_1 \partial x_n}; \ldots \right) = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
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If {{mvar|f}} is a [[linear function]] of {{mvar|u}} and its derivatives, then the PDE is called linear. Common examples of linear PDEs include the [[heat equation]], the [[wave equation]], [[Laplace's equation]], [[Helmholtz equation]], [[Klein–Gordon equation]], and [[Poisson's equation]].&lt;br /&gt;
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If  is a linear function of  and its derivatives, then the PDE is called linear. Common examples of linear PDEs include the heat equation, the wave equation, Laplace's equation, Helmholtz equation, Klein–Gordon equation, and Poisson's equation.&lt;br /&gt;
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如果 {{mvar|f}} 是函数 {{math|''u''}} 及其导数的线性函数，则偏微分方程称为线性函数。线性偏微分方程的常见例子包括热方程、波动方程、拉普拉斯方程、亥姆霍兹方程方程、克莱因-高登方程和泊松方程。&lt;br /&gt;
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A relatively simple PDE is&lt;br /&gt;
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A relatively simple PDE is&lt;br /&gt;
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一个相对简单的偏微分方程：&lt;br /&gt;
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: &amp;lt;math&amp;gt;\frac{\partial u}{\partial x}(x,y) = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;\frac{\partial u}{\partial x}(x,y) = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
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This relation [[Logical implication|implies]] that the function {{math|''u''(''x'',''y'')}} is independent of {{mvar|x}}. However, the equation gives no information on the function's dependence on the variable {{mvar|y}}. Hence the general solution of this equation is&lt;br /&gt;
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This relation implies that the function  is independent of . However, the equation gives no information on the function's dependence on the variable . Hence the general solution of this equation is&lt;br /&gt;
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这意味着函数 {{math|''u''(''x'',''y'')}} 独立于 {{mvar|x}} 的。然而，这个方程没有给出关于函数和自变量的相关性的信息。因此，这个方程的通解是&lt;br /&gt;
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: &amp;lt;math&amp;gt;u(x,y) = f(y),&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;u(x,y) = f(y),&amp;lt;/math&amp;gt;&lt;br /&gt;
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where {{mvar|f}} is an arbitrary function of {{mvar|y}}. The analogous ordinary differential equation is&lt;br /&gt;
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where  is an arbitrary function of . The analogous ordinary differential equation is&lt;br /&gt;
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其中， {{mvar|f}} 是 {{mvar|y}} 的任意函数。&lt;br /&gt;
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类似的常微分方程是：&lt;br /&gt;
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: &amp;lt;math&amp;gt;\frac{\mathrm{d} u}{\mathrm{d} x}(x) = 0,&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;\frac{\mathrm{d} u}{\mathrm{d} x}(x) = 0,&amp;lt;/math&amp;gt;&lt;br /&gt;
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&lt;br /&gt;
&lt;br /&gt;
which has the solution&lt;br /&gt;
&lt;br /&gt;
which has the solution&lt;br /&gt;
&lt;br /&gt;
它的解为&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt;u(x) = c,&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;u(x) = c,&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
where {{mvar|c}} is any [[Constant (mathematics)|constant]] value. These two examples illustrate that general solutions of ordinary differential equations (ODEs) involve arbitrary constants, but solutions of PDEs involve arbitrary functions.&lt;br /&gt;
&lt;br /&gt;
where  is any constant value. These two examples illustrate that general solutions of ordinary differential equations (ODEs) involve arbitrary constants, but solutions of PDEs involve arbitrary functions.&lt;br /&gt;
&lt;br /&gt;
这里，{{mvar|c}} 是一个任意常量。&lt;br /&gt;
&lt;br /&gt;
这两个例子说明常微分方程的一般解包含任意常数，但偏微分方程的解包含任意函数。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
A solution of a PDE is generally not [[Uniqueness quantification|unique]]; additional conditions must generally be specified on the [[Boundary (topology)|boundary]] of the region where the solution is defined. For instance, in the simple example above, the function {{math|''f''(''y'')}} can be determined if {{mvar|u}} is specified on the line {{math|''x'' {{=}} 0}}.&lt;br /&gt;
&lt;br /&gt;
A solution of a PDE is generally not unique; additional conditions must generally be specified on the boundary of the region where the solution is defined. For instance, in the simple example above, the function  can be determined if  is specified on the line  0}}.&lt;br /&gt;
&lt;br /&gt;
偏微分方程的解一般不是唯一的; 一般必须在定义解的区域边界上定义附加条件。 例如，在上面的简单示例中，如果在 {{math|''x'' {{=}} 0}} 时确定了 {{mvar|u}} 的值，则可以确定该函数 {{math|''f''(''y'')}}。&lt;br /&gt;
&lt;br /&gt;
== Existence and uniqueness ==&lt;br /&gt;
存在性和唯一性&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Although the issue of existence and uniqueness of solutions of ordinary differential equations has a very satisfactory answer with the [[Picard–Lindelöf theorem]], that is far from the case for partial differential equations. The [[Cauchy–Kowalevski theorem]] states that the [[Cauchy problem]] for any partial differential equation whose coefficients are [[Analytic function|analytic]] in the unknown function and its derivatives, has a locally unique analytic solution. Although this result might appear to settle the existence and uniqueness of solutions, there are examples of linear partial differential equations whose coefficients have derivatives of all orders (which are nevertheless not analytic) but which have no solutions at all: see [[Lewy's example|Lewy (1957)]]. Even if the solution of a partial differential equation exists and is unique, it may nevertheless have undesirable properties.  The mathematical study of these questions is usually in the more powerful context of [[weak solution]]s.&lt;br /&gt;
&lt;br /&gt;
Although the issue of existence and uniqueness of solutions of ordinary differential equations has a very satisfactory answer with the Picard–Lindelöf theorem, that is far from the case for partial differential equations. The Cauchy–Kowalevski theorem states that the Cauchy problem for any partial differential equation whose coefficients are analytic in the unknown function and its derivatives, has a locally unique analytic solution. Although this result might appear to settle the existence and uniqueness of solutions, there are examples of linear partial differential equations whose coefficients have derivatives of all orders (which are nevertheless not analytic) but which have no solutions at all: see Lewy (1957). Even if the solution of a partial differential equation exists and is unique, it may nevertheless have undesirable properties.  The mathematical study of these questions is usually in the more powerful context of weak solutions.&lt;br /&gt;
&lt;br /&gt;
尽管常微分方程解的存在性和唯一性用'''&amp;lt;font color=&amp;quot;#ff8000&amp;quot;&amp;gt;弗罗贝尼乌斯定理 Picard–Lindelöf Theorem&amp;lt;/font&amp;gt;得到了令人满意的结果，但偏微分方程解的存在性和唯一性却远没有得到解决。'''&amp;lt;font color=&amp;quot;#ff8000&amp;quot;&amp;gt;柯西-科瓦列夫斯基定理 Cauchy–Kowalevski theorem&amp;lt;/font&amp;gt;指出：对于任意系数在未知函数及其导数中解析的偏微分方程，柯西问题存在一个局部唯一的解析解。虽然这个结果似乎解决了解的存在性和唯一性问题，但是存在一些线性偏微分方程-其系数具有所有级数的导数(尽管这些导数不是解析的) ，但是根本没有解: 见 Lewy (1957)。即使偏微分方程的解存在且唯一，它仍然可能具有不可预料的性质。这些问题的数学研究通常是在更有力的弱解的背景下进行的。&lt;br /&gt;
&lt;br /&gt;
An example of pathological behavior is the sequence (depending upon {{mvar|n}}) of [[Cauchy problem]]s for the [[Laplace equation]]&lt;br /&gt;
&lt;br /&gt;
An example of pathological behavior is the sequence (depending upon ) of Cauchy problems for the Laplace equation&lt;br /&gt;
&lt;br /&gt;
反常特征的一个例子是拉普拉斯方程的柯西问题的序列(取决于{{mvar|n}})&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt;\frac{\partial^2 u}{\partial x^2} + \frac{\partial^2 u}{\partial y^2}=0,&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;\frac{\partial^2 u}{\partial x^2} + \frac{\partial^2 u}{\partial y^2}=0,&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
with [[boundary condition]]s&lt;br /&gt;
&lt;br /&gt;
with boundary conditions&lt;br /&gt;
&lt;br /&gt;
具有边界条件&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt;\begin{align} u(x,0) &amp;amp;= 0, \\ \frac{\partial u}{\partial y}(x,0) &amp;amp;= \frac{\sin nx}{n}, \end{align}&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;\begin{align} u(x,0) &amp;amp;= 0, \\ \frac{\partial u}{\partial y}(x,0) &amp;amp;= \frac{\sin nx}{n}, \end{align}&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
where {{mvar|n}} is an integer. The derivative of {{mvar|u}} with respect to {{mvar|y}} approaches zero [[uniform convergence|uniformly]] in {{mvar|x}} as {{mvar|n}} increases, but the solution is&lt;br /&gt;
&lt;br /&gt;
where  is an integer. The derivative of  with respect to  approaches zero uniformly in  as  increases, but the solution is&lt;br /&gt;
&lt;br /&gt;
其中 {{mvar|n}} 是整数。{{mvar|u}} 关于 {{mvar|y}} 的导数，一致地随着 {{mvar|n}} 的增加而趋于零，但解是&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt;u(x,y) = \frac{\sinh ny \sin nx}{n^2}.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;u(x,y) = \frac{\sinh ny \sin nx}{n^2}.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
This solution approaches infinity if {{mvar|nx}} is not an integer multiple of {{pi}} for any non-zero value of {{mvar|y}}. The Cauchy problem for the Laplace equation is called ''ill-posed'' or ''not [[Well-posed problem|well-posed]]'', since the solution does not continuously depend on the data of the problem. Such ill-posed problems are not usually satisfactory for physical applications.&lt;br /&gt;
&lt;br /&gt;
This solution approaches infinity if  is not an integer multiple of  for any non-zero value of . The Cauchy problem for the Laplace equation is called ill-posed or not well-posed, since the solution does not continuously depend on the data of the problem. Such ill-posed problems are not usually satisfactory for physical applications.&lt;br /&gt;
&lt;br /&gt;
对于任何非零的 {{mvar|y}}，如果 {{mvar|nx}} 不是模板 {{pi}} 的整数倍，这个解会接近于无穷大。拉普拉斯方程的柯西问题被称为不适定的（可以译为ill-posed或not well-posed），因为解不是连续地依赖于问题的数据。这种不适定问题通常不能满足物理应用。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The [[Navier–Stokes existence and smoothness|existence of solutions for the Navier–Stokes equations]], a partial differential equation, is part of one of the [[Millennium Prize Problems]].&lt;br /&gt;
&lt;br /&gt;
The existence of solutions for the Navier–Stokes equations, a partial differential equation, is part of one of the Millennium Prize Problems.&lt;br /&gt;
&lt;br /&gt;
偏微分方程”纳维-斯托克斯方程“的解的存在性就是千禧年大奖难题之一的一部分。&lt;br /&gt;
&lt;br /&gt;
== Notation ==&lt;br /&gt;
符号&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
In PDEs, it is common to denote partial derivatives using subscripts. That is:&lt;br /&gt;
&lt;br /&gt;
In PDEs, it is common to denote partial derivatives using subscripts. That is:&lt;br /&gt;
&lt;br /&gt;
在偏微分方程中，通常用下标表示偏导数。例如:&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt;u_x = \frac{\partial u}{\partial x}&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;u_x = \frac{\partial u}{\partial x}&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt;u_{xx} = \frac{\partial^2 u}{\partial x^2} &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;u_{xx} = \frac{\partial^2 u}{\partial x^2} &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt;u_{xy} = \frac{\partial^2 u}{\partial y\, \partial x} = \frac{\partial}{\partial y } \left(\frac{\partial u}{\partial x}\right). &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;u_{xy} = \frac{\partial^2 u}{\partial y\, \partial x} = \frac{\partial}{\partial y } \left(\frac{\partial u}{\partial x}\right). &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Especially in physics, [[del]] or nabla ({{math|∇}}) is often used to denote spatial derivatives, and {{math|''&amp;amp;#x307;u'', ''ü''}} for time derivatives. For example, the [[wave equation]] (mentioned below) can be written as&lt;br /&gt;
&lt;br /&gt;
Especially in physics, del or nabla () is often used to denote spatial derivatives, and  for time derivatives. For example, the wave equation (mentioned below) can be written as&lt;br /&gt;
&lt;br /&gt;
特别是在物理学中，[[del]] 或 nabla ({{math|∇}}) 经常用来表示空间导数和时间导数。例如，波动方程(在下文中提到)可以写成：&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt;\ddot u=c^2\nabla^2u&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt;\ddot u=c^2\nabla^2u&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
or&lt;br /&gt;
&lt;br /&gt;
or&lt;br /&gt;
&lt;br /&gt;
或&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt;\ddot u=c^2\Delta u&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt;\ddot u=c^2\Delta u&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
where {{math|Δ}} is the [[Laplace operator]].&lt;br /&gt;
&lt;br /&gt;
where  is the Laplace operator.&lt;br /&gt;
&lt;br /&gt;
其中，{{math|Δ}} 代表拉普拉斯算子。&lt;br /&gt;
&lt;br /&gt;
== Classification ==&lt;br /&gt;
分类&lt;br /&gt;
&lt;br /&gt;
Some linear, second-order partial differential equations can be classified as [[parabolic partial differential equation|parabolic]], [[hyperbolic partial differential equation|hyperbolic]] and [[elliptic partial differential equation|elliptic]]. Others, such as the [[Euler–Tricomi equation]], have different types in different regions. The classification provides a guide to appropriate initial and boundary conditions and to the smoothness of the solutions.&lt;br /&gt;
&lt;br /&gt;
Some linear, second-order partial differential equations can be classified as parabolic, hyperbolic and elliptic. Others, such as the Euler–Tricomi equation, have different types in different regions. The classification provides a guide to appropriate initial and boundary conditions and to the smoothness of the solutions.&lt;br /&gt;
&lt;br /&gt;
一些线性二阶偏微分方程可分为抛物型方程、双曲型方程和椭圆型方程。其他的方程，如欧拉-特里科米方程，在不同的领域有不同的类型。这种分类有助于选择适当的初始和边界条件以及提高解的平滑性。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
=== Equations of first order ===&lt;br /&gt;
一阶方程&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{{main|First-order partial differential equation}}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
=== Linear equations of second order ===&lt;br /&gt;
二阶线性方程&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Assuming {{math|''u&amp;lt;sub&amp;gt;xy&amp;lt;/sub&amp;gt;'' {{=}} ''u&amp;lt;sub&amp;gt;yx&amp;lt;/sub&amp;gt;''}}, the general linear second-order PDE in two independent variables has the form&lt;br /&gt;
&lt;br /&gt;
Assuming  u&amp;lt;sub&amp;gt;yx&amp;lt;/sub&amp;gt;}}, the general linear second-order PDE in two independent variables has the form&lt;br /&gt;
&lt;br /&gt;
假设 {{math|''u&amp;lt;sub&amp;gt;xy&amp;lt;/sub&amp;gt;'' {{=}} ''u&amp;lt;sub&amp;gt;yx&amp;lt;/sub&amp;gt;''}}，含有两个独立变量的一般线性二阶偏微分方程具有如下形式：&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt;Au_{xx} + 2Bu_{xy} + Cu_{yy} + \cdots \mbox{(lower order terms)} = 0,&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;Au_{xx} + 2Bu_{xy} + Cu_{yy} + \cdots \mbox{(lower order terms)} = 0,&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
where the coefficients {{mvar|A}}, {{mvar|B}}, {{mvar|C}}... may depend upon {{mvar|x}} and {{mvar|y}}. If {{math|''A''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; + ''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; + ''C''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; &amp;gt; 0}} over a region of the {{mvar|xy}}-plane, the PDE is second-order in that region. This form is analogous to the equation for a conic section:&lt;br /&gt;
&lt;br /&gt;
where the coefficients , , ... may depend upon  and . If  over a region of the -plane, the PDE is second-order in that region. This form is analogous to the equation for a conic section:&lt;br /&gt;
&lt;br /&gt;
其中的系数 {{mvar|A}}, {{mvar|B}}, {{mvar|C}}... 一般取决于 {{mvar|x}} 和 {{mvar|y}} 。如果在 {{mvar|xy}}-平面的一个区域上 {{math|''A''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; + ''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; + ''C''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; &amp;gt; 0}}，偏微分方程是二阶的，这种形式类似于圆锥截面的方程:&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt;Ax^2 + 2Bxy + Cy^2 + \cdots = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;Ax^2 + 2Bxy + Cy^2 + \cdots = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
More precisely, replacing {{math|∂&amp;lt;sub&amp;gt;''x''&amp;lt;/sub&amp;gt;}} by {{mvar|X}}, and likewise for other variables (formally this is done by a [[Fourier transform]]), converts a constant-coefficient PDE into a polynomial of the same degree, with the terms of the highest degree (a [[homogeneous polynomial]], here a [[quadratic form]]) being most significant for the classification.&lt;br /&gt;
&lt;br /&gt;
More precisely, replacing  by , and likewise for other variables (formally this is done by a Fourier transform), converts a constant-coefficient PDE into a polynomial of the same degree, with the terms of the highest degree (a homogeneous polynomial, here a quadratic form) being most significant for the classification.&lt;br /&gt;
&lt;br /&gt;
更准确地说，用 {{mvar|X}} 替换 {{math|∂&amp;lt;sub&amp;gt;''x''&amp;lt;/sub&amp;gt;}}，并同样替换其它变量(通常由傅里叶变换完成)，将一个常系数偏微分方程转换成一个相同次数的多项式，最高次数的项(齐次多项式，这里是一个二次形式)对于偏微分方程的分类最为重要。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Just as one classifies [[conic section]]s and quadratic forms into parabolic, hyperbolic, and elliptic based on the [[discriminant]] {{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − 4''AC''}}, the same can be done for a second-order PDE at a given point.  However, the [[discriminant]] in a PDE is given by {{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC''}} due to the convention of the {{mvar|xy}} term being {{math|2''B''}} rather than {{mvar|B}}; formally, the discriminant (of the associated quadratic form) is {{math|(2''B'')&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − 4''AC'' {{=}} 4(''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC'')}}, with the factor of 4 dropped for simplicity.&lt;br /&gt;
&lt;br /&gt;
Just as one classifies conic sections and quadratic forms into parabolic, hyperbolic, and elliptic based on the discriminant , the same can be done for a second-order PDE at a given point.  However, the discriminant in a PDE is given by  due to the convention of the  term being  rather than ; formally, the discriminant (of the associated quadratic form) is  4(B&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − AC)}}, with the factor of 4 dropped for simplicity.&lt;br /&gt;
&lt;br /&gt;
正如人们可以根据判别式 {{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − 4''AC''}} 将圆锥截面和二次型分为抛物型、双曲型和椭圆型一样，对于给定点的二阶偏微分方程也可以这样做。然而，偏微分方程中的判别式 {{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − 4''AC''}} 是根据交叉项的系数{{math|2''B''}} 而不是 {{mvar|B}} 给出的，形式上，判别式(关联二次型)是 {{math|(2''B'')&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − 4''AC'' {{=}} 4(''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC'')}}，为简单起见，去掉了因子4。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
# {{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC'' &amp;lt; 0}} (''[[elliptic partial differential equation]]''): Solutions of [[elliptic partial differential equation|elliptic PDEs]] are as smooth as the coefficients allow, within the interior of the region where the equation and solutions are defined. For example, solutions of [[Laplace's equation]] are analytic within the domain where they are defined, but solutions may assume boundary values that are not smooth. The motion of a fluid at subsonic speeds can be approximated with elliptic PDEs, and the Euler–Tricomi equation is elliptic where {{math|''x'' &amp;lt; 0}}.&lt;br /&gt;
&lt;br /&gt;
  (elliptic partial differential equation): Solutions of elliptic PDEs are as smooth as the coefficients allow, within the interior of the region where the equation and solutions are defined. For example, solutions of Laplace's equation are analytic within the domain where they are defined, but solutions may assume boundary values that are not smooth. The motion of a fluid at subsonic speeds can be approximated with elliptic PDEs, and the Euler–Tricomi equation is elliptic where .&lt;br /&gt;
&lt;br /&gt;
{{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC'' &amp;lt; 0}} (椭圆型微分方程)：在定义方程和解的区域内部，椭圆型偏微分方程的解在系数允许的程度内光滑。例如，拉普拉斯方程的解在它们被定义的区域内是解析的，但可能假设边界值是不光滑的。亚音速流体的运动可以用椭圆型偏微分方程近似，欧拉-特里科米方程在 {{math|''x'' &amp;lt; 0}} 时是椭圆型偏微分方程。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
# {{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC'' {{=}} 0}} (''[[parabolic partial differential equation]]''): Equations that are [[parabolic partial differential equation|parabolic]] at every point can be transformed into a form analogous to the [[heat equation]] by a change of independent variables. Solutions smooth out as the transformed time variable increases. The Euler–Tricomi equation has parabolic type on the line where {{math|''x'' {{=}} 0}}.&lt;br /&gt;
&lt;br /&gt;
  0}} (parabolic partial differential equation): Equations that are parabolic at every point can be transformed into a form analogous to the heat equation by a change of independent variables. Solutions smooth out as the transformed time variable increases. The Euler–Tricomi equation has parabolic type on the line where  0}}.&lt;br /&gt;
&lt;br /&gt;
{{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC'' {{=}} 0}}（抛物型偏微分方程）：在每一点上都是抛物线型的方程可以通过改变自变量从而转化成类似于热方程的形式。随着转换后的时间变量的增加，方程的解变得平滑。欧拉-特里科米方程在特征线 {{math|''x'' {{=}} 0}} 上是抛物线型的。&lt;br /&gt;
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# {{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC'' &amp;gt; 0}} (''[[hyperbolic partial differential equation]]''): [[hyperbolic partial differential equation|hyperbolic]] equations retain any discontinuities of functions or derivatives in the initial data. An example is the [[wave equation]]. The motion of a fluid at supersonic speeds can be approximated with hyperbolic PDEs, and the Euler–Tricomi equation is hyperbolic where {{math|''x'' &amp;gt; 0}}.&lt;br /&gt;
&lt;br /&gt;
  (hyperbolic partial differential equation): hyperbolic equations retain any discontinuities of functions or derivatives in the initial data. An example is the wave equation. The motion of a fluid at supersonic speeds can be approximated with hyperbolic PDEs, and the Euler–Tricomi equation is hyperbolic where .&lt;br /&gt;
&lt;br /&gt;
{{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC'' &amp;gt; 0}} (双曲型偏微分方程)：双曲型方程在初始数据中保留了函数或导数的任何不连续性。波动方程就是其中的一个例子。超音速流体的运动可以用双曲型偏微分方程近似，欧拉-特里科米方程在 {{math|''x'' &amp;gt; 0}} 时是双曲型的。&lt;br /&gt;
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If there are {{mvar|n}} independent variables {{math|''x''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;, ''x''&amp;lt;sub&amp;gt;2 &amp;lt;/sub&amp;gt;,… ''x''&amp;lt;sub&amp;gt;''n''&amp;lt;/sub&amp;gt;}}, a general linear partial differential equation of second order has the form&lt;br /&gt;
&lt;br /&gt;
If there are  independent variables , a general linear partial differential equation of second order has the form&lt;br /&gt;
&lt;br /&gt;
如果存在 {{mvar|n}} 个自变量 {{math|''x''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;, ''x''&amp;lt;sub&amp;gt;2 &amp;lt;/sub&amp;gt;,… ''x''&amp;lt;sub&amp;gt;''n''&amp;lt;/sub&amp;gt;}}，一般二阶线性偏微分方程的形式是：&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
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: &amp;lt;math&amp;gt;L u =\sum_{i=1}^n\sum_{j=1}^n a_{i,j} \frac{\partial^2 u}{\partial x_i \partial x_j} \quad \text{ plus lower-order terms} =0.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;L u =\sum_{i=1}^n\sum_{j=1}^n a_{i,j} \frac{\partial^2 u}{\partial x_i \partial x_j} \quad \text{ plus lower-order terms} =0.&amp;lt;/math&amp;gt;&lt;br /&gt;
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The classification depends upon the signature of the eigenvalues of the coefficient matrix {{math|''a''&amp;lt;sub&amp;gt;''i'',''j''&amp;lt;/sub&amp;gt;}}.&lt;br /&gt;
&lt;br /&gt;
The classification depends upon the signature of the eigenvalues of the coefficient matrix .&lt;br /&gt;
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这种分类取决于系数矩阵特征值的符号（正负性）。&lt;br /&gt;
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# Elliptic: the eigenvalues are all positive or all negative.&lt;br /&gt;
&lt;br /&gt;
 Elliptic: the eigenvalues are all positive or all negative.&lt;br /&gt;
&lt;br /&gt;
椭圆形方程: 特征值全部为正或全部为负。&lt;br /&gt;
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# Parabolic: the eigenvalues are all positive or all negative, save one that is zero.&lt;br /&gt;
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 Parabolic: the eigenvalues are all positive or all negative, save one that is zero.&lt;br /&gt;
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抛物线形方程:除了一个为零值，特征值全部为正或全部为负。&lt;br /&gt;
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# Hyperbolic: there is only one negative eigenvalue and all the rest are positive, or there is only one positive eigenvalue and all the rest are negative.&lt;br /&gt;
&lt;br /&gt;
 Hyperbolic: there is only one negative eigenvalue and all the rest are positive, or there is only one positive eigenvalue and all the rest are negative.&lt;br /&gt;
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双曲形方程: 只有一个负特征值，其余的都是正特征值，或者只有一个正特征值，其余的都是负特征值。&lt;br /&gt;
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# Ultrahyperbolic: there is more than one positive eigenvalue and more than one negative eigenvalue, and there are no zero eigenvalues. There is only a limited theory for ultrahyperbolic equations (Courant and Hilbert, 1962).&lt;br /&gt;
&lt;br /&gt;
 Ultrahyperbolic: there is more than one positive eigenvalue and more than one negative eigenvalue, and there are no zero eigenvalues. There is only a limited theory for ultrahyperbolic equations (Courant and Hilbert, 1962).&lt;br /&gt;
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超双形方程: 存在多于一个正特征值和多于一个的负特征值，且不存在零特征值。对于超双曲方程，只存在有限的理论(Courant 和 Hilbert，1962)。&lt;br /&gt;
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=== Systems of first-order equations and characteristic surfaces ===&lt;br /&gt;
一阶方程组和特征曲面&lt;br /&gt;
&lt;br /&gt;
The classification of partial differential equations can be extended to systems of first-order equations, where the unknown {{mvar|u}} is now a [[Euclidean vector|vector]] with {{mvar|m}} components, and the coefficient matrices {{mvar|A&amp;lt;sub&amp;gt;ν&amp;lt;/sub&amp;gt;}} are {{mvar|m}} by {{mvar|m}} matrices for {{math|''ν'' {{=}} 1, 2,… ''n''}}. The partial differential equation takes the form&lt;br /&gt;
&lt;br /&gt;
The classification of partial differential equations can be extended to systems of first-order equations, where the unknown  is now a vector with  components, and the coefficient matrices  are  by  matrices for  1, 2,… n}}. The partial differential equation takes the form&lt;br /&gt;
&lt;br /&gt;
偏微分方程的分类可以推广到一阶方程组，其中未知量 {{mvar|u}} 是有 {{mvar|m}} 个分量的向量。对于 {{math|''ν'' {{=}} 1, 2,… ''n''}}，系数矩阵 {{mvar|A&amp;lt;sub&amp;gt;ν&amp;lt;/sub&amp;gt;}} 是 {{mvar|m}} × {{mvar|m}} 的矩阵。偏微分方程形式如下：&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
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: &amp;lt;math&amp;gt;Lu = \sum_{\nu=1}^{n} A_\nu \frac{\partial u}{\partial x_\nu} + B=0,&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;Lu = \sum_{\nu=1}^{n} A_\nu \frac{\partial u}{\partial x_\nu} + B=0,&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
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where the coefficient matrices {{mvar|A&amp;lt;sub&amp;gt;ν&amp;lt;/sub&amp;gt;}} and the vector {{mvar|B}} may depend upon {{mvar|x}} and {{mvar|u}}. If a [[hypersurface]] {{mvar|S}} is given in the implicit form&lt;br /&gt;
&lt;br /&gt;
where the coefficient matrices  and the vector  may depend upon  and . If a hypersurface  is given in the implicit form&lt;br /&gt;
&lt;br /&gt;
其中，系数矩阵 {{mvar|A&amp;lt;sub&amp;gt;ν&amp;lt;/sub&amp;gt;}} 和向量 {{mvar|B}} 可能依赖于 {{mvar|x}} 和 {{mvar|u}}。如果超曲面是以以下隐式形式给出的，&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt;\varphi(x_1, x_2, \ldots x_n)=0,&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;\varphi(x_1, x_2, \ldots x_n)=0,&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
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where {{mvar|φ}} has a non-zero gradient, then {{mvar|S}} is a '''characteristic surface''' for the operator {{mvar|L}} at a given point if the characteristic form vanishes:&lt;br /&gt;
&lt;br /&gt;
where  has a non-zero gradient, then  is a characteristic surface for the operator  at a given point if the characteristic form vanishes:&lt;br /&gt;
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其中，存在一个非零的梯度 {{mvar|φ}}，对于在给定点上特征形式消失的算子，特征曲面 {{mvar|S}} 形式如下:&lt;br /&gt;
&lt;br /&gt;
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: &amp;lt;math&amp;gt;Q\left(\frac{\partial\varphi}{\partial x_1}, \ldots\frac{\partial\varphi}{\partial x_n}\right) =\det\left[\sum_{\nu=1}^nA_\nu \frac{\partial \varphi}{\partial x_\nu}\right]=0.\,&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;Q\left(\frac{\partial\varphi}{\partial x_1}, \ldots\frac{\partial\varphi}{\partial x_n}\right) =\det\left[\sum_{\nu=1}^nA_\nu \frac{\partial \varphi}{\partial x_\nu}\right]=0.\,&amp;lt;/math&amp;gt;&lt;br /&gt;
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The geometric interpretation of this condition is as follows: if data for {{mvar|u}} are prescribed on the surface {{mvar|S}}, then it may be possible to determine the normal derivative of {{mvar|u}} on {{mvar|S}} from the differential equation. If the data on {{mvar|S}} and the differential equation determine the normal derivative of {{mvar|u}} on {{mvar|S}}, then {{mvar|S}} is non-characteristic. If the data on {{mvar|S}} and the differential equation ''do not'' determine the normal derivative of {{mvar|u}} on {{mvar|S}}, then the surface is '''characteristic''', and the differential equation restricts the data on {{mvar|S}}: the differential equation is ''internal'' to {{mvar|S}}.&lt;br /&gt;
&lt;br /&gt;
The geometric interpretation of this condition is as follows: if data for  are prescribed on the surface , then it may be possible to determine the normal derivative of  on  from the differential equation. If the data on  and the differential equation determine the normal derivative of  on , then  is non-characteristic. If the data on  and the differential equation do not determine the normal derivative of  on , then the surface is characteristic, and the differential equation restricts the data on : the differential equation is internal to .&lt;br /&gt;
&lt;br /&gt;
这个条件的几何解释如下: 如果关于 {{mvar|u}} 的数据是在曲面 {{mvar|S}} 上规定的，那么就有可能依据微分方程确定曲面 {{mvar|S}} 上 {{mvar|u}} 的法向导数。如果曲面 {{mvar|S}} 上的数据和上面的微分方程能确定曲面 {{mvar|S}} 上 {{mvar|u}} 的法向导数，那么它就是非特征的。如果曲面 {{mvar|S}} 上的数据和上面的微分方程不能确定曲面 {{mvar|S}} 上 {{mvar|u}} 的法向导数，那么曲面是特征的，并且微分方程将数据限制在曲面 {{mvar|S}} 上：微分方程是在曲面 {{mvar|S}} 内部。&lt;br /&gt;
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# A first-order system {{math|''Lu'' {{=}} 0}} is ''elliptic'' if no surface is characteristic for {{mvar|L}}: the values of {{mvar|u}} on {{mvar|S}} and the differential equation always determine the normal derivative of {{mvar|u}} on {{mvar|S}}.&lt;br /&gt;
&lt;br /&gt;
 A first-order system  0}} is elliptic if no surface is characteristic for : the values of  on  and the differential equation always determine the normal derivative of  on .&lt;br /&gt;
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如果对于 {{mvar|L}} 没有曲面是特征的，则一阶系统 {{math|''Lu'' {{=}} 0}} 是椭圆形的：{{mvar|u}}在 {{mvar|S}} 的值和微分方程总能够决定 {{mvar|S}} 上 {{mvar|u}} 的法向导数。&lt;br /&gt;
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# A first-order system is ''hyperbolic'' at a point if there is a '''spacelike''' surface {{mvar|S}} with normal {{mvar|ξ}} at that point. This means that, given any non-trivial vector {{mvar|η}} orthogonal to {{mvar|ξ}}, and a scalar multiplier {{mvar|λ}}, the equation {{math|''Q''(''λξ'' + ''η'') {{=}} 0}} has {{mvar|m}} real roots {{math|''λ''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;, ''λ''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;,… ''λ''&amp;lt;sub&amp;gt;''m''&amp;lt;/sub&amp;gt;}}. The system is '''strictly hyperbolic''' if these roots are always distinct. The geometrical interpretation of this condition is as follows: the characteristic form {{math|''Q''(''ζ'') {{=}} 0}} defines a cone (the normal cone) with homogeneous coordinates ζ. In the hyperbolic case, this cone has {{mvar|m}} sheets, and the axis {{math|''ζ'' {{=}} ''λξ''}} runs inside these sheets: it does not intersect any of them. But when displaced from the origin by η, this axis intersects every sheet. In the elliptic case, the normal cone has no real sheets.&lt;br /&gt;
&lt;br /&gt;
 A first-order system is hyperbolic at a point if there is a spacelike surface  with normal  at that point. This means that, given any non-trivial vector  orthogonal to , and a scalar multiplier , the equation  0}} has  real roots . The system is strictly hyperbolic if these roots are always distinct. The geometrical interpretation of this condition is as follows: the characteristic form  0}} defines a cone (the normal cone) with homogeneous coordinates ζ. In the hyperbolic case, this cone has  sheets, and the axis  λξ}} runs inside these sheets: it does not intersect any of them. But when displaced from the origin by η, this axis intersects every sheet. In the elliptic case, the normal cone has no real sheets.&lt;br /&gt;
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如果在该点存在一个法向量为 {{mvar|ξ}}的 '''&amp;lt;font color=&amp;quot;#ff8000&amp;quot;&amp;gt;类空曲面 Spacclike Surface&amp;lt;/font&amp;gt; {{mvar|S}} ，则一阶系统在那一点是双曲的。这意味着，给定任意正交于 {{mvar|ξ}} 的非平凡向量 {{mvar|η}} 和一个标量乘子 {{mvar|λ}}，方程 {{math|''Q''(''λξ'' + ''η'') {{=}} 0}} 有 {{mvar|m}} 个实根 {{math|''λ''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;, ''λ''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;,… ''λ''&amp;lt;sub&amp;gt;''m''&amp;lt;/sub&amp;gt;}}。如果这些根始终不同，则该系统是严格双曲形的。这个条件的几何解释如下: 特征形式 {{math|''Q''(''ζ'') {{=}} 0}} 定义了一个具有齐次坐标 ζ的圆锥(法线圆锥)。在双曲形的情况下，这个圆锥体有 {{mvar|m}} 层，并且轴 {{math|''ζ'' {{=}} ''λξ''}} 在这些层中运动: 它不与任何一层相交。但是当从原点偏离η时，这条轴线与每一层都相交。在椭圆形的情况下，法向圆锥没有实层。&lt;br /&gt;
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==[[用户:Yuling|Yuling]]（[[用户讨论:Yuling|讨论]]） sheet 这个单词也不很理解，我直译为了“层”&lt;br /&gt;
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=== Equations of mixed type ===&lt;br /&gt;
混合型方程&lt;br /&gt;
&lt;br /&gt;
If a PDE has coefficients that are not constant, it is possible that it will not belong to any of these categories but rather be of '''mixed type'''. A simple but important example is the [[Euler–Tricomi equation]]&lt;br /&gt;
&lt;br /&gt;
If a PDE has coefficients that are not constant, it is possible that it will not belong to any of these categories but rather be of mixed type. A simple but important example is the Euler–Tricomi equation&lt;br /&gt;
&lt;br /&gt;
如果偏微分方程的系数不是常数，那么它可能不属于这些类别中的任何一个，而是属于混合类型。一个简单但重要的例子是欧拉-特里科米方程&lt;br /&gt;
&lt;br /&gt;
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: &amp;lt;math&amp;gt;u_{xx} = xu_{yy},&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;u_{xx} = xu_{yy},&amp;lt;/math&amp;gt;&lt;br /&gt;
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which is called '''elliptic-hyperbolic''' because it is elliptic in the region {{math|''x'' &amp;lt; 0}}, hyperbolic in the region {{math|''x'' &amp;gt; 0}}, and degenerate parabolic on the line {{math|''x'' {{=}} 0}}.&lt;br /&gt;
&lt;br /&gt;
which is called elliptic-hyperbolic because it is elliptic in the region , hyperbolic in the region , and degenerate parabolic on the line  0}}.&lt;br /&gt;
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它在 {{math|''x'' &amp;lt; 0}} 的区域上是椭圆形，在 {{math|''x'' &amp;gt; 0}} 区域上是双曲形，在 {{math|''x'' {{=}} 0}}这条线上是退化为抛物线形，因此称之为椭圆-双曲型。&lt;br /&gt;
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&amp;lt;!--&lt;br /&gt;
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&amp;lt;!--&lt;br /&gt;
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&amp;lt;!--&lt;br /&gt;
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''fill in: Dirichlet and Neumann boundaries, hyperbolic/parabolic/elliptic separation of variables, [[Fourier analysis]], [[Green's function]]s ...--&amp;gt;&lt;br /&gt;
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fill in: Dirichlet and Neumann boundaries, hyperbolic/parabolic/elliptic separation of variables, Fourier analysis, Green's functions ...--&amp;gt;&lt;br /&gt;
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填写: Dirichlet 和 Neumann 边界，双曲 / 抛物线 / 椭圆分离变量法，傅立叶分析，Green 函数... --&lt;br /&gt;
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=== Infinite-order PDEs in quantum mechanics ===&lt;br /&gt;
量子力学中的无限阶偏微分方程&lt;br /&gt;
&lt;br /&gt;
In the [[phase space formulation]] of quantum mechanics,  one may consider the [[Method of quantum characteristics|quantum Hamilton's equations]] for trajectories of quantum particles. These equations are infinite-order PDEs. However, in the semiclassical expansion, one has a finite system of ODEs at any fixed order of [[Dirac constant|{{mvar|ħ}}]].  The evolution equation of the [[Wigner quasi-probability distribution|c]] is also an infinite-order PDE. The quantum trajectories are [[Method of quantum characteristics|quantum characteristics]], with the use of which one could calculate the evolution of the Wigner function.&lt;br /&gt;
&lt;br /&gt;
In the phase space formulation of quantum mechanics,  one may consider the quantum Hamilton's equations for trajectories of quantum particles. These equations are infinite-order PDEs. However, in the semiclassical expansion, one has a finite system of ODEs at any fixed order of Dirac constant|.  The evolution equation of the Wigner function is also an infinite-order PDE. The quantum trajectories are quantum characteristics, with the use of which one could calculate the evolution of the Wigner function.&lt;br /&gt;
&lt;br /&gt;
在量子力学中的相空间表述中，我们可以考虑用于求解量子粒子的轨迹的量子哈密顿的方程。这些方程是无限阶偏微分方程。然而，在半经典展开中，我们在给定[[Dirac constant|{{mvar|ħ}}]]阶数下有一个有限的的常微分方程组。'''&amp;lt;font color=&amp;quot;#ff8000&amp;quot;&amp;gt;维格纳函数  Wigner Function&amp;lt;/font&amp;gt;的演化方程也是一个无限阶偏微分方程。由于量子轨道的量子特性，所以它通常可以用来计算维格纳函数的演化。&lt;br /&gt;
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== Analytical solutions ==&lt;br /&gt;
解析解&lt;br /&gt;
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===Separation of variables===&lt;br /&gt;
分离变量法&lt;br /&gt;
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{{main|Separable partial differential equation}}&lt;br /&gt;
&lt;br /&gt;
Linear PDEs can be reduced to systems of ordinary differential equations by the important technique of separation of variables. This technique rests on a characteristic of solutions to differential equations: if one can find any solution that solves the equation and satisfies the boundary conditions, then it is ''the'' solution (this also applies to ODEs). We assume as an [[ansatz]] that the dependence of a solution on the parameters space and time can be written as a product of terms that each depend on a single parameter, and then see if this can be made to solve the problem.&amp;lt;ref&amp;gt;{{cite book|last1=Gershenfeld|first1=Neil|title=The nature of mathematical modeling|date=2000|publisher=Cambridge Univ. Press|location=Cambridge|isbn=0521570956|page=27|edition=Reprinted (with corr.)}}&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
Linear PDEs can be reduced to systems of ordinary differential equations by the important technique of separation of variables. This technique rests on a characteristic of solutions to differential equations: if one can find any solution that solves the equation and satisfies the boundary conditions, then it is the solution (this also applies to ODEs). We assume as an ansatz that the dependence of a solution on the parameters space and time can be written as a product of terms that each depend on a single parameter, and then see if this can be made to solve the problem.&lt;br /&gt;
&lt;br /&gt;
线性偏微分方程组可以通过分离变量法这一重要方法来简化为常微分方程组。这种方法依赖于微分方程解的一个特征: 如果能找到任何一个满足方程和边界条件的解，那么这个解就是方程的解(这也适用于常微分方程)。我们假设解对参数空间和时间的依赖可以写成对它们每一项的依赖以及一个参数的乘积，然后再看看这是否可以用来解决这个问题。&lt;br /&gt;
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In the method of separation of variables, one reduces a PDE to a PDE in fewer variables, which is an ordinary differential equation if in one variable – these are in turn easier to solve.&lt;br /&gt;
&lt;br /&gt;
In the method of separation of variables, one reduces a PDE to a PDE in fewer variables, which is an ordinary differential equation if in one variable – these are in turn easier to solve.&lt;br /&gt;
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在分离变量法方法中，可以将偏微分方程简化为含有更少变量的偏微分方程，如果只有一个变量，那么就变成了一个'''&amp;lt;font color = &amp;quot;#ff8000&amp;quot;&amp;gt;常微分方程 Ordinary Differential Equation&amp;lt;/font&amp;gt;'''-- 反过来，这些方程也更容易求解。&lt;br /&gt;
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This is possible for simple PDEs, which are called [[separable partial differential equation]]s, and the domain is generally a rectangle (a product of intervals). Separable PDEs correspond to [[diagonal matrices]] – thinking of &amp;quot;the value for fixed {{mvar|x}}&amp;quot; as a coordinate, each coordinate can be understood separately.&lt;br /&gt;
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This is possible for simple PDEs, which are called separable partial differential equations, and the domain is generally a rectangle (a product of intervals). Separable PDEs correspond to diagonal matrices – thinking of &amp;quot;the value for fixed &amp;quot; as a coordinate, each coordinate can be understood separately.&lt;br /&gt;
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对于简单的偏微分方程(称为可分离偏微分方程)来说，这是可能的，而且方程通常定义在一个矩形区域(区间的乘积)上。可分离偏微分方程对应于对角线矩阵——以“固定值”为坐标，每个坐标可分开理解。&lt;br /&gt;
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This generalizes to the [[method of characteristics]], and is also used in [[integral transform]]s.&lt;br /&gt;
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This generalizes to the method of characteristics, and is also used in integral transforms.&lt;br /&gt;
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这种方法可以推广到特征曲线法，也可以用于积分变换。&lt;br /&gt;
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===Method of characteristics===&lt;br /&gt;
特征曲线法&lt;br /&gt;
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{{main|Method of characteristics}}&lt;br /&gt;
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In special cases, one can find characteristic curves on which the equation reduces to an ODE – changing coordinates in the domain to straighten these curves allows separation of variables, and is called the [[method of characteristics]].&lt;br /&gt;
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In special cases, one can find characteristic curves on which the equation reduces to an ODE – changing coordinates in the domain to straighten these curves allows separation of variables, and is called the method of characteristics.&lt;br /&gt;
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在特殊情况下，可以找到一些特征曲线，在这些曲线上方程可以变成一个常微分方程——意味着改变坐标从而使这些曲线变直从而达到分离变量的目的，这就是所谓的特征曲线法。&lt;br /&gt;
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More generally, one may find characteristic surfaces.&lt;br /&gt;
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More generally, one may find characteristic surfaces.&lt;br /&gt;
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更一般地说，人们可能会找到特征表面。&lt;br /&gt;
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===Integral transform===&lt;br /&gt;
积分变换&lt;br /&gt;
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An [[integral transform]] may transform the PDE to a simpler one, in particular, a separable PDE. This corresponds to diagonalizing an operator.&lt;br /&gt;
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An integral transform may transform the PDE to a simpler one, in particular, a separable PDE. This corresponds to diagonalizing an operator.&lt;br /&gt;
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积分变换可以将偏微分方程转换为更简单的偏微分方程，特别是可分离的偏微分方程。这对应于对角化算符。&lt;br /&gt;
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An important example of this is [[Fourier analysis]], which diagonalizes the heat equation using the [[eigenbasis]] of sinusoidal waves.&lt;br /&gt;
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An important example of this is Fourier analysis, which diagonalizes the heat equation using the eigenbasis of sinusoidal waves.&lt;br /&gt;
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这方面的一个重要例子是'''&amp;lt;font color = &amp;quot;#ff8000&amp;quot;&amp;gt;傅里叶分析  Fourier Analysis&amp;lt;/font&amp;gt;'''，它使用正弦波的特征基来对角化热方程。&lt;br /&gt;
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If the domain is finite or periodic, an infinite sum of solutions such as a [[Fourier series]] is appropriate, but an integral of solutions such as a [[Fourier integral]] is generally required for infinite domains. The solution for a point source for the heat equation given above is an example of the use of a Fourier integral.&lt;br /&gt;
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If the domain is finite or periodic, an infinite sum of solutions such as a Fourier series is appropriate, but an integral of solutions such as a Fourier integral is generally required for infinite domains. The solution for a point source for the heat equation given above is an example of the use of a Fourier integral.&lt;br /&gt;
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如果区域是有限的或周期性的，那么解为无限和的形式是恰当的，例如傅里叶级数，但是一个解的积分，例如傅立叶积分，一般是在无限区域上的。上面给出的热传导方程的点源解法就是使用傅里叶积分的一个例子。&lt;br /&gt;
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===Change of variables===&lt;br /&gt;
变量代换&lt;br /&gt;
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Often a PDE can be reduced to a simpler form with a known solution by a suitable [[Change of variables (PDE)|change of variables]].  For example, the [[Black–Scholes equation#Derivation|Black–Scholes]] PDE&lt;br /&gt;
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Often a PDE can be reduced to a simpler form with a known solution by a suitable change of variables.  For example, the Black–Scholes PDE&lt;br /&gt;
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偏微分方程通常可以通过变量的适当变化，用已知的解简化为更简单的形式。例如，布莱克-舒尔斯偏微分方程&lt;br /&gt;
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:&amp;lt;math&amp;gt; \frac{\partial V}{\partial t} + \tfrac{1}{2}\sigma^2 S^2\frac{\partial^2 V}{\partial S^2} + rS\frac{\partial V}{\partial S} - rV = 0 &amp;lt;/math&amp;gt;&lt;br /&gt;
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&amp;lt;math&amp;gt; \frac{\partial V}{\partial t} + \tfrac{1}{2}\sigma^2 S^2\frac{\partial^2 V}{\partial S^2} + rS\frac{\partial V}{\partial S} - rV = 0 &amp;lt;/math&amp;gt;&lt;br /&gt;
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is reducible to the [[heat equation]]&lt;br /&gt;
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is reducible to the heat equation&lt;br /&gt;
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可以简化为热传导方程&lt;br /&gt;
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:&amp;lt;math&amp;gt; \frac{\partial u}{\partial \tau} = \frac{\partial^2 u}{\partial x^2}&amp;lt;/math&amp;gt;&lt;br /&gt;
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&amp;lt;math&amp;gt; \frac{\partial u}{\partial \tau} = \frac{\partial^2 u}{\partial x^2}&amp;lt;/math&amp;gt;&lt;br /&gt;
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by the change of variables (for complete details see {{webarchive |url=https://web.archive.org/web/20080411030405/http://www.math.unl.edu/~sdunbar1/Teaching/MathematicalFinance/Lessons/BlackScholes/Solution/solution.shtml |date=April 11, 2008 |title=Solution of the Black Scholes Equation }})&lt;br /&gt;
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by the change of variables (for complete details see )&lt;br /&gt;
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通过变量替换(完整的细节见)&lt;br /&gt;
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:&amp;lt;math&amp;gt;\begin{align}&lt;br /&gt;
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V(S,t) &amp;amp;= K v(x,\tau),\\[5px]&lt;br /&gt;
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x &amp;amp;= \ln\left(\tfrac{S}{K} \right),\\[5px]&lt;br /&gt;
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\tau &amp;amp;= \tfrac{1}{2} \sigma^2 (T - t),\\[5px]&lt;br /&gt;
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v(x,\tau)&amp;amp;=e^{-\alpha x-\beta\tau} u(x,\tau).&lt;br /&gt;
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\end{align}&amp;lt;/math&amp;gt;&lt;br /&gt;
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===Fundamental solution===&lt;br /&gt;
基本解&lt;br /&gt;
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{{main|Fundamental solution}}&lt;br /&gt;
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Inhomogeneous equations can often be solved (for constant coefficient PDEs, always be solved) by finding the [[fundamental solution]] (the solution for a point source), then taking the [[convolution]] with the boundary conditions to get the solution.&lt;br /&gt;
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Inhomogeneous equations can often be solved (for constant coefficient PDEs, always be solved) by finding the fundamental solution (the solution for a point source), then taking the convolution with the boundary conditions to get the solution.&lt;br /&gt;
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非齐次方程(常系数偏微分方程)一般是通过先求出基本解(点源的解) ，然后利用带边界条件的卷积来求解。&lt;br /&gt;
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This is analogous in [[signal processing]] to understanding a filter by its [[impulse response]].&lt;br /&gt;
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This is analogous in signal processing to understanding a filter by its impulse response.&lt;br /&gt;
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这类似于在信号处理中通过滤波器的脉冲响应来理解滤波器。&lt;br /&gt;
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===Superposition principle===&lt;br /&gt;
叠加原理&lt;br /&gt;
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{{further| Superposition principle }}&lt;br /&gt;
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The superposition principle applies to any linear system, including linear systems of PDEs. A common visualization of this concept is the interaction of two waves in phase being combined to result in a greater amplitude, for example {{math|sin ''x'' + sin ''x'' {{=}} 2 sin ''x''}}. The same principle can be observed in PDEs where the solutions may be real or complex and additive. [[Superposition principle|superposition]]&lt;br /&gt;
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The superposition principle applies to any linear system, including linear systems of PDEs. A common visualization of this concept is the interaction of two waves in phase being combined to result in a greater amplitude, for example  2 sin x}}. The same principle can be observed in PDEs where the solutions may be real or complex and additive. superposition&lt;br /&gt;
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'''&amp;lt;font color = &amp;quot;#ff8000&amp;quot;&amp;gt;叠加原理 Superposition Principle&amp;lt;/font&amp;gt;适用于任何线性系统，包括偏微分方程的线性系统。这个概念的一个常见的可视化是两个同相位的波相互作用结合在一起会产生更大的振幅，例如 {{math|sin ''x'' + sin ''x'' {{=}} 2 sin ''x''}}。在偏微分方程中也可以观察到同样的原理，其中的解可能是真实的或复杂的和可加的。叠加&lt;br /&gt;
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If {{math|''u''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;}} and {{math|''u''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;}} are solutions of linear PDE in some function space {{mvar|R}}, then {{math|''u'' {{=}} ''c''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;''u''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; + ''c''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;''u''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;}} with any constants {{math|''c''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;}} and {{math|''c''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;}} are also a solution of that PDE in the same function space.&lt;br /&gt;
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If  and  are solutions of linear PDE in some function space , then  c&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;u&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; + c&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;u&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;}} with any constants  and  are also a solution of that PDE in the same function space.&lt;br /&gt;
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若线性偏微分方程在某个函数空间{{mvar|R}}中有解{{math|''u''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;}} 和 {{math|''u''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;}}，则{{math|''u'' {{=}} ''c''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;''u''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; + ''c''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;''u''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;}}也是该偏微分方程在同一函数空间中的解，其中{{math|''c''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;}} 和 {{math|''c''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;}} 是任意常数。&lt;br /&gt;
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===Methods for non-linear equations===&lt;br /&gt;
非线性方程的求解方法&lt;br /&gt;
{{see also|nonlinear partial differential equation}}&lt;br /&gt;
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There are no generally applicable methods to solve nonlinear PDEs. Still, existence and uniqueness results (such as the [[Cauchy–Kowalevski theorem]]) are often possible, as are proofs of important qualitative and quantitative properties of solutions (getting these results is a major part of [[mathematical analysis|analysis]]). Computational solution to the nonlinear PDEs, the [[split-step method]], exist for specific equations like [[nonlinear Schrödinger equation]].&lt;br /&gt;
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There are no generally applicable methods to solve nonlinear PDEs. Still, existence and uniqueness results (such as the Cauchy–Kowalevski theorem) are often possible, as are proofs of important qualitative and quantitative properties of solutions (getting these results is a major part of analysis). Computational solution to the nonlinear PDEs, the split-step method, exist for specific equations like nonlinear Schrödinger equation.&lt;br /&gt;
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对于非线性偏微分方程，目前还没有普遍适用的求解方法。然而，通常是可能知道解的存在性和唯一性(如柯西-科瓦列夫斯基定理)，也是可能得到解的重要定性和定量性质的证明(得到这些结果是分析的主要部分)。非线性偏微分方程的计算解，即分步法，对一些特定的方程适用，比如非线性'''&amp;lt;font color=&amp;quot;#ff8000&amp;quot;&amp;gt;薛定谔方程 Schrödinger equation&amp;lt;/font&amp;gt;'''。&lt;br /&gt;
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Nevertheless, some techniques can be used for several types of equations. The [[h-principle|{{mvar|h}}-principle]] is the most powerful method to solve [[Underdetermined system|underdetermined]] equations. The [[Riquier–Janet theory]] is an effective method for obtaining information about many analytic [[Overdetermined system|overdetermined]] systems.&lt;br /&gt;
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Nevertheless, some techniques can be used for several types of equations. The -principle is the most powerful method to solve underdetermined equations. The Riquier–Janet theory is an effective method for obtaining information about many analytic overdetermined systems.&lt;br /&gt;
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然而，一些技巧可以用于几种类型的方程。h-原理是求解欠定方程最有效的方法。里基尔-珍妮特理论是一种可以获得许多解析超定系统信息的有效方法。&lt;br /&gt;
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The [[method of characteristics]] can be used in some very special cases to solve partial differential equations.&lt;br /&gt;
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The method of characteristics can be used in some very special cases to solve partial differential equations.&lt;br /&gt;
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特征线法可用于求解某些特殊情况下的偏微分方程。&lt;br /&gt;
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In some cases, a PDE can be solved via [[perturbation analysis]] in which the solution is considered to be a correction to an equation with a known solution. Alternatives are [[numerical analysis]] techniques from simple [[finite difference]] schemes to the more mature [[multigrid]] and [[finite element method]]s. Many interesting problems in science and engineering are solved in this way using [[computer]]s, sometimes high performance [[supercomputer]]s.&lt;br /&gt;
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In some cases, a PDE can be solved via perturbation analysis in which the solution is considered to be a correction to an equation with a known solution. Alternatives are numerical analysis techniques from simple finite difference schemes to the more mature multigrid and finite element methods. Many interesting problems in science and engineering are solved in this way using computers, sometimes high performance supercomputers.&lt;br /&gt;
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在某些情况下，偏微分方程可以通过扰动分析来求解。在扰动分析中，通常是求解将具有已知解的方程修正后的新得到方程。可供选择的数值分析技术从简单的差分格式到更成熟的多重网格和有限元方法。许多有趣的科学和工程问题都是在计算机上用这种方法解决的，有时是高性能超级计算机。&lt;br /&gt;
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===Lie group method===&lt;br /&gt;
李群方法&lt;br /&gt;
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From 1870 [[Sophus Lie]]'s work put the theory of differential equations on a more satisfactory foundation. He showed that the integration theories of the older mathematicians can, by the introduction of what are now called [[Lie group]]s, be referred, to a common source; and that ordinary differential equations which admit the same [[infinitesimal transformation]]s present comparable difficulties of integration. He also emphasized the subject of [[contact transformation|transformations of contact]].&lt;br /&gt;
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From 1870 Sophus Lie's work put the theory of differential equations on a more satisfactory foundation. He showed that the integration theories of the older mathematicians can, by the introduction of what are now called Lie groups, be referred, to a common source; and that ordinary differential equations which admit the same infinitesimal transformations present comparable difficulties of integration. He also emphasized the subject of transformations of contact.&lt;br /&gt;
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从1870年起，索弗斯·李的工作为微分方程理论奠定了一个较为令人满意的基础。他指出，通过引入现在所谓的李群，老一辈数学家的积分理论可以引用到一个共同的来源; 承认相同的无穷小变换的常微分方程在积分方面存在相当的困难。他还强调了接触的转变这一主题。&lt;br /&gt;
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==[[用户:Yuling|Yuling]]（[[用户讨论:Yuling|讨论]]）这句话“He also emphasized the subject of transformations of contact.”中的transformations of contact翻译的不太好。&lt;br /&gt;
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A general approach to solving PDEs uses the symmetry property of differential equations, the continuous [[infinitesimal transformation]]s of solutions to solutions ([[Lie theory]]). Continuous [[group theory]], [[Lie algebras]] and [[differential geometry]] are used to understand the structure of linear and nonlinear partial differential equations for generating integrable equations, to find its [[Lax pair]]s, recursion operators, [[Bäcklund transform]] and finally finding exact analytic solutions to the PDE.&lt;br /&gt;
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A general approach to solving PDEs uses the symmetry property of differential equations, the continuous infinitesimal transformations of solutions to solutions (Lie theory). Continuous group theory, Lie algebras and differential geometry are used to understand the structure of linear and nonlinear partial differential equations for generating integrable equations, to find its Lax pairs, recursion operators, Bäcklund transform and finally finding exact analytic solutions to the PDE.&lt;br /&gt;
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求解偏微分方程的一般方法是利用微分方程的对称性，即解到解的连续无穷小变换(李理论)。连续群论、李代数和微分几何理论被用来理解生成可积方程的线性和非线性偏微分方程的结构，找到它的Lax对、递归算子、 贝克伦德变换，最后找到偏微分方程的精确解析解。&lt;br /&gt;
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Symmetry methods have been recognized to study differential equations arising in mathematics, physics, engineering, and many other disciplines.&lt;br /&gt;
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Symmetry methods have been recognized to study differential equations arising in mathematics, physics, engineering, and many other disciplines.&lt;br /&gt;
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对称方法已被公认可以用于研究出现在数学，物理，工程和许多其他学科的微分方程。&lt;br /&gt;
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===Semianalytical methods===&lt;br /&gt;
半解析方法&lt;br /&gt;
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The [[Adomian decomposition method]], the [[Aleksandr Lyapunov|Lyapunov]] artificial small parameter method, and He's [[homotopy perturbation method]] are all special cases of the more general [[homotopy analysis method]]. These are series expansion methods, and except for the Lyapunov method, are independent of small physical parameters as compared to the well known [[perturbation theory]], thus giving these methods greater flexibility and solution generality.&lt;br /&gt;
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The Adomian decomposition method, the Lyapunov artificial small parameter method, and He's homotopy perturbation method are all special cases of the more general homotopy analysis method. These are series expansion methods, and except for the Lyapunov method, are independent of small physical parameters as compared to the well known perturbation theory, thus giving these methods greater flexibility and solution generality.&lt;br /&gt;
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阿多米安分解法、李雅普诺夫人工小参数方法和何同伦摄动方法都是更一般的同伦分析方法的特殊情况。除了李雅普诺夫方法之外，这些都是级数展开方法，与为人熟知的摄动理论方法相比，它们与小的物理参数无关，因此这些方法具有更大的灵活性和解的通用性。&lt;br /&gt;
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== Numerical solutions ==&lt;br /&gt;
数值解&lt;br /&gt;
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The three most widely used [[Numerical partial differential equations|numerical methods to solve PDEs]] are the [[finite element analysis|finite element method]] (FEM), [[finite volume method]]s (FVM) and [[finite difference method]]s (FDM), as well other kind of methods called [[Meshfree methods]], which were made to solve problems where the before mentioned methods are limited. The FEM has a prominent position among these methods and especially its exceptionally efficient higher-order version [[hp-FEM]]. Other hybrid versions of FEM and Meshfree methods include the generalized finite element method (GFEM), [[extended finite element method]] (XFEM), [[Spectral element method|spectral finite element method]] (SFEM), [[Meshfree methods|meshfree finite element method]], [[Discontinuous Galerkin Method|discontinuous Galerkin finite element method]] (DGFEM), [[Element-Free Galerkin Method]] (EFGM), [[Interpolating Element-Free Galerkin Method]] (IEFGM), etc.&lt;br /&gt;
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The three most widely used numerical methods to solve PDEs are the finite element method (FEM), finite volume methods (FVM) and finite difference methods (FDM), as well other kind of methods called Meshfree methods, which were made to solve problems where the before mentioned methods are limited. The FEM has a prominent position among these methods and especially its exceptionally efficient higher-order version hp-FEM. Other hybrid versions of FEM and Meshfree methods include the generalized finite element method (GFEM), extended finite element method (XFEM), spectral finite element method (SFEM), meshfree finite element method, discontinuous Galerkin finite element method (DGFEM), Element-Free Galerkin Method (EFGM), Interpolating Element-Free Galerkin Method (IEFGM), etc.&lt;br /&gt;
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求解偏微分方程最常用的三种数值方法是有限元分析法、有限体积法和有限差分法，以及其他一些称为无网格法的方法。这些方法用于解决前面提到的方法受到的限制。在这些方法中，有限元方法，尤其是高效的高阶有限元方法，占有重要地位。其他有限元法和无网格法的混合形式包括广义有限元分析法(GFEM)、扩展有限元分析法(XFEM)、谱有限元分析法(SFEM)、无网格有限元分析法(DGFEM)、间断伽辽金有限元分析法(DGFEM)、无网格伽辽金法(EFGM)、插值无网格伽辽金法(IEFGM)等。&lt;br /&gt;
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=== Finite element method ===&lt;br /&gt;
有限元分析法&lt;br /&gt;
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{{main|Finite element method}}&lt;br /&gt;
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The finite element method (FEM) (its practical application often known as finite element analysis (FEA)) is a numerical technique for finding approximate solutions of partial differential equations (PDE) as well as of integral equations. The solution approach is based either on eliminating the differential equation completely (steady state problems), or rendering the PDE into an approximating system of ordinary differential equations, which are then numerically integrated using standard techniques such as Euler's method, Runge–Kutta, etc.&lt;br /&gt;
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The finite element method (FEM) (its practical application often known as finite element analysis (FEA)) is a numerical technique for finding approximate solutions of partial differential equations (PDE) as well as of integral equations. The solution approach is based either on eliminating the differential equation completely (steady state problems), or rendering the PDE into an approximating system of ordinary differential equations, which are then numerically integrated using standard techniques such as Euler's method, Runge–Kutta, etc.&lt;br /&gt;
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'''&amp;lt;font color = &amp;quot;#ff8000&amp;quot;&amp;gt;有限元分析法 Finite Element Method&amp;lt;/font&amp;gt;''' ((其实际应用通常被称为有限元分析(FEA))是一种寻找偏微分方程(PDE)和积分方程近似解的数值技术。这种求解方法要么基于完全消除微分方程(稳态问题) ，要么将偏微分方程转化为常微分方程的近似系统，然后使用标准技术进行数值积分，如欧拉方法、 Runge-Kutta 等。&lt;br /&gt;
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===Finite difference method===&lt;br /&gt;
有限差分法&lt;br /&gt;
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{{main|Finite difference method}}&lt;br /&gt;
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Finite-difference methods are numerical methods for approximating the solutions to differential equations using [[finite difference]] equations to approximate derivatives.&lt;br /&gt;
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Finite-difference methods are numerical methods for approximating the solutions to differential equations using finite difference equations to approximate derivatives.&lt;br /&gt;
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有限差分法是一种数值方法，用差分方程近似微分方程的解。&lt;br /&gt;
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=== Finite volume method ===&lt;br /&gt;
有限体积法&lt;br /&gt;
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{{main|Finite volume method}}&lt;br /&gt;
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Similar to the finite difference method or finite element method, values are calculated at discrete places on a meshed geometry. &amp;quot;Finite volume&amp;quot; refers to the small volume surrounding each node point on a mesh. In the finite volume method, surface integrals in a partial differential equation that contain a divergence term are converted to volume integrals, using the [[divergence theorem]]. These terms are then evaluated as fluxes at the surfaces of each finite volume. Because the flux entering a given volume is identical to that leaving the adjacent volume, these methods conserve mass by design.&lt;br /&gt;
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Similar to the finite difference method or finite element method, values are calculated at discrete places on a meshed geometry. &amp;quot;Finite volume&amp;quot; refers to the small volume surrounding each node point on a mesh. In the finite volume method, surface integrals in a partial differential equation that contain a divergence term are converted to volume integrals, using the divergence theorem. These terms are then evaluated as fluxes at the surfaces of each finite volume. Because the flux entering a given volume is identical to that leaving the adjacent volume, these methods conserve mass by design.&lt;br /&gt;
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类似于有限差分法或有限元分析，函数值是在网状几何体上的离散位置进行计算的。“有限体积”是指网格上每个节点周围的小体积。在有限体积法中，偏微分方程中含有散度项的面积分用散度定理积分转换成体积分。然后将这些项用于估算每个有限体积表面上的通量。由于进入给定体积的通量与转移到相邻体积元的通量相同，所以这些方法在设计上保证了质量守恒。&lt;br /&gt;
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==See also==&lt;br /&gt;
请参阅&lt;br /&gt;
* [[Dirichlet boundary condition]]&lt;br /&gt;
狄利克雷边界条件&lt;br /&gt;
* [[Jet bundle]]&lt;br /&gt;
射流丛&lt;br /&gt;
* [[Laplace transform applied to differential equations]]&lt;br /&gt;
微分方程中的拉普拉斯变换&lt;br /&gt;
* [[List of dynamical systems and differential equations topics]]&lt;br /&gt;
动力学系统和微分方程的列表&lt;br /&gt;
* [[Matrix differential equation]]&lt;br /&gt;
矩阵微分方程&lt;br /&gt;
* [[Neumann boundary condition]]&lt;br /&gt;
诺伊曼边界条件&lt;br /&gt;
* [[Numerical partial differential equations]]&lt;br /&gt;
数值偏微分方程&lt;br /&gt;
* [[Partial differential algebraic equation]]&lt;br /&gt;
偏微分代数方程&lt;br /&gt;
* [[Recurrence relation]]&lt;br /&gt;
递推关系&lt;br /&gt;
* [[Robin boundary condition]]&lt;br /&gt;
罗宾边界条件&lt;br /&gt;
* [[Stochastic processes and boundary value problems]]&lt;br /&gt;
随机过程和边值问题&lt;br /&gt;
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== The energy method ==&lt;br /&gt;
能量法&lt;br /&gt;
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The energy method is a mathematical procedure that can be used to verify well-posedness of initial-boundary-value-problems.&amp;lt;ref&amp;gt;{{cite book |title=High Order Difference Methods for Time Dependent PDE&lt;br /&gt;
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The energy method is a mathematical procedure that can be used to verify well-posedness of initial-boundary-value-problems.&amp;lt;ref&amp;gt;{{cite book |title=High Order Difference Methods for Time Dependent PDE&lt;br /&gt;
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能量法是验证初边值问题适定性的一种数学方法。 时变偏微分方程的高阶差分方法&lt;br /&gt;
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|first=Bertil|last=Gustafsson|publisher=Springer|year=2008|isbn=978-3-540-74992-9|doi=10.1007/978-3-540-74993-6}}&amp;lt;/ref&amp;gt; In the following example the energy method is used to decide where and which boundary conditions should be imposed such that the resulting IBVP is well-posed. Consider the one-dimensional hyperbolic PDE given by&lt;br /&gt;
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|first=Bertil|last=Gustafsson|publisher=Springer|year=2008|isbn=978-3-540-74992-9|doi=10.1007/978-3-540-74993-6}}&amp;lt;/ref&amp;gt; In the following example the energy method is used to decide where and which boundary conditions should be imposed such that the resulting IBVP is well-posed. Consider the one-dimensional hyperbolic PDE given by&lt;br /&gt;
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| first Bertil | last Gustafsson | publisher | Springer | year 2008 | isbn 978-3-540-74992-9 | doi 10.1007 / 978-3-540-74993-6} / ref 在下面的例子中，使用能量方法来决定应该施加哪些边界条件，使得得到的 IBVP适定。考虑一维双曲偏微分方程&lt;br /&gt;
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: &amp;lt;math&amp;gt;\frac{\partial u}{\partial t} + \alpha \frac{\partial u}{\partial x} = 0, \quad x \in [a,b], \operatorname t &amp;gt; 0,&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;\frac{\partial u}{\partial t} + \alpha \frac{\partial u}{\partial x} = 0, \quad x \in [a,b], \operatorname t &amp;gt; 0,&amp;lt;/math&amp;gt;&lt;br /&gt;
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where &amp;lt;math&amp;gt;\alpha \neq 0&amp;lt;/math&amp;gt; is a constant and &amp;lt;math&amp;gt;u(x,t)&amp;lt;/math&amp;gt; is an unknown function with initial condition &amp;lt;math&amp;gt;u(x,0) = f(x)&amp;lt;/math&amp;gt;. Multiplying with &amp;lt;math&amp;gt;u&amp;lt;/math&amp;gt; and integrating over the domain gives&lt;br /&gt;
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where &amp;lt;math&amp;gt;\alpha \neq 0&amp;lt;/math&amp;gt; is a constant and &amp;lt;math&amp;gt;u(x,t)&amp;lt;/math&amp;gt; is an unknown function with initial condition &amp;lt;math&amp;gt;u(x,0) = f(x)&amp;lt;/math&amp;gt;. Multiplying with &amp;lt;math&amp;gt;u&amp;lt;/math&amp;gt; and integrating over the domain gives&lt;br /&gt;
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其中 &amp;lt;math&amp;gt;\alpha \neq 0&amp;lt;/math&amp;gt; 是常数，并且 &amp;lt;math&amp;gt;u(x,t)&amp;lt;/math&amp;gt; 是未知函数，初始条件是 &amp;lt;math&amp;gt;u(x,0) = f(x)&amp;lt;/math&amp;gt;。乘以 &amp;lt;math&amp;gt;u&amp;lt;/math&amp;gt; 并在域上进行积分。&lt;br /&gt;
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能量法是一种数学过程，可用于验证初始边界值问题的适定性。在下面的示例中，将使用能量法决定应在何处施加哪些边界条件，以使得到的IBVP处于适当位置。考虑下式给出的一维双曲PDE&lt;br /&gt;
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: &amp;lt;math&amp;gt;\int_a^b u \frac{\partial u}{\partial t} \operatorname dx + \alpha \int _a ^b u \frac{\partial u}{\partial x} \operatorname dx = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;\int_a^b u \frac{\partial u}{\partial t} \operatorname dx + \alpha \int _a ^b u \frac{\partial u}{\partial x} \operatorname dx = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
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Using that&lt;br /&gt;
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Using that&lt;br /&gt;
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利用这一点&lt;br /&gt;
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: &amp;lt;math&amp;gt;\int _a ^b u \frac{\partial u}{\partial t} \operatorname dx = \frac{1}{2} \frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 \quad \text{and} \quad \int _a ^b u \frac{\partial u}{\partial x} \operatorname dx = \frac{1}{2} u(b,t)^2 - \frac{1}{2} u(a,t)^2,.&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;\int _a ^b u \frac{\partial u}{\partial t} \operatorname dx = \frac{1}{2} \frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 \quad \text{and} \quad \int _a ^b u \frac{\partial u}{\partial x} \operatorname dx = \frac{1}{2} u(b,t)^2 - \frac{1}{2} u(a,t)^2,.&amp;lt;/math&amp;gt;&lt;br /&gt;
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where integration by parts has been used for the second relationship, we get&lt;br /&gt;
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where integration by parts has been used for the second relationship, we get&lt;br /&gt;
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第二个关系中采用了分部积分法，我们可以得到&lt;br /&gt;
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: &amp;lt;math&amp;gt;\frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 + \alpha u(b,t)^2 - \alpha u(a,t)^2 = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;\frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 + \alpha u(b,t)^2 - \alpha u(a,t)^2 = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
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Here &amp;lt;math&amp;gt;\vert \vert \cdot \vert \vert&amp;lt;/math&amp;gt; denotes the standard L2-norm.&lt;br /&gt;
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Here &amp;lt;math&amp;gt;\vert \vert \cdot \vert \vert&amp;lt;/math&amp;gt; denotes the standard L2-norm.&lt;br /&gt;
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在这里，&amp;lt;math&amp;gt;\vert \vert \cdot \vert \vert&amp;lt;/math&amp;gt; 表示标准的 L2-正则。&lt;br /&gt;
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For well-posedness we require that the energy of the solution is non-increasing, i.e. that &amp;lt;math&amp;gt;\frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 \leq 0&amp;lt;/math&amp;gt;, which is achieved by specifying &amp;lt;math&amp;gt;u&amp;lt;/math&amp;gt; at &amp;lt;math&amp;gt;x = a&amp;lt;/math&amp;gt; if &amp;lt;math&amp;gt;\alpha &amp;gt; 0&amp;lt;/math&amp;gt; and at &amp;lt;math&amp;gt;x = b&amp;lt;/math&amp;gt; if &amp;lt;math&amp;gt;\alpha &amp;lt; 0&amp;lt;/math&amp;gt;. This corresponds to only imposing boundary conditions at the inflow. Note that well-posedness allows for growth in terms of data (initial and boundary) and thus it is sufficient to show that &amp;lt;math&amp;gt;\frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 \leq 0&amp;lt;/math&amp;gt; holds when all data is set to zero.&lt;br /&gt;
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For well-posedness we require that the energy of the solution is non-increasing, i.e. that &amp;lt;math&amp;gt;\frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 \leq 0&amp;lt;/math&amp;gt;, which is achieved by specifying &amp;lt;math&amp;gt;u&amp;lt;/math&amp;gt; at &amp;lt;math&amp;gt;x = a&amp;lt;/math&amp;gt; if &amp;lt;math&amp;gt;\alpha &amp;gt; 0&amp;lt;/math&amp;gt; and at &amp;lt;math&amp;gt;x = b&amp;lt;/math&amp;gt; if &amp;lt;math&amp;gt;\alpha &amp;lt; 0&amp;lt;/math&amp;gt;. This corresponds to only imposing boundary conditions at the inflow. Note that well-posedness allows for growth in terms of data (initial and boundary) and thus it is sufficient to show that &amp;lt;math&amp;gt;\frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 \leq 0&amp;lt;/math&amp;gt; holds when all data is set to zero.&lt;br /&gt;
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对于适定性，我们要解的能量是不增加的，即 &amp;lt;math&amp;gt;\frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 \leq 0&amp;lt;/math&amp;gt; ，这种关系可以通过在&amp;lt;math&amp;gt;x = a&amp;lt;/math&amp;gt;处 （如果 &amp;lt;math&amp;gt;\alpha &amp;gt; 0&amp;lt;/math&amp;gt;） 以及 &amp;lt;math&amp;gt;x = b&amp;lt;/math&amp;gt;处 （如果 &amp;lt;math&amp;gt;\alpha &amp;lt; 0&amp;lt;/math&amp;gt;）指定&amp;lt;math&amp;gt;u&amp;lt;/math&amp;gt;的值来实现。这只相当于在入流处附加边界条件。注意，适定性允许在数据(初始和边界)上的增长，因此它足以表明当所有数据设置为零时应有 &amp;lt;math&amp;gt;\frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 \leq 0&amp;lt;/math&amp;gt;。&lt;br /&gt;
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==[[用户:Yuling|Yuling]]（[[用户讨论:Yuling|讨论]]）“This corresponds to only imposing boundary conditions at the inflow.” 这句话中的inflow不是很理解&lt;br /&gt;
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==Notes==&lt;br /&gt;
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{{Reflist}}&lt;br /&gt;
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|first=Abdul-Majid|last=Wazwaz|publisher=Higher Education Press|year=2009|isbn=978-3-642-00251-9|page=}}&lt;br /&gt;
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|first=Abdul-Majid|last=Wazwaz|publisher=Higher Education Press|year=2009|isbn=978-3-642-00251-9|page=}}&lt;br /&gt;
&lt;br /&gt;
| first Abdul-Majid | last Wazwaz | publisher Higher Education Press | year 2009 | isbn 978-3-642-00251-9 | page }&lt;br /&gt;
&lt;br /&gt;
* {{cite book |title=Partial Differential Equations Methods and Applications&lt;br /&gt;
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|first=Abdul-Majid|last=Wazwaz|publisher=A.A. Balkema|year=2002|isbn=90-5809-369-7|page=}}&lt;br /&gt;
&lt;br /&gt;
|first=Abdul-Majid|last=Wazwaz|publisher=A.A. Balkema|year=2002|isbn=90-5809-369-7|page=}}&lt;br /&gt;
&lt;br /&gt;
| first Abdul-Majid | last Wazwaz | publisher a.a.Balkema | year 2002 | isbn 90-5809-369-7 | page }&lt;br /&gt;
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* {{Citation |first=D. |last=Zwillinger |title=Handbook of Differential Equations |publisher=Academic Press |location=Boston |year=1997 |edition=3rd |isbn=0-12-784395-7 }}.&lt;br /&gt;
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* {{Citation |authorlink=Neil Gershenfeld |first=N. |last=Gershenfeld |title=The Nature of Mathematical Modeling |location=New York |publisher=Cambridge University Press, New York, NY, USA |year=1999 |edition=1st |isbn=0-521-57095-6 }}.&lt;br /&gt;
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* {{Citation |first=I.S. |last=Krasil'shchik |lastauthoramp=yes |first2=A.M., Eds. |last2=Vinogradov |title=Symmetries and Conserwation Laws for Differential Equations of Mathematical Physics |publisher=American Mathematical Society, Providence, Rhode Island, USA |year=1999 |isbn=0-8218-0958-X }}.&lt;br /&gt;
&lt;br /&gt;
* {{Citation |first=I.S. |last=Krasil'shchik |first2=V.V. |last2=Lychagin|lastauthoramp=yes |first3=A.M. |last3=Vinogradov |title=Geometry of Jet Spaces and Nonlinear Partial Differential Equations |publisher=Gordon and Breach Science Publishers, New York, London, Paris, Montreux, Tokyo |year=1986 |isbn=2-88124-051-8 }}.&lt;br /&gt;
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* {{Citation |first=A.M. |last=Vinogradov |title=Cohomological Analysis of Partial Differential Equations and Secondary Calculus |publisher=American Mathematical Society, Providence, Rhode Island, USA |year=2001 |isbn=0-8218-2922-X }}.&lt;br /&gt;
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* {{cite book |title=High Order Difference Methods for Time Dependent PDE&lt;br /&gt;
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|first=Bertil|last=Gustafsson|publisher=Springer|year=2008|isbn=978-3-540-74992-9|doi=10.1007/978-3-540-74993-6}}&lt;br /&gt;
&lt;br /&gt;
|first=Bertil|last=Gustafsson|publisher=Springer|year=2008|isbn=978-3-540-74992-9|doi=10.1007/978-3-540-74993-6}}&lt;br /&gt;
&lt;br /&gt;
| first Bertil | last Gustafsson | Springer | year 2008 | isbn 978-3-540-74992-9 | doi 10.1007 / 978-3-540-74993-6}&lt;br /&gt;
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{{refend}}&lt;br /&gt;
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== Further reading ==&lt;br /&gt;
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* {{Cite journal|last=Cajori|first=Florian|authorlink=Florian Cajori|year=1928|title=The Early History of Partial Differential Equations and of Partial Differentiation and Integration|url=http://www.math.harvard.edu/archive/21a_fall_14/exhibits/cajori/cajori.pdf|journal=The American Mathematical Monthly|volume=35|issue=9|pages=459–467|doi=10.2307/2298771|access-date=2016-05-15|archive-url=https://web.archive.org/web/20181123102253/http://www.math.harvard.edu/archive/21a_fall_14/exhibits/cajori/cajori.pdf|archive-date=2018-11-23|url-status=dead}}&lt;br /&gt;
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== External links ==&lt;br /&gt;
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{{Sister project links| wikt=no | commons=Category:Solutions of PDE | b=Partial Differential Equations | n=no | q=Partial differential equation | s=no | v=no | voy=no | species=no | d=no}}&lt;br /&gt;
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* {{springer|title=Differential equation, partial|id=p/d031920}}&lt;br /&gt;
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* [http://eqworld.ipmnet.ru/en/pde-en.htm Partial Differential Equations: Exact Solutions] at EqWorld: The World of Mathematical Equations.&lt;br /&gt;
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* [http://eqworld.ipmnet.ru/en/solutions/eqindex/eqindex-pde.htm Partial Differential Equations: Index] at EqWorld: The World of Mathematical Equations.&lt;br /&gt;
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* [http://eqworld.ipmnet.ru/en/methods/meth-pde.htm Partial Differential Equations: Methods] at EqWorld: The World of Mathematical Equations.&lt;br /&gt;
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* [https://web.archive.org/web/20170701144823/http://www.exampleproblems.com/wiki/index.php?title=Partial_Differential_Equations Example problems with solutions] at exampleproblems.com&lt;br /&gt;
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* [http://mathworld.wolfram.com/PartialDifferentialEquation.html Partial Differential Equations] at mathworld.wolfram.com&lt;br /&gt;
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* [https://reference.wolfram.com/language/FEMDocumentation/tutorial/SolvingPDEwithFEM.html Partial Differential Equations] with Mathematica&lt;br /&gt;
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* [http://www.mathworks.com/moler/pdes.pdf Partial Differential Equations] in Cleve Moler: Numerical Computing with MATLAB&lt;br /&gt;
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* [http://www.nag.com/numeric/fl/nagdoc_fl24/html/D03/d03intro.html Partial Differential Equations] at nag.com&lt;br /&gt;
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* {{cite web |first=Grant |last=Sanderson |title=But what is a partial differential equation? |work=3Blue1Brown |date=April 21, 2019 |url=https://www.youtube.com/watch?v=ly4S0oi3Yz8&amp;amp;list=PLZHQObOWTQDNPOjrT6KVlfJuKtYTftqH6 |via=[[YouTube]] }}&lt;br /&gt;
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{{Differential equations topics}}&lt;br /&gt;
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[[Category:Partial differential equations| ]]&lt;br /&gt;
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[[Category:Multivariable calculus]]&lt;br /&gt;
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类别: 多元微积分&lt;br /&gt;
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[[Category:Differential equations]]&lt;br /&gt;
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Category:Differential equations&lt;br /&gt;
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类别: 微分方程&lt;br /&gt;
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Category:Concepts in physics&lt;br /&gt;
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&amp;lt;small&amp;gt;This page was moved from [[wikipedia:en:Partial differential equation]]. Its edit history can be viewed at [[偏微分方程/edithistory]]&amp;lt;/small&amp;gt;&amp;lt;/noinclude&amp;gt;&lt;br /&gt;
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[[Category:待整理页面]]&lt;/div&gt;</summary>
		<author><name>Ruili</name></author>
	</entry>
	<entry>
		<id>https://wiki.swarma.org/index.php?title=%E5%81%8F%E5%BE%AE%E5%88%86%E6%96%B9%E7%A8%8B&amp;diff=18295</id>
		<title>偏微分方程</title>
		<link rel="alternate" type="text/html" href="https://wiki.swarma.org/index.php?title=%E5%81%8F%E5%BE%AE%E5%88%86%E6%96%B9%E7%A8%8B&amp;diff=18295"/>
		<updated>2020-11-13T14:48:57Z</updated>

		<summary type="html">&lt;p&gt;Ruili：&lt;/p&gt;
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&lt;div&gt;此词条暂由Yuling翻译，未经人工整理和审校，带来阅读不便，请见谅。&lt;br /&gt;
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[[File:Heat.gif|thumb|right|A visualisation of a solution to the two-dimensional [[heat equation]] with temperature represented by the third dimension]]&lt;br /&gt;
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A visualisation of a solution to the two-dimensional [[heat equation with temperature represented by the third dimension]]&lt;br /&gt;
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以三维表示温度的二维热方程解的可视化&lt;br /&gt;
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In [[mathematics]], a '''partial differential equation''' ('''PDE''') is a [[differential equation]] that contains unknown [[Multivariable calculus|multivariable functions]] and their [[partial derivative]]s. PDEs are used to formulate problems involving functions of several variables, and are either solved by hand, or used to create a [[computer model]]. A special case is [[ordinary differential equation]]s (ODEs), which deal with functions of a single variable and their derivatives.&lt;br /&gt;
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In mathematics, a partial differential equation (PDE) is a differential equation that contains unknown multivariable functions and their partial derivatives. PDEs are used to formulate problems involving functions of several variables, and are either solved by hand, or used to create a computer model. A special case is ordinary differential equations (ODEs), which deal with functions of a single variable and their derivatives.&lt;br /&gt;
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在数学中，'''&amp;lt;font color = &amp;quot;#ff8000&amp;quot;&amp;gt; 偏微分方程函数 Partial Differential Equation&amp;lt;/font&amp;gt;'''是包含未知多元函数及其偏导数的微分方程。偏微分方程用于描述涉及多元函数的问题，可以通过人为求解，也可以通过建立计算机模型来求解。常微分方程是偏微分方程一种特殊情况，它处理的是一元函数及其导数。&lt;br /&gt;
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PDEs can be used to describe a wide variety of phenomena such as sound, heat, [[diffusion]], [[electrostatics]], [[Electromagnetism|electrodynamics]], [[fluid dynamics]], [[Elasticity (physics)|elasticity]], [[gravitation]] and [[quantum mechanics]]. These seemingly distinct physical phenomena can be formalised similarly in terms of PDEs. Just as ordinary differential equations often model one-dimensional [[dynamical system]]s, partial differential equations often model [[multidimensional system]]s. PDEs find their generalisation in [[stochastic partial differential equation]]s.&lt;br /&gt;
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PDEs can be used to describe a wide variety of phenomena such as sound, heat, diffusion, electrostatics, electrodynamics, fluid dynamics, elasticity, gravitation and quantum mechanics. These seemingly distinct physical phenomena can be formalised similarly in terms of PDEs. Just as ordinary differential equations often model one-dimensional dynamical systems, partial differential equations often model multidimensional systems. PDEs find their generalisation in stochastic partial differential equations.&lt;br /&gt;
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偏微分方程可以用来描述各种各样的物理现象，如声音，热量，扩散，静电，电动力学，流体力学，弹性力学，重力和量子力学。这些看起来截然不同的物理现象却可以用类似的偏微分方程来描述。正如常微分方程经常对一维动力系统进行建模一样，偏微分方程经常对多维系统进行建模。随机偏微分方程是偏微分方程的一种推广。&lt;br /&gt;
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== Introduction ==&lt;br /&gt;
引言&lt;br /&gt;
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Partial differential equations (PDEs) are equations that involve rates of change with respect to [[continuous variables]]. For example, the position of a [[rigid body]] is specified by six parameters,&amp;lt;ref&amp;gt;{{Cite book|url=https://books.google.com/books?id=v9PLbcYd9aUC&amp;amp;pg=PA32|title=Modelling and Control of Robot Manipulators|last=Sciavicco|first=Lorenzo|last2=Siciliano|first2=Bruno|date=2001-02-19|publisher=Springer Science &amp;amp; Business Media|isbn=9781852332211|language=en}}&amp;lt;/ref&amp;gt; but the configuration of a [[fluid]] is given by the [[continuous distribution]] of several parameters, such as the [[temperature]], [[pressure]], and so forth. The dynamics for the rigid body take place in a finite-dimensional [[Configuration space (physics)|configuration space]]; the dynamics for the fluid occur in an infinite-dimensional configuration space. This distinction usually makes PDEs much harder to solve than ordinary differential equations (ODEs), but here again, there will be simple solutions for linear problems. Classic domains where PDEs are used include [[acoustics]], [[fluid dynamics]], [[electrodynamics]], and [[heat transfer]].&lt;br /&gt;
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Partial differential equations (PDEs) are equations that involve rates of change with respect to continuous variables. For example, the position of a rigid body is specified by six parameters, but the configuration of a fluid is given by the continuous distribution of several parameters, such as the temperature, pressure, and so forth. The dynamics for the rigid body take place in a finite-dimensional configuration space; the dynamics for the fluid occur in an infinite-dimensional configuration space. This distinction usually makes PDEs much harder to solve than ordinary differential equations (ODEs), but here again, there will be simple solutions for linear problems. Classic domains where PDEs are used include acoustics, fluid dynamics, electrodynamics, and heat transfer.&lt;br /&gt;
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偏微分方程(简称为PDEs)涉及到方程相对于连续变量的变化率。例如，刚体的位置是由六个参数确定的，而流体的状态是由几个参数的连续分布给出的，如温度、压力等。刚体的动力学过程发生在有限维状态空间中，流体的动力学过程发生在无限维状态空间中。这种区别通常使偏微分方程比常微分方程更难求解，但是线性问题仍然有简单的求解方式。使用偏微分方程的经典领域包括声学、流体力学、电动力学和传热学。&lt;br /&gt;
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A partial differential equation (PDE) for the function {{math|''u''(''x''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;,… ''x&amp;lt;sub&amp;gt;n&amp;lt;/sub&amp;gt;'')}} is an equation of the form&lt;br /&gt;
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A partial differential equation (PDE) for the function  is an equation of the form&lt;br /&gt;
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函数 {{math|''u''(''x''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;,… ''x&amp;lt;sub&amp;gt;n&amp;lt;/sub&amp;gt;'')}} 的偏微分方程形式是：&lt;br /&gt;
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: &amp;lt;math&amp;gt;f \left (x_1, \ldots x_n; u, \frac{\partial u}{\partial x_1}, \ldots \frac{\partial u}{\partial x_n}; \frac{\partial^2 u}{\partial x_1 \partial x_1}, \ldots \frac{\partial^2 u}{\partial x_1 \partial x_n}; \ldots \right) = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;f \left (x_1, \ldots x_n; u, \frac{\partial u}{\partial x_1}, \ldots \frac{\partial u}{\partial x_n}; \frac{\partial^2 u}{\partial x_1 \partial x_1}, \ldots \frac{\partial^2 u}{\partial x_1 \partial x_n}; \ldots \right) = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
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If {{mvar|f}} is a [[linear function]] of {{mvar|u}} and its derivatives, then the PDE is called linear. Common examples of linear PDEs include the [[heat equation]], the [[wave equation]], [[Laplace's equation]], [[Helmholtz equation]], [[Klein–Gordon equation]], and [[Poisson's equation]].&lt;br /&gt;
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If  is a linear function of  and its derivatives, then the PDE is called linear. Common examples of linear PDEs include the heat equation, the wave equation, Laplace's equation, Helmholtz equation, Klein–Gordon equation, and Poisson's equation.&lt;br /&gt;
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如果 {{mvar|f}} 是函数 {{math|''u''}} 及其导数的线性函数，则偏微分方程称为线性函数。线性偏微分方程的常见例子包括热方程、波动方程、拉普拉斯方程、亥姆霍兹方程方程、克莱因-高登方程和泊松方程。&lt;br /&gt;
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A relatively simple PDE is&lt;br /&gt;
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A relatively simple PDE is&lt;br /&gt;
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一个相对简单的偏微分方程：&lt;br /&gt;
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: &amp;lt;math&amp;gt;\frac{\partial u}{\partial x}(x,y) = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;\frac{\partial u}{\partial x}(x,y) = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
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This relation [[Logical implication|implies]] that the function {{math|''u''(''x'',''y'')}} is independent of {{mvar|x}}. However, the equation gives no information on the function's dependence on the variable {{mvar|y}}. Hence the general solution of this equation is&lt;br /&gt;
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This relation implies that the function  is independent of . However, the equation gives no information on the function's dependence on the variable . Hence the general solution of this equation is&lt;br /&gt;
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这意味着函数 {{math|''u''(''x'',''y'')}} 独立于 {{mvar|x}} 的。然而，这个方程没有给出关于函数和自变量的相关性的信息。因此，这个方程的通解是&lt;br /&gt;
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: &amp;lt;math&amp;gt;u(x,y) = f(y),&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;u(x,y) = f(y),&amp;lt;/math&amp;gt;&lt;br /&gt;
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where {{mvar|f}} is an arbitrary function of {{mvar|y}}. The analogous ordinary differential equation is&lt;br /&gt;
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where  is an arbitrary function of . The analogous ordinary differential equation is&lt;br /&gt;
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其中， {{mvar|f}} 是 {{mvar|y}} 的任意函数。&lt;br /&gt;
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类似的常微分方程是：&lt;br /&gt;
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: &amp;lt;math&amp;gt;\frac{\mathrm{d} u}{\mathrm{d} x}(x) = 0,&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;\frac{\mathrm{d} u}{\mathrm{d} x}(x) = 0,&amp;lt;/math&amp;gt;&lt;br /&gt;
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which has the solution&lt;br /&gt;
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which has the solution&lt;br /&gt;
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它的解为&lt;br /&gt;
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: &amp;lt;math&amp;gt;u(x) = c,&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;u(x) = c,&amp;lt;/math&amp;gt;&lt;br /&gt;
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where {{mvar|c}} is any [[Constant (mathematics)|constant]] value. These two examples illustrate that general solutions of ordinary differential equations (ODEs) involve arbitrary constants, but solutions of PDEs involve arbitrary functions.&lt;br /&gt;
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where  is any constant value. These two examples illustrate that general solutions of ordinary differential equations (ODEs) involve arbitrary constants, but solutions of PDEs involve arbitrary functions.&lt;br /&gt;
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这里，{{mvar|c}} 是一个任意常量。&lt;br /&gt;
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这两个例子说明常微分方程的一般解包含任意常数，但偏微分方程的解包含任意函数。&lt;br /&gt;
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A solution of a PDE is generally not [[Uniqueness quantification|unique]]; additional conditions must generally be specified on the [[Boundary (topology)|boundary]] of the region where the solution is defined. For instance, in the simple example above, the function {{math|''f''(''y'')}} can be determined if {{mvar|u}} is specified on the line {{math|''x'' {{=}} 0}}.&lt;br /&gt;
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A solution of a PDE is generally not unique; additional conditions must generally be specified on the boundary of the region where the solution is defined. For instance, in the simple example above, the function  can be determined if  is specified on the line  0}}.&lt;br /&gt;
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偏微分方程的解一般不是唯一的; 一般必须在定义解的区域边界上定义附加条件。 例如，在上面的简单示例中，如果在 {{math|''x'' {{=}} 0}} 时确定了 {{mvar|u}} 的值，则可以确定该函数 {{math|''f''(''y'')}}。&lt;br /&gt;
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== Existence and uniqueness ==&lt;br /&gt;
存在性和唯一性&lt;br /&gt;
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Although the issue of existence and uniqueness of solutions of ordinary differential equations has a very satisfactory answer with the [[Picard–Lindelöf theorem]], that is far from the case for partial differential equations. The [[Cauchy–Kowalevski theorem]] states that the [[Cauchy problem]] for any partial differential equation whose coefficients are [[Analytic function|analytic]] in the unknown function and its derivatives, has a locally unique analytic solution. Although this result might appear to settle the existence and uniqueness of solutions, there are examples of linear partial differential equations whose coefficients have derivatives of all orders (which are nevertheless not analytic) but which have no solutions at all: see [[Lewy's example|Lewy (1957)]]. Even if the solution of a partial differential equation exists and is unique, it may nevertheless have undesirable properties.  The mathematical study of these questions is usually in the more powerful context of [[weak solution]]s.&lt;br /&gt;
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Although the issue of existence and uniqueness of solutions of ordinary differential equations has a very satisfactory answer with the Picard–Lindelöf theorem, that is far from the case for partial differential equations. The Cauchy–Kowalevski theorem states that the Cauchy problem for any partial differential equation whose coefficients are analytic in the unknown function and its derivatives, has a locally unique analytic solution. Although this result might appear to settle the existence and uniqueness of solutions, there are examples of linear partial differential equations whose coefficients have derivatives of all orders (which are nevertheless not analytic) but which have no solutions at all: see Lewy (1957). Even if the solution of a partial differential equation exists and is unique, it may nevertheless have undesirable properties.  The mathematical study of these questions is usually in the more powerful context of weak solutions.&lt;br /&gt;
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尽管常微分方程解的存在性和唯一性用'''&amp;lt;font color=&amp;quot;#ff8000&amp;quot;&amp;gt;弗罗贝尼乌斯定理 Picard–Lindelöf Theorem&amp;lt;/font&amp;gt;得到了令人满意的结果，但偏微分方程解的存在性和唯一性却远没有得到解决。'''&amp;lt;font color=&amp;quot;#ff8000&amp;quot;&amp;gt;柯西-科瓦列夫斯基定理 Cauchy–Kowalevski theorem&amp;lt;/font&amp;gt;指出：对于任意系数在未知函数及其导数中解析的偏微分方程，柯西问题存在一个局部唯一的解析解。虽然这个结果似乎解决了解的存在性和唯一性问题，但是存在一些线性偏微分方程-其系数具有所有级数的导数(尽管这些导数不是解析的) ，但是根本没有解: 见 Lewy (1957)。即使偏微分方程的解存在且唯一，它仍然可能具有不可预料的性质。这些问题的数学研究通常是在更有力的弱解的背景下进行的。&lt;br /&gt;
&lt;br /&gt;
An example of pathological behavior is the sequence (depending upon {{mvar|n}}) of [[Cauchy problem]]s for the [[Laplace equation]]&lt;br /&gt;
&lt;br /&gt;
An example of pathological behavior is the sequence (depending upon ) of Cauchy problems for the Laplace equation&lt;br /&gt;
&lt;br /&gt;
反常特征的一个例子是拉普拉斯方程的柯西问题的序列(取决于{{mvar|n}})&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt;\frac{\partial^2 u}{\partial x^2} + \frac{\partial^2 u}{\partial y^2}=0,&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;\frac{\partial^2 u}{\partial x^2} + \frac{\partial^2 u}{\partial y^2}=0,&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
with [[boundary condition]]s&lt;br /&gt;
&lt;br /&gt;
with boundary conditions&lt;br /&gt;
&lt;br /&gt;
具有边界条件&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt;\begin{align} u(x,0) &amp;amp;= 0, \\ \frac{\partial u}{\partial y}(x,0) &amp;amp;= \frac{\sin nx}{n}, \end{align}&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;\begin{align} u(x,0) &amp;amp;= 0, \\ \frac{\partial u}{\partial y}(x,0) &amp;amp;= \frac{\sin nx}{n}, \end{align}&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
where {{mvar|n}} is an integer. The derivative of {{mvar|u}} with respect to {{mvar|y}} approaches zero [[uniform convergence|uniformly]] in {{mvar|x}} as {{mvar|n}} increases, but the solution is&lt;br /&gt;
&lt;br /&gt;
where  is an integer. The derivative of  with respect to  approaches zero uniformly in  as  increases, but the solution is&lt;br /&gt;
&lt;br /&gt;
其中 {{mvar|n}} 是整数。{{mvar|u}} 关于 {{mvar|y}} 的导数，一致地随着 {{mvar|n}} 的增加而趋于零，但解是&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt;u(x,y) = \frac{\sinh ny \sin nx}{n^2}.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;u(x,y) = \frac{\sinh ny \sin nx}{n^2}.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
This solution approaches infinity if {{mvar|nx}} is not an integer multiple of {{pi}} for any non-zero value of {{mvar|y}}. The Cauchy problem for the Laplace equation is called ''ill-posed'' or ''not [[Well-posed problem|well-posed]]'', since the solution does not continuously depend on the data of the problem. Such ill-posed problems are not usually satisfactory for physical applications.&lt;br /&gt;
&lt;br /&gt;
This solution approaches infinity if  is not an integer multiple of  for any non-zero value of . The Cauchy problem for the Laplace equation is called ill-posed or not well-posed, since the solution does not continuously depend on the data of the problem. Such ill-posed problems are not usually satisfactory for physical applications.&lt;br /&gt;
&lt;br /&gt;
对于任何非零的 {{mvar|y}}，如果 {{mvar|nx}} 不是模板 {{pi}} 的整数倍，这个解会接近于无穷大。拉普拉斯方程的柯西问题被称为不适定的（可以译为ill-posed或not well-posed），因为解不是连续地依赖于问题的数据。这种不适定问题通常不能满足物理应用。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The [[Navier–Stokes existence and smoothness|existence of solutions for the Navier–Stokes equations]], a partial differential equation, is part of one of the [[Millennium Prize Problems]].&lt;br /&gt;
&lt;br /&gt;
The existence of solutions for the Navier–Stokes equations, a partial differential equation, is part of one of the Millennium Prize Problems.&lt;br /&gt;
&lt;br /&gt;
偏微分方程”纳维-斯托克斯方程“的解的存在性就是千禧年大奖难题之一的一部分。&lt;br /&gt;
&lt;br /&gt;
== Notation ==&lt;br /&gt;
符号&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
In PDEs, it is common to denote partial derivatives using subscripts. That is:&lt;br /&gt;
&lt;br /&gt;
In PDEs, it is common to denote partial derivatives using subscripts. That is:&lt;br /&gt;
&lt;br /&gt;
在偏微分方程中，通常用下标表示偏导数。例如:&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt;u_x = \frac{\partial u}{\partial x}&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;u_x = \frac{\partial u}{\partial x}&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt;u_{xx} = \frac{\partial^2 u}{\partial x^2} &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;u_{xx} = \frac{\partial^2 u}{\partial x^2} &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt;u_{xy} = \frac{\partial^2 u}{\partial y\, \partial x} = \frac{\partial}{\partial y } \left(\frac{\partial u}{\partial x}\right). &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;u_{xy} = \frac{\partial^2 u}{\partial y\, \partial x} = \frac{\partial}{\partial y } \left(\frac{\partial u}{\partial x}\right). &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Especially in physics, [[del]] or nabla ({{math|∇}}) is often used to denote spatial derivatives, and {{math|''&amp;amp;#x307;u'', ''ü''}} for time derivatives. For example, the [[wave equation]] (mentioned below) can be written as&lt;br /&gt;
&lt;br /&gt;
Especially in physics, del or nabla () is often used to denote spatial derivatives, and  for time derivatives. For example, the wave equation (mentioned below) can be written as&lt;br /&gt;
&lt;br /&gt;
特别是在物理学中，[[del]] 或 nabla ({{math|∇}}) 经常用来表示空间导数和时间导数。例如，波动方程(在下文中提到)可以写成：&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt;\ddot u=c^2\nabla^2u&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt;\ddot u=c^2\nabla^2u&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
or&lt;br /&gt;
&lt;br /&gt;
or&lt;br /&gt;
&lt;br /&gt;
或&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt;\ddot u=c^2\Delta u&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt;\ddot u=c^2\Delta u&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
where {{math|Δ}} is the [[Laplace operator]].&lt;br /&gt;
&lt;br /&gt;
where  is the Laplace operator.&lt;br /&gt;
&lt;br /&gt;
其中，{{math|Δ}} 代表拉普拉斯算子。&lt;br /&gt;
&lt;br /&gt;
== Classification ==&lt;br /&gt;
分类&lt;br /&gt;
&lt;br /&gt;
Some linear, second-order partial differential equations can be classified as [[parabolic partial differential equation|parabolic]], [[hyperbolic partial differential equation|hyperbolic]] and [[elliptic partial differential equation|elliptic]]. Others, such as the [[Euler–Tricomi equation]], have different types in different regions. The classification provides a guide to appropriate initial and boundary conditions and to the smoothness of the solutions.&lt;br /&gt;
&lt;br /&gt;
Some linear, second-order partial differential equations can be classified as parabolic, hyperbolic and elliptic. Others, such as the Euler–Tricomi equation, have different types in different regions. The classification provides a guide to appropriate initial and boundary conditions and to the smoothness of the solutions.&lt;br /&gt;
&lt;br /&gt;
一些线性二阶偏微分方程可分为抛物型方程、双曲型方程和椭圆型方程。其他的方程，如欧拉-特里科米方程，在不同的领域有不同的类型。这种分类有助于选择适当的初始和边界条件以及提高解的平滑性。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
=== Equations of first order ===&lt;br /&gt;
一阶方程&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{{main|First-order partial differential equation}}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
=== Linear equations of second order ===&lt;br /&gt;
二阶线性方程&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Assuming {{math|''u&amp;lt;sub&amp;gt;xy&amp;lt;/sub&amp;gt;'' {{=}} ''u&amp;lt;sub&amp;gt;yx&amp;lt;/sub&amp;gt;''}}, the general linear second-order PDE in two independent variables has the form&lt;br /&gt;
&lt;br /&gt;
Assuming  u&amp;lt;sub&amp;gt;yx&amp;lt;/sub&amp;gt;}}, the general linear second-order PDE in two independent variables has the form&lt;br /&gt;
&lt;br /&gt;
假设 {{math|''u&amp;lt;sub&amp;gt;xy&amp;lt;/sub&amp;gt;'' {{=}} ''u&amp;lt;sub&amp;gt;yx&amp;lt;/sub&amp;gt;''}}，含有两个独立变量的一般线性二阶偏微分方程具有如下形式：&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt;Au_{xx} + 2Bu_{xy} + Cu_{yy} + \cdots \mbox{(lower order terms)} = 0,&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;Au_{xx} + 2Bu_{xy} + Cu_{yy} + \cdots \mbox{(lower order terms)} = 0,&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
where the coefficients {{mvar|A}}, {{mvar|B}}, {{mvar|C}}... may depend upon {{mvar|x}} and {{mvar|y}}. If {{math|''A''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; + ''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; + ''C''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; &amp;gt; 0}} over a region of the {{mvar|xy}}-plane, the PDE is second-order in that region. This form is analogous to the equation for a conic section:&lt;br /&gt;
&lt;br /&gt;
where the coefficients , , ... may depend upon  and . If  over a region of the -plane, the PDE is second-order in that region. This form is analogous to the equation for a conic section:&lt;br /&gt;
&lt;br /&gt;
其中的系数 {{mvar|A}}, {{mvar|B}}, {{mvar|C}}... 一般取决于 {{mvar|x}} 和 {{mvar|y}} 。如果在 {{mvar|xy}}-平面的一个区域上 {{math|''A''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; + ''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; + ''C''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; &amp;gt; 0}}，偏微分方程是二阶的，这种形式类似于圆锥截面的方程:&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt;Ax^2 + 2Bxy + Cy^2 + \cdots = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;Ax^2 + 2Bxy + Cy^2 + \cdots = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
More precisely, replacing {{math|∂&amp;lt;sub&amp;gt;''x''&amp;lt;/sub&amp;gt;}} by {{mvar|X}}, and likewise for other variables (formally this is done by a [[Fourier transform]]), converts a constant-coefficient PDE into a polynomial of the same degree, with the terms of the highest degree (a [[homogeneous polynomial]], here a [[quadratic form]]) being most significant for the classification.&lt;br /&gt;
&lt;br /&gt;
More precisely, replacing  by , and likewise for other variables (formally this is done by a Fourier transform), converts a constant-coefficient PDE into a polynomial of the same degree, with the terms of the highest degree (a homogeneous polynomial, here a quadratic form) being most significant for the classification.&lt;br /&gt;
&lt;br /&gt;
更准确地说，用 {{mvar|X}} 替换 {{math|∂&amp;lt;sub&amp;gt;''x''&amp;lt;/sub&amp;gt;}}，并同样替换其它变量(通常由傅里叶变换完成)，将一个常系数偏微分方程转换成一个相同次数的多项式，最高次数的项(齐次多项式，这里是一个二次形式)对于偏微分方程的分类最为重要。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Just as one classifies [[conic section]]s and quadratic forms into parabolic, hyperbolic, and elliptic based on the [[discriminant]] {{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − 4''AC''}}, the same can be done for a second-order PDE at a given point.  However, the [[discriminant]] in a PDE is given by {{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC''}} due to the convention of the {{mvar|xy}} term being {{math|2''B''}} rather than {{mvar|B}}; formally, the discriminant (of the associated quadratic form) is {{math|(2''B'')&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − 4''AC'' {{=}} 4(''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC'')}}, with the factor of 4 dropped for simplicity.&lt;br /&gt;
&lt;br /&gt;
Just as one classifies conic sections and quadratic forms into parabolic, hyperbolic, and elliptic based on the discriminant , the same can be done for a second-order PDE at a given point.  However, the discriminant in a PDE is given by  due to the convention of the  term being  rather than ; formally, the discriminant (of the associated quadratic form) is  4(B&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − AC)}}, with the factor of 4 dropped for simplicity.&lt;br /&gt;
&lt;br /&gt;
正如人们可以根据判别式 {{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − 4''AC''}} 将圆锥截面和二次型分为抛物型、双曲型和椭圆型一样，对于给定点的二阶偏微分方程也可以这样做。然而，偏微分方程中的判别式 {{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − 4''AC''}} 是根据交叉项的系数{{math|2''B''}} 而不是 {{mvar|B}} 给出的，形式上，判别式(关联二次型)是 {{math|(2''B'')&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − 4''AC'' {{=}} 4(''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC'')}}，为简单起见，去掉了因子4。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
# {{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC'' &amp;lt; 0}} (''[[elliptic partial differential equation]]''): Solutions of [[elliptic partial differential equation|elliptic PDEs]] are as smooth as the coefficients allow, within the interior of the region where the equation and solutions are defined. For example, solutions of [[Laplace's equation]] are analytic within the domain where they are defined, but solutions may assume boundary values that are not smooth. The motion of a fluid at subsonic speeds can be approximated with elliptic PDEs, and the Euler–Tricomi equation is elliptic where {{math|''x'' &amp;lt; 0}}.&lt;br /&gt;
&lt;br /&gt;
  (elliptic partial differential equation): Solutions of elliptic PDEs are as smooth as the coefficients allow, within the interior of the region where the equation and solutions are defined. For example, solutions of Laplace's equation are analytic within the domain where they are defined, but solutions may assume boundary values that are not smooth. The motion of a fluid at subsonic speeds can be approximated with elliptic PDEs, and the Euler–Tricomi equation is elliptic where .&lt;br /&gt;
&lt;br /&gt;
{{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC'' &amp;lt; 0}} (椭圆型微分方程)：在定义方程和解的区域内部，椭圆型偏微分方程的解在系数允许的程度内光滑。例如，拉普拉斯方程的解在它们被定义的区域内是解析的，但可能假设边界值是不光滑的。亚音速流体的运动可以用椭圆型偏微分方程近似，欧拉-特里科米方程在 {{math|''x'' &amp;lt; 0}} 时是椭圆型偏微分方程。&lt;br /&gt;
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&lt;br /&gt;
&lt;br /&gt;
# {{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC'' {{=}} 0}} (''[[parabolic partial differential equation]]''): Equations that are [[parabolic partial differential equation|parabolic]] at every point can be transformed into a form analogous to the [[heat equation]] by a change of independent variables. Solutions smooth out as the transformed time variable increases. The Euler–Tricomi equation has parabolic type on the line where {{math|''x'' {{=}} 0}}.&lt;br /&gt;
&lt;br /&gt;
  0}} (parabolic partial differential equation): Equations that are parabolic at every point can be transformed into a form analogous to the heat equation by a change of independent variables. Solutions smooth out as the transformed time variable increases. The Euler–Tricomi equation has parabolic type on the line where  0}}.&lt;br /&gt;
&lt;br /&gt;
{{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC'' {{=}} 0}}（抛物型偏微分方程）：在每一点上都是抛物线型的方程可以通过改变自变量从而转化成类似于热方程的形式。随着转换后的时间变量的增加，方程的解变得平滑。欧拉-特里科米方程在特征线 {{math|''x'' {{=}} 0}} 上是抛物线型的。&lt;br /&gt;
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&lt;br /&gt;
&lt;br /&gt;
# {{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC'' &amp;gt; 0}} (''[[hyperbolic partial differential equation]]''): [[hyperbolic partial differential equation|hyperbolic]] equations retain any discontinuities of functions or derivatives in the initial data. An example is the [[wave equation]]. The motion of a fluid at supersonic speeds can be approximated with hyperbolic PDEs, and the Euler–Tricomi equation is hyperbolic where {{math|''x'' &amp;gt; 0}}.&lt;br /&gt;
&lt;br /&gt;
  (hyperbolic partial differential equation): hyperbolic equations retain any discontinuities of functions or derivatives in the initial data. An example is the wave equation. The motion of a fluid at supersonic speeds can be approximated with hyperbolic PDEs, and the Euler–Tricomi equation is hyperbolic where .&lt;br /&gt;
&lt;br /&gt;
{{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC'' &amp;gt; 0}} (双曲型偏微分方程)：双曲型方程在初始数据中保留了函数或导数的任何不连续性。波动方程就是其中的一个例子。超音速流体的运动可以用双曲型偏微分方程近似，欧拉-特里科米方程在 {{math|''x'' &amp;gt; 0}} 时是双曲型的。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
If there are {{mvar|n}} independent variables {{math|''x''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;, ''x''&amp;lt;sub&amp;gt;2 &amp;lt;/sub&amp;gt;,… ''x''&amp;lt;sub&amp;gt;''n''&amp;lt;/sub&amp;gt;}}, a general linear partial differential equation of second order has the form&lt;br /&gt;
&lt;br /&gt;
If there are  independent variables , a general linear partial differential equation of second order has the form&lt;br /&gt;
&lt;br /&gt;
如果存在 {{mvar|n}} 个自变量 {{math|''x''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;, ''x''&amp;lt;sub&amp;gt;2 &amp;lt;/sub&amp;gt;,… ''x''&amp;lt;sub&amp;gt;''n''&amp;lt;/sub&amp;gt;}}，一般二阶线性偏微分方程的形式是：&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt;L u =\sum_{i=1}^n\sum_{j=1}^n a_{i,j} \frac{\partial^2 u}{\partial x_i \partial x_j} \quad \text{ plus lower-order terms} =0.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;L u =\sum_{i=1}^n\sum_{j=1}^n a_{i,j} \frac{\partial^2 u}{\partial x_i \partial x_j} \quad \text{ plus lower-order terms} =0.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The classification depends upon the signature of the eigenvalues of the coefficient matrix {{math|''a''&amp;lt;sub&amp;gt;''i'',''j''&amp;lt;/sub&amp;gt;}}.&lt;br /&gt;
&lt;br /&gt;
The classification depends upon the signature of the eigenvalues of the coefficient matrix .&lt;br /&gt;
&lt;br /&gt;
这种分类取决于系数矩阵特征值的符号（正负性）。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
# Elliptic: the eigenvalues are all positive or all negative.&lt;br /&gt;
&lt;br /&gt;
 Elliptic: the eigenvalues are all positive or all negative.&lt;br /&gt;
&lt;br /&gt;
椭圆形方程: 特征值全部为正或全部为负。&lt;br /&gt;
&lt;br /&gt;
# Parabolic: the eigenvalues are all positive or all negative, save one that is zero.&lt;br /&gt;
&lt;br /&gt;
 Parabolic: the eigenvalues are all positive or all negative, save one that is zero.&lt;br /&gt;
&lt;br /&gt;
抛物线形方程:除了一个为零值，特征值全部为正或全部为负。&lt;br /&gt;
&lt;br /&gt;
# Hyperbolic: there is only one negative eigenvalue and all the rest are positive, or there is only one positive eigenvalue and all the rest are negative.&lt;br /&gt;
&lt;br /&gt;
 Hyperbolic: there is only one negative eigenvalue and all the rest are positive, or there is only one positive eigenvalue and all the rest are negative.&lt;br /&gt;
&lt;br /&gt;
双曲形方程: 只有一个负特征值，其余的都是正特征值，或者只有一个正特征值，其余的都是负特征值。&lt;br /&gt;
&lt;br /&gt;
# Ultrahyperbolic: there is more than one positive eigenvalue and more than one negative eigenvalue, and there are no zero eigenvalues. There is only a limited theory for ultrahyperbolic equations (Courant and Hilbert, 1962).&lt;br /&gt;
&lt;br /&gt;
 Ultrahyperbolic: there is more than one positive eigenvalue and more than one negative eigenvalue, and there are no zero eigenvalues. There is only a limited theory for ultrahyperbolic equations (Courant and Hilbert, 1962).&lt;br /&gt;
&lt;br /&gt;
超双形方程: 存在多于一个正特征值和多于一个的负特征值，且不存在零特征值。对于超双曲方程，只存在有限的理论(Courant 和 Hilbert，1962)。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
=== Systems of first-order equations and characteristic surfaces ===&lt;br /&gt;
一阶方程组和特征曲面&lt;br /&gt;
&lt;br /&gt;
The classification of partial differential equations can be extended to systems of first-order equations, where the unknown {{mvar|u}} is now a [[Euclidean vector|vector]] with {{mvar|m}} components, and the coefficient matrices {{mvar|A&amp;lt;sub&amp;gt;ν&amp;lt;/sub&amp;gt;}} are {{mvar|m}} by {{mvar|m}} matrices for {{math|''ν'' {{=}} 1, 2,… ''n''}}. The partial differential equation takes the form&lt;br /&gt;
&lt;br /&gt;
The classification of partial differential equations can be extended to systems of first-order equations, where the unknown  is now a vector with  components, and the coefficient matrices  are  by  matrices for  1, 2,… n}}. The partial differential equation takes the form&lt;br /&gt;
&lt;br /&gt;
偏微分方程的分类可以推广到一阶方程组，其中未知量 {{mvar|u}} 是有 {{mvar|m}} 个分量的向量。对于 {{math|''ν'' {{=}} 1, 2,… ''n''}}，系数矩阵 {{mvar|A&amp;lt;sub&amp;gt;ν&amp;lt;/sub&amp;gt;}} 是 {{mvar|m}} × {{mvar|m}} 的矩阵。偏微分方程形式如下：&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt;Lu = \sum_{\nu=1}^{n} A_\nu \frac{\partial u}{\partial x_\nu} + B=0,&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;Lu = \sum_{\nu=1}^{n} A_\nu \frac{\partial u}{\partial x_\nu} + B=0,&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
where the coefficient matrices {{mvar|A&amp;lt;sub&amp;gt;ν&amp;lt;/sub&amp;gt;}} and the vector {{mvar|B}} may depend upon {{mvar|x}} and {{mvar|u}}. If a [[hypersurface]] {{mvar|S}} is given in the implicit form&lt;br /&gt;
&lt;br /&gt;
where the coefficient matrices  and the vector  may depend upon  and . If a hypersurface  is given in the implicit form&lt;br /&gt;
&lt;br /&gt;
其中，系数矩阵 {{mvar|A&amp;lt;sub&amp;gt;ν&amp;lt;/sub&amp;gt;}} 和向量 {{mvar|B}} 可能依赖于 {{mvar|x}} 和 {{mvar|u}}。如果超曲面是以以下隐式形式给出的，&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt;\varphi(x_1, x_2, \ldots x_n)=0,&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;\varphi(x_1, x_2, \ldots x_n)=0,&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
where {{mvar|φ}} has a non-zero gradient, then {{mvar|S}} is a '''characteristic surface''' for the operator {{mvar|L}} at a given point if the characteristic form vanishes:&lt;br /&gt;
&lt;br /&gt;
where  has a non-zero gradient, then  is a characteristic surface for the operator  at a given point if the characteristic form vanishes:&lt;br /&gt;
&lt;br /&gt;
其中，存在一个非零的梯度 {{mvar|φ}}，对于在给定点上特征形式消失的算子，特征曲面 {{mvar|S}} 形式如下:&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt;Q\left(\frac{\partial\varphi}{\partial x_1}, \ldots\frac{\partial\varphi}{\partial x_n}\right) =\det\left[\sum_{\nu=1}^nA_\nu \frac{\partial \varphi}{\partial x_\nu}\right]=0.\,&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;Q\left(\frac{\partial\varphi}{\partial x_1}, \ldots\frac{\partial\varphi}{\partial x_n}\right) =\det\left[\sum_{\nu=1}^nA_\nu \frac{\partial \varphi}{\partial x_\nu}\right]=0.\,&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The geometric interpretation of this condition is as follows: if data for {{mvar|u}} are prescribed on the surface {{mvar|S}}, then it may be possible to determine the normal derivative of {{mvar|u}} on {{mvar|S}} from the differential equation. If the data on {{mvar|S}} and the differential equation determine the normal derivative of {{mvar|u}} on {{mvar|S}}, then {{mvar|S}} is non-characteristic. If the data on {{mvar|S}} and the differential equation ''do not'' determine the normal derivative of {{mvar|u}} on {{mvar|S}}, then the surface is '''characteristic''', and the differential equation restricts the data on {{mvar|S}}: the differential equation is ''internal'' to {{mvar|S}}.&lt;br /&gt;
&lt;br /&gt;
The geometric interpretation of this condition is as follows: if data for  are prescribed on the surface , then it may be possible to determine the normal derivative of  on  from the differential equation. If the data on  and the differential equation determine the normal derivative of  on , then  is non-characteristic. If the data on  and the differential equation do not determine the normal derivative of  on , then the surface is characteristic, and the differential equation restricts the data on : the differential equation is internal to .&lt;br /&gt;
&lt;br /&gt;
这个条件的几何解释如下: 如果关于 {{mvar|u}} 的数据是在曲面 {{mvar|S}} 上规定的，那么就有可能依据微分方程确定曲面 {{mvar|S}} 上 {{mvar|u}} 的法向导数。如果曲面 {{mvar|S}} 上的数据和上面的微分方程能确定曲面 {{mvar|S}} 上 {{mvar|u}} 的法向导数，那么它就是非特征的。如果曲面 {{mvar|S}} 上的数据和上面的微分方程不能确定曲面 {{mvar|S}} 上 {{mvar|u}} 的法向导数，那么曲面是特征的，并且微分方程将数据限制在曲面 {{mvar|S}} 上：微分方程是在曲面 {{mvar|S}} 内部。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
# A first-order system {{math|''Lu'' {{=}} 0}} is ''elliptic'' if no surface is characteristic for {{mvar|L}}: the values of {{mvar|u}} on {{mvar|S}} and the differential equation always determine the normal derivative of {{mvar|u}} on {{mvar|S}}.&lt;br /&gt;
&lt;br /&gt;
 A first-order system  0}} is elliptic if no surface is characteristic for : the values of  on  and the differential equation always determine the normal derivative of  on .&lt;br /&gt;
&lt;br /&gt;
如果对于 {{mvar|L}} 没有曲面是特征的，则一阶系统 {{math|''Lu'' {{=}} 0}} 是椭圆形的：{{mvar|u}}在 {{mvar|S}} 的值和微分方程总能够决定 {{mvar|S}} 上 {{mvar|u}} 的法向导数。&lt;br /&gt;
&lt;br /&gt;
# A first-order system is ''hyperbolic'' at a point if there is a '''spacelike''' surface {{mvar|S}} with normal {{mvar|ξ}} at that point. This means that, given any non-trivial vector {{mvar|η}} orthogonal to {{mvar|ξ}}, and a scalar multiplier {{mvar|λ}}, the equation {{math|''Q''(''λξ'' + ''η'') {{=}} 0}} has {{mvar|m}} real roots {{math|''λ''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;, ''λ''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;,… ''λ''&amp;lt;sub&amp;gt;''m''&amp;lt;/sub&amp;gt;}}. The system is '''strictly hyperbolic''' if these roots are always distinct. The geometrical interpretation of this condition is as follows: the characteristic form {{math|''Q''(''ζ'') {{=}} 0}} defines a cone (the normal cone) with homogeneous coordinates ζ. In the hyperbolic case, this cone has {{mvar|m}} sheets, and the axis {{math|''ζ'' {{=}} ''λξ''}} runs inside these sheets: it does not intersect any of them. But when displaced from the origin by η, this axis intersects every sheet. In the elliptic case, the normal cone has no real sheets.&lt;br /&gt;
&lt;br /&gt;
 A first-order system is hyperbolic at a point if there is a spacelike surface  with normal  at that point. This means that, given any non-trivial vector  orthogonal to , and a scalar multiplier , the equation  0}} has  real roots . The system is strictly hyperbolic if these roots are always distinct. The geometrical interpretation of this condition is as follows: the characteristic form  0}} defines a cone (the normal cone) with homogeneous coordinates ζ. In the hyperbolic case, this cone has  sheets, and the axis  λξ}} runs inside these sheets: it does not intersect any of them. But when displaced from the origin by η, this axis intersects every sheet. In the elliptic case, the normal cone has no real sheets.&lt;br /&gt;
&lt;br /&gt;
如果在该点存在一个法向量为 {{mvar|ξ}}的 '''&amp;lt;font color=&amp;quot;#ff8000&amp;quot;&amp;gt;类空曲面 Spacclike Surface&amp;lt;/font&amp;gt; {{mvar|S}} ，则一阶系统在那一点是双曲的。这意味着，给定任意正交于 {{mvar|ξ}} 的非平凡向量 {{mvar|η}} 和一个标量乘子 {{mvar|λ}}，方程 {{math|''Q''(''λξ'' + ''η'') {{=}} 0}} 有 {{mvar|m}} 个实根 {{math|''λ''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;, ''λ''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;,… ''λ''&amp;lt;sub&amp;gt;''m''&amp;lt;/sub&amp;gt;}}。如果这些根始终不同，则该系统是严格双曲形的。这个条件的几何解释如下: 特征形式 {{math|''Q''(''ζ'') {{=}} 0}} 定义了一个具有齐次坐标 ζ的圆锥(法线圆锥)。在双曲形的情况下，这个圆锥体有 {{mvar|m}} 层，并且轴 {{math|''ζ'' {{=}} ''λξ''}} 在这些层中运动: 它不与任何一层相交。但是当从原点偏离η时，这条轴线与每一层都相交。在椭圆形的情况下，法向圆锥没有实层。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==[[用户:Yuling|Yuling]]（[[用户讨论:Yuling|讨论]]） sheet 这个单词也不很理解，我直译为了“层”&lt;br /&gt;
&lt;br /&gt;
=== Equations of mixed type ===&lt;br /&gt;
混合型方程&lt;br /&gt;
&lt;br /&gt;
If a PDE has coefficients that are not constant, it is possible that it will not belong to any of these categories but rather be of '''mixed type'''. A simple but important example is the [[Euler–Tricomi equation]]&lt;br /&gt;
&lt;br /&gt;
If a PDE has coefficients that are not constant, it is possible that it will not belong to any of these categories but rather be of mixed type. A simple but important example is the Euler–Tricomi equation&lt;br /&gt;
&lt;br /&gt;
如果偏微分方程的系数不是常数，那么它可能不属于这些类别中的任何一个，而是属于混合类型。一个简单但重要的例子是欧拉-特里科米方程&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt;u_{xx} = xu_{yy},&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;u_{xx} = xu_{yy},&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
which is called '''elliptic-hyperbolic''' because it is elliptic in the region {{math|''x'' &amp;lt; 0}}, hyperbolic in the region {{math|''x'' &amp;gt; 0}}, and degenerate parabolic on the line {{math|''x'' {{=}} 0}}.&lt;br /&gt;
&lt;br /&gt;
which is called elliptic-hyperbolic because it is elliptic in the region , hyperbolic in the region , and degenerate parabolic on the line  0}}.&lt;br /&gt;
&lt;br /&gt;
它在 {{math|''x'' &amp;lt; 0}} 的区域上是椭圆形，在 {{math|''x'' &amp;gt; 0}} 区域上是双曲形，在 {{math|''x'' {{=}} 0}}这条线上是退化为抛物线形，因此称之为椭圆-双曲型。&lt;br /&gt;
&lt;br /&gt;
&amp;lt;!--&lt;br /&gt;
&lt;br /&gt;
&amp;lt;!--&lt;br /&gt;
&lt;br /&gt;
&amp;lt;!--&lt;br /&gt;
&lt;br /&gt;
''fill in: Dirichlet and Neumann boundaries, hyperbolic/parabolic/elliptic separation of variables, [[Fourier analysis]], [[Green's function]]s ...--&amp;gt;&lt;br /&gt;
&lt;br /&gt;
fill in: Dirichlet and Neumann boundaries, hyperbolic/parabolic/elliptic separation of variables, Fourier analysis, Green's functions ...--&amp;gt;&lt;br /&gt;
&lt;br /&gt;
填写: Dirichlet 和 Neumann 边界，双曲 / 抛物线 / 椭圆分离变量法，傅立叶分析，Green 函数... --&lt;br /&gt;
&lt;br /&gt;
=== Infinite-order PDEs in quantum mechanics ===&lt;br /&gt;
量子力学中的无限阶偏微分方程&lt;br /&gt;
&lt;br /&gt;
In the [[phase space formulation]] of quantum mechanics,  one may consider the [[Method of quantum characteristics|quantum Hamilton's equations]] for trajectories of quantum particles. These equations are infinite-order PDEs. However, in the semiclassical expansion, one has a finite system of ODEs at any fixed order of [[Dirac constant|{{mvar|ħ}}]].  The evolution equation of the [[Wigner quasi-probability distribution|c]] is also an infinite-order PDE. The quantum trajectories are [[Method of quantum characteristics|quantum characteristics]], with the use of which one could calculate the evolution of the Wigner function.&lt;br /&gt;
&lt;br /&gt;
In the phase space formulation of quantum mechanics,  one may consider the quantum Hamilton's equations for trajectories of quantum particles. These equations are infinite-order PDEs. However, in the semiclassical expansion, one has a finite system of ODEs at any fixed order of Dirac constant|.  The evolution equation of the Wigner function is also an infinite-order PDE. The quantum trajectories are quantum characteristics, with the use of which one could calculate the evolution of the Wigner function.&lt;br /&gt;
&lt;br /&gt;
在量子力学中的相空间表述中，我们可以考虑用于求解量子粒子的轨迹的量子哈密顿的方程。这些方程是无限阶偏微分方程。然而，在半经典展开中，我们在给定[[Dirac constant|{{mvar|ħ}}]]阶数下有一个有限的的常微分方程组。'''&amp;lt;font color=&amp;quot;#ff8000&amp;quot;&amp;gt;维格纳函数  Wigner Function&amp;lt;/font&amp;gt;的演化方程也是一个无限阶偏微分方程。由于量子轨道的量子特性，所以它通常可以用来计算维格纳函数的演化。&lt;br /&gt;
&lt;br /&gt;
== Analytical solutions ==&lt;br /&gt;
解析解&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
===Separation of variables===&lt;br /&gt;
分离变量法&lt;br /&gt;
&lt;br /&gt;
{{main|Separable partial differential equation}}&lt;br /&gt;
&lt;br /&gt;
Linear PDEs can be reduced to systems of ordinary differential equations by the important technique of separation of variables. This technique rests on a characteristic of solutions to differential equations: if one can find any solution that solves the equation and satisfies the boundary conditions, then it is ''the'' solution (this also applies to ODEs). We assume as an [[ansatz]] that the dependence of a solution on the parameters space and time can be written as a product of terms that each depend on a single parameter, and then see if this can be made to solve the problem.&amp;lt;ref&amp;gt;{{cite book|last1=Gershenfeld|first1=Neil|title=The nature of mathematical modeling|date=2000|publisher=Cambridge Univ. Press|location=Cambridge|isbn=0521570956|page=27|edition=Reprinted (with corr.)}}&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
Linear PDEs can be reduced to systems of ordinary differential equations by the important technique of separation of variables. This technique rests on a characteristic of solutions to differential equations: if one can find any solution that solves the equation and satisfies the boundary conditions, then it is the solution (this also applies to ODEs). We assume as an ansatz that the dependence of a solution on the parameters space and time can be written as a product of terms that each depend on a single parameter, and then see if this can be made to solve the problem.&lt;br /&gt;
&lt;br /&gt;
线性偏微分方程组可以通过分离变量法这一重要方法来简化为常微分方程组。这种方法依赖于微分方程解的一个特征: 如果能找到任何一个满足方程和边界条件的解，那么这个解就是方程的解(这也适用于常微分方程)。我们假设解对参数空间和时间的依赖可以写成对它们每一项的依赖以及一个参数的乘积，然后再看看这是否可以用来解决这个问题。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
In the method of separation of variables, one reduces a PDE to a PDE in fewer variables, which is an ordinary differential equation if in one variable – these are in turn easier to solve.&lt;br /&gt;
&lt;br /&gt;
In the method of separation of variables, one reduces a PDE to a PDE in fewer variables, which is an ordinary differential equation if in one variable – these are in turn easier to solve.&lt;br /&gt;
&lt;br /&gt;
在分离变量法方法中，可以将偏微分方程简化为含有更少变量的偏微分方程，如果只有一个变量，那么就变成了一个'''&amp;lt;font color = &amp;quot;#ff8000&amp;quot;&amp;gt;常微分方程 Ordinary Differential Equation&amp;lt;/font&amp;gt;'''-- 反过来，这些方程也更容易求解。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
This is possible for simple PDEs, which are called [[separable partial differential equation]]s, and the domain is generally a rectangle (a product of intervals). Separable PDEs correspond to [[diagonal matrices]] – thinking of &amp;quot;the value for fixed {{mvar|x}}&amp;quot; as a coordinate, each coordinate can be understood separately.&lt;br /&gt;
&lt;br /&gt;
This is possible for simple PDEs, which are called separable partial differential equations, and the domain is generally a rectangle (a product of intervals). Separable PDEs correspond to diagonal matrices – thinking of &amp;quot;the value for fixed &amp;quot; as a coordinate, each coordinate can be understood separately.&lt;br /&gt;
&lt;br /&gt;
对于简单的偏微分方程(称为可分离偏微分方程)来说，这是可能的，而且方程通常定义在一个矩形区域(区间的乘积)上。可分离偏微分方程对应于对角线矩阵——以“固定值”为坐标，每个坐标可分开理解。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
This generalizes to the [[method of characteristics]], and is also used in [[integral transform]]s.&lt;br /&gt;
&lt;br /&gt;
This generalizes to the method of characteristics, and is also used in integral transforms.&lt;br /&gt;
&lt;br /&gt;
这种方法可以推广到特征曲线法，也可以用于积分变换。&lt;br /&gt;
&lt;br /&gt;
===Method of characteristics===&lt;br /&gt;
特征曲线法&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{{main|Method of characteristics}}&lt;br /&gt;
&lt;br /&gt;
In special cases, one can find characteristic curves on which the equation reduces to an ODE – changing coordinates in the domain to straighten these curves allows separation of variables, and is called the [[method of characteristics]].&lt;br /&gt;
&lt;br /&gt;
In special cases, one can find characteristic curves on which the equation reduces to an ODE – changing coordinates in the domain to straighten these curves allows separation of variables, and is called the method of characteristics.&lt;br /&gt;
&lt;br /&gt;
在特殊情况下，可以找到一些特征曲线，在这些曲线上方程可以变成一个常微分方程——意味着改变坐标从而使这些曲线变直从而达到分离变量的目的，这就是所谓的特征曲线法。&lt;br /&gt;
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&lt;br /&gt;
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More generally, one may find characteristic surfaces.&lt;br /&gt;
&lt;br /&gt;
More generally, one may find characteristic surfaces.&lt;br /&gt;
&lt;br /&gt;
更一般地说，人们可能会找到特征表面。&lt;br /&gt;
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&lt;br /&gt;
&lt;br /&gt;
===Integral transform===&lt;br /&gt;
积分变换&lt;br /&gt;
&lt;br /&gt;
An [[integral transform]] may transform the PDE to a simpler one, in particular, a separable PDE. This corresponds to diagonalizing an operator.&lt;br /&gt;
&lt;br /&gt;
An integral transform may transform the PDE to a simpler one, in particular, a separable PDE. This corresponds to diagonalizing an operator.&lt;br /&gt;
&lt;br /&gt;
积分变换可以将偏微分方程转换为更简单的偏微分方程，特别是可分离的偏微分方程。这对应于对角化算符。&lt;br /&gt;
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An important example of this is [[Fourier analysis]], which diagonalizes the heat equation using the [[eigenbasis]] of sinusoidal waves.&lt;br /&gt;
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An important example of this is Fourier analysis, which diagonalizes the heat equation using the eigenbasis of sinusoidal waves.&lt;br /&gt;
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这方面的一个重要例子是'''&amp;lt;font color = &amp;quot;#ff8000&amp;quot;&amp;gt;傅里叶分析  Fourier Analysis&amp;lt;/font&amp;gt;'''，它使用正弦波的特征基来对角化热方程。&lt;br /&gt;
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If the domain is finite or periodic, an infinite sum of solutions such as a [[Fourier series]] is appropriate, but an integral of solutions such as a [[Fourier integral]] is generally required for infinite domains. The solution for a point source for the heat equation given above is an example of the use of a Fourier integral.&lt;br /&gt;
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If the domain is finite or periodic, an infinite sum of solutions such as a Fourier series is appropriate, but an integral of solutions such as a Fourier integral is generally required for infinite domains. The solution for a point source for the heat equation given above is an example of the use of a Fourier integral.&lt;br /&gt;
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如果区域是有限的或周期性的，那么解为无限和的形式是恰当的，例如傅里叶级数，但是一个解的积分，例如傅立叶积分，一般是在无限区域上的。上面给出的热传导方程的点源解法就是使用傅里叶积分的一个例子。&lt;br /&gt;
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===Change of variables===&lt;br /&gt;
变量代换&lt;br /&gt;
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Often a PDE can be reduced to a simpler form with a known solution by a suitable [[Change of variables (PDE)|change of variables]].  For example, the [[Black–Scholes equation#Derivation|Black–Scholes]] PDE&lt;br /&gt;
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Often a PDE can be reduced to a simpler form with a known solution by a suitable change of variables.  For example, the Black–Scholes PDE&lt;br /&gt;
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偏微分方程通常可以通过变量的适当变化，用已知的解简化为更简单的形式。例如，布莱克-舒尔斯偏微分方程&lt;br /&gt;
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:&amp;lt;math&amp;gt; \frac{\partial V}{\partial t} + \tfrac{1}{2}\sigma^2 S^2\frac{\partial^2 V}{\partial S^2} + rS\frac{\partial V}{\partial S} - rV = 0 &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \frac{\partial V}{\partial t} + \tfrac{1}{2}\sigma^2 S^2\frac{\partial^2 V}{\partial S^2} + rS\frac{\partial V}{\partial S} - rV = 0 &amp;lt;/math&amp;gt;&lt;br /&gt;
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is reducible to the [[heat equation]]&lt;br /&gt;
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is reducible to the heat equation&lt;br /&gt;
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可以简化为热传导方程&lt;br /&gt;
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:&amp;lt;math&amp;gt; \frac{\partial u}{\partial \tau} = \frac{\partial^2 u}{\partial x^2}&amp;lt;/math&amp;gt;&lt;br /&gt;
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&amp;lt;math&amp;gt; \frac{\partial u}{\partial \tau} = \frac{\partial^2 u}{\partial x^2}&amp;lt;/math&amp;gt;&lt;br /&gt;
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by the change of variables (for complete details see {{webarchive |url=https://web.archive.org/web/20080411030405/http://www.math.unl.edu/~sdunbar1/Teaching/MathematicalFinance/Lessons/BlackScholes/Solution/solution.shtml |date=April 11, 2008 |title=Solution of the Black Scholes Equation }})&lt;br /&gt;
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by the change of variables (for complete details see )&lt;br /&gt;
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通过变量替换(完整的细节见)&lt;br /&gt;
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:&amp;lt;math&amp;gt;\begin{align}&lt;br /&gt;
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V(S,t) &amp;amp;= K v(x,\tau),\\[5px]&lt;br /&gt;
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x &amp;amp;= \ln\left(\tfrac{S}{K} \right),\\[5px]&lt;br /&gt;
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\tau &amp;amp;= \tfrac{1}{2} \sigma^2 (T - t),\\[5px]&lt;br /&gt;
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v(x,\tau)&amp;amp;=e^{-\alpha x-\beta\tau} u(x,\tau).&lt;br /&gt;
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\end{align}&amp;lt;/math&amp;gt;&lt;br /&gt;
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===Fundamental solution===&lt;br /&gt;
基本解&lt;br /&gt;
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{{main|Fundamental solution}}&lt;br /&gt;
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Inhomogeneous equations can often be solved (for constant coefficient PDEs, always be solved) by finding the [[fundamental solution]] (the solution for a point source), then taking the [[convolution]] with the boundary conditions to get the solution.&lt;br /&gt;
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Inhomogeneous equations can often be solved (for constant coefficient PDEs, always be solved) by finding the fundamental solution (the solution for a point source), then taking the convolution with the boundary conditions to get the solution.&lt;br /&gt;
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非齐次方程(常系数偏微分方程)一般是通过先求出基本解(点源的解) ，然后利用带边界条件的卷积来求解。&lt;br /&gt;
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This is analogous in [[signal processing]] to understanding a filter by its [[impulse response]].&lt;br /&gt;
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This is analogous in signal processing to understanding a filter by its impulse response.&lt;br /&gt;
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这类似于在信号处理中通过滤波器的脉冲响应来理解滤波器。&lt;br /&gt;
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===Superposition principle===&lt;br /&gt;
叠加原理&lt;br /&gt;
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{{further| Superposition principle }}&lt;br /&gt;
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The superposition principle applies to any linear system, including linear systems of PDEs. A common visualization of this concept is the interaction of two waves in phase being combined to result in a greater amplitude, for example {{math|sin ''x'' + sin ''x'' {{=}} 2 sin ''x''}}. The same principle can be observed in PDEs where the solutions may be real or complex and additive. [[Superposition principle|superposition]]&lt;br /&gt;
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The superposition principle applies to any linear system, including linear systems of PDEs. A common visualization of this concept is the interaction of two waves in phase being combined to result in a greater amplitude, for example  2 sin x}}. The same principle can be observed in PDEs where the solutions may be real or complex and additive. superposition&lt;br /&gt;
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'''&amp;lt;font color = &amp;quot;#ff8000&amp;quot;&amp;gt;叠加原理 Superposition Principle&amp;lt;/font&amp;gt;适用于任何线性系统，包括偏微分方程的线性系统。这个概念的一个常见的可视化是两个同相位的波相互作用结合在一起会产生更大的振幅，例如 {{math|sin ''x'' + sin ''x'' {{=}} 2 sin ''x''}}。在偏微分方程中也可以观察到同样的原理，其中的解可能是真实的或复杂的和可加的。叠加&lt;br /&gt;
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If {{math|''u''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;}} and {{math|''u''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;}} are solutions of linear PDE in some function space {{mvar|R}}, then {{math|''u'' {{=}} ''c''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;''u''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; + ''c''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;''u''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;}} with any constants {{math|''c''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;}} and {{math|''c''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;}} are also a solution of that PDE in the same function space.&lt;br /&gt;
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If  and  are solutions of linear PDE in some function space , then  c&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;u&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; + c&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;u&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;}} with any constants  and  are also a solution of that PDE in the same function space.&lt;br /&gt;
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若线性偏微分方程在某个函数空间{{mvar|R}}中有解{{math|''u''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;}} 和 {{math|''u''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;}}，则{{math|''u'' {{=}} ''c''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;''u''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; + ''c''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;''u''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;}}也是该偏微分方程在同一函数空间中的解，其中{{math|''c''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;}} 和 {{math|''c''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;}} 是任意常数。&lt;br /&gt;
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===Methods for non-linear equations===&lt;br /&gt;
非线性方程的求解方法&lt;br /&gt;
{{see also|nonlinear partial differential equation}}&lt;br /&gt;
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There are no generally applicable methods to solve nonlinear PDEs. Still, existence and uniqueness results (such as the [[Cauchy–Kowalevski theorem]]) are often possible, as are proofs of important qualitative and quantitative properties of solutions (getting these results is a major part of [[mathematical analysis|analysis]]). Computational solution to the nonlinear PDEs, the [[split-step method]], exist for specific equations like [[nonlinear Schrödinger equation]].&lt;br /&gt;
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There are no generally applicable methods to solve nonlinear PDEs. Still, existence and uniqueness results (such as the Cauchy–Kowalevski theorem) are often possible, as are proofs of important qualitative and quantitative properties of solutions (getting these results is a major part of analysis). Computational solution to the nonlinear PDEs, the split-step method, exist for specific equations like nonlinear Schrödinger equation.&lt;br /&gt;
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对于非线性偏微分方程，目前还没有普遍适用的求解方法。然而，通常是可能知道解的存在性和唯一性(如柯西-科瓦列夫斯基定理)，也是可能得到解的重要定性和定量性质的证明(得到这些结果是分析的主要部分)。非线性偏微分方程的计算解，即分步法，对一些特定的方程适用，比如非线性'''&amp;lt;font color=&amp;quot;#ff8000&amp;quot;&amp;gt;薛定谔方程 Schrödinger equation&amp;lt;/font&amp;gt;'''。&lt;br /&gt;
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Nevertheless, some techniques can be used for several types of equations. The [[h-principle|{{mvar|h}}-principle]] is the most powerful method to solve [[Underdetermined system|underdetermined]] equations. The [[Riquier–Janet theory]] is an effective method for obtaining information about many analytic [[Overdetermined system|overdetermined]] systems.&lt;br /&gt;
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Nevertheless, some techniques can be used for several types of equations. The -principle is the most powerful method to solve underdetermined equations. The Riquier–Janet theory is an effective method for obtaining information about many analytic overdetermined systems.&lt;br /&gt;
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然而，一些技巧可以用于几种类型的方程。h-原理是求解欠定方程最有效的方法。里基尔-珍妮特理论是一种可以获得许多解析超定系统信息的有效方法。&lt;br /&gt;
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The [[method of characteristics]] can be used in some very special cases to solve partial differential equations.&lt;br /&gt;
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The method of characteristics can be used in some very special cases to solve partial differential equations.&lt;br /&gt;
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特征线法可用于求解某些特殊情况下的偏微分方程。&lt;br /&gt;
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In some cases, a PDE can be solved via [[perturbation analysis]] in which the solution is considered to be a correction to an equation with a known solution. Alternatives are [[numerical analysis]] techniques from simple [[finite difference]] schemes to the more mature [[multigrid]] and [[finite element method]]s. Many interesting problems in science and engineering are solved in this way using [[computer]]s, sometimes high performance [[supercomputer]]s.&lt;br /&gt;
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In some cases, a PDE can be solved via perturbation analysis in which the solution is considered to be a correction to an equation with a known solution. Alternatives are numerical analysis techniques from simple finite difference schemes to the more mature multigrid and finite element methods. Many interesting problems in science and engineering are solved in this way using computers, sometimes high performance supercomputers.&lt;br /&gt;
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在某些情况下，偏微分方程可以通过扰动分析来求解。在扰动分析中，通常是求解将具有已知解的方程修正后的新得到方程。可供选择的数值分析技术从简单的差分格式到更成熟的多重网格和有限元方法。许多有趣的科学和工程问题都是在计算机上用这种方法解决的，有时是高性能超级计算机。&lt;br /&gt;
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===Lie group method===&lt;br /&gt;
李群方法&lt;br /&gt;
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From 1870 [[Sophus Lie]]'s work put the theory of differential equations on a more satisfactory foundation. He showed that the integration theories of the older mathematicians can, by the introduction of what are now called [[Lie group]]s, be referred, to a common source; and that ordinary differential equations which admit the same [[infinitesimal transformation]]s present comparable difficulties of integration. He also emphasized the subject of [[contact transformation|transformations of contact]].&lt;br /&gt;
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From 1870 Sophus Lie's work put the theory of differential equations on a more satisfactory foundation. He showed that the integration theories of the older mathematicians can, by the introduction of what are now called Lie groups, be referred, to a common source; and that ordinary differential equations which admit the same infinitesimal transformations present comparable difficulties of integration. He also emphasized the subject of transformations of contact.&lt;br /&gt;
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从1870年起，索弗斯·李的工作为微分方程理论奠定了一个较为令人满意的基础。他指出，通过引入现在所谓的李群，老一辈数学家的积分理论可以引用到一个共同的来源; 承认相同的无穷小变换的常微分方程在积分方面存在相当的困难。他还强调了接触的转变这一主题。&lt;br /&gt;
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==[[用户:Yuling|Yuling]]（[[用户讨论:Yuling|讨论]]）这句话“He also emphasized the subject of transformations of contact.”中的transformations of contact翻译的不太好。&lt;br /&gt;
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A general approach to solving PDEs uses the symmetry property of differential equations, the continuous [[infinitesimal transformation]]s of solutions to solutions ([[Lie theory]]). Continuous [[group theory]], [[Lie algebras]] and [[differential geometry]] are used to understand the structure of linear and nonlinear partial differential equations for generating integrable equations, to find its [[Lax pair]]s, recursion operators, [[Bäcklund transform]] and finally finding exact analytic solutions to the PDE.&lt;br /&gt;
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A general approach to solving PDEs uses the symmetry property of differential equations, the continuous infinitesimal transformations of solutions to solutions (Lie theory). Continuous group theory, Lie algebras and differential geometry are used to understand the structure of linear and nonlinear partial differential equations for generating integrable equations, to find its Lax pairs, recursion operators, Bäcklund transform and finally finding exact analytic solutions to the PDE.&lt;br /&gt;
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求解偏微分方程的一般方法是利用微分方程的对称性，即解到解的连续无穷小变换(李理论)。连续群论、李代数和微分几何理论被用来理解生成可积方程的线性和非线性偏微分方程的结构，找到它的Lax对、递归算子、 贝克伦德变换，最后找到偏微分方程的精确解析解。&lt;br /&gt;
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Symmetry methods have been recognized to study differential equations arising in mathematics, physics, engineering, and many other disciplines.&lt;br /&gt;
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Symmetry methods have been recognized to study differential equations arising in mathematics, physics, engineering, and many other disciplines.&lt;br /&gt;
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对称方法已被公认可以用于研究出现在数学，物理，工程和许多其他学科的微分方程。&lt;br /&gt;
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===Semianalytical methods===&lt;br /&gt;
半解析方法&lt;br /&gt;
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The [[Adomian decomposition method]], the [[Aleksandr Lyapunov|Lyapunov]] artificial small parameter method, and He's [[homotopy perturbation method]] are all special cases of the more general [[homotopy analysis method]]. These are series expansion methods, and except for the Lyapunov method, are independent of small physical parameters as compared to the well known [[perturbation theory]], thus giving these methods greater flexibility and solution generality.&lt;br /&gt;
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The Adomian decomposition method, the Lyapunov artificial small parameter method, and He's homotopy perturbation method are all special cases of the more general homotopy analysis method. These are series expansion methods, and except for the Lyapunov method, are independent of small physical parameters as compared to the well known perturbation theory, thus giving these methods greater flexibility and solution generality.&lt;br /&gt;
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阿多米安分解法、李雅普诺夫人工小参数方法和何同伦摄动方法都是更一般的同伦分析方法的特殊情况。除了李雅普诺夫方法之外，这些都是级数展开方法，与为人熟知的摄动理论方法相比，它们与小的物理参数无关，因此这些方法具有更大的灵活性和解的通用性。&lt;br /&gt;
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== Numerical solutions ==&lt;br /&gt;
数值解&lt;br /&gt;
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The three most widely used [[Numerical partial differential equations|numerical methods to solve PDEs]] are the [[finite element analysis|finite element method]] (FEM), [[finite volume method]]s (FVM) and [[finite difference method]]s (FDM), as well other kind of methods called [[Meshfree methods]], which were made to solve problems where the before mentioned methods are limited. The FEM has a prominent position among these methods and especially its exceptionally efficient higher-order version [[hp-FEM]]. Other hybrid versions of FEM and Meshfree methods include the generalized finite element method (GFEM), [[extended finite element method]] (XFEM), [[Spectral element method|spectral finite element method]] (SFEM), [[Meshfree methods|meshfree finite element method]], [[Discontinuous Galerkin Method|discontinuous Galerkin finite element method]] (DGFEM), [[Element-Free Galerkin Method]] (EFGM), [[Interpolating Element-Free Galerkin Method]] (IEFGM), etc.&lt;br /&gt;
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The three most widely used numerical methods to solve PDEs are the finite element method (FEM), finite volume methods (FVM) and finite difference methods (FDM), as well other kind of methods called Meshfree methods, which were made to solve problems where the before mentioned methods are limited. The FEM has a prominent position among these methods and especially its exceptionally efficient higher-order version hp-FEM. Other hybrid versions of FEM and Meshfree methods include the generalized finite element method (GFEM), extended finite element method (XFEM), spectral finite element method (SFEM), meshfree finite element method, discontinuous Galerkin finite element method (DGFEM), Element-Free Galerkin Method (EFGM), Interpolating Element-Free Galerkin Method (IEFGM), etc.&lt;br /&gt;
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求解偏微分方程最常用的三种数值方法是有限元分析法、有限体积法和有限差分法，以及其他一些称为无网格法的方法。这些方法用于解决前面提到的方法受到的限制。在这些方法中，有限元方法，尤其是高效的高阶有限元方法，占有重要地位。其他有限元法和无网格法的混合形式包括广义有限元分析法(GFEM)、扩展有限元分析法(XFEM)、谱有限元分析法(SFEM)、无网格有限元分析法(DGFEM)、间断伽辽金有限元分析法(DGFEM)、无网格伽辽金法(EFGM)、插值无网格伽辽金法(IEFGM)等。&lt;br /&gt;
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=== Finite element method ===&lt;br /&gt;
有限元分析法&lt;br /&gt;
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{{main|Finite element method}}&lt;br /&gt;
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The finite element method (FEM) (its practical application often known as finite element analysis (FEA)) is a numerical technique for finding approximate solutions of partial differential equations (PDE) as well as of integral equations. The solution approach is based either on eliminating the differential equation completely (steady state problems), or rendering the PDE into an approximating system of ordinary differential equations, which are then numerically integrated using standard techniques such as Euler's method, Runge–Kutta, etc.&lt;br /&gt;
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The finite element method (FEM) (its practical application often known as finite element analysis (FEA)) is a numerical technique for finding approximate solutions of partial differential equations (PDE) as well as of integral equations. The solution approach is based either on eliminating the differential equation completely (steady state problems), or rendering the PDE into an approximating system of ordinary differential equations, which are then numerically integrated using standard techniques such as Euler's method, Runge–Kutta, etc.&lt;br /&gt;
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'''&amp;lt;font color = &amp;quot;#ff8000&amp;quot;&amp;gt;有限元分析法 Finite Element Method&amp;lt;/font&amp;gt;''' ((其实际应用通常被称为有限元分析(FEA))是一种寻找偏微分方程(PDE)和积分方程近似解的数值技术。这种求解方法要么基于完全消除微分方程(稳态问题) ，要么将偏微分方程转化为常微分方程的近似系统，然后使用标准技术进行数值积分，如欧拉方法、 Runge-Kutta 等。&lt;br /&gt;
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===Finite difference method===&lt;br /&gt;
有限差分法&lt;br /&gt;
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{{main|Finite difference method}}&lt;br /&gt;
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Finite-difference methods are numerical methods for approximating the solutions to differential equations using [[finite difference]] equations to approximate derivatives.&lt;br /&gt;
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Finite-difference methods are numerical methods for approximating the solutions to differential equations using finite difference equations to approximate derivatives.&lt;br /&gt;
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有限差分法是一种数值方法，用差分方程近似微分方程的解。&lt;br /&gt;
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=== Finite volume method ===&lt;br /&gt;
有限体积法&lt;br /&gt;
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{{main|Finite volume method}}&lt;br /&gt;
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Similar to the finite difference method or finite element method, values are calculated at discrete places on a meshed geometry. &amp;quot;Finite volume&amp;quot; refers to the small volume surrounding each node point on a mesh. In the finite volume method, surface integrals in a partial differential equation that contain a divergence term are converted to volume integrals, using the [[divergence theorem]]. These terms are then evaluated as fluxes at the surfaces of each finite volume. Because the flux entering a given volume is identical to that leaving the adjacent volume, these methods conserve mass by design.&lt;br /&gt;
&lt;br /&gt;
Similar to the finite difference method or finite element method, values are calculated at discrete places on a meshed geometry. &amp;quot;Finite volume&amp;quot; refers to the small volume surrounding each node point on a mesh. In the finite volume method, surface integrals in a partial differential equation that contain a divergence term are converted to volume integrals, using the divergence theorem. These terms are then evaluated as fluxes at the surfaces of each finite volume. Because the flux entering a given volume is identical to that leaving the adjacent volume, these methods conserve mass by design.&lt;br /&gt;
&lt;br /&gt;
类似于有限差分法或有限元分析，函数值是在网状几何体上的离散位置进行计算的。“有限体积”是指网格上每个节点周围的小体积。在有限体积法中，偏微分方程中含有散度项的面积分用散度定理积分转换成体积分。然后将这些项用于估算每个有限体积表面上的通量。由于进入给定体积的通量与转移到相邻体积元的通量相同，所以这些方法在设计上保证了质量守恒。&lt;br /&gt;
&lt;br /&gt;
==See also==&lt;br /&gt;
请参阅&lt;br /&gt;
* [[Dirichlet boundary condition]]&lt;br /&gt;
狄利克雷边界条件&lt;br /&gt;
* [[Jet bundle]]&lt;br /&gt;
射流丛&lt;br /&gt;
* [[Laplace transform applied to differential equations]]&lt;br /&gt;
微分方程中的拉普拉斯变换&lt;br /&gt;
* [[List of dynamical systems and differential equations topics]]&lt;br /&gt;
动力学系统和微分方程的列表&lt;br /&gt;
* [[Matrix differential equation]]&lt;br /&gt;
矩阵微分方程&lt;br /&gt;
* [[Neumann boundary condition]]&lt;br /&gt;
诺伊曼边界条件&lt;br /&gt;
* [[Numerical partial differential equations]]&lt;br /&gt;
数值偏微分方程&lt;br /&gt;
* [[Partial differential algebraic equation]]&lt;br /&gt;
偏微分代数方程&lt;br /&gt;
* [[Recurrence relation]]&lt;br /&gt;
递推关系&lt;br /&gt;
* [[Robin boundary condition]]&lt;br /&gt;
罗宾边界条件&lt;br /&gt;
* [[Stochastic processes and boundary value problems]]&lt;br /&gt;
随机过程和边值问题&lt;br /&gt;
&lt;br /&gt;
== The energy method ==&lt;br /&gt;
能量法&lt;br /&gt;
&lt;br /&gt;
The energy method is a mathematical procedure that can be used to verify well-posedness of initial-boundary-value-problems.&amp;lt;ref&amp;gt;{{cite book |title=High Order Difference Methods for Time Dependent PDE&lt;br /&gt;
&lt;br /&gt;
The energy method is a mathematical procedure that can be used to verify well-posedness of initial-boundary-value-problems.&amp;lt;ref&amp;gt;{{cite book |title=High Order Difference Methods for Time Dependent PDE&lt;br /&gt;
&lt;br /&gt;
能量法是验证初边值问题适定性的一种数学方法。 时变偏微分方程的高阶差分方法&lt;br /&gt;
&lt;br /&gt;
|first=Bertil|last=Gustafsson|publisher=Springer|year=2008|isbn=978-3-540-74992-9|doi=10.1007/978-3-540-74993-6}}&amp;lt;/ref&amp;gt; In the following example the energy method is used to decide where and which boundary conditions should be imposed such that the resulting IBVP is well-posed. Consider the one-dimensional hyperbolic PDE given by&lt;br /&gt;
&lt;br /&gt;
|first=Bertil|last=Gustafsson|publisher=Springer|year=2008|isbn=978-3-540-74992-9|doi=10.1007/978-3-540-74993-6}}&amp;lt;/ref&amp;gt; In the following example the energy method is used to decide where and which boundary conditions should be imposed such that the resulting IBVP is well-posed. Consider the one-dimensional hyperbolic PDE given by&lt;br /&gt;
&lt;br /&gt;
| first Bertil | last Gustafsson | publisher | Springer | year 2008 | isbn 978-3-540-74992-9 | doi 10.1007 / 978-3-540-74993-6} / ref 在下面的例子中，使用能量方法来决定应该施加哪些边界条件，使得得到的 IBVP适定。考虑一维双曲偏微分方程&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt;\frac{\partial u}{\partial t} + \alpha \frac{\partial u}{\partial x} = 0, \quad x \in [a,b], \operatorname t &amp;gt; 0,&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;\frac{\partial u}{\partial t} + \alpha \frac{\partial u}{\partial x} = 0, \quad x \in [a,b], \operatorname t &amp;gt; 0,&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
where &amp;lt;math&amp;gt;\alpha \neq 0&amp;lt;/math&amp;gt; is a constant and &amp;lt;math&amp;gt;u(x,t)&amp;lt;/math&amp;gt; is an unknown function with initial condition &amp;lt;math&amp;gt;u(x,0) = f(x)&amp;lt;/math&amp;gt;. Multiplying with &amp;lt;math&amp;gt;u&amp;lt;/math&amp;gt; and integrating over the domain gives&lt;br /&gt;
&lt;br /&gt;
where &amp;lt;math&amp;gt;\alpha \neq 0&amp;lt;/math&amp;gt; is a constant and &amp;lt;math&amp;gt;u(x,t)&amp;lt;/math&amp;gt; is an unknown function with initial condition &amp;lt;math&amp;gt;u(x,0) = f(x)&amp;lt;/math&amp;gt;. Multiplying with &amp;lt;math&amp;gt;u&amp;lt;/math&amp;gt; and integrating over the domain gives&lt;br /&gt;
&lt;br /&gt;
其中 &amp;lt;math&amp;gt;\alpha \neq 0&amp;lt;/math&amp;gt; 是常数，并且 &amp;lt;math&amp;gt;u(x,t)&amp;lt;/math&amp;gt; 是未知函数，初始条件是 &amp;lt;math&amp;gt;u(x,0) = f(x)&amp;lt;/math&amp;gt;。乘以 &amp;lt;math&amp;gt;u&amp;lt;/math&amp;gt; 并在域上进行积分。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt;\int_a^b u \frac{\partial u}{\partial t} \operatorname dx + \alpha \int _a ^b u \frac{\partial u}{\partial x} \operatorname dx = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;\int_a^b u \frac{\partial u}{\partial t} \operatorname dx + \alpha \int _a ^b u \frac{\partial u}{\partial x} \operatorname dx = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Using that&lt;br /&gt;
&lt;br /&gt;
Using that&lt;br /&gt;
&lt;br /&gt;
利用这一点&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt;\int _a ^b u \frac{\partial u}{\partial t} \operatorname dx = \frac{1}{2} \frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 \quad \text{and} \quad \int _a ^b u \frac{\partial u}{\partial x} \operatorname dx = \frac{1}{2} u(b,t)^2 - \frac{1}{2} u(a,t)^2,.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;\int _a ^b u \frac{\partial u}{\partial t} \operatorname dx = \frac{1}{2} \frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 \quad \text{and} \quad \int _a ^b u \frac{\partial u}{\partial x} \operatorname dx = \frac{1}{2} u(b,t)^2 - \frac{1}{2} u(a,t)^2,.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
where integration by parts has been used for the second relationship, we get&lt;br /&gt;
&lt;br /&gt;
where integration by parts has been used for the second relationship, we get&lt;br /&gt;
&lt;br /&gt;
第二个关系中采用了分部积分法，我们可以得到&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt;\frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 + \alpha u(b,t)^2 - \alpha u(a,t)^2 = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;\frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 + \alpha u(b,t)^2 - \alpha u(a,t)^2 = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Here &amp;lt;math&amp;gt;\vert \vert \cdot \vert \vert&amp;lt;/math&amp;gt; denotes the standard L2-norm.&lt;br /&gt;
&lt;br /&gt;
Here &amp;lt;math&amp;gt;\vert \vert \cdot \vert \vert&amp;lt;/math&amp;gt; denotes the standard L2-norm.&lt;br /&gt;
&lt;br /&gt;
在这里，&amp;lt;math&amp;gt;\vert \vert \cdot \vert \vert&amp;lt;/math&amp;gt; 表示标准的 L2-正则。&lt;br /&gt;
&lt;br /&gt;
For well-posedness we require that the energy of the solution is non-increasing, i.e. that &amp;lt;math&amp;gt;\frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 \leq 0&amp;lt;/math&amp;gt;, which is achieved by specifying &amp;lt;math&amp;gt;u&amp;lt;/math&amp;gt; at &amp;lt;math&amp;gt;x = a&amp;lt;/math&amp;gt; if &amp;lt;math&amp;gt;\alpha &amp;gt; 0&amp;lt;/math&amp;gt; and at &amp;lt;math&amp;gt;x = b&amp;lt;/math&amp;gt; if &amp;lt;math&amp;gt;\alpha &amp;lt; 0&amp;lt;/math&amp;gt;. This corresponds to only imposing boundary conditions at the inflow. Note that well-posedness allows for growth in terms of data (initial and boundary) and thus it is sufficient to show that &amp;lt;math&amp;gt;\frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 \leq 0&amp;lt;/math&amp;gt; holds when all data is set to zero.&lt;br /&gt;
&lt;br /&gt;
For well-posedness we require that the energy of the solution is non-increasing, i.e. that &amp;lt;math&amp;gt;\frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 \leq 0&amp;lt;/math&amp;gt;, which is achieved by specifying &amp;lt;math&amp;gt;u&amp;lt;/math&amp;gt; at &amp;lt;math&amp;gt;x = a&amp;lt;/math&amp;gt; if &amp;lt;math&amp;gt;\alpha &amp;gt; 0&amp;lt;/math&amp;gt; and at &amp;lt;math&amp;gt;x = b&amp;lt;/math&amp;gt; if &amp;lt;math&amp;gt;\alpha &amp;lt; 0&amp;lt;/math&amp;gt;. This corresponds to only imposing boundary conditions at the inflow. Note that well-posedness allows for growth in terms of data (initial and boundary) and thus it is sufficient to show that &amp;lt;math&amp;gt;\frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 \leq 0&amp;lt;/math&amp;gt; holds when all data is set to zero.&lt;br /&gt;
&lt;br /&gt;
对于适定性，我们要解的能量是不增加的，即 &amp;lt;math&amp;gt;\frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 \leq 0&amp;lt;/math&amp;gt; ，这种关系可以通过在&amp;lt;math&amp;gt;x = a&amp;lt;/math&amp;gt;处 （如果 &amp;lt;math&amp;gt;\alpha &amp;gt; 0&amp;lt;/math&amp;gt;） 以及 &amp;lt;math&amp;gt;x = b&amp;lt;/math&amp;gt;处 （如果 &amp;lt;math&amp;gt;\alpha &amp;lt; 0&amp;lt;/math&amp;gt;）指定&amp;lt;math&amp;gt;u&amp;lt;/math&amp;gt;的值来实现。这只相当于在入流处附加边界条件。注意，适定性允许在数据(初始和边界)上的增长，因此它足以表明当所有数据设置为零时应有 &amp;lt;math&amp;gt;\frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 \leq 0&amp;lt;/math&amp;gt;。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==[[用户:Yuling|Yuling]]（[[用户讨论:Yuling|讨论]]）“This corresponds to only imposing boundary conditions at the inflow.” 这句话中的inflow不是很理解&lt;br /&gt;
&lt;br /&gt;
==Notes==&lt;br /&gt;
&lt;br /&gt;
{{Reflist}}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
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* {{cite book |title=High Order Difference Methods for Time Dependent PDE&lt;br /&gt;
&lt;br /&gt;
|first=Bertil|last=Gustafsson|publisher=Springer|year=2008|isbn=978-3-540-74992-9|doi=10.1007/978-3-540-74993-6}}&lt;br /&gt;
&lt;br /&gt;
|first=Bertil|last=Gustafsson|publisher=Springer|year=2008|isbn=978-3-540-74992-9|doi=10.1007/978-3-540-74993-6}}&lt;br /&gt;
&lt;br /&gt;
| first Bertil | last Gustafsson | Springer | year 2008 | isbn 978-3-540-74992-9 | doi 10.1007 / 978-3-540-74993-6}&lt;br /&gt;
&lt;br /&gt;
{{refend}}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
== Further reading ==&lt;br /&gt;
&lt;br /&gt;
* {{Cite journal|last=Cajori|first=Florian|authorlink=Florian Cajori|year=1928|title=The Early History of Partial Differential Equations and of Partial Differentiation and Integration|url=http://www.math.harvard.edu/archive/21a_fall_14/exhibits/cajori/cajori.pdf|journal=The American Mathematical Monthly|volume=35|issue=9|pages=459–467|doi=10.2307/2298771|access-date=2016-05-15|archive-url=https://web.archive.org/web/20181123102253/http://www.math.harvard.edu/archive/21a_fall_14/exhibits/cajori/cajori.pdf|archive-date=2018-11-23|url-status=dead}}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
== External links ==&lt;br /&gt;
&lt;br /&gt;
{{Sister project links| wikt=no | commons=Category:Solutions of PDE | b=Partial Differential Equations | n=no | q=Partial differential equation | s=no | v=no | voy=no | species=no | d=no}}&lt;br /&gt;
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* {{springer|title=Differential equation, partial|id=p/d031920}}&lt;br /&gt;
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* [http://eqworld.ipmnet.ru/en/pde-en.htm Partial Differential Equations: Exact Solutions] at EqWorld: The World of Mathematical Equations.&lt;br /&gt;
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* [http://eqworld.ipmnet.ru/en/solutions/eqindex/eqindex-pde.htm Partial Differential Equations: Index] at EqWorld: The World of Mathematical Equations.&lt;br /&gt;
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* [http://eqworld.ipmnet.ru/en/methods/meth-pde.htm Partial Differential Equations: Methods] at EqWorld: The World of Mathematical Equations.&lt;br /&gt;
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* [https://web.archive.org/web/20170701144823/http://www.exampleproblems.com/wiki/index.php?title=Partial_Differential_Equations Example problems with solutions] at exampleproblems.com&lt;br /&gt;
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* [http://mathworld.wolfram.com/PartialDifferentialEquation.html Partial Differential Equations] at mathworld.wolfram.com&lt;br /&gt;
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* [https://reference.wolfram.com/language/FEMDocumentation/tutorial/SolvingPDEwithFEM.html Partial Differential Equations] with Mathematica&lt;br /&gt;
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* [http://www.mathworks.com/moler/pdes.pdf Partial Differential Equations] in Cleve Moler: Numerical Computing with MATLAB&lt;br /&gt;
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* [http://www.nag.com/numeric/fl/nagdoc_fl24/html/D03/d03intro.html Partial Differential Equations] at nag.com&lt;br /&gt;
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* {{cite web |first=Grant |last=Sanderson |title=But what is a partial differential equation? |work=3Blue1Brown |date=April 21, 2019 |url=https://www.youtube.com/watch?v=ly4S0oi3Yz8&amp;amp;list=PLZHQObOWTQDNPOjrT6KVlfJuKtYTftqH6 |via=[[YouTube]] }}&lt;br /&gt;
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[[Category:Partial differential equations| ]]&lt;br /&gt;
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[[Category:Multivariable calculus]]&lt;br /&gt;
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[[Category:Differential equations]]&lt;br /&gt;
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Category:Differential equations&lt;br /&gt;
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类别: 微分方程&lt;br /&gt;
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&amp;lt;small&amp;gt;This page was moved from [[wikipedia:en:Partial differential equation]]. Its edit history can be viewed at [[偏微分方程/edithistory]]&amp;lt;/small&amp;gt;&amp;lt;/noinclude&amp;gt;&lt;br /&gt;
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[[Category:待整理页面]]&lt;/div&gt;</summary>
		<author><name>Ruili</name></author>
	</entry>
	<entry>
		<id>https://wiki.swarma.org/index.php?title=%E5%81%8F%E5%BE%AE%E5%88%86%E6%96%B9%E7%A8%8B&amp;diff=18294</id>
		<title>偏微分方程</title>
		<link rel="alternate" type="text/html" href="https://wiki.swarma.org/index.php?title=%E5%81%8F%E5%BE%AE%E5%88%86%E6%96%B9%E7%A8%8B&amp;diff=18294"/>
		<updated>2020-11-13T14:27:00Z</updated>

		<summary type="html">&lt;p&gt;Ruili：&lt;/p&gt;
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&lt;div&gt;此词条暂由Yuling翻译，未经人工整理和审校，带来阅读不便，请见谅。&lt;br /&gt;
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[[File:Heat.gif|thumb|right|A visualisation of a solution to the two-dimensional [[heat equation]] with temperature represented by the third dimension]]&lt;br /&gt;
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A visualisation of a solution to the two-dimensional [[heat equation with temperature represented by the third dimension]]&lt;br /&gt;
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以三维表示温度的二维热方程解的可视化&lt;br /&gt;
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In [[mathematics]], a '''partial differential equation''' ('''PDE''') is a [[differential equation]] that contains unknown [[Multivariable calculus|multivariable functions]] and their [[partial derivative]]s. PDEs are used to formulate problems involving functions of several variables, and are either solved by hand, or used to create a [[computer model]]. A special case is [[ordinary differential equation]]s (ODEs), which deal with functions of a single variable and their derivatives.&lt;br /&gt;
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In mathematics, a partial differential equation (PDE) is a differential equation that contains unknown multivariable functions and their partial derivatives. PDEs are used to formulate problems involving functions of several variables, and are either solved by hand, or used to create a computer model. A special case is ordinary differential equations (ODEs), which deal with functions of a single variable and their derivatives.&lt;br /&gt;
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在数学中，'''&amp;lt;font color = &amp;quot;#ff8000&amp;quot;&amp;gt; 偏微分方程函数 Partial Differential Equation&amp;lt;/font&amp;gt;'''是包含未知多元函数及其偏导数的微分方程。偏微分方程用于描述涉及多元函数的问题，可以通过人为求解，也可以通过建立计算机模型来求解。常微分方程是偏微分方程一种特殊情况，它处理的是一元函数及其导数。&lt;br /&gt;
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PDEs can be used to describe a wide variety of phenomena such as sound, heat, [[diffusion]], [[electrostatics]], [[Electromagnetism|electrodynamics]], [[fluid dynamics]], [[Elasticity (physics)|elasticity]], [[gravitation]] and [[quantum mechanics]]. These seemingly distinct physical phenomena can be formalised similarly in terms of PDEs. Just as ordinary differential equations often model one-dimensional [[dynamical system]]s, partial differential equations often model [[multidimensional system]]s. PDEs find their generalisation in [[stochastic partial differential equation]]s.&lt;br /&gt;
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PDEs can be used to describe a wide variety of phenomena such as sound, heat, diffusion, electrostatics, electrodynamics, fluid dynamics, elasticity, gravitation and quantum mechanics. These seemingly distinct physical phenomena can be formalised similarly in terms of PDEs. Just as ordinary differential equations often model one-dimensional dynamical systems, partial differential equations often model multidimensional systems. PDEs find their generalisation in stochastic partial differential equations.&lt;br /&gt;
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偏微分方程可以用来描述各种各样的物理现象，如声音，热量，扩散，静电，电动力学，流体力学，弹性力学，重力和量子力学。这些看起来截然不同的物理现象却可以用类似的偏微分方程来描述。正如常微分方程经常对一维动力系统进行建模一样，偏微分方程经常对多维系统进行建模。随机偏微分方程是偏微分方程的一种推广。&lt;br /&gt;
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== Introduction ==&lt;br /&gt;
引言&lt;br /&gt;
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Partial differential equations (PDEs) are equations that involve rates of change with respect to [[continuous variables]]. For example, the position of a [[rigid body]] is specified by six parameters,&amp;lt;ref&amp;gt;{{Cite book|url=https://books.google.com/books?id=v9PLbcYd9aUC&amp;amp;pg=PA32|title=Modelling and Control of Robot Manipulators|last=Sciavicco|first=Lorenzo|last2=Siciliano|first2=Bruno|date=2001-02-19|publisher=Springer Science &amp;amp; Business Media|isbn=9781852332211|language=en}}&amp;lt;/ref&amp;gt; but the configuration of a [[fluid]] is given by the [[continuous distribution]] of several parameters, such as the [[temperature]], [[pressure]], and so forth. The dynamics for the rigid body take place in a finite-dimensional [[Configuration space (physics)|configuration space]]; the dynamics for the fluid occur in an infinite-dimensional configuration space. This distinction usually makes PDEs much harder to solve than ordinary differential equations (ODEs), but here again, there will be simple solutions for linear problems. Classic domains where PDEs are used include [[acoustics]], [[fluid dynamics]], [[electrodynamics]], and [[heat transfer]].&lt;br /&gt;
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Partial differential equations (PDEs) are equations that involve rates of change with respect to continuous variables. For example, the position of a rigid body is specified by six parameters, but the configuration of a fluid is given by the continuous distribution of several parameters, such as the temperature, pressure, and so forth. The dynamics for the rigid body take place in a finite-dimensional configuration space; the dynamics for the fluid occur in an infinite-dimensional configuration space. This distinction usually makes PDEs much harder to solve than ordinary differential equations (ODEs), but here again, there will be simple solutions for linear problems. Classic domains where PDEs are used include acoustics, fluid dynamics, electrodynamics, and heat transfer.&lt;br /&gt;
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偏微分方程(简称为PDEs)涉及到方程相对于连续变量的变化率。例如，刚体的位置是由六个参数确定的，而流体的状态是由几个参数的连续分布给出的，如温度、压力等。刚体的动力学过程发生在有限维状态空间中，流体的动力学过程发生在无限维状态空间中。这种区别通常使偏微分方程比常微分方程更难求解，但是线性问题仍然有简单的求解方式。使用偏微分方程的经典领域包括声学、流体力学、电动力学和传热学。&lt;br /&gt;
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A partial differential equation (PDE) for the function {{math|''u''(''x''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;,… ''x&amp;lt;sub&amp;gt;n&amp;lt;/sub&amp;gt;'')}} is an equation of the form&lt;br /&gt;
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A partial differential equation (PDE) for the function  is an equation of the form&lt;br /&gt;
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函数 {{math|''u''(''x''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;,… ''x&amp;lt;sub&amp;gt;n&amp;lt;/sub&amp;gt;'')}} 的偏微分方程形式是：&lt;br /&gt;
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: &amp;lt;math&amp;gt;f \left (x_1, \ldots x_n; u, \frac{\partial u}{\partial x_1}, \ldots \frac{\partial u}{\partial x_n}; \frac{\partial^2 u}{\partial x_1 \partial x_1}, \ldots \frac{\partial^2 u}{\partial x_1 \partial x_n}; \ldots \right) = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;f \left (x_1, \ldots x_n; u, \frac{\partial u}{\partial x_1}, \ldots \frac{\partial u}{\partial x_n}; \frac{\partial^2 u}{\partial x_1 \partial x_1}, \ldots \frac{\partial^2 u}{\partial x_1 \partial x_n}; \ldots \right) = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
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If {{mvar|f}} is a [[linear function]] of {{mvar|u}} and its derivatives, then the PDE is called linear. Common examples of linear PDEs include the [[heat equation]], the [[wave equation]], [[Laplace's equation]], [[Helmholtz equation]], [[Klein–Gordon equation]], and [[Poisson's equation]].&lt;br /&gt;
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If  is a linear function of  and its derivatives, then the PDE is called linear. Common examples of linear PDEs include the heat equation, the wave equation, Laplace's equation, Helmholtz equation, Klein–Gordon equation, and Poisson's equation.&lt;br /&gt;
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如果 {{mvar|f}} 是函数 {{math|''u''}} 及其导数的线性函数，则偏微分方程称为线性函数。线性偏微分方程的常见例子包括热方程、波动方程、拉普拉斯方程、亥姆霍兹方程方程、克莱因-高登方程和泊松方程。&lt;br /&gt;
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A relatively simple PDE is&lt;br /&gt;
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A relatively simple PDE is&lt;br /&gt;
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一个相对简单的偏微分方程：&lt;br /&gt;
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: &amp;lt;math&amp;gt;\frac{\partial u}{\partial x}(x,y) = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;\frac{\partial u}{\partial x}(x,y) = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
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This relation [[Logical implication|implies]] that the function {{math|''u''(''x'',''y'')}} is independent of {{mvar|x}}. However, the equation gives no information on the function's dependence on the variable {{mvar|y}}. Hence the general solution of this equation is&lt;br /&gt;
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This relation implies that the function  is independent of . However, the equation gives no information on the function's dependence on the variable . Hence the general solution of this equation is&lt;br /&gt;
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这意味着函数 {{math|''u''(''x'',''y'')}} 独立于 {{mvar|x}} 的。然而，这个方程没有给出关于函数和自变量的相关性的信息。因此，这个方程的通解是&lt;br /&gt;
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: &amp;lt;math&amp;gt;u(x,y) = f(y),&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;u(x,y) = f(y),&amp;lt;/math&amp;gt;&lt;br /&gt;
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where {{mvar|f}} is an arbitrary function of {{mvar|y}}. The analogous ordinary differential equation is&lt;br /&gt;
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where  is an arbitrary function of . The analogous ordinary differential equation is&lt;br /&gt;
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其中， {{mvar|f}} 是 {{mvar|y}} 的任意函数。&lt;br /&gt;
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类似的常微分方程是：&lt;br /&gt;
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: &amp;lt;math&amp;gt;\frac{\mathrm{d} u}{\mathrm{d} x}(x) = 0,&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;\frac{\mathrm{d} u}{\mathrm{d} x}(x) = 0,&amp;lt;/math&amp;gt;&lt;br /&gt;
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which has the solution&lt;br /&gt;
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which has the solution&lt;br /&gt;
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它的解为&lt;br /&gt;
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: &amp;lt;math&amp;gt;u(x) = c,&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;u(x) = c,&amp;lt;/math&amp;gt;&lt;br /&gt;
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where {{mvar|c}} is any [[Constant (mathematics)|constant]] value. These two examples illustrate that general solutions of ordinary differential equations (ODEs) involve arbitrary constants, but solutions of PDEs involve arbitrary functions.&lt;br /&gt;
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where  is any constant value. These two examples illustrate that general solutions of ordinary differential equations (ODEs) involve arbitrary constants, but solutions of PDEs involve arbitrary functions.&lt;br /&gt;
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这里，{{mvar|c}} 是一个任意常量。&lt;br /&gt;
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这两个例子说明常微分方程的一般解包含任意常数，但偏微分方程的解包含任意函数。&lt;br /&gt;
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A solution of a PDE is generally not [[Uniqueness quantification|unique]]; additional conditions must generally be specified on the [[Boundary (topology)|boundary]] of the region where the solution is defined. For instance, in the simple example above, the function {{math|''f''(''y'')}} can be determined if {{mvar|u}} is specified on the line {{math|''x'' {{=}} 0}}.&lt;br /&gt;
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A solution of a PDE is generally not unique; additional conditions must generally be specified on the boundary of the region where the solution is defined. For instance, in the simple example above, the function  can be determined if  is specified on the line  0}}.&lt;br /&gt;
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偏微分方程的解一般不是唯一的; 一般必须在定义解的区域边界上定义附加条件。 例如，在上面的简单示例中，如果在 {{math|''x'' {{=}} 0}} 时确定了 {{mvar|u}} 的值，则可以确定该函数 {{math|''f''(''y'')}}。&lt;br /&gt;
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== Existence and uniqueness ==&lt;br /&gt;
存在性和唯一性&lt;br /&gt;
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Although the issue of existence and uniqueness of solutions of ordinary differential equations has a very satisfactory answer with the [[Picard–Lindelöf theorem]], that is far from the case for partial differential equations. The [[Cauchy–Kowalevski theorem]] states that the [[Cauchy problem]] for any partial differential equation whose coefficients are [[Analytic function|analytic]] in the unknown function and its derivatives, has a locally unique analytic solution. Although this result might appear to settle the existence and uniqueness of solutions, there are examples of linear partial differential equations whose coefficients have derivatives of all orders (which are nevertheless not analytic) but which have no solutions at all: see [[Lewy's example|Lewy (1957)]]. Even if the solution of a partial differential equation exists and is unique, it may nevertheless have undesirable properties.  The mathematical study of these questions is usually in the more powerful context of [[weak solution]]s.&lt;br /&gt;
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Although the issue of existence and uniqueness of solutions of ordinary differential equations has a very satisfactory answer with the Picard–Lindelöf theorem, that is far from the case for partial differential equations. The Cauchy–Kowalevski theorem states that the Cauchy problem for any partial differential equation whose coefficients are analytic in the unknown function and its derivatives, has a locally unique analytic solution. Although this result might appear to settle the existence and uniqueness of solutions, there are examples of linear partial differential equations whose coefficients have derivatives of all orders (which are nevertheless not analytic) but which have no solutions at all: see Lewy (1957). Even if the solution of a partial differential equation exists and is unique, it may nevertheless have undesirable properties.  The mathematical study of these questions is usually in the more powerful context of weak solutions.&lt;br /&gt;
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尽管常微分方程解的存在性和唯一性用'''&amp;lt;font color=&amp;quot;#ff8000&amp;quot;&amp;gt;弗罗贝尼乌斯定理 Picard–Lindelöf Theorem&amp;lt;/font&amp;gt;得到了令人满意的结果，但偏微分方程解的存在性和唯一性却远没有得到解决。'''&amp;lt;font color=&amp;quot;#ff8000&amp;quot;&amp;gt;柯西-科瓦列夫斯基定理 Cauchy–Kowalevski theorem&amp;lt;/font&amp;gt;指出：对于任意系数在未知函数及其导数中解析的偏微分方程，柯西问题存在一个局部唯一的解析解。虽然这个结果似乎解决了解的存在性和唯一性问题，但是存在一些线性偏微分方程-其系数具有所有级数的导数(尽管这些导数不是解析的) ，但是根本没有解: 见 Lewy (1957)。即使偏微分方程的解存在且唯一，它仍然可能具有不可预料的性质。这些问题的数学研究通常是在更有力的弱解的背景下进行的。&lt;br /&gt;
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An example of pathological behavior is the sequence (depending upon {{mvar|n}}) of [[Cauchy problem]]s for the [[Laplace equation]]&lt;br /&gt;
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An example of pathological behavior is the sequence (depending upon ) of Cauchy problems for the Laplace equation&lt;br /&gt;
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反常特征的一个例子是拉普拉斯方程的柯西问题的序列(取决于{{mvar|n}})&lt;br /&gt;
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: &amp;lt;math&amp;gt;\frac{\partial^2 u}{\partial x^2} + \frac{\partial^2 u}{\partial y^2}=0,&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;\frac{\partial^2 u}{\partial x^2} + \frac{\partial^2 u}{\partial y^2}=0,&amp;lt;/math&amp;gt;&lt;br /&gt;
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with [[boundary condition]]s&lt;br /&gt;
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with boundary conditions&lt;br /&gt;
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具有边界条件&lt;br /&gt;
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: &amp;lt;math&amp;gt;\begin{align} u(x,0) &amp;amp;= 0, \\ \frac{\partial u}{\partial y}(x,0) &amp;amp;= \frac{\sin nx}{n}, \end{align}&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;\begin{align} u(x,0) &amp;amp;= 0, \\ \frac{\partial u}{\partial y}(x,0) &amp;amp;= \frac{\sin nx}{n}, \end{align}&amp;lt;/math&amp;gt;&lt;br /&gt;
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where {{mvar|n}} is an integer. The derivative of {{mvar|u}} with respect to {{mvar|y}} approaches zero [[uniform convergence|uniformly]] in {{mvar|x}} as {{mvar|n}} increases, but the solution is&lt;br /&gt;
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where  is an integer. The derivative of  with respect to  approaches zero uniformly in  as  increases, but the solution is&lt;br /&gt;
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其中 {{mvar|n}} 是整数。{{mvar|u}} 关于 {{mvar|y}} 的导数，一致地随着 {{mvar|n}} 的增加而趋于零，但解是&lt;br /&gt;
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: &amp;lt;math&amp;gt;u(x,y) = \frac{\sinh ny \sin nx}{n^2}.&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;u(x,y) = \frac{\sinh ny \sin nx}{n^2}.&amp;lt;/math&amp;gt;&lt;br /&gt;
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This solution approaches infinity if {{mvar|nx}} is not an integer multiple of {{pi}} for any non-zero value of {{mvar|y}}. The Cauchy problem for the Laplace equation is called ''ill-posed'' or ''not [[Well-posed problem|well-posed]]'', since the solution does not continuously depend on the data of the problem. Such ill-posed problems are not usually satisfactory for physical applications.&lt;br /&gt;
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This solution approaches infinity if  is not an integer multiple of  for any non-zero value of . The Cauchy problem for the Laplace equation is called ill-posed or not well-posed, since the solution does not continuously depend on the data of the problem. Such ill-posed problems are not usually satisfactory for physical applications.&lt;br /&gt;
&lt;br /&gt;
对于任何非零的 {{mvar|y}}，如果 {{mvar|nx}} 不是模板 {{pi}} 的整数倍，这个解会接近于无穷大。拉普拉斯方程的柯西问题被称为不适定的（可以译为ill-posed或not well-posed），因为解不是连续地依赖于问题的数据。这种不适定问题通常不能满足物理应用。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The [[Navier–Stokes existence and smoothness|existence of solutions for the Navier–Stokes equations]], a partial differential equation, is part of one of the [[Millennium Prize Problems]].&lt;br /&gt;
&lt;br /&gt;
The existence of solutions for the Navier–Stokes equations, a partial differential equation, is part of one of the Millennium Prize Problems.&lt;br /&gt;
&lt;br /&gt;
偏微分方程”纳维-斯托克斯方程“的解的存在性就是千禧年大奖难题之一的一部分。&lt;br /&gt;
&lt;br /&gt;
== Notation ==&lt;br /&gt;
符号&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
In PDEs, it is common to denote partial derivatives using subscripts. That is:&lt;br /&gt;
&lt;br /&gt;
In PDEs, it is common to denote partial derivatives using subscripts. That is:&lt;br /&gt;
&lt;br /&gt;
在偏微分方程中，通常用下标表示偏导数。例如:&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt;u_x = \frac{\partial u}{\partial x}&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;u_x = \frac{\partial u}{\partial x}&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt;u_{xx} = \frac{\partial^2 u}{\partial x^2} &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;u_{xx} = \frac{\partial^2 u}{\partial x^2} &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt;u_{xy} = \frac{\partial^2 u}{\partial y\, \partial x} = \frac{\partial}{\partial y } \left(\frac{\partial u}{\partial x}\right). &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;u_{xy} = \frac{\partial^2 u}{\partial y\, \partial x} = \frac{\partial}{\partial y } \left(\frac{\partial u}{\partial x}\right). &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Especially in physics, [[del]] or nabla ({{math|∇}}) is often used to denote spatial derivatives, and {{math|''&amp;amp;#x307;u'', ''ü''}} for time derivatives. For example, the [[wave equation]] (mentioned below) can be written as&lt;br /&gt;
&lt;br /&gt;
Especially in physics, del or nabla () is often used to denote spatial derivatives, and  for time derivatives. For example, the wave equation (mentioned below) can be written as&lt;br /&gt;
&lt;br /&gt;
特别是在物理学中，[[del]] 或 nabla ({{math|∇}}) 经常用来表示空间导数和时间导数。例如，波动方程(在下文中提到)可以写成：&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt;\ddot u=c^2\nabla^2u&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt;\ddot u=c^2\nabla^2u&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
or&lt;br /&gt;
&lt;br /&gt;
or&lt;br /&gt;
&lt;br /&gt;
或&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt;\ddot u=c^2\Delta u&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt;\ddot u=c^2\Delta u&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
where {{math|Δ}} is the [[Laplace operator]].&lt;br /&gt;
&lt;br /&gt;
where  is the Laplace operator.&lt;br /&gt;
&lt;br /&gt;
其中，{{math|Δ}} 代表拉普拉斯算子。&lt;br /&gt;
&lt;br /&gt;
== Classification ==&lt;br /&gt;
分类&lt;br /&gt;
&lt;br /&gt;
Some linear, second-order partial differential equations can be classified as [[parabolic partial differential equation|parabolic]], [[hyperbolic partial differential equation|hyperbolic]] and [[elliptic partial differential equation|elliptic]]. Others, such as the [[Euler–Tricomi equation]], have different types in different regions. The classification provides a guide to appropriate initial and boundary conditions and to the smoothness of the solutions.&lt;br /&gt;
&lt;br /&gt;
Some linear, second-order partial differential equations can be classified as parabolic, hyperbolic and elliptic. Others, such as the Euler–Tricomi equation, have different types in different regions. The classification provides a guide to appropriate initial and boundary conditions and to the smoothness of the solutions.&lt;br /&gt;
&lt;br /&gt;
一些线性二阶偏微分方程可分为抛物型方程、双曲型方程和椭圆型方程。其他的方程，如欧拉-特里科米方程，在不同的领域有不同的类型。这种分类有助于选择适当的初始和边界条件以及提高解的平滑性。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
=== Equations of first order ===&lt;br /&gt;
一阶方程&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{{main|First-order partial differential equation}}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
=== Linear equations of second order ===&lt;br /&gt;
二阶线性方程&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Assuming {{math|''u&amp;lt;sub&amp;gt;xy&amp;lt;/sub&amp;gt;'' {{=}} ''u&amp;lt;sub&amp;gt;yx&amp;lt;/sub&amp;gt;''}}, the general linear second-order PDE in two independent variables has the form&lt;br /&gt;
&lt;br /&gt;
Assuming  u&amp;lt;sub&amp;gt;yx&amp;lt;/sub&amp;gt;}}, the general linear second-order PDE in two independent variables has the form&lt;br /&gt;
&lt;br /&gt;
假设 {{math|''u&amp;lt;sub&amp;gt;xy&amp;lt;/sub&amp;gt;'' {{=}} ''u&amp;lt;sub&amp;gt;yx&amp;lt;/sub&amp;gt;''}}，含有两个独立变量的一般线性二阶偏微分方程具有如下形式：&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt;Au_{xx} + 2Bu_{xy} + Cu_{yy} + \cdots \mbox{(lower order terms)} = 0,&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;Au_{xx} + 2Bu_{xy} + Cu_{yy} + \cdots \mbox{(lower order terms)} = 0,&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
where the coefficients {{mvar|A}}, {{mvar|B}}, {{mvar|C}}... may depend upon {{mvar|x}} and {{mvar|y}}. If {{math|''A''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; + ''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; + ''C''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; &amp;gt; 0}} over a region of the {{mvar|xy}}-plane, the PDE is second-order in that region. This form is analogous to the equation for a conic section:&lt;br /&gt;
&lt;br /&gt;
where the coefficients , , ... may depend upon  and . If  over a region of the -plane, the PDE is second-order in that region. This form is analogous to the equation for a conic section:&lt;br /&gt;
&lt;br /&gt;
其中的系数 {{mvar|A}}, {{mvar|B}}, {{mvar|C}}... 一般取决于 {{mvar|x}} 和 {{mvar|y}} 。如果在 {{mvar|xy}}-平面的一个区域上 {{math|''A''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; + ''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; + ''C''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; &amp;gt; 0}}，偏微分方程是二阶的，这种形式类似于圆锥截面的方程:&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt;Ax^2 + 2Bxy + Cy^2 + \cdots = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;Ax^2 + 2Bxy + Cy^2 + \cdots = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
More precisely, replacing {{math|∂&amp;lt;sub&amp;gt;''x''&amp;lt;/sub&amp;gt;}} by {{mvar|X}}, and likewise for other variables (formally this is done by a [[Fourier transform]]), converts a constant-coefficient PDE into a polynomial of the same degree, with the terms of the highest degree (a [[homogeneous polynomial]], here a [[quadratic form]]) being most significant for the classification.&lt;br /&gt;
&lt;br /&gt;
More precisely, replacing  by , and likewise for other variables (formally this is done by a Fourier transform), converts a constant-coefficient PDE into a polynomial of the same degree, with the terms of the highest degree (a homogeneous polynomial, here a quadratic form) being most significant for the classification.&lt;br /&gt;
&lt;br /&gt;
更准确地说，用 {{mvar|X}} 替换 {{math|∂&amp;lt;sub&amp;gt;''x''&amp;lt;/sub&amp;gt;}}，并同样替换其它变量(通常由傅里叶变换完成)，将一个常系数偏微分方程转换成一个相同次数的多项式，最高次数的项(齐次多项式，这里是一个二次形式)对于偏微分方程的分类最为重要。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Just as one classifies [[conic section]]s and quadratic forms into parabolic, hyperbolic, and elliptic based on the [[discriminant]] {{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − 4''AC''}}, the same can be done for a second-order PDE at a given point.  However, the [[discriminant]] in a PDE is given by {{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC''}} due to the convention of the {{mvar|xy}} term being {{math|2''B''}} rather than {{mvar|B}}; formally, the discriminant (of the associated quadratic form) is {{math|(2''B'')&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − 4''AC'' {{=}} 4(''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC'')}}, with the factor of 4 dropped for simplicity.&lt;br /&gt;
&lt;br /&gt;
Just as one classifies conic sections and quadratic forms into parabolic, hyperbolic, and elliptic based on the discriminant , the same can be done for a second-order PDE at a given point.  However, the discriminant in a PDE is given by  due to the convention of the  term being  rather than ; formally, the discriminant (of the associated quadratic form) is  4(B&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − AC)}}, with the factor of 4 dropped for simplicity.&lt;br /&gt;
&lt;br /&gt;
正如人们可以根据判别式 {{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − 4''AC''}} 将圆锥截面和二次型分为抛物型、双曲型和椭圆型一样，对于给定点的二阶偏微分方程也可以这样做。然而，偏微分方程中的判别式 {{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − 4''AC''}} 是根据交叉项的系数{{math|2''B''}} 而不是 {{mvar|B}} 给出的，形式上，判别式(关联二次型)是 {{math|(2''B'')&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − 4''AC'' {{=}} 4(''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC'')}}，为简单起见，去掉了因子4。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
# {{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC'' &amp;lt; 0}} (''[[elliptic partial differential equation]]''): Solutions of [[elliptic partial differential equation|elliptic PDEs]] are as smooth as the coefficients allow, within the interior of the region where the equation and solutions are defined. For example, solutions of [[Laplace's equation]] are analytic within the domain where they are defined, but solutions may assume boundary values that are not smooth. The motion of a fluid at subsonic speeds can be approximated with elliptic PDEs, and the Euler–Tricomi equation is elliptic where {{math|''x'' &amp;lt; 0}}.&lt;br /&gt;
&lt;br /&gt;
  (elliptic partial differential equation): Solutions of elliptic PDEs are as smooth as the coefficients allow, within the interior of the region where the equation and solutions are defined. For example, solutions of Laplace's equation are analytic within the domain where they are defined, but solutions may assume boundary values that are not smooth. The motion of a fluid at subsonic speeds can be approximated with elliptic PDEs, and the Euler–Tricomi equation is elliptic where .&lt;br /&gt;
&lt;br /&gt;
{{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC'' &amp;lt; 0}} (椭圆型微分方程)：在定义方程和解的区域内部，椭圆型偏微分方程的解在系数允许的程度内光滑。例如，拉普拉斯方程的解在它们被定义的区域内是解析的，但可能假设边界值是不光滑的。亚音速流体的运动可以用椭圆型偏微分方程近似，欧拉-特里科米方程在 {{math|''x'' &amp;lt; 0}} 时是椭圆型偏微分方程。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
# {{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC'' {{=}} 0}} (''[[parabolic partial differential equation]]''): Equations that are [[parabolic partial differential equation|parabolic]] at every point can be transformed into a form analogous to the [[heat equation]] by a change of independent variables. Solutions smooth out as the transformed time variable increases. The Euler–Tricomi equation has parabolic type on the line where {{math|''x'' {{=}} 0}}.&lt;br /&gt;
&lt;br /&gt;
  0}} (parabolic partial differential equation): Equations that are parabolic at every point can be transformed into a form analogous to the heat equation by a change of independent variables. Solutions smooth out as the transformed time variable increases. The Euler–Tricomi equation has parabolic type on the line where  0}}.&lt;br /&gt;
&lt;br /&gt;
{{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC'' {{=}} 0}}（抛物型偏微分方程）：在每一点上都是抛物线型的方程可以通过改变自变量从而转化成类似于热方程的形式。随着转换后的时间变量的增加，方程的解变得平滑。欧拉-特里科米方程在特征线 {{math|''x'' {{=}} 0}} 上是抛物线型的。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
# {{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC'' &amp;gt; 0}} (''[[hyperbolic partial differential equation]]''): [[hyperbolic partial differential equation|hyperbolic]] equations retain any discontinuities of functions or derivatives in the initial data. An example is the [[wave equation]]. The motion of a fluid at supersonic speeds can be approximated with hyperbolic PDEs, and the Euler–Tricomi equation is hyperbolic where {{math|''x'' &amp;gt; 0}}.&lt;br /&gt;
&lt;br /&gt;
  (hyperbolic partial differential equation): hyperbolic equations retain any discontinuities of functions or derivatives in the initial data. An example is the wave equation. The motion of a fluid at supersonic speeds can be approximated with hyperbolic PDEs, and the Euler–Tricomi equation is hyperbolic where .&lt;br /&gt;
&lt;br /&gt;
{{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC'' &amp;gt; 0}} (双曲型偏微分方程)：双曲型方程在初始数据中保留了函数或导数的任何不连续性。波动方程就是其中的一个例子。超音速流体的运动可以用双曲型偏微分方程近似，欧拉-特里科米方程在 {{math|''x'' &amp;gt; 0}} 时是双曲型的。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
If there are {{mvar|n}} independent variables {{math|''x''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;, ''x''&amp;lt;sub&amp;gt;2 &amp;lt;/sub&amp;gt;,… ''x''&amp;lt;sub&amp;gt;''n''&amp;lt;/sub&amp;gt;}}, a general linear partial differential equation of second order has the form&lt;br /&gt;
&lt;br /&gt;
If there are  independent variables , a general linear partial differential equation of second order has the form&lt;br /&gt;
&lt;br /&gt;
如果存在 {{mvar|n}} 个自变量 {{math|''x''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;, ''x''&amp;lt;sub&amp;gt;2 &amp;lt;/sub&amp;gt;,… ''x''&amp;lt;sub&amp;gt;''n''&amp;lt;/sub&amp;gt;}}，一般二阶线性偏微分方程的形式是：&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt;L u =\sum_{i=1}^n\sum_{j=1}^n a_{i,j} \frac{\partial^2 u}{\partial x_i \partial x_j} \quad \text{ plus lower-order terms} =0.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;L u =\sum_{i=1}^n\sum_{j=1}^n a_{i,j} \frac{\partial^2 u}{\partial x_i \partial x_j} \quad \text{ plus lower-order terms} =0.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The classification depends upon the signature of the eigenvalues of the coefficient matrix {{math|''a''&amp;lt;sub&amp;gt;''i'',''j''&amp;lt;/sub&amp;gt;}}.&lt;br /&gt;
&lt;br /&gt;
The classification depends upon the signature of the eigenvalues of the coefficient matrix .&lt;br /&gt;
&lt;br /&gt;
这种分类取决于系数矩阵特征值的符号（正负性）。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
# Elliptic: the eigenvalues are all positive or all negative.&lt;br /&gt;
&lt;br /&gt;
 Elliptic: the eigenvalues are all positive or all negative.&lt;br /&gt;
&lt;br /&gt;
椭圆形方程: 特征值全部为正或全部为负。&lt;br /&gt;
&lt;br /&gt;
# Parabolic: the eigenvalues are all positive or all negative, save one that is zero.&lt;br /&gt;
&lt;br /&gt;
 Parabolic: the eigenvalues are all positive or all negative, save one that is zero.&lt;br /&gt;
&lt;br /&gt;
抛物线形方程:除了一个为零值，特征值全部为正或全部为负。&lt;br /&gt;
&lt;br /&gt;
# Hyperbolic: there is only one negative eigenvalue and all the rest are positive, or there is only one positive eigenvalue and all the rest are negative.&lt;br /&gt;
&lt;br /&gt;
 Hyperbolic: there is only one negative eigenvalue and all the rest are positive, or there is only one positive eigenvalue and all the rest are negative.&lt;br /&gt;
&lt;br /&gt;
双曲形方程: 只有一个负特征值，其余的都是正特征值，或者只有一个正特征值，其余的都是负特征值。&lt;br /&gt;
&lt;br /&gt;
# Ultrahyperbolic: there is more than one positive eigenvalue and more than one negative eigenvalue, and there are no zero eigenvalues. There is only a limited theory for ultrahyperbolic equations (Courant and Hilbert, 1962).&lt;br /&gt;
&lt;br /&gt;
 Ultrahyperbolic: there is more than one positive eigenvalue and more than one negative eigenvalue, and there are no zero eigenvalues. There is only a limited theory for ultrahyperbolic equations (Courant and Hilbert, 1962).&lt;br /&gt;
&lt;br /&gt;
超双形方程: 存在多于一个正特征值和多于一个的负特征值，且不存在零特征值。对于超双曲方程，只存在有限的理论(Courant 和 Hilbert，1962)。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
=== Systems of first-order equations and characteristic surfaces ===&lt;br /&gt;
一阶方程组和特征曲面&lt;br /&gt;
&lt;br /&gt;
The classification of partial differential equations can be extended to systems of first-order equations, where the unknown {{mvar|u}} is now a [[Euclidean vector|vector]] with {{mvar|m}} components, and the coefficient matrices {{mvar|A&amp;lt;sub&amp;gt;ν&amp;lt;/sub&amp;gt;}} are {{mvar|m}} by {{mvar|m}} matrices for {{math|''ν'' {{=}} 1, 2,… ''n''}}. The partial differential equation takes the form&lt;br /&gt;
&lt;br /&gt;
The classification of partial differential equations can be extended to systems of first-order equations, where the unknown  is now a vector with  components, and the coefficient matrices  are  by  matrices for  1, 2,… n}}. The partial differential equation takes the form&lt;br /&gt;
&lt;br /&gt;
偏微分方程组的分类可以推广到一阶方程组，其中未知量 {{mvar|u}} 是有 {{mvar|m}} 个分量的向量。对于 {{math|''ν'' {{=}} 1, 2,… ''n''}}，系数矩阵 {{mvar|A&amp;lt;sub&amp;gt;ν&amp;lt;/sub&amp;gt;}} 是 {{mvar|m}} × {{mvar|m}} 的矩阵。偏微分方程形式如下：&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt;Lu = \sum_{\nu=1}^{n} A_\nu \frac{\partial u}{\partial x_\nu} + B=0,&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;Lu = \sum_{\nu=1}^{n} A_\nu \frac{\partial u}{\partial x_\nu} + B=0,&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
where the coefficient matrices {{mvar|A&amp;lt;sub&amp;gt;ν&amp;lt;/sub&amp;gt;}} and the vector {{mvar|B}} may depend upon {{mvar|x}} and {{mvar|u}}. If a [[hypersurface]] {{mvar|S}} is given in the implicit form&lt;br /&gt;
&lt;br /&gt;
where the coefficient matrices  and the vector  may depend upon  and . If a hypersurface  is given in the implicit form&lt;br /&gt;
&lt;br /&gt;
其中系数矩阵 {{mvar|A&amp;lt;sub&amp;gt;ν&amp;lt;/sub&amp;gt;}} 和向量 {{mvar|B}} 可能依赖于 {{mvar|x}} 和 {{mvar|u}}。如果超曲面是以隐式形式给出的&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt;\varphi(x_1, x_2, \ldots x_n)=0,&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;\varphi(x_1, x_2, \ldots x_n)=0,&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
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where {{mvar|φ}} has a non-zero gradient, then {{mvar|S}} is a '''characteristic surface''' for the operator {{mvar|L}} at a given point if the characteristic form vanishes:&lt;br /&gt;
&lt;br /&gt;
where  has a non-zero gradient, then  is a characteristic surface for the operator  at a given point if the characteristic form vanishes:&lt;br /&gt;
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其中存在一个非零的梯度，那么如果特征形式消失，则在给定点上算子的特征曲面形式如下:&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
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: &amp;lt;math&amp;gt;Q\left(\frac{\partial\varphi}{\partial x_1}, \ldots\frac{\partial\varphi}{\partial x_n}\right) =\det\left[\sum_{\nu=1}^nA_\nu \frac{\partial \varphi}{\partial x_\nu}\right]=0.\,&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;Q\left(\frac{\partial\varphi}{\partial x_1}, \ldots\frac{\partial\varphi}{\partial x_n}\right) =\det\left[\sum_{\nu=1}^nA_\nu \frac{\partial \varphi}{\partial x_\nu}\right]=0.\,&amp;lt;/math&amp;gt;&lt;br /&gt;
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The geometric interpretation of this condition is as follows: if data for {{mvar|u}} are prescribed on the surface {{mvar|S}}, then it may be possible to determine the normal derivative of {{mvar|u}} on {{mvar|S}} from the differential equation. If the data on {{mvar|S}} and the differential equation determine the normal derivative of {{mvar|u}} on {{mvar|S}}, then {{mvar|S}} is non-characteristic. If the data on {{mvar|S}} and the differential equation ''do not'' determine the normal derivative of {{mvar|u}} on {{mvar|S}}, then the surface is '''characteristic''', and the differential equation restricts the data on {{mvar|S}}: the differential equation is ''internal'' to {{mvar|S}}.&lt;br /&gt;
&lt;br /&gt;
The geometric interpretation of this condition is as follows: if data for  are prescribed on the surface , then it may be possible to determine the normal derivative of  on  from the differential equation. If the data on  and the differential equation determine the normal derivative of  on , then  is non-characteristic. If the data on  and the differential equation do not determine the normal derivative of  on , then the surface is characteristic, and the differential equation restricts the data on : the differential equation is internal to .&lt;br /&gt;
&lt;br /&gt;
这个条件的几何解释如下: 如果关于 {{mvar|u}} 的数据是在曲面 {{mvar|S}} 上规定的，那么就有可能依据微分方程确定曲面 {{mvar|S}} 上 {{mvar|u}} 的法向导数。如果曲面 {{mvar|S}} 上的数据和上面的微分方程能确定曲面 {{mvar|S}} 上 {{mvar|u}} 的法向导数，那么它就是非特征的。如果曲面 {{mvar|S}} 上的数据和上面的微分方程不能确定曲面 {{mvar|S}} 上 {{mvar|u}} 的法向导数，那么曲面是特征的，并且微分方程将数据限制在曲面 {{mvar|S}} 上：微分方程是在曲面 {{mvar|S}} 内部。&lt;br /&gt;
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# A first-order system {{math|''Lu'' {{=}} 0}} is ''elliptic'' if no surface is characteristic for {{mvar|L}}: the values of {{mvar|u}} on {{mvar|S}} and the differential equation always determine the normal derivative of {{mvar|u}} on {{mvar|S}}.&lt;br /&gt;
&lt;br /&gt;
 A first-order system  0}} is elliptic if no surface is characteristic for : the values of  on  and the differential equation always determine the normal derivative of  on .&lt;br /&gt;
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如果对于 {{mvar|L}} 没有曲面是特征的，则一阶系统 {{math|''Lu'' {{=}} 0}} 是椭圆形的：{{mvar|u}}在 {{mvar|S}} 的值和微分方程总能够决定 {{mvar|S}} 上 {{mvar|u}} 的法向导数。&lt;br /&gt;
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# A first-order system is ''hyperbolic'' at a point if there is a '''spacelike''' surface {{mvar|S}} with normal {{mvar|ξ}} at that point. This means that, given any non-trivial vector {{mvar|η}} orthogonal to {{mvar|ξ}}, and a scalar multiplier {{mvar|λ}}, the equation {{math|''Q''(''λξ'' + ''η'') {{=}} 0}} has {{mvar|m}} real roots {{math|''λ''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;, ''λ''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;,… ''λ''&amp;lt;sub&amp;gt;''m''&amp;lt;/sub&amp;gt;}}. The system is '''strictly hyperbolic''' if these roots are always distinct. The geometrical interpretation of this condition is as follows: the characteristic form {{math|''Q''(''ζ'') {{=}} 0}} defines a cone (the normal cone) with homogeneous coordinates ζ. In the hyperbolic case, this cone has {{mvar|m}} sheets, and the axis {{math|''ζ'' {{=}} ''λξ''}} runs inside these sheets: it does not intersect any of them. But when displaced from the origin by η, this axis intersects every sheet. In the elliptic case, the normal cone has no real sheets.&lt;br /&gt;
&lt;br /&gt;
 A first-order system is hyperbolic at a point if there is a spacelike surface  with normal  at that point. This means that, given any non-trivial vector  orthogonal to , and a scalar multiplier , the equation  0}} has  real roots . The system is strictly hyperbolic if these roots are always distinct. The geometrical interpretation of this condition is as follows: the characteristic form  0}} defines a cone (the normal cone) with homogeneous coordinates ζ. In the hyperbolic case, this cone has  sheets, and the axis  λξ}} runs inside these sheets: it does not intersect any of them. But when displaced from the origin by η, this axis intersects every sheet. In the elliptic case, the normal cone has no real sheets.&lt;br /&gt;
&lt;br /&gt;
如果在该点存在一个法向量为 {{mvar|ξ}}的 '''&amp;lt;font color=&amp;quot;#ff8000&amp;quot;&amp;gt;类空曲面 Spacclike Surface&amp;lt;/font&amp;gt; {{mvar|S}} ，则一阶系统在那一点是双曲的。这意味着，给定任意正交于 {{mvar|ξ}} 的非平凡向量 {{mvar|η}} 和一个标量乘子 {{mvar|λ}}，方程 {{math|''Q''(''λξ'' + ''η'') {{=}} 0}} 有 {{mvar|m}} 个实根 {{math|''λ''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;, ''λ''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;,… ''λ''&amp;lt;sub&amp;gt;''m''&amp;lt;/sub&amp;gt;}}。如果这些根始终不同，则该系统是严格双曲形的。这个条件的几何解释如下: 特征形式 {{math|''Q''(''ζ'') {{=}} 0}} 定义了一个具有齐次坐标 ζ的圆锥(法线圆锥)。在双曲形的情况下，这个圆锥体有 {{mvar|m}} 层，并且轴 {{math|''ζ'' {{=}} ''λξ''}} 在这些层中运动: 它不与任何一层相交。但是当从原点偏离η时，这条轴线与每一层都相交。在椭圆形的情况下，法向圆锥没有实层。&lt;br /&gt;
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==[[用户:Yuling|Yuling]]（[[用户讨论:Yuling|讨论]]） sheet 这个单词也不很理解，我直译为了“层”&lt;br /&gt;
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=== Equations of mixed type ===&lt;br /&gt;
混合型方程&lt;br /&gt;
&lt;br /&gt;
If a PDE has coefficients that are not constant, it is possible that it will not belong to any of these categories but rather be of '''mixed type'''. A simple but important example is the [[Euler–Tricomi equation]]&lt;br /&gt;
&lt;br /&gt;
If a PDE has coefficients that are not constant, it is possible that it will not belong to any of these categories but rather be of mixed type. A simple but important example is the Euler–Tricomi equation&lt;br /&gt;
&lt;br /&gt;
如果偏微分方程的系数不是常数，那么它可能不属于这些类别中的任何一个，而是属于混合类型。一个简单但重要的例子是欧拉-特里科米方程&lt;br /&gt;
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: &amp;lt;math&amp;gt;u_{xx} = xu_{yy},&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;u_{xx} = xu_{yy},&amp;lt;/math&amp;gt;&lt;br /&gt;
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which is called '''elliptic-hyperbolic''' because it is elliptic in the region {{math|''x'' &amp;lt; 0}}, hyperbolic in the region {{math|''x'' &amp;gt; 0}}, and degenerate parabolic on the line {{math|''x'' {{=}} 0}}.&lt;br /&gt;
&lt;br /&gt;
which is called elliptic-hyperbolic because it is elliptic in the region , hyperbolic in the region , and degenerate parabolic on the line  0}}.&lt;br /&gt;
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它在 {{math|''x'' &amp;lt; 0}} 的区域上是椭圆形，在 {{math|''x'' &amp;gt; 0}} 区域上是双曲形，在 {{math|''x'' {{=}} 0}}这条线上是退化为抛物线形，因此称之为椭圆-双曲型。&lt;br /&gt;
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&amp;lt;!--&lt;br /&gt;
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&amp;lt;!--&lt;br /&gt;
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&amp;lt;!--&lt;br /&gt;
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''fill in: Dirichlet and Neumann boundaries, hyperbolic/parabolic/elliptic separation of variables, [[Fourier analysis]], [[Green's function]]s ...--&amp;gt;&lt;br /&gt;
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fill in: Dirichlet and Neumann boundaries, hyperbolic/parabolic/elliptic separation of variables, Fourier analysis, Green's functions ...--&amp;gt;&lt;br /&gt;
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填写: Dirichlet 和 Neumann 边界，双曲 / 抛物线 / 椭圆分离变量法，傅立叶分析，Green 函数... --&lt;br /&gt;
&lt;br /&gt;
=== Infinite-order PDEs in quantum mechanics ===&lt;br /&gt;
量子力学中的无限阶偏微分方程&lt;br /&gt;
&lt;br /&gt;
In the [[phase space formulation]] of quantum mechanics,  one may consider the [[Method of quantum characteristics|quantum Hamilton's equations]] for trajectories of quantum particles. These equations are infinite-order PDEs. However, in the semiclassical expansion, one has a finite system of ODEs at any fixed order of [[Dirac constant|{{mvar|ħ}}]].  The evolution equation of the [[Wigner quasi-probability distribution|c]] is also an infinite-order PDE. The quantum trajectories are [[Method of quantum characteristics|quantum characteristics]], with the use of which one could calculate the evolution of the Wigner function.&lt;br /&gt;
&lt;br /&gt;
In the phase space formulation of quantum mechanics,  one may consider the quantum Hamilton's equations for trajectories of quantum particles. These equations are infinite-order PDEs. However, in the semiclassical expansion, one has a finite system of ODEs at any fixed order of Dirac constant|.  The evolution equation of the Wigner function is also an infinite-order PDE. The quantum trajectories are quantum characteristics, with the use of which one could calculate the evolution of the Wigner function.&lt;br /&gt;
&lt;br /&gt;
在量子力学中的相空间表述中，我们可以考虑用于求解量子粒子的轨迹的量子哈密顿的方程。这些方程是无限阶偏微分方程。然而，在半经典展开中，我们在给定[[Dirac constant|{{mvar|ħ}}]]阶数下有一个有限的的常微分方程组。'''&amp;lt;font color=&amp;quot;#ff8000&amp;quot;&amp;gt;维格纳函数  Wigner Function&amp;lt;/font&amp;gt;的演化方程也是一个无限阶偏微分方程。由于量子轨道的量子特性，所以它通常可以用来计算维格纳函数的演化。&lt;br /&gt;
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== Analytical solutions ==&lt;br /&gt;
解析解&lt;br /&gt;
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===Separation of variables===&lt;br /&gt;
分离变量法&lt;br /&gt;
&lt;br /&gt;
{{main|Separable partial differential equation}}&lt;br /&gt;
&lt;br /&gt;
Linear PDEs can be reduced to systems of ordinary differential equations by the important technique of separation of variables. This technique rests on a characteristic of solutions to differential equations: if one can find any solution that solves the equation and satisfies the boundary conditions, then it is ''the'' solution (this also applies to ODEs). We assume as an [[ansatz]] that the dependence of a solution on the parameters space and time can be written as a product of terms that each depend on a single parameter, and then see if this can be made to solve the problem.&amp;lt;ref&amp;gt;{{cite book|last1=Gershenfeld|first1=Neil|title=The nature of mathematical modeling|date=2000|publisher=Cambridge Univ. Press|location=Cambridge|isbn=0521570956|page=27|edition=Reprinted (with corr.)}}&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
Linear PDEs can be reduced to systems of ordinary differential equations by the important technique of separation of variables. This technique rests on a characteristic of solutions to differential equations: if one can find any solution that solves the equation and satisfies the boundary conditions, then it is the solution (this also applies to ODEs). We assume as an ansatz that the dependence of a solution on the parameters space and time can be written as a product of terms that each depend on a single parameter, and then see if this can be made to solve the problem.&lt;br /&gt;
&lt;br /&gt;
线性偏微分方程组可以通过分离变量法这一重要方法来简化为常微分方程组。这种方法依赖于微分方程解的一个特征: 如果能找到任何一个满足方程和边界条件的解，那么这个解就是方程的解(这也适用于常微分方程)。我们假设解对参数空间和时间的依赖可以写成对它们每一项的依赖以及一个参数的乘积，然后再看看这是否可以用来解决这个问题。&lt;br /&gt;
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In the method of separation of variables, one reduces a PDE to a PDE in fewer variables, which is an ordinary differential equation if in one variable – these are in turn easier to solve.&lt;br /&gt;
&lt;br /&gt;
In the method of separation of variables, one reduces a PDE to a PDE in fewer variables, which is an ordinary differential equation if in one variable – these are in turn easier to solve.&lt;br /&gt;
&lt;br /&gt;
在分离变量法方法中，可以将偏微分方程简化为含有更少变量的偏微分方程，如果只有一个变量，那么就变成了一个'''&amp;lt;font color = &amp;quot;#ff8000&amp;quot;&amp;gt;常微分方程 Ordinary Differential Equation&amp;lt;/font&amp;gt;'''-- 反过来，这些方程也更容易求解。&lt;br /&gt;
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This is possible for simple PDEs, which are called [[separable partial differential equation]]s, and the domain is generally a rectangle (a product of intervals). Separable PDEs correspond to [[diagonal matrices]] – thinking of &amp;quot;the value for fixed {{mvar|x}}&amp;quot; as a coordinate, each coordinate can be understood separately.&lt;br /&gt;
&lt;br /&gt;
This is possible for simple PDEs, which are called separable partial differential equations, and the domain is generally a rectangle (a product of intervals). Separable PDEs correspond to diagonal matrices – thinking of &amp;quot;the value for fixed &amp;quot; as a coordinate, each coordinate can be understood separately.&lt;br /&gt;
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对于简单的偏微分方程(称为可分离偏微分方程)来说，这是可能的，而且方程通常定义在一个矩形区域(区间的乘积)上。可分离偏微分方程对应于对角线矩阵——以“固定值”为坐标，每个坐标可分开理解。&lt;br /&gt;
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This generalizes to the [[method of characteristics]], and is also used in [[integral transform]]s.&lt;br /&gt;
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This generalizes to the method of characteristics, and is also used in integral transforms.&lt;br /&gt;
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这种方法可以推广到特征曲线法，也可以用于积分变换。&lt;br /&gt;
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===Method of characteristics===&lt;br /&gt;
特征曲线法&lt;br /&gt;
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{{main|Method of characteristics}}&lt;br /&gt;
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In special cases, one can find characteristic curves on which the equation reduces to an ODE – changing coordinates in the domain to straighten these curves allows separation of variables, and is called the [[method of characteristics]].&lt;br /&gt;
&lt;br /&gt;
In special cases, one can find characteristic curves on which the equation reduces to an ODE – changing coordinates in the domain to straighten these curves allows separation of variables, and is called the method of characteristics.&lt;br /&gt;
&lt;br /&gt;
在特殊情况下，可以找到一些特征曲线，在这些曲线上方程可以变成一个常微分方程——意味着改变坐标从而使这些曲线变直从而达到分离变量的目的，这就是所谓的特征曲线法。&lt;br /&gt;
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More generally, one may find characteristic surfaces.&lt;br /&gt;
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More generally, one may find characteristic surfaces.&lt;br /&gt;
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更一般地说，人们可能会找到特征表面。&lt;br /&gt;
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===Integral transform===&lt;br /&gt;
积分变换&lt;br /&gt;
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An [[integral transform]] may transform the PDE to a simpler one, in particular, a separable PDE. This corresponds to diagonalizing an operator.&lt;br /&gt;
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An integral transform may transform the PDE to a simpler one, in particular, a separable PDE. This corresponds to diagonalizing an operator.&lt;br /&gt;
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积分变换可以将偏微分方程转换为更简单的偏微分方程，特别是可分离的偏微分方程。这对应于对角化算符。&lt;br /&gt;
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An important example of this is [[Fourier analysis]], which diagonalizes the heat equation using the [[eigenbasis]] of sinusoidal waves.&lt;br /&gt;
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An important example of this is Fourier analysis, which diagonalizes the heat equation using the eigenbasis of sinusoidal waves.&lt;br /&gt;
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这方面的一个重要例子是'''&amp;lt;font color = &amp;quot;#ff8000&amp;quot;&amp;gt;傅里叶分析  Fourier Analysis&amp;lt;/font&amp;gt;'''，它使用正弦波的特征基来对角化热方程。&lt;br /&gt;
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If the domain is finite or periodic, an infinite sum of solutions such as a [[Fourier series]] is appropriate, but an integral of solutions such as a [[Fourier integral]] is generally required for infinite domains. The solution for a point source for the heat equation given above is an example of the use of a Fourier integral.&lt;br /&gt;
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If the domain is finite or periodic, an infinite sum of solutions such as a Fourier series is appropriate, but an integral of solutions such as a Fourier integral is generally required for infinite domains. The solution for a point source for the heat equation given above is an example of the use of a Fourier integral.&lt;br /&gt;
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如果区域是有限的或周期性的，那么解为无限和的形式是恰当的，例如傅里叶级数，但是一个解的积分，例如傅立叶积分，一般是在无限区域上的。上面给出的热传导方程的点源解法就是使用傅里叶积分的一个例子。&lt;br /&gt;
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===Change of variables===&lt;br /&gt;
变量代换&lt;br /&gt;
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Often a PDE can be reduced to a simpler form with a known solution by a suitable [[Change of variables (PDE)|change of variables]].  For example, the [[Black–Scholes equation#Derivation|Black–Scholes]] PDE&lt;br /&gt;
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Often a PDE can be reduced to a simpler form with a known solution by a suitable change of variables.  For example, the Black–Scholes PDE&lt;br /&gt;
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偏微分方程通常可以通过变量的适当变化，用已知的解简化为更简单的形式。例如，布莱克-舒尔斯偏微分方程&lt;br /&gt;
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:&amp;lt;math&amp;gt; \frac{\partial V}{\partial t} + \tfrac{1}{2}\sigma^2 S^2\frac{\partial^2 V}{\partial S^2} + rS\frac{\partial V}{\partial S} - rV = 0 &amp;lt;/math&amp;gt;&lt;br /&gt;
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&amp;lt;math&amp;gt; \frac{\partial V}{\partial t} + \tfrac{1}{2}\sigma^2 S^2\frac{\partial^2 V}{\partial S^2} + rS\frac{\partial V}{\partial S} - rV = 0 &amp;lt;/math&amp;gt;&lt;br /&gt;
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is reducible to the [[heat equation]]&lt;br /&gt;
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is reducible to the heat equation&lt;br /&gt;
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可以简化为热传导方程&lt;br /&gt;
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:&amp;lt;math&amp;gt; \frac{\partial u}{\partial \tau} = \frac{\partial^2 u}{\partial x^2}&amp;lt;/math&amp;gt;&lt;br /&gt;
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&amp;lt;math&amp;gt; \frac{\partial u}{\partial \tau} = \frac{\partial^2 u}{\partial x^2}&amp;lt;/math&amp;gt;&lt;br /&gt;
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by the change of variables (for complete details see {{webarchive |url=https://web.archive.org/web/20080411030405/http://www.math.unl.edu/~sdunbar1/Teaching/MathematicalFinance/Lessons/BlackScholes/Solution/solution.shtml |date=April 11, 2008 |title=Solution of the Black Scholes Equation }})&lt;br /&gt;
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by the change of variables (for complete details see )&lt;br /&gt;
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通过变量替换(完整的细节见)&lt;br /&gt;
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:&amp;lt;math&amp;gt;\begin{align}&lt;br /&gt;
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V(S,t) &amp;amp;= K v(x,\tau),\\[5px]&lt;br /&gt;
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x &amp;amp;= \ln\left(\tfrac{S}{K} \right),\\[5px]&lt;br /&gt;
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\tau &amp;amp;= \tfrac{1}{2} \sigma^2 (T - t),\\[5px]&lt;br /&gt;
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v(x,\tau)&amp;amp;=e^{-\alpha x-\beta\tau} u(x,\tau).&lt;br /&gt;
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\end{align}&amp;lt;/math&amp;gt;&lt;br /&gt;
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===Fundamental solution===&lt;br /&gt;
基本解&lt;br /&gt;
&lt;br /&gt;
{{main|Fundamental solution}}&lt;br /&gt;
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Inhomogeneous equations can often be solved (for constant coefficient PDEs, always be solved) by finding the [[fundamental solution]] (the solution for a point source), then taking the [[convolution]] with the boundary conditions to get the solution.&lt;br /&gt;
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Inhomogeneous equations can often be solved (for constant coefficient PDEs, always be solved) by finding the fundamental solution (the solution for a point source), then taking the convolution with the boundary conditions to get the solution.&lt;br /&gt;
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非齐次方程(常系数偏微分方程)一般是通过先求出基本解(点源的解) ，然后利用带边界条件的卷积来求解。&lt;br /&gt;
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This is analogous in [[signal processing]] to understanding a filter by its [[impulse response]].&lt;br /&gt;
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This is analogous in signal processing to understanding a filter by its impulse response.&lt;br /&gt;
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这类似于在信号处理中通过滤波器的脉冲响应来理解滤波器。&lt;br /&gt;
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===Superposition principle===&lt;br /&gt;
叠加原理&lt;br /&gt;
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{{further| Superposition principle }}&lt;br /&gt;
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The superposition principle applies to any linear system, including linear systems of PDEs. A common visualization of this concept is the interaction of two waves in phase being combined to result in a greater amplitude, for example {{math|sin ''x'' + sin ''x'' {{=}} 2 sin ''x''}}. The same principle can be observed in PDEs where the solutions may be real or complex and additive. [[Superposition principle|superposition]]&lt;br /&gt;
&lt;br /&gt;
The superposition principle applies to any linear system, including linear systems of PDEs. A common visualization of this concept is the interaction of two waves in phase being combined to result in a greater amplitude, for example  2 sin x}}. The same principle can be observed in PDEs where the solutions may be real or complex and additive. superposition&lt;br /&gt;
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'''&amp;lt;font color = &amp;quot;#ff8000&amp;quot;&amp;gt;叠加原理 Superposition Principle&amp;lt;/font&amp;gt;适用于任何线性系统，包括偏微分方程的线性系统。这个概念的一个常见的可视化是两个同相位的波相互作用结合在一起会产生更大的振幅，例如 {{math|sin ''x'' + sin ''x'' {{=}} 2 sin ''x''}}。在偏微分方程中也可以观察到同样的原理，其中的解可能是真实的或复杂的和可加的。叠加&lt;br /&gt;
&lt;br /&gt;
If {{math|''u''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;}} and {{math|''u''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;}} are solutions of linear PDE in some function space {{mvar|R}}, then {{math|''u'' {{=}} ''c''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;''u''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; + ''c''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;''u''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;}} with any constants {{math|''c''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;}} and {{math|''c''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;}} are also a solution of that PDE in the same function space.&lt;br /&gt;
&lt;br /&gt;
If  and  are solutions of linear PDE in some function space , then  c&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;u&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; + c&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;u&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;}} with any constants  and  are also a solution of that PDE in the same function space.&lt;br /&gt;
&lt;br /&gt;
若线性偏微分方程在某个函数空间{{mvar|R}}中有解{{math|''u''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;}} 和 {{math|''u''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;}}，则{{math|''u'' {{=}} ''c''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;''u''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; + ''c''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;''u''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;}}也是该偏微分方程在同一函数空间中的解，其中{{math|''c''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;}} 和 {{math|''c''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;}} 是任意常数。&lt;br /&gt;
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===Methods for non-linear equations===&lt;br /&gt;
非线性方程的求解方法&lt;br /&gt;
{{see also|nonlinear partial differential equation}}&lt;br /&gt;
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There are no generally applicable methods to solve nonlinear PDEs. Still, existence and uniqueness results (such as the [[Cauchy–Kowalevski theorem]]) are often possible, as are proofs of important qualitative and quantitative properties of solutions (getting these results is a major part of [[mathematical analysis|analysis]]). Computational solution to the nonlinear PDEs, the [[split-step method]], exist for specific equations like [[nonlinear Schrödinger equation]].&lt;br /&gt;
&lt;br /&gt;
There are no generally applicable methods to solve nonlinear PDEs. Still, existence and uniqueness results (such as the Cauchy–Kowalevski theorem) are often possible, as are proofs of important qualitative and quantitative properties of solutions (getting these results is a major part of analysis). Computational solution to the nonlinear PDEs, the split-step method, exist for specific equations like nonlinear Schrödinger equation.&lt;br /&gt;
&lt;br /&gt;
对于非线性偏微分方程，目前还没有普遍适用的求解方法。然而，通常是可能知道解的存在性和唯一性(如柯西-科瓦列夫斯基定理)，也是可能得到解的重要定性和定量性质的证明(得到这些结果是分析的主要部分)。非线性偏微分方程的计算解，即分步法，对一些特定的方程适用，比如非线性'''&amp;lt;font color=&amp;quot;#ff8000&amp;quot;&amp;gt;薛定谔方程 Schrödinger equation&amp;lt;/font&amp;gt;'''。&lt;br /&gt;
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Nevertheless, some techniques can be used for several types of equations. The [[h-principle|{{mvar|h}}-principle]] is the most powerful method to solve [[Underdetermined system|underdetermined]] equations. The [[Riquier–Janet theory]] is an effective method for obtaining information about many analytic [[Overdetermined system|overdetermined]] systems.&lt;br /&gt;
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Nevertheless, some techniques can be used for several types of equations. The -principle is the most powerful method to solve underdetermined equations. The Riquier–Janet theory is an effective method for obtaining information about many analytic overdetermined systems.&lt;br /&gt;
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然而，一些技巧可以用于几种类型的方程。h-原理是求解欠定方程最有效的方法。里基尔-珍妮特理论是一种可以获得许多解析超定系统信息的有效方法。&lt;br /&gt;
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The [[method of characteristics]] can be used in some very special cases to solve partial differential equations.&lt;br /&gt;
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The method of characteristics can be used in some very special cases to solve partial differential equations.&lt;br /&gt;
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特征线法可用于求解某些特殊情况下的偏微分方程。&lt;br /&gt;
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In some cases, a PDE can be solved via [[perturbation analysis]] in which the solution is considered to be a correction to an equation with a known solution. Alternatives are [[numerical analysis]] techniques from simple [[finite difference]] schemes to the more mature [[multigrid]] and [[finite element method]]s. Many interesting problems in science and engineering are solved in this way using [[computer]]s, sometimes high performance [[supercomputer]]s.&lt;br /&gt;
&lt;br /&gt;
In some cases, a PDE can be solved via perturbation analysis in which the solution is considered to be a correction to an equation with a known solution. Alternatives are numerical analysis techniques from simple finite difference schemes to the more mature multigrid and finite element methods. Many interesting problems in science and engineering are solved in this way using computers, sometimes high performance supercomputers.&lt;br /&gt;
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在某些情况下，偏微分方程可以通过扰动分析来求解。在扰动分析中，通常是求解将具有已知解的方程修正后的新得到方程。可供选择的数值分析技术从简单的差分格式到更成熟的多重网格和有限元方法。许多有趣的科学和工程问题都是在计算机上用这种方法解决的，有时是高性能超级计算机。&lt;br /&gt;
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===Lie group method===&lt;br /&gt;
李群方法&lt;br /&gt;
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From 1870 [[Sophus Lie]]'s work put the theory of differential equations on a more satisfactory foundation. He showed that the integration theories of the older mathematicians can, by the introduction of what are now called [[Lie group]]s, be referred, to a common source; and that ordinary differential equations which admit the same [[infinitesimal transformation]]s present comparable difficulties of integration. He also emphasized the subject of [[contact transformation|transformations of contact]].&lt;br /&gt;
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From 1870 Sophus Lie's work put the theory of differential equations on a more satisfactory foundation. He showed that the integration theories of the older mathematicians can, by the introduction of what are now called Lie groups, be referred, to a common source; and that ordinary differential equations which admit the same infinitesimal transformations present comparable difficulties of integration. He also emphasized the subject of transformations of contact.&lt;br /&gt;
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从1870年起，索弗斯·李的工作为微分方程理论奠定了一个较为令人满意的基础。他指出，通过引入现在所谓的李群，老一辈数学家的积分理论可以引用到一个共同的来源; 承认相同的无穷小变换的常微分方程在积分方面存在相当的困难。他还强调了接触的转变这一主题。&lt;br /&gt;
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==[[用户:Yuling|Yuling]]（[[用户讨论:Yuling|讨论]]）这句话“He also emphasized the subject of transformations of contact.”中的transformations of contact翻译的不太好。&lt;br /&gt;
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A general approach to solving PDEs uses the symmetry property of differential equations, the continuous [[infinitesimal transformation]]s of solutions to solutions ([[Lie theory]]). Continuous [[group theory]], [[Lie algebras]] and [[differential geometry]] are used to understand the structure of linear and nonlinear partial differential equations for generating integrable equations, to find its [[Lax pair]]s, recursion operators, [[Bäcklund transform]] and finally finding exact analytic solutions to the PDE.&lt;br /&gt;
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A general approach to solving PDEs uses the symmetry property of differential equations, the continuous infinitesimal transformations of solutions to solutions (Lie theory). Continuous group theory, Lie algebras and differential geometry are used to understand the structure of linear and nonlinear partial differential equations for generating integrable equations, to find its Lax pairs, recursion operators, Bäcklund transform and finally finding exact analytic solutions to the PDE.&lt;br /&gt;
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求解偏微分方程的一般方法是利用微分方程的对称性，即解到解的连续无穷小变换(李理论)。连续群论、李代数和微分几何理论被用来理解生成可积方程的线性和非线性偏微分方程的结构，找到它的Lax对、递归算子、 贝克伦德变换，最后找到偏微分方程的精确解析解。&lt;br /&gt;
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Symmetry methods have been recognized to study differential equations arising in mathematics, physics, engineering, and many other disciplines.&lt;br /&gt;
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Symmetry methods have been recognized to study differential equations arising in mathematics, physics, engineering, and many other disciplines.&lt;br /&gt;
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对称方法已被公认可以用于研究出现在数学，物理，工程和许多其他学科的微分方程。&lt;br /&gt;
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===Semianalytical methods===&lt;br /&gt;
半解析方法&lt;br /&gt;
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The [[Adomian decomposition method]], the [[Aleksandr Lyapunov|Lyapunov]] artificial small parameter method, and He's [[homotopy perturbation method]] are all special cases of the more general [[homotopy analysis method]]. These are series expansion methods, and except for the Lyapunov method, are independent of small physical parameters as compared to the well known [[perturbation theory]], thus giving these methods greater flexibility and solution generality.&lt;br /&gt;
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The Adomian decomposition method, the Lyapunov artificial small parameter method, and He's homotopy perturbation method are all special cases of the more general homotopy analysis method. These are series expansion methods, and except for the Lyapunov method, are independent of small physical parameters as compared to the well known perturbation theory, thus giving these methods greater flexibility and solution generality.&lt;br /&gt;
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阿多米安分解法、李雅普诺夫人工小参数方法和何同伦摄动方法都是更一般的同伦分析方法的特殊情况。除了李雅普诺夫方法之外，这些都是级数展开方法，与为人熟知的摄动理论方法相比，它们与小的物理参数无关，因此这些方法具有更大的灵活性和解的通用性。&lt;br /&gt;
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== Numerical solutions ==&lt;br /&gt;
数值解&lt;br /&gt;
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The three most widely used [[Numerical partial differential equations|numerical methods to solve PDEs]] are the [[finite element analysis|finite element method]] (FEM), [[finite volume method]]s (FVM) and [[finite difference method]]s (FDM), as well other kind of methods called [[Meshfree methods]], which were made to solve problems where the before mentioned methods are limited. The FEM has a prominent position among these methods and especially its exceptionally efficient higher-order version [[hp-FEM]]. Other hybrid versions of FEM and Meshfree methods include the generalized finite element method (GFEM), [[extended finite element method]] (XFEM), [[Spectral element method|spectral finite element method]] (SFEM), [[Meshfree methods|meshfree finite element method]], [[Discontinuous Galerkin Method|discontinuous Galerkin finite element method]] (DGFEM), [[Element-Free Galerkin Method]] (EFGM), [[Interpolating Element-Free Galerkin Method]] (IEFGM), etc.&lt;br /&gt;
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The three most widely used numerical methods to solve PDEs are the finite element method (FEM), finite volume methods (FVM) and finite difference methods (FDM), as well other kind of methods called Meshfree methods, which were made to solve problems where the before mentioned methods are limited. The FEM has a prominent position among these methods and especially its exceptionally efficient higher-order version hp-FEM. Other hybrid versions of FEM and Meshfree methods include the generalized finite element method (GFEM), extended finite element method (XFEM), spectral finite element method (SFEM), meshfree finite element method, discontinuous Galerkin finite element method (DGFEM), Element-Free Galerkin Method (EFGM), Interpolating Element-Free Galerkin Method (IEFGM), etc.&lt;br /&gt;
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求解偏微分方程最常用的三种数值方法是有限元分析法、有限体积法和有限差分法，以及其他一些称为无网格法的方法。这些方法用于解决前面提到的方法受到的限制。在这些方法中，有限元方法，尤其是高效的高阶有限元方法，占有重要地位。其他有限元法和无网格法的混合形式包括广义有限元分析法(GFEM)、扩展有限元分析法(XFEM)、谱有限元分析法(SFEM)、无网格有限元分析法(DGFEM)、间断伽辽金有限元分析法(DGFEM)、无网格伽辽金法(EFGM)、插值无网格伽辽金法(IEFGM)等。&lt;br /&gt;
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=== Finite element method ===&lt;br /&gt;
有限元分析法&lt;br /&gt;
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{{main|Finite element method}}&lt;br /&gt;
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The finite element method (FEM) (its practical application often known as finite element analysis (FEA)) is a numerical technique for finding approximate solutions of partial differential equations (PDE) as well as of integral equations. The solution approach is based either on eliminating the differential equation completely (steady state problems), or rendering the PDE into an approximating system of ordinary differential equations, which are then numerically integrated using standard techniques such as Euler's method, Runge–Kutta, etc.&lt;br /&gt;
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The finite element method (FEM) (its practical application often known as finite element analysis (FEA)) is a numerical technique for finding approximate solutions of partial differential equations (PDE) as well as of integral equations. The solution approach is based either on eliminating the differential equation completely (steady state problems), or rendering the PDE into an approximating system of ordinary differential equations, which are then numerically integrated using standard techniques such as Euler's method, Runge–Kutta, etc.&lt;br /&gt;
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'''&amp;lt;font color = &amp;quot;#ff8000&amp;quot;&amp;gt;有限元分析法 Finite Element Method&amp;lt;/font&amp;gt;''' ((其实际应用通常被称为有限元分析(FEA))是一种寻找偏微分方程(PDE)和积分方程近似解的数值技术。这种求解方法要么基于完全消除微分方程(稳态问题) ，要么将偏微分方程转化为常微分方程的近似系统，然后使用标准技术进行数值积分，如欧拉方法、 Runge-Kutta 等。&lt;br /&gt;
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===Finite difference method===&lt;br /&gt;
有限差分法&lt;br /&gt;
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{{main|Finite difference method}}&lt;br /&gt;
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Finite-difference methods are numerical methods for approximating the solutions to differential equations using [[finite difference]] equations to approximate derivatives.&lt;br /&gt;
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Finite-difference methods are numerical methods for approximating the solutions to differential equations using finite difference equations to approximate derivatives.&lt;br /&gt;
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有限差分法是一种数值方法，用差分方程近似微分方程的解。&lt;br /&gt;
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=== Finite volume method ===&lt;br /&gt;
有限体积法&lt;br /&gt;
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{{main|Finite volume method}}&lt;br /&gt;
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Similar to the finite difference method or finite element method, values are calculated at discrete places on a meshed geometry. &amp;quot;Finite volume&amp;quot; refers to the small volume surrounding each node point on a mesh. In the finite volume method, surface integrals in a partial differential equation that contain a divergence term are converted to volume integrals, using the [[divergence theorem]]. These terms are then evaluated as fluxes at the surfaces of each finite volume. Because the flux entering a given volume is identical to that leaving the adjacent volume, these methods conserve mass by design.&lt;br /&gt;
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Similar to the finite difference method or finite element method, values are calculated at discrete places on a meshed geometry. &amp;quot;Finite volume&amp;quot; refers to the small volume surrounding each node point on a mesh. In the finite volume method, surface integrals in a partial differential equation that contain a divergence term are converted to volume integrals, using the divergence theorem. These terms are then evaluated as fluxes at the surfaces of each finite volume. Because the flux entering a given volume is identical to that leaving the adjacent volume, these methods conserve mass by design.&lt;br /&gt;
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类似于有限差分法或有限元分析，函数值是在网状几何体上的离散位置进行计算的。“有限体积”是指网格上每个节点周围的小体积。在有限体积法中，偏微分方程中含有散度项的面积分用散度定理积分转换成体积分。然后将这些项用于估算每个有限体积表面上的通量。由于进入给定体积的通量与转移到相邻体积元的通量相同，所以这些方法在设计上保证了质量守恒。&lt;br /&gt;
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==See also==&lt;br /&gt;
请参阅&lt;br /&gt;
* [[Dirichlet boundary condition]]&lt;br /&gt;
狄利克雷边界条件&lt;br /&gt;
* [[Jet bundle]]&lt;br /&gt;
射流丛&lt;br /&gt;
* [[Laplace transform applied to differential equations]]&lt;br /&gt;
微分方程中的拉普拉斯变换&lt;br /&gt;
* [[List of dynamical systems and differential equations topics]]&lt;br /&gt;
动力学系统和微分方程的列表&lt;br /&gt;
* [[Matrix differential equation]]&lt;br /&gt;
矩阵微分方程&lt;br /&gt;
* [[Neumann boundary condition]]&lt;br /&gt;
诺伊曼边界条件&lt;br /&gt;
* [[Numerical partial differential equations]]&lt;br /&gt;
数值偏微分方程&lt;br /&gt;
* [[Partial differential algebraic equation]]&lt;br /&gt;
偏微分代数方程&lt;br /&gt;
* [[Recurrence relation]]&lt;br /&gt;
递推关系&lt;br /&gt;
* [[Robin boundary condition]]&lt;br /&gt;
罗宾边界条件&lt;br /&gt;
* [[Stochastic processes and boundary value problems]]&lt;br /&gt;
随机过程和边值问题&lt;br /&gt;
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== The energy method ==&lt;br /&gt;
能量法&lt;br /&gt;
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The energy method is a mathematical procedure that can be used to verify well-posedness of initial-boundary-value-problems.&amp;lt;ref&amp;gt;{{cite book |title=High Order Difference Methods for Time Dependent PDE&lt;br /&gt;
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The energy method is a mathematical procedure that can be used to verify well-posedness of initial-boundary-value-problems.&amp;lt;ref&amp;gt;{{cite book |title=High Order Difference Methods for Time Dependent PDE&lt;br /&gt;
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能量法是验证初边值问题适定性的一种数学方法。 时变偏微分方程的高阶差分方法&lt;br /&gt;
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|first=Bertil|last=Gustafsson|publisher=Springer|year=2008|isbn=978-3-540-74992-9|doi=10.1007/978-3-540-74993-6}}&amp;lt;/ref&amp;gt; In the following example the energy method is used to decide where and which boundary conditions should be imposed such that the resulting IBVP is well-posed. Consider the one-dimensional hyperbolic PDE given by&lt;br /&gt;
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|first=Bertil|last=Gustafsson|publisher=Springer|year=2008|isbn=978-3-540-74992-9|doi=10.1007/978-3-540-74993-6}}&amp;lt;/ref&amp;gt; In the following example the energy method is used to decide where and which boundary conditions should be imposed such that the resulting IBVP is well-posed. Consider the one-dimensional hyperbolic PDE given by&lt;br /&gt;
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| first Bertil | last Gustafsson | publisher | Springer | year 2008 | isbn 978-3-540-74992-9 | doi 10.1007 / 978-3-540-74993-6} / ref 在下面的例子中，使用能量方法来决定应该施加哪些边界条件，使得得到的 IBVP适定。考虑一维双曲偏微分方程&lt;br /&gt;
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: &amp;lt;math&amp;gt;\frac{\partial u}{\partial t} + \alpha \frac{\partial u}{\partial x} = 0, \quad x \in [a,b], \operatorname t &amp;gt; 0,&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;\frac{\partial u}{\partial t} + \alpha \frac{\partial u}{\partial x} = 0, \quad x \in [a,b], \operatorname t &amp;gt; 0,&amp;lt;/math&amp;gt;&lt;br /&gt;
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where &amp;lt;math&amp;gt;\alpha \neq 0&amp;lt;/math&amp;gt; is a constant and &amp;lt;math&amp;gt;u(x,t)&amp;lt;/math&amp;gt; is an unknown function with initial condition &amp;lt;math&amp;gt;u(x,0) = f(x)&amp;lt;/math&amp;gt;. Multiplying with &amp;lt;math&amp;gt;u&amp;lt;/math&amp;gt; and integrating over the domain gives&lt;br /&gt;
&lt;br /&gt;
where &amp;lt;math&amp;gt;\alpha \neq 0&amp;lt;/math&amp;gt; is a constant and &amp;lt;math&amp;gt;u(x,t)&amp;lt;/math&amp;gt; is an unknown function with initial condition &amp;lt;math&amp;gt;u(x,0) = f(x)&amp;lt;/math&amp;gt;. Multiplying with &amp;lt;math&amp;gt;u&amp;lt;/math&amp;gt; and integrating over the domain gives&lt;br /&gt;
&lt;br /&gt;
其中 &amp;lt;math&amp;gt;\alpha \neq 0&amp;lt;/math&amp;gt; 是常数，并且 &amp;lt;math&amp;gt;u(x,t)&amp;lt;/math&amp;gt; 是未知函数，初始条件是 &amp;lt;math&amp;gt;u(x,0) = f(x)&amp;lt;/math&amp;gt;。乘以 &amp;lt;math&amp;gt;u&amp;lt;/math&amp;gt; 并在域上进行积分。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt;\int_a^b u \frac{\partial u}{\partial t} \operatorname dx + \alpha \int _a ^b u \frac{\partial u}{\partial x} \operatorname dx = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;\int_a^b u \frac{\partial u}{\partial t} \operatorname dx + \alpha \int _a ^b u \frac{\partial u}{\partial x} \operatorname dx = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Using that&lt;br /&gt;
&lt;br /&gt;
Using that&lt;br /&gt;
&lt;br /&gt;
利用这一点&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt;\int _a ^b u \frac{\partial u}{\partial t} \operatorname dx = \frac{1}{2} \frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 \quad \text{and} \quad \int _a ^b u \frac{\partial u}{\partial x} \operatorname dx = \frac{1}{2} u(b,t)^2 - \frac{1}{2} u(a,t)^2,.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;\int _a ^b u \frac{\partial u}{\partial t} \operatorname dx = \frac{1}{2} \frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 \quad \text{and} \quad \int _a ^b u \frac{\partial u}{\partial x} \operatorname dx = \frac{1}{2} u(b,t)^2 - \frac{1}{2} u(a,t)^2,.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
where integration by parts has been used for the second relationship, we get&lt;br /&gt;
&lt;br /&gt;
where integration by parts has been used for the second relationship, we get&lt;br /&gt;
&lt;br /&gt;
第二个关系中采用了分部积分法，我们可以得到&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt;\frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 + \alpha u(b,t)^2 - \alpha u(a,t)^2 = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;\frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 + \alpha u(b,t)^2 - \alpha u(a,t)^2 = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Here &amp;lt;math&amp;gt;\vert \vert \cdot \vert \vert&amp;lt;/math&amp;gt; denotes the standard L2-norm.&lt;br /&gt;
&lt;br /&gt;
Here &amp;lt;math&amp;gt;\vert \vert \cdot \vert \vert&amp;lt;/math&amp;gt; denotes the standard L2-norm.&lt;br /&gt;
&lt;br /&gt;
在这里，&amp;lt;math&amp;gt;\vert \vert \cdot \vert \vert&amp;lt;/math&amp;gt; 表示标准的 L2-正则。&lt;br /&gt;
&lt;br /&gt;
For well-posedness we require that the energy of the solution is non-increasing, i.e. that &amp;lt;math&amp;gt;\frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 \leq 0&amp;lt;/math&amp;gt;, which is achieved by specifying &amp;lt;math&amp;gt;u&amp;lt;/math&amp;gt; at &amp;lt;math&amp;gt;x = a&amp;lt;/math&amp;gt; if &amp;lt;math&amp;gt;\alpha &amp;gt; 0&amp;lt;/math&amp;gt; and at &amp;lt;math&amp;gt;x = b&amp;lt;/math&amp;gt; if &amp;lt;math&amp;gt;\alpha &amp;lt; 0&amp;lt;/math&amp;gt;. This corresponds to only imposing boundary conditions at the inflow. Note that well-posedness allows for growth in terms of data (initial and boundary) and thus it is sufficient to show that &amp;lt;math&amp;gt;\frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 \leq 0&amp;lt;/math&amp;gt; holds when all data is set to zero.&lt;br /&gt;
&lt;br /&gt;
For well-posedness we require that the energy of the solution is non-increasing, i.e. that &amp;lt;math&amp;gt;\frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 \leq 0&amp;lt;/math&amp;gt;, which is achieved by specifying &amp;lt;math&amp;gt;u&amp;lt;/math&amp;gt; at &amp;lt;math&amp;gt;x = a&amp;lt;/math&amp;gt; if &amp;lt;math&amp;gt;\alpha &amp;gt; 0&amp;lt;/math&amp;gt; and at &amp;lt;math&amp;gt;x = b&amp;lt;/math&amp;gt; if &amp;lt;math&amp;gt;\alpha &amp;lt; 0&amp;lt;/math&amp;gt;. This corresponds to only imposing boundary conditions at the inflow. Note that well-posedness allows for growth in terms of data (initial and boundary) and thus it is sufficient to show that &amp;lt;math&amp;gt;\frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 \leq 0&amp;lt;/math&amp;gt; holds when all data is set to zero.&lt;br /&gt;
&lt;br /&gt;
对于适定性，我们要解的能量是不增加的，即 &amp;lt;math&amp;gt;\frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 \leq 0&amp;lt;/math&amp;gt; ，这种关系可以通过在&amp;lt;math&amp;gt;x = a&amp;lt;/math&amp;gt;处 （如果 &amp;lt;math&amp;gt;\alpha &amp;gt; 0&amp;lt;/math&amp;gt;） 以及 &amp;lt;math&amp;gt;x = b&amp;lt;/math&amp;gt;处 （如果 &amp;lt;math&amp;gt;\alpha &amp;lt; 0&amp;lt;/math&amp;gt;）指定&amp;lt;math&amp;gt;u&amp;lt;/math&amp;gt;的值来实现。这只相当于在入流处附加边界条件。注意，适定性允许在数据(初始和边界)上的增长，因此它足以表明当所有数据设置为零时应有 &amp;lt;math&amp;gt;\frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 \leq 0&amp;lt;/math&amp;gt;。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==[[用户:Yuling|Yuling]]（[[用户讨论:Yuling|讨论]]）“This corresponds to only imposing boundary conditions at the inflow.” 这句话中的inflow不是很理解&lt;br /&gt;
&lt;br /&gt;
==Notes==&lt;br /&gt;
&lt;br /&gt;
{{Reflist}}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
== References ==&lt;br /&gt;
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&lt;br /&gt;
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&lt;br /&gt;
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&lt;br /&gt;
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| first Bertil | last Gustafsson | Springer | year 2008 | isbn 978-3-540-74992-9 | doi 10.1007 / 978-3-540-74993-6}&lt;br /&gt;
&lt;br /&gt;
{{refend}}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
== Further reading ==&lt;br /&gt;
&lt;br /&gt;
* {{Cite journal|last=Cajori|first=Florian|authorlink=Florian Cajori|year=1928|title=The Early History of Partial Differential Equations and of Partial Differentiation and Integration|url=http://www.math.harvard.edu/archive/21a_fall_14/exhibits/cajori/cajori.pdf|journal=The American Mathematical Monthly|volume=35|issue=9|pages=459–467|doi=10.2307/2298771|access-date=2016-05-15|archive-url=https://web.archive.org/web/20181123102253/http://www.math.harvard.edu/archive/21a_fall_14/exhibits/cajori/cajori.pdf|archive-date=2018-11-23|url-status=dead}}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
== External links ==&lt;br /&gt;
&lt;br /&gt;
{{Sister project links| wikt=no | commons=Category:Solutions of PDE | b=Partial Differential Equations | n=no | q=Partial differential equation | s=no | v=no | voy=no | species=no | d=no}}&lt;br /&gt;
&lt;br /&gt;
* {{springer|title=Differential equation, partial|id=p/d031920}}&lt;br /&gt;
&lt;br /&gt;
* [http://eqworld.ipmnet.ru/en/pde-en.htm Partial Differential Equations: Exact Solutions] at EqWorld: The World of Mathematical Equations.&lt;br /&gt;
&lt;br /&gt;
* [http://eqworld.ipmnet.ru/en/solutions/eqindex/eqindex-pde.htm Partial Differential Equations: Index] at EqWorld: The World of Mathematical Equations.&lt;br /&gt;
&lt;br /&gt;
* [http://eqworld.ipmnet.ru/en/methods/meth-pde.htm Partial Differential Equations: Methods] at EqWorld: The World of Mathematical Equations.&lt;br /&gt;
&lt;br /&gt;
* [https://web.archive.org/web/20170701144823/http://www.exampleproblems.com/wiki/index.php?title=Partial_Differential_Equations Example problems with solutions] at exampleproblems.com&lt;br /&gt;
&lt;br /&gt;
* [http://mathworld.wolfram.com/PartialDifferentialEquation.html Partial Differential Equations] at mathworld.wolfram.com&lt;br /&gt;
&lt;br /&gt;
* [https://reference.wolfram.com/language/FEMDocumentation/tutorial/SolvingPDEwithFEM.html Partial Differential Equations] with Mathematica&lt;br /&gt;
&lt;br /&gt;
* [http://www.mathworks.com/moler/pdes.pdf Partial Differential Equations] in Cleve Moler: Numerical Computing with MATLAB&lt;br /&gt;
&lt;br /&gt;
* [http://www.nag.com/numeric/fl/nagdoc_fl24/html/D03/d03intro.html Partial Differential Equations] at nag.com&lt;br /&gt;
&lt;br /&gt;
* {{cite web |first=Grant |last=Sanderson |title=But what is a partial differential equation? |work=3Blue1Brown |date=April 21, 2019 |url=https://www.youtube.com/watch?v=ly4S0oi3Yz8&amp;amp;list=PLZHQObOWTQDNPOjrT6KVlfJuKtYTftqH6 |via=[[YouTube]] }}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{{Differential equations topics}}&lt;br /&gt;
&lt;br /&gt;
{{Authority control}}&lt;br /&gt;
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&lt;br /&gt;
[[Category:Partial differential equations| ]]&lt;br /&gt;
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[[Category:Multivariable calculus]]&lt;br /&gt;
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Category:Multivariable calculus&lt;br /&gt;
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类别: 多元微积分&lt;br /&gt;
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[[Category:Differential equations]]&lt;br /&gt;
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Category:Differential equations&lt;br /&gt;
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类别: 微分方程&lt;br /&gt;
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Category:Concepts in physics&lt;br /&gt;
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分类: 物理概念&lt;br /&gt;
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&amp;lt;noinclude&amp;gt;&lt;br /&gt;
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&amp;lt;small&amp;gt;This page was moved from [[wikipedia:en:Partial differential equation]]. Its edit history can be viewed at [[偏微分方程/edithistory]]&amp;lt;/small&amp;gt;&amp;lt;/noinclude&amp;gt;&lt;br /&gt;
&lt;br /&gt;
[[Category:待整理页面]]&lt;/div&gt;</summary>
		<author><name>Ruili</name></author>
	</entry>
	<entry>
		<id>https://wiki.swarma.org/index.php?title=%E5%81%8F%E5%BE%AE%E5%88%86%E6%96%B9%E7%A8%8B&amp;diff=18206</id>
		<title>偏微分方程</title>
		<link rel="alternate" type="text/html" href="https://wiki.swarma.org/index.php?title=%E5%81%8F%E5%BE%AE%E5%88%86%E6%96%B9%E7%A8%8B&amp;diff=18206"/>
		<updated>2020-11-12T16:38:26Z</updated>

		<summary type="html">&lt;p&gt;Ruili：&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;此词条暂由Yuling翻译，未经人工整理和审校，带来阅读不便，请见谅。&lt;br /&gt;
&lt;br /&gt;
[[File:Heat.gif|thumb|right|A visualisation of a solution to the two-dimensional [[heat equation]] with temperature represented by the third dimension]]&lt;br /&gt;
&lt;br /&gt;
A visualisation of a solution to the two-dimensional [[heat equation with temperature represented by the third dimension]]&lt;br /&gt;
&lt;br /&gt;
以三维表示温度的二维热方程解的可视化&lt;br /&gt;
&lt;br /&gt;
In [[mathematics]], a '''partial differential equation''' ('''PDE''') is a [[differential equation]] that contains unknown [[Multivariable calculus|multivariable functions]] and their [[partial derivative]]s. PDEs are used to formulate problems involving functions of several variables, and are either solved by hand, or used to create a [[computer model]]. A special case is [[ordinary differential equation]]s (ODEs), which deal with functions of a single variable and their derivatives.&lt;br /&gt;
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In mathematics, a partial differential equation (PDE) is a differential equation that contains unknown multivariable functions and their partial derivatives. PDEs are used to formulate problems involving functions of several variables, and are either solved by hand, or used to create a computer model. A special case is ordinary differential equations (ODEs), which deal with functions of a single variable and their derivatives.&lt;br /&gt;
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在数学中，'''&amp;lt;font color = &amp;quot;#ff8000&amp;quot;&amp;gt; 偏微分方程函数 Partial Differential Equation&amp;lt;/font&amp;gt;'''是包含未知多元函数及其偏导数的微分方程。偏微分方程用于描述涉及多元函数的问题，可以通过人为求解，也可以通过建立计算机模型来求解。常微分方程是偏微分方程一种特殊情况，它处理的是一元函数及其导数。&lt;br /&gt;
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PDEs can be used to describe a wide variety of phenomena such as sound, heat, [[diffusion]], [[electrostatics]], [[Electromagnetism|electrodynamics]], [[fluid dynamics]], [[Elasticity (physics)|elasticity]], [[gravitation]] and [[quantum mechanics]]. These seemingly distinct physical phenomena can be formalised similarly in terms of PDEs. Just as ordinary differential equations often model one-dimensional [[dynamical system]]s, partial differential equations often model [[multidimensional system]]s. PDEs find their generalisation in [[stochastic partial differential equation]]s.&lt;br /&gt;
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PDEs can be used to describe a wide variety of phenomena such as sound, heat, diffusion, electrostatics, electrodynamics, fluid dynamics, elasticity, gravitation and quantum mechanics. These seemingly distinct physical phenomena can be formalised similarly in terms of PDEs. Just as ordinary differential equations often model one-dimensional dynamical systems, partial differential equations often model multidimensional systems. PDEs find their generalisation in stochastic partial differential equations.&lt;br /&gt;
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偏微分方程可以用来描述各种各样的物理现象，如声音，热量，扩散，静电，电动力学，流体力学，弹性力学，重力和量子力学。这些看起来截然不同的物理现象却可以用类似的偏微分方程来描述。正如常微分方程经常对一维动力系统进行建模一样，偏微分方程经常对多维系统进行建模。随机偏微分方程是偏微分方程的一种推广。&lt;br /&gt;
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== Introduction ==&lt;br /&gt;
引言&lt;br /&gt;
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Partial differential equations (PDEs) are equations that involve rates of change with respect to [[continuous variables]]. For example, the position of a [[rigid body]] is specified by six parameters,&amp;lt;ref&amp;gt;{{Cite book|url=https://books.google.com/books?id=v9PLbcYd9aUC&amp;amp;pg=PA32|title=Modelling and Control of Robot Manipulators|last=Sciavicco|first=Lorenzo|last2=Siciliano|first2=Bruno|date=2001-02-19|publisher=Springer Science &amp;amp; Business Media|isbn=9781852332211|language=en}}&amp;lt;/ref&amp;gt; but the configuration of a [[fluid]] is given by the [[continuous distribution]] of several parameters, such as the [[temperature]], [[pressure]], and so forth. The dynamics for the rigid body take place in a finite-dimensional [[Configuration space (physics)|configuration space]]; the dynamics for the fluid occur in an infinite-dimensional configuration space. This distinction usually makes PDEs much harder to solve than ordinary differential equations (ODEs), but here again, there will be simple solutions for linear problems. Classic domains where PDEs are used include [[acoustics]], [[fluid dynamics]], [[electrodynamics]], and [[heat transfer]].&lt;br /&gt;
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Partial differential equations (PDEs) are equations that involve rates of change with respect to continuous variables. For example, the position of a rigid body is specified by six parameters, but the configuration of a fluid is given by the continuous distribution of several parameters, such as the temperature, pressure, and so forth. The dynamics for the rigid body take place in a finite-dimensional configuration space; the dynamics for the fluid occur in an infinite-dimensional configuration space. This distinction usually makes PDEs much harder to solve than ordinary differential equations (ODEs), but here again, there will be simple solutions for linear problems. Classic domains where PDEs are used include acoustics, fluid dynamics, electrodynamics, and heat transfer.&lt;br /&gt;
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偏微分方程(简称为PDEs)涉及到方程相对于连续变量的变化率。例如，刚体的位置是由六个参数确定的，而流体的状态是由几个参数的连续分布给出的，如温度、压力等。刚体的动力学过程发生在有限维状态空间中，流体的动力学过程发生在无限维状态空间中。这种区别通常使偏微分方程比常微分方程更难求解，但是线性问题仍然有简单的求解方式。使用偏微分方程的经典领域包括声学、流体力学、电动力学和传热学。&lt;br /&gt;
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A partial differential equation (PDE) for the function {{math|''u''(''x''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;,… ''x&amp;lt;sub&amp;gt;n&amp;lt;/sub&amp;gt;'')}} is an equation of the form&lt;br /&gt;
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A partial differential equation (PDE) for the function  is an equation of the form&lt;br /&gt;
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函数 {{math|''u''(''x''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;,… ''x&amp;lt;sub&amp;gt;n&amp;lt;/sub&amp;gt;'')}} 的偏微分方程形式是：&lt;br /&gt;
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: &amp;lt;math&amp;gt;f \left (x_1, \ldots x_n; u, \frac{\partial u}{\partial x_1}, \ldots \frac{\partial u}{\partial x_n}; \frac{\partial^2 u}{\partial x_1 \partial x_1}, \ldots \frac{\partial^2 u}{\partial x_1 \partial x_n}; \ldots \right) = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;f \left (x_1, \ldots x_n; u, \frac{\partial u}{\partial x_1}, \ldots \frac{\partial u}{\partial x_n}; \frac{\partial^2 u}{\partial x_1 \partial x_1}, \ldots \frac{\partial^2 u}{\partial x_1 \partial x_n}; \ldots \right) = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
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If {{mvar|f}} is a [[linear function]] of {{mvar|u}} and its derivatives, then the PDE is called linear. Common examples of linear PDEs include the [[heat equation]], the [[wave equation]], [[Laplace's equation]], [[Helmholtz equation]], [[Klein–Gordon equation]], and [[Poisson's equation]].&lt;br /&gt;
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If  is a linear function of  and its derivatives, then the PDE is called linear. Common examples of linear PDEs include the heat equation, the wave equation, Laplace's equation, Helmholtz equation, Klein–Gordon equation, and Poisson's equation.&lt;br /&gt;
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如果 {{mvar|f}} 是函数 {{math|''u''}} 及其导数的线性函数，则偏微分方程称为线性函数。线性偏微分方程的常见例子包括热方程、波动方程、拉普拉斯方程、亥姆霍兹方程方程、克莱因-高登方程和泊松方程。&lt;br /&gt;
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A relatively simple PDE is&lt;br /&gt;
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A relatively simple PDE is&lt;br /&gt;
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一个相对简单的偏微分方程：&lt;br /&gt;
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: &amp;lt;math&amp;gt;\frac{\partial u}{\partial x}(x,y) = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;\frac{\partial u}{\partial x}(x,y) = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
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This relation [[Logical implication|implies]] that the function {{math|''u''(''x'',''y'')}} is independent of {{mvar|x}}. However, the equation gives no information on the function's dependence on the variable {{mvar|y}}. Hence the general solution of this equation is&lt;br /&gt;
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This relation implies that the function  is independent of . However, the equation gives no information on the function's dependence on the variable . Hence the general solution of this equation is&lt;br /&gt;
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这意味着函数 {{math|''u''(''x'',''y'')}} 独立于 {{mvar|x}} 的。然而，这个方程没有给出关于函数和自变量的相关性的信息。因此，这个方程的通解是&lt;br /&gt;
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: &amp;lt;math&amp;gt;u(x,y) = f(y),&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;u(x,y) = f(y),&amp;lt;/math&amp;gt;&lt;br /&gt;
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where {{mvar|f}} is an arbitrary function of {{mvar|y}}. The analogous ordinary differential equation is&lt;br /&gt;
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where  is an arbitrary function of . The analogous ordinary differential equation is&lt;br /&gt;
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其中， {{mvar|f}} 是 {{mvar|y}} 的任意函数。&lt;br /&gt;
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类似的常微分方程是：&lt;br /&gt;
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: &amp;lt;math&amp;gt;\frac{\mathrm{d} u}{\mathrm{d} x}(x) = 0,&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;\frac{\mathrm{d} u}{\mathrm{d} x}(x) = 0,&amp;lt;/math&amp;gt;&lt;br /&gt;
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which has the solution&lt;br /&gt;
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which has the solution&lt;br /&gt;
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它的解为&lt;br /&gt;
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: &amp;lt;math&amp;gt;u(x) = c,&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;u(x) = c,&amp;lt;/math&amp;gt;&lt;br /&gt;
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where {{mvar|c}} is any [[Constant (mathematics)|constant]] value. These two examples illustrate that general solutions of ordinary differential equations (ODEs) involve arbitrary constants, but solutions of PDEs involve arbitrary functions.&lt;br /&gt;
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where  is any constant value. These two examples illustrate that general solutions of ordinary differential equations (ODEs) involve arbitrary constants, but solutions of PDEs involve arbitrary functions.&lt;br /&gt;
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这里，{{mvar|c}} 是一个任意常量。&lt;br /&gt;
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这两个例子说明常微分方程的一般解包含任意常数，但偏微分方程的解包含任意函数。&lt;br /&gt;
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A solution of a PDE is generally not [[Uniqueness quantification|unique]]; additional conditions must generally be specified on the [[Boundary (topology)|boundary]] of the region where the solution is defined. For instance, in the simple example above, the function {{math|''f''(''y'')}} can be determined if {{mvar|u}} is specified on the line {{math|''x'' {{=}} 0}}.&lt;br /&gt;
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A solution of a PDE is generally not unique; additional conditions must generally be specified on the boundary of the region where the solution is defined. For instance, in the simple example above, the function  can be determined if  is specified on the line  0}}.&lt;br /&gt;
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偏微分方程的解一般不是唯一的; 一般必须在定义解的区域边界上定义附加条件。 例如，在上面的简单示例中，如果在 {{math|''x'' {{=}} 0}} 时确定了 {{mvar|u}} 的值，则可以确定该函数 {{math|''f''(''y'')}}。&lt;br /&gt;
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== Existence and uniqueness ==&lt;br /&gt;
存在性和唯一性&lt;br /&gt;
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Although the issue of existence and uniqueness of solutions of ordinary differential equations has a very satisfactory answer with the [[Picard–Lindelöf theorem]], that is far from the case for partial differential equations. The [[Cauchy–Kowalevski theorem]] states that the [[Cauchy problem]] for any partial differential equation whose coefficients are [[Analytic function|analytic]] in the unknown function and its derivatives, has a locally unique analytic solution. Although this result might appear to settle the existence and uniqueness of solutions, there are examples of linear partial differential equations whose coefficients have derivatives of all orders (which are nevertheless not analytic) but which have no solutions at all: see [[Lewy's example|Lewy (1957)]]. Even if the solution of a partial differential equation exists and is unique, it may nevertheless have undesirable properties.  The mathematical study of these questions is usually in the more powerful context of [[weak solution]]s.&lt;br /&gt;
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Although the issue of existence and uniqueness of solutions of ordinary differential equations has a very satisfactory answer with the Picard–Lindelöf theorem, that is far from the case for partial differential equations. The Cauchy–Kowalevski theorem states that the Cauchy problem for any partial differential equation whose coefficients are analytic in the unknown function and its derivatives, has a locally unique analytic solution. Although this result might appear to settle the existence and uniqueness of solutions, there are examples of linear partial differential equations whose coefficients have derivatives of all orders (which are nevertheless not analytic) but which have no solutions at all: see Lewy (1957). Even if the solution of a partial differential equation exists and is unique, it may nevertheless have undesirable properties.  The mathematical study of these questions is usually in the more powerful context of weak solutions.&lt;br /&gt;
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尽管常微分方程解的存在性和唯一性用'''&amp;lt;font color=&amp;quot;#ff8000&amp;quot;&amp;gt;弗罗贝尼乌斯定理 Picard–Lindelöf Theorem&amp;lt;/font&amp;gt;得到了令人满意的结果，但偏微分方程解的存在性和唯一性却远没有得到解决。'''&amp;lt;font color=&amp;quot;#ff8000&amp;quot;&amp;gt;柯西-科瓦列夫斯基定理 Cauchy–Kowalevski theorem&amp;lt;/font&amp;gt;指出：对于任意系数在未知函数及其导数中解析的偏微分方程，柯西问题存在一个局部唯一的解析解。虽然这个结果似乎解决了解的存在性和唯一性问题，但是存在一些线性偏微分方程-其系数具有所有级数的导数(尽管这些导数不是解析的) ，但是根本没有解: 见 Lewy (1957)。即使偏微分方程的解存在且唯一，它仍然可能具有不可预料的性质。这些问题的数学研究通常是在更有力的弱解的背景下进行的。&lt;br /&gt;
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An example of pathological behavior is the sequence (depending upon {{mvar|n}}) of [[Cauchy problem]]s for the [[Laplace equation]]&lt;br /&gt;
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An example of pathological behavior is the sequence (depending upon ) of Cauchy problems for the Laplace equation&lt;br /&gt;
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反常特征的一个例子是拉普拉斯方程的柯西问题的序列(取决于{{mvar|n}})&lt;br /&gt;
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: &amp;lt;math&amp;gt;\frac{\partial^2 u}{\partial x^2} + \frac{\partial^2 u}{\partial y^2}=0,&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;\frac{\partial^2 u}{\partial x^2} + \frac{\partial^2 u}{\partial y^2}=0,&amp;lt;/math&amp;gt;&lt;br /&gt;
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with [[boundary condition]]s&lt;br /&gt;
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with boundary conditions&lt;br /&gt;
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具有边界条件&lt;br /&gt;
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: &amp;lt;math&amp;gt;\begin{align} u(x,0) &amp;amp;= 0, \\ \frac{\partial u}{\partial y}(x,0) &amp;amp;= \frac{\sin nx}{n}, \end{align}&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;\begin{align} u(x,0) &amp;amp;= 0, \\ \frac{\partial u}{\partial y}(x,0) &amp;amp;= \frac{\sin nx}{n}, \end{align}&amp;lt;/math&amp;gt;&lt;br /&gt;
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where {{mvar|n}} is an integer. The derivative of {{mvar|u}} with respect to {{mvar|y}} approaches zero [[uniform convergence|uniformly]] in {{mvar|x}} as {{mvar|n}} increases, but the solution is&lt;br /&gt;
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where  is an integer. The derivative of  with respect to  approaches zero uniformly in  as  increases, but the solution is&lt;br /&gt;
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其中 {{mvar|n}} 是整数。{{mvar|u}} 关于 {{mvar|y}} 的导数，一致地随着 {{mvar|n}} 的增加而趋于零，但解是&lt;br /&gt;
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: &amp;lt;math&amp;gt;u(x,y) = \frac{\sinh ny \sin nx}{n^2}.&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;u(x,y) = \frac{\sinh ny \sin nx}{n^2}.&amp;lt;/math&amp;gt;&lt;br /&gt;
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This solution approaches infinity if {{mvar|nx}} is not an integer multiple of {{pi}} for any non-zero value of {{mvar|y}}. The Cauchy problem for the Laplace equation is called ''ill-posed'' or ''not [[Well-posed problem|well-posed]]'', since the solution does not continuously depend on the data of the problem. Such ill-posed problems are not usually satisfactory for physical applications.&lt;br /&gt;
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This solution approaches infinity if  is not an integer multiple of  for any non-zero value of . The Cauchy problem for the Laplace equation is called ill-posed or not well-posed, since the solution does not continuously depend on the data of the problem. Such ill-posed problems are not usually satisfactory for physical applications.&lt;br /&gt;
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对于任何非零的 {{mvar|y}}，如果 {{mvar|nx}} 不是模板 {{pi}} 的整数倍，这个解会接近于无穷大。拉普拉斯方程的柯西问题被称为不适定的（可以译为ill-posed或not well-posed），因为解不是连续地依赖于问题的数据。这种不适定问题通常不能满足物理应用。&lt;br /&gt;
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The [[Navier–Stokes existence and smoothness|existence of solutions for the Navier–Stokes equations]], a partial differential equation, is part of one of the [[Millennium Prize Problems]].&lt;br /&gt;
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The existence of solutions for the Navier–Stokes equations, a partial differential equation, is part of one of the Millennium Prize Problems.&lt;br /&gt;
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偏微分方程”纳维-斯托克斯方程“的解的存在性就是千禧年大奖难题之一的一部分。&lt;br /&gt;
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== Notation ==&lt;br /&gt;
符号&lt;br /&gt;
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In PDEs, it is common to denote partial derivatives using subscripts. That is:&lt;br /&gt;
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In PDEs, it is common to denote partial derivatives using subscripts. That is:&lt;br /&gt;
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在偏微分方程中，通常用下标表示偏导数。例如:&lt;br /&gt;
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: &amp;lt;math&amp;gt;u_x = \frac{\partial u}{\partial x}&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;u_x = \frac{\partial u}{\partial x}&amp;lt;/math&amp;gt;&lt;br /&gt;
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: &amp;lt;math&amp;gt;u_{xx} = \frac{\partial^2 u}{\partial x^2} &amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;u_{xx} = \frac{\partial^2 u}{\partial x^2} &amp;lt;/math&amp;gt;&lt;br /&gt;
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: &amp;lt;math&amp;gt;u_{xy} = \frac{\partial^2 u}{\partial y\, \partial x} = \frac{\partial}{\partial y } \left(\frac{\partial u}{\partial x}\right). &amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;u_{xy} = \frac{\partial^2 u}{\partial y\, \partial x} = \frac{\partial}{\partial y } \left(\frac{\partial u}{\partial x}\right). &amp;lt;/math&amp;gt;&lt;br /&gt;
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Especially in physics, [[del]] or nabla ({{math|∇}}) is often used to denote spatial derivatives, and {{math|''&amp;amp;#x307;u'', ''ü''}} for time derivatives. For example, the [[wave equation]] (mentioned below) can be written as&lt;br /&gt;
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Especially in physics, del or nabla () is often used to denote spatial derivatives, and  for time derivatives. For example, the wave equation (mentioned below) can be written as&lt;br /&gt;
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特别是在物理学中，[[del]] 或 nabla ({{math|∇}}) 经常用来表示空间导数和时间导数。例如，波动方程(在下文中提到)可以写成：&lt;br /&gt;
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:&amp;lt;math&amp;gt;\ddot u=c^2\nabla^2u&amp;lt;/math&amp;gt;&lt;br /&gt;
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&amp;lt;math&amp;gt;\ddot u=c^2\nabla^2u&amp;lt;/math&amp;gt;&lt;br /&gt;
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or&lt;br /&gt;
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or&lt;br /&gt;
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或&lt;br /&gt;
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:&amp;lt;math&amp;gt;\ddot u=c^2\Delta u&amp;lt;/math&amp;gt;&lt;br /&gt;
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&amp;lt;math&amp;gt;\ddot u=c^2\Delta u&amp;lt;/math&amp;gt;&lt;br /&gt;
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where {{math|Δ}} is the [[Laplace operator]].&lt;br /&gt;
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where  is the Laplace operator.&lt;br /&gt;
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其中，{{math|Δ}} 代表拉普拉斯算子。&lt;br /&gt;
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== Classification ==&lt;br /&gt;
分类&lt;br /&gt;
&lt;br /&gt;
Some linear, second-order partial differential equations can be classified as [[parabolic partial differential equation|parabolic]], [[hyperbolic partial differential equation|hyperbolic]] and [[elliptic partial differential equation|elliptic]]. Others, such as the [[Euler–Tricomi equation]], have different types in different regions. The classification provides a guide to appropriate initial and boundary conditions and to the smoothness of the solutions.&lt;br /&gt;
&lt;br /&gt;
Some linear, second-order partial differential equations can be classified as parabolic, hyperbolic and elliptic. Others, such as the Euler–Tricomi equation, have different types in different regions. The classification provides a guide to appropriate initial and boundary conditions and to the smoothness of the solutions.&lt;br /&gt;
&lt;br /&gt;
一些线性二阶偏微分方程可分为抛物型方程、双曲型方程和椭圆型方程。其他的方程，如欧拉-特里科米方程，在不同的领域有不同的类型。这种分类有助于选择适当的初始和边界条件以及提高解的平滑性。&lt;br /&gt;
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=== Equations of first order ===&lt;br /&gt;
一阶方程&lt;br /&gt;
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{{main|First-order partial differential equation}}&lt;br /&gt;
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=== Linear equations of second order ===&lt;br /&gt;
二阶线性方程&lt;br /&gt;
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Assuming {{math|''u&amp;lt;sub&amp;gt;xy&amp;lt;/sub&amp;gt;'' {{=}} ''u&amp;lt;sub&amp;gt;yx&amp;lt;/sub&amp;gt;''}}, the general linear second-order PDE in two independent variables has the form&lt;br /&gt;
&lt;br /&gt;
Assuming  u&amp;lt;sub&amp;gt;yx&amp;lt;/sub&amp;gt;}}, the general linear second-order PDE in two independent variables has the form&lt;br /&gt;
&lt;br /&gt;
假设 {{math|''u&amp;lt;sub&amp;gt;xy&amp;lt;/sub&amp;gt;'' {{=}} ''u&amp;lt;sub&amp;gt;yx&amp;lt;/sub&amp;gt;''}}，含有两个独立变量的一般线性二阶偏微分方程具有如下形式：&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt;Au_{xx} + 2Bu_{xy} + Cu_{yy} + \cdots \mbox{(lower order terms)} = 0,&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;Au_{xx} + 2Bu_{xy} + Cu_{yy} + \cdots \mbox{(lower order terms)} = 0,&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
where the coefficients {{mvar|A}}, {{mvar|B}}, {{mvar|C}}... may depend upon {{mvar|x}} and {{mvar|y}}. If {{math|''A''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; + ''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; + ''C''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; &amp;gt; 0}} over a region of the {{mvar|xy}}-plane, the PDE is second-order in that region. This form is analogous to the equation for a conic section:&lt;br /&gt;
&lt;br /&gt;
where the coefficients , , ... may depend upon  and . If  over a region of the -plane, the PDE is second-order in that region. This form is analogous to the equation for a conic section:&lt;br /&gt;
&lt;br /&gt;
其中的系数 {{mvar|A}}, {{mvar|B}}, {{mvar|C}}... 一般取决于 {{mvar|x}} 和 {{mvar|y}} 。如果在 {{mvar|xy}}-平面的一个区域上 {{math|''A''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; + ''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; + ''C''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; &amp;gt; 0}}，偏微分方程是二阶的，这种形式类似于圆锥截面的方程:&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt;Ax^2 + 2Bxy + Cy^2 + \cdots = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;Ax^2 + 2Bxy + Cy^2 + \cdots = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
More precisely, replacing {{math|∂&amp;lt;sub&amp;gt;''x''&amp;lt;/sub&amp;gt;}} by {{mvar|X}}, and likewise for other variables (formally this is done by a [[Fourier transform]]), converts a constant-coefficient PDE into a polynomial of the same degree, with the terms of the highest degree (a [[homogeneous polynomial]], here a [[quadratic form]]) being most significant for the classification.&lt;br /&gt;
&lt;br /&gt;
More precisely, replacing  by , and likewise for other variables (formally this is done by a Fourier transform), converts a constant-coefficient PDE into a polynomial of the same degree, with the terms of the highest degree (a homogeneous polynomial, here a quadratic form) being most significant for the classification.&lt;br /&gt;
&lt;br /&gt;
更准确地说，用 {{mvar|X}} 替换 {{math|∂&amp;lt;sub&amp;gt;''x''&amp;lt;/sub&amp;gt;}}，并同样替换其它变量(通常由傅里叶变换完成)，将一个常系数偏微分方程转换成一个相同次数的多项式，最高次数的项(齐次多项式，这里是一个二次形式)对于偏微分方程的分类最为重要。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Just as one classifies [[conic section]]s and quadratic forms into parabolic, hyperbolic, and elliptic based on the [[discriminant]] {{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − 4''AC''}}, the same can be done for a second-order PDE at a given point.  However, the [[discriminant]] in a PDE is given by {{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC''}} due to the convention of the {{mvar|xy}} term being {{math|2''B''}} rather than {{mvar|B}}; formally, the discriminant (of the associated quadratic form) is {{math|(2''B'')&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − 4''AC'' {{=}} 4(''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC'')}}, with the factor of 4 dropped for simplicity.&lt;br /&gt;
&lt;br /&gt;
Just as one classifies conic sections and quadratic forms into parabolic, hyperbolic, and elliptic based on the discriminant , the same can be done for a second-order PDE at a given point.  However, the discriminant in a PDE is given by  due to the convention of the  term being  rather than ; formally, the discriminant (of the associated quadratic form) is  4(B&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − AC)}}, with the factor of 4 dropped for simplicity.&lt;br /&gt;
&lt;br /&gt;
正如人们可以根据判别式 {{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − 4''AC''}} 将圆锥截面和二次型分为抛物型、双曲型和椭圆型一样，对于给定点的二阶偏微分方程也可以这样做。然而，偏微分方程中的判别式 {{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − 4''AC''}} 是根据交叉项的系数{{math|2''B''}} 而不是 {{mvar|B}} 给出的，形式上，判别式(关联二次型)是 {{math|(2''B'')&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − 4''AC'' {{=}} 4(''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC'')}}，为简单起见，去掉了因子4。&lt;br /&gt;
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&lt;br /&gt;
# {{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC'' &amp;lt; 0}} (''[[elliptic partial differential equation]]''): Solutions of [[elliptic partial differential equation|elliptic PDEs]] are as smooth as the coefficients allow, within the interior of the region where the equation and solutions are defined. For example, solutions of [[Laplace's equation]] are analytic within the domain where they are defined, but solutions may assume boundary values that are not smooth. The motion of a fluid at subsonic speeds can be approximated with elliptic PDEs, and the Euler–Tricomi equation is elliptic where {{math|''x'' &amp;lt; 0}}.&lt;br /&gt;
&lt;br /&gt;
  (elliptic partial differential equation): Solutions of elliptic PDEs are as smooth as the coefficients allow, within the interior of the region where the equation and solutions are defined. For example, solutions of Laplace's equation are analytic within the domain where they are defined, but solutions may assume boundary values that are not smooth. The motion of a fluid at subsonic speeds can be approximated with elliptic PDEs, and the Euler–Tricomi equation is elliptic where .&lt;br /&gt;
&lt;br /&gt;
{{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC'' &amp;lt; 0}} (椭圆形微分方程)：在定义方程和解的区域内部，椭圆型偏微分方程的解光滑到系数允许的程度。例如，拉普拉斯方程的解在它们被定义的区域内是解析的，但是解可能假设边界值是不光滑的。亚音速流体的运动可以用椭圆偏微分方程近似，其中欧拉-特里科米方程在 {{math|''x'' &amp;lt; 0}} 时是椭圆型偏微分方程。&lt;br /&gt;
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# {{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC'' {{=}} 0}} (''[[parabolic partial differential equation]]''): Equations that are [[parabolic partial differential equation|parabolic]] at every point can be transformed into a form analogous to the [[heat equation]] by a change of independent variables. Solutions smooth out as the transformed time variable increases. The Euler–Tricomi equation has parabolic type on the line where {{math|''x'' {{=}} 0}}.&lt;br /&gt;
&lt;br /&gt;
  0}} (parabolic partial differential equation): Equations that are parabolic at every point can be transformed into a form analogous to the heat equation by a change of independent variables. Solutions smooth out as the transformed time variable increases. The Euler–Tricomi equation has parabolic type on the line where  0}}.&lt;br /&gt;
&lt;br /&gt;
{{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC'' {{=}} 0}}（抛物线形偏微分方程）：在每一点上都是抛物线型的方程可以通过改变自变量从而转化成类似于热方程的形式。随着转换后的时间变量的增加，方程的解变得平滑。欧拉-特里科米方程在 {{math|''x'' {{=}} 0}} 这条特征线上是抛物线形的。&lt;br /&gt;
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# {{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC'' &amp;gt; 0}} (''[[hyperbolic partial differential equation]]''): [[hyperbolic partial differential equation|hyperbolic]] equations retain any discontinuities of functions or derivatives in the initial data. An example is the [[wave equation]]. The motion of a fluid at supersonic speeds can be approximated with hyperbolic PDEs, and the Euler–Tricomi equation is hyperbolic where {{math|''x'' &amp;gt; 0}}.&lt;br /&gt;
&lt;br /&gt;
  (hyperbolic partial differential equation): hyperbolic equations retain any discontinuities of functions or derivatives in the initial data. An example is the wave equation. The motion of a fluid at supersonic speeds can be approximated with hyperbolic PDEs, and the Euler–Tricomi equation is hyperbolic where .&lt;br /&gt;
&lt;br /&gt;
{{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC'' &amp;gt; 0}} (双曲形偏微分方程)：双曲形方程在初始数据中保留了函数或导数的任何不连续性，波动方程就是其中的一个例子。超音速流体的运动可以用双曲形偏微分方程近似，其中欧拉-特里科米方程在 {{math|''x'' &amp;gt; 0}} 时是双曲型的。&lt;br /&gt;
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If there are {{mvar|n}} independent variables {{math|''x''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;, ''x''&amp;lt;sub&amp;gt;2 &amp;lt;/sub&amp;gt;,… ''x''&amp;lt;sub&amp;gt;''n''&amp;lt;/sub&amp;gt;}}, a general linear partial differential equation of second order has the form&lt;br /&gt;
&lt;br /&gt;
If there are  independent variables , a general linear partial differential equation of second order has the form&lt;br /&gt;
&lt;br /&gt;
如果存在 {{mvar|n}} 个自变量 {{math|''x''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;, ''x''&amp;lt;sub&amp;gt;2 &amp;lt;/sub&amp;gt;,… ''x''&amp;lt;sub&amp;gt;''n''&amp;lt;/sub&amp;gt;}}，一般二阶线性偏微分方程的形式是&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
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: &amp;lt;math&amp;gt;L u =\sum_{i=1}^n\sum_{j=1}^n a_{i,j} \frac{\partial^2 u}{\partial x_i \partial x_j} \quad \text{ plus lower-order terms} =0.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;L u =\sum_{i=1}^n\sum_{j=1}^n a_{i,j} \frac{\partial^2 u}{\partial x_i \partial x_j} \quad \text{ plus lower-order terms} =0.&amp;lt;/math&amp;gt;&lt;br /&gt;
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The classification depends upon the signature of the eigenvalues of the coefficient matrix {{math|''a''&amp;lt;sub&amp;gt;''i'',''j''&amp;lt;/sub&amp;gt;}}.&lt;br /&gt;
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The classification depends upon the signature of the eigenvalues of the coefficient matrix .&lt;br /&gt;
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这种分类取决于系数矩阵本征值的符号（正负性）。&lt;br /&gt;
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# Elliptic: the eigenvalues are all positive or all negative.&lt;br /&gt;
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 Elliptic: the eigenvalues are all positive or all negative.&lt;br /&gt;
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椭圆形方程: 本征值全部为正或全部为负。&lt;br /&gt;
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# Parabolic: the eigenvalues are all positive or all negative, save one that is zero.&lt;br /&gt;
&lt;br /&gt;
 Parabolic: the eigenvalues are all positive or all negative, save one that is zero.&lt;br /&gt;
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抛物线形方程: 本征值全部为正或全部为负，除了一个为零。&lt;br /&gt;
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# Hyperbolic: there is only one negative eigenvalue and all the rest are positive, or there is only one positive eigenvalue and all the rest are negative.&lt;br /&gt;
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 Hyperbolic: there is only one negative eigenvalue and all the rest are positive, or there is only one positive eigenvalue and all the rest are negative.&lt;br /&gt;
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双曲形方程: 只有一个负特征值，其余的都是正特征值，或者只有一个正特征值，其余的都是负特征值。&lt;br /&gt;
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# Ultrahyperbolic: there is more than one positive eigenvalue and more than one negative eigenvalue, and there are no zero eigenvalues. There is only a limited theory for ultrahyperbolic equations (Courant and Hilbert, 1962).&lt;br /&gt;
&lt;br /&gt;
 Ultrahyperbolic: there is more than one positive eigenvalue and more than one negative eigenvalue, and there are no zero eigenvalues. There is only a limited theory for ultrahyperbolic equations (Courant and Hilbert, 1962).&lt;br /&gt;
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超双形方程: 存在多于一个正本征值和多于一个的负本征值，且不存在零本征值。对于超双曲方程，只存在一个有限理论(Courant 和 Hilbert，1962)。&lt;br /&gt;
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==[[用户:Yuling|Yuling]]（[[用户讨论:Yuling|讨论]]） 我对于limited theory这个单词对应的相关理论不太了解。&lt;br /&gt;
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=== Systems of first-order equations and characteristic surfaces ===&lt;br /&gt;
一阶方程组和特征曲面&lt;br /&gt;
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The classification of partial differential equations can be extended to systems of first-order equations, where the unknown {{mvar|u}} is now a [[Euclidean vector|vector]] with {{mvar|m}} components, and the coefficient matrices {{mvar|A&amp;lt;sub&amp;gt;ν&amp;lt;/sub&amp;gt;}} are {{mvar|m}} by {{mvar|m}} matrices for {{math|''ν'' {{=}} 1, 2,… ''n''}}. The partial differential equation takes the form&lt;br /&gt;
&lt;br /&gt;
The classification of partial differential equations can be extended to systems of first-order equations, where the unknown  is now a vector with  components, and the coefficient matrices  are  by  matrices for  1, 2,… n}}. The partial differential equation takes the form&lt;br /&gt;
&lt;br /&gt;
偏微分方程组的分类可以推广到一阶方程组，其中未知量 {{mvar|u}} 是有 {{mvar|m}} 个分量的向量。对于 {{math|''ν'' {{=}} 1, 2,… ''n''}}，系数矩阵 {{mvar|A&amp;lt;sub&amp;gt;ν&amp;lt;/sub&amp;gt;}} 是 {{mvar|m}} × {{mvar|m}} 的矩阵。偏微分方程形式如下：&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
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: &amp;lt;math&amp;gt;Lu = \sum_{\nu=1}^{n} A_\nu \frac{\partial u}{\partial x_\nu} + B=0,&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;Lu = \sum_{\nu=1}^{n} A_\nu \frac{\partial u}{\partial x_\nu} + B=0,&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
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where the coefficient matrices {{mvar|A&amp;lt;sub&amp;gt;ν&amp;lt;/sub&amp;gt;}} and the vector {{mvar|B}} may depend upon {{mvar|x}} and {{mvar|u}}. If a [[hypersurface]] {{mvar|S}} is given in the implicit form&lt;br /&gt;
&lt;br /&gt;
where the coefficient matrices  and the vector  may depend upon  and . If a hypersurface  is given in the implicit form&lt;br /&gt;
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其中系数矩阵 {{mvar|A&amp;lt;sub&amp;gt;ν&amp;lt;/sub&amp;gt;}} 和向量 {{mvar|B}} 可能依赖于 {{mvar|x}} 和 {{mvar|u}}。如果超曲面是以隐式形式给出的&lt;br /&gt;
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: &amp;lt;math&amp;gt;\varphi(x_1, x_2, \ldots x_n)=0,&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;\varphi(x_1, x_2, \ldots x_n)=0,&amp;lt;/math&amp;gt;&lt;br /&gt;
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where {{mvar|φ}} has a non-zero gradient, then {{mvar|S}} is a '''characteristic surface''' for the operator {{mvar|L}} at a given point if the characteristic form vanishes:&lt;br /&gt;
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where  has a non-zero gradient, then  is a characteristic surface for the operator  at a given point if the characteristic form vanishes:&lt;br /&gt;
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其中存在一个非零的梯度，那么如果特征形式消失，则在给定点上算子的特征曲面形式如下:&lt;br /&gt;
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: &amp;lt;math&amp;gt;Q\left(\frac{\partial\varphi}{\partial x_1}, \ldots\frac{\partial\varphi}{\partial x_n}\right) =\det\left[\sum_{\nu=1}^nA_\nu \frac{\partial \varphi}{\partial x_\nu}\right]=0.\,&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;Q\left(\frac{\partial\varphi}{\partial x_1}, \ldots\frac{\partial\varphi}{\partial x_n}\right) =\det\left[\sum_{\nu=1}^nA_\nu \frac{\partial \varphi}{\partial x_\nu}\right]=0.\,&amp;lt;/math&amp;gt;&lt;br /&gt;
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The geometric interpretation of this condition is as follows: if data for {{mvar|u}} are prescribed on the surface {{mvar|S}}, then it may be possible to determine the normal derivative of {{mvar|u}} on {{mvar|S}} from the differential equation. If the data on {{mvar|S}} and the differential equation determine the normal derivative of {{mvar|u}} on {{mvar|S}}, then {{mvar|S}} is non-characteristic. If the data on {{mvar|S}} and the differential equation ''do not'' determine the normal derivative of {{mvar|u}} on {{mvar|S}}, then the surface is '''characteristic''', and the differential equation restricts the data on {{mvar|S}}: the differential equation is ''internal'' to {{mvar|S}}.&lt;br /&gt;
&lt;br /&gt;
The geometric interpretation of this condition is as follows: if data for  are prescribed on the surface , then it may be possible to determine the normal derivative of  on  from the differential equation. If the data on  and the differential equation determine the normal derivative of  on , then  is non-characteristic. If the data on  and the differential equation do not determine the normal derivative of  on , then the surface is characteristic, and the differential equation restricts the data on : the differential equation is internal to .&lt;br /&gt;
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这个条件的几何解释如下: 如果关于 {{mvar|u}} 的数据是在曲面 {{mvar|S}} 上规定的，那么就有可能依据微分方程确定曲面 {{mvar|S}} 上 {{mvar|u}} 的法向导数。如果曲面 {{mvar|S}} 上的数据和上面的微分方程能确定曲面 {{mvar|S}} 上 {{mvar|u}} 的法向导数，那么它就是非特征的。如果曲面 {{mvar|S}} 上的数据和上面的微分方程不能确定曲面 {{mvar|S}} 上 {{mvar|u}} 的法向导数，那么曲面是特征的，并且微分方程将数据限制在曲面 {{mvar|S}} 上：微分方程是在曲面 {{mvar|S}} 内部。&lt;br /&gt;
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# A first-order system {{math|''Lu'' {{=}} 0}} is ''elliptic'' if no surface is characteristic for {{mvar|L}}: the values of {{mvar|u}} on {{mvar|S}} and the differential equation always determine the normal derivative of {{mvar|u}} on {{mvar|S}}.&lt;br /&gt;
&lt;br /&gt;
 A first-order system  0}} is elliptic if no surface is characteristic for : the values of  on  and the differential equation always determine the normal derivative of  on .&lt;br /&gt;
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如果对于 {{mvar|L}} 没有曲面是特征的，则一阶系统 {{math|''Lu'' {{=}} 0}} 是椭圆形的：{{mvar|u}}在 {{mvar|S}} 的值和微分方程总能够决定 {{mvar|S}} 上 {{mvar|u}} 的法向导数。&lt;br /&gt;
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# A first-order system is ''hyperbolic'' at a point if there is a '''spacelike''' surface {{mvar|S}} with normal {{mvar|ξ}} at that point. This means that, given any non-trivial vector {{mvar|η}} orthogonal to {{mvar|ξ}}, and a scalar multiplier {{mvar|λ}}, the equation {{math|''Q''(''λξ'' + ''η'') {{=}} 0}} has {{mvar|m}} real roots {{math|''λ''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;, ''λ''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;,… ''λ''&amp;lt;sub&amp;gt;''m''&amp;lt;/sub&amp;gt;}}. The system is '''strictly hyperbolic''' if these roots are always distinct. The geometrical interpretation of this condition is as follows: the characteristic form {{math|''Q''(''ζ'') {{=}} 0}} defines a cone (the normal cone) with homogeneous coordinates ζ. In the hyperbolic case, this cone has {{mvar|m}} sheets, and the axis {{math|''ζ'' {{=}} ''λξ''}} runs inside these sheets: it does not intersect any of them. But when displaced from the origin by η, this axis intersects every sheet. In the elliptic case, the normal cone has no real sheets.&lt;br /&gt;
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 A first-order system is hyperbolic at a point if there is a spacelike surface  with normal  at that point. This means that, given any non-trivial vector  orthogonal to , and a scalar multiplier , the equation  0}} has  real roots . The system is strictly hyperbolic if these roots are always distinct. The geometrical interpretation of this condition is as follows: the characteristic form  0}} defines a cone (the normal cone) with homogeneous coordinates ζ. In the hyperbolic case, this cone has  sheets, and the axis  λξ}} runs inside these sheets: it does not intersect any of them. But when displaced from the origin by η, this axis intersects every sheet. In the elliptic case, the normal cone has no real sheets.&lt;br /&gt;
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如果在该点存在一个法向量为 {{mvar|ξ}}的 '''&amp;lt;font color=&amp;quot;#ff8000&amp;quot;&amp;gt;类空曲面 Spacclike Surface&amp;lt;/font&amp;gt; {{mvar|S}} ，则一阶系统在那一点是双曲的。这意味着，给定任意正交于 {{mvar|ξ}} 的非平凡向量 {{mvar|η}} 和一个标量乘子 {{mvar|λ}}，方程 {{math|''Q''(''λξ'' + ''η'') {{=}} 0}} 有 {{mvar|m}} 个实根 {{math|''λ''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;, ''λ''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;,… ''λ''&amp;lt;sub&amp;gt;''m''&amp;lt;/sub&amp;gt;}}。如果这些根始终不同，则该系统是严格双曲形的。这个条件的几何解释如下: 特征形式 {{math|''Q''(''ζ'') {{=}} 0}} 定义了一个具有齐次坐标 ζ的圆锥(法线圆锥)。在双曲形的情况下，这个圆锥体有 {{mvar|m}} 层，并且轴 {{math|''ζ'' {{=}} ''λξ''}} 在这些层中运动: 它不与任何一层相交。但是当从原点偏离η时，这条轴线与每一层都相交。在椭圆形的情况下，法向圆锥没有实层。&lt;br /&gt;
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==[[用户:Yuling|Yuling]]（[[用户讨论:Yuling|讨论]]） sheet 这个单词也不很理解，我直译为了“层”&lt;br /&gt;
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=== Equations of mixed type ===&lt;br /&gt;
混合型方程&lt;br /&gt;
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If a PDE has coefficients that are not constant, it is possible that it will not belong to any of these categories but rather be of '''mixed type'''. A simple but important example is the [[Euler–Tricomi equation]]&lt;br /&gt;
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If a PDE has coefficients that are not constant, it is possible that it will not belong to any of these categories but rather be of mixed type. A simple but important example is the Euler–Tricomi equation&lt;br /&gt;
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如果偏微分方程的系数不是常数，那么它可能不属于这些类别中的任何一个，而是属于混合类型。一个简单但重要的例子是欧拉-特里科米方程&lt;br /&gt;
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: &amp;lt;math&amp;gt;u_{xx} = xu_{yy},&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;u_{xx} = xu_{yy},&amp;lt;/math&amp;gt;&lt;br /&gt;
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which is called '''elliptic-hyperbolic''' because it is elliptic in the region {{math|''x'' &amp;lt; 0}}, hyperbolic in the region {{math|''x'' &amp;gt; 0}}, and degenerate parabolic on the line {{math|''x'' {{=}} 0}}.&lt;br /&gt;
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which is called elliptic-hyperbolic because it is elliptic in the region , hyperbolic in the region , and degenerate parabolic on the line  0}}.&lt;br /&gt;
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它在 {{math|''x'' &amp;lt; 0}} 的区域上是椭圆形，在 {{math|''x'' &amp;gt; 0}} 区域上是双曲形，在 {{math|''x'' {{=}} 0}}这条线上是退化为抛物线形，因此称之为椭圆-双曲型。&lt;br /&gt;
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''fill in: Dirichlet and Neumann boundaries, hyperbolic/parabolic/elliptic separation of variables, [[Fourier analysis]], [[Green's function]]s ...--&amp;gt;&lt;br /&gt;
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fill in: Dirichlet and Neumann boundaries, hyperbolic/parabolic/elliptic separation of variables, Fourier analysis, Green's functions ...--&amp;gt;&lt;br /&gt;
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填写: Dirichlet 和 Neumann 边界，双曲 / 抛物线 / 椭圆分离变量法，傅立叶分析，Green 函数... --&lt;br /&gt;
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=== Infinite-order PDEs in quantum mechanics ===&lt;br /&gt;
量子力学中的无限阶偏微分方程&lt;br /&gt;
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In the [[phase space formulation]] of quantum mechanics,  one may consider the [[Method of quantum characteristics|quantum Hamilton's equations]] for trajectories of quantum particles. These equations are infinite-order PDEs. However, in the semiclassical expansion, one has a finite system of ODEs at any fixed order of [[Dirac constant|{{mvar|ħ}}]].  The evolution equation of the [[Wigner quasi-probability distribution|c]] is also an infinite-order PDE. The quantum trajectories are [[Method of quantum characteristics|quantum characteristics]], with the use of which one could calculate the evolution of the Wigner function.&lt;br /&gt;
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In the phase space formulation of quantum mechanics,  one may consider the quantum Hamilton's equations for trajectories of quantum particles. These equations are infinite-order PDEs. However, in the semiclassical expansion, one has a finite system of ODEs at any fixed order of Dirac constant|.  The evolution equation of the Wigner function is also an infinite-order PDE. The quantum trajectories are quantum characteristics, with the use of which one could calculate the evolution of the Wigner function.&lt;br /&gt;
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在量子力学中的相空间表述中，我们可以考虑用于求解量子粒子的轨迹的量子哈密顿的方程。这些方程是无限阶偏微分方程。然而，在半经典展开中，我们在给定[[Dirac constant|{{mvar|ħ}}]]阶数下有一个有限的的常微分方程组。'''&amp;lt;font color=&amp;quot;#ff8000&amp;quot;&amp;gt;维格纳函数  Wigner Function&amp;lt;/font&amp;gt;的演化方程也是一个无限阶偏微分方程。由于量子轨道的量子特性，所以它通常可以用来计算维格纳函数的演化。&lt;br /&gt;
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== Analytical solutions ==&lt;br /&gt;
解析解&lt;br /&gt;
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===Separation of variables===&lt;br /&gt;
分离变量法&lt;br /&gt;
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{{main|Separable partial differential equation}}&lt;br /&gt;
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Linear PDEs can be reduced to systems of ordinary differential equations by the important technique of separation of variables. This technique rests on a characteristic of solutions to differential equations: if one can find any solution that solves the equation and satisfies the boundary conditions, then it is ''the'' solution (this also applies to ODEs). We assume as an [[ansatz]] that the dependence of a solution on the parameters space and time can be written as a product of terms that each depend on a single parameter, and then see if this can be made to solve the problem.&amp;lt;ref&amp;gt;{{cite book|last1=Gershenfeld|first1=Neil|title=The nature of mathematical modeling|date=2000|publisher=Cambridge Univ. Press|location=Cambridge|isbn=0521570956|page=27|edition=Reprinted (with corr.)}}&amp;lt;/ref&amp;gt;&lt;br /&gt;
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Linear PDEs can be reduced to systems of ordinary differential equations by the important technique of separation of variables. This technique rests on a characteristic of solutions to differential equations: if one can find any solution that solves the equation and satisfies the boundary conditions, then it is the solution (this also applies to ODEs). We assume as an ansatz that the dependence of a solution on the parameters space and time can be written as a product of terms that each depend on a single parameter, and then see if this can be made to solve the problem.&lt;br /&gt;
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线性偏微分方程组可以通过分离变量法这一重要方法来简化为常微分方程组。这种方法依赖于微分方程解的一个特征: 如果能找到任何一个满足方程和边界条件的解，那么这个解就是方程的解(这也适用于常微分方程)。我们假设解对参数空间和时间的依赖可以写成对它们每一项的依赖以及一个参数的乘积，然后再看看这是否可以用来解决这个问题。&lt;br /&gt;
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In the method of separation of variables, one reduces a PDE to a PDE in fewer variables, which is an ordinary differential equation if in one variable – these are in turn easier to solve.&lt;br /&gt;
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In the method of separation of variables, one reduces a PDE to a PDE in fewer variables, which is an ordinary differential equation if in one variable – these are in turn easier to solve.&lt;br /&gt;
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在分离变量法方法中，可以将偏微分方程简化为含有更少变量的偏微分方程，如果只有一个变量，那么就变成了一个'''&amp;lt;font color = &amp;quot;#ff8000&amp;quot;&amp;gt;常微分方程 Ordinary Differential Equation&amp;lt;/font&amp;gt;'''-- 反过来，这些方程也更容易求解。&lt;br /&gt;
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This is possible for simple PDEs, which are called [[separable partial differential equation]]s, and the domain is generally a rectangle (a product of intervals). Separable PDEs correspond to [[diagonal matrices]] – thinking of &amp;quot;the value for fixed {{mvar|x}}&amp;quot; as a coordinate, each coordinate can be understood separately.&lt;br /&gt;
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This is possible for simple PDEs, which are called separable partial differential equations, and the domain is generally a rectangle (a product of intervals). Separable PDEs correspond to diagonal matrices – thinking of &amp;quot;the value for fixed &amp;quot; as a coordinate, each coordinate can be understood separately.&lt;br /&gt;
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对于简单的偏微分方程(称为可分离偏微分方程)来说，这是可能的，而且方程通常定义在一个矩形区域(区间的乘积)上。可分离偏微分方程对应于对角线矩阵——以“固定值”为坐标，每个坐标可分开理解。&lt;br /&gt;
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This generalizes to the [[method of characteristics]], and is also used in [[integral transform]]s.&lt;br /&gt;
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This generalizes to the method of characteristics, and is also used in integral transforms.&lt;br /&gt;
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这种方法可以推广到特征曲线法，也可以用于积分变换。&lt;br /&gt;
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===Method of characteristics===&lt;br /&gt;
特征曲线法&lt;br /&gt;
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{{main|Method of characteristics}}&lt;br /&gt;
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In special cases, one can find characteristic curves on which the equation reduces to an ODE – changing coordinates in the domain to straighten these curves allows separation of variables, and is called the [[method of characteristics]].&lt;br /&gt;
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In special cases, one can find characteristic curves on which the equation reduces to an ODE – changing coordinates in the domain to straighten these curves allows separation of variables, and is called the method of characteristics.&lt;br /&gt;
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在特殊情况下，可以找到一些特征曲线，在这些曲线上方程可以变成一个常微分方程——意味着改变坐标从而使这些曲线变直从而达到分离变量的目的，这就是所谓的特征曲线法。&lt;br /&gt;
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More generally, one may find characteristic surfaces.&lt;br /&gt;
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More generally, one may find characteristic surfaces.&lt;br /&gt;
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更一般地说，人们可能会找到特征表面。&lt;br /&gt;
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===Integral transform===&lt;br /&gt;
积分变换&lt;br /&gt;
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An [[integral transform]] may transform the PDE to a simpler one, in particular, a separable PDE. This corresponds to diagonalizing an operator.&lt;br /&gt;
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An integral transform may transform the PDE to a simpler one, in particular, a separable PDE. This corresponds to diagonalizing an operator.&lt;br /&gt;
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积分变换可以将偏微分方程转换为更简单的偏微分方程，特别是可分离的偏微分方程。这对应于对角化算符。&lt;br /&gt;
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An important example of this is [[Fourier analysis]], which diagonalizes the heat equation using the [[eigenbasis]] of sinusoidal waves.&lt;br /&gt;
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An important example of this is Fourier analysis, which diagonalizes the heat equation using the eigenbasis of sinusoidal waves.&lt;br /&gt;
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这方面的一个重要例子是'''&amp;lt;font color = &amp;quot;#ff8000&amp;quot;&amp;gt;傅里叶分析  Fourier Analysis&amp;lt;/font&amp;gt;'''，它使用正弦波的特征基来对角化热方程。&lt;br /&gt;
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If the domain is finite or periodic, an infinite sum of solutions such as a [[Fourier series]] is appropriate, but an integral of solutions such as a [[Fourier integral]] is generally required for infinite domains. The solution for a point source for the heat equation given above is an example of the use of a Fourier integral.&lt;br /&gt;
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If the domain is finite or periodic, an infinite sum of solutions such as a Fourier series is appropriate, but an integral of solutions such as a Fourier integral is generally required for infinite domains. The solution for a point source for the heat equation given above is an example of the use of a Fourier integral.&lt;br /&gt;
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如果区域是有限的或周期性的，那么解为无限和的形式是恰当的，例如傅里叶级数，但是一个解的积分，例如傅立叶积分，一般是在无限区域上的。上面给出的热传导方程的点源解法就是使用傅里叶积分的一个例子。&lt;br /&gt;
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===Change of variables===&lt;br /&gt;
变量代换&lt;br /&gt;
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Often a PDE can be reduced to a simpler form with a known solution by a suitable [[Change of variables (PDE)|change of variables]].  For example, the [[Black–Scholes equation#Derivation|Black–Scholes]] PDE&lt;br /&gt;
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Often a PDE can be reduced to a simpler form with a known solution by a suitable change of variables.  For example, the Black–Scholes PDE&lt;br /&gt;
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偏微分方程通常可以通过变量的适当变化，用已知的解简化为更简单的形式。例如，布莱克-舒尔斯偏微分方程&lt;br /&gt;
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:&amp;lt;math&amp;gt; \frac{\partial V}{\partial t} + \tfrac{1}{2}\sigma^2 S^2\frac{\partial^2 V}{\partial S^2} + rS\frac{\partial V}{\partial S} - rV = 0 &amp;lt;/math&amp;gt;&lt;br /&gt;
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&amp;lt;math&amp;gt; \frac{\partial V}{\partial t} + \tfrac{1}{2}\sigma^2 S^2\frac{\partial^2 V}{\partial S^2} + rS\frac{\partial V}{\partial S} - rV = 0 &amp;lt;/math&amp;gt;&lt;br /&gt;
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is reducible to the [[heat equation]]&lt;br /&gt;
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is reducible to the heat equation&lt;br /&gt;
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可以简化为热传导方程&lt;br /&gt;
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:&amp;lt;math&amp;gt; \frac{\partial u}{\partial \tau} = \frac{\partial^2 u}{\partial x^2}&amp;lt;/math&amp;gt;&lt;br /&gt;
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&amp;lt;math&amp;gt; \frac{\partial u}{\partial \tau} = \frac{\partial^2 u}{\partial x^2}&amp;lt;/math&amp;gt;&lt;br /&gt;
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by the change of variables (for complete details see {{webarchive |url=https://web.archive.org/web/20080411030405/http://www.math.unl.edu/~sdunbar1/Teaching/MathematicalFinance/Lessons/BlackScholes/Solution/solution.shtml |date=April 11, 2008 |title=Solution of the Black Scholes Equation }})&lt;br /&gt;
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by the change of variables (for complete details see )&lt;br /&gt;
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通过变量替换(完整的细节见)&lt;br /&gt;
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:&amp;lt;math&amp;gt;\begin{align}&lt;br /&gt;
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V(S,t) &amp;amp;= K v(x,\tau),\\[5px]&lt;br /&gt;
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x &amp;amp;= \ln\left(\tfrac{S}{K} \right),\\[5px]&lt;br /&gt;
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\tau &amp;amp;= \tfrac{1}{2} \sigma^2 (T - t),\\[5px]&lt;br /&gt;
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v(x,\tau)&amp;amp;=e^{-\alpha x-\beta\tau} u(x,\tau).&lt;br /&gt;
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\end{align}&amp;lt;/math&amp;gt;&lt;br /&gt;
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===Fundamental solution===&lt;br /&gt;
基本解&lt;br /&gt;
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{{main|Fundamental solution}}&lt;br /&gt;
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Inhomogeneous equations can often be solved (for constant coefficient PDEs, always be solved) by finding the [[fundamental solution]] (the solution for a point source), then taking the [[convolution]] with the boundary conditions to get the solution.&lt;br /&gt;
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Inhomogeneous equations can often be solved (for constant coefficient PDEs, always be solved) by finding the fundamental solution (the solution for a point source), then taking the convolution with the boundary conditions to get the solution.&lt;br /&gt;
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非齐次方程(常系数偏微分方程)一般是通过先求出基本解(点源的解) ，然后利用带边界条件的卷积来求解。&lt;br /&gt;
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This is analogous in [[signal processing]] to understanding a filter by its [[impulse response]].&lt;br /&gt;
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This is analogous in signal processing to understanding a filter by its impulse response.&lt;br /&gt;
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这类似于在信号处理中通过滤波器的脉冲响应来理解滤波器。&lt;br /&gt;
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===Superposition principle===&lt;br /&gt;
叠加原理&lt;br /&gt;
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{{further| Superposition principle }}&lt;br /&gt;
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The superposition principle applies to any linear system, including linear systems of PDEs. A common visualization of this concept is the interaction of two waves in phase being combined to result in a greater amplitude, for example {{math|sin ''x'' + sin ''x'' {{=}} 2 sin ''x''}}. The same principle can be observed in PDEs where the solutions may be real or complex and additive. [[Superposition principle|superposition]]&lt;br /&gt;
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The superposition principle applies to any linear system, including linear systems of PDEs. A common visualization of this concept is the interaction of two waves in phase being combined to result in a greater amplitude, for example  2 sin x}}. The same principle can be observed in PDEs where the solutions may be real or complex and additive. superposition&lt;br /&gt;
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'''&amp;lt;font color = &amp;quot;#ff8000&amp;quot;&amp;gt;叠加原理 Superposition Principle&amp;lt;/font&amp;gt;适用于任何线性系统，包括偏微分方程的线性系统。这个概念的一个常见的可视化是两个同相位的波相互作用结合在一起会产生更大的振幅，例如 {{math|sin ''x'' + sin ''x'' {{=}} 2 sin ''x''}}。在偏微分方程中也可以观察到同样的原理，其中的解可能是真实的或复杂的和可加的。叠加&lt;br /&gt;
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If {{math|''u''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;}} and {{math|''u''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;}} are solutions of linear PDE in some function space {{mvar|R}}, then {{math|''u'' {{=}} ''c''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;''u''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; + ''c''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;''u''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;}} with any constants {{math|''c''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;}} and {{math|''c''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;}} are also a solution of that PDE in the same function space.&lt;br /&gt;
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If  and  are solutions of linear PDE in some function space , then  c&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;u&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; + c&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;u&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;}} with any constants  and  are also a solution of that PDE in the same function space.&lt;br /&gt;
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若线性偏微分方程在某个函数空间{{mvar|R}}中有解{{math|''u''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;}} 和 {{math|''u''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;}}，则{{math|''u'' {{=}} ''c''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;''u''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; + ''c''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;''u''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;}}也是该偏微分方程在同一函数空间中的解，其中{{math|''c''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;}} 和 {{math|''c''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;}} 是任意常数。&lt;br /&gt;
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===Methods for non-linear equations===&lt;br /&gt;
非线性方程的求解方法&lt;br /&gt;
{{see also|nonlinear partial differential equation}}&lt;br /&gt;
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There are no generally applicable methods to solve nonlinear PDEs. Still, existence and uniqueness results (such as the [[Cauchy–Kowalevski theorem]]) are often possible, as are proofs of important qualitative and quantitative properties of solutions (getting these results is a major part of [[mathematical analysis|analysis]]). Computational solution to the nonlinear PDEs, the [[split-step method]], exist for specific equations like [[nonlinear Schrödinger equation]].&lt;br /&gt;
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There are no generally applicable methods to solve nonlinear PDEs. Still, existence and uniqueness results (such as the Cauchy–Kowalevski theorem) are often possible, as are proofs of important qualitative and quantitative properties of solutions (getting these results is a major part of analysis). Computational solution to the nonlinear PDEs, the split-step method, exist for specific equations like nonlinear Schrödinger equation.&lt;br /&gt;
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对于非线性偏微分方程，目前还没有普遍适用的求解方法。然而，通常是可能知道解的存在性和唯一性(如柯西-科瓦列夫斯基定理)，也是可能得到解的重要定性和定量性质的证明(得到这些结果是分析的主要部分)。非线性偏微分方程的计算解，即分步法，对一些特定的方程适用，比如非线性'''&amp;lt;font color=&amp;quot;#ff8000&amp;quot;&amp;gt;薛定谔方程 Schrödinger equation&amp;lt;/font&amp;gt;'''。&lt;br /&gt;
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Nevertheless, some techniques can be used for several types of equations. The [[h-principle|{{mvar|h}}-principle]] is the most powerful method to solve [[Underdetermined system|underdetermined]] equations. The [[Riquier–Janet theory]] is an effective method for obtaining information about many analytic [[Overdetermined system|overdetermined]] systems.&lt;br /&gt;
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Nevertheless, some techniques can be used for several types of equations. The -principle is the most powerful method to solve underdetermined equations. The Riquier–Janet theory is an effective method for obtaining information about many analytic overdetermined systems.&lt;br /&gt;
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然而，一些技巧可以用于几种类型的方程。h-原理是求解欠定方程最有效的方法。里基尔-珍妮特理论是一种可以获得许多解析超定系统信息的有效方法。&lt;br /&gt;
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The [[method of characteristics]] can be used in some very special cases to solve partial differential equations.&lt;br /&gt;
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The method of characteristics can be used in some very special cases to solve partial differential equations.&lt;br /&gt;
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特征线法可用于求解某些特殊情况下的偏微分方程。&lt;br /&gt;
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In some cases, a PDE can be solved via [[perturbation analysis]] in which the solution is considered to be a correction to an equation with a known solution. Alternatives are [[numerical analysis]] techniques from simple [[finite difference]] schemes to the more mature [[multigrid]] and [[finite element method]]s. Many interesting problems in science and engineering are solved in this way using [[computer]]s, sometimes high performance [[supercomputer]]s.&lt;br /&gt;
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In some cases, a PDE can be solved via perturbation analysis in which the solution is considered to be a correction to an equation with a known solution. Alternatives are numerical analysis techniques from simple finite difference schemes to the more mature multigrid and finite element methods. Many interesting problems in science and engineering are solved in this way using computers, sometimes high performance supercomputers.&lt;br /&gt;
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在某些情况下，偏微分方程可以通过扰动分析来求解。在扰动分析中，通常是求解将具有已知解的方程修正后的新得到方程。可供选择的数值分析技术从简单的差分格式到更成熟的多重网格和有限元方法。许多有趣的科学和工程问题都是在计算机上用这种方法解决的，有时是高性能超级计算机。&lt;br /&gt;
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===Lie group method===&lt;br /&gt;
李群方法&lt;br /&gt;
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From 1870 [[Sophus Lie]]'s work put the theory of differential equations on a more satisfactory foundation. He showed that the integration theories of the older mathematicians can, by the introduction of what are now called [[Lie group]]s, be referred, to a common source; and that ordinary differential equations which admit the same [[infinitesimal transformation]]s present comparable difficulties of integration. He also emphasized the subject of [[contact transformation|transformations of contact]].&lt;br /&gt;
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From 1870 Sophus Lie's work put the theory of differential equations on a more satisfactory foundation. He showed that the integration theories of the older mathematicians can, by the introduction of what are now called Lie groups, be referred, to a common source; and that ordinary differential equations which admit the same infinitesimal transformations present comparable difficulties of integration. He also emphasized the subject of transformations of contact.&lt;br /&gt;
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从1870年起，索弗斯·李的工作为微分方程理论奠定了一个较为令人满意的基础。他指出，通过引入现在所谓的李群，老一辈数学家的积分理论可以引用到一个共同的来源; 承认相同的无穷小变换的常微分方程在积分方面存在相当的困难。他还强调了接触的转变这一主题。&lt;br /&gt;
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==[[用户:Yuling|Yuling]]（[[用户讨论:Yuling|讨论]]）这句话“He also emphasized the subject of transformations of contact.”中的transformations of contact翻译的不太好。&lt;br /&gt;
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A general approach to solving PDEs uses the symmetry property of differential equations, the continuous [[infinitesimal transformation]]s of solutions to solutions ([[Lie theory]]). Continuous [[group theory]], [[Lie algebras]] and [[differential geometry]] are used to understand the structure of linear and nonlinear partial differential equations for generating integrable equations, to find its [[Lax pair]]s, recursion operators, [[Bäcklund transform]] and finally finding exact analytic solutions to the PDE.&lt;br /&gt;
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A general approach to solving PDEs uses the symmetry property of differential equations, the continuous infinitesimal transformations of solutions to solutions (Lie theory). Continuous group theory, Lie algebras and differential geometry are used to understand the structure of linear and nonlinear partial differential equations for generating integrable equations, to find its Lax pairs, recursion operators, Bäcklund transform and finally finding exact analytic solutions to the PDE.&lt;br /&gt;
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求解偏微分方程的一般方法是利用微分方程的对称性，即解到解的连续无穷小变换(李理论)。连续群论、李代数和微分几何理论被用来理解生成可积方程的线性和非线性偏微分方程的结构，找到它的Lax对、递归算子、 贝克伦德变换，最后找到偏微分方程的精确解析解。&lt;br /&gt;
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Symmetry methods have been recognized to study differential equations arising in mathematics, physics, engineering, and many other disciplines.&lt;br /&gt;
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Symmetry methods have been recognized to study differential equations arising in mathematics, physics, engineering, and many other disciplines.&lt;br /&gt;
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对称方法已被公认可以用于研究出现在数学，物理，工程和许多其他学科的微分方程。&lt;br /&gt;
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===Semianalytical methods===&lt;br /&gt;
半解析方法&lt;br /&gt;
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The [[Adomian decomposition method]], the [[Aleksandr Lyapunov|Lyapunov]] artificial small parameter method, and He's [[homotopy perturbation method]] are all special cases of the more general [[homotopy analysis method]]. These are series expansion methods, and except for the Lyapunov method, are independent of small physical parameters as compared to the well known [[perturbation theory]], thus giving these methods greater flexibility and solution generality.&lt;br /&gt;
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The Adomian decomposition method, the Lyapunov artificial small parameter method, and He's homotopy perturbation method are all special cases of the more general homotopy analysis method. These are series expansion methods, and except for the Lyapunov method, are independent of small physical parameters as compared to the well known perturbation theory, thus giving these methods greater flexibility and solution generality.&lt;br /&gt;
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阿多米安分解法、李雅普诺夫人工小参数方法和何同伦摄动方法都是更一般的同伦分析方法的特殊情况。除了李雅普诺夫方法之外，这些都是级数展开方法，与为人熟知的摄动理论方法相比，它们与小的物理参数无关，因此这些方法具有更大的灵活性和解的通用性。&lt;br /&gt;
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== Numerical solutions ==&lt;br /&gt;
数值解&lt;br /&gt;
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The three most widely used [[Numerical partial differential equations|numerical methods to solve PDEs]] are the [[finite element analysis|finite element method]] (FEM), [[finite volume method]]s (FVM) and [[finite difference method]]s (FDM), as well other kind of methods called [[Meshfree methods]], which were made to solve problems where the before mentioned methods are limited. The FEM has a prominent position among these methods and especially its exceptionally efficient higher-order version [[hp-FEM]]. Other hybrid versions of FEM and Meshfree methods include the generalized finite element method (GFEM), [[extended finite element method]] (XFEM), [[Spectral element method|spectral finite element method]] (SFEM), [[Meshfree methods|meshfree finite element method]], [[Discontinuous Galerkin Method|discontinuous Galerkin finite element method]] (DGFEM), [[Element-Free Galerkin Method]] (EFGM), [[Interpolating Element-Free Galerkin Method]] (IEFGM), etc.&lt;br /&gt;
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The three most widely used numerical methods to solve PDEs are the finite element method (FEM), finite volume methods (FVM) and finite difference methods (FDM), as well other kind of methods called Meshfree methods, which were made to solve problems where the before mentioned methods are limited. The FEM has a prominent position among these methods and especially its exceptionally efficient higher-order version hp-FEM. Other hybrid versions of FEM and Meshfree methods include the generalized finite element method (GFEM), extended finite element method (XFEM), spectral finite element method (SFEM), meshfree finite element method, discontinuous Galerkin finite element method (DGFEM), Element-Free Galerkin Method (EFGM), Interpolating Element-Free Galerkin Method (IEFGM), etc.&lt;br /&gt;
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求解偏微分方程最常用的三种数值方法是有限元分析法、有限体积法和有限差分法，以及其他一些称为无网格法的方法。这些方法用于解决前面提到的方法受到的限制。在这些方法中，有限元方法，尤其是高效的高阶有限元方法，占有重要地位。其他有限元法和无网格法的混合形式包括广义有限元分析法(GFEM)、扩展有限元分析法(XFEM)、谱有限元分析法(SFEM)、无网格有限元分析法(DGFEM)、间断伽辽金有限元分析法(DGFEM)、无网格伽辽金法(EFGM)、插值无网格伽辽金法(IEFGM)等。&lt;br /&gt;
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=== Finite element method ===&lt;br /&gt;
有限元分析法&lt;br /&gt;
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{{main|Finite element method}}&lt;br /&gt;
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The finite element method (FEM) (its practical application often known as finite element analysis (FEA)) is a numerical technique for finding approximate solutions of partial differential equations (PDE) as well as of integral equations. The solution approach is based either on eliminating the differential equation completely (steady state problems), or rendering the PDE into an approximating system of ordinary differential equations, which are then numerically integrated using standard techniques such as Euler's method, Runge–Kutta, etc.&lt;br /&gt;
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The finite element method (FEM) (its practical application often known as finite element analysis (FEA)) is a numerical technique for finding approximate solutions of partial differential equations (PDE) as well as of integral equations. The solution approach is based either on eliminating the differential equation completely (steady state problems), or rendering the PDE into an approximating system of ordinary differential equations, which are then numerically integrated using standard techniques such as Euler's method, Runge–Kutta, etc.&lt;br /&gt;
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'''&amp;lt;font color = &amp;quot;#ff8000&amp;quot;&amp;gt;有限元分析法 Finite Element Method&amp;lt;/font&amp;gt;''' ((其实际应用通常被称为有限元分析(FEA))是一种寻找偏微分方程(PDE)和积分方程近似解的数值技术。这种求解方法要么基于完全消除微分方程(稳态问题) ，要么将偏微分方程转化为常微分方程的近似系统，然后使用标准技术进行数值积分，如欧拉方法、 Runge-Kutta 等。&lt;br /&gt;
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===Finite difference method===&lt;br /&gt;
有限差分法&lt;br /&gt;
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{{main|Finite difference method}}&lt;br /&gt;
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Finite-difference methods are numerical methods for approximating the solutions to differential equations using [[finite difference]] equations to approximate derivatives.&lt;br /&gt;
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Finite-difference methods are numerical methods for approximating the solutions to differential equations using finite difference equations to approximate derivatives.&lt;br /&gt;
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有限差分法是一种数值方法，用差分方程近似微分方程的解。&lt;br /&gt;
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=== Finite volume method ===&lt;br /&gt;
有限体积法&lt;br /&gt;
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{{main|Finite volume method}}&lt;br /&gt;
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Similar to the finite difference method or finite element method, values are calculated at discrete places on a meshed geometry. &amp;quot;Finite volume&amp;quot; refers to the small volume surrounding each node point on a mesh. In the finite volume method, surface integrals in a partial differential equation that contain a divergence term are converted to volume integrals, using the [[divergence theorem]]. These terms are then evaluated as fluxes at the surfaces of each finite volume. Because the flux entering a given volume is identical to that leaving the adjacent volume, these methods conserve mass by design.&lt;br /&gt;
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Similar to the finite difference method or finite element method, values are calculated at discrete places on a meshed geometry. &amp;quot;Finite volume&amp;quot; refers to the small volume surrounding each node point on a mesh. In the finite volume method, surface integrals in a partial differential equation that contain a divergence term are converted to volume integrals, using the divergence theorem. These terms are then evaluated as fluxes at the surfaces of each finite volume. Because the flux entering a given volume is identical to that leaving the adjacent volume, these methods conserve mass by design.&lt;br /&gt;
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类似于有限差分法或有限元分析，函数值是在网状几何体上的离散位置进行计算的。“有限体积”是指网格上每个节点周围的小体积。在有限体积法中，偏微分方程中含有散度项的面积分用散度定理积分转换成体积分。然后将这些项用于估算每个有限体积表面上的通量。由于进入给定体积的通量与转移到相邻体积元的通量相同，所以这些方法在设计上保证了质量守恒。&lt;br /&gt;
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==See also==&lt;br /&gt;
请参阅&lt;br /&gt;
* [[Dirichlet boundary condition]]&lt;br /&gt;
狄利克雷边界条件&lt;br /&gt;
* [[Jet bundle]]&lt;br /&gt;
射流丛&lt;br /&gt;
* [[Laplace transform applied to differential equations]]&lt;br /&gt;
微分方程中的拉普拉斯变换&lt;br /&gt;
* [[List of dynamical systems and differential equations topics]]&lt;br /&gt;
动力学系统和微分方程的列表&lt;br /&gt;
* [[Matrix differential equation]]&lt;br /&gt;
矩阵微分方程&lt;br /&gt;
* [[Neumann boundary condition]]&lt;br /&gt;
诺伊曼边界条件&lt;br /&gt;
* [[Numerical partial differential equations]]&lt;br /&gt;
数值偏微分方程&lt;br /&gt;
* [[Partial differential algebraic equation]]&lt;br /&gt;
偏微分代数方程&lt;br /&gt;
* [[Recurrence relation]]&lt;br /&gt;
递推关系&lt;br /&gt;
* [[Robin boundary condition]]&lt;br /&gt;
罗宾边界条件&lt;br /&gt;
* [[Stochastic processes and boundary value problems]]&lt;br /&gt;
随机过程和边值问题&lt;br /&gt;
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== The energy method ==&lt;br /&gt;
能量法&lt;br /&gt;
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The energy method is a mathematical procedure that can be used to verify well-posedness of initial-boundary-value-problems.&amp;lt;ref&amp;gt;{{cite book |title=High Order Difference Methods for Time Dependent PDE&lt;br /&gt;
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The energy method is a mathematical procedure that can be used to verify well-posedness of initial-boundary-value-problems.&amp;lt;ref&amp;gt;{{cite book |title=High Order Difference Methods for Time Dependent PDE&lt;br /&gt;
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能量法是验证初边值问题适定性的一种数学方法。 时变偏微分方程的高阶差分方法&lt;br /&gt;
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|first=Bertil|last=Gustafsson|publisher=Springer|year=2008|isbn=978-3-540-74992-9|doi=10.1007/978-3-540-74993-6}}&amp;lt;/ref&amp;gt; In the following example the energy method is used to decide where and which boundary conditions should be imposed such that the resulting IBVP is well-posed. Consider the one-dimensional hyperbolic PDE given by&lt;br /&gt;
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|first=Bertil|last=Gustafsson|publisher=Springer|year=2008|isbn=978-3-540-74992-9|doi=10.1007/978-3-540-74993-6}}&amp;lt;/ref&amp;gt; In the following example the energy method is used to decide where and which boundary conditions should be imposed such that the resulting IBVP is well-posed. Consider the one-dimensional hyperbolic PDE given by&lt;br /&gt;
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| first Bertil | last Gustafsson | publisher | Springer | year 2008 | isbn 978-3-540-74992-9 | doi 10.1007 / 978-3-540-74993-6} / ref 在下面的例子中，使用能量方法来决定应该施加哪些边界条件，使得得到的 IBVP适定。考虑一维双曲偏微分方程&lt;br /&gt;
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: &amp;lt;math&amp;gt;\frac{\partial u}{\partial t} + \alpha \frac{\partial u}{\partial x} = 0, \quad x \in [a,b], \operatorname t &amp;gt; 0,&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;\frac{\partial u}{\partial t} + \alpha \frac{\partial u}{\partial x} = 0, \quad x \in [a,b], \operatorname t &amp;gt; 0,&amp;lt;/math&amp;gt;&lt;br /&gt;
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where &amp;lt;math&amp;gt;\alpha \neq 0&amp;lt;/math&amp;gt; is a constant and &amp;lt;math&amp;gt;u(x,t)&amp;lt;/math&amp;gt; is an unknown function with initial condition &amp;lt;math&amp;gt;u(x,0) = f(x)&amp;lt;/math&amp;gt;. Multiplying with &amp;lt;math&amp;gt;u&amp;lt;/math&amp;gt; and integrating over the domain gives&lt;br /&gt;
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where &amp;lt;math&amp;gt;\alpha \neq 0&amp;lt;/math&amp;gt; is a constant and &amp;lt;math&amp;gt;u(x,t)&amp;lt;/math&amp;gt; is an unknown function with initial condition &amp;lt;math&amp;gt;u(x,0) = f(x)&amp;lt;/math&amp;gt;. Multiplying with &amp;lt;math&amp;gt;u&amp;lt;/math&amp;gt; and integrating over the domain gives&lt;br /&gt;
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其中 &amp;lt;math&amp;gt;\alpha \neq 0&amp;lt;/math&amp;gt; 是常数，并且 &amp;lt;math&amp;gt;u(x,t)&amp;lt;/math&amp;gt; 是未知函数，初始条件是 &amp;lt;math&amp;gt;u(x,0) = f(x)&amp;lt;/math&amp;gt;。乘以 &amp;lt;math&amp;gt;u&amp;lt;/math&amp;gt; 并在域上进行积分。&lt;br /&gt;
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: &amp;lt;math&amp;gt;\int_a^b u \frac{\partial u}{\partial t} \operatorname dx + \alpha \int _a ^b u \frac{\partial u}{\partial x} \operatorname dx = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;\int_a^b u \frac{\partial u}{\partial t} \operatorname dx + \alpha \int _a ^b u \frac{\partial u}{\partial x} \operatorname dx = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
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Using that&lt;br /&gt;
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Using that&lt;br /&gt;
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利用这一点&lt;br /&gt;
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: &amp;lt;math&amp;gt;\int _a ^b u \frac{\partial u}{\partial t} \operatorname dx = \frac{1}{2} \frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 \quad \text{and} \quad \int _a ^b u \frac{\partial u}{\partial x} \operatorname dx = \frac{1}{2} u(b,t)^2 - \frac{1}{2} u(a,t)^2,.&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;\int _a ^b u \frac{\partial u}{\partial t} \operatorname dx = \frac{1}{2} \frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 \quad \text{and} \quad \int _a ^b u \frac{\partial u}{\partial x} \operatorname dx = \frac{1}{2} u(b,t)^2 - \frac{1}{2} u(a,t)^2,.&amp;lt;/math&amp;gt;&lt;br /&gt;
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where integration by parts has been used for the second relationship, we get&lt;br /&gt;
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where integration by parts has been used for the second relationship, we get&lt;br /&gt;
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第二个关系中采用了分部积分法，我们可以得到&lt;br /&gt;
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: &amp;lt;math&amp;gt;\frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 + \alpha u(b,t)^2 - \alpha u(a,t)^2 = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;\frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 + \alpha u(b,t)^2 - \alpha u(a,t)^2 = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
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Here &amp;lt;math&amp;gt;\vert \vert \cdot \vert \vert&amp;lt;/math&amp;gt; denotes the standard L2-norm.&lt;br /&gt;
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Here &amp;lt;math&amp;gt;\vert \vert \cdot \vert \vert&amp;lt;/math&amp;gt; denotes the standard L2-norm.&lt;br /&gt;
&lt;br /&gt;
在这里，&amp;lt;math&amp;gt;\vert \vert \cdot \vert \vert&amp;lt;/math&amp;gt; 表示标准的 L2-正则。&lt;br /&gt;
&lt;br /&gt;
For well-posedness we require that the energy of the solution is non-increasing, i.e. that &amp;lt;math&amp;gt;\frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 \leq 0&amp;lt;/math&amp;gt;, which is achieved by specifying &amp;lt;math&amp;gt;u&amp;lt;/math&amp;gt; at &amp;lt;math&amp;gt;x = a&amp;lt;/math&amp;gt; if &amp;lt;math&amp;gt;\alpha &amp;gt; 0&amp;lt;/math&amp;gt; and at &amp;lt;math&amp;gt;x = b&amp;lt;/math&amp;gt; if &amp;lt;math&amp;gt;\alpha &amp;lt; 0&amp;lt;/math&amp;gt;. This corresponds to only imposing boundary conditions at the inflow. Note that well-posedness allows for growth in terms of data (initial and boundary) and thus it is sufficient to show that &amp;lt;math&amp;gt;\frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 \leq 0&amp;lt;/math&amp;gt; holds when all data is set to zero.&lt;br /&gt;
&lt;br /&gt;
For well-posedness we require that the energy of the solution is non-increasing, i.e. that &amp;lt;math&amp;gt;\frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 \leq 0&amp;lt;/math&amp;gt;, which is achieved by specifying &amp;lt;math&amp;gt;u&amp;lt;/math&amp;gt; at &amp;lt;math&amp;gt;x = a&amp;lt;/math&amp;gt; if &amp;lt;math&amp;gt;\alpha &amp;gt; 0&amp;lt;/math&amp;gt; and at &amp;lt;math&amp;gt;x = b&amp;lt;/math&amp;gt; if &amp;lt;math&amp;gt;\alpha &amp;lt; 0&amp;lt;/math&amp;gt;. This corresponds to only imposing boundary conditions at the inflow. Note that well-posedness allows for growth in terms of data (initial and boundary) and thus it is sufficient to show that &amp;lt;math&amp;gt;\frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 \leq 0&amp;lt;/math&amp;gt; holds when all data is set to zero.&lt;br /&gt;
&lt;br /&gt;
对于适定性，我们要解的能量是不增加的，即 &amp;lt;math&amp;gt;\frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 \leq 0&amp;lt;/math&amp;gt; ，这种关系可以通过在&amp;lt;math&amp;gt;x = a&amp;lt;/math&amp;gt;处 （如果 &amp;lt;math&amp;gt;\alpha &amp;gt; 0&amp;lt;/math&amp;gt;） 以及 &amp;lt;math&amp;gt;x = b&amp;lt;/math&amp;gt;处 （如果 &amp;lt;math&amp;gt;\alpha &amp;lt; 0&amp;lt;/math&amp;gt;）指定&amp;lt;math&amp;gt;u&amp;lt;/math&amp;gt;的值来实现。这只相当于在入流处附加边界条件。注意，适定性允许在数据(初始和边界)上的增长，因此它足以表明当所有数据设置为零时应有 &amp;lt;math&amp;gt;\frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 \leq 0&amp;lt;/math&amp;gt;。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==[[用户:Yuling|Yuling]]（[[用户讨论:Yuling|讨论]]）“This corresponds to only imposing boundary conditions at the inflow.” 这句话中的inflow不是很理解&lt;br /&gt;
&lt;br /&gt;
==Notes==&lt;br /&gt;
&lt;br /&gt;
{{Reflist}}&lt;br /&gt;
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&lt;br /&gt;
== References ==&lt;br /&gt;
&lt;br /&gt;
{{refbegin|2}}&lt;br /&gt;
&lt;br /&gt;
* {{cite book |title=Solving Frontier problems of Physics: The decomposition method&lt;br /&gt;
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|first=G.|last=Adomian|publisher=Kluwer Academic Publishers|year=1994|isbn=|page=|url=https://books.google.com/books?id=UKPqCAAAQBAJ&amp;amp;printsec=frontcover#v=onepage&amp;amp;q=%22partial%20differential%22&amp;amp;f=false}}&lt;br /&gt;
&lt;br /&gt;
|first=G.|last=Adomian|publisher=Kluwer Academic Publishers|year=1994|isbn=|page=|url=https://books.google.com/books?id=UKPqCAAAQBAJ&amp;amp;printsec=frontcover#v=onepage&amp;amp;q=%22partial%20differential%22&amp;amp;f=false}}&lt;br /&gt;
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1994年 | isbn | 页面 | 网址: 施普林格科学+商业媒体 https://books.google.com/books?id=ukpqcaaaqbaj&amp;amp;printsec=frontcover#v=onepage&amp;amp;q=%22partial%20differential%22&amp;amp;f=false&lt;br /&gt;
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* {{Citation |authorlink=Ivan Petrovsky |first=I. G. |last=Petrovskii |title=Partial Differential Equations |publisher=W. B. Saunders Co. |location=Philadelphia |year=1967 }}.&lt;br /&gt;
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&lt;br /&gt;
* {{Citation |first=A. D. |last=Polyanin |first2=V. F. |last2=Zaitsev |lastauthoramp=yes |first3=A. |last3=Moussiaux |title=Handbook of First Order Partial Differential Equations |publisher=Taylor &amp;amp; Francis |location=London |year=2002 |isbn=0-415-27267-X }}.&lt;br /&gt;
&lt;br /&gt;
* {{citation|mr=3014456|last=Roubíček|first= T.|title=Nonlinear Partial Differential Equations with Applications|publisher= Birkhäuser|place= Basel, Boston, Berlin|edition=2nd|year= 2013|ISBN= 978-3-0348-0512-4|doi=10.1007/978-3-0348-0513-1|url=http://cds.cern.ch/record/880983/files/9783764372934_TOC.pdf}}&lt;br /&gt;
&lt;br /&gt;
* {{Citation |first=P. |last=Solin |title=Partial Differential Equations and the Finite Element Method |publisher=J. Wiley &amp;amp; Sons |location=Hoboken, NJ |year=2005 |isbn=0-471-72070-4 }}.&lt;br /&gt;
&lt;br /&gt;
* {{Citation |first=P. |last=Solin |first2=K. |last2=Segeth |lastauthoramp=yes |first3=I. |last3=Dolezel |title=Higher-Order Finite Element Methods |publisher=Chapman &amp;amp; Hall/CRC Press |location=Boca Raton |year=2003 |isbn=1-58488-438-X }}.&lt;br /&gt;
&lt;br /&gt;
* {{Citation |first=H. |last=Stephani |year=1989 |title=Differential Equations: Their Solution Using Symmetries. Edited by M. MacCallum |publisher=Cambridge University Press }}.&lt;br /&gt;
&lt;br /&gt;
* {{cite book |title=Partial Differential Equations and Solitary Waves Theory&lt;br /&gt;
&lt;br /&gt;
|first=Abdul-Majid|last=Wazwaz|publisher=Higher Education Press|year=2009|isbn=978-3-642-00251-9|page=}}&lt;br /&gt;
&lt;br /&gt;
|first=Abdul-Majid|last=Wazwaz|publisher=Higher Education Press|year=2009|isbn=978-3-642-00251-9|page=}}&lt;br /&gt;
&lt;br /&gt;
| first Abdul-Majid | last Wazwaz | publisher Higher Education Press | year 2009 | isbn 978-3-642-00251-9 | page }&lt;br /&gt;
&lt;br /&gt;
* {{cite book |title=Partial Differential Equations Methods and Applications&lt;br /&gt;
&lt;br /&gt;
|first=Abdul-Majid|last=Wazwaz|publisher=A.A. Balkema|year=2002|isbn=90-5809-369-7|page=}}&lt;br /&gt;
&lt;br /&gt;
|first=Abdul-Majid|last=Wazwaz|publisher=A.A. Balkema|year=2002|isbn=90-5809-369-7|page=}}&lt;br /&gt;
&lt;br /&gt;
| first Abdul-Majid | last Wazwaz | publisher a.a.Balkema | year 2002 | isbn 90-5809-369-7 | page }&lt;br /&gt;
&lt;br /&gt;
* {{Citation |first=D. |last=Zwillinger |title=Handbook of Differential Equations |publisher=Academic Press |location=Boston |year=1997 |edition=3rd |isbn=0-12-784395-7 }}.&lt;br /&gt;
&lt;br /&gt;
* {{Citation |authorlink=Neil Gershenfeld |first=N. |last=Gershenfeld |title=The Nature of Mathematical Modeling |location=New York |publisher=Cambridge University Press, New York, NY, USA |year=1999 |edition=1st |isbn=0-521-57095-6 }}.&lt;br /&gt;
&lt;br /&gt;
* {{Citation |first=I.S. |last=Krasil'shchik |lastauthoramp=yes |first2=A.M., Eds. |last2=Vinogradov |title=Symmetries and Conserwation Laws for Differential Equations of Mathematical Physics |publisher=American Mathematical Society, Providence, Rhode Island, USA |year=1999 |isbn=0-8218-0958-X }}.&lt;br /&gt;
&lt;br /&gt;
* {{Citation |first=I.S. |last=Krasil'shchik |first2=V.V. |last2=Lychagin|lastauthoramp=yes |first3=A.M. |last3=Vinogradov |title=Geometry of Jet Spaces and Nonlinear Partial Differential Equations |publisher=Gordon and Breach Science Publishers, New York, London, Paris, Montreux, Tokyo |year=1986 |isbn=2-88124-051-8 }}.&lt;br /&gt;
&lt;br /&gt;
* {{Citation |first=A.M. |last=Vinogradov |title=Cohomological Analysis of Partial Differential Equations and Secondary Calculus |publisher=American Mathematical Society, Providence, Rhode Island, USA |year=2001 |isbn=0-8218-2922-X }}.&lt;br /&gt;
&lt;br /&gt;
* {{cite book |title=High Order Difference Methods for Time Dependent PDE&lt;br /&gt;
&lt;br /&gt;
|first=Bertil|last=Gustafsson|publisher=Springer|year=2008|isbn=978-3-540-74992-9|doi=10.1007/978-3-540-74993-6}}&lt;br /&gt;
&lt;br /&gt;
|first=Bertil|last=Gustafsson|publisher=Springer|year=2008|isbn=978-3-540-74992-9|doi=10.1007/978-3-540-74993-6}}&lt;br /&gt;
&lt;br /&gt;
| first Bertil | last Gustafsson | Springer | year 2008 | isbn 978-3-540-74992-9 | doi 10.1007 / 978-3-540-74993-6}&lt;br /&gt;
&lt;br /&gt;
{{refend}}&lt;br /&gt;
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&lt;br /&gt;
== Further reading ==&lt;br /&gt;
&lt;br /&gt;
* {{Cite journal|last=Cajori|first=Florian|authorlink=Florian Cajori|year=1928|title=The Early History of Partial Differential Equations and of Partial Differentiation and Integration|url=http://www.math.harvard.edu/archive/21a_fall_14/exhibits/cajori/cajori.pdf|journal=The American Mathematical Monthly|volume=35|issue=9|pages=459–467|doi=10.2307/2298771|access-date=2016-05-15|archive-url=https://web.archive.org/web/20181123102253/http://www.math.harvard.edu/archive/21a_fall_14/exhibits/cajori/cajori.pdf|archive-date=2018-11-23|url-status=dead}}&lt;br /&gt;
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== External links ==&lt;br /&gt;
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{{Sister project links| wikt=no | commons=Category:Solutions of PDE | b=Partial Differential Equations | n=no | q=Partial differential equation | s=no | v=no | voy=no | species=no | d=no}}&lt;br /&gt;
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* {{springer|title=Differential equation, partial|id=p/d031920}}&lt;br /&gt;
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* [http://eqworld.ipmnet.ru/en/pde-en.htm Partial Differential Equations: Exact Solutions] at EqWorld: The World of Mathematical Equations.&lt;br /&gt;
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* [http://eqworld.ipmnet.ru/en/solutions/eqindex/eqindex-pde.htm Partial Differential Equations: Index] at EqWorld: The World of Mathematical Equations.&lt;br /&gt;
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* [http://eqworld.ipmnet.ru/en/methods/meth-pde.htm Partial Differential Equations: Methods] at EqWorld: The World of Mathematical Equations.&lt;br /&gt;
&lt;br /&gt;
* [https://web.archive.org/web/20170701144823/http://www.exampleproblems.com/wiki/index.php?title=Partial_Differential_Equations Example problems with solutions] at exampleproblems.com&lt;br /&gt;
&lt;br /&gt;
* [http://mathworld.wolfram.com/PartialDifferentialEquation.html Partial Differential Equations] at mathworld.wolfram.com&lt;br /&gt;
&lt;br /&gt;
* [https://reference.wolfram.com/language/FEMDocumentation/tutorial/SolvingPDEwithFEM.html Partial Differential Equations] with Mathematica&lt;br /&gt;
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* [http://www.mathworks.com/moler/pdes.pdf Partial Differential Equations] in Cleve Moler: Numerical Computing with MATLAB&lt;br /&gt;
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* [http://www.nag.com/numeric/fl/nagdoc_fl24/html/D03/d03intro.html Partial Differential Equations] at nag.com&lt;br /&gt;
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* {{cite web |first=Grant |last=Sanderson |title=But what is a partial differential equation? |work=3Blue1Brown |date=April 21, 2019 |url=https://www.youtube.com/watch?v=ly4S0oi3Yz8&amp;amp;list=PLZHQObOWTQDNPOjrT6KVlfJuKtYTftqH6 |via=[[YouTube]] }}&lt;br /&gt;
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{{Differential equations topics}}&lt;br /&gt;
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{{Authority control}}&lt;br /&gt;
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[[Category:Partial differential equations| ]]&lt;br /&gt;
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[[Category:Multivariable calculus]]&lt;br /&gt;
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Category:Multivariable calculus&lt;br /&gt;
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类别: 多元微积分&lt;br /&gt;
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[[Category:Differential equations]]&lt;br /&gt;
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Category:Differential equations&lt;br /&gt;
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类别: 微分方程&lt;br /&gt;
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[[Category:Concepts in physics]]&lt;br /&gt;
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Category:Concepts in physics&lt;br /&gt;
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分类: 物理概念&lt;br /&gt;
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&amp;lt;small&amp;gt;This page was moved from [[wikipedia:en:Partial differential equation]]. Its edit history can be viewed at [[偏微分方程/edithistory]]&amp;lt;/small&amp;gt;&amp;lt;/noinclude&amp;gt;&lt;br /&gt;
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[[Category:待整理页面]]&lt;/div&gt;</summary>
		<author><name>Ruili</name></author>
	</entry>
	<entry>
		<id>https://wiki.swarma.org/index.php?title=%E5%81%8F%E5%BE%AE%E5%88%86%E6%96%B9%E7%A8%8B&amp;diff=18205</id>
		<title>偏微分方程</title>
		<link rel="alternate" type="text/html" href="https://wiki.swarma.org/index.php?title=%E5%81%8F%E5%BE%AE%E5%88%86%E6%96%B9%E7%A8%8B&amp;diff=18205"/>
		<updated>2020-11-12T16:14:47Z</updated>

		<summary type="html">&lt;p&gt;Ruili：&lt;/p&gt;
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&lt;div&gt;此词条暂由Yuling翻译，未经人工整理和审校，带来阅读不便，请见谅。&lt;br /&gt;
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[[File:Heat.gif|thumb|right|A visualisation of a solution to the two-dimensional [[heat equation]] with temperature represented by the third dimension]]&lt;br /&gt;
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A visualisation of a solution to the two-dimensional [[heat equation with temperature represented by the third dimension]]&lt;br /&gt;
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以三维表示温度的二维热方程解的可视化&lt;br /&gt;
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In [[mathematics]], a '''partial differential equation''' ('''PDE''') is a [[differential equation]] that contains unknown [[Multivariable calculus|multivariable functions]] and their [[partial derivative]]s. PDEs are used to formulate problems involving functions of several variables, and are either solved by hand, or used to create a [[computer model]]. A special case is [[ordinary differential equation]]s (ODEs), which deal with functions of a single variable and their derivatives.&lt;br /&gt;
&lt;br /&gt;
In mathematics, a partial differential equation (PDE) is a differential equation that contains unknown multivariable functions and their partial derivatives. PDEs are used to formulate problems involving functions of several variables, and are either solved by hand, or used to create a computer model. A special case is ordinary differential equations (ODEs), which deal with functions of a single variable and their derivatives.&lt;br /&gt;
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在数学中，'''&amp;lt;font color = &amp;quot;#ff8000&amp;quot;&amp;gt; 偏微分方程函数 Partial Differential Equation&amp;lt;/font&amp;gt;'''是包含未知多元函数及其偏导数的微分方程。偏微分方程用于描述涉及多元函数的问题，可以通过人为求解，也可以通过建立计算机模型来求解。常微分方程是偏微分方程一种特殊情况，它处理的是一元函数及其导数。&lt;br /&gt;
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PDEs can be used to describe a wide variety of phenomena such as sound, heat, [[diffusion]], [[electrostatics]], [[Electromagnetism|electrodynamics]], [[fluid dynamics]], [[Elasticity (physics)|elasticity]], [[gravitation]] and [[quantum mechanics]]. These seemingly distinct physical phenomena can be formalised similarly in terms of PDEs. Just as ordinary differential equations often model one-dimensional [[dynamical system]]s, partial differential equations often model [[multidimensional system]]s. PDEs find their generalisation in [[stochastic partial differential equation]]s.&lt;br /&gt;
&lt;br /&gt;
PDEs can be used to describe a wide variety of phenomena such as sound, heat, diffusion, electrostatics, electrodynamics, fluid dynamics, elasticity, gravitation and quantum mechanics. These seemingly distinct physical phenomena can be formalised similarly in terms of PDEs. Just as ordinary differential equations often model one-dimensional dynamical systems, partial differential equations often model multidimensional systems. PDEs find their generalisation in stochastic partial differential equations.&lt;br /&gt;
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偏微分方程可以用来描述各种各样的物理现象，如声音，热量，扩散，静电，电动力学，流体力学，弹性力学，重力和量子力学。这些看起来截然不同的物理现象却可以用类似的偏微分方程来描述。正如常微分方程经常对一维动力系统进行建模一样，偏微分方程经常对多维系统进行建模。随机偏微分方程是偏微分方程的一种推广。&lt;br /&gt;
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== Introduction ==&lt;br /&gt;
引言&lt;br /&gt;
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Partial differential equations (PDEs) are equations that involve rates of change with respect to [[continuous variables]]. For example, the position of a [[rigid body]] is specified by six parameters,&amp;lt;ref&amp;gt;{{Cite book|url=https://books.google.com/books?id=v9PLbcYd9aUC&amp;amp;pg=PA32|title=Modelling and Control of Robot Manipulators|last=Sciavicco|first=Lorenzo|last2=Siciliano|first2=Bruno|date=2001-02-19|publisher=Springer Science &amp;amp; Business Media|isbn=9781852332211|language=en}}&amp;lt;/ref&amp;gt; but the configuration of a [[fluid]] is given by the [[continuous distribution]] of several parameters, such as the [[temperature]], [[pressure]], and so forth. The dynamics for the rigid body take place in a finite-dimensional [[Configuration space (physics)|configuration space]]; the dynamics for the fluid occur in an infinite-dimensional configuration space. This distinction usually makes PDEs much harder to solve than ordinary differential equations (ODEs), but here again, there will be simple solutions for linear problems. Classic domains where PDEs are used include [[acoustics]], [[fluid dynamics]], [[electrodynamics]], and [[heat transfer]].&lt;br /&gt;
&lt;br /&gt;
Partial differential equations (PDEs) are equations that involve rates of change with respect to continuous variables. For example, the position of a rigid body is specified by six parameters, but the configuration of a fluid is given by the continuous distribution of several parameters, such as the temperature, pressure, and so forth. The dynamics for the rigid body take place in a finite-dimensional configuration space; the dynamics for the fluid occur in an infinite-dimensional configuration space. This distinction usually makes PDEs much harder to solve than ordinary differential equations (ODEs), but here again, there will be simple solutions for linear problems. Classic domains where PDEs are used include acoustics, fluid dynamics, electrodynamics, and heat transfer.&lt;br /&gt;
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偏微分方程(简称为PDEs)涉及到方程相对于连续变量的变化率。例如，刚体的位置是由六个参数确定的，而流体的状态是由几个参数的连续分布给出的，如温度、压力等。刚体的动力学过程发生在有限维状态空间中，流体的动力学过程发生在无限维状态空间中。这种区别通常使偏微分方程比常微分方程更难求解，但是线性问题仍然有简单的求解方式。使用偏微分方程的经典领域包括声学、流体力学、电动力学和传热学。&lt;br /&gt;
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A partial differential equation (PDE) for the function {{math|''u''(''x''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;,… ''x&amp;lt;sub&amp;gt;n&amp;lt;/sub&amp;gt;'')}} is an equation of the form&lt;br /&gt;
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A partial differential equation (PDE) for the function  is an equation of the form&lt;br /&gt;
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函数 {{math|''u''(''x''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;,… ''x&amp;lt;sub&amp;gt;n&amp;lt;/sub&amp;gt;'')}} 的偏微分方程形式是：&lt;br /&gt;
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: &amp;lt;math&amp;gt;f \left (x_1, \ldots x_n; u, \frac{\partial u}{\partial x_1}, \ldots \frac{\partial u}{\partial x_n}; \frac{\partial^2 u}{\partial x_1 \partial x_1}, \ldots \frac{\partial^2 u}{\partial x_1 \partial x_n}; \ldots \right) = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;f \left (x_1, \ldots x_n; u, \frac{\partial u}{\partial x_1}, \ldots \frac{\partial u}{\partial x_n}; \frac{\partial^2 u}{\partial x_1 \partial x_1}, \ldots \frac{\partial^2 u}{\partial x_1 \partial x_n}; \ldots \right) = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
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If {{mvar|f}} is a [[linear function]] of {{mvar|u}} and its derivatives, then the PDE is called linear. Common examples of linear PDEs include the [[heat equation]], the [[wave equation]], [[Laplace's equation]], [[Helmholtz equation]], [[Klein–Gordon equation]], and [[Poisson's equation]].&lt;br /&gt;
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If  is a linear function of  and its derivatives, then the PDE is called linear. Common examples of linear PDEs include the heat equation, the wave equation, Laplace's equation, Helmholtz equation, Klein–Gordon equation, and Poisson's equation.&lt;br /&gt;
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如果 {{mvar|f}} 是函数 {{math|''u''}} 及其导数的线性函数，则偏微分方程称为线性函数。线性偏微分方程的常见例子包括热方程、波动方程、拉普拉斯方程、亥姆霍兹方程方程、克莱因-高登方程和泊松方程。&lt;br /&gt;
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A relatively simple PDE is&lt;br /&gt;
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A relatively simple PDE is&lt;br /&gt;
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一个相对简单的偏微分方程：&lt;br /&gt;
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: &amp;lt;math&amp;gt;\frac{\partial u}{\partial x}(x,y) = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;\frac{\partial u}{\partial x}(x,y) = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
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This relation [[Logical implication|implies]] that the function {{math|''u''(''x'',''y'')}} is independent of {{mvar|x}}. However, the equation gives no information on the function's dependence on the variable {{mvar|y}}. Hence the general solution of this equation is&lt;br /&gt;
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This relation implies that the function  is independent of . However, the equation gives no information on the function's dependence on the variable . Hence the general solution of this equation is&lt;br /&gt;
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这意味着函数 {{math|''u''(''x'',''y'')}} 独立于 {{mvar|x}} 的。然而，这个方程没有给出关于函数和自变量的相关性的信息。因此，这个方程的通解是&lt;br /&gt;
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: &amp;lt;math&amp;gt;u(x,y) = f(y),&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;u(x,y) = f(y),&amp;lt;/math&amp;gt;&lt;br /&gt;
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where {{mvar|f}} is an arbitrary function of {{mvar|y}}. The analogous ordinary differential equation is&lt;br /&gt;
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where  is an arbitrary function of . The analogous ordinary differential equation is&lt;br /&gt;
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其中， {{mvar|f}} 是 {{mvar|y}} 的任意函数。&lt;br /&gt;
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类似的常微分方程是：&lt;br /&gt;
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: &amp;lt;math&amp;gt;\frac{\mathrm{d} u}{\mathrm{d} x}(x) = 0,&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;\frac{\mathrm{d} u}{\mathrm{d} x}(x) = 0,&amp;lt;/math&amp;gt;&lt;br /&gt;
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which has the solution&lt;br /&gt;
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which has the solution&lt;br /&gt;
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它的解为&lt;br /&gt;
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: &amp;lt;math&amp;gt;u(x) = c,&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;u(x) = c,&amp;lt;/math&amp;gt;&lt;br /&gt;
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where {{mvar|c}} is any [[Constant (mathematics)|constant]] value. These two examples illustrate that general solutions of ordinary differential equations (ODEs) involve arbitrary constants, but solutions of PDEs involve arbitrary functions.&lt;br /&gt;
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where  is any constant value. These two examples illustrate that general solutions of ordinary differential equations (ODEs) involve arbitrary constants, but solutions of PDEs involve arbitrary functions.&lt;br /&gt;
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这里，{{mvar|c}} 是一个任意常量。&lt;br /&gt;
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这两个例子说明常微分方程的一般解包含任意常数，但偏微分方程的解包含任意函数。&lt;br /&gt;
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A solution of a PDE is generally not [[Uniqueness quantification|unique]]; additional conditions must generally be specified on the [[Boundary (topology)|boundary]] of the region where the solution is defined. For instance, in the simple example above, the function {{math|''f''(''y'')}} can be determined if {{mvar|u}} is specified on the line {{math|''x'' {{=}} 0}}.&lt;br /&gt;
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A solution of a PDE is generally not unique; additional conditions must generally be specified on the boundary of the region where the solution is defined. For instance, in the simple example above, the function  can be determined if  is specified on the line  0}}.&lt;br /&gt;
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偏微分方程的解一般不是唯一的; 一般必须在定义解的区域边界上定义附加条件。 例如，在上面的简单示例中，如果在 {{math|''x'' {{=}} 0}} 时确定了 {{mvar|u}} 的值，则可以确定该函数 {{math|''f''(''y'')}}。&lt;br /&gt;
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== Existence and uniqueness ==&lt;br /&gt;
存在性和唯一性&lt;br /&gt;
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Although the issue of existence and uniqueness of solutions of ordinary differential equations has a very satisfactory answer with the [[Picard–Lindelöf theorem]], that is far from the case for partial differential equations. The [[Cauchy–Kowalevski theorem]] states that the [[Cauchy problem]] for any partial differential equation whose coefficients are [[Analytic function|analytic]] in the unknown function and its derivatives, has a locally unique analytic solution. Although this result might appear to settle the existence and uniqueness of solutions, there are examples of linear partial differential equations whose coefficients have derivatives of all orders (which are nevertheless not analytic) but which have no solutions at all: see [[Lewy's example|Lewy (1957)]]. Even if the solution of a partial differential equation exists and is unique, it may nevertheless have undesirable properties.  The mathematical study of these questions is usually in the more powerful context of [[weak solution]]s.&lt;br /&gt;
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Although the issue of existence and uniqueness of solutions of ordinary differential equations has a very satisfactory answer with the Picard–Lindelöf theorem, that is far from the case for partial differential equations. The Cauchy–Kowalevski theorem states that the Cauchy problem for any partial differential equation whose coefficients are analytic in the unknown function and its derivatives, has a locally unique analytic solution. Although this result might appear to settle the existence and uniqueness of solutions, there are examples of linear partial differential equations whose coefficients have derivatives of all orders (which are nevertheless not analytic) but which have no solutions at all: see Lewy (1957). Even if the solution of a partial differential equation exists and is unique, it may nevertheless have undesirable properties.  The mathematical study of these questions is usually in the more powerful context of weak solutions.&lt;br /&gt;
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尽管常微分方程解的存在性和唯一性用'''&amp;lt;font color=&amp;quot;#ff8000&amp;quot;&amp;gt;弗罗贝尼乌斯定理 Picard–Lindelöf Theorem&amp;lt;/font&amp;gt;得到了令人满意的结果，但偏微分方程解的存在性和唯一性却远没有得到解决。'''&amp;lt;font color=&amp;quot;#ff8000&amp;quot;&amp;gt;柯西-科瓦列夫斯基定理 Cauchy–Kowalevski theorem&amp;lt;/font&amp;gt;指出：对于任意系数在未知函数及其导数中解析的偏微分方程，柯西问题存在一个局部唯一的解析解。虽然这个结果似乎解决了解的存在性和唯一性问题，但是存在一些线性偏微分方程-其系数具有所有级数的导数(尽管这些导数不是解析的) ，但是根本没有解: 见 Lewy (1957)。即使偏微分方程的解存在且唯一，它仍然可能具有不可预料的性质。这些问题的数学研究通常是在更有力的弱解的背景下进行的。&lt;br /&gt;
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An example of pathological behavior is the sequence (depending upon {{mvar|n}}) of [[Cauchy problem]]s for the [[Laplace equation]]&lt;br /&gt;
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An example of pathological behavior is the sequence (depending upon ) of Cauchy problems for the Laplace equation&lt;br /&gt;
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反常特征的一个例子是拉普拉斯方程的柯西问题的序列(取决于{{mvar|n}})&lt;br /&gt;
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: &amp;lt;math&amp;gt;\frac{\partial^2 u}{\partial x^2} + \frac{\partial^2 u}{\partial y^2}=0,&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;\frac{\partial^2 u}{\partial x^2} + \frac{\partial^2 u}{\partial y^2}=0,&amp;lt;/math&amp;gt;&lt;br /&gt;
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with [[boundary condition]]s&lt;br /&gt;
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with boundary conditions&lt;br /&gt;
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具有边界条件&lt;br /&gt;
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: &amp;lt;math&amp;gt;\begin{align} u(x,0) &amp;amp;= 0, \\ \frac{\partial u}{\partial y}(x,0) &amp;amp;= \frac{\sin nx}{n}, \end{align}&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;\begin{align} u(x,0) &amp;amp;= 0, \\ \frac{\partial u}{\partial y}(x,0) &amp;amp;= \frac{\sin nx}{n}, \end{align}&amp;lt;/math&amp;gt;&lt;br /&gt;
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where {{mvar|n}} is an integer. The derivative of {{mvar|u}} with respect to {{mvar|y}} approaches zero [[uniform convergence|uniformly]] in {{mvar|x}} as {{mvar|n}} increases, but the solution is&lt;br /&gt;
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where  is an integer. The derivative of  with respect to  approaches zero uniformly in  as  increases, but the solution is&lt;br /&gt;
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其中 {{mvar|n}} 是整数。{{mvar|u}} 关于 {{mvar|y}} 的导数，一致地随着 {{mvar|n}} 的增加而趋于零，但解是&lt;br /&gt;
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: &amp;lt;math&amp;gt;u(x,y) = \frac{\sinh ny \sin nx}{n^2}.&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;u(x,y) = \frac{\sinh ny \sin nx}{n^2}.&amp;lt;/math&amp;gt;&lt;br /&gt;
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This solution approaches infinity if {{mvar|nx}} is not an integer multiple of {{pi}} for any non-zero value of {{mvar|y}}. The Cauchy problem for the Laplace equation is called ''ill-posed'' or ''not [[Well-posed problem|well-posed]]'', since the solution does not continuously depend on the data of the problem. Such ill-posed problems are not usually satisfactory for physical applications.&lt;br /&gt;
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This solution approaches infinity if  is not an integer multiple of  for any non-zero value of . The Cauchy problem for the Laplace equation is called ill-posed or not well-posed, since the solution does not continuously depend on the data of the problem. Such ill-posed problems are not usually satisfactory for physical applications.&lt;br /&gt;
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对于任何非零的 {{mvar|y}}，如果 {{mvar|nx}} 不是模板 {{pi}} 的整数倍，这个解会接近于无穷大。拉普拉斯方程的柯西问题被称为不适定的（可以译为ill-posed或not well-posed），因为解不是连续地依赖于问题的数据。这种不适定问题通常不能满足物理应用。&lt;br /&gt;
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The [[Navier–Stokes existence and smoothness|existence of solutions for the Navier–Stokes equations]], a partial differential equation, is part of one of the [[Millennium Prize Problems]].&lt;br /&gt;
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The existence of solutions for the Navier–Stokes equations, a partial differential equation, is part of one of the Millennium Prize Problems.&lt;br /&gt;
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偏微分方程”纳维-斯托克斯方程“的解的存在性就是千禧年大奖难题之一的一部分。&lt;br /&gt;
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== Notation ==&lt;br /&gt;
符号&lt;br /&gt;
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In PDEs, it is common to denote partial derivatives using subscripts. That is:&lt;br /&gt;
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In PDEs, it is common to denote partial derivatives using subscripts. That is:&lt;br /&gt;
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在偏微分方程中，通常用下标表示偏导数。例如:&lt;br /&gt;
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: &amp;lt;math&amp;gt;u_x = \frac{\partial u}{\partial x}&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;u_x = \frac{\partial u}{\partial x}&amp;lt;/math&amp;gt;&lt;br /&gt;
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: &amp;lt;math&amp;gt;u_{xx} = \frac{\partial^2 u}{\partial x^2} &amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;u_{xx} = \frac{\partial^2 u}{\partial x^2} &amp;lt;/math&amp;gt;&lt;br /&gt;
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: &amp;lt;math&amp;gt;u_{xy} = \frac{\partial^2 u}{\partial y\, \partial x} = \frac{\partial}{\partial y } \left(\frac{\partial u}{\partial x}\right). &amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;u_{xy} = \frac{\partial^2 u}{\partial y\, \partial x} = \frac{\partial}{\partial y } \left(\frac{\partial u}{\partial x}\right). &amp;lt;/math&amp;gt;&lt;br /&gt;
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Especially in physics, [[del]] or nabla ({{math|∇}}) is often used to denote spatial derivatives, and {{math|''&amp;amp;#x307;u'', ''ü''}} for time derivatives. For example, the [[wave equation]] (mentioned below) can be written as&lt;br /&gt;
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Especially in physics, del or nabla () is often used to denote spatial derivatives, and  for time derivatives. For example, the wave equation (mentioned below) can be written as&lt;br /&gt;
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特别是在物理学中，[[del]] 或 nabla ({{math|∇}}) 经常用来表示空间导数和时间导数。例如，波动方程(在下文中提到)可以写成：&lt;br /&gt;
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:&amp;lt;math&amp;gt;\ddot u=c^2\nabla^2u&amp;lt;/math&amp;gt;&lt;br /&gt;
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&amp;lt;math&amp;gt;\ddot u=c^2\nabla^2u&amp;lt;/math&amp;gt;&lt;br /&gt;
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or&lt;br /&gt;
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or&lt;br /&gt;
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或&lt;br /&gt;
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:&amp;lt;math&amp;gt;\ddot u=c^2\Delta u&amp;lt;/math&amp;gt;&lt;br /&gt;
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&amp;lt;math&amp;gt;\ddot u=c^2\Delta u&amp;lt;/math&amp;gt;&lt;br /&gt;
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where {{math|Δ}} is the [[Laplace operator]].&lt;br /&gt;
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where  is the Laplace operator.&lt;br /&gt;
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其中，{{math|Δ}} 代表拉普拉斯算子。&lt;br /&gt;
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== Classification ==&lt;br /&gt;
分类&lt;br /&gt;
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Some linear, second-order partial differential equations can be classified as [[parabolic partial differential equation|parabolic]], [[hyperbolic partial differential equation|hyperbolic]] and [[elliptic partial differential equation|elliptic]]. Others, such as the [[Euler–Tricomi equation]], have different types in different regions. The classification provides a guide to appropriate initial and boundary conditions and to the smoothness of the solutions.&lt;br /&gt;
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Some linear, second-order partial differential equations can be classified as parabolic, hyperbolic and elliptic. Others, such as the Euler–Tricomi equation, have different types in different regions. The classification provides a guide to appropriate initial and boundary conditions and to the smoothness of the solutions.&lt;br /&gt;
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一些线性二阶偏微分方程可分为抛物型方程、双曲型方程和椭圆型方程。其他的方程，如欧拉-特里科米方程，在不同的领域有不同的类型。这种分类有助于选择适当的初始和边界条件以及提高解的平滑性。&lt;br /&gt;
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=== Equations of first order ===&lt;br /&gt;
一阶方程&lt;br /&gt;
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{{main|First-order partial differential equation}}&lt;br /&gt;
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=== Linear equations of second order ===&lt;br /&gt;
二阶线性方程&lt;br /&gt;
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Assuming {{math|''u&amp;lt;sub&amp;gt;xy&amp;lt;/sub&amp;gt;'' {{=}} ''u&amp;lt;sub&amp;gt;yx&amp;lt;/sub&amp;gt;''}}, the general linear second-order PDE in two independent variables has the form&lt;br /&gt;
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Assuming  u&amp;lt;sub&amp;gt;yx&amp;lt;/sub&amp;gt;}}, the general linear second-order PDE in two independent variables has the form&lt;br /&gt;
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假设 {{math|''u&amp;lt;sub&amp;gt;xy&amp;lt;/sub&amp;gt;'' {{=}} ''u&amp;lt;sub&amp;gt;yx&amp;lt;/sub&amp;gt;''}}，含有两个独立变量的一般线性二阶偏微分方程具有如下形式：&lt;br /&gt;
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: &amp;lt;math&amp;gt;Au_{xx} + 2Bu_{xy} + Cu_{yy} + \cdots \mbox{(lower order terms)} = 0,&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;Au_{xx} + 2Bu_{xy} + Cu_{yy} + \cdots \mbox{(lower order terms)} = 0,&amp;lt;/math&amp;gt;&lt;br /&gt;
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where the coefficients {{mvar|A}}, {{mvar|B}}, {{mvar|C}}... may depend upon {{mvar|x}} and {{mvar|y}}. If {{math|''A''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; + ''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; + ''C''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; &amp;gt; 0}} over a region of the {{mvar|xy}}-plane, the PDE is second-order in that region. This form is analogous to the equation for a conic section:&lt;br /&gt;
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where the coefficients , , ... may depend upon  and . If  over a region of the -plane, the PDE is second-order in that region. This form is analogous to the equation for a conic section:&lt;br /&gt;
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其中的系数 {{mvar|A}}, {{mvar|B}}, {{mvar|C}}... 一般取决于 {{mvar|x}} 和 {{mvar|y}} 。如果在 {{mvar|xy}}-平面的一个区域上 {{math|''A''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; + ''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; + ''C''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; &amp;gt; 0}}，偏微分方程是二阶的，这种形式类似于圆锥截面的方程:&lt;br /&gt;
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: &amp;lt;math&amp;gt;Ax^2 + 2Bxy + Cy^2 + \cdots = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;Ax^2 + 2Bxy + Cy^2 + \cdots = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
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More precisely, replacing {{math|∂&amp;lt;sub&amp;gt;''x''&amp;lt;/sub&amp;gt;}} by {{mvar|X}}, and likewise for other variables (formally this is done by a [[Fourier transform]]), converts a constant-coefficient PDE into a polynomial of the same degree, with the terms of the highest degree (a [[homogeneous polynomial]], here a [[quadratic form]]) being most significant for the classification.&lt;br /&gt;
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More precisely, replacing  by , and likewise for other variables (formally this is done by a Fourier transform), converts a constant-coefficient PDE into a polynomial of the same degree, with the terms of the highest degree (a homogeneous polynomial, here a quadratic form) being most significant for the classification.&lt;br /&gt;
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更准确地说，用 {{mvar|X}} 替换 {{math|∂&amp;lt;sub&amp;gt;''x''&amp;lt;/sub&amp;gt;}}，并同样替换其它变量(通常由傅里叶变换完成)，将一个常系数偏微分方程转换成一个相同次数的多项式，最高次数的项(齐次多项式，这里是一个二次形式)对于偏微分方程的分类最为重要。&lt;br /&gt;
===~~ most significant for the classification 意译为用于偏微分方程的分类。       significiant直译过来感觉不太合适&lt;br /&gt;
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Just as one classifies [[conic section]]s and quadratic forms into parabolic, hyperbolic, and elliptic based on the [[discriminant]] {{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − 4''AC''}}, the same can be done for a second-order PDE at a given point.  However, the [[discriminant]] in a PDE is given by {{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC''}} due to the convention of the {{mvar|xy}} term being {{math|2''B''}} rather than {{mvar|B}}; formally, the discriminant (of the associated quadratic form) is {{math|(2''B'')&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − 4''AC'' {{=}} 4(''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC'')}}, with the factor of 4 dropped for simplicity.&lt;br /&gt;
&lt;br /&gt;
Just as one classifies conic sections and quadratic forms into parabolic, hyperbolic, and elliptic based on the discriminant , the same can be done for a second-order PDE at a given point.  However, the discriminant in a PDE is given by  due to the convention of the  term being  rather than ; formally, the discriminant (of the associated quadratic form) is  4(B&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − AC)}}, with the factor of 4 dropped for simplicity.&lt;br /&gt;
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正如人们可以根据判别式 {{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − 4''AC''}} 将圆锥曲线和二次型分为抛物型、双曲型和椭圆型一样，对于给定点的二阶偏微分方程也可以这样做。然而，偏微分方程中的判别式 {{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − 4''AC''}} 是根据交叉项的系数{{math|2''B''}} 而不是 {{mvar|B}} 给出的，形式上，判别式(关联二次型)是 {{math|(2''B'')&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − 4''AC'' {{=}} 4(''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC'')}}，为简单起见，去掉了因子4。&lt;br /&gt;
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# {{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC'' &amp;lt; 0}} (''[[elliptic partial differential equation]]''): Solutions of [[elliptic partial differential equation|elliptic PDEs]] are as smooth as the coefficients allow, within the interior of the region where the equation and solutions are defined. For example, solutions of [[Laplace's equation]] are analytic within the domain where they are defined, but solutions may assume boundary values that are not smooth. The motion of a fluid at subsonic speeds can be approximated with elliptic PDEs, and the Euler–Tricomi equation is elliptic where {{math|''x'' &amp;lt; 0}}.&lt;br /&gt;
&lt;br /&gt;
  (elliptic partial differential equation): Solutions of elliptic PDEs are as smooth as the coefficients allow, within the interior of the region where the equation and solutions are defined. For example, solutions of Laplace's equation are analytic within the domain where they are defined, but solutions may assume boundary values that are not smooth. The motion of a fluid at subsonic speeds can be approximated with elliptic PDEs, and the Euler–Tricomi equation is elliptic where .&lt;br /&gt;
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{{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC'' &amp;lt; 0}} (椭圆形微分方程)：在定义方程和解的区域内部，椭圆型偏微分方程的解光滑到系数允许的程度。例如，拉普拉斯方程的解在它们被定义的区域内是解析的，但是解可能假设边界值是不光滑的。亚音速流体的运动可以用椭圆偏微分方程近似，其中欧拉-特里科米方程在 {{math|''x'' &amp;lt; 0}} 时是椭圆型偏微分方程。&lt;br /&gt;
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# {{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC'' {{=}} 0}} (''[[parabolic partial differential equation]]''): Equations that are [[parabolic partial differential equation|parabolic]] at every point can be transformed into a form analogous to the [[heat equation]] by a change of independent variables. Solutions smooth out as the transformed time variable increases. The Euler–Tricomi equation has parabolic type on the line where {{math|''x'' {{=}} 0}}.&lt;br /&gt;
&lt;br /&gt;
  0}} (parabolic partial differential equation): Equations that are parabolic at every point can be transformed into a form analogous to the heat equation by a change of independent variables. Solutions smooth out as the transformed time variable increases. The Euler–Tricomi equation has parabolic type on the line where  0}}.&lt;br /&gt;
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{{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC'' {{=}} 0}}（抛物线形偏微分方程）：在每一点上都是抛物线型的方程可以通过改变自变量从而转化成类似于热方程的形式。随着转换后的时间变量的增加，方程的解变得平滑。欧拉-特里科米方程在 {{math|''x'' {{=}} 0}} 这条特征线上是抛物线形的。&lt;br /&gt;
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# {{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC'' &amp;gt; 0}} (''[[hyperbolic partial differential equation]]''): [[hyperbolic partial differential equation|hyperbolic]] equations retain any discontinuities of functions or derivatives in the initial data. An example is the [[wave equation]]. The motion of a fluid at supersonic speeds can be approximated with hyperbolic PDEs, and the Euler–Tricomi equation is hyperbolic where {{math|''x'' &amp;gt; 0}}.&lt;br /&gt;
&lt;br /&gt;
  (hyperbolic partial differential equation): hyperbolic equations retain any discontinuities of functions or derivatives in the initial data. An example is the wave equation. The motion of a fluid at supersonic speeds can be approximated with hyperbolic PDEs, and the Euler–Tricomi equation is hyperbolic where .&lt;br /&gt;
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{{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC'' &amp;gt; 0}} (双曲形偏微分方程)：双曲形方程在初始数据中保留了函数或导数的任何不连续性，波动方程就是其中的一个例子。超音速流体的运动可以用双曲形偏微分方程近似，其中欧拉-特里科米方程在 {{math|''x'' &amp;gt; 0}} 时是双曲型的。&lt;br /&gt;
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If there are {{mvar|n}} independent variables {{math|''x''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;, ''x''&amp;lt;sub&amp;gt;2 &amp;lt;/sub&amp;gt;,… ''x''&amp;lt;sub&amp;gt;''n''&amp;lt;/sub&amp;gt;}}, a general linear partial differential equation of second order has the form&lt;br /&gt;
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If there are  independent variables , a general linear partial differential equation of second order has the form&lt;br /&gt;
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如果存在 {{mvar|n}} 个自变量 {{math|''x''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;, ''x''&amp;lt;sub&amp;gt;2 &amp;lt;/sub&amp;gt;,… ''x''&amp;lt;sub&amp;gt;''n''&amp;lt;/sub&amp;gt;}}，一般二阶线性偏微分方程的形式是&lt;br /&gt;
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: &amp;lt;math&amp;gt;L u =\sum_{i=1}^n\sum_{j=1}^n a_{i,j} \frac{\partial^2 u}{\partial x_i \partial x_j} \quad \text{ plus lower-order terms} =0.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;L u =\sum_{i=1}^n\sum_{j=1}^n a_{i,j} \frac{\partial^2 u}{\partial x_i \partial x_j} \quad \text{ plus lower-order terms} =0.&amp;lt;/math&amp;gt;&lt;br /&gt;
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The classification depends upon the signature of the eigenvalues of the coefficient matrix {{math|''a''&amp;lt;sub&amp;gt;''i'',''j''&amp;lt;/sub&amp;gt;}}.&lt;br /&gt;
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The classification depends upon the signature of the eigenvalues of the coefficient matrix .&lt;br /&gt;
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这种分类取决于系数矩阵本征值的符号（正负性）。&lt;br /&gt;
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# Elliptic: the eigenvalues are all positive or all negative.&lt;br /&gt;
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 Elliptic: the eigenvalues are all positive or all negative.&lt;br /&gt;
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椭圆形方程: 本征值全部为正或全部为负。&lt;br /&gt;
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# Parabolic: the eigenvalues are all positive or all negative, save one that is zero.&lt;br /&gt;
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 Parabolic: the eigenvalues are all positive or all negative, save one that is zero.&lt;br /&gt;
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抛物线形方程: 本征值全部为正或全部为负，除了一个为零。&lt;br /&gt;
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# Hyperbolic: there is only one negative eigenvalue and all the rest are positive, or there is only one positive eigenvalue and all the rest are negative.&lt;br /&gt;
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 Hyperbolic: there is only one negative eigenvalue and all the rest are positive, or there is only one positive eigenvalue and all the rest are negative.&lt;br /&gt;
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双曲形方程: 只有一个负特征值，其余的都是正特征值，或者只有一个正特征值，其余的都是负特征值。&lt;br /&gt;
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# Ultrahyperbolic: there is more than one positive eigenvalue and more than one negative eigenvalue, and there are no zero eigenvalues. There is only a limited theory for ultrahyperbolic equations (Courant and Hilbert, 1962).&lt;br /&gt;
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 Ultrahyperbolic: there is more than one positive eigenvalue and more than one negative eigenvalue, and there are no zero eigenvalues. There is only a limited theory for ultrahyperbolic equations (Courant and Hilbert, 1962).&lt;br /&gt;
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超双形方程: 存在多于一个正本征值和多于一个的负本征值，且不存在零本征值。对于超双曲方程，只存在一个有限理论(Courant 和 Hilbert，1962)。&lt;br /&gt;
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==[[用户:Yuling|Yuling]]（[[用户讨论:Yuling|讨论]]） 我对于limited theory这个单词对应的相关理论不太了解。&lt;br /&gt;
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=== Systems of first-order equations and characteristic surfaces ===&lt;br /&gt;
一阶方程组和特征曲面&lt;br /&gt;
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The classification of partial differential equations can be extended to systems of first-order equations, where the unknown {{mvar|u}} is now a [[Euclidean vector|vector]] with {{mvar|m}} components, and the coefficient matrices {{mvar|A&amp;lt;sub&amp;gt;ν&amp;lt;/sub&amp;gt;}} are {{mvar|m}} by {{mvar|m}} matrices for {{math|''ν'' {{=}} 1, 2,… ''n''}}. The partial differential equation takes the form&lt;br /&gt;
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The classification of partial differential equations can be extended to systems of first-order equations, where the unknown  is now a vector with  components, and the coefficient matrices  are  by  matrices for  1, 2,… n}}. The partial differential equation takes the form&lt;br /&gt;
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偏微分方程组的分类可以推广到一阶方程组，其中未知量 {{mvar|u}} 是有 {{mvar|m}} 个分量的向量。对于 {{math|''ν'' {{=}} 1, 2,… ''n''}}，系数矩阵 {{mvar|A&amp;lt;sub&amp;gt;ν&amp;lt;/sub&amp;gt;}} 是 {{mvar|m}} × {{mvar|m}} 的矩阵。偏微分方程形式如下：&lt;br /&gt;
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: &amp;lt;math&amp;gt;Lu = \sum_{\nu=1}^{n} A_\nu \frac{\partial u}{\partial x_\nu} + B=0,&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;Lu = \sum_{\nu=1}^{n} A_\nu \frac{\partial u}{\partial x_\nu} + B=0,&amp;lt;/math&amp;gt;&lt;br /&gt;
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where the coefficient matrices {{mvar|A&amp;lt;sub&amp;gt;ν&amp;lt;/sub&amp;gt;}} and the vector {{mvar|B}} may depend upon {{mvar|x}} and {{mvar|u}}. If a [[hypersurface]] {{mvar|S}} is given in the implicit form&lt;br /&gt;
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where the coefficient matrices  and the vector  may depend upon  and . If a hypersurface  is given in the implicit form&lt;br /&gt;
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其中系数矩阵 {{mvar|A&amp;lt;sub&amp;gt;ν&amp;lt;/sub&amp;gt;}} 和向量 {{mvar|B}} 可能依赖于 {{mvar|x}} 和 {{mvar|u}}。如果超曲面是以隐式形式给出的&lt;br /&gt;
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: &amp;lt;math&amp;gt;\varphi(x_1, x_2, \ldots x_n)=0,&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;\varphi(x_1, x_2, \ldots x_n)=0,&amp;lt;/math&amp;gt;&lt;br /&gt;
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where {{mvar|φ}} has a non-zero gradient, then {{mvar|S}} is a '''characteristic surface''' for the operator {{mvar|L}} at a given point if the characteristic form vanishes:&lt;br /&gt;
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where  has a non-zero gradient, then  is a characteristic surface for the operator  at a given point if the characteristic form vanishes:&lt;br /&gt;
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其中存在一个非零的梯度，那么如果特征形式消失，则在给定点上算子的特征曲面形式如下:&lt;br /&gt;
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: &amp;lt;math&amp;gt;Q\left(\frac{\partial\varphi}{\partial x_1}, \ldots\frac{\partial\varphi}{\partial x_n}\right) =\det\left[\sum_{\nu=1}^nA_\nu \frac{\partial \varphi}{\partial x_\nu}\right]=0.\,&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;Q\left(\frac{\partial\varphi}{\partial x_1}, \ldots\frac{\partial\varphi}{\partial x_n}\right) =\det\left[\sum_{\nu=1}^nA_\nu \frac{\partial \varphi}{\partial x_\nu}\right]=0.\,&amp;lt;/math&amp;gt;&lt;br /&gt;
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The geometric interpretation of this condition is as follows: if data for {{mvar|u}} are prescribed on the surface {{mvar|S}}, then it may be possible to determine the normal derivative of {{mvar|u}} on {{mvar|S}} from the differential equation. If the data on {{mvar|S}} and the differential equation determine the normal derivative of {{mvar|u}} on {{mvar|S}}, then {{mvar|S}} is non-characteristic. If the data on {{mvar|S}} and the differential equation ''do not'' determine the normal derivative of {{mvar|u}} on {{mvar|S}}, then the surface is '''characteristic''', and the differential equation restricts the data on {{mvar|S}}: the differential equation is ''internal'' to {{mvar|S}}.&lt;br /&gt;
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The geometric interpretation of this condition is as follows: if data for  are prescribed on the surface , then it may be possible to determine the normal derivative of  on  from the differential equation. If the data on  and the differential equation determine the normal derivative of  on , then  is non-characteristic. If the data on  and the differential equation do not determine the normal derivative of  on , then the surface is characteristic, and the differential equation restricts the data on : the differential equation is internal to .&lt;br /&gt;
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这个条件的几何解释如下: 如果关于 {{mvar|u}} 的数据是在曲面 {{mvar|S}} 上规定的，那么就有可能依据微分方程确定曲面 {{mvar|S}} 上 {{mvar|u}} 的法向导数。如果曲面 {{mvar|S}} 上的数据和上面的微分方程能确定曲面 {{mvar|S}} 上 {{mvar|u}} 的法向导数，那么它就是非特征的。如果曲面 {{mvar|S}} 上的数据和上面的微分方程不能确定曲面 {{mvar|S}} 上 {{mvar|u}} 的法向导数，那么曲面是特征的，并且微分方程将数据限制在曲面 {{mvar|S}} 上：微分方程是在曲面 {{mvar|S}} 内部。&lt;br /&gt;
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# A first-order system {{math|''Lu'' {{=}} 0}} is ''elliptic'' if no surface is characteristic for {{mvar|L}}: the values of {{mvar|u}} on {{mvar|S}} and the differential equation always determine the normal derivative of {{mvar|u}} on {{mvar|S}}.&lt;br /&gt;
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 A first-order system  0}} is elliptic if no surface is characteristic for : the values of  on  and the differential equation always determine the normal derivative of  on .&lt;br /&gt;
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如果对于 {{mvar|L}} 没有曲面是特征的，则一阶系统 {{math|''Lu'' {{=}} 0}} 是椭圆形的：{{mvar|u}}在 {{mvar|S}} 的值和微分方程总能够决定 {{mvar|S}} 上 {{mvar|u}} 的法向导数。&lt;br /&gt;
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# A first-order system is ''hyperbolic'' at a point if there is a '''spacelike''' surface {{mvar|S}} with normal {{mvar|ξ}} at that point. This means that, given any non-trivial vector {{mvar|η}} orthogonal to {{mvar|ξ}}, and a scalar multiplier {{mvar|λ}}, the equation {{math|''Q''(''λξ'' + ''η'') {{=}} 0}} has {{mvar|m}} real roots {{math|''λ''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;, ''λ''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;,… ''λ''&amp;lt;sub&amp;gt;''m''&amp;lt;/sub&amp;gt;}}. The system is '''strictly hyperbolic''' if these roots are always distinct. The geometrical interpretation of this condition is as follows: the characteristic form {{math|''Q''(''ζ'') {{=}} 0}} defines a cone (the normal cone) with homogeneous coordinates ζ. In the hyperbolic case, this cone has {{mvar|m}} sheets, and the axis {{math|''ζ'' {{=}} ''λξ''}} runs inside these sheets: it does not intersect any of them. But when displaced from the origin by η, this axis intersects every sheet. In the elliptic case, the normal cone has no real sheets.&lt;br /&gt;
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 A first-order system is hyperbolic at a point if there is a spacelike surface  with normal  at that point. This means that, given any non-trivial vector  orthogonal to , and a scalar multiplier , the equation  0}} has  real roots . The system is strictly hyperbolic if these roots are always distinct. The geometrical interpretation of this condition is as follows: the characteristic form  0}} defines a cone (the normal cone) with homogeneous coordinates ζ. In the hyperbolic case, this cone has  sheets, and the axis  λξ}} runs inside these sheets: it does not intersect any of them. But when displaced from the origin by η, this axis intersects every sheet. In the elliptic case, the normal cone has no real sheets.&lt;br /&gt;
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如果在该点存在一个法向量为 {{mvar|ξ}}的 '''&amp;lt;font color=&amp;quot;#ff8000&amp;quot;&amp;gt;类空曲面 Spacclike Surface&amp;lt;/font&amp;gt; {{mvar|S}} ，则一阶系统在那一点是双曲的。这意味着，给定任意正交于 {{mvar|ξ}} 的非平凡向量 {{mvar|η}} 和一个标量乘子 {{mvar|λ}}，方程 {{math|''Q''(''λξ'' + ''η'') {{=}} 0}} 有 {{mvar|m}} 个实根 {{math|''λ''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;, ''λ''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;,… ''λ''&amp;lt;sub&amp;gt;''m''&amp;lt;/sub&amp;gt;}}。如果这些根始终不同，则该系统是严格双曲形的。这个条件的几何解释如下: 特征形式 {{math|''Q''(''ζ'') {{=}} 0}} 定义了一个具有齐次坐标 ζ的圆锥(法线圆锥)。在双曲形的情况下，这个圆锥体有 {{mvar|m}} 层，并且轴 {{math|''ζ'' {{=}} ''λξ''}} 在这些层中运动: 它不与任何一层相交。但是当从原点偏离η时，这条轴线与每一层都相交。在椭圆形的情况下，法向圆锥没有实层。&lt;br /&gt;
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==[[用户:Yuling|Yuling]]（[[用户讨论:Yuling|讨论]]） sheet 这个单词也不很理解，我直译为了“层”&lt;br /&gt;
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=== Equations of mixed type ===&lt;br /&gt;
混合型方程&lt;br /&gt;
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If a PDE has coefficients that are not constant, it is possible that it will not belong to any of these categories but rather be of '''mixed type'''. A simple but important example is the [[Euler–Tricomi equation]]&lt;br /&gt;
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If a PDE has coefficients that are not constant, it is possible that it will not belong to any of these categories but rather be of mixed type. A simple but important example is the Euler–Tricomi equation&lt;br /&gt;
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如果偏微分方程的系数不是常数，那么它可能不属于这些类别中的任何一个，而是属于混合类型。一个简单但重要的例子是欧拉-特里科米方程&lt;br /&gt;
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: &amp;lt;math&amp;gt;u_{xx} = xu_{yy},&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;u_{xx} = xu_{yy},&amp;lt;/math&amp;gt;&lt;br /&gt;
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which is called '''elliptic-hyperbolic''' because it is elliptic in the region {{math|''x'' &amp;lt; 0}}, hyperbolic in the region {{math|''x'' &amp;gt; 0}}, and degenerate parabolic on the line {{math|''x'' {{=}} 0}}.&lt;br /&gt;
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which is called elliptic-hyperbolic because it is elliptic in the region , hyperbolic in the region , and degenerate parabolic on the line  0}}.&lt;br /&gt;
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它在 {{math|''x'' &amp;lt; 0}} 的区域上是椭圆形，在 {{math|''x'' &amp;gt; 0}} 区域上是双曲形，在 {{math|''x'' {{=}} 0}}这条线上是退化为抛物线形，因此称之为椭圆-双曲型。&lt;br /&gt;
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''fill in: Dirichlet and Neumann boundaries, hyperbolic/parabolic/elliptic separation of variables, [[Fourier analysis]], [[Green's function]]s ...--&amp;gt;&lt;br /&gt;
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fill in: Dirichlet and Neumann boundaries, hyperbolic/parabolic/elliptic separation of variables, Fourier analysis, Green's functions ...--&amp;gt;&lt;br /&gt;
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填写: Dirichlet 和 Neumann 边界，双曲 / 抛物线 / 椭圆分离变量法，傅立叶分析，Green 函数... --&lt;br /&gt;
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=== Infinite-order PDEs in quantum mechanics ===&lt;br /&gt;
量子力学中的无限阶偏微分方程&lt;br /&gt;
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In the [[phase space formulation]] of quantum mechanics,  one may consider the [[Method of quantum characteristics|quantum Hamilton's equations]] for trajectories of quantum particles. These equations are infinite-order PDEs. However, in the semiclassical expansion, one has a finite system of ODEs at any fixed order of [[Dirac constant|{{mvar|ħ}}]].  The evolution equation of the [[Wigner quasi-probability distribution|c]] is also an infinite-order PDE. The quantum trajectories are [[Method of quantum characteristics|quantum characteristics]], with the use of which one could calculate the evolution of the Wigner function.&lt;br /&gt;
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In the phase space formulation of quantum mechanics,  one may consider the quantum Hamilton's equations for trajectories of quantum particles. These equations are infinite-order PDEs. However, in the semiclassical expansion, one has a finite system of ODEs at any fixed order of Dirac constant|.  The evolution equation of the Wigner function is also an infinite-order PDE. The quantum trajectories are quantum characteristics, with the use of which one could calculate the evolution of the Wigner function.&lt;br /&gt;
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在量子力学中的相空间表述中，我们可以考虑用于求解量子粒子的轨迹的量子哈密顿的方程。这些方程是无限阶偏微分方程。然而，在半经典展开中，我们在给定[[Dirac constant|{{mvar|ħ}}]]阶数下有一个有限的的常微分方程组。'''&amp;lt;font color=&amp;quot;#ff8000&amp;quot;&amp;gt;维格纳函数  Wigner Function&amp;lt;/font&amp;gt;的演化方程也是一个无限阶偏微分方程。由于量子轨道的量子特性，所以它通常可以用来计算维格纳函数的演化。&lt;br /&gt;
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== Analytical solutions ==&lt;br /&gt;
解析解&lt;br /&gt;
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===Separation of variables===&lt;br /&gt;
分离变量法&lt;br /&gt;
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{{main|Separable partial differential equation}}&lt;br /&gt;
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Linear PDEs can be reduced to systems of ordinary differential equations by the important technique of separation of variables. This technique rests on a characteristic of solutions to differential equations: if one can find any solution that solves the equation and satisfies the boundary conditions, then it is ''the'' solution (this also applies to ODEs). We assume as an [[ansatz]] that the dependence of a solution on the parameters space and time can be written as a product of terms that each depend on a single parameter, and then see if this can be made to solve the problem.&amp;lt;ref&amp;gt;{{cite book|last1=Gershenfeld|first1=Neil|title=The nature of mathematical modeling|date=2000|publisher=Cambridge Univ. Press|location=Cambridge|isbn=0521570956|page=27|edition=Reprinted (with corr.)}}&amp;lt;/ref&amp;gt;&lt;br /&gt;
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Linear PDEs can be reduced to systems of ordinary differential equations by the important technique of separation of variables. This technique rests on a characteristic of solutions to differential equations: if one can find any solution that solves the equation and satisfies the boundary conditions, then it is the solution (this also applies to ODEs). We assume as an ansatz that the dependence of a solution on the parameters space and time can be written as a product of terms that each depend on a single parameter, and then see if this can be made to solve the problem.&lt;br /&gt;
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线性偏微分方程组可以通过分离变量法这一重要方法来简化为常微分方程组。这种方法依赖于微分方程解的一个特征: 如果能找到任何一个满足方程和边界条件的解，那么这个解就是方程的解(这也适用于常微分方程)。我们假设解对参数空间和时间的依赖可以写成对它们每一项的依赖以及一个参数的乘积，然后再看看这是否可以用来解决这个问题。&lt;br /&gt;
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In the method of separation of variables, one reduces a PDE to a PDE in fewer variables, which is an ordinary differential equation if in one variable – these are in turn easier to solve.&lt;br /&gt;
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In the method of separation of variables, one reduces a PDE to a PDE in fewer variables, which is an ordinary differential equation if in one variable – these are in turn easier to solve.&lt;br /&gt;
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在分离变量法方法中，可以将偏微分方程简化为含有更少变量的偏微分方程，如果只有一个变量，那么就变成了一个'''&amp;lt;font color = &amp;quot;#ff8000&amp;quot;&amp;gt;常微分方程 Ordinary Differential Equation&amp;lt;/font&amp;gt;'''-- 反过来，这些方程也更容易求解。&lt;br /&gt;
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This is possible for simple PDEs, which are called [[separable partial differential equation]]s, and the domain is generally a rectangle (a product of intervals). Separable PDEs correspond to [[diagonal matrices]] – thinking of &amp;quot;the value for fixed {{mvar|x}}&amp;quot; as a coordinate, each coordinate can be understood separately.&lt;br /&gt;
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This is possible for simple PDEs, which are called separable partial differential equations, and the domain is generally a rectangle (a product of intervals). Separable PDEs correspond to diagonal matrices – thinking of &amp;quot;the value for fixed &amp;quot; as a coordinate, each coordinate can be understood separately.&lt;br /&gt;
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对于简单的偏微分方程(称为可分离偏微分方程)来说，这是可能的，而且方程通常定义在一个矩形区域(区间的乘积)上。可分离偏微分方程对应于对角线矩阵——以“固定值”为坐标，每个坐标可分开理解。&lt;br /&gt;
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This generalizes to the [[method of characteristics]], and is also used in [[integral transform]]s.&lt;br /&gt;
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This generalizes to the method of characteristics, and is also used in integral transforms.&lt;br /&gt;
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这种方法可以推广到特征曲线法，也可以用于积分变换。&lt;br /&gt;
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===Method of characteristics===&lt;br /&gt;
特征曲线法&lt;br /&gt;
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{{main|Method of characteristics}}&lt;br /&gt;
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In special cases, one can find characteristic curves on which the equation reduces to an ODE – changing coordinates in the domain to straighten these curves allows separation of variables, and is called the [[method of characteristics]].&lt;br /&gt;
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In special cases, one can find characteristic curves on which the equation reduces to an ODE – changing coordinates in the domain to straighten these curves allows separation of variables, and is called the method of characteristics.&lt;br /&gt;
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在特殊情况下，可以找到一些特征曲线，在这些曲线上方程可以变成一个常微分方程——意味着改变坐标从而使这些曲线变直从而达到分离变量的目的，这就是所谓的特征曲线法。&lt;br /&gt;
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More generally, one may find characteristic surfaces.&lt;br /&gt;
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More generally, one may find characteristic surfaces.&lt;br /&gt;
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更一般地说，人们可能会找到特征表面。&lt;br /&gt;
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===Integral transform===&lt;br /&gt;
积分变换&lt;br /&gt;
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An [[integral transform]] may transform the PDE to a simpler one, in particular, a separable PDE. This corresponds to diagonalizing an operator.&lt;br /&gt;
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An integral transform may transform the PDE to a simpler one, in particular, a separable PDE. This corresponds to diagonalizing an operator.&lt;br /&gt;
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积分变换可以将偏微分方程转换为更简单的偏微分方程，特别是可分离的偏微分方程。这对应于对角化算符。&lt;br /&gt;
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An important example of this is [[Fourier analysis]], which diagonalizes the heat equation using the [[eigenbasis]] of sinusoidal waves.&lt;br /&gt;
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An important example of this is Fourier analysis, which diagonalizes the heat equation using the eigenbasis of sinusoidal waves.&lt;br /&gt;
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这方面的一个重要例子是'''&amp;lt;font color = &amp;quot;#ff8000&amp;quot;&amp;gt;傅里叶分析  Fourier Analysis&amp;lt;/font&amp;gt;'''，它使用正弦波的特征基来对角化热方程。&lt;br /&gt;
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If the domain is finite or periodic, an infinite sum of solutions such as a [[Fourier series]] is appropriate, but an integral of solutions such as a [[Fourier integral]] is generally required for infinite domains. The solution for a point source for the heat equation given above is an example of the use of a Fourier integral.&lt;br /&gt;
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If the domain is finite or periodic, an infinite sum of solutions such as a Fourier series is appropriate, but an integral of solutions such as a Fourier integral is generally required for infinite domains. The solution for a point source for the heat equation given above is an example of the use of a Fourier integral.&lt;br /&gt;
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如果区域是有限的或周期性的，那么解为无限和的形式是恰当的，例如傅里叶级数，但是一个解的积分，例如傅立叶积分，一般是在无限区域上的。上面给出的热传导方程的点源解法就是使用傅里叶积分的一个例子。&lt;br /&gt;
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===Change of variables===&lt;br /&gt;
变量代换&lt;br /&gt;
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Often a PDE can be reduced to a simpler form with a known solution by a suitable [[Change of variables (PDE)|change of variables]].  For example, the [[Black–Scholes equation#Derivation|Black–Scholes]] PDE&lt;br /&gt;
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Often a PDE can be reduced to a simpler form with a known solution by a suitable change of variables.  For example, the Black–Scholes PDE&lt;br /&gt;
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偏微分方程通常可以通过变量的适当变化，用已知的解简化为更简单的形式。例如，布莱克-舒尔斯偏微分方程&lt;br /&gt;
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:&amp;lt;math&amp;gt; \frac{\partial V}{\partial t} + \tfrac{1}{2}\sigma^2 S^2\frac{\partial^2 V}{\partial S^2} + rS\frac{\partial V}{\partial S} - rV = 0 &amp;lt;/math&amp;gt;&lt;br /&gt;
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&amp;lt;math&amp;gt; \frac{\partial V}{\partial t} + \tfrac{1}{2}\sigma^2 S^2\frac{\partial^2 V}{\partial S^2} + rS\frac{\partial V}{\partial S} - rV = 0 &amp;lt;/math&amp;gt;&lt;br /&gt;
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is reducible to the [[heat equation]]&lt;br /&gt;
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is reducible to the heat equation&lt;br /&gt;
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可以简化为热传导方程&lt;br /&gt;
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:&amp;lt;math&amp;gt; \frac{\partial u}{\partial \tau} = \frac{\partial^2 u}{\partial x^2}&amp;lt;/math&amp;gt;&lt;br /&gt;
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&amp;lt;math&amp;gt; \frac{\partial u}{\partial \tau} = \frac{\partial^2 u}{\partial x^2}&amp;lt;/math&amp;gt;&lt;br /&gt;
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by the change of variables (for complete details see {{webarchive |url=https://web.archive.org/web/20080411030405/http://www.math.unl.edu/~sdunbar1/Teaching/MathematicalFinance/Lessons/BlackScholes/Solution/solution.shtml |date=April 11, 2008 |title=Solution of the Black Scholes Equation }})&lt;br /&gt;
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by the change of variables (for complete details see )&lt;br /&gt;
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通过变量替换(完整的细节见)&lt;br /&gt;
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:&amp;lt;math&amp;gt;\begin{align}&lt;br /&gt;
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V(S,t) &amp;amp;= K v(x,\tau),\\[5px]&lt;br /&gt;
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x &amp;amp;= \ln\left(\tfrac{S}{K} \right),\\[5px]&lt;br /&gt;
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\tau &amp;amp;= \tfrac{1}{2} \sigma^2 (T - t),\\[5px]&lt;br /&gt;
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v(x,\tau)&amp;amp;=e^{-\alpha x-\beta\tau} u(x,\tau).&lt;br /&gt;
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\end{align}&amp;lt;/math&amp;gt;&lt;br /&gt;
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===Fundamental solution===&lt;br /&gt;
基本解&lt;br /&gt;
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{{main|Fundamental solution}}&lt;br /&gt;
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Inhomogeneous equations can often be solved (for constant coefficient PDEs, always be solved) by finding the [[fundamental solution]] (the solution for a point source), then taking the [[convolution]] with the boundary conditions to get the solution.&lt;br /&gt;
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Inhomogeneous equations can often be solved (for constant coefficient PDEs, always be solved) by finding the fundamental solution (the solution for a point source), then taking the convolution with the boundary conditions to get the solution.&lt;br /&gt;
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非齐次方程(常系数偏微分方程)一般是通过先求出基本解(点源的解) ，然后利用带边界条件的卷积来求解。&lt;br /&gt;
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This is analogous in [[signal processing]] to understanding a filter by its [[impulse response]].&lt;br /&gt;
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This is analogous in signal processing to understanding a filter by its impulse response.&lt;br /&gt;
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这类似于在信号处理中通过滤波器的脉冲响应来理解滤波器。&lt;br /&gt;
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===Superposition principle===&lt;br /&gt;
叠加原理&lt;br /&gt;
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{{further| Superposition principle }}&lt;br /&gt;
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The superposition principle applies to any linear system, including linear systems of PDEs. A common visualization of this concept is the interaction of two waves in phase being combined to result in a greater amplitude, for example {{math|sin ''x'' + sin ''x'' {{=}} 2 sin ''x''}}. The same principle can be observed in PDEs where the solutions may be real or complex and additive. [[Superposition principle|superposition]]&lt;br /&gt;
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The superposition principle applies to any linear system, including linear systems of PDEs. A common visualization of this concept is the interaction of two waves in phase being combined to result in a greater amplitude, for example  2 sin x}}. The same principle can be observed in PDEs where the solutions may be real or complex and additive. superposition&lt;br /&gt;
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'''&amp;lt;font color = &amp;quot;#ff8000&amp;quot;&amp;gt;叠加原理 Superposition Principle&amp;lt;/font&amp;gt;适用于任何线性系统，包括偏微分方程的线性系统。这个概念的一个常见的可视化是两个同相位的波相互作用结合在一起会产生更大的振幅，例如 {{math|sin ''x'' + sin ''x'' {{=}} 2 sin ''x''}}。在偏微分方程中也可以观察到同样的原理，其中的解可能是真实的或复杂的和可加的。叠加&lt;br /&gt;
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If {{math|''u''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;}} and {{math|''u''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;}} are solutions of linear PDE in some function space {{mvar|R}}, then {{math|''u'' {{=}} ''c''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;''u''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; + ''c''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;''u''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;}} with any constants {{math|''c''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;}} and {{math|''c''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;}} are also a solution of that PDE in the same function space.&lt;br /&gt;
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If  and  are solutions of linear PDE in some function space , then  c&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;u&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; + c&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;u&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;}} with any constants  and  are also a solution of that PDE in the same function space.&lt;br /&gt;
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若线性偏微分方程在某个函数空间{{mvar|R}}中有解{{math|''u''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;}} 和 {{math|''u''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;}}，则{{math|''u'' {{=}} ''c''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;''u''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; + ''c''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;''u''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;}}也是该偏微分方程在同一函数空间中的解，其中{{math|''c''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;}} 和 {{math|''c''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;}} 是任意常数。&lt;br /&gt;
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===Methods for non-linear equations===&lt;br /&gt;
非线性方程的求解方法&lt;br /&gt;
{{see also|nonlinear partial differential equation}}&lt;br /&gt;
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There are no generally applicable methods to solve nonlinear PDEs. Still, existence and uniqueness results (such as the [[Cauchy–Kowalevski theorem]]) are often possible, as are proofs of important qualitative and quantitative properties of solutions (getting these results is a major part of [[mathematical analysis|analysis]]). Computational solution to the nonlinear PDEs, the [[split-step method]], exist for specific equations like [[nonlinear Schrödinger equation]].&lt;br /&gt;
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There are no generally applicable methods to solve nonlinear PDEs. Still, existence and uniqueness results (such as the Cauchy–Kowalevski theorem) are often possible, as are proofs of important qualitative and quantitative properties of solutions (getting these results is a major part of analysis). Computational solution to the nonlinear PDEs, the split-step method, exist for specific equations like nonlinear Schrödinger equation.&lt;br /&gt;
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对于非线性偏微分方程，目前还没有普遍适用的求解方法。然而，通常是可能知道解的存在性和唯一性(如柯西-科瓦列夫斯基定理)，也是可能得到解的重要定性和定量性质的证明(得到这些结果是分析的主要部分)。非线性偏微分方程的计算解，即分步法，对一些特定的方程适用，比如非线性'''&amp;lt;font color=&amp;quot;#ff8000&amp;quot;&amp;gt;薛定谔方程 Schrödinger equation&amp;lt;/font&amp;gt;'''。&lt;br /&gt;
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Nevertheless, some techniques can be used for several types of equations. The [[h-principle|{{mvar|h}}-principle]] is the most powerful method to solve [[Underdetermined system|underdetermined]] equations. The [[Riquier–Janet theory]] is an effective method for obtaining information about many analytic [[Overdetermined system|overdetermined]] systems.&lt;br /&gt;
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Nevertheless, some techniques can be used for several types of equations. The -principle is the most powerful method to solve underdetermined equations. The Riquier–Janet theory is an effective method for obtaining information about many analytic overdetermined systems.&lt;br /&gt;
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然而，一些技巧可以用于几种类型的方程。h-原理是求解欠定方程最有效的方法。里基尔-珍妮特理论是一种可以获得许多解析超定系统信息的有效方法。&lt;br /&gt;
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The [[method of characteristics]] can be used in some very special cases to solve partial differential equations.&lt;br /&gt;
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The method of characteristics can be used in some very special cases to solve partial differential equations.&lt;br /&gt;
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特征线法可用于求解某些特殊情况下的偏微分方程。&lt;br /&gt;
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In some cases, a PDE can be solved via [[perturbation analysis]] in which the solution is considered to be a correction to an equation with a known solution. Alternatives are [[numerical analysis]] techniques from simple [[finite difference]] schemes to the more mature [[multigrid]] and [[finite element method]]s. Many interesting problems in science and engineering are solved in this way using [[computer]]s, sometimes high performance [[supercomputer]]s.&lt;br /&gt;
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In some cases, a PDE can be solved via perturbation analysis in which the solution is considered to be a correction to an equation with a known solution. Alternatives are numerical analysis techniques from simple finite difference schemes to the more mature multigrid and finite element methods. Many interesting problems in science and engineering are solved in this way using computers, sometimes high performance supercomputers.&lt;br /&gt;
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在某些情况下，偏微分方程可以通过扰动分析来求解。在扰动分析中，通常是求解将具有已知解的方程修正后的新得到方程。可供选择的数值分析技术从简单的差分格式到更成熟的多重网格和有限元方法。许多有趣的科学和工程问题都是在计算机上用这种方法解决的，有时是高性能超级计算机。&lt;br /&gt;
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===Lie group method===&lt;br /&gt;
李群方法&lt;br /&gt;
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From 1870 [[Sophus Lie]]'s work put the theory of differential equations on a more satisfactory foundation. He showed that the integration theories of the older mathematicians can, by the introduction of what are now called [[Lie group]]s, be referred, to a common source; and that ordinary differential equations which admit the same [[infinitesimal transformation]]s present comparable difficulties of integration. He also emphasized the subject of [[contact transformation|transformations of contact]].&lt;br /&gt;
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From 1870 Sophus Lie's work put the theory of differential equations on a more satisfactory foundation. He showed that the integration theories of the older mathematicians can, by the introduction of what are now called Lie groups, be referred, to a common source; and that ordinary differential equations which admit the same infinitesimal transformations present comparable difficulties of integration. He also emphasized the subject of transformations of contact.&lt;br /&gt;
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从1870年起，索弗斯·李的工作为微分方程理论奠定了一个较为令人满意的基础。他指出，通过引入现在所谓的李群，老一辈数学家的积分理论可以引用到一个共同的来源; 承认相同的无穷小变换的常微分方程在积分方面存在相当的困难。他还强调了接触的转变这一主题。&lt;br /&gt;
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==[[用户:Yuling|Yuling]]（[[用户讨论:Yuling|讨论]]）这句话“He also emphasized the subject of transformations of contact.”中的transformations of contact翻译的不太好。&lt;br /&gt;
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A general approach to solving PDEs uses the symmetry property of differential equations, the continuous [[infinitesimal transformation]]s of solutions to solutions ([[Lie theory]]). Continuous [[group theory]], [[Lie algebras]] and [[differential geometry]] are used to understand the structure of linear and nonlinear partial differential equations for generating integrable equations, to find its [[Lax pair]]s, recursion operators, [[Bäcklund transform]] and finally finding exact analytic solutions to the PDE.&lt;br /&gt;
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A general approach to solving PDEs uses the symmetry property of differential equations, the continuous infinitesimal transformations of solutions to solutions (Lie theory). Continuous group theory, Lie algebras and differential geometry are used to understand the structure of linear and nonlinear partial differential equations for generating integrable equations, to find its Lax pairs, recursion operators, Bäcklund transform and finally finding exact analytic solutions to the PDE.&lt;br /&gt;
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求解偏微分方程的一般方法是利用微分方程的对称性，即解到解的连续无穷小变换(李理论)。连续群论、李代数和微分几何理论被用来理解生成可积方程的线性和非线性偏微分方程的结构，找到它的Lax对、递归算子、 贝克伦德变换，最后找到偏微分方程的精确解析解。&lt;br /&gt;
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Symmetry methods have been recognized to study differential equations arising in mathematics, physics, engineering, and many other disciplines.&lt;br /&gt;
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Symmetry methods have been recognized to study differential equations arising in mathematics, physics, engineering, and many other disciplines.&lt;br /&gt;
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对称方法已被公认可以用于研究出现在数学，物理，工程和许多其他学科的微分方程。&lt;br /&gt;
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===Semianalytical methods===&lt;br /&gt;
半解析方法&lt;br /&gt;
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The [[Adomian decomposition method]], the [[Aleksandr Lyapunov|Lyapunov]] artificial small parameter method, and He's [[homotopy perturbation method]] are all special cases of the more general [[homotopy analysis method]]. These are series expansion methods, and except for the Lyapunov method, are independent of small physical parameters as compared to the well known [[perturbation theory]], thus giving these methods greater flexibility and solution generality.&lt;br /&gt;
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The Adomian decomposition method, the Lyapunov artificial small parameter method, and He's homotopy perturbation method are all special cases of the more general homotopy analysis method. These are series expansion methods, and except for the Lyapunov method, are independent of small physical parameters as compared to the well known perturbation theory, thus giving these methods greater flexibility and solution generality.&lt;br /&gt;
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阿多米安分解法、李雅普诺夫人工小参数方法和何同伦摄动方法都是更一般的同伦分析方法的特殊情况。除了李雅普诺夫方法之外，这些都是级数展开方法，与为人熟知的摄动理论方法相比，它们与小的物理参数无关，因此这些方法具有更大的灵活性和解的通用性。&lt;br /&gt;
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== Numerical solutions ==&lt;br /&gt;
数值解&lt;br /&gt;
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The three most widely used [[Numerical partial differential equations|numerical methods to solve PDEs]] are the [[finite element analysis|finite element method]] (FEM), [[finite volume method]]s (FVM) and [[finite difference method]]s (FDM), as well other kind of methods called [[Meshfree methods]], which were made to solve problems where the before mentioned methods are limited. The FEM has a prominent position among these methods and especially its exceptionally efficient higher-order version [[hp-FEM]]. Other hybrid versions of FEM and Meshfree methods include the generalized finite element method (GFEM), [[extended finite element method]] (XFEM), [[Spectral element method|spectral finite element method]] (SFEM), [[Meshfree methods|meshfree finite element method]], [[Discontinuous Galerkin Method|discontinuous Galerkin finite element method]] (DGFEM), [[Element-Free Galerkin Method]] (EFGM), [[Interpolating Element-Free Galerkin Method]] (IEFGM), etc.&lt;br /&gt;
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The three most widely used numerical methods to solve PDEs are the finite element method (FEM), finite volume methods (FVM) and finite difference methods (FDM), as well other kind of methods called Meshfree methods, which were made to solve problems where the before mentioned methods are limited. The FEM has a prominent position among these methods and especially its exceptionally efficient higher-order version hp-FEM. Other hybrid versions of FEM and Meshfree methods include the generalized finite element method (GFEM), extended finite element method (XFEM), spectral finite element method (SFEM), meshfree finite element method, discontinuous Galerkin finite element method (DGFEM), Element-Free Galerkin Method (EFGM), Interpolating Element-Free Galerkin Method (IEFGM), etc.&lt;br /&gt;
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求解偏微分方程最常用的三种数值方法是有限元分析法、有限体积法和有限差分法，以及其他一些称为无网格法的方法。这些方法用于解决前面提到的方法受到的限制。在这些方法中，有限元方法，尤其是高效的高阶有限元方法，占有重要地位。其他有限元法和无网格法的混合形式包括广义有限元分析法(GFEM)、扩展有限元分析法(XFEM)、谱有限元分析法(SFEM)、无网格有限元分析法(DGFEM)、间断伽辽金有限元分析法(DGFEM)、无网格伽辽金法(EFGM)、插值无网格伽辽金法(IEFGM)等。&lt;br /&gt;
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=== Finite element method ===&lt;br /&gt;
有限元分析法&lt;br /&gt;
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{{main|Finite element method}}&lt;br /&gt;
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The finite element method (FEM) (its practical application often known as finite element analysis (FEA)) is a numerical technique for finding approximate solutions of partial differential equations (PDE) as well as of integral equations. The solution approach is based either on eliminating the differential equation completely (steady state problems), or rendering the PDE into an approximating system of ordinary differential equations, which are then numerically integrated using standard techniques such as Euler's method, Runge–Kutta, etc.&lt;br /&gt;
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The finite element method (FEM) (its practical application often known as finite element analysis (FEA)) is a numerical technique for finding approximate solutions of partial differential equations (PDE) as well as of integral equations. The solution approach is based either on eliminating the differential equation completely (steady state problems), or rendering the PDE into an approximating system of ordinary differential equations, which are then numerically integrated using standard techniques such as Euler's method, Runge–Kutta, etc.&lt;br /&gt;
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'''&amp;lt;font color = &amp;quot;#ff8000&amp;quot;&amp;gt;有限元分析法 Finite Element Method&amp;lt;/font&amp;gt;''' ((其实际应用通常被称为有限元分析(FEA))是一种寻找偏微分方程(PDE)和积分方程近似解的数值技术。这种求解方法要么基于完全消除微分方程(稳态问题) ，要么将偏微分方程转化为常微分方程的近似系统，然后使用标准技术进行数值积分，如欧拉方法、 Runge-Kutta 等。&lt;br /&gt;
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===Finite difference method===&lt;br /&gt;
有限差分法&lt;br /&gt;
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{{main|Finite difference method}}&lt;br /&gt;
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Finite-difference methods are numerical methods for approximating the solutions to differential equations using [[finite difference]] equations to approximate derivatives.&lt;br /&gt;
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Finite-difference methods are numerical methods for approximating the solutions to differential equations using finite difference equations to approximate derivatives.&lt;br /&gt;
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有限差分法是一种数值方法，用差分方程近似微分方程的解。&lt;br /&gt;
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=== Finite volume method ===&lt;br /&gt;
有限体积法&lt;br /&gt;
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{{main|Finite volume method}}&lt;br /&gt;
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Similar to the finite difference method or finite element method, values are calculated at discrete places on a meshed geometry. &amp;quot;Finite volume&amp;quot; refers to the small volume surrounding each node point on a mesh. In the finite volume method, surface integrals in a partial differential equation that contain a divergence term are converted to volume integrals, using the [[divergence theorem]]. These terms are then evaluated as fluxes at the surfaces of each finite volume. Because the flux entering a given volume is identical to that leaving the adjacent volume, these methods conserve mass by design.&lt;br /&gt;
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Similar to the finite difference method or finite element method, values are calculated at discrete places on a meshed geometry. &amp;quot;Finite volume&amp;quot; refers to the small volume surrounding each node point on a mesh. In the finite volume method, surface integrals in a partial differential equation that contain a divergence term are converted to volume integrals, using the divergence theorem. These terms are then evaluated as fluxes at the surfaces of each finite volume. Because the flux entering a given volume is identical to that leaving the adjacent volume, these methods conserve mass by design.&lt;br /&gt;
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类似于有限差分法或有限元分析，函数值是在网状几何体上的离散位置进行计算的。“有限体积”是指网格上每个节点周围的小体积。在有限体积法中，偏微分方程中含有散度项的面积分用散度定理积分转换成体积分。然后将这些项用于估算每个有限体积表面上的通量。由于进入给定体积的通量与转移到相邻体积元的通量相同，所以这些方法在设计上保证了质量守恒。&lt;br /&gt;
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==See also==&lt;br /&gt;
请参阅&lt;br /&gt;
* [[Dirichlet boundary condition]]&lt;br /&gt;
狄利克雷边界条件&lt;br /&gt;
* [[Jet bundle]]&lt;br /&gt;
射流丛&lt;br /&gt;
* [[Laplace transform applied to differential equations]]&lt;br /&gt;
微分方程中的拉普拉斯变换&lt;br /&gt;
* [[List of dynamical systems and differential equations topics]]&lt;br /&gt;
动力学系统和微分方程的列表&lt;br /&gt;
* [[Matrix differential equation]]&lt;br /&gt;
矩阵微分方程&lt;br /&gt;
* [[Neumann boundary condition]]&lt;br /&gt;
诺伊曼边界条件&lt;br /&gt;
* [[Numerical partial differential equations]]&lt;br /&gt;
数值偏微分方程&lt;br /&gt;
* [[Partial differential algebraic equation]]&lt;br /&gt;
偏微分代数方程&lt;br /&gt;
* [[Recurrence relation]]&lt;br /&gt;
递推关系&lt;br /&gt;
* [[Robin boundary condition]]&lt;br /&gt;
罗宾边界条件&lt;br /&gt;
* [[Stochastic processes and boundary value problems]]&lt;br /&gt;
随机过程和边值问题&lt;br /&gt;
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== The energy method ==&lt;br /&gt;
能量法&lt;br /&gt;
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The energy method is a mathematical procedure that can be used to verify well-posedness of initial-boundary-value-problems.&amp;lt;ref&amp;gt;{{cite book |title=High Order Difference Methods for Time Dependent PDE&lt;br /&gt;
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The energy method is a mathematical procedure that can be used to verify well-posedness of initial-boundary-value-problems.&amp;lt;ref&amp;gt;{{cite book |title=High Order Difference Methods for Time Dependent PDE&lt;br /&gt;
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能量法是验证初边值问题适定性的一种数学方法。 时变偏微分方程的高阶差分方法&lt;br /&gt;
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|first=Bertil|last=Gustafsson|publisher=Springer|year=2008|isbn=978-3-540-74992-9|doi=10.1007/978-3-540-74993-6}}&amp;lt;/ref&amp;gt; In the following example the energy method is used to decide where and which boundary conditions should be imposed such that the resulting IBVP is well-posed. Consider the one-dimensional hyperbolic PDE given by&lt;br /&gt;
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|first=Bertil|last=Gustafsson|publisher=Springer|year=2008|isbn=978-3-540-74992-9|doi=10.1007/978-3-540-74993-6}}&amp;lt;/ref&amp;gt; In the following example the energy method is used to decide where and which boundary conditions should be imposed such that the resulting IBVP is well-posed. Consider the one-dimensional hyperbolic PDE given by&lt;br /&gt;
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| first Bertil | last Gustafsson | publisher | Springer | year 2008 | isbn 978-3-540-74992-9 | doi 10.1007 / 978-3-540-74993-6} / ref 在下面的例子中，使用能量方法来决定应该施加哪些边界条件，使得得到的 IBVP适定。考虑一维双曲偏微分方程&lt;br /&gt;
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: &amp;lt;math&amp;gt;\frac{\partial u}{\partial t} + \alpha \frac{\partial u}{\partial x} = 0, \quad x \in [a,b], \operatorname t &amp;gt; 0,&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;\frac{\partial u}{\partial t} + \alpha \frac{\partial u}{\partial x} = 0, \quad x \in [a,b], \operatorname t &amp;gt; 0,&amp;lt;/math&amp;gt;&lt;br /&gt;
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where &amp;lt;math&amp;gt;\alpha \neq 0&amp;lt;/math&amp;gt; is a constant and &amp;lt;math&amp;gt;u(x,t)&amp;lt;/math&amp;gt; is an unknown function with initial condition &amp;lt;math&amp;gt;u(x,0) = f(x)&amp;lt;/math&amp;gt;. Multiplying with &amp;lt;math&amp;gt;u&amp;lt;/math&amp;gt; and integrating over the domain gives&lt;br /&gt;
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where &amp;lt;math&amp;gt;\alpha \neq 0&amp;lt;/math&amp;gt; is a constant and &amp;lt;math&amp;gt;u(x,t)&amp;lt;/math&amp;gt; is an unknown function with initial condition &amp;lt;math&amp;gt;u(x,0) = f(x)&amp;lt;/math&amp;gt;. Multiplying with &amp;lt;math&amp;gt;u&amp;lt;/math&amp;gt; and integrating over the domain gives&lt;br /&gt;
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其中 &amp;lt;math&amp;gt;\alpha \neq 0&amp;lt;/math&amp;gt; 是常数，并且 &amp;lt;math&amp;gt;u(x,t)&amp;lt;/math&amp;gt; 是未知函数，初始条件是 &amp;lt;math&amp;gt;u(x,0) = f(x)&amp;lt;/math&amp;gt;。乘以 &amp;lt;math&amp;gt;u&amp;lt;/math&amp;gt; 并在域上进行积分。&lt;br /&gt;
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: &amp;lt;math&amp;gt;\int_a^b u \frac{\partial u}{\partial t} \operatorname dx + \alpha \int _a ^b u \frac{\partial u}{\partial x} \operatorname dx = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;\int_a^b u \frac{\partial u}{\partial t} \operatorname dx + \alpha \int _a ^b u \frac{\partial u}{\partial x} \operatorname dx = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
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Using that&lt;br /&gt;
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Using that&lt;br /&gt;
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利用这一点&lt;br /&gt;
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: &amp;lt;math&amp;gt;\int _a ^b u \frac{\partial u}{\partial t} \operatorname dx = \frac{1}{2} \frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 \quad \text{and} \quad \int _a ^b u \frac{\partial u}{\partial x} \operatorname dx = \frac{1}{2} u(b,t)^2 - \frac{1}{2} u(a,t)^2,.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;\int _a ^b u \frac{\partial u}{\partial t} \operatorname dx = \frac{1}{2} \frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 \quad \text{and} \quad \int _a ^b u \frac{\partial u}{\partial x} \operatorname dx = \frac{1}{2} u(b,t)^2 - \frac{1}{2} u(a,t)^2,.&amp;lt;/math&amp;gt;&lt;br /&gt;
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where integration by parts has been used for the second relationship, we get&lt;br /&gt;
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where integration by parts has been used for the second relationship, we get&lt;br /&gt;
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第二个关系中采用了分部积分法，我们可以得到&lt;br /&gt;
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: &amp;lt;math&amp;gt;\frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 + \alpha u(b,t)^2 - \alpha u(a,t)^2 = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;\frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 + \alpha u(b,t)^2 - \alpha u(a,t)^2 = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
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Here &amp;lt;math&amp;gt;\vert \vert \cdot \vert \vert&amp;lt;/math&amp;gt; denotes the standard L2-norm.&lt;br /&gt;
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Here &amp;lt;math&amp;gt;\vert \vert \cdot \vert \vert&amp;lt;/math&amp;gt; denotes the standard L2-norm.&lt;br /&gt;
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在这里，&amp;lt;math&amp;gt;\vert \vert \cdot \vert \vert&amp;lt;/math&amp;gt; 表示标准的 L2-正则。&lt;br /&gt;
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For well-posedness we require that the energy of the solution is non-increasing, i.e. that &amp;lt;math&amp;gt;\frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 \leq 0&amp;lt;/math&amp;gt;, which is achieved by specifying &amp;lt;math&amp;gt;u&amp;lt;/math&amp;gt; at &amp;lt;math&amp;gt;x = a&amp;lt;/math&amp;gt; if &amp;lt;math&amp;gt;\alpha &amp;gt; 0&amp;lt;/math&amp;gt; and at &amp;lt;math&amp;gt;x = b&amp;lt;/math&amp;gt; if &amp;lt;math&amp;gt;\alpha &amp;lt; 0&amp;lt;/math&amp;gt;. This corresponds to only imposing boundary conditions at the inflow. Note that well-posedness allows for growth in terms of data (initial and boundary) and thus it is sufficient to show that &amp;lt;math&amp;gt;\frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 \leq 0&amp;lt;/math&amp;gt; holds when all data is set to zero.&lt;br /&gt;
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For well-posedness we require that the energy of the solution is non-increasing, i.e. that &amp;lt;math&amp;gt;\frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 \leq 0&amp;lt;/math&amp;gt;, which is achieved by specifying &amp;lt;math&amp;gt;u&amp;lt;/math&amp;gt; at &amp;lt;math&amp;gt;x = a&amp;lt;/math&amp;gt; if &amp;lt;math&amp;gt;\alpha &amp;gt; 0&amp;lt;/math&amp;gt; and at &amp;lt;math&amp;gt;x = b&amp;lt;/math&amp;gt; if &amp;lt;math&amp;gt;\alpha &amp;lt; 0&amp;lt;/math&amp;gt;. This corresponds to only imposing boundary conditions at the inflow. Note that well-posedness allows for growth in terms of data (initial and boundary) and thus it is sufficient to show that &amp;lt;math&amp;gt;\frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 \leq 0&amp;lt;/math&amp;gt; holds when all data is set to zero.&lt;br /&gt;
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对于适定性，我们要解的能量是不增加的，即 &amp;lt;math&amp;gt;\frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 \leq 0&amp;lt;/math&amp;gt; ，这种关系可以通过在&amp;lt;math&amp;gt;x = a&amp;lt;/math&amp;gt;处 （如果 &amp;lt;math&amp;gt;\alpha &amp;gt; 0&amp;lt;/math&amp;gt;） 以及 &amp;lt;math&amp;gt;x = b&amp;lt;/math&amp;gt;处 （如果 &amp;lt;math&amp;gt;\alpha &amp;lt; 0&amp;lt;/math&amp;gt;）指定&amp;lt;math&amp;gt;u&amp;lt;/math&amp;gt;的值来实现。这只相当于在入流处附加边界条件。注意，适定性允许在数据(初始和边界)上的增长，因此它足以表明当所有数据设置为零时应有 &amp;lt;math&amp;gt;\frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 \leq 0&amp;lt;/math&amp;gt;。&lt;br /&gt;
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==[[用户:Yuling|Yuling]]（[[用户讨论:Yuling|讨论]]）“This corresponds to only imposing boundary conditions at the inflow.” 这句话中的inflow不是很理解&lt;br /&gt;
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==Notes==&lt;br /&gt;
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{{Reflist}}&lt;br /&gt;
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== References ==&lt;br /&gt;
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{{refbegin|2}}&lt;br /&gt;
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* {{cite book |title=Solving Frontier problems of Physics: The decomposition method&lt;br /&gt;
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|first=G.|last=Adomian|publisher=Kluwer Academic Publishers|year=1994|isbn=|page=|url=https://books.google.com/books?id=UKPqCAAAQBAJ&amp;amp;printsec=frontcover#v=onepage&amp;amp;q=%22partial%20differential%22&amp;amp;f=false}}&lt;br /&gt;
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1994年 | isbn | 页面 | 网址: 施普林格科学+商业媒体 https://books.google.com/books?id=ukpqcaaaqbaj&amp;amp;printsec=frontcover#v=onepage&amp;amp;q=%22partial%20differential%22&amp;amp;f=false&lt;br /&gt;
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* {{Citation |first=A. D. |last=Polyanin |title=Handbook of Linear Partial Differential Equations for Engineers and Scientists |publisher=Chapman &amp;amp; Hall/CRC Press |location=Boca Raton |year=2002 |isbn=1-58488-299-9 }}.&lt;br /&gt;
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* {{Citation |first=A. D. |last=Polyanin |lastauthoramp=yes |first2=V. F. |last2=Zaitsev |title=Handbook of Nonlinear Partial Differential Equations |publisher=Chapman &amp;amp; Hall/CRC Press |location=Boca Raton |year=2004 |isbn=1-58488-355-3 }}.&lt;br /&gt;
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* {{Citation |first=A. D. |last=Polyanin |first2=V. F. |last2=Zaitsev |lastauthoramp=yes |first3=A. |last3=Moussiaux |title=Handbook of First Order Partial Differential Equations |publisher=Taylor &amp;amp; Francis |location=London |year=2002 |isbn=0-415-27267-X }}.&lt;br /&gt;
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* {{citation|mr=3014456|last=Roubíček|first= T.|title=Nonlinear Partial Differential Equations with Applications|publisher= Birkhäuser|place= Basel, Boston, Berlin|edition=2nd|year= 2013|ISBN= 978-3-0348-0512-4|doi=10.1007/978-3-0348-0513-1|url=http://cds.cern.ch/record/880983/files/9783764372934_TOC.pdf}}&lt;br /&gt;
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* {{Citation |first=P. |last=Solin |title=Partial Differential Equations and the Finite Element Method |publisher=J. Wiley &amp;amp; Sons |location=Hoboken, NJ |year=2005 |isbn=0-471-72070-4 }}.&lt;br /&gt;
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* {{Citation |first=P. |last=Solin |first2=K. |last2=Segeth |lastauthoramp=yes |first3=I. |last3=Dolezel |title=Higher-Order Finite Element Methods |publisher=Chapman &amp;amp; Hall/CRC Press |location=Boca Raton |year=2003 |isbn=1-58488-438-X }}.&lt;br /&gt;
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* {{Citation |first=H. |last=Stephani |year=1989 |title=Differential Equations: Their Solution Using Symmetries. Edited by M. MacCallum |publisher=Cambridge University Press }}.&lt;br /&gt;
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* {{cite book |title=Partial Differential Equations and Solitary Waves Theory&lt;br /&gt;
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|first=Abdul-Majid|last=Wazwaz|publisher=Higher Education Press|year=2009|isbn=978-3-642-00251-9|page=}}&lt;br /&gt;
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| first Abdul-Majid | last Wazwaz | publisher Higher Education Press | year 2009 | isbn 978-3-642-00251-9 | page }&lt;br /&gt;
&lt;br /&gt;
* {{cite book |title=Partial Differential Equations Methods and Applications&lt;br /&gt;
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|first=Abdul-Majid|last=Wazwaz|publisher=A.A. Balkema|year=2002|isbn=90-5809-369-7|page=}}&lt;br /&gt;
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|first=Abdul-Majid|last=Wazwaz|publisher=A.A. Balkema|year=2002|isbn=90-5809-369-7|page=}}&lt;br /&gt;
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| first Abdul-Majid | last Wazwaz | publisher a.a.Balkema | year 2002 | isbn 90-5809-369-7 | page }&lt;br /&gt;
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* {{Citation |first=D. |last=Zwillinger |title=Handbook of Differential Equations |publisher=Academic Press |location=Boston |year=1997 |edition=3rd |isbn=0-12-784395-7 }}.&lt;br /&gt;
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* {{Citation |authorlink=Neil Gershenfeld |first=N. |last=Gershenfeld |title=The Nature of Mathematical Modeling |location=New York |publisher=Cambridge University Press, New York, NY, USA |year=1999 |edition=1st |isbn=0-521-57095-6 }}.&lt;br /&gt;
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* {{Citation |first=I.S. |last=Krasil'shchik |lastauthoramp=yes |first2=A.M., Eds. |last2=Vinogradov |title=Symmetries and Conserwation Laws for Differential Equations of Mathematical Physics |publisher=American Mathematical Society, Providence, Rhode Island, USA |year=1999 |isbn=0-8218-0958-X }}.&lt;br /&gt;
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* {{Citation |first=I.S. |last=Krasil'shchik |first2=V.V. |last2=Lychagin|lastauthoramp=yes |first3=A.M. |last3=Vinogradov |title=Geometry of Jet Spaces and Nonlinear Partial Differential Equations |publisher=Gordon and Breach Science Publishers, New York, London, Paris, Montreux, Tokyo |year=1986 |isbn=2-88124-051-8 }}.&lt;br /&gt;
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* {{Citation |first=A.M. |last=Vinogradov |title=Cohomological Analysis of Partial Differential Equations and Secondary Calculus |publisher=American Mathematical Society, Providence, Rhode Island, USA |year=2001 |isbn=0-8218-2922-X }}.&lt;br /&gt;
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* {{cite book |title=High Order Difference Methods for Time Dependent PDE&lt;br /&gt;
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|first=Bertil|last=Gustafsson|publisher=Springer|year=2008|isbn=978-3-540-74992-9|doi=10.1007/978-3-540-74993-6}}&lt;br /&gt;
&lt;br /&gt;
|first=Bertil|last=Gustafsson|publisher=Springer|year=2008|isbn=978-3-540-74992-9|doi=10.1007/978-3-540-74993-6}}&lt;br /&gt;
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| first Bertil | last Gustafsson | Springer | year 2008 | isbn 978-3-540-74992-9 | doi 10.1007 / 978-3-540-74993-6}&lt;br /&gt;
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{{refend}}&lt;br /&gt;
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== Further reading ==&lt;br /&gt;
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* {{Cite journal|last=Cajori|first=Florian|authorlink=Florian Cajori|year=1928|title=The Early History of Partial Differential Equations and of Partial Differentiation and Integration|url=http://www.math.harvard.edu/archive/21a_fall_14/exhibits/cajori/cajori.pdf|journal=The American Mathematical Monthly|volume=35|issue=9|pages=459–467|doi=10.2307/2298771|access-date=2016-05-15|archive-url=https://web.archive.org/web/20181123102253/http://www.math.harvard.edu/archive/21a_fall_14/exhibits/cajori/cajori.pdf|archive-date=2018-11-23|url-status=dead}}&lt;br /&gt;
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== External links ==&lt;br /&gt;
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{{Sister project links| wikt=no | commons=Category:Solutions of PDE | b=Partial Differential Equations | n=no | q=Partial differential equation | s=no | v=no | voy=no | species=no | d=no}}&lt;br /&gt;
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* {{springer|title=Differential equation, partial|id=p/d031920}}&lt;br /&gt;
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* [http://eqworld.ipmnet.ru/en/pde-en.htm Partial Differential Equations: Exact Solutions] at EqWorld: The World of Mathematical Equations.&lt;br /&gt;
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* [http://eqworld.ipmnet.ru/en/solutions/eqindex/eqindex-pde.htm Partial Differential Equations: Index] at EqWorld: The World of Mathematical Equations.&lt;br /&gt;
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* [http://eqworld.ipmnet.ru/en/methods/meth-pde.htm Partial Differential Equations: Methods] at EqWorld: The World of Mathematical Equations.&lt;br /&gt;
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* [https://web.archive.org/web/20170701144823/http://www.exampleproblems.com/wiki/index.php?title=Partial_Differential_Equations Example problems with solutions] at exampleproblems.com&lt;br /&gt;
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* [http://mathworld.wolfram.com/PartialDifferentialEquation.html Partial Differential Equations] at mathworld.wolfram.com&lt;br /&gt;
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* [https://reference.wolfram.com/language/FEMDocumentation/tutorial/SolvingPDEwithFEM.html Partial Differential Equations] with Mathematica&lt;br /&gt;
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* [http://www.mathworks.com/moler/pdes.pdf Partial Differential Equations] in Cleve Moler: Numerical Computing with MATLAB&lt;br /&gt;
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* [http://www.nag.com/numeric/fl/nagdoc_fl24/html/D03/d03intro.html Partial Differential Equations] at nag.com&lt;br /&gt;
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* {{cite web |first=Grant |last=Sanderson |title=But what is a partial differential equation? |work=3Blue1Brown |date=April 21, 2019 |url=https://www.youtube.com/watch?v=ly4S0oi3Yz8&amp;amp;list=PLZHQObOWTQDNPOjrT6KVlfJuKtYTftqH6 |via=[[YouTube]] }}&lt;br /&gt;
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{{Differential equations topics}}&lt;br /&gt;
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[[Category:Partial differential equations| ]]&lt;br /&gt;
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[[Category:Multivariable calculus]]&lt;br /&gt;
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Category:Multivariable calculus&lt;br /&gt;
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类别: 多元微积分&lt;br /&gt;
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[[Category:Differential equations]]&lt;br /&gt;
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Category:Differential equations&lt;br /&gt;
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类别: 微分方程&lt;br /&gt;
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[[Category:Concepts in physics]]&lt;br /&gt;
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Category:Concepts in physics&lt;br /&gt;
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&amp;lt;small&amp;gt;This page was moved from [[wikipedia:en:Partial differential equation]]. Its edit history can be viewed at [[偏微分方程/edithistory]]&amp;lt;/small&amp;gt;&amp;lt;/noinclude&amp;gt;&lt;br /&gt;
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[[Category:待整理页面]]&lt;/div&gt;</summary>
		<author><name>Ruili</name></author>
	</entry>
	<entry>
		<id>https://wiki.swarma.org/index.php?title=%E5%81%8F%E5%BE%AE%E5%88%86%E6%96%B9%E7%A8%8B&amp;diff=18204</id>
		<title>偏微分方程</title>
		<link rel="alternate" type="text/html" href="https://wiki.swarma.org/index.php?title=%E5%81%8F%E5%BE%AE%E5%88%86%E6%96%B9%E7%A8%8B&amp;diff=18204"/>
		<updated>2020-11-12T16:02:57Z</updated>

		<summary type="html">&lt;p&gt;Ruili：&lt;/p&gt;
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&lt;div&gt;此词条暂由Yuling翻译，未经人工整理和审校，带来阅读不便，请见谅。&lt;br /&gt;
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[[File:Heat.gif|thumb|right|A visualisation of a solution to the two-dimensional [[heat equation]] with temperature represented by the third dimension]]&lt;br /&gt;
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A visualisation of a solution to the two-dimensional [[heat equation with temperature represented by the third dimension]]&lt;br /&gt;
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以三维表示温度的二维热方程解的可视化&lt;br /&gt;
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In [[mathematics]], a '''partial differential equation''' ('''PDE''') is a [[differential equation]] that contains unknown [[Multivariable calculus|multivariable functions]] and their [[partial derivative]]s. PDEs are used to formulate problems involving functions of several variables, and are either solved by hand, or used to create a [[computer model]]. A special case is [[ordinary differential equation]]s (ODEs), which deal with functions of a single variable and their derivatives.&lt;br /&gt;
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In mathematics, a partial differential equation (PDE) is a differential equation that contains unknown multivariable functions and their partial derivatives. PDEs are used to formulate problems involving functions of several variables, and are either solved by hand, or used to create a computer model. A special case is ordinary differential equations (ODEs), which deal with functions of a single variable and their derivatives.&lt;br /&gt;
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在数学中，'''&amp;lt;font color = &amp;quot;#ff8000&amp;quot;&amp;gt; 偏微分方程函数 Partial Differential Equation&amp;lt;/font&amp;gt;'''是包含未知多元函数及其偏导数的微分方程。偏微分方程用于描述涉及多元函数的问题，可以通过人为求解，也可以通过建立计算机模型来求解。常微分方程是偏微分方程一种特殊情况，它处理的是一元函数及其导数。&lt;br /&gt;
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PDEs can be used to describe a wide variety of phenomena such as sound, heat, [[diffusion]], [[electrostatics]], [[Electromagnetism|electrodynamics]], [[fluid dynamics]], [[Elasticity (physics)|elasticity]], [[gravitation]] and [[quantum mechanics]]. These seemingly distinct physical phenomena can be formalised similarly in terms of PDEs. Just as ordinary differential equations often model one-dimensional [[dynamical system]]s, partial differential equations often model [[multidimensional system]]s. PDEs find their generalisation in [[stochastic partial differential equation]]s.&lt;br /&gt;
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PDEs can be used to describe a wide variety of phenomena such as sound, heat, diffusion, electrostatics, electrodynamics, fluid dynamics, elasticity, gravitation and quantum mechanics. These seemingly distinct physical phenomena can be formalised similarly in terms of PDEs. Just as ordinary differential equations often model one-dimensional dynamical systems, partial differential equations often model multidimensional systems. PDEs find their generalisation in stochastic partial differential equations.&lt;br /&gt;
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偏微分方程可以用来描述各种各样的物理现象，如声音，热量，扩散，静电，电动力学，流体力学，弹性力学，重力和量子力学。这些看起来截然不同的物理现象却可以用类似的偏微分方程来描述。正如常微分方程经常对一维动力系统进行建模一样，偏微分方程经常对多维系统进行建模。随机偏微分方程是偏微分方程的一种推广。&lt;br /&gt;
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== Introduction ==&lt;br /&gt;
引言&lt;br /&gt;
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Partial differential equations (PDEs) are equations that involve rates of change with respect to [[continuous variables]]. For example, the position of a [[rigid body]] is specified by six parameters,&amp;lt;ref&amp;gt;{{Cite book|url=https://books.google.com/books?id=v9PLbcYd9aUC&amp;amp;pg=PA32|title=Modelling and Control of Robot Manipulators|last=Sciavicco|first=Lorenzo|last2=Siciliano|first2=Bruno|date=2001-02-19|publisher=Springer Science &amp;amp; Business Media|isbn=9781852332211|language=en}}&amp;lt;/ref&amp;gt; but the configuration of a [[fluid]] is given by the [[continuous distribution]] of several parameters, such as the [[temperature]], [[pressure]], and so forth. The dynamics for the rigid body take place in a finite-dimensional [[Configuration space (physics)|configuration space]]; the dynamics for the fluid occur in an infinite-dimensional configuration space. This distinction usually makes PDEs much harder to solve than ordinary differential equations (ODEs), but here again, there will be simple solutions for linear problems. Classic domains where PDEs are used include [[acoustics]], [[fluid dynamics]], [[electrodynamics]], and [[heat transfer]].&lt;br /&gt;
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Partial differential equations (PDEs) are equations that involve rates of change with respect to continuous variables. For example, the position of a rigid body is specified by six parameters, but the configuration of a fluid is given by the continuous distribution of several parameters, such as the temperature, pressure, and so forth. The dynamics for the rigid body take place in a finite-dimensional configuration space; the dynamics for the fluid occur in an infinite-dimensional configuration space. This distinction usually makes PDEs much harder to solve than ordinary differential equations (ODEs), but here again, there will be simple solutions for linear problems. Classic domains where PDEs are used include acoustics, fluid dynamics, electrodynamics, and heat transfer.&lt;br /&gt;
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偏微分方程(简称为PDEs)涉及到方程相对于连续变量的变化率。例如，刚体的位置是由六个参数确定的，而流体的状态是由几个参数的连续分布给出的，如温度、压力等。刚体的动力学过程发生在有限维状态空间中，流体的动力学过程发生在无限维状态空间中。这种区别通常使偏微分方程比常微分方程更难求解，但是线性问题仍然有简单的求解方式。使用偏微分方程的经典领域包括声学、流体力学、电动力学和传热学。&lt;br /&gt;
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A partial differential equation (PDE) for the function {{math|''u''(''x''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;,… ''x&amp;lt;sub&amp;gt;n&amp;lt;/sub&amp;gt;'')}} is an equation of the form&lt;br /&gt;
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A partial differential equation (PDE) for the function  is an equation of the form&lt;br /&gt;
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函数 {{math|''u''(''x''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;,… ''x&amp;lt;sub&amp;gt;n&amp;lt;/sub&amp;gt;'')}} 的偏微分方程形式是：&lt;br /&gt;
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: &amp;lt;math&amp;gt;f \left (x_1, \ldots x_n; u, \frac{\partial u}{\partial x_1}, \ldots \frac{\partial u}{\partial x_n}; \frac{\partial^2 u}{\partial x_1 \partial x_1}, \ldots \frac{\partial^2 u}{\partial x_1 \partial x_n}; \ldots \right) = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;f \left (x_1, \ldots x_n; u, \frac{\partial u}{\partial x_1}, \ldots \frac{\partial u}{\partial x_n}; \frac{\partial^2 u}{\partial x_1 \partial x_1}, \ldots \frac{\partial^2 u}{\partial x_1 \partial x_n}; \ldots \right) = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
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If {{mvar|f}} is a [[linear function]] of {{mvar|u}} and its derivatives, then the PDE is called linear. Common examples of linear PDEs include the [[heat equation]], the [[wave equation]], [[Laplace's equation]], [[Helmholtz equation]], [[Klein–Gordon equation]], and [[Poisson's equation]].&lt;br /&gt;
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If  is a linear function of  and its derivatives, then the PDE is called linear. Common examples of linear PDEs include the heat equation, the wave equation, Laplace's equation, Helmholtz equation, Klein–Gordon equation, and Poisson's equation.&lt;br /&gt;
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如果 {{mvar|f}} 是函数 {{math|''u''}} 及其导数的线性函数，则偏微分方程称为线性函数。线性偏微分方程的常见例子包括热方程、波动方程、拉普拉斯方程、亥姆霍兹方程方程、克莱因-高登方程和泊松方程。&lt;br /&gt;
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A relatively simple PDE is&lt;br /&gt;
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A relatively simple PDE is&lt;br /&gt;
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一个相对简单的偏微分方程：&lt;br /&gt;
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: &amp;lt;math&amp;gt;\frac{\partial u}{\partial x}(x,y) = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;\frac{\partial u}{\partial x}(x,y) = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
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&lt;br /&gt;
&lt;br /&gt;
This relation [[Logical implication|implies]] that the function {{math|''u''(''x'',''y'')}} is independent of {{mvar|x}}. However, the equation gives no information on the function's dependence on the variable {{mvar|y}}. Hence the general solution of this equation is&lt;br /&gt;
&lt;br /&gt;
This relation implies that the function  is independent of . However, the equation gives no information on the function's dependence on the variable . Hence the general solution of this equation is&lt;br /&gt;
&lt;br /&gt;
这意味着函数 {{math|''u''(''x'',''y'')}} 独立于 {{mvar|x}} 的。然而，这个方程没有给出关于函数和自变量的相关性的信息。因此，这个方程的通解是&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt;u(x,y) = f(y),&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;u(x,y) = f(y),&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
where {{mvar|f}} is an arbitrary function of {{mvar|y}}. The analogous ordinary differential equation is&lt;br /&gt;
&lt;br /&gt;
where  is an arbitrary function of . The analogous ordinary differential equation is&lt;br /&gt;
&lt;br /&gt;
其中， {{mvar|f}} 是 {{mvar|y}} 的任意函数。&lt;br /&gt;
&lt;br /&gt;
类似的常微分方程是：&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt;\frac{\mathrm{d} u}{\mathrm{d} x}(x) = 0,&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;\frac{\mathrm{d} u}{\mathrm{d} x}(x) = 0,&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
which has the solution&lt;br /&gt;
&lt;br /&gt;
which has the solution&lt;br /&gt;
&lt;br /&gt;
它的解为&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt;u(x) = c,&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;u(x) = c,&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
where {{mvar|c}} is any [[Constant (mathematics)|constant]] value. These two examples illustrate that general solutions of ordinary differential equations (ODEs) involve arbitrary constants, but solutions of PDEs involve arbitrary functions.&lt;br /&gt;
&lt;br /&gt;
where  is any constant value. These two examples illustrate that general solutions of ordinary differential equations (ODEs) involve arbitrary constants, but solutions of PDEs involve arbitrary functions.&lt;br /&gt;
&lt;br /&gt;
这里，{{mvar|c}} 是一个任意常量。&lt;br /&gt;
&lt;br /&gt;
这两个例子说明常微分方程的一般解包含任意常数，但偏微分方程的解包含任意函数。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
A solution of a PDE is generally not [[Uniqueness quantification|unique]]; additional conditions must generally be specified on the [[Boundary (topology)|boundary]] of the region where the solution is defined. For instance, in the simple example above, the function {{math|''f''(''y'')}} can be determined if {{mvar|u}} is specified on the line {{math|''x'' {{=}} 0}}.&lt;br /&gt;
&lt;br /&gt;
A solution of a PDE is generally not unique; additional conditions must generally be specified on the boundary of the region where the solution is defined. For instance, in the simple example above, the function  can be determined if  is specified on the line  0}}.&lt;br /&gt;
&lt;br /&gt;
偏微分方程的解一般不是唯一的; 一般必须在定义解的区域边界上定义附加条件。 例如，在上面的简单示例中，如果在 {{math|''x'' {{=}} 0}} 时确定了 {{mvar|u}} 的值，则可以确定该函数 {{math|''f''(''y'')}}。&lt;br /&gt;
&lt;br /&gt;
== Existence and uniqueness ==&lt;br /&gt;
存在性和唯一性&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Although the issue of existence and uniqueness of solutions of ordinary differential equations has a very satisfactory answer with the [[Picard–Lindelöf theorem]], that is far from the case for partial differential equations. The [[Cauchy–Kowalevski theorem]] states that the [[Cauchy problem]] for any partial differential equation whose coefficients are [[Analytic function|analytic]] in the unknown function and its derivatives, has a locally unique analytic solution. Although this result might appear to settle the existence and uniqueness of solutions, there are examples of linear partial differential equations whose coefficients have derivatives of all orders (which are nevertheless not analytic) but which have no solutions at all: see [[Lewy's example|Lewy (1957)]]. Even if the solution of a partial differential equation exists and is unique, it may nevertheless have undesirable properties.  The mathematical study of these questions is usually in the more powerful context of [[weak solution]]s.&lt;br /&gt;
&lt;br /&gt;
Although the issue of existence and uniqueness of solutions of ordinary differential equations has a very satisfactory answer with the Picard–Lindelöf theorem, that is far from the case for partial differential equations. The Cauchy–Kowalevski theorem states that the Cauchy problem for any partial differential equation whose coefficients are analytic in the unknown function and its derivatives, has a locally unique analytic solution. Although this result might appear to settle the existence and uniqueness of solutions, there are examples of linear partial differential equations whose coefficients have derivatives of all orders (which are nevertheless not analytic) but which have no solutions at all: see Lewy (1957). Even if the solution of a partial differential equation exists and is unique, it may nevertheless have undesirable properties.  The mathematical study of these questions is usually in the more powerful context of weak solutions.&lt;br /&gt;
&lt;br /&gt;
尽管常微分方程解的存在性和唯一性用'''&amp;lt;font color=&amp;quot;#ff8000&amp;quot;&amp;gt;弗罗贝尼乌斯定理 Picard–Lindelöf Theorem&amp;lt;/font&amp;gt;得到了令人满意的结果，但偏微分方程解的存在性和唯一性却远没有得到解决。'''&amp;lt;font color=&amp;quot;#ff8000&amp;quot;&amp;gt;柯西-科瓦列夫斯基定理 Cauchy–Kowalevski theorem&amp;lt;/font&amp;gt;指出：对于任意系数在未知函数及其导数中解析的偏微分方程，柯西问题存在一个局部唯一的解析解。虽然这个结果似乎解决了解的存在性和唯一性问题，但是存在一些线性偏微分方程-其系数具有所有级数的导数(尽管这些导数不是解析的) ，但是根本没有解: 见 Lewy (1957)。即使偏微分方程的解存在且唯一，它仍然可能具有不可预料的性质。这些问题的数学研究通常是在更有力的弱解的背景下进行的。&lt;br /&gt;
&lt;br /&gt;
An example of pathological behavior is the sequence (depending upon {{mvar|n}}) of [[Cauchy problem]]s for the [[Laplace equation]]&lt;br /&gt;
&lt;br /&gt;
An example of pathological behavior is the sequence (depending upon ) of Cauchy problems for the Laplace equation&lt;br /&gt;
&lt;br /&gt;
反常特征的一个例子是拉普拉斯方程的柯西问题的序列(取决于{{mvar|n}})&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt;\frac{\partial^2 u}{\partial x^2} + \frac{\partial^2 u}{\partial y^2}=0,&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;\frac{\partial^2 u}{\partial x^2} + \frac{\partial^2 u}{\partial y^2}=0,&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
with [[boundary condition]]s&lt;br /&gt;
&lt;br /&gt;
with boundary conditions&lt;br /&gt;
&lt;br /&gt;
具有边界条件&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt;\begin{align} u(x,0) &amp;amp;= 0, \\ \frac{\partial u}{\partial y}(x,0) &amp;amp;= \frac{\sin nx}{n}, \end{align}&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;\begin{align} u(x,0) &amp;amp;= 0, \\ \frac{\partial u}{\partial y}(x,0) &amp;amp;= \frac{\sin nx}{n}, \end{align}&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
where {{mvar|n}} is an integer. The derivative of {{mvar|u}} with respect to {{mvar|y}} approaches zero [[uniform convergence|uniformly]] in {{mvar|x}} as {{mvar|n}} increases, but the solution is&lt;br /&gt;
&lt;br /&gt;
where  is an integer. The derivative of  with respect to  approaches zero uniformly in  as  increases, but the solution is&lt;br /&gt;
&lt;br /&gt;
其中 {{mvar|n}} 是整数。{{mvar|u}} 关于 {{mvar|y}} 的导数，一致地随着 {{mvar|n}} 的增加而趋于零，但解是&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt;u(x,y) = \frac{\sinh ny \sin nx}{n^2}.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;u(x,y) = \frac{\sinh ny \sin nx}{n^2}.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
This solution approaches infinity if {{mvar|nx}} is not an integer multiple of {{pi}} for any non-zero value of {{mvar|y}}. The Cauchy problem for the Laplace equation is called ''ill-posed'' or ''not [[Well-posed problem|well-posed]]'', since the solution does not continuously depend on the data of the problem. Such ill-posed problems are not usually satisfactory for physical applications.&lt;br /&gt;
&lt;br /&gt;
This solution approaches infinity if  is not an integer multiple of  for any non-zero value of . The Cauchy problem for the Laplace equation is called ill-posed or not well-posed, since the solution does not continuously depend on the data of the problem. Such ill-posed problems are not usually satisfactory for physical applications.&lt;br /&gt;
&lt;br /&gt;
对于任何非零的 {{mvar|y}}，如果 {{mvar|nx}} 不是模板 {{pi}} 的整数倍，这个解会接近于无穷大。拉普拉斯方程的柯西问题被称为不适定的（可以译为ill-posed或not well-posed），因为解不是连续地依赖于问题的数据。这种不适定问题通常不能满足物理应用。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The [[Navier–Stokes existence and smoothness|existence of solutions for the Navier–Stokes equations]], a partial differential equation, is part of one of the [[Millennium Prize Problems]].&lt;br /&gt;
&lt;br /&gt;
The existence of solutions for the Navier–Stokes equations, a partial differential equation, is part of one of the Millennium Prize Problems.&lt;br /&gt;
&lt;br /&gt;
偏微分方程”纳维-斯托克斯方程“的解的存在性就是千禧年大奖难题之一的一部分。&lt;br /&gt;
&lt;br /&gt;
== Notation ==&lt;br /&gt;
符号&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
In PDEs, it is common to denote partial derivatives using subscripts. That is:&lt;br /&gt;
&lt;br /&gt;
In PDEs, it is common to denote partial derivatives using subscripts. That is:&lt;br /&gt;
&lt;br /&gt;
在偏微分方程中，通常用下标表示偏导数。例如:&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt;u_x = \frac{\partial u}{\partial x}&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;u_x = \frac{\partial u}{\partial x}&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt;u_{xx} = \frac{\partial^2 u}{\partial x^2} &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;u_{xx} = \frac{\partial^2 u}{\partial x^2} &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt;u_{xy} = \frac{\partial^2 u}{\partial y\, \partial x} = \frac{\partial}{\partial y } \left(\frac{\partial u}{\partial x}\right). &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;u_{xy} = \frac{\partial^2 u}{\partial y\, \partial x} = \frac{\partial}{\partial y } \left(\frac{\partial u}{\partial x}\right). &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Especially in physics, [[del]] or nabla ({{math|∇}}) is often used to denote spatial derivatives, and {{math|''&amp;amp;#x307;u'', ''ü''}} for time derivatives. For example, the [[wave equation]] (mentioned below) can be written as&lt;br /&gt;
&lt;br /&gt;
Especially in physics, del or nabla () is often used to denote spatial derivatives, and  for time derivatives. For example, the wave equation (mentioned below) can be written as&lt;br /&gt;
&lt;br /&gt;
特别是在物理学中，[[del]] 或 nabla ({{math|∇}}) 经常用来表示空间导数和时间导数。例如，波动方程(在下文中提到)可以写成：&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt;\ddot u=c^2\nabla^2u&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt;\ddot u=c^2\nabla^2u&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
or&lt;br /&gt;
&lt;br /&gt;
or&lt;br /&gt;
&lt;br /&gt;
或&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt;\ddot u=c^2\Delta u&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt;\ddot u=c^2\Delta u&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
where {{math|Δ}} is the [[Laplace operator]].&lt;br /&gt;
&lt;br /&gt;
where  is the Laplace operator.&lt;br /&gt;
&lt;br /&gt;
其中，{{math|Δ}} 代表拉普拉斯算子。&lt;br /&gt;
&lt;br /&gt;
== Classification ==&lt;br /&gt;
分类&lt;br /&gt;
&lt;br /&gt;
Some linear, second-order partial differential equations can be classified as [[parabolic partial differential equation|parabolic]], [[hyperbolic partial differential equation|hyperbolic]] and [[elliptic partial differential equation|elliptic]]. Others, such as the [[Euler–Tricomi equation]], have different types in different regions. The classification provides a guide to appropriate initial and boundary conditions and to the smoothness of the solutions.&lt;br /&gt;
&lt;br /&gt;
Some linear, second-order partial differential equations can be classified as parabolic, hyperbolic and elliptic. Others, such as the Euler–Tricomi equation, have different types in different regions. The classification provides a guide to appropriate initial and boundary conditions and to the smoothness of the solutions.&lt;br /&gt;
&lt;br /&gt;
一些线性二阶偏微分方程可分为抛物型方程、双曲型方程和椭圆型方程。其他的方程，如欧拉-特里科米方程，在不同的区域有不同的类型。这种分类有助于选择适当的初始和边界条件以及提高解的平滑性。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
=== Equations of first order ===&lt;br /&gt;
一阶方程&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{{main|First-order partial differential equation}}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
=== Linear equations of second order ===&lt;br /&gt;
二阶线性方程&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Assuming {{math|''u&amp;lt;sub&amp;gt;xy&amp;lt;/sub&amp;gt;'' {{=}} ''u&amp;lt;sub&amp;gt;yx&amp;lt;/sub&amp;gt;''}}, the general linear second-order PDE in two independent variables has the form&lt;br /&gt;
&lt;br /&gt;
Assuming  u&amp;lt;sub&amp;gt;yx&amp;lt;/sub&amp;gt;}}, the general linear second-order PDE in two independent variables has the form&lt;br /&gt;
&lt;br /&gt;
假设 {{math|''u&amp;lt;sub&amp;gt;xy&amp;lt;/sub&amp;gt;'' {{=}} ''u&amp;lt;sub&amp;gt;yx&amp;lt;/sub&amp;gt;''}}，含有两个独立变量的一般的线性二阶偏微分方程具有如下这样的形式&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt;Au_{xx} + 2Bu_{xy} + Cu_{yy} + \cdots \mbox{(lower order terms)} = 0,&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;Au_{xx} + 2Bu_{xy} + Cu_{yy} + \cdots \mbox{(lower order terms)} = 0,&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
where the coefficients {{mvar|A}}, {{mvar|B}}, {{mvar|C}}... may depend upon {{mvar|x}} and {{mvar|y}}. If {{math|''A''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; + ''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; + ''C''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; &amp;gt; 0}} over a region of the {{mvar|xy}}-plane, the PDE is second-order in that region. This form is analogous to the equation for a conic section:&lt;br /&gt;
&lt;br /&gt;
where the coefficients , , ... may depend upon  and . If  over a region of the -plane, the PDE is second-order in that region. This form is analogous to the equation for a conic section:&lt;br /&gt;
&lt;br /&gt;
其中的系数 {{mvar|A}}, {{mvar|B}}, {{mvar|C}}... 一般取决于{{mvar|x}}和{{mvar|y}}。如果在{{mvar|xy}}-平面的一个区域上 {{math|''A''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; + ''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; + ''C''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; &amp;gt; 0}}，偏微分方程在该区域是二阶的。这种形式类似于圆锥曲线的方程:&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt;Ax^2 + 2Bxy + Cy^2 + \cdots = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;Ax^2 + 2Bxy + Cy^2 + \cdots = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
More precisely, replacing {{math|∂&amp;lt;sub&amp;gt;''x''&amp;lt;/sub&amp;gt;}} by {{mvar|X}}, and likewise for other variables (formally this is done by a [[Fourier transform]]), converts a constant-coefficient PDE into a polynomial of the same degree, with the terms of the highest degree (a [[homogeneous polynomial]], here a [[quadratic form]]) being most significant for the classification.&lt;br /&gt;
&lt;br /&gt;
More precisely, replacing  by , and likewise for other variables (formally this is done by a Fourier transform), converts a constant-coefficient PDE into a polynomial of the same degree, with the terms of the highest degree (a homogeneous polynomial, here a quadratic form) being most significant for the classification.&lt;br /&gt;
&lt;br /&gt;
更准确地说，用 {{mvar|X}} 替换 {{math|∂&amp;lt;sub&amp;gt;''x''&amp;lt;/sub&amp;gt;}}，对于其他变量做同样的操作(从形式上来说，这是由傅里叶变换来完成的)，将一个常系数偏微分方程转换成一个相同次数的多项式，最高次数的项(齐次多项式，这里是一个二次形式)一般会用于偏微分方程的分类。&lt;br /&gt;
===~~ most significant for the classification 意译为用于偏微分方程的分类。       significiant直译过来感觉不太合适&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Just as one classifies [[conic section]]s and quadratic forms into parabolic, hyperbolic, and elliptic based on the [[discriminant]] {{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − 4''AC''}}, the same can be done for a second-order PDE at a given point.  However, the [[discriminant]] in a PDE is given by {{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC''}} due to the convention of the {{mvar|xy}} term being {{math|2''B''}} rather than {{mvar|B}}; formally, the discriminant (of the associated quadratic form) is {{math|(2''B'')&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − 4''AC'' {{=}} 4(''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC'')}}, with the factor of 4 dropped for simplicity.&lt;br /&gt;
&lt;br /&gt;
Just as one classifies conic sections and quadratic forms into parabolic, hyperbolic, and elliptic based on the discriminant , the same can be done for a second-order PDE at a given point.  However, the discriminant in a PDE is given by  due to the convention of the  term being  rather than ; formally, the discriminant (of the associated quadratic form) is  4(B&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − AC)}}, with the factor of 4 dropped for simplicity.&lt;br /&gt;
&lt;br /&gt;
正如人们可以根据判别式 {{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − 4''AC''}} 将圆锥曲线和二次型分为抛物型、双曲型和椭圆型一样，对于给定点的二阶偏微分方程也可以这样做。然而，偏微分方程中的判别式 {{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − 4''AC''}} 是根据交叉项的系数{{math|2''B''}} 而不是 {{mvar|B}} 给出的，形式上，判别式(关联二次型)是 {{math|(2''B'')&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − 4''AC'' {{=}} 4(''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC'')}}，为简单起见，去掉了因子4。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
# {{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC'' &amp;lt; 0}} (''[[elliptic partial differential equation]]''): Solutions of [[elliptic partial differential equation|elliptic PDEs]] are as smooth as the coefficients allow, within the interior of the region where the equation and solutions are defined. For example, solutions of [[Laplace's equation]] are analytic within the domain where they are defined, but solutions may assume boundary values that are not smooth. The motion of a fluid at subsonic speeds can be approximated with elliptic PDEs, and the Euler–Tricomi equation is elliptic where {{math|''x'' &amp;lt; 0}}.&lt;br /&gt;
&lt;br /&gt;
  (elliptic partial differential equation): Solutions of elliptic PDEs are as smooth as the coefficients allow, within the interior of the region where the equation and solutions are defined. For example, solutions of Laplace's equation are analytic within the domain where they are defined, but solutions may assume boundary values that are not smooth. The motion of a fluid at subsonic speeds can be approximated with elliptic PDEs, and the Euler–Tricomi equation is elliptic where .&lt;br /&gt;
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{{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC'' &amp;lt; 0}} (椭圆形微分方程)：在定义方程和解的区域内部，椭圆型偏微分方程的解光滑到系数允许的程度。例如，拉普拉斯方程的解在它们被定义的区域内是解析的，但是解可能假设边界值是不光滑的。亚音速流体的运动可以用椭圆偏微分方程近似，其中欧拉-特里科米方程在 {{math|''x'' &amp;lt; 0}} 时是椭圆型偏微分方程。&lt;br /&gt;
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# {{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC'' {{=}} 0}} (''[[parabolic partial differential equation]]''): Equations that are [[parabolic partial differential equation|parabolic]] at every point can be transformed into a form analogous to the [[heat equation]] by a change of independent variables. Solutions smooth out as the transformed time variable increases. The Euler–Tricomi equation has parabolic type on the line where {{math|''x'' {{=}} 0}}.&lt;br /&gt;
&lt;br /&gt;
  0}} (parabolic partial differential equation): Equations that are parabolic at every point can be transformed into a form analogous to the heat equation by a change of independent variables. Solutions smooth out as the transformed time variable increases. The Euler–Tricomi equation has parabolic type on the line where  0}}.&lt;br /&gt;
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{{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC'' {{=}} 0}}（抛物线形偏微分方程）：在每一点上都是抛物线型的方程可以通过改变自变量从而转化成类似于热方程的形式。随着转换后的时间变量的增加，方程的解变得平滑。欧拉-特里科米方程在 {{math|''x'' {{=}} 0}} 这条特征线上是抛物线形的。&lt;br /&gt;
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# {{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC'' &amp;gt; 0}} (''[[hyperbolic partial differential equation]]''): [[hyperbolic partial differential equation|hyperbolic]] equations retain any discontinuities of functions or derivatives in the initial data. An example is the [[wave equation]]. The motion of a fluid at supersonic speeds can be approximated with hyperbolic PDEs, and the Euler–Tricomi equation is hyperbolic where {{math|''x'' &amp;gt; 0}}.&lt;br /&gt;
&lt;br /&gt;
  (hyperbolic partial differential equation): hyperbolic equations retain any discontinuities of functions or derivatives in the initial data. An example is the wave equation. The motion of a fluid at supersonic speeds can be approximated with hyperbolic PDEs, and the Euler–Tricomi equation is hyperbolic where .&lt;br /&gt;
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{{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC'' &amp;gt; 0}} (双曲形偏微分方程)：双曲形方程在初始数据中保留了函数或导数的任何不连续性，波动方程就是其中的一个例子。超音速流体的运动可以用双曲形偏微分方程近似，其中欧拉-特里科米方程在 {{math|''x'' &amp;gt; 0}} 时是双曲型的。&lt;br /&gt;
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If there are {{mvar|n}} independent variables {{math|''x''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;, ''x''&amp;lt;sub&amp;gt;2 &amp;lt;/sub&amp;gt;,… ''x''&amp;lt;sub&amp;gt;''n''&amp;lt;/sub&amp;gt;}}, a general linear partial differential equation of second order has the form&lt;br /&gt;
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If there are  independent variables , a general linear partial differential equation of second order has the form&lt;br /&gt;
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如果存在 {{mvar|n}} 个自变量 {{math|''x''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;, ''x''&amp;lt;sub&amp;gt;2 &amp;lt;/sub&amp;gt;,… ''x''&amp;lt;sub&amp;gt;''n''&amp;lt;/sub&amp;gt;}}，一般二阶线性偏微分方程的形式是&lt;br /&gt;
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: &amp;lt;math&amp;gt;L u =\sum_{i=1}^n\sum_{j=1}^n a_{i,j} \frac{\partial^2 u}{\partial x_i \partial x_j} \quad \text{ plus lower-order terms} =0.&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;L u =\sum_{i=1}^n\sum_{j=1}^n a_{i,j} \frac{\partial^2 u}{\partial x_i \partial x_j} \quad \text{ plus lower-order terms} =0.&amp;lt;/math&amp;gt;&lt;br /&gt;
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The classification depends upon the signature of the eigenvalues of the coefficient matrix {{math|''a''&amp;lt;sub&amp;gt;''i'',''j''&amp;lt;/sub&amp;gt;}}.&lt;br /&gt;
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The classification depends upon the signature of the eigenvalues of the coefficient matrix .&lt;br /&gt;
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这种分类取决于系数矩阵本征值的符号（正负性）。&lt;br /&gt;
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# Elliptic: the eigenvalues are all positive or all negative.&lt;br /&gt;
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 Elliptic: the eigenvalues are all positive or all negative.&lt;br /&gt;
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椭圆形方程: 本征值全部为正或全部为负。&lt;br /&gt;
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# Parabolic: the eigenvalues are all positive or all negative, save one that is zero.&lt;br /&gt;
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 Parabolic: the eigenvalues are all positive or all negative, save one that is zero.&lt;br /&gt;
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抛物线形方程: 本征值全部为正或全部为负，除了一个为零。&lt;br /&gt;
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# Hyperbolic: there is only one negative eigenvalue and all the rest are positive, or there is only one positive eigenvalue and all the rest are negative.&lt;br /&gt;
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 Hyperbolic: there is only one negative eigenvalue and all the rest are positive, or there is only one positive eigenvalue and all the rest are negative.&lt;br /&gt;
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双曲形方程: 只有一个负特征值，其余的都是正特征值，或者只有一个正特征值，其余的都是负特征值。&lt;br /&gt;
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# Ultrahyperbolic: there is more than one positive eigenvalue and more than one negative eigenvalue, and there are no zero eigenvalues. There is only a limited theory for ultrahyperbolic equations (Courant and Hilbert, 1962).&lt;br /&gt;
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 Ultrahyperbolic: there is more than one positive eigenvalue and more than one negative eigenvalue, and there are no zero eigenvalues. There is only a limited theory for ultrahyperbolic equations (Courant and Hilbert, 1962).&lt;br /&gt;
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超双形方程: 存在多于一个正本征值和多于一个的负本征值，且不存在零本征值。对于超双曲方程，只存在一个有限理论(Courant 和 Hilbert，1962)。&lt;br /&gt;
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==[[用户:Yuling|Yuling]]（[[用户讨论:Yuling|讨论]]） 我对于limited theory这个单词对应的相关理论不太了解。&lt;br /&gt;
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=== Systems of first-order equations and characteristic surfaces ===&lt;br /&gt;
一阶方程组和特征曲面&lt;br /&gt;
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The classification of partial differential equations can be extended to systems of first-order equations, where the unknown {{mvar|u}} is now a [[Euclidean vector|vector]] with {{mvar|m}} components, and the coefficient matrices {{mvar|A&amp;lt;sub&amp;gt;ν&amp;lt;/sub&amp;gt;}} are {{mvar|m}} by {{mvar|m}} matrices for {{math|''ν'' {{=}} 1, 2,… ''n''}}. The partial differential equation takes the form&lt;br /&gt;
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The classification of partial differential equations can be extended to systems of first-order equations, where the unknown  is now a vector with  components, and the coefficient matrices  are  by  matrices for  1, 2,… n}}. The partial differential equation takes the form&lt;br /&gt;
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偏微分方程组的分类可以推广到一阶方程组，其中未知量 {{mvar|u}} 是有 {{mvar|m}} 个分量的向量。对于 {{math|''ν'' {{=}} 1, 2,… ''n''}}，系数矩阵 {{mvar|A&amp;lt;sub&amp;gt;ν&amp;lt;/sub&amp;gt;}} 是 {{mvar|m}} × {{mvar|m}} 的矩阵。偏微分方程形式如下：&lt;br /&gt;
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: &amp;lt;math&amp;gt;Lu = \sum_{\nu=1}^{n} A_\nu \frac{\partial u}{\partial x_\nu} + B=0,&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;Lu = \sum_{\nu=1}^{n} A_\nu \frac{\partial u}{\partial x_\nu} + B=0,&amp;lt;/math&amp;gt;&lt;br /&gt;
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where the coefficient matrices {{mvar|A&amp;lt;sub&amp;gt;ν&amp;lt;/sub&amp;gt;}} and the vector {{mvar|B}} may depend upon {{mvar|x}} and {{mvar|u}}. If a [[hypersurface]] {{mvar|S}} is given in the implicit form&lt;br /&gt;
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where the coefficient matrices  and the vector  may depend upon  and . If a hypersurface  is given in the implicit form&lt;br /&gt;
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其中系数矩阵 {{mvar|A&amp;lt;sub&amp;gt;ν&amp;lt;/sub&amp;gt;}} 和向量 {{mvar|B}} 可能依赖于 {{mvar|x}} 和 {{mvar|u}}。如果超曲面是以隐式形式给出的&lt;br /&gt;
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: &amp;lt;math&amp;gt;\varphi(x_1, x_2, \ldots x_n)=0,&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;\varphi(x_1, x_2, \ldots x_n)=0,&amp;lt;/math&amp;gt;&lt;br /&gt;
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where {{mvar|φ}} has a non-zero gradient, then {{mvar|S}} is a '''characteristic surface''' for the operator {{mvar|L}} at a given point if the characteristic form vanishes:&lt;br /&gt;
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where  has a non-zero gradient, then  is a characteristic surface for the operator  at a given point if the characteristic form vanishes:&lt;br /&gt;
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其中存在一个非零的梯度，那么如果特征形式消失，则在给定点上算子的特征曲面形式如下:&lt;br /&gt;
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: &amp;lt;math&amp;gt;Q\left(\frac{\partial\varphi}{\partial x_1}, \ldots\frac{\partial\varphi}{\partial x_n}\right) =\det\left[\sum_{\nu=1}^nA_\nu \frac{\partial \varphi}{\partial x_\nu}\right]=0.\,&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;Q\left(\frac{\partial\varphi}{\partial x_1}, \ldots\frac{\partial\varphi}{\partial x_n}\right) =\det\left[\sum_{\nu=1}^nA_\nu \frac{\partial \varphi}{\partial x_\nu}\right]=0.\,&amp;lt;/math&amp;gt;&lt;br /&gt;
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The geometric interpretation of this condition is as follows: if data for {{mvar|u}} are prescribed on the surface {{mvar|S}}, then it may be possible to determine the normal derivative of {{mvar|u}} on {{mvar|S}} from the differential equation. If the data on {{mvar|S}} and the differential equation determine the normal derivative of {{mvar|u}} on {{mvar|S}}, then {{mvar|S}} is non-characteristic. If the data on {{mvar|S}} and the differential equation ''do not'' determine the normal derivative of {{mvar|u}} on {{mvar|S}}, then the surface is '''characteristic''', and the differential equation restricts the data on {{mvar|S}}: the differential equation is ''internal'' to {{mvar|S}}.&lt;br /&gt;
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The geometric interpretation of this condition is as follows: if data for  are prescribed on the surface , then it may be possible to determine the normal derivative of  on  from the differential equation. If the data on  and the differential equation determine the normal derivative of  on , then  is non-characteristic. If the data on  and the differential equation do not determine the normal derivative of  on , then the surface is characteristic, and the differential equation restricts the data on : the differential equation is internal to .&lt;br /&gt;
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这个条件的几何解释如下: 如果关于 {{mvar|u}} 的数据是在曲面 {{mvar|S}} 上规定的，那么就有可能依据微分方程确定曲面 {{mvar|S}} 上 {{mvar|u}} 的法向导数。如果曲面 {{mvar|S}} 上的数据和上面的微分方程能确定曲面 {{mvar|S}} 上 {{mvar|u}} 的法向导数，那么它就是非特征的。如果曲面 {{mvar|S}} 上的数据和上面的微分方程不能确定曲面 {{mvar|S}} 上 {{mvar|u}} 的法向导数，那么曲面是特征的，并且微分方程将数据限制在曲面 {{mvar|S}} 上：微分方程是在曲面 {{mvar|S}} 内部。&lt;br /&gt;
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# A first-order system {{math|''Lu'' {{=}} 0}} is ''elliptic'' if no surface is characteristic for {{mvar|L}}: the values of {{mvar|u}} on {{mvar|S}} and the differential equation always determine the normal derivative of {{mvar|u}} on {{mvar|S}}.&lt;br /&gt;
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 A first-order system  0}} is elliptic if no surface is characteristic for : the values of  on  and the differential equation always determine the normal derivative of  on .&lt;br /&gt;
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如果对于 {{mvar|L}} 没有曲面是特征的，则一阶系统 {{math|''Lu'' {{=}} 0}} 是椭圆形的：{{mvar|u}}在 {{mvar|S}} 的值和微分方程总能够决定 {{mvar|S}} 上 {{mvar|u}} 的法向导数。&lt;br /&gt;
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# A first-order system is ''hyperbolic'' at a point if there is a '''spacelike''' surface {{mvar|S}} with normal {{mvar|ξ}} at that point. This means that, given any non-trivial vector {{mvar|η}} orthogonal to {{mvar|ξ}}, and a scalar multiplier {{mvar|λ}}, the equation {{math|''Q''(''λξ'' + ''η'') {{=}} 0}} has {{mvar|m}} real roots {{math|''λ''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;, ''λ''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;,… ''λ''&amp;lt;sub&amp;gt;''m''&amp;lt;/sub&amp;gt;}}. The system is '''strictly hyperbolic''' if these roots are always distinct. The geometrical interpretation of this condition is as follows: the characteristic form {{math|''Q''(''ζ'') {{=}} 0}} defines a cone (the normal cone) with homogeneous coordinates ζ. In the hyperbolic case, this cone has {{mvar|m}} sheets, and the axis {{math|''ζ'' {{=}} ''λξ''}} runs inside these sheets: it does not intersect any of them. But when displaced from the origin by η, this axis intersects every sheet. In the elliptic case, the normal cone has no real sheets.&lt;br /&gt;
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 A first-order system is hyperbolic at a point if there is a spacelike surface  with normal  at that point. This means that, given any non-trivial vector  orthogonal to , and a scalar multiplier , the equation  0}} has  real roots . The system is strictly hyperbolic if these roots are always distinct. The geometrical interpretation of this condition is as follows: the characteristic form  0}} defines a cone (the normal cone) with homogeneous coordinates ζ. In the hyperbolic case, this cone has  sheets, and the axis  λξ}} runs inside these sheets: it does not intersect any of them. But when displaced from the origin by η, this axis intersects every sheet. In the elliptic case, the normal cone has no real sheets.&lt;br /&gt;
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如果在该点存在一个法向量为 {{mvar|ξ}}的 '''&amp;lt;font color=&amp;quot;#ff8000&amp;quot;&amp;gt;类空曲面 Spacclike Surface&amp;lt;/font&amp;gt; {{mvar|S}} ，则一阶系统在那一点是双曲的。这意味着，给定任意正交于 {{mvar|ξ}} 的非平凡向量 {{mvar|η}} 和一个标量乘子 {{mvar|λ}}，方程 {{math|''Q''(''λξ'' + ''η'') {{=}} 0}} 有 {{mvar|m}} 个实根 {{math|''λ''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;, ''λ''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;,… ''λ''&amp;lt;sub&amp;gt;''m''&amp;lt;/sub&amp;gt;}}。如果这些根始终不同，则该系统是严格双曲形的。这个条件的几何解释如下: 特征形式 {{math|''Q''(''ζ'') {{=}} 0}} 定义了一个具有齐次坐标 ζ的圆锥(法线圆锥)。在双曲形的情况下，这个圆锥体有 {{mvar|m}} 层，并且轴 {{math|''ζ'' {{=}} ''λξ''}} 在这些层中运动: 它不与任何一层相交。但是当从原点偏离η时，这条轴线与每一层都相交。在椭圆形的情况下，法向圆锥没有实层。&lt;br /&gt;
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==[[用户:Yuling|Yuling]]（[[用户讨论:Yuling|讨论]]） sheet 这个单词也不很理解，我直译为了“层”&lt;br /&gt;
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=== Equations of mixed type ===&lt;br /&gt;
混合型方程&lt;br /&gt;
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If a PDE has coefficients that are not constant, it is possible that it will not belong to any of these categories but rather be of '''mixed type'''. A simple but important example is the [[Euler–Tricomi equation]]&lt;br /&gt;
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If a PDE has coefficients that are not constant, it is possible that it will not belong to any of these categories but rather be of mixed type. A simple but important example is the Euler–Tricomi equation&lt;br /&gt;
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如果偏微分方程的系数不是常数，那么它可能不属于这些类别中的任何一个，而是属于混合类型。一个简单但重要的例子是欧拉-特里科米方程&lt;br /&gt;
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: &amp;lt;math&amp;gt;u_{xx} = xu_{yy},&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;u_{xx} = xu_{yy},&amp;lt;/math&amp;gt;&lt;br /&gt;
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which is called '''elliptic-hyperbolic''' because it is elliptic in the region {{math|''x'' &amp;lt; 0}}, hyperbolic in the region {{math|''x'' &amp;gt; 0}}, and degenerate parabolic on the line {{math|''x'' {{=}} 0}}.&lt;br /&gt;
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which is called elliptic-hyperbolic because it is elliptic in the region , hyperbolic in the region , and degenerate parabolic on the line  0}}.&lt;br /&gt;
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它在 {{math|''x'' &amp;lt; 0}} 的区域上是椭圆形，在 {{math|''x'' &amp;gt; 0}} 区域上是双曲形，在 {{math|''x'' {{=}} 0}}这条线上是退化为抛物线形，因此称之为椭圆-双曲型。&lt;br /&gt;
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''fill in: Dirichlet and Neumann boundaries, hyperbolic/parabolic/elliptic separation of variables, [[Fourier analysis]], [[Green's function]]s ...--&amp;gt;&lt;br /&gt;
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fill in: Dirichlet and Neumann boundaries, hyperbolic/parabolic/elliptic separation of variables, Fourier analysis, Green's functions ...--&amp;gt;&lt;br /&gt;
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填写: Dirichlet 和 Neumann 边界，双曲 / 抛物线 / 椭圆分离变量法，傅立叶分析，Green 函数... --&lt;br /&gt;
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=== Infinite-order PDEs in quantum mechanics ===&lt;br /&gt;
量子力学中的无限阶偏微分方程&lt;br /&gt;
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In the [[phase space formulation]] of quantum mechanics,  one may consider the [[Method of quantum characteristics|quantum Hamilton's equations]] for trajectories of quantum particles. These equations are infinite-order PDEs. However, in the semiclassical expansion, one has a finite system of ODEs at any fixed order of [[Dirac constant|{{mvar|ħ}}]].  The evolution equation of the [[Wigner quasi-probability distribution|c]] is also an infinite-order PDE. The quantum trajectories are [[Method of quantum characteristics|quantum characteristics]], with the use of which one could calculate the evolution of the Wigner function.&lt;br /&gt;
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In the phase space formulation of quantum mechanics,  one may consider the quantum Hamilton's equations for trajectories of quantum particles. These equations are infinite-order PDEs. However, in the semiclassical expansion, one has a finite system of ODEs at any fixed order of Dirac constant|.  The evolution equation of the Wigner function is also an infinite-order PDE. The quantum trajectories are quantum characteristics, with the use of which one could calculate the evolution of the Wigner function.&lt;br /&gt;
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在量子力学中的相空间表述中，我们可以考虑用于求解量子粒子的轨迹的量子哈密顿的方程。这些方程是无限阶偏微分方程。然而，在半经典展开中，我们在给定[[Dirac constant|{{mvar|ħ}}]]阶数下有一个有限的的常微分方程组。'''&amp;lt;font color=&amp;quot;#ff8000&amp;quot;&amp;gt;维格纳函数  Wigner Function&amp;lt;/font&amp;gt;的演化方程也是一个无限阶偏微分方程。由于量子轨道的量子特性，所以它通常可以用来计算维格纳函数的演化。&lt;br /&gt;
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== Analytical solutions ==&lt;br /&gt;
解析解&lt;br /&gt;
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===Separation of variables===&lt;br /&gt;
分离变量法&lt;br /&gt;
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{{main|Separable partial differential equation}}&lt;br /&gt;
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Linear PDEs can be reduced to systems of ordinary differential equations by the important technique of separation of variables. This technique rests on a characteristic of solutions to differential equations: if one can find any solution that solves the equation and satisfies the boundary conditions, then it is ''the'' solution (this also applies to ODEs). We assume as an [[ansatz]] that the dependence of a solution on the parameters space and time can be written as a product of terms that each depend on a single parameter, and then see if this can be made to solve the problem.&amp;lt;ref&amp;gt;{{cite book|last1=Gershenfeld|first1=Neil|title=The nature of mathematical modeling|date=2000|publisher=Cambridge Univ. Press|location=Cambridge|isbn=0521570956|page=27|edition=Reprinted (with corr.)}}&amp;lt;/ref&amp;gt;&lt;br /&gt;
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Linear PDEs can be reduced to systems of ordinary differential equations by the important technique of separation of variables. This technique rests on a characteristic of solutions to differential equations: if one can find any solution that solves the equation and satisfies the boundary conditions, then it is the solution (this also applies to ODEs). We assume as an ansatz that the dependence of a solution on the parameters space and time can be written as a product of terms that each depend on a single parameter, and then see if this can be made to solve the problem.&lt;br /&gt;
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线性偏微分方程组可以通过分离变量法这一重要方法来简化为常微分方程组。这种方法依赖于微分方程解的一个特征: 如果能找到任何一个满足方程和边界条件的解，那么这个解就是方程的解(这也适用于常微分方程)。我们假设解对参数空间和时间的依赖可以写成对它们每一项的依赖以及一个参数的乘积，然后再看看这是否可以用来解决这个问题。&lt;br /&gt;
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In the method of separation of variables, one reduces a PDE to a PDE in fewer variables, which is an ordinary differential equation if in one variable – these are in turn easier to solve.&lt;br /&gt;
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In the method of separation of variables, one reduces a PDE to a PDE in fewer variables, which is an ordinary differential equation if in one variable – these are in turn easier to solve.&lt;br /&gt;
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在分离变量法方法中，可以将偏微分方程简化为含有更少变量的偏微分方程，如果只有一个变量，那么就变成了一个'''&amp;lt;font color = &amp;quot;#ff8000&amp;quot;&amp;gt;常微分方程 Ordinary Differential Equation&amp;lt;/font&amp;gt;'''-- 反过来，这些方程也更容易求解。&lt;br /&gt;
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This is possible for simple PDEs, which are called [[separable partial differential equation]]s, and the domain is generally a rectangle (a product of intervals). Separable PDEs correspond to [[diagonal matrices]] – thinking of &amp;quot;the value for fixed {{mvar|x}}&amp;quot; as a coordinate, each coordinate can be understood separately.&lt;br /&gt;
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This is possible for simple PDEs, which are called separable partial differential equations, and the domain is generally a rectangle (a product of intervals). Separable PDEs correspond to diagonal matrices – thinking of &amp;quot;the value for fixed &amp;quot; as a coordinate, each coordinate can be understood separately.&lt;br /&gt;
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对于简单的偏微分方程(称为可分离偏微分方程)来说，这是可能的，而且方程通常定义在一个矩形区域(区间的乘积)上。可分离偏微分方程对应于对角线矩阵——以“固定值”为坐标，每个坐标可分开理解。&lt;br /&gt;
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This generalizes to the [[method of characteristics]], and is also used in [[integral transform]]s.&lt;br /&gt;
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This generalizes to the method of characteristics, and is also used in integral transforms.&lt;br /&gt;
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这种方法可以推广到特征曲线法，也可以用于积分变换。&lt;br /&gt;
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===Method of characteristics===&lt;br /&gt;
特征曲线法&lt;br /&gt;
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{{main|Method of characteristics}}&lt;br /&gt;
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In special cases, one can find characteristic curves on which the equation reduces to an ODE – changing coordinates in the domain to straighten these curves allows separation of variables, and is called the [[method of characteristics]].&lt;br /&gt;
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In special cases, one can find characteristic curves on which the equation reduces to an ODE – changing coordinates in the domain to straighten these curves allows separation of variables, and is called the method of characteristics.&lt;br /&gt;
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在特殊情况下，可以找到一些特征曲线，在这些曲线上方程可以变成一个常微分方程——意味着改变坐标从而使这些曲线变直从而达到分离变量的目的，这就是所谓的特征曲线法。&lt;br /&gt;
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More generally, one may find characteristic surfaces.&lt;br /&gt;
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More generally, one may find characteristic surfaces.&lt;br /&gt;
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更一般地说，人们可能会找到特征表面。&lt;br /&gt;
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===Integral transform===&lt;br /&gt;
积分变换&lt;br /&gt;
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An [[integral transform]] may transform the PDE to a simpler one, in particular, a separable PDE. This corresponds to diagonalizing an operator.&lt;br /&gt;
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An integral transform may transform the PDE to a simpler one, in particular, a separable PDE. This corresponds to diagonalizing an operator.&lt;br /&gt;
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积分变换可以将偏微分方程转换为更简单的偏微分方程，特别是可分离的偏微分方程。这对应于对角化算符。&lt;br /&gt;
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An important example of this is [[Fourier analysis]], which diagonalizes the heat equation using the [[eigenbasis]] of sinusoidal waves.&lt;br /&gt;
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An important example of this is Fourier analysis, which diagonalizes the heat equation using the eigenbasis of sinusoidal waves.&lt;br /&gt;
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这方面的一个重要例子是'''&amp;lt;font color = &amp;quot;#ff8000&amp;quot;&amp;gt;傅里叶分析  Fourier Analysis&amp;lt;/font&amp;gt;'''，它使用正弦波的特征基来对角化热方程。&lt;br /&gt;
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If the domain is finite or periodic, an infinite sum of solutions such as a [[Fourier series]] is appropriate, but an integral of solutions such as a [[Fourier integral]] is generally required for infinite domains. The solution for a point source for the heat equation given above is an example of the use of a Fourier integral.&lt;br /&gt;
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If the domain is finite or periodic, an infinite sum of solutions such as a Fourier series is appropriate, but an integral of solutions such as a Fourier integral is generally required for infinite domains. The solution for a point source for the heat equation given above is an example of the use of a Fourier integral.&lt;br /&gt;
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如果区域是有限的或周期性的，那么解为无限和的形式是恰当的，例如傅里叶级数，但是一个解的积分，例如傅立叶积分，一般是在无限区域上的。上面给出的热传导方程的点源解法就是使用傅里叶积分的一个例子。&lt;br /&gt;
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===Change of variables===&lt;br /&gt;
变量代换&lt;br /&gt;
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Often a PDE can be reduced to a simpler form with a known solution by a suitable [[Change of variables (PDE)|change of variables]].  For example, the [[Black–Scholes equation#Derivation|Black–Scholes]] PDE&lt;br /&gt;
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Often a PDE can be reduced to a simpler form with a known solution by a suitable change of variables.  For example, the Black–Scholes PDE&lt;br /&gt;
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偏微分方程通常可以通过变量的适当变化，用已知的解简化为更简单的形式。例如，布莱克-舒尔斯偏微分方程&lt;br /&gt;
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:&amp;lt;math&amp;gt; \frac{\partial V}{\partial t} + \tfrac{1}{2}\sigma^2 S^2\frac{\partial^2 V}{\partial S^2} + rS\frac{\partial V}{\partial S} - rV = 0 &amp;lt;/math&amp;gt;&lt;br /&gt;
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&amp;lt;math&amp;gt; \frac{\partial V}{\partial t} + \tfrac{1}{2}\sigma^2 S^2\frac{\partial^2 V}{\partial S^2} + rS\frac{\partial V}{\partial S} - rV = 0 &amp;lt;/math&amp;gt;&lt;br /&gt;
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is reducible to the [[heat equation]]&lt;br /&gt;
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is reducible to the heat equation&lt;br /&gt;
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可以简化为热传导方程&lt;br /&gt;
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:&amp;lt;math&amp;gt; \frac{\partial u}{\partial \tau} = \frac{\partial^2 u}{\partial x^2}&amp;lt;/math&amp;gt;&lt;br /&gt;
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&amp;lt;math&amp;gt; \frac{\partial u}{\partial \tau} = \frac{\partial^2 u}{\partial x^2}&amp;lt;/math&amp;gt;&lt;br /&gt;
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by the change of variables (for complete details see {{webarchive |url=https://web.archive.org/web/20080411030405/http://www.math.unl.edu/~sdunbar1/Teaching/MathematicalFinance/Lessons/BlackScholes/Solution/solution.shtml |date=April 11, 2008 |title=Solution of the Black Scholes Equation }})&lt;br /&gt;
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by the change of variables (for complete details see )&lt;br /&gt;
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通过变量替换(完整的细节见)&lt;br /&gt;
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:&amp;lt;math&amp;gt;\begin{align}&lt;br /&gt;
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V(S,t) &amp;amp;= K v(x,\tau),\\[5px]&lt;br /&gt;
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x &amp;amp;= \ln\left(\tfrac{S}{K} \right),\\[5px]&lt;br /&gt;
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\tau &amp;amp;= \tfrac{1}{2} \sigma^2 (T - t),\\[5px]&lt;br /&gt;
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v(x,\tau)&amp;amp;=e^{-\alpha x-\beta\tau} u(x,\tau).&lt;br /&gt;
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\end{align}&amp;lt;/math&amp;gt;&lt;br /&gt;
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===Fundamental solution===&lt;br /&gt;
基本解&lt;br /&gt;
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{{main|Fundamental solution}}&lt;br /&gt;
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Inhomogeneous equations can often be solved (for constant coefficient PDEs, always be solved) by finding the [[fundamental solution]] (the solution for a point source), then taking the [[convolution]] with the boundary conditions to get the solution.&lt;br /&gt;
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Inhomogeneous equations can often be solved (for constant coefficient PDEs, always be solved) by finding the fundamental solution (the solution for a point source), then taking the convolution with the boundary conditions to get the solution.&lt;br /&gt;
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非齐次方程(常系数偏微分方程)一般是通过先求出基本解(点源的解) ，然后利用带边界条件的卷积来求解。&lt;br /&gt;
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This is analogous in [[signal processing]] to understanding a filter by its [[impulse response]].&lt;br /&gt;
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This is analogous in signal processing to understanding a filter by its impulse response.&lt;br /&gt;
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这类似于在信号处理中通过滤波器的脉冲响应来理解滤波器。&lt;br /&gt;
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===Superposition principle===&lt;br /&gt;
叠加原理&lt;br /&gt;
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{{further| Superposition principle }}&lt;br /&gt;
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The superposition principle applies to any linear system, including linear systems of PDEs. A common visualization of this concept is the interaction of two waves in phase being combined to result in a greater amplitude, for example {{math|sin ''x'' + sin ''x'' {{=}} 2 sin ''x''}}. The same principle can be observed in PDEs where the solutions may be real or complex and additive. [[Superposition principle|superposition]]&lt;br /&gt;
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The superposition principle applies to any linear system, including linear systems of PDEs. A common visualization of this concept is the interaction of two waves in phase being combined to result in a greater amplitude, for example  2 sin x}}. The same principle can be observed in PDEs where the solutions may be real or complex and additive. superposition&lt;br /&gt;
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'''&amp;lt;font color = &amp;quot;#ff8000&amp;quot;&amp;gt;叠加原理 Superposition Principle&amp;lt;/font&amp;gt;适用于任何线性系统，包括偏微分方程的线性系统。这个概念的一个常见的可视化是两个同相位的波相互作用结合在一起会产生更大的振幅，例如 {{math|sin ''x'' + sin ''x'' {{=}} 2 sin ''x''}}。在偏微分方程中也可以观察到同样的原理，其中的解可能是真实的或复杂的和可加的。叠加&lt;br /&gt;
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If {{math|''u''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;}} and {{math|''u''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;}} are solutions of linear PDE in some function space {{mvar|R}}, then {{math|''u'' {{=}} ''c''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;''u''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; + ''c''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;''u''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;}} with any constants {{math|''c''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;}} and {{math|''c''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;}} are also a solution of that PDE in the same function space.&lt;br /&gt;
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If  and  are solutions of linear PDE in some function space , then  c&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;u&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; + c&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;u&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;}} with any constants  and  are also a solution of that PDE in the same function space.&lt;br /&gt;
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若线性偏微分方程在某个函数空间{{mvar|R}}中有解{{math|''u''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;}} 和 {{math|''u''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;}}，则{{math|''u'' {{=}} ''c''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;''u''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; + ''c''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;''u''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;}}也是该偏微分方程在同一函数空间中的解，其中{{math|''c''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;}} 和 {{math|''c''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;}} 是任意常数。&lt;br /&gt;
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===Methods for non-linear equations===&lt;br /&gt;
非线性方程的求解方法&lt;br /&gt;
{{see also|nonlinear partial differential equation}}&lt;br /&gt;
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There are no generally applicable methods to solve nonlinear PDEs. Still, existence and uniqueness results (such as the [[Cauchy–Kowalevski theorem]]) are often possible, as are proofs of important qualitative and quantitative properties of solutions (getting these results is a major part of [[mathematical analysis|analysis]]). Computational solution to the nonlinear PDEs, the [[split-step method]], exist for specific equations like [[nonlinear Schrödinger equation]].&lt;br /&gt;
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There are no generally applicable methods to solve nonlinear PDEs. Still, existence and uniqueness results (such as the Cauchy–Kowalevski theorem) are often possible, as are proofs of important qualitative and quantitative properties of solutions (getting these results is a major part of analysis). Computational solution to the nonlinear PDEs, the split-step method, exist for specific equations like nonlinear Schrödinger equation.&lt;br /&gt;
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对于非线性偏微分方程，目前还没有普遍适用的求解方法。然而，通常是可能知道解的存在性和唯一性(如柯西-科瓦列夫斯基定理)，也是可能得到解的重要定性和定量性质的证明(得到这些结果是分析的主要部分)。非线性偏微分方程的计算解，即分步法，对一些特定的方程适用，比如非线性'''&amp;lt;font color=&amp;quot;#ff8000&amp;quot;&amp;gt;薛定谔方程 Schrödinger equation&amp;lt;/font&amp;gt;'''。&lt;br /&gt;
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Nevertheless, some techniques can be used for several types of equations. The [[h-principle|{{mvar|h}}-principle]] is the most powerful method to solve [[Underdetermined system|underdetermined]] equations. The [[Riquier–Janet theory]] is an effective method for obtaining information about many analytic [[Overdetermined system|overdetermined]] systems.&lt;br /&gt;
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Nevertheless, some techniques can be used for several types of equations. The -principle is the most powerful method to solve underdetermined equations. The Riquier–Janet theory is an effective method for obtaining information about many analytic overdetermined systems.&lt;br /&gt;
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然而，一些技巧可以用于几种类型的方程。h-原理是求解欠定方程最有效的方法。里基尔-珍妮特理论是一种可以获得许多解析超定系统信息的有效方法。&lt;br /&gt;
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The [[method of characteristics]] can be used in some very special cases to solve partial differential equations.&lt;br /&gt;
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The method of characteristics can be used in some very special cases to solve partial differential equations.&lt;br /&gt;
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特征线法可用于求解某些特殊情况下的偏微分方程。&lt;br /&gt;
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In some cases, a PDE can be solved via [[perturbation analysis]] in which the solution is considered to be a correction to an equation with a known solution. Alternatives are [[numerical analysis]] techniques from simple [[finite difference]] schemes to the more mature [[multigrid]] and [[finite element method]]s. Many interesting problems in science and engineering are solved in this way using [[computer]]s, sometimes high performance [[supercomputer]]s.&lt;br /&gt;
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In some cases, a PDE can be solved via perturbation analysis in which the solution is considered to be a correction to an equation with a known solution. Alternatives are numerical analysis techniques from simple finite difference schemes to the more mature multigrid and finite element methods. Many interesting problems in science and engineering are solved in this way using computers, sometimes high performance supercomputers.&lt;br /&gt;
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在某些情况下，偏微分方程可以通过扰动分析来求解。在扰动分析中，通常是求解将具有已知解的方程修正后的新得到方程。可供选择的数值分析技术从简单的差分格式到更成熟的多重网格和有限元方法。许多有趣的科学和工程问题都是在计算机上用这种方法解决的，有时是高性能超级计算机。&lt;br /&gt;
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===Lie group method===&lt;br /&gt;
李群方法&lt;br /&gt;
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From 1870 [[Sophus Lie]]'s work put the theory of differential equations on a more satisfactory foundation. He showed that the integration theories of the older mathematicians can, by the introduction of what are now called [[Lie group]]s, be referred, to a common source; and that ordinary differential equations which admit the same [[infinitesimal transformation]]s present comparable difficulties of integration. He also emphasized the subject of [[contact transformation|transformations of contact]].&lt;br /&gt;
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From 1870 Sophus Lie's work put the theory of differential equations on a more satisfactory foundation. He showed that the integration theories of the older mathematicians can, by the introduction of what are now called Lie groups, be referred, to a common source; and that ordinary differential equations which admit the same infinitesimal transformations present comparable difficulties of integration. He also emphasized the subject of transformations of contact.&lt;br /&gt;
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从1870年起，索弗斯·李的工作为微分方程理论奠定了一个较为令人满意的基础。他指出，通过引入现在所谓的李群，老一辈数学家的积分理论可以引用到一个共同的来源; 承认相同的无穷小变换的常微分方程在积分方面存在相当的困难。他还强调了接触的转变这一主题。&lt;br /&gt;
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==[[用户:Yuling|Yuling]]（[[用户讨论:Yuling|讨论]]）这句话“He also emphasized the subject of transformations of contact.”中的transformations of contact翻译的不太好。&lt;br /&gt;
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A general approach to solving PDEs uses the symmetry property of differential equations, the continuous [[infinitesimal transformation]]s of solutions to solutions ([[Lie theory]]). Continuous [[group theory]], [[Lie algebras]] and [[differential geometry]] are used to understand the structure of linear and nonlinear partial differential equations for generating integrable equations, to find its [[Lax pair]]s, recursion operators, [[Bäcklund transform]] and finally finding exact analytic solutions to the PDE.&lt;br /&gt;
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A general approach to solving PDEs uses the symmetry property of differential equations, the continuous infinitesimal transformations of solutions to solutions (Lie theory). Continuous group theory, Lie algebras and differential geometry are used to understand the structure of linear and nonlinear partial differential equations for generating integrable equations, to find its Lax pairs, recursion operators, Bäcklund transform and finally finding exact analytic solutions to the PDE.&lt;br /&gt;
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求解偏微分方程的一般方法是利用微分方程的对称性，即解到解的连续无穷小变换(李理论)。连续群论、李代数和微分几何理论被用来理解生成可积方程的线性和非线性偏微分方程的结构，找到它的Lax对、递归算子、 贝克伦德变换，最后找到偏微分方程的精确解析解。&lt;br /&gt;
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Symmetry methods have been recognized to study differential equations arising in mathematics, physics, engineering, and many other disciplines.&lt;br /&gt;
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Symmetry methods have been recognized to study differential equations arising in mathematics, physics, engineering, and many other disciplines.&lt;br /&gt;
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对称方法已被公认可以用于研究出现在数学，物理，工程和许多其他学科的微分方程。&lt;br /&gt;
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===Semianalytical methods===&lt;br /&gt;
半解析方法&lt;br /&gt;
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The [[Adomian decomposition method]], the [[Aleksandr Lyapunov|Lyapunov]] artificial small parameter method, and He's [[homotopy perturbation method]] are all special cases of the more general [[homotopy analysis method]]. These are series expansion methods, and except for the Lyapunov method, are independent of small physical parameters as compared to the well known [[perturbation theory]], thus giving these methods greater flexibility and solution generality.&lt;br /&gt;
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The Adomian decomposition method, the Lyapunov artificial small parameter method, and He's homotopy perturbation method are all special cases of the more general homotopy analysis method. These are series expansion methods, and except for the Lyapunov method, are independent of small physical parameters as compared to the well known perturbation theory, thus giving these methods greater flexibility and solution generality.&lt;br /&gt;
&lt;br /&gt;
阿多米安分解法、李雅普诺夫人工小参数方法和何同伦摄动方法都是更一般的同伦分析方法的特殊情况。除了李雅普诺夫方法之外，这些都是级数展开方法，与为人熟知的摄动理论方法相比，它们与小的物理参数无关，因此这些方法具有更大的灵活性和解的通用性。&lt;br /&gt;
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== Numerical solutions ==&lt;br /&gt;
数值解&lt;br /&gt;
&lt;br /&gt;
The three most widely used [[Numerical partial differential equations|numerical methods to solve PDEs]] are the [[finite element analysis|finite element method]] (FEM), [[finite volume method]]s (FVM) and [[finite difference method]]s (FDM), as well other kind of methods called [[Meshfree methods]], which were made to solve problems where the before mentioned methods are limited. The FEM has a prominent position among these methods and especially its exceptionally efficient higher-order version [[hp-FEM]]. Other hybrid versions of FEM and Meshfree methods include the generalized finite element method (GFEM), [[extended finite element method]] (XFEM), [[Spectral element method|spectral finite element method]] (SFEM), [[Meshfree methods|meshfree finite element method]], [[Discontinuous Galerkin Method|discontinuous Galerkin finite element method]] (DGFEM), [[Element-Free Galerkin Method]] (EFGM), [[Interpolating Element-Free Galerkin Method]] (IEFGM), etc.&lt;br /&gt;
&lt;br /&gt;
The three most widely used numerical methods to solve PDEs are the finite element method (FEM), finite volume methods (FVM) and finite difference methods (FDM), as well other kind of methods called Meshfree methods, which were made to solve problems where the before mentioned methods are limited. The FEM has a prominent position among these methods and especially its exceptionally efficient higher-order version hp-FEM. Other hybrid versions of FEM and Meshfree methods include the generalized finite element method (GFEM), extended finite element method (XFEM), spectral finite element method (SFEM), meshfree finite element method, discontinuous Galerkin finite element method (DGFEM), Element-Free Galerkin Method (EFGM), Interpolating Element-Free Galerkin Method (IEFGM), etc.&lt;br /&gt;
&lt;br /&gt;
求解偏微分方程最常用的三种数值方法是有限元分析法、有限体积法和有限差分法，以及其他一些称为无网格法的方法。这些方法用于解决前面提到的方法受到的限制。在这些方法中，有限元方法，尤其是高效的高阶有限元方法，占有重要地位。其他有限元法和无网格法的混合形式包括广义有限元分析法(GFEM)、扩展有限元分析法(XFEM)、谱有限元分析法(SFEM)、无网格有限元分析法(DGFEM)、间断伽辽金有限元分析法(DGFEM)、无网格伽辽金法(EFGM)、插值无网格伽辽金法(IEFGM)等。&lt;br /&gt;
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=== Finite element method ===&lt;br /&gt;
有限元分析法&lt;br /&gt;
&lt;br /&gt;
{{main|Finite element method}}&lt;br /&gt;
&lt;br /&gt;
The finite element method (FEM) (its practical application often known as finite element analysis (FEA)) is a numerical technique for finding approximate solutions of partial differential equations (PDE) as well as of integral equations. The solution approach is based either on eliminating the differential equation completely (steady state problems), or rendering the PDE into an approximating system of ordinary differential equations, which are then numerically integrated using standard techniques such as Euler's method, Runge–Kutta, etc.&lt;br /&gt;
&lt;br /&gt;
The finite element method (FEM) (its practical application often known as finite element analysis (FEA)) is a numerical technique for finding approximate solutions of partial differential equations (PDE) as well as of integral equations. The solution approach is based either on eliminating the differential equation completely (steady state problems), or rendering the PDE into an approximating system of ordinary differential equations, which are then numerically integrated using standard techniques such as Euler's method, Runge–Kutta, etc.&lt;br /&gt;
&lt;br /&gt;
'''&amp;lt;font color = &amp;quot;#ff8000&amp;quot;&amp;gt;有限元分析法 Finite Element Method&amp;lt;/font&amp;gt;''' ((其实际应用通常被称为有限元分析(FEA))是一种寻找偏微分方程(PDE)和积分方程近似解的数值技术。这种求解方法要么基于完全消除微分方程(稳态问题) ，要么将偏微分方程转化为常微分方程的近似系统，然后使用标准技术进行数值积分，如欧拉方法、 Runge-Kutta 等。&lt;br /&gt;
&lt;br /&gt;
===Finite difference method===&lt;br /&gt;
有限差分法&lt;br /&gt;
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&lt;br /&gt;
{{main|Finite difference method}}&lt;br /&gt;
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Finite-difference methods are numerical methods for approximating the solutions to differential equations using [[finite difference]] equations to approximate derivatives.&lt;br /&gt;
&lt;br /&gt;
Finite-difference methods are numerical methods for approximating the solutions to differential equations using finite difference equations to approximate derivatives.&lt;br /&gt;
&lt;br /&gt;
有限差分法是一种数值方法，用差分方程近似微分方程的解。&lt;br /&gt;
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=== Finite volume method ===&lt;br /&gt;
有限体积法&lt;br /&gt;
&lt;br /&gt;
{{main|Finite volume method}}&lt;br /&gt;
&lt;br /&gt;
Similar to the finite difference method or finite element method, values are calculated at discrete places on a meshed geometry. &amp;quot;Finite volume&amp;quot; refers to the small volume surrounding each node point on a mesh. In the finite volume method, surface integrals in a partial differential equation that contain a divergence term are converted to volume integrals, using the [[divergence theorem]]. These terms are then evaluated as fluxes at the surfaces of each finite volume. Because the flux entering a given volume is identical to that leaving the adjacent volume, these methods conserve mass by design.&lt;br /&gt;
&lt;br /&gt;
Similar to the finite difference method or finite element method, values are calculated at discrete places on a meshed geometry. &amp;quot;Finite volume&amp;quot; refers to the small volume surrounding each node point on a mesh. In the finite volume method, surface integrals in a partial differential equation that contain a divergence term are converted to volume integrals, using the divergence theorem. These terms are then evaluated as fluxes at the surfaces of each finite volume. Because the flux entering a given volume is identical to that leaving the adjacent volume, these methods conserve mass by design.&lt;br /&gt;
&lt;br /&gt;
类似于有限差分法或有限元分析，函数值是在网状几何体上的离散位置进行计算的。“有限体积”是指网格上每个节点周围的小体积。在有限体积法中，偏微分方程中含有散度项的面积分用散度定理积分转换成体积分。然后将这些项用于估算每个有限体积表面上的通量。由于进入给定体积的通量与转移到相邻体积元的通量相同，所以这些方法在设计上保证了质量守恒。&lt;br /&gt;
&lt;br /&gt;
==See also==&lt;br /&gt;
请参阅&lt;br /&gt;
* [[Dirichlet boundary condition]]&lt;br /&gt;
狄利克雷边界条件&lt;br /&gt;
* [[Jet bundle]]&lt;br /&gt;
射流丛&lt;br /&gt;
* [[Laplace transform applied to differential equations]]&lt;br /&gt;
微分方程中的拉普拉斯变换&lt;br /&gt;
* [[List of dynamical systems and differential equations topics]]&lt;br /&gt;
动力学系统和微分方程的列表&lt;br /&gt;
* [[Matrix differential equation]]&lt;br /&gt;
矩阵微分方程&lt;br /&gt;
* [[Neumann boundary condition]]&lt;br /&gt;
诺伊曼边界条件&lt;br /&gt;
* [[Numerical partial differential equations]]&lt;br /&gt;
数值偏微分方程&lt;br /&gt;
* [[Partial differential algebraic equation]]&lt;br /&gt;
偏微分代数方程&lt;br /&gt;
* [[Recurrence relation]]&lt;br /&gt;
递推关系&lt;br /&gt;
* [[Robin boundary condition]]&lt;br /&gt;
罗宾边界条件&lt;br /&gt;
* [[Stochastic processes and boundary value problems]]&lt;br /&gt;
随机过程和边值问题&lt;br /&gt;
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== The energy method ==&lt;br /&gt;
能量法&lt;br /&gt;
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The energy method is a mathematical procedure that can be used to verify well-posedness of initial-boundary-value-problems.&amp;lt;ref&amp;gt;{{cite book |title=High Order Difference Methods for Time Dependent PDE&lt;br /&gt;
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The energy method is a mathematical procedure that can be used to verify well-posedness of initial-boundary-value-problems.&amp;lt;ref&amp;gt;{{cite book |title=High Order Difference Methods for Time Dependent PDE&lt;br /&gt;
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能量法是验证初边值问题适定性的一种数学方法。 时变偏微分方程的高阶差分方法&lt;br /&gt;
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|first=Bertil|last=Gustafsson|publisher=Springer|year=2008|isbn=978-3-540-74992-9|doi=10.1007/978-3-540-74993-6}}&amp;lt;/ref&amp;gt; In the following example the energy method is used to decide where and which boundary conditions should be imposed such that the resulting IBVP is well-posed. Consider the one-dimensional hyperbolic PDE given by&lt;br /&gt;
&lt;br /&gt;
|first=Bertil|last=Gustafsson|publisher=Springer|year=2008|isbn=978-3-540-74992-9|doi=10.1007/978-3-540-74993-6}}&amp;lt;/ref&amp;gt; In the following example the energy method is used to decide where and which boundary conditions should be imposed such that the resulting IBVP is well-posed. Consider the one-dimensional hyperbolic PDE given by&lt;br /&gt;
&lt;br /&gt;
| first Bertil | last Gustafsson | publisher | Springer | year 2008 | isbn 978-3-540-74992-9 | doi 10.1007 / 978-3-540-74993-6} / ref 在下面的例子中，使用能量方法来决定应该施加哪些边界条件，使得得到的 IBVP适定。考虑一维双曲偏微分方程&lt;br /&gt;
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: &amp;lt;math&amp;gt;\frac{\partial u}{\partial t} + \alpha \frac{\partial u}{\partial x} = 0, \quad x \in [a,b], \operatorname t &amp;gt; 0,&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;\frac{\partial u}{\partial t} + \alpha \frac{\partial u}{\partial x} = 0, \quad x \in [a,b], \operatorname t &amp;gt; 0,&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
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where &amp;lt;math&amp;gt;\alpha \neq 0&amp;lt;/math&amp;gt; is a constant and &amp;lt;math&amp;gt;u(x,t)&amp;lt;/math&amp;gt; is an unknown function with initial condition &amp;lt;math&amp;gt;u(x,0) = f(x)&amp;lt;/math&amp;gt;. Multiplying with &amp;lt;math&amp;gt;u&amp;lt;/math&amp;gt; and integrating over the domain gives&lt;br /&gt;
&lt;br /&gt;
where &amp;lt;math&amp;gt;\alpha \neq 0&amp;lt;/math&amp;gt; is a constant and &amp;lt;math&amp;gt;u(x,t)&amp;lt;/math&amp;gt; is an unknown function with initial condition &amp;lt;math&amp;gt;u(x,0) = f(x)&amp;lt;/math&amp;gt;. Multiplying with &amp;lt;math&amp;gt;u&amp;lt;/math&amp;gt; and integrating over the domain gives&lt;br /&gt;
&lt;br /&gt;
其中 &amp;lt;math&amp;gt;\alpha \neq 0&amp;lt;/math&amp;gt; 是常数，并且 &amp;lt;math&amp;gt;u(x,t)&amp;lt;/math&amp;gt; 是未知函数，初始条件是 &amp;lt;math&amp;gt;u(x,0) = f(x)&amp;lt;/math&amp;gt;。乘以 &amp;lt;math&amp;gt;u&amp;lt;/math&amp;gt; 并在域上进行积分。&lt;br /&gt;
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&lt;br /&gt;
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: &amp;lt;math&amp;gt;\int_a^b u \frac{\partial u}{\partial t} \operatorname dx + \alpha \int _a ^b u \frac{\partial u}{\partial x} \operatorname dx = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;\int_a^b u \frac{\partial u}{\partial t} \operatorname dx + \alpha \int _a ^b u \frac{\partial u}{\partial x} \operatorname dx = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
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Using that&lt;br /&gt;
&lt;br /&gt;
Using that&lt;br /&gt;
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利用这一点&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt;\int _a ^b u \frac{\partial u}{\partial t} \operatorname dx = \frac{1}{2} \frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 \quad \text{and} \quad \int _a ^b u \frac{\partial u}{\partial x} \operatorname dx = \frac{1}{2} u(b,t)^2 - \frac{1}{2} u(a,t)^2,.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;\int _a ^b u \frac{\partial u}{\partial t} \operatorname dx = \frac{1}{2} \frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 \quad \text{and} \quad \int _a ^b u \frac{\partial u}{\partial x} \operatorname dx = \frac{1}{2} u(b,t)^2 - \frac{1}{2} u(a,t)^2,.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
where integration by parts has been used for the second relationship, we get&lt;br /&gt;
&lt;br /&gt;
where integration by parts has been used for the second relationship, we get&lt;br /&gt;
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第二个关系中采用了分部积分法，我们可以得到&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt;\frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 + \alpha u(b,t)^2 - \alpha u(a,t)^2 = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;\frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 + \alpha u(b,t)^2 - \alpha u(a,t)^2 = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Here &amp;lt;math&amp;gt;\vert \vert \cdot \vert \vert&amp;lt;/math&amp;gt; denotes the standard L2-norm.&lt;br /&gt;
&lt;br /&gt;
Here &amp;lt;math&amp;gt;\vert \vert \cdot \vert \vert&amp;lt;/math&amp;gt; denotes the standard L2-norm.&lt;br /&gt;
&lt;br /&gt;
在这里，&amp;lt;math&amp;gt;\vert \vert \cdot \vert \vert&amp;lt;/math&amp;gt; 表示标准的 L2-正则。&lt;br /&gt;
&lt;br /&gt;
For well-posedness we require that the energy of the solution is non-increasing, i.e. that &amp;lt;math&amp;gt;\frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 \leq 0&amp;lt;/math&amp;gt;, which is achieved by specifying &amp;lt;math&amp;gt;u&amp;lt;/math&amp;gt; at &amp;lt;math&amp;gt;x = a&amp;lt;/math&amp;gt; if &amp;lt;math&amp;gt;\alpha &amp;gt; 0&amp;lt;/math&amp;gt; and at &amp;lt;math&amp;gt;x = b&amp;lt;/math&amp;gt; if &amp;lt;math&amp;gt;\alpha &amp;lt; 0&amp;lt;/math&amp;gt;. This corresponds to only imposing boundary conditions at the inflow. Note that well-posedness allows for growth in terms of data (initial and boundary) and thus it is sufficient to show that &amp;lt;math&amp;gt;\frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 \leq 0&amp;lt;/math&amp;gt; holds when all data is set to zero.&lt;br /&gt;
&lt;br /&gt;
For well-posedness we require that the energy of the solution is non-increasing, i.e. that &amp;lt;math&amp;gt;\frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 \leq 0&amp;lt;/math&amp;gt;, which is achieved by specifying &amp;lt;math&amp;gt;u&amp;lt;/math&amp;gt; at &amp;lt;math&amp;gt;x = a&amp;lt;/math&amp;gt; if &amp;lt;math&amp;gt;\alpha &amp;gt; 0&amp;lt;/math&amp;gt; and at &amp;lt;math&amp;gt;x = b&amp;lt;/math&amp;gt; if &amp;lt;math&amp;gt;\alpha &amp;lt; 0&amp;lt;/math&amp;gt;. This corresponds to only imposing boundary conditions at the inflow. Note that well-posedness allows for growth in terms of data (initial and boundary) and thus it is sufficient to show that &amp;lt;math&amp;gt;\frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 \leq 0&amp;lt;/math&amp;gt; holds when all data is set to zero.&lt;br /&gt;
&lt;br /&gt;
对于适定性，我们要解的能量是不增加的，即 &amp;lt;math&amp;gt;\frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 \leq 0&amp;lt;/math&amp;gt; ，这种关系可以通过在&amp;lt;math&amp;gt;x = a&amp;lt;/math&amp;gt;处 （如果 &amp;lt;math&amp;gt;\alpha &amp;gt; 0&amp;lt;/math&amp;gt;） 以及 &amp;lt;math&amp;gt;x = b&amp;lt;/math&amp;gt;处 （如果 &amp;lt;math&amp;gt;\alpha &amp;lt; 0&amp;lt;/math&amp;gt;）指定&amp;lt;math&amp;gt;u&amp;lt;/math&amp;gt;的值来实现。这只相当于在入流处附加边界条件。注意，适定性允许在数据(初始和边界)上的增长，因此它足以表明当所有数据设置为零时应有 &amp;lt;math&amp;gt;\frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 \leq 0&amp;lt;/math&amp;gt;。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==[[用户:Yuling|Yuling]]（[[用户讨论:Yuling|讨论]]）“This corresponds to only imposing boundary conditions at the inflow.” 这句话中的inflow不是很理解&lt;br /&gt;
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==Notes==&lt;br /&gt;
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{{Reflist}}&lt;br /&gt;
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== References ==&lt;br /&gt;
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{{refbegin|2}}&lt;br /&gt;
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&lt;br /&gt;
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&lt;br /&gt;
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* {{Citation |first=A. D. |last=Polyanin |first2=V. F. |last2=Zaitsev |lastauthoramp=yes |first3=A. |last3=Moussiaux |title=Handbook of First Order Partial Differential Equations |publisher=Taylor &amp;amp; Francis |location=London |year=2002 |isbn=0-415-27267-X }}.&lt;br /&gt;
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* {{citation|mr=3014456|last=Roubíček|first= T.|title=Nonlinear Partial Differential Equations with Applications|publisher= Birkhäuser|place= Basel, Boston, Berlin|edition=2nd|year= 2013|ISBN= 978-3-0348-0512-4|doi=10.1007/978-3-0348-0513-1|url=http://cds.cern.ch/record/880983/files/9783764372934_TOC.pdf}}&lt;br /&gt;
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* {{Citation |first=P. |last=Solin |title=Partial Differential Equations and the Finite Element Method |publisher=J. Wiley &amp;amp; Sons |location=Hoboken, NJ |year=2005 |isbn=0-471-72070-4 }}.&lt;br /&gt;
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* {{Citation |first=P. |last=Solin |first2=K. |last2=Segeth |lastauthoramp=yes |first3=I. |last3=Dolezel |title=Higher-Order Finite Element Methods |publisher=Chapman &amp;amp; Hall/CRC Press |location=Boca Raton |year=2003 |isbn=1-58488-438-X }}.&lt;br /&gt;
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* {{Citation |first=H. |last=Stephani |year=1989 |title=Differential Equations: Their Solution Using Symmetries. Edited by M. MacCallum |publisher=Cambridge University Press }}.&lt;br /&gt;
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* {{cite book |title=Partial Differential Equations and Solitary Waves Theory&lt;br /&gt;
&lt;br /&gt;
|first=Abdul-Majid|last=Wazwaz|publisher=Higher Education Press|year=2009|isbn=978-3-642-00251-9|page=}}&lt;br /&gt;
&lt;br /&gt;
|first=Abdul-Majid|last=Wazwaz|publisher=Higher Education Press|year=2009|isbn=978-3-642-00251-9|page=}}&lt;br /&gt;
&lt;br /&gt;
| first Abdul-Majid | last Wazwaz | publisher Higher Education Press | year 2009 | isbn 978-3-642-00251-9 | page }&lt;br /&gt;
&lt;br /&gt;
* {{cite book |title=Partial Differential Equations Methods and Applications&lt;br /&gt;
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|first=Abdul-Majid|last=Wazwaz|publisher=A.A. Balkema|year=2002|isbn=90-5809-369-7|page=}}&lt;br /&gt;
&lt;br /&gt;
|first=Abdul-Majid|last=Wazwaz|publisher=A.A. Balkema|year=2002|isbn=90-5809-369-7|page=}}&lt;br /&gt;
&lt;br /&gt;
| first Abdul-Majid | last Wazwaz | publisher a.a.Balkema | year 2002 | isbn 90-5809-369-7 | page }&lt;br /&gt;
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* {{Citation |first=D. |last=Zwillinger |title=Handbook of Differential Equations |publisher=Academic Press |location=Boston |year=1997 |edition=3rd |isbn=0-12-784395-7 }}.&lt;br /&gt;
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* {{Citation |authorlink=Neil Gershenfeld |first=N. |last=Gershenfeld |title=The Nature of Mathematical Modeling |location=New York |publisher=Cambridge University Press, New York, NY, USA |year=1999 |edition=1st |isbn=0-521-57095-6 }}.&lt;br /&gt;
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* {{Citation |first=I.S. |last=Krasil'shchik |lastauthoramp=yes |first2=A.M., Eds. |last2=Vinogradov |title=Symmetries and Conserwation Laws for Differential Equations of Mathematical Physics |publisher=American Mathematical Society, Providence, Rhode Island, USA |year=1999 |isbn=0-8218-0958-X }}.&lt;br /&gt;
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* {{Citation |first=I.S. |last=Krasil'shchik |first2=V.V. |last2=Lychagin|lastauthoramp=yes |first3=A.M. |last3=Vinogradov |title=Geometry of Jet Spaces and Nonlinear Partial Differential Equations |publisher=Gordon and Breach Science Publishers, New York, London, Paris, Montreux, Tokyo |year=1986 |isbn=2-88124-051-8 }}.&lt;br /&gt;
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* {{Citation |first=A.M. |last=Vinogradov |title=Cohomological Analysis of Partial Differential Equations and Secondary Calculus |publisher=American Mathematical Society, Providence, Rhode Island, USA |year=2001 |isbn=0-8218-2922-X }}.&lt;br /&gt;
&lt;br /&gt;
* {{cite book |title=High Order Difference Methods for Time Dependent PDE&lt;br /&gt;
&lt;br /&gt;
|first=Bertil|last=Gustafsson|publisher=Springer|year=2008|isbn=978-3-540-74992-9|doi=10.1007/978-3-540-74993-6}}&lt;br /&gt;
&lt;br /&gt;
|first=Bertil|last=Gustafsson|publisher=Springer|year=2008|isbn=978-3-540-74992-9|doi=10.1007/978-3-540-74993-6}}&lt;br /&gt;
&lt;br /&gt;
| first Bertil | last Gustafsson | Springer | year 2008 | isbn 978-3-540-74992-9 | doi 10.1007 / 978-3-540-74993-6}&lt;br /&gt;
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{{refend}}&lt;br /&gt;
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== Further reading ==&lt;br /&gt;
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* {{Cite journal|last=Cajori|first=Florian|authorlink=Florian Cajori|year=1928|title=The Early History of Partial Differential Equations and of Partial Differentiation and Integration|url=http://www.math.harvard.edu/archive/21a_fall_14/exhibits/cajori/cajori.pdf|journal=The American Mathematical Monthly|volume=35|issue=9|pages=459–467|doi=10.2307/2298771|access-date=2016-05-15|archive-url=https://web.archive.org/web/20181123102253/http://www.math.harvard.edu/archive/21a_fall_14/exhibits/cajori/cajori.pdf|archive-date=2018-11-23|url-status=dead}}&lt;br /&gt;
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== External links ==&lt;br /&gt;
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{{Sister project links| wikt=no | commons=Category:Solutions of PDE | b=Partial Differential Equations | n=no | q=Partial differential equation | s=no | v=no | voy=no | species=no | d=no}}&lt;br /&gt;
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* {{springer|title=Differential equation, partial|id=p/d031920}}&lt;br /&gt;
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* [http://eqworld.ipmnet.ru/en/pde-en.htm Partial Differential Equations: Exact Solutions] at EqWorld: The World of Mathematical Equations.&lt;br /&gt;
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* [http://eqworld.ipmnet.ru/en/solutions/eqindex/eqindex-pde.htm Partial Differential Equations: Index] at EqWorld: The World of Mathematical Equations.&lt;br /&gt;
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* [http://eqworld.ipmnet.ru/en/methods/meth-pde.htm Partial Differential Equations: Methods] at EqWorld: The World of Mathematical Equations.&lt;br /&gt;
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* [https://web.archive.org/web/20170701144823/http://www.exampleproblems.com/wiki/index.php?title=Partial_Differential_Equations Example problems with solutions] at exampleproblems.com&lt;br /&gt;
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* [http://mathworld.wolfram.com/PartialDifferentialEquation.html Partial Differential Equations] at mathworld.wolfram.com&lt;br /&gt;
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* [https://reference.wolfram.com/language/FEMDocumentation/tutorial/SolvingPDEwithFEM.html Partial Differential Equations] with Mathematica&lt;br /&gt;
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* [http://www.mathworks.com/moler/pdes.pdf Partial Differential Equations] in Cleve Moler: Numerical Computing with MATLAB&lt;br /&gt;
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* [http://www.nag.com/numeric/fl/nagdoc_fl24/html/D03/d03intro.html Partial Differential Equations] at nag.com&lt;br /&gt;
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* {{cite web |first=Grant |last=Sanderson |title=But what is a partial differential equation? |work=3Blue1Brown |date=April 21, 2019 |url=https://www.youtube.com/watch?v=ly4S0oi3Yz8&amp;amp;list=PLZHQObOWTQDNPOjrT6KVlfJuKtYTftqH6 |via=[[YouTube]] }}&lt;br /&gt;
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{{Differential equations topics}}&lt;br /&gt;
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[[Category:Partial differential equations| ]]&lt;br /&gt;
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[[Category:Multivariable calculus]]&lt;br /&gt;
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Category:Multivariable calculus&lt;br /&gt;
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类别: 多元微积分&lt;br /&gt;
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[[Category:Differential equations]]&lt;br /&gt;
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Category:Differential equations&lt;br /&gt;
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类别: 微分方程&lt;br /&gt;
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[[Category:Concepts in physics]]&lt;br /&gt;
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Category:Concepts in physics&lt;br /&gt;
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分类: 物理概念&lt;br /&gt;
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&amp;lt;small&amp;gt;This page was moved from [[wikipedia:en:Partial differential equation]]. Its edit history can be viewed at [[偏微分方程/edithistory]]&amp;lt;/small&amp;gt;&amp;lt;/noinclude&amp;gt;&lt;br /&gt;
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[[Category:待整理页面]]&lt;/div&gt;</summary>
		<author><name>Ruili</name></author>
	</entry>
	<entry>
		<id>https://wiki.swarma.org/index.php?title=%E5%81%8F%E5%BE%AE%E5%88%86%E6%96%B9%E7%A8%8B&amp;diff=18203</id>
		<title>偏微分方程</title>
		<link rel="alternate" type="text/html" href="https://wiki.swarma.org/index.php?title=%E5%81%8F%E5%BE%AE%E5%88%86%E6%96%B9%E7%A8%8B&amp;diff=18203"/>
		<updated>2020-11-12T15:57:56Z</updated>

		<summary type="html">&lt;p&gt;Ruili：&lt;/p&gt;
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&lt;div&gt;此词条暂由Yuling翻译，未经人工整理和审校，带来阅读不便，请见谅。&lt;br /&gt;
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[[File:Heat.gif|thumb|right|A visualisation of a solution to the two-dimensional [[heat equation]] with temperature represented by the third dimension]]&lt;br /&gt;
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A visualisation of a solution to the two-dimensional [[heat equation with temperature represented by the third dimension]]&lt;br /&gt;
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以三维表示温度的二维热方程解的可视化&lt;br /&gt;
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In [[mathematics]], a '''partial differential equation''' ('''PDE''') is a [[differential equation]] that contains unknown [[Multivariable calculus|multivariable functions]] and their [[partial derivative]]s. PDEs are used to formulate problems involving functions of several variables, and are either solved by hand, or used to create a [[computer model]]. A special case is [[ordinary differential equation]]s (ODEs), which deal with functions of a single variable and their derivatives.&lt;br /&gt;
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In mathematics, a partial differential equation (PDE) is a differential equation that contains unknown multivariable functions and their partial derivatives. PDEs are used to formulate problems involving functions of several variables, and are either solved by hand, or used to create a computer model. A special case is ordinary differential equations (ODEs), which deal with functions of a single variable and their derivatives.&lt;br /&gt;
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在数学中，'''&amp;lt;font color = &amp;quot;#ff8000&amp;quot;&amp;gt; 偏微分方程函数 Partial Differential Equation&amp;lt;/font&amp;gt;'''是包含未知多元函数及其偏导数的微分方程。偏微分方程用于描述涉及多元函数的问题，可以通过人为求解，也可以通过建立计算机模型来求解。常微分方程是偏微分方程一种特殊情况，它处理的是一元函数及其导数。&lt;br /&gt;
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PDEs can be used to describe a wide variety of phenomena such as sound, heat, [[diffusion]], [[electrostatics]], [[Electromagnetism|electrodynamics]], [[fluid dynamics]], [[Elasticity (physics)|elasticity]], [[gravitation]] and [[quantum mechanics]]. These seemingly distinct physical phenomena can be formalised similarly in terms of PDEs. Just as ordinary differential equations often model one-dimensional [[dynamical system]]s, partial differential equations often model [[multidimensional system]]s. PDEs find their generalisation in [[stochastic partial differential equation]]s.&lt;br /&gt;
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PDEs can be used to describe a wide variety of phenomena such as sound, heat, diffusion, electrostatics, electrodynamics, fluid dynamics, elasticity, gravitation and quantum mechanics. These seemingly distinct physical phenomena can be formalised similarly in terms of PDEs. Just as ordinary differential equations often model one-dimensional dynamical systems, partial differential equations often model multidimensional systems. PDEs find their generalisation in stochastic partial differential equations.&lt;br /&gt;
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偏微分方程可以用来描述各种各样的物理现象，如声音，热量，扩散，静电，电动力学，流体力学，弹性力学，重力和量子力学。这些看起来截然不同的物理现象却可以用类似的偏微分方程来描述。正如常微分方程经常对一维动力系统进行建模一样，偏微分方程经常对多维系统进行建模。随机偏微分方程是偏微分方程的一种推广。&lt;br /&gt;
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== Introduction ==&lt;br /&gt;
引言&lt;br /&gt;
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Partial differential equations (PDEs) are equations that involve rates of change with respect to [[continuous variables]]. For example, the position of a [[rigid body]] is specified by six parameters,&amp;lt;ref&amp;gt;{{Cite book|url=https://books.google.com/books?id=v9PLbcYd9aUC&amp;amp;pg=PA32|title=Modelling and Control of Robot Manipulators|last=Sciavicco|first=Lorenzo|last2=Siciliano|first2=Bruno|date=2001-02-19|publisher=Springer Science &amp;amp; Business Media|isbn=9781852332211|language=en}}&amp;lt;/ref&amp;gt; but the configuration of a [[fluid]] is given by the [[continuous distribution]] of several parameters, such as the [[temperature]], [[pressure]], and so forth. The dynamics for the rigid body take place in a finite-dimensional [[Configuration space (physics)|configuration space]]; the dynamics for the fluid occur in an infinite-dimensional configuration space. This distinction usually makes PDEs much harder to solve than ordinary differential equations (ODEs), but here again, there will be simple solutions for linear problems. Classic domains where PDEs are used include [[acoustics]], [[fluid dynamics]], [[electrodynamics]], and [[heat transfer]].&lt;br /&gt;
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Partial differential equations (PDEs) are equations that involve rates of change with respect to continuous variables. For example, the position of a rigid body is specified by six parameters, but the configuration of a fluid is given by the continuous distribution of several parameters, such as the temperature, pressure, and so forth. The dynamics for the rigid body take place in a finite-dimensional configuration space; the dynamics for the fluid occur in an infinite-dimensional configuration space. This distinction usually makes PDEs much harder to solve than ordinary differential equations (ODEs), but here again, there will be simple solutions for linear problems. Classic domains where PDEs are used include acoustics, fluid dynamics, electrodynamics, and heat transfer.&lt;br /&gt;
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偏微分方程(简称为PDEs)涉及到方程相对于连续变量的变化率。例如，刚体的位置是由六个参数确定的，而流体的状态是由几个参数的连续分布给出的，如温度、压力等。刚体的动力学过程发生在有限维状态空间中，流体的动力学过程发生在无限维状态空间中。这种区别通常使偏微分方程比常微分方程更难求解，但是线性问题仍然有简单的求解方式。使用偏微分方程的经典领域包括声学、流体力学、电动力学和传热学。&lt;br /&gt;
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A partial differential equation (PDE) for the function {{math|''u''(''x''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;,… ''x&amp;lt;sub&amp;gt;n&amp;lt;/sub&amp;gt;'')}} is an equation of the form&lt;br /&gt;
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A partial differential equation (PDE) for the function  is an equation of the form&lt;br /&gt;
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函数 {{math|''u''(''x''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;,… ''x&amp;lt;sub&amp;gt;n&amp;lt;/sub&amp;gt;'')}} 的偏微分方程形式是：&lt;br /&gt;
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: &amp;lt;math&amp;gt;f \left (x_1, \ldots x_n; u, \frac{\partial u}{\partial x_1}, \ldots \frac{\partial u}{\partial x_n}; \frac{\partial^2 u}{\partial x_1 \partial x_1}, \ldots \frac{\partial^2 u}{\partial x_1 \partial x_n}; \ldots \right) = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;f \left (x_1, \ldots x_n; u, \frac{\partial u}{\partial x_1}, \ldots \frac{\partial u}{\partial x_n}; \frac{\partial^2 u}{\partial x_1 \partial x_1}, \ldots \frac{\partial^2 u}{\partial x_1 \partial x_n}; \ldots \right) = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
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If {{mvar|f}} is a [[linear function]] of {{mvar|u}} and its derivatives, then the PDE is called linear. Common examples of linear PDEs include the [[heat equation]], the [[wave equation]], [[Laplace's equation]], [[Helmholtz equation]], [[Klein–Gordon equation]], and [[Poisson's equation]].&lt;br /&gt;
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If  is a linear function of  and its derivatives, then the PDE is called linear. Common examples of linear PDEs include the heat equation, the wave equation, Laplace's equation, Helmholtz equation, Klein–Gordon equation, and Poisson's equation.&lt;br /&gt;
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如果 {{mvar|f}} 是函数 {{math|''u''}} 及其导数的线性函数，则偏微分方程称为线性函数。线性偏微分方程的常见例子包括热方程、波动方程、拉普拉斯方程、亥姆霍兹方程方程、克莱因-高登方程和泊松方程。&lt;br /&gt;
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A relatively simple PDE is&lt;br /&gt;
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A relatively simple PDE is&lt;br /&gt;
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一个相对简单的偏微分方程：&lt;br /&gt;
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: &amp;lt;math&amp;gt;\frac{\partial u}{\partial x}(x,y) = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;\frac{\partial u}{\partial x}(x,y) = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
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This relation [[Logical implication|implies]] that the function {{math|''u''(''x'',''y'')}} is independent of {{mvar|x}}. However, the equation gives no information on the function's dependence on the variable {{mvar|y}}. Hence the general solution of this equation is&lt;br /&gt;
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This relation implies that the function  is independent of . However, the equation gives no information on the function's dependence on the variable . Hence the general solution of this equation is&lt;br /&gt;
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这意味着函数 {{math|''u''(''x'',''y'')}} 独立于 {{mvar|x}} 的。然而，这个方程没有给出关于函数和自变量的相关性的信息。因此，这个方程的通解是&lt;br /&gt;
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: &amp;lt;math&amp;gt;u(x,y) = f(y),&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;u(x,y) = f(y),&amp;lt;/math&amp;gt;&lt;br /&gt;
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where {{mvar|f}} is an arbitrary function of {{mvar|y}}. The analogous ordinary differential equation is&lt;br /&gt;
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where  is an arbitrary function of . The analogous ordinary differential equation is&lt;br /&gt;
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其中， {{mvar|f}} 是 {{mvar|y}} 的任意函数。&lt;br /&gt;
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类似的常微分方程是：&lt;br /&gt;
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: &amp;lt;math&amp;gt;\frac{\mathrm{d} u}{\mathrm{d} x}(x) = 0,&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;\frac{\mathrm{d} u}{\mathrm{d} x}(x) = 0,&amp;lt;/math&amp;gt;&lt;br /&gt;
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which has the solution&lt;br /&gt;
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which has the solution&lt;br /&gt;
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它的解为&lt;br /&gt;
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: &amp;lt;math&amp;gt;u(x) = c,&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;u(x) = c,&amp;lt;/math&amp;gt;&lt;br /&gt;
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where {{mvar|c}} is any [[Constant (mathematics)|constant]] value. These two examples illustrate that general solutions of ordinary differential equations (ODEs) involve arbitrary constants, but solutions of PDEs involve arbitrary functions.&lt;br /&gt;
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where  is any constant value. These two examples illustrate that general solutions of ordinary differential equations (ODEs) involve arbitrary constants, but solutions of PDEs involve arbitrary functions.&lt;br /&gt;
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这里，{{mvar|c}} 是一个任意常量。&lt;br /&gt;
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这两个例子说明常微分方程的一般解包含任意常数，但偏微分方程的解包含任意函数。&lt;br /&gt;
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A solution of a PDE is generally not [[Uniqueness quantification|unique]]; additional conditions must generally be specified on the [[Boundary (topology)|boundary]] of the region where the solution is defined. For instance, in the simple example above, the function {{math|''f''(''y'')}} can be determined if {{mvar|u}} is specified on the line {{math|''x'' {{=}} 0}}.&lt;br /&gt;
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A solution of a PDE is generally not unique; additional conditions must generally be specified on the boundary of the region where the solution is defined. For instance, in the simple example above, the function  can be determined if  is specified on the line  0}}.&lt;br /&gt;
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偏微分方程的解一般不是唯一的; 一般必须在定义解的区域边界上定义附加条件。 例如，在上面的简单示例中，如果在 {{math|''x'' {{=}} 0}} 时确定了 {{mvar|u}} 的值，则可以确定该函数 {{math|''f''(''y'')}}。&lt;br /&gt;
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== Existence and uniqueness ==&lt;br /&gt;
存在性和唯一性&lt;br /&gt;
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Although the issue of existence and uniqueness of solutions of ordinary differential equations has a very satisfactory answer with the [[Picard–Lindelöf theorem]], that is far from the case for partial differential equations. The [[Cauchy–Kowalevski theorem]] states that the [[Cauchy problem]] for any partial differential equation whose coefficients are [[Analytic function|analytic]] in the unknown function and its derivatives, has a locally unique analytic solution. Although this result might appear to settle the existence and uniqueness of solutions, there are examples of linear partial differential equations whose coefficients have derivatives of all orders (which are nevertheless not analytic) but which have no solutions at all: see [[Lewy's example|Lewy (1957)]]. Even if the solution of a partial differential equation exists and is unique, it may nevertheless have undesirable properties.  The mathematical study of these questions is usually in the more powerful context of [[weak solution]]s.&lt;br /&gt;
&lt;br /&gt;
Although the issue of existence and uniqueness of solutions of ordinary differential equations has a very satisfactory answer with the Picard–Lindelöf theorem, that is far from the case for partial differential equations. The Cauchy–Kowalevski theorem states that the Cauchy problem for any partial differential equation whose coefficients are analytic in the unknown function and its derivatives, has a locally unique analytic solution. Although this result might appear to settle the existence and uniqueness of solutions, there are examples of linear partial differential equations whose coefficients have derivatives of all orders (which are nevertheless not analytic) but which have no solutions at all: see Lewy (1957). Even if the solution of a partial differential equation exists and is unique, it may nevertheless have undesirable properties.  The mathematical study of these questions is usually in the more powerful context of weak solutions.&lt;br /&gt;
&lt;br /&gt;
尽管常微分方程解的存在性和唯一性用'''&amp;lt;font color=&amp;quot;#ff8000&amp;quot;&amp;gt;弗罗贝尼乌斯定理 Picard–Lindelöf Theorem&amp;lt;/font&amp;gt;得到了令人满意的结果，但偏微分方程解的存在性和唯一性却远没有得到解决。'''&amp;lt;font color=&amp;quot;#ff8000&amp;quot;&amp;gt;柯西-科瓦列夫斯基定理 Cauchy–Kowalevski theorem&amp;lt;/font&amp;gt;指出：对于任意系数在未知函数及其导数中解析的偏微分方程，柯西问题存在一个局部唯一的解析解。虽然这个结果似乎解决了解的存在性和唯一性问题，但是存在一些线性偏微分方程-其系数具有所有级数的导数(尽管这些导数不是解析的) ，但是根本没有解: 见 Lewy (1957)。即使偏微分方程的解存在且唯一，它仍然可能具有不可预料的性质。这些问题的数学研究通常是在更有力的弱解的背景下进行的。&lt;br /&gt;
&lt;br /&gt;
An example of pathological behavior is the sequence (depending upon {{mvar|n}}) of [[Cauchy problem]]s for the [[Laplace equation]]&lt;br /&gt;
&lt;br /&gt;
An example of pathological behavior is the sequence (depending upon ) of Cauchy problems for the Laplace equation&lt;br /&gt;
&lt;br /&gt;
反常特征的一个例子是拉普拉斯方程的柯西问题的序列(取决于{{mvar|n}})&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt;\frac{\partial^2 u}{\partial x^2} + \frac{\partial^2 u}{\partial y^2}=0,&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;\frac{\partial^2 u}{\partial x^2} + \frac{\partial^2 u}{\partial y^2}=0,&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
with [[boundary condition]]s&lt;br /&gt;
&lt;br /&gt;
with boundary conditions&lt;br /&gt;
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具有边界条件&lt;br /&gt;
&lt;br /&gt;
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&lt;br /&gt;
: &amp;lt;math&amp;gt;\begin{align} u(x,0) &amp;amp;= 0, \\ \frac{\partial u}{\partial y}(x,0) &amp;amp;= \frac{\sin nx}{n}, \end{align}&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;\begin{align} u(x,0) &amp;amp;= 0, \\ \frac{\partial u}{\partial y}(x,0) &amp;amp;= \frac{\sin nx}{n}, \end{align}&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
where {{mvar|n}} is an integer. The derivative of {{mvar|u}} with respect to {{mvar|y}} approaches zero [[uniform convergence|uniformly]] in {{mvar|x}} as {{mvar|n}} increases, but the solution is&lt;br /&gt;
&lt;br /&gt;
where  is an integer. The derivative of  with respect to  approaches zero uniformly in  as  increases, but the solution is&lt;br /&gt;
&lt;br /&gt;
其中 {{mvar|n}} 是整数。{{mvar|u}} 关于 {{mvar|y}} 的导数，一致地随着 {{mvar|n}} 的增加而趋于零，但解是&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt;u(x,y) = \frac{\sinh ny \sin nx}{n^2}.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;u(x,y) = \frac{\sinh ny \sin nx}{n^2}.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
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This solution approaches infinity if {{mvar|nx}} is not an integer multiple of {{pi}} for any non-zero value of {{mvar|y}}. The Cauchy problem for the Laplace equation is called ''ill-posed'' or ''not [[Well-posed problem|well-posed]]'', since the solution does not continuously depend on the data of the problem. Such ill-posed problems are not usually satisfactory for physical applications.&lt;br /&gt;
&lt;br /&gt;
This solution approaches infinity if  is not an integer multiple of  for any non-zero value of . The Cauchy problem for the Laplace equation is called ill-posed or not well-posed, since the solution does not continuously depend on the data of the problem. Such ill-posed problems are not usually satisfactory for physical applications.&lt;br /&gt;
&lt;br /&gt;
对于任何非零的 {{mvar|y}}，如果 {{mvar|nx}} 不是模板 {{pi}} 的整数倍，这个解会接近于无穷大。拉普拉斯方程的柯西问题被称为不适定的（可以译为ill-posed或not well-posed），因为解不是连续地依赖于问题的数据。这种不适定问题通常不能满足物理应用。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The [[Navier–Stokes existence and smoothness|existence of solutions for the Navier–Stokes equations]], a partial differential equation, is part of one of the [[Millennium Prize Problems]].&lt;br /&gt;
&lt;br /&gt;
The existence of solutions for the Navier–Stokes equations, a partial differential equation, is part of one of the Millennium Prize Problems.&lt;br /&gt;
&lt;br /&gt;
一种偏微分方程——纳维-斯托克斯方程——的解的存在性就是千禧年大奖难题的一部分。&lt;br /&gt;
&lt;br /&gt;
== Notation ==&lt;br /&gt;
符号&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
In PDEs, it is common to denote partial derivatives using subscripts. That is:&lt;br /&gt;
&lt;br /&gt;
In PDEs, it is common to denote partial derivatives using subscripts. That is:&lt;br /&gt;
&lt;br /&gt;
在偏微分方程中，通常用下标表示偏导数。例如:&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt;u_x = \frac{\partial u}{\partial x}&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;u_x = \frac{\partial u}{\partial x}&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt;u_{xx} = \frac{\partial^2 u}{\partial x^2} &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;u_{xx} = \frac{\partial^2 u}{\partial x^2} &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt;u_{xy} = \frac{\partial^2 u}{\partial y\, \partial x} = \frac{\partial}{\partial y } \left(\frac{\partial u}{\partial x}\right). &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;u_{xy} = \frac{\partial^2 u}{\partial y\, \partial x} = \frac{\partial}{\partial y } \left(\frac{\partial u}{\partial x}\right). &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Especially in physics, [[del]] or nabla ({{math|∇}}) is often used to denote spatial derivatives, and {{math|''&amp;amp;#x307;u'', ''ü''}} for time derivatives. For example, the [[wave equation]] (mentioned below) can be written as&lt;br /&gt;
&lt;br /&gt;
Especially in physics, del or nabla () is often used to denote spatial derivatives, and  for time derivatives. For example, the wave equation (mentioned below) can be written as&lt;br /&gt;
&lt;br /&gt;
特别是在物理学中，[[del]]或nabla ({{math|∇}})经常用来表示空间导数和时间导数。例如，波动方程(在下文中提到)可以写成&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt;\ddot u=c^2\nabla^2u&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt;\ddot u=c^2\nabla^2u&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
or&lt;br /&gt;
&lt;br /&gt;
or&lt;br /&gt;
&lt;br /&gt;
或&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt;\ddot u=c^2\Delta u&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt;\ddot u=c^2\Delta u&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
where {{math|Δ}} is the [[Laplace operator]].&lt;br /&gt;
&lt;br /&gt;
where  is the Laplace operator.&lt;br /&gt;
&lt;br /&gt;
其中{{math|Δ}}代表拉普拉斯算子&lt;br /&gt;
&lt;br /&gt;
== Classification ==&lt;br /&gt;
分类&lt;br /&gt;
&lt;br /&gt;
Some linear, second-order partial differential equations can be classified as [[parabolic partial differential equation|parabolic]], [[hyperbolic partial differential equation|hyperbolic]] and [[elliptic partial differential equation|elliptic]]. Others, such as the [[Euler–Tricomi equation]], have different types in different regions. The classification provides a guide to appropriate initial and boundary conditions and to the smoothness of the solutions.&lt;br /&gt;
&lt;br /&gt;
Some linear, second-order partial differential equations can be classified as parabolic, hyperbolic and elliptic. Others, such as the Euler–Tricomi equation, have different types in different regions. The classification provides a guide to appropriate initial and boundary conditions and to the smoothness of the solutions.&lt;br /&gt;
&lt;br /&gt;
一些线性二阶偏微分方程可分为抛物型方程、双曲型方程和椭圆型方程。其他的方程，如欧拉-特里科米方程，在不同的区域有不同的类型。这种分类有助于选择适当的初始和边界条件以及提高解的平滑性。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
=== Equations of first order ===&lt;br /&gt;
一阶方程&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{{main|First-order partial differential equation}}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
=== Linear equations of second order ===&lt;br /&gt;
二阶线性方程&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Assuming {{math|''u&amp;lt;sub&amp;gt;xy&amp;lt;/sub&amp;gt;'' {{=}} ''u&amp;lt;sub&amp;gt;yx&amp;lt;/sub&amp;gt;''}}, the general linear second-order PDE in two independent variables has the form&lt;br /&gt;
&lt;br /&gt;
Assuming  u&amp;lt;sub&amp;gt;yx&amp;lt;/sub&amp;gt;}}, the general linear second-order PDE in two independent variables has the form&lt;br /&gt;
&lt;br /&gt;
假设 {{math|''u&amp;lt;sub&amp;gt;xy&amp;lt;/sub&amp;gt;'' {{=}} ''u&amp;lt;sub&amp;gt;yx&amp;lt;/sub&amp;gt;''}}，含有两个独立变量的一般的线性二阶偏微分方程具有如下这样的形式&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt;Au_{xx} + 2Bu_{xy} + Cu_{yy} + \cdots \mbox{(lower order terms)} = 0,&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;Au_{xx} + 2Bu_{xy} + Cu_{yy} + \cdots \mbox{(lower order terms)} = 0,&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
where the coefficients {{mvar|A}}, {{mvar|B}}, {{mvar|C}}... may depend upon {{mvar|x}} and {{mvar|y}}. If {{math|''A''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; + ''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; + ''C''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; &amp;gt; 0}} over a region of the {{mvar|xy}}-plane, the PDE is second-order in that region. This form is analogous to the equation for a conic section:&lt;br /&gt;
&lt;br /&gt;
where the coefficients , , ... may depend upon  and . If  over a region of the -plane, the PDE is second-order in that region. This form is analogous to the equation for a conic section:&lt;br /&gt;
&lt;br /&gt;
其中的系数 {{mvar|A}}, {{mvar|B}}, {{mvar|C}}... 一般取决于{{mvar|x}}和{{mvar|y}}。如果在{{mvar|xy}}-平面的一个区域上 {{math|''A''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; + ''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; + ''C''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; &amp;gt; 0}}，偏微分方程在该区域是二阶的。这种形式类似于圆锥曲线的方程:&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt;Ax^2 + 2Bxy + Cy^2 + \cdots = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;Ax^2 + 2Bxy + Cy^2 + \cdots = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
More precisely, replacing {{math|∂&amp;lt;sub&amp;gt;''x''&amp;lt;/sub&amp;gt;}} by {{mvar|X}}, and likewise for other variables (formally this is done by a [[Fourier transform]]), converts a constant-coefficient PDE into a polynomial of the same degree, with the terms of the highest degree (a [[homogeneous polynomial]], here a [[quadratic form]]) being most significant for the classification.&lt;br /&gt;
&lt;br /&gt;
More precisely, replacing  by , and likewise for other variables (formally this is done by a Fourier transform), converts a constant-coefficient PDE into a polynomial of the same degree, with the terms of the highest degree (a homogeneous polynomial, here a quadratic form) being most significant for the classification.&lt;br /&gt;
&lt;br /&gt;
更准确地说，用 {{mvar|X}} 替换 {{math|∂&amp;lt;sub&amp;gt;''x''&amp;lt;/sub&amp;gt;}}，对于其他变量做同样的操作(从形式上来说，这是由傅里叶变换来完成的)，将一个常系数偏微分方程转换成一个相同次数的多项式，最高次数的项(齐次多项式，这里是一个二次形式)一般会用于偏微分方程的分类。&lt;br /&gt;
===~~ most significant for the classification 意译为用于偏微分方程的分类。       significiant直译过来感觉不太合适&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Just as one classifies [[conic section]]s and quadratic forms into parabolic, hyperbolic, and elliptic based on the [[discriminant]] {{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − 4''AC''}}, the same can be done for a second-order PDE at a given point.  However, the [[discriminant]] in a PDE is given by {{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC''}} due to the convention of the {{mvar|xy}} term being {{math|2''B''}} rather than {{mvar|B}}; formally, the discriminant (of the associated quadratic form) is {{math|(2''B'')&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − 4''AC'' {{=}} 4(''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC'')}}, with the factor of 4 dropped for simplicity.&lt;br /&gt;
&lt;br /&gt;
Just as one classifies conic sections and quadratic forms into parabolic, hyperbolic, and elliptic based on the discriminant , the same can be done for a second-order PDE at a given point.  However, the discriminant in a PDE is given by  due to the convention of the  term being  rather than ; formally, the discriminant (of the associated quadratic form) is  4(B&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − AC)}}, with the factor of 4 dropped for simplicity.&lt;br /&gt;
&lt;br /&gt;
正如人们可以根据判别式 {{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − 4''AC''}} 将圆锥曲线和二次型分为抛物型、双曲型和椭圆型一样，对于给定点的二阶偏微分方程也可以这样做。然而，偏微分方程中的判别式 {{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − 4''AC''}} 是根据交叉项的系数{{math|2''B''}} 而不是 {{mvar|B}} 给出的，形式上，判别式(关联二次型)是 {{math|(2''B'')&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − 4''AC'' {{=}} 4(''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC'')}}，为简单起见，去掉了因子4。&lt;br /&gt;
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# {{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC'' &amp;lt; 0}} (''[[elliptic partial differential equation]]''): Solutions of [[elliptic partial differential equation|elliptic PDEs]] are as smooth as the coefficients allow, within the interior of the region where the equation and solutions are defined. For example, solutions of [[Laplace's equation]] are analytic within the domain where they are defined, but solutions may assume boundary values that are not smooth. The motion of a fluid at subsonic speeds can be approximated with elliptic PDEs, and the Euler–Tricomi equation is elliptic where {{math|''x'' &amp;lt; 0}}.&lt;br /&gt;
&lt;br /&gt;
  (elliptic partial differential equation): Solutions of elliptic PDEs are as smooth as the coefficients allow, within the interior of the region where the equation and solutions are defined. For example, solutions of Laplace's equation are analytic within the domain where they are defined, but solutions may assume boundary values that are not smooth. The motion of a fluid at subsonic speeds can be approximated with elliptic PDEs, and the Euler–Tricomi equation is elliptic where .&lt;br /&gt;
&lt;br /&gt;
{{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC'' &amp;lt; 0}} (椭圆形微分方程)：在定义方程和解的区域内部，椭圆型偏微分方程的解光滑到系数允许的程度。例如，拉普拉斯方程的解在它们被定义的区域内是解析的，但是解可能假设边界值是不光滑的。亚音速流体的运动可以用椭圆偏微分方程近似，其中欧拉-特里科米方程在 {{math|''x'' &amp;lt; 0}} 时是椭圆型偏微分方程。&lt;br /&gt;
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&lt;br /&gt;
&lt;br /&gt;
# {{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC'' {{=}} 0}} (''[[parabolic partial differential equation]]''): Equations that are [[parabolic partial differential equation|parabolic]] at every point can be transformed into a form analogous to the [[heat equation]] by a change of independent variables. Solutions smooth out as the transformed time variable increases. The Euler–Tricomi equation has parabolic type on the line where {{math|''x'' {{=}} 0}}.&lt;br /&gt;
&lt;br /&gt;
  0}} (parabolic partial differential equation): Equations that are parabolic at every point can be transformed into a form analogous to the heat equation by a change of independent variables. Solutions smooth out as the transformed time variable increases. The Euler–Tricomi equation has parabolic type on the line where  0}}.&lt;br /&gt;
&lt;br /&gt;
{{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC'' {{=}} 0}}（抛物线形偏微分方程）：在每一点上都是抛物线型的方程可以通过改变自变量从而转化成类似于热方程的形式。随着转换后的时间变量的增加，方程的解变得平滑。欧拉-特里科米方程在 {{math|''x'' {{=}} 0}} 这条特征线上是抛物线形的。&lt;br /&gt;
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&lt;br /&gt;
&lt;br /&gt;
# {{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC'' &amp;gt; 0}} (''[[hyperbolic partial differential equation]]''): [[hyperbolic partial differential equation|hyperbolic]] equations retain any discontinuities of functions or derivatives in the initial data. An example is the [[wave equation]]. The motion of a fluid at supersonic speeds can be approximated with hyperbolic PDEs, and the Euler–Tricomi equation is hyperbolic where {{math|''x'' &amp;gt; 0}}.&lt;br /&gt;
&lt;br /&gt;
  (hyperbolic partial differential equation): hyperbolic equations retain any discontinuities of functions or derivatives in the initial data. An example is the wave equation. The motion of a fluid at supersonic speeds can be approximated with hyperbolic PDEs, and the Euler–Tricomi equation is hyperbolic where .&lt;br /&gt;
&lt;br /&gt;
{{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC'' &amp;gt; 0}} (双曲形偏微分方程)：双曲形方程在初始数据中保留了函数或导数的任何不连续性，波动方程就是其中的一个例子。超音速流体的运动可以用双曲形偏微分方程近似，其中欧拉-特里科米方程在 {{math|''x'' &amp;gt; 0}} 时是双曲型的。&lt;br /&gt;
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&lt;br /&gt;
&lt;br /&gt;
If there are {{mvar|n}} independent variables {{math|''x''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;, ''x''&amp;lt;sub&amp;gt;2 &amp;lt;/sub&amp;gt;,… ''x''&amp;lt;sub&amp;gt;''n''&amp;lt;/sub&amp;gt;}}, a general linear partial differential equation of second order has the form&lt;br /&gt;
&lt;br /&gt;
If there are  independent variables , a general linear partial differential equation of second order has the form&lt;br /&gt;
&lt;br /&gt;
如果存在 {{mvar|n}} 个自变量 {{math|''x''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;, ''x''&amp;lt;sub&amp;gt;2 &amp;lt;/sub&amp;gt;,… ''x''&amp;lt;sub&amp;gt;''n''&amp;lt;/sub&amp;gt;}}，一般二阶线性偏微分方程的形式是&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt;L u =\sum_{i=1}^n\sum_{j=1}^n a_{i,j} \frac{\partial^2 u}{\partial x_i \partial x_j} \quad \text{ plus lower-order terms} =0.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;L u =\sum_{i=1}^n\sum_{j=1}^n a_{i,j} \frac{\partial^2 u}{\partial x_i \partial x_j} \quad \text{ plus lower-order terms} =0.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The classification depends upon the signature of the eigenvalues of the coefficient matrix {{math|''a''&amp;lt;sub&amp;gt;''i'',''j''&amp;lt;/sub&amp;gt;}}.&lt;br /&gt;
&lt;br /&gt;
The classification depends upon the signature of the eigenvalues of the coefficient matrix .&lt;br /&gt;
&lt;br /&gt;
这种分类取决于系数矩阵本征值的符号（正负性）。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
# Elliptic: the eigenvalues are all positive or all negative.&lt;br /&gt;
&lt;br /&gt;
 Elliptic: the eigenvalues are all positive or all negative.&lt;br /&gt;
&lt;br /&gt;
椭圆形方程: 本征值全部为正或全部为负。&lt;br /&gt;
&lt;br /&gt;
# Parabolic: the eigenvalues are all positive or all negative, save one that is zero.&lt;br /&gt;
&lt;br /&gt;
 Parabolic: the eigenvalues are all positive or all negative, save one that is zero.&lt;br /&gt;
&lt;br /&gt;
抛物线形方程: 本征值全部为正或全部为负，除了一个为零。&lt;br /&gt;
&lt;br /&gt;
# Hyperbolic: there is only one negative eigenvalue and all the rest are positive, or there is only one positive eigenvalue and all the rest are negative.&lt;br /&gt;
&lt;br /&gt;
 Hyperbolic: there is only one negative eigenvalue and all the rest are positive, or there is only one positive eigenvalue and all the rest are negative.&lt;br /&gt;
&lt;br /&gt;
双曲形方程: 只有一个负特征值，其余的都是正特征值，或者只有一个正特征值，其余的都是负特征值。&lt;br /&gt;
&lt;br /&gt;
# Ultrahyperbolic: there is more than one positive eigenvalue and more than one negative eigenvalue, and there are no zero eigenvalues. There is only a limited theory for ultrahyperbolic equations (Courant and Hilbert, 1962).&lt;br /&gt;
&lt;br /&gt;
 Ultrahyperbolic: there is more than one positive eigenvalue and more than one negative eigenvalue, and there are no zero eigenvalues. There is only a limited theory for ultrahyperbolic equations (Courant and Hilbert, 1962).&lt;br /&gt;
&lt;br /&gt;
超双形方程: 存在多于一个正本征值和多于一个的负本征值，且不存在零本征值。对于超双曲方程，只存在一个有限理论(Courant 和 Hilbert，1962)。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==[[用户:Yuling|Yuling]]（[[用户讨论:Yuling|讨论]]） 我对于limited theory这个单词对应的相关理论不太了解。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
=== Systems of first-order equations and characteristic surfaces ===&lt;br /&gt;
一阶方程组和特征曲面&lt;br /&gt;
&lt;br /&gt;
The classification of partial differential equations can be extended to systems of first-order equations, where the unknown {{mvar|u}} is now a [[Euclidean vector|vector]] with {{mvar|m}} components, and the coefficient matrices {{mvar|A&amp;lt;sub&amp;gt;ν&amp;lt;/sub&amp;gt;}} are {{mvar|m}} by {{mvar|m}} matrices for {{math|''ν'' {{=}} 1, 2,… ''n''}}. The partial differential equation takes the form&lt;br /&gt;
&lt;br /&gt;
The classification of partial differential equations can be extended to systems of first-order equations, where the unknown  is now a vector with  components, and the coefficient matrices  are  by  matrices for  1, 2,… n}}. The partial differential equation takes the form&lt;br /&gt;
&lt;br /&gt;
偏微分方程组的分类可以推广到一阶方程组，其中未知量 {{mvar|u}} 是有 {{mvar|m}} 个分量的向量。对于 {{math|''ν'' {{=}} 1, 2,… ''n''}}，系数矩阵 {{mvar|A&amp;lt;sub&amp;gt;ν&amp;lt;/sub&amp;gt;}} 是 {{mvar|m}} × {{mvar|m}} 的矩阵。偏微分方程形式如下：&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt;Lu = \sum_{\nu=1}^{n} A_\nu \frac{\partial u}{\partial x_\nu} + B=0,&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;Lu = \sum_{\nu=1}^{n} A_\nu \frac{\partial u}{\partial x_\nu} + B=0,&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
where the coefficient matrices {{mvar|A&amp;lt;sub&amp;gt;ν&amp;lt;/sub&amp;gt;}} and the vector {{mvar|B}} may depend upon {{mvar|x}} and {{mvar|u}}. If a [[hypersurface]] {{mvar|S}} is given in the implicit form&lt;br /&gt;
&lt;br /&gt;
where the coefficient matrices  and the vector  may depend upon  and . If a hypersurface  is given in the implicit form&lt;br /&gt;
&lt;br /&gt;
其中系数矩阵 {{mvar|A&amp;lt;sub&amp;gt;ν&amp;lt;/sub&amp;gt;}} 和向量 {{mvar|B}} 可能依赖于 {{mvar|x}} 和 {{mvar|u}}。如果超曲面是以隐式形式给出的&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt;\varphi(x_1, x_2, \ldots x_n)=0,&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;\varphi(x_1, x_2, \ldots x_n)=0,&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
where {{mvar|φ}} has a non-zero gradient, then {{mvar|S}} is a '''characteristic surface''' for the operator {{mvar|L}} at a given point if the characteristic form vanishes:&lt;br /&gt;
&lt;br /&gt;
where  has a non-zero gradient, then  is a characteristic surface for the operator  at a given point if the characteristic form vanishes:&lt;br /&gt;
&lt;br /&gt;
其中存在一个非零的梯度，那么如果特征形式消失，则在给定点上算子的特征曲面形式如下:&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt;Q\left(\frac{\partial\varphi}{\partial x_1}, \ldots\frac{\partial\varphi}{\partial x_n}\right) =\det\left[\sum_{\nu=1}^nA_\nu \frac{\partial \varphi}{\partial x_\nu}\right]=0.\,&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;Q\left(\frac{\partial\varphi}{\partial x_1}, \ldots\frac{\partial\varphi}{\partial x_n}\right) =\det\left[\sum_{\nu=1}^nA_\nu \frac{\partial \varphi}{\partial x_\nu}\right]=0.\,&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The geometric interpretation of this condition is as follows: if data for {{mvar|u}} are prescribed on the surface {{mvar|S}}, then it may be possible to determine the normal derivative of {{mvar|u}} on {{mvar|S}} from the differential equation. If the data on {{mvar|S}} and the differential equation determine the normal derivative of {{mvar|u}} on {{mvar|S}}, then {{mvar|S}} is non-characteristic. If the data on {{mvar|S}} and the differential equation ''do not'' determine the normal derivative of {{mvar|u}} on {{mvar|S}}, then the surface is '''characteristic''', and the differential equation restricts the data on {{mvar|S}}: the differential equation is ''internal'' to {{mvar|S}}.&lt;br /&gt;
&lt;br /&gt;
The geometric interpretation of this condition is as follows: if data for  are prescribed on the surface , then it may be possible to determine the normal derivative of  on  from the differential equation. If the data on  and the differential equation determine the normal derivative of  on , then  is non-characteristic. If the data on  and the differential equation do not determine the normal derivative of  on , then the surface is characteristic, and the differential equation restricts the data on : the differential equation is internal to .&lt;br /&gt;
&lt;br /&gt;
这个条件的几何解释如下: 如果关于 {{mvar|u}} 的数据是在曲面 {{mvar|S}} 上规定的，那么就有可能依据微分方程确定曲面 {{mvar|S}} 上 {{mvar|u}} 的法向导数。如果曲面 {{mvar|S}} 上的数据和上面的微分方程能确定曲面 {{mvar|S}} 上 {{mvar|u}} 的法向导数，那么它就是非特征的。如果曲面 {{mvar|S}} 上的数据和上面的微分方程不能确定曲面 {{mvar|S}} 上 {{mvar|u}} 的法向导数，那么曲面是特征的，并且微分方程将数据限制在曲面 {{mvar|S}} 上：微分方程是在曲面 {{mvar|S}} 内部。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
# A first-order system {{math|''Lu'' {{=}} 0}} is ''elliptic'' if no surface is characteristic for {{mvar|L}}: the values of {{mvar|u}} on {{mvar|S}} and the differential equation always determine the normal derivative of {{mvar|u}} on {{mvar|S}}.&lt;br /&gt;
&lt;br /&gt;
 A first-order system  0}} is elliptic if no surface is characteristic for : the values of  on  and the differential equation always determine the normal derivative of  on .&lt;br /&gt;
&lt;br /&gt;
如果对于 {{mvar|L}} 没有曲面是特征的，则一阶系统 {{math|''Lu'' {{=}} 0}} 是椭圆形的：{{mvar|u}}在 {{mvar|S}} 的值和微分方程总能够决定 {{mvar|S}} 上 {{mvar|u}} 的法向导数。&lt;br /&gt;
&lt;br /&gt;
# A first-order system is ''hyperbolic'' at a point if there is a '''spacelike''' surface {{mvar|S}} with normal {{mvar|ξ}} at that point. This means that, given any non-trivial vector {{mvar|η}} orthogonal to {{mvar|ξ}}, and a scalar multiplier {{mvar|λ}}, the equation {{math|''Q''(''λξ'' + ''η'') {{=}} 0}} has {{mvar|m}} real roots {{math|''λ''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;, ''λ''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;,… ''λ''&amp;lt;sub&amp;gt;''m''&amp;lt;/sub&amp;gt;}}. The system is '''strictly hyperbolic''' if these roots are always distinct. The geometrical interpretation of this condition is as follows: the characteristic form {{math|''Q''(''ζ'') {{=}} 0}} defines a cone (the normal cone) with homogeneous coordinates ζ. In the hyperbolic case, this cone has {{mvar|m}} sheets, and the axis {{math|''ζ'' {{=}} ''λξ''}} runs inside these sheets: it does not intersect any of them. But when displaced from the origin by η, this axis intersects every sheet. In the elliptic case, the normal cone has no real sheets.&lt;br /&gt;
&lt;br /&gt;
 A first-order system is hyperbolic at a point if there is a spacelike surface  with normal  at that point. This means that, given any non-trivial vector  orthogonal to , and a scalar multiplier , the equation  0}} has  real roots . The system is strictly hyperbolic if these roots are always distinct. The geometrical interpretation of this condition is as follows: the characteristic form  0}} defines a cone (the normal cone) with homogeneous coordinates ζ. In the hyperbolic case, this cone has  sheets, and the axis  λξ}} runs inside these sheets: it does not intersect any of them. But when displaced from the origin by η, this axis intersects every sheet. In the elliptic case, the normal cone has no real sheets.&lt;br /&gt;
&lt;br /&gt;
如果在该点存在一个法向量为 {{mvar|ξ}}的 '''&amp;lt;font color=&amp;quot;#ff8000&amp;quot;&amp;gt;类空曲面 Spacclike Surface&amp;lt;/font&amp;gt; {{mvar|S}} ，则一阶系统在那一点是双曲的。这意味着，给定任意正交于 {{mvar|ξ}} 的非平凡向量 {{mvar|η}} 和一个标量乘子 {{mvar|λ}}，方程 {{math|''Q''(''λξ'' + ''η'') {{=}} 0}} 有 {{mvar|m}} 个实根 {{math|''λ''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;, ''λ''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;,… ''λ''&amp;lt;sub&amp;gt;''m''&amp;lt;/sub&amp;gt;}}。如果这些根始终不同，则该系统是严格双曲形的。这个条件的几何解释如下: 特征形式 {{math|''Q''(''ζ'') {{=}} 0}} 定义了一个具有齐次坐标 ζ的圆锥(法线圆锥)。在双曲形的情况下，这个圆锥体有 {{mvar|m}} 层，并且轴 {{math|''ζ'' {{=}} ''λξ''}} 在这些层中运动: 它不与任何一层相交。但是当从原点偏离η时，这条轴线与每一层都相交。在椭圆形的情况下，法向圆锥没有实层。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==[[用户:Yuling|Yuling]]（[[用户讨论:Yuling|讨论]]） sheet 这个单词也不很理解，我直译为了“层”&lt;br /&gt;
&lt;br /&gt;
=== Equations of mixed type ===&lt;br /&gt;
混合型方程&lt;br /&gt;
&lt;br /&gt;
If a PDE has coefficients that are not constant, it is possible that it will not belong to any of these categories but rather be of '''mixed type'''. A simple but important example is the [[Euler–Tricomi equation]]&lt;br /&gt;
&lt;br /&gt;
If a PDE has coefficients that are not constant, it is possible that it will not belong to any of these categories but rather be of mixed type. A simple but important example is the Euler–Tricomi equation&lt;br /&gt;
&lt;br /&gt;
如果偏微分方程的系数不是常数，那么它可能不属于这些类别中的任何一个，而是属于混合类型。一个简单但重要的例子是欧拉-特里科米方程&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt;u_{xx} = xu_{yy},&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;u_{xx} = xu_{yy},&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
which is called '''elliptic-hyperbolic''' because it is elliptic in the region {{math|''x'' &amp;lt; 0}}, hyperbolic in the region {{math|''x'' &amp;gt; 0}}, and degenerate parabolic on the line {{math|''x'' {{=}} 0}}.&lt;br /&gt;
&lt;br /&gt;
which is called elliptic-hyperbolic because it is elliptic in the region , hyperbolic in the region , and degenerate parabolic on the line  0}}.&lt;br /&gt;
&lt;br /&gt;
它在 {{math|''x'' &amp;lt; 0}} 的区域上是椭圆形，在 {{math|''x'' &amp;gt; 0}} 区域上是双曲形，在 {{math|''x'' {{=}} 0}}这条线上是退化为抛物线形，因此称之为椭圆-双曲型。&lt;br /&gt;
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&amp;lt;!--&lt;br /&gt;
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&amp;lt;!--&lt;br /&gt;
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&amp;lt;!--&lt;br /&gt;
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''fill in: Dirichlet and Neumann boundaries, hyperbolic/parabolic/elliptic separation of variables, [[Fourier analysis]], [[Green's function]]s ...--&amp;gt;&lt;br /&gt;
&lt;br /&gt;
fill in: Dirichlet and Neumann boundaries, hyperbolic/parabolic/elliptic separation of variables, Fourier analysis, Green's functions ...--&amp;gt;&lt;br /&gt;
&lt;br /&gt;
填写: Dirichlet 和 Neumann 边界，双曲 / 抛物线 / 椭圆分离变量法，傅立叶分析，Green 函数... --&lt;br /&gt;
&lt;br /&gt;
=== Infinite-order PDEs in quantum mechanics ===&lt;br /&gt;
量子力学中的无限阶偏微分方程&lt;br /&gt;
&lt;br /&gt;
In the [[phase space formulation]] of quantum mechanics,  one may consider the [[Method of quantum characteristics|quantum Hamilton's equations]] for trajectories of quantum particles. These equations are infinite-order PDEs. However, in the semiclassical expansion, one has a finite system of ODEs at any fixed order of [[Dirac constant|{{mvar|ħ}}]].  The evolution equation of the [[Wigner quasi-probability distribution|c]] is also an infinite-order PDE. The quantum trajectories are [[Method of quantum characteristics|quantum characteristics]], with the use of which one could calculate the evolution of the Wigner function.&lt;br /&gt;
&lt;br /&gt;
In the phase space formulation of quantum mechanics,  one may consider the quantum Hamilton's equations for trajectories of quantum particles. These equations are infinite-order PDEs. However, in the semiclassical expansion, one has a finite system of ODEs at any fixed order of Dirac constant|.  The evolution equation of the Wigner function is also an infinite-order PDE. The quantum trajectories are quantum characteristics, with the use of which one could calculate the evolution of the Wigner function.&lt;br /&gt;
&lt;br /&gt;
在量子力学中的相空间表述中，我们可以考虑用于求解量子粒子的轨迹的量子哈密顿的方程。这些方程是无限阶偏微分方程。然而，在半经典展开中，我们在给定[[Dirac constant|{{mvar|ħ}}]]阶数下有一个有限的的常微分方程组。'''&amp;lt;font color=&amp;quot;#ff8000&amp;quot;&amp;gt;维格纳函数  Wigner Function&amp;lt;/font&amp;gt;的演化方程也是一个无限阶偏微分方程。由于量子轨道的量子特性，所以它通常可以用来计算维格纳函数的演化。&lt;br /&gt;
&lt;br /&gt;
== Analytical solutions ==&lt;br /&gt;
解析解&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
===Separation of variables===&lt;br /&gt;
分离变量法&lt;br /&gt;
&lt;br /&gt;
{{main|Separable partial differential equation}}&lt;br /&gt;
&lt;br /&gt;
Linear PDEs can be reduced to systems of ordinary differential equations by the important technique of separation of variables. This technique rests on a characteristic of solutions to differential equations: if one can find any solution that solves the equation and satisfies the boundary conditions, then it is ''the'' solution (this also applies to ODEs). We assume as an [[ansatz]] that the dependence of a solution on the parameters space and time can be written as a product of terms that each depend on a single parameter, and then see if this can be made to solve the problem.&amp;lt;ref&amp;gt;{{cite book|last1=Gershenfeld|first1=Neil|title=The nature of mathematical modeling|date=2000|publisher=Cambridge Univ. Press|location=Cambridge|isbn=0521570956|page=27|edition=Reprinted (with corr.)}}&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
Linear PDEs can be reduced to systems of ordinary differential equations by the important technique of separation of variables. This technique rests on a characteristic of solutions to differential equations: if one can find any solution that solves the equation and satisfies the boundary conditions, then it is the solution (this also applies to ODEs). We assume as an ansatz that the dependence of a solution on the parameters space and time can be written as a product of terms that each depend on a single parameter, and then see if this can be made to solve the problem.&lt;br /&gt;
&lt;br /&gt;
线性偏微分方程组可以通过分离变量法这一重要方法来简化为常微分方程组。这种方法依赖于微分方程解的一个特征: 如果能找到任何一个满足方程和边界条件的解，那么这个解就是方程的解(这也适用于常微分方程)。我们假设解对参数空间和时间的依赖可以写成对它们每一项的依赖以及一个参数的乘积，然后再看看这是否可以用来解决这个问题。&lt;br /&gt;
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&lt;br /&gt;
&lt;br /&gt;
In the method of separation of variables, one reduces a PDE to a PDE in fewer variables, which is an ordinary differential equation if in one variable – these are in turn easier to solve.&lt;br /&gt;
&lt;br /&gt;
In the method of separation of variables, one reduces a PDE to a PDE in fewer variables, which is an ordinary differential equation if in one variable – these are in turn easier to solve.&lt;br /&gt;
&lt;br /&gt;
在分离变量法方法中，可以将偏微分方程简化为含有更少变量的偏微分方程，如果只有一个变量，那么就变成了一个'''&amp;lt;font color = &amp;quot;#ff8000&amp;quot;&amp;gt;常微分方程 Ordinary Differential Equation&amp;lt;/font&amp;gt;'''-- 反过来，这些方程也更容易求解。&lt;br /&gt;
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This is possible for simple PDEs, which are called [[separable partial differential equation]]s, and the domain is generally a rectangle (a product of intervals). Separable PDEs correspond to [[diagonal matrices]] – thinking of &amp;quot;the value for fixed {{mvar|x}}&amp;quot; as a coordinate, each coordinate can be understood separately.&lt;br /&gt;
&lt;br /&gt;
This is possible for simple PDEs, which are called separable partial differential equations, and the domain is generally a rectangle (a product of intervals). Separable PDEs correspond to diagonal matrices – thinking of &amp;quot;the value for fixed &amp;quot; as a coordinate, each coordinate can be understood separately.&lt;br /&gt;
&lt;br /&gt;
对于简单的偏微分方程(称为可分离偏微分方程)来说，这是可能的，而且方程通常定义在一个矩形区域(区间的乘积)上。可分离偏微分方程对应于对角线矩阵——以“固定值”为坐标，每个坐标可分开理解。&lt;br /&gt;
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This generalizes to the [[method of characteristics]], and is also used in [[integral transform]]s.&lt;br /&gt;
&lt;br /&gt;
This generalizes to the method of characteristics, and is also used in integral transforms.&lt;br /&gt;
&lt;br /&gt;
这种方法可以推广到特征曲线法，也可以用于积分变换。&lt;br /&gt;
&lt;br /&gt;
===Method of characteristics===&lt;br /&gt;
特征曲线法&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{{main|Method of characteristics}}&lt;br /&gt;
&lt;br /&gt;
In special cases, one can find characteristic curves on which the equation reduces to an ODE – changing coordinates in the domain to straighten these curves allows separation of variables, and is called the [[method of characteristics]].&lt;br /&gt;
&lt;br /&gt;
In special cases, one can find characteristic curves on which the equation reduces to an ODE – changing coordinates in the domain to straighten these curves allows separation of variables, and is called the method of characteristics.&lt;br /&gt;
&lt;br /&gt;
在特殊情况下，可以找到一些特征曲线，在这些曲线上方程可以变成一个常微分方程——意味着改变坐标从而使这些曲线变直从而达到分离变量的目的，这就是所谓的特征曲线法。&lt;br /&gt;
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More generally, one may find characteristic surfaces.&lt;br /&gt;
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More generally, one may find characteristic surfaces.&lt;br /&gt;
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更一般地说，人们可能会找到特征表面。&lt;br /&gt;
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===Integral transform===&lt;br /&gt;
积分变换&lt;br /&gt;
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An [[integral transform]] may transform the PDE to a simpler one, in particular, a separable PDE. This corresponds to diagonalizing an operator.&lt;br /&gt;
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An integral transform may transform the PDE to a simpler one, in particular, a separable PDE. This corresponds to diagonalizing an operator.&lt;br /&gt;
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积分变换可以将偏微分方程转换为更简单的偏微分方程，特别是可分离的偏微分方程。这对应于对角化算符。&lt;br /&gt;
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An important example of this is [[Fourier analysis]], which diagonalizes the heat equation using the [[eigenbasis]] of sinusoidal waves.&lt;br /&gt;
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An important example of this is Fourier analysis, which diagonalizes the heat equation using the eigenbasis of sinusoidal waves.&lt;br /&gt;
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这方面的一个重要例子是'''&amp;lt;font color = &amp;quot;#ff8000&amp;quot;&amp;gt;傅里叶分析  Fourier Analysis&amp;lt;/font&amp;gt;'''，它使用正弦波的特征基来对角化热方程。&lt;br /&gt;
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If the domain is finite or periodic, an infinite sum of solutions such as a [[Fourier series]] is appropriate, but an integral of solutions such as a [[Fourier integral]] is generally required for infinite domains. The solution for a point source for the heat equation given above is an example of the use of a Fourier integral.&lt;br /&gt;
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If the domain is finite or periodic, an infinite sum of solutions such as a Fourier series is appropriate, but an integral of solutions such as a Fourier integral is generally required for infinite domains. The solution for a point source for the heat equation given above is an example of the use of a Fourier integral.&lt;br /&gt;
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如果区域是有限的或周期性的，那么解为无限和的形式是恰当的，例如傅里叶级数，但是一个解的积分，例如傅立叶积分，一般是在无限区域上的。上面给出的热传导方程的点源解法就是使用傅里叶积分的一个例子。&lt;br /&gt;
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===Change of variables===&lt;br /&gt;
变量代换&lt;br /&gt;
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Often a PDE can be reduced to a simpler form with a known solution by a suitable [[Change of variables (PDE)|change of variables]].  For example, the [[Black–Scholes equation#Derivation|Black–Scholes]] PDE&lt;br /&gt;
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Often a PDE can be reduced to a simpler form with a known solution by a suitable change of variables.  For example, the Black–Scholes PDE&lt;br /&gt;
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偏微分方程通常可以通过变量的适当变化，用已知的解简化为更简单的形式。例如，布莱克-舒尔斯偏微分方程&lt;br /&gt;
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:&amp;lt;math&amp;gt; \frac{\partial V}{\partial t} + \tfrac{1}{2}\sigma^2 S^2\frac{\partial^2 V}{\partial S^2} + rS\frac{\partial V}{\partial S} - rV = 0 &amp;lt;/math&amp;gt;&lt;br /&gt;
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&amp;lt;math&amp;gt; \frac{\partial V}{\partial t} + \tfrac{1}{2}\sigma^2 S^2\frac{\partial^2 V}{\partial S^2} + rS\frac{\partial V}{\partial S} - rV = 0 &amp;lt;/math&amp;gt;&lt;br /&gt;
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is reducible to the [[heat equation]]&lt;br /&gt;
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is reducible to the heat equation&lt;br /&gt;
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可以简化为热传导方程&lt;br /&gt;
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:&amp;lt;math&amp;gt; \frac{\partial u}{\partial \tau} = \frac{\partial^2 u}{\partial x^2}&amp;lt;/math&amp;gt;&lt;br /&gt;
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&amp;lt;math&amp;gt; \frac{\partial u}{\partial \tau} = \frac{\partial^2 u}{\partial x^2}&amp;lt;/math&amp;gt;&lt;br /&gt;
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by the change of variables (for complete details see {{webarchive |url=https://web.archive.org/web/20080411030405/http://www.math.unl.edu/~sdunbar1/Teaching/MathematicalFinance/Lessons/BlackScholes/Solution/solution.shtml |date=April 11, 2008 |title=Solution of the Black Scholes Equation }})&lt;br /&gt;
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by the change of variables (for complete details see )&lt;br /&gt;
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通过变量替换(完整的细节见)&lt;br /&gt;
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:&amp;lt;math&amp;gt;\begin{align}&lt;br /&gt;
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V(S,t) &amp;amp;= K v(x,\tau),\\[5px]&lt;br /&gt;
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x &amp;amp;= \ln\left(\tfrac{S}{K} \right),\\[5px]&lt;br /&gt;
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\tau &amp;amp;= \tfrac{1}{2} \sigma^2 (T - t),\\[5px]&lt;br /&gt;
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v(x,\tau)&amp;amp;=e^{-\alpha x-\beta\tau} u(x,\tau).&lt;br /&gt;
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\end{align}&amp;lt;/math&amp;gt;&lt;br /&gt;
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===Fundamental solution===&lt;br /&gt;
基本解&lt;br /&gt;
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{{main|Fundamental solution}}&lt;br /&gt;
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Inhomogeneous equations can often be solved (for constant coefficient PDEs, always be solved) by finding the [[fundamental solution]] (the solution for a point source), then taking the [[convolution]] with the boundary conditions to get the solution.&lt;br /&gt;
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Inhomogeneous equations can often be solved (for constant coefficient PDEs, always be solved) by finding the fundamental solution (the solution for a point source), then taking the convolution with the boundary conditions to get the solution.&lt;br /&gt;
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非齐次方程(常系数偏微分方程)一般是通过先求出基本解(点源的解) ，然后利用带边界条件的卷积来求解。&lt;br /&gt;
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This is analogous in [[signal processing]] to understanding a filter by its [[impulse response]].&lt;br /&gt;
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This is analogous in signal processing to understanding a filter by its impulse response.&lt;br /&gt;
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这类似于在信号处理中通过滤波器的脉冲响应来理解滤波器。&lt;br /&gt;
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===Superposition principle===&lt;br /&gt;
叠加原理&lt;br /&gt;
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{{further| Superposition principle }}&lt;br /&gt;
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The superposition principle applies to any linear system, including linear systems of PDEs. A common visualization of this concept is the interaction of two waves in phase being combined to result in a greater amplitude, for example {{math|sin ''x'' + sin ''x'' {{=}} 2 sin ''x''}}. The same principle can be observed in PDEs where the solutions may be real or complex and additive. [[Superposition principle|superposition]]&lt;br /&gt;
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The superposition principle applies to any linear system, including linear systems of PDEs. A common visualization of this concept is the interaction of two waves in phase being combined to result in a greater amplitude, for example  2 sin x}}. The same principle can be observed in PDEs where the solutions may be real or complex and additive. superposition&lt;br /&gt;
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'''&amp;lt;font color = &amp;quot;#ff8000&amp;quot;&amp;gt;叠加原理 Superposition Principle&amp;lt;/font&amp;gt;适用于任何线性系统，包括偏微分方程的线性系统。这个概念的一个常见的可视化是两个同相位的波相互作用结合在一起会产生更大的振幅，例如 {{math|sin ''x'' + sin ''x'' {{=}} 2 sin ''x''}}。在偏微分方程中也可以观察到同样的原理，其中的解可能是真实的或复杂的和可加的。叠加&lt;br /&gt;
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If {{math|''u''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;}} and {{math|''u''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;}} are solutions of linear PDE in some function space {{mvar|R}}, then {{math|''u'' {{=}} ''c''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;''u''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; + ''c''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;''u''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;}} with any constants {{math|''c''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;}} and {{math|''c''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;}} are also a solution of that PDE in the same function space.&lt;br /&gt;
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If  and  are solutions of linear PDE in some function space , then  c&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;u&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; + c&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;u&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;}} with any constants  and  are also a solution of that PDE in the same function space.&lt;br /&gt;
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若线性偏微分方程在某个函数空间{{mvar|R}}中有解{{math|''u''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;}} 和 {{math|''u''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;}}，则{{math|''u'' {{=}} ''c''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;''u''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; + ''c''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;''u''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;}}也是该偏微分方程在同一函数空间中的解，其中{{math|''c''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;}} 和 {{math|''c''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;}} 是任意常数。&lt;br /&gt;
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===Methods for non-linear equations===&lt;br /&gt;
非线性方程的求解方法&lt;br /&gt;
{{see also|nonlinear partial differential equation}}&lt;br /&gt;
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There are no generally applicable methods to solve nonlinear PDEs. Still, existence and uniqueness results (such as the [[Cauchy–Kowalevski theorem]]) are often possible, as are proofs of important qualitative and quantitative properties of solutions (getting these results is a major part of [[mathematical analysis|analysis]]). Computational solution to the nonlinear PDEs, the [[split-step method]], exist for specific equations like [[nonlinear Schrödinger equation]].&lt;br /&gt;
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There are no generally applicable methods to solve nonlinear PDEs. Still, existence and uniqueness results (such as the Cauchy–Kowalevski theorem) are often possible, as are proofs of important qualitative and quantitative properties of solutions (getting these results is a major part of analysis). Computational solution to the nonlinear PDEs, the split-step method, exist for specific equations like nonlinear Schrödinger equation.&lt;br /&gt;
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对于非线性偏微分方程，目前还没有普遍适用的求解方法。然而，通常是可能知道解的存在性和唯一性(如柯西-科瓦列夫斯基定理)，也是可能得到解的重要定性和定量性质的证明(得到这些结果是分析的主要部分)。非线性偏微分方程的计算解，即分步法，对一些特定的方程适用，比如非线性'''&amp;lt;font color=&amp;quot;#ff8000&amp;quot;&amp;gt;薛定谔方程 Schrödinger equation&amp;lt;/font&amp;gt;'''。&lt;br /&gt;
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Nevertheless, some techniques can be used for several types of equations. The [[h-principle|{{mvar|h}}-principle]] is the most powerful method to solve [[Underdetermined system|underdetermined]] equations. The [[Riquier–Janet theory]] is an effective method for obtaining information about many analytic [[Overdetermined system|overdetermined]] systems.&lt;br /&gt;
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Nevertheless, some techniques can be used for several types of equations. The -principle is the most powerful method to solve underdetermined equations. The Riquier–Janet theory is an effective method for obtaining information about many analytic overdetermined systems.&lt;br /&gt;
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然而，一些技巧可以用于几种类型的方程。h-原理是求解欠定方程最有效的方法。里基尔-珍妮特理论是一种可以获得许多解析超定系统信息的有效方法。&lt;br /&gt;
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The [[method of characteristics]] can be used in some very special cases to solve partial differential equations.&lt;br /&gt;
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The method of characteristics can be used in some very special cases to solve partial differential equations.&lt;br /&gt;
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特征线法可用于求解某些特殊情况下的偏微分方程。&lt;br /&gt;
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In some cases, a PDE can be solved via [[perturbation analysis]] in which the solution is considered to be a correction to an equation with a known solution. Alternatives are [[numerical analysis]] techniques from simple [[finite difference]] schemes to the more mature [[multigrid]] and [[finite element method]]s. Many interesting problems in science and engineering are solved in this way using [[computer]]s, sometimes high performance [[supercomputer]]s.&lt;br /&gt;
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In some cases, a PDE can be solved via perturbation analysis in which the solution is considered to be a correction to an equation with a known solution. Alternatives are numerical analysis techniques from simple finite difference schemes to the more mature multigrid and finite element methods. Many interesting problems in science and engineering are solved in this way using computers, sometimes high performance supercomputers.&lt;br /&gt;
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在某些情况下，偏微分方程可以通过扰动分析来求解。在扰动分析中，通常是求解将具有已知解的方程修正后的新得到方程。可供选择的数值分析技术从简单的差分格式到更成熟的多重网格和有限元方法。许多有趣的科学和工程问题都是在计算机上用这种方法解决的，有时是高性能超级计算机。&lt;br /&gt;
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===Lie group method===&lt;br /&gt;
李群方法&lt;br /&gt;
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From 1870 [[Sophus Lie]]'s work put the theory of differential equations on a more satisfactory foundation. He showed that the integration theories of the older mathematicians can, by the introduction of what are now called [[Lie group]]s, be referred, to a common source; and that ordinary differential equations which admit the same [[infinitesimal transformation]]s present comparable difficulties of integration. He also emphasized the subject of [[contact transformation|transformations of contact]].&lt;br /&gt;
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From 1870 Sophus Lie's work put the theory of differential equations on a more satisfactory foundation. He showed that the integration theories of the older mathematicians can, by the introduction of what are now called Lie groups, be referred, to a common source; and that ordinary differential equations which admit the same infinitesimal transformations present comparable difficulties of integration. He also emphasized the subject of transformations of contact.&lt;br /&gt;
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从1870年起，索弗斯·李的工作为微分方程理论奠定了一个较为令人满意的基础。他指出，通过引入现在所谓的李群，老一辈数学家的积分理论可以引用到一个共同的来源; 承认相同的无穷小变换的常微分方程在积分方面存在相当的困难。他还强调了接触的转变这一主题。&lt;br /&gt;
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==[[用户:Yuling|Yuling]]（[[用户讨论:Yuling|讨论]]）这句话“He also emphasized the subject of transformations of contact.”中的transformations of contact翻译的不太好。&lt;br /&gt;
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A general approach to solving PDEs uses the symmetry property of differential equations, the continuous [[infinitesimal transformation]]s of solutions to solutions ([[Lie theory]]). Continuous [[group theory]], [[Lie algebras]] and [[differential geometry]] are used to understand the structure of linear and nonlinear partial differential equations for generating integrable equations, to find its [[Lax pair]]s, recursion operators, [[Bäcklund transform]] and finally finding exact analytic solutions to the PDE.&lt;br /&gt;
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A general approach to solving PDEs uses the symmetry property of differential equations, the continuous infinitesimal transformations of solutions to solutions (Lie theory). Continuous group theory, Lie algebras and differential geometry are used to understand the structure of linear and nonlinear partial differential equations for generating integrable equations, to find its Lax pairs, recursion operators, Bäcklund transform and finally finding exact analytic solutions to the PDE.&lt;br /&gt;
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求解偏微分方程的一般方法是利用微分方程的对称性，即解到解的连续无穷小变换(李理论)。连续群论、李代数和微分几何理论被用来理解生成可积方程的线性和非线性偏微分方程的结构，找到它的Lax对、递归算子、 贝克伦德变换，最后找到偏微分方程的精确解析解。&lt;br /&gt;
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Symmetry methods have been recognized to study differential equations arising in mathematics, physics, engineering, and many other disciplines.&lt;br /&gt;
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Symmetry methods have been recognized to study differential equations arising in mathematics, physics, engineering, and many other disciplines.&lt;br /&gt;
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对称方法已被公认可以用于研究出现在数学，物理，工程和许多其他学科的微分方程。&lt;br /&gt;
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===Semianalytical methods===&lt;br /&gt;
半解析方法&lt;br /&gt;
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The [[Adomian decomposition method]], the [[Aleksandr Lyapunov|Lyapunov]] artificial small parameter method, and He's [[homotopy perturbation method]] are all special cases of the more general [[homotopy analysis method]]. These are series expansion methods, and except for the Lyapunov method, are independent of small physical parameters as compared to the well known [[perturbation theory]], thus giving these methods greater flexibility and solution generality.&lt;br /&gt;
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The Adomian decomposition method, the Lyapunov artificial small parameter method, and He's homotopy perturbation method are all special cases of the more general homotopy analysis method. These are series expansion methods, and except for the Lyapunov method, are independent of small physical parameters as compared to the well known perturbation theory, thus giving these methods greater flexibility and solution generality.&lt;br /&gt;
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阿多米安分解法、李雅普诺夫人工小参数方法和何同伦摄动方法都是更一般的同伦分析方法的特殊情况。除了李雅普诺夫方法之外，这些都是级数展开方法，与为人熟知的摄动理论方法相比，它们与小的物理参数无关，因此这些方法具有更大的灵活性和解的通用性。&lt;br /&gt;
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== Numerical solutions ==&lt;br /&gt;
数值解&lt;br /&gt;
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The three most widely used [[Numerical partial differential equations|numerical methods to solve PDEs]] are the [[finite element analysis|finite element method]] (FEM), [[finite volume method]]s (FVM) and [[finite difference method]]s (FDM), as well other kind of methods called [[Meshfree methods]], which were made to solve problems where the before mentioned methods are limited. The FEM has a prominent position among these methods and especially its exceptionally efficient higher-order version [[hp-FEM]]. Other hybrid versions of FEM and Meshfree methods include the generalized finite element method (GFEM), [[extended finite element method]] (XFEM), [[Spectral element method|spectral finite element method]] (SFEM), [[Meshfree methods|meshfree finite element method]], [[Discontinuous Galerkin Method|discontinuous Galerkin finite element method]] (DGFEM), [[Element-Free Galerkin Method]] (EFGM), [[Interpolating Element-Free Galerkin Method]] (IEFGM), etc.&lt;br /&gt;
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The three most widely used numerical methods to solve PDEs are the finite element method (FEM), finite volume methods (FVM) and finite difference methods (FDM), as well other kind of methods called Meshfree methods, which were made to solve problems where the before mentioned methods are limited. The FEM has a prominent position among these methods and especially its exceptionally efficient higher-order version hp-FEM. Other hybrid versions of FEM and Meshfree methods include the generalized finite element method (GFEM), extended finite element method (XFEM), spectral finite element method (SFEM), meshfree finite element method, discontinuous Galerkin finite element method (DGFEM), Element-Free Galerkin Method (EFGM), Interpolating Element-Free Galerkin Method (IEFGM), etc.&lt;br /&gt;
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求解偏微分方程最常用的三种数值方法是有限元分析法、有限体积法和有限差分法，以及其他一些称为无网格法的方法。这些方法用于解决前面提到的方法受到的限制。在这些方法中，有限元方法，尤其是高效的高阶有限元方法，占有重要地位。其他有限元法和无网格法的混合形式包括广义有限元分析法(GFEM)、扩展有限元分析法(XFEM)、谱有限元分析法(SFEM)、无网格有限元分析法(DGFEM)、间断伽辽金有限元分析法(DGFEM)、无网格伽辽金法(EFGM)、插值无网格伽辽金法(IEFGM)等。&lt;br /&gt;
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=== Finite element method ===&lt;br /&gt;
有限元分析法&lt;br /&gt;
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{{main|Finite element method}}&lt;br /&gt;
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The finite element method (FEM) (its practical application often known as finite element analysis (FEA)) is a numerical technique for finding approximate solutions of partial differential equations (PDE) as well as of integral equations. The solution approach is based either on eliminating the differential equation completely (steady state problems), or rendering the PDE into an approximating system of ordinary differential equations, which are then numerically integrated using standard techniques such as Euler's method, Runge–Kutta, etc.&lt;br /&gt;
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The finite element method (FEM) (its practical application often known as finite element analysis (FEA)) is a numerical technique for finding approximate solutions of partial differential equations (PDE) as well as of integral equations. The solution approach is based either on eliminating the differential equation completely (steady state problems), or rendering the PDE into an approximating system of ordinary differential equations, which are then numerically integrated using standard techniques such as Euler's method, Runge–Kutta, etc.&lt;br /&gt;
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'''&amp;lt;font color = &amp;quot;#ff8000&amp;quot;&amp;gt;有限元分析法 Finite Element Method&amp;lt;/font&amp;gt;''' ((其实际应用通常被称为有限元分析(FEA))是一种寻找偏微分方程(PDE)和积分方程近似解的数值技术。这种求解方法要么基于完全消除微分方程(稳态问题) ，要么将偏微分方程转化为常微分方程的近似系统，然后使用标准技术进行数值积分，如欧拉方法、 Runge-Kutta 等。&lt;br /&gt;
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===Finite difference method===&lt;br /&gt;
有限差分法&lt;br /&gt;
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{{main|Finite difference method}}&lt;br /&gt;
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Finite-difference methods are numerical methods for approximating the solutions to differential equations using [[finite difference]] equations to approximate derivatives.&lt;br /&gt;
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Finite-difference methods are numerical methods for approximating the solutions to differential equations using finite difference equations to approximate derivatives.&lt;br /&gt;
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有限差分法是一种数值方法，用差分方程近似微分方程的解。&lt;br /&gt;
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=== Finite volume method ===&lt;br /&gt;
有限体积法&lt;br /&gt;
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{{main|Finite volume method}}&lt;br /&gt;
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Similar to the finite difference method or finite element method, values are calculated at discrete places on a meshed geometry. &amp;quot;Finite volume&amp;quot; refers to the small volume surrounding each node point on a mesh. In the finite volume method, surface integrals in a partial differential equation that contain a divergence term are converted to volume integrals, using the [[divergence theorem]]. These terms are then evaluated as fluxes at the surfaces of each finite volume. Because the flux entering a given volume is identical to that leaving the adjacent volume, these methods conserve mass by design.&lt;br /&gt;
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Similar to the finite difference method or finite element method, values are calculated at discrete places on a meshed geometry. &amp;quot;Finite volume&amp;quot; refers to the small volume surrounding each node point on a mesh. In the finite volume method, surface integrals in a partial differential equation that contain a divergence term are converted to volume integrals, using the divergence theorem. These terms are then evaluated as fluxes at the surfaces of each finite volume. Because the flux entering a given volume is identical to that leaving the adjacent volume, these methods conserve mass by design.&lt;br /&gt;
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类似于有限差分法或有限元分析，函数值是在网状几何体上的离散位置进行计算的。“有限体积”是指网格上每个节点周围的小体积。在有限体积法中，偏微分方程中含有散度项的面积分用散度定理积分转换成体积分。然后将这些项用于估算每个有限体积表面上的通量。由于进入给定体积的通量与转移到相邻体积元的通量相同，所以这些方法在设计上保证了质量守恒。&lt;br /&gt;
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==See also==&lt;br /&gt;
请参阅&lt;br /&gt;
* [[Dirichlet boundary condition]]&lt;br /&gt;
狄利克雷边界条件&lt;br /&gt;
* [[Jet bundle]]&lt;br /&gt;
射流丛&lt;br /&gt;
* [[Laplace transform applied to differential equations]]&lt;br /&gt;
微分方程中的拉普拉斯变换&lt;br /&gt;
* [[List of dynamical systems and differential equations topics]]&lt;br /&gt;
动力学系统和微分方程的列表&lt;br /&gt;
* [[Matrix differential equation]]&lt;br /&gt;
矩阵微分方程&lt;br /&gt;
* [[Neumann boundary condition]]&lt;br /&gt;
诺伊曼边界条件&lt;br /&gt;
* [[Numerical partial differential equations]]&lt;br /&gt;
数值偏微分方程&lt;br /&gt;
* [[Partial differential algebraic equation]]&lt;br /&gt;
偏微分代数方程&lt;br /&gt;
* [[Recurrence relation]]&lt;br /&gt;
递推关系&lt;br /&gt;
* [[Robin boundary condition]]&lt;br /&gt;
罗宾边界条件&lt;br /&gt;
* [[Stochastic processes and boundary value problems]]&lt;br /&gt;
随机过程和边值问题&lt;br /&gt;
&lt;br /&gt;
== The energy method ==&lt;br /&gt;
能量法&lt;br /&gt;
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The energy method is a mathematical procedure that can be used to verify well-posedness of initial-boundary-value-problems.&amp;lt;ref&amp;gt;{{cite book |title=High Order Difference Methods for Time Dependent PDE&lt;br /&gt;
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The energy method is a mathematical procedure that can be used to verify well-posedness of initial-boundary-value-problems.&amp;lt;ref&amp;gt;{{cite book |title=High Order Difference Methods for Time Dependent PDE&lt;br /&gt;
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能量法是验证初边值问题适定性的一种数学方法。 时变偏微分方程的高阶差分方法&lt;br /&gt;
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|first=Bertil|last=Gustafsson|publisher=Springer|year=2008|isbn=978-3-540-74992-9|doi=10.1007/978-3-540-74993-6}}&amp;lt;/ref&amp;gt; In the following example the energy method is used to decide where and which boundary conditions should be imposed such that the resulting IBVP is well-posed. Consider the one-dimensional hyperbolic PDE given by&lt;br /&gt;
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|first=Bertil|last=Gustafsson|publisher=Springer|year=2008|isbn=978-3-540-74992-9|doi=10.1007/978-3-540-74993-6}}&amp;lt;/ref&amp;gt; In the following example the energy method is used to decide where and which boundary conditions should be imposed such that the resulting IBVP is well-posed. Consider the one-dimensional hyperbolic PDE given by&lt;br /&gt;
&lt;br /&gt;
| first Bertil | last Gustafsson | publisher | Springer | year 2008 | isbn 978-3-540-74992-9 | doi 10.1007 / 978-3-540-74993-6} / ref 在下面的例子中，使用能量方法来决定应该施加哪些边界条件，使得得到的 IBVP适定。考虑一维双曲偏微分方程&lt;br /&gt;
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: &amp;lt;math&amp;gt;\frac{\partial u}{\partial t} + \alpha \frac{\partial u}{\partial x} = 0, \quad x \in [a,b], \operatorname t &amp;gt; 0,&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;\frac{\partial u}{\partial t} + \alpha \frac{\partial u}{\partial x} = 0, \quad x \in [a,b], \operatorname t &amp;gt; 0,&amp;lt;/math&amp;gt;&lt;br /&gt;
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where &amp;lt;math&amp;gt;\alpha \neq 0&amp;lt;/math&amp;gt; is a constant and &amp;lt;math&amp;gt;u(x,t)&amp;lt;/math&amp;gt; is an unknown function with initial condition &amp;lt;math&amp;gt;u(x,0) = f(x)&amp;lt;/math&amp;gt;. Multiplying with &amp;lt;math&amp;gt;u&amp;lt;/math&amp;gt; and integrating over the domain gives&lt;br /&gt;
&lt;br /&gt;
where &amp;lt;math&amp;gt;\alpha \neq 0&amp;lt;/math&amp;gt; is a constant and &amp;lt;math&amp;gt;u(x,t)&amp;lt;/math&amp;gt; is an unknown function with initial condition &amp;lt;math&amp;gt;u(x,0) = f(x)&amp;lt;/math&amp;gt;. Multiplying with &amp;lt;math&amp;gt;u&amp;lt;/math&amp;gt; and integrating over the domain gives&lt;br /&gt;
&lt;br /&gt;
其中 &amp;lt;math&amp;gt;\alpha \neq 0&amp;lt;/math&amp;gt; 是常数，并且 &amp;lt;math&amp;gt;u(x,t)&amp;lt;/math&amp;gt; 是未知函数，初始条件是 &amp;lt;math&amp;gt;u(x,0) = f(x)&amp;lt;/math&amp;gt;。乘以 &amp;lt;math&amp;gt;u&amp;lt;/math&amp;gt; 并在域上进行积分。&lt;br /&gt;
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: &amp;lt;math&amp;gt;\int_a^b u \frac{\partial u}{\partial t} \operatorname dx + \alpha \int _a ^b u \frac{\partial u}{\partial x} \operatorname dx = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;\int_a^b u \frac{\partial u}{\partial t} \operatorname dx + \alpha \int _a ^b u \frac{\partial u}{\partial x} \operatorname dx = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
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Using that&lt;br /&gt;
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Using that&lt;br /&gt;
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利用这一点&lt;br /&gt;
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: &amp;lt;math&amp;gt;\int _a ^b u \frac{\partial u}{\partial t} \operatorname dx = \frac{1}{2} \frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 \quad \text{and} \quad \int _a ^b u \frac{\partial u}{\partial x} \operatorname dx = \frac{1}{2} u(b,t)^2 - \frac{1}{2} u(a,t)^2,.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;\int _a ^b u \frac{\partial u}{\partial t} \operatorname dx = \frac{1}{2} \frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 \quad \text{and} \quad \int _a ^b u \frac{\partial u}{\partial x} \operatorname dx = \frac{1}{2} u(b,t)^2 - \frac{1}{2} u(a,t)^2,.&amp;lt;/math&amp;gt;&lt;br /&gt;
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where integration by parts has been used for the second relationship, we get&lt;br /&gt;
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where integration by parts has been used for the second relationship, we get&lt;br /&gt;
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第二个关系中采用了分部积分法，我们可以得到&lt;br /&gt;
&lt;br /&gt;
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: &amp;lt;math&amp;gt;\frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 + \alpha u(b,t)^2 - \alpha u(a,t)^2 = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;\frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 + \alpha u(b,t)^2 - \alpha u(a,t)^2 = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
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Here &amp;lt;math&amp;gt;\vert \vert \cdot \vert \vert&amp;lt;/math&amp;gt; denotes the standard L2-norm.&lt;br /&gt;
&lt;br /&gt;
Here &amp;lt;math&amp;gt;\vert \vert \cdot \vert \vert&amp;lt;/math&amp;gt; denotes the standard L2-norm.&lt;br /&gt;
&lt;br /&gt;
在这里，&amp;lt;math&amp;gt;\vert \vert \cdot \vert \vert&amp;lt;/math&amp;gt; 表示标准的 L2-正则。&lt;br /&gt;
&lt;br /&gt;
For well-posedness we require that the energy of the solution is non-increasing, i.e. that &amp;lt;math&amp;gt;\frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 \leq 0&amp;lt;/math&amp;gt;, which is achieved by specifying &amp;lt;math&amp;gt;u&amp;lt;/math&amp;gt; at &amp;lt;math&amp;gt;x = a&amp;lt;/math&amp;gt; if &amp;lt;math&amp;gt;\alpha &amp;gt; 0&amp;lt;/math&amp;gt; and at &amp;lt;math&amp;gt;x = b&amp;lt;/math&amp;gt; if &amp;lt;math&amp;gt;\alpha &amp;lt; 0&amp;lt;/math&amp;gt;. This corresponds to only imposing boundary conditions at the inflow. Note that well-posedness allows for growth in terms of data (initial and boundary) and thus it is sufficient to show that &amp;lt;math&amp;gt;\frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 \leq 0&amp;lt;/math&amp;gt; holds when all data is set to zero.&lt;br /&gt;
&lt;br /&gt;
For well-posedness we require that the energy of the solution is non-increasing, i.e. that &amp;lt;math&amp;gt;\frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 \leq 0&amp;lt;/math&amp;gt;, which is achieved by specifying &amp;lt;math&amp;gt;u&amp;lt;/math&amp;gt; at &amp;lt;math&amp;gt;x = a&amp;lt;/math&amp;gt; if &amp;lt;math&amp;gt;\alpha &amp;gt; 0&amp;lt;/math&amp;gt; and at &amp;lt;math&amp;gt;x = b&amp;lt;/math&amp;gt; if &amp;lt;math&amp;gt;\alpha &amp;lt; 0&amp;lt;/math&amp;gt;. This corresponds to only imposing boundary conditions at the inflow. Note that well-posedness allows for growth in terms of data (initial and boundary) and thus it is sufficient to show that &amp;lt;math&amp;gt;\frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 \leq 0&amp;lt;/math&amp;gt; holds when all data is set to zero.&lt;br /&gt;
&lt;br /&gt;
对于适定性，我们要解的能量是不增加的，即 &amp;lt;math&amp;gt;\frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 \leq 0&amp;lt;/math&amp;gt; ，这种关系可以通过在&amp;lt;math&amp;gt;x = a&amp;lt;/math&amp;gt;处 （如果 &amp;lt;math&amp;gt;\alpha &amp;gt; 0&amp;lt;/math&amp;gt;） 以及 &amp;lt;math&amp;gt;x = b&amp;lt;/math&amp;gt;处 （如果 &amp;lt;math&amp;gt;\alpha &amp;lt; 0&amp;lt;/math&amp;gt;）指定&amp;lt;math&amp;gt;u&amp;lt;/math&amp;gt;的值来实现。这只相当于在入流处附加边界条件。注意，适定性允许在数据(初始和边界)上的增长，因此它足以表明当所有数据设置为零时应有 &amp;lt;math&amp;gt;\frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 \leq 0&amp;lt;/math&amp;gt;。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==[[用户:Yuling|Yuling]]（[[用户讨论:Yuling|讨论]]）“This corresponds to only imposing boundary conditions at the inflow.” 这句话中的inflow不是很理解&lt;br /&gt;
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==Notes==&lt;br /&gt;
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{{Reflist}}&lt;br /&gt;
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* {{cite book |title=High Order Difference Methods for Time Dependent PDE&lt;br /&gt;
&lt;br /&gt;
|first=Bertil|last=Gustafsson|publisher=Springer|year=2008|isbn=978-3-540-74992-9|doi=10.1007/978-3-540-74993-6}}&lt;br /&gt;
&lt;br /&gt;
|first=Bertil|last=Gustafsson|publisher=Springer|year=2008|isbn=978-3-540-74992-9|doi=10.1007/978-3-540-74993-6}}&lt;br /&gt;
&lt;br /&gt;
| first Bertil | last Gustafsson | Springer | year 2008 | isbn 978-3-540-74992-9 | doi 10.1007 / 978-3-540-74993-6}&lt;br /&gt;
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{{refend}}&lt;br /&gt;
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== Further reading ==&lt;br /&gt;
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* {{Cite journal|last=Cajori|first=Florian|authorlink=Florian Cajori|year=1928|title=The Early History of Partial Differential Equations and of Partial Differentiation and Integration|url=http://www.math.harvard.edu/archive/21a_fall_14/exhibits/cajori/cajori.pdf|journal=The American Mathematical Monthly|volume=35|issue=9|pages=459–467|doi=10.2307/2298771|access-date=2016-05-15|archive-url=https://web.archive.org/web/20181123102253/http://www.math.harvard.edu/archive/21a_fall_14/exhibits/cajori/cajori.pdf|archive-date=2018-11-23|url-status=dead}}&lt;br /&gt;
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== External links ==&lt;br /&gt;
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{{Sister project links| wikt=no | commons=Category:Solutions of PDE | b=Partial Differential Equations | n=no | q=Partial differential equation | s=no | v=no | voy=no | species=no | d=no}}&lt;br /&gt;
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* {{springer|title=Differential equation, partial|id=p/d031920}}&lt;br /&gt;
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* [http://eqworld.ipmnet.ru/en/pde-en.htm Partial Differential Equations: Exact Solutions] at EqWorld: The World of Mathematical Equations.&lt;br /&gt;
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* [http://eqworld.ipmnet.ru/en/solutions/eqindex/eqindex-pde.htm Partial Differential Equations: Index] at EqWorld: The World of Mathematical Equations.&lt;br /&gt;
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* [http://eqworld.ipmnet.ru/en/methods/meth-pde.htm Partial Differential Equations: Methods] at EqWorld: The World of Mathematical Equations.&lt;br /&gt;
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* [https://web.archive.org/web/20170701144823/http://www.exampleproblems.com/wiki/index.php?title=Partial_Differential_Equations Example problems with solutions] at exampleproblems.com&lt;br /&gt;
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* [http://mathworld.wolfram.com/PartialDifferentialEquation.html Partial Differential Equations] at mathworld.wolfram.com&lt;br /&gt;
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* [https://reference.wolfram.com/language/FEMDocumentation/tutorial/SolvingPDEwithFEM.html Partial Differential Equations] with Mathematica&lt;br /&gt;
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* [http://www.mathworks.com/moler/pdes.pdf Partial Differential Equations] in Cleve Moler: Numerical Computing with MATLAB&lt;br /&gt;
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* [http://www.nag.com/numeric/fl/nagdoc_fl24/html/D03/d03intro.html Partial Differential Equations] at nag.com&lt;br /&gt;
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* {{cite web |first=Grant |last=Sanderson |title=But what is a partial differential equation? |work=3Blue1Brown |date=April 21, 2019 |url=https://www.youtube.com/watch?v=ly4S0oi3Yz8&amp;amp;list=PLZHQObOWTQDNPOjrT6KVlfJuKtYTftqH6 |via=[[YouTube]] }}&lt;br /&gt;
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[[Category:Partial differential equations| ]]&lt;br /&gt;
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Category:Multivariable calculus&lt;br /&gt;
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类别: 多元微积分&lt;br /&gt;
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[[Category:Differential equations]]&lt;br /&gt;
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Category:Differential equations&lt;br /&gt;
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类别: 微分方程&lt;br /&gt;
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Category:Concepts in physics&lt;br /&gt;
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&amp;lt;small&amp;gt;This page was moved from [[wikipedia:en:Partial differential equation]]. Its edit history can be viewed at [[偏微分方程/edithistory]]&amp;lt;/small&amp;gt;&amp;lt;/noinclude&amp;gt;&lt;br /&gt;
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[[Category:待整理页面]]&lt;/div&gt;</summary>
		<author><name>Ruili</name></author>
	</entry>
	<entry>
		<id>https://wiki.swarma.org/index.php?title=%E5%81%8F%E5%BE%AE%E5%88%86%E6%96%B9%E7%A8%8B&amp;diff=18202</id>
		<title>偏微分方程</title>
		<link rel="alternate" type="text/html" href="https://wiki.swarma.org/index.php?title=%E5%81%8F%E5%BE%AE%E5%88%86%E6%96%B9%E7%A8%8B&amp;diff=18202"/>
		<updated>2020-11-12T15:45:40Z</updated>

		<summary type="html">&lt;p&gt;Ruili：&lt;/p&gt;
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&lt;div&gt;此词条暂由Yuling翻译，未经人工整理和审校，带来阅读不便，请见谅。&lt;br /&gt;
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[[File:Heat.gif|thumb|right|A visualisation of a solution to the two-dimensional [[heat equation]] with temperature represented by the third dimension]]&lt;br /&gt;
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A visualisation of a solution to the two-dimensional [[heat equation with temperature represented by the third dimension]]&lt;br /&gt;
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以三维表示温度的二维热方程解的可视化&lt;br /&gt;
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In [[mathematics]], a '''partial differential equation''' ('''PDE''') is a [[differential equation]] that contains unknown [[Multivariable calculus|multivariable functions]] and their [[partial derivative]]s. PDEs are used to formulate problems involving functions of several variables, and are either solved by hand, or used to create a [[computer model]]. A special case is [[ordinary differential equation]]s (ODEs), which deal with functions of a single variable and their derivatives.&lt;br /&gt;
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In mathematics, a partial differential equation (PDE) is a differential equation that contains unknown multivariable functions and their partial derivatives. PDEs are used to formulate problems involving functions of several variables, and are either solved by hand, or used to create a computer model. A special case is ordinary differential equations (ODEs), which deal with functions of a single variable and their derivatives.&lt;br /&gt;
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在数学中，'''&amp;lt;font color = &amp;quot;#ff8000&amp;quot;&amp;gt; 偏微分方程函数 Partial Differential Equation&amp;lt;/font&amp;gt;'''是包含未知多元函数及其偏导数的微分方程。偏微分方程用于描述涉及多元函数的问题，可以通过人为求解，也可以通过建立计算机模型来求解。常微分方程是偏微分方程一种特殊情况，它处理的是一元函数及其导数。&lt;br /&gt;
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PDEs can be used to describe a wide variety of phenomena such as sound, heat, [[diffusion]], [[electrostatics]], [[Electromagnetism|electrodynamics]], [[fluid dynamics]], [[Elasticity (physics)|elasticity]], [[gravitation]] and [[quantum mechanics]]. These seemingly distinct physical phenomena can be formalised similarly in terms of PDEs. Just as ordinary differential equations often model one-dimensional [[dynamical system]]s, partial differential equations often model [[multidimensional system]]s. PDEs find their generalisation in [[stochastic partial differential equation]]s.&lt;br /&gt;
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PDEs can be used to describe a wide variety of phenomena such as sound, heat, diffusion, electrostatics, electrodynamics, fluid dynamics, elasticity, gravitation and quantum mechanics. These seemingly distinct physical phenomena can be formalised similarly in terms of PDEs. Just as ordinary differential equations often model one-dimensional dynamical systems, partial differential equations often model multidimensional systems. PDEs find their generalisation in stochastic partial differential equations.&lt;br /&gt;
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偏微分方程可以用来描述各种各样的物理现象，如声音，热量，扩散，静电，电动力学，流体力学，弹性力学，重力和量子力学。这些看起来截然不同的物理现象却可以用类似的偏微分方程来描述。正如常微分方程经常对一维动力系统进行建模一样，偏微分方程经常对多维系统进行建模。随机偏微分方程是偏微分方程的一种推广。&lt;br /&gt;
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== Introduction ==&lt;br /&gt;
引言&lt;br /&gt;
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Partial differential equations (PDEs) are equations that involve rates of change with respect to [[continuous variables]]. For example, the position of a [[rigid body]] is specified by six parameters,&amp;lt;ref&amp;gt;{{Cite book|url=https://books.google.com/books?id=v9PLbcYd9aUC&amp;amp;pg=PA32|title=Modelling and Control of Robot Manipulators|last=Sciavicco|first=Lorenzo|last2=Siciliano|first2=Bruno|date=2001-02-19|publisher=Springer Science &amp;amp; Business Media|isbn=9781852332211|language=en}}&amp;lt;/ref&amp;gt; but the configuration of a [[fluid]] is given by the [[continuous distribution]] of several parameters, such as the [[temperature]], [[pressure]], and so forth. The dynamics for the rigid body take place in a finite-dimensional [[Configuration space (physics)|configuration space]]; the dynamics for the fluid occur in an infinite-dimensional configuration space. This distinction usually makes PDEs much harder to solve than ordinary differential equations (ODEs), but here again, there will be simple solutions for linear problems. Classic domains where PDEs are used include [[acoustics]], [[fluid dynamics]], [[electrodynamics]], and [[heat transfer]].&lt;br /&gt;
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Partial differential equations (PDEs) are equations that involve rates of change with respect to continuous variables. For example, the position of a rigid body is specified by six parameters, but the configuration of a fluid is given by the continuous distribution of several parameters, such as the temperature, pressure, and so forth. The dynamics for the rigid body take place in a finite-dimensional configuration space; the dynamics for the fluid occur in an infinite-dimensional configuration space. This distinction usually makes PDEs much harder to solve than ordinary differential equations (ODEs), but here again, there will be simple solutions for linear problems. Classic domains where PDEs are used include acoustics, fluid dynamics, electrodynamics, and heat transfer.&lt;br /&gt;
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偏微分方程(简称为PDEs)涉及到方程相对于连续变量的变化率。例如，刚体的位置是由六个参数确定的，而流体的状态是由几个参数的连续分布给出的，如温度、压力等。刚体的动力学过程发生在有限维状态空间中，流体的动力学过程发生在无限维状态空间中。这种区别通常使偏微分方程比常微分方程更难求解，但是线性问题仍然有简单的求解方式。使用偏微分方程的经典领域包括声学、流体力学、电动力学和传热学。&lt;br /&gt;
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A partial differential equation (PDE) for the function {{math|''u''(''x''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;,… ''x&amp;lt;sub&amp;gt;n&amp;lt;/sub&amp;gt;'')}} is an equation of the form&lt;br /&gt;
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A partial differential equation (PDE) for the function  is an equation of the form&lt;br /&gt;
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函数 {{math|''u''(''x''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;,… ''x&amp;lt;sub&amp;gt;n&amp;lt;/sub&amp;gt;'')}} 的偏微分方程形式是：&lt;br /&gt;
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: &amp;lt;math&amp;gt;f \left (x_1, \ldots x_n; u, \frac{\partial u}{\partial x_1}, \ldots \frac{\partial u}{\partial x_n}; \frac{\partial^2 u}{\partial x_1 \partial x_1}, \ldots \frac{\partial^2 u}{\partial x_1 \partial x_n}; \ldots \right) = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;f \left (x_1, \ldots x_n; u, \frac{\partial u}{\partial x_1}, \ldots \frac{\partial u}{\partial x_n}; \frac{\partial^2 u}{\partial x_1 \partial x_1}, \ldots \frac{\partial^2 u}{\partial x_1 \partial x_n}; \ldots \right) = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
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If {{mvar|f}} is a [[linear function]] of {{mvar|u}} and its derivatives, then the PDE is called linear. Common examples of linear PDEs include the [[heat equation]], the [[wave equation]], [[Laplace's equation]], [[Helmholtz equation]], [[Klein–Gordon equation]], and [[Poisson's equation]].&lt;br /&gt;
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If  is a linear function of  and its derivatives, then the PDE is called linear. Common examples of linear PDEs include the heat equation, the wave equation, Laplace's equation, Helmholtz equation, Klein–Gordon equation, and Poisson's equation.&lt;br /&gt;
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如果 {{mvar|f}} 是函数 {{math|''u''}} 及其导数的线性函数，则偏微分方程称为线性函数。线性偏微分方程的常见例子包括热方程、波动方程、拉普拉斯方程、亥姆霍兹方程方程、克莱因-高登方程和泊松方程。&lt;br /&gt;
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A relatively simple PDE is&lt;br /&gt;
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A relatively simple PDE is&lt;br /&gt;
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一个相对简单的偏微分方程：&lt;br /&gt;
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: &amp;lt;math&amp;gt;\frac{\partial u}{\partial x}(x,y) = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;\frac{\partial u}{\partial x}(x,y) = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
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This relation [[Logical implication|implies]] that the function {{math|''u''(''x'',''y'')}} is independent of {{mvar|x}}. However, the equation gives no information on the function's dependence on the variable {{mvar|y}}. Hence the general solution of this equation is&lt;br /&gt;
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This relation implies that the function  is independent of . However, the equation gives no information on the function's dependence on the variable . Hence the general solution of this equation is&lt;br /&gt;
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这意味着函数 {{math|''u''(''x'',''y'')}} 独立于 {{mvar|x}} 的。然而，这个方程没有给出关于函数和自变量的相关性的信息。因此，这个方程的通解是&lt;br /&gt;
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: &amp;lt;math&amp;gt;u(x,y) = f(y),&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;u(x,y) = f(y),&amp;lt;/math&amp;gt;&lt;br /&gt;
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where {{mvar|f}} is an arbitrary function of {{mvar|y}}. The analogous ordinary differential equation is&lt;br /&gt;
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where  is an arbitrary function of . The analogous ordinary differential equation is&lt;br /&gt;
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其中， {{mvar|f}} 是 {{mvar|y}} 的任意函数。&lt;br /&gt;
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类似的常微分方程是：&lt;br /&gt;
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: &amp;lt;math&amp;gt;\frac{\mathrm{d} u}{\mathrm{d} x}(x) = 0,&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;\frac{\mathrm{d} u}{\mathrm{d} x}(x) = 0,&amp;lt;/math&amp;gt;&lt;br /&gt;
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which has the solution&lt;br /&gt;
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which has the solution&lt;br /&gt;
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它的解为&lt;br /&gt;
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: &amp;lt;math&amp;gt;u(x) = c,&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;u(x) = c,&amp;lt;/math&amp;gt;&lt;br /&gt;
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where {{mvar|c}} is any [[Constant (mathematics)|constant]] value. These two examples illustrate that general solutions of ordinary differential equations (ODEs) involve arbitrary constants, but solutions of PDEs involve arbitrary functions.&lt;br /&gt;
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where  is any constant value. These two examples illustrate that general solutions of ordinary differential equations (ODEs) involve arbitrary constants, but solutions of PDEs involve arbitrary functions.&lt;br /&gt;
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这里，{{mvar|c}} 是一个任意常量。&lt;br /&gt;
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这两个例子说明常微分方程的一般解包含任意常数，但偏微分方程的解包含任意函数。&lt;br /&gt;
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A solution of a PDE is generally not [[Uniqueness quantification|unique]]; additional conditions must generally be specified on the [[Boundary (topology)|boundary]] of the region where the solution is defined. For instance, in the simple example above, the function {{math|''f''(''y'')}} can be determined if {{mvar|u}} is specified on the line {{math|''x'' {{=}} 0}}.&lt;br /&gt;
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A solution of a PDE is generally not unique; additional conditions must generally be specified on the boundary of the region where the solution is defined. For instance, in the simple example above, the function  can be determined if  is specified on the line  0}}.&lt;br /&gt;
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偏微分方程的解一般不是唯一的; 一般必须在定义解的区域边界上定义附加条件。 例如，在上面的简单示例中，如果在 {{math|''x'' {{=}} 0}} 时确定了 {{mvar|u}} 的值，则可以确定该函数 {{math|''f''(''y'')}}。&lt;br /&gt;
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== Existence and uniqueness ==&lt;br /&gt;
存在性和唯一性&lt;br /&gt;
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Although the issue of existence and uniqueness of solutions of ordinary differential equations has a very satisfactory answer with the [[Picard–Lindelöf theorem]], that is far from the case for partial differential equations. The [[Cauchy–Kowalevski theorem]] states that the [[Cauchy problem]] for any partial differential equation whose coefficients are [[Analytic function|analytic]] in the unknown function and its derivatives, has a locally unique analytic solution. Although this result might appear to settle the existence and uniqueness of solutions, there are examples of linear partial differential equations whose coefficients have derivatives of all orders (which are nevertheless not analytic) but which have no solutions at all: see [[Lewy's example|Lewy (1957)]]. Even if the solution of a partial differential equation exists and is unique, it may nevertheless have undesirable properties.  The mathematical study of these questions is usually in the more powerful context of [[weak solution]]s.&lt;br /&gt;
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Although the issue of existence and uniqueness of solutions of ordinary differential equations has a very satisfactory answer with the Picard–Lindelöf theorem, that is far from the case for partial differential equations. The Cauchy–Kowalevski theorem states that the Cauchy problem for any partial differential equation whose coefficients are analytic in the unknown function and its derivatives, has a locally unique analytic solution. Although this result might appear to settle the existence and uniqueness of solutions, there are examples of linear partial differential equations whose coefficients have derivatives of all orders (which are nevertheless not analytic) but which have no solutions at all: see Lewy (1957). Even if the solution of a partial differential equation exists and is unique, it may nevertheless have undesirable properties.  The mathematical study of these questions is usually in the more powerful context of weak solutions.&lt;br /&gt;
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尽管常微分方程解的存在性和唯一性用'''&amp;lt;font color=&amp;quot;#ff8000&amp;quot;&amp;gt;弗罗贝尼乌斯定理 Picard–Lindelöf Theorem&amp;lt;/font&amp;gt;得到了令人满意的结果，但偏微分方程解的存在性和唯一性却远没有得到解决。'''&amp;lt;font color=&amp;quot;#ff8000&amp;quot;&amp;gt;柯西-科瓦列夫斯基定理 Cauchy–Kowalevski theorem&amp;lt;/font&amp;gt;指出：对于任意系数在未知函数及其导数中解析的偏微分方程，柯西问题存在一个局部唯一的解析解。虽然这个结果似乎解决了解的存在性和唯一性问题，但是存在一些线性偏微分方程-其系数具有所有级数的导数(尽管这些导数不是解析的) ，但是根本没有解: 见 Lewy (1957)。即使偏微分方程的解存在且唯一，它仍然可能具有不可预料的性质。这些问题的数学研究通常是在更有力的弱解的背景下进行的。&lt;br /&gt;
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An example of pathological behavior is the sequence (depending upon {{mvar|n}}) of [[Cauchy problem]]s for the [[Laplace equation]]&lt;br /&gt;
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An example of pathological behavior is the sequence (depending upon ) of Cauchy problems for the Laplace equation&lt;br /&gt;
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反常特征的一个例子是拉普拉斯方程的柯西问题的序列(取决于{{mvar|n}})&lt;br /&gt;
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: &amp;lt;math&amp;gt;\frac{\partial^2 u}{\partial x^2} + \frac{\partial^2 u}{\partial y^2}=0,&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;\frac{\partial^2 u}{\partial x^2} + \frac{\partial^2 u}{\partial y^2}=0,&amp;lt;/math&amp;gt;&lt;br /&gt;
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with [[boundary condition]]s&lt;br /&gt;
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with boundary conditions&lt;br /&gt;
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具有边界条件&lt;br /&gt;
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: &amp;lt;math&amp;gt;\begin{align} u(x,0) &amp;amp;= 0, \\ \frac{\partial u}{\partial y}(x,0) &amp;amp;= \frac{\sin nx}{n}, \end{align}&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;\begin{align} u(x,0) &amp;amp;= 0, \\ \frac{\partial u}{\partial y}(x,0) &amp;amp;= \frac{\sin nx}{n}, \end{align}&amp;lt;/math&amp;gt;&lt;br /&gt;
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where {{mvar|n}} is an integer. The derivative of {{mvar|u}} with respect to {{mvar|y}} approaches zero [[uniform convergence|uniformly]] in {{mvar|x}} as {{mvar|n}} increases, but the solution is&lt;br /&gt;
&lt;br /&gt;
where  is an integer. The derivative of  with respect to  approaches zero uniformly in  as  increases, but the solution is&lt;br /&gt;
&lt;br /&gt;
其中 {{mvar|n}} 是整数。{{mvar|u}} 关于 {{mvar|y}} 的导数，一致地随着 {{mvar|n}} 的增加而趋于零，但解是&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt;u(x,y) = \frac{\sinh ny \sin nx}{n^2}.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;u(x,y) = \frac{\sinh ny \sin nx}{n^2}.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
This solution approaches infinity if {{mvar|nx}} is not an integer multiple of {{pi}} for any non-zero value of {{mvar|y}}. The Cauchy problem for the Laplace equation is called ''ill-posed'' or ''not [[Well-posed problem|well-posed]]'', since the solution does not continuously depend on the data of the problem. Such ill-posed problems are not usually satisfactory for physical applications.&lt;br /&gt;
&lt;br /&gt;
This solution approaches infinity if  is not an integer multiple of  for any non-zero value of . The Cauchy problem for the Laplace equation is called ill-posed or not well-posed, since the solution does not continuously depend on the data of the problem. Such ill-posed problems are not usually satisfactory for physical applications.&lt;br /&gt;
&lt;br /&gt;
对于任何非零的{{mvar|y}}，如果{{mvar|nx}}不是{{pi}}的整数倍，这个解会接近于无穷大。拉普拉斯方程的柯西问题被称为不适定问题（可以译为ill-posed或not well-posed），因为该问题的解并不连续地依赖于该问题的数据。这种不适定问题在物理应用中通常不能令人满意。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The [[Navier–Stokes existence and smoothness|existence of solutions for the Navier–Stokes equations]], a partial differential equation, is part of one of the [[Millennium Prize Problems]].&lt;br /&gt;
&lt;br /&gt;
The existence of solutions for the Navier–Stokes equations, a partial differential equation, is part of one of the Millennium Prize Problems.&lt;br /&gt;
&lt;br /&gt;
一种偏微分方程——纳维-斯托克斯方程——的解的存在性就是千禧年大奖难题的一部分。&lt;br /&gt;
&lt;br /&gt;
== Notation ==&lt;br /&gt;
符号&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
In PDEs, it is common to denote partial derivatives using subscripts. That is:&lt;br /&gt;
&lt;br /&gt;
In PDEs, it is common to denote partial derivatives using subscripts. That is:&lt;br /&gt;
&lt;br /&gt;
在偏微分方程中，通常用下标表示偏导数。例如:&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt;u_x = \frac{\partial u}{\partial x}&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;u_x = \frac{\partial u}{\partial x}&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt;u_{xx} = \frac{\partial^2 u}{\partial x^2} &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;u_{xx} = \frac{\partial^2 u}{\partial x^2} &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt;u_{xy} = \frac{\partial^2 u}{\partial y\, \partial x} = \frac{\partial}{\partial y } \left(\frac{\partial u}{\partial x}\right). &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;u_{xy} = \frac{\partial^2 u}{\partial y\, \partial x} = \frac{\partial}{\partial y } \left(\frac{\partial u}{\partial x}\right). &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Especially in physics, [[del]] or nabla ({{math|∇}}) is often used to denote spatial derivatives, and {{math|''&amp;amp;#x307;u'', ''ü''}} for time derivatives. For example, the [[wave equation]] (mentioned below) can be written as&lt;br /&gt;
&lt;br /&gt;
Especially in physics, del or nabla () is often used to denote spatial derivatives, and  for time derivatives. For example, the wave equation (mentioned below) can be written as&lt;br /&gt;
&lt;br /&gt;
特别是在物理学中，[[del]]或nabla ({{math|∇}})经常用来表示空间导数和时间导数。例如，波动方程(在下文中提到)可以写成&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt;\ddot u=c^2\nabla^2u&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt;\ddot u=c^2\nabla^2u&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
or&lt;br /&gt;
&lt;br /&gt;
or&lt;br /&gt;
&lt;br /&gt;
或&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt;\ddot u=c^2\Delta u&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt;\ddot u=c^2\Delta u&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
where {{math|Δ}} is the [[Laplace operator]].&lt;br /&gt;
&lt;br /&gt;
where  is the Laplace operator.&lt;br /&gt;
&lt;br /&gt;
其中{{math|Δ}}代表拉普拉斯算子&lt;br /&gt;
&lt;br /&gt;
== Classification ==&lt;br /&gt;
分类&lt;br /&gt;
&lt;br /&gt;
Some linear, second-order partial differential equations can be classified as [[parabolic partial differential equation|parabolic]], [[hyperbolic partial differential equation|hyperbolic]] and [[elliptic partial differential equation|elliptic]]. Others, such as the [[Euler–Tricomi equation]], have different types in different regions. The classification provides a guide to appropriate initial and boundary conditions and to the smoothness of the solutions.&lt;br /&gt;
&lt;br /&gt;
Some linear, second-order partial differential equations can be classified as parabolic, hyperbolic and elliptic. Others, such as the Euler–Tricomi equation, have different types in different regions. The classification provides a guide to appropriate initial and boundary conditions and to the smoothness of the solutions.&lt;br /&gt;
&lt;br /&gt;
一些线性二阶偏微分方程可分为抛物型方程、双曲型方程和椭圆型方程。其他的方程，如欧拉-特里科米方程，在不同的区域有不同的类型。这种分类有助于选择适当的初始和边界条件以及提高解的平滑性。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
=== Equations of first order ===&lt;br /&gt;
一阶方程&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{{main|First-order partial differential equation}}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
=== Linear equations of second order ===&lt;br /&gt;
二阶线性方程&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Assuming {{math|''u&amp;lt;sub&amp;gt;xy&amp;lt;/sub&amp;gt;'' {{=}} ''u&amp;lt;sub&amp;gt;yx&amp;lt;/sub&amp;gt;''}}, the general linear second-order PDE in two independent variables has the form&lt;br /&gt;
&lt;br /&gt;
Assuming  u&amp;lt;sub&amp;gt;yx&amp;lt;/sub&amp;gt;}}, the general linear second-order PDE in two independent variables has the form&lt;br /&gt;
&lt;br /&gt;
假设 {{math|''u&amp;lt;sub&amp;gt;xy&amp;lt;/sub&amp;gt;'' {{=}} ''u&amp;lt;sub&amp;gt;yx&amp;lt;/sub&amp;gt;''}}，含有两个独立变量的一般的线性二阶偏微分方程具有如下这样的形式&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt;Au_{xx} + 2Bu_{xy} + Cu_{yy} + \cdots \mbox{(lower order terms)} = 0,&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;Au_{xx} + 2Bu_{xy} + Cu_{yy} + \cdots \mbox{(lower order terms)} = 0,&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
where the coefficients {{mvar|A}}, {{mvar|B}}, {{mvar|C}}... may depend upon {{mvar|x}} and {{mvar|y}}. If {{math|''A''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; + ''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; + ''C''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; &amp;gt; 0}} over a region of the {{mvar|xy}}-plane, the PDE is second-order in that region. This form is analogous to the equation for a conic section:&lt;br /&gt;
&lt;br /&gt;
where the coefficients , , ... may depend upon  and . If  over a region of the -plane, the PDE is second-order in that region. This form is analogous to the equation for a conic section:&lt;br /&gt;
&lt;br /&gt;
其中的系数 {{mvar|A}}, {{mvar|B}}, {{mvar|C}}... 一般取决于{{mvar|x}}和{{mvar|y}}。如果在{{mvar|xy}}-平面的一个区域上 {{math|''A''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; + ''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; + ''C''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; &amp;gt; 0}}，偏微分方程在该区域是二阶的。这种形式类似于圆锥曲线的方程:&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt;Ax^2 + 2Bxy + Cy^2 + \cdots = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;Ax^2 + 2Bxy + Cy^2 + \cdots = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
More precisely, replacing {{math|∂&amp;lt;sub&amp;gt;''x''&amp;lt;/sub&amp;gt;}} by {{mvar|X}}, and likewise for other variables (formally this is done by a [[Fourier transform]]), converts a constant-coefficient PDE into a polynomial of the same degree, with the terms of the highest degree (a [[homogeneous polynomial]], here a [[quadratic form]]) being most significant for the classification.&lt;br /&gt;
&lt;br /&gt;
More precisely, replacing  by , and likewise for other variables (formally this is done by a Fourier transform), converts a constant-coefficient PDE into a polynomial of the same degree, with the terms of the highest degree (a homogeneous polynomial, here a quadratic form) being most significant for the classification.&lt;br /&gt;
&lt;br /&gt;
更准确地说，用 {{mvar|X}} 替换 {{math|∂&amp;lt;sub&amp;gt;''x''&amp;lt;/sub&amp;gt;}}，对于其他变量做同样的操作(从形式上来说，这是由傅里叶变换来完成的)，将一个常系数偏微分方程转换成一个相同次数的多项式，最高次数的项(齐次多项式，这里是一个二次形式)一般会用于偏微分方程的分类。&lt;br /&gt;
===~~ most significant for the classification 意译为用于偏微分方程的分类。       significiant直译过来感觉不太合适&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Just as one classifies [[conic section]]s and quadratic forms into parabolic, hyperbolic, and elliptic based on the [[discriminant]] {{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − 4''AC''}}, the same can be done for a second-order PDE at a given point.  However, the [[discriminant]] in a PDE is given by {{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC''}} due to the convention of the {{mvar|xy}} term being {{math|2''B''}} rather than {{mvar|B}}; formally, the discriminant (of the associated quadratic form) is {{math|(2''B'')&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − 4''AC'' {{=}} 4(''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC'')}}, with the factor of 4 dropped for simplicity.&lt;br /&gt;
&lt;br /&gt;
Just as one classifies conic sections and quadratic forms into parabolic, hyperbolic, and elliptic based on the discriminant , the same can be done for a second-order PDE at a given point.  However, the discriminant in a PDE is given by  due to the convention of the  term being  rather than ; formally, the discriminant (of the associated quadratic form) is  4(B&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − AC)}}, with the factor of 4 dropped for simplicity.&lt;br /&gt;
&lt;br /&gt;
正如人们可以根据判别式 {{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − 4''AC''}} 将圆锥曲线和二次型分为抛物型、双曲型和椭圆型一样，对于给定点的二阶偏微分方程也可以这样做。然而，偏微分方程中的判别式 {{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − 4''AC''}} 是根据交叉项的系数{{math|2''B''}} 而不是 {{mvar|B}} 给出的，形式上，判别式(关联二次型)是 {{math|(2''B'')&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − 4''AC'' {{=}} 4(''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC'')}}，为简单起见，去掉了因子4。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
# {{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC'' &amp;lt; 0}} (''[[elliptic partial differential equation]]''): Solutions of [[elliptic partial differential equation|elliptic PDEs]] are as smooth as the coefficients allow, within the interior of the region where the equation and solutions are defined. For example, solutions of [[Laplace's equation]] are analytic within the domain where they are defined, but solutions may assume boundary values that are not smooth. The motion of a fluid at subsonic speeds can be approximated with elliptic PDEs, and the Euler–Tricomi equation is elliptic where {{math|''x'' &amp;lt; 0}}.&lt;br /&gt;
&lt;br /&gt;
  (elliptic partial differential equation): Solutions of elliptic PDEs are as smooth as the coefficients allow, within the interior of the region where the equation and solutions are defined. For example, solutions of Laplace's equation are analytic within the domain where they are defined, but solutions may assume boundary values that are not smooth. The motion of a fluid at subsonic speeds can be approximated with elliptic PDEs, and the Euler–Tricomi equation is elliptic where .&lt;br /&gt;
&lt;br /&gt;
{{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC'' &amp;lt; 0}} (椭圆形微分方程)：在定义方程和解的区域内部，椭圆型偏微分方程的解光滑到系数允许的程度。例如，拉普拉斯方程的解在它们被定义的区域内是解析的，但是解可能假设边界值是不光滑的。亚音速流体的运动可以用椭圆偏微分方程近似，其中欧拉-特里科米方程在 {{math|''x'' &amp;lt; 0}} 时是椭圆型偏微分方程。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
# {{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC'' {{=}} 0}} (''[[parabolic partial differential equation]]''): Equations that are [[parabolic partial differential equation|parabolic]] at every point can be transformed into a form analogous to the [[heat equation]] by a change of independent variables. Solutions smooth out as the transformed time variable increases. The Euler–Tricomi equation has parabolic type on the line where {{math|''x'' {{=}} 0}}.&lt;br /&gt;
&lt;br /&gt;
  0}} (parabolic partial differential equation): Equations that are parabolic at every point can be transformed into a form analogous to the heat equation by a change of independent variables. Solutions smooth out as the transformed time variable increases. The Euler–Tricomi equation has parabolic type on the line where  0}}.&lt;br /&gt;
&lt;br /&gt;
{{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC'' {{=}} 0}}（抛物线形偏微分方程）：在每一点上都是抛物线型的方程可以通过改变自变量从而转化成类似于热方程的形式。随着转换后的时间变量的增加，方程的解变得平滑。欧拉-特里科米方程在 {{math|''x'' {{=}} 0}} 这条特征线上是抛物线形的。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
# {{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC'' &amp;gt; 0}} (''[[hyperbolic partial differential equation]]''): [[hyperbolic partial differential equation|hyperbolic]] equations retain any discontinuities of functions or derivatives in the initial data. An example is the [[wave equation]]. The motion of a fluid at supersonic speeds can be approximated with hyperbolic PDEs, and the Euler–Tricomi equation is hyperbolic where {{math|''x'' &amp;gt; 0}}.&lt;br /&gt;
&lt;br /&gt;
  (hyperbolic partial differential equation): hyperbolic equations retain any discontinuities of functions or derivatives in the initial data. An example is the wave equation. The motion of a fluid at supersonic speeds can be approximated with hyperbolic PDEs, and the Euler–Tricomi equation is hyperbolic where .&lt;br /&gt;
&lt;br /&gt;
{{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC'' &amp;gt; 0}} (双曲形偏微分方程)：双曲形方程在初始数据中保留了函数或导数的任何不连续性，波动方程就是其中的一个例子。超音速流体的运动可以用双曲形偏微分方程近似，其中欧拉-特里科米方程在 {{math|''x'' &amp;gt; 0}} 时是双曲型的。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
If there are {{mvar|n}} independent variables {{math|''x''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;, ''x''&amp;lt;sub&amp;gt;2 &amp;lt;/sub&amp;gt;,… ''x''&amp;lt;sub&amp;gt;''n''&amp;lt;/sub&amp;gt;}}, a general linear partial differential equation of second order has the form&lt;br /&gt;
&lt;br /&gt;
If there are  independent variables , a general linear partial differential equation of second order has the form&lt;br /&gt;
&lt;br /&gt;
如果存在 {{mvar|n}} 个自变量 {{math|''x''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;, ''x''&amp;lt;sub&amp;gt;2 &amp;lt;/sub&amp;gt;,… ''x''&amp;lt;sub&amp;gt;''n''&amp;lt;/sub&amp;gt;}}，一般二阶线性偏微分方程的形式是&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt;L u =\sum_{i=1}^n\sum_{j=1}^n a_{i,j} \frac{\partial^2 u}{\partial x_i \partial x_j} \quad \text{ plus lower-order terms} =0.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;L u =\sum_{i=1}^n\sum_{j=1}^n a_{i,j} \frac{\partial^2 u}{\partial x_i \partial x_j} \quad \text{ plus lower-order terms} =0.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The classification depends upon the signature of the eigenvalues of the coefficient matrix {{math|''a''&amp;lt;sub&amp;gt;''i'',''j''&amp;lt;/sub&amp;gt;}}.&lt;br /&gt;
&lt;br /&gt;
The classification depends upon the signature of the eigenvalues of the coefficient matrix .&lt;br /&gt;
&lt;br /&gt;
这种分类取决于系数矩阵本征值的符号（正负性）。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
# Elliptic: the eigenvalues are all positive or all negative.&lt;br /&gt;
&lt;br /&gt;
 Elliptic: the eigenvalues are all positive or all negative.&lt;br /&gt;
&lt;br /&gt;
椭圆形方程: 本征值全部为正或全部为负。&lt;br /&gt;
&lt;br /&gt;
# Parabolic: the eigenvalues are all positive or all negative, save one that is zero.&lt;br /&gt;
&lt;br /&gt;
 Parabolic: the eigenvalues are all positive or all negative, save one that is zero.&lt;br /&gt;
&lt;br /&gt;
抛物线形方程: 本征值全部为正或全部为负，除了一个为零。&lt;br /&gt;
&lt;br /&gt;
# Hyperbolic: there is only one negative eigenvalue and all the rest are positive, or there is only one positive eigenvalue and all the rest are negative.&lt;br /&gt;
&lt;br /&gt;
 Hyperbolic: there is only one negative eigenvalue and all the rest are positive, or there is only one positive eigenvalue and all the rest are negative.&lt;br /&gt;
&lt;br /&gt;
双曲形方程: 只有一个负特征值，其余的都是正特征值，或者只有一个正特征值，其余的都是负特征值。&lt;br /&gt;
&lt;br /&gt;
# Ultrahyperbolic: there is more than one positive eigenvalue and more than one negative eigenvalue, and there are no zero eigenvalues. There is only a limited theory for ultrahyperbolic equations (Courant and Hilbert, 1962).&lt;br /&gt;
&lt;br /&gt;
 Ultrahyperbolic: there is more than one positive eigenvalue and more than one negative eigenvalue, and there are no zero eigenvalues. There is only a limited theory for ultrahyperbolic equations (Courant and Hilbert, 1962).&lt;br /&gt;
&lt;br /&gt;
超双形方程: 存在多于一个正本征值和多于一个的负本征值，且不存在零本征值。对于超双曲方程，只存在一个有限理论(Courant 和 Hilbert，1962)。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==[[用户:Yuling|Yuling]]（[[用户讨论:Yuling|讨论]]） 我对于limited theory这个单词对应的相关理论不太了解。&lt;br /&gt;
&lt;br /&gt;
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=== Systems of first-order equations and characteristic surfaces ===&lt;br /&gt;
一阶方程组和特征曲面&lt;br /&gt;
&lt;br /&gt;
The classification of partial differential equations can be extended to systems of first-order equations, where the unknown {{mvar|u}} is now a [[Euclidean vector|vector]] with {{mvar|m}} components, and the coefficient matrices {{mvar|A&amp;lt;sub&amp;gt;ν&amp;lt;/sub&amp;gt;}} are {{mvar|m}} by {{mvar|m}} matrices for {{math|''ν'' {{=}} 1, 2,… ''n''}}. The partial differential equation takes the form&lt;br /&gt;
&lt;br /&gt;
The classification of partial differential equations can be extended to systems of first-order equations, where the unknown  is now a vector with  components, and the coefficient matrices  are  by  matrices for  1, 2,… n}}. The partial differential equation takes the form&lt;br /&gt;
&lt;br /&gt;
偏微分方程组的分类可以推广到一阶方程组，其中未知量 {{mvar|u}} 是有 {{mvar|m}} 个分量的向量。对于 {{math|''ν'' {{=}} 1, 2,… ''n''}}，系数矩阵 {{mvar|A&amp;lt;sub&amp;gt;ν&amp;lt;/sub&amp;gt;}} 是 {{mvar|m}} × {{mvar|m}} 的矩阵。偏微分方程形式如下：&lt;br /&gt;
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&lt;br /&gt;
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: &amp;lt;math&amp;gt;Lu = \sum_{\nu=1}^{n} A_\nu \frac{\partial u}{\partial x_\nu} + B=0,&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;Lu = \sum_{\nu=1}^{n} A_\nu \frac{\partial u}{\partial x_\nu} + B=0,&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
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where the coefficient matrices {{mvar|A&amp;lt;sub&amp;gt;ν&amp;lt;/sub&amp;gt;}} and the vector {{mvar|B}} may depend upon {{mvar|x}} and {{mvar|u}}. If a [[hypersurface]] {{mvar|S}} is given in the implicit form&lt;br /&gt;
&lt;br /&gt;
where the coefficient matrices  and the vector  may depend upon  and . If a hypersurface  is given in the implicit form&lt;br /&gt;
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其中系数矩阵 {{mvar|A&amp;lt;sub&amp;gt;ν&amp;lt;/sub&amp;gt;}} 和向量 {{mvar|B}} 可能依赖于 {{mvar|x}} 和 {{mvar|u}}。如果超曲面是以隐式形式给出的&lt;br /&gt;
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: &amp;lt;math&amp;gt;\varphi(x_1, x_2, \ldots x_n)=0,&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;\varphi(x_1, x_2, \ldots x_n)=0,&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
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where {{mvar|φ}} has a non-zero gradient, then {{mvar|S}} is a '''characteristic surface''' for the operator {{mvar|L}} at a given point if the characteristic form vanishes:&lt;br /&gt;
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where  has a non-zero gradient, then  is a characteristic surface for the operator  at a given point if the characteristic form vanishes:&lt;br /&gt;
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其中存在一个非零的梯度，那么如果特征形式消失，则在给定点上算子的特征曲面形式如下:&lt;br /&gt;
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: &amp;lt;math&amp;gt;Q\left(\frac{\partial\varphi}{\partial x_1}, \ldots\frac{\partial\varphi}{\partial x_n}\right) =\det\left[\sum_{\nu=1}^nA_\nu \frac{\partial \varphi}{\partial x_\nu}\right]=0.\,&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;Q\left(\frac{\partial\varphi}{\partial x_1}, \ldots\frac{\partial\varphi}{\partial x_n}\right) =\det\left[\sum_{\nu=1}^nA_\nu \frac{\partial \varphi}{\partial x_\nu}\right]=0.\,&amp;lt;/math&amp;gt;&lt;br /&gt;
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The geometric interpretation of this condition is as follows: if data for {{mvar|u}} are prescribed on the surface {{mvar|S}}, then it may be possible to determine the normal derivative of {{mvar|u}} on {{mvar|S}} from the differential equation. If the data on {{mvar|S}} and the differential equation determine the normal derivative of {{mvar|u}} on {{mvar|S}}, then {{mvar|S}} is non-characteristic. If the data on {{mvar|S}} and the differential equation ''do not'' determine the normal derivative of {{mvar|u}} on {{mvar|S}}, then the surface is '''characteristic''', and the differential equation restricts the data on {{mvar|S}}: the differential equation is ''internal'' to {{mvar|S}}.&lt;br /&gt;
&lt;br /&gt;
The geometric interpretation of this condition is as follows: if data for  are prescribed on the surface , then it may be possible to determine the normal derivative of  on  from the differential equation. If the data on  and the differential equation determine the normal derivative of  on , then  is non-characteristic. If the data on  and the differential equation do not determine the normal derivative of  on , then the surface is characteristic, and the differential equation restricts the data on : the differential equation is internal to .&lt;br /&gt;
&lt;br /&gt;
这个条件的几何解释如下: 如果关于 {{mvar|u}} 的数据是在曲面 {{mvar|S}} 上规定的，那么就有可能依据微分方程确定曲面 {{mvar|S}} 上 {{mvar|u}} 的法向导数。如果曲面 {{mvar|S}} 上的数据和上面的微分方程能确定曲面 {{mvar|S}} 上 {{mvar|u}} 的法向导数，那么它就是非特征的。如果曲面 {{mvar|S}} 上的数据和上面的微分方程不能确定曲面 {{mvar|S}} 上 {{mvar|u}} 的法向导数，那么曲面是特征的，并且微分方程将数据限制在曲面 {{mvar|S}} 上：微分方程是在曲面 {{mvar|S}} 内部。&lt;br /&gt;
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# A first-order system {{math|''Lu'' {{=}} 0}} is ''elliptic'' if no surface is characteristic for {{mvar|L}}: the values of {{mvar|u}} on {{mvar|S}} and the differential equation always determine the normal derivative of {{mvar|u}} on {{mvar|S}}.&lt;br /&gt;
&lt;br /&gt;
 A first-order system  0}} is elliptic if no surface is characteristic for : the values of  on  and the differential equation always determine the normal derivative of  on .&lt;br /&gt;
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如果对于 {{mvar|L}} 没有曲面是特征的，则一阶系统 {{math|''Lu'' {{=}} 0}} 是椭圆形的：{{mvar|u}}在 {{mvar|S}} 的值和微分方程总能够决定 {{mvar|S}} 上 {{mvar|u}} 的法向导数。&lt;br /&gt;
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# A first-order system is ''hyperbolic'' at a point if there is a '''spacelike''' surface {{mvar|S}} with normal {{mvar|ξ}} at that point. This means that, given any non-trivial vector {{mvar|η}} orthogonal to {{mvar|ξ}}, and a scalar multiplier {{mvar|λ}}, the equation {{math|''Q''(''λξ'' + ''η'') {{=}} 0}} has {{mvar|m}} real roots {{math|''λ''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;, ''λ''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;,… ''λ''&amp;lt;sub&amp;gt;''m''&amp;lt;/sub&amp;gt;}}. The system is '''strictly hyperbolic''' if these roots are always distinct. The geometrical interpretation of this condition is as follows: the characteristic form {{math|''Q''(''ζ'') {{=}} 0}} defines a cone (the normal cone) with homogeneous coordinates ζ. In the hyperbolic case, this cone has {{mvar|m}} sheets, and the axis {{math|''ζ'' {{=}} ''λξ''}} runs inside these sheets: it does not intersect any of them. But when displaced from the origin by η, this axis intersects every sheet. In the elliptic case, the normal cone has no real sheets.&lt;br /&gt;
&lt;br /&gt;
 A first-order system is hyperbolic at a point if there is a spacelike surface  with normal  at that point. This means that, given any non-trivial vector  orthogonal to , and a scalar multiplier , the equation  0}} has  real roots . The system is strictly hyperbolic if these roots are always distinct. The geometrical interpretation of this condition is as follows: the characteristic form  0}} defines a cone (the normal cone) with homogeneous coordinates ζ. In the hyperbolic case, this cone has  sheets, and the axis  λξ}} runs inside these sheets: it does not intersect any of them. But when displaced from the origin by η, this axis intersects every sheet. In the elliptic case, the normal cone has no real sheets.&lt;br /&gt;
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如果在该点存在一个法向量为 {{mvar|ξ}}的 '''&amp;lt;font color=&amp;quot;#ff8000&amp;quot;&amp;gt;类空曲面 Spacclike Surface&amp;lt;/font&amp;gt; {{mvar|S}} ，则一阶系统在那一点是双曲的。这意味着，给定任意正交于 {{mvar|ξ}} 的非平凡向量 {{mvar|η}} 和一个标量乘子 {{mvar|λ}}，方程 {{math|''Q''(''λξ'' + ''η'') {{=}} 0}} 有 {{mvar|m}} 个实根 {{math|''λ''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;, ''λ''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;,… ''λ''&amp;lt;sub&amp;gt;''m''&amp;lt;/sub&amp;gt;}}。如果这些根始终不同，则该系统是严格双曲形的。这个条件的几何解释如下: 特征形式 {{math|''Q''(''ζ'') {{=}} 0}} 定义了一个具有齐次坐标 ζ的圆锥(法线圆锥)。在双曲形的情况下，这个圆锥体有 {{mvar|m}} 层，并且轴 {{math|''ζ'' {{=}} ''λξ''}} 在这些层中运动: 它不与任何一层相交。但是当从原点偏离η时，这条轴线与每一层都相交。在椭圆形的情况下，法向圆锥没有实层。&lt;br /&gt;
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==[[用户:Yuling|Yuling]]（[[用户讨论:Yuling|讨论]]） sheet 这个单词也不很理解，我直译为了“层”&lt;br /&gt;
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=== Equations of mixed type ===&lt;br /&gt;
混合型方程&lt;br /&gt;
&lt;br /&gt;
If a PDE has coefficients that are not constant, it is possible that it will not belong to any of these categories but rather be of '''mixed type'''. A simple but important example is the [[Euler–Tricomi equation]]&lt;br /&gt;
&lt;br /&gt;
If a PDE has coefficients that are not constant, it is possible that it will not belong to any of these categories but rather be of mixed type. A simple but important example is the Euler–Tricomi equation&lt;br /&gt;
&lt;br /&gt;
如果偏微分方程的系数不是常数，那么它可能不属于这些类别中的任何一个，而是属于混合类型。一个简单但重要的例子是欧拉-特里科米方程&lt;br /&gt;
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: &amp;lt;math&amp;gt;u_{xx} = xu_{yy},&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;u_{xx} = xu_{yy},&amp;lt;/math&amp;gt;&lt;br /&gt;
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which is called '''elliptic-hyperbolic''' because it is elliptic in the region {{math|''x'' &amp;lt; 0}}, hyperbolic in the region {{math|''x'' &amp;gt; 0}}, and degenerate parabolic on the line {{math|''x'' {{=}} 0}}.&lt;br /&gt;
&lt;br /&gt;
which is called elliptic-hyperbolic because it is elliptic in the region , hyperbolic in the region , and degenerate parabolic on the line  0}}.&lt;br /&gt;
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它在 {{math|''x'' &amp;lt; 0}} 的区域上是椭圆形，在 {{math|''x'' &amp;gt; 0}} 区域上是双曲形，在 {{math|''x'' {{=}} 0}}这条线上是退化为抛物线形，因此称之为椭圆-双曲型。&lt;br /&gt;
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&amp;lt;!--&lt;br /&gt;
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&amp;lt;!--&lt;br /&gt;
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&amp;lt;!--&lt;br /&gt;
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''fill in: Dirichlet and Neumann boundaries, hyperbolic/parabolic/elliptic separation of variables, [[Fourier analysis]], [[Green's function]]s ...--&amp;gt;&lt;br /&gt;
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fill in: Dirichlet and Neumann boundaries, hyperbolic/parabolic/elliptic separation of variables, Fourier analysis, Green's functions ...--&amp;gt;&lt;br /&gt;
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填写: Dirichlet 和 Neumann 边界，双曲 / 抛物线 / 椭圆分离变量法，傅立叶分析，Green 函数... --&lt;br /&gt;
&lt;br /&gt;
=== Infinite-order PDEs in quantum mechanics ===&lt;br /&gt;
量子力学中的无限阶偏微分方程&lt;br /&gt;
&lt;br /&gt;
In the [[phase space formulation]] of quantum mechanics,  one may consider the [[Method of quantum characteristics|quantum Hamilton's equations]] for trajectories of quantum particles. These equations are infinite-order PDEs. However, in the semiclassical expansion, one has a finite system of ODEs at any fixed order of [[Dirac constant|{{mvar|ħ}}]].  The evolution equation of the [[Wigner quasi-probability distribution|c]] is also an infinite-order PDE. The quantum trajectories are [[Method of quantum characteristics|quantum characteristics]], with the use of which one could calculate the evolution of the Wigner function.&lt;br /&gt;
&lt;br /&gt;
In the phase space formulation of quantum mechanics,  one may consider the quantum Hamilton's equations for trajectories of quantum particles. These equations are infinite-order PDEs. However, in the semiclassical expansion, one has a finite system of ODEs at any fixed order of Dirac constant|.  The evolution equation of the Wigner function is also an infinite-order PDE. The quantum trajectories are quantum characteristics, with the use of which one could calculate the evolution of the Wigner function.&lt;br /&gt;
&lt;br /&gt;
在量子力学中的相空间表述中，我们可以考虑用于求解量子粒子的轨迹的量子哈密顿的方程。这些方程是无限阶偏微分方程。然而，在半经典展开中，我们在给定[[Dirac constant|{{mvar|ħ}}]]阶数下有一个有限的的常微分方程组。'''&amp;lt;font color=&amp;quot;#ff8000&amp;quot;&amp;gt;维格纳函数  Wigner Function&amp;lt;/font&amp;gt;的演化方程也是一个无限阶偏微分方程。由于量子轨道的量子特性，所以它通常可以用来计算维格纳函数的演化。&lt;br /&gt;
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== Analytical solutions ==&lt;br /&gt;
解析解&lt;br /&gt;
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===Separation of variables===&lt;br /&gt;
分离变量法&lt;br /&gt;
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{{main|Separable partial differential equation}}&lt;br /&gt;
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Linear PDEs can be reduced to systems of ordinary differential equations by the important technique of separation of variables. This technique rests on a characteristic of solutions to differential equations: if one can find any solution that solves the equation and satisfies the boundary conditions, then it is ''the'' solution (this also applies to ODEs). We assume as an [[ansatz]] that the dependence of a solution on the parameters space and time can be written as a product of terms that each depend on a single parameter, and then see if this can be made to solve the problem.&amp;lt;ref&amp;gt;{{cite book|last1=Gershenfeld|first1=Neil|title=The nature of mathematical modeling|date=2000|publisher=Cambridge Univ. Press|location=Cambridge|isbn=0521570956|page=27|edition=Reprinted (with corr.)}}&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
Linear PDEs can be reduced to systems of ordinary differential equations by the important technique of separation of variables. This technique rests on a characteristic of solutions to differential equations: if one can find any solution that solves the equation and satisfies the boundary conditions, then it is the solution (this also applies to ODEs). We assume as an ansatz that the dependence of a solution on the parameters space and time can be written as a product of terms that each depend on a single parameter, and then see if this can be made to solve the problem.&lt;br /&gt;
&lt;br /&gt;
线性偏微分方程组可以通过分离变量法这一重要方法来简化为常微分方程组。这种方法依赖于微分方程解的一个特征: 如果能找到任何一个满足方程和边界条件的解，那么这个解就是方程的解(这也适用于常微分方程)。我们假设解对参数空间和时间的依赖可以写成对它们每一项的依赖以及一个参数的乘积，然后再看看这是否可以用来解决这个问题。&lt;br /&gt;
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In the method of separation of variables, one reduces a PDE to a PDE in fewer variables, which is an ordinary differential equation if in one variable – these are in turn easier to solve.&lt;br /&gt;
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In the method of separation of variables, one reduces a PDE to a PDE in fewer variables, which is an ordinary differential equation if in one variable – these are in turn easier to solve.&lt;br /&gt;
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在分离变量法方法中，可以将偏微分方程简化为含有更少变量的偏微分方程，如果只有一个变量，那么就变成了一个'''&amp;lt;font color = &amp;quot;#ff8000&amp;quot;&amp;gt;常微分方程 Ordinary Differential Equation&amp;lt;/font&amp;gt;'''-- 反过来，这些方程也更容易求解。&lt;br /&gt;
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This is possible for simple PDEs, which are called [[separable partial differential equation]]s, and the domain is generally a rectangle (a product of intervals). Separable PDEs correspond to [[diagonal matrices]] – thinking of &amp;quot;the value for fixed {{mvar|x}}&amp;quot; as a coordinate, each coordinate can be understood separately.&lt;br /&gt;
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This is possible for simple PDEs, which are called separable partial differential equations, and the domain is generally a rectangle (a product of intervals). Separable PDEs correspond to diagonal matrices – thinking of &amp;quot;the value for fixed &amp;quot; as a coordinate, each coordinate can be understood separately.&lt;br /&gt;
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对于简单的偏微分方程(称为可分离偏微分方程)来说，这是可能的，而且方程通常定义在一个矩形区域(区间的乘积)上。可分离偏微分方程对应于对角线矩阵——以“固定值”为坐标，每个坐标可分开理解。&lt;br /&gt;
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This generalizes to the [[method of characteristics]], and is also used in [[integral transform]]s.&lt;br /&gt;
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This generalizes to the method of characteristics, and is also used in integral transforms.&lt;br /&gt;
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这种方法可以推广到特征曲线法，也可以用于积分变换。&lt;br /&gt;
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===Method of characteristics===&lt;br /&gt;
特征曲线法&lt;br /&gt;
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{{main|Method of characteristics}}&lt;br /&gt;
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In special cases, one can find characteristic curves on which the equation reduces to an ODE – changing coordinates in the domain to straighten these curves allows separation of variables, and is called the [[method of characteristics]].&lt;br /&gt;
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In special cases, one can find characteristic curves on which the equation reduces to an ODE – changing coordinates in the domain to straighten these curves allows separation of variables, and is called the method of characteristics.&lt;br /&gt;
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在特殊情况下，可以找到一些特征曲线，在这些曲线上方程可以变成一个常微分方程——意味着改变坐标从而使这些曲线变直从而达到分离变量的目的，这就是所谓的特征曲线法。&lt;br /&gt;
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More generally, one may find characteristic surfaces.&lt;br /&gt;
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More generally, one may find characteristic surfaces.&lt;br /&gt;
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更一般地说，人们可能会找到特征表面。&lt;br /&gt;
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===Integral transform===&lt;br /&gt;
积分变换&lt;br /&gt;
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An [[integral transform]] may transform the PDE to a simpler one, in particular, a separable PDE. This corresponds to diagonalizing an operator.&lt;br /&gt;
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An integral transform may transform the PDE to a simpler one, in particular, a separable PDE. This corresponds to diagonalizing an operator.&lt;br /&gt;
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积分变换可以将偏微分方程转换为更简单的偏微分方程，特别是可分离的偏微分方程。这对应于对角化算符。&lt;br /&gt;
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An important example of this is [[Fourier analysis]], which diagonalizes the heat equation using the [[eigenbasis]] of sinusoidal waves.&lt;br /&gt;
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An important example of this is Fourier analysis, which diagonalizes the heat equation using the eigenbasis of sinusoidal waves.&lt;br /&gt;
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这方面的一个重要例子是'''&amp;lt;font color = &amp;quot;#ff8000&amp;quot;&amp;gt;傅里叶分析  Fourier Analysis&amp;lt;/font&amp;gt;'''，它使用正弦波的特征基来对角化热方程。&lt;br /&gt;
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If the domain is finite or periodic, an infinite sum of solutions such as a [[Fourier series]] is appropriate, but an integral of solutions such as a [[Fourier integral]] is generally required for infinite domains. The solution for a point source for the heat equation given above is an example of the use of a Fourier integral.&lt;br /&gt;
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If the domain is finite or periodic, an infinite sum of solutions such as a Fourier series is appropriate, but an integral of solutions such as a Fourier integral is generally required for infinite domains. The solution for a point source for the heat equation given above is an example of the use of a Fourier integral.&lt;br /&gt;
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如果区域是有限的或周期性的，那么解为无限和的形式是恰当的，例如傅里叶级数，但是一个解的积分，例如傅立叶积分，一般是在无限区域上的。上面给出的热传导方程的点源解法就是使用傅里叶积分的一个例子。&lt;br /&gt;
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===Change of variables===&lt;br /&gt;
变量代换&lt;br /&gt;
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Often a PDE can be reduced to a simpler form with a known solution by a suitable [[Change of variables (PDE)|change of variables]].  For example, the [[Black–Scholes equation#Derivation|Black–Scholes]] PDE&lt;br /&gt;
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Often a PDE can be reduced to a simpler form with a known solution by a suitable change of variables.  For example, the Black–Scholes PDE&lt;br /&gt;
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偏微分方程通常可以通过变量的适当变化，用已知的解简化为更简单的形式。例如，布莱克-舒尔斯偏微分方程&lt;br /&gt;
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:&amp;lt;math&amp;gt; \frac{\partial V}{\partial t} + \tfrac{1}{2}\sigma^2 S^2\frac{\partial^2 V}{\partial S^2} + rS\frac{\partial V}{\partial S} - rV = 0 &amp;lt;/math&amp;gt;&lt;br /&gt;
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&amp;lt;math&amp;gt; \frac{\partial V}{\partial t} + \tfrac{1}{2}\sigma^2 S^2\frac{\partial^2 V}{\partial S^2} + rS\frac{\partial V}{\partial S} - rV = 0 &amp;lt;/math&amp;gt;&lt;br /&gt;
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is reducible to the [[heat equation]]&lt;br /&gt;
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is reducible to the heat equation&lt;br /&gt;
&lt;br /&gt;
可以简化为热传导方程&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt; \frac{\partial u}{\partial \tau} = \frac{\partial^2 u}{\partial x^2}&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \frac{\partial u}{\partial \tau} = \frac{\partial^2 u}{\partial x^2}&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
by the change of variables (for complete details see {{webarchive |url=https://web.archive.org/web/20080411030405/http://www.math.unl.edu/~sdunbar1/Teaching/MathematicalFinance/Lessons/BlackScholes/Solution/solution.shtml |date=April 11, 2008 |title=Solution of the Black Scholes Equation }})&lt;br /&gt;
&lt;br /&gt;
by the change of variables (for complete details see )&lt;br /&gt;
&lt;br /&gt;
通过变量替换(完整的细节见)&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt;\begin{align}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
V(S,t) &amp;amp;= K v(x,\tau),\\[5px]&lt;br /&gt;
&lt;br /&gt;
x &amp;amp;= \ln\left(\tfrac{S}{K} \right),\\[5px]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
\tau &amp;amp;= \tfrac{1}{2} \sigma^2 (T - t),\\[5px]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
v(x,\tau)&amp;amp;=e^{-\alpha x-\beta\tau} u(x,\tau).&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
\end{align}&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
===Fundamental solution===&lt;br /&gt;
基本解&lt;br /&gt;
&lt;br /&gt;
{{main|Fundamental solution}}&lt;br /&gt;
&lt;br /&gt;
Inhomogeneous equations can often be solved (for constant coefficient PDEs, always be solved) by finding the [[fundamental solution]] (the solution for a point source), then taking the [[convolution]] with the boundary conditions to get the solution.&lt;br /&gt;
&lt;br /&gt;
Inhomogeneous equations can often be solved (for constant coefficient PDEs, always be solved) by finding the fundamental solution (the solution for a point source), then taking the convolution with the boundary conditions to get the solution.&lt;br /&gt;
&lt;br /&gt;
非齐次方程(常系数偏微分方程)一般是通过先求出基本解(点源的解) ，然后利用带边界条件的卷积来求解。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
This is analogous in [[signal processing]] to understanding a filter by its [[impulse response]].&lt;br /&gt;
&lt;br /&gt;
This is analogous in signal processing to understanding a filter by its impulse response.&lt;br /&gt;
&lt;br /&gt;
这类似于在信号处理中通过滤波器的脉冲响应来理解滤波器。&lt;br /&gt;
&lt;br /&gt;
===Superposition principle===&lt;br /&gt;
叠加原理&lt;br /&gt;
&lt;br /&gt;
{{further| Superposition principle }}&lt;br /&gt;
&lt;br /&gt;
The superposition principle applies to any linear system, including linear systems of PDEs. A common visualization of this concept is the interaction of two waves in phase being combined to result in a greater amplitude, for example {{math|sin ''x'' + sin ''x'' {{=}} 2 sin ''x''}}. The same principle can be observed in PDEs where the solutions may be real or complex and additive. [[Superposition principle|superposition]]&lt;br /&gt;
&lt;br /&gt;
The superposition principle applies to any linear system, including linear systems of PDEs. A common visualization of this concept is the interaction of two waves in phase being combined to result in a greater amplitude, for example  2 sin x}}. The same principle can be observed in PDEs where the solutions may be real or complex and additive. superposition&lt;br /&gt;
&lt;br /&gt;
'''&amp;lt;font color = &amp;quot;#ff8000&amp;quot;&amp;gt;叠加原理 Superposition Principle&amp;lt;/font&amp;gt;适用于任何线性系统，包括偏微分方程的线性系统。这个概念的一个常见的可视化是两个同相位的波相互作用结合在一起会产生更大的振幅，例如 {{math|sin ''x'' + sin ''x'' {{=}} 2 sin ''x''}}。在偏微分方程中也可以观察到同样的原理，其中的解可能是真实的或复杂的和可加的。叠加&lt;br /&gt;
&lt;br /&gt;
If {{math|''u''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;}} and {{math|''u''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;}} are solutions of linear PDE in some function space {{mvar|R}}, then {{math|''u'' {{=}} ''c''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;''u''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; + ''c''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;''u''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;}} with any constants {{math|''c''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;}} and {{math|''c''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;}} are also a solution of that PDE in the same function space.&lt;br /&gt;
&lt;br /&gt;
If  and  are solutions of linear PDE in some function space , then  c&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;u&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; + c&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;u&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;}} with any constants  and  are also a solution of that PDE in the same function space.&lt;br /&gt;
&lt;br /&gt;
若线性偏微分方程在某个函数空间{{mvar|R}}中有解{{math|''u''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;}} 和 {{math|''u''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;}}，则{{math|''u'' {{=}} ''c''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;''u''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; + ''c''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;''u''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;}}也是该偏微分方程在同一函数空间中的解，其中{{math|''c''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;}} 和 {{math|''c''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;}} 是任意常数。&lt;br /&gt;
&lt;br /&gt;
===Methods for non-linear equations===&lt;br /&gt;
非线性方程的求解方法&lt;br /&gt;
{{see also|nonlinear partial differential equation}}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
There are no generally applicable methods to solve nonlinear PDEs. Still, existence and uniqueness results (such as the [[Cauchy–Kowalevski theorem]]) are often possible, as are proofs of important qualitative and quantitative properties of solutions (getting these results is a major part of [[mathematical analysis|analysis]]). Computational solution to the nonlinear PDEs, the [[split-step method]], exist for specific equations like [[nonlinear Schrödinger equation]].&lt;br /&gt;
&lt;br /&gt;
There are no generally applicable methods to solve nonlinear PDEs. Still, existence and uniqueness results (such as the Cauchy–Kowalevski theorem) are often possible, as are proofs of important qualitative and quantitative properties of solutions (getting these results is a major part of analysis). Computational solution to the nonlinear PDEs, the split-step method, exist for specific equations like nonlinear Schrödinger equation.&lt;br /&gt;
&lt;br /&gt;
对于非线性偏微分方程，目前还没有普遍适用的求解方法。然而，通常是可能知道解的存在性和唯一性(如柯西-科瓦列夫斯基定理)，也是可能得到解的重要定性和定量性质的证明(得到这些结果是分析的主要部分)。非线性偏微分方程的计算解，即分步法，对一些特定的方程适用，比如非线性'''&amp;lt;font color=&amp;quot;#ff8000&amp;quot;&amp;gt;薛定谔方程 Schrödinger equation&amp;lt;/font&amp;gt;'''。&lt;br /&gt;
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&lt;br /&gt;
&lt;br /&gt;
Nevertheless, some techniques can be used for several types of equations. The [[h-principle|{{mvar|h}}-principle]] is the most powerful method to solve [[Underdetermined system|underdetermined]] equations. The [[Riquier–Janet theory]] is an effective method for obtaining information about many analytic [[Overdetermined system|overdetermined]] systems.&lt;br /&gt;
&lt;br /&gt;
Nevertheless, some techniques can be used for several types of equations. The -principle is the most powerful method to solve underdetermined equations. The Riquier–Janet theory is an effective method for obtaining information about many analytic overdetermined systems.&lt;br /&gt;
&lt;br /&gt;
然而，一些技巧可以用于几种类型的方程。h-原理是求解欠定方程最有效的方法。里基尔-珍妮特理论是一种可以获得许多解析超定系统信息的有效方法。&lt;br /&gt;
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&lt;br /&gt;
&lt;br /&gt;
The [[method of characteristics]] can be used in some very special cases to solve partial differential equations.&lt;br /&gt;
&lt;br /&gt;
The method of characteristics can be used in some very special cases to solve partial differential equations.&lt;br /&gt;
&lt;br /&gt;
特征线法可用于求解某些特殊情况下的偏微分方程。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
In some cases, a PDE can be solved via [[perturbation analysis]] in which the solution is considered to be a correction to an equation with a known solution. Alternatives are [[numerical analysis]] techniques from simple [[finite difference]] schemes to the more mature [[multigrid]] and [[finite element method]]s. Many interesting problems in science and engineering are solved in this way using [[computer]]s, sometimes high performance [[supercomputer]]s.&lt;br /&gt;
&lt;br /&gt;
In some cases, a PDE can be solved via perturbation analysis in which the solution is considered to be a correction to an equation with a known solution. Alternatives are numerical analysis techniques from simple finite difference schemes to the more mature multigrid and finite element methods. Many interesting problems in science and engineering are solved in this way using computers, sometimes high performance supercomputers.&lt;br /&gt;
&lt;br /&gt;
在某些情况下，偏微分方程可以通过扰动分析来求解。在扰动分析中，通常是求解将具有已知解的方程修正后的新得到方程。可供选择的数值分析技术从简单的差分格式到更成熟的多重网格和有限元方法。许多有趣的科学和工程问题都是在计算机上用这种方法解决的，有时是高性能超级计算机。&lt;br /&gt;
&lt;br /&gt;
===Lie group method===&lt;br /&gt;
李群方法&lt;br /&gt;
&lt;br /&gt;
From 1870 [[Sophus Lie]]'s work put the theory of differential equations on a more satisfactory foundation. He showed that the integration theories of the older mathematicians can, by the introduction of what are now called [[Lie group]]s, be referred, to a common source; and that ordinary differential equations which admit the same [[infinitesimal transformation]]s present comparable difficulties of integration. He also emphasized the subject of [[contact transformation|transformations of contact]].&lt;br /&gt;
&lt;br /&gt;
From 1870 Sophus Lie's work put the theory of differential equations on a more satisfactory foundation. He showed that the integration theories of the older mathematicians can, by the introduction of what are now called Lie groups, be referred, to a common source; and that ordinary differential equations which admit the same infinitesimal transformations present comparable difficulties of integration. He also emphasized the subject of transformations of contact.&lt;br /&gt;
&lt;br /&gt;
从1870年起，索弗斯·李的工作为微分方程理论奠定了一个较为令人满意的基础。他指出，通过引入现在所谓的李群，老一辈数学家的积分理论可以引用到一个共同的来源; 承认相同的无穷小变换的常微分方程在积分方面存在相当的困难。他还强调了接触的转变这一主题。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==[[用户:Yuling|Yuling]]（[[用户讨论:Yuling|讨论]]）这句话“He also emphasized the subject of transformations of contact.”中的transformations of contact翻译的不太好。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
A general approach to solving PDEs uses the symmetry property of differential equations, the continuous [[infinitesimal transformation]]s of solutions to solutions ([[Lie theory]]). Continuous [[group theory]], [[Lie algebras]] and [[differential geometry]] are used to understand the structure of linear and nonlinear partial differential equations for generating integrable equations, to find its [[Lax pair]]s, recursion operators, [[Bäcklund transform]] and finally finding exact analytic solutions to the PDE.&lt;br /&gt;
&lt;br /&gt;
A general approach to solving PDEs uses the symmetry property of differential equations, the continuous infinitesimal transformations of solutions to solutions (Lie theory). Continuous group theory, Lie algebras and differential geometry are used to understand the structure of linear and nonlinear partial differential equations for generating integrable equations, to find its Lax pairs, recursion operators, Bäcklund transform and finally finding exact analytic solutions to the PDE.&lt;br /&gt;
&lt;br /&gt;
求解偏微分方程的一般方法是利用微分方程的对称性，即解到解的连续无穷小变换(李理论)。连续群论、李代数和微分几何理论被用来理解生成可积方程的线性和非线性偏微分方程的结构，找到它的Lax对、递归算子、 贝克伦德变换，最后找到偏微分方程的精确解析解。&lt;br /&gt;
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Symmetry methods have been recognized to study differential equations arising in mathematics, physics, engineering, and many other disciplines.&lt;br /&gt;
&lt;br /&gt;
Symmetry methods have been recognized to study differential equations arising in mathematics, physics, engineering, and many other disciplines.&lt;br /&gt;
&lt;br /&gt;
对称方法已被公认可以用于研究出现在数学，物理，工程和许多其他学科的微分方程。&lt;br /&gt;
&lt;br /&gt;
===Semianalytical methods===&lt;br /&gt;
半解析方法&lt;br /&gt;
&lt;br /&gt;
The [[Adomian decomposition method]], the [[Aleksandr Lyapunov|Lyapunov]] artificial small parameter method, and He's [[homotopy perturbation method]] are all special cases of the more general [[homotopy analysis method]]. These are series expansion methods, and except for the Lyapunov method, are independent of small physical parameters as compared to the well known [[perturbation theory]], thus giving these methods greater flexibility and solution generality.&lt;br /&gt;
&lt;br /&gt;
The Adomian decomposition method, the Lyapunov artificial small parameter method, and He's homotopy perturbation method are all special cases of the more general homotopy analysis method. These are series expansion methods, and except for the Lyapunov method, are independent of small physical parameters as compared to the well known perturbation theory, thus giving these methods greater flexibility and solution generality.&lt;br /&gt;
&lt;br /&gt;
阿多米安分解法、李雅普诺夫人工小参数方法和何同伦摄动方法都是更一般的同伦分析方法的特殊情况。除了李雅普诺夫方法之外，这些都是级数展开方法，与为人熟知的摄动理论方法相比，它们与小的物理参数无关，因此这些方法具有更大的灵活性和解的通用性。&lt;br /&gt;
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== Numerical solutions ==&lt;br /&gt;
数值解&lt;br /&gt;
&lt;br /&gt;
The three most widely used [[Numerical partial differential equations|numerical methods to solve PDEs]] are the [[finite element analysis|finite element method]] (FEM), [[finite volume method]]s (FVM) and [[finite difference method]]s (FDM), as well other kind of methods called [[Meshfree methods]], which were made to solve problems where the before mentioned methods are limited. The FEM has a prominent position among these methods and especially its exceptionally efficient higher-order version [[hp-FEM]]. Other hybrid versions of FEM and Meshfree methods include the generalized finite element method (GFEM), [[extended finite element method]] (XFEM), [[Spectral element method|spectral finite element method]] (SFEM), [[Meshfree methods|meshfree finite element method]], [[Discontinuous Galerkin Method|discontinuous Galerkin finite element method]] (DGFEM), [[Element-Free Galerkin Method]] (EFGM), [[Interpolating Element-Free Galerkin Method]] (IEFGM), etc.&lt;br /&gt;
&lt;br /&gt;
The three most widely used numerical methods to solve PDEs are the finite element method (FEM), finite volume methods (FVM) and finite difference methods (FDM), as well other kind of methods called Meshfree methods, which were made to solve problems where the before mentioned methods are limited. The FEM has a prominent position among these methods and especially its exceptionally efficient higher-order version hp-FEM. Other hybrid versions of FEM and Meshfree methods include the generalized finite element method (GFEM), extended finite element method (XFEM), spectral finite element method (SFEM), meshfree finite element method, discontinuous Galerkin finite element method (DGFEM), Element-Free Galerkin Method (EFGM), Interpolating Element-Free Galerkin Method (IEFGM), etc.&lt;br /&gt;
&lt;br /&gt;
求解偏微分方程最常用的三种数值方法是有限元分析法、有限体积法和有限差分法，以及其他一些称为无网格法的方法。这些方法用于解决前面提到的方法受到的限制。在这些方法中，有限元方法，尤其是高效的高阶有限元方法，占有重要地位。其他有限元法和无网格法的混合形式包括广义有限元分析法(GFEM)、扩展有限元分析法(XFEM)、谱有限元分析法(SFEM)、无网格有限元分析法(DGFEM)、间断伽辽金有限元分析法(DGFEM)、无网格伽辽金法(EFGM)、插值无网格伽辽金法(IEFGM)等。&lt;br /&gt;
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=== Finite element method ===&lt;br /&gt;
有限元分析法&lt;br /&gt;
&lt;br /&gt;
{{main|Finite element method}}&lt;br /&gt;
&lt;br /&gt;
The finite element method (FEM) (its practical application often known as finite element analysis (FEA)) is a numerical technique for finding approximate solutions of partial differential equations (PDE) as well as of integral equations. The solution approach is based either on eliminating the differential equation completely (steady state problems), or rendering the PDE into an approximating system of ordinary differential equations, which are then numerically integrated using standard techniques such as Euler's method, Runge–Kutta, etc.&lt;br /&gt;
&lt;br /&gt;
The finite element method (FEM) (its practical application often known as finite element analysis (FEA)) is a numerical technique for finding approximate solutions of partial differential equations (PDE) as well as of integral equations. The solution approach is based either on eliminating the differential equation completely (steady state problems), or rendering the PDE into an approximating system of ordinary differential equations, which are then numerically integrated using standard techniques such as Euler's method, Runge–Kutta, etc.&lt;br /&gt;
&lt;br /&gt;
'''&amp;lt;font color = &amp;quot;#ff8000&amp;quot;&amp;gt;有限元分析法 Finite Element Method&amp;lt;/font&amp;gt;''' ((其实际应用通常被称为有限元分析(FEA))是一种寻找偏微分方程(PDE)和积分方程近似解的数值技术。这种求解方法要么基于完全消除微分方程(稳态问题) ，要么将偏微分方程转化为常微分方程的近似系统，然后使用标准技术进行数值积分，如欧拉方法、 Runge-Kutta 等。&lt;br /&gt;
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===Finite difference method===&lt;br /&gt;
有限差分法&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{{main|Finite difference method}}&lt;br /&gt;
&lt;br /&gt;
Finite-difference methods are numerical methods for approximating the solutions to differential equations using [[finite difference]] equations to approximate derivatives.&lt;br /&gt;
&lt;br /&gt;
Finite-difference methods are numerical methods for approximating the solutions to differential equations using finite difference equations to approximate derivatives.&lt;br /&gt;
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有限差分法是一种数值方法，用差分方程近似微分方程的解。&lt;br /&gt;
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=== Finite volume method ===&lt;br /&gt;
有限体积法&lt;br /&gt;
&lt;br /&gt;
{{main|Finite volume method}}&lt;br /&gt;
&lt;br /&gt;
Similar to the finite difference method or finite element method, values are calculated at discrete places on a meshed geometry. &amp;quot;Finite volume&amp;quot; refers to the small volume surrounding each node point on a mesh. In the finite volume method, surface integrals in a partial differential equation that contain a divergence term are converted to volume integrals, using the [[divergence theorem]]. These terms are then evaluated as fluxes at the surfaces of each finite volume. Because the flux entering a given volume is identical to that leaving the adjacent volume, these methods conserve mass by design.&lt;br /&gt;
&lt;br /&gt;
Similar to the finite difference method or finite element method, values are calculated at discrete places on a meshed geometry. &amp;quot;Finite volume&amp;quot; refers to the small volume surrounding each node point on a mesh. In the finite volume method, surface integrals in a partial differential equation that contain a divergence term are converted to volume integrals, using the divergence theorem. These terms are then evaluated as fluxes at the surfaces of each finite volume. Because the flux entering a given volume is identical to that leaving the adjacent volume, these methods conserve mass by design.&lt;br /&gt;
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类似于有限差分法或有限元分析，函数值是在网状几何体上的离散位置进行计算的。“有限体积”是指网格上每个节点周围的小体积。在有限体积法中，偏微分方程中含有散度项的面积分用散度定理积分转换成体积分。然后将这些项用于估算每个有限体积表面上的通量。由于进入给定体积的通量与转移到相邻体积元的通量相同，所以这些方法在设计上保证了质量守恒。&lt;br /&gt;
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==See also==&lt;br /&gt;
请参阅&lt;br /&gt;
* [[Dirichlet boundary condition]]&lt;br /&gt;
狄利克雷边界条件&lt;br /&gt;
* [[Jet bundle]]&lt;br /&gt;
射流丛&lt;br /&gt;
* [[Laplace transform applied to differential equations]]&lt;br /&gt;
微分方程中的拉普拉斯变换&lt;br /&gt;
* [[List of dynamical systems and differential equations topics]]&lt;br /&gt;
动力学系统和微分方程的列表&lt;br /&gt;
* [[Matrix differential equation]]&lt;br /&gt;
矩阵微分方程&lt;br /&gt;
* [[Neumann boundary condition]]&lt;br /&gt;
诺伊曼边界条件&lt;br /&gt;
* [[Numerical partial differential equations]]&lt;br /&gt;
数值偏微分方程&lt;br /&gt;
* [[Partial differential algebraic equation]]&lt;br /&gt;
偏微分代数方程&lt;br /&gt;
* [[Recurrence relation]]&lt;br /&gt;
递推关系&lt;br /&gt;
* [[Robin boundary condition]]&lt;br /&gt;
罗宾边界条件&lt;br /&gt;
* [[Stochastic processes and boundary value problems]]&lt;br /&gt;
随机过程和边值问题&lt;br /&gt;
&lt;br /&gt;
== The energy method ==&lt;br /&gt;
能量法&lt;br /&gt;
&lt;br /&gt;
The energy method is a mathematical procedure that can be used to verify well-posedness of initial-boundary-value-problems.&amp;lt;ref&amp;gt;{{cite book |title=High Order Difference Methods for Time Dependent PDE&lt;br /&gt;
&lt;br /&gt;
The energy method is a mathematical procedure that can be used to verify well-posedness of initial-boundary-value-problems.&amp;lt;ref&amp;gt;{{cite book |title=High Order Difference Methods for Time Dependent PDE&lt;br /&gt;
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能量法是验证初边值问题适定性的一种数学方法。 时变偏微分方程的高阶差分方法&lt;br /&gt;
&lt;br /&gt;
|first=Bertil|last=Gustafsson|publisher=Springer|year=2008|isbn=978-3-540-74992-9|doi=10.1007/978-3-540-74993-6}}&amp;lt;/ref&amp;gt; In the following example the energy method is used to decide where and which boundary conditions should be imposed such that the resulting IBVP is well-posed. Consider the one-dimensional hyperbolic PDE given by&lt;br /&gt;
&lt;br /&gt;
|first=Bertil|last=Gustafsson|publisher=Springer|year=2008|isbn=978-3-540-74992-9|doi=10.1007/978-3-540-74993-6}}&amp;lt;/ref&amp;gt; In the following example the energy method is used to decide where and which boundary conditions should be imposed such that the resulting IBVP is well-posed. Consider the one-dimensional hyperbolic PDE given by&lt;br /&gt;
&lt;br /&gt;
| first Bertil | last Gustafsson | publisher | Springer | year 2008 | isbn 978-3-540-74992-9 | doi 10.1007 / 978-3-540-74993-6} / ref 在下面的例子中，使用能量方法来决定应该施加哪些边界条件，使得得到的 IBVP适定。考虑一维双曲偏微分方程&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt;\frac{\partial u}{\partial t} + \alpha \frac{\partial u}{\partial x} = 0, \quad x \in [a,b], \operatorname t &amp;gt; 0,&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;\frac{\partial u}{\partial t} + \alpha \frac{\partial u}{\partial x} = 0, \quad x \in [a,b], \operatorname t &amp;gt; 0,&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
where &amp;lt;math&amp;gt;\alpha \neq 0&amp;lt;/math&amp;gt; is a constant and &amp;lt;math&amp;gt;u(x,t)&amp;lt;/math&amp;gt; is an unknown function with initial condition &amp;lt;math&amp;gt;u(x,0) = f(x)&amp;lt;/math&amp;gt;. Multiplying with &amp;lt;math&amp;gt;u&amp;lt;/math&amp;gt; and integrating over the domain gives&lt;br /&gt;
&lt;br /&gt;
where &amp;lt;math&amp;gt;\alpha \neq 0&amp;lt;/math&amp;gt; is a constant and &amp;lt;math&amp;gt;u(x,t)&amp;lt;/math&amp;gt; is an unknown function with initial condition &amp;lt;math&amp;gt;u(x,0) = f(x)&amp;lt;/math&amp;gt;. Multiplying with &amp;lt;math&amp;gt;u&amp;lt;/math&amp;gt; and integrating over the domain gives&lt;br /&gt;
&lt;br /&gt;
其中 &amp;lt;math&amp;gt;\alpha \neq 0&amp;lt;/math&amp;gt; 是常数，并且 &amp;lt;math&amp;gt;u(x,t)&amp;lt;/math&amp;gt; 是未知函数，初始条件是 &amp;lt;math&amp;gt;u(x,0) = f(x)&amp;lt;/math&amp;gt;。乘以 &amp;lt;math&amp;gt;u&amp;lt;/math&amp;gt; 并在域上进行积分。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt;\int_a^b u \frac{\partial u}{\partial t} \operatorname dx + \alpha \int _a ^b u \frac{\partial u}{\partial x} \operatorname dx = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;\int_a^b u \frac{\partial u}{\partial t} \operatorname dx + \alpha \int _a ^b u \frac{\partial u}{\partial x} \operatorname dx = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Using that&lt;br /&gt;
&lt;br /&gt;
Using that&lt;br /&gt;
&lt;br /&gt;
利用这一点&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt;\int _a ^b u \frac{\partial u}{\partial t} \operatorname dx = \frac{1}{2} \frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 \quad \text{and} \quad \int _a ^b u \frac{\partial u}{\partial x} \operatorname dx = \frac{1}{2} u(b,t)^2 - \frac{1}{2} u(a,t)^2,.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;\int _a ^b u \frac{\partial u}{\partial t} \operatorname dx = \frac{1}{2} \frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 \quad \text{and} \quad \int _a ^b u \frac{\partial u}{\partial x} \operatorname dx = \frac{1}{2} u(b,t)^2 - \frac{1}{2} u(a,t)^2,.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
where integration by parts has been used for the second relationship, we get&lt;br /&gt;
&lt;br /&gt;
where integration by parts has been used for the second relationship, we get&lt;br /&gt;
&lt;br /&gt;
第二个关系中采用了分部积分法，我们可以得到&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt;\frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 + \alpha u(b,t)^2 - \alpha u(a,t)^2 = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;\frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 + \alpha u(b,t)^2 - \alpha u(a,t)^2 = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Here &amp;lt;math&amp;gt;\vert \vert \cdot \vert \vert&amp;lt;/math&amp;gt; denotes the standard L2-norm.&lt;br /&gt;
&lt;br /&gt;
Here &amp;lt;math&amp;gt;\vert \vert \cdot \vert \vert&amp;lt;/math&amp;gt; denotes the standard L2-norm.&lt;br /&gt;
&lt;br /&gt;
在这里，&amp;lt;math&amp;gt;\vert \vert \cdot \vert \vert&amp;lt;/math&amp;gt; 表示标准的 L2-正则。&lt;br /&gt;
&lt;br /&gt;
For well-posedness we require that the energy of the solution is non-increasing, i.e. that &amp;lt;math&amp;gt;\frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 \leq 0&amp;lt;/math&amp;gt;, which is achieved by specifying &amp;lt;math&amp;gt;u&amp;lt;/math&amp;gt; at &amp;lt;math&amp;gt;x = a&amp;lt;/math&amp;gt; if &amp;lt;math&amp;gt;\alpha &amp;gt; 0&amp;lt;/math&amp;gt; and at &amp;lt;math&amp;gt;x = b&amp;lt;/math&amp;gt; if &amp;lt;math&amp;gt;\alpha &amp;lt; 0&amp;lt;/math&amp;gt;. This corresponds to only imposing boundary conditions at the inflow. Note that well-posedness allows for growth in terms of data (initial and boundary) and thus it is sufficient to show that &amp;lt;math&amp;gt;\frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 \leq 0&amp;lt;/math&amp;gt; holds when all data is set to zero.&lt;br /&gt;
&lt;br /&gt;
For well-posedness we require that the energy of the solution is non-increasing, i.e. that &amp;lt;math&amp;gt;\frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 \leq 0&amp;lt;/math&amp;gt;, which is achieved by specifying &amp;lt;math&amp;gt;u&amp;lt;/math&amp;gt; at &amp;lt;math&amp;gt;x = a&amp;lt;/math&amp;gt; if &amp;lt;math&amp;gt;\alpha &amp;gt; 0&amp;lt;/math&amp;gt; and at &amp;lt;math&amp;gt;x = b&amp;lt;/math&amp;gt; if &amp;lt;math&amp;gt;\alpha &amp;lt; 0&amp;lt;/math&amp;gt;. This corresponds to only imposing boundary conditions at the inflow. Note that well-posedness allows for growth in terms of data (initial and boundary) and thus it is sufficient to show that &amp;lt;math&amp;gt;\frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 \leq 0&amp;lt;/math&amp;gt; holds when all data is set to zero.&lt;br /&gt;
&lt;br /&gt;
对于适定性，我们要解的能量是不增加的，即 &amp;lt;math&amp;gt;\frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 \leq 0&amp;lt;/math&amp;gt; ，这种关系可以通过在&amp;lt;math&amp;gt;x = a&amp;lt;/math&amp;gt;处 （如果 &amp;lt;math&amp;gt;\alpha &amp;gt; 0&amp;lt;/math&amp;gt;） 以及 &amp;lt;math&amp;gt;x = b&amp;lt;/math&amp;gt;处 （如果 &amp;lt;math&amp;gt;\alpha &amp;lt; 0&amp;lt;/math&amp;gt;）指定&amp;lt;math&amp;gt;u&amp;lt;/math&amp;gt;的值来实现。这只相当于在入流处附加边界条件。注意，适定性允许在数据(初始和边界)上的增长，因此它足以表明当所有数据设置为零时应有 &amp;lt;math&amp;gt;\frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 \leq 0&amp;lt;/math&amp;gt;。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==[[用户:Yuling|Yuling]]（[[用户讨论:Yuling|讨论]]）“This corresponds to only imposing boundary conditions at the inflow.” 这句话中的inflow不是很理解&lt;br /&gt;
&lt;br /&gt;
==Notes==&lt;br /&gt;
&lt;br /&gt;
{{Reflist}}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
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| first Bertil | last Gustafsson | Springer | year 2008 | isbn 978-3-540-74992-9 | doi 10.1007 / 978-3-540-74993-6}&lt;br /&gt;
&lt;br /&gt;
{{refend}}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
== Further reading ==&lt;br /&gt;
&lt;br /&gt;
* {{Cite journal|last=Cajori|first=Florian|authorlink=Florian Cajori|year=1928|title=The Early History of Partial Differential Equations and of Partial Differentiation and Integration|url=http://www.math.harvard.edu/archive/21a_fall_14/exhibits/cajori/cajori.pdf|journal=The American Mathematical Monthly|volume=35|issue=9|pages=459–467|doi=10.2307/2298771|access-date=2016-05-15|archive-url=https://web.archive.org/web/20181123102253/http://www.math.harvard.edu/archive/21a_fall_14/exhibits/cajori/cajori.pdf|archive-date=2018-11-23|url-status=dead}}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
== External links ==&lt;br /&gt;
&lt;br /&gt;
{{Sister project links| wikt=no | commons=Category:Solutions of PDE | b=Partial Differential Equations | n=no | q=Partial differential equation | s=no | v=no | voy=no | species=no | d=no}}&lt;br /&gt;
&lt;br /&gt;
* {{springer|title=Differential equation, partial|id=p/d031920}}&lt;br /&gt;
&lt;br /&gt;
* [http://eqworld.ipmnet.ru/en/pde-en.htm Partial Differential Equations: Exact Solutions] at EqWorld: The World of Mathematical Equations.&lt;br /&gt;
&lt;br /&gt;
* [http://eqworld.ipmnet.ru/en/solutions/eqindex/eqindex-pde.htm Partial Differential Equations: Index] at EqWorld: The World of Mathematical Equations.&lt;br /&gt;
&lt;br /&gt;
* [http://eqworld.ipmnet.ru/en/methods/meth-pde.htm Partial Differential Equations: Methods] at EqWorld: The World of Mathematical Equations.&lt;br /&gt;
&lt;br /&gt;
* [https://web.archive.org/web/20170701144823/http://www.exampleproblems.com/wiki/index.php?title=Partial_Differential_Equations Example problems with solutions] at exampleproblems.com&lt;br /&gt;
&lt;br /&gt;
* [http://mathworld.wolfram.com/PartialDifferentialEquation.html Partial Differential Equations] at mathworld.wolfram.com&lt;br /&gt;
&lt;br /&gt;
* [https://reference.wolfram.com/language/FEMDocumentation/tutorial/SolvingPDEwithFEM.html Partial Differential Equations] with Mathematica&lt;br /&gt;
&lt;br /&gt;
* [http://www.mathworks.com/moler/pdes.pdf Partial Differential Equations] in Cleve Moler: Numerical Computing with MATLAB&lt;br /&gt;
&lt;br /&gt;
* [http://www.nag.com/numeric/fl/nagdoc_fl24/html/D03/d03intro.html Partial Differential Equations] at nag.com&lt;br /&gt;
&lt;br /&gt;
* {{cite web |first=Grant |last=Sanderson |title=But what is a partial differential equation? |work=3Blue1Brown |date=April 21, 2019 |url=https://www.youtube.com/watch?v=ly4S0oi3Yz8&amp;amp;list=PLZHQObOWTQDNPOjrT6KVlfJuKtYTftqH6 |via=[[YouTube]] }}&lt;br /&gt;
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{{Differential equations topics}}&lt;br /&gt;
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&amp;lt;small&amp;gt;This page was moved from [[wikipedia:en:Partial differential equation]]. Its edit history can be viewed at [[偏微分方程/edithistory]]&amp;lt;/small&amp;gt;&amp;lt;/noinclude&amp;gt;&lt;br /&gt;
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[[Category:待整理页面]]&lt;/div&gt;</summary>
		<author><name>Ruili</name></author>
	</entry>
	<entry>
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		<title>偏微分方程</title>
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		<updated>2020-11-11T14:22:31Z</updated>

		<summary type="html">&lt;p&gt;Ruili：&lt;/p&gt;
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&lt;div&gt;此词条暂由Yuling翻译，未经人工整理和审校，带来阅读不便，请见谅。&lt;br /&gt;
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[[File:Heat.gif|thumb|right|A visualisation of a solution to the two-dimensional [[heat equation]] with temperature represented by the third dimension]]&lt;br /&gt;
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A visualisation of a solution to the two-dimensional [[heat equation with temperature represented by the third dimension]]&lt;br /&gt;
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以三维表示温度的二维热方程解的可视化&lt;br /&gt;
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In [[mathematics]], a '''partial differential equation''' ('''PDE''') is a [[differential equation]] that contains unknown [[Multivariable calculus|multivariable functions]] and their [[partial derivative]]s. PDEs are used to formulate problems involving functions of several variables, and are either solved by hand, or used to create a [[computer model]]. A special case is [[ordinary differential equation]]s (ODEs), which deal with functions of a single variable and their derivatives.&lt;br /&gt;
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In mathematics, a partial differential equation (PDE) is a differential equation that contains unknown multivariable functions and their partial derivatives. PDEs are used to formulate problems involving functions of several variables, and are either solved by hand, or used to create a computer model. A special case is ordinary differential equations (ODEs), which deal with functions of a single variable and their derivatives.&lt;br /&gt;
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在数学中，'''&amp;lt;font color = &amp;quot;#ff8000&amp;quot;&amp;gt; 偏微分方程函数 Partial Differential Equation&amp;lt;/font&amp;gt;'''是包含未知多元函数及其偏导数的微分方程。偏微分方程用于描述涉及多元函数的问题，可以通过人为求解，也可以通过建立计算机模型来求解。常微分方程是偏微分方程一种特殊情况，它处理的是一元函数及其导数。&lt;br /&gt;
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PDEs can be used to describe a wide variety of phenomena such as sound, heat, [[diffusion]], [[electrostatics]], [[Electromagnetism|electrodynamics]], [[fluid dynamics]], [[Elasticity (physics)|elasticity]], [[gravitation]] and [[quantum mechanics]]. These seemingly distinct physical phenomena can be formalised similarly in terms of PDEs. Just as ordinary differential equations often model one-dimensional [[dynamical system]]s, partial differential equations often model [[multidimensional system]]s. PDEs find their generalisation in [[stochastic partial differential equation]]s.&lt;br /&gt;
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PDEs can be used to describe a wide variety of phenomena such as sound, heat, diffusion, electrostatics, electrodynamics, fluid dynamics, elasticity, gravitation and quantum mechanics. These seemingly distinct physical phenomena can be formalised similarly in terms of PDEs. Just as ordinary differential equations often model one-dimensional dynamical systems, partial differential equations often model multidimensional systems. PDEs find their generalisation in stochastic partial differential equations.&lt;br /&gt;
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偏微分方程可以用来描述各种各样的物理现象，如声音，热量，扩散，静电，电动力学，流体力学，弹性力学，重力和量子力学。这些看起来截然不同的物理现象却可以用类似的偏微分方程来描述。正如常微分方程经常对一维动力系统进行建模一样，偏微分方程经常对多维系统进行建模。随机偏微分方程是偏微分方程的一种推广。&lt;br /&gt;
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== Introduction ==&lt;br /&gt;
引言&lt;br /&gt;
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Partial differential equations (PDEs) are equations that involve rates of change with respect to [[continuous variables]]. For example, the position of a [[rigid body]] is specified by six parameters,&amp;lt;ref&amp;gt;{{Cite book|url=https://books.google.com/books?id=v9PLbcYd9aUC&amp;amp;pg=PA32|title=Modelling and Control of Robot Manipulators|last=Sciavicco|first=Lorenzo|last2=Siciliano|first2=Bruno|date=2001-02-19|publisher=Springer Science &amp;amp; Business Media|isbn=9781852332211|language=en}}&amp;lt;/ref&amp;gt; but the configuration of a [[fluid]] is given by the [[continuous distribution]] of several parameters, such as the [[temperature]], [[pressure]], and so forth. The dynamics for the rigid body take place in a finite-dimensional [[Configuration space (physics)|configuration space]]; the dynamics for the fluid occur in an infinite-dimensional configuration space. This distinction usually makes PDEs much harder to solve than ordinary differential equations (ODEs), but here again, there will be simple solutions for linear problems. Classic domains where PDEs are used include [[acoustics]], [[fluid dynamics]], [[electrodynamics]], and [[heat transfer]].&lt;br /&gt;
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Partial differential equations (PDEs) are equations that involve rates of change with respect to continuous variables. For example, the position of a rigid body is specified by six parameters, but the configuration of a fluid is given by the continuous distribution of several parameters, such as the temperature, pressure, and so forth. The dynamics for the rigid body take place in a finite-dimensional configuration space; the dynamics for the fluid occur in an infinite-dimensional configuration space. This distinction usually makes PDEs much harder to solve than ordinary differential equations (ODEs), but here again, there will be simple solutions for linear problems. Classic domains where PDEs are used include acoustics, fluid dynamics, electrodynamics, and heat transfer.&lt;br /&gt;
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偏微分方程(简称为PDEs)涉及到方程相对于连续变量的变化率。例如，刚体的位置是由六个参数确定的，而流体的状态是由几个参数的连续分布给出的，如温度、压力等。刚体的动力学过程发生在有限维状态空间中，流体的动力学过程发生在无限维状态空间中。这种区别通常使偏微分方程比常微分方程更难求解，但是线性问题仍然有简单的求解方式。使用偏微分方程的经典领域包括声学、流体力学、电动力学和传热学。&lt;br /&gt;
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A partial differential equation (PDE) for the function {{math|''u''(''x''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;,… ''x&amp;lt;sub&amp;gt;n&amp;lt;/sub&amp;gt;'')}} is an equation of the form&lt;br /&gt;
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A partial differential equation (PDE) for the function  is an equation of the form&lt;br /&gt;
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函数 {{math|''u''(''x''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;,… ''x&amp;lt;sub&amp;gt;n&amp;lt;/sub&amp;gt;'')}} 的偏微分方程形式是：&lt;br /&gt;
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: &amp;lt;math&amp;gt;f \left (x_1, \ldots x_n; u, \frac{\partial u}{\partial x_1}, \ldots \frac{\partial u}{\partial x_n}; \frac{\partial^2 u}{\partial x_1 \partial x_1}, \ldots \frac{\partial^2 u}{\partial x_1 \partial x_n}; \ldots \right) = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;f \left (x_1, \ldots x_n; u, \frac{\partial u}{\partial x_1}, \ldots \frac{\partial u}{\partial x_n}; \frac{\partial^2 u}{\partial x_1 \partial x_1}, \ldots \frac{\partial^2 u}{\partial x_1 \partial x_n}; \ldots \right) = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
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If {{mvar|f}} is a [[linear function]] of {{mvar|u}} and its derivatives, then the PDE is called linear. Common examples of linear PDEs include the [[heat equation]], the [[wave equation]], [[Laplace's equation]], [[Helmholtz equation]], [[Klein–Gordon equation]], and [[Poisson's equation]].&lt;br /&gt;
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If  is a linear function of  and its derivatives, then the PDE is called linear. Common examples of linear PDEs include the heat equation, the wave equation, Laplace's equation, Helmholtz equation, Klein–Gordon equation, and Poisson's equation.&lt;br /&gt;
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如果 {{mvar|f}} 是函数 {{math|''u''}} 及其导数的线性函数，则偏微分方程称为线性函数。线性偏微分方程的常见例子包括热方程、波动方程、拉普拉斯方程、亥姆霍兹方程方程、克莱因-高登方程和泊松方程。&lt;br /&gt;
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A relatively simple PDE is&lt;br /&gt;
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A relatively simple PDE is&lt;br /&gt;
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一个相对简单的偏微分方程：&lt;br /&gt;
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: &amp;lt;math&amp;gt;\frac{\partial u}{\partial x}(x,y) = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;\frac{\partial u}{\partial x}(x,y) = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
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This relation [[Logical implication|implies]] that the function {{math|''u''(''x'',''y'')}} is independent of {{mvar|x}}. However, the equation gives no information on the function's dependence on the variable {{mvar|y}}. Hence the general solution of this equation is&lt;br /&gt;
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This relation implies that the function  is independent of . However, the equation gives no information on the function's dependence on the variable . Hence the general solution of this equation is&lt;br /&gt;
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这意味着函数 {{math|''u''(''x'',''y'')}} 独立于 {{mvar|x}} 的。然而，这个方程没有给出关于函数和自变量的相关性的信息。因此，这个方程的通解是&lt;br /&gt;
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: &amp;lt;math&amp;gt;u(x,y) = f(y),&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;u(x,y) = f(y),&amp;lt;/math&amp;gt;&lt;br /&gt;
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where {{mvar|f}} is an arbitrary function of {{mvar|y}}. The analogous ordinary differential equation is&lt;br /&gt;
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where  is an arbitrary function of . The analogous ordinary differential equation is&lt;br /&gt;
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其中， {{mvar|f}} 是 {{mvar|y}} 的任意函数。&lt;br /&gt;
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类似的常微分方程是：&lt;br /&gt;
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: &amp;lt;math&amp;gt;\frac{\mathrm{d} u}{\mathrm{d} x}(x) = 0,&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;\frac{\mathrm{d} u}{\mathrm{d} x}(x) = 0,&amp;lt;/math&amp;gt;&lt;br /&gt;
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which has the solution&lt;br /&gt;
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which has the solution&lt;br /&gt;
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它的解为&lt;br /&gt;
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: &amp;lt;math&amp;gt;u(x) = c,&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;u(x) = c,&amp;lt;/math&amp;gt;&lt;br /&gt;
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where {{mvar|c}} is any [[Constant (mathematics)|constant]] value. These two examples illustrate that general solutions of ordinary differential equations (ODEs) involve arbitrary constants, but solutions of PDEs involve arbitrary functions.&lt;br /&gt;
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where  is any constant value. These two examples illustrate that general solutions of ordinary differential equations (ODEs) involve arbitrary constants, but solutions of PDEs involve arbitrary functions.&lt;br /&gt;
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这里，{{mvar|c}} 是一个任意常量。&lt;br /&gt;
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这两个例子说明常微分方程的一般解包含任意常数，但偏微分方程的解包含任意函数。&lt;br /&gt;
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A solution of a PDE is generally not [[Uniqueness quantification|unique]]; additional conditions must generally be specified on the [[Boundary (topology)|boundary]] of the region where the solution is defined. For instance, in the simple example above, the function {{math|''f''(''y'')}} can be determined if {{mvar|u}} is specified on the line {{math|''x'' {{=}} 0}}.&lt;br /&gt;
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A solution of a PDE is generally not unique; additional conditions must generally be specified on the boundary of the region where the solution is defined. For instance, in the simple example above, the function  can be determined if  is specified on the line  0}}.&lt;br /&gt;
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偏微分方程的解一般不是唯一的; 一般必须在定义解的区域边界上定义附加条件。 例如，在上面的简单示例中，如果在 {{math|''x'' {{=}} 0}} 时确定了 {{mvar|u}} 的值，则可以确定该函数 {{math|''f''(''y'')}}。&lt;br /&gt;
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== Existence and uniqueness ==&lt;br /&gt;
存在性和唯一性&lt;br /&gt;
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Although the issue of existence and uniqueness of solutions of ordinary differential equations has a very satisfactory answer with the [[Picard–Lindelöf theorem]], that is far from the case for partial differential equations. The [[Cauchy–Kowalevski theorem]] states that the [[Cauchy problem]] for any partial differential equation whose coefficients are [[Analytic function|analytic]] in the unknown function and its derivatives, has a locally unique analytic solution. Although this result might appear to settle the existence and uniqueness of solutions, there are examples of linear partial differential equations whose coefficients have derivatives of all orders (which are nevertheless not analytic) but which have no solutions at all: see [[Lewy's example|Lewy (1957)]]. Even if the solution of a partial differential equation exists and is unique, it may nevertheless have undesirable properties.  The mathematical study of these questions is usually in the more powerful context of [[weak solution]]s.&lt;br /&gt;
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Although the issue of existence and uniqueness of solutions of ordinary differential equations has a very satisfactory answer with the Picard–Lindelöf theorem, that is far from the case for partial differential equations. The Cauchy–Kowalevski theorem states that the Cauchy problem for any partial differential equation whose coefficients are analytic in the unknown function and its derivatives, has a locally unique analytic solution. Although this result might appear to settle the existence and uniqueness of solutions, there are examples of linear partial differential equations whose coefficients have derivatives of all orders (which are nevertheless not analytic) but which have no solutions at all: see Lewy (1957). Even if the solution of a partial differential equation exists and is unique, it may nevertheless have undesirable properties.  The mathematical study of these questions is usually in the more powerful context of weak solutions.&lt;br /&gt;
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尽管常微分方程解的存在性和唯一性用'''&amp;lt;font color=&amp;quot;#ff8000&amp;quot;&amp;gt;弗罗贝尼乌斯定理 Picard–Lindelöf Theorem&amp;lt;/font&amp;gt;得到了令人满意的结果，但偏微分方程解的存在性和唯一性却远没有得到解决。'''&amp;lt;font color=&amp;quot;#ff8000&amp;quot;&amp;gt;柯西-科瓦列夫斯基定理 Cauchy–Kowalevski theorem&amp;lt;/font&amp;gt;指出：对于任意系数在未知函数及其导数中解析的偏微分方程，柯西问题存在一个局部唯一的解析解。虽然这个结果似乎解决了解的存在性和唯一性问题，但是存在一些线性偏微分方程-其系数具有所有级数的导数(尽管这些导数不是解析的) ，但是根本没有解: 见 Lewy (1957)。即使偏微分方程的解存在且唯一，它仍然可能具有不可预料的性质。这些问题的数学研究通常是在更有力的弱解的背景下进行的。&lt;br /&gt;
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An example of pathological behavior is the sequence (depending upon {{mvar|n}}) of [[Cauchy problem]]s for the [[Laplace equation]]&lt;br /&gt;
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An example of pathological behavior is the sequence (depending upon ) of Cauchy problems for the Laplace equation&lt;br /&gt;
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反常特征的一个例子是拉普拉斯方程的柯西问题的序列(取决于{{mvar|n}})&lt;br /&gt;
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: &amp;lt;math&amp;gt;\frac{\partial^2 u}{\partial x^2} + \frac{\partial^2 u}{\partial y^2}=0,&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;\frac{\partial^2 u}{\partial x^2} + \frac{\partial^2 u}{\partial y^2}=0,&amp;lt;/math&amp;gt;&lt;br /&gt;
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with [[boundary condition]]s&lt;br /&gt;
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with boundary conditions&lt;br /&gt;
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具有边界条件&lt;br /&gt;
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: &amp;lt;math&amp;gt;\begin{align} u(x,0) &amp;amp;= 0, \\ \frac{\partial u}{\partial y}(x,0) &amp;amp;= \frac{\sin nx}{n}, \end{align}&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;\begin{align} u(x,0) &amp;amp;= 0, \\ \frac{\partial u}{\partial y}(x,0) &amp;amp;= \frac{\sin nx}{n}, \end{align}&amp;lt;/math&amp;gt;&lt;br /&gt;
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where {{mvar|n}} is an integer. The derivative of {{mvar|u}} with respect to {{mvar|y}} approaches zero [[uniform convergence|uniformly]] in {{mvar|x}} as {{mvar|n}} increases, but the solution is&lt;br /&gt;
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where  is an integer. The derivative of  with respect to  approaches zero uniformly in  as  increases, but the solution is&lt;br /&gt;
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其中{{mvar|n}}是整数。{{mvar|u}}是关于{{mvar|y}}的导数，一致地随着{{mvar|n}}的增加而趋于零，但是解是&lt;br /&gt;
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: &amp;lt;math&amp;gt;u(x,y) = \frac{\sinh ny \sin nx}{n^2}.&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;u(x,y) = \frac{\sinh ny \sin nx}{n^2}.&amp;lt;/math&amp;gt;&lt;br /&gt;
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This solution approaches infinity if {{mvar|nx}} is not an integer multiple of {{pi}} for any non-zero value of {{mvar|y}}. The Cauchy problem for the Laplace equation is called ''ill-posed'' or ''not [[Well-posed problem|well-posed]]'', since the solution does not continuously depend on the data of the problem. Such ill-posed problems are not usually satisfactory for physical applications.&lt;br /&gt;
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This solution approaches infinity if  is not an integer multiple of  for any non-zero value of . The Cauchy problem for the Laplace equation is called ill-posed or not well-posed, since the solution does not continuously depend on the data of the problem. Such ill-posed problems are not usually satisfactory for physical applications.&lt;br /&gt;
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对于任何非零的{{mvar|y}}，如果{{mvar|nx}}不是{{pi}}的整数倍，这个解会接近于无穷大。拉普拉斯方程的柯西问题被称为不适定问题（可以译为ill-posed或not well-posed），因为该问题的解并不连续地依赖于该问题的数据。这种不适定问题在物理应用中通常不能令人满意。&lt;br /&gt;
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The [[Navier–Stokes existence and smoothness|existence of solutions for the Navier–Stokes equations]], a partial differential equation, is part of one of the [[Millennium Prize Problems]].&lt;br /&gt;
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The existence of solutions for the Navier–Stokes equations, a partial differential equation, is part of one of the Millennium Prize Problems.&lt;br /&gt;
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一种偏微分方程——纳维-斯托克斯方程——的解的存在性就是千禧年大奖难题的一部分。&lt;br /&gt;
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== Notation ==&lt;br /&gt;
符号&lt;br /&gt;
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In PDEs, it is common to denote partial derivatives using subscripts. That is:&lt;br /&gt;
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In PDEs, it is common to denote partial derivatives using subscripts. That is:&lt;br /&gt;
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在偏微分方程中，通常用下标表示偏导数。例如:&lt;br /&gt;
&lt;br /&gt;
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: &amp;lt;math&amp;gt;u_x = \frac{\partial u}{\partial x}&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;u_x = \frac{\partial u}{\partial x}&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
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: &amp;lt;math&amp;gt;u_{xx} = \frac{\partial^2 u}{\partial x^2} &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;u_{xx} = \frac{\partial^2 u}{\partial x^2} &amp;lt;/math&amp;gt;&lt;br /&gt;
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: &amp;lt;math&amp;gt;u_{xy} = \frac{\partial^2 u}{\partial y\, \partial x} = \frac{\partial}{\partial y } \left(\frac{\partial u}{\partial x}\right). &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;u_{xy} = \frac{\partial^2 u}{\partial y\, \partial x} = \frac{\partial}{\partial y } \left(\frac{\partial u}{\partial x}\right). &amp;lt;/math&amp;gt;&lt;br /&gt;
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Especially in physics, [[del]] or nabla ({{math|∇}}) is often used to denote spatial derivatives, and {{math|''&amp;amp;#x307;u'', ''ü''}} for time derivatives. For example, the [[wave equation]] (mentioned below) can be written as&lt;br /&gt;
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Especially in physics, del or nabla () is often used to denote spatial derivatives, and  for time derivatives. For example, the wave equation (mentioned below) can be written as&lt;br /&gt;
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特别是在物理学中，[[del]]或nabla ({{math|∇}})经常用来表示空间导数和时间导数。例如，波动方程(在下文中提到)可以写成&lt;br /&gt;
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:&amp;lt;math&amp;gt;\ddot u=c^2\nabla^2u&amp;lt;/math&amp;gt;&lt;br /&gt;
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&amp;lt;math&amp;gt;\ddot u=c^2\nabla^2u&amp;lt;/math&amp;gt;&lt;br /&gt;
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or&lt;br /&gt;
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or&lt;br /&gt;
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或&lt;br /&gt;
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:&amp;lt;math&amp;gt;\ddot u=c^2\Delta u&amp;lt;/math&amp;gt;&lt;br /&gt;
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&amp;lt;math&amp;gt;\ddot u=c^2\Delta u&amp;lt;/math&amp;gt;&lt;br /&gt;
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where {{math|Δ}} is the [[Laplace operator]].&lt;br /&gt;
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where  is the Laplace operator.&lt;br /&gt;
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其中{{math|Δ}}代表拉普拉斯算子&lt;br /&gt;
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== Classification ==&lt;br /&gt;
分类&lt;br /&gt;
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Some linear, second-order partial differential equations can be classified as [[parabolic partial differential equation|parabolic]], [[hyperbolic partial differential equation|hyperbolic]] and [[elliptic partial differential equation|elliptic]]. Others, such as the [[Euler–Tricomi equation]], have different types in different regions. The classification provides a guide to appropriate initial and boundary conditions and to the smoothness of the solutions.&lt;br /&gt;
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Some linear, second-order partial differential equations can be classified as parabolic, hyperbolic and elliptic. Others, such as the Euler–Tricomi equation, have different types in different regions. The classification provides a guide to appropriate initial and boundary conditions and to the smoothness of the solutions.&lt;br /&gt;
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一些线性二阶偏微分方程可分为抛物型方程、双曲型方程和椭圆型方程。其他的方程，如欧拉-特里科米方程，在不同的区域有不同的类型。这种分类有助于选择适当的初始和边界条件以及提高解的平滑性。&lt;br /&gt;
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=== Equations of first order ===&lt;br /&gt;
一阶方程&lt;br /&gt;
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{{main|First-order partial differential equation}}&lt;br /&gt;
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=== Linear equations of second order ===&lt;br /&gt;
二阶线性方程&lt;br /&gt;
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Assuming {{math|''u&amp;lt;sub&amp;gt;xy&amp;lt;/sub&amp;gt;'' {{=}} ''u&amp;lt;sub&amp;gt;yx&amp;lt;/sub&amp;gt;''}}, the general linear second-order PDE in two independent variables has the form&lt;br /&gt;
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Assuming  u&amp;lt;sub&amp;gt;yx&amp;lt;/sub&amp;gt;}}, the general linear second-order PDE in two independent variables has the form&lt;br /&gt;
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假设 {{math|''u&amp;lt;sub&amp;gt;xy&amp;lt;/sub&amp;gt;'' {{=}} ''u&amp;lt;sub&amp;gt;yx&amp;lt;/sub&amp;gt;''}}，含有两个独立变量的一般的线性二阶偏微分方程具有如下这样的形式&lt;br /&gt;
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: &amp;lt;math&amp;gt;Au_{xx} + 2Bu_{xy} + Cu_{yy} + \cdots \mbox{(lower order terms)} = 0,&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;Au_{xx} + 2Bu_{xy} + Cu_{yy} + \cdots \mbox{(lower order terms)} = 0,&amp;lt;/math&amp;gt;&lt;br /&gt;
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where the coefficients {{mvar|A}}, {{mvar|B}}, {{mvar|C}}... may depend upon {{mvar|x}} and {{mvar|y}}. If {{math|''A''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; + ''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; + ''C''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; &amp;gt; 0}} over a region of the {{mvar|xy}}-plane, the PDE is second-order in that region. This form is analogous to the equation for a conic section:&lt;br /&gt;
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where the coefficients , , ... may depend upon  and . If  over a region of the -plane, the PDE is second-order in that region. This form is analogous to the equation for a conic section:&lt;br /&gt;
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其中的系数 {{mvar|A}}, {{mvar|B}}, {{mvar|C}}... 一般取决于{{mvar|x}}和{{mvar|y}}。如果在{{mvar|xy}}-平面的一个区域上 {{math|''A''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; + ''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; + ''C''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; &amp;gt; 0}}，偏微分方程在该区域是二阶的。这种形式类似于圆锥曲线的方程:&lt;br /&gt;
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: &amp;lt;math&amp;gt;Ax^2 + 2Bxy + Cy^2 + \cdots = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;Ax^2 + 2Bxy + Cy^2 + \cdots = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
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More precisely, replacing {{math|∂&amp;lt;sub&amp;gt;''x''&amp;lt;/sub&amp;gt;}} by {{mvar|X}}, and likewise for other variables (formally this is done by a [[Fourier transform]]), converts a constant-coefficient PDE into a polynomial of the same degree, with the terms of the highest degree (a [[homogeneous polynomial]], here a [[quadratic form]]) being most significant for the classification.&lt;br /&gt;
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More precisely, replacing  by , and likewise for other variables (formally this is done by a Fourier transform), converts a constant-coefficient PDE into a polynomial of the same degree, with the terms of the highest degree (a homogeneous polynomial, here a quadratic form) being most significant for the classification.&lt;br /&gt;
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更准确地说，用 {{mvar|X}} 替换 {{math|∂&amp;lt;sub&amp;gt;''x''&amp;lt;/sub&amp;gt;}}，对于其他变量做同样的操作(从形式上来说，这是由傅里叶变换来完成的)，将一个常系数偏微分方程转换成一个相同次数的多项式，最高次数的项(齐次多项式，这里是一个二次形式)一般会用于偏微分方程的分类。&lt;br /&gt;
===~~ most significant for the classification 意译为用于偏微分方程的分类。       significiant直译过来感觉不太合适&lt;br /&gt;
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Just as one classifies [[conic section]]s and quadratic forms into parabolic, hyperbolic, and elliptic based on the [[discriminant]] {{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − 4''AC''}}, the same can be done for a second-order PDE at a given point.  However, the [[discriminant]] in a PDE is given by {{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC''}} due to the convention of the {{mvar|xy}} term being {{math|2''B''}} rather than {{mvar|B}}; formally, the discriminant (of the associated quadratic form) is {{math|(2''B'')&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − 4''AC'' {{=}} 4(''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC'')}}, with the factor of 4 dropped for simplicity.&lt;br /&gt;
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Just as one classifies conic sections and quadratic forms into parabolic, hyperbolic, and elliptic based on the discriminant , the same can be done for a second-order PDE at a given point.  However, the discriminant in a PDE is given by  due to the convention of the  term being  rather than ; formally, the discriminant (of the associated quadratic form) is  4(B&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − AC)}}, with the factor of 4 dropped for simplicity.&lt;br /&gt;
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正如人们可以根据判别式 {{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − 4''AC''}} 将圆锥曲线和二次型分为抛物型、双曲型和椭圆型一样，对于给定点的二阶偏微分方程也可以这样做。然而，偏微分方程中的判别式 {{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − 4''AC''}} 是根据交叉项的系数{{math|2''B''}} 而不是 {{mvar|B}} 给出的，形式上，判别式(关联二次型)是 {{math|(2''B'')&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − 4''AC'' {{=}} 4(''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC'')}}，为简单起见，去掉了因子4。&lt;br /&gt;
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# {{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC'' &amp;lt; 0}} (''[[elliptic partial differential equation]]''): Solutions of [[elliptic partial differential equation|elliptic PDEs]] are as smooth as the coefficients allow, within the interior of the region where the equation and solutions are defined. For example, solutions of [[Laplace's equation]] are analytic within the domain where they are defined, but solutions may assume boundary values that are not smooth. The motion of a fluid at subsonic speeds can be approximated with elliptic PDEs, and the Euler–Tricomi equation is elliptic where {{math|''x'' &amp;lt; 0}}.&lt;br /&gt;
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  (elliptic partial differential equation): Solutions of elliptic PDEs are as smooth as the coefficients allow, within the interior of the region where the equation and solutions are defined. For example, solutions of Laplace's equation are analytic within the domain where they are defined, but solutions may assume boundary values that are not smooth. The motion of a fluid at subsonic speeds can be approximated with elliptic PDEs, and the Euler–Tricomi equation is elliptic where .&lt;br /&gt;
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{{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC'' &amp;lt; 0}} (椭圆形微分方程)：在定义方程和解的区域内部，椭圆型偏微分方程的解光滑到系数允许的程度。例如，拉普拉斯方程的解在它们被定义的区域内是解析的，但是解可能假设边界值是不光滑的。亚音速流体的运动可以用椭圆偏微分方程近似，其中欧拉-特里科米方程在 {{math|''x'' &amp;lt; 0}} 时是椭圆型偏微分方程。&lt;br /&gt;
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# {{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC'' {{=}} 0}} (''[[parabolic partial differential equation]]''): Equations that are [[parabolic partial differential equation|parabolic]] at every point can be transformed into a form analogous to the [[heat equation]] by a change of independent variables. Solutions smooth out as the transformed time variable increases. The Euler–Tricomi equation has parabolic type on the line where {{math|''x'' {{=}} 0}}.&lt;br /&gt;
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  0}} (parabolic partial differential equation): Equations that are parabolic at every point can be transformed into a form analogous to the heat equation by a change of independent variables. Solutions smooth out as the transformed time variable increases. The Euler–Tricomi equation has parabolic type on the line where  0}}.&lt;br /&gt;
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{{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC'' {{=}} 0}}（抛物线形偏微分方程）：在每一点上都是抛物线型的方程可以通过改变自变量从而转化成类似于热方程的形式。随着转换后的时间变量的增加，方程的解变得平滑。欧拉-特里科米方程在 {{math|''x'' {{=}} 0}} 这条特征线上是抛物线形的。&lt;br /&gt;
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# {{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC'' &amp;gt; 0}} (''[[hyperbolic partial differential equation]]''): [[hyperbolic partial differential equation|hyperbolic]] equations retain any discontinuities of functions or derivatives in the initial data. An example is the [[wave equation]]. The motion of a fluid at supersonic speeds can be approximated with hyperbolic PDEs, and the Euler–Tricomi equation is hyperbolic where {{math|''x'' &amp;gt; 0}}.&lt;br /&gt;
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  (hyperbolic partial differential equation): hyperbolic equations retain any discontinuities of functions or derivatives in the initial data. An example is the wave equation. The motion of a fluid at supersonic speeds can be approximated with hyperbolic PDEs, and the Euler–Tricomi equation is hyperbolic where .&lt;br /&gt;
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{{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC'' &amp;gt; 0}} (双曲形偏微分方程)：双曲形方程在初始数据中保留了函数或导数的任何不连续性，波动方程就是其中的一个例子。超音速流体的运动可以用双曲形偏微分方程近似，其中欧拉-特里科米方程在 {{math|''x'' &amp;gt; 0}} 时是双曲型的。&lt;br /&gt;
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If there are {{mvar|n}} independent variables {{math|''x''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;, ''x''&amp;lt;sub&amp;gt;2 &amp;lt;/sub&amp;gt;,… ''x''&amp;lt;sub&amp;gt;''n''&amp;lt;/sub&amp;gt;}}, a general linear partial differential equation of second order has the form&lt;br /&gt;
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If there are  independent variables , a general linear partial differential equation of second order has the form&lt;br /&gt;
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如果存在 {{mvar|n}} 个自变量 {{math|''x''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;, ''x''&amp;lt;sub&amp;gt;2 &amp;lt;/sub&amp;gt;,… ''x''&amp;lt;sub&amp;gt;''n''&amp;lt;/sub&amp;gt;}}，一般二阶线性偏微分方程的形式是&lt;br /&gt;
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: &amp;lt;math&amp;gt;L u =\sum_{i=1}^n\sum_{j=1}^n a_{i,j} \frac{\partial^2 u}{\partial x_i \partial x_j} \quad \text{ plus lower-order terms} =0.&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;L u =\sum_{i=1}^n\sum_{j=1}^n a_{i,j} \frac{\partial^2 u}{\partial x_i \partial x_j} \quad \text{ plus lower-order terms} =0.&amp;lt;/math&amp;gt;&lt;br /&gt;
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The classification depends upon the signature of the eigenvalues of the coefficient matrix {{math|''a''&amp;lt;sub&amp;gt;''i'',''j''&amp;lt;/sub&amp;gt;}}.&lt;br /&gt;
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The classification depends upon the signature of the eigenvalues of the coefficient matrix .&lt;br /&gt;
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这种分类取决于系数矩阵本征值的符号（正负性）。&lt;br /&gt;
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# Elliptic: the eigenvalues are all positive or all negative.&lt;br /&gt;
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 Elliptic: the eigenvalues are all positive or all negative.&lt;br /&gt;
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椭圆形方程: 本征值全部为正或全部为负。&lt;br /&gt;
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# Parabolic: the eigenvalues are all positive or all negative, save one that is zero.&lt;br /&gt;
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 Parabolic: the eigenvalues are all positive or all negative, save one that is zero.&lt;br /&gt;
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抛物线形方程: 本征值全部为正或全部为负，除了一个为零。&lt;br /&gt;
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# Hyperbolic: there is only one negative eigenvalue and all the rest are positive, or there is only one positive eigenvalue and all the rest are negative.&lt;br /&gt;
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 Hyperbolic: there is only one negative eigenvalue and all the rest are positive, or there is only one positive eigenvalue and all the rest are negative.&lt;br /&gt;
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双曲形方程: 只有一个负特征值，其余的都是正特征值，或者只有一个正特征值，其余的都是负特征值。&lt;br /&gt;
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# Ultrahyperbolic: there is more than one positive eigenvalue and more than one negative eigenvalue, and there are no zero eigenvalues. There is only a limited theory for ultrahyperbolic equations (Courant and Hilbert, 1962).&lt;br /&gt;
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 Ultrahyperbolic: there is more than one positive eigenvalue and more than one negative eigenvalue, and there are no zero eigenvalues. There is only a limited theory for ultrahyperbolic equations (Courant and Hilbert, 1962).&lt;br /&gt;
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超双形方程: 存在多于一个正本征值和多于一个的负本征值，且不存在零本征值。对于超双曲方程，只存在一个有限理论(Courant 和 Hilbert，1962)。&lt;br /&gt;
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==[[用户:Yuling|Yuling]]（[[用户讨论:Yuling|讨论]]） 我对于limited theory这个单词对应的相关理论不太了解。&lt;br /&gt;
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=== Systems of first-order equations and characteristic surfaces ===&lt;br /&gt;
一阶方程组和特征曲面&lt;br /&gt;
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The classification of partial differential equations can be extended to systems of first-order equations, where the unknown {{mvar|u}} is now a [[Euclidean vector|vector]] with {{mvar|m}} components, and the coefficient matrices {{mvar|A&amp;lt;sub&amp;gt;ν&amp;lt;/sub&amp;gt;}} are {{mvar|m}} by {{mvar|m}} matrices for {{math|''ν'' {{=}} 1, 2,… ''n''}}. The partial differential equation takes the form&lt;br /&gt;
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The classification of partial differential equations can be extended to systems of first-order equations, where the unknown  is now a vector with  components, and the coefficient matrices  are  by  matrices for  1, 2,… n}}. The partial differential equation takes the form&lt;br /&gt;
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偏微分方程组的分类可以推广到一阶方程组，其中未知量 {{mvar|u}} 是有 {{mvar|m}} 个分量的向量。对于 {{math|''ν'' {{=}} 1, 2,… ''n''}}，系数矩阵 {{mvar|A&amp;lt;sub&amp;gt;ν&amp;lt;/sub&amp;gt;}} 是 {{mvar|m}} × {{mvar|m}} 的矩阵。偏微分方程形式如下：&lt;br /&gt;
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: &amp;lt;math&amp;gt;Lu = \sum_{\nu=1}^{n} A_\nu \frac{\partial u}{\partial x_\nu} + B=0,&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;Lu = \sum_{\nu=1}^{n} A_\nu \frac{\partial u}{\partial x_\nu} + B=0,&amp;lt;/math&amp;gt;&lt;br /&gt;
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where the coefficient matrices {{mvar|A&amp;lt;sub&amp;gt;ν&amp;lt;/sub&amp;gt;}} and the vector {{mvar|B}} may depend upon {{mvar|x}} and {{mvar|u}}. If a [[hypersurface]] {{mvar|S}} is given in the implicit form&lt;br /&gt;
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where the coefficient matrices  and the vector  may depend upon  and . If a hypersurface  is given in the implicit form&lt;br /&gt;
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其中系数矩阵 {{mvar|A&amp;lt;sub&amp;gt;ν&amp;lt;/sub&amp;gt;}} 和向量 {{mvar|B}} 可能依赖于 {{mvar|x}} 和 {{mvar|u}}。如果超曲面是以隐式形式给出的&lt;br /&gt;
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: &amp;lt;math&amp;gt;\varphi(x_1, x_2, \ldots x_n)=0,&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;\varphi(x_1, x_2, \ldots x_n)=0,&amp;lt;/math&amp;gt;&lt;br /&gt;
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where {{mvar|φ}} has a non-zero gradient, then {{mvar|S}} is a '''characteristic surface''' for the operator {{mvar|L}} at a given point if the characteristic form vanishes:&lt;br /&gt;
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where  has a non-zero gradient, then  is a characteristic surface for the operator  at a given point if the characteristic form vanishes:&lt;br /&gt;
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其中存在一个非零的梯度，那么如果特征形式消失，则在给定点上算子的特征曲面形式如下:&lt;br /&gt;
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: &amp;lt;math&amp;gt;Q\left(\frac{\partial\varphi}{\partial x_1}, \ldots\frac{\partial\varphi}{\partial x_n}\right) =\det\left[\sum_{\nu=1}^nA_\nu \frac{\partial \varphi}{\partial x_\nu}\right]=0.\,&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;Q\left(\frac{\partial\varphi}{\partial x_1}, \ldots\frac{\partial\varphi}{\partial x_n}\right) =\det\left[\sum_{\nu=1}^nA_\nu \frac{\partial \varphi}{\partial x_\nu}\right]=0.\,&amp;lt;/math&amp;gt;&lt;br /&gt;
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The geometric interpretation of this condition is as follows: if data for {{mvar|u}} are prescribed on the surface {{mvar|S}}, then it may be possible to determine the normal derivative of {{mvar|u}} on {{mvar|S}} from the differential equation. If the data on {{mvar|S}} and the differential equation determine the normal derivative of {{mvar|u}} on {{mvar|S}}, then {{mvar|S}} is non-characteristic. If the data on {{mvar|S}} and the differential equation ''do not'' determine the normal derivative of {{mvar|u}} on {{mvar|S}}, then the surface is '''characteristic''', and the differential equation restricts the data on {{mvar|S}}: the differential equation is ''internal'' to {{mvar|S}}.&lt;br /&gt;
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The geometric interpretation of this condition is as follows: if data for  are prescribed on the surface , then it may be possible to determine the normal derivative of  on  from the differential equation. If the data on  and the differential equation determine the normal derivative of  on , then  is non-characteristic. If the data on  and the differential equation do not determine the normal derivative of  on , then the surface is characteristic, and the differential equation restricts the data on : the differential equation is internal to .&lt;br /&gt;
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这个条件的几何解释如下: 如果关于 {{mvar|u}} 的数据是在曲面 {{mvar|S}} 上规定的，那么就有可能依据微分方程确定曲面 {{mvar|S}} 上 {{mvar|u}} 的法向导数。如果曲面 {{mvar|S}} 上的数据和上面的微分方程能确定曲面 {{mvar|S}} 上 {{mvar|u}} 的法向导数，那么它就是非特征的。如果曲面 {{mvar|S}} 上的数据和上面的微分方程不能确定曲面 {{mvar|S}} 上 {{mvar|u}} 的法向导数，那么曲面是特征的，并且微分方程将数据限制在曲面 {{mvar|S}} 上：微分方程是在曲面 {{mvar|S}} 内部。&lt;br /&gt;
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# A first-order system {{math|''Lu'' {{=}} 0}} is ''elliptic'' if no surface is characteristic for {{mvar|L}}: the values of {{mvar|u}} on {{mvar|S}} and the differential equation always determine the normal derivative of {{mvar|u}} on {{mvar|S}}.&lt;br /&gt;
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 A first-order system  0}} is elliptic if no surface is characteristic for : the values of  on  and the differential equation always determine the normal derivative of  on .&lt;br /&gt;
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如果对于 {{mvar|L}} 没有曲面是特征的，则一阶系统 {{math|''Lu'' {{=}} 0}} 是椭圆形的：{{mvar|u}}在 {{mvar|S}} 的值和微分方程总能够决定 {{mvar|S}} 上 {{mvar|u}} 的法向导数。&lt;br /&gt;
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# A first-order system is ''hyperbolic'' at a point if there is a '''spacelike''' surface {{mvar|S}} with normal {{mvar|ξ}} at that point. This means that, given any non-trivial vector {{mvar|η}} orthogonal to {{mvar|ξ}}, and a scalar multiplier {{mvar|λ}}, the equation {{math|''Q''(''λξ'' + ''η'') {{=}} 0}} has {{mvar|m}} real roots {{math|''λ''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;, ''λ''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;,… ''λ''&amp;lt;sub&amp;gt;''m''&amp;lt;/sub&amp;gt;}}. The system is '''strictly hyperbolic''' if these roots are always distinct. The geometrical interpretation of this condition is as follows: the characteristic form {{math|''Q''(''ζ'') {{=}} 0}} defines a cone (the normal cone) with homogeneous coordinates ζ. In the hyperbolic case, this cone has {{mvar|m}} sheets, and the axis {{math|''ζ'' {{=}} ''λξ''}} runs inside these sheets: it does not intersect any of them. But when displaced from the origin by η, this axis intersects every sheet. In the elliptic case, the normal cone has no real sheets.&lt;br /&gt;
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 A first-order system is hyperbolic at a point if there is a spacelike surface  with normal  at that point. This means that, given any non-trivial vector  orthogonal to , and a scalar multiplier , the equation  0}} has  real roots . The system is strictly hyperbolic if these roots are always distinct. The geometrical interpretation of this condition is as follows: the characteristic form  0}} defines a cone (the normal cone) with homogeneous coordinates ζ. In the hyperbolic case, this cone has  sheets, and the axis  λξ}} runs inside these sheets: it does not intersect any of them. But when displaced from the origin by η, this axis intersects every sheet. In the elliptic case, the normal cone has no real sheets.&lt;br /&gt;
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如果在该点存在一个法向量为 {{mvar|ξ}}的 '''&amp;lt;font color=&amp;quot;#ff8000&amp;quot;&amp;gt;类空曲面 Spacclike Surface&amp;lt;/font&amp;gt; {{mvar|S}} ，则一阶系统在那一点是双曲的。这意味着，给定任意正交于 {{mvar|ξ}} 的非平凡向量 {{mvar|η}} 和一个标量乘子 {{mvar|λ}}，方程 {{math|''Q''(''λξ'' + ''η'') {{=}} 0}} 有 {{mvar|m}} 个实根 {{math|''λ''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;, ''λ''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;,… ''λ''&amp;lt;sub&amp;gt;''m''&amp;lt;/sub&amp;gt;}}。如果这些根始终不同，则该系统是严格双曲形的。这个条件的几何解释如下: 特征形式 {{math|''Q''(''ζ'') {{=}} 0}} 定义了一个具有齐次坐标 ζ的圆锥(法线圆锥)。在双曲形的情况下，这个圆锥体有 {{mvar|m}} 层，并且轴 {{math|''ζ'' {{=}} ''λξ''}} 在这些层中运动: 它不与任何一层相交。但是当从原点偏离η时，这条轴线与每一层都相交。在椭圆形的情况下，法向圆锥没有实层。&lt;br /&gt;
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==[[用户:Yuling|Yuling]]（[[用户讨论:Yuling|讨论]]） sheet 这个单词也不很理解，我直译为了“层”&lt;br /&gt;
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=== Equations of mixed type ===&lt;br /&gt;
混合型方程&lt;br /&gt;
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If a PDE has coefficients that are not constant, it is possible that it will not belong to any of these categories but rather be of '''mixed type'''. A simple but important example is the [[Euler–Tricomi equation]]&lt;br /&gt;
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If a PDE has coefficients that are not constant, it is possible that it will not belong to any of these categories but rather be of mixed type. A simple but important example is the Euler–Tricomi equation&lt;br /&gt;
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如果偏微分方程的系数不是常数，那么它可能不属于这些类别中的任何一个，而是属于混合类型。一个简单但重要的例子是欧拉-特里科米方程&lt;br /&gt;
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: &amp;lt;math&amp;gt;u_{xx} = xu_{yy},&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;u_{xx} = xu_{yy},&amp;lt;/math&amp;gt;&lt;br /&gt;
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which is called '''elliptic-hyperbolic''' because it is elliptic in the region {{math|''x'' &amp;lt; 0}}, hyperbolic in the region {{math|''x'' &amp;gt; 0}}, and degenerate parabolic on the line {{math|''x'' {{=}} 0}}.&lt;br /&gt;
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which is called elliptic-hyperbolic because it is elliptic in the region , hyperbolic in the region , and degenerate parabolic on the line  0}}.&lt;br /&gt;
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它在 {{math|''x'' &amp;lt; 0}} 的区域上是椭圆形，在 {{math|''x'' &amp;gt; 0}} 区域上是双曲形，在 {{math|''x'' {{=}} 0}}这条线上是退化为抛物线形，因此称之为椭圆-双曲型。&lt;br /&gt;
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''fill in: Dirichlet and Neumann boundaries, hyperbolic/parabolic/elliptic separation of variables, [[Fourier analysis]], [[Green's function]]s ...--&amp;gt;&lt;br /&gt;
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fill in: Dirichlet and Neumann boundaries, hyperbolic/parabolic/elliptic separation of variables, Fourier analysis, Green's functions ...--&amp;gt;&lt;br /&gt;
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填写: Dirichlet 和 Neumann 边界，双曲 / 抛物线 / 椭圆分离变量法，傅立叶分析，Green 函数... --&lt;br /&gt;
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=== Infinite-order PDEs in quantum mechanics ===&lt;br /&gt;
量子力学中的无限阶偏微分方程&lt;br /&gt;
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In the [[phase space formulation]] of quantum mechanics,  one may consider the [[Method of quantum characteristics|quantum Hamilton's equations]] for trajectories of quantum particles. These equations are infinite-order PDEs. However, in the semiclassical expansion, one has a finite system of ODEs at any fixed order of [[Dirac constant|{{mvar|ħ}}]].  The evolution equation of the [[Wigner quasi-probability distribution|c]] is also an infinite-order PDE. The quantum trajectories are [[Method of quantum characteristics|quantum characteristics]], with the use of which one could calculate the evolution of the Wigner function.&lt;br /&gt;
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In the phase space formulation of quantum mechanics,  one may consider the quantum Hamilton's equations for trajectories of quantum particles. These equations are infinite-order PDEs. However, in the semiclassical expansion, one has a finite system of ODEs at any fixed order of Dirac constant|.  The evolution equation of the Wigner function is also an infinite-order PDE. The quantum trajectories are quantum characteristics, with the use of which one could calculate the evolution of the Wigner function.&lt;br /&gt;
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在量子力学中的相空间表述中，我们可以考虑用于求解量子粒子的轨迹的量子哈密顿的方程。这些方程是无限阶偏微分方程。然而，在半经典展开中，我们在给定[[Dirac constant|{{mvar|ħ}}]]阶数下有一个有限的的常微分方程组。'''&amp;lt;font color=&amp;quot;#ff8000&amp;quot;&amp;gt;维格纳函数  Wigner Function&amp;lt;/font&amp;gt;的演化方程也是一个无限阶偏微分方程。由于量子轨道的量子特性，所以它通常可以用来计算维格纳函数的演化。&lt;br /&gt;
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== Analytical solutions ==&lt;br /&gt;
解析解&lt;br /&gt;
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===Separation of variables===&lt;br /&gt;
分离变量法&lt;br /&gt;
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{{main|Separable partial differential equation}}&lt;br /&gt;
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Linear PDEs can be reduced to systems of ordinary differential equations by the important technique of separation of variables. This technique rests on a characteristic of solutions to differential equations: if one can find any solution that solves the equation and satisfies the boundary conditions, then it is ''the'' solution (this also applies to ODEs). We assume as an [[ansatz]] that the dependence of a solution on the parameters space and time can be written as a product of terms that each depend on a single parameter, and then see if this can be made to solve the problem.&amp;lt;ref&amp;gt;{{cite book|last1=Gershenfeld|first1=Neil|title=The nature of mathematical modeling|date=2000|publisher=Cambridge Univ. Press|location=Cambridge|isbn=0521570956|page=27|edition=Reprinted (with corr.)}}&amp;lt;/ref&amp;gt;&lt;br /&gt;
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Linear PDEs can be reduced to systems of ordinary differential equations by the important technique of separation of variables. This technique rests on a characteristic of solutions to differential equations: if one can find any solution that solves the equation and satisfies the boundary conditions, then it is the solution (this also applies to ODEs). We assume as an ansatz that the dependence of a solution on the parameters space and time can be written as a product of terms that each depend on a single parameter, and then see if this can be made to solve the problem.&lt;br /&gt;
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线性偏微分方程组可以通过分离变量法这一重要方法来简化为常微分方程组。这种方法依赖于微分方程解的一个特征: 如果能找到任何一个满足方程和边界条件的解，那么这个解就是方程的解(这也适用于常微分方程)。我们假设解对参数空间和时间的依赖可以写成对它们每一项的依赖以及一个参数的乘积，然后再看看这是否可以用来解决这个问题。&lt;br /&gt;
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In the method of separation of variables, one reduces a PDE to a PDE in fewer variables, which is an ordinary differential equation if in one variable – these are in turn easier to solve.&lt;br /&gt;
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In the method of separation of variables, one reduces a PDE to a PDE in fewer variables, which is an ordinary differential equation if in one variable – these are in turn easier to solve.&lt;br /&gt;
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在分离变量法方法中，可以将偏微分方程简化为含有更少变量的偏微分方程，如果只有一个变量，那么就变成了一个'''&amp;lt;font color = &amp;quot;#ff8000&amp;quot;&amp;gt;常微分方程 Ordinary Differential Equation&amp;lt;/font&amp;gt;'''-- 反过来，这些方程也更容易求解。&lt;br /&gt;
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This is possible for simple PDEs, which are called [[separable partial differential equation]]s, and the domain is generally a rectangle (a product of intervals). Separable PDEs correspond to [[diagonal matrices]] – thinking of &amp;quot;the value for fixed {{mvar|x}}&amp;quot; as a coordinate, each coordinate can be understood separately.&lt;br /&gt;
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This is possible for simple PDEs, which are called separable partial differential equations, and the domain is generally a rectangle (a product of intervals). Separable PDEs correspond to diagonal matrices – thinking of &amp;quot;the value for fixed &amp;quot; as a coordinate, each coordinate can be understood separately.&lt;br /&gt;
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对于简单的偏微分方程(称为可分离偏微分方程)来说，这是可能的，而且方程通常定义在一个矩形区域(区间的乘积)上。可分离偏微分方程对应于对角线矩阵——以“固定值”为坐标，每个坐标可分开理解。&lt;br /&gt;
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This generalizes to the [[method of characteristics]], and is also used in [[integral transform]]s.&lt;br /&gt;
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This generalizes to the method of characteristics, and is also used in integral transforms.&lt;br /&gt;
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这种方法可以推广到特征曲线法，也可以用于积分变换。&lt;br /&gt;
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===Method of characteristics===&lt;br /&gt;
特征曲线法&lt;br /&gt;
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{{main|Method of characteristics}}&lt;br /&gt;
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In special cases, one can find characteristic curves on which the equation reduces to an ODE – changing coordinates in the domain to straighten these curves allows separation of variables, and is called the [[method of characteristics]].&lt;br /&gt;
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In special cases, one can find characteristic curves on which the equation reduces to an ODE – changing coordinates in the domain to straighten these curves allows separation of variables, and is called the method of characteristics.&lt;br /&gt;
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在特殊情况下，可以找到一些特征曲线，在这些曲线上方程可以变成一个常微分方程——意味着改变坐标从而使这些曲线变直从而达到分离变量的目的，这就是所谓的特征曲线法。&lt;br /&gt;
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More generally, one may find characteristic surfaces.&lt;br /&gt;
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More generally, one may find characteristic surfaces.&lt;br /&gt;
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更一般地说，人们可能会找到特征表面。&lt;br /&gt;
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===Integral transform===&lt;br /&gt;
积分变换&lt;br /&gt;
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An [[integral transform]] may transform the PDE to a simpler one, in particular, a separable PDE. This corresponds to diagonalizing an operator.&lt;br /&gt;
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An integral transform may transform the PDE to a simpler one, in particular, a separable PDE. This corresponds to diagonalizing an operator.&lt;br /&gt;
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积分变换可以将偏微分方程转换为更简单的偏微分方程，特别是可分离的偏微分方程。这对应于对角化算符。&lt;br /&gt;
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An important example of this is [[Fourier analysis]], which diagonalizes the heat equation using the [[eigenbasis]] of sinusoidal waves.&lt;br /&gt;
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An important example of this is Fourier analysis, which diagonalizes the heat equation using the eigenbasis of sinusoidal waves.&lt;br /&gt;
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这方面的一个重要例子是'''&amp;lt;font color = &amp;quot;#ff8000&amp;quot;&amp;gt;傅里叶分析  Fourier Analysis&amp;lt;/font&amp;gt;'''，它使用正弦波的特征基来对角化热方程。&lt;br /&gt;
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If the domain is finite or periodic, an infinite sum of solutions such as a [[Fourier series]] is appropriate, but an integral of solutions such as a [[Fourier integral]] is generally required for infinite domains. The solution for a point source for the heat equation given above is an example of the use of a Fourier integral.&lt;br /&gt;
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If the domain is finite or periodic, an infinite sum of solutions such as a Fourier series is appropriate, but an integral of solutions such as a Fourier integral is generally required for infinite domains. The solution for a point source for the heat equation given above is an example of the use of a Fourier integral.&lt;br /&gt;
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如果区域是有限的或周期性的，那么解为无限和的形式是恰当的，例如傅里叶级数，但是一个解的积分，例如傅立叶积分，一般是在无限区域上的。上面给出的热传导方程的点源解法就是使用傅里叶积分的一个例子。&lt;br /&gt;
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===Change of variables===&lt;br /&gt;
变量代换&lt;br /&gt;
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Often a PDE can be reduced to a simpler form with a known solution by a suitable [[Change of variables (PDE)|change of variables]].  For example, the [[Black–Scholes equation#Derivation|Black–Scholes]] PDE&lt;br /&gt;
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Often a PDE can be reduced to a simpler form with a known solution by a suitable change of variables.  For example, the Black–Scholes PDE&lt;br /&gt;
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偏微分方程通常可以通过变量的适当变化，用已知的解简化为更简单的形式。例如，布莱克-舒尔斯偏微分方程&lt;br /&gt;
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:&amp;lt;math&amp;gt; \frac{\partial V}{\partial t} + \tfrac{1}{2}\sigma^2 S^2\frac{\partial^2 V}{\partial S^2} + rS\frac{\partial V}{\partial S} - rV = 0 &amp;lt;/math&amp;gt;&lt;br /&gt;
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&amp;lt;math&amp;gt; \frac{\partial V}{\partial t} + \tfrac{1}{2}\sigma^2 S^2\frac{\partial^2 V}{\partial S^2} + rS\frac{\partial V}{\partial S} - rV = 0 &amp;lt;/math&amp;gt;&lt;br /&gt;
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is reducible to the [[heat equation]]&lt;br /&gt;
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is reducible to the heat equation&lt;br /&gt;
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可以简化为热传导方程&lt;br /&gt;
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:&amp;lt;math&amp;gt; \frac{\partial u}{\partial \tau} = \frac{\partial^2 u}{\partial x^2}&amp;lt;/math&amp;gt;&lt;br /&gt;
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&amp;lt;math&amp;gt; \frac{\partial u}{\partial \tau} = \frac{\partial^2 u}{\partial x^2}&amp;lt;/math&amp;gt;&lt;br /&gt;
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by the change of variables (for complete details see {{webarchive |url=https://web.archive.org/web/20080411030405/http://www.math.unl.edu/~sdunbar1/Teaching/MathematicalFinance/Lessons/BlackScholes/Solution/solution.shtml |date=April 11, 2008 |title=Solution of the Black Scholes Equation }})&lt;br /&gt;
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by the change of variables (for complete details see )&lt;br /&gt;
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通过变量替换(完整的细节见)&lt;br /&gt;
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:&amp;lt;math&amp;gt;\begin{align}&lt;br /&gt;
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V(S,t) &amp;amp;= K v(x,\tau),\\[5px]&lt;br /&gt;
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x &amp;amp;= \ln\left(\tfrac{S}{K} \right),\\[5px]&lt;br /&gt;
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\tau &amp;amp;= \tfrac{1}{2} \sigma^2 (T - t),\\[5px]&lt;br /&gt;
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v(x,\tau)&amp;amp;=e^{-\alpha x-\beta\tau} u(x,\tau).&lt;br /&gt;
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\end{align}&amp;lt;/math&amp;gt;&lt;br /&gt;
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===Fundamental solution===&lt;br /&gt;
基本解&lt;br /&gt;
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{{main|Fundamental solution}}&lt;br /&gt;
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Inhomogeneous equations can often be solved (for constant coefficient PDEs, always be solved) by finding the [[fundamental solution]] (the solution for a point source), then taking the [[convolution]] with the boundary conditions to get the solution.&lt;br /&gt;
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Inhomogeneous equations can often be solved (for constant coefficient PDEs, always be solved) by finding the fundamental solution (the solution for a point source), then taking the convolution with the boundary conditions to get the solution.&lt;br /&gt;
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非齐次方程(常系数偏微分方程)一般是通过先求出基本解(点源的解) ，然后利用带边界条件的卷积来求解。&lt;br /&gt;
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This is analogous in [[signal processing]] to understanding a filter by its [[impulse response]].&lt;br /&gt;
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This is analogous in signal processing to understanding a filter by its impulse response.&lt;br /&gt;
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这类似于在信号处理中通过滤波器的脉冲响应来理解滤波器。&lt;br /&gt;
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===Superposition principle===&lt;br /&gt;
叠加原理&lt;br /&gt;
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{{further| Superposition principle }}&lt;br /&gt;
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The superposition principle applies to any linear system, including linear systems of PDEs. A common visualization of this concept is the interaction of two waves in phase being combined to result in a greater amplitude, for example {{math|sin ''x'' + sin ''x'' {{=}} 2 sin ''x''}}. The same principle can be observed in PDEs where the solutions may be real or complex and additive. [[Superposition principle|superposition]]&lt;br /&gt;
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The superposition principle applies to any linear system, including linear systems of PDEs. A common visualization of this concept is the interaction of two waves in phase being combined to result in a greater amplitude, for example  2 sin x}}. The same principle can be observed in PDEs where the solutions may be real or complex and additive. superposition&lt;br /&gt;
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'''&amp;lt;font color = &amp;quot;#ff8000&amp;quot;&amp;gt;叠加原理 Superposition Principle&amp;lt;/font&amp;gt;适用于任何线性系统，包括偏微分方程的线性系统。这个概念的一个常见的可视化是两个同相位的波相互作用结合在一起会产生更大的振幅，例如 {{math|sin ''x'' + sin ''x'' {{=}} 2 sin ''x''}}。在偏微分方程中也可以观察到同样的原理，其中的解可能是真实的或复杂的和可加的。叠加&lt;br /&gt;
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If {{math|''u''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;}} and {{math|''u''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;}} are solutions of linear PDE in some function space {{mvar|R}}, then {{math|''u'' {{=}} ''c''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;''u''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; + ''c''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;''u''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;}} with any constants {{math|''c''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;}} and {{math|''c''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;}} are also a solution of that PDE in the same function space.&lt;br /&gt;
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If  and  are solutions of linear PDE in some function space , then  c&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;u&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; + c&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;u&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;}} with any constants  and  are also a solution of that PDE in the same function space.&lt;br /&gt;
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若线性偏微分方程在某个函数空间{{mvar|R}}中有解{{math|''u''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;}} 和 {{math|''u''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;}}，则{{math|''u'' {{=}} ''c''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;''u''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; + ''c''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;''u''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;}}也是该偏微分方程在同一函数空间中的解，其中{{math|''c''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;}} 和 {{math|''c''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;}} 是任意常数。&lt;br /&gt;
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===Methods for non-linear equations===&lt;br /&gt;
非线性方程的求解方法&lt;br /&gt;
{{see also|nonlinear partial differential equation}}&lt;br /&gt;
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There are no generally applicable methods to solve nonlinear PDEs. Still, existence and uniqueness results (such as the [[Cauchy–Kowalevski theorem]]) are often possible, as are proofs of important qualitative and quantitative properties of solutions (getting these results is a major part of [[mathematical analysis|analysis]]). Computational solution to the nonlinear PDEs, the [[split-step method]], exist for specific equations like [[nonlinear Schrödinger equation]].&lt;br /&gt;
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There are no generally applicable methods to solve nonlinear PDEs. Still, existence and uniqueness results (such as the Cauchy–Kowalevski theorem) are often possible, as are proofs of important qualitative and quantitative properties of solutions (getting these results is a major part of analysis). Computational solution to the nonlinear PDEs, the split-step method, exist for specific equations like nonlinear Schrödinger equation.&lt;br /&gt;
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对于非线性偏微分方程，目前还没有普遍适用的求解方法。然而，通常是可能知道解的存在性和唯一性(如柯西-科瓦列夫斯基定理)，也是可能得到解的重要定性和定量性质的证明(得到这些结果是分析的主要部分)。非线性偏微分方程的计算解，即分步法，对一些特定的方程适用，比如非线性'''&amp;lt;font color=&amp;quot;#ff8000&amp;quot;&amp;gt;薛定谔方程 Schrödinger equation&amp;lt;/font&amp;gt;'''。&lt;br /&gt;
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Nevertheless, some techniques can be used for several types of equations. The [[h-principle|{{mvar|h}}-principle]] is the most powerful method to solve [[Underdetermined system|underdetermined]] equations. The [[Riquier–Janet theory]] is an effective method for obtaining information about many analytic [[Overdetermined system|overdetermined]] systems.&lt;br /&gt;
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Nevertheless, some techniques can be used for several types of equations. The -principle is the most powerful method to solve underdetermined equations. The Riquier–Janet theory is an effective method for obtaining information about many analytic overdetermined systems.&lt;br /&gt;
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然而，一些技巧可以用于几种类型的方程。h-原理是求解欠定方程最有效的方法。里基尔-珍妮特理论是一种可以获得许多解析超定系统信息的有效方法。&lt;br /&gt;
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The [[method of characteristics]] can be used in some very special cases to solve partial differential equations.&lt;br /&gt;
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The method of characteristics can be used in some very special cases to solve partial differential equations.&lt;br /&gt;
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特征线法可用于求解某些特殊情况下的偏微分方程。&lt;br /&gt;
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In some cases, a PDE can be solved via [[perturbation analysis]] in which the solution is considered to be a correction to an equation with a known solution. Alternatives are [[numerical analysis]] techniques from simple [[finite difference]] schemes to the more mature [[multigrid]] and [[finite element method]]s. Many interesting problems in science and engineering are solved in this way using [[computer]]s, sometimes high performance [[supercomputer]]s.&lt;br /&gt;
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In some cases, a PDE can be solved via perturbation analysis in which the solution is considered to be a correction to an equation with a known solution. Alternatives are numerical analysis techniques from simple finite difference schemes to the more mature multigrid and finite element methods. Many interesting problems in science and engineering are solved in this way using computers, sometimes high performance supercomputers.&lt;br /&gt;
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在某些情况下，偏微分方程可以通过扰动分析来求解。在扰动分析中，通常是求解将具有已知解的方程修正后的新得到方程。可供选择的数值分析技术从简单的差分格式到更成熟的多重网格和有限元方法。许多有趣的科学和工程问题都是在计算机上用这种方法解决的，有时是高性能超级计算机。&lt;br /&gt;
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===Lie group method===&lt;br /&gt;
李群方法&lt;br /&gt;
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From 1870 [[Sophus Lie]]'s work put the theory of differential equations on a more satisfactory foundation. He showed that the integration theories of the older mathematicians can, by the introduction of what are now called [[Lie group]]s, be referred, to a common source; and that ordinary differential equations which admit the same [[infinitesimal transformation]]s present comparable difficulties of integration. He also emphasized the subject of [[contact transformation|transformations of contact]].&lt;br /&gt;
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From 1870 Sophus Lie's work put the theory of differential equations on a more satisfactory foundation. He showed that the integration theories of the older mathematicians can, by the introduction of what are now called Lie groups, be referred, to a common source; and that ordinary differential equations which admit the same infinitesimal transformations present comparable difficulties of integration. He also emphasized the subject of transformations of contact.&lt;br /&gt;
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从1870年起，索弗斯·李的工作为微分方程理论奠定了一个较为令人满意的基础。他指出，通过引入现在所谓的李群，老一辈数学家的积分理论可以引用到一个共同的来源; 承认相同的无穷小变换的常微分方程在积分方面存在相当的困难。他还强调了接触的转变这一主题。&lt;br /&gt;
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==[[用户:Yuling|Yuling]]（[[用户讨论:Yuling|讨论]]）这句话“He also emphasized the subject of transformations of contact.”中的transformations of contact翻译的不太好。&lt;br /&gt;
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A general approach to solving PDEs uses the symmetry property of differential equations, the continuous [[infinitesimal transformation]]s of solutions to solutions ([[Lie theory]]). Continuous [[group theory]], [[Lie algebras]] and [[differential geometry]] are used to understand the structure of linear and nonlinear partial differential equations for generating integrable equations, to find its [[Lax pair]]s, recursion operators, [[Bäcklund transform]] and finally finding exact analytic solutions to the PDE.&lt;br /&gt;
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A general approach to solving PDEs uses the symmetry property of differential equations, the continuous infinitesimal transformations of solutions to solutions (Lie theory). Continuous group theory, Lie algebras and differential geometry are used to understand the structure of linear and nonlinear partial differential equations for generating integrable equations, to find its Lax pairs, recursion operators, Bäcklund transform and finally finding exact analytic solutions to the PDE.&lt;br /&gt;
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求解偏微分方程的一般方法是利用微分方程的对称性，即解到解的连续无穷小变换(李理论)。连续群论、李代数和微分几何理论被用来理解生成可积方程的线性和非线性偏微分方程的结构，找到它的Lax对、递归算子、 贝克伦德变换，最后找到偏微分方程的精确解析解。&lt;br /&gt;
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Symmetry methods have been recognized to study differential equations arising in mathematics, physics, engineering, and many other disciplines.&lt;br /&gt;
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Symmetry methods have been recognized to study differential equations arising in mathematics, physics, engineering, and many other disciplines.&lt;br /&gt;
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对称方法已被公认可以用于研究出现在数学，物理，工程和许多其他学科的微分方程。&lt;br /&gt;
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===Semianalytical methods===&lt;br /&gt;
半解析方法&lt;br /&gt;
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The [[Adomian decomposition method]], the [[Aleksandr Lyapunov|Lyapunov]] artificial small parameter method, and He's [[homotopy perturbation method]] are all special cases of the more general [[homotopy analysis method]]. These are series expansion methods, and except for the Lyapunov method, are independent of small physical parameters as compared to the well known [[perturbation theory]], thus giving these methods greater flexibility and solution generality.&lt;br /&gt;
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The Adomian decomposition method, the Lyapunov artificial small parameter method, and He's homotopy perturbation method are all special cases of the more general homotopy analysis method. These are series expansion methods, and except for the Lyapunov method, are independent of small physical parameters as compared to the well known perturbation theory, thus giving these methods greater flexibility and solution generality.&lt;br /&gt;
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阿多米安分解法、李雅普诺夫人工小参数方法和何同伦摄动方法都是更一般的同伦分析方法的特殊情况。除了李雅普诺夫方法之外，这些都是级数展开方法，与为人熟知的摄动理论方法相比，它们与小的物理参数无关，因此这些方法具有更大的灵活性和解的通用性。&lt;br /&gt;
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== Numerical solutions ==&lt;br /&gt;
数值解&lt;br /&gt;
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The three most widely used [[Numerical partial differential equations|numerical methods to solve PDEs]] are the [[finite element analysis|finite element method]] (FEM), [[finite volume method]]s (FVM) and [[finite difference method]]s (FDM), as well other kind of methods called [[Meshfree methods]], which were made to solve problems where the before mentioned methods are limited. The FEM has a prominent position among these methods and especially its exceptionally efficient higher-order version [[hp-FEM]]. Other hybrid versions of FEM and Meshfree methods include the generalized finite element method (GFEM), [[extended finite element method]] (XFEM), [[Spectral element method|spectral finite element method]] (SFEM), [[Meshfree methods|meshfree finite element method]], [[Discontinuous Galerkin Method|discontinuous Galerkin finite element method]] (DGFEM), [[Element-Free Galerkin Method]] (EFGM), [[Interpolating Element-Free Galerkin Method]] (IEFGM), etc.&lt;br /&gt;
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The three most widely used numerical methods to solve PDEs are the finite element method (FEM), finite volume methods (FVM) and finite difference methods (FDM), as well other kind of methods called Meshfree methods, which were made to solve problems where the before mentioned methods are limited. The FEM has a prominent position among these methods and especially its exceptionally efficient higher-order version hp-FEM. Other hybrid versions of FEM and Meshfree methods include the generalized finite element method (GFEM), extended finite element method (XFEM), spectral finite element method (SFEM), meshfree finite element method, discontinuous Galerkin finite element method (DGFEM), Element-Free Galerkin Method (EFGM), Interpolating Element-Free Galerkin Method (IEFGM), etc.&lt;br /&gt;
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求解偏微分方程最常用的三种数值方法是有限元分析法、有限体积法和有限差分法，以及其他一些称为无网格法的方法。这些方法用于解决前面提到的方法受到的限制。在这些方法中，有限元方法，尤其是高效的高阶有限元方法，占有重要地位。其他有限元法和无网格法的混合形式包括广义有限元分析法(GFEM)、扩展有限元分析法(XFEM)、谱有限元分析法(SFEM)、无网格有限元分析法(DGFEM)、间断伽辽金有限元分析法(DGFEM)、无网格伽辽金法(EFGM)、插值无网格伽辽金法(IEFGM)等。&lt;br /&gt;
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=== Finite element method ===&lt;br /&gt;
有限元分析法&lt;br /&gt;
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{{main|Finite element method}}&lt;br /&gt;
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The finite element method (FEM) (its practical application often known as finite element analysis (FEA)) is a numerical technique for finding approximate solutions of partial differential equations (PDE) as well as of integral equations. The solution approach is based either on eliminating the differential equation completely (steady state problems), or rendering the PDE into an approximating system of ordinary differential equations, which are then numerically integrated using standard techniques such as Euler's method, Runge–Kutta, etc.&lt;br /&gt;
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The finite element method (FEM) (its practical application often known as finite element analysis (FEA)) is a numerical technique for finding approximate solutions of partial differential equations (PDE) as well as of integral equations. The solution approach is based either on eliminating the differential equation completely (steady state problems), or rendering the PDE into an approximating system of ordinary differential equations, which are then numerically integrated using standard techniques such as Euler's method, Runge–Kutta, etc.&lt;br /&gt;
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'''&amp;lt;font color = &amp;quot;#ff8000&amp;quot;&amp;gt;有限元分析法 Finite Element Method&amp;lt;/font&amp;gt;''' ((其实际应用通常被称为有限元分析(FEA))是一种寻找偏微分方程(PDE)和积分方程近似解的数值技术。这种求解方法要么基于完全消除微分方程(稳态问题) ，要么将偏微分方程转化为常微分方程的近似系统，然后使用标准技术进行数值积分，如欧拉方法、 Runge-Kutta 等。&lt;br /&gt;
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===Finite difference method===&lt;br /&gt;
有限差分法&lt;br /&gt;
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{{main|Finite difference method}}&lt;br /&gt;
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Finite-difference methods are numerical methods for approximating the solutions to differential equations using [[finite difference]] equations to approximate derivatives.&lt;br /&gt;
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Finite-difference methods are numerical methods for approximating the solutions to differential equations using finite difference equations to approximate derivatives.&lt;br /&gt;
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有限差分法是一种数值方法，用差分方程近似微分方程的解。&lt;br /&gt;
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=== Finite volume method ===&lt;br /&gt;
有限体积法&lt;br /&gt;
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{{main|Finite volume method}}&lt;br /&gt;
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Similar to the finite difference method or finite element method, values are calculated at discrete places on a meshed geometry. &amp;quot;Finite volume&amp;quot; refers to the small volume surrounding each node point on a mesh. In the finite volume method, surface integrals in a partial differential equation that contain a divergence term are converted to volume integrals, using the [[divergence theorem]]. These terms are then evaluated as fluxes at the surfaces of each finite volume. Because the flux entering a given volume is identical to that leaving the adjacent volume, these methods conserve mass by design.&lt;br /&gt;
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Similar to the finite difference method or finite element method, values are calculated at discrete places on a meshed geometry. &amp;quot;Finite volume&amp;quot; refers to the small volume surrounding each node point on a mesh. In the finite volume method, surface integrals in a partial differential equation that contain a divergence term are converted to volume integrals, using the divergence theorem. These terms are then evaluated as fluxes at the surfaces of each finite volume. Because the flux entering a given volume is identical to that leaving the adjacent volume, these methods conserve mass by design.&lt;br /&gt;
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类似于有限差分法或有限元分析，函数值是在网状几何体上的离散位置进行计算的。“有限体积”是指网格上每个节点周围的小体积。在有限体积法中，偏微分方程中含有散度项的面积分用散度定理积分转换成体积分。然后将这些项用于估算每个有限体积表面上的通量。由于进入给定体积的通量与转移到相邻体积元的通量相同，所以这些方法在设计上保证了质量守恒。&lt;br /&gt;
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==See also==&lt;br /&gt;
请参阅&lt;br /&gt;
* [[Dirichlet boundary condition]]&lt;br /&gt;
狄利克雷边界条件&lt;br /&gt;
* [[Jet bundle]]&lt;br /&gt;
射流丛&lt;br /&gt;
* [[Laplace transform applied to differential equations]]&lt;br /&gt;
微分方程中的拉普拉斯变换&lt;br /&gt;
* [[List of dynamical systems and differential equations topics]]&lt;br /&gt;
动力学系统和微分方程的列表&lt;br /&gt;
* [[Matrix differential equation]]&lt;br /&gt;
矩阵微分方程&lt;br /&gt;
* [[Neumann boundary condition]]&lt;br /&gt;
诺伊曼边界条件&lt;br /&gt;
* [[Numerical partial differential equations]]&lt;br /&gt;
数值偏微分方程&lt;br /&gt;
* [[Partial differential algebraic equation]]&lt;br /&gt;
偏微分代数方程&lt;br /&gt;
* [[Recurrence relation]]&lt;br /&gt;
递推关系&lt;br /&gt;
* [[Robin boundary condition]]&lt;br /&gt;
罗宾边界条件&lt;br /&gt;
* [[Stochastic processes and boundary value problems]]&lt;br /&gt;
随机过程和边值问题&lt;br /&gt;
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== The energy method ==&lt;br /&gt;
能量法&lt;br /&gt;
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The energy method is a mathematical procedure that can be used to verify well-posedness of initial-boundary-value-problems.&amp;lt;ref&amp;gt;{{cite book |title=High Order Difference Methods for Time Dependent PDE&lt;br /&gt;
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The energy method is a mathematical procedure that can be used to verify well-posedness of initial-boundary-value-problems.&amp;lt;ref&amp;gt;{{cite book |title=High Order Difference Methods for Time Dependent PDE&lt;br /&gt;
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能量法是验证初边值问题适定性的一种数学方法。 时变偏微分方程的高阶差分方法&lt;br /&gt;
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|first=Bertil|last=Gustafsson|publisher=Springer|year=2008|isbn=978-3-540-74992-9|doi=10.1007/978-3-540-74993-6}}&amp;lt;/ref&amp;gt; In the following example the energy method is used to decide where and which boundary conditions should be imposed such that the resulting IBVP is well-posed. Consider the one-dimensional hyperbolic PDE given by&lt;br /&gt;
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|first=Bertil|last=Gustafsson|publisher=Springer|year=2008|isbn=978-3-540-74992-9|doi=10.1007/978-3-540-74993-6}}&amp;lt;/ref&amp;gt; In the following example the energy method is used to decide where and which boundary conditions should be imposed such that the resulting IBVP is well-posed. Consider the one-dimensional hyperbolic PDE given by&lt;br /&gt;
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| first Bertil | last Gustafsson | publisher | Springer | year 2008 | isbn 978-3-540-74992-9 | doi 10.1007 / 978-3-540-74993-6} / ref 在下面的例子中，使用能量方法来决定应该施加哪些边界条件，使得得到的 IBVP适定。考虑一维双曲偏微分方程&lt;br /&gt;
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: &amp;lt;math&amp;gt;\frac{\partial u}{\partial t} + \alpha \frac{\partial u}{\partial x} = 0, \quad x \in [a,b], \operatorname t &amp;gt; 0,&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;\frac{\partial u}{\partial t} + \alpha \frac{\partial u}{\partial x} = 0, \quad x \in [a,b], \operatorname t &amp;gt; 0,&amp;lt;/math&amp;gt;&lt;br /&gt;
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where &amp;lt;math&amp;gt;\alpha \neq 0&amp;lt;/math&amp;gt; is a constant and &amp;lt;math&amp;gt;u(x,t)&amp;lt;/math&amp;gt; is an unknown function with initial condition &amp;lt;math&amp;gt;u(x,0) = f(x)&amp;lt;/math&amp;gt;. Multiplying with &amp;lt;math&amp;gt;u&amp;lt;/math&amp;gt; and integrating over the domain gives&lt;br /&gt;
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where &amp;lt;math&amp;gt;\alpha \neq 0&amp;lt;/math&amp;gt; is a constant and &amp;lt;math&amp;gt;u(x,t)&amp;lt;/math&amp;gt; is an unknown function with initial condition &amp;lt;math&amp;gt;u(x,0) = f(x)&amp;lt;/math&amp;gt;. Multiplying with &amp;lt;math&amp;gt;u&amp;lt;/math&amp;gt; and integrating over the domain gives&lt;br /&gt;
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其中 &amp;lt;math&amp;gt;\alpha \neq 0&amp;lt;/math&amp;gt; 是常数，并且 &amp;lt;math&amp;gt;u(x,t)&amp;lt;/math&amp;gt; 是未知函数，初始条件是 &amp;lt;math&amp;gt;u(x,0) = f(x)&amp;lt;/math&amp;gt;。乘以 &amp;lt;math&amp;gt;u&amp;lt;/math&amp;gt; 并在域上进行积分。&lt;br /&gt;
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: &amp;lt;math&amp;gt;\int_a^b u \frac{\partial u}{\partial t} \operatorname dx + \alpha \int _a ^b u \frac{\partial u}{\partial x} \operatorname dx = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;\int_a^b u \frac{\partial u}{\partial t} \operatorname dx + \alpha \int _a ^b u \frac{\partial u}{\partial x} \operatorname dx = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
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Using that&lt;br /&gt;
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Using that&lt;br /&gt;
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利用这一点&lt;br /&gt;
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: &amp;lt;math&amp;gt;\int _a ^b u \frac{\partial u}{\partial t} \operatorname dx = \frac{1}{2} \frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 \quad \text{and} \quad \int _a ^b u \frac{\partial u}{\partial x} \operatorname dx = \frac{1}{2} u(b,t)^2 - \frac{1}{2} u(a,t)^2,.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;\int _a ^b u \frac{\partial u}{\partial t} \operatorname dx = \frac{1}{2} \frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 \quad \text{and} \quad \int _a ^b u \frac{\partial u}{\partial x} \operatorname dx = \frac{1}{2} u(b,t)^2 - \frac{1}{2} u(a,t)^2,.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
where integration by parts has been used for the second relationship, we get&lt;br /&gt;
&lt;br /&gt;
where integration by parts has been used for the second relationship, we get&lt;br /&gt;
&lt;br /&gt;
第二个关系中采用了分部积分法，我们可以得到&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt;\frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 + \alpha u(b,t)^2 - \alpha u(a,t)^2 = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;\frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 + \alpha u(b,t)^2 - \alpha u(a,t)^2 = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Here &amp;lt;math&amp;gt;\vert \vert \cdot \vert \vert&amp;lt;/math&amp;gt; denotes the standard L2-norm.&lt;br /&gt;
&lt;br /&gt;
Here &amp;lt;math&amp;gt;\vert \vert \cdot \vert \vert&amp;lt;/math&amp;gt; denotes the standard L2-norm.&lt;br /&gt;
&lt;br /&gt;
在这里，&amp;lt;math&amp;gt;\vert \vert \cdot \vert \vert&amp;lt;/math&amp;gt; 表示标准的 L2-正则。&lt;br /&gt;
&lt;br /&gt;
For well-posedness we require that the energy of the solution is non-increasing, i.e. that &amp;lt;math&amp;gt;\frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 \leq 0&amp;lt;/math&amp;gt;, which is achieved by specifying &amp;lt;math&amp;gt;u&amp;lt;/math&amp;gt; at &amp;lt;math&amp;gt;x = a&amp;lt;/math&amp;gt; if &amp;lt;math&amp;gt;\alpha &amp;gt; 0&amp;lt;/math&amp;gt; and at &amp;lt;math&amp;gt;x = b&amp;lt;/math&amp;gt; if &amp;lt;math&amp;gt;\alpha &amp;lt; 0&amp;lt;/math&amp;gt;. This corresponds to only imposing boundary conditions at the inflow. Note that well-posedness allows for growth in terms of data (initial and boundary) and thus it is sufficient to show that &amp;lt;math&amp;gt;\frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 \leq 0&amp;lt;/math&amp;gt; holds when all data is set to zero.&lt;br /&gt;
&lt;br /&gt;
For well-posedness we require that the energy of the solution is non-increasing, i.e. that &amp;lt;math&amp;gt;\frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 \leq 0&amp;lt;/math&amp;gt;, which is achieved by specifying &amp;lt;math&amp;gt;u&amp;lt;/math&amp;gt; at &amp;lt;math&amp;gt;x = a&amp;lt;/math&amp;gt; if &amp;lt;math&amp;gt;\alpha &amp;gt; 0&amp;lt;/math&amp;gt; and at &amp;lt;math&amp;gt;x = b&amp;lt;/math&amp;gt; if &amp;lt;math&amp;gt;\alpha &amp;lt; 0&amp;lt;/math&amp;gt;. This corresponds to only imposing boundary conditions at the inflow. Note that well-posedness allows for growth in terms of data (initial and boundary) and thus it is sufficient to show that &amp;lt;math&amp;gt;\frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 \leq 0&amp;lt;/math&amp;gt; holds when all data is set to zero.&lt;br /&gt;
&lt;br /&gt;
对于适定性，我们要解的能量是不增加的，即 &amp;lt;math&amp;gt;\frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 \leq 0&amp;lt;/math&amp;gt; ，这种关系可以通过在&amp;lt;math&amp;gt;x = a&amp;lt;/math&amp;gt;处 （如果 &amp;lt;math&amp;gt;\alpha &amp;gt; 0&amp;lt;/math&amp;gt;） 以及 &amp;lt;math&amp;gt;x = b&amp;lt;/math&amp;gt;处 （如果 &amp;lt;math&amp;gt;\alpha &amp;lt; 0&amp;lt;/math&amp;gt;）指定&amp;lt;math&amp;gt;u&amp;lt;/math&amp;gt;的值来实现。这只相当于在入流处附加边界条件。注意，适定性允许在数据(初始和边界)上的增长，因此它足以表明当所有数据设置为零时应有 &amp;lt;math&amp;gt;\frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 \leq 0&amp;lt;/math&amp;gt;。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==[[用户:Yuling|Yuling]]（[[用户讨论:Yuling|讨论]]）“This corresponds to only imposing boundary conditions at the inflow.” 这句话中的inflow不是很理解&lt;br /&gt;
&lt;br /&gt;
==Notes==&lt;br /&gt;
&lt;br /&gt;
{{Reflist}}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
== References ==&lt;br /&gt;
&lt;br /&gt;
{{refbegin|2}}&lt;br /&gt;
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|first=G.|last=Adomian|publisher=Kluwer Academic Publishers|year=1994|isbn=|page=|url=https://books.google.com/books?id=UKPqCAAAQBAJ&amp;amp;printsec=frontcover#v=onepage&amp;amp;q=%22partial%20differential%22&amp;amp;f=false}}&lt;br /&gt;
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&lt;br /&gt;
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&lt;br /&gt;
* {{Citation |first=P. |last=Solin |first2=K. |last2=Segeth |lastauthoramp=yes |first3=I. |last3=Dolezel |title=Higher-Order Finite Element Methods |publisher=Chapman &amp;amp; Hall/CRC Press |location=Boca Raton |year=2003 |isbn=1-58488-438-X }}.&lt;br /&gt;
&lt;br /&gt;
* {{Citation |first=H. |last=Stephani |year=1989 |title=Differential Equations: Their Solution Using Symmetries. Edited by M. MacCallum |publisher=Cambridge University Press }}.&lt;br /&gt;
&lt;br /&gt;
* {{cite book |title=Partial Differential Equations and Solitary Waves Theory&lt;br /&gt;
&lt;br /&gt;
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| first Abdul-Majid | last Wazwaz | publisher Higher Education Press | year 2009 | isbn 978-3-642-00251-9 | page }&lt;br /&gt;
&lt;br /&gt;
* {{cite book |title=Partial Differential Equations Methods and Applications&lt;br /&gt;
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| first Abdul-Majid | last Wazwaz | publisher a.a.Balkema | year 2002 | isbn 90-5809-369-7 | page }&lt;br /&gt;
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&lt;br /&gt;
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&lt;br /&gt;
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&lt;br /&gt;
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&lt;br /&gt;
* {{cite book |title=High Order Difference Methods for Time Dependent PDE&lt;br /&gt;
&lt;br /&gt;
|first=Bertil|last=Gustafsson|publisher=Springer|year=2008|isbn=978-3-540-74992-9|doi=10.1007/978-3-540-74993-6}}&lt;br /&gt;
&lt;br /&gt;
|first=Bertil|last=Gustafsson|publisher=Springer|year=2008|isbn=978-3-540-74992-9|doi=10.1007/978-3-540-74993-6}}&lt;br /&gt;
&lt;br /&gt;
| first Bertil | last Gustafsson | Springer | year 2008 | isbn 978-3-540-74992-9 | doi 10.1007 / 978-3-540-74993-6}&lt;br /&gt;
&lt;br /&gt;
{{refend}}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
== Further reading ==&lt;br /&gt;
&lt;br /&gt;
* {{Cite journal|last=Cajori|first=Florian|authorlink=Florian Cajori|year=1928|title=The Early History of Partial Differential Equations and of Partial Differentiation and Integration|url=http://www.math.harvard.edu/archive/21a_fall_14/exhibits/cajori/cajori.pdf|journal=The American Mathematical Monthly|volume=35|issue=9|pages=459–467|doi=10.2307/2298771|access-date=2016-05-15|archive-url=https://web.archive.org/web/20181123102253/http://www.math.harvard.edu/archive/21a_fall_14/exhibits/cajori/cajori.pdf|archive-date=2018-11-23|url-status=dead}}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
== External links ==&lt;br /&gt;
&lt;br /&gt;
{{Sister project links| wikt=no | commons=Category:Solutions of PDE | b=Partial Differential Equations | n=no | q=Partial differential equation | s=no | v=no | voy=no | species=no | d=no}}&lt;br /&gt;
&lt;br /&gt;
* {{springer|title=Differential equation, partial|id=p/d031920}}&lt;br /&gt;
&lt;br /&gt;
* [http://eqworld.ipmnet.ru/en/pde-en.htm Partial Differential Equations: Exact Solutions] at EqWorld: The World of Mathematical Equations.&lt;br /&gt;
&lt;br /&gt;
* [http://eqworld.ipmnet.ru/en/solutions/eqindex/eqindex-pde.htm Partial Differential Equations: Index] at EqWorld: The World of Mathematical Equations.&lt;br /&gt;
&lt;br /&gt;
* [http://eqworld.ipmnet.ru/en/methods/meth-pde.htm Partial Differential Equations: Methods] at EqWorld: The World of Mathematical Equations.&lt;br /&gt;
&lt;br /&gt;
* [https://web.archive.org/web/20170701144823/http://www.exampleproblems.com/wiki/index.php?title=Partial_Differential_Equations Example problems with solutions] at exampleproblems.com&lt;br /&gt;
&lt;br /&gt;
* [http://mathworld.wolfram.com/PartialDifferentialEquation.html Partial Differential Equations] at mathworld.wolfram.com&lt;br /&gt;
&lt;br /&gt;
* [https://reference.wolfram.com/language/FEMDocumentation/tutorial/SolvingPDEwithFEM.html Partial Differential Equations] with Mathematica&lt;br /&gt;
&lt;br /&gt;
* [http://www.mathworks.com/moler/pdes.pdf Partial Differential Equations] in Cleve Moler: Numerical Computing with MATLAB&lt;br /&gt;
&lt;br /&gt;
* [http://www.nag.com/numeric/fl/nagdoc_fl24/html/D03/d03intro.html Partial Differential Equations] at nag.com&lt;br /&gt;
&lt;br /&gt;
* {{cite web |first=Grant |last=Sanderson |title=But what is a partial differential equation? |work=3Blue1Brown |date=April 21, 2019 |url=https://www.youtube.com/watch?v=ly4S0oi3Yz8&amp;amp;list=PLZHQObOWTQDNPOjrT6KVlfJuKtYTftqH6 |via=[[YouTube]] }}&lt;br /&gt;
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&lt;br /&gt;
{{Differential equations topics}}&lt;br /&gt;
&lt;br /&gt;
{{Authority control}}&lt;br /&gt;
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&lt;br /&gt;
[[Category:Partial differential equations| ]]&lt;br /&gt;
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[[Category:Multivariable calculus]]&lt;br /&gt;
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Category:Multivariable calculus&lt;br /&gt;
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类别: 多元微积分&lt;br /&gt;
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[[Category:Differential equations]]&lt;br /&gt;
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Category:Differential equations&lt;br /&gt;
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类别: 微分方程&lt;br /&gt;
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[[Category:Concepts in physics]]&lt;br /&gt;
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Category:Concepts in physics&lt;br /&gt;
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分类: 物理概念&lt;br /&gt;
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&amp;lt;noinclude&amp;gt;&lt;br /&gt;
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&amp;lt;small&amp;gt;This page was moved from [[wikipedia:en:Partial differential equation]]. Its edit history can be viewed at [[偏微分方程/edithistory]]&amp;lt;/small&amp;gt;&amp;lt;/noinclude&amp;gt;&lt;br /&gt;
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[[Category:待整理页面]]&lt;/div&gt;</summary>
		<author><name>Ruili</name></author>
	</entry>
	<entry>
		<id>https://wiki.swarma.org/index.php?title=%E5%81%8F%E5%BE%AE%E5%88%86%E6%96%B9%E7%A8%8B&amp;diff=18121</id>
		<title>偏微分方程</title>
		<link rel="alternate" type="text/html" href="https://wiki.swarma.org/index.php?title=%E5%81%8F%E5%BE%AE%E5%88%86%E6%96%B9%E7%A8%8B&amp;diff=18121"/>
		<updated>2020-11-11T14:04:22Z</updated>

		<summary type="html">&lt;p&gt;Ruili：&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;此词条暂由Yuling翻译，未经人工整理和审校，带来阅读不便，请见谅。&lt;br /&gt;
&lt;br /&gt;
[[File:Heat.gif|thumb|right|A visualisation of a solution to the two-dimensional [[heat equation]] with temperature represented by the third dimension]]&lt;br /&gt;
&lt;br /&gt;
A visualisation of a solution to the two-dimensional [[heat equation with temperature represented by the third dimension]]&lt;br /&gt;
&lt;br /&gt;
以三维表示温度的二维热方程解的可视化&lt;br /&gt;
&lt;br /&gt;
In [[mathematics]], a '''partial differential equation''' ('''PDE''') is a [[differential equation]] that contains unknown [[Multivariable calculus|multivariable functions]] and their [[partial derivative]]s. PDEs are used to formulate problems involving functions of several variables, and are either solved by hand, or used to create a [[computer model]]. A special case is [[ordinary differential equation]]s (ODEs), which deal with functions of a single variable and their derivatives.&lt;br /&gt;
&lt;br /&gt;
In mathematics, a partial differential equation (PDE) is a differential equation that contains unknown multivariable functions and their partial derivatives. PDEs are used to formulate problems involving functions of several variables, and are either solved by hand, or used to create a computer model. A special case is ordinary differential equations (ODEs), which deal with functions of a single variable and their derivatives.&lt;br /&gt;
&lt;br /&gt;
在数学中，'''&amp;lt;font color = &amp;quot;#ff8000&amp;quot;&amp;gt; 偏微分方程函数 Partial Differential Equation&amp;lt;/font&amp;gt;'''是包含未知多元函数及其偏导数的微分方程。偏微分方程用于描述涉及多元函数的问题，可以通过人为求解，也可以通过建立计算机模型来求解。常微分方程是偏微分方程一种特殊情况，它处理的是一元函数及其导数。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
PDEs can be used to describe a wide variety of phenomena such as sound, heat, [[diffusion]], [[electrostatics]], [[Electromagnetism|electrodynamics]], [[fluid dynamics]], [[Elasticity (physics)|elasticity]], [[gravitation]] and [[quantum mechanics]]. These seemingly distinct physical phenomena can be formalised similarly in terms of PDEs. Just as ordinary differential equations often model one-dimensional [[dynamical system]]s, partial differential equations often model [[multidimensional system]]s. PDEs find their generalisation in [[stochastic partial differential equation]]s.&lt;br /&gt;
&lt;br /&gt;
PDEs can be used to describe a wide variety of phenomena such as sound, heat, diffusion, electrostatics, electrodynamics, fluid dynamics, elasticity, gravitation and quantum mechanics. These seemingly distinct physical phenomena can be formalised similarly in terms of PDEs. Just as ordinary differential equations often model one-dimensional dynamical systems, partial differential equations often model multidimensional systems. PDEs find their generalisation in stochastic partial differential equations.&lt;br /&gt;
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偏微分方程可以用来描述各种各样的物理现象，如声音，热量，扩散，静电，电动力学，流体力学，弹性力学，重力和量子力学。这些看起来截然不同的物理现象却可以用类似的偏微分方程来描述。正如常微分方程经常对一维动力系统进行建模一样，偏微分方程经常对多维系统进行建模。随机偏微分方程是偏微分方程的一种推广。&lt;br /&gt;
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== Introduction ==&lt;br /&gt;
引言&lt;br /&gt;
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Partial differential equations (PDEs) are equations that involve rates of change with respect to [[continuous variables]]. For example, the position of a [[rigid body]] is specified by six parameters,&amp;lt;ref&amp;gt;{{Cite book|url=https://books.google.com/books?id=v9PLbcYd9aUC&amp;amp;pg=PA32|title=Modelling and Control of Robot Manipulators|last=Sciavicco|first=Lorenzo|last2=Siciliano|first2=Bruno|date=2001-02-19|publisher=Springer Science &amp;amp; Business Media|isbn=9781852332211|language=en}}&amp;lt;/ref&amp;gt; but the configuration of a [[fluid]] is given by the [[continuous distribution]] of several parameters, such as the [[temperature]], [[pressure]], and so forth. The dynamics for the rigid body take place in a finite-dimensional [[Configuration space (physics)|configuration space]]; the dynamics for the fluid occur in an infinite-dimensional configuration space. This distinction usually makes PDEs much harder to solve than ordinary differential equations (ODEs), but here again, there will be simple solutions for linear problems. Classic domains where PDEs are used include [[acoustics]], [[fluid dynamics]], [[electrodynamics]], and [[heat transfer]].&lt;br /&gt;
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Partial differential equations (PDEs) are equations that involve rates of change with respect to continuous variables. For example, the position of a rigid body is specified by six parameters, but the configuration of a fluid is given by the continuous distribution of several parameters, such as the temperature, pressure, and so forth. The dynamics for the rigid body take place in a finite-dimensional configuration space; the dynamics for the fluid occur in an infinite-dimensional configuration space. This distinction usually makes PDEs much harder to solve than ordinary differential equations (ODEs), but here again, there will be simple solutions for linear problems. Classic domains where PDEs are used include acoustics, fluid dynamics, electrodynamics, and heat transfer.&lt;br /&gt;
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偏微分方程(简称为PDEs)涉及到方程相对于连续变量的变化率。例如，刚体的位置是由六个参数确定的，而流体的状态是由几个参数的连续分布给出的，如温度、压力等。刚体的动力学过程发生在有限维状态空间中，流体的动力学过程发生在无限维状态空间中。这种区别通常使偏微分方程比常微分方程更难求解，但是线性问题仍然有简单的求解方式。使用偏微分方程的经典领域包括声学、流体力学、电动力学和传热学。&lt;br /&gt;
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A partial differential equation (PDE) for the function {{math|''u''(''x''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;,… ''x&amp;lt;sub&amp;gt;n&amp;lt;/sub&amp;gt;'')}} is an equation of the form&lt;br /&gt;
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A partial differential equation (PDE) for the function  is an equation of the form&lt;br /&gt;
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函数 {{math|''u''(''x''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;,… ''x&amp;lt;sub&amp;gt;n&amp;lt;/sub&amp;gt;'')}} 的偏微分方程形式是：&lt;br /&gt;
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: &amp;lt;math&amp;gt;f \left (x_1, \ldots x_n; u, \frac{\partial u}{\partial x_1}, \ldots \frac{\partial u}{\partial x_n}; \frac{\partial^2 u}{\partial x_1 \partial x_1}, \ldots \frac{\partial^2 u}{\partial x_1 \partial x_n}; \ldots \right) = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;f \left (x_1, \ldots x_n; u, \frac{\partial u}{\partial x_1}, \ldots \frac{\partial u}{\partial x_n}; \frac{\partial^2 u}{\partial x_1 \partial x_1}, \ldots \frac{\partial^2 u}{\partial x_1 \partial x_n}; \ldots \right) = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
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If {{mvar|f}} is a [[linear function]] of {{mvar|u}} and its derivatives, then the PDE is called linear. Common examples of linear PDEs include the [[heat equation]], the [[wave equation]], [[Laplace's equation]], [[Helmholtz equation]], [[Klein–Gordon equation]], and [[Poisson's equation]].&lt;br /&gt;
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If  is a linear function of  and its derivatives, then the PDE is called linear. Common examples of linear PDEs include the heat equation, the wave equation, Laplace's equation, Helmholtz equation, Klein–Gordon equation, and Poisson's equation.&lt;br /&gt;
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如果 {{mvar|f}} 是函数 {{math|''u''}} 及其导数的线性函数，则偏微分方程称为线性函数。线性偏微分方程的常见例子包括热方程、波动方程、拉普拉斯方程、亥姆霍兹方程方程、克莱因-高登方程和泊松方程。&lt;br /&gt;
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A relatively simple PDE is&lt;br /&gt;
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A relatively simple PDE is&lt;br /&gt;
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一个相对简单的偏微分方程：&lt;br /&gt;
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: &amp;lt;math&amp;gt;\frac{\partial u}{\partial x}(x,y) = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;\frac{\partial u}{\partial x}(x,y) = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
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This relation [[Logical implication|implies]] that the function {{math|''u''(''x'',''y'')}} is independent of {{mvar|x}}. However, the equation gives no information on the function's dependence on the variable {{mvar|y}}. Hence the general solution of this equation is&lt;br /&gt;
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This relation implies that the function  is independent of . However, the equation gives no information on the function's dependence on the variable . Hence the general solution of this equation is&lt;br /&gt;
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这意味着函数 {{math|''u''(''x'',''y'')}} 独立于 {{mvar|x}} 的。然而，这个方程没有给出关于函数和自变量的相关性的信息。因此，这个方程的通解是&lt;br /&gt;
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: &amp;lt;math&amp;gt;u(x,y) = f(y),&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;u(x,y) = f(y),&amp;lt;/math&amp;gt;&lt;br /&gt;
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where {{mvar|f}} is an arbitrary function of {{mvar|y}}. The analogous ordinary differential equation is&lt;br /&gt;
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where  is an arbitrary function of . The analogous ordinary differential equation is&lt;br /&gt;
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其中， {{mvar|f}} 是 {{mvar|y}} 的任意函数。&lt;br /&gt;
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类似的常微分方程是：&lt;br /&gt;
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: &amp;lt;math&amp;gt;\frac{\mathrm{d} u}{\mathrm{d} x}(x) = 0,&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;\frac{\mathrm{d} u}{\mathrm{d} x}(x) = 0,&amp;lt;/math&amp;gt;&lt;br /&gt;
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which has the solution&lt;br /&gt;
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which has the solution&lt;br /&gt;
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它的解为&lt;br /&gt;
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: &amp;lt;math&amp;gt;u(x) = c,&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;u(x) = c,&amp;lt;/math&amp;gt;&lt;br /&gt;
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where {{mvar|c}} is any [[Constant (mathematics)|constant]] value. These two examples illustrate that general solutions of ordinary differential equations (ODEs) involve arbitrary constants, but solutions of PDEs involve arbitrary functions.&lt;br /&gt;
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where  is any constant value. These two examples illustrate that general solutions of ordinary differential equations (ODEs) involve arbitrary constants, but solutions of PDEs involve arbitrary functions.&lt;br /&gt;
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这里，{{mvar|c}} 是一个任意常量。&lt;br /&gt;
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这两个例子说明常微分方程的一般解包含任意常数，但偏微分方程的解包含任意函数。&lt;br /&gt;
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A solution of a PDE is generally not [[Uniqueness quantification|unique]]; additional conditions must generally be specified on the [[Boundary (topology)|boundary]] of the region where the solution is defined. For instance, in the simple example above, the function {{math|''f''(''y'')}} can be determined if {{mvar|u}} is specified on the line {{math|''x'' {{=}} 0}}.&lt;br /&gt;
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A solution of a PDE is generally not unique; additional conditions must generally be specified on the boundary of the region where the solution is defined. For instance, in the simple example above, the function  can be determined if  is specified on the line  0}}.&lt;br /&gt;
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偏微分方程的解一般不是唯一的; 一般必须在定义解的区域边界上定义附加条件。 例如，在上面的简单示例中，如果在 {{math|''x'' {{=}} 0}} 时确定了 {{mvar|u}} 的值，则可以确定该函数 {{math|''f''(''y'')}}。&lt;br /&gt;
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== Existence and uniqueness ==&lt;br /&gt;
存在性和唯一性&lt;br /&gt;
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Although the issue of existence and uniqueness of solutions of ordinary differential equations has a very satisfactory answer with the [[Picard–Lindelöf theorem]], that is far from the case for partial differential equations. The [[Cauchy–Kowalevski theorem]] states that the [[Cauchy problem]] for any partial differential equation whose coefficients are [[Analytic function|analytic]] in the unknown function and its derivatives, has a locally unique analytic solution. Although this result might appear to settle the existence and uniqueness of solutions, there are examples of linear partial differential equations whose coefficients have derivatives of all orders (which are nevertheless not analytic) but which have no solutions at all: see [[Lewy's example|Lewy (1957)]]. Even if the solution of a partial differential equation exists and is unique, it may nevertheless have undesirable properties.  The mathematical study of these questions is usually in the more powerful context of [[weak solution]]s.&lt;br /&gt;
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Although the issue of existence and uniqueness of solutions of ordinary differential equations has a very satisfactory answer with the Picard–Lindelöf theorem, that is far from the case for partial differential equations. The Cauchy–Kowalevski theorem states that the Cauchy problem for any partial differential equation whose coefficients are analytic in the unknown function and its derivatives, has a locally unique analytic solution. Although this result might appear to settle the existence and uniqueness of solutions, there are examples of linear partial differential equations whose coefficients have derivatives of all orders (which are nevertheless not analytic) but which have no solutions at all: see Lewy (1957). Even if the solution of a partial differential equation exists and is unique, it may nevertheless have undesirable properties.  The mathematical study of these questions is usually in the more powerful context of weak solutions.&lt;br /&gt;
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尽管常微分方程解的存在性和唯一性用'''&amp;lt;font color=&amp;quot;#ff8000&amp;quot;&amp;gt;弗罗贝尼乌斯定理 Picard–Lindelöf Theorem&amp;lt;/font&amp;gt;得到了令人满意的结果，但偏微分方程解的存在性和唯一性却远没有得到解决。'''&amp;lt;font color=&amp;quot;#ff8000&amp;quot;&amp;gt;柯西-科瓦列夫斯基定理 Cauchy–Kowalevski theorem&amp;lt;/font&amp;gt;指出：对于任意系数在未知函数及其导数中解析的偏微分方程，柯西问题存在一个局部唯一的解析解。虽然这个结果似乎解决了解的存在性和唯一性问题，但是存在一些线性偏微分方程-其系数具有所有级数的导数(尽管这些导数不是解析的) ，但是根本没有解: 见 Lewy (1957)。即使偏微分方程的解存在且唯一，它仍然可能具有不可预料的性质。这些问题的数学研究通常是在更有力的弱解的背景下进行的。&lt;br /&gt;
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An example of pathological behavior is the sequence (depending upon {{mvar|n}}) of [[Cauchy problem]]s for the [[Laplace equation]]&lt;br /&gt;
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An example of pathological behavior is the sequence (depending upon ) of Cauchy problems for the Laplace equation&lt;br /&gt;
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反常特征的一个例子是拉普拉斯方程的柯西问题的序列(取决于{{mvar|n}})&lt;br /&gt;
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: &amp;lt;math&amp;gt;\frac{\partial^2 u}{\partial x^2} + \frac{\partial^2 u}{\partial y^2}=0,&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;\frac{\partial^2 u}{\partial x^2} + \frac{\partial^2 u}{\partial y^2}=0,&amp;lt;/math&amp;gt;&lt;br /&gt;
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with [[boundary condition]]s&lt;br /&gt;
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with boundary conditions&lt;br /&gt;
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有边界条件&lt;br /&gt;
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: &amp;lt;math&amp;gt;\begin{align} u(x,0) &amp;amp;= 0, \\ \frac{\partial u}{\partial y}(x,0) &amp;amp;= \frac{\sin nx}{n}, \end{align}&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;\begin{align} u(x,0) &amp;amp;= 0, \\ \frac{\partial u}{\partial y}(x,0) &amp;amp;= \frac{\sin nx}{n}, \end{align}&amp;lt;/math&amp;gt;&lt;br /&gt;
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where {{mvar|n}} is an integer. The derivative of {{mvar|u}} with respect to {{mvar|y}} approaches zero [[uniform convergence|uniformly]] in {{mvar|x}} as {{mvar|n}} increases, but the solution is&lt;br /&gt;
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where  is an integer. The derivative of  with respect to  approaches zero uniformly in  as  increases, but the solution is&lt;br /&gt;
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其中{{mvar|n}}是整数。{{mvar|u}}是关于{{mvar|y}}的导数，一致地随着{{mvar|n}}的增加而趋于零，但是解是&lt;br /&gt;
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: &amp;lt;math&amp;gt;u(x,y) = \frac{\sinh ny \sin nx}{n^2}.&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;u(x,y) = \frac{\sinh ny \sin nx}{n^2}.&amp;lt;/math&amp;gt;&lt;br /&gt;
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This solution approaches infinity if {{mvar|nx}} is not an integer multiple of {{pi}} for any non-zero value of {{mvar|y}}. The Cauchy problem for the Laplace equation is called ''ill-posed'' or ''not [[Well-posed problem|well-posed]]'', since the solution does not continuously depend on the data of the problem. Such ill-posed problems are not usually satisfactory for physical applications.&lt;br /&gt;
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This solution approaches infinity if  is not an integer multiple of  for any non-zero value of . The Cauchy problem for the Laplace equation is called ill-posed or not well-posed, since the solution does not continuously depend on the data of the problem. Such ill-posed problems are not usually satisfactory for physical applications.&lt;br /&gt;
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对于任何非零的{{mvar|y}}，如果{{mvar|nx}}不是{{pi}}的整数倍，这个解会接近于无穷大。拉普拉斯方程的柯西问题被称为不适定问题（可以译为ill-posed或not well-posed），因为该问题的解并不连续地依赖于该问题的数据。这种不适定问题在物理应用中通常不能令人满意。&lt;br /&gt;
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The [[Navier–Stokes existence and smoothness|existence of solutions for the Navier–Stokes equations]], a partial differential equation, is part of one of the [[Millennium Prize Problems]].&lt;br /&gt;
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The existence of solutions for the Navier–Stokes equations, a partial differential equation, is part of one of the Millennium Prize Problems.&lt;br /&gt;
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一种偏微分方程——纳维-斯托克斯方程——的解的存在性就是千禧年大奖难题的一部分。&lt;br /&gt;
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== Notation ==&lt;br /&gt;
符号&lt;br /&gt;
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In PDEs, it is common to denote partial derivatives using subscripts. That is:&lt;br /&gt;
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In PDEs, it is common to denote partial derivatives using subscripts. That is:&lt;br /&gt;
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在偏微分方程中，通常用下标表示偏导数。例如:&lt;br /&gt;
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: &amp;lt;math&amp;gt;u_x = \frac{\partial u}{\partial x}&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;u_x = \frac{\partial u}{\partial x}&amp;lt;/math&amp;gt;&lt;br /&gt;
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: &amp;lt;math&amp;gt;u_{xx} = \frac{\partial^2 u}{\partial x^2} &amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;u_{xx} = \frac{\partial^2 u}{\partial x^2} &amp;lt;/math&amp;gt;&lt;br /&gt;
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: &amp;lt;math&amp;gt;u_{xy} = \frac{\partial^2 u}{\partial y\, \partial x} = \frac{\partial}{\partial y } \left(\frac{\partial u}{\partial x}\right). &amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;u_{xy} = \frac{\partial^2 u}{\partial y\, \partial x} = \frac{\partial}{\partial y } \left(\frac{\partial u}{\partial x}\right). &amp;lt;/math&amp;gt;&lt;br /&gt;
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Especially in physics, [[del]] or nabla ({{math|∇}}) is often used to denote spatial derivatives, and {{math|''&amp;amp;#x307;u'', ''ü''}} for time derivatives. For example, the [[wave equation]] (mentioned below) can be written as&lt;br /&gt;
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Especially in physics, del or nabla () is often used to denote spatial derivatives, and  for time derivatives. For example, the wave equation (mentioned below) can be written as&lt;br /&gt;
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特别是在物理学中，[[del]]或nabla ({{math|∇}})经常用来表示空间导数和时间导数。例如，波动方程(在下文中提到)可以写成&lt;br /&gt;
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:&amp;lt;math&amp;gt;\ddot u=c^2\nabla^2u&amp;lt;/math&amp;gt;&lt;br /&gt;
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&amp;lt;math&amp;gt;\ddot u=c^2\nabla^2u&amp;lt;/math&amp;gt;&lt;br /&gt;
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or&lt;br /&gt;
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or&lt;br /&gt;
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或&lt;br /&gt;
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:&amp;lt;math&amp;gt;\ddot u=c^2\Delta u&amp;lt;/math&amp;gt;&lt;br /&gt;
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&amp;lt;math&amp;gt;\ddot u=c^2\Delta u&amp;lt;/math&amp;gt;&lt;br /&gt;
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where {{math|Δ}} is the [[Laplace operator]].&lt;br /&gt;
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where  is the Laplace operator.&lt;br /&gt;
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其中{{math|Δ}}代表拉普拉斯算子&lt;br /&gt;
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== Classification ==&lt;br /&gt;
分类&lt;br /&gt;
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Some linear, second-order partial differential equations can be classified as [[parabolic partial differential equation|parabolic]], [[hyperbolic partial differential equation|hyperbolic]] and [[elliptic partial differential equation|elliptic]]. Others, such as the [[Euler–Tricomi equation]], have different types in different regions. The classification provides a guide to appropriate initial and boundary conditions and to the smoothness of the solutions.&lt;br /&gt;
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Some linear, second-order partial differential equations can be classified as parabolic, hyperbolic and elliptic. Others, such as the Euler–Tricomi equation, have different types in different regions. The classification provides a guide to appropriate initial and boundary conditions and to the smoothness of the solutions.&lt;br /&gt;
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一些线性二阶偏微分方程可分为抛物型方程、双曲型方程和椭圆型方程。其他的方程，如欧拉-特里科米方程，在不同的区域有不同的类型。这种分类有助于选择适当的初始和边界条件以及提高解的平滑性。&lt;br /&gt;
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=== Equations of first order ===&lt;br /&gt;
一阶方程&lt;br /&gt;
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{{main|First-order partial differential equation}}&lt;br /&gt;
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=== Linear equations of second order ===&lt;br /&gt;
二阶线性方程&lt;br /&gt;
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Assuming {{math|''u&amp;lt;sub&amp;gt;xy&amp;lt;/sub&amp;gt;'' {{=}} ''u&amp;lt;sub&amp;gt;yx&amp;lt;/sub&amp;gt;''}}, the general linear second-order PDE in two independent variables has the form&lt;br /&gt;
&lt;br /&gt;
Assuming  u&amp;lt;sub&amp;gt;yx&amp;lt;/sub&amp;gt;}}, the general linear second-order PDE in two independent variables has the form&lt;br /&gt;
&lt;br /&gt;
假设 {{math|''u&amp;lt;sub&amp;gt;xy&amp;lt;/sub&amp;gt;'' {{=}} ''u&amp;lt;sub&amp;gt;yx&amp;lt;/sub&amp;gt;''}}，含有两个独立变量的一般的线性二阶偏微分方程具有如下这样的形式&lt;br /&gt;
&lt;br /&gt;
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: &amp;lt;math&amp;gt;Au_{xx} + 2Bu_{xy} + Cu_{yy} + \cdots \mbox{(lower order terms)} = 0,&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;Au_{xx} + 2Bu_{xy} + Cu_{yy} + \cdots \mbox{(lower order terms)} = 0,&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
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where the coefficients {{mvar|A}}, {{mvar|B}}, {{mvar|C}}... may depend upon {{mvar|x}} and {{mvar|y}}. If {{math|''A''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; + ''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; + ''C''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; &amp;gt; 0}} over a region of the {{mvar|xy}}-plane, the PDE is second-order in that region. This form is analogous to the equation for a conic section:&lt;br /&gt;
&lt;br /&gt;
where the coefficients , , ... may depend upon  and . If  over a region of the -plane, the PDE is second-order in that region. This form is analogous to the equation for a conic section:&lt;br /&gt;
&lt;br /&gt;
其中的系数 {{mvar|A}}, {{mvar|B}}, {{mvar|C}}... 一般取决于{{mvar|x}}和{{mvar|y}}。如果在{{mvar|xy}}-平面的一个区域上 {{math|''A''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; + ''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; + ''C''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; &amp;gt; 0}}，偏微分方程在该区域是二阶的。这种形式类似于圆锥曲线的方程:&lt;br /&gt;
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: &amp;lt;math&amp;gt;Ax^2 + 2Bxy + Cy^2 + \cdots = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;Ax^2 + 2Bxy + Cy^2 + \cdots = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
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More precisely, replacing {{math|∂&amp;lt;sub&amp;gt;''x''&amp;lt;/sub&amp;gt;}} by {{mvar|X}}, and likewise for other variables (formally this is done by a [[Fourier transform]]), converts a constant-coefficient PDE into a polynomial of the same degree, with the terms of the highest degree (a [[homogeneous polynomial]], here a [[quadratic form]]) being most significant for the classification.&lt;br /&gt;
&lt;br /&gt;
More precisely, replacing  by , and likewise for other variables (formally this is done by a Fourier transform), converts a constant-coefficient PDE into a polynomial of the same degree, with the terms of the highest degree (a homogeneous polynomial, here a quadratic form) being most significant for the classification.&lt;br /&gt;
&lt;br /&gt;
更准确地说，用 {{mvar|X}} 替换 {{math|∂&amp;lt;sub&amp;gt;''x''&amp;lt;/sub&amp;gt;}}，对于其他变量做同样的操作(从形式上来说，这是由傅里叶变换来完成的)，将一个常系数偏微分方程转换成一个相同次数的多项式，最高次数的项(齐次多项式，这里是一个二次形式)一般会用于偏微分方程的分类。&lt;br /&gt;
===~~ most significant for the classification 意译为用于偏微分方程的分类。       significiant直译过来感觉不太合适&lt;br /&gt;
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Just as one classifies [[conic section]]s and quadratic forms into parabolic, hyperbolic, and elliptic based on the [[discriminant]] {{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − 4''AC''}}, the same can be done for a second-order PDE at a given point.  However, the [[discriminant]] in a PDE is given by {{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC''}} due to the convention of the {{mvar|xy}} term being {{math|2''B''}} rather than {{mvar|B}}; formally, the discriminant (of the associated quadratic form) is {{math|(2''B'')&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − 4''AC'' {{=}} 4(''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC'')}}, with the factor of 4 dropped for simplicity.&lt;br /&gt;
&lt;br /&gt;
Just as one classifies conic sections and quadratic forms into parabolic, hyperbolic, and elliptic based on the discriminant , the same can be done for a second-order PDE at a given point.  However, the discriminant in a PDE is given by  due to the convention of the  term being  rather than ; formally, the discriminant (of the associated quadratic form) is  4(B&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − AC)}}, with the factor of 4 dropped for simplicity.&lt;br /&gt;
&lt;br /&gt;
正如人们可以根据判别式 {{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − 4''AC''}} 将圆锥曲线和二次型分为抛物型、双曲型和椭圆型一样，对于给定点的二阶偏微分方程也可以这样做。然而，偏微分方程中的判别式 {{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − 4''AC''}} 是根据交叉项的系数{{math|2''B''}} 而不是 {{mvar|B}} 给出的，形式上，判别式(关联二次型)是 {{math|(2''B'')&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − 4''AC'' {{=}} 4(''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC'')}}，为简单起见，去掉了因子4。&lt;br /&gt;
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# {{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC'' &amp;lt; 0}} (''[[elliptic partial differential equation]]''): Solutions of [[elliptic partial differential equation|elliptic PDEs]] are as smooth as the coefficients allow, within the interior of the region where the equation and solutions are defined. For example, solutions of [[Laplace's equation]] are analytic within the domain where they are defined, but solutions may assume boundary values that are not smooth. The motion of a fluid at subsonic speeds can be approximated with elliptic PDEs, and the Euler–Tricomi equation is elliptic where {{math|''x'' &amp;lt; 0}}.&lt;br /&gt;
&lt;br /&gt;
  (elliptic partial differential equation): Solutions of elliptic PDEs are as smooth as the coefficients allow, within the interior of the region where the equation and solutions are defined. For example, solutions of Laplace's equation are analytic within the domain where they are defined, but solutions may assume boundary values that are not smooth. The motion of a fluid at subsonic speeds can be approximated with elliptic PDEs, and the Euler–Tricomi equation is elliptic where .&lt;br /&gt;
&lt;br /&gt;
{{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC'' &amp;lt; 0}} (椭圆形微分方程)：在定义方程和解的区域内部，椭圆型偏微分方程的解光滑到系数允许的程度。例如，拉普拉斯方程的解在它们被定义的区域内是解析的，但是解可能假设边界值是不光滑的。亚音速流体的运动可以用椭圆偏微分方程近似，其中欧拉-特里科米方程在 {{math|''x'' &amp;lt; 0}} 时是椭圆型偏微分方程。&lt;br /&gt;
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# {{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC'' {{=}} 0}} (''[[parabolic partial differential equation]]''): Equations that are [[parabolic partial differential equation|parabolic]] at every point can be transformed into a form analogous to the [[heat equation]] by a change of independent variables. Solutions smooth out as the transformed time variable increases. The Euler–Tricomi equation has parabolic type on the line where {{math|''x'' {{=}} 0}}.&lt;br /&gt;
&lt;br /&gt;
  0}} (parabolic partial differential equation): Equations that are parabolic at every point can be transformed into a form analogous to the heat equation by a change of independent variables. Solutions smooth out as the transformed time variable increases. The Euler–Tricomi equation has parabolic type on the line where  0}}.&lt;br /&gt;
&lt;br /&gt;
{{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC'' {{=}} 0}}（抛物线形偏微分方程）：在每一点上都是抛物线型的方程可以通过改变自变量从而转化成类似于热方程的形式。随着转换后的时间变量的增加，方程的解变得平滑。欧拉-特里科米方程在 {{math|''x'' {{=}} 0}} 这条特征线上是抛物线形的。&lt;br /&gt;
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# {{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC'' &amp;gt; 0}} (''[[hyperbolic partial differential equation]]''): [[hyperbolic partial differential equation|hyperbolic]] equations retain any discontinuities of functions or derivatives in the initial data. An example is the [[wave equation]]. The motion of a fluid at supersonic speeds can be approximated with hyperbolic PDEs, and the Euler–Tricomi equation is hyperbolic where {{math|''x'' &amp;gt; 0}}.&lt;br /&gt;
&lt;br /&gt;
  (hyperbolic partial differential equation): hyperbolic equations retain any discontinuities of functions or derivatives in the initial data. An example is the wave equation. The motion of a fluid at supersonic speeds can be approximated with hyperbolic PDEs, and the Euler–Tricomi equation is hyperbolic where .&lt;br /&gt;
&lt;br /&gt;
{{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC'' &amp;gt; 0}} (双曲形偏微分方程)：双曲形方程在初始数据中保留了函数或导数的任何不连续性，波动方程就是其中的一个例子。超音速流体的运动可以用双曲形偏微分方程近似，其中欧拉-特里科米方程在 {{math|''x'' &amp;gt; 0}} 时是双曲型的。&lt;br /&gt;
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If there are {{mvar|n}} independent variables {{math|''x''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;, ''x''&amp;lt;sub&amp;gt;2 &amp;lt;/sub&amp;gt;,… ''x''&amp;lt;sub&amp;gt;''n''&amp;lt;/sub&amp;gt;}}, a general linear partial differential equation of second order has the form&lt;br /&gt;
&lt;br /&gt;
If there are  independent variables , a general linear partial differential equation of second order has the form&lt;br /&gt;
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如果存在 {{mvar|n}} 个自变量 {{math|''x''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;, ''x''&amp;lt;sub&amp;gt;2 &amp;lt;/sub&amp;gt;,… ''x''&amp;lt;sub&amp;gt;''n''&amp;lt;/sub&amp;gt;}}，一般二阶线性偏微分方程的形式是&lt;br /&gt;
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: &amp;lt;math&amp;gt;L u =\sum_{i=1}^n\sum_{j=1}^n a_{i,j} \frac{\partial^2 u}{\partial x_i \partial x_j} \quad \text{ plus lower-order terms} =0.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;L u =\sum_{i=1}^n\sum_{j=1}^n a_{i,j} \frac{\partial^2 u}{\partial x_i \partial x_j} \quad \text{ plus lower-order terms} =0.&amp;lt;/math&amp;gt;&lt;br /&gt;
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The classification depends upon the signature of the eigenvalues of the coefficient matrix {{math|''a''&amp;lt;sub&amp;gt;''i'',''j''&amp;lt;/sub&amp;gt;}}.&lt;br /&gt;
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The classification depends upon the signature of the eigenvalues of the coefficient matrix .&lt;br /&gt;
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这种分类取决于系数矩阵本征值的符号（正负性）。&lt;br /&gt;
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# Elliptic: the eigenvalues are all positive or all negative.&lt;br /&gt;
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 Elliptic: the eigenvalues are all positive or all negative.&lt;br /&gt;
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椭圆形方程: 本征值全部为正或全部为负。&lt;br /&gt;
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# Parabolic: the eigenvalues are all positive or all negative, save one that is zero.&lt;br /&gt;
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 Parabolic: the eigenvalues are all positive or all negative, save one that is zero.&lt;br /&gt;
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抛物线形方程: 本征值全部为正或全部为负，除了一个为零。&lt;br /&gt;
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# Hyperbolic: there is only one negative eigenvalue and all the rest are positive, or there is only one positive eigenvalue and all the rest are negative.&lt;br /&gt;
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 Hyperbolic: there is only one negative eigenvalue and all the rest are positive, or there is only one positive eigenvalue and all the rest are negative.&lt;br /&gt;
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双曲形方程: 只有一个负特征值，其余的都是正特征值，或者只有一个正特征值，其余的都是负特征值。&lt;br /&gt;
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# Ultrahyperbolic: there is more than one positive eigenvalue and more than one negative eigenvalue, and there are no zero eigenvalues. There is only a limited theory for ultrahyperbolic equations (Courant and Hilbert, 1962).&lt;br /&gt;
&lt;br /&gt;
 Ultrahyperbolic: there is more than one positive eigenvalue and more than one negative eigenvalue, and there are no zero eigenvalues. There is only a limited theory for ultrahyperbolic equations (Courant and Hilbert, 1962).&lt;br /&gt;
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超双形方程: 存在多于一个正本征值和多于一个的负本征值，且不存在零本征值。对于超双曲方程，只存在一个有限理论(Courant 和 Hilbert，1962)。&lt;br /&gt;
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==[[用户:Yuling|Yuling]]（[[用户讨论:Yuling|讨论]]） 我对于limited theory这个单词对应的相关理论不太了解。&lt;br /&gt;
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=== Systems of first-order equations and characteristic surfaces ===&lt;br /&gt;
一阶方程组和特征曲面&lt;br /&gt;
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The classification of partial differential equations can be extended to systems of first-order equations, where the unknown {{mvar|u}} is now a [[Euclidean vector|vector]] with {{mvar|m}} components, and the coefficient matrices {{mvar|A&amp;lt;sub&amp;gt;ν&amp;lt;/sub&amp;gt;}} are {{mvar|m}} by {{mvar|m}} matrices for {{math|''ν'' {{=}} 1, 2,… ''n''}}. The partial differential equation takes the form&lt;br /&gt;
&lt;br /&gt;
The classification of partial differential equations can be extended to systems of first-order equations, where the unknown  is now a vector with  components, and the coefficient matrices  are  by  matrices for  1, 2,… n}}. The partial differential equation takes the form&lt;br /&gt;
&lt;br /&gt;
偏微分方程组的分类可以推广到一阶方程组，其中未知量 {{mvar|u}} 是有 {{mvar|m}} 个分量的向量。对于 {{math|''ν'' {{=}} 1, 2,… ''n''}}，系数矩阵 {{mvar|A&amp;lt;sub&amp;gt;ν&amp;lt;/sub&amp;gt;}} 是 {{mvar|m}} × {{mvar|m}} 的矩阵。偏微分方程形式如下：&lt;br /&gt;
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: &amp;lt;math&amp;gt;Lu = \sum_{\nu=1}^{n} A_\nu \frac{\partial u}{\partial x_\nu} + B=0,&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;Lu = \sum_{\nu=1}^{n} A_\nu \frac{\partial u}{\partial x_\nu} + B=0,&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
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where the coefficient matrices {{mvar|A&amp;lt;sub&amp;gt;ν&amp;lt;/sub&amp;gt;}} and the vector {{mvar|B}} may depend upon {{mvar|x}} and {{mvar|u}}. If a [[hypersurface]] {{mvar|S}} is given in the implicit form&lt;br /&gt;
&lt;br /&gt;
where the coefficient matrices  and the vector  may depend upon  and . If a hypersurface  is given in the implicit form&lt;br /&gt;
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其中系数矩阵 {{mvar|A&amp;lt;sub&amp;gt;ν&amp;lt;/sub&amp;gt;}} 和向量 {{mvar|B}} 可能依赖于 {{mvar|x}} 和 {{mvar|u}}。如果超曲面是以隐式形式给出的&lt;br /&gt;
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: &amp;lt;math&amp;gt;\varphi(x_1, x_2, \ldots x_n)=0,&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;\varphi(x_1, x_2, \ldots x_n)=0,&amp;lt;/math&amp;gt;&lt;br /&gt;
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where {{mvar|φ}} has a non-zero gradient, then {{mvar|S}} is a '''characteristic surface''' for the operator {{mvar|L}} at a given point if the characteristic form vanishes:&lt;br /&gt;
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where  has a non-zero gradient, then  is a characteristic surface for the operator  at a given point if the characteristic form vanishes:&lt;br /&gt;
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其中存在一个非零的梯度，那么如果特征形式消失，则在给定点上算子的特征曲面形式如下:&lt;br /&gt;
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: &amp;lt;math&amp;gt;Q\left(\frac{\partial\varphi}{\partial x_1}, \ldots\frac{\partial\varphi}{\partial x_n}\right) =\det\left[\sum_{\nu=1}^nA_\nu \frac{\partial \varphi}{\partial x_\nu}\right]=0.\,&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;Q\left(\frac{\partial\varphi}{\partial x_1}, \ldots\frac{\partial\varphi}{\partial x_n}\right) =\det\left[\sum_{\nu=1}^nA_\nu \frac{\partial \varphi}{\partial x_\nu}\right]=0.\,&amp;lt;/math&amp;gt;&lt;br /&gt;
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The geometric interpretation of this condition is as follows: if data for {{mvar|u}} are prescribed on the surface {{mvar|S}}, then it may be possible to determine the normal derivative of {{mvar|u}} on {{mvar|S}} from the differential equation. If the data on {{mvar|S}} and the differential equation determine the normal derivative of {{mvar|u}} on {{mvar|S}}, then {{mvar|S}} is non-characteristic. If the data on {{mvar|S}} and the differential equation ''do not'' determine the normal derivative of {{mvar|u}} on {{mvar|S}}, then the surface is '''characteristic''', and the differential equation restricts the data on {{mvar|S}}: the differential equation is ''internal'' to {{mvar|S}}.&lt;br /&gt;
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The geometric interpretation of this condition is as follows: if data for  are prescribed on the surface , then it may be possible to determine the normal derivative of  on  from the differential equation. If the data on  and the differential equation determine the normal derivative of  on , then  is non-characteristic. If the data on  and the differential equation do not determine the normal derivative of  on , then the surface is characteristic, and the differential equation restricts the data on : the differential equation is internal to .&lt;br /&gt;
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这个条件的几何解释如下: 如果关于 {{mvar|u}} 的数据是在曲面 {{mvar|S}} 上规定的，那么就有可能依据微分方程确定曲面 {{mvar|S}} 上 {{mvar|u}} 的法向导数。如果曲面 {{mvar|S}} 上的数据和上面的微分方程能确定曲面 {{mvar|S}} 上 {{mvar|u}} 的法向导数，那么它就是非特征的。如果曲面 {{mvar|S}} 上的数据和上面的微分方程不能确定曲面 {{mvar|S}} 上 {{mvar|u}} 的法向导数，那么曲面是特征的，并且微分方程将数据限制在曲面 {{mvar|S}} 上：微分方程是在曲面 {{mvar|S}} 内部。&lt;br /&gt;
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# A first-order system {{math|''Lu'' {{=}} 0}} is ''elliptic'' if no surface is characteristic for {{mvar|L}}: the values of {{mvar|u}} on {{mvar|S}} and the differential equation always determine the normal derivative of {{mvar|u}} on {{mvar|S}}.&lt;br /&gt;
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 A first-order system  0}} is elliptic if no surface is characteristic for : the values of  on  and the differential equation always determine the normal derivative of  on .&lt;br /&gt;
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如果对于 {{mvar|L}} 没有曲面是特征的，则一阶系统 {{math|''Lu'' {{=}} 0}} 是椭圆形的：{{mvar|u}}在 {{mvar|S}} 的值和微分方程总能够决定 {{mvar|S}} 上 {{mvar|u}} 的法向导数。&lt;br /&gt;
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# A first-order system is ''hyperbolic'' at a point if there is a '''spacelike''' surface {{mvar|S}} with normal {{mvar|ξ}} at that point. This means that, given any non-trivial vector {{mvar|η}} orthogonal to {{mvar|ξ}}, and a scalar multiplier {{mvar|λ}}, the equation {{math|''Q''(''λξ'' + ''η'') {{=}} 0}} has {{mvar|m}} real roots {{math|''λ''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;, ''λ''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;,… ''λ''&amp;lt;sub&amp;gt;''m''&amp;lt;/sub&amp;gt;}}. The system is '''strictly hyperbolic''' if these roots are always distinct. The geometrical interpretation of this condition is as follows: the characteristic form {{math|''Q''(''ζ'') {{=}} 0}} defines a cone (the normal cone) with homogeneous coordinates ζ. In the hyperbolic case, this cone has {{mvar|m}} sheets, and the axis {{math|''ζ'' {{=}} ''λξ''}} runs inside these sheets: it does not intersect any of them. But when displaced from the origin by η, this axis intersects every sheet. In the elliptic case, the normal cone has no real sheets.&lt;br /&gt;
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 A first-order system is hyperbolic at a point if there is a spacelike surface  with normal  at that point. This means that, given any non-trivial vector  orthogonal to , and a scalar multiplier , the equation  0}} has  real roots . The system is strictly hyperbolic if these roots are always distinct. The geometrical interpretation of this condition is as follows: the characteristic form  0}} defines a cone (the normal cone) with homogeneous coordinates ζ. In the hyperbolic case, this cone has  sheets, and the axis  λξ}} runs inside these sheets: it does not intersect any of them. But when displaced from the origin by η, this axis intersects every sheet. In the elliptic case, the normal cone has no real sheets.&lt;br /&gt;
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如果在该点存在一个法向量为 {{mvar|ξ}}的 '''&amp;lt;font color=&amp;quot;#ff8000&amp;quot;&amp;gt;类空曲面 Spacclike Surface&amp;lt;/font&amp;gt; {{mvar|S}} ，则一阶系统在那一点是双曲的。这意味着，给定任意正交于 {{mvar|ξ}} 的非平凡向量 {{mvar|η}} 和一个标量乘子 {{mvar|λ}}，方程 {{math|''Q''(''λξ'' + ''η'') {{=}} 0}} 有 {{mvar|m}} 个实根 {{math|''λ''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;, ''λ''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;,… ''λ''&amp;lt;sub&amp;gt;''m''&amp;lt;/sub&amp;gt;}}。如果这些根始终不同，则该系统是严格双曲形的。这个条件的几何解释如下: 特征形式 {{math|''Q''(''ζ'') {{=}} 0}} 定义了一个具有齐次坐标 ζ的圆锥(法线圆锥)。在双曲形的情况下，这个圆锥体有 {{mvar|m}} 层，并且轴 {{math|''ζ'' {{=}} ''λξ''}} 在这些层中运动: 它不与任何一层相交。但是当从原点偏离η时，这条轴线与每一层都相交。在椭圆形的情况下，法向圆锥没有实层。&lt;br /&gt;
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==[[用户:Yuling|Yuling]]（[[用户讨论:Yuling|讨论]]） sheet 这个单词也不很理解，我直译为了“层”&lt;br /&gt;
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=== Equations of mixed type ===&lt;br /&gt;
混合型方程&lt;br /&gt;
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If a PDE has coefficients that are not constant, it is possible that it will not belong to any of these categories but rather be of '''mixed type'''. A simple but important example is the [[Euler–Tricomi equation]]&lt;br /&gt;
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If a PDE has coefficients that are not constant, it is possible that it will not belong to any of these categories but rather be of mixed type. A simple but important example is the Euler–Tricomi equation&lt;br /&gt;
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如果偏微分方程的系数不是常数，那么它可能不属于这些类别中的任何一个，而是属于混合类型。一个简单但重要的例子是欧拉-特里科米方程&lt;br /&gt;
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: &amp;lt;math&amp;gt;u_{xx} = xu_{yy},&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;u_{xx} = xu_{yy},&amp;lt;/math&amp;gt;&lt;br /&gt;
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which is called '''elliptic-hyperbolic''' because it is elliptic in the region {{math|''x'' &amp;lt; 0}}, hyperbolic in the region {{math|''x'' &amp;gt; 0}}, and degenerate parabolic on the line {{math|''x'' {{=}} 0}}.&lt;br /&gt;
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which is called elliptic-hyperbolic because it is elliptic in the region , hyperbolic in the region , and degenerate parabolic on the line  0}}.&lt;br /&gt;
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它在 {{math|''x'' &amp;lt; 0}} 的区域上是椭圆形，在 {{math|''x'' &amp;gt; 0}} 区域上是双曲形，在 {{math|''x'' {{=}} 0}}这条线上是退化为抛物线形，因此称之为椭圆-双曲型。&lt;br /&gt;
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''fill in: Dirichlet and Neumann boundaries, hyperbolic/parabolic/elliptic separation of variables, [[Fourier analysis]], [[Green's function]]s ...--&amp;gt;&lt;br /&gt;
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fill in: Dirichlet and Neumann boundaries, hyperbolic/parabolic/elliptic separation of variables, Fourier analysis, Green's functions ...--&amp;gt;&lt;br /&gt;
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填写: Dirichlet 和 Neumann 边界，双曲 / 抛物线 / 椭圆分离变量法，傅立叶分析，Green 函数... --&lt;br /&gt;
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=== Infinite-order PDEs in quantum mechanics ===&lt;br /&gt;
量子力学中的无限阶偏微分方程&lt;br /&gt;
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In the [[phase space formulation]] of quantum mechanics,  one may consider the [[Method of quantum characteristics|quantum Hamilton's equations]] for trajectories of quantum particles. These equations are infinite-order PDEs. However, in the semiclassical expansion, one has a finite system of ODEs at any fixed order of [[Dirac constant|{{mvar|ħ}}]].  The evolution equation of the [[Wigner quasi-probability distribution|c]] is also an infinite-order PDE. The quantum trajectories are [[Method of quantum characteristics|quantum characteristics]], with the use of which one could calculate the evolution of the Wigner function.&lt;br /&gt;
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In the phase space formulation of quantum mechanics,  one may consider the quantum Hamilton's equations for trajectories of quantum particles. These equations are infinite-order PDEs. However, in the semiclassical expansion, one has a finite system of ODEs at any fixed order of Dirac constant|.  The evolution equation of the Wigner function is also an infinite-order PDE. The quantum trajectories are quantum characteristics, with the use of which one could calculate the evolution of the Wigner function.&lt;br /&gt;
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在量子力学中的相空间表述中，我们可以考虑用于求解量子粒子的轨迹的量子哈密顿的方程。这些方程是无限阶偏微分方程。然而，在半经典展开中，我们在给定[[Dirac constant|{{mvar|ħ}}]]阶数下有一个有限的的常微分方程组。'''&amp;lt;font color=&amp;quot;#ff8000&amp;quot;&amp;gt;维格纳函数  Wigner Function&amp;lt;/font&amp;gt;的演化方程也是一个无限阶偏微分方程。由于量子轨道的量子特性，所以它通常可以用来计算维格纳函数的演化。&lt;br /&gt;
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== Analytical solutions ==&lt;br /&gt;
解析解&lt;br /&gt;
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===Separation of variables===&lt;br /&gt;
分离变量法&lt;br /&gt;
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{{main|Separable partial differential equation}}&lt;br /&gt;
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Linear PDEs can be reduced to systems of ordinary differential equations by the important technique of separation of variables. This technique rests on a characteristic of solutions to differential equations: if one can find any solution that solves the equation and satisfies the boundary conditions, then it is ''the'' solution (this also applies to ODEs). We assume as an [[ansatz]] that the dependence of a solution on the parameters space and time can be written as a product of terms that each depend on a single parameter, and then see if this can be made to solve the problem.&amp;lt;ref&amp;gt;{{cite book|last1=Gershenfeld|first1=Neil|title=The nature of mathematical modeling|date=2000|publisher=Cambridge Univ. Press|location=Cambridge|isbn=0521570956|page=27|edition=Reprinted (with corr.)}}&amp;lt;/ref&amp;gt;&lt;br /&gt;
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Linear PDEs can be reduced to systems of ordinary differential equations by the important technique of separation of variables. This technique rests on a characteristic of solutions to differential equations: if one can find any solution that solves the equation and satisfies the boundary conditions, then it is the solution (this also applies to ODEs). We assume as an ansatz that the dependence of a solution on the parameters space and time can be written as a product of terms that each depend on a single parameter, and then see if this can be made to solve the problem.&lt;br /&gt;
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线性偏微分方程组可以通过分离变量法这一重要方法来简化为常微分方程组。这种方法依赖于微分方程解的一个特征: 如果能找到任何一个满足方程和边界条件的解，那么这个解就是方程的解(这也适用于常微分方程)。我们假设解对参数空间和时间的依赖可以写成对它们每一项的依赖以及一个参数的乘积，然后再看看这是否可以用来解决这个问题。&lt;br /&gt;
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In the method of separation of variables, one reduces a PDE to a PDE in fewer variables, which is an ordinary differential equation if in one variable – these are in turn easier to solve.&lt;br /&gt;
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In the method of separation of variables, one reduces a PDE to a PDE in fewer variables, which is an ordinary differential equation if in one variable – these are in turn easier to solve.&lt;br /&gt;
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在分离变量法方法中，可以将偏微分方程简化为含有更少变量的偏微分方程，如果只有一个变量，那么就变成了一个'''&amp;lt;font color = &amp;quot;#ff8000&amp;quot;&amp;gt;常微分方程 Ordinary Differential Equation&amp;lt;/font&amp;gt;'''-- 反过来，这些方程也更容易求解。&lt;br /&gt;
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This is possible for simple PDEs, which are called [[separable partial differential equation]]s, and the domain is generally a rectangle (a product of intervals). Separable PDEs correspond to [[diagonal matrices]] – thinking of &amp;quot;the value for fixed {{mvar|x}}&amp;quot; as a coordinate, each coordinate can be understood separately.&lt;br /&gt;
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This is possible for simple PDEs, which are called separable partial differential equations, and the domain is generally a rectangle (a product of intervals). Separable PDEs correspond to diagonal matrices – thinking of &amp;quot;the value for fixed &amp;quot; as a coordinate, each coordinate can be understood separately.&lt;br /&gt;
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对于简单的偏微分方程(称为可分离偏微分方程)来说，这是可能的，而且方程通常定义在一个矩形区域(区间的乘积)上。可分离偏微分方程对应于对角线矩阵——以“固定值”为坐标，每个坐标可分开理解。&lt;br /&gt;
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This generalizes to the [[method of characteristics]], and is also used in [[integral transform]]s.&lt;br /&gt;
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This generalizes to the method of characteristics, and is also used in integral transforms.&lt;br /&gt;
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这种方法可以推广到特征曲线法，也可以用于积分变换。&lt;br /&gt;
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===Method of characteristics===&lt;br /&gt;
特征曲线法&lt;br /&gt;
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{{main|Method of characteristics}}&lt;br /&gt;
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In special cases, one can find characteristic curves on which the equation reduces to an ODE – changing coordinates in the domain to straighten these curves allows separation of variables, and is called the [[method of characteristics]].&lt;br /&gt;
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In special cases, one can find characteristic curves on which the equation reduces to an ODE – changing coordinates in the domain to straighten these curves allows separation of variables, and is called the method of characteristics.&lt;br /&gt;
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在特殊情况下，可以找到一些特征曲线，在这些曲线上方程可以变成一个常微分方程——意味着改变坐标从而使这些曲线变直从而达到分离变量的目的，这就是所谓的特征曲线法。&lt;br /&gt;
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More generally, one may find characteristic surfaces.&lt;br /&gt;
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More generally, one may find characteristic surfaces.&lt;br /&gt;
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更一般地说，人们可能会找到特征表面。&lt;br /&gt;
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===Integral transform===&lt;br /&gt;
积分变换&lt;br /&gt;
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An [[integral transform]] may transform the PDE to a simpler one, in particular, a separable PDE. This corresponds to diagonalizing an operator.&lt;br /&gt;
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An integral transform may transform the PDE to a simpler one, in particular, a separable PDE. This corresponds to diagonalizing an operator.&lt;br /&gt;
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积分变换可以将偏微分方程转换为更简单的偏微分方程，特别是可分离的偏微分方程。这对应于对角化算符。&lt;br /&gt;
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An important example of this is [[Fourier analysis]], which diagonalizes the heat equation using the [[eigenbasis]] of sinusoidal waves.&lt;br /&gt;
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An important example of this is Fourier analysis, which diagonalizes the heat equation using the eigenbasis of sinusoidal waves.&lt;br /&gt;
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这方面的一个重要例子是'''&amp;lt;font color = &amp;quot;#ff8000&amp;quot;&amp;gt;傅里叶分析  Fourier Analysis&amp;lt;/font&amp;gt;'''，它使用正弦波的特征基来对角化热方程。&lt;br /&gt;
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If the domain is finite or periodic, an infinite sum of solutions such as a [[Fourier series]] is appropriate, but an integral of solutions such as a [[Fourier integral]] is generally required for infinite domains. The solution for a point source for the heat equation given above is an example of the use of a Fourier integral.&lt;br /&gt;
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If the domain is finite or periodic, an infinite sum of solutions such as a Fourier series is appropriate, but an integral of solutions such as a Fourier integral is generally required for infinite domains. The solution for a point source for the heat equation given above is an example of the use of a Fourier integral.&lt;br /&gt;
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如果区域是有限的或周期性的，那么解为无限和的形式是恰当的，例如傅里叶级数，但是一个解的积分，例如傅立叶积分，一般是在无限区域上的。上面给出的热传导方程的点源解法就是使用傅里叶积分的一个例子。&lt;br /&gt;
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===Change of variables===&lt;br /&gt;
变量代换&lt;br /&gt;
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Often a PDE can be reduced to a simpler form with a known solution by a suitable [[Change of variables (PDE)|change of variables]].  For example, the [[Black–Scholes equation#Derivation|Black–Scholes]] PDE&lt;br /&gt;
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Often a PDE can be reduced to a simpler form with a known solution by a suitable change of variables.  For example, the Black–Scholes PDE&lt;br /&gt;
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偏微分方程通常可以通过变量的适当变化，用已知的解简化为更简单的形式。例如，布莱克-舒尔斯偏微分方程&lt;br /&gt;
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:&amp;lt;math&amp;gt; \frac{\partial V}{\partial t} + \tfrac{1}{2}\sigma^2 S^2\frac{\partial^2 V}{\partial S^2} + rS\frac{\partial V}{\partial S} - rV = 0 &amp;lt;/math&amp;gt;&lt;br /&gt;
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&amp;lt;math&amp;gt; \frac{\partial V}{\partial t} + \tfrac{1}{2}\sigma^2 S^2\frac{\partial^2 V}{\partial S^2} + rS\frac{\partial V}{\partial S} - rV = 0 &amp;lt;/math&amp;gt;&lt;br /&gt;
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is reducible to the [[heat equation]]&lt;br /&gt;
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is reducible to the heat equation&lt;br /&gt;
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可以简化为热传导方程&lt;br /&gt;
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:&amp;lt;math&amp;gt; \frac{\partial u}{\partial \tau} = \frac{\partial^2 u}{\partial x^2}&amp;lt;/math&amp;gt;&lt;br /&gt;
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&amp;lt;math&amp;gt; \frac{\partial u}{\partial \tau} = \frac{\partial^2 u}{\partial x^2}&amp;lt;/math&amp;gt;&lt;br /&gt;
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by the change of variables (for complete details see {{webarchive |url=https://web.archive.org/web/20080411030405/http://www.math.unl.edu/~sdunbar1/Teaching/MathematicalFinance/Lessons/BlackScholes/Solution/solution.shtml |date=April 11, 2008 |title=Solution of the Black Scholes Equation }})&lt;br /&gt;
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by the change of variables (for complete details see )&lt;br /&gt;
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通过变量替换(完整的细节见)&lt;br /&gt;
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:&amp;lt;math&amp;gt;\begin{align}&lt;br /&gt;
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V(S,t) &amp;amp;= K v(x,\tau),\\[5px]&lt;br /&gt;
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x &amp;amp;= \ln\left(\tfrac{S}{K} \right),\\[5px]&lt;br /&gt;
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\tau &amp;amp;= \tfrac{1}{2} \sigma^2 (T - t),\\[5px]&lt;br /&gt;
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v(x,\tau)&amp;amp;=e^{-\alpha x-\beta\tau} u(x,\tau).&lt;br /&gt;
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\end{align}&amp;lt;/math&amp;gt;&lt;br /&gt;
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===Fundamental solution===&lt;br /&gt;
基本解&lt;br /&gt;
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{{main|Fundamental solution}}&lt;br /&gt;
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Inhomogeneous equations can often be solved (for constant coefficient PDEs, always be solved) by finding the [[fundamental solution]] (the solution for a point source), then taking the [[convolution]] with the boundary conditions to get the solution.&lt;br /&gt;
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Inhomogeneous equations can often be solved (for constant coefficient PDEs, always be solved) by finding the fundamental solution (the solution for a point source), then taking the convolution with the boundary conditions to get the solution.&lt;br /&gt;
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非齐次方程(常系数偏微分方程)一般是通过先求出基本解(点源的解) ，然后利用带边界条件的卷积来求解。&lt;br /&gt;
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This is analogous in [[signal processing]] to understanding a filter by its [[impulse response]].&lt;br /&gt;
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This is analogous in signal processing to understanding a filter by its impulse response.&lt;br /&gt;
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这类似于在信号处理中通过滤波器的脉冲响应来理解滤波器。&lt;br /&gt;
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===Superposition principle===&lt;br /&gt;
叠加原理&lt;br /&gt;
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{{further| Superposition principle }}&lt;br /&gt;
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The superposition principle applies to any linear system, including linear systems of PDEs. A common visualization of this concept is the interaction of two waves in phase being combined to result in a greater amplitude, for example {{math|sin ''x'' + sin ''x'' {{=}} 2 sin ''x''}}. The same principle can be observed in PDEs where the solutions may be real or complex and additive. [[Superposition principle|superposition]]&lt;br /&gt;
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The superposition principle applies to any linear system, including linear systems of PDEs. A common visualization of this concept is the interaction of two waves in phase being combined to result in a greater amplitude, for example  2 sin x}}. The same principle can be observed in PDEs where the solutions may be real or complex and additive. superposition&lt;br /&gt;
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'''&amp;lt;font color = &amp;quot;#ff8000&amp;quot;&amp;gt;叠加原理 Superposition Principle&amp;lt;/font&amp;gt;适用于任何线性系统，包括偏微分方程的线性系统。这个概念的一个常见的可视化是两个同相位的波相互作用结合在一起会产生更大的振幅，例如 {{math|sin ''x'' + sin ''x'' {{=}} 2 sin ''x''}}。在偏微分方程中也可以观察到同样的原理，其中的解可能是真实的或复杂的和可加的。叠加&lt;br /&gt;
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If {{math|''u''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;}} and {{math|''u''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;}} are solutions of linear PDE in some function space {{mvar|R}}, then {{math|''u'' {{=}} ''c''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;''u''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; + ''c''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;''u''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;}} with any constants {{math|''c''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;}} and {{math|''c''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;}} are also a solution of that PDE in the same function space.&lt;br /&gt;
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If  and  are solutions of linear PDE in some function space , then  c&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;u&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; + c&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;u&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;}} with any constants  and  are also a solution of that PDE in the same function space.&lt;br /&gt;
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若线性偏微分方程在某个函数空间{{mvar|R}}中有解{{math|''u''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;}} 和 {{math|''u''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;}}，则{{math|''u'' {{=}} ''c''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;''u''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; + ''c''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;''u''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;}}也是该偏微分方程在同一函数空间中的解，其中{{math|''c''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;}} 和 {{math|''c''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;}} 是任意常数。&lt;br /&gt;
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===Methods for non-linear equations===&lt;br /&gt;
非线性方程的求解方法&lt;br /&gt;
{{see also|nonlinear partial differential equation}}&lt;br /&gt;
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There are no generally applicable methods to solve nonlinear PDEs. Still, existence and uniqueness results (such as the [[Cauchy–Kowalevski theorem]]) are often possible, as are proofs of important qualitative and quantitative properties of solutions (getting these results is a major part of [[mathematical analysis|analysis]]). Computational solution to the nonlinear PDEs, the [[split-step method]], exist for specific equations like [[nonlinear Schrödinger equation]].&lt;br /&gt;
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There are no generally applicable methods to solve nonlinear PDEs. Still, existence and uniqueness results (such as the Cauchy–Kowalevski theorem) are often possible, as are proofs of important qualitative and quantitative properties of solutions (getting these results is a major part of analysis). Computational solution to the nonlinear PDEs, the split-step method, exist for specific equations like nonlinear Schrödinger equation.&lt;br /&gt;
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对于非线性偏微分方程，目前还没有普遍适用的求解方法。然而，通常是可能知道解的存在性和唯一性(如柯西-科瓦列夫斯基定理)，也是可能得到解的重要定性和定量性质的证明(得到这些结果是分析的主要部分)。非线性偏微分方程的计算解，即分步法，对一些特定的方程适用，比如非线性'''&amp;lt;font color=&amp;quot;#ff8000&amp;quot;&amp;gt;薛定谔方程 Schrödinger equation&amp;lt;/font&amp;gt;'''。&lt;br /&gt;
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Nevertheless, some techniques can be used for several types of equations. The [[h-principle|{{mvar|h}}-principle]] is the most powerful method to solve [[Underdetermined system|underdetermined]] equations. The [[Riquier–Janet theory]] is an effective method for obtaining information about many analytic [[Overdetermined system|overdetermined]] systems.&lt;br /&gt;
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Nevertheless, some techniques can be used for several types of equations. The -principle is the most powerful method to solve underdetermined equations. The Riquier–Janet theory is an effective method for obtaining information about many analytic overdetermined systems.&lt;br /&gt;
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然而，一些技巧可以用于几种类型的方程。h-原理是求解欠定方程最有效的方法。里基尔-珍妮特理论是一种可以获得许多解析超定系统信息的有效方法。&lt;br /&gt;
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The [[method of characteristics]] can be used in some very special cases to solve partial differential equations.&lt;br /&gt;
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The method of characteristics can be used in some very special cases to solve partial differential equations.&lt;br /&gt;
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特征线法可用于求解某些特殊情况下的偏微分方程。&lt;br /&gt;
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In some cases, a PDE can be solved via [[perturbation analysis]] in which the solution is considered to be a correction to an equation with a known solution. Alternatives are [[numerical analysis]] techniques from simple [[finite difference]] schemes to the more mature [[multigrid]] and [[finite element method]]s. Many interesting problems in science and engineering are solved in this way using [[computer]]s, sometimes high performance [[supercomputer]]s.&lt;br /&gt;
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In some cases, a PDE can be solved via perturbation analysis in which the solution is considered to be a correction to an equation with a known solution. Alternatives are numerical analysis techniques from simple finite difference schemes to the more mature multigrid and finite element methods. Many interesting problems in science and engineering are solved in this way using computers, sometimes high performance supercomputers.&lt;br /&gt;
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在某些情况下，偏微分方程可以通过扰动分析来求解。在扰动分析中，通常是求解将具有已知解的方程修正后的新得到方程。可供选择的数值分析技术从简单的差分格式到更成熟的多重网格和有限元方法。许多有趣的科学和工程问题都是在计算机上用这种方法解决的，有时是高性能超级计算机。&lt;br /&gt;
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===Lie group method===&lt;br /&gt;
李群方法&lt;br /&gt;
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From 1870 [[Sophus Lie]]'s work put the theory of differential equations on a more satisfactory foundation. He showed that the integration theories of the older mathematicians can, by the introduction of what are now called [[Lie group]]s, be referred, to a common source; and that ordinary differential equations which admit the same [[infinitesimal transformation]]s present comparable difficulties of integration. He also emphasized the subject of [[contact transformation|transformations of contact]].&lt;br /&gt;
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From 1870 Sophus Lie's work put the theory of differential equations on a more satisfactory foundation. He showed that the integration theories of the older mathematicians can, by the introduction of what are now called Lie groups, be referred, to a common source; and that ordinary differential equations which admit the same infinitesimal transformations present comparable difficulties of integration. He also emphasized the subject of transformations of contact.&lt;br /&gt;
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从1870年起，索弗斯·李的工作为微分方程理论奠定了一个较为令人满意的基础。他指出，通过引入现在所谓的李群，老一辈数学家的积分理论可以引用到一个共同的来源; 承认相同的无穷小变换的常微分方程在积分方面存在相当的困难。他还强调了接触的转变这一主题。&lt;br /&gt;
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==[[用户:Yuling|Yuling]]（[[用户讨论:Yuling|讨论]]）这句话“He also emphasized the subject of transformations of contact.”中的transformations of contact翻译的不太好。&lt;br /&gt;
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A general approach to solving PDEs uses the symmetry property of differential equations, the continuous [[infinitesimal transformation]]s of solutions to solutions ([[Lie theory]]). Continuous [[group theory]], [[Lie algebras]] and [[differential geometry]] are used to understand the structure of linear and nonlinear partial differential equations for generating integrable equations, to find its [[Lax pair]]s, recursion operators, [[Bäcklund transform]] and finally finding exact analytic solutions to the PDE.&lt;br /&gt;
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A general approach to solving PDEs uses the symmetry property of differential equations, the continuous infinitesimal transformations of solutions to solutions (Lie theory). Continuous group theory, Lie algebras and differential geometry are used to understand the structure of linear and nonlinear partial differential equations for generating integrable equations, to find its Lax pairs, recursion operators, Bäcklund transform and finally finding exact analytic solutions to the PDE.&lt;br /&gt;
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求解偏微分方程的一般方法是利用微分方程的对称性，即解到解的连续无穷小变换(李理论)。连续群论、李代数和微分几何理论被用来理解生成可积方程的线性和非线性偏微分方程的结构，找到它的Lax对、递归算子、 贝克伦德变换，最后找到偏微分方程的精确解析解。&lt;br /&gt;
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Symmetry methods have been recognized to study differential equations arising in mathematics, physics, engineering, and many other disciplines.&lt;br /&gt;
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Symmetry methods have been recognized to study differential equations arising in mathematics, physics, engineering, and many other disciplines.&lt;br /&gt;
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对称方法已被公认可以用于研究出现在数学，物理，工程和许多其他学科的微分方程。&lt;br /&gt;
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===Semianalytical methods===&lt;br /&gt;
半解析方法&lt;br /&gt;
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The [[Adomian decomposition method]], the [[Aleksandr Lyapunov|Lyapunov]] artificial small parameter method, and He's [[homotopy perturbation method]] are all special cases of the more general [[homotopy analysis method]]. These are series expansion methods, and except for the Lyapunov method, are independent of small physical parameters as compared to the well known [[perturbation theory]], thus giving these methods greater flexibility and solution generality.&lt;br /&gt;
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The Adomian decomposition method, the Lyapunov artificial small parameter method, and He's homotopy perturbation method are all special cases of the more general homotopy analysis method. These are series expansion methods, and except for the Lyapunov method, are independent of small physical parameters as compared to the well known perturbation theory, thus giving these methods greater flexibility and solution generality.&lt;br /&gt;
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阿多米安分解法、李雅普诺夫人工小参数方法和何同伦摄动方法都是更一般的同伦分析方法的特殊情况。除了李雅普诺夫方法之外，这些都是级数展开方法，与为人熟知的摄动理论方法相比，它们与小的物理参数无关，因此这些方法具有更大的灵活性和解的通用性。&lt;br /&gt;
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== Numerical solutions ==&lt;br /&gt;
数值解&lt;br /&gt;
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The three most widely used [[Numerical partial differential equations|numerical methods to solve PDEs]] are the [[finite element analysis|finite element method]] (FEM), [[finite volume method]]s (FVM) and [[finite difference method]]s (FDM), as well other kind of methods called [[Meshfree methods]], which were made to solve problems where the before mentioned methods are limited. The FEM has a prominent position among these methods and especially its exceptionally efficient higher-order version [[hp-FEM]]. Other hybrid versions of FEM and Meshfree methods include the generalized finite element method (GFEM), [[extended finite element method]] (XFEM), [[Spectral element method|spectral finite element method]] (SFEM), [[Meshfree methods|meshfree finite element method]], [[Discontinuous Galerkin Method|discontinuous Galerkin finite element method]] (DGFEM), [[Element-Free Galerkin Method]] (EFGM), [[Interpolating Element-Free Galerkin Method]] (IEFGM), etc.&lt;br /&gt;
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The three most widely used numerical methods to solve PDEs are the finite element method (FEM), finite volume methods (FVM) and finite difference methods (FDM), as well other kind of methods called Meshfree methods, which were made to solve problems where the before mentioned methods are limited. The FEM has a prominent position among these methods and especially its exceptionally efficient higher-order version hp-FEM. Other hybrid versions of FEM and Meshfree methods include the generalized finite element method (GFEM), extended finite element method (XFEM), spectral finite element method (SFEM), meshfree finite element method, discontinuous Galerkin finite element method (DGFEM), Element-Free Galerkin Method (EFGM), Interpolating Element-Free Galerkin Method (IEFGM), etc.&lt;br /&gt;
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求解偏微分方程最常用的三种数值方法是有限元分析法、有限体积法和有限差分法，以及其他一些称为无网格法的方法。这些方法用于解决前面提到的方法受到的限制。在这些方法中，有限元方法，尤其是高效的高阶有限元方法，占有重要地位。其他有限元法和无网格法的混合形式包括广义有限元分析法(GFEM)、扩展有限元分析法(XFEM)、谱有限元分析法(SFEM)、无网格有限元分析法(DGFEM)、间断伽辽金有限元分析法(DGFEM)、无网格伽辽金法(EFGM)、插值无网格伽辽金法(IEFGM)等。&lt;br /&gt;
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=== Finite element method ===&lt;br /&gt;
有限元分析法&lt;br /&gt;
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{{main|Finite element method}}&lt;br /&gt;
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The finite element method (FEM) (its practical application often known as finite element analysis (FEA)) is a numerical technique for finding approximate solutions of partial differential equations (PDE) as well as of integral equations. The solution approach is based either on eliminating the differential equation completely (steady state problems), or rendering the PDE into an approximating system of ordinary differential equations, which are then numerically integrated using standard techniques such as Euler's method, Runge–Kutta, etc.&lt;br /&gt;
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The finite element method (FEM) (its practical application often known as finite element analysis (FEA)) is a numerical technique for finding approximate solutions of partial differential equations (PDE) as well as of integral equations. The solution approach is based either on eliminating the differential equation completely (steady state problems), or rendering the PDE into an approximating system of ordinary differential equations, which are then numerically integrated using standard techniques such as Euler's method, Runge–Kutta, etc.&lt;br /&gt;
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'''&amp;lt;font color = &amp;quot;#ff8000&amp;quot;&amp;gt;有限元分析法 Finite Element Method&amp;lt;/font&amp;gt;''' ((其实际应用通常被称为有限元分析(FEA))是一种寻找偏微分方程(PDE)和积分方程近似解的数值技术。这种求解方法要么基于完全消除微分方程(稳态问题) ，要么将偏微分方程转化为常微分方程的近似系统，然后使用标准技术进行数值积分，如欧拉方法、 Runge-Kutta 等。&lt;br /&gt;
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===Finite difference method===&lt;br /&gt;
有限差分法&lt;br /&gt;
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{{main|Finite difference method}}&lt;br /&gt;
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Finite-difference methods are numerical methods for approximating the solutions to differential equations using [[finite difference]] equations to approximate derivatives.&lt;br /&gt;
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Finite-difference methods are numerical methods for approximating the solutions to differential equations using finite difference equations to approximate derivatives.&lt;br /&gt;
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有限差分法是一种数值方法，用差分方程近似微分方程的解。&lt;br /&gt;
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=== Finite volume method ===&lt;br /&gt;
有限体积法&lt;br /&gt;
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{{main|Finite volume method}}&lt;br /&gt;
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Similar to the finite difference method or finite element method, values are calculated at discrete places on a meshed geometry. &amp;quot;Finite volume&amp;quot; refers to the small volume surrounding each node point on a mesh. In the finite volume method, surface integrals in a partial differential equation that contain a divergence term are converted to volume integrals, using the [[divergence theorem]]. These terms are then evaluated as fluxes at the surfaces of each finite volume. Because the flux entering a given volume is identical to that leaving the adjacent volume, these methods conserve mass by design.&lt;br /&gt;
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Similar to the finite difference method or finite element method, values are calculated at discrete places on a meshed geometry. &amp;quot;Finite volume&amp;quot; refers to the small volume surrounding each node point on a mesh. In the finite volume method, surface integrals in a partial differential equation that contain a divergence term are converted to volume integrals, using the divergence theorem. These terms are then evaluated as fluxes at the surfaces of each finite volume. Because the flux entering a given volume is identical to that leaving the adjacent volume, these methods conserve mass by design.&lt;br /&gt;
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类似于有限差分法或有限元分析，函数值是在网状几何体上的离散位置进行计算的。“有限体积”是指网格上每个节点周围的小体积。在有限体积法中，偏微分方程中含有散度项的面积分用散度定理积分转换成体积分。然后将这些项用于估算每个有限体积表面上的通量。由于进入给定体积的通量与转移到相邻体积元的通量相同，所以这些方法在设计上保证了质量守恒。&lt;br /&gt;
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==See also==&lt;br /&gt;
请参阅&lt;br /&gt;
* [[Dirichlet boundary condition]]&lt;br /&gt;
狄利克雷边界条件&lt;br /&gt;
* [[Jet bundle]]&lt;br /&gt;
射流丛&lt;br /&gt;
* [[Laplace transform applied to differential equations]]&lt;br /&gt;
微分方程中的拉普拉斯变换&lt;br /&gt;
* [[List of dynamical systems and differential equations topics]]&lt;br /&gt;
动力学系统和微分方程的列表&lt;br /&gt;
* [[Matrix differential equation]]&lt;br /&gt;
矩阵微分方程&lt;br /&gt;
* [[Neumann boundary condition]]&lt;br /&gt;
诺伊曼边界条件&lt;br /&gt;
* [[Numerical partial differential equations]]&lt;br /&gt;
数值偏微分方程&lt;br /&gt;
* [[Partial differential algebraic equation]]&lt;br /&gt;
偏微分代数方程&lt;br /&gt;
* [[Recurrence relation]]&lt;br /&gt;
递推关系&lt;br /&gt;
* [[Robin boundary condition]]&lt;br /&gt;
罗宾边界条件&lt;br /&gt;
* [[Stochastic processes and boundary value problems]]&lt;br /&gt;
随机过程和边值问题&lt;br /&gt;
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== The energy method ==&lt;br /&gt;
能量法&lt;br /&gt;
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The energy method is a mathematical procedure that can be used to verify well-posedness of initial-boundary-value-problems.&amp;lt;ref&amp;gt;{{cite book |title=High Order Difference Methods for Time Dependent PDE&lt;br /&gt;
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The energy method is a mathematical procedure that can be used to verify well-posedness of initial-boundary-value-problems.&amp;lt;ref&amp;gt;{{cite book |title=High Order Difference Methods for Time Dependent PDE&lt;br /&gt;
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能量法是验证初边值问题适定性的一种数学方法。 时变偏微分方程的高阶差分方法&lt;br /&gt;
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|first=Bertil|last=Gustafsson|publisher=Springer|year=2008|isbn=978-3-540-74992-9|doi=10.1007/978-3-540-74993-6}}&amp;lt;/ref&amp;gt; In the following example the energy method is used to decide where and which boundary conditions should be imposed such that the resulting IBVP is well-posed. Consider the one-dimensional hyperbolic PDE given by&lt;br /&gt;
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|first=Bertil|last=Gustafsson|publisher=Springer|year=2008|isbn=978-3-540-74992-9|doi=10.1007/978-3-540-74993-6}}&amp;lt;/ref&amp;gt; In the following example the energy method is used to decide where and which boundary conditions should be imposed such that the resulting IBVP is well-posed. Consider the one-dimensional hyperbolic PDE given by&lt;br /&gt;
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| first Bertil | last Gustafsson | publisher | Springer | year 2008 | isbn 978-3-540-74992-9 | doi 10.1007 / 978-3-540-74993-6} / ref 在下面的例子中，使用能量方法来决定应该施加哪些边界条件，使得得到的 IBVP适定。考虑一维双曲偏微分方程&lt;br /&gt;
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: &amp;lt;math&amp;gt;\frac{\partial u}{\partial t} + \alpha \frac{\partial u}{\partial x} = 0, \quad x \in [a,b], \operatorname t &amp;gt; 0,&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;\frac{\partial u}{\partial t} + \alpha \frac{\partial u}{\partial x} = 0, \quad x \in [a,b], \operatorname t &amp;gt; 0,&amp;lt;/math&amp;gt;&lt;br /&gt;
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where &amp;lt;math&amp;gt;\alpha \neq 0&amp;lt;/math&amp;gt; is a constant and &amp;lt;math&amp;gt;u(x,t)&amp;lt;/math&amp;gt; is an unknown function with initial condition &amp;lt;math&amp;gt;u(x,0) = f(x)&amp;lt;/math&amp;gt;. Multiplying with &amp;lt;math&amp;gt;u&amp;lt;/math&amp;gt; and integrating over the domain gives&lt;br /&gt;
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where &amp;lt;math&amp;gt;\alpha \neq 0&amp;lt;/math&amp;gt; is a constant and &amp;lt;math&amp;gt;u(x,t)&amp;lt;/math&amp;gt; is an unknown function with initial condition &amp;lt;math&amp;gt;u(x,0) = f(x)&amp;lt;/math&amp;gt;. Multiplying with &amp;lt;math&amp;gt;u&amp;lt;/math&amp;gt; and integrating over the domain gives&lt;br /&gt;
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其中 &amp;lt;math&amp;gt;\alpha \neq 0&amp;lt;/math&amp;gt; 是常数，并且 &amp;lt;math&amp;gt;u(x,t)&amp;lt;/math&amp;gt; 是未知函数，初始条件是 &amp;lt;math&amp;gt;u(x,0) = f(x)&amp;lt;/math&amp;gt;。乘以 &amp;lt;math&amp;gt;u&amp;lt;/math&amp;gt; 并在域上进行积分。&lt;br /&gt;
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: &amp;lt;math&amp;gt;\int_a^b u \frac{\partial u}{\partial t} \operatorname dx + \alpha \int _a ^b u \frac{\partial u}{\partial x} \operatorname dx = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;\int_a^b u \frac{\partial u}{\partial t} \operatorname dx + \alpha \int _a ^b u \frac{\partial u}{\partial x} \operatorname dx = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
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Using that&lt;br /&gt;
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Using that&lt;br /&gt;
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利用这一点&lt;br /&gt;
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: &amp;lt;math&amp;gt;\int _a ^b u \frac{\partial u}{\partial t} \operatorname dx = \frac{1}{2} \frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 \quad \text{and} \quad \int _a ^b u \frac{\partial u}{\partial x} \operatorname dx = \frac{1}{2} u(b,t)^2 - \frac{1}{2} u(a,t)^2,.&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;\int _a ^b u \frac{\partial u}{\partial t} \operatorname dx = \frac{1}{2} \frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 \quad \text{and} \quad \int _a ^b u \frac{\partial u}{\partial x} \operatorname dx = \frac{1}{2} u(b,t)^2 - \frac{1}{2} u(a,t)^2,.&amp;lt;/math&amp;gt;&lt;br /&gt;
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where integration by parts has been used for the second relationship, we get&lt;br /&gt;
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where integration by parts has been used for the second relationship, we get&lt;br /&gt;
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第二个关系中采用了分部积分法，我们可以得到&lt;br /&gt;
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: &amp;lt;math&amp;gt;\frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 + \alpha u(b,t)^2 - \alpha u(a,t)^2 = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;\frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 + \alpha u(b,t)^2 - \alpha u(a,t)^2 = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
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Here &amp;lt;math&amp;gt;\vert \vert \cdot \vert \vert&amp;lt;/math&amp;gt; denotes the standard L2-norm.&lt;br /&gt;
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Here &amp;lt;math&amp;gt;\vert \vert \cdot \vert \vert&amp;lt;/math&amp;gt; denotes the standard L2-norm.&lt;br /&gt;
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在这里，&amp;lt;math&amp;gt;\vert \vert \cdot \vert \vert&amp;lt;/math&amp;gt; 表示标准的 L2-正则。&lt;br /&gt;
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For well-posedness we require that the energy of the solution is non-increasing, i.e. that &amp;lt;math&amp;gt;\frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 \leq 0&amp;lt;/math&amp;gt;, which is achieved by specifying &amp;lt;math&amp;gt;u&amp;lt;/math&amp;gt; at &amp;lt;math&amp;gt;x = a&amp;lt;/math&amp;gt; if &amp;lt;math&amp;gt;\alpha &amp;gt; 0&amp;lt;/math&amp;gt; and at &amp;lt;math&amp;gt;x = b&amp;lt;/math&amp;gt; if &amp;lt;math&amp;gt;\alpha &amp;lt; 0&amp;lt;/math&amp;gt;. This corresponds to only imposing boundary conditions at the inflow. Note that well-posedness allows for growth in terms of data (initial and boundary) and thus it is sufficient to show that &amp;lt;math&amp;gt;\frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 \leq 0&amp;lt;/math&amp;gt; holds when all data is set to zero.&lt;br /&gt;
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For well-posedness we require that the energy of the solution is non-increasing, i.e. that &amp;lt;math&amp;gt;\frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 \leq 0&amp;lt;/math&amp;gt;, which is achieved by specifying &amp;lt;math&amp;gt;u&amp;lt;/math&amp;gt; at &amp;lt;math&amp;gt;x = a&amp;lt;/math&amp;gt; if &amp;lt;math&amp;gt;\alpha &amp;gt; 0&amp;lt;/math&amp;gt; and at &amp;lt;math&amp;gt;x = b&amp;lt;/math&amp;gt; if &amp;lt;math&amp;gt;\alpha &amp;lt; 0&amp;lt;/math&amp;gt;. This corresponds to only imposing boundary conditions at the inflow. Note that well-posedness allows for growth in terms of data (initial and boundary) and thus it is sufficient to show that &amp;lt;math&amp;gt;\frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 \leq 0&amp;lt;/math&amp;gt; holds when all data is set to zero.&lt;br /&gt;
&lt;br /&gt;
对于适定性，我们要解的能量是不增加的，即 &amp;lt;math&amp;gt;\frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 \leq 0&amp;lt;/math&amp;gt; ，这种关系可以通过在&amp;lt;math&amp;gt;x = a&amp;lt;/math&amp;gt;处 （如果 &amp;lt;math&amp;gt;\alpha &amp;gt; 0&amp;lt;/math&amp;gt;） 以及 &amp;lt;math&amp;gt;x = b&amp;lt;/math&amp;gt;处 （如果 &amp;lt;math&amp;gt;\alpha &amp;lt; 0&amp;lt;/math&amp;gt;）指定&amp;lt;math&amp;gt;u&amp;lt;/math&amp;gt;的值来实现。这只相当于在入流处附加边界条件。注意，适定性允许在数据(初始和边界)上的增长，因此它足以表明当所有数据设置为零时应有 &amp;lt;math&amp;gt;\frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 \leq 0&amp;lt;/math&amp;gt;。&lt;br /&gt;
&lt;br /&gt;
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==[[用户:Yuling|Yuling]]（[[用户讨论:Yuling|讨论]]）“This corresponds to only imposing boundary conditions at the inflow.” 这句话中的inflow不是很理解&lt;br /&gt;
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==Notes==&lt;br /&gt;
&lt;br /&gt;
{{Reflist}}&lt;br /&gt;
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== References ==&lt;br /&gt;
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{{refbegin|2}}&lt;br /&gt;
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|first=G.|last=Adomian|publisher=Kluwer Academic Publishers|year=1994|isbn=|page=|url=https://books.google.com/books?id=UKPqCAAAQBAJ&amp;amp;printsec=frontcover#v=onepage&amp;amp;q=%22partial%20differential%22&amp;amp;f=false}}&lt;br /&gt;
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&lt;br /&gt;
* {{Citation |first=A. D. |last=Polyanin |first2=V. F. |last2=Zaitsev |lastauthoramp=yes |first3=A. |last3=Moussiaux |title=Handbook of First Order Partial Differential Equations |publisher=Taylor &amp;amp; Francis |location=London |year=2002 |isbn=0-415-27267-X }}.&lt;br /&gt;
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* {{Citation |first=P. |last=Solin |title=Partial Differential Equations and the Finite Element Method |publisher=J. Wiley &amp;amp; Sons |location=Hoboken, NJ |year=2005 |isbn=0-471-72070-4 }}.&lt;br /&gt;
&lt;br /&gt;
* {{Citation |first=P. |last=Solin |first2=K. |last2=Segeth |lastauthoramp=yes |first3=I. |last3=Dolezel |title=Higher-Order Finite Element Methods |publisher=Chapman &amp;amp; Hall/CRC Press |location=Boca Raton |year=2003 |isbn=1-58488-438-X }}.&lt;br /&gt;
&lt;br /&gt;
* {{Citation |first=H. |last=Stephani |year=1989 |title=Differential Equations: Their Solution Using Symmetries. Edited by M. MacCallum |publisher=Cambridge University Press }}.&lt;br /&gt;
&lt;br /&gt;
* {{cite book |title=Partial Differential Equations and Solitary Waves Theory&lt;br /&gt;
&lt;br /&gt;
|first=Abdul-Majid|last=Wazwaz|publisher=Higher Education Press|year=2009|isbn=978-3-642-00251-9|page=}}&lt;br /&gt;
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|first=Abdul-Majid|last=Wazwaz|publisher=Higher Education Press|year=2009|isbn=978-3-642-00251-9|page=}}&lt;br /&gt;
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| first Abdul-Majid | last Wazwaz | publisher Higher Education Press | year 2009 | isbn 978-3-642-00251-9 | page }&lt;br /&gt;
&lt;br /&gt;
* {{cite book |title=Partial Differential Equations Methods and Applications&lt;br /&gt;
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|first=Abdul-Majid|last=Wazwaz|publisher=A.A. Balkema|year=2002|isbn=90-5809-369-7|page=}}&lt;br /&gt;
&lt;br /&gt;
| first Abdul-Majid | last Wazwaz | publisher a.a.Balkema | year 2002 | isbn 90-5809-369-7 | page }&lt;br /&gt;
&lt;br /&gt;
* {{Citation |first=D. |last=Zwillinger |title=Handbook of Differential Equations |publisher=Academic Press |location=Boston |year=1997 |edition=3rd |isbn=0-12-784395-7 }}.&lt;br /&gt;
&lt;br /&gt;
* {{Citation |authorlink=Neil Gershenfeld |first=N. |last=Gershenfeld |title=The Nature of Mathematical Modeling |location=New York |publisher=Cambridge University Press, New York, NY, USA |year=1999 |edition=1st |isbn=0-521-57095-6 }}.&lt;br /&gt;
&lt;br /&gt;
* {{Citation |first=I.S. |last=Krasil'shchik |lastauthoramp=yes |first2=A.M., Eds. |last2=Vinogradov |title=Symmetries and Conserwation Laws for Differential Equations of Mathematical Physics |publisher=American Mathematical Society, Providence, Rhode Island, USA |year=1999 |isbn=0-8218-0958-X }}.&lt;br /&gt;
&lt;br /&gt;
* {{Citation |first=I.S. |last=Krasil'shchik |first2=V.V. |last2=Lychagin|lastauthoramp=yes |first3=A.M. |last3=Vinogradov |title=Geometry of Jet Spaces and Nonlinear Partial Differential Equations |publisher=Gordon and Breach Science Publishers, New York, London, Paris, Montreux, Tokyo |year=1986 |isbn=2-88124-051-8 }}.&lt;br /&gt;
&lt;br /&gt;
* {{Citation |first=A.M. |last=Vinogradov |title=Cohomological Analysis of Partial Differential Equations and Secondary Calculus |publisher=American Mathematical Society, Providence, Rhode Island, USA |year=2001 |isbn=0-8218-2922-X }}.&lt;br /&gt;
&lt;br /&gt;
* {{cite book |title=High Order Difference Methods for Time Dependent PDE&lt;br /&gt;
&lt;br /&gt;
|first=Bertil|last=Gustafsson|publisher=Springer|year=2008|isbn=978-3-540-74992-9|doi=10.1007/978-3-540-74993-6}}&lt;br /&gt;
&lt;br /&gt;
|first=Bertil|last=Gustafsson|publisher=Springer|year=2008|isbn=978-3-540-74992-9|doi=10.1007/978-3-540-74993-6}}&lt;br /&gt;
&lt;br /&gt;
| first Bertil | last Gustafsson | Springer | year 2008 | isbn 978-3-540-74992-9 | doi 10.1007 / 978-3-540-74993-6}&lt;br /&gt;
&lt;br /&gt;
{{refend}}&lt;br /&gt;
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&lt;br /&gt;
== Further reading ==&lt;br /&gt;
&lt;br /&gt;
* {{Cite journal|last=Cajori|first=Florian|authorlink=Florian Cajori|year=1928|title=The Early History of Partial Differential Equations and of Partial Differentiation and Integration|url=http://www.math.harvard.edu/archive/21a_fall_14/exhibits/cajori/cajori.pdf|journal=The American Mathematical Monthly|volume=35|issue=9|pages=459–467|doi=10.2307/2298771|access-date=2016-05-15|archive-url=https://web.archive.org/web/20181123102253/http://www.math.harvard.edu/archive/21a_fall_14/exhibits/cajori/cajori.pdf|archive-date=2018-11-23|url-status=dead}}&lt;br /&gt;
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== External links ==&lt;br /&gt;
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{{Sister project links| wikt=no | commons=Category:Solutions of PDE | b=Partial Differential Equations | n=no | q=Partial differential equation | s=no | v=no | voy=no | species=no | d=no}}&lt;br /&gt;
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* {{springer|title=Differential equation, partial|id=p/d031920}}&lt;br /&gt;
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* [http://eqworld.ipmnet.ru/en/pde-en.htm Partial Differential Equations: Exact Solutions] at EqWorld: The World of Mathematical Equations.&lt;br /&gt;
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* [http://eqworld.ipmnet.ru/en/solutions/eqindex/eqindex-pde.htm Partial Differential Equations: Index] at EqWorld: The World of Mathematical Equations.&lt;br /&gt;
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* [http://eqworld.ipmnet.ru/en/methods/meth-pde.htm Partial Differential Equations: Methods] at EqWorld: The World of Mathematical Equations.&lt;br /&gt;
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* [https://web.archive.org/web/20170701144823/http://www.exampleproblems.com/wiki/index.php?title=Partial_Differential_Equations Example problems with solutions] at exampleproblems.com&lt;br /&gt;
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* [http://mathworld.wolfram.com/PartialDifferentialEquation.html Partial Differential Equations] at mathworld.wolfram.com&lt;br /&gt;
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* [https://reference.wolfram.com/language/FEMDocumentation/tutorial/SolvingPDEwithFEM.html Partial Differential Equations] with Mathematica&lt;br /&gt;
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* [http://www.mathworks.com/moler/pdes.pdf Partial Differential Equations] in Cleve Moler: Numerical Computing with MATLAB&lt;br /&gt;
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* [http://www.nag.com/numeric/fl/nagdoc_fl24/html/D03/d03intro.html Partial Differential Equations] at nag.com&lt;br /&gt;
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* {{cite web |first=Grant |last=Sanderson |title=But what is a partial differential equation? |work=3Blue1Brown |date=April 21, 2019 |url=https://www.youtube.com/watch?v=ly4S0oi3Yz8&amp;amp;list=PLZHQObOWTQDNPOjrT6KVlfJuKtYTftqH6 |via=[[YouTube]] }}&lt;br /&gt;
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{{Differential equations topics}}&lt;br /&gt;
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{{Authority control}}&lt;br /&gt;
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[[Category:Partial differential equations| ]]&lt;br /&gt;
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[[Category:Multivariable calculus]]&lt;br /&gt;
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Category:Multivariable calculus&lt;br /&gt;
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类别: 多元微积分&lt;br /&gt;
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[[Category:Differential equations]]&lt;br /&gt;
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Category:Differential equations&lt;br /&gt;
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类别: 微分方程&lt;br /&gt;
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[[Category:Concepts in physics]]&lt;br /&gt;
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Category:Concepts in physics&lt;br /&gt;
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分类: 物理概念&lt;br /&gt;
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&amp;lt;small&amp;gt;This page was moved from [[wikipedia:en:Partial differential equation]]. Its edit history can be viewed at [[偏微分方程/edithistory]]&amp;lt;/small&amp;gt;&amp;lt;/noinclude&amp;gt;&lt;br /&gt;
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[[Category:待整理页面]]&lt;/div&gt;</summary>
		<author><name>Ruili</name></author>
	</entry>
	<entry>
		<id>https://wiki.swarma.org/index.php?title=%E5%81%8F%E5%BE%AE%E5%88%86%E6%96%B9%E7%A8%8B&amp;diff=18120</id>
		<title>偏微分方程</title>
		<link rel="alternate" type="text/html" href="https://wiki.swarma.org/index.php?title=%E5%81%8F%E5%BE%AE%E5%88%86%E6%96%B9%E7%A8%8B&amp;diff=18120"/>
		<updated>2020-11-11T13:43:31Z</updated>

		<summary type="html">&lt;p&gt;Ruili：&lt;/p&gt;
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&lt;div&gt;此词条暂由Yuling翻译，未经人工整理和审校，带来阅读不便，请见谅。&lt;br /&gt;
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[[File:Heat.gif|thumb|right|A visualisation of a solution to the two-dimensional [[heat equation]] with temperature represented by the third dimension]]&lt;br /&gt;
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A visualisation of a solution to the two-dimensional [[heat equation with temperature represented by the third dimension]]&lt;br /&gt;
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以三维表示温度的二维热方程解的可视化&lt;br /&gt;
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In [[mathematics]], a '''partial differential equation''' ('''PDE''') is a [[differential equation]] that contains unknown [[Multivariable calculus|multivariable functions]] and their [[partial derivative]]s. PDEs are used to formulate problems involving functions of several variables, and are either solved by hand, or used to create a [[computer model]]. A special case is [[ordinary differential equation]]s (ODEs), which deal with functions of a single variable and their derivatives.&lt;br /&gt;
&lt;br /&gt;
In mathematics, a partial differential equation (PDE) is a differential equation that contains unknown multivariable functions and their partial derivatives. PDEs are used to formulate problems involving functions of several variables, and are either solved by hand, or used to create a computer model. A special case is ordinary differential equations (ODEs), which deal with functions of a single variable and their derivatives.&lt;br /&gt;
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在数学中，'''&amp;lt;font color = &amp;quot;#ff8000&amp;quot;&amp;gt; 偏微分方程函数 Partial Differential Equation&amp;lt;/font&amp;gt;'''是包含未知多元函数及其偏导数的微分方程。偏微分方程用于描述涉及多元函数的问题，可以通过人为求解，也可以通过建立计算机模型来求解。常微分方程是偏微分方程一种特殊情况，它处理的是一元函数及其导数。&lt;br /&gt;
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PDEs can be used to describe a wide variety of phenomena such as sound, heat, [[diffusion]], [[electrostatics]], [[Electromagnetism|electrodynamics]], [[fluid dynamics]], [[Elasticity (physics)|elasticity]], [[gravitation]] and [[quantum mechanics]]. These seemingly distinct physical phenomena can be formalised similarly in terms of PDEs. Just as ordinary differential equations often model one-dimensional [[dynamical system]]s, partial differential equations often model [[multidimensional system]]s. PDEs find their generalisation in [[stochastic partial differential equation]]s.&lt;br /&gt;
&lt;br /&gt;
PDEs can be used to describe a wide variety of phenomena such as sound, heat, diffusion, electrostatics, electrodynamics, fluid dynamics, elasticity, gravitation and quantum mechanics. These seemingly distinct physical phenomena can be formalised similarly in terms of PDEs. Just as ordinary differential equations often model one-dimensional dynamical systems, partial differential equations often model multidimensional systems. PDEs find their generalisation in stochastic partial differential equations.&lt;br /&gt;
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偏微分方程可以用来描述各种各样的物理现象，如声音，热量，扩散，静电，电动力学，流体力学，弹性力学，重力和量子力学。这些看起来截然不同的物理现象却可以用类似的偏微分方程来描述。正如常微分方程经常对一维动力系统进行建模一样，偏微分方程经常对多维系统进行建模。随机偏微分方程是偏微分方程的一种推广。&lt;br /&gt;
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== Introduction ==&lt;br /&gt;
引言&lt;br /&gt;
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Partial differential equations (PDEs) are equations that involve rates of change with respect to [[continuous variables]]. For example, the position of a [[rigid body]] is specified by six parameters,&amp;lt;ref&amp;gt;{{Cite book|url=https://books.google.com/books?id=v9PLbcYd9aUC&amp;amp;pg=PA32|title=Modelling and Control of Robot Manipulators|last=Sciavicco|first=Lorenzo|last2=Siciliano|first2=Bruno|date=2001-02-19|publisher=Springer Science &amp;amp; Business Media|isbn=9781852332211|language=en}}&amp;lt;/ref&amp;gt; but the configuration of a [[fluid]] is given by the [[continuous distribution]] of several parameters, such as the [[temperature]], [[pressure]], and so forth. The dynamics for the rigid body take place in a finite-dimensional [[Configuration space (physics)|configuration space]]; the dynamics for the fluid occur in an infinite-dimensional configuration space. This distinction usually makes PDEs much harder to solve than ordinary differential equations (ODEs), but here again, there will be simple solutions for linear problems. Classic domains where PDEs are used include [[acoustics]], [[fluid dynamics]], [[electrodynamics]], and [[heat transfer]].&lt;br /&gt;
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Partial differential equations (PDEs) are equations that involve rates of change with respect to continuous variables. For example, the position of a rigid body is specified by six parameters, but the configuration of a fluid is given by the continuous distribution of several parameters, such as the temperature, pressure, and so forth. The dynamics for the rigid body take place in a finite-dimensional configuration space; the dynamics for the fluid occur in an infinite-dimensional configuration space. This distinction usually makes PDEs much harder to solve than ordinary differential equations (ODEs), but here again, there will be simple solutions for linear problems. Classic domains where PDEs are used include acoustics, fluid dynamics, electrodynamics, and heat transfer.&lt;br /&gt;
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偏微分方程(简称为PDEs)涉及到方程相对于连续变量的变化率。例如，刚体的位置是由六个参数确定的，而流体的状态是由几个参数的连续分布给出的，如温度、压力等。刚体的动力学过程发生在有限维状态空间中，流体的动力学过程发生在无限维状态空间中。这种区别通常使偏微分方程比常微分方程更难求解，但是线性问题仍然有简单的求解方式。使用偏微分方程的经典领域包括声学、流体力学、电动力学和传热学。&lt;br /&gt;
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A partial differential equation (PDE) for the function {{math|''u''(''x''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;,… ''x&amp;lt;sub&amp;gt;n&amp;lt;/sub&amp;gt;'')}} is an equation of the form&lt;br /&gt;
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A partial differential equation (PDE) for the function  is an equation of the form&lt;br /&gt;
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函数 {{math|''u''(''x''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;,… ''x&amp;lt;sub&amp;gt;n&amp;lt;/sub&amp;gt;'')}} 的偏微分方程形式是：&lt;br /&gt;
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: &amp;lt;math&amp;gt;f \left (x_1, \ldots x_n; u, \frac{\partial u}{\partial x_1}, \ldots \frac{\partial u}{\partial x_n}; \frac{\partial^2 u}{\partial x_1 \partial x_1}, \ldots \frac{\partial^2 u}{\partial x_1 \partial x_n}; \ldots \right) = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;f \left (x_1, \ldots x_n; u, \frac{\partial u}{\partial x_1}, \ldots \frac{\partial u}{\partial x_n}; \frac{\partial^2 u}{\partial x_1 \partial x_1}, \ldots \frac{\partial^2 u}{\partial x_1 \partial x_n}; \ldots \right) = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
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If {{mvar|f}} is a [[linear function]] of {{mvar|u}} and its derivatives, then the PDE is called linear. Common examples of linear PDEs include the [[heat equation]], the [[wave equation]], [[Laplace's equation]], [[Helmholtz equation]], [[Klein–Gordon equation]], and [[Poisson's equation]].&lt;br /&gt;
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If  is a linear function of  and its derivatives, then the PDE is called linear. Common examples of linear PDEs include the heat equation, the wave equation, Laplace's equation, Helmholtz equation, Klein–Gordon equation, and Poisson's equation.&lt;br /&gt;
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如果 {{mvar|f}} 是函数 {{math|''u''}} 及其导数的线性函数，则偏微分方程称为线性函数。线性偏微分方程的常见例子包括热方程、波动方程、拉普拉斯方程、亥姆霍兹方程方程、克莱因-高登方程和泊松方程。&lt;br /&gt;
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A relatively simple PDE is&lt;br /&gt;
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A relatively simple PDE is&lt;br /&gt;
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一个相对简单的偏微分方程：&lt;br /&gt;
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: &amp;lt;math&amp;gt;\frac{\partial u}{\partial x}(x,y) = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;\frac{\partial u}{\partial x}(x,y) = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
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This relation [[Logical implication|implies]] that the function {{math|''u''(''x'',''y'')}} is independent of {{mvar|x}}. However, the equation gives no information on the function's dependence on the variable {{mvar|y}}. Hence the general solution of this equation is&lt;br /&gt;
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This relation implies that the function  is independent of . However, the equation gives no information on the function's dependence on the variable . Hence the general solution of this equation is&lt;br /&gt;
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这意味着函数 {{math|''u''(''x'',''y'')}} 独立于 {{mvar|x}} 的。然而，这个方程没有给出关于函数和自变量的相关性的信息。因此，这个方程的通解是&lt;br /&gt;
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: &amp;lt;math&amp;gt;u(x,y) = f(y),&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;u(x,y) = f(y),&amp;lt;/math&amp;gt;&lt;br /&gt;
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where {{mvar|f}} is an arbitrary function of {{mvar|y}}. The analogous ordinary differential equation is&lt;br /&gt;
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where  is an arbitrary function of . The analogous ordinary differential equation is&lt;br /&gt;
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其中， {{mvar|f}} 是 {{mvar|y}} 的任意函数。&lt;br /&gt;
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类似的常微分方程是：&lt;br /&gt;
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: &amp;lt;math&amp;gt;\frac{\mathrm{d} u}{\mathrm{d} x}(x) = 0,&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;\frac{\mathrm{d} u}{\mathrm{d} x}(x) = 0,&amp;lt;/math&amp;gt;&lt;br /&gt;
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which has the solution&lt;br /&gt;
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which has the solution&lt;br /&gt;
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它的解为&lt;br /&gt;
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: &amp;lt;math&amp;gt;u(x) = c,&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;u(x) = c,&amp;lt;/math&amp;gt;&lt;br /&gt;
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where {{mvar|c}} is any [[Constant (mathematics)|constant]] value. These two examples illustrate that general solutions of ordinary differential equations (ODEs) involve arbitrary constants, but solutions of PDEs involve arbitrary functions.&lt;br /&gt;
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where  is any constant value. These two examples illustrate that general solutions of ordinary differential equations (ODEs) involve arbitrary constants, but solutions of PDEs involve arbitrary functions.&lt;br /&gt;
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这里，{{mvar|c}} 是一个任意常量。&lt;br /&gt;
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这两个例子说明常微分方程的一般解包含任意常数，但偏微分方程的解包含任意函数。&lt;br /&gt;
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A solution of a PDE is generally not [[Uniqueness quantification|unique]]; additional conditions must generally be specified on the [[Boundary (topology)|boundary]] of the region where the solution is defined. For instance, in the simple example above, the function {{math|''f''(''y'')}} can be determined if {{mvar|u}} is specified on the line {{math|''x'' {{=}} 0}}.&lt;br /&gt;
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A solution of a PDE is generally not unique; additional conditions must generally be specified on the boundary of the region where the solution is defined. For instance, in the simple example above, the function  can be determined if  is specified on the line  0}}.&lt;br /&gt;
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偏微分方程的解一般不是唯一的; 一般必须在定义解的区域边界上定义附加条件。 例如，在上面的简单示例中，如果在 {{math|''x'' {{=}} 0}} 时确定了 {{mvar|u}} 的值，则可以确定该函数 {{math|''f''(''y'')}}。&lt;br /&gt;
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== Existence and uniqueness ==&lt;br /&gt;
存在性和唯一性&lt;br /&gt;
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Although the issue of existence and uniqueness of solutions of ordinary differential equations has a very satisfactory answer with the [[Picard–Lindelöf theorem]], that is far from the case for partial differential equations. The [[Cauchy–Kowalevski theorem]] states that the [[Cauchy problem]] for any partial differential equation whose coefficients are [[Analytic function|analytic]] in the unknown function and its derivatives, has a locally unique analytic solution. Although this result might appear to settle the existence and uniqueness of solutions, there are examples of linear partial differential equations whose coefficients have derivatives of all orders (which are nevertheless not analytic) but which have no solutions at all: see [[Lewy's example|Lewy (1957)]]. Even if the solution of a partial differential equation exists and is unique, it may nevertheless have undesirable properties.  The mathematical study of these questions is usually in the more powerful context of [[weak solution]]s.&lt;br /&gt;
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Although the issue of existence and uniqueness of solutions of ordinary differential equations has a very satisfactory answer with the Picard–Lindelöf theorem, that is far from the case for partial differential equations. The Cauchy–Kowalevski theorem states that the Cauchy problem for any partial differential equation whose coefficients are analytic in the unknown function and its derivatives, has a locally unique analytic solution. Although this result might appear to settle the existence and uniqueness of solutions, there are examples of linear partial differential equations whose coefficients have derivatives of all orders (which are nevertheless not analytic) but which have no solutions at all: see Lewy (1957). Even if the solution of a partial differential equation exists and is unique, it may nevertheless have undesirable properties.  The mathematical study of these questions is usually in the more powerful context of weak solutions.&lt;br /&gt;
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虽然常微分方程解的存在唯一性问题用'''&amp;lt;font color=&amp;quot;#ff8000&amp;quot;&amp;gt;弗罗贝尼乌斯定理 Picard–Lindelöf Theorem&amp;lt;/font&amp;gt;得到了令人满意的结果，但应用到偏微分方程上却不尽如意。'''&amp;lt;font color=&amp;quot;#ff8000&amp;quot;&amp;gt;柯西-科瓦列夫斯基定理 Cauchy–Kowalevski theorem&amp;lt;/font&amp;gt;指出，对于任何在未知函数及其导数中系数是解析的偏微分方程，柯西问题有一个局部唯一的解析解。虽然这个结果似乎解决了解的存在性和唯一性问题，但是有一些线性偏微分方程的系数具有所有级数的导数(尽管这些导数不是解析的) ，但是根本没有解: 见 Lewy (1957)。即使偏微分方程的解存在且唯一，它仍然可能具有人们所不希望的性质。这些问题的数学研究通常是在更有力的弱解的背景下进行的。&lt;br /&gt;
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An example of pathological behavior is the sequence (depending upon {{mvar|n}}) of [[Cauchy problem]]s for the [[Laplace equation]]&lt;br /&gt;
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An example of pathological behavior is the sequence (depending upon ) of Cauchy problems for the Laplace equation&lt;br /&gt;
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反常特征的一个例子是拉普拉斯方程的柯西问题的序列(取决于{{mvar|n}})&lt;br /&gt;
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: &amp;lt;math&amp;gt;\frac{\partial^2 u}{\partial x^2} + \frac{\partial^2 u}{\partial y^2}=0,&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;\frac{\partial^2 u}{\partial x^2} + \frac{\partial^2 u}{\partial y^2}=0,&amp;lt;/math&amp;gt;&lt;br /&gt;
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with [[boundary condition]]s&lt;br /&gt;
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with boundary conditions&lt;br /&gt;
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有边界条件&lt;br /&gt;
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: &amp;lt;math&amp;gt;\begin{align} u(x,0) &amp;amp;= 0, \\ \frac{\partial u}{\partial y}(x,0) &amp;amp;= \frac{\sin nx}{n}, \end{align}&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;\begin{align} u(x,0) &amp;amp;= 0, \\ \frac{\partial u}{\partial y}(x,0) &amp;amp;= \frac{\sin nx}{n}, \end{align}&amp;lt;/math&amp;gt;&lt;br /&gt;
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where {{mvar|n}} is an integer. The derivative of {{mvar|u}} with respect to {{mvar|y}} approaches zero [[uniform convergence|uniformly]] in {{mvar|x}} as {{mvar|n}} increases, but the solution is&lt;br /&gt;
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where  is an integer. The derivative of  with respect to  approaches zero uniformly in  as  increases, but the solution is&lt;br /&gt;
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其中{{mvar|n}}是整数。{{mvar|u}}是关于{{mvar|y}}的导数，一致地随着{{mvar|n}}的增加而趋于零，但是解是&lt;br /&gt;
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: &amp;lt;math&amp;gt;u(x,y) = \frac{\sinh ny \sin nx}{n^2}.&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;u(x,y) = \frac{\sinh ny \sin nx}{n^2}.&amp;lt;/math&amp;gt;&lt;br /&gt;
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This solution approaches infinity if {{mvar|nx}} is not an integer multiple of {{pi}} for any non-zero value of {{mvar|y}}. The Cauchy problem for the Laplace equation is called ''ill-posed'' or ''not [[Well-posed problem|well-posed]]'', since the solution does not continuously depend on the data of the problem. Such ill-posed problems are not usually satisfactory for physical applications.&lt;br /&gt;
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This solution approaches infinity if  is not an integer multiple of  for any non-zero value of . The Cauchy problem for the Laplace equation is called ill-posed or not well-posed, since the solution does not continuously depend on the data of the problem. Such ill-posed problems are not usually satisfactory for physical applications.&lt;br /&gt;
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对于任何非零的{{mvar|y}}，如果{{mvar|nx}}不是{{pi}}的整数倍，这个解会接近于无穷大。拉普拉斯方程的柯西问题被称为不适定问题（可以译为ill-posed或not well-posed），因为该问题的解并不连续地依赖于该问题的数据。这种不适定问题在物理应用中通常不能令人满意。&lt;br /&gt;
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The [[Navier–Stokes existence and smoothness|existence of solutions for the Navier–Stokes equations]], a partial differential equation, is part of one of the [[Millennium Prize Problems]].&lt;br /&gt;
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The existence of solutions for the Navier–Stokes equations, a partial differential equation, is part of one of the Millennium Prize Problems.&lt;br /&gt;
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一种偏微分方程——纳维-斯托克斯方程——的解的存在性就是千禧年大奖难题的一部分。&lt;br /&gt;
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== Notation ==&lt;br /&gt;
符号&lt;br /&gt;
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In PDEs, it is common to denote partial derivatives using subscripts. That is:&lt;br /&gt;
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In PDEs, it is common to denote partial derivatives using subscripts. That is:&lt;br /&gt;
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在偏微分方程中，通常用下标表示偏导数。例如:&lt;br /&gt;
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: &amp;lt;math&amp;gt;u_x = \frac{\partial u}{\partial x}&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;u_x = \frac{\partial u}{\partial x}&amp;lt;/math&amp;gt;&lt;br /&gt;
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: &amp;lt;math&amp;gt;u_{xx} = \frac{\partial^2 u}{\partial x^2} &amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;u_{xx} = \frac{\partial^2 u}{\partial x^2} &amp;lt;/math&amp;gt;&lt;br /&gt;
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: &amp;lt;math&amp;gt;u_{xy} = \frac{\partial^2 u}{\partial y\, \partial x} = \frac{\partial}{\partial y } \left(\frac{\partial u}{\partial x}\right). &amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;u_{xy} = \frac{\partial^2 u}{\partial y\, \partial x} = \frac{\partial}{\partial y } \left(\frac{\partial u}{\partial x}\right). &amp;lt;/math&amp;gt;&lt;br /&gt;
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Especially in physics, [[del]] or nabla ({{math|∇}}) is often used to denote spatial derivatives, and {{math|''&amp;amp;#x307;u'', ''ü''}} for time derivatives. For example, the [[wave equation]] (mentioned below) can be written as&lt;br /&gt;
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Especially in physics, del or nabla () is often used to denote spatial derivatives, and  for time derivatives. For example, the wave equation (mentioned below) can be written as&lt;br /&gt;
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特别是在物理学中，[[del]]或nabla ({{math|∇}})经常用来表示空间导数和时间导数。例如，波动方程(在下文中提到)可以写成&lt;br /&gt;
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:&amp;lt;math&amp;gt;\ddot u=c^2\nabla^2u&amp;lt;/math&amp;gt;&lt;br /&gt;
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&amp;lt;math&amp;gt;\ddot u=c^2\nabla^2u&amp;lt;/math&amp;gt;&lt;br /&gt;
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or&lt;br /&gt;
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or&lt;br /&gt;
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或&lt;br /&gt;
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:&amp;lt;math&amp;gt;\ddot u=c^2\Delta u&amp;lt;/math&amp;gt;&lt;br /&gt;
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&amp;lt;math&amp;gt;\ddot u=c^2\Delta u&amp;lt;/math&amp;gt;&lt;br /&gt;
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where {{math|Δ}} is the [[Laplace operator]].&lt;br /&gt;
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where  is the Laplace operator.&lt;br /&gt;
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其中{{math|Δ}}代表拉普拉斯算子&lt;br /&gt;
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== Classification ==&lt;br /&gt;
分类&lt;br /&gt;
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Some linear, second-order partial differential equations can be classified as [[parabolic partial differential equation|parabolic]], [[hyperbolic partial differential equation|hyperbolic]] and [[elliptic partial differential equation|elliptic]]. Others, such as the [[Euler–Tricomi equation]], have different types in different regions. The classification provides a guide to appropriate initial and boundary conditions and to the smoothness of the solutions.&lt;br /&gt;
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Some linear, second-order partial differential equations can be classified as parabolic, hyperbolic and elliptic. Others, such as the Euler–Tricomi equation, have different types in different regions. The classification provides a guide to appropriate initial and boundary conditions and to the smoothness of the solutions.&lt;br /&gt;
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一些线性二阶偏微分方程可分为抛物型方程、双曲型方程和椭圆型方程。其他的方程，如欧拉-特里科米方程，在不同的区域有不同的类型。这种分类有助于选择适当的初始和边界条件以及提高解的平滑性。&lt;br /&gt;
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=== Equations of first order ===&lt;br /&gt;
一阶方程&lt;br /&gt;
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{{main|First-order partial differential equation}}&lt;br /&gt;
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=== Linear equations of second order ===&lt;br /&gt;
二阶线性方程&lt;br /&gt;
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Assuming {{math|''u&amp;lt;sub&amp;gt;xy&amp;lt;/sub&amp;gt;'' {{=}} ''u&amp;lt;sub&amp;gt;yx&amp;lt;/sub&amp;gt;''}}, the general linear second-order PDE in two independent variables has the form&lt;br /&gt;
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Assuming  u&amp;lt;sub&amp;gt;yx&amp;lt;/sub&amp;gt;}}, the general linear second-order PDE in two independent variables has the form&lt;br /&gt;
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假设 {{math|''u&amp;lt;sub&amp;gt;xy&amp;lt;/sub&amp;gt;'' {{=}} ''u&amp;lt;sub&amp;gt;yx&amp;lt;/sub&amp;gt;''}}，含有两个独立变量的一般的线性二阶偏微分方程具有如下这样的形式&lt;br /&gt;
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: &amp;lt;math&amp;gt;Au_{xx} + 2Bu_{xy} + Cu_{yy} + \cdots \mbox{(lower order terms)} = 0,&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;Au_{xx} + 2Bu_{xy} + Cu_{yy} + \cdots \mbox{(lower order terms)} = 0,&amp;lt;/math&amp;gt;&lt;br /&gt;
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where the coefficients {{mvar|A}}, {{mvar|B}}, {{mvar|C}}... may depend upon {{mvar|x}} and {{mvar|y}}. If {{math|''A''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; + ''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; + ''C''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; &amp;gt; 0}} over a region of the {{mvar|xy}}-plane, the PDE is second-order in that region. This form is analogous to the equation for a conic section:&lt;br /&gt;
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where the coefficients , , ... may depend upon  and . If  over a region of the -plane, the PDE is second-order in that region. This form is analogous to the equation for a conic section:&lt;br /&gt;
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其中的系数 {{mvar|A}}, {{mvar|B}}, {{mvar|C}}... 一般取决于{{mvar|x}}和{{mvar|y}}。如果在{{mvar|xy}}-平面的一个区域上 {{math|''A''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; + ''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; + ''C''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; &amp;gt; 0}}，偏微分方程在该区域是二阶的。这种形式类似于圆锥曲线的方程:&lt;br /&gt;
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: &amp;lt;math&amp;gt;Ax^2 + 2Bxy + Cy^2 + \cdots = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;Ax^2 + 2Bxy + Cy^2 + \cdots = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
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More precisely, replacing {{math|∂&amp;lt;sub&amp;gt;''x''&amp;lt;/sub&amp;gt;}} by {{mvar|X}}, and likewise for other variables (formally this is done by a [[Fourier transform]]), converts a constant-coefficient PDE into a polynomial of the same degree, with the terms of the highest degree (a [[homogeneous polynomial]], here a [[quadratic form]]) being most significant for the classification.&lt;br /&gt;
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More precisely, replacing  by , and likewise for other variables (formally this is done by a Fourier transform), converts a constant-coefficient PDE into a polynomial of the same degree, with the terms of the highest degree (a homogeneous polynomial, here a quadratic form) being most significant for the classification.&lt;br /&gt;
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更准确地说，用 {{mvar|X}} 替换 {{math|∂&amp;lt;sub&amp;gt;''x''&amp;lt;/sub&amp;gt;}}，对于其他变量做同样的操作(从形式上来说，这是由傅里叶变换来完成的)，将一个常系数偏微分方程转换成一个相同次数的多项式，最高次数的项(齐次多项式，这里是一个二次形式)一般会用于偏微分方程的分类。&lt;br /&gt;
===~~ most significant for the classification 意译为用于偏微分方程的分类。       significiant直译过来感觉不太合适&lt;br /&gt;
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Just as one classifies [[conic section]]s and quadratic forms into parabolic, hyperbolic, and elliptic based on the [[discriminant]] {{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − 4''AC''}}, the same can be done for a second-order PDE at a given point.  However, the [[discriminant]] in a PDE is given by {{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC''}} due to the convention of the {{mvar|xy}} term being {{math|2''B''}} rather than {{mvar|B}}; formally, the discriminant (of the associated quadratic form) is {{math|(2''B'')&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − 4''AC'' {{=}} 4(''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC'')}}, with the factor of 4 dropped for simplicity.&lt;br /&gt;
&lt;br /&gt;
Just as one classifies conic sections and quadratic forms into parabolic, hyperbolic, and elliptic based on the discriminant , the same can be done for a second-order PDE at a given point.  However, the discriminant in a PDE is given by  due to the convention of the  term being  rather than ; formally, the discriminant (of the associated quadratic form) is  4(B&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − AC)}}, with the factor of 4 dropped for simplicity.&lt;br /&gt;
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正如人们可以根据判别式 {{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − 4''AC''}} 将圆锥曲线和二次型分为抛物型、双曲型和椭圆型一样，对于给定点的二阶偏微分方程也可以这样做。然而，偏微分方程中的判别式 {{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − 4''AC''}} 是根据交叉项的系数{{math|2''B''}} 而不是 {{mvar|B}} 给出的，形式上，判别式(关联二次型)是 {{math|(2''B'')&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − 4''AC'' {{=}} 4(''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC'')}}，为简单起见，去掉了因子4。&lt;br /&gt;
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# {{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC'' &amp;lt; 0}} (''[[elliptic partial differential equation]]''): Solutions of [[elliptic partial differential equation|elliptic PDEs]] are as smooth as the coefficients allow, within the interior of the region where the equation and solutions are defined. For example, solutions of [[Laplace's equation]] are analytic within the domain where they are defined, but solutions may assume boundary values that are not smooth. The motion of a fluid at subsonic speeds can be approximated with elliptic PDEs, and the Euler–Tricomi equation is elliptic where {{math|''x'' &amp;lt; 0}}.&lt;br /&gt;
&lt;br /&gt;
  (elliptic partial differential equation): Solutions of elliptic PDEs are as smooth as the coefficients allow, within the interior of the region where the equation and solutions are defined. For example, solutions of Laplace's equation are analytic within the domain where they are defined, but solutions may assume boundary values that are not smooth. The motion of a fluid at subsonic speeds can be approximated with elliptic PDEs, and the Euler–Tricomi equation is elliptic where .&lt;br /&gt;
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{{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC'' &amp;lt; 0}} (椭圆形微分方程)：在定义方程和解的区域内部，椭圆型偏微分方程的解光滑到系数允许的程度。例如，拉普拉斯方程的解在它们被定义的区域内是解析的，但是解可能假设边界值是不光滑的。亚音速流体的运动可以用椭圆偏微分方程近似，其中欧拉-特里科米方程在 {{math|''x'' &amp;lt; 0}} 时是椭圆型偏微分方程。&lt;br /&gt;
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# {{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC'' {{=}} 0}} (''[[parabolic partial differential equation]]''): Equations that are [[parabolic partial differential equation|parabolic]] at every point can be transformed into a form analogous to the [[heat equation]] by a change of independent variables. Solutions smooth out as the transformed time variable increases. The Euler–Tricomi equation has parabolic type on the line where {{math|''x'' {{=}} 0}}.&lt;br /&gt;
&lt;br /&gt;
  0}} (parabolic partial differential equation): Equations that are parabolic at every point can be transformed into a form analogous to the heat equation by a change of independent variables. Solutions smooth out as the transformed time variable increases. The Euler–Tricomi equation has parabolic type on the line where  0}}.&lt;br /&gt;
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{{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC'' {{=}} 0}}（抛物线形偏微分方程）：在每一点上都是抛物线型的方程可以通过改变自变量从而转化成类似于热方程的形式。随着转换后的时间变量的增加，方程的解变得平滑。欧拉-特里科米方程在 {{math|''x'' {{=}} 0}} 这条特征线上是抛物线形的。&lt;br /&gt;
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# {{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC'' &amp;gt; 0}} (''[[hyperbolic partial differential equation]]''): [[hyperbolic partial differential equation|hyperbolic]] equations retain any discontinuities of functions or derivatives in the initial data. An example is the [[wave equation]]. The motion of a fluid at supersonic speeds can be approximated with hyperbolic PDEs, and the Euler–Tricomi equation is hyperbolic where {{math|''x'' &amp;gt; 0}}.&lt;br /&gt;
&lt;br /&gt;
  (hyperbolic partial differential equation): hyperbolic equations retain any discontinuities of functions or derivatives in the initial data. An example is the wave equation. The motion of a fluid at supersonic speeds can be approximated with hyperbolic PDEs, and the Euler–Tricomi equation is hyperbolic where .&lt;br /&gt;
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{{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC'' &amp;gt; 0}} (双曲形偏微分方程)：双曲形方程在初始数据中保留了函数或导数的任何不连续性，波动方程就是其中的一个例子。超音速流体的运动可以用双曲形偏微分方程近似，其中欧拉-特里科米方程在 {{math|''x'' &amp;gt; 0}} 时是双曲型的。&lt;br /&gt;
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If there are {{mvar|n}} independent variables {{math|''x''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;, ''x''&amp;lt;sub&amp;gt;2 &amp;lt;/sub&amp;gt;,… ''x''&amp;lt;sub&amp;gt;''n''&amp;lt;/sub&amp;gt;}}, a general linear partial differential equation of second order has the form&lt;br /&gt;
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If there are  independent variables , a general linear partial differential equation of second order has the form&lt;br /&gt;
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如果存在 {{mvar|n}} 个自变量 {{math|''x''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;, ''x''&amp;lt;sub&amp;gt;2 &amp;lt;/sub&amp;gt;,… ''x''&amp;lt;sub&amp;gt;''n''&amp;lt;/sub&amp;gt;}}，一般二阶线性偏微分方程的形式是&lt;br /&gt;
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: &amp;lt;math&amp;gt;L u =\sum_{i=1}^n\sum_{j=1}^n a_{i,j} \frac{\partial^2 u}{\partial x_i \partial x_j} \quad \text{ plus lower-order terms} =0.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;L u =\sum_{i=1}^n\sum_{j=1}^n a_{i,j} \frac{\partial^2 u}{\partial x_i \partial x_j} \quad \text{ plus lower-order terms} =0.&amp;lt;/math&amp;gt;&lt;br /&gt;
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The classification depends upon the signature of the eigenvalues of the coefficient matrix {{math|''a''&amp;lt;sub&amp;gt;''i'',''j''&amp;lt;/sub&amp;gt;}}.&lt;br /&gt;
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The classification depends upon the signature of the eigenvalues of the coefficient matrix .&lt;br /&gt;
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这种分类取决于系数矩阵本征值的符号（正负性）。&lt;br /&gt;
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# Elliptic: the eigenvalues are all positive or all negative.&lt;br /&gt;
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 Elliptic: the eigenvalues are all positive or all negative.&lt;br /&gt;
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椭圆形方程: 本征值全部为正或全部为负。&lt;br /&gt;
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# Parabolic: the eigenvalues are all positive or all negative, save one that is zero.&lt;br /&gt;
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 Parabolic: the eigenvalues are all positive or all negative, save one that is zero.&lt;br /&gt;
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抛物线形方程: 本征值全部为正或全部为负，除了一个为零。&lt;br /&gt;
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# Hyperbolic: there is only one negative eigenvalue and all the rest are positive, or there is only one positive eigenvalue and all the rest are negative.&lt;br /&gt;
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 Hyperbolic: there is only one negative eigenvalue and all the rest are positive, or there is only one positive eigenvalue and all the rest are negative.&lt;br /&gt;
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双曲形方程: 只有一个负特征值，其余的都是正特征值，或者只有一个正特征值，其余的都是负特征值。&lt;br /&gt;
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# Ultrahyperbolic: there is more than one positive eigenvalue and more than one negative eigenvalue, and there are no zero eigenvalues. There is only a limited theory for ultrahyperbolic equations (Courant and Hilbert, 1962).&lt;br /&gt;
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 Ultrahyperbolic: there is more than one positive eigenvalue and more than one negative eigenvalue, and there are no zero eigenvalues. There is only a limited theory for ultrahyperbolic equations (Courant and Hilbert, 1962).&lt;br /&gt;
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超双形方程: 存在多于一个正本征值和多于一个的负本征值，且不存在零本征值。对于超双曲方程，只存在一个有限理论(Courant 和 Hilbert，1962)。&lt;br /&gt;
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==[[用户:Yuling|Yuling]]（[[用户讨论:Yuling|讨论]]） 我对于limited theory这个单词对应的相关理论不太了解。&lt;br /&gt;
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=== Systems of first-order equations and characteristic surfaces ===&lt;br /&gt;
一阶方程组和特征曲面&lt;br /&gt;
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The classification of partial differential equations can be extended to systems of first-order equations, where the unknown {{mvar|u}} is now a [[Euclidean vector|vector]] with {{mvar|m}} components, and the coefficient matrices {{mvar|A&amp;lt;sub&amp;gt;ν&amp;lt;/sub&amp;gt;}} are {{mvar|m}} by {{mvar|m}} matrices for {{math|''ν'' {{=}} 1, 2,… ''n''}}. The partial differential equation takes the form&lt;br /&gt;
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The classification of partial differential equations can be extended to systems of first-order equations, where the unknown  is now a vector with  components, and the coefficient matrices  are  by  matrices for  1, 2,… n}}. The partial differential equation takes the form&lt;br /&gt;
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偏微分方程组的分类可以推广到一阶方程组，其中未知量 {{mvar|u}} 是有 {{mvar|m}} 个分量的向量。对于 {{math|''ν'' {{=}} 1, 2,… ''n''}}，系数矩阵 {{mvar|A&amp;lt;sub&amp;gt;ν&amp;lt;/sub&amp;gt;}} 是 {{mvar|m}} × {{mvar|m}} 的矩阵。偏微分方程形式如下：&lt;br /&gt;
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: &amp;lt;math&amp;gt;Lu = \sum_{\nu=1}^{n} A_\nu \frac{\partial u}{\partial x_\nu} + B=0,&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;Lu = \sum_{\nu=1}^{n} A_\nu \frac{\partial u}{\partial x_\nu} + B=0,&amp;lt;/math&amp;gt;&lt;br /&gt;
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where the coefficient matrices {{mvar|A&amp;lt;sub&amp;gt;ν&amp;lt;/sub&amp;gt;}} and the vector {{mvar|B}} may depend upon {{mvar|x}} and {{mvar|u}}. If a [[hypersurface]] {{mvar|S}} is given in the implicit form&lt;br /&gt;
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where the coefficient matrices  and the vector  may depend upon  and . If a hypersurface  is given in the implicit form&lt;br /&gt;
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其中系数矩阵 {{mvar|A&amp;lt;sub&amp;gt;ν&amp;lt;/sub&amp;gt;}} 和向量 {{mvar|B}} 可能依赖于 {{mvar|x}} 和 {{mvar|u}}。如果超曲面是以隐式形式给出的&lt;br /&gt;
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: &amp;lt;math&amp;gt;\varphi(x_1, x_2, \ldots x_n)=0,&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;\varphi(x_1, x_2, \ldots x_n)=0,&amp;lt;/math&amp;gt;&lt;br /&gt;
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where {{mvar|φ}} has a non-zero gradient, then {{mvar|S}} is a '''characteristic surface''' for the operator {{mvar|L}} at a given point if the characteristic form vanishes:&lt;br /&gt;
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where  has a non-zero gradient, then  is a characteristic surface for the operator  at a given point if the characteristic form vanishes:&lt;br /&gt;
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其中存在一个非零的梯度，那么如果特征形式消失，则在给定点上算子的特征曲面形式如下:&lt;br /&gt;
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: &amp;lt;math&amp;gt;Q\left(\frac{\partial\varphi}{\partial x_1}, \ldots\frac{\partial\varphi}{\partial x_n}\right) =\det\left[\sum_{\nu=1}^nA_\nu \frac{\partial \varphi}{\partial x_\nu}\right]=0.\,&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;Q\left(\frac{\partial\varphi}{\partial x_1}, \ldots\frac{\partial\varphi}{\partial x_n}\right) =\det\left[\sum_{\nu=1}^nA_\nu \frac{\partial \varphi}{\partial x_\nu}\right]=0.\,&amp;lt;/math&amp;gt;&lt;br /&gt;
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The geometric interpretation of this condition is as follows: if data for {{mvar|u}} are prescribed on the surface {{mvar|S}}, then it may be possible to determine the normal derivative of {{mvar|u}} on {{mvar|S}} from the differential equation. If the data on {{mvar|S}} and the differential equation determine the normal derivative of {{mvar|u}} on {{mvar|S}}, then {{mvar|S}} is non-characteristic. If the data on {{mvar|S}} and the differential equation ''do not'' determine the normal derivative of {{mvar|u}} on {{mvar|S}}, then the surface is '''characteristic''', and the differential equation restricts the data on {{mvar|S}}: the differential equation is ''internal'' to {{mvar|S}}.&lt;br /&gt;
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The geometric interpretation of this condition is as follows: if data for  are prescribed on the surface , then it may be possible to determine the normal derivative of  on  from the differential equation. If the data on  and the differential equation determine the normal derivative of  on , then  is non-characteristic. If the data on  and the differential equation do not determine the normal derivative of  on , then the surface is characteristic, and the differential equation restricts the data on : the differential equation is internal to .&lt;br /&gt;
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这个条件的几何解释如下: 如果关于 {{mvar|u}} 的数据是在曲面 {{mvar|S}} 上规定的，那么就有可能依据微分方程确定曲面 {{mvar|S}} 上 {{mvar|u}} 的法向导数。如果曲面 {{mvar|S}} 上的数据和上面的微分方程能确定曲面 {{mvar|S}} 上 {{mvar|u}} 的法向导数，那么它就是非特征的。如果曲面 {{mvar|S}} 上的数据和上面的微分方程不能确定曲面 {{mvar|S}} 上 {{mvar|u}} 的法向导数，那么曲面是特征的，并且微分方程将数据限制在曲面 {{mvar|S}} 上：微分方程是在曲面 {{mvar|S}} 内部。&lt;br /&gt;
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# A first-order system {{math|''Lu'' {{=}} 0}} is ''elliptic'' if no surface is characteristic for {{mvar|L}}: the values of {{mvar|u}} on {{mvar|S}} and the differential equation always determine the normal derivative of {{mvar|u}} on {{mvar|S}}.&lt;br /&gt;
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 A first-order system  0}} is elliptic if no surface is characteristic for : the values of  on  and the differential equation always determine the normal derivative of  on .&lt;br /&gt;
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如果对于 {{mvar|L}} 没有曲面是特征的，则一阶系统 {{math|''Lu'' {{=}} 0}} 是椭圆形的：{{mvar|u}}在 {{mvar|S}} 的值和微分方程总能够决定 {{mvar|S}} 上 {{mvar|u}} 的法向导数。&lt;br /&gt;
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# A first-order system is ''hyperbolic'' at a point if there is a '''spacelike''' surface {{mvar|S}} with normal {{mvar|ξ}} at that point. This means that, given any non-trivial vector {{mvar|η}} orthogonal to {{mvar|ξ}}, and a scalar multiplier {{mvar|λ}}, the equation {{math|''Q''(''λξ'' + ''η'') {{=}} 0}} has {{mvar|m}} real roots {{math|''λ''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;, ''λ''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;,… ''λ''&amp;lt;sub&amp;gt;''m''&amp;lt;/sub&amp;gt;}}. The system is '''strictly hyperbolic''' if these roots are always distinct. The geometrical interpretation of this condition is as follows: the characteristic form {{math|''Q''(''ζ'') {{=}} 0}} defines a cone (the normal cone) with homogeneous coordinates ζ. In the hyperbolic case, this cone has {{mvar|m}} sheets, and the axis {{math|''ζ'' {{=}} ''λξ''}} runs inside these sheets: it does not intersect any of them. But when displaced from the origin by η, this axis intersects every sheet. In the elliptic case, the normal cone has no real sheets.&lt;br /&gt;
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 A first-order system is hyperbolic at a point if there is a spacelike surface  with normal  at that point. This means that, given any non-trivial vector  orthogonal to , and a scalar multiplier , the equation  0}} has  real roots . The system is strictly hyperbolic if these roots are always distinct. The geometrical interpretation of this condition is as follows: the characteristic form  0}} defines a cone (the normal cone) with homogeneous coordinates ζ. In the hyperbolic case, this cone has  sheets, and the axis  λξ}} runs inside these sheets: it does not intersect any of them. But when displaced from the origin by η, this axis intersects every sheet. In the elliptic case, the normal cone has no real sheets.&lt;br /&gt;
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如果在该点存在一个法向量为 {{mvar|ξ}}的 '''&amp;lt;font color=&amp;quot;#ff8000&amp;quot;&amp;gt;类空曲面 Spacclike Surface&amp;lt;/font&amp;gt; {{mvar|S}} ，则一阶系统在那一点是双曲的。这意味着，给定任意正交于 {{mvar|ξ}} 的非平凡向量 {{mvar|η}} 和一个标量乘子 {{mvar|λ}}，方程 {{math|''Q''(''λξ'' + ''η'') {{=}} 0}} 有 {{mvar|m}} 个实根 {{math|''λ''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;, ''λ''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;,… ''λ''&amp;lt;sub&amp;gt;''m''&amp;lt;/sub&amp;gt;}}。如果这些根始终不同，则该系统是严格双曲形的。这个条件的几何解释如下: 特征形式 {{math|''Q''(''ζ'') {{=}} 0}} 定义了一个具有齐次坐标 ζ的圆锥(法线圆锥)。在双曲形的情况下，这个圆锥体有 {{mvar|m}} 层，并且轴 {{math|''ζ'' {{=}} ''λξ''}} 在这些层中运动: 它不与任何一层相交。但是当从原点偏离η时，这条轴线与每一层都相交。在椭圆形的情况下，法向圆锥没有实层。&lt;br /&gt;
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==[[用户:Yuling|Yuling]]（[[用户讨论:Yuling|讨论]]） sheet 这个单词也不很理解，我直译为了“层”&lt;br /&gt;
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=== Equations of mixed type ===&lt;br /&gt;
混合型方程&lt;br /&gt;
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If a PDE has coefficients that are not constant, it is possible that it will not belong to any of these categories but rather be of '''mixed type'''. A simple but important example is the [[Euler–Tricomi equation]]&lt;br /&gt;
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If a PDE has coefficients that are not constant, it is possible that it will not belong to any of these categories but rather be of mixed type. A simple but important example is the Euler–Tricomi equation&lt;br /&gt;
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如果偏微分方程的系数不是常数，那么它可能不属于这些类别中的任何一个，而是属于混合类型。一个简单但重要的例子是欧拉-特里科米方程&lt;br /&gt;
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: &amp;lt;math&amp;gt;u_{xx} = xu_{yy},&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;u_{xx} = xu_{yy},&amp;lt;/math&amp;gt;&lt;br /&gt;
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which is called '''elliptic-hyperbolic''' because it is elliptic in the region {{math|''x'' &amp;lt; 0}}, hyperbolic in the region {{math|''x'' &amp;gt; 0}}, and degenerate parabolic on the line {{math|''x'' {{=}} 0}}.&lt;br /&gt;
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which is called elliptic-hyperbolic because it is elliptic in the region , hyperbolic in the region , and degenerate parabolic on the line  0}}.&lt;br /&gt;
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它在 {{math|''x'' &amp;lt; 0}} 的区域上是椭圆形，在 {{math|''x'' &amp;gt; 0}} 区域上是双曲形，在 {{math|''x'' {{=}} 0}}这条线上是退化为抛物线形，因此称之为椭圆-双曲型。&lt;br /&gt;
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''fill in: Dirichlet and Neumann boundaries, hyperbolic/parabolic/elliptic separation of variables, [[Fourier analysis]], [[Green's function]]s ...--&amp;gt;&lt;br /&gt;
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fill in: Dirichlet and Neumann boundaries, hyperbolic/parabolic/elliptic separation of variables, Fourier analysis, Green's functions ...--&amp;gt;&lt;br /&gt;
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填写: Dirichlet 和 Neumann 边界，双曲 / 抛物线 / 椭圆分离变量法，傅立叶分析，Green 函数... --&lt;br /&gt;
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=== Infinite-order PDEs in quantum mechanics ===&lt;br /&gt;
量子力学中的无限阶偏微分方程&lt;br /&gt;
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In the [[phase space formulation]] of quantum mechanics,  one may consider the [[Method of quantum characteristics|quantum Hamilton's equations]] for trajectories of quantum particles. These equations are infinite-order PDEs. However, in the semiclassical expansion, one has a finite system of ODEs at any fixed order of [[Dirac constant|{{mvar|ħ}}]].  The evolution equation of the [[Wigner quasi-probability distribution|c]] is also an infinite-order PDE. The quantum trajectories are [[Method of quantum characteristics|quantum characteristics]], with the use of which one could calculate the evolution of the Wigner function.&lt;br /&gt;
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In the phase space formulation of quantum mechanics,  one may consider the quantum Hamilton's equations for trajectories of quantum particles. These equations are infinite-order PDEs. However, in the semiclassical expansion, one has a finite system of ODEs at any fixed order of Dirac constant|.  The evolution equation of the Wigner function is also an infinite-order PDE. The quantum trajectories are quantum characteristics, with the use of which one could calculate the evolution of the Wigner function.&lt;br /&gt;
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在量子力学中的相空间表述中，我们可以考虑用于求解量子粒子的轨迹的量子哈密顿的方程。这些方程是无限阶偏微分方程。然而，在半经典展开中，我们在给定[[Dirac constant|{{mvar|ħ}}]]阶数下有一个有限的的常微分方程组。'''&amp;lt;font color=&amp;quot;#ff8000&amp;quot;&amp;gt;维格纳函数  Wigner Function&amp;lt;/font&amp;gt;的演化方程也是一个无限阶偏微分方程。由于量子轨道的量子特性，所以它通常可以用来计算维格纳函数的演化。&lt;br /&gt;
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== Analytical solutions ==&lt;br /&gt;
解析解&lt;br /&gt;
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===Separation of variables===&lt;br /&gt;
分离变量法&lt;br /&gt;
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{{main|Separable partial differential equation}}&lt;br /&gt;
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Linear PDEs can be reduced to systems of ordinary differential equations by the important technique of separation of variables. This technique rests on a characteristic of solutions to differential equations: if one can find any solution that solves the equation and satisfies the boundary conditions, then it is ''the'' solution (this also applies to ODEs). We assume as an [[ansatz]] that the dependence of a solution on the parameters space and time can be written as a product of terms that each depend on a single parameter, and then see if this can be made to solve the problem.&amp;lt;ref&amp;gt;{{cite book|last1=Gershenfeld|first1=Neil|title=The nature of mathematical modeling|date=2000|publisher=Cambridge Univ. Press|location=Cambridge|isbn=0521570956|page=27|edition=Reprinted (with corr.)}}&amp;lt;/ref&amp;gt;&lt;br /&gt;
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Linear PDEs can be reduced to systems of ordinary differential equations by the important technique of separation of variables. This technique rests on a characteristic of solutions to differential equations: if one can find any solution that solves the equation and satisfies the boundary conditions, then it is the solution (this also applies to ODEs). We assume as an ansatz that the dependence of a solution on the parameters space and time can be written as a product of terms that each depend on a single parameter, and then see if this can be made to solve the problem.&lt;br /&gt;
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线性偏微分方程组可以通过分离变量法这一重要方法来简化为常微分方程组。这种方法依赖于微分方程解的一个特征: 如果能找到任何一个满足方程和边界条件的解，那么这个解就是方程的解(这也适用于常微分方程)。我们假设解对参数空间和时间的依赖可以写成对它们每一项的依赖以及一个参数的乘积，然后再看看这是否可以用来解决这个问题。&lt;br /&gt;
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In the method of separation of variables, one reduces a PDE to a PDE in fewer variables, which is an ordinary differential equation if in one variable – these are in turn easier to solve.&lt;br /&gt;
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In the method of separation of variables, one reduces a PDE to a PDE in fewer variables, which is an ordinary differential equation if in one variable – these are in turn easier to solve.&lt;br /&gt;
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在分离变量法方法中，可以将偏微分方程简化为含有更少变量的偏微分方程，如果只有一个变量，那么就变成了一个'''&amp;lt;font color = &amp;quot;#ff8000&amp;quot;&amp;gt;常微分方程 Ordinary Differential Equation&amp;lt;/font&amp;gt;'''-- 反过来，这些方程也更容易求解。&lt;br /&gt;
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This is possible for simple PDEs, which are called [[separable partial differential equation]]s, and the domain is generally a rectangle (a product of intervals). Separable PDEs correspond to [[diagonal matrices]] – thinking of &amp;quot;the value for fixed {{mvar|x}}&amp;quot; as a coordinate, each coordinate can be understood separately.&lt;br /&gt;
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This is possible for simple PDEs, which are called separable partial differential equations, and the domain is generally a rectangle (a product of intervals). Separable PDEs correspond to diagonal matrices – thinking of &amp;quot;the value for fixed &amp;quot; as a coordinate, each coordinate can be understood separately.&lt;br /&gt;
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对于简单的偏微分方程(称为可分离偏微分方程)来说，这是可能的，而且方程通常定义在一个矩形区域(区间的乘积)上。可分离偏微分方程对应于对角线矩阵——以“固定值”为坐标，每个坐标可分开理解。&lt;br /&gt;
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This generalizes to the [[method of characteristics]], and is also used in [[integral transform]]s.&lt;br /&gt;
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This generalizes to the method of characteristics, and is also used in integral transforms.&lt;br /&gt;
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这种方法可以推广到特征曲线法，也可以用于积分变换。&lt;br /&gt;
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===Method of characteristics===&lt;br /&gt;
特征曲线法&lt;br /&gt;
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{{main|Method of characteristics}}&lt;br /&gt;
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In special cases, one can find characteristic curves on which the equation reduces to an ODE – changing coordinates in the domain to straighten these curves allows separation of variables, and is called the [[method of characteristics]].&lt;br /&gt;
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In special cases, one can find characteristic curves on which the equation reduces to an ODE – changing coordinates in the domain to straighten these curves allows separation of variables, and is called the method of characteristics.&lt;br /&gt;
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在特殊情况下，可以找到一些特征曲线，在这些曲线上方程可以变成一个常微分方程——意味着改变坐标从而使这些曲线变直从而达到分离变量的目的，这就是所谓的特征曲线法。&lt;br /&gt;
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More generally, one may find characteristic surfaces.&lt;br /&gt;
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More generally, one may find characteristic surfaces.&lt;br /&gt;
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更一般地说，人们可能会找到特征表面。&lt;br /&gt;
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===Integral transform===&lt;br /&gt;
积分变换&lt;br /&gt;
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An [[integral transform]] may transform the PDE to a simpler one, in particular, a separable PDE. This corresponds to diagonalizing an operator.&lt;br /&gt;
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An integral transform may transform the PDE to a simpler one, in particular, a separable PDE. This corresponds to diagonalizing an operator.&lt;br /&gt;
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积分变换可以将偏微分方程转换为更简单的偏微分方程，特别是可分离的偏微分方程。这对应于对角化算符。&lt;br /&gt;
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An important example of this is [[Fourier analysis]], which diagonalizes the heat equation using the [[eigenbasis]] of sinusoidal waves.&lt;br /&gt;
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An important example of this is Fourier analysis, which diagonalizes the heat equation using the eigenbasis of sinusoidal waves.&lt;br /&gt;
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这方面的一个重要例子是'''&amp;lt;font color = &amp;quot;#ff8000&amp;quot;&amp;gt;傅里叶分析  Fourier Analysis&amp;lt;/font&amp;gt;'''，它使用正弦波的特征基来对角化热方程。&lt;br /&gt;
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If the domain is finite or periodic, an infinite sum of solutions such as a [[Fourier series]] is appropriate, but an integral of solutions such as a [[Fourier integral]] is generally required for infinite domains. The solution for a point source for the heat equation given above is an example of the use of a Fourier integral.&lt;br /&gt;
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If the domain is finite or periodic, an infinite sum of solutions such as a Fourier series is appropriate, but an integral of solutions such as a Fourier integral is generally required for infinite domains. The solution for a point source for the heat equation given above is an example of the use of a Fourier integral.&lt;br /&gt;
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如果区域是有限的或周期性的，那么解为无限和的形式是恰当的，例如傅里叶级数，但是一个解的积分，例如傅立叶积分，一般是在无限区域上的。上面给出的热传导方程的点源解法就是使用傅里叶积分的一个例子。&lt;br /&gt;
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===Change of variables===&lt;br /&gt;
变量代换&lt;br /&gt;
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Often a PDE can be reduced to a simpler form with a known solution by a suitable [[Change of variables (PDE)|change of variables]].  For example, the [[Black–Scholes equation#Derivation|Black–Scholes]] PDE&lt;br /&gt;
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Often a PDE can be reduced to a simpler form with a known solution by a suitable change of variables.  For example, the Black–Scholes PDE&lt;br /&gt;
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偏微分方程通常可以通过变量的适当变化，用已知的解简化为更简单的形式。例如，布莱克-舒尔斯偏微分方程&lt;br /&gt;
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:&amp;lt;math&amp;gt; \frac{\partial V}{\partial t} + \tfrac{1}{2}\sigma^2 S^2\frac{\partial^2 V}{\partial S^2} + rS\frac{\partial V}{\partial S} - rV = 0 &amp;lt;/math&amp;gt;&lt;br /&gt;
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&amp;lt;math&amp;gt; \frac{\partial V}{\partial t} + \tfrac{1}{2}\sigma^2 S^2\frac{\partial^2 V}{\partial S^2} + rS\frac{\partial V}{\partial S} - rV = 0 &amp;lt;/math&amp;gt;&lt;br /&gt;
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is reducible to the [[heat equation]]&lt;br /&gt;
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is reducible to the heat equation&lt;br /&gt;
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可以简化为热传导方程&lt;br /&gt;
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:&amp;lt;math&amp;gt; \frac{\partial u}{\partial \tau} = \frac{\partial^2 u}{\partial x^2}&amp;lt;/math&amp;gt;&lt;br /&gt;
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&amp;lt;math&amp;gt; \frac{\partial u}{\partial \tau} = \frac{\partial^2 u}{\partial x^2}&amp;lt;/math&amp;gt;&lt;br /&gt;
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by the change of variables (for complete details see {{webarchive |url=https://web.archive.org/web/20080411030405/http://www.math.unl.edu/~sdunbar1/Teaching/MathematicalFinance/Lessons/BlackScholes/Solution/solution.shtml |date=April 11, 2008 |title=Solution of the Black Scholes Equation }})&lt;br /&gt;
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by the change of variables (for complete details see )&lt;br /&gt;
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通过变量替换(完整的细节见)&lt;br /&gt;
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:&amp;lt;math&amp;gt;\begin{align}&lt;br /&gt;
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V(S,t) &amp;amp;= K v(x,\tau),\\[5px]&lt;br /&gt;
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x &amp;amp;= \ln\left(\tfrac{S}{K} \right),\\[5px]&lt;br /&gt;
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\tau &amp;amp;= \tfrac{1}{2} \sigma^2 (T - t),\\[5px]&lt;br /&gt;
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v(x,\tau)&amp;amp;=e^{-\alpha x-\beta\tau} u(x,\tau).&lt;br /&gt;
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\end{align}&amp;lt;/math&amp;gt;&lt;br /&gt;
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===Fundamental solution===&lt;br /&gt;
基本解&lt;br /&gt;
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{{main|Fundamental solution}}&lt;br /&gt;
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Inhomogeneous equations can often be solved (for constant coefficient PDEs, always be solved) by finding the [[fundamental solution]] (the solution for a point source), then taking the [[convolution]] with the boundary conditions to get the solution.&lt;br /&gt;
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Inhomogeneous equations can often be solved (for constant coefficient PDEs, always be solved) by finding the fundamental solution (the solution for a point source), then taking the convolution with the boundary conditions to get the solution.&lt;br /&gt;
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非齐次方程(常系数偏微分方程)一般是通过先求出基本解(点源的解) ，然后利用带边界条件的卷积来求解。&lt;br /&gt;
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This is analogous in [[signal processing]] to understanding a filter by its [[impulse response]].&lt;br /&gt;
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This is analogous in signal processing to understanding a filter by its impulse response.&lt;br /&gt;
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这类似于在信号处理中通过滤波器的脉冲响应来理解滤波器。&lt;br /&gt;
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===Superposition principle===&lt;br /&gt;
叠加原理&lt;br /&gt;
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{{further| Superposition principle }}&lt;br /&gt;
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The superposition principle applies to any linear system, including linear systems of PDEs. A common visualization of this concept is the interaction of two waves in phase being combined to result in a greater amplitude, for example {{math|sin ''x'' + sin ''x'' {{=}} 2 sin ''x''}}. The same principle can be observed in PDEs where the solutions may be real or complex and additive. [[Superposition principle|superposition]]&lt;br /&gt;
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The superposition principle applies to any linear system, including linear systems of PDEs. A common visualization of this concept is the interaction of two waves in phase being combined to result in a greater amplitude, for example  2 sin x}}. The same principle can be observed in PDEs where the solutions may be real or complex and additive. superposition&lt;br /&gt;
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'''&amp;lt;font color = &amp;quot;#ff8000&amp;quot;&amp;gt;叠加原理 Superposition Principle&amp;lt;/font&amp;gt;适用于任何线性系统，包括偏微分方程的线性系统。这个概念的一个常见的可视化是两个同相位的波相互作用结合在一起会产生更大的振幅，例如 {{math|sin ''x'' + sin ''x'' {{=}} 2 sin ''x''}}。在偏微分方程中也可以观察到同样的原理，其中的解可能是真实的或复杂的和可加的。叠加&lt;br /&gt;
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If {{math|''u''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;}} and {{math|''u''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;}} are solutions of linear PDE in some function space {{mvar|R}}, then {{math|''u'' {{=}} ''c''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;''u''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; + ''c''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;''u''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;}} with any constants {{math|''c''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;}} and {{math|''c''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;}} are also a solution of that PDE in the same function space.&lt;br /&gt;
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If  and  are solutions of linear PDE in some function space , then  c&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;u&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; + c&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;u&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;}} with any constants  and  are also a solution of that PDE in the same function space.&lt;br /&gt;
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若线性偏微分方程在某个函数空间{{mvar|R}}中有解{{math|''u''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;}} 和 {{math|''u''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;}}，则{{math|''u'' {{=}} ''c''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;''u''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; + ''c''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;''u''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;}}也是该偏微分方程在同一函数空间中的解，其中{{math|''c''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;}} 和 {{math|''c''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;}} 是任意常数。&lt;br /&gt;
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===Methods for non-linear equations===&lt;br /&gt;
非线性方程的求解方法&lt;br /&gt;
{{see also|nonlinear partial differential equation}}&lt;br /&gt;
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There are no generally applicable methods to solve nonlinear PDEs. Still, existence and uniqueness results (such as the [[Cauchy–Kowalevski theorem]]) are often possible, as are proofs of important qualitative and quantitative properties of solutions (getting these results is a major part of [[mathematical analysis|analysis]]). Computational solution to the nonlinear PDEs, the [[split-step method]], exist for specific equations like [[nonlinear Schrödinger equation]].&lt;br /&gt;
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There are no generally applicable methods to solve nonlinear PDEs. Still, existence and uniqueness results (such as the Cauchy–Kowalevski theorem) are often possible, as are proofs of important qualitative and quantitative properties of solutions (getting these results is a major part of analysis). Computational solution to the nonlinear PDEs, the split-step method, exist for specific equations like nonlinear Schrödinger equation.&lt;br /&gt;
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对于非线性偏微分方程，目前还没有普遍适用的求解方法。然而，通常是可能知道解的存在性和唯一性(如柯西-科瓦列夫斯基定理)，也是可能得到解的重要定性和定量性质的证明(得到这些结果是分析的主要部分)。非线性偏微分方程的计算解，即分步法，对一些特定的方程适用，比如非线性'''&amp;lt;font color=&amp;quot;#ff8000&amp;quot;&amp;gt;薛定谔方程 Schrödinger equation&amp;lt;/font&amp;gt;'''。&lt;br /&gt;
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Nevertheless, some techniques can be used for several types of equations. The [[h-principle|{{mvar|h}}-principle]] is the most powerful method to solve [[Underdetermined system|underdetermined]] equations. The [[Riquier–Janet theory]] is an effective method for obtaining information about many analytic [[Overdetermined system|overdetermined]] systems.&lt;br /&gt;
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Nevertheless, some techniques can be used for several types of equations. The -principle is the most powerful method to solve underdetermined equations. The Riquier–Janet theory is an effective method for obtaining information about many analytic overdetermined systems.&lt;br /&gt;
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然而，一些技巧可以用于几种类型的方程。h-原理是求解欠定方程最有效的方法。里基尔-珍妮特理论是一种可以获得许多解析超定系统信息的有效方法。&lt;br /&gt;
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The [[method of characteristics]] can be used in some very special cases to solve partial differential equations.&lt;br /&gt;
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The method of characteristics can be used in some very special cases to solve partial differential equations.&lt;br /&gt;
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特征线法可用于求解某些特殊情况下的偏微分方程。&lt;br /&gt;
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In some cases, a PDE can be solved via [[perturbation analysis]] in which the solution is considered to be a correction to an equation with a known solution. Alternatives are [[numerical analysis]] techniques from simple [[finite difference]] schemes to the more mature [[multigrid]] and [[finite element method]]s. Many interesting problems in science and engineering are solved in this way using [[computer]]s, sometimes high performance [[supercomputer]]s.&lt;br /&gt;
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In some cases, a PDE can be solved via perturbation analysis in which the solution is considered to be a correction to an equation with a known solution. Alternatives are numerical analysis techniques from simple finite difference schemes to the more mature multigrid and finite element methods. Many interesting problems in science and engineering are solved in this way using computers, sometimes high performance supercomputers.&lt;br /&gt;
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在某些情况下，偏微分方程可以通过扰动分析来求解。在扰动分析中，通常是求解将具有已知解的方程修正后的新得到方程。可供选择的数值分析技术从简单的差分格式到更成熟的多重网格和有限元方法。许多有趣的科学和工程问题都是在计算机上用这种方法解决的，有时是高性能超级计算机。&lt;br /&gt;
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===Lie group method===&lt;br /&gt;
李群方法&lt;br /&gt;
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From 1870 [[Sophus Lie]]'s work put the theory of differential equations on a more satisfactory foundation. He showed that the integration theories of the older mathematicians can, by the introduction of what are now called [[Lie group]]s, be referred, to a common source; and that ordinary differential equations which admit the same [[infinitesimal transformation]]s present comparable difficulties of integration. He also emphasized the subject of [[contact transformation|transformations of contact]].&lt;br /&gt;
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From 1870 Sophus Lie's work put the theory of differential equations on a more satisfactory foundation. He showed that the integration theories of the older mathematicians can, by the introduction of what are now called Lie groups, be referred, to a common source; and that ordinary differential equations which admit the same infinitesimal transformations present comparable difficulties of integration. He also emphasized the subject of transformations of contact.&lt;br /&gt;
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从1870年起，索弗斯·李的工作为微分方程理论奠定了一个较为令人满意的基础。他指出，通过引入现在所谓的李群，老一辈数学家的积分理论可以引用到一个共同的来源; 承认相同的无穷小变换的常微分方程在积分方面存在相当的困难。他还强调了接触的转变这一主题。&lt;br /&gt;
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==[[用户:Yuling|Yuling]]（[[用户讨论:Yuling|讨论]]）这句话“He also emphasized the subject of transformations of contact.”中的transformations of contact翻译的不太好。&lt;br /&gt;
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A general approach to solving PDEs uses the symmetry property of differential equations, the continuous [[infinitesimal transformation]]s of solutions to solutions ([[Lie theory]]). Continuous [[group theory]], [[Lie algebras]] and [[differential geometry]] are used to understand the structure of linear and nonlinear partial differential equations for generating integrable equations, to find its [[Lax pair]]s, recursion operators, [[Bäcklund transform]] and finally finding exact analytic solutions to the PDE.&lt;br /&gt;
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A general approach to solving PDEs uses the symmetry property of differential equations, the continuous infinitesimal transformations of solutions to solutions (Lie theory). Continuous group theory, Lie algebras and differential geometry are used to understand the structure of linear and nonlinear partial differential equations for generating integrable equations, to find its Lax pairs, recursion operators, Bäcklund transform and finally finding exact analytic solutions to the PDE.&lt;br /&gt;
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求解偏微分方程的一般方法是利用微分方程的对称性，即解到解的连续无穷小变换(李理论)。连续群论、李代数和微分几何理论被用来理解生成可积方程的线性和非线性偏微分方程的结构，找到它的Lax对、递归算子、 贝克伦德变换，最后找到偏微分方程的精确解析解。&lt;br /&gt;
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Symmetry methods have been recognized to study differential equations arising in mathematics, physics, engineering, and many other disciplines.&lt;br /&gt;
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Symmetry methods have been recognized to study differential equations arising in mathematics, physics, engineering, and many other disciplines.&lt;br /&gt;
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对称方法已被公认可以用于研究出现在数学，物理，工程和许多其他学科的微分方程。&lt;br /&gt;
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===Semianalytical methods===&lt;br /&gt;
半解析方法&lt;br /&gt;
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The [[Adomian decomposition method]], the [[Aleksandr Lyapunov|Lyapunov]] artificial small parameter method, and He's [[homotopy perturbation method]] are all special cases of the more general [[homotopy analysis method]]. These are series expansion methods, and except for the Lyapunov method, are independent of small physical parameters as compared to the well known [[perturbation theory]], thus giving these methods greater flexibility and solution generality.&lt;br /&gt;
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The Adomian decomposition method, the Lyapunov artificial small parameter method, and He's homotopy perturbation method are all special cases of the more general homotopy analysis method. These are series expansion methods, and except for the Lyapunov method, are independent of small physical parameters as compared to the well known perturbation theory, thus giving these methods greater flexibility and solution generality.&lt;br /&gt;
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阿多米安分解法、李雅普诺夫人工小参数方法和何同伦摄动方法都是更一般的同伦分析方法的特殊情况。除了李雅普诺夫方法之外，这些都是级数展开方法，与为人熟知的摄动理论方法相比，它们与小的物理参数无关，因此这些方法具有更大的灵活性和解的通用性。&lt;br /&gt;
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== Numerical solutions ==&lt;br /&gt;
数值解&lt;br /&gt;
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The three most widely used [[Numerical partial differential equations|numerical methods to solve PDEs]] are the [[finite element analysis|finite element method]] (FEM), [[finite volume method]]s (FVM) and [[finite difference method]]s (FDM), as well other kind of methods called [[Meshfree methods]], which were made to solve problems where the before mentioned methods are limited. The FEM has a prominent position among these methods and especially its exceptionally efficient higher-order version [[hp-FEM]]. Other hybrid versions of FEM and Meshfree methods include the generalized finite element method (GFEM), [[extended finite element method]] (XFEM), [[Spectral element method|spectral finite element method]] (SFEM), [[Meshfree methods|meshfree finite element method]], [[Discontinuous Galerkin Method|discontinuous Galerkin finite element method]] (DGFEM), [[Element-Free Galerkin Method]] (EFGM), [[Interpolating Element-Free Galerkin Method]] (IEFGM), etc.&lt;br /&gt;
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The three most widely used numerical methods to solve PDEs are the finite element method (FEM), finite volume methods (FVM) and finite difference methods (FDM), as well other kind of methods called Meshfree methods, which were made to solve problems where the before mentioned methods are limited. The FEM has a prominent position among these methods and especially its exceptionally efficient higher-order version hp-FEM. Other hybrid versions of FEM and Meshfree methods include the generalized finite element method (GFEM), extended finite element method (XFEM), spectral finite element method (SFEM), meshfree finite element method, discontinuous Galerkin finite element method (DGFEM), Element-Free Galerkin Method (EFGM), Interpolating Element-Free Galerkin Method (IEFGM), etc.&lt;br /&gt;
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求解偏微分方程最常用的三种数值方法是有限元分析法、有限体积法和有限差分法，以及其他一些称为无网格法的方法。这些方法用于解决前面提到的方法受到的限制。在这些方法中，有限元方法，尤其是高效的高阶有限元方法，占有重要地位。其他有限元法和无网格法的混合形式包括广义有限元分析法(GFEM)、扩展有限元分析法(XFEM)、谱有限元分析法(SFEM)、无网格有限元分析法(DGFEM)、间断伽辽金有限元分析法(DGFEM)、无网格伽辽金法(EFGM)、插值无网格伽辽金法(IEFGM)等。&lt;br /&gt;
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=== Finite element method ===&lt;br /&gt;
有限元分析法&lt;br /&gt;
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{{main|Finite element method}}&lt;br /&gt;
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The finite element method (FEM) (its practical application often known as finite element analysis (FEA)) is a numerical technique for finding approximate solutions of partial differential equations (PDE) as well as of integral equations. The solution approach is based either on eliminating the differential equation completely (steady state problems), or rendering the PDE into an approximating system of ordinary differential equations, which are then numerically integrated using standard techniques such as Euler's method, Runge–Kutta, etc.&lt;br /&gt;
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The finite element method (FEM) (its practical application often known as finite element analysis (FEA)) is a numerical technique for finding approximate solutions of partial differential equations (PDE) as well as of integral equations. The solution approach is based either on eliminating the differential equation completely (steady state problems), or rendering the PDE into an approximating system of ordinary differential equations, which are then numerically integrated using standard techniques such as Euler's method, Runge–Kutta, etc.&lt;br /&gt;
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'''&amp;lt;font color = &amp;quot;#ff8000&amp;quot;&amp;gt;有限元分析法 Finite Element Method&amp;lt;/font&amp;gt;''' ((其实际应用通常被称为有限元分析(FEA))是一种寻找偏微分方程(PDE)和积分方程近似解的数值技术。这种求解方法要么基于完全消除微分方程(稳态问题) ，要么将偏微分方程转化为常微分方程的近似系统，然后使用标准技术进行数值积分，如欧拉方法、 Runge-Kutta 等。&lt;br /&gt;
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===Finite difference method===&lt;br /&gt;
有限差分法&lt;br /&gt;
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{{main|Finite difference method}}&lt;br /&gt;
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Finite-difference methods are numerical methods for approximating the solutions to differential equations using [[finite difference]] equations to approximate derivatives.&lt;br /&gt;
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Finite-difference methods are numerical methods for approximating the solutions to differential equations using finite difference equations to approximate derivatives.&lt;br /&gt;
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有限差分法是一种数值方法，用差分方程近似微分方程的解。&lt;br /&gt;
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=== Finite volume method ===&lt;br /&gt;
有限体积法&lt;br /&gt;
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{{main|Finite volume method}}&lt;br /&gt;
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Similar to the finite difference method or finite element method, values are calculated at discrete places on a meshed geometry. &amp;quot;Finite volume&amp;quot; refers to the small volume surrounding each node point on a mesh. In the finite volume method, surface integrals in a partial differential equation that contain a divergence term are converted to volume integrals, using the [[divergence theorem]]. These terms are then evaluated as fluxes at the surfaces of each finite volume. Because the flux entering a given volume is identical to that leaving the adjacent volume, these methods conserve mass by design.&lt;br /&gt;
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Similar to the finite difference method or finite element method, values are calculated at discrete places on a meshed geometry. &amp;quot;Finite volume&amp;quot; refers to the small volume surrounding each node point on a mesh. In the finite volume method, surface integrals in a partial differential equation that contain a divergence term are converted to volume integrals, using the divergence theorem. These terms are then evaluated as fluxes at the surfaces of each finite volume. Because the flux entering a given volume is identical to that leaving the adjacent volume, these methods conserve mass by design.&lt;br /&gt;
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类似于有限差分法或有限元分析，函数值是在网状几何体上的离散位置进行计算的。“有限体积”是指网格上每个节点周围的小体积。在有限体积法中，偏微分方程中含有散度项的面积分用散度定理积分转换成体积分。然后将这些项用于估算每个有限体积表面上的通量。由于进入给定体积的通量与转移到相邻体积元的通量相同，所以这些方法在设计上保证了质量守恒。&lt;br /&gt;
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==See also==&lt;br /&gt;
请参阅&lt;br /&gt;
* [[Dirichlet boundary condition]]&lt;br /&gt;
狄利克雷边界条件&lt;br /&gt;
* [[Jet bundle]]&lt;br /&gt;
射流丛&lt;br /&gt;
* [[Laplace transform applied to differential equations]]&lt;br /&gt;
微分方程中的拉普拉斯变换&lt;br /&gt;
* [[List of dynamical systems and differential equations topics]]&lt;br /&gt;
动力学系统和微分方程的列表&lt;br /&gt;
* [[Matrix differential equation]]&lt;br /&gt;
矩阵微分方程&lt;br /&gt;
* [[Neumann boundary condition]]&lt;br /&gt;
诺伊曼边界条件&lt;br /&gt;
* [[Numerical partial differential equations]]&lt;br /&gt;
数值偏微分方程&lt;br /&gt;
* [[Partial differential algebraic equation]]&lt;br /&gt;
偏微分代数方程&lt;br /&gt;
* [[Recurrence relation]]&lt;br /&gt;
递推关系&lt;br /&gt;
* [[Robin boundary condition]]&lt;br /&gt;
罗宾边界条件&lt;br /&gt;
* [[Stochastic processes and boundary value problems]]&lt;br /&gt;
随机过程和边值问题&lt;br /&gt;
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== The energy method ==&lt;br /&gt;
能量法&lt;br /&gt;
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The energy method is a mathematical procedure that can be used to verify well-posedness of initial-boundary-value-problems.&amp;lt;ref&amp;gt;{{cite book |title=High Order Difference Methods for Time Dependent PDE&lt;br /&gt;
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The energy method is a mathematical procedure that can be used to verify well-posedness of initial-boundary-value-problems.&amp;lt;ref&amp;gt;{{cite book |title=High Order Difference Methods for Time Dependent PDE&lt;br /&gt;
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能量法是验证初边值问题适定性的一种数学方法。 时变偏微分方程的高阶差分方法&lt;br /&gt;
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|first=Bertil|last=Gustafsson|publisher=Springer|year=2008|isbn=978-3-540-74992-9|doi=10.1007/978-3-540-74993-6}}&amp;lt;/ref&amp;gt; In the following example the energy method is used to decide where and which boundary conditions should be imposed such that the resulting IBVP is well-posed. Consider the one-dimensional hyperbolic PDE given by&lt;br /&gt;
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|first=Bertil|last=Gustafsson|publisher=Springer|year=2008|isbn=978-3-540-74992-9|doi=10.1007/978-3-540-74993-6}}&amp;lt;/ref&amp;gt; In the following example the energy method is used to decide where and which boundary conditions should be imposed such that the resulting IBVP is well-posed. Consider the one-dimensional hyperbolic PDE given by&lt;br /&gt;
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| first Bertil | last Gustafsson | publisher | Springer | year 2008 | isbn 978-3-540-74992-9 | doi 10.1007 / 978-3-540-74993-6} / ref 在下面的例子中，使用能量方法来决定应该施加哪些边界条件，使得得到的 IBVP适定。考虑一维双曲偏微分方程&lt;br /&gt;
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: &amp;lt;math&amp;gt;\frac{\partial u}{\partial t} + \alpha \frac{\partial u}{\partial x} = 0, \quad x \in [a,b], \operatorname t &amp;gt; 0,&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;\frac{\partial u}{\partial t} + \alpha \frac{\partial u}{\partial x} = 0, \quad x \in [a,b], \operatorname t &amp;gt; 0,&amp;lt;/math&amp;gt;&lt;br /&gt;
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where &amp;lt;math&amp;gt;\alpha \neq 0&amp;lt;/math&amp;gt; is a constant and &amp;lt;math&amp;gt;u(x,t)&amp;lt;/math&amp;gt; is an unknown function with initial condition &amp;lt;math&amp;gt;u(x,0) = f(x)&amp;lt;/math&amp;gt;. Multiplying with &amp;lt;math&amp;gt;u&amp;lt;/math&amp;gt; and integrating over the domain gives&lt;br /&gt;
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where &amp;lt;math&amp;gt;\alpha \neq 0&amp;lt;/math&amp;gt; is a constant and &amp;lt;math&amp;gt;u(x,t)&amp;lt;/math&amp;gt; is an unknown function with initial condition &amp;lt;math&amp;gt;u(x,0) = f(x)&amp;lt;/math&amp;gt;. Multiplying with &amp;lt;math&amp;gt;u&amp;lt;/math&amp;gt; and integrating over the domain gives&lt;br /&gt;
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其中 &amp;lt;math&amp;gt;\alpha \neq 0&amp;lt;/math&amp;gt; 是常数，并且 &amp;lt;math&amp;gt;u(x,t)&amp;lt;/math&amp;gt; 是未知函数，初始条件是 &amp;lt;math&amp;gt;u(x,0) = f(x)&amp;lt;/math&amp;gt;。乘以 &amp;lt;math&amp;gt;u&amp;lt;/math&amp;gt; 并在域上进行积分。&lt;br /&gt;
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: &amp;lt;math&amp;gt;\int_a^b u \frac{\partial u}{\partial t} \operatorname dx + \alpha \int _a ^b u \frac{\partial u}{\partial x} \operatorname dx = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;\int_a^b u \frac{\partial u}{\partial t} \operatorname dx + \alpha \int _a ^b u \frac{\partial u}{\partial x} \operatorname dx = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
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Using that&lt;br /&gt;
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Using that&lt;br /&gt;
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利用这一点&lt;br /&gt;
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: &amp;lt;math&amp;gt;\int _a ^b u \frac{\partial u}{\partial t} \operatorname dx = \frac{1}{2} \frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 \quad \text{and} \quad \int _a ^b u \frac{\partial u}{\partial x} \operatorname dx = \frac{1}{2} u(b,t)^2 - \frac{1}{2} u(a,t)^2,.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;\int _a ^b u \frac{\partial u}{\partial t} \operatorname dx = \frac{1}{2} \frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 \quad \text{and} \quad \int _a ^b u \frac{\partial u}{\partial x} \operatorname dx = \frac{1}{2} u(b,t)^2 - \frac{1}{2} u(a,t)^2,.&amp;lt;/math&amp;gt;&lt;br /&gt;
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where integration by parts has been used for the second relationship, we get&lt;br /&gt;
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where integration by parts has been used for the second relationship, we get&lt;br /&gt;
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第二个关系中采用了分部积分法，我们可以得到&lt;br /&gt;
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: &amp;lt;math&amp;gt;\frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 + \alpha u(b,t)^2 - \alpha u(a,t)^2 = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;\frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 + \alpha u(b,t)^2 - \alpha u(a,t)^2 = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
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Here &amp;lt;math&amp;gt;\vert \vert \cdot \vert \vert&amp;lt;/math&amp;gt; denotes the standard L2-norm.&lt;br /&gt;
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Here &amp;lt;math&amp;gt;\vert \vert \cdot \vert \vert&amp;lt;/math&amp;gt; denotes the standard L2-norm.&lt;br /&gt;
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在这里，&amp;lt;math&amp;gt;\vert \vert \cdot \vert \vert&amp;lt;/math&amp;gt; 表示标准的 L2-正则。&lt;br /&gt;
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For well-posedness we require that the energy of the solution is non-increasing, i.e. that &amp;lt;math&amp;gt;\frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 \leq 0&amp;lt;/math&amp;gt;, which is achieved by specifying &amp;lt;math&amp;gt;u&amp;lt;/math&amp;gt; at &amp;lt;math&amp;gt;x = a&amp;lt;/math&amp;gt; if &amp;lt;math&amp;gt;\alpha &amp;gt; 0&amp;lt;/math&amp;gt; and at &amp;lt;math&amp;gt;x = b&amp;lt;/math&amp;gt; if &amp;lt;math&amp;gt;\alpha &amp;lt; 0&amp;lt;/math&amp;gt;. This corresponds to only imposing boundary conditions at the inflow. Note that well-posedness allows for growth in terms of data (initial and boundary) and thus it is sufficient to show that &amp;lt;math&amp;gt;\frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 \leq 0&amp;lt;/math&amp;gt; holds when all data is set to zero.&lt;br /&gt;
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For well-posedness we require that the energy of the solution is non-increasing, i.e. that &amp;lt;math&amp;gt;\frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 \leq 0&amp;lt;/math&amp;gt;, which is achieved by specifying &amp;lt;math&amp;gt;u&amp;lt;/math&amp;gt; at &amp;lt;math&amp;gt;x = a&amp;lt;/math&amp;gt; if &amp;lt;math&amp;gt;\alpha &amp;gt; 0&amp;lt;/math&amp;gt; and at &amp;lt;math&amp;gt;x = b&amp;lt;/math&amp;gt; if &amp;lt;math&amp;gt;\alpha &amp;lt; 0&amp;lt;/math&amp;gt;. This corresponds to only imposing boundary conditions at the inflow. Note that well-posedness allows for growth in terms of data (initial and boundary) and thus it is sufficient to show that &amp;lt;math&amp;gt;\frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 \leq 0&amp;lt;/math&amp;gt; holds when all data is set to zero.&lt;br /&gt;
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对于适定性，我们要解的能量是不增加的，即 &amp;lt;math&amp;gt;\frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 \leq 0&amp;lt;/math&amp;gt; ，这种关系可以通过在&amp;lt;math&amp;gt;x = a&amp;lt;/math&amp;gt;处 （如果 &amp;lt;math&amp;gt;\alpha &amp;gt; 0&amp;lt;/math&amp;gt;） 以及 &amp;lt;math&amp;gt;x = b&amp;lt;/math&amp;gt;处 （如果 &amp;lt;math&amp;gt;\alpha &amp;lt; 0&amp;lt;/math&amp;gt;）指定&amp;lt;math&amp;gt;u&amp;lt;/math&amp;gt;的值来实现。这只相当于在入流处附加边界条件。注意，适定性允许在数据(初始和边界)上的增长，因此它足以表明当所有数据设置为零时应有 &amp;lt;math&amp;gt;\frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 \leq 0&amp;lt;/math&amp;gt;。&lt;br /&gt;
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==[[用户:Yuling|Yuling]]（[[用户讨论:Yuling|讨论]]）“This corresponds to only imposing boundary conditions at the inflow.” 这句话中的inflow不是很理解&lt;br /&gt;
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==Notes==&lt;br /&gt;
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{{Reflist}}&lt;br /&gt;
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== References ==&lt;br /&gt;
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{{refbegin|2}}&lt;br /&gt;
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* {{cite book |title=Solving Frontier problems of Physics: The decomposition method&lt;br /&gt;
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|first=G.|last=Adomian|publisher=Kluwer Academic Publishers|year=1994|isbn=|page=|url=https://books.google.com/books?id=UKPqCAAAQBAJ&amp;amp;printsec=frontcover#v=onepage&amp;amp;q=%22partial%20differential%22&amp;amp;f=false}}&lt;br /&gt;
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1994年 | isbn | 页面 | 网址: 施普林格科学+商业媒体 https://books.google.com/books?id=ukpqcaaaqbaj&amp;amp;printsec=frontcover#v=onepage&amp;amp;q=%22partial%20differential%22&amp;amp;f=false&lt;br /&gt;
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* {{Citation |first=A. D. |last=Polyanin |title=Handbook of Linear Partial Differential Equations for Engineers and Scientists |publisher=Chapman &amp;amp; Hall/CRC Press |location=Boca Raton |year=2002 |isbn=1-58488-299-9 }}.&lt;br /&gt;
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* {{Citation |first=A. D. |last=Polyanin |lastauthoramp=yes |first2=V. F. |last2=Zaitsev |title=Handbook of Nonlinear Partial Differential Equations |publisher=Chapman &amp;amp; Hall/CRC Press |location=Boca Raton |year=2004 |isbn=1-58488-355-3 }}.&lt;br /&gt;
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* {{Citation |first=A. D. |last=Polyanin |first2=V. F. |last2=Zaitsev |lastauthoramp=yes |first3=A. |last3=Moussiaux |title=Handbook of First Order Partial Differential Equations |publisher=Taylor &amp;amp; Francis |location=London |year=2002 |isbn=0-415-27267-X }}.&lt;br /&gt;
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* {{citation|mr=3014456|last=Roubíček|first= T.|title=Nonlinear Partial Differential Equations with Applications|publisher= Birkhäuser|place= Basel, Boston, Berlin|edition=2nd|year= 2013|ISBN= 978-3-0348-0512-4|doi=10.1007/978-3-0348-0513-1|url=http://cds.cern.ch/record/880983/files/9783764372934_TOC.pdf}}&lt;br /&gt;
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* {{Citation |first=P. |last=Solin |title=Partial Differential Equations and the Finite Element Method |publisher=J. Wiley &amp;amp; Sons |location=Hoboken, NJ |year=2005 |isbn=0-471-72070-4 }}.&lt;br /&gt;
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* {{Citation |first=P. |last=Solin |first2=K. |last2=Segeth |lastauthoramp=yes |first3=I. |last3=Dolezel |title=Higher-Order Finite Element Methods |publisher=Chapman &amp;amp; Hall/CRC Press |location=Boca Raton |year=2003 |isbn=1-58488-438-X }}.&lt;br /&gt;
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* {{Citation |first=H. |last=Stephani |year=1989 |title=Differential Equations: Their Solution Using Symmetries. Edited by M. MacCallum |publisher=Cambridge University Press }}.&lt;br /&gt;
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* {{cite book |title=Partial Differential Equations and Solitary Waves Theory&lt;br /&gt;
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|first=Abdul-Majid|last=Wazwaz|publisher=Higher Education Press|year=2009|isbn=978-3-642-00251-9|page=}}&lt;br /&gt;
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|first=Abdul-Majid|last=Wazwaz|publisher=Higher Education Press|year=2009|isbn=978-3-642-00251-9|page=}}&lt;br /&gt;
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| first Abdul-Majid | last Wazwaz | publisher Higher Education Press | year 2009 | isbn 978-3-642-00251-9 | page }&lt;br /&gt;
&lt;br /&gt;
* {{cite book |title=Partial Differential Equations Methods and Applications&lt;br /&gt;
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|first=Abdul-Majid|last=Wazwaz|publisher=A.A. Balkema|year=2002|isbn=90-5809-369-7|page=}}&lt;br /&gt;
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|first=Abdul-Majid|last=Wazwaz|publisher=A.A. Balkema|year=2002|isbn=90-5809-369-7|page=}}&lt;br /&gt;
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| first Abdul-Majid | last Wazwaz | publisher a.a.Balkema | year 2002 | isbn 90-5809-369-7 | page }&lt;br /&gt;
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* {{Citation |first=D. |last=Zwillinger |title=Handbook of Differential Equations |publisher=Academic Press |location=Boston |year=1997 |edition=3rd |isbn=0-12-784395-7 }}.&lt;br /&gt;
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* {{Citation |authorlink=Neil Gershenfeld |first=N. |last=Gershenfeld |title=The Nature of Mathematical Modeling |location=New York |publisher=Cambridge University Press, New York, NY, USA |year=1999 |edition=1st |isbn=0-521-57095-6 }}.&lt;br /&gt;
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* {{Citation |first=I.S. |last=Krasil'shchik |lastauthoramp=yes |first2=A.M., Eds. |last2=Vinogradov |title=Symmetries and Conserwation Laws for Differential Equations of Mathematical Physics |publisher=American Mathematical Society, Providence, Rhode Island, USA |year=1999 |isbn=0-8218-0958-X }}.&lt;br /&gt;
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* {{Citation |first=I.S. |last=Krasil'shchik |first2=V.V. |last2=Lychagin|lastauthoramp=yes |first3=A.M. |last3=Vinogradov |title=Geometry of Jet Spaces and Nonlinear Partial Differential Equations |publisher=Gordon and Breach Science Publishers, New York, London, Paris, Montreux, Tokyo |year=1986 |isbn=2-88124-051-8 }}.&lt;br /&gt;
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* {{Citation |first=A.M. |last=Vinogradov |title=Cohomological Analysis of Partial Differential Equations and Secondary Calculus |publisher=American Mathematical Society, Providence, Rhode Island, USA |year=2001 |isbn=0-8218-2922-X }}.&lt;br /&gt;
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* {{cite book |title=High Order Difference Methods for Time Dependent PDE&lt;br /&gt;
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|first=Bertil|last=Gustafsson|publisher=Springer|year=2008|isbn=978-3-540-74992-9|doi=10.1007/978-3-540-74993-6}}&lt;br /&gt;
&lt;br /&gt;
|first=Bertil|last=Gustafsson|publisher=Springer|year=2008|isbn=978-3-540-74992-9|doi=10.1007/978-3-540-74993-6}}&lt;br /&gt;
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| first Bertil | last Gustafsson | Springer | year 2008 | isbn 978-3-540-74992-9 | doi 10.1007 / 978-3-540-74993-6}&lt;br /&gt;
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{{refend}}&lt;br /&gt;
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== Further reading ==&lt;br /&gt;
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* {{Cite journal|last=Cajori|first=Florian|authorlink=Florian Cajori|year=1928|title=The Early History of Partial Differential Equations and of Partial Differentiation and Integration|url=http://www.math.harvard.edu/archive/21a_fall_14/exhibits/cajori/cajori.pdf|journal=The American Mathematical Monthly|volume=35|issue=9|pages=459–467|doi=10.2307/2298771|access-date=2016-05-15|archive-url=https://web.archive.org/web/20181123102253/http://www.math.harvard.edu/archive/21a_fall_14/exhibits/cajori/cajori.pdf|archive-date=2018-11-23|url-status=dead}}&lt;br /&gt;
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== External links ==&lt;br /&gt;
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{{Sister project links| wikt=no | commons=Category:Solutions of PDE | b=Partial Differential Equations | n=no | q=Partial differential equation | s=no | v=no | voy=no | species=no | d=no}}&lt;br /&gt;
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* {{springer|title=Differential equation, partial|id=p/d031920}}&lt;br /&gt;
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* [http://eqworld.ipmnet.ru/en/pde-en.htm Partial Differential Equations: Exact Solutions] at EqWorld: The World of Mathematical Equations.&lt;br /&gt;
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* [http://eqworld.ipmnet.ru/en/solutions/eqindex/eqindex-pde.htm Partial Differential Equations: Index] at EqWorld: The World of Mathematical Equations.&lt;br /&gt;
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* [http://eqworld.ipmnet.ru/en/methods/meth-pde.htm Partial Differential Equations: Methods] at EqWorld: The World of Mathematical Equations.&lt;br /&gt;
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* [https://web.archive.org/web/20170701144823/http://www.exampleproblems.com/wiki/index.php?title=Partial_Differential_Equations Example problems with solutions] at exampleproblems.com&lt;br /&gt;
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* [http://mathworld.wolfram.com/PartialDifferentialEquation.html Partial Differential Equations] at mathworld.wolfram.com&lt;br /&gt;
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* [https://reference.wolfram.com/language/FEMDocumentation/tutorial/SolvingPDEwithFEM.html Partial Differential Equations] with Mathematica&lt;br /&gt;
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* [http://www.mathworks.com/moler/pdes.pdf Partial Differential Equations] in Cleve Moler: Numerical Computing with MATLAB&lt;br /&gt;
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* [http://www.nag.com/numeric/fl/nagdoc_fl24/html/D03/d03intro.html Partial Differential Equations] at nag.com&lt;br /&gt;
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* {{cite web |first=Grant |last=Sanderson |title=But what is a partial differential equation? |work=3Blue1Brown |date=April 21, 2019 |url=https://www.youtube.com/watch?v=ly4S0oi3Yz8&amp;amp;list=PLZHQObOWTQDNPOjrT6KVlfJuKtYTftqH6 |via=[[YouTube]] }}&lt;br /&gt;
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{{Differential equations topics}}&lt;br /&gt;
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[[Category:Partial differential equations| ]]&lt;br /&gt;
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[[Category:Multivariable calculus]]&lt;br /&gt;
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Category:Multivariable calculus&lt;br /&gt;
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类别: 多元微积分&lt;br /&gt;
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[[Category:Differential equations]]&lt;br /&gt;
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Category:Differential equations&lt;br /&gt;
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类别: 微分方程&lt;br /&gt;
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[[Category:Concepts in physics]]&lt;br /&gt;
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Category:Concepts in physics&lt;br /&gt;
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分类: 物理概念&lt;br /&gt;
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&amp;lt;small&amp;gt;This page was moved from [[wikipedia:en:Partial differential equation]]. Its edit history can be viewed at [[偏微分方程/edithistory]]&amp;lt;/small&amp;gt;&amp;lt;/noinclude&amp;gt;&lt;br /&gt;
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[[Category:待整理页面]]&lt;/div&gt;</summary>
		<author><name>Ruili</name></author>
	</entry>
	<entry>
		<id>https://wiki.swarma.org/index.php?title=%E5%81%8F%E5%BE%AE%E5%88%86%E6%96%B9%E7%A8%8B&amp;diff=18119</id>
		<title>偏微分方程</title>
		<link rel="alternate" type="text/html" href="https://wiki.swarma.org/index.php?title=%E5%81%8F%E5%BE%AE%E5%88%86%E6%96%B9%E7%A8%8B&amp;diff=18119"/>
		<updated>2020-11-11T13:40:36Z</updated>

		<summary type="html">&lt;p&gt;Ruili：&lt;/p&gt;
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&lt;div&gt;此词条暂由Yuling翻译，未经人工整理和审校，带来阅读不便，请见谅。&lt;br /&gt;
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[[File:Heat.gif|thumb|right|A visualisation of a solution to the two-dimensional [[heat equation]] with temperature represented by the third dimension]]&lt;br /&gt;
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A visualisation of a solution to the two-dimensional [[heat equation with temperature represented by the third dimension]]&lt;br /&gt;
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以三维表示温度的二维热方程解的可视化&lt;br /&gt;
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In [[mathematics]], a '''partial differential equation''' ('''PDE''') is a [[differential equation]] that contains unknown [[Multivariable calculus|multivariable functions]] and their [[partial derivative]]s. PDEs are used to formulate problems involving functions of several variables, and are either solved by hand, or used to create a [[computer model]]. A special case is [[ordinary differential equation]]s (ODEs), which deal with functions of a single variable and their derivatives.&lt;br /&gt;
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In mathematics, a partial differential equation (PDE) is a differential equation that contains unknown multivariable functions and their partial derivatives. PDEs are used to formulate problems involving functions of several variables, and are either solved by hand, or used to create a computer model. A special case is ordinary differential equations (ODEs), which deal with functions of a single variable and their derivatives.&lt;br /&gt;
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在数学中，'''&amp;lt;font color = &amp;quot;#ff8000&amp;quot;&amp;gt; 偏微分方程函数 Partial Differential Equation&amp;lt;/font&amp;gt;'''是包含未知多元函数及其偏导数的微分方程。偏微分方程用于描述涉及多元函数的问题，可以通过人为求解，也可以通过建立计算机模型来求解。常微分方程是偏微分方程一种特殊情况，它处理的是一元函数及其导数。&lt;br /&gt;
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PDEs can be used to describe a wide variety of phenomena such as sound, heat, [[diffusion]], [[electrostatics]], [[Electromagnetism|electrodynamics]], [[fluid dynamics]], [[Elasticity (physics)|elasticity]], [[gravitation]] and [[quantum mechanics]]. These seemingly distinct physical phenomena can be formalised similarly in terms of PDEs. Just as ordinary differential equations often model one-dimensional [[dynamical system]]s, partial differential equations often model [[multidimensional system]]s. PDEs find their generalisation in [[stochastic partial differential equation]]s.&lt;br /&gt;
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PDEs can be used to describe a wide variety of phenomena such as sound, heat, diffusion, electrostatics, electrodynamics, fluid dynamics, elasticity, gravitation and quantum mechanics. These seemingly distinct physical phenomena can be formalised similarly in terms of PDEs. Just as ordinary differential equations often model one-dimensional dynamical systems, partial differential equations often model multidimensional systems. PDEs find their generalisation in stochastic partial differential equations.&lt;br /&gt;
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偏微分方程可以用来描述各种各样的物理现象，如声音，热量，扩散，静电，电动力学，流体力学，弹性力学，重力和量子力学。这些看起来截然不同的物理现象却可以用类似的偏微分方程来描述。正如常微分方程经常对一维动力系统进行建模一样，偏微分方程经常对多维系统进行建模。随机偏微分方程是偏微分方程的一种推广。&lt;br /&gt;
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== Introduction ==&lt;br /&gt;
引言&lt;br /&gt;
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Partial differential equations (PDEs) are equations that involve rates of change with respect to [[continuous variables]]. For example, the position of a [[rigid body]] is specified by six parameters,&amp;lt;ref&amp;gt;{{Cite book|url=https://books.google.com/books?id=v9PLbcYd9aUC&amp;amp;pg=PA32|title=Modelling and Control of Robot Manipulators|last=Sciavicco|first=Lorenzo|last2=Siciliano|first2=Bruno|date=2001-02-19|publisher=Springer Science &amp;amp; Business Media|isbn=9781852332211|language=en}}&amp;lt;/ref&amp;gt; but the configuration of a [[fluid]] is given by the [[continuous distribution]] of several parameters, such as the [[temperature]], [[pressure]], and so forth. The dynamics for the rigid body take place in a finite-dimensional [[Configuration space (physics)|configuration space]]; the dynamics for the fluid occur in an infinite-dimensional configuration space. This distinction usually makes PDEs much harder to solve than ordinary differential equations (ODEs), but here again, there will be simple solutions for linear problems. Classic domains where PDEs are used include [[acoustics]], [[fluid dynamics]], [[electrodynamics]], and [[heat transfer]].&lt;br /&gt;
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Partial differential equations (PDEs) are equations that involve rates of change with respect to continuous variables. For example, the position of a rigid body is specified by six parameters, but the configuration of a fluid is given by the continuous distribution of several parameters, such as the temperature, pressure, and so forth. The dynamics for the rigid body take place in a finite-dimensional configuration space; the dynamics for the fluid occur in an infinite-dimensional configuration space. This distinction usually makes PDEs much harder to solve than ordinary differential equations (ODEs), but here again, there will be simple solutions for linear problems. Classic domains where PDEs are used include acoustics, fluid dynamics, electrodynamics, and heat transfer.&lt;br /&gt;
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偏微分方程(简称为PDEs)涉及到方程相对于连续变量的变化率。例如，刚体的位置是由六个参数确定的，而流体的状态是由几个参数的连续分布给出的，如温度、压力等。刚体的动力学过程发生在有限维状态空间中，流体的动力学过程发生在无限维状态空间中。这种区别通常使偏微分方程比常微分方程更难求解，但是线性问题仍然有简单的求解方式。使用偏微分方程的经典领域包括声学、流体力学、电动力学和传热学。&lt;br /&gt;
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A partial differential equation (PDE) for the function {{math|''u''(''x''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;,… ''x&amp;lt;sub&amp;gt;n&amp;lt;/sub&amp;gt;'')}} is an equation of the form&lt;br /&gt;
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A partial differential equation (PDE) for the function  is an equation of the form&lt;br /&gt;
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函数 {{math|''u''(''x''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;,… ''x&amp;lt;sub&amp;gt;n&amp;lt;/sub&amp;gt;'')}} 的偏微分方程形式是：&lt;br /&gt;
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: &amp;lt;math&amp;gt;f \left (x_1, \ldots x_n; u, \frac{\partial u}{\partial x_1}, \ldots \frac{\partial u}{\partial x_n}; \frac{\partial^2 u}{\partial x_1 \partial x_1}, \ldots \frac{\partial^2 u}{\partial x_1 \partial x_n}; \ldots \right) = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;f \left (x_1, \ldots x_n; u, \frac{\partial u}{\partial x_1}, \ldots \frac{\partial u}{\partial x_n}; \frac{\partial^2 u}{\partial x_1 \partial x_1}, \ldots \frac{\partial^2 u}{\partial x_1 \partial x_n}; \ldots \right) = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
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If {{mvar|f}} is a [[linear function]] of {{mvar|u}} and its derivatives, then the PDE is called linear. Common examples of linear PDEs include the [[heat equation]], the [[wave equation]], [[Laplace's equation]], [[Helmholtz equation]], [[Klein–Gordon equation]], and [[Poisson's equation]].&lt;br /&gt;
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If  is a linear function of  and its derivatives, then the PDE is called linear. Common examples of linear PDEs include the heat equation, the wave equation, Laplace's equation, Helmholtz equation, Klein–Gordon equation, and Poisson's equation.&lt;br /&gt;
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如果 {{mvar|f}}是函数{{math|''u''}} 及其导数的线性函数，则偏微分方程称为线性函数。线性偏微分方程的常见例子包括热方程、波动方程、拉普拉斯方程、亥姆霍兹方程方程、克莱因-高登方程和泊松方程。&lt;br /&gt;
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A relatively simple PDE is&lt;br /&gt;
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A relatively simple PDE is&lt;br /&gt;
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一个相对简单的偏微分方程：&lt;br /&gt;
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: &amp;lt;math&amp;gt;\frac{\partial u}{\partial x}(x,y) = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;\frac{\partial u}{\partial x}(x,y) = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
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This relation [[Logical implication|implies]] that the function {{math|''u''(''x'',''y'')}} is independent of {{mvar|x}}. However, the equation gives no information on the function's dependence on the variable {{mvar|y}}. Hence the general solution of this equation is&lt;br /&gt;
&lt;br /&gt;
This relation implies that the function  is independent of . However, the equation gives no information on the function's dependence on the variable . Hence the general solution of this equation is&lt;br /&gt;
&lt;br /&gt;
这意味着函数 {{math|''u''(''x'',''y'')}} 独立于 {{mvar|x}} 的。然而，这个方程没有给出关于函数和自变量的相关性的信息。因此，这个方程的通解是&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt;u(x,y) = f(y),&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;u(x,y) = f(y),&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
where {{mvar|f}} is an arbitrary function of {{mvar|y}}. The analogous ordinary differential equation is&lt;br /&gt;
&lt;br /&gt;
where  is an arbitrary function of . The analogous ordinary differential equation is&lt;br /&gt;
&lt;br /&gt;
其中， {{mvar|f}} 是 {{mvar|y}} 的任意函数。&lt;br /&gt;
&lt;br /&gt;
类似的常微分方程是：&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt;\frac{\mathrm{d} u}{\mathrm{d} x}(x) = 0,&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;\frac{\mathrm{d} u}{\mathrm{d} x}(x) = 0,&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
which has the solution&lt;br /&gt;
&lt;br /&gt;
which has the solution&lt;br /&gt;
&lt;br /&gt;
它的解为&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt;u(x) = c,&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;u(x) = c,&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
where {{mvar|c}} is any [[Constant (mathematics)|constant]] value. These two examples illustrate that general solutions of ordinary differential equations (ODEs) involve arbitrary constants, but solutions of PDEs involve arbitrary functions.&lt;br /&gt;
&lt;br /&gt;
where  is any constant value. These two examples illustrate that general solutions of ordinary differential equations (ODEs) involve arbitrary constants, but solutions of PDEs involve arbitrary functions.&lt;br /&gt;
&lt;br /&gt;
这里，{{mvar|c}} 是一个任意常量。&lt;br /&gt;
&lt;br /&gt;
这两个例子说明常微分方程的一般解包含任意常数，但偏微分方程的解包含任意函数。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
A solution of a PDE is generally not [[Uniqueness quantification|unique]]; additional conditions must generally be specified on the [[Boundary (topology)|boundary]] of the region where the solution is defined. For instance, in the simple example above, the function {{math|''f''(''y'')}} can be determined if {{mvar|u}} is specified on the line {{math|''x'' {{=}} 0}}.&lt;br /&gt;
&lt;br /&gt;
A solution of a PDE is generally not unique; additional conditions must generally be specified on the boundary of the region where the solution is defined. For instance, in the simple example above, the function  can be determined if  is specified on the line  0}}.&lt;br /&gt;
&lt;br /&gt;
偏微分方程的解一般不是唯一的; 一般必须在定义解的区域边界上定义附加条件。 例如，在上面的简单示例中，如果在 {{math|''x'' {{=}} 0}} 时确定了 {{mvar|u}} 的值，则可以确定该函数 {{math|''f''(''y'')}}。&lt;br /&gt;
&lt;br /&gt;
== Existence and uniqueness ==&lt;br /&gt;
存在性和唯一性&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Although the issue of existence and uniqueness of solutions of ordinary differential equations has a very satisfactory answer with the [[Picard–Lindelöf theorem]], that is far from the case for partial differential equations. The [[Cauchy–Kowalevski theorem]] states that the [[Cauchy problem]] for any partial differential equation whose coefficients are [[Analytic function|analytic]] in the unknown function and its derivatives, has a locally unique analytic solution. Although this result might appear to settle the existence and uniqueness of solutions, there are examples of linear partial differential equations whose coefficients have derivatives of all orders (which are nevertheless not analytic) but which have no solutions at all: see [[Lewy's example|Lewy (1957)]]. Even if the solution of a partial differential equation exists and is unique, it may nevertheless have undesirable properties.  The mathematical study of these questions is usually in the more powerful context of [[weak solution]]s.&lt;br /&gt;
&lt;br /&gt;
Although the issue of existence and uniqueness of solutions of ordinary differential equations has a very satisfactory answer with the Picard–Lindelöf theorem, that is far from the case for partial differential equations. The Cauchy–Kowalevski theorem states that the Cauchy problem for any partial differential equation whose coefficients are analytic in the unknown function and its derivatives, has a locally unique analytic solution. Although this result might appear to settle the existence and uniqueness of solutions, there are examples of linear partial differential equations whose coefficients have derivatives of all orders (which are nevertheless not analytic) but which have no solutions at all: see Lewy (1957). Even if the solution of a partial differential equation exists and is unique, it may nevertheless have undesirable properties.  The mathematical study of these questions is usually in the more powerful context of weak solutions.&lt;br /&gt;
&lt;br /&gt;
虽然常微分方程解的存在唯一性问题用'''&amp;lt;font color=&amp;quot;#ff8000&amp;quot;&amp;gt;弗罗贝尼乌斯定理 Picard–Lindelöf Theorem&amp;lt;/font&amp;gt;得到了令人满意的结果，但应用到偏微分方程上却不尽如意。'''&amp;lt;font color=&amp;quot;#ff8000&amp;quot;&amp;gt;柯西-科瓦列夫斯基定理 Cauchy–Kowalevski theorem&amp;lt;/font&amp;gt;指出，对于任何在未知函数及其导数中系数是解析的偏微分方程，柯西问题有一个局部唯一的解析解。虽然这个结果似乎解决了解的存在性和唯一性问题，但是有一些线性偏微分方程的系数具有所有级数的导数(尽管这些导数不是解析的) ，但是根本没有解: 见 Lewy (1957)。即使偏微分方程的解存在且唯一，它仍然可能具有人们所不希望的性质。这些问题的数学研究通常是在更有力的弱解的背景下进行的。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
An example of pathological behavior is the sequence (depending upon {{mvar|n}}) of [[Cauchy problem]]s for the [[Laplace equation]]&lt;br /&gt;
&lt;br /&gt;
An example of pathological behavior is the sequence (depending upon ) of Cauchy problems for the Laplace equation&lt;br /&gt;
&lt;br /&gt;
反常特征的一个例子是拉普拉斯方程的柯西问题的序列(取决于{{mvar|n}})&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt;\frac{\partial^2 u}{\partial x^2} + \frac{\partial^2 u}{\partial y^2}=0,&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;\frac{\partial^2 u}{\partial x^2} + \frac{\partial^2 u}{\partial y^2}=0,&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
with [[boundary condition]]s&lt;br /&gt;
&lt;br /&gt;
with boundary conditions&lt;br /&gt;
&lt;br /&gt;
有边界条件&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt;\begin{align} u(x,0) &amp;amp;= 0, \\ \frac{\partial u}{\partial y}(x,0) &amp;amp;= \frac{\sin nx}{n}, \end{align}&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;\begin{align} u(x,0) &amp;amp;= 0, \\ \frac{\partial u}{\partial y}(x,0) &amp;amp;= \frac{\sin nx}{n}, \end{align}&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
where {{mvar|n}} is an integer. The derivative of {{mvar|u}} with respect to {{mvar|y}} approaches zero [[uniform convergence|uniformly]] in {{mvar|x}} as {{mvar|n}} increases, but the solution is&lt;br /&gt;
&lt;br /&gt;
where  is an integer. The derivative of  with respect to  approaches zero uniformly in  as  increases, but the solution is&lt;br /&gt;
&lt;br /&gt;
其中{{mvar|n}}是整数。{{mvar|u}}是关于{{mvar|y}}的导数，一致地随着{{mvar|n}}的增加而趋于零，但是解是&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt;u(x,y) = \frac{\sinh ny \sin nx}{n^2}.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;u(x,y) = \frac{\sinh ny \sin nx}{n^2}.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
This solution approaches infinity if {{mvar|nx}} is not an integer multiple of {{pi}} for any non-zero value of {{mvar|y}}. The Cauchy problem for the Laplace equation is called ''ill-posed'' or ''not [[Well-posed problem|well-posed]]'', since the solution does not continuously depend on the data of the problem. Such ill-posed problems are not usually satisfactory for physical applications.&lt;br /&gt;
&lt;br /&gt;
This solution approaches infinity if  is not an integer multiple of  for any non-zero value of . The Cauchy problem for the Laplace equation is called ill-posed or not well-posed, since the solution does not continuously depend on the data of the problem. Such ill-posed problems are not usually satisfactory for physical applications.&lt;br /&gt;
&lt;br /&gt;
对于任何非零的{{mvar|y}}，如果{{mvar|nx}}不是{{pi}}的整数倍，这个解会接近于无穷大。拉普拉斯方程的柯西问题被称为不适定问题（可以译为ill-posed或not well-posed），因为该问题的解并不连续地依赖于该问题的数据。这种不适定问题在物理应用中通常不能令人满意。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The [[Navier–Stokes existence and smoothness|existence of solutions for the Navier–Stokes equations]], a partial differential equation, is part of one of the [[Millennium Prize Problems]].&lt;br /&gt;
&lt;br /&gt;
The existence of solutions for the Navier–Stokes equations, a partial differential equation, is part of one of the Millennium Prize Problems.&lt;br /&gt;
&lt;br /&gt;
一种偏微分方程——纳维-斯托克斯方程——的解的存在性就是千禧年大奖难题的一部分。&lt;br /&gt;
&lt;br /&gt;
== Notation ==&lt;br /&gt;
符号&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
In PDEs, it is common to denote partial derivatives using subscripts. That is:&lt;br /&gt;
&lt;br /&gt;
In PDEs, it is common to denote partial derivatives using subscripts. That is:&lt;br /&gt;
&lt;br /&gt;
在偏微分方程中，通常用下标表示偏导数。例如:&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt;u_x = \frac{\partial u}{\partial x}&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;u_x = \frac{\partial u}{\partial x}&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt;u_{xx} = \frac{\partial^2 u}{\partial x^2} &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;u_{xx} = \frac{\partial^2 u}{\partial x^2} &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt;u_{xy} = \frac{\partial^2 u}{\partial y\, \partial x} = \frac{\partial}{\partial y } \left(\frac{\partial u}{\partial x}\right). &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;u_{xy} = \frac{\partial^2 u}{\partial y\, \partial x} = \frac{\partial}{\partial y } \left(\frac{\partial u}{\partial x}\right). &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Especially in physics, [[del]] or nabla ({{math|∇}}) is often used to denote spatial derivatives, and {{math|''&amp;amp;#x307;u'', ''ü''}} for time derivatives. For example, the [[wave equation]] (mentioned below) can be written as&lt;br /&gt;
&lt;br /&gt;
Especially in physics, del or nabla () is often used to denote spatial derivatives, and  for time derivatives. For example, the wave equation (mentioned below) can be written as&lt;br /&gt;
&lt;br /&gt;
特别是在物理学中，[[del]]或nabla ({{math|∇}})经常用来表示空间导数和时间导数。例如，波动方程(在下文中提到)可以写成&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt;\ddot u=c^2\nabla^2u&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt;\ddot u=c^2\nabla^2u&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
or&lt;br /&gt;
&lt;br /&gt;
or&lt;br /&gt;
&lt;br /&gt;
或&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt;\ddot u=c^2\Delta u&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt;\ddot u=c^2\Delta u&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
where {{math|Δ}} is the [[Laplace operator]].&lt;br /&gt;
&lt;br /&gt;
where  is the Laplace operator.&lt;br /&gt;
&lt;br /&gt;
其中{{math|Δ}}代表拉普拉斯算子&lt;br /&gt;
&lt;br /&gt;
== Classification ==&lt;br /&gt;
分类&lt;br /&gt;
&lt;br /&gt;
Some linear, second-order partial differential equations can be classified as [[parabolic partial differential equation|parabolic]], [[hyperbolic partial differential equation|hyperbolic]] and [[elliptic partial differential equation|elliptic]]. Others, such as the [[Euler–Tricomi equation]], have different types in different regions. The classification provides a guide to appropriate initial and boundary conditions and to the smoothness of the solutions.&lt;br /&gt;
&lt;br /&gt;
Some linear, second-order partial differential equations can be classified as parabolic, hyperbolic and elliptic. Others, such as the Euler–Tricomi equation, have different types in different regions. The classification provides a guide to appropriate initial and boundary conditions and to the smoothness of the solutions.&lt;br /&gt;
&lt;br /&gt;
一些线性二阶偏微分方程可分为抛物型方程、双曲型方程和椭圆型方程。其他的方程，如欧拉-特里科米方程，在不同的区域有不同的类型。这种分类有助于选择适当的初始和边界条件以及提高解的平滑性。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
=== Equations of first order ===&lt;br /&gt;
一阶方程&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{{main|First-order partial differential equation}}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
=== Linear equations of second order ===&lt;br /&gt;
二阶线性方程&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Assuming {{math|''u&amp;lt;sub&amp;gt;xy&amp;lt;/sub&amp;gt;'' {{=}} ''u&amp;lt;sub&amp;gt;yx&amp;lt;/sub&amp;gt;''}}, the general linear second-order PDE in two independent variables has the form&lt;br /&gt;
&lt;br /&gt;
Assuming  u&amp;lt;sub&amp;gt;yx&amp;lt;/sub&amp;gt;}}, the general linear second-order PDE in two independent variables has the form&lt;br /&gt;
&lt;br /&gt;
假设 {{math|''u&amp;lt;sub&amp;gt;xy&amp;lt;/sub&amp;gt;'' {{=}} ''u&amp;lt;sub&amp;gt;yx&amp;lt;/sub&amp;gt;''}}，含有两个独立变量的一般的线性二阶偏微分方程具有如下这样的形式&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt;Au_{xx} + 2Bu_{xy} + Cu_{yy} + \cdots \mbox{(lower order terms)} = 0,&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;Au_{xx} + 2Bu_{xy} + Cu_{yy} + \cdots \mbox{(lower order terms)} = 0,&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
where the coefficients {{mvar|A}}, {{mvar|B}}, {{mvar|C}}... may depend upon {{mvar|x}} and {{mvar|y}}. If {{math|''A''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; + ''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; + ''C''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; &amp;gt; 0}} over a region of the {{mvar|xy}}-plane, the PDE is second-order in that region. This form is analogous to the equation for a conic section:&lt;br /&gt;
&lt;br /&gt;
where the coefficients , , ... may depend upon  and . If  over a region of the -plane, the PDE is second-order in that region. This form is analogous to the equation for a conic section:&lt;br /&gt;
&lt;br /&gt;
其中的系数 {{mvar|A}}, {{mvar|B}}, {{mvar|C}}... 一般取决于{{mvar|x}}和{{mvar|y}}。如果在{{mvar|xy}}-平面的一个区域上 {{math|''A''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; + ''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; + ''C''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; &amp;gt; 0}}，偏微分方程在该区域是二阶的。这种形式类似于圆锥曲线的方程:&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt;Ax^2 + 2Bxy + Cy^2 + \cdots = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;Ax^2 + 2Bxy + Cy^2 + \cdots = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
More precisely, replacing {{math|∂&amp;lt;sub&amp;gt;''x''&amp;lt;/sub&amp;gt;}} by {{mvar|X}}, and likewise for other variables (formally this is done by a [[Fourier transform]]), converts a constant-coefficient PDE into a polynomial of the same degree, with the terms of the highest degree (a [[homogeneous polynomial]], here a [[quadratic form]]) being most significant for the classification.&lt;br /&gt;
&lt;br /&gt;
More precisely, replacing  by , and likewise for other variables (formally this is done by a Fourier transform), converts a constant-coefficient PDE into a polynomial of the same degree, with the terms of the highest degree (a homogeneous polynomial, here a quadratic form) being most significant for the classification.&lt;br /&gt;
&lt;br /&gt;
更准确地说，用 {{mvar|X}} 替换 {{math|∂&amp;lt;sub&amp;gt;''x''&amp;lt;/sub&amp;gt;}}，对于其他变量做同样的操作(从形式上来说，这是由傅里叶变换来完成的)，将一个常系数偏微分方程转换成一个相同次数的多项式，最高次数的项(齐次多项式，这里是一个二次形式)一般会用于偏微分方程的分类。&lt;br /&gt;
===~~ most significant for the classification 意译为用于偏微分方程的分类。       significiant直译过来感觉不太合适&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Just as one classifies [[conic section]]s and quadratic forms into parabolic, hyperbolic, and elliptic based on the [[discriminant]] {{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − 4''AC''}}, the same can be done for a second-order PDE at a given point.  However, the [[discriminant]] in a PDE is given by {{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC''}} due to the convention of the {{mvar|xy}} term being {{math|2''B''}} rather than {{mvar|B}}; formally, the discriminant (of the associated quadratic form) is {{math|(2''B'')&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − 4''AC'' {{=}} 4(''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC'')}}, with the factor of 4 dropped for simplicity.&lt;br /&gt;
&lt;br /&gt;
Just as one classifies conic sections and quadratic forms into parabolic, hyperbolic, and elliptic based on the discriminant , the same can be done for a second-order PDE at a given point.  However, the discriminant in a PDE is given by  due to the convention of the  term being  rather than ; formally, the discriminant (of the associated quadratic form) is  4(B&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − AC)}}, with the factor of 4 dropped for simplicity.&lt;br /&gt;
&lt;br /&gt;
正如人们可以根据判别式 {{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − 4''AC''}} 将圆锥曲线和二次型分为抛物型、双曲型和椭圆型一样，对于给定点的二阶偏微分方程也可以这样做。然而，偏微分方程中的判别式 {{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − 4''AC''}} 是根据交叉项的系数{{math|2''B''}} 而不是 {{mvar|B}} 给出的，形式上，判别式(关联二次型)是 {{math|(2''B'')&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − 4''AC'' {{=}} 4(''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC'')}}，为简单起见，去掉了因子4。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
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# {{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC'' &amp;lt; 0}} (''[[elliptic partial differential equation]]''): Solutions of [[elliptic partial differential equation|elliptic PDEs]] are as smooth as the coefficients allow, within the interior of the region where the equation and solutions are defined. For example, solutions of [[Laplace's equation]] are analytic within the domain where they are defined, but solutions may assume boundary values that are not smooth. The motion of a fluid at subsonic speeds can be approximated with elliptic PDEs, and the Euler–Tricomi equation is elliptic where {{math|''x'' &amp;lt; 0}}.&lt;br /&gt;
&lt;br /&gt;
  (elliptic partial differential equation): Solutions of elliptic PDEs are as smooth as the coefficients allow, within the interior of the region where the equation and solutions are defined. For example, solutions of Laplace's equation are analytic within the domain where they are defined, but solutions may assume boundary values that are not smooth. The motion of a fluid at subsonic speeds can be approximated with elliptic PDEs, and the Euler–Tricomi equation is elliptic where .&lt;br /&gt;
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{{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC'' &amp;lt; 0}} (椭圆形微分方程)：在定义方程和解的区域内部，椭圆型偏微分方程的解光滑到系数允许的程度。例如，拉普拉斯方程的解在它们被定义的区域内是解析的，但是解可能假设边界值是不光滑的。亚音速流体的运动可以用椭圆偏微分方程近似，其中欧拉-特里科米方程在 {{math|''x'' &amp;lt; 0}} 时是椭圆型偏微分方程。&lt;br /&gt;
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# {{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC'' {{=}} 0}} (''[[parabolic partial differential equation]]''): Equations that are [[parabolic partial differential equation|parabolic]] at every point can be transformed into a form analogous to the [[heat equation]] by a change of independent variables. Solutions smooth out as the transformed time variable increases. The Euler–Tricomi equation has parabolic type on the line where {{math|''x'' {{=}} 0}}.&lt;br /&gt;
&lt;br /&gt;
  0}} (parabolic partial differential equation): Equations that are parabolic at every point can be transformed into a form analogous to the heat equation by a change of independent variables. Solutions smooth out as the transformed time variable increases. The Euler–Tricomi equation has parabolic type on the line where  0}}.&lt;br /&gt;
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{{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC'' {{=}} 0}}（抛物线形偏微分方程）：在每一点上都是抛物线型的方程可以通过改变自变量从而转化成类似于热方程的形式。随着转换后的时间变量的增加，方程的解变得平滑。欧拉-特里科米方程在 {{math|''x'' {{=}} 0}} 这条特征线上是抛物线形的。&lt;br /&gt;
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# {{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC'' &amp;gt; 0}} (''[[hyperbolic partial differential equation]]''): [[hyperbolic partial differential equation|hyperbolic]] equations retain any discontinuities of functions or derivatives in the initial data. An example is the [[wave equation]]. The motion of a fluid at supersonic speeds can be approximated with hyperbolic PDEs, and the Euler–Tricomi equation is hyperbolic where {{math|''x'' &amp;gt; 0}}.&lt;br /&gt;
&lt;br /&gt;
  (hyperbolic partial differential equation): hyperbolic equations retain any discontinuities of functions or derivatives in the initial data. An example is the wave equation. The motion of a fluid at supersonic speeds can be approximated with hyperbolic PDEs, and the Euler–Tricomi equation is hyperbolic where .&lt;br /&gt;
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{{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC'' &amp;gt; 0}} (双曲形偏微分方程)：双曲形方程在初始数据中保留了函数或导数的任何不连续性，波动方程就是其中的一个例子。超音速流体的运动可以用双曲形偏微分方程近似，其中欧拉-特里科米方程在 {{math|''x'' &amp;gt; 0}} 时是双曲型的。&lt;br /&gt;
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If there are {{mvar|n}} independent variables {{math|''x''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;, ''x''&amp;lt;sub&amp;gt;2 &amp;lt;/sub&amp;gt;,… ''x''&amp;lt;sub&amp;gt;''n''&amp;lt;/sub&amp;gt;}}, a general linear partial differential equation of second order has the form&lt;br /&gt;
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If there are  independent variables , a general linear partial differential equation of second order has the form&lt;br /&gt;
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如果存在 {{mvar|n}} 个自变量 {{math|''x''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;, ''x''&amp;lt;sub&amp;gt;2 &amp;lt;/sub&amp;gt;,… ''x''&amp;lt;sub&amp;gt;''n''&amp;lt;/sub&amp;gt;}}，一般二阶线性偏微分方程的形式是&lt;br /&gt;
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: &amp;lt;math&amp;gt;L u =\sum_{i=1}^n\sum_{j=1}^n a_{i,j} \frac{\partial^2 u}{\partial x_i \partial x_j} \quad \text{ plus lower-order terms} =0.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;L u =\sum_{i=1}^n\sum_{j=1}^n a_{i,j} \frac{\partial^2 u}{\partial x_i \partial x_j} \quad \text{ plus lower-order terms} =0.&amp;lt;/math&amp;gt;&lt;br /&gt;
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The classification depends upon the signature of the eigenvalues of the coefficient matrix {{math|''a''&amp;lt;sub&amp;gt;''i'',''j''&amp;lt;/sub&amp;gt;}}.&lt;br /&gt;
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The classification depends upon the signature of the eigenvalues of the coefficient matrix .&lt;br /&gt;
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这种分类取决于系数矩阵本征值的符号（正负性）。&lt;br /&gt;
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# Elliptic: the eigenvalues are all positive or all negative.&lt;br /&gt;
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 Elliptic: the eigenvalues are all positive or all negative.&lt;br /&gt;
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椭圆形方程: 本征值全部为正或全部为负。&lt;br /&gt;
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# Parabolic: the eigenvalues are all positive or all negative, save one that is zero.&lt;br /&gt;
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 Parabolic: the eigenvalues are all positive or all negative, save one that is zero.&lt;br /&gt;
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抛物线形方程: 本征值全部为正或全部为负，除了一个为零。&lt;br /&gt;
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# Hyperbolic: there is only one negative eigenvalue and all the rest are positive, or there is only one positive eigenvalue and all the rest are negative.&lt;br /&gt;
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 Hyperbolic: there is only one negative eigenvalue and all the rest are positive, or there is only one positive eigenvalue and all the rest are negative.&lt;br /&gt;
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双曲形方程: 只有一个负特征值，其余的都是正特征值，或者只有一个正特征值，其余的都是负特征值。&lt;br /&gt;
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# Ultrahyperbolic: there is more than one positive eigenvalue and more than one negative eigenvalue, and there are no zero eigenvalues. There is only a limited theory for ultrahyperbolic equations (Courant and Hilbert, 1962).&lt;br /&gt;
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 Ultrahyperbolic: there is more than one positive eigenvalue and more than one negative eigenvalue, and there are no zero eigenvalues. There is only a limited theory for ultrahyperbolic equations (Courant and Hilbert, 1962).&lt;br /&gt;
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超双形方程: 存在多于一个正本征值和多于一个的负本征值，且不存在零本征值。对于超双曲方程，只存在一个有限理论(Courant 和 Hilbert，1962)。&lt;br /&gt;
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==[[用户:Yuling|Yuling]]（[[用户讨论:Yuling|讨论]]） 我对于limited theory这个单词对应的相关理论不太了解。&lt;br /&gt;
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=== Systems of first-order equations and characteristic surfaces ===&lt;br /&gt;
一阶方程组和特征曲面&lt;br /&gt;
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The classification of partial differential equations can be extended to systems of first-order equations, where the unknown {{mvar|u}} is now a [[Euclidean vector|vector]] with {{mvar|m}} components, and the coefficient matrices {{mvar|A&amp;lt;sub&amp;gt;ν&amp;lt;/sub&amp;gt;}} are {{mvar|m}} by {{mvar|m}} matrices for {{math|''ν'' {{=}} 1, 2,… ''n''}}. The partial differential equation takes the form&lt;br /&gt;
&lt;br /&gt;
The classification of partial differential equations can be extended to systems of first-order equations, where the unknown  is now a vector with  components, and the coefficient matrices  are  by  matrices for  1, 2,… n}}. The partial differential equation takes the form&lt;br /&gt;
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偏微分方程组的分类可以推广到一阶方程组，其中未知量 {{mvar|u}} 是有 {{mvar|m}} 个分量的向量。对于 {{math|''ν'' {{=}} 1, 2,… ''n''}}，系数矩阵 {{mvar|A&amp;lt;sub&amp;gt;ν&amp;lt;/sub&amp;gt;}} 是 {{mvar|m}} × {{mvar|m}} 的矩阵。偏微分方程形式如下：&lt;br /&gt;
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: &amp;lt;math&amp;gt;Lu = \sum_{\nu=1}^{n} A_\nu \frac{\partial u}{\partial x_\nu} + B=0,&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;Lu = \sum_{\nu=1}^{n} A_\nu \frac{\partial u}{\partial x_\nu} + B=0,&amp;lt;/math&amp;gt;&lt;br /&gt;
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where the coefficient matrices {{mvar|A&amp;lt;sub&amp;gt;ν&amp;lt;/sub&amp;gt;}} and the vector {{mvar|B}} may depend upon {{mvar|x}} and {{mvar|u}}. If a [[hypersurface]] {{mvar|S}} is given in the implicit form&lt;br /&gt;
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where the coefficient matrices  and the vector  may depend upon  and . If a hypersurface  is given in the implicit form&lt;br /&gt;
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其中系数矩阵 {{mvar|A&amp;lt;sub&amp;gt;ν&amp;lt;/sub&amp;gt;}} 和向量 {{mvar|B}} 可能依赖于 {{mvar|x}} 和 {{mvar|u}}。如果超曲面是以隐式形式给出的&lt;br /&gt;
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: &amp;lt;math&amp;gt;\varphi(x_1, x_2, \ldots x_n)=0,&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;\varphi(x_1, x_2, \ldots x_n)=0,&amp;lt;/math&amp;gt;&lt;br /&gt;
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where {{mvar|φ}} has a non-zero gradient, then {{mvar|S}} is a '''characteristic surface''' for the operator {{mvar|L}} at a given point if the characteristic form vanishes:&lt;br /&gt;
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where  has a non-zero gradient, then  is a characteristic surface for the operator  at a given point if the characteristic form vanishes:&lt;br /&gt;
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其中存在一个非零的梯度，那么如果特征形式消失，则在给定点上算子的特征曲面形式如下:&lt;br /&gt;
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: &amp;lt;math&amp;gt;Q\left(\frac{\partial\varphi}{\partial x_1}, \ldots\frac{\partial\varphi}{\partial x_n}\right) =\det\left[\sum_{\nu=1}^nA_\nu \frac{\partial \varphi}{\partial x_\nu}\right]=0.\,&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;Q\left(\frac{\partial\varphi}{\partial x_1}, \ldots\frac{\partial\varphi}{\partial x_n}\right) =\det\left[\sum_{\nu=1}^nA_\nu \frac{\partial \varphi}{\partial x_\nu}\right]=0.\,&amp;lt;/math&amp;gt;&lt;br /&gt;
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The geometric interpretation of this condition is as follows: if data for {{mvar|u}} are prescribed on the surface {{mvar|S}}, then it may be possible to determine the normal derivative of {{mvar|u}} on {{mvar|S}} from the differential equation. If the data on {{mvar|S}} and the differential equation determine the normal derivative of {{mvar|u}} on {{mvar|S}}, then {{mvar|S}} is non-characteristic. If the data on {{mvar|S}} and the differential equation ''do not'' determine the normal derivative of {{mvar|u}} on {{mvar|S}}, then the surface is '''characteristic''', and the differential equation restricts the data on {{mvar|S}}: the differential equation is ''internal'' to {{mvar|S}}.&lt;br /&gt;
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The geometric interpretation of this condition is as follows: if data for  are prescribed on the surface , then it may be possible to determine the normal derivative of  on  from the differential equation. If the data on  and the differential equation determine the normal derivative of  on , then  is non-characteristic. If the data on  and the differential equation do not determine the normal derivative of  on , then the surface is characteristic, and the differential equation restricts the data on : the differential equation is internal to .&lt;br /&gt;
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这个条件的几何解释如下: 如果关于 {{mvar|u}} 的数据是在曲面 {{mvar|S}} 上规定的，那么就有可能依据微分方程确定曲面 {{mvar|S}} 上 {{mvar|u}} 的法向导数。如果曲面 {{mvar|S}} 上的数据和上面的微分方程能确定曲面 {{mvar|S}} 上 {{mvar|u}} 的法向导数，那么它就是非特征的。如果曲面 {{mvar|S}} 上的数据和上面的微分方程不能确定曲面 {{mvar|S}} 上 {{mvar|u}} 的法向导数，那么曲面是特征的，并且微分方程将数据限制在曲面 {{mvar|S}} 上：微分方程是在曲面 {{mvar|S}} 内部。&lt;br /&gt;
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# A first-order system {{math|''Lu'' {{=}} 0}} is ''elliptic'' if no surface is characteristic for {{mvar|L}}: the values of {{mvar|u}} on {{mvar|S}} and the differential equation always determine the normal derivative of {{mvar|u}} on {{mvar|S}}.&lt;br /&gt;
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 A first-order system  0}} is elliptic if no surface is characteristic for : the values of  on  and the differential equation always determine the normal derivative of  on .&lt;br /&gt;
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如果对于 {{mvar|L}} 没有曲面是特征的，则一阶系统 {{math|''Lu'' {{=}} 0}} 是椭圆形的：{{mvar|u}}在 {{mvar|S}} 的值和微分方程总能够决定 {{mvar|S}} 上 {{mvar|u}} 的法向导数。&lt;br /&gt;
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# A first-order system is ''hyperbolic'' at a point if there is a '''spacelike''' surface {{mvar|S}} with normal {{mvar|ξ}} at that point. This means that, given any non-trivial vector {{mvar|η}} orthogonal to {{mvar|ξ}}, and a scalar multiplier {{mvar|λ}}, the equation {{math|''Q''(''λξ'' + ''η'') {{=}} 0}} has {{mvar|m}} real roots {{math|''λ''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;, ''λ''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;,… ''λ''&amp;lt;sub&amp;gt;''m''&amp;lt;/sub&amp;gt;}}. The system is '''strictly hyperbolic''' if these roots are always distinct. The geometrical interpretation of this condition is as follows: the characteristic form {{math|''Q''(''ζ'') {{=}} 0}} defines a cone (the normal cone) with homogeneous coordinates ζ. In the hyperbolic case, this cone has {{mvar|m}} sheets, and the axis {{math|''ζ'' {{=}} ''λξ''}} runs inside these sheets: it does not intersect any of them. But when displaced from the origin by η, this axis intersects every sheet. In the elliptic case, the normal cone has no real sheets.&lt;br /&gt;
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 A first-order system is hyperbolic at a point if there is a spacelike surface  with normal  at that point. This means that, given any non-trivial vector  orthogonal to , and a scalar multiplier , the equation  0}} has  real roots . The system is strictly hyperbolic if these roots are always distinct. The geometrical interpretation of this condition is as follows: the characteristic form  0}} defines a cone (the normal cone) with homogeneous coordinates ζ. In the hyperbolic case, this cone has  sheets, and the axis  λξ}} runs inside these sheets: it does not intersect any of them. But when displaced from the origin by η, this axis intersects every sheet. In the elliptic case, the normal cone has no real sheets.&lt;br /&gt;
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如果在该点存在一个法向量为 {{mvar|ξ}}的 '''&amp;lt;font color=&amp;quot;#ff8000&amp;quot;&amp;gt;类空曲面 Spacclike Surface&amp;lt;/font&amp;gt; {{mvar|S}} ，则一阶系统在那一点是双曲的。这意味着，给定任意正交于 {{mvar|ξ}} 的非平凡向量 {{mvar|η}} 和一个标量乘子 {{mvar|λ}}，方程 {{math|''Q''(''λξ'' + ''η'') {{=}} 0}} 有 {{mvar|m}} 个实根 {{math|''λ''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;, ''λ''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;,… ''λ''&amp;lt;sub&amp;gt;''m''&amp;lt;/sub&amp;gt;}}。如果这些根始终不同，则该系统是严格双曲形的。这个条件的几何解释如下: 特征形式 {{math|''Q''(''ζ'') {{=}} 0}} 定义了一个具有齐次坐标 ζ的圆锥(法线圆锥)。在双曲形的情况下，这个圆锥体有 {{mvar|m}} 层，并且轴 {{math|''ζ'' {{=}} ''λξ''}} 在这些层中运动: 它不与任何一层相交。但是当从原点偏离η时，这条轴线与每一层都相交。在椭圆形的情况下，法向圆锥没有实层。&lt;br /&gt;
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==[[用户:Yuling|Yuling]]（[[用户讨论:Yuling|讨论]]） sheet 这个单词也不很理解，我直译为了“层”&lt;br /&gt;
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=== Equations of mixed type ===&lt;br /&gt;
混合型方程&lt;br /&gt;
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If a PDE has coefficients that are not constant, it is possible that it will not belong to any of these categories but rather be of '''mixed type'''. A simple but important example is the [[Euler–Tricomi equation]]&lt;br /&gt;
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If a PDE has coefficients that are not constant, it is possible that it will not belong to any of these categories but rather be of mixed type. A simple but important example is the Euler–Tricomi equation&lt;br /&gt;
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如果偏微分方程的系数不是常数，那么它可能不属于这些类别中的任何一个，而是属于混合类型。一个简单但重要的例子是欧拉-特里科米方程&lt;br /&gt;
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: &amp;lt;math&amp;gt;u_{xx} = xu_{yy},&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;u_{xx} = xu_{yy},&amp;lt;/math&amp;gt;&lt;br /&gt;
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which is called '''elliptic-hyperbolic''' because it is elliptic in the region {{math|''x'' &amp;lt; 0}}, hyperbolic in the region {{math|''x'' &amp;gt; 0}}, and degenerate parabolic on the line {{math|''x'' {{=}} 0}}.&lt;br /&gt;
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which is called elliptic-hyperbolic because it is elliptic in the region , hyperbolic in the region , and degenerate parabolic on the line  0}}.&lt;br /&gt;
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它在 {{math|''x'' &amp;lt; 0}} 的区域上是椭圆形，在 {{math|''x'' &amp;gt; 0}} 区域上是双曲形，在 {{math|''x'' {{=}} 0}}这条线上是退化为抛物线形，因此称之为椭圆-双曲型。&lt;br /&gt;
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''fill in: Dirichlet and Neumann boundaries, hyperbolic/parabolic/elliptic separation of variables, [[Fourier analysis]], [[Green's function]]s ...--&amp;gt;&lt;br /&gt;
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fill in: Dirichlet and Neumann boundaries, hyperbolic/parabolic/elliptic separation of variables, Fourier analysis, Green's functions ...--&amp;gt;&lt;br /&gt;
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填写: Dirichlet 和 Neumann 边界，双曲 / 抛物线 / 椭圆分离变量法，傅立叶分析，Green 函数... --&lt;br /&gt;
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=== Infinite-order PDEs in quantum mechanics ===&lt;br /&gt;
量子力学中的无限阶偏微分方程&lt;br /&gt;
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In the [[phase space formulation]] of quantum mechanics,  one may consider the [[Method of quantum characteristics|quantum Hamilton's equations]] for trajectories of quantum particles. These equations are infinite-order PDEs. However, in the semiclassical expansion, one has a finite system of ODEs at any fixed order of [[Dirac constant|{{mvar|ħ}}]].  The evolution equation of the [[Wigner quasi-probability distribution|c]] is also an infinite-order PDE. The quantum trajectories are [[Method of quantum characteristics|quantum characteristics]], with the use of which one could calculate the evolution of the Wigner function.&lt;br /&gt;
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In the phase space formulation of quantum mechanics,  one may consider the quantum Hamilton's equations for trajectories of quantum particles. These equations are infinite-order PDEs. However, in the semiclassical expansion, one has a finite system of ODEs at any fixed order of Dirac constant|.  The evolution equation of the Wigner function is also an infinite-order PDE. The quantum trajectories are quantum characteristics, with the use of which one could calculate the evolution of the Wigner function.&lt;br /&gt;
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在量子力学中的相空间表述中，我们可以考虑用于求解量子粒子的轨迹的量子哈密顿的方程。这些方程是无限阶偏微分方程。然而，在半经典展开中，我们在给定[[Dirac constant|{{mvar|ħ}}]]阶数下有一个有限的的常微分方程组。'''&amp;lt;font color=&amp;quot;#ff8000&amp;quot;&amp;gt;维格纳函数  Wigner Function&amp;lt;/font&amp;gt;的演化方程也是一个无限阶偏微分方程。由于量子轨道的量子特性，所以它通常可以用来计算维格纳函数的演化。&lt;br /&gt;
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== Analytical solutions ==&lt;br /&gt;
解析解&lt;br /&gt;
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===Separation of variables===&lt;br /&gt;
分离变量法&lt;br /&gt;
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{{main|Separable partial differential equation}}&lt;br /&gt;
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Linear PDEs can be reduced to systems of ordinary differential equations by the important technique of separation of variables. This technique rests on a characteristic of solutions to differential equations: if one can find any solution that solves the equation and satisfies the boundary conditions, then it is ''the'' solution (this also applies to ODEs). We assume as an [[ansatz]] that the dependence of a solution on the parameters space and time can be written as a product of terms that each depend on a single parameter, and then see if this can be made to solve the problem.&amp;lt;ref&amp;gt;{{cite book|last1=Gershenfeld|first1=Neil|title=The nature of mathematical modeling|date=2000|publisher=Cambridge Univ. Press|location=Cambridge|isbn=0521570956|page=27|edition=Reprinted (with corr.)}}&amp;lt;/ref&amp;gt;&lt;br /&gt;
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Linear PDEs can be reduced to systems of ordinary differential equations by the important technique of separation of variables. This technique rests on a characteristic of solutions to differential equations: if one can find any solution that solves the equation and satisfies the boundary conditions, then it is the solution (this also applies to ODEs). We assume as an ansatz that the dependence of a solution on the parameters space and time can be written as a product of terms that each depend on a single parameter, and then see if this can be made to solve the problem.&lt;br /&gt;
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线性偏微分方程组可以通过分离变量法这一重要方法来简化为常微分方程组。这种方法依赖于微分方程解的一个特征: 如果能找到任何一个满足方程和边界条件的解，那么这个解就是方程的解(这也适用于常微分方程)。我们假设解对参数空间和时间的依赖可以写成对它们每一项的依赖以及一个参数的乘积，然后再看看这是否可以用来解决这个问题。&lt;br /&gt;
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In the method of separation of variables, one reduces a PDE to a PDE in fewer variables, which is an ordinary differential equation if in one variable – these are in turn easier to solve.&lt;br /&gt;
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In the method of separation of variables, one reduces a PDE to a PDE in fewer variables, which is an ordinary differential equation if in one variable – these are in turn easier to solve.&lt;br /&gt;
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在分离变量法方法中，可以将偏微分方程简化为含有更少变量的偏微分方程，如果只有一个变量，那么就变成了一个'''&amp;lt;font color = &amp;quot;#ff8000&amp;quot;&amp;gt;常微分方程 Ordinary Differential Equation&amp;lt;/font&amp;gt;'''-- 反过来，这些方程也更容易求解。&lt;br /&gt;
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This is possible for simple PDEs, which are called [[separable partial differential equation]]s, and the domain is generally a rectangle (a product of intervals). Separable PDEs correspond to [[diagonal matrices]] – thinking of &amp;quot;the value for fixed {{mvar|x}}&amp;quot; as a coordinate, each coordinate can be understood separately.&lt;br /&gt;
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This is possible for simple PDEs, which are called separable partial differential equations, and the domain is generally a rectangle (a product of intervals). Separable PDEs correspond to diagonal matrices – thinking of &amp;quot;the value for fixed &amp;quot; as a coordinate, each coordinate can be understood separately.&lt;br /&gt;
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对于简单的偏微分方程(称为可分离偏微分方程)来说，这是可能的，而且方程通常定义在一个矩形区域(区间的乘积)上。可分离偏微分方程对应于对角线矩阵——以“固定值”为坐标，每个坐标可分开理解。&lt;br /&gt;
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This generalizes to the [[method of characteristics]], and is also used in [[integral transform]]s.&lt;br /&gt;
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This generalizes to the method of characteristics, and is also used in integral transforms.&lt;br /&gt;
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这种方法可以推广到特征曲线法，也可以用于积分变换。&lt;br /&gt;
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===Method of characteristics===&lt;br /&gt;
特征曲线法&lt;br /&gt;
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{{main|Method of characteristics}}&lt;br /&gt;
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In special cases, one can find characteristic curves on which the equation reduces to an ODE – changing coordinates in the domain to straighten these curves allows separation of variables, and is called the [[method of characteristics]].&lt;br /&gt;
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In special cases, one can find characteristic curves on which the equation reduces to an ODE – changing coordinates in the domain to straighten these curves allows separation of variables, and is called the method of characteristics.&lt;br /&gt;
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在特殊情况下，可以找到一些特征曲线，在这些曲线上方程可以变成一个常微分方程——意味着改变坐标从而使这些曲线变直从而达到分离变量的目的，这就是所谓的特征曲线法。&lt;br /&gt;
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More generally, one may find characteristic surfaces.&lt;br /&gt;
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More generally, one may find characteristic surfaces.&lt;br /&gt;
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更一般地说，人们可能会找到特征表面。&lt;br /&gt;
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===Integral transform===&lt;br /&gt;
积分变换&lt;br /&gt;
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An [[integral transform]] may transform the PDE to a simpler one, in particular, a separable PDE. This corresponds to diagonalizing an operator.&lt;br /&gt;
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An integral transform may transform the PDE to a simpler one, in particular, a separable PDE. This corresponds to diagonalizing an operator.&lt;br /&gt;
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积分变换可以将偏微分方程转换为更简单的偏微分方程，特别是可分离的偏微分方程。这对应于对角化算符。&lt;br /&gt;
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An important example of this is [[Fourier analysis]], which diagonalizes the heat equation using the [[eigenbasis]] of sinusoidal waves.&lt;br /&gt;
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An important example of this is Fourier analysis, which diagonalizes the heat equation using the eigenbasis of sinusoidal waves.&lt;br /&gt;
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这方面的一个重要例子是'''&amp;lt;font color = &amp;quot;#ff8000&amp;quot;&amp;gt;傅里叶分析  Fourier Analysis&amp;lt;/font&amp;gt;'''，它使用正弦波的特征基来对角化热方程。&lt;br /&gt;
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If the domain is finite or periodic, an infinite sum of solutions such as a [[Fourier series]] is appropriate, but an integral of solutions such as a [[Fourier integral]] is generally required for infinite domains. The solution for a point source for the heat equation given above is an example of the use of a Fourier integral.&lt;br /&gt;
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If the domain is finite or periodic, an infinite sum of solutions such as a Fourier series is appropriate, but an integral of solutions such as a Fourier integral is generally required for infinite domains. The solution for a point source for the heat equation given above is an example of the use of a Fourier integral.&lt;br /&gt;
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如果区域是有限的或周期性的，那么解为无限和的形式是恰当的，例如傅里叶级数，但是一个解的积分，例如傅立叶积分，一般是在无限区域上的。上面给出的热传导方程的点源解法就是使用傅里叶积分的一个例子。&lt;br /&gt;
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===Change of variables===&lt;br /&gt;
变量代换&lt;br /&gt;
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Often a PDE can be reduced to a simpler form with a known solution by a suitable [[Change of variables (PDE)|change of variables]].  For example, the [[Black–Scholes equation#Derivation|Black–Scholes]] PDE&lt;br /&gt;
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Often a PDE can be reduced to a simpler form with a known solution by a suitable change of variables.  For example, the Black–Scholes PDE&lt;br /&gt;
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偏微分方程通常可以通过变量的适当变化，用已知的解简化为更简单的形式。例如，布莱克-舒尔斯偏微分方程&lt;br /&gt;
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:&amp;lt;math&amp;gt; \frac{\partial V}{\partial t} + \tfrac{1}{2}\sigma^2 S^2\frac{\partial^2 V}{\partial S^2} + rS\frac{\partial V}{\partial S} - rV = 0 &amp;lt;/math&amp;gt;&lt;br /&gt;
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&amp;lt;math&amp;gt; \frac{\partial V}{\partial t} + \tfrac{1}{2}\sigma^2 S^2\frac{\partial^2 V}{\partial S^2} + rS\frac{\partial V}{\partial S} - rV = 0 &amp;lt;/math&amp;gt;&lt;br /&gt;
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is reducible to the [[heat equation]]&lt;br /&gt;
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is reducible to the heat equation&lt;br /&gt;
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可以简化为热传导方程&lt;br /&gt;
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:&amp;lt;math&amp;gt; \frac{\partial u}{\partial \tau} = \frac{\partial^2 u}{\partial x^2}&amp;lt;/math&amp;gt;&lt;br /&gt;
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&amp;lt;math&amp;gt; \frac{\partial u}{\partial \tau} = \frac{\partial^2 u}{\partial x^2}&amp;lt;/math&amp;gt;&lt;br /&gt;
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by the change of variables (for complete details see {{webarchive |url=https://web.archive.org/web/20080411030405/http://www.math.unl.edu/~sdunbar1/Teaching/MathematicalFinance/Lessons/BlackScholes/Solution/solution.shtml |date=April 11, 2008 |title=Solution of the Black Scholes Equation }})&lt;br /&gt;
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by the change of variables (for complete details see )&lt;br /&gt;
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通过变量替换(完整的细节见)&lt;br /&gt;
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:&amp;lt;math&amp;gt;\begin{align}&lt;br /&gt;
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V(S,t) &amp;amp;= K v(x,\tau),\\[5px]&lt;br /&gt;
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x &amp;amp;= \ln\left(\tfrac{S}{K} \right),\\[5px]&lt;br /&gt;
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\tau &amp;amp;= \tfrac{1}{2} \sigma^2 (T - t),\\[5px]&lt;br /&gt;
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v(x,\tau)&amp;amp;=e^{-\alpha x-\beta\tau} u(x,\tau).&lt;br /&gt;
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\end{align}&amp;lt;/math&amp;gt;&lt;br /&gt;
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===Fundamental solution===&lt;br /&gt;
基本解&lt;br /&gt;
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{{main|Fundamental solution}}&lt;br /&gt;
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Inhomogeneous equations can often be solved (for constant coefficient PDEs, always be solved) by finding the [[fundamental solution]] (the solution for a point source), then taking the [[convolution]] with the boundary conditions to get the solution.&lt;br /&gt;
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Inhomogeneous equations can often be solved (for constant coefficient PDEs, always be solved) by finding the fundamental solution (the solution for a point source), then taking the convolution with the boundary conditions to get the solution.&lt;br /&gt;
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非齐次方程(常系数偏微分方程)一般是通过先求出基本解(点源的解) ，然后利用带边界条件的卷积来求解。&lt;br /&gt;
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This is analogous in [[signal processing]] to understanding a filter by its [[impulse response]].&lt;br /&gt;
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This is analogous in signal processing to understanding a filter by its impulse response.&lt;br /&gt;
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这类似于在信号处理中通过滤波器的脉冲响应来理解滤波器。&lt;br /&gt;
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===Superposition principle===&lt;br /&gt;
叠加原理&lt;br /&gt;
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{{further| Superposition principle }}&lt;br /&gt;
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The superposition principle applies to any linear system, including linear systems of PDEs. A common visualization of this concept is the interaction of two waves in phase being combined to result in a greater amplitude, for example {{math|sin ''x'' + sin ''x'' {{=}} 2 sin ''x''}}. The same principle can be observed in PDEs where the solutions may be real or complex and additive. [[Superposition principle|superposition]]&lt;br /&gt;
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The superposition principle applies to any linear system, including linear systems of PDEs. A common visualization of this concept is the interaction of two waves in phase being combined to result in a greater amplitude, for example  2 sin x}}. The same principle can be observed in PDEs where the solutions may be real or complex and additive. superposition&lt;br /&gt;
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'''&amp;lt;font color = &amp;quot;#ff8000&amp;quot;&amp;gt;叠加原理 Superposition Principle&amp;lt;/font&amp;gt;适用于任何线性系统，包括偏微分方程的线性系统。这个概念的一个常见的可视化是两个同相位的波相互作用结合在一起会产生更大的振幅，例如 {{math|sin ''x'' + sin ''x'' {{=}} 2 sin ''x''}}。在偏微分方程中也可以观察到同样的原理，其中的解可能是真实的或复杂的和可加的。叠加&lt;br /&gt;
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If {{math|''u''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;}} and {{math|''u''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;}} are solutions of linear PDE in some function space {{mvar|R}}, then {{math|''u'' {{=}} ''c''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;''u''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; + ''c''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;''u''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;}} with any constants {{math|''c''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;}} and {{math|''c''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;}} are also a solution of that PDE in the same function space.&lt;br /&gt;
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If  and  are solutions of linear PDE in some function space , then  c&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;u&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; + c&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;u&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;}} with any constants  and  are also a solution of that PDE in the same function space.&lt;br /&gt;
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若线性偏微分方程在某个函数空间{{mvar|R}}中有解{{math|''u''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;}} 和 {{math|''u''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;}}，则{{math|''u'' {{=}} ''c''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;''u''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; + ''c''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;''u''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;}}也是该偏微分方程在同一函数空间中的解，其中{{math|''c''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;}} 和 {{math|''c''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;}} 是任意常数。&lt;br /&gt;
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===Methods for non-linear equations===&lt;br /&gt;
非线性方程的求解方法&lt;br /&gt;
{{see also|nonlinear partial differential equation}}&lt;br /&gt;
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There are no generally applicable methods to solve nonlinear PDEs. Still, existence and uniqueness results (such as the [[Cauchy–Kowalevski theorem]]) are often possible, as are proofs of important qualitative and quantitative properties of solutions (getting these results is a major part of [[mathematical analysis|analysis]]). Computational solution to the nonlinear PDEs, the [[split-step method]], exist for specific equations like [[nonlinear Schrödinger equation]].&lt;br /&gt;
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There are no generally applicable methods to solve nonlinear PDEs. Still, existence and uniqueness results (such as the Cauchy–Kowalevski theorem) are often possible, as are proofs of important qualitative and quantitative properties of solutions (getting these results is a major part of analysis). Computational solution to the nonlinear PDEs, the split-step method, exist for specific equations like nonlinear Schrödinger equation.&lt;br /&gt;
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对于非线性偏微分方程，目前还没有普遍适用的求解方法。然而，通常是可能知道解的存在性和唯一性(如柯西-科瓦列夫斯基定理)，也是可能得到解的重要定性和定量性质的证明(得到这些结果是分析的主要部分)。非线性偏微分方程的计算解，即分步法，对一些特定的方程适用，比如非线性'''&amp;lt;font color=&amp;quot;#ff8000&amp;quot;&amp;gt;薛定谔方程 Schrödinger equation&amp;lt;/font&amp;gt;'''。&lt;br /&gt;
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Nevertheless, some techniques can be used for several types of equations. The [[h-principle|{{mvar|h}}-principle]] is the most powerful method to solve [[Underdetermined system|underdetermined]] equations. The [[Riquier–Janet theory]] is an effective method for obtaining information about many analytic [[Overdetermined system|overdetermined]] systems.&lt;br /&gt;
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Nevertheless, some techniques can be used for several types of equations. The -principle is the most powerful method to solve underdetermined equations. The Riquier–Janet theory is an effective method for obtaining information about many analytic overdetermined systems.&lt;br /&gt;
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然而，一些技巧可以用于几种类型的方程。h-原理是求解欠定方程最有效的方法。里基尔-珍妮特理论是一种可以获得许多解析超定系统信息的有效方法。&lt;br /&gt;
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The [[method of characteristics]] can be used in some very special cases to solve partial differential equations.&lt;br /&gt;
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The method of characteristics can be used in some very special cases to solve partial differential equations.&lt;br /&gt;
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特征线法可用于求解某些特殊情况下的偏微分方程。&lt;br /&gt;
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In some cases, a PDE can be solved via [[perturbation analysis]] in which the solution is considered to be a correction to an equation with a known solution. Alternatives are [[numerical analysis]] techniques from simple [[finite difference]] schemes to the more mature [[multigrid]] and [[finite element method]]s. Many interesting problems in science and engineering are solved in this way using [[computer]]s, sometimes high performance [[supercomputer]]s.&lt;br /&gt;
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In some cases, a PDE can be solved via perturbation analysis in which the solution is considered to be a correction to an equation with a known solution. Alternatives are numerical analysis techniques from simple finite difference schemes to the more mature multigrid and finite element methods. Many interesting problems in science and engineering are solved in this way using computers, sometimes high performance supercomputers.&lt;br /&gt;
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在某些情况下，偏微分方程可以通过扰动分析来求解。在扰动分析中，通常是求解将具有已知解的方程修正后的新得到方程。可供选择的数值分析技术从简单的差分格式到更成熟的多重网格和有限元方法。许多有趣的科学和工程问题都是在计算机上用这种方法解决的，有时是高性能超级计算机。&lt;br /&gt;
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===Lie group method===&lt;br /&gt;
李群方法&lt;br /&gt;
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From 1870 [[Sophus Lie]]'s work put the theory of differential equations on a more satisfactory foundation. He showed that the integration theories of the older mathematicians can, by the introduction of what are now called [[Lie group]]s, be referred, to a common source; and that ordinary differential equations which admit the same [[infinitesimal transformation]]s present comparable difficulties of integration. He also emphasized the subject of [[contact transformation|transformations of contact]].&lt;br /&gt;
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From 1870 Sophus Lie's work put the theory of differential equations on a more satisfactory foundation. He showed that the integration theories of the older mathematicians can, by the introduction of what are now called Lie groups, be referred, to a common source; and that ordinary differential equations which admit the same infinitesimal transformations present comparable difficulties of integration. He also emphasized the subject of transformations of contact.&lt;br /&gt;
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从1870年起，索弗斯·李的工作为微分方程理论奠定了一个较为令人满意的基础。他指出，通过引入现在所谓的李群，老一辈数学家的积分理论可以引用到一个共同的来源; 承认相同的无穷小变换的常微分方程在积分方面存在相当的困难。他还强调了接触的转变这一主题。&lt;br /&gt;
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==[[用户:Yuling|Yuling]]（[[用户讨论:Yuling|讨论]]）这句话“He also emphasized the subject of transformations of contact.”中的transformations of contact翻译的不太好。&lt;br /&gt;
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A general approach to solving PDEs uses the symmetry property of differential equations, the continuous [[infinitesimal transformation]]s of solutions to solutions ([[Lie theory]]). Continuous [[group theory]], [[Lie algebras]] and [[differential geometry]] are used to understand the structure of linear and nonlinear partial differential equations for generating integrable equations, to find its [[Lax pair]]s, recursion operators, [[Bäcklund transform]] and finally finding exact analytic solutions to the PDE.&lt;br /&gt;
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A general approach to solving PDEs uses the symmetry property of differential equations, the continuous infinitesimal transformations of solutions to solutions (Lie theory). Continuous group theory, Lie algebras and differential geometry are used to understand the structure of linear and nonlinear partial differential equations for generating integrable equations, to find its Lax pairs, recursion operators, Bäcklund transform and finally finding exact analytic solutions to the PDE.&lt;br /&gt;
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求解偏微分方程的一般方法是利用微分方程的对称性，即解到解的连续无穷小变换(李理论)。连续群论、李代数和微分几何理论被用来理解生成可积方程的线性和非线性偏微分方程的结构，找到它的Lax对、递归算子、 贝克伦德变换，最后找到偏微分方程的精确解析解。&lt;br /&gt;
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Symmetry methods have been recognized to study differential equations arising in mathematics, physics, engineering, and many other disciplines.&lt;br /&gt;
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Symmetry methods have been recognized to study differential equations arising in mathematics, physics, engineering, and many other disciplines.&lt;br /&gt;
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对称方法已被公认可以用于研究出现在数学，物理，工程和许多其他学科的微分方程。&lt;br /&gt;
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===Semianalytical methods===&lt;br /&gt;
半解析方法&lt;br /&gt;
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The [[Adomian decomposition method]], the [[Aleksandr Lyapunov|Lyapunov]] artificial small parameter method, and He's [[homotopy perturbation method]] are all special cases of the more general [[homotopy analysis method]]. These are series expansion methods, and except for the Lyapunov method, are independent of small physical parameters as compared to the well known [[perturbation theory]], thus giving these methods greater flexibility and solution generality.&lt;br /&gt;
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The Adomian decomposition method, the Lyapunov artificial small parameter method, and He's homotopy perturbation method are all special cases of the more general homotopy analysis method. These are series expansion methods, and except for the Lyapunov method, are independent of small physical parameters as compared to the well known perturbation theory, thus giving these methods greater flexibility and solution generality.&lt;br /&gt;
&lt;br /&gt;
阿多米安分解法、李雅普诺夫人工小参数方法和何同伦摄动方法都是更一般的同伦分析方法的特殊情况。除了李雅普诺夫方法之外，这些都是级数展开方法，与为人熟知的摄动理论方法相比，它们与小的物理参数无关，因此这些方法具有更大的灵活性和解的通用性。&lt;br /&gt;
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== Numerical solutions ==&lt;br /&gt;
数值解&lt;br /&gt;
&lt;br /&gt;
The three most widely used [[Numerical partial differential equations|numerical methods to solve PDEs]] are the [[finite element analysis|finite element method]] (FEM), [[finite volume method]]s (FVM) and [[finite difference method]]s (FDM), as well other kind of methods called [[Meshfree methods]], which were made to solve problems where the before mentioned methods are limited. The FEM has a prominent position among these methods and especially its exceptionally efficient higher-order version [[hp-FEM]]. Other hybrid versions of FEM and Meshfree methods include the generalized finite element method (GFEM), [[extended finite element method]] (XFEM), [[Spectral element method|spectral finite element method]] (SFEM), [[Meshfree methods|meshfree finite element method]], [[Discontinuous Galerkin Method|discontinuous Galerkin finite element method]] (DGFEM), [[Element-Free Galerkin Method]] (EFGM), [[Interpolating Element-Free Galerkin Method]] (IEFGM), etc.&lt;br /&gt;
&lt;br /&gt;
The three most widely used numerical methods to solve PDEs are the finite element method (FEM), finite volume methods (FVM) and finite difference methods (FDM), as well other kind of methods called Meshfree methods, which were made to solve problems where the before mentioned methods are limited. The FEM has a prominent position among these methods and especially its exceptionally efficient higher-order version hp-FEM. Other hybrid versions of FEM and Meshfree methods include the generalized finite element method (GFEM), extended finite element method (XFEM), spectral finite element method (SFEM), meshfree finite element method, discontinuous Galerkin finite element method (DGFEM), Element-Free Galerkin Method (EFGM), Interpolating Element-Free Galerkin Method (IEFGM), etc.&lt;br /&gt;
&lt;br /&gt;
求解偏微分方程最常用的三种数值方法是有限元分析法、有限体积法和有限差分法，以及其他一些称为无网格法的方法。这些方法用于解决前面提到的方法受到的限制。在这些方法中，有限元方法，尤其是高效的高阶有限元方法，占有重要地位。其他有限元法和无网格法的混合形式包括广义有限元分析法(GFEM)、扩展有限元分析法(XFEM)、谱有限元分析法(SFEM)、无网格有限元分析法(DGFEM)、间断伽辽金有限元分析法(DGFEM)、无网格伽辽金法(EFGM)、插值无网格伽辽金法(IEFGM)等。&lt;br /&gt;
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=== Finite element method ===&lt;br /&gt;
有限元分析法&lt;br /&gt;
&lt;br /&gt;
{{main|Finite element method}}&lt;br /&gt;
&lt;br /&gt;
The finite element method (FEM) (its practical application often known as finite element analysis (FEA)) is a numerical technique for finding approximate solutions of partial differential equations (PDE) as well as of integral equations. The solution approach is based either on eliminating the differential equation completely (steady state problems), or rendering the PDE into an approximating system of ordinary differential equations, which are then numerically integrated using standard techniques such as Euler's method, Runge–Kutta, etc.&lt;br /&gt;
&lt;br /&gt;
The finite element method (FEM) (its practical application often known as finite element analysis (FEA)) is a numerical technique for finding approximate solutions of partial differential equations (PDE) as well as of integral equations. The solution approach is based either on eliminating the differential equation completely (steady state problems), or rendering the PDE into an approximating system of ordinary differential equations, which are then numerically integrated using standard techniques such as Euler's method, Runge–Kutta, etc.&lt;br /&gt;
&lt;br /&gt;
'''&amp;lt;font color = &amp;quot;#ff8000&amp;quot;&amp;gt;有限元分析法 Finite Element Method&amp;lt;/font&amp;gt;''' ((其实际应用通常被称为有限元分析(FEA))是一种寻找偏微分方程(PDE)和积分方程近似解的数值技术。这种求解方法要么基于完全消除微分方程(稳态问题) ，要么将偏微分方程转化为常微分方程的近似系统，然后使用标准技术进行数值积分，如欧拉方法、 Runge-Kutta 等。&lt;br /&gt;
&lt;br /&gt;
===Finite difference method===&lt;br /&gt;
有限差分法&lt;br /&gt;
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&lt;br /&gt;
{{main|Finite difference method}}&lt;br /&gt;
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Finite-difference methods are numerical methods for approximating the solutions to differential equations using [[finite difference]] equations to approximate derivatives.&lt;br /&gt;
&lt;br /&gt;
Finite-difference methods are numerical methods for approximating the solutions to differential equations using finite difference equations to approximate derivatives.&lt;br /&gt;
&lt;br /&gt;
有限差分法是一种数值方法，用差分方程近似微分方程的解。&lt;br /&gt;
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=== Finite volume method ===&lt;br /&gt;
有限体积法&lt;br /&gt;
&lt;br /&gt;
{{main|Finite volume method}}&lt;br /&gt;
&lt;br /&gt;
Similar to the finite difference method or finite element method, values are calculated at discrete places on a meshed geometry. &amp;quot;Finite volume&amp;quot; refers to the small volume surrounding each node point on a mesh. In the finite volume method, surface integrals in a partial differential equation that contain a divergence term are converted to volume integrals, using the [[divergence theorem]]. These terms are then evaluated as fluxes at the surfaces of each finite volume. Because the flux entering a given volume is identical to that leaving the adjacent volume, these methods conserve mass by design.&lt;br /&gt;
&lt;br /&gt;
Similar to the finite difference method or finite element method, values are calculated at discrete places on a meshed geometry. &amp;quot;Finite volume&amp;quot; refers to the small volume surrounding each node point on a mesh. In the finite volume method, surface integrals in a partial differential equation that contain a divergence term are converted to volume integrals, using the divergence theorem. These terms are then evaluated as fluxes at the surfaces of each finite volume. Because the flux entering a given volume is identical to that leaving the adjacent volume, these methods conserve mass by design.&lt;br /&gt;
&lt;br /&gt;
类似于有限差分法或有限元分析，函数值是在网状几何体上的离散位置进行计算的。“有限体积”是指网格上每个节点周围的小体积。在有限体积法中，偏微分方程中含有散度项的面积分用散度定理积分转换成体积分。然后将这些项用于估算每个有限体积表面上的通量。由于进入给定体积的通量与转移到相邻体积元的通量相同，所以这些方法在设计上保证了质量守恒。&lt;br /&gt;
&lt;br /&gt;
==See also==&lt;br /&gt;
请参阅&lt;br /&gt;
* [[Dirichlet boundary condition]]&lt;br /&gt;
狄利克雷边界条件&lt;br /&gt;
* [[Jet bundle]]&lt;br /&gt;
射流丛&lt;br /&gt;
* [[Laplace transform applied to differential equations]]&lt;br /&gt;
微分方程中的拉普拉斯变换&lt;br /&gt;
* [[List of dynamical systems and differential equations topics]]&lt;br /&gt;
动力学系统和微分方程的列表&lt;br /&gt;
* [[Matrix differential equation]]&lt;br /&gt;
矩阵微分方程&lt;br /&gt;
* [[Neumann boundary condition]]&lt;br /&gt;
诺伊曼边界条件&lt;br /&gt;
* [[Numerical partial differential equations]]&lt;br /&gt;
数值偏微分方程&lt;br /&gt;
* [[Partial differential algebraic equation]]&lt;br /&gt;
偏微分代数方程&lt;br /&gt;
* [[Recurrence relation]]&lt;br /&gt;
递推关系&lt;br /&gt;
* [[Robin boundary condition]]&lt;br /&gt;
罗宾边界条件&lt;br /&gt;
* [[Stochastic processes and boundary value problems]]&lt;br /&gt;
随机过程和边值问题&lt;br /&gt;
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== The energy method ==&lt;br /&gt;
能量法&lt;br /&gt;
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The energy method is a mathematical procedure that can be used to verify well-posedness of initial-boundary-value-problems.&amp;lt;ref&amp;gt;{{cite book |title=High Order Difference Methods for Time Dependent PDE&lt;br /&gt;
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The energy method is a mathematical procedure that can be used to verify well-posedness of initial-boundary-value-problems.&amp;lt;ref&amp;gt;{{cite book |title=High Order Difference Methods for Time Dependent PDE&lt;br /&gt;
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能量法是验证初边值问题适定性的一种数学方法。 时变偏微分方程的高阶差分方法&lt;br /&gt;
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|first=Bertil|last=Gustafsson|publisher=Springer|year=2008|isbn=978-3-540-74992-9|doi=10.1007/978-3-540-74993-6}}&amp;lt;/ref&amp;gt; In the following example the energy method is used to decide where and which boundary conditions should be imposed such that the resulting IBVP is well-posed. Consider the one-dimensional hyperbolic PDE given by&lt;br /&gt;
&lt;br /&gt;
|first=Bertil|last=Gustafsson|publisher=Springer|year=2008|isbn=978-3-540-74992-9|doi=10.1007/978-3-540-74993-6}}&amp;lt;/ref&amp;gt; In the following example the energy method is used to decide where and which boundary conditions should be imposed such that the resulting IBVP is well-posed. Consider the one-dimensional hyperbolic PDE given by&lt;br /&gt;
&lt;br /&gt;
| first Bertil | last Gustafsson | publisher | Springer | year 2008 | isbn 978-3-540-74992-9 | doi 10.1007 / 978-3-540-74993-6} / ref 在下面的例子中，使用能量方法来决定应该施加哪些边界条件，使得得到的 IBVP适定。考虑一维双曲偏微分方程&lt;br /&gt;
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: &amp;lt;math&amp;gt;\frac{\partial u}{\partial t} + \alpha \frac{\partial u}{\partial x} = 0, \quad x \in [a,b], \operatorname t &amp;gt; 0,&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;\frac{\partial u}{\partial t} + \alpha \frac{\partial u}{\partial x} = 0, \quad x \in [a,b], \operatorname t &amp;gt; 0,&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
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where &amp;lt;math&amp;gt;\alpha \neq 0&amp;lt;/math&amp;gt; is a constant and &amp;lt;math&amp;gt;u(x,t)&amp;lt;/math&amp;gt; is an unknown function with initial condition &amp;lt;math&amp;gt;u(x,0) = f(x)&amp;lt;/math&amp;gt;. Multiplying with &amp;lt;math&amp;gt;u&amp;lt;/math&amp;gt; and integrating over the domain gives&lt;br /&gt;
&lt;br /&gt;
where &amp;lt;math&amp;gt;\alpha \neq 0&amp;lt;/math&amp;gt; is a constant and &amp;lt;math&amp;gt;u(x,t)&amp;lt;/math&amp;gt; is an unknown function with initial condition &amp;lt;math&amp;gt;u(x,0) = f(x)&amp;lt;/math&amp;gt;. Multiplying with &amp;lt;math&amp;gt;u&amp;lt;/math&amp;gt; and integrating over the domain gives&lt;br /&gt;
&lt;br /&gt;
其中 &amp;lt;math&amp;gt;\alpha \neq 0&amp;lt;/math&amp;gt; 是常数，并且 &amp;lt;math&amp;gt;u(x,t)&amp;lt;/math&amp;gt; 是未知函数，初始条件是 &amp;lt;math&amp;gt;u(x,0) = f(x)&amp;lt;/math&amp;gt;。乘以 &amp;lt;math&amp;gt;u&amp;lt;/math&amp;gt; 并在域上进行积分。&lt;br /&gt;
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&lt;br /&gt;
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: &amp;lt;math&amp;gt;\int_a^b u \frac{\partial u}{\partial t} \operatorname dx + \alpha \int _a ^b u \frac{\partial u}{\partial x} \operatorname dx = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;\int_a^b u \frac{\partial u}{\partial t} \operatorname dx + \alpha \int _a ^b u \frac{\partial u}{\partial x} \operatorname dx = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
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Using that&lt;br /&gt;
&lt;br /&gt;
Using that&lt;br /&gt;
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利用这一点&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt;\int _a ^b u \frac{\partial u}{\partial t} \operatorname dx = \frac{1}{2} \frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 \quad \text{and} \quad \int _a ^b u \frac{\partial u}{\partial x} \operatorname dx = \frac{1}{2} u(b,t)^2 - \frac{1}{2} u(a,t)^2,.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;\int _a ^b u \frac{\partial u}{\partial t} \operatorname dx = \frac{1}{2} \frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 \quad \text{and} \quad \int _a ^b u \frac{\partial u}{\partial x} \operatorname dx = \frac{1}{2} u(b,t)^2 - \frac{1}{2} u(a,t)^2,.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
where integration by parts has been used for the second relationship, we get&lt;br /&gt;
&lt;br /&gt;
where integration by parts has been used for the second relationship, we get&lt;br /&gt;
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第二个关系中采用了分部积分法，我们可以得到&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt;\frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 + \alpha u(b,t)^2 - \alpha u(a,t)^2 = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;\frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 + \alpha u(b,t)^2 - \alpha u(a,t)^2 = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Here &amp;lt;math&amp;gt;\vert \vert \cdot \vert \vert&amp;lt;/math&amp;gt; denotes the standard L2-norm.&lt;br /&gt;
&lt;br /&gt;
Here &amp;lt;math&amp;gt;\vert \vert \cdot \vert \vert&amp;lt;/math&amp;gt; denotes the standard L2-norm.&lt;br /&gt;
&lt;br /&gt;
在这里，&amp;lt;math&amp;gt;\vert \vert \cdot \vert \vert&amp;lt;/math&amp;gt; 表示标准的 L2-正则。&lt;br /&gt;
&lt;br /&gt;
For well-posedness we require that the energy of the solution is non-increasing, i.e. that &amp;lt;math&amp;gt;\frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 \leq 0&amp;lt;/math&amp;gt;, which is achieved by specifying &amp;lt;math&amp;gt;u&amp;lt;/math&amp;gt; at &amp;lt;math&amp;gt;x = a&amp;lt;/math&amp;gt; if &amp;lt;math&amp;gt;\alpha &amp;gt; 0&amp;lt;/math&amp;gt; and at &amp;lt;math&amp;gt;x = b&amp;lt;/math&amp;gt; if &amp;lt;math&amp;gt;\alpha &amp;lt; 0&amp;lt;/math&amp;gt;. This corresponds to only imposing boundary conditions at the inflow. Note that well-posedness allows for growth in terms of data (initial and boundary) and thus it is sufficient to show that &amp;lt;math&amp;gt;\frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 \leq 0&amp;lt;/math&amp;gt; holds when all data is set to zero.&lt;br /&gt;
&lt;br /&gt;
For well-posedness we require that the energy of the solution is non-increasing, i.e. that &amp;lt;math&amp;gt;\frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 \leq 0&amp;lt;/math&amp;gt;, which is achieved by specifying &amp;lt;math&amp;gt;u&amp;lt;/math&amp;gt; at &amp;lt;math&amp;gt;x = a&amp;lt;/math&amp;gt; if &amp;lt;math&amp;gt;\alpha &amp;gt; 0&amp;lt;/math&amp;gt; and at &amp;lt;math&amp;gt;x = b&amp;lt;/math&amp;gt; if &amp;lt;math&amp;gt;\alpha &amp;lt; 0&amp;lt;/math&amp;gt;. This corresponds to only imposing boundary conditions at the inflow. Note that well-posedness allows for growth in terms of data (initial and boundary) and thus it is sufficient to show that &amp;lt;math&amp;gt;\frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 \leq 0&amp;lt;/math&amp;gt; holds when all data is set to zero.&lt;br /&gt;
&lt;br /&gt;
对于适定性，我们要解的能量是不增加的，即 &amp;lt;math&amp;gt;\frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 \leq 0&amp;lt;/math&amp;gt; ，这种关系可以通过在&amp;lt;math&amp;gt;x = a&amp;lt;/math&amp;gt;处 （如果 &amp;lt;math&amp;gt;\alpha &amp;gt; 0&amp;lt;/math&amp;gt;） 以及 &amp;lt;math&amp;gt;x = b&amp;lt;/math&amp;gt;处 （如果 &amp;lt;math&amp;gt;\alpha &amp;lt; 0&amp;lt;/math&amp;gt;）指定&amp;lt;math&amp;gt;u&amp;lt;/math&amp;gt;的值来实现。这只相当于在入流处附加边界条件。注意，适定性允许在数据(初始和边界)上的增长，因此它足以表明当所有数据设置为零时应有 &amp;lt;math&amp;gt;\frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 \leq 0&amp;lt;/math&amp;gt;。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==[[用户:Yuling|Yuling]]（[[用户讨论:Yuling|讨论]]）“This corresponds to only imposing boundary conditions at the inflow.” 这句话中的inflow不是很理解&lt;br /&gt;
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==Notes==&lt;br /&gt;
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{{Reflist}}&lt;br /&gt;
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== References ==&lt;br /&gt;
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{{refbegin|2}}&lt;br /&gt;
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&lt;br /&gt;
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&lt;br /&gt;
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* {{Citation |first=A. D. |last=Polyanin |first2=V. F. |last2=Zaitsev |lastauthoramp=yes |first3=A. |last3=Moussiaux |title=Handbook of First Order Partial Differential Equations |publisher=Taylor &amp;amp; Francis |location=London |year=2002 |isbn=0-415-27267-X }}.&lt;br /&gt;
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* {{citation|mr=3014456|last=Roubíček|first= T.|title=Nonlinear Partial Differential Equations with Applications|publisher= Birkhäuser|place= Basel, Boston, Berlin|edition=2nd|year= 2013|ISBN= 978-3-0348-0512-4|doi=10.1007/978-3-0348-0513-1|url=http://cds.cern.ch/record/880983/files/9783764372934_TOC.pdf}}&lt;br /&gt;
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* {{Citation |first=P. |last=Solin |title=Partial Differential Equations and the Finite Element Method |publisher=J. Wiley &amp;amp; Sons |location=Hoboken, NJ |year=2005 |isbn=0-471-72070-4 }}.&lt;br /&gt;
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* {{Citation |first=P. |last=Solin |first2=K. |last2=Segeth |lastauthoramp=yes |first3=I. |last3=Dolezel |title=Higher-Order Finite Element Methods |publisher=Chapman &amp;amp; Hall/CRC Press |location=Boca Raton |year=2003 |isbn=1-58488-438-X }}.&lt;br /&gt;
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* {{Citation |first=H. |last=Stephani |year=1989 |title=Differential Equations: Their Solution Using Symmetries. Edited by M. MacCallum |publisher=Cambridge University Press }}.&lt;br /&gt;
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* {{cite book |title=Partial Differential Equations and Solitary Waves Theory&lt;br /&gt;
&lt;br /&gt;
|first=Abdul-Majid|last=Wazwaz|publisher=Higher Education Press|year=2009|isbn=978-3-642-00251-9|page=}}&lt;br /&gt;
&lt;br /&gt;
|first=Abdul-Majid|last=Wazwaz|publisher=Higher Education Press|year=2009|isbn=978-3-642-00251-9|page=}}&lt;br /&gt;
&lt;br /&gt;
| first Abdul-Majid | last Wazwaz | publisher Higher Education Press | year 2009 | isbn 978-3-642-00251-9 | page }&lt;br /&gt;
&lt;br /&gt;
* {{cite book |title=Partial Differential Equations Methods and Applications&lt;br /&gt;
&lt;br /&gt;
|first=Abdul-Majid|last=Wazwaz|publisher=A.A. Balkema|year=2002|isbn=90-5809-369-7|page=}}&lt;br /&gt;
&lt;br /&gt;
|first=Abdul-Majid|last=Wazwaz|publisher=A.A. Balkema|year=2002|isbn=90-5809-369-7|page=}}&lt;br /&gt;
&lt;br /&gt;
| first Abdul-Majid | last Wazwaz | publisher a.a.Balkema | year 2002 | isbn 90-5809-369-7 | page }&lt;br /&gt;
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* {{Citation |first=D. |last=Zwillinger |title=Handbook of Differential Equations |publisher=Academic Press |location=Boston |year=1997 |edition=3rd |isbn=0-12-784395-7 }}.&lt;br /&gt;
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* {{Citation |authorlink=Neil Gershenfeld |first=N. |last=Gershenfeld |title=The Nature of Mathematical Modeling |location=New York |publisher=Cambridge University Press, New York, NY, USA |year=1999 |edition=1st |isbn=0-521-57095-6 }}.&lt;br /&gt;
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* {{Citation |first=I.S. |last=Krasil'shchik |lastauthoramp=yes |first2=A.M., Eds. |last2=Vinogradov |title=Symmetries and Conserwation Laws for Differential Equations of Mathematical Physics |publisher=American Mathematical Society, Providence, Rhode Island, USA |year=1999 |isbn=0-8218-0958-X }}.&lt;br /&gt;
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* {{Citation |first=I.S. |last=Krasil'shchik |first2=V.V. |last2=Lychagin|lastauthoramp=yes |first3=A.M. |last3=Vinogradov |title=Geometry of Jet Spaces and Nonlinear Partial Differential Equations |publisher=Gordon and Breach Science Publishers, New York, London, Paris, Montreux, Tokyo |year=1986 |isbn=2-88124-051-8 }}.&lt;br /&gt;
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* {{Citation |first=A.M. |last=Vinogradov |title=Cohomological Analysis of Partial Differential Equations and Secondary Calculus |publisher=American Mathematical Society, Providence, Rhode Island, USA |year=2001 |isbn=0-8218-2922-X }}.&lt;br /&gt;
&lt;br /&gt;
* {{cite book |title=High Order Difference Methods for Time Dependent PDE&lt;br /&gt;
&lt;br /&gt;
|first=Bertil|last=Gustafsson|publisher=Springer|year=2008|isbn=978-3-540-74992-9|doi=10.1007/978-3-540-74993-6}}&lt;br /&gt;
&lt;br /&gt;
|first=Bertil|last=Gustafsson|publisher=Springer|year=2008|isbn=978-3-540-74992-9|doi=10.1007/978-3-540-74993-6}}&lt;br /&gt;
&lt;br /&gt;
| first Bertil | last Gustafsson | Springer | year 2008 | isbn 978-3-540-74992-9 | doi 10.1007 / 978-3-540-74993-6}&lt;br /&gt;
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{{refend}}&lt;br /&gt;
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== Further reading ==&lt;br /&gt;
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* {{Cite journal|last=Cajori|first=Florian|authorlink=Florian Cajori|year=1928|title=The Early History of Partial Differential Equations and of Partial Differentiation and Integration|url=http://www.math.harvard.edu/archive/21a_fall_14/exhibits/cajori/cajori.pdf|journal=The American Mathematical Monthly|volume=35|issue=9|pages=459–467|doi=10.2307/2298771|access-date=2016-05-15|archive-url=https://web.archive.org/web/20181123102253/http://www.math.harvard.edu/archive/21a_fall_14/exhibits/cajori/cajori.pdf|archive-date=2018-11-23|url-status=dead}}&lt;br /&gt;
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== External links ==&lt;br /&gt;
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{{Sister project links| wikt=no | commons=Category:Solutions of PDE | b=Partial Differential Equations | n=no | q=Partial differential equation | s=no | v=no | voy=no | species=no | d=no}}&lt;br /&gt;
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* {{springer|title=Differential equation, partial|id=p/d031920}}&lt;br /&gt;
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* [http://eqworld.ipmnet.ru/en/pde-en.htm Partial Differential Equations: Exact Solutions] at EqWorld: The World of Mathematical Equations.&lt;br /&gt;
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* [http://eqworld.ipmnet.ru/en/solutions/eqindex/eqindex-pde.htm Partial Differential Equations: Index] at EqWorld: The World of Mathematical Equations.&lt;br /&gt;
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* [http://eqworld.ipmnet.ru/en/methods/meth-pde.htm Partial Differential Equations: Methods] at EqWorld: The World of Mathematical Equations.&lt;br /&gt;
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* [https://web.archive.org/web/20170701144823/http://www.exampleproblems.com/wiki/index.php?title=Partial_Differential_Equations Example problems with solutions] at exampleproblems.com&lt;br /&gt;
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* [http://mathworld.wolfram.com/PartialDifferentialEquation.html Partial Differential Equations] at mathworld.wolfram.com&lt;br /&gt;
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* [https://reference.wolfram.com/language/FEMDocumentation/tutorial/SolvingPDEwithFEM.html Partial Differential Equations] with Mathematica&lt;br /&gt;
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* [http://www.mathworks.com/moler/pdes.pdf Partial Differential Equations] in Cleve Moler: Numerical Computing with MATLAB&lt;br /&gt;
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* [http://www.nag.com/numeric/fl/nagdoc_fl24/html/D03/d03intro.html Partial Differential Equations] at nag.com&lt;br /&gt;
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* {{cite web |first=Grant |last=Sanderson |title=But what is a partial differential equation? |work=3Blue1Brown |date=April 21, 2019 |url=https://www.youtube.com/watch?v=ly4S0oi3Yz8&amp;amp;list=PLZHQObOWTQDNPOjrT6KVlfJuKtYTftqH6 |via=[[YouTube]] }}&lt;br /&gt;
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{{Differential equations topics}}&lt;br /&gt;
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[[Category:Partial differential equations| ]]&lt;br /&gt;
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[[Category:Multivariable calculus]]&lt;br /&gt;
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Category:Multivariable calculus&lt;br /&gt;
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类别: 多元微积分&lt;br /&gt;
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[[Category:Differential equations]]&lt;br /&gt;
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Category:Differential equations&lt;br /&gt;
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类别: 微分方程&lt;br /&gt;
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[[Category:Concepts in physics]]&lt;br /&gt;
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Category:Concepts in physics&lt;br /&gt;
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&amp;lt;small&amp;gt;This page was moved from [[wikipedia:en:Partial differential equation]]. Its edit history can be viewed at [[偏微分方程/edithistory]]&amp;lt;/small&amp;gt;&amp;lt;/noinclude&amp;gt;&lt;br /&gt;
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[[Category:待整理页面]]&lt;/div&gt;</summary>
		<author><name>Ruili</name></author>
	</entry>
	<entry>
		<id>https://wiki.swarma.org/index.php?title=%E5%81%8F%E5%BE%AE%E5%88%86%E6%96%B9%E7%A8%8B&amp;diff=18118</id>
		<title>偏微分方程</title>
		<link rel="alternate" type="text/html" href="https://wiki.swarma.org/index.php?title=%E5%81%8F%E5%BE%AE%E5%88%86%E6%96%B9%E7%A8%8B&amp;diff=18118"/>
		<updated>2020-11-11T13:36:40Z</updated>

		<summary type="html">&lt;p&gt;Ruili：&lt;/p&gt;
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&lt;div&gt;此词条暂由Yuling翻译，未经人工整理和审校，带来阅读不便，请见谅。&lt;br /&gt;
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[[File:Heat.gif|thumb|right|A visualisation of a solution to the two-dimensional [[heat equation]] with temperature represented by the third dimension]]&lt;br /&gt;
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A visualisation of a solution to the two-dimensional [[heat equation with temperature represented by the third dimension]]&lt;br /&gt;
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以三维表示温度的二维热方程解的可视化&lt;br /&gt;
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In [[mathematics]], a '''partial differential equation''' ('''PDE''') is a [[differential equation]] that contains unknown [[Multivariable calculus|multivariable functions]] and their [[partial derivative]]s. PDEs are used to formulate problems involving functions of several variables, and are either solved by hand, or used to create a [[computer model]]. A special case is [[ordinary differential equation]]s (ODEs), which deal with functions of a single variable and their derivatives.&lt;br /&gt;
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In mathematics, a partial differential equation (PDE) is a differential equation that contains unknown multivariable functions and their partial derivatives. PDEs are used to formulate problems involving functions of several variables, and are either solved by hand, or used to create a computer model. A special case is ordinary differential equations (ODEs), which deal with functions of a single variable and their derivatives.&lt;br /&gt;
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在数学中，'''&amp;lt;font color = &amp;quot;#ff8000&amp;quot;&amp;gt;偏微分方程函数 Partial Differential Equation&amp;lt;/font&amp;gt;'''是包含未知多元函数及其偏导数的微分方程。偏微分方程用于描述涉及多元函数的问题，可以通过人为求解，也可以通过建立计算机模型来求解。常微分方程是偏微分方程一种特殊情况，它处理的是一元函数及其导数。&lt;br /&gt;
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PDEs can be used to describe a wide variety of phenomena such as sound, heat, [[diffusion]], [[electrostatics]], [[Electromagnetism|electrodynamics]], [[fluid dynamics]], [[Elasticity (physics)|elasticity]], [[gravitation]] and [[quantum mechanics]]. These seemingly distinct physical phenomena can be formalised similarly in terms of PDEs. Just as ordinary differential equations often model one-dimensional [[dynamical system]]s, partial differential equations often model [[multidimensional system]]s. PDEs find their generalisation in [[stochastic partial differential equation]]s.&lt;br /&gt;
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PDEs can be used to describe a wide variety of phenomena such as sound, heat, diffusion, electrostatics, electrodynamics, fluid dynamics, elasticity, gravitation and quantum mechanics. These seemingly distinct physical phenomena can be formalised similarly in terms of PDEs. Just as ordinary differential equations often model one-dimensional dynamical systems, partial differential equations often model multidimensional systems. PDEs find their generalisation in stochastic partial differential equations.&lt;br /&gt;
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偏微分方程可以用来描述各种各样的物理现象，如声音，热量，扩散，静电，电动力学，流体力学，弹性力学，重力和量子力学。这些看起来截然不同的物理现象却可以用类似的偏微分方程来描述。正如常微分方程经常对一维动力系统进行建模一样，偏微分方程经常对多维系统进行建模。随机偏微分方程是偏微分方程的一种推广。&lt;br /&gt;
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== Introduction ==&lt;br /&gt;
引言&lt;br /&gt;
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Partial differential equations (PDEs) are equations that involve rates of change with respect to [[continuous variables]]. For example, the position of a [[rigid body]] is specified by six parameters,&amp;lt;ref&amp;gt;{{Cite book|url=https://books.google.com/books?id=v9PLbcYd9aUC&amp;amp;pg=PA32|title=Modelling and Control of Robot Manipulators|last=Sciavicco|first=Lorenzo|last2=Siciliano|first2=Bruno|date=2001-02-19|publisher=Springer Science &amp;amp; Business Media|isbn=9781852332211|language=en}}&amp;lt;/ref&amp;gt; but the configuration of a [[fluid]] is given by the [[continuous distribution]] of several parameters, such as the [[temperature]], [[pressure]], and so forth. The dynamics for the rigid body take place in a finite-dimensional [[Configuration space (physics)|configuration space]]; the dynamics for the fluid occur in an infinite-dimensional configuration space. This distinction usually makes PDEs much harder to solve than ordinary differential equations (ODEs), but here again, there will be simple solutions for linear problems. Classic domains where PDEs are used include [[acoustics]], [[fluid dynamics]], [[electrodynamics]], and [[heat transfer]].&lt;br /&gt;
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Partial differential equations (PDEs) are equations that involve rates of change with respect to continuous variables. For example, the position of a rigid body is specified by six parameters, but the configuration of a fluid is given by the continuous distribution of several parameters, such as the temperature, pressure, and so forth. The dynamics for the rigid body take place in a finite-dimensional configuration space; the dynamics for the fluid occur in an infinite-dimensional configuration space. This distinction usually makes PDEs much harder to solve than ordinary differential equations (ODEs), but here again, there will be simple solutions for linear problems. Classic domains where PDEs are used include acoustics, fluid dynamics, electrodynamics, and heat transfer.&lt;br /&gt;
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偏微分方程(简称为PDEs)涉及到方程相对于连续变量的变化率。例如，刚体的位置是由六个参数确定的，而流体的状态是由几个参数的连续分布给出的，如温度、压力等。刚体的动力学过程发生在有限维状态空间中，流体的动力学过程发生在无限维状态空间中。这种区别通常使偏微分方程比常微分方程更难求解，但是线性问题仍然有简单的求解方式。使用偏微分方程的经典领域包括声学、流体力学、电动力学和传热学。&lt;br /&gt;
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A partial differential equation (PDE) for the function {{math|''u''(''x''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;,… ''x&amp;lt;sub&amp;gt;n&amp;lt;/sub&amp;gt;'')}} is an equation of the form&lt;br /&gt;
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A partial differential equation (PDE) for the function  is an equation of the form&lt;br /&gt;
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函数{{math|''u''(''x''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;,… ''x&amp;lt;sub&amp;gt;n&amp;lt;/sub&amp;gt;'')}}的偏微分方程形式是：&lt;br /&gt;
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: &amp;lt;math&amp;gt;f \left (x_1, \ldots x_n; u, \frac{\partial u}{\partial x_1}, \ldots \frac{\partial u}{\partial x_n}; \frac{\partial^2 u}{\partial x_1 \partial x_1}, \ldots \frac{\partial^2 u}{\partial x_1 \partial x_n}; \ldots \right) = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;f \left (x_1, \ldots x_n; u, \frac{\partial u}{\partial x_1}, \ldots \frac{\partial u}{\partial x_n}; \frac{\partial^2 u}{\partial x_1 \partial x_1}, \ldots \frac{\partial^2 u}{\partial x_1 \partial x_n}; \ldots \right) = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
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If {{mvar|f}} is a [[linear function]] of {{mvar|u}} and its derivatives, then the PDE is called linear. Common examples of linear PDEs include the [[heat equation]], the [[wave equation]], [[Laplace's equation]], [[Helmholtz equation]], [[Klein–Gordon equation]], and [[Poisson's equation]].&lt;br /&gt;
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If  is a linear function of  and its derivatives, then the PDE is called linear. Common examples of linear PDEs include the heat equation, the wave equation, Laplace's equation, Helmholtz equation, Klein–Gordon equation, and Poisson's equation.&lt;br /&gt;
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如果 {{mvar|f}}是函数{{math|''u''}} 及其导数的线性函数，则偏微分方程称为线性函数。线性偏微分方程的常见例子包括热方程、波动方程、拉普拉斯方程、亥姆霍兹方程方程、克莱因-高登方程和泊松方程。&lt;br /&gt;
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A relatively simple PDE is&lt;br /&gt;
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A relatively simple PDE is&lt;br /&gt;
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一个相对简单的偏微分方程：&lt;br /&gt;
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: &amp;lt;math&amp;gt;\frac{\partial u}{\partial x}(x,y) = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;\frac{\partial u}{\partial x}(x,y) = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
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This relation [[Logical implication|implies]] that the function {{math|''u''(''x'',''y'')}} is independent of {{mvar|x}}. However, the equation gives no information on the function's dependence on the variable {{mvar|y}}. Hence the general solution of this equation is&lt;br /&gt;
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This relation implies that the function  is independent of . However, the equation gives no information on the function's dependence on the variable . Hence the general solution of this equation is&lt;br /&gt;
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这意味着函数 {{math|''u''(''x'',''y'')}} 独立于 {{mvar|x}} 的。然而，这个方程没有给出关于函数和自变量的相关性的信息。因此，这个方程的通解是&lt;br /&gt;
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: &amp;lt;math&amp;gt;u(x,y) = f(y),&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;u(x,y) = f(y),&amp;lt;/math&amp;gt;&lt;br /&gt;
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where {{mvar|f}} is an arbitrary function of {{mvar|y}}. The analogous ordinary differential equation is&lt;br /&gt;
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where  is an arbitrary function of . The analogous ordinary differential equation is&lt;br /&gt;
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其中， {{mvar|f}} 是 {{mvar|y}} 的任意函数。&lt;br /&gt;
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类似的常微分方程是：&lt;br /&gt;
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: &amp;lt;math&amp;gt;\frac{\mathrm{d} u}{\mathrm{d} x}(x) = 0,&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;\frac{\mathrm{d} u}{\mathrm{d} x}(x) = 0,&amp;lt;/math&amp;gt;&lt;br /&gt;
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which has the solution&lt;br /&gt;
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which has the solution&lt;br /&gt;
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它的解为&lt;br /&gt;
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: &amp;lt;math&amp;gt;u(x) = c,&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;u(x) = c,&amp;lt;/math&amp;gt;&lt;br /&gt;
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where {{mvar|c}} is any [[Constant (mathematics)|constant]] value. These two examples illustrate that general solutions of ordinary differential equations (ODEs) involve arbitrary constants, but solutions of PDEs involve arbitrary functions.&lt;br /&gt;
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where  is any constant value. These two examples illustrate that general solutions of ordinary differential equations (ODEs) involve arbitrary constants, but solutions of PDEs involve arbitrary functions.&lt;br /&gt;
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这里，{{mvar|c}} 是一个任意常量。&lt;br /&gt;
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这两个例子说明常微分方程的一般解包含任意常数，但偏微分方程的解包含任意函数。&lt;br /&gt;
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A solution of a PDE is generally not [[Uniqueness quantification|unique]]; additional conditions must generally be specified on the [[Boundary (topology)|boundary]] of the region where the solution is defined. For instance, in the simple example above, the function {{math|''f''(''y'')}} can be determined if {{mvar|u}} is specified on the line {{math|''x'' {{=}} 0}}.&lt;br /&gt;
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A solution of a PDE is generally not unique; additional conditions must generally be specified on the boundary of the region where the solution is defined. For instance, in the simple example above, the function  can be determined if  is specified on the line  0}}.&lt;br /&gt;
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偏微分方程的解一般不是唯一的; 一般必须在定义解的区域边界上定义附加条件。 例如，在上面的简单示例中，如果在 {{math|''x'' {{=}} 0}} 时确定了 {{mvar|u}} 的值，则可以确定该函数 {{math|''f''(''y'')}}。&lt;br /&gt;
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== Existence and uniqueness ==&lt;br /&gt;
存在性和唯一性&lt;br /&gt;
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Although the issue of existence and uniqueness of solutions of ordinary differential equations has a very satisfactory answer with the [[Picard–Lindelöf theorem]], that is far from the case for partial differential equations. The [[Cauchy–Kowalevski theorem]] states that the [[Cauchy problem]] for any partial differential equation whose coefficients are [[Analytic function|analytic]] in the unknown function and its derivatives, has a locally unique analytic solution. Although this result might appear to settle the existence and uniqueness of solutions, there are examples of linear partial differential equations whose coefficients have derivatives of all orders (which are nevertheless not analytic) but which have no solutions at all: see [[Lewy's example|Lewy (1957)]]. Even if the solution of a partial differential equation exists and is unique, it may nevertheless have undesirable properties.  The mathematical study of these questions is usually in the more powerful context of [[weak solution]]s.&lt;br /&gt;
&lt;br /&gt;
Although the issue of existence and uniqueness of solutions of ordinary differential equations has a very satisfactory answer with the Picard–Lindelöf theorem, that is far from the case for partial differential equations. The Cauchy–Kowalevski theorem states that the Cauchy problem for any partial differential equation whose coefficients are analytic in the unknown function and its derivatives, has a locally unique analytic solution. Although this result might appear to settle the existence and uniqueness of solutions, there are examples of linear partial differential equations whose coefficients have derivatives of all orders (which are nevertheless not analytic) but which have no solutions at all: see Lewy (1957). Even if the solution of a partial differential equation exists and is unique, it may nevertheless have undesirable properties.  The mathematical study of these questions is usually in the more powerful context of weak solutions.&lt;br /&gt;
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虽然常微分方程解的存在唯一性问题用'''&amp;lt;font color=&amp;quot;#ff8000&amp;quot;&amp;gt;弗罗贝尼乌斯定理 Picard–Lindelöf Theorem&amp;lt;/font&amp;gt;得到了令人满意的结果，但应用到偏微分方程上却不尽如意。'''&amp;lt;font color=&amp;quot;#ff8000&amp;quot;&amp;gt;柯西-科瓦列夫斯基定理 Cauchy–Kowalevski theorem&amp;lt;/font&amp;gt;指出，对于任何在未知函数及其导数中系数是解析的偏微分方程，柯西问题有一个局部唯一的解析解。虽然这个结果似乎解决了解的存在性和唯一性问题，但是有一些线性偏微分方程的系数具有所有级数的导数(尽管这些导数不是解析的) ，但是根本没有解: 见 Lewy (1957)。即使偏微分方程的解存在且唯一，它仍然可能具有人们所不希望的性质。这些问题的数学研究通常是在更有力的弱解的背景下进行的。&lt;br /&gt;
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An example of pathological behavior is the sequence (depending upon {{mvar|n}}) of [[Cauchy problem]]s for the [[Laplace equation]]&lt;br /&gt;
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An example of pathological behavior is the sequence (depending upon ) of Cauchy problems for the Laplace equation&lt;br /&gt;
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反常特征的一个例子是拉普拉斯方程的柯西问题的序列(取决于{{mvar|n}})&lt;br /&gt;
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: &amp;lt;math&amp;gt;\frac{\partial^2 u}{\partial x^2} + \frac{\partial^2 u}{\partial y^2}=0,&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;\frac{\partial^2 u}{\partial x^2} + \frac{\partial^2 u}{\partial y^2}=0,&amp;lt;/math&amp;gt;&lt;br /&gt;
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with [[boundary condition]]s&lt;br /&gt;
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with boundary conditions&lt;br /&gt;
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有边界条件&lt;br /&gt;
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: &amp;lt;math&amp;gt;\begin{align} u(x,0) &amp;amp;= 0, \\ \frac{\partial u}{\partial y}(x,0) &amp;amp;= \frac{\sin nx}{n}, \end{align}&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;\begin{align} u(x,0) &amp;amp;= 0, \\ \frac{\partial u}{\partial y}(x,0) &amp;amp;= \frac{\sin nx}{n}, \end{align}&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
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where {{mvar|n}} is an integer. The derivative of {{mvar|u}} with respect to {{mvar|y}} approaches zero [[uniform convergence|uniformly]] in {{mvar|x}} as {{mvar|n}} increases, but the solution is&lt;br /&gt;
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where  is an integer. The derivative of  with respect to  approaches zero uniformly in  as  increases, but the solution is&lt;br /&gt;
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其中{{mvar|n}}是整数。{{mvar|u}}是关于{{mvar|y}}的导数，一致地随着{{mvar|n}}的增加而趋于零，但是解是&lt;br /&gt;
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: &amp;lt;math&amp;gt;u(x,y) = \frac{\sinh ny \sin nx}{n^2}.&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;u(x,y) = \frac{\sinh ny \sin nx}{n^2}.&amp;lt;/math&amp;gt;&lt;br /&gt;
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This solution approaches infinity if {{mvar|nx}} is not an integer multiple of {{pi}} for any non-zero value of {{mvar|y}}. The Cauchy problem for the Laplace equation is called ''ill-posed'' or ''not [[Well-posed problem|well-posed]]'', since the solution does not continuously depend on the data of the problem. Such ill-posed problems are not usually satisfactory for physical applications.&lt;br /&gt;
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This solution approaches infinity if  is not an integer multiple of  for any non-zero value of . The Cauchy problem for the Laplace equation is called ill-posed or not well-posed, since the solution does not continuously depend on the data of the problem. Such ill-posed problems are not usually satisfactory for physical applications.&lt;br /&gt;
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对于任何非零的{{mvar|y}}，如果{{mvar|nx}}不是{{pi}}的整数倍，这个解会接近于无穷大。拉普拉斯方程的柯西问题被称为不适定问题（可以译为ill-posed或not well-posed），因为该问题的解并不连续地依赖于该问题的数据。这种不适定问题在物理应用中通常不能令人满意。&lt;br /&gt;
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The [[Navier–Stokes existence and smoothness|existence of solutions for the Navier–Stokes equations]], a partial differential equation, is part of one of the [[Millennium Prize Problems]].&lt;br /&gt;
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The existence of solutions for the Navier–Stokes equations, a partial differential equation, is part of one of the Millennium Prize Problems.&lt;br /&gt;
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一种偏微分方程——纳维-斯托克斯方程——的解的存在性就是千禧年大奖难题的一部分。&lt;br /&gt;
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== Notation ==&lt;br /&gt;
符号&lt;br /&gt;
&lt;br /&gt;
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In PDEs, it is common to denote partial derivatives using subscripts. That is:&lt;br /&gt;
&lt;br /&gt;
In PDEs, it is common to denote partial derivatives using subscripts. That is:&lt;br /&gt;
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在偏微分方程中，通常用下标表示偏导数。例如:&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt;u_x = \frac{\partial u}{\partial x}&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;u_x = \frac{\partial u}{\partial x}&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt;u_{xx} = \frac{\partial^2 u}{\partial x^2} &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;u_{xx} = \frac{\partial^2 u}{\partial x^2} &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
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: &amp;lt;math&amp;gt;u_{xy} = \frac{\partial^2 u}{\partial y\, \partial x} = \frac{\partial}{\partial y } \left(\frac{\partial u}{\partial x}\right). &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;u_{xy} = \frac{\partial^2 u}{\partial y\, \partial x} = \frac{\partial}{\partial y } \left(\frac{\partial u}{\partial x}\right). &amp;lt;/math&amp;gt;&lt;br /&gt;
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Especially in physics, [[del]] or nabla ({{math|∇}}) is often used to denote spatial derivatives, and {{math|''&amp;amp;#x307;u'', ''ü''}} for time derivatives. For example, the [[wave equation]] (mentioned below) can be written as&lt;br /&gt;
&lt;br /&gt;
Especially in physics, del or nabla () is often used to denote spatial derivatives, and  for time derivatives. For example, the wave equation (mentioned below) can be written as&lt;br /&gt;
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特别是在物理学中，[[del]]或nabla ({{math|∇}})经常用来表示空间导数和时间导数。例如，波动方程(在下文中提到)可以写成&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
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:&amp;lt;math&amp;gt;\ddot u=c^2\nabla^2u&amp;lt;/math&amp;gt;&lt;br /&gt;
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&amp;lt;math&amp;gt;\ddot u=c^2\nabla^2u&amp;lt;/math&amp;gt;&lt;br /&gt;
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or&lt;br /&gt;
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or&lt;br /&gt;
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或&lt;br /&gt;
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:&amp;lt;math&amp;gt;\ddot u=c^2\Delta u&amp;lt;/math&amp;gt;&lt;br /&gt;
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&amp;lt;math&amp;gt;\ddot u=c^2\Delta u&amp;lt;/math&amp;gt;&lt;br /&gt;
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where {{math|Δ}} is the [[Laplace operator]].&lt;br /&gt;
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where  is the Laplace operator.&lt;br /&gt;
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其中{{math|Δ}}代表拉普拉斯算子&lt;br /&gt;
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== Classification ==&lt;br /&gt;
分类&lt;br /&gt;
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Some linear, second-order partial differential equations can be classified as [[parabolic partial differential equation|parabolic]], [[hyperbolic partial differential equation|hyperbolic]] and [[elliptic partial differential equation|elliptic]]. Others, such as the [[Euler–Tricomi equation]], have different types in different regions. The classification provides a guide to appropriate initial and boundary conditions and to the smoothness of the solutions.&lt;br /&gt;
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Some linear, second-order partial differential equations can be classified as parabolic, hyperbolic and elliptic. Others, such as the Euler–Tricomi equation, have different types in different regions. The classification provides a guide to appropriate initial and boundary conditions and to the smoothness of the solutions.&lt;br /&gt;
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一些线性二阶偏微分方程可分为抛物型方程、双曲型方程和椭圆型方程。其他的方程，如欧拉-特里科米方程，在不同的区域有不同的类型。这种分类有助于选择适当的初始和边界条件以及提高解的平滑性。&lt;br /&gt;
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=== Equations of first order ===&lt;br /&gt;
一阶方程&lt;br /&gt;
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{{main|First-order partial differential equation}}&lt;br /&gt;
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=== Linear equations of second order ===&lt;br /&gt;
二阶线性方程&lt;br /&gt;
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Assuming {{math|''u&amp;lt;sub&amp;gt;xy&amp;lt;/sub&amp;gt;'' {{=}} ''u&amp;lt;sub&amp;gt;yx&amp;lt;/sub&amp;gt;''}}, the general linear second-order PDE in two independent variables has the form&lt;br /&gt;
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Assuming  u&amp;lt;sub&amp;gt;yx&amp;lt;/sub&amp;gt;}}, the general linear second-order PDE in two independent variables has the form&lt;br /&gt;
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假设 {{math|''u&amp;lt;sub&amp;gt;xy&amp;lt;/sub&amp;gt;'' {{=}} ''u&amp;lt;sub&amp;gt;yx&amp;lt;/sub&amp;gt;''}}，含有两个独立变量的一般的线性二阶偏微分方程具有如下这样的形式&lt;br /&gt;
&lt;br /&gt;
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: &amp;lt;math&amp;gt;Au_{xx} + 2Bu_{xy} + Cu_{yy} + \cdots \mbox{(lower order terms)} = 0,&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;Au_{xx} + 2Bu_{xy} + Cu_{yy} + \cdots \mbox{(lower order terms)} = 0,&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
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where the coefficients {{mvar|A}}, {{mvar|B}}, {{mvar|C}}... may depend upon {{mvar|x}} and {{mvar|y}}. If {{math|''A''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; + ''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; + ''C''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; &amp;gt; 0}} over a region of the {{mvar|xy}}-plane, the PDE is second-order in that region. This form is analogous to the equation for a conic section:&lt;br /&gt;
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where the coefficients , , ... may depend upon  and . If  over a region of the -plane, the PDE is second-order in that region. This form is analogous to the equation for a conic section:&lt;br /&gt;
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其中的系数 {{mvar|A}}, {{mvar|B}}, {{mvar|C}}... 一般取决于{{mvar|x}}和{{mvar|y}}。如果在{{mvar|xy}}-平面的一个区域上 {{math|''A''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; + ''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; + ''C''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; &amp;gt; 0}}，偏微分方程在该区域是二阶的。这种形式类似于圆锥曲线的方程:&lt;br /&gt;
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: &amp;lt;math&amp;gt;Ax^2 + 2Bxy + Cy^2 + \cdots = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;Ax^2 + 2Bxy + Cy^2 + \cdots = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
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More precisely, replacing {{math|∂&amp;lt;sub&amp;gt;''x''&amp;lt;/sub&amp;gt;}} by {{mvar|X}}, and likewise for other variables (formally this is done by a [[Fourier transform]]), converts a constant-coefficient PDE into a polynomial of the same degree, with the terms of the highest degree (a [[homogeneous polynomial]], here a [[quadratic form]]) being most significant for the classification.&lt;br /&gt;
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More precisely, replacing  by , and likewise for other variables (formally this is done by a Fourier transform), converts a constant-coefficient PDE into a polynomial of the same degree, with the terms of the highest degree (a homogeneous polynomial, here a quadratic form) being most significant for the classification.&lt;br /&gt;
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更准确地说，用 {{mvar|X}} 替换 {{math|∂&amp;lt;sub&amp;gt;''x''&amp;lt;/sub&amp;gt;}}，对于其他变量做同样的操作(从形式上来说，这是由傅里叶变换来完成的)，将一个常系数偏微分方程转换成一个相同次数的多项式，最高次数的项(齐次多项式，这里是一个二次形式)一般会用于偏微分方程的分类。&lt;br /&gt;
===~~ most significant for the classification 意译为用于偏微分方程的分类。       significiant直译过来感觉不太合适&lt;br /&gt;
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Just as one classifies [[conic section]]s and quadratic forms into parabolic, hyperbolic, and elliptic based on the [[discriminant]] {{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − 4''AC''}}, the same can be done for a second-order PDE at a given point.  However, the [[discriminant]] in a PDE is given by {{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC''}} due to the convention of the {{mvar|xy}} term being {{math|2''B''}} rather than {{mvar|B}}; formally, the discriminant (of the associated quadratic form) is {{math|(2''B'')&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − 4''AC'' {{=}} 4(''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC'')}}, with the factor of 4 dropped for simplicity.&lt;br /&gt;
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Just as one classifies conic sections and quadratic forms into parabolic, hyperbolic, and elliptic based on the discriminant , the same can be done for a second-order PDE at a given point.  However, the discriminant in a PDE is given by  due to the convention of the  term being  rather than ; formally, the discriminant (of the associated quadratic form) is  4(B&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − AC)}}, with the factor of 4 dropped for simplicity.&lt;br /&gt;
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正如人们可以根据判别式 {{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − 4''AC''}} 将圆锥曲线和二次型分为抛物型、双曲型和椭圆型一样，对于给定点的二阶偏微分方程也可以这样做。然而，偏微分方程中的判别式 {{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − 4''AC''}} 是根据交叉项的系数{{math|2''B''}} 而不是 {{mvar|B}} 给出的，形式上，判别式(关联二次型)是 {{math|(2''B'')&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − 4''AC'' {{=}} 4(''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC'')}}，为简单起见，去掉了因子4。&lt;br /&gt;
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# {{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC'' &amp;lt; 0}} (''[[elliptic partial differential equation]]''): Solutions of [[elliptic partial differential equation|elliptic PDEs]] are as smooth as the coefficients allow, within the interior of the region where the equation and solutions are defined. For example, solutions of [[Laplace's equation]] are analytic within the domain where they are defined, but solutions may assume boundary values that are not smooth. The motion of a fluid at subsonic speeds can be approximated with elliptic PDEs, and the Euler–Tricomi equation is elliptic where {{math|''x'' &amp;lt; 0}}.&lt;br /&gt;
&lt;br /&gt;
  (elliptic partial differential equation): Solutions of elliptic PDEs are as smooth as the coefficients allow, within the interior of the region where the equation and solutions are defined. For example, solutions of Laplace's equation are analytic within the domain where they are defined, but solutions may assume boundary values that are not smooth. The motion of a fluid at subsonic speeds can be approximated with elliptic PDEs, and the Euler–Tricomi equation is elliptic where .&lt;br /&gt;
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{{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC'' &amp;lt; 0}} (椭圆形微分方程)：在定义方程和解的区域内部，椭圆型偏微分方程的解光滑到系数允许的程度。例如，拉普拉斯方程的解在它们被定义的区域内是解析的，但是解可能假设边界值是不光滑的。亚音速流体的运动可以用椭圆偏微分方程近似，其中欧拉-特里科米方程在 {{math|''x'' &amp;lt; 0}} 时是椭圆型偏微分方程。&lt;br /&gt;
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# {{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC'' {{=}} 0}} (''[[parabolic partial differential equation]]''): Equations that are [[parabolic partial differential equation|parabolic]] at every point can be transformed into a form analogous to the [[heat equation]] by a change of independent variables. Solutions smooth out as the transformed time variable increases. The Euler–Tricomi equation has parabolic type on the line where {{math|''x'' {{=}} 0}}.&lt;br /&gt;
&lt;br /&gt;
  0}} (parabolic partial differential equation): Equations that are parabolic at every point can be transformed into a form analogous to the heat equation by a change of independent variables. Solutions smooth out as the transformed time variable increases. The Euler–Tricomi equation has parabolic type on the line where  0}}.&lt;br /&gt;
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{{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC'' {{=}} 0}}（抛物线形偏微分方程）：在每一点上都是抛物线型的方程可以通过改变自变量从而转化成类似于热方程的形式。随着转换后的时间变量的增加，方程的解变得平滑。欧拉-特里科米方程在 {{math|''x'' {{=}} 0}} 这条特征线上是抛物线形的。&lt;br /&gt;
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# {{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC'' &amp;gt; 0}} (''[[hyperbolic partial differential equation]]''): [[hyperbolic partial differential equation|hyperbolic]] equations retain any discontinuities of functions or derivatives in the initial data. An example is the [[wave equation]]. The motion of a fluid at supersonic speeds can be approximated with hyperbolic PDEs, and the Euler–Tricomi equation is hyperbolic where {{math|''x'' &amp;gt; 0}}.&lt;br /&gt;
&lt;br /&gt;
  (hyperbolic partial differential equation): hyperbolic equations retain any discontinuities of functions or derivatives in the initial data. An example is the wave equation. The motion of a fluid at supersonic speeds can be approximated with hyperbolic PDEs, and the Euler–Tricomi equation is hyperbolic where .&lt;br /&gt;
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{{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC'' &amp;gt; 0}} (双曲形偏微分方程)：双曲形方程在初始数据中保留了函数或导数的任何不连续性，波动方程就是其中的一个例子。超音速流体的运动可以用双曲形偏微分方程近似，其中欧拉-特里科米方程在 {{math|''x'' &amp;gt; 0}} 时是双曲型的。&lt;br /&gt;
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&lt;br /&gt;
&lt;br /&gt;
If there are {{mvar|n}} independent variables {{math|''x''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;, ''x''&amp;lt;sub&amp;gt;2 &amp;lt;/sub&amp;gt;,… ''x''&amp;lt;sub&amp;gt;''n''&amp;lt;/sub&amp;gt;}}, a general linear partial differential equation of second order has the form&lt;br /&gt;
&lt;br /&gt;
If there are  independent variables , a general linear partial differential equation of second order has the form&lt;br /&gt;
&lt;br /&gt;
如果存在 {{mvar|n}} 个自变量 {{math|''x''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;, ''x''&amp;lt;sub&amp;gt;2 &amp;lt;/sub&amp;gt;,… ''x''&amp;lt;sub&amp;gt;''n''&amp;lt;/sub&amp;gt;}}，一般二阶线性偏微分方程的形式是&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt;L u =\sum_{i=1}^n\sum_{j=1}^n a_{i,j} \frac{\partial^2 u}{\partial x_i \partial x_j} \quad \text{ plus lower-order terms} =0.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;L u =\sum_{i=1}^n\sum_{j=1}^n a_{i,j} \frac{\partial^2 u}{\partial x_i \partial x_j} \quad \text{ plus lower-order terms} =0.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The classification depends upon the signature of the eigenvalues of the coefficient matrix {{math|''a''&amp;lt;sub&amp;gt;''i'',''j''&amp;lt;/sub&amp;gt;}}.&lt;br /&gt;
&lt;br /&gt;
The classification depends upon the signature of the eigenvalues of the coefficient matrix .&lt;br /&gt;
&lt;br /&gt;
这种分类取决于系数矩阵本征值的符号（正负性）。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
# Elliptic: the eigenvalues are all positive or all negative.&lt;br /&gt;
&lt;br /&gt;
 Elliptic: the eigenvalues are all positive or all negative.&lt;br /&gt;
&lt;br /&gt;
椭圆形方程: 本征值全部为正或全部为负。&lt;br /&gt;
&lt;br /&gt;
# Parabolic: the eigenvalues are all positive or all negative, save one that is zero.&lt;br /&gt;
&lt;br /&gt;
 Parabolic: the eigenvalues are all positive or all negative, save one that is zero.&lt;br /&gt;
&lt;br /&gt;
抛物线形方程: 本征值全部为正或全部为负，除了一个为零。&lt;br /&gt;
&lt;br /&gt;
# Hyperbolic: there is only one negative eigenvalue and all the rest are positive, or there is only one positive eigenvalue and all the rest are negative.&lt;br /&gt;
&lt;br /&gt;
 Hyperbolic: there is only one negative eigenvalue and all the rest are positive, or there is only one positive eigenvalue and all the rest are negative.&lt;br /&gt;
&lt;br /&gt;
双曲形方程: 只有一个负特征值，其余的都是正特征值，或者只有一个正特征值，其余的都是负特征值。&lt;br /&gt;
&lt;br /&gt;
# Ultrahyperbolic: there is more than one positive eigenvalue and more than one negative eigenvalue, and there are no zero eigenvalues. There is only a limited theory for ultrahyperbolic equations (Courant and Hilbert, 1962).&lt;br /&gt;
&lt;br /&gt;
 Ultrahyperbolic: there is more than one positive eigenvalue and more than one negative eigenvalue, and there are no zero eigenvalues. There is only a limited theory for ultrahyperbolic equations (Courant and Hilbert, 1962).&lt;br /&gt;
&lt;br /&gt;
超双形方程: 存在多于一个正本征值和多于一个的负本征值，且不存在零本征值。对于超双曲方程，只存在一个有限理论(Courant 和 Hilbert，1962)。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==[[用户:Yuling|Yuling]]（[[用户讨论:Yuling|讨论]]） 我对于limited theory这个单词对应的相关理论不太了解。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
=== Systems of first-order equations and characteristic surfaces ===&lt;br /&gt;
一阶方程组和特征曲面&lt;br /&gt;
&lt;br /&gt;
The classification of partial differential equations can be extended to systems of first-order equations, where the unknown {{mvar|u}} is now a [[Euclidean vector|vector]] with {{mvar|m}} components, and the coefficient matrices {{mvar|A&amp;lt;sub&amp;gt;ν&amp;lt;/sub&amp;gt;}} are {{mvar|m}} by {{mvar|m}} matrices for {{math|''ν'' {{=}} 1, 2,… ''n''}}. The partial differential equation takes the form&lt;br /&gt;
&lt;br /&gt;
The classification of partial differential equations can be extended to systems of first-order equations, where the unknown  is now a vector with  components, and the coefficient matrices  are  by  matrices for  1, 2,… n}}. The partial differential equation takes the form&lt;br /&gt;
&lt;br /&gt;
偏微分方程组的分类可以推广到一阶方程组，其中未知量 {{mvar|u}} 是有 {{mvar|m}} 个分量的向量。对于 {{math|''ν'' {{=}} 1, 2,… ''n''}}，系数矩阵 {{mvar|A&amp;lt;sub&amp;gt;ν&amp;lt;/sub&amp;gt;}} 是 {{mvar|m}} × {{mvar|m}} 的矩阵。偏微分方程形式如下：&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt;Lu = \sum_{\nu=1}^{n} A_\nu \frac{\partial u}{\partial x_\nu} + B=0,&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;Lu = \sum_{\nu=1}^{n} A_\nu \frac{\partial u}{\partial x_\nu} + B=0,&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
where the coefficient matrices {{mvar|A&amp;lt;sub&amp;gt;ν&amp;lt;/sub&amp;gt;}} and the vector {{mvar|B}} may depend upon {{mvar|x}} and {{mvar|u}}. If a [[hypersurface]] {{mvar|S}} is given in the implicit form&lt;br /&gt;
&lt;br /&gt;
where the coefficient matrices  and the vector  may depend upon  and . If a hypersurface  is given in the implicit form&lt;br /&gt;
&lt;br /&gt;
其中系数矩阵 {{mvar|A&amp;lt;sub&amp;gt;ν&amp;lt;/sub&amp;gt;}} 和向量 {{mvar|B}} 可能依赖于 {{mvar|x}} 和 {{mvar|u}}。如果超曲面是以隐式形式给出的&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt;\varphi(x_1, x_2, \ldots x_n)=0,&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;\varphi(x_1, x_2, \ldots x_n)=0,&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
where {{mvar|φ}} has a non-zero gradient, then {{mvar|S}} is a '''characteristic surface''' for the operator {{mvar|L}} at a given point if the characteristic form vanishes:&lt;br /&gt;
&lt;br /&gt;
where  has a non-zero gradient, then  is a characteristic surface for the operator  at a given point if the characteristic form vanishes:&lt;br /&gt;
&lt;br /&gt;
其中存在一个非零的梯度，那么如果特征形式消失，则在给定点上算子的特征曲面形式如下:&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt;Q\left(\frac{\partial\varphi}{\partial x_1}, \ldots\frac{\partial\varphi}{\partial x_n}\right) =\det\left[\sum_{\nu=1}^nA_\nu \frac{\partial \varphi}{\partial x_\nu}\right]=0.\,&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;Q\left(\frac{\partial\varphi}{\partial x_1}, \ldots\frac{\partial\varphi}{\partial x_n}\right) =\det\left[\sum_{\nu=1}^nA_\nu \frac{\partial \varphi}{\partial x_\nu}\right]=0.\,&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The geometric interpretation of this condition is as follows: if data for {{mvar|u}} are prescribed on the surface {{mvar|S}}, then it may be possible to determine the normal derivative of {{mvar|u}} on {{mvar|S}} from the differential equation. If the data on {{mvar|S}} and the differential equation determine the normal derivative of {{mvar|u}} on {{mvar|S}}, then {{mvar|S}} is non-characteristic. If the data on {{mvar|S}} and the differential equation ''do not'' determine the normal derivative of {{mvar|u}} on {{mvar|S}}, then the surface is '''characteristic''', and the differential equation restricts the data on {{mvar|S}}: the differential equation is ''internal'' to {{mvar|S}}.&lt;br /&gt;
&lt;br /&gt;
The geometric interpretation of this condition is as follows: if data for  are prescribed on the surface , then it may be possible to determine the normal derivative of  on  from the differential equation. If the data on  and the differential equation determine the normal derivative of  on , then  is non-characteristic. If the data on  and the differential equation do not determine the normal derivative of  on , then the surface is characteristic, and the differential equation restricts the data on : the differential equation is internal to .&lt;br /&gt;
&lt;br /&gt;
这个条件的几何解释如下: 如果关于 {{mvar|u}} 的数据是在曲面 {{mvar|S}} 上规定的，那么就有可能依据微分方程确定曲面 {{mvar|S}} 上 {{mvar|u}} 的法向导数。如果曲面 {{mvar|S}} 上的数据和上面的微分方程能确定曲面 {{mvar|S}} 上 {{mvar|u}} 的法向导数，那么它就是非特征的。如果曲面 {{mvar|S}} 上的数据和上面的微分方程不能确定曲面 {{mvar|S}} 上 {{mvar|u}} 的法向导数，那么曲面是特征的，并且微分方程将数据限制在曲面 {{mvar|S}} 上：微分方程是在曲面 {{mvar|S}} 内部。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
# A first-order system {{math|''Lu'' {{=}} 0}} is ''elliptic'' if no surface is characteristic for {{mvar|L}}: the values of {{mvar|u}} on {{mvar|S}} and the differential equation always determine the normal derivative of {{mvar|u}} on {{mvar|S}}.&lt;br /&gt;
&lt;br /&gt;
 A first-order system  0}} is elliptic if no surface is characteristic for : the values of  on  and the differential equation always determine the normal derivative of  on .&lt;br /&gt;
&lt;br /&gt;
如果对于 {{mvar|L}} 没有曲面是特征的，则一阶系统 {{math|''Lu'' {{=}} 0}} 是椭圆形的：{{mvar|u}}在 {{mvar|S}} 的值和微分方程总能够决定 {{mvar|S}} 上 {{mvar|u}} 的法向导数。&lt;br /&gt;
&lt;br /&gt;
# A first-order system is ''hyperbolic'' at a point if there is a '''spacelike''' surface {{mvar|S}} with normal {{mvar|ξ}} at that point. This means that, given any non-trivial vector {{mvar|η}} orthogonal to {{mvar|ξ}}, and a scalar multiplier {{mvar|λ}}, the equation {{math|''Q''(''λξ'' + ''η'') {{=}} 0}} has {{mvar|m}} real roots {{math|''λ''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;, ''λ''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;,… ''λ''&amp;lt;sub&amp;gt;''m''&amp;lt;/sub&amp;gt;}}. The system is '''strictly hyperbolic''' if these roots are always distinct. The geometrical interpretation of this condition is as follows: the characteristic form {{math|''Q''(''ζ'') {{=}} 0}} defines a cone (the normal cone) with homogeneous coordinates ζ. In the hyperbolic case, this cone has {{mvar|m}} sheets, and the axis {{math|''ζ'' {{=}} ''λξ''}} runs inside these sheets: it does not intersect any of them. But when displaced from the origin by η, this axis intersects every sheet. In the elliptic case, the normal cone has no real sheets.&lt;br /&gt;
&lt;br /&gt;
 A first-order system is hyperbolic at a point if there is a spacelike surface  with normal  at that point. This means that, given any non-trivial vector  orthogonal to , and a scalar multiplier , the equation  0}} has  real roots . The system is strictly hyperbolic if these roots are always distinct. The geometrical interpretation of this condition is as follows: the characteristic form  0}} defines a cone (the normal cone) with homogeneous coordinates ζ. In the hyperbolic case, this cone has  sheets, and the axis  λξ}} runs inside these sheets: it does not intersect any of them. But when displaced from the origin by η, this axis intersects every sheet. In the elliptic case, the normal cone has no real sheets.&lt;br /&gt;
&lt;br /&gt;
如果在该点存在一个法向量为 {{mvar|ξ}}的 '''&amp;lt;font color=&amp;quot;#ff8000&amp;quot;&amp;gt;类空曲面 Spacclike Surface&amp;lt;/font&amp;gt; {{mvar|S}} ，则一阶系统在那一点是双曲的。这意味着，给定任意正交于 {{mvar|ξ}} 的非平凡向量 {{mvar|η}} 和一个标量乘子 {{mvar|λ}}，方程 {{math|''Q''(''λξ'' + ''η'') {{=}} 0}} 有 {{mvar|m}} 个实根 {{math|''λ''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;, ''λ''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;,… ''λ''&amp;lt;sub&amp;gt;''m''&amp;lt;/sub&amp;gt;}}。如果这些根始终不同，则该系统是严格双曲形的。这个条件的几何解释如下: 特征形式 {{math|''Q''(''ζ'') {{=}} 0}} 定义了一个具有齐次坐标 ζ的圆锥(法线圆锥)。在双曲形的情况下，这个圆锥体有 {{mvar|m}} 层，并且轴 {{math|''ζ'' {{=}} ''λξ''}} 在这些层中运动: 它不与任何一层相交。但是当从原点偏离η时，这条轴线与每一层都相交。在椭圆形的情况下，法向圆锥没有实层。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==[[用户:Yuling|Yuling]]（[[用户讨论:Yuling|讨论]]） sheet 这个单词也不很理解，我直译为了“层”&lt;br /&gt;
&lt;br /&gt;
=== Equations of mixed type ===&lt;br /&gt;
混合型方程&lt;br /&gt;
&lt;br /&gt;
If a PDE has coefficients that are not constant, it is possible that it will not belong to any of these categories but rather be of '''mixed type'''. A simple but important example is the [[Euler–Tricomi equation]]&lt;br /&gt;
&lt;br /&gt;
If a PDE has coefficients that are not constant, it is possible that it will not belong to any of these categories but rather be of mixed type. A simple but important example is the Euler–Tricomi equation&lt;br /&gt;
&lt;br /&gt;
如果偏微分方程的系数不是常数，那么它可能不属于这些类别中的任何一个，而是属于混合类型。一个简单但重要的例子是欧拉-特里科米方程&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt;u_{xx} = xu_{yy},&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;u_{xx} = xu_{yy},&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
which is called '''elliptic-hyperbolic''' because it is elliptic in the region {{math|''x'' &amp;lt; 0}}, hyperbolic in the region {{math|''x'' &amp;gt; 0}}, and degenerate parabolic on the line {{math|''x'' {{=}} 0}}.&lt;br /&gt;
&lt;br /&gt;
which is called elliptic-hyperbolic because it is elliptic in the region , hyperbolic in the region , and degenerate parabolic on the line  0}}.&lt;br /&gt;
&lt;br /&gt;
它在 {{math|''x'' &amp;lt; 0}} 的区域上是椭圆形，在 {{math|''x'' &amp;gt; 0}} 区域上是双曲形，在 {{math|''x'' {{=}} 0}}这条线上是退化为抛物线形，因此称之为椭圆-双曲型。&lt;br /&gt;
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&amp;lt;!--&lt;br /&gt;
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&amp;lt;!--&lt;br /&gt;
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&amp;lt;!--&lt;br /&gt;
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''fill in: Dirichlet and Neumann boundaries, hyperbolic/parabolic/elliptic separation of variables, [[Fourier analysis]], [[Green's function]]s ...--&amp;gt;&lt;br /&gt;
&lt;br /&gt;
fill in: Dirichlet and Neumann boundaries, hyperbolic/parabolic/elliptic separation of variables, Fourier analysis, Green's functions ...--&amp;gt;&lt;br /&gt;
&lt;br /&gt;
填写: Dirichlet 和 Neumann 边界，双曲 / 抛物线 / 椭圆分离变量法，傅立叶分析，Green 函数... --&lt;br /&gt;
&lt;br /&gt;
=== Infinite-order PDEs in quantum mechanics ===&lt;br /&gt;
量子力学中的无限阶偏微分方程&lt;br /&gt;
&lt;br /&gt;
In the [[phase space formulation]] of quantum mechanics,  one may consider the [[Method of quantum characteristics|quantum Hamilton's equations]] for trajectories of quantum particles. These equations are infinite-order PDEs. However, in the semiclassical expansion, one has a finite system of ODEs at any fixed order of [[Dirac constant|{{mvar|ħ}}]].  The evolution equation of the [[Wigner quasi-probability distribution|c]] is also an infinite-order PDE. The quantum trajectories are [[Method of quantum characteristics|quantum characteristics]], with the use of which one could calculate the evolution of the Wigner function.&lt;br /&gt;
&lt;br /&gt;
In the phase space formulation of quantum mechanics,  one may consider the quantum Hamilton's equations for trajectories of quantum particles. These equations are infinite-order PDEs. However, in the semiclassical expansion, one has a finite system of ODEs at any fixed order of Dirac constant|.  The evolution equation of the Wigner function is also an infinite-order PDE. The quantum trajectories are quantum characteristics, with the use of which one could calculate the evolution of the Wigner function.&lt;br /&gt;
&lt;br /&gt;
在量子力学中的相空间表述中，我们可以考虑用于求解量子粒子的轨迹的量子哈密顿的方程。这些方程是无限阶偏微分方程。然而，在半经典展开中，我们在给定[[Dirac constant|{{mvar|ħ}}]]阶数下有一个有限的的常微分方程组。'''&amp;lt;font color=&amp;quot;#ff8000&amp;quot;&amp;gt;维格纳函数  Wigner Function&amp;lt;/font&amp;gt;的演化方程也是一个无限阶偏微分方程。由于量子轨道的量子特性，所以它通常可以用来计算维格纳函数的演化。&lt;br /&gt;
&lt;br /&gt;
== Analytical solutions ==&lt;br /&gt;
解析解&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
===Separation of variables===&lt;br /&gt;
分离变量法&lt;br /&gt;
&lt;br /&gt;
{{main|Separable partial differential equation}}&lt;br /&gt;
&lt;br /&gt;
Linear PDEs can be reduced to systems of ordinary differential equations by the important technique of separation of variables. This technique rests on a characteristic of solutions to differential equations: if one can find any solution that solves the equation and satisfies the boundary conditions, then it is ''the'' solution (this also applies to ODEs). We assume as an [[ansatz]] that the dependence of a solution on the parameters space and time can be written as a product of terms that each depend on a single parameter, and then see if this can be made to solve the problem.&amp;lt;ref&amp;gt;{{cite book|last1=Gershenfeld|first1=Neil|title=The nature of mathematical modeling|date=2000|publisher=Cambridge Univ. Press|location=Cambridge|isbn=0521570956|page=27|edition=Reprinted (with corr.)}}&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
Linear PDEs can be reduced to systems of ordinary differential equations by the important technique of separation of variables. This technique rests on a characteristic of solutions to differential equations: if one can find any solution that solves the equation and satisfies the boundary conditions, then it is the solution (this also applies to ODEs). We assume as an ansatz that the dependence of a solution on the parameters space and time can be written as a product of terms that each depend on a single parameter, and then see if this can be made to solve the problem.&lt;br /&gt;
&lt;br /&gt;
线性偏微分方程组可以通过分离变量法这一重要方法来简化为常微分方程组。这种方法依赖于微分方程解的一个特征: 如果能找到任何一个满足方程和边界条件的解，那么这个解就是方程的解(这也适用于常微分方程)。我们假设解对参数空间和时间的依赖可以写成对它们每一项的依赖以及一个参数的乘积，然后再看看这是否可以用来解决这个问题。&lt;br /&gt;
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&lt;br /&gt;
&lt;br /&gt;
In the method of separation of variables, one reduces a PDE to a PDE in fewer variables, which is an ordinary differential equation if in one variable – these are in turn easier to solve.&lt;br /&gt;
&lt;br /&gt;
In the method of separation of variables, one reduces a PDE to a PDE in fewer variables, which is an ordinary differential equation if in one variable – these are in turn easier to solve.&lt;br /&gt;
&lt;br /&gt;
在分离变量法方法中，可以将偏微分方程简化为含有更少变量的偏微分方程，如果只有一个变量，那么就变成了一个'''&amp;lt;font color = &amp;quot;#ff8000&amp;quot;&amp;gt;常微分方程 Ordinary Differential Equation&amp;lt;/font&amp;gt;'''-- 反过来，这些方程也更容易求解。&lt;br /&gt;
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This is possible for simple PDEs, which are called [[separable partial differential equation]]s, and the domain is generally a rectangle (a product of intervals). Separable PDEs correspond to [[diagonal matrices]] – thinking of &amp;quot;the value for fixed {{mvar|x}}&amp;quot; as a coordinate, each coordinate can be understood separately.&lt;br /&gt;
&lt;br /&gt;
This is possible for simple PDEs, which are called separable partial differential equations, and the domain is generally a rectangle (a product of intervals). Separable PDEs correspond to diagonal matrices – thinking of &amp;quot;the value for fixed &amp;quot; as a coordinate, each coordinate can be understood separately.&lt;br /&gt;
&lt;br /&gt;
对于简单的偏微分方程(称为可分离偏微分方程)来说，这是可能的，而且方程通常定义在一个矩形区域(区间的乘积)上。可分离偏微分方程对应于对角线矩阵——以“固定值”为坐标，每个坐标可分开理解。&lt;br /&gt;
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This generalizes to the [[method of characteristics]], and is also used in [[integral transform]]s.&lt;br /&gt;
&lt;br /&gt;
This generalizes to the method of characteristics, and is also used in integral transforms.&lt;br /&gt;
&lt;br /&gt;
这种方法可以推广到特征曲线法，也可以用于积分变换。&lt;br /&gt;
&lt;br /&gt;
===Method of characteristics===&lt;br /&gt;
特征曲线法&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{{main|Method of characteristics}}&lt;br /&gt;
&lt;br /&gt;
In special cases, one can find characteristic curves on which the equation reduces to an ODE – changing coordinates in the domain to straighten these curves allows separation of variables, and is called the [[method of characteristics]].&lt;br /&gt;
&lt;br /&gt;
In special cases, one can find characteristic curves on which the equation reduces to an ODE – changing coordinates in the domain to straighten these curves allows separation of variables, and is called the method of characteristics.&lt;br /&gt;
&lt;br /&gt;
在特殊情况下，可以找到一些特征曲线，在这些曲线上方程可以变成一个常微分方程——意味着改变坐标从而使这些曲线变直从而达到分离变量的目的，这就是所谓的特征曲线法。&lt;br /&gt;
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More generally, one may find characteristic surfaces.&lt;br /&gt;
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More generally, one may find characteristic surfaces.&lt;br /&gt;
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更一般地说，人们可能会找到特征表面。&lt;br /&gt;
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===Integral transform===&lt;br /&gt;
积分变换&lt;br /&gt;
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An [[integral transform]] may transform the PDE to a simpler one, in particular, a separable PDE. This corresponds to diagonalizing an operator.&lt;br /&gt;
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An integral transform may transform the PDE to a simpler one, in particular, a separable PDE. This corresponds to diagonalizing an operator.&lt;br /&gt;
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积分变换可以将偏微分方程转换为更简单的偏微分方程，特别是可分离的偏微分方程。这对应于对角化算符。&lt;br /&gt;
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An important example of this is [[Fourier analysis]], which diagonalizes the heat equation using the [[eigenbasis]] of sinusoidal waves.&lt;br /&gt;
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An important example of this is Fourier analysis, which diagonalizes the heat equation using the eigenbasis of sinusoidal waves.&lt;br /&gt;
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这方面的一个重要例子是'''&amp;lt;font color = &amp;quot;#ff8000&amp;quot;&amp;gt;傅里叶分析  Fourier Analysis&amp;lt;/font&amp;gt;'''，它使用正弦波的特征基来对角化热方程。&lt;br /&gt;
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If the domain is finite or periodic, an infinite sum of solutions such as a [[Fourier series]] is appropriate, but an integral of solutions such as a [[Fourier integral]] is generally required for infinite domains. The solution for a point source for the heat equation given above is an example of the use of a Fourier integral.&lt;br /&gt;
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If the domain is finite or periodic, an infinite sum of solutions such as a Fourier series is appropriate, but an integral of solutions such as a Fourier integral is generally required for infinite domains. The solution for a point source for the heat equation given above is an example of the use of a Fourier integral.&lt;br /&gt;
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如果区域是有限的或周期性的，那么解为无限和的形式是恰当的，例如傅里叶级数，但是一个解的积分，例如傅立叶积分，一般是在无限区域上的。上面给出的热传导方程的点源解法就是使用傅里叶积分的一个例子。&lt;br /&gt;
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===Change of variables===&lt;br /&gt;
变量代换&lt;br /&gt;
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Often a PDE can be reduced to a simpler form with a known solution by a suitable [[Change of variables (PDE)|change of variables]].  For example, the [[Black–Scholes equation#Derivation|Black–Scholes]] PDE&lt;br /&gt;
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Often a PDE can be reduced to a simpler form with a known solution by a suitable change of variables.  For example, the Black–Scholes PDE&lt;br /&gt;
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偏微分方程通常可以通过变量的适当变化，用已知的解简化为更简单的形式。例如，布莱克-舒尔斯偏微分方程&lt;br /&gt;
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:&amp;lt;math&amp;gt; \frac{\partial V}{\partial t} + \tfrac{1}{2}\sigma^2 S^2\frac{\partial^2 V}{\partial S^2} + rS\frac{\partial V}{\partial S} - rV = 0 &amp;lt;/math&amp;gt;&lt;br /&gt;
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&amp;lt;math&amp;gt; \frac{\partial V}{\partial t} + \tfrac{1}{2}\sigma^2 S^2\frac{\partial^2 V}{\partial S^2} + rS\frac{\partial V}{\partial S} - rV = 0 &amp;lt;/math&amp;gt;&lt;br /&gt;
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is reducible to the [[heat equation]]&lt;br /&gt;
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is reducible to the heat equation&lt;br /&gt;
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可以简化为热传导方程&lt;br /&gt;
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:&amp;lt;math&amp;gt; \frac{\partial u}{\partial \tau} = \frac{\partial^2 u}{\partial x^2}&amp;lt;/math&amp;gt;&lt;br /&gt;
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&amp;lt;math&amp;gt; \frac{\partial u}{\partial \tau} = \frac{\partial^2 u}{\partial x^2}&amp;lt;/math&amp;gt;&lt;br /&gt;
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by the change of variables (for complete details see {{webarchive |url=https://web.archive.org/web/20080411030405/http://www.math.unl.edu/~sdunbar1/Teaching/MathematicalFinance/Lessons/BlackScholes/Solution/solution.shtml |date=April 11, 2008 |title=Solution of the Black Scholes Equation }})&lt;br /&gt;
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by the change of variables (for complete details see )&lt;br /&gt;
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通过变量替换(完整的细节见)&lt;br /&gt;
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:&amp;lt;math&amp;gt;\begin{align}&lt;br /&gt;
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V(S,t) &amp;amp;= K v(x,\tau),\\[5px]&lt;br /&gt;
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x &amp;amp;= \ln\left(\tfrac{S}{K} \right),\\[5px]&lt;br /&gt;
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\tau &amp;amp;= \tfrac{1}{2} \sigma^2 (T - t),\\[5px]&lt;br /&gt;
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v(x,\tau)&amp;amp;=e^{-\alpha x-\beta\tau} u(x,\tau).&lt;br /&gt;
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\end{align}&amp;lt;/math&amp;gt;&lt;br /&gt;
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===Fundamental solution===&lt;br /&gt;
基本解&lt;br /&gt;
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{{main|Fundamental solution}}&lt;br /&gt;
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Inhomogeneous equations can often be solved (for constant coefficient PDEs, always be solved) by finding the [[fundamental solution]] (the solution for a point source), then taking the [[convolution]] with the boundary conditions to get the solution.&lt;br /&gt;
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Inhomogeneous equations can often be solved (for constant coefficient PDEs, always be solved) by finding the fundamental solution (the solution for a point source), then taking the convolution with the boundary conditions to get the solution.&lt;br /&gt;
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非齐次方程(常系数偏微分方程)一般是通过先求出基本解(点源的解) ，然后利用带边界条件的卷积来求解。&lt;br /&gt;
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This is analogous in [[signal processing]] to understanding a filter by its [[impulse response]].&lt;br /&gt;
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This is analogous in signal processing to understanding a filter by its impulse response.&lt;br /&gt;
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这类似于在信号处理中通过滤波器的脉冲响应来理解滤波器。&lt;br /&gt;
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===Superposition principle===&lt;br /&gt;
叠加原理&lt;br /&gt;
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{{further| Superposition principle }}&lt;br /&gt;
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The superposition principle applies to any linear system, including linear systems of PDEs. A common visualization of this concept is the interaction of two waves in phase being combined to result in a greater amplitude, for example {{math|sin ''x'' + sin ''x'' {{=}} 2 sin ''x''}}. The same principle can be observed in PDEs where the solutions may be real or complex and additive. [[Superposition principle|superposition]]&lt;br /&gt;
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The superposition principle applies to any linear system, including linear systems of PDEs. A common visualization of this concept is the interaction of two waves in phase being combined to result in a greater amplitude, for example  2 sin x}}. The same principle can be observed in PDEs where the solutions may be real or complex and additive. superposition&lt;br /&gt;
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'''&amp;lt;font color = &amp;quot;#ff8000&amp;quot;&amp;gt;叠加原理 Superposition Principle&amp;lt;/font&amp;gt;适用于任何线性系统，包括偏微分方程的线性系统。这个概念的一个常见的可视化是两个同相位的波相互作用结合在一起会产生更大的振幅，例如 {{math|sin ''x'' + sin ''x'' {{=}} 2 sin ''x''}}。在偏微分方程中也可以观察到同样的原理，其中的解可能是真实的或复杂的和可加的。叠加&lt;br /&gt;
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If {{math|''u''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;}} and {{math|''u''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;}} are solutions of linear PDE in some function space {{mvar|R}}, then {{math|''u'' {{=}} ''c''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;''u''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; + ''c''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;''u''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;}} with any constants {{math|''c''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;}} and {{math|''c''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;}} are also a solution of that PDE in the same function space.&lt;br /&gt;
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If  and  are solutions of linear PDE in some function space , then  c&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;u&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; + c&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;u&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;}} with any constants  and  are also a solution of that PDE in the same function space.&lt;br /&gt;
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若线性偏微分方程在某个函数空间{{mvar|R}}中有解{{math|''u''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;}} 和 {{math|''u''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;}}，则{{math|''u'' {{=}} ''c''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;''u''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; + ''c''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;''u''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;}}也是该偏微分方程在同一函数空间中的解，其中{{math|''c''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;}} 和 {{math|''c''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;}} 是任意常数。&lt;br /&gt;
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===Methods for non-linear equations===&lt;br /&gt;
非线性方程的求解方法&lt;br /&gt;
{{see also|nonlinear partial differential equation}}&lt;br /&gt;
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There are no generally applicable methods to solve nonlinear PDEs. Still, existence and uniqueness results (such as the [[Cauchy–Kowalevski theorem]]) are often possible, as are proofs of important qualitative and quantitative properties of solutions (getting these results is a major part of [[mathematical analysis|analysis]]). Computational solution to the nonlinear PDEs, the [[split-step method]], exist for specific equations like [[nonlinear Schrödinger equation]].&lt;br /&gt;
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There are no generally applicable methods to solve nonlinear PDEs. Still, existence and uniqueness results (such as the Cauchy–Kowalevski theorem) are often possible, as are proofs of important qualitative and quantitative properties of solutions (getting these results is a major part of analysis). Computational solution to the nonlinear PDEs, the split-step method, exist for specific equations like nonlinear Schrödinger equation.&lt;br /&gt;
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对于非线性偏微分方程，目前还没有普遍适用的求解方法。然而，通常是可能知道解的存在性和唯一性(如柯西-科瓦列夫斯基定理)，也是可能得到解的重要定性和定量性质的证明(得到这些结果是分析的主要部分)。非线性偏微分方程的计算解，即分步法，对一些特定的方程适用，比如非线性'''&amp;lt;font color=&amp;quot;#ff8000&amp;quot;&amp;gt;薛定谔方程 Schrödinger equation&amp;lt;/font&amp;gt;'''。&lt;br /&gt;
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Nevertheless, some techniques can be used for several types of equations. The [[h-principle|{{mvar|h}}-principle]] is the most powerful method to solve [[Underdetermined system|underdetermined]] equations. The [[Riquier–Janet theory]] is an effective method for obtaining information about many analytic [[Overdetermined system|overdetermined]] systems.&lt;br /&gt;
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Nevertheless, some techniques can be used for several types of equations. The -principle is the most powerful method to solve underdetermined equations. The Riquier–Janet theory is an effective method for obtaining information about many analytic overdetermined systems.&lt;br /&gt;
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然而，一些技巧可以用于几种类型的方程。h-原理是求解欠定方程最有效的方法。里基尔-珍妮特理论是一种可以获得许多解析超定系统信息的有效方法。&lt;br /&gt;
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The [[method of characteristics]] can be used in some very special cases to solve partial differential equations.&lt;br /&gt;
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The method of characteristics can be used in some very special cases to solve partial differential equations.&lt;br /&gt;
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特征线法可用于求解某些特殊情况下的偏微分方程。&lt;br /&gt;
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In some cases, a PDE can be solved via [[perturbation analysis]] in which the solution is considered to be a correction to an equation with a known solution. Alternatives are [[numerical analysis]] techniques from simple [[finite difference]] schemes to the more mature [[multigrid]] and [[finite element method]]s. Many interesting problems in science and engineering are solved in this way using [[computer]]s, sometimes high performance [[supercomputer]]s.&lt;br /&gt;
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In some cases, a PDE can be solved via perturbation analysis in which the solution is considered to be a correction to an equation with a known solution. Alternatives are numerical analysis techniques from simple finite difference schemes to the more mature multigrid and finite element methods. Many interesting problems in science and engineering are solved in this way using computers, sometimes high performance supercomputers.&lt;br /&gt;
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在某些情况下，偏微分方程可以通过扰动分析来求解。在扰动分析中，通常是求解将具有已知解的方程修正后的新得到方程。可供选择的数值分析技术从简单的差分格式到更成熟的多重网格和有限元方法。许多有趣的科学和工程问题都是在计算机上用这种方法解决的，有时是高性能超级计算机。&lt;br /&gt;
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===Lie group method===&lt;br /&gt;
李群方法&lt;br /&gt;
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From 1870 [[Sophus Lie]]'s work put the theory of differential equations on a more satisfactory foundation. He showed that the integration theories of the older mathematicians can, by the introduction of what are now called [[Lie group]]s, be referred, to a common source; and that ordinary differential equations which admit the same [[infinitesimal transformation]]s present comparable difficulties of integration. He also emphasized the subject of [[contact transformation|transformations of contact]].&lt;br /&gt;
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From 1870 Sophus Lie's work put the theory of differential equations on a more satisfactory foundation. He showed that the integration theories of the older mathematicians can, by the introduction of what are now called Lie groups, be referred, to a common source; and that ordinary differential equations which admit the same infinitesimal transformations present comparable difficulties of integration. He also emphasized the subject of transformations of contact.&lt;br /&gt;
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从1870年起，索弗斯·李的工作为微分方程理论奠定了一个较为令人满意的基础。他指出，通过引入现在所谓的李群，老一辈数学家的积分理论可以引用到一个共同的来源; 承认相同的无穷小变换的常微分方程在积分方面存在相当的困难。他还强调了接触的转变这一主题。&lt;br /&gt;
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==[[用户:Yuling|Yuling]]（[[用户讨论:Yuling|讨论]]）这句话“He also emphasized the subject of transformations of contact.”中的transformations of contact翻译的不太好。&lt;br /&gt;
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A general approach to solving PDEs uses the symmetry property of differential equations, the continuous [[infinitesimal transformation]]s of solutions to solutions ([[Lie theory]]). Continuous [[group theory]], [[Lie algebras]] and [[differential geometry]] are used to understand the structure of linear and nonlinear partial differential equations for generating integrable equations, to find its [[Lax pair]]s, recursion operators, [[Bäcklund transform]] and finally finding exact analytic solutions to the PDE.&lt;br /&gt;
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A general approach to solving PDEs uses the symmetry property of differential equations, the continuous infinitesimal transformations of solutions to solutions (Lie theory). Continuous group theory, Lie algebras and differential geometry are used to understand the structure of linear and nonlinear partial differential equations for generating integrable equations, to find its Lax pairs, recursion operators, Bäcklund transform and finally finding exact analytic solutions to the PDE.&lt;br /&gt;
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求解偏微分方程的一般方法是利用微分方程的对称性，即解到解的连续无穷小变换(李理论)。连续群论、李代数和微分几何理论被用来理解生成可积方程的线性和非线性偏微分方程的结构，找到它的Lax对、递归算子、 贝克伦德变换，最后找到偏微分方程的精确解析解。&lt;br /&gt;
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Symmetry methods have been recognized to study differential equations arising in mathematics, physics, engineering, and many other disciplines.&lt;br /&gt;
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Symmetry methods have been recognized to study differential equations arising in mathematics, physics, engineering, and many other disciplines.&lt;br /&gt;
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对称方法已被公认可以用于研究出现在数学，物理，工程和许多其他学科的微分方程。&lt;br /&gt;
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===Semianalytical methods===&lt;br /&gt;
半解析方法&lt;br /&gt;
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The [[Adomian decomposition method]], the [[Aleksandr Lyapunov|Lyapunov]] artificial small parameter method, and He's [[homotopy perturbation method]] are all special cases of the more general [[homotopy analysis method]]. These are series expansion methods, and except for the Lyapunov method, are independent of small physical parameters as compared to the well known [[perturbation theory]], thus giving these methods greater flexibility and solution generality.&lt;br /&gt;
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The Adomian decomposition method, the Lyapunov artificial small parameter method, and He's homotopy perturbation method are all special cases of the more general homotopy analysis method. These are series expansion methods, and except for the Lyapunov method, are independent of small physical parameters as compared to the well known perturbation theory, thus giving these methods greater flexibility and solution generality.&lt;br /&gt;
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阿多米安分解法、李雅普诺夫人工小参数方法和何同伦摄动方法都是更一般的同伦分析方法的特殊情况。除了李雅普诺夫方法之外，这些都是级数展开方法，与为人熟知的摄动理论方法相比，它们与小的物理参数无关，因此这些方法具有更大的灵活性和解的通用性。&lt;br /&gt;
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== Numerical solutions ==&lt;br /&gt;
数值解&lt;br /&gt;
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The three most widely used [[Numerical partial differential equations|numerical methods to solve PDEs]] are the [[finite element analysis|finite element method]] (FEM), [[finite volume method]]s (FVM) and [[finite difference method]]s (FDM), as well other kind of methods called [[Meshfree methods]], which were made to solve problems where the before mentioned methods are limited. The FEM has a prominent position among these methods and especially its exceptionally efficient higher-order version [[hp-FEM]]. Other hybrid versions of FEM and Meshfree methods include the generalized finite element method (GFEM), [[extended finite element method]] (XFEM), [[Spectral element method|spectral finite element method]] (SFEM), [[Meshfree methods|meshfree finite element method]], [[Discontinuous Galerkin Method|discontinuous Galerkin finite element method]] (DGFEM), [[Element-Free Galerkin Method]] (EFGM), [[Interpolating Element-Free Galerkin Method]] (IEFGM), etc.&lt;br /&gt;
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The three most widely used numerical methods to solve PDEs are the finite element method (FEM), finite volume methods (FVM) and finite difference methods (FDM), as well other kind of methods called Meshfree methods, which were made to solve problems where the before mentioned methods are limited. The FEM has a prominent position among these methods and especially its exceptionally efficient higher-order version hp-FEM. Other hybrid versions of FEM and Meshfree methods include the generalized finite element method (GFEM), extended finite element method (XFEM), spectral finite element method (SFEM), meshfree finite element method, discontinuous Galerkin finite element method (DGFEM), Element-Free Galerkin Method (EFGM), Interpolating Element-Free Galerkin Method (IEFGM), etc.&lt;br /&gt;
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求解偏微分方程最常用的三种数值方法是有限元分析法、有限体积法和有限差分法，以及其他一些称为无网格法的方法。这些方法用于解决前面提到的方法受到的限制。在这些方法中，有限元方法，尤其是高效的高阶有限元方法，占有重要地位。其他有限元法和无网格法的混合形式包括广义有限元分析法(GFEM)、扩展有限元分析法(XFEM)、谱有限元分析法(SFEM)、无网格有限元分析法(DGFEM)、间断伽辽金有限元分析法(DGFEM)、无网格伽辽金法(EFGM)、插值无网格伽辽金法(IEFGM)等。&lt;br /&gt;
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=== Finite element method ===&lt;br /&gt;
有限元分析法&lt;br /&gt;
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{{main|Finite element method}}&lt;br /&gt;
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The finite element method (FEM) (its practical application often known as finite element analysis (FEA)) is a numerical technique for finding approximate solutions of partial differential equations (PDE) as well as of integral equations. The solution approach is based either on eliminating the differential equation completely (steady state problems), or rendering the PDE into an approximating system of ordinary differential equations, which are then numerically integrated using standard techniques such as Euler's method, Runge–Kutta, etc.&lt;br /&gt;
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The finite element method (FEM) (its practical application often known as finite element analysis (FEA)) is a numerical technique for finding approximate solutions of partial differential equations (PDE) as well as of integral equations. The solution approach is based either on eliminating the differential equation completely (steady state problems), or rendering the PDE into an approximating system of ordinary differential equations, which are then numerically integrated using standard techniques such as Euler's method, Runge–Kutta, etc.&lt;br /&gt;
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'''&amp;lt;font color = &amp;quot;#ff8000&amp;quot;&amp;gt;有限元分析法 Finite Element Method&amp;lt;/font&amp;gt;''' ((其实际应用通常被称为有限元分析(FEA))是一种寻找偏微分方程(PDE)和积分方程近似解的数值技术。这种求解方法要么基于完全消除微分方程(稳态问题) ，要么将偏微分方程转化为常微分方程的近似系统，然后使用标准技术进行数值积分，如欧拉方法、 Runge-Kutta 等。&lt;br /&gt;
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===Finite difference method===&lt;br /&gt;
有限差分法&lt;br /&gt;
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{{main|Finite difference method}}&lt;br /&gt;
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Finite-difference methods are numerical methods for approximating the solutions to differential equations using [[finite difference]] equations to approximate derivatives.&lt;br /&gt;
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Finite-difference methods are numerical methods for approximating the solutions to differential equations using finite difference equations to approximate derivatives.&lt;br /&gt;
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有限差分法是一种数值方法，用差分方程近似微分方程的解。&lt;br /&gt;
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=== Finite volume method ===&lt;br /&gt;
有限体积法&lt;br /&gt;
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{{main|Finite volume method}}&lt;br /&gt;
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Similar to the finite difference method or finite element method, values are calculated at discrete places on a meshed geometry. &amp;quot;Finite volume&amp;quot; refers to the small volume surrounding each node point on a mesh. In the finite volume method, surface integrals in a partial differential equation that contain a divergence term are converted to volume integrals, using the [[divergence theorem]]. These terms are then evaluated as fluxes at the surfaces of each finite volume. Because the flux entering a given volume is identical to that leaving the adjacent volume, these methods conserve mass by design.&lt;br /&gt;
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Similar to the finite difference method or finite element method, values are calculated at discrete places on a meshed geometry. &amp;quot;Finite volume&amp;quot; refers to the small volume surrounding each node point on a mesh. In the finite volume method, surface integrals in a partial differential equation that contain a divergence term are converted to volume integrals, using the divergence theorem. These terms are then evaluated as fluxes at the surfaces of each finite volume. Because the flux entering a given volume is identical to that leaving the adjacent volume, these methods conserve mass by design.&lt;br /&gt;
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类似于有限差分法或有限元分析，函数值是在网状几何体上的离散位置进行计算的。“有限体积”是指网格上每个节点周围的小体积。在有限体积法中，偏微分方程中含有散度项的面积分用散度定理积分转换成体积分。然后将这些项用于估算每个有限体积表面上的通量。由于进入给定体积的通量与转移到相邻体积元的通量相同，所以这些方法在设计上保证了质量守恒。&lt;br /&gt;
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==See also==&lt;br /&gt;
请参阅&lt;br /&gt;
* [[Dirichlet boundary condition]]&lt;br /&gt;
狄利克雷边界条件&lt;br /&gt;
* [[Jet bundle]]&lt;br /&gt;
射流丛&lt;br /&gt;
* [[Laplace transform applied to differential equations]]&lt;br /&gt;
微分方程中的拉普拉斯变换&lt;br /&gt;
* [[List of dynamical systems and differential equations topics]]&lt;br /&gt;
动力学系统和微分方程的列表&lt;br /&gt;
* [[Matrix differential equation]]&lt;br /&gt;
矩阵微分方程&lt;br /&gt;
* [[Neumann boundary condition]]&lt;br /&gt;
诺伊曼边界条件&lt;br /&gt;
* [[Numerical partial differential equations]]&lt;br /&gt;
数值偏微分方程&lt;br /&gt;
* [[Partial differential algebraic equation]]&lt;br /&gt;
偏微分代数方程&lt;br /&gt;
* [[Recurrence relation]]&lt;br /&gt;
递推关系&lt;br /&gt;
* [[Robin boundary condition]]&lt;br /&gt;
罗宾边界条件&lt;br /&gt;
* [[Stochastic processes and boundary value problems]]&lt;br /&gt;
随机过程和边值问题&lt;br /&gt;
&lt;br /&gt;
== The energy method ==&lt;br /&gt;
能量法&lt;br /&gt;
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The energy method is a mathematical procedure that can be used to verify well-posedness of initial-boundary-value-problems.&amp;lt;ref&amp;gt;{{cite book |title=High Order Difference Methods for Time Dependent PDE&lt;br /&gt;
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The energy method is a mathematical procedure that can be used to verify well-posedness of initial-boundary-value-problems.&amp;lt;ref&amp;gt;{{cite book |title=High Order Difference Methods for Time Dependent PDE&lt;br /&gt;
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能量法是验证初边值问题适定性的一种数学方法。 时变偏微分方程的高阶差分方法&lt;br /&gt;
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|first=Bertil|last=Gustafsson|publisher=Springer|year=2008|isbn=978-3-540-74992-9|doi=10.1007/978-3-540-74993-6}}&amp;lt;/ref&amp;gt; In the following example the energy method is used to decide where and which boundary conditions should be imposed such that the resulting IBVP is well-posed. Consider the one-dimensional hyperbolic PDE given by&lt;br /&gt;
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|first=Bertil|last=Gustafsson|publisher=Springer|year=2008|isbn=978-3-540-74992-9|doi=10.1007/978-3-540-74993-6}}&amp;lt;/ref&amp;gt; In the following example the energy method is used to decide where and which boundary conditions should be imposed such that the resulting IBVP is well-posed. Consider the one-dimensional hyperbolic PDE given by&lt;br /&gt;
&lt;br /&gt;
| first Bertil | last Gustafsson | publisher | Springer | year 2008 | isbn 978-3-540-74992-9 | doi 10.1007 / 978-3-540-74993-6} / ref 在下面的例子中，使用能量方法来决定应该施加哪些边界条件，使得得到的 IBVP适定。考虑一维双曲偏微分方程&lt;br /&gt;
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: &amp;lt;math&amp;gt;\frac{\partial u}{\partial t} + \alpha \frac{\partial u}{\partial x} = 0, \quad x \in [a,b], \operatorname t &amp;gt; 0,&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;\frac{\partial u}{\partial t} + \alpha \frac{\partial u}{\partial x} = 0, \quad x \in [a,b], \operatorname t &amp;gt; 0,&amp;lt;/math&amp;gt;&lt;br /&gt;
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where &amp;lt;math&amp;gt;\alpha \neq 0&amp;lt;/math&amp;gt; is a constant and &amp;lt;math&amp;gt;u(x,t)&amp;lt;/math&amp;gt; is an unknown function with initial condition &amp;lt;math&amp;gt;u(x,0) = f(x)&amp;lt;/math&amp;gt;. Multiplying with &amp;lt;math&amp;gt;u&amp;lt;/math&amp;gt; and integrating over the domain gives&lt;br /&gt;
&lt;br /&gt;
where &amp;lt;math&amp;gt;\alpha \neq 0&amp;lt;/math&amp;gt; is a constant and &amp;lt;math&amp;gt;u(x,t)&amp;lt;/math&amp;gt; is an unknown function with initial condition &amp;lt;math&amp;gt;u(x,0) = f(x)&amp;lt;/math&amp;gt;. Multiplying with &amp;lt;math&amp;gt;u&amp;lt;/math&amp;gt; and integrating over the domain gives&lt;br /&gt;
&lt;br /&gt;
其中 &amp;lt;math&amp;gt;\alpha \neq 0&amp;lt;/math&amp;gt; 是常数，并且 &amp;lt;math&amp;gt;u(x,t)&amp;lt;/math&amp;gt; 是未知函数，初始条件是 &amp;lt;math&amp;gt;u(x,0) = f(x)&amp;lt;/math&amp;gt;。乘以 &amp;lt;math&amp;gt;u&amp;lt;/math&amp;gt; 并在域上进行积分。&lt;br /&gt;
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: &amp;lt;math&amp;gt;\int_a^b u \frac{\partial u}{\partial t} \operatorname dx + \alpha \int _a ^b u \frac{\partial u}{\partial x} \operatorname dx = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;\int_a^b u \frac{\partial u}{\partial t} \operatorname dx + \alpha \int _a ^b u \frac{\partial u}{\partial x} \operatorname dx = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
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Using that&lt;br /&gt;
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Using that&lt;br /&gt;
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利用这一点&lt;br /&gt;
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: &amp;lt;math&amp;gt;\int _a ^b u \frac{\partial u}{\partial t} \operatorname dx = \frac{1}{2} \frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 \quad \text{and} \quad \int _a ^b u \frac{\partial u}{\partial x} \operatorname dx = \frac{1}{2} u(b,t)^2 - \frac{1}{2} u(a,t)^2,.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;\int _a ^b u \frac{\partial u}{\partial t} \operatorname dx = \frac{1}{2} \frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 \quad \text{and} \quad \int _a ^b u \frac{\partial u}{\partial x} \operatorname dx = \frac{1}{2} u(b,t)^2 - \frac{1}{2} u(a,t)^2,.&amp;lt;/math&amp;gt;&lt;br /&gt;
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where integration by parts has been used for the second relationship, we get&lt;br /&gt;
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where integration by parts has been used for the second relationship, we get&lt;br /&gt;
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第二个关系中采用了分部积分法，我们可以得到&lt;br /&gt;
&lt;br /&gt;
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: &amp;lt;math&amp;gt;\frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 + \alpha u(b,t)^2 - \alpha u(a,t)^2 = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;\frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 + \alpha u(b,t)^2 - \alpha u(a,t)^2 = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
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Here &amp;lt;math&amp;gt;\vert \vert \cdot \vert \vert&amp;lt;/math&amp;gt; denotes the standard L2-norm.&lt;br /&gt;
&lt;br /&gt;
Here &amp;lt;math&amp;gt;\vert \vert \cdot \vert \vert&amp;lt;/math&amp;gt; denotes the standard L2-norm.&lt;br /&gt;
&lt;br /&gt;
在这里，&amp;lt;math&amp;gt;\vert \vert \cdot \vert \vert&amp;lt;/math&amp;gt; 表示标准的 L2-正则。&lt;br /&gt;
&lt;br /&gt;
For well-posedness we require that the energy of the solution is non-increasing, i.e. that &amp;lt;math&amp;gt;\frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 \leq 0&amp;lt;/math&amp;gt;, which is achieved by specifying &amp;lt;math&amp;gt;u&amp;lt;/math&amp;gt; at &amp;lt;math&amp;gt;x = a&amp;lt;/math&amp;gt; if &amp;lt;math&amp;gt;\alpha &amp;gt; 0&amp;lt;/math&amp;gt; and at &amp;lt;math&amp;gt;x = b&amp;lt;/math&amp;gt; if &amp;lt;math&amp;gt;\alpha &amp;lt; 0&amp;lt;/math&amp;gt;. This corresponds to only imposing boundary conditions at the inflow. Note that well-posedness allows for growth in terms of data (initial and boundary) and thus it is sufficient to show that &amp;lt;math&amp;gt;\frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 \leq 0&amp;lt;/math&amp;gt; holds when all data is set to zero.&lt;br /&gt;
&lt;br /&gt;
For well-posedness we require that the energy of the solution is non-increasing, i.e. that &amp;lt;math&amp;gt;\frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 \leq 0&amp;lt;/math&amp;gt;, which is achieved by specifying &amp;lt;math&amp;gt;u&amp;lt;/math&amp;gt; at &amp;lt;math&amp;gt;x = a&amp;lt;/math&amp;gt; if &amp;lt;math&amp;gt;\alpha &amp;gt; 0&amp;lt;/math&amp;gt; and at &amp;lt;math&amp;gt;x = b&amp;lt;/math&amp;gt; if &amp;lt;math&amp;gt;\alpha &amp;lt; 0&amp;lt;/math&amp;gt;. This corresponds to only imposing boundary conditions at the inflow. Note that well-posedness allows for growth in terms of data (initial and boundary) and thus it is sufficient to show that &amp;lt;math&amp;gt;\frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 \leq 0&amp;lt;/math&amp;gt; holds when all data is set to zero.&lt;br /&gt;
&lt;br /&gt;
对于适定性，我们要解的能量是不增加的，即 &amp;lt;math&amp;gt;\frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 \leq 0&amp;lt;/math&amp;gt; ，这种关系可以通过在&amp;lt;math&amp;gt;x = a&amp;lt;/math&amp;gt;处 （如果 &amp;lt;math&amp;gt;\alpha &amp;gt; 0&amp;lt;/math&amp;gt;） 以及 &amp;lt;math&amp;gt;x = b&amp;lt;/math&amp;gt;处 （如果 &amp;lt;math&amp;gt;\alpha &amp;lt; 0&amp;lt;/math&amp;gt;）指定&amp;lt;math&amp;gt;u&amp;lt;/math&amp;gt;的值来实现。这只相当于在入流处附加边界条件。注意，适定性允许在数据(初始和边界)上的增长，因此它足以表明当所有数据设置为零时应有 &amp;lt;math&amp;gt;\frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 \leq 0&amp;lt;/math&amp;gt;。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==[[用户:Yuling|Yuling]]（[[用户讨论:Yuling|讨论]]）“This corresponds to only imposing boundary conditions at the inflow.” 这句话中的inflow不是很理解&lt;br /&gt;
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==Notes==&lt;br /&gt;
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{{Reflist}}&lt;br /&gt;
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* {{cite book |title=High Order Difference Methods for Time Dependent PDE&lt;br /&gt;
&lt;br /&gt;
|first=Bertil|last=Gustafsson|publisher=Springer|year=2008|isbn=978-3-540-74992-9|doi=10.1007/978-3-540-74993-6}}&lt;br /&gt;
&lt;br /&gt;
|first=Bertil|last=Gustafsson|publisher=Springer|year=2008|isbn=978-3-540-74992-9|doi=10.1007/978-3-540-74993-6}}&lt;br /&gt;
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| first Bertil | last Gustafsson | Springer | year 2008 | isbn 978-3-540-74992-9 | doi 10.1007 / 978-3-540-74993-6}&lt;br /&gt;
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{{refend}}&lt;br /&gt;
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== Further reading ==&lt;br /&gt;
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* {{Cite journal|last=Cajori|first=Florian|authorlink=Florian Cajori|year=1928|title=The Early History of Partial Differential Equations and of Partial Differentiation and Integration|url=http://www.math.harvard.edu/archive/21a_fall_14/exhibits/cajori/cajori.pdf|journal=The American Mathematical Monthly|volume=35|issue=9|pages=459–467|doi=10.2307/2298771|access-date=2016-05-15|archive-url=https://web.archive.org/web/20181123102253/http://www.math.harvard.edu/archive/21a_fall_14/exhibits/cajori/cajori.pdf|archive-date=2018-11-23|url-status=dead}}&lt;br /&gt;
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== External links ==&lt;br /&gt;
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{{Sister project links| wikt=no | commons=Category:Solutions of PDE | b=Partial Differential Equations | n=no | q=Partial differential equation | s=no | v=no | voy=no | species=no | d=no}}&lt;br /&gt;
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* {{springer|title=Differential equation, partial|id=p/d031920}}&lt;br /&gt;
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* [http://eqworld.ipmnet.ru/en/pde-en.htm Partial Differential Equations: Exact Solutions] at EqWorld: The World of Mathematical Equations.&lt;br /&gt;
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* [http://eqworld.ipmnet.ru/en/solutions/eqindex/eqindex-pde.htm Partial Differential Equations: Index] at EqWorld: The World of Mathematical Equations.&lt;br /&gt;
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* [http://eqworld.ipmnet.ru/en/methods/meth-pde.htm Partial Differential Equations: Methods] at EqWorld: The World of Mathematical Equations.&lt;br /&gt;
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* [https://web.archive.org/web/20170701144823/http://www.exampleproblems.com/wiki/index.php?title=Partial_Differential_Equations Example problems with solutions] at exampleproblems.com&lt;br /&gt;
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* [http://mathworld.wolfram.com/PartialDifferentialEquation.html Partial Differential Equations] at mathworld.wolfram.com&lt;br /&gt;
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* [https://reference.wolfram.com/language/FEMDocumentation/tutorial/SolvingPDEwithFEM.html Partial Differential Equations] with Mathematica&lt;br /&gt;
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* [http://www.mathworks.com/moler/pdes.pdf Partial Differential Equations] in Cleve Moler: Numerical Computing with MATLAB&lt;br /&gt;
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* [http://www.nag.com/numeric/fl/nagdoc_fl24/html/D03/d03intro.html Partial Differential Equations] at nag.com&lt;br /&gt;
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* {{cite web |first=Grant |last=Sanderson |title=But what is a partial differential equation? |work=3Blue1Brown |date=April 21, 2019 |url=https://www.youtube.com/watch?v=ly4S0oi3Yz8&amp;amp;list=PLZHQObOWTQDNPOjrT6KVlfJuKtYTftqH6 |via=[[YouTube]] }}&lt;br /&gt;
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[[Category:Partial differential equations| ]]&lt;br /&gt;
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Category:Multivariable calculus&lt;br /&gt;
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类别: 多元微积分&lt;br /&gt;
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[[Category:Differential equations]]&lt;br /&gt;
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Category:Differential equations&lt;br /&gt;
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类别: 微分方程&lt;br /&gt;
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Category:Concepts in physics&lt;br /&gt;
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&amp;lt;small&amp;gt;This page was moved from [[wikipedia:en:Partial differential equation]]. Its edit history can be viewed at [[偏微分方程/edithistory]]&amp;lt;/small&amp;gt;&amp;lt;/noinclude&amp;gt;&lt;br /&gt;
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[[Category:待整理页面]]&lt;/div&gt;</summary>
		<author><name>Ruili</name></author>
	</entry>
	<entry>
		<id>https://wiki.swarma.org/index.php?title=%E5%81%8F%E5%BE%AE%E5%88%86%E6%96%B9%E7%A8%8B&amp;diff=18117</id>
		<title>偏微分方程</title>
		<link rel="alternate" type="text/html" href="https://wiki.swarma.org/index.php?title=%E5%81%8F%E5%BE%AE%E5%88%86%E6%96%B9%E7%A8%8B&amp;diff=18117"/>
		<updated>2020-11-11T13:28:10Z</updated>

		<summary type="html">&lt;p&gt;Ruili：&lt;/p&gt;
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&lt;div&gt;此词条暂由Yuling翻译，未经人工整理和审校，带来阅读不便，请见谅。&lt;br /&gt;
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[[File:Heat.gif|thumb|right|A visualisation of a solution to the two-dimensional [[heat equation]] with temperature represented by the third dimension]]&lt;br /&gt;
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A visualisation of a solution to the two-dimensional [[heat equation with temperature represented by the third dimension]]&lt;br /&gt;
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以三维表示温度的二维热方程解的可视化&lt;br /&gt;
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In [[mathematics]], a '''partial differential equation''' ('''PDE''') is a [[differential equation]] that contains unknown [[Multivariable calculus|multivariable functions]] and their [[partial derivative]]s. PDEs are used to formulate problems involving functions of several variables, and are either solved by hand, or used to create a [[computer model]]. A special case is [[ordinary differential equation]]s (ODEs), which deal with functions of a single variable and their derivatives.&lt;br /&gt;
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In mathematics, a partial differential equation (PDE) is a differential equation that contains unknown multivariable functions and their partial derivatives. PDEs are used to formulate problems involving functions of several variables, and are either solved by hand, or used to create a computer model. A special case is ordinary differential equations (ODEs), which deal with functions of a single variable and their derivatives.&lt;br /&gt;
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在数学中，'''&amp;lt;font color = &amp;quot;#ff8000&amp;quot;&amp;gt;偏微分方程函数 Partial Differential Equation&amp;lt;/font&amp;gt;'''是包含未知多元函数及其偏导数的微分方程。偏微分方程用于描述涉及多元函数的问题，可以通过人为求解，也可以通过建立计算机模型来求解。常微分方程是偏微分方程一种特殊情况，它处理的是一元函数及其导数。&lt;br /&gt;
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PDEs can be used to describe a wide variety of phenomena such as sound, heat, [[diffusion]], [[electrostatics]], [[Electromagnetism|electrodynamics]], [[fluid dynamics]], [[Elasticity (physics)|elasticity]], [[gravitation]] and [[quantum mechanics]]. These seemingly distinct physical phenomena can be formalised similarly in terms of PDEs. Just as ordinary differential equations often model one-dimensional [[dynamical system]]s, partial differential equations often model [[multidimensional system]]s. PDEs find their generalisation in [[stochastic partial differential equation]]s.&lt;br /&gt;
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PDEs can be used to describe a wide variety of phenomena such as sound, heat, diffusion, electrostatics, electrodynamics, fluid dynamics, elasticity, gravitation and quantum mechanics. These seemingly distinct physical phenomena can be formalised similarly in terms of PDEs. Just as ordinary differential equations often model one-dimensional dynamical systems, partial differential equations often model multidimensional systems. PDEs find their generalisation in stochastic partial differential equations.&lt;br /&gt;
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偏微分方程可以用来描述各种各样的物理现象，如声音，热量，扩散，静电，电动力学，流体力学，弹性力学，重力和量子力学。这些看起来截然不同的物理现象却可以用类似的偏微分方程来描述。正如常微分方程经常对一维动力系统进行建模一样，偏微分方程经常对多维系统进行建模。随机偏微分方程是偏微分方程的一种推广。&lt;br /&gt;
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== Introduction ==&lt;br /&gt;
引言&lt;br /&gt;
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Partial differential equations (PDEs) are equations that involve rates of change with respect to [[continuous variables]]. For example, the position of a [[rigid body]] is specified by six parameters,&amp;lt;ref&amp;gt;{{Cite book|url=https://books.google.com/books?id=v9PLbcYd9aUC&amp;amp;pg=PA32|title=Modelling and Control of Robot Manipulators|last=Sciavicco|first=Lorenzo|last2=Siciliano|first2=Bruno|date=2001-02-19|publisher=Springer Science &amp;amp; Business Media|isbn=9781852332211|language=en}}&amp;lt;/ref&amp;gt; but the configuration of a [[fluid]] is given by the [[continuous distribution]] of several parameters, such as the [[temperature]], [[pressure]], and so forth. The dynamics for the rigid body take place in a finite-dimensional [[Configuration space (physics)|configuration space]]; the dynamics for the fluid occur in an infinite-dimensional configuration space. This distinction usually makes PDEs much harder to solve than ordinary differential equations (ODEs), but here again, there will be simple solutions for linear problems. Classic domains where PDEs are used include [[acoustics]], [[fluid dynamics]], [[electrodynamics]], and [[heat transfer]].&lt;br /&gt;
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Partial differential equations (PDEs) are equations that involve rates of change with respect to continuous variables. For example, the position of a rigid body is specified by six parameters, but the configuration of a fluid is given by the continuous distribution of several parameters, such as the temperature, pressure, and so forth. The dynamics for the rigid body take place in a finite-dimensional configuration space; the dynamics for the fluid occur in an infinite-dimensional configuration space. This distinction usually makes PDEs much harder to solve than ordinary differential equations (ODEs), but here again, there will be simple solutions for linear problems. Classic domains where PDEs are used include acoustics, fluid dynamics, electrodynamics, and heat transfer.&lt;br /&gt;
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偏微分方程(简称为PDEs)涉及到方程相对于连续变量的变化率。例如，刚体的位置是由六个参数确定的，而流体的状态是由几个参数的连续分布给出的，如温度、压力等。刚体的动力学过程发生在有限维状态空间中，流体的动力学过程发生在无限维状态空间中。这种区别通常使偏微分方程比常微分方程更难求解，但是线性问题仍然有简单的求解方式。使用偏微分方程的经典领域包括声学、流体力学、电动力学和传热学。&lt;br /&gt;
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A partial differential equation (PDE) for the function {{math|''u''(''x''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;,… ''x&amp;lt;sub&amp;gt;n&amp;lt;/sub&amp;gt;'')}} is an equation of the form&lt;br /&gt;
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A partial differential equation (PDE) for the function  is an equation of the form&lt;br /&gt;
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函数{{math|''u''(''x''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;,… ''x&amp;lt;sub&amp;gt;n&amp;lt;/sub&amp;gt;'')}}的偏微分方程形式是：&lt;br /&gt;
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: &amp;lt;math&amp;gt;f \left (x_1, \ldots x_n; u, \frac{\partial u}{\partial x_1}, \ldots \frac{\partial u}{\partial x_n}; \frac{\partial^2 u}{\partial x_1 \partial x_1}, \ldots \frac{\partial^2 u}{\partial x_1 \partial x_n}; \ldots \right) = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;f \left (x_1, \ldots x_n; u, \frac{\partial u}{\partial x_1}, \ldots \frac{\partial u}{\partial x_n}; \frac{\partial^2 u}{\partial x_1 \partial x_1}, \ldots \frac{\partial^2 u}{\partial x_1 \partial x_n}; \ldots \right) = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
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If {{mvar|f}} is a [[linear function]] of {{mvar|u}} and its derivatives, then the PDE is called linear. Common examples of linear PDEs include the [[heat equation]], the [[wave equation]], [[Laplace's equation]], [[Helmholtz equation]], [[Klein–Gordon equation]], and [[Poisson's equation]].&lt;br /&gt;
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If  is a linear function of  and its derivatives, then the PDE is called linear. Common examples of linear PDEs include the heat equation, the wave equation, Laplace's equation, Helmholtz equation, Klein–Gordon equation, and Poisson's equation.&lt;br /&gt;
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如果{{mvar|f}}是函数{{math|''u''}}及其导数的线性函数，则偏微分方程称为线性函数。线性偏微分方程的常见例子包括热方程、波动方程、拉普拉斯方程、亥姆霍兹方程方程、克莱因-高登方程和泊松方程。&lt;br /&gt;
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A relatively simple PDE is&lt;br /&gt;
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A relatively simple PDE is&lt;br /&gt;
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一个相对简单的偏微分方程：&lt;br /&gt;
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: &amp;lt;math&amp;gt;\frac{\partial u}{\partial x}(x,y) = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;\frac{\partial u}{\partial x}(x,y) = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
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This relation [[Logical implication|implies]] that the function {{math|''u''(''x'',''y'')}} is independent of {{mvar|x}}. However, the equation gives no information on the function's dependence on the variable {{mvar|y}}. Hence the general solution of this equation is&lt;br /&gt;
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This relation implies that the function  is independent of . However, the equation gives no information on the function's dependence on the variable . Hence the general solution of this equation is&lt;br /&gt;
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这意味着函数{{math|''u''(''x'',''y'')}}独立于{{mvar|x}}的。然而，这个方程没有给出关于函数和自变量的相关性的信息。因此，这个方程的通解是&lt;br /&gt;
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: &amp;lt;math&amp;gt;u(x,y) = f(y),&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;u(x,y) = f(y),&amp;lt;/math&amp;gt;&lt;br /&gt;
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where {{mvar|f}} is an arbitrary function of {{mvar|y}}. The analogous ordinary differential equation is&lt;br /&gt;
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where  is an arbitrary function of . The analogous ordinary differential equation is&lt;br /&gt;
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其中{{mvar|f}}是{{mvar|y}}的任意函数。&lt;br /&gt;
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类似的常微分方程是：&lt;br /&gt;
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: &amp;lt;math&amp;gt;\frac{\mathrm{d} u}{\mathrm{d} x}(x) = 0,&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;\frac{\mathrm{d} u}{\mathrm{d} x}(x) = 0,&amp;lt;/math&amp;gt;&lt;br /&gt;
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which has the solution&lt;br /&gt;
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which has the solution&lt;br /&gt;
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它的解为&lt;br /&gt;
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: &amp;lt;math&amp;gt;u(x) = c,&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;u(x) = c,&amp;lt;/math&amp;gt;&lt;br /&gt;
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where {{mvar|c}} is any [[Constant (mathematics)|constant]] value. These two examples illustrate that general solutions of ordinary differential equations (ODEs) involve arbitrary constants, but solutions of PDEs involve arbitrary functions.&lt;br /&gt;
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where  is any constant value. These two examples illustrate that general solutions of ordinary differential equations (ODEs) involve arbitrary constants, but solutions of PDEs involve arbitrary functions.&lt;br /&gt;
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这里，{{mvar|c}}是一个任意常量。&lt;br /&gt;
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这两个例子说明常微分方程的一般解包含任意常数，但偏微分方程的解包含任意函数。&lt;br /&gt;
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A solution of a PDE is generally not [[Uniqueness quantification|unique]]; additional conditions must generally be specified on the [[Boundary (topology)|boundary]] of the region where the solution is defined. For instance, in the simple example above, the function {{math|''f''(''y'')}} can be determined if {{mvar|u}} is specified on the line {{math|''x'' {{=}} 0}}.&lt;br /&gt;
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A solution of a PDE is generally not unique; additional conditions must generally be specified on the boundary of the region where the solution is defined. For instance, in the simple example above, the function  can be determined if  is specified on the line  0}}.&lt;br /&gt;
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偏微分方程的解一般不是唯一的; 附加条件一般必须在定义解的区域边界上定义。例如，在上面的简单示例中，如果在{{math|''x'' {{=}} 0}}时确定了{{mvar|u}}的值，则可以确定该函数{{math|''f''(''y'')}}。&lt;br /&gt;
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== Existence and uniqueness ==&lt;br /&gt;
存在性和唯一性&lt;br /&gt;
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Although the issue of existence and uniqueness of solutions of ordinary differential equations has a very satisfactory answer with the [[Picard–Lindelöf theorem]], that is far from the case for partial differential equations. The [[Cauchy–Kowalevski theorem]] states that the [[Cauchy problem]] for any partial differential equation whose coefficients are [[Analytic function|analytic]] in the unknown function and its derivatives, has a locally unique analytic solution. Although this result might appear to settle the existence and uniqueness of solutions, there are examples of linear partial differential equations whose coefficients have derivatives of all orders (which are nevertheless not analytic) but which have no solutions at all: see [[Lewy's example|Lewy (1957)]]. Even if the solution of a partial differential equation exists and is unique, it may nevertheless have undesirable properties.  The mathematical study of these questions is usually in the more powerful context of [[weak solution]]s.&lt;br /&gt;
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Although the issue of existence and uniqueness of solutions of ordinary differential equations has a very satisfactory answer with the Picard–Lindelöf theorem, that is far from the case for partial differential equations. The Cauchy–Kowalevski theorem states that the Cauchy problem for any partial differential equation whose coefficients are analytic in the unknown function and its derivatives, has a locally unique analytic solution. Although this result might appear to settle the existence and uniqueness of solutions, there are examples of linear partial differential equations whose coefficients have derivatives of all orders (which are nevertheless not analytic) but which have no solutions at all: see Lewy (1957). Even if the solution of a partial differential equation exists and is unique, it may nevertheless have undesirable properties.  The mathematical study of these questions is usually in the more powerful context of weak solutions.&lt;br /&gt;
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虽然常微分方程解的存在唯一性问题用'''&amp;lt;font color=&amp;quot;#ff8000&amp;quot;&amp;gt;弗罗贝尼乌斯定理 Picard–Lindelöf Theorem&amp;lt;/font&amp;gt;得到了令人满意的结果，但应用到偏微分方程上却不尽如意。'''&amp;lt;font color=&amp;quot;#ff8000&amp;quot;&amp;gt;柯西-科瓦列夫斯基定理 Cauchy–Kowalevski theorem&amp;lt;/font&amp;gt;指出，对于任何在未知函数及其导数中系数是解析的偏微分方程，柯西问题有一个局部唯一的解析解。虽然这个结果似乎解决了解的存在性和唯一性问题，但是有一些线性偏微分方程的系数具有所有级数的导数(尽管这些导数不是解析的) ，但是根本没有解: 见 Lewy (1957)。即使偏微分方程的解存在且唯一，它仍然可能具有人们所不希望的性质。这些问题的数学研究通常是在更有力的弱解的背景下进行的。&lt;br /&gt;
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An example of pathological behavior is the sequence (depending upon {{mvar|n}}) of [[Cauchy problem]]s for the [[Laplace equation]]&lt;br /&gt;
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An example of pathological behavior is the sequence (depending upon ) of Cauchy problems for the Laplace equation&lt;br /&gt;
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反常特征的一个例子是拉普拉斯方程的柯西问题的序列(取决于{{mvar|n}})&lt;br /&gt;
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: &amp;lt;math&amp;gt;\frac{\partial^2 u}{\partial x^2} + \frac{\partial^2 u}{\partial y^2}=0,&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;\frac{\partial^2 u}{\partial x^2} + \frac{\partial^2 u}{\partial y^2}=0,&amp;lt;/math&amp;gt;&lt;br /&gt;
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with [[boundary condition]]s&lt;br /&gt;
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with boundary conditions&lt;br /&gt;
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有边界条件&lt;br /&gt;
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: &amp;lt;math&amp;gt;\begin{align} u(x,0) &amp;amp;= 0, \\ \frac{\partial u}{\partial y}(x,0) &amp;amp;= \frac{\sin nx}{n}, \end{align}&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;\begin{align} u(x,0) &amp;amp;= 0, \\ \frac{\partial u}{\partial y}(x,0) &amp;amp;= \frac{\sin nx}{n}, \end{align}&amp;lt;/math&amp;gt;&lt;br /&gt;
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where {{mvar|n}} is an integer. The derivative of {{mvar|u}} with respect to {{mvar|y}} approaches zero [[uniform convergence|uniformly]] in {{mvar|x}} as {{mvar|n}} increases, but the solution is&lt;br /&gt;
&lt;br /&gt;
where  is an integer. The derivative of  with respect to  approaches zero uniformly in  as  increases, but the solution is&lt;br /&gt;
&lt;br /&gt;
其中{{mvar|n}}是整数。{{mvar|u}}是关于{{mvar|y}}的导数，一致地随着{{mvar|n}}的增加而趋于零，但是解是&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt;u(x,y) = \frac{\sinh ny \sin nx}{n^2}.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;u(x,y) = \frac{\sinh ny \sin nx}{n^2}.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
This solution approaches infinity if {{mvar|nx}} is not an integer multiple of {{pi}} for any non-zero value of {{mvar|y}}. The Cauchy problem for the Laplace equation is called ''ill-posed'' or ''not [[Well-posed problem|well-posed]]'', since the solution does not continuously depend on the data of the problem. Such ill-posed problems are not usually satisfactory for physical applications.&lt;br /&gt;
&lt;br /&gt;
This solution approaches infinity if  is not an integer multiple of  for any non-zero value of . The Cauchy problem for the Laplace equation is called ill-posed or not well-posed, since the solution does not continuously depend on the data of the problem. Such ill-posed problems are not usually satisfactory for physical applications.&lt;br /&gt;
&lt;br /&gt;
对于任何非零的{{mvar|y}}，如果{{mvar|nx}}不是{{pi}}的整数倍，这个解会接近于无穷大。拉普拉斯方程的柯西问题被称为不适定问题（可以译为ill-posed或not well-posed），因为该问题的解并不连续地依赖于该问题的数据。这种不适定问题在物理应用中通常不能令人满意。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The [[Navier–Stokes existence and smoothness|existence of solutions for the Navier–Stokes equations]], a partial differential equation, is part of one of the [[Millennium Prize Problems]].&lt;br /&gt;
&lt;br /&gt;
The existence of solutions for the Navier–Stokes equations, a partial differential equation, is part of one of the Millennium Prize Problems.&lt;br /&gt;
&lt;br /&gt;
一种偏微分方程——纳维-斯托克斯方程——的解的存在性就是千禧年大奖难题的一部分。&lt;br /&gt;
&lt;br /&gt;
== Notation ==&lt;br /&gt;
符号&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
In PDEs, it is common to denote partial derivatives using subscripts. That is:&lt;br /&gt;
&lt;br /&gt;
In PDEs, it is common to denote partial derivatives using subscripts. That is:&lt;br /&gt;
&lt;br /&gt;
在偏微分方程中，通常用下标表示偏导数。例如:&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt;u_x = \frac{\partial u}{\partial x}&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;u_x = \frac{\partial u}{\partial x}&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt;u_{xx} = \frac{\partial^2 u}{\partial x^2} &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;u_{xx} = \frac{\partial^2 u}{\partial x^2} &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt;u_{xy} = \frac{\partial^2 u}{\partial y\, \partial x} = \frac{\partial}{\partial y } \left(\frac{\partial u}{\partial x}\right). &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;u_{xy} = \frac{\partial^2 u}{\partial y\, \partial x} = \frac{\partial}{\partial y } \left(\frac{\partial u}{\partial x}\right). &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Especially in physics, [[del]] or nabla ({{math|∇}}) is often used to denote spatial derivatives, and {{math|''&amp;amp;#x307;u'', ''ü''}} for time derivatives. For example, the [[wave equation]] (mentioned below) can be written as&lt;br /&gt;
&lt;br /&gt;
Especially in physics, del or nabla () is often used to denote spatial derivatives, and  for time derivatives. For example, the wave equation (mentioned below) can be written as&lt;br /&gt;
&lt;br /&gt;
特别是在物理学中，[[del]]或nabla ({{math|∇}})经常用来表示空间导数和时间导数。例如，波动方程(在下文中提到)可以写成&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt;\ddot u=c^2\nabla^2u&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt;\ddot u=c^2\nabla^2u&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
or&lt;br /&gt;
&lt;br /&gt;
or&lt;br /&gt;
&lt;br /&gt;
或&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt;\ddot u=c^2\Delta u&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt;\ddot u=c^2\Delta u&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
where {{math|Δ}} is the [[Laplace operator]].&lt;br /&gt;
&lt;br /&gt;
where  is the Laplace operator.&lt;br /&gt;
&lt;br /&gt;
其中{{math|Δ}}代表拉普拉斯算子&lt;br /&gt;
&lt;br /&gt;
== Classification ==&lt;br /&gt;
分类&lt;br /&gt;
&lt;br /&gt;
Some linear, second-order partial differential equations can be classified as [[parabolic partial differential equation|parabolic]], [[hyperbolic partial differential equation|hyperbolic]] and [[elliptic partial differential equation|elliptic]]. Others, such as the [[Euler–Tricomi equation]], have different types in different regions. The classification provides a guide to appropriate initial and boundary conditions and to the smoothness of the solutions.&lt;br /&gt;
&lt;br /&gt;
Some linear, second-order partial differential equations can be classified as parabolic, hyperbolic and elliptic. Others, such as the Euler–Tricomi equation, have different types in different regions. The classification provides a guide to appropriate initial and boundary conditions and to the smoothness of the solutions.&lt;br /&gt;
&lt;br /&gt;
一些线性二阶偏微分方程可分为抛物型方程、双曲型方程和椭圆型方程。其他的方程，如欧拉-特里科米方程，在不同的区域有不同的类型。这种分类有助于选择适当的初始和边界条件以及提高解的平滑性。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
=== Equations of first order ===&lt;br /&gt;
一阶方程&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{{main|First-order partial differential equation}}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
=== Linear equations of second order ===&lt;br /&gt;
二阶线性方程&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Assuming {{math|''u&amp;lt;sub&amp;gt;xy&amp;lt;/sub&amp;gt;'' {{=}} ''u&amp;lt;sub&amp;gt;yx&amp;lt;/sub&amp;gt;''}}, the general linear second-order PDE in two independent variables has the form&lt;br /&gt;
&lt;br /&gt;
Assuming  u&amp;lt;sub&amp;gt;yx&amp;lt;/sub&amp;gt;}}, the general linear second-order PDE in two independent variables has the form&lt;br /&gt;
&lt;br /&gt;
假设 {{math|''u&amp;lt;sub&amp;gt;xy&amp;lt;/sub&amp;gt;'' {{=}} ''u&amp;lt;sub&amp;gt;yx&amp;lt;/sub&amp;gt;''}}，含有两个独立变量的一般的线性二阶偏微分方程具有如下这样的形式&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt;Au_{xx} + 2Bu_{xy} + Cu_{yy} + \cdots \mbox{(lower order terms)} = 0,&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;Au_{xx} + 2Bu_{xy} + Cu_{yy} + \cdots \mbox{(lower order terms)} = 0,&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
where the coefficients {{mvar|A}}, {{mvar|B}}, {{mvar|C}}... may depend upon {{mvar|x}} and {{mvar|y}}. If {{math|''A''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; + ''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; + ''C''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; &amp;gt; 0}} over a region of the {{mvar|xy}}-plane, the PDE is second-order in that region. This form is analogous to the equation for a conic section:&lt;br /&gt;
&lt;br /&gt;
where the coefficients , , ... may depend upon  and . If  over a region of the -plane, the PDE is second-order in that region. This form is analogous to the equation for a conic section:&lt;br /&gt;
&lt;br /&gt;
其中的系数 {{mvar|A}}, {{mvar|B}}, {{mvar|C}}... 一般取决于{{mvar|x}}和{{mvar|y}}。如果在{{mvar|xy}}-平面的一个区域上 {{math|''A''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; + ''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; + ''C''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; &amp;gt; 0}}，偏微分方程在该区域是二阶的。这种形式类似于圆锥曲线的方程:&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt;Ax^2 + 2Bxy + Cy^2 + \cdots = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;Ax^2 + 2Bxy + Cy^2 + \cdots = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
More precisely, replacing {{math|∂&amp;lt;sub&amp;gt;''x''&amp;lt;/sub&amp;gt;}} by {{mvar|X}}, and likewise for other variables (formally this is done by a [[Fourier transform]]), converts a constant-coefficient PDE into a polynomial of the same degree, with the terms of the highest degree (a [[homogeneous polynomial]], here a [[quadratic form]]) being most significant for the classification.&lt;br /&gt;
&lt;br /&gt;
More precisely, replacing  by , and likewise for other variables (formally this is done by a Fourier transform), converts a constant-coefficient PDE into a polynomial of the same degree, with the terms of the highest degree (a homogeneous polynomial, here a quadratic form) being most significant for the classification.&lt;br /&gt;
&lt;br /&gt;
更准确地说，用 {{mvar|X}} 替换 {{math|∂&amp;lt;sub&amp;gt;''x''&amp;lt;/sub&amp;gt;}}，对于其他变量做同样的操作(从形式上来说，这是由傅里叶变换来完成的)，将一个常系数偏微分方程转换成一个相同次数的多项式，最高次数的项(齐次多项式，这里是一个二次形式)一般会用于偏微分方程的分类。&lt;br /&gt;
===~~ most significant for the classification 意译为用于偏微分方程的分类。       significiant直译过来感觉不太合适&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Just as one classifies [[conic section]]s and quadratic forms into parabolic, hyperbolic, and elliptic based on the [[discriminant]] {{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − 4''AC''}}, the same can be done for a second-order PDE at a given point.  However, the [[discriminant]] in a PDE is given by {{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC''}} due to the convention of the {{mvar|xy}} term being {{math|2''B''}} rather than {{mvar|B}}; formally, the discriminant (of the associated quadratic form) is {{math|(2''B'')&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − 4''AC'' {{=}} 4(''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC'')}}, with the factor of 4 dropped for simplicity.&lt;br /&gt;
&lt;br /&gt;
Just as one classifies conic sections and quadratic forms into parabolic, hyperbolic, and elliptic based on the discriminant , the same can be done for a second-order PDE at a given point.  However, the discriminant in a PDE is given by  due to the convention of the  term being  rather than ; formally, the discriminant (of the associated quadratic form) is  4(B&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − AC)}}, with the factor of 4 dropped for simplicity.&lt;br /&gt;
&lt;br /&gt;
正如人们可以根据判别式 {{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − 4''AC''}} 将圆锥曲线和二次型分为抛物型、双曲型和椭圆型一样，对于给定点的二阶偏微分方程也可以这样做。然而，偏微分方程中的判别式 {{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − 4''AC''}} 是根据交叉项的系数{{math|2''B''}} 而不是 {{mvar|B}} 给出的，形式上，判别式(关联二次型)是 {{math|(2''B'')&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − 4''AC'' {{=}} 4(''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC'')}}，为简单起见，去掉了因子4。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
# {{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC'' &amp;lt; 0}} (''[[elliptic partial differential equation]]''): Solutions of [[elliptic partial differential equation|elliptic PDEs]] are as smooth as the coefficients allow, within the interior of the region where the equation and solutions are defined. For example, solutions of [[Laplace's equation]] are analytic within the domain where they are defined, but solutions may assume boundary values that are not smooth. The motion of a fluid at subsonic speeds can be approximated with elliptic PDEs, and the Euler–Tricomi equation is elliptic where {{math|''x'' &amp;lt; 0}}.&lt;br /&gt;
&lt;br /&gt;
  (elliptic partial differential equation): Solutions of elliptic PDEs are as smooth as the coefficients allow, within the interior of the region where the equation and solutions are defined. For example, solutions of Laplace's equation are analytic within the domain where they are defined, but solutions may assume boundary values that are not smooth. The motion of a fluid at subsonic speeds can be approximated with elliptic PDEs, and the Euler–Tricomi equation is elliptic where .&lt;br /&gt;
&lt;br /&gt;
{{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC'' &amp;lt; 0}} (椭圆形微分方程)：在定义方程和解的区域内部，椭圆型偏微分方程的解光滑到系数允许的程度。例如，拉普拉斯方程的解在它们被定义的区域内是解析的，但是解可能假设边界值是不光滑的。亚音速流体的运动可以用椭圆偏微分方程近似，其中欧拉-特里科米方程在 {{math|''x'' &amp;lt; 0}} 时是椭圆型偏微分方程。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
# {{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC'' {{=}} 0}} (''[[parabolic partial differential equation]]''): Equations that are [[parabolic partial differential equation|parabolic]] at every point can be transformed into a form analogous to the [[heat equation]] by a change of independent variables. Solutions smooth out as the transformed time variable increases. The Euler–Tricomi equation has parabolic type on the line where {{math|''x'' {{=}} 0}}.&lt;br /&gt;
&lt;br /&gt;
  0}} (parabolic partial differential equation): Equations that are parabolic at every point can be transformed into a form analogous to the heat equation by a change of independent variables. Solutions smooth out as the transformed time variable increases. The Euler–Tricomi equation has parabolic type on the line where  0}}.&lt;br /&gt;
&lt;br /&gt;
{{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC'' {{=}} 0}}（抛物线形偏微分方程）：在每一点上都是抛物线型的方程可以通过改变自变量从而转化成类似于热方程的形式。随着转换后的时间变量的增加，方程的解变得平滑。欧拉-特里科米方程在 {{math|''x'' {{=}} 0}} 这条特征线上是抛物线形的。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
# {{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC'' &amp;gt; 0}} (''[[hyperbolic partial differential equation]]''): [[hyperbolic partial differential equation|hyperbolic]] equations retain any discontinuities of functions or derivatives in the initial data. An example is the [[wave equation]]. The motion of a fluid at supersonic speeds can be approximated with hyperbolic PDEs, and the Euler–Tricomi equation is hyperbolic where {{math|''x'' &amp;gt; 0}}.&lt;br /&gt;
&lt;br /&gt;
  (hyperbolic partial differential equation): hyperbolic equations retain any discontinuities of functions or derivatives in the initial data. An example is the wave equation. The motion of a fluid at supersonic speeds can be approximated with hyperbolic PDEs, and the Euler–Tricomi equation is hyperbolic where .&lt;br /&gt;
&lt;br /&gt;
{{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC'' &amp;gt; 0}} (双曲形偏微分方程)：双曲形方程在初始数据中保留了函数或导数的任何不连续性，波动方程就是其中的一个例子。超音速流体的运动可以用双曲形偏微分方程近似，其中欧拉-特里科米方程在 {{math|''x'' &amp;gt; 0}} 时是双曲型的。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
If there are {{mvar|n}} independent variables {{math|''x''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;, ''x''&amp;lt;sub&amp;gt;2 &amp;lt;/sub&amp;gt;,… ''x''&amp;lt;sub&amp;gt;''n''&amp;lt;/sub&amp;gt;}}, a general linear partial differential equation of second order has the form&lt;br /&gt;
&lt;br /&gt;
If there are  independent variables , a general linear partial differential equation of second order has the form&lt;br /&gt;
&lt;br /&gt;
如果存在 {{mvar|n}} 个自变量 {{math|''x''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;, ''x''&amp;lt;sub&amp;gt;2 &amp;lt;/sub&amp;gt;,… ''x''&amp;lt;sub&amp;gt;''n''&amp;lt;/sub&amp;gt;}}，一般二阶线性偏微分方程的形式是&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt;L u =\sum_{i=1}^n\sum_{j=1}^n a_{i,j} \frac{\partial^2 u}{\partial x_i \partial x_j} \quad \text{ plus lower-order terms} =0.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;L u =\sum_{i=1}^n\sum_{j=1}^n a_{i,j} \frac{\partial^2 u}{\partial x_i \partial x_j} \quad \text{ plus lower-order terms} =0.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The classification depends upon the signature of the eigenvalues of the coefficient matrix {{math|''a''&amp;lt;sub&amp;gt;''i'',''j''&amp;lt;/sub&amp;gt;}}.&lt;br /&gt;
&lt;br /&gt;
The classification depends upon the signature of the eigenvalues of the coefficient matrix .&lt;br /&gt;
&lt;br /&gt;
这种分类取决于系数矩阵本征值的符号（正负性）。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
# Elliptic: the eigenvalues are all positive or all negative.&lt;br /&gt;
&lt;br /&gt;
 Elliptic: the eigenvalues are all positive or all negative.&lt;br /&gt;
&lt;br /&gt;
椭圆形方程: 本征值全部为正或全部为负。&lt;br /&gt;
&lt;br /&gt;
# Parabolic: the eigenvalues are all positive or all negative, save one that is zero.&lt;br /&gt;
&lt;br /&gt;
 Parabolic: the eigenvalues are all positive or all negative, save one that is zero.&lt;br /&gt;
&lt;br /&gt;
抛物线形方程: 本征值全部为正或全部为负，除了一个为零。&lt;br /&gt;
&lt;br /&gt;
# Hyperbolic: there is only one negative eigenvalue and all the rest are positive, or there is only one positive eigenvalue and all the rest are negative.&lt;br /&gt;
&lt;br /&gt;
 Hyperbolic: there is only one negative eigenvalue and all the rest are positive, or there is only one positive eigenvalue and all the rest are negative.&lt;br /&gt;
&lt;br /&gt;
双曲形方程: 只有一个负特征值，其余的都是正特征值，或者只有一个正特征值，其余的都是负特征值。&lt;br /&gt;
&lt;br /&gt;
# Ultrahyperbolic: there is more than one positive eigenvalue and more than one negative eigenvalue, and there are no zero eigenvalues. There is only a limited theory for ultrahyperbolic equations (Courant and Hilbert, 1962).&lt;br /&gt;
&lt;br /&gt;
 Ultrahyperbolic: there is more than one positive eigenvalue and more than one negative eigenvalue, and there are no zero eigenvalues. There is only a limited theory for ultrahyperbolic equations (Courant and Hilbert, 1962).&lt;br /&gt;
&lt;br /&gt;
超双形方程: 存在多于一个正本征值和多于一个的负本征值，且不存在零本征值。对于超双曲方程，只存在一个有限理论(Courant 和 Hilbert，1962)。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==[[用户:Yuling|Yuling]]（[[用户讨论:Yuling|讨论]]） 我对于limited theory这个单词对应的相关理论不太了解。&lt;br /&gt;
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=== Systems of first-order equations and characteristic surfaces ===&lt;br /&gt;
一阶方程组和特征曲面&lt;br /&gt;
&lt;br /&gt;
The classification of partial differential equations can be extended to systems of first-order equations, where the unknown {{mvar|u}} is now a [[Euclidean vector|vector]] with {{mvar|m}} components, and the coefficient matrices {{mvar|A&amp;lt;sub&amp;gt;ν&amp;lt;/sub&amp;gt;}} are {{mvar|m}} by {{mvar|m}} matrices for {{math|''ν'' {{=}} 1, 2,… ''n''}}. The partial differential equation takes the form&lt;br /&gt;
&lt;br /&gt;
The classification of partial differential equations can be extended to systems of first-order equations, where the unknown  is now a vector with  components, and the coefficient matrices  are  by  matrices for  1, 2,… n}}. The partial differential equation takes the form&lt;br /&gt;
&lt;br /&gt;
偏微分方程组的分类可以推广到一阶方程组，其中未知量 {{mvar|u}} 是有 {{mvar|m}} 个分量的向量。对于 {{math|''ν'' {{=}} 1, 2,… ''n''}}，系数矩阵 {{mvar|A&amp;lt;sub&amp;gt;ν&amp;lt;/sub&amp;gt;}} 是 {{mvar|m}} × {{mvar|m}} 的矩阵。偏微分方程形式如下：&lt;br /&gt;
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&lt;br /&gt;
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: &amp;lt;math&amp;gt;Lu = \sum_{\nu=1}^{n} A_\nu \frac{\partial u}{\partial x_\nu} + B=0,&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;Lu = \sum_{\nu=1}^{n} A_\nu \frac{\partial u}{\partial x_\nu} + B=0,&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
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where the coefficient matrices {{mvar|A&amp;lt;sub&amp;gt;ν&amp;lt;/sub&amp;gt;}} and the vector {{mvar|B}} may depend upon {{mvar|x}} and {{mvar|u}}. If a [[hypersurface]] {{mvar|S}} is given in the implicit form&lt;br /&gt;
&lt;br /&gt;
where the coefficient matrices  and the vector  may depend upon  and . If a hypersurface  is given in the implicit form&lt;br /&gt;
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其中系数矩阵 {{mvar|A&amp;lt;sub&amp;gt;ν&amp;lt;/sub&amp;gt;}} 和向量 {{mvar|B}} 可能依赖于 {{mvar|x}} 和 {{mvar|u}}。如果超曲面是以隐式形式给出的&lt;br /&gt;
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: &amp;lt;math&amp;gt;\varphi(x_1, x_2, \ldots x_n)=0,&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;\varphi(x_1, x_2, \ldots x_n)=0,&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
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where {{mvar|φ}} has a non-zero gradient, then {{mvar|S}} is a '''characteristic surface''' for the operator {{mvar|L}} at a given point if the characteristic form vanishes:&lt;br /&gt;
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where  has a non-zero gradient, then  is a characteristic surface for the operator  at a given point if the characteristic form vanishes:&lt;br /&gt;
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其中存在一个非零的梯度，那么如果特征形式消失，则在给定点上算子的特征曲面形式如下:&lt;br /&gt;
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: &amp;lt;math&amp;gt;Q\left(\frac{\partial\varphi}{\partial x_1}, \ldots\frac{\partial\varphi}{\partial x_n}\right) =\det\left[\sum_{\nu=1}^nA_\nu \frac{\partial \varphi}{\partial x_\nu}\right]=0.\,&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;Q\left(\frac{\partial\varphi}{\partial x_1}, \ldots\frac{\partial\varphi}{\partial x_n}\right) =\det\left[\sum_{\nu=1}^nA_\nu \frac{\partial \varphi}{\partial x_\nu}\right]=0.\,&amp;lt;/math&amp;gt;&lt;br /&gt;
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The geometric interpretation of this condition is as follows: if data for {{mvar|u}} are prescribed on the surface {{mvar|S}}, then it may be possible to determine the normal derivative of {{mvar|u}} on {{mvar|S}} from the differential equation. If the data on {{mvar|S}} and the differential equation determine the normal derivative of {{mvar|u}} on {{mvar|S}}, then {{mvar|S}} is non-characteristic. If the data on {{mvar|S}} and the differential equation ''do not'' determine the normal derivative of {{mvar|u}} on {{mvar|S}}, then the surface is '''characteristic''', and the differential equation restricts the data on {{mvar|S}}: the differential equation is ''internal'' to {{mvar|S}}.&lt;br /&gt;
&lt;br /&gt;
The geometric interpretation of this condition is as follows: if data for  are prescribed on the surface , then it may be possible to determine the normal derivative of  on  from the differential equation. If the data on  and the differential equation determine the normal derivative of  on , then  is non-characteristic. If the data on  and the differential equation do not determine the normal derivative of  on , then the surface is characteristic, and the differential equation restricts the data on : the differential equation is internal to .&lt;br /&gt;
&lt;br /&gt;
这个条件的几何解释如下: 如果关于 {{mvar|u}} 的数据是在曲面 {{mvar|S}} 上规定的，那么就有可能依据微分方程确定曲面 {{mvar|S}} 上 {{mvar|u}} 的法向导数。如果曲面 {{mvar|S}} 上的数据和上面的微分方程能确定曲面 {{mvar|S}} 上 {{mvar|u}} 的法向导数，那么它就是非特征的。如果曲面 {{mvar|S}} 上的数据和上面的微分方程不能确定曲面 {{mvar|S}} 上 {{mvar|u}} 的法向导数，那么曲面是特征的，并且微分方程将数据限制在曲面 {{mvar|S}} 上：微分方程是在曲面 {{mvar|S}} 内部。&lt;br /&gt;
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# A first-order system {{math|''Lu'' {{=}} 0}} is ''elliptic'' if no surface is characteristic for {{mvar|L}}: the values of {{mvar|u}} on {{mvar|S}} and the differential equation always determine the normal derivative of {{mvar|u}} on {{mvar|S}}.&lt;br /&gt;
&lt;br /&gt;
 A first-order system  0}} is elliptic if no surface is characteristic for : the values of  on  and the differential equation always determine the normal derivative of  on .&lt;br /&gt;
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如果对于 {{mvar|L}} 没有曲面是特征的，则一阶系统 {{math|''Lu'' {{=}} 0}} 是椭圆形的：{{mvar|u}}在 {{mvar|S}} 的值和微分方程总能够决定 {{mvar|S}} 上 {{mvar|u}} 的法向导数。&lt;br /&gt;
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# A first-order system is ''hyperbolic'' at a point if there is a '''spacelike''' surface {{mvar|S}} with normal {{mvar|ξ}} at that point. This means that, given any non-trivial vector {{mvar|η}} orthogonal to {{mvar|ξ}}, and a scalar multiplier {{mvar|λ}}, the equation {{math|''Q''(''λξ'' + ''η'') {{=}} 0}} has {{mvar|m}} real roots {{math|''λ''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;, ''λ''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;,… ''λ''&amp;lt;sub&amp;gt;''m''&amp;lt;/sub&amp;gt;}}. The system is '''strictly hyperbolic''' if these roots are always distinct. The geometrical interpretation of this condition is as follows: the characteristic form {{math|''Q''(''ζ'') {{=}} 0}} defines a cone (the normal cone) with homogeneous coordinates ζ. In the hyperbolic case, this cone has {{mvar|m}} sheets, and the axis {{math|''ζ'' {{=}} ''λξ''}} runs inside these sheets: it does not intersect any of them. But when displaced from the origin by η, this axis intersects every sheet. In the elliptic case, the normal cone has no real sheets.&lt;br /&gt;
&lt;br /&gt;
 A first-order system is hyperbolic at a point if there is a spacelike surface  with normal  at that point. This means that, given any non-trivial vector  orthogonal to , and a scalar multiplier , the equation  0}} has  real roots . The system is strictly hyperbolic if these roots are always distinct. The geometrical interpretation of this condition is as follows: the characteristic form  0}} defines a cone (the normal cone) with homogeneous coordinates ζ. In the hyperbolic case, this cone has  sheets, and the axis  λξ}} runs inside these sheets: it does not intersect any of them. But when displaced from the origin by η, this axis intersects every sheet. In the elliptic case, the normal cone has no real sheets.&lt;br /&gt;
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如果在该点存在一个法向量为 {{mvar|ξ}}的 '''&amp;lt;font color=&amp;quot;#ff8000&amp;quot;&amp;gt;类空曲面 Spacclike Surface&amp;lt;/font&amp;gt; {{mvar|S}} ，则一阶系统在那一点是双曲的。这意味着，给定任意正交于 {{mvar|ξ}} 的非平凡向量 {{mvar|η}} 和一个标量乘子 {{mvar|λ}}，方程 {{math|''Q''(''λξ'' + ''η'') {{=}} 0}} 有 {{mvar|m}} 个实根 {{math|''λ''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;, ''λ''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;,… ''λ''&amp;lt;sub&amp;gt;''m''&amp;lt;/sub&amp;gt;}}。如果这些根始终不同，则该系统是严格双曲形的。这个条件的几何解释如下: 特征形式 {{math|''Q''(''ζ'') {{=}} 0}} 定义了一个具有齐次坐标 ζ的圆锥(法线圆锥)。在双曲形的情况下，这个圆锥体有 {{mvar|m}} 层，并且轴 {{math|''ζ'' {{=}} ''λξ''}} 在这些层中运动: 它不与任何一层相交。但是当从原点偏离η时，这条轴线与每一层都相交。在椭圆形的情况下，法向圆锥没有实层。&lt;br /&gt;
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==[[用户:Yuling|Yuling]]（[[用户讨论:Yuling|讨论]]） sheet 这个单词也不很理解，我直译为了“层”&lt;br /&gt;
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=== Equations of mixed type ===&lt;br /&gt;
混合型方程&lt;br /&gt;
&lt;br /&gt;
If a PDE has coefficients that are not constant, it is possible that it will not belong to any of these categories but rather be of '''mixed type'''. A simple but important example is the [[Euler–Tricomi equation]]&lt;br /&gt;
&lt;br /&gt;
If a PDE has coefficients that are not constant, it is possible that it will not belong to any of these categories but rather be of mixed type. A simple but important example is the Euler–Tricomi equation&lt;br /&gt;
&lt;br /&gt;
如果偏微分方程的系数不是常数，那么它可能不属于这些类别中的任何一个，而是属于混合类型。一个简单但重要的例子是欧拉-特里科米方程&lt;br /&gt;
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: &amp;lt;math&amp;gt;u_{xx} = xu_{yy},&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;u_{xx} = xu_{yy},&amp;lt;/math&amp;gt;&lt;br /&gt;
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which is called '''elliptic-hyperbolic''' because it is elliptic in the region {{math|''x'' &amp;lt; 0}}, hyperbolic in the region {{math|''x'' &amp;gt; 0}}, and degenerate parabolic on the line {{math|''x'' {{=}} 0}}.&lt;br /&gt;
&lt;br /&gt;
which is called elliptic-hyperbolic because it is elliptic in the region , hyperbolic in the region , and degenerate parabolic on the line  0}}.&lt;br /&gt;
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它在 {{math|''x'' &amp;lt; 0}} 的区域上是椭圆形，在 {{math|''x'' &amp;gt; 0}} 区域上是双曲形，在 {{math|''x'' {{=}} 0}}这条线上是退化为抛物线形，因此称之为椭圆-双曲型。&lt;br /&gt;
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&amp;lt;!--&lt;br /&gt;
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&amp;lt;!--&lt;br /&gt;
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&amp;lt;!--&lt;br /&gt;
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''fill in: Dirichlet and Neumann boundaries, hyperbolic/parabolic/elliptic separation of variables, [[Fourier analysis]], [[Green's function]]s ...--&amp;gt;&lt;br /&gt;
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fill in: Dirichlet and Neumann boundaries, hyperbolic/parabolic/elliptic separation of variables, Fourier analysis, Green's functions ...--&amp;gt;&lt;br /&gt;
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填写: Dirichlet 和 Neumann 边界，双曲 / 抛物线 / 椭圆分离变量法，傅立叶分析，Green 函数... --&lt;br /&gt;
&lt;br /&gt;
=== Infinite-order PDEs in quantum mechanics ===&lt;br /&gt;
量子力学中的无限阶偏微分方程&lt;br /&gt;
&lt;br /&gt;
In the [[phase space formulation]] of quantum mechanics,  one may consider the [[Method of quantum characteristics|quantum Hamilton's equations]] for trajectories of quantum particles. These equations are infinite-order PDEs. However, in the semiclassical expansion, one has a finite system of ODEs at any fixed order of [[Dirac constant|{{mvar|ħ}}]].  The evolution equation of the [[Wigner quasi-probability distribution|c]] is also an infinite-order PDE. The quantum trajectories are [[Method of quantum characteristics|quantum characteristics]], with the use of which one could calculate the evolution of the Wigner function.&lt;br /&gt;
&lt;br /&gt;
In the phase space formulation of quantum mechanics,  one may consider the quantum Hamilton's equations for trajectories of quantum particles. These equations are infinite-order PDEs. However, in the semiclassical expansion, one has a finite system of ODEs at any fixed order of Dirac constant|.  The evolution equation of the Wigner function is also an infinite-order PDE. The quantum trajectories are quantum characteristics, with the use of which one could calculate the evolution of the Wigner function.&lt;br /&gt;
&lt;br /&gt;
在量子力学中的相空间表述中，我们可以考虑用于求解量子粒子的轨迹的量子哈密顿的方程。这些方程是无限阶偏微分方程。然而，在半经典展开中，我们在给定[[Dirac constant|{{mvar|ħ}}]]阶数下有一个有限的的常微分方程组。'''&amp;lt;font color=&amp;quot;#ff8000&amp;quot;&amp;gt;维格纳函数  Wigner Function&amp;lt;/font&amp;gt;的演化方程也是一个无限阶偏微分方程。由于量子轨道的量子特性，所以它通常可以用来计算维格纳函数的演化。&lt;br /&gt;
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== Analytical solutions ==&lt;br /&gt;
解析解&lt;br /&gt;
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===Separation of variables===&lt;br /&gt;
分离变量法&lt;br /&gt;
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{{main|Separable partial differential equation}}&lt;br /&gt;
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Linear PDEs can be reduced to systems of ordinary differential equations by the important technique of separation of variables. This technique rests on a characteristic of solutions to differential equations: if one can find any solution that solves the equation and satisfies the boundary conditions, then it is ''the'' solution (this also applies to ODEs). We assume as an [[ansatz]] that the dependence of a solution on the parameters space and time can be written as a product of terms that each depend on a single parameter, and then see if this can be made to solve the problem.&amp;lt;ref&amp;gt;{{cite book|last1=Gershenfeld|first1=Neil|title=The nature of mathematical modeling|date=2000|publisher=Cambridge Univ. Press|location=Cambridge|isbn=0521570956|page=27|edition=Reprinted (with corr.)}}&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
Linear PDEs can be reduced to systems of ordinary differential equations by the important technique of separation of variables. This technique rests on a characteristic of solutions to differential equations: if one can find any solution that solves the equation and satisfies the boundary conditions, then it is the solution (this also applies to ODEs). We assume as an ansatz that the dependence of a solution on the parameters space and time can be written as a product of terms that each depend on a single parameter, and then see if this can be made to solve the problem.&lt;br /&gt;
&lt;br /&gt;
线性偏微分方程组可以通过分离变量法这一重要方法来简化为常微分方程组。这种方法依赖于微分方程解的一个特征: 如果能找到任何一个满足方程和边界条件的解，那么这个解就是方程的解(这也适用于常微分方程)。我们假设解对参数空间和时间的依赖可以写成对它们每一项的依赖以及一个参数的乘积，然后再看看这是否可以用来解决这个问题。&lt;br /&gt;
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In the method of separation of variables, one reduces a PDE to a PDE in fewer variables, which is an ordinary differential equation if in one variable – these are in turn easier to solve.&lt;br /&gt;
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In the method of separation of variables, one reduces a PDE to a PDE in fewer variables, which is an ordinary differential equation if in one variable – these are in turn easier to solve.&lt;br /&gt;
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在分离变量法方法中，可以将偏微分方程简化为含有更少变量的偏微分方程，如果只有一个变量，那么就变成了一个'''&amp;lt;font color = &amp;quot;#ff8000&amp;quot;&amp;gt;常微分方程 Ordinary Differential Equation&amp;lt;/font&amp;gt;'''-- 反过来，这些方程也更容易求解。&lt;br /&gt;
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This is possible for simple PDEs, which are called [[separable partial differential equation]]s, and the domain is generally a rectangle (a product of intervals). Separable PDEs correspond to [[diagonal matrices]] – thinking of &amp;quot;the value for fixed {{mvar|x}}&amp;quot; as a coordinate, each coordinate can be understood separately.&lt;br /&gt;
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This is possible for simple PDEs, which are called separable partial differential equations, and the domain is generally a rectangle (a product of intervals). Separable PDEs correspond to diagonal matrices – thinking of &amp;quot;the value for fixed &amp;quot; as a coordinate, each coordinate can be understood separately.&lt;br /&gt;
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对于简单的偏微分方程(称为可分离偏微分方程)来说，这是可能的，而且方程通常定义在一个矩形区域(区间的乘积)上。可分离偏微分方程对应于对角线矩阵——以“固定值”为坐标，每个坐标可分开理解。&lt;br /&gt;
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This generalizes to the [[method of characteristics]], and is also used in [[integral transform]]s.&lt;br /&gt;
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This generalizes to the method of characteristics, and is also used in integral transforms.&lt;br /&gt;
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这种方法可以推广到特征曲线法，也可以用于积分变换。&lt;br /&gt;
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===Method of characteristics===&lt;br /&gt;
特征曲线法&lt;br /&gt;
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{{main|Method of characteristics}}&lt;br /&gt;
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In special cases, one can find characteristic curves on which the equation reduces to an ODE – changing coordinates in the domain to straighten these curves allows separation of variables, and is called the [[method of characteristics]].&lt;br /&gt;
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In special cases, one can find characteristic curves on which the equation reduces to an ODE – changing coordinates in the domain to straighten these curves allows separation of variables, and is called the method of characteristics.&lt;br /&gt;
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在特殊情况下，可以找到一些特征曲线，在这些曲线上方程可以变成一个常微分方程——意味着改变坐标从而使这些曲线变直从而达到分离变量的目的，这就是所谓的特征曲线法。&lt;br /&gt;
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More generally, one may find characteristic surfaces.&lt;br /&gt;
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More generally, one may find characteristic surfaces.&lt;br /&gt;
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更一般地说，人们可能会找到特征表面。&lt;br /&gt;
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===Integral transform===&lt;br /&gt;
积分变换&lt;br /&gt;
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An [[integral transform]] may transform the PDE to a simpler one, in particular, a separable PDE. This corresponds to diagonalizing an operator.&lt;br /&gt;
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An integral transform may transform the PDE to a simpler one, in particular, a separable PDE. This corresponds to diagonalizing an operator.&lt;br /&gt;
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积分变换可以将偏微分方程转换为更简单的偏微分方程，特别是可分离的偏微分方程。这对应于对角化算符。&lt;br /&gt;
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An important example of this is [[Fourier analysis]], which diagonalizes the heat equation using the [[eigenbasis]] of sinusoidal waves.&lt;br /&gt;
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An important example of this is Fourier analysis, which diagonalizes the heat equation using the eigenbasis of sinusoidal waves.&lt;br /&gt;
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这方面的一个重要例子是'''&amp;lt;font color = &amp;quot;#ff8000&amp;quot;&amp;gt;傅里叶分析  Fourier Analysis&amp;lt;/font&amp;gt;'''，它使用正弦波的特征基来对角化热方程。&lt;br /&gt;
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If the domain is finite or periodic, an infinite sum of solutions such as a [[Fourier series]] is appropriate, but an integral of solutions such as a [[Fourier integral]] is generally required for infinite domains. The solution for a point source for the heat equation given above is an example of the use of a Fourier integral.&lt;br /&gt;
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If the domain is finite or periodic, an infinite sum of solutions such as a Fourier series is appropriate, but an integral of solutions such as a Fourier integral is generally required for infinite domains. The solution for a point source for the heat equation given above is an example of the use of a Fourier integral.&lt;br /&gt;
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如果区域是有限的或周期性的，那么解为无限和的形式是恰当的，例如傅里叶级数，但是一个解的积分，例如傅立叶积分，一般是在无限区域上的。上面给出的热传导方程的点源解法就是使用傅里叶积分的一个例子。&lt;br /&gt;
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===Change of variables===&lt;br /&gt;
变量代换&lt;br /&gt;
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Often a PDE can be reduced to a simpler form with a known solution by a suitable [[Change of variables (PDE)|change of variables]].  For example, the [[Black–Scholes equation#Derivation|Black–Scholes]] PDE&lt;br /&gt;
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Often a PDE can be reduced to a simpler form with a known solution by a suitable change of variables.  For example, the Black–Scholes PDE&lt;br /&gt;
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偏微分方程通常可以通过变量的适当变化，用已知的解简化为更简单的形式。例如，布莱克-舒尔斯偏微分方程&lt;br /&gt;
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:&amp;lt;math&amp;gt; \frac{\partial V}{\partial t} + \tfrac{1}{2}\sigma^2 S^2\frac{\partial^2 V}{\partial S^2} + rS\frac{\partial V}{\partial S} - rV = 0 &amp;lt;/math&amp;gt;&lt;br /&gt;
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&amp;lt;math&amp;gt; \frac{\partial V}{\partial t} + \tfrac{1}{2}\sigma^2 S^2\frac{\partial^2 V}{\partial S^2} + rS\frac{\partial V}{\partial S} - rV = 0 &amp;lt;/math&amp;gt;&lt;br /&gt;
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is reducible to the [[heat equation]]&lt;br /&gt;
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is reducible to the heat equation&lt;br /&gt;
&lt;br /&gt;
可以简化为热传导方程&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt; \frac{\partial u}{\partial \tau} = \frac{\partial^2 u}{\partial x^2}&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \frac{\partial u}{\partial \tau} = \frac{\partial^2 u}{\partial x^2}&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
by the change of variables (for complete details see {{webarchive |url=https://web.archive.org/web/20080411030405/http://www.math.unl.edu/~sdunbar1/Teaching/MathematicalFinance/Lessons/BlackScholes/Solution/solution.shtml |date=April 11, 2008 |title=Solution of the Black Scholes Equation }})&lt;br /&gt;
&lt;br /&gt;
by the change of variables (for complete details see )&lt;br /&gt;
&lt;br /&gt;
通过变量替换(完整的细节见)&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt;\begin{align}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
V(S,t) &amp;amp;= K v(x,\tau),\\[5px]&lt;br /&gt;
&lt;br /&gt;
x &amp;amp;= \ln\left(\tfrac{S}{K} \right),\\[5px]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
\tau &amp;amp;= \tfrac{1}{2} \sigma^2 (T - t),\\[5px]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
v(x,\tau)&amp;amp;=e^{-\alpha x-\beta\tau} u(x,\tau).&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
\end{align}&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
===Fundamental solution===&lt;br /&gt;
基本解&lt;br /&gt;
&lt;br /&gt;
{{main|Fundamental solution}}&lt;br /&gt;
&lt;br /&gt;
Inhomogeneous equations can often be solved (for constant coefficient PDEs, always be solved) by finding the [[fundamental solution]] (the solution for a point source), then taking the [[convolution]] with the boundary conditions to get the solution.&lt;br /&gt;
&lt;br /&gt;
Inhomogeneous equations can often be solved (for constant coefficient PDEs, always be solved) by finding the fundamental solution (the solution for a point source), then taking the convolution with the boundary conditions to get the solution.&lt;br /&gt;
&lt;br /&gt;
非齐次方程(常系数偏微分方程)一般是通过先求出基本解(点源的解) ，然后利用带边界条件的卷积来求解。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
This is analogous in [[signal processing]] to understanding a filter by its [[impulse response]].&lt;br /&gt;
&lt;br /&gt;
This is analogous in signal processing to understanding a filter by its impulse response.&lt;br /&gt;
&lt;br /&gt;
这类似于在信号处理中通过滤波器的脉冲响应来理解滤波器。&lt;br /&gt;
&lt;br /&gt;
===Superposition principle===&lt;br /&gt;
叠加原理&lt;br /&gt;
&lt;br /&gt;
{{further| Superposition principle }}&lt;br /&gt;
&lt;br /&gt;
The superposition principle applies to any linear system, including linear systems of PDEs. A common visualization of this concept is the interaction of two waves in phase being combined to result in a greater amplitude, for example {{math|sin ''x'' + sin ''x'' {{=}} 2 sin ''x''}}. The same principle can be observed in PDEs where the solutions may be real or complex and additive. [[Superposition principle|superposition]]&lt;br /&gt;
&lt;br /&gt;
The superposition principle applies to any linear system, including linear systems of PDEs. A common visualization of this concept is the interaction of two waves in phase being combined to result in a greater amplitude, for example  2 sin x}}. The same principle can be observed in PDEs where the solutions may be real or complex and additive. superposition&lt;br /&gt;
&lt;br /&gt;
'''&amp;lt;font color = &amp;quot;#ff8000&amp;quot;&amp;gt;叠加原理 Superposition Principle&amp;lt;/font&amp;gt;适用于任何线性系统，包括偏微分方程的线性系统。这个概念的一个常见的可视化是两个同相位的波相互作用结合在一起会产生更大的振幅，例如 {{math|sin ''x'' + sin ''x'' {{=}} 2 sin ''x''}}。在偏微分方程中也可以观察到同样的原理，其中的解可能是真实的或复杂的和可加的。叠加&lt;br /&gt;
&lt;br /&gt;
If {{math|''u''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;}} and {{math|''u''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;}} are solutions of linear PDE in some function space {{mvar|R}}, then {{math|''u'' {{=}} ''c''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;''u''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; + ''c''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;''u''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;}} with any constants {{math|''c''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;}} and {{math|''c''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;}} are also a solution of that PDE in the same function space.&lt;br /&gt;
&lt;br /&gt;
If  and  are solutions of linear PDE in some function space , then  c&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;u&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; + c&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;u&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;}} with any constants  and  are also a solution of that PDE in the same function space.&lt;br /&gt;
&lt;br /&gt;
若线性偏微分方程在某个函数空间{{mvar|R}}中有解{{math|''u''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;}} 和 {{math|''u''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;}}，则{{math|''u'' {{=}} ''c''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;''u''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; + ''c''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;''u''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;}}也是该偏微分方程在同一函数空间中的解，其中{{math|''c''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;}} 和 {{math|''c''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;}} 是任意常数。&lt;br /&gt;
&lt;br /&gt;
===Methods for non-linear equations===&lt;br /&gt;
非线性方程的求解方法&lt;br /&gt;
{{see also|nonlinear partial differential equation}}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
There are no generally applicable methods to solve nonlinear PDEs. Still, existence and uniqueness results (such as the [[Cauchy–Kowalevski theorem]]) are often possible, as are proofs of important qualitative and quantitative properties of solutions (getting these results is a major part of [[mathematical analysis|analysis]]). Computational solution to the nonlinear PDEs, the [[split-step method]], exist for specific equations like [[nonlinear Schrödinger equation]].&lt;br /&gt;
&lt;br /&gt;
There are no generally applicable methods to solve nonlinear PDEs. Still, existence and uniqueness results (such as the Cauchy–Kowalevski theorem) are often possible, as are proofs of important qualitative and quantitative properties of solutions (getting these results is a major part of analysis). Computational solution to the nonlinear PDEs, the split-step method, exist for specific equations like nonlinear Schrödinger equation.&lt;br /&gt;
&lt;br /&gt;
对于非线性偏微分方程，目前还没有普遍适用的求解方法。然而，通常是可能知道解的存在性和唯一性(如柯西-科瓦列夫斯基定理)，也是可能得到解的重要定性和定量性质的证明(得到这些结果是分析的主要部分)。非线性偏微分方程的计算解，即分步法，对一些特定的方程适用，比如非线性'''&amp;lt;font color=&amp;quot;#ff8000&amp;quot;&amp;gt;薛定谔方程 Schrödinger equation&amp;lt;/font&amp;gt;'''。&lt;br /&gt;
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&lt;br /&gt;
&lt;br /&gt;
Nevertheless, some techniques can be used for several types of equations. The [[h-principle|{{mvar|h}}-principle]] is the most powerful method to solve [[Underdetermined system|underdetermined]] equations. The [[Riquier–Janet theory]] is an effective method for obtaining information about many analytic [[Overdetermined system|overdetermined]] systems.&lt;br /&gt;
&lt;br /&gt;
Nevertheless, some techniques can be used for several types of equations. The -principle is the most powerful method to solve underdetermined equations. The Riquier–Janet theory is an effective method for obtaining information about many analytic overdetermined systems.&lt;br /&gt;
&lt;br /&gt;
然而，一些技巧可以用于几种类型的方程。h-原理是求解欠定方程最有效的方法。里基尔-珍妮特理论是一种可以获得许多解析超定系统信息的有效方法。&lt;br /&gt;
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&lt;br /&gt;
&lt;br /&gt;
The [[method of characteristics]] can be used in some very special cases to solve partial differential equations.&lt;br /&gt;
&lt;br /&gt;
The method of characteristics can be used in some very special cases to solve partial differential equations.&lt;br /&gt;
&lt;br /&gt;
特征线法可用于求解某些特殊情况下的偏微分方程。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
In some cases, a PDE can be solved via [[perturbation analysis]] in which the solution is considered to be a correction to an equation with a known solution. Alternatives are [[numerical analysis]] techniques from simple [[finite difference]] schemes to the more mature [[multigrid]] and [[finite element method]]s. Many interesting problems in science and engineering are solved in this way using [[computer]]s, sometimes high performance [[supercomputer]]s.&lt;br /&gt;
&lt;br /&gt;
In some cases, a PDE can be solved via perturbation analysis in which the solution is considered to be a correction to an equation with a known solution. Alternatives are numerical analysis techniques from simple finite difference schemes to the more mature multigrid and finite element methods. Many interesting problems in science and engineering are solved in this way using computers, sometimes high performance supercomputers.&lt;br /&gt;
&lt;br /&gt;
在某些情况下，偏微分方程可以通过扰动分析来求解。在扰动分析中，通常是求解将具有已知解的方程修正后的新得到方程。可供选择的数值分析技术从简单的差分格式到更成熟的多重网格和有限元方法。许多有趣的科学和工程问题都是在计算机上用这种方法解决的，有时是高性能超级计算机。&lt;br /&gt;
&lt;br /&gt;
===Lie group method===&lt;br /&gt;
李群方法&lt;br /&gt;
&lt;br /&gt;
From 1870 [[Sophus Lie]]'s work put the theory of differential equations on a more satisfactory foundation. He showed that the integration theories of the older mathematicians can, by the introduction of what are now called [[Lie group]]s, be referred, to a common source; and that ordinary differential equations which admit the same [[infinitesimal transformation]]s present comparable difficulties of integration. He also emphasized the subject of [[contact transformation|transformations of contact]].&lt;br /&gt;
&lt;br /&gt;
From 1870 Sophus Lie's work put the theory of differential equations on a more satisfactory foundation. He showed that the integration theories of the older mathematicians can, by the introduction of what are now called Lie groups, be referred, to a common source; and that ordinary differential equations which admit the same infinitesimal transformations present comparable difficulties of integration. He also emphasized the subject of transformations of contact.&lt;br /&gt;
&lt;br /&gt;
从1870年起，索弗斯·李的工作为微分方程理论奠定了一个较为令人满意的基础。他指出，通过引入现在所谓的李群，老一辈数学家的积分理论可以引用到一个共同的来源; 承认相同的无穷小变换的常微分方程在积分方面存在相当的困难。他还强调了接触的转变这一主题。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==[[用户:Yuling|Yuling]]（[[用户讨论:Yuling|讨论]]）这句话“He also emphasized the subject of transformations of contact.”中的transformations of contact翻译的不太好。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
A general approach to solving PDEs uses the symmetry property of differential equations, the continuous [[infinitesimal transformation]]s of solutions to solutions ([[Lie theory]]). Continuous [[group theory]], [[Lie algebras]] and [[differential geometry]] are used to understand the structure of linear and nonlinear partial differential equations for generating integrable equations, to find its [[Lax pair]]s, recursion operators, [[Bäcklund transform]] and finally finding exact analytic solutions to the PDE.&lt;br /&gt;
&lt;br /&gt;
A general approach to solving PDEs uses the symmetry property of differential equations, the continuous infinitesimal transformations of solutions to solutions (Lie theory). Continuous group theory, Lie algebras and differential geometry are used to understand the structure of linear and nonlinear partial differential equations for generating integrable equations, to find its Lax pairs, recursion operators, Bäcklund transform and finally finding exact analytic solutions to the PDE.&lt;br /&gt;
&lt;br /&gt;
求解偏微分方程的一般方法是利用微分方程的对称性，即解到解的连续无穷小变换(李理论)。连续群论、李代数和微分几何理论被用来理解生成可积方程的线性和非线性偏微分方程的结构，找到它的Lax对、递归算子、 贝克伦德变换，最后找到偏微分方程的精确解析解。&lt;br /&gt;
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Symmetry methods have been recognized to study differential equations arising in mathematics, physics, engineering, and many other disciplines.&lt;br /&gt;
&lt;br /&gt;
Symmetry methods have been recognized to study differential equations arising in mathematics, physics, engineering, and many other disciplines.&lt;br /&gt;
&lt;br /&gt;
对称方法已被公认可以用于研究出现在数学，物理，工程和许多其他学科的微分方程。&lt;br /&gt;
&lt;br /&gt;
===Semianalytical methods===&lt;br /&gt;
半解析方法&lt;br /&gt;
&lt;br /&gt;
The [[Adomian decomposition method]], the [[Aleksandr Lyapunov|Lyapunov]] artificial small parameter method, and He's [[homotopy perturbation method]] are all special cases of the more general [[homotopy analysis method]]. These are series expansion methods, and except for the Lyapunov method, are independent of small physical parameters as compared to the well known [[perturbation theory]], thus giving these methods greater flexibility and solution generality.&lt;br /&gt;
&lt;br /&gt;
The Adomian decomposition method, the Lyapunov artificial small parameter method, and He's homotopy perturbation method are all special cases of the more general homotopy analysis method. These are series expansion methods, and except for the Lyapunov method, are independent of small physical parameters as compared to the well known perturbation theory, thus giving these methods greater flexibility and solution generality.&lt;br /&gt;
&lt;br /&gt;
阿多米安分解法、李雅普诺夫人工小参数方法和何同伦摄动方法都是更一般的同伦分析方法的特殊情况。除了李雅普诺夫方法之外，这些都是级数展开方法，与为人熟知的摄动理论方法相比，它们与小的物理参数无关，因此这些方法具有更大的灵活性和解的通用性。&lt;br /&gt;
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== Numerical solutions ==&lt;br /&gt;
数值解&lt;br /&gt;
&lt;br /&gt;
The three most widely used [[Numerical partial differential equations|numerical methods to solve PDEs]] are the [[finite element analysis|finite element method]] (FEM), [[finite volume method]]s (FVM) and [[finite difference method]]s (FDM), as well other kind of methods called [[Meshfree methods]], which were made to solve problems where the before mentioned methods are limited. The FEM has a prominent position among these methods and especially its exceptionally efficient higher-order version [[hp-FEM]]. Other hybrid versions of FEM and Meshfree methods include the generalized finite element method (GFEM), [[extended finite element method]] (XFEM), [[Spectral element method|spectral finite element method]] (SFEM), [[Meshfree methods|meshfree finite element method]], [[Discontinuous Galerkin Method|discontinuous Galerkin finite element method]] (DGFEM), [[Element-Free Galerkin Method]] (EFGM), [[Interpolating Element-Free Galerkin Method]] (IEFGM), etc.&lt;br /&gt;
&lt;br /&gt;
The three most widely used numerical methods to solve PDEs are the finite element method (FEM), finite volume methods (FVM) and finite difference methods (FDM), as well other kind of methods called Meshfree methods, which were made to solve problems where the before mentioned methods are limited. The FEM has a prominent position among these methods and especially its exceptionally efficient higher-order version hp-FEM. Other hybrid versions of FEM and Meshfree methods include the generalized finite element method (GFEM), extended finite element method (XFEM), spectral finite element method (SFEM), meshfree finite element method, discontinuous Galerkin finite element method (DGFEM), Element-Free Galerkin Method (EFGM), Interpolating Element-Free Galerkin Method (IEFGM), etc.&lt;br /&gt;
&lt;br /&gt;
求解偏微分方程最常用的三种数值方法是有限元分析法、有限体积法和有限差分法，以及其他一些称为无网格法的方法。这些方法用于解决前面提到的方法受到的限制。在这些方法中，有限元方法，尤其是高效的高阶有限元方法，占有重要地位。其他有限元法和无网格法的混合形式包括广义有限元分析法(GFEM)、扩展有限元分析法(XFEM)、谱有限元分析法(SFEM)、无网格有限元分析法(DGFEM)、间断伽辽金有限元分析法(DGFEM)、无网格伽辽金法(EFGM)、插值无网格伽辽金法(IEFGM)等。&lt;br /&gt;
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=== Finite element method ===&lt;br /&gt;
有限元分析法&lt;br /&gt;
&lt;br /&gt;
{{main|Finite element method}}&lt;br /&gt;
&lt;br /&gt;
The finite element method (FEM) (its practical application often known as finite element analysis (FEA)) is a numerical technique for finding approximate solutions of partial differential equations (PDE) as well as of integral equations. The solution approach is based either on eliminating the differential equation completely (steady state problems), or rendering the PDE into an approximating system of ordinary differential equations, which are then numerically integrated using standard techniques such as Euler's method, Runge–Kutta, etc.&lt;br /&gt;
&lt;br /&gt;
The finite element method (FEM) (its practical application often known as finite element analysis (FEA)) is a numerical technique for finding approximate solutions of partial differential equations (PDE) as well as of integral equations. The solution approach is based either on eliminating the differential equation completely (steady state problems), or rendering the PDE into an approximating system of ordinary differential equations, which are then numerically integrated using standard techniques such as Euler's method, Runge–Kutta, etc.&lt;br /&gt;
&lt;br /&gt;
'''&amp;lt;font color = &amp;quot;#ff8000&amp;quot;&amp;gt;有限元分析法 Finite Element Method&amp;lt;/font&amp;gt;''' ((其实际应用通常被称为有限元分析(FEA))是一种寻找偏微分方程(PDE)和积分方程近似解的数值技术。这种求解方法要么基于完全消除微分方程(稳态问题) ，要么将偏微分方程转化为常微分方程的近似系统，然后使用标准技术进行数值积分，如欧拉方法、 Runge-Kutta 等。&lt;br /&gt;
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===Finite difference method===&lt;br /&gt;
有限差分法&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{{main|Finite difference method}}&lt;br /&gt;
&lt;br /&gt;
Finite-difference methods are numerical methods for approximating the solutions to differential equations using [[finite difference]] equations to approximate derivatives.&lt;br /&gt;
&lt;br /&gt;
Finite-difference methods are numerical methods for approximating the solutions to differential equations using finite difference equations to approximate derivatives.&lt;br /&gt;
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有限差分法是一种数值方法，用差分方程近似微分方程的解。&lt;br /&gt;
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=== Finite volume method ===&lt;br /&gt;
有限体积法&lt;br /&gt;
&lt;br /&gt;
{{main|Finite volume method}}&lt;br /&gt;
&lt;br /&gt;
Similar to the finite difference method or finite element method, values are calculated at discrete places on a meshed geometry. &amp;quot;Finite volume&amp;quot; refers to the small volume surrounding each node point on a mesh. In the finite volume method, surface integrals in a partial differential equation that contain a divergence term are converted to volume integrals, using the [[divergence theorem]]. These terms are then evaluated as fluxes at the surfaces of each finite volume. Because the flux entering a given volume is identical to that leaving the adjacent volume, these methods conserve mass by design.&lt;br /&gt;
&lt;br /&gt;
Similar to the finite difference method or finite element method, values are calculated at discrete places on a meshed geometry. &amp;quot;Finite volume&amp;quot; refers to the small volume surrounding each node point on a mesh. In the finite volume method, surface integrals in a partial differential equation that contain a divergence term are converted to volume integrals, using the divergence theorem. These terms are then evaluated as fluxes at the surfaces of each finite volume. Because the flux entering a given volume is identical to that leaving the adjacent volume, these methods conserve mass by design.&lt;br /&gt;
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类似于有限差分法或有限元分析，函数值是在网状几何体上的离散位置进行计算的。“有限体积”是指网格上每个节点周围的小体积。在有限体积法中，偏微分方程中含有散度项的面积分用散度定理积分转换成体积分。然后将这些项用于估算每个有限体积表面上的通量。由于进入给定体积的通量与转移到相邻体积元的通量相同，所以这些方法在设计上保证了质量守恒。&lt;br /&gt;
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==See also==&lt;br /&gt;
请参阅&lt;br /&gt;
* [[Dirichlet boundary condition]]&lt;br /&gt;
狄利克雷边界条件&lt;br /&gt;
* [[Jet bundle]]&lt;br /&gt;
射流丛&lt;br /&gt;
* [[Laplace transform applied to differential equations]]&lt;br /&gt;
微分方程中的拉普拉斯变换&lt;br /&gt;
* [[List of dynamical systems and differential equations topics]]&lt;br /&gt;
动力学系统和微分方程的列表&lt;br /&gt;
* [[Matrix differential equation]]&lt;br /&gt;
矩阵微分方程&lt;br /&gt;
* [[Neumann boundary condition]]&lt;br /&gt;
诺伊曼边界条件&lt;br /&gt;
* [[Numerical partial differential equations]]&lt;br /&gt;
数值偏微分方程&lt;br /&gt;
* [[Partial differential algebraic equation]]&lt;br /&gt;
偏微分代数方程&lt;br /&gt;
* [[Recurrence relation]]&lt;br /&gt;
递推关系&lt;br /&gt;
* [[Robin boundary condition]]&lt;br /&gt;
罗宾边界条件&lt;br /&gt;
* [[Stochastic processes and boundary value problems]]&lt;br /&gt;
随机过程和边值问题&lt;br /&gt;
&lt;br /&gt;
== The energy method ==&lt;br /&gt;
能量法&lt;br /&gt;
&lt;br /&gt;
The energy method is a mathematical procedure that can be used to verify well-posedness of initial-boundary-value-problems.&amp;lt;ref&amp;gt;{{cite book |title=High Order Difference Methods for Time Dependent PDE&lt;br /&gt;
&lt;br /&gt;
The energy method is a mathematical procedure that can be used to verify well-posedness of initial-boundary-value-problems.&amp;lt;ref&amp;gt;{{cite book |title=High Order Difference Methods for Time Dependent PDE&lt;br /&gt;
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能量法是验证初边值问题适定性的一种数学方法。 时变偏微分方程的高阶差分方法&lt;br /&gt;
&lt;br /&gt;
|first=Bertil|last=Gustafsson|publisher=Springer|year=2008|isbn=978-3-540-74992-9|doi=10.1007/978-3-540-74993-6}}&amp;lt;/ref&amp;gt; In the following example the energy method is used to decide where and which boundary conditions should be imposed such that the resulting IBVP is well-posed. Consider the one-dimensional hyperbolic PDE given by&lt;br /&gt;
&lt;br /&gt;
|first=Bertil|last=Gustafsson|publisher=Springer|year=2008|isbn=978-3-540-74992-9|doi=10.1007/978-3-540-74993-6}}&amp;lt;/ref&amp;gt; In the following example the energy method is used to decide where and which boundary conditions should be imposed such that the resulting IBVP is well-posed. Consider the one-dimensional hyperbolic PDE given by&lt;br /&gt;
&lt;br /&gt;
| first Bertil | last Gustafsson | publisher | Springer | year 2008 | isbn 978-3-540-74992-9 | doi 10.1007 / 978-3-540-74993-6} / ref 在下面的例子中，使用能量方法来决定应该施加哪些边界条件，使得得到的 IBVP适定。考虑一维双曲偏微分方程&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt;\frac{\partial u}{\partial t} + \alpha \frac{\partial u}{\partial x} = 0, \quad x \in [a,b], \operatorname t &amp;gt; 0,&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;\frac{\partial u}{\partial t} + \alpha \frac{\partial u}{\partial x} = 0, \quad x \in [a,b], \operatorname t &amp;gt; 0,&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
where &amp;lt;math&amp;gt;\alpha \neq 0&amp;lt;/math&amp;gt; is a constant and &amp;lt;math&amp;gt;u(x,t)&amp;lt;/math&amp;gt; is an unknown function with initial condition &amp;lt;math&amp;gt;u(x,0) = f(x)&amp;lt;/math&amp;gt;. Multiplying with &amp;lt;math&amp;gt;u&amp;lt;/math&amp;gt; and integrating over the domain gives&lt;br /&gt;
&lt;br /&gt;
where &amp;lt;math&amp;gt;\alpha \neq 0&amp;lt;/math&amp;gt; is a constant and &amp;lt;math&amp;gt;u(x,t)&amp;lt;/math&amp;gt; is an unknown function with initial condition &amp;lt;math&amp;gt;u(x,0) = f(x)&amp;lt;/math&amp;gt;. Multiplying with &amp;lt;math&amp;gt;u&amp;lt;/math&amp;gt; and integrating over the domain gives&lt;br /&gt;
&lt;br /&gt;
其中 &amp;lt;math&amp;gt;\alpha \neq 0&amp;lt;/math&amp;gt; 是常数，并且 &amp;lt;math&amp;gt;u(x,t)&amp;lt;/math&amp;gt; 是未知函数，初始条件是 &amp;lt;math&amp;gt;u(x,0) = f(x)&amp;lt;/math&amp;gt;。乘以 &amp;lt;math&amp;gt;u&amp;lt;/math&amp;gt; 并在域上进行积分。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt;\int_a^b u \frac{\partial u}{\partial t} \operatorname dx + \alpha \int _a ^b u \frac{\partial u}{\partial x} \operatorname dx = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;\int_a^b u \frac{\partial u}{\partial t} \operatorname dx + \alpha \int _a ^b u \frac{\partial u}{\partial x} \operatorname dx = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Using that&lt;br /&gt;
&lt;br /&gt;
Using that&lt;br /&gt;
&lt;br /&gt;
利用这一点&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt;\int _a ^b u \frac{\partial u}{\partial t} \operatorname dx = \frac{1}{2} \frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 \quad \text{and} \quad \int _a ^b u \frac{\partial u}{\partial x} \operatorname dx = \frac{1}{2} u(b,t)^2 - \frac{1}{2} u(a,t)^2,.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;\int _a ^b u \frac{\partial u}{\partial t} \operatorname dx = \frac{1}{2} \frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 \quad \text{and} \quad \int _a ^b u \frac{\partial u}{\partial x} \operatorname dx = \frac{1}{2} u(b,t)^2 - \frac{1}{2} u(a,t)^2,.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
where integration by parts has been used for the second relationship, we get&lt;br /&gt;
&lt;br /&gt;
where integration by parts has been used for the second relationship, we get&lt;br /&gt;
&lt;br /&gt;
第二个关系中采用了分部积分法，我们可以得到&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt;\frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 + \alpha u(b,t)^2 - \alpha u(a,t)^2 = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;\frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 + \alpha u(b,t)^2 - \alpha u(a,t)^2 = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Here &amp;lt;math&amp;gt;\vert \vert \cdot \vert \vert&amp;lt;/math&amp;gt; denotes the standard L2-norm.&lt;br /&gt;
&lt;br /&gt;
Here &amp;lt;math&amp;gt;\vert \vert \cdot \vert \vert&amp;lt;/math&amp;gt; denotes the standard L2-norm.&lt;br /&gt;
&lt;br /&gt;
在这里，&amp;lt;math&amp;gt;\vert \vert \cdot \vert \vert&amp;lt;/math&amp;gt; 表示标准的 L2-正则。&lt;br /&gt;
&lt;br /&gt;
For well-posedness we require that the energy of the solution is non-increasing, i.e. that &amp;lt;math&amp;gt;\frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 \leq 0&amp;lt;/math&amp;gt;, which is achieved by specifying &amp;lt;math&amp;gt;u&amp;lt;/math&amp;gt; at &amp;lt;math&amp;gt;x = a&amp;lt;/math&amp;gt; if &amp;lt;math&amp;gt;\alpha &amp;gt; 0&amp;lt;/math&amp;gt; and at &amp;lt;math&amp;gt;x = b&amp;lt;/math&amp;gt; if &amp;lt;math&amp;gt;\alpha &amp;lt; 0&amp;lt;/math&amp;gt;. This corresponds to only imposing boundary conditions at the inflow. Note that well-posedness allows for growth in terms of data (initial and boundary) and thus it is sufficient to show that &amp;lt;math&amp;gt;\frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 \leq 0&amp;lt;/math&amp;gt; holds when all data is set to zero.&lt;br /&gt;
&lt;br /&gt;
For well-posedness we require that the energy of the solution is non-increasing, i.e. that &amp;lt;math&amp;gt;\frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 \leq 0&amp;lt;/math&amp;gt;, which is achieved by specifying &amp;lt;math&amp;gt;u&amp;lt;/math&amp;gt; at &amp;lt;math&amp;gt;x = a&amp;lt;/math&amp;gt; if &amp;lt;math&amp;gt;\alpha &amp;gt; 0&amp;lt;/math&amp;gt; and at &amp;lt;math&amp;gt;x = b&amp;lt;/math&amp;gt; if &amp;lt;math&amp;gt;\alpha &amp;lt; 0&amp;lt;/math&amp;gt;. This corresponds to only imposing boundary conditions at the inflow. Note that well-posedness allows for growth in terms of data (initial and boundary) and thus it is sufficient to show that &amp;lt;math&amp;gt;\frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 \leq 0&amp;lt;/math&amp;gt; holds when all data is set to zero.&lt;br /&gt;
&lt;br /&gt;
对于适定性，我们要解的能量是不增加的，即 &amp;lt;math&amp;gt;\frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 \leq 0&amp;lt;/math&amp;gt; ，这种关系可以通过在&amp;lt;math&amp;gt;x = a&amp;lt;/math&amp;gt;处 （如果 &amp;lt;math&amp;gt;\alpha &amp;gt; 0&amp;lt;/math&amp;gt;） 以及 &amp;lt;math&amp;gt;x = b&amp;lt;/math&amp;gt;处 （如果 &amp;lt;math&amp;gt;\alpha &amp;lt; 0&amp;lt;/math&amp;gt;）指定&amp;lt;math&amp;gt;u&amp;lt;/math&amp;gt;的值来实现。这只相当于在入流处附加边界条件。注意，适定性允许在数据(初始和边界)上的增长，因此它足以表明当所有数据设置为零时应有 &amp;lt;math&amp;gt;\frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 \leq 0&amp;lt;/math&amp;gt;。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==[[用户:Yuling|Yuling]]（[[用户讨论:Yuling|讨论]]）“This corresponds to only imposing boundary conditions at the inflow.” 这句话中的inflow不是很理解&lt;br /&gt;
&lt;br /&gt;
==Notes==&lt;br /&gt;
&lt;br /&gt;
{{Reflist}}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
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| first Bertil | last Gustafsson | Springer | year 2008 | isbn 978-3-540-74992-9 | doi 10.1007 / 978-3-540-74993-6}&lt;br /&gt;
&lt;br /&gt;
{{refend}}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
== Further reading ==&lt;br /&gt;
&lt;br /&gt;
* {{Cite journal|last=Cajori|first=Florian|authorlink=Florian Cajori|year=1928|title=The Early History of Partial Differential Equations and of Partial Differentiation and Integration|url=http://www.math.harvard.edu/archive/21a_fall_14/exhibits/cajori/cajori.pdf|journal=The American Mathematical Monthly|volume=35|issue=9|pages=459–467|doi=10.2307/2298771|access-date=2016-05-15|archive-url=https://web.archive.org/web/20181123102253/http://www.math.harvard.edu/archive/21a_fall_14/exhibits/cajori/cajori.pdf|archive-date=2018-11-23|url-status=dead}}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
== External links ==&lt;br /&gt;
&lt;br /&gt;
{{Sister project links| wikt=no | commons=Category:Solutions of PDE | b=Partial Differential Equations | n=no | q=Partial differential equation | s=no | v=no | voy=no | species=no | d=no}}&lt;br /&gt;
&lt;br /&gt;
* {{springer|title=Differential equation, partial|id=p/d031920}}&lt;br /&gt;
&lt;br /&gt;
* [http://eqworld.ipmnet.ru/en/pde-en.htm Partial Differential Equations: Exact Solutions] at EqWorld: The World of Mathematical Equations.&lt;br /&gt;
&lt;br /&gt;
* [http://eqworld.ipmnet.ru/en/solutions/eqindex/eqindex-pde.htm Partial Differential Equations: Index] at EqWorld: The World of Mathematical Equations.&lt;br /&gt;
&lt;br /&gt;
* [http://eqworld.ipmnet.ru/en/methods/meth-pde.htm Partial Differential Equations: Methods] at EqWorld: The World of Mathematical Equations.&lt;br /&gt;
&lt;br /&gt;
* [https://web.archive.org/web/20170701144823/http://www.exampleproblems.com/wiki/index.php?title=Partial_Differential_Equations Example problems with solutions] at exampleproblems.com&lt;br /&gt;
&lt;br /&gt;
* [http://mathworld.wolfram.com/PartialDifferentialEquation.html Partial Differential Equations] at mathworld.wolfram.com&lt;br /&gt;
&lt;br /&gt;
* [https://reference.wolfram.com/language/FEMDocumentation/tutorial/SolvingPDEwithFEM.html Partial Differential Equations] with Mathematica&lt;br /&gt;
&lt;br /&gt;
* [http://www.mathworks.com/moler/pdes.pdf Partial Differential Equations] in Cleve Moler: Numerical Computing with MATLAB&lt;br /&gt;
&lt;br /&gt;
* [http://www.nag.com/numeric/fl/nagdoc_fl24/html/D03/d03intro.html Partial Differential Equations] at nag.com&lt;br /&gt;
&lt;br /&gt;
* {{cite web |first=Grant |last=Sanderson |title=But what is a partial differential equation? |work=3Blue1Brown |date=April 21, 2019 |url=https://www.youtube.com/watch?v=ly4S0oi3Yz8&amp;amp;list=PLZHQObOWTQDNPOjrT6KVlfJuKtYTftqH6 |via=[[YouTube]] }}&lt;br /&gt;
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{{Differential equations topics}}&lt;br /&gt;
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&amp;lt;small&amp;gt;This page was moved from [[wikipedia:en:Partial differential equation]]. Its edit history can be viewed at [[偏微分方程/edithistory]]&amp;lt;/small&amp;gt;&amp;lt;/noinclude&amp;gt;&lt;br /&gt;
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[[Category:待整理页面]]&lt;/div&gt;</summary>
		<author><name>Ruili</name></author>
	</entry>
	<entry>
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		<title>偏微分方程</title>
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		<updated>2020-11-11T13:17:40Z</updated>

		<summary type="html">&lt;p&gt;Ruili：&lt;/p&gt;
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&lt;div&gt;此词条暂由Yuling翻译，未经人工整理和审校，带来阅读不便，请见谅。&lt;br /&gt;
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[[File:Heat.gif|thumb|right|A visualisation of a solution to the two-dimensional [[heat equation]] with temperature represented by the third dimension]]&lt;br /&gt;
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A visualisation of a solution to the two-dimensional [[heat equation with temperature represented by the third dimension]]&lt;br /&gt;
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以三维表示温度的二维热方程解的可视化&lt;br /&gt;
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In [[mathematics]], a '''partial differential equation''' ('''PDE''') is a [[differential equation]] that contains unknown [[Multivariable calculus|multivariable functions]] and their [[partial derivative]]s. PDEs are used to formulate problems involving functions of several variables, and are either solved by hand, or used to create a [[computer model]]. A special case is [[ordinary differential equation]]s (ODEs), which deal with functions of a single variable and their derivatives.&lt;br /&gt;
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In mathematics, a partial differential equation (PDE) is a differential equation that contains unknown multivariable functions and their partial derivatives. PDEs are used to formulate problems involving functions of several variables, and are either solved by hand, or used to create a computer model. A special case is ordinary differential equations (ODEs), which deal with functions of a single variable and their derivatives.&lt;br /&gt;
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在数学中，'''&amp;lt;font color = &amp;quot;#ff8000&amp;quot;&amp;gt;偏微分方程函数 Partial Differential Equation&amp;lt;/font&amp;gt;'''是包含未知多元函数及其偏导数的微分方程。偏微分方程用于描述涉及多元函数的问题，可以通过人为求解，也可以通过建立计算机模型来求解。常微分方程是偏微分方程一种特殊情况，它处理的是一元函数及其导数。&lt;br /&gt;
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PDEs can be used to describe a wide variety of phenomena such as sound, heat, [[diffusion]], [[electrostatics]], [[Electromagnetism|electrodynamics]], [[fluid dynamics]], [[Elasticity (physics)|elasticity]], [[gravitation]] and [[quantum mechanics]]. These seemingly distinct physical phenomena can be formalised similarly in terms of PDEs. Just as ordinary differential equations often model one-dimensional [[dynamical system]]s, partial differential equations often model [[multidimensional system]]s. PDEs find their generalisation in [[stochastic partial differential equation]]s.&lt;br /&gt;
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PDEs can be used to describe a wide variety of phenomena such as sound, heat, diffusion, electrostatics, electrodynamics, fluid dynamics, elasticity, gravitation and quantum mechanics. These seemingly distinct physical phenomena can be formalised similarly in terms of PDEs. Just as ordinary differential equations often model one-dimensional dynamical systems, partial differential equations often model multidimensional systems. PDEs find their generalisation in stochastic partial differential equations.&lt;br /&gt;
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偏微分方程可以用来描述各种各样的物理现象，如声音，热量，扩散，静电，电动力学，流体力学，弹性力学，重力和量子力学。这些看起来截然不同的物理现象却可以用类似的偏微分方程来描述。正如常微分方程经常对一维动力系统进行建模一样，偏微分方程经常对多维系统进行建模。随机偏微分方程是偏微分方程的一种推广。&lt;br /&gt;
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== Introduction ==&lt;br /&gt;
引言&lt;br /&gt;
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Partial differential equations (PDEs) are equations that involve rates of change with respect to [[continuous variables]]. For example, the position of a [[rigid body]] is specified by six parameters,&amp;lt;ref&amp;gt;{{Cite book|url=https://books.google.com/books?id=v9PLbcYd9aUC&amp;amp;pg=PA32|title=Modelling and Control of Robot Manipulators|last=Sciavicco|first=Lorenzo|last2=Siciliano|first2=Bruno|date=2001-02-19|publisher=Springer Science &amp;amp; Business Media|isbn=9781852332211|language=en}}&amp;lt;/ref&amp;gt; but the configuration of a [[fluid]] is given by the [[continuous distribution]] of several parameters, such as the [[temperature]], [[pressure]], and so forth. The dynamics for the rigid body take place in a finite-dimensional [[Configuration space (physics)|configuration space]]; the dynamics for the fluid occur in an infinite-dimensional configuration space. This distinction usually makes PDEs much harder to solve than ordinary differential equations (ODEs), but here again, there will be simple solutions for linear problems. Classic domains where PDEs are used include [[acoustics]], [[fluid dynamics]], [[electrodynamics]], and [[heat transfer]].&lt;br /&gt;
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Partial differential equations (PDEs) are equations that involve rates of change with respect to continuous variables. For example, the position of a rigid body is specified by six parameters, but the configuration of a fluid is given by the continuous distribution of several parameters, such as the temperature, pressure, and so forth. The dynamics for the rigid body take place in a finite-dimensional configuration space; the dynamics for the fluid occur in an infinite-dimensional configuration space. This distinction usually makes PDEs much harder to solve than ordinary differential equations (ODEs), but here again, there will be simple solutions for linear problems. Classic domains where PDEs are used include acoustics, fluid dynamics, electrodynamics, and heat transfer.&lt;br /&gt;
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偏微分方程(简称为PDEs)涉及到方程相对于连续变量的变化率。例如，刚体的位置是由六个参数确定的，而流体的状态是由几个参数的连续分布给出的，如温度、压力等。刚体的动力学过程发生在有限维状态空间中，流体的动力学过程发生在无限维状态空间中。这种区别通常使偏微分方程比常微分方程更难求解，但是线性问题仍然有简单的求解方式。使用偏微分方程的经典领域包括声学、流体力学、电动力学和传热学。&lt;br /&gt;
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A partial differential equation (PDE) for the function {{math|''u''(''x''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;,… ''x&amp;lt;sub&amp;gt;n&amp;lt;/sub&amp;gt;'')}} is an equation of the form&lt;br /&gt;
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A partial differential equation (PDE) for the function  is an equation of the form&lt;br /&gt;
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函数{{math|''u''(''x''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;,… ''x&amp;lt;sub&amp;gt;n&amp;lt;/sub&amp;gt;'')}}的偏微分方程形式是：&lt;br /&gt;
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: &amp;lt;math&amp;gt;f \left (x_1, \ldots x_n; u, \frac{\partial u}{\partial x_1}, \ldots \frac{\partial u}{\partial x_n}; \frac{\partial^2 u}{\partial x_1 \partial x_1}, \ldots \frac{\partial^2 u}{\partial x_1 \partial x_n}; \ldots \right) = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;f \left (x_1, \ldots x_n; u, \frac{\partial u}{\partial x_1}, \ldots \frac{\partial u}{\partial x_n}; \frac{\partial^2 u}{\partial x_1 \partial x_1}, \ldots \frac{\partial^2 u}{\partial x_1 \partial x_n}; \ldots \right) = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
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If {{mvar|f}} is a [[linear function]] of {{mvar|u}} and its derivatives, then the PDE is called linear. Common examples of linear PDEs include the [[heat equation]], the [[wave equation]], [[Laplace's equation]], [[Helmholtz equation]], [[Klein–Gordon equation]], and [[Poisson's equation]].&lt;br /&gt;
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If  is a linear function of  and its derivatives, then the PDE is called linear. Common examples of linear PDEs include the heat equation, the wave equation, Laplace's equation, Helmholtz equation, Klein–Gordon equation, and Poisson's equation.&lt;br /&gt;
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如果{{mvar|f}}是函数及其导数的线性函数，则偏微分方程称为线性函数。线性偏微分方程的常见例子包括热方程、波动方程、拉普拉斯方程、亥姆霍兹方程方程、克莱因-高登方程和泊松方程。&lt;br /&gt;
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A relatively simple PDE is&lt;br /&gt;
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A relatively simple PDE is&lt;br /&gt;
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一个相对简单的偏微分方程是：&lt;br /&gt;
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: &amp;lt;math&amp;gt;\frac{\partial u}{\partial x}(x,y) = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;\frac{\partial u}{\partial x}(x,y) = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
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This relation [[Logical implication|implies]] that the function {{math|''u''(''x'',''y'')}} is independent of {{mvar|x}}. However, the equation gives no information on the function's dependence on the variable {{mvar|y}}. Hence the general solution of this equation is&lt;br /&gt;
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This relation implies that the function  is independent of . However, the equation gives no information on the function's dependence on the variable . Hence the general solution of this equation is&lt;br /&gt;
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这个关系意味着函数是独立于{{mvar|x}}的。然而，这个方程没有给出关于函数和自变量的相关性的信息。因此，这个方程的通解是&lt;br /&gt;
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: &amp;lt;math&amp;gt;u(x,y) = f(y),&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;u(x,y) = f(y),&amp;lt;/math&amp;gt;&lt;br /&gt;
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where {{mvar|f}} is an arbitrary function of {{mvar|y}}. The analogous ordinary differential equation is&lt;br /&gt;
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where  is an arbitrary function of . The analogous ordinary differential equation is&lt;br /&gt;
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其中{{mvar|f}}是{{mvar|y}}的任意函数。类似的常微分方程是&lt;br /&gt;
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: &amp;lt;math&amp;gt;\frac{\mathrm{d} u}{\mathrm{d} x}(x) = 0,&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;\frac{\mathrm{d} u}{\mathrm{d} x}(x) = 0,&amp;lt;/math&amp;gt;&lt;br /&gt;
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which has the solution&lt;br /&gt;
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which has the solution&lt;br /&gt;
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它的解为&lt;br /&gt;
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: &amp;lt;math&amp;gt;u(x) = c,&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;u(x) = c,&amp;lt;/math&amp;gt;&lt;br /&gt;
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where {{mvar|c}} is any [[Constant (mathematics)|constant]] value. These two examples illustrate that general solutions of ordinary differential equations (ODEs) involve arbitrary constants, but solutions of PDEs involve arbitrary functions.&lt;br /&gt;
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where  is any constant value. These two examples illustrate that general solutions of ordinary differential equations (ODEs) involve arbitrary constants, but solutions of PDEs involve arbitrary functions.&lt;br /&gt;
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这里的{{mvar|c}}是常量。这两个例子说明常微分方程的一般解包含任意常数，但偏微分方程的解包含任意函数。&lt;br /&gt;
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A solution of a PDE is generally not [[Uniqueness quantification|unique]]; additional conditions must generally be specified on the [[Boundary (topology)|boundary]] of the region where the solution is defined. For instance, in the simple example above, the function {{math|''f''(''y'')}} can be determined if {{mvar|u}} is specified on the line {{math|''x'' {{=}} 0}}.&lt;br /&gt;
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A solution of a PDE is generally not unique; additional conditions must generally be specified on the boundary of the region where the solution is defined. For instance, in the simple example above, the function  can be determined if  is specified on the line  0}}.&lt;br /&gt;
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偏微分方程的解一般不是唯一的; 附加条件一般必须在定义解的区域边界上定义。例如，在上面的简单示例中，如果在{{math|''x'' {{=}} 0}}时确定了{{mvar|u}}的值，则可以确定该函数{{math|''f''(''y'')}}。&lt;br /&gt;
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== Existence and uniqueness ==&lt;br /&gt;
存在性和唯一性&lt;br /&gt;
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Although the issue of existence and uniqueness of solutions of ordinary differential equations has a very satisfactory answer with the [[Picard–Lindelöf theorem]], that is far from the case for partial differential equations. The [[Cauchy–Kowalevski theorem]] states that the [[Cauchy problem]] for any partial differential equation whose coefficients are [[Analytic function|analytic]] in the unknown function and its derivatives, has a locally unique analytic solution. Although this result might appear to settle the existence and uniqueness of solutions, there are examples of linear partial differential equations whose coefficients have derivatives of all orders (which are nevertheless not analytic) but which have no solutions at all: see [[Lewy's example|Lewy (1957)]]. Even if the solution of a partial differential equation exists and is unique, it may nevertheless have undesirable properties.  The mathematical study of these questions is usually in the more powerful context of [[weak solution]]s.&lt;br /&gt;
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Although the issue of existence and uniqueness of solutions of ordinary differential equations has a very satisfactory answer with the Picard–Lindelöf theorem, that is far from the case for partial differential equations. The Cauchy–Kowalevski theorem states that the Cauchy problem for any partial differential equation whose coefficients are analytic in the unknown function and its derivatives, has a locally unique analytic solution. Although this result might appear to settle the existence and uniqueness of solutions, there are examples of linear partial differential equations whose coefficients have derivatives of all orders (which are nevertheless not analytic) but which have no solutions at all: see Lewy (1957). Even if the solution of a partial differential equation exists and is unique, it may nevertheless have undesirable properties.  The mathematical study of these questions is usually in the more powerful context of weak solutions.&lt;br /&gt;
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虽然常微分方程解的存在唯一性问题用'''&amp;lt;font color=&amp;quot;#ff8000&amp;quot;&amp;gt;弗罗贝尼乌斯定理 Picard–Lindelöf Theorem&amp;lt;/font&amp;gt;得到了令人满意的结果，但应用到偏微分方程上却不尽如意。'''&amp;lt;font color=&amp;quot;#ff8000&amp;quot;&amp;gt;柯西-科瓦列夫斯基定理 Cauchy–Kowalevski theorem&amp;lt;/font&amp;gt;指出，对于任何在未知函数及其导数中系数是解析的偏微分方程，柯西问题有一个局部唯一的解析解。虽然这个结果似乎解决了解的存在性和唯一性问题，但是有一些线性偏微分方程的系数具有所有级数的导数(尽管这些导数不是解析的) ，但是根本没有解: 见 Lewy (1957)。即使偏微分方程的解存在且唯一，它仍然可能具有人们所不希望的性质。这些问题的数学研究通常是在更有力的弱解的背景下进行的。&lt;br /&gt;
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An example of pathological behavior is the sequence (depending upon {{mvar|n}}) of [[Cauchy problem]]s for the [[Laplace equation]]&lt;br /&gt;
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An example of pathological behavior is the sequence (depending upon ) of Cauchy problems for the Laplace equation&lt;br /&gt;
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反常特征的一个例子是拉普拉斯方程的柯西问题的序列(取决于{{mvar|n}})&lt;br /&gt;
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: &amp;lt;math&amp;gt;\frac{\partial^2 u}{\partial x^2} + \frac{\partial^2 u}{\partial y^2}=0,&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;\frac{\partial^2 u}{\partial x^2} + \frac{\partial^2 u}{\partial y^2}=0,&amp;lt;/math&amp;gt;&lt;br /&gt;
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with [[boundary condition]]s&lt;br /&gt;
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with boundary conditions&lt;br /&gt;
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有边界条件&lt;br /&gt;
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: &amp;lt;math&amp;gt;\begin{align} u(x,0) &amp;amp;= 0, \\ \frac{\partial u}{\partial y}(x,0) &amp;amp;= \frac{\sin nx}{n}, \end{align}&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;\begin{align} u(x,0) &amp;amp;= 0, \\ \frac{\partial u}{\partial y}(x,0) &amp;amp;= \frac{\sin nx}{n}, \end{align}&amp;lt;/math&amp;gt;&lt;br /&gt;
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where {{mvar|n}} is an integer. The derivative of {{mvar|u}} with respect to {{mvar|y}} approaches zero [[uniform convergence|uniformly]] in {{mvar|x}} as {{mvar|n}} increases, but the solution is&lt;br /&gt;
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where  is an integer. The derivative of  with respect to  approaches zero uniformly in  as  increases, but the solution is&lt;br /&gt;
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其中{{mvar|n}}是整数。{{mvar|u}}是关于{{mvar|y}}的导数，一致地随着{{mvar|n}}的增加而趋于零，但是解是&lt;br /&gt;
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: &amp;lt;math&amp;gt;u(x,y) = \frac{\sinh ny \sin nx}{n^2}.&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;u(x,y) = \frac{\sinh ny \sin nx}{n^2}.&amp;lt;/math&amp;gt;&lt;br /&gt;
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This solution approaches infinity if {{mvar|nx}} is not an integer multiple of {{pi}} for any non-zero value of {{mvar|y}}. The Cauchy problem for the Laplace equation is called ''ill-posed'' or ''not [[Well-posed problem|well-posed]]'', since the solution does not continuously depend on the data of the problem. Such ill-posed problems are not usually satisfactory for physical applications.&lt;br /&gt;
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This solution approaches infinity if  is not an integer multiple of  for any non-zero value of . The Cauchy problem for the Laplace equation is called ill-posed or not well-posed, since the solution does not continuously depend on the data of the problem. Such ill-posed problems are not usually satisfactory for physical applications.&lt;br /&gt;
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对于任何非零的{{mvar|y}}，如果{{mvar|nx}}不是{{pi}}的整数倍，这个解会接近于无穷大。拉普拉斯方程的柯西问题被称为不适定问题（可以译为ill-posed或not well-posed），因为该问题的解并不连续地依赖于该问题的数据。这种不适定问题在物理应用中通常不能令人满意。&lt;br /&gt;
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The [[Navier–Stokes existence and smoothness|existence of solutions for the Navier–Stokes equations]], a partial differential equation, is part of one of the [[Millennium Prize Problems]].&lt;br /&gt;
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The existence of solutions for the Navier–Stokes equations, a partial differential equation, is part of one of the Millennium Prize Problems.&lt;br /&gt;
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一种偏微分方程——纳维-斯托克斯方程——的解的存在性就是千禧年大奖难题的一部分。&lt;br /&gt;
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== Notation ==&lt;br /&gt;
符号&lt;br /&gt;
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In PDEs, it is common to denote partial derivatives using subscripts. That is:&lt;br /&gt;
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In PDEs, it is common to denote partial derivatives using subscripts. That is:&lt;br /&gt;
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在偏微分方程中，通常用下标表示偏导数。例如:&lt;br /&gt;
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: &amp;lt;math&amp;gt;u_x = \frac{\partial u}{\partial x}&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;u_x = \frac{\partial u}{\partial x}&amp;lt;/math&amp;gt;&lt;br /&gt;
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: &amp;lt;math&amp;gt;u_{xx} = \frac{\partial^2 u}{\partial x^2} &amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;u_{xx} = \frac{\partial^2 u}{\partial x^2} &amp;lt;/math&amp;gt;&lt;br /&gt;
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: &amp;lt;math&amp;gt;u_{xy} = \frac{\partial^2 u}{\partial y\, \partial x} = \frac{\partial}{\partial y } \left(\frac{\partial u}{\partial x}\right). &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;u_{xy} = \frac{\partial^2 u}{\partial y\, \partial x} = \frac{\partial}{\partial y } \left(\frac{\partial u}{\partial x}\right). &amp;lt;/math&amp;gt;&lt;br /&gt;
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Especially in physics, [[del]] or nabla ({{math|∇}}) is often used to denote spatial derivatives, and {{math|''&amp;amp;#x307;u'', ''ü''}} for time derivatives. For example, the [[wave equation]] (mentioned below) can be written as&lt;br /&gt;
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Especially in physics, del or nabla () is often used to denote spatial derivatives, and  for time derivatives. For example, the wave equation (mentioned below) can be written as&lt;br /&gt;
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特别是在物理学中，[[del]]或nabla ({{math|∇}})经常用来表示空间导数和时间导数。例如，波动方程(在下文中提到)可以写成&lt;br /&gt;
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:&amp;lt;math&amp;gt;\ddot u=c^2\nabla^2u&amp;lt;/math&amp;gt;&lt;br /&gt;
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&amp;lt;math&amp;gt;\ddot u=c^2\nabla^2u&amp;lt;/math&amp;gt;&lt;br /&gt;
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or&lt;br /&gt;
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or&lt;br /&gt;
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或&lt;br /&gt;
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:&amp;lt;math&amp;gt;\ddot u=c^2\Delta u&amp;lt;/math&amp;gt;&lt;br /&gt;
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&amp;lt;math&amp;gt;\ddot u=c^2\Delta u&amp;lt;/math&amp;gt;&lt;br /&gt;
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where {{math|Δ}} is the [[Laplace operator]].&lt;br /&gt;
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where  is the Laplace operator.&lt;br /&gt;
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其中{{math|Δ}}代表拉普拉斯算子&lt;br /&gt;
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== Classification ==&lt;br /&gt;
分类&lt;br /&gt;
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Some linear, second-order partial differential equations can be classified as [[parabolic partial differential equation|parabolic]], [[hyperbolic partial differential equation|hyperbolic]] and [[elliptic partial differential equation|elliptic]]. Others, such as the [[Euler–Tricomi equation]], have different types in different regions. The classification provides a guide to appropriate initial and boundary conditions and to the smoothness of the solutions.&lt;br /&gt;
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Some linear, second-order partial differential equations can be classified as parabolic, hyperbolic and elliptic. Others, such as the Euler–Tricomi equation, have different types in different regions. The classification provides a guide to appropriate initial and boundary conditions and to the smoothness of the solutions.&lt;br /&gt;
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一些线性二阶偏微分方程可分为抛物型方程、双曲型方程和椭圆型方程。其他的方程，如欧拉-特里科米方程，在不同的区域有不同的类型。这种分类有助于选择适当的初始和边界条件以及提高解的平滑性。&lt;br /&gt;
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=== Equations of first order ===&lt;br /&gt;
一阶方程&lt;br /&gt;
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{{main|First-order partial differential equation}}&lt;br /&gt;
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=== Linear equations of second order ===&lt;br /&gt;
二阶线性方程&lt;br /&gt;
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Assuming {{math|''u&amp;lt;sub&amp;gt;xy&amp;lt;/sub&amp;gt;'' {{=}} ''u&amp;lt;sub&amp;gt;yx&amp;lt;/sub&amp;gt;''}}, the general linear second-order PDE in two independent variables has the form&lt;br /&gt;
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Assuming  u&amp;lt;sub&amp;gt;yx&amp;lt;/sub&amp;gt;}}, the general linear second-order PDE in two independent variables has the form&lt;br /&gt;
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假设 {{math|''u&amp;lt;sub&amp;gt;xy&amp;lt;/sub&amp;gt;'' {{=}} ''u&amp;lt;sub&amp;gt;yx&amp;lt;/sub&amp;gt;''}}，含有两个独立变量的一般的线性二阶偏微分方程具有如下这样的形式&lt;br /&gt;
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: &amp;lt;math&amp;gt;Au_{xx} + 2Bu_{xy} + Cu_{yy} + \cdots \mbox{(lower order terms)} = 0,&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;Au_{xx} + 2Bu_{xy} + Cu_{yy} + \cdots \mbox{(lower order terms)} = 0,&amp;lt;/math&amp;gt;&lt;br /&gt;
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where the coefficients {{mvar|A}}, {{mvar|B}}, {{mvar|C}}... may depend upon {{mvar|x}} and {{mvar|y}}. If {{math|''A''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; + ''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; + ''C''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; &amp;gt; 0}} over a region of the {{mvar|xy}}-plane, the PDE is second-order in that region. This form is analogous to the equation for a conic section:&lt;br /&gt;
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where the coefficients , , ... may depend upon  and . If  over a region of the -plane, the PDE is second-order in that region. This form is analogous to the equation for a conic section:&lt;br /&gt;
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其中的系数 {{mvar|A}}, {{mvar|B}}, {{mvar|C}}... 一般取决于{{mvar|x}}和{{mvar|y}}。如果在{{mvar|xy}}-平面的一个区域上 {{math|''A''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; + ''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; + ''C''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; &amp;gt; 0}}，偏微分方程在该区域是二阶的。这种形式类似于圆锥曲线的方程:&lt;br /&gt;
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: &amp;lt;math&amp;gt;Ax^2 + 2Bxy + Cy^2 + \cdots = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;Ax^2 + 2Bxy + Cy^2 + \cdots = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
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More precisely, replacing {{math|∂&amp;lt;sub&amp;gt;''x''&amp;lt;/sub&amp;gt;}} by {{mvar|X}}, and likewise for other variables (formally this is done by a [[Fourier transform]]), converts a constant-coefficient PDE into a polynomial of the same degree, with the terms of the highest degree (a [[homogeneous polynomial]], here a [[quadratic form]]) being most significant for the classification.&lt;br /&gt;
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More precisely, replacing  by , and likewise for other variables (formally this is done by a Fourier transform), converts a constant-coefficient PDE into a polynomial of the same degree, with the terms of the highest degree (a homogeneous polynomial, here a quadratic form) being most significant for the classification.&lt;br /&gt;
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更准确地说，用 {{mvar|X}} 替换 {{math|∂&amp;lt;sub&amp;gt;''x''&amp;lt;/sub&amp;gt;}}，对于其他变量做同样的操作(从形式上来说，这是由傅里叶变换来完成的)，将一个常系数偏微分方程转换成一个相同次数的多项式，最高次数的项(齐次多项式，这里是一个二次形式)一般会用于偏微分方程的分类。&lt;br /&gt;
===~~ most significant for the classification 意译为用于偏微分方程的分类。       significiant直译过来感觉不太合适&lt;br /&gt;
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Just as one classifies [[conic section]]s and quadratic forms into parabolic, hyperbolic, and elliptic based on the [[discriminant]] {{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − 4''AC''}}, the same can be done for a second-order PDE at a given point.  However, the [[discriminant]] in a PDE is given by {{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC''}} due to the convention of the {{mvar|xy}} term being {{math|2''B''}} rather than {{mvar|B}}; formally, the discriminant (of the associated quadratic form) is {{math|(2''B'')&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − 4''AC'' {{=}} 4(''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC'')}}, with the factor of 4 dropped for simplicity.&lt;br /&gt;
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Just as one classifies conic sections and quadratic forms into parabolic, hyperbolic, and elliptic based on the discriminant , the same can be done for a second-order PDE at a given point.  However, the discriminant in a PDE is given by  due to the convention of the  term being  rather than ; formally, the discriminant (of the associated quadratic form) is  4(B&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − AC)}}, with the factor of 4 dropped for simplicity.&lt;br /&gt;
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正如人们可以根据判别式 {{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − 4''AC''}} 将圆锥曲线和二次型分为抛物型、双曲型和椭圆型一样，对于给定点的二阶偏微分方程也可以这样做。然而，偏微分方程中的判别式 {{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − 4''AC''}} 是根据交叉项的系数{{math|2''B''}} 而不是 {{mvar|B}} 给出的，形式上，判别式(关联二次型)是 {{math|(2''B'')&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − 4''AC'' {{=}} 4(''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC'')}}，为简单起见，去掉了因子4。&lt;br /&gt;
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# {{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC'' &amp;lt; 0}} (''[[elliptic partial differential equation]]''): Solutions of [[elliptic partial differential equation|elliptic PDEs]] are as smooth as the coefficients allow, within the interior of the region where the equation and solutions are defined. For example, solutions of [[Laplace's equation]] are analytic within the domain where they are defined, but solutions may assume boundary values that are not smooth. The motion of a fluid at subsonic speeds can be approximated with elliptic PDEs, and the Euler–Tricomi equation is elliptic where {{math|''x'' &amp;lt; 0}}.&lt;br /&gt;
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  (elliptic partial differential equation): Solutions of elliptic PDEs are as smooth as the coefficients allow, within the interior of the region where the equation and solutions are defined. For example, solutions of Laplace's equation are analytic within the domain where they are defined, but solutions may assume boundary values that are not smooth. The motion of a fluid at subsonic speeds can be approximated with elliptic PDEs, and the Euler–Tricomi equation is elliptic where .&lt;br /&gt;
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{{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC'' &amp;lt; 0}} (椭圆形微分方程)：在定义方程和解的区域内部，椭圆型偏微分方程的解光滑到系数允许的程度。例如，拉普拉斯方程的解在它们被定义的区域内是解析的，但是解可能假设边界值是不光滑的。亚音速流体的运动可以用椭圆偏微分方程近似，其中欧拉-特里科米方程在 {{math|''x'' &amp;lt; 0}} 时是椭圆型偏微分方程。&lt;br /&gt;
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# {{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC'' {{=}} 0}} (''[[parabolic partial differential equation]]''): Equations that are [[parabolic partial differential equation|parabolic]] at every point can be transformed into a form analogous to the [[heat equation]] by a change of independent variables. Solutions smooth out as the transformed time variable increases. The Euler–Tricomi equation has parabolic type on the line where {{math|''x'' {{=}} 0}}.&lt;br /&gt;
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  0}} (parabolic partial differential equation): Equations that are parabolic at every point can be transformed into a form analogous to the heat equation by a change of independent variables. Solutions smooth out as the transformed time variable increases. The Euler–Tricomi equation has parabolic type on the line where  0}}.&lt;br /&gt;
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{{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC'' {{=}} 0}}（抛物线形偏微分方程）：在每一点上都是抛物线型的方程可以通过改变自变量从而转化成类似于热方程的形式。随着转换后的时间变量的增加，方程的解变得平滑。欧拉-特里科米方程在 {{math|''x'' {{=}} 0}} 这条特征线上是抛物线形的。&lt;br /&gt;
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# {{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC'' &amp;gt; 0}} (''[[hyperbolic partial differential equation]]''): [[hyperbolic partial differential equation|hyperbolic]] equations retain any discontinuities of functions or derivatives in the initial data. An example is the [[wave equation]]. The motion of a fluid at supersonic speeds can be approximated with hyperbolic PDEs, and the Euler–Tricomi equation is hyperbolic where {{math|''x'' &amp;gt; 0}}.&lt;br /&gt;
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  (hyperbolic partial differential equation): hyperbolic equations retain any discontinuities of functions or derivatives in the initial data. An example is the wave equation. The motion of a fluid at supersonic speeds can be approximated with hyperbolic PDEs, and the Euler–Tricomi equation is hyperbolic where .&lt;br /&gt;
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{{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC'' &amp;gt; 0}} (双曲形偏微分方程)：双曲形方程在初始数据中保留了函数或导数的任何不连续性，波动方程就是其中的一个例子。超音速流体的运动可以用双曲形偏微分方程近似，其中欧拉-特里科米方程在 {{math|''x'' &amp;gt; 0}} 时是双曲型的。&lt;br /&gt;
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If there are {{mvar|n}} independent variables {{math|''x''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;, ''x''&amp;lt;sub&amp;gt;2 &amp;lt;/sub&amp;gt;,… ''x''&amp;lt;sub&amp;gt;''n''&amp;lt;/sub&amp;gt;}}, a general linear partial differential equation of second order has the form&lt;br /&gt;
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If there are  independent variables , a general linear partial differential equation of second order has the form&lt;br /&gt;
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如果存在 {{mvar|n}} 个自变量 {{math|''x''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;, ''x''&amp;lt;sub&amp;gt;2 &amp;lt;/sub&amp;gt;,… ''x''&amp;lt;sub&amp;gt;''n''&amp;lt;/sub&amp;gt;}}，一般二阶线性偏微分方程的形式是&lt;br /&gt;
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: &amp;lt;math&amp;gt;L u =\sum_{i=1}^n\sum_{j=1}^n a_{i,j} \frac{\partial^2 u}{\partial x_i \partial x_j} \quad \text{ plus lower-order terms} =0.&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;L u =\sum_{i=1}^n\sum_{j=1}^n a_{i,j} \frac{\partial^2 u}{\partial x_i \partial x_j} \quad \text{ plus lower-order terms} =0.&amp;lt;/math&amp;gt;&lt;br /&gt;
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The classification depends upon the signature of the eigenvalues of the coefficient matrix {{math|''a''&amp;lt;sub&amp;gt;''i'',''j''&amp;lt;/sub&amp;gt;}}.&lt;br /&gt;
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The classification depends upon the signature of the eigenvalues of the coefficient matrix .&lt;br /&gt;
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这种分类取决于系数矩阵本征值的符号（正负性）。&lt;br /&gt;
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# Elliptic: the eigenvalues are all positive or all negative.&lt;br /&gt;
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 Elliptic: the eigenvalues are all positive or all negative.&lt;br /&gt;
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椭圆形方程: 本征值全部为正或全部为负。&lt;br /&gt;
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# Parabolic: the eigenvalues are all positive or all negative, save one that is zero.&lt;br /&gt;
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 Parabolic: the eigenvalues are all positive or all negative, save one that is zero.&lt;br /&gt;
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抛物线形方程: 本征值全部为正或全部为负，除了一个为零。&lt;br /&gt;
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# Hyperbolic: there is only one negative eigenvalue and all the rest are positive, or there is only one positive eigenvalue and all the rest are negative.&lt;br /&gt;
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 Hyperbolic: there is only one negative eigenvalue and all the rest are positive, or there is only one positive eigenvalue and all the rest are negative.&lt;br /&gt;
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双曲形方程: 只有一个负特征值，其余的都是正特征值，或者只有一个正特征值，其余的都是负特征值。&lt;br /&gt;
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# Ultrahyperbolic: there is more than one positive eigenvalue and more than one negative eigenvalue, and there are no zero eigenvalues. There is only a limited theory for ultrahyperbolic equations (Courant and Hilbert, 1962).&lt;br /&gt;
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 Ultrahyperbolic: there is more than one positive eigenvalue and more than one negative eigenvalue, and there are no zero eigenvalues. There is only a limited theory for ultrahyperbolic equations (Courant and Hilbert, 1962).&lt;br /&gt;
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超双形方程: 存在多于一个正本征值和多于一个的负本征值，且不存在零本征值。对于超双曲方程，只存在一个有限理论(Courant 和 Hilbert，1962)。&lt;br /&gt;
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==[[用户:Yuling|Yuling]]（[[用户讨论:Yuling|讨论]]） 我对于limited theory这个单词对应的相关理论不太了解。&lt;br /&gt;
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=== Systems of first-order equations and characteristic surfaces ===&lt;br /&gt;
一阶方程组和特征曲面&lt;br /&gt;
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The classification of partial differential equations can be extended to systems of first-order equations, where the unknown {{mvar|u}} is now a [[Euclidean vector|vector]] with {{mvar|m}} components, and the coefficient matrices {{mvar|A&amp;lt;sub&amp;gt;ν&amp;lt;/sub&amp;gt;}} are {{mvar|m}} by {{mvar|m}} matrices for {{math|''ν'' {{=}} 1, 2,… ''n''}}. The partial differential equation takes the form&lt;br /&gt;
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The classification of partial differential equations can be extended to systems of first-order equations, where the unknown  is now a vector with  components, and the coefficient matrices  are  by  matrices for  1, 2,… n}}. The partial differential equation takes the form&lt;br /&gt;
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偏微分方程组的分类可以推广到一阶方程组，其中未知量 {{mvar|u}} 是有 {{mvar|m}} 个分量的向量。对于 {{math|''ν'' {{=}} 1, 2,… ''n''}}，系数矩阵 {{mvar|A&amp;lt;sub&amp;gt;ν&amp;lt;/sub&amp;gt;}} 是 {{mvar|m}} × {{mvar|m}} 的矩阵。偏微分方程形式如下：&lt;br /&gt;
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: &amp;lt;math&amp;gt;Lu = \sum_{\nu=1}^{n} A_\nu \frac{\partial u}{\partial x_\nu} + B=0,&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;Lu = \sum_{\nu=1}^{n} A_\nu \frac{\partial u}{\partial x_\nu} + B=0,&amp;lt;/math&amp;gt;&lt;br /&gt;
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where the coefficient matrices {{mvar|A&amp;lt;sub&amp;gt;ν&amp;lt;/sub&amp;gt;}} and the vector {{mvar|B}} may depend upon {{mvar|x}} and {{mvar|u}}. If a [[hypersurface]] {{mvar|S}} is given in the implicit form&lt;br /&gt;
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where the coefficient matrices  and the vector  may depend upon  and . If a hypersurface  is given in the implicit form&lt;br /&gt;
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其中系数矩阵 {{mvar|A&amp;lt;sub&amp;gt;ν&amp;lt;/sub&amp;gt;}} 和向量 {{mvar|B}} 可能依赖于 {{mvar|x}} 和 {{mvar|u}}。如果超曲面是以隐式形式给出的&lt;br /&gt;
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: &amp;lt;math&amp;gt;\varphi(x_1, x_2, \ldots x_n)=0,&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;\varphi(x_1, x_2, \ldots x_n)=0,&amp;lt;/math&amp;gt;&lt;br /&gt;
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where {{mvar|φ}} has a non-zero gradient, then {{mvar|S}} is a '''characteristic surface''' for the operator {{mvar|L}} at a given point if the characteristic form vanishes:&lt;br /&gt;
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where  has a non-zero gradient, then  is a characteristic surface for the operator  at a given point if the characteristic form vanishes:&lt;br /&gt;
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其中存在一个非零的梯度，那么如果特征形式消失，则在给定点上算子的特征曲面形式如下:&lt;br /&gt;
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: &amp;lt;math&amp;gt;Q\left(\frac{\partial\varphi}{\partial x_1}, \ldots\frac{\partial\varphi}{\partial x_n}\right) =\det\left[\sum_{\nu=1}^nA_\nu \frac{\partial \varphi}{\partial x_\nu}\right]=0.\,&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;Q\left(\frac{\partial\varphi}{\partial x_1}, \ldots\frac{\partial\varphi}{\partial x_n}\right) =\det\left[\sum_{\nu=1}^nA_\nu \frac{\partial \varphi}{\partial x_\nu}\right]=0.\,&amp;lt;/math&amp;gt;&lt;br /&gt;
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The geometric interpretation of this condition is as follows: if data for {{mvar|u}} are prescribed on the surface {{mvar|S}}, then it may be possible to determine the normal derivative of {{mvar|u}} on {{mvar|S}} from the differential equation. If the data on {{mvar|S}} and the differential equation determine the normal derivative of {{mvar|u}} on {{mvar|S}}, then {{mvar|S}} is non-characteristic. If the data on {{mvar|S}} and the differential equation ''do not'' determine the normal derivative of {{mvar|u}} on {{mvar|S}}, then the surface is '''characteristic''', and the differential equation restricts the data on {{mvar|S}}: the differential equation is ''internal'' to {{mvar|S}}.&lt;br /&gt;
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The geometric interpretation of this condition is as follows: if data for  are prescribed on the surface , then it may be possible to determine the normal derivative of  on  from the differential equation. If the data on  and the differential equation determine the normal derivative of  on , then  is non-characteristic. If the data on  and the differential equation do not determine the normal derivative of  on , then the surface is characteristic, and the differential equation restricts the data on : the differential equation is internal to .&lt;br /&gt;
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这个条件的几何解释如下: 如果关于 {{mvar|u}} 的数据是在曲面 {{mvar|S}} 上规定的，那么就有可能依据微分方程确定曲面 {{mvar|S}} 上 {{mvar|u}} 的法向导数。如果曲面 {{mvar|S}} 上的数据和上面的微分方程能确定曲面 {{mvar|S}} 上 {{mvar|u}} 的法向导数，那么它就是非特征的。如果曲面 {{mvar|S}} 上的数据和上面的微分方程不能确定曲面 {{mvar|S}} 上 {{mvar|u}} 的法向导数，那么曲面是特征的，并且微分方程将数据限制在曲面 {{mvar|S}} 上：微分方程是在曲面 {{mvar|S}} 内部。&lt;br /&gt;
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# A first-order system {{math|''Lu'' {{=}} 0}} is ''elliptic'' if no surface is characteristic for {{mvar|L}}: the values of {{mvar|u}} on {{mvar|S}} and the differential equation always determine the normal derivative of {{mvar|u}} on {{mvar|S}}.&lt;br /&gt;
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 A first-order system  0}} is elliptic if no surface is characteristic for : the values of  on  and the differential equation always determine the normal derivative of  on .&lt;br /&gt;
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如果对于 {{mvar|L}} 没有曲面是特征的，则一阶系统 {{math|''Lu'' {{=}} 0}} 是椭圆形的：{{mvar|u}}在 {{mvar|S}} 的值和微分方程总能够决定 {{mvar|S}} 上 {{mvar|u}} 的法向导数。&lt;br /&gt;
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# A first-order system is ''hyperbolic'' at a point if there is a '''spacelike''' surface {{mvar|S}} with normal {{mvar|ξ}} at that point. This means that, given any non-trivial vector {{mvar|η}} orthogonal to {{mvar|ξ}}, and a scalar multiplier {{mvar|λ}}, the equation {{math|''Q''(''λξ'' + ''η'') {{=}} 0}} has {{mvar|m}} real roots {{math|''λ''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;, ''λ''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;,… ''λ''&amp;lt;sub&amp;gt;''m''&amp;lt;/sub&amp;gt;}}. The system is '''strictly hyperbolic''' if these roots are always distinct. The geometrical interpretation of this condition is as follows: the characteristic form {{math|''Q''(''ζ'') {{=}} 0}} defines a cone (the normal cone) with homogeneous coordinates ζ. In the hyperbolic case, this cone has {{mvar|m}} sheets, and the axis {{math|''ζ'' {{=}} ''λξ''}} runs inside these sheets: it does not intersect any of them. But when displaced from the origin by η, this axis intersects every sheet. In the elliptic case, the normal cone has no real sheets.&lt;br /&gt;
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 A first-order system is hyperbolic at a point if there is a spacelike surface  with normal  at that point. This means that, given any non-trivial vector  orthogonal to , and a scalar multiplier , the equation  0}} has  real roots . The system is strictly hyperbolic if these roots are always distinct. The geometrical interpretation of this condition is as follows: the characteristic form  0}} defines a cone (the normal cone) with homogeneous coordinates ζ. In the hyperbolic case, this cone has  sheets, and the axis  λξ}} runs inside these sheets: it does not intersect any of them. But when displaced from the origin by η, this axis intersects every sheet. In the elliptic case, the normal cone has no real sheets.&lt;br /&gt;
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如果在该点存在一个法向量为 {{mvar|ξ}}的 '''&amp;lt;font color=&amp;quot;#ff8000&amp;quot;&amp;gt;类空曲面 Spacclike Surface&amp;lt;/font&amp;gt; {{mvar|S}} ，则一阶系统在那一点是双曲的。这意味着，给定任意正交于 {{mvar|ξ}} 的非平凡向量 {{mvar|η}} 和一个标量乘子 {{mvar|λ}}，方程 {{math|''Q''(''λξ'' + ''η'') {{=}} 0}} 有 {{mvar|m}} 个实根 {{math|''λ''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;, ''λ''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;,… ''λ''&amp;lt;sub&amp;gt;''m''&amp;lt;/sub&amp;gt;}}。如果这些根始终不同，则该系统是严格双曲形的。这个条件的几何解释如下: 特征形式 {{math|''Q''(''ζ'') {{=}} 0}} 定义了一个具有齐次坐标 ζ的圆锥(法线圆锥)。在双曲形的情况下，这个圆锥体有 {{mvar|m}} 层，并且轴 {{math|''ζ'' {{=}} ''λξ''}} 在这些层中运动: 它不与任何一层相交。但是当从原点偏离η时，这条轴线与每一层都相交。在椭圆形的情况下，法向圆锥没有实层。&lt;br /&gt;
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==[[用户:Yuling|Yuling]]（[[用户讨论:Yuling|讨论]]） sheet 这个单词也不很理解，我直译为了“层”&lt;br /&gt;
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=== Equations of mixed type ===&lt;br /&gt;
混合型方程&lt;br /&gt;
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If a PDE has coefficients that are not constant, it is possible that it will not belong to any of these categories but rather be of '''mixed type'''. A simple but important example is the [[Euler–Tricomi equation]]&lt;br /&gt;
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If a PDE has coefficients that are not constant, it is possible that it will not belong to any of these categories but rather be of mixed type. A simple but important example is the Euler–Tricomi equation&lt;br /&gt;
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如果偏微分方程的系数不是常数，那么它可能不属于这些类别中的任何一个，而是属于混合类型。一个简单但重要的例子是欧拉-特里科米方程&lt;br /&gt;
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: &amp;lt;math&amp;gt;u_{xx} = xu_{yy},&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;u_{xx} = xu_{yy},&amp;lt;/math&amp;gt;&lt;br /&gt;
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which is called '''elliptic-hyperbolic''' because it is elliptic in the region {{math|''x'' &amp;lt; 0}}, hyperbolic in the region {{math|''x'' &amp;gt; 0}}, and degenerate parabolic on the line {{math|''x'' {{=}} 0}}.&lt;br /&gt;
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which is called elliptic-hyperbolic because it is elliptic in the region , hyperbolic in the region , and degenerate parabolic on the line  0}}.&lt;br /&gt;
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它在 {{math|''x'' &amp;lt; 0}} 的区域上是椭圆形，在 {{math|''x'' &amp;gt; 0}} 区域上是双曲形，在 {{math|''x'' {{=}} 0}}这条线上是退化为抛物线形，因此称之为椭圆-双曲型。&lt;br /&gt;
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''fill in: Dirichlet and Neumann boundaries, hyperbolic/parabolic/elliptic separation of variables, [[Fourier analysis]], [[Green's function]]s ...--&amp;gt;&lt;br /&gt;
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fill in: Dirichlet and Neumann boundaries, hyperbolic/parabolic/elliptic separation of variables, Fourier analysis, Green's functions ...--&amp;gt;&lt;br /&gt;
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填写: Dirichlet 和 Neumann 边界，双曲 / 抛物线 / 椭圆分离变量法，傅立叶分析，Green 函数... --&lt;br /&gt;
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=== Infinite-order PDEs in quantum mechanics ===&lt;br /&gt;
量子力学中的无限阶偏微分方程&lt;br /&gt;
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In the [[phase space formulation]] of quantum mechanics,  one may consider the [[Method of quantum characteristics|quantum Hamilton's equations]] for trajectories of quantum particles. These equations are infinite-order PDEs. However, in the semiclassical expansion, one has a finite system of ODEs at any fixed order of [[Dirac constant|{{mvar|ħ}}]].  The evolution equation of the [[Wigner quasi-probability distribution|c]] is also an infinite-order PDE. The quantum trajectories are [[Method of quantum characteristics|quantum characteristics]], with the use of which one could calculate the evolution of the Wigner function.&lt;br /&gt;
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In the phase space formulation of quantum mechanics,  one may consider the quantum Hamilton's equations for trajectories of quantum particles. These equations are infinite-order PDEs. However, in the semiclassical expansion, one has a finite system of ODEs at any fixed order of Dirac constant|.  The evolution equation of the Wigner function is also an infinite-order PDE. The quantum trajectories are quantum characteristics, with the use of which one could calculate the evolution of the Wigner function.&lt;br /&gt;
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在量子力学中的相空间表述中，我们可以考虑用于求解量子粒子的轨迹的量子哈密顿的方程。这些方程是无限阶偏微分方程。然而，在半经典展开中，我们在给定[[Dirac constant|{{mvar|ħ}}]]阶数下有一个有限的的常微分方程组。'''&amp;lt;font color=&amp;quot;#ff8000&amp;quot;&amp;gt;维格纳函数  Wigner Function&amp;lt;/font&amp;gt;的演化方程也是一个无限阶偏微分方程。由于量子轨道的量子特性，所以它通常可以用来计算维格纳函数的演化。&lt;br /&gt;
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== Analytical solutions ==&lt;br /&gt;
解析解&lt;br /&gt;
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===Separation of variables===&lt;br /&gt;
分离变量法&lt;br /&gt;
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{{main|Separable partial differential equation}}&lt;br /&gt;
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Linear PDEs can be reduced to systems of ordinary differential equations by the important technique of separation of variables. This technique rests on a characteristic of solutions to differential equations: if one can find any solution that solves the equation and satisfies the boundary conditions, then it is ''the'' solution (this also applies to ODEs). We assume as an [[ansatz]] that the dependence of a solution on the parameters space and time can be written as a product of terms that each depend on a single parameter, and then see if this can be made to solve the problem.&amp;lt;ref&amp;gt;{{cite book|last1=Gershenfeld|first1=Neil|title=The nature of mathematical modeling|date=2000|publisher=Cambridge Univ. Press|location=Cambridge|isbn=0521570956|page=27|edition=Reprinted (with corr.)}}&amp;lt;/ref&amp;gt;&lt;br /&gt;
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Linear PDEs can be reduced to systems of ordinary differential equations by the important technique of separation of variables. This technique rests on a characteristic of solutions to differential equations: if one can find any solution that solves the equation and satisfies the boundary conditions, then it is the solution (this also applies to ODEs). We assume as an ansatz that the dependence of a solution on the parameters space and time can be written as a product of terms that each depend on a single parameter, and then see if this can be made to solve the problem.&lt;br /&gt;
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线性偏微分方程组可以通过分离变量法这一重要方法来简化为常微分方程组。这种方法依赖于微分方程解的一个特征: 如果能找到任何一个满足方程和边界条件的解，那么这个解就是方程的解(这也适用于常微分方程)。我们假设解对参数空间和时间的依赖可以写成对它们每一项的依赖以及一个参数的乘积，然后再看看这是否可以用来解决这个问题。&lt;br /&gt;
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In the method of separation of variables, one reduces a PDE to a PDE in fewer variables, which is an ordinary differential equation if in one variable – these are in turn easier to solve.&lt;br /&gt;
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In the method of separation of variables, one reduces a PDE to a PDE in fewer variables, which is an ordinary differential equation if in one variable – these are in turn easier to solve.&lt;br /&gt;
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在分离变量法方法中，可以将偏微分方程简化为含有更少变量的偏微分方程，如果只有一个变量，那么就变成了一个'''&amp;lt;font color = &amp;quot;#ff8000&amp;quot;&amp;gt;常微分方程 Ordinary Differential Equation&amp;lt;/font&amp;gt;'''-- 反过来，这些方程也更容易求解。&lt;br /&gt;
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This is possible for simple PDEs, which are called [[separable partial differential equation]]s, and the domain is generally a rectangle (a product of intervals). Separable PDEs correspond to [[diagonal matrices]] – thinking of &amp;quot;the value for fixed {{mvar|x}}&amp;quot; as a coordinate, each coordinate can be understood separately.&lt;br /&gt;
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This is possible for simple PDEs, which are called separable partial differential equations, and the domain is generally a rectangle (a product of intervals). Separable PDEs correspond to diagonal matrices – thinking of &amp;quot;the value for fixed &amp;quot; as a coordinate, each coordinate can be understood separately.&lt;br /&gt;
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对于简单的偏微分方程(称为可分离偏微分方程)来说，这是可能的，而且方程通常定义在一个矩形区域(区间的乘积)上。可分离偏微分方程对应于对角线矩阵——以“固定值”为坐标，每个坐标可分开理解。&lt;br /&gt;
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This generalizes to the [[method of characteristics]], and is also used in [[integral transform]]s.&lt;br /&gt;
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This generalizes to the method of characteristics, and is also used in integral transforms.&lt;br /&gt;
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这种方法可以推广到特征曲线法，也可以用于积分变换。&lt;br /&gt;
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===Method of characteristics===&lt;br /&gt;
特征曲线法&lt;br /&gt;
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{{main|Method of characteristics}}&lt;br /&gt;
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In special cases, one can find characteristic curves on which the equation reduces to an ODE – changing coordinates in the domain to straighten these curves allows separation of variables, and is called the [[method of characteristics]].&lt;br /&gt;
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In special cases, one can find characteristic curves on which the equation reduces to an ODE – changing coordinates in the domain to straighten these curves allows separation of variables, and is called the method of characteristics.&lt;br /&gt;
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在特殊情况下，可以找到一些特征曲线，在这些曲线上方程可以变成一个常微分方程——意味着改变坐标从而使这些曲线变直从而达到分离变量的目的，这就是所谓的特征曲线法。&lt;br /&gt;
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More generally, one may find characteristic surfaces.&lt;br /&gt;
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More generally, one may find characteristic surfaces.&lt;br /&gt;
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更一般地说，人们可能会找到特征表面。&lt;br /&gt;
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===Integral transform===&lt;br /&gt;
积分变换&lt;br /&gt;
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An [[integral transform]] may transform the PDE to a simpler one, in particular, a separable PDE. This corresponds to diagonalizing an operator.&lt;br /&gt;
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An integral transform may transform the PDE to a simpler one, in particular, a separable PDE. This corresponds to diagonalizing an operator.&lt;br /&gt;
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积分变换可以将偏微分方程转换为更简单的偏微分方程，特别是可分离的偏微分方程。这对应于对角化算符。&lt;br /&gt;
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An important example of this is [[Fourier analysis]], which diagonalizes the heat equation using the [[eigenbasis]] of sinusoidal waves.&lt;br /&gt;
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An important example of this is Fourier analysis, which diagonalizes the heat equation using the eigenbasis of sinusoidal waves.&lt;br /&gt;
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这方面的一个重要例子是'''&amp;lt;font color = &amp;quot;#ff8000&amp;quot;&amp;gt;傅里叶分析  Fourier Analysis&amp;lt;/font&amp;gt;'''，它使用正弦波的特征基来对角化热方程。&lt;br /&gt;
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If the domain is finite or periodic, an infinite sum of solutions such as a [[Fourier series]] is appropriate, but an integral of solutions such as a [[Fourier integral]] is generally required for infinite domains. The solution for a point source for the heat equation given above is an example of the use of a Fourier integral.&lt;br /&gt;
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If the domain is finite or periodic, an infinite sum of solutions such as a Fourier series is appropriate, but an integral of solutions such as a Fourier integral is generally required for infinite domains. The solution for a point source for the heat equation given above is an example of the use of a Fourier integral.&lt;br /&gt;
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如果区域是有限的或周期性的，那么解为无限和的形式是恰当的，例如傅里叶级数，但是一个解的积分，例如傅立叶积分，一般是在无限区域上的。上面给出的热传导方程的点源解法就是使用傅里叶积分的一个例子。&lt;br /&gt;
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===Change of variables===&lt;br /&gt;
变量代换&lt;br /&gt;
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Often a PDE can be reduced to a simpler form with a known solution by a suitable [[Change of variables (PDE)|change of variables]].  For example, the [[Black–Scholes equation#Derivation|Black–Scholes]] PDE&lt;br /&gt;
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Often a PDE can be reduced to a simpler form with a known solution by a suitable change of variables.  For example, the Black–Scholes PDE&lt;br /&gt;
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偏微分方程通常可以通过变量的适当变化，用已知的解简化为更简单的形式。例如，布莱克-舒尔斯偏微分方程&lt;br /&gt;
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:&amp;lt;math&amp;gt; \frac{\partial V}{\partial t} + \tfrac{1}{2}\sigma^2 S^2\frac{\partial^2 V}{\partial S^2} + rS\frac{\partial V}{\partial S} - rV = 0 &amp;lt;/math&amp;gt;&lt;br /&gt;
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&amp;lt;math&amp;gt; \frac{\partial V}{\partial t} + \tfrac{1}{2}\sigma^2 S^2\frac{\partial^2 V}{\partial S^2} + rS\frac{\partial V}{\partial S} - rV = 0 &amp;lt;/math&amp;gt;&lt;br /&gt;
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is reducible to the [[heat equation]]&lt;br /&gt;
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is reducible to the heat equation&lt;br /&gt;
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可以简化为热传导方程&lt;br /&gt;
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:&amp;lt;math&amp;gt; \frac{\partial u}{\partial \tau} = \frac{\partial^2 u}{\partial x^2}&amp;lt;/math&amp;gt;&lt;br /&gt;
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&amp;lt;math&amp;gt; \frac{\partial u}{\partial \tau} = \frac{\partial^2 u}{\partial x^2}&amp;lt;/math&amp;gt;&lt;br /&gt;
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by the change of variables (for complete details see {{webarchive |url=https://web.archive.org/web/20080411030405/http://www.math.unl.edu/~sdunbar1/Teaching/MathematicalFinance/Lessons/BlackScholes/Solution/solution.shtml |date=April 11, 2008 |title=Solution of the Black Scholes Equation }})&lt;br /&gt;
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by the change of variables (for complete details see )&lt;br /&gt;
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通过变量替换(完整的细节见)&lt;br /&gt;
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:&amp;lt;math&amp;gt;\begin{align}&lt;br /&gt;
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V(S,t) &amp;amp;= K v(x,\tau),\\[5px]&lt;br /&gt;
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x &amp;amp;= \ln\left(\tfrac{S}{K} \right),\\[5px]&lt;br /&gt;
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\tau &amp;amp;= \tfrac{1}{2} \sigma^2 (T - t),\\[5px]&lt;br /&gt;
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v(x,\tau)&amp;amp;=e^{-\alpha x-\beta\tau} u(x,\tau).&lt;br /&gt;
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\end{align}&amp;lt;/math&amp;gt;&lt;br /&gt;
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===Fundamental solution===&lt;br /&gt;
基本解&lt;br /&gt;
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{{main|Fundamental solution}}&lt;br /&gt;
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Inhomogeneous equations can often be solved (for constant coefficient PDEs, always be solved) by finding the [[fundamental solution]] (the solution for a point source), then taking the [[convolution]] with the boundary conditions to get the solution.&lt;br /&gt;
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Inhomogeneous equations can often be solved (for constant coefficient PDEs, always be solved) by finding the fundamental solution (the solution for a point source), then taking the convolution with the boundary conditions to get the solution.&lt;br /&gt;
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非齐次方程(常系数偏微分方程)一般是通过先求出基本解(点源的解) ，然后利用带边界条件的卷积来求解。&lt;br /&gt;
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This is analogous in [[signal processing]] to understanding a filter by its [[impulse response]].&lt;br /&gt;
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This is analogous in signal processing to understanding a filter by its impulse response.&lt;br /&gt;
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这类似于在信号处理中通过滤波器的脉冲响应来理解滤波器。&lt;br /&gt;
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===Superposition principle===&lt;br /&gt;
叠加原理&lt;br /&gt;
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{{further| Superposition principle }}&lt;br /&gt;
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The superposition principle applies to any linear system, including linear systems of PDEs. A common visualization of this concept is the interaction of two waves in phase being combined to result in a greater amplitude, for example {{math|sin ''x'' + sin ''x'' {{=}} 2 sin ''x''}}. The same principle can be observed in PDEs where the solutions may be real or complex and additive. [[Superposition principle|superposition]]&lt;br /&gt;
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The superposition principle applies to any linear system, including linear systems of PDEs. A common visualization of this concept is the interaction of two waves in phase being combined to result in a greater amplitude, for example  2 sin x}}. The same principle can be observed in PDEs where the solutions may be real or complex and additive. superposition&lt;br /&gt;
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'''&amp;lt;font color = &amp;quot;#ff8000&amp;quot;&amp;gt;叠加原理 Superposition Principle&amp;lt;/font&amp;gt;适用于任何线性系统，包括偏微分方程的线性系统。这个概念的一个常见的可视化是两个同相位的波相互作用结合在一起会产生更大的振幅，例如 {{math|sin ''x'' + sin ''x'' {{=}} 2 sin ''x''}}。在偏微分方程中也可以观察到同样的原理，其中的解可能是真实的或复杂的和可加的。叠加&lt;br /&gt;
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If {{math|''u''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;}} and {{math|''u''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;}} are solutions of linear PDE in some function space {{mvar|R}}, then {{math|''u'' {{=}} ''c''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;''u''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; + ''c''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;''u''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;}} with any constants {{math|''c''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;}} and {{math|''c''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;}} are also a solution of that PDE in the same function space.&lt;br /&gt;
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If  and  are solutions of linear PDE in some function space , then  c&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;u&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; + c&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;u&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;}} with any constants  and  are also a solution of that PDE in the same function space.&lt;br /&gt;
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若线性偏微分方程在某个函数空间{{mvar|R}}中有解{{math|''u''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;}} 和 {{math|''u''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;}}，则{{math|''u'' {{=}} ''c''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;''u''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; + ''c''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;''u''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;}}也是该偏微分方程在同一函数空间中的解，其中{{math|''c''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;}} 和 {{math|''c''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;}} 是任意常数。&lt;br /&gt;
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===Methods for non-linear equations===&lt;br /&gt;
非线性方程的求解方法&lt;br /&gt;
{{see also|nonlinear partial differential equation}}&lt;br /&gt;
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There are no generally applicable methods to solve nonlinear PDEs. Still, existence and uniqueness results (such as the [[Cauchy–Kowalevski theorem]]) are often possible, as are proofs of important qualitative and quantitative properties of solutions (getting these results is a major part of [[mathematical analysis|analysis]]). Computational solution to the nonlinear PDEs, the [[split-step method]], exist for specific equations like [[nonlinear Schrödinger equation]].&lt;br /&gt;
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There are no generally applicable methods to solve nonlinear PDEs. Still, existence and uniqueness results (such as the Cauchy–Kowalevski theorem) are often possible, as are proofs of important qualitative and quantitative properties of solutions (getting these results is a major part of analysis). Computational solution to the nonlinear PDEs, the split-step method, exist for specific equations like nonlinear Schrödinger equation.&lt;br /&gt;
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对于非线性偏微分方程，目前还没有普遍适用的求解方法。然而，通常是可能知道解的存在性和唯一性(如柯西-科瓦列夫斯基定理)，也是可能得到解的重要定性和定量性质的证明(得到这些结果是分析的主要部分)。非线性偏微分方程的计算解，即分步法，对一些特定的方程适用，比如非线性'''&amp;lt;font color=&amp;quot;#ff8000&amp;quot;&amp;gt;薛定谔方程 Schrödinger equation&amp;lt;/font&amp;gt;'''。&lt;br /&gt;
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Nevertheless, some techniques can be used for several types of equations. The [[h-principle|{{mvar|h}}-principle]] is the most powerful method to solve [[Underdetermined system|underdetermined]] equations. The [[Riquier–Janet theory]] is an effective method for obtaining information about many analytic [[Overdetermined system|overdetermined]] systems.&lt;br /&gt;
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Nevertheless, some techniques can be used for several types of equations. The -principle is the most powerful method to solve underdetermined equations. The Riquier–Janet theory is an effective method for obtaining information about many analytic overdetermined systems.&lt;br /&gt;
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然而，一些技巧可以用于几种类型的方程。h-原理是求解欠定方程最有效的方法。里基尔-珍妮特理论是一种可以获得许多解析超定系统信息的有效方法。&lt;br /&gt;
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The [[method of characteristics]] can be used in some very special cases to solve partial differential equations.&lt;br /&gt;
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The method of characteristics can be used in some very special cases to solve partial differential equations.&lt;br /&gt;
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特征线法可用于求解某些特殊情况下的偏微分方程。&lt;br /&gt;
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In some cases, a PDE can be solved via [[perturbation analysis]] in which the solution is considered to be a correction to an equation with a known solution. Alternatives are [[numerical analysis]] techniques from simple [[finite difference]] schemes to the more mature [[multigrid]] and [[finite element method]]s. Many interesting problems in science and engineering are solved in this way using [[computer]]s, sometimes high performance [[supercomputer]]s.&lt;br /&gt;
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In some cases, a PDE can be solved via perturbation analysis in which the solution is considered to be a correction to an equation with a known solution. Alternatives are numerical analysis techniques from simple finite difference schemes to the more mature multigrid and finite element methods. Many interesting problems in science and engineering are solved in this way using computers, sometimes high performance supercomputers.&lt;br /&gt;
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在某些情况下，偏微分方程可以通过扰动分析来求解。在扰动分析中，通常是求解将具有已知解的方程修正后的新得到方程。可供选择的数值分析技术从简单的差分格式到更成熟的多重网格和有限元方法。许多有趣的科学和工程问题都是在计算机上用这种方法解决的，有时是高性能超级计算机。&lt;br /&gt;
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===Lie group method===&lt;br /&gt;
李群方法&lt;br /&gt;
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From 1870 [[Sophus Lie]]'s work put the theory of differential equations on a more satisfactory foundation. He showed that the integration theories of the older mathematicians can, by the introduction of what are now called [[Lie group]]s, be referred, to a common source; and that ordinary differential equations which admit the same [[infinitesimal transformation]]s present comparable difficulties of integration. He also emphasized the subject of [[contact transformation|transformations of contact]].&lt;br /&gt;
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From 1870 Sophus Lie's work put the theory of differential equations on a more satisfactory foundation. He showed that the integration theories of the older mathematicians can, by the introduction of what are now called Lie groups, be referred, to a common source; and that ordinary differential equations which admit the same infinitesimal transformations present comparable difficulties of integration. He also emphasized the subject of transformations of contact.&lt;br /&gt;
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从1870年起，索弗斯·李的工作为微分方程理论奠定了一个较为令人满意的基础。他指出，通过引入现在所谓的李群，老一辈数学家的积分理论可以引用到一个共同的来源; 承认相同的无穷小变换的常微分方程在积分方面存在相当的困难。他还强调了接触的转变这一主题。&lt;br /&gt;
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==[[用户:Yuling|Yuling]]（[[用户讨论:Yuling|讨论]]）这句话“He also emphasized the subject of transformations of contact.”中的transformations of contact翻译的不太好。&lt;br /&gt;
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A general approach to solving PDEs uses the symmetry property of differential equations, the continuous [[infinitesimal transformation]]s of solutions to solutions ([[Lie theory]]). Continuous [[group theory]], [[Lie algebras]] and [[differential geometry]] are used to understand the structure of linear and nonlinear partial differential equations for generating integrable equations, to find its [[Lax pair]]s, recursion operators, [[Bäcklund transform]] and finally finding exact analytic solutions to the PDE.&lt;br /&gt;
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A general approach to solving PDEs uses the symmetry property of differential equations, the continuous infinitesimal transformations of solutions to solutions (Lie theory). Continuous group theory, Lie algebras and differential geometry are used to understand the structure of linear and nonlinear partial differential equations for generating integrable equations, to find its Lax pairs, recursion operators, Bäcklund transform and finally finding exact analytic solutions to the PDE.&lt;br /&gt;
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求解偏微分方程的一般方法是利用微分方程的对称性，即解到解的连续无穷小变换(李理论)。连续群论、李代数和微分几何理论被用来理解生成可积方程的线性和非线性偏微分方程的结构，找到它的Lax对、递归算子、 贝克伦德变换，最后找到偏微分方程的精确解析解。&lt;br /&gt;
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Symmetry methods have been recognized to study differential equations arising in mathematics, physics, engineering, and many other disciplines.&lt;br /&gt;
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Symmetry methods have been recognized to study differential equations arising in mathematics, physics, engineering, and many other disciplines.&lt;br /&gt;
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对称方法已被公认可以用于研究出现在数学，物理，工程和许多其他学科的微分方程。&lt;br /&gt;
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===Semianalytical methods===&lt;br /&gt;
半解析方法&lt;br /&gt;
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The [[Adomian decomposition method]], the [[Aleksandr Lyapunov|Lyapunov]] artificial small parameter method, and He's [[homotopy perturbation method]] are all special cases of the more general [[homotopy analysis method]]. These are series expansion methods, and except for the Lyapunov method, are independent of small physical parameters as compared to the well known [[perturbation theory]], thus giving these methods greater flexibility and solution generality.&lt;br /&gt;
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The Adomian decomposition method, the Lyapunov artificial small parameter method, and He's homotopy perturbation method are all special cases of the more general homotopy analysis method. These are series expansion methods, and except for the Lyapunov method, are independent of small physical parameters as compared to the well known perturbation theory, thus giving these methods greater flexibility and solution generality.&lt;br /&gt;
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阿多米安分解法、李雅普诺夫人工小参数方法和何同伦摄动方法都是更一般的同伦分析方法的特殊情况。除了李雅普诺夫方法之外，这些都是级数展开方法，与为人熟知的摄动理论方法相比，它们与小的物理参数无关，因此这些方法具有更大的灵活性和解的通用性。&lt;br /&gt;
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== Numerical solutions ==&lt;br /&gt;
数值解&lt;br /&gt;
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The three most widely used [[Numerical partial differential equations|numerical methods to solve PDEs]] are the [[finite element analysis|finite element method]] (FEM), [[finite volume method]]s (FVM) and [[finite difference method]]s (FDM), as well other kind of methods called [[Meshfree methods]], which were made to solve problems where the before mentioned methods are limited. The FEM has a prominent position among these methods and especially its exceptionally efficient higher-order version [[hp-FEM]]. Other hybrid versions of FEM and Meshfree methods include the generalized finite element method (GFEM), [[extended finite element method]] (XFEM), [[Spectral element method|spectral finite element method]] (SFEM), [[Meshfree methods|meshfree finite element method]], [[Discontinuous Galerkin Method|discontinuous Galerkin finite element method]] (DGFEM), [[Element-Free Galerkin Method]] (EFGM), [[Interpolating Element-Free Galerkin Method]] (IEFGM), etc.&lt;br /&gt;
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The three most widely used numerical methods to solve PDEs are the finite element method (FEM), finite volume methods (FVM) and finite difference methods (FDM), as well other kind of methods called Meshfree methods, which were made to solve problems where the before mentioned methods are limited. The FEM has a prominent position among these methods and especially its exceptionally efficient higher-order version hp-FEM. Other hybrid versions of FEM and Meshfree methods include the generalized finite element method (GFEM), extended finite element method (XFEM), spectral finite element method (SFEM), meshfree finite element method, discontinuous Galerkin finite element method (DGFEM), Element-Free Galerkin Method (EFGM), Interpolating Element-Free Galerkin Method (IEFGM), etc.&lt;br /&gt;
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求解偏微分方程最常用的三种数值方法是有限元分析法、有限体积法和有限差分法，以及其他一些称为无网格法的方法。这些方法用于解决前面提到的方法受到的限制。在这些方法中，有限元方法，尤其是高效的高阶有限元方法，占有重要地位。其他有限元法和无网格法的混合形式包括广义有限元分析法(GFEM)、扩展有限元分析法(XFEM)、谱有限元分析法(SFEM)、无网格有限元分析法(DGFEM)、间断伽辽金有限元分析法(DGFEM)、无网格伽辽金法(EFGM)、插值无网格伽辽金法(IEFGM)等。&lt;br /&gt;
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=== Finite element method ===&lt;br /&gt;
有限元分析法&lt;br /&gt;
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{{main|Finite element method}}&lt;br /&gt;
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The finite element method (FEM) (its practical application often known as finite element analysis (FEA)) is a numerical technique for finding approximate solutions of partial differential equations (PDE) as well as of integral equations. The solution approach is based either on eliminating the differential equation completely (steady state problems), or rendering the PDE into an approximating system of ordinary differential equations, which are then numerically integrated using standard techniques such as Euler's method, Runge–Kutta, etc.&lt;br /&gt;
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The finite element method (FEM) (its practical application often known as finite element analysis (FEA)) is a numerical technique for finding approximate solutions of partial differential equations (PDE) as well as of integral equations. The solution approach is based either on eliminating the differential equation completely (steady state problems), or rendering the PDE into an approximating system of ordinary differential equations, which are then numerically integrated using standard techniques such as Euler's method, Runge–Kutta, etc.&lt;br /&gt;
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'''&amp;lt;font color = &amp;quot;#ff8000&amp;quot;&amp;gt;有限元分析法 Finite Element Method&amp;lt;/font&amp;gt;''' ((其实际应用通常被称为有限元分析(FEA))是一种寻找偏微分方程(PDE)和积分方程近似解的数值技术。这种求解方法要么基于完全消除微分方程(稳态问题) ，要么将偏微分方程转化为常微分方程的近似系统，然后使用标准技术进行数值积分，如欧拉方法、 Runge-Kutta 等。&lt;br /&gt;
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===Finite difference method===&lt;br /&gt;
有限差分法&lt;br /&gt;
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{{main|Finite difference method}}&lt;br /&gt;
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Finite-difference methods are numerical methods for approximating the solutions to differential equations using [[finite difference]] equations to approximate derivatives.&lt;br /&gt;
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Finite-difference methods are numerical methods for approximating the solutions to differential equations using finite difference equations to approximate derivatives.&lt;br /&gt;
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有限差分法是一种数值方法，用差分方程近似微分方程的解。&lt;br /&gt;
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=== Finite volume method ===&lt;br /&gt;
有限体积法&lt;br /&gt;
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{{main|Finite volume method}}&lt;br /&gt;
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Similar to the finite difference method or finite element method, values are calculated at discrete places on a meshed geometry. &amp;quot;Finite volume&amp;quot; refers to the small volume surrounding each node point on a mesh. In the finite volume method, surface integrals in a partial differential equation that contain a divergence term are converted to volume integrals, using the [[divergence theorem]]. These terms are then evaluated as fluxes at the surfaces of each finite volume. Because the flux entering a given volume is identical to that leaving the adjacent volume, these methods conserve mass by design.&lt;br /&gt;
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Similar to the finite difference method or finite element method, values are calculated at discrete places on a meshed geometry. &amp;quot;Finite volume&amp;quot; refers to the small volume surrounding each node point on a mesh. In the finite volume method, surface integrals in a partial differential equation that contain a divergence term are converted to volume integrals, using the divergence theorem. These terms are then evaluated as fluxes at the surfaces of each finite volume. Because the flux entering a given volume is identical to that leaving the adjacent volume, these methods conserve mass by design.&lt;br /&gt;
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类似于有限差分法或有限元分析，函数值是在网状几何体上的离散位置进行计算的。“有限体积”是指网格上每个节点周围的小体积。在有限体积法中，偏微分方程中含有散度项的面积分用散度定理积分转换成体积分。然后将这些项用于估算每个有限体积表面上的通量。由于进入给定体积的通量与转移到相邻体积元的通量相同，所以这些方法在设计上保证了质量守恒。&lt;br /&gt;
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==See also==&lt;br /&gt;
请参阅&lt;br /&gt;
* [[Dirichlet boundary condition]]&lt;br /&gt;
狄利克雷边界条件&lt;br /&gt;
* [[Jet bundle]]&lt;br /&gt;
射流丛&lt;br /&gt;
* [[Laplace transform applied to differential equations]]&lt;br /&gt;
微分方程中的拉普拉斯变换&lt;br /&gt;
* [[List of dynamical systems and differential equations topics]]&lt;br /&gt;
动力学系统和微分方程的列表&lt;br /&gt;
* [[Matrix differential equation]]&lt;br /&gt;
矩阵微分方程&lt;br /&gt;
* [[Neumann boundary condition]]&lt;br /&gt;
诺伊曼边界条件&lt;br /&gt;
* [[Numerical partial differential equations]]&lt;br /&gt;
数值偏微分方程&lt;br /&gt;
* [[Partial differential algebraic equation]]&lt;br /&gt;
偏微分代数方程&lt;br /&gt;
* [[Recurrence relation]]&lt;br /&gt;
递推关系&lt;br /&gt;
* [[Robin boundary condition]]&lt;br /&gt;
罗宾边界条件&lt;br /&gt;
* [[Stochastic processes and boundary value problems]]&lt;br /&gt;
随机过程和边值问题&lt;br /&gt;
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== The energy method ==&lt;br /&gt;
能量法&lt;br /&gt;
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The energy method is a mathematical procedure that can be used to verify well-posedness of initial-boundary-value-problems.&amp;lt;ref&amp;gt;{{cite book |title=High Order Difference Methods for Time Dependent PDE&lt;br /&gt;
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The energy method is a mathematical procedure that can be used to verify well-posedness of initial-boundary-value-problems.&amp;lt;ref&amp;gt;{{cite book |title=High Order Difference Methods for Time Dependent PDE&lt;br /&gt;
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能量法是验证初边值问题适定性的一种数学方法。 时变偏微分方程的高阶差分方法&lt;br /&gt;
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|first=Bertil|last=Gustafsson|publisher=Springer|year=2008|isbn=978-3-540-74992-9|doi=10.1007/978-3-540-74993-6}}&amp;lt;/ref&amp;gt; In the following example the energy method is used to decide where and which boundary conditions should be imposed such that the resulting IBVP is well-posed. Consider the one-dimensional hyperbolic PDE given by&lt;br /&gt;
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|first=Bertil|last=Gustafsson|publisher=Springer|year=2008|isbn=978-3-540-74992-9|doi=10.1007/978-3-540-74993-6}}&amp;lt;/ref&amp;gt; In the following example the energy method is used to decide where and which boundary conditions should be imposed such that the resulting IBVP is well-posed. Consider the one-dimensional hyperbolic PDE given by&lt;br /&gt;
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| first Bertil | last Gustafsson | publisher | Springer | year 2008 | isbn 978-3-540-74992-9 | doi 10.1007 / 978-3-540-74993-6} / ref 在下面的例子中，使用能量方法来决定应该施加哪些边界条件，使得得到的 IBVP适定。考虑一维双曲偏微分方程&lt;br /&gt;
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: &amp;lt;math&amp;gt;\frac{\partial u}{\partial t} + \alpha \frac{\partial u}{\partial x} = 0, \quad x \in [a,b], \operatorname t &amp;gt; 0,&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;\frac{\partial u}{\partial t} + \alpha \frac{\partial u}{\partial x} = 0, \quad x \in [a,b], \operatorname t &amp;gt; 0,&amp;lt;/math&amp;gt;&lt;br /&gt;
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where &amp;lt;math&amp;gt;\alpha \neq 0&amp;lt;/math&amp;gt; is a constant and &amp;lt;math&amp;gt;u(x,t)&amp;lt;/math&amp;gt; is an unknown function with initial condition &amp;lt;math&amp;gt;u(x,0) = f(x)&amp;lt;/math&amp;gt;. Multiplying with &amp;lt;math&amp;gt;u&amp;lt;/math&amp;gt; and integrating over the domain gives&lt;br /&gt;
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where &amp;lt;math&amp;gt;\alpha \neq 0&amp;lt;/math&amp;gt; is a constant and &amp;lt;math&amp;gt;u(x,t)&amp;lt;/math&amp;gt; is an unknown function with initial condition &amp;lt;math&amp;gt;u(x,0) = f(x)&amp;lt;/math&amp;gt;. Multiplying with &amp;lt;math&amp;gt;u&amp;lt;/math&amp;gt; and integrating over the domain gives&lt;br /&gt;
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其中 &amp;lt;math&amp;gt;\alpha \neq 0&amp;lt;/math&amp;gt; 是常数，并且 &amp;lt;math&amp;gt;u(x,t)&amp;lt;/math&amp;gt; 是未知函数，初始条件是 &amp;lt;math&amp;gt;u(x,0) = f(x)&amp;lt;/math&amp;gt;。乘以 &amp;lt;math&amp;gt;u&amp;lt;/math&amp;gt; 并在域上进行积分。&lt;br /&gt;
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: &amp;lt;math&amp;gt;\int_a^b u \frac{\partial u}{\partial t} \operatorname dx + \alpha \int _a ^b u \frac{\partial u}{\partial x} \operatorname dx = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;\int_a^b u \frac{\partial u}{\partial t} \operatorname dx + \alpha \int _a ^b u \frac{\partial u}{\partial x} \operatorname dx = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
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Using that&lt;br /&gt;
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Using that&lt;br /&gt;
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利用这一点&lt;br /&gt;
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: &amp;lt;math&amp;gt;\int _a ^b u \frac{\partial u}{\partial t} \operatorname dx = \frac{1}{2} \frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 \quad \text{and} \quad \int _a ^b u \frac{\partial u}{\partial x} \operatorname dx = \frac{1}{2} u(b,t)^2 - \frac{1}{2} u(a,t)^2,.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;\int _a ^b u \frac{\partial u}{\partial t} \operatorname dx = \frac{1}{2} \frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 \quad \text{and} \quad \int _a ^b u \frac{\partial u}{\partial x} \operatorname dx = \frac{1}{2} u(b,t)^2 - \frac{1}{2} u(a,t)^2,.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
where integration by parts has been used for the second relationship, we get&lt;br /&gt;
&lt;br /&gt;
where integration by parts has been used for the second relationship, we get&lt;br /&gt;
&lt;br /&gt;
第二个关系中采用了分部积分法，我们可以得到&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt;\frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 + \alpha u(b,t)^2 - \alpha u(a,t)^2 = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;\frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 + \alpha u(b,t)^2 - \alpha u(a,t)^2 = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Here &amp;lt;math&amp;gt;\vert \vert \cdot \vert \vert&amp;lt;/math&amp;gt; denotes the standard L2-norm.&lt;br /&gt;
&lt;br /&gt;
Here &amp;lt;math&amp;gt;\vert \vert \cdot \vert \vert&amp;lt;/math&amp;gt; denotes the standard L2-norm.&lt;br /&gt;
&lt;br /&gt;
在这里，&amp;lt;math&amp;gt;\vert \vert \cdot \vert \vert&amp;lt;/math&amp;gt; 表示标准的 L2-正则。&lt;br /&gt;
&lt;br /&gt;
For well-posedness we require that the energy of the solution is non-increasing, i.e. that &amp;lt;math&amp;gt;\frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 \leq 0&amp;lt;/math&amp;gt;, which is achieved by specifying &amp;lt;math&amp;gt;u&amp;lt;/math&amp;gt; at &amp;lt;math&amp;gt;x = a&amp;lt;/math&amp;gt; if &amp;lt;math&amp;gt;\alpha &amp;gt; 0&amp;lt;/math&amp;gt; and at &amp;lt;math&amp;gt;x = b&amp;lt;/math&amp;gt; if &amp;lt;math&amp;gt;\alpha &amp;lt; 0&amp;lt;/math&amp;gt;. This corresponds to only imposing boundary conditions at the inflow. Note that well-posedness allows for growth in terms of data (initial and boundary) and thus it is sufficient to show that &amp;lt;math&amp;gt;\frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 \leq 0&amp;lt;/math&amp;gt; holds when all data is set to zero.&lt;br /&gt;
&lt;br /&gt;
For well-posedness we require that the energy of the solution is non-increasing, i.e. that &amp;lt;math&amp;gt;\frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 \leq 0&amp;lt;/math&amp;gt;, which is achieved by specifying &amp;lt;math&amp;gt;u&amp;lt;/math&amp;gt; at &amp;lt;math&amp;gt;x = a&amp;lt;/math&amp;gt; if &amp;lt;math&amp;gt;\alpha &amp;gt; 0&amp;lt;/math&amp;gt; and at &amp;lt;math&amp;gt;x = b&amp;lt;/math&amp;gt; if &amp;lt;math&amp;gt;\alpha &amp;lt; 0&amp;lt;/math&amp;gt;. This corresponds to only imposing boundary conditions at the inflow. Note that well-posedness allows for growth in terms of data (initial and boundary) and thus it is sufficient to show that &amp;lt;math&amp;gt;\frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 \leq 0&amp;lt;/math&amp;gt; holds when all data is set to zero.&lt;br /&gt;
&lt;br /&gt;
对于适定性，我们要解的能量是不增加的，即 &amp;lt;math&amp;gt;\frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 \leq 0&amp;lt;/math&amp;gt; ，这种关系可以通过在&amp;lt;math&amp;gt;x = a&amp;lt;/math&amp;gt;处 （如果 &amp;lt;math&amp;gt;\alpha &amp;gt; 0&amp;lt;/math&amp;gt;） 以及 &amp;lt;math&amp;gt;x = b&amp;lt;/math&amp;gt;处 （如果 &amp;lt;math&amp;gt;\alpha &amp;lt; 0&amp;lt;/math&amp;gt;）指定&amp;lt;math&amp;gt;u&amp;lt;/math&amp;gt;的值来实现。这只相当于在入流处附加边界条件。注意，适定性允许在数据(初始和边界)上的增长，因此它足以表明当所有数据设置为零时应有 &amp;lt;math&amp;gt;\frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 \leq 0&amp;lt;/math&amp;gt;。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==[[用户:Yuling|Yuling]]（[[用户讨论:Yuling|讨论]]）“This corresponds to only imposing boundary conditions at the inflow.” 这句话中的inflow不是很理解&lt;br /&gt;
&lt;br /&gt;
==Notes==&lt;br /&gt;
&lt;br /&gt;
{{Reflist}}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
== References ==&lt;br /&gt;
&lt;br /&gt;
{{refbegin|2}}&lt;br /&gt;
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|first=G.|last=Adomian|publisher=Kluwer Academic Publishers|year=1994|isbn=|page=|url=https://books.google.com/books?id=UKPqCAAAQBAJ&amp;amp;printsec=frontcover#v=onepage&amp;amp;q=%22partial%20differential%22&amp;amp;f=false}}&lt;br /&gt;
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&lt;br /&gt;
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&lt;br /&gt;
* {{Citation |first=P. |last=Solin |first2=K. |last2=Segeth |lastauthoramp=yes |first3=I. |last3=Dolezel |title=Higher-Order Finite Element Methods |publisher=Chapman &amp;amp; Hall/CRC Press |location=Boca Raton |year=2003 |isbn=1-58488-438-X }}.&lt;br /&gt;
&lt;br /&gt;
* {{Citation |first=H. |last=Stephani |year=1989 |title=Differential Equations: Their Solution Using Symmetries. Edited by M. MacCallum |publisher=Cambridge University Press }}.&lt;br /&gt;
&lt;br /&gt;
* {{cite book |title=Partial Differential Equations and Solitary Waves Theory&lt;br /&gt;
&lt;br /&gt;
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| first Abdul-Majid | last Wazwaz | publisher Higher Education Press | year 2009 | isbn 978-3-642-00251-9 | page }&lt;br /&gt;
&lt;br /&gt;
* {{cite book |title=Partial Differential Equations Methods and Applications&lt;br /&gt;
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| first Abdul-Majid | last Wazwaz | publisher a.a.Balkema | year 2002 | isbn 90-5809-369-7 | page }&lt;br /&gt;
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&lt;br /&gt;
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&lt;br /&gt;
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&lt;br /&gt;
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&lt;br /&gt;
* {{cite book |title=High Order Difference Methods for Time Dependent PDE&lt;br /&gt;
&lt;br /&gt;
|first=Bertil|last=Gustafsson|publisher=Springer|year=2008|isbn=978-3-540-74992-9|doi=10.1007/978-3-540-74993-6}}&lt;br /&gt;
&lt;br /&gt;
|first=Bertil|last=Gustafsson|publisher=Springer|year=2008|isbn=978-3-540-74992-9|doi=10.1007/978-3-540-74993-6}}&lt;br /&gt;
&lt;br /&gt;
| first Bertil | last Gustafsson | Springer | year 2008 | isbn 978-3-540-74992-9 | doi 10.1007 / 978-3-540-74993-6}&lt;br /&gt;
&lt;br /&gt;
{{refend}}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
== Further reading ==&lt;br /&gt;
&lt;br /&gt;
* {{Cite journal|last=Cajori|first=Florian|authorlink=Florian Cajori|year=1928|title=The Early History of Partial Differential Equations and of Partial Differentiation and Integration|url=http://www.math.harvard.edu/archive/21a_fall_14/exhibits/cajori/cajori.pdf|journal=The American Mathematical Monthly|volume=35|issue=9|pages=459–467|doi=10.2307/2298771|access-date=2016-05-15|archive-url=https://web.archive.org/web/20181123102253/http://www.math.harvard.edu/archive/21a_fall_14/exhibits/cajori/cajori.pdf|archive-date=2018-11-23|url-status=dead}}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
== External links ==&lt;br /&gt;
&lt;br /&gt;
{{Sister project links| wikt=no | commons=Category:Solutions of PDE | b=Partial Differential Equations | n=no | q=Partial differential equation | s=no | v=no | voy=no | species=no | d=no}}&lt;br /&gt;
&lt;br /&gt;
* {{springer|title=Differential equation, partial|id=p/d031920}}&lt;br /&gt;
&lt;br /&gt;
* [http://eqworld.ipmnet.ru/en/pde-en.htm Partial Differential Equations: Exact Solutions] at EqWorld: The World of Mathematical Equations.&lt;br /&gt;
&lt;br /&gt;
* [http://eqworld.ipmnet.ru/en/solutions/eqindex/eqindex-pde.htm Partial Differential Equations: Index] at EqWorld: The World of Mathematical Equations.&lt;br /&gt;
&lt;br /&gt;
* [http://eqworld.ipmnet.ru/en/methods/meth-pde.htm Partial Differential Equations: Methods] at EqWorld: The World of Mathematical Equations.&lt;br /&gt;
&lt;br /&gt;
* [https://web.archive.org/web/20170701144823/http://www.exampleproblems.com/wiki/index.php?title=Partial_Differential_Equations Example problems with solutions] at exampleproblems.com&lt;br /&gt;
&lt;br /&gt;
* [http://mathworld.wolfram.com/PartialDifferentialEquation.html Partial Differential Equations] at mathworld.wolfram.com&lt;br /&gt;
&lt;br /&gt;
* [https://reference.wolfram.com/language/FEMDocumentation/tutorial/SolvingPDEwithFEM.html Partial Differential Equations] with Mathematica&lt;br /&gt;
&lt;br /&gt;
* [http://www.mathworks.com/moler/pdes.pdf Partial Differential Equations] in Cleve Moler: Numerical Computing with MATLAB&lt;br /&gt;
&lt;br /&gt;
* [http://www.nag.com/numeric/fl/nagdoc_fl24/html/D03/d03intro.html Partial Differential Equations] at nag.com&lt;br /&gt;
&lt;br /&gt;
* {{cite web |first=Grant |last=Sanderson |title=But what is a partial differential equation? |work=3Blue1Brown |date=April 21, 2019 |url=https://www.youtube.com/watch?v=ly4S0oi3Yz8&amp;amp;list=PLZHQObOWTQDNPOjrT6KVlfJuKtYTftqH6 |via=[[YouTube]] }}&lt;br /&gt;
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&lt;br /&gt;
{{Differential equations topics}}&lt;br /&gt;
&lt;br /&gt;
{{Authority control}}&lt;br /&gt;
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&lt;br /&gt;
[[Category:Partial differential equations| ]]&lt;br /&gt;
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[[Category:Multivariable calculus]]&lt;br /&gt;
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Category:Multivariable calculus&lt;br /&gt;
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类别: 多元微积分&lt;br /&gt;
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[[Category:Differential equations]]&lt;br /&gt;
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Category:Differential equations&lt;br /&gt;
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类别: 微分方程&lt;br /&gt;
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[[Category:Concepts in physics]]&lt;br /&gt;
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Category:Concepts in physics&lt;br /&gt;
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分类: 物理概念&lt;br /&gt;
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&amp;lt;noinclude&amp;gt;&lt;br /&gt;
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&amp;lt;small&amp;gt;This page was moved from [[wikipedia:en:Partial differential equation]]. Its edit history can be viewed at [[偏微分方程/edithistory]]&amp;lt;/small&amp;gt;&amp;lt;/noinclude&amp;gt;&lt;br /&gt;
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[[Category:待整理页面]]&lt;/div&gt;</summary>
		<author><name>Ruili</name></author>
	</entry>
	<entry>
		<id>https://wiki.swarma.org/index.php?title=%E5%81%8F%E5%BE%AE%E5%88%86%E6%96%B9%E7%A8%8B&amp;diff=18115</id>
		<title>偏微分方程</title>
		<link rel="alternate" type="text/html" href="https://wiki.swarma.org/index.php?title=%E5%81%8F%E5%BE%AE%E5%88%86%E6%96%B9%E7%A8%8B&amp;diff=18115"/>
		<updated>2020-11-11T13:13:47Z</updated>

		<summary type="html">&lt;p&gt;Ruili：&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;此词条暂由Yuling翻译，未经人工整理和审校，带来阅读不便，请见谅。&lt;br /&gt;
&lt;br /&gt;
[[File:Heat.gif|thumb|right|A visualisation of a solution to the two-dimensional [[heat equation]] with temperature represented by the third dimension]]&lt;br /&gt;
&lt;br /&gt;
A visualisation of a solution to the two-dimensional [[heat equation with temperature represented by the third dimension]]&lt;br /&gt;
&lt;br /&gt;
以三维表示温度的二维热方程解的可视化&lt;br /&gt;
&lt;br /&gt;
In [[mathematics]], a '''partial differential equation''' ('''PDE''') is a [[differential equation]] that contains unknown [[Multivariable calculus|multivariable functions]] and their [[partial derivative]]s. PDEs are used to formulate problems involving functions of several variables, and are either solved by hand, or used to create a [[computer model]]. A special case is [[ordinary differential equation]]s (ODEs), which deal with functions of a single variable and their derivatives.&lt;br /&gt;
&lt;br /&gt;
In mathematics, a partial differential equation (PDE) is a differential equation that contains unknown multivariable functions and their partial derivatives. PDEs are used to formulate problems involving functions of several variables, and are either solved by hand, or used to create a computer model. A special case is ordinary differential equations (ODEs), which deal with functions of a single variable and their derivatives.&lt;br /&gt;
&lt;br /&gt;
在数学中，'''&amp;lt;font color = &amp;quot;#ff8000&amp;quot;&amp;gt;偏微分方程函数 Partial Differential Equation&amp;lt;/font&amp;gt;'''是包含未知多元函数及其偏导数的微分方程。偏微分方程用于描述涉及多元函数的问题，可以通过人为求解，也可以通过建立计算机模型来求解。常微分方程是偏微分方程一种特殊情况，它处理的是一元函数及其导数。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
PDEs can be used to describe a wide variety of phenomena such as sound, heat, [[diffusion]], [[electrostatics]], [[Electromagnetism|electrodynamics]], [[fluid dynamics]], [[Elasticity (physics)|elasticity]], [[gravitation]] and [[quantum mechanics]]. These seemingly distinct physical phenomena can be formalised similarly in terms of PDEs. Just as ordinary differential equations often model one-dimensional [[dynamical system]]s, partial differential equations often model [[multidimensional system]]s. PDEs find their generalisation in [[stochastic partial differential equation]]s.&lt;br /&gt;
&lt;br /&gt;
PDEs can be used to describe a wide variety of phenomena such as sound, heat, diffusion, electrostatics, electrodynamics, fluid dynamics, elasticity, gravitation and quantum mechanics. These seemingly distinct physical phenomena can be formalised similarly in terms of PDEs. Just as ordinary differential equations often model one-dimensional dynamical systems, partial differential equations often model multidimensional systems. PDEs find their generalisation in stochastic partial differential equations.&lt;br /&gt;
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偏微分方程可以用来描述各种各样的物理现象，如声音，热量，扩散，静电，电动力学，流体力学，弹性力学，重力和量子力学。这些看起来截然不同的物理现象却可以用类似的偏微分方程来描述。正如常微分方程经常对一维动力系统进行建模一样，偏微分方程经常对多维系统进行建模。随机偏微分方程是偏微分方程的一种推广。&lt;br /&gt;
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== Introduction ==&lt;br /&gt;
引言&lt;br /&gt;
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Partial differential equations (PDEs) are equations that involve rates of change with respect to [[continuous variables]]. For example, the position of a [[rigid body]] is specified by six parameters,&amp;lt;ref&amp;gt;{{Cite book|url=https://books.google.com/books?id=v9PLbcYd9aUC&amp;amp;pg=PA32|title=Modelling and Control of Robot Manipulators|last=Sciavicco|first=Lorenzo|last2=Siciliano|first2=Bruno|date=2001-02-19|publisher=Springer Science &amp;amp; Business Media|isbn=9781852332211|language=en}}&amp;lt;/ref&amp;gt; but the configuration of a [[fluid]] is given by the [[continuous distribution]] of several parameters, such as the [[temperature]], [[pressure]], and so forth. The dynamics for the rigid body take place in a finite-dimensional [[Configuration space (physics)|configuration space]]; the dynamics for the fluid occur in an infinite-dimensional configuration space. This distinction usually makes PDEs much harder to solve than ordinary differential equations (ODEs), but here again, there will be simple solutions for linear problems. Classic domains where PDEs are used include [[acoustics]], [[fluid dynamics]], [[electrodynamics]], and [[heat transfer]].&lt;br /&gt;
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Partial differential equations (PDEs) are equations that involve rates of change with respect to continuous variables. For example, the position of a rigid body is specified by six parameters, but the configuration of a fluid is given by the continuous distribution of several parameters, such as the temperature, pressure, and so forth. The dynamics for the rigid body take place in a finite-dimensional configuration space; the dynamics for the fluid occur in an infinite-dimensional configuration space. This distinction usually makes PDEs much harder to solve than ordinary differential equations (ODEs), but here again, there will be simple solutions for linear problems. Classic domains where PDEs are used include acoustics, fluid dynamics, electrodynamics, and heat transfer.&lt;br /&gt;
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偏微分方程(简称为PDEs)涉及到方程相对于连续变量的变化率。例如，刚体的位置是由六个参数确定的，而流体的状态是由几个参数的连续分布给出的，如温度、压力等。刚体的动力学过程发生在有限维状态空间中，流体的动力学过程发生在无限维状态空间中。这种区别通常使偏微分方程比常微分方程更难求解，但是线性问题仍然有简单的求解方式。使用偏微分方程的经典领域包括声学、流体力学、电动力学和传热学。&lt;br /&gt;
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A partial differential equation (PDE) for the function {{math|''u''(''x''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;,… ''x&amp;lt;sub&amp;gt;n&amp;lt;/sub&amp;gt;'')}} is an equation of the form&lt;br /&gt;
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A partial differential equation (PDE) for the function  is an equation of the form&lt;br /&gt;
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函数{{math|''u''(''x''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;,… ''x&amp;lt;sub&amp;gt;n&amp;lt;/sub&amp;gt;'')}}的偏微分方程形式是：&lt;br /&gt;
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: &amp;lt;math&amp;gt;f \left (x_1, \ldots x_n; u, \frac{\partial u}{\partial x_1}, \ldots \frac{\partial u}{\partial x_n}; \frac{\partial^2 u}{\partial x_1 \partial x_1}, \ldots \frac{\partial^2 u}{\partial x_1 \partial x_n}; \ldots \right) = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;f \left (x_1, \ldots x_n; u, \frac{\partial u}{\partial x_1}, \ldots \frac{\partial u}{\partial x_n}; \frac{\partial^2 u}{\partial x_1 \partial x_1}, \ldots \frac{\partial^2 u}{\partial x_1 \partial x_n}; \ldots \right) = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
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If {{mvar|f}} is a [[linear function]] of {{mvar|u}} and its derivatives, then the PDE is called linear. Common examples of linear PDEs include the [[heat equation]], the [[wave equation]], [[Laplace's equation]], [[Helmholtz equation]], [[Klein–Gordon equation]], and [[Poisson's equation]].&lt;br /&gt;
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If  is a linear function of  and its derivatives, then the PDE is called linear. Common examples of linear PDEs include the heat equation, the wave equation, Laplace's equation, Helmholtz equation, Klein–Gordon equation, and Poisson's equation.&lt;br /&gt;
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如果{{mvar|f}}是函数及其导数的线性方程，则偏微分方程称为线性函数。线性偏微分方程的常见例子包括热方程、波动方程、拉普拉斯方程、亥姆霍兹方程方程、克莱因-高登方程和泊松方程。&lt;br /&gt;
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A relatively simple PDE is&lt;br /&gt;
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A relatively simple PDE is&lt;br /&gt;
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一个相对简单的偏微分方程是：&lt;br /&gt;
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: &amp;lt;math&amp;gt;\frac{\partial u}{\partial x}(x,y) = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;\frac{\partial u}{\partial x}(x,y) = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
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This relation [[Logical implication|implies]] that the function {{math|''u''(''x'',''y'')}} is independent of {{mvar|x}}. However, the equation gives no information on the function's dependence on the variable {{mvar|y}}. Hence the general solution of this equation is&lt;br /&gt;
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This relation implies that the function  is independent of . However, the equation gives no information on the function's dependence on the variable . Hence the general solution of this equation is&lt;br /&gt;
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这个关系意味着函数是独立于{{mvar|x}}的。然而，这个方程没有给出关于函数和自变量的相关性的信息。因此，这个方程的通解是&lt;br /&gt;
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: &amp;lt;math&amp;gt;u(x,y) = f(y),&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;u(x,y) = f(y),&amp;lt;/math&amp;gt;&lt;br /&gt;
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where {{mvar|f}} is an arbitrary function of {{mvar|y}}. The analogous ordinary differential equation is&lt;br /&gt;
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where  is an arbitrary function of . The analogous ordinary differential equation is&lt;br /&gt;
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其中{{mvar|f}}是{{mvar|y}}的任意函数。类似的常微分方程是&lt;br /&gt;
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: &amp;lt;math&amp;gt;\frac{\mathrm{d} u}{\mathrm{d} x}(x) = 0,&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;\frac{\mathrm{d} u}{\mathrm{d} x}(x) = 0,&amp;lt;/math&amp;gt;&lt;br /&gt;
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which has the solution&lt;br /&gt;
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which has the solution&lt;br /&gt;
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它的解为&lt;br /&gt;
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: &amp;lt;math&amp;gt;u(x) = c,&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;u(x) = c,&amp;lt;/math&amp;gt;&lt;br /&gt;
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where {{mvar|c}} is any [[Constant (mathematics)|constant]] value. These two examples illustrate that general solutions of ordinary differential equations (ODEs) involve arbitrary constants, but solutions of PDEs involve arbitrary functions.&lt;br /&gt;
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where  is any constant value. These two examples illustrate that general solutions of ordinary differential equations (ODEs) involve arbitrary constants, but solutions of PDEs involve arbitrary functions.&lt;br /&gt;
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这里的{{mvar|c}}是常量。这两个例子说明常微分方程的一般解包含任意常数，但偏微分方程的解包含任意函数。&lt;br /&gt;
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A solution of a PDE is generally not [[Uniqueness quantification|unique]]; additional conditions must generally be specified on the [[Boundary (topology)|boundary]] of the region where the solution is defined. For instance, in the simple example above, the function {{math|''f''(''y'')}} can be determined if {{mvar|u}} is specified on the line {{math|''x'' {{=}} 0}}.&lt;br /&gt;
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A solution of a PDE is generally not unique; additional conditions must generally be specified on the boundary of the region where the solution is defined. For instance, in the simple example above, the function  can be determined if  is specified on the line  0}}.&lt;br /&gt;
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偏微分方程的解一般不是唯一的; 附加条件一般必须在定义解的区域边界上定义。例如，在上面的简单示例中，如果在{{math|''x'' {{=}} 0}}时确定了{{mvar|u}}的值，则可以确定该函数{{math|''f''(''y'')}}。&lt;br /&gt;
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== Existence and uniqueness ==&lt;br /&gt;
存在性和唯一性&lt;br /&gt;
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Although the issue of existence and uniqueness of solutions of ordinary differential equations has a very satisfactory answer with the [[Picard–Lindelöf theorem]], that is far from the case for partial differential equations. The [[Cauchy–Kowalevski theorem]] states that the [[Cauchy problem]] for any partial differential equation whose coefficients are [[Analytic function|analytic]] in the unknown function and its derivatives, has a locally unique analytic solution. Although this result might appear to settle the existence and uniqueness of solutions, there are examples of linear partial differential equations whose coefficients have derivatives of all orders (which are nevertheless not analytic) but which have no solutions at all: see [[Lewy's example|Lewy (1957)]]. Even if the solution of a partial differential equation exists and is unique, it may nevertheless have undesirable properties.  The mathematical study of these questions is usually in the more powerful context of [[weak solution]]s.&lt;br /&gt;
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Although the issue of existence and uniqueness of solutions of ordinary differential equations has a very satisfactory answer with the Picard–Lindelöf theorem, that is far from the case for partial differential equations. The Cauchy–Kowalevski theorem states that the Cauchy problem for any partial differential equation whose coefficients are analytic in the unknown function and its derivatives, has a locally unique analytic solution. Although this result might appear to settle the existence and uniqueness of solutions, there are examples of linear partial differential equations whose coefficients have derivatives of all orders (which are nevertheless not analytic) but which have no solutions at all: see Lewy (1957). Even if the solution of a partial differential equation exists and is unique, it may nevertheless have undesirable properties.  The mathematical study of these questions is usually in the more powerful context of weak solutions.&lt;br /&gt;
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虽然常微分方程解的存在唯一性问题用'''&amp;lt;font color=&amp;quot;#ff8000&amp;quot;&amp;gt;弗罗贝尼乌斯定理 Picard–Lindelöf Theorem&amp;lt;/font&amp;gt;得到了令人满意的结果，但应用到偏微分方程上却不尽如意。'''&amp;lt;font color=&amp;quot;#ff8000&amp;quot;&amp;gt;柯西-科瓦列夫斯基定理 Cauchy–Kowalevski theorem&amp;lt;/font&amp;gt;指出，对于任何在未知函数及其导数中系数是解析的偏微分方程，柯西问题有一个局部唯一的解析解。虽然这个结果似乎解决了解的存在性和唯一性问题，但是有一些线性偏微分方程的系数具有所有级数的导数(尽管这些导数不是解析的) ，但是根本没有解: 见 Lewy (1957)。即使偏微分方程的解存在且唯一，它仍然可能具有人们所不希望的性质。这些问题的数学研究通常是在更有力的弱解的背景下进行的。&lt;br /&gt;
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An example of pathological behavior is the sequence (depending upon {{mvar|n}}) of [[Cauchy problem]]s for the [[Laplace equation]]&lt;br /&gt;
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An example of pathological behavior is the sequence (depending upon ) of Cauchy problems for the Laplace equation&lt;br /&gt;
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反常特征的一个例子是拉普拉斯方程的柯西问题的序列(取决于{{mvar|n}})&lt;br /&gt;
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: &amp;lt;math&amp;gt;\frac{\partial^2 u}{\partial x^2} + \frac{\partial^2 u}{\partial y^2}=0,&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;\frac{\partial^2 u}{\partial x^2} + \frac{\partial^2 u}{\partial y^2}=0,&amp;lt;/math&amp;gt;&lt;br /&gt;
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with [[boundary condition]]s&lt;br /&gt;
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with boundary conditions&lt;br /&gt;
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有边界条件&lt;br /&gt;
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: &amp;lt;math&amp;gt;\begin{align} u(x,0) &amp;amp;= 0, \\ \frac{\partial u}{\partial y}(x,0) &amp;amp;= \frac{\sin nx}{n}, \end{align}&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;\begin{align} u(x,0) &amp;amp;= 0, \\ \frac{\partial u}{\partial y}(x,0) &amp;amp;= \frac{\sin nx}{n}, \end{align}&amp;lt;/math&amp;gt;&lt;br /&gt;
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where {{mvar|n}} is an integer. The derivative of {{mvar|u}} with respect to {{mvar|y}} approaches zero [[uniform convergence|uniformly]] in {{mvar|x}} as {{mvar|n}} increases, but the solution is&lt;br /&gt;
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where  is an integer. The derivative of  with respect to  approaches zero uniformly in  as  increases, but the solution is&lt;br /&gt;
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其中{{mvar|n}}是整数。{{mvar|u}}是关于{{mvar|y}}的导数，一致地随着{{mvar|n}}的增加而趋于零，但是解是&lt;br /&gt;
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: &amp;lt;math&amp;gt;u(x,y) = \frac{\sinh ny \sin nx}{n^2}.&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;u(x,y) = \frac{\sinh ny \sin nx}{n^2}.&amp;lt;/math&amp;gt;&lt;br /&gt;
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This solution approaches infinity if {{mvar|nx}} is not an integer multiple of {{pi}} for any non-zero value of {{mvar|y}}. The Cauchy problem for the Laplace equation is called ''ill-posed'' or ''not [[Well-posed problem|well-posed]]'', since the solution does not continuously depend on the data of the problem. Such ill-posed problems are not usually satisfactory for physical applications.&lt;br /&gt;
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This solution approaches infinity if  is not an integer multiple of  for any non-zero value of . The Cauchy problem for the Laplace equation is called ill-posed or not well-posed, since the solution does not continuously depend on the data of the problem. Such ill-posed problems are not usually satisfactory for physical applications.&lt;br /&gt;
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对于任何非零的{{mvar|y}}，如果{{mvar|nx}}不是{{pi}}的整数倍，这个解会接近于无穷大。拉普拉斯方程的柯西问题被称为不适定问题（可以译为ill-posed或not well-posed），因为该问题的解并不连续地依赖于该问题的数据。这种不适定问题在物理应用中通常不能令人满意。&lt;br /&gt;
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The [[Navier–Stokes existence and smoothness|existence of solutions for the Navier–Stokes equations]], a partial differential equation, is part of one of the [[Millennium Prize Problems]].&lt;br /&gt;
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The existence of solutions for the Navier–Stokes equations, a partial differential equation, is part of one of the Millennium Prize Problems.&lt;br /&gt;
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一种偏微分方程——纳维-斯托克斯方程——的解的存在性就是千禧年大奖难题的一部分。&lt;br /&gt;
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== Notation ==&lt;br /&gt;
符号&lt;br /&gt;
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In PDEs, it is common to denote partial derivatives using subscripts. That is:&lt;br /&gt;
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In PDEs, it is common to denote partial derivatives using subscripts. That is:&lt;br /&gt;
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在偏微分方程中，通常用下标表示偏导数。例如:&lt;br /&gt;
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: &amp;lt;math&amp;gt;u_x = \frac{\partial u}{\partial x}&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;u_x = \frac{\partial u}{\partial x}&amp;lt;/math&amp;gt;&lt;br /&gt;
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: &amp;lt;math&amp;gt;u_{xx} = \frac{\partial^2 u}{\partial x^2} &amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;u_{xx} = \frac{\partial^2 u}{\partial x^2} &amp;lt;/math&amp;gt;&lt;br /&gt;
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: &amp;lt;math&amp;gt;u_{xy} = \frac{\partial^2 u}{\partial y\, \partial x} = \frac{\partial}{\partial y } \left(\frac{\partial u}{\partial x}\right). &amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;u_{xy} = \frac{\partial^2 u}{\partial y\, \partial x} = \frac{\partial}{\partial y } \left(\frac{\partial u}{\partial x}\right). &amp;lt;/math&amp;gt;&lt;br /&gt;
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Especially in physics, [[del]] or nabla ({{math|∇}}) is often used to denote spatial derivatives, and {{math|''&amp;amp;#x307;u'', ''ü''}} for time derivatives. For example, the [[wave equation]] (mentioned below) can be written as&lt;br /&gt;
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Especially in physics, del or nabla () is often used to denote spatial derivatives, and  for time derivatives. For example, the wave equation (mentioned below) can be written as&lt;br /&gt;
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特别是在物理学中，[[del]]或nabla ({{math|∇}})经常用来表示空间导数和时间导数。例如，波动方程(在下文中提到)可以写成&lt;br /&gt;
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:&amp;lt;math&amp;gt;\ddot u=c^2\nabla^2u&amp;lt;/math&amp;gt;&lt;br /&gt;
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&amp;lt;math&amp;gt;\ddot u=c^2\nabla^2u&amp;lt;/math&amp;gt;&lt;br /&gt;
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or&lt;br /&gt;
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or&lt;br /&gt;
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或&lt;br /&gt;
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:&amp;lt;math&amp;gt;\ddot u=c^2\Delta u&amp;lt;/math&amp;gt;&lt;br /&gt;
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&amp;lt;math&amp;gt;\ddot u=c^2\Delta u&amp;lt;/math&amp;gt;&lt;br /&gt;
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where {{math|Δ}} is the [[Laplace operator]].&lt;br /&gt;
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where  is the Laplace operator.&lt;br /&gt;
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其中{{math|Δ}}代表拉普拉斯算子&lt;br /&gt;
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== Classification ==&lt;br /&gt;
分类&lt;br /&gt;
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Some linear, second-order partial differential equations can be classified as [[parabolic partial differential equation|parabolic]], [[hyperbolic partial differential equation|hyperbolic]] and [[elliptic partial differential equation|elliptic]]. Others, such as the [[Euler–Tricomi equation]], have different types in different regions. The classification provides a guide to appropriate initial and boundary conditions and to the smoothness of the solutions.&lt;br /&gt;
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Some linear, second-order partial differential equations can be classified as parabolic, hyperbolic and elliptic. Others, such as the Euler–Tricomi equation, have different types in different regions. The classification provides a guide to appropriate initial and boundary conditions and to the smoothness of the solutions.&lt;br /&gt;
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一些线性二阶偏微分方程可分为抛物型方程、双曲型方程和椭圆型方程。其他的方程，如欧拉-特里科米方程，在不同的区域有不同的类型。这种分类有助于选择适当的初始和边界条件以及提高解的平滑性。&lt;br /&gt;
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=== Equations of first order ===&lt;br /&gt;
一阶方程&lt;br /&gt;
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{{main|First-order partial differential equation}}&lt;br /&gt;
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=== Linear equations of second order ===&lt;br /&gt;
二阶线性方程&lt;br /&gt;
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Assuming {{math|''u&amp;lt;sub&amp;gt;xy&amp;lt;/sub&amp;gt;'' {{=}} ''u&amp;lt;sub&amp;gt;yx&amp;lt;/sub&amp;gt;''}}, the general linear second-order PDE in two independent variables has the form&lt;br /&gt;
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Assuming  u&amp;lt;sub&amp;gt;yx&amp;lt;/sub&amp;gt;}}, the general linear second-order PDE in two independent variables has the form&lt;br /&gt;
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假设 {{math|''u&amp;lt;sub&amp;gt;xy&amp;lt;/sub&amp;gt;'' {{=}} ''u&amp;lt;sub&amp;gt;yx&amp;lt;/sub&amp;gt;''}}，含有两个独立变量的一般的线性二阶偏微分方程具有如下这样的形式&lt;br /&gt;
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: &amp;lt;math&amp;gt;Au_{xx} + 2Bu_{xy} + Cu_{yy} + \cdots \mbox{(lower order terms)} = 0,&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;Au_{xx} + 2Bu_{xy} + Cu_{yy} + \cdots \mbox{(lower order terms)} = 0,&amp;lt;/math&amp;gt;&lt;br /&gt;
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where the coefficients {{mvar|A}}, {{mvar|B}}, {{mvar|C}}... may depend upon {{mvar|x}} and {{mvar|y}}. If {{math|''A''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; + ''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; + ''C''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; &amp;gt; 0}} over a region of the {{mvar|xy}}-plane, the PDE is second-order in that region. This form is analogous to the equation for a conic section:&lt;br /&gt;
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where the coefficients , , ... may depend upon  and . If  over a region of the -plane, the PDE is second-order in that region. This form is analogous to the equation for a conic section:&lt;br /&gt;
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其中的系数 {{mvar|A}}, {{mvar|B}}, {{mvar|C}}... 一般取决于{{mvar|x}}和{{mvar|y}}。如果在{{mvar|xy}}-平面的一个区域上 {{math|''A''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; + ''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; + ''C''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; &amp;gt; 0}}，偏微分方程在该区域是二阶的。这种形式类似于圆锥曲线的方程:&lt;br /&gt;
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: &amp;lt;math&amp;gt;Ax^2 + 2Bxy + Cy^2 + \cdots = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;Ax^2 + 2Bxy + Cy^2 + \cdots = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
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More precisely, replacing {{math|∂&amp;lt;sub&amp;gt;''x''&amp;lt;/sub&amp;gt;}} by {{mvar|X}}, and likewise for other variables (formally this is done by a [[Fourier transform]]), converts a constant-coefficient PDE into a polynomial of the same degree, with the terms of the highest degree (a [[homogeneous polynomial]], here a [[quadratic form]]) being most significant for the classification.&lt;br /&gt;
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More precisely, replacing  by , and likewise for other variables (formally this is done by a Fourier transform), converts a constant-coefficient PDE into a polynomial of the same degree, with the terms of the highest degree (a homogeneous polynomial, here a quadratic form) being most significant for the classification.&lt;br /&gt;
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更准确地说，用 {{mvar|X}} 替换 {{math|∂&amp;lt;sub&amp;gt;''x''&amp;lt;/sub&amp;gt;}}，对于其他变量做同样的操作(从形式上来说，这是由傅里叶变换来完成的)，将一个常系数偏微分方程转换成一个相同次数的多项式，最高次数的项(齐次多项式，这里是一个二次形式)一般会用于偏微分方程的分类。&lt;br /&gt;
===~~ most significant for the classification 意译为用于偏微分方程的分类。       significiant直译过来感觉不太合适&lt;br /&gt;
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Just as one classifies [[conic section]]s and quadratic forms into parabolic, hyperbolic, and elliptic based on the [[discriminant]] {{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − 4''AC''}}, the same can be done for a second-order PDE at a given point.  However, the [[discriminant]] in a PDE is given by {{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC''}} due to the convention of the {{mvar|xy}} term being {{math|2''B''}} rather than {{mvar|B}}; formally, the discriminant (of the associated quadratic form) is {{math|(2''B'')&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − 4''AC'' {{=}} 4(''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC'')}}, with the factor of 4 dropped for simplicity.&lt;br /&gt;
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Just as one classifies conic sections and quadratic forms into parabolic, hyperbolic, and elliptic based on the discriminant , the same can be done for a second-order PDE at a given point.  However, the discriminant in a PDE is given by  due to the convention of the  term being  rather than ; formally, the discriminant (of the associated quadratic form) is  4(B&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − AC)}}, with the factor of 4 dropped for simplicity.&lt;br /&gt;
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正如人们可以根据判别式 {{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − 4''AC''}} 将圆锥曲线和二次型分为抛物型、双曲型和椭圆型一样，对于给定点的二阶偏微分方程也可以这样做。然而，偏微分方程中的判别式 {{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − 4''AC''}} 是根据交叉项的系数{{math|2''B''}} 而不是 {{mvar|B}} 给出的，形式上，判别式(关联二次型)是 {{math|(2''B'')&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − 4''AC'' {{=}} 4(''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC'')}}，为简单起见，去掉了因子4。&lt;br /&gt;
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# {{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC'' &amp;lt; 0}} (''[[elliptic partial differential equation]]''): Solutions of [[elliptic partial differential equation|elliptic PDEs]] are as smooth as the coefficients allow, within the interior of the region where the equation and solutions are defined. For example, solutions of [[Laplace's equation]] are analytic within the domain where they are defined, but solutions may assume boundary values that are not smooth. The motion of a fluid at subsonic speeds can be approximated with elliptic PDEs, and the Euler–Tricomi equation is elliptic where {{math|''x'' &amp;lt; 0}}.&lt;br /&gt;
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  (elliptic partial differential equation): Solutions of elliptic PDEs are as smooth as the coefficients allow, within the interior of the region where the equation and solutions are defined. For example, solutions of Laplace's equation are analytic within the domain where they are defined, but solutions may assume boundary values that are not smooth. The motion of a fluid at subsonic speeds can be approximated with elliptic PDEs, and the Euler–Tricomi equation is elliptic where .&lt;br /&gt;
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{{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC'' &amp;lt; 0}} (椭圆形微分方程)：在定义方程和解的区域内部，椭圆型偏微分方程的解光滑到系数允许的程度。例如，拉普拉斯方程的解在它们被定义的区域内是解析的，但是解可能假设边界值是不光滑的。亚音速流体的运动可以用椭圆偏微分方程近似，其中欧拉-特里科米方程在 {{math|''x'' &amp;lt; 0}} 时是椭圆型偏微分方程。&lt;br /&gt;
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# {{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC'' {{=}} 0}} (''[[parabolic partial differential equation]]''): Equations that are [[parabolic partial differential equation|parabolic]] at every point can be transformed into a form analogous to the [[heat equation]] by a change of independent variables. Solutions smooth out as the transformed time variable increases. The Euler–Tricomi equation has parabolic type on the line where {{math|''x'' {{=}} 0}}.&lt;br /&gt;
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  0}} (parabolic partial differential equation): Equations that are parabolic at every point can be transformed into a form analogous to the heat equation by a change of independent variables. Solutions smooth out as the transformed time variable increases. The Euler–Tricomi equation has parabolic type on the line where  0}}.&lt;br /&gt;
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{{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC'' {{=}} 0}}（抛物线形偏微分方程）：在每一点上都是抛物线型的方程可以通过改变自变量从而转化成类似于热方程的形式。随着转换后的时间变量的增加，方程的解变得平滑。欧拉-特里科米方程在 {{math|''x'' {{=}} 0}} 这条特征线上是抛物线形的。&lt;br /&gt;
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# {{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC'' &amp;gt; 0}} (''[[hyperbolic partial differential equation]]''): [[hyperbolic partial differential equation|hyperbolic]] equations retain any discontinuities of functions or derivatives in the initial data. An example is the [[wave equation]]. The motion of a fluid at supersonic speeds can be approximated with hyperbolic PDEs, and the Euler–Tricomi equation is hyperbolic where {{math|''x'' &amp;gt; 0}}.&lt;br /&gt;
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  (hyperbolic partial differential equation): hyperbolic equations retain any discontinuities of functions or derivatives in the initial data. An example is the wave equation. The motion of a fluid at supersonic speeds can be approximated with hyperbolic PDEs, and the Euler–Tricomi equation is hyperbolic where .&lt;br /&gt;
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{{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC'' &amp;gt; 0}} (双曲形偏微分方程)：双曲形方程在初始数据中保留了函数或导数的任何不连续性，波动方程就是其中的一个例子。超音速流体的运动可以用双曲形偏微分方程近似，其中欧拉-特里科米方程在 {{math|''x'' &amp;gt; 0}} 时是双曲型的。&lt;br /&gt;
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If there are {{mvar|n}} independent variables {{math|''x''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;, ''x''&amp;lt;sub&amp;gt;2 &amp;lt;/sub&amp;gt;,… ''x''&amp;lt;sub&amp;gt;''n''&amp;lt;/sub&amp;gt;}}, a general linear partial differential equation of second order has the form&lt;br /&gt;
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If there are  independent variables , a general linear partial differential equation of second order has the form&lt;br /&gt;
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如果存在 {{mvar|n}} 个自变量 {{math|''x''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;, ''x''&amp;lt;sub&amp;gt;2 &amp;lt;/sub&amp;gt;,… ''x''&amp;lt;sub&amp;gt;''n''&amp;lt;/sub&amp;gt;}}，一般二阶线性偏微分方程的形式是&lt;br /&gt;
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: &amp;lt;math&amp;gt;L u =\sum_{i=1}^n\sum_{j=1}^n a_{i,j} \frac{\partial^2 u}{\partial x_i \partial x_j} \quad \text{ plus lower-order terms} =0.&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;L u =\sum_{i=1}^n\sum_{j=1}^n a_{i,j} \frac{\partial^2 u}{\partial x_i \partial x_j} \quad \text{ plus lower-order terms} =0.&amp;lt;/math&amp;gt;&lt;br /&gt;
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The classification depends upon the signature of the eigenvalues of the coefficient matrix {{math|''a''&amp;lt;sub&amp;gt;''i'',''j''&amp;lt;/sub&amp;gt;}}.&lt;br /&gt;
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The classification depends upon the signature of the eigenvalues of the coefficient matrix .&lt;br /&gt;
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这种分类取决于系数矩阵本征值的符号（正负性）。&lt;br /&gt;
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# Elliptic: the eigenvalues are all positive or all negative.&lt;br /&gt;
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 Elliptic: the eigenvalues are all positive or all negative.&lt;br /&gt;
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椭圆形方程: 本征值全部为正或全部为负。&lt;br /&gt;
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# Parabolic: the eigenvalues are all positive or all negative, save one that is zero.&lt;br /&gt;
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 Parabolic: the eigenvalues are all positive or all negative, save one that is zero.&lt;br /&gt;
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抛物线形方程: 本征值全部为正或全部为负，除了一个为零。&lt;br /&gt;
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# Hyperbolic: there is only one negative eigenvalue and all the rest are positive, or there is only one positive eigenvalue and all the rest are negative.&lt;br /&gt;
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 Hyperbolic: there is only one negative eigenvalue and all the rest are positive, or there is only one positive eigenvalue and all the rest are negative.&lt;br /&gt;
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双曲形方程: 只有一个负特征值，其余的都是正特征值，或者只有一个正特征值，其余的都是负特征值。&lt;br /&gt;
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# Ultrahyperbolic: there is more than one positive eigenvalue and more than one negative eigenvalue, and there are no zero eigenvalues. There is only a limited theory for ultrahyperbolic equations (Courant and Hilbert, 1962).&lt;br /&gt;
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 Ultrahyperbolic: there is more than one positive eigenvalue and more than one negative eigenvalue, and there are no zero eigenvalues. There is only a limited theory for ultrahyperbolic equations (Courant and Hilbert, 1962).&lt;br /&gt;
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超双形方程: 存在多于一个正本征值和多于一个的负本征值，且不存在零本征值。对于超双曲方程，只存在一个有限理论(Courant 和 Hilbert，1962)。&lt;br /&gt;
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==[[用户:Yuling|Yuling]]（[[用户讨论:Yuling|讨论]]） 我对于limited theory这个单词对应的相关理论不太了解。&lt;br /&gt;
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=== Systems of first-order equations and characteristic surfaces ===&lt;br /&gt;
一阶方程组和特征曲面&lt;br /&gt;
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The classification of partial differential equations can be extended to systems of first-order equations, where the unknown {{mvar|u}} is now a [[Euclidean vector|vector]] with {{mvar|m}} components, and the coefficient matrices {{mvar|A&amp;lt;sub&amp;gt;ν&amp;lt;/sub&amp;gt;}} are {{mvar|m}} by {{mvar|m}} matrices for {{math|''ν'' {{=}} 1, 2,… ''n''}}. The partial differential equation takes the form&lt;br /&gt;
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The classification of partial differential equations can be extended to systems of first-order equations, where the unknown  is now a vector with  components, and the coefficient matrices  are  by  matrices for  1, 2,… n}}. The partial differential equation takes the form&lt;br /&gt;
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偏微分方程组的分类可以推广到一阶方程组，其中未知量 {{mvar|u}} 是有 {{mvar|m}} 个分量的向量。对于 {{math|''ν'' {{=}} 1, 2,… ''n''}}，系数矩阵 {{mvar|A&amp;lt;sub&amp;gt;ν&amp;lt;/sub&amp;gt;}} 是 {{mvar|m}} × {{mvar|m}} 的矩阵。偏微分方程形式如下：&lt;br /&gt;
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: &amp;lt;math&amp;gt;Lu = \sum_{\nu=1}^{n} A_\nu \frac{\partial u}{\partial x_\nu} + B=0,&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;Lu = \sum_{\nu=1}^{n} A_\nu \frac{\partial u}{\partial x_\nu} + B=0,&amp;lt;/math&amp;gt;&lt;br /&gt;
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where the coefficient matrices {{mvar|A&amp;lt;sub&amp;gt;ν&amp;lt;/sub&amp;gt;}} and the vector {{mvar|B}} may depend upon {{mvar|x}} and {{mvar|u}}. If a [[hypersurface]] {{mvar|S}} is given in the implicit form&lt;br /&gt;
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where the coefficient matrices  and the vector  may depend upon  and . If a hypersurface  is given in the implicit form&lt;br /&gt;
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其中系数矩阵 {{mvar|A&amp;lt;sub&amp;gt;ν&amp;lt;/sub&amp;gt;}} 和向量 {{mvar|B}} 可能依赖于 {{mvar|x}} 和 {{mvar|u}}。如果超曲面是以隐式形式给出的&lt;br /&gt;
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: &amp;lt;math&amp;gt;\varphi(x_1, x_2, \ldots x_n)=0,&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;\varphi(x_1, x_2, \ldots x_n)=0,&amp;lt;/math&amp;gt;&lt;br /&gt;
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where {{mvar|φ}} has a non-zero gradient, then {{mvar|S}} is a '''characteristic surface''' for the operator {{mvar|L}} at a given point if the characteristic form vanishes:&lt;br /&gt;
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where  has a non-zero gradient, then  is a characteristic surface for the operator  at a given point if the characteristic form vanishes:&lt;br /&gt;
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其中存在一个非零的梯度，那么如果特征形式消失，则在给定点上算子的特征曲面形式如下:&lt;br /&gt;
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: &amp;lt;math&amp;gt;Q\left(\frac{\partial\varphi}{\partial x_1}, \ldots\frac{\partial\varphi}{\partial x_n}\right) =\det\left[\sum_{\nu=1}^nA_\nu \frac{\partial \varphi}{\partial x_\nu}\right]=0.\,&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;Q\left(\frac{\partial\varphi}{\partial x_1}, \ldots\frac{\partial\varphi}{\partial x_n}\right) =\det\left[\sum_{\nu=1}^nA_\nu \frac{\partial \varphi}{\partial x_\nu}\right]=0.\,&amp;lt;/math&amp;gt;&lt;br /&gt;
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The geometric interpretation of this condition is as follows: if data for {{mvar|u}} are prescribed on the surface {{mvar|S}}, then it may be possible to determine the normal derivative of {{mvar|u}} on {{mvar|S}} from the differential equation. If the data on {{mvar|S}} and the differential equation determine the normal derivative of {{mvar|u}} on {{mvar|S}}, then {{mvar|S}} is non-characteristic. If the data on {{mvar|S}} and the differential equation ''do not'' determine the normal derivative of {{mvar|u}} on {{mvar|S}}, then the surface is '''characteristic''', and the differential equation restricts the data on {{mvar|S}}: the differential equation is ''internal'' to {{mvar|S}}.&lt;br /&gt;
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The geometric interpretation of this condition is as follows: if data for  are prescribed on the surface , then it may be possible to determine the normal derivative of  on  from the differential equation. If the data on  and the differential equation determine the normal derivative of  on , then  is non-characteristic. If the data on  and the differential equation do not determine the normal derivative of  on , then the surface is characteristic, and the differential equation restricts the data on : the differential equation is internal to .&lt;br /&gt;
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这个条件的几何解释如下: 如果关于 {{mvar|u}} 的数据是在曲面 {{mvar|S}} 上规定的，那么就有可能依据微分方程确定曲面 {{mvar|S}} 上 {{mvar|u}} 的法向导数。如果曲面 {{mvar|S}} 上的数据和上面的微分方程能确定曲面 {{mvar|S}} 上 {{mvar|u}} 的法向导数，那么它就是非特征的。如果曲面 {{mvar|S}} 上的数据和上面的微分方程不能确定曲面 {{mvar|S}} 上 {{mvar|u}} 的法向导数，那么曲面是特征的，并且微分方程将数据限制在曲面 {{mvar|S}} 上：微分方程是在曲面 {{mvar|S}} 内部。&lt;br /&gt;
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# A first-order system {{math|''Lu'' {{=}} 0}} is ''elliptic'' if no surface is characteristic for {{mvar|L}}: the values of {{mvar|u}} on {{mvar|S}} and the differential equation always determine the normal derivative of {{mvar|u}} on {{mvar|S}}.&lt;br /&gt;
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 A first-order system  0}} is elliptic if no surface is characteristic for : the values of  on  and the differential equation always determine the normal derivative of  on .&lt;br /&gt;
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如果对于 {{mvar|L}} 没有曲面是特征的，则一阶系统 {{math|''Lu'' {{=}} 0}} 是椭圆形的：{{mvar|u}}在 {{mvar|S}} 的值和微分方程总能够决定 {{mvar|S}} 上 {{mvar|u}} 的法向导数。&lt;br /&gt;
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# A first-order system is ''hyperbolic'' at a point if there is a '''spacelike''' surface {{mvar|S}} with normal {{mvar|ξ}} at that point. This means that, given any non-trivial vector {{mvar|η}} orthogonal to {{mvar|ξ}}, and a scalar multiplier {{mvar|λ}}, the equation {{math|''Q''(''λξ'' + ''η'') {{=}} 0}} has {{mvar|m}} real roots {{math|''λ''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;, ''λ''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;,… ''λ''&amp;lt;sub&amp;gt;''m''&amp;lt;/sub&amp;gt;}}. The system is '''strictly hyperbolic''' if these roots are always distinct. The geometrical interpretation of this condition is as follows: the characteristic form {{math|''Q''(''ζ'') {{=}} 0}} defines a cone (the normal cone) with homogeneous coordinates ζ. In the hyperbolic case, this cone has {{mvar|m}} sheets, and the axis {{math|''ζ'' {{=}} ''λξ''}} runs inside these sheets: it does not intersect any of them. But when displaced from the origin by η, this axis intersects every sheet. In the elliptic case, the normal cone has no real sheets.&lt;br /&gt;
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 A first-order system is hyperbolic at a point if there is a spacelike surface  with normal  at that point. This means that, given any non-trivial vector  orthogonal to , and a scalar multiplier , the equation  0}} has  real roots . The system is strictly hyperbolic if these roots are always distinct. The geometrical interpretation of this condition is as follows: the characteristic form  0}} defines a cone (the normal cone) with homogeneous coordinates ζ. In the hyperbolic case, this cone has  sheets, and the axis  λξ}} runs inside these sheets: it does not intersect any of them. But when displaced from the origin by η, this axis intersects every sheet. In the elliptic case, the normal cone has no real sheets.&lt;br /&gt;
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如果在该点存在一个法向量为 {{mvar|ξ}}的 '''&amp;lt;font color=&amp;quot;#ff8000&amp;quot;&amp;gt;类空曲面 Spacclike Surface&amp;lt;/font&amp;gt; {{mvar|S}} ，则一阶系统在那一点是双曲的。这意味着，给定任意正交于 {{mvar|ξ}} 的非平凡向量 {{mvar|η}} 和一个标量乘子 {{mvar|λ}}，方程 {{math|''Q''(''λξ'' + ''η'') {{=}} 0}} 有 {{mvar|m}} 个实根 {{math|''λ''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;, ''λ''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;,… ''λ''&amp;lt;sub&amp;gt;''m''&amp;lt;/sub&amp;gt;}}。如果这些根始终不同，则该系统是严格双曲形的。这个条件的几何解释如下: 特征形式 {{math|''Q''(''ζ'') {{=}} 0}} 定义了一个具有齐次坐标 ζ的圆锥(法线圆锥)。在双曲形的情况下，这个圆锥体有 {{mvar|m}} 层，并且轴 {{math|''ζ'' {{=}} ''λξ''}} 在这些层中运动: 它不与任何一层相交。但是当从原点偏离η时，这条轴线与每一层都相交。在椭圆形的情况下，法向圆锥没有实层。&lt;br /&gt;
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==[[用户:Yuling|Yuling]]（[[用户讨论:Yuling|讨论]]） sheet 这个单词也不很理解，我直译为了“层”&lt;br /&gt;
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=== Equations of mixed type ===&lt;br /&gt;
混合型方程&lt;br /&gt;
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If a PDE has coefficients that are not constant, it is possible that it will not belong to any of these categories but rather be of '''mixed type'''. A simple but important example is the [[Euler–Tricomi equation]]&lt;br /&gt;
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If a PDE has coefficients that are not constant, it is possible that it will not belong to any of these categories but rather be of mixed type. A simple but important example is the Euler–Tricomi equation&lt;br /&gt;
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如果偏微分方程的系数不是常数，那么它可能不属于这些类别中的任何一个，而是属于混合类型。一个简单但重要的例子是欧拉-特里科米方程&lt;br /&gt;
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: &amp;lt;math&amp;gt;u_{xx} = xu_{yy},&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;u_{xx} = xu_{yy},&amp;lt;/math&amp;gt;&lt;br /&gt;
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which is called '''elliptic-hyperbolic''' because it is elliptic in the region {{math|''x'' &amp;lt; 0}}, hyperbolic in the region {{math|''x'' &amp;gt; 0}}, and degenerate parabolic on the line {{math|''x'' {{=}} 0}}.&lt;br /&gt;
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which is called elliptic-hyperbolic because it is elliptic in the region , hyperbolic in the region , and degenerate parabolic on the line  0}}.&lt;br /&gt;
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它在 {{math|''x'' &amp;lt; 0}} 的区域上是椭圆形，在 {{math|''x'' &amp;gt; 0}} 区域上是双曲形，在 {{math|''x'' {{=}} 0}}这条线上是退化为抛物线形，因此称之为椭圆-双曲型。&lt;br /&gt;
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''fill in: Dirichlet and Neumann boundaries, hyperbolic/parabolic/elliptic separation of variables, [[Fourier analysis]], [[Green's function]]s ...--&amp;gt;&lt;br /&gt;
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fill in: Dirichlet and Neumann boundaries, hyperbolic/parabolic/elliptic separation of variables, Fourier analysis, Green's functions ...--&amp;gt;&lt;br /&gt;
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填写: Dirichlet 和 Neumann 边界，双曲 / 抛物线 / 椭圆分离变量法，傅立叶分析，Green 函数... --&lt;br /&gt;
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=== Infinite-order PDEs in quantum mechanics ===&lt;br /&gt;
量子力学中的无限阶偏微分方程&lt;br /&gt;
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In the [[phase space formulation]] of quantum mechanics,  one may consider the [[Method of quantum characteristics|quantum Hamilton's equations]] for trajectories of quantum particles. These equations are infinite-order PDEs. However, in the semiclassical expansion, one has a finite system of ODEs at any fixed order of [[Dirac constant|{{mvar|ħ}}]].  The evolution equation of the [[Wigner quasi-probability distribution|c]] is also an infinite-order PDE. The quantum trajectories are [[Method of quantum characteristics|quantum characteristics]], with the use of which one could calculate the evolution of the Wigner function.&lt;br /&gt;
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In the phase space formulation of quantum mechanics,  one may consider the quantum Hamilton's equations for trajectories of quantum particles. These equations are infinite-order PDEs. However, in the semiclassical expansion, one has a finite system of ODEs at any fixed order of Dirac constant|.  The evolution equation of the Wigner function is also an infinite-order PDE. The quantum trajectories are quantum characteristics, with the use of which one could calculate the evolution of the Wigner function.&lt;br /&gt;
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在量子力学中的相空间表述中，我们可以考虑用于求解量子粒子的轨迹的量子哈密顿的方程。这些方程是无限阶偏微分方程。然而，在半经典展开中，我们在给定[[Dirac constant|{{mvar|ħ}}]]阶数下有一个有限的的常微分方程组。'''&amp;lt;font color=&amp;quot;#ff8000&amp;quot;&amp;gt;维格纳函数  Wigner Function&amp;lt;/font&amp;gt;的演化方程也是一个无限阶偏微分方程。由于量子轨道的量子特性，所以它通常可以用来计算维格纳函数的演化。&lt;br /&gt;
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== Analytical solutions ==&lt;br /&gt;
解析解&lt;br /&gt;
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===Separation of variables===&lt;br /&gt;
分离变量法&lt;br /&gt;
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{{main|Separable partial differential equation}}&lt;br /&gt;
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Linear PDEs can be reduced to systems of ordinary differential equations by the important technique of separation of variables. This technique rests on a characteristic of solutions to differential equations: if one can find any solution that solves the equation and satisfies the boundary conditions, then it is ''the'' solution (this also applies to ODEs). We assume as an [[ansatz]] that the dependence of a solution on the parameters space and time can be written as a product of terms that each depend on a single parameter, and then see if this can be made to solve the problem.&amp;lt;ref&amp;gt;{{cite book|last1=Gershenfeld|first1=Neil|title=The nature of mathematical modeling|date=2000|publisher=Cambridge Univ. Press|location=Cambridge|isbn=0521570956|page=27|edition=Reprinted (with corr.)}}&amp;lt;/ref&amp;gt;&lt;br /&gt;
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Linear PDEs can be reduced to systems of ordinary differential equations by the important technique of separation of variables. This technique rests on a characteristic of solutions to differential equations: if one can find any solution that solves the equation and satisfies the boundary conditions, then it is the solution (this also applies to ODEs). We assume as an ansatz that the dependence of a solution on the parameters space and time can be written as a product of terms that each depend on a single parameter, and then see if this can be made to solve the problem.&lt;br /&gt;
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线性偏微分方程组可以通过分离变量法这一重要方法来简化为常微分方程组。这种方法依赖于微分方程解的一个特征: 如果能找到任何一个满足方程和边界条件的解，那么这个解就是方程的解(这也适用于常微分方程)。我们假设解对参数空间和时间的依赖可以写成对它们每一项的依赖以及一个参数的乘积，然后再看看这是否可以用来解决这个问题。&lt;br /&gt;
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In the method of separation of variables, one reduces a PDE to a PDE in fewer variables, which is an ordinary differential equation if in one variable – these are in turn easier to solve.&lt;br /&gt;
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In the method of separation of variables, one reduces a PDE to a PDE in fewer variables, which is an ordinary differential equation if in one variable – these are in turn easier to solve.&lt;br /&gt;
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在分离变量法方法中，可以将偏微分方程简化为含有更少变量的偏微分方程，如果只有一个变量，那么就变成了一个'''&amp;lt;font color = &amp;quot;#ff8000&amp;quot;&amp;gt;常微分方程 Ordinary Differential Equation&amp;lt;/font&amp;gt;'''-- 反过来，这些方程也更容易求解。&lt;br /&gt;
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This is possible for simple PDEs, which are called [[separable partial differential equation]]s, and the domain is generally a rectangle (a product of intervals). Separable PDEs correspond to [[diagonal matrices]] – thinking of &amp;quot;the value for fixed {{mvar|x}}&amp;quot; as a coordinate, each coordinate can be understood separately.&lt;br /&gt;
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This is possible for simple PDEs, which are called separable partial differential equations, and the domain is generally a rectangle (a product of intervals). Separable PDEs correspond to diagonal matrices – thinking of &amp;quot;the value for fixed &amp;quot; as a coordinate, each coordinate can be understood separately.&lt;br /&gt;
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对于简单的偏微分方程(称为可分离偏微分方程)来说，这是可能的，而且方程通常定义在一个矩形区域(区间的乘积)上。可分离偏微分方程对应于对角线矩阵——以“固定值”为坐标，每个坐标可分开理解。&lt;br /&gt;
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This generalizes to the [[method of characteristics]], and is also used in [[integral transform]]s.&lt;br /&gt;
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This generalizes to the method of characteristics, and is also used in integral transforms.&lt;br /&gt;
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这种方法可以推广到特征曲线法，也可以用于积分变换。&lt;br /&gt;
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===Method of characteristics===&lt;br /&gt;
特征曲线法&lt;br /&gt;
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{{main|Method of characteristics}}&lt;br /&gt;
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In special cases, one can find characteristic curves on which the equation reduces to an ODE – changing coordinates in the domain to straighten these curves allows separation of variables, and is called the [[method of characteristics]].&lt;br /&gt;
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In special cases, one can find characteristic curves on which the equation reduces to an ODE – changing coordinates in the domain to straighten these curves allows separation of variables, and is called the method of characteristics.&lt;br /&gt;
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在特殊情况下，可以找到一些特征曲线，在这些曲线上方程可以变成一个常微分方程——意味着改变坐标从而使这些曲线变直从而达到分离变量的目的，这就是所谓的特征曲线法。&lt;br /&gt;
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More generally, one may find characteristic surfaces.&lt;br /&gt;
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More generally, one may find characteristic surfaces.&lt;br /&gt;
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更一般地说，人们可能会找到特征表面。&lt;br /&gt;
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===Integral transform===&lt;br /&gt;
积分变换&lt;br /&gt;
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An [[integral transform]] may transform the PDE to a simpler one, in particular, a separable PDE. This corresponds to diagonalizing an operator.&lt;br /&gt;
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An integral transform may transform the PDE to a simpler one, in particular, a separable PDE. This corresponds to diagonalizing an operator.&lt;br /&gt;
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积分变换可以将偏微分方程转换为更简单的偏微分方程，特别是可分离的偏微分方程。这对应于对角化算符。&lt;br /&gt;
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An important example of this is [[Fourier analysis]], which diagonalizes the heat equation using the [[eigenbasis]] of sinusoidal waves.&lt;br /&gt;
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An important example of this is Fourier analysis, which diagonalizes the heat equation using the eigenbasis of sinusoidal waves.&lt;br /&gt;
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这方面的一个重要例子是'''&amp;lt;font color = &amp;quot;#ff8000&amp;quot;&amp;gt;傅里叶分析  Fourier Analysis&amp;lt;/font&amp;gt;'''，它使用正弦波的特征基来对角化热方程。&lt;br /&gt;
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If the domain is finite or periodic, an infinite sum of solutions such as a [[Fourier series]] is appropriate, but an integral of solutions such as a [[Fourier integral]] is generally required for infinite domains. The solution for a point source for the heat equation given above is an example of the use of a Fourier integral.&lt;br /&gt;
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If the domain is finite or periodic, an infinite sum of solutions such as a Fourier series is appropriate, but an integral of solutions such as a Fourier integral is generally required for infinite domains. The solution for a point source for the heat equation given above is an example of the use of a Fourier integral.&lt;br /&gt;
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如果区域是有限的或周期性的，那么解为无限和的形式是恰当的，例如傅里叶级数，但是一个解的积分，例如傅立叶积分，一般是在无限区域上的。上面给出的热传导方程的点源解法就是使用傅里叶积分的一个例子。&lt;br /&gt;
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===Change of variables===&lt;br /&gt;
变量代换&lt;br /&gt;
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Often a PDE can be reduced to a simpler form with a known solution by a suitable [[Change of variables (PDE)|change of variables]].  For example, the [[Black–Scholes equation#Derivation|Black–Scholes]] PDE&lt;br /&gt;
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Often a PDE can be reduced to a simpler form with a known solution by a suitable change of variables.  For example, the Black–Scholes PDE&lt;br /&gt;
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偏微分方程通常可以通过变量的适当变化，用已知的解简化为更简单的形式。例如，布莱克-舒尔斯偏微分方程&lt;br /&gt;
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:&amp;lt;math&amp;gt; \frac{\partial V}{\partial t} + \tfrac{1}{2}\sigma^2 S^2\frac{\partial^2 V}{\partial S^2} + rS\frac{\partial V}{\partial S} - rV = 0 &amp;lt;/math&amp;gt;&lt;br /&gt;
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&amp;lt;math&amp;gt; \frac{\partial V}{\partial t} + \tfrac{1}{2}\sigma^2 S^2\frac{\partial^2 V}{\partial S^2} + rS\frac{\partial V}{\partial S} - rV = 0 &amp;lt;/math&amp;gt;&lt;br /&gt;
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is reducible to the [[heat equation]]&lt;br /&gt;
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is reducible to the heat equation&lt;br /&gt;
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可以简化为热传导方程&lt;br /&gt;
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:&amp;lt;math&amp;gt; \frac{\partial u}{\partial \tau} = \frac{\partial^2 u}{\partial x^2}&amp;lt;/math&amp;gt;&lt;br /&gt;
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&amp;lt;math&amp;gt; \frac{\partial u}{\partial \tau} = \frac{\partial^2 u}{\partial x^2}&amp;lt;/math&amp;gt;&lt;br /&gt;
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by the change of variables (for complete details see {{webarchive |url=https://web.archive.org/web/20080411030405/http://www.math.unl.edu/~sdunbar1/Teaching/MathematicalFinance/Lessons/BlackScholes/Solution/solution.shtml |date=April 11, 2008 |title=Solution of the Black Scholes Equation }})&lt;br /&gt;
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by the change of variables (for complete details see )&lt;br /&gt;
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通过变量替换(完整的细节见)&lt;br /&gt;
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:&amp;lt;math&amp;gt;\begin{align}&lt;br /&gt;
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V(S,t) &amp;amp;= K v(x,\tau),\\[5px]&lt;br /&gt;
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x &amp;amp;= \ln\left(\tfrac{S}{K} \right),\\[5px]&lt;br /&gt;
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\tau &amp;amp;= \tfrac{1}{2} \sigma^2 (T - t),\\[5px]&lt;br /&gt;
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v(x,\tau)&amp;amp;=e^{-\alpha x-\beta\tau} u(x,\tau).&lt;br /&gt;
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\end{align}&amp;lt;/math&amp;gt;&lt;br /&gt;
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===Fundamental solution===&lt;br /&gt;
基本解&lt;br /&gt;
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{{main|Fundamental solution}}&lt;br /&gt;
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Inhomogeneous equations can often be solved (for constant coefficient PDEs, always be solved) by finding the [[fundamental solution]] (the solution for a point source), then taking the [[convolution]] with the boundary conditions to get the solution.&lt;br /&gt;
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Inhomogeneous equations can often be solved (for constant coefficient PDEs, always be solved) by finding the fundamental solution (the solution for a point source), then taking the convolution with the boundary conditions to get the solution.&lt;br /&gt;
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非齐次方程(常系数偏微分方程)一般是通过先求出基本解(点源的解) ，然后利用带边界条件的卷积来求解。&lt;br /&gt;
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This is analogous in [[signal processing]] to understanding a filter by its [[impulse response]].&lt;br /&gt;
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This is analogous in signal processing to understanding a filter by its impulse response.&lt;br /&gt;
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这类似于在信号处理中通过滤波器的脉冲响应来理解滤波器。&lt;br /&gt;
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===Superposition principle===&lt;br /&gt;
叠加原理&lt;br /&gt;
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{{further| Superposition principle }}&lt;br /&gt;
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The superposition principle applies to any linear system, including linear systems of PDEs. A common visualization of this concept is the interaction of two waves in phase being combined to result in a greater amplitude, for example {{math|sin ''x'' + sin ''x'' {{=}} 2 sin ''x''}}. The same principle can be observed in PDEs where the solutions may be real or complex and additive. [[Superposition principle|superposition]]&lt;br /&gt;
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The superposition principle applies to any linear system, including linear systems of PDEs. A common visualization of this concept is the interaction of two waves in phase being combined to result in a greater amplitude, for example  2 sin x}}. The same principle can be observed in PDEs where the solutions may be real or complex and additive. superposition&lt;br /&gt;
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'''&amp;lt;font color = &amp;quot;#ff8000&amp;quot;&amp;gt;叠加原理 Superposition Principle&amp;lt;/font&amp;gt;适用于任何线性系统，包括偏微分方程的线性系统。这个概念的一个常见的可视化是两个同相位的波相互作用结合在一起会产生更大的振幅，例如 {{math|sin ''x'' + sin ''x'' {{=}} 2 sin ''x''}}。在偏微分方程中也可以观察到同样的原理，其中的解可能是真实的或复杂的和可加的。叠加&lt;br /&gt;
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If {{math|''u''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;}} and {{math|''u''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;}} are solutions of linear PDE in some function space {{mvar|R}}, then {{math|''u'' {{=}} ''c''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;''u''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; + ''c''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;''u''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;}} with any constants {{math|''c''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;}} and {{math|''c''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;}} are also a solution of that PDE in the same function space.&lt;br /&gt;
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If  and  are solutions of linear PDE in some function space , then  c&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;u&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; + c&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;u&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;}} with any constants  and  are also a solution of that PDE in the same function space.&lt;br /&gt;
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若线性偏微分方程在某个函数空间{{mvar|R}}中有解{{math|''u''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;}} 和 {{math|''u''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;}}，则{{math|''u'' {{=}} ''c''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;''u''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; + ''c''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;''u''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;}}也是该偏微分方程在同一函数空间中的解，其中{{math|''c''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;}} 和 {{math|''c''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;}} 是任意常数。&lt;br /&gt;
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===Methods for non-linear equations===&lt;br /&gt;
非线性方程的求解方法&lt;br /&gt;
{{see also|nonlinear partial differential equation}}&lt;br /&gt;
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There are no generally applicable methods to solve nonlinear PDEs. Still, existence and uniqueness results (such as the [[Cauchy–Kowalevski theorem]]) are often possible, as are proofs of important qualitative and quantitative properties of solutions (getting these results is a major part of [[mathematical analysis|analysis]]). Computational solution to the nonlinear PDEs, the [[split-step method]], exist for specific equations like [[nonlinear Schrödinger equation]].&lt;br /&gt;
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There are no generally applicable methods to solve nonlinear PDEs. Still, existence and uniqueness results (such as the Cauchy–Kowalevski theorem) are often possible, as are proofs of important qualitative and quantitative properties of solutions (getting these results is a major part of analysis). Computational solution to the nonlinear PDEs, the split-step method, exist for specific equations like nonlinear Schrödinger equation.&lt;br /&gt;
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对于非线性偏微分方程，目前还没有普遍适用的求解方法。然而，通常是可能知道解的存在性和唯一性(如柯西-科瓦列夫斯基定理)，也是可能得到解的重要定性和定量性质的证明(得到这些结果是分析的主要部分)。非线性偏微分方程的计算解，即分步法，对一些特定的方程适用，比如非线性'''&amp;lt;font color=&amp;quot;#ff8000&amp;quot;&amp;gt;薛定谔方程 Schrödinger equation&amp;lt;/font&amp;gt;'''。&lt;br /&gt;
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Nevertheless, some techniques can be used for several types of equations. The [[h-principle|{{mvar|h}}-principle]] is the most powerful method to solve [[Underdetermined system|underdetermined]] equations. The [[Riquier–Janet theory]] is an effective method for obtaining information about many analytic [[Overdetermined system|overdetermined]] systems.&lt;br /&gt;
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Nevertheless, some techniques can be used for several types of equations. The -principle is the most powerful method to solve underdetermined equations. The Riquier–Janet theory is an effective method for obtaining information about many analytic overdetermined systems.&lt;br /&gt;
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然而，一些技巧可以用于几种类型的方程。h-原理是求解欠定方程最有效的方法。里基尔-珍妮特理论是一种可以获得许多解析超定系统信息的有效方法。&lt;br /&gt;
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The [[method of characteristics]] can be used in some very special cases to solve partial differential equations.&lt;br /&gt;
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The method of characteristics can be used in some very special cases to solve partial differential equations.&lt;br /&gt;
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特征线法可用于求解某些特殊情况下的偏微分方程。&lt;br /&gt;
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In some cases, a PDE can be solved via [[perturbation analysis]] in which the solution is considered to be a correction to an equation with a known solution. Alternatives are [[numerical analysis]] techniques from simple [[finite difference]] schemes to the more mature [[multigrid]] and [[finite element method]]s. Many interesting problems in science and engineering are solved in this way using [[computer]]s, sometimes high performance [[supercomputer]]s.&lt;br /&gt;
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In some cases, a PDE can be solved via perturbation analysis in which the solution is considered to be a correction to an equation with a known solution. Alternatives are numerical analysis techniques from simple finite difference schemes to the more mature multigrid and finite element methods. Many interesting problems in science and engineering are solved in this way using computers, sometimes high performance supercomputers.&lt;br /&gt;
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在某些情况下，偏微分方程可以通过扰动分析来求解。在扰动分析中，通常是求解将具有已知解的方程修正后的新得到方程。可供选择的数值分析技术从简单的差分格式到更成熟的多重网格和有限元方法。许多有趣的科学和工程问题都是在计算机上用这种方法解决的，有时是高性能超级计算机。&lt;br /&gt;
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===Lie group method===&lt;br /&gt;
李群方法&lt;br /&gt;
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From 1870 [[Sophus Lie]]'s work put the theory of differential equations on a more satisfactory foundation. He showed that the integration theories of the older mathematicians can, by the introduction of what are now called [[Lie group]]s, be referred, to a common source; and that ordinary differential equations which admit the same [[infinitesimal transformation]]s present comparable difficulties of integration. He also emphasized the subject of [[contact transformation|transformations of contact]].&lt;br /&gt;
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From 1870 Sophus Lie's work put the theory of differential equations on a more satisfactory foundation. He showed that the integration theories of the older mathematicians can, by the introduction of what are now called Lie groups, be referred, to a common source; and that ordinary differential equations which admit the same infinitesimal transformations present comparable difficulties of integration. He also emphasized the subject of transformations of contact.&lt;br /&gt;
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从1870年起，索弗斯·李的工作为微分方程理论奠定了一个较为令人满意的基础。他指出，通过引入现在所谓的李群，老一辈数学家的积分理论可以引用到一个共同的来源; 承认相同的无穷小变换的常微分方程在积分方面存在相当的困难。他还强调了接触的转变这一主题。&lt;br /&gt;
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==[[用户:Yuling|Yuling]]（[[用户讨论:Yuling|讨论]]）这句话“He also emphasized the subject of transformations of contact.”中的transformations of contact翻译的不太好。&lt;br /&gt;
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A general approach to solving PDEs uses the symmetry property of differential equations, the continuous [[infinitesimal transformation]]s of solutions to solutions ([[Lie theory]]). Continuous [[group theory]], [[Lie algebras]] and [[differential geometry]] are used to understand the structure of linear and nonlinear partial differential equations for generating integrable equations, to find its [[Lax pair]]s, recursion operators, [[Bäcklund transform]] and finally finding exact analytic solutions to the PDE.&lt;br /&gt;
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A general approach to solving PDEs uses the symmetry property of differential equations, the continuous infinitesimal transformations of solutions to solutions (Lie theory). Continuous group theory, Lie algebras and differential geometry are used to understand the structure of linear and nonlinear partial differential equations for generating integrable equations, to find its Lax pairs, recursion operators, Bäcklund transform and finally finding exact analytic solutions to the PDE.&lt;br /&gt;
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求解偏微分方程的一般方法是利用微分方程的对称性，即解到解的连续无穷小变换(李理论)。连续群论、李代数和微分几何理论被用来理解生成可积方程的线性和非线性偏微分方程的结构，找到它的Lax对、递归算子、 贝克伦德变换，最后找到偏微分方程的精确解析解。&lt;br /&gt;
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Symmetry methods have been recognized to study differential equations arising in mathematics, physics, engineering, and many other disciplines.&lt;br /&gt;
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Symmetry methods have been recognized to study differential equations arising in mathematics, physics, engineering, and many other disciplines.&lt;br /&gt;
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对称方法已被公认可以用于研究出现在数学，物理，工程和许多其他学科的微分方程。&lt;br /&gt;
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===Semianalytical methods===&lt;br /&gt;
半解析方法&lt;br /&gt;
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The [[Adomian decomposition method]], the [[Aleksandr Lyapunov|Lyapunov]] artificial small parameter method, and He's [[homotopy perturbation method]] are all special cases of the more general [[homotopy analysis method]]. These are series expansion methods, and except for the Lyapunov method, are independent of small physical parameters as compared to the well known [[perturbation theory]], thus giving these methods greater flexibility and solution generality.&lt;br /&gt;
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The Adomian decomposition method, the Lyapunov artificial small parameter method, and He's homotopy perturbation method are all special cases of the more general homotopy analysis method. These are series expansion methods, and except for the Lyapunov method, are independent of small physical parameters as compared to the well known perturbation theory, thus giving these methods greater flexibility and solution generality.&lt;br /&gt;
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阿多米安分解法、李雅普诺夫人工小参数方法和何同伦摄动方法都是更一般的同伦分析方法的特殊情况。除了李雅普诺夫方法之外，这些都是级数展开方法，与为人熟知的摄动理论方法相比，它们与小的物理参数无关，因此这些方法具有更大的灵活性和解的通用性。&lt;br /&gt;
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== Numerical solutions ==&lt;br /&gt;
数值解&lt;br /&gt;
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The three most widely used [[Numerical partial differential equations|numerical methods to solve PDEs]] are the [[finite element analysis|finite element method]] (FEM), [[finite volume method]]s (FVM) and [[finite difference method]]s (FDM), as well other kind of methods called [[Meshfree methods]], which were made to solve problems where the before mentioned methods are limited. The FEM has a prominent position among these methods and especially its exceptionally efficient higher-order version [[hp-FEM]]. Other hybrid versions of FEM and Meshfree methods include the generalized finite element method (GFEM), [[extended finite element method]] (XFEM), [[Spectral element method|spectral finite element method]] (SFEM), [[Meshfree methods|meshfree finite element method]], [[Discontinuous Galerkin Method|discontinuous Galerkin finite element method]] (DGFEM), [[Element-Free Galerkin Method]] (EFGM), [[Interpolating Element-Free Galerkin Method]] (IEFGM), etc.&lt;br /&gt;
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The three most widely used numerical methods to solve PDEs are the finite element method (FEM), finite volume methods (FVM) and finite difference methods (FDM), as well other kind of methods called Meshfree methods, which were made to solve problems where the before mentioned methods are limited. The FEM has a prominent position among these methods and especially its exceptionally efficient higher-order version hp-FEM. Other hybrid versions of FEM and Meshfree methods include the generalized finite element method (GFEM), extended finite element method (XFEM), spectral finite element method (SFEM), meshfree finite element method, discontinuous Galerkin finite element method (DGFEM), Element-Free Galerkin Method (EFGM), Interpolating Element-Free Galerkin Method (IEFGM), etc.&lt;br /&gt;
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求解偏微分方程最常用的三种数值方法是有限元分析法、有限体积法和有限差分法，以及其他一些称为无网格法的方法。这些方法用于解决前面提到的方法受到的限制。在这些方法中，有限元方法，尤其是高效的高阶有限元方法，占有重要地位。其他有限元法和无网格法的混合形式包括广义有限元分析法(GFEM)、扩展有限元分析法(XFEM)、谱有限元分析法(SFEM)、无网格有限元分析法(DGFEM)、间断伽辽金有限元分析法(DGFEM)、无网格伽辽金法(EFGM)、插值无网格伽辽金法(IEFGM)等。&lt;br /&gt;
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=== Finite element method ===&lt;br /&gt;
有限元分析法&lt;br /&gt;
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{{main|Finite element method}}&lt;br /&gt;
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The finite element method (FEM) (its practical application often known as finite element analysis (FEA)) is a numerical technique for finding approximate solutions of partial differential equations (PDE) as well as of integral equations. The solution approach is based either on eliminating the differential equation completely (steady state problems), or rendering the PDE into an approximating system of ordinary differential equations, which are then numerically integrated using standard techniques such as Euler's method, Runge–Kutta, etc.&lt;br /&gt;
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The finite element method (FEM) (its practical application often known as finite element analysis (FEA)) is a numerical technique for finding approximate solutions of partial differential equations (PDE) as well as of integral equations. The solution approach is based either on eliminating the differential equation completely (steady state problems), or rendering the PDE into an approximating system of ordinary differential equations, which are then numerically integrated using standard techniques such as Euler's method, Runge–Kutta, etc.&lt;br /&gt;
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'''&amp;lt;font color = &amp;quot;#ff8000&amp;quot;&amp;gt;有限元分析法 Finite Element Method&amp;lt;/font&amp;gt;''' ((其实际应用通常被称为有限元分析(FEA))是一种寻找偏微分方程(PDE)和积分方程近似解的数值技术。这种求解方法要么基于完全消除微分方程(稳态问题) ，要么将偏微分方程转化为常微分方程的近似系统，然后使用标准技术进行数值积分，如欧拉方法、 Runge-Kutta 等。&lt;br /&gt;
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===Finite difference method===&lt;br /&gt;
有限差分法&lt;br /&gt;
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{{main|Finite difference method}}&lt;br /&gt;
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Finite-difference methods are numerical methods for approximating the solutions to differential equations using [[finite difference]] equations to approximate derivatives.&lt;br /&gt;
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Finite-difference methods are numerical methods for approximating the solutions to differential equations using finite difference equations to approximate derivatives.&lt;br /&gt;
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有限差分法是一种数值方法，用差分方程近似微分方程的解。&lt;br /&gt;
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=== Finite volume method ===&lt;br /&gt;
有限体积法&lt;br /&gt;
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{{main|Finite volume method}}&lt;br /&gt;
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Similar to the finite difference method or finite element method, values are calculated at discrete places on a meshed geometry. &amp;quot;Finite volume&amp;quot; refers to the small volume surrounding each node point on a mesh. In the finite volume method, surface integrals in a partial differential equation that contain a divergence term are converted to volume integrals, using the [[divergence theorem]]. These terms are then evaluated as fluxes at the surfaces of each finite volume. Because the flux entering a given volume is identical to that leaving the adjacent volume, these methods conserve mass by design.&lt;br /&gt;
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Similar to the finite difference method or finite element method, values are calculated at discrete places on a meshed geometry. &amp;quot;Finite volume&amp;quot; refers to the small volume surrounding each node point on a mesh. In the finite volume method, surface integrals in a partial differential equation that contain a divergence term are converted to volume integrals, using the divergence theorem. These terms are then evaluated as fluxes at the surfaces of each finite volume. Because the flux entering a given volume is identical to that leaving the adjacent volume, these methods conserve mass by design.&lt;br /&gt;
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类似于有限差分法或有限元分析，函数值是在网状几何体上的离散位置进行计算的。“有限体积”是指网格上每个节点周围的小体积。在有限体积法中，偏微分方程中含有散度项的面积分用散度定理积分转换成体积分。然后将这些项用于估算每个有限体积表面上的通量。由于进入给定体积的通量与转移到相邻体积元的通量相同，所以这些方法在设计上保证了质量守恒。&lt;br /&gt;
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==See also==&lt;br /&gt;
请参阅&lt;br /&gt;
* [[Dirichlet boundary condition]]&lt;br /&gt;
狄利克雷边界条件&lt;br /&gt;
* [[Jet bundle]]&lt;br /&gt;
射流丛&lt;br /&gt;
* [[Laplace transform applied to differential equations]]&lt;br /&gt;
微分方程中的拉普拉斯变换&lt;br /&gt;
* [[List of dynamical systems and differential equations topics]]&lt;br /&gt;
动力学系统和微分方程的列表&lt;br /&gt;
* [[Matrix differential equation]]&lt;br /&gt;
矩阵微分方程&lt;br /&gt;
* [[Neumann boundary condition]]&lt;br /&gt;
诺伊曼边界条件&lt;br /&gt;
* [[Numerical partial differential equations]]&lt;br /&gt;
数值偏微分方程&lt;br /&gt;
* [[Partial differential algebraic equation]]&lt;br /&gt;
偏微分代数方程&lt;br /&gt;
* [[Recurrence relation]]&lt;br /&gt;
递推关系&lt;br /&gt;
* [[Robin boundary condition]]&lt;br /&gt;
罗宾边界条件&lt;br /&gt;
* [[Stochastic processes and boundary value problems]]&lt;br /&gt;
随机过程和边值问题&lt;br /&gt;
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== The energy method ==&lt;br /&gt;
能量法&lt;br /&gt;
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The energy method is a mathematical procedure that can be used to verify well-posedness of initial-boundary-value-problems.&amp;lt;ref&amp;gt;{{cite book |title=High Order Difference Methods for Time Dependent PDE&lt;br /&gt;
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The energy method is a mathematical procedure that can be used to verify well-posedness of initial-boundary-value-problems.&amp;lt;ref&amp;gt;{{cite book |title=High Order Difference Methods for Time Dependent PDE&lt;br /&gt;
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能量法是验证初边值问题适定性的一种数学方法。 时变偏微分方程的高阶差分方法&lt;br /&gt;
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|first=Bertil|last=Gustafsson|publisher=Springer|year=2008|isbn=978-3-540-74992-9|doi=10.1007/978-3-540-74993-6}}&amp;lt;/ref&amp;gt; In the following example the energy method is used to decide where and which boundary conditions should be imposed such that the resulting IBVP is well-posed. Consider the one-dimensional hyperbolic PDE given by&lt;br /&gt;
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|first=Bertil|last=Gustafsson|publisher=Springer|year=2008|isbn=978-3-540-74992-9|doi=10.1007/978-3-540-74993-6}}&amp;lt;/ref&amp;gt; In the following example the energy method is used to decide where and which boundary conditions should be imposed such that the resulting IBVP is well-posed. Consider the one-dimensional hyperbolic PDE given by&lt;br /&gt;
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| first Bertil | last Gustafsson | publisher | Springer | year 2008 | isbn 978-3-540-74992-9 | doi 10.1007 / 978-3-540-74993-6} / ref 在下面的例子中，使用能量方法来决定应该施加哪些边界条件，使得得到的 IBVP适定。考虑一维双曲偏微分方程&lt;br /&gt;
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: &amp;lt;math&amp;gt;\frac{\partial u}{\partial t} + \alpha \frac{\partial u}{\partial x} = 0, \quad x \in [a,b], \operatorname t &amp;gt; 0,&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;\frac{\partial u}{\partial t} + \alpha \frac{\partial u}{\partial x} = 0, \quad x \in [a,b], \operatorname t &amp;gt; 0,&amp;lt;/math&amp;gt;&lt;br /&gt;
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where &amp;lt;math&amp;gt;\alpha \neq 0&amp;lt;/math&amp;gt; is a constant and &amp;lt;math&amp;gt;u(x,t)&amp;lt;/math&amp;gt; is an unknown function with initial condition &amp;lt;math&amp;gt;u(x,0) = f(x)&amp;lt;/math&amp;gt;. Multiplying with &amp;lt;math&amp;gt;u&amp;lt;/math&amp;gt; and integrating over the domain gives&lt;br /&gt;
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where &amp;lt;math&amp;gt;\alpha \neq 0&amp;lt;/math&amp;gt; is a constant and &amp;lt;math&amp;gt;u(x,t)&amp;lt;/math&amp;gt; is an unknown function with initial condition &amp;lt;math&amp;gt;u(x,0) = f(x)&amp;lt;/math&amp;gt;. Multiplying with &amp;lt;math&amp;gt;u&amp;lt;/math&amp;gt; and integrating over the domain gives&lt;br /&gt;
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其中 &amp;lt;math&amp;gt;\alpha \neq 0&amp;lt;/math&amp;gt; 是常数，并且 &amp;lt;math&amp;gt;u(x,t)&amp;lt;/math&amp;gt; 是未知函数，初始条件是 &amp;lt;math&amp;gt;u(x,0) = f(x)&amp;lt;/math&amp;gt;。乘以 &amp;lt;math&amp;gt;u&amp;lt;/math&amp;gt; 并在域上进行积分。&lt;br /&gt;
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: &amp;lt;math&amp;gt;\int_a^b u \frac{\partial u}{\partial t} \operatorname dx + \alpha \int _a ^b u \frac{\partial u}{\partial x} \operatorname dx = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;\int_a^b u \frac{\partial u}{\partial t} \operatorname dx + \alpha \int _a ^b u \frac{\partial u}{\partial x} \operatorname dx = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
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Using that&lt;br /&gt;
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Using that&lt;br /&gt;
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利用这一点&lt;br /&gt;
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: &amp;lt;math&amp;gt;\int _a ^b u \frac{\partial u}{\partial t} \operatorname dx = \frac{1}{2} \frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 \quad \text{and} \quad \int _a ^b u \frac{\partial u}{\partial x} \operatorname dx = \frac{1}{2} u(b,t)^2 - \frac{1}{2} u(a,t)^2,.&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;\int _a ^b u \frac{\partial u}{\partial t} \operatorname dx = \frac{1}{2} \frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 \quad \text{and} \quad \int _a ^b u \frac{\partial u}{\partial x} \operatorname dx = \frac{1}{2} u(b,t)^2 - \frac{1}{2} u(a,t)^2,.&amp;lt;/math&amp;gt;&lt;br /&gt;
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where integration by parts has been used for the second relationship, we get&lt;br /&gt;
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where integration by parts has been used for the second relationship, we get&lt;br /&gt;
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第二个关系中采用了分部积分法，我们可以得到&lt;br /&gt;
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: &amp;lt;math&amp;gt;\frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 + \alpha u(b,t)^2 - \alpha u(a,t)^2 = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;\frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 + \alpha u(b,t)^2 - \alpha u(a,t)^2 = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
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Here &amp;lt;math&amp;gt;\vert \vert \cdot \vert \vert&amp;lt;/math&amp;gt; denotes the standard L2-norm.&lt;br /&gt;
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Here &amp;lt;math&amp;gt;\vert \vert \cdot \vert \vert&amp;lt;/math&amp;gt; denotes the standard L2-norm.&lt;br /&gt;
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在这里，&amp;lt;math&amp;gt;\vert \vert \cdot \vert \vert&amp;lt;/math&amp;gt; 表示标准的 L2-正则。&lt;br /&gt;
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For well-posedness we require that the energy of the solution is non-increasing, i.e. that &amp;lt;math&amp;gt;\frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 \leq 0&amp;lt;/math&amp;gt;, which is achieved by specifying &amp;lt;math&amp;gt;u&amp;lt;/math&amp;gt; at &amp;lt;math&amp;gt;x = a&amp;lt;/math&amp;gt; if &amp;lt;math&amp;gt;\alpha &amp;gt; 0&amp;lt;/math&amp;gt; and at &amp;lt;math&amp;gt;x = b&amp;lt;/math&amp;gt; if &amp;lt;math&amp;gt;\alpha &amp;lt; 0&amp;lt;/math&amp;gt;. This corresponds to only imposing boundary conditions at the inflow. Note that well-posedness allows for growth in terms of data (initial and boundary) and thus it is sufficient to show that &amp;lt;math&amp;gt;\frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 \leq 0&amp;lt;/math&amp;gt; holds when all data is set to zero.&lt;br /&gt;
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For well-posedness we require that the energy of the solution is non-increasing, i.e. that &amp;lt;math&amp;gt;\frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 \leq 0&amp;lt;/math&amp;gt;, which is achieved by specifying &amp;lt;math&amp;gt;u&amp;lt;/math&amp;gt; at &amp;lt;math&amp;gt;x = a&amp;lt;/math&amp;gt; if &amp;lt;math&amp;gt;\alpha &amp;gt; 0&amp;lt;/math&amp;gt; and at &amp;lt;math&amp;gt;x = b&amp;lt;/math&amp;gt; if &amp;lt;math&amp;gt;\alpha &amp;lt; 0&amp;lt;/math&amp;gt;. This corresponds to only imposing boundary conditions at the inflow. Note that well-posedness allows for growth in terms of data (initial and boundary) and thus it is sufficient to show that &amp;lt;math&amp;gt;\frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 \leq 0&amp;lt;/math&amp;gt; holds when all data is set to zero.&lt;br /&gt;
&lt;br /&gt;
对于适定性，我们要解的能量是不增加的，即 &amp;lt;math&amp;gt;\frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 \leq 0&amp;lt;/math&amp;gt; ，这种关系可以通过在&amp;lt;math&amp;gt;x = a&amp;lt;/math&amp;gt;处 （如果 &amp;lt;math&amp;gt;\alpha &amp;gt; 0&amp;lt;/math&amp;gt;） 以及 &amp;lt;math&amp;gt;x = b&amp;lt;/math&amp;gt;处 （如果 &amp;lt;math&amp;gt;\alpha &amp;lt; 0&amp;lt;/math&amp;gt;）指定&amp;lt;math&amp;gt;u&amp;lt;/math&amp;gt;的值来实现。这只相当于在入流处附加边界条件。注意，适定性允许在数据(初始和边界)上的增长，因此它足以表明当所有数据设置为零时应有 &amp;lt;math&amp;gt;\frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 \leq 0&amp;lt;/math&amp;gt;。&lt;br /&gt;
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==[[用户:Yuling|Yuling]]（[[用户讨论:Yuling|讨论]]）“This corresponds to only imposing boundary conditions at the inflow.” 这句话中的inflow不是很理解&lt;br /&gt;
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==Notes==&lt;br /&gt;
&lt;br /&gt;
{{Reflist}}&lt;br /&gt;
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== References ==&lt;br /&gt;
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{{refbegin|2}}&lt;br /&gt;
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* {{cite book |title=Solving Frontier problems of Physics: The decomposition method&lt;br /&gt;
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|first=G.|last=Adomian|publisher=Kluwer Academic Publishers|year=1994|isbn=|page=|url=https://books.google.com/books?id=UKPqCAAAQBAJ&amp;amp;printsec=frontcover#v=onepage&amp;amp;q=%22partial%20differential%22&amp;amp;f=false}}&lt;br /&gt;
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&lt;br /&gt;
* {{Citation |first=A. D. |last=Polyanin |first2=V. F. |last2=Zaitsev |lastauthoramp=yes |first3=A. |last3=Moussiaux |title=Handbook of First Order Partial Differential Equations |publisher=Taylor &amp;amp; Francis |location=London |year=2002 |isbn=0-415-27267-X }}.&lt;br /&gt;
&lt;br /&gt;
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&lt;br /&gt;
* {{Citation |first=P. |last=Solin |title=Partial Differential Equations and the Finite Element Method |publisher=J. Wiley &amp;amp; Sons |location=Hoboken, NJ |year=2005 |isbn=0-471-72070-4 }}.&lt;br /&gt;
&lt;br /&gt;
* {{Citation |first=P. |last=Solin |first2=K. |last2=Segeth |lastauthoramp=yes |first3=I. |last3=Dolezel |title=Higher-Order Finite Element Methods |publisher=Chapman &amp;amp; Hall/CRC Press |location=Boca Raton |year=2003 |isbn=1-58488-438-X }}.&lt;br /&gt;
&lt;br /&gt;
* {{Citation |first=H. |last=Stephani |year=1989 |title=Differential Equations: Their Solution Using Symmetries. Edited by M. MacCallum |publisher=Cambridge University Press }}.&lt;br /&gt;
&lt;br /&gt;
* {{cite book |title=Partial Differential Equations and Solitary Waves Theory&lt;br /&gt;
&lt;br /&gt;
|first=Abdul-Majid|last=Wazwaz|publisher=Higher Education Press|year=2009|isbn=978-3-642-00251-9|page=}}&lt;br /&gt;
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|first=Abdul-Majid|last=Wazwaz|publisher=Higher Education Press|year=2009|isbn=978-3-642-00251-9|page=}}&lt;br /&gt;
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| first Abdul-Majid | last Wazwaz | publisher Higher Education Press | year 2009 | isbn 978-3-642-00251-9 | page }&lt;br /&gt;
&lt;br /&gt;
* {{cite book |title=Partial Differential Equations Methods and Applications&lt;br /&gt;
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|first=Abdul-Majid|last=Wazwaz|publisher=A.A. Balkema|year=2002|isbn=90-5809-369-7|page=}}&lt;br /&gt;
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|first=Abdul-Majid|last=Wazwaz|publisher=A.A. Balkema|year=2002|isbn=90-5809-369-7|page=}}&lt;br /&gt;
&lt;br /&gt;
| first Abdul-Majid | last Wazwaz | publisher a.a.Balkema | year 2002 | isbn 90-5809-369-7 | page }&lt;br /&gt;
&lt;br /&gt;
* {{Citation |first=D. |last=Zwillinger |title=Handbook of Differential Equations |publisher=Academic Press |location=Boston |year=1997 |edition=3rd |isbn=0-12-784395-7 }}.&lt;br /&gt;
&lt;br /&gt;
* {{Citation |authorlink=Neil Gershenfeld |first=N. |last=Gershenfeld |title=The Nature of Mathematical Modeling |location=New York |publisher=Cambridge University Press, New York, NY, USA |year=1999 |edition=1st |isbn=0-521-57095-6 }}.&lt;br /&gt;
&lt;br /&gt;
* {{Citation |first=I.S. |last=Krasil'shchik |lastauthoramp=yes |first2=A.M., Eds. |last2=Vinogradov |title=Symmetries and Conserwation Laws for Differential Equations of Mathematical Physics |publisher=American Mathematical Society, Providence, Rhode Island, USA |year=1999 |isbn=0-8218-0958-X }}.&lt;br /&gt;
&lt;br /&gt;
* {{Citation |first=I.S. |last=Krasil'shchik |first2=V.V. |last2=Lychagin|lastauthoramp=yes |first3=A.M. |last3=Vinogradov |title=Geometry of Jet Spaces and Nonlinear Partial Differential Equations |publisher=Gordon and Breach Science Publishers, New York, London, Paris, Montreux, Tokyo |year=1986 |isbn=2-88124-051-8 }}.&lt;br /&gt;
&lt;br /&gt;
* {{Citation |first=A.M. |last=Vinogradov |title=Cohomological Analysis of Partial Differential Equations and Secondary Calculus |publisher=American Mathematical Society, Providence, Rhode Island, USA |year=2001 |isbn=0-8218-2922-X }}.&lt;br /&gt;
&lt;br /&gt;
* {{cite book |title=High Order Difference Methods for Time Dependent PDE&lt;br /&gt;
&lt;br /&gt;
|first=Bertil|last=Gustafsson|publisher=Springer|year=2008|isbn=978-3-540-74992-9|doi=10.1007/978-3-540-74993-6}}&lt;br /&gt;
&lt;br /&gt;
|first=Bertil|last=Gustafsson|publisher=Springer|year=2008|isbn=978-3-540-74992-9|doi=10.1007/978-3-540-74993-6}}&lt;br /&gt;
&lt;br /&gt;
| first Bertil | last Gustafsson | Springer | year 2008 | isbn 978-3-540-74992-9 | doi 10.1007 / 978-3-540-74993-6}&lt;br /&gt;
&lt;br /&gt;
{{refend}}&lt;br /&gt;
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&lt;br /&gt;
== Further reading ==&lt;br /&gt;
&lt;br /&gt;
* {{Cite journal|last=Cajori|first=Florian|authorlink=Florian Cajori|year=1928|title=The Early History of Partial Differential Equations and of Partial Differentiation and Integration|url=http://www.math.harvard.edu/archive/21a_fall_14/exhibits/cajori/cajori.pdf|journal=The American Mathematical Monthly|volume=35|issue=9|pages=459–467|doi=10.2307/2298771|access-date=2016-05-15|archive-url=https://web.archive.org/web/20181123102253/http://www.math.harvard.edu/archive/21a_fall_14/exhibits/cajori/cajori.pdf|archive-date=2018-11-23|url-status=dead}}&lt;br /&gt;
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== External links ==&lt;br /&gt;
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{{Sister project links| wikt=no | commons=Category:Solutions of PDE | b=Partial Differential Equations | n=no | q=Partial differential equation | s=no | v=no | voy=no | species=no | d=no}}&lt;br /&gt;
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* {{springer|title=Differential equation, partial|id=p/d031920}}&lt;br /&gt;
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* [http://eqworld.ipmnet.ru/en/pde-en.htm Partial Differential Equations: Exact Solutions] at EqWorld: The World of Mathematical Equations.&lt;br /&gt;
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* [http://eqworld.ipmnet.ru/en/solutions/eqindex/eqindex-pde.htm Partial Differential Equations: Index] at EqWorld: The World of Mathematical Equations.&lt;br /&gt;
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* [http://eqworld.ipmnet.ru/en/methods/meth-pde.htm Partial Differential Equations: Methods] at EqWorld: The World of Mathematical Equations.&lt;br /&gt;
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* [https://web.archive.org/web/20170701144823/http://www.exampleproblems.com/wiki/index.php?title=Partial_Differential_Equations Example problems with solutions] at exampleproblems.com&lt;br /&gt;
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* [http://mathworld.wolfram.com/PartialDifferentialEquation.html Partial Differential Equations] at mathworld.wolfram.com&lt;br /&gt;
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* [https://reference.wolfram.com/language/FEMDocumentation/tutorial/SolvingPDEwithFEM.html Partial Differential Equations] with Mathematica&lt;br /&gt;
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* [http://www.mathworks.com/moler/pdes.pdf Partial Differential Equations] in Cleve Moler: Numerical Computing with MATLAB&lt;br /&gt;
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* [http://www.nag.com/numeric/fl/nagdoc_fl24/html/D03/d03intro.html Partial Differential Equations] at nag.com&lt;br /&gt;
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* {{cite web |first=Grant |last=Sanderson |title=But what is a partial differential equation? |work=3Blue1Brown |date=April 21, 2019 |url=https://www.youtube.com/watch?v=ly4S0oi3Yz8&amp;amp;list=PLZHQObOWTQDNPOjrT6KVlfJuKtYTftqH6 |via=[[YouTube]] }}&lt;br /&gt;
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{{Differential equations topics}}&lt;br /&gt;
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{{Authority control}}&lt;br /&gt;
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[[Category:Partial differential equations| ]]&lt;br /&gt;
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[[Category:Multivariable calculus]]&lt;br /&gt;
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Category:Multivariable calculus&lt;br /&gt;
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类别: 多元微积分&lt;br /&gt;
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[[Category:Differential equations]]&lt;br /&gt;
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Category:Differential equations&lt;br /&gt;
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类别: 微分方程&lt;br /&gt;
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[[Category:Concepts in physics]]&lt;br /&gt;
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Category:Concepts in physics&lt;br /&gt;
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分类: 物理概念&lt;br /&gt;
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&amp;lt;small&amp;gt;This page was moved from [[wikipedia:en:Partial differential equation]]. Its edit history can be viewed at [[偏微分方程/edithistory]]&amp;lt;/small&amp;gt;&amp;lt;/noinclude&amp;gt;&lt;br /&gt;
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[[Category:待整理页面]]&lt;/div&gt;</summary>
		<author><name>Ruili</name></author>
	</entry>
	<entry>
		<id>https://wiki.swarma.org/index.php?title=%E5%81%8F%E5%BE%AE%E5%88%86%E6%96%B9%E7%A8%8B&amp;diff=18114</id>
		<title>偏微分方程</title>
		<link rel="alternate" type="text/html" href="https://wiki.swarma.org/index.php?title=%E5%81%8F%E5%BE%AE%E5%88%86%E6%96%B9%E7%A8%8B&amp;diff=18114"/>
		<updated>2020-11-11T13:11:25Z</updated>

		<summary type="html">&lt;p&gt;Ruili：&lt;/p&gt;
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&lt;div&gt;此词条暂由Yuling翻译，未经人工整理和审校，带来阅读不便，请见谅。&lt;br /&gt;
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[[File:Heat.gif|thumb|right|A visualisation of a solution to the two-dimensional [[heat equation]] with temperature represented by the third dimension]]&lt;br /&gt;
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A visualisation of a solution to the two-dimensional [[heat equation with temperature represented by the third dimension]]&lt;br /&gt;
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以三维表示温度的二维热方程解的可视化&lt;br /&gt;
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In [[mathematics]], a '''partial differential equation''' ('''PDE''') is a [[differential equation]] that contains unknown [[Multivariable calculus|multivariable functions]] and their [[partial derivative]]s. PDEs are used to formulate problems involving functions of several variables, and are either solved by hand, or used to create a [[computer model]]. A special case is [[ordinary differential equation]]s (ODEs), which deal with functions of a single variable and their derivatives.&lt;br /&gt;
&lt;br /&gt;
In mathematics, a partial differential equation (PDE) is a differential equation that contains unknown multivariable functions and their partial derivatives. PDEs are used to formulate problems involving functions of several variables, and are either solved by hand, or used to create a computer model. A special case is ordinary differential equations (ODEs), which deal with functions of a single variable and their derivatives.&lt;br /&gt;
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在数学中，'''&amp;lt;font color = &amp;quot;#ff8000&amp;quot;&amp;gt;偏微分方程函数 Partial Differential Equation&amp;lt;/font&amp;gt;'''是包含未知多元函数及其偏导数的微分方程。偏微分方程用于描述涉及多元函数的问题，可以通过人为求解，也可以通过建立计算机模型来求解。常微分方程是偏微分方程一种特殊情况，它处理的是一元函数及其导数。&lt;br /&gt;
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PDEs can be used to describe a wide variety of phenomena such as sound, heat, [[diffusion]], [[electrostatics]], [[Electromagnetism|electrodynamics]], [[fluid dynamics]], [[Elasticity (physics)|elasticity]], [[gravitation]] and [[quantum mechanics]]. These seemingly distinct physical phenomena can be formalised similarly in terms of PDEs. Just as ordinary differential equations often model one-dimensional [[dynamical system]]s, partial differential equations often model [[multidimensional system]]s. PDEs find their generalisation in [[stochastic partial differential equation]]s.&lt;br /&gt;
&lt;br /&gt;
PDEs can be used to describe a wide variety of phenomena such as sound, heat, diffusion, electrostatics, electrodynamics, fluid dynamics, elasticity, gravitation and quantum mechanics. These seemingly distinct physical phenomena can be formalised similarly in terms of PDEs. Just as ordinary differential equations often model one-dimensional dynamical systems, partial differential equations often model multidimensional systems. PDEs find their generalisation in stochastic partial differential equations.&lt;br /&gt;
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偏微分方程可以用来描述各种各样的物理现象，如声音，热量，扩散，静电，电动力学，流体力学，弹性力学，重力和量子力学。这些看起来截然不同的物理现象却可以用类似的偏微分方程来描述。正如常微分方程经常对一维动力系统进行建模一样，偏微分方程经常对多维系统进行建模。随机偏微分方程是偏微分方程的一种推广。&lt;br /&gt;
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== Introduction ==&lt;br /&gt;
引言&lt;br /&gt;
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Partial differential equations (PDEs) are equations that involve rates of change with respect to [[continuous variables]]. For example, the position of a [[rigid body]] is specified by six parameters,&amp;lt;ref&amp;gt;{{Cite book|url=https://books.google.com/books?id=v9PLbcYd9aUC&amp;amp;pg=PA32|title=Modelling and Control of Robot Manipulators|last=Sciavicco|first=Lorenzo|last2=Siciliano|first2=Bruno|date=2001-02-19|publisher=Springer Science &amp;amp; Business Media|isbn=9781852332211|language=en}}&amp;lt;/ref&amp;gt; but the configuration of a [[fluid]] is given by the [[continuous distribution]] of several parameters, such as the [[temperature]], [[pressure]], and so forth. The dynamics for the rigid body take place in a finite-dimensional [[Configuration space (physics)|configuration space]]; the dynamics for the fluid occur in an infinite-dimensional configuration space. This distinction usually makes PDEs much harder to solve than ordinary differential equations (ODEs), but here again, there will be simple solutions for linear problems. Classic domains where PDEs are used include [[acoustics]], [[fluid dynamics]], [[electrodynamics]], and [[heat transfer]].&lt;br /&gt;
&lt;br /&gt;
Partial differential equations (PDEs) are equations that involve rates of change with respect to continuous variables. For example, the position of a rigid body is specified by six parameters, but the configuration of a fluid is given by the continuous distribution of several parameters, such as the temperature, pressure, and so forth. The dynamics for the rigid body take place in a finite-dimensional configuration space; the dynamics for the fluid occur in an infinite-dimensional configuration space. This distinction usually makes PDEs much harder to solve than ordinary differential equations (ODEs), but here again, there will be simple solutions for linear problems. Classic domains where PDEs are used include acoustics, fluid dynamics, electrodynamics, and heat transfer.&lt;br /&gt;
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偏微分方程(简称为PDEs)涉及到方程相对于连续变量的变化率。例如，刚体的位置是由六个参数确定的，而流体的状态是由几个参数的连续分布给出的，如温度、压力等。刚体的动力学过程发生在有限维状态空间中，流体的动力学过程发生在无限维状态空间中。这种区别通常使偏微分方程比常微分方程更难求解，但是线性问题仍然有简单的求解方式。使用偏微分方程的经典领域包括声学、流体力学、电动力学和传热学。&lt;br /&gt;
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A partial differential equation (PDE) for the function {{math|''u''(''x''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;,… ''x&amp;lt;sub&amp;gt;n&amp;lt;/sub&amp;gt;'')}} is an equation of the form&lt;br /&gt;
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A partial differential equation (PDE) for the function  is an equation of the form&lt;br /&gt;
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对于函数{{math|''u''(''x''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;,… ''x&amp;lt;sub&amp;gt;n&amp;lt;/sub&amp;gt;'')}}，它的的偏微分方程形式是：&lt;br /&gt;
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: &amp;lt;math&amp;gt;f \left (x_1, \ldots x_n; u, \frac{\partial u}{\partial x_1}, \ldots \frac{\partial u}{\partial x_n}; \frac{\partial^2 u}{\partial x_1 \partial x_1}, \ldots \frac{\partial^2 u}{\partial x_1 \partial x_n}; \ldots \right) = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;f \left (x_1, \ldots x_n; u, \frac{\partial u}{\partial x_1}, \ldots \frac{\partial u}{\partial x_n}; \frac{\partial^2 u}{\partial x_1 \partial x_1}, \ldots \frac{\partial^2 u}{\partial x_1 \partial x_n}; \ldots \right) = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
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If {{mvar|f}} is a [[linear function]] of {{mvar|u}} and its derivatives, then the PDE is called linear. Common examples of linear PDEs include the [[heat equation]], the [[wave equation]], [[Laplace's equation]], [[Helmholtz equation]], [[Klein–Gordon equation]], and [[Poisson's equation]].&lt;br /&gt;
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If  is a linear function of  and its derivatives, then the PDE is called linear. Common examples of linear PDEs include the heat equation, the wave equation, Laplace's equation, Helmholtz equation, Klein–Gordon equation, and Poisson's equation.&lt;br /&gt;
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如果{{mvar|f}}是函数及其导数的线性方程，则偏微分方程称为线性函数。线性偏微分方程的常见例子包括热方程、波动方程、拉普拉斯方程、亥姆霍兹方程方程、克莱因-高登方程和泊松方程。&lt;br /&gt;
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A relatively simple PDE is&lt;br /&gt;
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A relatively simple PDE is&lt;br /&gt;
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一个相对简单的偏微分方程是：&lt;br /&gt;
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: &amp;lt;math&amp;gt;\frac{\partial u}{\partial x}(x,y) = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;\frac{\partial u}{\partial x}(x,y) = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
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This relation [[Logical implication|implies]] that the function {{math|''u''(''x'',''y'')}} is independent of {{mvar|x}}. However, the equation gives no information on the function's dependence on the variable {{mvar|y}}. Hence the general solution of this equation is&lt;br /&gt;
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This relation implies that the function  is independent of . However, the equation gives no information on the function's dependence on the variable . Hence the general solution of this equation is&lt;br /&gt;
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这个关系意味着函数是独立于{{mvar|x}}的。然而，这个方程没有给出关于函数和自变量的相关性的信息。因此，这个方程的通解是&lt;br /&gt;
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: &amp;lt;math&amp;gt;u(x,y) = f(y),&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;u(x,y) = f(y),&amp;lt;/math&amp;gt;&lt;br /&gt;
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where {{mvar|f}} is an arbitrary function of {{mvar|y}}. The analogous ordinary differential equation is&lt;br /&gt;
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where  is an arbitrary function of . The analogous ordinary differential equation is&lt;br /&gt;
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其中{{mvar|f}}是{{mvar|y}}的任意函数。类似的常微分方程是&lt;br /&gt;
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: &amp;lt;math&amp;gt;\frac{\mathrm{d} u}{\mathrm{d} x}(x) = 0,&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;\frac{\mathrm{d} u}{\mathrm{d} x}(x) = 0,&amp;lt;/math&amp;gt;&lt;br /&gt;
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which has the solution&lt;br /&gt;
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which has the solution&lt;br /&gt;
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它的解为&lt;br /&gt;
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: &amp;lt;math&amp;gt;u(x) = c,&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;u(x) = c,&amp;lt;/math&amp;gt;&lt;br /&gt;
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where {{mvar|c}} is any [[Constant (mathematics)|constant]] value. These two examples illustrate that general solutions of ordinary differential equations (ODEs) involve arbitrary constants, but solutions of PDEs involve arbitrary functions.&lt;br /&gt;
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where  is any constant value. These two examples illustrate that general solutions of ordinary differential equations (ODEs) involve arbitrary constants, but solutions of PDEs involve arbitrary functions.&lt;br /&gt;
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这里的{{mvar|c}}是常量。这两个例子说明常微分方程的一般解包含任意常数，但偏微分方程的解包含任意函数。&lt;br /&gt;
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A solution of a PDE is generally not [[Uniqueness quantification|unique]]; additional conditions must generally be specified on the [[Boundary (topology)|boundary]] of the region where the solution is defined. For instance, in the simple example above, the function {{math|''f''(''y'')}} can be determined if {{mvar|u}} is specified on the line {{math|''x'' {{=}} 0}}.&lt;br /&gt;
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A solution of a PDE is generally not unique; additional conditions must generally be specified on the boundary of the region where the solution is defined. For instance, in the simple example above, the function  can be determined if  is specified on the line  0}}.&lt;br /&gt;
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偏微分方程的解一般不是唯一的; 附加条件一般必须在定义解的区域边界上定义。例如，在上面的简单示例中，如果在{{math|''x'' {{=}} 0}}时确定了{{mvar|u}}的值，则可以确定该函数{{math|''f''(''y'')}}。&lt;br /&gt;
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== Existence and uniqueness ==&lt;br /&gt;
存在性和唯一性&lt;br /&gt;
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Although the issue of existence and uniqueness of solutions of ordinary differential equations has a very satisfactory answer with the [[Picard–Lindelöf theorem]], that is far from the case for partial differential equations. The [[Cauchy–Kowalevski theorem]] states that the [[Cauchy problem]] for any partial differential equation whose coefficients are [[Analytic function|analytic]] in the unknown function and its derivatives, has a locally unique analytic solution. Although this result might appear to settle the existence and uniqueness of solutions, there are examples of linear partial differential equations whose coefficients have derivatives of all orders (which are nevertheless not analytic) but which have no solutions at all: see [[Lewy's example|Lewy (1957)]]. Even if the solution of a partial differential equation exists and is unique, it may nevertheless have undesirable properties.  The mathematical study of these questions is usually in the more powerful context of [[weak solution]]s.&lt;br /&gt;
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Although the issue of existence and uniqueness of solutions of ordinary differential equations has a very satisfactory answer with the Picard–Lindelöf theorem, that is far from the case for partial differential equations. The Cauchy–Kowalevski theorem states that the Cauchy problem for any partial differential equation whose coefficients are analytic in the unknown function and its derivatives, has a locally unique analytic solution. Although this result might appear to settle the existence and uniqueness of solutions, there are examples of linear partial differential equations whose coefficients have derivatives of all orders (which are nevertheless not analytic) but which have no solutions at all: see Lewy (1957). Even if the solution of a partial differential equation exists and is unique, it may nevertheless have undesirable properties.  The mathematical study of these questions is usually in the more powerful context of weak solutions.&lt;br /&gt;
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虽然常微分方程解的存在唯一性问题用'''&amp;lt;font color=&amp;quot;#ff8000&amp;quot;&amp;gt;弗罗贝尼乌斯定理 Picard–Lindelöf Theorem&amp;lt;/font&amp;gt;得到了令人满意的结果，但应用到偏微分方程上却不尽如意。'''&amp;lt;font color=&amp;quot;#ff8000&amp;quot;&amp;gt;柯西-科瓦列夫斯基定理 Cauchy–Kowalevski theorem&amp;lt;/font&amp;gt;指出，对于任何在未知函数及其导数中系数是解析的偏微分方程，柯西问题有一个局部唯一的解析解。虽然这个结果似乎解决了解的存在性和唯一性问题，但是有一些线性偏微分方程的系数具有所有级数的导数(尽管这些导数不是解析的) ，但是根本没有解: 见 Lewy (1957)。即使偏微分方程的解存在且唯一，它仍然可能具有人们所不希望的性质。这些问题的数学研究通常是在更有力的弱解的背景下进行的。&lt;br /&gt;
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An example of pathological behavior is the sequence (depending upon {{mvar|n}}) of [[Cauchy problem]]s for the [[Laplace equation]]&lt;br /&gt;
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An example of pathological behavior is the sequence (depending upon ) of Cauchy problems for the Laplace equation&lt;br /&gt;
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反常特征的一个例子是拉普拉斯方程的柯西问题的序列(取决于{{mvar|n}})&lt;br /&gt;
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: &amp;lt;math&amp;gt;\frac{\partial^2 u}{\partial x^2} + \frac{\partial^2 u}{\partial y^2}=0,&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;\frac{\partial^2 u}{\partial x^2} + \frac{\partial^2 u}{\partial y^2}=0,&amp;lt;/math&amp;gt;&lt;br /&gt;
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with [[boundary condition]]s&lt;br /&gt;
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with boundary conditions&lt;br /&gt;
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有边界条件&lt;br /&gt;
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: &amp;lt;math&amp;gt;\begin{align} u(x,0) &amp;amp;= 0, \\ \frac{\partial u}{\partial y}(x,0) &amp;amp;= \frac{\sin nx}{n}, \end{align}&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;\begin{align} u(x,0) &amp;amp;= 0, \\ \frac{\partial u}{\partial y}(x,0) &amp;amp;= \frac{\sin nx}{n}, \end{align}&amp;lt;/math&amp;gt;&lt;br /&gt;
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where {{mvar|n}} is an integer. The derivative of {{mvar|u}} with respect to {{mvar|y}} approaches zero [[uniform convergence|uniformly]] in {{mvar|x}} as {{mvar|n}} increases, but the solution is&lt;br /&gt;
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where  is an integer. The derivative of  with respect to  approaches zero uniformly in  as  increases, but the solution is&lt;br /&gt;
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其中{{mvar|n}}是整数。{{mvar|u}}是关于{{mvar|y}}的导数，一致地随着{{mvar|n}}的增加而趋于零，但是解是&lt;br /&gt;
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: &amp;lt;math&amp;gt;u(x,y) = \frac{\sinh ny \sin nx}{n^2}.&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;u(x,y) = \frac{\sinh ny \sin nx}{n^2}.&amp;lt;/math&amp;gt;&lt;br /&gt;
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This solution approaches infinity if {{mvar|nx}} is not an integer multiple of {{pi}} for any non-zero value of {{mvar|y}}. The Cauchy problem for the Laplace equation is called ''ill-posed'' or ''not [[Well-posed problem|well-posed]]'', since the solution does not continuously depend on the data of the problem. Such ill-posed problems are not usually satisfactory for physical applications.&lt;br /&gt;
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This solution approaches infinity if  is not an integer multiple of  for any non-zero value of . The Cauchy problem for the Laplace equation is called ill-posed or not well-posed, since the solution does not continuously depend on the data of the problem. Such ill-posed problems are not usually satisfactory for physical applications.&lt;br /&gt;
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对于任何非零的{{mvar|y}}，如果{{mvar|nx}}不是{{pi}}的整数倍，这个解会接近于无穷大。拉普拉斯方程的柯西问题被称为不适定问题（可以译为ill-posed或not well-posed），因为该问题的解并不连续地依赖于该问题的数据。这种不适定问题在物理应用中通常不能令人满意。&lt;br /&gt;
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The [[Navier–Stokes existence and smoothness|existence of solutions for the Navier–Stokes equations]], a partial differential equation, is part of one of the [[Millennium Prize Problems]].&lt;br /&gt;
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The existence of solutions for the Navier–Stokes equations, a partial differential equation, is part of one of the Millennium Prize Problems.&lt;br /&gt;
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一种偏微分方程——纳维-斯托克斯方程——的解的存在性就是千禧年大奖难题的一部分。&lt;br /&gt;
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== Notation ==&lt;br /&gt;
符号&lt;br /&gt;
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In PDEs, it is common to denote partial derivatives using subscripts. That is:&lt;br /&gt;
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In PDEs, it is common to denote partial derivatives using subscripts. That is:&lt;br /&gt;
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在偏微分方程中，通常用下标表示偏导数。例如:&lt;br /&gt;
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: &amp;lt;math&amp;gt;u_x = \frac{\partial u}{\partial x}&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;u_x = \frac{\partial u}{\partial x}&amp;lt;/math&amp;gt;&lt;br /&gt;
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: &amp;lt;math&amp;gt;u_{xx} = \frac{\partial^2 u}{\partial x^2} &amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;u_{xx} = \frac{\partial^2 u}{\partial x^2} &amp;lt;/math&amp;gt;&lt;br /&gt;
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: &amp;lt;math&amp;gt;u_{xy} = \frac{\partial^2 u}{\partial y\, \partial x} = \frac{\partial}{\partial y } \left(\frac{\partial u}{\partial x}\right). &amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;u_{xy} = \frac{\partial^2 u}{\partial y\, \partial x} = \frac{\partial}{\partial y } \left(\frac{\partial u}{\partial x}\right). &amp;lt;/math&amp;gt;&lt;br /&gt;
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Especially in physics, [[del]] or nabla ({{math|∇}}) is often used to denote spatial derivatives, and {{math|''&amp;amp;#x307;u'', ''ü''}} for time derivatives. For example, the [[wave equation]] (mentioned below) can be written as&lt;br /&gt;
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Especially in physics, del or nabla () is often used to denote spatial derivatives, and  for time derivatives. For example, the wave equation (mentioned below) can be written as&lt;br /&gt;
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特别是在物理学中，[[del]]或nabla ({{math|∇}})经常用来表示空间导数和时间导数。例如，波动方程(在下文中提到)可以写成&lt;br /&gt;
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:&amp;lt;math&amp;gt;\ddot u=c^2\nabla^2u&amp;lt;/math&amp;gt;&lt;br /&gt;
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&amp;lt;math&amp;gt;\ddot u=c^2\nabla^2u&amp;lt;/math&amp;gt;&lt;br /&gt;
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or&lt;br /&gt;
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or&lt;br /&gt;
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或&lt;br /&gt;
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:&amp;lt;math&amp;gt;\ddot u=c^2\Delta u&amp;lt;/math&amp;gt;&lt;br /&gt;
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&amp;lt;math&amp;gt;\ddot u=c^2\Delta u&amp;lt;/math&amp;gt;&lt;br /&gt;
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where {{math|Δ}} is the [[Laplace operator]].&lt;br /&gt;
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where  is the Laplace operator.&lt;br /&gt;
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其中{{math|Δ}}代表拉普拉斯算子&lt;br /&gt;
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== Classification ==&lt;br /&gt;
分类&lt;br /&gt;
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Some linear, second-order partial differential equations can be classified as [[parabolic partial differential equation|parabolic]], [[hyperbolic partial differential equation|hyperbolic]] and [[elliptic partial differential equation|elliptic]]. Others, such as the [[Euler–Tricomi equation]], have different types in different regions. The classification provides a guide to appropriate initial and boundary conditions and to the smoothness of the solutions.&lt;br /&gt;
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Some linear, second-order partial differential equations can be classified as parabolic, hyperbolic and elliptic. Others, such as the Euler–Tricomi equation, have different types in different regions. The classification provides a guide to appropriate initial and boundary conditions and to the smoothness of the solutions.&lt;br /&gt;
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一些线性二阶偏微分方程可分为抛物型方程、双曲型方程和椭圆型方程。其他的方程，如欧拉-特里科米方程，在不同的区域有不同的类型。这种分类有助于选择适当的初始和边界条件以及提高解的平滑性。&lt;br /&gt;
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=== Equations of first order ===&lt;br /&gt;
一阶方程&lt;br /&gt;
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{{main|First-order partial differential equation}}&lt;br /&gt;
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=== Linear equations of second order ===&lt;br /&gt;
二阶线性方程&lt;br /&gt;
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Assuming {{math|''u&amp;lt;sub&amp;gt;xy&amp;lt;/sub&amp;gt;'' {{=}} ''u&amp;lt;sub&amp;gt;yx&amp;lt;/sub&amp;gt;''}}, the general linear second-order PDE in two independent variables has the form&lt;br /&gt;
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Assuming  u&amp;lt;sub&amp;gt;yx&amp;lt;/sub&amp;gt;}}, the general linear second-order PDE in two independent variables has the form&lt;br /&gt;
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假设 {{math|''u&amp;lt;sub&amp;gt;xy&amp;lt;/sub&amp;gt;'' {{=}} ''u&amp;lt;sub&amp;gt;yx&amp;lt;/sub&amp;gt;''}}，含有两个独立变量的一般的线性二阶偏微分方程具有如下这样的形式&lt;br /&gt;
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: &amp;lt;math&amp;gt;Au_{xx} + 2Bu_{xy} + Cu_{yy} + \cdots \mbox{(lower order terms)} = 0,&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;Au_{xx} + 2Bu_{xy} + Cu_{yy} + \cdots \mbox{(lower order terms)} = 0,&amp;lt;/math&amp;gt;&lt;br /&gt;
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where the coefficients {{mvar|A}}, {{mvar|B}}, {{mvar|C}}... may depend upon {{mvar|x}} and {{mvar|y}}. If {{math|''A''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; + ''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; + ''C''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; &amp;gt; 0}} over a region of the {{mvar|xy}}-plane, the PDE is second-order in that region. This form is analogous to the equation for a conic section:&lt;br /&gt;
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where the coefficients , , ... may depend upon  and . If  over a region of the -plane, the PDE is second-order in that region. This form is analogous to the equation for a conic section:&lt;br /&gt;
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其中的系数 {{mvar|A}}, {{mvar|B}}, {{mvar|C}}... 一般取决于{{mvar|x}}和{{mvar|y}}。如果在{{mvar|xy}}-平面的一个区域上 {{math|''A''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; + ''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; + ''C''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; &amp;gt; 0}}，偏微分方程在该区域是二阶的。这种形式类似于圆锥曲线的方程:&lt;br /&gt;
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: &amp;lt;math&amp;gt;Ax^2 + 2Bxy + Cy^2 + \cdots = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;Ax^2 + 2Bxy + Cy^2 + \cdots = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
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More precisely, replacing {{math|∂&amp;lt;sub&amp;gt;''x''&amp;lt;/sub&amp;gt;}} by {{mvar|X}}, and likewise for other variables (formally this is done by a [[Fourier transform]]), converts a constant-coefficient PDE into a polynomial of the same degree, with the terms of the highest degree (a [[homogeneous polynomial]], here a [[quadratic form]]) being most significant for the classification.&lt;br /&gt;
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More precisely, replacing  by , and likewise for other variables (formally this is done by a Fourier transform), converts a constant-coefficient PDE into a polynomial of the same degree, with the terms of the highest degree (a homogeneous polynomial, here a quadratic form) being most significant for the classification.&lt;br /&gt;
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更准确地说，用 {{mvar|X}} 替换 {{math|∂&amp;lt;sub&amp;gt;''x''&amp;lt;/sub&amp;gt;}}，对于其他变量做同样的操作(从形式上来说，这是由傅里叶变换来完成的)，将一个常系数偏微分方程转换成一个相同次数的多项式，最高次数的项(齐次多项式，这里是一个二次形式)一般会用于偏微分方程的分类。&lt;br /&gt;
===~~ most significant for the classification 意译为用于偏微分方程的分类。       significiant直译过来感觉不太合适&lt;br /&gt;
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Just as one classifies [[conic section]]s and quadratic forms into parabolic, hyperbolic, and elliptic based on the [[discriminant]] {{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − 4''AC''}}, the same can be done for a second-order PDE at a given point.  However, the [[discriminant]] in a PDE is given by {{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC''}} due to the convention of the {{mvar|xy}} term being {{math|2''B''}} rather than {{mvar|B}}; formally, the discriminant (of the associated quadratic form) is {{math|(2''B'')&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − 4''AC'' {{=}} 4(''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC'')}}, with the factor of 4 dropped for simplicity.&lt;br /&gt;
&lt;br /&gt;
Just as one classifies conic sections and quadratic forms into parabolic, hyperbolic, and elliptic based on the discriminant , the same can be done for a second-order PDE at a given point.  However, the discriminant in a PDE is given by  due to the convention of the  term being  rather than ; formally, the discriminant (of the associated quadratic form) is  4(B&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − AC)}}, with the factor of 4 dropped for simplicity.&lt;br /&gt;
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正如人们可以根据判别式 {{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − 4''AC''}} 将圆锥曲线和二次型分为抛物型、双曲型和椭圆型一样，对于给定点的二阶偏微分方程也可以这样做。然而，偏微分方程中的判别式 {{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − 4''AC''}} 是根据交叉项的系数{{math|2''B''}} 而不是 {{mvar|B}} 给出的，形式上，判别式(关联二次型)是 {{math|(2''B'')&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − 4''AC'' {{=}} 4(''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC'')}}，为简单起见，去掉了因子4。&lt;br /&gt;
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# {{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC'' &amp;lt; 0}} (''[[elliptic partial differential equation]]''): Solutions of [[elliptic partial differential equation|elliptic PDEs]] are as smooth as the coefficients allow, within the interior of the region where the equation and solutions are defined. For example, solutions of [[Laplace's equation]] are analytic within the domain where they are defined, but solutions may assume boundary values that are not smooth. The motion of a fluid at subsonic speeds can be approximated with elliptic PDEs, and the Euler–Tricomi equation is elliptic where {{math|''x'' &amp;lt; 0}}.&lt;br /&gt;
&lt;br /&gt;
  (elliptic partial differential equation): Solutions of elliptic PDEs are as smooth as the coefficients allow, within the interior of the region where the equation and solutions are defined. For example, solutions of Laplace's equation are analytic within the domain where they are defined, but solutions may assume boundary values that are not smooth. The motion of a fluid at subsonic speeds can be approximated with elliptic PDEs, and the Euler–Tricomi equation is elliptic where .&lt;br /&gt;
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{{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC'' &amp;lt; 0}} (椭圆形微分方程)：在定义方程和解的区域内部，椭圆型偏微分方程的解光滑到系数允许的程度。例如，拉普拉斯方程的解在它们被定义的区域内是解析的，但是解可能假设边界值是不光滑的。亚音速流体的运动可以用椭圆偏微分方程近似，其中欧拉-特里科米方程在 {{math|''x'' &amp;lt; 0}} 时是椭圆型偏微分方程。&lt;br /&gt;
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# {{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC'' {{=}} 0}} (''[[parabolic partial differential equation]]''): Equations that are [[parabolic partial differential equation|parabolic]] at every point can be transformed into a form analogous to the [[heat equation]] by a change of independent variables. Solutions smooth out as the transformed time variable increases. The Euler–Tricomi equation has parabolic type on the line where {{math|''x'' {{=}} 0}}.&lt;br /&gt;
&lt;br /&gt;
  0}} (parabolic partial differential equation): Equations that are parabolic at every point can be transformed into a form analogous to the heat equation by a change of independent variables. Solutions smooth out as the transformed time variable increases. The Euler–Tricomi equation has parabolic type on the line where  0}}.&lt;br /&gt;
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{{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC'' {{=}} 0}}（抛物线形偏微分方程）：在每一点上都是抛物线型的方程可以通过改变自变量从而转化成类似于热方程的形式。随着转换后的时间变量的增加，方程的解变得平滑。欧拉-特里科米方程在 {{math|''x'' {{=}} 0}} 这条特征线上是抛物线形的。&lt;br /&gt;
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# {{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC'' &amp;gt; 0}} (''[[hyperbolic partial differential equation]]''): [[hyperbolic partial differential equation|hyperbolic]] equations retain any discontinuities of functions or derivatives in the initial data. An example is the [[wave equation]]. The motion of a fluid at supersonic speeds can be approximated with hyperbolic PDEs, and the Euler–Tricomi equation is hyperbolic where {{math|''x'' &amp;gt; 0}}.&lt;br /&gt;
&lt;br /&gt;
  (hyperbolic partial differential equation): hyperbolic equations retain any discontinuities of functions or derivatives in the initial data. An example is the wave equation. The motion of a fluid at supersonic speeds can be approximated with hyperbolic PDEs, and the Euler–Tricomi equation is hyperbolic where .&lt;br /&gt;
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{{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC'' &amp;gt; 0}} (双曲形偏微分方程)：双曲形方程在初始数据中保留了函数或导数的任何不连续性，波动方程就是其中的一个例子。超音速流体的运动可以用双曲形偏微分方程近似，其中欧拉-特里科米方程在 {{math|''x'' &amp;gt; 0}} 时是双曲型的。&lt;br /&gt;
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If there are {{mvar|n}} independent variables {{math|''x''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;, ''x''&amp;lt;sub&amp;gt;2 &amp;lt;/sub&amp;gt;,… ''x''&amp;lt;sub&amp;gt;''n''&amp;lt;/sub&amp;gt;}}, a general linear partial differential equation of second order has the form&lt;br /&gt;
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If there are  independent variables , a general linear partial differential equation of second order has the form&lt;br /&gt;
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如果存在 {{mvar|n}} 个自变量 {{math|''x''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;, ''x''&amp;lt;sub&amp;gt;2 &amp;lt;/sub&amp;gt;,… ''x''&amp;lt;sub&amp;gt;''n''&amp;lt;/sub&amp;gt;}}，一般二阶线性偏微分方程的形式是&lt;br /&gt;
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: &amp;lt;math&amp;gt;L u =\sum_{i=1}^n\sum_{j=1}^n a_{i,j} \frac{\partial^2 u}{\partial x_i \partial x_j} \quad \text{ plus lower-order terms} =0.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;L u =\sum_{i=1}^n\sum_{j=1}^n a_{i,j} \frac{\partial^2 u}{\partial x_i \partial x_j} \quad \text{ plus lower-order terms} =0.&amp;lt;/math&amp;gt;&lt;br /&gt;
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The classification depends upon the signature of the eigenvalues of the coefficient matrix {{math|''a''&amp;lt;sub&amp;gt;''i'',''j''&amp;lt;/sub&amp;gt;}}.&lt;br /&gt;
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The classification depends upon the signature of the eigenvalues of the coefficient matrix .&lt;br /&gt;
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这种分类取决于系数矩阵本征值的符号（正负性）。&lt;br /&gt;
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# Elliptic: the eigenvalues are all positive or all negative.&lt;br /&gt;
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 Elliptic: the eigenvalues are all positive or all negative.&lt;br /&gt;
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椭圆形方程: 本征值全部为正或全部为负。&lt;br /&gt;
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# Parabolic: the eigenvalues are all positive or all negative, save one that is zero.&lt;br /&gt;
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 Parabolic: the eigenvalues are all positive or all negative, save one that is zero.&lt;br /&gt;
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抛物线形方程: 本征值全部为正或全部为负，除了一个为零。&lt;br /&gt;
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# Hyperbolic: there is only one negative eigenvalue and all the rest are positive, or there is only one positive eigenvalue and all the rest are negative.&lt;br /&gt;
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 Hyperbolic: there is only one negative eigenvalue and all the rest are positive, or there is only one positive eigenvalue and all the rest are negative.&lt;br /&gt;
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双曲形方程: 只有一个负特征值，其余的都是正特征值，或者只有一个正特征值，其余的都是负特征值。&lt;br /&gt;
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# Ultrahyperbolic: there is more than one positive eigenvalue and more than one negative eigenvalue, and there are no zero eigenvalues. There is only a limited theory for ultrahyperbolic equations (Courant and Hilbert, 1962).&lt;br /&gt;
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 Ultrahyperbolic: there is more than one positive eigenvalue and more than one negative eigenvalue, and there are no zero eigenvalues. There is only a limited theory for ultrahyperbolic equations (Courant and Hilbert, 1962).&lt;br /&gt;
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超双形方程: 存在多于一个正本征值和多于一个的负本征值，且不存在零本征值。对于超双曲方程，只存在一个有限理论(Courant 和 Hilbert，1962)。&lt;br /&gt;
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==[[用户:Yuling|Yuling]]（[[用户讨论:Yuling|讨论]]） 我对于limited theory这个单词对应的相关理论不太了解。&lt;br /&gt;
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=== Systems of first-order equations and characteristic surfaces ===&lt;br /&gt;
一阶方程组和特征曲面&lt;br /&gt;
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The classification of partial differential equations can be extended to systems of first-order equations, where the unknown {{mvar|u}} is now a [[Euclidean vector|vector]] with {{mvar|m}} components, and the coefficient matrices {{mvar|A&amp;lt;sub&amp;gt;ν&amp;lt;/sub&amp;gt;}} are {{mvar|m}} by {{mvar|m}} matrices for {{math|''ν'' {{=}} 1, 2,… ''n''}}. The partial differential equation takes the form&lt;br /&gt;
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The classification of partial differential equations can be extended to systems of first-order equations, where the unknown  is now a vector with  components, and the coefficient matrices  are  by  matrices for  1, 2,… n}}. The partial differential equation takes the form&lt;br /&gt;
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偏微分方程组的分类可以推广到一阶方程组，其中未知量 {{mvar|u}} 是有 {{mvar|m}} 个分量的向量。对于 {{math|''ν'' {{=}} 1, 2,… ''n''}}，系数矩阵 {{mvar|A&amp;lt;sub&amp;gt;ν&amp;lt;/sub&amp;gt;}} 是 {{mvar|m}} × {{mvar|m}} 的矩阵。偏微分方程形式如下：&lt;br /&gt;
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: &amp;lt;math&amp;gt;Lu = \sum_{\nu=1}^{n} A_\nu \frac{\partial u}{\partial x_\nu} + B=0,&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;Lu = \sum_{\nu=1}^{n} A_\nu \frac{\partial u}{\partial x_\nu} + B=0,&amp;lt;/math&amp;gt;&lt;br /&gt;
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where the coefficient matrices {{mvar|A&amp;lt;sub&amp;gt;ν&amp;lt;/sub&amp;gt;}} and the vector {{mvar|B}} may depend upon {{mvar|x}} and {{mvar|u}}. If a [[hypersurface]] {{mvar|S}} is given in the implicit form&lt;br /&gt;
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where the coefficient matrices  and the vector  may depend upon  and . If a hypersurface  is given in the implicit form&lt;br /&gt;
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其中系数矩阵 {{mvar|A&amp;lt;sub&amp;gt;ν&amp;lt;/sub&amp;gt;}} 和向量 {{mvar|B}} 可能依赖于 {{mvar|x}} 和 {{mvar|u}}。如果超曲面是以隐式形式给出的&lt;br /&gt;
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: &amp;lt;math&amp;gt;\varphi(x_1, x_2, \ldots x_n)=0,&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;\varphi(x_1, x_2, \ldots x_n)=0,&amp;lt;/math&amp;gt;&lt;br /&gt;
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where {{mvar|φ}} has a non-zero gradient, then {{mvar|S}} is a '''characteristic surface''' for the operator {{mvar|L}} at a given point if the characteristic form vanishes:&lt;br /&gt;
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where  has a non-zero gradient, then  is a characteristic surface for the operator  at a given point if the characteristic form vanishes:&lt;br /&gt;
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其中存在一个非零的梯度，那么如果特征形式消失，则在给定点上算子的特征曲面形式如下:&lt;br /&gt;
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: &amp;lt;math&amp;gt;Q\left(\frac{\partial\varphi}{\partial x_1}, \ldots\frac{\partial\varphi}{\partial x_n}\right) =\det\left[\sum_{\nu=1}^nA_\nu \frac{\partial \varphi}{\partial x_\nu}\right]=0.\,&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;Q\left(\frac{\partial\varphi}{\partial x_1}, \ldots\frac{\partial\varphi}{\partial x_n}\right) =\det\left[\sum_{\nu=1}^nA_\nu \frac{\partial \varphi}{\partial x_\nu}\right]=0.\,&amp;lt;/math&amp;gt;&lt;br /&gt;
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The geometric interpretation of this condition is as follows: if data for {{mvar|u}} are prescribed on the surface {{mvar|S}}, then it may be possible to determine the normal derivative of {{mvar|u}} on {{mvar|S}} from the differential equation. If the data on {{mvar|S}} and the differential equation determine the normal derivative of {{mvar|u}} on {{mvar|S}}, then {{mvar|S}} is non-characteristic. If the data on {{mvar|S}} and the differential equation ''do not'' determine the normal derivative of {{mvar|u}} on {{mvar|S}}, then the surface is '''characteristic''', and the differential equation restricts the data on {{mvar|S}}: the differential equation is ''internal'' to {{mvar|S}}.&lt;br /&gt;
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The geometric interpretation of this condition is as follows: if data for  are prescribed on the surface , then it may be possible to determine the normal derivative of  on  from the differential equation. If the data on  and the differential equation determine the normal derivative of  on , then  is non-characteristic. If the data on  and the differential equation do not determine the normal derivative of  on , then the surface is characteristic, and the differential equation restricts the data on : the differential equation is internal to .&lt;br /&gt;
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这个条件的几何解释如下: 如果关于 {{mvar|u}} 的数据是在曲面 {{mvar|S}} 上规定的，那么就有可能依据微分方程确定曲面 {{mvar|S}} 上 {{mvar|u}} 的法向导数。如果曲面 {{mvar|S}} 上的数据和上面的微分方程能确定曲面 {{mvar|S}} 上 {{mvar|u}} 的法向导数，那么它就是非特征的。如果曲面 {{mvar|S}} 上的数据和上面的微分方程不能确定曲面 {{mvar|S}} 上 {{mvar|u}} 的法向导数，那么曲面是特征的，并且微分方程将数据限制在曲面 {{mvar|S}} 上：微分方程是在曲面 {{mvar|S}} 内部。&lt;br /&gt;
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# A first-order system {{math|''Lu'' {{=}} 0}} is ''elliptic'' if no surface is characteristic for {{mvar|L}}: the values of {{mvar|u}} on {{mvar|S}} and the differential equation always determine the normal derivative of {{mvar|u}} on {{mvar|S}}.&lt;br /&gt;
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 A first-order system  0}} is elliptic if no surface is characteristic for : the values of  on  and the differential equation always determine the normal derivative of  on .&lt;br /&gt;
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如果对于 {{mvar|L}} 没有曲面是特征的，则一阶系统 {{math|''Lu'' {{=}} 0}} 是椭圆形的：{{mvar|u}}在 {{mvar|S}} 的值和微分方程总能够决定 {{mvar|S}} 上 {{mvar|u}} 的法向导数。&lt;br /&gt;
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# A first-order system is ''hyperbolic'' at a point if there is a '''spacelike''' surface {{mvar|S}} with normal {{mvar|ξ}} at that point. This means that, given any non-trivial vector {{mvar|η}} orthogonal to {{mvar|ξ}}, and a scalar multiplier {{mvar|λ}}, the equation {{math|''Q''(''λξ'' + ''η'') {{=}} 0}} has {{mvar|m}} real roots {{math|''λ''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;, ''λ''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;,… ''λ''&amp;lt;sub&amp;gt;''m''&amp;lt;/sub&amp;gt;}}. The system is '''strictly hyperbolic''' if these roots are always distinct. The geometrical interpretation of this condition is as follows: the characteristic form {{math|''Q''(''ζ'') {{=}} 0}} defines a cone (the normal cone) with homogeneous coordinates ζ. In the hyperbolic case, this cone has {{mvar|m}} sheets, and the axis {{math|''ζ'' {{=}} ''λξ''}} runs inside these sheets: it does not intersect any of them. But when displaced from the origin by η, this axis intersects every sheet. In the elliptic case, the normal cone has no real sheets.&lt;br /&gt;
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 A first-order system is hyperbolic at a point if there is a spacelike surface  with normal  at that point. This means that, given any non-trivial vector  orthogonal to , and a scalar multiplier , the equation  0}} has  real roots . The system is strictly hyperbolic if these roots are always distinct. The geometrical interpretation of this condition is as follows: the characteristic form  0}} defines a cone (the normal cone) with homogeneous coordinates ζ. In the hyperbolic case, this cone has  sheets, and the axis  λξ}} runs inside these sheets: it does not intersect any of them. But when displaced from the origin by η, this axis intersects every sheet. In the elliptic case, the normal cone has no real sheets.&lt;br /&gt;
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如果在该点存在一个法向量为 {{mvar|ξ}}的 '''&amp;lt;font color=&amp;quot;#ff8000&amp;quot;&amp;gt;类空曲面 Spacclike Surface&amp;lt;/font&amp;gt; {{mvar|S}} ，则一阶系统在那一点是双曲的。这意味着，给定任意正交于 {{mvar|ξ}} 的非平凡向量 {{mvar|η}} 和一个标量乘子 {{mvar|λ}}，方程 {{math|''Q''(''λξ'' + ''η'') {{=}} 0}} 有 {{mvar|m}} 个实根 {{math|''λ''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;, ''λ''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;,… ''λ''&amp;lt;sub&amp;gt;''m''&amp;lt;/sub&amp;gt;}}。如果这些根始终不同，则该系统是严格双曲形的。这个条件的几何解释如下: 特征形式 {{math|''Q''(''ζ'') {{=}} 0}} 定义了一个具有齐次坐标 ζ的圆锥(法线圆锥)。在双曲形的情况下，这个圆锥体有 {{mvar|m}} 层，并且轴 {{math|''ζ'' {{=}} ''λξ''}} 在这些层中运动: 它不与任何一层相交。但是当从原点偏离η时，这条轴线与每一层都相交。在椭圆形的情况下，法向圆锥没有实层。&lt;br /&gt;
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==[[用户:Yuling|Yuling]]（[[用户讨论:Yuling|讨论]]） sheet 这个单词也不很理解，我直译为了“层”&lt;br /&gt;
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=== Equations of mixed type ===&lt;br /&gt;
混合型方程&lt;br /&gt;
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If a PDE has coefficients that are not constant, it is possible that it will not belong to any of these categories but rather be of '''mixed type'''. A simple but important example is the [[Euler–Tricomi equation]]&lt;br /&gt;
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If a PDE has coefficients that are not constant, it is possible that it will not belong to any of these categories but rather be of mixed type. A simple but important example is the Euler–Tricomi equation&lt;br /&gt;
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如果偏微分方程的系数不是常数，那么它可能不属于这些类别中的任何一个，而是属于混合类型。一个简单但重要的例子是欧拉-特里科米方程&lt;br /&gt;
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: &amp;lt;math&amp;gt;u_{xx} = xu_{yy},&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;u_{xx} = xu_{yy},&amp;lt;/math&amp;gt;&lt;br /&gt;
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which is called '''elliptic-hyperbolic''' because it is elliptic in the region {{math|''x'' &amp;lt; 0}}, hyperbolic in the region {{math|''x'' &amp;gt; 0}}, and degenerate parabolic on the line {{math|''x'' {{=}} 0}}.&lt;br /&gt;
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which is called elliptic-hyperbolic because it is elliptic in the region , hyperbolic in the region , and degenerate parabolic on the line  0}}.&lt;br /&gt;
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它在 {{math|''x'' &amp;lt; 0}} 的区域上是椭圆形，在 {{math|''x'' &amp;gt; 0}} 区域上是双曲形，在 {{math|''x'' {{=}} 0}}这条线上是退化为抛物线形，因此称之为椭圆-双曲型。&lt;br /&gt;
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''fill in: Dirichlet and Neumann boundaries, hyperbolic/parabolic/elliptic separation of variables, [[Fourier analysis]], [[Green's function]]s ...--&amp;gt;&lt;br /&gt;
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fill in: Dirichlet and Neumann boundaries, hyperbolic/parabolic/elliptic separation of variables, Fourier analysis, Green's functions ...--&amp;gt;&lt;br /&gt;
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填写: Dirichlet 和 Neumann 边界，双曲 / 抛物线 / 椭圆分离变量法，傅立叶分析，Green 函数... --&lt;br /&gt;
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=== Infinite-order PDEs in quantum mechanics ===&lt;br /&gt;
量子力学中的无限阶偏微分方程&lt;br /&gt;
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In the [[phase space formulation]] of quantum mechanics,  one may consider the [[Method of quantum characteristics|quantum Hamilton's equations]] for trajectories of quantum particles. These equations are infinite-order PDEs. However, in the semiclassical expansion, one has a finite system of ODEs at any fixed order of [[Dirac constant|{{mvar|ħ}}]].  The evolution equation of the [[Wigner quasi-probability distribution|c]] is also an infinite-order PDE. The quantum trajectories are [[Method of quantum characteristics|quantum characteristics]], with the use of which one could calculate the evolution of the Wigner function.&lt;br /&gt;
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In the phase space formulation of quantum mechanics,  one may consider the quantum Hamilton's equations for trajectories of quantum particles. These equations are infinite-order PDEs. However, in the semiclassical expansion, one has a finite system of ODEs at any fixed order of Dirac constant|.  The evolution equation of the Wigner function is also an infinite-order PDE. The quantum trajectories are quantum characteristics, with the use of which one could calculate the evolution of the Wigner function.&lt;br /&gt;
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在量子力学中的相空间表述中，我们可以考虑用于求解量子粒子的轨迹的量子哈密顿的方程。这些方程是无限阶偏微分方程。然而，在半经典展开中，我们在给定[[Dirac constant|{{mvar|ħ}}]]阶数下有一个有限的的常微分方程组。'''&amp;lt;font color=&amp;quot;#ff8000&amp;quot;&amp;gt;维格纳函数  Wigner Function&amp;lt;/font&amp;gt;的演化方程也是一个无限阶偏微分方程。由于量子轨道的量子特性，所以它通常可以用来计算维格纳函数的演化。&lt;br /&gt;
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== Analytical solutions ==&lt;br /&gt;
解析解&lt;br /&gt;
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===Separation of variables===&lt;br /&gt;
分离变量法&lt;br /&gt;
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{{main|Separable partial differential equation}}&lt;br /&gt;
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Linear PDEs can be reduced to systems of ordinary differential equations by the important technique of separation of variables. This technique rests on a characteristic of solutions to differential equations: if one can find any solution that solves the equation and satisfies the boundary conditions, then it is ''the'' solution (this also applies to ODEs). We assume as an [[ansatz]] that the dependence of a solution on the parameters space and time can be written as a product of terms that each depend on a single parameter, and then see if this can be made to solve the problem.&amp;lt;ref&amp;gt;{{cite book|last1=Gershenfeld|first1=Neil|title=The nature of mathematical modeling|date=2000|publisher=Cambridge Univ. Press|location=Cambridge|isbn=0521570956|page=27|edition=Reprinted (with corr.)}}&amp;lt;/ref&amp;gt;&lt;br /&gt;
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Linear PDEs can be reduced to systems of ordinary differential equations by the important technique of separation of variables. This technique rests on a characteristic of solutions to differential equations: if one can find any solution that solves the equation and satisfies the boundary conditions, then it is the solution (this also applies to ODEs). We assume as an ansatz that the dependence of a solution on the parameters space and time can be written as a product of terms that each depend on a single parameter, and then see if this can be made to solve the problem.&lt;br /&gt;
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线性偏微分方程组可以通过分离变量法这一重要方法来简化为常微分方程组。这种方法依赖于微分方程解的一个特征: 如果能找到任何一个满足方程和边界条件的解，那么这个解就是方程的解(这也适用于常微分方程)。我们假设解对参数空间和时间的依赖可以写成对它们每一项的依赖以及一个参数的乘积，然后再看看这是否可以用来解决这个问题。&lt;br /&gt;
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In the method of separation of variables, one reduces a PDE to a PDE in fewer variables, which is an ordinary differential equation if in one variable – these are in turn easier to solve.&lt;br /&gt;
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In the method of separation of variables, one reduces a PDE to a PDE in fewer variables, which is an ordinary differential equation if in one variable – these are in turn easier to solve.&lt;br /&gt;
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在分离变量法方法中，可以将偏微分方程简化为含有更少变量的偏微分方程，如果只有一个变量，那么就变成了一个'''&amp;lt;font color = &amp;quot;#ff8000&amp;quot;&amp;gt;常微分方程 Ordinary Differential Equation&amp;lt;/font&amp;gt;'''-- 反过来，这些方程也更容易求解。&lt;br /&gt;
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This is possible for simple PDEs, which are called [[separable partial differential equation]]s, and the domain is generally a rectangle (a product of intervals). Separable PDEs correspond to [[diagonal matrices]] – thinking of &amp;quot;the value for fixed {{mvar|x}}&amp;quot; as a coordinate, each coordinate can be understood separately.&lt;br /&gt;
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This is possible for simple PDEs, which are called separable partial differential equations, and the domain is generally a rectangle (a product of intervals). Separable PDEs correspond to diagonal matrices – thinking of &amp;quot;the value for fixed &amp;quot; as a coordinate, each coordinate can be understood separately.&lt;br /&gt;
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对于简单的偏微分方程(称为可分离偏微分方程)来说，这是可能的，而且方程通常定义在一个矩形区域(区间的乘积)上。可分离偏微分方程对应于对角线矩阵——以“固定值”为坐标，每个坐标可分开理解。&lt;br /&gt;
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This generalizes to the [[method of characteristics]], and is also used in [[integral transform]]s.&lt;br /&gt;
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This generalizes to the method of characteristics, and is also used in integral transforms.&lt;br /&gt;
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这种方法可以推广到特征曲线法，也可以用于积分变换。&lt;br /&gt;
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===Method of characteristics===&lt;br /&gt;
特征曲线法&lt;br /&gt;
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{{main|Method of characteristics}}&lt;br /&gt;
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In special cases, one can find characteristic curves on which the equation reduces to an ODE – changing coordinates in the domain to straighten these curves allows separation of variables, and is called the [[method of characteristics]].&lt;br /&gt;
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In special cases, one can find characteristic curves on which the equation reduces to an ODE – changing coordinates in the domain to straighten these curves allows separation of variables, and is called the method of characteristics.&lt;br /&gt;
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在特殊情况下，可以找到一些特征曲线，在这些曲线上方程可以变成一个常微分方程——意味着改变坐标从而使这些曲线变直从而达到分离变量的目的，这就是所谓的特征曲线法。&lt;br /&gt;
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More generally, one may find characteristic surfaces.&lt;br /&gt;
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More generally, one may find characteristic surfaces.&lt;br /&gt;
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更一般地说，人们可能会找到特征表面。&lt;br /&gt;
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===Integral transform===&lt;br /&gt;
积分变换&lt;br /&gt;
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An [[integral transform]] may transform the PDE to a simpler one, in particular, a separable PDE. This corresponds to diagonalizing an operator.&lt;br /&gt;
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An integral transform may transform the PDE to a simpler one, in particular, a separable PDE. This corresponds to diagonalizing an operator.&lt;br /&gt;
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积分变换可以将偏微分方程转换为更简单的偏微分方程，特别是可分离的偏微分方程。这对应于对角化算符。&lt;br /&gt;
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An important example of this is [[Fourier analysis]], which diagonalizes the heat equation using the [[eigenbasis]] of sinusoidal waves.&lt;br /&gt;
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An important example of this is Fourier analysis, which diagonalizes the heat equation using the eigenbasis of sinusoidal waves.&lt;br /&gt;
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这方面的一个重要例子是'''&amp;lt;font color = &amp;quot;#ff8000&amp;quot;&amp;gt;傅里叶分析  Fourier Analysis&amp;lt;/font&amp;gt;'''，它使用正弦波的特征基来对角化热方程。&lt;br /&gt;
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If the domain is finite or periodic, an infinite sum of solutions such as a [[Fourier series]] is appropriate, but an integral of solutions such as a [[Fourier integral]] is generally required for infinite domains. The solution for a point source for the heat equation given above is an example of the use of a Fourier integral.&lt;br /&gt;
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If the domain is finite or periodic, an infinite sum of solutions such as a Fourier series is appropriate, but an integral of solutions such as a Fourier integral is generally required for infinite domains. The solution for a point source for the heat equation given above is an example of the use of a Fourier integral.&lt;br /&gt;
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如果区域是有限的或周期性的，那么解为无限和的形式是恰当的，例如傅里叶级数，但是一个解的积分，例如傅立叶积分，一般是在无限区域上的。上面给出的热传导方程的点源解法就是使用傅里叶积分的一个例子。&lt;br /&gt;
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===Change of variables===&lt;br /&gt;
变量代换&lt;br /&gt;
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Often a PDE can be reduced to a simpler form with a known solution by a suitable [[Change of variables (PDE)|change of variables]].  For example, the [[Black–Scholes equation#Derivation|Black–Scholes]] PDE&lt;br /&gt;
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Often a PDE can be reduced to a simpler form with a known solution by a suitable change of variables.  For example, the Black–Scholes PDE&lt;br /&gt;
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偏微分方程通常可以通过变量的适当变化，用已知的解简化为更简单的形式。例如，布莱克-舒尔斯偏微分方程&lt;br /&gt;
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:&amp;lt;math&amp;gt; \frac{\partial V}{\partial t} + \tfrac{1}{2}\sigma^2 S^2\frac{\partial^2 V}{\partial S^2} + rS\frac{\partial V}{\partial S} - rV = 0 &amp;lt;/math&amp;gt;&lt;br /&gt;
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&amp;lt;math&amp;gt; \frac{\partial V}{\partial t} + \tfrac{1}{2}\sigma^2 S^2\frac{\partial^2 V}{\partial S^2} + rS\frac{\partial V}{\partial S} - rV = 0 &amp;lt;/math&amp;gt;&lt;br /&gt;
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is reducible to the [[heat equation]]&lt;br /&gt;
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is reducible to the heat equation&lt;br /&gt;
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可以简化为热传导方程&lt;br /&gt;
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:&amp;lt;math&amp;gt; \frac{\partial u}{\partial \tau} = \frac{\partial^2 u}{\partial x^2}&amp;lt;/math&amp;gt;&lt;br /&gt;
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&amp;lt;math&amp;gt; \frac{\partial u}{\partial \tau} = \frac{\partial^2 u}{\partial x^2}&amp;lt;/math&amp;gt;&lt;br /&gt;
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by the change of variables (for complete details see {{webarchive |url=https://web.archive.org/web/20080411030405/http://www.math.unl.edu/~sdunbar1/Teaching/MathematicalFinance/Lessons/BlackScholes/Solution/solution.shtml |date=April 11, 2008 |title=Solution of the Black Scholes Equation }})&lt;br /&gt;
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by the change of variables (for complete details see )&lt;br /&gt;
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通过变量替换(完整的细节见)&lt;br /&gt;
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:&amp;lt;math&amp;gt;\begin{align}&lt;br /&gt;
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V(S,t) &amp;amp;= K v(x,\tau),\\[5px]&lt;br /&gt;
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x &amp;amp;= \ln\left(\tfrac{S}{K} \right),\\[5px]&lt;br /&gt;
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\tau &amp;amp;= \tfrac{1}{2} \sigma^2 (T - t),\\[5px]&lt;br /&gt;
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v(x,\tau)&amp;amp;=e^{-\alpha x-\beta\tau} u(x,\tau).&lt;br /&gt;
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\end{align}&amp;lt;/math&amp;gt;&lt;br /&gt;
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===Fundamental solution===&lt;br /&gt;
基本解&lt;br /&gt;
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{{main|Fundamental solution}}&lt;br /&gt;
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Inhomogeneous equations can often be solved (for constant coefficient PDEs, always be solved) by finding the [[fundamental solution]] (the solution for a point source), then taking the [[convolution]] with the boundary conditions to get the solution.&lt;br /&gt;
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Inhomogeneous equations can often be solved (for constant coefficient PDEs, always be solved) by finding the fundamental solution (the solution for a point source), then taking the convolution with the boundary conditions to get the solution.&lt;br /&gt;
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非齐次方程(常系数偏微分方程)一般是通过先求出基本解(点源的解) ，然后利用带边界条件的卷积来求解。&lt;br /&gt;
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This is analogous in [[signal processing]] to understanding a filter by its [[impulse response]].&lt;br /&gt;
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This is analogous in signal processing to understanding a filter by its impulse response.&lt;br /&gt;
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这类似于在信号处理中通过滤波器的脉冲响应来理解滤波器。&lt;br /&gt;
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===Superposition principle===&lt;br /&gt;
叠加原理&lt;br /&gt;
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{{further| Superposition principle }}&lt;br /&gt;
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The superposition principle applies to any linear system, including linear systems of PDEs. A common visualization of this concept is the interaction of two waves in phase being combined to result in a greater amplitude, for example {{math|sin ''x'' + sin ''x'' {{=}} 2 sin ''x''}}. The same principle can be observed in PDEs where the solutions may be real or complex and additive. [[Superposition principle|superposition]]&lt;br /&gt;
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The superposition principle applies to any linear system, including linear systems of PDEs. A common visualization of this concept is the interaction of two waves in phase being combined to result in a greater amplitude, for example  2 sin x}}. The same principle can be observed in PDEs where the solutions may be real or complex and additive. superposition&lt;br /&gt;
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'''&amp;lt;font color = &amp;quot;#ff8000&amp;quot;&amp;gt;叠加原理 Superposition Principle&amp;lt;/font&amp;gt;适用于任何线性系统，包括偏微分方程的线性系统。这个概念的一个常见的可视化是两个同相位的波相互作用结合在一起会产生更大的振幅，例如 {{math|sin ''x'' + sin ''x'' {{=}} 2 sin ''x''}}。在偏微分方程中也可以观察到同样的原理，其中的解可能是真实的或复杂的和可加的。叠加&lt;br /&gt;
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If {{math|''u''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;}} and {{math|''u''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;}} are solutions of linear PDE in some function space {{mvar|R}}, then {{math|''u'' {{=}} ''c''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;''u''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; + ''c''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;''u''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;}} with any constants {{math|''c''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;}} and {{math|''c''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;}} are also a solution of that PDE in the same function space.&lt;br /&gt;
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If  and  are solutions of linear PDE in some function space , then  c&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;u&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; + c&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;u&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;}} with any constants  and  are also a solution of that PDE in the same function space.&lt;br /&gt;
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若线性偏微分方程在某个函数空间{{mvar|R}}中有解{{math|''u''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;}} 和 {{math|''u''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;}}，则{{math|''u'' {{=}} ''c''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;''u''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; + ''c''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;''u''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;}}也是该偏微分方程在同一函数空间中的解，其中{{math|''c''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;}} 和 {{math|''c''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;}} 是任意常数。&lt;br /&gt;
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===Methods for non-linear equations===&lt;br /&gt;
非线性方程的求解方法&lt;br /&gt;
{{see also|nonlinear partial differential equation}}&lt;br /&gt;
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There are no generally applicable methods to solve nonlinear PDEs. Still, existence and uniqueness results (such as the [[Cauchy–Kowalevski theorem]]) are often possible, as are proofs of important qualitative and quantitative properties of solutions (getting these results is a major part of [[mathematical analysis|analysis]]). Computational solution to the nonlinear PDEs, the [[split-step method]], exist for specific equations like [[nonlinear Schrödinger equation]].&lt;br /&gt;
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There are no generally applicable methods to solve nonlinear PDEs. Still, existence and uniqueness results (such as the Cauchy–Kowalevski theorem) are often possible, as are proofs of important qualitative and quantitative properties of solutions (getting these results is a major part of analysis). Computational solution to the nonlinear PDEs, the split-step method, exist for specific equations like nonlinear Schrödinger equation.&lt;br /&gt;
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对于非线性偏微分方程，目前还没有普遍适用的求解方法。然而，通常是可能知道解的存在性和唯一性(如柯西-科瓦列夫斯基定理)，也是可能得到解的重要定性和定量性质的证明(得到这些结果是分析的主要部分)。非线性偏微分方程的计算解，即分步法，对一些特定的方程适用，比如非线性'''&amp;lt;font color=&amp;quot;#ff8000&amp;quot;&amp;gt;薛定谔方程 Schrödinger equation&amp;lt;/font&amp;gt;'''。&lt;br /&gt;
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Nevertheless, some techniques can be used for several types of equations. The [[h-principle|{{mvar|h}}-principle]] is the most powerful method to solve [[Underdetermined system|underdetermined]] equations. The [[Riquier–Janet theory]] is an effective method for obtaining information about many analytic [[Overdetermined system|overdetermined]] systems.&lt;br /&gt;
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Nevertheless, some techniques can be used for several types of equations. The -principle is the most powerful method to solve underdetermined equations. The Riquier–Janet theory is an effective method for obtaining information about many analytic overdetermined systems.&lt;br /&gt;
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然而，一些技巧可以用于几种类型的方程。h-原理是求解欠定方程最有效的方法。里基尔-珍妮特理论是一种可以获得许多解析超定系统信息的有效方法。&lt;br /&gt;
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The [[method of characteristics]] can be used in some very special cases to solve partial differential equations.&lt;br /&gt;
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The method of characteristics can be used in some very special cases to solve partial differential equations.&lt;br /&gt;
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特征线法可用于求解某些特殊情况下的偏微分方程。&lt;br /&gt;
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In some cases, a PDE can be solved via [[perturbation analysis]] in which the solution is considered to be a correction to an equation with a known solution. Alternatives are [[numerical analysis]] techniques from simple [[finite difference]] schemes to the more mature [[multigrid]] and [[finite element method]]s. Many interesting problems in science and engineering are solved in this way using [[computer]]s, sometimes high performance [[supercomputer]]s.&lt;br /&gt;
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In some cases, a PDE can be solved via perturbation analysis in which the solution is considered to be a correction to an equation with a known solution. Alternatives are numerical analysis techniques from simple finite difference schemes to the more mature multigrid and finite element methods. Many interesting problems in science and engineering are solved in this way using computers, sometimes high performance supercomputers.&lt;br /&gt;
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在某些情况下，偏微分方程可以通过扰动分析来求解。在扰动分析中，通常是求解将具有已知解的方程修正后的新得到方程。可供选择的数值分析技术从简单的差分格式到更成熟的多重网格和有限元方法。许多有趣的科学和工程问题都是在计算机上用这种方法解决的，有时是高性能超级计算机。&lt;br /&gt;
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===Lie group method===&lt;br /&gt;
李群方法&lt;br /&gt;
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From 1870 [[Sophus Lie]]'s work put the theory of differential equations on a more satisfactory foundation. He showed that the integration theories of the older mathematicians can, by the introduction of what are now called [[Lie group]]s, be referred, to a common source; and that ordinary differential equations which admit the same [[infinitesimal transformation]]s present comparable difficulties of integration. He also emphasized the subject of [[contact transformation|transformations of contact]].&lt;br /&gt;
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From 1870 Sophus Lie's work put the theory of differential equations on a more satisfactory foundation. He showed that the integration theories of the older mathematicians can, by the introduction of what are now called Lie groups, be referred, to a common source; and that ordinary differential equations which admit the same infinitesimal transformations present comparable difficulties of integration. He also emphasized the subject of transformations of contact.&lt;br /&gt;
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从1870年起，索弗斯·李的工作为微分方程理论奠定了一个较为令人满意的基础。他指出，通过引入现在所谓的李群，老一辈数学家的积分理论可以引用到一个共同的来源; 承认相同的无穷小变换的常微分方程在积分方面存在相当的困难。他还强调了接触的转变这一主题。&lt;br /&gt;
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==[[用户:Yuling|Yuling]]（[[用户讨论:Yuling|讨论]]）这句话“He also emphasized the subject of transformations of contact.”中的transformations of contact翻译的不太好。&lt;br /&gt;
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A general approach to solving PDEs uses the symmetry property of differential equations, the continuous [[infinitesimal transformation]]s of solutions to solutions ([[Lie theory]]). Continuous [[group theory]], [[Lie algebras]] and [[differential geometry]] are used to understand the structure of linear and nonlinear partial differential equations for generating integrable equations, to find its [[Lax pair]]s, recursion operators, [[Bäcklund transform]] and finally finding exact analytic solutions to the PDE.&lt;br /&gt;
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A general approach to solving PDEs uses the symmetry property of differential equations, the continuous infinitesimal transformations of solutions to solutions (Lie theory). Continuous group theory, Lie algebras and differential geometry are used to understand the structure of linear and nonlinear partial differential equations for generating integrable equations, to find its Lax pairs, recursion operators, Bäcklund transform and finally finding exact analytic solutions to the PDE.&lt;br /&gt;
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求解偏微分方程的一般方法是利用微分方程的对称性，即解到解的连续无穷小变换(李理论)。连续群论、李代数和微分几何理论被用来理解生成可积方程的线性和非线性偏微分方程的结构，找到它的Lax对、递归算子、 贝克伦德变换，最后找到偏微分方程的精确解析解。&lt;br /&gt;
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Symmetry methods have been recognized to study differential equations arising in mathematics, physics, engineering, and many other disciplines.&lt;br /&gt;
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Symmetry methods have been recognized to study differential equations arising in mathematics, physics, engineering, and many other disciplines.&lt;br /&gt;
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对称方法已被公认可以用于研究出现在数学，物理，工程和许多其他学科的微分方程。&lt;br /&gt;
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===Semianalytical methods===&lt;br /&gt;
半解析方法&lt;br /&gt;
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The [[Adomian decomposition method]], the [[Aleksandr Lyapunov|Lyapunov]] artificial small parameter method, and He's [[homotopy perturbation method]] are all special cases of the more general [[homotopy analysis method]]. These are series expansion methods, and except for the Lyapunov method, are independent of small physical parameters as compared to the well known [[perturbation theory]], thus giving these methods greater flexibility and solution generality.&lt;br /&gt;
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The Adomian decomposition method, the Lyapunov artificial small parameter method, and He's homotopy perturbation method are all special cases of the more general homotopy analysis method. These are series expansion methods, and except for the Lyapunov method, are independent of small physical parameters as compared to the well known perturbation theory, thus giving these methods greater flexibility and solution generality.&lt;br /&gt;
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阿多米安分解法、李雅普诺夫人工小参数方法和何同伦摄动方法都是更一般的同伦分析方法的特殊情况。除了李雅普诺夫方法之外，这些都是级数展开方法，与为人熟知的摄动理论方法相比，它们与小的物理参数无关，因此这些方法具有更大的灵活性和解的通用性。&lt;br /&gt;
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== Numerical solutions ==&lt;br /&gt;
数值解&lt;br /&gt;
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The three most widely used [[Numerical partial differential equations|numerical methods to solve PDEs]] are the [[finite element analysis|finite element method]] (FEM), [[finite volume method]]s (FVM) and [[finite difference method]]s (FDM), as well other kind of methods called [[Meshfree methods]], which were made to solve problems where the before mentioned methods are limited. The FEM has a prominent position among these methods and especially its exceptionally efficient higher-order version [[hp-FEM]]. Other hybrid versions of FEM and Meshfree methods include the generalized finite element method (GFEM), [[extended finite element method]] (XFEM), [[Spectral element method|spectral finite element method]] (SFEM), [[Meshfree methods|meshfree finite element method]], [[Discontinuous Galerkin Method|discontinuous Galerkin finite element method]] (DGFEM), [[Element-Free Galerkin Method]] (EFGM), [[Interpolating Element-Free Galerkin Method]] (IEFGM), etc.&lt;br /&gt;
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The three most widely used numerical methods to solve PDEs are the finite element method (FEM), finite volume methods (FVM) and finite difference methods (FDM), as well other kind of methods called Meshfree methods, which were made to solve problems where the before mentioned methods are limited. The FEM has a prominent position among these methods and especially its exceptionally efficient higher-order version hp-FEM. Other hybrid versions of FEM and Meshfree methods include the generalized finite element method (GFEM), extended finite element method (XFEM), spectral finite element method (SFEM), meshfree finite element method, discontinuous Galerkin finite element method (DGFEM), Element-Free Galerkin Method (EFGM), Interpolating Element-Free Galerkin Method (IEFGM), etc.&lt;br /&gt;
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求解偏微分方程最常用的三种数值方法是有限元分析法、有限体积法和有限差分法，以及其他一些称为无网格法的方法。这些方法用于解决前面提到的方法受到的限制。在这些方法中，有限元方法，尤其是高效的高阶有限元方法，占有重要地位。其他有限元法和无网格法的混合形式包括广义有限元分析法(GFEM)、扩展有限元分析法(XFEM)、谱有限元分析法(SFEM)、无网格有限元分析法(DGFEM)、间断伽辽金有限元分析法(DGFEM)、无网格伽辽金法(EFGM)、插值无网格伽辽金法(IEFGM)等。&lt;br /&gt;
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=== Finite element method ===&lt;br /&gt;
有限元分析法&lt;br /&gt;
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{{main|Finite element method}}&lt;br /&gt;
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The finite element method (FEM) (its practical application often known as finite element analysis (FEA)) is a numerical technique for finding approximate solutions of partial differential equations (PDE) as well as of integral equations. The solution approach is based either on eliminating the differential equation completely (steady state problems), or rendering the PDE into an approximating system of ordinary differential equations, which are then numerically integrated using standard techniques such as Euler's method, Runge–Kutta, etc.&lt;br /&gt;
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The finite element method (FEM) (its practical application often known as finite element analysis (FEA)) is a numerical technique for finding approximate solutions of partial differential equations (PDE) as well as of integral equations. The solution approach is based either on eliminating the differential equation completely (steady state problems), or rendering the PDE into an approximating system of ordinary differential equations, which are then numerically integrated using standard techniques such as Euler's method, Runge–Kutta, etc.&lt;br /&gt;
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'''&amp;lt;font color = &amp;quot;#ff8000&amp;quot;&amp;gt;有限元分析法 Finite Element Method&amp;lt;/font&amp;gt;''' ((其实际应用通常被称为有限元分析(FEA))是一种寻找偏微分方程(PDE)和积分方程近似解的数值技术。这种求解方法要么基于完全消除微分方程(稳态问题) ，要么将偏微分方程转化为常微分方程的近似系统，然后使用标准技术进行数值积分，如欧拉方法、 Runge-Kutta 等。&lt;br /&gt;
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===Finite difference method===&lt;br /&gt;
有限差分法&lt;br /&gt;
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{{main|Finite difference method}}&lt;br /&gt;
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Finite-difference methods are numerical methods for approximating the solutions to differential equations using [[finite difference]] equations to approximate derivatives.&lt;br /&gt;
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Finite-difference methods are numerical methods for approximating the solutions to differential equations using finite difference equations to approximate derivatives.&lt;br /&gt;
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有限差分法是一种数值方法，用差分方程近似微分方程的解。&lt;br /&gt;
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=== Finite volume method ===&lt;br /&gt;
有限体积法&lt;br /&gt;
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{{main|Finite volume method}}&lt;br /&gt;
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Similar to the finite difference method or finite element method, values are calculated at discrete places on a meshed geometry. &amp;quot;Finite volume&amp;quot; refers to the small volume surrounding each node point on a mesh. In the finite volume method, surface integrals in a partial differential equation that contain a divergence term are converted to volume integrals, using the [[divergence theorem]]. These terms are then evaluated as fluxes at the surfaces of each finite volume. Because the flux entering a given volume is identical to that leaving the adjacent volume, these methods conserve mass by design.&lt;br /&gt;
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Similar to the finite difference method or finite element method, values are calculated at discrete places on a meshed geometry. &amp;quot;Finite volume&amp;quot; refers to the small volume surrounding each node point on a mesh. In the finite volume method, surface integrals in a partial differential equation that contain a divergence term are converted to volume integrals, using the divergence theorem. These terms are then evaluated as fluxes at the surfaces of each finite volume. Because the flux entering a given volume is identical to that leaving the adjacent volume, these methods conserve mass by design.&lt;br /&gt;
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类似于有限差分法或有限元分析，函数值是在网状几何体上的离散位置进行计算的。“有限体积”是指网格上每个节点周围的小体积。在有限体积法中，偏微分方程中含有散度项的面积分用散度定理积分转换成体积分。然后将这些项用于估算每个有限体积表面上的通量。由于进入给定体积的通量与转移到相邻体积元的通量相同，所以这些方法在设计上保证了质量守恒。&lt;br /&gt;
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==See also==&lt;br /&gt;
请参阅&lt;br /&gt;
* [[Dirichlet boundary condition]]&lt;br /&gt;
狄利克雷边界条件&lt;br /&gt;
* [[Jet bundle]]&lt;br /&gt;
射流丛&lt;br /&gt;
* [[Laplace transform applied to differential equations]]&lt;br /&gt;
微分方程中的拉普拉斯变换&lt;br /&gt;
* [[List of dynamical systems and differential equations topics]]&lt;br /&gt;
动力学系统和微分方程的列表&lt;br /&gt;
* [[Matrix differential equation]]&lt;br /&gt;
矩阵微分方程&lt;br /&gt;
* [[Neumann boundary condition]]&lt;br /&gt;
诺伊曼边界条件&lt;br /&gt;
* [[Numerical partial differential equations]]&lt;br /&gt;
数值偏微分方程&lt;br /&gt;
* [[Partial differential algebraic equation]]&lt;br /&gt;
偏微分代数方程&lt;br /&gt;
* [[Recurrence relation]]&lt;br /&gt;
递推关系&lt;br /&gt;
* [[Robin boundary condition]]&lt;br /&gt;
罗宾边界条件&lt;br /&gt;
* [[Stochastic processes and boundary value problems]]&lt;br /&gt;
随机过程和边值问题&lt;br /&gt;
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== The energy method ==&lt;br /&gt;
能量法&lt;br /&gt;
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The energy method is a mathematical procedure that can be used to verify well-posedness of initial-boundary-value-problems.&amp;lt;ref&amp;gt;{{cite book |title=High Order Difference Methods for Time Dependent PDE&lt;br /&gt;
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The energy method is a mathematical procedure that can be used to verify well-posedness of initial-boundary-value-problems.&amp;lt;ref&amp;gt;{{cite book |title=High Order Difference Methods for Time Dependent PDE&lt;br /&gt;
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能量法是验证初边值问题适定性的一种数学方法。 时变偏微分方程的高阶差分方法&lt;br /&gt;
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|first=Bertil|last=Gustafsson|publisher=Springer|year=2008|isbn=978-3-540-74992-9|doi=10.1007/978-3-540-74993-6}}&amp;lt;/ref&amp;gt; In the following example the energy method is used to decide where and which boundary conditions should be imposed such that the resulting IBVP is well-posed. Consider the one-dimensional hyperbolic PDE given by&lt;br /&gt;
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|first=Bertil|last=Gustafsson|publisher=Springer|year=2008|isbn=978-3-540-74992-9|doi=10.1007/978-3-540-74993-6}}&amp;lt;/ref&amp;gt; In the following example the energy method is used to decide where and which boundary conditions should be imposed such that the resulting IBVP is well-posed. Consider the one-dimensional hyperbolic PDE given by&lt;br /&gt;
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| first Bertil | last Gustafsson | publisher | Springer | year 2008 | isbn 978-3-540-74992-9 | doi 10.1007 / 978-3-540-74993-6} / ref 在下面的例子中，使用能量方法来决定应该施加哪些边界条件，使得得到的 IBVP适定。考虑一维双曲偏微分方程&lt;br /&gt;
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: &amp;lt;math&amp;gt;\frac{\partial u}{\partial t} + \alpha \frac{\partial u}{\partial x} = 0, \quad x \in [a,b], \operatorname t &amp;gt; 0,&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;\frac{\partial u}{\partial t} + \alpha \frac{\partial u}{\partial x} = 0, \quad x \in [a,b], \operatorname t &amp;gt; 0,&amp;lt;/math&amp;gt;&lt;br /&gt;
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where &amp;lt;math&amp;gt;\alpha \neq 0&amp;lt;/math&amp;gt; is a constant and &amp;lt;math&amp;gt;u(x,t)&amp;lt;/math&amp;gt; is an unknown function with initial condition &amp;lt;math&amp;gt;u(x,0) = f(x)&amp;lt;/math&amp;gt;. Multiplying with &amp;lt;math&amp;gt;u&amp;lt;/math&amp;gt; and integrating over the domain gives&lt;br /&gt;
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where &amp;lt;math&amp;gt;\alpha \neq 0&amp;lt;/math&amp;gt; is a constant and &amp;lt;math&amp;gt;u(x,t)&amp;lt;/math&amp;gt; is an unknown function with initial condition &amp;lt;math&amp;gt;u(x,0) = f(x)&amp;lt;/math&amp;gt;. Multiplying with &amp;lt;math&amp;gt;u&amp;lt;/math&amp;gt; and integrating over the domain gives&lt;br /&gt;
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其中 &amp;lt;math&amp;gt;\alpha \neq 0&amp;lt;/math&amp;gt; 是常数，并且 &amp;lt;math&amp;gt;u(x,t)&amp;lt;/math&amp;gt; 是未知函数，初始条件是 &amp;lt;math&amp;gt;u(x,0) = f(x)&amp;lt;/math&amp;gt;。乘以 &amp;lt;math&amp;gt;u&amp;lt;/math&amp;gt; 并在域上进行积分。&lt;br /&gt;
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: &amp;lt;math&amp;gt;\int_a^b u \frac{\partial u}{\partial t} \operatorname dx + \alpha \int _a ^b u \frac{\partial u}{\partial x} \operatorname dx = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;\int_a^b u \frac{\partial u}{\partial t} \operatorname dx + \alpha \int _a ^b u \frac{\partial u}{\partial x} \operatorname dx = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
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Using that&lt;br /&gt;
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Using that&lt;br /&gt;
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利用这一点&lt;br /&gt;
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: &amp;lt;math&amp;gt;\int _a ^b u \frac{\partial u}{\partial t} \operatorname dx = \frac{1}{2} \frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 \quad \text{and} \quad \int _a ^b u \frac{\partial u}{\partial x} \operatorname dx = \frac{1}{2} u(b,t)^2 - \frac{1}{2} u(a,t)^2,.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;\int _a ^b u \frac{\partial u}{\partial t} \operatorname dx = \frac{1}{2} \frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 \quad \text{and} \quad \int _a ^b u \frac{\partial u}{\partial x} \operatorname dx = \frac{1}{2} u(b,t)^2 - \frac{1}{2} u(a,t)^2,.&amp;lt;/math&amp;gt;&lt;br /&gt;
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where integration by parts has been used for the second relationship, we get&lt;br /&gt;
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where integration by parts has been used for the second relationship, we get&lt;br /&gt;
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第二个关系中采用了分部积分法，我们可以得到&lt;br /&gt;
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: &amp;lt;math&amp;gt;\frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 + \alpha u(b,t)^2 - \alpha u(a,t)^2 = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;\frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 + \alpha u(b,t)^2 - \alpha u(a,t)^2 = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
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Here &amp;lt;math&amp;gt;\vert \vert \cdot \vert \vert&amp;lt;/math&amp;gt; denotes the standard L2-norm.&lt;br /&gt;
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Here &amp;lt;math&amp;gt;\vert \vert \cdot \vert \vert&amp;lt;/math&amp;gt; denotes the standard L2-norm.&lt;br /&gt;
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在这里，&amp;lt;math&amp;gt;\vert \vert \cdot \vert \vert&amp;lt;/math&amp;gt; 表示标准的 L2-正则。&lt;br /&gt;
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For well-posedness we require that the energy of the solution is non-increasing, i.e. that &amp;lt;math&amp;gt;\frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 \leq 0&amp;lt;/math&amp;gt;, which is achieved by specifying &amp;lt;math&amp;gt;u&amp;lt;/math&amp;gt; at &amp;lt;math&amp;gt;x = a&amp;lt;/math&amp;gt; if &amp;lt;math&amp;gt;\alpha &amp;gt; 0&amp;lt;/math&amp;gt; and at &amp;lt;math&amp;gt;x = b&amp;lt;/math&amp;gt; if &amp;lt;math&amp;gt;\alpha &amp;lt; 0&amp;lt;/math&amp;gt;. This corresponds to only imposing boundary conditions at the inflow. Note that well-posedness allows for growth in terms of data (initial and boundary) and thus it is sufficient to show that &amp;lt;math&amp;gt;\frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 \leq 0&amp;lt;/math&amp;gt; holds when all data is set to zero.&lt;br /&gt;
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For well-posedness we require that the energy of the solution is non-increasing, i.e. that &amp;lt;math&amp;gt;\frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 \leq 0&amp;lt;/math&amp;gt;, which is achieved by specifying &amp;lt;math&amp;gt;u&amp;lt;/math&amp;gt; at &amp;lt;math&amp;gt;x = a&amp;lt;/math&amp;gt; if &amp;lt;math&amp;gt;\alpha &amp;gt; 0&amp;lt;/math&amp;gt; and at &amp;lt;math&amp;gt;x = b&amp;lt;/math&amp;gt; if &amp;lt;math&amp;gt;\alpha &amp;lt; 0&amp;lt;/math&amp;gt;. This corresponds to only imposing boundary conditions at the inflow. Note that well-posedness allows for growth in terms of data (initial and boundary) and thus it is sufficient to show that &amp;lt;math&amp;gt;\frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 \leq 0&amp;lt;/math&amp;gt; holds when all data is set to zero.&lt;br /&gt;
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对于适定性，我们要解的能量是不增加的，即 &amp;lt;math&amp;gt;\frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 \leq 0&amp;lt;/math&amp;gt; ，这种关系可以通过在&amp;lt;math&amp;gt;x = a&amp;lt;/math&amp;gt;处 （如果 &amp;lt;math&amp;gt;\alpha &amp;gt; 0&amp;lt;/math&amp;gt;） 以及 &amp;lt;math&amp;gt;x = b&amp;lt;/math&amp;gt;处 （如果 &amp;lt;math&amp;gt;\alpha &amp;lt; 0&amp;lt;/math&amp;gt;）指定&amp;lt;math&amp;gt;u&amp;lt;/math&amp;gt;的值来实现。这只相当于在入流处附加边界条件。注意，适定性允许在数据(初始和边界)上的增长，因此它足以表明当所有数据设置为零时应有 &amp;lt;math&amp;gt;\frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 \leq 0&amp;lt;/math&amp;gt;。&lt;br /&gt;
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==[[用户:Yuling|Yuling]]（[[用户讨论:Yuling|讨论]]）“This corresponds to only imposing boundary conditions at the inflow.” 这句话中的inflow不是很理解&lt;br /&gt;
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==Notes==&lt;br /&gt;
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{{Reflist}}&lt;br /&gt;
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== References ==&lt;br /&gt;
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{{refbegin|2}}&lt;br /&gt;
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* {{cite book |title=Solving Frontier problems of Physics: The decomposition method&lt;br /&gt;
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|first=G.|last=Adomian|publisher=Kluwer Academic Publishers|year=1994|isbn=|page=|url=https://books.google.com/books?id=UKPqCAAAQBAJ&amp;amp;printsec=frontcover#v=onepage&amp;amp;q=%22partial%20differential%22&amp;amp;f=false}}&lt;br /&gt;
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1994年 | isbn | 页面 | 网址: 施普林格科学+商业媒体 https://books.google.com/books?id=ukpqcaaaqbaj&amp;amp;printsec=frontcover#v=onepage&amp;amp;q=%22partial%20differential%22&amp;amp;f=false&lt;br /&gt;
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* {{Citation |first=A. D. |last=Polyanin |title=Handbook of Linear Partial Differential Equations for Engineers and Scientists |publisher=Chapman &amp;amp; Hall/CRC Press |location=Boca Raton |year=2002 |isbn=1-58488-299-9 }}.&lt;br /&gt;
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* {{Citation |first=A. D. |last=Polyanin |lastauthoramp=yes |first2=V. F. |last2=Zaitsev |title=Handbook of Nonlinear Partial Differential Equations |publisher=Chapman &amp;amp; Hall/CRC Press |location=Boca Raton |year=2004 |isbn=1-58488-355-3 }}.&lt;br /&gt;
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* {{Citation |first=A. D. |last=Polyanin |first2=V. F. |last2=Zaitsev |lastauthoramp=yes |first3=A. |last3=Moussiaux |title=Handbook of First Order Partial Differential Equations |publisher=Taylor &amp;amp; Francis |location=London |year=2002 |isbn=0-415-27267-X }}.&lt;br /&gt;
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* {{citation|mr=3014456|last=Roubíček|first= T.|title=Nonlinear Partial Differential Equations with Applications|publisher= Birkhäuser|place= Basel, Boston, Berlin|edition=2nd|year= 2013|ISBN= 978-3-0348-0512-4|doi=10.1007/978-3-0348-0513-1|url=http://cds.cern.ch/record/880983/files/9783764372934_TOC.pdf}}&lt;br /&gt;
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* {{Citation |first=P. |last=Solin |title=Partial Differential Equations and the Finite Element Method |publisher=J. Wiley &amp;amp; Sons |location=Hoboken, NJ |year=2005 |isbn=0-471-72070-4 }}.&lt;br /&gt;
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* {{Citation |first=P. |last=Solin |first2=K. |last2=Segeth |lastauthoramp=yes |first3=I. |last3=Dolezel |title=Higher-Order Finite Element Methods |publisher=Chapman &amp;amp; Hall/CRC Press |location=Boca Raton |year=2003 |isbn=1-58488-438-X }}.&lt;br /&gt;
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* {{Citation |first=H. |last=Stephani |year=1989 |title=Differential Equations: Their Solution Using Symmetries. Edited by M. MacCallum |publisher=Cambridge University Press }}.&lt;br /&gt;
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* {{cite book |title=Partial Differential Equations and Solitary Waves Theory&lt;br /&gt;
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|first=Abdul-Majid|last=Wazwaz|publisher=Higher Education Press|year=2009|isbn=978-3-642-00251-9|page=}}&lt;br /&gt;
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|first=Abdul-Majid|last=Wazwaz|publisher=Higher Education Press|year=2009|isbn=978-3-642-00251-9|page=}}&lt;br /&gt;
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| first Abdul-Majid | last Wazwaz | publisher Higher Education Press | year 2009 | isbn 978-3-642-00251-9 | page }&lt;br /&gt;
&lt;br /&gt;
* {{cite book |title=Partial Differential Equations Methods and Applications&lt;br /&gt;
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|first=Abdul-Majid|last=Wazwaz|publisher=A.A. Balkema|year=2002|isbn=90-5809-369-7|page=}}&lt;br /&gt;
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|first=Abdul-Majid|last=Wazwaz|publisher=A.A. Balkema|year=2002|isbn=90-5809-369-7|page=}}&lt;br /&gt;
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| first Abdul-Majid | last Wazwaz | publisher a.a.Balkema | year 2002 | isbn 90-5809-369-7 | page }&lt;br /&gt;
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* {{Citation |first=D. |last=Zwillinger |title=Handbook of Differential Equations |publisher=Academic Press |location=Boston |year=1997 |edition=3rd |isbn=0-12-784395-7 }}.&lt;br /&gt;
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* {{Citation |authorlink=Neil Gershenfeld |first=N. |last=Gershenfeld |title=The Nature of Mathematical Modeling |location=New York |publisher=Cambridge University Press, New York, NY, USA |year=1999 |edition=1st |isbn=0-521-57095-6 }}.&lt;br /&gt;
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* {{Citation |first=I.S. |last=Krasil'shchik |lastauthoramp=yes |first2=A.M., Eds. |last2=Vinogradov |title=Symmetries and Conserwation Laws for Differential Equations of Mathematical Physics |publisher=American Mathematical Society, Providence, Rhode Island, USA |year=1999 |isbn=0-8218-0958-X }}.&lt;br /&gt;
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* {{Citation |first=I.S. |last=Krasil'shchik |first2=V.V. |last2=Lychagin|lastauthoramp=yes |first3=A.M. |last3=Vinogradov |title=Geometry of Jet Spaces and Nonlinear Partial Differential Equations |publisher=Gordon and Breach Science Publishers, New York, London, Paris, Montreux, Tokyo |year=1986 |isbn=2-88124-051-8 }}.&lt;br /&gt;
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* {{Citation |first=A.M. |last=Vinogradov |title=Cohomological Analysis of Partial Differential Equations and Secondary Calculus |publisher=American Mathematical Society, Providence, Rhode Island, USA |year=2001 |isbn=0-8218-2922-X }}.&lt;br /&gt;
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* {{cite book |title=High Order Difference Methods for Time Dependent PDE&lt;br /&gt;
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|first=Bertil|last=Gustafsson|publisher=Springer|year=2008|isbn=978-3-540-74992-9|doi=10.1007/978-3-540-74993-6}}&lt;br /&gt;
&lt;br /&gt;
|first=Bertil|last=Gustafsson|publisher=Springer|year=2008|isbn=978-3-540-74992-9|doi=10.1007/978-3-540-74993-6}}&lt;br /&gt;
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| first Bertil | last Gustafsson | Springer | year 2008 | isbn 978-3-540-74992-9 | doi 10.1007 / 978-3-540-74993-6}&lt;br /&gt;
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{{refend}}&lt;br /&gt;
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== Further reading ==&lt;br /&gt;
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* {{Cite journal|last=Cajori|first=Florian|authorlink=Florian Cajori|year=1928|title=The Early History of Partial Differential Equations and of Partial Differentiation and Integration|url=http://www.math.harvard.edu/archive/21a_fall_14/exhibits/cajori/cajori.pdf|journal=The American Mathematical Monthly|volume=35|issue=9|pages=459–467|doi=10.2307/2298771|access-date=2016-05-15|archive-url=https://web.archive.org/web/20181123102253/http://www.math.harvard.edu/archive/21a_fall_14/exhibits/cajori/cajori.pdf|archive-date=2018-11-23|url-status=dead}}&lt;br /&gt;
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== External links ==&lt;br /&gt;
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{{Sister project links| wikt=no | commons=Category:Solutions of PDE | b=Partial Differential Equations | n=no | q=Partial differential equation | s=no | v=no | voy=no | species=no | d=no}}&lt;br /&gt;
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* {{springer|title=Differential equation, partial|id=p/d031920}}&lt;br /&gt;
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* [http://eqworld.ipmnet.ru/en/pde-en.htm Partial Differential Equations: Exact Solutions] at EqWorld: The World of Mathematical Equations.&lt;br /&gt;
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* [http://eqworld.ipmnet.ru/en/solutions/eqindex/eqindex-pde.htm Partial Differential Equations: Index] at EqWorld: The World of Mathematical Equations.&lt;br /&gt;
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* [http://eqworld.ipmnet.ru/en/methods/meth-pde.htm Partial Differential Equations: Methods] at EqWorld: The World of Mathematical Equations.&lt;br /&gt;
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* [https://web.archive.org/web/20170701144823/http://www.exampleproblems.com/wiki/index.php?title=Partial_Differential_Equations Example problems with solutions] at exampleproblems.com&lt;br /&gt;
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* [http://mathworld.wolfram.com/PartialDifferentialEquation.html Partial Differential Equations] at mathworld.wolfram.com&lt;br /&gt;
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* [https://reference.wolfram.com/language/FEMDocumentation/tutorial/SolvingPDEwithFEM.html Partial Differential Equations] with Mathematica&lt;br /&gt;
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* [http://www.mathworks.com/moler/pdes.pdf Partial Differential Equations] in Cleve Moler: Numerical Computing with MATLAB&lt;br /&gt;
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* [http://www.nag.com/numeric/fl/nagdoc_fl24/html/D03/d03intro.html Partial Differential Equations] at nag.com&lt;br /&gt;
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* {{cite web |first=Grant |last=Sanderson |title=But what is a partial differential equation? |work=3Blue1Brown |date=April 21, 2019 |url=https://www.youtube.com/watch?v=ly4S0oi3Yz8&amp;amp;list=PLZHQObOWTQDNPOjrT6KVlfJuKtYTftqH6 |via=[[YouTube]] }}&lt;br /&gt;
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{{Differential equations topics}}&lt;br /&gt;
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[[Category:Partial differential equations| ]]&lt;br /&gt;
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[[Category:Multivariable calculus]]&lt;br /&gt;
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Category:Multivariable calculus&lt;br /&gt;
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类别: 多元微积分&lt;br /&gt;
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[[Category:Differential equations]]&lt;br /&gt;
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Category:Differential equations&lt;br /&gt;
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类别: 微分方程&lt;br /&gt;
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[[Category:Concepts in physics]]&lt;br /&gt;
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Category:Concepts in physics&lt;br /&gt;
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分类: 物理概念&lt;br /&gt;
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&amp;lt;small&amp;gt;This page was moved from [[wikipedia:en:Partial differential equation]]. Its edit history can be viewed at [[偏微分方程/edithistory]]&amp;lt;/small&amp;gt;&amp;lt;/noinclude&amp;gt;&lt;br /&gt;
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[[Category:待整理页面]]&lt;/div&gt;</summary>
		<author><name>Ruili</name></author>
	</entry>
	<entry>
		<id>https://wiki.swarma.org/index.php?title=%E5%81%8F%E5%BE%AE%E5%88%86%E6%96%B9%E7%A8%8B&amp;diff=18112</id>
		<title>偏微分方程</title>
		<link rel="alternate" type="text/html" href="https://wiki.swarma.org/index.php?title=%E5%81%8F%E5%BE%AE%E5%88%86%E6%96%B9%E7%A8%8B&amp;diff=18112"/>
		<updated>2020-11-10T14:46:17Z</updated>

		<summary type="html">&lt;p&gt;Ruili：&lt;/p&gt;
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&lt;div&gt;此词条暂由Yuling翻译，未经人工整理和审校，带来阅读不便，请见谅。&lt;br /&gt;
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[[File:Heat.gif|thumb|right|A visualisation of a solution to the two-dimensional [[heat equation]] with temperature represented by the third dimension]]&lt;br /&gt;
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A visualisation of a solution to the two-dimensional [[heat equation with temperature represented by the third dimension]]&lt;br /&gt;
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以三维表示温度的二维热方程解的可视化&lt;br /&gt;
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In [[mathematics]], a '''partial differential equation''' ('''PDE''') is a [[differential equation]] that contains unknown [[Multivariable calculus|multivariable functions]] and their [[partial derivative]]s. PDEs are used to formulate problems involving functions of several variables, and are either solved by hand, or used to create a [[computer model]]. A special case is [[ordinary differential equation]]s (ODEs), which deal with functions of a single variable and their derivatives.&lt;br /&gt;
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In mathematics, a partial differential equation (PDE) is a differential equation that contains unknown multivariable functions and their partial derivatives. PDEs are used to formulate problems involving functions of several variables, and are either solved by hand, or used to create a computer model. A special case is ordinary differential equations (ODEs), which deal with functions of a single variable and their derivatives.&lt;br /&gt;
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在数学中，'''&amp;lt;font color = &amp;quot;#ff8000&amp;quot;&amp;gt;偏微分方程函数 Partial Differential Equation&amp;lt;/font&amp;gt;'''是包含未知多元函数及其偏导数的微分方程。偏微分方程用于描述涉及多元函数的问题，可以通过人为求解，也可以通过建立计算机模型来求解。常微分方程是偏微分方程一种特殊情况，它处理的是一元函数及其导数。&lt;br /&gt;
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PDEs can be used to describe a wide variety of phenomena such as sound, heat, [[diffusion]], [[electrostatics]], [[Electromagnetism|electrodynamics]], [[fluid dynamics]], [[Elasticity (physics)|elasticity]], [[gravitation]] and [[quantum mechanics]]. These seemingly distinct physical phenomena can be formalised similarly in terms of PDEs. Just as ordinary differential equations often model one-dimensional [[dynamical system]]s, partial differential equations often model [[multidimensional system]]s. PDEs find their generalisation in [[stochastic partial differential equation]]s.&lt;br /&gt;
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PDEs can be used to describe a wide variety of phenomena such as sound, heat, diffusion, electrostatics, electrodynamics, fluid dynamics, elasticity, gravitation and quantum mechanics. These seemingly distinct physical phenomena can be formalised similarly in terms of PDEs. Just as ordinary differential equations often model one-dimensional dynamical systems, partial differential equations often model multidimensional systems. PDEs find their generalisation in stochastic partial differential equations.&lt;br /&gt;
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偏微分方程可以用来描述各种各样的物理现象，如声音，热量，扩散，静电，电动力学，流体力学，弹性力学，重力和量子力学。这些看起来截然不同的物理现象却可以用类似的偏微分方程来描述。正如常微分方程经常对一维动力系统进行建模一样，偏微分方程经常对多维系统进行建模。随机偏微分方程是偏微分方程的一种推广。&lt;br /&gt;
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== Introduction ==&lt;br /&gt;
引言&lt;br /&gt;
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Partial differential equations (PDEs) are equations that involve rates of change with respect to [[continuous variables]]. For example, the position of a [[rigid body]] is specified by six parameters,&amp;lt;ref&amp;gt;{{Cite book|url=https://books.google.com/books?id=v9PLbcYd9aUC&amp;amp;pg=PA32|title=Modelling and Control of Robot Manipulators|last=Sciavicco|first=Lorenzo|last2=Siciliano|first2=Bruno|date=2001-02-19|publisher=Springer Science &amp;amp; Business Media|isbn=9781852332211|language=en}}&amp;lt;/ref&amp;gt; but the configuration of a [[fluid]] is given by the [[continuous distribution]] of several parameters, such as the [[temperature]], [[pressure]], and so forth. The dynamics for the rigid body take place in a finite-dimensional [[Configuration space (physics)|configuration space]]; the dynamics for the fluid occur in an infinite-dimensional configuration space. This distinction usually makes PDEs much harder to solve than ordinary differential equations (ODEs), but here again, there will be simple solutions for linear problems. Classic domains where PDEs are used include [[acoustics]], [[fluid dynamics]], [[electrodynamics]], and [[heat transfer]].&lt;br /&gt;
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Partial differential equations (PDEs) are equations that involve rates of change with respect to continuous variables. For example, the position of a rigid body is specified by six parameters, but the configuration of a fluid is given by the continuous distribution of several parameters, such as the temperature, pressure, and so forth. The dynamics for the rigid body take place in a finite-dimensional configuration space; the dynamics for the fluid occur in an infinite-dimensional configuration space. This distinction usually makes PDEs much harder to solve than ordinary differential equations (ODEs), but here again, there will be simple solutions for linear problems. Classic domains where PDEs are used include acoustics, fluid dynamics, electrodynamics, and heat transfer.&lt;br /&gt;
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偏微分方程(简称为PDEs)涉及到连续变量的变化率。例如，刚体的位置是由六个参数确定的，而流体的形状是由几个参数的连续分布给出的，如温度、压力等。刚体的动力学过程发生在有限维位形空间中，流体的动力学过程发生在无限维位形空间中。这种区别通常使偏微分方程比常微分方程更难求解，但是线性问题也有简单的解。使用偏微分方程的经典领域包括声学、流体力学、电动力学和传热学。&lt;br /&gt;
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A partial differential equation (PDE) for the function {{math|''u''(''x''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;,… ''x&amp;lt;sub&amp;gt;n&amp;lt;/sub&amp;gt;'')}} is an equation of the form&lt;br /&gt;
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A partial differential equation (PDE) for the function  is an equation of the form&lt;br /&gt;
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对于函数{{math|''u''(''x''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;,… ''x&amp;lt;sub&amp;gt;n&amp;lt;/sub&amp;gt;'')}}，它的的偏微分方程形式是：&lt;br /&gt;
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: &amp;lt;math&amp;gt;f \left (x_1, \ldots x_n; u, \frac{\partial u}{\partial x_1}, \ldots \frac{\partial u}{\partial x_n}; \frac{\partial^2 u}{\partial x_1 \partial x_1}, \ldots \frac{\partial^2 u}{\partial x_1 \partial x_n}; \ldots \right) = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;f \left (x_1, \ldots x_n; u, \frac{\partial u}{\partial x_1}, \ldots \frac{\partial u}{\partial x_n}; \frac{\partial^2 u}{\partial x_1 \partial x_1}, \ldots \frac{\partial^2 u}{\partial x_1 \partial x_n}; \ldots \right) = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
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If {{mvar|f}} is a [[linear function]] of {{mvar|u}} and its derivatives, then the PDE is called linear. Common examples of linear PDEs include the [[heat equation]], the [[wave equation]], [[Laplace's equation]], [[Helmholtz equation]], [[Klein–Gordon equation]], and [[Poisson's equation]].&lt;br /&gt;
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If  is a linear function of  and its derivatives, then the PDE is called linear. Common examples of linear PDEs include the heat equation, the wave equation, Laplace's equation, Helmholtz equation, Klein–Gordon equation, and Poisson's equation.&lt;br /&gt;
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如果{{mvar|f}}是函数及其导数的线性方程，则偏微分方程称为线性函数。线性偏微分方程的常见例子包括热方程、波动方程、拉普拉斯方程、亥姆霍兹方程方程、克莱因-高登方程和泊松方程。&lt;br /&gt;
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A relatively simple PDE is&lt;br /&gt;
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A relatively simple PDE is&lt;br /&gt;
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一个相对简单的偏微分方程是：&lt;br /&gt;
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: &amp;lt;math&amp;gt;\frac{\partial u}{\partial x}(x,y) = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;\frac{\partial u}{\partial x}(x,y) = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
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This relation [[Logical implication|implies]] that the function {{math|''u''(''x'',''y'')}} is independent of {{mvar|x}}. However, the equation gives no information on the function's dependence on the variable {{mvar|y}}. Hence the general solution of this equation is&lt;br /&gt;
&lt;br /&gt;
This relation implies that the function  is independent of . However, the equation gives no information on the function's dependence on the variable . Hence the general solution of this equation is&lt;br /&gt;
&lt;br /&gt;
这个关系意味着函数是独立于{{mvar|x}}的。然而，这个方程没有给出关于函数和自变量的相关性的信息。因此，这个方程的通解是&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt;u(x,y) = f(y),&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;u(x,y) = f(y),&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
where {{mvar|f}} is an arbitrary function of {{mvar|y}}. The analogous ordinary differential equation is&lt;br /&gt;
&lt;br /&gt;
where  is an arbitrary function of . The analogous ordinary differential equation is&lt;br /&gt;
&lt;br /&gt;
其中{{mvar|f}}是{{mvar|y}}的任意函数。类似的常微分方程是&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt;\frac{\mathrm{d} u}{\mathrm{d} x}(x) = 0,&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;\frac{\mathrm{d} u}{\mathrm{d} x}(x) = 0,&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
which has the solution&lt;br /&gt;
&lt;br /&gt;
which has the solution&lt;br /&gt;
&lt;br /&gt;
它的解为&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt;u(x) = c,&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;u(x) = c,&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
where {{mvar|c}} is any [[Constant (mathematics)|constant]] value. These two examples illustrate that general solutions of ordinary differential equations (ODEs) involve arbitrary constants, but solutions of PDEs involve arbitrary functions.&lt;br /&gt;
&lt;br /&gt;
where  is any constant value. These two examples illustrate that general solutions of ordinary differential equations (ODEs) involve arbitrary constants, but solutions of PDEs involve arbitrary functions.&lt;br /&gt;
&lt;br /&gt;
这里的{{mvar|c}}是常量。这两个例子说明常微分方程的一般解包含任意常数，但偏微分方程的解包含任意函数。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
A solution of a PDE is generally not [[Uniqueness quantification|unique]]; additional conditions must generally be specified on the [[Boundary (topology)|boundary]] of the region where the solution is defined. For instance, in the simple example above, the function {{math|''f''(''y'')}} can be determined if {{mvar|u}} is specified on the line {{math|''x'' {{=}} 0}}.&lt;br /&gt;
&lt;br /&gt;
A solution of a PDE is generally not unique; additional conditions must generally be specified on the boundary of the region where the solution is defined. For instance, in the simple example above, the function  can be determined if  is specified on the line  0}}.&lt;br /&gt;
&lt;br /&gt;
偏微分方程的解一般不是唯一的; 附加条件一般必须在定义解的区域边界上定义。例如，在上面的简单示例中，如果在{{math|''x'' {{=}} 0}}时确定了{{mvar|u}}的值，则可以确定该函数{{math|''f''(''y'')}}。&lt;br /&gt;
&lt;br /&gt;
== Existence and uniqueness ==&lt;br /&gt;
存在性和唯一性&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Although the issue of existence and uniqueness of solutions of ordinary differential equations has a very satisfactory answer with the [[Picard–Lindelöf theorem]], that is far from the case for partial differential equations. The [[Cauchy–Kowalevski theorem]] states that the [[Cauchy problem]] for any partial differential equation whose coefficients are [[Analytic function|analytic]] in the unknown function and its derivatives, has a locally unique analytic solution. Although this result might appear to settle the existence and uniqueness of solutions, there are examples of linear partial differential equations whose coefficients have derivatives of all orders (which are nevertheless not analytic) but which have no solutions at all: see [[Lewy's example|Lewy (1957)]]. Even if the solution of a partial differential equation exists and is unique, it may nevertheless have undesirable properties.  The mathematical study of these questions is usually in the more powerful context of [[weak solution]]s.&lt;br /&gt;
&lt;br /&gt;
Although the issue of existence and uniqueness of solutions of ordinary differential equations has a very satisfactory answer with the Picard–Lindelöf theorem, that is far from the case for partial differential equations. The Cauchy–Kowalevski theorem states that the Cauchy problem for any partial differential equation whose coefficients are analytic in the unknown function and its derivatives, has a locally unique analytic solution. Although this result might appear to settle the existence and uniqueness of solutions, there are examples of linear partial differential equations whose coefficients have derivatives of all orders (which are nevertheless not analytic) but which have no solutions at all: see Lewy (1957). Even if the solution of a partial differential equation exists and is unique, it may nevertheless have undesirable properties.  The mathematical study of these questions is usually in the more powerful context of weak solutions.&lt;br /&gt;
&lt;br /&gt;
虽然常微分方程解的存在唯一性问题用'''&amp;lt;font color=&amp;quot;#ff8000&amp;quot;&amp;gt;弗罗贝尼乌斯定理 Picard–Lindelöf Theorem&amp;lt;/font&amp;gt;得到了令人满意的结果，但应用到偏微分方程上却不尽如意。'''&amp;lt;font color=&amp;quot;#ff8000&amp;quot;&amp;gt;柯西-科瓦列夫斯基定理 Cauchy–Kowalevski theorem&amp;lt;/font&amp;gt;指出，对于任何在未知函数及其导数中系数是解析的偏微分方程，柯西问题有一个局部唯一的解析解。虽然这个结果似乎解决了解的存在性和唯一性问题，但是有一些线性偏微分方程的系数具有所有级数的导数(尽管这些导数不是解析的) ，但是根本没有解: 见 Lewy (1957)。即使偏微分方程的解存在且唯一，它仍然可能具有人们所不希望的性质。这些问题的数学研究通常是在更有力的弱解的背景下进行的。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
An example of pathological behavior is the sequence (depending upon {{mvar|n}}) of [[Cauchy problem]]s for the [[Laplace equation]]&lt;br /&gt;
&lt;br /&gt;
An example of pathological behavior is the sequence (depending upon ) of Cauchy problems for the Laplace equation&lt;br /&gt;
&lt;br /&gt;
反常特征的一个例子是拉普拉斯方程的柯西问题的序列(取决于{{mvar|n}})&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt;\frac{\partial^2 u}{\partial x^2} + \frac{\partial^2 u}{\partial y^2}=0,&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;\frac{\partial^2 u}{\partial x^2} + \frac{\partial^2 u}{\partial y^2}=0,&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
with [[boundary condition]]s&lt;br /&gt;
&lt;br /&gt;
with boundary conditions&lt;br /&gt;
&lt;br /&gt;
有边界条件&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt;\begin{align} u(x,0) &amp;amp;= 0, \\ \frac{\partial u}{\partial y}(x,0) &amp;amp;= \frac{\sin nx}{n}, \end{align}&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;\begin{align} u(x,0) &amp;amp;= 0, \\ \frac{\partial u}{\partial y}(x,0) &amp;amp;= \frac{\sin nx}{n}, \end{align}&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
where {{mvar|n}} is an integer. The derivative of {{mvar|u}} with respect to {{mvar|y}} approaches zero [[uniform convergence|uniformly]] in {{mvar|x}} as {{mvar|n}} increases, but the solution is&lt;br /&gt;
&lt;br /&gt;
where  is an integer. The derivative of  with respect to  approaches zero uniformly in  as  increases, but the solution is&lt;br /&gt;
&lt;br /&gt;
其中{{mvar|n}}是整数。{{mvar|u}}是关于{{mvar|y}}的导数，一致地随着{{mvar|n}}的增加而趋于零，但是解是&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt;u(x,y) = \frac{\sinh ny \sin nx}{n^2}.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;u(x,y) = \frac{\sinh ny \sin nx}{n^2}.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
This solution approaches infinity if {{mvar|nx}} is not an integer multiple of {{pi}} for any non-zero value of {{mvar|y}}. The Cauchy problem for the Laplace equation is called ''ill-posed'' or ''not [[Well-posed problem|well-posed]]'', since the solution does not continuously depend on the data of the problem. Such ill-posed problems are not usually satisfactory for physical applications.&lt;br /&gt;
&lt;br /&gt;
This solution approaches infinity if  is not an integer multiple of  for any non-zero value of . The Cauchy problem for the Laplace equation is called ill-posed or not well-posed, since the solution does not continuously depend on the data of the problem. Such ill-posed problems are not usually satisfactory for physical applications.&lt;br /&gt;
&lt;br /&gt;
对于任何非零的{{mvar|y}}，如果{{mvar|nx}}不是{{pi}}的整数倍，这个解会接近于无穷大。拉普拉斯方程的柯西问题被称为不适定问题（可以译为ill-posed或not well-posed），因为该问题的解并不连续地依赖于该问题的数据。这种不适定问题在物理应用中通常不能令人满意。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The [[Navier–Stokes existence and smoothness|existence of solutions for the Navier–Stokes equations]], a partial differential equation, is part of one of the [[Millennium Prize Problems]].&lt;br /&gt;
&lt;br /&gt;
The existence of solutions for the Navier–Stokes equations, a partial differential equation, is part of one of the Millennium Prize Problems.&lt;br /&gt;
&lt;br /&gt;
一种偏微分方程——纳维-斯托克斯方程——的解的存在性就是千禧年大奖难题的一部分。&lt;br /&gt;
&lt;br /&gt;
== Notation ==&lt;br /&gt;
符号&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
In PDEs, it is common to denote partial derivatives using subscripts. That is:&lt;br /&gt;
&lt;br /&gt;
In PDEs, it is common to denote partial derivatives using subscripts. That is:&lt;br /&gt;
&lt;br /&gt;
在偏微分方程中，通常用下标表示偏导数。例如:&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt;u_x = \frac{\partial u}{\partial x}&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;u_x = \frac{\partial u}{\partial x}&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt;u_{xx} = \frac{\partial^2 u}{\partial x^2} &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;u_{xx} = \frac{\partial^2 u}{\partial x^2} &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt;u_{xy} = \frac{\partial^2 u}{\partial y\, \partial x} = \frac{\partial}{\partial y } \left(\frac{\partial u}{\partial x}\right). &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;u_{xy} = \frac{\partial^2 u}{\partial y\, \partial x} = \frac{\partial}{\partial y } \left(\frac{\partial u}{\partial x}\right). &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Especially in physics, [[del]] or nabla ({{math|∇}}) is often used to denote spatial derivatives, and {{math|''&amp;amp;#x307;u'', ''ü''}} for time derivatives. For example, the [[wave equation]] (mentioned below) can be written as&lt;br /&gt;
&lt;br /&gt;
Especially in physics, del or nabla () is often used to denote spatial derivatives, and  for time derivatives. For example, the wave equation (mentioned below) can be written as&lt;br /&gt;
&lt;br /&gt;
特别是在物理学中，[[del]]或nabla ({{math|∇}})经常用来表示空间导数和时间导数。例如，波动方程(在下文中提到)可以写成&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt;\ddot u=c^2\nabla^2u&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt;\ddot u=c^2\nabla^2u&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
or&lt;br /&gt;
&lt;br /&gt;
or&lt;br /&gt;
&lt;br /&gt;
或&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt;\ddot u=c^2\Delta u&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt;\ddot u=c^2\Delta u&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
where {{math|Δ}} is the [[Laplace operator]].&lt;br /&gt;
&lt;br /&gt;
where  is the Laplace operator.&lt;br /&gt;
&lt;br /&gt;
其中{{math|Δ}}代表拉普拉斯算子&lt;br /&gt;
&lt;br /&gt;
== Classification ==&lt;br /&gt;
分类&lt;br /&gt;
&lt;br /&gt;
Some linear, second-order partial differential equations can be classified as [[parabolic partial differential equation|parabolic]], [[hyperbolic partial differential equation|hyperbolic]] and [[elliptic partial differential equation|elliptic]]. Others, such as the [[Euler–Tricomi equation]], have different types in different regions. The classification provides a guide to appropriate initial and boundary conditions and to the smoothness of the solutions.&lt;br /&gt;
&lt;br /&gt;
Some linear, second-order partial differential equations can be classified as parabolic, hyperbolic and elliptic. Others, such as the Euler–Tricomi equation, have different types in different regions. The classification provides a guide to appropriate initial and boundary conditions and to the smoothness of the solutions.&lt;br /&gt;
&lt;br /&gt;
一些线性二阶偏微分方程可分为抛物型方程、双曲型方程和椭圆型方程。其他的方程，如欧拉-特里科米方程，在不同的区域有不同的类型。这种分类有助于选择适当的初始和边界条件以及提高解的平滑性。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
=== Equations of first order ===&lt;br /&gt;
一阶方程&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{{main|First-order partial differential equation}}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
=== Linear equations of second order ===&lt;br /&gt;
二阶线性方程&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Assuming {{math|''u&amp;lt;sub&amp;gt;xy&amp;lt;/sub&amp;gt;'' {{=}} ''u&amp;lt;sub&amp;gt;yx&amp;lt;/sub&amp;gt;''}}, the general linear second-order PDE in two independent variables has the form&lt;br /&gt;
&lt;br /&gt;
Assuming  u&amp;lt;sub&amp;gt;yx&amp;lt;/sub&amp;gt;}}, the general linear second-order PDE in two independent variables has the form&lt;br /&gt;
&lt;br /&gt;
假设 {{math|''u&amp;lt;sub&amp;gt;xy&amp;lt;/sub&amp;gt;'' {{=}} ''u&amp;lt;sub&amp;gt;yx&amp;lt;/sub&amp;gt;''}}，含有两个独立变量的一般的线性二阶偏微分方程具有如下这样的形式&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt;Au_{xx} + 2Bu_{xy} + Cu_{yy} + \cdots \mbox{(lower order terms)} = 0,&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;Au_{xx} + 2Bu_{xy} + Cu_{yy} + \cdots \mbox{(lower order terms)} = 0,&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
where the coefficients {{mvar|A}}, {{mvar|B}}, {{mvar|C}}... may depend upon {{mvar|x}} and {{mvar|y}}. If {{math|''A''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; + ''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; + ''C''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; &amp;gt; 0}} over a region of the {{mvar|xy}}-plane, the PDE is second-order in that region. This form is analogous to the equation for a conic section:&lt;br /&gt;
&lt;br /&gt;
where the coefficients , , ... may depend upon  and . If  over a region of the -plane, the PDE is second-order in that region. This form is analogous to the equation for a conic section:&lt;br /&gt;
&lt;br /&gt;
其中的系数 {{mvar|A}}, {{mvar|B}}, {{mvar|C}}... 一般取决于{{mvar|x}}和{{mvar|y}}。如果在{{mvar|xy}}-平面的一个区域上 {{math|''A''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; + ''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; + ''C''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; &amp;gt; 0}}，偏微分方程在该区域是二阶的。这种形式类似于圆锥曲线的方程:&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt;Ax^2 + 2Bxy + Cy^2 + \cdots = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;Ax^2 + 2Bxy + Cy^2 + \cdots = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
More precisely, replacing {{math|∂&amp;lt;sub&amp;gt;''x''&amp;lt;/sub&amp;gt;}} by {{mvar|X}}, and likewise for other variables (formally this is done by a [[Fourier transform]]), converts a constant-coefficient PDE into a polynomial of the same degree, with the terms of the highest degree (a [[homogeneous polynomial]], here a [[quadratic form]]) being most significant for the classification.&lt;br /&gt;
&lt;br /&gt;
More precisely, replacing  by , and likewise for other variables (formally this is done by a Fourier transform), converts a constant-coefficient PDE into a polynomial of the same degree, with the terms of the highest degree (a homogeneous polynomial, here a quadratic form) being most significant for the classification.&lt;br /&gt;
&lt;br /&gt;
更准确地说，用 {{mvar|X}} 替换 {{math|∂&amp;lt;sub&amp;gt;''x''&amp;lt;/sub&amp;gt;}}，对于其他变量做同样的操作(从形式上来说，这是由傅里叶变换来完成的)，将一个常系数偏微分方程转换成一个相同次数的多项式，最高次数的项(齐次多项式，这里是一个二次形式)一般会用于偏微分方程的分类。&lt;br /&gt;
===~~ most significant for the classification 意译为用于偏微分方程的分类。       significiant直译过来感觉不太合适&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Just as one classifies [[conic section]]s and quadratic forms into parabolic, hyperbolic, and elliptic based on the [[discriminant]] {{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − 4''AC''}}, the same can be done for a second-order PDE at a given point.  However, the [[discriminant]] in a PDE is given by {{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC''}} due to the convention of the {{mvar|xy}} term being {{math|2''B''}} rather than {{mvar|B}}; formally, the discriminant (of the associated quadratic form) is {{math|(2''B'')&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − 4''AC'' {{=}} 4(''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC'')}}, with the factor of 4 dropped for simplicity.&lt;br /&gt;
&lt;br /&gt;
Just as one classifies conic sections and quadratic forms into parabolic, hyperbolic, and elliptic based on the discriminant , the same can be done for a second-order PDE at a given point.  However, the discriminant in a PDE is given by  due to the convention of the  term being  rather than ; formally, the discriminant (of the associated quadratic form) is  4(B&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − AC)}}, with the factor of 4 dropped for simplicity.&lt;br /&gt;
&lt;br /&gt;
正如人们可以根据判别式 {{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − 4''AC''}} 将圆锥曲线和二次型分为抛物型、双曲型和椭圆型一样，对于给定点的二阶偏微分方程也可以这样做。然而，偏微分方程中的判别式 {{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − 4''AC''}} 是根据交叉项的系数{{math|2''B''}} 而不是 {{mvar|B}} 给出的，形式上，判别式(关联二次型)是 {{math|(2''B'')&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − 4''AC'' {{=}} 4(''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC'')}}，为简单起见，去掉了因子4。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
# {{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC'' &amp;lt; 0}} (''[[elliptic partial differential equation]]''): Solutions of [[elliptic partial differential equation|elliptic PDEs]] are as smooth as the coefficients allow, within the interior of the region where the equation and solutions are defined. For example, solutions of [[Laplace's equation]] are analytic within the domain where they are defined, but solutions may assume boundary values that are not smooth. The motion of a fluid at subsonic speeds can be approximated with elliptic PDEs, and the Euler–Tricomi equation is elliptic where {{math|''x'' &amp;lt; 0}}.&lt;br /&gt;
&lt;br /&gt;
  (elliptic partial differential equation): Solutions of elliptic PDEs are as smooth as the coefficients allow, within the interior of the region where the equation and solutions are defined. For example, solutions of Laplace's equation are analytic within the domain where they are defined, but solutions may assume boundary values that are not smooth. The motion of a fluid at subsonic speeds can be approximated with elliptic PDEs, and the Euler–Tricomi equation is elliptic where .&lt;br /&gt;
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{{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC'' &amp;lt; 0}} (椭圆形微分方程)：在定义方程和解的区域内部，椭圆型偏微分方程的解光滑到系数允许的程度。例如，拉普拉斯方程的解在它们被定义的区域内是解析的，但是解可能假设边界值是不光滑的。亚音速流体的运动可以用椭圆偏微分方程近似，其中欧拉-特里科米方程在 {{math|''x'' &amp;lt; 0}} 时是椭圆型偏微分方程。&lt;br /&gt;
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# {{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC'' {{=}} 0}} (''[[parabolic partial differential equation]]''): Equations that are [[parabolic partial differential equation|parabolic]] at every point can be transformed into a form analogous to the [[heat equation]] by a change of independent variables. Solutions smooth out as the transformed time variable increases. The Euler–Tricomi equation has parabolic type on the line where {{math|''x'' {{=}} 0}}.&lt;br /&gt;
&lt;br /&gt;
  0}} (parabolic partial differential equation): Equations that are parabolic at every point can be transformed into a form analogous to the heat equation by a change of independent variables. Solutions smooth out as the transformed time variable increases. The Euler–Tricomi equation has parabolic type on the line where  0}}.&lt;br /&gt;
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{{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC'' {{=}} 0}}（抛物线形偏微分方程）：在每一点上都是抛物线型的方程可以通过改变自变量从而转化成类似于热方程的形式。随着转换后的时间变量的增加，方程的解变得平滑。欧拉-特里科米方程在 {{math|''x'' {{=}} 0}} 这条特征线上是抛物线形的。&lt;br /&gt;
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# {{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC'' &amp;gt; 0}} (''[[hyperbolic partial differential equation]]''): [[hyperbolic partial differential equation|hyperbolic]] equations retain any discontinuities of functions or derivatives in the initial data. An example is the [[wave equation]]. The motion of a fluid at supersonic speeds can be approximated with hyperbolic PDEs, and the Euler–Tricomi equation is hyperbolic where {{math|''x'' &amp;gt; 0}}.&lt;br /&gt;
&lt;br /&gt;
  (hyperbolic partial differential equation): hyperbolic equations retain any discontinuities of functions or derivatives in the initial data. An example is the wave equation. The motion of a fluid at supersonic speeds can be approximated with hyperbolic PDEs, and the Euler–Tricomi equation is hyperbolic where .&lt;br /&gt;
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{{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC'' &amp;gt; 0}} (双曲形偏微分方程)：双曲形方程在初始数据中保留了函数或导数的任何不连续性，波动方程就是其中的一个例子。超音速流体的运动可以用双曲形偏微分方程近似，其中欧拉-特里科米方程在 {{math|''x'' &amp;gt; 0}} 时是双曲型的。&lt;br /&gt;
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If there are {{mvar|n}} independent variables {{math|''x''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;, ''x''&amp;lt;sub&amp;gt;2 &amp;lt;/sub&amp;gt;,… ''x''&amp;lt;sub&amp;gt;''n''&amp;lt;/sub&amp;gt;}}, a general linear partial differential equation of second order has the form&lt;br /&gt;
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If there are  independent variables , a general linear partial differential equation of second order has the form&lt;br /&gt;
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如果存在 {{mvar|n}} 个自变量 {{math|''x''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;, ''x''&amp;lt;sub&amp;gt;2 &amp;lt;/sub&amp;gt;,… ''x''&amp;lt;sub&amp;gt;''n''&amp;lt;/sub&amp;gt;}}，一般二阶线性偏微分方程的形式是&lt;br /&gt;
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: &amp;lt;math&amp;gt;L u =\sum_{i=1}^n\sum_{j=1}^n a_{i,j} \frac{\partial^2 u}{\partial x_i \partial x_j} \quad \text{ plus lower-order terms} =0.&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;L u =\sum_{i=1}^n\sum_{j=1}^n a_{i,j} \frac{\partial^2 u}{\partial x_i \partial x_j} \quad \text{ plus lower-order terms} =0.&amp;lt;/math&amp;gt;&lt;br /&gt;
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The classification depends upon the signature of the eigenvalues of the coefficient matrix {{math|''a''&amp;lt;sub&amp;gt;''i'',''j''&amp;lt;/sub&amp;gt;}}.&lt;br /&gt;
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The classification depends upon the signature of the eigenvalues of the coefficient matrix .&lt;br /&gt;
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这种分类取决于系数矩阵本征值的符号（正负性）。&lt;br /&gt;
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# Elliptic: the eigenvalues are all positive or all negative.&lt;br /&gt;
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 Elliptic: the eigenvalues are all positive or all negative.&lt;br /&gt;
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椭圆形方程: 本征值全部为正或全部为负。&lt;br /&gt;
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# Parabolic: the eigenvalues are all positive or all negative, save one that is zero.&lt;br /&gt;
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 Parabolic: the eigenvalues are all positive or all negative, save one that is zero.&lt;br /&gt;
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抛物线形方程: 本征值全部为正或全部为负，除了一个为零。&lt;br /&gt;
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# Hyperbolic: there is only one negative eigenvalue and all the rest are positive, or there is only one positive eigenvalue and all the rest are negative.&lt;br /&gt;
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 Hyperbolic: there is only one negative eigenvalue and all the rest are positive, or there is only one positive eigenvalue and all the rest are negative.&lt;br /&gt;
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双曲形方程: 只有一个负特征值，其余的都是正特征值，或者只有一个正特征值，其余的都是负特征值。&lt;br /&gt;
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# Ultrahyperbolic: there is more than one positive eigenvalue and more than one negative eigenvalue, and there are no zero eigenvalues. There is only a limited theory for ultrahyperbolic equations (Courant and Hilbert, 1962).&lt;br /&gt;
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 Ultrahyperbolic: there is more than one positive eigenvalue and more than one negative eigenvalue, and there are no zero eigenvalues. There is only a limited theory for ultrahyperbolic equations (Courant and Hilbert, 1962).&lt;br /&gt;
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超双形方程: 存在多于一个正本征值和多于一个的负本征值，且不存在零本征值。对于超双曲方程，只存在一个有限理论(Courant 和 Hilbert，1962)。&lt;br /&gt;
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==[[用户:Yuling|Yuling]]（[[用户讨论:Yuling|讨论]]） 我对于limited theory这个单词对应的相关理论不太了解。&lt;br /&gt;
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=== Systems of first-order equations and characteristic surfaces ===&lt;br /&gt;
一阶方程组和特征曲面&lt;br /&gt;
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The classification of partial differential equations can be extended to systems of first-order equations, where the unknown {{mvar|u}} is now a [[Euclidean vector|vector]] with {{mvar|m}} components, and the coefficient matrices {{mvar|A&amp;lt;sub&amp;gt;ν&amp;lt;/sub&amp;gt;}} are {{mvar|m}} by {{mvar|m}} matrices for {{math|''ν'' {{=}} 1, 2,… ''n''}}. The partial differential equation takes the form&lt;br /&gt;
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The classification of partial differential equations can be extended to systems of first-order equations, where the unknown  is now a vector with  components, and the coefficient matrices  are  by  matrices for  1, 2,… n}}. The partial differential equation takes the form&lt;br /&gt;
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偏微分方程组的分类可以推广到一阶方程组，其中未知量 {{mvar|u}} 是有 {{mvar|m}} 个分量的向量。对于 {{math|''ν'' {{=}} 1, 2,… ''n''}}，系数矩阵 {{mvar|A&amp;lt;sub&amp;gt;ν&amp;lt;/sub&amp;gt;}} 是 {{mvar|m}} × {{mvar|m}} 的矩阵。偏微分方程形式如下：&lt;br /&gt;
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: &amp;lt;math&amp;gt;Lu = \sum_{\nu=1}^{n} A_\nu \frac{\partial u}{\partial x_\nu} + B=0,&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;Lu = \sum_{\nu=1}^{n} A_\nu \frac{\partial u}{\partial x_\nu} + B=0,&amp;lt;/math&amp;gt;&lt;br /&gt;
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where the coefficient matrices {{mvar|A&amp;lt;sub&amp;gt;ν&amp;lt;/sub&amp;gt;}} and the vector {{mvar|B}} may depend upon {{mvar|x}} and {{mvar|u}}. If a [[hypersurface]] {{mvar|S}} is given in the implicit form&lt;br /&gt;
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where the coefficient matrices  and the vector  may depend upon  and . If a hypersurface  is given in the implicit form&lt;br /&gt;
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其中系数矩阵 {{mvar|A&amp;lt;sub&amp;gt;ν&amp;lt;/sub&amp;gt;}} 和向量 {{mvar|B}} 可能依赖于 {{mvar|x}} 和 {{mvar|u}}。如果超曲面是以隐式形式给出的&lt;br /&gt;
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: &amp;lt;math&amp;gt;\varphi(x_1, x_2, \ldots x_n)=0,&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;\varphi(x_1, x_2, \ldots x_n)=0,&amp;lt;/math&amp;gt;&lt;br /&gt;
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where {{mvar|φ}} has a non-zero gradient, then {{mvar|S}} is a '''characteristic surface''' for the operator {{mvar|L}} at a given point if the characteristic form vanishes:&lt;br /&gt;
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where  has a non-zero gradient, then  is a characteristic surface for the operator  at a given point if the characteristic form vanishes:&lt;br /&gt;
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其中存在一个非零的梯度，那么如果特征形式消失，则在给定点上算子的特征曲面形式如下:&lt;br /&gt;
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: &amp;lt;math&amp;gt;Q\left(\frac{\partial\varphi}{\partial x_1}, \ldots\frac{\partial\varphi}{\partial x_n}\right) =\det\left[\sum_{\nu=1}^nA_\nu \frac{\partial \varphi}{\partial x_\nu}\right]=0.\,&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;Q\left(\frac{\partial\varphi}{\partial x_1}, \ldots\frac{\partial\varphi}{\partial x_n}\right) =\det\left[\sum_{\nu=1}^nA_\nu \frac{\partial \varphi}{\partial x_\nu}\right]=0.\,&amp;lt;/math&amp;gt;&lt;br /&gt;
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The geometric interpretation of this condition is as follows: if data for {{mvar|u}} are prescribed on the surface {{mvar|S}}, then it may be possible to determine the normal derivative of {{mvar|u}} on {{mvar|S}} from the differential equation. If the data on {{mvar|S}} and the differential equation determine the normal derivative of {{mvar|u}} on {{mvar|S}}, then {{mvar|S}} is non-characteristic. If the data on {{mvar|S}} and the differential equation ''do not'' determine the normal derivative of {{mvar|u}} on {{mvar|S}}, then the surface is '''characteristic''', and the differential equation restricts the data on {{mvar|S}}: the differential equation is ''internal'' to {{mvar|S}}.&lt;br /&gt;
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The geometric interpretation of this condition is as follows: if data for  are prescribed on the surface , then it may be possible to determine the normal derivative of  on  from the differential equation. If the data on  and the differential equation determine the normal derivative of  on , then  is non-characteristic. If the data on  and the differential equation do not determine the normal derivative of  on , then the surface is characteristic, and the differential equation restricts the data on : the differential equation is internal to .&lt;br /&gt;
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这个条件的几何解释如下: 如果关于 {{mvar|u}} 的数据是在曲面 {{mvar|S}} 上规定的，那么就有可能依据微分方程确定曲面 {{mvar|S}} 上 {{mvar|u}} 的法向导数。如果曲面 {{mvar|S}} 上的数据和上面的微分方程能确定曲面 {{mvar|S}} 上 {{mvar|u}} 的法向导数，那么它就是非特征的。如果曲面 {{mvar|S}} 上的数据和上面的微分方程不能确定曲面 {{mvar|S}} 上 {{mvar|u}} 的法向导数，那么曲面是特征的，并且微分方程将数据限制在曲面 {{mvar|S}} 上：微分方程是在曲面 {{mvar|S}} 内部。&lt;br /&gt;
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# A first-order system {{math|''Lu'' {{=}} 0}} is ''elliptic'' if no surface is characteristic for {{mvar|L}}: the values of {{mvar|u}} on {{mvar|S}} and the differential equation always determine the normal derivative of {{mvar|u}} on {{mvar|S}}.&lt;br /&gt;
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 A first-order system  0}} is elliptic if no surface is characteristic for : the values of  on  and the differential equation always determine the normal derivative of  on .&lt;br /&gt;
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如果对于 {{mvar|L}} 没有曲面是特征的，则一阶系统 {{math|''Lu'' {{=}} 0}} 是椭圆形的：{{mvar|u}}在 {{mvar|S}} 的值和微分方程总能够决定 {{mvar|S}} 上 {{mvar|u}} 的法向导数。&lt;br /&gt;
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# A first-order system is ''hyperbolic'' at a point if there is a '''spacelike''' surface {{mvar|S}} with normal {{mvar|ξ}} at that point. This means that, given any non-trivial vector {{mvar|η}} orthogonal to {{mvar|ξ}}, and a scalar multiplier {{mvar|λ}}, the equation {{math|''Q''(''λξ'' + ''η'') {{=}} 0}} has {{mvar|m}} real roots {{math|''λ''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;, ''λ''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;,… ''λ''&amp;lt;sub&amp;gt;''m''&amp;lt;/sub&amp;gt;}}. The system is '''strictly hyperbolic''' if these roots are always distinct. The geometrical interpretation of this condition is as follows: the characteristic form {{math|''Q''(''ζ'') {{=}} 0}} defines a cone (the normal cone) with homogeneous coordinates ζ. In the hyperbolic case, this cone has {{mvar|m}} sheets, and the axis {{math|''ζ'' {{=}} ''λξ''}} runs inside these sheets: it does not intersect any of them. But when displaced from the origin by η, this axis intersects every sheet. In the elliptic case, the normal cone has no real sheets.&lt;br /&gt;
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 A first-order system is hyperbolic at a point if there is a spacelike surface  with normal  at that point. This means that, given any non-trivial vector  orthogonal to , and a scalar multiplier , the equation  0}} has  real roots . The system is strictly hyperbolic if these roots are always distinct. The geometrical interpretation of this condition is as follows: the characteristic form  0}} defines a cone (the normal cone) with homogeneous coordinates ζ. In the hyperbolic case, this cone has  sheets, and the axis  λξ}} runs inside these sheets: it does not intersect any of them. But when displaced from the origin by η, this axis intersects every sheet. In the elliptic case, the normal cone has no real sheets.&lt;br /&gt;
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如果在该点存在一个法向量为 {{mvar|ξ}}的 '''&amp;lt;font color=&amp;quot;#ff8000&amp;quot;&amp;gt;类空曲面 Spacclike Surface&amp;lt;/font&amp;gt; {{mvar|S}} ，则一阶系统在那一点是双曲的。这意味着，给定任意正交于 {{mvar|ξ}} 的非平凡向量 {{mvar|η}} 和一个标量乘子 {{mvar|λ}}，方程 {{math|''Q''(''λξ'' + ''η'') {{=}} 0}} 有 {{mvar|m}} 个实根 {{math|''λ''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;, ''λ''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;,… ''λ''&amp;lt;sub&amp;gt;''m''&amp;lt;/sub&amp;gt;}}。如果这些根始终不同，则该系统是严格双曲形的。这个条件的几何解释如下: 特征形式 {{math|''Q''(''ζ'') {{=}} 0}} 定义了一个具有齐次坐标 ζ的圆锥(法线圆锥)。在双曲形的情况下，这个圆锥体有 {{mvar|m}} 层，并且轴 {{math|''ζ'' {{=}} ''λξ''}} 在这些层中运动: 它不与任何一层相交。但是当从原点偏离η时，这条轴线与每一层都相交。在椭圆形的情况下，法向圆锥没有实层。&lt;br /&gt;
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==[[用户:Yuling|Yuling]]（[[用户讨论:Yuling|讨论]]） sheet 这个单词也不很理解，我直译为了“层”&lt;br /&gt;
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=== Equations of mixed type ===&lt;br /&gt;
混合型方程&lt;br /&gt;
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If a PDE has coefficients that are not constant, it is possible that it will not belong to any of these categories but rather be of '''mixed type'''. A simple but important example is the [[Euler–Tricomi equation]]&lt;br /&gt;
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If a PDE has coefficients that are not constant, it is possible that it will not belong to any of these categories but rather be of mixed type. A simple but important example is the Euler–Tricomi equation&lt;br /&gt;
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如果偏微分方程的系数不是常数，那么它可能不属于这些类别中的任何一个，而是属于混合类型。一个简单但重要的例子是欧拉-特里科米方程&lt;br /&gt;
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: &amp;lt;math&amp;gt;u_{xx} = xu_{yy},&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;u_{xx} = xu_{yy},&amp;lt;/math&amp;gt;&lt;br /&gt;
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which is called '''elliptic-hyperbolic''' because it is elliptic in the region {{math|''x'' &amp;lt; 0}}, hyperbolic in the region {{math|''x'' &amp;gt; 0}}, and degenerate parabolic on the line {{math|''x'' {{=}} 0}}.&lt;br /&gt;
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which is called elliptic-hyperbolic because it is elliptic in the region , hyperbolic in the region , and degenerate parabolic on the line  0}}.&lt;br /&gt;
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它在 {{math|''x'' &amp;lt; 0}} 的区域上是椭圆形，在 {{math|''x'' &amp;gt; 0}} 区域上是双曲形，在 {{math|''x'' {{=}} 0}}这条线上是退化为抛物线形，因此称之为椭圆-双曲型。&lt;br /&gt;
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''fill in: Dirichlet and Neumann boundaries, hyperbolic/parabolic/elliptic separation of variables, [[Fourier analysis]], [[Green's function]]s ...--&amp;gt;&lt;br /&gt;
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fill in: Dirichlet and Neumann boundaries, hyperbolic/parabolic/elliptic separation of variables, Fourier analysis, Green's functions ...--&amp;gt;&lt;br /&gt;
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填写: Dirichlet 和 Neumann 边界，双曲 / 抛物线 / 椭圆分离变量法，傅立叶分析，Green 函数... --&lt;br /&gt;
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=== Infinite-order PDEs in quantum mechanics ===&lt;br /&gt;
量子力学中的无限阶偏微分方程&lt;br /&gt;
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In the [[phase space formulation]] of quantum mechanics,  one may consider the [[Method of quantum characteristics|quantum Hamilton's equations]] for trajectories of quantum particles. These equations are infinite-order PDEs. However, in the semiclassical expansion, one has a finite system of ODEs at any fixed order of [[Dirac constant|{{mvar|ħ}}]].  The evolution equation of the [[Wigner quasi-probability distribution|c]] is also an infinite-order PDE. The quantum trajectories are [[Method of quantum characteristics|quantum characteristics]], with the use of which one could calculate the evolution of the Wigner function.&lt;br /&gt;
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In the phase space formulation of quantum mechanics,  one may consider the quantum Hamilton's equations for trajectories of quantum particles. These equations are infinite-order PDEs. However, in the semiclassical expansion, one has a finite system of ODEs at any fixed order of Dirac constant|.  The evolution equation of the Wigner function is also an infinite-order PDE. The quantum trajectories are quantum characteristics, with the use of which one could calculate the evolution of the Wigner function.&lt;br /&gt;
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在量子力学中的相空间表述中，我们可以考虑用于求解量子粒子的轨迹的量子哈密顿的方程。这些方程是无限阶偏微分方程。然而，在半经典展开中，我们在给定[[Dirac constant|{{mvar|ħ}}]]阶数下有一个有限的的常微分方程组。'''&amp;lt;font color=&amp;quot;#ff8000&amp;quot;&amp;gt;维格纳函数  Wigner Function&amp;lt;/font&amp;gt;的演化方程也是一个无限阶偏微分方程。由于量子轨道的量子特性，所以它通常可以用来计算维格纳函数的演化。&lt;br /&gt;
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== Analytical solutions ==&lt;br /&gt;
解析解&lt;br /&gt;
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===Separation of variables===&lt;br /&gt;
分离变量法&lt;br /&gt;
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{{main|Separable partial differential equation}}&lt;br /&gt;
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Linear PDEs can be reduced to systems of ordinary differential equations by the important technique of separation of variables. This technique rests on a characteristic of solutions to differential equations: if one can find any solution that solves the equation and satisfies the boundary conditions, then it is ''the'' solution (this also applies to ODEs). We assume as an [[ansatz]] that the dependence of a solution on the parameters space and time can be written as a product of terms that each depend on a single parameter, and then see if this can be made to solve the problem.&amp;lt;ref&amp;gt;{{cite book|last1=Gershenfeld|first1=Neil|title=The nature of mathematical modeling|date=2000|publisher=Cambridge Univ. Press|location=Cambridge|isbn=0521570956|page=27|edition=Reprinted (with corr.)}}&amp;lt;/ref&amp;gt;&lt;br /&gt;
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Linear PDEs can be reduced to systems of ordinary differential equations by the important technique of separation of variables. This technique rests on a characteristic of solutions to differential equations: if one can find any solution that solves the equation and satisfies the boundary conditions, then it is the solution (this also applies to ODEs). We assume as an ansatz that the dependence of a solution on the parameters space and time can be written as a product of terms that each depend on a single parameter, and then see if this can be made to solve the problem.&lt;br /&gt;
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线性偏微分方程组可以通过分离变量法这一重要方法来简化为常微分方程组。这种方法依赖于微分方程解的一个特征: 如果能找到任何一个满足方程和边界条件的解，那么这个解就是方程的解(这也适用于常微分方程)。我们假设解对参数空间和时间的依赖可以写成对它们每一项的依赖以及一个参数的乘积，然后再看看这是否可以用来解决这个问题。&lt;br /&gt;
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In the method of separation of variables, one reduces a PDE to a PDE in fewer variables, which is an ordinary differential equation if in one variable – these are in turn easier to solve.&lt;br /&gt;
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In the method of separation of variables, one reduces a PDE to a PDE in fewer variables, which is an ordinary differential equation if in one variable – these are in turn easier to solve.&lt;br /&gt;
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在分离变量法方法中，可以将偏微分方程简化为含有更少变量的偏微分方程，如果只有一个变量，那么就变成了一个'''&amp;lt;font color = &amp;quot;#ff8000&amp;quot;&amp;gt;常微分方程 Ordinary Differential Equation&amp;lt;/font&amp;gt;'''-- 反过来，这些方程也更容易求解。&lt;br /&gt;
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This is possible for simple PDEs, which are called [[separable partial differential equation]]s, and the domain is generally a rectangle (a product of intervals). Separable PDEs correspond to [[diagonal matrices]] – thinking of &amp;quot;the value for fixed {{mvar|x}}&amp;quot; as a coordinate, each coordinate can be understood separately.&lt;br /&gt;
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This is possible for simple PDEs, which are called separable partial differential equations, and the domain is generally a rectangle (a product of intervals). Separable PDEs correspond to diagonal matrices – thinking of &amp;quot;the value for fixed &amp;quot; as a coordinate, each coordinate can be understood separately.&lt;br /&gt;
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对于简单的偏微分方程(称为可分离偏微分方程)来说，这是可能的，而且方程通常定义在一个矩形区域(区间的乘积)上。可分离偏微分方程对应于对角线矩阵——以“固定值”为坐标，每个坐标可分开理解。&lt;br /&gt;
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This generalizes to the [[method of characteristics]], and is also used in [[integral transform]]s.&lt;br /&gt;
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This generalizes to the method of characteristics, and is also used in integral transforms.&lt;br /&gt;
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这种方法可以推广到特征曲线法，也可以用于积分变换。&lt;br /&gt;
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===Method of characteristics===&lt;br /&gt;
特征曲线法&lt;br /&gt;
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{{main|Method of characteristics}}&lt;br /&gt;
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In special cases, one can find characteristic curves on which the equation reduces to an ODE – changing coordinates in the domain to straighten these curves allows separation of variables, and is called the [[method of characteristics]].&lt;br /&gt;
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In special cases, one can find characteristic curves on which the equation reduces to an ODE – changing coordinates in the domain to straighten these curves allows separation of variables, and is called the method of characteristics.&lt;br /&gt;
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在特殊情况下，可以找到一些特征曲线，在这些曲线上方程可以变成一个常微分方程——意味着改变坐标从而使这些曲线变直从而达到分离变量的目的，这就是所谓的特征曲线法。&lt;br /&gt;
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More generally, one may find characteristic surfaces.&lt;br /&gt;
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More generally, one may find characteristic surfaces.&lt;br /&gt;
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更一般地说，人们可能会找到特征表面。&lt;br /&gt;
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===Integral transform===&lt;br /&gt;
积分变换&lt;br /&gt;
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An [[integral transform]] may transform the PDE to a simpler one, in particular, a separable PDE. This corresponds to diagonalizing an operator.&lt;br /&gt;
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An integral transform may transform the PDE to a simpler one, in particular, a separable PDE. This corresponds to diagonalizing an operator.&lt;br /&gt;
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积分变换可以将偏微分方程转换为更简单的偏微分方程，特别是可分离的偏微分方程。这对应于对角化算符。&lt;br /&gt;
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An important example of this is [[Fourier analysis]], which diagonalizes the heat equation using the [[eigenbasis]] of sinusoidal waves.&lt;br /&gt;
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An important example of this is Fourier analysis, which diagonalizes the heat equation using the eigenbasis of sinusoidal waves.&lt;br /&gt;
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这方面的一个重要例子是'''&amp;lt;font color = &amp;quot;#ff8000&amp;quot;&amp;gt;傅里叶分析  Fourier Analysis&amp;lt;/font&amp;gt;'''，它使用正弦波的特征基来对角化热方程。&lt;br /&gt;
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If the domain is finite or periodic, an infinite sum of solutions such as a [[Fourier series]] is appropriate, but an integral of solutions such as a [[Fourier integral]] is generally required for infinite domains. The solution for a point source for the heat equation given above is an example of the use of a Fourier integral.&lt;br /&gt;
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If the domain is finite or periodic, an infinite sum of solutions such as a Fourier series is appropriate, but an integral of solutions such as a Fourier integral is generally required for infinite domains. The solution for a point source for the heat equation given above is an example of the use of a Fourier integral.&lt;br /&gt;
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如果区域是有限的或周期性的，那么解为无限和的形式是恰当的，例如傅里叶级数，但是一个解的积分，例如傅立叶积分，一般是在无限区域上的。上面给出的热传导方程的点源解法就是使用傅里叶积分的一个例子。&lt;br /&gt;
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===Change of variables===&lt;br /&gt;
变量代换&lt;br /&gt;
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Often a PDE can be reduced to a simpler form with a known solution by a suitable [[Change of variables (PDE)|change of variables]].  For example, the [[Black–Scholes equation#Derivation|Black–Scholes]] PDE&lt;br /&gt;
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Often a PDE can be reduced to a simpler form with a known solution by a suitable change of variables.  For example, the Black–Scholes PDE&lt;br /&gt;
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偏微分方程通常可以通过变量的适当变化，用已知的解简化为更简单的形式。例如，布莱克-舒尔斯偏微分方程&lt;br /&gt;
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:&amp;lt;math&amp;gt; \frac{\partial V}{\partial t} + \tfrac{1}{2}\sigma^2 S^2\frac{\partial^2 V}{\partial S^2} + rS\frac{\partial V}{\partial S} - rV = 0 &amp;lt;/math&amp;gt;&lt;br /&gt;
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&amp;lt;math&amp;gt; \frac{\partial V}{\partial t} + \tfrac{1}{2}\sigma^2 S^2\frac{\partial^2 V}{\partial S^2} + rS\frac{\partial V}{\partial S} - rV = 0 &amp;lt;/math&amp;gt;&lt;br /&gt;
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is reducible to the [[heat equation]]&lt;br /&gt;
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is reducible to the heat equation&lt;br /&gt;
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可以简化为热传导方程&lt;br /&gt;
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:&amp;lt;math&amp;gt; \frac{\partial u}{\partial \tau} = \frac{\partial^2 u}{\partial x^2}&amp;lt;/math&amp;gt;&lt;br /&gt;
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&amp;lt;math&amp;gt; \frac{\partial u}{\partial \tau} = \frac{\partial^2 u}{\partial x^2}&amp;lt;/math&amp;gt;&lt;br /&gt;
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by the change of variables (for complete details see {{webarchive |url=https://web.archive.org/web/20080411030405/http://www.math.unl.edu/~sdunbar1/Teaching/MathematicalFinance/Lessons/BlackScholes/Solution/solution.shtml |date=April 11, 2008 |title=Solution of the Black Scholes Equation }})&lt;br /&gt;
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by the change of variables (for complete details see )&lt;br /&gt;
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通过变量替换(完整的细节见)&lt;br /&gt;
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:&amp;lt;math&amp;gt;\begin{align}&lt;br /&gt;
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V(S,t) &amp;amp;= K v(x,\tau),\\[5px]&lt;br /&gt;
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x &amp;amp;= \ln\left(\tfrac{S}{K} \right),\\[5px]&lt;br /&gt;
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\tau &amp;amp;= \tfrac{1}{2} \sigma^2 (T - t),\\[5px]&lt;br /&gt;
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v(x,\tau)&amp;amp;=e^{-\alpha x-\beta\tau} u(x,\tau).&lt;br /&gt;
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\end{align}&amp;lt;/math&amp;gt;&lt;br /&gt;
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===Fundamental solution===&lt;br /&gt;
基本解&lt;br /&gt;
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{{main|Fundamental solution}}&lt;br /&gt;
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Inhomogeneous equations can often be solved (for constant coefficient PDEs, always be solved) by finding the [[fundamental solution]] (the solution for a point source), then taking the [[convolution]] with the boundary conditions to get the solution.&lt;br /&gt;
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Inhomogeneous equations can often be solved (for constant coefficient PDEs, always be solved) by finding the fundamental solution (the solution for a point source), then taking the convolution with the boundary conditions to get the solution.&lt;br /&gt;
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非齐次方程(常系数偏微分方程)一般是通过先求出基本解(点源的解) ，然后利用带边界条件的卷积来求解。&lt;br /&gt;
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This is analogous in [[signal processing]] to understanding a filter by its [[impulse response]].&lt;br /&gt;
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This is analogous in signal processing to understanding a filter by its impulse response.&lt;br /&gt;
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这类似于在信号处理中通过滤波器的脉冲响应来理解滤波器。&lt;br /&gt;
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===Superposition principle===&lt;br /&gt;
叠加原理&lt;br /&gt;
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{{further| Superposition principle }}&lt;br /&gt;
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The superposition principle applies to any linear system, including linear systems of PDEs. A common visualization of this concept is the interaction of two waves in phase being combined to result in a greater amplitude, for example {{math|sin ''x'' + sin ''x'' {{=}} 2 sin ''x''}}. The same principle can be observed in PDEs where the solutions may be real or complex and additive. [[Superposition principle|superposition]]&lt;br /&gt;
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The superposition principle applies to any linear system, including linear systems of PDEs. A common visualization of this concept is the interaction of two waves in phase being combined to result in a greater amplitude, for example  2 sin x}}. The same principle can be observed in PDEs where the solutions may be real or complex and additive. superposition&lt;br /&gt;
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'''&amp;lt;font color = &amp;quot;#ff8000&amp;quot;&amp;gt;叠加原理 Superposition Principle&amp;lt;/font&amp;gt;适用于任何线性系统，包括偏微分方程的线性系统。这个概念的一个常见的可视化是两个同相位的波相互作用结合在一起会产生更大的振幅，例如 {{math|sin ''x'' + sin ''x'' {{=}} 2 sin ''x''}}。在偏微分方程中也可以观察到同样的原理，其中的解可能是真实的或复杂的和可加的。叠加&lt;br /&gt;
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If {{math|''u''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;}} and {{math|''u''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;}} are solutions of linear PDE in some function space {{mvar|R}}, then {{math|''u'' {{=}} ''c''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;''u''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; + ''c''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;''u''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;}} with any constants {{math|''c''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;}} and {{math|''c''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;}} are also a solution of that PDE in the same function space.&lt;br /&gt;
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If  and  are solutions of linear PDE in some function space , then  c&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;u&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; + c&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;u&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;}} with any constants  and  are also a solution of that PDE in the same function space.&lt;br /&gt;
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若线性偏微分方程在某个函数空间{{mvar|R}}中有解{{math|''u''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;}} 和 {{math|''u''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;}}，则{{math|''u'' {{=}} ''c''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;''u''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; + ''c''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;''u''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;}}也是该偏微分方程在同一函数空间中的解，其中{{math|''c''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;}} 和 {{math|''c''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;}} 是任意常数。&lt;br /&gt;
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===Methods for non-linear equations===&lt;br /&gt;
非线性方程的求解方法&lt;br /&gt;
{{see also|nonlinear partial differential equation}}&lt;br /&gt;
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There are no generally applicable methods to solve nonlinear PDEs. Still, existence and uniqueness results (such as the [[Cauchy–Kowalevski theorem]]) are often possible, as are proofs of important qualitative and quantitative properties of solutions (getting these results is a major part of [[mathematical analysis|analysis]]). Computational solution to the nonlinear PDEs, the [[split-step method]], exist for specific equations like [[nonlinear Schrödinger equation]].&lt;br /&gt;
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There are no generally applicable methods to solve nonlinear PDEs. Still, existence and uniqueness results (such as the Cauchy–Kowalevski theorem) are often possible, as are proofs of important qualitative and quantitative properties of solutions (getting these results is a major part of analysis). Computational solution to the nonlinear PDEs, the split-step method, exist for specific equations like nonlinear Schrödinger equation.&lt;br /&gt;
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对于非线性偏微分方程，目前还没有普遍适用的求解方法。然而，通常是可能知道解的存在性和唯一性(如柯西-科瓦列夫斯基定理)，也是可能得到解的重要定性和定量性质的证明(得到这些结果是分析的主要部分)。非线性偏微分方程的计算解，即分步法，对一些特定的方程适用，比如非线性'''&amp;lt;font color=&amp;quot;#ff8000&amp;quot;&amp;gt;薛定谔方程 Schrödinger equation&amp;lt;/font&amp;gt;'''。&lt;br /&gt;
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Nevertheless, some techniques can be used for several types of equations. The [[h-principle|{{mvar|h}}-principle]] is the most powerful method to solve [[Underdetermined system|underdetermined]] equations. The [[Riquier–Janet theory]] is an effective method for obtaining information about many analytic [[Overdetermined system|overdetermined]] systems.&lt;br /&gt;
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Nevertheless, some techniques can be used for several types of equations. The -principle is the most powerful method to solve underdetermined equations. The Riquier–Janet theory is an effective method for obtaining information about many analytic overdetermined systems.&lt;br /&gt;
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然而，一些技巧可以用于几种类型的方程。h-原理是求解欠定方程最有效的方法。里基尔-珍妮特理论是一种可以获得许多解析超定系统信息的有效方法。&lt;br /&gt;
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The [[method of characteristics]] can be used in some very special cases to solve partial differential equations.&lt;br /&gt;
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The method of characteristics can be used in some very special cases to solve partial differential equations.&lt;br /&gt;
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特征线法可用于求解某些特殊情况下的偏微分方程。&lt;br /&gt;
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In some cases, a PDE can be solved via [[perturbation analysis]] in which the solution is considered to be a correction to an equation with a known solution. Alternatives are [[numerical analysis]] techniques from simple [[finite difference]] schemes to the more mature [[multigrid]] and [[finite element method]]s. Many interesting problems in science and engineering are solved in this way using [[computer]]s, sometimes high performance [[supercomputer]]s.&lt;br /&gt;
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In some cases, a PDE can be solved via perturbation analysis in which the solution is considered to be a correction to an equation with a known solution. Alternatives are numerical analysis techniques from simple finite difference schemes to the more mature multigrid and finite element methods. Many interesting problems in science and engineering are solved in this way using computers, sometimes high performance supercomputers.&lt;br /&gt;
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在某些情况下，偏微分方程可以通过扰动分析来求解。在扰动分析中，通常是求解将具有已知解的方程修正后的新得到方程。可供选择的数值分析技术从简单的差分格式到更成熟的多重网格和有限元方法。许多有趣的科学和工程问题都是在计算机上用这种方法解决的，有时是高性能超级计算机。&lt;br /&gt;
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===Lie group method===&lt;br /&gt;
李群方法&lt;br /&gt;
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From 1870 [[Sophus Lie]]'s work put the theory of differential equations on a more satisfactory foundation. He showed that the integration theories of the older mathematicians can, by the introduction of what are now called [[Lie group]]s, be referred, to a common source; and that ordinary differential equations which admit the same [[infinitesimal transformation]]s present comparable difficulties of integration. He also emphasized the subject of [[contact transformation|transformations of contact]].&lt;br /&gt;
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From 1870 Sophus Lie's work put the theory of differential equations on a more satisfactory foundation. He showed that the integration theories of the older mathematicians can, by the introduction of what are now called Lie groups, be referred, to a common source; and that ordinary differential equations which admit the same infinitesimal transformations present comparable difficulties of integration. He also emphasized the subject of transformations of contact.&lt;br /&gt;
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从1870年起，索弗斯·李的工作为微分方程理论奠定了一个较为令人满意的基础。他指出，通过引入现在所谓的李群，老一辈数学家的积分理论可以引用到一个共同的来源; 承认相同的无穷小变换的常微分方程在积分方面存在相当的困难。他还强调了接触的转变这一主题。&lt;br /&gt;
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==[[用户:Yuling|Yuling]]（[[用户讨论:Yuling|讨论]]）这句话“He also emphasized the subject of transformations of contact.”中的transformations of contact翻译的不太好。&lt;br /&gt;
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A general approach to solving PDEs uses the symmetry property of differential equations, the continuous [[infinitesimal transformation]]s of solutions to solutions ([[Lie theory]]). Continuous [[group theory]], [[Lie algebras]] and [[differential geometry]] are used to understand the structure of linear and nonlinear partial differential equations for generating integrable equations, to find its [[Lax pair]]s, recursion operators, [[Bäcklund transform]] and finally finding exact analytic solutions to the PDE.&lt;br /&gt;
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A general approach to solving PDEs uses the symmetry property of differential equations, the continuous infinitesimal transformations of solutions to solutions (Lie theory). Continuous group theory, Lie algebras and differential geometry are used to understand the structure of linear and nonlinear partial differential equations for generating integrable equations, to find its Lax pairs, recursion operators, Bäcklund transform and finally finding exact analytic solutions to the PDE.&lt;br /&gt;
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求解偏微分方程的一般方法是利用微分方程的对称性，即解到解的连续无穷小变换(李理论)。连续群论、李代数和微分几何理论被用来理解生成可积方程的线性和非线性偏微分方程的结构，找到它的Lax对、递归算子、 贝克伦德变换，最后找到偏微分方程的精确解析解。&lt;br /&gt;
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Symmetry methods have been recognized to study differential equations arising in mathematics, physics, engineering, and many other disciplines.&lt;br /&gt;
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Symmetry methods have been recognized to study differential equations arising in mathematics, physics, engineering, and many other disciplines.&lt;br /&gt;
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对称方法已被公认可以用于研究出现在数学，物理，工程和许多其他学科的微分方程。&lt;br /&gt;
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===Semianalytical methods===&lt;br /&gt;
半解析方法&lt;br /&gt;
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The [[Adomian decomposition method]], the [[Aleksandr Lyapunov|Lyapunov]] artificial small parameter method, and He's [[homotopy perturbation method]] are all special cases of the more general [[homotopy analysis method]]. These are series expansion methods, and except for the Lyapunov method, are independent of small physical parameters as compared to the well known [[perturbation theory]], thus giving these methods greater flexibility and solution generality.&lt;br /&gt;
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The Adomian decomposition method, the Lyapunov artificial small parameter method, and He's homotopy perturbation method are all special cases of the more general homotopy analysis method. These are series expansion methods, and except for the Lyapunov method, are independent of small physical parameters as compared to the well known perturbation theory, thus giving these methods greater flexibility and solution generality.&lt;br /&gt;
&lt;br /&gt;
阿多米安分解法、李雅普诺夫人工小参数方法和何同伦摄动方法都是更一般的同伦分析方法的特殊情况。除了李雅普诺夫方法之外，这些都是级数展开方法，与为人熟知的摄动理论方法相比，它们与小的物理参数无关，因此这些方法具有更大的灵活性和解的通用性。&lt;br /&gt;
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== Numerical solutions ==&lt;br /&gt;
数值解&lt;br /&gt;
&lt;br /&gt;
The three most widely used [[Numerical partial differential equations|numerical methods to solve PDEs]] are the [[finite element analysis|finite element method]] (FEM), [[finite volume method]]s (FVM) and [[finite difference method]]s (FDM), as well other kind of methods called [[Meshfree methods]], which were made to solve problems where the before mentioned methods are limited. The FEM has a prominent position among these methods and especially its exceptionally efficient higher-order version [[hp-FEM]]. Other hybrid versions of FEM and Meshfree methods include the generalized finite element method (GFEM), [[extended finite element method]] (XFEM), [[Spectral element method|spectral finite element method]] (SFEM), [[Meshfree methods|meshfree finite element method]], [[Discontinuous Galerkin Method|discontinuous Galerkin finite element method]] (DGFEM), [[Element-Free Galerkin Method]] (EFGM), [[Interpolating Element-Free Galerkin Method]] (IEFGM), etc.&lt;br /&gt;
&lt;br /&gt;
The three most widely used numerical methods to solve PDEs are the finite element method (FEM), finite volume methods (FVM) and finite difference methods (FDM), as well other kind of methods called Meshfree methods, which were made to solve problems where the before mentioned methods are limited. The FEM has a prominent position among these methods and especially its exceptionally efficient higher-order version hp-FEM. Other hybrid versions of FEM and Meshfree methods include the generalized finite element method (GFEM), extended finite element method (XFEM), spectral finite element method (SFEM), meshfree finite element method, discontinuous Galerkin finite element method (DGFEM), Element-Free Galerkin Method (EFGM), Interpolating Element-Free Galerkin Method (IEFGM), etc.&lt;br /&gt;
&lt;br /&gt;
求解偏微分方程最常用的三种数值方法是有限元分析法、有限体积法和有限差分法，以及其他一些称为无网格法的方法。这些方法用于解决前面提到的方法受到的限制。在这些方法中，有限元方法，尤其是高效的高阶有限元方法，占有重要地位。其他有限元法和无网格法的混合形式包括广义有限元分析法(GFEM)、扩展有限元分析法(XFEM)、谱有限元分析法(SFEM)、无网格有限元分析法(DGFEM)、间断伽辽金有限元分析法(DGFEM)、无网格伽辽金法(EFGM)、插值无网格伽辽金法(IEFGM)等。&lt;br /&gt;
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=== Finite element method ===&lt;br /&gt;
有限元分析法&lt;br /&gt;
&lt;br /&gt;
{{main|Finite element method}}&lt;br /&gt;
&lt;br /&gt;
The finite element method (FEM) (its practical application often known as finite element analysis (FEA)) is a numerical technique for finding approximate solutions of partial differential equations (PDE) as well as of integral equations. The solution approach is based either on eliminating the differential equation completely (steady state problems), or rendering the PDE into an approximating system of ordinary differential equations, which are then numerically integrated using standard techniques such as Euler's method, Runge–Kutta, etc.&lt;br /&gt;
&lt;br /&gt;
The finite element method (FEM) (its practical application often known as finite element analysis (FEA)) is a numerical technique for finding approximate solutions of partial differential equations (PDE) as well as of integral equations. The solution approach is based either on eliminating the differential equation completely (steady state problems), or rendering the PDE into an approximating system of ordinary differential equations, which are then numerically integrated using standard techniques such as Euler's method, Runge–Kutta, etc.&lt;br /&gt;
&lt;br /&gt;
'''&amp;lt;font color = &amp;quot;#ff8000&amp;quot;&amp;gt;有限元分析法 Finite Element Method&amp;lt;/font&amp;gt;''' ((其实际应用通常被称为有限元分析(FEA))是一种寻找偏微分方程(PDE)和积分方程近似解的数值技术。这种求解方法要么基于完全消除微分方程(稳态问题) ，要么将偏微分方程转化为常微分方程的近似系统，然后使用标准技术进行数值积分，如欧拉方法、 Runge-Kutta 等。&lt;br /&gt;
&lt;br /&gt;
===Finite difference method===&lt;br /&gt;
有限差分法&lt;br /&gt;
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&lt;br /&gt;
{{main|Finite difference method}}&lt;br /&gt;
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Finite-difference methods are numerical methods for approximating the solutions to differential equations using [[finite difference]] equations to approximate derivatives.&lt;br /&gt;
&lt;br /&gt;
Finite-difference methods are numerical methods for approximating the solutions to differential equations using finite difference equations to approximate derivatives.&lt;br /&gt;
&lt;br /&gt;
有限差分法是一种数值方法，用差分方程近似微分方程的解。&lt;br /&gt;
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=== Finite volume method ===&lt;br /&gt;
有限体积法&lt;br /&gt;
&lt;br /&gt;
{{main|Finite volume method}}&lt;br /&gt;
&lt;br /&gt;
Similar to the finite difference method or finite element method, values are calculated at discrete places on a meshed geometry. &amp;quot;Finite volume&amp;quot; refers to the small volume surrounding each node point on a mesh. In the finite volume method, surface integrals in a partial differential equation that contain a divergence term are converted to volume integrals, using the [[divergence theorem]]. These terms are then evaluated as fluxes at the surfaces of each finite volume. Because the flux entering a given volume is identical to that leaving the adjacent volume, these methods conserve mass by design.&lt;br /&gt;
&lt;br /&gt;
Similar to the finite difference method or finite element method, values are calculated at discrete places on a meshed geometry. &amp;quot;Finite volume&amp;quot; refers to the small volume surrounding each node point on a mesh. In the finite volume method, surface integrals in a partial differential equation that contain a divergence term are converted to volume integrals, using the divergence theorem. These terms are then evaluated as fluxes at the surfaces of each finite volume. Because the flux entering a given volume is identical to that leaving the adjacent volume, these methods conserve mass by design.&lt;br /&gt;
&lt;br /&gt;
类似于有限差分法或有限元分析，函数值是在网状几何体上的离散位置进行计算的。“有限体积”是指网格上每个节点周围的小体积。在有限体积法中，偏微分方程中含有散度项的面积分用散度定理积分转换成体积分。然后将这些项用于估算每个有限体积表面上的通量。由于进入给定体积的通量与转移到相邻体积元的通量相同，所以这些方法在设计上保证了质量守恒。&lt;br /&gt;
&lt;br /&gt;
==See also==&lt;br /&gt;
请参阅&lt;br /&gt;
* [[Dirichlet boundary condition]]&lt;br /&gt;
狄利克雷边界条件&lt;br /&gt;
* [[Jet bundle]]&lt;br /&gt;
射流丛&lt;br /&gt;
* [[Laplace transform applied to differential equations]]&lt;br /&gt;
微分方程中的拉普拉斯变换&lt;br /&gt;
* [[List of dynamical systems and differential equations topics]]&lt;br /&gt;
动力学系统和微分方程的列表&lt;br /&gt;
* [[Matrix differential equation]]&lt;br /&gt;
矩阵微分方程&lt;br /&gt;
* [[Neumann boundary condition]]&lt;br /&gt;
诺伊曼边界条件&lt;br /&gt;
* [[Numerical partial differential equations]]&lt;br /&gt;
数值偏微分方程&lt;br /&gt;
* [[Partial differential algebraic equation]]&lt;br /&gt;
偏微分代数方程&lt;br /&gt;
* [[Recurrence relation]]&lt;br /&gt;
递推关系&lt;br /&gt;
* [[Robin boundary condition]]&lt;br /&gt;
罗宾边界条件&lt;br /&gt;
* [[Stochastic processes and boundary value problems]]&lt;br /&gt;
随机过程和边值问题&lt;br /&gt;
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== The energy method ==&lt;br /&gt;
能量法&lt;br /&gt;
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The energy method is a mathematical procedure that can be used to verify well-posedness of initial-boundary-value-problems.&amp;lt;ref&amp;gt;{{cite book |title=High Order Difference Methods for Time Dependent PDE&lt;br /&gt;
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The energy method is a mathematical procedure that can be used to verify well-posedness of initial-boundary-value-problems.&amp;lt;ref&amp;gt;{{cite book |title=High Order Difference Methods for Time Dependent PDE&lt;br /&gt;
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能量法是验证初边值问题适定性的一种数学方法。 时变偏微分方程的高阶差分方法&lt;br /&gt;
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|first=Bertil|last=Gustafsson|publisher=Springer|year=2008|isbn=978-3-540-74992-9|doi=10.1007/978-3-540-74993-6}}&amp;lt;/ref&amp;gt; In the following example the energy method is used to decide where and which boundary conditions should be imposed such that the resulting IBVP is well-posed. Consider the one-dimensional hyperbolic PDE given by&lt;br /&gt;
&lt;br /&gt;
|first=Bertil|last=Gustafsson|publisher=Springer|year=2008|isbn=978-3-540-74992-9|doi=10.1007/978-3-540-74993-6}}&amp;lt;/ref&amp;gt; In the following example the energy method is used to decide where and which boundary conditions should be imposed such that the resulting IBVP is well-posed. Consider the one-dimensional hyperbolic PDE given by&lt;br /&gt;
&lt;br /&gt;
| first Bertil | last Gustafsson | publisher | Springer | year 2008 | isbn 978-3-540-74992-9 | doi 10.1007 / 978-3-540-74993-6} / ref 在下面的例子中，使用能量方法来决定应该施加哪些边界条件，使得得到的 IBVP适定。考虑一维双曲偏微分方程&lt;br /&gt;
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: &amp;lt;math&amp;gt;\frac{\partial u}{\partial t} + \alpha \frac{\partial u}{\partial x} = 0, \quad x \in [a,b], \operatorname t &amp;gt; 0,&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;\frac{\partial u}{\partial t} + \alpha \frac{\partial u}{\partial x} = 0, \quad x \in [a,b], \operatorname t &amp;gt; 0,&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
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where &amp;lt;math&amp;gt;\alpha \neq 0&amp;lt;/math&amp;gt; is a constant and &amp;lt;math&amp;gt;u(x,t)&amp;lt;/math&amp;gt; is an unknown function with initial condition &amp;lt;math&amp;gt;u(x,0) = f(x)&amp;lt;/math&amp;gt;. Multiplying with &amp;lt;math&amp;gt;u&amp;lt;/math&amp;gt; and integrating over the domain gives&lt;br /&gt;
&lt;br /&gt;
where &amp;lt;math&amp;gt;\alpha \neq 0&amp;lt;/math&amp;gt; is a constant and &amp;lt;math&amp;gt;u(x,t)&amp;lt;/math&amp;gt; is an unknown function with initial condition &amp;lt;math&amp;gt;u(x,0) = f(x)&amp;lt;/math&amp;gt;. Multiplying with &amp;lt;math&amp;gt;u&amp;lt;/math&amp;gt; and integrating over the domain gives&lt;br /&gt;
&lt;br /&gt;
其中 &amp;lt;math&amp;gt;\alpha \neq 0&amp;lt;/math&amp;gt; 是常数，并且 &amp;lt;math&amp;gt;u(x,t)&amp;lt;/math&amp;gt; 是未知函数，初始条件是 &amp;lt;math&amp;gt;u(x,0) = f(x)&amp;lt;/math&amp;gt;。乘以 &amp;lt;math&amp;gt;u&amp;lt;/math&amp;gt; 并在域上进行积分。&lt;br /&gt;
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&lt;br /&gt;
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: &amp;lt;math&amp;gt;\int_a^b u \frac{\partial u}{\partial t} \operatorname dx + \alpha \int _a ^b u \frac{\partial u}{\partial x} \operatorname dx = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;\int_a^b u \frac{\partial u}{\partial t} \operatorname dx + \alpha \int _a ^b u \frac{\partial u}{\partial x} \operatorname dx = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
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Using that&lt;br /&gt;
&lt;br /&gt;
Using that&lt;br /&gt;
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利用这一点&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt;\int _a ^b u \frac{\partial u}{\partial t} \operatorname dx = \frac{1}{2} \frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 \quad \text{and} \quad \int _a ^b u \frac{\partial u}{\partial x} \operatorname dx = \frac{1}{2} u(b,t)^2 - \frac{1}{2} u(a,t)^2,.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;\int _a ^b u \frac{\partial u}{\partial t} \operatorname dx = \frac{1}{2} \frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 \quad \text{and} \quad \int _a ^b u \frac{\partial u}{\partial x} \operatorname dx = \frac{1}{2} u(b,t)^2 - \frac{1}{2} u(a,t)^2,.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
where integration by parts has been used for the second relationship, we get&lt;br /&gt;
&lt;br /&gt;
where integration by parts has been used for the second relationship, we get&lt;br /&gt;
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第二个关系中采用了分部积分法，我们可以得到&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt;\frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 + \alpha u(b,t)^2 - \alpha u(a,t)^2 = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;\frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 + \alpha u(b,t)^2 - \alpha u(a,t)^2 = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Here &amp;lt;math&amp;gt;\vert \vert \cdot \vert \vert&amp;lt;/math&amp;gt; denotes the standard L2-norm.&lt;br /&gt;
&lt;br /&gt;
Here &amp;lt;math&amp;gt;\vert \vert \cdot \vert \vert&amp;lt;/math&amp;gt; denotes the standard L2-norm.&lt;br /&gt;
&lt;br /&gt;
在这里，&amp;lt;math&amp;gt;\vert \vert \cdot \vert \vert&amp;lt;/math&amp;gt; 表示标准的 L2-正则。&lt;br /&gt;
&lt;br /&gt;
For well-posedness we require that the energy of the solution is non-increasing, i.e. that &amp;lt;math&amp;gt;\frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 \leq 0&amp;lt;/math&amp;gt;, which is achieved by specifying &amp;lt;math&amp;gt;u&amp;lt;/math&amp;gt; at &amp;lt;math&amp;gt;x = a&amp;lt;/math&amp;gt; if &amp;lt;math&amp;gt;\alpha &amp;gt; 0&amp;lt;/math&amp;gt; and at &amp;lt;math&amp;gt;x = b&amp;lt;/math&amp;gt; if &amp;lt;math&amp;gt;\alpha &amp;lt; 0&amp;lt;/math&amp;gt;. This corresponds to only imposing boundary conditions at the inflow. Note that well-posedness allows for growth in terms of data (initial and boundary) and thus it is sufficient to show that &amp;lt;math&amp;gt;\frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 \leq 0&amp;lt;/math&amp;gt; holds when all data is set to zero.&lt;br /&gt;
&lt;br /&gt;
For well-posedness we require that the energy of the solution is non-increasing, i.e. that &amp;lt;math&amp;gt;\frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 \leq 0&amp;lt;/math&amp;gt;, which is achieved by specifying &amp;lt;math&amp;gt;u&amp;lt;/math&amp;gt; at &amp;lt;math&amp;gt;x = a&amp;lt;/math&amp;gt; if &amp;lt;math&amp;gt;\alpha &amp;gt; 0&amp;lt;/math&amp;gt; and at &amp;lt;math&amp;gt;x = b&amp;lt;/math&amp;gt; if &amp;lt;math&amp;gt;\alpha &amp;lt; 0&amp;lt;/math&amp;gt;. This corresponds to only imposing boundary conditions at the inflow. Note that well-posedness allows for growth in terms of data (initial and boundary) and thus it is sufficient to show that &amp;lt;math&amp;gt;\frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 \leq 0&amp;lt;/math&amp;gt; holds when all data is set to zero.&lt;br /&gt;
&lt;br /&gt;
对于适定性，我们要解的能量是不增加的，即 &amp;lt;math&amp;gt;\frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 \leq 0&amp;lt;/math&amp;gt; ，这种关系可以通过在&amp;lt;math&amp;gt;x = a&amp;lt;/math&amp;gt;处 （如果 &amp;lt;math&amp;gt;\alpha &amp;gt; 0&amp;lt;/math&amp;gt;） 以及 &amp;lt;math&amp;gt;x = b&amp;lt;/math&amp;gt;处 （如果 &amp;lt;math&amp;gt;\alpha &amp;lt; 0&amp;lt;/math&amp;gt;）指定&amp;lt;math&amp;gt;u&amp;lt;/math&amp;gt;的值来实现。这只相当于在入流处附加边界条件。注意，适定性允许在数据(初始和边界)上的增长，因此它足以表明当所有数据设置为零时应有 &amp;lt;math&amp;gt;\frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 \leq 0&amp;lt;/math&amp;gt;。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==[[用户:Yuling|Yuling]]（[[用户讨论:Yuling|讨论]]）“This corresponds to only imposing boundary conditions at the inflow.” 这句话中的inflow不是很理解&lt;br /&gt;
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==Notes==&lt;br /&gt;
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{{Reflist}}&lt;br /&gt;
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== References ==&lt;br /&gt;
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{{refbegin|2}}&lt;br /&gt;
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&lt;br /&gt;
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&lt;br /&gt;
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* {{Citation |first=A. D. |last=Polyanin |first2=V. F. |last2=Zaitsev |lastauthoramp=yes |first3=A. |last3=Moussiaux |title=Handbook of First Order Partial Differential Equations |publisher=Taylor &amp;amp; Francis |location=London |year=2002 |isbn=0-415-27267-X }}.&lt;br /&gt;
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* {{citation|mr=3014456|last=Roubíček|first= T.|title=Nonlinear Partial Differential Equations with Applications|publisher= Birkhäuser|place= Basel, Boston, Berlin|edition=2nd|year= 2013|ISBN= 978-3-0348-0512-4|doi=10.1007/978-3-0348-0513-1|url=http://cds.cern.ch/record/880983/files/9783764372934_TOC.pdf}}&lt;br /&gt;
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* {{Citation |first=P. |last=Solin |title=Partial Differential Equations and the Finite Element Method |publisher=J. Wiley &amp;amp; Sons |location=Hoboken, NJ |year=2005 |isbn=0-471-72070-4 }}.&lt;br /&gt;
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* {{Citation |first=P. |last=Solin |first2=K. |last2=Segeth |lastauthoramp=yes |first3=I. |last3=Dolezel |title=Higher-Order Finite Element Methods |publisher=Chapman &amp;amp; Hall/CRC Press |location=Boca Raton |year=2003 |isbn=1-58488-438-X }}.&lt;br /&gt;
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* {{Citation |first=H. |last=Stephani |year=1989 |title=Differential Equations: Their Solution Using Symmetries. Edited by M. MacCallum |publisher=Cambridge University Press }}.&lt;br /&gt;
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* {{cite book |title=Partial Differential Equations and Solitary Waves Theory&lt;br /&gt;
&lt;br /&gt;
|first=Abdul-Majid|last=Wazwaz|publisher=Higher Education Press|year=2009|isbn=978-3-642-00251-9|page=}}&lt;br /&gt;
&lt;br /&gt;
|first=Abdul-Majid|last=Wazwaz|publisher=Higher Education Press|year=2009|isbn=978-3-642-00251-9|page=}}&lt;br /&gt;
&lt;br /&gt;
| first Abdul-Majid | last Wazwaz | publisher Higher Education Press | year 2009 | isbn 978-3-642-00251-9 | page }&lt;br /&gt;
&lt;br /&gt;
* {{cite book |title=Partial Differential Equations Methods and Applications&lt;br /&gt;
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|first=Abdul-Majid|last=Wazwaz|publisher=A.A. Balkema|year=2002|isbn=90-5809-369-7|page=}}&lt;br /&gt;
&lt;br /&gt;
|first=Abdul-Majid|last=Wazwaz|publisher=A.A. Balkema|year=2002|isbn=90-5809-369-7|page=}}&lt;br /&gt;
&lt;br /&gt;
| first Abdul-Majid | last Wazwaz | publisher a.a.Balkema | year 2002 | isbn 90-5809-369-7 | page }&lt;br /&gt;
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* {{Citation |first=D. |last=Zwillinger |title=Handbook of Differential Equations |publisher=Academic Press |location=Boston |year=1997 |edition=3rd |isbn=0-12-784395-7 }}.&lt;br /&gt;
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* {{Citation |authorlink=Neil Gershenfeld |first=N. |last=Gershenfeld |title=The Nature of Mathematical Modeling |location=New York |publisher=Cambridge University Press, New York, NY, USA |year=1999 |edition=1st |isbn=0-521-57095-6 }}.&lt;br /&gt;
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* {{Citation |first=I.S. |last=Krasil'shchik |lastauthoramp=yes |first2=A.M., Eds. |last2=Vinogradov |title=Symmetries and Conserwation Laws for Differential Equations of Mathematical Physics |publisher=American Mathematical Society, Providence, Rhode Island, USA |year=1999 |isbn=0-8218-0958-X }}.&lt;br /&gt;
&lt;br /&gt;
* {{Citation |first=I.S. |last=Krasil'shchik |first2=V.V. |last2=Lychagin|lastauthoramp=yes |first3=A.M. |last3=Vinogradov |title=Geometry of Jet Spaces and Nonlinear Partial Differential Equations |publisher=Gordon and Breach Science Publishers, New York, London, Paris, Montreux, Tokyo |year=1986 |isbn=2-88124-051-8 }}.&lt;br /&gt;
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* {{Citation |first=A.M. |last=Vinogradov |title=Cohomological Analysis of Partial Differential Equations and Secondary Calculus |publisher=American Mathematical Society, Providence, Rhode Island, USA |year=2001 |isbn=0-8218-2922-X }}.&lt;br /&gt;
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* {{cite book |title=High Order Difference Methods for Time Dependent PDE&lt;br /&gt;
&lt;br /&gt;
|first=Bertil|last=Gustafsson|publisher=Springer|year=2008|isbn=978-3-540-74992-9|doi=10.1007/978-3-540-74993-6}}&lt;br /&gt;
&lt;br /&gt;
|first=Bertil|last=Gustafsson|publisher=Springer|year=2008|isbn=978-3-540-74992-9|doi=10.1007/978-3-540-74993-6}}&lt;br /&gt;
&lt;br /&gt;
| first Bertil | last Gustafsson | Springer | year 2008 | isbn 978-3-540-74992-9 | doi 10.1007 / 978-3-540-74993-6}&lt;br /&gt;
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{{refend}}&lt;br /&gt;
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== Further reading ==&lt;br /&gt;
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* {{Cite journal|last=Cajori|first=Florian|authorlink=Florian Cajori|year=1928|title=The Early History of Partial Differential Equations and of Partial Differentiation and Integration|url=http://www.math.harvard.edu/archive/21a_fall_14/exhibits/cajori/cajori.pdf|journal=The American Mathematical Monthly|volume=35|issue=9|pages=459–467|doi=10.2307/2298771|access-date=2016-05-15|archive-url=https://web.archive.org/web/20181123102253/http://www.math.harvard.edu/archive/21a_fall_14/exhibits/cajori/cajori.pdf|archive-date=2018-11-23|url-status=dead}}&lt;br /&gt;
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== External links ==&lt;br /&gt;
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{{Sister project links| wikt=no | commons=Category:Solutions of PDE | b=Partial Differential Equations | n=no | q=Partial differential equation | s=no | v=no | voy=no | species=no | d=no}}&lt;br /&gt;
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* {{springer|title=Differential equation, partial|id=p/d031920}}&lt;br /&gt;
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* [http://eqworld.ipmnet.ru/en/pde-en.htm Partial Differential Equations: Exact Solutions] at EqWorld: The World of Mathematical Equations.&lt;br /&gt;
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* [http://eqworld.ipmnet.ru/en/solutions/eqindex/eqindex-pde.htm Partial Differential Equations: Index] at EqWorld: The World of Mathematical Equations.&lt;br /&gt;
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* [http://eqworld.ipmnet.ru/en/methods/meth-pde.htm Partial Differential Equations: Methods] at EqWorld: The World of Mathematical Equations.&lt;br /&gt;
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* [https://web.archive.org/web/20170701144823/http://www.exampleproblems.com/wiki/index.php?title=Partial_Differential_Equations Example problems with solutions] at exampleproblems.com&lt;br /&gt;
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* [http://mathworld.wolfram.com/PartialDifferentialEquation.html Partial Differential Equations] at mathworld.wolfram.com&lt;br /&gt;
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* [https://reference.wolfram.com/language/FEMDocumentation/tutorial/SolvingPDEwithFEM.html Partial Differential Equations] with Mathematica&lt;br /&gt;
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* [http://www.mathworks.com/moler/pdes.pdf Partial Differential Equations] in Cleve Moler: Numerical Computing with MATLAB&lt;br /&gt;
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* [http://www.nag.com/numeric/fl/nagdoc_fl24/html/D03/d03intro.html Partial Differential Equations] at nag.com&lt;br /&gt;
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* {{cite web |first=Grant |last=Sanderson |title=But what is a partial differential equation? |work=3Blue1Brown |date=April 21, 2019 |url=https://www.youtube.com/watch?v=ly4S0oi3Yz8&amp;amp;list=PLZHQObOWTQDNPOjrT6KVlfJuKtYTftqH6 |via=[[YouTube]] }}&lt;br /&gt;
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{{Differential equations topics}}&lt;br /&gt;
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[[Category:Partial differential equations| ]]&lt;br /&gt;
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[[Category:Multivariable calculus]]&lt;br /&gt;
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Category:Multivariable calculus&lt;br /&gt;
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类别: 多元微积分&lt;br /&gt;
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[[Category:Differential equations]]&lt;br /&gt;
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Category:Differential equations&lt;br /&gt;
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类别: 微分方程&lt;br /&gt;
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[[Category:Concepts in physics]]&lt;br /&gt;
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Category:Concepts in physics&lt;br /&gt;
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&amp;lt;small&amp;gt;This page was moved from [[wikipedia:en:Partial differential equation]]. Its edit history can be viewed at [[偏微分方程/edithistory]]&amp;lt;/small&amp;gt;&amp;lt;/noinclude&amp;gt;&lt;br /&gt;
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[[Category:待整理页面]]&lt;/div&gt;</summary>
		<author><name>Ruili</name></author>
	</entry>
	<entry>
		<id>https://wiki.swarma.org/index.php?title=%E5%81%8F%E5%BE%AE%E5%88%86%E6%96%B9%E7%A8%8B&amp;diff=17749</id>
		<title>偏微分方程</title>
		<link rel="alternate" type="text/html" href="https://wiki.swarma.org/index.php?title=%E5%81%8F%E5%BE%AE%E5%88%86%E6%96%B9%E7%A8%8B&amp;diff=17749"/>
		<updated>2020-11-01T18:31:25Z</updated>

		<summary type="html">&lt;p&gt;Ruili：&lt;/p&gt;
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&lt;div&gt;此词条暂由Yuling翻译，未经人工整理和审校，带来阅读不便，请见谅。&lt;br /&gt;
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[[File:Heat.gif|thumb|right|A visualisation of a solution to the two-dimensional [[heat equation]] with temperature represented by the third dimension]]&lt;br /&gt;
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A visualisation of a solution to the two-dimensional [[heat equation with temperature represented by the third dimension]]&lt;br /&gt;
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二维热传导方程解的可视化，图中第三个维度表示温度的大小。&lt;br /&gt;
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In [[mathematics]], a '''partial differential equation''' ('''PDE''') is a [[differential equation]] that contains unknown [[Multivariable calculus|multivariable functions]] and their [[partial derivative]]s. PDEs are used to formulate problems involving functions of several variables, and are either solved by hand, or used to create a [[computer model]]. A special case is [[ordinary differential equation]]s (ODEs), which deal with functions of a single variable and their derivatives.&lt;br /&gt;
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In mathematics, a partial differential equation (PDE) is a differential equation that contains unknown multivariable functions and their partial derivatives. PDEs are used to formulate problems involving functions of several variables, and are either solved by hand, or used to create a computer model. A special case is ordinary differential equations (ODEs), which deal with functions of a single variable and their derivatives.&lt;br /&gt;
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在数学中，'''&amp;lt;font color = &amp;quot;#ff8000&amp;quot;&amp;gt;偏微分方程函数 Partial Differential Equation&amp;lt;/font&amp;gt;'''是包含未知多元函数及其偏导数的微分方程。偏微分方程用于描述涉及多元函数的问题，可以通过人为求解，也可以通过建立计算机模型来求解。常微分方程是偏微分方程一种特殊情况，它处理的是一元函数及其导数。&lt;br /&gt;
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PDEs can be used to describe a wide variety of phenomena such as sound, heat, [[diffusion]], [[electrostatics]], [[Electromagnetism|electrodynamics]], [[fluid dynamics]], [[Elasticity (physics)|elasticity]], [[gravitation]] and [[quantum mechanics]]. These seemingly distinct physical phenomena can be formalised similarly in terms of PDEs. Just as ordinary differential equations often model one-dimensional [[dynamical system]]s, partial differential equations often model [[multidimensional system]]s. PDEs find their generalisation in [[stochastic partial differential equation]]s.&lt;br /&gt;
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PDEs can be used to describe a wide variety of phenomena such as sound, heat, diffusion, electrostatics, electrodynamics, fluid dynamics, elasticity, gravitation and quantum mechanics. These seemingly distinct physical phenomena can be formalised similarly in terms of PDEs. Just as ordinary differential equations often model one-dimensional dynamical systems, partial differential equations often model multidimensional systems. PDEs find their generalisation in stochastic partial differential equations.&lt;br /&gt;
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偏微分方程可以用来描述各种各样的物理现象，如声音，热量，扩散，静电，电动力学，流体力学，弹性力学，重力和量子力学。这些看起来截然不同的物理现象却可以用类似的偏微分方程来描述。正如常微分方程经常对一维动力系统进行建模一样，偏微分方程经常对多维系统进行建模。随机偏微分方程是偏微分方程的一种推广。&lt;br /&gt;
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== Introduction ==&lt;br /&gt;
引言&lt;br /&gt;
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Partial differential equations (PDEs) are equations that involve rates of change with respect to [[continuous variables]]. For example, the position of a [[rigid body]] is specified by six parameters,&amp;lt;ref&amp;gt;{{Cite book|url=https://books.google.com/books?id=v9PLbcYd9aUC&amp;amp;pg=PA32|title=Modelling and Control of Robot Manipulators|last=Sciavicco|first=Lorenzo|last2=Siciliano|first2=Bruno|date=2001-02-19|publisher=Springer Science &amp;amp; Business Media|isbn=9781852332211|language=en}}&amp;lt;/ref&amp;gt; but the configuration of a [[fluid]] is given by the [[continuous distribution]] of several parameters, such as the [[temperature]], [[pressure]], and so forth. The dynamics for the rigid body take place in a finite-dimensional [[Configuration space (physics)|configuration space]]; the dynamics for the fluid occur in an infinite-dimensional configuration space. This distinction usually makes PDEs much harder to solve than ordinary differential equations (ODEs), but here again, there will be simple solutions for linear problems. Classic domains where PDEs are used include [[acoustics]], [[fluid dynamics]], [[electrodynamics]], and [[heat transfer]].&lt;br /&gt;
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Partial differential equations (PDEs) are equations that involve rates of change with respect to continuous variables. For example, the position of a rigid body is specified by six parameters, but the configuration of a fluid is given by the continuous distribution of several parameters, such as the temperature, pressure, and so forth. The dynamics for the rigid body take place in a finite-dimensional configuration space; the dynamics for the fluid occur in an infinite-dimensional configuration space. This distinction usually makes PDEs much harder to solve than ordinary differential equations (ODEs), but here again, there will be simple solutions for linear problems. Classic domains where PDEs are used include acoustics, fluid dynamics, electrodynamics, and heat transfer.&lt;br /&gt;
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偏微分方程(简称为PDEs)涉及到连续变量的变化率。例如，刚体的位置是由六个参数确定的，而流体的形状是由几个参数的连续分布给出的，如温度、压力等。刚体的动力学过程发生在有限维位形空间中，流体的动力学过程发生在无限维位形空间中。这种区别通常使偏微分方程比常微分方程更难求解，但是线性问题也有简单的解。使用偏微分方程的经典领域包括声学、流体力学、电动力学和传热学。&lt;br /&gt;
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A partial differential equation (PDE) for the function {{math|''u''(''x''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;,… ''x&amp;lt;sub&amp;gt;n&amp;lt;/sub&amp;gt;'')}} is an equation of the form&lt;br /&gt;
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A partial differential equation (PDE) for the function  is an equation of the form&lt;br /&gt;
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对于函数{{math|''u''(''x''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;,… ''x&amp;lt;sub&amp;gt;n&amp;lt;/sub&amp;gt;'')}}，它的的偏微分方程形式是：&lt;br /&gt;
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: &amp;lt;math&amp;gt;f \left (x_1, \ldots x_n; u, \frac{\partial u}{\partial x_1}, \ldots \frac{\partial u}{\partial x_n}; \frac{\partial^2 u}{\partial x_1 \partial x_1}, \ldots \frac{\partial^2 u}{\partial x_1 \partial x_n}; \ldots \right) = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;f \left (x_1, \ldots x_n; u, \frac{\partial u}{\partial x_1}, \ldots \frac{\partial u}{\partial x_n}; \frac{\partial^2 u}{\partial x_1 \partial x_1}, \ldots \frac{\partial^2 u}{\partial x_1 \partial x_n}; \ldots \right) = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
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If {{mvar|f}} is a [[linear function]] of {{mvar|u}} and its derivatives, then the PDE is called linear. Common examples of linear PDEs include the [[heat equation]], the [[wave equation]], [[Laplace's equation]], [[Helmholtz equation]], [[Klein–Gordon equation]], and [[Poisson's equation]].&lt;br /&gt;
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If  is a linear function of  and its derivatives, then the PDE is called linear. Common examples of linear PDEs include the heat equation, the wave equation, Laplace's equation, Helmholtz equation, Klein–Gordon equation, and Poisson's equation.&lt;br /&gt;
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如果{{mvar|f}}是函数及其导数的线性方程，则偏微分方程称为线性函数。线性偏微分方程的常见例子包括热方程、波动方程、拉普拉斯方程、亥姆霍兹方程方程、克莱因-高登方程和泊松方程。&lt;br /&gt;
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A relatively simple PDE is&lt;br /&gt;
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A relatively simple PDE is&lt;br /&gt;
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一个相对简单的偏微分方程是：&lt;br /&gt;
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: &amp;lt;math&amp;gt;\frac{\partial u}{\partial x}(x,y) = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;\frac{\partial u}{\partial x}(x,y) = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
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This relation [[Logical implication|implies]] that the function {{math|''u''(''x'',''y'')}} is independent of {{mvar|x}}. However, the equation gives no information on the function's dependence on the variable {{mvar|y}}. Hence the general solution of this equation is&lt;br /&gt;
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This relation implies that the function  is independent of . However, the equation gives no information on the function's dependence on the variable . Hence the general solution of this equation is&lt;br /&gt;
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这个关系意味着函数是独立于{{mvar|x}}的。然而，这个方程没有给出关于函数和自变量的相关性的信息。因此，这个方程的通解是&lt;br /&gt;
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: &amp;lt;math&amp;gt;u(x,y) = f(y),&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;u(x,y) = f(y),&amp;lt;/math&amp;gt;&lt;br /&gt;
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where {{mvar|f}} is an arbitrary function of {{mvar|y}}. The analogous ordinary differential equation is&lt;br /&gt;
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where  is an arbitrary function of . The analogous ordinary differential equation is&lt;br /&gt;
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其中{{mvar|f}}是{{mvar|y}}的任意函数。类似的常微分方程是&lt;br /&gt;
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: &amp;lt;math&amp;gt;\frac{\mathrm{d} u}{\mathrm{d} x}(x) = 0,&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;\frac{\mathrm{d} u}{\mathrm{d} x}(x) = 0,&amp;lt;/math&amp;gt;&lt;br /&gt;
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which has the solution&lt;br /&gt;
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which has the solution&lt;br /&gt;
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它的解为&lt;br /&gt;
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: &amp;lt;math&amp;gt;u(x) = c,&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;u(x) = c,&amp;lt;/math&amp;gt;&lt;br /&gt;
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where {{mvar|c}} is any [[Constant (mathematics)|constant]] value. These two examples illustrate that general solutions of ordinary differential equations (ODEs) involve arbitrary constants, but solutions of PDEs involve arbitrary functions.&lt;br /&gt;
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where  is any constant value. These two examples illustrate that general solutions of ordinary differential equations (ODEs) involve arbitrary constants, but solutions of PDEs involve arbitrary functions.&lt;br /&gt;
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这里的{{mvar|c}}是常量。这两个例子说明常微分方程的一般解包含任意常数，但偏微分方程的解包含任意函数。&lt;br /&gt;
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A solution of a PDE is generally not [[Uniqueness quantification|unique]]; additional conditions must generally be specified on the [[Boundary (topology)|boundary]] of the region where the solution is defined. For instance, in the simple example above, the function {{math|''f''(''y'')}} can be determined if {{mvar|u}} is specified on the line {{math|''x'' {{=}} 0}}.&lt;br /&gt;
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A solution of a PDE is generally not unique; additional conditions must generally be specified on the boundary of the region where the solution is defined. For instance, in the simple example above, the function  can be determined if  is specified on the line  0}}.&lt;br /&gt;
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偏微分方程的解一般不是唯一的; 附加条件一般必须在定义解的区域边界上定义。例如，在上面的简单示例中，如果在{{math|''x'' {{=}} 0}}时确定了{{mvar|u}}的值，则可以确定该函数{{math|''f''(''y'')}}。&lt;br /&gt;
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== Existence and uniqueness ==&lt;br /&gt;
存在性和唯一性&lt;br /&gt;
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Although the issue of existence and uniqueness of solutions of ordinary differential equations has a very satisfactory answer with the [[Picard–Lindelöf theorem]], that is far from the case for partial differential equations. The [[Cauchy–Kowalevski theorem]] states that the [[Cauchy problem]] for any partial differential equation whose coefficients are [[Analytic function|analytic]] in the unknown function and its derivatives, has a locally unique analytic solution. Although this result might appear to settle the existence and uniqueness of solutions, there are examples of linear partial differential equations whose coefficients have derivatives of all orders (which are nevertheless not analytic) but which have no solutions at all: see [[Lewy's example|Lewy (1957)]]. Even if the solution of a partial differential equation exists and is unique, it may nevertheless have undesirable properties.  The mathematical study of these questions is usually in the more powerful context of [[weak solution]]s.&lt;br /&gt;
&lt;br /&gt;
Although the issue of existence and uniqueness of solutions of ordinary differential equations has a very satisfactory answer with the Picard–Lindelöf theorem, that is far from the case for partial differential equations. The Cauchy–Kowalevski theorem states that the Cauchy problem for any partial differential equation whose coefficients are analytic in the unknown function and its derivatives, has a locally unique analytic solution. Although this result might appear to settle the existence and uniqueness of solutions, there are examples of linear partial differential equations whose coefficients have derivatives of all orders (which are nevertheless not analytic) but which have no solutions at all: see Lewy (1957). Even if the solution of a partial differential equation exists and is unique, it may nevertheless have undesirable properties.  The mathematical study of these questions is usually in the more powerful context of weak solutions.&lt;br /&gt;
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虽然常微分方程解的存在唯一性问题用'''&amp;lt;font color=&amp;quot;#ff8000&amp;quot;&amp;gt;弗罗贝尼乌斯定理 Picard–Lindelöf Theorem&amp;lt;/font&amp;gt;得到了令人满意的结果，但应用到偏微分方程上却不尽如意。'''&amp;lt;font color=&amp;quot;#ff8000&amp;quot;&amp;gt;柯西-科瓦列夫斯基定理 Cauchy–Kowalevski theorem&amp;lt;/font&amp;gt;指出，对于任何在未知函数及其导数中系数是解析的偏微分方程，柯西问题有一个局部唯一的解析解。虽然这个结果似乎解决了解的存在性和唯一性问题，但是有一些线性偏微分方程的系数具有所有级数的导数(尽管这些导数不是解析的) ，但是根本没有解: 见 Lewy (1957)。即使偏微分方程的解存在且唯一，它仍然可能具有人们所不希望的性质。这些问题的数学研究通常是在更有力的弱解的背景下进行的。&lt;br /&gt;
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An example of pathological behavior is the sequence (depending upon {{mvar|n}}) of [[Cauchy problem]]s for the [[Laplace equation]]&lt;br /&gt;
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An example of pathological behavior is the sequence (depending upon ) of Cauchy problems for the Laplace equation&lt;br /&gt;
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反常特征的一个例子是拉普拉斯方程的柯西问题的序列(取决于{{mvar|n}})&lt;br /&gt;
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: &amp;lt;math&amp;gt;\frac{\partial^2 u}{\partial x^2} + \frac{\partial^2 u}{\partial y^2}=0,&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;\frac{\partial^2 u}{\partial x^2} + \frac{\partial^2 u}{\partial y^2}=0,&amp;lt;/math&amp;gt;&lt;br /&gt;
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with [[boundary condition]]s&lt;br /&gt;
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with boundary conditions&lt;br /&gt;
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有边界条件&lt;br /&gt;
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: &amp;lt;math&amp;gt;\begin{align} u(x,0) &amp;amp;= 0, \\ \frac{\partial u}{\partial y}(x,0) &amp;amp;= \frac{\sin nx}{n}, \end{align}&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;\begin{align} u(x,0) &amp;amp;= 0, \\ \frac{\partial u}{\partial y}(x,0) &amp;amp;= \frac{\sin nx}{n}, \end{align}&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
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where {{mvar|n}} is an integer. The derivative of {{mvar|u}} with respect to {{mvar|y}} approaches zero [[uniform convergence|uniformly]] in {{mvar|x}} as {{mvar|n}} increases, but the solution is&lt;br /&gt;
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where  is an integer. The derivative of  with respect to  approaches zero uniformly in  as  increases, but the solution is&lt;br /&gt;
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其中{{mvar|n}}是整数。{{mvar|u}}是关于{{mvar|y}}的导数，一致地随着{{mvar|n}}的增加而趋于零，但是解是&lt;br /&gt;
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: &amp;lt;math&amp;gt;u(x,y) = \frac{\sinh ny \sin nx}{n^2}.&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;u(x,y) = \frac{\sinh ny \sin nx}{n^2}.&amp;lt;/math&amp;gt;&lt;br /&gt;
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This solution approaches infinity if {{mvar|nx}} is not an integer multiple of {{pi}} for any non-zero value of {{mvar|y}}. The Cauchy problem for the Laplace equation is called ''ill-posed'' or ''not [[Well-posed problem|well-posed]]'', since the solution does not continuously depend on the data of the problem. Such ill-posed problems are not usually satisfactory for physical applications.&lt;br /&gt;
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This solution approaches infinity if  is not an integer multiple of  for any non-zero value of . The Cauchy problem for the Laplace equation is called ill-posed or not well-posed, since the solution does not continuously depend on the data of the problem. Such ill-posed problems are not usually satisfactory for physical applications.&lt;br /&gt;
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对于任何非零的{{mvar|y}}，如果{{mvar|nx}}不是{{pi}}的整数倍，这个解会接近于无穷大。拉普拉斯方程的柯西问题被称为不适定问题（可以译为ill-posed或not well-posed），因为该问题的解并不连续地依赖于该问题的数据。这种不适定问题在物理应用中通常不能令人满意。&lt;br /&gt;
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The [[Navier–Stokes existence and smoothness|existence of solutions for the Navier–Stokes equations]], a partial differential equation, is part of one of the [[Millennium Prize Problems]].&lt;br /&gt;
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The existence of solutions for the Navier–Stokes equations, a partial differential equation, is part of one of the Millennium Prize Problems.&lt;br /&gt;
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一种偏微分方程——纳维-斯托克斯方程——的解的存在性就是千禧年大奖难题的一部分。&lt;br /&gt;
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== Notation ==&lt;br /&gt;
符号&lt;br /&gt;
&lt;br /&gt;
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In PDEs, it is common to denote partial derivatives using subscripts. That is:&lt;br /&gt;
&lt;br /&gt;
In PDEs, it is common to denote partial derivatives using subscripts. That is:&lt;br /&gt;
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在偏微分方程中，通常用下标表示偏导数。例如:&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt;u_x = \frac{\partial u}{\partial x}&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;u_x = \frac{\partial u}{\partial x}&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt;u_{xx} = \frac{\partial^2 u}{\partial x^2} &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;u_{xx} = \frac{\partial^2 u}{\partial x^2} &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
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: &amp;lt;math&amp;gt;u_{xy} = \frac{\partial^2 u}{\partial y\, \partial x} = \frac{\partial}{\partial y } \left(\frac{\partial u}{\partial x}\right). &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;u_{xy} = \frac{\partial^2 u}{\partial y\, \partial x} = \frac{\partial}{\partial y } \left(\frac{\partial u}{\partial x}\right). &amp;lt;/math&amp;gt;&lt;br /&gt;
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Especially in physics, [[del]] or nabla ({{math|∇}}) is often used to denote spatial derivatives, and {{math|''&amp;amp;#x307;u'', ''ü''}} for time derivatives. For example, the [[wave equation]] (mentioned below) can be written as&lt;br /&gt;
&lt;br /&gt;
Especially in physics, del or nabla () is often used to denote spatial derivatives, and  for time derivatives. For example, the wave equation (mentioned below) can be written as&lt;br /&gt;
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特别是在物理学中，[[del]]或nabla ({{math|∇}})经常用来表示空间导数和时间导数。例如，波动方程(在下文中提到)可以写成&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
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:&amp;lt;math&amp;gt;\ddot u=c^2\nabla^2u&amp;lt;/math&amp;gt;&lt;br /&gt;
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&amp;lt;math&amp;gt;\ddot u=c^2\nabla^2u&amp;lt;/math&amp;gt;&lt;br /&gt;
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or&lt;br /&gt;
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or&lt;br /&gt;
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或&lt;br /&gt;
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:&amp;lt;math&amp;gt;\ddot u=c^2\Delta u&amp;lt;/math&amp;gt;&lt;br /&gt;
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&amp;lt;math&amp;gt;\ddot u=c^2\Delta u&amp;lt;/math&amp;gt;&lt;br /&gt;
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where {{math|Δ}} is the [[Laplace operator]].&lt;br /&gt;
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where  is the Laplace operator.&lt;br /&gt;
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其中{{math|Δ}}代表拉普拉斯算子&lt;br /&gt;
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== Classification ==&lt;br /&gt;
分类&lt;br /&gt;
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Some linear, second-order partial differential equations can be classified as [[parabolic partial differential equation|parabolic]], [[hyperbolic partial differential equation|hyperbolic]] and [[elliptic partial differential equation|elliptic]]. Others, such as the [[Euler–Tricomi equation]], have different types in different regions. The classification provides a guide to appropriate initial and boundary conditions and to the smoothness of the solutions.&lt;br /&gt;
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Some linear, second-order partial differential equations can be classified as parabolic, hyperbolic and elliptic. Others, such as the Euler–Tricomi equation, have different types in different regions. The classification provides a guide to appropriate initial and boundary conditions and to the smoothness of the solutions.&lt;br /&gt;
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一些线性二阶偏微分方程可分为抛物型方程、双曲型方程和椭圆型方程。其他的方程，如欧拉-特里科米方程，在不同的区域有不同的类型。这种分类有助于选择适当的初始和边界条件以及提高解的平滑性。&lt;br /&gt;
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=== Equations of first order ===&lt;br /&gt;
一阶方程&lt;br /&gt;
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{{main|First-order partial differential equation}}&lt;br /&gt;
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=== Linear equations of second order ===&lt;br /&gt;
二阶线性方程&lt;br /&gt;
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Assuming {{math|''u&amp;lt;sub&amp;gt;xy&amp;lt;/sub&amp;gt;'' {{=}} ''u&amp;lt;sub&amp;gt;yx&amp;lt;/sub&amp;gt;''}}, the general linear second-order PDE in two independent variables has the form&lt;br /&gt;
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Assuming  u&amp;lt;sub&amp;gt;yx&amp;lt;/sub&amp;gt;}}, the general linear second-order PDE in two independent variables has the form&lt;br /&gt;
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假设 {{math|''u&amp;lt;sub&amp;gt;xy&amp;lt;/sub&amp;gt;'' {{=}} ''u&amp;lt;sub&amp;gt;yx&amp;lt;/sub&amp;gt;''}}，含有两个独立变量的一般的线性二阶偏微分方程具有如下这样的形式&lt;br /&gt;
&lt;br /&gt;
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: &amp;lt;math&amp;gt;Au_{xx} + 2Bu_{xy} + Cu_{yy} + \cdots \mbox{(lower order terms)} = 0,&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;Au_{xx} + 2Bu_{xy} + Cu_{yy} + \cdots \mbox{(lower order terms)} = 0,&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
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where the coefficients {{mvar|A}}, {{mvar|B}}, {{mvar|C}}... may depend upon {{mvar|x}} and {{mvar|y}}. If {{math|''A''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; + ''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; + ''C''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; &amp;gt; 0}} over a region of the {{mvar|xy}}-plane, the PDE is second-order in that region. This form is analogous to the equation for a conic section:&lt;br /&gt;
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where the coefficients , , ... may depend upon  and . If  over a region of the -plane, the PDE is second-order in that region. This form is analogous to the equation for a conic section:&lt;br /&gt;
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其中的系数 {{mvar|A}}, {{mvar|B}}, {{mvar|C}}... 一般取决于{{mvar|x}}和{{mvar|y}}。如果在{{mvar|xy}}-平面的一个区域上 {{math|''A''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; + ''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; + ''C''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; &amp;gt; 0}}，偏微分方程在该区域是二阶的。这种形式类似于圆锥曲线的方程:&lt;br /&gt;
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: &amp;lt;math&amp;gt;Ax^2 + 2Bxy + Cy^2 + \cdots = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;Ax^2 + 2Bxy + Cy^2 + \cdots = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
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More precisely, replacing {{math|∂&amp;lt;sub&amp;gt;''x''&amp;lt;/sub&amp;gt;}} by {{mvar|X}}, and likewise for other variables (formally this is done by a [[Fourier transform]]), converts a constant-coefficient PDE into a polynomial of the same degree, with the terms of the highest degree (a [[homogeneous polynomial]], here a [[quadratic form]]) being most significant for the classification.&lt;br /&gt;
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More precisely, replacing  by , and likewise for other variables (formally this is done by a Fourier transform), converts a constant-coefficient PDE into a polynomial of the same degree, with the terms of the highest degree (a homogeneous polynomial, here a quadratic form) being most significant for the classification.&lt;br /&gt;
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更准确地说，用 {{mvar|X}} 替换 {{math|∂&amp;lt;sub&amp;gt;''x''&amp;lt;/sub&amp;gt;}}，对于其他变量做同样的操作(从形式上来说，这是由傅里叶变换来完成的)，将一个常系数偏微分方程转换成一个相同次数的多项式，最高次数的项(齐次多项式，这里是一个二次形式)一般会用于偏微分方程的分类。&lt;br /&gt;
===~~ most significant for the classification 意译为用于偏微分方程的分类。       significiant直译过来感觉不太合适&lt;br /&gt;
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Just as one classifies [[conic section]]s and quadratic forms into parabolic, hyperbolic, and elliptic based on the [[discriminant]] {{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − 4''AC''}}, the same can be done for a second-order PDE at a given point.  However, the [[discriminant]] in a PDE is given by {{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC''}} due to the convention of the {{mvar|xy}} term being {{math|2''B''}} rather than {{mvar|B}}; formally, the discriminant (of the associated quadratic form) is {{math|(2''B'')&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − 4''AC'' {{=}} 4(''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC'')}}, with the factor of 4 dropped for simplicity.&lt;br /&gt;
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Just as one classifies conic sections and quadratic forms into parabolic, hyperbolic, and elliptic based on the discriminant , the same can be done for a second-order PDE at a given point.  However, the discriminant in a PDE is given by  due to the convention of the  term being  rather than ; formally, the discriminant (of the associated quadratic form) is  4(B&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − AC)}}, with the factor of 4 dropped for simplicity.&lt;br /&gt;
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正如人们可以根据判别式 {{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − 4''AC''}} 将圆锥曲线和二次型分为抛物型、双曲型和椭圆型一样，对于给定点的二阶偏微分方程也可以这样做。然而，偏微分方程中的判别式 {{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − 4''AC''}} 是根据交叉项的系数{{math|2''B''}} 而不是 {{mvar|B}} 给出的，形式上，判别式(关联二次型)是 {{math|(2''B'')&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − 4''AC'' {{=}} 4(''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC'')}}，为简单起见，去掉了因子4。&lt;br /&gt;
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# {{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC'' &amp;lt; 0}} (''[[elliptic partial differential equation]]''): Solutions of [[elliptic partial differential equation|elliptic PDEs]] are as smooth as the coefficients allow, within the interior of the region where the equation and solutions are defined. For example, solutions of [[Laplace's equation]] are analytic within the domain where they are defined, but solutions may assume boundary values that are not smooth. The motion of a fluid at subsonic speeds can be approximated with elliptic PDEs, and the Euler–Tricomi equation is elliptic where {{math|''x'' &amp;lt; 0}}.&lt;br /&gt;
&lt;br /&gt;
  (elliptic partial differential equation): Solutions of elliptic PDEs are as smooth as the coefficients allow, within the interior of the region where the equation and solutions are defined. For example, solutions of Laplace's equation are analytic within the domain where they are defined, but solutions may assume boundary values that are not smooth. The motion of a fluid at subsonic speeds can be approximated with elliptic PDEs, and the Euler–Tricomi equation is elliptic where .&lt;br /&gt;
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{{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC'' &amp;lt; 0}} (椭圆形微分方程)：在定义方程和解的区域内部，椭圆型偏微分方程的解光滑到系数允许的程度。例如，拉普拉斯方程的解在它们被定义的区域内是解析的，但是解可能假设边界值是不光滑的。亚音速流体的运动可以用椭圆偏微分方程近似，其中欧拉-特里科米方程在 {{math|''x'' &amp;lt; 0}} 时是椭圆型偏微分方程。&lt;br /&gt;
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# {{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC'' {{=}} 0}} (''[[parabolic partial differential equation]]''): Equations that are [[parabolic partial differential equation|parabolic]] at every point can be transformed into a form analogous to the [[heat equation]] by a change of independent variables. Solutions smooth out as the transformed time variable increases. The Euler–Tricomi equation has parabolic type on the line where {{math|''x'' {{=}} 0}}.&lt;br /&gt;
&lt;br /&gt;
  0}} (parabolic partial differential equation): Equations that are parabolic at every point can be transformed into a form analogous to the heat equation by a change of independent variables. Solutions smooth out as the transformed time variable increases. The Euler–Tricomi equation has parabolic type on the line where  0}}.&lt;br /&gt;
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{{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC'' {{=}} 0}}（抛物线形偏微分方程）：在每一点上都是抛物线型的方程可以通过改变自变量从而转化成类似于热方程的形式。随着转换后的时间变量的增加，方程的解变得平滑。欧拉-特里科米方程在 {{math|''x'' {{=}} 0}} 这条特征线上是抛物线形的。&lt;br /&gt;
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# {{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC'' &amp;gt; 0}} (''[[hyperbolic partial differential equation]]''): [[hyperbolic partial differential equation|hyperbolic]] equations retain any discontinuities of functions or derivatives in the initial data. An example is the [[wave equation]]. The motion of a fluid at supersonic speeds can be approximated with hyperbolic PDEs, and the Euler–Tricomi equation is hyperbolic where {{math|''x'' &amp;gt; 0}}.&lt;br /&gt;
&lt;br /&gt;
  (hyperbolic partial differential equation): hyperbolic equations retain any discontinuities of functions or derivatives in the initial data. An example is the wave equation. The motion of a fluid at supersonic speeds can be approximated with hyperbolic PDEs, and the Euler–Tricomi equation is hyperbolic where .&lt;br /&gt;
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{{math|''B''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; − ''AC'' &amp;gt; 0}} (双曲形偏微分方程)：双曲形方程在初始数据中保留了函数或导数的任何不连续性，波动方程就是其中的一个例子。超音速流体的运动可以用双曲形偏微分方程近似，其中欧拉-特里科米方程在 {{math|''x'' &amp;gt; 0}} 时是双曲型的。&lt;br /&gt;
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&lt;br /&gt;
&lt;br /&gt;
If there are {{mvar|n}} independent variables {{math|''x''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;, ''x''&amp;lt;sub&amp;gt;2 &amp;lt;/sub&amp;gt;,… ''x''&amp;lt;sub&amp;gt;''n''&amp;lt;/sub&amp;gt;}}, a general linear partial differential equation of second order has the form&lt;br /&gt;
&lt;br /&gt;
If there are  independent variables , a general linear partial differential equation of second order has the form&lt;br /&gt;
&lt;br /&gt;
如果存在 {{mvar|n}} 个自变量 {{math|''x''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;, ''x''&amp;lt;sub&amp;gt;2 &amp;lt;/sub&amp;gt;,… ''x''&amp;lt;sub&amp;gt;''n''&amp;lt;/sub&amp;gt;}}，一般二阶线性偏微分方程的形式是&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt;L u =\sum_{i=1}^n\sum_{j=1}^n a_{i,j} \frac{\partial^2 u}{\partial x_i \partial x_j} \quad \text{ plus lower-order terms} =0.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;L u =\sum_{i=1}^n\sum_{j=1}^n a_{i,j} \frac{\partial^2 u}{\partial x_i \partial x_j} \quad \text{ plus lower-order terms} =0.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The classification depends upon the signature of the eigenvalues of the coefficient matrix {{math|''a''&amp;lt;sub&amp;gt;''i'',''j''&amp;lt;/sub&amp;gt;}}.&lt;br /&gt;
&lt;br /&gt;
The classification depends upon the signature of the eigenvalues of the coefficient matrix .&lt;br /&gt;
&lt;br /&gt;
这种分类取决于系数矩阵本征值的符号（正负性）。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
# Elliptic: the eigenvalues are all positive or all negative.&lt;br /&gt;
&lt;br /&gt;
 Elliptic: the eigenvalues are all positive or all negative.&lt;br /&gt;
&lt;br /&gt;
椭圆形方程: 本征值全部为正或全部为负。&lt;br /&gt;
&lt;br /&gt;
# Parabolic: the eigenvalues are all positive or all negative, save one that is zero.&lt;br /&gt;
&lt;br /&gt;
 Parabolic: the eigenvalues are all positive or all negative, save one that is zero.&lt;br /&gt;
&lt;br /&gt;
抛物线形方程: 本征值全部为正或全部为负，除了一个为零。&lt;br /&gt;
&lt;br /&gt;
# Hyperbolic: there is only one negative eigenvalue and all the rest are positive, or there is only one positive eigenvalue and all the rest are negative.&lt;br /&gt;
&lt;br /&gt;
 Hyperbolic: there is only one negative eigenvalue and all the rest are positive, or there is only one positive eigenvalue and all the rest are negative.&lt;br /&gt;
&lt;br /&gt;
双曲形方程: 只有一个负特征值，其余的都是正特征值，或者只有一个正特征值，其余的都是负特征值。&lt;br /&gt;
&lt;br /&gt;
# Ultrahyperbolic: there is more than one positive eigenvalue and more than one negative eigenvalue, and there are no zero eigenvalues. There is only a limited theory for ultrahyperbolic equations (Courant and Hilbert, 1962).&lt;br /&gt;
&lt;br /&gt;
 Ultrahyperbolic: there is more than one positive eigenvalue and more than one negative eigenvalue, and there are no zero eigenvalues. There is only a limited theory for ultrahyperbolic equations (Courant and Hilbert, 1962).&lt;br /&gt;
&lt;br /&gt;
超双形方程: 存在多于一个正本征值和多于一个的负本征值，且不存在零本征值。对于超双曲方程，只存在一个有限理论(Courant 和 Hilbert，1962)。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==[[用户:Yuling|Yuling]]（[[用户讨论:Yuling|讨论]]） 我对于limited theory这个单词对应的相关理论不太了解。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
=== Systems of first-order equations and characteristic surfaces ===&lt;br /&gt;
一阶方程组和特征曲面&lt;br /&gt;
&lt;br /&gt;
The classification of partial differential equations can be extended to systems of first-order equations, where the unknown {{mvar|u}} is now a [[Euclidean vector|vector]] with {{mvar|m}} components, and the coefficient matrices {{mvar|A&amp;lt;sub&amp;gt;ν&amp;lt;/sub&amp;gt;}} are {{mvar|m}} by {{mvar|m}} matrices for {{math|''ν'' {{=}} 1, 2,… ''n''}}. The partial differential equation takes the form&lt;br /&gt;
&lt;br /&gt;
The classification of partial differential equations can be extended to systems of first-order equations, where the unknown  is now a vector with  components, and the coefficient matrices  are  by  matrices for  1, 2,… n}}. The partial differential equation takes the form&lt;br /&gt;
&lt;br /&gt;
偏微分方程组的分类可以推广到一阶方程组，其中未知量 {{mvar|u}} 是有 {{mvar|m}} 个分量的向量。对于 {{math|''ν'' {{=}} 1, 2,… ''n''}}，系数矩阵 {{mvar|A&amp;lt;sub&amp;gt;ν&amp;lt;/sub&amp;gt;}} 是 {{mvar|m}} × {{mvar|m}} 的矩阵。偏微分方程形式如下：&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt;Lu = \sum_{\nu=1}^{n} A_\nu \frac{\partial u}{\partial x_\nu} + B=0,&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;Lu = \sum_{\nu=1}^{n} A_\nu \frac{\partial u}{\partial x_\nu} + B=0,&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
where the coefficient matrices {{mvar|A&amp;lt;sub&amp;gt;ν&amp;lt;/sub&amp;gt;}} and the vector {{mvar|B}} may depend upon {{mvar|x}} and {{mvar|u}}. If a [[hypersurface]] {{mvar|S}} is given in the implicit form&lt;br /&gt;
&lt;br /&gt;
where the coefficient matrices  and the vector  may depend upon  and . If a hypersurface  is given in the implicit form&lt;br /&gt;
&lt;br /&gt;
其中系数矩阵 {{mvar|A&amp;lt;sub&amp;gt;ν&amp;lt;/sub&amp;gt;}} 和向量 {{mvar|B}} 可能依赖于 {{mvar|x}} 和 {{mvar|u}}。如果超曲面是以隐式形式给出的&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt;\varphi(x_1, x_2, \ldots x_n)=0,&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;\varphi(x_1, x_2, \ldots x_n)=0,&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
where {{mvar|φ}} has a non-zero gradient, then {{mvar|S}} is a '''characteristic surface''' for the operator {{mvar|L}} at a given point if the characteristic form vanishes:&lt;br /&gt;
&lt;br /&gt;
where  has a non-zero gradient, then  is a characteristic surface for the operator  at a given point if the characteristic form vanishes:&lt;br /&gt;
&lt;br /&gt;
其中存在一个非零的梯度，那么如果特征形式消失，则在给定点上算子的特征曲面形式如下:&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt;Q\left(\frac{\partial\varphi}{\partial x_1}, \ldots\frac{\partial\varphi}{\partial x_n}\right) =\det\left[\sum_{\nu=1}^nA_\nu \frac{\partial \varphi}{\partial x_\nu}\right]=0.\,&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;Q\left(\frac{\partial\varphi}{\partial x_1}, \ldots\frac{\partial\varphi}{\partial x_n}\right) =\det\left[\sum_{\nu=1}^nA_\nu \frac{\partial \varphi}{\partial x_\nu}\right]=0.\,&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The geometric interpretation of this condition is as follows: if data for {{mvar|u}} are prescribed on the surface {{mvar|S}}, then it may be possible to determine the normal derivative of {{mvar|u}} on {{mvar|S}} from the differential equation. If the data on {{mvar|S}} and the differential equation determine the normal derivative of {{mvar|u}} on {{mvar|S}}, then {{mvar|S}} is non-characteristic. If the data on {{mvar|S}} and the differential equation ''do not'' determine the normal derivative of {{mvar|u}} on {{mvar|S}}, then the surface is '''characteristic''', and the differential equation restricts the data on {{mvar|S}}: the differential equation is ''internal'' to {{mvar|S}}.&lt;br /&gt;
&lt;br /&gt;
The geometric interpretation of this condition is as follows: if data for  are prescribed on the surface , then it may be possible to determine the normal derivative of  on  from the differential equation. If the data on  and the differential equation determine the normal derivative of  on , then  is non-characteristic. If the data on  and the differential equation do not determine the normal derivative of  on , then the surface is characteristic, and the differential equation restricts the data on : the differential equation is internal to .&lt;br /&gt;
&lt;br /&gt;
这个条件的几何解释如下: 如果关于 {{mvar|u}} 的数据是在曲面 {{mvar|S}} 上规定的，那么就有可能依据微分方程确定曲面 {{mvar|S}} 上 {{mvar|u}} 的法向导数。如果曲面 {{mvar|S}} 上的数据和上面的微分方程能确定曲面 {{mvar|S}} 上 {{mvar|u}} 的法向导数，那么它就是非特征的。如果曲面 {{mvar|S}} 上的数据和上面的微分方程不能确定曲面 {{mvar|S}} 上 {{mvar|u}} 的法向导数，那么曲面是特征的，并且微分方程将数据限制在曲面 {{mvar|S}} 上：微分方程是在曲面 {{mvar|S}} 内部。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
# A first-order system {{math|''Lu'' {{=}} 0}} is ''elliptic'' if no surface is characteristic for {{mvar|L}}: the values of {{mvar|u}} on {{mvar|S}} and the differential equation always determine the normal derivative of {{mvar|u}} on {{mvar|S}}.&lt;br /&gt;
&lt;br /&gt;
 A first-order system  0}} is elliptic if no surface is characteristic for : the values of  on  and the differential equation always determine the normal derivative of  on .&lt;br /&gt;
&lt;br /&gt;
如果对于 {{mvar|L}} 没有曲面是特征的，则一阶系统 {{math|''Lu'' {{=}} 0}} 是椭圆形的：{{mvar|u}}在 {{mvar|S}} 的值和微分方程总能够决定 {{mvar|S}} 上 {{mvar|u}} 的法向导数。&lt;br /&gt;
&lt;br /&gt;
# A first-order system is ''hyperbolic'' at a point if there is a '''spacelike''' surface {{mvar|S}} with normal {{mvar|ξ}} at that point. This means that, given any non-trivial vector {{mvar|η}} orthogonal to {{mvar|ξ}}, and a scalar multiplier {{mvar|λ}}, the equation {{math|''Q''(''λξ'' + ''η'') {{=}} 0}} has {{mvar|m}} real roots {{math|''λ''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;, ''λ''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;,… ''λ''&amp;lt;sub&amp;gt;''m''&amp;lt;/sub&amp;gt;}}. The system is '''strictly hyperbolic''' if these roots are always distinct. The geometrical interpretation of this condition is as follows: the characteristic form {{math|''Q''(''ζ'') {{=}} 0}} defines a cone (the normal cone) with homogeneous coordinates ζ. In the hyperbolic case, this cone has {{mvar|m}} sheets, and the axis {{math|''ζ'' {{=}} ''λξ''}} runs inside these sheets: it does not intersect any of them. But when displaced from the origin by η, this axis intersects every sheet. In the elliptic case, the normal cone has no real sheets.&lt;br /&gt;
&lt;br /&gt;
 A first-order system is hyperbolic at a point if there is a spacelike surface  with normal  at that point. This means that, given any non-trivial vector  orthogonal to , and a scalar multiplier , the equation  0}} has  real roots . The system is strictly hyperbolic if these roots are always distinct. The geometrical interpretation of this condition is as follows: the characteristic form  0}} defines a cone (the normal cone) with homogeneous coordinates ζ. In the hyperbolic case, this cone has  sheets, and the axis  λξ}} runs inside these sheets: it does not intersect any of them. But when displaced from the origin by η, this axis intersects every sheet. In the elliptic case, the normal cone has no real sheets.&lt;br /&gt;
&lt;br /&gt;
如果在该点存在一个法向量为 {{mvar|ξ}}的 '''&amp;lt;font color=&amp;quot;#ff8000&amp;quot;&amp;gt;类空曲面 Spacclike Surface&amp;lt;/font&amp;gt; {{mvar|S}} ，则一阶系统在那一点是双曲的。这意味着，给定任意正交于 {{mvar|ξ}} 的非平凡向量 {{mvar|η}} 和一个标量乘子 {{mvar|λ}}，方程 {{math|''Q''(''λξ'' + ''η'') {{=}} 0}} 有 {{mvar|m}} 个实根 {{math|''λ''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;, ''λ''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;,… ''λ''&amp;lt;sub&amp;gt;''m''&amp;lt;/sub&amp;gt;}}。如果这些根始终不同，则该系统是严格双曲形的。这个条件的几何解释如下: 特征形式 {{math|''Q''(''ζ'') {{=}} 0}} 定义了一个具有齐次坐标 ζ的圆锥(法线圆锥)。在双曲形的情况下，这个圆锥体有 {{mvar|m}} 层，并且轴 {{math|''ζ'' {{=}} ''λξ''}} 在这些层中运动: 它不与任何一层相交。但是当从原点偏离η时，这条轴线与每一层都相交。在椭圆形的情况下，法向圆锥没有实层。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==[[用户:Yuling|Yuling]]（[[用户讨论:Yuling|讨论]]） sheet 这个单词也不很理解，我直译为了“层”&lt;br /&gt;
&lt;br /&gt;
=== Equations of mixed type ===&lt;br /&gt;
混合型方程&lt;br /&gt;
&lt;br /&gt;
If a PDE has coefficients that are not constant, it is possible that it will not belong to any of these categories but rather be of '''mixed type'''. A simple but important example is the [[Euler–Tricomi equation]]&lt;br /&gt;
&lt;br /&gt;
If a PDE has coefficients that are not constant, it is possible that it will not belong to any of these categories but rather be of mixed type. A simple but important example is the Euler–Tricomi equation&lt;br /&gt;
&lt;br /&gt;
如果偏微分方程的系数不是常数，那么它可能不属于这些类别中的任何一个，而是属于混合类型。一个简单但重要的例子是欧拉-特里科米方程&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt;u_{xx} = xu_{yy},&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;u_{xx} = xu_{yy},&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
which is called '''elliptic-hyperbolic''' because it is elliptic in the region {{math|''x'' &amp;lt; 0}}, hyperbolic in the region {{math|''x'' &amp;gt; 0}}, and degenerate parabolic on the line {{math|''x'' {{=}} 0}}.&lt;br /&gt;
&lt;br /&gt;
which is called elliptic-hyperbolic because it is elliptic in the region , hyperbolic in the region , and degenerate parabolic on the line  0}}.&lt;br /&gt;
&lt;br /&gt;
它在 {{math|''x'' &amp;lt; 0}} 的区域上是椭圆形，在 {{math|''x'' &amp;gt; 0}} 区域上是双曲形，在 {{math|''x'' {{=}} 0}}这条线上是退化为抛物线形，因此称之为椭圆-双曲型。&lt;br /&gt;
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&amp;lt;!--&lt;br /&gt;
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&amp;lt;!--&lt;br /&gt;
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&amp;lt;!--&lt;br /&gt;
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''fill in: Dirichlet and Neumann boundaries, hyperbolic/parabolic/elliptic separation of variables, [[Fourier analysis]], [[Green's function]]s ...--&amp;gt;&lt;br /&gt;
&lt;br /&gt;
fill in: Dirichlet and Neumann boundaries, hyperbolic/parabolic/elliptic separation of variables, Fourier analysis, Green's functions ...--&amp;gt;&lt;br /&gt;
&lt;br /&gt;
填写: Dirichlet 和 Neumann 边界，双曲 / 抛物线 / 椭圆分离变量法，傅立叶分析，Green 函数... --&lt;br /&gt;
&lt;br /&gt;
=== Infinite-order PDEs in quantum mechanics ===&lt;br /&gt;
量子力学中的无限阶偏微分方程&lt;br /&gt;
&lt;br /&gt;
In the [[phase space formulation]] of quantum mechanics,  one may consider the [[Method of quantum characteristics|quantum Hamilton's equations]] for trajectories of quantum particles. These equations are infinite-order PDEs. However, in the semiclassical expansion, one has a finite system of ODEs at any fixed order of [[Dirac constant|{{mvar|ħ}}]].  The evolution equation of the [[Wigner quasi-probability distribution|c]] is also an infinite-order PDE. The quantum trajectories are [[Method of quantum characteristics|quantum characteristics]], with the use of which one could calculate the evolution of the Wigner function.&lt;br /&gt;
&lt;br /&gt;
In the phase space formulation of quantum mechanics,  one may consider the quantum Hamilton's equations for trajectories of quantum particles. These equations are infinite-order PDEs. However, in the semiclassical expansion, one has a finite system of ODEs at any fixed order of Dirac constant|.  The evolution equation of the Wigner function is also an infinite-order PDE. The quantum trajectories are quantum characteristics, with the use of which one could calculate the evolution of the Wigner function.&lt;br /&gt;
&lt;br /&gt;
在量子力学中的相空间表述中，我们可以考虑用于求解量子粒子的轨迹的量子哈密顿的方程。这些方程是无限阶偏微分方程。然而，在半经典展开中，我们在给定[[Dirac constant|{{mvar|ħ}}]]阶数下有一个有限的的常微分方程组。'''&amp;lt;font color=&amp;quot;#ff8000&amp;quot;&amp;gt;维格纳函数  Wigner Function&amp;lt;/font&amp;gt;的演化方程也是一个无限阶偏微分方程。由于量子轨道的量子特性，所以它通常可以用来计算维格纳函数的演化。&lt;br /&gt;
&lt;br /&gt;
== Analytical solutions ==&lt;br /&gt;
解析解&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
===Separation of variables===&lt;br /&gt;
分离变量法&lt;br /&gt;
&lt;br /&gt;
{{main|Separable partial differential equation}}&lt;br /&gt;
&lt;br /&gt;
Linear PDEs can be reduced to systems of ordinary differential equations by the important technique of separation of variables. This technique rests on a characteristic of solutions to differential equations: if one can find any solution that solves the equation and satisfies the boundary conditions, then it is ''the'' solution (this also applies to ODEs). We assume as an [[ansatz]] that the dependence of a solution on the parameters space and time can be written as a product of terms that each depend on a single parameter, and then see if this can be made to solve the problem.&amp;lt;ref&amp;gt;{{cite book|last1=Gershenfeld|first1=Neil|title=The nature of mathematical modeling|date=2000|publisher=Cambridge Univ. Press|location=Cambridge|isbn=0521570956|page=27|edition=Reprinted (with corr.)}}&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
Linear PDEs can be reduced to systems of ordinary differential equations by the important technique of separation of variables. This technique rests on a characteristic of solutions to differential equations: if one can find any solution that solves the equation and satisfies the boundary conditions, then it is the solution (this also applies to ODEs). We assume as an ansatz that the dependence of a solution on the parameters space and time can be written as a product of terms that each depend on a single parameter, and then see if this can be made to solve the problem.&lt;br /&gt;
&lt;br /&gt;
线性偏微分方程组可以通过分离变量法这一重要方法来简化为常微分方程组。这种方法依赖于微分方程解的一个特征: 如果能找到任何一个满足方程和边界条件的解，那么这个解就是方程的解(这也适用于常微分方程)。我们假设解对参数空间和时间的依赖可以写成对它们每一项的依赖以及一个参数的乘积，然后再看看这是否可以用来解决这个问题。&lt;br /&gt;
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&lt;br /&gt;
&lt;br /&gt;
In the method of separation of variables, one reduces a PDE to a PDE in fewer variables, which is an ordinary differential equation if in one variable – these are in turn easier to solve.&lt;br /&gt;
&lt;br /&gt;
In the method of separation of variables, one reduces a PDE to a PDE in fewer variables, which is an ordinary differential equation if in one variable – these are in turn easier to solve.&lt;br /&gt;
&lt;br /&gt;
在分离变量法方法中，可以将偏微分方程简化为含有更少变量的偏微分方程，如果只有一个变量，那么就变成了一个'''&amp;lt;font color = &amp;quot;#ff8000&amp;quot;&amp;gt;常微分方程 Ordinary Differential Equation&amp;lt;/font&amp;gt;'''-- 反过来，这些方程也更容易求解。&lt;br /&gt;
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This is possible for simple PDEs, which are called [[separable partial differential equation]]s, and the domain is generally a rectangle (a product of intervals). Separable PDEs correspond to [[diagonal matrices]] – thinking of &amp;quot;the value for fixed {{mvar|x}}&amp;quot; as a coordinate, each coordinate can be understood separately.&lt;br /&gt;
&lt;br /&gt;
This is possible for simple PDEs, which are called separable partial differential equations, and the domain is generally a rectangle (a product of intervals). Separable PDEs correspond to diagonal matrices – thinking of &amp;quot;the value for fixed &amp;quot; as a coordinate, each coordinate can be understood separately.&lt;br /&gt;
&lt;br /&gt;
对于简单的偏微分方程(称为可分离偏微分方程)来说，这是可能的，而且方程通常定义在一个矩形区域(区间的乘积)上。可分离偏微分方程对应于对角线矩阵——以“固定值”为坐标，每个坐标可分开理解。&lt;br /&gt;
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This generalizes to the [[method of characteristics]], and is also used in [[integral transform]]s.&lt;br /&gt;
&lt;br /&gt;
This generalizes to the method of characteristics, and is also used in integral transforms.&lt;br /&gt;
&lt;br /&gt;
这种方法可以推广到特征曲线法，也可以用于积分变换。&lt;br /&gt;
&lt;br /&gt;
===Method of characteristics===&lt;br /&gt;
特征曲线法&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{{main|Method of characteristics}}&lt;br /&gt;
&lt;br /&gt;
In special cases, one can find characteristic curves on which the equation reduces to an ODE – changing coordinates in the domain to straighten these curves allows separation of variables, and is called the [[method of characteristics]].&lt;br /&gt;
&lt;br /&gt;
In special cases, one can find characteristic curves on which the equation reduces to an ODE – changing coordinates in the domain to straighten these curves allows separation of variables, and is called the method of characteristics.&lt;br /&gt;
&lt;br /&gt;
在特殊情况下，可以找到一些特征曲线，在这些曲线上方程可以变成一个常微分方程——意味着改变坐标从而使这些曲线变直从而达到分离变量的目的，这就是所谓的特征曲线法。&lt;br /&gt;
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More generally, one may find characteristic surfaces.&lt;br /&gt;
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More generally, one may find characteristic surfaces.&lt;br /&gt;
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更一般地说，人们可能会找到特征表面。&lt;br /&gt;
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===Integral transform===&lt;br /&gt;
积分变换&lt;br /&gt;
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An [[integral transform]] may transform the PDE to a simpler one, in particular, a separable PDE. This corresponds to diagonalizing an operator.&lt;br /&gt;
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An integral transform may transform the PDE to a simpler one, in particular, a separable PDE. This corresponds to diagonalizing an operator.&lt;br /&gt;
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积分变换可以将偏微分方程转换为更简单的偏微分方程，特别是可分离的偏微分方程。这对应于对角化算符。&lt;br /&gt;
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An important example of this is [[Fourier analysis]], which diagonalizes the heat equation using the [[eigenbasis]] of sinusoidal waves.&lt;br /&gt;
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An important example of this is Fourier analysis, which diagonalizes the heat equation using the eigenbasis of sinusoidal waves.&lt;br /&gt;
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这方面的一个重要例子是'''&amp;lt;font color = &amp;quot;#ff8000&amp;quot;&amp;gt;傅里叶分析  Fourier Analysis&amp;lt;/font&amp;gt;'''，它使用正弦波的特征基来对角化热方程。&lt;br /&gt;
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If the domain is finite or periodic, an infinite sum of solutions such as a [[Fourier series]] is appropriate, but an integral of solutions such as a [[Fourier integral]] is generally required for infinite domains. The solution for a point source for the heat equation given above is an example of the use of a Fourier integral.&lt;br /&gt;
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If the domain is finite or periodic, an infinite sum of solutions such as a Fourier series is appropriate, but an integral of solutions such as a Fourier integral is generally required for infinite domains. The solution for a point source for the heat equation given above is an example of the use of a Fourier integral.&lt;br /&gt;
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如果区域是有限的或周期性的，那么解为无限和的形式是恰当的，例如傅里叶级数，但是一个解的积分，例如傅立叶积分，一般是在无限区域上的。上面给出的热传导方程的点源解法就是使用傅里叶积分的一个例子。&lt;br /&gt;
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===Change of variables===&lt;br /&gt;
变量代换&lt;br /&gt;
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Often a PDE can be reduced to a simpler form with a known solution by a suitable [[Change of variables (PDE)|change of variables]].  For example, the [[Black–Scholes equation#Derivation|Black–Scholes]] PDE&lt;br /&gt;
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Often a PDE can be reduced to a simpler form with a known solution by a suitable change of variables.  For example, the Black–Scholes PDE&lt;br /&gt;
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偏微分方程通常可以通过变量的适当变化，用已知的解简化为更简单的形式。例如，布莱克-舒尔斯偏微分方程&lt;br /&gt;
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:&amp;lt;math&amp;gt; \frac{\partial V}{\partial t} + \tfrac{1}{2}\sigma^2 S^2\frac{\partial^2 V}{\partial S^2} + rS\frac{\partial V}{\partial S} - rV = 0 &amp;lt;/math&amp;gt;&lt;br /&gt;
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&amp;lt;math&amp;gt; \frac{\partial V}{\partial t} + \tfrac{1}{2}\sigma^2 S^2\frac{\partial^2 V}{\partial S^2} + rS\frac{\partial V}{\partial S} - rV = 0 &amp;lt;/math&amp;gt;&lt;br /&gt;
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is reducible to the [[heat equation]]&lt;br /&gt;
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is reducible to the heat equation&lt;br /&gt;
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可以简化为热传导方程&lt;br /&gt;
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:&amp;lt;math&amp;gt; \frac{\partial u}{\partial \tau} = \frac{\partial^2 u}{\partial x^2}&amp;lt;/math&amp;gt;&lt;br /&gt;
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&amp;lt;math&amp;gt; \frac{\partial u}{\partial \tau} = \frac{\partial^2 u}{\partial x^2}&amp;lt;/math&amp;gt;&lt;br /&gt;
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by the change of variables (for complete details see {{webarchive |url=https://web.archive.org/web/20080411030405/http://www.math.unl.edu/~sdunbar1/Teaching/MathematicalFinance/Lessons/BlackScholes/Solution/solution.shtml |date=April 11, 2008 |title=Solution of the Black Scholes Equation }})&lt;br /&gt;
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by the change of variables (for complete details see )&lt;br /&gt;
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通过变量替换(完整的细节见)&lt;br /&gt;
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:&amp;lt;math&amp;gt;\begin{align}&lt;br /&gt;
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V(S,t) &amp;amp;= K v(x,\tau),\\[5px]&lt;br /&gt;
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x &amp;amp;= \ln\left(\tfrac{S}{K} \right),\\[5px]&lt;br /&gt;
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\tau &amp;amp;= \tfrac{1}{2} \sigma^2 (T - t),\\[5px]&lt;br /&gt;
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v(x,\tau)&amp;amp;=e^{-\alpha x-\beta\tau} u(x,\tau).&lt;br /&gt;
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\end{align}&amp;lt;/math&amp;gt;&lt;br /&gt;
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===Fundamental solution===&lt;br /&gt;
基本解&lt;br /&gt;
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{{main|Fundamental solution}}&lt;br /&gt;
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Inhomogeneous equations can often be solved (for constant coefficient PDEs, always be solved) by finding the [[fundamental solution]] (the solution for a point source), then taking the [[convolution]] with the boundary conditions to get the solution.&lt;br /&gt;
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Inhomogeneous equations can often be solved (for constant coefficient PDEs, always be solved) by finding the fundamental solution (the solution for a point source), then taking the convolution with the boundary conditions to get the solution.&lt;br /&gt;
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非齐次方程(常系数偏微分方程)一般是通过先求出基本解(点源的解) ，然后利用带边界条件的卷积来求解。&lt;br /&gt;
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This is analogous in [[signal processing]] to understanding a filter by its [[impulse response]].&lt;br /&gt;
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This is analogous in signal processing to understanding a filter by its impulse response.&lt;br /&gt;
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这类似于在信号处理中通过滤波器的脉冲响应来理解滤波器。&lt;br /&gt;
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===Superposition principle===&lt;br /&gt;
叠加原理&lt;br /&gt;
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{{further| Superposition principle }}&lt;br /&gt;
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The superposition principle applies to any linear system, including linear systems of PDEs. A common visualization of this concept is the interaction of two waves in phase being combined to result in a greater amplitude, for example {{math|sin ''x'' + sin ''x'' {{=}} 2 sin ''x''}}. The same principle can be observed in PDEs where the solutions may be real or complex and additive. [[Superposition principle|superposition]]&lt;br /&gt;
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The superposition principle applies to any linear system, including linear systems of PDEs. A common visualization of this concept is the interaction of two waves in phase being combined to result in a greater amplitude, for example  2 sin x}}. The same principle can be observed in PDEs where the solutions may be real or complex and additive. superposition&lt;br /&gt;
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'''&amp;lt;font color = &amp;quot;#ff8000&amp;quot;&amp;gt;叠加原理 Superposition Principle&amp;lt;/font&amp;gt;适用于任何线性系统，包括偏微分方程的线性系统。这个概念的一个常见的可视化是两个同相位的波相互作用结合在一起会产生更大的振幅，例如 {{math|sin ''x'' + sin ''x'' {{=}} 2 sin ''x''}}。在偏微分方程中也可以观察到同样的原理，其中的解可能是真实的或复杂的和可加的。叠加&lt;br /&gt;
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If {{math|''u''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;}} and {{math|''u''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;}} are solutions of linear PDE in some function space {{mvar|R}}, then {{math|''u'' {{=}} ''c''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;''u''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; + ''c''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;''u''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;}} with any constants {{math|''c''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;}} and {{math|''c''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;}} are also a solution of that PDE in the same function space.&lt;br /&gt;
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If  and  are solutions of linear PDE in some function space , then  c&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;u&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; + c&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;u&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;}} with any constants  and  are also a solution of that PDE in the same function space.&lt;br /&gt;
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若线性偏微分方程在某个函数空间{{mvar|R}}中有解{{math|''u''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;}} 和 {{math|''u''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;}}，则{{math|''u'' {{=}} ''c''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;''u''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; + ''c''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;''u''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;}}也是该偏微分方程在同一函数空间中的解，其中{{math|''c''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;}} 和 {{math|''c''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;}} 是任意常数。&lt;br /&gt;
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===Methods for non-linear equations===&lt;br /&gt;
非线性方程的求解方法&lt;br /&gt;
{{see also|nonlinear partial differential equation}}&lt;br /&gt;
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There are no generally applicable methods to solve nonlinear PDEs. Still, existence and uniqueness results (such as the [[Cauchy–Kowalevski theorem]]) are often possible, as are proofs of important qualitative and quantitative properties of solutions (getting these results is a major part of [[mathematical analysis|analysis]]). Computational solution to the nonlinear PDEs, the [[split-step method]], exist for specific equations like [[nonlinear Schrödinger equation]].&lt;br /&gt;
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There are no generally applicable methods to solve nonlinear PDEs. Still, existence and uniqueness results (such as the Cauchy–Kowalevski theorem) are often possible, as are proofs of important qualitative and quantitative properties of solutions (getting these results is a major part of analysis). Computational solution to the nonlinear PDEs, the split-step method, exist for specific equations like nonlinear Schrödinger equation.&lt;br /&gt;
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对于非线性偏微分方程，目前还没有普遍适用的求解方法。然而，通常是可能知道解的存在性和唯一性(如柯西-科瓦列夫斯基定理)，也是可能得到解的重要定性和定量性质的证明(得到这些结果是分析的主要部分)。非线性偏微分方程的计算解，即分步法，对一些特定的方程适用，比如非线性'''&amp;lt;font color=&amp;quot;#ff8000&amp;quot;&amp;gt;薛定谔方程 Schrödinger equation&amp;lt;/font&amp;gt;'''。&lt;br /&gt;
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Nevertheless, some techniques can be used for several types of equations. The [[h-principle|{{mvar|h}}-principle]] is the most powerful method to solve [[Underdetermined system|underdetermined]] equations. The [[Riquier–Janet theory]] is an effective method for obtaining information about many analytic [[Overdetermined system|overdetermined]] systems.&lt;br /&gt;
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Nevertheless, some techniques can be used for several types of equations. The -principle is the most powerful method to solve underdetermined equations. The Riquier–Janet theory is an effective method for obtaining information about many analytic overdetermined systems.&lt;br /&gt;
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然而，一些技巧可以用于几种类型的方程。h-原理是求解欠定方程最有效的方法。里基尔-珍妮特理论是一种可以获得许多解析超定系统信息的有效方法。&lt;br /&gt;
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The [[method of characteristics]] can be used in some very special cases to solve partial differential equations.&lt;br /&gt;
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The method of characteristics can be used in some very special cases to solve partial differential equations.&lt;br /&gt;
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特征线法可用于求解某些特殊情况下的偏微分方程。&lt;br /&gt;
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In some cases, a PDE can be solved via [[perturbation analysis]] in which the solution is considered to be a correction to an equation with a known solution. Alternatives are [[numerical analysis]] techniques from simple [[finite difference]] schemes to the more mature [[multigrid]] and [[finite element method]]s. Many interesting problems in science and engineering are solved in this way using [[computer]]s, sometimes high performance [[supercomputer]]s.&lt;br /&gt;
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In some cases, a PDE can be solved via perturbation analysis in which the solution is considered to be a correction to an equation with a known solution. Alternatives are numerical analysis techniques from simple finite difference schemes to the more mature multigrid and finite element methods. Many interesting problems in science and engineering are solved in this way using computers, sometimes high performance supercomputers.&lt;br /&gt;
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在某些情况下，偏微分方程可以通过扰动分析来求解。在扰动分析中，通常是求解将具有已知解的方程修正后的新得到方程。可供选择的数值分析技术从简单的差分格式到更成熟的多重网格和有限元方法。许多有趣的科学和工程问题都是在计算机上用这种方法解决的，有时是高性能超级计算机。&lt;br /&gt;
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===Lie group method===&lt;br /&gt;
李群方法&lt;br /&gt;
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From 1870 [[Sophus Lie]]'s work put the theory of differential equations on a more satisfactory foundation. He showed that the integration theories of the older mathematicians can, by the introduction of what are now called [[Lie group]]s, be referred, to a common source; and that ordinary differential equations which admit the same [[infinitesimal transformation]]s present comparable difficulties of integration. He also emphasized the subject of [[contact transformation|transformations of contact]].&lt;br /&gt;
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From 1870 Sophus Lie's work put the theory of differential equations on a more satisfactory foundation. He showed that the integration theories of the older mathematicians can, by the introduction of what are now called Lie groups, be referred, to a common source; and that ordinary differential equations which admit the same infinitesimal transformations present comparable difficulties of integration. He also emphasized the subject of transformations of contact.&lt;br /&gt;
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从1870年起，索弗斯·李的工作为微分方程理论奠定了一个较为令人满意的基础。他指出，通过引入现在所谓的李群，老一辈数学家的积分理论可以引用到一个共同的来源; 承认相同的无穷小变换的常微分方程在积分方面存在相当的困难。他还强调了接触的转变这一主题。&lt;br /&gt;
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==[[用户:Yuling|Yuling]]（[[用户讨论:Yuling|讨论]]）这句话“He also emphasized the subject of transformations of contact.”中的transformations of contact翻译的不太好。&lt;br /&gt;
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A general approach to solving PDEs uses the symmetry property of differential equations, the continuous [[infinitesimal transformation]]s of solutions to solutions ([[Lie theory]]). Continuous [[group theory]], [[Lie algebras]] and [[differential geometry]] are used to understand the structure of linear and nonlinear partial differential equations for generating integrable equations, to find its [[Lax pair]]s, recursion operators, [[Bäcklund transform]] and finally finding exact analytic solutions to the PDE.&lt;br /&gt;
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A general approach to solving PDEs uses the symmetry property of differential equations, the continuous infinitesimal transformations of solutions to solutions (Lie theory). Continuous group theory, Lie algebras and differential geometry are used to understand the structure of linear and nonlinear partial differential equations for generating integrable equations, to find its Lax pairs, recursion operators, Bäcklund transform and finally finding exact analytic solutions to the PDE.&lt;br /&gt;
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求解偏微分方程的一般方法是利用微分方程的对称性，即解到解的连续无穷小变换(李理论)。连续群论、李代数和微分几何理论被用来理解生成可积方程的线性和非线性偏微分方程的结构，找到它的Lax对、递归算子、 贝克伦德变换，最后找到偏微分方程的精确解析解。&lt;br /&gt;
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Symmetry methods have been recognized to study differential equations arising in mathematics, physics, engineering, and many other disciplines.&lt;br /&gt;
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Symmetry methods have been recognized to study differential equations arising in mathematics, physics, engineering, and many other disciplines.&lt;br /&gt;
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对称方法已被公认可以用于研究出现在数学，物理，工程和许多其他学科的微分方程。&lt;br /&gt;
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===Semianalytical methods===&lt;br /&gt;
半解析方法&lt;br /&gt;
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The [[Adomian decomposition method]], the [[Aleksandr Lyapunov|Lyapunov]] artificial small parameter method, and He's [[homotopy perturbation method]] are all special cases of the more general [[homotopy analysis method]]. These are series expansion methods, and except for the Lyapunov method, are independent of small physical parameters as compared to the well known [[perturbation theory]], thus giving these methods greater flexibility and solution generality.&lt;br /&gt;
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The Adomian decomposition method, the Lyapunov artificial small parameter method, and He's homotopy perturbation method are all special cases of the more general homotopy analysis method. These are series expansion methods, and except for the Lyapunov method, are independent of small physical parameters as compared to the well known perturbation theory, thus giving these methods greater flexibility and solution generality.&lt;br /&gt;
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阿多米安分解法、李雅普诺夫人工小参数方法和何同伦摄动方法都是更一般的同伦分析方法的特殊情况。除了李雅普诺夫方法之外，这些都是级数展开方法，与为人熟知的摄动理论方法相比，它们与小的物理参数无关，因此这些方法具有更大的灵活性和解的通用性。&lt;br /&gt;
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== Numerical solutions ==&lt;br /&gt;
数值解&lt;br /&gt;
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The three most widely used [[Numerical partial differential equations|numerical methods to solve PDEs]] are the [[finite element analysis|finite element method]] (FEM), [[finite volume method]]s (FVM) and [[finite difference method]]s (FDM), as well other kind of methods called [[Meshfree methods]], which were made to solve problems where the before mentioned methods are limited. The FEM has a prominent position among these methods and especially its exceptionally efficient higher-order version [[hp-FEM]]. Other hybrid versions of FEM and Meshfree methods include the generalized finite element method (GFEM), [[extended finite element method]] (XFEM), [[Spectral element method|spectral finite element method]] (SFEM), [[Meshfree methods|meshfree finite element method]], [[Discontinuous Galerkin Method|discontinuous Galerkin finite element method]] (DGFEM), [[Element-Free Galerkin Method]] (EFGM), [[Interpolating Element-Free Galerkin Method]] (IEFGM), etc.&lt;br /&gt;
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The three most widely used numerical methods to solve PDEs are the finite element method (FEM), finite volume methods (FVM) and finite difference methods (FDM), as well other kind of methods called Meshfree methods, which were made to solve problems where the before mentioned methods are limited. The FEM has a prominent position among these methods and especially its exceptionally efficient higher-order version hp-FEM. Other hybrid versions of FEM and Meshfree methods include the generalized finite element method (GFEM), extended finite element method (XFEM), spectral finite element method (SFEM), meshfree finite element method, discontinuous Galerkin finite element method (DGFEM), Element-Free Galerkin Method (EFGM), Interpolating Element-Free Galerkin Method (IEFGM), etc.&lt;br /&gt;
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求解偏微分方程最常用的三种数值方法是有限元分析法、有限体积法和有限差分法，以及其他一些称为无网格法的方法。这些方法用于解决前面提到的方法受到的限制。在这些方法中，有限元方法，尤其是高效的高阶有限元方法，占有重要地位。其他有限元法和无网格法的混合形式包括广义有限元分析法(GFEM)、扩展有限元分析法(XFEM)、谱有限元分析法(SFEM)、无网格有限元分析法(DGFEM)、间断伽辽金有限元分析法(DGFEM)、无网格伽辽金法(EFGM)、插值无网格伽辽金法(IEFGM)等。&lt;br /&gt;
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=== Finite element method ===&lt;br /&gt;
有限元分析法&lt;br /&gt;
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{{main|Finite element method}}&lt;br /&gt;
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The finite element method (FEM) (its practical application often known as finite element analysis (FEA)) is a numerical technique for finding approximate solutions of partial differential equations (PDE) as well as of integral equations. The solution approach is based either on eliminating the differential equation completely (steady state problems), or rendering the PDE into an approximating system of ordinary differential equations, which are then numerically integrated using standard techniques such as Euler's method, Runge–Kutta, etc.&lt;br /&gt;
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The finite element method (FEM) (its practical application often known as finite element analysis (FEA)) is a numerical technique for finding approximate solutions of partial differential equations (PDE) as well as of integral equations. The solution approach is based either on eliminating the differential equation completely (steady state problems), or rendering the PDE into an approximating system of ordinary differential equations, which are then numerically integrated using standard techniques such as Euler's method, Runge–Kutta, etc.&lt;br /&gt;
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'''&amp;lt;font color = &amp;quot;#ff8000&amp;quot;&amp;gt;有限元分析法 Finite Element Method&amp;lt;/font&amp;gt;''' ((其实际应用通常被称为有限元分析(FEA))是一种寻找偏微分方程(PDE)和积分方程近似解的数值技术。这种求解方法要么基于完全消除微分方程(稳态问题) ，要么将偏微分方程转化为常微分方程的近似系统，然后使用标准技术进行数值积分，如欧拉方法、 Runge-Kutta 等。&lt;br /&gt;
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===Finite difference method===&lt;br /&gt;
有限差分法&lt;br /&gt;
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{{main|Finite difference method}}&lt;br /&gt;
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Finite-difference methods are numerical methods for approximating the solutions to differential equations using [[finite difference]] equations to approximate derivatives.&lt;br /&gt;
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Finite-difference methods are numerical methods for approximating the solutions to differential equations using finite difference equations to approximate derivatives.&lt;br /&gt;
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有限差分法是一种数值方法，用差分方程近似微分方程的解。&lt;br /&gt;
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=== Finite volume method ===&lt;br /&gt;
有限体积法&lt;br /&gt;
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{{main|Finite volume method}}&lt;br /&gt;
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Similar to the finite difference method or finite element method, values are calculated at discrete places on a meshed geometry. &amp;quot;Finite volume&amp;quot; refers to the small volume surrounding each node point on a mesh. In the finite volume method, surface integrals in a partial differential equation that contain a divergence term are converted to volume integrals, using the [[divergence theorem]]. These terms are then evaluated as fluxes at the surfaces of each finite volume. Because the flux entering a given volume is identical to that leaving the adjacent volume, these methods conserve mass by design.&lt;br /&gt;
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Similar to the finite difference method or finite element method, values are calculated at discrete places on a meshed geometry. &amp;quot;Finite volume&amp;quot; refers to the small volume surrounding each node point on a mesh. In the finite volume method, surface integrals in a partial differential equation that contain a divergence term are converted to volume integrals, using the divergence theorem. These terms are then evaluated as fluxes at the surfaces of each finite volume. Because the flux entering a given volume is identical to that leaving the adjacent volume, these methods conserve mass by design.&lt;br /&gt;
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类似于有限差分法或有限元分析，函数值是在网状几何体上的离散位置进行计算的。“有限体积”是指网格上每个节点周围的小体积。在有限体积法中，偏微分方程中含有散度项的面积分用散度定理积分转换成体积分。然后将这些项用于估算每个有限体积表面上的通量。由于进入给定体积的通量与转移到相邻体积元的通量相同，所以这些方法在设计上保证了质量守恒。&lt;br /&gt;
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==See also==&lt;br /&gt;
请参阅&lt;br /&gt;
* [[Dirichlet boundary condition]]&lt;br /&gt;
狄利克雷边界条件&lt;br /&gt;
* [[Jet bundle]]&lt;br /&gt;
射流丛&lt;br /&gt;
* [[Laplace transform applied to differential equations]]&lt;br /&gt;
微分方程中的拉普拉斯变换&lt;br /&gt;
* [[List of dynamical systems and differential equations topics]]&lt;br /&gt;
动力学系统和微分方程的列表&lt;br /&gt;
* [[Matrix differential equation]]&lt;br /&gt;
矩阵微分方程&lt;br /&gt;
* [[Neumann boundary condition]]&lt;br /&gt;
诺伊曼边界条件&lt;br /&gt;
* [[Numerical partial differential equations]]&lt;br /&gt;
数值偏微分方程&lt;br /&gt;
* [[Partial differential algebraic equation]]&lt;br /&gt;
偏微分代数方程&lt;br /&gt;
* [[Recurrence relation]]&lt;br /&gt;
递推关系&lt;br /&gt;
* [[Robin boundary condition]]&lt;br /&gt;
罗宾边界条件&lt;br /&gt;
* [[Stochastic processes and boundary value problems]]&lt;br /&gt;
随机过程和边值问题&lt;br /&gt;
&lt;br /&gt;
== The energy method ==&lt;br /&gt;
能量法&lt;br /&gt;
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The energy method is a mathematical procedure that can be used to verify well-posedness of initial-boundary-value-problems.&amp;lt;ref&amp;gt;{{cite book |title=High Order Difference Methods for Time Dependent PDE&lt;br /&gt;
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The energy method is a mathematical procedure that can be used to verify well-posedness of initial-boundary-value-problems.&amp;lt;ref&amp;gt;{{cite book |title=High Order Difference Methods for Time Dependent PDE&lt;br /&gt;
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能量法是验证初边值问题适定性的一种数学方法。 时变偏微分方程的高阶差分方法&lt;br /&gt;
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|first=Bertil|last=Gustafsson|publisher=Springer|year=2008|isbn=978-3-540-74992-9|doi=10.1007/978-3-540-74993-6}}&amp;lt;/ref&amp;gt; In the following example the energy method is used to decide where and which boundary conditions should be imposed such that the resulting IBVP is well-posed. Consider the one-dimensional hyperbolic PDE given by&lt;br /&gt;
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|first=Bertil|last=Gustafsson|publisher=Springer|year=2008|isbn=978-3-540-74992-9|doi=10.1007/978-3-540-74993-6}}&amp;lt;/ref&amp;gt; In the following example the energy method is used to decide where and which boundary conditions should be imposed such that the resulting IBVP is well-posed. Consider the one-dimensional hyperbolic PDE given by&lt;br /&gt;
&lt;br /&gt;
| first Bertil | last Gustafsson | publisher | Springer | year 2008 | isbn 978-3-540-74992-9 | doi 10.1007 / 978-3-540-74993-6} / ref 在下面的例子中，使用能量方法来决定应该施加哪些边界条件，使得得到的 IBVP适定。考虑一维双曲偏微分方程&lt;br /&gt;
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: &amp;lt;math&amp;gt;\frac{\partial u}{\partial t} + \alpha \frac{\partial u}{\partial x} = 0, \quad x \in [a,b], \operatorname t &amp;gt; 0,&amp;lt;/math&amp;gt;&lt;br /&gt;
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 &amp;lt;math&amp;gt;\frac{\partial u}{\partial t} + \alpha \frac{\partial u}{\partial x} = 0, \quad x \in [a,b], \operatorname t &amp;gt; 0,&amp;lt;/math&amp;gt;&lt;br /&gt;
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where &amp;lt;math&amp;gt;\alpha \neq 0&amp;lt;/math&amp;gt; is a constant and &amp;lt;math&amp;gt;u(x,t)&amp;lt;/math&amp;gt; is an unknown function with initial condition &amp;lt;math&amp;gt;u(x,0) = f(x)&amp;lt;/math&amp;gt;. Multiplying with &amp;lt;math&amp;gt;u&amp;lt;/math&amp;gt; and integrating over the domain gives&lt;br /&gt;
&lt;br /&gt;
where &amp;lt;math&amp;gt;\alpha \neq 0&amp;lt;/math&amp;gt; is a constant and &amp;lt;math&amp;gt;u(x,t)&amp;lt;/math&amp;gt; is an unknown function with initial condition &amp;lt;math&amp;gt;u(x,0) = f(x)&amp;lt;/math&amp;gt;. Multiplying with &amp;lt;math&amp;gt;u&amp;lt;/math&amp;gt; and integrating over the domain gives&lt;br /&gt;
&lt;br /&gt;
其中 &amp;lt;math&amp;gt;\alpha \neq 0&amp;lt;/math&amp;gt; 是常数，并且 &amp;lt;math&amp;gt;u(x,t)&amp;lt;/math&amp;gt; 是未知函数，初始条件是 &amp;lt;math&amp;gt;u(x,0) = f(x)&amp;lt;/math&amp;gt;。乘以 &amp;lt;math&amp;gt;u&amp;lt;/math&amp;gt; 并在域上进行积分。&lt;br /&gt;
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: &amp;lt;math&amp;gt;\int_a^b u \frac{\partial u}{\partial t} \operatorname dx + \alpha \int _a ^b u \frac{\partial u}{\partial x} \operatorname dx = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;\int_a^b u \frac{\partial u}{\partial t} \operatorname dx + \alpha \int _a ^b u \frac{\partial u}{\partial x} \operatorname dx = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
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Using that&lt;br /&gt;
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Using that&lt;br /&gt;
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利用这一点&lt;br /&gt;
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: &amp;lt;math&amp;gt;\int _a ^b u \frac{\partial u}{\partial t} \operatorname dx = \frac{1}{2} \frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 \quad \text{and} \quad \int _a ^b u \frac{\partial u}{\partial x} \operatorname dx = \frac{1}{2} u(b,t)^2 - \frac{1}{2} u(a,t)^2,.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;\int _a ^b u \frac{\partial u}{\partial t} \operatorname dx = \frac{1}{2} \frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 \quad \text{and} \quad \int _a ^b u \frac{\partial u}{\partial x} \operatorname dx = \frac{1}{2} u(b,t)^2 - \frac{1}{2} u(a,t)^2,.&amp;lt;/math&amp;gt;&lt;br /&gt;
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where integration by parts has been used for the second relationship, we get&lt;br /&gt;
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where integration by parts has been used for the second relationship, we get&lt;br /&gt;
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第二个关系中采用了分部积分法，我们可以得到&lt;br /&gt;
&lt;br /&gt;
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: &amp;lt;math&amp;gt;\frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 + \alpha u(b,t)^2 - \alpha u(a,t)^2 = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;\frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 + \alpha u(b,t)^2 - \alpha u(a,t)^2 = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
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Here &amp;lt;math&amp;gt;\vert \vert \cdot \vert \vert&amp;lt;/math&amp;gt; denotes the standard L2-norm.&lt;br /&gt;
&lt;br /&gt;
Here &amp;lt;math&amp;gt;\vert \vert \cdot \vert \vert&amp;lt;/math&amp;gt; denotes the standard L2-norm.&lt;br /&gt;
&lt;br /&gt;
在这里，&amp;lt;math&amp;gt;\vert \vert \cdot \vert \vert&amp;lt;/math&amp;gt; 表示标准的 L2-正则。&lt;br /&gt;
&lt;br /&gt;
For well-posedness we require that the energy of the solution is non-increasing, i.e. that &amp;lt;math&amp;gt;\frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 \leq 0&amp;lt;/math&amp;gt;, which is achieved by specifying &amp;lt;math&amp;gt;u&amp;lt;/math&amp;gt; at &amp;lt;math&amp;gt;x = a&amp;lt;/math&amp;gt; if &amp;lt;math&amp;gt;\alpha &amp;gt; 0&amp;lt;/math&amp;gt; and at &amp;lt;math&amp;gt;x = b&amp;lt;/math&amp;gt; if &amp;lt;math&amp;gt;\alpha &amp;lt; 0&amp;lt;/math&amp;gt;. This corresponds to only imposing boundary conditions at the inflow. Note that well-posedness allows for growth in terms of data (initial and boundary) and thus it is sufficient to show that &amp;lt;math&amp;gt;\frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 \leq 0&amp;lt;/math&amp;gt; holds when all data is set to zero.&lt;br /&gt;
&lt;br /&gt;
For well-posedness we require that the energy of the solution is non-increasing, i.e. that &amp;lt;math&amp;gt;\frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 \leq 0&amp;lt;/math&amp;gt;, which is achieved by specifying &amp;lt;math&amp;gt;u&amp;lt;/math&amp;gt; at &amp;lt;math&amp;gt;x = a&amp;lt;/math&amp;gt; if &amp;lt;math&amp;gt;\alpha &amp;gt; 0&amp;lt;/math&amp;gt; and at &amp;lt;math&amp;gt;x = b&amp;lt;/math&amp;gt; if &amp;lt;math&amp;gt;\alpha &amp;lt; 0&amp;lt;/math&amp;gt;. This corresponds to only imposing boundary conditions at the inflow. Note that well-posedness allows for growth in terms of data (initial and boundary) and thus it is sufficient to show that &amp;lt;math&amp;gt;\frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 \leq 0&amp;lt;/math&amp;gt; holds when all data is set to zero.&lt;br /&gt;
&lt;br /&gt;
对于适定性，我们要解的能量是不增加的，即 &amp;lt;math&amp;gt;\frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 \leq 0&amp;lt;/math&amp;gt; ，这种关系可以通过在&amp;lt;math&amp;gt;x = a&amp;lt;/math&amp;gt;处 （如果 &amp;lt;math&amp;gt;\alpha &amp;gt; 0&amp;lt;/math&amp;gt;） 以及 &amp;lt;math&amp;gt;x = b&amp;lt;/math&amp;gt;处 （如果 &amp;lt;math&amp;gt;\alpha &amp;lt; 0&amp;lt;/math&amp;gt;）指定&amp;lt;math&amp;gt;u&amp;lt;/math&amp;gt;的值来实现。这只相当于在入流处附加边界条件。注意，适定性允许在数据(初始和边界)上的增长，因此它足以表明当所有数据设置为零时应有 &amp;lt;math&amp;gt;\frac{\partial}{\partial t} \vert \vert u \vert \vert ^2 \leq 0&amp;lt;/math&amp;gt;。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==[[用户:Yuling|Yuling]]（[[用户讨论:Yuling|讨论]]）“This corresponds to only imposing boundary conditions at the inflow.” 这句话中的inflow不是很理解&lt;br /&gt;
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==Notes==&lt;br /&gt;
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{{Reflist}}&lt;br /&gt;
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* {{cite book |title=High Order Difference Methods for Time Dependent PDE&lt;br /&gt;
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|first=Bertil|last=Gustafsson|publisher=Springer|year=2008|isbn=978-3-540-74992-9|doi=10.1007/978-3-540-74993-6}}&lt;br /&gt;
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|first=Bertil|last=Gustafsson|publisher=Springer|year=2008|isbn=978-3-540-74992-9|doi=10.1007/978-3-540-74993-6}}&lt;br /&gt;
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| first Bertil | last Gustafsson | Springer | year 2008 | isbn 978-3-540-74992-9 | doi 10.1007 / 978-3-540-74993-6}&lt;br /&gt;
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== Further reading ==&lt;br /&gt;
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* {{Cite journal|last=Cajori|first=Florian|authorlink=Florian Cajori|year=1928|title=The Early History of Partial Differential Equations and of Partial Differentiation and Integration|url=http://www.math.harvard.edu/archive/21a_fall_14/exhibits/cajori/cajori.pdf|journal=The American Mathematical Monthly|volume=35|issue=9|pages=459–467|doi=10.2307/2298771|access-date=2016-05-15|archive-url=https://web.archive.org/web/20181123102253/http://www.math.harvard.edu/archive/21a_fall_14/exhibits/cajori/cajori.pdf|archive-date=2018-11-23|url-status=dead}}&lt;br /&gt;
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== External links ==&lt;br /&gt;
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{{Sister project links| wikt=no | commons=Category:Solutions of PDE | b=Partial Differential Equations | n=no | q=Partial differential equation | s=no | v=no | voy=no | species=no | d=no}}&lt;br /&gt;
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* {{springer|title=Differential equation, partial|id=p/d031920}}&lt;br /&gt;
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* [http://eqworld.ipmnet.ru/en/pde-en.htm Partial Differential Equations: Exact Solutions] at EqWorld: The World of Mathematical Equations.&lt;br /&gt;
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* [http://eqworld.ipmnet.ru/en/solutions/eqindex/eqindex-pde.htm Partial Differential Equations: Index] at EqWorld: The World of Mathematical Equations.&lt;br /&gt;
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* [http://eqworld.ipmnet.ru/en/methods/meth-pde.htm Partial Differential Equations: Methods] at EqWorld: The World of Mathematical Equations.&lt;br /&gt;
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* [https://web.archive.org/web/20170701144823/http://www.exampleproblems.com/wiki/index.php?title=Partial_Differential_Equations Example problems with solutions] at exampleproblems.com&lt;br /&gt;
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* [http://mathworld.wolfram.com/PartialDifferentialEquation.html Partial Differential Equations] at mathworld.wolfram.com&lt;br /&gt;
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* [https://reference.wolfram.com/language/FEMDocumentation/tutorial/SolvingPDEwithFEM.html Partial Differential Equations] with Mathematica&lt;br /&gt;
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* [http://www.mathworks.com/moler/pdes.pdf Partial Differential Equations] in Cleve Moler: Numerical Computing with MATLAB&lt;br /&gt;
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* [http://www.nag.com/numeric/fl/nagdoc_fl24/html/D03/d03intro.html Partial Differential Equations] at nag.com&lt;br /&gt;
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* {{cite web |first=Grant |last=Sanderson |title=But what is a partial differential equation? |work=3Blue1Brown |date=April 21, 2019 |url=https://www.youtube.com/watch?v=ly4S0oi3Yz8&amp;amp;list=PLZHQObOWTQDNPOjrT6KVlfJuKtYTftqH6 |via=[[YouTube]] }}&lt;br /&gt;
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		<author><name>Ruili</name></author>
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	<entry>
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		<title>分形维数</title>
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		<updated>2020-11-01T18:17:50Z</updated>

		<summary type="html">&lt;p&gt;Ruili：&lt;/p&gt;
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&lt;div&gt;此词条暂由彩云小译翻译，未经人工整理和审校，带来阅读不便，请见谅。&lt;br /&gt;
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Example of non-integer dimensions. The first four [[iteration]]s of the [[Koch snowflake|Koch curve]], where after each iteration, all original line segments are replaced with four, each a self-similar copy that is 1/3 the length of the original. One formalism of the Hausdorff dimension uses this scale factor (3) and the number of self-similar objects (4) to calculate the dimension, D, after the first iteration to be D = (log N)/(log S) = (log 4)/(log 3) ≈ 1.26.&amp;lt;ref name=CampbellAnnenberg15&amp;gt;MacGregor Campbell, 2013, &amp;quot;5.6 Scaling and the Hausdorff Dimension,&amp;quot; at ''Annenberg Learner:MATHematics illuminated'', see [http://www.learner.org/courses/mathilluminated/units/5/textbook/06.php], accessed 5 March 2015.&amp;lt;/ref&amp;gt; That is, while the Hausdorff dimension of a single [[point (geometry)|point]] is zero, of a [[line segment]] is 1, of a [[square]] is 2, and of a [[cube]] is 3, for [[fractal]]s such as this, the object can have a non-integer dimension.&lt;br /&gt;
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Example of non-integer dimensions. The first four iterations of the Koch curve, where after each iteration, all original line segments are replaced with four, each a self-similar copy that is 1/3 the length of the original. One formalism of the Hausdorff dimension uses this scale factor (3) and the number of self-similar objects (4) to calculate the dimension, D, after the first iteration to be D = (log N)/(log S) = (log 4)/(log 3) ≈ 1.26. That is, while the Hausdorff dimension of a single point is zero, of a line segment is 1, of a square is 2, and of a cube is 3, for fractals such as this, the object can have a non-integer dimension.&lt;br /&gt;
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非整数维度示例：前四个[[Koch 曲线]]的迭代，在每次迭代后，所有原始线段都被替换为四个，每个自相似的复制是原始线段长度的1 / 3。豪斯多夫维数的一个建模是使用比例因子(3)和自相似对象的数量(4)来计算维度 D，在第一次迭代后为 D = (log N)/(log S) = (log 4)/(log 3) ≈ 1.26.&amp;lt;ref name=CampbellAnnenberg15&amp;gt;。MacGregor Campbell, 2013, &amp;quot;5.6 Scaling and the Hausdorff Dimension,&amp;quot; 在 ''Annenberg Learner:MATHematics illuminated'', 参见 [http://www.learner.org/courses/mathilluminated/units/5/textbook/06.php], accessed 5 March 2015.&amp;lt;/ref&amp;gt; 也就是说，单点的豪斯多夫维数为零，线段为1，正方形为2，立方体为3时，但对于分形，对象可以有一个非整数维度。&lt;br /&gt;
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In [[mathematics]], '''Hausdorff dimension''' is a measure of ''roughness'', or more specifically, [[fractal dimension]], that was first introduced in 1918 by [[mathematician]] [[Felix Hausdorff]].&amp;lt;ref&amp;gt;{{Cite journal |arxiv = 1101.1444|doi = 10.1214/11-STS370|title = Estimators of Fractal Dimension: Assessing the Roughness of Time Series and Spatial Data|journal = Statistical Science|volume = 27|issue = 2|pages = 247–277|year = 2012|last1 = Gneiting|first1 = Tilmann|last2 = Ševčíková|first2 = Hana|last3 = Percival|first3 = Donald B.}}&amp;lt;/ref&amp;gt; For instance, the Hausdorff dimension of a single [[point (geometry)|point]] is zero, of a [[line segment]] is 1, of a [[square]] is 2, and of a [[cube]] is 3. That is, for sets of points that define a smooth shape or a shape that has a small number of corners—the shapes of traditional geometry and science—the Hausdorff dimension is an [[integer]] agreeing with the usual sense of dimension, also known as the [[Inductive dimension|topological dimension]]. However, formulas have also been developed that allow calculation of the dimension of other less simple objects, where, solely on the basis of their properties of [[scaling (geometry)|scaling]] and [[self-similarity]], one is led to the conclusion that particular objects—including [[fractal]]s—have non-integer Hausdorff dimensions. Because of the significant technical advances made by [[Abram Samoilovitch Besicovitch]] allowing computation of dimensions for highly irregular or &amp;quot;rough&amp;quot; sets, this dimension is also commonly referred to as the ''Hausdorff–Besicovitch dimension.''&lt;br /&gt;
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In mathematics, Hausdorff dimension is a measure of roughness, or more specifically, fractal dimension, that was first introduced in 1918 by mathematician Felix Hausdorff. For instance, the Hausdorff dimension of a single point is zero, of a line segment is 1, of a square is 2, and of a cube is 3. That is, for sets of points that define a smooth shape or a shape that has a small number of corners—the shapes of traditional geometry and science—the Hausdorff dimension is an integer agreeing with the usual sense of dimension, also known as the topological dimension. However, formulas have also been developed that allow calculation of the dimension of other less simple objects, where, solely on the basis of their properties of scaling and self-similarity, one is led to the conclusion that particular objects—including fractals—have non-integer Hausdorff dimensions. Because of the significant technical advances made by Abram Samoilovitch Besicovitch allowing computation of dimensions for highly irregular or &amp;quot;rough&amp;quot; sets, this dimension is also commonly referred to as the Hausdorff–Besicovitch dimension.&lt;br /&gt;
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在[[数学]]中，'''&amp;lt;font color = '#ff8000'&amp;gt;豪斯多夫维数Hausdorff dimension&amp;lt;/font&amp;gt;'''是一种粗糙度的度量单位，或者更确切地说，分形维数，是由数学家 Felix Hausdorff 在1918年首次提出的。例如，单点的豪斯多夫维数为零，线段为1，正方形为2，立方体为3。也就是说，对于定义了一个光滑形状或一个有少数几个角的形状---- 传统几何学和科学的形状---- 的点集来说，豪斯多夫维数是一个整数，符合通常的维度意义，也称为拓扑维度。然而，还有一些公式允许计算其他不太简单的对象的维数，其中仅仅根据它们的标度和自相似特性，就可以得出结论: 特定的对象ー包括分形ー具有非整数的 Hausdorff 维数。由于阿布拉姆·萨莫伊洛维奇·贝西科维奇的重大技术进步，允许计算高度不规则或“粗糙”集的维度，这个维度通常也被称为 Hausdorff-Besicovitch 维度。 &lt;br /&gt;
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The Hausdorff dimension, more specifically, is a further dimensional number associated with a given set, where the distances between all members of that set are defined. Such a set is termed a [[metric space]]. The dimension is drawn from the [[Extended real number line|extended real numbers]], &amp;lt;math&amp;gt;\overline{\mathbb{R}}&amp;lt;/math&amp;gt;, as opposed to the more intuitive notion of dimension, which is not associated to general metric spaces, and only takes values in the non-negative integers.&lt;br /&gt;
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The Hausdorff dimension, more specifically, is a further dimensional number associated with a given set, where the distances between all members of that set are defined. Such a set is termed a metric space. The dimension is drawn from the extended real numbers, &amp;lt;math&amp;gt;\overline{\mathbb{R}}&amp;lt;/math&amp;gt;, as opposed to the more intuitive notion of dimension, which is not associated to general metric spaces, and only takes values in the non-negative integers.&lt;br /&gt;
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更具体地说，豪斯多夫维数是一个与给定集合相关联的更进一步的维数，其中定义了该集合所有成员之间的距离。这样的集合称为度量空间。维数是从扩展的实数，&amp;lt;math&amp;gt;\overline{\mathbb{R}}&amp;lt;/math&amp;gt;，而不是更直观的维数概念(它不与一般的度量空间相关联，只取非负整数的值)。&lt;br /&gt;
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In mathematical terms, the Hausdorff dimension generalizes the notion of the dimension of a real [[vector space]]. That is, the Hausdorff dimension of an ''n''-dimensional [[inner product space]] equals ''n''. This underlies the earlier statement that the Hausdorff dimension of a point is zero, of a line is one, etc., and that [[fractal|irregular sets]] can have noninteger Hausdorff dimensions. For instance, the [[Koch snowflake]] shown at right is constructed from an equilateral triangle; in each iteration, its component line segments are divided into 3 segments of unit length, the newly created middle segment is used as the base of a new [[equilateral]] triangle that points outward, and this base segment is then deleted to leave a final object from the iteration of unit length of 4.&amp;lt;ref&amp;gt;Larry Riddle, 2014, &amp;quot;Classic Iterated Function Systems: Koch Snowflake&amp;quot;, Agnes Scott College e-Academy (online), see [http://ecademy.agnesscott.edu/~lriddle/ifs/ksnow/ksnow.htm], accessed 5 March 2015.&amp;lt;/ref&amp;gt; That is, after the first iteration, each original line segment has been replaced with N=4, where each self-similar copy is 1/S = 1/3 as long as the original.&amp;lt;ref name=CampbellAnnenberg15/&amp;gt; Stated another way, we have taken an object with Euclidean dimension, D, and reduced its linear scale by 1/3 in each direction, so that its length increases to N=S&amp;lt;sup&amp;gt;D&amp;lt;/sup&amp;gt;.&amp;lt;ref name=ClaytonSCTPLS96&amp;gt;Keith Clayton, 1996, &amp;quot;Fractals and the Fractal Dimension,&amp;quot; ''Basic Concepts in Nonlinear Dynamics and Chaos'' (workshop), Society for Chaos Theory in Psychology and the Life Sciences annual meeting, June 28, 1996, Berkeley, California, see [http://www.vanderbilt.edu/AnS/psychology/cogsci/chaos/workshop/Workshop.html], accessed 5 March 2015.&amp;lt;/ref&amp;gt; This equation is easily solved for D, yielding the ratio of logarithms (or [[natural logarithm]]s) appearing in the figures, and giving—in the Koch and other fractal cases—non-integer dimensions for these objects.&lt;br /&gt;
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In mathematical terms, the Hausdorff dimension generalizes the notion of the dimension of a real vector space. That is, the Hausdorff dimension of an n-dimensional inner product space equals n. This underlies the earlier statement that the Hausdorff dimension of a point is zero, of a line is one, etc., and that irregular sets can have noninteger Hausdorff dimensions. For instance, the Koch snowflake shown at right is constructed from an equilateral triangle; in each iteration, its component line segments are divided into 3 segments of unit length, the newly created middle segment is used as the base of a new equilateral triangle that points outward, and this base segment is then deleted to leave a final object from the iteration of unit length of 4. That is, after the first iteration, each original line segment has been replaced with N=4, where each self-similar copy is 1/S = 1/3 as long as the original. This equation is easily solved for D, yielding the ratio of logarithms (or natural logarithms) appearing in the figures, and giving—in the Koch and other fractal cases—non-integer dimensions for these objects.&lt;br /&gt;
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用数学术语来说，豪斯多夫维数概括了实向量空间维数的概念。也就是说，n 维内积空间的豪斯多夫维数等于 n。 这就是早期假设的基础，一个点的豪斯多夫维数是零，一条线是一等等，不规则集可以有非整数的豪斯多夫维数。例如，右边所示的 Koch 雪花是由一个正三角形构成的; 在每次迭代中，它的组成线段被分成单位长度的3段，新创建的中间线段被用作一个指向外部的新正三角形的基础，然后人们删除这个基础线段用来保留单位长度4的迭代中的最终对象。也就是说，在第一次迭代之后，每个原始线段都被替换为 N=4，其中每个自相似拷贝的长度是原始线段的1/S = 1/3 。这个方程很容易求解为 D，产生出现在图形中的对数(或自然对数)的比率，并给出——在 Koch 和其他分形情况下——这些对象的非整数维数。&lt;br /&gt;
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The Hausdorff dimension is a successor to the simpler, but usually equivalent, box-counting or [[Minkowski–Bouligand dimension]].&lt;br /&gt;
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The Hausdorff dimension is a successor to the simpler, but usually equivalent, box-counting or Minkowski–Bouligand dimension.&lt;br /&gt;
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豪斯多夫维数是更简单但通常等价的'''&amp;lt;font color = '#ff8000'&amp;gt;计盒维数box-counting&amp;lt;/font&amp;gt;'''或'''&amp;lt;font color = '#ff8000'&amp;gt;闵可夫斯基维数Minkowski-Bouligand&amp;lt;/font&amp;gt;'''的继承者。&lt;br /&gt;
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==Intuition概念==&lt;br /&gt;
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The intuitive concept of dimension of a geometric object ''X'' is the number of independent parameters one needs to pick out a unique point inside. However, any point specified by two parameters can be instead specified by one, because the [[cardinality]] of the [[real plane]] is equal to the cardinality of the [[real line]] (this can be seen by an [[Cantor's diagonal argument|argument]] involving interweaving the digits of two numbers to yield a single number encoding the same information). The example of a [[space-filling curve]] shows that one can even map the real line to the real plane [[Surjective function|surjectively]] (taking one real number into a pair of real numbers in a way so that all pairs of numbers are covered) and ''continuously'', so that a one-dimensional object completely fills up a higher-dimensional object.&lt;br /&gt;
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The intuitive concept of dimension of a geometric object X is the number of independent parameters one needs to pick out a unique point inside. However, any point specified by two parameters can be instead specified by one, because the cardinality of the real plane is equal to the cardinality of the real line (this can be seen by an argument involving interweaving the digits of two numbers to yield a single number encoding the same information). The example of a space-filling curve shows that one can even map the real line to the real plane surjectively (taking one real number into a pair of real numbers in a way so that all pairs of numbers are covered) and continuously, so that a one-dimensional object completely fills up a higher-dimensional object.&lt;br /&gt;
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几何对象X的尺寸的直观概念是指需要多少个独立参数才能找到一个独特的点。但是，任何由两个参数指定的点都可以由一个参数指定，因为为实平面的基数等于实线的基数(这可以通过交织两个数字以产生一个编码相同信息的单个数字看到)。'''&amp;lt;font color = '#ff8000'&amp;gt;皮亚诺曲线&amp;lt;/font&amp;gt;'''的例子表明，可以将实线完美和连续地映射到实平面(把一个实数转换成一对实数，从而覆盖所有实数对)，由此一维对象完全填充了一个高维对象。&lt;br /&gt;
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Every space filling curve hits some points multiple times, and does not have a continuous inverse. It is impossible to map two dimensions onto one in a way that is continuous and continuously invertible. The topological dimension, also called [[Lebesgue covering dimension]], explains why. This dimension is ''n'' if, in every covering of ''X'' by small open balls, there is at least one point where ''n''&amp;amp;nbsp;+&amp;amp;nbsp;1 balls overlap. For example, when one covers a line with short open intervals, some points must be covered twice, giving dimension&amp;amp;nbsp;''n''&amp;amp;nbsp;=&amp;amp;nbsp;1.&lt;br /&gt;
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Every space filling curve hits some points multiple times, and does not have a continuous inverse. It is impossible to map two dimensions onto one in a way that is continuous and continuously invertible. The topological dimension, also called Lebesgue covering dimension, explains why. This dimension is n if, in every covering of X by small open balls, there is at least one point where n&amp;amp;nbsp;+&amp;amp;nbsp;1 balls overlap. For example, when one covers a line with short open intervals, some points must be covered twice, giving dimension&amp;amp;nbsp;n&amp;amp;nbsp;=&amp;amp;nbsp;1.&lt;br /&gt;
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每条空间填充曲线都会多次击中某些点，且不存在连续的逆。将二维以连续和连续可逆的方式映射到一维是不可能的。'''&amp;lt;font color = '#ff8000'&amp;gt;拓扑维度 topological dimension&amp;lt;/font&amp;gt;'''，也被称为Lebesgue覆盖维数，解释了为什么。如果在 x 的每个小开球覆盖中，至少有一个点 n + 1个球重叠，这个维度是 n。例如，当用短的开区间覆盖一条线时，某些点必须被覆盖两次，给出维数''n''&amp;amp;nbsp;=&amp;amp;nbsp;1。&lt;br /&gt;
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But topological dimension is a very crude measure of the local size of a space (size near a point). A curve that is almost space-filling can still have topological dimension one, even if it fills up most of the area of a region. A [[fractal]] has an integer topological dimension, but in terms of the amount of space it takes up, it behaves like a higher-dimensional space.&lt;br /&gt;
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But topological dimension is a very crude measure of the local size of a space (size near a point). A curve that is almost space-filling can still have topological dimension one, even if it fills up most of the area of a region. A fractal has an integer topological dimension, but in terms of the amount of space it takes up, it behaves like a higher-dimensional space.&lt;br /&gt;
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但是，拓扑维度是对空间局部尺寸(点附近的尺寸)的一个非常粗略的度量。一条几乎是空间填充的曲线仍然可以有一维拓扑，即使它填充了一个区域的大部分面积。分形具有整数的拓扑维数，但就其所占的空间量而言，它看起来像一个更高维的空间。&lt;br /&gt;
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The Hausdorff dimension measures the local size of a space taking into account the distance between points, the [[metric space|metric]]. Consider the number ''N''(''r'') of [[ball (mathematics)|balls]] of radius at most ''r'' required to cover ''X'' completely. When ''r'' is very small, ''N''(''r'') grows polynomially with 1/''r''. For a sufficiently well-behaved  ''X'', the Hausdorff dimension is the unique number ''d'' such that N(''r'') grows as 1/''r&amp;lt;sup&amp;gt;d&amp;lt;/sup&amp;gt;'' as ''r'' approaches zero. More precisely, this defines the [[Minkowski–Bouligand dimension|box-counting dimension]], which equals the Hausdorff dimension when the value ''d'' is a critical boundary between growth rates that are insufficient to cover the space, and growth rates that are overabundant.&lt;br /&gt;
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The Hausdorff dimension measures the local size of a space taking into account the distance between points, the metric. Consider the number N(r) of balls of radius at most r required to cover X completely. When r is very small, N(r) grows polynomially with 1/r. For a sufficiently well-behaved  X, the Hausdorff dimension is the unique number d such that N(r) grows as 1/r&amp;lt;sup&amp;gt;d&amp;lt;/sup&amp;gt; as r approaches zero. More precisely, this defines the box-counting dimension, which equals the Hausdorff dimension when the value d is a critical boundary between growth rates that are insufficient to cover the space, and growth rates that are overabundant.&lt;br /&gt;
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豪斯多夫维数测量一个空间的局部大小时，会考虑到点之间距离（度量）。考虑半径最大为 r 的球数 ''N'' (r) ，需要完全覆盖 ''X''。当 r 很小时，n (r)以1/''r'' 的多项式增长。对于一个表现足够好的 ''X''，豪斯多夫维数是唯一的数 d，这样当 r 趋近于零时， N(r)增长为1/r&amp;lt;sup&amp;gt;d&amp;lt;/sup&amp;gt; 。更确切地说，这定义了盒子计数维度，当值 d 是不足以覆盖空间的增长率和过度充裕的增长率之间的临界边界时，它等于豪斯多夫维数。&lt;br /&gt;
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For shapes that are smooth, or shapes with a small number of corners, the shapes of traditional geometry and science, the Hausdorff dimension is an integer agreeing with the topological dimension. But [[Benoit Mandelbrot]] observed that [[fractal]]s, sets with noninteger Hausdorff dimensions, are found everywhere in nature. He observed that the proper idealization of most rough shapes you see around you is not in terms of smooth idealized shapes, but in terms of fractal idealized shapes:&lt;br /&gt;
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For shapes that are smooth, or shapes with a small number of corners, the shapes of traditional geometry and science, the Hausdorff dimension is an integer agreeing with the topological dimension. But Benoit Mandelbrot observed that fractals, sets with noninteger Hausdorff dimensions, are found everywhere in nature. He observed that the proper idealization of most rough shapes you see around you is not in terms of smooth idealized shapes, but in terms of fractal idealized shapes:&lt;br /&gt;
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对于光滑的形状，或者有少量棱角的形状，传统几何和科学的形状，豪斯多夫维数是一个整数，与拓扑维度一致。但是伯努·曼德布洛特观察到分形---- 具有非整数豪斯多夫维数的集合---- 在自然界中随处可见。他观察到，我们周围大多数粗糙形状的理想化不是光滑的理想化形状，而是分形理想化形状:&lt;br /&gt;
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&amp;lt;blockquote&amp;gt;Clouds are not spheres, mountains are not cones, coastlines are not circles, and bark is not smooth, nor does lightning travel in a straight line.&amp;lt;ref name=&amp;quot;mandelbrot&amp;quot;&amp;gt;{{cite book   | last = Mandelbrot   | first = Benoît   | authorlink = Benoit Mandelbrot   | title = The Fractal Geometry of Nature   | publisher = W. H. Freeman   | series = Lecture notes in mathematics 1358   | year = 1982   | doi =    | isbn = 0-7167-1186-9   | url-access = registration   | url = https://archive.org/details/fractalgeometryo00beno   }}&amp;lt;/ref&amp;gt;&amp;lt;/blockquote&amp;gt;&lt;br /&gt;
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&amp;lt;blockquote&amp;gt;Clouds are not spheres, mountains are not cones, coastlines are not circles, and bark is not smooth, nor does lightning travel in a straight line.&amp;lt;/blockquote&amp;gt;&lt;br /&gt;
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&amp;lt;blockquote&amp;gt;云不是球体，山不是锥体，海岸线不是圆圈，树皮不平滑，闪电也不是直线运动。 &amp;lt;/blockquote&amp;gt;&lt;br /&gt;
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For fractals that occur in nature, the Hausdorff and [[Minkowski–Bouligand dimension|box-counting dimension]] coincide. The [[packing dimension]] is yet another similar notion which gives the same value for many shapes, but there are well documented exceptions where all these dimensions differ.&lt;br /&gt;
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For fractals that occur in nature, the Hausdorff and box-counting dimension coincide. The packing dimension is yet another similar notion which gives the same value for many shapes, but there are well documented exceptions where all these dimensions differ.&lt;br /&gt;
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对于自然界中出现的分形，豪斯多夫维数和盒计数维数是一致的。封装尺寸是另一个类似的概念，它为许多形状提供相同的值，但是在所有这些尺寸不同的情况，都做了很好的说明。&lt;br /&gt;
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==Formal definitions形式化定义==&lt;br /&gt;
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{{unreferenced section|date=March 2015}}&lt;br /&gt;
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===Hausdorff content豪斯多夫集===&lt;br /&gt;
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Let ''X'' be a [[metric space]]. If ''S'' ⊂ ''X'' and ''d'' ∈ [0, ∞), the ''d''-dimensional '''unlimited Hausdorff content''' of ''S'' is defined by&lt;br /&gt;
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Let X be a metric space. If S ⊂ X and d ∈ [0, ∞), the d-dimensional unlimited Hausdorff content of S is defined by&lt;br /&gt;
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设 ''X''是度量空间。若''S'' ⊂ ''X'' 和 ''d'' ∈ [0, ∞) ，则 ''S'' 的''d''维无限 豪斯多夫集定义为&lt;br /&gt;
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:&amp;lt;math&amp;gt;C_H^d(S):=\inf\Bigl\{\sum_i r_i^d:\text{ there is a cover of } S\text{ by balls with radii }r_i&amp;gt;0\Bigr\}.&amp;lt;/math&amp;gt;&lt;br /&gt;
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&amp;lt;math&amp;gt;C_H^d(S):=\inf\Bigl\{\sum_i r_i^d:\text{ there is a cover of } S\text{ by balls with radii }r_i&amp;gt;0\Bigr\}.&amp;lt;/math&amp;gt;&lt;br /&gt;
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&amp;lt;math&amp;gt;C_H^d(S):=\inf\Bigl\{\sum_i r_i^d:\text{ there is a cover of } S\text{ by balls with radii }r_i&amp;gt;0\Bigr\}.&amp;lt;/math&amp;gt;&lt;br /&gt;
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In other words, &amp;lt;math&amp;gt;C_H^d(S)&amp;lt;/math&amp;gt; is the [[infimum]] of the set of numbers &amp;lt;math&amp;gt;\delta \geq 0&amp;lt;/math&amp;gt; such that there is some (indexed) collection of [[ball (mathematics)|ball]]s &amp;lt;math&amp;gt;\{B(x_i,r_i):i\in I\}&amp;lt;/math&amp;gt; covering ''S'' with ''r&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;''&amp;amp;nbsp;&amp;gt;&amp;amp;nbsp;0 for each ''i''&amp;amp;nbsp;∈&amp;amp;nbsp;''I'' that satisfies &amp;lt;math&amp;gt;\sum_{i\in I} r_i^d&amp;lt;\delta &amp;lt;/math&amp;gt;. (Here, we use the standard convention that [[infimum|inf&amp;amp;nbsp;Ø&amp;amp;nbsp;=&amp;amp;nbsp;∞]].)&lt;br /&gt;
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In other words, &amp;lt;math&amp;gt;C_H^d(S)&amp;lt;/math&amp;gt; is the infimum of the set of numbers &amp;lt;math&amp;gt;\delta \geq 0&amp;lt;/math&amp;gt; such that there is some (indexed) collection of balls &amp;lt;math&amp;gt;\{B(x_i,r_i):i\in I\}&amp;lt;/math&amp;gt; covering S with r&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;&amp;amp;nbsp;&amp;gt;&amp;amp;nbsp;0 for each i&amp;amp;nbsp;∈&amp;amp;nbsp;I that satisfies &amp;lt;math&amp;gt;\sum_{i\in I} r_i^d&amp;lt;\delta &amp;lt;/math&amp;gt;. (Here, we use the standard convention that inf&amp;amp;nbsp;Ø&amp;amp;nbsp;=&amp;amp;nbsp;∞.)&lt;br /&gt;
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换句话说，&amp;lt;math&amp;gt;C_H^d(S)&amp;lt;/math&amp;gt; 是数字集合&amp;lt;math&amp;gt;\delta \geq 0&amp;lt;/math&amp;gt;的下确界，使得在 ''i''&amp;amp;nbsp;∈&amp;amp;nbsp中存在一些球集合 &amp;lt;math&amp;gt;\{B(x_i,r_i):i\in I\}&amp;lt;/math&amp;gt;  i 包含 s，对于每个 ''r&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;''&amp;amp;nbsp;&amp;gt;&amp;amp;nbsp;0 满足 i 中的和&amp;lt;math&amp;gt;\sum_{i\in I} r_i^d&amp;lt;\delta &amp;lt;/math&amp;gt; (在这里，我们使用inf&amp;amp;nbsp;Ø&amp;amp;nbsp;=&amp;amp;nbsp;∞ 的标准约定)。&lt;br /&gt;
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===Hausdorff measurement豪斯多夫分形测量===&lt;br /&gt;
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The Hausdorff outer measure is different from the unbounded Hausdorf content in that rather than considering all possible coverings of ''S'', we see what happens when the sizes of the balls go to zero. This is  for &amp;lt;math&amp;gt;d \geq 0 &amp;lt;/math&amp;gt;, we define the ''d''-dimensional Hausdorff outer measure of ''S'' as&lt;br /&gt;
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The Hausdorff outer measure is different from the unbounded Hausdorf content in that rather than considering all possible coverings of S, we see what happens when the sizes of the balls go to zero. This is  for &amp;lt;math&amp;gt;d \geq 0 &amp;lt;/math&amp;gt;, we define the d-dimensional Hausdorff outer measure of S as&lt;br /&gt;
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豪斯多夫外测度不同于无界的豪斯多夫，因为我们不考虑 s 的所有可能，我们看到当球的大小变为零时会发生什么。对于 &amp;lt;math&amp;gt;d \geq 0 &amp;lt;/math&amp;gt;，我们定义了  ''S''的 ''d''维豪斯多夫Hausdorff 外测度为&lt;br /&gt;
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:&amp;lt;math&amp;gt; \mathcal{H}^d(S):=\lim_{r \to 0} \inf\Bigl\{\sum_i r_i^d:\text{ there is a cover of } S\text{ by balls with radii } 0 &amp;lt; r_i &amp;lt; r\Bigr\}.&amp;lt;/math&amp;gt;&lt;br /&gt;
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&amp;lt;math&amp;gt; \mathcal{H}^d(S):=\lim_{r \to 0} \inf\Bigl\{\sum_i r_i^d:\text{ there is a cover of } S\text{ by balls with radii } 0 &amp;lt; r_i &amp;lt; r\Bigr\}.&amp;lt;/math&amp;gt;&lt;br /&gt;
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&amp;lt;math&amp;gt; \mathcal{H}^d(S):=\lim_{r \to 0} \inf\Bigl\{\sum_i r_i^d:\text{有一个面} S\text{ 球 } 0 &amp;lt; r_i &amp;lt; r\Bigr\}.&amp;lt;/math&amp;gt;&lt;br /&gt;
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===Hausdorff dimension豪斯多夫维数===&lt;br /&gt;
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The '''Hausdorff dimension''' of ''X'' is defined by&lt;br /&gt;
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The Hausdorff dimension of X is defined by&lt;br /&gt;
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X 的豪斯多夫维数定义为&lt;br /&gt;
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:&amp;lt;math&amp;gt;\dim_{\operatorname{H}}(X):=\inf\{d\ge 0: \mathcal{H}^d(X)=0\}.&amp;lt;/math&amp;gt;&lt;br /&gt;
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&amp;lt;math&amp;gt;\dim_{\operatorname{H}}(X):=\inf\{d\ge 0: \mathcal{H}^d(X)=0\}.&amp;lt;/math&amp;gt;&lt;br /&gt;
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Equivalently, dim&amp;lt;sub&amp;gt;H&amp;lt;/sub&amp;gt;(''X'') may be defined as the [[infimum]] of the set of ''d'' ∈ [0, ∞) such that the ''d''-dimensional [[Hausdorff measure]] of ''X'' is zero. This is the same as the supremum of the set of ''d''&amp;amp;nbsp;∈&amp;amp;nbsp;[0,&amp;amp;nbsp;∞) such that the ''d''-dimensional Hausdorff measure of ''X'' is infinite (except that when this latter set of numbers ''d'' is empty the Hausdorff dimension is zero).&lt;br /&gt;
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Equivalently, dim&amp;lt;sub&amp;gt;H&amp;lt;/sub&amp;gt;(X) may be defined as the infimum of the set of d ∈ [0, ∞) such that the d-dimensional Hausdorff measure of X is zero. This is the same as the supremum of the set of d&amp;amp;nbsp;∈&amp;amp;nbsp;[0,&amp;amp;nbsp;∞) such that the d-dimensional Hausdorff measure of X is infinite (except that when this latter set of numbers d is empty the Hausdorff dimension is zero).&lt;br /&gt;
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等价地，dim &amp;lt;sub&amp;gt;H&amp;lt;/sub&amp;gt;(''X'')可定义为 ''d'' ∈ [0, ∞) 集的下确界，使得''X'' 的''d''-维 [[豪斯多夫测度]] 为零。这与 ''d''&amp;amp;nbsp;∈&amp;amp;nbsp;[0,&amp;amp;nbsp;∞)的集合的上确界相同，因此''X''的 d 维豪斯多夫测度是无限的(除非后一个集合 ''d'' 是空的，豪斯多夫维数为零)。&lt;br /&gt;
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==Examples实例==&lt;br /&gt;
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[[Image:Sierpinski deep.svg|thumb|250px|Dimension of a further [[fractal]] example. The [[Sierpinski triangle]], an object with Hausdorff dimension of log(3)/log(2)≈1.58.&amp;lt;ref name=ClaytonSCTPLS96/&amp;gt;]]&lt;br /&gt;
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Dimension of a further [[fractal example. The Sierpinski triangle, an object with Hausdorff dimension of log(3)/log(2)≈1.58.]]&lt;br /&gt;
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[[Image:谢尔宾斯基三角形 deep.svg|thumb|250px|进一步的[[分形维数]]的例子，进一步的分形维数的例子是谢尔宾斯基三角形，它是一个豪斯多夫维数为log(3)/log(2)≈1.58.&amp;lt;ref name=ClaytonSCTPLS96/&amp;gt;的物体]]&lt;br /&gt;
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* [[Countable set]]s have Hausdorff dimension 0.&amp;lt;ref name=&amp;quot;schleicher&amp;quot;&amp;gt;{{cite journal |last1=Schleicher |first1=Dierk |title=Hausdorff Dimension, Its Properties, and Its Surprises |journal=The American Mathematical Monthly |date=June 2007 |volume=114 |issue=6 |pages=509–528 |doi=10.1080/00029890.2007.11920440 |language=en |issn=0002-9890|arxiv=math/0505099 }}&amp;lt;/ref&amp;gt;&lt;br /&gt;
*[[可数集]]拥有豪斯多夫维数0.&amp;lt;ref name=&amp;quot;schleicher&amp;quot;&amp;gt;{{cite journal |last1=Schleicher |first1=Dierk |title=豪斯多夫维数, Its Properties, and Its Surprises |journal=The American Mathematical Monthly美国数学期刊 |date=June 2007 |volume=114 |issue=6 |pages=509–528 |doi=10.1080/00029890.2007.11920440 |language=en |issn=0002-9890|arxiv=math/0505099 }}&amp;lt;/ref&amp;gt;&lt;br /&gt;
* The [[Euclidean space]] ℝ&amp;lt;sup&amp;gt;''n''&amp;lt;/sup&amp;gt; has Hausdorff dimension ''n'', and the circle '''S'''&amp;lt;sup&amp;gt;1&amp;lt;/sup&amp;gt; has Hausdorff dimension 1.&amp;lt;ref name=&amp;quot;schleicher&amp;quot; /&amp;gt;&lt;br /&gt;
*[[教育空间]] ℝ&amp;lt;sup&amp;gt;''n''&amp;lt;/sup&amp;gt; 有豪斯多夫维数 ''n''，循环'''S'''&amp;lt;sup&amp;gt;1&amp;lt;/sup&amp;gt; 拥有豪斯多夫维数1.&amp;lt;ref name=&amp;quot;schleicher&amp;quot; /&amp;gt;&lt;br /&gt;
* [[Fractal]]s often are spaces whose Hausdorff dimension strictly exceeds the [[topological dimension]].&amp;lt;ref name=&amp;quot;mandelbrot&amp;quot; /&amp;gt; For example, the [[Cantor set]], a zero-dimensional topological space, is a union of two copies of itself, each copy shrunk by a factor 1/3; hence, it can be shown that its Hausdorff dimension is ln(2)/ln(3)&amp;amp;nbsp;≈&amp;amp;nbsp;0.63.&amp;lt;ref&amp;gt;{{cite book | last=Falconer | first = Kenneth |title=Fractal Geometry: Mathematical Foundations and Applications | publisher=[[John Wiley and Sons]] | edition=2nd | year=2003}}&amp;lt;/ref&amp;gt; The [[Sierpinski triangle]] is a union of three copies of itself, each copy shrunk by a factor of&amp;amp;nbsp;1/2; this yields a Hausdorff dimension of ln(3)/ln(2)&amp;amp;nbsp;≈&amp;amp;nbsp;1.58.&amp;lt;ref name=CampbellAnnenberg15/&amp;gt; These Hausdorff dimensions are related to the &amp;quot;critical exponent&amp;quot; of the [[Master theorem (analysis of algorithms)|Master theorem]] for solving [[Recurrence relation|recurrence relations]] in the [[analysis of algorithms]].&lt;br /&gt;
*[[分形]]一般是那些豪斯多夫维数直接超过其拓扑维数的空间。例如[[康托尔集]]是一个o维拓扑空间，由两个自己复制而成，每一个复制品都是原来的三分之一，因此它的豪斯多夫维数是 ln(2)/ln(3)&amp;amp;nbsp;≈&amp;amp;nbsp;0.63。&amp;lt;ref&amp;gt;{{cite book | last=Falconer | first = Kenneth |title=Fractal Geometry: Mathematical Foundations and Applications | publisher=[[John Wiley and Sons]] | edition=2nd | year=2003}}&amp;lt;/ref&amp;gt;一个[[谢尔宾斯基三角]]是他自身三个复制的组合。每一个是原来的&amp;amp;nbsp;1/2，它的豪斯多夫维数ln(3)/ln(2)&amp;amp;nbsp;≈&amp;amp;nbsp;1.58。&amp;lt;ref name=CampbellAnnenberg15/&amp;gt;在递归算法中解决递归关系时，这些豪斯多夫维数与[[算法分析主定理]]的临界指标相联系。&lt;br /&gt;
* [[Space-filling curve]]s like the [[Peano curve]] have the same Hausdorff dimension as the space they fill.&lt;br /&gt;
*[[空间填充曲线]]拥有和他们填充空间同样的豪斯多夫维数，如[[皮亚诺曲线]]。&lt;br /&gt;
* The trajectory of [[Brownian motion]] in dimension 2 and above is conjectured to be Hausdorff dimension 2.&amp;lt;ref&amp;gt;{{cite book | last=Morters | first=Peres | title= Brownian Motion | publisher=[[Cambridge University Press]] | year=2010 }}&amp;lt;/ref&amp;gt;&lt;br /&gt;
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[[image:Great Britain Hausdorff.svg|thumb|250px|Estimating the Hausdorff dimension of the [[How Long Is the Coast of Britain? Statistical Self-Similarity and Fractional Dimension|coast of Great Britain]]]]&lt;br /&gt;
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coast of Great Britain]]&lt;br /&gt;
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[[大不列颠海岸&lt;br /&gt;
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* 刘易斯·弗赖伊·理查森[[Lewis Fry Richardson]] has performed detailed experiments to measure the approximate Hausdorff dimension for various coastlines. His results have varied from 1.02 for the coastline of [[South Africa]] to 1.25 for the west coast of [[Great Britain]].&amp;lt;ref name=&amp;quot;mandelbrot&amp;quot; /&amp;gt;&lt;br /&gt;
*刘易斯·弗赖伊·理查森（Lewis Fry Richardson）已经通过豪斯多夫维数去测量了很多海岸线。它的结果涵盖从1.02的南非海岸线到1.25的大英帝国西海岸模型。]]&lt;br /&gt;
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==Properties of Hausdorff dimension豪斯多夫维数特性==&lt;br /&gt;
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{{refimprove section|date=March 2015}}&lt;br /&gt;
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=== Hausdorff dimension and inductive dimension 豪斯多夫维数和归纳维数===&lt;br /&gt;
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Let ''X'' be an arbitrary [[Separable space|separable]] metric space. There is a [[topology|topological]] notion of [[inductive dimension]] for ''X'' which is defined recursively. It is always an integer (or +∞) and is denoted dim&amp;lt;sub&amp;gt;ind&amp;lt;/sub&amp;gt;(''X'').&lt;br /&gt;
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Let X be an arbitrary separable metric space. There is a topological notion of inductive dimension for X which is defined recursively. It is always an integer (or +∞) and is denoted dim&amp;lt;sub&amp;gt;ind&amp;lt;/sub&amp;gt;(X).&lt;br /&gt;
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设''X'' 是[[任意可分度量空间]]。对于''X'' 有一个递归定义的归纳维数拓扑概念。它总是一个整数(或 + ∞) ，记为dim&amp;lt;sub&amp;gt;ind&amp;lt;/sub&amp;gt;(''X'')。&lt;br /&gt;
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'''Theorem'''. Suppose ''X'' is non-empty. Then &lt;br /&gt;
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Theorem. Suppose X is non-empty. Then &lt;br /&gt;
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'''定理'''：假设''X'' 是非空的, 那么&lt;br /&gt;
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:&amp;lt;math&amp;gt; \dim_{\mathrm{Haus}}(X) \geq \dim_{\operatorname{ind}}(X). &amp;lt;/math&amp;gt;&lt;br /&gt;
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&amp;lt;math&amp;gt; \dim_{\mathrm{Haus}}(X) \geq \dim_{\operatorname{ind}}(X). &amp;lt;/math&amp;gt;&lt;br /&gt;
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Moreover,&lt;br /&gt;
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Moreover,&lt;br /&gt;
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此外,&lt;br /&gt;
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&amp;lt;math&amp;gt; \inf_Y \dim_{\operatorname{Haus}}(Y) =\dim_{\operatorname{ind}}(X), &amp;lt;/math&amp;gt;&lt;br /&gt;
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&amp;lt;math&amp;gt; \inf_Y \dim_{\operatorname{Haus}}(Y) =\dim_{\operatorname{ind}}(X), &amp;lt;/math&amp;gt;&lt;br /&gt;
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where ''Y'' ranges over metric spaces [[homeomorphic]] to ''X''. In other words, ''X'' and ''Y'' have the same underlying set of points and the metric ''d''&amp;lt;sub&amp;gt;''Y''&amp;lt;/sub&amp;gt; of ''Y'' is topologically equivalent to ''d''&amp;lt;sub&amp;gt;''X''&amp;lt;/sub&amp;gt;.&lt;br /&gt;
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where Y ranges over metric spaces homeomorphic to X. In other words, X and Y have the same underlying set of points and the metric d&amp;lt;sub&amp;gt;Y&amp;lt;/sub&amp;gt; of Y is topologically equivalent to d&amp;lt;sub&amp;gt;X&amp;lt;/sub&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
其中''Y''是度量空间同胚到 ''X''的范围。换句话说， ''X''和 ''Y''具有相同的基本点集，''Y''的度量''d''&amp;lt;sub&amp;gt;''Y''&amp;lt;/sub&amp;gt; 拓扑等价于''d''&amp;lt;sub&amp;gt;''X''&amp;lt;/sub&amp;gt;。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
These results were originally established by [[Edward Szpilrajn]] (1907–1976), e.g., see Hurewicz and Wallman, Chapter VII.{{full citation needed|date=March 2015}}&lt;br /&gt;
&lt;br /&gt;
These results were originally established by Edward Szpilrajn (1907–1976), e.g., see Hurewicz and Wallman, Chapter VII.&lt;br /&gt;
&lt;br /&gt;
这些结果最初是由 [[Edward Szpilrajn]] (1907–1976)建立的,  参见 Hurewicz and Wallman, Chapter VII.{{full citation needed|date=March 2015}}第七章。&lt;br /&gt;
&lt;br /&gt;
=== Hausdorff dimension and Minkowski dimension 豪斯多夫维数和闵可夫斯基维度===&lt;br /&gt;
&lt;br /&gt;
The [[Minkowski dimension]] is similar to, and at least as large as, the Hausdorff dimension, and they are equal in many situations. However, the set of [[rational number|rational]] points in [0, 1] has Hausdorff dimension zero and Minkowski dimension one. There are also compact sets for which the Minkowski dimension is strictly larger than the Hausdorff dimension.&lt;br /&gt;
&lt;br /&gt;
The Minkowski dimension is similar to, and at least as large as, the Hausdorff dimension, and they are equal in many situations. However, the set of rational points in [0, 1] has Hausdorff dimension zero and Minkowski dimension one. There are also compact sets for which the Minkowski dimension is strictly larger than the Hausdorff dimension.&lt;br /&gt;
&lt;br /&gt;
[[闵可夫斯基维数]]与豪斯多夫维数相似，至少和它一样大，而且在许多情况下是相等的。然而，[0,1]中有理点集的豪斯多夫维数为0，闵可夫斯基维数为1。还有一些紧集的闵可夫斯基维数严格大于豪斯多夫维数。&lt;br /&gt;
&lt;br /&gt;
=== Hausdorff dimensions and Frostman measures 豪斯多夫维度和弗洛斯曼测度===&lt;br /&gt;
&lt;br /&gt;
If there is a [[measure (mathematics)|measure]] μ defined on [[Borel measure|Borel]] subsets of a metric space ''X'' such that ''μ''(''X'') &amp;gt; 0 and ''μ''(''B''(''x'', ''r'')) ≤ ''r&amp;lt;sup&amp;gt;s&amp;lt;/sup&amp;gt;'' holds for some constant ''s'' &amp;gt; 0 and for every ball ''B''(''x'', ''r'') in ''X'', then dim&amp;lt;sub&amp;gt;Haus&amp;lt;/sub&amp;gt;(''X'') ≥ ''s''. A partial converse is provided by [[Frostman's lemma]].{{citation needed|date=March 2015}}&amp;lt;ref&amp;gt;This Wikipedia article also discusses further useful characterizations of the Hausdorff dimension.{{clarify|date=March 2015}}&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
If there is a measure μ defined on Borel subsets of a metric space X such that μ(X) &amp;gt; 0 and μ(B(x, r)) ≤ r&amp;lt;sup&amp;gt;s&amp;lt;/sup&amp;gt; holds for some constant s &amp;gt; 0 and for every ball B(x, r) in X, then dim&amp;lt;sub&amp;gt;Haus&amp;lt;/sub&amp;gt;(X) ≥ s. A partial converse is provided by Frostman's lemma.&lt;br /&gt;
&lt;br /&gt;
如果在度量空间 ''X'' 的 Borel 子集上定义一个测度 μ，使得''μ''(''X'') &amp;gt; 0 和''μ''(''B''(''x'', ''r'')) ≤ ''r&amp;lt;sup&amp;gt;s&amp;lt;/sup&amp;gt;''，对于某个常数 ''s'' &amp;gt; 0  和 ''X'' 中的每个球 ''B''(''x'', ''r'') 成立，则 dim&amp;lt;sub&amp;gt;Haus&amp;lt;/sub&amp;gt;(''X'') ≥ ''s'' 。 部分逆向转换由弗洛斯曼引理定义。&lt;br /&gt;
&lt;br /&gt;
=== Behaviour under unions and products ===&lt;br /&gt;
&lt;br /&gt;
If &amp;lt;math&amp;gt;X=\bigcup_{i\in I}X_i&amp;lt;/math&amp;gt; is a finite or countable union, then&lt;br /&gt;
&lt;br /&gt;
If &amp;lt;math&amp;gt;X=\bigcup_{i\in I}X_i&amp;lt;/math&amp;gt; is a finite or countable union, then&lt;br /&gt;
&lt;br /&gt;
如果 &amp;lt;math&amp;gt;X=\bigcup_{i\in I}X_i&amp;lt;/math&amp;gt; 是一个有限或可数的联合，则&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \dim_{\operatorname{Haus}}(X) =\sup_{i\in I} \dim_{\operatorname{Haus}}(X_i).&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \dim_{\operatorname{Haus}}(X) =\sup_{i\in I} \dim_{\operatorname{Haus}}(X_i).&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
This can be verified directly from the definition.&lt;br /&gt;
&lt;br /&gt;
This can be verified directly from the definition.&lt;br /&gt;
&lt;br /&gt;
这可以直接从定义得到验证。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
If ''X'' and ''Y'' are non-empty metric spaces, then the Hausdorff dimension of their product satisfies&amp;lt;ref&amp;gt;{{cite journal |author=Marstrand, J. M. |title=The dimension of Cartesian product sets |journal=Proc. Cambridge Philos. Soc. |volume=50 |issue=3 |pages=198–202 |year=1954 |doi=10.1017/S0305004100029236 |bibcode = 1954PCPS...50..198M }}&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
If X and Y are non-empty metric spaces, then the Hausdorff dimension of their product satisfies&lt;br /&gt;
&lt;br /&gt;
如果 ''X'' 和''Y''是非空度量空间，那么它们乘积的豪斯多夫维数满足&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt; \dim_{\operatorname{Haus}}(X\times Y)\ge \dim_{\operatorname{Haus}}(X)+ \dim_{\operatorname{Haus}}(Y).&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \dim_{\operatorname{Haus}}(X\times Y)\ge \dim_{\operatorname{Haus}}(X)+ \dim_{\operatorname{Haus}}(Y).&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
This inequality can be strict. It is possible to find two sets of dimension 0 whose product has dimension 1.&amp;lt;ref&amp;gt;{{cite book  | last = Falconer  | first = Kenneth J.  | title = Fractal geometry. Mathematical foundations and applications  | publisher = John Wiley &amp;amp; Sons, Inc., Hoboken, New Jersey  | year = 2003  | doi =   | isbn = }}&amp;lt;/ref&amp;gt; In the opposite direction, it is known that when ''X'' and ''Y'' are Borel subsets of '''R'''&amp;lt;sup&amp;gt;''n''&amp;lt;/sup&amp;gt;, the Hausdorff dimension of ''X'' × ''Y'' is bounded from above by the Hausdorff dimension of ''X'' plus the [[packing dimension|upper packing dimension]] of ''Y''. These facts are discussed in Mattila (1995).&lt;br /&gt;
&lt;br /&gt;
This inequality can be strict. It is possible to find two sets of dimension 0 whose product has dimension 1. In the opposite direction, it is known that when X and Y are Borel subsets of R&amp;lt;sup&amp;gt;n&amp;lt;/sup&amp;gt;, the Hausdorff dimension of X × Y is bounded from above by the Hausdorff dimension of X plus the upper packing dimension of Y. These facts are discussed in Mattila (1995).&lt;br /&gt;
&lt;br /&gt;
这种不平等可以是严格的。有可能找到两个维数为0的集合，其乘积的维数为1。相反，我们知道当''X''和''Y''是 '''R'''&amp;lt;sup&amp;gt;''n''&amp;lt;/sup&amp;gt;的 Borel 子集时， ''X'' × ''Y''的豪斯多夫维数从上面以 ''X''的豪斯多夫维数加上 ''Y''的上填充维数为界。Mattila (1995)曾就这些情况进行了讨论。&lt;br /&gt;
&lt;br /&gt;
==Self-similar sets自相似集合==&lt;br /&gt;
&lt;br /&gt;
{{refimprove section|date=March 2015}}&lt;br /&gt;
&lt;br /&gt;
Many sets defined by a self-similarity condition have dimensions which can be determined explicitly. Roughly, a set ''E'' is self-similar if it is the fixed point of a set-valued transformation ψ, that is ψ(''E'') = ''E'', although the exact definition is given below.&lt;br /&gt;
&lt;br /&gt;
Many sets defined by a self-similarity condition have dimensions which can be determined explicitly. Roughly, a set E is self-similar if it is the fixed point of a set-valued transformation ψ, that is ψ(E) = E, although the exact definition is given below.&lt;br /&gt;
&lt;br /&gt;
许多由自相似条件定义的集合具有可以显式确定的维数。粗略地说，如果集合''E''是集值ψ变换的不动点，即ψ(''E'') = ''E''， 则它是自相似的，尽管下面给出了确切的定义。&lt;br /&gt;
&lt;br /&gt;
&amp;lt;blockquote&amp;gt;'''Theorem'''. Suppose&lt;br /&gt;
&lt;br /&gt;
&amp;lt;blockquote&amp;gt;Theorem. Suppose&lt;br /&gt;
&lt;br /&gt;
&amp;lt;blockquote&amp;gt;'''定理'''：假设&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt; \psi_i: \mathbf{R}^n \rightarrow \mathbf{R}^n, \quad i=1, \ldots , m &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \psi_i: \mathbf{R}^n \rightarrow \mathbf{R}^n, \quad i=1, \ldots , m &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
are [[Contraction mapping|contractive]] mappings on '''R'''&amp;lt;sup&amp;gt;''n''&amp;lt;/sup&amp;gt; with contraction constant ''r&amp;lt;sub&amp;gt;j&amp;lt;/sub&amp;gt;'' &amp;lt; 1. Then there is a unique ''non-empty'' compact set ''A'' such that&lt;br /&gt;
&lt;br /&gt;
are contractive mappings on R&amp;lt;sup&amp;gt;n&amp;lt;/sup&amp;gt; with contraction constant r&amp;lt;sub&amp;gt;j&amp;lt;/sub&amp;gt; &amp;lt; 1. Then there is a unique non-empty compact set A such that&lt;br /&gt;
&lt;br /&gt;
是'''R'''&amp;lt;sup&amp;gt;''n''&amp;lt;/sup&amp;gt;上的压缩常数''r&amp;lt;sub&amp;gt;j&amp;lt;/sub&amp;gt;'&amp;lt; 1的压缩映射。则有一个唯一的非空紧集A &lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt; A = \bigcup_{i=1}^m \psi_i (A). &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; A = \bigcup_{i=1}^m \psi_i (A). &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&amp;lt;/blockquote&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;/blockquote&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The theorem follows from [[Stefan Banach]]'s [[Contractive mapping theorem|contractive mapping fixed point theorem]] applied to the complete metric space of non-empty compact subsets of '''R'''&amp;lt;sup&amp;gt;''n''&amp;lt;/sup&amp;gt; with the [[Hausdorff distance]].&amp;lt;ref&amp;gt;{{cite book |author=Falconer, K. J. |title=The Geometry of Fractal Sets |publisher=Cambridge University Press |location=Cambridge, UK |year=1985 |isbn=0-521-25694-1 |chapter=Theorem 8.3}}&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
The theorem follows from Stefan Banach's contractive mapping fixed point theorem applied to the complete metric space of non-empty compact subsets of R&amp;lt;sup&amp;gt;n&amp;lt;/sup&amp;gt; with the Hausdorff distance.&lt;br /&gt;
&lt;br /&gt;
这个定理来源于 Stefan Banach 的压缩映射不动点定理，该定理应用于 具有豪斯多夫距离的'''R'''&amp;lt;sup&amp;gt;''n''&amp;lt;/sup&amp;gt; 的非空紧子集的完整度量空间。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
===The open set condition开集条件===&lt;br /&gt;
&lt;br /&gt;
To determine the dimension of the self-similar set ''A'' (in certain cases), we need a technical condition called the ''open set condition'' (OSC) on the sequence of contractions ψ&amp;lt;sub&amp;gt;''i''&amp;lt;/sub&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
To determine the dimension of the self-similar set A (in certain cases), we need a technical condition called the open set condition (OSC) on the sequence of contractions ψ&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
为了确定自相似集''A'' 的维数(在某些情况下) ，我们需要一个关于收缩序列的称为''开集条件''(OSC)的技术条件ψ&amp;lt;sub&amp;gt;''i''&amp;lt;/sub&amp;gt;。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
There is a relatively compact open set ''V'' such that&lt;br /&gt;
&lt;br /&gt;
There is a relatively compact open set V such that&lt;br /&gt;
&lt;br /&gt;
有一个相对紧的开集''V''&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt; \bigcup_{i=1}^m\psi_i (V) \subseteq V, &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \bigcup_{i=1}^m\psi_i (V) \subseteq V, &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
where the sets in union on the left are pairwise [[disjoint sets|disjoint]].&lt;br /&gt;
&lt;br /&gt;
where the sets in union on the left are pairwise disjoint.&lt;br /&gt;
&lt;br /&gt;
左边并集的集合成对不相交。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The open set condition is a separation condition that ensures the images ψ&amp;lt;sub&amp;gt;''i''&amp;lt;/sub&amp;gt;(''V'') do not overlap &amp;quot;too much&amp;quot;.&lt;br /&gt;
&lt;br /&gt;
The open set condition is a separation condition that ensures the images ψ&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;(V) do not overlap &amp;quot;too much&amp;quot;.&lt;br /&gt;
&lt;br /&gt;
开集条件是保证图像ψ&amp;lt;sub&amp;gt;''i''&amp;lt;/sub&amp;gt;(''V'') 不重叠“太多”的分离条件。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
'''Theorem'''. Suppose the open set condition holds and each ψ&amp;lt;sub&amp;gt;''i''&amp;lt;/sub&amp;gt; is a similitude, that is a composition of an [[isometry]] and a [[dilation (metric space)|dilation]] around some point. Then the unique fixed point of ψ is a set whose Hausdorff dimension is ''s'' where ''s'' is the unique solution of&amp;lt;ref&amp;gt;{{cite journal | last=Hutchinson | first=John E. | title=Fractals and self similarity | journal=Indiana Univ. Math. J. | volume=30 | year=1981 | pages=713–747 | doi=10.1512/iumj.1981.30.30055 | issue=5 | doi-access=free }}&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
Theorem. Suppose the open set condition holds and each ψ&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt; is a similitude, that is a composition of an isometry and a dilation around some point. Then the unique fixed point of ψ is a set whose Hausdorff dimension is s where s is the unique solution of&lt;br /&gt;
&lt;br /&gt;
'''定理'''假设开集条件成立，并且每个ψ&amp;lt;sub&amp;gt;''i''&amp;lt;/sub&amp;gt; 是一个相似度，即等距和某个点周围的膨胀的组合。。那么唯一的不动点是Hausdorff维数为 ''s'' 的集合，其中  ''s'' 是 ''s'' &amp;lt;ref&amp;gt;{{cite journal | last=Hutchinson | first=John E. | title=Fractals and self similarity | journal=Indiana Univ. Math. J. | volume=30 | year=1981 | pages=713–747 | doi=10.1512/iumj.1981.30.30055 | issue=5 | doi-access=free }}&amp;lt;/ref&amp;gt;的唯一解&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt; \sum_{i=1}^m r_i^s = 1. &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \sum_{i=1}^m r_i^s = 1. &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The contraction coefficient of a similitude is the magnitude of the dilation.&lt;br /&gt;
&lt;br /&gt;
The contraction coefficient of a similitude is the magnitude of the dilation.&lt;br /&gt;
&lt;br /&gt;
相似物的收缩系数就是膨胀的大小。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
We can use this theorem to compute the Hausdorff dimension of the Sierpinski triangle (or sometimes called Sierpinski gasket). Consider three [[non-collinear points]] ''a''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;, ''a''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;, ''a''&amp;lt;sub&amp;gt;3&amp;lt;/sub&amp;gt; in the plane '''R'''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; and let ψ&amp;lt;sub&amp;gt;''i''&amp;lt;/sub&amp;gt; be the dilation of ratio 1/2 around ''a&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;''. The unique non-empty fixed point of the corresponding mapping ψ is a Sierpinski gasket and the dimension ''s'' is the unique solution of&lt;br /&gt;
&lt;br /&gt;
We can use this theorem to compute the Hausdorff dimension of the Sierpinski triangle (or sometimes called Sierpinski gasket). Consider three non-collinear points a&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;, a&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;, a&amp;lt;sub&amp;gt;3&amp;lt;/sub&amp;gt; in the plane R&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; and let ψ&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt; be the dilation of ratio 1/2 around a&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;. The unique non-empty fixed point of the corresponding mapping ψ is a Sierpinski gasket and the dimension s is the unique solution of&lt;br /&gt;
&lt;br /&gt;
我们可以使用这个定理来计算谢尔宾斯基三角形的豪斯多夫维数(或者有时候叫做谢尔宾斯基垫圈)。考虑R&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; 平面上的三个非共线点，''a''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;，''a''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;，''a''&amp;lt;sub&amp;gt;3&amp;lt;/sub&amp;gt;，让ψ&amp;lt;sub&amp;gt;''i''&amp;lt;/sub&amp;gt;是围绕着''a&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;''比率1/2的膨胀。对应映射的唯一非空不动点是一个谢尔宾斯基垫圈，其维数''s''是对应映射的唯一解&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt; \left(\frac{1}{2}\right)^s+\left(\frac{1}{2}\right)^s+\left(\frac{1}{2}\right)^s = 3 \left(\frac{1}{2}\right)^s =1. &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \left(\frac{1}{2}\right)^s+\left(\frac{1}{2}\right)^s+\left(\frac{1}{2}\right)^s = 3 \left(\frac{1}{2}\right)^s =1. &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Taking [[natural logarithm]]s of both sides of the above equation, we can solve for ''s'', that is: ''s'' = ln(3)/ln(2).  The Sierpinski gasket is self-similar and satisfies the OSC. In general a set ''E'' which is a fixed point of a mapping&lt;br /&gt;
&lt;br /&gt;
Taking natural logarithms of both sides of the above equation, we can solve for s, that is: s = ln(3)/ln(2).  The Sierpinski gasket is self-similar and satisfies the OSC. In general a set E which is a fixed point of a mapping&lt;br /&gt;
&lt;br /&gt;
取上述方程两边的自然对数，我们可以求出 ''s''，即: ''s'' = ln(3)/ln(2)。该密封垫具有自相似性，满足 OSC 要求。一般来说，集合 ''E''是一个映射的不动点&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt; A \mapsto \psi(A) = \bigcup_{i=1}^m \psi_i(A) &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt; A \mapsto \psi(A) = \bigcup_{i=1}^m \psi_i(A) &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
is self-similar if and only if the intersections&lt;br /&gt;
&lt;br /&gt;
is self-similar if and only if the intersections&lt;br /&gt;
&lt;br /&gt;
是自相似的，当且仅当&lt;br /&gt;
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:&amp;lt;math&amp;gt; H^s\left(\psi_i(E) \cap \psi_j(E)\right) =0, &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; H^s\left(\psi_i(E) \cap \psi_j(E)\right) =0, &amp;lt;/math&amp;gt;&lt;br /&gt;
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where ''s'' is the Hausdorff dimension of ''E'' and ''H&amp;lt;sup&amp;gt;s&amp;lt;/sup&amp;gt;'' denotes [[Hausdorff measure]]. This is clear in the case of the Sierpinski gasket (the intersections are just points), but is also true more generally:&lt;br /&gt;
&lt;br /&gt;
where s is the Hausdorff dimension of E and H&amp;lt;sup&amp;gt;s&amp;lt;/sup&amp;gt; denotes Hausdorff measure. This is clear in the case of the Sierpinski gasket (the intersections are just points), but is also true more generally:&lt;br /&gt;
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其中 ''s''是''E''的豪斯多夫维数， ''H&amp;lt;sup&amp;gt;s&amp;lt;/sup&amp;gt;'' 表示 豪斯多夫测度。对于谢尔宾斯基垫圈(交叉点就是点)来说，这一点很明显，但更普遍的情况是:&lt;br /&gt;
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'''Theorem'''. Under the same conditions as the previous theorem, the unique fixed point of ψ is self-similar.&lt;br /&gt;
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Theorem. Under the same conditions as the previous theorem, the unique fixed point of ψ is self-similar.&lt;br /&gt;
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'''定理'''：在与前一定理相同的条件下，其唯一不动点是自相似的。&lt;br /&gt;
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==See also参阅==&lt;br /&gt;
&lt;br /&gt;
* [[List of fractals by Hausdorff dimension豪斯多夫分形维数列表]] Examples of deterministic fractals, random and natural fractals.确定性分形与随机和自然分形的示例。&lt;br /&gt;
&lt;br /&gt;
* [[Assouad dimension  Assouad维数]], another variation of fractal dimension that, like Hausdorff dimension, is defined using coverings by balls其他被球覆盖方式定义的分形维数，例如豪斯多夫维数。&lt;br /&gt;
&lt;br /&gt;
* [[Intrinsic dimension固有维数]]&lt;br /&gt;
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* [[Packing dimension填充维数]]&lt;br /&gt;
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* [[Fractal dimension分形维数]]&lt;br /&gt;
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==References参考文献==&lt;br /&gt;
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{{reflist}}&lt;br /&gt;
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==Further reading拓展阅读==&lt;br /&gt;
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* {{cite book |last1=Dodson |first1=M. Maurice |title=Fractal Geometry and Applications: A Jubilee of Benoît Mandelbrot |volume=72 |issue=1 |pages=305–347 |last2=Kristensen |first2=Simon |chapter=Hausdorff Dimension and Diophantine Approximation |date=June 12, 2003 |arxiv=math/0305399 |bibcode = 2003math......5399D |doi=10.1090/pspum/072.1/2112110|series=Proceedings of Symposia in Pure Mathematics |isbn=9780821836378 }}&lt;br /&gt;
&lt;br /&gt;
* {{cite book |last1=Hurewicz |first1=Witold |authorlink1=Witold Hurewicz |last2=Wallman |first2=Henry |authorlink2=Henry Wallman |title=Dimension Theory |url=https://archive.org/details/in.ernet.dli.2015.84609 |publisher=Princeton University Press |year=1948 }}&lt;br /&gt;
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* {{cite journal |author作者=E. Szpilrajn |authorlink=Edward Marczewski |title=La dimension et la mesure |journal=Fundamenta Mathematicae |volume=28 |pages=81–9 |year=1937 }}&lt;br /&gt;
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* {{cite journal&lt;br /&gt;
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 | last1=Marstrand&lt;br /&gt;
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 | last1=Marstrand&lt;br /&gt;
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 | last1=马斯特兰德&lt;br /&gt;
&lt;br /&gt;
 | first1=J. M. | title=The dimension of cartesian product sets | year=1954 | journal=Proc. Cambridge Philos. Soc.&lt;br /&gt;
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 | first1=J. M. | title=The dimension of cartesian product sets | year=1954 | journal=Proc. Cambridge Philos. Soc.&lt;br /&gt;
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 | first1= J. M. | title=笛卡儿积集的维数 | 1954年 |  journal=Proc. Cambridge Philos. Soc.&lt;br /&gt;
&lt;br /&gt;
 | volume=50&lt;br /&gt;
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 | volume=50&lt;br /&gt;
&lt;br /&gt;
 | 第50卷&lt;br /&gt;
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 | issue=3&lt;br /&gt;
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 | issue=3&lt;br /&gt;
&lt;br /&gt;
 | 第三期&lt;br /&gt;
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 | pages=198–202&lt;br /&gt;
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 | pages=198–202&lt;br /&gt;
&lt;br /&gt;
 | 第198-202页&lt;br /&gt;
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 | doi=10.1017/S0305004100029236|bibcode = 1954PCPS...50..198M }}&lt;br /&gt;
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 | doi=10.1017/S0305004100029236|bibcode = 1954PCPS...50..198M }}&lt;br /&gt;
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10.1017 / S0305004100029236 | bibcode 1954PCPS... 50. . 198 m }&lt;br /&gt;
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* {{Cite book&lt;br /&gt;
&lt;br /&gt;
 | last1=Mattila&lt;br /&gt;
&lt;br /&gt;
 | last1=Mattila&lt;br /&gt;
&lt;br /&gt;
 | last1=Mattila&lt;br /&gt;
&lt;br /&gt;
 | first1=Pertti | author1-link=Pertti Mattila| title=Geometry of sets and measures in Euclidean spaces | publisher=[[Cambridge University Press]]&lt;br /&gt;
&lt;br /&gt;
 | first1=Pertti | author1-link=Pertti Mattila| title=Geometry of sets and measures in Euclidean spaces | publisher=Cambridge University Press&lt;br /&gt;
&lt;br /&gt;
| first1 Pertti | author1-link Pertti Mattila | title 欧几里德空间中集合和度量的几何 | 出版商剑桥大学出版社&lt;br /&gt;
&lt;br /&gt;
 | isbn=978-0-521-65595-8 | year=1995}}&lt;br /&gt;
&lt;br /&gt;
 | isbn=978-0-521-65595-8 | year=1995}}&lt;br /&gt;
&lt;br /&gt;
| isbn 978-0-521-65595-8 | year 1995}&lt;br /&gt;
&lt;br /&gt;
* {{cite journal |author=A. S. Besicovitch |authorlink=A. S. Besicovitch |title=On Linear Sets of Points of Fractional Dimensions |journal=[[Mathematische Annalen]] |volume=101 |year=1929 | doi=10.1007/BF01454831| issue=1 |pages= 161–193}}&lt;br /&gt;
&lt;br /&gt;
* {{cite journal |author1=A. S. Besicovitch |authorlink1=A. S. Besicovitch |author2=H. D. Ursell |authorlink2=H. D. Ursell |title=Sets of Fractional Dimensions |journal=Journal of the London Mathematical Society |volume=12 |year=1937 | issue=1 | doi=10.1112/jlms/s1-12.45.18  | pages=18–25 }}&amp;lt;br/&amp;gt;Several selections from this volume are reprinted in {{cite book |author=Edgar, Gerald A. |title=Classics on fractals |publisher=Addison-Wesley |location=Boston |year=1993 |isbn=0-201-58701-7}} See chapters 9,10,11&lt;br /&gt;
&lt;br /&gt;
* {{cite journal |author=F. Hausdorff |authorlink=F. Hausdorff |title=Dimension und äußeres Maß |journal=Mathematische Annalen |volume=79 |issue=1–2 |pages=157–179 |date=March 1919 |doi=10.1007/BF01457179|hdl=10338.dmlcz/100363 |url=http://dml.cz/bitstream/handle/10338.dmlcz/100363/CzechMathJ_09-1959-3_5.pdf }}&lt;br /&gt;
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* {{cite journal | last=Hutchinson | first=John E. | title=Fractals and self similarity | journal=Indiana Univ. Math. J. | volume=30 | year=1981 | pages=713–747 | doi=10.1512/iumj.1981.30.30055 | issue=5 | doi-access=free }}&lt;br /&gt;
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*{{cite book | last=Falconer | first = Kenneth |title=Fractal Geometry: Mathematical Foundations and Applications | publisher=[[John Wiley and Sons]] | edition=2nd | year=2003}}&lt;br /&gt;
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==External links外部链接==&lt;br /&gt;
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* [https://www.encyclopediaofmath.org/index.php/Hausdorff_dimension Hausdorff dimension] 在 [https://www.encyclopediaofmath.org/ Encyclopedia of Mathematics]&lt;br /&gt;
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* [https://www.encyclopediaofmath.org/index.php/Hausdorff_measure Hausdorff measure] 在 [https://www.encyclopediaofmath.org/ Encyclopedia of Mathematics]&lt;br /&gt;
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{{DEFAULTSORT:Hausdorff Dimension豪斯多夫维数}}&lt;br /&gt;
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[[Category分类:Fractals分形]]&lt;br /&gt;
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[[Category分类:Metric geometry度量几何]]&lt;br /&gt;
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[[Category分类:Dimension theory维度理论]]&lt;br /&gt;
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&amp;lt;small&amp;gt;This page was moved from [[wikipedia:en:Hausdorff dimension]]. Its edit history can be viewed at [[分形维数/edithistory]]&amp;lt;/small&amp;gt;&amp;lt;/noinclude&amp;gt;&lt;br /&gt;
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[[Category:待整理页面]]&lt;/div&gt;</summary>
		<author><name>Ruili</name></author>
	</entry>
	<entry>
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		<title>分形维数</title>
		<link rel="alternate" type="text/html" href="https://wiki.swarma.org/index.php?title=%E5%88%86%E5%BD%A2%E7%BB%B4%E6%95%B0&amp;diff=17747"/>
		<updated>2020-11-01T18:11:03Z</updated>

		<summary type="html">&lt;p&gt;Ruili：&lt;/p&gt;
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&lt;div&gt;此词条暂由彩云小译翻译，未经人工整理和审校，带来阅读不便，请见谅。&lt;br /&gt;
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{{short description|Invariant}}&lt;br /&gt;
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Example of non-integer dimensions. The first four [[iteration]]s of the [[Koch snowflake|Koch curve]], where after each iteration, all original line segments are replaced with four, each a self-similar copy that is 1/3 the length of the original. One formalism of the Hausdorff dimension uses this scale factor (3) and the number of self-similar objects (4) to calculate the dimension, D, after the first iteration to be D = (log N)/(log S) = (log 4)/(log 3) ≈ 1.26.&amp;lt;ref name=CampbellAnnenberg15&amp;gt;MacGregor Campbell, 2013, &amp;quot;5.6 Scaling and the Hausdorff Dimension,&amp;quot; at ''Annenberg Learner:MATHematics illuminated'', see [http://www.learner.org/courses/mathilluminated/units/5/textbook/06.php], accessed 5 March 2015.&amp;lt;/ref&amp;gt; That is, while the Hausdorff dimension of a single [[point (geometry)|point]] is zero, of a [[line segment]] is 1, of a [[square]] is 2, and of a [[cube]] is 3, for [[fractal]]s such as this, the object can have a non-integer dimension.&lt;br /&gt;
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Example of non-integer dimensions. The first four iterations of the Koch curve, where after each iteration, all original line segments are replaced with four, each a self-similar copy that is 1/3 the length of the original. One formalism of the Hausdorff dimension uses this scale factor (3) and the number of self-similar objects (4) to calculate the dimension, D, after the first iteration to be D = (log N)/(log S) = (log 4)/(log 3) ≈ 1.26. That is, while the Hausdorff dimension of a single point is zero, of a line segment is 1, of a square is 2, and of a cube is 3, for fractals such as this, the object can have a non-integer dimension.&lt;br /&gt;
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非整数维度示例：前四个[[Koch 曲线]]的迭代，在每次迭代后，所有原始线段都被替换为四个，每个自相似的复制是原始线段长度的1 / 3。豪斯多夫维数的一个建模是使用比例因子(3)和自相似对象的数量(4)来计算维度 D，在第一次迭代后为 D = (log N)/(log S) = (log 4)/(log 3) ≈ 1.26.&amp;lt;ref name=CampbellAnnenberg15&amp;gt;。MacGregor Campbell, 2013, &amp;quot;5.6 Scaling and the Hausdorff Dimension,&amp;quot; 在 ''Annenberg Learner:MATHematics illuminated'', 参见 [http://www.learner.org/courses/mathilluminated/units/5/textbook/06.php], accessed 5 March 2015.&amp;lt;/ref&amp;gt; 也就是说，单点的豪斯多夫维数为零，线段为1，正方形为2，立方体为3时，但对于分形，对象可以有一个非整数维度。&lt;br /&gt;
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In [[mathematics]], '''Hausdorff dimension''' is a measure of ''roughness'', or more specifically, [[fractal dimension]], that was first introduced in 1918 by [[mathematician]] [[Felix Hausdorff]].&amp;lt;ref&amp;gt;{{Cite journal |arxiv = 1101.1444|doi = 10.1214/11-STS370|title = Estimators of Fractal Dimension: Assessing the Roughness of Time Series and Spatial Data|journal = Statistical Science|volume = 27|issue = 2|pages = 247–277|year = 2012|last1 = Gneiting|first1 = Tilmann|last2 = Ševčíková|first2 = Hana|last3 = Percival|first3 = Donald B.}}&amp;lt;/ref&amp;gt; For instance, the Hausdorff dimension of a single [[point (geometry)|point]] is zero, of a [[line segment]] is 1, of a [[square]] is 2, and of a [[cube]] is 3. That is, for sets of points that define a smooth shape or a shape that has a small number of corners—the shapes of traditional geometry and science—the Hausdorff dimension is an [[integer]] agreeing with the usual sense of dimension, also known as the [[Inductive dimension|topological dimension]]. However, formulas have also been developed that allow calculation of the dimension of other less simple objects, where, solely on the basis of their properties of [[scaling (geometry)|scaling]] and [[self-similarity]], one is led to the conclusion that particular objects—including [[fractal]]s—have non-integer Hausdorff dimensions. Because of the significant technical advances made by [[Abram Samoilovitch Besicovitch]] allowing computation of dimensions for highly irregular or &amp;quot;rough&amp;quot; sets, this dimension is also commonly referred to as the ''Hausdorff–Besicovitch dimension.''&lt;br /&gt;
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In mathematics, Hausdorff dimension is a measure of roughness, or more specifically, fractal dimension, that was first introduced in 1918 by mathematician Felix Hausdorff. For instance, the Hausdorff dimension of a single point is zero, of a line segment is 1, of a square is 2, and of a cube is 3. That is, for sets of points that define a smooth shape or a shape that has a small number of corners—the shapes of traditional geometry and science—the Hausdorff dimension is an integer agreeing with the usual sense of dimension, also known as the topological dimension. However, formulas have also been developed that allow calculation of the dimension of other less simple objects, where, solely on the basis of their properties of scaling and self-similarity, one is led to the conclusion that particular objects—including fractals—have non-integer Hausdorff dimensions. Because of the significant technical advances made by Abram Samoilovitch Besicovitch allowing computation of dimensions for highly irregular or &amp;quot;rough&amp;quot; sets, this dimension is also commonly referred to as the Hausdorff–Besicovitch dimension.&lt;br /&gt;
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在[[数学]]中，'''&amp;lt;font color = '#ff8000'&amp;gt;豪斯多夫维数Hausdorff dimension&amp;lt;/font&amp;gt;'''是一种粗糙度的度量单位，或者更确切地说，分形维数，是由数学家 Felix Hausdorff 在1918年首次提出的。例如，单点的豪斯多夫维数为零，线段为1，正方形为2，立方体为3。也就是说，对于定义了一个光滑形状或一个有少数几个角的形状---- 传统几何学和科学的形状---- 的点集来说，豪斯多夫维数是一个整数，符合通常的维度意义，也称为拓扑维度。然而，还有一些公式允许计算其他不太简单的对象的维数，其中仅仅根据它们的标度和自相似特性，就可以得出结论: 特定的对象ー包括分形ー具有非整数的 Hausdorff 维数。由于阿布拉姆·萨莫伊洛维奇·贝西科维奇的重大技术进步，允许计算高度不规则或“粗糙”集的维度，这个维度通常也被称为 Hausdorff-Besicovitch 维度。 &lt;br /&gt;
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The Hausdorff dimension, more specifically, is a further dimensional number associated with a given set, where the distances between all members of that set are defined. Such a set is termed a [[metric space]]. The dimension is drawn from the [[Extended real number line|extended real numbers]], &amp;lt;math&amp;gt;\overline{\mathbb{R}}&amp;lt;/math&amp;gt;, as opposed to the more intuitive notion of dimension, which is not associated to general metric spaces, and only takes values in the non-negative integers.&lt;br /&gt;
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The Hausdorff dimension, more specifically, is a further dimensional number associated with a given set, where the distances between all members of that set are defined. Such a set is termed a metric space. The dimension is drawn from the extended real numbers, &amp;lt;math&amp;gt;\overline{\mathbb{R}}&amp;lt;/math&amp;gt;, as opposed to the more intuitive notion of dimension, which is not associated to general metric spaces, and only takes values in the non-negative integers.&lt;br /&gt;
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更具体地说，豪斯多夫维数是一个与给定集合相关联的更进一步的维数，其中定义了该集合所有成员之间的距离。这样的集合称为度量空间。维数是从扩展的实数，&amp;lt;math&amp;gt;\overline{\mathbb{R}}&amp;lt;/math&amp;gt;，而不是更直观的维数概念(它不与一般的度量空间相关联，只取非负整数的值)。&lt;br /&gt;
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In mathematical terms, the Hausdorff dimension generalizes the notion of the dimension of a real [[vector space]]. That is, the Hausdorff dimension of an ''n''-dimensional [[inner product space]] equals ''n''. This underlies the earlier statement that the Hausdorff dimension of a point is zero, of a line is one, etc., and that [[fractal|irregular sets]] can have noninteger Hausdorff dimensions. For instance, the [[Koch snowflake]] shown at right is constructed from an equilateral triangle; in each iteration, its component line segments are divided into 3 segments of unit length, the newly created middle segment is used as the base of a new [[equilateral]] triangle that points outward, and this base segment is then deleted to leave a final object from the iteration of unit length of 4.&amp;lt;ref&amp;gt;Larry Riddle, 2014, &amp;quot;Classic Iterated Function Systems: Koch Snowflake&amp;quot;, Agnes Scott College e-Academy (online), see [http://ecademy.agnesscott.edu/~lriddle/ifs/ksnow/ksnow.htm], accessed 5 March 2015.&amp;lt;/ref&amp;gt; That is, after the first iteration, each original line segment has been replaced with N=4, where each self-similar copy is 1/S = 1/3 as long as the original.&amp;lt;ref name=CampbellAnnenberg15/&amp;gt; Stated another way, we have taken an object with Euclidean dimension, D, and reduced its linear scale by 1/3 in each direction, so that its length increases to N=S&amp;lt;sup&amp;gt;D&amp;lt;/sup&amp;gt;.&amp;lt;ref name=ClaytonSCTPLS96&amp;gt;Keith Clayton, 1996, &amp;quot;Fractals and the Fractal Dimension,&amp;quot; ''Basic Concepts in Nonlinear Dynamics and Chaos'' (workshop), Society for Chaos Theory in Psychology and the Life Sciences annual meeting, June 28, 1996, Berkeley, California, see [http://www.vanderbilt.edu/AnS/psychology/cogsci/chaos/workshop/Workshop.html], accessed 5 March 2015.&amp;lt;/ref&amp;gt; This equation is easily solved for D, yielding the ratio of logarithms (or [[natural logarithm]]s) appearing in the figures, and giving—in the Koch and other fractal cases—non-integer dimensions for these objects.&lt;br /&gt;
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In mathematical terms, the Hausdorff dimension generalizes the notion of the dimension of a real vector space. That is, the Hausdorff dimension of an n-dimensional inner product space equals n. This underlies the earlier statement that the Hausdorff dimension of a point is zero, of a line is one, etc., and that irregular sets can have noninteger Hausdorff dimensions. For instance, the Koch snowflake shown at right is constructed from an equilateral triangle; in each iteration, its component line segments are divided into 3 segments of unit length, the newly created middle segment is used as the base of a new equilateral triangle that points outward, and this base segment is then deleted to leave a final object from the iteration of unit length of 4. That is, after the first iteration, each original line segment has been replaced with N=4, where each self-similar copy is 1/S = 1/3 as long as the original. This equation is easily solved for D, yielding the ratio of logarithms (or natural logarithms) appearing in the figures, and giving—in the Koch and other fractal cases—non-integer dimensions for these objects.&lt;br /&gt;
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用数学术语来说，豪斯多夫维数概括了实向量空间维数的概念。也就是说，n 维内积空间的豪斯多夫维数等于 n。 这就是早期假设的基础，一个点的豪斯多夫维数是零，一条线是一等等，不规则集可以有非整数的豪斯多夫维数。例如，右边所示的 Koch 雪花是由一个正三角形构成的; 在每次迭代中，它的组成线段被分成单位长度的3段，新创建的中间线段被用作一个指向外部的新正三角形的基础，然后人们删除这个基础线段用来保留单位长度4的迭代中的最终对象。也就是说，在第一次迭代之后，每个原始线段都被替换为 N=4，其中每个自相似拷贝的长度是原始线段的1/S = 1/3 。这个方程很容易求解为 D，产生出现在图形中的对数(或自然对数)的比率，并给出——在 Koch 和其他分形情况下——这些对象的非整数维数。&lt;br /&gt;
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The Hausdorff dimension is a successor to the simpler, but usually equivalent, box-counting or [[Minkowski–Bouligand dimension]].&lt;br /&gt;
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The Hausdorff dimension is a successor to the simpler, but usually equivalent, box-counting or Minkowski–Bouligand dimension.&lt;br /&gt;
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豪斯多夫维数是更简单但通常等价的'''&amp;lt;font color = '#ff8000'&amp;gt;计盒维数box-counting&amp;lt;/font&amp;gt;'''或'''&amp;lt;font color = '#ff8000'&amp;gt;闵可夫斯基维数Minkowski-Bouligand&amp;lt;/font&amp;gt;'''的继承者。&lt;br /&gt;
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==Intuition概念==&lt;br /&gt;
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The intuitive concept of dimension of a geometric object ''X'' is the number of independent parameters one needs to pick out a unique point inside. However, any point specified by two parameters can be instead specified by one, because the [[cardinality]] of the [[real plane]] is equal to the cardinality of the [[real line]] (this can be seen by an [[Cantor's diagonal argument|argument]] involving interweaving the digits of two numbers to yield a single number encoding the same information). The example of a [[space-filling curve]] shows that one can even map the real line to the real plane [[Surjective function|surjectively]] (taking one real number into a pair of real numbers in a way so that all pairs of numbers are covered) and ''continuously'', so that a one-dimensional object completely fills up a higher-dimensional object.&lt;br /&gt;
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The intuitive concept of dimension of a geometric object X is the number of independent parameters one needs to pick out a unique point inside. However, any point specified by two parameters can be instead specified by one, because the cardinality of the real plane is equal to the cardinality of the real line (this can be seen by an argument involving interweaving the digits of two numbers to yield a single number encoding the same information). The example of a space-filling curve shows that one can even map the real line to the real plane surjectively (taking one real number into a pair of real numbers in a way so that all pairs of numbers are covered) and continuously, so that a one-dimensional object completely fills up a higher-dimensional object.&lt;br /&gt;
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几何对象X的尺寸的直观概念是指需要多少个独立参数才能找到一个独特的点。但是，任何由两个参数指定的点都可以由一个参数指定，因为为实平面的基数等于实线的基数(这可以通过交织两个数字以产生一个编码相同信息的单个数字看到)。'''&amp;lt;font color = '#ff8000'&amp;gt;皮亚诺曲线&amp;lt;/font&amp;gt;'''的例子表明，可以将实线完美和连续地映射到实平面(把一个实数转换成一对实数，从而覆盖所有实数对)，由此一维对象完全填充了一个高维对象。&lt;br /&gt;
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Every space filling curve hits some points multiple times, and does not have a continuous inverse. It is impossible to map two dimensions onto one in a way that is continuous and continuously invertible. The topological dimension, also called [[Lebesgue covering dimension]], explains why. This dimension is ''n'' if, in every covering of ''X'' by small open balls, there is at least one point where ''n''&amp;amp;nbsp;+&amp;amp;nbsp;1 balls overlap. For example, when one covers a line with short open intervals, some points must be covered twice, giving dimension&amp;amp;nbsp;''n''&amp;amp;nbsp;=&amp;amp;nbsp;1.&lt;br /&gt;
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Every space filling curve hits some points multiple times, and does not have a continuous inverse. It is impossible to map two dimensions onto one in a way that is continuous and continuously invertible. The topological dimension, also called Lebesgue covering dimension, explains why. This dimension is n if, in every covering of X by small open balls, there is at least one point where n&amp;amp;nbsp;+&amp;amp;nbsp;1 balls overlap. For example, when one covers a line with short open intervals, some points must be covered twice, giving dimension&amp;amp;nbsp;n&amp;amp;nbsp;=&amp;amp;nbsp;1.&lt;br /&gt;
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每条空间填充曲线都会多次击中某些点，且不存在连续的逆。将二维以连续和连续可逆的方式映射到一维是不可能的。'''&amp;lt;font color = '#ff8000'&amp;gt;拓扑维度 topological dimension&amp;lt;/font&amp;gt;'''，也被称为Lebesgue覆盖维数，解释了为什么。如果在 x 的每个小开球覆盖中，至少有一个点 n + 1个球重叠，这个维度是 n。例如，当用短的开区间覆盖一条线时，某些点必须被覆盖两次，给出维数''n''&amp;amp;nbsp;=&amp;amp;nbsp;1。&lt;br /&gt;
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But topological dimension is a very crude measure of the local size of a space (size near a point). A curve that is almost space-filling can still have topological dimension one, even if it fills up most of the area of a region. A [[fractal]] has an integer topological dimension, but in terms of the amount of space it takes up, it behaves like a higher-dimensional space.&lt;br /&gt;
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But topological dimension is a very crude measure of the local size of a space (size near a point). A curve that is almost space-filling can still have topological dimension one, even if it fills up most of the area of a region. A fractal has an integer topological dimension, but in terms of the amount of space it takes up, it behaves like a higher-dimensional space.&lt;br /&gt;
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但是，拓扑维度是对空间局部尺寸(点附近的尺寸)的一个非常粗略的度量。一条几乎是空间填充的曲线仍然可以有一维拓扑，即使它填充了一个区域的大部分面积。分形具有整数的拓扑维数，但就其所占的空间量而言，它看起来像一个更高维的空间。&lt;br /&gt;
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The Hausdorff dimension measures the local size of a space taking into account the distance between points, the [[metric space|metric]]. Consider the number ''N''(''r'') of [[ball (mathematics)|balls]] of radius at most ''r'' required to cover ''X'' completely. When ''r'' is very small, ''N''(''r'') grows polynomially with 1/''r''. For a sufficiently well-behaved  ''X'', the Hausdorff dimension is the unique number ''d'' such that N(''r'') grows as 1/''r&amp;lt;sup&amp;gt;d&amp;lt;/sup&amp;gt;'' as ''r'' approaches zero. More precisely, this defines the [[Minkowski–Bouligand dimension|box-counting dimension]], which equals the Hausdorff dimension when the value ''d'' is a critical boundary between growth rates that are insufficient to cover the space, and growth rates that are overabundant.&lt;br /&gt;
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The Hausdorff dimension measures the local size of a space taking into account the distance between points, the metric. Consider the number N(r) of balls of radius at most r required to cover X completely. When r is very small, N(r) grows polynomially with 1/r. For a sufficiently well-behaved  X, the Hausdorff dimension is the unique number d such that N(r) grows as 1/r&amp;lt;sup&amp;gt;d&amp;lt;/sup&amp;gt; as r approaches zero. More precisely, this defines the box-counting dimension, which equals the Hausdorff dimension when the value d is a critical boundary between growth rates that are insufficient to cover the space, and growth rates that are overabundant.&lt;br /&gt;
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豪斯多夫维数测量一个空间的局部大小时，会考虑到点之间距离的度量。考虑半径最大为 r 的球数 ''N'' (r) ，需要完全覆盖 ''X''。当 r 很小时，n (r)以1/''r'' 增长多项式。对于一个表现足够好的 ''X''，豪斯多夫维数是唯一的数 d，这样当 r 趋近于零时， N(r)增长为1/r&amp;lt;sup&amp;gt;d&amp;lt;/sup&amp;gt; 。更确切地说，这定义了盒子计数维度，当值 d 是不足以覆盖空间的增长率和过度充裕的增长率之间的关键边界时，它等于豪斯多夫维数。&lt;br /&gt;
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For shapes that are smooth, or shapes with a small number of corners, the shapes of traditional geometry and science, the Hausdorff dimension is an integer agreeing with the topological dimension. But [[Benoit Mandelbrot]] observed that [[fractal]]s, sets with noninteger Hausdorff dimensions, are found everywhere in nature. He observed that the proper idealization of most rough shapes you see around you is not in terms of smooth idealized shapes, but in terms of fractal idealized shapes:&lt;br /&gt;
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For shapes that are smooth, or shapes with a small number of corners, the shapes of traditional geometry and science, the Hausdorff dimension is an integer agreeing with the topological dimension. But Benoit Mandelbrot observed that fractals, sets with noninteger Hausdorff dimensions, are found everywhere in nature. He observed that the proper idealization of most rough shapes you see around you is not in terms of smooth idealized shapes, but in terms of fractal idealized shapes:&lt;br /&gt;
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对于光滑的形状，或者有少量棱角的形状，传统几何和科学的形状，豪斯多夫维数是一个整数，与拓扑维度一致。但是伯努·曼德布洛特观察到分形---- 具有非整数豪斯多夫维数的集合---- 在自然界中随处可见。他观察到，我们周围大多数粗糙形状的理想化不是光滑的理想化形状，而是分形理想化形状:&lt;br /&gt;
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&amp;lt;blockquote&amp;gt;Clouds are not spheres, mountains are not cones, coastlines are not circles, and bark is not smooth, nor does lightning travel in a straight line.&amp;lt;ref name=&amp;quot;mandelbrot&amp;quot;&amp;gt;{{cite book   | last = Mandelbrot   | first = Benoît   | authorlink = Benoit Mandelbrot   | title = The Fractal Geometry of Nature   | publisher = W. H. Freeman   | series = Lecture notes in mathematics 1358   | year = 1982   | doi =    | isbn = 0-7167-1186-9   | url-access = registration   | url = https://archive.org/details/fractalgeometryo00beno   }}&amp;lt;/ref&amp;gt;&amp;lt;/blockquote&amp;gt;&lt;br /&gt;
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&amp;lt;blockquote&amp;gt;Clouds are not spheres, mountains are not cones, coastlines are not circles, and bark is not smooth, nor does lightning travel in a straight line.&amp;lt;/blockquote&amp;gt;&lt;br /&gt;
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&amp;lt;blockquote&amp;gt;云不是球体，山不是锥体，海岸线不是圆圈，树皮不平滑，闪电也不是直线运动。 &amp;lt;/blockquote&amp;gt;&lt;br /&gt;
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For fractals that occur in nature, the Hausdorff and [[Minkowski–Bouligand dimension|box-counting dimension]] coincide. The [[packing dimension]] is yet another similar notion which gives the same value for many shapes, but there are well documented exceptions where all these dimensions differ.&lt;br /&gt;
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For fractals that occur in nature, the Hausdorff and box-counting dimension coincide. The packing dimension is yet another similar notion which gives the same value for many shapes, but there are well documented exceptions where all these dimensions differ.&lt;br /&gt;
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对于自然界中出现的分形，豪斯多夫维数和盒计数维数是一致的。封装尺寸是另一个类似的概念，它为许多形状提供相同的值，但是在所有这些尺寸不同的情况，都做了很好的说明。&lt;br /&gt;
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==Formal definitions形式化定义==&lt;br /&gt;
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{{unreferenced section|date=March 2015}}&lt;br /&gt;
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===Hausdorff content豪斯多夫集===&lt;br /&gt;
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Let ''X'' be a [[metric space]]. If ''S'' ⊂ ''X'' and ''d'' ∈ [0, ∞), the ''d''-dimensional '''unlimited Hausdorff content''' of ''S'' is defined by&lt;br /&gt;
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Let X be a metric space. If S ⊂ X and d ∈ [0, ∞), the d-dimensional unlimited Hausdorff content of S is defined by&lt;br /&gt;
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设 ''X''是度量空间。若''S'' ⊂ ''X'' 和 ''d'' ∈ [0, ∞) ，则 ''S'' 的''d''维无限 豪斯多夫集定义为&lt;br /&gt;
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:&amp;lt;math&amp;gt;C_H^d(S):=\inf\Bigl\{\sum_i r_i^d:\text{ there is a cover of } S\text{ by balls with radii }r_i&amp;gt;0\Bigr\}.&amp;lt;/math&amp;gt;&lt;br /&gt;
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&amp;lt;math&amp;gt;C_H^d(S):=\inf\Bigl\{\sum_i r_i^d:\text{ there is a cover of } S\text{ by balls with radii }r_i&amp;gt;0\Bigr\}.&amp;lt;/math&amp;gt;&lt;br /&gt;
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&amp;lt;math&amp;gt;C_H^d(S):=\inf\Bigl\{\sum_i r_i^d:\text{ there is a cover of } S\text{ by balls with radii }r_i&amp;gt;0\Bigr\}.&amp;lt;/math&amp;gt;&lt;br /&gt;
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In other words, &amp;lt;math&amp;gt;C_H^d(S)&amp;lt;/math&amp;gt; is the [[infimum]] of the set of numbers &amp;lt;math&amp;gt;\delta \geq 0&amp;lt;/math&amp;gt; such that there is some (indexed) collection of [[ball (mathematics)|ball]]s &amp;lt;math&amp;gt;\{B(x_i,r_i):i\in I\}&amp;lt;/math&amp;gt; covering ''S'' with ''r&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;''&amp;amp;nbsp;&amp;gt;&amp;amp;nbsp;0 for each ''i''&amp;amp;nbsp;∈&amp;amp;nbsp;''I'' that satisfies &amp;lt;math&amp;gt;\sum_{i\in I} r_i^d&amp;lt;\delta &amp;lt;/math&amp;gt;. (Here, we use the standard convention that [[infimum|inf&amp;amp;nbsp;Ø&amp;amp;nbsp;=&amp;amp;nbsp;∞]].)&lt;br /&gt;
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In other words, &amp;lt;math&amp;gt;C_H^d(S)&amp;lt;/math&amp;gt; is the infimum of the set of numbers &amp;lt;math&amp;gt;\delta \geq 0&amp;lt;/math&amp;gt; such that there is some (indexed) collection of balls &amp;lt;math&amp;gt;\{B(x_i,r_i):i\in I\}&amp;lt;/math&amp;gt; covering S with r&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;&amp;amp;nbsp;&amp;gt;&amp;amp;nbsp;0 for each i&amp;amp;nbsp;∈&amp;amp;nbsp;I that satisfies &amp;lt;math&amp;gt;\sum_{i\in I} r_i^d&amp;lt;\delta &amp;lt;/math&amp;gt;. (Here, we use the standard convention that inf&amp;amp;nbsp;Ø&amp;amp;nbsp;=&amp;amp;nbsp;∞.)&lt;br /&gt;
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换句话说，&amp;lt;math&amp;gt;C_H^d(S)&amp;lt;/math&amp;gt; 是数字集合&amp;lt;math&amp;gt;\delta \geq 0&amp;lt;/math&amp;gt;的下确界，使得在 ''i''&amp;amp;nbsp;∈&amp;amp;nbsp中存在一些球集合 &amp;lt;math&amp;gt;\{B(x_i,r_i):i\in I\}&amp;lt;/math&amp;gt;  i 包含 s，对于每个 ''r&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;''&amp;amp;nbsp;&amp;gt;&amp;amp;nbsp;0 满足 i 中的和&amp;lt;math&amp;gt;\sum_{i\in I} r_i^d&amp;lt;\delta &amp;lt;/math&amp;gt; (在这里，我们使用inf&amp;amp;nbsp;Ø&amp;amp;nbsp;=&amp;amp;nbsp;∞ 的标准约定)。&lt;br /&gt;
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===Hausdorff measurement豪斯多夫分形测量===&lt;br /&gt;
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The Hausdorff outer measure is different from the unbounded Hausdorf content in that rather than considering all possible coverings of ''S'', we see what happens when the sizes of the balls go to zero. This is  for &amp;lt;math&amp;gt;d \geq 0 &amp;lt;/math&amp;gt;, we define the ''d''-dimensional Hausdorff outer measure of ''S'' as&lt;br /&gt;
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The Hausdorff outer measure is different from the unbounded Hausdorf content in that rather than considering all possible coverings of S, we see what happens when the sizes of the balls go to zero. This is  for &amp;lt;math&amp;gt;d \geq 0 &amp;lt;/math&amp;gt;, we define the d-dimensional Hausdorff outer measure of S as&lt;br /&gt;
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豪斯多夫外测度不同于无界的豪斯多夫，因为我们不考虑 s 的所有可能，我们看到当球的大小变为零时会发生什么。对于 &amp;lt;math&amp;gt;d \geq 0 &amp;lt;/math&amp;gt;，我们定义了  ''S''的 ''d''维豪斯多夫Hausdorff 外测度为&lt;br /&gt;
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:&amp;lt;math&amp;gt; \mathcal{H}^d(S):=\lim_{r \to 0} \inf\Bigl\{\sum_i r_i^d:\text{ there is a cover of } S\text{ by balls with radii } 0 &amp;lt; r_i &amp;lt; r\Bigr\}.&amp;lt;/math&amp;gt;&lt;br /&gt;
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&amp;lt;math&amp;gt; \mathcal{H}^d(S):=\lim_{r \to 0} \inf\Bigl\{\sum_i r_i^d:\text{ there is a cover of } S\text{ by balls with radii } 0 &amp;lt; r_i &amp;lt; r\Bigr\}.&amp;lt;/math&amp;gt;&lt;br /&gt;
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&amp;lt;math&amp;gt; \mathcal{H}^d(S):=\lim_{r \to 0} \inf\Bigl\{\sum_i r_i^d:\text{有一个面} S\text{ 球 } 0 &amp;lt; r_i &amp;lt; r\Bigr\}.&amp;lt;/math&amp;gt;&lt;br /&gt;
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===Hausdorff dimension豪斯多夫维数===&lt;br /&gt;
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The '''Hausdorff dimension''' of ''X'' is defined by&lt;br /&gt;
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The Hausdorff dimension of X is defined by&lt;br /&gt;
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X 的豪斯多夫维数定义为&lt;br /&gt;
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:&amp;lt;math&amp;gt;\dim_{\operatorname{H}}(X):=\inf\{d\ge 0: \mathcal{H}^d(X)=0\}.&amp;lt;/math&amp;gt;&lt;br /&gt;
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&amp;lt;math&amp;gt;\dim_{\operatorname{H}}(X):=\inf\{d\ge 0: \mathcal{H}^d(X)=0\}.&amp;lt;/math&amp;gt;&lt;br /&gt;
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Equivalently, dim&amp;lt;sub&amp;gt;H&amp;lt;/sub&amp;gt;(''X'') may be defined as the [[infimum]] of the set of ''d'' ∈ [0, ∞) such that the ''d''-dimensional [[Hausdorff measure]] of ''X'' is zero. This is the same as the supremum of the set of ''d''&amp;amp;nbsp;∈&amp;amp;nbsp;[0,&amp;amp;nbsp;∞) such that the ''d''-dimensional Hausdorff measure of ''X'' is infinite (except that when this latter set of numbers ''d'' is empty the Hausdorff dimension is zero).&lt;br /&gt;
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Equivalently, dim&amp;lt;sub&amp;gt;H&amp;lt;/sub&amp;gt;(X) may be defined as the infimum of the set of d ∈ [0, ∞) such that the d-dimensional Hausdorff measure of X is zero. This is the same as the supremum of the set of d&amp;amp;nbsp;∈&amp;amp;nbsp;[0,&amp;amp;nbsp;∞) such that the d-dimensional Hausdorff measure of X is infinite (except that when this latter set of numbers d is empty the Hausdorff dimension is zero).&lt;br /&gt;
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等价地，dim &amp;lt;sub&amp;gt;H&amp;lt;/sub&amp;gt;(''X'')可定义为 ''d'' ∈ [0, ∞) 集的下确界，使得''X'' 的''d''-维 [[豪斯多夫测度]] 为零。这与 ''d''&amp;amp;nbsp;∈&amp;amp;nbsp;[0,&amp;amp;nbsp;∞)的集合的上确界相同，因此''X''的 d 维豪斯多夫测度是无限的(除非后一个集合 ''d'' 是空的，豪斯多夫维数为零)。&lt;br /&gt;
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==Examples实例==&lt;br /&gt;
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[[Image:Sierpinski deep.svg|thumb|250px|Dimension of a further [[fractal]] example. The [[Sierpinski triangle]], an object with Hausdorff dimension of log(3)/log(2)≈1.58.&amp;lt;ref name=ClaytonSCTPLS96/&amp;gt;]]&lt;br /&gt;
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Dimension of a further [[fractal example. The Sierpinski triangle, an object with Hausdorff dimension of log(3)/log(2)≈1.58.]]&lt;br /&gt;
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[[Image:谢尔宾斯基三角形 deep.svg|thumb|250px|进一步的[[分形维数]]的例子，进一步的分形维数的例子是谢尔宾斯基三角形，它是一个豪斯多夫维数为log(3)/log(2)≈1.58.&amp;lt;ref name=ClaytonSCTPLS96/&amp;gt;的物体]]&lt;br /&gt;
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* [[Countable set]]s have Hausdorff dimension 0.&amp;lt;ref name=&amp;quot;schleicher&amp;quot;&amp;gt;{{cite journal |last1=Schleicher |first1=Dierk |title=Hausdorff Dimension, Its Properties, and Its Surprises |journal=The American Mathematical Monthly |date=June 2007 |volume=114 |issue=6 |pages=509–528 |doi=10.1080/00029890.2007.11920440 |language=en |issn=0002-9890|arxiv=math/0505099 }}&amp;lt;/ref&amp;gt;&lt;br /&gt;
*[[可数集]]拥有豪斯多夫维数0.&amp;lt;ref name=&amp;quot;schleicher&amp;quot;&amp;gt;{{cite journal |last1=Schleicher |first1=Dierk |title=豪斯多夫维数, Its Properties, and Its Surprises |journal=The American Mathematical Monthly美国数学期刊 |date=June 2007 |volume=114 |issue=6 |pages=509–528 |doi=10.1080/00029890.2007.11920440 |language=en |issn=0002-9890|arxiv=math/0505099 }}&amp;lt;/ref&amp;gt;&lt;br /&gt;
* The [[Euclidean space]] ℝ&amp;lt;sup&amp;gt;''n''&amp;lt;/sup&amp;gt; has Hausdorff dimension ''n'', and the circle '''S'''&amp;lt;sup&amp;gt;1&amp;lt;/sup&amp;gt; has Hausdorff dimension 1.&amp;lt;ref name=&amp;quot;schleicher&amp;quot; /&amp;gt;&lt;br /&gt;
*[[教育空间]] ℝ&amp;lt;sup&amp;gt;''n''&amp;lt;/sup&amp;gt; 有豪斯多夫维数 ''n''，循环'''S'''&amp;lt;sup&amp;gt;1&amp;lt;/sup&amp;gt; 拥有豪斯多夫维数1.&amp;lt;ref name=&amp;quot;schleicher&amp;quot; /&amp;gt;&lt;br /&gt;
* [[Fractal]]s often are spaces whose Hausdorff dimension strictly exceeds the [[topological dimension]].&amp;lt;ref name=&amp;quot;mandelbrot&amp;quot; /&amp;gt; For example, the [[Cantor set]], a zero-dimensional topological space, is a union of two copies of itself, each copy shrunk by a factor 1/3; hence, it can be shown that its Hausdorff dimension is ln(2)/ln(3)&amp;amp;nbsp;≈&amp;amp;nbsp;0.63.&amp;lt;ref&amp;gt;{{cite book | last=Falconer | first = Kenneth |title=Fractal Geometry: Mathematical Foundations and Applications | publisher=[[John Wiley and Sons]] | edition=2nd | year=2003}}&amp;lt;/ref&amp;gt; The [[Sierpinski triangle]] is a union of three copies of itself, each copy shrunk by a factor of&amp;amp;nbsp;1/2; this yields a Hausdorff dimension of ln(3)/ln(2)&amp;amp;nbsp;≈&amp;amp;nbsp;1.58.&amp;lt;ref name=CampbellAnnenberg15/&amp;gt; These Hausdorff dimensions are related to the &amp;quot;critical exponent&amp;quot; of the [[Master theorem (analysis of algorithms)|Master theorem]] for solving [[Recurrence relation|recurrence relations]] in the [[analysis of algorithms]].&lt;br /&gt;
*[[分形]]一般是那些豪斯多夫维数直接超过其拓扑维数的空间。例如[[康托尔集]]是一个o维拓扑空间，由两个自己复制而成，每一个复制品都是原来的三分之一，因此它的豪斯多夫维数是 ln(2)/ln(3)&amp;amp;nbsp;≈&amp;amp;nbsp;0.63。&amp;lt;ref&amp;gt;{{cite book | last=Falconer | first = Kenneth |title=Fractal Geometry: Mathematical Foundations and Applications | publisher=[[John Wiley and Sons]] | edition=2nd | year=2003}}&amp;lt;/ref&amp;gt;一个[[谢尔宾斯基三角]]是他自身三个复制的组合。每一个是原来的&amp;amp;nbsp;1/2，它的豪斯多夫维数ln(3)/ln(2)&amp;amp;nbsp;≈&amp;amp;nbsp;1.58。&amp;lt;ref name=CampbellAnnenberg15/&amp;gt;在递归算法中解决递归关系时，这些豪斯多夫维数与[[算法分析主定理]]的临界指标相联系。&lt;br /&gt;
* [[Space-filling curve]]s like the [[Peano curve]] have the same Hausdorff dimension as the space they fill.&lt;br /&gt;
*[[空间填充曲线]]拥有和他们填充空间同样的豪斯多夫维数，如[[皮亚诺曲线]]。&lt;br /&gt;
* The trajectory of [[Brownian motion]] in dimension 2 and above is conjectured to be Hausdorff dimension 2.&amp;lt;ref&amp;gt;{{cite book | last=Morters | first=Peres | title= Brownian Motion | publisher=[[Cambridge University Press]] | year=2010 }}&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
[[image:Great Britain Hausdorff.svg|thumb|250px|Estimating the Hausdorff dimension of the [[How Long Is the Coast of Britain? Statistical Self-Similarity and Fractional Dimension|coast of Great Britain]]]]&lt;br /&gt;
&lt;br /&gt;
coast of Great Britain]]&lt;br /&gt;
&lt;br /&gt;
[[大不列颠海岸&lt;br /&gt;
&lt;br /&gt;
* 刘易斯·弗赖伊·理查森[[Lewis Fry Richardson]] has performed detailed experiments to measure the approximate Hausdorff dimension for various coastlines. His results have varied from 1.02 for the coastline of [[South Africa]] to 1.25 for the west coast of [[Great Britain]].&amp;lt;ref name=&amp;quot;mandelbrot&amp;quot; /&amp;gt;&lt;br /&gt;
*刘易斯·弗赖伊·理查森（Lewis Fry Richardson）已经通过豪斯多夫维数去测量了很多海岸线。它的结果涵盖从1.02的南非海岸线到1.25的大英帝国西海岸模型。]]&lt;br /&gt;
&lt;br /&gt;
==Properties of Hausdorff dimension豪斯多夫维数特性==&lt;br /&gt;
&lt;br /&gt;
{{refimprove section|date=March 2015}}&lt;br /&gt;
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&lt;br /&gt;
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=== Hausdorff dimension and inductive dimension 豪斯多夫维数和归纳维数===&lt;br /&gt;
&lt;br /&gt;
Let ''X'' be an arbitrary [[Separable space|separable]] metric space. There is a [[topology|topological]] notion of [[inductive dimension]] for ''X'' which is defined recursively. It is always an integer (or +∞) and is denoted dim&amp;lt;sub&amp;gt;ind&amp;lt;/sub&amp;gt;(''X'').&lt;br /&gt;
&lt;br /&gt;
Let X be an arbitrary separable metric space. There is a topological notion of inductive dimension for X which is defined recursively. It is always an integer (or +∞) and is denoted dim&amp;lt;sub&amp;gt;ind&amp;lt;/sub&amp;gt;(X).&lt;br /&gt;
&lt;br /&gt;
设''X'' 是[[任意可分度量空间]]。对于''X'' 有一个递归定义的归纳维数拓扑概念。它总是一个整数(或 + ∞) ，记为dim&amp;lt;sub&amp;gt;ind&amp;lt;/sub&amp;gt;(''X'')。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
'''Theorem'''. Suppose ''X'' is non-empty. Then &lt;br /&gt;
&lt;br /&gt;
Theorem. Suppose X is non-empty. Then &lt;br /&gt;
&lt;br /&gt;
'''定理'''：假设''X'' 是非空的, 那么&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt; \dim_{\mathrm{Haus}}(X) \geq \dim_{\operatorname{ind}}(X). &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \dim_{\mathrm{Haus}}(X) \geq \dim_{\operatorname{ind}}(X). &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Moreover,&lt;br /&gt;
&lt;br /&gt;
Moreover,&lt;br /&gt;
&lt;br /&gt;
此外,&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \inf_Y \dim_{\operatorname{Haus}}(Y) =\dim_{\operatorname{ind}}(X), &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \inf_Y \dim_{\operatorname{Haus}}(Y) =\dim_{\operatorname{ind}}(X), &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
where ''Y'' ranges over metric spaces [[homeomorphic]] to ''X''. In other words, ''X'' and ''Y'' have the same underlying set of points and the metric ''d''&amp;lt;sub&amp;gt;''Y''&amp;lt;/sub&amp;gt; of ''Y'' is topologically equivalent to ''d''&amp;lt;sub&amp;gt;''X''&amp;lt;/sub&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
where Y ranges over metric spaces homeomorphic to X. In other words, X and Y have the same underlying set of points and the metric d&amp;lt;sub&amp;gt;Y&amp;lt;/sub&amp;gt; of Y is topologically equivalent to d&amp;lt;sub&amp;gt;X&amp;lt;/sub&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
其中''Y''是度量空间同胚到 ''X''的范围。换句话说， ''X''和 ''Y''具有相同的基本点集，''Y''的度量''d''&amp;lt;sub&amp;gt;''Y''&amp;lt;/sub&amp;gt; 拓扑等价于''d''&amp;lt;sub&amp;gt;''X''&amp;lt;/sub&amp;gt;。&lt;br /&gt;
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&lt;br /&gt;
&lt;br /&gt;
These results were originally established by [[Edward Szpilrajn]] (1907–1976), e.g., see Hurewicz and Wallman, Chapter VII.{{full citation needed|date=March 2015}}&lt;br /&gt;
&lt;br /&gt;
These results were originally established by Edward Szpilrajn (1907–1976), e.g., see Hurewicz and Wallman, Chapter VII.&lt;br /&gt;
&lt;br /&gt;
这些结果最初是由 [[Edward Szpilrajn]] (1907–1976)建立的,  参见 Hurewicz and Wallman, Chapter VII.{{full citation needed|date=March 2015}}第七章。&lt;br /&gt;
&lt;br /&gt;
=== Hausdorff dimension and Minkowski dimension 豪斯多夫维数和闵可夫斯基维度===&lt;br /&gt;
&lt;br /&gt;
The [[Minkowski dimension]] is similar to, and at least as large as, the Hausdorff dimension, and they are equal in many situations. However, the set of [[rational number|rational]] points in [0, 1] has Hausdorff dimension zero and Minkowski dimension one. There are also compact sets for which the Minkowski dimension is strictly larger than the Hausdorff dimension.&lt;br /&gt;
&lt;br /&gt;
The Minkowski dimension is similar to, and at least as large as, the Hausdorff dimension, and they are equal in many situations. However, the set of rational points in [0, 1] has Hausdorff dimension zero and Minkowski dimension one. There are also compact sets for which the Minkowski dimension is strictly larger than the Hausdorff dimension.&lt;br /&gt;
&lt;br /&gt;
[[闵可夫斯基维数]]与豪斯多夫维数相似，至少和它一样大，而且在许多情况下是相等的。然而，[0,1]中有理点集的豪斯多夫维数为0，闵可夫斯基维数为1。还有一些紧集的闵可夫斯基维数严格大于豪斯多夫维数。&lt;br /&gt;
&lt;br /&gt;
=== Hausdorff dimensions and Frostman measures 豪斯多夫维度和弗洛斯曼测度===&lt;br /&gt;
&lt;br /&gt;
If there is a [[measure (mathematics)|measure]] μ defined on [[Borel measure|Borel]] subsets of a metric space ''X'' such that ''μ''(''X'') &amp;gt; 0 and ''μ''(''B''(''x'', ''r'')) ≤ ''r&amp;lt;sup&amp;gt;s&amp;lt;/sup&amp;gt;'' holds for some constant ''s'' &amp;gt; 0 and for every ball ''B''(''x'', ''r'') in ''X'', then dim&amp;lt;sub&amp;gt;Haus&amp;lt;/sub&amp;gt;(''X'') ≥ ''s''. A partial converse is provided by [[Frostman's lemma]].{{citation needed|date=March 2015}}&amp;lt;ref&amp;gt;This Wikipedia article also discusses further useful characterizations of the Hausdorff dimension.{{clarify|date=March 2015}}&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
If there is a measure μ defined on Borel subsets of a metric space X such that μ(X) &amp;gt; 0 and μ(B(x, r)) ≤ r&amp;lt;sup&amp;gt;s&amp;lt;/sup&amp;gt; holds for some constant s &amp;gt; 0 and for every ball B(x, r) in X, then dim&amp;lt;sub&amp;gt;Haus&amp;lt;/sub&amp;gt;(X) ≥ s. A partial converse is provided by Frostman's lemma.&lt;br /&gt;
&lt;br /&gt;
如果在度量空间 ''X'' 的 Borel 子集上定义一个测度 μ，使得''μ''(''X'') &amp;gt; 0 和''μ''(''B''(''x'', ''r'')) ≤ ''r&amp;lt;sup&amp;gt;s&amp;lt;/sup&amp;gt;''，对于某个常数 ''s'' &amp;gt; 0  和 ''X'' 中的每个球 ''B''(''x'', ''r'') 成立，则 dim&amp;lt;sub&amp;gt;Haus&amp;lt;/sub&amp;gt;(''X'') ≥ ''s'' 。 部分逆向转换由弗洛斯曼引理定义。&lt;br /&gt;
&lt;br /&gt;
=== Behaviour under unions and products ===&lt;br /&gt;
&lt;br /&gt;
If &amp;lt;math&amp;gt;X=\bigcup_{i\in I}X_i&amp;lt;/math&amp;gt; is a finite or countable union, then&lt;br /&gt;
&lt;br /&gt;
If &amp;lt;math&amp;gt;X=\bigcup_{i\in I}X_i&amp;lt;/math&amp;gt; is a finite or countable union, then&lt;br /&gt;
&lt;br /&gt;
如果 &amp;lt;math&amp;gt;X=\bigcup_{i\in I}X_i&amp;lt;/math&amp;gt; 是一个有限或可数的联合，则&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \dim_{\operatorname{Haus}}(X) =\sup_{i\in I} \dim_{\operatorname{Haus}}(X_i).&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \dim_{\operatorname{Haus}}(X) =\sup_{i\in I} \dim_{\operatorname{Haus}}(X_i).&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
This can be verified directly from the definition.&lt;br /&gt;
&lt;br /&gt;
This can be verified directly from the definition.&lt;br /&gt;
&lt;br /&gt;
这可以直接从定义得到验证。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
If ''X'' and ''Y'' are non-empty metric spaces, then the Hausdorff dimension of their product satisfies&amp;lt;ref&amp;gt;{{cite journal |author=Marstrand, J. M. |title=The dimension of Cartesian product sets |journal=Proc. Cambridge Philos. Soc. |volume=50 |issue=3 |pages=198–202 |year=1954 |doi=10.1017/S0305004100029236 |bibcode = 1954PCPS...50..198M }}&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
If X and Y are non-empty metric spaces, then the Hausdorff dimension of their product satisfies&lt;br /&gt;
&lt;br /&gt;
如果 ''X'' 和''Y''是非空度量空间，那么它们乘积的豪斯多夫维数满足&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt; \dim_{\operatorname{Haus}}(X\times Y)\ge \dim_{\operatorname{Haus}}(X)+ \dim_{\operatorname{Haus}}(Y).&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \dim_{\operatorname{Haus}}(X\times Y)\ge \dim_{\operatorname{Haus}}(X)+ \dim_{\operatorname{Haus}}(Y).&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
This inequality can be strict. It is possible to find two sets of dimension 0 whose product has dimension 1.&amp;lt;ref&amp;gt;{{cite book  | last = Falconer  | first = Kenneth J.  | title = Fractal geometry. Mathematical foundations and applications  | publisher = John Wiley &amp;amp; Sons, Inc., Hoboken, New Jersey  | year = 2003  | doi =   | isbn = }}&amp;lt;/ref&amp;gt; In the opposite direction, it is known that when ''X'' and ''Y'' are Borel subsets of '''R'''&amp;lt;sup&amp;gt;''n''&amp;lt;/sup&amp;gt;, the Hausdorff dimension of ''X'' × ''Y'' is bounded from above by the Hausdorff dimension of ''X'' plus the [[packing dimension|upper packing dimension]] of ''Y''. These facts are discussed in Mattila (1995).&lt;br /&gt;
&lt;br /&gt;
This inequality can be strict. It is possible to find two sets of dimension 0 whose product has dimension 1. In the opposite direction, it is known that when X and Y are Borel subsets of R&amp;lt;sup&amp;gt;n&amp;lt;/sup&amp;gt;, the Hausdorff dimension of X × Y is bounded from above by the Hausdorff dimension of X plus the upper packing dimension of Y. These facts are discussed in Mattila (1995).&lt;br /&gt;
&lt;br /&gt;
这种不平等可以是严格的。有可能找到两个维数为0的集合，其乘积的维数为1。相反，我们知道当''X''和''Y''是 '''R'''&amp;lt;sup&amp;gt;''n''&amp;lt;/sup&amp;gt;的 Borel 子集时， ''X'' × ''Y''的豪斯多夫维数从上面以 ''X''的豪斯多夫维数加上 ''Y''的上填充维数为界。Mattila (1995)曾就这些情况进行了讨论。&lt;br /&gt;
&lt;br /&gt;
==Self-similar sets自相似集合==&lt;br /&gt;
&lt;br /&gt;
{{refimprove section|date=March 2015}}&lt;br /&gt;
&lt;br /&gt;
Many sets defined by a self-similarity condition have dimensions which can be determined explicitly. Roughly, a set ''E'' is self-similar if it is the fixed point of a set-valued transformation ψ, that is ψ(''E'') = ''E'', although the exact definition is given below.&lt;br /&gt;
&lt;br /&gt;
Many sets defined by a self-similarity condition have dimensions which can be determined explicitly. Roughly, a set E is self-similar if it is the fixed point of a set-valued transformation ψ, that is ψ(E) = E, although the exact definition is given below.&lt;br /&gt;
&lt;br /&gt;
许多由自相似条件定义的集合具有可以显式确定的维数。粗略地说，如果集合''E''是集值ψ变换的不动点，即ψ(''E'') = ''E''， 则它是自相似的，尽管下面给出了确切的定义。&lt;br /&gt;
&lt;br /&gt;
&amp;lt;blockquote&amp;gt;'''Theorem'''. Suppose&lt;br /&gt;
&lt;br /&gt;
&amp;lt;blockquote&amp;gt;Theorem. Suppose&lt;br /&gt;
&lt;br /&gt;
&amp;lt;blockquote&amp;gt;'''定理'''：假设&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt; \psi_i: \mathbf{R}^n \rightarrow \mathbf{R}^n, \quad i=1, \ldots , m &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \psi_i: \mathbf{R}^n \rightarrow \mathbf{R}^n, \quad i=1, \ldots , m &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
are [[Contraction mapping|contractive]] mappings on '''R'''&amp;lt;sup&amp;gt;''n''&amp;lt;/sup&amp;gt; with contraction constant ''r&amp;lt;sub&amp;gt;j&amp;lt;/sub&amp;gt;'' &amp;lt; 1. Then there is a unique ''non-empty'' compact set ''A'' such that&lt;br /&gt;
&lt;br /&gt;
are contractive mappings on R&amp;lt;sup&amp;gt;n&amp;lt;/sup&amp;gt; with contraction constant r&amp;lt;sub&amp;gt;j&amp;lt;/sub&amp;gt; &amp;lt; 1. Then there is a unique non-empty compact set A such that&lt;br /&gt;
&lt;br /&gt;
是'''R'''&amp;lt;sup&amp;gt;''n''&amp;lt;/sup&amp;gt;上的压缩常数''r&amp;lt;sub&amp;gt;j&amp;lt;/sub&amp;gt;'&amp;lt; 1的压缩映射。则有一个唯一的非空紧集A &lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt; A = \bigcup_{i=1}^m \psi_i (A). &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; A = \bigcup_{i=1}^m \psi_i (A). &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&amp;lt;/blockquote&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;/blockquote&amp;gt;&lt;br /&gt;
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&lt;br /&gt;
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The theorem follows from [[Stefan Banach]]'s [[Contractive mapping theorem|contractive mapping fixed point theorem]] applied to the complete metric space of non-empty compact subsets of '''R'''&amp;lt;sup&amp;gt;''n''&amp;lt;/sup&amp;gt; with the [[Hausdorff distance]].&amp;lt;ref&amp;gt;{{cite book |author=Falconer, K. J. |title=The Geometry of Fractal Sets |publisher=Cambridge University Press |location=Cambridge, UK |year=1985 |isbn=0-521-25694-1 |chapter=Theorem 8.3}}&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
The theorem follows from Stefan Banach's contractive mapping fixed point theorem applied to the complete metric space of non-empty compact subsets of R&amp;lt;sup&amp;gt;n&amp;lt;/sup&amp;gt; with the Hausdorff distance.&lt;br /&gt;
&lt;br /&gt;
这个定理来源于 Stefan Banach 的压缩映射不动点定理，该定理应用于 具有豪斯多夫距离的'''R'''&amp;lt;sup&amp;gt;''n''&amp;lt;/sup&amp;gt; 的非空紧子集的完整度量空间。&lt;br /&gt;
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&lt;br /&gt;
===The open set condition开集条件===&lt;br /&gt;
&lt;br /&gt;
To determine the dimension of the self-similar set ''A'' (in certain cases), we need a technical condition called the ''open set condition'' (OSC) on the sequence of contractions ψ&amp;lt;sub&amp;gt;''i''&amp;lt;/sub&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
To determine the dimension of the self-similar set A (in certain cases), we need a technical condition called the open set condition (OSC) on the sequence of contractions ψ&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
为了确定自相似集''A'' 的维数(在某些情况下) ，我们需要一个关于收缩序列的称为''开集条件''(OSC)的技术条件ψ&amp;lt;sub&amp;gt;''i''&amp;lt;/sub&amp;gt;。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
There is a relatively compact open set ''V'' such that&lt;br /&gt;
&lt;br /&gt;
There is a relatively compact open set V such that&lt;br /&gt;
&lt;br /&gt;
有一个相对紧的开集''V''&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt; \bigcup_{i=1}^m\psi_i (V) \subseteq V, &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \bigcup_{i=1}^m\psi_i (V) \subseteq V, &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
where the sets in union on the left are pairwise [[disjoint sets|disjoint]].&lt;br /&gt;
&lt;br /&gt;
where the sets in union on the left are pairwise disjoint.&lt;br /&gt;
&lt;br /&gt;
左边并集的集合成对不相交。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The open set condition is a separation condition that ensures the images ψ&amp;lt;sub&amp;gt;''i''&amp;lt;/sub&amp;gt;(''V'') do not overlap &amp;quot;too much&amp;quot;.&lt;br /&gt;
&lt;br /&gt;
The open set condition is a separation condition that ensures the images ψ&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;(V) do not overlap &amp;quot;too much&amp;quot;.&lt;br /&gt;
&lt;br /&gt;
开集条件是保证图像ψ&amp;lt;sub&amp;gt;''i''&amp;lt;/sub&amp;gt;(''V'') 不重叠“太多”的分离条件。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
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'''Theorem'''. Suppose the open set condition holds and each ψ&amp;lt;sub&amp;gt;''i''&amp;lt;/sub&amp;gt; is a similitude, that is a composition of an [[isometry]] and a [[dilation (metric space)|dilation]] around some point. Then the unique fixed point of ψ is a set whose Hausdorff dimension is ''s'' where ''s'' is the unique solution of&amp;lt;ref&amp;gt;{{cite journal | last=Hutchinson | first=John E. | title=Fractals and self similarity | journal=Indiana Univ. Math. J. | volume=30 | year=1981 | pages=713–747 | doi=10.1512/iumj.1981.30.30055 | issue=5 | doi-access=free }}&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
Theorem. Suppose the open set condition holds and each ψ&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt; is a similitude, that is a composition of an isometry and a dilation around some point. Then the unique fixed point of ψ is a set whose Hausdorff dimension is s where s is the unique solution of&lt;br /&gt;
&lt;br /&gt;
'''定理'''假设开集条件成立，并且每个ψ&amp;lt;sub&amp;gt;''i''&amp;lt;/sub&amp;gt; 是一个相似度，即等距和某个点周围的膨胀的组合。。那么唯一的不动点是Hausdorff维数为 ''s'' 的集合，其中  ''s'' 是 ''s'' &amp;lt;ref&amp;gt;{{cite journal | last=Hutchinson | first=John E. | title=Fractals and self similarity | journal=Indiana Univ. Math. J. | volume=30 | year=1981 | pages=713–747 | doi=10.1512/iumj.1981.30.30055 | issue=5 | doi-access=free }}&amp;lt;/ref&amp;gt;的唯一解&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt; \sum_{i=1}^m r_i^s = 1. &amp;lt;/math&amp;gt;&lt;br /&gt;
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&amp;lt;math&amp;gt; \sum_{i=1}^m r_i^s = 1. &amp;lt;/math&amp;gt;&lt;br /&gt;
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The contraction coefficient of a similitude is the magnitude of the dilation.&lt;br /&gt;
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The contraction coefficient of a similitude is the magnitude of the dilation.&lt;br /&gt;
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相似物的收缩系数就是膨胀的大小。&lt;br /&gt;
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We can use this theorem to compute the Hausdorff dimension of the Sierpinski triangle (or sometimes called Sierpinski gasket). Consider three [[non-collinear points]] ''a''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;, ''a''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;, ''a''&amp;lt;sub&amp;gt;3&amp;lt;/sub&amp;gt; in the plane '''R'''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; and let ψ&amp;lt;sub&amp;gt;''i''&amp;lt;/sub&amp;gt; be the dilation of ratio 1/2 around ''a&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;''. The unique non-empty fixed point of the corresponding mapping ψ is a Sierpinski gasket and the dimension ''s'' is the unique solution of&lt;br /&gt;
&lt;br /&gt;
We can use this theorem to compute the Hausdorff dimension of the Sierpinski triangle (or sometimes called Sierpinski gasket). Consider three non-collinear points a&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;, a&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;, a&amp;lt;sub&amp;gt;3&amp;lt;/sub&amp;gt; in the plane R&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; and let ψ&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt; be the dilation of ratio 1/2 around a&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;. The unique non-empty fixed point of the corresponding mapping ψ is a Sierpinski gasket and the dimension s is the unique solution of&lt;br /&gt;
&lt;br /&gt;
我们可以使用这个定理来计算谢尔宾斯基三角形的豪斯多夫维数(或者有时候叫做谢尔宾斯基垫圈)。考虑R&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; 平面上的三个非共线点，''a''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;，''a''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;，''a''&amp;lt;sub&amp;gt;3&amp;lt;/sub&amp;gt;，让ψ&amp;lt;sub&amp;gt;''i''&amp;lt;/sub&amp;gt;是围绕着''a&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;''比率1/2的膨胀。对应映射的唯一非空不动点是一个谢尔宾斯基垫圈，其维数''s''是对应映射的唯一解&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt; \left(\frac{1}{2}\right)^s+\left(\frac{1}{2}\right)^s+\left(\frac{1}{2}\right)^s = 3 \left(\frac{1}{2}\right)^s =1. &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \left(\frac{1}{2}\right)^s+\left(\frac{1}{2}\right)^s+\left(\frac{1}{2}\right)^s = 3 \left(\frac{1}{2}\right)^s =1. &amp;lt;/math&amp;gt;&lt;br /&gt;
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Taking [[natural logarithm]]s of both sides of the above equation, we can solve for ''s'', that is: ''s'' = ln(3)/ln(2).  The Sierpinski gasket is self-similar and satisfies the OSC. In general a set ''E'' which is a fixed point of a mapping&lt;br /&gt;
&lt;br /&gt;
Taking natural logarithms of both sides of the above equation, we can solve for s, that is: s = ln(3)/ln(2).  The Sierpinski gasket is self-similar and satisfies the OSC. In general a set E which is a fixed point of a mapping&lt;br /&gt;
&lt;br /&gt;
取上述方程两边的自然对数，我们可以求出 ''s''，即: ''s'' = ln(3)/ln(2)。该密封垫具有自相似性，满足 OSC 要求。一般来说，集合 ''E''是一个映射的不动点&lt;br /&gt;
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: &amp;lt;math&amp;gt; A \mapsto \psi(A) = \bigcup_{i=1}^m \psi_i(A) &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt; A \mapsto \psi(A) = \bigcup_{i=1}^m \psi_i(A) &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
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is self-similar if and only if the intersections&lt;br /&gt;
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is self-similar if and only if the intersections&lt;br /&gt;
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是自相似的，当且仅当&lt;br /&gt;
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:&amp;lt;math&amp;gt; H^s\left(\psi_i(E) \cap \psi_j(E)\right) =0, &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; H^s\left(\psi_i(E) \cap \psi_j(E)\right) =0, &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
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where ''s'' is the Hausdorff dimension of ''E'' and ''H&amp;lt;sup&amp;gt;s&amp;lt;/sup&amp;gt;'' denotes [[Hausdorff measure]]. This is clear in the case of the Sierpinski gasket (the intersections are just points), but is also true more generally:&lt;br /&gt;
&lt;br /&gt;
where s is the Hausdorff dimension of E and H&amp;lt;sup&amp;gt;s&amp;lt;/sup&amp;gt; denotes Hausdorff measure. This is clear in the case of the Sierpinski gasket (the intersections are just points), but is also true more generally:&lt;br /&gt;
&lt;br /&gt;
其中 ''s''是''E''的豪斯多夫维数， ''H&amp;lt;sup&amp;gt;s&amp;lt;/sup&amp;gt;'' 表示 豪斯多夫测度。对于谢尔宾斯基垫圈(交叉点就是点)来说，这一点很明显，但更普遍的情况是:&lt;br /&gt;
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'''Theorem'''. Under the same conditions as the previous theorem, the unique fixed point of ψ is self-similar.&lt;br /&gt;
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Theorem. Under the same conditions as the previous theorem, the unique fixed point of ψ is self-similar.&lt;br /&gt;
&lt;br /&gt;
'''定理'''：在与前一定理相同的条件下，其唯一不动点是自相似的。&lt;br /&gt;
&lt;br /&gt;
==See also参阅==&lt;br /&gt;
&lt;br /&gt;
* [[List of fractals by Hausdorff dimension豪斯多夫分形维数列表]] Examples of deterministic fractals, random and natural fractals.确定性分形与随机和自然分形的示例。&lt;br /&gt;
&lt;br /&gt;
* [[Assouad dimension  Assouad维数]], another variation of fractal dimension that, like Hausdorff dimension, is defined using coverings by balls其他被球覆盖方式定义的分形维数，例如豪斯多夫维数。&lt;br /&gt;
&lt;br /&gt;
* [[Intrinsic dimension固有维数]]&lt;br /&gt;
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* [[Packing dimension填充维数]]&lt;br /&gt;
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* [[Fractal dimension分形维数]]&lt;br /&gt;
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==References参考文献==&lt;br /&gt;
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{{reflist}}&lt;br /&gt;
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==Further reading拓展阅读==&lt;br /&gt;
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* {{cite book |last1=Dodson |first1=M. Maurice |title=Fractal Geometry and Applications: A Jubilee of Benoît Mandelbrot |volume=72 |issue=1 |pages=305–347 |last2=Kristensen |first2=Simon |chapter=Hausdorff Dimension and Diophantine Approximation |date=June 12, 2003 |arxiv=math/0305399 |bibcode = 2003math......5399D |doi=10.1090/pspum/072.1/2112110|series=Proceedings of Symposia in Pure Mathematics |isbn=9780821836378 }}&lt;br /&gt;
&lt;br /&gt;
* {{cite book |last1=Hurewicz |first1=Witold |authorlink1=Witold Hurewicz |last2=Wallman |first2=Henry |authorlink2=Henry Wallman |title=Dimension Theory |url=https://archive.org/details/in.ernet.dli.2015.84609 |publisher=Princeton University Press |year=1948 }}&lt;br /&gt;
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* {{cite journal |author作者=E. Szpilrajn |authorlink=Edward Marczewski |title=La dimension et la mesure |journal=Fundamenta Mathematicae |volume=28 |pages=81–9 |year=1937 }}&lt;br /&gt;
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* {{cite journal&lt;br /&gt;
&lt;br /&gt;
 | last1=Marstrand&lt;br /&gt;
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 | last1=Marstrand&lt;br /&gt;
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 | last1=马斯特兰德&lt;br /&gt;
&lt;br /&gt;
 | first1=J. M. | title=The dimension of cartesian product sets | year=1954 | journal=Proc. Cambridge Philos. Soc.&lt;br /&gt;
&lt;br /&gt;
 | first1=J. M. | title=The dimension of cartesian product sets | year=1954 | journal=Proc. Cambridge Philos. Soc.&lt;br /&gt;
&lt;br /&gt;
 | first1= J. M. | title=笛卡儿积集的维数 | 1954年 |  journal=Proc. Cambridge Philos. Soc.&lt;br /&gt;
&lt;br /&gt;
 | volume=50&lt;br /&gt;
&lt;br /&gt;
 | volume=50&lt;br /&gt;
&lt;br /&gt;
 | 第50卷&lt;br /&gt;
&lt;br /&gt;
 | issue=3&lt;br /&gt;
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 | issue=3&lt;br /&gt;
&lt;br /&gt;
 | 第三期&lt;br /&gt;
&lt;br /&gt;
 | pages=198–202&lt;br /&gt;
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 | pages=198–202&lt;br /&gt;
&lt;br /&gt;
 | 第198-202页&lt;br /&gt;
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 | doi=10.1017/S0305004100029236|bibcode = 1954PCPS...50..198M }}&lt;br /&gt;
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 | doi=10.1017/S0305004100029236|bibcode = 1954PCPS...50..198M }}&lt;br /&gt;
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10.1017 / S0305004100029236 | bibcode 1954PCPS... 50. . 198 m }&lt;br /&gt;
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* {{Cite book&lt;br /&gt;
&lt;br /&gt;
 | last1=Mattila&lt;br /&gt;
&lt;br /&gt;
 | last1=Mattila&lt;br /&gt;
&lt;br /&gt;
 | last1=Mattila&lt;br /&gt;
&lt;br /&gt;
 | first1=Pertti | author1-link=Pertti Mattila| title=Geometry of sets and measures in Euclidean spaces | publisher=[[Cambridge University Press]]&lt;br /&gt;
&lt;br /&gt;
 | first1=Pertti | author1-link=Pertti Mattila| title=Geometry of sets and measures in Euclidean spaces | publisher=Cambridge University Press&lt;br /&gt;
&lt;br /&gt;
| first1 Pertti | author1-link Pertti Mattila | title 欧几里德空间中集合和度量的几何 | 出版商剑桥大学出版社&lt;br /&gt;
&lt;br /&gt;
 | isbn=978-0-521-65595-8 | year=1995}}&lt;br /&gt;
&lt;br /&gt;
 | isbn=978-0-521-65595-8 | year=1995}}&lt;br /&gt;
&lt;br /&gt;
| isbn 978-0-521-65595-8 | year 1995}&lt;br /&gt;
&lt;br /&gt;
* {{cite journal |author=A. S. Besicovitch |authorlink=A. S. Besicovitch |title=On Linear Sets of Points of Fractional Dimensions |journal=[[Mathematische Annalen]] |volume=101 |year=1929 | doi=10.1007/BF01454831| issue=1 |pages= 161–193}}&lt;br /&gt;
&lt;br /&gt;
* {{cite journal |author1=A. S. Besicovitch |authorlink1=A. S. Besicovitch |author2=H. D. Ursell |authorlink2=H. D. Ursell |title=Sets of Fractional Dimensions |journal=Journal of the London Mathematical Society |volume=12 |year=1937 | issue=1 | doi=10.1112/jlms/s1-12.45.18  | pages=18–25 }}&amp;lt;br/&amp;gt;Several selections from this volume are reprinted in {{cite book |author=Edgar, Gerald A. |title=Classics on fractals |publisher=Addison-Wesley |location=Boston |year=1993 |isbn=0-201-58701-7}} See chapters 9,10,11&lt;br /&gt;
&lt;br /&gt;
* {{cite journal |author=F. Hausdorff |authorlink=F. Hausdorff |title=Dimension und äußeres Maß |journal=Mathematische Annalen |volume=79 |issue=1–2 |pages=157–179 |date=March 1919 |doi=10.1007/BF01457179|hdl=10338.dmlcz/100363 |url=http://dml.cz/bitstream/handle/10338.dmlcz/100363/CzechMathJ_09-1959-3_5.pdf }}&lt;br /&gt;
&lt;br /&gt;
* {{cite journal | last=Hutchinson | first=John E. | title=Fractals and self similarity | journal=Indiana Univ. Math. J. | volume=30 | year=1981 | pages=713–747 | doi=10.1512/iumj.1981.30.30055 | issue=5 | doi-access=free }}&lt;br /&gt;
&lt;br /&gt;
*{{cite book | last=Falconer | first = Kenneth |title=Fractal Geometry: Mathematical Foundations and Applications | publisher=[[John Wiley and Sons]] | edition=2nd | year=2003}}&lt;br /&gt;
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==External links外部链接==&lt;br /&gt;
&lt;br /&gt;
* [https://www.encyclopediaofmath.org/index.php/Hausdorff_dimension Hausdorff dimension] 在 [https://www.encyclopediaofmath.org/ Encyclopedia of Mathematics]&lt;br /&gt;
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* [https://www.encyclopediaofmath.org/index.php/Hausdorff_measure Hausdorff measure] 在 [https://www.encyclopediaofmath.org/ Encyclopedia of Mathematics]&lt;br /&gt;
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{{DEFAULTSORT:Hausdorff Dimension豪斯多夫维数}}&lt;br /&gt;
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[[Category分类:Fractals分形]]&lt;br /&gt;
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[[Category分类:Metric geometry度量几何]]&lt;br /&gt;
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[[Category分类:Dimension theory维度理论]]&lt;br /&gt;
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&amp;lt;small&amp;gt;This page was moved from [[wikipedia:en:Hausdorff dimension]]. Its edit history can be viewed at [[分形维数/edithistory]]&amp;lt;/small&amp;gt;&amp;lt;/noinclude&amp;gt;&lt;br /&gt;
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[[Category:待整理页面]]&lt;/div&gt;</summary>
		<author><name>Ruili</name></author>
	</entry>
	<entry>
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		<title>分形维数</title>
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		<updated>2020-11-01T18:07:32Z</updated>

		<summary type="html">&lt;p&gt;Ruili：&lt;/p&gt;
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&lt;div&gt;此词条暂由彩云小译翻译，未经人工整理和审校，带来阅读不便，请见谅。&lt;br /&gt;
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{{short description|Invariant}}&lt;br /&gt;
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Example of non-integer dimensions. The first four [[iteration]]s of the [[Koch snowflake|Koch curve]], where after each iteration, all original line segments are replaced with four, each a self-similar copy that is 1/3 the length of the original. One formalism of the Hausdorff dimension uses this scale factor (3) and the number of self-similar objects (4) to calculate the dimension, D, after the first iteration to be D = (log N)/(log S) = (log 4)/(log 3) ≈ 1.26.&amp;lt;ref name=CampbellAnnenberg15&amp;gt;MacGregor Campbell, 2013, &amp;quot;5.6 Scaling and the Hausdorff Dimension,&amp;quot; at ''Annenberg Learner:MATHematics illuminated'', see [http://www.learner.org/courses/mathilluminated/units/5/textbook/06.php], accessed 5 March 2015.&amp;lt;/ref&amp;gt; That is, while the Hausdorff dimension of a single [[point (geometry)|point]] is zero, of a [[line segment]] is 1, of a [[square]] is 2, and of a [[cube]] is 3, for [[fractal]]s such as this, the object can have a non-integer dimension.&lt;br /&gt;
&lt;br /&gt;
Example of non-integer dimensions. The first four iterations of the Koch curve, where after each iteration, all original line segments are replaced with four, each a self-similar copy that is 1/3 the length of the original. One formalism of the Hausdorff dimension uses this scale factor (3) and the number of self-similar objects (4) to calculate the dimension, D, after the first iteration to be D = (log N)/(log S) = (log 4)/(log 3) ≈ 1.26. That is, while the Hausdorff dimension of a single point is zero, of a line segment is 1, of a square is 2, and of a cube is 3, for fractals such as this, the object can have a non-integer dimension.&lt;br /&gt;
&lt;br /&gt;
非整数维度示例：前四个[[Koch 曲线]]的迭代，在每次迭代后，所有原始线段都被替换为四个，每个自相似的复制是原始线段长度的1 / 3。豪斯多夫维数的一个建模是使用比例因子(3)和自相似对象的数量(4)来计算维度 D，在第一次迭代后为 D = (log N)/(log S) = (log 4)/(log 3) ≈ 1.26.&amp;lt;ref name=CampbellAnnenberg15&amp;gt;。MacGregor Campbell, 2013, &amp;quot;5.6 Scaling and the Hausdorff Dimension,&amp;quot; 在 ''Annenberg Learner:MATHematics illuminated'', 参见 [http://www.learner.org/courses/mathilluminated/units/5/textbook/06.php], accessed 5 March 2015.&amp;lt;/ref&amp;gt; 也就是说，单点的豪斯多夫维数为零，线段为1，正方形为2，立方体为3时，但对于分形，对象可以有一个非整数维度。&lt;br /&gt;
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In [[mathematics]], '''Hausdorff dimension''' is a measure of ''roughness'', or more specifically, [[fractal dimension]], that was first introduced in 1918 by [[mathematician]] [[Felix Hausdorff]].&amp;lt;ref&amp;gt;{{Cite journal |arxiv = 1101.1444|doi = 10.1214/11-STS370|title = Estimators of Fractal Dimension: Assessing the Roughness of Time Series and Spatial Data|journal = Statistical Science|volume = 27|issue = 2|pages = 247–277|year = 2012|last1 = Gneiting|first1 = Tilmann|last2 = Ševčíková|first2 = Hana|last3 = Percival|first3 = Donald B.}}&amp;lt;/ref&amp;gt; For instance, the Hausdorff dimension of a single [[point (geometry)|point]] is zero, of a [[line segment]] is 1, of a [[square]] is 2, and of a [[cube]] is 3. That is, for sets of points that define a smooth shape or a shape that has a small number of corners—the shapes of traditional geometry and science—the Hausdorff dimension is an [[integer]] agreeing with the usual sense of dimension, also known as the [[Inductive dimension|topological dimension]]. However, formulas have also been developed that allow calculation of the dimension of other less simple objects, where, solely on the basis of their properties of [[scaling (geometry)|scaling]] and [[self-similarity]], one is led to the conclusion that particular objects—including [[fractal]]s—have non-integer Hausdorff dimensions. Because of the significant technical advances made by [[Abram Samoilovitch Besicovitch]] allowing computation of dimensions for highly irregular or &amp;quot;rough&amp;quot; sets, this dimension is also commonly referred to as the ''Hausdorff–Besicovitch dimension.''&lt;br /&gt;
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In mathematics, Hausdorff dimension is a measure of roughness, or more specifically, fractal dimension, that was first introduced in 1918 by mathematician Felix Hausdorff. For instance, the Hausdorff dimension of a single point is zero, of a line segment is 1, of a square is 2, and of a cube is 3. That is, for sets of points that define a smooth shape or a shape that has a small number of corners—the shapes of traditional geometry and science—the Hausdorff dimension is an integer agreeing with the usual sense of dimension, also known as the topological dimension. However, formulas have also been developed that allow calculation of the dimension of other less simple objects, where, solely on the basis of their properties of scaling and self-similarity, one is led to the conclusion that particular objects—including fractals—have non-integer Hausdorff dimensions. Because of the significant technical advances made by Abram Samoilovitch Besicovitch allowing computation of dimensions for highly irregular or &amp;quot;rough&amp;quot; sets, this dimension is also commonly referred to as the Hausdorff–Besicovitch dimension.&lt;br /&gt;
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在[[数学]]中，'''&amp;lt;font color = '#ff8000'&amp;gt;豪斯多夫维数Hausdorff dimension&amp;lt;/font&amp;gt;'''是一种粗糙度的度量单位，或者更确切地说，分形维数，是由数学家 Felix Hausdorff 在1918年首次提出的。例如，单点的豪斯多夫维数为零，线段为1，正方形为2，立方体为3。也就是说，对于定义了一个光滑形状或一个有少数几个角的形状---- 传统几何学和科学的形状---- 的点集来说，豪斯多夫维数是一个整数，符合通常的维度意义，也称为拓扑维度。然而，还有一些公式允许计算其他不太简单的对象的维数，其中仅仅根据它们的标度和自相似特性，就可以得出结论: 特定的对象ー包括分形ー具有非整数的 Hausdorff 维数。由于阿布拉姆·萨莫伊洛维奇·贝西科维奇的重大技术进步，允许计算高度不规则或“粗糙”集的维度，这个维度通常也被称为 Hausdorff-Besicovitch 维度。 &lt;br /&gt;
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The Hausdorff dimension, more specifically, is a further dimensional number associated with a given set, where the distances between all members of that set are defined. Such a set is termed a [[metric space]]. The dimension is drawn from the [[Extended real number line|extended real numbers]], &amp;lt;math&amp;gt;\overline{\mathbb{R}}&amp;lt;/math&amp;gt;, as opposed to the more intuitive notion of dimension, which is not associated to general metric spaces, and only takes values in the non-negative integers.&lt;br /&gt;
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The Hausdorff dimension, more specifically, is a further dimensional number associated with a given set, where the distances between all members of that set are defined. Such a set is termed a metric space. The dimension is drawn from the extended real numbers, &amp;lt;math&amp;gt;\overline{\mathbb{R}}&amp;lt;/math&amp;gt;, as opposed to the more intuitive notion of dimension, which is not associated to general metric spaces, and only takes values in the non-negative integers.&lt;br /&gt;
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更具体地说，豪斯多夫维数是一个与给定集合相关联的更进一步的维数，其中定义了该集合所有成员之间的距离。这样的集合称为度量空间。维数是从扩展的实数，&amp;lt;math&amp;gt;\overline{\mathbb{R}}&amp;lt;/math&amp;gt;，而不是更直观的维数概念(它不与一般的度量空间相关联，只取非负整数的值)。&lt;br /&gt;
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In mathematical terms, the Hausdorff dimension generalizes the notion of the dimension of a real [[vector space]]. That is, the Hausdorff dimension of an ''n''-dimensional [[inner product space]] equals ''n''. This underlies the earlier statement that the Hausdorff dimension of a point is zero, of a line is one, etc., and that [[fractal|irregular sets]] can have noninteger Hausdorff dimensions. For instance, the [[Koch snowflake]] shown at right is constructed from an equilateral triangle; in each iteration, its component line segments are divided into 3 segments of unit length, the newly created middle segment is used as the base of a new [[equilateral]] triangle that points outward, and this base segment is then deleted to leave a final object from the iteration of unit length of 4.&amp;lt;ref&amp;gt;Larry Riddle, 2014, &amp;quot;Classic Iterated Function Systems: Koch Snowflake&amp;quot;, Agnes Scott College e-Academy (online), see [http://ecademy.agnesscott.edu/~lriddle/ifs/ksnow/ksnow.htm], accessed 5 March 2015.&amp;lt;/ref&amp;gt; That is, after the first iteration, each original line segment has been replaced with N=4, where each self-similar copy is 1/S = 1/3 as long as the original.&amp;lt;ref name=CampbellAnnenberg15/&amp;gt; Stated another way, we have taken an object with Euclidean dimension, D, and reduced its linear scale by 1/3 in each direction, so that its length increases to N=S&amp;lt;sup&amp;gt;D&amp;lt;/sup&amp;gt;.&amp;lt;ref name=ClaytonSCTPLS96&amp;gt;Keith Clayton, 1996, &amp;quot;Fractals and the Fractal Dimension,&amp;quot; ''Basic Concepts in Nonlinear Dynamics and Chaos'' (workshop), Society for Chaos Theory in Psychology and the Life Sciences annual meeting, June 28, 1996, Berkeley, California, see [http://www.vanderbilt.edu/AnS/psychology/cogsci/chaos/workshop/Workshop.html], accessed 5 March 2015.&amp;lt;/ref&amp;gt; This equation is easily solved for D, yielding the ratio of logarithms (or [[natural logarithm]]s) appearing in the figures, and giving—in the Koch and other fractal cases—non-integer dimensions for these objects.&lt;br /&gt;
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In mathematical terms, the Hausdorff dimension generalizes the notion of the dimension of a real vector space. That is, the Hausdorff dimension of an n-dimensional inner product space equals n. This underlies the earlier statement that the Hausdorff dimension of a point is zero, of a line is one, etc., and that irregular sets can have noninteger Hausdorff dimensions. For instance, the Koch snowflake shown at right is constructed from an equilateral triangle; in each iteration, its component line segments are divided into 3 segments of unit length, the newly created middle segment is used as the base of a new equilateral triangle that points outward, and this base segment is then deleted to leave a final object from the iteration of unit length of 4. That is, after the first iteration, each original line segment has been replaced with N=4, where each self-similar copy is 1/S = 1/3 as long as the original. This equation is easily solved for D, yielding the ratio of logarithms (or natural logarithms) appearing in the figures, and giving—in the Koch and other fractal cases—non-integer dimensions for these objects.&lt;br /&gt;
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用数学术语来说，豪斯多夫维数概括了实向量空间维数的概念。也就是说，n 维内积空间的豪斯多夫维数等于 n。 这就是早期假设的基础，一个点的豪斯多夫维数是零，一条线是一等等，不规则集可以有非整数的豪斯多夫维数。例如，右边所示的 Koch 雪花是由一个正三角形构成的; 在每次迭代中，它的组成线段被分成单位长度的3段，新创建的中间线段被用作一个指向外部的新正三角形的基础，然后人们删除这个基础线段用来保留单位长度4的迭代中的最终对象。也就是说，在第一次迭代之后，每个原始线段都被替换为 N=4，其中每个自相似拷贝的长度是原始线段的1/S = 1/3 。这个方程很容易求解为 D，产生出现在图形中的对数(或自然对数)的比率，并给出——在 Koch 和其他分形情况下——这些对象的非整数维数。&lt;br /&gt;
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The Hausdorff dimension is a successor to the simpler, but usually equivalent, box-counting or [[Minkowski–Bouligand dimension]].&lt;br /&gt;
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The Hausdorff dimension is a successor to the simpler, but usually equivalent, box-counting or Minkowski–Bouligand dimension.&lt;br /&gt;
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豪斯多夫维数是更简单但通常等价的'''&amp;lt;font color = '#ff8000'&amp;gt;计盒维数box-counting&amp;lt;/font&amp;gt;'''或'''&amp;lt;font color = '#ff8000'&amp;gt;闵可夫斯基维数Minkowski-Bouligand&amp;lt;/font&amp;gt;'''的继承者。&lt;br /&gt;
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==Intuition概念==&lt;br /&gt;
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The intuitive concept of dimension of a geometric object ''X'' is the number of independent parameters one needs to pick out a unique point inside. However, any point specified by two parameters can be instead specified by one, because the [[cardinality]] of the [[real plane]] is equal to the cardinality of the [[real line]] (this can be seen by an [[Cantor's diagonal argument|argument]] involving interweaving the digits of two numbers to yield a single number encoding the same information). The example of a [[space-filling curve]] shows that one can even map the real line to the real plane [[Surjective function|surjectively]] (taking one real number into a pair of real numbers in a way so that all pairs of numbers are covered) and ''continuously'', so that a one-dimensional object completely fills up a higher-dimensional object.&lt;br /&gt;
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The intuitive concept of dimension of a geometric object X is the number of independent parameters one needs to pick out a unique point inside. However, any point specified by two parameters can be instead specified by one, because the cardinality of the real plane is equal to the cardinality of the real line (this can be seen by an argument involving interweaving the digits of two numbers to yield a single number encoding the same information). The example of a space-filling curve shows that one can even map the real line to the real plane surjectively (taking one real number into a pair of real numbers in a way so that all pairs of numbers are covered) and continuously, so that a one-dimensional object completely fills up a higher-dimensional object.&lt;br /&gt;
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几何对象X的尺寸的直观概念是指需要多少个独立参数才能找到一个独特的点。但是，任何由两个参数指定的点都可以由一个参数指定，因为为实平面的基数等于实线的基数(这可以通过交织两个数字以产生一个编码相同信息的单个数字看到)。'''&amp;lt;font color = '#ff8000'&amp;gt;皮亚诺曲线&amp;lt;/font&amp;gt;'''的例子表明，可以将实线完美和连续地映射到实平面(把一个实数转换成一对实数，从而覆盖所有实数对)，由此一维对象完全填充了一个高维对象。&lt;br /&gt;
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Every space filling curve hits some points multiple times, and does not have a continuous inverse. It is impossible to map two dimensions onto one in a way that is continuous and continuously invertible. The topological dimension, also called [[Lebesgue covering dimension]], explains why. This dimension is ''n'' if, in every covering of ''X'' by small open balls, there is at least one point where ''n''&amp;amp;nbsp;+&amp;amp;nbsp;1 balls overlap. For example, when one covers a line with short open intervals, some points must be covered twice, giving dimension&amp;amp;nbsp;''n''&amp;amp;nbsp;=&amp;amp;nbsp;1.&lt;br /&gt;
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Every space filling curve hits some points multiple times, and does not have a continuous inverse. It is impossible to map two dimensions onto one in a way that is continuous and continuously invertible. The topological dimension, also called Lebesgue covering dimension, explains why. This dimension is n if, in every covering of X by small open balls, there is at least one point where n&amp;amp;nbsp;+&amp;amp;nbsp;1 balls overlap. For example, when one covers a line with short open intervals, some points must be covered twice, giving dimension&amp;amp;nbsp;n&amp;amp;nbsp;=&amp;amp;nbsp;1.&lt;br /&gt;
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每条空间填充曲线都会多次击中某些点，且不存在连续的逆。将二维以连续和连续可逆的方式映射到一维是不可能的。'''&amp;lt;font color = '#ff8000'&amp;gt;拓扑维度 topological dimension&amp;lt;/font&amp;gt;'''，也被称为Lebesgue覆盖维数，解释了为什么。如果在 x 的每个小开球覆盖中，至少有一个点 n + 1个球重叠，这个维度是 n。例如，当用短的开区间覆盖一条线时，某些点必须被覆盖两次，给出维数''n''&amp;amp;nbsp;=&amp;amp;nbsp;1。&lt;br /&gt;
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But topological dimension is a very crude measure of the local size of a space (size near a point). A curve that is almost space-filling can still have topological dimension one, even if it fills up most of the area of a region. A [[fractal]] has an integer topological dimension, but in terms of the amount of space it takes up, it behaves like a higher-dimensional space.&lt;br /&gt;
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But topological dimension is a very crude measure of the local size of a space (size near a point). A curve that is almost space-filling can still have topological dimension one, even if it fills up most of the area of a region. A fractal has an integer topological dimension, but in terms of the amount of space it takes up, it behaves like a higher-dimensional space.&lt;br /&gt;
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但是，拓扑维度是对空间局部尺寸(点附近的尺寸)的一个非常粗略的度量。一条几乎是空间填充的曲线仍然可以有一维拓扑，即使它填充了一个区域的大部分面积。分形具有整数的拓扑维数，但就其所占的空间量而言，它看起来像一个更高维的空间。&lt;br /&gt;
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The Hausdorff dimension measures the local size of a space taking into account the distance between points, the [[metric space|metric]]. Consider the number ''N''(''r'') of [[ball (mathematics)|balls]] of radius at most ''r'' required to cover ''X'' completely. When ''r'' is very small, ''N''(''r'') grows polynomially with 1/''r''. For a sufficiently well-behaved  ''X'', the Hausdorff dimension is the unique number ''d'' such that N(''r'') grows as 1/''r&amp;lt;sup&amp;gt;d&amp;lt;/sup&amp;gt;'' as ''r'' approaches zero. More precisely, this defines the [[Minkowski–Bouligand dimension|box-counting dimension]], which equals the Hausdorff dimension when the value ''d'' is a critical boundary between growth rates that are insufficient to cover the space, and growth rates that are overabundant.&lt;br /&gt;
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The Hausdorff dimension measures the local size of a space taking into account the distance between points, the metric. Consider the number N(r) of balls of radius at most r required to cover X completely. When r is very small, N(r) grows polynomially with 1/r. For a sufficiently well-behaved  X, the Hausdorff dimension is the unique number d such that N(r) grows as 1/r&amp;lt;sup&amp;gt;d&amp;lt;/sup&amp;gt; as r approaches zero. More precisely, this defines the box-counting dimension, which equals the Hausdorff dimension when the value d is a critical boundary between growth rates that are insufficient to cover the space, and growth rates that are overabundant.&lt;br /&gt;
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豪斯多夫维数测量一个空间的局部大小时，会考虑到点之间距离的度量。考虑半径最大为 r 的球数 ''N'' (r) ，需要完全覆盖 ''X''。当 r 很小时，n (r)以1/''r'' 增长多项式。对于一个表现足够好的 ''X''，豪斯多夫维数是唯一的数 d，这样当 r 趋近于零时， N(r)增长为1/r&amp;lt;sup&amp;gt;d&amp;lt;/sup&amp;gt; 。更确切地说，这定义了盒子计数维度，当值 d 是不足以覆盖空间的增长率和过度充裕的增长率之间的关键边界时，它等于豪斯多夫维数。&lt;br /&gt;
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For shapes that are smooth, or shapes with a small number of corners, the shapes of traditional geometry and science, the Hausdorff dimension is an integer agreeing with the topological dimension. But [[Benoit Mandelbrot]] observed that [[fractal]]s, sets with noninteger Hausdorff dimensions, are found everywhere in nature. He observed that the proper idealization of most rough shapes you see around you is not in terms of smooth idealized shapes, but in terms of fractal idealized shapes:&lt;br /&gt;
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For shapes that are smooth, or shapes with a small number of corners, the shapes of traditional geometry and science, the Hausdorff dimension is an integer agreeing with the topological dimension. But Benoit Mandelbrot observed that fractals, sets with noninteger Hausdorff dimensions, are found everywhere in nature. He observed that the proper idealization of most rough shapes you see around you is not in terms of smooth idealized shapes, but in terms of fractal idealized shapes:&lt;br /&gt;
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对于光滑的形状，或者有少量棱角的形状，传统几何和科学的形状，豪斯多夫维数是一个整数，与拓扑维度一致。但是伯努·曼德布洛特观察到分形---- 具有非整数豪斯多夫维数的集合---- 在自然界中随处可见。他观察到，我们周围大多数粗糙形状的理想化不是光滑的理想化形状，而是分形理想化形状:&lt;br /&gt;
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&amp;lt;blockquote&amp;gt;Clouds are not spheres, mountains are not cones, coastlines are not circles, and bark is not smooth, nor does lightning travel in a straight line.&amp;lt;ref name=&amp;quot;mandelbrot&amp;quot;&amp;gt;{{cite book   | last = Mandelbrot   | first = Benoît   | authorlink = Benoit Mandelbrot   | title = The Fractal Geometry of Nature   | publisher = W. H. Freeman   | series = Lecture notes in mathematics 1358   | year = 1982   | doi =    | isbn = 0-7167-1186-9   | url-access = registration   | url = https://archive.org/details/fractalgeometryo00beno   }}&amp;lt;/ref&amp;gt;&amp;lt;/blockquote&amp;gt;&lt;br /&gt;
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&amp;lt;blockquote&amp;gt;Clouds are not spheres, mountains are not cones, coastlines are not circles, and bark is not smooth, nor does lightning travel in a straight line.&amp;lt;/blockquote&amp;gt;&lt;br /&gt;
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&amp;lt;blockquote&amp;gt;云不是球体，山不是锥体，海岸线不是圆圈，树皮不平滑，闪电也不是直线运动。 &amp;lt;/blockquote&amp;gt;&lt;br /&gt;
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For fractals that occur in nature, the Hausdorff and [[Minkowski–Bouligand dimension|box-counting dimension]] coincide. The [[packing dimension]] is yet another similar notion which gives the same value for many shapes, but there are well documented exceptions where all these dimensions differ.&lt;br /&gt;
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For fractals that occur in nature, the Hausdorff and box-counting dimension coincide. The packing dimension is yet another similar notion which gives the same value for many shapes, but there are well documented exceptions where all these dimensions differ.&lt;br /&gt;
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对于自然界中出现的分形，豪斯多夫维数和盒计数维数是一致的。封装尺寸是另一个类似的概念，它为许多形状提供相同的值，但是在所有这些尺寸不同的情况，都做了很好的说明。&lt;br /&gt;
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==Formal definitions形式化定义==&lt;br /&gt;
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===Hausdorff content豪斯多夫集===&lt;br /&gt;
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Let ''X'' be a [[metric space]]. If ''S'' ⊂ ''X'' and ''d'' ∈ [0, ∞), the ''d''-dimensional '''unlimited Hausdorff content''' of ''S'' is defined by&lt;br /&gt;
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Let X be a metric space. If S ⊂ X and d ∈ [0, ∞), the d-dimensional unlimited Hausdorff content of S is defined by&lt;br /&gt;
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设 ''X''是度量空间。若''S'' ⊂ ''X'' 和 ''d'' ∈ [0, ∞) ，则 ''S'' 的''d''维无限 豪斯多夫集定义为&lt;br /&gt;
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:&amp;lt;math&amp;gt;C_H^d(S):=\inf\Bigl\{\sum_i r_i^d:\text{ there is a cover of } S\text{ by balls with radii }r_i&amp;gt;0\Bigr\}.&amp;lt;/math&amp;gt;&lt;br /&gt;
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&amp;lt;math&amp;gt;C_H^d(S):=\inf\Bigl\{\sum_i r_i^d:\text{ there is a cover of } S\text{ by balls with radii }r_i&amp;gt;0\Bigr\}.&amp;lt;/math&amp;gt;&lt;br /&gt;
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&amp;lt;math&amp;gt;C_H^d(S):=\inf\Bigl\{\sum_i r_i^d:\text{ there is a cover of } S\text{ by balls with radii }r_i&amp;gt;0\Bigr\}.&amp;lt;/math&amp;gt;&lt;br /&gt;
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In other words, &amp;lt;math&amp;gt;C_H^d(S)&amp;lt;/math&amp;gt; is the [[infimum]] of the set of numbers &amp;lt;math&amp;gt;\delta \geq 0&amp;lt;/math&amp;gt; such that there is some (indexed) collection of [[ball (mathematics)|ball]]s &amp;lt;math&amp;gt;\{B(x_i,r_i):i\in I\}&amp;lt;/math&amp;gt; covering ''S'' with ''r&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;''&amp;amp;nbsp;&amp;gt;&amp;amp;nbsp;0 for each ''i''&amp;amp;nbsp;∈&amp;amp;nbsp;''I'' that satisfies &amp;lt;math&amp;gt;\sum_{i\in I} r_i^d&amp;lt;\delta &amp;lt;/math&amp;gt;. (Here, we use the standard convention that [[infimum|inf&amp;amp;nbsp;Ø&amp;amp;nbsp;=&amp;amp;nbsp;∞]].)&lt;br /&gt;
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In other words, &amp;lt;math&amp;gt;C_H^d(S)&amp;lt;/math&amp;gt; is the infimum of the set of numbers &amp;lt;math&amp;gt;\delta \geq 0&amp;lt;/math&amp;gt; such that there is some (indexed) collection of balls &amp;lt;math&amp;gt;\{B(x_i,r_i):i\in I\}&amp;lt;/math&amp;gt; covering S with r&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;&amp;amp;nbsp;&amp;gt;&amp;amp;nbsp;0 for each i&amp;amp;nbsp;∈&amp;amp;nbsp;I that satisfies &amp;lt;math&amp;gt;\sum_{i\in I} r_i^d&amp;lt;\delta &amp;lt;/math&amp;gt;. (Here, we use the standard convention that inf&amp;amp;nbsp;Ø&amp;amp;nbsp;=&amp;amp;nbsp;∞.)&lt;br /&gt;
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换句话说，&amp;lt;math&amp;gt;C_H^d(S)&amp;lt;/math&amp;gt; 是数字集合&amp;lt;math&amp;gt;\delta \geq 0&amp;lt;/math&amp;gt;的下确界，使得在 ''i''&amp;amp;nbsp;∈&amp;amp;nbsp中存在一些球集合 &amp;lt;math&amp;gt;\{B(x_i,r_i):i\in I\}&amp;lt;/math&amp;gt;  i 包含 s，对于每个 ''r&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;''&amp;amp;nbsp;&amp;gt;&amp;amp;nbsp;0 满足 i 中的和&amp;lt;math&amp;gt;\sum_{i\in I} r_i^d&amp;lt;\delta &amp;lt;/math&amp;gt; (在这里，我们使用inf&amp;amp;nbsp;Ø&amp;amp;nbsp;=&amp;amp;nbsp;∞ )的标准约定。&lt;br /&gt;
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===Hausdorff measurement豪斯多夫分形测量===&lt;br /&gt;
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The Hausdorff outer measure is different from the unbounded Hausdorf content in that rather than considering all possible coverings of ''S'', we see what happens when the sizes of the balls go to zero. This is  for &amp;lt;math&amp;gt;d \geq 0 &amp;lt;/math&amp;gt;, we define the ''d''-dimensional Hausdorff outer measure of ''S'' as&lt;br /&gt;
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The Hausdorff outer measure is different from the unbounded Hausdorf content in that rather than considering all possible coverings of S, we see what happens when the sizes of the balls go to zero. This is  for &amp;lt;math&amp;gt;d \geq 0 &amp;lt;/math&amp;gt;, we define the d-dimensional Hausdorff outer measure of S as&lt;br /&gt;
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豪斯多夫外测度不同于无界的豪斯多夫，因为我们不考虑 s 的所有可能，我们看到当球的大小变为零时会发生什么。对于 &amp;lt;math&amp;gt;d \geq 0 &amp;lt;/math&amp;gt;，我们定义了  ''S''的 ''d''维豪斯多夫Hausdorff 外测度为&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt; \mathcal{H}^d(S):=\lim_{r \to 0} \inf\Bigl\{\sum_i r_i^d:\text{ there is a cover of } S\text{ by balls with radii } 0 &amp;lt; r_i &amp;lt; r\Bigr\}.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \mathcal{H}^d(S):=\lim_{r \to 0} \inf\Bigl\{\sum_i r_i^d:\text{ there is a cover of } S\text{ by balls with radii } 0 &amp;lt; r_i &amp;lt; r\Bigr\}.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \mathcal{H}^d(S):=\lim_{r \to 0} \inf\Bigl\{\sum_i r_i^d:\text{有一个面} S\text{ 球 } 0 &amp;lt; r_i &amp;lt; r\Bigr\}.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
===Hausdorff dimension豪斯多夫维数===&lt;br /&gt;
&lt;br /&gt;
The '''Hausdorff dimension''' of ''X'' is defined by&lt;br /&gt;
&lt;br /&gt;
The Hausdorff dimension of X is defined by&lt;br /&gt;
&lt;br /&gt;
X 的豪斯多夫维数定义为&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt;\dim_{\operatorname{H}}(X):=\inf\{d\ge 0: \mathcal{H}^d(X)=0\}.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt;\dim_{\operatorname{H}}(X):=\inf\{d\ge 0: \mathcal{H}^d(X)=0\}.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Equivalently, dim&amp;lt;sub&amp;gt;H&amp;lt;/sub&amp;gt;(''X'') may be defined as the [[infimum]] of the set of ''d'' ∈ [0, ∞) such that the ''d''-dimensional [[Hausdorff measure]] of ''X'' is zero. This is the same as the supremum of the set of ''d''&amp;amp;nbsp;∈&amp;amp;nbsp;[0,&amp;amp;nbsp;∞) such that the ''d''-dimensional Hausdorff measure of ''X'' is infinite (except that when this latter set of numbers ''d'' is empty the Hausdorff dimension is zero).&lt;br /&gt;
&lt;br /&gt;
Equivalently, dim&amp;lt;sub&amp;gt;H&amp;lt;/sub&amp;gt;(X) may be defined as the infimum of the set of d ∈ [0, ∞) such that the d-dimensional Hausdorff measure of X is zero. This is the same as the supremum of the set of d&amp;amp;nbsp;∈&amp;amp;nbsp;[0,&amp;amp;nbsp;∞) such that the d-dimensional Hausdorff measure of X is infinite (except that when this latter set of numbers d is empty the Hausdorff dimension is zero).&lt;br /&gt;
&lt;br /&gt;
等价地，dim &amp;lt;sub&amp;gt;H&amp;lt;/sub&amp;gt;(''X'')可定义为 ''d'' ∈ [0, ∞) 集的下确界，使得''X'' 的''d''-维 [[豪斯多夫测度]] 为零。这与 ''d''&amp;amp;nbsp;∈&amp;amp;nbsp;[0,&amp;amp;nbsp;∞)的集合的上确界相同，因此''X''的 d 维豪斯多夫测度是无限的(除非后一个集合 ''d'' 是空的，豪斯多夫维数为零)。&lt;br /&gt;
&lt;br /&gt;
==Examples实例==&lt;br /&gt;
&lt;br /&gt;
[[Image:Sierpinski deep.svg|thumb|250px|Dimension of a further [[fractal]] example. The [[Sierpinski triangle]], an object with Hausdorff dimension of log(3)/log(2)≈1.58.&amp;lt;ref name=ClaytonSCTPLS96/&amp;gt;]]&lt;br /&gt;
&lt;br /&gt;
Dimension of a further [[fractal example. The Sierpinski triangle, an object with Hausdorff dimension of log(3)/log(2)≈1.58.]]&lt;br /&gt;
&lt;br /&gt;
[[Image:谢尔宾斯基三角形 deep.svg|thumb|250px|进一步的[[分形维数]]的例子，进一步的分形维数的例子是谢尔宾斯基三角形，它是一个豪斯多夫维数为log(3)/log(2)≈1.58.&amp;lt;ref name=ClaytonSCTPLS96/&amp;gt;的物体]]&lt;br /&gt;
&lt;br /&gt;
* [[Countable set]]s have Hausdorff dimension 0.&amp;lt;ref name=&amp;quot;schleicher&amp;quot;&amp;gt;{{cite journal |last1=Schleicher |first1=Dierk |title=Hausdorff Dimension, Its Properties, and Its Surprises |journal=The American Mathematical Monthly |date=June 2007 |volume=114 |issue=6 |pages=509–528 |doi=10.1080/00029890.2007.11920440 |language=en |issn=0002-9890|arxiv=math/0505099 }}&amp;lt;/ref&amp;gt;&lt;br /&gt;
*[[可数集]]拥有豪斯多夫维数0.&amp;lt;ref name=&amp;quot;schleicher&amp;quot;&amp;gt;{{cite journal |last1=Schleicher |first1=Dierk |title=豪斯多夫维数, Its Properties, and Its Surprises |journal=The American Mathematical Monthly美国数学期刊 |date=June 2007 |volume=114 |issue=6 |pages=509–528 |doi=10.1080/00029890.2007.11920440 |language=en |issn=0002-9890|arxiv=math/0505099 }}&amp;lt;/ref&amp;gt;&lt;br /&gt;
* The [[Euclidean space]] ℝ&amp;lt;sup&amp;gt;''n''&amp;lt;/sup&amp;gt; has Hausdorff dimension ''n'', and the circle '''S'''&amp;lt;sup&amp;gt;1&amp;lt;/sup&amp;gt; has Hausdorff dimension 1.&amp;lt;ref name=&amp;quot;schleicher&amp;quot; /&amp;gt;&lt;br /&gt;
*[[教育空间]] ℝ&amp;lt;sup&amp;gt;''n''&amp;lt;/sup&amp;gt; 有豪斯多夫维数 ''n''，循环'''S'''&amp;lt;sup&amp;gt;1&amp;lt;/sup&amp;gt; 拥有豪斯多夫维数1.&amp;lt;ref name=&amp;quot;schleicher&amp;quot; /&amp;gt;&lt;br /&gt;
* [[Fractal]]s often are spaces whose Hausdorff dimension strictly exceeds the [[topological dimension]].&amp;lt;ref name=&amp;quot;mandelbrot&amp;quot; /&amp;gt; For example, the [[Cantor set]], a zero-dimensional topological space, is a union of two copies of itself, each copy shrunk by a factor 1/3; hence, it can be shown that its Hausdorff dimension is ln(2)/ln(3)&amp;amp;nbsp;≈&amp;amp;nbsp;0.63.&amp;lt;ref&amp;gt;{{cite book | last=Falconer | first = Kenneth |title=Fractal Geometry: Mathematical Foundations and Applications | publisher=[[John Wiley and Sons]] | edition=2nd | year=2003}}&amp;lt;/ref&amp;gt; The [[Sierpinski triangle]] is a union of three copies of itself, each copy shrunk by a factor of&amp;amp;nbsp;1/2; this yields a Hausdorff dimension of ln(3)/ln(2)&amp;amp;nbsp;≈&amp;amp;nbsp;1.58.&amp;lt;ref name=CampbellAnnenberg15/&amp;gt; These Hausdorff dimensions are related to the &amp;quot;critical exponent&amp;quot; of the [[Master theorem (analysis of algorithms)|Master theorem]] for solving [[Recurrence relation|recurrence relations]] in the [[analysis of algorithms]].&lt;br /&gt;
*[[分形]]一般是那些豪斯多夫维数直接超过其拓扑维数的空间。例如[[康托尔集]]是一个o维拓扑空间，由两个自己复制而成，每一个复制品都是原来的三分之一，因此它的豪斯多夫维数是 ln(2)/ln(3)&amp;amp;nbsp;≈&amp;amp;nbsp;0.63。&amp;lt;ref&amp;gt;{{cite book | last=Falconer | first = Kenneth |title=Fractal Geometry: Mathematical Foundations and Applications | publisher=[[John Wiley and Sons]] | edition=2nd | year=2003}}&amp;lt;/ref&amp;gt;一个[[谢尔宾斯基三角]]是他自身三个复制的组合。每一个是原来的&amp;amp;nbsp;1/2，它的豪斯多夫维数ln(3)/ln(2)&amp;amp;nbsp;≈&amp;amp;nbsp;1.58。&amp;lt;ref name=CampbellAnnenberg15/&amp;gt;在递归算法中解决递归关系时，这些豪斯多夫维数与[[算法分析主定理]]的临界指标相联系。&lt;br /&gt;
* [[Space-filling curve]]s like the [[Peano curve]] have the same Hausdorff dimension as the space they fill.&lt;br /&gt;
*[[空间填充曲线]]拥有和他们填充空间同样的豪斯多夫维数，如[[皮亚诺曲线]]。&lt;br /&gt;
* The trajectory of [[Brownian motion]] in dimension 2 and above is conjectured to be Hausdorff dimension 2.&amp;lt;ref&amp;gt;{{cite book | last=Morters | first=Peres | title= Brownian Motion | publisher=[[Cambridge University Press]] | year=2010 }}&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
[[image:Great Britain Hausdorff.svg|thumb|250px|Estimating the Hausdorff dimension of the [[How Long Is the Coast of Britain? Statistical Self-Similarity and Fractional Dimension|coast of Great Britain]]]]&lt;br /&gt;
&lt;br /&gt;
coast of Great Britain]]&lt;br /&gt;
&lt;br /&gt;
[[大不列颠海岸&lt;br /&gt;
&lt;br /&gt;
* 刘易斯·弗赖伊·理查森[[Lewis Fry Richardson]] has performed detailed experiments to measure the approximate Hausdorff dimension for various coastlines. His results have varied from 1.02 for the coastline of [[South Africa]] to 1.25 for the west coast of [[Great Britain]].&amp;lt;ref name=&amp;quot;mandelbrot&amp;quot; /&amp;gt;&lt;br /&gt;
*刘易斯·弗赖伊·理查森（Lewis Fry Richardson）已经通过豪斯多夫维数去测量了很多海岸线。它的结果涵盖从1.02的南非海岸线到1.25的大英帝国西海岸模型。]]&lt;br /&gt;
&lt;br /&gt;
==Properties of Hausdorff dimension豪斯多夫维数特性==&lt;br /&gt;
&lt;br /&gt;
{{refimprove section|date=March 2015}}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
=== Hausdorff dimension and inductive dimension 豪斯多夫维数和归纳维数===&lt;br /&gt;
&lt;br /&gt;
Let ''X'' be an arbitrary [[Separable space|separable]] metric space. There is a [[topology|topological]] notion of [[inductive dimension]] for ''X'' which is defined recursively. It is always an integer (or +∞) and is denoted dim&amp;lt;sub&amp;gt;ind&amp;lt;/sub&amp;gt;(''X'').&lt;br /&gt;
&lt;br /&gt;
Let X be an arbitrary separable metric space. There is a topological notion of inductive dimension for X which is defined recursively. It is always an integer (or +∞) and is denoted dim&amp;lt;sub&amp;gt;ind&amp;lt;/sub&amp;gt;(X).&lt;br /&gt;
&lt;br /&gt;
设''X'' 是[[任意可分度量空间]]。对于''X'' 有一个递归定义的归纳维数拓扑概念。它总是一个整数(或 + ∞) ，记为dim&amp;lt;sub&amp;gt;ind&amp;lt;/sub&amp;gt;(''X'')。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
'''Theorem'''. Suppose ''X'' is non-empty. Then &lt;br /&gt;
&lt;br /&gt;
Theorem. Suppose X is non-empty. Then &lt;br /&gt;
&lt;br /&gt;
'''定理'''：假设''X'' 是非空的, 那么&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt; \dim_{\mathrm{Haus}}(X) \geq \dim_{\operatorname{ind}}(X). &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \dim_{\mathrm{Haus}}(X) \geq \dim_{\operatorname{ind}}(X). &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Moreover,&lt;br /&gt;
&lt;br /&gt;
Moreover,&lt;br /&gt;
&lt;br /&gt;
此外,&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \inf_Y \dim_{\operatorname{Haus}}(Y) =\dim_{\operatorname{ind}}(X), &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \inf_Y \dim_{\operatorname{Haus}}(Y) =\dim_{\operatorname{ind}}(X), &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
where ''Y'' ranges over metric spaces [[homeomorphic]] to ''X''. In other words, ''X'' and ''Y'' have the same underlying set of points and the metric ''d''&amp;lt;sub&amp;gt;''Y''&amp;lt;/sub&amp;gt; of ''Y'' is topologically equivalent to ''d''&amp;lt;sub&amp;gt;''X''&amp;lt;/sub&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
where Y ranges over metric spaces homeomorphic to X. In other words, X and Y have the same underlying set of points and the metric d&amp;lt;sub&amp;gt;Y&amp;lt;/sub&amp;gt; of Y is topologically equivalent to d&amp;lt;sub&amp;gt;X&amp;lt;/sub&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
其中''Y''是度量空间同胚到 ''X''的范围。换句话说， ''X''和 ''Y''具有相同的基本点集，''Y''的度量''d''&amp;lt;sub&amp;gt;''Y''&amp;lt;/sub&amp;gt; 拓扑等价于''d''&amp;lt;sub&amp;gt;''X''&amp;lt;/sub&amp;gt;。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
These results were originally established by [[Edward Szpilrajn]] (1907–1976), e.g., see Hurewicz and Wallman, Chapter VII.{{full citation needed|date=March 2015}}&lt;br /&gt;
&lt;br /&gt;
These results were originally established by Edward Szpilrajn (1907–1976), e.g., see Hurewicz and Wallman, Chapter VII.&lt;br /&gt;
&lt;br /&gt;
这些结果最初是由 [[Edward Szpilrajn]] (1907–1976)建立的,  参见 Hurewicz and Wallman, Chapter VII.{{full citation needed|date=March 2015}}第七章。&lt;br /&gt;
&lt;br /&gt;
=== Hausdorff dimension and Minkowski dimension 豪斯多夫维数和闵可夫斯基维度===&lt;br /&gt;
&lt;br /&gt;
The [[Minkowski dimension]] is similar to, and at least as large as, the Hausdorff dimension, and they are equal in many situations. However, the set of [[rational number|rational]] points in [0, 1] has Hausdorff dimension zero and Minkowski dimension one. There are also compact sets for which the Minkowski dimension is strictly larger than the Hausdorff dimension.&lt;br /&gt;
&lt;br /&gt;
The Minkowski dimension is similar to, and at least as large as, the Hausdorff dimension, and they are equal in many situations. However, the set of rational points in [0, 1] has Hausdorff dimension zero and Minkowski dimension one. There are also compact sets for which the Minkowski dimension is strictly larger than the Hausdorff dimension.&lt;br /&gt;
&lt;br /&gt;
[[闵可夫斯基维数]]与豪斯多夫维数相似，至少和它一样大，而且在许多情况下是相等的。然而，[0,1]中有理点集的豪斯多夫维数为0，闵可夫斯基维数为1。还有一些紧集的闵可夫斯基维数严格大于豪斯多夫维数。&lt;br /&gt;
&lt;br /&gt;
=== Hausdorff dimensions and Frostman measures 豪斯多夫维度和弗洛斯曼测度===&lt;br /&gt;
&lt;br /&gt;
If there is a [[measure (mathematics)|measure]] μ defined on [[Borel measure|Borel]] subsets of a metric space ''X'' such that ''μ''(''X'') &amp;gt; 0 and ''μ''(''B''(''x'', ''r'')) ≤ ''r&amp;lt;sup&amp;gt;s&amp;lt;/sup&amp;gt;'' holds for some constant ''s'' &amp;gt; 0 and for every ball ''B''(''x'', ''r'') in ''X'', then dim&amp;lt;sub&amp;gt;Haus&amp;lt;/sub&amp;gt;(''X'') ≥ ''s''. A partial converse is provided by [[Frostman's lemma]].{{citation needed|date=March 2015}}&amp;lt;ref&amp;gt;This Wikipedia article also discusses further useful characterizations of the Hausdorff dimension.{{clarify|date=March 2015}}&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
If there is a measure μ defined on Borel subsets of a metric space X such that μ(X) &amp;gt; 0 and μ(B(x, r)) ≤ r&amp;lt;sup&amp;gt;s&amp;lt;/sup&amp;gt; holds for some constant s &amp;gt; 0 and for every ball B(x, r) in X, then dim&amp;lt;sub&amp;gt;Haus&amp;lt;/sub&amp;gt;(X) ≥ s. A partial converse is provided by Frostman's lemma.&lt;br /&gt;
&lt;br /&gt;
如果在度量空间 ''X'' 的 Borel 子集上定义一个测度 μ，使得''μ''(''X'') &amp;gt; 0 和''μ''(''B''(''x'', ''r'')) ≤ ''r&amp;lt;sup&amp;gt;s&amp;lt;/sup&amp;gt;''，对于某个常数 ''s'' &amp;gt; 0  和 ''X'' 中的每个球 ''B''(''x'', ''r'') 成立，则 dim&amp;lt;sub&amp;gt;Haus&amp;lt;/sub&amp;gt;(''X'') ≥ ''s'' 。 部分逆向转换由弗洛斯曼引理定义。&lt;br /&gt;
&lt;br /&gt;
=== Behaviour under unions and products ===&lt;br /&gt;
&lt;br /&gt;
If &amp;lt;math&amp;gt;X=\bigcup_{i\in I}X_i&amp;lt;/math&amp;gt; is a finite or countable union, then&lt;br /&gt;
&lt;br /&gt;
If &amp;lt;math&amp;gt;X=\bigcup_{i\in I}X_i&amp;lt;/math&amp;gt; is a finite or countable union, then&lt;br /&gt;
&lt;br /&gt;
如果 &amp;lt;math&amp;gt;X=\bigcup_{i\in I}X_i&amp;lt;/math&amp;gt; 是一个有限或可数的联合，则&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \dim_{\operatorname{Haus}}(X) =\sup_{i\in I} \dim_{\operatorname{Haus}}(X_i).&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \dim_{\operatorname{Haus}}(X) =\sup_{i\in I} \dim_{\operatorname{Haus}}(X_i).&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
This can be verified directly from the definition.&lt;br /&gt;
&lt;br /&gt;
This can be verified directly from the definition.&lt;br /&gt;
&lt;br /&gt;
这可以直接从定义得到验证。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
If ''X'' and ''Y'' are non-empty metric spaces, then the Hausdorff dimension of their product satisfies&amp;lt;ref&amp;gt;{{cite journal |author=Marstrand, J. M. |title=The dimension of Cartesian product sets |journal=Proc. Cambridge Philos. Soc. |volume=50 |issue=3 |pages=198–202 |year=1954 |doi=10.1017/S0305004100029236 |bibcode = 1954PCPS...50..198M }}&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
If X and Y are non-empty metric spaces, then the Hausdorff dimension of their product satisfies&lt;br /&gt;
&lt;br /&gt;
如果 ''X'' 和''Y''是非空度量空间，那么它们乘积的豪斯多夫维数满足&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt; \dim_{\operatorname{Haus}}(X\times Y)\ge \dim_{\operatorname{Haus}}(X)+ \dim_{\operatorname{Haus}}(Y).&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \dim_{\operatorname{Haus}}(X\times Y)\ge \dim_{\operatorname{Haus}}(X)+ \dim_{\operatorname{Haus}}(Y).&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
This inequality can be strict. It is possible to find two sets of dimension 0 whose product has dimension 1.&amp;lt;ref&amp;gt;{{cite book  | last = Falconer  | first = Kenneth J.  | title = Fractal geometry. Mathematical foundations and applications  | publisher = John Wiley &amp;amp; Sons, Inc., Hoboken, New Jersey  | year = 2003  | doi =   | isbn = }}&amp;lt;/ref&amp;gt; In the opposite direction, it is known that when ''X'' and ''Y'' are Borel subsets of '''R'''&amp;lt;sup&amp;gt;''n''&amp;lt;/sup&amp;gt;, the Hausdorff dimension of ''X'' × ''Y'' is bounded from above by the Hausdorff dimension of ''X'' plus the [[packing dimension|upper packing dimension]] of ''Y''. These facts are discussed in Mattila (1995).&lt;br /&gt;
&lt;br /&gt;
This inequality can be strict. It is possible to find two sets of dimension 0 whose product has dimension 1. In the opposite direction, it is known that when X and Y are Borel subsets of R&amp;lt;sup&amp;gt;n&amp;lt;/sup&amp;gt;, the Hausdorff dimension of X × Y is bounded from above by the Hausdorff dimension of X plus the upper packing dimension of Y. These facts are discussed in Mattila (1995).&lt;br /&gt;
&lt;br /&gt;
这种不平等可以是严格的。有可能找到两个维数为0的集合，其乘积的维数为1。相反，我们知道当''X''和''Y''是 '''R'''&amp;lt;sup&amp;gt;''n''&amp;lt;/sup&amp;gt;的 Borel 子集时， ''X'' × ''Y''的豪斯多夫维数从上面以 ''X''的豪斯多夫维数加上 ''Y''的上填充维数为界。Mattila (1995)曾就这些情况进行了讨论。&lt;br /&gt;
&lt;br /&gt;
==Self-similar sets自相似集合==&lt;br /&gt;
&lt;br /&gt;
{{refimprove section|date=March 2015}}&lt;br /&gt;
&lt;br /&gt;
Many sets defined by a self-similarity condition have dimensions which can be determined explicitly. Roughly, a set ''E'' is self-similar if it is the fixed point of a set-valued transformation ψ, that is ψ(''E'') = ''E'', although the exact definition is given below.&lt;br /&gt;
&lt;br /&gt;
Many sets defined by a self-similarity condition have dimensions which can be determined explicitly. Roughly, a set E is self-similar if it is the fixed point of a set-valued transformation ψ, that is ψ(E) = E, although the exact definition is given below.&lt;br /&gt;
&lt;br /&gt;
许多由自相似条件定义的集合具有可以显式确定的维数。粗略地说，如果集合''E''是集值ψ变换的不动点，即ψ(''E'') = ''E''， 则它是自相似的，尽管下面给出了确切的定义。&lt;br /&gt;
&lt;br /&gt;
&amp;lt;blockquote&amp;gt;'''Theorem'''. Suppose&lt;br /&gt;
&lt;br /&gt;
&amp;lt;blockquote&amp;gt;Theorem. Suppose&lt;br /&gt;
&lt;br /&gt;
&amp;lt;blockquote&amp;gt;'''定理'''：假设&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt; \psi_i: \mathbf{R}^n \rightarrow \mathbf{R}^n, \quad i=1, \ldots , m &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \psi_i: \mathbf{R}^n \rightarrow \mathbf{R}^n, \quad i=1, \ldots , m &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
are [[Contraction mapping|contractive]] mappings on '''R'''&amp;lt;sup&amp;gt;''n''&amp;lt;/sup&amp;gt; with contraction constant ''r&amp;lt;sub&amp;gt;j&amp;lt;/sub&amp;gt;'' &amp;lt; 1. Then there is a unique ''non-empty'' compact set ''A'' such that&lt;br /&gt;
&lt;br /&gt;
are contractive mappings on R&amp;lt;sup&amp;gt;n&amp;lt;/sup&amp;gt; with contraction constant r&amp;lt;sub&amp;gt;j&amp;lt;/sub&amp;gt; &amp;lt; 1. Then there is a unique non-empty compact set A such that&lt;br /&gt;
&lt;br /&gt;
是'''R'''&amp;lt;sup&amp;gt;''n''&amp;lt;/sup&amp;gt;上的压缩常数''r&amp;lt;sub&amp;gt;j&amp;lt;/sub&amp;gt;'&amp;lt; 1的压缩映射。则有一个唯一的非空紧集A &lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt; A = \bigcup_{i=1}^m \psi_i (A). &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; A = \bigcup_{i=1}^m \psi_i (A). &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&amp;lt;/blockquote&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;/blockquote&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The theorem follows from [[Stefan Banach]]'s [[Contractive mapping theorem|contractive mapping fixed point theorem]] applied to the complete metric space of non-empty compact subsets of '''R'''&amp;lt;sup&amp;gt;''n''&amp;lt;/sup&amp;gt; with the [[Hausdorff distance]].&amp;lt;ref&amp;gt;{{cite book |author=Falconer, K. J. |title=The Geometry of Fractal Sets |publisher=Cambridge University Press |location=Cambridge, UK |year=1985 |isbn=0-521-25694-1 |chapter=Theorem 8.3}}&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
The theorem follows from Stefan Banach's contractive mapping fixed point theorem applied to the complete metric space of non-empty compact subsets of R&amp;lt;sup&amp;gt;n&amp;lt;/sup&amp;gt; with the Hausdorff distance.&lt;br /&gt;
&lt;br /&gt;
这个定理来源于 Stefan Banach 的压缩映射不动点定理，该定理应用于 具有豪斯多夫距离的'''R'''&amp;lt;sup&amp;gt;''n''&amp;lt;/sup&amp;gt; 的非空紧子集的完整度量空间。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
===The open set condition开集条件===&lt;br /&gt;
&lt;br /&gt;
To determine the dimension of the self-similar set ''A'' (in certain cases), we need a technical condition called the ''open set condition'' (OSC) on the sequence of contractions ψ&amp;lt;sub&amp;gt;''i''&amp;lt;/sub&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
To determine the dimension of the self-similar set A (in certain cases), we need a technical condition called the open set condition (OSC) on the sequence of contractions ψ&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
为了确定自相似集''A'' 的维数(在某些情况下) ，我们需要一个关于收缩序列的称为''开集条件''(OSC)的技术条件ψ&amp;lt;sub&amp;gt;''i''&amp;lt;/sub&amp;gt;。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
There is a relatively compact open set ''V'' such that&lt;br /&gt;
&lt;br /&gt;
There is a relatively compact open set V such that&lt;br /&gt;
&lt;br /&gt;
有一个相对紧的开集''V''&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt; \bigcup_{i=1}^m\psi_i (V) \subseteq V, &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \bigcup_{i=1}^m\psi_i (V) \subseteq V, &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
where the sets in union on the left are pairwise [[disjoint sets|disjoint]].&lt;br /&gt;
&lt;br /&gt;
where the sets in union on the left are pairwise disjoint.&lt;br /&gt;
&lt;br /&gt;
左边并集的集合成对不相交。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The open set condition is a separation condition that ensures the images ψ&amp;lt;sub&amp;gt;''i''&amp;lt;/sub&amp;gt;(''V'') do not overlap &amp;quot;too much&amp;quot;.&lt;br /&gt;
&lt;br /&gt;
The open set condition is a separation condition that ensures the images ψ&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;(V) do not overlap &amp;quot;too much&amp;quot;.&lt;br /&gt;
&lt;br /&gt;
开集条件是保证图像ψ&amp;lt;sub&amp;gt;''i''&amp;lt;/sub&amp;gt;(''V'') 不重叠“太多”的分离条件。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
'''Theorem'''. Suppose the open set condition holds and each ψ&amp;lt;sub&amp;gt;''i''&amp;lt;/sub&amp;gt; is a similitude, that is a composition of an [[isometry]] and a [[dilation (metric space)|dilation]] around some point. Then the unique fixed point of ψ is a set whose Hausdorff dimension is ''s'' where ''s'' is the unique solution of&amp;lt;ref&amp;gt;{{cite journal | last=Hutchinson | first=John E. | title=Fractals and self similarity | journal=Indiana Univ. Math. J. | volume=30 | year=1981 | pages=713–747 | doi=10.1512/iumj.1981.30.30055 | issue=5 | doi-access=free }}&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
Theorem. Suppose the open set condition holds and each ψ&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt; is a similitude, that is a composition of an isometry and a dilation around some point. Then the unique fixed point of ψ is a set whose Hausdorff dimension is s where s is the unique solution of&lt;br /&gt;
&lt;br /&gt;
'''定理'''假设开集条件成立，并且每个ψ&amp;lt;sub&amp;gt;''i''&amp;lt;/sub&amp;gt; 是一个相似度，即等距和某个点周围的膨胀的组合。。那么唯一的不动点是Hausdorff维数为 ''s'' 的集合，其中  ''s'' 是 ''s'' &amp;lt;ref&amp;gt;{{cite journal | last=Hutchinson | first=John E. | title=Fractals and self similarity | journal=Indiana Univ. Math. J. | volume=30 | year=1981 | pages=713–747 | doi=10.1512/iumj.1981.30.30055 | issue=5 | doi-access=free }}&amp;lt;/ref&amp;gt;的唯一解&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt; \sum_{i=1}^m r_i^s = 1. &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \sum_{i=1}^m r_i^s = 1. &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The contraction coefficient of a similitude is the magnitude of the dilation.&lt;br /&gt;
&lt;br /&gt;
The contraction coefficient of a similitude is the magnitude of the dilation.&lt;br /&gt;
&lt;br /&gt;
相似物的收缩系数就是膨胀的大小。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
We can use this theorem to compute the Hausdorff dimension of the Sierpinski triangle (or sometimes called Sierpinski gasket). Consider three [[non-collinear points]] ''a''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;, ''a''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;, ''a''&amp;lt;sub&amp;gt;3&amp;lt;/sub&amp;gt; in the plane '''R'''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; and let ψ&amp;lt;sub&amp;gt;''i''&amp;lt;/sub&amp;gt; be the dilation of ratio 1/2 around ''a&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;''. The unique non-empty fixed point of the corresponding mapping ψ is a Sierpinski gasket and the dimension ''s'' is the unique solution of&lt;br /&gt;
&lt;br /&gt;
We can use this theorem to compute the Hausdorff dimension of the Sierpinski triangle (or sometimes called Sierpinski gasket). Consider three non-collinear points a&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;, a&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;, a&amp;lt;sub&amp;gt;3&amp;lt;/sub&amp;gt; in the plane R&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; and let ψ&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt; be the dilation of ratio 1/2 around a&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;. The unique non-empty fixed point of the corresponding mapping ψ is a Sierpinski gasket and the dimension s is the unique solution of&lt;br /&gt;
&lt;br /&gt;
我们可以使用这个定理来计算谢尔宾斯基三角形的豪斯多夫维数(或者有时候叫做谢尔宾斯基垫圈)。考虑R&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; 平面上的三个非共线点，''a''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;，''a''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;，''a''&amp;lt;sub&amp;gt;3&amp;lt;/sub&amp;gt;，让ψ&amp;lt;sub&amp;gt;''i''&amp;lt;/sub&amp;gt;是围绕着''a&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;''比率1/2的膨胀。对应映射的唯一非空不动点是一个谢尔宾斯基垫圈，其维数''s''是对应映射的唯一解&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt; \left(\frac{1}{2}\right)^s+\left(\frac{1}{2}\right)^s+\left(\frac{1}{2}\right)^s = 3 \left(\frac{1}{2}\right)^s =1. &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \left(\frac{1}{2}\right)^s+\left(\frac{1}{2}\right)^s+\left(\frac{1}{2}\right)^s = 3 \left(\frac{1}{2}\right)^s =1. &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Taking [[natural logarithm]]s of both sides of the above equation, we can solve for ''s'', that is: ''s'' = ln(3)/ln(2).  The Sierpinski gasket is self-similar and satisfies the OSC. In general a set ''E'' which is a fixed point of a mapping&lt;br /&gt;
&lt;br /&gt;
Taking natural logarithms of both sides of the above equation, we can solve for s, that is: s = ln(3)/ln(2).  The Sierpinski gasket is self-similar and satisfies the OSC. In general a set E which is a fixed point of a mapping&lt;br /&gt;
&lt;br /&gt;
取上述方程两边的自然对数，我们可以求出 ''s''，即: ''s'' = ln(3)/ln(2)。该密封垫具有自相似性，满足 OSC 要求。一般来说，集合 ''E''是一个映射的不动点&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt; A \mapsto \psi(A) = \bigcup_{i=1}^m \psi_i(A) &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt; A \mapsto \psi(A) = \bigcup_{i=1}^m \psi_i(A) &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
is self-similar if and only if the intersections&lt;br /&gt;
&lt;br /&gt;
is self-similar if and only if the intersections&lt;br /&gt;
&lt;br /&gt;
是自相似的，当且仅当&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt; H^s\left(\psi_i(E) \cap \psi_j(E)\right) =0, &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; H^s\left(\psi_i(E) \cap \psi_j(E)\right) =0, &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
where ''s'' is the Hausdorff dimension of ''E'' and ''H&amp;lt;sup&amp;gt;s&amp;lt;/sup&amp;gt;'' denotes [[Hausdorff measure]]. This is clear in the case of the Sierpinski gasket (the intersections are just points), but is also true more generally:&lt;br /&gt;
&lt;br /&gt;
where s is the Hausdorff dimension of E and H&amp;lt;sup&amp;gt;s&amp;lt;/sup&amp;gt; denotes Hausdorff measure. This is clear in the case of the Sierpinski gasket (the intersections are just points), but is also true more generally:&lt;br /&gt;
&lt;br /&gt;
其中 ''s''是''E''的豪斯多夫维数， ''H&amp;lt;sup&amp;gt;s&amp;lt;/sup&amp;gt;'' 表示 豪斯多夫测度。对于谢尔宾斯基垫圈(交叉点就是点)来说，这一点很明显，但更普遍的情况是:&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
'''Theorem'''. Under the same conditions as the previous theorem, the unique fixed point of ψ is self-similar.&lt;br /&gt;
&lt;br /&gt;
Theorem. Under the same conditions as the previous theorem, the unique fixed point of ψ is self-similar.&lt;br /&gt;
&lt;br /&gt;
'''定理'''：在与前一定理相同的条件下，其唯一不动点是自相似的。&lt;br /&gt;
&lt;br /&gt;
==See also参阅==&lt;br /&gt;
&lt;br /&gt;
* [[List of fractals by Hausdorff dimension豪斯多夫分形维数列表]] Examples of deterministic fractals, random and natural fractals.确定性分形与随机和自然分形的示例。&lt;br /&gt;
&lt;br /&gt;
* [[Assouad dimension  Assouad维数]], another variation of fractal dimension that, like Hausdorff dimension, is defined using coverings by balls其他被球覆盖方式定义的分形维数，例如豪斯多夫维数。&lt;br /&gt;
&lt;br /&gt;
* [[Intrinsic dimension固有维数]]&lt;br /&gt;
&lt;br /&gt;
* [[Packing dimension填充维数]]&lt;br /&gt;
&lt;br /&gt;
* [[Fractal dimension分形维数]]&lt;br /&gt;
&lt;br /&gt;
==References参考文献==&lt;br /&gt;
&lt;br /&gt;
{{reflist}}&lt;br /&gt;
&lt;br /&gt;
==Further reading拓展阅读==&lt;br /&gt;
&lt;br /&gt;
* {{cite book |last1=Dodson |first1=M. Maurice |title=Fractal Geometry and Applications: A Jubilee of Benoît Mandelbrot |volume=72 |issue=1 |pages=305–347 |last2=Kristensen |first2=Simon |chapter=Hausdorff Dimension and Diophantine Approximation |date=June 12, 2003 |arxiv=math/0305399 |bibcode = 2003math......5399D |doi=10.1090/pspum/072.1/2112110|series=Proceedings of Symposia in Pure Mathematics |isbn=9780821836378 }}&lt;br /&gt;
&lt;br /&gt;
* {{cite book |last1=Hurewicz |first1=Witold |authorlink1=Witold Hurewicz |last2=Wallman |first2=Henry |authorlink2=Henry Wallman |title=Dimension Theory |url=https://archive.org/details/in.ernet.dli.2015.84609 |publisher=Princeton University Press |year=1948 }}&lt;br /&gt;
&lt;br /&gt;
* {{cite journal |author作者=E. Szpilrajn |authorlink=Edward Marczewski |title=La dimension et la mesure |journal=Fundamenta Mathematicae |volume=28 |pages=81–9 |year=1937 }}&lt;br /&gt;
&lt;br /&gt;
* {{cite journal&lt;br /&gt;
&lt;br /&gt;
 | last1=Marstrand&lt;br /&gt;
&lt;br /&gt;
 | last1=Marstrand&lt;br /&gt;
&lt;br /&gt;
 | last1=马斯特兰德&lt;br /&gt;
&lt;br /&gt;
 | first1=J. M. | title=The dimension of cartesian product sets | year=1954 | journal=Proc. Cambridge Philos. Soc.&lt;br /&gt;
&lt;br /&gt;
 | first1=J. M. | title=The dimension of cartesian product sets | year=1954 | journal=Proc. Cambridge Philos. Soc.&lt;br /&gt;
&lt;br /&gt;
 | first1= J. M. | title=笛卡儿积集的维数 | 1954年 |  journal=Proc. Cambridge Philos. Soc.&lt;br /&gt;
&lt;br /&gt;
 | volume=50&lt;br /&gt;
&lt;br /&gt;
 | volume=50&lt;br /&gt;
&lt;br /&gt;
 | 第50卷&lt;br /&gt;
&lt;br /&gt;
 | issue=3&lt;br /&gt;
&lt;br /&gt;
 | issue=3&lt;br /&gt;
&lt;br /&gt;
 | 第三期&lt;br /&gt;
&lt;br /&gt;
 | pages=198–202&lt;br /&gt;
&lt;br /&gt;
 | pages=198–202&lt;br /&gt;
&lt;br /&gt;
 | 第198-202页&lt;br /&gt;
&lt;br /&gt;
 | doi=10.1017/S0305004100029236|bibcode = 1954PCPS...50..198M }}&lt;br /&gt;
&lt;br /&gt;
 | doi=10.1017/S0305004100029236|bibcode = 1954PCPS...50..198M }}&lt;br /&gt;
&lt;br /&gt;
10.1017 / S0305004100029236 | bibcode 1954PCPS... 50. . 198 m }&lt;br /&gt;
&lt;br /&gt;
* {{Cite book&lt;br /&gt;
&lt;br /&gt;
 | last1=Mattila&lt;br /&gt;
&lt;br /&gt;
 | last1=Mattila&lt;br /&gt;
&lt;br /&gt;
 | last1=Mattila&lt;br /&gt;
&lt;br /&gt;
 | first1=Pertti | author1-link=Pertti Mattila| title=Geometry of sets and measures in Euclidean spaces | publisher=[[Cambridge University Press]]&lt;br /&gt;
&lt;br /&gt;
 | first1=Pertti | author1-link=Pertti Mattila| title=Geometry of sets and measures in Euclidean spaces | publisher=Cambridge University Press&lt;br /&gt;
&lt;br /&gt;
| first1 Pertti | author1-link Pertti Mattila | title 欧几里德空间中集合和度量的几何 | 出版商剑桥大学出版社&lt;br /&gt;
&lt;br /&gt;
 | isbn=978-0-521-65595-8 | year=1995}}&lt;br /&gt;
&lt;br /&gt;
 | isbn=978-0-521-65595-8 | year=1995}}&lt;br /&gt;
&lt;br /&gt;
| isbn 978-0-521-65595-8 | year 1995}&lt;br /&gt;
&lt;br /&gt;
* {{cite journal |author=A. S. Besicovitch |authorlink=A. S. Besicovitch |title=On Linear Sets of Points of Fractional Dimensions |journal=[[Mathematische Annalen]] |volume=101 |year=1929 | doi=10.1007/BF01454831| issue=1 |pages= 161–193}}&lt;br /&gt;
&lt;br /&gt;
* {{cite journal |author1=A. S. Besicovitch |authorlink1=A. S. Besicovitch |author2=H. D. Ursell |authorlink2=H. D. Ursell |title=Sets of Fractional Dimensions |journal=Journal of the London Mathematical Society |volume=12 |year=1937 | issue=1 | doi=10.1112/jlms/s1-12.45.18  | pages=18–25 }}&amp;lt;br/&amp;gt;Several selections from this volume are reprinted in {{cite book |author=Edgar, Gerald A. |title=Classics on fractals |publisher=Addison-Wesley |location=Boston |year=1993 |isbn=0-201-58701-7}} See chapters 9,10,11&lt;br /&gt;
&lt;br /&gt;
* {{cite journal |author=F. Hausdorff |authorlink=F. Hausdorff |title=Dimension und äußeres Maß |journal=Mathematische Annalen |volume=79 |issue=1–2 |pages=157–179 |date=March 1919 |doi=10.1007/BF01457179|hdl=10338.dmlcz/100363 |url=http://dml.cz/bitstream/handle/10338.dmlcz/100363/CzechMathJ_09-1959-3_5.pdf }}&lt;br /&gt;
&lt;br /&gt;
* {{cite journal | last=Hutchinson | first=John E. | title=Fractals and self similarity | journal=Indiana Univ. Math. J. | volume=30 | year=1981 | pages=713–747 | doi=10.1512/iumj.1981.30.30055 | issue=5 | doi-access=free }}&lt;br /&gt;
&lt;br /&gt;
*{{cite book | last=Falconer | first = Kenneth |title=Fractal Geometry: Mathematical Foundations and Applications | publisher=[[John Wiley and Sons]] | edition=2nd | year=2003}}&lt;br /&gt;
&lt;br /&gt;
==External links外部链接==&lt;br /&gt;
&lt;br /&gt;
* [https://www.encyclopediaofmath.org/index.php/Hausdorff_dimension Hausdorff dimension] 在 [https://www.encyclopediaofmath.org/ Encyclopedia of Mathematics]&lt;br /&gt;
&lt;br /&gt;
* [https://www.encyclopediaofmath.org/index.php/Hausdorff_measure Hausdorff measure] 在 [https://www.encyclopediaofmath.org/ Encyclopedia of Mathematics]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{{DEFAULTSORT:Hausdorff Dimension豪斯多夫维数}}&lt;br /&gt;
&lt;br /&gt;
[[Category分类:Fractals分形]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[Category分类:Metric geometry度量几何]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[Category分类:Dimension theory维度理论]]&lt;br /&gt;
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&lt;br /&gt;
&lt;br /&gt;
&amp;lt;noinclude&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;small&amp;gt;This page was moved from [[wikipedia:en:Hausdorff dimension]]. Its edit history can be viewed at [[分形维数/edithistory]]&amp;lt;/small&amp;gt;&amp;lt;/noinclude&amp;gt;&lt;br /&gt;
&lt;br /&gt;
[[Category:待整理页面]]&lt;/div&gt;</summary>
		<author><name>Ruili</name></author>
	</entry>
	<entry>
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		<title>分形维数</title>
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		<updated>2020-11-01T17:54:07Z</updated>

		<summary type="html">&lt;p&gt;Ruili：&lt;/p&gt;
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&lt;div&gt;此词条暂由彩云小译翻译，未经人工整理和审校，带来阅读不便，请见谅。&lt;br /&gt;
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Example of non-integer dimensions. The first four [[iteration]]s of the [[Koch snowflake|Koch curve]], where after each iteration, all original line segments are replaced with four, each a self-similar copy that is 1/3 the length of the original. One formalism of the Hausdorff dimension uses this scale factor (3) and the number of self-similar objects (4) to calculate the dimension, D, after the first iteration to be D = (log N)/(log S) = (log 4)/(log 3) ≈ 1.26.&amp;lt;ref name=CampbellAnnenberg15&amp;gt;MacGregor Campbell, 2013, &amp;quot;5.6 Scaling and the Hausdorff Dimension,&amp;quot; at ''Annenberg Learner:MATHematics illuminated'', see [http://www.learner.org/courses/mathilluminated/units/5/textbook/06.php], accessed 5 March 2015.&amp;lt;/ref&amp;gt; That is, while the Hausdorff dimension of a single [[point (geometry)|point]] is zero, of a [[line segment]] is 1, of a [[square]] is 2, and of a [[cube]] is 3, for [[fractal]]s such as this, the object can have a non-integer dimension.&lt;br /&gt;
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Example of non-integer dimensions. The first four iterations of the Koch curve, where after each iteration, all original line segments are replaced with four, each a self-similar copy that is 1/3 the length of the original. One formalism of the Hausdorff dimension uses this scale factor (3) and the number of self-similar objects (4) to calculate the dimension, D, after the first iteration to be D = (log N)/(log S) = (log 4)/(log 3) ≈ 1.26. That is, while the Hausdorff dimension of a single point is zero, of a line segment is 1, of a square is 2, and of a cube is 3, for fractals such as this, the object can have a non-integer dimension.&lt;br /&gt;
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非整数维度示例：前四个[[Koch 曲线]]的迭代，在每次迭代后，所有原始线段都被替换为四个，每个自相似的复制是原始线段长度的1 / 3。豪斯多夫维数的一个建模是使用比例因子(3)和自相似对象的数量(4)来计算维度 D，在第一次迭代后为 D = (log N)/(log S) = (log 4)/(log 3) ≈ 1.26.&amp;lt;ref name=CampbellAnnenberg15&amp;gt;。MacGregor Campbell, 2013, &amp;quot;5.6 Scaling and the Hausdorff Dimension,&amp;quot; 在 ''Annenberg Learner:MATHematics illuminated'', 参见 [http://www.learner.org/courses/mathilluminated/units/5/textbook/06.php], accessed 5 March 2015.&amp;lt;/ref&amp;gt; 也就是说，单点的豪斯多夫维数为零，线段为1，正方形为2，立方体为3时，但对于分形，对象可以有一个非整数维度。&lt;br /&gt;
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In [[mathematics]], '''Hausdorff dimension''' is a measure of ''roughness'', or more specifically, [[fractal dimension]], that was first introduced in 1918 by [[mathematician]] [[Felix Hausdorff]].&amp;lt;ref&amp;gt;{{Cite journal |arxiv = 1101.1444|doi = 10.1214/11-STS370|title = Estimators of Fractal Dimension: Assessing the Roughness of Time Series and Spatial Data|journal = Statistical Science|volume = 27|issue = 2|pages = 247–277|year = 2012|last1 = Gneiting|first1 = Tilmann|last2 = Ševčíková|first2 = Hana|last3 = Percival|first3 = Donald B.}}&amp;lt;/ref&amp;gt; For instance, the Hausdorff dimension of a single [[point (geometry)|point]] is zero, of a [[line segment]] is 1, of a [[square]] is 2, and of a [[cube]] is 3. That is, for sets of points that define a smooth shape or a shape that has a small number of corners—the shapes of traditional geometry and science—the Hausdorff dimension is an [[integer]] agreeing with the usual sense of dimension, also known as the [[Inductive dimension|topological dimension]]. However, formulas have also been developed that allow calculation of the dimension of other less simple objects, where, solely on the basis of their properties of [[scaling (geometry)|scaling]] and [[self-similarity]], one is led to the conclusion that particular objects—including [[fractal]]s—have non-integer Hausdorff dimensions. Because of the significant technical advances made by [[Abram Samoilovitch Besicovitch]] allowing computation of dimensions for highly irregular or &amp;quot;rough&amp;quot; sets, this dimension is also commonly referred to as the ''Hausdorff–Besicovitch dimension.''&lt;br /&gt;
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In mathematics, Hausdorff dimension is a measure of roughness, or more specifically, fractal dimension, that was first introduced in 1918 by mathematician Felix Hausdorff. For instance, the Hausdorff dimension of a single point is zero, of a line segment is 1, of a square is 2, and of a cube is 3. That is, for sets of points that define a smooth shape or a shape that has a small number of corners—the shapes of traditional geometry and science—the Hausdorff dimension is an integer agreeing with the usual sense of dimension, also known as the topological dimension. However, formulas have also been developed that allow calculation of the dimension of other less simple objects, where, solely on the basis of their properties of scaling and self-similarity, one is led to the conclusion that particular objects—including fractals—have non-integer Hausdorff dimensions. Because of the significant technical advances made by Abram Samoilovitch Besicovitch allowing computation of dimensions for highly irregular or &amp;quot;rough&amp;quot; sets, this dimension is also commonly referred to as the Hausdorff–Besicovitch dimension.&lt;br /&gt;
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在[[数学]]中，'''&amp;lt;font color = '#ff8000'&amp;gt;豪斯多夫维数Hausdorff dimension&amp;lt;/font&amp;gt;'''是一种粗糙度的度量单位，或者更确切地说，分形维数，是由数学家 Felix Hausdorff 在1918年首次提出的。例如，单点的豪斯多夫维数为零，线段为1，正方形为2，立方体为3。也就是说，对于定义了一个光滑形状或一个有少数几个角的形状---- 传统几何学和科学的形状---- 的点集来说，豪斯多夫维数是一个整数，符合通常的维度意义，也称为拓扑维度。然而，还有一些公式允许计算其他不太简单的对象的维数，其中仅仅根据它们的标度和自相似特性，就可以得出结论: 特定的对象ー包括分形ー具有非整数的 Hausdorff 维数。由于阿布拉姆·萨莫伊洛维奇·贝西科维奇的重大技术进步，允许计算高度不规则或“粗糙”集的维度，这个维度通常也被称为 Hausdorff-Besicovitch 维度。 &lt;br /&gt;
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The Hausdorff dimension, more specifically, is a further dimensional number associated with a given set, where the distances between all members of that set are defined. Such a set is termed a [[metric space]]. The dimension is drawn from the [[Extended real number line|extended real numbers]], &amp;lt;math&amp;gt;\overline{\mathbb{R}}&amp;lt;/math&amp;gt;, as opposed to the more intuitive notion of dimension, which is not associated to general metric spaces, and only takes values in the non-negative integers.&lt;br /&gt;
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The Hausdorff dimension, more specifically, is a further dimensional number associated with a given set, where the distances between all members of that set are defined. Such a set is termed a metric space. The dimension is drawn from the extended real numbers, &amp;lt;math&amp;gt;\overline{\mathbb{R}}&amp;lt;/math&amp;gt;, as opposed to the more intuitive notion of dimension, which is not associated to general metric spaces, and only takes values in the non-negative integers.&lt;br /&gt;
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更具体地说，豪斯多夫维数是一个与给定集合相关联的更进一步的维数，其中定义了该集合所有成员之间的距离。这样的集合称为度量空间。维数是从扩展的实数，&amp;lt;math&amp;gt;\overline{\mathbb{R}}&amp;lt;/math&amp;gt;，而不是更直观的维数概念(它不与一般的度量空间相关联，只取非负整数的值)。&lt;br /&gt;
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In mathematical terms, the Hausdorff dimension generalizes the notion of the dimension of a real [[vector space]]. That is, the Hausdorff dimension of an ''n''-dimensional [[inner product space]] equals ''n''. This underlies the earlier statement that the Hausdorff dimension of a point is zero, of a line is one, etc., and that [[fractal|irregular sets]] can have noninteger Hausdorff dimensions. For instance, the [[Koch snowflake]] shown at right is constructed from an equilateral triangle; in each iteration, its component line segments are divided into 3 segments of unit length, the newly created middle segment is used as the base of a new [[equilateral]] triangle that points outward, and this base segment is then deleted to leave a final object from the iteration of unit length of 4.&amp;lt;ref&amp;gt;Larry Riddle, 2014, &amp;quot;Classic Iterated Function Systems: Koch Snowflake&amp;quot;, Agnes Scott College e-Academy (online), see [http://ecademy.agnesscott.edu/~lriddle/ifs/ksnow/ksnow.htm], accessed 5 March 2015.&amp;lt;/ref&amp;gt; That is, after the first iteration, each original line segment has been replaced with N=4, where each self-similar copy is 1/S = 1/3 as long as the original.&amp;lt;ref name=CampbellAnnenberg15/&amp;gt; Stated another way, we have taken an object with Euclidean dimension, D, and reduced its linear scale by 1/3 in each direction, so that its length increases to N=S&amp;lt;sup&amp;gt;D&amp;lt;/sup&amp;gt;.&amp;lt;ref name=ClaytonSCTPLS96&amp;gt;Keith Clayton, 1996, &amp;quot;Fractals and the Fractal Dimension,&amp;quot; ''Basic Concepts in Nonlinear Dynamics and Chaos'' (workshop), Society for Chaos Theory in Psychology and the Life Sciences annual meeting, June 28, 1996, Berkeley, California, see [http://www.vanderbilt.edu/AnS/psychology/cogsci/chaos/workshop/Workshop.html], accessed 5 March 2015.&amp;lt;/ref&amp;gt; This equation is easily solved for D, yielding the ratio of logarithms (or [[natural logarithm]]s) appearing in the figures, and giving—in the Koch and other fractal cases—non-integer dimensions for these objects.&lt;br /&gt;
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In mathematical terms, the Hausdorff dimension generalizes the notion of the dimension of a real vector space. That is, the Hausdorff dimension of an n-dimensional inner product space equals n. This underlies the earlier statement that the Hausdorff dimension of a point is zero, of a line is one, etc., and that irregular sets can have noninteger Hausdorff dimensions. For instance, the Koch snowflake shown at right is constructed from an equilateral triangle; in each iteration, its component line segments are divided into 3 segments of unit length, the newly created middle segment is used as the base of a new equilateral triangle that points outward, and this base segment is then deleted to leave a final object from the iteration of unit length of 4. That is, after the first iteration, each original line segment has been replaced with N=4, where each self-similar copy is 1/S = 1/3 as long as the original. This equation is easily solved for D, yielding the ratio of logarithms (or natural logarithms) appearing in the figures, and giving—in the Koch and other fractal cases—non-integer dimensions for these objects.&lt;br /&gt;
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用数学术语来说，豪斯多夫维数概括了实向量空间维数的概念。也就是说，n 维内积空间的豪斯多夫维数等于 n。 这就是早期假设的基础，一个点的豪斯多夫维数是零，一条线是一等等，不规则集可以有非整数的豪斯多夫维数。例如，右边所示的 Koch 雪花是由一个正三角形构成的; 在每次迭代中，它的组成线段被分成单位长度的3段，新创建的中间线段被用作一个指向外部的新正三角形的基础，然后人们删除这个基础线段用来保留单位长度4的迭代中的最终对象。也就是说，在第一次迭代之后，每个原始线段都被替换为 N=4，其中每个自相似拷贝的长度是原始线段的1/S = 1/3 。这个方程很容易求解为 D，产生出现在图形中的对数(或自然对数)的比率，并给出——在 Koch 和其他分形情况下——这些对象的非整数维数。&lt;br /&gt;
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The Hausdorff dimension is a successor to the simpler, but usually equivalent, box-counting or [[Minkowski–Bouligand dimension]].&lt;br /&gt;
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The Hausdorff dimension is a successor to the simpler, but usually equivalent, box-counting or Minkowski–Bouligand dimension.&lt;br /&gt;
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豪斯多夫维数是更简单但通常等价的'''&amp;lt;font color = '#ff8000'&amp;gt;计盒维数box-counting&amp;lt;/font&amp;gt;'''或'''&amp;lt;font color = '#ff8000'&amp;gt;闵可夫斯基维数Minkowski-Bouligand&amp;lt;/font&amp;gt;'''的继承者。&lt;br /&gt;
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==Intuition概念==&lt;br /&gt;
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The intuitive concept of dimension of a geometric object ''X'' is the number of independent parameters one needs to pick out a unique point inside. However, any point specified by two parameters can be instead specified by one, because the [[cardinality]] of the [[real plane]] is equal to the cardinality of the [[real line]] (this can be seen by an [[Cantor's diagonal argument|argument]] involving interweaving the digits of two numbers to yield a single number encoding the same information). The example of a [[space-filling curve]] shows that one can even map the real line to the real plane [[Surjective function|surjectively]] (taking one real number into a pair of real numbers in a way so that all pairs of numbers are covered) and ''continuously'', so that a one-dimensional object completely fills up a higher-dimensional object.&lt;br /&gt;
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The intuitive concept of dimension of a geometric object X is the number of independent parameters one needs to pick out a unique point inside. However, any point specified by two parameters can be instead specified by one, because the cardinality of the real plane is equal to the cardinality of the real line (this can be seen by an argument involving interweaving the digits of two numbers to yield a single number encoding the same information). The example of a space-filling curve shows that one can even map the real line to the real plane surjectively (taking one real number into a pair of real numbers in a way so that all pairs of numbers are covered) and continuously, so that a one-dimensional object completely fills up a higher-dimensional object.&lt;br /&gt;
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几何对象X的尺寸的直观概念是指需要多少个独立参数才能找到一个独特的点。但是，任何由两个参数指定的点都可以由一个参数指定，因为为实平面的基数等于实线的基数(这可以通过交织两个数字以产生一个编码相同信息的单个数字看到)。'''&amp;lt;font color = '#ff8000'&amp;gt;皮亚诺曲线&amp;lt;/font&amp;gt;'''的例子表明，可以将实线完美和连续地映射到实平面(把一个实数转换成一对实数，从而覆盖所有实数对)，由此一维对象完全填充了一个高维对象。&lt;br /&gt;
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Every space filling curve hits some points multiple times, and does not have a continuous inverse. It is impossible to map two dimensions onto one in a way that is continuous and continuously invertible. The topological dimension, also called [[Lebesgue covering dimension]], explains why. This dimension is ''n'' if, in every covering of ''X'' by small open balls, there is at least one point where ''n''&amp;amp;nbsp;+&amp;amp;nbsp;1 balls overlap. For example, when one covers a line with short open intervals, some points must be covered twice, giving dimension&amp;amp;nbsp;''n''&amp;amp;nbsp;=&amp;amp;nbsp;1.&lt;br /&gt;
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Every space filling curve hits some points multiple times, and does not have a continuous inverse. It is impossible to map two dimensions onto one in a way that is continuous and continuously invertible. The topological dimension, also called Lebesgue covering dimension, explains why. This dimension is n if, in every covering of X by small open balls, there is at least one point where n&amp;amp;nbsp;+&amp;amp;nbsp;1 balls overlap. For example, when one covers a line with short open intervals, some points must be covered twice, giving dimension&amp;amp;nbsp;n&amp;amp;nbsp;=&amp;amp;nbsp;1.&lt;br /&gt;
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每条空间填充曲线都会多次击中某些点，且不存在连续的逆。将二维以连续和连续可逆的方式映射到一维是不可能的。'''&amp;lt;font color = '#ff8000'&amp;gt;拓扑维度 topological dimension&amp;lt;/font&amp;gt;'''，也被称为Lebesgue覆盖维数，解释了为什么。如果在 x 的每个小开球覆盖中，至少有一个点 n + 1个球重叠，这个维度是 n。例如，当用短的开区间覆盖一条线时，某些点必须被覆盖两次，给出维数''n''&amp;amp;nbsp;=&amp;amp;nbsp;1。&lt;br /&gt;
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But topological dimension is a very crude measure of the local size of a space (size near a point). A curve that is almost space-filling can still have topological dimension one, even if it fills up most of the area of a region. A [[fractal]] has an integer topological dimension, but in terms of the amount of space it takes up, it behaves like a higher-dimensional space.&lt;br /&gt;
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But topological dimension is a very crude measure of the local size of a space (size near a point). A curve that is almost space-filling can still have topological dimension one, even if it fills up most of the area of a region. A fractal has an integer topological dimension, but in terms of the amount of space it takes up, it behaves like a higher-dimensional space.&lt;br /&gt;
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但是，拓扑维度是对空间局部尺寸(点附近的尺寸)的一个非常粗略的度量。一条几乎是空间填充的曲线仍然可以有一维拓扑，即使它填充了一个区域的大部分面积。分形具有整数的拓扑维数，但就其所占的空间量而言，它看起来像一个更高维的空间。&lt;br /&gt;
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The Hausdorff dimension measures the local size of a space taking into account the distance between points, the [[metric space|metric]]. Consider the number ''N''(''r'') of [[ball (mathematics)|balls]] of radius at most ''r'' required to cover ''X'' completely. When ''r'' is very small, ''N''(''r'') grows polynomially with 1/''r''. For a sufficiently well-behaved  ''X'', the Hausdorff dimension is the unique number ''d'' such that N(''r'') grows as 1/''r&amp;lt;sup&amp;gt;d&amp;lt;/sup&amp;gt;'' as ''r'' approaches zero. More precisely, this defines the [[Minkowski–Bouligand dimension|box-counting dimension]], which equals the Hausdorff dimension when the value ''d'' is a critical boundary between growth rates that are insufficient to cover the space, and growth rates that are overabundant.&lt;br /&gt;
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The Hausdorff dimension measures the local size of a space taking into account the distance between points, the metric. Consider the number N(r) of balls of radius at most r required to cover X completely. When r is very small, N(r) grows polynomially with 1/r. For a sufficiently well-behaved  X, the Hausdorff dimension is the unique number d such that N(r) grows as 1/r&amp;lt;sup&amp;gt;d&amp;lt;/sup&amp;gt; as r approaches zero. More precisely, this defines the box-counting dimension, which equals the Hausdorff dimension when the value d is a critical boundary between growth rates that are insufficient to cover the space, and growth rates that are overabundant.&lt;br /&gt;
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豪斯多夫维数测量一个空间的局部大小时，会考虑到点之间距离的度量。考虑半径最大为 r 的球数 ''N'' (r) ，需要完全覆盖 ''X''。当 r 很小时，n (r)以1/''r'' 增长多项式。对于一个表现足够好的 ''X''，豪斯多夫维数是唯一的数 d，这样当 r 趋近于零时， N(r)增长为1/r&amp;lt;sup&amp;gt;d&amp;lt;/sup&amp;gt; 。更确切地说，这定义了盒子计数维度，当值 d 是不足以覆盖空间的增长率和过度充裕的增长率之间的关键边界时，它等于豪斯多夫维数。&lt;br /&gt;
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For shapes that are smooth, or shapes with a small number of corners, the shapes of traditional geometry and science, the Hausdorff dimension is an integer agreeing with the topological dimension. But [[Benoit Mandelbrot]] observed that [[fractal]]s, sets with noninteger Hausdorff dimensions, are found everywhere in nature. He observed that the proper idealization of most rough shapes you see around you is not in terms of smooth idealized shapes, but in terms of fractal idealized shapes:&lt;br /&gt;
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For shapes that are smooth, or shapes with a small number of corners, the shapes of traditional geometry and science, the Hausdorff dimension is an integer agreeing with the topological dimension. But Benoit Mandelbrot observed that fractals, sets with noninteger Hausdorff dimensions, are found everywhere in nature. He observed that the proper idealization of most rough shapes you see around you is not in terms of smooth idealized shapes, but in terms of fractal idealized shapes:&lt;br /&gt;
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对于光滑的形状，或者有少量棱角的形状，传统几何和科学的形状，豪斯多夫维数是一个整数，与拓扑维度一致。但是伯努·曼德布洛特观察到分形---- 具有非整数豪斯多夫维数的集合---- 在自然界中随处可见。他观察到，我们周围大多数粗糙形状的理想化不是光滑的理想化形状，而是分形理想化形状:&lt;br /&gt;
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&amp;lt;blockquote&amp;gt;Clouds are not spheres, mountains are not cones, coastlines are not circles, and bark is not smooth, nor does lightning travel in a straight line.&amp;lt;ref name=&amp;quot;mandelbrot&amp;quot;&amp;gt;{{cite book   | last = Mandelbrot   | first = Benoît   | authorlink = Benoit Mandelbrot   | title = The Fractal Geometry of Nature   | publisher = W. H. Freeman   | series = Lecture notes in mathematics 1358   | year = 1982   | doi =    | isbn = 0-7167-1186-9   | url-access = registration   | url = https://archive.org/details/fractalgeometryo00beno   }}&amp;lt;/ref&amp;gt;&amp;lt;/blockquote&amp;gt;&lt;br /&gt;
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&amp;lt;blockquote&amp;gt;Clouds are not spheres, mountains are not cones, coastlines are not circles, and bark is not smooth, nor does lightning travel in a straight line.&amp;lt;/blockquote&amp;gt;&lt;br /&gt;
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&amp;lt;blockquote&amp;gt;云不是球体，山不是锥体，海岸线不是圆圈，树皮不平滑，闪电也不是直线运动。 &amp;lt;/blockquote&amp;gt;&lt;br /&gt;
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For fractals that occur in nature, the Hausdorff and [[Minkowski–Bouligand dimension|box-counting dimension]] coincide. The [[packing dimension]] is yet another similar notion which gives the same value for many shapes, but there are well documented exceptions where all these dimensions differ.&lt;br /&gt;
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For fractals that occur in nature, the Hausdorff and box-counting dimension coincide. The packing dimension is yet another similar notion which gives the same value for many shapes, but there are well documented exceptions where all these dimensions differ.&lt;br /&gt;
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对于自然界中出现的分形，豪斯多夫维数和盒计数维数是一致的。封装尺寸是另一个类似的概念，它为许多形状提供相同的值，但是在所有这些尺寸不同的情况，都做了很好的说明。&lt;br /&gt;
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==Formal definitions形式化定义==&lt;br /&gt;
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===Hausdorff content豪斯多夫集===&lt;br /&gt;
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Let ''X'' be a [[metric space]]. If ''S'' ⊂ ''X'' and ''d'' ∈ [0, ∞), the ''d''-dimensional '''unlimited Hausdorff content''' of ''S'' is defined by&lt;br /&gt;
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Let X be a metric space. If S ⊂ X and d ∈ [0, ∞), the d-dimensional unlimited Hausdorff content of S is defined by&lt;br /&gt;
&lt;br /&gt;
设 ''X''是度量空间。若''S'' ⊂ ''X'' 和 ''d'' ∈ [0, ∞) ，则 ''S'' 的''d''维无限 豪斯多夫集定义为&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt;C_H^d(S):=\inf\Bigl\{\sum_i r_i^d:\text{ there is a cover of } S\text{ by balls with radii }r_i&amp;gt;0\Bigr\}.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt;C_H^d(S):=\inf\Bigl\{\sum_i r_i^d:\text{ there is a cover of } S\text{ by balls with radii }r_i&amp;gt;0\Bigr\}.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt;C_H^d(S):=\inf\Bigl\{\sum_i r_i^d:\text{ there is a cover of } S\text{ by balls with radii }r_i&amp;gt;0\Bigr\}.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
In other words, &amp;lt;math&amp;gt;C_H^d(S)&amp;lt;/math&amp;gt; is the [[infimum]] of the set of numbers &amp;lt;math&amp;gt;\delta \geq 0&amp;lt;/math&amp;gt; such that there is some (indexed) collection of [[ball (mathematics)|ball]]s &amp;lt;math&amp;gt;\{B(x_i,r_i):i\in I\}&amp;lt;/math&amp;gt; covering ''S'' with ''r&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;''&amp;amp;nbsp;&amp;gt;&amp;amp;nbsp;0 for each ''i''&amp;amp;nbsp;∈&amp;amp;nbsp;''I'' that satisfies &amp;lt;math&amp;gt;\sum_{i\in I} r_i^d&amp;lt;\delta &amp;lt;/math&amp;gt;. (Here, we use the standard convention that [[infimum|inf&amp;amp;nbsp;Ø&amp;amp;nbsp;=&amp;amp;nbsp;∞]].)&lt;br /&gt;
&lt;br /&gt;
In other words, &amp;lt;math&amp;gt;C_H^d(S)&amp;lt;/math&amp;gt; is the infimum of the set of numbers &amp;lt;math&amp;gt;\delta \geq 0&amp;lt;/math&amp;gt; such that there is some (indexed) collection of balls &amp;lt;math&amp;gt;\{B(x_i,r_i):i\in I\}&amp;lt;/math&amp;gt; covering S with r&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;&amp;amp;nbsp;&amp;gt;&amp;amp;nbsp;0 for each i&amp;amp;nbsp;∈&amp;amp;nbsp;I that satisfies &amp;lt;math&amp;gt;\sum_{i\in I} r_i^d&amp;lt;\delta &amp;lt;/math&amp;gt;. (Here, we use the standard convention that inf&amp;amp;nbsp;Ø&amp;amp;nbsp;=&amp;amp;nbsp;∞.)&lt;br /&gt;
&lt;br /&gt;
换句话说，&amp;lt;math&amp;gt;C_H^d(S)&amp;lt;/math&amp;gt; 是数字集合&amp;lt;math&amp;gt;\delta \geq 0&amp;lt;/math&amp;gt;的下确界，使得在 ''i''&amp;amp;nbsp;∈&amp;amp;nbsp中存在一些球集合 &amp;lt;math&amp;gt;\{B(x_i,r_i):i\in I\}&amp;lt;/math&amp;gt;  i 包含 s，对于每个 ''r&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;''&amp;amp;nbsp;&amp;gt;&amp;amp;nbsp;0 满足 i 中的和&amp;lt;math&amp;gt;\sum_{i\in I} r_i^d&amp;lt;\delta &amp;lt;/math&amp;gt; (在这里，我们使用inf&amp;amp;nbsp;Ø&amp;amp;nbsp;=&amp;amp;nbsp;∞ )的标准约定。&lt;br /&gt;
&lt;br /&gt;
===Hausdorff measurement豪斯多夫分形测量===&lt;br /&gt;
&lt;br /&gt;
The Hausdorff outer measure is different from the unbounded Hausdorf content in that rather than considering all possible coverings of ''S'', we see what happens when the sizes of the balls go to zero. This is  for &amp;lt;math&amp;gt;d \geq 0 &amp;lt;/math&amp;gt;, we define the ''d''-dimensional Hausdorff outer measure of ''S'' as&lt;br /&gt;
&lt;br /&gt;
The Hausdorff outer measure is different from the unbounded Hausdorf content in that rather than considering all possible coverings of S, we see what happens when the sizes of the balls go to zero. This is  for &amp;lt;math&amp;gt;d \geq 0 &amp;lt;/math&amp;gt;, we define the d-dimensional Hausdorff outer measure of S as&lt;br /&gt;
&lt;br /&gt;
豪斯多夫外测度不同于无界的豪斯多夫，因为我们不考虑 s 的所有可能，我们看到当球的大小为零时会发生什么。这是为了数学  &amp;lt;math&amp;gt;d \geq 0 &amp;lt;/math&amp;gt;，我们定义了  ''S''的 ''d''维豪斯多夫Hausdorff 外测度为&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt; \mathcal{H}^d(S):=\lim_{r \to 0} \inf\Bigl\{\sum_i r_i^d:\text{ there is a cover of } S\text{ by balls with radii } 0 &amp;lt; r_i &amp;lt; r\Bigr\}.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \mathcal{H}^d(S):=\lim_{r \to 0} \inf\Bigl\{\sum_i r_i^d:\text{ there is a cover of } S\text{ by balls with radii } 0 &amp;lt; r_i &amp;lt; r\Bigr\}.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \mathcal{H}^d(S):=\lim_{r \to 0} \inf\Bigl\{\sum_i r_i^d:\text{有一个面} S\text{ 球 } 0 &amp;lt; r_i &amp;lt; r\Bigr\}.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
===Hausdorff dimension豪斯多夫维数===&lt;br /&gt;
&lt;br /&gt;
The '''Hausdorff dimension''' of ''X'' is defined by&lt;br /&gt;
&lt;br /&gt;
The Hausdorff dimension of X is defined by&lt;br /&gt;
&lt;br /&gt;
X 的豪斯多夫维数定义为&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt;\dim_{\operatorname{H}}(X):=\inf\{d\ge 0: \mathcal{H}^d(X)=0\}.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt;\dim_{\operatorname{H}}(X):=\inf\{d\ge 0: \mathcal{H}^d(X)=0\}.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Equivalently, dim&amp;lt;sub&amp;gt;H&amp;lt;/sub&amp;gt;(''X'') may be defined as the [[infimum]] of the set of ''d'' ∈ [0, ∞) such that the ''d''-dimensional [[Hausdorff measure]] of ''X'' is zero. This is the same as the supremum of the set of ''d''&amp;amp;nbsp;∈&amp;amp;nbsp;[0,&amp;amp;nbsp;∞) such that the ''d''-dimensional Hausdorff measure of ''X'' is infinite (except that when this latter set of numbers ''d'' is empty the Hausdorff dimension is zero).&lt;br /&gt;
&lt;br /&gt;
Equivalently, dim&amp;lt;sub&amp;gt;H&amp;lt;/sub&amp;gt;(X) may be defined as the infimum of the set of d ∈ [0, ∞) such that the d-dimensional Hausdorff measure of X is zero. This is the same as the supremum of the set of d&amp;amp;nbsp;∈&amp;amp;nbsp;[0,&amp;amp;nbsp;∞) such that the d-dimensional Hausdorff measure of X is infinite (except that when this latter set of numbers d is empty the Hausdorff dimension is zero).&lt;br /&gt;
&lt;br /&gt;
等价地，dim &amp;lt;sub&amp;gt;H&amp;lt;/sub&amp;gt;(''X'')可定义为 ''d'' ∈ [0, ∞) 集的下确界，使得''X'' 的''d''-维 [[豪斯多夫测度]] 为零。这与 ''d''&amp;amp;nbsp;∈&amp;amp;nbsp;[0,&amp;amp;nbsp;∞)的集合的上确界相同，因此''X''的 d 维豪斯多夫测度是无限的(除非后一个集合 ''d'' 是空的，豪斯多夫维数为零)。&lt;br /&gt;
&lt;br /&gt;
==Examples实例==&lt;br /&gt;
&lt;br /&gt;
[[Image:Sierpinski deep.svg|thumb|250px|Dimension of a further [[fractal]] example. The [[Sierpinski triangle]], an object with Hausdorff dimension of log(3)/log(2)≈1.58.&amp;lt;ref name=ClaytonSCTPLS96/&amp;gt;]]&lt;br /&gt;
&lt;br /&gt;
Dimension of a further [[fractal example. The Sierpinski triangle, an object with Hausdorff dimension of log(3)/log(2)≈1.58.]]&lt;br /&gt;
&lt;br /&gt;
[[Image:谢尔宾斯基三角形 deep.svg|thumb|250px|进一步的[[分形维数]]的例子，进一步的分形维数的例子是谢尔宾斯基三角形，它是一个豪斯多夫维数为log(3)/log(2)≈1.58.&amp;lt;ref name=ClaytonSCTPLS96/&amp;gt;的物体]]&lt;br /&gt;
&lt;br /&gt;
* [[Countable set]]s have Hausdorff dimension 0.&amp;lt;ref name=&amp;quot;schleicher&amp;quot;&amp;gt;{{cite journal |last1=Schleicher |first1=Dierk |title=Hausdorff Dimension, Its Properties, and Its Surprises |journal=The American Mathematical Monthly |date=June 2007 |volume=114 |issue=6 |pages=509–528 |doi=10.1080/00029890.2007.11920440 |language=en |issn=0002-9890|arxiv=math/0505099 }}&amp;lt;/ref&amp;gt;&lt;br /&gt;
*[[可数集]]拥有豪斯多夫维数0.&amp;lt;ref name=&amp;quot;schleicher&amp;quot;&amp;gt;{{cite journal |last1=Schleicher |first1=Dierk |title=豪斯多夫维数, Its Properties, and Its Surprises |journal=The American Mathematical Monthly美国数学期刊 |date=June 2007 |volume=114 |issue=6 |pages=509–528 |doi=10.1080/00029890.2007.11920440 |language=en |issn=0002-9890|arxiv=math/0505099 }}&amp;lt;/ref&amp;gt;&lt;br /&gt;
* The [[Euclidean space]] ℝ&amp;lt;sup&amp;gt;''n''&amp;lt;/sup&amp;gt; has Hausdorff dimension ''n'', and the circle '''S'''&amp;lt;sup&amp;gt;1&amp;lt;/sup&amp;gt; has Hausdorff dimension 1.&amp;lt;ref name=&amp;quot;schleicher&amp;quot; /&amp;gt;&lt;br /&gt;
*[[教育空间]] ℝ&amp;lt;sup&amp;gt;''n''&amp;lt;/sup&amp;gt; 有豪斯多夫维数 ''n''，循环'''S'''&amp;lt;sup&amp;gt;1&amp;lt;/sup&amp;gt; 拥有豪斯多夫维数1.&amp;lt;ref name=&amp;quot;schleicher&amp;quot; /&amp;gt;&lt;br /&gt;
* [[Fractal]]s often are spaces whose Hausdorff dimension strictly exceeds the [[topological dimension]].&amp;lt;ref name=&amp;quot;mandelbrot&amp;quot; /&amp;gt; For example, the [[Cantor set]], a zero-dimensional topological space, is a union of two copies of itself, each copy shrunk by a factor 1/3; hence, it can be shown that its Hausdorff dimension is ln(2)/ln(3)&amp;amp;nbsp;≈&amp;amp;nbsp;0.63.&amp;lt;ref&amp;gt;{{cite book | last=Falconer | first = Kenneth |title=Fractal Geometry: Mathematical Foundations and Applications | publisher=[[John Wiley and Sons]] | edition=2nd | year=2003}}&amp;lt;/ref&amp;gt; The [[Sierpinski triangle]] is a union of three copies of itself, each copy shrunk by a factor of&amp;amp;nbsp;1/2; this yields a Hausdorff dimension of ln(3)/ln(2)&amp;amp;nbsp;≈&amp;amp;nbsp;1.58.&amp;lt;ref name=CampbellAnnenberg15/&amp;gt; These Hausdorff dimensions are related to the &amp;quot;critical exponent&amp;quot; of the [[Master theorem (analysis of algorithms)|Master theorem]] for solving [[Recurrence relation|recurrence relations]] in the [[analysis of algorithms]].&lt;br /&gt;
*[[分形]]一般是那些豪斯多夫维数直接超过其拓扑维数的空间。例如[[康托尔集]]是一个o维拓扑空间，由两个自己复制而成，每一个复制品都是原来的三分之一，因此它的豪斯多夫维数是 ln(2)/ln(3)&amp;amp;nbsp;≈&amp;amp;nbsp;0.63。&amp;lt;ref&amp;gt;{{cite book | last=Falconer | first = Kenneth |title=Fractal Geometry: Mathematical Foundations and Applications | publisher=[[John Wiley and Sons]] | edition=2nd | year=2003}}&amp;lt;/ref&amp;gt;一个[[谢尔宾斯基三角]]是他自身三个复制的组合。每一个是原来的&amp;amp;nbsp;1/2，它的豪斯多夫维数ln(3)/ln(2)&amp;amp;nbsp;≈&amp;amp;nbsp;1.58。&amp;lt;ref name=CampbellAnnenberg15/&amp;gt;在递归算法中解决递归关系时，这些豪斯多夫维数与[[算法分析主定理]]的临界指标相联系。&lt;br /&gt;
* [[Space-filling curve]]s like the [[Peano curve]] have the same Hausdorff dimension as the space they fill.&lt;br /&gt;
*[[空间填充曲线]]拥有和他们填充空间同样的豪斯多夫维数，如[[皮亚诺曲线]]。&lt;br /&gt;
* The trajectory of [[Brownian motion]] in dimension 2 and above is conjectured to be Hausdorff dimension 2.&amp;lt;ref&amp;gt;{{cite book | last=Morters | first=Peres | title= Brownian Motion | publisher=[[Cambridge University Press]] | year=2010 }}&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
[[image:Great Britain Hausdorff.svg|thumb|250px|Estimating the Hausdorff dimension of the [[How Long Is the Coast of Britain? Statistical Self-Similarity and Fractional Dimension|coast of Great Britain]]]]&lt;br /&gt;
&lt;br /&gt;
coast of Great Britain]]&lt;br /&gt;
&lt;br /&gt;
[[大不列颠海岸&lt;br /&gt;
&lt;br /&gt;
* 刘易斯·弗赖伊·理查森[[Lewis Fry Richardson]] has performed detailed experiments to measure the approximate Hausdorff dimension for various coastlines. His results have varied from 1.02 for the coastline of [[South Africa]] to 1.25 for the west coast of [[Great Britain]].&amp;lt;ref name=&amp;quot;mandelbrot&amp;quot; /&amp;gt;&lt;br /&gt;
*刘易斯·弗赖伊·理查森（Lewis Fry Richardson）已经通过豪斯多夫维数去测量了很多海岸线。它的结果涵盖从1.02的南非海岸线到1.25的大英帝国西海岸模型。]]&lt;br /&gt;
&lt;br /&gt;
==Properties of Hausdorff dimension豪斯多夫维数特性==&lt;br /&gt;
&lt;br /&gt;
{{refimprove section|date=March 2015}}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
=== Hausdorff dimension and inductive dimension 豪斯多夫维数和归纳维数===&lt;br /&gt;
&lt;br /&gt;
Let ''X'' be an arbitrary [[Separable space|separable]] metric space. There is a [[topology|topological]] notion of [[inductive dimension]] for ''X'' which is defined recursively. It is always an integer (or +∞) and is denoted dim&amp;lt;sub&amp;gt;ind&amp;lt;/sub&amp;gt;(''X'').&lt;br /&gt;
&lt;br /&gt;
Let X be an arbitrary separable metric space. There is a topological notion of inductive dimension for X which is defined recursively. It is always an integer (or +∞) and is denoted dim&amp;lt;sub&amp;gt;ind&amp;lt;/sub&amp;gt;(X).&lt;br /&gt;
&lt;br /&gt;
设''X'' 是[[任意可分度量空间]]。对于''X'' 有一个递归定义的归纳维数拓扑概念。它总是一个整数(或 + ∞) ，记为dim&amp;lt;sub&amp;gt;ind&amp;lt;/sub&amp;gt;(''X'')。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
'''Theorem'''. Suppose ''X'' is non-empty. Then &lt;br /&gt;
&lt;br /&gt;
Theorem. Suppose X is non-empty. Then &lt;br /&gt;
&lt;br /&gt;
'''定理'''：假设''X'' 是非空的, 那么&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt; \dim_{\mathrm{Haus}}(X) \geq \dim_{\operatorname{ind}}(X). &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \dim_{\mathrm{Haus}}(X) \geq \dim_{\operatorname{ind}}(X). &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Moreover,&lt;br /&gt;
&lt;br /&gt;
Moreover,&lt;br /&gt;
&lt;br /&gt;
此外,&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \inf_Y \dim_{\operatorname{Haus}}(Y) =\dim_{\operatorname{ind}}(X), &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \inf_Y \dim_{\operatorname{Haus}}(Y) =\dim_{\operatorname{ind}}(X), &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
where ''Y'' ranges over metric spaces [[homeomorphic]] to ''X''. In other words, ''X'' and ''Y'' have the same underlying set of points and the metric ''d''&amp;lt;sub&amp;gt;''Y''&amp;lt;/sub&amp;gt; of ''Y'' is topologically equivalent to ''d''&amp;lt;sub&amp;gt;''X''&amp;lt;/sub&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
where Y ranges over metric spaces homeomorphic to X. In other words, X and Y have the same underlying set of points and the metric d&amp;lt;sub&amp;gt;Y&amp;lt;/sub&amp;gt; of Y is topologically equivalent to d&amp;lt;sub&amp;gt;X&amp;lt;/sub&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
其中''Y''是度量空间同胚到 ''X''的范围。换句话说， ''X''和 ''Y''具有相同的基本点集，''Y''的度量''d''&amp;lt;sub&amp;gt;''Y''&amp;lt;/sub&amp;gt; 拓扑等价于''d''&amp;lt;sub&amp;gt;''X''&amp;lt;/sub&amp;gt;。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
These results were originally established by [[Edward Szpilrajn]] (1907–1976), e.g., see Hurewicz and Wallman, Chapter VII.{{full citation needed|date=March 2015}}&lt;br /&gt;
&lt;br /&gt;
These results were originally established by Edward Szpilrajn (1907–1976), e.g., see Hurewicz and Wallman, Chapter VII.&lt;br /&gt;
&lt;br /&gt;
这些结果最初是由 [[Edward Szpilrajn]] (1907–1976)建立的,  参见 Hurewicz and Wallman, Chapter VII.{{full citation needed|date=March 2015}}第七章。&lt;br /&gt;
&lt;br /&gt;
=== Hausdorff dimension and Minkowski dimension 豪斯多夫维数和闵可夫斯基维度===&lt;br /&gt;
&lt;br /&gt;
The [[Minkowski dimension]] is similar to, and at least as large as, the Hausdorff dimension, and they are equal in many situations. However, the set of [[rational number|rational]] points in [0, 1] has Hausdorff dimension zero and Minkowski dimension one. There are also compact sets for which the Minkowski dimension is strictly larger than the Hausdorff dimension.&lt;br /&gt;
&lt;br /&gt;
The Minkowski dimension is similar to, and at least as large as, the Hausdorff dimension, and they are equal in many situations. However, the set of rational points in [0, 1] has Hausdorff dimension zero and Minkowski dimension one. There are also compact sets for which the Minkowski dimension is strictly larger than the Hausdorff dimension.&lt;br /&gt;
&lt;br /&gt;
[[闵可夫斯基维数]]与豪斯多夫维数相似，至少和它一样大，而且在许多情况下是相等的。然而，[0,1]中有理点集的豪斯多夫维数为0，闵可夫斯基维数为1。还有一些紧集的闵可夫斯基维数严格大于豪斯多夫维数。&lt;br /&gt;
&lt;br /&gt;
=== Hausdorff dimensions and Frostman measures 豪斯多夫维度和弗洛斯曼测度===&lt;br /&gt;
&lt;br /&gt;
If there is a [[measure (mathematics)|measure]] μ defined on [[Borel measure|Borel]] subsets of a metric space ''X'' such that ''μ''(''X'') &amp;gt; 0 and ''μ''(''B''(''x'', ''r'')) ≤ ''r&amp;lt;sup&amp;gt;s&amp;lt;/sup&amp;gt;'' holds for some constant ''s'' &amp;gt; 0 and for every ball ''B''(''x'', ''r'') in ''X'', then dim&amp;lt;sub&amp;gt;Haus&amp;lt;/sub&amp;gt;(''X'') ≥ ''s''. A partial converse is provided by [[Frostman's lemma]].{{citation needed|date=March 2015}}&amp;lt;ref&amp;gt;This Wikipedia article also discusses further useful characterizations of the Hausdorff dimension.{{clarify|date=March 2015}}&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
If there is a measure μ defined on Borel subsets of a metric space X such that μ(X) &amp;gt; 0 and μ(B(x, r)) ≤ r&amp;lt;sup&amp;gt;s&amp;lt;/sup&amp;gt; holds for some constant s &amp;gt; 0 and for every ball B(x, r) in X, then dim&amp;lt;sub&amp;gt;Haus&amp;lt;/sub&amp;gt;(X) ≥ s. A partial converse is provided by Frostman's lemma.&lt;br /&gt;
&lt;br /&gt;
如果在度量空间 ''X'' 的 Borel 子集上定义一个测度 μ，使得''μ''(''X'') &amp;gt; 0 和''μ''(''B''(''x'', ''r'')) ≤ ''r&amp;lt;sup&amp;gt;s&amp;lt;/sup&amp;gt;''，对于某个常数 ''s'' &amp;gt; 0  和 ''X'' 中的每个球 ''B''(''x'', ''r'') 成立，则 dim&amp;lt;sub&amp;gt;Haus&amp;lt;/sub&amp;gt;(''X'') ≥ ''s'' 。 部分逆向转换由弗洛斯曼引理定义。&lt;br /&gt;
&lt;br /&gt;
=== Behaviour under unions and products ===&lt;br /&gt;
&lt;br /&gt;
If &amp;lt;math&amp;gt;X=\bigcup_{i\in I}X_i&amp;lt;/math&amp;gt; is a finite or countable union, then&lt;br /&gt;
&lt;br /&gt;
If &amp;lt;math&amp;gt;X=\bigcup_{i\in I}X_i&amp;lt;/math&amp;gt; is a finite or countable union, then&lt;br /&gt;
&lt;br /&gt;
如果 &amp;lt;math&amp;gt;X=\bigcup_{i\in I}X_i&amp;lt;/math&amp;gt; 是一个有限或可数的联合，则&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \dim_{\operatorname{Haus}}(X) =\sup_{i\in I} \dim_{\operatorname{Haus}}(X_i).&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \dim_{\operatorname{Haus}}(X) =\sup_{i\in I} \dim_{\operatorname{Haus}}(X_i).&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
This can be verified directly from the definition.&lt;br /&gt;
&lt;br /&gt;
This can be verified directly from the definition.&lt;br /&gt;
&lt;br /&gt;
这可以直接从定义得到验证。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
If ''X'' and ''Y'' are non-empty metric spaces, then the Hausdorff dimension of their product satisfies&amp;lt;ref&amp;gt;{{cite journal |author=Marstrand, J. M. |title=The dimension of Cartesian product sets |journal=Proc. Cambridge Philos. Soc. |volume=50 |issue=3 |pages=198–202 |year=1954 |doi=10.1017/S0305004100029236 |bibcode = 1954PCPS...50..198M }}&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
If X and Y are non-empty metric spaces, then the Hausdorff dimension of their product satisfies&lt;br /&gt;
&lt;br /&gt;
如果 ''X'' 和''Y''是非空度量空间，那么它们乘积的豪斯多夫维数满足&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt; \dim_{\operatorname{Haus}}(X\times Y)\ge \dim_{\operatorname{Haus}}(X)+ \dim_{\operatorname{Haus}}(Y).&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \dim_{\operatorname{Haus}}(X\times Y)\ge \dim_{\operatorname{Haus}}(X)+ \dim_{\operatorname{Haus}}(Y).&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
This inequality can be strict. It is possible to find two sets of dimension 0 whose product has dimension 1.&amp;lt;ref&amp;gt;{{cite book  | last = Falconer  | first = Kenneth J.  | title = Fractal geometry. Mathematical foundations and applications  | publisher = John Wiley &amp;amp; Sons, Inc., Hoboken, New Jersey  | year = 2003  | doi =   | isbn = }}&amp;lt;/ref&amp;gt; In the opposite direction, it is known that when ''X'' and ''Y'' are Borel subsets of '''R'''&amp;lt;sup&amp;gt;''n''&amp;lt;/sup&amp;gt;, the Hausdorff dimension of ''X'' × ''Y'' is bounded from above by the Hausdorff dimension of ''X'' plus the [[packing dimension|upper packing dimension]] of ''Y''. These facts are discussed in Mattila (1995).&lt;br /&gt;
&lt;br /&gt;
This inequality can be strict. It is possible to find two sets of dimension 0 whose product has dimension 1. In the opposite direction, it is known that when X and Y are Borel subsets of R&amp;lt;sup&amp;gt;n&amp;lt;/sup&amp;gt;, the Hausdorff dimension of X × Y is bounded from above by the Hausdorff dimension of X plus the upper packing dimension of Y. These facts are discussed in Mattila (1995).&lt;br /&gt;
&lt;br /&gt;
这种不平等可以是严格的。有可能找到两个维数为0的集合，其乘积的维数为1。相反，我们知道当''X''和''Y''是 '''R'''&amp;lt;sup&amp;gt;''n''&amp;lt;/sup&amp;gt;的 Borel 子集时， ''X'' × ''Y''的豪斯多夫维数从上面以 ''X''的豪斯多夫维数加上 ''Y''的上填充维数为界。Mattila (1995)曾就这些情况进行了讨论。&lt;br /&gt;
&lt;br /&gt;
==Self-similar sets自相似集合==&lt;br /&gt;
&lt;br /&gt;
{{refimprove section|date=March 2015}}&lt;br /&gt;
&lt;br /&gt;
Many sets defined by a self-similarity condition have dimensions which can be determined explicitly. Roughly, a set ''E'' is self-similar if it is the fixed point of a set-valued transformation ψ, that is ψ(''E'') = ''E'', although the exact definition is given below.&lt;br /&gt;
&lt;br /&gt;
Many sets defined by a self-similarity condition have dimensions which can be determined explicitly. Roughly, a set E is self-similar if it is the fixed point of a set-valued transformation ψ, that is ψ(E) = E, although the exact definition is given below.&lt;br /&gt;
&lt;br /&gt;
许多由自相似条件定义的集合具有可以显式确定的维数。粗略地说，如果集合''E''是集值ψ变换的不动点，即ψ(''E'') = ''E''， 则它是自相似的，尽管下面给出了确切的定义。&lt;br /&gt;
&lt;br /&gt;
&amp;lt;blockquote&amp;gt;'''Theorem'''. Suppose&lt;br /&gt;
&lt;br /&gt;
&amp;lt;blockquote&amp;gt;Theorem. Suppose&lt;br /&gt;
&lt;br /&gt;
&amp;lt;blockquote&amp;gt;'''定理'''：假设&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt; \psi_i: \mathbf{R}^n \rightarrow \mathbf{R}^n, \quad i=1, \ldots , m &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \psi_i: \mathbf{R}^n \rightarrow \mathbf{R}^n, \quad i=1, \ldots , m &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
are [[Contraction mapping|contractive]] mappings on '''R'''&amp;lt;sup&amp;gt;''n''&amp;lt;/sup&amp;gt; with contraction constant ''r&amp;lt;sub&amp;gt;j&amp;lt;/sub&amp;gt;'' &amp;lt; 1. Then there is a unique ''non-empty'' compact set ''A'' such that&lt;br /&gt;
&lt;br /&gt;
are contractive mappings on R&amp;lt;sup&amp;gt;n&amp;lt;/sup&amp;gt; with contraction constant r&amp;lt;sub&amp;gt;j&amp;lt;/sub&amp;gt; &amp;lt; 1. Then there is a unique non-empty compact set A such that&lt;br /&gt;
&lt;br /&gt;
是'''R'''&amp;lt;sup&amp;gt;''n''&amp;lt;/sup&amp;gt;上的压缩常数''r&amp;lt;sub&amp;gt;j&amp;lt;/sub&amp;gt;'&amp;lt; 1的压缩映射。则有一个唯一的非空紧集A &lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt; A = \bigcup_{i=1}^m \psi_i (A). &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; A = \bigcup_{i=1}^m \psi_i (A). &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&amp;lt;/blockquote&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;/blockquote&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The theorem follows from [[Stefan Banach]]'s [[Contractive mapping theorem|contractive mapping fixed point theorem]] applied to the complete metric space of non-empty compact subsets of '''R'''&amp;lt;sup&amp;gt;''n''&amp;lt;/sup&amp;gt; with the [[Hausdorff distance]].&amp;lt;ref&amp;gt;{{cite book |author=Falconer, K. J. |title=The Geometry of Fractal Sets |publisher=Cambridge University Press |location=Cambridge, UK |year=1985 |isbn=0-521-25694-1 |chapter=Theorem 8.3}}&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
The theorem follows from Stefan Banach's contractive mapping fixed point theorem applied to the complete metric space of non-empty compact subsets of R&amp;lt;sup&amp;gt;n&amp;lt;/sup&amp;gt; with the Hausdorff distance.&lt;br /&gt;
&lt;br /&gt;
这个定理来源于 Stefan Banach 的压缩映射不动点定理，该定理应用于 具有豪斯多夫距离的'''R'''&amp;lt;sup&amp;gt;''n''&amp;lt;/sup&amp;gt; 的非空紧子集的完整度量空间。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
===The open set condition开集条件===&lt;br /&gt;
&lt;br /&gt;
To determine the dimension of the self-similar set ''A'' (in certain cases), we need a technical condition called the ''open set condition'' (OSC) on the sequence of contractions ψ&amp;lt;sub&amp;gt;''i''&amp;lt;/sub&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
To determine the dimension of the self-similar set A (in certain cases), we need a technical condition called the open set condition (OSC) on the sequence of contractions ψ&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
为了确定自相似集''A'' 的维数(在某些情况下) ，我们需要一个关于收缩序列的称为''开集条件''(OSC)的技术条件ψ&amp;lt;sub&amp;gt;''i''&amp;lt;/sub&amp;gt;。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
There is a relatively compact open set ''V'' such that&lt;br /&gt;
&lt;br /&gt;
There is a relatively compact open set V such that&lt;br /&gt;
&lt;br /&gt;
有一个相对紧的开集''V''&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt; \bigcup_{i=1}^m\psi_i (V) \subseteq V, &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \bigcup_{i=1}^m\psi_i (V) \subseteq V, &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
where the sets in union on the left are pairwise [[disjoint sets|disjoint]].&lt;br /&gt;
&lt;br /&gt;
where the sets in union on the left are pairwise disjoint.&lt;br /&gt;
&lt;br /&gt;
左边并集的集合成对不相交。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The open set condition is a separation condition that ensures the images ψ&amp;lt;sub&amp;gt;''i''&amp;lt;/sub&amp;gt;(''V'') do not overlap &amp;quot;too much&amp;quot;.&lt;br /&gt;
&lt;br /&gt;
The open set condition is a separation condition that ensures the images ψ&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;(V) do not overlap &amp;quot;too much&amp;quot;.&lt;br /&gt;
&lt;br /&gt;
开集条件是保证图像ψ&amp;lt;sub&amp;gt;''i''&amp;lt;/sub&amp;gt;(''V'') 不重叠“太多”的分离条件。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
'''Theorem'''. Suppose the open set condition holds and each ψ&amp;lt;sub&amp;gt;''i''&amp;lt;/sub&amp;gt; is a similitude, that is a composition of an [[isometry]] and a [[dilation (metric space)|dilation]] around some point. Then the unique fixed point of ψ is a set whose Hausdorff dimension is ''s'' where ''s'' is the unique solution of&amp;lt;ref&amp;gt;{{cite journal | last=Hutchinson | first=John E. | title=Fractals and self similarity | journal=Indiana Univ. Math. J. | volume=30 | year=1981 | pages=713–747 | doi=10.1512/iumj.1981.30.30055 | issue=5 | doi-access=free }}&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
Theorem. Suppose the open set condition holds and each ψ&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt; is a similitude, that is a composition of an isometry and a dilation around some point. Then the unique fixed point of ψ is a set whose Hausdorff dimension is s where s is the unique solution of&lt;br /&gt;
&lt;br /&gt;
'''定理'''假设开集条件成立，并且每个ψ&amp;lt;sub&amp;gt;''i''&amp;lt;/sub&amp;gt; 是一个相似度，即等距和某个点周围的膨胀的组合。。那么唯一的不动点是Hausdorff维数为 ''s'' 的集合，其中  ''s'' 是 ''s'' &amp;lt;ref&amp;gt;{{cite journal | last=Hutchinson | first=John E. | title=Fractals and self similarity | journal=Indiana Univ. Math. J. | volume=30 | year=1981 | pages=713–747 | doi=10.1512/iumj.1981.30.30055 | issue=5 | doi-access=free }}&amp;lt;/ref&amp;gt;的唯一解&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt; \sum_{i=1}^m r_i^s = 1. &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \sum_{i=1}^m r_i^s = 1. &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The contraction coefficient of a similitude is the magnitude of the dilation.&lt;br /&gt;
&lt;br /&gt;
The contraction coefficient of a similitude is the magnitude of the dilation.&lt;br /&gt;
&lt;br /&gt;
相似物的收缩系数就是膨胀的大小。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
We can use this theorem to compute the Hausdorff dimension of the Sierpinski triangle (or sometimes called Sierpinski gasket). Consider three [[non-collinear points]] ''a''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;, ''a''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;, ''a''&amp;lt;sub&amp;gt;3&amp;lt;/sub&amp;gt; in the plane '''R'''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; and let ψ&amp;lt;sub&amp;gt;''i''&amp;lt;/sub&amp;gt; be the dilation of ratio 1/2 around ''a&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;''. The unique non-empty fixed point of the corresponding mapping ψ is a Sierpinski gasket and the dimension ''s'' is the unique solution of&lt;br /&gt;
&lt;br /&gt;
We can use this theorem to compute the Hausdorff dimension of the Sierpinski triangle (or sometimes called Sierpinski gasket). Consider three non-collinear points a&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;, a&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;, a&amp;lt;sub&amp;gt;3&amp;lt;/sub&amp;gt; in the plane R&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; and let ψ&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt; be the dilation of ratio 1/2 around a&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;. The unique non-empty fixed point of the corresponding mapping ψ is a Sierpinski gasket and the dimension s is the unique solution of&lt;br /&gt;
&lt;br /&gt;
我们可以使用这个定理来计算谢尔宾斯基三角形的豪斯多夫维数(或者有时候叫做谢尔宾斯基垫圈)。考虑R&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; 平面上的三个非共线点，''a''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;，''a''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;，''a''&amp;lt;sub&amp;gt;3&amp;lt;/sub&amp;gt;，让ψ&amp;lt;sub&amp;gt;''i''&amp;lt;/sub&amp;gt;是围绕着''a&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;''比率1/2的膨胀。对应映射的唯一非空不动点是一个谢尔宾斯基垫圈，其维数''s''是对应映射的唯一解&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt; \left(\frac{1}{2}\right)^s+\left(\frac{1}{2}\right)^s+\left(\frac{1}{2}\right)^s = 3 \left(\frac{1}{2}\right)^s =1. &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \left(\frac{1}{2}\right)^s+\left(\frac{1}{2}\right)^s+\left(\frac{1}{2}\right)^s = 3 \left(\frac{1}{2}\right)^s =1. &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Taking [[natural logarithm]]s of both sides of the above equation, we can solve for ''s'', that is: ''s'' = ln(3)/ln(2).  The Sierpinski gasket is self-similar and satisfies the OSC. In general a set ''E'' which is a fixed point of a mapping&lt;br /&gt;
&lt;br /&gt;
Taking natural logarithms of both sides of the above equation, we can solve for s, that is: s = ln(3)/ln(2).  The Sierpinski gasket is self-similar and satisfies the OSC. In general a set E which is a fixed point of a mapping&lt;br /&gt;
&lt;br /&gt;
取上述方程两边的自然对数，我们可以求出 ''s''，即: ''s'' = ln(3)/ln(2)。该密封垫具有自相似性，满足 OSC 要求。一般来说，集合 ''E''是一个映射的不动点&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt; A \mapsto \psi(A) = \bigcup_{i=1}^m \psi_i(A) &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt; A \mapsto \psi(A) = \bigcup_{i=1}^m \psi_i(A) &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
is self-similar if and only if the intersections&lt;br /&gt;
&lt;br /&gt;
is self-similar if and only if the intersections&lt;br /&gt;
&lt;br /&gt;
是自相似的，当且仅当&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt; H^s\left(\psi_i(E) \cap \psi_j(E)\right) =0, &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; H^s\left(\psi_i(E) \cap \psi_j(E)\right) =0, &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
where ''s'' is the Hausdorff dimension of ''E'' and ''H&amp;lt;sup&amp;gt;s&amp;lt;/sup&amp;gt;'' denotes [[Hausdorff measure]]. This is clear in the case of the Sierpinski gasket (the intersections are just points), but is also true more generally:&lt;br /&gt;
&lt;br /&gt;
where s is the Hausdorff dimension of E and H&amp;lt;sup&amp;gt;s&amp;lt;/sup&amp;gt; denotes Hausdorff measure. This is clear in the case of the Sierpinski gasket (the intersections are just points), but is also true more generally:&lt;br /&gt;
&lt;br /&gt;
其中 ''s''是''E''的豪斯多夫维数， ''H&amp;lt;sup&amp;gt;s&amp;lt;/sup&amp;gt;'' 表示 豪斯多夫测度。对于谢尔宾斯基垫圈(交叉点就是点)来说，这一点很明显，但更普遍的情况是:&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
'''Theorem'''. Under the same conditions as the previous theorem, the unique fixed point of ψ is self-similar.&lt;br /&gt;
&lt;br /&gt;
Theorem. Under the same conditions as the previous theorem, the unique fixed point of ψ is self-similar.&lt;br /&gt;
&lt;br /&gt;
'''定理'''：在与前一定理相同的条件下，其唯一不动点是自相似的。&lt;br /&gt;
&lt;br /&gt;
==See also参阅==&lt;br /&gt;
&lt;br /&gt;
* [[List of fractals by Hausdorff dimension豪斯多夫分形维数列表]] Examples of deterministic fractals, random and natural fractals.确定性分形与随机和自然分形的示例。&lt;br /&gt;
&lt;br /&gt;
* [[Assouad dimension  Assouad维数]], another variation of fractal dimension that, like Hausdorff dimension, is defined using coverings by balls其他被球覆盖方式定义的分形维数，例如豪斯多夫维数。&lt;br /&gt;
&lt;br /&gt;
* [[Intrinsic dimension固有维数]]&lt;br /&gt;
&lt;br /&gt;
* [[Packing dimension填充维数]]&lt;br /&gt;
&lt;br /&gt;
* [[Fractal dimension分形维数]]&lt;br /&gt;
&lt;br /&gt;
==References参考文献==&lt;br /&gt;
&lt;br /&gt;
{{reflist}}&lt;br /&gt;
&lt;br /&gt;
==Further reading拓展阅读==&lt;br /&gt;
&lt;br /&gt;
* {{cite book |last1=Dodson |first1=M. Maurice |title=Fractal Geometry and Applications: A Jubilee of Benoît Mandelbrot |volume=72 |issue=1 |pages=305–347 |last2=Kristensen |first2=Simon |chapter=Hausdorff Dimension and Diophantine Approximation |date=June 12, 2003 |arxiv=math/0305399 |bibcode = 2003math......5399D |doi=10.1090/pspum/072.1/2112110|series=Proceedings of Symposia in Pure Mathematics |isbn=9780821836378 }}&lt;br /&gt;
&lt;br /&gt;
* {{cite book |last1=Hurewicz |first1=Witold |authorlink1=Witold Hurewicz |last2=Wallman |first2=Henry |authorlink2=Henry Wallman |title=Dimension Theory |url=https://archive.org/details/in.ernet.dli.2015.84609 |publisher=Princeton University Press |year=1948 }}&lt;br /&gt;
&lt;br /&gt;
* {{cite journal |author作者=E. Szpilrajn |authorlink=Edward Marczewski |title=La dimension et la mesure |journal=Fundamenta Mathematicae |volume=28 |pages=81–9 |year=1937 }}&lt;br /&gt;
&lt;br /&gt;
* {{cite journal&lt;br /&gt;
&lt;br /&gt;
 | last1=Marstrand&lt;br /&gt;
&lt;br /&gt;
 | last1=Marstrand&lt;br /&gt;
&lt;br /&gt;
 | last1=马斯特兰德&lt;br /&gt;
&lt;br /&gt;
 | first1=J. M. | title=The dimension of cartesian product sets | year=1954 | journal=Proc. Cambridge Philos. Soc.&lt;br /&gt;
&lt;br /&gt;
 | first1=J. M. | title=The dimension of cartesian product sets | year=1954 | journal=Proc. Cambridge Philos. Soc.&lt;br /&gt;
&lt;br /&gt;
 | first1= J. M. | title=笛卡儿积集的维数 | 1954年 |  journal=Proc. Cambridge Philos. Soc.&lt;br /&gt;
&lt;br /&gt;
 | volume=50&lt;br /&gt;
&lt;br /&gt;
 | volume=50&lt;br /&gt;
&lt;br /&gt;
 | 第50卷&lt;br /&gt;
&lt;br /&gt;
 | issue=3&lt;br /&gt;
&lt;br /&gt;
 | issue=3&lt;br /&gt;
&lt;br /&gt;
 | 第三期&lt;br /&gt;
&lt;br /&gt;
 | pages=198–202&lt;br /&gt;
&lt;br /&gt;
 | pages=198–202&lt;br /&gt;
&lt;br /&gt;
 | 第198-202页&lt;br /&gt;
&lt;br /&gt;
 | doi=10.1017/S0305004100029236|bibcode = 1954PCPS...50..198M }}&lt;br /&gt;
&lt;br /&gt;
 | doi=10.1017/S0305004100029236|bibcode = 1954PCPS...50..198M }}&lt;br /&gt;
&lt;br /&gt;
10.1017 / S0305004100029236 | bibcode 1954PCPS... 50. . 198 m }&lt;br /&gt;
&lt;br /&gt;
* {{Cite book&lt;br /&gt;
&lt;br /&gt;
 | last1=Mattila&lt;br /&gt;
&lt;br /&gt;
 | last1=Mattila&lt;br /&gt;
&lt;br /&gt;
 | last1=Mattila&lt;br /&gt;
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 | first1=Pertti | author1-link=Pertti Mattila| title=Geometry of sets and measures in Euclidean spaces | publisher=[[Cambridge University Press]]&lt;br /&gt;
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 | first1=Pertti | author1-link=Pertti Mattila| title=Geometry of sets and measures in Euclidean spaces | publisher=Cambridge University Press&lt;br /&gt;
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| first1 Pertti | author1-link Pertti Mattila | title 欧几里德空间中集合和度量的几何 | 出版商剑桥大学出版社&lt;br /&gt;
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 | isbn=978-0-521-65595-8 | year=1995}}&lt;br /&gt;
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 | isbn=978-0-521-65595-8 | year=1995}}&lt;br /&gt;
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| isbn 978-0-521-65595-8 | year 1995}&lt;br /&gt;
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* {{cite journal |author=A. S. Besicovitch |authorlink=A. S. Besicovitch |title=On Linear Sets of Points of Fractional Dimensions |journal=[[Mathematische Annalen]] |volume=101 |year=1929 | doi=10.1007/BF01454831| issue=1 |pages= 161–193}}&lt;br /&gt;
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* {{cite journal |author1=A. S. Besicovitch |authorlink1=A. S. Besicovitch |author2=H. D. Ursell |authorlink2=H. D. Ursell |title=Sets of Fractional Dimensions |journal=Journal of the London Mathematical Society |volume=12 |year=1937 | issue=1 | doi=10.1112/jlms/s1-12.45.18  | pages=18–25 }}&amp;lt;br/&amp;gt;Several selections from this volume are reprinted in {{cite book |author=Edgar, Gerald A. |title=Classics on fractals |publisher=Addison-Wesley |location=Boston |year=1993 |isbn=0-201-58701-7}} See chapters 9,10,11&lt;br /&gt;
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* {{cite journal |author=F. Hausdorff |authorlink=F. Hausdorff |title=Dimension und äußeres Maß |journal=Mathematische Annalen |volume=79 |issue=1–2 |pages=157–179 |date=March 1919 |doi=10.1007/BF01457179|hdl=10338.dmlcz/100363 |url=http://dml.cz/bitstream/handle/10338.dmlcz/100363/CzechMathJ_09-1959-3_5.pdf }}&lt;br /&gt;
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* {{cite journal | last=Hutchinson | first=John E. | title=Fractals and self similarity | journal=Indiana Univ. Math. J. | volume=30 | year=1981 | pages=713–747 | doi=10.1512/iumj.1981.30.30055 | issue=5 | doi-access=free }}&lt;br /&gt;
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*{{cite book | last=Falconer | first = Kenneth |title=Fractal Geometry: Mathematical Foundations and Applications | publisher=[[John Wiley and Sons]] | edition=2nd | year=2003}}&lt;br /&gt;
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==External links外部链接==&lt;br /&gt;
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* [https://www.encyclopediaofmath.org/index.php/Hausdorff_dimension Hausdorff dimension] 在 [https://www.encyclopediaofmath.org/ Encyclopedia of Mathematics]&lt;br /&gt;
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* [https://www.encyclopediaofmath.org/index.php/Hausdorff_measure Hausdorff measure] 在 [https://www.encyclopediaofmath.org/ Encyclopedia of Mathematics]&lt;br /&gt;
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{{DEFAULTSORT:Hausdorff Dimension豪斯多夫维数}}&lt;br /&gt;
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[[Category分类:Fractals分形]]&lt;br /&gt;
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[[Category分类:Metric geometry度量几何]]&lt;br /&gt;
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[[Category分类:Dimension theory维度理论]]&lt;br /&gt;
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&amp;lt;small&amp;gt;This page was moved from [[wikipedia:en:Hausdorff dimension]]. Its edit history can be viewed at [[分形维数/edithistory]]&amp;lt;/small&amp;gt;&amp;lt;/noinclude&amp;gt;&lt;br /&gt;
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[[Category:待整理页面]]&lt;/div&gt;</summary>
		<author><name>Ruili</name></author>
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		<title>分形维数</title>
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		<updated>2020-11-01T17:42:59Z</updated>

		<summary type="html">&lt;p&gt;Ruili：&lt;/p&gt;
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&lt;div&gt;此词条暂由彩云小译翻译，未经人工整理和审校，带来阅读不便，请见谅。&lt;br /&gt;
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Example of non-integer dimensions. The first four [[iteration]]s of the [[Koch snowflake|Koch curve]], where after each iteration, all original line segments are replaced with four, each a self-similar copy that is 1/3 the length of the original. One formalism of the Hausdorff dimension uses this scale factor (3) and the number of self-similar objects (4) to calculate the dimension, D, after the first iteration to be D = (log N)/(log S) = (log 4)/(log 3) ≈ 1.26.&amp;lt;ref name=CampbellAnnenberg15&amp;gt;MacGregor Campbell, 2013, &amp;quot;5.6 Scaling and the Hausdorff Dimension,&amp;quot; at ''Annenberg Learner:MATHematics illuminated'', see [http://www.learner.org/courses/mathilluminated/units/5/textbook/06.php], accessed 5 March 2015.&amp;lt;/ref&amp;gt; That is, while the Hausdorff dimension of a single [[point (geometry)|point]] is zero, of a [[line segment]] is 1, of a [[square]] is 2, and of a [[cube]] is 3, for [[fractal]]s such as this, the object can have a non-integer dimension.&lt;br /&gt;
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Example of non-integer dimensions. The first four iterations of the Koch curve, where after each iteration, all original line segments are replaced with four, each a self-similar copy that is 1/3 the length of the original. One formalism of the Hausdorff dimension uses this scale factor (3) and the number of self-similar objects (4) to calculate the dimension, D, after the first iteration to be D = (log N)/(log S) = (log 4)/(log 3) ≈ 1.26. That is, while the Hausdorff dimension of a single point is zero, of a line segment is 1, of a square is 2, and of a cube is 3, for fractals such as this, the object can have a non-integer dimension.&lt;br /&gt;
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非整数维度示例：前四个[[Koch 曲线]]的迭代，在每次迭代后，所有原始线段都被替换为四个，每个自相似的复制是原始线段长度的1 / 3。豪斯多夫维数的一个建模是使用比例因子(3)和自相似对象的数量(4)来计算维度 D，在第一次迭代后为 D = (log N)/(log S) = (log 4)/(log 3) ≈ 1.26.&amp;lt;ref name=CampbellAnnenberg15&amp;gt;。MacGregor Campbell, 2013, &amp;quot;5.6 Scaling and the Hausdorff Dimension,&amp;quot; 在 ''Annenberg Learner:MATHematics illuminated'', 参见 [http://www.learner.org/courses/mathilluminated/units/5/textbook/06.php], accessed 5 March 2015.&amp;lt;/ref&amp;gt; 也就是说，单点的豪斯多夫维数为零，线段为1，正方形为2，立方体为3时，但对于分形，对象可以有一个非整数维度。&lt;br /&gt;
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In [[mathematics]], '''Hausdorff dimension''' is a measure of ''roughness'', or more specifically, [[fractal dimension]], that was first introduced in 1918 by [[mathematician]] [[Felix Hausdorff]].&amp;lt;ref&amp;gt;{{Cite journal |arxiv = 1101.1444|doi = 10.1214/11-STS370|title = Estimators of Fractal Dimension: Assessing the Roughness of Time Series and Spatial Data|journal = Statistical Science|volume = 27|issue = 2|pages = 247–277|year = 2012|last1 = Gneiting|first1 = Tilmann|last2 = Ševčíková|first2 = Hana|last3 = Percival|first3 = Donald B.}}&amp;lt;/ref&amp;gt; For instance, the Hausdorff dimension of a single [[point (geometry)|point]] is zero, of a [[line segment]] is 1, of a [[square]] is 2, and of a [[cube]] is 3. That is, for sets of points that define a smooth shape or a shape that has a small number of corners—the shapes of traditional geometry and science—the Hausdorff dimension is an [[integer]] agreeing with the usual sense of dimension, also known as the [[Inductive dimension|topological dimension]]. However, formulas have also been developed that allow calculation of the dimension of other less simple objects, where, solely on the basis of their properties of [[scaling (geometry)|scaling]] and [[self-similarity]], one is led to the conclusion that particular objects—including [[fractal]]s—have non-integer Hausdorff dimensions. Because of the significant technical advances made by [[Abram Samoilovitch Besicovitch]] allowing computation of dimensions for highly irregular or &amp;quot;rough&amp;quot; sets, this dimension is also commonly referred to as the ''Hausdorff–Besicovitch dimension.''&lt;br /&gt;
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In mathematics, Hausdorff dimension is a measure of roughness, or more specifically, fractal dimension, that was first introduced in 1918 by mathematician Felix Hausdorff. For instance, the Hausdorff dimension of a single point is zero, of a line segment is 1, of a square is 2, and of a cube is 3. That is, for sets of points that define a smooth shape or a shape that has a small number of corners—the shapes of traditional geometry and science—the Hausdorff dimension is an integer agreeing with the usual sense of dimension, also known as the topological dimension. However, formulas have also been developed that allow calculation of the dimension of other less simple objects, where, solely on the basis of their properties of scaling and self-similarity, one is led to the conclusion that particular objects—including fractals—have non-integer Hausdorff dimensions. Because of the significant technical advances made by Abram Samoilovitch Besicovitch allowing computation of dimensions for highly irregular or &amp;quot;rough&amp;quot; sets, this dimension is also commonly referred to as the Hausdorff–Besicovitch dimension.&lt;br /&gt;
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在[[数学]]中，'''&amp;lt;font color = '#ff8000'&amp;gt;豪斯多夫维数Hausdorff dimension&amp;lt;/font&amp;gt;'''是一种粗糙度的度量单位，或者更确切地说，分形维数，是由数学家 Felix Hausdorff 在1918年首次提出的。例如，单点的豪斯多夫维数为零，线段为1，正方形为2，立方体为3。也就是说，对于定义了一个光滑形状或一个有少数几个角的形状---- 传统几何学和科学的形状---- 的点集来说，豪斯多夫维数是一个整数，符合通常的维度意义，也称为拓扑维度。然而，还有一些公式允许计算其他不太简单的对象的维数，其中仅仅根据它们的标度和自相似特性，就可以得出结论: 特定的对象ー包括分形ー具有非整数的 Hausdorff 维数。由于阿布拉姆·萨莫伊洛维奇·贝西科维奇的重大技术进步，允许计算高度不规则或“粗糙”集的维度，这个维度通常也被称为 Hausdorff-Besicovitch 维度。 &lt;br /&gt;
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The Hausdorff dimension, more specifically, is a further dimensional number associated with a given set, where the distances between all members of that set are defined. Such a set is termed a [[metric space]]. The dimension is drawn from the [[Extended real number line|extended real numbers]], &amp;lt;math&amp;gt;\overline{\mathbb{R}}&amp;lt;/math&amp;gt;, as opposed to the more intuitive notion of dimension, which is not associated to general metric spaces, and only takes values in the non-negative integers.&lt;br /&gt;
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The Hausdorff dimension, more specifically, is a further dimensional number associated with a given set, where the distances between all members of that set are defined. Such a set is termed a metric space. The dimension is drawn from the extended real numbers, &amp;lt;math&amp;gt;\overline{\mathbb{R}}&amp;lt;/math&amp;gt;, as opposed to the more intuitive notion of dimension, which is not associated to general metric spaces, and only takes values in the non-negative integers.&lt;br /&gt;
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更具体地说，豪斯多夫维数是一个与给定集合相关联的更进一步的维数，其中定义了该集合所有成员之间的距离。这样的集合称为度量空间。维数是从扩展的实数，&amp;lt;math&amp;gt;\overline{\mathbb{R}}&amp;lt;/math&amp;gt;，而不是更直观的维数概念(它不与一般的度量空间相关联，只取非负整数的值)。&lt;br /&gt;
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In mathematical terms, the Hausdorff dimension generalizes the notion of the dimension of a real [[vector space]]. That is, the Hausdorff dimension of an ''n''-dimensional [[inner product space]] equals ''n''. This underlies the earlier statement that the Hausdorff dimension of a point is zero, of a line is one, etc., and that [[fractal|irregular sets]] can have noninteger Hausdorff dimensions. For instance, the [[Koch snowflake]] shown at right is constructed from an equilateral triangle; in each iteration, its component line segments are divided into 3 segments of unit length, the newly created middle segment is used as the base of a new [[equilateral]] triangle that points outward, and this base segment is then deleted to leave a final object from the iteration of unit length of 4.&amp;lt;ref&amp;gt;Larry Riddle, 2014, &amp;quot;Classic Iterated Function Systems: Koch Snowflake&amp;quot;, Agnes Scott College e-Academy (online), see [http://ecademy.agnesscott.edu/~lriddle/ifs/ksnow/ksnow.htm], accessed 5 March 2015.&amp;lt;/ref&amp;gt; That is, after the first iteration, each original line segment has been replaced with N=4, where each self-similar copy is 1/S = 1/3 as long as the original.&amp;lt;ref name=CampbellAnnenberg15/&amp;gt; Stated another way, we have taken an object with Euclidean dimension, D, and reduced its linear scale by 1/3 in each direction, so that its length increases to N=S&amp;lt;sup&amp;gt;D&amp;lt;/sup&amp;gt;.&amp;lt;ref name=ClaytonSCTPLS96&amp;gt;Keith Clayton, 1996, &amp;quot;Fractals and the Fractal Dimension,&amp;quot; ''Basic Concepts in Nonlinear Dynamics and Chaos'' (workshop), Society for Chaos Theory in Psychology and the Life Sciences annual meeting, June 28, 1996, Berkeley, California, see [http://www.vanderbilt.edu/AnS/psychology/cogsci/chaos/workshop/Workshop.html], accessed 5 March 2015.&amp;lt;/ref&amp;gt; This equation is easily solved for D, yielding the ratio of logarithms (or [[natural logarithm]]s) appearing in the figures, and giving—in the Koch and other fractal cases—non-integer dimensions for these objects.&lt;br /&gt;
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In mathematical terms, the Hausdorff dimension generalizes the notion of the dimension of a real vector space. That is, the Hausdorff dimension of an n-dimensional inner product space equals n. This underlies the earlier statement that the Hausdorff dimension of a point is zero, of a line is one, etc., and that irregular sets can have noninteger Hausdorff dimensions. For instance, the Koch snowflake shown at right is constructed from an equilateral triangle; in each iteration, its component line segments are divided into 3 segments of unit length, the newly created middle segment is used as the base of a new equilateral triangle that points outward, and this base segment is then deleted to leave a final object from the iteration of unit length of 4. That is, after the first iteration, each original line segment has been replaced with N=4, where each self-similar copy is 1/S = 1/3 as long as the original. This equation is easily solved for D, yielding the ratio of logarithms (or natural logarithms) appearing in the figures, and giving—in the Koch and other fractal cases—non-integer dimensions for these objects.&lt;br /&gt;
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用数学术语来说，豪斯多夫维数概括了实向量空间维数的概念。也就是说，n 维内积空间的豪斯多夫维数等于 n。 这就是早期假设的基础，一个点的豪斯多夫维数是零，一条线是一等等，不规则集可以有非整数的豪斯多夫维数。例如，右边所示的 Koch 雪花是由一个正三角形构成的; 在每次迭代中，它的组成线段被分成单位长度的3段，新创建的中间线段被用作一个指向外部的新正三角形的基础，然后人们删除这个基础线段用来保留单位长度4的迭代中的最终对象。也就是说，在第一次迭代之后，每个原始线段都被替换为 N=4，其中每个自相似拷贝的长度是原始线段的1/S = 1/3 。这个方程很容易求解为 D，产生出现在图形中的对数(或自然对数)的比率，并给出——在 Koch 和其他分形情况下——这些对象的非整数维数。&lt;br /&gt;
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The Hausdorff dimension is a successor to the simpler, but usually equivalent, box-counting or [[Minkowski–Bouligand dimension]].&lt;br /&gt;
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The Hausdorff dimension is a successor to the simpler, but usually equivalent, box-counting or Minkowski–Bouligand dimension.&lt;br /&gt;
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豪斯多夫维数是更简单但通常等价的'''&amp;lt;font color = '#ff8000'&amp;gt;计盒维数box-counting&amp;lt;/font&amp;gt;'''或'''&amp;lt;font color = '#ff8000'&amp;gt;闵可夫斯基维数Minkowski-Bouligand&amp;lt;/font&amp;gt;'''的继承者。&lt;br /&gt;
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==Intuition概念==&lt;br /&gt;
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The intuitive concept of dimension of a geometric object ''X'' is the number of independent parameters one needs to pick out a unique point inside. However, any point specified by two parameters can be instead specified by one, because the [[cardinality]] of the [[real plane]] is equal to the cardinality of the [[real line]] (this can be seen by an [[Cantor's diagonal argument|argument]] involving interweaving the digits of two numbers to yield a single number encoding the same information). The example of a [[space-filling curve]] shows that one can even map the real line to the real plane [[Surjective function|surjectively]] (taking one real number into a pair of real numbers in a way so that all pairs of numbers are covered) and ''continuously'', so that a one-dimensional object completely fills up a higher-dimensional object.&lt;br /&gt;
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The intuitive concept of dimension of a geometric object X is the number of independent parameters one needs to pick out a unique point inside. However, any point specified by two parameters can be instead specified by one, because the cardinality of the real plane is equal to the cardinality of the real line (this can be seen by an argument involving interweaving the digits of two numbers to yield a single number encoding the same information). The example of a space-filling curve shows that one can even map the real line to the real plane surjectively (taking one real number into a pair of real numbers in a way so that all pairs of numbers are covered) and continuously, so that a one-dimensional object completely fills up a higher-dimensional object.&lt;br /&gt;
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几何对象X的尺寸的直观概念是指需要多少个独立参数才能找到一个独特的点。但是，任何由两个参数指定的点都可以由一个参数指定，因为为实平面的基数等于实线的基数(这可以通过交织两个数字以产生一个编码相同信息的单个数字看到)。'''&amp;lt;font color = '#ff8000'&amp;gt;皮亚诺曲线&amp;lt;/font&amp;gt;'''的例子表明，可以将实线完美和连续地映射到实平面(把一个实数转换成一对实数，从而覆盖所有实数对)，由此一维对象完全填充了一个高维对象。&lt;br /&gt;
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Every space filling curve hits some points multiple times, and does not have a continuous inverse. It is impossible to map two dimensions onto one in a way that is continuous and continuously invertible. The topological dimension, also called [[Lebesgue covering dimension]], explains why. This dimension is ''n'' if, in every covering of ''X'' by small open balls, there is at least one point where ''n''&amp;amp;nbsp;+&amp;amp;nbsp;1 balls overlap. For example, when one covers a line with short open intervals, some points must be covered twice, giving dimension&amp;amp;nbsp;''n''&amp;amp;nbsp;=&amp;amp;nbsp;1.&lt;br /&gt;
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Every space filling curve hits some points multiple times, and does not have a continuous inverse. It is impossible to map two dimensions onto one in a way that is continuous and continuously invertible. The topological dimension, also called Lebesgue covering dimension, explains why. This dimension is n if, in every covering of X by small open balls, there is at least one point where n&amp;amp;nbsp;+&amp;amp;nbsp;1 balls overlap. For example, when one covers a line with short open intervals, some points must be covered twice, giving dimension&amp;amp;nbsp;n&amp;amp;nbsp;=&amp;amp;nbsp;1.&lt;br /&gt;
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每条空间填充曲线都会多次击中某些点，且不存在连续的逆。将二维以连续和连续可逆的方式映射到一维是不可能的。'''&amp;lt;font color = '#ff8000'&amp;gt;拓扑维度 topological dimension&amp;lt;/font&amp;gt;'''，也被称为Lebesgue覆盖维数，解释了为什么。如果在 x 的每个小开球覆盖中，至少有一个点 n + 1个球重叠，这个维度是 n。例如，当用短的开区间覆盖一条线时，某些点必须被覆盖两次，给出维数''n''&amp;amp;nbsp;=&amp;amp;nbsp;1。&lt;br /&gt;
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But topological dimension is a very crude measure of the local size of a space (size near a point). A curve that is almost space-filling can still have topological dimension one, even if it fills up most of the area of a region. A [[fractal]] has an integer topological dimension, but in terms of the amount of space it takes up, it behaves like a higher-dimensional space.&lt;br /&gt;
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But topological dimension is a very crude measure of the local size of a space (size near a point). A curve that is almost space-filling can still have topological dimension one, even if it fills up most of the area of a region. A fractal has an integer topological dimension, but in terms of the amount of space it takes up, it behaves like a higher-dimensional space.&lt;br /&gt;
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但是，拓扑维度是对空间局部尺寸(点附近的尺寸)的一个非常粗略的度量。一条几乎是空间填充的曲线仍然可以有一维拓扑，即使它填充了一个区域的大部分面积。分形具有整数的拓扑维数，但就其所占的空间量而言，它看起来像一个更高维的空间。&lt;br /&gt;
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The Hausdorff dimension measures the local size of a space taking into account the distance between points, the [[metric space|metric]]. Consider the number ''N''(''r'') of [[ball (mathematics)|balls]] of radius at most ''r'' required to cover ''X'' completely. When ''r'' is very small, ''N''(''r'') grows polynomially with 1/''r''. For a sufficiently well-behaved  ''X'', the Hausdorff dimension is the unique number ''d'' such that N(''r'') grows as 1/''r&amp;lt;sup&amp;gt;d&amp;lt;/sup&amp;gt;'' as ''r'' approaches zero. More precisely, this defines the [[Minkowski–Bouligand dimension|box-counting dimension]], which equals the Hausdorff dimension when the value ''d'' is a critical boundary between growth rates that are insufficient to cover the space, and growth rates that are overabundant.&lt;br /&gt;
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The Hausdorff dimension measures the local size of a space taking into account the distance between points, the metric. Consider the number N(r) of balls of radius at most r required to cover X completely. When r is very small, N(r) grows polynomially with 1/r. For a sufficiently well-behaved  X, the Hausdorff dimension is the unique number d such that N(r) grows as 1/r&amp;lt;sup&amp;gt;d&amp;lt;/sup&amp;gt; as r approaches zero. More precisely, this defines the box-counting dimension, which equals the Hausdorff dimension when the value d is a critical boundary between growth rates that are insufficient to cover the space, and growth rates that are overabundant.&lt;br /&gt;
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豪斯多夫维数测量一个空间的局部大小时，会考虑到点之间距离的度量。考虑半径最大为 r 的球数 ''N'' (r) ，需要完全覆盖 ''X''。当 r 很小时，n (r)以1/''r'' 增长多项式。对于一个表现足够好的 ''X''，豪斯多夫维数是唯一的数 d，这样当 r 趋近于零时， N(r)增长为1/r&amp;lt;sup&amp;gt;d&amp;lt;/sup&amp;gt; 。更确切地说，这定义了盒子计数维度，当值 d 是不足以覆盖空间的增长率和过度充裕的增长率之间的关键边界时，它等于豪斯多夫维数。&lt;br /&gt;
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For shapes that are smooth, or shapes with a small number of corners, the shapes of traditional geometry and science, the Hausdorff dimension is an integer agreeing with the topological dimension. But [[Benoit Mandelbrot]] observed that [[fractal]]s, sets with noninteger Hausdorff dimensions, are found everywhere in nature. He observed that the proper idealization of most rough shapes you see around you is not in terms of smooth idealized shapes, but in terms of fractal idealized shapes:&lt;br /&gt;
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For shapes that are smooth, or shapes with a small number of corners, the shapes of traditional geometry and science, the Hausdorff dimension is an integer agreeing with the topological dimension. But Benoit Mandelbrot observed that fractals, sets with noninteger Hausdorff dimensions, are found everywhere in nature. He observed that the proper idealization of most rough shapes you see around you is not in terms of smooth idealized shapes, but in terms of fractal idealized shapes:&lt;br /&gt;
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对于光滑的形状，或者有少量棱角的形状，传统几何和科学的形状，豪斯多夫维数是一个整数，与拓扑维度一致。但是伯努·曼德布洛特观察到分形---- 具有非整数豪斯多夫维数的集合---- 在自然界中随处可见。他观察到，我们周围大多数粗糙形状的理想化不是光滑的理想化形状，而是分形理想化形状:&lt;br /&gt;
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&amp;lt;blockquote&amp;gt;Clouds are not spheres, mountains are not cones, coastlines are not circles, and bark is not smooth, nor does lightning travel in a straight line.&amp;lt;ref name=&amp;quot;mandelbrot&amp;quot;&amp;gt;{{cite book   | last = Mandelbrot   | first = Benoît   | authorlink = Benoit Mandelbrot   | title = The Fractal Geometry of Nature   | publisher = W. H. Freeman   | series = Lecture notes in mathematics 1358   | year = 1982   | doi =    | isbn = 0-7167-1186-9   | url-access = registration   | url = https://archive.org/details/fractalgeometryo00beno   }}&amp;lt;/ref&amp;gt;&amp;lt;/blockquote&amp;gt;&lt;br /&gt;
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&amp;lt;blockquote&amp;gt;Clouds are not spheres, mountains are not cones, coastlines are not circles, and bark is not smooth, nor does lightning travel in a straight line.&amp;lt;/blockquote&amp;gt;&lt;br /&gt;
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&amp;lt;blockquote&amp;gt;云不是球体，山不是锥体，海岸线不是圆圈，树皮不平滑，闪电也不是直线运动。 &amp;lt;/blockquote&amp;gt;&lt;br /&gt;
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For fractals that occur in nature, the Hausdorff and [[Minkowski–Bouligand dimension|box-counting dimension]] coincide. The [[packing dimension]] is yet another similar notion which gives the same value for many shapes, but there are well documented exceptions where all these dimensions differ.&lt;br /&gt;
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For fractals that occur in nature, the Hausdorff and box-counting dimension coincide. The packing dimension is yet another similar notion which gives the same value for many shapes, but there are well documented exceptions where all these dimensions differ.&lt;br /&gt;
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对于自然界中出现的分形，豪斯多夫维数和盒计数维数是一致的。封装尺寸是另一个类似的概念，它给出了许多形状相同的值，但是在所有这些尺寸不同的情况，都做了很好的说明。&lt;br /&gt;
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==Formal definitions形式化定义==&lt;br /&gt;
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{{unreferenced section|date=March 2015}}&lt;br /&gt;
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===Hausdorff content豪斯多夫集===&lt;br /&gt;
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Let ''X'' be a [[metric space]]. If ''S'' ⊂ ''X'' and ''d'' ∈ [0, ∞), the ''d''-dimensional '''unlimited Hausdorff content''' of ''S'' is defined by&lt;br /&gt;
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Let X be a metric space. If S ⊂ X and d ∈ [0, ∞), the d-dimensional unlimited Hausdorff content of S is defined by&lt;br /&gt;
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设 ''X''是度量空间。若''S'' ⊂ ''X'' 和 ''d'' ∈ [0, ∞) ，则 ''S'' 的''d''维无限 豪斯多夫集定义为&lt;br /&gt;
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:&amp;lt;math&amp;gt;C_H^d(S):=\inf\Bigl\{\sum_i r_i^d:\text{ there is a cover of } S\text{ by balls with radii }r_i&amp;gt;0\Bigr\}.&amp;lt;/math&amp;gt;&lt;br /&gt;
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&amp;lt;math&amp;gt;C_H^d(S):=\inf\Bigl\{\sum_i r_i^d:\text{ there is a cover of } S\text{ by balls with radii }r_i&amp;gt;0\Bigr\}.&amp;lt;/math&amp;gt;&lt;br /&gt;
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&amp;lt;math&amp;gt;C_H^d(S):=\inf\Bigl\{\sum_i r_i^d:\text{ there is a cover of } S\text{ by balls with radii }r_i&amp;gt;0\Bigr\}.&amp;lt;/math&amp;gt;&lt;br /&gt;
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In other words, &amp;lt;math&amp;gt;C_H^d(S)&amp;lt;/math&amp;gt; is the [[infimum]] of the set of numbers &amp;lt;math&amp;gt;\delta \geq 0&amp;lt;/math&amp;gt; such that there is some (indexed) collection of [[ball (mathematics)|ball]]s &amp;lt;math&amp;gt;\{B(x_i,r_i):i\in I\}&amp;lt;/math&amp;gt; covering ''S'' with ''r&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;''&amp;amp;nbsp;&amp;gt;&amp;amp;nbsp;0 for each ''i''&amp;amp;nbsp;∈&amp;amp;nbsp;''I'' that satisfies &amp;lt;math&amp;gt;\sum_{i\in I} r_i^d&amp;lt;\delta &amp;lt;/math&amp;gt;. (Here, we use the standard convention that [[infimum|inf&amp;amp;nbsp;Ø&amp;amp;nbsp;=&amp;amp;nbsp;∞]].)&lt;br /&gt;
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In other words, &amp;lt;math&amp;gt;C_H^d(S)&amp;lt;/math&amp;gt; is the infimum of the set of numbers &amp;lt;math&amp;gt;\delta \geq 0&amp;lt;/math&amp;gt; such that there is some (indexed) collection of balls &amp;lt;math&amp;gt;\{B(x_i,r_i):i\in I\}&amp;lt;/math&amp;gt; covering S with r&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;&amp;amp;nbsp;&amp;gt;&amp;amp;nbsp;0 for each i&amp;amp;nbsp;∈&amp;amp;nbsp;I that satisfies &amp;lt;math&amp;gt;\sum_{i\in I} r_i^d&amp;lt;\delta &amp;lt;/math&amp;gt;. (Here, we use the standard convention that inf&amp;amp;nbsp;Ø&amp;amp;nbsp;=&amp;amp;nbsp;∞.)&lt;br /&gt;
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换句话说，&amp;lt;math&amp;gt;C_H^d(S)&amp;lt;/math&amp;gt; 是数字集合&amp;lt;math&amp;gt;\delta \geq 0&amp;lt;/math&amp;gt;的下确界，使得在 ''i''&amp;amp;nbsp;∈&amp;amp;nbsp中存在一些球集合 &amp;lt;math&amp;gt;\{B(x_i,r_i):i\in I\}&amp;lt;/math&amp;gt;  i 包含 s，对于每个 ''r&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;''&amp;amp;nbsp;&amp;gt;&amp;amp;nbsp;0 满足 i 中的和&amp;lt;math&amp;gt;\sum_{i\in I} r_i^d&amp;lt;\delta &amp;lt;/math&amp;gt; (在这里，我们使用inf&amp;amp;nbsp;Ø&amp;amp;nbsp;=&amp;amp;nbsp;∞ )的标准约定。&lt;br /&gt;
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===Hausdorff measurement豪斯多夫分形测量===&lt;br /&gt;
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The Hausdorff outer measure is different from the unbounded Hausdorf content in that rather than considering all possible coverings of ''S'', we see what happens when the sizes of the balls go to zero. This is  for &amp;lt;math&amp;gt;d \geq 0 &amp;lt;/math&amp;gt;, we define the ''d''-dimensional Hausdorff outer measure of ''S'' as&lt;br /&gt;
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The Hausdorff outer measure is different from the unbounded Hausdorf content in that rather than considering all possible coverings of S, we see what happens when the sizes of the balls go to zero. This is  for &amp;lt;math&amp;gt;d \geq 0 &amp;lt;/math&amp;gt;, we define the d-dimensional Hausdorff outer measure of S as&lt;br /&gt;
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豪斯多夫外测度不同于无界的豪斯多夫，因为我们不考虑 s 的所有可能，我们看到当球的大小为零时会发生什么。这是为了数学  &amp;lt;math&amp;gt;d \geq 0 &amp;lt;/math&amp;gt;，我们定义了  ''S''的 ''d''维豪斯多夫Hausdorff 外测度为&lt;br /&gt;
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:&amp;lt;math&amp;gt; \mathcal{H}^d(S):=\lim_{r \to 0} \inf\Bigl\{\sum_i r_i^d:\text{ there is a cover of } S\text{ by balls with radii } 0 &amp;lt; r_i &amp;lt; r\Bigr\}.&amp;lt;/math&amp;gt;&lt;br /&gt;
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&amp;lt;math&amp;gt; \mathcal{H}^d(S):=\lim_{r \to 0} \inf\Bigl\{\sum_i r_i^d:\text{ there is a cover of } S\text{ by balls with radii } 0 &amp;lt; r_i &amp;lt; r\Bigr\}.&amp;lt;/math&amp;gt;&lt;br /&gt;
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&amp;lt;math&amp;gt; \mathcal{H}^d(S):=\lim_{r \to 0} \inf\Bigl\{\sum_i r_i^d:\text{有一个面} S\text{ 球 } 0 &amp;lt; r_i &amp;lt; r\Bigr\}.&amp;lt;/math&amp;gt;&lt;br /&gt;
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===Hausdorff dimension豪斯多夫维数===&lt;br /&gt;
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The '''Hausdorff dimension''' of ''X'' is defined by&lt;br /&gt;
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The Hausdorff dimension of X is defined by&lt;br /&gt;
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X 的豪斯多夫维数定义为&lt;br /&gt;
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:&amp;lt;math&amp;gt;\dim_{\operatorname{H}}(X):=\inf\{d\ge 0: \mathcal{H}^d(X)=0\}.&amp;lt;/math&amp;gt;&lt;br /&gt;
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&amp;lt;math&amp;gt;\dim_{\operatorname{H}}(X):=\inf\{d\ge 0: \mathcal{H}^d(X)=0\}.&amp;lt;/math&amp;gt;&lt;br /&gt;
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Equivalently, dim&amp;lt;sub&amp;gt;H&amp;lt;/sub&amp;gt;(''X'') may be defined as the [[infimum]] of the set of ''d'' ∈ [0, ∞) such that the ''d''-dimensional [[Hausdorff measure]] of ''X'' is zero. This is the same as the supremum of the set of ''d''&amp;amp;nbsp;∈&amp;amp;nbsp;[0,&amp;amp;nbsp;∞) such that the ''d''-dimensional Hausdorff measure of ''X'' is infinite (except that when this latter set of numbers ''d'' is empty the Hausdorff dimension is zero).&lt;br /&gt;
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Equivalently, dim&amp;lt;sub&amp;gt;H&amp;lt;/sub&amp;gt;(X) may be defined as the infimum of the set of d ∈ [0, ∞) such that the d-dimensional Hausdorff measure of X is zero. This is the same as the supremum of the set of d&amp;amp;nbsp;∈&amp;amp;nbsp;[0,&amp;amp;nbsp;∞) such that the d-dimensional Hausdorff measure of X is infinite (except that when this latter set of numbers d is empty the Hausdorff dimension is zero).&lt;br /&gt;
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等价地，dim &amp;lt;sub&amp;gt;H&amp;lt;/sub&amp;gt;(''X'')可定义为 ''d'' ∈ [0, ∞) 集的下确界，使得''X'' 的''d''-维 [[豪斯多夫测度]] 为零。这与 ''d''&amp;amp;nbsp;∈&amp;amp;nbsp;[0,&amp;amp;nbsp;∞)的集合的上确界相同，因此''X''的 d 维豪斯多夫测度是无限的(除非后一个集合 ''d'' 是空的，豪斯多夫维数为零)。&lt;br /&gt;
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==Examples实例==&lt;br /&gt;
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[[Image:Sierpinski deep.svg|thumb|250px|Dimension of a further [[fractal]] example. The [[Sierpinski triangle]], an object with Hausdorff dimension of log(3)/log(2)≈1.58.&amp;lt;ref name=ClaytonSCTPLS96/&amp;gt;]]&lt;br /&gt;
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Dimension of a further [[fractal example. The Sierpinski triangle, an object with Hausdorff dimension of log(3)/log(2)≈1.58.]]&lt;br /&gt;
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[[Image:谢尔宾斯基三角形 deep.svg|thumb|250px|进一步的[[分形维数]]的例子，进一步的分形维数的例子是谢尔宾斯基三角形，它是一个豪斯多夫维数为log(3)/log(2)≈1.58.&amp;lt;ref name=ClaytonSCTPLS96/&amp;gt;的物体]]&lt;br /&gt;
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* [[Countable set]]s have Hausdorff dimension 0.&amp;lt;ref name=&amp;quot;schleicher&amp;quot;&amp;gt;{{cite journal |last1=Schleicher |first1=Dierk |title=Hausdorff Dimension, Its Properties, and Its Surprises |journal=The American Mathematical Monthly |date=June 2007 |volume=114 |issue=6 |pages=509–528 |doi=10.1080/00029890.2007.11920440 |language=en |issn=0002-9890|arxiv=math/0505099 }}&amp;lt;/ref&amp;gt;&lt;br /&gt;
*[[可数集]]拥有豪斯多夫维数0.&amp;lt;ref name=&amp;quot;schleicher&amp;quot;&amp;gt;{{cite journal |last1=Schleicher |first1=Dierk |title=豪斯多夫维数, Its Properties, and Its Surprises |journal=The American Mathematical Monthly美国数学期刊 |date=June 2007 |volume=114 |issue=6 |pages=509–528 |doi=10.1080/00029890.2007.11920440 |language=en |issn=0002-9890|arxiv=math/0505099 }}&amp;lt;/ref&amp;gt;&lt;br /&gt;
* The [[Euclidean space]] ℝ&amp;lt;sup&amp;gt;''n''&amp;lt;/sup&amp;gt; has Hausdorff dimension ''n'', and the circle '''S'''&amp;lt;sup&amp;gt;1&amp;lt;/sup&amp;gt; has Hausdorff dimension 1.&amp;lt;ref name=&amp;quot;schleicher&amp;quot; /&amp;gt;&lt;br /&gt;
*[[教育空间]] ℝ&amp;lt;sup&amp;gt;''n''&amp;lt;/sup&amp;gt; 有豪斯多夫维数 ''n''，循环'''S'''&amp;lt;sup&amp;gt;1&amp;lt;/sup&amp;gt; 拥有豪斯多夫维数1.&amp;lt;ref name=&amp;quot;schleicher&amp;quot; /&amp;gt;&lt;br /&gt;
* [[Fractal]]s often are spaces whose Hausdorff dimension strictly exceeds the [[topological dimension]].&amp;lt;ref name=&amp;quot;mandelbrot&amp;quot; /&amp;gt; For example, the [[Cantor set]], a zero-dimensional topological space, is a union of two copies of itself, each copy shrunk by a factor 1/3; hence, it can be shown that its Hausdorff dimension is ln(2)/ln(3)&amp;amp;nbsp;≈&amp;amp;nbsp;0.63.&amp;lt;ref&amp;gt;{{cite book | last=Falconer | first = Kenneth |title=Fractal Geometry: Mathematical Foundations and Applications | publisher=[[John Wiley and Sons]] | edition=2nd | year=2003}}&amp;lt;/ref&amp;gt; The [[Sierpinski triangle]] is a union of three copies of itself, each copy shrunk by a factor of&amp;amp;nbsp;1/2; this yields a Hausdorff dimension of ln(3)/ln(2)&amp;amp;nbsp;≈&amp;amp;nbsp;1.58.&amp;lt;ref name=CampbellAnnenberg15/&amp;gt; These Hausdorff dimensions are related to the &amp;quot;critical exponent&amp;quot; of the [[Master theorem (analysis of algorithms)|Master theorem]] for solving [[Recurrence relation|recurrence relations]] in the [[analysis of algorithms]].&lt;br /&gt;
*[[分形]]一般是那些豪斯多夫维数直接超过其拓扑维数的空间。例如[[康托尔集]]是一个o维拓扑空间，由两个自己复制而成，每一个复制品都是原来的三分之一，因此它的豪斯多夫维数是 ln(2)/ln(3)&amp;amp;nbsp;≈&amp;amp;nbsp;0.63。&amp;lt;ref&amp;gt;{{cite book | last=Falconer | first = Kenneth |title=Fractal Geometry: Mathematical Foundations and Applications | publisher=[[John Wiley and Sons]] | edition=2nd | year=2003}}&amp;lt;/ref&amp;gt;一个[[谢尔宾斯基三角]]是他自身三个复制的组合。每一个是原来的&amp;amp;nbsp;1/2，它的豪斯多夫维数ln(3)/ln(2)&amp;amp;nbsp;≈&amp;amp;nbsp;1.58。&amp;lt;ref name=CampbellAnnenberg15/&amp;gt;在递归算法中解决递归关系时，这些豪斯多夫维数与[[算法分析主定理]]的临界指标相联系。&lt;br /&gt;
* [[Space-filling curve]]s like the [[Peano curve]] have the same Hausdorff dimension as the space they fill.&lt;br /&gt;
*[[空间填充曲线]]拥有和他们填充空间同样的豪斯多夫维数，如[[皮亚诺曲线]]。&lt;br /&gt;
* The trajectory of [[Brownian motion]] in dimension 2 and above is conjectured to be Hausdorff dimension 2.&amp;lt;ref&amp;gt;{{cite book | last=Morters | first=Peres | title= Brownian Motion | publisher=[[Cambridge University Press]] | year=2010 }}&amp;lt;/ref&amp;gt;&lt;br /&gt;
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[[image:Great Britain Hausdorff.svg|thumb|250px|Estimating the Hausdorff dimension of the [[How Long Is the Coast of Britain? Statistical Self-Similarity and Fractional Dimension|coast of Great Britain]]]]&lt;br /&gt;
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coast of Great Britain]]&lt;br /&gt;
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[[大不列颠海岸&lt;br /&gt;
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* 刘易斯·弗赖伊·理查森[[Lewis Fry Richardson]] has performed detailed experiments to measure the approximate Hausdorff dimension for various coastlines. His results have varied from 1.02 for the coastline of [[South Africa]] to 1.25 for the west coast of [[Great Britain]].&amp;lt;ref name=&amp;quot;mandelbrot&amp;quot; /&amp;gt;&lt;br /&gt;
*刘易斯·弗赖伊·理查森（Lewis Fry Richardson）已经通过豪斯多夫维数去测量了很多海岸线。它的结果涵盖从1.02的南非海岸线到1.25的大英帝国西海岸模型。]]&lt;br /&gt;
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==Properties of Hausdorff dimension豪斯多夫维数特性==&lt;br /&gt;
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{{refimprove section|date=March 2015}}&lt;br /&gt;
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=== Hausdorff dimension and inductive dimension 豪斯多夫维数和归纳维数===&lt;br /&gt;
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Let ''X'' be an arbitrary [[Separable space|separable]] metric space. There is a [[topology|topological]] notion of [[inductive dimension]] for ''X'' which is defined recursively. It is always an integer (or +∞) and is denoted dim&amp;lt;sub&amp;gt;ind&amp;lt;/sub&amp;gt;(''X'').&lt;br /&gt;
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Let X be an arbitrary separable metric space. There is a topological notion of inductive dimension for X which is defined recursively. It is always an integer (or +∞) and is denoted dim&amp;lt;sub&amp;gt;ind&amp;lt;/sub&amp;gt;(X).&lt;br /&gt;
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设''X'' 是[[任意可分度量空间]]。对于''X'' 有一个递归定义的归纳维数拓扑概念。它总是一个整数(或 + ∞) ，记为dim&amp;lt;sub&amp;gt;ind&amp;lt;/sub&amp;gt;(''X'')。&lt;br /&gt;
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'''Theorem'''. Suppose ''X'' is non-empty. Then &lt;br /&gt;
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Theorem. Suppose X is non-empty. Then &lt;br /&gt;
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'''定理'''：假设''X'' 是非空的, 那么&lt;br /&gt;
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:&amp;lt;math&amp;gt; \dim_{\mathrm{Haus}}(X) \geq \dim_{\operatorname{ind}}(X). &amp;lt;/math&amp;gt;&lt;br /&gt;
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&amp;lt;math&amp;gt; \dim_{\mathrm{Haus}}(X) \geq \dim_{\operatorname{ind}}(X). &amp;lt;/math&amp;gt;&lt;br /&gt;
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Moreover,&lt;br /&gt;
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Moreover,&lt;br /&gt;
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此外,&lt;br /&gt;
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&amp;lt;math&amp;gt; \inf_Y \dim_{\operatorname{Haus}}(Y) =\dim_{\operatorname{ind}}(X), &amp;lt;/math&amp;gt;&lt;br /&gt;
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&amp;lt;math&amp;gt; \inf_Y \dim_{\operatorname{Haus}}(Y) =\dim_{\operatorname{ind}}(X), &amp;lt;/math&amp;gt;&lt;br /&gt;
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where ''Y'' ranges over metric spaces [[homeomorphic]] to ''X''. In other words, ''X'' and ''Y'' have the same underlying set of points and the metric ''d''&amp;lt;sub&amp;gt;''Y''&amp;lt;/sub&amp;gt; of ''Y'' is topologically equivalent to ''d''&amp;lt;sub&amp;gt;''X''&amp;lt;/sub&amp;gt;.&lt;br /&gt;
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where Y ranges over metric spaces homeomorphic to X. In other words, X and Y have the same underlying set of points and the metric d&amp;lt;sub&amp;gt;Y&amp;lt;/sub&amp;gt; of Y is topologically equivalent to d&amp;lt;sub&amp;gt;X&amp;lt;/sub&amp;gt;.&lt;br /&gt;
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其中''Y''是度量空间同胚到 ''X''的范围。换句话说， ''X''和 ''Y''具有相同的基本点集，''Y''的度量''d''&amp;lt;sub&amp;gt;''Y''&amp;lt;/sub&amp;gt; 拓扑等价于''d''&amp;lt;sub&amp;gt;''X''&amp;lt;/sub&amp;gt;。&lt;br /&gt;
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&lt;br /&gt;
&lt;br /&gt;
These results were originally established by [[Edward Szpilrajn]] (1907–1976), e.g., see Hurewicz and Wallman, Chapter VII.{{full citation needed|date=March 2015}}&lt;br /&gt;
&lt;br /&gt;
These results were originally established by Edward Szpilrajn (1907–1976), e.g., see Hurewicz and Wallman, Chapter VII.&lt;br /&gt;
&lt;br /&gt;
这些结果最初是由 [[Edward Szpilrajn]] (1907–1976)建立的,  参见 Hurewicz and Wallman, Chapter VII.{{full citation needed|date=March 2015}}第七章。&lt;br /&gt;
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=== Hausdorff dimension and Minkowski dimension 豪斯多夫维数和闵可夫斯基维度===&lt;br /&gt;
&lt;br /&gt;
The [[Minkowski dimension]] is similar to, and at least as large as, the Hausdorff dimension, and they are equal in many situations. However, the set of [[rational number|rational]] points in [0, 1] has Hausdorff dimension zero and Minkowski dimension one. There are also compact sets for which the Minkowski dimension is strictly larger than the Hausdorff dimension.&lt;br /&gt;
&lt;br /&gt;
The Minkowski dimension is similar to, and at least as large as, the Hausdorff dimension, and they are equal in many situations. However, the set of rational points in [0, 1] has Hausdorff dimension zero and Minkowski dimension one. There are also compact sets for which the Minkowski dimension is strictly larger than the Hausdorff dimension.&lt;br /&gt;
&lt;br /&gt;
[[闵可夫斯基维数]]与豪斯多夫维数相似，至少和它一样大，而且在许多情况下是相等的。然而，[0,1]中有理点集的豪斯多夫维数为0，闵可夫斯基维数为1。还有一些紧集的闵可夫斯基维数严格大于豪斯多夫维数。&lt;br /&gt;
&lt;br /&gt;
=== Hausdorff dimensions and Frostman measures 豪斯多夫维度和弗洛斯曼测度===&lt;br /&gt;
&lt;br /&gt;
If there is a [[measure (mathematics)|measure]] μ defined on [[Borel measure|Borel]] subsets of a metric space ''X'' such that ''μ''(''X'') &amp;gt; 0 and ''μ''(''B''(''x'', ''r'')) ≤ ''r&amp;lt;sup&amp;gt;s&amp;lt;/sup&amp;gt;'' holds for some constant ''s'' &amp;gt; 0 and for every ball ''B''(''x'', ''r'') in ''X'', then dim&amp;lt;sub&amp;gt;Haus&amp;lt;/sub&amp;gt;(''X'') ≥ ''s''. A partial converse is provided by [[Frostman's lemma]].{{citation needed|date=March 2015}}&amp;lt;ref&amp;gt;This Wikipedia article also discusses further useful characterizations of the Hausdorff dimension.{{clarify|date=March 2015}}&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
If there is a measure μ defined on Borel subsets of a metric space X such that μ(X) &amp;gt; 0 and μ(B(x, r)) ≤ r&amp;lt;sup&amp;gt;s&amp;lt;/sup&amp;gt; holds for some constant s &amp;gt; 0 and for every ball B(x, r) in X, then dim&amp;lt;sub&amp;gt;Haus&amp;lt;/sub&amp;gt;(X) ≥ s. A partial converse is provided by Frostman's lemma.&lt;br /&gt;
&lt;br /&gt;
如果在度量空间 ''X'' 的 Borel 子集上定义一个测度 μ，使得''μ''(''X'') &amp;gt; 0 和''μ''(''B''(''x'', ''r'')) ≤ ''r&amp;lt;sup&amp;gt;s&amp;lt;/sup&amp;gt;''，对于某个常数 ''s'' &amp;gt; 0  和 ''X'' 中的每个球 ''B''(''x'', ''r'') 成立，则 dim&amp;lt;sub&amp;gt;Haus&amp;lt;/sub&amp;gt;(''X'') ≥ ''s'' 。 部分逆向转换由弗洛斯曼引理定义。&lt;br /&gt;
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=== Behaviour under unions and products ===&lt;br /&gt;
&lt;br /&gt;
If &amp;lt;math&amp;gt;X=\bigcup_{i\in I}X_i&amp;lt;/math&amp;gt; is a finite or countable union, then&lt;br /&gt;
&lt;br /&gt;
If &amp;lt;math&amp;gt;X=\bigcup_{i\in I}X_i&amp;lt;/math&amp;gt; is a finite or countable union, then&lt;br /&gt;
&lt;br /&gt;
如果 &amp;lt;math&amp;gt;X=\bigcup_{i\in I}X_i&amp;lt;/math&amp;gt; 是一个有限或可数的联合，则&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \dim_{\operatorname{Haus}}(X) =\sup_{i\in I} \dim_{\operatorname{Haus}}(X_i).&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \dim_{\operatorname{Haus}}(X) =\sup_{i\in I} \dim_{\operatorname{Haus}}(X_i).&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
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&lt;br /&gt;
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This can be verified directly from the definition.&lt;br /&gt;
&lt;br /&gt;
This can be verified directly from the definition.&lt;br /&gt;
&lt;br /&gt;
这可以直接从定义得到验证。&lt;br /&gt;
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If ''X'' and ''Y'' are non-empty metric spaces, then the Hausdorff dimension of their product satisfies&amp;lt;ref&amp;gt;{{cite journal |author=Marstrand, J. M. |title=The dimension of Cartesian product sets |journal=Proc. Cambridge Philos. Soc. |volume=50 |issue=3 |pages=198–202 |year=1954 |doi=10.1017/S0305004100029236 |bibcode = 1954PCPS...50..198M }}&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
If X and Y are non-empty metric spaces, then the Hausdorff dimension of their product satisfies&lt;br /&gt;
&lt;br /&gt;
如果 ''X'' 和''Y''是非空度量空间，那么它们乘积的豪斯多夫维数满足&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt; \dim_{\operatorname{Haus}}(X\times Y)\ge \dim_{\operatorname{Haus}}(X)+ \dim_{\operatorname{Haus}}(Y).&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \dim_{\operatorname{Haus}}(X\times Y)\ge \dim_{\operatorname{Haus}}(X)+ \dim_{\operatorname{Haus}}(Y).&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
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This inequality can be strict. It is possible to find two sets of dimension 0 whose product has dimension 1.&amp;lt;ref&amp;gt;{{cite book  | last = Falconer  | first = Kenneth J.  | title = Fractal geometry. Mathematical foundations and applications  | publisher = John Wiley &amp;amp; Sons, Inc., Hoboken, New Jersey  | year = 2003  | doi =   | isbn = }}&amp;lt;/ref&amp;gt; In the opposite direction, it is known that when ''X'' and ''Y'' are Borel subsets of '''R'''&amp;lt;sup&amp;gt;''n''&amp;lt;/sup&amp;gt;, the Hausdorff dimension of ''X'' × ''Y'' is bounded from above by the Hausdorff dimension of ''X'' plus the [[packing dimension|upper packing dimension]] of ''Y''. These facts are discussed in Mattila (1995).&lt;br /&gt;
&lt;br /&gt;
This inequality can be strict. It is possible to find two sets of dimension 0 whose product has dimension 1. In the opposite direction, it is known that when X and Y are Borel subsets of R&amp;lt;sup&amp;gt;n&amp;lt;/sup&amp;gt;, the Hausdorff dimension of X × Y is bounded from above by the Hausdorff dimension of X plus the upper packing dimension of Y. These facts are discussed in Mattila (1995).&lt;br /&gt;
&lt;br /&gt;
这种不平等可以是严格的。有可能找到两个维数为0的集合，其乘积的维数为1。相反，我们知道当''X''和''Y''是 '''R'''&amp;lt;sup&amp;gt;''n''&amp;lt;/sup&amp;gt;的 Borel 子集时， ''X'' × ''Y''的豪斯多夫维数从上面以 ''X''的豪斯多夫维数加上 ''Y''的上填充维数为界。Mattila (1995)曾就这些情况进行了讨论。&lt;br /&gt;
&lt;br /&gt;
==Self-similar sets自相似集合==&lt;br /&gt;
&lt;br /&gt;
{{refimprove section|date=March 2015}}&lt;br /&gt;
&lt;br /&gt;
Many sets defined by a self-similarity condition have dimensions which can be determined explicitly. Roughly, a set ''E'' is self-similar if it is the fixed point of a set-valued transformation ψ, that is ψ(''E'') = ''E'', although the exact definition is given below.&lt;br /&gt;
&lt;br /&gt;
Many sets defined by a self-similarity condition have dimensions which can be determined explicitly. Roughly, a set E is self-similar if it is the fixed point of a set-valued transformation ψ, that is ψ(E) = E, although the exact definition is given below.&lt;br /&gt;
&lt;br /&gt;
许多由自相似条件定义的集合具有可以显式确定的维数。粗略地说，如果集合''E''是集值ψ变换的不动点，即ψ(''E'') = ''E''， 则它是自相似的，尽管下面给出了确切的定义。&lt;br /&gt;
&lt;br /&gt;
&amp;lt;blockquote&amp;gt;'''Theorem'''. Suppose&lt;br /&gt;
&lt;br /&gt;
&amp;lt;blockquote&amp;gt;Theorem. Suppose&lt;br /&gt;
&lt;br /&gt;
&amp;lt;blockquote&amp;gt;'''定理'''：假设&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt; \psi_i: \mathbf{R}^n \rightarrow \mathbf{R}^n, \quad i=1, \ldots , m &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \psi_i: \mathbf{R}^n \rightarrow \mathbf{R}^n, \quad i=1, \ldots , m &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
are [[Contraction mapping|contractive]] mappings on '''R'''&amp;lt;sup&amp;gt;''n''&amp;lt;/sup&amp;gt; with contraction constant ''r&amp;lt;sub&amp;gt;j&amp;lt;/sub&amp;gt;'' &amp;lt; 1. Then there is a unique ''non-empty'' compact set ''A'' such that&lt;br /&gt;
&lt;br /&gt;
are contractive mappings on R&amp;lt;sup&amp;gt;n&amp;lt;/sup&amp;gt; with contraction constant r&amp;lt;sub&amp;gt;j&amp;lt;/sub&amp;gt; &amp;lt; 1. Then there is a unique non-empty compact set A such that&lt;br /&gt;
&lt;br /&gt;
是'''R'''&amp;lt;sup&amp;gt;''n''&amp;lt;/sup&amp;gt;上的压缩常数''r&amp;lt;sub&amp;gt;j&amp;lt;/sub&amp;gt;'&amp;lt; 1的压缩映射。则有一个唯一的非空紧集A &lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt; A = \bigcup_{i=1}^m \psi_i (A). &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; A = \bigcup_{i=1}^m \psi_i (A). &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&amp;lt;/blockquote&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;/blockquote&amp;gt;&lt;br /&gt;
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&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The theorem follows from [[Stefan Banach]]'s [[Contractive mapping theorem|contractive mapping fixed point theorem]] applied to the complete metric space of non-empty compact subsets of '''R'''&amp;lt;sup&amp;gt;''n''&amp;lt;/sup&amp;gt; with the [[Hausdorff distance]].&amp;lt;ref&amp;gt;{{cite book |author=Falconer, K. J. |title=The Geometry of Fractal Sets |publisher=Cambridge University Press |location=Cambridge, UK |year=1985 |isbn=0-521-25694-1 |chapter=Theorem 8.3}}&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
The theorem follows from Stefan Banach's contractive mapping fixed point theorem applied to the complete metric space of non-empty compact subsets of R&amp;lt;sup&amp;gt;n&amp;lt;/sup&amp;gt; with the Hausdorff distance.&lt;br /&gt;
&lt;br /&gt;
这个定理来源于 Stefan Banach 的压缩映射不动点定理，该定理应用于 具有豪斯多夫距离的'''R'''&amp;lt;sup&amp;gt;''n''&amp;lt;/sup&amp;gt; 的非空紧子集的完整度量空间。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
===The open set condition开集条件===&lt;br /&gt;
&lt;br /&gt;
To determine the dimension of the self-similar set ''A'' (in certain cases), we need a technical condition called the ''open set condition'' (OSC) on the sequence of contractions ψ&amp;lt;sub&amp;gt;''i''&amp;lt;/sub&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
To determine the dimension of the self-similar set A (in certain cases), we need a technical condition called the open set condition (OSC) on the sequence of contractions ψ&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
为了确定自相似集''A'' 的维数(在某些情况下) ，我们需要一个关于收缩序列的称为''开集条件''(OSC)的技术条件ψ&amp;lt;sub&amp;gt;''i''&amp;lt;/sub&amp;gt;。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
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There is a relatively compact open set ''V'' such that&lt;br /&gt;
&lt;br /&gt;
There is a relatively compact open set V such that&lt;br /&gt;
&lt;br /&gt;
有一个相对紧的开集''V''&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt; \bigcup_{i=1}^m\psi_i (V) \subseteq V, &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \bigcup_{i=1}^m\psi_i (V) \subseteq V, &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
where the sets in union on the left are pairwise [[disjoint sets|disjoint]].&lt;br /&gt;
&lt;br /&gt;
where the sets in union on the left are pairwise disjoint.&lt;br /&gt;
&lt;br /&gt;
左边并集的集合成对不相交。&lt;br /&gt;
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&lt;br /&gt;
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The open set condition is a separation condition that ensures the images ψ&amp;lt;sub&amp;gt;''i''&amp;lt;/sub&amp;gt;(''V'') do not overlap &amp;quot;too much&amp;quot;.&lt;br /&gt;
&lt;br /&gt;
The open set condition is a separation condition that ensures the images ψ&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;(V) do not overlap &amp;quot;too much&amp;quot;.&lt;br /&gt;
&lt;br /&gt;
开集条件是保证图像ψ&amp;lt;sub&amp;gt;''i''&amp;lt;/sub&amp;gt;(''V'') 不重叠“太多”的分离条件。&lt;br /&gt;
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'''Theorem'''. Suppose the open set condition holds and each ψ&amp;lt;sub&amp;gt;''i''&amp;lt;/sub&amp;gt; is a similitude, that is a composition of an [[isometry]] and a [[dilation (metric space)|dilation]] around some point. Then the unique fixed point of ψ is a set whose Hausdorff dimension is ''s'' where ''s'' is the unique solution of&amp;lt;ref&amp;gt;{{cite journal | last=Hutchinson | first=John E. | title=Fractals and self similarity | journal=Indiana Univ. Math. J. | volume=30 | year=1981 | pages=713–747 | doi=10.1512/iumj.1981.30.30055 | issue=5 | doi-access=free }}&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
Theorem. Suppose the open set condition holds and each ψ&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt; is a similitude, that is a composition of an isometry and a dilation around some point. Then the unique fixed point of ψ is a set whose Hausdorff dimension is s where s is the unique solution of&lt;br /&gt;
&lt;br /&gt;
'''定理'''假设开集条件成立，并且每个ψ&amp;lt;sub&amp;gt;''i''&amp;lt;/sub&amp;gt; 是一个相似度，即等距和某个点周围的膨胀的组合。。那么唯一的不动点是Hausdorff维数为 ''s'' 的集合，其中  ''s'' 是 ''s'' &amp;lt;ref&amp;gt;{{cite journal | last=Hutchinson | first=John E. | title=Fractals and self similarity | journal=Indiana Univ. Math. J. | volume=30 | year=1981 | pages=713–747 | doi=10.1512/iumj.1981.30.30055 | issue=5 | doi-access=free }}&amp;lt;/ref&amp;gt;的唯一解&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt; \sum_{i=1}^m r_i^s = 1. &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \sum_{i=1}^m r_i^s = 1. &amp;lt;/math&amp;gt;&lt;br /&gt;
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The contraction coefficient of a similitude is the magnitude of the dilation.&lt;br /&gt;
&lt;br /&gt;
The contraction coefficient of a similitude is the magnitude of the dilation.&lt;br /&gt;
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相似物的收缩系数就是膨胀的大小。&lt;br /&gt;
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&lt;br /&gt;
We can use this theorem to compute the Hausdorff dimension of the Sierpinski triangle (or sometimes called Sierpinski gasket). Consider three [[non-collinear points]] ''a''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;, ''a''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;, ''a''&amp;lt;sub&amp;gt;3&amp;lt;/sub&amp;gt; in the plane '''R'''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; and let ψ&amp;lt;sub&amp;gt;''i''&amp;lt;/sub&amp;gt; be the dilation of ratio 1/2 around ''a&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;''. The unique non-empty fixed point of the corresponding mapping ψ is a Sierpinski gasket and the dimension ''s'' is the unique solution of&lt;br /&gt;
&lt;br /&gt;
We can use this theorem to compute the Hausdorff dimension of the Sierpinski triangle (or sometimes called Sierpinski gasket). Consider three non-collinear points a&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;, a&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;, a&amp;lt;sub&amp;gt;3&amp;lt;/sub&amp;gt; in the plane R&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; and let ψ&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt; be the dilation of ratio 1/2 around a&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;. The unique non-empty fixed point of the corresponding mapping ψ is a Sierpinski gasket and the dimension s is the unique solution of&lt;br /&gt;
&lt;br /&gt;
我们可以使用这个定理来计算谢尔宾斯基三角形的豪斯多夫维数(或者有时候叫做谢尔宾斯基垫圈)。考虑R&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; 平面上的三个非共线点，''a''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;，''a''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;，''a''&amp;lt;sub&amp;gt;3&amp;lt;/sub&amp;gt;，让ψ&amp;lt;sub&amp;gt;''i''&amp;lt;/sub&amp;gt;是围绕着''a&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;''比率1/2的膨胀。对应映射的唯一非空不动点是一个谢尔宾斯基垫圈，其维数''s''是对应映射的唯一解&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt; \left(\frac{1}{2}\right)^s+\left(\frac{1}{2}\right)^s+\left(\frac{1}{2}\right)^s = 3 \left(\frac{1}{2}\right)^s =1. &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \left(\frac{1}{2}\right)^s+\left(\frac{1}{2}\right)^s+\left(\frac{1}{2}\right)^s = 3 \left(\frac{1}{2}\right)^s =1. &amp;lt;/math&amp;gt;&lt;br /&gt;
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Taking [[natural logarithm]]s of both sides of the above equation, we can solve for ''s'', that is: ''s'' = ln(3)/ln(2).  The Sierpinski gasket is self-similar and satisfies the OSC. In general a set ''E'' which is a fixed point of a mapping&lt;br /&gt;
&lt;br /&gt;
Taking natural logarithms of both sides of the above equation, we can solve for s, that is: s = ln(3)/ln(2).  The Sierpinski gasket is self-similar and satisfies the OSC. In general a set E which is a fixed point of a mapping&lt;br /&gt;
&lt;br /&gt;
取上述方程两边的自然对数，我们可以求出 ''s''，即: ''s'' = ln(3)/ln(2)。该密封垫具有自相似性，满足 OSC 要求。一般来说，集合 ''E''是一个映射的不动点&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt; A \mapsto \psi(A) = \bigcup_{i=1}^m \psi_i(A) &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt; A \mapsto \psi(A) = \bigcup_{i=1}^m \psi_i(A) &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
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is self-similar if and only if the intersections&lt;br /&gt;
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is self-similar if and only if the intersections&lt;br /&gt;
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是自相似的，当且仅当&lt;br /&gt;
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&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt; H^s\left(\psi_i(E) \cap \psi_j(E)\right) =0, &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; H^s\left(\psi_i(E) \cap \psi_j(E)\right) =0, &amp;lt;/math&amp;gt;&lt;br /&gt;
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where ''s'' is the Hausdorff dimension of ''E'' and ''H&amp;lt;sup&amp;gt;s&amp;lt;/sup&amp;gt;'' denotes [[Hausdorff measure]]. This is clear in the case of the Sierpinski gasket (the intersections are just points), but is also true more generally:&lt;br /&gt;
&lt;br /&gt;
where s is the Hausdorff dimension of E and H&amp;lt;sup&amp;gt;s&amp;lt;/sup&amp;gt; denotes Hausdorff measure. This is clear in the case of the Sierpinski gasket (the intersections are just points), but is also true more generally:&lt;br /&gt;
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其中 ''s''是''E''的豪斯多夫维数， ''H&amp;lt;sup&amp;gt;s&amp;lt;/sup&amp;gt;'' 表示 豪斯多夫测度。对于谢尔宾斯基垫圈(交叉点就是点)来说，这一点很明显，但更普遍的情况是:&lt;br /&gt;
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'''Theorem'''. Under the same conditions as the previous theorem, the unique fixed point of ψ is self-similar.&lt;br /&gt;
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Theorem. Under the same conditions as the previous theorem, the unique fixed point of ψ is self-similar.&lt;br /&gt;
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'''定理'''：在与前一定理相同的条件下，其唯一不动点是自相似的。&lt;br /&gt;
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==See also参阅==&lt;br /&gt;
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* [[List of fractals by Hausdorff dimension豪斯多夫分形维数列表]] Examples of deterministic fractals, random and natural fractals.确定性分形与随机和自然分形的示例。&lt;br /&gt;
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* [[Assouad dimension  Assouad维数]], another variation of fractal dimension that, like Hausdorff dimension, is defined using coverings by balls其他被球覆盖方式定义的分形维数，例如豪斯多夫维数。&lt;br /&gt;
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* [[Intrinsic dimension固有维数]]&lt;br /&gt;
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* [[Packing dimension填充维数]]&lt;br /&gt;
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* [[Fractal dimension分形维数]]&lt;br /&gt;
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==References参考文献==&lt;br /&gt;
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{{reflist}}&lt;br /&gt;
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==Further reading拓展阅读==&lt;br /&gt;
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* {{cite book |last1=Dodson |first1=M. Maurice |title=Fractal Geometry and Applications: A Jubilee of Benoît Mandelbrot |volume=72 |issue=1 |pages=305–347 |last2=Kristensen |first2=Simon |chapter=Hausdorff Dimension and Diophantine Approximation |date=June 12, 2003 |arxiv=math/0305399 |bibcode = 2003math......5399D |doi=10.1090/pspum/072.1/2112110|series=Proceedings of Symposia in Pure Mathematics |isbn=9780821836378 }}&lt;br /&gt;
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* {{cite book |last1=Hurewicz |first1=Witold |authorlink1=Witold Hurewicz |last2=Wallman |first2=Henry |authorlink2=Henry Wallman |title=Dimension Theory |url=https://archive.org/details/in.ernet.dli.2015.84609 |publisher=Princeton University Press |year=1948 }}&lt;br /&gt;
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* {{cite journal |author作者=E. Szpilrajn |authorlink=Edward Marczewski |title=La dimension et la mesure |journal=Fundamenta Mathematicae |volume=28 |pages=81–9 |year=1937 }}&lt;br /&gt;
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* {{cite journal&lt;br /&gt;
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 | last1=Marstrand&lt;br /&gt;
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 | last1=Marstrand&lt;br /&gt;
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 | last1=马斯特兰德&lt;br /&gt;
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 | first1=J. M. | title=The dimension of cartesian product sets | year=1954 | journal=Proc. Cambridge Philos. Soc.&lt;br /&gt;
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 | first1=J. M. | title=The dimension of cartesian product sets | year=1954 | journal=Proc. Cambridge Philos. Soc.&lt;br /&gt;
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 | first1= J. M. | title=笛卡儿积集的维数 | 1954年 |  journal=Proc. Cambridge Philos. Soc.&lt;br /&gt;
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 | volume=50&lt;br /&gt;
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 | volume=50&lt;br /&gt;
&lt;br /&gt;
 | 第50卷&lt;br /&gt;
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 | issue=3&lt;br /&gt;
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 | issue=3&lt;br /&gt;
&lt;br /&gt;
 | 第三期&lt;br /&gt;
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 | pages=198–202&lt;br /&gt;
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 | pages=198–202&lt;br /&gt;
&lt;br /&gt;
 | 第198-202页&lt;br /&gt;
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 | doi=10.1017/S0305004100029236|bibcode = 1954PCPS...50..198M }}&lt;br /&gt;
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 | doi=10.1017/S0305004100029236|bibcode = 1954PCPS...50..198M }}&lt;br /&gt;
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10.1017 / S0305004100029236 | bibcode 1954PCPS... 50. . 198 m }&lt;br /&gt;
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* {{Cite book&lt;br /&gt;
&lt;br /&gt;
 | last1=Mattila&lt;br /&gt;
&lt;br /&gt;
 | last1=Mattila&lt;br /&gt;
&lt;br /&gt;
 | last1=Mattila&lt;br /&gt;
&lt;br /&gt;
 | first1=Pertti | author1-link=Pertti Mattila| title=Geometry of sets and measures in Euclidean spaces | publisher=[[Cambridge University Press]]&lt;br /&gt;
&lt;br /&gt;
 | first1=Pertti | author1-link=Pertti Mattila| title=Geometry of sets and measures in Euclidean spaces | publisher=Cambridge University Press&lt;br /&gt;
&lt;br /&gt;
| first1 Pertti | author1-link Pertti Mattila | title 欧几里德空间中集合和度量的几何 | 出版商剑桥大学出版社&lt;br /&gt;
&lt;br /&gt;
 | isbn=978-0-521-65595-8 | year=1995}}&lt;br /&gt;
&lt;br /&gt;
 | isbn=978-0-521-65595-8 | year=1995}}&lt;br /&gt;
&lt;br /&gt;
| isbn 978-0-521-65595-8 | year 1995}&lt;br /&gt;
&lt;br /&gt;
* {{cite journal |author=A. S. Besicovitch |authorlink=A. S. Besicovitch |title=On Linear Sets of Points of Fractional Dimensions |journal=[[Mathematische Annalen]] |volume=101 |year=1929 | doi=10.1007/BF01454831| issue=1 |pages= 161–193}}&lt;br /&gt;
&lt;br /&gt;
* {{cite journal |author1=A. S. Besicovitch |authorlink1=A. S. Besicovitch |author2=H. D. Ursell |authorlink2=H. D. Ursell |title=Sets of Fractional Dimensions |journal=Journal of the London Mathematical Society |volume=12 |year=1937 | issue=1 | doi=10.1112/jlms/s1-12.45.18  | pages=18–25 }}&amp;lt;br/&amp;gt;Several selections from this volume are reprinted in {{cite book |author=Edgar, Gerald A. |title=Classics on fractals |publisher=Addison-Wesley |location=Boston |year=1993 |isbn=0-201-58701-7}} See chapters 9,10,11&lt;br /&gt;
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* {{cite journal |author=F. Hausdorff |authorlink=F. Hausdorff |title=Dimension und äußeres Maß |journal=Mathematische Annalen |volume=79 |issue=1–2 |pages=157–179 |date=March 1919 |doi=10.1007/BF01457179|hdl=10338.dmlcz/100363 |url=http://dml.cz/bitstream/handle/10338.dmlcz/100363/CzechMathJ_09-1959-3_5.pdf }}&lt;br /&gt;
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* {{cite journal | last=Hutchinson | first=John E. | title=Fractals and self similarity | journal=Indiana Univ. Math. J. | volume=30 | year=1981 | pages=713–747 | doi=10.1512/iumj.1981.30.30055 | issue=5 | doi-access=free }}&lt;br /&gt;
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*{{cite book | last=Falconer | first = Kenneth |title=Fractal Geometry: Mathematical Foundations and Applications | publisher=[[John Wiley and Sons]] | edition=2nd | year=2003}}&lt;br /&gt;
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==External links外部链接==&lt;br /&gt;
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* [https://www.encyclopediaofmath.org/index.php/Hausdorff_dimension Hausdorff dimension] 在 [https://www.encyclopediaofmath.org/ Encyclopedia of Mathematics]&lt;br /&gt;
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* [https://www.encyclopediaofmath.org/index.php/Hausdorff_measure Hausdorff measure] 在 [https://www.encyclopediaofmath.org/ Encyclopedia of Mathematics]&lt;br /&gt;
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{{DEFAULTSORT:Hausdorff Dimension豪斯多夫维数}}&lt;br /&gt;
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[[Category分类:Fractals分形]]&lt;br /&gt;
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[[Category分类:Metric geometry度量几何]]&lt;br /&gt;
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[[Category分类:Dimension theory维度理论]]&lt;br /&gt;
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&amp;lt;small&amp;gt;This page was moved from [[wikipedia:en:Hausdorff dimension]]. Its edit history can be viewed at [[分形维数/edithistory]]&amp;lt;/small&amp;gt;&amp;lt;/noinclude&amp;gt;&lt;br /&gt;
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[[Category:待整理页面]]&lt;/div&gt;</summary>
		<author><name>Ruili</name></author>
	</entry>
	<entry>
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		<title>分形维数</title>
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		<updated>2020-11-01T17:40:18Z</updated>

		<summary type="html">&lt;p&gt;Ruili：&lt;/p&gt;
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&lt;div&gt;此词条暂由彩云小译翻译，未经人工整理和审校，带来阅读不便，请见谅。&lt;br /&gt;
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{{short description|Invariant}}&lt;br /&gt;
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Example of non-integer dimensions. The first four [[iteration]]s of the [[Koch snowflake|Koch curve]], where after each iteration, all original line segments are replaced with four, each a self-similar copy that is 1/3 the length of the original. One formalism of the Hausdorff dimension uses this scale factor (3) and the number of self-similar objects (4) to calculate the dimension, D, after the first iteration to be D = (log N)/(log S) = (log 4)/(log 3) ≈ 1.26.&amp;lt;ref name=CampbellAnnenberg15&amp;gt;MacGregor Campbell, 2013, &amp;quot;5.6 Scaling and the Hausdorff Dimension,&amp;quot; at ''Annenberg Learner:MATHematics illuminated'', see [http://www.learner.org/courses/mathilluminated/units/5/textbook/06.php], accessed 5 March 2015.&amp;lt;/ref&amp;gt; That is, while the Hausdorff dimension of a single [[point (geometry)|point]] is zero, of a [[line segment]] is 1, of a [[square]] is 2, and of a [[cube]] is 3, for [[fractal]]s such as this, the object can have a non-integer dimension.&lt;br /&gt;
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Example of non-integer dimensions. The first four iterations of the Koch curve, where after each iteration, all original line segments are replaced with four, each a self-similar copy that is 1/3 the length of the original. One formalism of the Hausdorff dimension uses this scale factor (3) and the number of self-similar objects (4) to calculate the dimension, D, after the first iteration to be D = (log N)/(log S) = (log 4)/(log 3) ≈ 1.26. That is, while the Hausdorff dimension of a single point is zero, of a line segment is 1, of a square is 2, and of a cube is 3, for fractals such as this, the object can have a non-integer dimension.&lt;br /&gt;
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非整数维度示例：前四个[[Koch 曲线]]的迭代，在每次迭代后，所有原始线段都被替换为四个，每个自相似的复制是原始线段长度的1 / 3。豪斯多夫维数的一个建模是使用比例因子(3)和自相似对象的数量(4)来计算维度 D，在第一次迭代后为 D = (log N)/(log S) = (log 4)/(log 3) ≈ 1.26.&amp;lt;ref name=CampbellAnnenberg15&amp;gt;。MacGregor Campbell, 2013, &amp;quot;5.6 Scaling and the Hausdorff Dimension,&amp;quot; 在 ''Annenberg Learner:MATHematics illuminated'', 参见 [http://www.learner.org/courses/mathilluminated/units/5/textbook/06.php], accessed 5 March 2015.&amp;lt;/ref&amp;gt; 也就是说，单点的豪斯多夫维数为零，线段为1，正方形为2，立方体为3时，但对于分形，对象可以有一个非整数维度。&lt;br /&gt;
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In [[mathematics]], '''Hausdorff dimension''' is a measure of ''roughness'', or more specifically, [[fractal dimension]], that was first introduced in 1918 by [[mathematician]] [[Felix Hausdorff]].&amp;lt;ref&amp;gt;{{Cite journal |arxiv = 1101.1444|doi = 10.1214/11-STS370|title = Estimators of Fractal Dimension: Assessing the Roughness of Time Series and Spatial Data|journal = Statistical Science|volume = 27|issue = 2|pages = 247–277|year = 2012|last1 = Gneiting|first1 = Tilmann|last2 = Ševčíková|first2 = Hana|last3 = Percival|first3 = Donald B.}}&amp;lt;/ref&amp;gt; For instance, the Hausdorff dimension of a single [[point (geometry)|point]] is zero, of a [[line segment]] is 1, of a [[square]] is 2, and of a [[cube]] is 3. That is, for sets of points that define a smooth shape or a shape that has a small number of corners—the shapes of traditional geometry and science—the Hausdorff dimension is an [[integer]] agreeing with the usual sense of dimension, also known as the [[Inductive dimension|topological dimension]]. However, formulas have also been developed that allow calculation of the dimension of other less simple objects, where, solely on the basis of their properties of [[scaling (geometry)|scaling]] and [[self-similarity]], one is led to the conclusion that particular objects—including [[fractal]]s—have non-integer Hausdorff dimensions. Because of the significant technical advances made by [[Abram Samoilovitch Besicovitch]] allowing computation of dimensions for highly irregular or &amp;quot;rough&amp;quot; sets, this dimension is also commonly referred to as the ''Hausdorff–Besicovitch dimension.''&lt;br /&gt;
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In mathematics, Hausdorff dimension is a measure of roughness, or more specifically, fractal dimension, that was first introduced in 1918 by mathematician Felix Hausdorff. For instance, the Hausdorff dimension of a single point is zero, of a line segment is 1, of a square is 2, and of a cube is 3. That is, for sets of points that define a smooth shape or a shape that has a small number of corners—the shapes of traditional geometry and science—the Hausdorff dimension is an integer agreeing with the usual sense of dimension, also known as the topological dimension. However, formulas have also been developed that allow calculation of the dimension of other less simple objects, where, solely on the basis of their properties of scaling and self-similarity, one is led to the conclusion that particular objects—including fractals—have non-integer Hausdorff dimensions. Because of the significant technical advances made by Abram Samoilovitch Besicovitch allowing computation of dimensions for highly irregular or &amp;quot;rough&amp;quot; sets, this dimension is also commonly referred to as the Hausdorff–Besicovitch dimension.&lt;br /&gt;
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在[[数学]]中，'''&amp;lt;font color = '#ff8000'&amp;gt;豪斯多夫维数Hausdorff dimension&amp;lt;/font&amp;gt;'''是一种粗糙度的度量单位，或者更确切地说，分形维数，是由数学家 Felix Hausdorff 在1918年首次提出的。例如，单点的豪斯多夫维数为零，线段为1，正方形为2，立方体为3。也就是说，对于定义了一个光滑形状或一个有少数几个角的形状---- 传统几何学和科学的形状---- 的点集来说，豪斯多夫维数是一个整数，符合通常的维度意义，也称为拓扑维度。然而，还有一些公式允许计算其他不太简单的对象的维数，其中仅仅根据它们的标度和自相似特性，就可以得出结论: 特定的对象ー包括分形ー具有非整数的 Hausdorff 维数。由于阿布拉姆·萨莫伊洛维奇·贝西科维奇的重大技术进步，允许计算高度不规则或“粗糙”集的维度，这个维度通常也被称为 Hausdorff-Besicovitch 维度。 &lt;br /&gt;
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The Hausdorff dimension, more specifically, is a further dimensional number associated with a given set, where the distances between all members of that set are defined. Such a set is termed a [[metric space]]. The dimension is drawn from the [[Extended real number line|extended real numbers]], &amp;lt;math&amp;gt;\overline{\mathbb{R}}&amp;lt;/math&amp;gt;, as opposed to the more intuitive notion of dimension, which is not associated to general metric spaces, and only takes values in the non-negative integers.&lt;br /&gt;
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The Hausdorff dimension, more specifically, is a further dimensional number associated with a given set, where the distances between all members of that set are defined. Such a set is termed a metric space. The dimension is drawn from the extended real numbers, &amp;lt;math&amp;gt;\overline{\mathbb{R}}&amp;lt;/math&amp;gt;, as opposed to the more intuitive notion of dimension, which is not associated to general metric spaces, and only takes values in the non-negative integers.&lt;br /&gt;
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更具体地说，豪斯多夫维数是一个与给定集合相关联的更进一步的维数，其中定义了该集合所有成员之间的距离。这样的集合称为度量空间。维数是从扩展的实数，&amp;lt;math&amp;gt;\overline{\mathbb{R}}&amp;lt;/math&amp;gt;，而不是更直观的维数概念(它不与一般的度量空间相关联，只取非负整数的值)。&lt;br /&gt;
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In mathematical terms, the Hausdorff dimension generalizes the notion of the dimension of a real [[vector space]]. That is, the Hausdorff dimension of an ''n''-dimensional [[inner product space]] equals ''n''. This underlies the earlier statement that the Hausdorff dimension of a point is zero, of a line is one, etc., and that [[fractal|irregular sets]] can have noninteger Hausdorff dimensions. For instance, the [[Koch snowflake]] shown at right is constructed from an equilateral triangle; in each iteration, its component line segments are divided into 3 segments of unit length, the newly created middle segment is used as the base of a new [[equilateral]] triangle that points outward, and this base segment is then deleted to leave a final object from the iteration of unit length of 4.&amp;lt;ref&amp;gt;Larry Riddle, 2014, &amp;quot;Classic Iterated Function Systems: Koch Snowflake&amp;quot;, Agnes Scott College e-Academy (online), see [http://ecademy.agnesscott.edu/~lriddle/ifs/ksnow/ksnow.htm], accessed 5 March 2015.&amp;lt;/ref&amp;gt; That is, after the first iteration, each original line segment has been replaced with N=4, where each self-similar copy is 1/S = 1/3 as long as the original.&amp;lt;ref name=CampbellAnnenberg15/&amp;gt; Stated another way, we have taken an object with Euclidean dimension, D, and reduced its linear scale by 1/3 in each direction, so that its length increases to N=S&amp;lt;sup&amp;gt;D&amp;lt;/sup&amp;gt;.&amp;lt;ref name=ClaytonSCTPLS96&amp;gt;Keith Clayton, 1996, &amp;quot;Fractals and the Fractal Dimension,&amp;quot; ''Basic Concepts in Nonlinear Dynamics and Chaos'' (workshop), Society for Chaos Theory in Psychology and the Life Sciences annual meeting, June 28, 1996, Berkeley, California, see [http://www.vanderbilt.edu/AnS/psychology/cogsci/chaos/workshop/Workshop.html], accessed 5 March 2015.&amp;lt;/ref&amp;gt; This equation is easily solved for D, yielding the ratio of logarithms (or [[natural logarithm]]s) appearing in the figures, and giving—in the Koch and other fractal cases—non-integer dimensions for these objects.&lt;br /&gt;
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In mathematical terms, the Hausdorff dimension generalizes the notion of the dimension of a real vector space. That is, the Hausdorff dimension of an n-dimensional inner product space equals n. This underlies the earlier statement that the Hausdorff dimension of a point is zero, of a line is one, etc., and that irregular sets can have noninteger Hausdorff dimensions. For instance, the Koch snowflake shown at right is constructed from an equilateral triangle; in each iteration, its component line segments are divided into 3 segments of unit length, the newly created middle segment is used as the base of a new equilateral triangle that points outward, and this base segment is then deleted to leave a final object from the iteration of unit length of 4. That is, after the first iteration, each original line segment has been replaced with N=4, where each self-similar copy is 1/S = 1/3 as long as the original. This equation is easily solved for D, yielding the ratio of logarithms (or natural logarithms) appearing in the figures, and giving—in the Koch and other fractal cases—non-integer dimensions for these objects.&lt;br /&gt;
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用数学术语来说，豪斯多夫维数概括了实向量空间维数的概念。也就是说，n 维内积空间的豪斯多夫维数等于 n。 这就是早期假设的基础，一个点的豪斯多夫维数是零，一条线是一等等，不规则集可以有非整数的豪斯多夫维数。例如，右边所示的 Koch 雪花是由一个正三角形构成的; 在每次迭代中，它的组成线段被分成单位长度的3段，新创建的中间线段被用作一个指向外部的新正三角形的基础，然后人们删除这个基础线段用来保留单位长度4的迭代中的最终对象。也就是说，在第一次迭代之后，每个原始线段都被替换为 N=4，其中每个自相似拷贝的长度是原始线段的1/S = 1/3 。这个方程很容易求解为 D，产生出现在图形中的对数(或自然对数)的比率，并给出——在 Koch 和其他分形情况下——这些对象的非整数维数。&lt;br /&gt;
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The Hausdorff dimension is a successor to the simpler, but usually equivalent, box-counting or [[Minkowski–Bouligand dimension]].&lt;br /&gt;
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The Hausdorff dimension is a successor to the simpler, but usually equivalent, box-counting or Minkowski–Bouligand dimension.&lt;br /&gt;
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豪斯多夫维数是更简单但通常等价的'''&amp;lt;font color = '#ff8000'&amp;gt;计盒维数box-counting&amp;lt;/font&amp;gt;'''或'''&amp;lt;font color = '#ff8000'&amp;gt;闵可夫斯基维数Minkowski-Bouligand&amp;lt;/font&amp;gt;'''的继承者。&lt;br /&gt;
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==Intuition概念==&lt;br /&gt;
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{{refimprove section|date=March 2015}}&lt;br /&gt;
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The intuitive concept of dimension of a geometric object ''X'' is the number of independent parameters one needs to pick out a unique point inside. However, any point specified by two parameters can be instead specified by one, because the [[cardinality]] of the [[real plane]] is equal to the cardinality of the [[real line]] (this can be seen by an [[Cantor's diagonal argument|argument]] involving interweaving the digits of two numbers to yield a single number encoding the same information). The example of a [[space-filling curve]] shows that one can even map the real line to the real plane [[Surjective function|surjectively]] (taking one real number into a pair of real numbers in a way so that all pairs of numbers are covered) and ''continuously'', so that a one-dimensional object completely fills up a higher-dimensional object.&lt;br /&gt;
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The intuitive concept of dimension of a geometric object X is the number of independent parameters one needs to pick out a unique point inside. However, any point specified by two parameters can be instead specified by one, because the cardinality of the real plane is equal to the cardinality of the real line (this can be seen by an argument involving interweaving the digits of two numbers to yield a single number encoding the same information). The example of a space-filling curve shows that one can even map the real line to the real plane surjectively (taking one real number into a pair of real numbers in a way so that all pairs of numbers are covered) and continuously, so that a one-dimensional object completely fills up a higher-dimensional object.&lt;br /&gt;
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几何对象X的尺寸的直观概念是指需要多少个独立参数才能找到一个独特的点。但是，任何由两个参数指定的点都可以由一个参数指定，因为为实平面的基数等于实线的基数(这可以通过交织两个数字以产生一个编码相同信息的单个数字看到)。'''&amp;lt;font color = '#ff8000'&amp;gt;皮亚诺曲线&amp;lt;/font&amp;gt;'''的例子表明，可以将实线完美和连续地映射到实平面(把一个实数转换成一对实数，从而覆盖所有实数对)，由此一维对象完全填充了一个高维对象。&lt;br /&gt;
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Every space filling curve hits some points multiple times, and does not have a continuous inverse. It is impossible to map two dimensions onto one in a way that is continuous and continuously invertible. The topological dimension, also called [[Lebesgue covering dimension]], explains why. This dimension is ''n'' if, in every covering of ''X'' by small open balls, there is at least one point where ''n''&amp;amp;nbsp;+&amp;amp;nbsp;1 balls overlap. For example, when one covers a line with short open intervals, some points must be covered twice, giving dimension&amp;amp;nbsp;''n''&amp;amp;nbsp;=&amp;amp;nbsp;1.&lt;br /&gt;
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Every space filling curve hits some points multiple times, and does not have a continuous inverse. It is impossible to map two dimensions onto one in a way that is continuous and continuously invertible. The topological dimension, also called Lebesgue covering dimension, explains why. This dimension is n if, in every covering of X by small open balls, there is at least one point where n&amp;amp;nbsp;+&amp;amp;nbsp;1 balls overlap. For example, when one covers a line with short open intervals, some points must be covered twice, giving dimension&amp;amp;nbsp;n&amp;amp;nbsp;=&amp;amp;nbsp;1.&lt;br /&gt;
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每条空间填充曲线都会多次击中某些点，且不存在连续的逆。将二维以连续和连续可逆的方式映射到一维是不可能的。'''&amp;lt;font color = '#ff8000'&amp;gt;拓扑维度 topological dimension&amp;lt;/font&amp;gt;'''，也被称为Lebesgue覆盖维数，解释了为什么。如果在 x 的每个小开球覆盖中，至少有一个点 n + 1个球重叠，这个维度是 n。例如，当用短的开区间覆盖一条线时，某些点必须被覆盖两次，给出维数''n''&amp;amp;nbsp;=&amp;amp;nbsp;1。&lt;br /&gt;
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But topological dimension is a very crude measure of the local size of a space (size near a point). A curve that is almost space-filling can still have topological dimension one, even if it fills up most of the area of a region. A [[fractal]] has an integer topological dimension, but in terms of the amount of space it takes up, it behaves like a higher-dimensional space.&lt;br /&gt;
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But topological dimension is a very crude measure of the local size of a space (size near a point). A curve that is almost space-filling can still have topological dimension one, even if it fills up most of the area of a region. A fractal has an integer topological dimension, but in terms of the amount of space it takes up, it behaves like a higher-dimensional space.&lt;br /&gt;
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但是，拓扑维度是对空间局部尺寸(点附近的尺寸)的一个非常粗略的度量。一条几乎是空间填充的曲线仍然可以有一维拓扑，即使它填充了一个区域的大部分面积。分形具有整数的拓扑维数，但就其所占的空间量而言，它看起来像一个更高维的空间。&lt;br /&gt;
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The Hausdorff dimension measures the local size of a space taking into account the distance between points, the [[metric space|metric]]. Consider the number ''N''(''r'') of [[ball (mathematics)|balls]] of radius at most ''r'' required to cover ''X'' completely. When ''r'' is very small, ''N''(''r'') grows polynomially with 1/''r''. For a sufficiently well-behaved  ''X'', the Hausdorff dimension is the unique number ''d'' such that N(''r'') grows as 1/''r&amp;lt;sup&amp;gt;d&amp;lt;/sup&amp;gt;'' as ''r'' approaches zero. More precisely, this defines the [[Minkowski–Bouligand dimension|box-counting dimension]], which equals the Hausdorff dimension when the value ''d'' is a critical boundary between growth rates that are insufficient to cover the space, and growth rates that are overabundant.&lt;br /&gt;
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The Hausdorff dimension measures the local size of a space taking into account the distance between points, the metric. Consider the number N(r) of balls of radius at most r required to cover X completely. When r is very small, N(r) grows polynomially with 1/r. For a sufficiently well-behaved  X, the Hausdorff dimension is the unique number d such that N(r) grows as 1/r&amp;lt;sup&amp;gt;d&amp;lt;/sup&amp;gt; as r approaches zero. More precisely, this defines the box-counting dimension, which equals the Hausdorff dimension when the value d is a critical boundary between growth rates that are insufficient to cover the space, and growth rates that are overabundant.&lt;br /&gt;
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豪斯多夫维数测量一个空间的局部大小时，会考虑到点之间距离的度量。考虑半径最大为 r 的球数 ''N'' (r) ，需要完全覆盖 ''X''。当 r 很小时，n (r)以1/''r'' 增长多项式。对于一个表现足够好的 ''X''，豪斯多夫维数是唯一的数 d，这样当 r 趋近于零时， N(r)增长为1/r&amp;lt;sup&amp;gt;d&amp;lt;/sup&amp;gt; 。更确切地说，这定义了盒子计数维度，当值 d 是不足以覆盖空间的增长率和过度充裕的增长率之间的关键边界时，它等于豪斯多夫维数。&lt;br /&gt;
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For shapes that are smooth, or shapes with a small number of corners, the shapes of traditional geometry and science, the Hausdorff dimension is an integer agreeing with the topological dimension. But [[Benoit Mandelbrot]] observed that [[fractal]]s, sets with noninteger Hausdorff dimensions, are found everywhere in nature. He observed that the proper idealization of most rough shapes you see around you is not in terms of smooth idealized shapes, but in terms of fractal idealized shapes:&lt;br /&gt;
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For shapes that are smooth, or shapes with a small number of corners, the shapes of traditional geometry and science, the Hausdorff dimension is an integer agreeing with the topological dimension. But Benoit Mandelbrot observed that fractals, sets with noninteger Hausdorff dimensions, are found everywhere in nature. He observed that the proper idealization of most rough shapes you see around you is not in terms of smooth idealized shapes, but in terms of fractal idealized shapes:&lt;br /&gt;
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对于光滑的形状，或者有少量棱角的形状，传统几何和科学的形状，豪斯多夫维数是一个整数，与拓扑维度一致。但是伯努·曼德布洛特观察到分形---- 具有非整数豪斯多夫维数的集合---- 在自然界中随处可见。他观察到，我们周围大多数粗糙形状的理想化不是光滑的理想化形状，而是分形理想化形状:&lt;br /&gt;
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&amp;lt;blockquote&amp;gt;Clouds are not spheres, mountains are not cones, coastlines are not circles, and bark is not smooth, nor does lightning travel in a straight line.&amp;lt;ref name=&amp;quot;mandelbrot&amp;quot;&amp;gt;{{cite book   | last = Mandelbrot   | first = Benoît   | authorlink = Benoit Mandelbrot   | title = The Fractal Geometry of Nature   | publisher = W. H. Freeman   | series = Lecture notes in mathematics 1358   | year = 1982   | doi =    | isbn = 0-7167-1186-9   | url-access = registration   | url = https://archive.org/details/fractalgeometryo00beno   }}&amp;lt;/ref&amp;gt;&amp;lt;/blockquote&amp;gt;&lt;br /&gt;
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&amp;lt;blockquote&amp;gt;Clouds are not spheres, mountains are not cones, coastlines are not circles, and bark is not smooth, nor does lightning travel in a straight line.&amp;lt;/blockquote&amp;gt;&lt;br /&gt;
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&amp;lt;blockquote&amp;gt;云不是球体，山不是锥体，海岸线不是圆圈，树皮不平滑，闪电也不是直线运动。 &amp;lt;/blockquote&amp;gt;&lt;br /&gt;
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For fractals that occur in nature, the Hausdorff and [[Minkowski–Bouligand dimension|box-counting dimension]] coincide. The [[packing dimension]] is yet another similar notion which gives the same value for many shapes, but there are well documented exceptions where all these dimensions differ.&lt;br /&gt;
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For fractals that occur in nature, the Hausdorff and box-counting dimension coincide. The packing dimension is yet another similar notion which gives the same value for many shapes, but there are well documented exceptions where all these dimensions differ.&lt;br /&gt;
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对于自然界中出现的分形，豪斯多夫维数和盒计数维数是一致的。封装尺寸是另一个类似的概念，它给出了许多形状相同的值，但是在所有这些尺寸不同的情况，都做了很好的说明。&lt;br /&gt;
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==Formal definitions形式化定义==&lt;br /&gt;
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{{unreferenced section|date=March 2015}}&lt;br /&gt;
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===Hausdorff content豪斯多夫集===&lt;br /&gt;
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Let ''X'' be a [[metric space]]. If ''S'' ⊂ ''X'' and ''d'' ∈ [0, ∞), the ''d''-dimensional '''unlimited Hausdorff content''' of ''S'' is defined by&lt;br /&gt;
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Let X be a metric space. If S ⊂ X and d ∈ [0, ∞), the d-dimensional unlimited Hausdorff content of S is defined by&lt;br /&gt;
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设 ''X''是度量空间。若''S'' ⊂ ''X'' 和 ''d'' ∈ [0, ∞) ，则 ''S'' 的''d''维无限 豪斯多夫集定义为&lt;br /&gt;
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:&amp;lt;math&amp;gt;C_H^d(S):=\inf\Bigl\{\sum_i r_i^d:\text{ there is a cover of } S\text{ by balls with radii }r_i&amp;gt;0\Bigr\}.&amp;lt;/math&amp;gt;&lt;br /&gt;
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&amp;lt;math&amp;gt;C_H^d(S):=\inf\Bigl\{\sum_i r_i^d:\text{ there is a cover of } S\text{ by balls with radii }r_i&amp;gt;0\Bigr\}.&amp;lt;/math&amp;gt;&lt;br /&gt;
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&amp;lt;math&amp;gt;C_H^d(S):=\inf\Bigl\{\sum_i r_i^d:\text{ there is a cover of } S\text{ by balls with radii }r_i&amp;gt;0\Bigr\}.&amp;lt;/math&amp;gt;&lt;br /&gt;
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In other words, &amp;lt;math&amp;gt;C_H^d(S)&amp;lt;/math&amp;gt; is the [[infimum]] of the set of numbers &amp;lt;math&amp;gt;\delta \geq 0&amp;lt;/math&amp;gt; such that there is some (indexed) collection of [[ball (mathematics)|ball]]s &amp;lt;math&amp;gt;\{B(x_i,r_i):i\in I\}&amp;lt;/math&amp;gt; covering ''S'' with ''r&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;''&amp;amp;nbsp;&amp;gt;&amp;amp;nbsp;0 for each ''i''&amp;amp;nbsp;∈&amp;amp;nbsp;''I'' that satisfies &amp;lt;math&amp;gt;\sum_{i\in I} r_i^d&amp;lt;\delta &amp;lt;/math&amp;gt;. (Here, we use the standard convention that [[infimum|inf&amp;amp;nbsp;Ø&amp;amp;nbsp;=&amp;amp;nbsp;∞]].)&lt;br /&gt;
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In other words, &amp;lt;math&amp;gt;C_H^d(S)&amp;lt;/math&amp;gt; is the infimum of the set of numbers &amp;lt;math&amp;gt;\delta \geq 0&amp;lt;/math&amp;gt; such that there is some (indexed) collection of balls &amp;lt;math&amp;gt;\{B(x_i,r_i):i\in I\}&amp;lt;/math&amp;gt; covering S with r&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;&amp;amp;nbsp;&amp;gt;&amp;amp;nbsp;0 for each i&amp;amp;nbsp;∈&amp;amp;nbsp;I that satisfies &amp;lt;math&amp;gt;\sum_{i\in I} r_i^d&amp;lt;\delta &amp;lt;/math&amp;gt;. (Here, we use the standard convention that inf&amp;amp;nbsp;Ø&amp;amp;nbsp;=&amp;amp;nbsp;∞.)&lt;br /&gt;
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换句话说，&amp;lt;math&amp;gt;C_H^d(S)&amp;lt;/math&amp;gt; 是数字集合&amp;lt;math&amp;gt;\delta \geq 0&amp;lt;/math&amp;gt;的下确界，使得在 ''i''&amp;amp;nbsp;∈&amp;amp;nbsp中存在一些球集合 &amp;lt;math&amp;gt;\{B(x_i,r_i):i\in I\}&amp;lt;/math&amp;gt;  i 包含 s，对于每个 ''r&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;''&amp;amp;nbsp;&amp;gt;&amp;amp;nbsp;0 满足 i 中的和&amp;lt;math&amp;gt;\sum_{i\in I} r_i^d&amp;lt;\delta &amp;lt;/math&amp;gt; (在这里，我们使用inf&amp;amp;nbsp;Ø&amp;amp;nbsp;=&amp;amp;nbsp;∞ )的标准约定。&lt;br /&gt;
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===Hausdorff measurement豪斯多夫分形测量===&lt;br /&gt;
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The Hausdorff outer measure is different from the unbounded Hausdorf content in that rather than considering all possible coverings of ''S'', we see what happens when the sizes of the balls go to zero. This is  for &amp;lt;math&amp;gt;d \geq 0 &amp;lt;/math&amp;gt;, we define the ''d''-dimensional Hausdorff outer measure of ''S'' as&lt;br /&gt;
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The Hausdorff outer measure is different from the unbounded Hausdorf content in that rather than considering all possible coverings of S, we see what happens when the sizes of the balls go to zero. This is  for &amp;lt;math&amp;gt;d \geq 0 &amp;lt;/math&amp;gt;, we define the d-dimensional Hausdorff outer measure of S as&lt;br /&gt;
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豪斯多夫外测度不同于无界的豪斯多夫，因为我们不考虑 s 的所有可能，我们看到当球的大小为零时会发生什么。这是为了数学  &amp;lt;math&amp;gt;d \geq 0 &amp;lt;/math&amp;gt;，我们定义了  ''S''的 ''d''维豪斯多夫Hausdorff 外测度为&lt;br /&gt;
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:&amp;lt;math&amp;gt; \mathcal{H}^d(S):=\lim_{r \to 0} \inf\Bigl\{\sum_i r_i^d:\text{ there is a cover of } S\text{ by balls with radii } 0 &amp;lt; r_i &amp;lt; r\Bigr\}.&amp;lt;/math&amp;gt;&lt;br /&gt;
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&amp;lt;math&amp;gt; \mathcal{H}^d(S):=\lim_{r \to 0} \inf\Bigl\{\sum_i r_i^d:\text{ there is a cover of } S\text{ by balls with radii } 0 &amp;lt; r_i &amp;lt; r\Bigr\}.&amp;lt;/math&amp;gt;&lt;br /&gt;
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&amp;lt;math&amp;gt; \mathcal{H}^d(S):=\lim_{r \to 0} \inf\Bigl\{\sum_i r_i^d:\text{有一个面} S\text{ 球 } 0 &amp;lt; r_i &amp;lt; r\Bigr\}.&amp;lt;/math&amp;gt;&lt;br /&gt;
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===Hausdorff dimension豪斯多夫维数===&lt;br /&gt;
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The '''Hausdorff dimension''' of ''X'' is defined by&lt;br /&gt;
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The Hausdorff dimension of X is defined by&lt;br /&gt;
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X 的豪斯多夫维数定义为&lt;br /&gt;
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:&amp;lt;math&amp;gt;\dim_{\operatorname{H}}(X):=\inf\{d\ge 0: \mathcal{H}^d(X)=0\}.&amp;lt;/math&amp;gt;&lt;br /&gt;
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&amp;lt;math&amp;gt;\dim_{\operatorname{H}}(X):=\inf\{d\ge 0: \mathcal{H}^d(X)=0\}.&amp;lt;/math&amp;gt;&lt;br /&gt;
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Equivalently, dim&amp;lt;sub&amp;gt;H&amp;lt;/sub&amp;gt;(''X'') may be defined as the [[infimum]] of the set of ''d'' ∈ [0, ∞) such that the ''d''-dimensional [[Hausdorff measure]] of ''X'' is zero. This is the same as the supremum of the set of ''d''&amp;amp;nbsp;∈&amp;amp;nbsp;[0,&amp;amp;nbsp;∞) such that the ''d''-dimensional Hausdorff measure of ''X'' is infinite (except that when this latter set of numbers ''d'' is empty the Hausdorff dimension is zero).&lt;br /&gt;
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Equivalently, dim&amp;lt;sub&amp;gt;H&amp;lt;/sub&amp;gt;(X) may be defined as the infimum of the set of d ∈ [0, ∞) such that the d-dimensional Hausdorff measure of X is zero. This is the same as the supremum of the set of d&amp;amp;nbsp;∈&amp;amp;nbsp;[0,&amp;amp;nbsp;∞) such that the d-dimensional Hausdorff measure of X is infinite (except that when this latter set of numbers d is empty the Hausdorff dimension is zero).&lt;br /&gt;
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等价地，dim &amp;lt;sub&amp;gt;H&amp;lt;/sub&amp;gt;(''X'')可定义为 ''d'' ∈ [0, ∞) 集的下确界，使得''X'' 的''d''-维 [[豪斯多夫测度]] 为零。这与 ''d''&amp;amp;nbsp;∈&amp;amp;nbsp;[0,&amp;amp;nbsp;∞)的集合的上确界相同，因此''X''的 d 维豪斯多夫测度是无限的(除非后一个集合 ''d'' 是空的，豪斯多夫维数为零)。&lt;br /&gt;
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==Examples实例==&lt;br /&gt;
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[[Image:Sierpinski deep.svg|thumb|250px|Dimension of a further [[fractal]] example. The [[Sierpinski triangle]], an object with Hausdorff dimension of log(3)/log(2)≈1.58.&amp;lt;ref name=ClaytonSCTPLS96/&amp;gt;]]&lt;br /&gt;
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Dimension of a further [[fractal example. The Sierpinski triangle, an object with Hausdorff dimension of log(3)/log(2)≈1.58.]]&lt;br /&gt;
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[[Image:谢尔宾斯基三角形 deep.svg|thumb|250px|进一步的[[分形维数]]的例子，进一步的分形维数的例子是谢尔宾斯基三角形，它是一个豪斯多夫维数为log(3)/log(2)≈1.58.&amp;lt;ref name=ClaytonSCTPLS96/&amp;gt;的物体]]&lt;br /&gt;
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* [[Countable set]]s have Hausdorff dimension 0.&amp;lt;ref name=&amp;quot;schleicher&amp;quot;&amp;gt;{{cite journal |last1=Schleicher |first1=Dierk |title=Hausdorff Dimension, Its Properties, and Its Surprises |journal=The American Mathematical Monthly |date=June 2007 |volume=114 |issue=6 |pages=509–528 |doi=10.1080/00029890.2007.11920440 |language=en |issn=0002-9890|arxiv=math/0505099 }}&amp;lt;/ref&amp;gt;&lt;br /&gt;
*[[可数集]]拥有豪斯多夫维数0.&amp;lt;ref name=&amp;quot;schleicher&amp;quot;&amp;gt;{{cite journal |last1=Schleicher |first1=Dierk |title=豪斯多夫维数, Its Properties, and Its Surprises |journal=The American Mathematical Monthly美国数学期刊 |date=June 2007 |volume=114 |issue=6 |pages=509–528 |doi=10.1080/00029890.2007.11920440 |language=en |issn=0002-9890|arxiv=math/0505099 }}&amp;lt;/ref&amp;gt;&lt;br /&gt;
* The [[Euclidean space]] ℝ&amp;lt;sup&amp;gt;''n''&amp;lt;/sup&amp;gt; has Hausdorff dimension ''n'', and the circle '''S'''&amp;lt;sup&amp;gt;1&amp;lt;/sup&amp;gt; has Hausdorff dimension 1.&amp;lt;ref name=&amp;quot;schleicher&amp;quot; /&amp;gt;&lt;br /&gt;
*[[教育空间]] ℝ&amp;lt;sup&amp;gt;''n''&amp;lt;/sup&amp;gt; 有豪斯多夫维数 ''n''，循环'''S'''&amp;lt;sup&amp;gt;1&amp;lt;/sup&amp;gt; 拥有豪斯多夫维数1.&amp;lt;ref name=&amp;quot;schleicher&amp;quot; /&amp;gt;&lt;br /&gt;
* [[Fractal]]s often are spaces whose Hausdorff dimension strictly exceeds the [[topological dimension]].&amp;lt;ref name=&amp;quot;mandelbrot&amp;quot; /&amp;gt; For example, the [[Cantor set]], a zero-dimensional topological space, is a union of two copies of itself, each copy shrunk by a factor 1/3; hence, it can be shown that its Hausdorff dimension is ln(2)/ln(3)&amp;amp;nbsp;≈&amp;amp;nbsp;0.63.&amp;lt;ref&amp;gt;{{cite book | last=Falconer | first = Kenneth |title=Fractal Geometry: Mathematical Foundations and Applications | publisher=[[John Wiley and Sons]] | edition=2nd | year=2003}}&amp;lt;/ref&amp;gt; The [[Sierpinski triangle]] is a union of three copies of itself, each copy shrunk by a factor of&amp;amp;nbsp;1/2; this yields a Hausdorff dimension of ln(3)/ln(2)&amp;amp;nbsp;≈&amp;amp;nbsp;1.58.&amp;lt;ref name=CampbellAnnenberg15/&amp;gt; These Hausdorff dimensions are related to the &amp;quot;critical exponent&amp;quot; of the [[Master theorem (analysis of algorithms)|Master theorem]] for solving [[Recurrence relation|recurrence relations]] in the [[analysis of algorithms]].&lt;br /&gt;
*[[分形]]一般是那些豪斯多夫维数直接超过其拓扑维数的空间。例如[[康托尔集]]是一个o维拓扑空间，由两个自己复制而成，每一个复制品都是原来的三分之一，因此它的豪斯多夫维数是 ln(2)/ln(3)&amp;amp;nbsp;≈&amp;amp;nbsp;0.63。&amp;lt;ref&amp;gt;{{cite book | last=Falconer | first = Kenneth |title=Fractal Geometry: Mathematical Foundations and Applications | publisher=[[John Wiley and Sons]] | edition=2nd | year=2003}}&amp;lt;/ref&amp;gt;一个[[谢尔宾斯基三角]]是他自身三个复制的组合。每一个是原来的&amp;amp;nbsp;1/2，它的豪斯多夫维数ln(3)/ln(2)&amp;amp;nbsp;≈&amp;amp;nbsp;1.58。&amp;lt;ref name=CampbellAnnenberg15/&amp;gt;在递归算法中解决递归关系时，这些豪斯多夫维数与[[算法分析主定理]]的临界指标相联系。&lt;br /&gt;
* [[Space-filling curve]]s like the [[Peano curve]] have the same Hausdorff dimension as the space they fill.&lt;br /&gt;
*[[空间填充曲线]]拥有和他们填充空间同样的豪斯多夫维数，如[[皮亚诺曲线]]。&lt;br /&gt;
* The trajectory of [[Brownian motion]] in dimension 2 and above is conjectured to be Hausdorff dimension 2.&amp;lt;ref&amp;gt;{{cite book | last=Morters | first=Peres | title= Brownian Motion | publisher=[[Cambridge University Press]] | year=2010 }}&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
[[image:Great Britain Hausdorff.svg|thumb|250px|Estimating the Hausdorff dimension of the [[How Long Is the Coast of Britain? Statistical Self-Similarity and Fractional Dimension|coast of Great Britain]]]]&lt;br /&gt;
&lt;br /&gt;
coast of Great Britain]]&lt;br /&gt;
&lt;br /&gt;
[[大不列颠海岸&lt;br /&gt;
&lt;br /&gt;
* 刘易斯·弗赖伊·理查森[[Lewis Fry Richardson]] has performed detailed experiments to measure the approximate Hausdorff dimension for various coastlines. His results have varied from 1.02 for the coastline of [[South Africa]] to 1.25 for the west coast of [[Great Britain]].&amp;lt;ref name=&amp;quot;mandelbrot&amp;quot; /&amp;gt;&lt;br /&gt;
*刘易斯·弗赖伊·理查森（Lewis Fry Richardson）已经通过豪斯多夫维数去测量了很多海岸线。它的结果涵盖从1.02的南非海岸线到1.25的大英帝国西海岸模型。]]&lt;br /&gt;
&lt;br /&gt;
==Properties of Hausdorff dimension豪斯多夫维数特性==&lt;br /&gt;
&lt;br /&gt;
{{refimprove section|date=March 2015}}&lt;br /&gt;
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&lt;br /&gt;
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=== Hausdorff dimension and inductive dimension 豪斯多夫维数和归纳维数===&lt;br /&gt;
&lt;br /&gt;
Let ''X'' be an arbitrary [[Separable space|separable]] metric space. There is a [[topology|topological]] notion of [[inductive dimension]] for ''X'' which is defined recursively. It is always an integer (or +∞) and is denoted dim&amp;lt;sub&amp;gt;ind&amp;lt;/sub&amp;gt;(''X'').&lt;br /&gt;
&lt;br /&gt;
Let X be an arbitrary separable metric space. There is a topological notion of inductive dimension for X which is defined recursively. It is always an integer (or +∞) and is denoted dim&amp;lt;sub&amp;gt;ind&amp;lt;/sub&amp;gt;(X).&lt;br /&gt;
&lt;br /&gt;
设''X'' 是[[任意可分度量空间]]。对于''X'' 有一个递归定义的归纳维数拓扑概念。它总是一个整数(或 + ∞) ，记为dim&amp;lt;sub&amp;gt;ind&amp;lt;/sub&amp;gt;(''X'')。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
'''Theorem'''. Suppose ''X'' is non-empty. Then &lt;br /&gt;
&lt;br /&gt;
Theorem. Suppose X is non-empty. Then &lt;br /&gt;
&lt;br /&gt;
'''定理'''：假设''X'' 是非空的, 那么&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt; \dim_{\mathrm{Haus}}(X) \geq \dim_{\operatorname{ind}}(X). &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \dim_{\mathrm{Haus}}(X) \geq \dim_{\operatorname{ind}}(X). &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Moreover,&lt;br /&gt;
&lt;br /&gt;
Moreover,&lt;br /&gt;
&lt;br /&gt;
此外,&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \inf_Y \dim_{\operatorname{Haus}}(Y) =\dim_{\operatorname{ind}}(X), &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \inf_Y \dim_{\operatorname{Haus}}(Y) =\dim_{\operatorname{ind}}(X), &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
where ''Y'' ranges over metric spaces [[homeomorphic]] to ''X''. In other words, ''X'' and ''Y'' have the same underlying set of points and the metric ''d''&amp;lt;sub&amp;gt;''Y''&amp;lt;/sub&amp;gt; of ''Y'' is topologically equivalent to ''d''&amp;lt;sub&amp;gt;''X''&amp;lt;/sub&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
where Y ranges over metric spaces homeomorphic to X. In other words, X and Y have the same underlying set of points and the metric d&amp;lt;sub&amp;gt;Y&amp;lt;/sub&amp;gt; of Y is topologically equivalent to d&amp;lt;sub&amp;gt;X&amp;lt;/sub&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
其中''Y''是度量空间同胚到 ''X''的范围。换句话说， ''X''和 ''Y''具有相同的基本点集，''Y''的度量''d''&amp;lt;sub&amp;gt;''Y''&amp;lt;/sub&amp;gt; 拓扑等价于''d''&amp;lt;sub&amp;gt;''X''&amp;lt;/sub&amp;gt;。&lt;br /&gt;
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&lt;br /&gt;
&lt;br /&gt;
These results were originally established by [[Edward Szpilrajn]] (1907–1976), e.g., see Hurewicz and Wallman, Chapter VII.{{full citation needed|date=March 2015}}&lt;br /&gt;
&lt;br /&gt;
These results were originally established by Edward Szpilrajn (1907–1976), e.g., see Hurewicz and Wallman, Chapter VII.&lt;br /&gt;
&lt;br /&gt;
这些结果最初是由 [[Edward Szpilrajn]] (1907–1976)建立的,  参见 Hurewicz and Wallman, Chapter VII.{{full citation needed|date=March 2015}}第七章。&lt;br /&gt;
&lt;br /&gt;
=== Hausdorff dimension and Minkowski dimension 豪斯多夫维数和闵可夫斯基维度===&lt;br /&gt;
&lt;br /&gt;
The [[Minkowski dimension]] is similar to, and at least as large as, the Hausdorff dimension, and they are equal in many situations. However, the set of [[rational number|rational]] points in [0, 1] has Hausdorff dimension zero and Minkowski dimension one. There are also compact sets for which the Minkowski dimension is strictly larger than the Hausdorff dimension.&lt;br /&gt;
&lt;br /&gt;
The Minkowski dimension is similar to, and at least as large as, the Hausdorff dimension, and they are equal in many situations. However, the set of rational points in [0, 1] has Hausdorff dimension zero and Minkowski dimension one. There are also compact sets for which the Minkowski dimension is strictly larger than the Hausdorff dimension.&lt;br /&gt;
&lt;br /&gt;
[[闵可夫斯基维数]]与豪斯多夫维数相似，至少和它一样大，而且在许多情况下是相等的。然而，[0,1]中有理点集的豪斯多夫维数为0，闵可夫斯基维数为1。还有一些紧集的闵可夫斯基维数严格大于豪斯多夫维数。&lt;br /&gt;
&lt;br /&gt;
=== Hausdorff dimensions and Frostman measures 豪斯多夫维度和弗洛斯曼测度===&lt;br /&gt;
&lt;br /&gt;
If there is a [[measure (mathematics)|measure]] μ defined on [[Borel measure|Borel]] subsets of a metric space ''X'' such that ''μ''(''X'') &amp;gt; 0 and ''μ''(''B''(''x'', ''r'')) ≤ ''r&amp;lt;sup&amp;gt;s&amp;lt;/sup&amp;gt;'' holds for some constant ''s'' &amp;gt; 0 and for every ball ''B''(''x'', ''r'') in ''X'', then dim&amp;lt;sub&amp;gt;Haus&amp;lt;/sub&amp;gt;(''X'') ≥ ''s''. A partial converse is provided by [[Frostman's lemma]].{{citation needed|date=March 2015}}&amp;lt;ref&amp;gt;This Wikipedia article also discusses further useful characterizations of the Hausdorff dimension.{{clarify|date=March 2015}}&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
If there is a measure μ defined on Borel subsets of a metric space X such that μ(X) &amp;gt; 0 and μ(B(x, r)) ≤ r&amp;lt;sup&amp;gt;s&amp;lt;/sup&amp;gt; holds for some constant s &amp;gt; 0 and for every ball B(x, r) in X, then dim&amp;lt;sub&amp;gt;Haus&amp;lt;/sub&amp;gt;(X) ≥ s. A partial converse is provided by Frostman's lemma.&lt;br /&gt;
&lt;br /&gt;
如果在度量空间 ''X'' 的 Borel 子集上定义一个测度 μ，使得''μ''(''X'') &amp;gt; 0 和''μ''(''B''(''x'', ''r'')) ≤ ''r&amp;lt;sup&amp;gt;s&amp;lt;/sup&amp;gt;''，对于某个常数 ''s'' &amp;gt; 0  和 ''X'' 中的每个球 ''B''(''x'', ''r'') 成立，则 dim&amp;lt;sub&amp;gt;Haus&amp;lt;/sub&amp;gt;(''X'') ≥ ''s'' 。 部分逆向转换由弗洛斯曼引理定义。&lt;br /&gt;
&lt;br /&gt;
=== Behaviour under unions and products ===&lt;br /&gt;
&lt;br /&gt;
If &amp;lt;math&amp;gt;X=\bigcup_{i\in I}X_i&amp;lt;/math&amp;gt; is a finite or countable union, then&lt;br /&gt;
&lt;br /&gt;
If &amp;lt;math&amp;gt;X=\bigcup_{i\in I}X_i&amp;lt;/math&amp;gt; is a finite or countable union, then&lt;br /&gt;
&lt;br /&gt;
如果 &amp;lt;math&amp;gt;X=\bigcup_{i\in I}X_i&amp;lt;/math&amp;gt; 是一个有限或可数的联合，则&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \dim_{\operatorname{Haus}}(X) =\sup_{i\in I} \dim_{\operatorname{Haus}}(X_i).&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \dim_{\operatorname{Haus}}(X) =\sup_{i\in I} \dim_{\operatorname{Haus}}(X_i).&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
This can be verified directly from the definition.&lt;br /&gt;
&lt;br /&gt;
This can be verified directly from the definition.&lt;br /&gt;
&lt;br /&gt;
这可以直接从定义得到验证。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
If ''X'' and ''Y'' are non-empty metric spaces, then the Hausdorff dimension of their product satisfies&amp;lt;ref&amp;gt;{{cite journal |author=Marstrand, J. M. |title=The dimension of Cartesian product sets |journal=Proc. Cambridge Philos. Soc. |volume=50 |issue=3 |pages=198–202 |year=1954 |doi=10.1017/S0305004100029236 |bibcode = 1954PCPS...50..198M }}&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
If X and Y are non-empty metric spaces, then the Hausdorff dimension of their product satisfies&lt;br /&gt;
&lt;br /&gt;
如果 ''X'' 和''Y''是非空度量空间，那么它们乘积的豪斯多夫维数满足&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt; \dim_{\operatorname{Haus}}(X\times Y)\ge \dim_{\operatorname{Haus}}(X)+ \dim_{\operatorname{Haus}}(Y).&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \dim_{\operatorname{Haus}}(X\times Y)\ge \dim_{\operatorname{Haus}}(X)+ \dim_{\operatorname{Haus}}(Y).&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
This inequality can be strict. It is possible to find two sets of dimension 0 whose product has dimension 1.&amp;lt;ref&amp;gt;{{cite book  | last = Falconer  | first = Kenneth J.  | title = Fractal geometry. Mathematical foundations and applications  | publisher = John Wiley &amp;amp; Sons, Inc., Hoboken, New Jersey  | year = 2003  | doi =   | isbn = }}&amp;lt;/ref&amp;gt; In the opposite direction, it is known that when ''X'' and ''Y'' are Borel subsets of '''R'''&amp;lt;sup&amp;gt;''n''&amp;lt;/sup&amp;gt;, the Hausdorff dimension of ''X'' × ''Y'' is bounded from above by the Hausdorff dimension of ''X'' plus the [[packing dimension|upper packing dimension]] of ''Y''. These facts are discussed in Mattila (1995).&lt;br /&gt;
&lt;br /&gt;
This inequality can be strict. It is possible to find two sets of dimension 0 whose product has dimension 1. In the opposite direction, it is known that when X and Y are Borel subsets of R&amp;lt;sup&amp;gt;n&amp;lt;/sup&amp;gt;, the Hausdorff dimension of X × Y is bounded from above by the Hausdorff dimension of X plus the upper packing dimension of Y. These facts are discussed in Mattila (1995).&lt;br /&gt;
&lt;br /&gt;
这种不平等可以是严格的。有可能找到两个维数为0的集合，其乘积的维数为1。相反，我们知道当''X''和''Y''是 '''R'''&amp;lt;sup&amp;gt;''n''&amp;lt;/sup&amp;gt;的 Borel 子集时， ''X'' × ''Y''的豪斯多夫维数从上面以 ''X''的豪斯多夫维数加上 ''Y''的上填充维数为界。Mattila (1995)曾就这些情况进行了讨论。&lt;br /&gt;
&lt;br /&gt;
==Self-similar sets自相似集合==&lt;br /&gt;
&lt;br /&gt;
{{refimprove section|date=March 2015}}&lt;br /&gt;
&lt;br /&gt;
Many sets defined by a self-similarity condition have dimensions which can be determined explicitly. Roughly, a set ''E'' is self-similar if it is the fixed point of a set-valued transformation ψ, that is ψ(''E'') = ''E'', although the exact definition is given below.&lt;br /&gt;
&lt;br /&gt;
Many sets defined by a self-similarity condition have dimensions which can be determined explicitly. Roughly, a set E is self-similar if it is the fixed point of a set-valued transformation ψ, that is ψ(E) = E, although the exact definition is given below.&lt;br /&gt;
&lt;br /&gt;
许多由自相似条件定义的集合具有可以显式确定的维数。粗略地说，如果集合''E''是集值ψ变换的不动点，即ψ(''E'') = ''E''， 则它是自相似的，尽管下面给出了确切的定义。&lt;br /&gt;
&lt;br /&gt;
&amp;lt;blockquote&amp;gt;'''Theorem'''. Suppose&lt;br /&gt;
&lt;br /&gt;
&amp;lt;blockquote&amp;gt;Theorem. Suppose&lt;br /&gt;
&lt;br /&gt;
&amp;lt;blockquote&amp;gt;'''定理'''：假设&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt; \psi_i: \mathbf{R}^n \rightarrow \mathbf{R}^n, \quad i=1, \ldots , m &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \psi_i: \mathbf{R}^n \rightarrow \mathbf{R}^n, \quad i=1, \ldots , m &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
are [[Contraction mapping|contractive]] mappings on '''R'''&amp;lt;sup&amp;gt;''n''&amp;lt;/sup&amp;gt; with contraction constant ''r&amp;lt;sub&amp;gt;j&amp;lt;/sub&amp;gt;'' &amp;lt; 1. Then there is a unique ''non-empty'' compact set ''A'' such that&lt;br /&gt;
&lt;br /&gt;
are contractive mappings on R&amp;lt;sup&amp;gt;n&amp;lt;/sup&amp;gt; with contraction constant r&amp;lt;sub&amp;gt;j&amp;lt;/sub&amp;gt; &amp;lt; 1. Then there is a unique non-empty compact set A such that&lt;br /&gt;
&lt;br /&gt;
是'''R'''&amp;lt;sup&amp;gt;''n''&amp;lt;/sup&amp;gt;上的压缩常数''r&amp;lt;sub&amp;gt;j&amp;lt;/sub&amp;gt;'&amp;lt; 1的压缩映射。然后有一个唯一的非空紧集A &lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt; A = \bigcup_{i=1}^m \psi_i (A). &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; A = \bigcup_{i=1}^m \psi_i (A). &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&amp;lt;/blockquote&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;/blockquote&amp;gt;&lt;br /&gt;
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&lt;br /&gt;
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&lt;br /&gt;
The theorem follows from [[Stefan Banach]]'s [[Contractive mapping theorem|contractive mapping fixed point theorem]] applied to the complete metric space of non-empty compact subsets of '''R'''&amp;lt;sup&amp;gt;''n''&amp;lt;/sup&amp;gt; with the [[Hausdorff distance]].&amp;lt;ref&amp;gt;{{cite book |author=Falconer, K. J. |title=The Geometry of Fractal Sets |publisher=Cambridge University Press |location=Cambridge, UK |year=1985 |isbn=0-521-25694-1 |chapter=Theorem 8.3}}&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
The theorem follows from Stefan Banach's contractive mapping fixed point theorem applied to the complete metric space of non-empty compact subsets of R&amp;lt;sup&amp;gt;n&amp;lt;/sup&amp;gt; with the Hausdorff distance.&lt;br /&gt;
&lt;br /&gt;
这个定理来源于 Stefan Banach 的压缩映射不动点定理，该定理应用于 具有豪斯多夫距离的'''R'''&amp;lt;sup&amp;gt;''n''&amp;lt;/sup&amp;gt; 的非空紧子集的完整度量空间。&lt;br /&gt;
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&lt;br /&gt;
===The open set condition开集条件===&lt;br /&gt;
&lt;br /&gt;
To determine the dimension of the self-similar set ''A'' (in certain cases), we need a technical condition called the ''open set condition'' (OSC) on the sequence of contractions ψ&amp;lt;sub&amp;gt;''i''&amp;lt;/sub&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
To determine the dimension of the self-similar set A (in certain cases), we need a technical condition called the open set condition (OSC) on the sequence of contractions ψ&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
为了确定自相似集''A'' 的维数(在某些情况下) ，我们需要一个关于收缩序列的称为''开集条件''(OSC)的技术条件ψ&amp;lt;sub&amp;gt;''i''&amp;lt;/sub&amp;gt;。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
There is a relatively compact open set ''V'' such that&lt;br /&gt;
&lt;br /&gt;
There is a relatively compact open set V such that&lt;br /&gt;
&lt;br /&gt;
有一个相对紧的开集''V''&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt; \bigcup_{i=1}^m\psi_i (V) \subseteq V, &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \bigcup_{i=1}^m\psi_i (V) \subseteq V, &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
where the sets in union on the left are pairwise [[disjoint sets|disjoint]].&lt;br /&gt;
&lt;br /&gt;
where the sets in union on the left are pairwise disjoint.&lt;br /&gt;
&lt;br /&gt;
左边并集的集合成对不相交。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The open set condition is a separation condition that ensures the images ψ&amp;lt;sub&amp;gt;''i''&amp;lt;/sub&amp;gt;(''V'') do not overlap &amp;quot;too much&amp;quot;.&lt;br /&gt;
&lt;br /&gt;
The open set condition is a separation condition that ensures the images ψ&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;(V) do not overlap &amp;quot;too much&amp;quot;.&lt;br /&gt;
&lt;br /&gt;
开集条件是保证图像ψ&amp;lt;sub&amp;gt;''i''&amp;lt;/sub&amp;gt;(''V'') 不重叠“太多”的分离条件。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
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'''Theorem'''. Suppose the open set condition holds and each ψ&amp;lt;sub&amp;gt;''i''&amp;lt;/sub&amp;gt; is a similitude, that is a composition of an [[isometry]] and a [[dilation (metric space)|dilation]] around some point. Then the unique fixed point of ψ is a set whose Hausdorff dimension is ''s'' where ''s'' is the unique solution of&amp;lt;ref&amp;gt;{{cite journal | last=Hutchinson | first=John E. | title=Fractals and self similarity | journal=Indiana Univ. Math. J. | volume=30 | year=1981 | pages=713–747 | doi=10.1512/iumj.1981.30.30055 | issue=5 | doi-access=free }}&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
Theorem. Suppose the open set condition holds and each ψ&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt; is a similitude, that is a composition of an isometry and a dilation around some point. Then the unique fixed point of ψ is a set whose Hausdorff dimension is s where s is the unique solution of&lt;br /&gt;
&lt;br /&gt;
'''定理'''假设开集条件成立，并且每个ψ&amp;lt;sub&amp;gt;''i''&amp;lt;/sub&amp;gt; 是一个相似度，即等距和某个点周围的膨胀的组合。。那么唯一的不动点是Hausdorff维数为 ''s'' 的集合，其中  ''s'' 是 ''s'' &amp;lt;ref&amp;gt;{{cite journal | last=Hutchinson | first=John E. | title=Fractals and self similarity | journal=Indiana Univ. Math. J. | volume=30 | year=1981 | pages=713–747 | doi=10.1512/iumj.1981.30.30055 | issue=5 | doi-access=free }}&amp;lt;/ref&amp;gt;的唯一解&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt; \sum_{i=1}^m r_i^s = 1. &amp;lt;/math&amp;gt;&lt;br /&gt;
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&amp;lt;math&amp;gt; \sum_{i=1}^m r_i^s = 1. &amp;lt;/math&amp;gt;&lt;br /&gt;
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The contraction coefficient of a similitude is the magnitude of the dilation.&lt;br /&gt;
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The contraction coefficient of a similitude is the magnitude of the dilation.&lt;br /&gt;
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相似物的收缩系数就是膨胀的大小。&lt;br /&gt;
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We can use this theorem to compute the Hausdorff dimension of the Sierpinski triangle (or sometimes called Sierpinski gasket). Consider three [[non-collinear points]] ''a''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;, ''a''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;, ''a''&amp;lt;sub&amp;gt;3&amp;lt;/sub&amp;gt; in the plane '''R'''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; and let ψ&amp;lt;sub&amp;gt;''i''&amp;lt;/sub&amp;gt; be the dilation of ratio 1/2 around ''a&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;''. The unique non-empty fixed point of the corresponding mapping ψ is a Sierpinski gasket and the dimension ''s'' is the unique solution of&lt;br /&gt;
&lt;br /&gt;
We can use this theorem to compute the Hausdorff dimension of the Sierpinski triangle (or sometimes called Sierpinski gasket). Consider three non-collinear points a&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;, a&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;, a&amp;lt;sub&amp;gt;3&amp;lt;/sub&amp;gt; in the plane R&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; and let ψ&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt; be the dilation of ratio 1/2 around a&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;. The unique non-empty fixed point of the corresponding mapping ψ is a Sierpinski gasket and the dimension s is the unique solution of&lt;br /&gt;
&lt;br /&gt;
我们可以使用这个定理来计算谢尔宾斯基三角形的豪斯多夫维数(或者有时候叫做谢尔宾斯基垫圈)。考虑R&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; 平面上的三个非共线点，''a''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;，''a''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;，''a''&amp;lt;sub&amp;gt;3&amp;lt;/sub&amp;gt;，让ψ&amp;lt;sub&amp;gt;''i''&amp;lt;/sub&amp;gt;是围绕着''a&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;''比率1/2的膨胀。对应映射的唯一非空不动点是一个谢尔宾斯基垫圈，其维数''s''是对应映射的唯一解&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt; \left(\frac{1}{2}\right)^s+\left(\frac{1}{2}\right)^s+\left(\frac{1}{2}\right)^s = 3 \left(\frac{1}{2}\right)^s =1. &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \left(\frac{1}{2}\right)^s+\left(\frac{1}{2}\right)^s+\left(\frac{1}{2}\right)^s = 3 \left(\frac{1}{2}\right)^s =1. &amp;lt;/math&amp;gt;&lt;br /&gt;
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Taking [[natural logarithm]]s of both sides of the above equation, we can solve for ''s'', that is: ''s'' = ln(3)/ln(2).  The Sierpinski gasket is self-similar and satisfies the OSC. In general a set ''E'' which is a fixed point of a mapping&lt;br /&gt;
&lt;br /&gt;
Taking natural logarithms of both sides of the above equation, we can solve for s, that is: s = ln(3)/ln(2).  The Sierpinski gasket is self-similar and satisfies the OSC. In general a set E which is a fixed point of a mapping&lt;br /&gt;
&lt;br /&gt;
取上述方程两边的自然对数，我们可以求出 ''s''，即: ''s'' = ln(3)/ln(2)。该密封垫具有自相似性，满足 OSC 要求。一般来说，集合 ''E''是一个映射的不动点&lt;br /&gt;
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: &amp;lt;math&amp;gt; A \mapsto \psi(A) = \bigcup_{i=1}^m \psi_i(A) &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt; A \mapsto \psi(A) = \bigcup_{i=1}^m \psi_i(A) &amp;lt;/math&amp;gt;&lt;br /&gt;
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is self-similar if and only if the intersections&lt;br /&gt;
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is self-similar if and only if the intersections&lt;br /&gt;
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是自相似的，当且仅当&lt;br /&gt;
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:&amp;lt;math&amp;gt; H^s\left(\psi_i(E) \cap \psi_j(E)\right) =0, &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; H^s\left(\psi_i(E) \cap \psi_j(E)\right) =0, &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
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where ''s'' is the Hausdorff dimension of ''E'' and ''H&amp;lt;sup&amp;gt;s&amp;lt;/sup&amp;gt;'' denotes [[Hausdorff measure]]. This is clear in the case of the Sierpinski gasket (the intersections are just points), but is also true more generally:&lt;br /&gt;
&lt;br /&gt;
where s is the Hausdorff dimension of E and H&amp;lt;sup&amp;gt;s&amp;lt;/sup&amp;gt; denotes Hausdorff measure. This is clear in the case of the Sierpinski gasket (the intersections are just points), but is also true more generally:&lt;br /&gt;
&lt;br /&gt;
其中 ''s''是''E''的豪斯多夫维数， ''H&amp;lt;sup&amp;gt;s&amp;lt;/sup&amp;gt;'' 表示 豪斯多夫测度。对于谢尔宾斯基垫圈(交叉点就是点)来说，这一点很明显，但更普遍的情况是:&lt;br /&gt;
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'''Theorem'''. Under the same conditions as the previous theorem, the unique fixed point of ψ is self-similar.&lt;br /&gt;
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Theorem. Under the same conditions as the previous theorem, the unique fixed point of ψ is self-similar.&lt;br /&gt;
&lt;br /&gt;
'''定理'''：在与前一定理相同的条件下，其唯一不动点是自相似的。&lt;br /&gt;
&lt;br /&gt;
==See also参阅==&lt;br /&gt;
&lt;br /&gt;
* [[List of fractals by Hausdorff dimension豪斯多夫分形维数列表]] Examples of deterministic fractals, random and natural fractals.确定性分形与随机和自然分形的示例。&lt;br /&gt;
&lt;br /&gt;
* [[Assouad dimension  Assouad维数]], another variation of fractal dimension that, like Hausdorff dimension, is defined using coverings by balls其他被球覆盖方式定义的分形维数，例如豪斯多夫维数。&lt;br /&gt;
&lt;br /&gt;
* [[Intrinsic dimension固有维数]]&lt;br /&gt;
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* [[Packing dimension填充维数]]&lt;br /&gt;
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* [[Fractal dimension分形维数]]&lt;br /&gt;
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==References参考文献==&lt;br /&gt;
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{{reflist}}&lt;br /&gt;
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==Further reading拓展阅读==&lt;br /&gt;
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* {{cite book |last1=Dodson |first1=M. Maurice |title=Fractal Geometry and Applications: A Jubilee of Benoît Mandelbrot |volume=72 |issue=1 |pages=305–347 |last2=Kristensen |first2=Simon |chapter=Hausdorff Dimension and Diophantine Approximation |date=June 12, 2003 |arxiv=math/0305399 |bibcode = 2003math......5399D |doi=10.1090/pspum/072.1/2112110|series=Proceedings of Symposia in Pure Mathematics |isbn=9780821836378 }}&lt;br /&gt;
&lt;br /&gt;
* {{cite book |last1=Hurewicz |first1=Witold |authorlink1=Witold Hurewicz |last2=Wallman |first2=Henry |authorlink2=Henry Wallman |title=Dimension Theory |url=https://archive.org/details/in.ernet.dli.2015.84609 |publisher=Princeton University Press |year=1948 }}&lt;br /&gt;
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* {{cite journal |author作者=E. Szpilrajn |authorlink=Edward Marczewski |title=La dimension et la mesure |journal=Fundamenta Mathematicae |volume=28 |pages=81–9 |year=1937 }}&lt;br /&gt;
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* {{cite journal&lt;br /&gt;
&lt;br /&gt;
 | last1=Marstrand&lt;br /&gt;
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 | last1=Marstrand&lt;br /&gt;
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 | last1=马斯特兰德&lt;br /&gt;
&lt;br /&gt;
 | first1=J. M. | title=The dimension of cartesian product sets | year=1954 | journal=Proc. Cambridge Philos. Soc.&lt;br /&gt;
&lt;br /&gt;
 | first1=J. M. | title=The dimension of cartesian product sets | year=1954 | journal=Proc. Cambridge Philos. Soc.&lt;br /&gt;
&lt;br /&gt;
 | first1= J. M. | title=笛卡儿积集的维数 | 1954年 |  journal=Proc. Cambridge Philos. Soc.&lt;br /&gt;
&lt;br /&gt;
 | volume=50&lt;br /&gt;
&lt;br /&gt;
 | volume=50&lt;br /&gt;
&lt;br /&gt;
 | 第50卷&lt;br /&gt;
&lt;br /&gt;
 | issue=3&lt;br /&gt;
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 | issue=3&lt;br /&gt;
&lt;br /&gt;
 | 第三期&lt;br /&gt;
&lt;br /&gt;
 | pages=198–202&lt;br /&gt;
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 | pages=198–202&lt;br /&gt;
&lt;br /&gt;
 | 第198-202页&lt;br /&gt;
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 | doi=10.1017/S0305004100029236|bibcode = 1954PCPS...50..198M }}&lt;br /&gt;
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 | doi=10.1017/S0305004100029236|bibcode = 1954PCPS...50..198M }}&lt;br /&gt;
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10.1017 / S0305004100029236 | bibcode 1954PCPS... 50. . 198 m }&lt;br /&gt;
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* {{Cite book&lt;br /&gt;
&lt;br /&gt;
 | last1=Mattila&lt;br /&gt;
&lt;br /&gt;
 | last1=Mattila&lt;br /&gt;
&lt;br /&gt;
 | last1=Mattila&lt;br /&gt;
&lt;br /&gt;
 | first1=Pertti | author1-link=Pertti Mattila| title=Geometry of sets and measures in Euclidean spaces | publisher=[[Cambridge University Press]]&lt;br /&gt;
&lt;br /&gt;
 | first1=Pertti | author1-link=Pertti Mattila| title=Geometry of sets and measures in Euclidean spaces | publisher=Cambridge University Press&lt;br /&gt;
&lt;br /&gt;
| first1 Pertti | author1-link Pertti Mattila | title 欧几里德空间中集合和度量的几何 | 出版商剑桥大学出版社&lt;br /&gt;
&lt;br /&gt;
 | isbn=978-0-521-65595-8 | year=1995}}&lt;br /&gt;
&lt;br /&gt;
 | isbn=978-0-521-65595-8 | year=1995}}&lt;br /&gt;
&lt;br /&gt;
| isbn 978-0-521-65595-8 | year 1995}&lt;br /&gt;
&lt;br /&gt;
* {{cite journal |author=A. S. Besicovitch |authorlink=A. S. Besicovitch |title=On Linear Sets of Points of Fractional Dimensions |journal=[[Mathematische Annalen]] |volume=101 |year=1929 | doi=10.1007/BF01454831| issue=1 |pages= 161–193}}&lt;br /&gt;
&lt;br /&gt;
* {{cite journal |author1=A. S. Besicovitch |authorlink1=A. S. Besicovitch |author2=H. D. Ursell |authorlink2=H. D. Ursell |title=Sets of Fractional Dimensions |journal=Journal of the London Mathematical Society |volume=12 |year=1937 | issue=1 | doi=10.1112/jlms/s1-12.45.18  | pages=18–25 }}&amp;lt;br/&amp;gt;Several selections from this volume are reprinted in {{cite book |author=Edgar, Gerald A. |title=Classics on fractals |publisher=Addison-Wesley |location=Boston |year=1993 |isbn=0-201-58701-7}} See chapters 9,10,11&lt;br /&gt;
&lt;br /&gt;
* {{cite journal |author=F. Hausdorff |authorlink=F. Hausdorff |title=Dimension und äußeres Maß |journal=Mathematische Annalen |volume=79 |issue=1–2 |pages=157–179 |date=March 1919 |doi=10.1007/BF01457179|hdl=10338.dmlcz/100363 |url=http://dml.cz/bitstream/handle/10338.dmlcz/100363/CzechMathJ_09-1959-3_5.pdf }}&lt;br /&gt;
&lt;br /&gt;
* {{cite journal | last=Hutchinson | first=John E. | title=Fractals and self similarity | journal=Indiana Univ. Math. J. | volume=30 | year=1981 | pages=713–747 | doi=10.1512/iumj.1981.30.30055 | issue=5 | doi-access=free }}&lt;br /&gt;
&lt;br /&gt;
*{{cite book | last=Falconer | first = Kenneth |title=Fractal Geometry: Mathematical Foundations and Applications | publisher=[[John Wiley and Sons]] | edition=2nd | year=2003}}&lt;br /&gt;
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==External links外部链接==&lt;br /&gt;
&lt;br /&gt;
* [https://www.encyclopediaofmath.org/index.php/Hausdorff_dimension Hausdorff dimension] 在 [https://www.encyclopediaofmath.org/ Encyclopedia of Mathematics]&lt;br /&gt;
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* [https://www.encyclopediaofmath.org/index.php/Hausdorff_measure Hausdorff measure] 在 [https://www.encyclopediaofmath.org/ Encyclopedia of Mathematics]&lt;br /&gt;
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{{DEFAULTSORT:Hausdorff Dimension豪斯多夫维数}}&lt;br /&gt;
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[[Category分类:Fractals分形]]&lt;br /&gt;
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[[Category分类:Metric geometry度量几何]]&lt;br /&gt;
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[[Category分类:Dimension theory维度理论]]&lt;br /&gt;
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&amp;lt;small&amp;gt;This page was moved from [[wikipedia:en:Hausdorff dimension]]. Its edit history can be viewed at [[分形维数/edithistory]]&amp;lt;/small&amp;gt;&amp;lt;/noinclude&amp;gt;&lt;br /&gt;
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[[Category:待整理页面]]&lt;/div&gt;</summary>
		<author><name>Ruili</name></author>
	</entry>
	<entry>
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		<title>分形维数</title>
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		<updated>2020-11-01T17:26:42Z</updated>

		<summary type="html">&lt;p&gt;Ruili：&lt;/p&gt;
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&lt;div&gt;此词条暂由彩云小译翻译，未经人工整理和审校，带来阅读不便，请见谅。&lt;br /&gt;
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{{short description|Invariant}}&lt;br /&gt;
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Example of non-integer dimensions. The first four [[iteration]]s of the [[Koch snowflake|Koch curve]], where after each iteration, all original line segments are replaced with four, each a self-similar copy that is 1/3 the length of the original. One formalism of the Hausdorff dimension uses this scale factor (3) and the number of self-similar objects (4) to calculate the dimension, D, after the first iteration to be D = (log N)/(log S) = (log 4)/(log 3) ≈ 1.26.&amp;lt;ref name=CampbellAnnenberg15&amp;gt;MacGregor Campbell, 2013, &amp;quot;5.6 Scaling and the Hausdorff Dimension,&amp;quot; at ''Annenberg Learner:MATHematics illuminated'', see [http://www.learner.org/courses/mathilluminated/units/5/textbook/06.php], accessed 5 March 2015.&amp;lt;/ref&amp;gt; That is, while the Hausdorff dimension of a single [[point (geometry)|point]] is zero, of a [[line segment]] is 1, of a [[square]] is 2, and of a [[cube]] is 3, for [[fractal]]s such as this, the object can have a non-integer dimension.&lt;br /&gt;
&lt;br /&gt;
Example of non-integer dimensions. The first four iterations of the Koch curve, where after each iteration, all original line segments are replaced with four, each a self-similar copy that is 1/3 the length of the original. One formalism of the Hausdorff dimension uses this scale factor (3) and the number of self-similar objects (4) to calculate the dimension, D, after the first iteration to be D = (log N)/(log S) = (log 4)/(log 3) ≈ 1.26. That is, while the Hausdorff dimension of a single point is zero, of a line segment is 1, of a square is 2, and of a cube is 3, for fractals such as this, the object can have a non-integer dimension.&lt;br /&gt;
&lt;br /&gt;
非整数维度示例：前四个[[Koch 曲线]]的迭代，在每次迭代后，所有原始线段都被替换为四个，每个自相似的复制是原始线段长度的1 / 3。豪斯多夫维数的一个建模是使用比例因子(3)和自相似对象的数量(4)来计算维度 D，在第一次迭代后为 D = (log N)/(log S) = (log 4)/(log 3) ≈ 1.26.&amp;lt;ref name=CampbellAnnenberg15&amp;gt;。MacGregor Campbell, 2013, &amp;quot;5.6 Scaling and the Hausdorff Dimension,&amp;quot; 在 ''Annenberg Learner:MATHematics illuminated'', 参见 [http://www.learner.org/courses/mathilluminated/units/5/textbook/06.php], accessed 5 March 2015.&amp;lt;/ref&amp;gt; 也就是说，单点的豪斯多夫维数为零，线段为1，正方形为2，立方体为3时，但对于分形，对象可以有一个非整数维度。&lt;br /&gt;
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In [[mathematics]], '''Hausdorff dimension''' is a measure of ''roughness'', or more specifically, [[fractal dimension]], that was first introduced in 1918 by [[mathematician]] [[Felix Hausdorff]].&amp;lt;ref&amp;gt;{{Cite journal |arxiv = 1101.1444|doi = 10.1214/11-STS370|title = Estimators of Fractal Dimension: Assessing the Roughness of Time Series and Spatial Data|journal = Statistical Science|volume = 27|issue = 2|pages = 247–277|year = 2012|last1 = Gneiting|first1 = Tilmann|last2 = Ševčíková|first2 = Hana|last3 = Percival|first3 = Donald B.}}&amp;lt;/ref&amp;gt; For instance, the Hausdorff dimension of a single [[point (geometry)|point]] is zero, of a [[line segment]] is 1, of a [[square]] is 2, and of a [[cube]] is 3. That is, for sets of points that define a smooth shape or a shape that has a small number of corners—the shapes of traditional geometry and science—the Hausdorff dimension is an [[integer]] agreeing with the usual sense of dimension, also known as the [[Inductive dimension|topological dimension]]. However, formulas have also been developed that allow calculation of the dimension of other less simple objects, where, solely on the basis of their properties of [[scaling (geometry)|scaling]] and [[self-similarity]], one is led to the conclusion that particular objects—including [[fractal]]s—have non-integer Hausdorff dimensions. Because of the significant technical advances made by [[Abram Samoilovitch Besicovitch]] allowing computation of dimensions for highly irregular or &amp;quot;rough&amp;quot; sets, this dimension is also commonly referred to as the ''Hausdorff–Besicovitch dimension.''&lt;br /&gt;
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In mathematics, Hausdorff dimension is a measure of roughness, or more specifically, fractal dimension, that was first introduced in 1918 by mathematician Felix Hausdorff. For instance, the Hausdorff dimension of a single point is zero, of a line segment is 1, of a square is 2, and of a cube is 3. That is, for sets of points that define a smooth shape or a shape that has a small number of corners—the shapes of traditional geometry and science—the Hausdorff dimension is an integer agreeing with the usual sense of dimension, also known as the topological dimension. However, formulas have also been developed that allow calculation of the dimension of other less simple objects, where, solely on the basis of their properties of scaling and self-similarity, one is led to the conclusion that particular objects—including fractals—have non-integer Hausdorff dimensions. Because of the significant technical advances made by Abram Samoilovitch Besicovitch allowing computation of dimensions for highly irregular or &amp;quot;rough&amp;quot; sets, this dimension is also commonly referred to as the Hausdorff–Besicovitch dimension.&lt;br /&gt;
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在[[数学]]中，'''&amp;lt;font color = '#ff8000'&amp;gt;豪斯多夫维数Hausdorff dimension&amp;lt;/font&amp;gt;'''是一种粗糙度的度量单位，或者更确切地说，分形维数，是由数学家 Felix Hausdorff 在1918年首次提出的。例如，单点的豪斯多夫维数为零，线段为1，正方形为2，立方体为3。也就是说，对于定义了一个光滑形状或一个有少数几个角的形状---- 传统几何学和科学的形状---- 的点集来说，豪斯多夫维数是一个整数，符合通常的维度意义，也称为拓扑维度。然而，还有一些公式允许计算其他不太简单的对象的维数，其中仅仅根据它们的标度和自相似特性，就可以得出结论: 特定的对象ー包括分形ー具有非整数的 Hausdorff 维数。由于阿布拉姆·萨莫伊洛维奇·贝西科维奇的重大技术进步，允许计算高度不规则或“粗糙”集的维度，这个维度通常也被称为 Hausdorff-Besicovitch 维度。 &lt;br /&gt;
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The Hausdorff dimension, more specifically, is a further dimensional number associated with a given set, where the distances between all members of that set are defined. Such a set is termed a [[metric space]]. The dimension is drawn from the [[Extended real number line|extended real numbers]], &amp;lt;math&amp;gt;\overline{\mathbb{R}}&amp;lt;/math&amp;gt;, as opposed to the more intuitive notion of dimension, which is not associated to general metric spaces, and only takes values in the non-negative integers.&lt;br /&gt;
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The Hausdorff dimension, more specifically, is a further dimensional number associated with a given set, where the distances between all members of that set are defined. Such a set is termed a metric space. The dimension is drawn from the extended real numbers, &amp;lt;math&amp;gt;\overline{\mathbb{R}}&amp;lt;/math&amp;gt;, as opposed to the more intuitive notion of dimension, which is not associated to general metric spaces, and only takes values in the non-negative integers.&lt;br /&gt;
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更具体地说，豪斯多夫维数是一个与给定集合相关联的更进一步的维数，其中定义了该集合所有成员之间的距离。这样的集合称为度量空间。维数是从扩展的实数，&amp;lt;math&amp;gt;\overline{\mathbb{R}}&amp;lt;/math&amp;gt;，而不是更直观的维数概念(它不与一般的度量空间相关联，只取非负整数的值)。&lt;br /&gt;
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In mathematical terms, the Hausdorff dimension generalizes the notion of the dimension of a real [[vector space]]. That is, the Hausdorff dimension of an ''n''-dimensional [[inner product space]] equals ''n''. This underlies the earlier statement that the Hausdorff dimension of a point is zero, of a line is one, etc., and that [[fractal|irregular sets]] can have noninteger Hausdorff dimensions. For instance, the [[Koch snowflake]] shown at right is constructed from an equilateral triangle; in each iteration, its component line segments are divided into 3 segments of unit length, the newly created middle segment is used as the base of a new [[equilateral]] triangle that points outward, and this base segment is then deleted to leave a final object from the iteration of unit length of 4.&amp;lt;ref&amp;gt;Larry Riddle, 2014, &amp;quot;Classic Iterated Function Systems: Koch Snowflake&amp;quot;, Agnes Scott College e-Academy (online), see [http://ecademy.agnesscott.edu/~lriddle/ifs/ksnow/ksnow.htm], accessed 5 March 2015.&amp;lt;/ref&amp;gt; That is, after the first iteration, each original line segment has been replaced with N=4, where each self-similar copy is 1/S = 1/3 as long as the original.&amp;lt;ref name=CampbellAnnenberg15/&amp;gt; Stated another way, we have taken an object with Euclidean dimension, D, and reduced its linear scale by 1/3 in each direction, so that its length increases to N=S&amp;lt;sup&amp;gt;D&amp;lt;/sup&amp;gt;.&amp;lt;ref name=ClaytonSCTPLS96&amp;gt;Keith Clayton, 1996, &amp;quot;Fractals and the Fractal Dimension,&amp;quot; ''Basic Concepts in Nonlinear Dynamics and Chaos'' (workshop), Society for Chaos Theory in Psychology and the Life Sciences annual meeting, June 28, 1996, Berkeley, California, see [http://www.vanderbilt.edu/AnS/psychology/cogsci/chaos/workshop/Workshop.html], accessed 5 March 2015.&amp;lt;/ref&amp;gt; This equation is easily solved for D, yielding the ratio of logarithms (or [[natural logarithm]]s) appearing in the figures, and giving—in the Koch and other fractal cases—non-integer dimensions for these objects.&lt;br /&gt;
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In mathematical terms, the Hausdorff dimension generalizes the notion of the dimension of a real vector space. That is, the Hausdorff dimension of an n-dimensional inner product space equals n. This underlies the earlier statement that the Hausdorff dimension of a point is zero, of a line is one, etc., and that irregular sets can have noninteger Hausdorff dimensions. For instance, the Koch snowflake shown at right is constructed from an equilateral triangle; in each iteration, its component line segments are divided into 3 segments of unit length, the newly created middle segment is used as the base of a new equilateral triangle that points outward, and this base segment is then deleted to leave a final object from the iteration of unit length of 4. That is, after the first iteration, each original line segment has been replaced with N=4, where each self-similar copy is 1/S = 1/3 as long as the original. This equation is easily solved for D, yielding the ratio of logarithms (or natural logarithms) appearing in the figures, and giving—in the Koch and other fractal cases—non-integer dimensions for these objects.&lt;br /&gt;
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用数学术语来说，豪斯多夫维数概括了实向量空间维数的概念。也就是说，n 维内积空间的豪斯多夫维数等于 n。 这就是早期假设的基础，一个点的豪斯多夫维数是零，一条线是一等等，不规则集可以有非整数的豪斯多夫维数。例如，右边所示的 Koch 雪花是由一个正三角形构成的; 在每次迭代中，它的组成线段被分成单位长度的3段，新创建的中间线段被用作一个指向外部的新正三角形的基础，然后人们删除这个基础线段用来保留单位长度4的迭代中的最终对象。也就是说，在第一次迭代之后，每个原始线段都被替换为 N=4，其中每个自相似拷贝的长度是原始线段的1/S = 1/3 。这个方程很容易求解为 D，产生出现在图形中的对数(或自然对数)的比率，并给出——在 Koch 和其他分形情况下——这些对象的非整数维数。&lt;br /&gt;
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The Hausdorff dimension is a successor to the simpler, but usually equivalent, box-counting or [[Minkowski–Bouligand dimension]].&lt;br /&gt;
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The Hausdorff dimension is a successor to the simpler, but usually equivalent, box-counting or Minkowski–Bouligand dimension.&lt;br /&gt;
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豪斯多夫维数是更简单但通常等价的'''&amp;lt;font color = '#ff8000'&amp;gt;计盒维数box-counting&amp;lt;/font&amp;gt;'''或'''&amp;lt;font color = '#ff8000'&amp;gt;闵可夫斯基维数Minkowski-Bouligand&amp;lt;/font&amp;gt;'''的继承者。&lt;br /&gt;
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==Intuition概念==&lt;br /&gt;
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The intuitive concept of dimension of a geometric object ''X'' is the number of independent parameters one needs to pick out a unique point inside. However, any point specified by two parameters can be instead specified by one, because the [[cardinality]] of the [[real plane]] is equal to the cardinality of the [[real line]] (this can be seen by an [[Cantor's diagonal argument|argument]] involving interweaving the digits of two numbers to yield a single number encoding the same information). The example of a [[space-filling curve]] shows that one can even map the real line to the real plane [[Surjective function|surjectively]] (taking one real number into a pair of real numbers in a way so that all pairs of numbers are covered) and ''continuously'', so that a one-dimensional object completely fills up a higher-dimensional object.&lt;br /&gt;
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The intuitive concept of dimension of a geometric object X is the number of independent parameters one needs to pick out a unique point inside. However, any point specified by two parameters can be instead specified by one, because the cardinality of the real plane is equal to the cardinality of the real line (this can be seen by an argument involving interweaving the digits of two numbers to yield a single number encoding the same information). The example of a space-filling curve shows that one can even map the real line to the real plane surjectively (taking one real number into a pair of real numbers in a way so that all pairs of numbers are covered) and continuously, so that a one-dimensional object completely fills up a higher-dimensional object.&lt;br /&gt;
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几何对象X的尺寸的直观概念是指需要多少个独立参数才能找到一个独特的点。但是，任何由两个参数指定的点都可以由一个参数指定，因为为实平面的基数等于实线的基数(这可以通过交织两个数字以产生一个编码相同信息的单个数字看到)。'''&amp;lt;font color = '#ff8000'&amp;gt;皮亚诺曲线&amp;lt;/font&amp;gt;'''的例子表明，可以将实线完美和连续地映射到实平面(把一个实数转换成一对实数，从而覆盖所有实数对)，由此一维对象完全填充了一个高维对象。&lt;br /&gt;
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Every space filling curve hits some points multiple times, and does not have a continuous inverse. It is impossible to map two dimensions onto one in a way that is continuous and continuously invertible. The topological dimension, also called [[Lebesgue covering dimension]], explains why. This dimension is ''n'' if, in every covering of ''X'' by small open balls, there is at least one point where ''n''&amp;amp;nbsp;+&amp;amp;nbsp;1 balls overlap. For example, when one covers a line with short open intervals, some points must be covered twice, giving dimension&amp;amp;nbsp;''n''&amp;amp;nbsp;=&amp;amp;nbsp;1.&lt;br /&gt;
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Every space filling curve hits some points multiple times, and does not have a continuous inverse. It is impossible to map two dimensions onto one in a way that is continuous and continuously invertible. The topological dimension, also called Lebesgue covering dimension, explains why. This dimension is n if, in every covering of X by small open balls, there is at least one point where n&amp;amp;nbsp;+&amp;amp;nbsp;1 balls overlap. For example, when one covers a line with short open intervals, some points must be covered twice, giving dimension&amp;amp;nbsp;n&amp;amp;nbsp;=&amp;amp;nbsp;1.&lt;br /&gt;
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每条空间填充曲线都会多次击中某些点，且不存在连续的逆。将二维以连续和连续可逆的方式映射到一维是不可能的。'''&amp;lt;font color = '#ff8000'&amp;gt;拓扑维度 topological dimension&amp;lt;/font&amp;gt;'''，也被称为Lebesgue覆盖维数，解释了为什么。如果在 x 的每个小开球覆盖中，至少有一个点 n + 1个球重叠，这个维度是 n。例如，当用短的开区间覆盖一条线时，某些点必须被覆盖两次，给出维数''n''&amp;amp;nbsp;=&amp;amp;nbsp;1。&lt;br /&gt;
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But topological dimension is a very crude measure of the local size of a space (size near a point). A curve that is almost space-filling can still have topological dimension one, even if it fills up most of the area of a region. A [[fractal]] has an integer topological dimension, but in terms of the amount of space it takes up, it behaves like a higher-dimensional space.&lt;br /&gt;
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But topological dimension is a very crude measure of the local size of a space (size near a point). A curve that is almost space-filling can still have topological dimension one, even if it fills up most of the area of a region. A fractal has an integer topological dimension, but in terms of the amount of space it takes up, it behaves like a higher-dimensional space.&lt;br /&gt;
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但是，拓扑维度是对空间局部尺寸(点附近的尺寸)的一个非常粗略的度量。一条几乎是空间填充的曲线仍然可以有一维拓扑，即使它填充了一个区域的大部分面积。分形具有整数的拓扑维数，但就其所占的空间量而言，它看起来像一个更高维的空间。&lt;br /&gt;
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The Hausdorff dimension measures the local size of a space taking into account the distance between points, the [[metric space|metric]]. Consider the number ''N''(''r'') of [[ball (mathematics)|balls]] of radius at most ''r'' required to cover ''X'' completely. When ''r'' is very small, ''N''(''r'') grows polynomially with 1/''r''. For a sufficiently well-behaved  ''X'', the Hausdorff dimension is the unique number ''d'' such that N(''r'') grows as 1/''r&amp;lt;sup&amp;gt;d&amp;lt;/sup&amp;gt;'' as ''r'' approaches zero. More precisely, this defines the [[Minkowski–Bouligand dimension|box-counting dimension]], which equals the Hausdorff dimension when the value ''d'' is a critical boundary between growth rates that are insufficient to cover the space, and growth rates that are overabundant.&lt;br /&gt;
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The Hausdorff dimension measures the local size of a space taking into account the distance between points, the metric. Consider the number N(r) of balls of radius at most r required to cover X completely. When r is very small, N(r) grows polynomially with 1/r. For a sufficiently well-behaved  X, the Hausdorff dimension is the unique number d such that N(r) grows as 1/r&amp;lt;sup&amp;gt;d&amp;lt;/sup&amp;gt; as r approaches zero. More precisely, this defines the box-counting dimension, which equals the Hausdorff dimension when the value d is a critical boundary between growth rates that are insufficient to cover the space, and growth rates that are overabundant.&lt;br /&gt;
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豪斯多夫维数测量一个空间的局部大小时，会考虑到点之间距离的度量。考虑半径最大为 r 的球数 ''N'' (r) ，需要完全覆盖 ''X''。当 r 很小时，n (r)以1/''r'' 增长多项式。对于一个表现足够好的 ''X''，豪斯多夫维数是唯一的数 d，这样当 r 趋近于零时， N(r)增长为1/r&amp;lt;sup&amp;gt;d&amp;lt;/sup&amp;gt; 。更确切地说，这定义了盒子计数维度，当值 d 是不足以覆盖空间的增长率和过度充裕的增长率之间的关键边界时，它等于豪斯多夫维数。&lt;br /&gt;
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For shapes that are smooth, or shapes with a small number of corners, the shapes of traditional geometry and science, the Hausdorff dimension is an integer agreeing with the topological dimension. But [[Benoit Mandelbrot]] observed that [[fractal]]s, sets with noninteger Hausdorff dimensions, are found everywhere in nature. He observed that the proper idealization of most rough shapes you see around you is not in terms of smooth idealized shapes, but in terms of fractal idealized shapes:&lt;br /&gt;
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For shapes that are smooth, or shapes with a small number of corners, the shapes of traditional geometry and science, the Hausdorff dimension is an integer agreeing with the topological dimension. But Benoit Mandelbrot observed that fractals, sets with noninteger Hausdorff dimensions, are found everywhere in nature. He observed that the proper idealization of most rough shapes you see around you is not in terms of smooth idealized shapes, but in terms of fractal idealized shapes:&lt;br /&gt;
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对于光滑的形状，或者有少量棱角的形状，传统几何和科学的形状，豪斯多夫维数是一个整数，与拓扑维度一致。但是伯努·曼德布洛特观察到分形---- 具有非整数豪斯多夫维数的集合---- 在自然界中随处可见。他观察到，我们周围大多数粗糙形状的理想化不是光滑的理想化形状，而是分形理想化形状:&lt;br /&gt;
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&amp;lt;blockquote&amp;gt;Clouds are not spheres, mountains are not cones, coastlines are not circles, and bark is not smooth, nor does lightning travel in a straight line.&amp;lt;ref name=&amp;quot;mandelbrot&amp;quot;&amp;gt;{{cite book   | last = Mandelbrot   | first = Benoît   | authorlink = Benoit Mandelbrot   | title = The Fractal Geometry of Nature   | publisher = W. H. Freeman   | series = Lecture notes in mathematics 1358   | year = 1982   | doi =    | isbn = 0-7167-1186-9   | url-access = registration   | url = https://archive.org/details/fractalgeometryo00beno   }}&amp;lt;/ref&amp;gt;&amp;lt;/blockquote&amp;gt;&lt;br /&gt;
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&amp;lt;blockquote&amp;gt;Clouds are not spheres, mountains are not cones, coastlines are not circles, and bark is not smooth, nor does lightning travel in a straight line.&amp;lt;/blockquote&amp;gt;&lt;br /&gt;
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&amp;lt;blockquote&amp;gt;云不是球体，山不是锥体，海岸线不是圆圈，树皮不平滑，闪电也不是直线运动。 &amp;lt;/blockquote&amp;gt;&lt;br /&gt;
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For fractals that occur in nature, the Hausdorff and [[Minkowski–Bouligand dimension|box-counting dimension]] coincide. The [[packing dimension]] is yet another similar notion which gives the same value for many shapes, but there are well documented exceptions where all these dimensions differ.&lt;br /&gt;
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For fractals that occur in nature, the Hausdorff and box-counting dimension coincide. The packing dimension is yet another similar notion which gives the same value for many shapes, but there are well documented exceptions where all these dimensions differ.&lt;br /&gt;
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对于自然界中出现的分形，豪斯多夫维数和盒计数维数是一致的。封装尺寸是另一个类似的概念，它给出了许多形状相同的值，但是在所有这些尺寸不同的情况，都做了很好的说明。&lt;br /&gt;
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==Formal definitions形式化定义==&lt;br /&gt;
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===Hausdorff content豪斯多夫集===&lt;br /&gt;
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Let ''X'' be a [[metric space]]. If ''S'' ⊂ ''X'' and ''d'' ∈ [0, ∞), the ''d''-dimensional '''unlimited Hausdorff content''' of ''S'' is defined by&lt;br /&gt;
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Let X be a metric space. If S ⊂ X and d ∈ [0, ∞), the d-dimensional unlimited Hausdorff content of S is defined by&lt;br /&gt;
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设 ''X''是度量空间。若''S'' ⊂ ''X'' 和 ''d'' ∈ [0, ∞) ，则 ''S'' 的''d''维无限 豪斯多夫集定义为&lt;br /&gt;
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:&amp;lt;math&amp;gt;C_H^d(S):=\inf\Bigl\{\sum_i r_i^d:\text{ there is a cover of } S\text{ by balls with radii }r_i&amp;gt;0\Bigr\}.&amp;lt;/math&amp;gt;&lt;br /&gt;
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&amp;lt;math&amp;gt;C_H^d(S):=\inf\Bigl\{\sum_i r_i^d:\text{ there is a cover of } S\text{ by balls with radii }r_i&amp;gt;0\Bigr\}.&amp;lt;/math&amp;gt;&lt;br /&gt;
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&amp;lt;math&amp;gt;C_H^d(S):=\inf\Bigl\{\sum_i r_i^d:\text{ there is a cover of } S\text{ by balls with radii }r_i&amp;gt;0\Bigr\}.&amp;lt;/math&amp;gt;&lt;br /&gt;
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In other words, &amp;lt;math&amp;gt;C_H^d(S)&amp;lt;/math&amp;gt; is the [[infimum]] of the set of numbers &amp;lt;math&amp;gt;\delta \geq 0&amp;lt;/math&amp;gt; such that there is some (indexed) collection of [[ball (mathematics)|ball]]s &amp;lt;math&amp;gt;\{B(x_i,r_i):i\in I\}&amp;lt;/math&amp;gt; covering ''S'' with ''r&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;''&amp;amp;nbsp;&amp;gt;&amp;amp;nbsp;0 for each ''i''&amp;amp;nbsp;∈&amp;amp;nbsp;''I'' that satisfies &amp;lt;math&amp;gt;\sum_{i\in I} r_i^d&amp;lt;\delta &amp;lt;/math&amp;gt;. (Here, we use the standard convention that [[infimum|inf&amp;amp;nbsp;Ø&amp;amp;nbsp;=&amp;amp;nbsp;∞]].)&lt;br /&gt;
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In other words, &amp;lt;math&amp;gt;C_H^d(S)&amp;lt;/math&amp;gt; is the infimum of the set of numbers &amp;lt;math&amp;gt;\delta \geq 0&amp;lt;/math&amp;gt; such that there is some (indexed) collection of balls &amp;lt;math&amp;gt;\{B(x_i,r_i):i\in I\}&amp;lt;/math&amp;gt; covering S with r&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;&amp;amp;nbsp;&amp;gt;&amp;amp;nbsp;0 for each i&amp;amp;nbsp;∈&amp;amp;nbsp;I that satisfies &amp;lt;math&amp;gt;\sum_{i\in I} r_i^d&amp;lt;\delta &amp;lt;/math&amp;gt;. (Here, we use the standard convention that inf&amp;amp;nbsp;Ø&amp;amp;nbsp;=&amp;amp;nbsp;∞.)&lt;br /&gt;
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换句话说，&amp;lt;math&amp;gt;C_H^d(S)&amp;lt;/math&amp;gt; 是数字集合&amp;lt;math&amp;gt;\delta \geq 0&amp;lt;/math&amp;gt;的下确界，使得在 ''i''&amp;amp;nbsp;∈&amp;amp;nbsp中存在一些球集合 &amp;lt;math&amp;gt;\{B(x_i,r_i):i\in I\}&amp;lt;/math&amp;gt;  i 包含 s，对于每个 ''r&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;''&amp;amp;nbsp;&amp;gt;&amp;amp;nbsp;0 满足 i 中的和&amp;lt;math&amp;gt;\sum_{i\in I} r_i^d&amp;lt;\delta &amp;lt;/math&amp;gt; (在这里，我们使用inf&amp;amp;nbsp;Ø&amp;amp;nbsp;=&amp;amp;nbsp;∞ )的标准约定。&lt;br /&gt;
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===Hausdorff measurement豪斯多夫分形测量===&lt;br /&gt;
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The Hausdorff outer measure is different from the unbounded Hausdorf content in that rather than considering all possible coverings of ''S'', we see what happens when the sizes of the balls go to zero. This is  for &amp;lt;math&amp;gt;d \geq 0 &amp;lt;/math&amp;gt;, we define the ''d''-dimensional Hausdorff outer measure of ''S'' as&lt;br /&gt;
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The Hausdorff outer measure is different from the unbounded Hausdorf content in that rather than considering all possible coverings of S, we see what happens when the sizes of the balls go to zero. This is  for &amp;lt;math&amp;gt;d \geq 0 &amp;lt;/math&amp;gt;, we define the d-dimensional Hausdorff outer measure of S as&lt;br /&gt;
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豪斯多夫外测度不同于无界的豪斯多夫，因为我们不考虑 s 的所有可能，我们看到当球的大小为零时会发生什么。这是为了数学  &amp;lt;math&amp;gt;d \geq 0 &amp;lt;/math&amp;gt;，我们定义了  ''S''的 ''d''维豪斯多夫Hausdorff 外测度为&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt; \mathcal{H}^d(S):=\lim_{r \to 0} \inf\Bigl\{\sum_i r_i^d:\text{ there is a cover of } S\text{ by balls with radii } 0 &amp;lt; r_i &amp;lt; r\Bigr\}.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \mathcal{H}^d(S):=\lim_{r \to 0} \inf\Bigl\{\sum_i r_i^d:\text{ there is a cover of } S\text{ by balls with radii } 0 &amp;lt; r_i &amp;lt; r\Bigr\}.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \mathcal{H}^d(S):=\lim_{r \to 0} \inf\Bigl\{\sum_i r_i^d:\text{有一个面} S\text{ 球 } 0 &amp;lt; r_i &amp;lt; r\Bigr\}.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
===Hausdorff dimension豪斯多夫维数===&lt;br /&gt;
&lt;br /&gt;
The '''Hausdorff dimension''' of ''X'' is defined by&lt;br /&gt;
&lt;br /&gt;
The Hausdorff dimension of X is defined by&lt;br /&gt;
&lt;br /&gt;
X 的豪斯多夫维数定义为&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt;\dim_{\operatorname{H}}(X):=\inf\{d\ge 0: \mathcal{H}^d(X)=0\}.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt;\dim_{\operatorname{H}}(X):=\inf\{d\ge 0: \mathcal{H}^d(X)=0\}.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Equivalently, dim&amp;lt;sub&amp;gt;H&amp;lt;/sub&amp;gt;(''X'') may be defined as the [[infimum]] of the set of ''d'' ∈ [0, ∞) such that the ''d''-dimensional [[Hausdorff measure]] of ''X'' is zero. This is the same as the supremum of the set of ''d''&amp;amp;nbsp;∈&amp;amp;nbsp;[0,&amp;amp;nbsp;∞) such that the ''d''-dimensional Hausdorff measure of ''X'' is infinite (except that when this latter set of numbers ''d'' is empty the Hausdorff dimension is zero).&lt;br /&gt;
&lt;br /&gt;
Equivalently, dim&amp;lt;sub&amp;gt;H&amp;lt;/sub&amp;gt;(X) may be defined as the infimum of the set of d ∈ [0, ∞) such that the d-dimensional Hausdorff measure of X is zero. This is the same as the supremum of the set of d&amp;amp;nbsp;∈&amp;amp;nbsp;[0,&amp;amp;nbsp;∞) such that the d-dimensional Hausdorff measure of X is infinite (except that when this latter set of numbers d is empty the Hausdorff dimension is zero).&lt;br /&gt;
&lt;br /&gt;
等价地，dim &amp;lt;sub&amp;gt;H&amp;lt;/sub&amp;gt;(''X'')可定义为 ''d'' ∈ [0, ∞) 集的下确界，使得''X'' 的''d''-维 [[豪斯多夫测度]] 为零。这与 ''d''&amp;amp;nbsp;∈&amp;amp;nbsp;[0,&amp;amp;nbsp;∞)的集合的上确界相同，因此''X''的 d 维豪斯多夫测度是无限的(除非后一个集合 ''d'' 是空的，豪斯多夫维数为零)。&lt;br /&gt;
&lt;br /&gt;
==Examples实例==&lt;br /&gt;
&lt;br /&gt;
[[Image:Sierpinski deep.svg|thumb|250px|Dimension of a further [[fractal]] example. The [[Sierpinski triangle]], an object with Hausdorff dimension of log(3)/log(2)≈1.58.&amp;lt;ref name=ClaytonSCTPLS96/&amp;gt;]]&lt;br /&gt;
&lt;br /&gt;
Dimension of a further [[fractal example. The Sierpinski triangle, an object with Hausdorff dimension of log(3)/log(2)≈1.58.]]&lt;br /&gt;
&lt;br /&gt;
[[Image:谢尔宾斯基三角形 deep.svg|thumb|250px|进一步的[[分形维数]]的例子，进一步的分形维数的例子是谢尔宾斯基三角形，它是一个豪斯多夫维数为log(3)/log(2)≈1.58.&amp;lt;ref name=ClaytonSCTPLS96/&amp;gt;的物体]]&lt;br /&gt;
&lt;br /&gt;
* [[Countable set]]s have Hausdorff dimension 0.&amp;lt;ref name=&amp;quot;schleicher&amp;quot;&amp;gt;{{cite journal |last1=Schleicher |first1=Dierk |title=Hausdorff Dimension, Its Properties, and Its Surprises |journal=The American Mathematical Monthly |date=June 2007 |volume=114 |issue=6 |pages=509–528 |doi=10.1080/00029890.2007.11920440 |language=en |issn=0002-9890|arxiv=math/0505099 }}&amp;lt;/ref&amp;gt;&lt;br /&gt;
*[[可数集]]拥有豪斯多夫维数0.&amp;lt;ref name=&amp;quot;schleicher&amp;quot;&amp;gt;{{cite journal |last1=Schleicher |first1=Dierk |title=豪斯多夫维数, Its Properties, and Its Surprises |journal=The American Mathematical Monthly美国数学期刊 |date=June 2007 |volume=114 |issue=6 |pages=509–528 |doi=10.1080/00029890.2007.11920440 |language=en |issn=0002-9890|arxiv=math/0505099 }}&amp;lt;/ref&amp;gt;&lt;br /&gt;
* The [[Euclidean space]] ℝ&amp;lt;sup&amp;gt;''n''&amp;lt;/sup&amp;gt; has Hausdorff dimension ''n'', and the circle '''S'''&amp;lt;sup&amp;gt;1&amp;lt;/sup&amp;gt; has Hausdorff dimension 1.&amp;lt;ref name=&amp;quot;schleicher&amp;quot; /&amp;gt;&lt;br /&gt;
*[[教育空间]] ℝ&amp;lt;sup&amp;gt;''n''&amp;lt;/sup&amp;gt; 有豪斯多夫维数 ''n''，循环'''S'''&amp;lt;sup&amp;gt;1&amp;lt;/sup&amp;gt; 拥有豪斯多夫维数1.&amp;lt;ref name=&amp;quot;schleicher&amp;quot; /&amp;gt;&lt;br /&gt;
* [[Fractal]]s often are spaces whose Hausdorff dimension strictly exceeds the [[topological dimension]].&amp;lt;ref name=&amp;quot;mandelbrot&amp;quot; /&amp;gt; For example, the [[Cantor set]], a zero-dimensional topological space, is a union of two copies of itself, each copy shrunk by a factor 1/3; hence, it can be shown that its Hausdorff dimension is ln(2)/ln(3)&amp;amp;nbsp;≈&amp;amp;nbsp;0.63.&amp;lt;ref&amp;gt;{{cite book | last=Falconer | first = Kenneth |title=Fractal Geometry: Mathematical Foundations and Applications | publisher=[[John Wiley and Sons]] | edition=2nd | year=2003}}&amp;lt;/ref&amp;gt; The [[Sierpinski triangle]] is a union of three copies of itself, each copy shrunk by a factor of&amp;amp;nbsp;1/2; this yields a Hausdorff dimension of ln(3)/ln(2)&amp;amp;nbsp;≈&amp;amp;nbsp;1.58.&amp;lt;ref name=CampbellAnnenberg15/&amp;gt; These Hausdorff dimensions are related to the &amp;quot;critical exponent&amp;quot; of the [[Master theorem (analysis of algorithms)|Master theorem]] for solving [[Recurrence relation|recurrence relations]] in the [[analysis of algorithms]].&lt;br /&gt;
*[[分形]]一般是那些豪斯多夫维数直接超过其拓扑维数的空间。例如[[康托尔集]]是一个o维拓扑空间，由两个自己复制而成，每一个复制品都是原来的三分之一，因此它的豪斯多夫维数是 ln(2)/ln(3)&amp;amp;nbsp;≈&amp;amp;nbsp;0.63。&amp;lt;ref&amp;gt;{{cite book | last=Falconer | first = Kenneth |title=Fractal Geometry: Mathematical Foundations and Applications | publisher=[[John Wiley and Sons]] | edition=2nd | year=2003}}&amp;lt;/ref&amp;gt;一个[[谢尔宾斯基三角]]是他自身三个复制的组合。每一个是原来的&amp;amp;nbsp;1/2，它的豪斯多夫维数ln(3)/ln(2)&amp;amp;nbsp;≈&amp;amp;nbsp;1.58。&amp;lt;ref name=CampbellAnnenberg15/&amp;gt;在递归算法中解决递归关系时，这些豪斯多夫维数与[[算法分析主定理]]的临界指标相联系。&lt;br /&gt;
* [[Space-filling curve]]s like the [[Peano curve]] have the same Hausdorff dimension as the space they fill.&lt;br /&gt;
*[[空间填充曲线]]拥有和他们填充空间同样的豪斯多夫维数，如[[皮亚诺曲线]]。&lt;br /&gt;
* The trajectory of [[Brownian motion]] in dimension 2 and above is conjectured to be Hausdorff dimension 2.&amp;lt;ref&amp;gt;{{cite book | last=Morters | first=Peres | title= Brownian Motion | publisher=[[Cambridge University Press]] | year=2010 }}&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
[[image:Great Britain Hausdorff.svg|thumb|250px|Estimating the Hausdorff dimension of the [[How Long Is the Coast of Britain? Statistical Self-Similarity and Fractional Dimension|coast of Great Britain]]]]&lt;br /&gt;
&lt;br /&gt;
coast of Great Britain]]&lt;br /&gt;
&lt;br /&gt;
[[大不列颠海岸&lt;br /&gt;
&lt;br /&gt;
* 刘易斯·弗赖伊·理查森[[Lewis Fry Richardson]] has performed detailed experiments to measure the approximate Hausdorff dimension for various coastlines. His results have varied from 1.02 for the coastline of [[South Africa]] to 1.25 for the west coast of [[Great Britain]].&amp;lt;ref name=&amp;quot;mandelbrot&amp;quot; /&amp;gt;&lt;br /&gt;
*刘易斯·弗赖伊·理查森（Lewis Fry Richardson）已经通过豪斯多夫维数去测量了很多海岸线。它的结果涵盖从1.02的南非海岸线到1.25的大英帝国西海岸模型。]]&lt;br /&gt;
&lt;br /&gt;
==Properties of Hausdorff dimension豪斯多夫维数特性==&lt;br /&gt;
&lt;br /&gt;
{{refimprove section|date=March 2015}}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
=== Hausdorff dimension and inductive dimension 豪斯多夫维数和归纳维数===&lt;br /&gt;
&lt;br /&gt;
Let ''X'' be an arbitrary [[Separable space|separable]] metric space. There is a [[topology|topological]] notion of [[inductive dimension]] for ''X'' which is defined recursively. It is always an integer (or +∞) and is denoted dim&amp;lt;sub&amp;gt;ind&amp;lt;/sub&amp;gt;(''X'').&lt;br /&gt;
&lt;br /&gt;
Let X be an arbitrary separable metric space. There is a topological notion of inductive dimension for X which is defined recursively. It is always an integer (or +∞) and is denoted dim&amp;lt;sub&amp;gt;ind&amp;lt;/sub&amp;gt;(X).&lt;br /&gt;
&lt;br /&gt;
设''X'' 是[[任意可分度量空间]]。对于''X'' 有一个递归定义的归纳维数拓扑概念。它总是一个整数(或 + ∞) ，记为dim&amp;lt;sub&amp;gt;ind&amp;lt;/sub&amp;gt;(''X'')。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
'''Theorem'''. Suppose ''X'' is non-empty. Then &lt;br /&gt;
&lt;br /&gt;
Theorem. Suppose X is non-empty. Then &lt;br /&gt;
&lt;br /&gt;
'''定理'''：假设''X'' 是非空的, 那么&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt; \dim_{\mathrm{Haus}}(X) \geq \dim_{\operatorname{ind}}(X). &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \dim_{\mathrm{Haus}}(X) \geq \dim_{\operatorname{ind}}(X). &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Moreover,&lt;br /&gt;
&lt;br /&gt;
Moreover,&lt;br /&gt;
&lt;br /&gt;
此外,&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \inf_Y \dim_{\operatorname{Haus}}(Y) =\dim_{\operatorname{ind}}(X), &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \inf_Y \dim_{\operatorname{Haus}}(Y) =\dim_{\operatorname{ind}}(X), &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
where ''Y'' ranges over metric spaces [[homeomorphic]] to ''X''. In other words, ''X'' and ''Y'' have the same underlying set of points and the metric ''d''&amp;lt;sub&amp;gt;''Y''&amp;lt;/sub&amp;gt; of ''Y'' is topologically equivalent to ''d''&amp;lt;sub&amp;gt;''X''&amp;lt;/sub&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
where Y ranges over metric spaces homeomorphic to X. In other words, X and Y have the same underlying set of points and the metric d&amp;lt;sub&amp;gt;Y&amp;lt;/sub&amp;gt; of Y is topologically equivalent to d&amp;lt;sub&amp;gt;X&amp;lt;/sub&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
其中''Y''是度量空间同胚到 ''X''的范围。换句话说， ''X''和 ''Y''具有相同的基本点集，''Y''的度量''d''&amp;lt;sub&amp;gt;''Y''&amp;lt;/sub&amp;gt; 拓扑等价于''d''&amp;lt;sub&amp;gt;''X''&amp;lt;/sub&amp;gt;。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
These results were originally established by [[Edward Szpilrajn]] (1907–1976), e.g., see Hurewicz and Wallman, Chapter VII.{{full citation needed|date=March 2015}}&lt;br /&gt;
&lt;br /&gt;
These results were originally established by Edward Szpilrajn (1907–1976), e.g., see Hurewicz and Wallman, Chapter VII.&lt;br /&gt;
&lt;br /&gt;
这些结果最初是由 [[Edward Szpilrajn]] (1907–1976)建立的,  参见 Hurewicz and Wallman, Chapter VII.{{full citation needed|date=March 2015}}第七章。&lt;br /&gt;
&lt;br /&gt;
=== Hausdorff dimension and Minkowski dimension 豪斯多夫维数和闵可夫斯基维度===&lt;br /&gt;
&lt;br /&gt;
The [[Minkowski dimension]] is similar to, and at least as large as, the Hausdorff dimension, and they are equal in many situations. However, the set of [[rational number|rational]] points in [0, 1] has Hausdorff dimension zero and Minkowski dimension one. There are also compact sets for which the Minkowski dimension is strictly larger than the Hausdorff dimension.&lt;br /&gt;
&lt;br /&gt;
The Minkowski dimension is similar to, and at least as large as, the Hausdorff dimension, and they are equal in many situations. However, the set of rational points in [0, 1] has Hausdorff dimension zero and Minkowski dimension one. There are also compact sets for which the Minkowski dimension is strictly larger than the Hausdorff dimension.&lt;br /&gt;
&lt;br /&gt;
[[闵可夫斯基维数]]与豪斯多夫维数相似，至少和它一样大，而且在许多情况下是相等的。然而，[0,1]中有理点集的豪斯多夫维数为0，闵可夫斯基维数为1。还有一些紧集的闵可夫斯基维数绝对大于豪斯多夫维数。&lt;br /&gt;
&lt;br /&gt;
=== Hausdorff dimensions and Frostman measures 豪斯多夫维度和弗洛斯曼测度===&lt;br /&gt;
&lt;br /&gt;
If there is a [[measure (mathematics)|measure]] μ defined on [[Borel measure|Borel]] subsets of a metric space ''X'' such that ''μ''(''X'') &amp;gt; 0 and ''μ''(''B''(''x'', ''r'')) ≤ ''r&amp;lt;sup&amp;gt;s&amp;lt;/sup&amp;gt;'' holds for some constant ''s'' &amp;gt; 0 and for every ball ''B''(''x'', ''r'') in ''X'', then dim&amp;lt;sub&amp;gt;Haus&amp;lt;/sub&amp;gt;(''X'') ≥ ''s''. A partial converse is provided by [[Frostman's lemma]].{{citation needed|date=March 2015}}&amp;lt;ref&amp;gt;This Wikipedia article also discusses further useful characterizations of the Hausdorff dimension.{{clarify|date=March 2015}}&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
If there is a measure μ defined on Borel subsets of a metric space X such that μ(X) &amp;gt; 0 and μ(B(x, r)) ≤ r&amp;lt;sup&amp;gt;s&amp;lt;/sup&amp;gt; holds for some constant s &amp;gt; 0 and for every ball B(x, r) in X, then dim&amp;lt;sub&amp;gt;Haus&amp;lt;/sub&amp;gt;(X) ≥ s. A partial converse is provided by Frostman's lemma.&lt;br /&gt;
&lt;br /&gt;
如果在度量空间 ''X'' 的 Borel 子集上定义一个测度 μ，使得''μ''(''X'') &amp;gt; 0 和''μ''(''B''(''x'', ''r'')) ≤ ''r&amp;lt;sup&amp;gt;s&amp;lt;/sup&amp;gt;''，对于某个常数 ''s'' &amp;gt; 0  和 ''X'' 中的每个球 ''B''(''x'', ''r'') 成立，则 dim&amp;lt;sub&amp;gt;Haus&amp;lt;/sub&amp;gt;(''X'') ≥ ''s'' 。 部分逆向转换由弗洛斯曼引理定义。&lt;br /&gt;
&lt;br /&gt;
=== Behaviour under unions and products ===&lt;br /&gt;
&lt;br /&gt;
If &amp;lt;math&amp;gt;X=\bigcup_{i\in I}X_i&amp;lt;/math&amp;gt; is a finite or countable union, then&lt;br /&gt;
&lt;br /&gt;
If &amp;lt;math&amp;gt;X=\bigcup_{i\in I}X_i&amp;lt;/math&amp;gt; is a finite or countable union, then&lt;br /&gt;
&lt;br /&gt;
如果 &amp;lt;math&amp;gt;X=\bigcup_{i\in I}X_i&amp;lt;/math&amp;gt; 是一个有限或可数的联合，则&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \dim_{\operatorname{Haus}}(X) =\sup_{i\in I} \dim_{\operatorname{Haus}}(X_i).&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \dim_{\operatorname{Haus}}(X) =\sup_{i\in I} \dim_{\operatorname{Haus}}(X_i).&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
This can be verified directly from the definition.&lt;br /&gt;
&lt;br /&gt;
This can be verified directly from the definition.&lt;br /&gt;
&lt;br /&gt;
这可以直接从定义得到验证。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
If ''X'' and ''Y'' are non-empty metric spaces, then the Hausdorff dimension of their product satisfies&amp;lt;ref&amp;gt;{{cite journal |author=Marstrand, J. M. |title=The dimension of Cartesian product sets |journal=Proc. Cambridge Philos. Soc. |volume=50 |issue=3 |pages=198–202 |year=1954 |doi=10.1017/S0305004100029236 |bibcode = 1954PCPS...50..198M }}&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
If X and Y are non-empty metric spaces, then the Hausdorff dimension of their product satisfies&lt;br /&gt;
&lt;br /&gt;
如果 ''X'' 和''Y''是非空度量空间，那么它们乘积的豪斯多夫维数满足&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt; \dim_{\operatorname{Haus}}(X\times Y)\ge \dim_{\operatorname{Haus}}(X)+ \dim_{\operatorname{Haus}}(Y).&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \dim_{\operatorname{Haus}}(X\times Y)\ge \dim_{\operatorname{Haus}}(X)+ \dim_{\operatorname{Haus}}(Y).&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
This inequality can be strict. It is possible to find two sets of dimension 0 whose product has dimension 1.&amp;lt;ref&amp;gt;{{cite book  | last = Falconer  | first = Kenneth J.  | title = Fractal geometry. Mathematical foundations and applications  | publisher = John Wiley &amp;amp; Sons, Inc., Hoboken, New Jersey  | year = 2003  | doi =   | isbn = }}&amp;lt;/ref&amp;gt; In the opposite direction, it is known that when ''X'' and ''Y'' are Borel subsets of '''R'''&amp;lt;sup&amp;gt;''n''&amp;lt;/sup&amp;gt;, the Hausdorff dimension of ''X'' × ''Y'' is bounded from above by the Hausdorff dimension of ''X'' plus the [[packing dimension|upper packing dimension]] of ''Y''. These facts are discussed in Mattila (1995).&lt;br /&gt;
&lt;br /&gt;
This inequality can be strict. It is possible to find two sets of dimension 0 whose product has dimension 1. In the opposite direction, it is known that when X and Y are Borel subsets of R&amp;lt;sup&amp;gt;n&amp;lt;/sup&amp;gt;, the Hausdorff dimension of X × Y is bounded from above by the Hausdorff dimension of X plus the upper packing dimension of Y. These facts are discussed in Mattila (1995).&lt;br /&gt;
&lt;br /&gt;
这种不平等可以是绝对的。有可能找到两个维数为0的集合，其乘积的维数为1。相反，我们知道当''X''和''Y''是 '''R'''&amp;lt;sup&amp;gt;''n''&amp;lt;/sup&amp;gt;的 Borel 子集时， ''X'' × ''Y''的豪斯多夫维数从上面以 ''X''的豪斯多夫维数加上 ''Y''的填充维数为界。Mattila (1995)曾就这些情况进行了讨论。&lt;br /&gt;
&lt;br /&gt;
==Self-similar sets自相似集合==&lt;br /&gt;
&lt;br /&gt;
{{refimprove section|date=March 2015}}&lt;br /&gt;
&lt;br /&gt;
Many sets defined by a self-similarity condition have dimensions which can be determined explicitly. Roughly, a set ''E'' is self-similar if it is the fixed point of a set-valued transformation ψ, that is ψ(''E'') = ''E'', although the exact definition is given below.&lt;br /&gt;
&lt;br /&gt;
Many sets defined by a self-similarity condition have dimensions which can be determined explicitly. Roughly, a set E is self-similar if it is the fixed point of a set-valued transformation ψ, that is ψ(E) = E, although the exact definition is given below.&lt;br /&gt;
&lt;br /&gt;
许多由自相似条件定义的集合具有可以显式确定的维数。粗略地说，如果集合''E''是集值ψ变换的不动点，即ψ(''E'') = ''E''， 则它是自相似的，尽管下面给出了确切的定义。&lt;br /&gt;
&lt;br /&gt;
&amp;lt;blockquote&amp;gt;'''Theorem'''. Suppose&lt;br /&gt;
&lt;br /&gt;
&amp;lt;blockquote&amp;gt;Theorem. Suppose&lt;br /&gt;
&lt;br /&gt;
&amp;lt;blockquote&amp;gt;'''定理'''：假设&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt; \psi_i: \mathbf{R}^n \rightarrow \mathbf{R}^n, \quad i=1, \ldots , m &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \psi_i: \mathbf{R}^n \rightarrow \mathbf{R}^n, \quad i=1, \ldots , m &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
are [[Contraction mapping|contractive]] mappings on '''R'''&amp;lt;sup&amp;gt;''n''&amp;lt;/sup&amp;gt; with contraction constant ''r&amp;lt;sub&amp;gt;j&amp;lt;/sub&amp;gt;'' &amp;lt; 1. Then there is a unique ''non-empty'' compact set ''A'' such that&lt;br /&gt;
&lt;br /&gt;
are contractive mappings on R&amp;lt;sup&amp;gt;n&amp;lt;/sup&amp;gt; with contraction constant r&amp;lt;sub&amp;gt;j&amp;lt;/sub&amp;gt; &amp;lt; 1. Then there is a unique non-empty compact set A such that&lt;br /&gt;
&lt;br /&gt;
是'''R'''&amp;lt;sup&amp;gt;''n''&amp;lt;/sup&amp;gt;上的压缩常数''r&amp;lt;sub&amp;gt;j&amp;lt;/sub&amp;gt;'&amp;lt; 1的压缩映射。然后有一个唯一的非空紧集A &lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt; A = \bigcup_{i=1}^m \psi_i (A). &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; A = \bigcup_{i=1}^m \psi_i (A). &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&amp;lt;/blockquote&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;/blockquote&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The theorem follows from [[Stefan Banach]]'s [[Contractive mapping theorem|contractive mapping fixed point theorem]] applied to the complete metric space of non-empty compact subsets of '''R'''&amp;lt;sup&amp;gt;''n''&amp;lt;/sup&amp;gt; with the [[Hausdorff distance]].&amp;lt;ref&amp;gt;{{cite book |author=Falconer, K. J. |title=The Geometry of Fractal Sets |publisher=Cambridge University Press |location=Cambridge, UK |year=1985 |isbn=0-521-25694-1 |chapter=Theorem 8.3}}&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
The theorem follows from Stefan Banach's contractive mapping fixed point theorem applied to the complete metric space of non-empty compact subsets of R&amp;lt;sup&amp;gt;n&amp;lt;/sup&amp;gt; with the Hausdorff distance.&lt;br /&gt;
&lt;br /&gt;
这个定理来源于 Stefan Banach 的压缩映射不动点定理，该定理应用于 具有豪斯多夫距离的'''R'''&amp;lt;sup&amp;gt;''n''&amp;lt;/sup&amp;gt; 的非空紧子集的完整度量空间。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
===The open set condition开集条件===&lt;br /&gt;
&lt;br /&gt;
To determine the dimension of the self-similar set ''A'' (in certain cases), we need a technical condition called the ''open set condition'' (OSC) on the sequence of contractions ψ&amp;lt;sub&amp;gt;''i''&amp;lt;/sub&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
To determine the dimension of the self-similar set A (in certain cases), we need a technical condition called the open set condition (OSC) on the sequence of contractions ψ&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
为了确定自相似集''A'' 的维数(在某些情况下) ，我们需要一个关于收缩序列的称为''开集条件''(OSC)的技术条件ψ&amp;lt;sub&amp;gt;''i''&amp;lt;/sub&amp;gt;。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
There is a relatively compact open set ''V'' such that&lt;br /&gt;
&lt;br /&gt;
There is a relatively compact open set V such that&lt;br /&gt;
&lt;br /&gt;
有一个相对紧的开集''V''&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt; \bigcup_{i=1}^m\psi_i (V) \subseteq V, &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \bigcup_{i=1}^m\psi_i (V) \subseteq V, &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
where the sets in union on the left are pairwise [[disjoint sets|disjoint]].&lt;br /&gt;
&lt;br /&gt;
where the sets in union on the left are pairwise disjoint.&lt;br /&gt;
&lt;br /&gt;
左边并集的集合成对不相交。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The open set condition is a separation condition that ensures the images ψ&amp;lt;sub&amp;gt;''i''&amp;lt;/sub&amp;gt;(''V'') do not overlap &amp;quot;too much&amp;quot;.&lt;br /&gt;
&lt;br /&gt;
The open set condition is a separation condition that ensures the images ψ&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;(V) do not overlap &amp;quot;too much&amp;quot;.&lt;br /&gt;
&lt;br /&gt;
开集条件是保证图像ψ&amp;lt;sub&amp;gt;''i''&amp;lt;/sub&amp;gt;(''V'') 不重叠“太多”的分离条件。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
'''Theorem'''. Suppose the open set condition holds and each ψ&amp;lt;sub&amp;gt;''i''&amp;lt;/sub&amp;gt; is a similitude, that is a composition of an [[isometry]] and a [[dilation (metric space)|dilation]] around some point. Then the unique fixed point of ψ is a set whose Hausdorff dimension is ''s'' where ''s'' is the unique solution of&amp;lt;ref&amp;gt;{{cite journal | last=Hutchinson | first=John E. | title=Fractals and self similarity | journal=Indiana Univ. Math. J. | volume=30 | year=1981 | pages=713–747 | doi=10.1512/iumj.1981.30.30055 | issue=5 | doi-access=free }}&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
Theorem. Suppose the open set condition holds and each ψ&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt; is a similitude, that is a composition of an isometry and a dilation around some point. Then the unique fixed point of ψ is a set whose Hausdorff dimension is s where s is the unique solution of&lt;br /&gt;
&lt;br /&gt;
'''定理'''假设开集条件成立，并且每个ψ&amp;lt;sub&amp;gt;''i''&amp;lt;/sub&amp;gt; 是一个相似度，即等距和某个点周围的膨胀的组合。。那么唯一的不动点是Hausdorff维数为 ''s'' 的集合，其中  ''s'' 是 ''s'' &amp;lt;ref&amp;gt;{{cite journal | last=Hutchinson | first=John E. | title=Fractals and self similarity | journal=Indiana Univ. Math. J. | volume=30 | year=1981 | pages=713–747 | doi=10.1512/iumj.1981.30.30055 | issue=5 | doi-access=free }}&amp;lt;/ref&amp;gt;的唯一解&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt; \sum_{i=1}^m r_i^s = 1. &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \sum_{i=1}^m r_i^s = 1. &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The contraction coefficient of a similitude is the magnitude of the dilation.&lt;br /&gt;
&lt;br /&gt;
The contraction coefficient of a similitude is the magnitude of the dilation.&lt;br /&gt;
&lt;br /&gt;
相似物的收缩系数就是膨胀的大小。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
We can use this theorem to compute the Hausdorff dimension of the Sierpinski triangle (or sometimes called Sierpinski gasket). Consider three [[non-collinear points]] ''a''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;, ''a''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;, ''a''&amp;lt;sub&amp;gt;3&amp;lt;/sub&amp;gt; in the plane '''R'''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; and let ψ&amp;lt;sub&amp;gt;''i''&amp;lt;/sub&amp;gt; be the dilation of ratio 1/2 around ''a&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;''. The unique non-empty fixed point of the corresponding mapping ψ is a Sierpinski gasket and the dimension ''s'' is the unique solution of&lt;br /&gt;
&lt;br /&gt;
We can use this theorem to compute the Hausdorff dimension of the Sierpinski triangle (or sometimes called Sierpinski gasket). Consider three non-collinear points a&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;, a&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;, a&amp;lt;sub&amp;gt;3&amp;lt;/sub&amp;gt; in the plane R&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; and let ψ&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt; be the dilation of ratio 1/2 around a&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;. The unique non-empty fixed point of the corresponding mapping ψ is a Sierpinski gasket and the dimension s is the unique solution of&lt;br /&gt;
&lt;br /&gt;
我们可以使用这个定理来计算谢尔宾斯基三角形的豪斯多夫维数(或者有时候叫做谢尔宾斯基垫圈)。考虑R&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; 平面上的三个非共线点，''a''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;，''a''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;，''a''&amp;lt;sub&amp;gt;3&amp;lt;/sub&amp;gt;，让ψ&amp;lt;sub&amp;gt;''i''&amp;lt;/sub&amp;gt;是围绕着''a&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;''比率1/2的膨胀。对应映射的唯一非空不动点是一个谢尔宾斯基垫圈，其维数''s''是对应映射的唯一解&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt; \left(\frac{1}{2}\right)^s+\left(\frac{1}{2}\right)^s+\left(\frac{1}{2}\right)^s = 3 \left(\frac{1}{2}\right)^s =1. &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \left(\frac{1}{2}\right)^s+\left(\frac{1}{2}\right)^s+\left(\frac{1}{2}\right)^s = 3 \left(\frac{1}{2}\right)^s =1. &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Taking [[natural logarithm]]s of both sides of the above equation, we can solve for ''s'', that is: ''s'' = ln(3)/ln(2).  The Sierpinski gasket is self-similar and satisfies the OSC. In general a set ''E'' which is a fixed point of a mapping&lt;br /&gt;
&lt;br /&gt;
Taking natural logarithms of both sides of the above equation, we can solve for s, that is: s = ln(3)/ln(2).  The Sierpinski gasket is self-similar and satisfies the OSC. In general a set E which is a fixed point of a mapping&lt;br /&gt;
&lt;br /&gt;
取上述方程两边的自然对数，我们可以求出 ''s''，即: ''s'' = ln(3)/ln(2)。该密封垫具有自相似性，满足 OSC 要求。一般来说，集合 ''E''是一个映射的不动点&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt; A \mapsto \psi(A) = \bigcup_{i=1}^m \psi_i(A) &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt; A \mapsto \psi(A) = \bigcup_{i=1}^m \psi_i(A) &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
is self-similar if and only if the intersections&lt;br /&gt;
&lt;br /&gt;
is self-similar if and only if the intersections&lt;br /&gt;
&lt;br /&gt;
是自相似的，当且仅当&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt; H^s\left(\psi_i(E) \cap \psi_j(E)\right) =0, &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; H^s\left(\psi_i(E) \cap \psi_j(E)\right) =0, &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
where ''s'' is the Hausdorff dimension of ''E'' and ''H&amp;lt;sup&amp;gt;s&amp;lt;/sup&amp;gt;'' denotes [[Hausdorff measure]]. This is clear in the case of the Sierpinski gasket (the intersections are just points), but is also true more generally:&lt;br /&gt;
&lt;br /&gt;
where s is the Hausdorff dimension of E and H&amp;lt;sup&amp;gt;s&amp;lt;/sup&amp;gt; denotes Hausdorff measure. This is clear in the case of the Sierpinski gasket (the intersections are just points), but is also true more generally:&lt;br /&gt;
&lt;br /&gt;
其中 ''s''是''E''的豪斯多夫维数， ''H&amp;lt;sup&amp;gt;s&amp;lt;/sup&amp;gt;'' 表示 豪斯多夫测度。对于谢尔宾斯基垫圈(交叉点就是点)来说，这一点很明显，但更普遍的情况是:&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
'''Theorem'''. Under the same conditions as the previous theorem, the unique fixed point of ψ is self-similar.&lt;br /&gt;
&lt;br /&gt;
Theorem. Under the same conditions as the previous theorem, the unique fixed point of ψ is self-similar.&lt;br /&gt;
&lt;br /&gt;
'''定理'''：在与前一定理相同的条件下，其唯一不动点是自相似的。&lt;br /&gt;
&lt;br /&gt;
==See also参阅==&lt;br /&gt;
&lt;br /&gt;
* [[List of fractals by Hausdorff dimension豪斯多夫分形维数列表]] Examples of deterministic fractals, random and natural fractals.确定性分形与随机和自然分形的示例。&lt;br /&gt;
&lt;br /&gt;
* [[Assouad dimension  Assouad维数]], another variation of fractal dimension that, like Hausdorff dimension, is defined using coverings by balls其他被球覆盖方式定义的分形维数，例如豪斯多夫维数。&lt;br /&gt;
&lt;br /&gt;
* [[Intrinsic dimension固有维数]]&lt;br /&gt;
&lt;br /&gt;
* [[Packing dimension填充维数]]&lt;br /&gt;
&lt;br /&gt;
* [[Fractal dimension分形维数]]&lt;br /&gt;
&lt;br /&gt;
==References参考文献==&lt;br /&gt;
&lt;br /&gt;
{{reflist}}&lt;br /&gt;
&lt;br /&gt;
==Further reading拓展阅读==&lt;br /&gt;
&lt;br /&gt;
* {{cite book |last1=Dodson |first1=M. Maurice |title=Fractal Geometry and Applications: A Jubilee of Benoît Mandelbrot |volume=72 |issue=1 |pages=305–347 |last2=Kristensen |first2=Simon |chapter=Hausdorff Dimension and Diophantine Approximation |date=June 12, 2003 |arxiv=math/0305399 |bibcode = 2003math......5399D |doi=10.1090/pspum/072.1/2112110|series=Proceedings of Symposia in Pure Mathematics |isbn=9780821836378 }}&lt;br /&gt;
&lt;br /&gt;
* {{cite book |last1=Hurewicz |first1=Witold |authorlink1=Witold Hurewicz |last2=Wallman |first2=Henry |authorlink2=Henry Wallman |title=Dimension Theory |url=https://archive.org/details/in.ernet.dli.2015.84609 |publisher=Princeton University Press |year=1948 }}&lt;br /&gt;
&lt;br /&gt;
* {{cite journal |author作者=E. Szpilrajn |authorlink=Edward Marczewski |title=La dimension et la mesure |journal=Fundamenta Mathematicae |volume=28 |pages=81–9 |year=1937 }}&lt;br /&gt;
&lt;br /&gt;
* {{cite journal&lt;br /&gt;
&lt;br /&gt;
 | last1=Marstrand&lt;br /&gt;
&lt;br /&gt;
 | last1=Marstrand&lt;br /&gt;
&lt;br /&gt;
 | last1=马斯特兰德&lt;br /&gt;
&lt;br /&gt;
 | first1=J. M. | title=The dimension of cartesian product sets | year=1954 | journal=Proc. Cambridge Philos. Soc.&lt;br /&gt;
&lt;br /&gt;
 | first1=J. M. | title=The dimension of cartesian product sets | year=1954 | journal=Proc. Cambridge Philos. Soc.&lt;br /&gt;
&lt;br /&gt;
 | first1= J. M. | title=笛卡儿积集的维数 | 1954年 |  journal=Proc. Cambridge Philos. Soc.&lt;br /&gt;
&lt;br /&gt;
 | volume=50&lt;br /&gt;
&lt;br /&gt;
 | volume=50&lt;br /&gt;
&lt;br /&gt;
 | 第50卷&lt;br /&gt;
&lt;br /&gt;
 | issue=3&lt;br /&gt;
&lt;br /&gt;
 | issue=3&lt;br /&gt;
&lt;br /&gt;
 | 第三期&lt;br /&gt;
&lt;br /&gt;
 | pages=198–202&lt;br /&gt;
&lt;br /&gt;
 | pages=198–202&lt;br /&gt;
&lt;br /&gt;
 | 第198-202页&lt;br /&gt;
&lt;br /&gt;
 | doi=10.1017/S0305004100029236|bibcode = 1954PCPS...50..198M }}&lt;br /&gt;
&lt;br /&gt;
 | doi=10.1017/S0305004100029236|bibcode = 1954PCPS...50..198M }}&lt;br /&gt;
&lt;br /&gt;
10.1017 / S0305004100029236 | bibcode 1954PCPS... 50. . 198 m }&lt;br /&gt;
&lt;br /&gt;
* {{Cite book&lt;br /&gt;
&lt;br /&gt;
 | last1=Mattila&lt;br /&gt;
&lt;br /&gt;
 | last1=Mattila&lt;br /&gt;
&lt;br /&gt;
 | last1=Mattila&lt;br /&gt;
&lt;br /&gt;
 | first1=Pertti | author1-link=Pertti Mattila| title=Geometry of sets and measures in Euclidean spaces | publisher=[[Cambridge University Press]]&lt;br /&gt;
&lt;br /&gt;
 | first1=Pertti | author1-link=Pertti Mattila| title=Geometry of sets and measures in Euclidean spaces | publisher=Cambridge University Press&lt;br /&gt;
&lt;br /&gt;
| first1 Pertti | author1-link Pertti Mattila | title 欧几里德空间中集合和度量的几何 | 出版商剑桥大学出版社&lt;br /&gt;
&lt;br /&gt;
 | isbn=978-0-521-65595-8 | year=1995}}&lt;br /&gt;
&lt;br /&gt;
 | isbn=978-0-521-65595-8 | year=1995}}&lt;br /&gt;
&lt;br /&gt;
| isbn 978-0-521-65595-8 | year 1995}&lt;br /&gt;
&lt;br /&gt;
* {{cite journal |author=A. S. Besicovitch |authorlink=A. S. Besicovitch |title=On Linear Sets of Points of Fractional Dimensions |journal=[[Mathematische Annalen]] |volume=101 |year=1929 | doi=10.1007/BF01454831| issue=1 |pages= 161–193}}&lt;br /&gt;
&lt;br /&gt;
* {{cite journal |author1=A. S. Besicovitch |authorlink1=A. S. Besicovitch |author2=H. D. Ursell |authorlink2=H. D. Ursell |title=Sets of Fractional Dimensions |journal=Journal of the London Mathematical Society |volume=12 |year=1937 | issue=1 | doi=10.1112/jlms/s1-12.45.18  | pages=18–25 }}&amp;lt;br/&amp;gt;Several selections from this volume are reprinted in {{cite book |author=Edgar, Gerald A. |title=Classics on fractals |publisher=Addison-Wesley |location=Boston |year=1993 |isbn=0-201-58701-7}} See chapters 9,10,11&lt;br /&gt;
&lt;br /&gt;
* {{cite journal |author=F. Hausdorff |authorlink=F. Hausdorff |title=Dimension und äußeres Maß |journal=Mathematische Annalen |volume=79 |issue=1–2 |pages=157–179 |date=March 1919 |doi=10.1007/BF01457179|hdl=10338.dmlcz/100363 |url=http://dml.cz/bitstream/handle/10338.dmlcz/100363/CzechMathJ_09-1959-3_5.pdf }}&lt;br /&gt;
&lt;br /&gt;
* {{cite journal | last=Hutchinson | first=John E. | title=Fractals and self similarity | journal=Indiana Univ. Math. J. | volume=30 | year=1981 | pages=713–747 | doi=10.1512/iumj.1981.30.30055 | issue=5 | doi-access=free }}&lt;br /&gt;
&lt;br /&gt;
*{{cite book | last=Falconer | first = Kenneth |title=Fractal Geometry: Mathematical Foundations and Applications | publisher=[[John Wiley and Sons]] | edition=2nd | year=2003}}&lt;br /&gt;
&lt;br /&gt;
==External links外部链接==&lt;br /&gt;
&lt;br /&gt;
* [https://www.encyclopediaofmath.org/index.php/Hausdorff_dimension Hausdorff dimension] 在 [https://www.encyclopediaofmath.org/ Encyclopedia of Mathematics]&lt;br /&gt;
&lt;br /&gt;
* [https://www.encyclopediaofmath.org/index.php/Hausdorff_measure Hausdorff measure] 在 [https://www.encyclopediaofmath.org/ Encyclopedia of Mathematics]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{{DEFAULTSORT:Hausdorff Dimension豪斯多夫维数}}&lt;br /&gt;
&lt;br /&gt;
[[Category分类:Fractals分形]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[Category分类:Metric geometry度量几何]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[Category分类:Dimension theory维度理论]]&lt;br /&gt;
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&lt;br /&gt;
&lt;br /&gt;
&amp;lt;noinclude&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;small&amp;gt;This page was moved from [[wikipedia:en:Hausdorff dimension]]. Its edit history can be viewed at [[分形维数/edithistory]]&amp;lt;/small&amp;gt;&amp;lt;/noinclude&amp;gt;&lt;br /&gt;
&lt;br /&gt;
[[Category:待整理页面]]&lt;/div&gt;</summary>
		<author><name>Ruili</name></author>
	</entry>
	<entry>
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		<title>分形维数</title>
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		<updated>2020-11-01T17:17:15Z</updated>

		<summary type="html">&lt;p&gt;Ruili：&lt;/p&gt;
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&lt;div&gt;此词条暂由彩云小译翻译，未经人工整理和审校，带来阅读不便，请见谅。&lt;br /&gt;
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Example of non-integer dimensions. The first four [[iteration]]s of the [[Koch snowflake|Koch curve]], where after each iteration, all original line segments are replaced with four, each a self-similar copy that is 1/3 the length of the original. One formalism of the Hausdorff dimension uses this scale factor (3) and the number of self-similar objects (4) to calculate the dimension, D, after the first iteration to be D = (log N)/(log S) = (log 4)/(log 3) ≈ 1.26.&amp;lt;ref name=CampbellAnnenberg15&amp;gt;MacGregor Campbell, 2013, &amp;quot;5.6 Scaling and the Hausdorff Dimension,&amp;quot; at ''Annenberg Learner:MATHematics illuminated'', see [http://www.learner.org/courses/mathilluminated/units/5/textbook/06.php], accessed 5 March 2015.&amp;lt;/ref&amp;gt; That is, while the Hausdorff dimension of a single [[point (geometry)|point]] is zero, of a [[line segment]] is 1, of a [[square]] is 2, and of a [[cube]] is 3, for [[fractal]]s such as this, the object can have a non-integer dimension.&lt;br /&gt;
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Example of non-integer dimensions. The first four iterations of the Koch curve, where after each iteration, all original line segments are replaced with four, each a self-similar copy that is 1/3 the length of the original. One formalism of the Hausdorff dimension uses this scale factor (3) and the number of self-similar objects (4) to calculate the dimension, D, after the first iteration to be D = (log N)/(log S) = (log 4)/(log 3) ≈ 1.26. That is, while the Hausdorff dimension of a single point is zero, of a line segment is 1, of a square is 2, and of a cube is 3, for fractals such as this, the object can have a non-integer dimension.&lt;br /&gt;
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非整数维度示例：前四个[[Koch 曲线]]的迭代，在每次迭代后，所有原始线段都被替换为四个，每个自相似的复制是原始线段长度的1 / 3。豪斯多夫维数的一个建模是使用比例因子(3)和自相似对象的数量(4)来计算维度 D，在第一次迭代后为 D = (log N)/(log S) = (log 4)/(log 3) ≈ 1.26.&amp;lt;ref name=CampbellAnnenberg15&amp;gt;。MacGregor Campbell, 2013, &amp;quot;5.6 Scaling and the Hausdorff Dimension,&amp;quot; 在 ''Annenberg Learner:MATHematics illuminated'', 参见 [http://www.learner.org/courses/mathilluminated/units/5/textbook/06.php], accessed 5 March 2015.&amp;lt;/ref&amp;gt; 也就是说，单点的豪斯多夫维数为零，线段为1，正方形为2，立方体为3时，但对于分形，对象可以有一个非整数维度。&lt;br /&gt;
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In [[mathematics]], '''Hausdorff dimension''' is a measure of ''roughness'', or more specifically, [[fractal dimension]], that was first introduced in 1918 by [[mathematician]] [[Felix Hausdorff]].&amp;lt;ref&amp;gt;{{Cite journal |arxiv = 1101.1444|doi = 10.1214/11-STS370|title = Estimators of Fractal Dimension: Assessing the Roughness of Time Series and Spatial Data|journal = Statistical Science|volume = 27|issue = 2|pages = 247–277|year = 2012|last1 = Gneiting|first1 = Tilmann|last2 = Ševčíková|first2 = Hana|last3 = Percival|first3 = Donald B.}}&amp;lt;/ref&amp;gt; For instance, the Hausdorff dimension of a single [[point (geometry)|point]] is zero, of a [[line segment]] is 1, of a [[square]] is 2, and of a [[cube]] is 3. That is, for sets of points that define a smooth shape or a shape that has a small number of corners—the shapes of traditional geometry and science—the Hausdorff dimension is an [[integer]] agreeing with the usual sense of dimension, also known as the [[Inductive dimension|topological dimension]]. However, formulas have also been developed that allow calculation of the dimension of other less simple objects, where, solely on the basis of their properties of [[scaling (geometry)|scaling]] and [[self-similarity]], one is led to the conclusion that particular objects—including [[fractal]]s—have non-integer Hausdorff dimensions. Because of the significant technical advances made by [[Abram Samoilovitch Besicovitch]] allowing computation of dimensions for highly irregular or &amp;quot;rough&amp;quot; sets, this dimension is also commonly referred to as the ''Hausdorff–Besicovitch dimension.''&lt;br /&gt;
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In mathematics, Hausdorff dimension is a measure of roughness, or more specifically, fractal dimension, that was first introduced in 1918 by mathematician Felix Hausdorff. For instance, the Hausdorff dimension of a single point is zero, of a line segment is 1, of a square is 2, and of a cube is 3. That is, for sets of points that define a smooth shape or a shape that has a small number of corners—the shapes of traditional geometry and science—the Hausdorff dimension is an integer agreeing with the usual sense of dimension, also known as the topological dimension. However, formulas have also been developed that allow calculation of the dimension of other less simple objects, where, solely on the basis of their properties of scaling and self-similarity, one is led to the conclusion that particular objects—including fractals—have non-integer Hausdorff dimensions. Because of the significant technical advances made by Abram Samoilovitch Besicovitch allowing computation of dimensions for highly irregular or &amp;quot;rough&amp;quot; sets, this dimension is also commonly referred to as the Hausdorff–Besicovitch dimension.&lt;br /&gt;
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在[[数学]]中，'''&amp;lt;font color = '#ff8000'&amp;gt;豪斯多夫维数Hausdorff dimension&amp;lt;/font&amp;gt;'''是一种粗糙度的度量单位，或者更确切地说，分形维数，是由数学家 Felix Hausdorff 在1918年首次提出的。例如，单点的豪斯多夫维数为零，线段为1，正方形为2，立方体为3。也就是说，对于定义了一个光滑形状或一个有少数几个角的形状---- 传统几何学和科学的形状---- 的点集来说，豪斯多夫维数是一个整数，符合通常的维度意义，也称为拓扑维度。然而，还有一些公式允许计算其他不太简单的对象的维数，其中仅仅根据它们的标度和自相似特性，就可以得出结论: 特定的对象ー包括分形ー具有非整数的 Hausdorff 维数。由于阿布拉姆·萨莫伊洛维奇·贝西科维奇的重大技术进步，允许计算高度不规则或“粗糙”集的维度，这个维度通常也被称为 Hausdorff-Besicovitch 维度。 &lt;br /&gt;
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The Hausdorff dimension, more specifically, is a further dimensional number associated with a given set, where the distances between all members of that set are defined. Such a set is termed a [[metric space]]. The dimension is drawn from the [[Extended real number line|extended real numbers]], &amp;lt;math&amp;gt;\overline{\mathbb{R}}&amp;lt;/math&amp;gt;, as opposed to the more intuitive notion of dimension, which is not associated to general metric spaces, and only takes values in the non-negative integers.&lt;br /&gt;
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The Hausdorff dimension, more specifically, is a further dimensional number associated with a given set, where the distances between all members of that set are defined. Such a set is termed a metric space. The dimension is drawn from the extended real numbers, &amp;lt;math&amp;gt;\overline{\mathbb{R}}&amp;lt;/math&amp;gt;, as opposed to the more intuitive notion of dimension, which is not associated to general metric spaces, and only takes values in the non-negative integers.&lt;br /&gt;
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更具体地说，豪斯多夫维数是一个与给定集合相关联的更进一步的维数，其中定义了该集合所有成员之间的距离。这样的集合称为度量空间。维数是从扩展的实数，&amp;lt;math&amp;gt;\overline{\mathbb{R}}&amp;lt;/math&amp;gt;，而不是更直观的维数概念(它不与一般的度量空间相关联，只取非负整数的值)。&lt;br /&gt;
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In mathematical terms, the Hausdorff dimension generalizes the notion of the dimension of a real [[vector space]]. That is, the Hausdorff dimension of an ''n''-dimensional [[inner product space]] equals ''n''. This underlies the earlier statement that the Hausdorff dimension of a point is zero, of a line is one, etc., and that [[fractal|irregular sets]] can have noninteger Hausdorff dimensions. For instance, the [[Koch snowflake]] shown at right is constructed from an equilateral triangle; in each iteration, its component line segments are divided into 3 segments of unit length, the newly created middle segment is used as the base of a new [[equilateral]] triangle that points outward, and this base segment is then deleted to leave a final object from the iteration of unit length of 4.&amp;lt;ref&amp;gt;Larry Riddle, 2014, &amp;quot;Classic Iterated Function Systems: Koch Snowflake&amp;quot;, Agnes Scott College e-Academy (online), see [http://ecademy.agnesscott.edu/~lriddle/ifs/ksnow/ksnow.htm], accessed 5 March 2015.&amp;lt;/ref&amp;gt; That is, after the first iteration, each original line segment has been replaced with N=4, where each self-similar copy is 1/S = 1/3 as long as the original.&amp;lt;ref name=CampbellAnnenberg15/&amp;gt; Stated another way, we have taken an object with Euclidean dimension, D, and reduced its linear scale by 1/3 in each direction, so that its length increases to N=S&amp;lt;sup&amp;gt;D&amp;lt;/sup&amp;gt;.&amp;lt;ref name=ClaytonSCTPLS96&amp;gt;Keith Clayton, 1996, &amp;quot;Fractals and the Fractal Dimension,&amp;quot; ''Basic Concepts in Nonlinear Dynamics and Chaos'' (workshop), Society for Chaos Theory in Psychology and the Life Sciences annual meeting, June 28, 1996, Berkeley, California, see [http://www.vanderbilt.edu/AnS/psychology/cogsci/chaos/workshop/Workshop.html], accessed 5 March 2015.&amp;lt;/ref&amp;gt; This equation is easily solved for D, yielding the ratio of logarithms (or [[natural logarithm]]s) appearing in the figures, and giving—in the Koch and other fractal cases—non-integer dimensions for these objects.&lt;br /&gt;
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In mathematical terms, the Hausdorff dimension generalizes the notion of the dimension of a real vector space. That is, the Hausdorff dimension of an n-dimensional inner product space equals n. This underlies the earlier statement that the Hausdorff dimension of a point is zero, of a line is one, etc., and that irregular sets can have noninteger Hausdorff dimensions. For instance, the Koch snowflake shown at right is constructed from an equilateral triangle; in each iteration, its component line segments are divided into 3 segments of unit length, the newly created middle segment is used as the base of a new equilateral triangle that points outward, and this base segment is then deleted to leave a final object from the iteration of unit length of 4. That is, after the first iteration, each original line segment has been replaced with N=4, where each self-similar copy is 1/S = 1/3 as long as the original. This equation is easily solved for D, yielding the ratio of logarithms (or natural logarithms) appearing in the figures, and giving—in the Koch and other fractal cases—non-integer dimensions for these objects.&lt;br /&gt;
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用数学术语来说，豪斯多夫维数概括了实向量空间维数的概念。也就是说，n 维内积空间的豪斯多夫维数等于 n。 这就是早期假设的基础，一个点的豪斯多夫维数是零，一条线是一等等，不规则集可以有非整数的豪斯多夫维数。例如，右边所示的 Koch 雪花是由一个正三角形构成的; 在每次迭代中，它的组成线段被分成单位长度的3段，新创建的中间线段被用作一个指向外部的新正三角形的基础，然后人们删除这个基础线段用来保留单位长度4的迭代中的最终对象。也就是说，在第一次迭代之后，每个原始线段都被替换为 N=4，其中每个自相似拷贝的长度是原始线段的1/S = 1/3 。这个方程很容易求解为 D，产生出现在图形中的对数(或自然对数)的比率，并给出——在 Koch 和其他分形情况下——这些对象的非整数维数。&lt;br /&gt;
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The Hausdorff dimension is a successor to the simpler, but usually equivalent, box-counting or [[Minkowski–Bouligand dimension]].&lt;br /&gt;
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The Hausdorff dimension is a successor to the simpler, but usually equivalent, box-counting or Minkowski–Bouligand dimension.&lt;br /&gt;
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豪斯多夫维数是更简单但通常等价的'''&amp;lt;font color = '#ff8000'&amp;gt;计盒维数box-counting&amp;lt;/font&amp;gt;'''或'''&amp;lt;font color = '#ff8000'&amp;gt;闵可夫斯基维数Minkowski-Bouligand&amp;lt;/font&amp;gt;'''的继承者。&lt;br /&gt;
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==Intuition概念==&lt;br /&gt;
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The intuitive concept of dimension of a geometric object ''X'' is the number of independent parameters one needs to pick out a unique point inside. However, any point specified by two parameters can be instead specified by one, because the [[cardinality]] of the [[real plane]] is equal to the cardinality of the [[real line]] (this can be seen by an [[Cantor's diagonal argument|argument]] involving interweaving the digits of two numbers to yield a single number encoding the same information). The example of a [[space-filling curve]] shows that one can even map the real line to the real plane [[Surjective function|surjectively]] (taking one real number into a pair of real numbers in a way so that all pairs of numbers are covered) and ''continuously'', so that a one-dimensional object completely fills up a higher-dimensional object.&lt;br /&gt;
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The intuitive concept of dimension of a geometric object X is the number of independent parameters one needs to pick out a unique point inside. However, any point specified by two parameters can be instead specified by one, because the cardinality of the real plane is equal to the cardinality of the real line (this can be seen by an argument involving interweaving the digits of two numbers to yield a single number encoding the same information). The example of a space-filling curve shows that one can even map the real line to the real plane surjectively (taking one real number into a pair of real numbers in a way so that all pairs of numbers are covered) and continuously, so that a one-dimensional object completely fills up a higher-dimensional object.&lt;br /&gt;
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几何对象X的尺寸的直观概念是指需要多少个独立参数才能找到一个独特的点。但是，任何由两个参数指定的点都可以由一个参数指定，因为为实平面的基数等于实线的基数(这可以通过交织两个数字以产生一个编码相同信息的单个数字看到)。'''&amp;lt;font color = '#ff8000'&amp;gt;皮亚诺曲线&amp;lt;/font&amp;gt;'''的例子表明，可以将实线完美和连续地映射到实平面(把一个实数转换成一对实数，从而覆盖所有实数对)，由此一维对象完全填充了一个高维对象。&lt;br /&gt;
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Every space filling curve hits some points multiple times, and does not have a continuous inverse. It is impossible to map two dimensions onto one in a way that is continuous and continuously invertible. The topological dimension, also called [[Lebesgue covering dimension]], explains why. This dimension is ''n'' if, in every covering of ''X'' by small open balls, there is at least one point where ''n''&amp;amp;nbsp;+&amp;amp;nbsp;1 balls overlap. For example, when one covers a line with short open intervals, some points must be covered twice, giving dimension&amp;amp;nbsp;''n''&amp;amp;nbsp;=&amp;amp;nbsp;1.&lt;br /&gt;
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Every space filling curve hits some points multiple times, and does not have a continuous inverse. It is impossible to map two dimensions onto one in a way that is continuous and continuously invertible. The topological dimension, also called Lebesgue covering dimension, explains why. This dimension is n if, in every covering of X by small open balls, there is at least one point where n&amp;amp;nbsp;+&amp;amp;nbsp;1 balls overlap. For example, when one covers a line with short open intervals, some points must be covered twice, giving dimension&amp;amp;nbsp;n&amp;amp;nbsp;=&amp;amp;nbsp;1.&lt;br /&gt;
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每条空间填充曲线都会多次击中某些点，且不存在连续的逆。将二维以连续和连续可逆的方式映射到一维是不可能的。'''&amp;lt;font color = '#ff8000'&amp;gt;拓扑维度 topological dimension&amp;lt;/font&amp;gt;'''，也被称为Lebesgue覆盖维数，解释了为什么。如果在 x 的每个小开球覆盖中，至少有一个点 n + 1个球重叠，这个维度是 n。例如，当用短的开区间覆盖一条线时，某些点必须被覆盖两次，给出维数''n''&amp;amp;nbsp;=&amp;amp;nbsp;1。&lt;br /&gt;
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But topological dimension is a very crude measure of the local size of a space (size near a point). A curve that is almost space-filling can still have topological dimension one, even if it fills up most of the area of a region. A [[fractal]] has an integer topological dimension, but in terms of the amount of space it takes up, it behaves like a higher-dimensional space.&lt;br /&gt;
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But topological dimension is a very crude measure of the local size of a space (size near a point). A curve that is almost space-filling can still have topological dimension one, even if it fills up most of the area of a region. A fractal has an integer topological dimension, but in terms of the amount of space it takes up, it behaves like a higher-dimensional space.&lt;br /&gt;
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但是，拓扑维度是对空间局部尺寸(点附近的尺寸)的一个非常粗略的度量。一条几乎是空间填充的曲线仍然可以有一维拓扑，即使它填充了一个区域的大部分面积。分形具有整数的拓扑维数，但就其所占的空间量而言，它看起来像一个更高维的空间。&lt;br /&gt;
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The Hausdorff dimension measures the local size of a space taking into account the distance between points, the [[metric space|metric]]. Consider the number ''N''(''r'') of [[ball (mathematics)|balls]] of radius at most ''r'' required to cover ''X'' completely. When ''r'' is very small, ''N''(''r'') grows polynomially with 1/''r''. For a sufficiently well-behaved  ''X'', the Hausdorff dimension is the unique number ''d'' such that N(''r'') grows as 1/''r&amp;lt;sup&amp;gt;d&amp;lt;/sup&amp;gt;'' as ''r'' approaches zero. More precisely, this defines the [[Minkowski–Bouligand dimension|box-counting dimension]], which equals the Hausdorff dimension when the value ''d'' is a critical boundary between growth rates that are insufficient to cover the space, and growth rates that are overabundant.&lt;br /&gt;
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The Hausdorff dimension measures the local size of a space taking into account the distance between points, the metric. Consider the number N(r) of balls of radius at most r required to cover X completely. When r is very small, N(r) grows polynomially with 1/r. For a sufficiently well-behaved  X, the Hausdorff dimension is the unique number d such that N(r) grows as 1/r&amp;lt;sup&amp;gt;d&amp;lt;/sup&amp;gt; as r approaches zero. More precisely, this defines the box-counting dimension, which equals the Hausdorff dimension when the value d is a critical boundary between growth rates that are insufficient to cover the space, and growth rates that are overabundant.&lt;br /&gt;
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豪斯多夫维数测量一个空间的局部大小时，会考虑到点之间距离的度量。考虑半径最大为 r 的球数 ''N'' (r) ，需要完全覆盖 ''X''。当 r 很小时，n (r)以1/''r'' 增长多项式。对于一个表现足够好的 ''X''，豪斯多夫维数是唯一的数 d，这样当 r 趋近于零时， N(r)增长为1/r&amp;lt;sup&amp;gt;d&amp;lt;/sup&amp;gt; 。更确切地说，这定义了盒子计数维度，当值 d 是不足以覆盖空间的增长率和过度充裕的增长率之间的关键边界时，它等于豪斯多夫维数。&lt;br /&gt;
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For shapes that are smooth, or shapes with a small number of corners, the shapes of traditional geometry and science, the Hausdorff dimension is an integer agreeing with the topological dimension. But [[Benoit Mandelbrot]] observed that [[fractal]]s, sets with noninteger Hausdorff dimensions, are found everywhere in nature. He observed that the proper idealization of most rough shapes you see around you is not in terms of smooth idealized shapes, but in terms of fractal idealized shapes:&lt;br /&gt;
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For shapes that are smooth, or shapes with a small number of corners, the shapes of traditional geometry and science, the Hausdorff dimension is an integer agreeing with the topological dimension. But Benoit Mandelbrot observed that fractals, sets with noninteger Hausdorff dimensions, are found everywhere in nature. He observed that the proper idealization of most rough shapes you see around you is not in terms of smooth idealized shapes, but in terms of fractal idealized shapes:&lt;br /&gt;
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对于光滑的形状，或者有少量棱角的形状，传统几何和科学的形状，豪斯多夫维数是一个整数，与拓扑维度一致。但是伯努·曼德布洛特观察到分形---- 具有非整数豪斯多夫维数的集合---- 在自然界中随处可见。他观察到，我们周围大多数粗糙形状的理想化不是光滑的理想化形状，而是分形理想化形状:&lt;br /&gt;
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&amp;lt;blockquote&amp;gt;Clouds are not spheres, mountains are not cones, coastlines are not circles, and bark is not smooth, nor does lightning travel in a straight line.&amp;lt;ref name=&amp;quot;mandelbrot&amp;quot;&amp;gt;{{cite book   | last = Mandelbrot   | first = Benoît   | authorlink = Benoit Mandelbrot   | title = The Fractal Geometry of Nature   | publisher = W. H. Freeman   | series = Lecture notes in mathematics 1358   | year = 1982   | doi =    | isbn = 0-7167-1186-9   | url-access = registration   | url = https://archive.org/details/fractalgeometryo00beno   }}&amp;lt;/ref&amp;gt;&amp;lt;/blockquote&amp;gt;&lt;br /&gt;
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&amp;lt;blockquote&amp;gt;Clouds are not spheres, mountains are not cones, coastlines are not circles, and bark is not smooth, nor does lightning travel in a straight line.&amp;lt;/blockquote&amp;gt;&lt;br /&gt;
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&amp;lt;blockquote&amp;gt;云不是球体，山不是锥体，海岸线不是圆圈，树皮不平滑，闪电也不是直线运动。 &amp;lt;/blockquote&amp;gt;&lt;br /&gt;
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For fractals that occur in nature, the Hausdorff and [[Minkowski–Bouligand dimension|box-counting dimension]] coincide. The [[packing dimension]] is yet another similar notion which gives the same value for many shapes, but there are well documented exceptions where all these dimensions differ.&lt;br /&gt;
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For fractals that occur in nature, the Hausdorff and box-counting dimension coincide. The packing dimension is yet another similar notion which gives the same value for many shapes, but there are well documented exceptions where all these dimensions differ.&lt;br /&gt;
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对于自然界中出现的分形，豪斯多夫维数和盒计数维数是一致的。封装尺寸是另一个类似的概念，它给出了许多形状相同的值，但是在所有这些尺寸不同的情况，都做了很好的说明。&lt;br /&gt;
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==Formal definitions形式化定义==&lt;br /&gt;
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===Hausdorff content豪斯多夫集===&lt;br /&gt;
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Let ''X'' be a [[metric space]]. If ''S'' ⊂ ''X'' and ''d'' ∈ [0, ∞), the ''d''-dimensional '''unlimited Hausdorff content''' of ''S'' is defined by&lt;br /&gt;
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Let X be a metric space. If S ⊂ X and d ∈ [0, ∞), the d-dimensional unlimited Hausdorff content of S is defined by&lt;br /&gt;
&lt;br /&gt;
设 ''X''是度量空间。若''S'' ⊂ ''X'' 和 ''d'' ∈ [0, ∞) ，则 ''S'' 的''d''维无限 豪斯多夫集定义为&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt;C_H^d(S):=\inf\Bigl\{\sum_i r_i^d:\text{ there is a cover of } S\text{ by balls with radii }r_i&amp;gt;0\Bigr\}.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt;C_H^d(S):=\inf\Bigl\{\sum_i r_i^d:\text{ there is a cover of } S\text{ by balls with radii }r_i&amp;gt;0\Bigr\}.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt;C_H^d(S):=\inf\Bigl\{\sum_i r_i^d:\text{ there is a cover of } S\text{ by balls with radii }r_i&amp;gt;0\Bigr\}.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
In other words, &amp;lt;math&amp;gt;C_H^d(S)&amp;lt;/math&amp;gt; is the [[infimum]] of the set of numbers &amp;lt;math&amp;gt;\delta \geq 0&amp;lt;/math&amp;gt; such that there is some (indexed) collection of [[ball (mathematics)|ball]]s &amp;lt;math&amp;gt;\{B(x_i,r_i):i\in I\}&amp;lt;/math&amp;gt; covering ''S'' with ''r&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;''&amp;amp;nbsp;&amp;gt;&amp;amp;nbsp;0 for each ''i''&amp;amp;nbsp;∈&amp;amp;nbsp;''I'' that satisfies &amp;lt;math&amp;gt;\sum_{i\in I} r_i^d&amp;lt;\delta &amp;lt;/math&amp;gt;. (Here, we use the standard convention that [[infimum|inf&amp;amp;nbsp;Ø&amp;amp;nbsp;=&amp;amp;nbsp;∞]].)&lt;br /&gt;
&lt;br /&gt;
In other words, &amp;lt;math&amp;gt;C_H^d(S)&amp;lt;/math&amp;gt; is the infimum of the set of numbers &amp;lt;math&amp;gt;\delta \geq 0&amp;lt;/math&amp;gt; such that there is some (indexed) collection of balls &amp;lt;math&amp;gt;\{B(x_i,r_i):i\in I\}&amp;lt;/math&amp;gt; covering S with r&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;&amp;amp;nbsp;&amp;gt;&amp;amp;nbsp;0 for each i&amp;amp;nbsp;∈&amp;amp;nbsp;I that satisfies &amp;lt;math&amp;gt;\sum_{i\in I} r_i^d&amp;lt;\delta &amp;lt;/math&amp;gt;. (Here, we use the standard convention that inf&amp;amp;nbsp;Ø&amp;amp;nbsp;=&amp;amp;nbsp;∞.)&lt;br /&gt;
&lt;br /&gt;
换句话说，&amp;lt;math&amp;gt;C_H^d(S)&amp;lt;/math&amp;gt; 是数字集合&amp;lt;math&amp;gt;\delta \geq 0&amp;lt;/math&amp;gt;的下确界，使得在 ''i''&amp;amp;nbsp;∈&amp;amp;nbsp中存在一些球集合 &amp;lt;math&amp;gt;\{B(x_i,r_i):i\in I\}&amp;lt;/math&amp;gt;  i 包含 s，对于每个 ''r&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;''&amp;amp;nbsp;&amp;gt;&amp;amp;nbsp;0 满足 i 中的和&amp;lt;math&amp;gt;\sum_{i\in I} r_i^d&amp;lt;\delta &amp;lt;/math&amp;gt; (在这里，我们使用inf&amp;amp;nbsp;Ø&amp;amp;nbsp;=&amp;amp;nbsp;∞ )的标准约定。&lt;br /&gt;
&lt;br /&gt;
===Hausdorff measurement豪斯多夫分形测量===&lt;br /&gt;
&lt;br /&gt;
The Hausdorff outer measure is different from the unbounded Hausdorf content in that rather than considering all possible coverings of ''S'', we see what happens when the sizes of the balls go to zero. This is  for &amp;lt;math&amp;gt;d \geq 0 &amp;lt;/math&amp;gt;, we define the ''d''-dimensional Hausdorff outer measure of ''S'' as&lt;br /&gt;
&lt;br /&gt;
The Hausdorff outer measure is different from the unbounded Hausdorf content in that rather than considering all possible coverings of S, we see what happens when the sizes of the balls go to zero. This is  for &amp;lt;math&amp;gt;d \geq 0 &amp;lt;/math&amp;gt;, we define the d-dimensional Hausdorff outer measure of S as&lt;br /&gt;
&lt;br /&gt;
豪斯多夫外测度不同于无界的豪斯多夫，因为我们不考虑 s 的所有可能，我们看到当球的大小为零时会发生什么。这是为了数学  &amp;lt;math&amp;gt;d \geq 0 &amp;lt;/math&amp;gt;，我们定义了  ''S''的 ''d''维豪斯多夫Hausdorff 外测度为&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt; \mathcal{H}^d(S):=\lim_{r \to 0} \inf\Bigl\{\sum_i r_i^d:\text{ there is a cover of } S\text{ by balls with radii } 0 &amp;lt; r_i &amp;lt; r\Bigr\}.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \mathcal{H}^d(S):=\lim_{r \to 0} \inf\Bigl\{\sum_i r_i^d:\text{ there is a cover of } S\text{ by balls with radii } 0 &amp;lt; r_i &amp;lt; r\Bigr\}.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \mathcal{H}^d(S):=\lim_{r \to 0} \inf\Bigl\{\sum_i r_i^d:\text{有一个面} S\text{ 球 } 0 &amp;lt; r_i &amp;lt; r\Bigr\}.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
===Hausdorff dimension豪斯多夫维数===&lt;br /&gt;
&lt;br /&gt;
The '''Hausdorff dimension''' of ''X'' is defined by&lt;br /&gt;
&lt;br /&gt;
The Hausdorff dimension of X is defined by&lt;br /&gt;
&lt;br /&gt;
X 的豪斯多夫维数定义为&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt;\dim_{\operatorname{H}}(X):=\inf\{d\ge 0: \mathcal{H}^d(X)=0\}.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt;\dim_{\operatorname{H}}(X):=\inf\{d\ge 0: \mathcal{H}^d(X)=0\}.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Equivalently, dim&amp;lt;sub&amp;gt;H&amp;lt;/sub&amp;gt;(''X'') may be defined as the [[infimum]] of the set of ''d'' ∈ [0, ∞) such that the ''d''-dimensional [[Hausdorff measure]] of ''X'' is zero. This is the same as the supremum of the set of ''d''&amp;amp;nbsp;∈&amp;amp;nbsp;[0,&amp;amp;nbsp;∞) such that the ''d''-dimensional Hausdorff measure of ''X'' is infinite (except that when this latter set of numbers ''d'' is empty the Hausdorff dimension is zero).&lt;br /&gt;
&lt;br /&gt;
Equivalently, dim&amp;lt;sub&amp;gt;H&amp;lt;/sub&amp;gt;(X) may be defined as the infimum of the set of d ∈ [0, ∞) such that the d-dimensional Hausdorff measure of X is zero. This is the same as the supremum of the set of d&amp;amp;nbsp;∈&amp;amp;nbsp;[0,&amp;amp;nbsp;∞) such that the d-dimensional Hausdorff measure of X is infinite (except that when this latter set of numbers d is empty the Hausdorff dimension is zero).&lt;br /&gt;
&lt;br /&gt;
等价地，dim &amp;lt;sub&amp;gt;H&amp;lt;/sub&amp;gt;(''X'')可定义为 ''d'' ∈ [0, ∞) 集的下确界，使得''X'' 的''d''-维 [[豪斯多夫测度]] 为零。这与 ''d''&amp;amp;nbsp;∈&amp;amp;nbsp;[0,&amp;amp;nbsp;∞)的集合的上确界相同，因此''X''的 d 维豪斯多夫测度是无限的(除非后一个集合 ''d'' 是空的，豪斯多夫维数为零)。&lt;br /&gt;
&lt;br /&gt;
==Examples实例==&lt;br /&gt;
&lt;br /&gt;
[[Image:Sierpinski deep.svg|thumb|250px|Dimension of a further [[fractal]] example. The [[Sierpinski triangle]], an object with Hausdorff dimension of log(3)/log(2)≈1.58.&amp;lt;ref name=ClaytonSCTPLS96/&amp;gt;]]&lt;br /&gt;
&lt;br /&gt;
Dimension of a further [[fractal example. The Sierpinski triangle, an object with Hausdorff dimension of log(3)/log(2)≈1.58.]]&lt;br /&gt;
&lt;br /&gt;
[[Image:谢尔宾斯基三角形 deep.svg|thumb|250px|进一步的[[分形维数]]的例子，进一步的分形维数的例子是谢尔宾斯基三角形，它是一个豪斯多夫维数为log(3)/log(2)≈1.58.&amp;lt;ref name=ClaytonSCTPLS96/&amp;gt;的物体]]&lt;br /&gt;
&lt;br /&gt;
* [[Countable set]]s have Hausdorff dimension 0.&amp;lt;ref name=&amp;quot;schleicher&amp;quot;&amp;gt;{{cite journal |last1=Schleicher |first1=Dierk |title=Hausdorff Dimension, Its Properties, and Its Surprises |journal=The American Mathematical Monthly |date=June 2007 |volume=114 |issue=6 |pages=509–528 |doi=10.1080/00029890.2007.11920440 |language=en |issn=0002-9890|arxiv=math/0505099 }}&amp;lt;/ref&amp;gt;&lt;br /&gt;
*[[可数集]]拥有豪斯多夫维数0.&amp;lt;ref name=&amp;quot;schleicher&amp;quot;&amp;gt;{{cite journal |last1=Schleicher |first1=Dierk |title=豪斯多夫维数, Its Properties, and Its Surprises |journal=The American Mathematical Monthly美国数学期刊 |date=June 2007 |volume=114 |issue=6 |pages=509–528 |doi=10.1080/00029890.2007.11920440 |language=en |issn=0002-9890|arxiv=math/0505099 }}&amp;lt;/ref&amp;gt;&lt;br /&gt;
* The [[Euclidean space]] ℝ&amp;lt;sup&amp;gt;''n''&amp;lt;/sup&amp;gt; has Hausdorff dimension ''n'', and the circle '''S'''&amp;lt;sup&amp;gt;1&amp;lt;/sup&amp;gt; has Hausdorff dimension 1.&amp;lt;ref name=&amp;quot;schleicher&amp;quot; /&amp;gt;&lt;br /&gt;
*[[教育空间]] ℝ&amp;lt;sup&amp;gt;''n''&amp;lt;/sup&amp;gt; 有豪斯多夫维数 ''n''，循环'''S'''&amp;lt;sup&amp;gt;1&amp;lt;/sup&amp;gt; 拥有豪斯多夫维数1.&amp;lt;ref name=&amp;quot;schleicher&amp;quot; /&amp;gt;&lt;br /&gt;
* [[Fractal]]s often are spaces whose Hausdorff dimension strictly exceeds the [[topological dimension]].&amp;lt;ref name=&amp;quot;mandelbrot&amp;quot; /&amp;gt; For example, the [[Cantor set]], a zero-dimensional topological space, is a union of two copies of itself, each copy shrunk by a factor 1/3; hence, it can be shown that its Hausdorff dimension is ln(2)/ln(3)&amp;amp;nbsp;≈&amp;amp;nbsp;0.63.&amp;lt;ref&amp;gt;{{cite book | last=Falconer | first = Kenneth |title=Fractal Geometry: Mathematical Foundations and Applications | publisher=[[John Wiley and Sons]] | edition=2nd | year=2003}}&amp;lt;/ref&amp;gt; The [[Sierpinski triangle]] is a union of three copies of itself, each copy shrunk by a factor of&amp;amp;nbsp;1/2; this yields a Hausdorff dimension of ln(3)/ln(2)&amp;amp;nbsp;≈&amp;amp;nbsp;1.58.&amp;lt;ref name=CampbellAnnenberg15/&amp;gt; These Hausdorff dimensions are related to the &amp;quot;critical exponent&amp;quot; of the [[Master theorem (analysis of algorithms)|Master theorem]] for solving [[Recurrence relation|recurrence relations]] in the [[analysis of algorithms]].&lt;br /&gt;
*[[分形]]一般是那些豪斯多夫维数直接超过其拓扑维数的空间。例如[[康托尔集]]是一个o维拓扑空间，由两个自己复制而成，每一个复制品都是原来的三分之一，因此它的豪斯多夫维数是 ln(2)/ln(3)&amp;amp;nbsp;≈&amp;amp;nbsp;0.63。&amp;lt;ref&amp;gt;{{cite book | last=Falconer | first = Kenneth |title=Fractal Geometry: Mathematical Foundations and Applications | publisher=[[John Wiley and Sons]] | edition=2nd | year=2003}}&amp;lt;/ref&amp;gt;一个[[谢尔宾斯基三角]]是他自身三个复制的组合。每一个是原来的&amp;amp;nbsp;1/2，它的豪斯多夫维数ln(3)/ln(2)&amp;amp;nbsp;≈&amp;amp;nbsp;1.58。&amp;lt;ref name=CampbellAnnenberg15/&amp;gt;在递归算法中解决递归关系时，这些豪斯多夫维数与[[算法分析主定理]]的临界指标相联系。&lt;br /&gt;
* [[Space-filling curve]]s like the [[Peano curve]] have the same Hausdorff dimension as the space they fill.&lt;br /&gt;
*[[空间填充曲线]]拥有和他们填充空间同样的豪斯多夫维数，如[[皮亚诺曲线]]。&lt;br /&gt;
* The trajectory of [[Brownian motion]] in dimension 2 and above is conjectured to be Hausdorff dimension 2.&amp;lt;ref&amp;gt;{{cite book | last=Morters | first=Peres | title= Brownian Motion | publisher=[[Cambridge University Press]] | year=2010 }}&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
[[image:Great Britain Hausdorff.svg|thumb|250px|Estimating the Hausdorff dimension of the [[How Long Is the Coast of Britain? Statistical Self-Similarity and Fractional Dimension|coast of Great Britain]]]]&lt;br /&gt;
&lt;br /&gt;
coast of Great Britain]]&lt;br /&gt;
&lt;br /&gt;
[[大不列颠海岸&lt;br /&gt;
&lt;br /&gt;
* 刘易斯·弗赖伊·理查森[[Lewis Fry Richardson]] has performed detailed experiments to measure the approximate Hausdorff dimension for various coastlines. His results have varied from 1.02 for the coastline of [[South Africa]] to 1.25 for the west coast of [[Great Britain]].&amp;lt;ref name=&amp;quot;mandelbrot&amp;quot; /&amp;gt;&lt;br /&gt;
*刘易斯·弗赖伊·理查森（Lewis Fry Richardson）已经通过豪斯多夫维数去测量了很多海岸线。它的结果涵盖从1.02的南非海岸线到1.25的大英帝国西海岸模型。]]&lt;br /&gt;
&lt;br /&gt;
==Properties of Hausdorff dimension豪斯多夫维数特性==&lt;br /&gt;
&lt;br /&gt;
{{refimprove section|date=March 2015}}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
=== Hausdorff dimension and inductive dimension 豪斯多夫维数和归纳维数===&lt;br /&gt;
&lt;br /&gt;
Let ''X'' be an arbitrary [[Separable space|separable]] metric space. There is a [[topology|topological]] notion of [[inductive dimension]] for ''X'' which is defined recursively. It is always an integer (or +∞) and is denoted dim&amp;lt;sub&amp;gt;ind&amp;lt;/sub&amp;gt;(''X'').&lt;br /&gt;
&lt;br /&gt;
Let X be an arbitrary separable metric space. There is a topological notion of inductive dimension for X which is defined recursively. It is always an integer (or +∞) and is denoted dim&amp;lt;sub&amp;gt;ind&amp;lt;/sub&amp;gt;(X).&lt;br /&gt;
&lt;br /&gt;
设''X'' 是[[任意可分度量空间]]。对于''X'' 有一个递归定义的归纳维数拓扑概念。它总是一个整数(或 + ∞) ，并且表示dim&amp;lt;sub&amp;gt;ind&amp;lt;/sub&amp;gt;(''X'')。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
'''Theorem'''. Suppose ''X'' is non-empty. Then &lt;br /&gt;
&lt;br /&gt;
Theorem. Suppose X is non-empty. Then &lt;br /&gt;
&lt;br /&gt;
'''定理'''：假设''X'' 是非空的。那么&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt; \dim_{\mathrm{Haus}}(X) \geq \dim_{\operatorname{ind}}(X). &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \dim_{\mathrm{Haus}}(X) \geq \dim_{\operatorname{ind}}(X). &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Moreover,&lt;br /&gt;
&lt;br /&gt;
Moreover,&lt;br /&gt;
&lt;br /&gt;
此外,&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \inf_Y \dim_{\operatorname{Haus}}(Y) =\dim_{\operatorname{ind}}(X), &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \inf_Y \dim_{\operatorname{Haus}}(Y) =\dim_{\operatorname{ind}}(X), &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
where ''Y'' ranges over metric spaces [[homeomorphic]] to ''X''. In other words, ''X'' and ''Y'' have the same underlying set of points and the metric ''d''&amp;lt;sub&amp;gt;''Y''&amp;lt;/sub&amp;gt; of ''Y'' is topologically equivalent to ''d''&amp;lt;sub&amp;gt;''X''&amp;lt;/sub&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
where Y ranges over metric spaces homeomorphic to X. In other words, X and Y have the same underlying set of points and the metric d&amp;lt;sub&amp;gt;Y&amp;lt;/sub&amp;gt; of Y is topologically equivalent to d&amp;lt;sub&amp;gt;X&amp;lt;/sub&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
其中''Y''是度量空间同胚到 ''X''的范围。换句话说， ''X''和 ''Y''具有相同的基本点集，''Y''的度规''d''&amp;lt;sub&amp;gt;''Y''&amp;lt;/sub&amp;gt; 的子拓扑等价于''d''&amp;lt;sub&amp;gt;''X''&amp;lt;/sub&amp;gt;。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
These results were originally established by [[Edward Szpilrajn]] (1907–1976), e.g., see Hurewicz and Wallman, Chapter VII.{{full citation needed|date=March 2015}}&lt;br /&gt;
&lt;br /&gt;
These results were originally established by Edward Szpilrajn (1907–1976), e.g., see Hurewicz and Wallman, Chapter VII.&lt;br /&gt;
&lt;br /&gt;
这些结果最初是由 [[Edward Szpilrajn]] (1907–1976)建立的,  参见 Hurewicz and Wallman, Chapter VII.{{full citation needed|date=March 2015}}第七章。&lt;br /&gt;
&lt;br /&gt;
=== Hausdorff dimension and Minkowski dimension 豪斯多夫维数和闵可夫斯基维度===&lt;br /&gt;
&lt;br /&gt;
The [[Minkowski dimension]] is similar to, and at least as large as, the Hausdorff dimension, and they are equal in many situations. However, the set of [[rational number|rational]] points in [0, 1] has Hausdorff dimension zero and Minkowski dimension one. There are also compact sets for which the Minkowski dimension is strictly larger than the Hausdorff dimension.&lt;br /&gt;
&lt;br /&gt;
The Minkowski dimension is similar to, and at least as large as, the Hausdorff dimension, and they are equal in many situations. However, the set of rational points in [0, 1] has Hausdorff dimension zero and Minkowski dimension one. There are also compact sets for which the Minkowski dimension is strictly larger than the Hausdorff dimension.&lt;br /&gt;
&lt;br /&gt;
[[闵可夫斯基维数]]与豪斯多夫维数相似，至少和它一样大，而且在许多情况下是相等的。然而，[0,1]中有理点集的豪斯多夫维数为0，闵可夫斯基维数为1。还有一些紧集的闵可夫斯基维数绝对大于豪斯多夫维数。&lt;br /&gt;
&lt;br /&gt;
=== Hausdorff dimensions and Frostman measures 豪斯多夫维度和弗洛斯曼测度===&lt;br /&gt;
&lt;br /&gt;
If there is a [[measure (mathematics)|measure]] μ defined on [[Borel measure|Borel]] subsets of a metric space ''X'' such that ''μ''(''X'') &amp;gt; 0 and ''μ''(''B''(''x'', ''r'')) ≤ ''r&amp;lt;sup&amp;gt;s&amp;lt;/sup&amp;gt;'' holds for some constant ''s'' &amp;gt; 0 and for every ball ''B''(''x'', ''r'') in ''X'', then dim&amp;lt;sub&amp;gt;Haus&amp;lt;/sub&amp;gt;(''X'') ≥ ''s''. A partial converse is provided by [[Frostman's lemma]].{{citation needed|date=March 2015}}&amp;lt;ref&amp;gt;This Wikipedia article also discusses further useful characterizations of the Hausdorff dimension.{{clarify|date=March 2015}}&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
If there is a measure μ defined on Borel subsets of a metric space X such that μ(X) &amp;gt; 0 and μ(B(x, r)) ≤ r&amp;lt;sup&amp;gt;s&amp;lt;/sup&amp;gt; holds for some constant s &amp;gt; 0 and for every ball B(x, r) in X, then dim&amp;lt;sub&amp;gt;Haus&amp;lt;/sub&amp;gt;(X) ≥ s. A partial converse is provided by Frostman's lemma.&lt;br /&gt;
&lt;br /&gt;
如果在度量空间 ''X'' 的 Borel 子集上定义一个测度 μ，使得''μ''(''X'') &amp;gt; 0 和''μ''(''B''(''x'', ''r'')) ≤ ''r&amp;lt;sup&amp;gt;s&amp;lt;/sup&amp;gt;''，对于某个常数 ''s'' &amp;gt; 0  和 ''X'' 中的每个球 ''B''(''x'', ''r'') 成立，则 dim&amp;lt;sub&amp;gt;Haus&amp;lt;/sub&amp;gt;(''X'') ≥ ''s'' 。 部分逆向转换由弗洛斯曼引理定义。&lt;br /&gt;
&lt;br /&gt;
=== Behaviour under unions and products ===&lt;br /&gt;
&lt;br /&gt;
If &amp;lt;math&amp;gt;X=\bigcup_{i\in I}X_i&amp;lt;/math&amp;gt; is a finite or countable union, then&lt;br /&gt;
&lt;br /&gt;
If &amp;lt;math&amp;gt;X=\bigcup_{i\in I}X_i&amp;lt;/math&amp;gt; is a finite or countable union, then&lt;br /&gt;
&lt;br /&gt;
如果 &amp;lt;math&amp;gt;X=\bigcup_{i\in I}X_i&amp;lt;/math&amp;gt; 是一个有限或可数的联合，则&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \dim_{\operatorname{Haus}}(X) =\sup_{i\in I} \dim_{\operatorname{Haus}}(X_i).&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \dim_{\operatorname{Haus}}(X) =\sup_{i\in I} \dim_{\operatorname{Haus}}(X_i).&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
This can be verified directly from the definition.&lt;br /&gt;
&lt;br /&gt;
This can be verified directly from the definition.&lt;br /&gt;
&lt;br /&gt;
这可以直接从定义得到验证。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
If ''X'' and ''Y'' are non-empty metric spaces, then the Hausdorff dimension of their product satisfies&amp;lt;ref&amp;gt;{{cite journal |author=Marstrand, J. M. |title=The dimension of Cartesian product sets |journal=Proc. Cambridge Philos. Soc. |volume=50 |issue=3 |pages=198–202 |year=1954 |doi=10.1017/S0305004100029236 |bibcode = 1954PCPS...50..198M }}&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
If X and Y are non-empty metric spaces, then the Hausdorff dimension of their product satisfies&lt;br /&gt;
&lt;br /&gt;
如果 ''X'' 和''Y''是非空度量空间，那么它们乘积的豪斯多夫维数满足&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt; \dim_{\operatorname{Haus}}(X\times Y)\ge \dim_{\operatorname{Haus}}(X)+ \dim_{\operatorname{Haus}}(Y).&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \dim_{\operatorname{Haus}}(X\times Y)\ge \dim_{\operatorname{Haus}}(X)+ \dim_{\operatorname{Haus}}(Y).&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
This inequality can be strict. It is possible to find two sets of dimension 0 whose product has dimension 1.&amp;lt;ref&amp;gt;{{cite book  | last = Falconer  | first = Kenneth J.  | title = Fractal geometry. Mathematical foundations and applications  | publisher = John Wiley &amp;amp; Sons, Inc., Hoboken, New Jersey  | year = 2003  | doi =   | isbn = }}&amp;lt;/ref&amp;gt; In the opposite direction, it is known that when ''X'' and ''Y'' are Borel subsets of '''R'''&amp;lt;sup&amp;gt;''n''&amp;lt;/sup&amp;gt;, the Hausdorff dimension of ''X'' × ''Y'' is bounded from above by the Hausdorff dimension of ''X'' plus the [[packing dimension|upper packing dimension]] of ''Y''. These facts are discussed in Mattila (1995).&lt;br /&gt;
&lt;br /&gt;
This inequality can be strict. It is possible to find two sets of dimension 0 whose product has dimension 1. In the opposite direction, it is known that when X and Y are Borel subsets of R&amp;lt;sup&amp;gt;n&amp;lt;/sup&amp;gt;, the Hausdorff dimension of X × Y is bounded from above by the Hausdorff dimension of X plus the upper packing dimension of Y. These facts are discussed in Mattila (1995).&lt;br /&gt;
&lt;br /&gt;
这种不平等可以是绝对的。有可能找到两个维数为0的集合，其乘积的维数为1。相反，我们知道当''X''和''Y''是 '''R'''&amp;lt;sup&amp;gt;''n''&amp;lt;/sup&amp;gt;的 Borel 子集时， ''X'' × ''Y''的豪斯多夫维数从上面以 ''X''的豪斯多夫维数加上 ''Y''的填充维数为界。Mattila (1995)曾就这些情况进行了讨论。&lt;br /&gt;
&lt;br /&gt;
==Self-similar sets自相似集合==&lt;br /&gt;
&lt;br /&gt;
{{refimprove section|date=March 2015}}&lt;br /&gt;
&lt;br /&gt;
Many sets defined by a self-similarity condition have dimensions which can be determined explicitly. Roughly, a set ''E'' is self-similar if it is the fixed point of a set-valued transformation ψ, that is ψ(''E'') = ''E'', although the exact definition is given below.&lt;br /&gt;
&lt;br /&gt;
Many sets defined by a self-similarity condition have dimensions which can be determined explicitly. Roughly, a set E is self-similar if it is the fixed point of a set-valued transformation ψ, that is ψ(E) = E, although the exact definition is given below.&lt;br /&gt;
&lt;br /&gt;
许多由自相似条件定义的集合具有可以显式确定的维数。粗略地说，如果集合''E''是集值ψ变换的不动点，即ψ(''E'') = ''E''， 则它是自相似的，尽管下面给出了确切的定义。&lt;br /&gt;
&lt;br /&gt;
&amp;lt;blockquote&amp;gt;'''Theorem'''. Suppose&lt;br /&gt;
&lt;br /&gt;
&amp;lt;blockquote&amp;gt;Theorem. Suppose&lt;br /&gt;
&lt;br /&gt;
&amp;lt;blockquote&amp;gt;'''定理'''：假设&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt; \psi_i: \mathbf{R}^n \rightarrow \mathbf{R}^n, \quad i=1, \ldots , m &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \psi_i: \mathbf{R}^n \rightarrow \mathbf{R}^n, \quad i=1, \ldots , m &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
are [[Contraction mapping|contractive]] mappings on '''R'''&amp;lt;sup&amp;gt;''n''&amp;lt;/sup&amp;gt; with contraction constant ''r&amp;lt;sub&amp;gt;j&amp;lt;/sub&amp;gt;'' &amp;lt; 1. Then there is a unique ''non-empty'' compact set ''A'' such that&lt;br /&gt;
&lt;br /&gt;
are contractive mappings on R&amp;lt;sup&amp;gt;n&amp;lt;/sup&amp;gt; with contraction constant r&amp;lt;sub&amp;gt;j&amp;lt;/sub&amp;gt; &amp;lt; 1. Then there is a unique non-empty compact set A such that&lt;br /&gt;
&lt;br /&gt;
是'''R'''&amp;lt;sup&amp;gt;''n''&amp;lt;/sup&amp;gt;上的压缩常数''r&amp;lt;sub&amp;gt;j&amp;lt;/sub&amp;gt;'&amp;lt; 1的压缩映射。然后有一个唯一的非空紧集A &lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt; A = \bigcup_{i=1}^m \psi_i (A). &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; A = \bigcup_{i=1}^m \psi_i (A). &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&amp;lt;/blockquote&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;/blockquote&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The theorem follows from [[Stefan Banach]]'s [[Contractive mapping theorem|contractive mapping fixed point theorem]] applied to the complete metric space of non-empty compact subsets of '''R'''&amp;lt;sup&amp;gt;''n''&amp;lt;/sup&amp;gt; with the [[Hausdorff distance]].&amp;lt;ref&amp;gt;{{cite book |author=Falconer, K. J. |title=The Geometry of Fractal Sets |publisher=Cambridge University Press |location=Cambridge, UK |year=1985 |isbn=0-521-25694-1 |chapter=Theorem 8.3}}&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
The theorem follows from Stefan Banach's contractive mapping fixed point theorem applied to the complete metric space of non-empty compact subsets of R&amp;lt;sup&amp;gt;n&amp;lt;/sup&amp;gt; with the Hausdorff distance.&lt;br /&gt;
&lt;br /&gt;
这个定理来源于 Stefan Banach 的压缩映射不动点定理，该定理应用于 具有豪斯多夫距离的'''R'''&amp;lt;sup&amp;gt;''n''&amp;lt;/sup&amp;gt; 的非空紧子集的完整度量空间。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
===The open set condition开集条件===&lt;br /&gt;
&lt;br /&gt;
To determine the dimension of the self-similar set ''A'' (in certain cases), we need a technical condition called the ''open set condition'' (OSC) on the sequence of contractions ψ&amp;lt;sub&amp;gt;''i''&amp;lt;/sub&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
To determine the dimension of the self-similar set A (in certain cases), we need a technical condition called the open set condition (OSC) on the sequence of contractions ψ&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
为了确定自相似集''A'' 的维数(在某些情况下) ，我们需要一个关于收缩序列的称为''开集条件''(OSC)的技术条件ψ&amp;lt;sub&amp;gt;''i''&amp;lt;/sub&amp;gt;。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
There is a relatively compact open set ''V'' such that&lt;br /&gt;
&lt;br /&gt;
There is a relatively compact open set V such that&lt;br /&gt;
&lt;br /&gt;
有一个相对紧的开集''V''&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt; \bigcup_{i=1}^m\psi_i (V) \subseteq V, &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \bigcup_{i=1}^m\psi_i (V) \subseteq V, &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
where the sets in union on the left are pairwise [[disjoint sets|disjoint]].&lt;br /&gt;
&lt;br /&gt;
where the sets in union on the left are pairwise disjoint.&lt;br /&gt;
&lt;br /&gt;
左边并集的集合成对不相交。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The open set condition is a separation condition that ensures the images ψ&amp;lt;sub&amp;gt;''i''&amp;lt;/sub&amp;gt;(''V'') do not overlap &amp;quot;too much&amp;quot;.&lt;br /&gt;
&lt;br /&gt;
The open set condition is a separation condition that ensures the images ψ&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;(V) do not overlap &amp;quot;too much&amp;quot;.&lt;br /&gt;
&lt;br /&gt;
开集条件是保证图像ψ&amp;lt;sub&amp;gt;''i''&amp;lt;/sub&amp;gt;(''V'') 不重叠“太多”的分离条件。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
'''Theorem'''. Suppose the open set condition holds and each ψ&amp;lt;sub&amp;gt;''i''&amp;lt;/sub&amp;gt; is a similitude, that is a composition of an [[isometry]] and a [[dilation (metric space)|dilation]] around some point. Then the unique fixed point of ψ is a set whose Hausdorff dimension is ''s'' where ''s'' is the unique solution of&amp;lt;ref&amp;gt;{{cite journal | last=Hutchinson | first=John E. | title=Fractals and self similarity | journal=Indiana Univ. Math. J. | volume=30 | year=1981 | pages=713–747 | doi=10.1512/iumj.1981.30.30055 | issue=5 | doi-access=free }}&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
Theorem. Suppose the open set condition holds and each ψ&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt; is a similitude, that is a composition of an isometry and a dilation around some point. Then the unique fixed point of ψ is a set whose Hausdorff dimension is s where s is the unique solution of&lt;br /&gt;
&lt;br /&gt;
'''定理'''假设开集条件成立，并且每个ψ&amp;lt;sub&amp;gt;''i''&amp;lt;/sub&amp;gt; 是一个相似度，即等距和某个点周围的膨胀的组合。。那么唯一的不动点是Hausdorff维数为 ''s'' 的集合，其中  ''s'' 是 ''s'' &amp;lt;ref&amp;gt;{{cite journal | last=Hutchinson | first=John E. | title=Fractals and self similarity | journal=Indiana Univ. Math. J. | volume=30 | year=1981 | pages=713–747 | doi=10.1512/iumj.1981.30.30055 | issue=5 | doi-access=free }}&amp;lt;/ref&amp;gt;的唯一解&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt; \sum_{i=1}^m r_i^s = 1. &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \sum_{i=1}^m r_i^s = 1. &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The contraction coefficient of a similitude is the magnitude of the dilation.&lt;br /&gt;
&lt;br /&gt;
The contraction coefficient of a similitude is the magnitude of the dilation.&lt;br /&gt;
&lt;br /&gt;
相似物的收缩系数就是膨胀的大小。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
We can use this theorem to compute the Hausdorff dimension of the Sierpinski triangle (or sometimes called Sierpinski gasket). Consider three [[non-collinear points]] ''a''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;, ''a''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;, ''a''&amp;lt;sub&amp;gt;3&amp;lt;/sub&amp;gt; in the plane '''R'''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; and let ψ&amp;lt;sub&amp;gt;''i''&amp;lt;/sub&amp;gt; be the dilation of ratio 1/2 around ''a&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;''. The unique non-empty fixed point of the corresponding mapping ψ is a Sierpinski gasket and the dimension ''s'' is the unique solution of&lt;br /&gt;
&lt;br /&gt;
We can use this theorem to compute the Hausdorff dimension of the Sierpinski triangle (or sometimes called Sierpinski gasket). Consider three non-collinear points a&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;, a&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;, a&amp;lt;sub&amp;gt;3&amp;lt;/sub&amp;gt; in the plane R&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; and let ψ&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt; be the dilation of ratio 1/2 around a&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;. The unique non-empty fixed point of the corresponding mapping ψ is a Sierpinski gasket and the dimension s is the unique solution of&lt;br /&gt;
&lt;br /&gt;
我们可以使用这个定理来计算谢尔宾斯基三角形的豪斯多夫维数(或者有时候叫做谢尔宾斯基垫圈)。考虑R&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; 平面上的三个非共线点，''a''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;，''a''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;，''a''&amp;lt;sub&amp;gt;3&amp;lt;/sub&amp;gt;，让ψ&amp;lt;sub&amp;gt;''i''&amp;lt;/sub&amp;gt;是围绕着''a&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;''比率1/2的膨胀。对应映射的唯一非空不动点是一个谢尔宾斯基垫圈，其维数''s''是对应映射的唯一解&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt; \left(\frac{1}{2}\right)^s+\left(\frac{1}{2}\right)^s+\left(\frac{1}{2}\right)^s = 3 \left(\frac{1}{2}\right)^s =1. &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \left(\frac{1}{2}\right)^s+\left(\frac{1}{2}\right)^s+\left(\frac{1}{2}\right)^s = 3 \left(\frac{1}{2}\right)^s =1. &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Taking [[natural logarithm]]s of both sides of the above equation, we can solve for ''s'', that is: ''s'' = ln(3)/ln(2).  The Sierpinski gasket is self-similar and satisfies the OSC. In general a set ''E'' which is a fixed point of a mapping&lt;br /&gt;
&lt;br /&gt;
Taking natural logarithms of both sides of the above equation, we can solve for s, that is: s = ln(3)/ln(2).  The Sierpinski gasket is self-similar and satisfies the OSC. In general a set E which is a fixed point of a mapping&lt;br /&gt;
&lt;br /&gt;
取上述方程两边的自然对数，我们可以求出 ''s''，即: ''s'' = ln(3)/ln(2)。该密封垫具有自相似性，满足 OSC 要求。一般来说，集合 ''E''是一个映射的不动点&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt; A \mapsto \psi(A) = \bigcup_{i=1}^m \psi_i(A) &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt; A \mapsto \psi(A) = \bigcup_{i=1}^m \psi_i(A) &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
is self-similar if and only if the intersections&lt;br /&gt;
&lt;br /&gt;
is self-similar if and only if the intersections&lt;br /&gt;
&lt;br /&gt;
是自相似的，当且仅当&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt; H^s\left(\psi_i(E) \cap \psi_j(E)\right) =0, &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; H^s\left(\psi_i(E) \cap \psi_j(E)\right) =0, &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
where ''s'' is the Hausdorff dimension of ''E'' and ''H&amp;lt;sup&amp;gt;s&amp;lt;/sup&amp;gt;'' denotes [[Hausdorff measure]]. This is clear in the case of the Sierpinski gasket (the intersections are just points), but is also true more generally:&lt;br /&gt;
&lt;br /&gt;
where s is the Hausdorff dimension of E and H&amp;lt;sup&amp;gt;s&amp;lt;/sup&amp;gt; denotes Hausdorff measure. This is clear in the case of the Sierpinski gasket (the intersections are just points), but is also true more generally:&lt;br /&gt;
&lt;br /&gt;
其中 ''s''是''E''的豪斯多夫维数， ''H&amp;lt;sup&amp;gt;s&amp;lt;/sup&amp;gt;'' 表示 豪斯多夫测度。对于谢尔宾斯基垫圈(交叉点就是点)来说，这一点很明显，但更普遍的情况是:&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
'''Theorem'''. Under the same conditions as the previous theorem, the unique fixed point of ψ is self-similar.&lt;br /&gt;
&lt;br /&gt;
Theorem. Under the same conditions as the previous theorem, the unique fixed point of ψ is self-similar.&lt;br /&gt;
&lt;br /&gt;
'''定理'''：在与前一定理相同的条件下，其唯一不动点是自相似的。&lt;br /&gt;
&lt;br /&gt;
==See also参阅==&lt;br /&gt;
&lt;br /&gt;
* [[List of fractals by Hausdorff dimension豪斯多夫分形维数列表]] Examples of deterministic fractals, random and natural fractals.确定性分形与随机和自然分形的示例。&lt;br /&gt;
&lt;br /&gt;
* [[Assouad dimension  Assouad维数]], another variation of fractal dimension that, like Hausdorff dimension, is defined using coverings by balls其他被球覆盖方式定义的分形维数，例如豪斯多夫维数。&lt;br /&gt;
&lt;br /&gt;
* [[Intrinsic dimension固有维数]]&lt;br /&gt;
&lt;br /&gt;
* [[Packing dimension填充维数]]&lt;br /&gt;
&lt;br /&gt;
* [[Fractal dimension分形维数]]&lt;br /&gt;
&lt;br /&gt;
==References参考文献==&lt;br /&gt;
&lt;br /&gt;
{{reflist}}&lt;br /&gt;
&lt;br /&gt;
==Further reading拓展阅读==&lt;br /&gt;
&lt;br /&gt;
* {{cite book |last1=Dodson |first1=M. Maurice |title=Fractal Geometry and Applications: A Jubilee of Benoît Mandelbrot |volume=72 |issue=1 |pages=305–347 |last2=Kristensen |first2=Simon |chapter=Hausdorff Dimension and Diophantine Approximation |date=June 12, 2003 |arxiv=math/0305399 |bibcode = 2003math......5399D |doi=10.1090/pspum/072.1/2112110|series=Proceedings of Symposia in Pure Mathematics |isbn=9780821836378 }}&lt;br /&gt;
&lt;br /&gt;
* {{cite book |last1=Hurewicz |first1=Witold |authorlink1=Witold Hurewicz |last2=Wallman |first2=Henry |authorlink2=Henry Wallman |title=Dimension Theory |url=https://archive.org/details/in.ernet.dli.2015.84609 |publisher=Princeton University Press |year=1948 }}&lt;br /&gt;
&lt;br /&gt;
* {{cite journal |author作者=E. Szpilrajn |authorlink=Edward Marczewski |title=La dimension et la mesure |journal=Fundamenta Mathematicae |volume=28 |pages=81–9 |year=1937 }}&lt;br /&gt;
&lt;br /&gt;
* {{cite journal&lt;br /&gt;
&lt;br /&gt;
 | last1=Marstrand&lt;br /&gt;
&lt;br /&gt;
 | last1=Marstrand&lt;br /&gt;
&lt;br /&gt;
 | last1=马斯特兰德&lt;br /&gt;
&lt;br /&gt;
 | first1=J. M. | title=The dimension of cartesian product sets | year=1954 | journal=Proc. Cambridge Philos. Soc.&lt;br /&gt;
&lt;br /&gt;
 | first1=J. M. | title=The dimension of cartesian product sets | year=1954 | journal=Proc. Cambridge Philos. Soc.&lt;br /&gt;
&lt;br /&gt;
 | first1= J. M. | title=笛卡儿积集的维数 | 1954年 |  journal=Proc. Cambridge Philos. Soc.&lt;br /&gt;
&lt;br /&gt;
 | volume=50&lt;br /&gt;
&lt;br /&gt;
 | volume=50&lt;br /&gt;
&lt;br /&gt;
 | 第50卷&lt;br /&gt;
&lt;br /&gt;
 | issue=3&lt;br /&gt;
&lt;br /&gt;
 | issue=3&lt;br /&gt;
&lt;br /&gt;
 | 第三期&lt;br /&gt;
&lt;br /&gt;
 | pages=198–202&lt;br /&gt;
&lt;br /&gt;
 | pages=198–202&lt;br /&gt;
&lt;br /&gt;
 | 第198-202页&lt;br /&gt;
&lt;br /&gt;
 | doi=10.1017/S0305004100029236|bibcode = 1954PCPS...50..198M }}&lt;br /&gt;
&lt;br /&gt;
 | doi=10.1017/S0305004100029236|bibcode = 1954PCPS...50..198M }}&lt;br /&gt;
&lt;br /&gt;
10.1017 / S0305004100029236 | bibcode 1954PCPS... 50. . 198 m }&lt;br /&gt;
&lt;br /&gt;
* {{Cite book&lt;br /&gt;
&lt;br /&gt;
 | last1=Mattila&lt;br /&gt;
&lt;br /&gt;
 | last1=Mattila&lt;br /&gt;
&lt;br /&gt;
 | last1=Mattila&lt;br /&gt;
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 | first1=Pertti | author1-link=Pertti Mattila| title=Geometry of sets and measures in Euclidean spaces | publisher=[[Cambridge University Press]]&lt;br /&gt;
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 | first1=Pertti | author1-link=Pertti Mattila| title=Geometry of sets and measures in Euclidean spaces | publisher=Cambridge University Press&lt;br /&gt;
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| first1 Pertti | author1-link Pertti Mattila | title 欧几里德空间中集合和度量的几何 | 出版商剑桥大学出版社&lt;br /&gt;
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 | isbn=978-0-521-65595-8 | year=1995}}&lt;br /&gt;
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 | isbn=978-0-521-65595-8 | year=1995}}&lt;br /&gt;
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| isbn 978-0-521-65595-8 | year 1995}&lt;br /&gt;
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* {{cite journal |author=A. S. Besicovitch |authorlink=A. S. Besicovitch |title=On Linear Sets of Points of Fractional Dimensions |journal=[[Mathematische Annalen]] |volume=101 |year=1929 | doi=10.1007/BF01454831| issue=1 |pages= 161–193}}&lt;br /&gt;
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* {{cite journal |author1=A. S. Besicovitch |authorlink1=A. S. Besicovitch |author2=H. D. Ursell |authorlink2=H. D. Ursell |title=Sets of Fractional Dimensions |journal=Journal of the London Mathematical Society |volume=12 |year=1937 | issue=1 | doi=10.1112/jlms/s1-12.45.18  | pages=18–25 }}&amp;lt;br/&amp;gt;Several selections from this volume are reprinted in {{cite book |author=Edgar, Gerald A. |title=Classics on fractals |publisher=Addison-Wesley |location=Boston |year=1993 |isbn=0-201-58701-7}} See chapters 9,10,11&lt;br /&gt;
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* {{cite journal |author=F. Hausdorff |authorlink=F. Hausdorff |title=Dimension und äußeres Maß |journal=Mathematische Annalen |volume=79 |issue=1–2 |pages=157–179 |date=March 1919 |doi=10.1007/BF01457179|hdl=10338.dmlcz/100363 |url=http://dml.cz/bitstream/handle/10338.dmlcz/100363/CzechMathJ_09-1959-3_5.pdf }}&lt;br /&gt;
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* {{cite journal | last=Hutchinson | first=John E. | title=Fractals and self similarity | journal=Indiana Univ. Math. J. | volume=30 | year=1981 | pages=713–747 | doi=10.1512/iumj.1981.30.30055 | issue=5 | doi-access=free }}&lt;br /&gt;
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*{{cite book | last=Falconer | first = Kenneth |title=Fractal Geometry: Mathematical Foundations and Applications | publisher=[[John Wiley and Sons]] | edition=2nd | year=2003}}&lt;br /&gt;
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==External links外部链接==&lt;br /&gt;
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* [https://www.encyclopediaofmath.org/index.php/Hausdorff_dimension Hausdorff dimension] 在 [https://www.encyclopediaofmath.org/ Encyclopedia of Mathematics]&lt;br /&gt;
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* [https://www.encyclopediaofmath.org/index.php/Hausdorff_measure Hausdorff measure] 在 [https://www.encyclopediaofmath.org/ Encyclopedia of Mathematics]&lt;br /&gt;
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{{DEFAULTSORT:Hausdorff Dimension豪斯多夫维数}}&lt;br /&gt;
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[[Category分类:Fractals分形]]&lt;br /&gt;
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[[Category分类:Metric geometry度量几何]]&lt;br /&gt;
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[[Category分类:Dimension theory维度理论]]&lt;br /&gt;
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&amp;lt;small&amp;gt;This page was moved from [[wikipedia:en:Hausdorff dimension]]. Its edit history can be viewed at [[分形维数/edithistory]]&amp;lt;/small&amp;gt;&amp;lt;/noinclude&amp;gt;&lt;br /&gt;
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[[Category:待整理页面]]&lt;/div&gt;</summary>
		<author><name>Ruili</name></author>
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		<title>分形维数</title>
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		<updated>2020-11-01T17:11:16Z</updated>

		<summary type="html">&lt;p&gt;Ruili：&lt;/p&gt;
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&lt;div&gt;此词条暂由彩云小译翻译，未经人工整理和审校，带来阅读不便，请见谅。&lt;br /&gt;
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Example of non-integer dimensions. The first four [[iteration]]s of the [[Koch snowflake|Koch curve]], where after each iteration, all original line segments are replaced with four, each a self-similar copy that is 1/3 the length of the original. One formalism of the Hausdorff dimension uses this scale factor (3) and the number of self-similar objects (4) to calculate the dimension, D, after the first iteration to be D = (log N)/(log S) = (log 4)/(log 3) ≈ 1.26.&amp;lt;ref name=CampbellAnnenberg15&amp;gt;MacGregor Campbell, 2013, &amp;quot;5.6 Scaling and the Hausdorff Dimension,&amp;quot; at ''Annenberg Learner:MATHematics illuminated'', see [http://www.learner.org/courses/mathilluminated/units/5/textbook/06.php], accessed 5 March 2015.&amp;lt;/ref&amp;gt; That is, while the Hausdorff dimension of a single [[point (geometry)|point]] is zero, of a [[line segment]] is 1, of a [[square]] is 2, and of a [[cube]] is 3, for [[fractal]]s such as this, the object can have a non-integer dimension.&lt;br /&gt;
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Example of non-integer dimensions. The first four iterations of the Koch curve, where after each iteration, all original line segments are replaced with four, each a self-similar copy that is 1/3 the length of the original. One formalism of the Hausdorff dimension uses this scale factor (3) and the number of self-similar objects (4) to calculate the dimension, D, after the first iteration to be D = (log N)/(log S) = (log 4)/(log 3) ≈ 1.26. That is, while the Hausdorff dimension of a single point is zero, of a line segment is 1, of a square is 2, and of a cube is 3, for fractals such as this, the object can have a non-integer dimension.&lt;br /&gt;
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非整数维度示例：前四个[[Koch 曲线]]的迭代，在每次迭代后，所有原始线段都被替换为四个，每个自相似的复制是原始线段长度的1 / 3。豪斯多夫维数的一个建模是使用比例因子(3)和自相似对象的数量(4)来计算维度 D，在第一次迭代后为 D = (log N)/(log S) = (log 4)/(log 3) ≈ 1.26.&amp;lt;ref name=CampbellAnnenberg15&amp;gt;。MacGregor Campbell, 2013, &amp;quot;5.6 Scaling and the Hausdorff Dimension,&amp;quot; 在 ''Annenberg Learner:MATHematics illuminated'', 参见 [http://www.learner.org/courses/mathilluminated/units/5/textbook/06.php], accessed 5 March 2015.&amp;lt;/ref&amp;gt; 也就是说，单点的豪斯多夫维数为零，线段为1，正方形为2，立方体为3时，但对于分形，对象可以有一个非整数维度。&lt;br /&gt;
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In [[mathematics]], '''Hausdorff dimension''' is a measure of ''roughness'', or more specifically, [[fractal dimension]], that was first introduced in 1918 by [[mathematician]] [[Felix Hausdorff]].&amp;lt;ref&amp;gt;{{Cite journal |arxiv = 1101.1444|doi = 10.1214/11-STS370|title = Estimators of Fractal Dimension: Assessing the Roughness of Time Series and Spatial Data|journal = Statistical Science|volume = 27|issue = 2|pages = 247–277|year = 2012|last1 = Gneiting|first1 = Tilmann|last2 = Ševčíková|first2 = Hana|last3 = Percival|first3 = Donald B.}}&amp;lt;/ref&amp;gt; For instance, the Hausdorff dimension of a single [[point (geometry)|point]] is zero, of a [[line segment]] is 1, of a [[square]] is 2, and of a [[cube]] is 3. That is, for sets of points that define a smooth shape or a shape that has a small number of corners—the shapes of traditional geometry and science—the Hausdorff dimension is an [[integer]] agreeing with the usual sense of dimension, also known as the [[Inductive dimension|topological dimension]]. However, formulas have also been developed that allow calculation of the dimension of other less simple objects, where, solely on the basis of their properties of [[scaling (geometry)|scaling]] and [[self-similarity]], one is led to the conclusion that particular objects—including [[fractal]]s—have non-integer Hausdorff dimensions. Because of the significant technical advances made by [[Abram Samoilovitch Besicovitch]] allowing computation of dimensions for highly irregular or &amp;quot;rough&amp;quot; sets, this dimension is also commonly referred to as the ''Hausdorff–Besicovitch dimension.''&lt;br /&gt;
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In mathematics, Hausdorff dimension is a measure of roughness, or more specifically, fractal dimension, that was first introduced in 1918 by mathematician Felix Hausdorff. For instance, the Hausdorff dimension of a single point is zero, of a line segment is 1, of a square is 2, and of a cube is 3. That is, for sets of points that define a smooth shape or a shape that has a small number of corners—the shapes of traditional geometry and science—the Hausdorff dimension is an integer agreeing with the usual sense of dimension, also known as the topological dimension. However, formulas have also been developed that allow calculation of the dimension of other less simple objects, where, solely on the basis of their properties of scaling and self-similarity, one is led to the conclusion that particular objects—including fractals—have non-integer Hausdorff dimensions. Because of the significant technical advances made by Abram Samoilovitch Besicovitch allowing computation of dimensions for highly irregular or &amp;quot;rough&amp;quot; sets, this dimension is also commonly referred to as the Hausdorff–Besicovitch dimension.&lt;br /&gt;
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在[[数学]]中，'''&amp;lt;font color = '#ff8000'&amp;gt;豪斯多夫维数Hausdorff dimension&amp;lt;/font&amp;gt;'''是一种粗糙度的度量单位，或者更确切地说，分形维数，是由数学家 Felix Hausdorff 在1918年首次提出的。例如，单点的豪斯多夫维数为零，线段为1，正方形为2，立方体为3。也就是说，对于定义了一个光滑形状或一个有少数几个角的形状---- 传统几何学和科学的形状---- 的点集来说，豪斯多夫维数是一个整数，符合通常的维度意义，也称为拓扑维度。然而，还有一些公式允许计算其他不太简单的对象的维数，其中仅仅根据它们的标度和自相似特性，就可以得出结论: 特定的对象ー包括分形ー具有非整数的 Hausdorff 维数。由于阿布拉姆·萨莫伊洛维奇·贝西科维奇的重大技术进步，允许计算高度不规则或“粗糙”集的维度，这个维度通常也被称为 Hausdorff-Besicovitch 维度。 &lt;br /&gt;
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The Hausdorff dimension, more specifically, is a further dimensional number associated with a given set, where the distances between all members of that set are defined. Such a set is termed a [[metric space]]. The dimension is drawn from the [[Extended real number line|extended real numbers]], &amp;lt;math&amp;gt;\overline{\mathbb{R}}&amp;lt;/math&amp;gt;, as opposed to the more intuitive notion of dimension, which is not associated to general metric spaces, and only takes values in the non-negative integers.&lt;br /&gt;
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The Hausdorff dimension, more specifically, is a further dimensional number associated with a given set, where the distances between all members of that set are defined. Such a set is termed a metric space. The dimension is drawn from the extended real numbers, &amp;lt;math&amp;gt;\overline{\mathbb{R}}&amp;lt;/math&amp;gt;, as opposed to the more intuitive notion of dimension, which is not associated to general metric spaces, and only takes values in the non-negative integers.&lt;br /&gt;
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更具体地说，豪斯多夫维数是一个与给定集合相关联的更进一步的维数，其中定义了该集合所有成员之间的距离。这样的集合称为度量空间。维数是从扩展的实数，&amp;lt;math&amp;gt;\overline{\mathbb{R}}&amp;lt;/math&amp;gt;，而不是更直观的维数概念(它不与一般的度量空间相关联，只取非负整数的值)。&lt;br /&gt;
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In mathematical terms, the Hausdorff dimension generalizes the notion of the dimension of a real [[vector space]]. That is, the Hausdorff dimension of an ''n''-dimensional [[inner product space]] equals ''n''. This underlies the earlier statement that the Hausdorff dimension of a point is zero, of a line is one, etc., and that [[fractal|irregular sets]] can have noninteger Hausdorff dimensions. For instance, the [[Koch snowflake]] shown at right is constructed from an equilateral triangle; in each iteration, its component line segments are divided into 3 segments of unit length, the newly created middle segment is used as the base of a new [[equilateral]] triangle that points outward, and this base segment is then deleted to leave a final object from the iteration of unit length of 4.&amp;lt;ref&amp;gt;Larry Riddle, 2014, &amp;quot;Classic Iterated Function Systems: Koch Snowflake&amp;quot;, Agnes Scott College e-Academy (online), see [http://ecademy.agnesscott.edu/~lriddle/ifs/ksnow/ksnow.htm], accessed 5 March 2015.&amp;lt;/ref&amp;gt; That is, after the first iteration, each original line segment has been replaced with N=4, where each self-similar copy is 1/S = 1/3 as long as the original.&amp;lt;ref name=CampbellAnnenberg15/&amp;gt; Stated another way, we have taken an object with Euclidean dimension, D, and reduced its linear scale by 1/3 in each direction, so that its length increases to N=S&amp;lt;sup&amp;gt;D&amp;lt;/sup&amp;gt;.&amp;lt;ref name=ClaytonSCTPLS96&amp;gt;Keith Clayton, 1996, &amp;quot;Fractals and the Fractal Dimension,&amp;quot; ''Basic Concepts in Nonlinear Dynamics and Chaos'' (workshop), Society for Chaos Theory in Psychology and the Life Sciences annual meeting, June 28, 1996, Berkeley, California, see [http://www.vanderbilt.edu/AnS/psychology/cogsci/chaos/workshop/Workshop.html], accessed 5 March 2015.&amp;lt;/ref&amp;gt; This equation is easily solved for D, yielding the ratio of logarithms (or [[natural logarithm]]s) appearing in the figures, and giving—in the Koch and other fractal cases—non-integer dimensions for these objects.&lt;br /&gt;
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In mathematical terms, the Hausdorff dimension generalizes the notion of the dimension of a real vector space. That is, the Hausdorff dimension of an n-dimensional inner product space equals n. This underlies the earlier statement that the Hausdorff dimension of a point is zero, of a line is one, etc., and that irregular sets can have noninteger Hausdorff dimensions. For instance, the Koch snowflake shown at right is constructed from an equilateral triangle; in each iteration, its component line segments are divided into 3 segments of unit length, the newly created middle segment is used as the base of a new equilateral triangle that points outward, and this base segment is then deleted to leave a final object from the iteration of unit length of 4. That is, after the first iteration, each original line segment has been replaced with N=4, where each self-similar copy is 1/S = 1/3 as long as the original. This equation is easily solved for D, yielding the ratio of logarithms (or natural logarithms) appearing in the figures, and giving—in the Koch and other fractal cases—non-integer dimensions for these objects.&lt;br /&gt;
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用数学术语来说，豪斯多夫维数概括了实向量空间维数的概念。也就是说，n 维内积空间的豪斯多夫维数等于 n。 这就是早期假设的基础，一个点的豪斯多夫维数是零，一条线是一等等，不规则集可以有非整数的豪斯多夫维数。例如，右边所示的 Koch 雪花是由一个正三角形构成的; 在每次迭代中，它的组成线段被分成单位长度的3段，新创建的中间线段被用作一个指向外部的新正三角形的基础，然后人们删除这个基础线段用来保留单位长度4的迭代中的最终对象。也就是说，在第一次迭代之后，每个原始线段都被替换为 N=4，其中每个自相似拷贝的长度是原始线段的1/S = 1/3 。这个方程很容易求解为 D，产生出现在图形中的对数(或自然对数)的比率，并给出——在 Koch 和其他分形情况下——这些对象的非整数维数。&lt;br /&gt;
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The Hausdorff dimension is a successor to the simpler, but usually equivalent, box-counting or [[Minkowski–Bouligand dimension]].&lt;br /&gt;
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The Hausdorff dimension is a successor to the simpler, but usually equivalent, box-counting or Minkowski–Bouligand dimension.&lt;br /&gt;
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豪斯多夫维数是更简单但通常等价的'''&amp;lt;font color = '#ff8000'&amp;gt;计盒维数box-counting&amp;lt;/font&amp;gt;'''或'''&amp;lt;font color = '#ff8000'&amp;gt;闵可夫斯基维数Minkowski-Bouligand&amp;lt;/font&amp;gt;'''的继承者。&lt;br /&gt;
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==Intuition概念==&lt;br /&gt;
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The intuitive concept of dimension of a geometric object ''X'' is the number of independent parameters one needs to pick out a unique point inside. However, any point specified by two parameters can be instead specified by one, because the [[cardinality]] of the [[real plane]] is equal to the cardinality of the [[real line]] (this can be seen by an [[Cantor's diagonal argument|argument]] involving interweaving the digits of two numbers to yield a single number encoding the same information). The example of a [[space-filling curve]] shows that one can even map the real line to the real plane [[Surjective function|surjectively]] (taking one real number into a pair of real numbers in a way so that all pairs of numbers are covered) and ''continuously'', so that a one-dimensional object completely fills up a higher-dimensional object.&lt;br /&gt;
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The intuitive concept of dimension of a geometric object X is the number of independent parameters one needs to pick out a unique point inside. However, any point specified by two parameters can be instead specified by one, because the cardinality of the real plane is equal to the cardinality of the real line (this can be seen by an argument involving interweaving the digits of two numbers to yield a single number encoding the same information). The example of a space-filling curve shows that one can even map the real line to the real plane surjectively (taking one real number into a pair of real numbers in a way so that all pairs of numbers are covered) and continuously, so that a one-dimensional object completely fills up a higher-dimensional object.&lt;br /&gt;
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几何对象X的尺寸的直观概念是指需要多少个独立参数才能找到一个独特的点。但是，任何由两个参数指定的点都可以由一个参数指定，因为为实平面的基数等于实线的基数(这可以通过交织两个数字以产生一个编码相同信息的单个数字看到)。'''&amp;lt;font color = '#ff8000'&amp;gt;皮亚诺曲线&amp;lt;/font&amp;gt;'''的例子表明，可以将实线完美和连续地映射到实平面(把一个实数转换成一对实数，从而覆盖所有实数对)，由此一维对象完全填充了一个高维对象。&lt;br /&gt;
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Every space filling curve hits some points multiple times, and does not have a continuous inverse. It is impossible to map two dimensions onto one in a way that is continuous and continuously invertible. The topological dimension, also called [[Lebesgue covering dimension]], explains why. This dimension is ''n'' if, in every covering of ''X'' by small open balls, there is at least one point where ''n''&amp;amp;nbsp;+&amp;amp;nbsp;1 balls overlap. For example, when one covers a line with short open intervals, some points must be covered twice, giving dimension&amp;amp;nbsp;''n''&amp;amp;nbsp;=&amp;amp;nbsp;1.&lt;br /&gt;
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Every space filling curve hits some points multiple times, and does not have a continuous inverse. It is impossible to map two dimensions onto one in a way that is continuous and continuously invertible. The topological dimension, also called Lebesgue covering dimension, explains why. This dimension is n if, in every covering of X by small open balls, there is at least one point where n&amp;amp;nbsp;+&amp;amp;nbsp;1 balls overlap. For example, when one covers a line with short open intervals, some points must be covered twice, giving dimension&amp;amp;nbsp;n&amp;amp;nbsp;=&amp;amp;nbsp;1.&lt;br /&gt;
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每条空间填充曲线都会多次击中某些点，且不存在连续的逆。将二维以连续和连续可逆的方式映射到一维是不可能的。'''&amp;lt;font color = '#ff8000'&amp;gt;拓扑维度 topological dimension&amp;lt;/font&amp;gt;'''，也被称为Lebesgue覆盖维数，解释了为什么。如果在 x 的每个小开球覆盖中，至少有一个点 n + 1个球重叠，这个维度是 n。例如，当用短的开区间覆盖一条线时，某些点必须被覆盖两次，给出维数''n''&amp;amp;nbsp;=&amp;amp;nbsp;1。&lt;br /&gt;
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But topological dimension is a very crude measure of the local size of a space (size near a point). A curve that is almost space-filling can still have topological dimension one, even if it fills up most of the area of a region. A [[fractal]] has an integer topological dimension, but in terms of the amount of space it takes up, it behaves like a higher-dimensional space.&lt;br /&gt;
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But topological dimension is a very crude measure of the local size of a space (size near a point). A curve that is almost space-filling can still have topological dimension one, even if it fills up most of the area of a region. A fractal has an integer topological dimension, but in terms of the amount of space it takes up, it behaves like a higher-dimensional space.&lt;br /&gt;
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但是，拓扑维度是对空间局部尺寸(点附近的尺寸)的一个非常粗略的度量。一条几乎是空间填充的曲线仍然可以有一维拓扑，即使它填充了一个区域的大部分面积。分形具有整数的拓扑维数，但就其所占的空间量而言，它看起来像一个更高维的空间。&lt;br /&gt;
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The Hausdorff dimension measures the local size of a space taking into account the distance between points, the [[metric space|metric]]. Consider the number ''N''(''r'') of [[ball (mathematics)|balls]] of radius at most ''r'' required to cover ''X'' completely. When ''r'' is very small, ''N''(''r'') grows polynomially with 1/''r''. For a sufficiently well-behaved  ''X'', the Hausdorff dimension is the unique number ''d'' such that N(''r'') grows as 1/''r&amp;lt;sup&amp;gt;d&amp;lt;/sup&amp;gt;'' as ''r'' approaches zero. More precisely, this defines the [[Minkowski–Bouligand dimension|box-counting dimension]], which equals the Hausdorff dimension when the value ''d'' is a critical boundary between growth rates that are insufficient to cover the space, and growth rates that are overabundant.&lt;br /&gt;
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The Hausdorff dimension measures the local size of a space taking into account the distance between points, the metric. Consider the number N(r) of balls of radius at most r required to cover X completely. When r is very small, N(r) grows polynomially with 1/r. For a sufficiently well-behaved  X, the Hausdorff dimension is the unique number d such that N(r) grows as 1/r&amp;lt;sup&amp;gt;d&amp;lt;/sup&amp;gt; as r approaches zero. More precisely, this defines the box-counting dimension, which equals the Hausdorff dimension when the value d is a critical boundary between growth rates that are insufficient to cover the space, and growth rates that are overabundant.&lt;br /&gt;
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豪斯多夫维数测量一个空间的局部大小时，会考虑到点之间距离的度量。考虑半径最大为 r 的球数 ''N'' (r) ，需要完全覆盖 ''X''。当 r 很小时，n (r)以1/''r'' 增长多项式。对于一个表现足够好的 ''X''，豪斯多夫维数是唯一的数 d，这样当 r 趋近于零时， N(r)增长为1/r&amp;lt;sup&amp;gt;d&amp;lt;/sup&amp;gt; 。更确切地说，这定义了盒子计数维度，当值 d 是不足以覆盖空间的增长率和过度充裕的增长率之间的关键边界时，它等于豪斯多夫维数。&lt;br /&gt;
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For shapes that are smooth, or shapes with a small number of corners, the shapes of traditional geometry and science, the Hausdorff dimension is an integer agreeing with the topological dimension. But [[Benoit Mandelbrot]] observed that [[fractal]]s, sets with noninteger Hausdorff dimensions, are found everywhere in nature. He observed that the proper idealization of most rough shapes you see around you is not in terms of smooth idealized shapes, but in terms of fractal idealized shapes:&lt;br /&gt;
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For shapes that are smooth, or shapes with a small number of corners, the shapes of traditional geometry and science, the Hausdorff dimension is an integer agreeing with the topological dimension. But Benoit Mandelbrot observed that fractals, sets with noninteger Hausdorff dimensions, are found everywhere in nature. He observed that the proper idealization of most rough shapes you see around you is not in terms of smooth idealized shapes, but in terms of fractal idealized shapes:&lt;br /&gt;
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对于光滑的形状，或者有少量棱角的形状，传统几何和科学的形状，豪斯多夫维数是一个整数，与拓扑维度一致。但是伯努·曼德布洛特观察到分形---- 具有非整数豪斯多夫维数的集合---- 在自然界中随处可见。他观察到，我们周围大多数粗糙形状的理想化不是光滑的理想化形状，而是分形理想化形状:&lt;br /&gt;
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&amp;lt;blockquote&amp;gt;Clouds are not spheres, mountains are not cones, coastlines are not circles, and bark is not smooth, nor does lightning travel in a straight line.&amp;lt;ref name=&amp;quot;mandelbrot&amp;quot;&amp;gt;{{cite book   | last = Mandelbrot   | first = Benoît   | authorlink = Benoit Mandelbrot   | title = The Fractal Geometry of Nature   | publisher = W. H. Freeman   | series = Lecture notes in mathematics 1358   | year = 1982   | doi =    | isbn = 0-7167-1186-9   | url-access = registration   | url = https://archive.org/details/fractalgeometryo00beno   }}&amp;lt;/ref&amp;gt;&amp;lt;/blockquote&amp;gt;&lt;br /&gt;
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&amp;lt;blockquote&amp;gt;Clouds are not spheres, mountains are not cones, coastlines are not circles, and bark is not smooth, nor does lightning travel in a straight line.&amp;lt;/blockquote&amp;gt;&lt;br /&gt;
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&amp;lt;blockquote&amp;gt;云不是球体，山不是锥体，海岸线不是圆圈，树皮不平滑，闪电也不是直线运动。 &amp;lt;/blockquote&amp;gt;&lt;br /&gt;
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For fractals that occur in nature, the Hausdorff and [[Minkowski–Bouligand dimension|box-counting dimension]] coincide. The [[packing dimension]] is yet another similar notion which gives the same value for many shapes, but there are well documented exceptions where all these dimensions differ.&lt;br /&gt;
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For fractals that occur in nature, the Hausdorff and box-counting dimension coincide. The packing dimension is yet another similar notion which gives the same value for many shapes, but there are well documented exceptions where all these dimensions differ.&lt;br /&gt;
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对于自然界中出现的分形，豪斯多夫维数和盒计数维数是一致的。封装尺寸是另一个类似的概念，它给出了许多形状相同的值，但是在所有这些尺寸不同的情况，都做了很好的说明。&lt;br /&gt;
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==Formal definitions形式化定义==&lt;br /&gt;
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{{unreferenced section|date=March 2015}}&lt;br /&gt;
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===Hausdorff content豪斯多夫集===&lt;br /&gt;
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Let ''X'' be a [[metric space]]. If ''S'' ⊂ ''X'' and ''d'' ∈ [0, ∞), the ''d''-dimensional '''unlimited Hausdorff content''' of ''S'' is defined by&lt;br /&gt;
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Let X be a metric space. If S ⊂ X and d ∈ [0, ∞), the d-dimensional unlimited Hausdorff content of S is defined by&lt;br /&gt;
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设 ''X''是度量空间。若''S'' ⊂ ''X'' 和 ''d'' ∈ [0, ∞) ，则 ''S'' 的''d''维无限 豪斯多夫集定义为&lt;br /&gt;
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:&amp;lt;math&amp;gt;C_H^d(S):=\inf\Bigl\{\sum_i r_i^d:\text{ there is a cover of } S\text{ by balls with radii }r_i&amp;gt;0\Bigr\}.&amp;lt;/math&amp;gt;&lt;br /&gt;
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&amp;lt;math&amp;gt;C_H^d(S):=\inf\Bigl\{\sum_i r_i^d:\text{ there is a cover of } S\text{ by balls with radii }r_i&amp;gt;0\Bigr\}.&amp;lt;/math&amp;gt;&lt;br /&gt;
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&amp;lt;math&amp;gt;C_H^d(S):=\inf\Bigl\{\sum_i r_i^d:\text{ there is a cover of } S\text{ by balls with radii }r_i&amp;gt;0\Bigr\}.&amp;lt;/math&amp;gt;&lt;br /&gt;
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In other words, &amp;lt;math&amp;gt;C_H^d(S)&amp;lt;/math&amp;gt; is the [[infimum]] of the set of numbers &amp;lt;math&amp;gt;\delta \geq 0&amp;lt;/math&amp;gt; such that there is some (indexed) collection of [[ball (mathematics)|ball]]s &amp;lt;math&amp;gt;\{B(x_i,r_i):i\in I\}&amp;lt;/math&amp;gt; covering ''S'' with ''r&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;''&amp;amp;nbsp;&amp;gt;&amp;amp;nbsp;0 for each ''i''&amp;amp;nbsp;∈&amp;amp;nbsp;''I'' that satisfies &amp;lt;math&amp;gt;\sum_{i\in I} r_i^d&amp;lt;\delta &amp;lt;/math&amp;gt;. (Here, we use the standard convention that [[infimum|inf&amp;amp;nbsp;Ø&amp;amp;nbsp;=&amp;amp;nbsp;∞]].)&lt;br /&gt;
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In other words, &amp;lt;math&amp;gt;C_H^d(S)&amp;lt;/math&amp;gt; is the infimum of the set of numbers &amp;lt;math&amp;gt;\delta \geq 0&amp;lt;/math&amp;gt; such that there is some (indexed) collection of balls &amp;lt;math&amp;gt;\{B(x_i,r_i):i\in I\}&amp;lt;/math&amp;gt; covering S with r&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;&amp;amp;nbsp;&amp;gt;&amp;amp;nbsp;0 for each i&amp;amp;nbsp;∈&amp;amp;nbsp;I that satisfies &amp;lt;math&amp;gt;\sum_{i\in I} r_i^d&amp;lt;\delta &amp;lt;/math&amp;gt;. (Here, we use the standard convention that inf&amp;amp;nbsp;Ø&amp;amp;nbsp;=&amp;amp;nbsp;∞.)&lt;br /&gt;
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换句话说，&amp;lt;math&amp;gt;C_H^d(S)&amp;lt;/math&amp;gt; 是数字集合&amp;lt;math&amp;gt;\delta \geq 0&amp;lt;/math&amp;gt;的下确界，使得在 ''i''&amp;amp;nbsp;∈&amp;amp;nbsp中存在一些球集合 &amp;lt;math&amp;gt;\{B(x_i,r_i):i\in I\}&amp;lt;/math&amp;gt;  i 包含 s，对于每个 ''r&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;''&amp;amp;nbsp;&amp;gt;&amp;amp;nbsp;0 满足 i 中的和&amp;lt;math&amp;gt;\sum_{i\in I} r_i^d&amp;lt;\delta &amp;lt;/math&amp;gt; (在这里，我们使用inf&amp;amp;nbsp;Ø&amp;amp;nbsp;=&amp;amp;nbsp;∞ )的标准约定。&lt;br /&gt;
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===Hausdorff measurement豪斯多夫分形测量===&lt;br /&gt;
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The Hausdorff outer measure is different from the unbounded Hausdorf content in that rather than considering all possible coverings of ''S'', we see what happens when the sizes of the balls go to zero. This is  for &amp;lt;math&amp;gt;d \geq 0 &amp;lt;/math&amp;gt;, we define the ''d''-dimensional Hausdorff outer measure of ''S'' as&lt;br /&gt;
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The Hausdorff outer measure is different from the unbounded Hausdorf content in that rather than considering all possible coverings of S, we see what happens when the sizes of the balls go to zero. This is  for &amp;lt;math&amp;gt;d \geq 0 &amp;lt;/math&amp;gt;, we define the d-dimensional Hausdorff outer measure of S as&lt;br /&gt;
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豪斯多夫外测度不同于无界的豪斯多夫，因为我们不考虑 s 的所有可能，我们看到当球的大小为零时会发生什么。这是为了数学  &amp;lt;math&amp;gt;d \geq 0 &amp;lt;/math&amp;gt;，我们定义了  ''S''的 ''d''维豪斯多夫Hausdorff 外测度为&lt;br /&gt;
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:&amp;lt;math&amp;gt; \mathcal{H}^d(S):=\lim_{r \to 0} \inf\Bigl\{\sum_i r_i^d:\text{ there is a cover of } S\text{ by balls with radii } 0 &amp;lt; r_i &amp;lt; r\Bigr\}.&amp;lt;/math&amp;gt;&lt;br /&gt;
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&amp;lt;math&amp;gt; \mathcal{H}^d(S):=\lim_{r \to 0} \inf\Bigl\{\sum_i r_i^d:\text{ there is a cover of } S\text{ by balls with radii } 0 &amp;lt; r_i &amp;lt; r\Bigr\}.&amp;lt;/math&amp;gt;&lt;br /&gt;
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&amp;lt;math&amp;gt; \mathcal{H}^d(S):=\lim_{r \to 0} \inf\Bigl\{\sum_i r_i^d:\text{有一个面} S\text{ 球 } 0 &amp;lt; r_i &amp;lt; r\Bigr\}.&amp;lt;/math&amp;gt;&lt;br /&gt;
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===Hausdorff dimension豪斯多夫维数===&lt;br /&gt;
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The '''Hausdorff dimension''' of ''X'' is defined by&lt;br /&gt;
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The Hausdorff dimension of X is defined by&lt;br /&gt;
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X 的豪斯多夫维数定义为&lt;br /&gt;
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:&amp;lt;math&amp;gt;\dim_{\operatorname{H}}(X):=\inf\{d\ge 0: \mathcal{H}^d(X)=0\}.&amp;lt;/math&amp;gt;&lt;br /&gt;
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&amp;lt;math&amp;gt;\dim_{\operatorname{H}}(X):=\inf\{d\ge 0: \mathcal{H}^d(X)=0\}.&amp;lt;/math&amp;gt;&lt;br /&gt;
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Equivalently, dim&amp;lt;sub&amp;gt;H&amp;lt;/sub&amp;gt;(''X'') may be defined as the [[infimum]] of the set of ''d'' ∈ [0, ∞) such that the ''d''-dimensional [[Hausdorff measure]] of ''X'' is zero. This is the same as the supremum of the set of ''d''&amp;amp;nbsp;∈&amp;amp;nbsp;[0,&amp;amp;nbsp;∞) such that the ''d''-dimensional Hausdorff measure of ''X'' is infinite (except that when this latter set of numbers ''d'' is empty the Hausdorff dimension is zero).&lt;br /&gt;
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Equivalently, dim&amp;lt;sub&amp;gt;H&amp;lt;/sub&amp;gt;(X) may be defined as the infimum of the set of d ∈ [0, ∞) such that the d-dimensional Hausdorff measure of X is zero. This is the same as the supremum of the set of d&amp;amp;nbsp;∈&amp;amp;nbsp;[0,&amp;amp;nbsp;∞) such that the d-dimensional Hausdorff measure of X is infinite (except that when this latter set of numbers d is empty the Hausdorff dimension is zero).&lt;br /&gt;
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等价地，dim &amp;lt;sub&amp;gt;H&amp;lt;/sub&amp;gt;(''X'')可定义为 ''d'' ∈ [0, ∞) 集的下确界，使得''X'' 的''d''-维 [[豪斯多夫测度]] 为零。这与 ''d''&amp;amp;nbsp;∈&amp;amp;nbsp;[0,&amp;amp;nbsp;∞)的集合的上确界相同，因此''X''的 d 维豪斯多夫测度是无限的(除非后一个集合 ''d'' 是空的，豪斯多夫维数为零)。&lt;br /&gt;
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==Examples实例==&lt;br /&gt;
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[[Image:Sierpinski deep.svg|thumb|250px|Dimension of a further [[fractal]] example. The [[Sierpinski triangle]], an object with Hausdorff dimension of log(3)/log(2)≈1.58.&amp;lt;ref name=ClaytonSCTPLS96/&amp;gt;]]&lt;br /&gt;
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Dimension of a further [[fractal example. The Sierpinski triangle, an object with Hausdorff dimension of log(3)/log(2)≈1.58.]]&lt;br /&gt;
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[[Image:谢尔宾斯基三角形 deep.svg|thumb|250px|进一步的[[分形维数]]的例子，进一步的分形维数的例子是谢尔宾斯基三角形，它是一个豪斯多夫维数为log(3)/log(2)≈1.58.&amp;lt;ref name=ClaytonSCTPLS96/&amp;gt;的物体]]&lt;br /&gt;
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* [[Countable set]]s have Hausdorff dimension 0.&amp;lt;ref name=&amp;quot;schleicher&amp;quot;&amp;gt;{{cite journal |last1=Schleicher |first1=Dierk |title=Hausdorff Dimension, Its Properties, and Its Surprises |journal=The American Mathematical Monthly |date=June 2007 |volume=114 |issue=6 |pages=509–528 |doi=10.1080/00029890.2007.11920440 |language=en |issn=0002-9890|arxiv=math/0505099 }}&amp;lt;/ref&amp;gt;&lt;br /&gt;
*[[可数集]]拥有豪斯多夫维数0.&amp;lt;ref name=&amp;quot;schleicher&amp;quot;&amp;gt;{{cite journal |last1=Schleicher |first1=Dierk |title=豪斯多夫维数, Its Properties, and Its Surprises |journal=The American Mathematical Monthly美国数学期刊 |date=June 2007 |volume=114 |issue=6 |pages=509–528 |doi=10.1080/00029890.2007.11920440 |language=en |issn=0002-9890|arxiv=math/0505099 }}&amp;lt;/ref&amp;gt;&lt;br /&gt;
* The [[Euclidean space]] ℝ&amp;lt;sup&amp;gt;''n''&amp;lt;/sup&amp;gt; has Hausdorff dimension ''n'', and the circle '''S'''&amp;lt;sup&amp;gt;1&amp;lt;/sup&amp;gt; has Hausdorff dimension 1.&amp;lt;ref name=&amp;quot;schleicher&amp;quot; /&amp;gt;&lt;br /&gt;
*[[教育空间]] ℝ&amp;lt;sup&amp;gt;''n''&amp;lt;/sup&amp;gt; 有豪斯多夫维数 ''n''，循环'''S'''&amp;lt;sup&amp;gt;1&amp;lt;/sup&amp;gt; 拥有豪斯多夫维数1.&amp;lt;ref name=&amp;quot;schleicher&amp;quot; /&amp;gt;&lt;br /&gt;
* [[Fractal]]s often are spaces whose Hausdorff dimension strictly exceeds the [[topological dimension]].&amp;lt;ref name=&amp;quot;mandelbrot&amp;quot; /&amp;gt; For example, the [[Cantor set]], a zero-dimensional topological space, is a union of two copies of itself, each copy shrunk by a factor 1/3; hence, it can be shown that its Hausdorff dimension is ln(2)/ln(3)&amp;amp;nbsp;≈&amp;amp;nbsp;0.63.&amp;lt;ref&amp;gt;{{cite book | last=Falconer | first = Kenneth |title=Fractal Geometry: Mathematical Foundations and Applications | publisher=[[John Wiley and Sons]] | edition=2nd | year=2003}}&amp;lt;/ref&amp;gt; The [[Sierpinski triangle]] is a union of three copies of itself, each copy shrunk by a factor of&amp;amp;nbsp;1/2; this yields a Hausdorff dimension of ln(3)/ln(2)&amp;amp;nbsp;≈&amp;amp;nbsp;1.58.&amp;lt;ref name=CampbellAnnenberg15/&amp;gt; These Hausdorff dimensions are related to the &amp;quot;critical exponent&amp;quot; of the [[Master theorem (analysis of algorithms)|Master theorem]] for solving [[Recurrence relation|recurrence relations]] in the [[analysis of algorithms]].&lt;br /&gt;
*[[分形]]一般是那些豪斯多夫维数直接超过其拓扑维数的空间。例如[[康托尔集]]是一个o维拓扑空间，由两个自己复制而成，每一个复制品都是原来的三分之一，因此它的豪斯多夫维数是 ln(2)/ln(3)&amp;amp;nbsp;≈&amp;amp;nbsp;0.63。&amp;lt;ref&amp;gt;{{cite book | last=Falconer | first = Kenneth |title=Fractal Geometry: Mathematical Foundations and Applications | publisher=[[John Wiley and Sons]] | edition=2nd | year=2003}}&amp;lt;/ref&amp;gt;一个[[谢尔宾斯基三角]]是他自身三个复制的组合。每一个是原来的&amp;amp;nbsp;1/2，它的豪斯多夫维数ln(3)/ln(2)&amp;amp;nbsp;≈&amp;amp;nbsp;1.58。&amp;lt;ref name=CampbellAnnenberg15/&amp;gt;在递归算法中解决递归关系时，这些豪斯多夫维数与[[算法分析主定理]]的临界指标相联系。&lt;br /&gt;
* [[Space-filling curve]]s like the [[Peano curve]] have the same Hausdorff dimension as the space they fill.&lt;br /&gt;
*[[空间填充曲线]]拥有和他们填充空间同样的豪斯多夫维数，如[[皮亚诺曲线]]。&lt;br /&gt;
* The trajectory of [[Brownian motion]] in dimension 2 and above is conjectured to be Hausdorff dimension 2.&amp;lt;ref&amp;gt;{{cite book | last=Morters | first=Peres | title= Brownian Motion | publisher=[[Cambridge University Press]] | year=2010 }}&amp;lt;/ref&amp;gt;&lt;br /&gt;
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[[image:Great Britain Hausdorff.svg|thumb|250px|Estimating the Hausdorff dimension of the [[How Long Is the Coast of Britain? Statistical Self-Similarity and Fractional Dimension|coast of Great Britain]]]]&lt;br /&gt;
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coast of Great Britain]]&lt;br /&gt;
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[[大不列颠海岸&lt;br /&gt;
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* 刘易斯·弗赖伊·理查森[[Lewis Fry Richardson]] has performed detailed experiments to measure the approximate Hausdorff dimension for various coastlines. His results have varied from 1.02 for the coastline of [[South Africa]] to 1.25 for the west coast of [[Great Britain]].&amp;lt;ref name=&amp;quot;mandelbrot&amp;quot; /&amp;gt;&lt;br /&gt;
*刘易斯·弗赖伊·理查森（Lewis Fry Richardson）已经通过豪斯多夫维数去测量了很多海岸线。它的结果涵盖从1.02的南非海岸线到1.25的大英帝国西海岸模型。]]&lt;br /&gt;
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==Properties of Hausdorff dimension豪斯多夫维数特性==&lt;br /&gt;
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{{refimprove section|date=March 2015}}&lt;br /&gt;
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=== Hausdorff dimension and inductive dimension 豪斯多夫维数和归纳维数===&lt;br /&gt;
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Let ''X'' be an arbitrary [[Separable space|separable]] metric space. There is a [[topology|topological]] notion of [[inductive dimension]] for ''X'' which is defined recursively. It is always an integer (or +∞) and is denoted dim&amp;lt;sub&amp;gt;ind&amp;lt;/sub&amp;gt;(''X'').&lt;br /&gt;
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Let X be an arbitrary separable metric space. There is a topological notion of inductive dimension for X which is defined recursively. It is always an integer (or +∞) and is denoted dim&amp;lt;sub&amp;gt;ind&amp;lt;/sub&amp;gt;(X).&lt;br /&gt;
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设''X'' 是[[任意可分度量空间]]。对于''X'' 有一个递归定义的归纳维数拓扑概念。它总是一个整数(或 + ∞) ，并且表示dim&amp;lt;sub&amp;gt;ind&amp;lt;/sub&amp;gt;(''X'')。&lt;br /&gt;
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'''Theorem'''. Suppose ''X'' is non-empty. Then &lt;br /&gt;
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Theorem. Suppose X is non-empty. Then &lt;br /&gt;
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'''定理'''：假设''X'' 是非空的。那么&lt;br /&gt;
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:&amp;lt;math&amp;gt; \dim_{\mathrm{Haus}}(X) \geq \dim_{\operatorname{ind}}(X). &amp;lt;/math&amp;gt;&lt;br /&gt;
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&amp;lt;math&amp;gt; \dim_{\mathrm{Haus}}(X) \geq \dim_{\operatorname{ind}}(X). &amp;lt;/math&amp;gt;&lt;br /&gt;
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Moreover,&lt;br /&gt;
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Moreover,&lt;br /&gt;
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此外,&lt;br /&gt;
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&amp;lt;math&amp;gt; \inf_Y \dim_{\operatorname{Haus}}(Y) =\dim_{\operatorname{ind}}(X), &amp;lt;/math&amp;gt;&lt;br /&gt;
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&amp;lt;math&amp;gt; \inf_Y \dim_{\operatorname{Haus}}(Y) =\dim_{\operatorname{ind}}(X), &amp;lt;/math&amp;gt;&lt;br /&gt;
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where ''Y'' ranges over metric spaces [[homeomorphic]] to ''X''. In other words, ''X'' and ''Y'' have the same underlying set of points and the metric ''d''&amp;lt;sub&amp;gt;''Y''&amp;lt;/sub&amp;gt; of ''Y'' is topologically equivalent to ''d''&amp;lt;sub&amp;gt;''X''&amp;lt;/sub&amp;gt;.&lt;br /&gt;
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where Y ranges over metric spaces homeomorphic to X. In other words, X and Y have the same underlying set of points and the metric d&amp;lt;sub&amp;gt;Y&amp;lt;/sub&amp;gt; of Y is topologically equivalent to d&amp;lt;sub&amp;gt;X&amp;lt;/sub&amp;gt;.&lt;br /&gt;
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其中''Y''是度量空间同胚到 ''X''的范围。换句话说， ''X''和 ''Y''具有相同的基本点集，''Y''的度规''d''&amp;lt;sub&amp;gt;''Y''&amp;lt;/sub&amp;gt; 的子拓扑等价于''d''&amp;lt;sub&amp;gt;''X''&amp;lt;/sub&amp;gt;。&lt;br /&gt;
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&lt;br /&gt;
&lt;br /&gt;
These results were originally established by [[Edward Szpilrajn]] (1907–1976), e.g., see Hurewicz and Wallman, Chapter VII.{{full citation needed|date=March 2015}}&lt;br /&gt;
&lt;br /&gt;
These results were originally established by Edward Szpilrajn (1907–1976), e.g., see Hurewicz and Wallman, Chapter VII.&lt;br /&gt;
&lt;br /&gt;
这些结果最初是由 [[Edward Szpilrajn]] (1907–1976)建立的,  参见 Hurewicz and Wallman, Chapter VII.{{full citation needed|date=March 2015}}第七章。&lt;br /&gt;
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=== Hausdorff dimension and Minkowski dimension 豪斯多夫维数和闵可夫斯基维度===&lt;br /&gt;
&lt;br /&gt;
The [[Minkowski dimension]] is similar to, and at least as large as, the Hausdorff dimension, and they are equal in many situations. However, the set of [[rational number|rational]] points in [0, 1] has Hausdorff dimension zero and Minkowski dimension one. There are also compact sets for which the Minkowski dimension is strictly larger than the Hausdorff dimension.&lt;br /&gt;
&lt;br /&gt;
The Minkowski dimension is similar to, and at least as large as, the Hausdorff dimension, and they are equal in many situations. However, the set of rational points in [0, 1] has Hausdorff dimension zero and Minkowski dimension one. There are also compact sets for which the Minkowski dimension is strictly larger than the Hausdorff dimension.&lt;br /&gt;
&lt;br /&gt;
[[闵可夫斯基维数]]与豪斯多夫维数相似，至少和它一样大，而且在许多情况下是相等的。然而，[0,1]中有理点集的豪斯多夫维数为0，闵可夫斯基维数为1。还有一些紧集的闵可夫斯基维数绝对大于豪斯多夫维数。&lt;br /&gt;
&lt;br /&gt;
=== Hausdorff dimensions and Frostman measures 豪斯多夫维度和弗洛斯曼测度===&lt;br /&gt;
&lt;br /&gt;
If there is a [[measure (mathematics)|measure]] μ defined on [[Borel measure|Borel]] subsets of a metric space ''X'' such that ''μ''(''X'') &amp;gt; 0 and ''μ''(''B''(''x'', ''r'')) ≤ ''r&amp;lt;sup&amp;gt;s&amp;lt;/sup&amp;gt;'' holds for some constant ''s'' &amp;gt; 0 and for every ball ''B''(''x'', ''r'') in ''X'', then dim&amp;lt;sub&amp;gt;Haus&amp;lt;/sub&amp;gt;(''X'') ≥ ''s''. A partial converse is provided by [[Frostman's lemma]].{{citation needed|date=March 2015}}&amp;lt;ref&amp;gt;This Wikipedia article also discusses further useful characterizations of the Hausdorff dimension.{{clarify|date=March 2015}}&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
If there is a measure μ defined on Borel subsets of a metric space X such that μ(X) &amp;gt; 0 and μ(B(x, r)) ≤ r&amp;lt;sup&amp;gt;s&amp;lt;/sup&amp;gt; holds for some constant s &amp;gt; 0 and for every ball B(x, r) in X, then dim&amp;lt;sub&amp;gt;Haus&amp;lt;/sub&amp;gt;(X) ≥ s. A partial converse is provided by Frostman's lemma.&lt;br /&gt;
&lt;br /&gt;
如果在度量空间 ''X'' 的 Borel 子集上定义一个测度 μ，使得''μ''(''X'') &amp;gt; 0 和''μ''(''B''(''x'', ''r'')) ≤ ''r&amp;lt;sup&amp;gt;s&amp;lt;/sup&amp;gt;''，对于某个常数 ''s'' &amp;gt; 0  和 ''X'' 中的每个球 ''B''(''x'', ''r'') 成立，则 dim&amp;lt;sub&amp;gt;Haus&amp;lt;/sub&amp;gt;(''X'') ≥ ''s'' 。 部分逆向转换由弗洛斯曼引理定义。&lt;br /&gt;
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=== Behaviour under unions and products ===&lt;br /&gt;
&lt;br /&gt;
If &amp;lt;math&amp;gt;X=\bigcup_{i\in I}X_i&amp;lt;/math&amp;gt; is a finite or countable union, then&lt;br /&gt;
&lt;br /&gt;
If &amp;lt;math&amp;gt;X=\bigcup_{i\in I}X_i&amp;lt;/math&amp;gt; is a finite or countable union, then&lt;br /&gt;
&lt;br /&gt;
如果 &amp;lt;math&amp;gt;X=\bigcup_{i\in I}X_i&amp;lt;/math&amp;gt; 是一个有限或可数的联合，则&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \dim_{\operatorname{Haus}}(X) =\sup_{i\in I} \dim_{\operatorname{Haus}}(X_i).&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \dim_{\operatorname{Haus}}(X) =\sup_{i\in I} \dim_{\operatorname{Haus}}(X_i).&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
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This can be verified directly from the definition.&lt;br /&gt;
&lt;br /&gt;
This can be verified directly from the definition.&lt;br /&gt;
&lt;br /&gt;
这可以直接从定义得到验证。&lt;br /&gt;
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If ''X'' and ''Y'' are non-empty metric spaces, then the Hausdorff dimension of their product satisfies&amp;lt;ref&amp;gt;{{cite journal |author=Marstrand, J. M. |title=The dimension of Cartesian product sets |journal=Proc. Cambridge Philos. Soc. |volume=50 |issue=3 |pages=198–202 |year=1954 |doi=10.1017/S0305004100029236 |bibcode = 1954PCPS...50..198M }}&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
If X and Y are non-empty metric spaces, then the Hausdorff dimension of their product satisfies&lt;br /&gt;
&lt;br /&gt;
如果 ''X'' 和''Y''是非空度量空间，那么它们乘积的豪斯多夫维数满足&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt; \dim_{\operatorname{Haus}}(X\times Y)\ge \dim_{\operatorname{Haus}}(X)+ \dim_{\operatorname{Haus}}(Y).&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \dim_{\operatorname{Haus}}(X\times Y)\ge \dim_{\operatorname{Haus}}(X)+ \dim_{\operatorname{Haus}}(Y).&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
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This inequality can be strict. It is possible to find two sets of dimension 0 whose product has dimension 1.&amp;lt;ref&amp;gt;{{cite book  | last = Falconer  | first = Kenneth J.  | title = Fractal geometry. Mathematical foundations and applications  | publisher = John Wiley &amp;amp; Sons, Inc., Hoboken, New Jersey  | year = 2003  | doi =   | isbn = }}&amp;lt;/ref&amp;gt; In the opposite direction, it is known that when ''X'' and ''Y'' are Borel subsets of '''R'''&amp;lt;sup&amp;gt;''n''&amp;lt;/sup&amp;gt;, the Hausdorff dimension of ''X'' × ''Y'' is bounded from above by the Hausdorff dimension of ''X'' plus the [[packing dimension|upper packing dimension]] of ''Y''. These facts are discussed in Mattila (1995).&lt;br /&gt;
&lt;br /&gt;
This inequality can be strict. It is possible to find two sets of dimension 0 whose product has dimension 1. In the opposite direction, it is known that when X and Y are Borel subsets of R&amp;lt;sup&amp;gt;n&amp;lt;/sup&amp;gt;, the Hausdorff dimension of X × Y is bounded from above by the Hausdorff dimension of X plus the upper packing dimension of Y. These facts are discussed in Mattila (1995).&lt;br /&gt;
&lt;br /&gt;
这种不平等可以是绝对的。有可能找到两个维数为0的集合，其乘积的维数为1。相反，我们知道当''X''和''Y''是 '''R'''&amp;lt;sup&amp;gt;''n''&amp;lt;/sup&amp;gt;的 Borel 子集时， ''X'' × ''Y''的豪斯多夫维数从上面以 ''X''的豪斯多夫维数加上 ''Y''的填充维数为界。Mattila (1995)曾就这些情况进行了讨论。&lt;br /&gt;
&lt;br /&gt;
==Self-similar sets自相似集合==&lt;br /&gt;
&lt;br /&gt;
{{refimprove section|date=March 2015}}&lt;br /&gt;
&lt;br /&gt;
Many sets defined by a self-similarity condition have dimensions which can be determined explicitly. Roughly, a set ''E'' is self-similar if it is the fixed point of a set-valued transformation ψ, that is ψ(''E'') = ''E'', although the exact definition is given below.&lt;br /&gt;
&lt;br /&gt;
Many sets defined by a self-similarity condition have dimensions which can be determined explicitly. Roughly, a set E is self-similar if it is the fixed point of a set-valued transformation ψ, that is ψ(E) = E, although the exact definition is given below.&lt;br /&gt;
&lt;br /&gt;
许多由自相似条件定义的集合具有可以显式确定的维数。粗略地说，集合''E'' 是自相似的，如果它是集值ψ变换的不动点，即ψ(''E'') = ''E''，尽管下面给出了确切的定义。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&amp;lt;blockquote&amp;gt;'''Theorem'''. Suppose&lt;br /&gt;
&lt;br /&gt;
&amp;lt;blockquote&amp;gt;Theorem. Suppose&lt;br /&gt;
&lt;br /&gt;
&amp;lt;blockquote&amp;gt;'''定理'''：假设&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt; \psi_i: \mathbf{R}^n \rightarrow \mathbf{R}^n, \quad i=1, \ldots , m &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \psi_i: \mathbf{R}^n \rightarrow \mathbf{R}^n, \quad i=1, \ldots , m &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
are [[Contraction mapping|contractive]] mappings on '''R'''&amp;lt;sup&amp;gt;''n''&amp;lt;/sup&amp;gt; with contraction constant ''r&amp;lt;sub&amp;gt;j&amp;lt;/sub&amp;gt;'' &amp;lt; 1. Then there is a unique ''non-empty'' compact set ''A'' such that&lt;br /&gt;
&lt;br /&gt;
are contractive mappings on R&amp;lt;sup&amp;gt;n&amp;lt;/sup&amp;gt; with contraction constant r&amp;lt;sub&amp;gt;j&amp;lt;/sub&amp;gt; &amp;lt; 1. Then there is a unique non-empty compact set A such that&lt;br /&gt;
&lt;br /&gt;
是'''R'''&amp;lt;sup&amp;gt;''n''&amp;lt;/sup&amp;gt;上的压缩常数''r&amp;lt;sub&amp;gt;j&amp;lt;/sub&amp;gt;'&amp;lt; 1的压缩映射。然后有一个唯一的非空紧集A &lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt; A = \bigcup_{i=1}^m \psi_i (A). &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; A = \bigcup_{i=1}^m \psi_i (A). &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&amp;lt;/blockquote&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;/blockquote&amp;gt;&lt;br /&gt;
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&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The theorem follows from [[Stefan Banach]]'s [[Contractive mapping theorem|contractive mapping fixed point theorem]] applied to the complete metric space of non-empty compact subsets of '''R'''&amp;lt;sup&amp;gt;''n''&amp;lt;/sup&amp;gt; with the [[Hausdorff distance]].&amp;lt;ref&amp;gt;{{cite book |author=Falconer, K. J. |title=The Geometry of Fractal Sets |publisher=Cambridge University Press |location=Cambridge, UK |year=1985 |isbn=0-521-25694-1 |chapter=Theorem 8.3}}&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
The theorem follows from Stefan Banach's contractive mapping fixed point theorem applied to the complete metric space of non-empty compact subsets of R&amp;lt;sup&amp;gt;n&amp;lt;/sup&amp;gt; with the Hausdorff distance.&lt;br /&gt;
&lt;br /&gt;
这个定理来源于 Stefan Banach 的压缩映射不动点定理，该定理应用于 具有豪斯多夫距离的'''R'''&amp;lt;sup&amp;gt;''n''&amp;lt;/sup&amp;gt; 的非空紧子集的完整度量空间。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
===The open set condition开集条件===&lt;br /&gt;
&lt;br /&gt;
To determine the dimension of the self-similar set ''A'' (in certain cases), we need a technical condition called the ''open set condition'' (OSC) on the sequence of contractions ψ&amp;lt;sub&amp;gt;''i''&amp;lt;/sub&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
To determine the dimension of the self-similar set A (in certain cases), we need a technical condition called the open set condition (OSC) on the sequence of contractions ψ&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
为了确定自相似集''A'' 的维数(在某些情况下) ，我们需要一个关于收缩序列的称为''开集条件''(OSC)的技术条件ψ&amp;lt;sub&amp;gt;''i''&amp;lt;/sub&amp;gt;。&lt;br /&gt;
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&lt;br /&gt;
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There is a relatively compact open set ''V'' such that&lt;br /&gt;
&lt;br /&gt;
There is a relatively compact open set V such that&lt;br /&gt;
&lt;br /&gt;
有一个相对紧的开集''V''&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt; \bigcup_{i=1}^m\psi_i (V) \subseteq V, &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \bigcup_{i=1}^m\psi_i (V) \subseteq V, &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
where the sets in union on the left are pairwise [[disjoint sets|disjoint]].&lt;br /&gt;
&lt;br /&gt;
where the sets in union on the left are pairwise disjoint.&lt;br /&gt;
&lt;br /&gt;
左边并集的集合成对不相交。&lt;br /&gt;
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&lt;br /&gt;
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The open set condition is a separation condition that ensures the images ψ&amp;lt;sub&amp;gt;''i''&amp;lt;/sub&amp;gt;(''V'') do not overlap &amp;quot;too much&amp;quot;.&lt;br /&gt;
&lt;br /&gt;
The open set condition is a separation condition that ensures the images ψ&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;(V) do not overlap &amp;quot;too much&amp;quot;.&lt;br /&gt;
&lt;br /&gt;
开集条件是保证图像ψ&amp;lt;sub&amp;gt;''i''&amp;lt;/sub&amp;gt;(''V'') 不重叠“太多”的分离条件。&lt;br /&gt;
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'''Theorem'''. Suppose the open set condition holds and each ψ&amp;lt;sub&amp;gt;''i''&amp;lt;/sub&amp;gt; is a similitude, that is a composition of an [[isometry]] and a [[dilation (metric space)|dilation]] around some point. Then the unique fixed point of ψ is a set whose Hausdorff dimension is ''s'' where ''s'' is the unique solution of&amp;lt;ref&amp;gt;{{cite journal | last=Hutchinson | first=John E. | title=Fractals and self similarity | journal=Indiana Univ. Math. J. | volume=30 | year=1981 | pages=713–747 | doi=10.1512/iumj.1981.30.30055 | issue=5 | doi-access=free }}&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
Theorem. Suppose the open set condition holds and each ψ&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt; is a similitude, that is a composition of an isometry and a dilation around some point. Then the unique fixed point of ψ is a set whose Hausdorff dimension is s where s is the unique solution of&lt;br /&gt;
&lt;br /&gt;
'''定理'''假设开集条件成立，并且每个ψ&amp;lt;sub&amp;gt;''i''&amp;lt;/sub&amp;gt; 是一个相似度，即等距和某个点周围的膨胀的组合。。那么唯一的不动点是Hausdorff维数为 ''s'' 的集合，其中  ''s'' 是 ''s'' &amp;lt;ref&amp;gt;{{cite journal | last=Hutchinson | first=John E. | title=Fractals and self similarity | journal=Indiana Univ. Math. J. | volume=30 | year=1981 | pages=713–747 | doi=10.1512/iumj.1981.30.30055 | issue=5 | doi-access=free }}&amp;lt;/ref&amp;gt;的唯一解&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt; \sum_{i=1}^m r_i^s = 1. &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \sum_{i=1}^m r_i^s = 1. &amp;lt;/math&amp;gt;&lt;br /&gt;
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The contraction coefficient of a similitude is the magnitude of the dilation.&lt;br /&gt;
&lt;br /&gt;
The contraction coefficient of a similitude is the magnitude of the dilation.&lt;br /&gt;
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相似物的收缩系数就是膨胀的大小。&lt;br /&gt;
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&lt;br /&gt;
We can use this theorem to compute the Hausdorff dimension of the Sierpinski triangle (or sometimes called Sierpinski gasket). Consider three [[non-collinear points]] ''a''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;, ''a''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;, ''a''&amp;lt;sub&amp;gt;3&amp;lt;/sub&amp;gt; in the plane '''R'''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; and let ψ&amp;lt;sub&amp;gt;''i''&amp;lt;/sub&amp;gt; be the dilation of ratio 1/2 around ''a&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;''. The unique non-empty fixed point of the corresponding mapping ψ is a Sierpinski gasket and the dimension ''s'' is the unique solution of&lt;br /&gt;
&lt;br /&gt;
We can use this theorem to compute the Hausdorff dimension of the Sierpinski triangle (or sometimes called Sierpinski gasket). Consider three non-collinear points a&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;, a&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;, a&amp;lt;sub&amp;gt;3&amp;lt;/sub&amp;gt; in the plane R&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; and let ψ&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt; be the dilation of ratio 1/2 around a&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;. The unique non-empty fixed point of the corresponding mapping ψ is a Sierpinski gasket and the dimension s is the unique solution of&lt;br /&gt;
&lt;br /&gt;
我们可以使用这个定理来计算谢尔宾斯基三角形的豪斯多夫维数(或者有时候叫做谢尔宾斯基垫圈)。考虑R&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; 平面上的三个非共线点，''a''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;，''a''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;，''a''&amp;lt;sub&amp;gt;3&amp;lt;/sub&amp;gt;，让ψ&amp;lt;sub&amp;gt;''i''&amp;lt;/sub&amp;gt;是围绕着''a&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;''比率1/2的膨胀。对应映射的唯一非空不动点是一个谢尔宾斯基垫圈，其维数''s''是对应映射的唯一解&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt; \left(\frac{1}{2}\right)^s+\left(\frac{1}{2}\right)^s+\left(\frac{1}{2}\right)^s = 3 \left(\frac{1}{2}\right)^s =1. &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \left(\frac{1}{2}\right)^s+\left(\frac{1}{2}\right)^s+\left(\frac{1}{2}\right)^s = 3 \left(\frac{1}{2}\right)^s =1. &amp;lt;/math&amp;gt;&lt;br /&gt;
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Taking [[natural logarithm]]s of both sides of the above equation, we can solve for ''s'', that is: ''s'' = ln(3)/ln(2).  The Sierpinski gasket is self-similar and satisfies the OSC. In general a set ''E'' which is a fixed point of a mapping&lt;br /&gt;
&lt;br /&gt;
Taking natural logarithms of both sides of the above equation, we can solve for s, that is: s = ln(3)/ln(2).  The Sierpinski gasket is self-similar and satisfies the OSC. In general a set E which is a fixed point of a mapping&lt;br /&gt;
&lt;br /&gt;
取上述方程两边的自然对数，我们可以求出 ''s''，即: ''s'' = ln(3)/ln(2)。该密封垫具有自相似性，满足 OSC 要求。一般来说，集合 ''E''是一个映射的不动点&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt; A \mapsto \psi(A) = \bigcup_{i=1}^m \psi_i(A) &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt; A \mapsto \psi(A) = \bigcup_{i=1}^m \psi_i(A) &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
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is self-similar if and only if the intersections&lt;br /&gt;
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is self-similar if and only if the intersections&lt;br /&gt;
&lt;br /&gt;
是自相似的，当且仅当&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt; H^s\left(\psi_i(E) \cap \psi_j(E)\right) =0, &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; H^s\left(\psi_i(E) \cap \psi_j(E)\right) =0, &amp;lt;/math&amp;gt;&lt;br /&gt;
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where ''s'' is the Hausdorff dimension of ''E'' and ''H&amp;lt;sup&amp;gt;s&amp;lt;/sup&amp;gt;'' denotes [[Hausdorff measure]]. This is clear in the case of the Sierpinski gasket (the intersections are just points), but is also true more generally:&lt;br /&gt;
&lt;br /&gt;
where s is the Hausdorff dimension of E and H&amp;lt;sup&amp;gt;s&amp;lt;/sup&amp;gt; denotes Hausdorff measure. This is clear in the case of the Sierpinski gasket (the intersections are just points), but is also true more generally:&lt;br /&gt;
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其中 ''s''是''E''的豪斯多夫维数， ''H&amp;lt;sup&amp;gt;s&amp;lt;/sup&amp;gt;'' 表示 豪斯多夫测度。对于谢尔宾斯基垫圈(交叉点就是点)来说，这一点很明显，但更普遍的情况是:&lt;br /&gt;
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'''Theorem'''. Under the same conditions as the previous theorem, the unique fixed point of ψ is self-similar.&lt;br /&gt;
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Theorem. Under the same conditions as the previous theorem, the unique fixed point of ψ is self-similar.&lt;br /&gt;
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'''定理'''：在与前一定理相同的条件下，其唯一不动点是自相似的。&lt;br /&gt;
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==See also参阅==&lt;br /&gt;
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* [[List of fractals by Hausdorff dimension豪斯多夫分形维数列表]] Examples of deterministic fractals, random and natural fractals.确定性分形与随机和自然分形的示例。&lt;br /&gt;
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* [[Assouad dimension  Assouad维数]], another variation of fractal dimension that, like Hausdorff dimension, is defined using coverings by balls其他被球覆盖方式定义的分形维数，例如豪斯多夫维数。&lt;br /&gt;
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* [[Intrinsic dimension固有维数]]&lt;br /&gt;
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* [[Packing dimension填充维数]]&lt;br /&gt;
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* [[Fractal dimension分形维数]]&lt;br /&gt;
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==References参考文献==&lt;br /&gt;
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{{reflist}}&lt;br /&gt;
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==Further reading拓展阅读==&lt;br /&gt;
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* {{cite book |last1=Dodson |first1=M. Maurice |title=Fractal Geometry and Applications: A Jubilee of Benoît Mandelbrot |volume=72 |issue=1 |pages=305–347 |last2=Kristensen |first2=Simon |chapter=Hausdorff Dimension and Diophantine Approximation |date=June 12, 2003 |arxiv=math/0305399 |bibcode = 2003math......5399D |doi=10.1090/pspum/072.1/2112110|series=Proceedings of Symposia in Pure Mathematics |isbn=9780821836378 }}&lt;br /&gt;
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* {{cite book |last1=Hurewicz |first1=Witold |authorlink1=Witold Hurewicz |last2=Wallman |first2=Henry |authorlink2=Henry Wallman |title=Dimension Theory |url=https://archive.org/details/in.ernet.dli.2015.84609 |publisher=Princeton University Press |year=1948 }}&lt;br /&gt;
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* {{cite journal |author作者=E. Szpilrajn |authorlink=Edward Marczewski |title=La dimension et la mesure |journal=Fundamenta Mathematicae |volume=28 |pages=81–9 |year=1937 }}&lt;br /&gt;
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* {{cite journal&lt;br /&gt;
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 | last1=Marstrand&lt;br /&gt;
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 | last1=Marstrand&lt;br /&gt;
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 | last1=马斯特兰德&lt;br /&gt;
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 | first1=J. M. | title=The dimension of cartesian product sets | year=1954 | journal=Proc. Cambridge Philos. Soc.&lt;br /&gt;
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 | first1=J. M. | title=The dimension of cartesian product sets | year=1954 | journal=Proc. Cambridge Philos. Soc.&lt;br /&gt;
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 | first1= J. M. | title=笛卡儿积集的维数 | 1954年 |  journal=Proc. Cambridge Philos. Soc.&lt;br /&gt;
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 | volume=50&lt;br /&gt;
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 | volume=50&lt;br /&gt;
&lt;br /&gt;
 | 第50卷&lt;br /&gt;
&lt;br /&gt;
 | issue=3&lt;br /&gt;
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 | issue=3&lt;br /&gt;
&lt;br /&gt;
 | 第三期&lt;br /&gt;
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 | pages=198–202&lt;br /&gt;
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 | pages=198–202&lt;br /&gt;
&lt;br /&gt;
 | 第198-202页&lt;br /&gt;
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 | doi=10.1017/S0305004100029236|bibcode = 1954PCPS...50..198M }}&lt;br /&gt;
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 | doi=10.1017/S0305004100029236|bibcode = 1954PCPS...50..198M }}&lt;br /&gt;
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10.1017 / S0305004100029236 | bibcode 1954PCPS... 50. . 198 m }&lt;br /&gt;
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* {{Cite book&lt;br /&gt;
&lt;br /&gt;
 | last1=Mattila&lt;br /&gt;
&lt;br /&gt;
 | last1=Mattila&lt;br /&gt;
&lt;br /&gt;
 | last1=Mattila&lt;br /&gt;
&lt;br /&gt;
 | first1=Pertti | author1-link=Pertti Mattila| title=Geometry of sets and measures in Euclidean spaces | publisher=[[Cambridge University Press]]&lt;br /&gt;
&lt;br /&gt;
 | first1=Pertti | author1-link=Pertti Mattila| title=Geometry of sets and measures in Euclidean spaces | publisher=Cambridge University Press&lt;br /&gt;
&lt;br /&gt;
| first1 Pertti | author1-link Pertti Mattila | title 欧几里德空间中集合和度量的几何 | 出版商剑桥大学出版社&lt;br /&gt;
&lt;br /&gt;
 | isbn=978-0-521-65595-8 | year=1995}}&lt;br /&gt;
&lt;br /&gt;
 | isbn=978-0-521-65595-8 | year=1995}}&lt;br /&gt;
&lt;br /&gt;
| isbn 978-0-521-65595-8 | year 1995}&lt;br /&gt;
&lt;br /&gt;
* {{cite journal |author=A. S. Besicovitch |authorlink=A. S. Besicovitch |title=On Linear Sets of Points of Fractional Dimensions |journal=[[Mathematische Annalen]] |volume=101 |year=1929 | doi=10.1007/BF01454831| issue=1 |pages= 161–193}}&lt;br /&gt;
&lt;br /&gt;
* {{cite journal |author1=A. S. Besicovitch |authorlink1=A. S. Besicovitch |author2=H. D. Ursell |authorlink2=H. D. Ursell |title=Sets of Fractional Dimensions |journal=Journal of the London Mathematical Society |volume=12 |year=1937 | issue=1 | doi=10.1112/jlms/s1-12.45.18  | pages=18–25 }}&amp;lt;br/&amp;gt;Several selections from this volume are reprinted in {{cite book |author=Edgar, Gerald A. |title=Classics on fractals |publisher=Addison-Wesley |location=Boston |year=1993 |isbn=0-201-58701-7}} See chapters 9,10,11&lt;br /&gt;
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* {{cite journal |author=F. Hausdorff |authorlink=F. Hausdorff |title=Dimension und äußeres Maß |journal=Mathematische Annalen |volume=79 |issue=1–2 |pages=157–179 |date=March 1919 |doi=10.1007/BF01457179|hdl=10338.dmlcz/100363 |url=http://dml.cz/bitstream/handle/10338.dmlcz/100363/CzechMathJ_09-1959-3_5.pdf }}&lt;br /&gt;
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* {{cite journal | last=Hutchinson | first=John E. | title=Fractals and self similarity | journal=Indiana Univ. Math. J. | volume=30 | year=1981 | pages=713–747 | doi=10.1512/iumj.1981.30.30055 | issue=5 | doi-access=free }}&lt;br /&gt;
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*{{cite book | last=Falconer | first = Kenneth |title=Fractal Geometry: Mathematical Foundations and Applications | publisher=[[John Wiley and Sons]] | edition=2nd | year=2003}}&lt;br /&gt;
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==External links外部链接==&lt;br /&gt;
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* [https://www.encyclopediaofmath.org/index.php/Hausdorff_dimension Hausdorff dimension] 在 [https://www.encyclopediaofmath.org/ Encyclopedia of Mathematics]&lt;br /&gt;
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* [https://www.encyclopediaofmath.org/index.php/Hausdorff_measure Hausdorff measure] 在 [https://www.encyclopediaofmath.org/ Encyclopedia of Mathematics]&lt;br /&gt;
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{{DEFAULTSORT:Hausdorff Dimension豪斯多夫维数}}&lt;br /&gt;
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[[Category分类:Fractals分形]]&lt;br /&gt;
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[[Category分类:Metric geometry度量几何]]&lt;br /&gt;
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[[Category分类:Dimension theory维度理论]]&lt;br /&gt;
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&amp;lt;small&amp;gt;This page was moved from [[wikipedia:en:Hausdorff dimension]]. Its edit history can be viewed at [[分形维数/edithistory]]&amp;lt;/small&amp;gt;&amp;lt;/noinclude&amp;gt;&lt;br /&gt;
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[[Category:待整理页面]]&lt;/div&gt;</summary>
		<author><name>Ruili</name></author>
	</entry>
	<entry>
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		<title>分形维数</title>
		<link rel="alternate" type="text/html" href="https://wiki.swarma.org/index.php?title=%E5%88%86%E5%BD%A2%E7%BB%B4%E6%95%B0&amp;diff=17739"/>
		<updated>2020-11-01T17:05:48Z</updated>

		<summary type="html">&lt;p&gt;Ruili：&lt;/p&gt;
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&lt;div&gt;此词条暂由彩云小译翻译，未经人工整理和审校，带来阅读不便，请见谅。&lt;br /&gt;
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{{short description|Invariant}}&lt;br /&gt;
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Example of non-integer dimensions. The first four [[iteration]]s of the [[Koch snowflake|Koch curve]], where after each iteration, all original line segments are replaced with four, each a self-similar copy that is 1/3 the length of the original. One formalism of the Hausdorff dimension uses this scale factor (3) and the number of self-similar objects (4) to calculate the dimension, D, after the first iteration to be D = (log N)/(log S) = (log 4)/(log 3) ≈ 1.26.&amp;lt;ref name=CampbellAnnenberg15&amp;gt;MacGregor Campbell, 2013, &amp;quot;5.6 Scaling and the Hausdorff Dimension,&amp;quot; at ''Annenberg Learner:MATHematics illuminated'', see [http://www.learner.org/courses/mathilluminated/units/5/textbook/06.php], accessed 5 March 2015.&amp;lt;/ref&amp;gt; That is, while the Hausdorff dimension of a single [[point (geometry)|point]] is zero, of a [[line segment]] is 1, of a [[square]] is 2, and of a [[cube]] is 3, for [[fractal]]s such as this, the object can have a non-integer dimension.&lt;br /&gt;
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Example of non-integer dimensions. The first four iterations of the Koch curve, where after each iteration, all original line segments are replaced with four, each a self-similar copy that is 1/3 the length of the original. One formalism of the Hausdorff dimension uses this scale factor (3) and the number of self-similar objects (4) to calculate the dimension, D, after the first iteration to be D = (log N)/(log S) = (log 4)/(log 3) ≈ 1.26. That is, while the Hausdorff dimension of a single point is zero, of a line segment is 1, of a square is 2, and of a cube is 3, for fractals such as this, the object can have a non-integer dimension.&lt;br /&gt;
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非整数维度示例：前四个[[Koch 曲线]]的迭代，在每次迭代后，所有原始线段都被替换为四个，每个自相似的复制是原始线段长度的1 / 3。豪斯多夫维数的一个建模是使用比例因子(3)和自相似对象的数量(4)来计算维度 D，在第一次迭代后为 D = (log N)/(log S) = (log 4)/(log 3) ≈ 1.26.&amp;lt;ref name=CampbellAnnenberg15&amp;gt;。MacGregor Campbell, 2013, &amp;quot;5.6 Scaling and the Hausdorff Dimension,&amp;quot; 在 ''Annenberg Learner:MATHematics illuminated'', 参见 [http://www.learner.org/courses/mathilluminated/units/5/textbook/06.php], accessed 5 March 2015.&amp;lt;/ref&amp;gt; 也就是说，单点的豪斯多夫维数为零，线段为1，正方形为2，立方体为3时，但对于分形，对象可以有一个非整数维度。&lt;br /&gt;
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In [[mathematics]], '''Hausdorff dimension''' is a measure of ''roughness'', or more specifically, [[fractal dimension]], that was first introduced in 1918 by [[mathematician]] [[Felix Hausdorff]].&amp;lt;ref&amp;gt;{{Cite journal |arxiv = 1101.1444|doi = 10.1214/11-STS370|title = Estimators of Fractal Dimension: Assessing the Roughness of Time Series and Spatial Data|journal = Statistical Science|volume = 27|issue = 2|pages = 247–277|year = 2012|last1 = Gneiting|first1 = Tilmann|last2 = Ševčíková|first2 = Hana|last3 = Percival|first3 = Donald B.}}&amp;lt;/ref&amp;gt; For instance, the Hausdorff dimension of a single [[point (geometry)|point]] is zero, of a [[line segment]] is 1, of a [[square]] is 2, and of a [[cube]] is 3. That is, for sets of points that define a smooth shape or a shape that has a small number of corners—the shapes of traditional geometry and science—the Hausdorff dimension is an [[integer]] agreeing with the usual sense of dimension, also known as the [[Inductive dimension|topological dimension]]. However, formulas have also been developed that allow calculation of the dimension of other less simple objects, where, solely on the basis of their properties of [[scaling (geometry)|scaling]] and [[self-similarity]], one is led to the conclusion that particular objects—including [[fractal]]s—have non-integer Hausdorff dimensions. Because of the significant technical advances made by [[Abram Samoilovitch Besicovitch]] allowing computation of dimensions for highly irregular or &amp;quot;rough&amp;quot; sets, this dimension is also commonly referred to as the ''Hausdorff–Besicovitch dimension.''&lt;br /&gt;
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In mathematics, Hausdorff dimension is a measure of roughness, or more specifically, fractal dimension, that was first introduced in 1918 by mathematician Felix Hausdorff. For instance, the Hausdorff dimension of a single point is zero, of a line segment is 1, of a square is 2, and of a cube is 3. That is, for sets of points that define a smooth shape or a shape that has a small number of corners—the shapes of traditional geometry and science—the Hausdorff dimension is an integer agreeing with the usual sense of dimension, also known as the topological dimension. However, formulas have also been developed that allow calculation of the dimension of other less simple objects, where, solely on the basis of their properties of scaling and self-similarity, one is led to the conclusion that particular objects—including fractals—have non-integer Hausdorff dimensions. Because of the significant technical advances made by Abram Samoilovitch Besicovitch allowing computation of dimensions for highly irregular or &amp;quot;rough&amp;quot; sets, this dimension is also commonly referred to as the Hausdorff–Besicovitch dimension.&lt;br /&gt;
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在[[数学]]中，'''&amp;lt;font color = '#ff8000'&amp;gt;豪斯多夫维数Hausdorff dimension&amp;lt;/font&amp;gt;'''是一种粗糙度的度量单位，或者更确切地说，分形维数，是由数学家 Felix Hausdorff 在1918年首次提出的。例如，单点的豪斯多夫维数为零，线段为1，正方形为2，立方体为3。也就是说，对于定义了一个光滑形状或一个有少数几个角的形状---- 传统几何学和科学的形状---- 的点集来说，豪斯多夫维数是一个整数，符合通常的维度意义，也称为拓扑维度。然而，还有一些公式允许计算其他不太简单的对象的维数，其中仅仅根据它们的标度和自相似特性，就可以得出结论: 特定的对象ー包括分形ー具有非整数的 Hausdorff 维数。由于阿布拉姆·萨莫伊洛维奇·贝西科维奇的重大技术进步，允许计算高度不规则或“粗糙”集的维度，这个维度通常也被称为 Hausdorff-Besicovitch 维度。 &lt;br /&gt;
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The Hausdorff dimension, more specifically, is a further dimensional number associated with a given set, where the distances between all members of that set are defined. Such a set is termed a [[metric space]]. The dimension is drawn from the [[Extended real number line|extended real numbers]], &amp;lt;math&amp;gt;\overline{\mathbb{R}}&amp;lt;/math&amp;gt;, as opposed to the more intuitive notion of dimension, which is not associated to general metric spaces, and only takes values in the non-negative integers.&lt;br /&gt;
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The Hausdorff dimension, more specifically, is a further dimensional number associated with a given set, where the distances between all members of that set are defined. Such a set is termed a metric space. The dimension is drawn from the extended real numbers, &amp;lt;math&amp;gt;\overline{\mathbb{R}}&amp;lt;/math&amp;gt;, as opposed to the more intuitive notion of dimension, which is not associated to general metric spaces, and only takes values in the non-negative integers.&lt;br /&gt;
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更具体地说，豪斯多夫维数是一个与给定集合相关联的更进一步的维数，其中定义了该集合所有成员之间的距离。这样的集合称为度量空间。维数是从扩展的实数，&amp;lt;math&amp;gt;\overline{\mathbb{R}}&amp;lt;/math&amp;gt;，而不是更直观的维数概念(它不与一般的度量空间相关联，只取非负整数的值)。&lt;br /&gt;
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In mathematical terms, the Hausdorff dimension generalizes the notion of the dimension of a real [[vector space]]. That is, the Hausdorff dimension of an ''n''-dimensional [[inner product space]] equals ''n''. This underlies the earlier statement that the Hausdorff dimension of a point is zero, of a line is one, etc., and that [[fractal|irregular sets]] can have noninteger Hausdorff dimensions. For instance, the [[Koch snowflake]] shown at right is constructed from an equilateral triangle; in each iteration, its component line segments are divided into 3 segments of unit length, the newly created middle segment is used as the base of a new [[equilateral]] triangle that points outward, and this base segment is then deleted to leave a final object from the iteration of unit length of 4.&amp;lt;ref&amp;gt;Larry Riddle, 2014, &amp;quot;Classic Iterated Function Systems: Koch Snowflake&amp;quot;, Agnes Scott College e-Academy (online), see [http://ecademy.agnesscott.edu/~lriddle/ifs/ksnow/ksnow.htm], accessed 5 March 2015.&amp;lt;/ref&amp;gt; That is, after the first iteration, each original line segment has been replaced with N=4, where each self-similar copy is 1/S = 1/3 as long as the original.&amp;lt;ref name=CampbellAnnenberg15/&amp;gt; Stated another way, we have taken an object with Euclidean dimension, D, and reduced its linear scale by 1/3 in each direction, so that its length increases to N=S&amp;lt;sup&amp;gt;D&amp;lt;/sup&amp;gt;.&amp;lt;ref name=ClaytonSCTPLS96&amp;gt;Keith Clayton, 1996, &amp;quot;Fractals and the Fractal Dimension,&amp;quot; ''Basic Concepts in Nonlinear Dynamics and Chaos'' (workshop), Society for Chaos Theory in Psychology and the Life Sciences annual meeting, June 28, 1996, Berkeley, California, see [http://www.vanderbilt.edu/AnS/psychology/cogsci/chaos/workshop/Workshop.html], accessed 5 March 2015.&amp;lt;/ref&amp;gt; This equation is easily solved for D, yielding the ratio of logarithms (or [[natural logarithm]]s) appearing in the figures, and giving—in the Koch and other fractal cases—non-integer dimensions for these objects.&lt;br /&gt;
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In mathematical terms, the Hausdorff dimension generalizes the notion of the dimension of a real vector space. That is, the Hausdorff dimension of an n-dimensional inner product space equals n. This underlies the earlier statement that the Hausdorff dimension of a point is zero, of a line is one, etc., and that irregular sets can have noninteger Hausdorff dimensions. For instance, the Koch snowflake shown at right is constructed from an equilateral triangle; in each iteration, its component line segments are divided into 3 segments of unit length, the newly created middle segment is used as the base of a new equilateral triangle that points outward, and this base segment is then deleted to leave a final object from the iteration of unit length of 4. That is, after the first iteration, each original line segment has been replaced with N=4, where each self-similar copy is 1/S = 1/3 as long as the original. This equation is easily solved for D, yielding the ratio of logarithms (or natural logarithms) appearing in the figures, and giving—in the Koch and other fractal cases—non-integer dimensions for these objects.&lt;br /&gt;
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用数学术语来说，豪斯多夫维数概括了实向量空间维数的概念。也就是说，n 维内积空间的豪斯多夫维数等于 n。 这就是早期假设的基础，一个点的豪斯多夫维数是零，一条线是一等等，不规则集可以有非整数的豪斯多夫维数。例如，右边所示的 Koch 雪花是由一个正三角形构成的; 在每次迭代中，它的组成线段被分成单位长度的3段，新创建的中间线段被用作一个指向外部的新正三角形的基础，然后人们删除这个基础线段用来保留单位长度4的迭代中的最终对象。也就是说，在第一次迭代之后，每个原始线段都被替换为 N=4，其中每个自相似拷贝的长度是原始线段的1/S = 1/3 。这个方程很容易求解为 D，产生出现在图形中的对数(或自然对数)的比率，并给出——在 Koch 和其他分形情况下——这些对象的非整数维数。&lt;br /&gt;
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The Hausdorff dimension is a successor to the simpler, but usually equivalent, box-counting or [[Minkowski–Bouligand dimension]].&lt;br /&gt;
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The Hausdorff dimension is a successor to the simpler, but usually equivalent, box-counting or Minkowski–Bouligand dimension.&lt;br /&gt;
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豪斯多夫维数是更简单但通常等价的'''&amp;lt;font color = '#ff8000'&amp;gt;计盒维数box-counting&amp;lt;/font&amp;gt;'''或'''&amp;lt;font color = '#ff8000'&amp;gt;闵可夫斯基维数Minkowski-Bouligand&amp;lt;/font&amp;gt;'''的继承者。&lt;br /&gt;
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==Intuition概念==&lt;br /&gt;
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{{refimprove section|date=March 2015}}&lt;br /&gt;
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The intuitive concept of dimension of a geometric object ''X'' is the number of independent parameters one needs to pick out a unique point inside. However, any point specified by two parameters can be instead specified by one, because the [[cardinality]] of the [[real plane]] is equal to the cardinality of the [[real line]] (this can be seen by an [[Cantor's diagonal argument|argument]] involving interweaving the digits of two numbers to yield a single number encoding the same information). The example of a [[space-filling curve]] shows that one can even map the real line to the real plane [[Surjective function|surjectively]] (taking one real number into a pair of real numbers in a way so that all pairs of numbers are covered) and ''continuously'', so that a one-dimensional object completely fills up a higher-dimensional object.&lt;br /&gt;
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The intuitive concept of dimension of a geometric object X is the number of independent parameters one needs to pick out a unique point inside. However, any point specified by two parameters can be instead specified by one, because the cardinality of the real plane is equal to the cardinality of the real line (this can be seen by an argument involving interweaving the digits of two numbers to yield a single number encoding the same information). The example of a space-filling curve shows that one can even map the real line to the real plane surjectively (taking one real number into a pair of real numbers in a way so that all pairs of numbers are covered) and continuously, so that a one-dimensional object completely fills up a higher-dimensional object.&lt;br /&gt;
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几何对象X的尺寸的直观概念是指需要多少个独立参数才能找到一个独特的点。但是，任何由两个参数指定的点都可以由一个参数指定，因为为实平面的基数等于实线的基数(这可以通过交织两个数字以产生一个编码相同信息的单个数字看到)。'''&amp;lt;font color = '#ff8000'&amp;gt;皮亚诺曲线&amp;lt;/font&amp;gt;'''的例子表明，可以将实线完美和连续地映射到实平面(把一个实数转换成一对实数，从而覆盖所有实数对)，由此一维对象完全填充了一个高维对象。&lt;br /&gt;
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Every space filling curve hits some points multiple times, and does not have a continuous inverse. It is impossible to map two dimensions onto one in a way that is continuous and continuously invertible. The topological dimension, also called [[Lebesgue covering dimension]], explains why. This dimension is ''n'' if, in every covering of ''X'' by small open balls, there is at least one point where ''n''&amp;amp;nbsp;+&amp;amp;nbsp;1 balls overlap. For example, when one covers a line with short open intervals, some points must be covered twice, giving dimension&amp;amp;nbsp;''n''&amp;amp;nbsp;=&amp;amp;nbsp;1.&lt;br /&gt;
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Every space filling curve hits some points multiple times, and does not have a continuous inverse. It is impossible to map two dimensions onto one in a way that is continuous and continuously invertible. The topological dimension, also called Lebesgue covering dimension, explains why. This dimension is n if, in every covering of X by small open balls, there is at least one point where n&amp;amp;nbsp;+&amp;amp;nbsp;1 balls overlap. For example, when one covers a line with short open intervals, some points must be covered twice, giving dimension&amp;amp;nbsp;n&amp;amp;nbsp;=&amp;amp;nbsp;1.&lt;br /&gt;
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每条空间填充曲线都会多次击中某些点，且不存在连续的逆。将二维以连续和连续可逆的方式映射到一维是不可能的。'''&amp;lt;font color = '#ff8000'&amp;gt;拓扑维度 topological dimension&amp;lt;/font&amp;gt;'''，也被称为Lebesgue覆盖维数，解释了为什么。如果在 x 的每个小开球覆盖中，至少有一个点 n + 1个球重叠，这个维度是 n。例如，当用短的开区间覆盖一条线时，某些点必须被覆盖两次，给出维数''n''&amp;amp;nbsp;=&amp;amp;nbsp;1。&lt;br /&gt;
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But topological dimension is a very crude measure of the local size of a space (size near a point). A curve that is almost space-filling can still have topological dimension one, even if it fills up most of the area of a region. A [[fractal]] has an integer topological dimension, but in terms of the amount of space it takes up, it behaves like a higher-dimensional space.&lt;br /&gt;
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But topological dimension is a very crude measure of the local size of a space (size near a point). A curve that is almost space-filling can still have topological dimension one, even if it fills up most of the area of a region. A fractal has an integer topological dimension, but in terms of the amount of space it takes up, it behaves like a higher-dimensional space.&lt;br /&gt;
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但是，拓扑维度是对空间局部尺寸(点附近的尺寸)的一个非常粗略的度量。一条几乎是空间填充的曲线仍然可以有一维拓扑，即使它填充了一个区域的大部分面积。分形具有整数的拓扑维数，但就其所占的空间量而言，它看起来像一个更高维的空间。&lt;br /&gt;
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The Hausdorff dimension measures the local size of a space taking into account the distance between points, the [[metric space|metric]]. Consider the number ''N''(''r'') of [[ball (mathematics)|balls]] of radius at most ''r'' required to cover ''X'' completely. When ''r'' is very small, ''N''(''r'') grows polynomially with 1/''r''. For a sufficiently well-behaved  ''X'', the Hausdorff dimension is the unique number ''d'' such that N(''r'') grows as 1/''r&amp;lt;sup&amp;gt;d&amp;lt;/sup&amp;gt;'' as ''r'' approaches zero. More precisely, this defines the [[Minkowski–Bouligand dimension|box-counting dimension]], which equals the Hausdorff dimension when the value ''d'' is a critical boundary between growth rates that are insufficient to cover the space, and growth rates that are overabundant.&lt;br /&gt;
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The Hausdorff dimension measures the local size of a space taking into account the distance between points, the metric. Consider the number N(r) of balls of radius at most r required to cover X completely. When r is very small, N(r) grows polynomially with 1/r. For a sufficiently well-behaved  X, the Hausdorff dimension is the unique number d such that N(r) grows as 1/r&amp;lt;sup&amp;gt;d&amp;lt;/sup&amp;gt; as r approaches zero. More precisely, this defines the box-counting dimension, which equals the Hausdorff dimension when the value d is a critical boundary between growth rates that are insufficient to cover the space, and growth rates that are overabundant.&lt;br /&gt;
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豪斯多夫维数测量一个空间的局部大小时，会考虑到点之间距离的度量。考虑半径最大为 r 的球数 ''N'' (r) ，需要完全覆盖 ''X''。当 r 很小时，n (r)以1/''r'' 增长多项式。对于一个表现足够好的 ''X''，豪斯多夫维数是唯一的数 d，这样当 r 趋近于零时， N(r)增长为1/r&amp;lt;sup&amp;gt;d&amp;lt;/sup&amp;gt; 。更确切地说，这定义了盒子计数维度，当值 d 是不足以覆盖空间的增长率和过度充裕的增长率之间的关键边界时，它等于豪斯多夫维数。&lt;br /&gt;
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For shapes that are smooth, or shapes with a small number of corners, the shapes of traditional geometry and science, the Hausdorff dimension is an integer agreeing with the topological dimension. But [[Benoit Mandelbrot]] observed that [[fractal]]s, sets with noninteger Hausdorff dimensions, are found everywhere in nature. He observed that the proper idealization of most rough shapes you see around you is not in terms of smooth idealized shapes, but in terms of fractal idealized shapes:&lt;br /&gt;
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For shapes that are smooth, or shapes with a small number of corners, the shapes of traditional geometry and science, the Hausdorff dimension is an integer agreeing with the topological dimension. But Benoit Mandelbrot observed that fractals, sets with noninteger Hausdorff dimensions, are found everywhere in nature. He observed that the proper idealization of most rough shapes you see around you is not in terms of smooth idealized shapes, but in terms of fractal idealized shapes:&lt;br /&gt;
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对于光滑的形状，或者有少量棱角的形状，传统几何和科学的形状，豪斯多夫维数是一个整数，与拓扑维度一致。但是伯努·曼德布洛特观察到分形---- 具有非整数豪斯多夫维数的集合---- 在自然界中随处可见。他观察到，我们周围大多数粗糙形状的理想化不是光滑的理想化形状，而是分形理想化形状:&lt;br /&gt;
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&amp;lt;blockquote&amp;gt;Clouds are not spheres, mountains are not cones, coastlines are not circles, and bark is not smooth, nor does lightning travel in a straight line.&amp;lt;ref name=&amp;quot;mandelbrot&amp;quot;&amp;gt;{{cite book   | last = Mandelbrot   | first = Benoît   | authorlink = Benoit Mandelbrot   | title = The Fractal Geometry of Nature   | publisher = W. H. Freeman   | series = Lecture notes in mathematics 1358   | year = 1982   | doi =    | isbn = 0-7167-1186-9   | url-access = registration   | url = https://archive.org/details/fractalgeometryo00beno   }}&amp;lt;/ref&amp;gt;&amp;lt;/blockquote&amp;gt;&lt;br /&gt;
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&amp;lt;blockquote&amp;gt;Clouds are not spheres, mountains are not cones, coastlines are not circles, and bark is not smooth, nor does lightning travel in a straight line.&amp;lt;/blockquote&amp;gt;&lt;br /&gt;
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&amp;lt;blockquote&amp;gt;云不是球体，山不是锥体，海岸线不是圆圈，树皮不平滑，闪电也不是直线运动。 &amp;lt;/blockquote&amp;gt;&lt;br /&gt;
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For fractals that occur in nature, the Hausdorff and [[Minkowski–Bouligand dimension|box-counting dimension]] coincide. The [[packing dimension]] is yet another similar notion which gives the same value for many shapes, but there are well documented exceptions where all these dimensions differ.&lt;br /&gt;
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For fractals that occur in nature, the Hausdorff and box-counting dimension coincide. The packing dimension is yet another similar notion which gives the same value for many shapes, but there are well documented exceptions where all these dimensions differ.&lt;br /&gt;
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对于自然界中出现的分形，豪斯多夫维数和盒计数维数是一致的。封装尺寸是另一个类似的概念，它给出了许多形状相同的值，但是在所有这些尺寸不同的情况，都做了很好的说明。&lt;br /&gt;
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==Formal definitions形式化定义==&lt;br /&gt;
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{{unreferenced section|date=March 2015}}&lt;br /&gt;
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===Hausdorff content豪斯多夫集===&lt;br /&gt;
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Let ''X'' be a [[metric space]]. If ''S'' ⊂ ''X'' and ''d'' ∈ [0, ∞), the ''d''-dimensional '''unlimited Hausdorff content''' of ''S'' is defined by&lt;br /&gt;
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Let X be a metric space. If S ⊂ X and d ∈ [0, ∞), the d-dimensional unlimited Hausdorff content of S is defined by&lt;br /&gt;
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设 ''X''是度量空间。若''S'' ⊂ ''X'' 和 ''d'' ∈ [0, ∞) ，则 ''S'' 的''d''维无限 豪斯多夫集定义为&lt;br /&gt;
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:&amp;lt;math&amp;gt;C_H^d(S):=\inf\Bigl\{\sum_i r_i^d:\text{ there is a cover of } S\text{ by balls with radii }r_i&amp;gt;0\Bigr\}.&amp;lt;/math&amp;gt;&lt;br /&gt;
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&amp;lt;math&amp;gt;C_H^d(S):=\inf\Bigl\{\sum_i r_i^d:\text{ there is a cover of } S\text{ by balls with radii }r_i&amp;gt;0\Bigr\}.&amp;lt;/math&amp;gt;&lt;br /&gt;
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&amp;lt;math&amp;gt;C_H^d(S):=\inf\Bigl\{\sum_i r_i^d:\text{ there is a cover of } S\text{ by balls with radii }r_i&amp;gt;0\Bigr\}.&amp;lt;/math&amp;gt;&lt;br /&gt;
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In other words, &amp;lt;math&amp;gt;C_H^d(S)&amp;lt;/math&amp;gt; is the [[infimum]] of the set of numbers &amp;lt;math&amp;gt;\delta \geq 0&amp;lt;/math&amp;gt; such that there is some (indexed) collection of [[ball (mathematics)|ball]]s &amp;lt;math&amp;gt;\{B(x_i,r_i):i\in I\}&amp;lt;/math&amp;gt; covering ''S'' with ''r&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;''&amp;amp;nbsp;&amp;gt;&amp;amp;nbsp;0 for each ''i''&amp;amp;nbsp;∈&amp;amp;nbsp;''I'' that satisfies &amp;lt;math&amp;gt;\sum_{i\in I} r_i^d&amp;lt;\delta &amp;lt;/math&amp;gt;. (Here, we use the standard convention that [[infimum|inf&amp;amp;nbsp;Ø&amp;amp;nbsp;=&amp;amp;nbsp;∞]].)&lt;br /&gt;
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In other words, &amp;lt;math&amp;gt;C_H^d(S)&amp;lt;/math&amp;gt; is the infimum of the set of numbers &amp;lt;math&amp;gt;\delta \geq 0&amp;lt;/math&amp;gt; such that there is some (indexed) collection of balls &amp;lt;math&amp;gt;\{B(x_i,r_i):i\in I\}&amp;lt;/math&amp;gt; covering S with r&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;&amp;amp;nbsp;&amp;gt;&amp;amp;nbsp;0 for each i&amp;amp;nbsp;∈&amp;amp;nbsp;I that satisfies &amp;lt;math&amp;gt;\sum_{i\in I} r_i^d&amp;lt;\delta &amp;lt;/math&amp;gt;. (Here, we use the standard convention that inf&amp;amp;nbsp;Ø&amp;amp;nbsp;=&amp;amp;nbsp;∞.)&lt;br /&gt;
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换句话说，&amp;lt;math&amp;gt;C_H^d(S)&amp;lt;/math&amp;gt; 是数字集合&amp;lt;math&amp;gt;\delta \geq 0&amp;lt;/math&amp;gt;的下确界，使得在 ''i''&amp;amp;nbsp;∈&amp;amp;nbsp中存在一些球集合 &amp;lt;math&amp;gt;\{B(x_i,r_i):i\in I\}&amp;lt;/math&amp;gt;  i 包含 s，对于每个 ''r&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;''&amp;amp;nbsp;&amp;gt;&amp;amp;nbsp;0 满足 i 中的和&amp;lt;math&amp;gt;\sum_{i\in I} r_i^d&amp;lt;\delta &amp;lt;/math&amp;gt; (在这里，我们使用inf&amp;amp;nbsp;Ø&amp;amp;nbsp;=&amp;amp;nbsp;∞ )的标准约定。&lt;br /&gt;
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===Hausdorff measurement豪斯多夫分形测量===&lt;br /&gt;
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The Hausdorff outer measure is different from the unbounded Hausdorf content in that rather than considering all possible coverings of ''S'', we see what happens when the sizes of the balls go to zero. This is  for &amp;lt;math&amp;gt;d \geq 0 &amp;lt;/math&amp;gt;, we define the ''d''-dimensional Hausdorff outer measure of ''S'' as&lt;br /&gt;
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The Hausdorff outer measure is different from the unbounded Hausdorf content in that rather than considering all possible coverings of S, we see what happens when the sizes of the balls go to zero. This is  for &amp;lt;math&amp;gt;d \geq 0 &amp;lt;/math&amp;gt;, we define the d-dimensional Hausdorff outer measure of S as&lt;br /&gt;
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豪斯多夫外测度不同于无界的豪斯多夫，因为我们不考虑 s 的所有可能，我们看到当球的大小为零时会发生什么。这是为了数学  &amp;lt;math&amp;gt;d \geq 0 &amp;lt;/math&amp;gt;，我们定义了  ''S''的 ''d''维豪斯多夫Hausdorff 外测度为&lt;br /&gt;
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:&amp;lt;math&amp;gt; \mathcal{H}^d(S):=\lim_{r \to 0} \inf\Bigl\{\sum_i r_i^d:\text{ there is a cover of } S\text{ by balls with radii } 0 &amp;lt; r_i &amp;lt; r\Bigr\}.&amp;lt;/math&amp;gt;&lt;br /&gt;
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&amp;lt;math&amp;gt; \mathcal{H}^d(S):=\lim_{r \to 0} \inf\Bigl\{\sum_i r_i^d:\text{ there is a cover of } S\text{ by balls with radii } 0 &amp;lt; r_i &amp;lt; r\Bigr\}.&amp;lt;/math&amp;gt;&lt;br /&gt;
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&amp;lt;math&amp;gt; \mathcal{H}^d(S):=\lim_{r \to 0} \inf\Bigl\{\sum_i r_i^d:\text{有一个面} S\text{ 球 } 0 &amp;lt; r_i &amp;lt; r\Bigr\}.&amp;lt;/math&amp;gt;&lt;br /&gt;
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===Hausdorff dimension豪斯多夫维数===&lt;br /&gt;
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The '''Hausdorff dimension''' of ''X'' is defined by&lt;br /&gt;
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The Hausdorff dimension of X is defined by&lt;br /&gt;
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X 的豪斯多夫维数定义为&lt;br /&gt;
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:&amp;lt;math&amp;gt;\dim_{\operatorname{H}}(X):=\inf\{d\ge 0: \mathcal{H}^d(X)=0\}.&amp;lt;/math&amp;gt;&lt;br /&gt;
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&amp;lt;math&amp;gt;\dim_{\operatorname{H}}(X):=\inf\{d\ge 0: \mathcal{H}^d(X)=0\}.&amp;lt;/math&amp;gt;&lt;br /&gt;
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Equivalently, dim&amp;lt;sub&amp;gt;H&amp;lt;/sub&amp;gt;(''X'') may be defined as the [[infimum]] of the set of ''d'' ∈ [0, ∞) such that the ''d''-dimensional [[Hausdorff measure]] of ''X'' is zero. This is the same as the supremum of the set of ''d''&amp;amp;nbsp;∈&amp;amp;nbsp;[0,&amp;amp;nbsp;∞) such that the ''d''-dimensional Hausdorff measure of ''X'' is infinite (except that when this latter set of numbers ''d'' is empty the Hausdorff dimension is zero).&lt;br /&gt;
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Equivalently, dim&amp;lt;sub&amp;gt;H&amp;lt;/sub&amp;gt;(X) may be defined as the infimum of the set of d ∈ [0, ∞) such that the d-dimensional Hausdorff measure of X is zero. This is the same as the supremum of the set of d&amp;amp;nbsp;∈&amp;amp;nbsp;[0,&amp;amp;nbsp;∞) such that the d-dimensional Hausdorff measure of X is infinite (except that when this latter set of numbers d is empty the Hausdorff dimension is zero).&lt;br /&gt;
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等价地，dim &amp;lt;sub&amp;gt;H&amp;lt;/sub&amp;gt;(''X'')可定义为 ''d'' ∈ [0, ∞) 集的下确界，使得''X'' 的''d''-维 [[豪斯多夫测度]] 为零。这与 ''d''&amp;amp;nbsp;∈&amp;amp;nbsp;[0,&amp;amp;nbsp;∞)的集合的上确界相同，因此''X''的 d 维豪斯多夫测度是无限的(除非后一个集合 ''d'' 是空的，豪斯多夫维数为零)。&lt;br /&gt;
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==Examples实例==&lt;br /&gt;
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[[Image:Sierpinski deep.svg|thumb|250px|Dimension of a further [[fractal]] example. The [[Sierpinski triangle]], an object with Hausdorff dimension of log(3)/log(2)≈1.58.&amp;lt;ref name=ClaytonSCTPLS96/&amp;gt;]]&lt;br /&gt;
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Dimension of a further [[fractal example. The Sierpinski triangle, an object with Hausdorff dimension of log(3)/log(2)≈1.58.]]&lt;br /&gt;
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[[Image:谢尔宾斯基三角形 deep.svg|thumb|250px|进一步的[[分形维数]]的例子，进一步的分形维数的例子是谢尔宾斯基三角形，它是一个豪斯多夫维数为log(3)/log(2)≈1.58.&amp;lt;ref name=ClaytonSCTPLS96/&amp;gt;的物体]]&lt;br /&gt;
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* [[Countable set]]s have Hausdorff dimension 0.&amp;lt;ref name=&amp;quot;schleicher&amp;quot;&amp;gt;{{cite journal |last1=Schleicher |first1=Dierk |title=Hausdorff Dimension, Its Properties, and Its Surprises |journal=The American Mathematical Monthly |date=June 2007 |volume=114 |issue=6 |pages=509–528 |doi=10.1080/00029890.2007.11920440 |language=en |issn=0002-9890|arxiv=math/0505099 }}&amp;lt;/ref&amp;gt;&lt;br /&gt;
*[[可数集]]拥有豪斯多夫维数0.&amp;lt;ref name=&amp;quot;schleicher&amp;quot;&amp;gt;{{cite journal |last1=Schleicher |first1=Dierk |title=豪斯多夫维数, Its Properties, and Its Surprises |journal=The American Mathematical Monthly美国数学期刊 |date=June 2007 |volume=114 |issue=6 |pages=509–528 |doi=10.1080/00029890.2007.11920440 |language=en |issn=0002-9890|arxiv=math/0505099 }}&amp;lt;/ref&amp;gt;&lt;br /&gt;
* The [[Euclidean space]] ℝ&amp;lt;sup&amp;gt;''n''&amp;lt;/sup&amp;gt; has Hausdorff dimension ''n'', and the circle '''S'''&amp;lt;sup&amp;gt;1&amp;lt;/sup&amp;gt; has Hausdorff dimension 1.&amp;lt;ref name=&amp;quot;schleicher&amp;quot; /&amp;gt;&lt;br /&gt;
*[[教育空间]] ℝ&amp;lt;sup&amp;gt;''n''&amp;lt;/sup&amp;gt; 有豪斯多夫维数 ''n''，循环'''S'''&amp;lt;sup&amp;gt;1&amp;lt;/sup&amp;gt; 拥有豪斯多夫维数1.&amp;lt;ref name=&amp;quot;schleicher&amp;quot; /&amp;gt;&lt;br /&gt;
* [[Fractal]]s often are spaces whose Hausdorff dimension strictly exceeds the [[topological dimension]].&amp;lt;ref name=&amp;quot;mandelbrot&amp;quot; /&amp;gt; For example, the [[Cantor set]], a zero-dimensional topological space, is a union of two copies of itself, each copy shrunk by a factor 1/3; hence, it can be shown that its Hausdorff dimension is ln(2)/ln(3)&amp;amp;nbsp;≈&amp;amp;nbsp;0.63.&amp;lt;ref&amp;gt;{{cite book | last=Falconer | first = Kenneth |title=Fractal Geometry: Mathematical Foundations and Applications | publisher=[[John Wiley and Sons]] | edition=2nd | year=2003}}&amp;lt;/ref&amp;gt; The [[Sierpinski triangle]] is a union of three copies of itself, each copy shrunk by a factor of&amp;amp;nbsp;1/2; this yields a Hausdorff dimension of ln(3)/ln(2)&amp;amp;nbsp;≈&amp;amp;nbsp;1.58.&amp;lt;ref name=CampbellAnnenberg15/&amp;gt; These Hausdorff dimensions are related to the &amp;quot;critical exponent&amp;quot; of the [[Master theorem (analysis of algorithms)|Master theorem]] for solving [[Recurrence relation|recurrence relations]] in the [[analysis of algorithms]].&lt;br /&gt;
*[[分形]]一般是那些豪斯多夫维数直接超过其拓扑维数的空间。例如[[康托尔集]]是一个o维拓扑空间，由两个自己复制而成，每一个复制品都是原来的三分之一，因此它的豪斯多夫维数是 ln(2)/ln(3)&amp;amp;nbsp;≈&amp;amp;nbsp;0.63。&amp;lt;ref&amp;gt;{{cite book | last=Falconer | first = Kenneth |title=Fractal Geometry: Mathematical Foundations and Applications | publisher=[[John Wiley and Sons]] | edition=2nd | year=2003}}&amp;lt;/ref&amp;gt;一个[[谢尔宾斯基三角]]是他自身三个复制的组合。每一个是原来的&amp;amp;nbsp;1/2，它的豪斯多夫维数ln(3)/ln(2)&amp;amp;nbsp;≈&amp;amp;nbsp;1.58。&amp;lt;ref name=CampbellAnnenberg15/&amp;gt;在递归算法中解决递归关系时，这些豪斯多夫维数与[[算法分析主定理]]的临界指标相联系。&lt;br /&gt;
* [[Space-filling curve]]s like the [[Peano curve]] have the same Hausdorff dimension as the space they fill.&lt;br /&gt;
*[[空间填充曲线]]拥有和他们填充空间同样的豪斯多夫维数，如[[皮亚诺曲线]]。&lt;br /&gt;
* The trajectory of [[Brownian motion]] in dimension 2 and above is conjectured to be Hausdorff dimension 2.&amp;lt;ref&amp;gt;{{cite book | last=Morters | first=Peres | title= Brownian Motion | publisher=[[Cambridge University Press]] | year=2010 }}&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
[[image:Great Britain Hausdorff.svg|thumb|250px|Estimating the Hausdorff dimension of the [[How Long Is the Coast of Britain? Statistical Self-Similarity and Fractional Dimension|coast of Great Britain]]]]&lt;br /&gt;
&lt;br /&gt;
coast of Great Britain]]&lt;br /&gt;
&lt;br /&gt;
[[大不列颠海岸&lt;br /&gt;
&lt;br /&gt;
* 刘易斯·弗赖伊·理查森[[Lewis Fry Richardson]] has performed detailed experiments to measure the approximate Hausdorff dimension for various coastlines. His results have varied from 1.02 for the coastline of [[South Africa]] to 1.25 for the west coast of [[Great Britain]].&amp;lt;ref name=&amp;quot;mandelbrot&amp;quot; /&amp;gt;&lt;br /&gt;
*刘易斯·弗赖伊·理查森（Lewis Fry Richardson）已经通过豪斯多夫维数去测量了很多海岸线。它的结果涵盖从1.02的南非海岸线到1.25的大英帝国西海岸模型。]]&lt;br /&gt;
&lt;br /&gt;
==Properties of Hausdorff dimension豪斯多夫维数特性==&lt;br /&gt;
&lt;br /&gt;
{{refimprove section|date=March 2015}}&lt;br /&gt;
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&lt;br /&gt;
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=== Hausdorff dimension and inductive dimension 豪斯多夫维数和归纳维数===&lt;br /&gt;
&lt;br /&gt;
Let ''X'' be an arbitrary [[Separable space|separable]] metric space. There is a [[topology|topological]] notion of [[inductive dimension]] for ''X'' which is defined recursively. It is always an integer (or +∞) and is denoted dim&amp;lt;sub&amp;gt;ind&amp;lt;/sub&amp;gt;(''X'').&lt;br /&gt;
&lt;br /&gt;
Let X be an arbitrary separable metric space. There is a topological notion of inductive dimension for X which is defined recursively. It is always an integer (or +∞) and is denoted dim&amp;lt;sub&amp;gt;ind&amp;lt;/sub&amp;gt;(X).&lt;br /&gt;
&lt;br /&gt;
设''X'' 是[[任意可分度量空间]]。对于''X'' 有一个递归定义的归纳维数拓扑概念。它总是一个整数(或 + ∞) ，并且表示dim&amp;lt;sub&amp;gt;ind&amp;lt;/sub&amp;gt;(''X'')。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
'''Theorem'''. Suppose ''X'' is non-empty. Then &lt;br /&gt;
&lt;br /&gt;
Theorem. Suppose X is non-empty. Then &lt;br /&gt;
&lt;br /&gt;
'''定理'''：假设''X'' 是非空的。那么&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt; \dim_{\mathrm{Haus}}(X) \geq \dim_{\operatorname{ind}}(X). &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \dim_{\mathrm{Haus}}(X) \geq \dim_{\operatorname{ind}}(X). &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Moreover,&lt;br /&gt;
&lt;br /&gt;
Moreover,&lt;br /&gt;
&lt;br /&gt;
此外,&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \inf_Y \dim_{\operatorname{Haus}}(Y) =\dim_{\operatorname{ind}}(X), &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \inf_Y \dim_{\operatorname{Haus}}(Y) =\dim_{\operatorname{ind}}(X), &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
where ''Y'' ranges over metric spaces [[homeomorphic]] to ''X''. In other words, ''X'' and ''Y'' have the same underlying set of points and the metric ''d''&amp;lt;sub&amp;gt;''Y''&amp;lt;/sub&amp;gt; of ''Y'' is topologically equivalent to ''d''&amp;lt;sub&amp;gt;''X''&amp;lt;/sub&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
where Y ranges over metric spaces homeomorphic to X. In other words, X and Y have the same underlying set of points and the metric d&amp;lt;sub&amp;gt;Y&amp;lt;/sub&amp;gt; of Y is topologically equivalent to d&amp;lt;sub&amp;gt;X&amp;lt;/sub&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
其中''Y''是度量空间同胚到 ''X''的范围。换句话说， ''X''和 ''Y''具有相同的基本点集，''Y''的度规''d''&amp;lt;sub&amp;gt;''Y''&amp;lt;/sub&amp;gt; 的子拓扑等价于''d''&amp;lt;sub&amp;gt;''X''&amp;lt;/sub&amp;gt;。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
These results were originally established by [[Edward Szpilrajn]] (1907–1976), e.g., see Hurewicz and Wallman, Chapter VII.{{full citation needed|date=March 2015}}&lt;br /&gt;
&lt;br /&gt;
These results were originally established by Edward Szpilrajn (1907–1976), e.g., see Hurewicz and Wallman, Chapter VII.&lt;br /&gt;
&lt;br /&gt;
这些结果最初是由 [[Edward Szpilrajn]] (1907–1976)建立的,  参见 Hurewicz and Wallman, Chapter VII.{{full citation needed|date=March 2015}}第七章。&lt;br /&gt;
&lt;br /&gt;
=== Hausdorff dimension and Minkowski dimension 豪斯多夫维数和闵可夫斯基维度===&lt;br /&gt;
&lt;br /&gt;
The [[Minkowski dimension]] is similar to, and at least as large as, the Hausdorff dimension, and they are equal in many situations. However, the set of [[rational number|rational]] points in [0, 1] has Hausdorff dimension zero and Minkowski dimension one. There are also compact sets for which the Minkowski dimension is strictly larger than the Hausdorff dimension.&lt;br /&gt;
&lt;br /&gt;
The Minkowski dimension is similar to, and at least as large as, the Hausdorff dimension, and they are equal in many situations. However, the set of rational points in [0, 1] has Hausdorff dimension zero and Minkowski dimension one. There are also compact sets for which the Minkowski dimension is strictly larger than the Hausdorff dimension.&lt;br /&gt;
&lt;br /&gt;
[[闵可夫斯基维数]]与豪斯多夫维数相似，至少和它一样大，而且在许多情况下是相等的。然而，[0,1]中有理点集的豪斯多夫维数为0，闵可夫斯基维数为1。还有一些紧集的闵可夫斯基维数绝对大于豪斯多夫维数。&lt;br /&gt;
&lt;br /&gt;
=== Hausdorff dimensions and Frostman measures 豪斯多夫维度和弗洛斯曼测度===&lt;br /&gt;
&lt;br /&gt;
If there is a [[measure (mathematics)|measure]] μ defined on [[Borel measure|Borel]] subsets of a metric space ''X'' such that ''μ''(''X'') &amp;gt; 0 and ''μ''(''B''(''x'', ''r'')) ≤ ''r&amp;lt;sup&amp;gt;s&amp;lt;/sup&amp;gt;'' holds for some constant ''s'' &amp;gt; 0 and for every ball ''B''(''x'', ''r'') in ''X'', then dim&amp;lt;sub&amp;gt;Haus&amp;lt;/sub&amp;gt;(''X'') ≥ ''s''. A partial converse is provided by [[Frostman's lemma]].{{citation needed|date=March 2015}}&amp;lt;ref&amp;gt;This Wikipedia article also discusses further useful characterizations of the Hausdorff dimension.{{clarify|date=March 2015}}&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
If there is a measure μ defined on Borel subsets of a metric space X such that μ(X) &amp;gt; 0 and μ(B(x, r)) ≤ r&amp;lt;sup&amp;gt;s&amp;lt;/sup&amp;gt; holds for some constant s &amp;gt; 0 and for every ball B(x, r) in X, then dim&amp;lt;sub&amp;gt;Haus&amp;lt;/sub&amp;gt;(X) ≥ s. A partial converse is provided by Frostman's lemma.&lt;br /&gt;
&lt;br /&gt;
如果在度量空间 ''X'' 的 Borel 子集上定义一个测度 μ，使得''μ''(''X'') &amp;gt; 0 和''μ''(''B''(''x'', ''r'')) ≤ ''r&amp;lt;sup&amp;gt;s&amp;lt;/sup&amp;gt;''，对于某个常数 ''s'' &amp;gt; 0  和 ''X'' 中的每个球 ''B''(''x'', ''r'') 成立，则 dim&amp;lt;sub&amp;gt;Haus&amp;lt;/sub&amp;gt;(''X'') ≥ ''s'' 。 部分逆向转换由弗洛斯曼引理定义。&lt;br /&gt;
&lt;br /&gt;
=== Behaviour under unions and products ===&lt;br /&gt;
&lt;br /&gt;
If &amp;lt;math&amp;gt;X=\bigcup_{i\in I}X_i&amp;lt;/math&amp;gt; is a finite or countable union, then&lt;br /&gt;
&lt;br /&gt;
If &amp;lt;math&amp;gt;X=\bigcup_{i\in I}X_i&amp;lt;/math&amp;gt; is a finite or countable union, then&lt;br /&gt;
&lt;br /&gt;
如果 &amp;lt;math&amp;gt;X=\bigcup_{i\in I}X_i&amp;lt;/math&amp;gt; 是一个有限或可数的联合，则&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \dim_{\operatorname{Haus}}(X) =\sup_{i\in I} \dim_{\operatorname{Haus}}(X_i).&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \dim_{\operatorname{Haus}}(X) =\sup_{i\in I} \dim_{\operatorname{Haus}}(X_i).&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
This can be verified directly from the definition.&lt;br /&gt;
&lt;br /&gt;
This can be verified directly from the definition.&lt;br /&gt;
&lt;br /&gt;
这可以直接从定义得到验证。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
If ''X'' and ''Y'' are non-empty metric spaces, then the Hausdorff dimension of their product satisfies&amp;lt;ref&amp;gt;{{cite journal |author=Marstrand, J. M. |title=The dimension of Cartesian product sets |journal=Proc. Cambridge Philos. Soc. |volume=50 |issue=3 |pages=198–202 |year=1954 |doi=10.1017/S0305004100029236 |bibcode = 1954PCPS...50..198M }}&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
If X and Y are non-empty metric spaces, then the Hausdorff dimension of their product satisfies&lt;br /&gt;
&lt;br /&gt;
如果 ''X'' 和''Y''是非空度量空间，那么它们乘积的豪斯多夫维数满足&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt; \dim_{\operatorname{Haus}}(X\times Y)\ge \dim_{\operatorname{Haus}}(X)+ \dim_{\operatorname{Haus}}(Y).&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \dim_{\operatorname{Haus}}(X\times Y)\ge \dim_{\operatorname{Haus}}(X)+ \dim_{\operatorname{Haus}}(Y).&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
This inequality can be strict. It is possible to find two sets of dimension 0 whose product has dimension 1.&amp;lt;ref&amp;gt;{{cite book  | last = Falconer  | first = Kenneth J.  | title = Fractal geometry. Mathematical foundations and applications  | publisher = John Wiley &amp;amp; Sons, Inc., Hoboken, New Jersey  | year = 2003  | doi =   | isbn = }}&amp;lt;/ref&amp;gt; In the opposite direction, it is known that when ''X'' and ''Y'' are Borel subsets of '''R'''&amp;lt;sup&amp;gt;''n''&amp;lt;/sup&amp;gt;, the Hausdorff dimension of ''X'' × ''Y'' is bounded from above by the Hausdorff dimension of ''X'' plus the [[packing dimension|upper packing dimension]] of ''Y''. These facts are discussed in Mattila (1995).&lt;br /&gt;
&lt;br /&gt;
This inequality can be strict. It is possible to find two sets of dimension 0 whose product has dimension 1. In the opposite direction, it is known that when X and Y are Borel subsets of R&amp;lt;sup&amp;gt;n&amp;lt;/sup&amp;gt;, the Hausdorff dimension of X × Y is bounded from above by the Hausdorff dimension of X plus the upper packing dimension of Y. These facts are discussed in Mattila (1995).&lt;br /&gt;
&lt;br /&gt;
这种不平等可以是绝对的。有可能找到两个维数为0的集合，其乘积的维数为1。相反，我们知道当''X''和''Y''是 '''R'''&amp;lt;sup&amp;gt;''n''&amp;lt;/sup&amp;gt;的 Borel 子集时， ''X'' × ''Y''的豪斯多夫维数从上面以 ''X''的豪斯多夫维数加上 ''Y''的填充维数为界。Mattila (1995)曾就这些情况进行了讨论。&lt;br /&gt;
&lt;br /&gt;
==Self-similar sets自相似集合==&lt;br /&gt;
&lt;br /&gt;
{{refimprove section|date=March 2015}}&lt;br /&gt;
&lt;br /&gt;
Many sets defined by a self-similarity condition have dimensions which can be determined explicitly. Roughly, a set ''E'' is self-similar if it is the fixed point of a set-valued transformation ψ, that is ψ(''E'') = ''E'', although the exact definition is given below.&lt;br /&gt;
&lt;br /&gt;
Many sets defined by a self-similarity condition have dimensions which can be determined explicitly. Roughly, a set E is self-similar if it is the fixed point of a set-valued transformation ψ, that is ψ(E) = E, although the exact definition is given below.&lt;br /&gt;
&lt;br /&gt;
许多由自相似条件定义的集合具有可以显式确定的维数。粗略地说，集合''E'' 是自相似的，如果它是集值ψ变换的不动点，即ψ(''E'') = ''E''，尽管下面给出了确切的定义。&lt;br /&gt;
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&lt;br /&gt;
&lt;br /&gt;
&amp;lt;blockquote&amp;gt;'''Theorem'''. Suppose&lt;br /&gt;
&lt;br /&gt;
&amp;lt;blockquote&amp;gt;Theorem. Suppose&lt;br /&gt;
&lt;br /&gt;
&amp;lt;blockquote&amp;gt;'''定理'''：假设&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt; \psi_i: \mathbf{R}^n \rightarrow \mathbf{R}^n, \quad i=1, \ldots , m &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \psi_i: \mathbf{R}^n \rightarrow \mathbf{R}^n, \quad i=1, \ldots , m &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
are [[Contraction mapping|contractive]] mappings on '''R'''&amp;lt;sup&amp;gt;''n''&amp;lt;/sup&amp;gt; with contraction constant ''r&amp;lt;sub&amp;gt;j&amp;lt;/sub&amp;gt;'' &amp;lt; 1. Then there is a unique ''non-empty'' compact set ''A'' such that&lt;br /&gt;
&lt;br /&gt;
are contractive mappings on R&amp;lt;sup&amp;gt;n&amp;lt;/sup&amp;gt; with contraction constant r&amp;lt;sub&amp;gt;j&amp;lt;/sub&amp;gt; &amp;lt; 1. Then there is a unique non-empty compact set A such that&lt;br /&gt;
&lt;br /&gt;
是'''R'''&amp;lt;sup&amp;gt;''n''&amp;lt;/sup&amp;gt;上的压缩常数''r&amp;lt;sub&amp;gt;j&amp;lt;/sub&amp;gt;'&amp;lt; 1的压缩映射。然后有一个唯一的非空紧集A &lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt; A = \bigcup_{i=1}^m \psi_i (A). &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; A = \bigcup_{i=1}^m \psi_i (A). &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&amp;lt;/blockquote&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;/blockquote&amp;gt;&lt;br /&gt;
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&lt;br /&gt;
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&lt;br /&gt;
The theorem follows from [[Stefan Banach]]'s [[Contractive mapping theorem|contractive mapping fixed point theorem]] applied to the complete metric space of non-empty compact subsets of '''R'''&amp;lt;sup&amp;gt;''n''&amp;lt;/sup&amp;gt; with the [[Hausdorff distance]].&amp;lt;ref&amp;gt;{{cite book |author=Falconer, K. J. |title=The Geometry of Fractal Sets |publisher=Cambridge University Press |location=Cambridge, UK |year=1985 |isbn=0-521-25694-1 |chapter=Theorem 8.3}}&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
The theorem follows from Stefan Banach's contractive mapping fixed point theorem applied to the complete metric space of non-empty compact subsets of R&amp;lt;sup&amp;gt;n&amp;lt;/sup&amp;gt; with the Hausdorff distance.&lt;br /&gt;
&lt;br /&gt;
这个定理来源于 Stefan Banach 的压缩映射不动点定理，该定理应用于 '''R'''&amp;lt;sup&amp;gt;''n''&amp;lt;/sup&amp;gt; 的非空紧子集的完备空间豪斯多夫距离。&lt;br /&gt;
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&lt;br /&gt;
&lt;br /&gt;
===The open set condition开集条件===&lt;br /&gt;
&lt;br /&gt;
To determine the dimension of the self-similar set ''A'' (in certain cases), we need a technical condition called the ''open set condition'' (OSC) on the sequence of contractions ψ&amp;lt;sub&amp;gt;''i''&amp;lt;/sub&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
To determine the dimension of the self-similar set A (in certain cases), we need a technical condition called the open set condition (OSC) on the sequence of contractions ψ&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
为了确定自相似集''A'' 的维数(在某些情况下) ，我们需要一个关于收缩序列的称为''开集条件''(OSC)的技术条件ψ&amp;lt;sub&amp;gt;''i''&amp;lt;/sub&amp;gt;。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
There is a relatively compact open set ''V'' such that&lt;br /&gt;
&lt;br /&gt;
There is a relatively compact open set V such that&lt;br /&gt;
&lt;br /&gt;
有一个相对紧的开集''V''&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt; \bigcup_{i=1}^m\psi_i (V) \subseteq V, &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \bigcup_{i=1}^m\psi_i (V) \subseteq V, &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
where the sets in union on the left are pairwise [[disjoint sets|disjoint]].&lt;br /&gt;
&lt;br /&gt;
where the sets in union on the left are pairwise disjoint.&lt;br /&gt;
&lt;br /&gt;
左边并集的集合成对不相交。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The open set condition is a separation condition that ensures the images ψ&amp;lt;sub&amp;gt;''i''&amp;lt;/sub&amp;gt;(''V'') do not overlap &amp;quot;too much&amp;quot;.&lt;br /&gt;
&lt;br /&gt;
The open set condition is a separation condition that ensures the images ψ&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;(V) do not overlap &amp;quot;too much&amp;quot;.&lt;br /&gt;
&lt;br /&gt;
开集条件是保证图像ψ&amp;lt;sub&amp;gt;''i''&amp;lt;/sub&amp;gt;(''V'') 不重叠“太多”的分离条件。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
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'''Theorem'''. Suppose the open set condition holds and each ψ&amp;lt;sub&amp;gt;''i''&amp;lt;/sub&amp;gt; is a similitude, that is a composition of an [[isometry]] and a [[dilation (metric space)|dilation]] around some point. Then the unique fixed point of ψ is a set whose Hausdorff dimension is ''s'' where ''s'' is the unique solution of&amp;lt;ref&amp;gt;{{cite journal | last=Hutchinson | first=John E. | title=Fractals and self similarity | journal=Indiana Univ. Math. J. | volume=30 | year=1981 | pages=713–747 | doi=10.1512/iumj.1981.30.30055 | issue=5 | doi-access=free }}&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
Theorem. Suppose the open set condition holds and each ψ&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt; is a similitude, that is a composition of an isometry and a dilation around some point. Then the unique fixed point of ψ is a set whose Hausdorff dimension is s where s is the unique solution of&lt;br /&gt;
&lt;br /&gt;
'''定理'''假设开集条件成立，并且每个ψ&amp;lt;sub&amp;gt;''i''&amp;lt;/sub&amp;gt; 是一个相似度，即等距和某个点周围的膨胀的组合。。那么唯一的不动点是Hausdorff维数为 ''s'' 的集合，其中  ''s'' 是 ''s'' &amp;lt;ref&amp;gt;{{cite journal | last=Hutchinson | first=John E. | title=Fractals and self similarity | journal=Indiana Univ. Math. J. | volume=30 | year=1981 | pages=713–747 | doi=10.1512/iumj.1981.30.30055 | issue=5 | doi-access=free }}&amp;lt;/ref&amp;gt;的唯一解&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt; \sum_{i=1}^m r_i^s = 1. &amp;lt;/math&amp;gt;&lt;br /&gt;
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&amp;lt;math&amp;gt; \sum_{i=1}^m r_i^s = 1. &amp;lt;/math&amp;gt;&lt;br /&gt;
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The contraction coefficient of a similitude is the magnitude of the dilation.&lt;br /&gt;
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The contraction coefficient of a similitude is the magnitude of the dilation.&lt;br /&gt;
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相似物的收缩系数就是膨胀的大小。&lt;br /&gt;
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We can use this theorem to compute the Hausdorff dimension of the Sierpinski triangle (or sometimes called Sierpinski gasket). Consider three [[non-collinear points]] ''a''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;, ''a''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;, ''a''&amp;lt;sub&amp;gt;3&amp;lt;/sub&amp;gt; in the plane '''R'''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; and let ψ&amp;lt;sub&amp;gt;''i''&amp;lt;/sub&amp;gt; be the dilation of ratio 1/2 around ''a&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;''. The unique non-empty fixed point of the corresponding mapping ψ is a Sierpinski gasket and the dimension ''s'' is the unique solution of&lt;br /&gt;
&lt;br /&gt;
We can use this theorem to compute the Hausdorff dimension of the Sierpinski triangle (or sometimes called Sierpinski gasket). Consider three non-collinear points a&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;, a&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;, a&amp;lt;sub&amp;gt;3&amp;lt;/sub&amp;gt; in the plane R&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; and let ψ&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt; be the dilation of ratio 1/2 around a&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;. The unique non-empty fixed point of the corresponding mapping ψ is a Sierpinski gasket and the dimension s is the unique solution of&lt;br /&gt;
&lt;br /&gt;
我们可以使用这个定理来计算谢尔宾斯基三角形的豪斯多夫维数(或者有时候叫做谢尔宾斯基垫圈)。考虑R&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; 平面上的三个非共线点，''a''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;，''a''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;，''a''&amp;lt;sub&amp;gt;3&amp;lt;/sub&amp;gt;，让ψ&amp;lt;sub&amp;gt;''i''&amp;lt;/sub&amp;gt;是围绕着''a&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;''比率1/2的膨胀。对应映射的唯一非空不动点是一个谢尔宾斯基垫圈，其维数''s''是对应映射的唯一解&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt; \left(\frac{1}{2}\right)^s+\left(\frac{1}{2}\right)^s+\left(\frac{1}{2}\right)^s = 3 \left(\frac{1}{2}\right)^s =1. &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \left(\frac{1}{2}\right)^s+\left(\frac{1}{2}\right)^s+\left(\frac{1}{2}\right)^s = 3 \left(\frac{1}{2}\right)^s =1. &amp;lt;/math&amp;gt;&lt;br /&gt;
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Taking [[natural logarithm]]s of both sides of the above equation, we can solve for ''s'', that is: ''s'' = ln(3)/ln(2).  The Sierpinski gasket is self-similar and satisfies the OSC. In general a set ''E'' which is a fixed point of a mapping&lt;br /&gt;
&lt;br /&gt;
Taking natural logarithms of both sides of the above equation, we can solve for s, that is: s = ln(3)/ln(2).  The Sierpinski gasket is self-similar and satisfies the OSC. In general a set E which is a fixed point of a mapping&lt;br /&gt;
&lt;br /&gt;
取上述方程两边的自然对数，我们可以求出 ''s''，即: ''s'' = ln(3)/ln(2)。该密封垫具有自相似性，满足 OSC 要求。一般来说，集合 ''E''是一个映射的不动点&lt;br /&gt;
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: &amp;lt;math&amp;gt; A \mapsto \psi(A) = \bigcup_{i=1}^m \psi_i(A) &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt; A \mapsto \psi(A) = \bigcup_{i=1}^m \psi_i(A) &amp;lt;/math&amp;gt;&lt;br /&gt;
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is self-similar if and only if the intersections&lt;br /&gt;
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is self-similar if and only if the intersections&lt;br /&gt;
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是自相似的，当且仅当&lt;br /&gt;
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:&amp;lt;math&amp;gt; H^s\left(\psi_i(E) \cap \psi_j(E)\right) =0, &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; H^s\left(\psi_i(E) \cap \psi_j(E)\right) =0, &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
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where ''s'' is the Hausdorff dimension of ''E'' and ''H&amp;lt;sup&amp;gt;s&amp;lt;/sup&amp;gt;'' denotes [[Hausdorff measure]]. This is clear in the case of the Sierpinski gasket (the intersections are just points), but is also true more generally:&lt;br /&gt;
&lt;br /&gt;
where s is the Hausdorff dimension of E and H&amp;lt;sup&amp;gt;s&amp;lt;/sup&amp;gt; denotes Hausdorff measure. This is clear in the case of the Sierpinski gasket (the intersections are just points), but is also true more generally:&lt;br /&gt;
&lt;br /&gt;
其中 ''s''是''E''的豪斯多夫维数， ''H&amp;lt;sup&amp;gt;s&amp;lt;/sup&amp;gt;'' 表示 豪斯多夫测度。对于谢尔宾斯基垫圈(交叉点就是点)来说，这一点很明显，但更普遍的情况是:&lt;br /&gt;
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'''Theorem'''. Under the same conditions as the previous theorem, the unique fixed point of ψ is self-similar.&lt;br /&gt;
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Theorem. Under the same conditions as the previous theorem, the unique fixed point of ψ is self-similar.&lt;br /&gt;
&lt;br /&gt;
'''定理'''：在与前一定理相同的条件下，其唯一不动点是自相似的。&lt;br /&gt;
&lt;br /&gt;
==See also参阅==&lt;br /&gt;
&lt;br /&gt;
* [[List of fractals by Hausdorff dimension豪斯多夫分形维数列表]] Examples of deterministic fractals, random and natural fractals.确定性分形与随机和自然分形的示例。&lt;br /&gt;
&lt;br /&gt;
* [[Assouad dimension  Assouad维数]], another variation of fractal dimension that, like Hausdorff dimension, is defined using coverings by balls其他被球覆盖方式定义的分形维数，例如豪斯多夫维数。&lt;br /&gt;
&lt;br /&gt;
* [[Intrinsic dimension固有维数]]&lt;br /&gt;
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* [[Packing dimension填充维数]]&lt;br /&gt;
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* [[Fractal dimension分形维数]]&lt;br /&gt;
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==References参考文献==&lt;br /&gt;
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{{reflist}}&lt;br /&gt;
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==Further reading拓展阅读==&lt;br /&gt;
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* {{cite book |last1=Dodson |first1=M. Maurice |title=Fractal Geometry and Applications: A Jubilee of Benoît Mandelbrot |volume=72 |issue=1 |pages=305–347 |last2=Kristensen |first2=Simon |chapter=Hausdorff Dimension and Diophantine Approximation |date=June 12, 2003 |arxiv=math/0305399 |bibcode = 2003math......5399D |doi=10.1090/pspum/072.1/2112110|series=Proceedings of Symposia in Pure Mathematics |isbn=9780821836378 }}&lt;br /&gt;
&lt;br /&gt;
* {{cite book |last1=Hurewicz |first1=Witold |authorlink1=Witold Hurewicz |last2=Wallman |first2=Henry |authorlink2=Henry Wallman |title=Dimension Theory |url=https://archive.org/details/in.ernet.dli.2015.84609 |publisher=Princeton University Press |year=1948 }}&lt;br /&gt;
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* {{cite journal |author作者=E. Szpilrajn |authorlink=Edward Marczewski |title=La dimension et la mesure |journal=Fundamenta Mathematicae |volume=28 |pages=81–9 |year=1937 }}&lt;br /&gt;
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* {{cite journal&lt;br /&gt;
&lt;br /&gt;
 | last1=Marstrand&lt;br /&gt;
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 | last1=Marstrand&lt;br /&gt;
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 | last1=马斯特兰德&lt;br /&gt;
&lt;br /&gt;
 | first1=J. M. | title=The dimension of cartesian product sets | year=1954 | journal=Proc. Cambridge Philos. Soc.&lt;br /&gt;
&lt;br /&gt;
 | first1=J. M. | title=The dimension of cartesian product sets | year=1954 | journal=Proc. Cambridge Philos. Soc.&lt;br /&gt;
&lt;br /&gt;
 | first1= J. M. | title=笛卡儿积集的维数 | 1954年 |  journal=Proc. Cambridge Philos. Soc.&lt;br /&gt;
&lt;br /&gt;
 | volume=50&lt;br /&gt;
&lt;br /&gt;
 | volume=50&lt;br /&gt;
&lt;br /&gt;
 | 第50卷&lt;br /&gt;
&lt;br /&gt;
 | issue=3&lt;br /&gt;
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 | issue=3&lt;br /&gt;
&lt;br /&gt;
 | 第三期&lt;br /&gt;
&lt;br /&gt;
 | pages=198–202&lt;br /&gt;
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 | pages=198–202&lt;br /&gt;
&lt;br /&gt;
 | 第198-202页&lt;br /&gt;
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 | doi=10.1017/S0305004100029236|bibcode = 1954PCPS...50..198M }}&lt;br /&gt;
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 | doi=10.1017/S0305004100029236|bibcode = 1954PCPS...50..198M }}&lt;br /&gt;
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10.1017 / S0305004100029236 | bibcode 1954PCPS... 50. . 198 m }&lt;br /&gt;
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* {{Cite book&lt;br /&gt;
&lt;br /&gt;
 | last1=Mattila&lt;br /&gt;
&lt;br /&gt;
 | last1=Mattila&lt;br /&gt;
&lt;br /&gt;
 | last1=Mattila&lt;br /&gt;
&lt;br /&gt;
 | first1=Pertti | author1-link=Pertti Mattila| title=Geometry of sets and measures in Euclidean spaces | publisher=[[Cambridge University Press]]&lt;br /&gt;
&lt;br /&gt;
 | first1=Pertti | author1-link=Pertti Mattila| title=Geometry of sets and measures in Euclidean spaces | publisher=Cambridge University Press&lt;br /&gt;
&lt;br /&gt;
| first1 Pertti | author1-link Pertti Mattila | title 欧几里德空间中集合和度量的几何 | 出版商剑桥大学出版社&lt;br /&gt;
&lt;br /&gt;
 | isbn=978-0-521-65595-8 | year=1995}}&lt;br /&gt;
&lt;br /&gt;
 | isbn=978-0-521-65595-8 | year=1995}}&lt;br /&gt;
&lt;br /&gt;
| isbn 978-0-521-65595-8 | year 1995}&lt;br /&gt;
&lt;br /&gt;
* {{cite journal |author=A. S. Besicovitch |authorlink=A. S. Besicovitch |title=On Linear Sets of Points of Fractional Dimensions |journal=[[Mathematische Annalen]] |volume=101 |year=1929 | doi=10.1007/BF01454831| issue=1 |pages= 161–193}}&lt;br /&gt;
&lt;br /&gt;
* {{cite journal |author1=A. S. Besicovitch |authorlink1=A. S. Besicovitch |author2=H. D. Ursell |authorlink2=H. D. Ursell |title=Sets of Fractional Dimensions |journal=Journal of the London Mathematical Society |volume=12 |year=1937 | issue=1 | doi=10.1112/jlms/s1-12.45.18  | pages=18–25 }}&amp;lt;br/&amp;gt;Several selections from this volume are reprinted in {{cite book |author=Edgar, Gerald A. |title=Classics on fractals |publisher=Addison-Wesley |location=Boston |year=1993 |isbn=0-201-58701-7}} See chapters 9,10,11&lt;br /&gt;
&lt;br /&gt;
* {{cite journal |author=F. Hausdorff |authorlink=F. Hausdorff |title=Dimension und äußeres Maß |journal=Mathematische Annalen |volume=79 |issue=1–2 |pages=157–179 |date=March 1919 |doi=10.1007/BF01457179|hdl=10338.dmlcz/100363 |url=http://dml.cz/bitstream/handle/10338.dmlcz/100363/CzechMathJ_09-1959-3_5.pdf }}&lt;br /&gt;
&lt;br /&gt;
* {{cite journal | last=Hutchinson | first=John E. | title=Fractals and self similarity | journal=Indiana Univ. Math. J. | volume=30 | year=1981 | pages=713–747 | doi=10.1512/iumj.1981.30.30055 | issue=5 | doi-access=free }}&lt;br /&gt;
&lt;br /&gt;
*{{cite book | last=Falconer | first = Kenneth |title=Fractal Geometry: Mathematical Foundations and Applications | publisher=[[John Wiley and Sons]] | edition=2nd | year=2003}}&lt;br /&gt;
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==External links外部链接==&lt;br /&gt;
&lt;br /&gt;
* [https://www.encyclopediaofmath.org/index.php/Hausdorff_dimension Hausdorff dimension] 在 [https://www.encyclopediaofmath.org/ Encyclopedia of Mathematics]&lt;br /&gt;
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* [https://www.encyclopediaofmath.org/index.php/Hausdorff_measure Hausdorff measure] 在 [https://www.encyclopediaofmath.org/ Encyclopedia of Mathematics]&lt;br /&gt;
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{{DEFAULTSORT:Hausdorff Dimension豪斯多夫维数}}&lt;br /&gt;
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[[Category分类:Fractals分形]]&lt;br /&gt;
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[[Category分类:Metric geometry度量几何]]&lt;br /&gt;
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[[Category分类:Dimension theory维度理论]]&lt;br /&gt;
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&amp;lt;small&amp;gt;This page was moved from [[wikipedia:en:Hausdorff dimension]]. Its edit history can be viewed at [[分形维数/edithistory]]&amp;lt;/small&amp;gt;&amp;lt;/noinclude&amp;gt;&lt;br /&gt;
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[[Category:待整理页面]]&lt;/div&gt;</summary>
		<author><name>Ruili</name></author>
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	<entry>
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		<title>分形维数</title>
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		<updated>2020-11-01T16:59:38Z</updated>

		<summary type="html">&lt;p&gt;Ruili：&lt;/p&gt;
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&lt;div&gt;此词条暂由彩云小译翻译，未经人工整理和审校，带来阅读不便，请见谅。&lt;br /&gt;
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{{short description|Invariant}}&lt;br /&gt;
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Example of non-integer dimensions. The first four [[iteration]]s of the [[Koch snowflake|Koch curve]], where after each iteration, all original line segments are replaced with four, each a self-similar copy that is 1/3 the length of the original. One formalism of the Hausdorff dimension uses this scale factor (3) and the number of self-similar objects (4) to calculate the dimension, D, after the first iteration to be D = (log N)/(log S) = (log 4)/(log 3) ≈ 1.26.&amp;lt;ref name=CampbellAnnenberg15&amp;gt;MacGregor Campbell, 2013, &amp;quot;5.6 Scaling and the Hausdorff Dimension,&amp;quot; at ''Annenberg Learner:MATHematics illuminated'', see [http://www.learner.org/courses/mathilluminated/units/5/textbook/06.php], accessed 5 March 2015.&amp;lt;/ref&amp;gt; That is, while the Hausdorff dimension of a single [[point (geometry)|point]] is zero, of a [[line segment]] is 1, of a [[square]] is 2, and of a [[cube]] is 3, for [[fractal]]s such as this, the object can have a non-integer dimension.&lt;br /&gt;
&lt;br /&gt;
Example of non-integer dimensions. The first four iterations of the Koch curve, where after each iteration, all original line segments are replaced with four, each a self-similar copy that is 1/3 the length of the original. One formalism of the Hausdorff dimension uses this scale factor (3) and the number of self-similar objects (4) to calculate the dimension, D, after the first iteration to be D = (log N)/(log S) = (log 4)/(log 3) ≈ 1.26. That is, while the Hausdorff dimension of a single point is zero, of a line segment is 1, of a square is 2, and of a cube is 3, for fractals such as this, the object can have a non-integer dimension.&lt;br /&gt;
&lt;br /&gt;
非整数维度示例：前四个[[Koch 曲线]]的迭代，在每次迭代后，所有原始线段都被替换为四个，每个自相似的复制是原始线段长度的1 / 3。豪斯多夫维数的一个建模是使用比例因子(3)和自相似对象的数量(4)来计算维度 D，在第一次迭代后为 D = (log N)/(log S) = (log 4)/(log 3) ≈ 1.26.&amp;lt;ref name=CampbellAnnenberg15&amp;gt;。MacGregor Campbell, 2013, &amp;quot;5.6 Scaling and the Hausdorff Dimension,&amp;quot; 在 ''Annenberg Learner:MATHematics illuminated'', 参见 [http://www.learner.org/courses/mathilluminated/units/5/textbook/06.php], accessed 5 March 2015.&amp;lt;/ref&amp;gt; 也就是说，单点的豪斯多夫维数为零，线段为1，正方形为2，立方体为3时，但对于分形，对象可以有一个非整数维度。&lt;br /&gt;
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In [[mathematics]], '''Hausdorff dimension''' is a measure of ''roughness'', or more specifically, [[fractal dimension]], that was first introduced in 1918 by [[mathematician]] [[Felix Hausdorff]].&amp;lt;ref&amp;gt;{{Cite journal |arxiv = 1101.1444|doi = 10.1214/11-STS370|title = Estimators of Fractal Dimension: Assessing the Roughness of Time Series and Spatial Data|journal = Statistical Science|volume = 27|issue = 2|pages = 247–277|year = 2012|last1 = Gneiting|first1 = Tilmann|last2 = Ševčíková|first2 = Hana|last3 = Percival|first3 = Donald B.}}&amp;lt;/ref&amp;gt; For instance, the Hausdorff dimension of a single [[point (geometry)|point]] is zero, of a [[line segment]] is 1, of a [[square]] is 2, and of a [[cube]] is 3. That is, for sets of points that define a smooth shape or a shape that has a small number of corners—the shapes of traditional geometry and science—the Hausdorff dimension is an [[integer]] agreeing with the usual sense of dimension, also known as the [[Inductive dimension|topological dimension]]. However, formulas have also been developed that allow calculation of the dimension of other less simple objects, where, solely on the basis of their properties of [[scaling (geometry)|scaling]] and [[self-similarity]], one is led to the conclusion that particular objects—including [[fractal]]s—have non-integer Hausdorff dimensions. Because of the significant technical advances made by [[Abram Samoilovitch Besicovitch]] allowing computation of dimensions for highly irregular or &amp;quot;rough&amp;quot; sets, this dimension is also commonly referred to as the ''Hausdorff–Besicovitch dimension.''&lt;br /&gt;
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In mathematics, Hausdorff dimension is a measure of roughness, or more specifically, fractal dimension, that was first introduced in 1918 by mathematician Felix Hausdorff. For instance, the Hausdorff dimension of a single point is zero, of a line segment is 1, of a square is 2, and of a cube is 3. That is, for sets of points that define a smooth shape or a shape that has a small number of corners—the shapes of traditional geometry and science—the Hausdorff dimension is an integer agreeing with the usual sense of dimension, also known as the topological dimension. However, formulas have also been developed that allow calculation of the dimension of other less simple objects, where, solely on the basis of their properties of scaling and self-similarity, one is led to the conclusion that particular objects—including fractals—have non-integer Hausdorff dimensions. Because of the significant technical advances made by Abram Samoilovitch Besicovitch allowing computation of dimensions for highly irregular or &amp;quot;rough&amp;quot; sets, this dimension is also commonly referred to as the Hausdorff–Besicovitch dimension.&lt;br /&gt;
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在[[数学]]中，'''&amp;lt;font color = '#ff8000'&amp;gt;豪斯多夫维数Hausdorff dimension&amp;lt;/font&amp;gt;'''是一种粗糙度的度量单位，或者更确切地说，分形维数，是由数学家 Felix Hausdorff 在1918年首次提出的。例如，单点的豪斯多夫维数为零，线段为1，正方形为2，立方体为3。也就是说，对于定义了一个光滑形状或一个有少数几个角的形状---- 传统几何学和科学的形状---- 的点集来说，豪斯多夫维数是一个整数，符合通常的维度意义，也称为拓扑维度。然而，还有一些公式允许计算其他不太简单的对象的维数，其中仅仅根据它们的标度和自相似特性，就可以得出结论: 特定的对象ー包括分形ー具有非整数的 Hausdorff 维数。由于阿布拉姆·萨莫伊洛维奇·贝西科维奇的重大技术进步，允许计算高度不规则或“粗糙”集的维度，这个维度通常也被称为 Hausdorff-Besicovitch 维度。 &lt;br /&gt;
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The Hausdorff dimension, more specifically, is a further dimensional number associated with a given set, where the distances between all members of that set are defined. Such a set is termed a [[metric space]]. The dimension is drawn from the [[Extended real number line|extended real numbers]], &amp;lt;math&amp;gt;\overline{\mathbb{R}}&amp;lt;/math&amp;gt;, as opposed to the more intuitive notion of dimension, which is not associated to general metric spaces, and only takes values in the non-negative integers.&lt;br /&gt;
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The Hausdorff dimension, more specifically, is a further dimensional number associated with a given set, where the distances between all members of that set are defined. Such a set is termed a metric space. The dimension is drawn from the extended real numbers, &amp;lt;math&amp;gt;\overline{\mathbb{R}}&amp;lt;/math&amp;gt;, as opposed to the more intuitive notion of dimension, which is not associated to general metric spaces, and only takes values in the non-negative integers.&lt;br /&gt;
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更具体地说，豪斯多夫维数是一个与给定集合相关联的更进一步的维数，其中定义了该集合所有成员之间的距离。这样的集合称为度量空间。维数是从扩展的实数，&amp;lt;math&amp;gt;\overline{\mathbb{R}}&amp;lt;/math&amp;gt;，而不是更直观的维数概念(它不与一般的度量空间相关联，只取非负整数的值)。&lt;br /&gt;
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In mathematical terms, the Hausdorff dimension generalizes the notion of the dimension of a real [[vector space]]. That is, the Hausdorff dimension of an ''n''-dimensional [[inner product space]] equals ''n''. This underlies the earlier statement that the Hausdorff dimension of a point is zero, of a line is one, etc., and that [[fractal|irregular sets]] can have noninteger Hausdorff dimensions. For instance, the [[Koch snowflake]] shown at right is constructed from an equilateral triangle; in each iteration, its component line segments are divided into 3 segments of unit length, the newly created middle segment is used as the base of a new [[equilateral]] triangle that points outward, and this base segment is then deleted to leave a final object from the iteration of unit length of 4.&amp;lt;ref&amp;gt;Larry Riddle, 2014, &amp;quot;Classic Iterated Function Systems: Koch Snowflake&amp;quot;, Agnes Scott College e-Academy (online), see [http://ecademy.agnesscott.edu/~lriddle/ifs/ksnow/ksnow.htm], accessed 5 March 2015.&amp;lt;/ref&amp;gt; That is, after the first iteration, each original line segment has been replaced with N=4, where each self-similar copy is 1/S = 1/3 as long as the original.&amp;lt;ref name=CampbellAnnenberg15/&amp;gt; Stated another way, we have taken an object with Euclidean dimension, D, and reduced its linear scale by 1/3 in each direction, so that its length increases to N=S&amp;lt;sup&amp;gt;D&amp;lt;/sup&amp;gt;.&amp;lt;ref name=ClaytonSCTPLS96&amp;gt;Keith Clayton, 1996, &amp;quot;Fractals and the Fractal Dimension,&amp;quot; ''Basic Concepts in Nonlinear Dynamics and Chaos'' (workshop), Society for Chaos Theory in Psychology and the Life Sciences annual meeting, June 28, 1996, Berkeley, California, see [http://www.vanderbilt.edu/AnS/psychology/cogsci/chaos/workshop/Workshop.html], accessed 5 March 2015.&amp;lt;/ref&amp;gt; This equation is easily solved for D, yielding the ratio of logarithms (or [[natural logarithm]]s) appearing in the figures, and giving—in the Koch and other fractal cases—non-integer dimensions for these objects.&lt;br /&gt;
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In mathematical terms, the Hausdorff dimension generalizes the notion of the dimension of a real vector space. That is, the Hausdorff dimension of an n-dimensional inner product space equals n. This underlies the earlier statement that the Hausdorff dimension of a point is zero, of a line is one, etc., and that irregular sets can have noninteger Hausdorff dimensions. For instance, the Koch snowflake shown at right is constructed from an equilateral triangle; in each iteration, its component line segments are divided into 3 segments of unit length, the newly created middle segment is used as the base of a new equilateral triangle that points outward, and this base segment is then deleted to leave a final object from the iteration of unit length of 4. That is, after the first iteration, each original line segment has been replaced with N=4, where each self-similar copy is 1/S = 1/3 as long as the original. This equation is easily solved for D, yielding the ratio of logarithms (or natural logarithms) appearing in the figures, and giving—in the Koch and other fractal cases—non-integer dimensions for these objects.&lt;br /&gt;
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用数学术语来说，豪斯多夫维数概括了实向量空间维数的概念。也就是说，n 维内积空间的豪斯多夫维数等于 n。 这就是早期假设的基础，一个点的豪斯多夫维数是零，一条线是一等等，不规则集可以有非整数的豪斯多夫维数。例如，右边所示的 Koch 雪花是由一个正三角形构成的; 在每次迭代中，它的组成线段被分成单位长度的3段，新创建的中间线段被用作一个指向外部的新正三角形的基础，然后人们删除这个基础线段用来保留单位长度4的迭代中的最终对象。也就是说，在第一次迭代之后，每个原始线段都被替换为 N=4，其中每个自相似拷贝的长度是原始线段的1/S = 1/3 。这个方程很容易求解为 D，产生出现在图形中的对数(或自然对数)的比率，并给出——在 Koch 和其他分形情况下——这些对象的非整数维数。&lt;br /&gt;
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The Hausdorff dimension is a successor to the simpler, but usually equivalent, box-counting or [[Minkowski–Bouligand dimension]].&lt;br /&gt;
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The Hausdorff dimension is a successor to the simpler, but usually equivalent, box-counting or Minkowski–Bouligand dimension.&lt;br /&gt;
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豪斯多夫维数是更简单但通常等价的'''&amp;lt;font color = '#ff8000'&amp;gt;计盒维数box-counting&amp;lt;/font&amp;gt;'''或'''&amp;lt;font color = '#ff8000'&amp;gt;闵可夫斯基维数Minkowski-Bouligand&amp;lt;/font&amp;gt;'''的继承者。&lt;br /&gt;
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==Intuition概念==&lt;br /&gt;
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The intuitive concept of dimension of a geometric object ''X'' is the number of independent parameters one needs to pick out a unique point inside. However, any point specified by two parameters can be instead specified by one, because the [[cardinality]] of the [[real plane]] is equal to the cardinality of the [[real line]] (this can be seen by an [[Cantor's diagonal argument|argument]] involving interweaving the digits of two numbers to yield a single number encoding the same information). The example of a [[space-filling curve]] shows that one can even map the real line to the real plane [[Surjective function|surjectively]] (taking one real number into a pair of real numbers in a way so that all pairs of numbers are covered) and ''continuously'', so that a one-dimensional object completely fills up a higher-dimensional object.&lt;br /&gt;
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The intuitive concept of dimension of a geometric object X is the number of independent parameters one needs to pick out a unique point inside. However, any point specified by two parameters can be instead specified by one, because the cardinality of the real plane is equal to the cardinality of the real line (this can be seen by an argument involving interweaving the digits of two numbers to yield a single number encoding the same information). The example of a space-filling curve shows that one can even map the real line to the real plane surjectively (taking one real number into a pair of real numbers in a way so that all pairs of numbers are covered) and continuously, so that a one-dimensional object completely fills up a higher-dimensional object.&lt;br /&gt;
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几何对象X的尺寸的直观概念是指需要多少个独立参数才能找到一个独特的点。但是，任何由两个参数指定的点都可以由一个参数指定，因为为实平面的基数等于实线的基数(这可以通过交织两个数字以产生一个编码相同信息的单个数字看到)。'''&amp;lt;font color = '#ff8000'&amp;gt;皮亚诺曲线&amp;lt;/font&amp;gt;'''的例子表明，可以将实线完美和连续地映射到实平面(把一个实数转换成一对实数，从而覆盖所有实数对)，由此一维对象完全填充了一个高维对象。&lt;br /&gt;
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Every space filling curve hits some points multiple times, and does not have a continuous inverse. It is impossible to map two dimensions onto one in a way that is continuous and continuously invertible. The topological dimension, also called [[Lebesgue covering dimension]], explains why. This dimension is ''n'' if, in every covering of ''X'' by small open balls, there is at least one point where ''n''&amp;amp;nbsp;+&amp;amp;nbsp;1 balls overlap. For example, when one covers a line with short open intervals, some points must be covered twice, giving dimension&amp;amp;nbsp;''n''&amp;amp;nbsp;=&amp;amp;nbsp;1.&lt;br /&gt;
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Every space filling curve hits some points multiple times, and does not have a continuous inverse. It is impossible to map two dimensions onto one in a way that is continuous and continuously invertible. The topological dimension, also called Lebesgue covering dimension, explains why. This dimension is n if, in every covering of X by small open balls, there is at least one point where n&amp;amp;nbsp;+&amp;amp;nbsp;1 balls overlap. For example, when one covers a line with short open intervals, some points must be covered twice, giving dimension&amp;amp;nbsp;n&amp;amp;nbsp;=&amp;amp;nbsp;1.&lt;br /&gt;
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每条空间填充曲线都会多次击中某些点，且不存在连续的逆。将二维以连续和连续可逆的方式映射到一维是不可能的。'''&amp;lt;font color = '#ff8000'&amp;gt;拓扑维度 topological dimension&amp;lt;/font&amp;gt;'''，也被称为Lebesgue覆盖维数，解释了为什么。如果在 x 的每个小开球覆盖中，至少有一个点 n + 1个球重叠，这个维度是 n。例如，当用短的开区间覆盖一条线时，某些点必须被覆盖两次，给出维数''n''&amp;amp;nbsp;=&amp;amp;nbsp;1。&lt;br /&gt;
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But topological dimension is a very crude measure of the local size of a space (size near a point). A curve that is almost space-filling can still have topological dimension one, even if it fills up most of the area of a region. A [[fractal]] has an integer topological dimension, but in terms of the amount of space it takes up, it behaves like a higher-dimensional space.&lt;br /&gt;
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But topological dimension is a very crude measure of the local size of a space (size near a point). A curve that is almost space-filling can still have topological dimension one, even if it fills up most of the area of a region. A fractal has an integer topological dimension, but in terms of the amount of space it takes up, it behaves like a higher-dimensional space.&lt;br /&gt;
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但是，拓扑维度是对空间局部尺寸(点附近的尺寸)的一个非常粗略的度量。一条几乎是空间填充的曲线仍然可以有一维拓扑，即使它填充了一个区域的大部分面积。分形具有整数的拓扑维数，但就其所占的空间量而言，它看起来像一个更高维的空间。&lt;br /&gt;
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The Hausdorff dimension measures the local size of a space taking into account the distance between points, the [[metric space|metric]]. Consider the number ''N''(''r'') of [[ball (mathematics)|balls]] of radius at most ''r'' required to cover ''X'' completely. When ''r'' is very small, ''N''(''r'') grows polynomially with 1/''r''. For a sufficiently well-behaved  ''X'', the Hausdorff dimension is the unique number ''d'' such that N(''r'') grows as 1/''r&amp;lt;sup&amp;gt;d&amp;lt;/sup&amp;gt;'' as ''r'' approaches zero. More precisely, this defines the [[Minkowski–Bouligand dimension|box-counting dimension]], which equals the Hausdorff dimension when the value ''d'' is a critical boundary between growth rates that are insufficient to cover the space, and growth rates that are overabundant.&lt;br /&gt;
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The Hausdorff dimension measures the local size of a space taking into account the distance between points, the metric. Consider the number N(r) of balls of radius at most r required to cover X completely. When r is very small, N(r) grows polynomially with 1/r. For a sufficiently well-behaved  X, the Hausdorff dimension is the unique number d such that N(r) grows as 1/r&amp;lt;sup&amp;gt;d&amp;lt;/sup&amp;gt; as r approaches zero. More precisely, this defines the box-counting dimension, which equals the Hausdorff dimension when the value d is a critical boundary between growth rates that are insufficient to cover the space, and growth rates that are overabundant.&lt;br /&gt;
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豪斯多夫维数测量一个空间的局部大小时，会考虑到点之间距离的度量。考虑半径最大为 r 的球数 ''N'' (r) ，需要完全覆盖 ''X''。当 r 很小时，n (r)以1/''r'' 增长多项式。对于一个表现足够好的 ''X''，豪斯多夫维数是唯一的数 d，这样当 r 趋近于零时， N(r)增长为1/r&amp;lt;sup&amp;gt;d&amp;lt;/sup&amp;gt; 。更确切地说，这定义了盒子计数维度，当值 d 是不足以覆盖空间的增长率和过度充裕的增长率之间的关键边界时，它等于豪斯多夫维数。&lt;br /&gt;
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For shapes that are smooth, or shapes with a small number of corners, the shapes of traditional geometry and science, the Hausdorff dimension is an integer agreeing with the topological dimension. But [[Benoit Mandelbrot]] observed that [[fractal]]s, sets with noninteger Hausdorff dimensions, are found everywhere in nature. He observed that the proper idealization of most rough shapes you see around you is not in terms of smooth idealized shapes, but in terms of fractal idealized shapes:&lt;br /&gt;
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For shapes that are smooth, or shapes with a small number of corners, the shapes of traditional geometry and science, the Hausdorff dimension is an integer agreeing with the topological dimension. But Benoit Mandelbrot observed that fractals, sets with noninteger Hausdorff dimensions, are found everywhere in nature. He observed that the proper idealization of most rough shapes you see around you is not in terms of smooth idealized shapes, but in terms of fractal idealized shapes:&lt;br /&gt;
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对于光滑的形状，或者有少量棱角的形状，传统几何和科学的形状，豪斯多夫维数是一个整数，与拓扑维度一致。但是伯努·曼德布洛特观察到分形---- 具有非整数豪斯多夫维数的集合---- 在自然界中随处可见。他观察到，我们周围大多数粗糙形状的理想化不是光滑的理想化形状，而是分形理想化形状:&lt;br /&gt;
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&amp;lt;blockquote&amp;gt;Clouds are not spheres, mountains are not cones, coastlines are not circles, and bark is not smooth, nor does lightning travel in a straight line.&amp;lt;ref name=&amp;quot;mandelbrot&amp;quot;&amp;gt;{{cite book   | last = Mandelbrot   | first = Benoît   | authorlink = Benoit Mandelbrot   | title = The Fractal Geometry of Nature   | publisher = W. H. Freeman   | series = Lecture notes in mathematics 1358   | year = 1982   | doi =    | isbn = 0-7167-1186-9   | url-access = registration   | url = https://archive.org/details/fractalgeometryo00beno   }}&amp;lt;/ref&amp;gt;&amp;lt;/blockquote&amp;gt;&lt;br /&gt;
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&amp;lt;blockquote&amp;gt;Clouds are not spheres, mountains are not cones, coastlines are not circles, and bark is not smooth, nor does lightning travel in a straight line.&amp;lt;/blockquote&amp;gt;&lt;br /&gt;
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&amp;lt;blockquote&amp;gt;云不是球体，山不是锥体，海岸线不是圆圈，树皮不平滑，闪电也不是直线运动。 &amp;lt;/blockquote&amp;gt;&lt;br /&gt;
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For fractals that occur in nature, the Hausdorff and [[Minkowski–Bouligand dimension|box-counting dimension]] coincide. The [[packing dimension]] is yet another similar notion which gives the same value for many shapes, but there are well documented exceptions where all these dimensions differ.&lt;br /&gt;
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For fractals that occur in nature, the Hausdorff and box-counting dimension coincide. The packing dimension is yet another similar notion which gives the same value for many shapes, but there are well documented exceptions where all these dimensions differ.&lt;br /&gt;
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对于自然界中出现的分形，豪斯多夫维数和盒计数维数是一致的。封装尺寸是另一个类似的概念，它给出了许多形状相同的值，但是在所有这些尺寸不同的情况，都做了很好的说明。&lt;br /&gt;
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==Formal definitions形式化定义==&lt;br /&gt;
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===Hausdorff content豪斯多夫集===&lt;br /&gt;
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Let ''X'' be a [[metric space]]. If ''S'' ⊂ ''X'' and ''d'' ∈ [0, ∞), the ''d''-dimensional '''unlimited Hausdorff content''' of ''S'' is defined by&lt;br /&gt;
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Let X be a metric space. If S ⊂ X and d ∈ [0, ∞), the d-dimensional unlimited Hausdorff content of S is defined by&lt;br /&gt;
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设 ''X''是度量空间。若''S'' ⊂ ''X'' 和 ''d'' ∈ [0, ∞) ，则 ''S'' 的''d''维无限 豪斯多夫集定义为&lt;br /&gt;
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:&amp;lt;math&amp;gt;C_H^d(S):=\inf\Bigl\{\sum_i r_i^d:\text{ there is a cover of } S\text{ by balls with radii }r_i&amp;gt;0\Bigr\}.&amp;lt;/math&amp;gt;&lt;br /&gt;
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&amp;lt;math&amp;gt;C_H^d(S):=\inf\Bigl\{\sum_i r_i^d:\text{ there is a cover of } S\text{ by balls with radii }r_i&amp;gt;0\Bigr\}.&amp;lt;/math&amp;gt;&lt;br /&gt;
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&amp;lt;math&amp;gt;C_H^d(S):=\inf\Bigl\{\sum_i r_i^d:\text{ there is a cover of } S\text{ by balls with radii }r_i&amp;gt;0\Bigr\}.&amp;lt;/math&amp;gt;&lt;br /&gt;
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In other words, &amp;lt;math&amp;gt;C_H^d(S)&amp;lt;/math&amp;gt; is the [[infimum]] of the set of numbers &amp;lt;math&amp;gt;\delta \geq 0&amp;lt;/math&amp;gt; such that there is some (indexed) collection of [[ball (mathematics)|ball]]s &amp;lt;math&amp;gt;\{B(x_i,r_i):i\in I\}&amp;lt;/math&amp;gt; covering ''S'' with ''r&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;''&amp;amp;nbsp;&amp;gt;&amp;amp;nbsp;0 for each ''i''&amp;amp;nbsp;∈&amp;amp;nbsp;''I'' that satisfies &amp;lt;math&amp;gt;\sum_{i\in I} r_i^d&amp;lt;\delta &amp;lt;/math&amp;gt;. (Here, we use the standard convention that [[infimum|inf&amp;amp;nbsp;Ø&amp;amp;nbsp;=&amp;amp;nbsp;∞]].)&lt;br /&gt;
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In other words, &amp;lt;math&amp;gt;C_H^d(S)&amp;lt;/math&amp;gt; is the infimum of the set of numbers &amp;lt;math&amp;gt;\delta \geq 0&amp;lt;/math&amp;gt; such that there is some (indexed) collection of balls &amp;lt;math&amp;gt;\{B(x_i,r_i):i\in I\}&amp;lt;/math&amp;gt; covering S with r&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;&amp;amp;nbsp;&amp;gt;&amp;amp;nbsp;0 for each i&amp;amp;nbsp;∈&amp;amp;nbsp;I that satisfies &amp;lt;math&amp;gt;\sum_{i\in I} r_i^d&amp;lt;\delta &amp;lt;/math&amp;gt;. (Here, we use the standard convention that inf&amp;amp;nbsp;Ø&amp;amp;nbsp;=&amp;amp;nbsp;∞.)&lt;br /&gt;
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换句话说，&amp;lt;math&amp;gt;C_H^d(S)&amp;lt;/math&amp;gt; 是数字集合&amp;lt;math&amp;gt;\delta \geq 0&amp;lt;/math&amp;gt;的下确界，使得在 ''i''&amp;amp;nbsp;∈&amp;amp;nbsp中存在一些球集合 &amp;lt;math&amp;gt;\{B(x_i,r_i):i\in I\}&amp;lt;/math&amp;gt;  i 包含 s，对于每个 ''r&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;''&amp;amp;nbsp;&amp;gt;&amp;amp;nbsp;0 满足 i 中的和&amp;lt;math&amp;gt;\sum_{i\in I} r_i^d&amp;lt;\delta &amp;lt;/math&amp;gt; (在这里，我们使用inf&amp;amp;nbsp;Ø&amp;amp;nbsp;=&amp;amp;nbsp;∞ )的标准约定。&lt;br /&gt;
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===Hausdorff measurement豪斯多夫分形测量===&lt;br /&gt;
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The Hausdorff outer measure is different from the unbounded Hausdorf content in that rather than considering all possible coverings of ''S'', we see what happens when the sizes of the balls go to zero. This is  for &amp;lt;math&amp;gt;d \geq 0 &amp;lt;/math&amp;gt;, we define the ''d''-dimensional Hausdorff outer measure of ''S'' as&lt;br /&gt;
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The Hausdorff outer measure is different from the unbounded Hausdorf content in that rather than considering all possible coverings of S, we see what happens when the sizes of the balls go to zero. This is  for &amp;lt;math&amp;gt;d \geq 0 &amp;lt;/math&amp;gt;, we define the d-dimensional Hausdorff outer measure of S as&lt;br /&gt;
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豪斯多夫外测度不同于无界的豪斯多夫，因为我们不考虑 s 的所有可能，我们看到当球的大小为零时会发生什么。这是为了数学  &amp;lt;math&amp;gt;d \geq 0 &amp;lt;/math&amp;gt;，我们定义了  ''S''的 ''d''维豪斯多夫Hausdorff 外测度为&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt; \mathcal{H}^d(S):=\lim_{r \to 0} \inf\Bigl\{\sum_i r_i^d:\text{ there is a cover of } S\text{ by balls with radii } 0 &amp;lt; r_i &amp;lt; r\Bigr\}.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \mathcal{H}^d(S):=\lim_{r \to 0} \inf\Bigl\{\sum_i r_i^d:\text{ there is a cover of } S\text{ by balls with radii } 0 &amp;lt; r_i &amp;lt; r\Bigr\}.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \mathcal{H}^d(S):=\lim_{r \to 0} \inf\Bigl\{\sum_i r_i^d:\text{有一个面} S\text{ 球 } 0 &amp;lt; r_i &amp;lt; r\Bigr\}.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
===Hausdorff dimension豪斯多夫维数===&lt;br /&gt;
&lt;br /&gt;
The '''Hausdorff dimension''' of ''X'' is defined by&lt;br /&gt;
&lt;br /&gt;
The Hausdorff dimension of X is defined by&lt;br /&gt;
&lt;br /&gt;
X 的豪斯多夫维数定义为&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt;\dim_{\operatorname{H}}(X):=\inf\{d\ge 0: \mathcal{H}^d(X)=0\}.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt;\dim_{\operatorname{H}}(X):=\inf\{d\ge 0: \mathcal{H}^d(X)=0\}.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Equivalently, dim&amp;lt;sub&amp;gt;H&amp;lt;/sub&amp;gt;(''X'') may be defined as the [[infimum]] of the set of ''d'' ∈ [0, ∞) such that the ''d''-dimensional [[Hausdorff measure]] of ''X'' is zero. This is the same as the supremum of the set of ''d''&amp;amp;nbsp;∈&amp;amp;nbsp;[0,&amp;amp;nbsp;∞) such that the ''d''-dimensional Hausdorff measure of ''X'' is infinite (except that when this latter set of numbers ''d'' is empty the Hausdorff dimension is zero).&lt;br /&gt;
&lt;br /&gt;
Equivalently, dim&amp;lt;sub&amp;gt;H&amp;lt;/sub&amp;gt;(X) may be defined as the infimum of the set of d ∈ [0, ∞) such that the d-dimensional Hausdorff measure of X is zero. This is the same as the supremum of the set of d&amp;amp;nbsp;∈&amp;amp;nbsp;[0,&amp;amp;nbsp;∞) such that the d-dimensional Hausdorff measure of X is infinite (except that when this latter set of numbers d is empty the Hausdorff dimension is zero).&lt;br /&gt;
&lt;br /&gt;
等价地，dim &amp;lt;sub&amp;gt;H&amp;lt;/sub&amp;gt;(''X'')可定义为 ''d'' ∈ [0, ∞) 集的下确界，使得''X'' 的''d''-维 [[豪斯多夫测度]] 为零。这与 ''d''&amp;amp;nbsp;∈&amp;amp;nbsp;[0,&amp;amp;nbsp;∞)的集合的上确界相同，因此''X''的 d 维豪斯多夫测度是无限的(除非后一个集合 ''d'' 是空的，豪斯多夫维数为零)。&lt;br /&gt;
&lt;br /&gt;
==Examples实例==&lt;br /&gt;
&lt;br /&gt;
[[Image:Sierpinski deep.svg|thumb|250px|Dimension of a further [[fractal]] example. The [[Sierpinski triangle]], an object with Hausdorff dimension of log(3)/log(2)≈1.58.&amp;lt;ref name=ClaytonSCTPLS96/&amp;gt;]]&lt;br /&gt;
&lt;br /&gt;
Dimension of a further [[fractal example. The Sierpinski triangle, an object with Hausdorff dimension of log(3)/log(2)≈1.58.]]&lt;br /&gt;
&lt;br /&gt;
[[Image:谢尔宾斯基三角形 deep.svg|thumb|250px|进一步的[[分形维数]]的例子，进一步的分形维数的例子是谢尔宾斯基三角形，它是一个豪斯多夫维数为log(3)/log(2)≈1.58.&amp;lt;ref name=ClaytonSCTPLS96/&amp;gt;的物体]]&lt;br /&gt;
&lt;br /&gt;
* [[Countable set]]s have Hausdorff dimension 0.&amp;lt;ref name=&amp;quot;schleicher&amp;quot;&amp;gt;{{cite journal |last1=Schleicher |first1=Dierk |title=Hausdorff Dimension, Its Properties, and Its Surprises |journal=The American Mathematical Monthly |date=June 2007 |volume=114 |issue=6 |pages=509–528 |doi=10.1080/00029890.2007.11920440 |language=en |issn=0002-9890|arxiv=math/0505099 }}&amp;lt;/ref&amp;gt;&lt;br /&gt;
*[[可数集]]拥有豪斯多夫维数0.&amp;lt;ref name=&amp;quot;schleicher&amp;quot;&amp;gt;{{cite journal |last1=Schleicher |first1=Dierk |title=豪斯多夫维数, Its Properties, and Its Surprises |journal=The American Mathematical Monthly美国数学期刊 |date=June 2007 |volume=114 |issue=6 |pages=509–528 |doi=10.1080/00029890.2007.11920440 |language=en |issn=0002-9890|arxiv=math/0505099 }}&amp;lt;/ref&amp;gt;&lt;br /&gt;
* The [[Euclidean space]] ℝ&amp;lt;sup&amp;gt;''n''&amp;lt;/sup&amp;gt; has Hausdorff dimension ''n'', and the circle '''S'''&amp;lt;sup&amp;gt;1&amp;lt;/sup&amp;gt; has Hausdorff dimension 1.&amp;lt;ref name=&amp;quot;schleicher&amp;quot; /&amp;gt;&lt;br /&gt;
*[[教育空间]] ℝ&amp;lt;sup&amp;gt;''n''&amp;lt;/sup&amp;gt; 有豪斯多夫维数 ''n''，循环'''S'''&amp;lt;sup&amp;gt;1&amp;lt;/sup&amp;gt; 拥有豪斯多夫维数1.&amp;lt;ref name=&amp;quot;schleicher&amp;quot; /&amp;gt;&lt;br /&gt;
* [[Fractal]]s often are spaces whose Hausdorff dimension strictly exceeds the [[topological dimension]].&amp;lt;ref name=&amp;quot;mandelbrot&amp;quot; /&amp;gt; For example, the [[Cantor set]], a zero-dimensional topological space, is a union of two copies of itself, each copy shrunk by a factor 1/3; hence, it can be shown that its Hausdorff dimension is ln(2)/ln(3)&amp;amp;nbsp;≈&amp;amp;nbsp;0.63.&amp;lt;ref&amp;gt;{{cite book | last=Falconer | first = Kenneth |title=Fractal Geometry: Mathematical Foundations and Applications | publisher=[[John Wiley and Sons]] | edition=2nd | year=2003}}&amp;lt;/ref&amp;gt; The [[Sierpinski triangle]] is a union of three copies of itself, each copy shrunk by a factor of&amp;amp;nbsp;1/2; this yields a Hausdorff dimension of ln(3)/ln(2)&amp;amp;nbsp;≈&amp;amp;nbsp;1.58.&amp;lt;ref name=CampbellAnnenberg15/&amp;gt; These Hausdorff dimensions are related to the &amp;quot;critical exponent&amp;quot; of the [[Master theorem (analysis of algorithms)|Master theorem]] for solving [[Recurrence relation|recurrence relations]] in the [[analysis of algorithms]].&lt;br /&gt;
*[[分形]]一般是那些豪斯多夫维数直接超过其拓扑维数的空间。例如[[康托尔集]]是一个o维拓扑空间，由两个自己复制而成，每一个复制品都是原来的三分之一，因此它的豪斯多夫维数是 ln(2)/ln(3)&amp;amp;nbsp;≈&amp;amp;nbsp;0.63。&amp;lt;ref&amp;gt;{{cite book | last=Falconer | first = Kenneth |title=Fractal Geometry: Mathematical Foundations and Applications | publisher=[[John Wiley and Sons]] | edition=2nd | year=2003}}&amp;lt;/ref&amp;gt;一个[[谢尔宾斯基三角]]是他自身三个复制的组合。每一个是原来的&amp;amp;nbsp;1/2，它的豪斯多夫维数ln(3)/ln(2)&amp;amp;nbsp;≈&amp;amp;nbsp;1.58。&amp;lt;ref name=CampbellAnnenberg15/&amp;gt;在递归算法中解决递归关系时，这些豪斯多夫维数与[[算法分析主定理]]的临界指标相联系。&lt;br /&gt;
* [[Space-filling curve]]s like the [[Peano curve]] have the same Hausdorff dimension as the space they fill.&lt;br /&gt;
*[[空间填充曲线]]拥有和他们填充空间同样的豪斯多夫维数，如[[皮亚诺曲线]]。&lt;br /&gt;
* The trajectory of [[Brownian motion]] in dimension 2 and above is conjectured to be Hausdorff dimension 2.&amp;lt;ref&amp;gt;{{cite book | last=Morters | first=Peres | title= Brownian Motion | publisher=[[Cambridge University Press]] | year=2010 }}&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
[[image:Great Britain Hausdorff.svg|thumb|250px|Estimating the Hausdorff dimension of the [[How Long Is the Coast of Britain? Statistical Self-Similarity and Fractional Dimension|coast of Great Britain]]]]&lt;br /&gt;
&lt;br /&gt;
coast of Great Britain]]&lt;br /&gt;
&lt;br /&gt;
[[大不列颠海岸&lt;br /&gt;
&lt;br /&gt;
* 刘易斯·弗赖伊·理查森[[Lewis Fry Richardson]] has performed detailed experiments to measure the approximate Hausdorff dimension for various coastlines. His results have varied from 1.02 for the coastline of [[South Africa]] to 1.25 for the west coast of [[Great Britain]].&amp;lt;ref name=&amp;quot;mandelbrot&amp;quot; /&amp;gt;&lt;br /&gt;
*刘易斯·弗赖伊·理查森（Lewis Fry Richardson）已经通过豪斯多夫维数去测量了很多海岸线。它的结果涵盖从1.02的南非海岸线到1.25的大英帝国西海岸模型。]]&lt;br /&gt;
&lt;br /&gt;
==Properties of Hausdorff dimension豪斯多夫维数特性==&lt;br /&gt;
&lt;br /&gt;
{{refimprove section|date=March 2015}}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
=== Hausdorff dimension and inductive dimension 豪斯多夫维数和归纳维数===&lt;br /&gt;
&lt;br /&gt;
Let ''X'' be an arbitrary [[Separable space|separable]] metric space. There is a [[topology|topological]] notion of [[inductive dimension]] for ''X'' which is defined recursively. It is always an integer (or +∞) and is denoted dim&amp;lt;sub&amp;gt;ind&amp;lt;/sub&amp;gt;(''X'').&lt;br /&gt;
&lt;br /&gt;
Let X be an arbitrary separable metric space. There is a topological notion of inductive dimension for X which is defined recursively. It is always an integer (or +∞) and is denoted dim&amp;lt;sub&amp;gt;ind&amp;lt;/sub&amp;gt;(X).&lt;br /&gt;
&lt;br /&gt;
设''X'' 是[[任意可分度量空间]]。对于''X'' 有一个递归定义的归纳维数拓扑概念。它总是一个整数(或 + ∞) ，并且表示dim&amp;lt;sub&amp;gt;ind&amp;lt;/sub&amp;gt;(''X'')。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
'''Theorem'''. Suppose ''X'' is non-empty. Then &lt;br /&gt;
&lt;br /&gt;
Theorem. Suppose X is non-empty. Then &lt;br /&gt;
&lt;br /&gt;
'''定理'''：假设''X'' 是非空的。那么&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt; \dim_{\mathrm{Haus}}(X) \geq \dim_{\operatorname{ind}}(X). &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \dim_{\mathrm{Haus}}(X) \geq \dim_{\operatorname{ind}}(X). &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Moreover,&lt;br /&gt;
&lt;br /&gt;
Moreover,&lt;br /&gt;
&lt;br /&gt;
此外,&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \inf_Y \dim_{\operatorname{Haus}}(Y) =\dim_{\operatorname{ind}}(X), &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \inf_Y \dim_{\operatorname{Haus}}(Y) =\dim_{\operatorname{ind}}(X), &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
where ''Y'' ranges over metric spaces [[homeomorphic]] to ''X''. In other words, ''X'' and ''Y'' have the same underlying set of points and the metric ''d''&amp;lt;sub&amp;gt;''Y''&amp;lt;/sub&amp;gt; of ''Y'' is topologically equivalent to ''d''&amp;lt;sub&amp;gt;''X''&amp;lt;/sub&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
where Y ranges over metric spaces homeomorphic to X. In other words, X and Y have the same underlying set of points and the metric d&amp;lt;sub&amp;gt;Y&amp;lt;/sub&amp;gt; of Y is topologically equivalent to d&amp;lt;sub&amp;gt;X&amp;lt;/sub&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
其中''Y''是度量空间同胚到 ''X''的范围。换句话说， ''X''和 ''Y''具有相同的基本点集，''Y''的度规''d''&amp;lt;sub&amp;gt;''Y''&amp;lt;/sub&amp;gt; 的子拓扑等价于''d''&amp;lt;sub&amp;gt;''X''&amp;lt;/sub&amp;gt;。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
These results were originally established by [[Edward Szpilrajn]] (1907–1976), e.g., see Hurewicz and Wallman, Chapter VII.{{full citation needed|date=March 2015}}&lt;br /&gt;
&lt;br /&gt;
These results were originally established by Edward Szpilrajn (1907–1976), e.g., see Hurewicz and Wallman, Chapter VII.&lt;br /&gt;
&lt;br /&gt;
这些结果最初是由 [[Edward Szpilrajn]] (1907–1976)建立的,  参见 Hurewicz and Wallman, Chapter VII.{{full citation needed|date=March 2015}}第七章。&lt;br /&gt;
&lt;br /&gt;
=== Hausdorff dimension and Minkowski dimension 豪斯多夫维数和闵可夫斯基维度===&lt;br /&gt;
&lt;br /&gt;
The [[Minkowski dimension]] is similar to, and at least as large as, the Hausdorff dimension, and they are equal in many situations. However, the set of [[rational number|rational]] points in [0, 1] has Hausdorff dimension zero and Minkowski dimension one. There are also compact sets for which the Minkowski dimension is strictly larger than the Hausdorff dimension.&lt;br /&gt;
&lt;br /&gt;
The Minkowski dimension is similar to, and at least as large as, the Hausdorff dimension, and they are equal in many situations. However, the set of rational points in [0, 1] has Hausdorff dimension zero and Minkowski dimension one. There are also compact sets for which the Minkowski dimension is strictly larger than the Hausdorff dimension.&lt;br /&gt;
&lt;br /&gt;
[[闵可夫斯基维数]]与豪斯多夫维数相似，至少和它一样大，而且在许多情况下是相等的。然而，[0,1]中有理点集的豪斯多夫维数为0，闵可夫斯基维数为1。还有一些紧集的闵可夫斯基维数绝对大于豪斯多夫维数。&lt;br /&gt;
&lt;br /&gt;
=== Hausdorff dimensions and Frostman measures 豪斯多夫维度和弗洛斯曼测度===&lt;br /&gt;
&lt;br /&gt;
If there is a [[measure (mathematics)|measure]] μ defined on [[Borel measure|Borel]] subsets of a metric space ''X'' such that ''μ''(''X'') &amp;gt; 0 and ''μ''(''B''(''x'', ''r'')) ≤ ''r&amp;lt;sup&amp;gt;s&amp;lt;/sup&amp;gt;'' holds for some constant ''s'' &amp;gt; 0 and for every ball ''B''(''x'', ''r'') in ''X'', then dim&amp;lt;sub&amp;gt;Haus&amp;lt;/sub&amp;gt;(''X'') ≥ ''s''. A partial converse is provided by [[Frostman's lemma]].{{citation needed|date=March 2015}}&amp;lt;ref&amp;gt;This Wikipedia article also discusses further useful characterizations of the Hausdorff dimension.{{clarify|date=March 2015}}&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
If there is a measure μ defined on Borel subsets of a metric space X such that μ(X) &amp;gt; 0 and μ(B(x, r)) ≤ r&amp;lt;sup&amp;gt;s&amp;lt;/sup&amp;gt; holds for some constant s &amp;gt; 0 and for every ball B(x, r) in X, then dim&amp;lt;sub&amp;gt;Haus&amp;lt;/sub&amp;gt;(X) ≥ s. A partial converse is provided by Frostman's lemma.&lt;br /&gt;
&lt;br /&gt;
如果在度量空间 ''X'' 的 Borel 子集上定义一个测度 μ，使得''μ''(''X'') &amp;gt; 0 和''μ''(''B''(''x'', ''r'')) ≤ ''r&amp;lt;sup&amp;gt;s&amp;lt;/sup&amp;gt;''，对于某个常数 ''s'' &amp;gt; 0  和 ''X'' 中的每个球 ''B''(''x'', ''r'') 成立，则 dim&amp;lt;sub&amp;gt;Haus&amp;lt;/sub&amp;gt;(''X'') ≥ ''s'' 。 部分逆向转换由弗洛斯曼引理定义。&lt;br /&gt;
&lt;br /&gt;
=== Behaviour under unions and products ===&lt;br /&gt;
&lt;br /&gt;
If &amp;lt;math&amp;gt;X=\bigcup_{i\in I}X_i&amp;lt;/math&amp;gt; is a finite or countable union, then&lt;br /&gt;
&lt;br /&gt;
If &amp;lt;math&amp;gt;X=\bigcup_{i\in I}X_i&amp;lt;/math&amp;gt; is a finite or countable union, then&lt;br /&gt;
&lt;br /&gt;
如果 &amp;lt;math&amp;gt;X=\bigcup_{i\in I}X_i&amp;lt;/math&amp;gt; 是一个有限或可数的联合，则&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \dim_{\operatorname{Haus}}(X) =\sup_{i\in I} \dim_{\operatorname{Haus}}(X_i).&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \dim_{\operatorname{Haus}}(X) =\sup_{i\in I} \dim_{\operatorname{Haus}}(X_i).&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
This can be verified directly from the definition.&lt;br /&gt;
&lt;br /&gt;
This can be verified directly from the definition.&lt;br /&gt;
&lt;br /&gt;
这可以直接从定义得到验证。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
If ''X'' and ''Y'' are non-empty metric spaces, then the Hausdorff dimension of their product satisfies&amp;lt;ref&amp;gt;{{cite journal |author=Marstrand, J. M. |title=The dimension of Cartesian product sets |journal=Proc. Cambridge Philos. Soc. |volume=50 |issue=3 |pages=198–202 |year=1954 |doi=10.1017/S0305004100029236 |bibcode = 1954PCPS...50..198M }}&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
If X and Y are non-empty metric spaces, then the Hausdorff dimension of their product satisfies&lt;br /&gt;
&lt;br /&gt;
如果 ''X'' 和''Y''是非空度量空间，那么它们乘积的豪斯多夫维数满足&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt; \dim_{\operatorname{Haus}}(X\times Y)\ge \dim_{\operatorname{Haus}}(X)+ \dim_{\operatorname{Haus}}(Y).&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \dim_{\operatorname{Haus}}(X\times Y)\ge \dim_{\operatorname{Haus}}(X)+ \dim_{\operatorname{Haus}}(Y).&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
This inequality can be strict. It is possible to find two sets of dimension 0 whose product has dimension 1.&amp;lt;ref&amp;gt;{{cite book  | last = Falconer  | first = Kenneth J.  | title = Fractal geometry. Mathematical foundations and applications  | publisher = John Wiley &amp;amp; Sons, Inc., Hoboken, New Jersey  | year = 2003  | doi =   | isbn = }}&amp;lt;/ref&amp;gt; In the opposite direction, it is known that when ''X'' and ''Y'' are Borel subsets of '''R'''&amp;lt;sup&amp;gt;''n''&amp;lt;/sup&amp;gt;, the Hausdorff dimension of ''X'' × ''Y'' is bounded from above by the Hausdorff dimension of ''X'' plus the [[packing dimension|upper packing dimension]] of ''Y''. These facts are discussed in Mattila (1995).&lt;br /&gt;
&lt;br /&gt;
This inequality can be strict. It is possible to find two sets of dimension 0 whose product has dimension 1. In the opposite direction, it is known that when X and Y are Borel subsets of R&amp;lt;sup&amp;gt;n&amp;lt;/sup&amp;gt;, the Hausdorff dimension of X × Y is bounded from above by the Hausdorff dimension of X plus the upper packing dimension of Y. These facts are discussed in Mattila (1995).&lt;br /&gt;
&lt;br /&gt;
这种不平等可以是绝对的。有可能找到两个维数为0的集合，其乘积的维数为1。相反，我们知道当''X''和''Y''是 '''R'''&amp;lt;sup&amp;gt;''n''&amp;lt;/sup&amp;gt;的 Borel 子集时， ''X'' × ''Y''的豪斯多夫维数从上面以 ''X''的豪斯多夫维数加上 ''Y''的填充维数为界。Mattila (1995)曾就这些情况进行了讨论。&lt;br /&gt;
&lt;br /&gt;
==Self-similar sets自相似集合==&lt;br /&gt;
&lt;br /&gt;
{{refimprove section|date=March 2015}}&lt;br /&gt;
&lt;br /&gt;
Many sets defined by a self-similarity condition have dimensions which can be determined explicitly. Roughly, a set ''E'' is self-similar if it is the fixed point of a set-valued transformation ψ, that is ψ(''E'') = ''E'', although the exact definition is given below.&lt;br /&gt;
&lt;br /&gt;
Many sets defined by a self-similarity condition have dimensions which can be determined explicitly. Roughly, a set E is self-similar if it is the fixed point of a set-valued transformation ψ, that is ψ(E) = E, although the exact definition is given below.&lt;br /&gt;
&lt;br /&gt;
许多由自相似条件定义的集合具有可以显式确定的维数。粗略地说，集合''E'' 是自相似的，如果它是集值ψ变换的不动点，即ψ(''E'') = ''E''，尽管下面给出了确切的定义。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&amp;lt;blockquote&amp;gt;'''Theorem'''. Suppose&lt;br /&gt;
&lt;br /&gt;
&amp;lt;blockquote&amp;gt;Theorem. Suppose&lt;br /&gt;
&lt;br /&gt;
&amp;lt;blockquote&amp;gt;'''定理'''：假设&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt; \psi_i: \mathbf{R}^n \rightarrow \mathbf{R}^n, \quad i=1, \ldots , m &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \psi_i: \mathbf{R}^n \rightarrow \mathbf{R}^n, \quad i=1, \ldots , m &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
are [[Contraction mapping|contractive]] mappings on '''R'''&amp;lt;sup&amp;gt;''n''&amp;lt;/sup&amp;gt; with contraction constant ''r&amp;lt;sub&amp;gt;j&amp;lt;/sub&amp;gt;'' &amp;lt; 1. Then there is a unique ''non-empty'' compact set ''A'' such that&lt;br /&gt;
&lt;br /&gt;
are contractive mappings on R&amp;lt;sup&amp;gt;n&amp;lt;/sup&amp;gt; with contraction constant r&amp;lt;sub&amp;gt;j&amp;lt;/sub&amp;gt; &amp;lt; 1. Then there is a unique non-empty compact set A such that&lt;br /&gt;
&lt;br /&gt;
是'''R'''&amp;lt;sup&amp;gt;''n''&amp;lt;/sup&amp;gt;上的压缩常数''r&amp;lt;sub&amp;gt;j&amp;lt;/sub&amp;gt;'&amp;lt; 1的压缩映射。然后有一个唯一的非空紧集A &lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt; A = \bigcup_{i=1}^m \psi_i (A). &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; A = \bigcup_{i=1}^m \psi_i (A). &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&amp;lt;/blockquote&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;/blockquote&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The theorem follows from [[Stefan Banach]]'s [[Contractive mapping theorem|contractive mapping fixed point theorem]] applied to the complete metric space of non-empty compact subsets of '''R'''&amp;lt;sup&amp;gt;''n''&amp;lt;/sup&amp;gt; with the [[Hausdorff distance]].&amp;lt;ref&amp;gt;{{cite book |author=Falconer, K. J. |title=The Geometry of Fractal Sets |publisher=Cambridge University Press |location=Cambridge, UK |year=1985 |isbn=0-521-25694-1 |chapter=Theorem 8.3}}&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
The theorem follows from Stefan Banach's contractive mapping fixed point theorem applied to the complete metric space of non-empty compact subsets of R&amp;lt;sup&amp;gt;n&amp;lt;/sup&amp;gt; with the Hausdorff distance.&lt;br /&gt;
&lt;br /&gt;
这个定理来源于 Stefan Banach 的压缩映射不动点定理，该定理应用于 '''R'''&amp;lt;sup&amp;gt;''n''&amp;lt;/sup&amp;gt; 的非空紧子集的完备空间豪斯多夫距离。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
===The open set condition开集条件===&lt;br /&gt;
&lt;br /&gt;
To determine the dimension of the self-similar set ''A'' (in certain cases), we need a technical condition called the ''open set condition'' (OSC) on the sequence of contractions ψ&amp;lt;sub&amp;gt;''i''&amp;lt;/sub&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
To determine the dimension of the self-similar set A (in certain cases), we need a technical condition called the open set condition (OSC) on the sequence of contractions ψ&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
为了确定自相似集''A'' 的维数(在某些情况下) ，我们需要一个称为''开集条件''(OSC)的技术条件ψ&amp;lt;sub&amp;gt;''i''&amp;lt;/sub&amp;gt;。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
There is a relatively compact open set ''V'' such that&lt;br /&gt;
&lt;br /&gt;
There is a relatively compact open set V such that&lt;br /&gt;
&lt;br /&gt;
有一个相对紧的开集''V''&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt; \bigcup_{i=1}^m\psi_i (V) \subseteq V, &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \bigcup_{i=1}^m\psi_i (V) \subseteq V, &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
where the sets in union on the left are pairwise [[disjoint sets|disjoint]].&lt;br /&gt;
&lt;br /&gt;
where the sets in union on the left are pairwise disjoint.&lt;br /&gt;
&lt;br /&gt;
左边的集合是成对不相交的。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The open set condition is a separation condition that ensures the images ψ&amp;lt;sub&amp;gt;''i''&amp;lt;/sub&amp;gt;(''V'') do not overlap &amp;quot;too much&amp;quot;.&lt;br /&gt;
&lt;br /&gt;
The open set condition is a separation condition that ensures the images ψ&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;(V) do not overlap &amp;quot;too much&amp;quot;.&lt;br /&gt;
&lt;br /&gt;
开集条件是保证图像子ψ&amp;lt;sub&amp;gt;''i''&amp;lt;/sub&amp;gt;(''V'') 不重叠“太多”的分离条件。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
'''Theorem'''. Suppose the open set condition holds and each ψ&amp;lt;sub&amp;gt;''i''&amp;lt;/sub&amp;gt; is a similitude, that is a composition of an [[isometry]] and a [[dilation (metric space)|dilation]] around some point. Then the unique fixed point of ψ is a set whose Hausdorff dimension is ''s'' where ''s'' is the unique solution of&amp;lt;ref&amp;gt;{{cite journal | last=Hutchinson | first=John E. | title=Fractals and self similarity | journal=Indiana Univ. Math. J. | volume=30 | year=1981 | pages=713–747 | doi=10.1512/iumj.1981.30.30055 | issue=5 | doi-access=free }}&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
Theorem. Suppose the open set condition holds and each ψ&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt; is a similitude, that is a composition of an isometry and a dilation around some point. Then the unique fixed point of ψ is a set whose Hausdorff dimension is s where s is the unique solution of&lt;br /&gt;
&lt;br /&gt;
'''定理'''假设开集条件成立，并且每个ψ&amp;lt;sub&amp;gt;''i''&amp;lt;/sub&amp;gt; 是一个相似度，即等距和某个点周围的膨胀的组合。。那么唯一的不动点是Hausdorff维数为 ''s'' 的集合，其中  ''s'' 是 ''s'' &amp;lt;ref&amp;gt;{{cite journal | last=Hutchinson | first=John E. | title=Fractals and self similarity | journal=Indiana Univ. Math. J. | volume=30 | year=1981 | pages=713–747 | doi=10.1512/iumj.1981.30.30055 | issue=5 | doi-access=free }}&amp;lt;/ref&amp;gt;的唯一解&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt; \sum_{i=1}^m r_i^s = 1. &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \sum_{i=1}^m r_i^s = 1. &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The contraction coefficient of a similitude is the magnitude of the dilation.&lt;br /&gt;
&lt;br /&gt;
The contraction coefficient of a similitude is the magnitude of the dilation.&lt;br /&gt;
&lt;br /&gt;
相似物的收缩系数就是膨胀的大小。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
We can use this theorem to compute the Hausdorff dimension of the Sierpinski triangle (or sometimes called Sierpinski gasket). Consider three [[non-collinear points]] ''a''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;, ''a''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;, ''a''&amp;lt;sub&amp;gt;3&amp;lt;/sub&amp;gt; in the plane '''R'''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; and let ψ&amp;lt;sub&amp;gt;''i''&amp;lt;/sub&amp;gt; be the dilation of ratio 1/2 around ''a&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;''. The unique non-empty fixed point of the corresponding mapping ψ is a Sierpinski gasket and the dimension ''s'' is the unique solution of&lt;br /&gt;
&lt;br /&gt;
We can use this theorem to compute the Hausdorff dimension of the Sierpinski triangle (or sometimes called Sierpinski gasket). Consider three non-collinear points a&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;, a&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;, a&amp;lt;sub&amp;gt;3&amp;lt;/sub&amp;gt; in the plane R&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; and let ψ&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt; be the dilation of ratio 1/2 around a&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;. The unique non-empty fixed point of the corresponding mapping ψ is a Sierpinski gasket and the dimension s is the unique solution of&lt;br /&gt;
&lt;br /&gt;
我们可以使用这个定理来计算谢尔宾斯基三角形的豪斯多夫维数(或者有时候叫做谢尔宾斯基垫圈)。考虑R&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; 平面上的三个非共线点，''a''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;，''a''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;，''a''&amp;lt;sub&amp;gt;3&amp;lt;/sub&amp;gt;，让ψ&amp;lt;sub&amp;gt;''i''&amp;lt;/sub&amp;gt;是围绕着''a&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;''比率1/2的膨胀。对应映射的唯一非空不动点是一个谢尔宾斯基垫圈，其维数''s''是对应映射的唯一解&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt; \left(\frac{1}{2}\right)^s+\left(\frac{1}{2}\right)^s+\left(\frac{1}{2}\right)^s = 3 \left(\frac{1}{2}\right)^s =1. &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \left(\frac{1}{2}\right)^s+\left(\frac{1}{2}\right)^s+\left(\frac{1}{2}\right)^s = 3 \left(\frac{1}{2}\right)^s =1. &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Taking [[natural logarithm]]s of both sides of the above equation, we can solve for ''s'', that is: ''s'' = ln(3)/ln(2).  The Sierpinski gasket is self-similar and satisfies the OSC. In general a set ''E'' which is a fixed point of a mapping&lt;br /&gt;
&lt;br /&gt;
Taking natural logarithms of both sides of the above equation, we can solve for s, that is: s = ln(3)/ln(2).  The Sierpinski gasket is self-similar and satisfies the OSC. In general a set E which is a fixed point of a mapping&lt;br /&gt;
&lt;br /&gt;
取上述方程两边的自然对数，我们可以求出 ''s''，即: ''s'' = ln(3)/ln(2)。该密封垫具有自相似性，满足 OSC 要求。一般来说，集合 ''E''是一个映射的不动点&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt; A \mapsto \psi(A) = \bigcup_{i=1}^m \psi_i(A) &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt; A \mapsto \psi(A) = \bigcup_{i=1}^m \psi_i(A) &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
is self-similar if and only if the intersections&lt;br /&gt;
&lt;br /&gt;
is self-similar if and only if the intersections&lt;br /&gt;
&lt;br /&gt;
是自相似的，当且仅当&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt; H^s\left(\psi_i(E) \cap \psi_j(E)\right) =0, &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; H^s\left(\psi_i(E) \cap \psi_j(E)\right) =0, &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
where ''s'' is the Hausdorff dimension of ''E'' and ''H&amp;lt;sup&amp;gt;s&amp;lt;/sup&amp;gt;'' denotes [[Hausdorff measure]]. This is clear in the case of the Sierpinski gasket (the intersections are just points), but is also true more generally:&lt;br /&gt;
&lt;br /&gt;
where s is the Hausdorff dimension of E and H&amp;lt;sup&amp;gt;s&amp;lt;/sup&amp;gt; denotes Hausdorff measure. This is clear in the case of the Sierpinski gasket (the intersections are just points), but is also true more generally:&lt;br /&gt;
&lt;br /&gt;
其中 ''s''是''E''的豪斯多夫维数， ''H&amp;lt;sup&amp;gt;s&amp;lt;/sup&amp;gt;'' 表示 豪斯多夫测度。对于谢尔宾斯基垫圈(交叉点就是点)来说，这一点很明显，但更普遍的情况是:&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
'''Theorem'''. Under the same conditions as the previous theorem, the unique fixed point of ψ is self-similar.&lt;br /&gt;
&lt;br /&gt;
Theorem. Under the same conditions as the previous theorem, the unique fixed point of ψ is self-similar.&lt;br /&gt;
&lt;br /&gt;
'''定理'''：在与前一定理相同的条件下，其唯一不动点是自相似的。&lt;br /&gt;
&lt;br /&gt;
==See also参阅==&lt;br /&gt;
&lt;br /&gt;
* [[List of fractals by Hausdorff dimension豪斯多夫分形维数列表]] Examples of deterministic fractals, random and natural fractals.确定性分形与随机和自然分形的示例。&lt;br /&gt;
&lt;br /&gt;
* [[Assouad dimension  Assouad维数]], another variation of fractal dimension that, like Hausdorff dimension, is defined using coverings by balls其他被球覆盖方式定义的分形维数，例如豪斯多夫维数。&lt;br /&gt;
&lt;br /&gt;
* [[Intrinsic dimension固有维数]]&lt;br /&gt;
&lt;br /&gt;
* [[Packing dimension填充维数]]&lt;br /&gt;
&lt;br /&gt;
* [[Fractal dimension分形维数]]&lt;br /&gt;
&lt;br /&gt;
==References参考文献==&lt;br /&gt;
&lt;br /&gt;
{{reflist}}&lt;br /&gt;
&lt;br /&gt;
==Further reading拓展阅读==&lt;br /&gt;
&lt;br /&gt;
* {{cite book |last1=Dodson |first1=M. Maurice |title=Fractal Geometry and Applications: A Jubilee of Benoît Mandelbrot |volume=72 |issue=1 |pages=305–347 |last2=Kristensen |first2=Simon |chapter=Hausdorff Dimension and Diophantine Approximation |date=June 12, 2003 |arxiv=math/0305399 |bibcode = 2003math......5399D |doi=10.1090/pspum/072.1/2112110|series=Proceedings of Symposia in Pure Mathematics |isbn=9780821836378 }}&lt;br /&gt;
&lt;br /&gt;
* {{cite book |last1=Hurewicz |first1=Witold |authorlink1=Witold Hurewicz |last2=Wallman |first2=Henry |authorlink2=Henry Wallman |title=Dimension Theory |url=https://archive.org/details/in.ernet.dli.2015.84609 |publisher=Princeton University Press |year=1948 }}&lt;br /&gt;
&lt;br /&gt;
* {{cite journal |author作者=E. Szpilrajn |authorlink=Edward Marczewski |title=La dimension et la mesure |journal=Fundamenta Mathematicae |volume=28 |pages=81–9 |year=1937 }}&lt;br /&gt;
&lt;br /&gt;
* {{cite journal&lt;br /&gt;
&lt;br /&gt;
 | last1=Marstrand&lt;br /&gt;
&lt;br /&gt;
 | last1=Marstrand&lt;br /&gt;
&lt;br /&gt;
 | last1=马斯特兰德&lt;br /&gt;
&lt;br /&gt;
 | first1=J. M. | title=The dimension of cartesian product sets | year=1954 | journal=Proc. Cambridge Philos. Soc.&lt;br /&gt;
&lt;br /&gt;
 | first1=J. M. | title=The dimension of cartesian product sets | year=1954 | journal=Proc. Cambridge Philos. Soc.&lt;br /&gt;
&lt;br /&gt;
 | first1= J. M. | title=笛卡儿积集的维数 | 1954年 |  journal=Proc. Cambridge Philos. Soc.&lt;br /&gt;
&lt;br /&gt;
 | volume=50&lt;br /&gt;
&lt;br /&gt;
 | volume=50&lt;br /&gt;
&lt;br /&gt;
 | 第50卷&lt;br /&gt;
&lt;br /&gt;
 | issue=3&lt;br /&gt;
&lt;br /&gt;
 | issue=3&lt;br /&gt;
&lt;br /&gt;
 | 第三期&lt;br /&gt;
&lt;br /&gt;
 | pages=198–202&lt;br /&gt;
&lt;br /&gt;
 | pages=198–202&lt;br /&gt;
&lt;br /&gt;
 | 第198-202页&lt;br /&gt;
&lt;br /&gt;
 | doi=10.1017/S0305004100029236|bibcode = 1954PCPS...50..198M }}&lt;br /&gt;
&lt;br /&gt;
 | doi=10.1017/S0305004100029236|bibcode = 1954PCPS...50..198M }}&lt;br /&gt;
&lt;br /&gt;
10.1017 / S0305004100029236 | bibcode 1954PCPS... 50. . 198 m }&lt;br /&gt;
&lt;br /&gt;
* {{Cite book&lt;br /&gt;
&lt;br /&gt;
 | last1=Mattila&lt;br /&gt;
&lt;br /&gt;
 | last1=Mattila&lt;br /&gt;
&lt;br /&gt;
 | last1=Mattila&lt;br /&gt;
&lt;br /&gt;
 | first1=Pertti | author1-link=Pertti Mattila| title=Geometry of sets and measures in Euclidean spaces | publisher=[[Cambridge University Press]]&lt;br /&gt;
&lt;br /&gt;
 | first1=Pertti | author1-link=Pertti Mattila| title=Geometry of sets and measures in Euclidean spaces | publisher=Cambridge University Press&lt;br /&gt;
&lt;br /&gt;
| first1 Pertti | author1-link Pertti Mattila | title 欧几里德空间中集合和度量的几何 | 出版商剑桥大学出版社&lt;br /&gt;
&lt;br /&gt;
 | isbn=978-0-521-65595-8 | year=1995}}&lt;br /&gt;
&lt;br /&gt;
 | isbn=978-0-521-65595-8 | year=1995}}&lt;br /&gt;
&lt;br /&gt;
| isbn 978-0-521-65595-8 | year 1995}&lt;br /&gt;
&lt;br /&gt;
* {{cite journal |author=A. S. Besicovitch |authorlink=A. S. Besicovitch |title=On Linear Sets of Points of Fractional Dimensions |journal=[[Mathematische Annalen]] |volume=101 |year=1929 | doi=10.1007/BF01454831| issue=1 |pages= 161–193}}&lt;br /&gt;
&lt;br /&gt;
* {{cite journal |author1=A. S. Besicovitch |authorlink1=A. S. Besicovitch |author2=H. D. Ursell |authorlink2=H. D. Ursell |title=Sets of Fractional Dimensions |journal=Journal of the London Mathematical Society |volume=12 |year=1937 | issue=1 | doi=10.1112/jlms/s1-12.45.18  | pages=18–25 }}&amp;lt;br/&amp;gt;Several selections from this volume are reprinted in {{cite book |author=Edgar, Gerald A. |title=Classics on fractals |publisher=Addison-Wesley |location=Boston |year=1993 |isbn=0-201-58701-7}} See chapters 9,10,11&lt;br /&gt;
&lt;br /&gt;
* {{cite journal |author=F. Hausdorff |authorlink=F. Hausdorff |title=Dimension und äußeres Maß |journal=Mathematische Annalen |volume=79 |issue=1–2 |pages=157–179 |date=March 1919 |doi=10.1007/BF01457179|hdl=10338.dmlcz/100363 |url=http://dml.cz/bitstream/handle/10338.dmlcz/100363/CzechMathJ_09-1959-3_5.pdf }}&lt;br /&gt;
&lt;br /&gt;
* {{cite journal | last=Hutchinson | first=John E. | title=Fractals and self similarity | journal=Indiana Univ. Math. J. | volume=30 | year=1981 | pages=713–747 | doi=10.1512/iumj.1981.30.30055 | issue=5 | doi-access=free }}&lt;br /&gt;
&lt;br /&gt;
*{{cite book | last=Falconer | first = Kenneth |title=Fractal Geometry: Mathematical Foundations and Applications | publisher=[[John Wiley and Sons]] | edition=2nd | year=2003}}&lt;br /&gt;
&lt;br /&gt;
==External links外部链接==&lt;br /&gt;
&lt;br /&gt;
* [https://www.encyclopediaofmath.org/index.php/Hausdorff_dimension Hausdorff dimension] 在 [https://www.encyclopediaofmath.org/ Encyclopedia of Mathematics]&lt;br /&gt;
&lt;br /&gt;
* [https://www.encyclopediaofmath.org/index.php/Hausdorff_measure Hausdorff measure] 在 [https://www.encyclopediaofmath.org/ Encyclopedia of Mathematics]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{{DEFAULTSORT:Hausdorff Dimension豪斯多夫维数}}&lt;br /&gt;
&lt;br /&gt;
[[Category分类:Fractals分形]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[Category分类:Metric geometry度量几何]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[Category分类:Dimension theory维度理论]]&lt;br /&gt;
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&lt;br /&gt;
&lt;br /&gt;
&amp;lt;noinclude&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;small&amp;gt;This page was moved from [[wikipedia:en:Hausdorff dimension]]. Its edit history can be viewed at [[分形维数/edithistory]]&amp;lt;/small&amp;gt;&amp;lt;/noinclude&amp;gt;&lt;br /&gt;
&lt;br /&gt;
[[Category:待整理页面]]&lt;/div&gt;</summary>
		<author><name>Ruili</name></author>
	</entry>
	<entry>
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		<title>分形维数</title>
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		<updated>2020-11-01T16:51:26Z</updated>

		<summary type="html">&lt;p&gt;Ruili：&lt;/p&gt;
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&lt;div&gt;此词条暂由彩云小译翻译，未经人工整理和审校，带来阅读不便，请见谅。&lt;br /&gt;
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Example of non-integer dimensions. The first four [[iteration]]s of the [[Koch snowflake|Koch curve]], where after each iteration, all original line segments are replaced with four, each a self-similar copy that is 1/3 the length of the original. One formalism of the Hausdorff dimension uses this scale factor (3) and the number of self-similar objects (4) to calculate the dimension, D, after the first iteration to be D = (log N)/(log S) = (log 4)/(log 3) ≈ 1.26.&amp;lt;ref name=CampbellAnnenberg15&amp;gt;MacGregor Campbell, 2013, &amp;quot;5.6 Scaling and the Hausdorff Dimension,&amp;quot; at ''Annenberg Learner:MATHematics illuminated'', see [http://www.learner.org/courses/mathilluminated/units/5/textbook/06.php], accessed 5 March 2015.&amp;lt;/ref&amp;gt; That is, while the Hausdorff dimension of a single [[point (geometry)|point]] is zero, of a [[line segment]] is 1, of a [[square]] is 2, and of a [[cube]] is 3, for [[fractal]]s such as this, the object can have a non-integer dimension.&lt;br /&gt;
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Example of non-integer dimensions. The first four iterations of the Koch curve, where after each iteration, all original line segments are replaced with four, each a self-similar copy that is 1/3 the length of the original. One formalism of the Hausdorff dimension uses this scale factor (3) and the number of self-similar objects (4) to calculate the dimension, D, after the first iteration to be D = (log N)/(log S) = (log 4)/(log 3) ≈ 1.26. That is, while the Hausdorff dimension of a single point is zero, of a line segment is 1, of a square is 2, and of a cube is 3, for fractals such as this, the object can have a non-integer dimension.&lt;br /&gt;
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非整数维度示例：前四个[[Koch 曲线]]的迭代，在每次迭代后，所有原始线段都被替换为四个，每个自相似的复制是原始线段长度的1 / 3。豪斯多夫维数的一个建模是使用比例因子(3)和自相似对象的数量(4)来计算维度 D，在第一次迭代后为 D = (log N)/(log S) = (log 4)/(log 3) ≈ 1.26.&amp;lt;ref name=CampbellAnnenberg15&amp;gt;。MacGregor Campbell, 2013, &amp;quot;5.6 Scaling and the Hausdorff Dimension,&amp;quot; 在 ''Annenberg Learner:MATHematics illuminated'', 参见 [http://www.learner.org/courses/mathilluminated/units/5/textbook/06.php], accessed 5 March 2015.&amp;lt;/ref&amp;gt; 也就是说，单点的豪斯多夫维数为零，线段为1，正方形为2，立方体为3时，但对于分形，对象可以有一个非整数维度。&lt;br /&gt;
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In [[mathematics]], '''Hausdorff dimension''' is a measure of ''roughness'', or more specifically, [[fractal dimension]], that was first introduced in 1918 by [[mathematician]] [[Felix Hausdorff]].&amp;lt;ref&amp;gt;{{Cite journal |arxiv = 1101.1444|doi = 10.1214/11-STS370|title = Estimators of Fractal Dimension: Assessing the Roughness of Time Series and Spatial Data|journal = Statistical Science|volume = 27|issue = 2|pages = 247–277|year = 2012|last1 = Gneiting|first1 = Tilmann|last2 = Ševčíková|first2 = Hana|last3 = Percival|first3 = Donald B.}}&amp;lt;/ref&amp;gt; For instance, the Hausdorff dimension of a single [[point (geometry)|point]] is zero, of a [[line segment]] is 1, of a [[square]] is 2, and of a [[cube]] is 3. That is, for sets of points that define a smooth shape or a shape that has a small number of corners—the shapes of traditional geometry and science—the Hausdorff dimension is an [[integer]] agreeing with the usual sense of dimension, also known as the [[Inductive dimension|topological dimension]]. However, formulas have also been developed that allow calculation of the dimension of other less simple objects, where, solely on the basis of their properties of [[scaling (geometry)|scaling]] and [[self-similarity]], one is led to the conclusion that particular objects—including [[fractal]]s—have non-integer Hausdorff dimensions. Because of the significant technical advances made by [[Abram Samoilovitch Besicovitch]] allowing computation of dimensions for highly irregular or &amp;quot;rough&amp;quot; sets, this dimension is also commonly referred to as the ''Hausdorff–Besicovitch dimension.''&lt;br /&gt;
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In mathematics, Hausdorff dimension is a measure of roughness, or more specifically, fractal dimension, that was first introduced in 1918 by mathematician Felix Hausdorff. For instance, the Hausdorff dimension of a single point is zero, of a line segment is 1, of a square is 2, and of a cube is 3. That is, for sets of points that define a smooth shape or a shape that has a small number of corners—the shapes of traditional geometry and science—the Hausdorff dimension is an integer agreeing with the usual sense of dimension, also known as the topological dimension. However, formulas have also been developed that allow calculation of the dimension of other less simple objects, where, solely on the basis of their properties of scaling and self-similarity, one is led to the conclusion that particular objects—including fractals—have non-integer Hausdorff dimensions. Because of the significant technical advances made by Abram Samoilovitch Besicovitch allowing computation of dimensions for highly irregular or &amp;quot;rough&amp;quot; sets, this dimension is also commonly referred to as the Hausdorff–Besicovitch dimension.&lt;br /&gt;
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在[[数学]]中，'''&amp;lt;font color = '#ff8000'&amp;gt;豪斯多夫维数Hausdorff dimension&amp;lt;/font&amp;gt;'''是一种粗糙度的度量单位，或者更确切地说，分形维数，是由数学家 Felix Hausdorff 在1918年首次提出的。例如，单点的豪斯多夫维数为零，线段为1，正方形为2，立方体为3。也就是说，对于定义了一个光滑形状或一个有少数几个角的形状---- 传统几何学和科学的形状---- 的点集来说，豪斯多夫维数是一个整数，符合通常的维度意义，也称为拓扑维度。然而，还有一些公式允许计算其他不太简单的对象的维数，其中仅仅根据它们的标度和自相似特性，就可以得出结论: 特定的对象ー包括分形ー具有非整数的 Hausdorff 维数。由于阿布拉姆·萨莫伊洛维奇·贝西科维奇的重大技术进步，允许计算高度不规则或“粗糙”集的维度，这个维度通常也被称为 Hausdorff-Besicovitch 维度。 &lt;br /&gt;
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The Hausdorff dimension, more specifically, is a further dimensional number associated with a given set, where the distances between all members of that set are defined. Such a set is termed a [[metric space]]. The dimension is drawn from the [[Extended real number line|extended real numbers]], &amp;lt;math&amp;gt;\overline{\mathbb{R}}&amp;lt;/math&amp;gt;, as opposed to the more intuitive notion of dimension, which is not associated to general metric spaces, and only takes values in the non-negative integers.&lt;br /&gt;
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The Hausdorff dimension, more specifically, is a further dimensional number associated with a given set, where the distances between all members of that set are defined. Such a set is termed a metric space. The dimension is drawn from the extended real numbers, &amp;lt;math&amp;gt;\overline{\mathbb{R}}&amp;lt;/math&amp;gt;, as opposed to the more intuitive notion of dimension, which is not associated to general metric spaces, and only takes values in the non-negative integers.&lt;br /&gt;
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更具体地说，豪斯多夫维数是一个与给定集合相关联的更进一步的维数，其中定义了该集合所有成员之间的距离。这样的集合称为度量空间。维数是从扩展的实数，&amp;lt;math&amp;gt;\overline{\mathbb{R}}&amp;lt;/math&amp;gt;，而不是更直观的维数概念(它不与一般的度量空间相关联，只取非负整数的值)。&lt;br /&gt;
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In mathematical terms, the Hausdorff dimension generalizes the notion of the dimension of a real [[vector space]]. That is, the Hausdorff dimension of an ''n''-dimensional [[inner product space]] equals ''n''. This underlies the earlier statement that the Hausdorff dimension of a point is zero, of a line is one, etc., and that [[fractal|irregular sets]] can have noninteger Hausdorff dimensions. For instance, the [[Koch snowflake]] shown at right is constructed from an equilateral triangle; in each iteration, its component line segments are divided into 3 segments of unit length, the newly created middle segment is used as the base of a new [[equilateral]] triangle that points outward, and this base segment is then deleted to leave a final object from the iteration of unit length of 4.&amp;lt;ref&amp;gt;Larry Riddle, 2014, &amp;quot;Classic Iterated Function Systems: Koch Snowflake&amp;quot;, Agnes Scott College e-Academy (online), see [http://ecademy.agnesscott.edu/~lriddle/ifs/ksnow/ksnow.htm], accessed 5 March 2015.&amp;lt;/ref&amp;gt; That is, after the first iteration, each original line segment has been replaced with N=4, where each self-similar copy is 1/S = 1/3 as long as the original.&amp;lt;ref name=CampbellAnnenberg15/&amp;gt; Stated another way, we have taken an object with Euclidean dimension, D, and reduced its linear scale by 1/3 in each direction, so that its length increases to N=S&amp;lt;sup&amp;gt;D&amp;lt;/sup&amp;gt;.&amp;lt;ref name=ClaytonSCTPLS96&amp;gt;Keith Clayton, 1996, &amp;quot;Fractals and the Fractal Dimension,&amp;quot; ''Basic Concepts in Nonlinear Dynamics and Chaos'' (workshop), Society for Chaos Theory in Psychology and the Life Sciences annual meeting, June 28, 1996, Berkeley, California, see [http://www.vanderbilt.edu/AnS/psychology/cogsci/chaos/workshop/Workshop.html], accessed 5 March 2015.&amp;lt;/ref&amp;gt; This equation is easily solved for D, yielding the ratio of logarithms (or [[natural logarithm]]s) appearing in the figures, and giving—in the Koch and other fractal cases—non-integer dimensions for these objects.&lt;br /&gt;
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In mathematical terms, the Hausdorff dimension generalizes the notion of the dimension of a real vector space. That is, the Hausdorff dimension of an n-dimensional inner product space equals n. This underlies the earlier statement that the Hausdorff dimension of a point is zero, of a line is one, etc., and that irregular sets can have noninteger Hausdorff dimensions. For instance, the Koch snowflake shown at right is constructed from an equilateral triangle; in each iteration, its component line segments are divided into 3 segments of unit length, the newly created middle segment is used as the base of a new equilateral triangle that points outward, and this base segment is then deleted to leave a final object from the iteration of unit length of 4. That is, after the first iteration, each original line segment has been replaced with N=4, where each self-similar copy is 1/S = 1/3 as long as the original. This equation is easily solved for D, yielding the ratio of logarithms (or natural logarithms) appearing in the figures, and giving—in the Koch and other fractal cases—non-integer dimensions for these objects.&lt;br /&gt;
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用数学术语来说，豪斯多夫维数概括了实向量空间维数的概念。也就是说，n 维内积空间的豪斯多夫维数等于 n。 这就是早期假设的基础，一个点的豪斯多夫维数是零，一条线是一等等，不规则集可以有非整数的豪斯多夫维数。例如，右边所示的 Koch 雪花是由一个正三角形构成的; 在每次迭代中，它的组成线段被分成单位长度的3段，新创建的中间线段被用作一个指向外部的新正三角形的基础，然后人们删除这个基础线段用来保留单位长度4的迭代中的最终对象。也就是说，在第一次迭代之后，每个原始线段都被替换为 N=4，其中每个自相似拷贝的长度是原始线段的1/S = 1/3 。这个方程很容易求解为 D，产生出现在图形中的对数(或自然对数)的比率，并给出——在 Koch 和其他分形情况下——这些对象的非整数维数。&lt;br /&gt;
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The Hausdorff dimension is a successor to the simpler, but usually equivalent, box-counting or [[Minkowski–Bouligand dimension]].&lt;br /&gt;
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The Hausdorff dimension is a successor to the simpler, but usually equivalent, box-counting or Minkowski–Bouligand dimension.&lt;br /&gt;
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豪斯多夫维数是更简单但通常等价的'''&amp;lt;font color = '#ff8000'&amp;gt;计盒维数box-counting&amp;lt;/font&amp;gt;'''或'''&amp;lt;font color = '#ff8000'&amp;gt;闵可夫斯基维数Minkowski-Bouligand&amp;lt;/font&amp;gt;'''的继承者。&lt;br /&gt;
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==Intuition概念==&lt;br /&gt;
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The intuitive concept of dimension of a geometric object ''X'' is the number of independent parameters one needs to pick out a unique point inside. However, any point specified by two parameters can be instead specified by one, because the [[cardinality]] of the [[real plane]] is equal to the cardinality of the [[real line]] (this can be seen by an [[Cantor's diagonal argument|argument]] involving interweaving the digits of two numbers to yield a single number encoding the same information). The example of a [[space-filling curve]] shows that one can even map the real line to the real plane [[Surjective function|surjectively]] (taking one real number into a pair of real numbers in a way so that all pairs of numbers are covered) and ''continuously'', so that a one-dimensional object completely fills up a higher-dimensional object.&lt;br /&gt;
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The intuitive concept of dimension of a geometric object X is the number of independent parameters one needs to pick out a unique point inside. However, any point specified by two parameters can be instead specified by one, because the cardinality of the real plane is equal to the cardinality of the real line (this can be seen by an argument involving interweaving the digits of two numbers to yield a single number encoding the same information). The example of a space-filling curve shows that one can even map the real line to the real plane surjectively (taking one real number into a pair of real numbers in a way so that all pairs of numbers are covered) and continuously, so that a one-dimensional object completely fills up a higher-dimensional object.&lt;br /&gt;
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几何对象X的尺寸的直观概念是指需要多少个独立参数才能找到一个独特的点。但是，任何由两个参数指定的点都可以由一个参数指定，因为为实平面的基数等于实线的基数(这可以通过交织两个数字以产生一个编码相同信息的单个数字看到)。'''&amp;lt;font color = '#ff8000'&amp;gt;皮亚诺曲线&amp;lt;/font&amp;gt;'''的例子表明，可以将实线完美和连续地映射到实平面(把一个实数转换成一对实数，从而覆盖所有实数对)，由此一维对象完全填充了一个高维对象。&lt;br /&gt;
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Every space filling curve hits some points multiple times, and does not have a continuous inverse. It is impossible to map two dimensions onto one in a way that is continuous and continuously invertible. The topological dimension, also called [[Lebesgue covering dimension]], explains why. This dimension is ''n'' if, in every covering of ''X'' by small open balls, there is at least one point where ''n''&amp;amp;nbsp;+&amp;amp;nbsp;1 balls overlap. For example, when one covers a line with short open intervals, some points must be covered twice, giving dimension&amp;amp;nbsp;''n''&amp;amp;nbsp;=&amp;amp;nbsp;1.&lt;br /&gt;
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Every space filling curve hits some points multiple times, and does not have a continuous inverse. It is impossible to map two dimensions onto one in a way that is continuous and continuously invertible. The topological dimension, also called Lebesgue covering dimension, explains why. This dimension is n if, in every covering of X by small open balls, there is at least one point where n&amp;amp;nbsp;+&amp;amp;nbsp;1 balls overlap. For example, when one covers a line with short open intervals, some points must be covered twice, giving dimension&amp;amp;nbsp;n&amp;amp;nbsp;=&amp;amp;nbsp;1.&lt;br /&gt;
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每条空间填充曲线都会多次击中某些点，且不存在连续的逆。将二维以连续和连续可逆的方式映射到一维是不可能的。'''&amp;lt;font color = '#ff8000'&amp;gt;拓扑维度 topological dimension&amp;lt;/font&amp;gt;'''，也被称为Lebesgue覆盖维数，解释了为什么。如果在 x 的每个小开球覆盖中，至少有一个点 n + 1个球重叠，这个维度是 n。例如，当用短的开区间覆盖一条线时，某些点必须被覆盖两次，给出维数''n''&amp;amp;nbsp;=&amp;amp;nbsp;1。&lt;br /&gt;
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But topological dimension is a very crude measure of the local size of a space (size near a point). A curve that is almost space-filling can still have topological dimension one, even if it fills up most of the area of a region. A [[fractal]] has an integer topological dimension, but in terms of the amount of space it takes up, it behaves like a higher-dimensional space.&lt;br /&gt;
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But topological dimension is a very crude measure of the local size of a space (size near a point). A curve that is almost space-filling can still have topological dimension one, even if it fills up most of the area of a region. A fractal has an integer topological dimension, but in terms of the amount of space it takes up, it behaves like a higher-dimensional space.&lt;br /&gt;
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但是，拓扑维度是对空间局部尺寸(点附近的尺寸)的一个非常粗略的度量。一条几乎是空间填充的曲线仍然可以有一维拓扑，即使它填充了一个区域的大部分面积。分形具有整数的拓扑维数，但就其所占的空间量而言，它看起来像一个更高维的空间。&lt;br /&gt;
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The Hausdorff dimension measures the local size of a space taking into account the distance between points, the [[metric space|metric]]. Consider the number ''N''(''r'') of [[ball (mathematics)|balls]] of radius at most ''r'' required to cover ''X'' completely. When ''r'' is very small, ''N''(''r'') grows polynomially with 1/''r''. For a sufficiently well-behaved  ''X'', the Hausdorff dimension is the unique number ''d'' such that N(''r'') grows as 1/''r&amp;lt;sup&amp;gt;d&amp;lt;/sup&amp;gt;'' as ''r'' approaches zero. More precisely, this defines the [[Minkowski–Bouligand dimension|box-counting dimension]], which equals the Hausdorff dimension when the value ''d'' is a critical boundary between growth rates that are insufficient to cover the space, and growth rates that are overabundant.&lt;br /&gt;
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The Hausdorff dimension measures the local size of a space taking into account the distance between points, the metric. Consider the number N(r) of balls of radius at most r required to cover X completely. When r is very small, N(r) grows polynomially with 1/r. For a sufficiently well-behaved  X, the Hausdorff dimension is the unique number d such that N(r) grows as 1/r&amp;lt;sup&amp;gt;d&amp;lt;/sup&amp;gt; as r approaches zero. More precisely, this defines the box-counting dimension, which equals the Hausdorff dimension when the value d is a critical boundary between growth rates that are insufficient to cover the space, and growth rates that are overabundant.&lt;br /&gt;
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豪斯多夫维数测量一个空间的局部大小时，会考虑到点之间距离的度量。考虑半径最大为 r 的球数 ''N'' (r) ，需要完全覆盖 ''X''。当 r 很小时，n (r)以1/''r'' 增长多项式。对于一个表现足够好的 ''X''，豪斯多夫维数是唯一的数 d，这样当 r 趋近于零时， N(r)增长为1/r&amp;lt;sup&amp;gt;d&amp;lt;/sup&amp;gt; 。更确切地说，这定义了盒子计数维度，当值 d 是不足以覆盖空间的增长率和过度充裕的增长率之间的关键边界时，它等于豪斯多夫维数。&lt;br /&gt;
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For shapes that are smooth, or shapes with a small number of corners, the shapes of traditional geometry and science, the Hausdorff dimension is an integer agreeing with the topological dimension. But [[Benoit Mandelbrot]] observed that [[fractal]]s, sets with noninteger Hausdorff dimensions, are found everywhere in nature. He observed that the proper idealization of most rough shapes you see around you is not in terms of smooth idealized shapes, but in terms of fractal idealized shapes:&lt;br /&gt;
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For shapes that are smooth, or shapes with a small number of corners, the shapes of traditional geometry and science, the Hausdorff dimension is an integer agreeing with the topological dimension. But Benoit Mandelbrot observed that fractals, sets with noninteger Hausdorff dimensions, are found everywhere in nature. He observed that the proper idealization of most rough shapes you see around you is not in terms of smooth idealized shapes, but in terms of fractal idealized shapes:&lt;br /&gt;
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对于光滑的形状，或者有少量棱角的形状，传统几何和科学的形状，豪斯多夫维数是一个整数，与拓扑维度一致。但是伯努·曼德布洛特观察到分形---- 具有非整数豪斯多夫维数的集合---- 在自然界中随处可见。他观察到，我们周围大多数粗糙形状的理想化不是光滑的理想化形状，而是分形理想化形状:&lt;br /&gt;
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&amp;lt;blockquote&amp;gt;Clouds are not spheres, mountains are not cones, coastlines are not circles, and bark is not smooth, nor does lightning travel in a straight line.&amp;lt;ref name=&amp;quot;mandelbrot&amp;quot;&amp;gt;{{cite book   | last = Mandelbrot   | first = Benoît   | authorlink = Benoit Mandelbrot   | title = The Fractal Geometry of Nature   | publisher = W. H. Freeman   | series = Lecture notes in mathematics 1358   | year = 1982   | doi =    | isbn = 0-7167-1186-9   | url-access = registration   | url = https://archive.org/details/fractalgeometryo00beno   }}&amp;lt;/ref&amp;gt;&amp;lt;/blockquote&amp;gt;&lt;br /&gt;
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&amp;lt;blockquote&amp;gt;Clouds are not spheres, mountains are not cones, coastlines are not circles, and bark is not smooth, nor does lightning travel in a straight line.&amp;lt;/blockquote&amp;gt;&lt;br /&gt;
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&amp;lt;blockquote&amp;gt;云不是球体，山不是锥体，海岸线不是圆圈，树皮不平滑，闪电也不是直线运动。 &amp;lt;/blockquote&amp;gt;&lt;br /&gt;
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For fractals that occur in nature, the Hausdorff and [[Minkowski–Bouligand dimension|box-counting dimension]] coincide. The [[packing dimension]] is yet another similar notion which gives the same value for many shapes, but there are well documented exceptions where all these dimensions differ.&lt;br /&gt;
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For fractals that occur in nature, the Hausdorff and box-counting dimension coincide. The packing dimension is yet another similar notion which gives the same value for many shapes, but there are well documented exceptions where all these dimensions differ.&lt;br /&gt;
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对于自然界中出现的分形，豪斯多夫维数和盒计数维数是一致的。封装尺寸是另一个类似的概念，它给出了许多形状相同的值，但是在所有这些尺寸不同的情况，都做了很好的说明。&lt;br /&gt;
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==Formal definitions形式化定义==&lt;br /&gt;
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===Hausdorff content豪斯多夫集===&lt;br /&gt;
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Let ''X'' be a [[metric space]]. If ''S'' ⊂ ''X'' and ''d'' ∈ [0, ∞), the ''d''-dimensional '''unlimited Hausdorff content''' of ''S'' is defined by&lt;br /&gt;
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Let X be a metric space. If S ⊂ X and d ∈ [0, ∞), the d-dimensional unlimited Hausdorff content of S is defined by&lt;br /&gt;
&lt;br /&gt;
设 ''X''是度量空间。若''S'' ⊂ ''X'' 和 ''d'' ∈ [0, ∞) ，则 ''S'' 的''d''维无限 豪斯多夫集定义为&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt;C_H^d(S):=\inf\Bigl\{\sum_i r_i^d:\text{ there is a cover of } S\text{ by balls with radii }r_i&amp;gt;0\Bigr\}.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt;C_H^d(S):=\inf\Bigl\{\sum_i r_i^d:\text{ there is a cover of } S\text{ by balls with radii }r_i&amp;gt;0\Bigr\}.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt;C_H^d(S):=\inf\Bigl\{\sum_i r_i^d:\text{ there is a cover of } S\text{ by balls with radii }r_i&amp;gt;0\Bigr\}.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
In other words, &amp;lt;math&amp;gt;C_H^d(S)&amp;lt;/math&amp;gt; is the [[infimum]] of the set of numbers &amp;lt;math&amp;gt;\delta \geq 0&amp;lt;/math&amp;gt; such that there is some (indexed) collection of [[ball (mathematics)|ball]]s &amp;lt;math&amp;gt;\{B(x_i,r_i):i\in I\}&amp;lt;/math&amp;gt; covering ''S'' with ''r&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;''&amp;amp;nbsp;&amp;gt;&amp;amp;nbsp;0 for each ''i''&amp;amp;nbsp;∈&amp;amp;nbsp;''I'' that satisfies &amp;lt;math&amp;gt;\sum_{i\in I} r_i^d&amp;lt;\delta &amp;lt;/math&amp;gt;. (Here, we use the standard convention that [[infimum|inf&amp;amp;nbsp;Ø&amp;amp;nbsp;=&amp;amp;nbsp;∞]].)&lt;br /&gt;
&lt;br /&gt;
In other words, &amp;lt;math&amp;gt;C_H^d(S)&amp;lt;/math&amp;gt; is the infimum of the set of numbers &amp;lt;math&amp;gt;\delta \geq 0&amp;lt;/math&amp;gt; such that there is some (indexed) collection of balls &amp;lt;math&amp;gt;\{B(x_i,r_i):i\in I\}&amp;lt;/math&amp;gt; covering S with r&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;&amp;amp;nbsp;&amp;gt;&amp;amp;nbsp;0 for each i&amp;amp;nbsp;∈&amp;amp;nbsp;I that satisfies &amp;lt;math&amp;gt;\sum_{i\in I} r_i^d&amp;lt;\delta &amp;lt;/math&amp;gt;. (Here, we use the standard convention that inf&amp;amp;nbsp;Ø&amp;amp;nbsp;=&amp;amp;nbsp;∞.)&lt;br /&gt;
&lt;br /&gt;
换句话说，&amp;lt;math&amp;gt;C_H^d(S)&amp;lt;/math&amp;gt; 是数字集合&amp;lt;math&amp;gt;\delta \geq 0&amp;lt;/math&amp;gt;的下确界，使得在 ''i''&amp;amp;nbsp;∈&amp;amp;nbsp中存在一些球集合 &amp;lt;math&amp;gt;\{B(x_i,r_i):i\in I\}&amp;lt;/math&amp;gt;  i 包含 s，对于每个 ''r&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;''&amp;amp;nbsp;&amp;gt;&amp;amp;nbsp;0 满足 i 中的和&amp;lt;math&amp;gt;\sum_{i\in I} r_i^d&amp;lt;\delta &amp;lt;/math&amp;gt; (在这里，我们使用inf&amp;amp;nbsp;Ø&amp;amp;nbsp;=&amp;amp;nbsp;∞ )的标准约定。&lt;br /&gt;
&lt;br /&gt;
===Hausdorff measurement豪斯多夫分形测量===&lt;br /&gt;
&lt;br /&gt;
The Hausdorff outer measure is different from the unbounded Hausdorf content in that rather than considering all possible coverings of ''S'', we see what happens when the sizes of the balls go to zero. This is  for &amp;lt;math&amp;gt;d \geq 0 &amp;lt;/math&amp;gt;, we define the ''d''-dimensional Hausdorff outer measure of ''S'' as&lt;br /&gt;
&lt;br /&gt;
The Hausdorff outer measure is different from the unbounded Hausdorf content in that rather than considering all possible coverings of S, we see what happens when the sizes of the balls go to zero. This is  for &amp;lt;math&amp;gt;d \geq 0 &amp;lt;/math&amp;gt;, we define the d-dimensional Hausdorff outer measure of S as&lt;br /&gt;
&lt;br /&gt;
豪斯多夫外测度不同于无界的豪斯多夫，因为我们不考虑 s 的所有可能，我们看到当球的大小为零时会发生什么。这是为了数学  &amp;lt;math&amp;gt;d \geq 0 &amp;lt;/math&amp;gt;，我们定义了  ''S''的 ''d''维豪斯多夫Hausdorff 外测度为&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt; \mathcal{H}^d(S):=\lim_{r \to 0} \inf\Bigl\{\sum_i r_i^d:\text{ there is a cover of } S\text{ by balls with radii } 0 &amp;lt; r_i &amp;lt; r\Bigr\}.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \mathcal{H}^d(S):=\lim_{r \to 0} \inf\Bigl\{\sum_i r_i^d:\text{ there is a cover of } S\text{ by balls with radii } 0 &amp;lt; r_i &amp;lt; r\Bigr\}.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \mathcal{H}^d(S):=\lim_{r \to 0} \inf\Bigl\{\sum_i r_i^d:\text{有一个面} S\text{ 球 } 0 &amp;lt; r_i &amp;lt; r\Bigr\}.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
===Hausdorff dimension豪斯多夫维数===&lt;br /&gt;
&lt;br /&gt;
The '''Hausdorff dimension''' of ''X'' is defined by&lt;br /&gt;
&lt;br /&gt;
The Hausdorff dimension of X is defined by&lt;br /&gt;
&lt;br /&gt;
X 的豪斯多夫维数定义为&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt;\dim_{\operatorname{H}}(X):=\inf\{d\ge 0: \mathcal{H}^d(X)=0\}.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt;\dim_{\operatorname{H}}(X):=\inf\{d\ge 0: \mathcal{H}^d(X)=0\}.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Equivalently, dim&amp;lt;sub&amp;gt;H&amp;lt;/sub&amp;gt;(''X'') may be defined as the [[infimum]] of the set of ''d'' ∈ [0, ∞) such that the ''d''-dimensional [[Hausdorff measure]] of ''X'' is zero. This is the same as the supremum of the set of ''d''&amp;amp;nbsp;∈&amp;amp;nbsp;[0,&amp;amp;nbsp;∞) such that the ''d''-dimensional Hausdorff measure of ''X'' is infinite (except that when this latter set of numbers ''d'' is empty the Hausdorff dimension is zero).&lt;br /&gt;
&lt;br /&gt;
Equivalently, dim&amp;lt;sub&amp;gt;H&amp;lt;/sub&amp;gt;(X) may be defined as the infimum of the set of d ∈ [0, ∞) such that the d-dimensional Hausdorff measure of X is zero. This is the same as the supremum of the set of d&amp;amp;nbsp;∈&amp;amp;nbsp;[0,&amp;amp;nbsp;∞) such that the d-dimensional Hausdorff measure of X is infinite (except that when this latter set of numbers d is empty the Hausdorff dimension is zero).&lt;br /&gt;
&lt;br /&gt;
等价地，dim &amp;lt;sub&amp;gt;H&amp;lt;/sub&amp;gt;(''X'')可定义为 ''d'' ∈ [0, ∞) 集的下确界，使得''X'' 的''d''-维 [[豪斯多夫测度]] 为零。这与 ''d''&amp;amp;nbsp;∈&amp;amp;nbsp;[0,&amp;amp;nbsp;∞)的集合的上确界相同，因此''X''的 d 维豪斯多夫测度是无限的(除非后一个集合 ''d'' 是空的，豪斯多夫维数为零)。&lt;br /&gt;
&lt;br /&gt;
==Examples实例==&lt;br /&gt;
&lt;br /&gt;
[[Image:Sierpinski deep.svg|thumb|250px|Dimension of a further [[fractal]] example. The [[Sierpinski triangle]], an object with Hausdorff dimension of log(3)/log(2)≈1.58.&amp;lt;ref name=ClaytonSCTPLS96/&amp;gt;]]&lt;br /&gt;
&lt;br /&gt;
Dimension of a further [[fractal example. The Sierpinski triangle, an object with Hausdorff dimension of log(3)/log(2)≈1.58.]]&lt;br /&gt;
&lt;br /&gt;
[[Image:谢尔宾斯基三角形 deep.svg|thumb|250px|进一步的[[分形维数]]的例子，进一步的分形维数的例子是谢尔宾斯基三角形，它是一个豪斯多夫维数为log(3)/log(2)≈1.58.&amp;lt;ref name=ClaytonSCTPLS96/&amp;gt;的物体]]&lt;br /&gt;
&lt;br /&gt;
* [[Countable set]]s have Hausdorff dimension 0.&amp;lt;ref name=&amp;quot;schleicher&amp;quot;&amp;gt;{{cite journal |last1=Schleicher |first1=Dierk |title=Hausdorff Dimension, Its Properties, and Its Surprises |journal=The American Mathematical Monthly |date=June 2007 |volume=114 |issue=6 |pages=509–528 |doi=10.1080/00029890.2007.11920440 |language=en |issn=0002-9890|arxiv=math/0505099 }}&amp;lt;/ref&amp;gt;&lt;br /&gt;
*[[可数集]]拥有豪斯多夫维数0.&amp;lt;ref name=&amp;quot;schleicher&amp;quot;&amp;gt;{{cite journal |last1=Schleicher |first1=Dierk |title=豪斯多夫维数, Its Properties, and Its Surprises |journal=The American Mathematical Monthly美国数学期刊 |date=June 2007 |volume=114 |issue=6 |pages=509–528 |doi=10.1080/00029890.2007.11920440 |language=en |issn=0002-9890|arxiv=math/0505099 }}&amp;lt;/ref&amp;gt;&lt;br /&gt;
* The [[Euclidean space]] ℝ&amp;lt;sup&amp;gt;''n''&amp;lt;/sup&amp;gt; has Hausdorff dimension ''n'', and the circle '''S'''&amp;lt;sup&amp;gt;1&amp;lt;/sup&amp;gt; has Hausdorff dimension 1.&amp;lt;ref name=&amp;quot;schleicher&amp;quot; /&amp;gt;&lt;br /&gt;
*[[教育空间]] ℝ&amp;lt;sup&amp;gt;''n''&amp;lt;/sup&amp;gt; 有豪斯多夫维数 ''n''，循环'''S'''&amp;lt;sup&amp;gt;1&amp;lt;/sup&amp;gt; 拥有豪斯多夫维数1.&amp;lt;ref name=&amp;quot;schleicher&amp;quot; /&amp;gt;&lt;br /&gt;
* [[Fractal]]s often are spaces whose Hausdorff dimension strictly exceeds the [[topological dimension]].&amp;lt;ref name=&amp;quot;mandelbrot&amp;quot; /&amp;gt; For example, the [[Cantor set]], a zero-dimensional topological space, is a union of two copies of itself, each copy shrunk by a factor 1/3; hence, it can be shown that its Hausdorff dimension is ln(2)/ln(3)&amp;amp;nbsp;≈&amp;amp;nbsp;0.63.&amp;lt;ref&amp;gt;{{cite book | last=Falconer | first = Kenneth |title=Fractal Geometry: Mathematical Foundations and Applications | publisher=[[John Wiley and Sons]] | edition=2nd | year=2003}}&amp;lt;/ref&amp;gt; The [[Sierpinski triangle]] is a union of three copies of itself, each copy shrunk by a factor of&amp;amp;nbsp;1/2; this yields a Hausdorff dimension of ln(3)/ln(2)&amp;amp;nbsp;≈&amp;amp;nbsp;1.58.&amp;lt;ref name=CampbellAnnenberg15/&amp;gt; These Hausdorff dimensions are related to the &amp;quot;critical exponent&amp;quot; of the [[Master theorem (analysis of algorithms)|Master theorem]] for solving [[Recurrence relation|recurrence relations]] in the [[analysis of algorithms]].&lt;br /&gt;
*[[分形]]一般是那些豪斯多夫维数直接超过其拓扑维数的空间。例如[[康托尔集]]是一个o维拓扑空间，由两个自己复制而成，每一个复制品都是原来的三分之一，因此它的豪斯多夫维数是 ln(2)/ln(3)&amp;amp;nbsp;≈&amp;amp;nbsp;0.63。&amp;lt;ref&amp;gt;{{cite book | last=Falconer | first = Kenneth |title=Fractal Geometry: Mathematical Foundations and Applications | publisher=[[John Wiley and Sons]] | edition=2nd | year=2003}}&amp;lt;/ref&amp;gt;一个[[谢尔宾斯基三角]]是他自身三个复制的组合。每一个是原来的&amp;amp;nbsp;1/2，它的豪斯多夫维数ln(3)/ln(2)&amp;amp;nbsp;≈&amp;amp;nbsp;1.58。&amp;lt;ref name=CampbellAnnenberg15/&amp;gt;在递归算法中解决递归关系时，这些豪斯多夫维数与[[算法分析主定理]]的临界指标相联系。&lt;br /&gt;
* [[Space-filling curve]]s like the [[Peano curve]] have the same Hausdorff dimension as the space they fill.&lt;br /&gt;
*[[空间填充曲线]]拥有和他们填充空间同样的豪斯多夫维数，如[[皮亚诺曲线]]。&lt;br /&gt;
* The trajectory of [[Brownian motion]] in dimension 2 and above is conjectured to be Hausdorff dimension 2.&amp;lt;ref&amp;gt;{{cite book | last=Morters | first=Peres | title= Brownian Motion | publisher=[[Cambridge University Press]] | year=2010 }}&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
[[image:Great Britain Hausdorff.svg|thumb|250px|Estimating the Hausdorff dimension of the [[How Long Is the Coast of Britain? Statistical Self-Similarity and Fractional Dimension|coast of Great Britain]]]]&lt;br /&gt;
&lt;br /&gt;
coast of Great Britain]]&lt;br /&gt;
&lt;br /&gt;
[[大不列颠海岸&lt;br /&gt;
&lt;br /&gt;
* 刘易斯·弗赖伊·理查森[[Lewis Fry Richardson]] has performed detailed experiments to measure the approximate Hausdorff dimension for various coastlines. His results have varied from 1.02 for the coastline of [[South Africa]] to 1.25 for the west coast of [[Great Britain]].&amp;lt;ref name=&amp;quot;mandelbrot&amp;quot; /&amp;gt;&lt;br /&gt;
*刘易斯·弗赖伊·理查森（Lewis Fry Richardson）已经通过豪斯多夫维数去测量了很多海岸线。它的结果涵盖从1.02的南非海岸线到1.25的大英帝国西海岸模型。]]&lt;br /&gt;
&lt;br /&gt;
==Properties of Hausdorff dimension豪斯多夫维数特性==&lt;br /&gt;
&lt;br /&gt;
{{refimprove section|date=March 2015}}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
=== Hausdorff dimension and inductive dimension 豪斯多夫维数和归纳维数===&lt;br /&gt;
&lt;br /&gt;
Let ''X'' be an arbitrary [[Separable space|separable]] metric space. There is a [[topology|topological]] notion of [[inductive dimension]] for ''X'' which is defined recursively. It is always an integer (or +∞) and is denoted dim&amp;lt;sub&amp;gt;ind&amp;lt;/sub&amp;gt;(''X'').&lt;br /&gt;
&lt;br /&gt;
Let X be an arbitrary separable metric space. There is a topological notion of inductive dimension for X which is defined recursively. It is always an integer (or +∞) and is denoted dim&amp;lt;sub&amp;gt;ind&amp;lt;/sub&amp;gt;(X).&lt;br /&gt;
&lt;br /&gt;
设''X'' 是[[任意可分度量空间]]。对于''X'' 有一个递归定义的归纳维数拓扑概念。它总是一个整数(或 + ∞) ，并且表示dim&amp;lt;sub&amp;gt;ind&amp;lt;/sub&amp;gt;(''X'')。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
'''Theorem'''. Suppose ''X'' is non-empty. Then &lt;br /&gt;
&lt;br /&gt;
Theorem. Suppose X is non-empty. Then &lt;br /&gt;
&lt;br /&gt;
'''定理'''：假设''X'' 是非空的。那么&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt; \dim_{\mathrm{Haus}}(X) \geq \dim_{\operatorname{ind}}(X). &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \dim_{\mathrm{Haus}}(X) \geq \dim_{\operatorname{ind}}(X). &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Moreover,&lt;br /&gt;
&lt;br /&gt;
Moreover,&lt;br /&gt;
&lt;br /&gt;
此外,&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \inf_Y \dim_{\operatorname{Haus}}(Y) =\dim_{\operatorname{ind}}(X), &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \inf_Y \dim_{\operatorname{Haus}}(Y) =\dim_{\operatorname{ind}}(X), &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
where ''Y'' ranges over metric spaces [[homeomorphic]] to ''X''. In other words, ''X'' and ''Y'' have the same underlying set of points and the metric ''d''&amp;lt;sub&amp;gt;''Y''&amp;lt;/sub&amp;gt; of ''Y'' is topologically equivalent to ''d''&amp;lt;sub&amp;gt;''X''&amp;lt;/sub&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
where Y ranges over metric spaces homeomorphic to X. In other words, X and Y have the same underlying set of points and the metric d&amp;lt;sub&amp;gt;Y&amp;lt;/sub&amp;gt; of Y is topologically equivalent to d&amp;lt;sub&amp;gt;X&amp;lt;/sub&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
其中''Y''是度量空间同胚到 ''X''的范围。换句话说， ''X''和 ''Y''具有相同的基本点集，''Y''的度规''d''&amp;lt;sub&amp;gt;''Y''&amp;lt;/sub&amp;gt; 的子拓扑等价于''d''&amp;lt;sub&amp;gt;''X''&amp;lt;/sub&amp;gt;。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
These results were originally established by [[Edward Szpilrajn]] (1907–1976), e.g., see Hurewicz and Wallman, Chapter VII.{{full citation needed|date=March 2015}}&lt;br /&gt;
&lt;br /&gt;
These results were originally established by Edward Szpilrajn (1907–1976), e.g., see Hurewicz and Wallman, Chapter VII.&lt;br /&gt;
&lt;br /&gt;
这些结果最初是由 [[Edward Szpilrajn]] (1907–1976)建立的,  参见 Hurewicz and Wallman, Chapter VII.{{full citation needed|date=March 2015}}第七章。&lt;br /&gt;
&lt;br /&gt;
=== Hausdorff dimension and Minkowski dimension 豪斯多夫维数和闵可夫斯基维度===&lt;br /&gt;
&lt;br /&gt;
The [[Minkowski dimension]] is similar to, and at least as large as, the Hausdorff dimension, and they are equal in many situations. However, the set of [[rational number|rational]] points in [0, 1] has Hausdorff dimension zero and Minkowski dimension one. There are also compact sets for which the Minkowski dimension is strictly larger than the Hausdorff dimension.&lt;br /&gt;
&lt;br /&gt;
The Minkowski dimension is similar to, and at least as large as, the Hausdorff dimension, and they are equal in many situations. However, the set of rational points in [0, 1] has Hausdorff dimension zero and Minkowski dimension one. There are also compact sets for which the Minkowski dimension is strictly larger than the Hausdorff dimension.&lt;br /&gt;
&lt;br /&gt;
[[闵可夫斯基维数]]与豪斯多夫维数相似，至少和它一样大，而且在许多情况下是相等的。然而，[0,1]中有理点集的豪斯多夫维数为0，闵可夫斯基维数为1。还有一些紧集的闵可夫斯基维数绝对大于豪斯多夫维数。&lt;br /&gt;
&lt;br /&gt;
=== Hausdorff dimensions and Frostman measures 豪斯多夫维度和弗洛斯曼测度===&lt;br /&gt;
&lt;br /&gt;
If there is a [[measure (mathematics)|measure]] μ defined on [[Borel measure|Borel]] subsets of a metric space ''X'' such that ''μ''(''X'') &amp;gt; 0 and ''μ''(''B''(''x'', ''r'')) ≤ ''r&amp;lt;sup&amp;gt;s&amp;lt;/sup&amp;gt;'' holds for some constant ''s'' &amp;gt; 0 and for every ball ''B''(''x'', ''r'') in ''X'', then dim&amp;lt;sub&amp;gt;Haus&amp;lt;/sub&amp;gt;(''X'') ≥ ''s''. A partial converse is provided by [[Frostman's lemma]].{{citation needed|date=March 2015}}&amp;lt;ref&amp;gt;This Wikipedia article also discusses further useful characterizations of the Hausdorff dimension.{{clarify|date=March 2015}}&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
If there is a measure μ defined on Borel subsets of a metric space X such that μ(X) &amp;gt; 0 and μ(B(x, r)) ≤ r&amp;lt;sup&amp;gt;s&amp;lt;/sup&amp;gt; holds for some constant s &amp;gt; 0 and for every ball B(x, r) in X, then dim&amp;lt;sub&amp;gt;Haus&amp;lt;/sub&amp;gt;(X) ≥ s. A partial converse is provided by Frostman's lemma.&lt;br /&gt;
&lt;br /&gt;
如果在度量空间 ''X'' 的 Borel 子集上定义一个测度 μ，使得''μ''(''X'') &amp;gt; 0 和''μ''(''B''(''x'', ''r'')) ≤ ''r&amp;lt;sup&amp;gt;s&amp;lt;/sup&amp;gt;''，对于某个常数 ''s'' &amp;gt; 0  和 ''X'' 中的每个球 ''B''(''x'', ''r'') 成立，则 dim&amp;lt;sub&amp;gt;Haus&amp;lt;/sub&amp;gt;(''X'') ≥ ''s'' 。 部分逆向转换由弗洛斯曼引理定义。&lt;br /&gt;
&lt;br /&gt;
=== Behaviour under unions and products ===&lt;br /&gt;
&lt;br /&gt;
If &amp;lt;math&amp;gt;X=\bigcup_{i\in I}X_i&amp;lt;/math&amp;gt; is a finite or countable union, then&lt;br /&gt;
&lt;br /&gt;
If &amp;lt;math&amp;gt;X=\bigcup_{i\in I}X_i&amp;lt;/math&amp;gt; is a finite or countable union, then&lt;br /&gt;
&lt;br /&gt;
如果 &amp;lt;math&amp;gt;X=\bigcup_{i\in I}X_i&amp;lt;/math&amp;gt; 是一个有限或可数的联合，则&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \dim_{\operatorname{Haus}}(X) =\sup_{i\in I} \dim_{\operatorname{Haus}}(X_i).&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \dim_{\operatorname{Haus}}(X) =\sup_{i\in I} \dim_{\operatorname{Haus}}(X_i).&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
This can be verified directly from the definition.&lt;br /&gt;
&lt;br /&gt;
This can be verified directly from the definition.&lt;br /&gt;
&lt;br /&gt;
这可以直接从定义得到验证。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
If ''X'' and ''Y'' are non-empty metric spaces, then the Hausdorff dimension of their product satisfies&amp;lt;ref&amp;gt;{{cite journal |author=Marstrand, J. M. |title=The dimension of Cartesian product sets |journal=Proc. Cambridge Philos. Soc. |volume=50 |issue=3 |pages=198–202 |year=1954 |doi=10.1017/S0305004100029236 |bibcode = 1954PCPS...50..198M }}&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
If X and Y are non-empty metric spaces, then the Hausdorff dimension of their product satisfies&lt;br /&gt;
&lt;br /&gt;
如果 ''X'' 和''Y''是非空度量空间，那么它们乘积的豪斯多夫维数满足&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt; \dim_{\operatorname{Haus}}(X\times Y)\ge \dim_{\operatorname{Haus}}(X)+ \dim_{\operatorname{Haus}}(Y).&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \dim_{\operatorname{Haus}}(X\times Y)\ge \dim_{\operatorname{Haus}}(X)+ \dim_{\operatorname{Haus}}(Y).&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
This inequality can be strict. It is possible to find two sets of dimension 0 whose product has dimension 1.&amp;lt;ref&amp;gt;{{cite book  | last = Falconer  | first = Kenneth J.  | title = Fractal geometry. Mathematical foundations and applications  | publisher = John Wiley &amp;amp; Sons, Inc., Hoboken, New Jersey  | year = 2003  | doi =   | isbn = }}&amp;lt;/ref&amp;gt; In the opposite direction, it is known that when ''X'' and ''Y'' are Borel subsets of '''R'''&amp;lt;sup&amp;gt;''n''&amp;lt;/sup&amp;gt;, the Hausdorff dimension of ''X'' × ''Y'' is bounded from above by the Hausdorff dimension of ''X'' plus the [[packing dimension|upper packing dimension]] of ''Y''. These facts are discussed in Mattila (1995).&lt;br /&gt;
&lt;br /&gt;
This inequality can be strict. It is possible to find two sets of dimension 0 whose product has dimension 1. In the opposite direction, it is known that when X and Y are Borel subsets of R&amp;lt;sup&amp;gt;n&amp;lt;/sup&amp;gt;, the Hausdorff dimension of X × Y is bounded from above by the Hausdorff dimension of X plus the upper packing dimension of Y. These facts are discussed in Mattila (1995).&lt;br /&gt;
&lt;br /&gt;
这种不平等可以是绝对的。有可能找到两个维数为0的集合，其乘积的维数为1。相反，我们知道当''X''和''Y''是 '''R'''&amp;lt;sup&amp;gt;''n''&amp;lt;/sup&amp;gt;的 Borel 子集时， ''X'' × ''Y''的豪斯多夫维数从上面以 ''X''的豪斯多夫维数加上 ''Y''的填充维数为界。Mattila (1995)曾就这些情况进行了讨论。&lt;br /&gt;
&lt;br /&gt;
==Self-similar sets自相似集合==&lt;br /&gt;
&lt;br /&gt;
{{refimprove section|date=March 2015}}&lt;br /&gt;
&lt;br /&gt;
Many sets defined by a self-similarity condition have dimensions which can be determined explicitly. Roughly, a set ''E'' is self-similar if it is the fixed point of a set-valued transformation ψ, that is ψ(''E'') = ''E'', although the exact definition is given below.&lt;br /&gt;
&lt;br /&gt;
Many sets defined by a self-similarity condition have dimensions which can be determined explicitly. Roughly, a set E is self-similar if it is the fixed point of a set-valued transformation ψ, that is ψ(E) = E, although the exact definition is given below.&lt;br /&gt;
&lt;br /&gt;
许多由自相似条件定义的集合具有可以显式确定的维数。粗略地说，集合''E'' 是自相似的，如果它是集值ψ变换的不动点，即ψ(''E'') = ''E''，尽管下面给出了确切的定义。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&amp;lt;blockquote&amp;gt;'''Theorem'''. Suppose&lt;br /&gt;
&lt;br /&gt;
&amp;lt;blockquote&amp;gt;Theorem. Suppose&lt;br /&gt;
&lt;br /&gt;
&amp;lt;blockquote&amp;gt;'''定理'''：假设&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt; \psi_i: \mathbf{R}^n \rightarrow \mathbf{R}^n, \quad i=1, \ldots , m &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \psi_i: \mathbf{R}^n \rightarrow \mathbf{R}^n, \quad i=1, \ldots , m &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
are [[Contraction mapping|contractive]] mappings on '''R'''&amp;lt;sup&amp;gt;''n''&amp;lt;/sup&amp;gt; with contraction constant ''r&amp;lt;sub&amp;gt;j&amp;lt;/sub&amp;gt;'' &amp;lt; 1. Then there is a unique ''non-empty'' compact set ''A'' such that&lt;br /&gt;
&lt;br /&gt;
are contractive mappings on R&amp;lt;sup&amp;gt;n&amp;lt;/sup&amp;gt; with contraction constant r&amp;lt;sub&amp;gt;j&amp;lt;/sub&amp;gt; &amp;lt; 1. Then there is a unique non-empty compact set A such that&lt;br /&gt;
&lt;br /&gt;
是'''R'''&amp;lt;sup&amp;gt;''n''&amp;lt;/sup&amp;gt;上的压缩常数''r&amp;lt;sub&amp;gt;j&amp;lt;/sub&amp;gt;'&amp;lt; 1的压缩映射。然后有一个唯一的非空紧集A &lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt; A = \bigcup_{i=1}^m \psi_i (A). &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; A = \bigcup_{i=1}^m \psi_i (A). &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&amp;lt;/blockquote&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;/blockquote&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The theorem follows from [[Stefan Banach]]'s [[Contractive mapping theorem|contractive mapping fixed point theorem]] applied to the complete metric space of non-empty compact subsets of '''R'''&amp;lt;sup&amp;gt;''n''&amp;lt;/sup&amp;gt; with the [[Hausdorff distance]].&amp;lt;ref&amp;gt;{{cite book |author=Falconer, K. J. |title=The Geometry of Fractal Sets |publisher=Cambridge University Press |location=Cambridge, UK |year=1985 |isbn=0-521-25694-1 |chapter=Theorem 8.3}}&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
The theorem follows from Stefan Banach's contractive mapping fixed point theorem applied to the complete metric space of non-empty compact subsets of R&amp;lt;sup&amp;gt;n&amp;lt;/sup&amp;gt; with the Hausdorff distance.&lt;br /&gt;
&lt;br /&gt;
这个定理来源于 Stefan Banach 的压缩映射不动点定理，该定理应用于 '''R'''&amp;lt;sup&amp;gt;''n''&amp;lt;/sup&amp;gt; 的非空紧子集的完备空间豪斯多夫距离。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
===The open set condition开集条件===&lt;br /&gt;
&lt;br /&gt;
To determine the dimension of the self-similar set ''A'' (in certain cases), we need a technical condition called the ''open set condition'' (OSC) on the sequence of contractions ψ&amp;lt;sub&amp;gt;''i''&amp;lt;/sub&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
To determine the dimension of the self-similar set A (in certain cases), we need a technical condition called the open set condition (OSC) on the sequence of contractions ψ&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
为了确定自相似集''A'' 的维数(在某些情况下) ，我们需要一个称为''开集条件''(OSC)的技术条件ψ&amp;lt;sub&amp;gt;''i''&amp;lt;/sub&amp;gt;。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
There is a relatively compact open set ''V'' such that&lt;br /&gt;
&lt;br /&gt;
There is a relatively compact open set V such that&lt;br /&gt;
&lt;br /&gt;
有一个相对紧的开集''V''&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt; \bigcup_{i=1}^m\psi_i (V) \subseteq V, &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \bigcup_{i=1}^m\psi_i (V) \subseteq V, &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
where the sets in union on the left are pairwise [[disjoint sets|disjoint]].&lt;br /&gt;
&lt;br /&gt;
where the sets in union on the left are pairwise disjoint.&lt;br /&gt;
&lt;br /&gt;
左边的集合是成对不相交的。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The open set condition is a separation condition that ensures the images ψ&amp;lt;sub&amp;gt;''i''&amp;lt;/sub&amp;gt;(''V'') do not overlap &amp;quot;too much&amp;quot;.&lt;br /&gt;
&lt;br /&gt;
The open set condition is a separation condition that ensures the images ψ&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;(V) do not overlap &amp;quot;too much&amp;quot;.&lt;br /&gt;
&lt;br /&gt;
开集条件是保证图像子ψ&amp;lt;sub&amp;gt;''i''&amp;lt;/sub&amp;gt;(''V'') 不重叠“太多”的分离条件。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
'''Theorem'''. Suppose the open set condition holds and each ψ&amp;lt;sub&amp;gt;''i''&amp;lt;/sub&amp;gt; is a similitude, that is a composition of an [[isometry]] and a [[dilation (metric space)|dilation]] around some point. Then the unique fixed point of ψ is a set whose Hausdorff dimension is ''s'' where ''s'' is the unique solution of&amp;lt;ref&amp;gt;{{cite journal | last=Hutchinson | first=John E. | title=Fractals and self similarity | journal=Indiana Univ. Math. J. | volume=30 | year=1981 | pages=713–747 | doi=10.1512/iumj.1981.30.30055 | issue=5 | doi-access=free }}&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
Theorem. Suppose the open set condition holds and each ψ&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt; is a similitude, that is a composition of an isometry and a dilation around some point. Then the unique fixed point of ψ is a set whose Hausdorff dimension is s where s is the unique solution of&lt;br /&gt;
&lt;br /&gt;
'''定理'''假设开集条件成立，并且每个ψ&amp;lt;sub&amp;gt;''i''&amp;lt;/sub&amp;gt; 是一个相似量，这是一个等距和围绕某一点的膨胀的合成。那么唯一的不动点是一个集合，它的豪斯多夫维数是 ''s'' ，其中  ''s'' 是 ''s'' &amp;lt;ref&amp;gt;{{cite journal | last=Hutchinson | first=John E. | title=Fractals and self similarity | journal=Indiana Univ. Math. J. | volume=30 | year=1981 | pages=713–747 | doi=10.1512/iumj.1981.30.30055 | issue=5 | doi-access=free }}&amp;lt;/ref&amp;gt;的唯一解&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt; \sum_{i=1}^m r_i^s = 1. &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \sum_{i=1}^m r_i^s = 1. &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The contraction coefficient of a similitude is the magnitude of the dilation.&lt;br /&gt;
&lt;br /&gt;
The contraction coefficient of a similitude is the magnitude of the dilation.&lt;br /&gt;
&lt;br /&gt;
相似物的收缩系数就是膨胀的大小。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
We can use this theorem to compute the Hausdorff dimension of the Sierpinski triangle (or sometimes called Sierpinski gasket). Consider three [[non-collinear points]] ''a''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;, ''a''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;, ''a''&amp;lt;sub&amp;gt;3&amp;lt;/sub&amp;gt; in the plane '''R'''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; and let ψ&amp;lt;sub&amp;gt;''i''&amp;lt;/sub&amp;gt; be the dilation of ratio 1/2 around ''a&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;''. The unique non-empty fixed point of the corresponding mapping ψ is a Sierpinski gasket and the dimension ''s'' is the unique solution of&lt;br /&gt;
&lt;br /&gt;
We can use this theorem to compute the Hausdorff dimension of the Sierpinski triangle (or sometimes called Sierpinski gasket). Consider three non-collinear points a&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;, a&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;, a&amp;lt;sub&amp;gt;3&amp;lt;/sub&amp;gt; in the plane R&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; and let ψ&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt; be the dilation of ratio 1/2 around a&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;. The unique non-empty fixed point of the corresponding mapping ψ is a Sierpinski gasket and the dimension s is the unique solution of&lt;br /&gt;
&lt;br /&gt;
我们可以使用这个定理来计算谢尔宾斯基三角形的豪斯多夫维数(或者有时候叫做谢尔宾斯基垫圈)。考虑R&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; 平面上的三个非共线点，''a''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;，''a''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;，''a''&amp;lt;sub&amp;gt;3&amp;lt;/sub&amp;gt;，让ψ&amp;lt;sub&amp;gt;''i''&amp;lt;/sub&amp;gt;是围绕着''a&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;''比率1/2的膨胀。对应映射的唯一非空不动点是一个谢尔宾斯基垫圈，其维数''s''是对应映射的唯一解&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt; \left(\frac{1}{2}\right)^s+\left(\frac{1}{2}\right)^s+\left(\frac{1}{2}\right)^s = 3 \left(\frac{1}{2}\right)^s =1. &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \left(\frac{1}{2}\right)^s+\left(\frac{1}{2}\right)^s+\left(\frac{1}{2}\right)^s = 3 \left(\frac{1}{2}\right)^s =1. &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Taking [[natural logarithm]]s of both sides of the above equation, we can solve for ''s'', that is: ''s'' = ln(3)/ln(2).  The Sierpinski gasket is self-similar and satisfies the OSC. In general a set ''E'' which is a fixed point of a mapping&lt;br /&gt;
&lt;br /&gt;
Taking natural logarithms of both sides of the above equation, we can solve for s, that is: s = ln(3)/ln(2).  The Sierpinski gasket is self-similar and satisfies the OSC. In general a set E which is a fixed point of a mapping&lt;br /&gt;
&lt;br /&gt;
取上述方程两边的自然对数，我们可以求出 ''s''，即: ''s'' = ln(3)/ln(2)。该密封垫具有自相似性，满足 OSC 要求。一般来说，集合 ''E''是一个映射的不动点&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt; A \mapsto \psi(A) = \bigcup_{i=1}^m \psi_i(A) &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt; A \mapsto \psi(A) = \bigcup_{i=1}^m \psi_i(A) &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
is self-similar if and only if the intersections&lt;br /&gt;
&lt;br /&gt;
is self-similar if and only if the intersections&lt;br /&gt;
&lt;br /&gt;
是自相似的，当且仅当&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt; H^s\left(\psi_i(E) \cap \psi_j(E)\right) =0, &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; H^s\left(\psi_i(E) \cap \psi_j(E)\right) =0, &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
where ''s'' is the Hausdorff dimension of ''E'' and ''H&amp;lt;sup&amp;gt;s&amp;lt;/sup&amp;gt;'' denotes [[Hausdorff measure]]. This is clear in the case of the Sierpinski gasket (the intersections are just points), but is also true more generally:&lt;br /&gt;
&lt;br /&gt;
where s is the Hausdorff dimension of E and H&amp;lt;sup&amp;gt;s&amp;lt;/sup&amp;gt; denotes Hausdorff measure. This is clear in the case of the Sierpinski gasket (the intersections are just points), but is also true more generally:&lt;br /&gt;
&lt;br /&gt;
其中 ''s''是''E''的豪斯多夫维数， ''H&amp;lt;sup&amp;gt;s&amp;lt;/sup&amp;gt;'' 表示 豪斯多夫测度。对于谢尔宾斯基垫圈(交叉点就是点)来说，这一点很明显，但更普遍的情况是:&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
'''Theorem'''. Under the same conditions as the previous theorem, the unique fixed point of ψ is self-similar.&lt;br /&gt;
&lt;br /&gt;
Theorem. Under the same conditions as the previous theorem, the unique fixed point of ψ is self-similar.&lt;br /&gt;
&lt;br /&gt;
'''定理'''：在与前一定理相同的条件下，其唯一不动点是自相似的。&lt;br /&gt;
&lt;br /&gt;
==See also参阅==&lt;br /&gt;
&lt;br /&gt;
* [[List of fractals by Hausdorff dimension豪斯多夫分形维数列表]] Examples of deterministic fractals, random and natural fractals.确定性分形与随机和自然分形的示例。&lt;br /&gt;
&lt;br /&gt;
* [[Assouad dimension  Assouad维数]], another variation of fractal dimension that, like Hausdorff dimension, is defined using coverings by balls其他被球覆盖方式定义的分形维数，例如豪斯多夫维数。&lt;br /&gt;
&lt;br /&gt;
* [[Intrinsic dimension固有维数]]&lt;br /&gt;
&lt;br /&gt;
* [[Packing dimension填充维数]]&lt;br /&gt;
&lt;br /&gt;
* [[Fractal dimension分形维数]]&lt;br /&gt;
&lt;br /&gt;
==References参考文献==&lt;br /&gt;
&lt;br /&gt;
{{reflist}}&lt;br /&gt;
&lt;br /&gt;
==Further reading拓展阅读==&lt;br /&gt;
&lt;br /&gt;
* {{cite book |last1=Dodson |first1=M. Maurice |title=Fractal Geometry and Applications: A Jubilee of Benoît Mandelbrot |volume=72 |issue=1 |pages=305–347 |last2=Kristensen |first2=Simon |chapter=Hausdorff Dimension and Diophantine Approximation |date=June 12, 2003 |arxiv=math/0305399 |bibcode = 2003math......5399D |doi=10.1090/pspum/072.1/2112110|series=Proceedings of Symposia in Pure Mathematics |isbn=9780821836378 }}&lt;br /&gt;
&lt;br /&gt;
* {{cite book |last1=Hurewicz |first1=Witold |authorlink1=Witold Hurewicz |last2=Wallman |first2=Henry |authorlink2=Henry Wallman |title=Dimension Theory |url=https://archive.org/details/in.ernet.dli.2015.84609 |publisher=Princeton University Press |year=1948 }}&lt;br /&gt;
&lt;br /&gt;
* {{cite journal |author作者=E. Szpilrajn |authorlink=Edward Marczewski |title=La dimension et la mesure |journal=Fundamenta Mathematicae |volume=28 |pages=81–9 |year=1937 }}&lt;br /&gt;
&lt;br /&gt;
* {{cite journal&lt;br /&gt;
&lt;br /&gt;
 | last1=Marstrand&lt;br /&gt;
&lt;br /&gt;
 | last1=Marstrand&lt;br /&gt;
&lt;br /&gt;
 | last1=马斯特兰德&lt;br /&gt;
&lt;br /&gt;
 | first1=J. M. | title=The dimension of cartesian product sets | year=1954 | journal=Proc. Cambridge Philos. Soc.&lt;br /&gt;
&lt;br /&gt;
 | first1=J. M. | title=The dimension of cartesian product sets | year=1954 | journal=Proc. Cambridge Philos. Soc.&lt;br /&gt;
&lt;br /&gt;
 | first1= J. M. | title=笛卡儿积集的维数 | 1954年 |  journal=Proc. Cambridge Philos. Soc.&lt;br /&gt;
&lt;br /&gt;
 | volume=50&lt;br /&gt;
&lt;br /&gt;
 | volume=50&lt;br /&gt;
&lt;br /&gt;
 | 第50卷&lt;br /&gt;
&lt;br /&gt;
 | issue=3&lt;br /&gt;
&lt;br /&gt;
 | issue=3&lt;br /&gt;
&lt;br /&gt;
 | 第三期&lt;br /&gt;
&lt;br /&gt;
 | pages=198–202&lt;br /&gt;
&lt;br /&gt;
 | pages=198–202&lt;br /&gt;
&lt;br /&gt;
 | 第198-202页&lt;br /&gt;
&lt;br /&gt;
 | doi=10.1017/S0305004100029236|bibcode = 1954PCPS...50..198M }}&lt;br /&gt;
&lt;br /&gt;
 | doi=10.1017/S0305004100029236|bibcode = 1954PCPS...50..198M }}&lt;br /&gt;
&lt;br /&gt;
10.1017 / S0305004100029236 | bibcode 1954PCPS... 50. . 198 m }&lt;br /&gt;
&lt;br /&gt;
* {{Cite book&lt;br /&gt;
&lt;br /&gt;
 | last1=Mattila&lt;br /&gt;
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 | last1=Mattila&lt;br /&gt;
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 | first1=Pertti | author1-link=Pertti Mattila| title=Geometry of sets and measures in Euclidean spaces | publisher=[[Cambridge University Press]]&lt;br /&gt;
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 | first1=Pertti | author1-link=Pertti Mattila| title=Geometry of sets and measures in Euclidean spaces | publisher=Cambridge University Press&lt;br /&gt;
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| first1 Pertti | author1-link Pertti Mattila | title 欧几里德空间中集合和度量的几何 | 出版商剑桥大学出版社&lt;br /&gt;
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 | isbn=978-0-521-65595-8 | year=1995}}&lt;br /&gt;
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 | isbn=978-0-521-65595-8 | year=1995}}&lt;br /&gt;
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| isbn 978-0-521-65595-8 | year 1995}&lt;br /&gt;
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* {{cite journal |author=A. S. Besicovitch |authorlink=A. S. Besicovitch |title=On Linear Sets of Points of Fractional Dimensions |journal=[[Mathematische Annalen]] |volume=101 |year=1929 | doi=10.1007/BF01454831| issue=1 |pages= 161–193}}&lt;br /&gt;
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* {{cite journal |author1=A. S. Besicovitch |authorlink1=A. S. Besicovitch |author2=H. D. Ursell |authorlink2=H. D. Ursell |title=Sets of Fractional Dimensions |journal=Journal of the London Mathematical Society |volume=12 |year=1937 | issue=1 | doi=10.1112/jlms/s1-12.45.18  | pages=18–25 }}&amp;lt;br/&amp;gt;Several selections from this volume are reprinted in {{cite book |author=Edgar, Gerald A. |title=Classics on fractals |publisher=Addison-Wesley |location=Boston |year=1993 |isbn=0-201-58701-7}} See chapters 9,10,11&lt;br /&gt;
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* {{cite journal |author=F. Hausdorff |authorlink=F. Hausdorff |title=Dimension und äußeres Maß |journal=Mathematische Annalen |volume=79 |issue=1–2 |pages=157–179 |date=March 1919 |doi=10.1007/BF01457179|hdl=10338.dmlcz/100363 |url=http://dml.cz/bitstream/handle/10338.dmlcz/100363/CzechMathJ_09-1959-3_5.pdf }}&lt;br /&gt;
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* {{cite journal | last=Hutchinson | first=John E. | title=Fractals and self similarity | journal=Indiana Univ. Math. J. | volume=30 | year=1981 | pages=713–747 | doi=10.1512/iumj.1981.30.30055 | issue=5 | doi-access=free }}&lt;br /&gt;
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*{{cite book | last=Falconer | first = Kenneth |title=Fractal Geometry: Mathematical Foundations and Applications | publisher=[[John Wiley and Sons]] | edition=2nd | year=2003}}&lt;br /&gt;
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==External links外部链接==&lt;br /&gt;
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* [https://www.encyclopediaofmath.org/index.php/Hausdorff_dimension Hausdorff dimension] 在 [https://www.encyclopediaofmath.org/ Encyclopedia of Mathematics]&lt;br /&gt;
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* [https://www.encyclopediaofmath.org/index.php/Hausdorff_measure Hausdorff measure] 在 [https://www.encyclopediaofmath.org/ Encyclopedia of Mathematics]&lt;br /&gt;
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{{DEFAULTSORT:Hausdorff Dimension豪斯多夫维数}}&lt;br /&gt;
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[[Category分类:Fractals分形]]&lt;br /&gt;
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[[Category分类:Metric geometry度量几何]]&lt;br /&gt;
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[[Category分类:Dimension theory维度理论]]&lt;br /&gt;
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&amp;lt;small&amp;gt;This page was moved from [[wikipedia:en:Hausdorff dimension]]. Its edit history can be viewed at [[分形维数/edithistory]]&amp;lt;/small&amp;gt;&amp;lt;/noinclude&amp;gt;&lt;br /&gt;
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[[Category:待整理页面]]&lt;/div&gt;</summary>
		<author><name>Ruili</name></author>
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		<title>分形维数</title>
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		<updated>2020-11-01T16:43:15Z</updated>

		<summary type="html">&lt;p&gt;Ruili：&lt;/p&gt;
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&lt;div&gt;此词条暂由彩云小译翻译，未经人工整理和审校，带来阅读不便，请见谅。&lt;br /&gt;
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Example of non-integer dimensions. The first four [[iteration]]s of the [[Koch snowflake|Koch curve]], where after each iteration, all original line segments are replaced with four, each a self-similar copy that is 1/3 the length of the original. One formalism of the Hausdorff dimension uses this scale factor (3) and the number of self-similar objects (4) to calculate the dimension, D, after the first iteration to be D = (log N)/(log S) = (log 4)/(log 3) ≈ 1.26.&amp;lt;ref name=CampbellAnnenberg15&amp;gt;MacGregor Campbell, 2013, &amp;quot;5.6 Scaling and the Hausdorff Dimension,&amp;quot; at ''Annenberg Learner:MATHematics illuminated'', see [http://www.learner.org/courses/mathilluminated/units/5/textbook/06.php], accessed 5 March 2015.&amp;lt;/ref&amp;gt; That is, while the Hausdorff dimension of a single [[point (geometry)|point]] is zero, of a [[line segment]] is 1, of a [[square]] is 2, and of a [[cube]] is 3, for [[fractal]]s such as this, the object can have a non-integer dimension.&lt;br /&gt;
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Example of non-integer dimensions. The first four iterations of the Koch curve, where after each iteration, all original line segments are replaced with four, each a self-similar copy that is 1/3 the length of the original. One formalism of the Hausdorff dimension uses this scale factor (3) and the number of self-similar objects (4) to calculate the dimension, D, after the first iteration to be D = (log N)/(log S) = (log 4)/(log 3) ≈ 1.26. That is, while the Hausdorff dimension of a single point is zero, of a line segment is 1, of a square is 2, and of a cube is 3, for fractals such as this, the object can have a non-integer dimension.&lt;br /&gt;
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非整数维度示例：前四个[[Koch 曲线]]的迭代，在每次迭代后，所有原始线段都被替换为四个，每个自相似的复制是原始线段长度的1 / 3。豪斯多夫维数的一个建模是使用比例因子(3)和自相似对象的数量(4)来计算维度 D，在第一次迭代后为 D = (log N)/(log S) = (log 4)/(log 3) ≈ 1.26.&amp;lt;ref name=CampbellAnnenberg15&amp;gt;。MacGregor Campbell, 2013, &amp;quot;5.6 Scaling and the Hausdorff Dimension,&amp;quot; 在 ''Annenberg Learner:MATHematics illuminated'', 参见 [http://www.learner.org/courses/mathilluminated/units/5/textbook/06.php], accessed 5 March 2015.&amp;lt;/ref&amp;gt; 也就是说，单点的豪斯多夫维数为零，线段为1，正方形为2，立方体为3时，但对于分形，对象可以有一个非整数维度。&lt;br /&gt;
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In [[mathematics]], '''Hausdorff dimension''' is a measure of ''roughness'', or more specifically, [[fractal dimension]], that was first introduced in 1918 by [[mathematician]] [[Felix Hausdorff]].&amp;lt;ref&amp;gt;{{Cite journal |arxiv = 1101.1444|doi = 10.1214/11-STS370|title = Estimators of Fractal Dimension: Assessing the Roughness of Time Series and Spatial Data|journal = Statistical Science|volume = 27|issue = 2|pages = 247–277|year = 2012|last1 = Gneiting|first1 = Tilmann|last2 = Ševčíková|first2 = Hana|last3 = Percival|first3 = Donald B.}}&amp;lt;/ref&amp;gt; For instance, the Hausdorff dimension of a single [[point (geometry)|point]] is zero, of a [[line segment]] is 1, of a [[square]] is 2, and of a [[cube]] is 3. That is, for sets of points that define a smooth shape or a shape that has a small number of corners—the shapes of traditional geometry and science—the Hausdorff dimension is an [[integer]] agreeing with the usual sense of dimension, also known as the [[Inductive dimension|topological dimension]]. However, formulas have also been developed that allow calculation of the dimension of other less simple objects, where, solely on the basis of their properties of [[scaling (geometry)|scaling]] and [[self-similarity]], one is led to the conclusion that particular objects—including [[fractal]]s—have non-integer Hausdorff dimensions. Because of the significant technical advances made by [[Abram Samoilovitch Besicovitch]] allowing computation of dimensions for highly irregular or &amp;quot;rough&amp;quot; sets, this dimension is also commonly referred to as the ''Hausdorff–Besicovitch dimension.''&lt;br /&gt;
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In mathematics, Hausdorff dimension is a measure of roughness, or more specifically, fractal dimension, that was first introduced in 1918 by mathematician Felix Hausdorff. For instance, the Hausdorff dimension of a single point is zero, of a line segment is 1, of a square is 2, and of a cube is 3. That is, for sets of points that define a smooth shape or a shape that has a small number of corners—the shapes of traditional geometry and science—the Hausdorff dimension is an integer agreeing with the usual sense of dimension, also known as the topological dimension. However, formulas have also been developed that allow calculation of the dimension of other less simple objects, where, solely on the basis of their properties of scaling and self-similarity, one is led to the conclusion that particular objects—including fractals—have non-integer Hausdorff dimensions. Because of the significant technical advances made by Abram Samoilovitch Besicovitch allowing computation of dimensions for highly irregular or &amp;quot;rough&amp;quot; sets, this dimension is also commonly referred to as the Hausdorff–Besicovitch dimension.&lt;br /&gt;
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在[[数学]]中，'''&amp;lt;font color = '#ff8000'&amp;gt;豪斯多夫维数Hausdorff dimension&amp;lt;/font&amp;gt;'''是一种粗糙度的度量单位，或者更确切地说，分形维数，是由数学家 Felix Hausdorff 在1918年首次提出的。例如，单点的豪斯多夫维数为零，线段为1，正方形为2，立方体为3。也就是说，对于定义了一个光滑形状或一个有少数几个角的形状---- 传统几何学和科学的形状---- 的点集来说，豪斯多夫维数是一个整数，符合通常的维度意义，也称为拓扑维度。然而，还有一些公式允许计算其他不太简单的对象的维数，其中仅仅根据它们的标度和自相似特性，就可以得出结论: 特定的对象ー包括分形ー具有非整数的 Hausdorff 维数。由于阿布拉姆·萨莫伊洛维奇·贝西科维奇的重大技术进步，允许计算高度不规则或“粗糙”集的维度，这个维度通常也被称为 Hausdorff-Besicovitch 维度。 &lt;br /&gt;
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The Hausdorff dimension, more specifically, is a further dimensional number associated with a given set, where the distances between all members of that set are defined. Such a set is termed a [[metric space]]. The dimension is drawn from the [[Extended real number line|extended real numbers]], &amp;lt;math&amp;gt;\overline{\mathbb{R}}&amp;lt;/math&amp;gt;, as opposed to the more intuitive notion of dimension, which is not associated to general metric spaces, and only takes values in the non-negative integers.&lt;br /&gt;
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The Hausdorff dimension, more specifically, is a further dimensional number associated with a given set, where the distances between all members of that set are defined. Such a set is termed a metric space. The dimension is drawn from the extended real numbers, &amp;lt;math&amp;gt;\overline{\mathbb{R}}&amp;lt;/math&amp;gt;, as opposed to the more intuitive notion of dimension, which is not associated to general metric spaces, and only takes values in the non-negative integers.&lt;br /&gt;
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更具体地说，豪斯多夫维数是一个与给定集合相关联的更进一步的维数，其中定义了该集合所有成员之间的距离。这样的集合称为度量空间。维数是从扩展的实数，&amp;lt;math&amp;gt;\overline{\mathbb{R}}&amp;lt;/math&amp;gt;，而不是更直观的维数概念(它不与一般的度量空间相关联，只取非负整数的值)。&lt;br /&gt;
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In mathematical terms, the Hausdorff dimension generalizes the notion of the dimension of a real [[vector space]]. That is, the Hausdorff dimension of an ''n''-dimensional [[inner product space]] equals ''n''. This underlies the earlier statement that the Hausdorff dimension of a point is zero, of a line is one, etc., and that [[fractal|irregular sets]] can have noninteger Hausdorff dimensions. For instance, the [[Koch snowflake]] shown at right is constructed from an equilateral triangle; in each iteration, its component line segments are divided into 3 segments of unit length, the newly created middle segment is used as the base of a new [[equilateral]] triangle that points outward, and this base segment is then deleted to leave a final object from the iteration of unit length of 4.&amp;lt;ref&amp;gt;Larry Riddle, 2014, &amp;quot;Classic Iterated Function Systems: Koch Snowflake&amp;quot;, Agnes Scott College e-Academy (online), see [http://ecademy.agnesscott.edu/~lriddle/ifs/ksnow/ksnow.htm], accessed 5 March 2015.&amp;lt;/ref&amp;gt; That is, after the first iteration, each original line segment has been replaced with N=4, where each self-similar copy is 1/S = 1/3 as long as the original.&amp;lt;ref name=CampbellAnnenberg15/&amp;gt; Stated another way, we have taken an object with Euclidean dimension, D, and reduced its linear scale by 1/3 in each direction, so that its length increases to N=S&amp;lt;sup&amp;gt;D&amp;lt;/sup&amp;gt;.&amp;lt;ref name=ClaytonSCTPLS96&amp;gt;Keith Clayton, 1996, &amp;quot;Fractals and the Fractal Dimension,&amp;quot; ''Basic Concepts in Nonlinear Dynamics and Chaos'' (workshop), Society for Chaos Theory in Psychology and the Life Sciences annual meeting, June 28, 1996, Berkeley, California, see [http://www.vanderbilt.edu/AnS/psychology/cogsci/chaos/workshop/Workshop.html], accessed 5 March 2015.&amp;lt;/ref&amp;gt; This equation is easily solved for D, yielding the ratio of logarithms (or [[natural logarithm]]s) appearing in the figures, and giving—in the Koch and other fractal cases—non-integer dimensions for these objects.&lt;br /&gt;
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In mathematical terms, the Hausdorff dimension generalizes the notion of the dimension of a real vector space. That is, the Hausdorff dimension of an n-dimensional inner product space equals n. This underlies the earlier statement that the Hausdorff dimension of a point is zero, of a line is one, etc., and that irregular sets can have noninteger Hausdorff dimensions. For instance, the Koch snowflake shown at right is constructed from an equilateral triangle; in each iteration, its component line segments are divided into 3 segments of unit length, the newly created middle segment is used as the base of a new equilateral triangle that points outward, and this base segment is then deleted to leave a final object from the iteration of unit length of 4. That is, after the first iteration, each original line segment has been replaced with N=4, where each self-similar copy is 1/S = 1/3 as long as the original. This equation is easily solved for D, yielding the ratio of logarithms (or natural logarithms) appearing in the figures, and giving—in the Koch and other fractal cases—non-integer dimensions for these objects.&lt;br /&gt;
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用数学术语来说，豪斯多夫维数概括了实向量空间维数的概念。也就是说，n 维内积空间的豪斯多夫维数等于 n。 这就是早期假设的基础，一个点的豪斯多夫维数是零，一条线是一等等，不规则集可以有非整数的豪斯多夫维数。例如，右边所示的 Koch 雪花是由一个正三角形构成的; 在每次迭代中，它的组成线段被分成单位长度的3段，新创建的中间线段被用作一个指向外部的新正三角形的基础，然后人们删除这个基础线段用来保留单位长度4的迭代中的最终对象。也就是说，在第一次迭代之后，每个原始线段都被替换为 N=4，其中每个自相似拷贝的长度是原始线段的1/S = 1/3 。这个方程很容易求解为 D，产生出现在图形中的对数(或自然对数)的比率，并给出——在 Koch 和其他分形情况下——这些对象的非整数维数。&lt;br /&gt;
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The Hausdorff dimension is a successor to the simpler, but usually equivalent, box-counting or [[Minkowski–Bouligand dimension]].&lt;br /&gt;
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The Hausdorff dimension is a successor to the simpler, but usually equivalent, box-counting or Minkowski–Bouligand dimension.&lt;br /&gt;
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豪斯多夫维数是更简单但通常等价的'''&amp;lt;font color = '#ff8000'&amp;gt;计盒维数box-counting&amp;lt;/font&amp;gt;'''或'''&amp;lt;font color = '#ff8000'&amp;gt;闵可夫斯基维数Minkowski-Bouligand&amp;lt;/font&amp;gt;'''的继承者。&lt;br /&gt;
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==Intuition概念==&lt;br /&gt;
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The intuitive concept of dimension of a geometric object ''X'' is the number of independent parameters one needs to pick out a unique point inside. However, any point specified by two parameters can be instead specified by one, because the [[cardinality]] of the [[real plane]] is equal to the cardinality of the [[real line]] (this can be seen by an [[Cantor's diagonal argument|argument]] involving interweaving the digits of two numbers to yield a single number encoding the same information). The example of a [[space-filling curve]] shows that one can even map the real line to the real plane [[Surjective function|surjectively]] (taking one real number into a pair of real numbers in a way so that all pairs of numbers are covered) and ''continuously'', so that a one-dimensional object completely fills up a higher-dimensional object.&lt;br /&gt;
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The intuitive concept of dimension of a geometric object X is the number of independent parameters one needs to pick out a unique point inside. However, any point specified by two parameters can be instead specified by one, because the cardinality of the real plane is equal to the cardinality of the real line (this can be seen by an argument involving interweaving the digits of two numbers to yield a single number encoding the same information). The example of a space-filling curve shows that one can even map the real line to the real plane surjectively (taking one real number into a pair of real numbers in a way so that all pairs of numbers are covered) and continuously, so that a one-dimensional object completely fills up a higher-dimensional object.&lt;br /&gt;
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几何对象X的尺寸的直观概念是指需要多少个独立参数才能找到一个独特的点。但是，任何由两个参数指定的点都可以由一个参数指定，因为为实平面的基数等于实线的基数(这可以通过交织两个数字以产生一个编码相同信息的单个数字看到)。'''&amp;lt;font color = '#ff8000'&amp;gt;皮亚诺曲线&amp;lt;/font&amp;gt;'''的例子表明，可以将实线完美和连续地映射到实平面(把一个实数转换成一对实数，从而覆盖所有实数对)，由此一维对象完全填充了一个高维对象。&lt;br /&gt;
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Every space filling curve hits some points multiple times, and does not have a continuous inverse. It is impossible to map two dimensions onto one in a way that is continuous and continuously invertible. The topological dimension, also called [[Lebesgue covering dimension]], explains why. This dimension is ''n'' if, in every covering of ''X'' by small open balls, there is at least one point where ''n''&amp;amp;nbsp;+&amp;amp;nbsp;1 balls overlap. For example, when one covers a line with short open intervals, some points must be covered twice, giving dimension&amp;amp;nbsp;''n''&amp;amp;nbsp;=&amp;amp;nbsp;1.&lt;br /&gt;
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Every space filling curve hits some points multiple times, and does not have a continuous inverse. It is impossible to map two dimensions onto one in a way that is continuous and continuously invertible. The topological dimension, also called Lebesgue covering dimension, explains why. This dimension is n if, in every covering of X by small open balls, there is at least one point where n&amp;amp;nbsp;+&amp;amp;nbsp;1 balls overlap. For example, when one covers a line with short open intervals, some points must be covered twice, giving dimension&amp;amp;nbsp;n&amp;amp;nbsp;=&amp;amp;nbsp;1.&lt;br /&gt;
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每条空间填充曲线都会多次击中某些点，且不存在连续的逆。将二维以连续和连续可逆的方式映射到一维是不可能的。'''&amp;lt;font color = '#ff8000'&amp;gt;拓扑维度 topological dimension&amp;lt;/font&amp;gt;'''，也被称为Lebesgue覆盖维数，解释了为什么。如果在 x 的每个小开球覆盖中，至少有一个点 n + 1个球重叠，这个维度是 n。例如，当用短的开区间覆盖一条线时，某些点必须被覆盖两次，给出维数''n''&amp;amp;nbsp;=&amp;amp;nbsp;1。&lt;br /&gt;
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But topological dimension is a very crude measure of the local size of a space (size near a point). A curve that is almost space-filling can still have topological dimension one, even if it fills up most of the area of a region. A [[fractal]] has an integer topological dimension, but in terms of the amount of space it takes up, it behaves like a higher-dimensional space.&lt;br /&gt;
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But topological dimension is a very crude measure of the local size of a space (size near a point). A curve that is almost space-filling can still have topological dimension one, even if it fills up most of the area of a region. A fractal has an integer topological dimension, but in terms of the amount of space it takes up, it behaves like a higher-dimensional space.&lt;br /&gt;
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但是，拓扑维度是对空间局部尺寸(点附近的尺寸)的一个非常粗略的度量。一条几乎是空间填充的曲线仍然可以有一维拓扑，即使它填充了一个区域的大部分面积。分形具有整数的拓扑维数，但就其所占的空间量而言，它看起来像一个更高维的空间。&lt;br /&gt;
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The Hausdorff dimension measures the local size of a space taking into account the distance between points, the [[metric space|metric]]. Consider the number ''N''(''r'') of [[ball (mathematics)|balls]] of radius at most ''r'' required to cover ''X'' completely. When ''r'' is very small, ''N''(''r'') grows polynomially with 1/''r''. For a sufficiently well-behaved  ''X'', the Hausdorff dimension is the unique number ''d'' such that N(''r'') grows as 1/''r&amp;lt;sup&amp;gt;d&amp;lt;/sup&amp;gt;'' as ''r'' approaches zero. More precisely, this defines the [[Minkowski–Bouligand dimension|box-counting dimension]], which equals the Hausdorff dimension when the value ''d'' is a critical boundary between growth rates that are insufficient to cover the space, and growth rates that are overabundant.&lt;br /&gt;
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The Hausdorff dimension measures the local size of a space taking into account the distance between points, the metric. Consider the number N(r) of balls of radius at most r required to cover X completely. When r is very small, N(r) grows polynomially with 1/r. For a sufficiently well-behaved  X, the Hausdorff dimension is the unique number d such that N(r) grows as 1/r&amp;lt;sup&amp;gt;d&amp;lt;/sup&amp;gt; as r approaches zero. More precisely, this defines the box-counting dimension, which equals the Hausdorff dimension when the value d is a critical boundary between growth rates that are insufficient to cover the space, and growth rates that are overabundant.&lt;br /&gt;
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豪斯多夫维数测量一个空间的局部大小时，会考虑到点之间距离的度量。考虑半径最大为 r 的球数 ''N'' (r) ，需要完全覆盖 ''X''。当 r 很小时，n (r)以1/''r'' 增长多项式。对于一个表现足够好的 ''X''，豪斯多夫维数是唯一的数 d，这样当 r 趋近于零时， N(r)增长为1/r&amp;lt;sup&amp;gt;d&amp;lt;/sup&amp;gt; 。更确切地说，这定义了盒子计数维度，当值 d 是不足以覆盖空间的增长率和过度充裕的增长率之间的关键边界时，它等于豪斯多夫维数。&lt;br /&gt;
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For shapes that are smooth, or shapes with a small number of corners, the shapes of traditional geometry and science, the Hausdorff dimension is an integer agreeing with the topological dimension. But [[Benoit Mandelbrot]] observed that [[fractal]]s, sets with noninteger Hausdorff dimensions, are found everywhere in nature. He observed that the proper idealization of most rough shapes you see around you is not in terms of smooth idealized shapes, but in terms of fractal idealized shapes:&lt;br /&gt;
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For shapes that are smooth, or shapes with a small number of corners, the shapes of traditional geometry and science, the Hausdorff dimension is an integer agreeing with the topological dimension. But Benoit Mandelbrot observed that fractals, sets with noninteger Hausdorff dimensions, are found everywhere in nature. He observed that the proper idealization of most rough shapes you see around you is not in terms of smooth idealized shapes, but in terms of fractal idealized shapes:&lt;br /&gt;
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对于光滑的形状，或者有少量棱角的形状，传统几何和科学的形状，豪斯多夫维数是一个整数，与拓扑维度一致。但是伯努·曼德布洛特观察到分形---- 具有非整数豪斯多夫维数的集合---- 在自然界中随处可见。他观察到，我们周围大多数粗糙形状的理想化不是光滑的理想化形状，而是分形理想化形状:&lt;br /&gt;
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&amp;lt;blockquote&amp;gt;Clouds are not spheres, mountains are not cones, coastlines are not circles, and bark is not smooth, nor does lightning travel in a straight line.&amp;lt;ref name=&amp;quot;mandelbrot&amp;quot;&amp;gt;{{cite book   | last = Mandelbrot   | first = Benoît   | authorlink = Benoit Mandelbrot   | title = The Fractal Geometry of Nature   | publisher = W. H. Freeman   | series = Lecture notes in mathematics 1358   | year = 1982   | doi =    | isbn = 0-7167-1186-9   | url-access = registration   | url = https://archive.org/details/fractalgeometryo00beno   }}&amp;lt;/ref&amp;gt;&amp;lt;/blockquote&amp;gt;&lt;br /&gt;
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&amp;lt;blockquote&amp;gt;Clouds are not spheres, mountains are not cones, coastlines are not circles, and bark is not smooth, nor does lightning travel in a straight line.&amp;lt;/blockquote&amp;gt;&lt;br /&gt;
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&amp;lt;blockquote&amp;gt;云不是球体，山不是锥体，海岸线不是圆圈，树皮不平滑，闪电也不是直线运动。 &amp;lt;/blockquote&amp;gt;&lt;br /&gt;
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For fractals that occur in nature, the Hausdorff and [[Minkowski–Bouligand dimension|box-counting dimension]] coincide. The [[packing dimension]] is yet another similar notion which gives the same value for many shapes, but there are well documented exceptions where all these dimensions differ.&lt;br /&gt;
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For fractals that occur in nature, the Hausdorff and box-counting dimension coincide. The packing dimension is yet another similar notion which gives the same value for many shapes, but there are well documented exceptions where all these dimensions differ.&lt;br /&gt;
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对于自然界中出现的分形，豪斯多夫维数和盒计数维数是一致的。封装尺寸是另一个类似的概念，它给出了许多形状相同的值，但是在所有这些尺寸不同的情况，都做了很好的说明。&lt;br /&gt;
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==Formal definitions形式化定义==&lt;br /&gt;
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{{unreferenced section|date=March 2015}}&lt;br /&gt;
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===Hausdorff content豪斯多夫集===&lt;br /&gt;
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Let ''X'' be a [[metric space]]. If ''S'' ⊂ ''X'' and ''d'' ∈ [0, ∞), the ''d''-dimensional '''unlimited Hausdorff content''' of ''S'' is defined by&lt;br /&gt;
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Let X be a metric space. If S ⊂ X and d ∈ [0, ∞), the d-dimensional unlimited Hausdorff content of S is defined by&lt;br /&gt;
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设 ''X''是度量空间。若''S'' ⊂ ''X'' 和 ''d'' ∈ [0, ∞) ，则 ''S'' 的''d''维无限 豪斯多夫集定义为&lt;br /&gt;
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:&amp;lt;math&amp;gt;C_H^d(S):=\inf\Bigl\{\sum_i r_i^d:\text{ there is a cover of } S\text{ by balls with radii }r_i&amp;gt;0\Bigr\}.&amp;lt;/math&amp;gt;&lt;br /&gt;
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&amp;lt;math&amp;gt;C_H^d(S):=\inf\Bigl\{\sum_i r_i^d:\text{ there is a cover of } S\text{ by balls with radii }r_i&amp;gt;0\Bigr\}.&amp;lt;/math&amp;gt;&lt;br /&gt;
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&amp;lt;math&amp;gt;C_H^d(S):=\inf\Bigl\{\sum_i r_i^d:\text{ there is a cover of } S\text{ by balls with radii }r_i&amp;gt;0\Bigr\}.&amp;lt;/math&amp;gt;&lt;br /&gt;
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In other words, &amp;lt;math&amp;gt;C_H^d(S)&amp;lt;/math&amp;gt; is the [[infimum]] of the set of numbers &amp;lt;math&amp;gt;\delta \geq 0&amp;lt;/math&amp;gt; such that there is some (indexed) collection of [[ball (mathematics)|ball]]s &amp;lt;math&amp;gt;\{B(x_i,r_i):i\in I\}&amp;lt;/math&amp;gt; covering ''S'' with ''r&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;''&amp;amp;nbsp;&amp;gt;&amp;amp;nbsp;0 for each ''i''&amp;amp;nbsp;∈&amp;amp;nbsp;''I'' that satisfies &amp;lt;math&amp;gt;\sum_{i\in I} r_i^d&amp;lt;\delta &amp;lt;/math&amp;gt;. (Here, we use the standard convention that [[infimum|inf&amp;amp;nbsp;Ø&amp;amp;nbsp;=&amp;amp;nbsp;∞]].)&lt;br /&gt;
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In other words, &amp;lt;math&amp;gt;C_H^d(S)&amp;lt;/math&amp;gt; is the infimum of the set of numbers &amp;lt;math&amp;gt;\delta \geq 0&amp;lt;/math&amp;gt; such that there is some (indexed) collection of balls &amp;lt;math&amp;gt;\{B(x_i,r_i):i\in I\}&amp;lt;/math&amp;gt; covering S with r&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;&amp;amp;nbsp;&amp;gt;&amp;amp;nbsp;0 for each i&amp;amp;nbsp;∈&amp;amp;nbsp;I that satisfies &amp;lt;math&amp;gt;\sum_{i\in I} r_i^d&amp;lt;\delta &amp;lt;/math&amp;gt;. (Here, we use the standard convention that inf&amp;amp;nbsp;Ø&amp;amp;nbsp;=&amp;amp;nbsp;∞.)&lt;br /&gt;
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换句话说，&amp;lt;math&amp;gt;C_H^d(S)&amp;lt;/math&amp;gt; 是数字集合&amp;lt;math&amp;gt;\delta \geq 0&amp;lt;/math&amp;gt;的下确界，使得在 ''i''&amp;amp;nbsp;∈&amp;amp;nbsp中存在一些球集合 &amp;lt;math&amp;gt;\{B(x_i,r_i):i\in I\}&amp;lt;/math&amp;gt;  i 包含 s，对于每个 ''r&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;''&amp;amp;nbsp;&amp;gt;&amp;amp;nbsp;0 满足 i 中的和&amp;lt;math&amp;gt;\sum_{i\in I} r_i^d&amp;lt;\delta &amp;lt;/math&amp;gt; (在这里，我们使用inf&amp;amp;nbsp;Ø&amp;amp;nbsp;=&amp;amp;nbsp;∞ )的标准约定。&lt;br /&gt;
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===Hausdorff measurement豪斯多夫分形测量===&lt;br /&gt;
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The Hausdorff outer measure is different from the unbounded Hausdorf content in that rather than considering all possible coverings of ''S'', we see what happens when the sizes of the balls go to zero. This is  for &amp;lt;math&amp;gt;d \geq 0 &amp;lt;/math&amp;gt;, we define the ''d''-dimensional Hausdorff outer measure of ''S'' as&lt;br /&gt;
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The Hausdorff outer measure is different from the unbounded Hausdorf content in that rather than considering all possible coverings of S, we see what happens when the sizes of the balls go to zero. This is  for &amp;lt;math&amp;gt;d \geq 0 &amp;lt;/math&amp;gt;, we define the d-dimensional Hausdorff outer measure of S as&lt;br /&gt;
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豪斯多夫外测度不同于无界的豪斯多夫，因为我们不考虑 s 的所有可能，我们看到当球的大小为零时会发生什么。这是为了数学  &amp;lt;math&amp;gt;d \geq 0 &amp;lt;/math&amp;gt;，我们定义了  ''S''的 ''d''维豪斯多夫Hausdorff 外测度为&lt;br /&gt;
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:&amp;lt;math&amp;gt; \mathcal{H}^d(S):=\lim_{r \to 0} \inf\Bigl\{\sum_i r_i^d:\text{ there is a cover of } S\text{ by balls with radii } 0 &amp;lt; r_i &amp;lt; r\Bigr\}.&amp;lt;/math&amp;gt;&lt;br /&gt;
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&amp;lt;math&amp;gt; \mathcal{H}^d(S):=\lim_{r \to 0} \inf\Bigl\{\sum_i r_i^d:\text{ there is a cover of } S\text{ by balls with radii } 0 &amp;lt; r_i &amp;lt; r\Bigr\}.&amp;lt;/math&amp;gt;&lt;br /&gt;
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&amp;lt;math&amp;gt; \mathcal{H}^d(S):=\lim_{r \to 0} \inf\Bigl\{\sum_i r_i^d:\text{有一个面} S\text{ 球 } 0 &amp;lt; r_i &amp;lt; r\Bigr\}.&amp;lt;/math&amp;gt;&lt;br /&gt;
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===Hausdorff dimension豪斯多夫维数===&lt;br /&gt;
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The '''Hausdorff dimension''' of ''X'' is defined by&lt;br /&gt;
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The Hausdorff dimension of X is defined by&lt;br /&gt;
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X 的豪斯多夫维数定义为&lt;br /&gt;
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:&amp;lt;math&amp;gt;\dim_{\operatorname{H}}(X):=\inf\{d\ge 0: \mathcal{H}^d(X)=0\}.&amp;lt;/math&amp;gt;&lt;br /&gt;
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&amp;lt;math&amp;gt;\dim_{\operatorname{H}}(X):=\inf\{d\ge 0: \mathcal{H}^d(X)=0\}.&amp;lt;/math&amp;gt;&lt;br /&gt;
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Equivalently, dim&amp;lt;sub&amp;gt;H&amp;lt;/sub&amp;gt;(''X'') may be defined as the [[infimum]] of the set of ''d'' ∈ [0, ∞) such that the ''d''-dimensional [[Hausdorff measure]] of ''X'' is zero. This is the same as the supremum of the set of ''d''&amp;amp;nbsp;∈&amp;amp;nbsp;[0,&amp;amp;nbsp;∞) such that the ''d''-dimensional Hausdorff measure of ''X'' is infinite (except that when this latter set of numbers ''d'' is empty the Hausdorff dimension is zero).&lt;br /&gt;
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Equivalently, dim&amp;lt;sub&amp;gt;H&amp;lt;/sub&amp;gt;(X) may be defined as the infimum of the set of d ∈ [0, ∞) such that the d-dimensional Hausdorff measure of X is zero. This is the same as the supremum of the set of d&amp;amp;nbsp;∈&amp;amp;nbsp;[0,&amp;amp;nbsp;∞) such that the d-dimensional Hausdorff measure of X is infinite (except that when this latter set of numbers d is empty the Hausdorff dimension is zero).&lt;br /&gt;
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等价地，dim &amp;lt;sub&amp;gt;H&amp;lt;/sub&amp;gt;(''X'')可定义为 ''d'' ∈ [0, ∞) 集的下确界，使得''X'' 的''d''-维 [[豪斯多夫测度]] 为零。这与 ''d''&amp;amp;nbsp;∈&amp;amp;nbsp;[0,&amp;amp;nbsp;∞)的集合的上确界相同，因此''X''的 d 维豪斯多夫测度是无限的(除非后一个集合 ''d'' 是空的，豪斯多夫维数为零)。&lt;br /&gt;
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==Examples实例==&lt;br /&gt;
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[[Image:Sierpinski deep.svg|thumb|250px|Dimension of a further [[fractal]] example. The [[Sierpinski triangle]], an object with Hausdorff dimension of log(3)/log(2)≈1.58.&amp;lt;ref name=ClaytonSCTPLS96/&amp;gt;]]&lt;br /&gt;
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Dimension of a further [[fractal example. The Sierpinski triangle, an object with Hausdorff dimension of log(3)/log(2)≈1.58.]]&lt;br /&gt;
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[[Image:谢尔宾斯基三角形 deep.svg|thumb|250px|进一步的[[分形维数]]的例子，进一步的分形维数的例子是谢尔宾斯基三角形，它是一个豪斯多夫维数为log(3)/log(2)≈1.58.&amp;lt;ref name=ClaytonSCTPLS96/&amp;gt;的物体]]&lt;br /&gt;
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* [[Countable set]]s have Hausdorff dimension 0.&amp;lt;ref name=&amp;quot;schleicher&amp;quot;&amp;gt;{{cite journal |last1=Schleicher |first1=Dierk |title=Hausdorff Dimension, Its Properties, and Its Surprises |journal=The American Mathematical Monthly |date=June 2007 |volume=114 |issue=6 |pages=509–528 |doi=10.1080/00029890.2007.11920440 |language=en |issn=0002-9890|arxiv=math/0505099 }}&amp;lt;/ref&amp;gt;&lt;br /&gt;
*[[可数集]]拥有豪斯多夫维数0.&amp;lt;ref name=&amp;quot;schleicher&amp;quot;&amp;gt;{{cite journal |last1=Schleicher |first1=Dierk |title=豪斯多夫维数, Its Properties, and Its Surprises |journal=The American Mathematical Monthly美国数学期刊 |date=June 2007 |volume=114 |issue=6 |pages=509–528 |doi=10.1080/00029890.2007.11920440 |language=en |issn=0002-9890|arxiv=math/0505099 }}&amp;lt;/ref&amp;gt;&lt;br /&gt;
* The [[Euclidean space]] ℝ&amp;lt;sup&amp;gt;''n''&amp;lt;/sup&amp;gt; has Hausdorff dimension ''n'', and the circle '''S'''&amp;lt;sup&amp;gt;1&amp;lt;/sup&amp;gt; has Hausdorff dimension 1.&amp;lt;ref name=&amp;quot;schleicher&amp;quot; /&amp;gt;&lt;br /&gt;
*[[教育空间]] ℝ&amp;lt;sup&amp;gt;''n''&amp;lt;/sup&amp;gt; 有豪斯多夫维数 ''n''，循环'''S'''&amp;lt;sup&amp;gt;1&amp;lt;/sup&amp;gt; 拥有豪斯多夫维数1.&amp;lt;ref name=&amp;quot;schleicher&amp;quot; /&amp;gt;&lt;br /&gt;
* [[Fractal]]s often are spaces whose Hausdorff dimension strictly exceeds the [[topological dimension]].&amp;lt;ref name=&amp;quot;mandelbrot&amp;quot; /&amp;gt; For example, the [[Cantor set]], a zero-dimensional topological space, is a union of two copies of itself, each copy shrunk by a factor 1/3; hence, it can be shown that its Hausdorff dimension is ln(2)/ln(3)&amp;amp;nbsp;≈&amp;amp;nbsp;0.63.&amp;lt;ref&amp;gt;{{cite book | last=Falconer | first = Kenneth |title=Fractal Geometry: Mathematical Foundations and Applications | publisher=[[John Wiley and Sons]] | edition=2nd | year=2003}}&amp;lt;/ref&amp;gt; The [[Sierpinski triangle]] is a union of three copies of itself, each copy shrunk by a factor of&amp;amp;nbsp;1/2; this yields a Hausdorff dimension of ln(3)/ln(2)&amp;amp;nbsp;≈&amp;amp;nbsp;1.58.&amp;lt;ref name=CampbellAnnenberg15/&amp;gt; These Hausdorff dimensions are related to the &amp;quot;critical exponent&amp;quot; of the [[Master theorem (analysis of algorithms)|Master theorem]] for solving [[Recurrence relation|recurrence relations]] in the [[analysis of algorithms]].&lt;br /&gt;
*[[分形]]一般是那些豪斯多夫维数直接超过其拓扑维数的空间。例如[[康托尔集]]是一个o维拓扑空间，由两个自己复制而成，每一个复制品都是原来的三分之一，因此它的豪斯多夫维数是 ln(2)/ln(3)&amp;amp;nbsp;≈&amp;amp;nbsp;0.63。&amp;lt;ref&amp;gt;{{cite book | last=Falconer | first = Kenneth |title=Fractal Geometry: Mathematical Foundations and Applications | publisher=[[John Wiley and Sons]] | edition=2nd | year=2003}}&amp;lt;/ref&amp;gt;一个[[谢尔宾斯基三角]]是他自身三个复制的组合。每一个是原来的&amp;amp;nbsp;1/2，它的豪斯多夫维数ln(3)/ln(2)&amp;amp;nbsp;≈&amp;amp;nbsp;1.58。&amp;lt;ref name=CampbellAnnenberg15/&amp;gt;在递归算法中解决递归关系时，这些豪斯多夫维数与[[算法分析主定理]]的临界指标相联系。&lt;br /&gt;
* [[Space-filling curve]]s like the [[Peano curve]] have the same Hausdorff dimension as the space they fill.&lt;br /&gt;
*[[空间填充曲线]]拥有和他们填充空间同样的豪斯多夫维数，如[[皮亚诺曲线]]。&lt;br /&gt;
* The trajectory of [[Brownian motion]] in dimension 2 and above is conjectured to be Hausdorff dimension 2.&amp;lt;ref&amp;gt;{{cite book | last=Morters | first=Peres | title= Brownian Motion | publisher=[[Cambridge University Press]] | year=2010 }}&amp;lt;/ref&amp;gt;&lt;br /&gt;
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[[image:Great Britain Hausdorff.svg|thumb|250px|Estimating the Hausdorff dimension of the [[How Long Is the Coast of Britain? Statistical Self-Similarity and Fractional Dimension|coast of Great Britain]]]]&lt;br /&gt;
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coast of Great Britain]]&lt;br /&gt;
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[[大不列颠海岸&lt;br /&gt;
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* 刘易斯·弗赖伊·理查森[[Lewis Fry Richardson]] has performed detailed experiments to measure the approximate Hausdorff dimension for various coastlines. His results have varied from 1.02 for the coastline of [[South Africa]] to 1.25 for the west coast of [[Great Britain]].&amp;lt;ref name=&amp;quot;mandelbrot&amp;quot; /&amp;gt;&lt;br /&gt;
*刘易斯·弗赖伊·理查森（Lewis Fry Richardson）已经通过豪斯多夫维数去测量了很多海岸线。它的结果涵盖从1.02的南非海岸线到1.25的大英帝国西海岸模型。]]&lt;br /&gt;
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==Properties of Hausdorff dimension豪斯多夫维数特性==&lt;br /&gt;
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{{refimprove section|date=March 2015}}&lt;br /&gt;
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=== Hausdorff dimension and inductive dimension 豪斯多夫维数和归纳维数===&lt;br /&gt;
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Let ''X'' be an arbitrary [[Separable space|separable]] metric space. There is a [[topology|topological]] notion of [[inductive dimension]] for ''X'' which is defined recursively. It is always an integer (or +∞) and is denoted dim&amp;lt;sub&amp;gt;ind&amp;lt;/sub&amp;gt;(''X'').&lt;br /&gt;
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Let X be an arbitrary separable metric space. There is a topological notion of inductive dimension for X which is defined recursively. It is always an integer (or +∞) and is denoted dim&amp;lt;sub&amp;gt;ind&amp;lt;/sub&amp;gt;(X).&lt;br /&gt;
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设''X'' 是[[任意可分度量空间]]。对于''X'' 有一个递归定义的归纳维数拓扑概念。它总是一个整数(或 + ∞) ，并且表示dim&amp;lt;sub&amp;gt;ind&amp;lt;/sub&amp;gt;(''X'')。&lt;br /&gt;
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'''Theorem'''. Suppose ''X'' is non-empty. Then &lt;br /&gt;
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Theorem. Suppose X is non-empty. Then &lt;br /&gt;
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'''定理'''：假设''X'' 是非空的。那么&lt;br /&gt;
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:&amp;lt;math&amp;gt; \dim_{\mathrm{Haus}}(X) \geq \dim_{\operatorname{ind}}(X). &amp;lt;/math&amp;gt;&lt;br /&gt;
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&amp;lt;math&amp;gt; \dim_{\mathrm{Haus}}(X) \geq \dim_{\operatorname{ind}}(X). &amp;lt;/math&amp;gt;&lt;br /&gt;
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Moreover,&lt;br /&gt;
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Moreover,&lt;br /&gt;
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此外,&lt;br /&gt;
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&amp;lt;math&amp;gt; \inf_Y \dim_{\operatorname{Haus}}(Y) =\dim_{\operatorname{ind}}(X), &amp;lt;/math&amp;gt;&lt;br /&gt;
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&amp;lt;math&amp;gt; \inf_Y \dim_{\operatorname{Haus}}(Y) =\dim_{\operatorname{ind}}(X), &amp;lt;/math&amp;gt;&lt;br /&gt;
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where ''Y'' ranges over metric spaces [[homeomorphic]] to ''X''. In other words, ''X'' and ''Y'' have the same underlying set of points and the metric ''d''&amp;lt;sub&amp;gt;''Y''&amp;lt;/sub&amp;gt; of ''Y'' is topologically equivalent to ''d''&amp;lt;sub&amp;gt;''X''&amp;lt;/sub&amp;gt;.&lt;br /&gt;
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where Y ranges over metric spaces homeomorphic to X. In other words, X and Y have the same underlying set of points and the metric d&amp;lt;sub&amp;gt;Y&amp;lt;/sub&amp;gt; of Y is topologically equivalent to d&amp;lt;sub&amp;gt;X&amp;lt;/sub&amp;gt;.&lt;br /&gt;
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其中''Y''是度量空间同胚到 ''X''的范围。换句话说， ''X''和 ''Y''具有相同的基本点集，''Y''的度规''d''&amp;lt;sub&amp;gt;''Y''&amp;lt;/sub&amp;gt; 的子拓扑等价于''d''&amp;lt;sub&amp;gt;''X''&amp;lt;/sub&amp;gt;。&lt;br /&gt;
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&lt;br /&gt;
&lt;br /&gt;
These results were originally established by [[Edward Szpilrajn]] (1907–1976), e.g., see Hurewicz and Wallman, Chapter VII.{{full citation needed|date=March 2015}}&lt;br /&gt;
&lt;br /&gt;
These results were originally established by Edward Szpilrajn (1907–1976), e.g., see Hurewicz and Wallman, Chapter VII.&lt;br /&gt;
&lt;br /&gt;
这些结果最初是由 [[Edward Szpilrajn]] (1907–1976)建立的,  参见 Hurewicz and Wallman, Chapter VII.{{full citation needed|date=March 2015}}第七章。&lt;br /&gt;
&lt;br /&gt;
=== Hausdorff dimension and Minkowski dimension 豪斯多夫维数和闵可夫斯基维度===&lt;br /&gt;
&lt;br /&gt;
The [[Minkowski dimension]] is similar to, and at least as large as, the Hausdorff dimension, and they are equal in many situations. However, the set of [[rational number|rational]] points in [0, 1] has Hausdorff dimension zero and Minkowski dimension one. There are also compact sets for which the Minkowski dimension is strictly larger than the Hausdorff dimension.&lt;br /&gt;
&lt;br /&gt;
The Minkowski dimension is similar to, and at least as large as, the Hausdorff dimension, and they are equal in many situations. However, the set of rational points in [0, 1] has Hausdorff dimension zero and Minkowski dimension one. There are also compact sets for which the Minkowski dimension is strictly larger than the Hausdorff dimension.&lt;br /&gt;
&lt;br /&gt;
[[闵可夫斯基维数]]与豪斯多夫维数相似，至少和它一样大，而且在许多情况下是相等的。然而，[0,1]中有理点集的豪斯多夫维数为0，闵可夫斯基维数为1。还有一些紧集的闵可夫斯基维数绝对大于豪斯多夫维数。&lt;br /&gt;
&lt;br /&gt;
=== Hausdorff dimensions and Frostman measures 豪斯多夫维度和弗洛斯曼测度===&lt;br /&gt;
&lt;br /&gt;
If there is a [[measure (mathematics)|measure]] μ defined on [[Borel measure|Borel]] subsets of a metric space ''X'' such that ''μ''(''X'') &amp;gt; 0 and ''μ''(''B''(''x'', ''r'')) ≤ ''r&amp;lt;sup&amp;gt;s&amp;lt;/sup&amp;gt;'' holds for some constant ''s'' &amp;gt; 0 and for every ball ''B''(''x'', ''r'') in ''X'', then dim&amp;lt;sub&amp;gt;Haus&amp;lt;/sub&amp;gt;(''X'') ≥ ''s''. A partial converse is provided by [[Frostman's lemma]].{{citation needed|date=March 2015}}&amp;lt;ref&amp;gt;This Wikipedia article also discusses further useful characterizations of the Hausdorff dimension.{{clarify|date=March 2015}}&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
If there is a measure μ defined on Borel subsets of a metric space X such that μ(X) &amp;gt; 0 and μ(B(x, r)) ≤ r&amp;lt;sup&amp;gt;s&amp;lt;/sup&amp;gt; holds for some constant s &amp;gt; 0 and for every ball B(x, r) in X, then dim&amp;lt;sub&amp;gt;Haus&amp;lt;/sub&amp;gt;(X) ≥ s. A partial converse is provided by Frostman's lemma.&lt;br /&gt;
&lt;br /&gt;
如果在度量空间 ''X'' 的 Borel 子集上定义一个测度 μ，使得''μ''(''X'') &amp;gt; 0 和''μ''(''B''(''x'', ''r'')) ≤ ''r&amp;lt;sup&amp;gt;s&amp;lt;/sup&amp;gt;''，对于某个常数 ''s'' &amp;gt; 0  和 ''X'' 中的每个球 ''B''(''x'', ''r'') 成立，则 dim&amp;lt;sub&amp;gt;Haus&amp;lt;/sub&amp;gt;(''X'') ≥ ''s'' 。 部分逆向转换由弗洛斯曼引理定义。&lt;br /&gt;
&lt;br /&gt;
=== Behaviour under unions and products ===&lt;br /&gt;
&lt;br /&gt;
If &amp;lt;math&amp;gt;X=\bigcup_{i\in I}X_i&amp;lt;/math&amp;gt; is a finite or countable union, then&lt;br /&gt;
&lt;br /&gt;
If &amp;lt;math&amp;gt;X=\bigcup_{i\in I}X_i&amp;lt;/math&amp;gt; is a finite or countable union, then&lt;br /&gt;
&lt;br /&gt;
如果 &amp;lt;math&amp;gt;X=\bigcup_{i\in I}X_i&amp;lt;/math&amp;gt; 是一个有限或可数的联合，则&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \dim_{\operatorname{Haus}}(X) =\sup_{i\in I} \dim_{\operatorname{Haus}}(X_i).&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \dim_{\operatorname{Haus}}(X) =\sup_{i\in I} \dim_{\operatorname{Haus}}(X_i).&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
This can be verified directly from the definition.&lt;br /&gt;
&lt;br /&gt;
This can be verified directly from the definition.&lt;br /&gt;
&lt;br /&gt;
这可以直接从定义得到验证。&lt;br /&gt;
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&lt;br /&gt;
&lt;br /&gt;
If ''X'' and ''Y'' are non-empty metric spaces, then the Hausdorff dimension of their product satisfies&amp;lt;ref&amp;gt;{{cite journal |author=Marstrand, J. M. |title=The dimension of Cartesian product sets |journal=Proc. Cambridge Philos. Soc. |volume=50 |issue=3 |pages=198–202 |year=1954 |doi=10.1017/S0305004100029236 |bibcode = 1954PCPS...50..198M }}&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
If X and Y are non-empty metric spaces, then the Hausdorff dimension of their product satisfies&lt;br /&gt;
&lt;br /&gt;
如果 ''X'' 和''Y''是非空度量空间，那么它们乘积的豪斯多夫维数满足&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt; \dim_{\operatorname{Haus}}(X\times Y)\ge \dim_{\operatorname{Haus}}(X)+ \dim_{\operatorname{Haus}}(Y).&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \dim_{\operatorname{Haus}}(X\times Y)\ge \dim_{\operatorname{Haus}}(X)+ \dim_{\operatorname{Haus}}(Y).&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
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This inequality can be strict. It is possible to find two sets of dimension 0 whose product has dimension 1.&amp;lt;ref&amp;gt;{{cite book  | last = Falconer  | first = Kenneth J.  | title = Fractal geometry. Mathematical foundations and applications  | publisher = John Wiley &amp;amp; Sons, Inc., Hoboken, New Jersey  | year = 2003  | doi =   | isbn = }}&amp;lt;/ref&amp;gt; In the opposite direction, it is known that when ''X'' and ''Y'' are Borel subsets of '''R'''&amp;lt;sup&amp;gt;''n''&amp;lt;/sup&amp;gt;, the Hausdorff dimension of ''X'' × ''Y'' is bounded from above by the Hausdorff dimension of ''X'' plus the [[packing dimension|upper packing dimension]] of ''Y''. These facts are discussed in Mattila (1995).&lt;br /&gt;
&lt;br /&gt;
This inequality can be strict. It is possible to find two sets of dimension 0 whose product has dimension 1. In the opposite direction, it is known that when X and Y are Borel subsets of R&amp;lt;sup&amp;gt;n&amp;lt;/sup&amp;gt;, the Hausdorff dimension of X × Y is bounded from above by the Hausdorff dimension of X plus the upper packing dimension of Y. These facts are discussed in Mattila (1995).&lt;br /&gt;
&lt;br /&gt;
这种不平等可以是绝对的。有可能找到两个维数为0的集合，其乘积的维数为1。相反，我们知道当''X''和''Y''是 '''R'''&amp;lt;sup&amp;gt;''n''&amp;lt;/sup&amp;gt;的 Borel 子集时， ''X'' × ''Y''的豪斯多夫维数从上面以 ''X''的豪斯多夫维数加上 ''Y''的填充维数为界。Mattila (1995)曾就这些情况进行了讨论。&lt;br /&gt;
&lt;br /&gt;
==Self-similar sets自相似集合==&lt;br /&gt;
&lt;br /&gt;
{{refimprove section|date=March 2015}}&lt;br /&gt;
&lt;br /&gt;
Many sets defined by a self-similarity condition have dimensions which can be determined explicitly. Roughly, a set ''E'' is self-similar if it is the fixed point of a set-valued transformation ψ, that is ψ(''E'') = ''E'', although the exact definition is given below.&lt;br /&gt;
&lt;br /&gt;
Many sets defined by a self-similarity condition have dimensions which can be determined explicitly. Roughly, a set E is self-similar if it is the fixed point of a set-valued transformation ψ, that is ψ(E) = E, although the exact definition is given below.&lt;br /&gt;
&lt;br /&gt;
许多由自相似条件定义的集合具有可以显式确定的维数。粗略地说，集合''E'' 是自相似的，如果它是集值ψ变换的不动点，即ψ(''E'') = ''E''，尽管下面给出了确切的定义。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&amp;lt;blockquote&amp;gt;'''Theorem'''. Suppose&lt;br /&gt;
&lt;br /&gt;
&amp;lt;blockquote&amp;gt;Theorem. Suppose&lt;br /&gt;
&lt;br /&gt;
&amp;lt;blockquote&amp;gt;'''定理'''：假设&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt; \psi_i: \mathbf{R}^n \rightarrow \mathbf{R}^n, \quad i=1, \ldots , m &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \psi_i: \mathbf{R}^n \rightarrow \mathbf{R}^n, \quad i=1, \ldots , m &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
are [[Contraction mapping|contractive]] mappings on '''R'''&amp;lt;sup&amp;gt;''n''&amp;lt;/sup&amp;gt; with contraction constant ''r&amp;lt;sub&amp;gt;j&amp;lt;/sub&amp;gt;'' &amp;lt; 1. Then there is a unique ''non-empty'' compact set ''A'' such that&lt;br /&gt;
&lt;br /&gt;
are contractive mappings on R&amp;lt;sup&amp;gt;n&amp;lt;/sup&amp;gt; with contraction constant r&amp;lt;sub&amp;gt;j&amp;lt;/sub&amp;gt; &amp;lt; 1. Then there is a unique non-empty compact set A such that&lt;br /&gt;
&lt;br /&gt;
是'''R'''&amp;lt;sup&amp;gt;''n''&amp;lt;/sup&amp;gt;上的压缩常数''r&amp;lt;sub&amp;gt;j&amp;lt;/sub&amp;gt;'&amp;lt; 1的压缩映射。然后有一个唯一的非空紧集A &lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt; A = \bigcup_{i=1}^m \psi_i (A). &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; A = \bigcup_{i=1}^m \psi_i (A). &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&amp;lt;/blockquote&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;/blockquote&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The theorem follows from [[Stefan Banach]]'s [[Contractive mapping theorem|contractive mapping fixed point theorem]] applied to the complete metric space of non-empty compact subsets of '''R'''&amp;lt;sup&amp;gt;''n''&amp;lt;/sup&amp;gt; with the [[Hausdorff distance]].&amp;lt;ref&amp;gt;{{cite book |author=Falconer, K. J. |title=The Geometry of Fractal Sets |publisher=Cambridge University Press |location=Cambridge, UK |year=1985 |isbn=0-521-25694-1 |chapter=Theorem 8.3}}&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
The theorem follows from Stefan Banach's contractive mapping fixed point theorem applied to the complete metric space of non-empty compact subsets of R&amp;lt;sup&amp;gt;n&amp;lt;/sup&amp;gt; with the Hausdorff distance.&lt;br /&gt;
&lt;br /&gt;
这个定理来源于 Stefan Banach 的压缩映射不动点定理，该定理应用于 '''R'''&amp;lt;sup&amp;gt;''n''&amp;lt;/sup&amp;gt; 的非空紧子集的完备空间豪斯多夫距离。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
===The open set condition开集条件===&lt;br /&gt;
&lt;br /&gt;
To determine the dimension of the self-similar set ''A'' (in certain cases), we need a technical condition called the ''open set condition'' (OSC) on the sequence of contractions ψ&amp;lt;sub&amp;gt;''i''&amp;lt;/sub&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
To determine the dimension of the self-similar set A (in certain cases), we need a technical condition called the open set condition (OSC) on the sequence of contractions ψ&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
为了确定自相似集''A'' 的维数(在某些情况下) ，我们需要一个称为''开集条件''(OSC)的技术条件ψ&amp;lt;sub&amp;gt;''i''&amp;lt;/sub&amp;gt;。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
There is a relatively compact open set ''V'' such that&lt;br /&gt;
&lt;br /&gt;
There is a relatively compact open set V such that&lt;br /&gt;
&lt;br /&gt;
有一个相对紧的开集''V''&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt; \bigcup_{i=1}^m\psi_i (V) \subseteq V, &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \bigcup_{i=1}^m\psi_i (V) \subseteq V, &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
where the sets in union on the left are pairwise [[disjoint sets|disjoint]].&lt;br /&gt;
&lt;br /&gt;
where the sets in union on the left are pairwise disjoint.&lt;br /&gt;
&lt;br /&gt;
左边的集合是成对不相交的。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The open set condition is a separation condition that ensures the images ψ&amp;lt;sub&amp;gt;''i''&amp;lt;/sub&amp;gt;(''V'') do not overlap &amp;quot;too much&amp;quot;.&lt;br /&gt;
&lt;br /&gt;
The open set condition is a separation condition that ensures the images ψ&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;(V) do not overlap &amp;quot;too much&amp;quot;.&lt;br /&gt;
&lt;br /&gt;
开集条件是保证图像子ψ&amp;lt;sub&amp;gt;''i''&amp;lt;/sub&amp;gt;(''V'') 不重叠“太多”的分离条件。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
'''Theorem'''. Suppose the open set condition holds and each ψ&amp;lt;sub&amp;gt;''i''&amp;lt;/sub&amp;gt; is a similitude, that is a composition of an [[isometry]] and a [[dilation (metric space)|dilation]] around some point. Then the unique fixed point of ψ is a set whose Hausdorff dimension is ''s'' where ''s'' is the unique solution of&amp;lt;ref&amp;gt;{{cite journal | last=Hutchinson | first=John E. | title=Fractals and self similarity | journal=Indiana Univ. Math. J. | volume=30 | year=1981 | pages=713–747 | doi=10.1512/iumj.1981.30.30055 | issue=5 | doi-access=free }}&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
Theorem. Suppose the open set condition holds and each ψ&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt; is a similitude, that is a composition of an isometry and a dilation around some point. Then the unique fixed point of ψ is a set whose Hausdorff dimension is s where s is the unique solution of&lt;br /&gt;
&lt;br /&gt;
'''定理'''假设开集条件成立，并且每个ψ&amp;lt;sub&amp;gt;''i''&amp;lt;/sub&amp;gt; 是一个相似量，这是一个等距和围绕某一点的膨胀的合成。那么唯一的不动点是一个集合，它的豪斯多夫维数是 ''s'' ，其中  ''s'' 是 ''s'' &amp;lt;ref&amp;gt;{{cite journal | last=Hutchinson | first=John E. | title=Fractals and self similarity | journal=Indiana Univ. Math. J. | volume=30 | year=1981 | pages=713–747 | doi=10.1512/iumj.1981.30.30055 | issue=5 | doi-access=free }}&amp;lt;/ref&amp;gt;的唯一解&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt; \sum_{i=1}^m r_i^s = 1. &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \sum_{i=1}^m r_i^s = 1. &amp;lt;/math&amp;gt;&lt;br /&gt;
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The contraction coefficient of a similitude is the magnitude of the dilation.&lt;br /&gt;
&lt;br /&gt;
The contraction coefficient of a similitude is the magnitude of the dilation.&lt;br /&gt;
&lt;br /&gt;
相似物的收缩系数就是膨胀的大小。&lt;br /&gt;
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&lt;br /&gt;
&lt;br /&gt;
We can use this theorem to compute the Hausdorff dimension of the Sierpinski triangle (or sometimes called Sierpinski gasket). Consider three [[non-collinear points]] ''a''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;, ''a''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;, ''a''&amp;lt;sub&amp;gt;3&amp;lt;/sub&amp;gt; in the plane '''R'''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; and let ψ&amp;lt;sub&amp;gt;''i''&amp;lt;/sub&amp;gt; be the dilation of ratio 1/2 around ''a&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;''. The unique non-empty fixed point of the corresponding mapping ψ is a Sierpinski gasket and the dimension ''s'' is the unique solution of&lt;br /&gt;
&lt;br /&gt;
We can use this theorem to compute the Hausdorff dimension of the Sierpinski triangle (or sometimes called Sierpinski gasket). Consider three non-collinear points a&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;, a&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;, a&amp;lt;sub&amp;gt;3&amp;lt;/sub&amp;gt; in the plane R&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; and let ψ&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt; be the dilation of ratio 1/2 around a&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;. The unique non-empty fixed point of the corresponding mapping ψ is a Sierpinski gasket and the dimension s is the unique solution of&lt;br /&gt;
&lt;br /&gt;
我们可以使用这个定理来计算谢尔宾斯基三角形的豪斯多夫维数(或者有时候叫做谢尔宾斯基垫圈)。考虑R&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; 平面上的三个非共线点，''a''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;，''a''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;，''a''&amp;lt;sub&amp;gt;3&amp;lt;/sub&amp;gt;，让ψ&amp;lt;sub&amp;gt;''i''&amp;lt;/sub&amp;gt;是围绕着''a&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;''膨胀比率的1/2。对应映射的唯一非空不动点是一个谢尔宾斯基垫圈，其维数''s''是对应映射的唯一解&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt; \left(\frac{1}{2}\right)^s+\left(\frac{1}{2}\right)^s+\left(\frac{1}{2}\right)^s = 3 \left(\frac{1}{2}\right)^s =1. &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \left(\frac{1}{2}\right)^s+\left(\frac{1}{2}\right)^s+\left(\frac{1}{2}\right)^s = 3 \left(\frac{1}{2}\right)^s =1. &amp;lt;/math&amp;gt;&lt;br /&gt;
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Taking [[natural logarithm]]s of both sides of the above equation, we can solve for ''s'', that is: ''s'' = ln(3)/ln(2).  The Sierpinski gasket is self-similar and satisfies the OSC. In general a set ''E'' which is a fixed point of a mapping&lt;br /&gt;
&lt;br /&gt;
Taking natural logarithms of both sides of the above equation, we can solve for s, that is: s = ln(3)/ln(2).  The Sierpinski gasket is self-similar and satisfies the OSC. In general a set E which is a fixed point of a mapping&lt;br /&gt;
&lt;br /&gt;
取上述方程两边的自然对数，我们可以求出 ''s''，即: ''s'' = ln(3)/ln(2)。该密封垫具有自相似性，满足 OSC 要求。一般来说，集合 ''E''是一个映射的不动点&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt; A \mapsto \psi(A) = \bigcup_{i=1}^m \psi_i(A) &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt; A \mapsto \psi(A) = \bigcup_{i=1}^m \psi_i(A) &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
is self-similar if and only if the intersections&lt;br /&gt;
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is self-similar if and only if the intersections&lt;br /&gt;
&lt;br /&gt;
是自相似的，当且仅当&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt; H^s\left(\psi_i(E) \cap \psi_j(E)\right) =0, &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; H^s\left(\psi_i(E) \cap \psi_j(E)\right) =0, &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
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where ''s'' is the Hausdorff dimension of ''E'' and ''H&amp;lt;sup&amp;gt;s&amp;lt;/sup&amp;gt;'' denotes [[Hausdorff measure]]. This is clear in the case of the Sierpinski gasket (the intersections are just points), but is also true more generally:&lt;br /&gt;
&lt;br /&gt;
where s is the Hausdorff dimension of E and H&amp;lt;sup&amp;gt;s&amp;lt;/sup&amp;gt; denotes Hausdorff measure. This is clear in the case of the Sierpinski gasket (the intersections are just points), but is also true more generally:&lt;br /&gt;
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其中 ''s''是''E''的豪斯多夫维数， ''H&amp;lt;sup&amp;gt;s&amp;lt;/sup&amp;gt;'' 表示 豪斯多夫测度。对于谢尔宾斯基垫圈(交叉点就是点)来说，这一点很明显，但更普遍的情况是:&lt;br /&gt;
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'''Theorem'''. Under the same conditions as the previous theorem, the unique fixed point of ψ is self-similar.&lt;br /&gt;
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Theorem. Under the same conditions as the previous theorem, the unique fixed point of ψ is self-similar.&lt;br /&gt;
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'''定理'''：在与前一定理相同的条件下，其唯一不动点是自相似的。&lt;br /&gt;
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==See also参阅==&lt;br /&gt;
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* [[List of fractals by Hausdorff dimension豪斯多夫分形维数列表]] Examples of deterministic fractals, random and natural fractals.确定性分形与随机和自然分形的示例。&lt;br /&gt;
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* [[Assouad dimension  Assouad维数]], another variation of fractal dimension that, like Hausdorff dimension, is defined using coverings by balls其他被球覆盖方式定义的分形维数，例如豪斯多夫维数。&lt;br /&gt;
&lt;br /&gt;
* [[Intrinsic dimension固有维数]]&lt;br /&gt;
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* [[Packing dimension填充维数]]&lt;br /&gt;
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* [[Fractal dimension分形维数]]&lt;br /&gt;
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==References参考文献==&lt;br /&gt;
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{{reflist}}&lt;br /&gt;
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==Further reading拓展阅读==&lt;br /&gt;
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* {{cite book |last1=Dodson |first1=M. Maurice |title=Fractal Geometry and Applications: A Jubilee of Benoît Mandelbrot |volume=72 |issue=1 |pages=305–347 |last2=Kristensen |first2=Simon |chapter=Hausdorff Dimension and Diophantine Approximation |date=June 12, 2003 |arxiv=math/0305399 |bibcode = 2003math......5399D |doi=10.1090/pspum/072.1/2112110|series=Proceedings of Symposia in Pure Mathematics |isbn=9780821836378 }}&lt;br /&gt;
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* {{cite book |last1=Hurewicz |first1=Witold |authorlink1=Witold Hurewicz |last2=Wallman |first2=Henry |authorlink2=Henry Wallman |title=Dimension Theory |url=https://archive.org/details/in.ernet.dli.2015.84609 |publisher=Princeton University Press |year=1948 }}&lt;br /&gt;
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* {{cite journal |author作者=E. Szpilrajn |authorlink=Edward Marczewski |title=La dimension et la mesure |journal=Fundamenta Mathematicae |volume=28 |pages=81–9 |year=1937 }}&lt;br /&gt;
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* {{cite journal&lt;br /&gt;
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 | last1=Marstrand&lt;br /&gt;
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 | last1=Marstrand&lt;br /&gt;
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 | last1=马斯特兰德&lt;br /&gt;
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 | first1=J. M. | title=The dimension of cartesian product sets | year=1954 | journal=Proc. Cambridge Philos. Soc.&lt;br /&gt;
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 | first1=J. M. | title=The dimension of cartesian product sets | year=1954 | journal=Proc. Cambridge Philos. Soc.&lt;br /&gt;
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 | first1= J. M. | title=笛卡儿积集的维数 | 1954年 |  journal=Proc. Cambridge Philos. Soc.&lt;br /&gt;
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 | volume=50&lt;br /&gt;
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 | volume=50&lt;br /&gt;
&lt;br /&gt;
 | 第50卷&lt;br /&gt;
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 | issue=3&lt;br /&gt;
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 | issue=3&lt;br /&gt;
&lt;br /&gt;
 | 第三期&lt;br /&gt;
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 | pages=198–202&lt;br /&gt;
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 | pages=198–202&lt;br /&gt;
&lt;br /&gt;
 | 第198-202页&lt;br /&gt;
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 | doi=10.1017/S0305004100029236|bibcode = 1954PCPS...50..198M }}&lt;br /&gt;
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 | doi=10.1017/S0305004100029236|bibcode = 1954PCPS...50..198M }}&lt;br /&gt;
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10.1017 / S0305004100029236 | bibcode 1954PCPS... 50. . 198 m }&lt;br /&gt;
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* {{Cite book&lt;br /&gt;
&lt;br /&gt;
 | last1=Mattila&lt;br /&gt;
&lt;br /&gt;
 | last1=Mattila&lt;br /&gt;
&lt;br /&gt;
 | last1=Mattila&lt;br /&gt;
&lt;br /&gt;
 | first1=Pertti | author1-link=Pertti Mattila| title=Geometry of sets and measures in Euclidean spaces | publisher=[[Cambridge University Press]]&lt;br /&gt;
&lt;br /&gt;
 | first1=Pertti | author1-link=Pertti Mattila| title=Geometry of sets and measures in Euclidean spaces | publisher=Cambridge University Press&lt;br /&gt;
&lt;br /&gt;
| first1 Pertti | author1-link Pertti Mattila | title 欧几里德空间中集合和度量的几何 | 出版商剑桥大学出版社&lt;br /&gt;
&lt;br /&gt;
 | isbn=978-0-521-65595-8 | year=1995}}&lt;br /&gt;
&lt;br /&gt;
 | isbn=978-0-521-65595-8 | year=1995}}&lt;br /&gt;
&lt;br /&gt;
| isbn 978-0-521-65595-8 | year 1995}&lt;br /&gt;
&lt;br /&gt;
* {{cite journal |author=A. S. Besicovitch |authorlink=A. S. Besicovitch |title=On Linear Sets of Points of Fractional Dimensions |journal=[[Mathematische Annalen]] |volume=101 |year=1929 | doi=10.1007/BF01454831| issue=1 |pages= 161–193}}&lt;br /&gt;
&lt;br /&gt;
* {{cite journal |author1=A. S. Besicovitch |authorlink1=A. S. Besicovitch |author2=H. D. Ursell |authorlink2=H. D. Ursell |title=Sets of Fractional Dimensions |journal=Journal of the London Mathematical Society |volume=12 |year=1937 | issue=1 | doi=10.1112/jlms/s1-12.45.18  | pages=18–25 }}&amp;lt;br/&amp;gt;Several selections from this volume are reprinted in {{cite book |author=Edgar, Gerald A. |title=Classics on fractals |publisher=Addison-Wesley |location=Boston |year=1993 |isbn=0-201-58701-7}} See chapters 9,10,11&lt;br /&gt;
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* {{cite journal |author=F. Hausdorff |authorlink=F. Hausdorff |title=Dimension und äußeres Maß |journal=Mathematische Annalen |volume=79 |issue=1–2 |pages=157–179 |date=March 1919 |doi=10.1007/BF01457179|hdl=10338.dmlcz/100363 |url=http://dml.cz/bitstream/handle/10338.dmlcz/100363/CzechMathJ_09-1959-3_5.pdf }}&lt;br /&gt;
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* {{cite journal | last=Hutchinson | first=John E. | title=Fractals and self similarity | journal=Indiana Univ. Math. J. | volume=30 | year=1981 | pages=713–747 | doi=10.1512/iumj.1981.30.30055 | issue=5 | doi-access=free }}&lt;br /&gt;
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*{{cite book | last=Falconer | first = Kenneth |title=Fractal Geometry: Mathematical Foundations and Applications | publisher=[[John Wiley and Sons]] | edition=2nd | year=2003}}&lt;br /&gt;
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==External links外部链接==&lt;br /&gt;
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* [https://www.encyclopediaofmath.org/index.php/Hausdorff_dimension Hausdorff dimension] 在 [https://www.encyclopediaofmath.org/ Encyclopedia of Mathematics]&lt;br /&gt;
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* [https://www.encyclopediaofmath.org/index.php/Hausdorff_measure Hausdorff measure] 在 [https://www.encyclopediaofmath.org/ Encyclopedia of Mathematics]&lt;br /&gt;
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{{DEFAULTSORT:Hausdorff Dimension豪斯多夫维数}}&lt;br /&gt;
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[[Category分类:Fractals分形]]&lt;br /&gt;
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[[Category分类:Metric geometry度量几何]]&lt;br /&gt;
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[[Category分类:Dimension theory维度理论]]&lt;br /&gt;
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&amp;lt;small&amp;gt;This page was moved from [[wikipedia:en:Hausdorff dimension]]. Its edit history can be viewed at [[分形维数/edithistory]]&amp;lt;/small&amp;gt;&amp;lt;/noinclude&amp;gt;&lt;br /&gt;
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[[Category:待整理页面]]&lt;/div&gt;</summary>
		<author><name>Ruili</name></author>
	</entry>
	<entry>
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		<title>分形维数</title>
		<link rel="alternate" type="text/html" href="https://wiki.swarma.org/index.php?title=%E5%88%86%E5%BD%A2%E7%BB%B4%E6%95%B0&amp;diff=17698"/>
		<updated>2020-11-01T10:13:06Z</updated>

		<summary type="html">&lt;p&gt;Ruili：&lt;/p&gt;
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&lt;div&gt;此词条暂由彩云小译翻译，未经人工整理和审校，带来阅读不便，请见谅。&lt;br /&gt;
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{{short description|Invariant}}&lt;br /&gt;
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Example of non-integer dimensions. The first four [[iteration]]s of the [[Koch snowflake|Koch curve]], where after each iteration, all original line segments are replaced with four, each a self-similar copy that is 1/3 the length of the original. One formalism of the Hausdorff dimension uses this scale factor (3) and the number of self-similar objects (4) to calculate the dimension, D, after the first iteration to be D = (log N)/(log S) = (log 4)/(log 3) ≈ 1.26.&amp;lt;ref name=CampbellAnnenberg15&amp;gt;MacGregor Campbell, 2013, &amp;quot;5.6 Scaling and the Hausdorff Dimension,&amp;quot; at ''Annenberg Learner:MATHematics illuminated'', see [http://www.learner.org/courses/mathilluminated/units/5/textbook/06.php], accessed 5 March 2015.&amp;lt;/ref&amp;gt; That is, while the Hausdorff dimension of a single [[point (geometry)|point]] is zero, of a [[line segment]] is 1, of a [[square]] is 2, and of a [[cube]] is 3, for [[fractal]]s such as this, the object can have a non-integer dimension.&lt;br /&gt;
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Example of non-integer dimensions. The first four iterations of the Koch curve, where after each iteration, all original line segments are replaced with four, each a self-similar copy that is 1/3 the length of the original. One formalism of the Hausdorff dimension uses this scale factor (3) and the number of self-similar objects (4) to calculate the dimension, D, after the first iteration to be D = (log N)/(log S) = (log 4)/(log 3) ≈ 1.26. That is, while the Hausdorff dimension of a single point is zero, of a line segment is 1, of a square is 2, and of a cube is 3, for fractals such as this, the object can have a non-integer dimension.&lt;br /&gt;
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非整数维度示例：前四个[[Koch 曲线]]的迭代，在每次迭代后，所有原始线段都被替换为四个，每个自相似的复制是原始线段长度的1 / 3。豪斯多夫维数的一个建模是使用比例因子(3)和自相似对象的数量(4)来计算维度 D，在第一次迭代后为 D = (log N)/(log S) = (log 4)/(log 3) ≈ 1.26.&amp;lt;ref name=CampbellAnnenberg15&amp;gt;。MacGregor Campbell, 2013, &amp;quot;5.6 Scaling and the Hausdorff Dimension,&amp;quot; 在 ''Annenberg Learner:MATHematics illuminated'', 参见 [http://www.learner.org/courses/mathilluminated/units/5/textbook/06.php], accessed 5 March 2015.&amp;lt;/ref&amp;gt; 也就是说，单点的豪斯多夫维数为零，线段为1，正方形为2，立方体为3时，但对于分形，对象可以有一个非整数维度。&lt;br /&gt;
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In [[mathematics]], '''Hausdorff dimension''' is a measure of ''roughness'', or more specifically, [[fractal dimension]], that was first introduced in 1918 by [[mathematician]] [[Felix Hausdorff]].&amp;lt;ref&amp;gt;{{Cite journal |arxiv = 1101.1444|doi = 10.1214/11-STS370|title = Estimators of Fractal Dimension: Assessing the Roughness of Time Series and Spatial Data|journal = Statistical Science|volume = 27|issue = 2|pages = 247–277|year = 2012|last1 = Gneiting|first1 = Tilmann|last2 = Ševčíková|first2 = Hana|last3 = Percival|first3 = Donald B.}}&amp;lt;/ref&amp;gt; For instance, the Hausdorff dimension of a single [[point (geometry)|point]] is zero, of a [[line segment]] is 1, of a [[square]] is 2, and of a [[cube]] is 3. That is, for sets of points that define a smooth shape or a shape that has a small number of corners—the shapes of traditional geometry and science—the Hausdorff dimension is an [[integer]] agreeing with the usual sense of dimension, also known as the [[Inductive dimension|topological dimension]]. However, formulas have also been developed that allow calculation of the dimension of other less simple objects, where, solely on the basis of their properties of [[scaling (geometry)|scaling]] and [[self-similarity]], one is led to the conclusion that particular objects—including [[fractal]]s—have non-integer Hausdorff dimensions. Because of the significant technical advances made by [[Abram Samoilovitch Besicovitch]] allowing computation of dimensions for highly irregular or &amp;quot;rough&amp;quot; sets, this dimension is also commonly referred to as the ''Hausdorff–Besicovitch dimension.''&lt;br /&gt;
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In mathematics, Hausdorff dimension is a measure of roughness, or more specifically, fractal dimension, that was first introduced in 1918 by mathematician Felix Hausdorff. For instance, the Hausdorff dimension of a single point is zero, of a line segment is 1, of a square is 2, and of a cube is 3. That is, for sets of points that define a smooth shape or a shape that has a small number of corners—the shapes of traditional geometry and science—the Hausdorff dimension is an integer agreeing with the usual sense of dimension, also known as the topological dimension. However, formulas have also been developed that allow calculation of the dimension of other less simple objects, where, solely on the basis of their properties of scaling and self-similarity, one is led to the conclusion that particular objects—including fractals—have non-integer Hausdorff dimensions. Because of the significant technical advances made by Abram Samoilovitch Besicovitch allowing computation of dimensions for highly irregular or &amp;quot;rough&amp;quot; sets, this dimension is also commonly referred to as the Hausdorff–Besicovitch dimension.&lt;br /&gt;
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在[[数学]]中，'''&amp;lt;font color = '#ff8000'&amp;gt;豪斯多夫维数Hausdorff dimension&amp;lt;/font&amp;gt;'''是一种粗糙度的度量单位，或者更确切地说，分形维数，是由数学家 Felix Hausdorff 在1918年首次提出的。例如，单点的豪斯多夫维数为零，线段为1，正方形为2，立方体为3。也就是说，对于定义了一个光滑形状或一个有少数几个角的形状---- 传统几何学和科学的形状---- 的点集来说，豪斯多夫维数是一个整数，符合通常的维度意义，也称为拓扑维度。然而，还有一些公式允许计算其他不太简单的对象的维数，其中仅仅根据它们的标度和自相似特性，就可以得出结论: 特定的对象ー包括分形ー具有非整数的 Hausdorff 维数。由于阿布拉姆·萨莫伊洛维奇·贝西科维奇的重大技术进步，允许计算高度不规则或“粗糙”集的维度，这个维度通常也被称为 Hausdorff-Besicovitch 维度。 &lt;br /&gt;
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The Hausdorff dimension, more specifically, is a further dimensional number associated with a given set, where the distances between all members of that set are defined. Such a set is termed a [[metric space]]. The dimension is drawn from the [[Extended real number line|extended real numbers]], &amp;lt;math&amp;gt;\overline{\mathbb{R}}&amp;lt;/math&amp;gt;, as opposed to the more intuitive notion of dimension, which is not associated to general metric spaces, and only takes values in the non-negative integers.&lt;br /&gt;
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The Hausdorff dimension, more specifically, is a further dimensional number associated with a given set, where the distances between all members of that set are defined. Such a set is termed a metric space. The dimension is drawn from the extended real numbers, &amp;lt;math&amp;gt;\overline{\mathbb{R}}&amp;lt;/math&amp;gt;, as opposed to the more intuitive notion of dimension, which is not associated to general metric spaces, and only takes values in the non-negative integers.&lt;br /&gt;
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更具体地说，豪斯多夫维数是一个与给定集合相关联的更进一步的维数，其中定义了该集合所有成员之间的距离。这样的集合称为度量空间。维数是从扩展的实数，&amp;lt;math&amp;gt;\overline{\mathbb{R}}&amp;lt;/math&amp;gt;，而不是更直观的维数概念(它不与一般的度量空间相关联，只取非负整数的值)。&lt;br /&gt;
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In mathematical terms, the Hausdorff dimension generalizes the notion of the dimension of a real [[vector space]]. That is, the Hausdorff dimension of an ''n''-dimensional [[inner product space]] equals ''n''. This underlies the earlier statement that the Hausdorff dimension of a point is zero, of a line is one, etc., and that [[fractal|irregular sets]] can have noninteger Hausdorff dimensions. For instance, the [[Koch snowflake]] shown at right is constructed from an equilateral triangle; in each iteration, its component line segments are divided into 3 segments of unit length, the newly created middle segment is used as the base of a new [[equilateral]] triangle that points outward, and this base segment is then deleted to leave a final object from the iteration of unit length of 4.&amp;lt;ref&amp;gt;Larry Riddle, 2014, &amp;quot;Classic Iterated Function Systems: Koch Snowflake&amp;quot;, Agnes Scott College e-Academy (online), see [http://ecademy.agnesscott.edu/~lriddle/ifs/ksnow/ksnow.htm], accessed 5 March 2015.&amp;lt;/ref&amp;gt; That is, after the first iteration, each original line segment has been replaced with N=4, where each self-similar copy is 1/S = 1/3 as long as the original.&amp;lt;ref name=CampbellAnnenberg15/&amp;gt; Stated another way, we have taken an object with Euclidean dimension, D, and reduced its linear scale by 1/3 in each direction, so that its length increases to N=S&amp;lt;sup&amp;gt;D&amp;lt;/sup&amp;gt;.&amp;lt;ref name=ClaytonSCTPLS96&amp;gt;Keith Clayton, 1996, &amp;quot;Fractals and the Fractal Dimension,&amp;quot; ''Basic Concepts in Nonlinear Dynamics and Chaos'' (workshop), Society for Chaos Theory in Psychology and the Life Sciences annual meeting, June 28, 1996, Berkeley, California, see [http://www.vanderbilt.edu/AnS/psychology/cogsci/chaos/workshop/Workshop.html], accessed 5 March 2015.&amp;lt;/ref&amp;gt; This equation is easily solved for D, yielding the ratio of logarithms (or [[natural logarithm]]s) appearing in the figures, and giving—in the Koch and other fractal cases—non-integer dimensions for these objects.&lt;br /&gt;
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In mathematical terms, the Hausdorff dimension generalizes the notion of the dimension of a real vector space. That is, the Hausdorff dimension of an n-dimensional inner product space equals n. This underlies the earlier statement that the Hausdorff dimension of a point is zero, of a line is one, etc., and that irregular sets can have noninteger Hausdorff dimensions. For instance, the Koch snowflake shown at right is constructed from an equilateral triangle; in each iteration, its component line segments are divided into 3 segments of unit length, the newly created middle segment is used as the base of a new equilateral triangle that points outward, and this base segment is then deleted to leave a final object from the iteration of unit length of 4. That is, after the first iteration, each original line segment has been replaced with N=4, where each self-similar copy is 1/S = 1/3 as long as the original. This equation is easily solved for D, yielding the ratio of logarithms (or natural logarithms) appearing in the figures, and giving—in the Koch and other fractal cases—non-integer dimensions for these objects.&lt;br /&gt;
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用数学术语来说，豪斯多夫维数概括了实向量空间维数的概念。也就是说，n 维内积空间的豪斯多夫维数等于 n。 这就是早期假设的基础，一个点的豪斯多夫维数是零，一条线是一等等，不规则集可以有非整数的豪斯多夫维数。例如，右边所示的 Koch 雪花是由一个正三角形构成的; 在每次迭代中，它的组成线段被分成单位长度的3段，新创建的中间线段被用作一个指向外部的新正三角形的基础，然后人们删除这个基础线段用来保留单位长度4的迭代中的最终对象。也就是说，在第一次迭代之后，每个原始线段都被替换为 N=4，其中每个自相似拷贝的长度是原始线段的1/S = 1/3 。这个方程很容易求解为 D，产生出现在图形中的对数(或自然对数)的比率，并给出——在 Koch 和其他分形情况下——这些对象的非整数维数。&lt;br /&gt;
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The Hausdorff dimension is a successor to the simpler, but usually equivalent, box-counting or [[Minkowski–Bouligand dimension]].&lt;br /&gt;
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The Hausdorff dimension is a successor to the simpler, but usually equivalent, box-counting or Minkowski–Bouligand dimension.&lt;br /&gt;
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豪斯多夫维数是更简单但通常等价的'''&amp;lt;font color = '#ff8000'&amp;gt;计盒维数box-counting&amp;lt;/font&amp;gt;'''或'''&amp;lt;font color = '#ff8000'&amp;gt;闵可夫斯基维数Minkowski-Bouligand&amp;lt;/font&amp;gt;'''的继承者。&lt;br /&gt;
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==Intuition概念==&lt;br /&gt;
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{{refimprove section|date=March 2015}}&lt;br /&gt;
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The intuitive concept of dimension of a geometric object ''X'' is the number of independent parameters one needs to pick out a unique point inside. However, any point specified by two parameters can be instead specified by one, because the [[cardinality]] of the [[real plane]] is equal to the cardinality of the [[real line]] (this can be seen by an [[Cantor's diagonal argument|argument]] involving interweaving the digits of two numbers to yield a single number encoding the same information). The example of a [[space-filling curve]] shows that one can even map the real line to the real plane [[Surjective function|surjectively]] (taking one real number into a pair of real numbers in a way so that all pairs of numbers are covered) and ''continuously'', so that a one-dimensional object completely fills up a higher-dimensional object.&lt;br /&gt;
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The intuitive concept of dimension of a geometric object X is the number of independent parameters one needs to pick out a unique point inside. However, any point specified by two parameters can be instead specified by one, because the cardinality of the real plane is equal to the cardinality of the real line (this can be seen by an argument involving interweaving the digits of two numbers to yield a single number encoding the same information). The example of a space-filling curve shows that one can even map the real line to the real plane surjectively (taking one real number into a pair of real numbers in a way so that all pairs of numbers are covered) and continuously, so that a one-dimensional object completely fills up a higher-dimensional object.&lt;br /&gt;
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几何对象X的尺寸的直观概念是指需要多少个独立参数才能找到一个独特的点。但是，任何由两个参数指定的点都可以由一个参数指定，因为为实平面的基数等于实线的基数(这可以通过交织两个数字以产生一个编码相同信息的单个数字看到)。'''&amp;lt;font color = '#ff8000'&amp;gt;皮亚诺曲线&amp;lt;/font&amp;gt;'''的例子表明，可以将实线完美和连续地映射到实平面(把一个实数转换成一对实数，从而覆盖所有实数对)，由此一维对象完全填充了一个高维对象。&lt;br /&gt;
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Every space filling curve hits some points multiple times, and does not have a continuous inverse. It is impossible to map two dimensions onto one in a way that is continuous and continuously invertible. The topological dimension, also called [[Lebesgue covering dimension]], explains why. This dimension is ''n'' if, in every covering of ''X'' by small open balls, there is at least one point where ''n''&amp;amp;nbsp;+&amp;amp;nbsp;1 balls overlap. For example, when one covers a line with short open intervals, some points must be covered twice, giving dimension&amp;amp;nbsp;''n''&amp;amp;nbsp;=&amp;amp;nbsp;1.&lt;br /&gt;
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Every space filling curve hits some points multiple times, and does not have a continuous inverse. It is impossible to map two dimensions onto one in a way that is continuous and continuously invertible. The topological dimension, also called Lebesgue covering dimension, explains why. This dimension is n if, in every covering of X by small open balls, there is at least one point where n&amp;amp;nbsp;+&amp;amp;nbsp;1 balls overlap. For example, when one covers a line with short open intervals, some points must be covered twice, giving dimension&amp;amp;nbsp;n&amp;amp;nbsp;=&amp;amp;nbsp;1.&lt;br /&gt;
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每条空间填充曲线都会多次击中某些点，且不存在连续的逆。将二维以连续和连续可逆的方式映射到一维是不可能的。'''&amp;lt;font color = '#ff8000'&amp;gt;拓扑维度 topological dimension&amp;lt;/font&amp;gt;'''，也被称为Lebesgue覆盖维数，解释了为什么。如果在 x 的每个小开球覆盖中，至少有一个点 n + 1个球重叠，这个维度是 n。例如，当用短的开区间覆盖一条线时，某些点必须被覆盖两次，给出维数''n''&amp;amp;nbsp;=&amp;amp;nbsp;1。&lt;br /&gt;
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But topological dimension is a very crude measure of the local size of a space (size near a point). A curve that is almost space-filling can still have topological dimension one, even if it fills up most of the area of a region. A [[fractal]] has an integer topological dimension, but in terms of the amount of space it takes up, it behaves like a higher-dimensional space.&lt;br /&gt;
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But topological dimension is a very crude measure of the local size of a space (size near a point). A curve that is almost space-filling can still have topological dimension one, even if it fills up most of the area of a region. A fractal has an integer topological dimension, but in terms of the amount of space it takes up, it behaves like a higher-dimensional space.&lt;br /&gt;
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但是，拓扑维度是对空间局部尺寸(点附近的尺寸)的一个非常粗略的度量。一条几乎是空间填充的曲线仍然可以有一维拓扑，即使它填充了一个区域的大部分面积。分形具有整数的拓扑维数，但就其所占的空间量而言，它看起来像一个更高维的空间。&lt;br /&gt;
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The Hausdorff dimension measures the local size of a space taking into account the distance between points, the [[metric space|metric]]. Consider the number ''N''(''r'') of [[ball (mathematics)|balls]] of radius at most ''r'' required to cover ''X'' completely. When ''r'' is very small, ''N''(''r'') grows polynomially with 1/''r''. For a sufficiently well-behaved  ''X'', the Hausdorff dimension is the unique number ''d'' such that N(''r'') grows as 1/''r&amp;lt;sup&amp;gt;d&amp;lt;/sup&amp;gt;'' as ''r'' approaches zero. More precisely, this defines the [[Minkowski–Bouligand dimension|box-counting dimension]], which equals the Hausdorff dimension when the value ''d'' is a critical boundary between growth rates that are insufficient to cover the space, and growth rates that are overabundant.&lt;br /&gt;
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The Hausdorff dimension measures the local size of a space taking into account the distance between points, the metric. Consider the number N(r) of balls of radius at most r required to cover X completely. When r is very small, N(r) grows polynomially with 1/r. For a sufficiently well-behaved  X, the Hausdorff dimension is the unique number d such that N(r) grows as 1/r&amp;lt;sup&amp;gt;d&amp;lt;/sup&amp;gt; as r approaches zero. More precisely, this defines the box-counting dimension, which equals the Hausdorff dimension when the value d is a critical boundary between growth rates that are insufficient to cover the space, and growth rates that are overabundant.&lt;br /&gt;
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豪斯多夫维数测量一个空间的局部大小时，会考虑到点之间距离的度量。考虑半径最大为 r 的球数 ''N'' (r) ，需要完全覆盖 ''X''。当 r 很小时，n (r)以1/''r'' 增长多项式。对于一个表现足够好的 ''X''，豪斯多夫维数是唯一的数 d，这样当 r 趋近于零时， N(r)增长为1/r&amp;lt;sup&amp;gt;d&amp;lt;/sup&amp;gt; 。更确切地说，这定义了盒子计数维度，当值 d 是不足以覆盖空间的增长率和过度充裕的增长率之间的关键边界时，它等于豪斯多夫维数。&lt;br /&gt;
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For shapes that are smooth, or shapes with a small number of corners, the shapes of traditional geometry and science, the Hausdorff dimension is an integer agreeing with the topological dimension. But [[Benoit Mandelbrot]] observed that [[fractal]]s, sets with noninteger Hausdorff dimensions, are found everywhere in nature. He observed that the proper idealization of most rough shapes you see around you is not in terms of smooth idealized shapes, but in terms of fractal idealized shapes:&lt;br /&gt;
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For shapes that are smooth, or shapes with a small number of corners, the shapes of traditional geometry and science, the Hausdorff dimension is an integer agreeing with the topological dimension. But Benoit Mandelbrot observed that fractals, sets with noninteger Hausdorff dimensions, are found everywhere in nature. He observed that the proper idealization of most rough shapes you see around you is not in terms of smooth idealized shapes, but in terms of fractal idealized shapes:&lt;br /&gt;
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对于光滑的形状，或者有少量棱角的形状，传统几何和科学的形状，豪斯多夫维数是一个整数，与拓扑维度一致。但是伯努·曼德布洛特观察到分形---- 具有非整数豪斯多夫维数的集合---- 在自然界中随处可见。他观察到，我们周围大多数粗糙形状的理想化不是光滑的理想化形状，而是分形理想化形状:&lt;br /&gt;
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&amp;lt;blockquote&amp;gt;Clouds are not spheres, mountains are not cones, coastlines are not circles, and bark is not smooth, nor does lightning travel in a straight line.&amp;lt;ref name=&amp;quot;mandelbrot&amp;quot;&amp;gt;{{cite book   | last = Mandelbrot   | first = Benoît   | authorlink = Benoit Mandelbrot   | title = The Fractal Geometry of Nature   | publisher = W. H. Freeman   | series = Lecture notes in mathematics 1358   | year = 1982   | doi =    | isbn = 0-7167-1186-9   | url-access = registration   | url = https://archive.org/details/fractalgeometryo00beno   }}&amp;lt;/ref&amp;gt;&amp;lt;/blockquote&amp;gt;&lt;br /&gt;
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&amp;lt;blockquote&amp;gt;Clouds are not spheres, mountains are not cones, coastlines are not circles, and bark is not smooth, nor does lightning travel in a straight line.&amp;lt;/blockquote&amp;gt;&lt;br /&gt;
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&amp;lt;blockquote&amp;gt;云不是球体，山不是锥体，海岸线不是圆圈，树皮不平滑，闪电也不是直线运动。 &amp;lt;/blockquote&amp;gt;&lt;br /&gt;
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For fractals that occur in nature, the Hausdorff and [[Minkowski–Bouligand dimension|box-counting dimension]] coincide. The [[packing dimension]] is yet another similar notion which gives the same value for many shapes, but there are well documented exceptions where all these dimensions differ.&lt;br /&gt;
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For fractals that occur in nature, the Hausdorff and box-counting dimension coincide. The packing dimension is yet another similar notion which gives the same value for many shapes, but there are well documented exceptions where all these dimensions differ.&lt;br /&gt;
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对于自然界中出现的分形，豪斯多夫维数和盒计数维数是一致的。封装尺寸是另一个类似的概念，它给出了许多形状相同的值，但是在所有这些尺寸不同的情况，都做了很好的说明。&lt;br /&gt;
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==Formal definitions形式化定义==&lt;br /&gt;
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{{unreferenced section|date=March 2015}}&lt;br /&gt;
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===Hausdorff content豪斯多夫集===&lt;br /&gt;
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Let ''X'' be a [[metric space]]. If ''S'' ⊂ ''X'' and ''d'' ∈ [0, ∞), the ''d''-dimensional '''unlimited Hausdorff content''' of ''S'' is defined by&lt;br /&gt;
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Let X be a metric space. If S ⊂ X and d ∈ [0, ∞), the d-dimensional unlimited Hausdorff content of S is defined by&lt;br /&gt;
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设 ''X''是度量空间。若''S'' ⊂ ''X'' 和 ''d'' ∈ [0, ∞) ，则 ''S'' 的''d''维无限 豪斯多夫集定义为&lt;br /&gt;
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:&amp;lt;math&amp;gt;C_H^d(S):=\inf\Bigl\{\sum_i r_i^d:\text{ there is a cover of } S\text{ by balls with radii }r_i&amp;gt;0\Bigr\}.&amp;lt;/math&amp;gt;&lt;br /&gt;
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&amp;lt;math&amp;gt;C_H^d(S):=\inf\Bigl\{\sum_i r_i^d:\text{ there is a cover of } S\text{ by balls with radii }r_i&amp;gt;0\Bigr\}.&amp;lt;/math&amp;gt;&lt;br /&gt;
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&amp;lt;math&amp;gt;C_H^d(S):=\inf\Bigl\{\sum_i r_i^d:\text{ there is a cover of } S\text{ by balls with radii }r_i&amp;gt;0\Bigr\}.&amp;lt;/math&amp;gt;&lt;br /&gt;
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In other words, &amp;lt;math&amp;gt;C_H^d(S)&amp;lt;/math&amp;gt; is the [[infimum]] of the set of numbers &amp;lt;math&amp;gt;\delta \geq 0&amp;lt;/math&amp;gt; such that there is some (indexed) collection of [[ball (mathematics)|ball]]s &amp;lt;math&amp;gt;\{B(x_i,r_i):i\in I\}&amp;lt;/math&amp;gt; covering ''S'' with ''r&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;''&amp;amp;nbsp;&amp;gt;&amp;amp;nbsp;0 for each ''i''&amp;amp;nbsp;∈&amp;amp;nbsp;''I'' that satisfies &amp;lt;math&amp;gt;\sum_{i\in I} r_i^d&amp;lt;\delta &amp;lt;/math&amp;gt;. (Here, we use the standard convention that [[infimum|inf&amp;amp;nbsp;Ø&amp;amp;nbsp;=&amp;amp;nbsp;∞]].)&lt;br /&gt;
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In other words, &amp;lt;math&amp;gt;C_H^d(S)&amp;lt;/math&amp;gt; is the infimum of the set of numbers &amp;lt;math&amp;gt;\delta \geq 0&amp;lt;/math&amp;gt; such that there is some (indexed) collection of balls &amp;lt;math&amp;gt;\{B(x_i,r_i):i\in I\}&amp;lt;/math&amp;gt; covering S with r&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;&amp;amp;nbsp;&amp;gt;&amp;amp;nbsp;0 for each i&amp;amp;nbsp;∈&amp;amp;nbsp;I that satisfies &amp;lt;math&amp;gt;\sum_{i\in I} r_i^d&amp;lt;\delta &amp;lt;/math&amp;gt;. (Here, we use the standard convention that inf&amp;amp;nbsp;Ø&amp;amp;nbsp;=&amp;amp;nbsp;∞.)&lt;br /&gt;
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换句话说，&amp;lt;math&amp;gt;C_H^d(S)&amp;lt;/math&amp;gt; 是数字集合&amp;lt;math&amp;gt;\delta \geq 0&amp;lt;/math&amp;gt;的下确界，使得在 ''i''&amp;amp;nbsp;∈&amp;amp;nbsp中存在一些球集合 &amp;lt;math&amp;gt;\{B(x_i,r_i):i\in I\}&amp;lt;/math&amp;gt;  i 包含 s，对于每个 ''r&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;''&amp;amp;nbsp;&amp;gt;&amp;amp;nbsp;0 满足 i 中的和&amp;lt;math&amp;gt;\sum_{i\in I} r_i^d&amp;lt;\delta &amp;lt;/math&amp;gt; (在这里，我们使用inf&amp;amp;nbsp;Ø&amp;amp;nbsp;=&amp;amp;nbsp;∞ )的标准约定。&lt;br /&gt;
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===Hausdorff measurement豪斯多夫分形测量===&lt;br /&gt;
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The Hausdorff outer measure is different from the unbounded Hausdorf content in that rather than considering all possible coverings of ''S'', we see what happens when the sizes of the balls go to zero. This is  for &amp;lt;math&amp;gt;d \geq 0 &amp;lt;/math&amp;gt;, we define the ''d''-dimensional Hausdorff outer measure of ''S'' as&lt;br /&gt;
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The Hausdorff outer measure is different from the unbounded Hausdorf content in that rather than considering all possible coverings of S, we see what happens when the sizes of the balls go to zero. This is  for &amp;lt;math&amp;gt;d \geq 0 &amp;lt;/math&amp;gt;, we define the d-dimensional Hausdorff outer measure of S as&lt;br /&gt;
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豪斯多夫外测度不同于无界的豪斯多夫，因为我们不考虑 s 的所有可能，我们看到当球的大小为零时会发生什么。这是为了数学  &amp;lt;math&amp;gt;d \geq 0 &amp;lt;/math&amp;gt;，我们定义了  ''S''的 ''d''维豪斯多夫Hausdorff 外测度为&lt;br /&gt;
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:&amp;lt;math&amp;gt; \mathcal{H}^d(S):=\lim_{r \to 0} \inf\Bigl\{\sum_i r_i^d:\text{ there is a cover of } S\text{ by balls with radii } 0 &amp;lt; r_i &amp;lt; r\Bigr\}.&amp;lt;/math&amp;gt;&lt;br /&gt;
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&amp;lt;math&amp;gt; \mathcal{H}^d(S):=\lim_{r \to 0} \inf\Bigl\{\sum_i r_i^d:\text{ there is a cover of } S\text{ by balls with radii } 0 &amp;lt; r_i &amp;lt; r\Bigr\}.&amp;lt;/math&amp;gt;&lt;br /&gt;
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&amp;lt;math&amp;gt; \mathcal{H}^d(S):=\lim_{r \to 0} \inf\Bigl\{\sum_i r_i^d:\text{有一个面} S\text{ 球 } 0 &amp;lt; r_i &amp;lt; r\Bigr\}.&amp;lt;/math&amp;gt;&lt;br /&gt;
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===Hausdorff dimension豪斯多夫维数===&lt;br /&gt;
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The '''Hausdorff dimension''' of ''X'' is defined by&lt;br /&gt;
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The Hausdorff dimension of X is defined by&lt;br /&gt;
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X 的豪斯多夫维数定义为&lt;br /&gt;
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:&amp;lt;math&amp;gt;\dim_{\operatorname{H}}(X):=\inf\{d\ge 0: \mathcal{H}^d(X)=0\}.&amp;lt;/math&amp;gt;&lt;br /&gt;
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&amp;lt;math&amp;gt;\dim_{\operatorname{H}}(X):=\inf\{d\ge 0: \mathcal{H}^d(X)=0\}.&amp;lt;/math&amp;gt;&lt;br /&gt;
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Equivalently, dim&amp;lt;sub&amp;gt;H&amp;lt;/sub&amp;gt;(''X'') may be defined as the [[infimum]] of the set of ''d'' ∈ [0, ∞) such that the ''d''-dimensional [[Hausdorff measure]] of ''X'' is zero. This is the same as the supremum of the set of ''d''&amp;amp;nbsp;∈&amp;amp;nbsp;[0,&amp;amp;nbsp;∞) such that the ''d''-dimensional Hausdorff measure of ''X'' is infinite (except that when this latter set of numbers ''d'' is empty the Hausdorff dimension is zero).&lt;br /&gt;
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Equivalently, dim&amp;lt;sub&amp;gt;H&amp;lt;/sub&amp;gt;(X) may be defined as the infimum of the set of d ∈ [0, ∞) such that the d-dimensional Hausdorff measure of X is zero. This is the same as the supremum of the set of d&amp;amp;nbsp;∈&amp;amp;nbsp;[0,&amp;amp;nbsp;∞) such that the d-dimensional Hausdorff measure of X is infinite (except that when this latter set of numbers d is empty the Hausdorff dimension is zero).&lt;br /&gt;
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等价地，dim &amp;lt;sub&amp;gt;H&amp;lt;/sub&amp;gt;(''X'')可定义为 ''d'' ∈ [0, ∞) 集的下确界，使得''X'' 的''d''-维 [[豪斯多夫测度]] 为零。这与 ''d''&amp;amp;nbsp;∈&amp;amp;nbsp;[0,&amp;amp;nbsp;∞)的集合的上确界相同，因此''X''的 d 维豪斯多夫测度是无限的(除非后一个集合 ''d'' 是空的，豪斯多夫维数为零)。&lt;br /&gt;
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==Examples实例==&lt;br /&gt;
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[[Image:Sierpinski deep.svg|thumb|250px|Dimension of a further [[fractal]] example. The [[Sierpinski triangle]], an object with Hausdorff dimension of log(3)/log(2)≈1.58.&amp;lt;ref name=ClaytonSCTPLS96/&amp;gt;]]&lt;br /&gt;
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Dimension of a further [[fractal example. The Sierpinski triangle, an object with Hausdorff dimension of log(3)/log(2)≈1.58.]]&lt;br /&gt;
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[[Image:谢尔宾斯基三角形 deep.svg|thumb|250px|进一步的[[分形维数]]的例子，进一步的分形维数的例子是谢尔宾斯基三角形，它是一个豪斯多夫维数为log(3)/log(2)≈1.58.&amp;lt;ref name=ClaytonSCTPLS96/&amp;gt;的物体]]&lt;br /&gt;
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* [[Countable set]]s have Hausdorff dimension 0.&amp;lt;ref name=&amp;quot;schleicher&amp;quot;&amp;gt;{{cite journal |last1=Schleicher |first1=Dierk |title=Hausdorff Dimension, Its Properties, and Its Surprises |journal=The American Mathematical Monthly |date=June 2007 |volume=114 |issue=6 |pages=509–528 |doi=10.1080/00029890.2007.11920440 |language=en |issn=0002-9890|arxiv=math/0505099 }}&amp;lt;/ref&amp;gt;&lt;br /&gt;
*[[可数集]]拥有豪斯多夫维数0.&amp;lt;ref name=&amp;quot;schleicher&amp;quot;&amp;gt;{{cite journal |last1=Schleicher |first1=Dierk |title=豪斯多夫维数, Its Properties, and Its Surprises |journal=The American Mathematical Monthly美国数学期刊 |date=June 2007 |volume=114 |issue=6 |pages=509–528 |doi=10.1080/00029890.2007.11920440 |language=en |issn=0002-9890|arxiv=math/0505099 }}&amp;lt;/ref&amp;gt;&lt;br /&gt;
* The [[Euclidean space]] ℝ&amp;lt;sup&amp;gt;''n''&amp;lt;/sup&amp;gt; has Hausdorff dimension ''n'', and the circle '''S'''&amp;lt;sup&amp;gt;1&amp;lt;/sup&amp;gt; has Hausdorff dimension 1.&amp;lt;ref name=&amp;quot;schleicher&amp;quot; /&amp;gt;&lt;br /&gt;
*[[教育空间]] ℝ&amp;lt;sup&amp;gt;''n''&amp;lt;/sup&amp;gt; 有豪斯多夫维数 ''n''，循环'''S'''&amp;lt;sup&amp;gt;1&amp;lt;/sup&amp;gt; 拥有豪斯多夫维数1.&amp;lt;ref name=&amp;quot;schleicher&amp;quot; /&amp;gt;&lt;br /&gt;
* [[Fractal]]s often are spaces whose Hausdorff dimension strictly exceeds the [[topological dimension]].&amp;lt;ref name=&amp;quot;mandelbrot&amp;quot; /&amp;gt; For example, the [[Cantor set]], a zero-dimensional topological space, is a union of two copies of itself, each copy shrunk by a factor 1/3; hence, it can be shown that its Hausdorff dimension is ln(2)/ln(3)&amp;amp;nbsp;≈&amp;amp;nbsp;0.63.&amp;lt;ref&amp;gt;{{cite book | last=Falconer | first = Kenneth |title=Fractal Geometry: Mathematical Foundations and Applications | publisher=[[John Wiley and Sons]] | edition=2nd | year=2003}}&amp;lt;/ref&amp;gt; The [[Sierpinski triangle]] is a union of three copies of itself, each copy shrunk by a factor of&amp;amp;nbsp;1/2; this yields a Hausdorff dimension of ln(3)/ln(2)&amp;amp;nbsp;≈&amp;amp;nbsp;1.58.&amp;lt;ref name=CampbellAnnenberg15/&amp;gt; These Hausdorff dimensions are related to the &amp;quot;critical exponent&amp;quot; of the [[Master theorem (analysis of algorithms)|Master theorem]] for solving [[Recurrence relation|recurrence relations]] in the [[analysis of algorithms]].&lt;br /&gt;
*[[分形]]一般是那些豪斯多夫维数直接超过其拓扑维数的空间。例如[[康托尔集]]是一个o维拓扑空间，由两个自己复制而成，每一个复制品都是原来的三分之一，因此它的豪斯多夫维数是 ln(2)/ln(3)&amp;amp;nbsp;≈&amp;amp;nbsp;0.63。&amp;lt;ref&amp;gt;{{cite book | last=Falconer | first = Kenneth |title=Fractal Geometry: Mathematical Foundations and Applications | publisher=[[John Wiley and Sons]] | edition=2nd | year=2003}}&amp;lt;/ref&amp;gt;一个[[谢尔宾斯基三角]]是他自身三个复制的组合。每一个是原来的&amp;amp;nbsp;1/2，它的豪斯多夫维数ln(3)/ln(2)&amp;amp;nbsp;≈&amp;amp;nbsp;1.58。&amp;lt;ref name=CampbellAnnenberg15/&amp;gt;在递归算法中解决递归关系时，这些豪斯多夫维数与[[算法分析主定理]]的临界指标相联系。&lt;br /&gt;
* [[Space-filling curve]]s like the [[Peano curve]] have the same Hausdorff dimension as the space they fill.&lt;br /&gt;
*[[空间填充曲线]]拥有和他们填充空间同样的豪斯多夫维数，如[[皮亚诺曲线]]。&lt;br /&gt;
* The trajectory of [[Brownian motion]] in dimension 2 and above is conjectured to be Hausdorff dimension 2.&amp;lt;ref&amp;gt;{{cite book | last=Morters | first=Peres | title= Brownian Motion | publisher=[[Cambridge University Press]] | year=2010 }}&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
[[image:Great Britain Hausdorff.svg|thumb|250px|Estimating the Hausdorff dimension of the [[How Long Is the Coast of Britain? Statistical Self-Similarity and Fractional Dimension|coast of Great Britain]]]]&lt;br /&gt;
&lt;br /&gt;
coast of Great Britain]]&lt;br /&gt;
&lt;br /&gt;
[[大不列颠海岸&lt;br /&gt;
&lt;br /&gt;
* 刘易斯·弗赖伊·理查森[[Lewis Fry Richardson]] has performed detailed experiments to measure the approximate Hausdorff dimension for various coastlines. His results have varied from 1.02 for the coastline of [[South Africa]] to 1.25 for the west coast of [[Great Britain]].&amp;lt;ref name=&amp;quot;mandelbrot&amp;quot; /&amp;gt;&lt;br /&gt;
*刘易斯·弗赖伊·理查森（Lewis Fry Richardson）已经通过豪斯多夫维数去测量了很多海岸线。它的结果涵盖从1.02的南非海岸线到1.25的大英帝国西海岸模型。]]&lt;br /&gt;
&lt;br /&gt;
==Properties of Hausdorff dimension豪斯多夫维数特性==&lt;br /&gt;
&lt;br /&gt;
{{refimprove section|date=March 2015}}&lt;br /&gt;
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&lt;br /&gt;
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=== Hausdorff dimension and inductive dimension 豪斯多夫维数和归纳维数===&lt;br /&gt;
&lt;br /&gt;
Let ''X'' be an arbitrary [[Separable space|separable]] metric space. There is a [[topology|topological]] notion of [[inductive dimension]] for ''X'' which is defined recursively. It is always an integer (or +∞) and is denoted dim&amp;lt;sub&amp;gt;ind&amp;lt;/sub&amp;gt;(''X'').&lt;br /&gt;
&lt;br /&gt;
Let X be an arbitrary separable metric space. There is a topological notion of inductive dimension for X which is defined recursively. It is always an integer (or +∞) and is denoted dim&amp;lt;sub&amp;gt;ind&amp;lt;/sub&amp;gt;(X).&lt;br /&gt;
&lt;br /&gt;
设''X'' 是[[任意可分度量空间]]。对于''X'' 有一个递归定义的归纳维数拓扑概念。它总是一个整数(或 + ∞) ，并且表示dim&amp;lt;sub&amp;gt;ind&amp;lt;/sub&amp;gt;(''X'')。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
'''Theorem'''. Suppose ''X'' is non-empty. Then &lt;br /&gt;
&lt;br /&gt;
Theorem. Suppose X is non-empty. Then &lt;br /&gt;
&lt;br /&gt;
'''定理'''：假设''X'' 是非空的。那么&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt; \dim_{\mathrm{Haus}}(X) \geq \dim_{\operatorname{ind}}(X). &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \dim_{\mathrm{Haus}}(X) \geq \dim_{\operatorname{ind}}(X). &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Moreover,&lt;br /&gt;
&lt;br /&gt;
Moreover,&lt;br /&gt;
&lt;br /&gt;
此外,&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \inf_Y \dim_{\operatorname{Haus}}(Y) =\dim_{\operatorname{ind}}(X), &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \inf_Y \dim_{\operatorname{Haus}}(Y) =\dim_{\operatorname{ind}}(X), &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
where ''Y'' ranges over metric spaces [[homeomorphic]] to ''X''. In other words, ''X'' and ''Y'' have the same underlying set of points and the metric ''d''&amp;lt;sub&amp;gt;''Y''&amp;lt;/sub&amp;gt; of ''Y'' is topologically equivalent to ''d''&amp;lt;sub&amp;gt;''X''&amp;lt;/sub&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
where Y ranges over metric spaces homeomorphic to X. In other words, X and Y have the same underlying set of points and the metric d&amp;lt;sub&amp;gt;Y&amp;lt;/sub&amp;gt; of Y is topologically equivalent to d&amp;lt;sub&amp;gt;X&amp;lt;/sub&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
其中''Y''是度量空间同胚到 ''X''的范围。换句话说， ''X''和 ''Y''具有相同的基本点集，''Y''的度规''d''&amp;lt;sub&amp;gt;''Y''&amp;lt;/sub&amp;gt; 的子拓扑等价于''d''&amp;lt;sub&amp;gt;''X''&amp;lt;/sub&amp;gt;。&lt;br /&gt;
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&lt;br /&gt;
&lt;br /&gt;
These results were originally established by [[Edward Szpilrajn]] (1907–1976), e.g., see Hurewicz and Wallman, Chapter VII.{{full citation needed|date=March 2015}}&lt;br /&gt;
&lt;br /&gt;
These results were originally established by Edward Szpilrajn (1907–1976), e.g., see Hurewicz and Wallman, Chapter VII.&lt;br /&gt;
&lt;br /&gt;
这些结果最初是由 [[Edward Szpilrajn]] (1907–1976)建立的,  参见 Hurewicz and Wallman, Chapter VII.{{full citation needed|date=March 2015}}第七章。&lt;br /&gt;
&lt;br /&gt;
=== Hausdorff dimension and Minkowski dimension 豪斯多夫维数和闵可夫斯基维度===&lt;br /&gt;
&lt;br /&gt;
The [[Minkowski dimension]] is similar to, and at least as large as, the Hausdorff dimension, and they are equal in many situations. However, the set of [[rational number|rational]] points in [0, 1] has Hausdorff dimension zero and Minkowski dimension one. There are also compact sets for which the Minkowski dimension is strictly larger than the Hausdorff dimension.&lt;br /&gt;
&lt;br /&gt;
The Minkowski dimension is similar to, and at least as large as, the Hausdorff dimension, and they are equal in many situations. However, the set of rational points in [0, 1] has Hausdorff dimension zero and Minkowski dimension one. There are also compact sets for which the Minkowski dimension is strictly larger than the Hausdorff dimension.&lt;br /&gt;
&lt;br /&gt;
[[闵可夫斯基维数]]与豪斯多夫维数相似，至少和它一样大，而且在许多情况下是相等的。然而，[0,1]中有理点集的豪斯多夫维数为0，闵可夫斯基维数为1。还有一些紧集的闵可夫斯基维数绝对大于豪斯多夫维数。&lt;br /&gt;
&lt;br /&gt;
=== Hausdorff dimensions and Frostman measures 豪斯多夫维度和弗洛斯曼测度===&lt;br /&gt;
&lt;br /&gt;
If there is a [[measure (mathematics)|measure]] μ defined on [[Borel measure|Borel]] subsets of a metric space ''X'' such that ''μ''(''X'') &amp;gt; 0 and ''μ''(''B''(''x'', ''r'')) ≤ ''r&amp;lt;sup&amp;gt;s&amp;lt;/sup&amp;gt;'' holds for some constant ''s'' &amp;gt; 0 and for every ball ''B''(''x'', ''r'') in ''X'', then dim&amp;lt;sub&amp;gt;Haus&amp;lt;/sub&amp;gt;(''X'') ≥ ''s''. A partial converse is provided by [[Frostman's lemma]].{{citation needed|date=March 2015}}&amp;lt;ref&amp;gt;This Wikipedia article also discusses further useful characterizations of the Hausdorff dimension.{{clarify|date=March 2015}}&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
If there is a measure μ defined on Borel subsets of a metric space X such that μ(X) &amp;gt; 0 and μ(B(x, r)) ≤ r&amp;lt;sup&amp;gt;s&amp;lt;/sup&amp;gt; holds for some constant s &amp;gt; 0 and for every ball B(x, r) in X, then dim&amp;lt;sub&amp;gt;Haus&amp;lt;/sub&amp;gt;(X) ≥ s. A partial converse is provided by Frostman's lemma.&lt;br /&gt;
&lt;br /&gt;
如果在度量空间 ''X'' 的 Borel 子集上定义一个测度 μ，使得''μ''(''X'') &amp;gt; 0 和''μ''(''B''(''x'', ''r'')) ≤ ''r&amp;lt;sup&amp;gt;s&amp;lt;/sup&amp;gt;''，对于某个常数 ''s'' &amp;gt; 0  和 ''X'' 中的每个球 ''B''(''x'', ''r'') 成立，则 dim&amp;lt;sub&amp;gt;Haus&amp;lt;/sub&amp;gt;(''X'') ≥ ''s'' 。 部分逆向转换由弗洛斯曼引理定义。&lt;br /&gt;
&lt;br /&gt;
=== Behaviour under unions and products ===&lt;br /&gt;
&lt;br /&gt;
If &amp;lt;math&amp;gt;X=\bigcup_{i\in I}X_i&amp;lt;/math&amp;gt; is a finite or countable union, then&lt;br /&gt;
&lt;br /&gt;
If &amp;lt;math&amp;gt;X=\bigcup_{i\in I}X_i&amp;lt;/math&amp;gt; is a finite or countable union, then&lt;br /&gt;
&lt;br /&gt;
如果 &amp;lt;math&amp;gt;X=\bigcup_{i\in I}X_i&amp;lt;/math&amp;gt; 是一个有限或可数的联合，则&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \dim_{\operatorname{Haus}}(X) =\sup_{i\in I} \dim_{\operatorname{Haus}}(X_i).&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \dim_{\operatorname{Haus}}(X) =\sup_{i\in I} \dim_{\operatorname{Haus}}(X_i).&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
This can be verified directly from the definition.&lt;br /&gt;
&lt;br /&gt;
This can be verified directly from the definition.&lt;br /&gt;
&lt;br /&gt;
这可以直接从定义得到验证。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
If ''X'' and ''Y'' are non-empty metric spaces, then the Hausdorff dimension of their product satisfies&amp;lt;ref&amp;gt;{{cite journal |author=Marstrand, J. M. |title=The dimension of Cartesian product sets |journal=Proc. Cambridge Philos. Soc. |volume=50 |issue=3 |pages=198–202 |year=1954 |doi=10.1017/S0305004100029236 |bibcode = 1954PCPS...50..198M }}&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
If X and Y are non-empty metric spaces, then the Hausdorff dimension of their product satisfies&lt;br /&gt;
&lt;br /&gt;
如果 ''X'' 和''Y''是非空度量空间，那么它们乘积的豪斯多夫维数满足&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt; \dim_{\operatorname{Haus}}(X\times Y)\ge \dim_{\operatorname{Haus}}(X)+ \dim_{\operatorname{Haus}}(Y).&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \dim_{\operatorname{Haus}}(X\times Y)\ge \dim_{\operatorname{Haus}}(X)+ \dim_{\operatorname{Haus}}(Y).&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
This inequality can be strict. It is possible to find two sets of dimension 0 whose product has dimension 1.&amp;lt;ref&amp;gt;{{cite book  | last = Falconer  | first = Kenneth J.  | title = Fractal geometry. Mathematical foundations and applications  | publisher = John Wiley &amp;amp; Sons, Inc., Hoboken, New Jersey  | year = 2003  | doi =   | isbn = }}&amp;lt;/ref&amp;gt; In the opposite direction, it is known that when ''X'' and ''Y'' are Borel subsets of '''R'''&amp;lt;sup&amp;gt;''n''&amp;lt;/sup&amp;gt;, the Hausdorff dimension of ''X'' × ''Y'' is bounded from above by the Hausdorff dimension of ''X'' plus the [[packing dimension|upper packing dimension]] of ''Y''. These facts are discussed in Mattila (1995).&lt;br /&gt;
&lt;br /&gt;
This inequality can be strict. It is possible to find two sets of dimension 0 whose product has dimension 1. In the opposite direction, it is known that when X and Y are Borel subsets of R&amp;lt;sup&amp;gt;n&amp;lt;/sup&amp;gt;, the Hausdorff dimension of X × Y is bounded from above by the Hausdorff dimension of X plus the upper packing dimension of Y. These facts are discussed in Mattila (1995).&lt;br /&gt;
&lt;br /&gt;
这种不平等可以是绝对的。有可能找到两个维数为0的集合，其乘积的维数为1。相反，我们知道当''X''和''Y''是 '''R'''&amp;lt;sup&amp;gt;''n''&amp;lt;/sup&amp;gt;的 Borel 子集时， ''X'' × ''Y''的豪斯多夫维数从上面以 ''X''的豪斯多夫维数加上 ''Y''的填充维数为界。Mattila (1995)曾就这些情况进行了讨论。&lt;br /&gt;
&lt;br /&gt;
==Self-similar sets自相似集合==&lt;br /&gt;
&lt;br /&gt;
{{refimprove section|date=March 2015}}&lt;br /&gt;
&lt;br /&gt;
Many sets defined by a self-similarity condition have dimensions which can be determined explicitly. Roughly, a set ''E'' is self-similar if it is the fixed point of a set-valued transformation ψ, that is ψ(''E'') = ''E'', although the exact definition is given below.&lt;br /&gt;
&lt;br /&gt;
Many sets defined by a self-similarity condition have dimensions which can be determined explicitly. Roughly, a set E is self-similar if it is the fixed point of a set-valued transformation ψ, that is ψ(E) = E, although the exact definition is given below.&lt;br /&gt;
&lt;br /&gt;
许多由自相似条件定义的集合具有可以显式确定的维数。粗略地说，集合''E'' 是自相似的，如果它是集值ψ变换的不动点，即ψ(''E'') = ''E''，尽管下面给出了确切的定义。&lt;br /&gt;
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&lt;br /&gt;
&lt;br /&gt;
&amp;lt;blockquote&amp;gt;'''Theorem'''. Suppose&lt;br /&gt;
&lt;br /&gt;
&amp;lt;blockquote&amp;gt;Theorem. Suppose&lt;br /&gt;
&lt;br /&gt;
&amp;lt;blockquote&amp;gt;'''定理'''：假设&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt; \psi_i: \mathbf{R}^n \rightarrow \mathbf{R}^n, \quad i=1, \ldots , m &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \psi_i: \mathbf{R}^n \rightarrow \mathbf{R}^n, \quad i=1, \ldots , m &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
are [[Contraction mapping|contractive]] mappings on '''R'''&amp;lt;sup&amp;gt;''n''&amp;lt;/sup&amp;gt; with contraction constant ''r&amp;lt;sub&amp;gt;j&amp;lt;/sub&amp;gt;'' &amp;lt; 1. Then there is a unique ''non-empty'' compact set ''A'' such that&lt;br /&gt;
&lt;br /&gt;
are contractive mappings on R&amp;lt;sup&amp;gt;n&amp;lt;/sup&amp;gt; with contraction constant r&amp;lt;sub&amp;gt;j&amp;lt;/sub&amp;gt; &amp;lt; 1. Then there is a unique non-empty compact set A such that&lt;br /&gt;
&lt;br /&gt;
是'''R'''&amp;lt;sup&amp;gt;''n''&amp;lt;/sup&amp;gt;上的压缩常数''r&amp;lt;sub&amp;gt;j&amp;lt;/sub&amp;gt;'&amp;lt; 1的压缩映射。然后有一个唯一的非空紧集A &lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt; A = \bigcup_{i=1}^m \psi_i (A). &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; A = \bigcup_{i=1}^m \psi_i (A). &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&amp;lt;/blockquote&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;/blockquote&amp;gt;&lt;br /&gt;
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&lt;br /&gt;
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&lt;br /&gt;
The theorem follows from [[Stefan Banach]]'s [[Contractive mapping theorem|contractive mapping fixed point theorem]] applied to the complete metric space of non-empty compact subsets of '''R'''&amp;lt;sup&amp;gt;''n''&amp;lt;/sup&amp;gt; with the [[Hausdorff distance]].&amp;lt;ref&amp;gt;{{cite book |author=Falconer, K. J. |title=The Geometry of Fractal Sets |publisher=Cambridge University Press |location=Cambridge, UK |year=1985 |isbn=0-521-25694-1 |chapter=Theorem 8.3}}&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
The theorem follows from Stefan Banach's contractive mapping fixed point theorem applied to the complete metric space of non-empty compact subsets of R&amp;lt;sup&amp;gt;n&amp;lt;/sup&amp;gt; with the Hausdorff distance.&lt;br /&gt;
&lt;br /&gt;
这个定理来源于 Stefan Banach 的压缩映射不动点定理，该定理应用于 '''R'''&amp;lt;sup&amp;gt;''n''&amp;lt;/sup&amp;gt; 的非空紧子集的完备空间豪斯多夫距离。&lt;br /&gt;
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&lt;br /&gt;
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===The open set condition开集条件===&lt;br /&gt;
&lt;br /&gt;
To determine the dimension of the self-similar set ''A'' (in certain cases), we need a technical condition called the ''open set condition'' (OSC) on the sequence of contractions ψ&amp;lt;sub&amp;gt;''i''&amp;lt;/sub&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
To determine the dimension of the self-similar set A (in certain cases), we need a technical condition called the open set condition (OSC) on the sequence of contractions ψ&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
为了确定自相似集''A'' 的维数(在某些情况下) ，我们需要一个称为''开集条件''(OSC)的技术条件ψ&amp;lt;sub&amp;gt;''i''&amp;lt;/sub&amp;gt;。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
There is a relatively compact open set ''V'' such that&lt;br /&gt;
&lt;br /&gt;
There is a relatively compact open set V such that&lt;br /&gt;
&lt;br /&gt;
有一个相对紧的开集''V''&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt; \bigcup_{i=1}^m\psi_i (V) \subseteq V, &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \bigcup_{i=1}^m\psi_i (V) \subseteq V, &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
where the sets in union on the left are pairwise [[disjoint sets|disjoint]].&lt;br /&gt;
&lt;br /&gt;
where the sets in union on the left are pairwise disjoint.&lt;br /&gt;
&lt;br /&gt;
左边的集合是成对不相交的。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The open set condition is a separation condition that ensures the images ψ&amp;lt;sub&amp;gt;''i''&amp;lt;/sub&amp;gt;(''V'') do not overlap &amp;quot;too much&amp;quot;.&lt;br /&gt;
&lt;br /&gt;
The open set condition is a separation condition that ensures the images ψ&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;(V) do not overlap &amp;quot;too much&amp;quot;.&lt;br /&gt;
&lt;br /&gt;
开集条件是保证图像子ψ&amp;lt;sub&amp;gt;''i''&amp;lt;/sub&amp;gt;(''V'') 不重叠“太多”的分离条件。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
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'''Theorem'''. Suppose the open set condition holds and each ψ&amp;lt;sub&amp;gt;''i''&amp;lt;/sub&amp;gt; is a similitude, that is a composition of an [[isometry]] and a [[dilation (metric space)|dilation]] around some point. Then the unique fixed point of ψ is a set whose Hausdorff dimension is ''s'' where ''s'' is the unique solution of&amp;lt;ref&amp;gt;{{cite journal | last=Hutchinson | first=John E. | title=Fractals and self similarity | journal=Indiana Univ. Math. J. | volume=30 | year=1981 | pages=713–747 | doi=10.1512/iumj.1981.30.30055 | issue=5 | doi-access=free }}&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
Theorem. Suppose the open set condition holds and each ψ&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt; is a similitude, that is a composition of an isometry and a dilation around some point. Then the unique fixed point of ψ is a set whose Hausdorff dimension is s where s is the unique solution of&lt;br /&gt;
&lt;br /&gt;
'''定理'''假设开集条件成立，并且每个ψ&amp;lt;sub&amp;gt;''i''&amp;lt;/sub&amp;gt; 是一个相似量，这是一个等距和围绕某一点的膨胀的合成。那么唯一的不动点是一个集合，它的豪斯多夫维数是 ''s'' ，其中  ''s'' 是 ''s'' &amp;lt;ref&amp;gt;{{cite journal | last=Hutchinson | first=John E. | title=Fractals and self similarity | journal=Indiana Univ. Math. J. | volume=30 | year=1981 | pages=713–747 | doi=10.1512/iumj.1981.30.30055 | issue=5 | doi-access=free }}&amp;lt;/ref&amp;gt;的唯一解&lt;br /&gt;
&lt;br /&gt;
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:&amp;lt;math&amp;gt; \sum_{i=1}^m r_i^s = 1. &amp;lt;/math&amp;gt;&lt;br /&gt;
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&amp;lt;math&amp;gt; \sum_{i=1}^m r_i^s = 1. &amp;lt;/math&amp;gt;&lt;br /&gt;
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The contraction coefficient of a similitude is the magnitude of the dilation.&lt;br /&gt;
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The contraction coefficient of a similitude is the magnitude of the dilation.&lt;br /&gt;
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相似物的收缩系数就是膨胀的大小。&lt;br /&gt;
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We can use this theorem to compute the Hausdorff dimension of the Sierpinski triangle (or sometimes called Sierpinski gasket). Consider three [[non-collinear points]] ''a''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;, ''a''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;, ''a''&amp;lt;sub&amp;gt;3&amp;lt;/sub&amp;gt; in the plane '''R'''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; and let ψ&amp;lt;sub&amp;gt;''i''&amp;lt;/sub&amp;gt; be the dilation of ratio 1/2 around ''a&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;''. The unique non-empty fixed point of the corresponding mapping ψ is a Sierpinski gasket and the dimension ''s'' is the unique solution of&lt;br /&gt;
&lt;br /&gt;
We can use this theorem to compute the Hausdorff dimension of the Sierpinski triangle (or sometimes called Sierpinski gasket). Consider three non-collinear points a&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;, a&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;, a&amp;lt;sub&amp;gt;3&amp;lt;/sub&amp;gt; in the plane R&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; and let ψ&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt; be the dilation of ratio 1/2 around a&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;. The unique non-empty fixed point of the corresponding mapping ψ is a Sierpinski gasket and the dimension s is the unique solution of&lt;br /&gt;
&lt;br /&gt;
我们可以使用这个定理来计算谢尔宾斯基三角形的豪斯多夫维数(或者有时候叫做谢尔宾斯基垫圈)。考虑R&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; 平面上的三个非共线点，''a''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;，''a''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;，''a''&amp;lt;sub&amp;gt;3&amp;lt;/sub&amp;gt;，让ψ&amp;lt;sub&amp;gt;''i''&amp;lt;/sub&amp;gt;是围绕着''a&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;''膨胀比率的1/2。对应映射的唯一非空不动点是一个谢尔宾斯基垫圈，其维数''s''是对应映射的唯一解&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt; \left(\frac{1}{2}\right)^s+\left(\frac{1}{2}\right)^s+\left(\frac{1}{2}\right)^s = 3 \left(\frac{1}{2}\right)^s =1. &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \left(\frac{1}{2}\right)^s+\left(\frac{1}{2}\right)^s+\left(\frac{1}{2}\right)^s = 3 \left(\frac{1}{2}\right)^s =1. &amp;lt;/math&amp;gt;&lt;br /&gt;
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Taking [[natural logarithm]]s of both sides of the above equation, we can solve for ''s'', that is: ''s'' = ln(3)/ln(2).  The Sierpinski gasket is self-similar and satisfies the OSC. In general a set ''E'' which is a fixed point of a mapping&lt;br /&gt;
&lt;br /&gt;
Taking natural logarithms of both sides of the above equation, we can solve for s, that is: s = ln(3)/ln(2).  The Sierpinski gasket is self-similar and satisfies the OSC. In general a set E which is a fixed point of a mapping&lt;br /&gt;
&lt;br /&gt;
取上述方程两边的自然对数，我们可以求出 ''s''，即: ''s'' = ln(3)/ln(2)。该密封垫具有自相似性，满足 OSC 要求。一般来说，集合 ''E''是一个映射的不动点&lt;br /&gt;
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: &amp;lt;math&amp;gt; A \mapsto \psi(A) = \bigcup_{i=1}^m \psi_i(A) &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt; A \mapsto \psi(A) = \bigcup_{i=1}^m \psi_i(A) &amp;lt;/math&amp;gt;&lt;br /&gt;
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is self-similar if and only if the intersections&lt;br /&gt;
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is self-similar if and only if the intersections&lt;br /&gt;
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是自相似的，当且仅当&lt;br /&gt;
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:&amp;lt;math&amp;gt; H^s\left(\psi_i(E) \cap \psi_j(E)\right) =0, &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; H^s\left(\psi_i(E) \cap \psi_j(E)\right) =0, &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
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where ''s'' is the Hausdorff dimension of ''E'' and ''H&amp;lt;sup&amp;gt;s&amp;lt;/sup&amp;gt;'' denotes [[Hausdorff measure]]. This is clear in the case of the Sierpinski gasket (the intersections are just points), but is also true more generally:&lt;br /&gt;
&lt;br /&gt;
where s is the Hausdorff dimension of E and H&amp;lt;sup&amp;gt;s&amp;lt;/sup&amp;gt; denotes Hausdorff measure. This is clear in the case of the Sierpinski gasket (the intersections are just points), but is also true more generally:&lt;br /&gt;
&lt;br /&gt;
其中 ''s''是''E''的豪斯多夫维数， ''E'' and ''H&amp;lt;sup&amp;gt;s&amp;lt;/sup&amp;gt;'' 表示 豪斯多夫测度。对于谢尔宾斯基垫圈(交叉点就是点)来说，这一点很明显，但更普遍的情况是:&lt;br /&gt;
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'''Theorem'''. Under the same conditions as the previous theorem, the unique fixed point of ψ is self-similar.&lt;br /&gt;
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Theorem. Under the same conditions as the previous theorem, the unique fixed point of ψ is self-similar.&lt;br /&gt;
&lt;br /&gt;
'''定理'''：在与前一定理相同的条件下，其唯一不动点是自相似的。&lt;br /&gt;
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==See also参阅==&lt;br /&gt;
&lt;br /&gt;
* [[List of fractals by Hausdorff dimension豪斯多夫分形维数列表]] Examples of deterministic fractals, random and natural fractals.确定性分形与随机和自然分形的示例。&lt;br /&gt;
&lt;br /&gt;
* [[Assouad dimension  Assouad维数]], another variation of fractal dimension that, like Hausdorff dimension, is defined using coverings by balls其他被球覆盖方式定义的分形维数，例如豪斯多夫维数。&lt;br /&gt;
&lt;br /&gt;
* [[Intrinsic dimension固有维数]]&lt;br /&gt;
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* [[Packing dimension填充维数]]&lt;br /&gt;
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* [[Fractal dimension分形维数]]&lt;br /&gt;
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==References参考文献==&lt;br /&gt;
&lt;br /&gt;
{{reflist}}&lt;br /&gt;
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==Further reading拓展阅读==&lt;br /&gt;
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* {{cite book |last1=Dodson |first1=M. Maurice |title=Fractal Geometry and Applications: A Jubilee of Benoît Mandelbrot |volume=72 |issue=1 |pages=305–347 |last2=Kristensen |first2=Simon |chapter=Hausdorff Dimension and Diophantine Approximation |date=June 12, 2003 |arxiv=math/0305399 |bibcode = 2003math......5399D |doi=10.1090/pspum/072.1/2112110|series=Proceedings of Symposia in Pure Mathematics |isbn=9780821836378 }}&lt;br /&gt;
&lt;br /&gt;
* {{cite book |last1=Hurewicz |first1=Witold |authorlink1=Witold Hurewicz |last2=Wallman |first2=Henry |authorlink2=Henry Wallman |title=Dimension Theory |url=https://archive.org/details/in.ernet.dli.2015.84609 |publisher=Princeton University Press |year=1948 }}&lt;br /&gt;
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* {{cite journal |author作者=E. Szpilrajn |authorlink=Edward Marczewski |title=La dimension et la mesure |journal=Fundamenta Mathematicae |volume=28 |pages=81–9 |year=1937 }}&lt;br /&gt;
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* {{cite journal&lt;br /&gt;
&lt;br /&gt;
 | last1=Marstrand&lt;br /&gt;
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 | last1=Marstrand&lt;br /&gt;
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 | last1=马斯特兰德&lt;br /&gt;
&lt;br /&gt;
 | first1=J. M. | title=The dimension of cartesian product sets | year=1954 | journal=Proc. Cambridge Philos. Soc.&lt;br /&gt;
&lt;br /&gt;
 | first1=J. M. | title=The dimension of cartesian product sets | year=1954 | journal=Proc. Cambridge Philos. Soc.&lt;br /&gt;
&lt;br /&gt;
 | first1= J. M. | title=笛卡儿积集的维数 | 1954年 |  journal=Proc. Cambridge Philos. Soc.&lt;br /&gt;
&lt;br /&gt;
 | volume=50&lt;br /&gt;
&lt;br /&gt;
 | volume=50&lt;br /&gt;
&lt;br /&gt;
 | 第50卷&lt;br /&gt;
&lt;br /&gt;
 | issue=3&lt;br /&gt;
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 | issue=3&lt;br /&gt;
&lt;br /&gt;
 | 第三期&lt;br /&gt;
&lt;br /&gt;
 | pages=198–202&lt;br /&gt;
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 | pages=198–202&lt;br /&gt;
&lt;br /&gt;
 | 第198-202页&lt;br /&gt;
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 | doi=10.1017/S0305004100029236|bibcode = 1954PCPS...50..198M }}&lt;br /&gt;
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 | doi=10.1017/S0305004100029236|bibcode = 1954PCPS...50..198M }}&lt;br /&gt;
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10.1017 / S0305004100029236 | bibcode 1954PCPS... 50. . 198 m }&lt;br /&gt;
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* {{Cite book&lt;br /&gt;
&lt;br /&gt;
 | last1=Mattila&lt;br /&gt;
&lt;br /&gt;
 | last1=Mattila&lt;br /&gt;
&lt;br /&gt;
 | last1=Mattila&lt;br /&gt;
&lt;br /&gt;
 | first1=Pertti | author1-link=Pertti Mattila| title=Geometry of sets and measures in Euclidean spaces | publisher=[[Cambridge University Press]]&lt;br /&gt;
&lt;br /&gt;
 | first1=Pertti | author1-link=Pertti Mattila| title=Geometry of sets and measures in Euclidean spaces | publisher=Cambridge University Press&lt;br /&gt;
&lt;br /&gt;
| first1 Pertti | author1-link Pertti Mattila | title 欧几里德空间中集合和度量的几何 | 出版商剑桥大学出版社&lt;br /&gt;
&lt;br /&gt;
 | isbn=978-0-521-65595-8 | year=1995}}&lt;br /&gt;
&lt;br /&gt;
 | isbn=978-0-521-65595-8 | year=1995}}&lt;br /&gt;
&lt;br /&gt;
| isbn 978-0-521-65595-8 | year 1995}&lt;br /&gt;
&lt;br /&gt;
* {{cite journal |author=A. S. Besicovitch |authorlink=A. S. Besicovitch |title=On Linear Sets of Points of Fractional Dimensions |journal=[[Mathematische Annalen]] |volume=101 |year=1929 | doi=10.1007/BF01454831| issue=1 |pages= 161–193}}&lt;br /&gt;
&lt;br /&gt;
* {{cite journal |author1=A. S. Besicovitch |authorlink1=A. S. Besicovitch |author2=H. D. Ursell |authorlink2=H. D. Ursell |title=Sets of Fractional Dimensions |journal=Journal of the London Mathematical Society |volume=12 |year=1937 | issue=1 | doi=10.1112/jlms/s1-12.45.18  | pages=18–25 }}&amp;lt;br/&amp;gt;Several selections from this volume are reprinted in {{cite book |author=Edgar, Gerald A. |title=Classics on fractals |publisher=Addison-Wesley |location=Boston |year=1993 |isbn=0-201-58701-7}} See chapters 9,10,11&lt;br /&gt;
&lt;br /&gt;
* {{cite journal |author=F. Hausdorff |authorlink=F. Hausdorff |title=Dimension und äußeres Maß |journal=Mathematische Annalen |volume=79 |issue=1–2 |pages=157–179 |date=March 1919 |doi=10.1007/BF01457179|hdl=10338.dmlcz/100363 |url=http://dml.cz/bitstream/handle/10338.dmlcz/100363/CzechMathJ_09-1959-3_5.pdf }}&lt;br /&gt;
&lt;br /&gt;
* {{cite journal | last=Hutchinson | first=John E. | title=Fractals and self similarity | journal=Indiana Univ. Math. J. | volume=30 | year=1981 | pages=713–747 | doi=10.1512/iumj.1981.30.30055 | issue=5 | doi-access=free }}&lt;br /&gt;
&lt;br /&gt;
*{{cite book | last=Falconer | first = Kenneth |title=Fractal Geometry: Mathematical Foundations and Applications | publisher=[[John Wiley and Sons]] | edition=2nd | year=2003}}&lt;br /&gt;
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==External links外部链接==&lt;br /&gt;
&lt;br /&gt;
* [https://www.encyclopediaofmath.org/index.php/Hausdorff_dimension Hausdorff dimension] 在 [https://www.encyclopediaofmath.org/ Encyclopedia of Mathematics]&lt;br /&gt;
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* [https://www.encyclopediaofmath.org/index.php/Hausdorff_measure Hausdorff measure] 在 [https://www.encyclopediaofmath.org/ Encyclopedia of Mathematics]&lt;br /&gt;
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{{DEFAULTSORT:Hausdorff Dimension豪斯多夫维数}}&lt;br /&gt;
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[[Category分类:Fractals分形]]&lt;br /&gt;
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[[Category分类:Metric geometry度量几何]]&lt;br /&gt;
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[[Category分类:Dimension theory维度理论]]&lt;br /&gt;
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&amp;lt;small&amp;gt;This page was moved from [[wikipedia:en:Hausdorff dimension]]. Its edit history can be viewed at [[分形维数/edithistory]]&amp;lt;/small&amp;gt;&amp;lt;/noinclude&amp;gt;&lt;br /&gt;
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[[Category:待整理页面]]&lt;/div&gt;</summary>
		<author><name>Ruili</name></author>
	</entry>
	<entry>
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		<title>分形维数</title>
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		<updated>2020-11-01T09:48:58Z</updated>

		<summary type="html">&lt;p&gt;Ruili：&lt;/p&gt;
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&lt;div&gt;此词条暂由彩云小译翻译，未经人工整理和审校，带来阅读不便，请见谅。&lt;br /&gt;
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{{short description|Invariant}}&lt;br /&gt;
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Example of non-integer dimensions. The first four [[iteration]]s of the [[Koch snowflake|Koch curve]], where after each iteration, all original line segments are replaced with four, each a self-similar copy that is 1/3 the length of the original. One formalism of the Hausdorff dimension uses this scale factor (3) and the number of self-similar objects (4) to calculate the dimension, D, after the first iteration to be D = (log N)/(log S) = (log 4)/(log 3) ≈ 1.26.&amp;lt;ref name=CampbellAnnenberg15&amp;gt;MacGregor Campbell, 2013, &amp;quot;5.6 Scaling and the Hausdorff Dimension,&amp;quot; at ''Annenberg Learner:MATHematics illuminated'', see [http://www.learner.org/courses/mathilluminated/units/5/textbook/06.php], accessed 5 March 2015.&amp;lt;/ref&amp;gt; That is, while the Hausdorff dimension of a single [[point (geometry)|point]] is zero, of a [[line segment]] is 1, of a [[square]] is 2, and of a [[cube]] is 3, for [[fractal]]s such as this, the object can have a non-integer dimension.&lt;br /&gt;
&lt;br /&gt;
Example of non-integer dimensions. The first four iterations of the Koch curve, where after each iteration, all original line segments are replaced with four, each a self-similar copy that is 1/3 the length of the original. One formalism of the Hausdorff dimension uses this scale factor (3) and the number of self-similar objects (4) to calculate the dimension, D, after the first iteration to be D = (log N)/(log S) = (log 4)/(log 3) ≈ 1.26. That is, while the Hausdorff dimension of a single point is zero, of a line segment is 1, of a square is 2, and of a cube is 3, for fractals such as this, the object can have a non-integer dimension.&lt;br /&gt;
&lt;br /&gt;
非整数维度示例：前四个[[Koch 曲线]]的迭代，在每次迭代后，所有原始线段都被替换为四个，每个自相似的复制是原始线段长度的1 / 3。豪斯多夫维数的一个建模是使用比例因子(3)和自相似对象的数量(4)来计算维度 D，在第一次迭代后为 D = (log N)/(log S) = (log 4)/(log 3) ≈ 1.26.&amp;lt;ref name=CampbellAnnenberg15&amp;gt;。MacGregor Campbell, 2013, &amp;quot;5.6 Scaling and the Hausdorff Dimension,&amp;quot; 在 ''Annenberg Learner:MATHematics illuminated'', 参见 [http://www.learner.org/courses/mathilluminated/units/5/textbook/06.php], accessed 5 March 2015.&amp;lt;/ref&amp;gt; 也就是说，单点的豪斯多夫维数为零，线段为1，正方形为2，立方体为3时，但对于分形，对象可以有一个非整数维度。&lt;br /&gt;
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In [[mathematics]], '''Hausdorff dimension''' is a measure of ''roughness'', or more specifically, [[fractal dimension]], that was first introduced in 1918 by [[mathematician]] [[Felix Hausdorff]].&amp;lt;ref&amp;gt;{{Cite journal |arxiv = 1101.1444|doi = 10.1214/11-STS370|title = Estimators of Fractal Dimension: Assessing the Roughness of Time Series and Spatial Data|journal = Statistical Science|volume = 27|issue = 2|pages = 247–277|year = 2012|last1 = Gneiting|first1 = Tilmann|last2 = Ševčíková|first2 = Hana|last3 = Percival|first3 = Donald B.}}&amp;lt;/ref&amp;gt; For instance, the Hausdorff dimension of a single [[point (geometry)|point]] is zero, of a [[line segment]] is 1, of a [[square]] is 2, and of a [[cube]] is 3. That is, for sets of points that define a smooth shape or a shape that has a small number of corners—the shapes of traditional geometry and science—the Hausdorff dimension is an [[integer]] agreeing with the usual sense of dimension, also known as the [[Inductive dimension|topological dimension]]. However, formulas have also been developed that allow calculation of the dimension of other less simple objects, where, solely on the basis of their properties of [[scaling (geometry)|scaling]] and [[self-similarity]], one is led to the conclusion that particular objects—including [[fractal]]s—have non-integer Hausdorff dimensions. Because of the significant technical advances made by [[Abram Samoilovitch Besicovitch]] allowing computation of dimensions for highly irregular or &amp;quot;rough&amp;quot; sets, this dimension is also commonly referred to as the ''Hausdorff–Besicovitch dimension.''&lt;br /&gt;
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In mathematics, Hausdorff dimension is a measure of roughness, or more specifically, fractal dimension, that was first introduced in 1918 by mathematician Felix Hausdorff. For instance, the Hausdorff dimension of a single point is zero, of a line segment is 1, of a square is 2, and of a cube is 3. That is, for sets of points that define a smooth shape or a shape that has a small number of corners—the shapes of traditional geometry and science—the Hausdorff dimension is an integer agreeing with the usual sense of dimension, also known as the topological dimension. However, formulas have also been developed that allow calculation of the dimension of other less simple objects, where, solely on the basis of their properties of scaling and self-similarity, one is led to the conclusion that particular objects—including fractals—have non-integer Hausdorff dimensions. Because of the significant technical advances made by Abram Samoilovitch Besicovitch allowing computation of dimensions for highly irregular or &amp;quot;rough&amp;quot; sets, this dimension is also commonly referred to as the Hausdorff–Besicovitch dimension.&lt;br /&gt;
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在[[数学]]中，'''&amp;lt;font color = '#ff8000'&amp;gt;豪斯多夫维数Hausdorff dimension&amp;lt;/font&amp;gt;'''是一种粗糙度的度量单位，或者更确切地说，分形维数，是由数学家 Felix Hausdorff 在1918年首次提出的。例如，单点的豪斯多夫维数为零，线段为1，正方形为2，立方体为3。也就是说，对于定义了一个光滑形状或一个有少数几个角的形状---- 传统几何学和科学的形状---- 的点集来说，豪斯多夫维数是一个整数，符合通常的维度意义，也称为拓扑维度。然而，还有一些公式允许计算其他不太简单的对象的维数，其中仅仅根据它们的标度和自相似特性，就可以得出结论: 特定的对象ー包括分形ー具有非整数的 Hausdorff 维数。由于阿布拉姆·萨莫伊洛维奇·贝西科维奇的重大技术进步，允许计算高度不规则或“粗糙”集的维度，这个维度通常也被称为 Hausdorff-Besicovitch 维度。 &lt;br /&gt;
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The Hausdorff dimension, more specifically, is a further dimensional number associated with a given set, where the distances between all members of that set are defined. Such a set is termed a [[metric space]]. The dimension is drawn from the [[Extended real number line|extended real numbers]], &amp;lt;math&amp;gt;\overline{\mathbb{R}}&amp;lt;/math&amp;gt;, as opposed to the more intuitive notion of dimension, which is not associated to general metric spaces, and only takes values in the non-negative integers.&lt;br /&gt;
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The Hausdorff dimension, more specifically, is a further dimensional number associated with a given set, where the distances between all members of that set are defined. Such a set is termed a metric space. The dimension is drawn from the extended real numbers, &amp;lt;math&amp;gt;\overline{\mathbb{R}}&amp;lt;/math&amp;gt;, as opposed to the more intuitive notion of dimension, which is not associated to general metric spaces, and only takes values in the non-negative integers.&lt;br /&gt;
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更具体地说，豪斯多夫维数是一个与给定集合相关联的更进一步的维数，其中定义了该集合所有成员之间的距离。这样的集合称为度量空间。维数是从扩展的实数，&amp;lt;math&amp;gt;\overline{\mathbb{R}}&amp;lt;/math&amp;gt;，而不是更直观的维数概念(它不与一般的度量空间相关联，只取非负整数的值)。&lt;br /&gt;
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In mathematical terms, the Hausdorff dimension generalizes the notion of the dimension of a real [[vector space]]. That is, the Hausdorff dimension of an ''n''-dimensional [[inner product space]] equals ''n''. This underlies the earlier statement that the Hausdorff dimension of a point is zero, of a line is one, etc., and that [[fractal|irregular sets]] can have noninteger Hausdorff dimensions. For instance, the [[Koch snowflake]] shown at right is constructed from an equilateral triangle; in each iteration, its component line segments are divided into 3 segments of unit length, the newly created middle segment is used as the base of a new [[equilateral]] triangle that points outward, and this base segment is then deleted to leave a final object from the iteration of unit length of 4.&amp;lt;ref&amp;gt;Larry Riddle, 2014, &amp;quot;Classic Iterated Function Systems: Koch Snowflake&amp;quot;, Agnes Scott College e-Academy (online), see [http://ecademy.agnesscott.edu/~lriddle/ifs/ksnow/ksnow.htm], accessed 5 March 2015.&amp;lt;/ref&amp;gt; That is, after the first iteration, each original line segment has been replaced with N=4, where each self-similar copy is 1/S = 1/3 as long as the original.&amp;lt;ref name=CampbellAnnenberg15/&amp;gt; Stated another way, we have taken an object with Euclidean dimension, D, and reduced its linear scale by 1/3 in each direction, so that its length increases to N=S&amp;lt;sup&amp;gt;D&amp;lt;/sup&amp;gt;.&amp;lt;ref name=ClaytonSCTPLS96&amp;gt;Keith Clayton, 1996, &amp;quot;Fractals and the Fractal Dimension,&amp;quot; ''Basic Concepts in Nonlinear Dynamics and Chaos'' (workshop), Society for Chaos Theory in Psychology and the Life Sciences annual meeting, June 28, 1996, Berkeley, California, see [http://www.vanderbilt.edu/AnS/psychology/cogsci/chaos/workshop/Workshop.html], accessed 5 March 2015.&amp;lt;/ref&amp;gt; This equation is easily solved for D, yielding the ratio of logarithms (or [[natural logarithm]]s) appearing in the figures, and giving—in the Koch and other fractal cases—non-integer dimensions for these objects.&lt;br /&gt;
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In mathematical terms, the Hausdorff dimension generalizes the notion of the dimension of a real vector space. That is, the Hausdorff dimension of an n-dimensional inner product space equals n. This underlies the earlier statement that the Hausdorff dimension of a point is zero, of a line is one, etc., and that irregular sets can have noninteger Hausdorff dimensions. For instance, the Koch snowflake shown at right is constructed from an equilateral triangle; in each iteration, its component line segments are divided into 3 segments of unit length, the newly created middle segment is used as the base of a new equilateral triangle that points outward, and this base segment is then deleted to leave a final object from the iteration of unit length of 4. That is, after the first iteration, each original line segment has been replaced with N=4, where each self-similar copy is 1/S = 1/3 as long as the original. This equation is easily solved for D, yielding the ratio of logarithms (or natural logarithms) appearing in the figures, and giving—in the Koch and other fractal cases—non-integer dimensions for these objects.&lt;br /&gt;
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用数学术语来说，豪斯多夫维数概括了实向量空间维数的概念。也就是说，n 维内积空间的豪斯多夫维数等于 n。 这就是早期假设的基础，一个点的豪斯多夫维数是零，一条线是一等等，不规则集可以有非整数的豪斯多夫维数。例如，右边所示的 Koch 雪花是由一个正三角形构成的; 在每次迭代中，它的组成线段被分成单位长度的3段，新创建的中间线段被用作一个指向外部的新正三角形的基础，然后人们删除这个基础线段用来保留单位长度4的迭代中的最终对象。也就是说，在第一次迭代之后，每个原始线段都被替换为 N=4，其中每个自相似拷贝的长度是原始线段的1/S = 1/3 。这个方程很容易求解为 D，产生出现在图形中的对数(或自然对数)的比率，并给出——在 Koch 和其他分形情况下——这些对象的非整数维数。&lt;br /&gt;
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The Hausdorff dimension is a successor to the simpler, but usually equivalent, box-counting or [[Minkowski–Bouligand dimension]].&lt;br /&gt;
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The Hausdorff dimension is a successor to the simpler, but usually equivalent, box-counting or Minkowski–Bouligand dimension.&lt;br /&gt;
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豪斯多夫维数是更简单但通常等价的'''&amp;lt;font color = '#ff8000'&amp;gt;计盒维数box-counting&amp;lt;/font&amp;gt;'''或'''&amp;lt;font color = '#ff8000'&amp;gt;闵可夫斯基维数Minkowski-Bouligand&amp;lt;/font&amp;gt;'''的继承者。&lt;br /&gt;
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==Intuition概念==&lt;br /&gt;
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The intuitive concept of dimension of a geometric object ''X'' is the number of independent parameters one needs to pick out a unique point inside. However, any point specified by two parameters can be instead specified by one, because the [[cardinality]] of the [[real plane]] is equal to the cardinality of the [[real line]] (this can be seen by an [[Cantor's diagonal argument|argument]] involving interweaving the digits of two numbers to yield a single number encoding the same information). The example of a [[space-filling curve]] shows that one can even map the real line to the real plane [[Surjective function|surjectively]] (taking one real number into a pair of real numbers in a way so that all pairs of numbers are covered) and ''continuously'', so that a one-dimensional object completely fills up a higher-dimensional object.&lt;br /&gt;
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The intuitive concept of dimension of a geometric object X is the number of independent parameters one needs to pick out a unique point inside. However, any point specified by two parameters can be instead specified by one, because the cardinality of the real plane is equal to the cardinality of the real line (this can be seen by an argument involving interweaving the digits of two numbers to yield a single number encoding the same information). The example of a space-filling curve shows that one can even map the real line to the real plane surjectively (taking one real number into a pair of real numbers in a way so that all pairs of numbers are covered) and continuously, so that a one-dimensional object completely fills up a higher-dimensional object.&lt;br /&gt;
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几何对象X的尺寸的直观概念是指需要多少个独立参数才能找到一个独特的点。但是，任何由两个参数指定的点都可以由一个参数指定，因为为实平面的基数等于实线的基数(这可以通过交织两个数字以产生一个编码相同信息的单个数字看到)。'''&amp;lt;font color = '#ff8000'&amp;gt;皮亚诺曲线&amp;lt;/font&amp;gt;'''的例子表明，可以将实线完美和连续地映射到实平面(把一个实数转换成一对实数，从而覆盖所有实数对)，由此一维对象完全填充了一个高维对象。&lt;br /&gt;
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Every space filling curve hits some points multiple times, and does not have a continuous inverse. It is impossible to map two dimensions onto one in a way that is continuous and continuously invertible. The topological dimension, also called [[Lebesgue covering dimension]], explains why. This dimension is ''n'' if, in every covering of ''X'' by small open balls, there is at least one point where ''n''&amp;amp;nbsp;+&amp;amp;nbsp;1 balls overlap. For example, when one covers a line with short open intervals, some points must be covered twice, giving dimension&amp;amp;nbsp;''n''&amp;amp;nbsp;=&amp;amp;nbsp;1.&lt;br /&gt;
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Every space filling curve hits some points multiple times, and does not have a continuous inverse. It is impossible to map two dimensions onto one in a way that is continuous and continuously invertible. The topological dimension, also called Lebesgue covering dimension, explains why. This dimension is n if, in every covering of X by small open balls, there is at least one point where n&amp;amp;nbsp;+&amp;amp;nbsp;1 balls overlap. For example, when one covers a line with short open intervals, some points must be covered twice, giving dimension&amp;amp;nbsp;n&amp;amp;nbsp;=&amp;amp;nbsp;1.&lt;br /&gt;
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每条空间填充曲线都会多次击中某些点，且不存在连续的逆。将二维以连续和连续可逆的方式映射到一维是不可能的。'''&amp;lt;font color = '#ff8000'&amp;gt;拓扑维度 topological dimension&amp;lt;/font&amp;gt;'''，也被称为Lebesgue覆盖维数，解释了为什么。如果在 x 的每个小开球覆盖中，至少有一个点 n + 1个球重叠，这个维度是 n。例如，当用短的开区间覆盖一条线时，某些点必须被覆盖两次，给出维数''n''&amp;amp;nbsp;=&amp;amp;nbsp;1。&lt;br /&gt;
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But topological dimension is a very crude measure of the local size of a space (size near a point). A curve that is almost space-filling can still have topological dimension one, even if it fills up most of the area of a region. A [[fractal]] has an integer topological dimension, but in terms of the amount of space it takes up, it behaves like a higher-dimensional space.&lt;br /&gt;
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But topological dimension is a very crude measure of the local size of a space (size near a point). A curve that is almost space-filling can still have topological dimension one, even if it fills up most of the area of a region. A fractal has an integer topological dimension, but in terms of the amount of space it takes up, it behaves like a higher-dimensional space.&lt;br /&gt;
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但是，拓扑维度是对空间局部尺寸(点附近的尺寸)的一个非常粗略的度量。一条几乎是空间填充的曲线仍然可以有一维拓扑，即使它填充了一个区域的大部分面积。分形具有整数的拓扑维数，但就其所占空间的空间量而言，它看起来像一个更高维的空间。&lt;br /&gt;
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The Hausdorff dimension measures the local size of a space taking into account the distance between points, the [[metric space|metric]]. Consider the number ''N''(''r'') of [[ball (mathematics)|balls]] of radius at most ''r'' required to cover ''X'' completely. When ''r'' is very small, ''N''(''r'') grows polynomially with 1/''r''. For a sufficiently well-behaved  ''X'', the Hausdorff dimension is the unique number ''d'' such that N(''r'') grows as 1/''r&amp;lt;sup&amp;gt;d&amp;lt;/sup&amp;gt;'' as ''r'' approaches zero. More precisely, this defines the [[Minkowski–Bouligand dimension|box-counting dimension]], which equals the Hausdorff dimension when the value ''d'' is a critical boundary between growth rates that are insufficient to cover the space, and growth rates that are overabundant.&lt;br /&gt;
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The Hausdorff dimension measures the local size of a space taking into account the distance between points, the metric. Consider the number N(r) of balls of radius at most r required to cover X completely. When r is very small, N(r) grows polynomially with 1/r. For a sufficiently well-behaved  X, the Hausdorff dimension is the unique number d such that N(r) grows as 1/r&amp;lt;sup&amp;gt;d&amp;lt;/sup&amp;gt; as r approaches zero. More precisely, this defines the box-counting dimension, which equals the Hausdorff dimension when the value d is a critical boundary between growth rates that are insufficient to cover the space, and growth rates that are overabundant.&lt;br /&gt;
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豪斯多夫维数测量一个空间的局部大小时，会考虑到点之间距离的度量。考虑半径最大为 r 的球数 ''N'' (r) ，需要完全覆盖 ''X''。当 r 很小时，n (r)以1/''r'' 增长多项式。对于一个表现足够好的 ''X''，豪斯多夫维数是唯一的数 d，这样当 r 趋近于零时， N(r)增长为1/r&amp;lt;sup&amp;gt;d&amp;lt;/sup&amp;gt; 。更确切地说，这定义了盒子计数维度，当值 d 是不足以覆盖空间的增长率和过度充裕的增长率之间的关键边界时，它等于豪斯多夫维数。&lt;br /&gt;
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For shapes that are smooth, or shapes with a small number of corners, the shapes of traditional geometry and science, the Hausdorff dimension is an integer agreeing with the topological dimension. But [[Benoit Mandelbrot]] observed that [[fractal]]s, sets with noninteger Hausdorff dimensions, are found everywhere in nature. He observed that the proper idealization of most rough shapes you see around you is not in terms of smooth idealized shapes, but in terms of fractal idealized shapes:&lt;br /&gt;
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For shapes that are smooth, or shapes with a small number of corners, the shapes of traditional geometry and science, the Hausdorff dimension is an integer agreeing with the topological dimension. But Benoit Mandelbrot observed that fractals, sets with noninteger Hausdorff dimensions, are found everywhere in nature. He observed that the proper idealization of most rough shapes you see around you is not in terms of smooth idealized shapes, but in terms of fractal idealized shapes:&lt;br /&gt;
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对于光滑的形状，或者有少量棱角的形状，传统几何和科学的形状，豪斯多夫维数是一个整数，与拓扑维度一致。但是伯努·曼德布洛特观察到分形---- 具有非整数豪斯多夫维数的集合---- 在自然界中随处可见。他观察到，我们周围大多数粗糙形状的理想化不是光滑的理想化形状，而是分形理想化形状:&lt;br /&gt;
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&amp;lt;blockquote&amp;gt;Clouds are not spheres, mountains are not cones, coastlines are not circles, and bark is not smooth, nor does lightning travel in a straight line.&amp;lt;ref name=&amp;quot;mandelbrot&amp;quot;&amp;gt;{{cite book   | last = Mandelbrot   | first = Benoît   | authorlink = Benoit Mandelbrot   | title = The Fractal Geometry of Nature   | publisher = W. H. Freeman   | series = Lecture notes in mathematics 1358   | year = 1982   | doi =    | isbn = 0-7167-1186-9   | url-access = registration   | url = https://archive.org/details/fractalgeometryo00beno   }}&amp;lt;/ref&amp;gt;&amp;lt;/blockquote&amp;gt;&lt;br /&gt;
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&amp;lt;blockquote&amp;gt;Clouds are not spheres, mountains are not cones, coastlines are not circles, and bark is not smooth, nor does lightning travel in a straight line.&amp;lt;/blockquote&amp;gt;&lt;br /&gt;
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&amp;lt;blockquote&amp;gt;云不是球体，山不是锥体，海岸线不是圆圈，树皮不平滑，闪电也不是直线运动。 &amp;lt;/blockquote&amp;gt;&lt;br /&gt;
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For fractals that occur in nature, the Hausdorff and [[Minkowski–Bouligand dimension|box-counting dimension]] coincide. The [[packing dimension]] is yet another similar notion which gives the same value for many shapes, but there are well documented exceptions where all these dimensions differ.&lt;br /&gt;
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For fractals that occur in nature, the Hausdorff and box-counting dimension coincide. The packing dimension is yet another similar notion which gives the same value for many shapes, but there are well documented exceptions where all these dimensions differ.&lt;br /&gt;
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对于自然界中出现的分形，豪斯多夫维数和盒计数维数是一致的。封装尺寸是另一个类似的概念，它给出了许多形状相同的值，但是在所有这些尺寸不同的情况，都做了很好的说明。&lt;br /&gt;
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==Formal definitions形式化定义==&lt;br /&gt;
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===Hausdorff content豪斯多夫集===&lt;br /&gt;
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Let ''X'' be a [[metric space]]. If ''S'' ⊂ ''X'' and ''d'' ∈ [0, ∞), the ''d''-dimensional '''unlimited Hausdorff content''' of ''S'' is defined by&lt;br /&gt;
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Let X be a metric space. If S ⊂ X and d ∈ [0, ∞), the d-dimensional unlimited Hausdorff content of S is defined by&lt;br /&gt;
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设 ''X''是度量空间。若''S'' ⊂ ''X'' 和 ''d'' ∈ [0, ∞) ，则 ''S'' 的''d''维无限 豪斯多夫集定义为&lt;br /&gt;
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:&amp;lt;math&amp;gt;C_H^d(S):=\inf\Bigl\{\sum_i r_i^d:\text{ there is a cover of } S\text{ by balls with radii }r_i&amp;gt;0\Bigr\}.&amp;lt;/math&amp;gt;&lt;br /&gt;
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&amp;lt;math&amp;gt;C_H^d(S):=\inf\Bigl\{\sum_i r_i^d:\text{ there is a cover of } S\text{ by balls with radii }r_i&amp;gt;0\Bigr\}.&amp;lt;/math&amp;gt;&lt;br /&gt;
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&amp;lt;math&amp;gt;C_H^d(S):=\inf\Bigl\{\sum_i r_i^d:\text{ there is a cover of } S\text{ by balls with radii }r_i&amp;gt;0\Bigr\}.&amp;lt;/math&amp;gt;&lt;br /&gt;
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In other words, &amp;lt;math&amp;gt;C_H^d(S)&amp;lt;/math&amp;gt; is the [[infimum]] of the set of numbers &amp;lt;math&amp;gt;\delta \geq 0&amp;lt;/math&amp;gt; such that there is some (indexed) collection of [[ball (mathematics)|ball]]s &amp;lt;math&amp;gt;\{B(x_i,r_i):i\in I\}&amp;lt;/math&amp;gt; covering ''S'' with ''r&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;''&amp;amp;nbsp;&amp;gt;&amp;amp;nbsp;0 for each ''i''&amp;amp;nbsp;∈&amp;amp;nbsp;''I'' that satisfies &amp;lt;math&amp;gt;\sum_{i\in I} r_i^d&amp;lt;\delta &amp;lt;/math&amp;gt;. (Here, we use the standard convention that [[infimum|inf&amp;amp;nbsp;Ø&amp;amp;nbsp;=&amp;amp;nbsp;∞]].)&lt;br /&gt;
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In other words, &amp;lt;math&amp;gt;C_H^d(S)&amp;lt;/math&amp;gt; is the infimum of the set of numbers &amp;lt;math&amp;gt;\delta \geq 0&amp;lt;/math&amp;gt; such that there is some (indexed) collection of balls &amp;lt;math&amp;gt;\{B(x_i,r_i):i\in I\}&amp;lt;/math&amp;gt; covering S with r&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;&amp;amp;nbsp;&amp;gt;&amp;amp;nbsp;0 for each i&amp;amp;nbsp;∈&amp;amp;nbsp;I that satisfies &amp;lt;math&amp;gt;\sum_{i\in I} r_i^d&amp;lt;\delta &amp;lt;/math&amp;gt;. (Here, we use the standard convention that inf&amp;amp;nbsp;Ø&amp;amp;nbsp;=&amp;amp;nbsp;∞.)&lt;br /&gt;
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换句话说，&amp;lt;math&amp;gt;C_H^d(S)&amp;lt;/math&amp;gt; 是数字集合&amp;lt;math&amp;gt;\delta \geq 0&amp;lt;/math&amp;gt;的下确界，使得在 ''i''&amp;amp;nbsp;∈&amp;amp;nbsp中存在一些球集合 &amp;lt;math&amp;gt;\{B(x_i,r_i):i\in I\}&amp;lt;/math&amp;gt;  i 包含 s，对于每个 ''r&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;''&amp;amp;nbsp;&amp;gt;&amp;amp;nbsp;0 满足 i 中的和&amp;lt;math&amp;gt;\sum_{i\in I} r_i^d&amp;lt;\delta &amp;lt;/math&amp;gt; (在这里，我们使用inf&amp;amp;nbsp;Ø&amp;amp;nbsp;=&amp;amp;nbsp;∞ )的标准约定。&lt;br /&gt;
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===Hausdorff measurement豪斯多夫分形测量===&lt;br /&gt;
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The Hausdorff outer measure is different from the unbounded Hausdorf content in that rather than considering all possible coverings of ''S'', we see what happens when the sizes of the balls go to zero. This is  for &amp;lt;math&amp;gt;d \geq 0 &amp;lt;/math&amp;gt;, we define the ''d''-dimensional Hausdorff outer measure of ''S'' as&lt;br /&gt;
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The Hausdorff outer measure is different from the unbounded Hausdorf content in that rather than considering all possible coverings of S, we see what happens when the sizes of the balls go to zero. This is  for &amp;lt;math&amp;gt;d \geq 0 &amp;lt;/math&amp;gt;, we define the d-dimensional Hausdorff outer measure of S as&lt;br /&gt;
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豪斯多夫外测度不同于无界的豪斯多夫，因为我们不考虑 s 的所有可能，我们看到当球的大小为零时会发生什么。这是为了数学  &amp;lt;math&amp;gt;d \geq 0 &amp;lt;/math&amp;gt;，我们定义了  ''S''的 ''d''维豪斯多夫Hausdorff 外测度为&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt; \mathcal{H}^d(S):=\lim_{r \to 0} \inf\Bigl\{\sum_i r_i^d:\text{ there is a cover of } S\text{ by balls with radii } 0 &amp;lt; r_i &amp;lt; r\Bigr\}.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \mathcal{H}^d(S):=\lim_{r \to 0} \inf\Bigl\{\sum_i r_i^d:\text{ there is a cover of } S\text{ by balls with radii } 0 &amp;lt; r_i &amp;lt; r\Bigr\}.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \mathcal{H}^d(S):=\lim_{r \to 0} \inf\Bigl\{\sum_i r_i^d:\text{有一个面} S\text{ 球 } 0 &amp;lt; r_i &amp;lt; r\Bigr\}.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
===Hausdorff dimension豪斯多夫维数===&lt;br /&gt;
&lt;br /&gt;
The '''Hausdorff dimension''' of ''X'' is defined by&lt;br /&gt;
&lt;br /&gt;
The Hausdorff dimension of X is defined by&lt;br /&gt;
&lt;br /&gt;
X 的豪斯多夫维数定义为&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt;\dim_{\operatorname{H}}(X):=\inf\{d\ge 0: \mathcal{H}^d(X)=0\}.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt;\dim_{\operatorname{H}}(X):=\inf\{d\ge 0: \mathcal{H}^d(X)=0\}.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Equivalently, dim&amp;lt;sub&amp;gt;H&amp;lt;/sub&amp;gt;(''X'') may be defined as the [[infimum]] of the set of ''d'' ∈ [0, ∞) such that the ''d''-dimensional [[Hausdorff measure]] of ''X'' is zero. This is the same as the supremum of the set of ''d''&amp;amp;nbsp;∈&amp;amp;nbsp;[0,&amp;amp;nbsp;∞) such that the ''d''-dimensional Hausdorff measure of ''X'' is infinite (except that when this latter set of numbers ''d'' is empty the Hausdorff dimension is zero).&lt;br /&gt;
&lt;br /&gt;
Equivalently, dim&amp;lt;sub&amp;gt;H&amp;lt;/sub&amp;gt;(X) may be defined as the infimum of the set of d ∈ [0, ∞) such that the d-dimensional Hausdorff measure of X is zero. This is the same as the supremum of the set of d&amp;amp;nbsp;∈&amp;amp;nbsp;[0,&amp;amp;nbsp;∞) such that the d-dimensional Hausdorff measure of X is infinite (except that when this latter set of numbers d is empty the Hausdorff dimension is zero).&lt;br /&gt;
&lt;br /&gt;
等价地，dim &amp;lt;sub&amp;gt;H&amp;lt;/sub&amp;gt;(''X'')可定义为 ''d'' ∈ [0, ∞) 集的下确界，使得''X'' 的''d''-维 [[豪斯多夫测度]] 为零。这与 ''d''&amp;amp;nbsp;∈&amp;amp;nbsp;[0,&amp;amp;nbsp;∞)的集合的上确界相同，因此''X''的 d 维豪斯多夫测度是无限的(除非后一个集合 ''d'' 是空的，豪斯多夫维数为零)。&lt;br /&gt;
&lt;br /&gt;
==Examples实例==&lt;br /&gt;
&lt;br /&gt;
[[Image:Sierpinski deep.svg|thumb|250px|Dimension of a further [[fractal]] example. The [[Sierpinski triangle]], an object with Hausdorff dimension of log(3)/log(2)≈1.58.&amp;lt;ref name=ClaytonSCTPLS96/&amp;gt;]]&lt;br /&gt;
&lt;br /&gt;
Dimension of a further [[fractal example. The Sierpinski triangle, an object with Hausdorff dimension of log(3)/log(2)≈1.58.]]&lt;br /&gt;
&lt;br /&gt;
[[Image:谢尔宾斯基三角形 deep.svg|thumb|250px|进一步的[[分形维数]]的例子，进一步的分形维数的例子是谢尔宾斯基三角形，它是一个豪斯多夫维数为log(3)/log(2)≈1.58.&amp;lt;ref name=ClaytonSCTPLS96/&amp;gt;的物体]]&lt;br /&gt;
&lt;br /&gt;
* [[Countable set]]s have Hausdorff dimension 0.&amp;lt;ref name=&amp;quot;schleicher&amp;quot;&amp;gt;{{cite journal |last1=Schleicher |first1=Dierk |title=Hausdorff Dimension, Its Properties, and Its Surprises |journal=The American Mathematical Monthly |date=June 2007 |volume=114 |issue=6 |pages=509–528 |doi=10.1080/00029890.2007.11920440 |language=en |issn=0002-9890|arxiv=math/0505099 }}&amp;lt;/ref&amp;gt;&lt;br /&gt;
*[[可数集]]拥有豪斯多夫维数0.&amp;lt;ref name=&amp;quot;schleicher&amp;quot;&amp;gt;{{cite journal |last1=Schleicher |first1=Dierk |title=豪斯多夫维数, Its Properties, and Its Surprises |journal=The American Mathematical Monthly美国数学期刊 |date=June 2007 |volume=114 |issue=6 |pages=509–528 |doi=10.1080/00029890.2007.11920440 |language=en |issn=0002-9890|arxiv=math/0505099 }}&amp;lt;/ref&amp;gt;&lt;br /&gt;
* The [[Euclidean space]] ℝ&amp;lt;sup&amp;gt;''n''&amp;lt;/sup&amp;gt; has Hausdorff dimension ''n'', and the circle '''S'''&amp;lt;sup&amp;gt;1&amp;lt;/sup&amp;gt; has Hausdorff dimension 1.&amp;lt;ref name=&amp;quot;schleicher&amp;quot; /&amp;gt;&lt;br /&gt;
*[[教育空间]] ℝ&amp;lt;sup&amp;gt;''n''&amp;lt;/sup&amp;gt; 有豪斯多夫维数 ''n''，循环'''S'''&amp;lt;sup&amp;gt;1&amp;lt;/sup&amp;gt; 拥有豪斯多夫维数1.&amp;lt;ref name=&amp;quot;schleicher&amp;quot; /&amp;gt;&lt;br /&gt;
* [[Fractal]]s often are spaces whose Hausdorff dimension strictly exceeds the [[topological dimension]].&amp;lt;ref name=&amp;quot;mandelbrot&amp;quot; /&amp;gt; For example, the [[Cantor set]], a zero-dimensional topological space, is a union of two copies of itself, each copy shrunk by a factor 1/3; hence, it can be shown that its Hausdorff dimension is ln(2)/ln(3)&amp;amp;nbsp;≈&amp;amp;nbsp;0.63.&amp;lt;ref&amp;gt;{{cite book | last=Falconer | first = Kenneth |title=Fractal Geometry: Mathematical Foundations and Applications | publisher=[[John Wiley and Sons]] | edition=2nd | year=2003}}&amp;lt;/ref&amp;gt; The [[Sierpinski triangle]] is a union of three copies of itself, each copy shrunk by a factor of&amp;amp;nbsp;1/2; this yields a Hausdorff dimension of ln(3)/ln(2)&amp;amp;nbsp;≈&amp;amp;nbsp;1.58.&amp;lt;ref name=CampbellAnnenberg15/&amp;gt; These Hausdorff dimensions are related to the &amp;quot;critical exponent&amp;quot; of the [[Master theorem (analysis of algorithms)|Master theorem]] for solving [[Recurrence relation|recurrence relations]] in the [[analysis of algorithms]].&lt;br /&gt;
*[[分形]]一般是那些豪斯多夫维数直接超过其拓扑维数的空间。例如[[康托尔集]]是一个o维拓扑空间，由两个自己复制而成，每一个复制品都是原来的三分之一，因此它的豪斯多夫维数是 ln(2)/ln(3)&amp;amp;nbsp;≈&amp;amp;nbsp;0.63。&amp;lt;ref&amp;gt;{{cite book | last=Falconer | first = Kenneth |title=Fractal Geometry: Mathematical Foundations and Applications | publisher=[[John Wiley and Sons]] | edition=2nd | year=2003}}&amp;lt;/ref&amp;gt;一个[[谢尔宾斯基三角]]是他自身三个复制的组合。每一个是原来的&amp;amp;nbsp;1/2，它的豪斯多夫维数ln(3)/ln(2)&amp;amp;nbsp;≈&amp;amp;nbsp;1.58。&amp;lt;ref name=CampbellAnnenberg15/&amp;gt;在递归算法中解决递归关系时，这些豪斯多夫维数与[[算法分析主定理]]的临界指标相联系。&lt;br /&gt;
* [[Space-filling curve]]s like the [[Peano curve]] have the same Hausdorff dimension as the space they fill.&lt;br /&gt;
*[[空间填充曲线]]拥有和他们填充空间同样的豪斯多夫维数，如[[皮亚诺曲线]]。&lt;br /&gt;
* The trajectory of [[Brownian motion]] in dimension 2 and above is conjectured to be Hausdorff dimension 2.&amp;lt;ref&amp;gt;{{cite book | last=Morters | first=Peres | title= Brownian Motion | publisher=[[Cambridge University Press]] | year=2010 }}&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
[[image:Great Britain Hausdorff.svg|thumb|250px|Estimating the Hausdorff dimension of the [[How Long Is the Coast of Britain? Statistical Self-Similarity and Fractional Dimension|coast of Great Britain]]]]&lt;br /&gt;
&lt;br /&gt;
coast of Great Britain]]&lt;br /&gt;
&lt;br /&gt;
[[大不列颠海岸&lt;br /&gt;
&lt;br /&gt;
* 刘易斯·弗赖伊·理查森[[Lewis Fry Richardson]] has performed detailed experiments to measure the approximate Hausdorff dimension for various coastlines. His results have varied from 1.02 for the coastline of [[South Africa]] to 1.25 for the west coast of [[Great Britain]].&amp;lt;ref name=&amp;quot;mandelbrot&amp;quot; /&amp;gt;&lt;br /&gt;
*刘易斯·弗赖伊·理查森（Lewis Fry Richardson）已经通过豪斯多夫维数去测量了很多海岸线。它的结果涵盖从1.02的南非海岸线到1.25的大英帝国西海岸模型。]]&lt;br /&gt;
&lt;br /&gt;
==Properties of Hausdorff dimension豪斯多夫维数特性==&lt;br /&gt;
&lt;br /&gt;
{{refimprove section|date=March 2015}}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
=== Hausdorff dimension and inductive dimension 豪斯多夫维数和归纳维数===&lt;br /&gt;
&lt;br /&gt;
Let ''X'' be an arbitrary [[Separable space|separable]] metric space. There is a [[topology|topological]] notion of [[inductive dimension]] for ''X'' which is defined recursively. It is always an integer (or +∞) and is denoted dim&amp;lt;sub&amp;gt;ind&amp;lt;/sub&amp;gt;(''X'').&lt;br /&gt;
&lt;br /&gt;
Let X be an arbitrary separable metric space. There is a topological notion of inductive dimension for X which is defined recursively. It is always an integer (or +∞) and is denoted dim&amp;lt;sub&amp;gt;ind&amp;lt;/sub&amp;gt;(X).&lt;br /&gt;
&lt;br /&gt;
设''X'' 是[[任意可分度量空间]]。对于''X'' 有一个递归定义的归纳维数拓扑概念。它总是一个整数(或 + ∞) ，并且表示dim&amp;lt;sub&amp;gt;ind&amp;lt;/sub&amp;gt;(''X'')。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
'''Theorem'''. Suppose ''X'' is non-empty. Then &lt;br /&gt;
&lt;br /&gt;
Theorem. Suppose X is non-empty. Then &lt;br /&gt;
&lt;br /&gt;
'''定理'''：假设''X'' 是非空的。那么&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt; \dim_{\mathrm{Haus}}(X) \geq \dim_{\operatorname{ind}}(X). &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \dim_{\mathrm{Haus}}(X) \geq \dim_{\operatorname{ind}}(X). &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Moreover,&lt;br /&gt;
&lt;br /&gt;
Moreover,&lt;br /&gt;
&lt;br /&gt;
此外,&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \inf_Y \dim_{\operatorname{Haus}}(Y) =\dim_{\operatorname{ind}}(X), &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \inf_Y \dim_{\operatorname{Haus}}(Y) =\dim_{\operatorname{ind}}(X), &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
where ''Y'' ranges over metric spaces [[homeomorphic]] to ''X''. In other words, ''X'' and ''Y'' have the same underlying set of points and the metric ''d''&amp;lt;sub&amp;gt;''Y''&amp;lt;/sub&amp;gt; of ''Y'' is topologically equivalent to ''d''&amp;lt;sub&amp;gt;''X''&amp;lt;/sub&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
where Y ranges over metric spaces homeomorphic to X. In other words, X and Y have the same underlying set of points and the metric d&amp;lt;sub&amp;gt;Y&amp;lt;/sub&amp;gt; of Y is topologically equivalent to d&amp;lt;sub&amp;gt;X&amp;lt;/sub&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
其中''Y''是度量空间同胚到 ''X''的范围。换句话说， ''X''和 ''Y''具有相同的基本点集，''Y''的度规''d''&amp;lt;sub&amp;gt;''Y''&amp;lt;/sub&amp;gt; 的子拓扑等价于''d''&amp;lt;sub&amp;gt;''X''&amp;lt;/sub&amp;gt;。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
These results were originally established by [[Edward Szpilrajn]] (1907–1976), e.g., see Hurewicz and Wallman, Chapter VII.{{full citation needed|date=March 2015}}&lt;br /&gt;
&lt;br /&gt;
These results were originally established by Edward Szpilrajn (1907–1976), e.g., see Hurewicz and Wallman, Chapter VII.&lt;br /&gt;
&lt;br /&gt;
这些结果最初是由 [[Edward Szpilrajn]] (1907–1976)建立的,  参见 Hurewicz and Wallman, Chapter VII.{{full citation needed|date=March 2015}}第七章。&lt;br /&gt;
&lt;br /&gt;
=== Hausdorff dimension and Minkowski dimension 豪斯多夫维数和闵可夫斯基维度===&lt;br /&gt;
&lt;br /&gt;
The [[Minkowski dimension]] is similar to, and at least as large as, the Hausdorff dimension, and they are equal in many situations. However, the set of [[rational number|rational]] points in [0, 1] has Hausdorff dimension zero and Minkowski dimension one. There are also compact sets for which the Minkowski dimension is strictly larger than the Hausdorff dimension.&lt;br /&gt;
&lt;br /&gt;
The Minkowski dimension is similar to, and at least as large as, the Hausdorff dimension, and they are equal in many situations. However, the set of rational points in [0, 1] has Hausdorff dimension zero and Minkowski dimension one. There are also compact sets for which the Minkowski dimension is strictly larger than the Hausdorff dimension.&lt;br /&gt;
&lt;br /&gt;
[[闵可夫斯基维数]]与豪斯多夫维数相似，至少和它一样大，而且在许多情况下是相等的。然而，[0,1]中有理点集的豪斯多夫维数为0，闵可夫斯基维数为1。还有一些紧集的闵可夫斯基维数绝对大于豪斯多夫维数。&lt;br /&gt;
&lt;br /&gt;
=== Hausdorff dimensions and Frostman measures 豪斯多夫维度和弗洛斯曼测度===&lt;br /&gt;
&lt;br /&gt;
If there is a [[measure (mathematics)|measure]] μ defined on [[Borel measure|Borel]] subsets of a metric space ''X'' such that ''μ''(''X'') &amp;gt; 0 and ''μ''(''B''(''x'', ''r'')) ≤ ''r&amp;lt;sup&amp;gt;s&amp;lt;/sup&amp;gt;'' holds for some constant ''s'' &amp;gt; 0 and for every ball ''B''(''x'', ''r'') in ''X'', then dim&amp;lt;sub&amp;gt;Haus&amp;lt;/sub&amp;gt;(''X'') ≥ ''s''. A partial converse is provided by [[Frostman's lemma]].{{citation needed|date=March 2015}}&amp;lt;ref&amp;gt;This Wikipedia article also discusses further useful characterizations of the Hausdorff dimension.{{clarify|date=March 2015}}&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
If there is a measure μ defined on Borel subsets of a metric space X such that μ(X) &amp;gt; 0 and μ(B(x, r)) ≤ r&amp;lt;sup&amp;gt;s&amp;lt;/sup&amp;gt; holds for some constant s &amp;gt; 0 and for every ball B(x, r) in X, then dim&amp;lt;sub&amp;gt;Haus&amp;lt;/sub&amp;gt;(X) ≥ s. A partial converse is provided by Frostman's lemma.&lt;br /&gt;
&lt;br /&gt;
如果在度量空间 ''X'' 的 Borel 子集上定义一个测度 μ，使得''μ''(''X'') &amp;gt; 0 和''μ''(''B''(''x'', ''r'')) ≤ ''r&amp;lt;sup&amp;gt;s&amp;lt;/sup&amp;gt;''，对于某个常数 ''s'' &amp;gt; 0  和 ''X'' 中的每个球 ''B''(''x'', ''r'') 成立，则 dim&amp;lt;sub&amp;gt;Haus&amp;lt;/sub&amp;gt;(''X'') ≥ ''s'' 。 部分逆向转换由弗洛斯曼引理定义。&lt;br /&gt;
&lt;br /&gt;
=== Behaviour under unions and products ===&lt;br /&gt;
&lt;br /&gt;
If &amp;lt;math&amp;gt;X=\bigcup_{i\in I}X_i&amp;lt;/math&amp;gt; is a finite or countable union, then&lt;br /&gt;
&lt;br /&gt;
If &amp;lt;math&amp;gt;X=\bigcup_{i\in I}X_i&amp;lt;/math&amp;gt; is a finite or countable union, then&lt;br /&gt;
&lt;br /&gt;
如果 &amp;lt;math&amp;gt;X=\bigcup_{i\in I}X_i&amp;lt;/math&amp;gt; 是一个有限或可数的联合，则&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \dim_{\operatorname{Haus}}(X) =\sup_{i\in I} \dim_{\operatorname{Haus}}(X_i).&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \dim_{\operatorname{Haus}}(X) =\sup_{i\in I} \dim_{\operatorname{Haus}}(X_i).&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
This can be verified directly from the definition.&lt;br /&gt;
&lt;br /&gt;
This can be verified directly from the definition.&lt;br /&gt;
&lt;br /&gt;
这可以直接从定义得到验证。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
If ''X'' and ''Y'' are non-empty metric spaces, then the Hausdorff dimension of their product satisfies&amp;lt;ref&amp;gt;{{cite journal |author=Marstrand, J. M. |title=The dimension of Cartesian product sets |journal=Proc. Cambridge Philos. Soc. |volume=50 |issue=3 |pages=198–202 |year=1954 |doi=10.1017/S0305004100029236 |bibcode = 1954PCPS...50..198M }}&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
If X and Y are non-empty metric spaces, then the Hausdorff dimension of their product satisfies&lt;br /&gt;
&lt;br /&gt;
如果 ''X'' 和''Y''是非空度量空间，那么它们乘积的豪斯多夫维数满足&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt; \dim_{\operatorname{Haus}}(X\times Y)\ge \dim_{\operatorname{Haus}}(X)+ \dim_{\operatorname{Haus}}(Y).&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \dim_{\operatorname{Haus}}(X\times Y)\ge \dim_{\operatorname{Haus}}(X)+ \dim_{\operatorname{Haus}}(Y).&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
This inequality can be strict. It is possible to find two sets of dimension 0 whose product has dimension 1.&amp;lt;ref&amp;gt;{{cite book  | last = Falconer  | first = Kenneth J.  | title = Fractal geometry. Mathematical foundations and applications  | publisher = John Wiley &amp;amp; Sons, Inc., Hoboken, New Jersey  | year = 2003  | doi =   | isbn = }}&amp;lt;/ref&amp;gt; In the opposite direction, it is known that when ''X'' and ''Y'' are Borel subsets of '''R'''&amp;lt;sup&amp;gt;''n''&amp;lt;/sup&amp;gt;, the Hausdorff dimension of ''X'' × ''Y'' is bounded from above by the Hausdorff dimension of ''X'' plus the [[packing dimension|upper packing dimension]] of ''Y''. These facts are discussed in Mattila (1995).&lt;br /&gt;
&lt;br /&gt;
This inequality can be strict. It is possible to find two sets of dimension 0 whose product has dimension 1. In the opposite direction, it is known that when X and Y are Borel subsets of R&amp;lt;sup&amp;gt;n&amp;lt;/sup&amp;gt;, the Hausdorff dimension of X × Y is bounded from above by the Hausdorff dimension of X plus the upper packing dimension of Y. These facts are discussed in Mattila (1995).&lt;br /&gt;
&lt;br /&gt;
这种不平等可以是绝对的。有可能找到两个维数为0的集合，其乘积的维数为1。相反，我们知道当''X''和''Y''是 '''R'''&amp;lt;sup&amp;gt;''n''&amp;lt;/sup&amp;gt;的 Borel 子集时， ''X'' × ''Y''的豪斯多夫维数从上面以 ''X''的豪斯多夫维数加上 ''Y''的填充维数为界。Mattila (1995)曾就这些情况进行了讨论。&lt;br /&gt;
&lt;br /&gt;
==Self-similar sets自相似集合==&lt;br /&gt;
&lt;br /&gt;
{{refimprove section|date=March 2015}}&lt;br /&gt;
&lt;br /&gt;
Many sets defined by a self-similarity condition have dimensions which can be determined explicitly. Roughly, a set ''E'' is self-similar if it is the fixed point of a set-valued transformation ψ, that is ψ(''E'') = ''E'', although the exact definition is given below.&lt;br /&gt;
&lt;br /&gt;
Many sets defined by a self-similarity condition have dimensions which can be determined explicitly. Roughly, a set E is self-similar if it is the fixed point of a set-valued transformation ψ, that is ψ(E) = E, although the exact definition is given below.&lt;br /&gt;
&lt;br /&gt;
许多由自相似条件定义的集合具有可以显式确定的维数。粗略地说，集合''E'' 是自相似的，如果它是集值ψ变换的不动点，即ψ(''E'') = ''E''，尽管下面给出了确切的定义。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&amp;lt;blockquote&amp;gt;'''Theorem'''. Suppose&lt;br /&gt;
&lt;br /&gt;
&amp;lt;blockquote&amp;gt;Theorem. Suppose&lt;br /&gt;
&lt;br /&gt;
&amp;lt;blockquote&amp;gt;'''定理'''：假设&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt; \psi_i: \mathbf{R}^n \rightarrow \mathbf{R}^n, \quad i=1, \ldots , m &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \psi_i: \mathbf{R}^n \rightarrow \mathbf{R}^n, \quad i=1, \ldots , m &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
are [[Contraction mapping|contractive]] mappings on '''R'''&amp;lt;sup&amp;gt;''n''&amp;lt;/sup&amp;gt; with contraction constant ''r&amp;lt;sub&amp;gt;j&amp;lt;/sub&amp;gt;'' &amp;lt; 1. Then there is a unique ''non-empty'' compact set ''A'' such that&lt;br /&gt;
&lt;br /&gt;
are contractive mappings on R&amp;lt;sup&amp;gt;n&amp;lt;/sup&amp;gt; with contraction constant r&amp;lt;sub&amp;gt;j&amp;lt;/sub&amp;gt; &amp;lt; 1. Then there is a unique non-empty compact set A such that&lt;br /&gt;
&lt;br /&gt;
是'''R'''&amp;lt;sup&amp;gt;''n''&amp;lt;/sup&amp;gt;上的压缩常数''r&amp;lt;sub&amp;gt;j&amp;lt;/sub&amp;gt;'&amp;lt; 1的压缩映射。然后有一个唯一的非空紧集A &lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt; A = \bigcup_{i=1}^m \psi_i (A). &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; A = \bigcup_{i=1}^m \psi_i (A). &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&amp;lt;/blockquote&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;/blockquote&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The theorem follows from [[Stefan Banach]]'s [[Contractive mapping theorem|contractive mapping fixed point theorem]] applied to the complete metric space of non-empty compact subsets of '''R'''&amp;lt;sup&amp;gt;''n''&amp;lt;/sup&amp;gt; with the [[Hausdorff distance]].&amp;lt;ref&amp;gt;{{cite book |author=Falconer, K. J. |title=The Geometry of Fractal Sets |publisher=Cambridge University Press |location=Cambridge, UK |year=1985 |isbn=0-521-25694-1 |chapter=Theorem 8.3}}&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
The theorem follows from Stefan Banach's contractive mapping fixed point theorem applied to the complete metric space of non-empty compact subsets of R&amp;lt;sup&amp;gt;n&amp;lt;/sup&amp;gt; with the Hausdorff distance.&lt;br /&gt;
&lt;br /&gt;
这个定理来源于 Stefan Banach 的压缩映射不动点定理，该定理应用于 '''R'''&amp;lt;sup&amp;gt;''n''&amp;lt;/sup&amp;gt; 的非空紧子集的完备空间豪斯多夫距离。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
===The open set condition开集条件===&lt;br /&gt;
&lt;br /&gt;
To determine the dimension of the self-similar set ''A'' (in certain cases), we need a technical condition called the ''open set condition'' (OSC) on the sequence of contractions ψ&amp;lt;sub&amp;gt;''i''&amp;lt;/sub&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
To determine the dimension of the self-similar set A (in certain cases), we need a technical condition called the open set condition (OSC) on the sequence of contractions ψ&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
为了确定自相似集''A'' 的维数(在某些情况下) ，我们需要一个称为''开集条件''(OSC)的技术条件ψ&amp;lt;sub&amp;gt;''i''&amp;lt;/sub&amp;gt;。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
There is a relatively compact open set ''V'' such that&lt;br /&gt;
&lt;br /&gt;
There is a relatively compact open set V such that&lt;br /&gt;
&lt;br /&gt;
有一个相对紧的开集''V''&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt; \bigcup_{i=1}^m\psi_i (V) \subseteq V, &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \bigcup_{i=1}^m\psi_i (V) \subseteq V, &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
where the sets in union on the left are pairwise [[disjoint sets|disjoint]].&lt;br /&gt;
&lt;br /&gt;
where the sets in union on the left are pairwise disjoint.&lt;br /&gt;
&lt;br /&gt;
左边的集合是成对不相交的。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The open set condition is a separation condition that ensures the images ψ&amp;lt;sub&amp;gt;''i''&amp;lt;/sub&amp;gt;(''V'') do not overlap &amp;quot;too much&amp;quot;.&lt;br /&gt;
&lt;br /&gt;
The open set condition is a separation condition that ensures the images ψ&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;(V) do not overlap &amp;quot;too much&amp;quot;.&lt;br /&gt;
&lt;br /&gt;
开集条件是保证图像子ψ&amp;lt;sub&amp;gt;''i''&amp;lt;/sub&amp;gt;(''V'') 不重叠“太多”的分离条件。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
'''Theorem'''. Suppose the open set condition holds and each ψ&amp;lt;sub&amp;gt;''i''&amp;lt;/sub&amp;gt; is a similitude, that is a composition of an [[isometry]] and a [[dilation (metric space)|dilation]] around some point. Then the unique fixed point of ψ is a set whose Hausdorff dimension is ''s'' where ''s'' is the unique solution of&amp;lt;ref&amp;gt;{{cite journal | last=Hutchinson | first=John E. | title=Fractals and self similarity | journal=Indiana Univ. Math. J. | volume=30 | year=1981 | pages=713–747 | doi=10.1512/iumj.1981.30.30055 | issue=5 | doi-access=free }}&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
Theorem. Suppose the open set condition holds and each ψ&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt; is a similitude, that is a composition of an isometry and a dilation around some point. Then the unique fixed point of ψ is a set whose Hausdorff dimension is s where s is the unique solution of&lt;br /&gt;
&lt;br /&gt;
'''定理'''假设开集条件成立，并且每个ψ&amp;lt;sub&amp;gt;''i''&amp;lt;/sub&amp;gt; 是一个相似量，这是一个等距和围绕某一点的膨胀的合成。那么唯一的不动点是一个集合，它的豪斯多夫维数是 ''s'' ，其中  ''s'' 是 ''s'' &amp;lt;ref&amp;gt;{{cite journal | last=Hutchinson | first=John E. | title=Fractals and self similarity | journal=Indiana Univ. Math. J. | volume=30 | year=1981 | pages=713–747 | doi=10.1512/iumj.1981.30.30055 | issue=5 | doi-access=free }}&amp;lt;/ref&amp;gt;的唯一解&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt; \sum_{i=1}^m r_i^s = 1. &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \sum_{i=1}^m r_i^s = 1. &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The contraction coefficient of a similitude is the magnitude of the dilation.&lt;br /&gt;
&lt;br /&gt;
The contraction coefficient of a similitude is the magnitude of the dilation.&lt;br /&gt;
&lt;br /&gt;
相似物的收缩系数就是膨胀的大小。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
We can use this theorem to compute the Hausdorff dimension of the Sierpinski triangle (or sometimes called Sierpinski gasket). Consider three [[non-collinear points]] ''a''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;, ''a''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;, ''a''&amp;lt;sub&amp;gt;3&amp;lt;/sub&amp;gt; in the plane '''R'''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; and let ψ&amp;lt;sub&amp;gt;''i''&amp;lt;/sub&amp;gt; be the dilation of ratio 1/2 around ''a&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;''. The unique non-empty fixed point of the corresponding mapping ψ is a Sierpinski gasket and the dimension ''s'' is the unique solution of&lt;br /&gt;
&lt;br /&gt;
We can use this theorem to compute the Hausdorff dimension of the Sierpinski triangle (or sometimes called Sierpinski gasket). Consider three non-collinear points a&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;, a&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;, a&amp;lt;sub&amp;gt;3&amp;lt;/sub&amp;gt; in the plane R&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; and let ψ&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt; be the dilation of ratio 1/2 around a&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;. The unique non-empty fixed point of the corresponding mapping ψ is a Sierpinski gasket and the dimension s is the unique solution of&lt;br /&gt;
&lt;br /&gt;
我们可以使用这个定理来计算谢尔宾斯基三角形的豪斯多夫维数(或者有时候叫做谢尔宾斯基垫圈)。考虑R&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; 平面上的三个非共线点，''a''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;，''a''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;，''a''&amp;lt;sub&amp;gt;3&amp;lt;/sub&amp;gt;，让ψ&amp;lt;sub&amp;gt;''i''&amp;lt;/sub&amp;gt;是围绕着''a&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;''膨胀比率的1/2。对应映射的唯一非空不动点是一个谢尔宾斯基垫圈，其维数''s''是对应映射的唯一解&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt; \left(\frac{1}{2}\right)^s+\left(\frac{1}{2}\right)^s+\left(\frac{1}{2}\right)^s = 3 \left(\frac{1}{2}\right)^s =1. &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \left(\frac{1}{2}\right)^s+\left(\frac{1}{2}\right)^s+\left(\frac{1}{2}\right)^s = 3 \left(\frac{1}{2}\right)^s =1. &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Taking [[natural logarithm]]s of both sides of the above equation, we can solve for ''s'', that is: ''s'' = ln(3)/ln(2).  The Sierpinski gasket is self-similar and satisfies the OSC. In general a set ''E'' which is a fixed point of a mapping&lt;br /&gt;
&lt;br /&gt;
Taking natural logarithms of both sides of the above equation, we can solve for s, that is: s = ln(3)/ln(2).  The Sierpinski gasket is self-similar and satisfies the OSC. In general a set E which is a fixed point of a mapping&lt;br /&gt;
&lt;br /&gt;
取上述方程两边的自然对数，我们可以求出 ''s''，即: ''s'' = ln(3)/ln(2)。该密封垫具有自相似性，满足 OSC 要求。一般来说，集合 ''E''是一个映射的不动点&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt; A \mapsto \psi(A) = \bigcup_{i=1}^m \psi_i(A) &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt; A \mapsto \psi(A) = \bigcup_{i=1}^m \psi_i(A) &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
is self-similar if and only if the intersections&lt;br /&gt;
&lt;br /&gt;
is self-similar if and only if the intersections&lt;br /&gt;
&lt;br /&gt;
是自相似的，当且仅当&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt; H^s\left(\psi_i(E) \cap \psi_j(E)\right) =0, &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; H^s\left(\psi_i(E) \cap \psi_j(E)\right) =0, &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
where ''s'' is the Hausdorff dimension of ''E'' and ''H&amp;lt;sup&amp;gt;s&amp;lt;/sup&amp;gt;'' denotes [[Hausdorff measure]]. This is clear in the case of the Sierpinski gasket (the intersections are just points), but is also true more generally:&lt;br /&gt;
&lt;br /&gt;
where s is the Hausdorff dimension of E and H&amp;lt;sup&amp;gt;s&amp;lt;/sup&amp;gt; denotes Hausdorff measure. This is clear in the case of the Sierpinski gasket (the intersections are just points), but is also true more generally:&lt;br /&gt;
&lt;br /&gt;
其中 ''s''是''E''的豪斯多夫维数， ''E'' and ''H&amp;lt;sup&amp;gt;s&amp;lt;/sup&amp;gt;'' 表示 豪斯多夫测度。对于谢尔宾斯基垫圈(交叉点就是点)来说，这一点很明显，但更普遍的情况是:&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
'''Theorem'''. Under the same conditions as the previous theorem, the unique fixed point of ψ is self-similar.&lt;br /&gt;
&lt;br /&gt;
Theorem. Under the same conditions as the previous theorem, the unique fixed point of ψ is self-similar.&lt;br /&gt;
&lt;br /&gt;
'''定理'''：在与前一定理相同的条件下，其唯一不动点是自相似的。&lt;br /&gt;
&lt;br /&gt;
==See also参阅==&lt;br /&gt;
&lt;br /&gt;
* [[List of fractals by Hausdorff dimension豪斯多夫分形维数列表]] Examples of deterministic fractals, random and natural fractals.确定性分形与随机和自然分形的示例。&lt;br /&gt;
&lt;br /&gt;
* [[Assouad dimension  Assouad维数]], another variation of fractal dimension that, like Hausdorff dimension, is defined using coverings by balls其他被球覆盖方式定义的分形维数，例如豪斯多夫维数。&lt;br /&gt;
&lt;br /&gt;
* [[Intrinsic dimension固有维数]]&lt;br /&gt;
&lt;br /&gt;
* [[Packing dimension填充维数]]&lt;br /&gt;
&lt;br /&gt;
* [[Fractal dimension分形维数]]&lt;br /&gt;
&lt;br /&gt;
==References参考文献==&lt;br /&gt;
&lt;br /&gt;
{{reflist}}&lt;br /&gt;
&lt;br /&gt;
==Further reading拓展阅读==&lt;br /&gt;
&lt;br /&gt;
* {{cite book |last1=Dodson |first1=M. Maurice |title=Fractal Geometry and Applications: A Jubilee of Benoît Mandelbrot |volume=72 |issue=1 |pages=305–347 |last2=Kristensen |first2=Simon |chapter=Hausdorff Dimension and Diophantine Approximation |date=June 12, 2003 |arxiv=math/0305399 |bibcode = 2003math......5399D |doi=10.1090/pspum/072.1/2112110|series=Proceedings of Symposia in Pure Mathematics |isbn=9780821836378 }}&lt;br /&gt;
&lt;br /&gt;
* {{cite book |last1=Hurewicz |first1=Witold |authorlink1=Witold Hurewicz |last2=Wallman |first2=Henry |authorlink2=Henry Wallman |title=Dimension Theory |url=https://archive.org/details/in.ernet.dli.2015.84609 |publisher=Princeton University Press |year=1948 }}&lt;br /&gt;
&lt;br /&gt;
* {{cite journal |author作者=E. Szpilrajn |authorlink=Edward Marczewski |title=La dimension et la mesure |journal=Fundamenta Mathematicae |volume=28 |pages=81–9 |year=1937 }}&lt;br /&gt;
&lt;br /&gt;
* {{cite journal&lt;br /&gt;
&lt;br /&gt;
 | last1=Marstrand&lt;br /&gt;
&lt;br /&gt;
 | last1=Marstrand&lt;br /&gt;
&lt;br /&gt;
 | last1=马斯特兰德&lt;br /&gt;
&lt;br /&gt;
 | first1=J. M. | title=The dimension of cartesian product sets | year=1954 | journal=Proc. Cambridge Philos. Soc.&lt;br /&gt;
&lt;br /&gt;
 | first1=J. M. | title=The dimension of cartesian product sets | year=1954 | journal=Proc. Cambridge Philos. Soc.&lt;br /&gt;
&lt;br /&gt;
 | first1= J. M. | title=笛卡儿积集的维数 | 1954年 |  journal=Proc. Cambridge Philos. Soc.&lt;br /&gt;
&lt;br /&gt;
 | volume=50&lt;br /&gt;
&lt;br /&gt;
 | volume=50&lt;br /&gt;
&lt;br /&gt;
 | 第50卷&lt;br /&gt;
&lt;br /&gt;
 | issue=3&lt;br /&gt;
&lt;br /&gt;
 | issue=3&lt;br /&gt;
&lt;br /&gt;
 | 第三期&lt;br /&gt;
&lt;br /&gt;
 | pages=198–202&lt;br /&gt;
&lt;br /&gt;
 | pages=198–202&lt;br /&gt;
&lt;br /&gt;
 | 第198-202页&lt;br /&gt;
&lt;br /&gt;
 | doi=10.1017/S0305004100029236|bibcode = 1954PCPS...50..198M }}&lt;br /&gt;
&lt;br /&gt;
 | doi=10.1017/S0305004100029236|bibcode = 1954PCPS...50..198M }}&lt;br /&gt;
&lt;br /&gt;
10.1017 / S0305004100029236 | bibcode 1954PCPS... 50. . 198 m }&lt;br /&gt;
&lt;br /&gt;
* {{Cite book&lt;br /&gt;
&lt;br /&gt;
 | last1=Mattila&lt;br /&gt;
&lt;br /&gt;
 | last1=Mattila&lt;br /&gt;
&lt;br /&gt;
 | last1=Mattila&lt;br /&gt;
&lt;br /&gt;
 | first1=Pertti | author1-link=Pertti Mattila| title=Geometry of sets and measures in Euclidean spaces | publisher=[[Cambridge University Press]]&lt;br /&gt;
&lt;br /&gt;
 | first1=Pertti | author1-link=Pertti Mattila| title=Geometry of sets and measures in Euclidean spaces | publisher=Cambridge University Press&lt;br /&gt;
&lt;br /&gt;
| first1 Pertti | author1-link Pertti Mattila | title 欧几里德空间中集合和度量的几何 | 出版商剑桥大学出版社&lt;br /&gt;
&lt;br /&gt;
 | isbn=978-0-521-65595-8 | year=1995}}&lt;br /&gt;
&lt;br /&gt;
 | isbn=978-0-521-65595-8 | year=1995}}&lt;br /&gt;
&lt;br /&gt;
| isbn 978-0-521-65595-8 | year 1995}&lt;br /&gt;
&lt;br /&gt;
* {{cite journal |author=A. S. Besicovitch |authorlink=A. S. Besicovitch |title=On Linear Sets of Points of Fractional Dimensions |journal=[[Mathematische Annalen]] |volume=101 |year=1929 | doi=10.1007/BF01454831| issue=1 |pages= 161–193}}&lt;br /&gt;
&lt;br /&gt;
* {{cite journal |author1=A. S. Besicovitch |authorlink1=A. S. Besicovitch |author2=H. D. Ursell |authorlink2=H. D. Ursell |title=Sets of Fractional Dimensions |journal=Journal of the London Mathematical Society |volume=12 |year=1937 | issue=1 | doi=10.1112/jlms/s1-12.45.18  | pages=18–25 }}&amp;lt;br/&amp;gt;Several selections from this volume are reprinted in {{cite book |author=Edgar, Gerald A. |title=Classics on fractals |publisher=Addison-Wesley |location=Boston |year=1993 |isbn=0-201-58701-7}} See chapters 9,10,11&lt;br /&gt;
&lt;br /&gt;
* {{cite journal |author=F. Hausdorff |authorlink=F. Hausdorff |title=Dimension und äußeres Maß |journal=Mathematische Annalen |volume=79 |issue=1–2 |pages=157–179 |date=March 1919 |doi=10.1007/BF01457179|hdl=10338.dmlcz/100363 |url=http://dml.cz/bitstream/handle/10338.dmlcz/100363/CzechMathJ_09-1959-3_5.pdf }}&lt;br /&gt;
&lt;br /&gt;
* {{cite journal | last=Hutchinson | first=John E. | title=Fractals and self similarity | journal=Indiana Univ. Math. J. | volume=30 | year=1981 | pages=713–747 | doi=10.1512/iumj.1981.30.30055 | issue=5 | doi-access=free }}&lt;br /&gt;
&lt;br /&gt;
*{{cite book | last=Falconer | first = Kenneth |title=Fractal Geometry: Mathematical Foundations and Applications | publisher=[[John Wiley and Sons]] | edition=2nd | year=2003}}&lt;br /&gt;
&lt;br /&gt;
==External links外部链接==&lt;br /&gt;
&lt;br /&gt;
* [https://www.encyclopediaofmath.org/index.php/Hausdorff_dimension Hausdorff dimension] 在 [https://www.encyclopediaofmath.org/ Encyclopedia of Mathematics]&lt;br /&gt;
&lt;br /&gt;
* [https://www.encyclopediaofmath.org/index.php/Hausdorff_measure Hausdorff measure] 在 [https://www.encyclopediaofmath.org/ Encyclopedia of Mathematics]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{{DEFAULTSORT:Hausdorff Dimension豪斯多夫维数}}&lt;br /&gt;
&lt;br /&gt;
[[Category分类:Fractals分形]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[Category分类:Metric geometry度量几何]]&lt;br /&gt;
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&lt;br /&gt;
&lt;br /&gt;
[[Category分类:Dimension theory维度理论]]&lt;br /&gt;
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&lt;br /&gt;
&amp;lt;noinclude&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;small&amp;gt;This page was moved from [[wikipedia:en:Hausdorff dimension]]. Its edit history can be viewed at [[分形维数/edithistory]]&amp;lt;/small&amp;gt;&amp;lt;/noinclude&amp;gt;&lt;br /&gt;
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[[Category:待整理页面]]&lt;/div&gt;</summary>
		<author><name>Ruili</name></author>
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		<title>分形维数</title>
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		<updated>2020-11-01T09:44:51Z</updated>

		<summary type="html">&lt;p&gt;Ruili：&lt;/p&gt;
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&lt;div&gt;此词条暂由彩云小译翻译，未经人工整理和审校，带来阅读不便，请见谅。&lt;br /&gt;
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Example of non-integer dimensions. The first four [[iteration]]s of the [[Koch snowflake|Koch curve]], where after each iteration, all original line segments are replaced with four, each a self-similar copy that is 1/3 the length of the original. One formalism of the Hausdorff dimension uses this scale factor (3) and the number of self-similar objects (4) to calculate the dimension, D, after the first iteration to be D = (log N)/(log S) = (log 4)/(log 3) ≈ 1.26.&amp;lt;ref name=CampbellAnnenberg15&amp;gt;MacGregor Campbell, 2013, &amp;quot;5.6 Scaling and the Hausdorff Dimension,&amp;quot; at ''Annenberg Learner:MATHematics illuminated'', see [http://www.learner.org/courses/mathilluminated/units/5/textbook/06.php], accessed 5 March 2015.&amp;lt;/ref&amp;gt; That is, while the Hausdorff dimension of a single [[point (geometry)|point]] is zero, of a [[line segment]] is 1, of a [[square]] is 2, and of a [[cube]] is 3, for [[fractal]]s such as this, the object can have a non-integer dimension.&lt;br /&gt;
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Example of non-integer dimensions. The first four iterations of the Koch curve, where after each iteration, all original line segments are replaced with four, each a self-similar copy that is 1/3 the length of the original. One formalism of the Hausdorff dimension uses this scale factor (3) and the number of self-similar objects (4) to calculate the dimension, D, after the first iteration to be D = (log N)/(log S) = (log 4)/(log 3) ≈ 1.26. That is, while the Hausdorff dimension of a single point is zero, of a line segment is 1, of a square is 2, and of a cube is 3, for fractals such as this, the object can have a non-integer dimension.&lt;br /&gt;
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非整数维度示例：前四个[[Koch 曲线]]的迭代，在每次迭代后，所有原始线段都被替换为四个，每个自相似的复制是原始线段长度的1 / 3。豪斯多夫维数的一个建模是使用比例因子(3)和自相似对象的数量(4)来计算维度 D，在第一次迭代后为 D = (log N)/(log S) = (log 4)/(log 3) ≈ 1.26.&amp;lt;ref name=CampbellAnnenberg15&amp;gt;。MacGregor Campbell, 2013, &amp;quot;5.6 Scaling and the Hausdorff Dimension,&amp;quot; 在 ''Annenberg Learner:MATHematics illuminated'', 参见 [http://www.learner.org/courses/mathilluminated/units/5/textbook/06.php], accessed 5 March 2015.&amp;lt;/ref&amp;gt; 也就是说，单点的豪斯多夫维数为零，线段为1，正方形为2，立方体为3时，但对于分形，对象可以有一个非整数维度。&lt;br /&gt;
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In [[mathematics]], '''Hausdorff dimension''' is a measure of ''roughness'', or more specifically, [[fractal dimension]], that was first introduced in 1918 by [[mathematician]] [[Felix Hausdorff]].&amp;lt;ref&amp;gt;{{Cite journal |arxiv = 1101.1444|doi = 10.1214/11-STS370|title = Estimators of Fractal Dimension: Assessing the Roughness of Time Series and Spatial Data|journal = Statistical Science|volume = 27|issue = 2|pages = 247–277|year = 2012|last1 = Gneiting|first1 = Tilmann|last2 = Ševčíková|first2 = Hana|last3 = Percival|first3 = Donald B.}}&amp;lt;/ref&amp;gt; For instance, the Hausdorff dimension of a single [[point (geometry)|point]] is zero, of a [[line segment]] is 1, of a [[square]] is 2, and of a [[cube]] is 3. That is, for sets of points that define a smooth shape or a shape that has a small number of corners—the shapes of traditional geometry and science—the Hausdorff dimension is an [[integer]] agreeing with the usual sense of dimension, also known as the [[Inductive dimension|topological dimension]]. However, formulas have also been developed that allow calculation of the dimension of other less simple objects, where, solely on the basis of their properties of [[scaling (geometry)|scaling]] and [[self-similarity]], one is led to the conclusion that particular objects—including [[fractal]]s—have non-integer Hausdorff dimensions. Because of the significant technical advances made by [[Abram Samoilovitch Besicovitch]] allowing computation of dimensions for highly irregular or &amp;quot;rough&amp;quot; sets, this dimension is also commonly referred to as the ''Hausdorff–Besicovitch dimension.''&lt;br /&gt;
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In mathematics, Hausdorff dimension is a measure of roughness, or more specifically, fractal dimension, that was first introduced in 1918 by mathematician Felix Hausdorff. For instance, the Hausdorff dimension of a single point is zero, of a line segment is 1, of a square is 2, and of a cube is 3. That is, for sets of points that define a smooth shape or a shape that has a small number of corners—the shapes of traditional geometry and science—the Hausdorff dimension is an integer agreeing with the usual sense of dimension, also known as the topological dimension. However, formulas have also been developed that allow calculation of the dimension of other less simple objects, where, solely on the basis of their properties of scaling and self-similarity, one is led to the conclusion that particular objects—including fractals—have non-integer Hausdorff dimensions. Because of the significant technical advances made by Abram Samoilovitch Besicovitch allowing computation of dimensions for highly irregular or &amp;quot;rough&amp;quot; sets, this dimension is also commonly referred to as the Hausdorff–Besicovitch dimension.&lt;br /&gt;
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在[[数学]]中，'''&amp;lt;font color = '#ff8000'&amp;gt;豪斯多夫维数Hausdorff dimension&amp;lt;/font&amp;gt;'''是一种粗糙度的度量单位，或者更确切地说，分形维数，是由数学家 Felix Hausdorff 在1918年首次提出的。例如，单点的豪斯多夫维数为零，线段为1，正方形为2，立方体为3。也就是说，对于定义了一个光滑形状或一个有少数几个角的形状---- 传统几何学和科学的形状---- 的点集来说，豪斯多夫维数是一个整数，符合通常的维度意义，也称为拓扑维度。然而，还有一些公式允许计算其他不太简单的对象的维数，其中仅仅根据它们的标度和自相似特性，就可以得出结论: 特定的对象ー包括分形ー具有非整数的 Hausdorff 维数。由于阿布拉姆·萨莫伊洛维奇·贝西科维奇的重大技术进步，允许计算高度不规则或“粗糙”集的维度，这个维度通常也被称为 Hausdorff-Besicovitch 维度。 &lt;br /&gt;
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The Hausdorff dimension, more specifically, is a further dimensional number associated with a given set, where the distances between all members of that set are defined. Such a set is termed a [[metric space]]. The dimension is drawn from the [[Extended real number line|extended real numbers]], &amp;lt;math&amp;gt;\overline{\mathbb{R}}&amp;lt;/math&amp;gt;, as opposed to the more intuitive notion of dimension, which is not associated to general metric spaces, and only takes values in the non-negative integers.&lt;br /&gt;
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The Hausdorff dimension, more specifically, is a further dimensional number associated with a given set, where the distances between all members of that set are defined. Such a set is termed a metric space. The dimension is drawn from the extended real numbers, &amp;lt;math&amp;gt;\overline{\mathbb{R}}&amp;lt;/math&amp;gt;, as opposed to the more intuitive notion of dimension, which is not associated to general metric spaces, and only takes values in the non-negative integers.&lt;br /&gt;
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更具体地说，豪斯多夫维数是一个与给定集合相关联的更进一步的维数，其中定义了该集合所有成员之间的距离。这样的集合称为度量空间。维数是从扩展的实数，&amp;lt;math&amp;gt;\overline{\mathbb{R}}&amp;lt;/math&amp;gt;，而不是更直观的维数概念(它不与一般的度量空间相关联，只取非负整数的值)。&lt;br /&gt;
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In mathematical terms, the Hausdorff dimension generalizes the notion of the dimension of a real [[vector space]]. That is, the Hausdorff dimension of an ''n''-dimensional [[inner product space]] equals ''n''. This underlies the earlier statement that the Hausdorff dimension of a point is zero, of a line is one, etc., and that [[fractal|irregular sets]] can have noninteger Hausdorff dimensions. For instance, the [[Koch snowflake]] shown at right is constructed from an equilateral triangle; in each iteration, its component line segments are divided into 3 segments of unit length, the newly created middle segment is used as the base of a new [[equilateral]] triangle that points outward, and this base segment is then deleted to leave a final object from the iteration of unit length of 4.&amp;lt;ref&amp;gt;Larry Riddle, 2014, &amp;quot;Classic Iterated Function Systems: Koch Snowflake&amp;quot;, Agnes Scott College e-Academy (online), see [http://ecademy.agnesscott.edu/~lriddle/ifs/ksnow/ksnow.htm], accessed 5 March 2015.&amp;lt;/ref&amp;gt; That is, after the first iteration, each original line segment has been replaced with N=4, where each self-similar copy is 1/S = 1/3 as long as the original.&amp;lt;ref name=CampbellAnnenberg15/&amp;gt; Stated another way, we have taken an object with Euclidean dimension, D, and reduced its linear scale by 1/3 in each direction, so that its length increases to N=S&amp;lt;sup&amp;gt;D&amp;lt;/sup&amp;gt;.&amp;lt;ref name=ClaytonSCTPLS96&amp;gt;Keith Clayton, 1996, &amp;quot;Fractals and the Fractal Dimension,&amp;quot; ''Basic Concepts in Nonlinear Dynamics and Chaos'' (workshop), Society for Chaos Theory in Psychology and the Life Sciences annual meeting, June 28, 1996, Berkeley, California, see [http://www.vanderbilt.edu/AnS/psychology/cogsci/chaos/workshop/Workshop.html], accessed 5 March 2015.&amp;lt;/ref&amp;gt; This equation is easily solved for D, yielding the ratio of logarithms (or [[natural logarithm]]s) appearing in the figures, and giving—in the Koch and other fractal cases—non-integer dimensions for these objects.&lt;br /&gt;
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In mathematical terms, the Hausdorff dimension generalizes the notion of the dimension of a real vector space. That is, the Hausdorff dimension of an n-dimensional inner product space equals n. This underlies the earlier statement that the Hausdorff dimension of a point is zero, of a line is one, etc., and that irregular sets can have noninteger Hausdorff dimensions. For instance, the Koch snowflake shown at right is constructed from an equilateral triangle; in each iteration, its component line segments are divided into 3 segments of unit length, the newly created middle segment is used as the base of a new equilateral triangle that points outward, and this base segment is then deleted to leave a final object from the iteration of unit length of 4. That is, after the first iteration, each original line segment has been replaced with N=4, where each self-similar copy is 1/S = 1/3 as long as the original. This equation is easily solved for D, yielding the ratio of logarithms (or natural logarithms) appearing in the figures, and giving—in the Koch and other fractal cases—non-integer dimensions for these objects.&lt;br /&gt;
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用数学术语来说，豪斯多夫维数概括了实向量空间维数的概念。也就是说，n 维内积空间的豪斯多夫维数等于 n。 这就是早期假设的基础，一个点的豪斯多夫维数是零，一条线是一等等，不规则集可以有非整数的豪斯多夫维数。例如，右边所示的 Koch 雪花是由一个正三角形构成的; 在每次迭代中，它的组成线段被分成单位长度的3段，新创建的中间线段被用作一个指向外部的新正三角形的基础，然后人们删除这个基础线段用来保留单位长度4的迭代中的最终对象。也就是说，在第一次迭代之后，每个原始线段都被替换为 N=4，其中每个自相似拷贝的长度是原始线段的1/S = 1/3 。这个方程很容易求解为 D，产生出现在图形中的对数(或自然对数)的比率，并给出——在 Koch 和其他分形情况下——这些对象的非整数维数。&lt;br /&gt;
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The Hausdorff dimension is a successor to the simpler, but usually equivalent, box-counting or [[Minkowski–Bouligand dimension]].&lt;br /&gt;
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The Hausdorff dimension is a successor to the simpler, but usually equivalent, box-counting or Minkowski–Bouligand dimension.&lt;br /&gt;
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豪斯多夫维数是更简单但通常等价的'''&amp;lt;font color = '#ff8000'&amp;gt;计盒维数box-counting&amp;lt;/font&amp;gt;'''或'''&amp;lt;font color = '#ff8000'&amp;gt;闵可夫斯基维数Minkowski-Bouligand&amp;lt;/font&amp;gt;'''的继承者。&lt;br /&gt;
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==Intuition概念==&lt;br /&gt;
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The intuitive concept of dimension of a geometric object ''X'' is the number of independent parameters one needs to pick out a unique point inside. However, any point specified by two parameters can be instead specified by one, because the [[cardinality]] of the [[real plane]] is equal to the cardinality of the [[real line]] (this can be seen by an [[Cantor's diagonal argument|argument]] involving interweaving the digits of two numbers to yield a single number encoding the same information). The example of a [[space-filling curve]] shows that one can even map the real line to the real plane [[Surjective function|surjectively]] (taking one real number into a pair of real numbers in a way so that all pairs of numbers are covered) and ''continuously'', so that a one-dimensional object completely fills up a higher-dimensional object.&lt;br /&gt;
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The intuitive concept of dimension of a geometric object X is the number of independent parameters one needs to pick out a unique point inside. However, any point specified by two parameters can be instead specified by one, because the cardinality of the real plane is equal to the cardinality of the real line (this can be seen by an argument involving interweaving the digits of two numbers to yield a single number encoding the same information). The example of a space-filling curve shows that one can even map the real line to the real plane surjectively (taking one real number into a pair of real numbers in a way so that all pairs of numbers are covered) and continuously, so that a one-dimensional object completely fills up a higher-dimensional object.&lt;br /&gt;
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几何对象X的尺寸的直观概念是指需要多少个独立参数才能找到一个独特的点。但是，任何由两个参数指定的点都可以由一个参数指定，因为为实平面的基数等于实线的基数(这可以通过交织两个数字以产生一个编码相同信息的单个数字看到)。'''&amp;lt;font color = '#ff8000'&amp;gt;皮亚诺曲线&amp;lt;/font&amp;gt;'''的例子表明，可以将实线完美和连续地映射到实平面(把一个实数转换成一对实数，从而覆盖所有实数对)，由此一维对象完全填充了一个高维对象。&lt;br /&gt;
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Every space filling curve hits some points multiple times, and does not have a continuous inverse. It is impossible to map two dimensions onto one in a way that is continuous and continuously invertible. The topological dimension, also called [[Lebesgue covering dimension]], explains why. This dimension is ''n'' if, in every covering of ''X'' by small open balls, there is at least one point where ''n''&amp;amp;nbsp;+&amp;amp;nbsp;1 balls overlap. For example, when one covers a line with short open intervals, some points must be covered twice, giving dimension&amp;amp;nbsp;''n''&amp;amp;nbsp;=&amp;amp;nbsp;1.&lt;br /&gt;
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Every space filling curve hits some points multiple times, and does not have a continuous inverse. It is impossible to map two dimensions onto one in a way that is continuous and continuously invertible. The topological dimension, also called Lebesgue covering dimension, explains why. This dimension is n if, in every covering of X by small open balls, there is at least one point where n&amp;amp;nbsp;+&amp;amp;nbsp;1 balls overlap. For example, when one covers a line with short open intervals, some points must be covered twice, giving dimension&amp;amp;nbsp;n&amp;amp;nbsp;=&amp;amp;nbsp;1.&lt;br /&gt;
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每条空间填充曲线都会多次击中某些点，且不存在连续的逆。将二维以连续和连续可逆的方式映射到一维是不可能的。'''&amp;lt;font color = '#ff8000'&amp;gt;拓扑维度 topological dimension&amp;lt;/font&amp;gt;'''，也被称为Lebesgue覆盖维数，解释了为什么。如果在 x 的每个小开球覆盖中，至少有一个点 n + 1个球重叠，这个维度是 n。例如，当用短的开区间覆盖一条线时，某些点必须被覆盖两次，给出维数''n''&amp;amp;nbsp;=&amp;amp;nbsp;1。&lt;br /&gt;
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But topological dimension is a very crude measure of the local size of a space (size near a point). A curve that is almost space-filling can still have topological dimension one, even if it fills up most of the area of a region. A [[fractal]] has an integer topological dimension, but in terms of the amount of space it takes up, it behaves like a higher-dimensional space.&lt;br /&gt;
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But topological dimension is a very crude measure of the local size of a space (size near a point). A curve that is almost space-filling can still have topological dimension one, even if it fills up most of the area of a region. A fractal has an integer topological dimension, but in terms of the amount of space it takes up, it behaves like a higher-dimensional space.&lt;br /&gt;
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但是，拓扑维度是对空间局部尺寸(点附近的尺寸)的一个非常粗略的度量。一条几乎是空间填充的曲线仍然可以有一维拓扑，即使它填充了一个区域的大部分面积。分形具有整数的拓扑维数，但就其所占空间的数量而言，它看起来像一个更高维的空间。&lt;br /&gt;
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The Hausdorff dimension measures the local size of a space taking into account the distance between points, the [[metric space|metric]]. Consider the number ''N''(''r'') of [[ball (mathematics)|balls]] of radius at most ''r'' required to cover ''X'' completely. When ''r'' is very small, ''N''(''r'') grows polynomially with 1/''r''. For a sufficiently well-behaved  ''X'', the Hausdorff dimension is the unique number ''d'' such that N(''r'') grows as 1/''r&amp;lt;sup&amp;gt;d&amp;lt;/sup&amp;gt;'' as ''r'' approaches zero. More precisely, this defines the [[Minkowski–Bouligand dimension|box-counting dimension]], which equals the Hausdorff dimension when the value ''d'' is a critical boundary between growth rates that are insufficient to cover the space, and growth rates that are overabundant.&lt;br /&gt;
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The Hausdorff dimension measures the local size of a space taking into account the distance between points, the metric. Consider the number N(r) of balls of radius at most r required to cover X completely. When r is very small, N(r) grows polynomially with 1/r. For a sufficiently well-behaved  X, the Hausdorff dimension is the unique number d such that N(r) grows as 1/r&amp;lt;sup&amp;gt;d&amp;lt;/sup&amp;gt; as r approaches zero. More precisely, this defines the box-counting dimension, which equals the Hausdorff dimension when the value d is a critical boundary between growth rates that are insufficient to cover the space, and growth rates that are overabundant.&lt;br /&gt;
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豪斯多夫维数测量一个空间的局部大小时，会考虑到点之间距离的度量。考虑半径最大为 r 的球数 ''N'' (r) ，需要完全覆盖 ''X''。当 r 很小时，n (r)以1/''r'' 增长多项式。对于一个表现足够好的 ''X''，豪斯多夫维数是唯一的数 d，这样当 r 趋近于零时， N(r)增长为1/r&amp;lt;sup&amp;gt;d&amp;lt;/sup&amp;gt; 。更确切地说，这定义了盒子计数维度，当值 d 是不足以覆盖空间的增长率和过度充裕的增长率之间的关键边界时，它等于豪斯多夫维数。&lt;br /&gt;
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For shapes that are smooth, or shapes with a small number of corners, the shapes of traditional geometry and science, the Hausdorff dimension is an integer agreeing with the topological dimension. But [[Benoit Mandelbrot]] observed that [[fractal]]s, sets with noninteger Hausdorff dimensions, are found everywhere in nature. He observed that the proper idealization of most rough shapes you see around you is not in terms of smooth idealized shapes, but in terms of fractal idealized shapes:&lt;br /&gt;
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For shapes that are smooth, or shapes with a small number of corners, the shapes of traditional geometry and science, the Hausdorff dimension is an integer agreeing with the topological dimension. But Benoit Mandelbrot observed that fractals, sets with noninteger Hausdorff dimensions, are found everywhere in nature. He observed that the proper idealization of most rough shapes you see around you is not in terms of smooth idealized shapes, but in terms of fractal idealized shapes:&lt;br /&gt;
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对于光滑的形状，或者有少量棱角的形状，传统几何和科学的形状，豪斯多夫维数是一个整数，与拓扑维度一致。但是伯努·曼德布洛特观察到分形---- 具有非整数豪斯多夫维数的集合---- 在自然界中随处可见。他观察到，我们周围大多数粗糙形状的理想化不是光滑的理想化形状，而是分形理想化形状:&lt;br /&gt;
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&amp;lt;blockquote&amp;gt;Clouds are not spheres, mountains are not cones, coastlines are not circles, and bark is not smooth, nor does lightning travel in a straight line.&amp;lt;ref name=&amp;quot;mandelbrot&amp;quot;&amp;gt;{{cite book   | last = Mandelbrot   | first = Benoît   | authorlink = Benoit Mandelbrot   | title = The Fractal Geometry of Nature   | publisher = W. H. Freeman   | series = Lecture notes in mathematics 1358   | year = 1982   | doi =    | isbn = 0-7167-1186-9   | url-access = registration   | url = https://archive.org/details/fractalgeometryo00beno   }}&amp;lt;/ref&amp;gt;&amp;lt;/blockquote&amp;gt;&lt;br /&gt;
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&amp;lt;blockquote&amp;gt;Clouds are not spheres, mountains are not cones, coastlines are not circles, and bark is not smooth, nor does lightning travel in a straight line.&amp;lt;/blockquote&amp;gt;&lt;br /&gt;
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&amp;lt;blockquote&amp;gt;云不是球体，山不是锥体，海岸线不是圆圈，树皮不平滑，闪电也不是直线运动。 &amp;lt;/blockquote&amp;gt;&lt;br /&gt;
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For fractals that occur in nature, the Hausdorff and [[Minkowski–Bouligand dimension|box-counting dimension]] coincide. The [[packing dimension]] is yet another similar notion which gives the same value for many shapes, but there are well documented exceptions where all these dimensions differ.&lt;br /&gt;
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For fractals that occur in nature, the Hausdorff and box-counting dimension coincide. The packing dimension is yet another similar notion which gives the same value for many shapes, but there are well documented exceptions where all these dimensions differ.&lt;br /&gt;
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对于自然界中出现的分形，豪斯多夫维数和盒计数维数是一致的。封装尺寸是另一个类似的概念，它给出了许多形状相同的值，但是在所有这些尺寸不同的情况，都做了很好的说明。&lt;br /&gt;
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==Formal definitions形式化定义==&lt;br /&gt;
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===Hausdorff content豪斯多夫集===&lt;br /&gt;
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Let ''X'' be a [[metric space]]. If ''S'' ⊂ ''X'' and ''d'' ∈ [0, ∞), the ''d''-dimensional '''unlimited Hausdorff content''' of ''S'' is defined by&lt;br /&gt;
&lt;br /&gt;
Let X be a metric space. If S ⊂ X and d ∈ [0, ∞), the d-dimensional unlimited Hausdorff content of S is defined by&lt;br /&gt;
&lt;br /&gt;
设 ''X''是度量空间。若''S'' ⊂ ''X'' 和 ''d'' ∈ [0, ∞) ，则 ''S'' 的''d''维无限 豪斯多夫集定义为&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt;C_H^d(S):=\inf\Bigl\{\sum_i r_i^d:\text{ there is a cover of } S\text{ by balls with radii }r_i&amp;gt;0\Bigr\}.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt;C_H^d(S):=\inf\Bigl\{\sum_i r_i^d:\text{ there is a cover of } S\text{ by balls with radii }r_i&amp;gt;0\Bigr\}.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt;C_H^d(S):=\inf\Bigl\{\sum_i r_i^d:\text{ there is a cover of } S\text{ by balls with radii }r_i&amp;gt;0\Bigr\}.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
In other words, &amp;lt;math&amp;gt;C_H^d(S)&amp;lt;/math&amp;gt; is the [[infimum]] of the set of numbers &amp;lt;math&amp;gt;\delta \geq 0&amp;lt;/math&amp;gt; such that there is some (indexed) collection of [[ball (mathematics)|ball]]s &amp;lt;math&amp;gt;\{B(x_i,r_i):i\in I\}&amp;lt;/math&amp;gt; covering ''S'' with ''r&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;''&amp;amp;nbsp;&amp;gt;&amp;amp;nbsp;0 for each ''i''&amp;amp;nbsp;∈&amp;amp;nbsp;''I'' that satisfies &amp;lt;math&amp;gt;\sum_{i\in I} r_i^d&amp;lt;\delta &amp;lt;/math&amp;gt;. (Here, we use the standard convention that [[infimum|inf&amp;amp;nbsp;Ø&amp;amp;nbsp;=&amp;amp;nbsp;∞]].)&lt;br /&gt;
&lt;br /&gt;
In other words, &amp;lt;math&amp;gt;C_H^d(S)&amp;lt;/math&amp;gt; is the infimum of the set of numbers &amp;lt;math&amp;gt;\delta \geq 0&amp;lt;/math&amp;gt; such that there is some (indexed) collection of balls &amp;lt;math&amp;gt;\{B(x_i,r_i):i\in I\}&amp;lt;/math&amp;gt; covering S with r&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;&amp;amp;nbsp;&amp;gt;&amp;amp;nbsp;0 for each i&amp;amp;nbsp;∈&amp;amp;nbsp;I that satisfies &amp;lt;math&amp;gt;\sum_{i\in I} r_i^d&amp;lt;\delta &amp;lt;/math&amp;gt;. (Here, we use the standard convention that inf&amp;amp;nbsp;Ø&amp;amp;nbsp;=&amp;amp;nbsp;∞.)&lt;br /&gt;
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换句话说，&amp;lt;math&amp;gt;C_H^d(S)&amp;lt;/math&amp;gt; 是数字集合&amp;lt;math&amp;gt;\delta \geq 0&amp;lt;/math&amp;gt;的下确界，使得在 ''i''&amp;amp;nbsp;∈&amp;amp;nbsp中存在一些球集合 &amp;lt;math&amp;gt;\{B(x_i,r_i):i\in I\}&amp;lt;/math&amp;gt;  i 包含 s，对于每个 ''r&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;''&amp;amp;nbsp;&amp;gt;&amp;amp;nbsp;0 满足 i 中的和&amp;lt;math&amp;gt;\sum_{i\in I} r_i^d&amp;lt;\delta &amp;lt;/math&amp;gt; (在这里，我们使用inf&amp;amp;nbsp;Ø&amp;amp;nbsp;=&amp;amp;nbsp;∞ )的标准约定。&lt;br /&gt;
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===Hausdorff measurement豪斯多夫分形测量===&lt;br /&gt;
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The Hausdorff outer measure is different from the unbounded Hausdorf content in that rather than considering all possible coverings of ''S'', we see what happens when the sizes of the balls go to zero. This is  for &amp;lt;math&amp;gt;d \geq 0 &amp;lt;/math&amp;gt;, we define the ''d''-dimensional Hausdorff outer measure of ''S'' as&lt;br /&gt;
&lt;br /&gt;
The Hausdorff outer measure is different from the unbounded Hausdorf content in that rather than considering all possible coverings of S, we see what happens when the sizes of the balls go to zero. This is  for &amp;lt;math&amp;gt;d \geq 0 &amp;lt;/math&amp;gt;, we define the d-dimensional Hausdorff outer measure of S as&lt;br /&gt;
&lt;br /&gt;
豪斯多夫外测度不同于无界的豪斯多夫，因为我们不考虑 s 的所有可能，我们看到当球的大小为零时会发生什么。这是为了数学  &amp;lt;math&amp;gt;d \geq 0 &amp;lt;/math&amp;gt;，我们定义了  ''S''的 ''d''维豪斯多夫Hausdorff 外测度为&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt; \mathcal{H}^d(S):=\lim_{r \to 0} \inf\Bigl\{\sum_i r_i^d:\text{ there is a cover of } S\text{ by balls with radii } 0 &amp;lt; r_i &amp;lt; r\Bigr\}.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \mathcal{H}^d(S):=\lim_{r \to 0} \inf\Bigl\{\sum_i r_i^d:\text{ there is a cover of } S\text{ by balls with radii } 0 &amp;lt; r_i &amp;lt; r\Bigr\}.&amp;lt;/math&amp;gt;&lt;br /&gt;
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&amp;lt;math&amp;gt; \mathcal{H}^d(S):=\lim_{r \to 0} \inf\Bigl\{\sum_i r_i^d:\text{有一个面} S\text{ 球 } 0 &amp;lt; r_i &amp;lt; r\Bigr\}.&amp;lt;/math&amp;gt;&lt;br /&gt;
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===Hausdorff dimension豪斯多夫维数===&lt;br /&gt;
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The '''Hausdorff dimension''' of ''X'' is defined by&lt;br /&gt;
&lt;br /&gt;
The Hausdorff dimension of X is defined by&lt;br /&gt;
&lt;br /&gt;
X 的豪斯多夫维数定义为&lt;br /&gt;
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:&amp;lt;math&amp;gt;\dim_{\operatorname{H}}(X):=\inf\{d\ge 0: \mathcal{H}^d(X)=0\}.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt;\dim_{\operatorname{H}}(X):=\inf\{d\ge 0: \mathcal{H}^d(X)=0\}.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
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Equivalently, dim&amp;lt;sub&amp;gt;H&amp;lt;/sub&amp;gt;(''X'') may be defined as the [[infimum]] of the set of ''d'' ∈ [0, ∞) such that the ''d''-dimensional [[Hausdorff measure]] of ''X'' is zero. This is the same as the supremum of the set of ''d''&amp;amp;nbsp;∈&amp;amp;nbsp;[0,&amp;amp;nbsp;∞) such that the ''d''-dimensional Hausdorff measure of ''X'' is infinite (except that when this latter set of numbers ''d'' is empty the Hausdorff dimension is zero).&lt;br /&gt;
&lt;br /&gt;
Equivalently, dim&amp;lt;sub&amp;gt;H&amp;lt;/sub&amp;gt;(X) may be defined as the infimum of the set of d ∈ [0, ∞) such that the d-dimensional Hausdorff measure of X is zero. This is the same as the supremum of the set of d&amp;amp;nbsp;∈&amp;amp;nbsp;[0,&amp;amp;nbsp;∞) such that the d-dimensional Hausdorff measure of X is infinite (except that when this latter set of numbers d is empty the Hausdorff dimension is zero).&lt;br /&gt;
&lt;br /&gt;
等价地，dim &amp;lt;sub&amp;gt;H&amp;lt;/sub&amp;gt;(''X'')可定义为 ''d'' ∈ [0, ∞) 集的下确界，使得''X'' 的''d''-维 [[豪斯多夫测度]] 为零。这与 ''d''&amp;amp;nbsp;∈&amp;amp;nbsp;[0,&amp;amp;nbsp;∞)的集合的上确界相同，因此''X''的 d 维豪斯多夫测度是无限的(除非后一个集合 ''d'' 是空的，豪斯多夫维数为零)。&lt;br /&gt;
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==Examples实例==&lt;br /&gt;
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[[Image:Sierpinski deep.svg|thumb|250px|Dimension of a further [[fractal]] example. The [[Sierpinski triangle]], an object with Hausdorff dimension of log(3)/log(2)≈1.58.&amp;lt;ref name=ClaytonSCTPLS96/&amp;gt;]]&lt;br /&gt;
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Dimension of a further [[fractal example. The Sierpinski triangle, an object with Hausdorff dimension of log(3)/log(2)≈1.58.]]&lt;br /&gt;
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[[Image:谢尔宾斯基三角形 deep.svg|thumb|250px|进一步的[[分形维数]]的例子，进一步的分形维数的例子是谢尔宾斯基三角形，它是一个豪斯多夫维数为log(3)/log(2)≈1.58.&amp;lt;ref name=ClaytonSCTPLS96/&amp;gt;的物体]]&lt;br /&gt;
&lt;br /&gt;
* [[Countable set]]s have Hausdorff dimension 0.&amp;lt;ref name=&amp;quot;schleicher&amp;quot;&amp;gt;{{cite journal |last1=Schleicher |first1=Dierk |title=Hausdorff Dimension, Its Properties, and Its Surprises |journal=The American Mathematical Monthly |date=June 2007 |volume=114 |issue=6 |pages=509–528 |doi=10.1080/00029890.2007.11920440 |language=en |issn=0002-9890|arxiv=math/0505099 }}&amp;lt;/ref&amp;gt;&lt;br /&gt;
*[[可数集]]拥有豪斯多夫维数0.&amp;lt;ref name=&amp;quot;schleicher&amp;quot;&amp;gt;{{cite journal |last1=Schleicher |first1=Dierk |title=豪斯多夫维数, Its Properties, and Its Surprises |journal=The American Mathematical Monthly美国数学期刊 |date=June 2007 |volume=114 |issue=6 |pages=509–528 |doi=10.1080/00029890.2007.11920440 |language=en |issn=0002-9890|arxiv=math/0505099 }}&amp;lt;/ref&amp;gt;&lt;br /&gt;
* The [[Euclidean space]] ℝ&amp;lt;sup&amp;gt;''n''&amp;lt;/sup&amp;gt; has Hausdorff dimension ''n'', and the circle '''S'''&amp;lt;sup&amp;gt;1&amp;lt;/sup&amp;gt; has Hausdorff dimension 1.&amp;lt;ref name=&amp;quot;schleicher&amp;quot; /&amp;gt;&lt;br /&gt;
*[[教育空间]] ℝ&amp;lt;sup&amp;gt;''n''&amp;lt;/sup&amp;gt; 有豪斯多夫维数 ''n''，循环'''S'''&amp;lt;sup&amp;gt;1&amp;lt;/sup&amp;gt; 拥有豪斯多夫维数1.&amp;lt;ref name=&amp;quot;schleicher&amp;quot; /&amp;gt;&lt;br /&gt;
* [[Fractal]]s often are spaces whose Hausdorff dimension strictly exceeds the [[topological dimension]].&amp;lt;ref name=&amp;quot;mandelbrot&amp;quot; /&amp;gt; For example, the [[Cantor set]], a zero-dimensional topological space, is a union of two copies of itself, each copy shrunk by a factor 1/3; hence, it can be shown that its Hausdorff dimension is ln(2)/ln(3)&amp;amp;nbsp;≈&amp;amp;nbsp;0.63.&amp;lt;ref&amp;gt;{{cite book | last=Falconer | first = Kenneth |title=Fractal Geometry: Mathematical Foundations and Applications | publisher=[[John Wiley and Sons]] | edition=2nd | year=2003}}&amp;lt;/ref&amp;gt; The [[Sierpinski triangle]] is a union of three copies of itself, each copy shrunk by a factor of&amp;amp;nbsp;1/2; this yields a Hausdorff dimension of ln(3)/ln(2)&amp;amp;nbsp;≈&amp;amp;nbsp;1.58.&amp;lt;ref name=CampbellAnnenberg15/&amp;gt; These Hausdorff dimensions are related to the &amp;quot;critical exponent&amp;quot; of the [[Master theorem (analysis of algorithms)|Master theorem]] for solving [[Recurrence relation|recurrence relations]] in the [[analysis of algorithms]].&lt;br /&gt;
*[[分形]]一般是那些豪斯多夫维数直接超过其拓扑维数的空间。例如[[康托尔集]]是一个o维拓扑空间，由两个自己复制而成，每一个复制品都是原来的三分之一，因此它的豪斯多夫维数是 ln(2)/ln(3)&amp;amp;nbsp;≈&amp;amp;nbsp;0.63。&amp;lt;ref&amp;gt;{{cite book | last=Falconer | first = Kenneth |title=Fractal Geometry: Mathematical Foundations and Applications | publisher=[[John Wiley and Sons]] | edition=2nd | year=2003}}&amp;lt;/ref&amp;gt;一个[[谢尔宾斯基三角]]是他自身三个复制的组合。每一个是原来的&amp;amp;nbsp;1/2，它的豪斯多夫维数ln(3)/ln(2)&amp;amp;nbsp;≈&amp;amp;nbsp;1.58。&amp;lt;ref name=CampbellAnnenberg15/&amp;gt;在递归算法中解决递归关系时，这些豪斯多夫维数与[[算法分析主定理]]的临界指标相联系。&lt;br /&gt;
* [[Space-filling curve]]s like the [[Peano curve]] have the same Hausdorff dimension as the space they fill.&lt;br /&gt;
*[[空间填充曲线]]拥有和他们填充空间同样的豪斯多夫维数，如[[皮亚诺曲线]]。&lt;br /&gt;
* The trajectory of [[Brownian motion]] in dimension 2 and above is conjectured to be Hausdorff dimension 2.&amp;lt;ref&amp;gt;{{cite book | last=Morters | first=Peres | title= Brownian Motion | publisher=[[Cambridge University Press]] | year=2010 }}&amp;lt;/ref&amp;gt;&lt;br /&gt;
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[[image:Great Britain Hausdorff.svg|thumb|250px|Estimating the Hausdorff dimension of the [[How Long Is the Coast of Britain? Statistical Self-Similarity and Fractional Dimension|coast of Great Britain]]]]&lt;br /&gt;
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coast of Great Britain]]&lt;br /&gt;
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[[大不列颠海岸&lt;br /&gt;
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* 刘易斯·弗赖伊·理查森[[Lewis Fry Richardson]] has performed detailed experiments to measure the approximate Hausdorff dimension for various coastlines. His results have varied from 1.02 for the coastline of [[South Africa]] to 1.25 for the west coast of [[Great Britain]].&amp;lt;ref name=&amp;quot;mandelbrot&amp;quot; /&amp;gt;&lt;br /&gt;
*刘易斯·弗赖伊·理查森（Lewis Fry Richardson）已经通过豪斯多夫维数去测量了很多海岸线。它的结果涵盖从1.02的南非海岸线到1.25的大英帝国西海岸模型。]]&lt;br /&gt;
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==Properties of Hausdorff dimension豪斯多夫维数特性==&lt;br /&gt;
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{{refimprove section|date=March 2015}}&lt;br /&gt;
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=== Hausdorff dimension and inductive dimension 豪斯多夫维数和归纳维数===&lt;br /&gt;
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Let ''X'' be an arbitrary [[Separable space|separable]] metric space. There is a [[topology|topological]] notion of [[inductive dimension]] for ''X'' which is defined recursively. It is always an integer (or +∞) and is denoted dim&amp;lt;sub&amp;gt;ind&amp;lt;/sub&amp;gt;(''X'').&lt;br /&gt;
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Let X be an arbitrary separable metric space. There is a topological notion of inductive dimension for X which is defined recursively. It is always an integer (or +∞) and is denoted dim&amp;lt;sub&amp;gt;ind&amp;lt;/sub&amp;gt;(X).&lt;br /&gt;
&lt;br /&gt;
设''X'' 是[[任意可分度量空间]]。对于''X'' 有一个递归定义的归纳维数拓扑概念。它总是一个整数(或 + ∞) ，并且表示dim&amp;lt;sub&amp;gt;ind&amp;lt;/sub&amp;gt;(''X'')。&lt;br /&gt;
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'''Theorem'''. Suppose ''X'' is non-empty. Then &lt;br /&gt;
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Theorem. Suppose X is non-empty. Then &lt;br /&gt;
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'''定理'''：假设''X'' 是非空的。那么&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt; \dim_{\mathrm{Haus}}(X) \geq \dim_{\operatorname{ind}}(X). &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \dim_{\mathrm{Haus}}(X) \geq \dim_{\operatorname{ind}}(X). &amp;lt;/math&amp;gt;&lt;br /&gt;
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&lt;br /&gt;
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Moreover,&lt;br /&gt;
&lt;br /&gt;
Moreover,&lt;br /&gt;
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此外,&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \inf_Y \dim_{\operatorname{Haus}}(Y) =\dim_{\operatorname{ind}}(X), &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \inf_Y \dim_{\operatorname{Haus}}(Y) =\dim_{\operatorname{ind}}(X), &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
where ''Y'' ranges over metric spaces [[homeomorphic]] to ''X''. In other words, ''X'' and ''Y'' have the same underlying set of points and the metric ''d''&amp;lt;sub&amp;gt;''Y''&amp;lt;/sub&amp;gt; of ''Y'' is topologically equivalent to ''d''&amp;lt;sub&amp;gt;''X''&amp;lt;/sub&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
where Y ranges over metric spaces homeomorphic to X. In other words, X and Y have the same underlying set of points and the metric d&amp;lt;sub&amp;gt;Y&amp;lt;/sub&amp;gt; of Y is topologically equivalent to d&amp;lt;sub&amp;gt;X&amp;lt;/sub&amp;gt;.&lt;br /&gt;
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其中''Y''是度量空间同胚到 ''X''的范围。换句话说， ''X''和 ''Y''具有相同的基本点集，''Y''的度规''d''&amp;lt;sub&amp;gt;''Y''&amp;lt;/sub&amp;gt; 的子拓扑等价于''d''&amp;lt;sub&amp;gt;''X''&amp;lt;/sub&amp;gt;。&lt;br /&gt;
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These results were originally established by [[Edward Szpilrajn]] (1907–1976), e.g., see Hurewicz and Wallman, Chapter VII.{{full citation needed|date=March 2015}}&lt;br /&gt;
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These results were originally established by Edward Szpilrajn (1907–1976), e.g., see Hurewicz and Wallman, Chapter VII.&lt;br /&gt;
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这些结果最初是由 [[Edward Szpilrajn]] (1907–1976)建立的,  参见 Hurewicz and Wallman, Chapter VII.{{full citation needed|date=March 2015}}第七章。&lt;br /&gt;
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=== Hausdorff dimension and Minkowski dimension 豪斯多夫维数和闵可夫斯基维度===&lt;br /&gt;
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The [[Minkowski dimension]] is similar to, and at least as large as, the Hausdorff dimension, and they are equal in many situations. However, the set of [[rational number|rational]] points in [0, 1] has Hausdorff dimension zero and Minkowski dimension one. There are also compact sets for which the Minkowski dimension is strictly larger than the Hausdorff dimension.&lt;br /&gt;
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The Minkowski dimension is similar to, and at least as large as, the Hausdorff dimension, and they are equal in many situations. However, the set of rational points in [0, 1] has Hausdorff dimension zero and Minkowski dimension one. There are also compact sets for which the Minkowski dimension is strictly larger than the Hausdorff dimension.&lt;br /&gt;
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[[闵可夫斯基维数]]与豪斯多夫维数相似，至少和它一样大，而且在许多情况下是相等的。然而，[0,1]中有理点集的豪斯多夫维数为0，闵可夫斯基维数为1。还有一些紧集的闵可夫斯基维数绝对大于豪斯多夫维数。&lt;br /&gt;
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=== Hausdorff dimensions and Frostman measures 豪斯多夫维度和弗洛斯曼测度===&lt;br /&gt;
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If there is a [[measure (mathematics)|measure]] μ defined on [[Borel measure|Borel]] subsets of a metric space ''X'' such that ''μ''(''X'') &amp;gt; 0 and ''μ''(''B''(''x'', ''r'')) ≤ ''r&amp;lt;sup&amp;gt;s&amp;lt;/sup&amp;gt;'' holds for some constant ''s'' &amp;gt; 0 and for every ball ''B''(''x'', ''r'') in ''X'', then dim&amp;lt;sub&amp;gt;Haus&amp;lt;/sub&amp;gt;(''X'') ≥ ''s''. A partial converse is provided by [[Frostman's lemma]].{{citation needed|date=March 2015}}&amp;lt;ref&amp;gt;This Wikipedia article also discusses further useful characterizations of the Hausdorff dimension.{{clarify|date=March 2015}}&amp;lt;/ref&amp;gt;&lt;br /&gt;
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If there is a measure μ defined on Borel subsets of a metric space X such that μ(X) &amp;gt; 0 and μ(B(x, r)) ≤ r&amp;lt;sup&amp;gt;s&amp;lt;/sup&amp;gt; holds for some constant s &amp;gt; 0 and for every ball B(x, r) in X, then dim&amp;lt;sub&amp;gt;Haus&amp;lt;/sub&amp;gt;(X) ≥ s. A partial converse is provided by Frostman's lemma.&lt;br /&gt;
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如果在度量空间 ''X'' 的 Borel 子集上定义一个测度 μ，使得''μ''(''X'') &amp;gt; 0 和''μ''(''B''(''x'', ''r'')) ≤ ''r&amp;lt;sup&amp;gt;s&amp;lt;/sup&amp;gt;''，对于某个常数 ''s'' &amp;gt; 0  和 ''X'' 中的每个球 ''B''(''x'', ''r'') 成立，则 dim&amp;lt;sub&amp;gt;Haus&amp;lt;/sub&amp;gt;(''X'') ≥ ''s'' 。 部分逆向转换由弗洛斯曼引理定义。&lt;br /&gt;
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=== Behaviour under unions and products ===&lt;br /&gt;
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If &amp;lt;math&amp;gt;X=\bigcup_{i\in I}X_i&amp;lt;/math&amp;gt; is a finite or countable union, then&lt;br /&gt;
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If &amp;lt;math&amp;gt;X=\bigcup_{i\in I}X_i&amp;lt;/math&amp;gt; is a finite or countable union, then&lt;br /&gt;
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如果 &amp;lt;math&amp;gt;X=\bigcup_{i\in I}X_i&amp;lt;/math&amp;gt; 是一个有限或可数的联合，则&lt;br /&gt;
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&amp;lt;math&amp;gt; \dim_{\operatorname{Haus}}(X) =\sup_{i\in I} \dim_{\operatorname{Haus}}(X_i).&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \dim_{\operatorname{Haus}}(X) =\sup_{i\in I} \dim_{\operatorname{Haus}}(X_i).&amp;lt;/math&amp;gt;&lt;br /&gt;
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This can be verified directly from the definition.&lt;br /&gt;
&lt;br /&gt;
This can be verified directly from the definition.&lt;br /&gt;
&lt;br /&gt;
这可以直接从定义得到验证。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
If ''X'' and ''Y'' are non-empty metric spaces, then the Hausdorff dimension of their product satisfies&amp;lt;ref&amp;gt;{{cite journal |author=Marstrand, J. M. |title=The dimension of Cartesian product sets |journal=Proc. Cambridge Philos. Soc. |volume=50 |issue=3 |pages=198–202 |year=1954 |doi=10.1017/S0305004100029236 |bibcode = 1954PCPS...50..198M }}&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
If X and Y are non-empty metric spaces, then the Hausdorff dimension of their product satisfies&lt;br /&gt;
&lt;br /&gt;
如果 ''X'' 和''Y''是非空度量空间，那么它们乘积的豪斯多夫维数满足&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt; \dim_{\operatorname{Haus}}(X\times Y)\ge \dim_{\operatorname{Haus}}(X)+ \dim_{\operatorname{Haus}}(Y).&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \dim_{\operatorname{Haus}}(X\times Y)\ge \dim_{\operatorname{Haus}}(X)+ \dim_{\operatorname{Haus}}(Y).&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
This inequality can be strict. It is possible to find two sets of dimension 0 whose product has dimension 1.&amp;lt;ref&amp;gt;{{cite book  | last = Falconer  | first = Kenneth J.  | title = Fractal geometry. Mathematical foundations and applications  | publisher = John Wiley &amp;amp; Sons, Inc., Hoboken, New Jersey  | year = 2003  | doi =   | isbn = }}&amp;lt;/ref&amp;gt; In the opposite direction, it is known that when ''X'' and ''Y'' are Borel subsets of '''R'''&amp;lt;sup&amp;gt;''n''&amp;lt;/sup&amp;gt;, the Hausdorff dimension of ''X'' × ''Y'' is bounded from above by the Hausdorff dimension of ''X'' plus the [[packing dimension|upper packing dimension]] of ''Y''. These facts are discussed in Mattila (1995).&lt;br /&gt;
&lt;br /&gt;
This inequality can be strict. It is possible to find two sets of dimension 0 whose product has dimension 1. In the opposite direction, it is known that when X and Y are Borel subsets of R&amp;lt;sup&amp;gt;n&amp;lt;/sup&amp;gt;, the Hausdorff dimension of X × Y is bounded from above by the Hausdorff dimension of X plus the upper packing dimension of Y. These facts are discussed in Mattila (1995).&lt;br /&gt;
&lt;br /&gt;
这种不平等可以是绝对的。有可能找到两个维数为0的集合，其乘积的维数为1。相反，我们知道当''X''和''Y''是 '''R'''&amp;lt;sup&amp;gt;''n''&amp;lt;/sup&amp;gt;的 Borel 子集时， ''X'' × ''Y''的豪斯多夫维数从上面以 ''X''的豪斯多夫维数加上 ''Y''的填充维数为界。Mattila (1995)曾就这些情况进行了讨论。&lt;br /&gt;
&lt;br /&gt;
==Self-similar sets自相似集合==&lt;br /&gt;
&lt;br /&gt;
{{refimprove section|date=March 2015}}&lt;br /&gt;
&lt;br /&gt;
Many sets defined by a self-similarity condition have dimensions which can be determined explicitly. Roughly, a set ''E'' is self-similar if it is the fixed point of a set-valued transformation ψ, that is ψ(''E'') = ''E'', although the exact definition is given below.&lt;br /&gt;
&lt;br /&gt;
Many sets defined by a self-similarity condition have dimensions which can be determined explicitly. Roughly, a set E is self-similar if it is the fixed point of a set-valued transformation ψ, that is ψ(E) = E, although the exact definition is given below.&lt;br /&gt;
&lt;br /&gt;
许多由自相似条件定义的集合具有可以显式确定的维数。粗略地说，集合''E'' 是自相似的，如果它是集值ψ变换的不动点，即ψ(''E'') = ''E''，尽管下面给出了确切的定义。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&amp;lt;blockquote&amp;gt;'''Theorem'''. Suppose&lt;br /&gt;
&lt;br /&gt;
&amp;lt;blockquote&amp;gt;Theorem. Suppose&lt;br /&gt;
&lt;br /&gt;
&amp;lt;blockquote&amp;gt;'''定理'''：假设&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt; \psi_i: \mathbf{R}^n \rightarrow \mathbf{R}^n, \quad i=1, \ldots , m &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \psi_i: \mathbf{R}^n \rightarrow \mathbf{R}^n, \quad i=1, \ldots , m &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
are [[Contraction mapping|contractive]] mappings on '''R'''&amp;lt;sup&amp;gt;''n''&amp;lt;/sup&amp;gt; with contraction constant ''r&amp;lt;sub&amp;gt;j&amp;lt;/sub&amp;gt;'' &amp;lt; 1. Then there is a unique ''non-empty'' compact set ''A'' such that&lt;br /&gt;
&lt;br /&gt;
are contractive mappings on R&amp;lt;sup&amp;gt;n&amp;lt;/sup&amp;gt; with contraction constant r&amp;lt;sub&amp;gt;j&amp;lt;/sub&amp;gt; &amp;lt; 1. Then there is a unique non-empty compact set A such that&lt;br /&gt;
&lt;br /&gt;
是'''R'''&amp;lt;sup&amp;gt;''n''&amp;lt;/sup&amp;gt;上的压缩常数''r&amp;lt;sub&amp;gt;j&amp;lt;/sub&amp;gt;'&amp;lt; 1的压缩映射。然后有一个唯一的非空紧集A &lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt; A = \bigcup_{i=1}^m \psi_i (A). &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; A = \bigcup_{i=1}^m \psi_i (A). &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&amp;lt;/blockquote&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;/blockquote&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The theorem follows from [[Stefan Banach]]'s [[Contractive mapping theorem|contractive mapping fixed point theorem]] applied to the complete metric space of non-empty compact subsets of '''R'''&amp;lt;sup&amp;gt;''n''&amp;lt;/sup&amp;gt; with the [[Hausdorff distance]].&amp;lt;ref&amp;gt;{{cite book |author=Falconer, K. J. |title=The Geometry of Fractal Sets |publisher=Cambridge University Press |location=Cambridge, UK |year=1985 |isbn=0-521-25694-1 |chapter=Theorem 8.3}}&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
The theorem follows from Stefan Banach's contractive mapping fixed point theorem applied to the complete metric space of non-empty compact subsets of R&amp;lt;sup&amp;gt;n&amp;lt;/sup&amp;gt; with the Hausdorff distance.&lt;br /&gt;
&lt;br /&gt;
这个定理来源于 Stefan Banach 的压缩映射不动点定理，该定理应用于 '''R'''&amp;lt;sup&amp;gt;''n''&amp;lt;/sup&amp;gt; 的非空紧子集的完备空间豪斯多夫距离。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
===The open set condition开集条件===&lt;br /&gt;
&lt;br /&gt;
To determine the dimension of the self-similar set ''A'' (in certain cases), we need a technical condition called the ''open set condition'' (OSC) on the sequence of contractions ψ&amp;lt;sub&amp;gt;''i''&amp;lt;/sub&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
To determine the dimension of the self-similar set A (in certain cases), we need a technical condition called the open set condition (OSC) on the sequence of contractions ψ&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
为了确定自相似集''A'' 的维数(在某些情况下) ，我们需要一个称为''开集条件''(OSC)的技术条件ψ&amp;lt;sub&amp;gt;''i''&amp;lt;/sub&amp;gt;。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
There is a relatively compact open set ''V'' such that&lt;br /&gt;
&lt;br /&gt;
There is a relatively compact open set V such that&lt;br /&gt;
&lt;br /&gt;
有一个相对紧的开集''V''&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt; \bigcup_{i=1}^m\psi_i (V) \subseteq V, &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \bigcup_{i=1}^m\psi_i (V) \subseteq V, &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
where the sets in union on the left are pairwise [[disjoint sets|disjoint]].&lt;br /&gt;
&lt;br /&gt;
where the sets in union on the left are pairwise disjoint.&lt;br /&gt;
&lt;br /&gt;
左边的集合是成对不相交的。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The open set condition is a separation condition that ensures the images ψ&amp;lt;sub&amp;gt;''i''&amp;lt;/sub&amp;gt;(''V'') do not overlap &amp;quot;too much&amp;quot;.&lt;br /&gt;
&lt;br /&gt;
The open set condition is a separation condition that ensures the images ψ&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;(V) do not overlap &amp;quot;too much&amp;quot;.&lt;br /&gt;
&lt;br /&gt;
开集条件是保证图像子ψ&amp;lt;sub&amp;gt;''i''&amp;lt;/sub&amp;gt;(''V'') 不重叠“太多”的分离条件。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
'''Theorem'''. Suppose the open set condition holds and each ψ&amp;lt;sub&amp;gt;''i''&amp;lt;/sub&amp;gt; is a similitude, that is a composition of an [[isometry]] and a [[dilation (metric space)|dilation]] around some point. Then the unique fixed point of ψ is a set whose Hausdorff dimension is ''s'' where ''s'' is the unique solution of&amp;lt;ref&amp;gt;{{cite journal | last=Hutchinson | first=John E. | title=Fractals and self similarity | journal=Indiana Univ. Math. J. | volume=30 | year=1981 | pages=713–747 | doi=10.1512/iumj.1981.30.30055 | issue=5 | doi-access=free }}&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
Theorem. Suppose the open set condition holds and each ψ&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt; is a similitude, that is a composition of an isometry and a dilation around some point. Then the unique fixed point of ψ is a set whose Hausdorff dimension is s where s is the unique solution of&lt;br /&gt;
&lt;br /&gt;
'''定理'''假设开集条件成立，并且每个ψ&amp;lt;sub&amp;gt;''i''&amp;lt;/sub&amp;gt; 是一个相似量，这是一个等距和围绕某一点的膨胀的合成。那么唯一的不动点是一个集合，它的豪斯多夫维数是 ''s'' ，其中  ''s'' 是 ''s'' &amp;lt;ref&amp;gt;{{cite journal | last=Hutchinson | first=John E. | title=Fractals and self similarity | journal=Indiana Univ. Math. J. | volume=30 | year=1981 | pages=713–747 | doi=10.1512/iumj.1981.30.30055 | issue=5 | doi-access=free }}&amp;lt;/ref&amp;gt;的唯一解&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt; \sum_{i=1}^m r_i^s = 1. &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \sum_{i=1}^m r_i^s = 1. &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The contraction coefficient of a similitude is the magnitude of the dilation.&lt;br /&gt;
&lt;br /&gt;
The contraction coefficient of a similitude is the magnitude of the dilation.&lt;br /&gt;
&lt;br /&gt;
相似物的收缩系数就是膨胀的大小。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
We can use this theorem to compute the Hausdorff dimension of the Sierpinski triangle (or sometimes called Sierpinski gasket). Consider three [[non-collinear points]] ''a''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;, ''a''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;, ''a''&amp;lt;sub&amp;gt;3&amp;lt;/sub&amp;gt; in the plane '''R'''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; and let ψ&amp;lt;sub&amp;gt;''i''&amp;lt;/sub&amp;gt; be the dilation of ratio 1/2 around ''a&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;''. The unique non-empty fixed point of the corresponding mapping ψ is a Sierpinski gasket and the dimension ''s'' is the unique solution of&lt;br /&gt;
&lt;br /&gt;
We can use this theorem to compute the Hausdorff dimension of the Sierpinski triangle (or sometimes called Sierpinski gasket). Consider three non-collinear points a&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;, a&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;, a&amp;lt;sub&amp;gt;3&amp;lt;/sub&amp;gt; in the plane R&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; and let ψ&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt; be the dilation of ratio 1/2 around a&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;. The unique non-empty fixed point of the corresponding mapping ψ is a Sierpinski gasket and the dimension s is the unique solution of&lt;br /&gt;
&lt;br /&gt;
我们可以使用这个定理来计算谢尔宾斯基三角形的豪斯多夫维数(或者有时候叫做谢尔宾斯基垫圈)。考虑R&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; 平面上的三个非共线点，''a''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;，''a''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;，''a''&amp;lt;sub&amp;gt;3&amp;lt;/sub&amp;gt;，让ψ&amp;lt;sub&amp;gt;''i''&amp;lt;/sub&amp;gt;是围绕着''a&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;''膨胀比率的1/2。对应映射的唯一非空不动点是一个谢尔宾斯基垫圈，其维数''s''是对应映射的唯一解&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt; \left(\frac{1}{2}\right)^s+\left(\frac{1}{2}\right)^s+\left(\frac{1}{2}\right)^s = 3 \left(\frac{1}{2}\right)^s =1. &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \left(\frac{1}{2}\right)^s+\left(\frac{1}{2}\right)^s+\left(\frac{1}{2}\right)^s = 3 \left(\frac{1}{2}\right)^s =1. &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Taking [[natural logarithm]]s of both sides of the above equation, we can solve for ''s'', that is: ''s'' = ln(3)/ln(2).  The Sierpinski gasket is self-similar and satisfies the OSC. In general a set ''E'' which is a fixed point of a mapping&lt;br /&gt;
&lt;br /&gt;
Taking natural logarithms of both sides of the above equation, we can solve for s, that is: s = ln(3)/ln(2).  The Sierpinski gasket is self-similar and satisfies the OSC. In general a set E which is a fixed point of a mapping&lt;br /&gt;
&lt;br /&gt;
取上述方程两边的自然对数，我们可以求出 ''s''，即: ''s'' = ln(3)/ln(2)。该密封垫具有自相似性，满足 OSC 要求。一般来说，集合 ''E''是一个映射的不动点&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt; A \mapsto \psi(A) = \bigcup_{i=1}^m \psi_i(A) &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt; A \mapsto \psi(A) = \bigcup_{i=1}^m \psi_i(A) &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
is self-similar if and only if the intersections&lt;br /&gt;
&lt;br /&gt;
is self-similar if and only if the intersections&lt;br /&gt;
&lt;br /&gt;
是自相似的，当且仅当&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt; H^s\left(\psi_i(E) \cap \psi_j(E)\right) =0, &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; H^s\left(\psi_i(E) \cap \psi_j(E)\right) =0, &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
where ''s'' is the Hausdorff dimension of ''E'' and ''H&amp;lt;sup&amp;gt;s&amp;lt;/sup&amp;gt;'' denotes [[Hausdorff measure]]. This is clear in the case of the Sierpinski gasket (the intersections are just points), but is also true more generally:&lt;br /&gt;
&lt;br /&gt;
where s is the Hausdorff dimension of E and H&amp;lt;sup&amp;gt;s&amp;lt;/sup&amp;gt; denotes Hausdorff measure. This is clear in the case of the Sierpinski gasket (the intersections are just points), but is also true more generally:&lt;br /&gt;
&lt;br /&gt;
其中 ''s''是''E''的豪斯多夫维数， ''E'' and ''H&amp;lt;sup&amp;gt;s&amp;lt;/sup&amp;gt;'' 表示 豪斯多夫测度。对于谢尔宾斯基垫圈(交叉点就是点)来说，这一点很明显，但更普遍的情况是:&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
'''Theorem'''. Under the same conditions as the previous theorem, the unique fixed point of ψ is self-similar.&lt;br /&gt;
&lt;br /&gt;
Theorem. Under the same conditions as the previous theorem, the unique fixed point of ψ is self-similar.&lt;br /&gt;
&lt;br /&gt;
'''定理'''：在与前一定理相同的条件下，其唯一不动点是自相似的。&lt;br /&gt;
&lt;br /&gt;
==See also参阅==&lt;br /&gt;
&lt;br /&gt;
* [[List of fractals by Hausdorff dimension豪斯多夫分形维数列表]] Examples of deterministic fractals, random and natural fractals.确定性分形与随机和自然分形的示例。&lt;br /&gt;
&lt;br /&gt;
* [[Assouad dimension  Assouad维数]], another variation of fractal dimension that, like Hausdorff dimension, is defined using coverings by balls其他被球覆盖方式定义的分形维数，例如豪斯多夫维数。&lt;br /&gt;
&lt;br /&gt;
* [[Intrinsic dimension固有维数]]&lt;br /&gt;
&lt;br /&gt;
* [[Packing dimension填充维数]]&lt;br /&gt;
&lt;br /&gt;
* [[Fractal dimension分形维数]]&lt;br /&gt;
&lt;br /&gt;
==References参考文献==&lt;br /&gt;
&lt;br /&gt;
{{reflist}}&lt;br /&gt;
&lt;br /&gt;
==Further reading拓展阅读==&lt;br /&gt;
&lt;br /&gt;
* {{cite book |last1=Dodson |first1=M. Maurice |title=Fractal Geometry and Applications: A Jubilee of Benoît Mandelbrot |volume=72 |issue=1 |pages=305–347 |last2=Kristensen |first2=Simon |chapter=Hausdorff Dimension and Diophantine Approximation |date=June 12, 2003 |arxiv=math/0305399 |bibcode = 2003math......5399D |doi=10.1090/pspum/072.1/2112110|series=Proceedings of Symposia in Pure Mathematics |isbn=9780821836378 }}&lt;br /&gt;
&lt;br /&gt;
* {{cite book |last1=Hurewicz |first1=Witold |authorlink1=Witold Hurewicz |last2=Wallman |first2=Henry |authorlink2=Henry Wallman |title=Dimension Theory |url=https://archive.org/details/in.ernet.dli.2015.84609 |publisher=Princeton University Press |year=1948 }}&lt;br /&gt;
&lt;br /&gt;
* {{cite journal |author作者=E. Szpilrajn |authorlink=Edward Marczewski |title=La dimension et la mesure |journal=Fundamenta Mathematicae |volume=28 |pages=81–9 |year=1937 }}&lt;br /&gt;
&lt;br /&gt;
* {{cite journal&lt;br /&gt;
&lt;br /&gt;
 | last1=Marstrand&lt;br /&gt;
&lt;br /&gt;
 | last1=Marstrand&lt;br /&gt;
&lt;br /&gt;
 | last1=马斯特兰德&lt;br /&gt;
&lt;br /&gt;
 | first1=J. M. | title=The dimension of cartesian product sets | year=1954 | journal=Proc. Cambridge Philos. Soc.&lt;br /&gt;
&lt;br /&gt;
 | first1=J. M. | title=The dimension of cartesian product sets | year=1954 | journal=Proc. Cambridge Philos. Soc.&lt;br /&gt;
&lt;br /&gt;
 | first1= J. M. | title=笛卡儿积集的维数 | 1954年 |  journal=Proc. Cambridge Philos. Soc.&lt;br /&gt;
&lt;br /&gt;
 | volume=50&lt;br /&gt;
&lt;br /&gt;
 | volume=50&lt;br /&gt;
&lt;br /&gt;
 | 第50卷&lt;br /&gt;
&lt;br /&gt;
 | issue=3&lt;br /&gt;
&lt;br /&gt;
 | issue=3&lt;br /&gt;
&lt;br /&gt;
 | 第三期&lt;br /&gt;
&lt;br /&gt;
 | pages=198–202&lt;br /&gt;
&lt;br /&gt;
 | pages=198–202&lt;br /&gt;
&lt;br /&gt;
 | 第198-202页&lt;br /&gt;
&lt;br /&gt;
 | doi=10.1017/S0305004100029236|bibcode = 1954PCPS...50..198M }}&lt;br /&gt;
&lt;br /&gt;
 | doi=10.1017/S0305004100029236|bibcode = 1954PCPS...50..198M }}&lt;br /&gt;
&lt;br /&gt;
10.1017 / S0305004100029236 | bibcode 1954PCPS... 50. . 198 m }&lt;br /&gt;
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* {{Cite book&lt;br /&gt;
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 | last1=Mattila&lt;br /&gt;
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 | last1=Mattila&lt;br /&gt;
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 | first1=Pertti | author1-link=Pertti Mattila| title=Geometry of sets and measures in Euclidean spaces | publisher=[[Cambridge University Press]]&lt;br /&gt;
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 | first1=Pertti | author1-link=Pertti Mattila| title=Geometry of sets and measures in Euclidean spaces | publisher=Cambridge University Press&lt;br /&gt;
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| first1 Pertti | author1-link Pertti Mattila | title 欧几里德空间中集合和度量的几何 | 出版商剑桥大学出版社&lt;br /&gt;
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 | isbn=978-0-521-65595-8 | year=1995}}&lt;br /&gt;
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 | isbn=978-0-521-65595-8 | year=1995}}&lt;br /&gt;
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| isbn 978-0-521-65595-8 | year 1995}&lt;br /&gt;
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* {{cite journal |author=A. S. Besicovitch |authorlink=A. S. Besicovitch |title=On Linear Sets of Points of Fractional Dimensions |journal=[[Mathematische Annalen]] |volume=101 |year=1929 | doi=10.1007/BF01454831| issue=1 |pages= 161–193}}&lt;br /&gt;
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* {{cite journal |author1=A. S. Besicovitch |authorlink1=A. S. Besicovitch |author2=H. D. Ursell |authorlink2=H. D. Ursell |title=Sets of Fractional Dimensions |journal=Journal of the London Mathematical Society |volume=12 |year=1937 | issue=1 | doi=10.1112/jlms/s1-12.45.18  | pages=18–25 }}&amp;lt;br/&amp;gt;Several selections from this volume are reprinted in {{cite book |author=Edgar, Gerald A. |title=Classics on fractals |publisher=Addison-Wesley |location=Boston |year=1993 |isbn=0-201-58701-7}} See chapters 9,10,11&lt;br /&gt;
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* {{cite journal |author=F. Hausdorff |authorlink=F. Hausdorff |title=Dimension und äußeres Maß |journal=Mathematische Annalen |volume=79 |issue=1–2 |pages=157–179 |date=March 1919 |doi=10.1007/BF01457179|hdl=10338.dmlcz/100363 |url=http://dml.cz/bitstream/handle/10338.dmlcz/100363/CzechMathJ_09-1959-3_5.pdf }}&lt;br /&gt;
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* {{cite journal | last=Hutchinson | first=John E. | title=Fractals and self similarity | journal=Indiana Univ. Math. J. | volume=30 | year=1981 | pages=713–747 | doi=10.1512/iumj.1981.30.30055 | issue=5 | doi-access=free }}&lt;br /&gt;
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*{{cite book | last=Falconer | first = Kenneth |title=Fractal Geometry: Mathematical Foundations and Applications | publisher=[[John Wiley and Sons]] | edition=2nd | year=2003}}&lt;br /&gt;
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==External links外部链接==&lt;br /&gt;
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* [https://www.encyclopediaofmath.org/index.php/Hausdorff_dimension Hausdorff dimension] 在 [https://www.encyclopediaofmath.org/ Encyclopedia of Mathematics]&lt;br /&gt;
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* [https://www.encyclopediaofmath.org/index.php/Hausdorff_measure Hausdorff measure] 在 [https://www.encyclopediaofmath.org/ Encyclopedia of Mathematics]&lt;br /&gt;
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{{DEFAULTSORT:Hausdorff Dimension豪斯多夫维数}}&lt;br /&gt;
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[[Category分类:Metric geometry度量几何]]&lt;br /&gt;
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[[Category分类:Dimension theory维度理论]]&lt;br /&gt;
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&amp;lt;small&amp;gt;This page was moved from [[wikipedia:en:Hausdorff dimension]]. Its edit history can be viewed at [[分形维数/edithistory]]&amp;lt;/small&amp;gt;&amp;lt;/noinclude&amp;gt;&lt;br /&gt;
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[[Category:待整理页面]]&lt;/div&gt;</summary>
		<author><name>Ruili</name></author>
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		<title>分形维数</title>
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		<updated>2020-11-01T09:14:07Z</updated>

		<summary type="html">&lt;p&gt;Ruili：&lt;/p&gt;
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&lt;div&gt;此词条暂由彩云小译翻译，未经人工整理和审校，带来阅读不便，请见谅。&lt;br /&gt;
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Example of non-integer dimensions. The first four [[iteration]]s of the [[Koch snowflake|Koch curve]], where after each iteration, all original line segments are replaced with four, each a self-similar copy that is 1/3 the length of the original. One formalism of the Hausdorff dimension uses this scale factor (3) and the number of self-similar objects (4) to calculate the dimension, D, after the first iteration to be D = (log N)/(log S) = (log 4)/(log 3) ≈ 1.26.&amp;lt;ref name=CampbellAnnenberg15&amp;gt;MacGregor Campbell, 2013, &amp;quot;5.6 Scaling and the Hausdorff Dimension,&amp;quot; at ''Annenberg Learner:MATHematics illuminated'', see [http://www.learner.org/courses/mathilluminated/units/5/textbook/06.php], accessed 5 March 2015.&amp;lt;/ref&amp;gt; That is, while the Hausdorff dimension of a single [[point (geometry)|point]] is zero, of a [[line segment]] is 1, of a [[square]] is 2, and of a [[cube]] is 3, for [[fractal]]s such as this, the object can have a non-integer dimension.&lt;br /&gt;
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Example of non-integer dimensions. The first four iterations of the Koch curve, where after each iteration, all original line segments are replaced with four, each a self-similar copy that is 1/3 the length of the original. One formalism of the Hausdorff dimension uses this scale factor (3) and the number of self-similar objects (4) to calculate the dimension, D, after the first iteration to be D = (log N)/(log S) = (log 4)/(log 3) ≈ 1.26. That is, while the Hausdorff dimension of a single point is zero, of a line segment is 1, of a square is 2, and of a cube is 3, for fractals such as this, the object can have a non-integer dimension.&lt;br /&gt;
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非整数维度示例：前四个[[Koch 曲线]]的迭代，在每次迭代后，所有原始线段都被替换为四个，每个自相似的复制是原始线段长度的1 / 3。豪斯多夫维数的一个建模是使用比例因子(3)和自相似对象的数量(4)来计算维度 D，在第一次迭代后为 D = (log N)/(log S) = (log 4)/(log 3) ≈ 1.26.&amp;lt;ref name=CampbellAnnenberg15&amp;gt;。MacGregor Campbell, 2013, &amp;quot;5.6 Scaling and the Hausdorff Dimension,&amp;quot; 在 ''Annenberg Learner:MATHematics illuminated'', 参见 [http://www.learner.org/courses/mathilluminated/units/5/textbook/06.php], accessed 5 March 2015.&amp;lt;/ref&amp;gt; 也就是说，单点的豪斯多夫维数为零，线段为1，正方形为2，立方体为3时，但对于分形，对象可以有一个非整数维度。&lt;br /&gt;
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In [[mathematics]], '''Hausdorff dimension''' is a measure of ''roughness'', or more specifically, [[fractal dimension]], that was first introduced in 1918 by [[mathematician]] [[Felix Hausdorff]].&amp;lt;ref&amp;gt;{{Cite journal |arxiv = 1101.1444|doi = 10.1214/11-STS370|title = Estimators of Fractal Dimension: Assessing the Roughness of Time Series and Spatial Data|journal = Statistical Science|volume = 27|issue = 2|pages = 247–277|year = 2012|last1 = Gneiting|first1 = Tilmann|last2 = Ševčíková|first2 = Hana|last3 = Percival|first3 = Donald B.}}&amp;lt;/ref&amp;gt; For instance, the Hausdorff dimension of a single [[point (geometry)|point]] is zero, of a [[line segment]] is 1, of a [[square]] is 2, and of a [[cube]] is 3. That is, for sets of points that define a smooth shape or a shape that has a small number of corners—the shapes of traditional geometry and science—the Hausdorff dimension is an [[integer]] agreeing with the usual sense of dimension, also known as the [[Inductive dimension|topological dimension]]. However, formulas have also been developed that allow calculation of the dimension of other less simple objects, where, solely on the basis of their properties of [[scaling (geometry)|scaling]] and [[self-similarity]], one is led to the conclusion that particular objects—including [[fractal]]s—have non-integer Hausdorff dimensions. Because of the significant technical advances made by [[Abram Samoilovitch Besicovitch]] allowing computation of dimensions for highly irregular or &amp;quot;rough&amp;quot; sets, this dimension is also commonly referred to as the ''Hausdorff–Besicovitch dimension.''&lt;br /&gt;
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In mathematics, Hausdorff dimension is a measure of roughness, or more specifically, fractal dimension, that was first introduced in 1918 by mathematician Felix Hausdorff. For instance, the Hausdorff dimension of a single point is zero, of a line segment is 1, of a square is 2, and of a cube is 3. That is, for sets of points that define a smooth shape or a shape that has a small number of corners—the shapes of traditional geometry and science—the Hausdorff dimension is an integer agreeing with the usual sense of dimension, also known as the topological dimension. However, formulas have also been developed that allow calculation of the dimension of other less simple objects, where, solely on the basis of their properties of scaling and self-similarity, one is led to the conclusion that particular objects—including fractals—have non-integer Hausdorff dimensions. Because of the significant technical advances made by Abram Samoilovitch Besicovitch allowing computation of dimensions for highly irregular or &amp;quot;rough&amp;quot; sets, this dimension is also commonly referred to as the Hausdorff–Besicovitch dimension.&lt;br /&gt;
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在[[数学]]中，'''&amp;lt;font color = '#ff8000'&amp;gt;豪斯多夫维数Hausdorff dimension&amp;lt;/font&amp;gt;'''是一种粗糙度的度量单位，或者更确切地说，分形维数，是由数学家 Felix Hausdorff 在1918年首次提出的。例如，单点的豪斯多夫维数为零，线段为1，正方形为2，立方体为3。也就是说，对于定义了一个光滑形状或一个有少数几个角的形状---- 传统几何学和科学的形状---- 的点集来说，豪斯多夫维数是一个整数，符合通常的维度意义，也称为拓扑维度。然而，还有一些公式允许计算其他不太简单的对象的维数，其中仅仅根据它们的标度和自相似特性，就可以得出结论: 特定的对象ー包括分形ー具有非整数的 Hausdorff 维数。由于阿布拉姆·萨莫伊洛维奇·贝西科维奇的重大技术进步，允许计算高度不规则或“粗糙”集的维度，这个维度通常也被称为 Hausdorff-Besicovitch 维度。 &lt;br /&gt;
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The Hausdorff dimension, more specifically, is a further dimensional number associated with a given set, where the distances between all members of that set are defined. Such a set is termed a [[metric space]]. The dimension is drawn from the [[Extended real number line|extended real numbers]], &amp;lt;math&amp;gt;\overline{\mathbb{R}}&amp;lt;/math&amp;gt;, as opposed to the more intuitive notion of dimension, which is not associated to general metric spaces, and only takes values in the non-negative integers.&lt;br /&gt;
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The Hausdorff dimension, more specifically, is a further dimensional number associated with a given set, where the distances between all members of that set are defined. Such a set is termed a metric space. The dimension is drawn from the extended real numbers, &amp;lt;math&amp;gt;\overline{\mathbb{R}}&amp;lt;/math&amp;gt;, as opposed to the more intuitive notion of dimension, which is not associated to general metric spaces, and only takes values in the non-negative integers.&lt;br /&gt;
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更具体地说，豪斯多夫维数是一个与给定集合相关联的更进一步的维数，其中定义了该集合所有成员之间的距离。这样的集合称为度量空间。维数是从扩展的实数，&amp;lt;math&amp;gt;\overline{\mathbb{R}}&amp;lt;/math&amp;gt;，而不是更直观的维数概念(它不与一般的度量空间相关联，只取非负整数的值)。&lt;br /&gt;
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In mathematical terms, the Hausdorff dimension generalizes the notion of the dimension of a real [[vector space]]. That is, the Hausdorff dimension of an ''n''-dimensional [[inner product space]] equals ''n''. This underlies the earlier statement that the Hausdorff dimension of a point is zero, of a line is one, etc., and that [[fractal|irregular sets]] can have noninteger Hausdorff dimensions. For instance, the [[Koch snowflake]] shown at right is constructed from an equilateral triangle; in each iteration, its component line segments are divided into 3 segments of unit length, the newly created middle segment is used as the base of a new [[equilateral]] triangle that points outward, and this base segment is then deleted to leave a final object from the iteration of unit length of 4.&amp;lt;ref&amp;gt;Larry Riddle, 2014, &amp;quot;Classic Iterated Function Systems: Koch Snowflake&amp;quot;, Agnes Scott College e-Academy (online), see [http://ecademy.agnesscott.edu/~lriddle/ifs/ksnow/ksnow.htm], accessed 5 March 2015.&amp;lt;/ref&amp;gt; That is, after the first iteration, each original line segment has been replaced with N=4, where each self-similar copy is 1/S = 1/3 as long as the original.&amp;lt;ref name=CampbellAnnenberg15/&amp;gt; Stated another way, we have taken an object with Euclidean dimension, D, and reduced its linear scale by 1/3 in each direction, so that its length increases to N=S&amp;lt;sup&amp;gt;D&amp;lt;/sup&amp;gt;.&amp;lt;ref name=ClaytonSCTPLS96&amp;gt;Keith Clayton, 1996, &amp;quot;Fractals and the Fractal Dimension,&amp;quot; ''Basic Concepts in Nonlinear Dynamics and Chaos'' (workshop), Society for Chaos Theory in Psychology and the Life Sciences annual meeting, June 28, 1996, Berkeley, California, see [http://www.vanderbilt.edu/AnS/psychology/cogsci/chaos/workshop/Workshop.html], accessed 5 March 2015.&amp;lt;/ref&amp;gt; This equation is easily solved for D, yielding the ratio of logarithms (or [[natural logarithm]]s) appearing in the figures, and giving—in the Koch and other fractal cases—non-integer dimensions for these objects.&lt;br /&gt;
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In mathematical terms, the Hausdorff dimension generalizes the notion of the dimension of a real vector space. That is, the Hausdorff dimension of an n-dimensional inner product space equals n. This underlies the earlier statement that the Hausdorff dimension of a point is zero, of a line is one, etc., and that irregular sets can have noninteger Hausdorff dimensions. For instance, the Koch snowflake shown at right is constructed from an equilateral triangle; in each iteration, its component line segments are divided into 3 segments of unit length, the newly created middle segment is used as the base of a new equilateral triangle that points outward, and this base segment is then deleted to leave a final object from the iteration of unit length of 4. That is, after the first iteration, each original line segment has been replaced with N=4, where each self-similar copy is 1/S = 1/3 as long as the original. This equation is easily solved for D, yielding the ratio of logarithms (or natural logarithms) appearing in the figures, and giving—in the Koch and other fractal cases—non-integer dimensions for these objects.&lt;br /&gt;
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用数学术语来说，豪斯多夫维数概括了实向量空间维数的概念。也就是说，n 维内积空间的豪斯多夫维数等于 n。 这就是早期假设的基础，一个点的豪斯多夫维数是零，一条线是一等等，不规则集可以有非整数的豪斯多夫维数。例如，右边所示的 Koch 雪花是由一个正三角形构成的; 在每次迭代中，它的组成线段被分成单位长度的3段，新创建的中间线段被用作一个指向外部的新正三角形的基础，然后人们删除这个基础线段用来保留单位长度4的迭代中的最终对象。也就是说，在第一次迭代之后，每个原始线段都被替换为 N=4，其中每个自相似拷贝的长度是原始线段的1/S = 1/3 。这个方程很容易求解为 D，产生出现在图形中的对数(或自然对数)的比率，并给出——在 Koch 和其他分形情况下——这些对象的非整数维数。&lt;br /&gt;
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The Hausdorff dimension is a successor to the simpler, but usually equivalent, box-counting or [[Minkowski–Bouligand dimension]].&lt;br /&gt;
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The Hausdorff dimension is a successor to the simpler, but usually equivalent, box-counting or Minkowski–Bouligand dimension.&lt;br /&gt;
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豪斯多夫维数是更简单但通常等价的'''&amp;lt;font color = '#ff8000'&amp;gt;计盒维数box-counting&amp;lt;/font&amp;gt;'''或'''&amp;lt;font color = '#ff8000'&amp;gt;闵可夫斯基维数Minkowski-Bouligand&amp;lt;/font&amp;gt;'''的继承者。&lt;br /&gt;
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==Intuition概念==&lt;br /&gt;
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The intuitive concept of dimension of a geometric object ''X'' is the number of independent parameters one needs to pick out a unique point inside. However, any point specified by two parameters can be instead specified by one, because the [[cardinality]] of the [[real plane]] is equal to the cardinality of the [[real line]] (this can be seen by an [[Cantor's diagonal argument|argument]] involving interweaving the digits of two numbers to yield a single number encoding the same information). The example of a [[space-filling curve]] shows that one can even map the real line to the real plane [[Surjective function|surjectively]] (taking one real number into a pair of real numbers in a way so that all pairs of numbers are covered) and ''continuously'', so that a one-dimensional object completely fills up a higher-dimensional object.&lt;br /&gt;
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The intuitive concept of dimension of a geometric object X is the number of independent parameters one needs to pick out a unique point inside. However, any point specified by two parameters can be instead specified by one, because the cardinality of the real plane is equal to the cardinality of the real line (this can be seen by an argument involving interweaving the digits of two numbers to yield a single number encoding the same information). The example of a space-filling curve shows that one can even map the real line to the real plane surjectively (taking one real number into a pair of real numbers in a way so that all pairs of numbers are covered) and continuously, so that a one-dimensional object completely fills up a higher-dimensional object.&lt;br /&gt;
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几何对象X的尺寸的直观概念是指需要多少个独立参数才能找到一个独特的点。但是，任何由两个参数指定的点都可以由一个参数指定，因为为实平面的基数等于实线的基数(这可以通过交织两个数字以产生一个编码相同信息的单个数字看到)。'''&amp;lt;font color = '#ff8000'&amp;gt;皮亚诺曲线&amp;lt;/font&amp;gt;'''的例子表明，可以将实线完美和连续地映射到实平面(把一个实数转换成一对实数，从而覆盖所有实数对)，由此一维对象完全填充了一个高维对象。&lt;br /&gt;
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Every space filling curve hits some points multiple times, and does not have a continuous inverse. It is impossible to map two dimensions onto one in a way that is continuous and continuously invertible. The topological dimension, also called [[Lebesgue covering dimension]], explains why. This dimension is ''n'' if, in every covering of ''X'' by small open balls, there is at least one point where ''n''&amp;amp;nbsp;+&amp;amp;nbsp;1 balls overlap. For example, when one covers a line with short open intervals, some points must be covered twice, giving dimension&amp;amp;nbsp;''n''&amp;amp;nbsp;=&amp;amp;nbsp;1.&lt;br /&gt;
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Every space filling curve hits some points multiple times, and does not have a continuous inverse. It is impossible to map two dimensions onto one in a way that is continuous and continuously invertible. The topological dimension, also called Lebesgue covering dimension, explains why. This dimension is n if, in every covering of X by small open balls, there is at least one point where n&amp;amp;nbsp;+&amp;amp;nbsp;1 balls overlap. For example, when one covers a line with short open intervals, some points must be covered twice, giving dimension&amp;amp;nbsp;n&amp;amp;nbsp;=&amp;amp;nbsp;1.&lt;br /&gt;
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每条空间填充曲线都会多次撞击某些点，且不存在连续的倒数。将两个维度以连续和连续可逆的方式映射到一个维度是不可能的。'''&amp;lt;font color = '#ff8000'&amp;gt;拓扑维度 topological dimension&amp;lt;/font&amp;gt;'''，也被称为拓朴维数，解释了为什么。这个维度是 n，如果在 x 的每个小开球覆盖中，至少有一个点 n + 1个球重叠。例如，当一个点覆盖一条具有短开区间的直线时，某些点必须被覆盖两次，给出维数''n''&amp;amp;nbsp;=&amp;amp;nbsp;1。&lt;br /&gt;
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But topological dimension is a very crude measure of the local size of a space (size near a point). A curve that is almost space-filling can still have topological dimension one, even if it fills up most of the area of a region. A [[fractal]] has an integer topological dimension, but in terms of the amount of space it takes up, it behaves like a higher-dimensional space.&lt;br /&gt;
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But topological dimension is a very crude measure of the local size of a space (size near a point). A curve that is almost space-filling can still have topological dimension one, even if it fills up most of the area of a region. A fractal has an integer topological dimension, but in terms of the amount of space it takes up, it behaves like a higher-dimensional space.&lt;br /&gt;
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但是，拓扑维度是对空间局部尺寸(点附近的尺寸)的一个非常粗略的度量。一条几乎是空间填充的曲线仍然可以有一维拓扑，即使它填充了一个区域的大部分面积。分形具有整数的拓扑维数，但就其所占空间的数量而言，它看起来像一个更高维的空间。&lt;br /&gt;
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The Hausdorff dimension measures the local size of a space taking into account the distance between points, the [[metric space|metric]]. Consider the number ''N''(''r'') of [[ball (mathematics)|balls]] of radius at most ''r'' required to cover ''X'' completely. When ''r'' is very small, ''N''(''r'') grows polynomially with 1/''r''. For a sufficiently well-behaved  ''X'', the Hausdorff dimension is the unique number ''d'' such that N(''r'') grows as 1/''r&amp;lt;sup&amp;gt;d&amp;lt;/sup&amp;gt;'' as ''r'' approaches zero. More precisely, this defines the [[Minkowski–Bouligand dimension|box-counting dimension]], which equals the Hausdorff dimension when the value ''d'' is a critical boundary between growth rates that are insufficient to cover the space, and growth rates that are overabundant.&lt;br /&gt;
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The Hausdorff dimension measures the local size of a space taking into account the distance between points, the metric. Consider the number N(r) of balls of radius at most r required to cover X completely. When r is very small, N(r) grows polynomially with 1/r. For a sufficiently well-behaved  X, the Hausdorff dimension is the unique number d such that N(r) grows as 1/r&amp;lt;sup&amp;gt;d&amp;lt;/sup&amp;gt; as r approaches zero. More precisely, this defines the box-counting dimension, which equals the Hausdorff dimension when the value d is a critical boundary between growth rates that are insufficient to cover the space, and growth rates that are overabundant.&lt;br /&gt;
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豪斯多夫维数测量一个空间的局部大小时，会考虑到点之间距离的度量。考虑半径最大为 r 的球数 ''N'' (r) ，需要完全覆盖 ''X''。当 r 很小时，n (r)以1/''r'' 增长多项式。对于一个表现足够好的 ''X''，豪斯多夫维数是唯一的数 d，这样当 r 趋近于零时， N(r)增长为1/r&amp;lt;sup&amp;gt;d&amp;lt;/sup&amp;gt; 。更确切地说，这定义了盒子计数维度，当值 d 是不足以覆盖空间的增长率和过度充裕的增长率之间的关键边界时，它等于豪斯多夫维数。&lt;br /&gt;
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For shapes that are smooth, or shapes with a small number of corners, the shapes of traditional geometry and science, the Hausdorff dimension is an integer agreeing with the topological dimension. But [[Benoit Mandelbrot]] observed that [[fractal]]s, sets with noninteger Hausdorff dimensions, are found everywhere in nature. He observed that the proper idealization of most rough shapes you see around you is not in terms of smooth idealized shapes, but in terms of fractal idealized shapes:&lt;br /&gt;
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For shapes that are smooth, or shapes with a small number of corners, the shapes of traditional geometry and science, the Hausdorff dimension is an integer agreeing with the topological dimension. But Benoit Mandelbrot observed that fractals, sets with noninteger Hausdorff dimensions, are found everywhere in nature. He observed that the proper idealization of most rough shapes you see around you is not in terms of smooth idealized shapes, but in terms of fractal idealized shapes:&lt;br /&gt;
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对于光滑的形状，或者有少量棱角的形状，传统几何和科学的形状，豪斯多夫维数是一个整数，与拓扑维度一致。但是伯努·曼德布洛特观察到分形---- 具有非整数豪斯多夫维数的集合---- 在自然界中随处可见。他观察到，我们周围大多数粗糙形状的理想化不是光滑的理想化形状，而是分形理想化形状:&lt;br /&gt;
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&amp;lt;blockquote&amp;gt;Clouds are not spheres, mountains are not cones, coastlines are not circles, and bark is not smooth, nor does lightning travel in a straight line.&amp;lt;ref name=&amp;quot;mandelbrot&amp;quot;&amp;gt;{{cite book   | last = Mandelbrot   | first = Benoît   | authorlink = Benoit Mandelbrot   | title = The Fractal Geometry of Nature   | publisher = W. H. Freeman   | series = Lecture notes in mathematics 1358   | year = 1982   | doi =    | isbn = 0-7167-1186-9   | url-access = registration   | url = https://archive.org/details/fractalgeometryo00beno   }}&amp;lt;/ref&amp;gt;&amp;lt;/blockquote&amp;gt;&lt;br /&gt;
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&amp;lt;blockquote&amp;gt;Clouds are not spheres, mountains are not cones, coastlines are not circles, and bark is not smooth, nor does lightning travel in a straight line.&amp;lt;/blockquote&amp;gt;&lt;br /&gt;
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&amp;lt;blockquote&amp;gt;云不是球体，山不是锥体，海岸线不是圆圈，树皮不平滑，闪电也不是直线运动。 &amp;lt;/blockquote&amp;gt;&lt;br /&gt;
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For fractals that occur in nature, the Hausdorff and [[Minkowski–Bouligand dimension|box-counting dimension]] coincide. The [[packing dimension]] is yet another similar notion which gives the same value for many shapes, but there are well documented exceptions where all these dimensions differ.&lt;br /&gt;
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For fractals that occur in nature, the Hausdorff and box-counting dimension coincide. The packing dimension is yet another similar notion which gives the same value for many shapes, but there are well documented exceptions where all these dimensions differ.&lt;br /&gt;
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对于自然界中出现的分形，豪斯多夫维数和盒计数维数是一致的。封装尺寸是另一个类似的概念，它给出了许多形状相同的值，但是在所有这些尺寸不同的情况，都做了很好的说明。&lt;br /&gt;
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==Formal definitions形式化定义==&lt;br /&gt;
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{{unreferenced section|date=March 2015}}&lt;br /&gt;
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===Hausdorff content豪斯多夫集===&lt;br /&gt;
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Let ''X'' be a [[metric space]]. If ''S'' ⊂ ''X'' and ''d'' ∈ [0, ∞), the ''d''-dimensional '''unlimited Hausdorff content''' of ''S'' is defined by&lt;br /&gt;
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Let X be a metric space. If S ⊂ X and d ∈ [0, ∞), the d-dimensional unlimited Hausdorff content of S is defined by&lt;br /&gt;
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设 ''X''是度量空间。若''S'' ⊂ ''X'' 和 ''d'' ∈ [0, ∞) ，则 ''S'' 的''d''维无限 豪斯多夫集定义为&lt;br /&gt;
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:&amp;lt;math&amp;gt;C_H^d(S):=\inf\Bigl\{\sum_i r_i^d:\text{ there is a cover of } S\text{ by balls with radii }r_i&amp;gt;0\Bigr\}.&amp;lt;/math&amp;gt;&lt;br /&gt;
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&amp;lt;math&amp;gt;C_H^d(S):=\inf\Bigl\{\sum_i r_i^d:\text{ there is a cover of } S\text{ by balls with radii }r_i&amp;gt;0\Bigr\}.&amp;lt;/math&amp;gt;&lt;br /&gt;
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&amp;lt;math&amp;gt;C_H^d(S):=\inf\Bigl\{\sum_i r_i^d:\text{ there is a cover of } S\text{ by balls with radii }r_i&amp;gt;0\Bigr\}.&amp;lt;/math&amp;gt;&lt;br /&gt;
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In other words, &amp;lt;math&amp;gt;C_H^d(S)&amp;lt;/math&amp;gt; is the [[infimum]] of the set of numbers &amp;lt;math&amp;gt;\delta \geq 0&amp;lt;/math&amp;gt; such that there is some (indexed) collection of [[ball (mathematics)|ball]]s &amp;lt;math&amp;gt;\{B(x_i,r_i):i\in I\}&amp;lt;/math&amp;gt; covering ''S'' with ''r&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;''&amp;amp;nbsp;&amp;gt;&amp;amp;nbsp;0 for each ''i''&amp;amp;nbsp;∈&amp;amp;nbsp;''I'' that satisfies &amp;lt;math&amp;gt;\sum_{i\in I} r_i^d&amp;lt;\delta &amp;lt;/math&amp;gt;. (Here, we use the standard convention that [[infimum|inf&amp;amp;nbsp;Ø&amp;amp;nbsp;=&amp;amp;nbsp;∞]].)&lt;br /&gt;
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In other words, &amp;lt;math&amp;gt;C_H^d(S)&amp;lt;/math&amp;gt; is the infimum of the set of numbers &amp;lt;math&amp;gt;\delta \geq 0&amp;lt;/math&amp;gt; such that there is some (indexed) collection of balls &amp;lt;math&amp;gt;\{B(x_i,r_i):i\in I\}&amp;lt;/math&amp;gt; covering S with r&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;&amp;amp;nbsp;&amp;gt;&amp;amp;nbsp;0 for each i&amp;amp;nbsp;∈&amp;amp;nbsp;I that satisfies &amp;lt;math&amp;gt;\sum_{i\in I} r_i^d&amp;lt;\delta &amp;lt;/math&amp;gt;. (Here, we use the standard convention that inf&amp;amp;nbsp;Ø&amp;amp;nbsp;=&amp;amp;nbsp;∞.)&lt;br /&gt;
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换句话说，&amp;lt;math&amp;gt;C_H^d(S)&amp;lt;/math&amp;gt; 是数字集合&amp;lt;math&amp;gt;\delta \geq 0&amp;lt;/math&amp;gt;的下确界，使得在 ''i''&amp;amp;nbsp;∈&amp;amp;nbsp中存在一些球集合 &amp;lt;math&amp;gt;\{B(x_i,r_i):i\in I\}&amp;lt;/math&amp;gt;  i 包含 s，对于每个 ''r&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;''&amp;amp;nbsp;&amp;gt;&amp;amp;nbsp;0 满足 i 中的和&amp;lt;math&amp;gt;\sum_{i\in I} r_i^d&amp;lt;\delta &amp;lt;/math&amp;gt; (在这里，我们使用inf&amp;amp;nbsp;Ø&amp;amp;nbsp;=&amp;amp;nbsp;∞ )的标准约定。&lt;br /&gt;
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===Hausdorff measurement豪斯多夫分形测量===&lt;br /&gt;
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The Hausdorff outer measure is different from the unbounded Hausdorf content in that rather than considering all possible coverings of ''S'', we see what happens when the sizes of the balls go to zero. This is  for &amp;lt;math&amp;gt;d \geq 0 &amp;lt;/math&amp;gt;, we define the ''d''-dimensional Hausdorff outer measure of ''S'' as&lt;br /&gt;
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The Hausdorff outer measure is different from the unbounded Hausdorf content in that rather than considering all possible coverings of S, we see what happens when the sizes of the balls go to zero. This is  for &amp;lt;math&amp;gt;d \geq 0 &amp;lt;/math&amp;gt;, we define the d-dimensional Hausdorff outer measure of S as&lt;br /&gt;
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豪斯多夫外测度不同于无界的豪斯多夫，因为我们不考虑 s 的所有可能，我们看到当球的大小为零时会发生什么。这是为了数学  &amp;lt;math&amp;gt;d \geq 0 &amp;lt;/math&amp;gt;，我们定义了  ''S''的 ''d''维豪斯多夫Hausdorff 外测度为&lt;br /&gt;
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:&amp;lt;math&amp;gt; \mathcal{H}^d(S):=\lim_{r \to 0} \inf\Bigl\{\sum_i r_i^d:\text{ there is a cover of } S\text{ by balls with radii } 0 &amp;lt; r_i &amp;lt; r\Bigr\}.&amp;lt;/math&amp;gt;&lt;br /&gt;
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&amp;lt;math&amp;gt; \mathcal{H}^d(S):=\lim_{r \to 0} \inf\Bigl\{\sum_i r_i^d:\text{ there is a cover of } S\text{ by balls with radii } 0 &amp;lt; r_i &amp;lt; r\Bigr\}.&amp;lt;/math&amp;gt;&lt;br /&gt;
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&amp;lt;math&amp;gt; \mathcal{H}^d(S):=\lim_{r \to 0} \inf\Bigl\{\sum_i r_i^d:\text{有一个面} S\text{ 球 } 0 &amp;lt; r_i &amp;lt; r\Bigr\}.&amp;lt;/math&amp;gt;&lt;br /&gt;
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===Hausdorff dimension豪斯多夫维数===&lt;br /&gt;
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The '''Hausdorff dimension''' of ''X'' is defined by&lt;br /&gt;
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The Hausdorff dimension of X is defined by&lt;br /&gt;
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X 的豪斯多夫维数定义为&lt;br /&gt;
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:&amp;lt;math&amp;gt;\dim_{\operatorname{H}}(X):=\inf\{d\ge 0: \mathcal{H}^d(X)=0\}.&amp;lt;/math&amp;gt;&lt;br /&gt;
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&amp;lt;math&amp;gt;\dim_{\operatorname{H}}(X):=\inf\{d\ge 0: \mathcal{H}^d(X)=0\}.&amp;lt;/math&amp;gt;&lt;br /&gt;
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Equivalently, dim&amp;lt;sub&amp;gt;H&amp;lt;/sub&amp;gt;(''X'') may be defined as the [[infimum]] of the set of ''d'' ∈ [0, ∞) such that the ''d''-dimensional [[Hausdorff measure]] of ''X'' is zero. This is the same as the supremum of the set of ''d''&amp;amp;nbsp;∈&amp;amp;nbsp;[0,&amp;amp;nbsp;∞) such that the ''d''-dimensional Hausdorff measure of ''X'' is infinite (except that when this latter set of numbers ''d'' is empty the Hausdorff dimension is zero).&lt;br /&gt;
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Equivalently, dim&amp;lt;sub&amp;gt;H&amp;lt;/sub&amp;gt;(X) may be defined as the infimum of the set of d ∈ [0, ∞) such that the d-dimensional Hausdorff measure of X is zero. This is the same as the supremum of the set of d&amp;amp;nbsp;∈&amp;amp;nbsp;[0,&amp;amp;nbsp;∞) such that the d-dimensional Hausdorff measure of X is infinite (except that when this latter set of numbers d is empty the Hausdorff dimension is zero).&lt;br /&gt;
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等价地，dim &amp;lt;sub&amp;gt;H&amp;lt;/sub&amp;gt;(''X'')可定义为 ''d'' ∈ [0, ∞) 集的下确界，使得''X'' 的''d''-维 [[豪斯多夫测度]] 为零。这与 ''d''&amp;amp;nbsp;∈&amp;amp;nbsp;[0,&amp;amp;nbsp;∞)的集合的上确界相同，因此''X''的 d 维豪斯多夫测度是无限的(除非后一个集合 ''d'' 是空的，豪斯多夫维数为零)。&lt;br /&gt;
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==Examples实例==&lt;br /&gt;
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[[Image:Sierpinski deep.svg|thumb|250px|Dimension of a further [[fractal]] example. The [[Sierpinski triangle]], an object with Hausdorff dimension of log(3)/log(2)≈1.58.&amp;lt;ref name=ClaytonSCTPLS96/&amp;gt;]]&lt;br /&gt;
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Dimension of a further [[fractal example. The Sierpinski triangle, an object with Hausdorff dimension of log(3)/log(2)≈1.58.]]&lt;br /&gt;
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[[Image:谢尔宾斯基三角形 deep.svg|thumb|250px|进一步的[[分形维数]]的例子，进一步的分形维数的例子是谢尔宾斯基三角形，它是一个豪斯多夫维数为log(3)/log(2)≈1.58.&amp;lt;ref name=ClaytonSCTPLS96/&amp;gt;的物体]]&lt;br /&gt;
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* [[Countable set]]s have Hausdorff dimension 0.&amp;lt;ref name=&amp;quot;schleicher&amp;quot;&amp;gt;{{cite journal |last1=Schleicher |first1=Dierk |title=Hausdorff Dimension, Its Properties, and Its Surprises |journal=The American Mathematical Monthly |date=June 2007 |volume=114 |issue=6 |pages=509–528 |doi=10.1080/00029890.2007.11920440 |language=en |issn=0002-9890|arxiv=math/0505099 }}&amp;lt;/ref&amp;gt;&lt;br /&gt;
*[[可数集]]拥有豪斯多夫维数0.&amp;lt;ref name=&amp;quot;schleicher&amp;quot;&amp;gt;{{cite journal |last1=Schleicher |first1=Dierk |title=豪斯多夫维数, Its Properties, and Its Surprises |journal=The American Mathematical Monthly美国数学期刊 |date=June 2007 |volume=114 |issue=6 |pages=509–528 |doi=10.1080/00029890.2007.11920440 |language=en |issn=0002-9890|arxiv=math/0505099 }}&amp;lt;/ref&amp;gt;&lt;br /&gt;
* The [[Euclidean space]] ℝ&amp;lt;sup&amp;gt;''n''&amp;lt;/sup&amp;gt; has Hausdorff dimension ''n'', and the circle '''S'''&amp;lt;sup&amp;gt;1&amp;lt;/sup&amp;gt; has Hausdorff dimension 1.&amp;lt;ref name=&amp;quot;schleicher&amp;quot; /&amp;gt;&lt;br /&gt;
*[[教育空间]] ℝ&amp;lt;sup&amp;gt;''n''&amp;lt;/sup&amp;gt; 有豪斯多夫维数 ''n''，循环'''S'''&amp;lt;sup&amp;gt;1&amp;lt;/sup&amp;gt; 拥有豪斯多夫维数1.&amp;lt;ref name=&amp;quot;schleicher&amp;quot; /&amp;gt;&lt;br /&gt;
* [[Fractal]]s often are spaces whose Hausdorff dimension strictly exceeds the [[topological dimension]].&amp;lt;ref name=&amp;quot;mandelbrot&amp;quot; /&amp;gt; For example, the [[Cantor set]], a zero-dimensional topological space, is a union of two copies of itself, each copy shrunk by a factor 1/3; hence, it can be shown that its Hausdorff dimension is ln(2)/ln(3)&amp;amp;nbsp;≈&amp;amp;nbsp;0.63.&amp;lt;ref&amp;gt;{{cite book | last=Falconer | first = Kenneth |title=Fractal Geometry: Mathematical Foundations and Applications | publisher=[[John Wiley and Sons]] | edition=2nd | year=2003}}&amp;lt;/ref&amp;gt; The [[Sierpinski triangle]] is a union of three copies of itself, each copy shrunk by a factor of&amp;amp;nbsp;1/2; this yields a Hausdorff dimension of ln(3)/ln(2)&amp;amp;nbsp;≈&amp;amp;nbsp;1.58.&amp;lt;ref name=CampbellAnnenberg15/&amp;gt; These Hausdorff dimensions are related to the &amp;quot;critical exponent&amp;quot; of the [[Master theorem (analysis of algorithms)|Master theorem]] for solving [[Recurrence relation|recurrence relations]] in the [[analysis of algorithms]].&lt;br /&gt;
*[[分形]]一般是那些豪斯多夫维数直接超过其拓扑维数的空间。例如[[康托尔集]]是一个o维拓扑空间，由两个自己复制而成，每一个复制品都是原来的三分之一，因此它的豪斯多夫维数是 ln(2)/ln(3)&amp;amp;nbsp;≈&amp;amp;nbsp;0.63。&amp;lt;ref&amp;gt;{{cite book | last=Falconer | first = Kenneth |title=Fractal Geometry: Mathematical Foundations and Applications | publisher=[[John Wiley and Sons]] | edition=2nd | year=2003}}&amp;lt;/ref&amp;gt;一个[[谢尔宾斯基三角]]是他自身三个复制的组合。每一个是原来的&amp;amp;nbsp;1/2，它的豪斯多夫维数ln(3)/ln(2)&amp;amp;nbsp;≈&amp;amp;nbsp;1.58。&amp;lt;ref name=CampbellAnnenberg15/&amp;gt;在递归算法中解决递归关系时，这些豪斯多夫维数与[[算法分析主定理]]的临界指标相联系。&lt;br /&gt;
* [[Space-filling curve]]s like the [[Peano curve]] have the same Hausdorff dimension as the space they fill.&lt;br /&gt;
*[[空间填充曲线]]拥有和他们填充空间同样的豪斯多夫维数，如[[皮亚诺曲线]]。&lt;br /&gt;
* The trajectory of [[Brownian motion]] in dimension 2 and above is conjectured to be Hausdorff dimension 2.&amp;lt;ref&amp;gt;{{cite book | last=Morters | first=Peres | title= Brownian Motion | publisher=[[Cambridge University Press]] | year=2010 }}&amp;lt;/ref&amp;gt;&lt;br /&gt;
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[[image:Great Britain Hausdorff.svg|thumb|250px|Estimating the Hausdorff dimension of the [[How Long Is the Coast of Britain? Statistical Self-Similarity and Fractional Dimension|coast of Great Britain]]]]&lt;br /&gt;
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coast of Great Britain]]&lt;br /&gt;
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[[大不列颠海岸&lt;br /&gt;
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* 刘易斯·弗赖伊·理查森[[Lewis Fry Richardson]] has performed detailed experiments to measure the approximate Hausdorff dimension for various coastlines. His results have varied from 1.02 for the coastline of [[South Africa]] to 1.25 for the west coast of [[Great Britain]].&amp;lt;ref name=&amp;quot;mandelbrot&amp;quot; /&amp;gt;&lt;br /&gt;
*刘易斯·弗赖伊·理查森（Lewis Fry Richardson）已经通过豪斯多夫维数去测量了很多海岸线。它的结果涵盖从1.02的南非海岸线到1.25的大英帝国西海岸模型。]]&lt;br /&gt;
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==Properties of Hausdorff dimension豪斯多夫维数特性==&lt;br /&gt;
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{{refimprove section|date=March 2015}}&lt;br /&gt;
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=== Hausdorff dimension and inductive dimension 豪斯多夫维数和归纳维数===&lt;br /&gt;
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Let ''X'' be an arbitrary [[Separable space|separable]] metric space. There is a [[topology|topological]] notion of [[inductive dimension]] for ''X'' which is defined recursively. It is always an integer (or +∞) and is denoted dim&amp;lt;sub&amp;gt;ind&amp;lt;/sub&amp;gt;(''X'').&lt;br /&gt;
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Let X be an arbitrary separable metric space. There is a topological notion of inductive dimension for X which is defined recursively. It is always an integer (or +∞) and is denoted dim&amp;lt;sub&amp;gt;ind&amp;lt;/sub&amp;gt;(X).&lt;br /&gt;
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设''X'' 是[[任意可分度量空间]]。对于''X'' 有一个递归定义的归纳维数拓扑概念。它总是一个整数(或 + ∞) ，并且表示dim&amp;lt;sub&amp;gt;ind&amp;lt;/sub&amp;gt;(''X'')。&lt;br /&gt;
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'''Theorem'''. Suppose ''X'' is non-empty. Then &lt;br /&gt;
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Theorem. Suppose X is non-empty. Then &lt;br /&gt;
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'''定理'''：假设''X'' 是非空的。那么&lt;br /&gt;
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:&amp;lt;math&amp;gt; \dim_{\mathrm{Haus}}(X) \geq \dim_{\operatorname{ind}}(X). &amp;lt;/math&amp;gt;&lt;br /&gt;
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&amp;lt;math&amp;gt; \dim_{\mathrm{Haus}}(X) \geq \dim_{\operatorname{ind}}(X). &amp;lt;/math&amp;gt;&lt;br /&gt;
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Moreover,&lt;br /&gt;
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Moreover,&lt;br /&gt;
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此外,&lt;br /&gt;
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&amp;lt;math&amp;gt; \inf_Y \dim_{\operatorname{Haus}}(Y) =\dim_{\operatorname{ind}}(X), &amp;lt;/math&amp;gt;&lt;br /&gt;
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&amp;lt;math&amp;gt; \inf_Y \dim_{\operatorname{Haus}}(Y) =\dim_{\operatorname{ind}}(X), &amp;lt;/math&amp;gt;&lt;br /&gt;
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where ''Y'' ranges over metric spaces [[homeomorphic]] to ''X''. In other words, ''X'' and ''Y'' have the same underlying set of points and the metric ''d''&amp;lt;sub&amp;gt;''Y''&amp;lt;/sub&amp;gt; of ''Y'' is topologically equivalent to ''d''&amp;lt;sub&amp;gt;''X''&amp;lt;/sub&amp;gt;.&lt;br /&gt;
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where Y ranges over metric spaces homeomorphic to X. In other words, X and Y have the same underlying set of points and the metric d&amp;lt;sub&amp;gt;Y&amp;lt;/sub&amp;gt; of Y is topologically equivalent to d&amp;lt;sub&amp;gt;X&amp;lt;/sub&amp;gt;.&lt;br /&gt;
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其中''Y''是度量空间同胚到 ''X''的范围。换句话说， ''X''和 ''Y''具有相同的基本点集，''Y''的度规''d''&amp;lt;sub&amp;gt;''Y''&amp;lt;/sub&amp;gt; 的子拓扑等价于''d''&amp;lt;sub&amp;gt;''X''&amp;lt;/sub&amp;gt;。&lt;br /&gt;
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&lt;br /&gt;
&lt;br /&gt;
These results were originally established by [[Edward Szpilrajn]] (1907–1976), e.g., see Hurewicz and Wallman, Chapter VII.{{full citation needed|date=March 2015}}&lt;br /&gt;
&lt;br /&gt;
These results were originally established by Edward Szpilrajn (1907–1976), e.g., see Hurewicz and Wallman, Chapter VII.&lt;br /&gt;
&lt;br /&gt;
这些结果最初是由 [[Edward Szpilrajn]] (1907–1976)建立的,  参见 Hurewicz and Wallman, Chapter VII.{{full citation needed|date=March 2015}}第七章。&lt;br /&gt;
&lt;br /&gt;
=== Hausdorff dimension and Minkowski dimension 豪斯多夫维数和闵可夫斯基维度===&lt;br /&gt;
&lt;br /&gt;
The [[Minkowski dimension]] is similar to, and at least as large as, the Hausdorff dimension, and they are equal in many situations. However, the set of [[rational number|rational]] points in [0, 1] has Hausdorff dimension zero and Minkowski dimension one. There are also compact sets for which the Minkowski dimension is strictly larger than the Hausdorff dimension.&lt;br /&gt;
&lt;br /&gt;
The Minkowski dimension is similar to, and at least as large as, the Hausdorff dimension, and they are equal in many situations. However, the set of rational points in [0, 1] has Hausdorff dimension zero and Minkowski dimension one. There are also compact sets for which the Minkowski dimension is strictly larger than the Hausdorff dimension.&lt;br /&gt;
&lt;br /&gt;
[[闵可夫斯基维数]]与豪斯多夫维数相似，至少和它一样大，而且在许多情况下是相等的。然而，[0,1]中有理点集的豪斯多夫维数为0，闵可夫斯基维数为1。还有一些紧集的闵可夫斯基维数绝对大于豪斯多夫维数。&lt;br /&gt;
&lt;br /&gt;
=== Hausdorff dimensions and Frostman measures 豪斯多夫维度和弗洛斯曼测度===&lt;br /&gt;
&lt;br /&gt;
If there is a [[measure (mathematics)|measure]] μ defined on [[Borel measure|Borel]] subsets of a metric space ''X'' such that ''μ''(''X'') &amp;gt; 0 and ''μ''(''B''(''x'', ''r'')) ≤ ''r&amp;lt;sup&amp;gt;s&amp;lt;/sup&amp;gt;'' holds for some constant ''s'' &amp;gt; 0 and for every ball ''B''(''x'', ''r'') in ''X'', then dim&amp;lt;sub&amp;gt;Haus&amp;lt;/sub&amp;gt;(''X'') ≥ ''s''. A partial converse is provided by [[Frostman's lemma]].{{citation needed|date=March 2015}}&amp;lt;ref&amp;gt;This Wikipedia article also discusses further useful characterizations of the Hausdorff dimension.{{clarify|date=March 2015}}&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
If there is a measure μ defined on Borel subsets of a metric space X such that μ(X) &amp;gt; 0 and μ(B(x, r)) ≤ r&amp;lt;sup&amp;gt;s&amp;lt;/sup&amp;gt; holds for some constant s &amp;gt; 0 and for every ball B(x, r) in X, then dim&amp;lt;sub&amp;gt;Haus&amp;lt;/sub&amp;gt;(X) ≥ s. A partial converse is provided by Frostman's lemma.&lt;br /&gt;
&lt;br /&gt;
如果在度量空间 ''X'' 的 Borel 子集上定义一个测度 μ，使得''μ''(''X'') &amp;gt; 0 和''μ''(''B''(''x'', ''r'')) ≤ ''r&amp;lt;sup&amp;gt;s&amp;lt;/sup&amp;gt;''，对于某个常数 ''s'' &amp;gt; 0  和 ''X'' 中的每个球 ''B''(''x'', ''r'') 成立，则 dim&amp;lt;sub&amp;gt;Haus&amp;lt;/sub&amp;gt;(''X'') ≥ ''s'' 。 部分逆向转换由弗洛斯曼引理定义。&lt;br /&gt;
&lt;br /&gt;
=== Behaviour under unions and products ===&lt;br /&gt;
&lt;br /&gt;
If &amp;lt;math&amp;gt;X=\bigcup_{i\in I}X_i&amp;lt;/math&amp;gt; is a finite or countable union, then&lt;br /&gt;
&lt;br /&gt;
If &amp;lt;math&amp;gt;X=\bigcup_{i\in I}X_i&amp;lt;/math&amp;gt; is a finite or countable union, then&lt;br /&gt;
&lt;br /&gt;
如果 &amp;lt;math&amp;gt;X=\bigcup_{i\in I}X_i&amp;lt;/math&amp;gt; 是一个有限或可数的联合，则&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \dim_{\operatorname{Haus}}(X) =\sup_{i\in I} \dim_{\operatorname{Haus}}(X_i).&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \dim_{\operatorname{Haus}}(X) =\sup_{i\in I} \dim_{\operatorname{Haus}}(X_i).&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
This can be verified directly from the definition.&lt;br /&gt;
&lt;br /&gt;
This can be verified directly from the definition.&lt;br /&gt;
&lt;br /&gt;
这可以直接从定义得到验证。&lt;br /&gt;
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&lt;br /&gt;
&lt;br /&gt;
If ''X'' and ''Y'' are non-empty metric spaces, then the Hausdorff dimension of their product satisfies&amp;lt;ref&amp;gt;{{cite journal |author=Marstrand, J. M. |title=The dimension of Cartesian product sets |journal=Proc. Cambridge Philos. Soc. |volume=50 |issue=3 |pages=198–202 |year=1954 |doi=10.1017/S0305004100029236 |bibcode = 1954PCPS...50..198M }}&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
If X and Y are non-empty metric spaces, then the Hausdorff dimension of their product satisfies&lt;br /&gt;
&lt;br /&gt;
如果 ''X'' 和''Y''是非空度量空间，那么它们乘积的豪斯多夫维数满足&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt; \dim_{\operatorname{Haus}}(X\times Y)\ge \dim_{\operatorname{Haus}}(X)+ \dim_{\operatorname{Haus}}(Y).&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \dim_{\operatorname{Haus}}(X\times Y)\ge \dim_{\operatorname{Haus}}(X)+ \dim_{\operatorname{Haus}}(Y).&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
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This inequality can be strict. It is possible to find two sets of dimension 0 whose product has dimension 1.&amp;lt;ref&amp;gt;{{cite book  | last = Falconer  | first = Kenneth J.  | title = Fractal geometry. Mathematical foundations and applications  | publisher = John Wiley &amp;amp; Sons, Inc., Hoboken, New Jersey  | year = 2003  | doi =   | isbn = }}&amp;lt;/ref&amp;gt; In the opposite direction, it is known that when ''X'' and ''Y'' are Borel subsets of '''R'''&amp;lt;sup&amp;gt;''n''&amp;lt;/sup&amp;gt;, the Hausdorff dimension of ''X'' × ''Y'' is bounded from above by the Hausdorff dimension of ''X'' plus the [[packing dimension|upper packing dimension]] of ''Y''. These facts are discussed in Mattila (1995).&lt;br /&gt;
&lt;br /&gt;
This inequality can be strict. It is possible to find two sets of dimension 0 whose product has dimension 1. In the opposite direction, it is known that when X and Y are Borel subsets of R&amp;lt;sup&amp;gt;n&amp;lt;/sup&amp;gt;, the Hausdorff dimension of X × Y is bounded from above by the Hausdorff dimension of X plus the upper packing dimension of Y. These facts are discussed in Mattila (1995).&lt;br /&gt;
&lt;br /&gt;
这种不平等可以是绝对的。有可能找到两个维数为0的集合，其乘积的维数为1。相反，我们知道当''X''和''Y''是 '''R'''&amp;lt;sup&amp;gt;''n''&amp;lt;/sup&amp;gt;的 Borel 子集时， ''X'' × ''Y''的豪斯多夫维数从上面以 ''X''的豪斯多夫维数加上 ''Y''的填充维数为界。Mattila (1995)曾就这些情况进行了讨论。&lt;br /&gt;
&lt;br /&gt;
==Self-similar sets自相似集合==&lt;br /&gt;
&lt;br /&gt;
{{refimprove section|date=March 2015}}&lt;br /&gt;
&lt;br /&gt;
Many sets defined by a self-similarity condition have dimensions which can be determined explicitly. Roughly, a set ''E'' is self-similar if it is the fixed point of a set-valued transformation ψ, that is ψ(''E'') = ''E'', although the exact definition is given below.&lt;br /&gt;
&lt;br /&gt;
Many sets defined by a self-similarity condition have dimensions which can be determined explicitly. Roughly, a set E is self-similar if it is the fixed point of a set-valued transformation ψ, that is ψ(E) = E, although the exact definition is given below.&lt;br /&gt;
&lt;br /&gt;
许多由自相似条件定义的集合具有可以显式确定的维数。粗略地说，集合''E'' 是自相似的，如果它是集值ψ变换的不动点，即ψ(''E'') = ''E''，尽管下面给出了确切的定义。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&amp;lt;blockquote&amp;gt;'''Theorem'''. Suppose&lt;br /&gt;
&lt;br /&gt;
&amp;lt;blockquote&amp;gt;Theorem. Suppose&lt;br /&gt;
&lt;br /&gt;
&amp;lt;blockquote&amp;gt;'''定理'''：假设&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt; \psi_i: \mathbf{R}^n \rightarrow \mathbf{R}^n, \quad i=1, \ldots , m &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \psi_i: \mathbf{R}^n \rightarrow \mathbf{R}^n, \quad i=1, \ldots , m &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
are [[Contraction mapping|contractive]] mappings on '''R'''&amp;lt;sup&amp;gt;''n''&amp;lt;/sup&amp;gt; with contraction constant ''r&amp;lt;sub&amp;gt;j&amp;lt;/sub&amp;gt;'' &amp;lt; 1. Then there is a unique ''non-empty'' compact set ''A'' such that&lt;br /&gt;
&lt;br /&gt;
are contractive mappings on R&amp;lt;sup&amp;gt;n&amp;lt;/sup&amp;gt; with contraction constant r&amp;lt;sub&amp;gt;j&amp;lt;/sub&amp;gt; &amp;lt; 1. Then there is a unique non-empty compact set A such that&lt;br /&gt;
&lt;br /&gt;
是'''R'''&amp;lt;sup&amp;gt;''n''&amp;lt;/sup&amp;gt;上的压缩常数''r&amp;lt;sub&amp;gt;j&amp;lt;/sub&amp;gt;'&amp;lt; 1的压缩映射。然后有一个唯一的非空紧集A &lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt; A = \bigcup_{i=1}^m \psi_i (A). &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; A = \bigcup_{i=1}^m \psi_i (A). &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&amp;lt;/blockquote&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;/blockquote&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The theorem follows from [[Stefan Banach]]'s [[Contractive mapping theorem|contractive mapping fixed point theorem]] applied to the complete metric space of non-empty compact subsets of '''R'''&amp;lt;sup&amp;gt;''n''&amp;lt;/sup&amp;gt; with the [[Hausdorff distance]].&amp;lt;ref&amp;gt;{{cite book |author=Falconer, K. J. |title=The Geometry of Fractal Sets |publisher=Cambridge University Press |location=Cambridge, UK |year=1985 |isbn=0-521-25694-1 |chapter=Theorem 8.3}}&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
The theorem follows from Stefan Banach's contractive mapping fixed point theorem applied to the complete metric space of non-empty compact subsets of R&amp;lt;sup&amp;gt;n&amp;lt;/sup&amp;gt; with the Hausdorff distance.&lt;br /&gt;
&lt;br /&gt;
这个定理来源于 Stefan Banach 的压缩映射不动点定理，该定理应用于 '''R'''&amp;lt;sup&amp;gt;''n''&amp;lt;/sup&amp;gt; 的非空紧子集的完备空间豪斯多夫距离。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
===The open set condition开集条件===&lt;br /&gt;
&lt;br /&gt;
To determine the dimension of the self-similar set ''A'' (in certain cases), we need a technical condition called the ''open set condition'' (OSC) on the sequence of contractions ψ&amp;lt;sub&amp;gt;''i''&amp;lt;/sub&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
To determine the dimension of the self-similar set A (in certain cases), we need a technical condition called the open set condition (OSC) on the sequence of contractions ψ&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
为了确定自相似集''A'' 的维数(在某些情况下) ，我们需要一个称为''开集条件''(OSC)的技术条件ψ&amp;lt;sub&amp;gt;''i''&amp;lt;/sub&amp;gt;。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
There is a relatively compact open set ''V'' such that&lt;br /&gt;
&lt;br /&gt;
There is a relatively compact open set V such that&lt;br /&gt;
&lt;br /&gt;
有一个相对紧的开集''V''&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt; \bigcup_{i=1}^m\psi_i (V) \subseteq V, &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \bigcup_{i=1}^m\psi_i (V) \subseteq V, &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
where the sets in union on the left are pairwise [[disjoint sets|disjoint]].&lt;br /&gt;
&lt;br /&gt;
where the sets in union on the left are pairwise disjoint.&lt;br /&gt;
&lt;br /&gt;
左边的集合是成对不相交的。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The open set condition is a separation condition that ensures the images ψ&amp;lt;sub&amp;gt;''i''&amp;lt;/sub&amp;gt;(''V'') do not overlap &amp;quot;too much&amp;quot;.&lt;br /&gt;
&lt;br /&gt;
The open set condition is a separation condition that ensures the images ψ&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;(V) do not overlap &amp;quot;too much&amp;quot;.&lt;br /&gt;
&lt;br /&gt;
开集条件是保证图像子ψ&amp;lt;sub&amp;gt;''i''&amp;lt;/sub&amp;gt;(''V'') 不重叠“太多”的分离条件。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
'''Theorem'''. Suppose the open set condition holds and each ψ&amp;lt;sub&amp;gt;''i''&amp;lt;/sub&amp;gt; is a similitude, that is a composition of an [[isometry]] and a [[dilation (metric space)|dilation]] around some point. Then the unique fixed point of ψ is a set whose Hausdorff dimension is ''s'' where ''s'' is the unique solution of&amp;lt;ref&amp;gt;{{cite journal | last=Hutchinson | first=John E. | title=Fractals and self similarity | journal=Indiana Univ. Math. J. | volume=30 | year=1981 | pages=713–747 | doi=10.1512/iumj.1981.30.30055 | issue=5 | doi-access=free }}&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
Theorem. Suppose the open set condition holds and each ψ&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt; is a similitude, that is a composition of an isometry and a dilation around some point. Then the unique fixed point of ψ is a set whose Hausdorff dimension is s where s is the unique solution of&lt;br /&gt;
&lt;br /&gt;
'''定理'''假设开集条件成立，并且每个ψ&amp;lt;sub&amp;gt;''i''&amp;lt;/sub&amp;gt; 是一个相似量，这是一个等距和围绕某一点的膨胀的合成。那么唯一的不动点是一个集合，它的豪斯多夫维数是 ''s'' ，其中  ''s'' 是 ''s'' &amp;lt;ref&amp;gt;{{cite journal | last=Hutchinson | first=John E. | title=Fractals and self similarity | journal=Indiana Univ. Math. J. | volume=30 | year=1981 | pages=713–747 | doi=10.1512/iumj.1981.30.30055 | issue=5 | doi-access=free }}&amp;lt;/ref&amp;gt;的唯一解&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt; \sum_{i=1}^m r_i^s = 1. &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \sum_{i=1}^m r_i^s = 1. &amp;lt;/math&amp;gt;&lt;br /&gt;
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The contraction coefficient of a similitude is the magnitude of the dilation.&lt;br /&gt;
&lt;br /&gt;
The contraction coefficient of a similitude is the magnitude of the dilation.&lt;br /&gt;
&lt;br /&gt;
相似物的收缩系数就是膨胀的大小。&lt;br /&gt;
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&lt;br /&gt;
&lt;br /&gt;
We can use this theorem to compute the Hausdorff dimension of the Sierpinski triangle (or sometimes called Sierpinski gasket). Consider three [[non-collinear points]] ''a''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;, ''a''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;, ''a''&amp;lt;sub&amp;gt;3&amp;lt;/sub&amp;gt; in the plane '''R'''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; and let ψ&amp;lt;sub&amp;gt;''i''&amp;lt;/sub&amp;gt; be the dilation of ratio 1/2 around ''a&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;''. The unique non-empty fixed point of the corresponding mapping ψ is a Sierpinski gasket and the dimension ''s'' is the unique solution of&lt;br /&gt;
&lt;br /&gt;
We can use this theorem to compute the Hausdorff dimension of the Sierpinski triangle (or sometimes called Sierpinski gasket). Consider three non-collinear points a&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;, a&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;, a&amp;lt;sub&amp;gt;3&amp;lt;/sub&amp;gt; in the plane R&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; and let ψ&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt; be the dilation of ratio 1/2 around a&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;. The unique non-empty fixed point of the corresponding mapping ψ is a Sierpinski gasket and the dimension s is the unique solution of&lt;br /&gt;
&lt;br /&gt;
我们可以使用这个定理来计算谢尔宾斯基三角形的豪斯多夫维数(或者有时候叫做谢尔宾斯基垫圈)。考虑R&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; 平面上的三个非共线点，''a''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;，''a''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;，''a''&amp;lt;sub&amp;gt;3&amp;lt;/sub&amp;gt;，让ψ&amp;lt;sub&amp;gt;''i''&amp;lt;/sub&amp;gt;是围绕着''a&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;''膨胀比率的1/2。对应映射的唯一非空不动点是一个谢尔宾斯基垫圈，其维数''s''是对应映射的唯一解&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt; \left(\frac{1}{2}\right)^s+\left(\frac{1}{2}\right)^s+\left(\frac{1}{2}\right)^s = 3 \left(\frac{1}{2}\right)^s =1. &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \left(\frac{1}{2}\right)^s+\left(\frac{1}{2}\right)^s+\left(\frac{1}{2}\right)^s = 3 \left(\frac{1}{2}\right)^s =1. &amp;lt;/math&amp;gt;&lt;br /&gt;
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Taking [[natural logarithm]]s of both sides of the above equation, we can solve for ''s'', that is: ''s'' = ln(3)/ln(2).  The Sierpinski gasket is self-similar and satisfies the OSC. In general a set ''E'' which is a fixed point of a mapping&lt;br /&gt;
&lt;br /&gt;
Taking natural logarithms of both sides of the above equation, we can solve for s, that is: s = ln(3)/ln(2).  The Sierpinski gasket is self-similar and satisfies the OSC. In general a set E which is a fixed point of a mapping&lt;br /&gt;
&lt;br /&gt;
取上述方程两边的自然对数，我们可以求出 ''s''，即: ''s'' = ln(3)/ln(2)。该密封垫具有自相似性，满足 OSC 要求。一般来说，集合 ''E''是一个映射的不动点&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt; A \mapsto \psi(A) = \bigcup_{i=1}^m \psi_i(A) &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt; A \mapsto \psi(A) = \bigcup_{i=1}^m \psi_i(A) &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
is self-similar if and only if the intersections&lt;br /&gt;
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is self-similar if and only if the intersections&lt;br /&gt;
&lt;br /&gt;
是自相似的，当且仅当&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt; H^s\left(\psi_i(E) \cap \psi_j(E)\right) =0, &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; H^s\left(\psi_i(E) \cap \psi_j(E)\right) =0, &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
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where ''s'' is the Hausdorff dimension of ''E'' and ''H&amp;lt;sup&amp;gt;s&amp;lt;/sup&amp;gt;'' denotes [[Hausdorff measure]]. This is clear in the case of the Sierpinski gasket (the intersections are just points), but is also true more generally:&lt;br /&gt;
&lt;br /&gt;
where s is the Hausdorff dimension of E and H&amp;lt;sup&amp;gt;s&amp;lt;/sup&amp;gt; denotes Hausdorff measure. This is clear in the case of the Sierpinski gasket (the intersections are just points), but is also true more generally:&lt;br /&gt;
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其中 ''s''是''E''的豪斯多夫维数， ''E'' and ''H&amp;lt;sup&amp;gt;s&amp;lt;/sup&amp;gt;'' 表示 豪斯多夫测度。对于谢尔宾斯基垫圈(交叉点就是点)来说，这一点很明显，但更普遍的情况是:&lt;br /&gt;
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'''Theorem'''. Under the same conditions as the previous theorem, the unique fixed point of ψ is self-similar.&lt;br /&gt;
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Theorem. Under the same conditions as the previous theorem, the unique fixed point of ψ is self-similar.&lt;br /&gt;
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'''定理'''：在与前一定理相同的条件下，其唯一不动点是自相似的。&lt;br /&gt;
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==See also参阅==&lt;br /&gt;
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* [[List of fractals by Hausdorff dimension豪斯多夫分形维数列表]] Examples of deterministic fractals, random and natural fractals.确定性分形与随机和自然分形的示例。&lt;br /&gt;
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* [[Assouad dimension  Assouad维数]], another variation of fractal dimension that, like Hausdorff dimension, is defined using coverings by balls其他被球覆盖方式定义的分形维数，例如豪斯多夫维数。&lt;br /&gt;
&lt;br /&gt;
* [[Intrinsic dimension固有维数]]&lt;br /&gt;
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* [[Packing dimension填充维数]]&lt;br /&gt;
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* [[Fractal dimension分形维数]]&lt;br /&gt;
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==References参考文献==&lt;br /&gt;
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{{reflist}}&lt;br /&gt;
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==Further reading拓展阅读==&lt;br /&gt;
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* {{cite book |last1=Dodson |first1=M. Maurice |title=Fractal Geometry and Applications: A Jubilee of Benoît Mandelbrot |volume=72 |issue=1 |pages=305–347 |last2=Kristensen |first2=Simon |chapter=Hausdorff Dimension and Diophantine Approximation |date=June 12, 2003 |arxiv=math/0305399 |bibcode = 2003math......5399D |doi=10.1090/pspum/072.1/2112110|series=Proceedings of Symposia in Pure Mathematics |isbn=9780821836378 }}&lt;br /&gt;
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* {{cite book |last1=Hurewicz |first1=Witold |authorlink1=Witold Hurewicz |last2=Wallman |first2=Henry |authorlink2=Henry Wallman |title=Dimension Theory |url=https://archive.org/details/in.ernet.dli.2015.84609 |publisher=Princeton University Press |year=1948 }}&lt;br /&gt;
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* {{cite journal |author作者=E. Szpilrajn |authorlink=Edward Marczewski |title=La dimension et la mesure |journal=Fundamenta Mathematicae |volume=28 |pages=81–9 |year=1937 }}&lt;br /&gt;
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* {{cite journal&lt;br /&gt;
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 | last1=Marstrand&lt;br /&gt;
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 | last1=Marstrand&lt;br /&gt;
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 | last1=马斯特兰德&lt;br /&gt;
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 | first1=J. M. | title=The dimension of cartesian product sets | year=1954 | journal=Proc. Cambridge Philos. Soc.&lt;br /&gt;
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 | first1=J. M. | title=The dimension of cartesian product sets | year=1954 | journal=Proc. Cambridge Philos. Soc.&lt;br /&gt;
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 | first1= J. M. | title=笛卡儿积集的维数 | 1954年 |  journal=Proc. Cambridge Philos. Soc.&lt;br /&gt;
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 | volume=50&lt;br /&gt;
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 | volume=50&lt;br /&gt;
&lt;br /&gt;
 | 第50卷&lt;br /&gt;
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 | issue=3&lt;br /&gt;
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 | issue=3&lt;br /&gt;
&lt;br /&gt;
 | 第三期&lt;br /&gt;
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 | pages=198–202&lt;br /&gt;
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 | pages=198–202&lt;br /&gt;
&lt;br /&gt;
 | 第198-202页&lt;br /&gt;
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 | doi=10.1017/S0305004100029236|bibcode = 1954PCPS...50..198M }}&lt;br /&gt;
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 | doi=10.1017/S0305004100029236|bibcode = 1954PCPS...50..198M }}&lt;br /&gt;
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10.1017 / S0305004100029236 | bibcode 1954PCPS... 50. . 198 m }&lt;br /&gt;
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* {{Cite book&lt;br /&gt;
&lt;br /&gt;
 | last1=Mattila&lt;br /&gt;
&lt;br /&gt;
 | last1=Mattila&lt;br /&gt;
&lt;br /&gt;
 | last1=Mattila&lt;br /&gt;
&lt;br /&gt;
 | first1=Pertti | author1-link=Pertti Mattila| title=Geometry of sets and measures in Euclidean spaces | publisher=[[Cambridge University Press]]&lt;br /&gt;
&lt;br /&gt;
 | first1=Pertti | author1-link=Pertti Mattila| title=Geometry of sets and measures in Euclidean spaces | publisher=Cambridge University Press&lt;br /&gt;
&lt;br /&gt;
| first1 Pertti | author1-link Pertti Mattila | title 欧几里德空间中集合和度量的几何 | 出版商剑桥大学出版社&lt;br /&gt;
&lt;br /&gt;
 | isbn=978-0-521-65595-8 | year=1995}}&lt;br /&gt;
&lt;br /&gt;
 | isbn=978-0-521-65595-8 | year=1995}}&lt;br /&gt;
&lt;br /&gt;
| isbn 978-0-521-65595-8 | year 1995}&lt;br /&gt;
&lt;br /&gt;
* {{cite journal |author=A. S. Besicovitch |authorlink=A. S. Besicovitch |title=On Linear Sets of Points of Fractional Dimensions |journal=[[Mathematische Annalen]] |volume=101 |year=1929 | doi=10.1007/BF01454831| issue=1 |pages= 161–193}}&lt;br /&gt;
&lt;br /&gt;
* {{cite journal |author1=A. S. Besicovitch |authorlink1=A. S. Besicovitch |author2=H. D. Ursell |authorlink2=H. D. Ursell |title=Sets of Fractional Dimensions |journal=Journal of the London Mathematical Society |volume=12 |year=1937 | issue=1 | doi=10.1112/jlms/s1-12.45.18  | pages=18–25 }}&amp;lt;br/&amp;gt;Several selections from this volume are reprinted in {{cite book |author=Edgar, Gerald A. |title=Classics on fractals |publisher=Addison-Wesley |location=Boston |year=1993 |isbn=0-201-58701-7}} See chapters 9,10,11&lt;br /&gt;
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* {{cite journal |author=F. Hausdorff |authorlink=F. Hausdorff |title=Dimension und äußeres Maß |journal=Mathematische Annalen |volume=79 |issue=1–2 |pages=157–179 |date=March 1919 |doi=10.1007/BF01457179|hdl=10338.dmlcz/100363 |url=http://dml.cz/bitstream/handle/10338.dmlcz/100363/CzechMathJ_09-1959-3_5.pdf }}&lt;br /&gt;
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* {{cite journal | last=Hutchinson | first=John E. | title=Fractals and self similarity | journal=Indiana Univ. Math. J. | volume=30 | year=1981 | pages=713–747 | doi=10.1512/iumj.1981.30.30055 | issue=5 | doi-access=free }}&lt;br /&gt;
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*{{cite book | last=Falconer | first = Kenneth |title=Fractal Geometry: Mathematical Foundations and Applications | publisher=[[John Wiley and Sons]] | edition=2nd | year=2003}}&lt;br /&gt;
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==External links外部链接==&lt;br /&gt;
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* [https://www.encyclopediaofmath.org/index.php/Hausdorff_dimension Hausdorff dimension] 在 [https://www.encyclopediaofmath.org/ Encyclopedia of Mathematics]&lt;br /&gt;
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* [https://www.encyclopediaofmath.org/index.php/Hausdorff_measure Hausdorff measure] 在 [https://www.encyclopediaofmath.org/ Encyclopedia of Mathematics]&lt;br /&gt;
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{{DEFAULTSORT:Hausdorff Dimension豪斯多夫维数}}&lt;br /&gt;
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[[Category分类:Fractals分形]]&lt;br /&gt;
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[[Category分类:Metric geometry度量几何]]&lt;br /&gt;
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[[Category分类:Dimension theory维度理论]]&lt;br /&gt;
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&amp;lt;small&amp;gt;This page was moved from [[wikipedia:en:Hausdorff dimension]]. Its edit history can be viewed at [[分形维数/edithistory]]&amp;lt;/small&amp;gt;&amp;lt;/noinclude&amp;gt;&lt;br /&gt;
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[[Category:待整理页面]]&lt;/div&gt;</summary>
		<author><name>Ruili</name></author>
	</entry>
	<entry>
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		<title>分形维数</title>
		<link rel="alternate" type="text/html" href="https://wiki.swarma.org/index.php?title=%E5%88%86%E5%BD%A2%E7%BB%B4%E6%95%B0&amp;diff=17694"/>
		<updated>2020-11-01T09:13:02Z</updated>

		<summary type="html">&lt;p&gt;Ruili：&lt;/p&gt;
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&lt;div&gt;此词条暂由彩云小译翻译，未经人工整理和审校，带来阅读不便，请见谅。&lt;br /&gt;
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{{short description|Invariant}}&lt;br /&gt;
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Example of non-integer dimensions. The first four [[iteration]]s of the [[Koch snowflake|Koch curve]], where after each iteration, all original line segments are replaced with four, each a self-similar copy that is 1/3 the length of the original. One formalism of the Hausdorff dimension uses this scale factor (3) and the number of self-similar objects (4) to calculate the dimension, D, after the first iteration to be D = (log N)/(log S) = (log 4)/(log 3) ≈ 1.26.&amp;lt;ref name=CampbellAnnenberg15&amp;gt;MacGregor Campbell, 2013, &amp;quot;5.6 Scaling and the Hausdorff Dimension,&amp;quot; at ''Annenberg Learner:MATHematics illuminated'', see [http://www.learner.org/courses/mathilluminated/units/5/textbook/06.php], accessed 5 March 2015.&amp;lt;/ref&amp;gt; That is, while the Hausdorff dimension of a single [[point (geometry)|point]] is zero, of a [[line segment]] is 1, of a [[square]] is 2, and of a [[cube]] is 3, for [[fractal]]s such as this, the object can have a non-integer dimension.&lt;br /&gt;
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Example of non-integer dimensions. The first four iterations of the Koch curve, where after each iteration, all original line segments are replaced with four, each a self-similar copy that is 1/3 the length of the original. One formalism of the Hausdorff dimension uses this scale factor (3) and the number of self-similar objects (4) to calculate the dimension, D, after the first iteration to be D = (log N)/(log S) = (log 4)/(log 3) ≈ 1.26. That is, while the Hausdorff dimension of a single point is zero, of a line segment is 1, of a square is 2, and of a cube is 3, for fractals such as this, the object can have a non-integer dimension.&lt;br /&gt;
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非整数维度示例：前四个[[Koch 曲线]]的迭代，在每次迭代后，所有原始线段都被替换为四个，每个自相似的复制是原始线段长度的1 / 3。豪斯多夫维数的一个建模是使用比例因子(3)和自相似对象的数量(4)来计算维度 D，在第一次迭代后为 D = (log N)/(log S) = (log 4)/(log 3) ≈ 1.26.&amp;lt;ref name=CampbellAnnenberg15&amp;gt;。MacGregor Campbell, 2013, &amp;quot;5.6 Scaling and the Hausdorff Dimension,&amp;quot; 在 ''Annenberg Learner:MATHematics illuminated'', 参见 [http://www.learner.org/courses/mathilluminated/units/5/textbook/06.php], accessed 5 March 2015.&amp;lt;/ref&amp;gt; 也就是说，单点的豪斯多夫维数为零，线段为1，正方形为2，立方体为3时，但对于分形，对象可以有一个非整数维度。&lt;br /&gt;
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In [[mathematics]], '''Hausdorff dimension''' is a measure of ''roughness'', or more specifically, [[fractal dimension]], that was first introduced in 1918 by [[mathematician]] [[Felix Hausdorff]].&amp;lt;ref&amp;gt;{{Cite journal |arxiv = 1101.1444|doi = 10.1214/11-STS370|title = Estimators of Fractal Dimension: Assessing the Roughness of Time Series and Spatial Data|journal = Statistical Science|volume = 27|issue = 2|pages = 247–277|year = 2012|last1 = Gneiting|first1 = Tilmann|last2 = Ševčíková|first2 = Hana|last3 = Percival|first3 = Donald B.}}&amp;lt;/ref&amp;gt; For instance, the Hausdorff dimension of a single [[point (geometry)|point]] is zero, of a [[line segment]] is 1, of a [[square]] is 2, and of a [[cube]] is 3. That is, for sets of points that define a smooth shape or a shape that has a small number of corners—the shapes of traditional geometry and science—the Hausdorff dimension is an [[integer]] agreeing with the usual sense of dimension, also known as the [[Inductive dimension|topological dimension]]. However, formulas have also been developed that allow calculation of the dimension of other less simple objects, where, solely on the basis of their properties of [[scaling (geometry)|scaling]] and [[self-similarity]], one is led to the conclusion that particular objects—including [[fractal]]s—have non-integer Hausdorff dimensions. Because of the significant technical advances made by [[Abram Samoilovitch Besicovitch]] allowing computation of dimensions for highly irregular or &amp;quot;rough&amp;quot; sets, this dimension is also commonly referred to as the ''Hausdorff–Besicovitch dimension.''&lt;br /&gt;
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In mathematics, Hausdorff dimension is a measure of roughness, or more specifically, fractal dimension, that was first introduced in 1918 by mathematician Felix Hausdorff. For instance, the Hausdorff dimension of a single point is zero, of a line segment is 1, of a square is 2, and of a cube is 3. That is, for sets of points that define a smooth shape or a shape that has a small number of corners—the shapes of traditional geometry and science—the Hausdorff dimension is an integer agreeing with the usual sense of dimension, also known as the topological dimension. However, formulas have also been developed that allow calculation of the dimension of other less simple objects, where, solely on the basis of their properties of scaling and self-similarity, one is led to the conclusion that particular objects—including fractals—have non-integer Hausdorff dimensions. Because of the significant technical advances made by Abram Samoilovitch Besicovitch allowing computation of dimensions for highly irregular or &amp;quot;rough&amp;quot; sets, this dimension is also commonly referred to as the Hausdorff–Besicovitch dimension.&lt;br /&gt;
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在[[数学]]中，'''&amp;lt;font color = '#ff8000'&amp;gt;豪斯多夫维数Hausdorff dimension&amp;lt;/font&amp;gt;'''是一种粗糙度的度量单位，或者更确切地说，分形维数，是由数学家 Felix Hausdorff 在1918年首次提出的。例如，单点的豪斯多夫维数为零，线段为1，正方形为2，立方体为3。也就是说，对于定义了一个光滑形状或一个有少数几个角的形状---- 传统几何学和科学的形状---- 的点集来说，豪斯多夫维数是一个整数，符合通常的维度意义，也称为拓扑维度。然而，还有一些公式允许计算其他不太简单的对象的维数，其中仅仅根据它们的标度和自相似特性，就可以得出结论: 特定的对象ー包括分形ー具有非整数的 Hausdorff 维数。由于阿布拉姆·萨莫伊洛维奇·贝西科维奇的重大技术进步，允许计算高度不规则或“粗糙”集的维度，这个维度通常也被称为 Hausdorff-Besicovitch 维度。 &lt;br /&gt;
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The Hausdorff dimension, more specifically, is a further dimensional number associated with a given set, where the distances between all members of that set are defined. Such a set is termed a [[metric space]]. The dimension is drawn from the [[Extended real number line|extended real numbers]], &amp;lt;math&amp;gt;\overline{\mathbb{R}}&amp;lt;/math&amp;gt;, as opposed to the more intuitive notion of dimension, which is not associated to general metric spaces, and only takes values in the non-negative integers.&lt;br /&gt;
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The Hausdorff dimension, more specifically, is a further dimensional number associated with a given set, where the distances between all members of that set are defined. Such a set is termed a metric space. The dimension is drawn from the extended real numbers, &amp;lt;math&amp;gt;\overline{\mathbb{R}}&amp;lt;/math&amp;gt;, as opposed to the more intuitive notion of dimension, which is not associated to general metric spaces, and only takes values in the non-negative integers.&lt;br /&gt;
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更具体地说，豪斯多夫维数是一个与给定集合相关联的更进一步的维数，其中定义了该集合所有成员之间的距离。这样的集合称为度量空间。维数是从扩展的实数，&amp;lt;math&amp;gt;\overline{\mathbb{R}}&amp;lt;/math&amp;gt;，而不是更直观的维数概念(它不与一般的度量空间相关联，只取非负整数的值)。&lt;br /&gt;
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In mathematical terms, the Hausdorff dimension generalizes the notion of the dimension of a real [[vector space]]. That is, the Hausdorff dimension of an ''n''-dimensional [[inner product space]] equals ''n''. This underlies the earlier statement that the Hausdorff dimension of a point is zero, of a line is one, etc., and that [[fractal|irregular sets]] can have noninteger Hausdorff dimensions. For instance, the [[Koch snowflake]] shown at right is constructed from an equilateral triangle; in each iteration, its component line segments are divided into 3 segments of unit length, the newly created middle segment is used as the base of a new [[equilateral]] triangle that points outward, and this base segment is then deleted to leave a final object from the iteration of unit length of 4.&amp;lt;ref&amp;gt;Larry Riddle, 2014, &amp;quot;Classic Iterated Function Systems: Koch Snowflake&amp;quot;, Agnes Scott College e-Academy (online), see [http://ecademy.agnesscott.edu/~lriddle/ifs/ksnow/ksnow.htm], accessed 5 March 2015.&amp;lt;/ref&amp;gt; That is, after the first iteration, each original line segment has been replaced with N=4, where each self-similar copy is 1/S = 1/3 as long as the original.&amp;lt;ref name=CampbellAnnenberg15/&amp;gt; Stated another way, we have taken an object with Euclidean dimension, D, and reduced its linear scale by 1/3 in each direction, so that its length increases to N=S&amp;lt;sup&amp;gt;D&amp;lt;/sup&amp;gt;.&amp;lt;ref name=ClaytonSCTPLS96&amp;gt;Keith Clayton, 1996, &amp;quot;Fractals and the Fractal Dimension,&amp;quot; ''Basic Concepts in Nonlinear Dynamics and Chaos'' (workshop), Society for Chaos Theory in Psychology and the Life Sciences annual meeting, June 28, 1996, Berkeley, California, see [http://www.vanderbilt.edu/AnS/psychology/cogsci/chaos/workshop/Workshop.html], accessed 5 March 2015.&amp;lt;/ref&amp;gt; This equation is easily solved for D, yielding the ratio of logarithms (or [[natural logarithm]]s) appearing in the figures, and giving—in the Koch and other fractal cases—non-integer dimensions for these objects.&lt;br /&gt;
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In mathematical terms, the Hausdorff dimension generalizes the notion of the dimension of a real vector space. That is, the Hausdorff dimension of an n-dimensional inner product space equals n. This underlies the earlier statement that the Hausdorff dimension of a point is zero, of a line is one, etc., and that irregular sets can have noninteger Hausdorff dimensions. For instance, the Koch snowflake shown at right is constructed from an equilateral triangle; in each iteration, its component line segments are divided into 3 segments of unit length, the newly created middle segment is used as the base of a new equilateral triangle that points outward, and this base segment is then deleted to leave a final object from the iteration of unit length of 4. That is, after the first iteration, each original line segment has been replaced with N=4, where each self-similar copy is 1/S = 1/3 as long as the original. This equation is easily solved for D, yielding the ratio of logarithms (or natural logarithms) appearing in the figures, and giving—in the Koch and other fractal cases—non-integer dimensions for these objects.&lt;br /&gt;
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用数学术语来说，豪斯多夫维数概括了实向量空间维数的概念。也就是说，n 维内积空间的豪斯多夫维数等于 n。 这就是早期假设的基础，一个点的豪斯多夫维数是零，一条线是一等等，不规则集可以有非整数的豪斯多夫维数。例如，右边所示的 Koch 雪花是由一个正三角形构成的; 在每次迭代中，它的组成线段被分成单位长度的3段，新创建的中间线段被用作一个指向外部的新正三角形的基础，然后人们删除这个基础线段用来保留单位长度4的迭代中的最终对象。也就是说，在第一次迭代之后，每个原始线段都被替换为 N=4，其中每个自相似拷贝的长度是原始线段的1/S = 1/3 。这个方程很容易求解为 D，产生出现在图形中的对数(或自然对数)的比率，并给出——在 Koch 和其他分形情况下——这些对象的非整数维数。&lt;br /&gt;
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The Hausdorff dimension is a successor to the simpler, but usually equivalent, box-counting or [[Minkowski–Bouligand dimension]].&lt;br /&gt;
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The Hausdorff dimension is a successor to the simpler, but usually equivalent, box-counting or Minkowski–Bouligand dimension.&lt;br /&gt;
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豪斯多夫维数是更简单但通常等价的'''&amp;lt;font color = '#ff8000'&amp;gt;计盒维数box-counting&amp;lt;/font&amp;gt;'''或'''&amp;lt;font color = '#ff8000'&amp;gt;闵可夫斯基维数Minkowski-Bouligand&amp;lt;/font&amp;gt;'''的继承者。&lt;br /&gt;
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==Intuition概念==&lt;br /&gt;
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{{refimprove section|date=March 2015}}&lt;br /&gt;
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The intuitive concept of dimension of a geometric object ''X'' is the number of independent parameters one needs to pick out a unique point inside. However, any point specified by two parameters can be instead specified by one, because the [[cardinality]] of the [[real plane]] is equal to the cardinality of the [[real line]] (this can be seen by an [[Cantor's diagonal argument|argument]] involving interweaving the digits of two numbers to yield a single number encoding the same information). The example of a [[space-filling curve]] shows that one can even map the real line to the real plane [[Surjective function|surjectively]] (taking one real number into a pair of real numbers in a way so that all pairs of numbers are covered) and ''continuously'', so that a one-dimensional object completely fills up a higher-dimensional object.&lt;br /&gt;
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The intuitive concept of dimension of a geometric object X is the number of independent parameters one needs to pick out a unique point inside. However, any point specified by two parameters can be instead specified by one, because the cardinality of the real plane is equal to the cardinality of the real line (this can be seen by an argument involving interweaving the digits of two numbers to yield a single number encoding the same information). The example of a space-filling curve shows that one can even map the real line to the real plane surjectively (taking one real number into a pair of real numbers in a way so that all pairs of numbers are covered) and continuously, so that a one-dimensional object completely fills up a higher-dimensional object.&lt;br /&gt;
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几何物体X的直观尺寸概念就是一个物体需要多少个独立参数才能找到一个独特的点。但是，任何由两个参数指定的点都可以由一个参数指定，因为实际平面的基数等于实际行的基数(这可以通过一个参数看到，该参数涉及交织两个数字的数字以产生一个编码相同信息的单个数字)。'''&amp;lt;font color = '#ff8000'&amp;gt;皮亚诺曲线&amp;lt;/font&amp;gt;'''的例子表明，一个人甚至可以完美和连续地映射实际线到真正的平面(把一个实数转换成一对实数，这样所有的数对都被覆盖)，由此一维物体完全填充了一个高维物体。&lt;br /&gt;
几何对象X的尺寸的直观概念是指需要多少个独立参数才能找到一个独特的点。但是，任何由两个参数指定的点都可以由一个参数指定，因为为实平面的基数等于实线的基数(这可以通过交织两个数字以产生一个编码相同信息的单个数字看到)。'''&amp;lt;font color = '#ff8000'&amp;gt;皮亚诺曲线&amp;lt;/font&amp;gt;'''的例子表明，可以将实线完美和连续地映射到实平面(把一个实数转换成一对实数，从而覆盖所有实数对)，由此一维对象完全填充了一个高维对象。&lt;br /&gt;
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Every space filling curve hits some points multiple times, and does not have a continuous inverse. It is impossible to map two dimensions onto one in a way that is continuous and continuously invertible. The topological dimension, also called [[Lebesgue covering dimension]], explains why. This dimension is ''n'' if, in every covering of ''X'' by small open balls, there is at least one point where ''n''&amp;amp;nbsp;+&amp;amp;nbsp;1 balls overlap. For example, when one covers a line with short open intervals, some points must be covered twice, giving dimension&amp;amp;nbsp;''n''&amp;amp;nbsp;=&amp;amp;nbsp;1.&lt;br /&gt;
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Every space filling curve hits some points multiple times, and does not have a continuous inverse. It is impossible to map two dimensions onto one in a way that is continuous and continuously invertible. The topological dimension, also called Lebesgue covering dimension, explains why. This dimension is n if, in every covering of X by small open balls, there is at least one point where n&amp;amp;nbsp;+&amp;amp;nbsp;1 balls overlap. For example, when one covers a line with short open intervals, some points must be covered twice, giving dimension&amp;amp;nbsp;n&amp;amp;nbsp;=&amp;amp;nbsp;1.&lt;br /&gt;
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每条空间填充曲线都会多次撞击某些点，且不存在连续的倒数。将两个维度以连续和连续可逆的方式映射到一个维度是不可能的。'''&amp;lt;font color = '#ff8000'&amp;gt;拓扑维度 topological dimension&amp;lt;/font&amp;gt;'''，也被称为拓朴维数，解释了为什么。这个维度是 n，如果在 x 的每个小开球覆盖中，至少有一个点 n + 1个球重叠。例如，当一个点覆盖一条具有短开区间的直线时，某些点必须被覆盖两次，给出维数''n''&amp;amp;nbsp;=&amp;amp;nbsp;1。&lt;br /&gt;
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But topological dimension is a very crude measure of the local size of a space (size near a point). A curve that is almost space-filling can still have topological dimension one, even if it fills up most of the area of a region. A [[fractal]] has an integer topological dimension, but in terms of the amount of space it takes up, it behaves like a higher-dimensional space.&lt;br /&gt;
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But topological dimension is a very crude measure of the local size of a space (size near a point). A curve that is almost space-filling can still have topological dimension one, even if it fills up most of the area of a region. A fractal has an integer topological dimension, but in terms of the amount of space it takes up, it behaves like a higher-dimensional space.&lt;br /&gt;
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但是，拓扑维度是对空间局部尺寸(点附近的尺寸)的一个非常粗略的度量。一条几乎是空间填充的曲线仍然可以有一维拓扑，即使它填充了一个区域的大部分面积。分形具有整数的拓扑维数，但就其所占空间的数量而言，它看起来像一个更高维的空间。&lt;br /&gt;
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The Hausdorff dimension measures the local size of a space taking into account the distance between points, the [[metric space|metric]]. Consider the number ''N''(''r'') of [[ball (mathematics)|balls]] of radius at most ''r'' required to cover ''X'' completely. When ''r'' is very small, ''N''(''r'') grows polynomially with 1/''r''. For a sufficiently well-behaved  ''X'', the Hausdorff dimension is the unique number ''d'' such that N(''r'') grows as 1/''r&amp;lt;sup&amp;gt;d&amp;lt;/sup&amp;gt;'' as ''r'' approaches zero. More precisely, this defines the [[Minkowski–Bouligand dimension|box-counting dimension]], which equals the Hausdorff dimension when the value ''d'' is a critical boundary between growth rates that are insufficient to cover the space, and growth rates that are overabundant.&lt;br /&gt;
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The Hausdorff dimension measures the local size of a space taking into account the distance between points, the metric. Consider the number N(r) of balls of radius at most r required to cover X completely. When r is very small, N(r) grows polynomially with 1/r. For a sufficiently well-behaved  X, the Hausdorff dimension is the unique number d such that N(r) grows as 1/r&amp;lt;sup&amp;gt;d&amp;lt;/sup&amp;gt; as r approaches zero. More precisely, this defines the box-counting dimension, which equals the Hausdorff dimension when the value d is a critical boundary between growth rates that are insufficient to cover the space, and growth rates that are overabundant.&lt;br /&gt;
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豪斯多夫维数测量一个空间的局部大小时，会考虑到点之间距离的度量。考虑半径最大为 r 的球数 ''N'' (r) ，需要完全覆盖 ''X''。当 r 很小时，n (r)以1/''r'' 增长多项式。对于一个表现足够好的 ''X''，豪斯多夫维数是唯一的数 d，这样当 r 趋近于零时， N(r)增长为1/r&amp;lt;sup&amp;gt;d&amp;lt;/sup&amp;gt; 。更确切地说，这定义了盒子计数维度，当值 d 是不足以覆盖空间的增长率和过度充裕的增长率之间的关键边界时，它等于豪斯多夫维数。&lt;br /&gt;
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For shapes that are smooth, or shapes with a small number of corners, the shapes of traditional geometry and science, the Hausdorff dimension is an integer agreeing with the topological dimension. But [[Benoit Mandelbrot]] observed that [[fractal]]s, sets with noninteger Hausdorff dimensions, are found everywhere in nature. He observed that the proper idealization of most rough shapes you see around you is not in terms of smooth idealized shapes, but in terms of fractal idealized shapes:&lt;br /&gt;
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For shapes that are smooth, or shapes with a small number of corners, the shapes of traditional geometry and science, the Hausdorff dimension is an integer agreeing with the topological dimension. But Benoit Mandelbrot observed that fractals, sets with noninteger Hausdorff dimensions, are found everywhere in nature. He observed that the proper idealization of most rough shapes you see around you is not in terms of smooth idealized shapes, but in terms of fractal idealized shapes:&lt;br /&gt;
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对于光滑的形状，或者有少量棱角的形状，传统几何和科学的形状，豪斯多夫维数是一个整数，与拓扑维度一致。但是伯努·曼德布洛特观察到分形---- 具有非整数豪斯多夫维数的集合---- 在自然界中随处可见。他观察到，我们周围大多数粗糙形状的理想化不是光滑的理想化形状，而是分形理想化形状:&lt;br /&gt;
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&amp;lt;blockquote&amp;gt;Clouds are not spheres, mountains are not cones, coastlines are not circles, and bark is not smooth, nor does lightning travel in a straight line.&amp;lt;ref name=&amp;quot;mandelbrot&amp;quot;&amp;gt;{{cite book   | last = Mandelbrot   | first = Benoît   | authorlink = Benoit Mandelbrot   | title = The Fractal Geometry of Nature   | publisher = W. H. Freeman   | series = Lecture notes in mathematics 1358   | year = 1982   | doi =    | isbn = 0-7167-1186-9   | url-access = registration   | url = https://archive.org/details/fractalgeometryo00beno   }}&amp;lt;/ref&amp;gt;&amp;lt;/blockquote&amp;gt;&lt;br /&gt;
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&amp;lt;blockquote&amp;gt;Clouds are not spheres, mountains are not cones, coastlines are not circles, and bark is not smooth, nor does lightning travel in a straight line.&amp;lt;/blockquote&amp;gt;&lt;br /&gt;
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&amp;lt;blockquote&amp;gt;云不是球体，山不是锥体，海岸线不是圆圈，树皮不平滑，闪电也不是直线运动。 &amp;lt;/blockquote&amp;gt;&lt;br /&gt;
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For fractals that occur in nature, the Hausdorff and [[Minkowski–Bouligand dimension|box-counting dimension]] coincide. The [[packing dimension]] is yet another similar notion which gives the same value for many shapes, but there are well documented exceptions where all these dimensions differ.&lt;br /&gt;
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For fractals that occur in nature, the Hausdorff and box-counting dimension coincide. The packing dimension is yet another similar notion which gives the same value for many shapes, but there are well documented exceptions where all these dimensions differ.&lt;br /&gt;
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对于自然界中出现的分形，豪斯多夫维数和盒计数维数是一致的。封装尺寸是另一个类似的概念，它给出了许多形状相同的值，但是在所有这些尺寸不同的情况，都做了很好的说明。&lt;br /&gt;
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==Formal definitions形式化定义==&lt;br /&gt;
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{{unreferenced section|date=March 2015}}&lt;br /&gt;
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===Hausdorff content豪斯多夫集===&lt;br /&gt;
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Let ''X'' be a [[metric space]]. If ''S'' ⊂ ''X'' and ''d'' ∈ [0, ∞), the ''d''-dimensional '''unlimited Hausdorff content''' of ''S'' is defined by&lt;br /&gt;
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Let X be a metric space. If S ⊂ X and d ∈ [0, ∞), the d-dimensional unlimited Hausdorff content of S is defined by&lt;br /&gt;
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设 ''X''是度量空间。若''S'' ⊂ ''X'' 和 ''d'' ∈ [0, ∞) ，则 ''S'' 的''d''维无限 豪斯多夫集定义为&lt;br /&gt;
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:&amp;lt;math&amp;gt;C_H^d(S):=\inf\Bigl\{\sum_i r_i^d:\text{ there is a cover of } S\text{ by balls with radii }r_i&amp;gt;0\Bigr\}.&amp;lt;/math&amp;gt;&lt;br /&gt;
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&amp;lt;math&amp;gt;C_H^d(S):=\inf\Bigl\{\sum_i r_i^d:\text{ there is a cover of } S\text{ by balls with radii }r_i&amp;gt;0\Bigr\}.&amp;lt;/math&amp;gt;&lt;br /&gt;
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&amp;lt;math&amp;gt;C_H^d(S):=\inf\Bigl\{\sum_i r_i^d:\text{ there is a cover of } S\text{ by balls with radii }r_i&amp;gt;0\Bigr\}.&amp;lt;/math&amp;gt;&lt;br /&gt;
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In other words, &amp;lt;math&amp;gt;C_H^d(S)&amp;lt;/math&amp;gt; is the [[infimum]] of the set of numbers &amp;lt;math&amp;gt;\delta \geq 0&amp;lt;/math&amp;gt; such that there is some (indexed) collection of [[ball (mathematics)|ball]]s &amp;lt;math&amp;gt;\{B(x_i,r_i):i\in I\}&amp;lt;/math&amp;gt; covering ''S'' with ''r&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;''&amp;amp;nbsp;&amp;gt;&amp;amp;nbsp;0 for each ''i''&amp;amp;nbsp;∈&amp;amp;nbsp;''I'' that satisfies &amp;lt;math&amp;gt;\sum_{i\in I} r_i^d&amp;lt;\delta &amp;lt;/math&amp;gt;. (Here, we use the standard convention that [[infimum|inf&amp;amp;nbsp;Ø&amp;amp;nbsp;=&amp;amp;nbsp;∞]].)&lt;br /&gt;
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In other words, &amp;lt;math&amp;gt;C_H^d(S)&amp;lt;/math&amp;gt; is the infimum of the set of numbers &amp;lt;math&amp;gt;\delta \geq 0&amp;lt;/math&amp;gt; such that there is some (indexed) collection of balls &amp;lt;math&amp;gt;\{B(x_i,r_i):i\in I\}&amp;lt;/math&amp;gt; covering S with r&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;&amp;amp;nbsp;&amp;gt;&amp;amp;nbsp;0 for each i&amp;amp;nbsp;∈&amp;amp;nbsp;I that satisfies &amp;lt;math&amp;gt;\sum_{i\in I} r_i^d&amp;lt;\delta &amp;lt;/math&amp;gt;. (Here, we use the standard convention that inf&amp;amp;nbsp;Ø&amp;amp;nbsp;=&amp;amp;nbsp;∞.)&lt;br /&gt;
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换句话说，&amp;lt;math&amp;gt;C_H^d(S)&amp;lt;/math&amp;gt; 是数字集合&amp;lt;math&amp;gt;\delta \geq 0&amp;lt;/math&amp;gt;的下确界，使得在 ''i''&amp;amp;nbsp;∈&amp;amp;nbsp中存在一些球集合 &amp;lt;math&amp;gt;\{B(x_i,r_i):i\in I\}&amp;lt;/math&amp;gt;  i 包含 s，对于每个 ''r&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;''&amp;amp;nbsp;&amp;gt;&amp;amp;nbsp;0 满足 i 中的和&amp;lt;math&amp;gt;\sum_{i\in I} r_i^d&amp;lt;\delta &amp;lt;/math&amp;gt; (在这里，我们使用inf&amp;amp;nbsp;Ø&amp;amp;nbsp;=&amp;amp;nbsp;∞ )的标准约定。&lt;br /&gt;
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===Hausdorff measurement豪斯多夫分形测量===&lt;br /&gt;
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The Hausdorff outer measure is different from the unbounded Hausdorf content in that rather than considering all possible coverings of ''S'', we see what happens when the sizes of the balls go to zero. This is  for &amp;lt;math&amp;gt;d \geq 0 &amp;lt;/math&amp;gt;, we define the ''d''-dimensional Hausdorff outer measure of ''S'' as&lt;br /&gt;
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The Hausdorff outer measure is different from the unbounded Hausdorf content in that rather than considering all possible coverings of S, we see what happens when the sizes of the balls go to zero. This is  for &amp;lt;math&amp;gt;d \geq 0 &amp;lt;/math&amp;gt;, we define the d-dimensional Hausdorff outer measure of S as&lt;br /&gt;
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豪斯多夫外测度不同于无界的豪斯多夫，因为我们不考虑 s 的所有可能，我们看到当球的大小为零时会发生什么。这是为了数学  &amp;lt;math&amp;gt;d \geq 0 &amp;lt;/math&amp;gt;，我们定义了  ''S''的 ''d''维豪斯多夫Hausdorff 外测度为&lt;br /&gt;
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:&amp;lt;math&amp;gt; \mathcal{H}^d(S):=\lim_{r \to 0} \inf\Bigl\{\sum_i r_i^d:\text{ there is a cover of } S\text{ by balls with radii } 0 &amp;lt; r_i &amp;lt; r\Bigr\}.&amp;lt;/math&amp;gt;&lt;br /&gt;
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&amp;lt;math&amp;gt; \mathcal{H}^d(S):=\lim_{r \to 0} \inf\Bigl\{\sum_i r_i^d:\text{ there is a cover of } S\text{ by balls with radii } 0 &amp;lt; r_i &amp;lt; r\Bigr\}.&amp;lt;/math&amp;gt;&lt;br /&gt;
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&amp;lt;math&amp;gt; \mathcal{H}^d(S):=\lim_{r \to 0} \inf\Bigl\{\sum_i r_i^d:\text{有一个面} S\text{ 球 } 0 &amp;lt; r_i &amp;lt; r\Bigr\}.&amp;lt;/math&amp;gt;&lt;br /&gt;
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===Hausdorff dimension豪斯多夫维数===&lt;br /&gt;
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The '''Hausdorff dimension''' of ''X'' is defined by&lt;br /&gt;
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The Hausdorff dimension of X is defined by&lt;br /&gt;
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X 的豪斯多夫维数定义为&lt;br /&gt;
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:&amp;lt;math&amp;gt;\dim_{\operatorname{H}}(X):=\inf\{d\ge 0: \mathcal{H}^d(X)=0\}.&amp;lt;/math&amp;gt;&lt;br /&gt;
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&amp;lt;math&amp;gt;\dim_{\operatorname{H}}(X):=\inf\{d\ge 0: \mathcal{H}^d(X)=0\}.&amp;lt;/math&amp;gt;&lt;br /&gt;
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Equivalently, dim&amp;lt;sub&amp;gt;H&amp;lt;/sub&amp;gt;(''X'') may be defined as the [[infimum]] of the set of ''d'' ∈ [0, ∞) such that the ''d''-dimensional [[Hausdorff measure]] of ''X'' is zero. This is the same as the supremum of the set of ''d''&amp;amp;nbsp;∈&amp;amp;nbsp;[0,&amp;amp;nbsp;∞) such that the ''d''-dimensional Hausdorff measure of ''X'' is infinite (except that when this latter set of numbers ''d'' is empty the Hausdorff dimension is zero).&lt;br /&gt;
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Equivalently, dim&amp;lt;sub&amp;gt;H&amp;lt;/sub&amp;gt;(X) may be defined as the infimum of the set of d ∈ [0, ∞) such that the d-dimensional Hausdorff measure of X is zero. This is the same as the supremum of the set of d&amp;amp;nbsp;∈&amp;amp;nbsp;[0,&amp;amp;nbsp;∞) such that the d-dimensional Hausdorff measure of X is infinite (except that when this latter set of numbers d is empty the Hausdorff dimension is zero).&lt;br /&gt;
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等价地，dim &amp;lt;sub&amp;gt;H&amp;lt;/sub&amp;gt;(''X'')可定义为 ''d'' ∈ [0, ∞) 集的下确界，使得''X'' 的''d''-维 [[豪斯多夫测度]] 为零。这与 ''d''&amp;amp;nbsp;∈&amp;amp;nbsp;[0,&amp;amp;nbsp;∞)的集合的上确界相同，因此''X''的 d 维豪斯多夫测度是无限的(除非后一个集合 ''d'' 是空的，豪斯多夫维数为零)。&lt;br /&gt;
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==Examples实例==&lt;br /&gt;
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[[Image:Sierpinski deep.svg|thumb|250px|Dimension of a further [[fractal]] example. The [[Sierpinski triangle]], an object with Hausdorff dimension of log(3)/log(2)≈1.58.&amp;lt;ref name=ClaytonSCTPLS96/&amp;gt;]]&lt;br /&gt;
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Dimension of a further [[fractal example. The Sierpinski triangle, an object with Hausdorff dimension of log(3)/log(2)≈1.58.]]&lt;br /&gt;
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[[Image:谢尔宾斯基三角形 deep.svg|thumb|250px|进一步的[[分形维数]]的例子，进一步的分形维数的例子是谢尔宾斯基三角形，它是一个豪斯多夫维数为log(3)/log(2)≈1.58.&amp;lt;ref name=ClaytonSCTPLS96/&amp;gt;的物体]]&lt;br /&gt;
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* [[Countable set]]s have Hausdorff dimension 0.&amp;lt;ref name=&amp;quot;schleicher&amp;quot;&amp;gt;{{cite journal |last1=Schleicher |first1=Dierk |title=Hausdorff Dimension, Its Properties, and Its Surprises |journal=The American Mathematical Monthly |date=June 2007 |volume=114 |issue=6 |pages=509–528 |doi=10.1080/00029890.2007.11920440 |language=en |issn=0002-9890|arxiv=math/0505099 }}&amp;lt;/ref&amp;gt;&lt;br /&gt;
*[[可数集]]拥有豪斯多夫维数0.&amp;lt;ref name=&amp;quot;schleicher&amp;quot;&amp;gt;{{cite journal |last1=Schleicher |first1=Dierk |title=豪斯多夫维数, Its Properties, and Its Surprises |journal=The American Mathematical Monthly美国数学期刊 |date=June 2007 |volume=114 |issue=6 |pages=509–528 |doi=10.1080/00029890.2007.11920440 |language=en |issn=0002-9890|arxiv=math/0505099 }}&amp;lt;/ref&amp;gt;&lt;br /&gt;
* The [[Euclidean space]] ℝ&amp;lt;sup&amp;gt;''n''&amp;lt;/sup&amp;gt; has Hausdorff dimension ''n'', and the circle '''S'''&amp;lt;sup&amp;gt;1&amp;lt;/sup&amp;gt; has Hausdorff dimension 1.&amp;lt;ref name=&amp;quot;schleicher&amp;quot; /&amp;gt;&lt;br /&gt;
*[[教育空间]] ℝ&amp;lt;sup&amp;gt;''n''&amp;lt;/sup&amp;gt; 有豪斯多夫维数 ''n''，循环'''S'''&amp;lt;sup&amp;gt;1&amp;lt;/sup&amp;gt; 拥有豪斯多夫维数1.&amp;lt;ref name=&amp;quot;schleicher&amp;quot; /&amp;gt;&lt;br /&gt;
* [[Fractal]]s often are spaces whose Hausdorff dimension strictly exceeds the [[topological dimension]].&amp;lt;ref name=&amp;quot;mandelbrot&amp;quot; /&amp;gt; For example, the [[Cantor set]], a zero-dimensional topological space, is a union of two copies of itself, each copy shrunk by a factor 1/3; hence, it can be shown that its Hausdorff dimension is ln(2)/ln(3)&amp;amp;nbsp;≈&amp;amp;nbsp;0.63.&amp;lt;ref&amp;gt;{{cite book | last=Falconer | first = Kenneth |title=Fractal Geometry: Mathematical Foundations and Applications | publisher=[[John Wiley and Sons]] | edition=2nd | year=2003}}&amp;lt;/ref&amp;gt; The [[Sierpinski triangle]] is a union of three copies of itself, each copy shrunk by a factor of&amp;amp;nbsp;1/2; this yields a Hausdorff dimension of ln(3)/ln(2)&amp;amp;nbsp;≈&amp;amp;nbsp;1.58.&amp;lt;ref name=CampbellAnnenberg15/&amp;gt; These Hausdorff dimensions are related to the &amp;quot;critical exponent&amp;quot; of the [[Master theorem (analysis of algorithms)|Master theorem]] for solving [[Recurrence relation|recurrence relations]] in the [[analysis of algorithms]].&lt;br /&gt;
*[[分形]]一般是那些豪斯多夫维数直接超过其拓扑维数的空间。例如[[康托尔集]]是一个o维拓扑空间，由两个自己复制而成，每一个复制品都是原来的三分之一，因此它的豪斯多夫维数是 ln(2)/ln(3)&amp;amp;nbsp;≈&amp;amp;nbsp;0.63。&amp;lt;ref&amp;gt;{{cite book | last=Falconer | first = Kenneth |title=Fractal Geometry: Mathematical Foundations and Applications | publisher=[[John Wiley and Sons]] | edition=2nd | year=2003}}&amp;lt;/ref&amp;gt;一个[[谢尔宾斯基三角]]是他自身三个复制的组合。每一个是原来的&amp;amp;nbsp;1/2，它的豪斯多夫维数ln(3)/ln(2)&amp;amp;nbsp;≈&amp;amp;nbsp;1.58。&amp;lt;ref name=CampbellAnnenberg15/&amp;gt;在递归算法中解决递归关系时，这些豪斯多夫维数与[[算法分析主定理]]的临界指标相联系。&lt;br /&gt;
* [[Space-filling curve]]s like the [[Peano curve]] have the same Hausdorff dimension as the space they fill.&lt;br /&gt;
*[[空间填充曲线]]拥有和他们填充空间同样的豪斯多夫维数，如[[皮亚诺曲线]]。&lt;br /&gt;
* The trajectory of [[Brownian motion]] in dimension 2 and above is conjectured to be Hausdorff dimension 2.&amp;lt;ref&amp;gt;{{cite book | last=Morters | first=Peres | title= Brownian Motion | publisher=[[Cambridge University Press]] | year=2010 }}&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
[[image:Great Britain Hausdorff.svg|thumb|250px|Estimating the Hausdorff dimension of the [[How Long Is the Coast of Britain? Statistical Self-Similarity and Fractional Dimension|coast of Great Britain]]]]&lt;br /&gt;
&lt;br /&gt;
coast of Great Britain]]&lt;br /&gt;
&lt;br /&gt;
[[大不列颠海岸&lt;br /&gt;
&lt;br /&gt;
* 刘易斯·弗赖伊·理查森[[Lewis Fry Richardson]] has performed detailed experiments to measure the approximate Hausdorff dimension for various coastlines. His results have varied from 1.02 for the coastline of [[South Africa]] to 1.25 for the west coast of [[Great Britain]].&amp;lt;ref name=&amp;quot;mandelbrot&amp;quot; /&amp;gt;&lt;br /&gt;
*刘易斯·弗赖伊·理查森（Lewis Fry Richardson）已经通过豪斯多夫维数去测量了很多海岸线。它的结果涵盖从1.02的南非海岸线到1.25的大英帝国西海岸模型。]]&lt;br /&gt;
&lt;br /&gt;
==Properties of Hausdorff dimension豪斯多夫维数特性==&lt;br /&gt;
&lt;br /&gt;
{{refimprove section|date=March 2015}}&lt;br /&gt;
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&lt;br /&gt;
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=== Hausdorff dimension and inductive dimension 豪斯多夫维数和归纳维数===&lt;br /&gt;
&lt;br /&gt;
Let ''X'' be an arbitrary [[Separable space|separable]] metric space. There is a [[topology|topological]] notion of [[inductive dimension]] for ''X'' which is defined recursively. It is always an integer (or +∞) and is denoted dim&amp;lt;sub&amp;gt;ind&amp;lt;/sub&amp;gt;(''X'').&lt;br /&gt;
&lt;br /&gt;
Let X be an arbitrary separable metric space. There is a topological notion of inductive dimension for X which is defined recursively. It is always an integer (or +∞) and is denoted dim&amp;lt;sub&amp;gt;ind&amp;lt;/sub&amp;gt;(X).&lt;br /&gt;
&lt;br /&gt;
设''X'' 是[[任意可分度量空间]]。对于''X'' 有一个递归定义的归纳维数拓扑概念。它总是一个整数(或 + ∞) ，并且表示dim&amp;lt;sub&amp;gt;ind&amp;lt;/sub&amp;gt;(''X'')。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
'''Theorem'''. Suppose ''X'' is non-empty. Then &lt;br /&gt;
&lt;br /&gt;
Theorem. Suppose X is non-empty. Then &lt;br /&gt;
&lt;br /&gt;
'''定理'''：假设''X'' 是非空的。那么&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt; \dim_{\mathrm{Haus}}(X) \geq \dim_{\operatorname{ind}}(X). &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \dim_{\mathrm{Haus}}(X) \geq \dim_{\operatorname{ind}}(X). &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Moreover,&lt;br /&gt;
&lt;br /&gt;
Moreover,&lt;br /&gt;
&lt;br /&gt;
此外,&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \inf_Y \dim_{\operatorname{Haus}}(Y) =\dim_{\operatorname{ind}}(X), &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \inf_Y \dim_{\operatorname{Haus}}(Y) =\dim_{\operatorname{ind}}(X), &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
where ''Y'' ranges over metric spaces [[homeomorphic]] to ''X''. In other words, ''X'' and ''Y'' have the same underlying set of points and the metric ''d''&amp;lt;sub&amp;gt;''Y''&amp;lt;/sub&amp;gt; of ''Y'' is topologically equivalent to ''d''&amp;lt;sub&amp;gt;''X''&amp;lt;/sub&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
where Y ranges over metric spaces homeomorphic to X. In other words, X and Y have the same underlying set of points and the metric d&amp;lt;sub&amp;gt;Y&amp;lt;/sub&amp;gt; of Y is topologically equivalent to d&amp;lt;sub&amp;gt;X&amp;lt;/sub&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
其中''Y''是度量空间同胚到 ''X''的范围。换句话说， ''X''和 ''Y''具有相同的基本点集，''Y''的度规''d''&amp;lt;sub&amp;gt;''Y''&amp;lt;/sub&amp;gt; 的子拓扑等价于''d''&amp;lt;sub&amp;gt;''X''&amp;lt;/sub&amp;gt;。&lt;br /&gt;
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&lt;br /&gt;
&lt;br /&gt;
These results were originally established by [[Edward Szpilrajn]] (1907–1976), e.g., see Hurewicz and Wallman, Chapter VII.{{full citation needed|date=March 2015}}&lt;br /&gt;
&lt;br /&gt;
These results were originally established by Edward Szpilrajn (1907–1976), e.g., see Hurewicz and Wallman, Chapter VII.&lt;br /&gt;
&lt;br /&gt;
这些结果最初是由 [[Edward Szpilrajn]] (1907–1976)建立的,  参见 Hurewicz and Wallman, Chapter VII.{{full citation needed|date=March 2015}}第七章。&lt;br /&gt;
&lt;br /&gt;
=== Hausdorff dimension and Minkowski dimension 豪斯多夫维数和闵可夫斯基维度===&lt;br /&gt;
&lt;br /&gt;
The [[Minkowski dimension]] is similar to, and at least as large as, the Hausdorff dimension, and they are equal in many situations. However, the set of [[rational number|rational]] points in [0, 1] has Hausdorff dimension zero and Minkowski dimension one. There are also compact sets for which the Minkowski dimension is strictly larger than the Hausdorff dimension.&lt;br /&gt;
&lt;br /&gt;
The Minkowski dimension is similar to, and at least as large as, the Hausdorff dimension, and they are equal in many situations. However, the set of rational points in [0, 1] has Hausdorff dimension zero and Minkowski dimension one. There are also compact sets for which the Minkowski dimension is strictly larger than the Hausdorff dimension.&lt;br /&gt;
&lt;br /&gt;
[[闵可夫斯基维数]]与豪斯多夫维数相似，至少和它一样大，而且在许多情况下是相等的。然而，[0,1]中有理点集的豪斯多夫维数为0，闵可夫斯基维数为1。还有一些紧集的闵可夫斯基维数绝对大于豪斯多夫维数。&lt;br /&gt;
&lt;br /&gt;
=== Hausdorff dimensions and Frostman measures 豪斯多夫维度和弗洛斯曼测度===&lt;br /&gt;
&lt;br /&gt;
If there is a [[measure (mathematics)|measure]] μ defined on [[Borel measure|Borel]] subsets of a metric space ''X'' such that ''μ''(''X'') &amp;gt; 0 and ''μ''(''B''(''x'', ''r'')) ≤ ''r&amp;lt;sup&amp;gt;s&amp;lt;/sup&amp;gt;'' holds for some constant ''s'' &amp;gt; 0 and for every ball ''B''(''x'', ''r'') in ''X'', then dim&amp;lt;sub&amp;gt;Haus&amp;lt;/sub&amp;gt;(''X'') ≥ ''s''. A partial converse is provided by [[Frostman's lemma]].{{citation needed|date=March 2015}}&amp;lt;ref&amp;gt;This Wikipedia article also discusses further useful characterizations of the Hausdorff dimension.{{clarify|date=March 2015}}&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
If there is a measure μ defined on Borel subsets of a metric space X such that μ(X) &amp;gt; 0 and μ(B(x, r)) ≤ r&amp;lt;sup&amp;gt;s&amp;lt;/sup&amp;gt; holds for some constant s &amp;gt; 0 and for every ball B(x, r) in X, then dim&amp;lt;sub&amp;gt;Haus&amp;lt;/sub&amp;gt;(X) ≥ s. A partial converse is provided by Frostman's lemma.&lt;br /&gt;
&lt;br /&gt;
如果在度量空间 ''X'' 的 Borel 子集上定义一个测度 μ，使得''μ''(''X'') &amp;gt; 0 和''μ''(''B''(''x'', ''r'')) ≤ ''r&amp;lt;sup&amp;gt;s&amp;lt;/sup&amp;gt;''，对于某个常数 ''s'' &amp;gt; 0  和 ''X'' 中的每个球 ''B''(''x'', ''r'') 成立，则 dim&amp;lt;sub&amp;gt;Haus&amp;lt;/sub&amp;gt;(''X'') ≥ ''s'' 。 部分逆向转换由弗洛斯曼引理定义。&lt;br /&gt;
&lt;br /&gt;
=== Behaviour under unions and products ===&lt;br /&gt;
&lt;br /&gt;
If &amp;lt;math&amp;gt;X=\bigcup_{i\in I}X_i&amp;lt;/math&amp;gt; is a finite or countable union, then&lt;br /&gt;
&lt;br /&gt;
If &amp;lt;math&amp;gt;X=\bigcup_{i\in I}X_i&amp;lt;/math&amp;gt; is a finite or countable union, then&lt;br /&gt;
&lt;br /&gt;
如果 &amp;lt;math&amp;gt;X=\bigcup_{i\in I}X_i&amp;lt;/math&amp;gt; 是一个有限或可数的联合，则&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \dim_{\operatorname{Haus}}(X) =\sup_{i\in I} \dim_{\operatorname{Haus}}(X_i).&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \dim_{\operatorname{Haus}}(X) =\sup_{i\in I} \dim_{\operatorname{Haus}}(X_i).&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
This can be verified directly from the definition.&lt;br /&gt;
&lt;br /&gt;
This can be verified directly from the definition.&lt;br /&gt;
&lt;br /&gt;
这可以直接从定义得到验证。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
If ''X'' and ''Y'' are non-empty metric spaces, then the Hausdorff dimension of their product satisfies&amp;lt;ref&amp;gt;{{cite journal |author=Marstrand, J. M. |title=The dimension of Cartesian product sets |journal=Proc. Cambridge Philos. Soc. |volume=50 |issue=3 |pages=198–202 |year=1954 |doi=10.1017/S0305004100029236 |bibcode = 1954PCPS...50..198M }}&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
If X and Y are non-empty metric spaces, then the Hausdorff dimension of their product satisfies&lt;br /&gt;
&lt;br /&gt;
如果 ''X'' 和''Y''是非空度量空间，那么它们乘积的豪斯多夫维数满足&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt; \dim_{\operatorname{Haus}}(X\times Y)\ge \dim_{\operatorname{Haus}}(X)+ \dim_{\operatorname{Haus}}(Y).&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \dim_{\operatorname{Haus}}(X\times Y)\ge \dim_{\operatorname{Haus}}(X)+ \dim_{\operatorname{Haus}}(Y).&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
This inequality can be strict. It is possible to find two sets of dimension 0 whose product has dimension 1.&amp;lt;ref&amp;gt;{{cite book  | last = Falconer  | first = Kenneth J.  | title = Fractal geometry. Mathematical foundations and applications  | publisher = John Wiley &amp;amp; Sons, Inc., Hoboken, New Jersey  | year = 2003  | doi =   | isbn = }}&amp;lt;/ref&amp;gt; In the opposite direction, it is known that when ''X'' and ''Y'' are Borel subsets of '''R'''&amp;lt;sup&amp;gt;''n''&amp;lt;/sup&amp;gt;, the Hausdorff dimension of ''X'' × ''Y'' is bounded from above by the Hausdorff dimension of ''X'' plus the [[packing dimension|upper packing dimension]] of ''Y''. These facts are discussed in Mattila (1995).&lt;br /&gt;
&lt;br /&gt;
This inequality can be strict. It is possible to find two sets of dimension 0 whose product has dimension 1. In the opposite direction, it is known that when X and Y are Borel subsets of R&amp;lt;sup&amp;gt;n&amp;lt;/sup&amp;gt;, the Hausdorff dimension of X × Y is bounded from above by the Hausdorff dimension of X plus the upper packing dimension of Y. These facts are discussed in Mattila (1995).&lt;br /&gt;
&lt;br /&gt;
这种不平等可以是绝对的。有可能找到两个维数为0的集合，其乘积的维数为1。相反，我们知道当''X''和''Y''是 '''R'''&amp;lt;sup&amp;gt;''n''&amp;lt;/sup&amp;gt;的 Borel 子集时， ''X'' × ''Y''的豪斯多夫维数从上面以 ''X''的豪斯多夫维数加上 ''Y''的填充维数为界。Mattila (1995)曾就这些情况进行了讨论。&lt;br /&gt;
&lt;br /&gt;
==Self-similar sets自相似集合==&lt;br /&gt;
&lt;br /&gt;
{{refimprove section|date=March 2015}}&lt;br /&gt;
&lt;br /&gt;
Many sets defined by a self-similarity condition have dimensions which can be determined explicitly. Roughly, a set ''E'' is self-similar if it is the fixed point of a set-valued transformation ψ, that is ψ(''E'') = ''E'', although the exact definition is given below.&lt;br /&gt;
&lt;br /&gt;
Many sets defined by a self-similarity condition have dimensions which can be determined explicitly. Roughly, a set E is self-similar if it is the fixed point of a set-valued transformation ψ, that is ψ(E) = E, although the exact definition is given below.&lt;br /&gt;
&lt;br /&gt;
许多由自相似条件定义的集合具有可以显式确定的维数。粗略地说，集合''E'' 是自相似的，如果它是集值ψ变换的不动点，即ψ(''E'') = ''E''，尽管下面给出了确切的定义。&lt;br /&gt;
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&lt;br /&gt;
&lt;br /&gt;
&amp;lt;blockquote&amp;gt;'''Theorem'''. Suppose&lt;br /&gt;
&lt;br /&gt;
&amp;lt;blockquote&amp;gt;Theorem. Suppose&lt;br /&gt;
&lt;br /&gt;
&amp;lt;blockquote&amp;gt;'''定理'''：假设&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt; \psi_i: \mathbf{R}^n \rightarrow \mathbf{R}^n, \quad i=1, \ldots , m &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \psi_i: \mathbf{R}^n \rightarrow \mathbf{R}^n, \quad i=1, \ldots , m &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
are [[Contraction mapping|contractive]] mappings on '''R'''&amp;lt;sup&amp;gt;''n''&amp;lt;/sup&amp;gt; with contraction constant ''r&amp;lt;sub&amp;gt;j&amp;lt;/sub&amp;gt;'' &amp;lt; 1. Then there is a unique ''non-empty'' compact set ''A'' such that&lt;br /&gt;
&lt;br /&gt;
are contractive mappings on R&amp;lt;sup&amp;gt;n&amp;lt;/sup&amp;gt; with contraction constant r&amp;lt;sub&amp;gt;j&amp;lt;/sub&amp;gt; &amp;lt; 1. Then there is a unique non-empty compact set A such that&lt;br /&gt;
&lt;br /&gt;
是'''R'''&amp;lt;sup&amp;gt;''n''&amp;lt;/sup&amp;gt;上的压缩常数''r&amp;lt;sub&amp;gt;j&amp;lt;/sub&amp;gt;'&amp;lt; 1的压缩映射。然后有一个唯一的非空紧集A &lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt; A = \bigcup_{i=1}^m \psi_i (A). &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; A = \bigcup_{i=1}^m \psi_i (A). &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&amp;lt;/blockquote&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;/blockquote&amp;gt;&lt;br /&gt;
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&lt;br /&gt;
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&lt;br /&gt;
The theorem follows from [[Stefan Banach]]'s [[Contractive mapping theorem|contractive mapping fixed point theorem]] applied to the complete metric space of non-empty compact subsets of '''R'''&amp;lt;sup&amp;gt;''n''&amp;lt;/sup&amp;gt; with the [[Hausdorff distance]].&amp;lt;ref&amp;gt;{{cite book |author=Falconer, K. J. |title=The Geometry of Fractal Sets |publisher=Cambridge University Press |location=Cambridge, UK |year=1985 |isbn=0-521-25694-1 |chapter=Theorem 8.3}}&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
The theorem follows from Stefan Banach's contractive mapping fixed point theorem applied to the complete metric space of non-empty compact subsets of R&amp;lt;sup&amp;gt;n&amp;lt;/sup&amp;gt; with the Hausdorff distance.&lt;br /&gt;
&lt;br /&gt;
这个定理来源于 Stefan Banach 的压缩映射不动点定理，该定理应用于 '''R'''&amp;lt;sup&amp;gt;''n''&amp;lt;/sup&amp;gt; 的非空紧子集的完备空间豪斯多夫距离。&lt;br /&gt;
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&lt;br /&gt;
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===The open set condition开集条件===&lt;br /&gt;
&lt;br /&gt;
To determine the dimension of the self-similar set ''A'' (in certain cases), we need a technical condition called the ''open set condition'' (OSC) on the sequence of contractions ψ&amp;lt;sub&amp;gt;''i''&amp;lt;/sub&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
To determine the dimension of the self-similar set A (in certain cases), we need a technical condition called the open set condition (OSC) on the sequence of contractions ψ&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
为了确定自相似集''A'' 的维数(在某些情况下) ，我们需要一个称为''开集条件''(OSC)的技术条件ψ&amp;lt;sub&amp;gt;''i''&amp;lt;/sub&amp;gt;。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
There is a relatively compact open set ''V'' such that&lt;br /&gt;
&lt;br /&gt;
There is a relatively compact open set V such that&lt;br /&gt;
&lt;br /&gt;
有一个相对紧的开集''V''&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt; \bigcup_{i=1}^m\psi_i (V) \subseteq V, &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \bigcup_{i=1}^m\psi_i (V) \subseteq V, &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
where the sets in union on the left are pairwise [[disjoint sets|disjoint]].&lt;br /&gt;
&lt;br /&gt;
where the sets in union on the left are pairwise disjoint.&lt;br /&gt;
&lt;br /&gt;
左边的集合是成对不相交的。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The open set condition is a separation condition that ensures the images ψ&amp;lt;sub&amp;gt;''i''&amp;lt;/sub&amp;gt;(''V'') do not overlap &amp;quot;too much&amp;quot;.&lt;br /&gt;
&lt;br /&gt;
The open set condition is a separation condition that ensures the images ψ&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;(V) do not overlap &amp;quot;too much&amp;quot;.&lt;br /&gt;
&lt;br /&gt;
开集条件是保证图像子ψ&amp;lt;sub&amp;gt;''i''&amp;lt;/sub&amp;gt;(''V'') 不重叠“太多”的分离条件。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
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'''Theorem'''. Suppose the open set condition holds and each ψ&amp;lt;sub&amp;gt;''i''&amp;lt;/sub&amp;gt; is a similitude, that is a composition of an [[isometry]] and a [[dilation (metric space)|dilation]] around some point. Then the unique fixed point of ψ is a set whose Hausdorff dimension is ''s'' where ''s'' is the unique solution of&amp;lt;ref&amp;gt;{{cite journal | last=Hutchinson | first=John E. | title=Fractals and self similarity | journal=Indiana Univ. Math. J. | volume=30 | year=1981 | pages=713–747 | doi=10.1512/iumj.1981.30.30055 | issue=5 | doi-access=free }}&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
Theorem. Suppose the open set condition holds and each ψ&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt; is a similitude, that is a composition of an isometry and a dilation around some point. Then the unique fixed point of ψ is a set whose Hausdorff dimension is s where s is the unique solution of&lt;br /&gt;
&lt;br /&gt;
'''定理'''假设开集条件成立，并且每个ψ&amp;lt;sub&amp;gt;''i''&amp;lt;/sub&amp;gt; 是一个相似量，这是一个等距和围绕某一点的膨胀的合成。那么唯一的不动点是一个集合，它的豪斯多夫维数是 ''s'' ，其中  ''s'' 是 ''s'' &amp;lt;ref&amp;gt;{{cite journal | last=Hutchinson | first=John E. | title=Fractals and self similarity | journal=Indiana Univ. Math. J. | volume=30 | year=1981 | pages=713–747 | doi=10.1512/iumj.1981.30.30055 | issue=5 | doi-access=free }}&amp;lt;/ref&amp;gt;的唯一解&lt;br /&gt;
&lt;br /&gt;
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:&amp;lt;math&amp;gt; \sum_{i=1}^m r_i^s = 1. &amp;lt;/math&amp;gt;&lt;br /&gt;
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&amp;lt;math&amp;gt; \sum_{i=1}^m r_i^s = 1. &amp;lt;/math&amp;gt;&lt;br /&gt;
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The contraction coefficient of a similitude is the magnitude of the dilation.&lt;br /&gt;
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The contraction coefficient of a similitude is the magnitude of the dilation.&lt;br /&gt;
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相似物的收缩系数就是膨胀的大小。&lt;br /&gt;
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We can use this theorem to compute the Hausdorff dimension of the Sierpinski triangle (or sometimes called Sierpinski gasket). Consider three [[non-collinear points]] ''a''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;, ''a''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;, ''a''&amp;lt;sub&amp;gt;3&amp;lt;/sub&amp;gt; in the plane '''R'''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; and let ψ&amp;lt;sub&amp;gt;''i''&amp;lt;/sub&amp;gt; be the dilation of ratio 1/2 around ''a&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;''. The unique non-empty fixed point of the corresponding mapping ψ is a Sierpinski gasket and the dimension ''s'' is the unique solution of&lt;br /&gt;
&lt;br /&gt;
We can use this theorem to compute the Hausdorff dimension of the Sierpinski triangle (or sometimes called Sierpinski gasket). Consider three non-collinear points a&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;, a&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;, a&amp;lt;sub&amp;gt;3&amp;lt;/sub&amp;gt; in the plane R&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; and let ψ&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt; be the dilation of ratio 1/2 around a&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;. The unique non-empty fixed point of the corresponding mapping ψ is a Sierpinski gasket and the dimension s is the unique solution of&lt;br /&gt;
&lt;br /&gt;
我们可以使用这个定理来计算谢尔宾斯基三角形的豪斯多夫维数(或者有时候叫做谢尔宾斯基垫圈)。考虑R&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; 平面上的三个非共线点，''a''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;，''a''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;，''a''&amp;lt;sub&amp;gt;3&amp;lt;/sub&amp;gt;，让ψ&amp;lt;sub&amp;gt;''i''&amp;lt;/sub&amp;gt;是围绕着''a&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;''膨胀比率的1/2。对应映射的唯一非空不动点是一个谢尔宾斯基垫圈，其维数''s''是对应映射的唯一解&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt; \left(\frac{1}{2}\right)^s+\left(\frac{1}{2}\right)^s+\left(\frac{1}{2}\right)^s = 3 \left(\frac{1}{2}\right)^s =1. &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \left(\frac{1}{2}\right)^s+\left(\frac{1}{2}\right)^s+\left(\frac{1}{2}\right)^s = 3 \left(\frac{1}{2}\right)^s =1. &amp;lt;/math&amp;gt;&lt;br /&gt;
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Taking [[natural logarithm]]s of both sides of the above equation, we can solve for ''s'', that is: ''s'' = ln(3)/ln(2).  The Sierpinski gasket is self-similar and satisfies the OSC. In general a set ''E'' which is a fixed point of a mapping&lt;br /&gt;
&lt;br /&gt;
Taking natural logarithms of both sides of the above equation, we can solve for s, that is: s = ln(3)/ln(2).  The Sierpinski gasket is self-similar and satisfies the OSC. In general a set E which is a fixed point of a mapping&lt;br /&gt;
&lt;br /&gt;
取上述方程两边的自然对数，我们可以求出 ''s''，即: ''s'' = ln(3)/ln(2)。该密封垫具有自相似性，满足 OSC 要求。一般来说，集合 ''E''是一个映射的不动点&lt;br /&gt;
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: &amp;lt;math&amp;gt; A \mapsto \psi(A) = \bigcup_{i=1}^m \psi_i(A) &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt; A \mapsto \psi(A) = \bigcup_{i=1}^m \psi_i(A) &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
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is self-similar if and only if the intersections&lt;br /&gt;
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is self-similar if and only if the intersections&lt;br /&gt;
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是自相似的，当且仅当&lt;br /&gt;
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:&amp;lt;math&amp;gt; H^s\left(\psi_i(E) \cap \psi_j(E)\right) =0, &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; H^s\left(\psi_i(E) \cap \psi_j(E)\right) =0, &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
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where ''s'' is the Hausdorff dimension of ''E'' and ''H&amp;lt;sup&amp;gt;s&amp;lt;/sup&amp;gt;'' denotes [[Hausdorff measure]]. This is clear in the case of the Sierpinski gasket (the intersections are just points), but is also true more generally:&lt;br /&gt;
&lt;br /&gt;
where s is the Hausdorff dimension of E and H&amp;lt;sup&amp;gt;s&amp;lt;/sup&amp;gt; denotes Hausdorff measure. This is clear in the case of the Sierpinski gasket (the intersections are just points), but is also true more generally:&lt;br /&gt;
&lt;br /&gt;
其中 ''s''是''E''的豪斯多夫维数， ''E'' and ''H&amp;lt;sup&amp;gt;s&amp;lt;/sup&amp;gt;'' 表示 豪斯多夫测度。对于谢尔宾斯基垫圈(交叉点就是点)来说，这一点很明显，但更普遍的情况是:&lt;br /&gt;
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'''Theorem'''. Under the same conditions as the previous theorem, the unique fixed point of ψ is self-similar.&lt;br /&gt;
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Theorem. Under the same conditions as the previous theorem, the unique fixed point of ψ is self-similar.&lt;br /&gt;
&lt;br /&gt;
'''定理'''：在与前一定理相同的条件下，其唯一不动点是自相似的。&lt;br /&gt;
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==See also参阅==&lt;br /&gt;
&lt;br /&gt;
* [[List of fractals by Hausdorff dimension豪斯多夫分形维数列表]] Examples of deterministic fractals, random and natural fractals.确定性分形与随机和自然分形的示例。&lt;br /&gt;
&lt;br /&gt;
* [[Assouad dimension  Assouad维数]], another variation of fractal dimension that, like Hausdorff dimension, is defined using coverings by balls其他被球覆盖方式定义的分形维数，例如豪斯多夫维数。&lt;br /&gt;
&lt;br /&gt;
* [[Intrinsic dimension固有维数]]&lt;br /&gt;
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* [[Packing dimension填充维数]]&lt;br /&gt;
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* [[Fractal dimension分形维数]]&lt;br /&gt;
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==References参考文献==&lt;br /&gt;
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{{reflist}}&lt;br /&gt;
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==Further reading拓展阅读==&lt;br /&gt;
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* {{cite book |last1=Dodson |first1=M. Maurice |title=Fractal Geometry and Applications: A Jubilee of Benoît Mandelbrot |volume=72 |issue=1 |pages=305–347 |last2=Kristensen |first2=Simon |chapter=Hausdorff Dimension and Diophantine Approximation |date=June 12, 2003 |arxiv=math/0305399 |bibcode = 2003math......5399D |doi=10.1090/pspum/072.1/2112110|series=Proceedings of Symposia in Pure Mathematics |isbn=9780821836378 }}&lt;br /&gt;
&lt;br /&gt;
* {{cite book |last1=Hurewicz |first1=Witold |authorlink1=Witold Hurewicz |last2=Wallman |first2=Henry |authorlink2=Henry Wallman |title=Dimension Theory |url=https://archive.org/details/in.ernet.dli.2015.84609 |publisher=Princeton University Press |year=1948 }}&lt;br /&gt;
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* {{cite journal |author作者=E. Szpilrajn |authorlink=Edward Marczewski |title=La dimension et la mesure |journal=Fundamenta Mathematicae |volume=28 |pages=81–9 |year=1937 }}&lt;br /&gt;
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* {{cite journal&lt;br /&gt;
&lt;br /&gt;
 | last1=Marstrand&lt;br /&gt;
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 | last1=Marstrand&lt;br /&gt;
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 | last1=马斯特兰德&lt;br /&gt;
&lt;br /&gt;
 | first1=J. M. | title=The dimension of cartesian product sets | year=1954 | journal=Proc. Cambridge Philos. Soc.&lt;br /&gt;
&lt;br /&gt;
 | first1=J. M. | title=The dimension of cartesian product sets | year=1954 | journal=Proc. Cambridge Philos. Soc.&lt;br /&gt;
&lt;br /&gt;
 | first1= J. M. | title=笛卡儿积集的维数 | 1954年 |  journal=Proc. Cambridge Philos. Soc.&lt;br /&gt;
&lt;br /&gt;
 | volume=50&lt;br /&gt;
&lt;br /&gt;
 | volume=50&lt;br /&gt;
&lt;br /&gt;
 | 第50卷&lt;br /&gt;
&lt;br /&gt;
 | issue=3&lt;br /&gt;
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 | issue=3&lt;br /&gt;
&lt;br /&gt;
 | 第三期&lt;br /&gt;
&lt;br /&gt;
 | pages=198–202&lt;br /&gt;
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 | pages=198–202&lt;br /&gt;
&lt;br /&gt;
 | 第198-202页&lt;br /&gt;
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 | doi=10.1017/S0305004100029236|bibcode = 1954PCPS...50..198M }}&lt;br /&gt;
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 | doi=10.1017/S0305004100029236|bibcode = 1954PCPS...50..198M }}&lt;br /&gt;
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10.1017 / S0305004100029236 | bibcode 1954PCPS... 50. . 198 m }&lt;br /&gt;
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* {{Cite book&lt;br /&gt;
&lt;br /&gt;
 | last1=Mattila&lt;br /&gt;
&lt;br /&gt;
 | last1=Mattila&lt;br /&gt;
&lt;br /&gt;
 | last1=Mattila&lt;br /&gt;
&lt;br /&gt;
 | first1=Pertti | author1-link=Pertti Mattila| title=Geometry of sets and measures in Euclidean spaces | publisher=[[Cambridge University Press]]&lt;br /&gt;
&lt;br /&gt;
 | first1=Pertti | author1-link=Pertti Mattila| title=Geometry of sets and measures in Euclidean spaces | publisher=Cambridge University Press&lt;br /&gt;
&lt;br /&gt;
| first1 Pertti | author1-link Pertti Mattila | title 欧几里德空间中集合和度量的几何 | 出版商剑桥大学出版社&lt;br /&gt;
&lt;br /&gt;
 | isbn=978-0-521-65595-8 | year=1995}}&lt;br /&gt;
&lt;br /&gt;
 | isbn=978-0-521-65595-8 | year=1995}}&lt;br /&gt;
&lt;br /&gt;
| isbn 978-0-521-65595-8 | year 1995}&lt;br /&gt;
&lt;br /&gt;
* {{cite journal |author=A. S. Besicovitch |authorlink=A. S. Besicovitch |title=On Linear Sets of Points of Fractional Dimensions |journal=[[Mathematische Annalen]] |volume=101 |year=1929 | doi=10.1007/BF01454831| issue=1 |pages= 161–193}}&lt;br /&gt;
&lt;br /&gt;
* {{cite journal |author1=A. S. Besicovitch |authorlink1=A. S. Besicovitch |author2=H. D. Ursell |authorlink2=H. D. Ursell |title=Sets of Fractional Dimensions |journal=Journal of the London Mathematical Society |volume=12 |year=1937 | issue=1 | doi=10.1112/jlms/s1-12.45.18  | pages=18–25 }}&amp;lt;br/&amp;gt;Several selections from this volume are reprinted in {{cite book |author=Edgar, Gerald A. |title=Classics on fractals |publisher=Addison-Wesley |location=Boston |year=1993 |isbn=0-201-58701-7}} See chapters 9,10,11&lt;br /&gt;
&lt;br /&gt;
* {{cite journal |author=F. Hausdorff |authorlink=F. Hausdorff |title=Dimension und äußeres Maß |journal=Mathematische Annalen |volume=79 |issue=1–2 |pages=157–179 |date=March 1919 |doi=10.1007/BF01457179|hdl=10338.dmlcz/100363 |url=http://dml.cz/bitstream/handle/10338.dmlcz/100363/CzechMathJ_09-1959-3_5.pdf }}&lt;br /&gt;
&lt;br /&gt;
* {{cite journal | last=Hutchinson | first=John E. | title=Fractals and self similarity | journal=Indiana Univ. Math. J. | volume=30 | year=1981 | pages=713–747 | doi=10.1512/iumj.1981.30.30055 | issue=5 | doi-access=free }}&lt;br /&gt;
&lt;br /&gt;
*{{cite book | last=Falconer | first = Kenneth |title=Fractal Geometry: Mathematical Foundations and Applications | publisher=[[John Wiley and Sons]] | edition=2nd | year=2003}}&lt;br /&gt;
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==External links外部链接==&lt;br /&gt;
&lt;br /&gt;
* [https://www.encyclopediaofmath.org/index.php/Hausdorff_dimension Hausdorff dimension] 在 [https://www.encyclopediaofmath.org/ Encyclopedia of Mathematics]&lt;br /&gt;
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* [https://www.encyclopediaofmath.org/index.php/Hausdorff_measure Hausdorff measure] 在 [https://www.encyclopediaofmath.org/ Encyclopedia of Mathematics]&lt;br /&gt;
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{{DEFAULTSORT:Hausdorff Dimension豪斯多夫维数}}&lt;br /&gt;
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[[Category分类:Fractals分形]]&lt;br /&gt;
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[[Category分类:Metric geometry度量几何]]&lt;br /&gt;
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[[Category分类:Dimension theory维度理论]]&lt;br /&gt;
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&amp;lt;small&amp;gt;This page was moved from [[wikipedia:en:Hausdorff dimension]]. Its edit history can be viewed at [[分形维数/edithistory]]&amp;lt;/small&amp;gt;&amp;lt;/noinclude&amp;gt;&lt;br /&gt;
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[[Category:待整理页面]]&lt;/div&gt;</summary>
		<author><name>Ruili</name></author>
	</entry>
	<entry>
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		<title>分形维数</title>
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		<updated>2020-10-27T16:16:16Z</updated>

		<summary type="html">&lt;p&gt;Ruili：&lt;/p&gt;
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&lt;div&gt;此词条暂由彩云小译翻译，未经人工整理和审校，带来阅读不便，请见谅。&lt;br /&gt;
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{{short description|Invariant}}&lt;br /&gt;
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Example of non-integer dimensions. The first four [[iteration]]s of the [[Koch snowflake|Koch curve]], where after each iteration, all original line segments are replaced with four, each a self-similar copy that is 1/3 the length of the original. One formalism of the Hausdorff dimension uses this scale factor (3) and the number of self-similar objects (4) to calculate the dimension, D, after the first iteration to be D = (log N)/(log S) = (log 4)/(log 3) ≈ 1.26.&amp;lt;ref name=CampbellAnnenberg15&amp;gt;MacGregor Campbell, 2013, &amp;quot;5.6 Scaling and the Hausdorff Dimension,&amp;quot; at ''Annenberg Learner:MATHematics illuminated'', see [http://www.learner.org/courses/mathilluminated/units/5/textbook/06.php], accessed 5 March 2015.&amp;lt;/ref&amp;gt; That is, while the Hausdorff dimension of a single [[point (geometry)|point]] is zero, of a [[line segment]] is 1, of a [[square]] is 2, and of a [[cube]] is 3, for [[fractal]]s such as this, the object can have a non-integer dimension.&lt;br /&gt;
&lt;br /&gt;
Example of non-integer dimensions. The first four iterations of the Koch curve, where after each iteration, all original line segments are replaced with four, each a self-similar copy that is 1/3 the length of the original. One formalism of the Hausdorff dimension uses this scale factor (3) and the number of self-similar objects (4) to calculate the dimension, D, after the first iteration to be D = (log N)/(log S) = (log 4)/(log 3) ≈ 1.26. That is, while the Hausdorff dimension of a single point is zero, of a line segment is 1, of a square is 2, and of a cube is 3, for fractals such as this, the object can have a non-integer dimension.&lt;br /&gt;
&lt;br /&gt;
非整数维度示例：前四个[[Koch 曲线]]的迭代，在每次迭代后，所有原始线段都被替换为四个，每个自相似的复制是原始线段长度的1 / 3。豪斯多夫维数的一个建模是使用比例因子(3)和自相似对象的数量(4)来计算维度 D，在第一次迭代后为 D = (log N)/(log S) = (log 4)/(log 3) ≈ 1.26.&amp;lt;ref name=CampbellAnnenberg15&amp;gt;。MacGregor Campbell, 2013, &amp;quot;5.6 Scaling and the Hausdorff Dimension,&amp;quot; 在 ''Annenberg Learner:MATHematics illuminated'', 参见 [http://www.learner.org/courses/mathilluminated/units/5/textbook/06.php], accessed 5 March 2015.&amp;lt;/ref&amp;gt; 也就是说，单点的豪斯多夫维数为零，线段为1，正方形为2，立方体为3时，但对于分形，对象可以有一个非整数维度。&lt;br /&gt;
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In [[mathematics]], '''Hausdorff dimension''' is a measure of ''roughness'', or more specifically, [[fractal dimension]], that was first introduced in 1918 by [[mathematician]] [[Felix Hausdorff]].&amp;lt;ref&amp;gt;{{Cite journal |arxiv = 1101.1444|doi = 10.1214/11-STS370|title = Estimators of Fractal Dimension: Assessing the Roughness of Time Series and Spatial Data|journal = Statistical Science|volume = 27|issue = 2|pages = 247–277|year = 2012|last1 = Gneiting|first1 = Tilmann|last2 = Ševčíková|first2 = Hana|last3 = Percival|first3 = Donald B.}}&amp;lt;/ref&amp;gt; For instance, the Hausdorff dimension of a single [[point (geometry)|point]] is zero, of a [[line segment]] is 1, of a [[square]] is 2, and of a [[cube]] is 3. That is, for sets of points that define a smooth shape or a shape that has a small number of corners—the shapes of traditional geometry and science—the Hausdorff dimension is an [[integer]] agreeing with the usual sense of dimension, also known as the [[Inductive dimension|topological dimension]]. However, formulas have also been developed that allow calculation of the dimension of other less simple objects, where, solely on the basis of their properties of [[scaling (geometry)|scaling]] and [[self-similarity]], one is led to the conclusion that particular objects—including [[fractal]]s—have non-integer Hausdorff dimensions. Because of the significant technical advances made by [[Abram Samoilovitch Besicovitch]] allowing computation of dimensions for highly irregular or &amp;quot;rough&amp;quot; sets, this dimension is also commonly referred to as the ''Hausdorff–Besicovitch dimension.''&lt;br /&gt;
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In mathematics, Hausdorff dimension is a measure of roughness, or more specifically, fractal dimension, that was first introduced in 1918 by mathematician Felix Hausdorff. For instance, the Hausdorff dimension of a single point is zero, of a line segment is 1, of a square is 2, and of a cube is 3. That is, for sets of points that define a smooth shape or a shape that has a small number of corners—the shapes of traditional geometry and science—the Hausdorff dimension is an integer agreeing with the usual sense of dimension, also known as the topological dimension. However, formulas have also been developed that allow calculation of the dimension of other less simple objects, where, solely on the basis of their properties of scaling and self-similarity, one is led to the conclusion that particular objects—including fractals—have non-integer Hausdorff dimensions. Because of the significant technical advances made by Abram Samoilovitch Besicovitch allowing computation of dimensions for highly irregular or &amp;quot;rough&amp;quot; sets, this dimension is also commonly referred to as the Hausdorff–Besicovitch dimension.&lt;br /&gt;
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在[[数学]]中，'''&amp;lt;font color = '#ff8000'&amp;gt;豪斯多夫维数Hausdorff dimension&amp;lt;/font&amp;gt;'''是一种粗糙度的度量单位，或者更确切地说，分形维数，是由数学家 Felix Hausdorff 在1918年首次提出的。例如，单点的豪斯多夫维数为零，线段为1，正方形为2，立方体为3。也就是说，对于定义了一个光滑形状或一个有少数几个角的形状---- 传统几何学和科学的形状---- 的点集来说，豪斯多夫维数是一个整数，符合通常的维度意义，也称为拓扑维度。然而，还有一些公式允许计算其他不太简单的对象的维数，其中仅仅根据它们的标度和自相似特性，就可以得出结论: 特定的对象ー包括分形ー具有非整数的 Hausdorff 维数。由于阿布拉姆·萨莫伊洛维奇·贝西科维奇的重大技术进步，允许计算高度不规则或“粗糙”集的维度，这个维度通常也被称为 Hausdorff-Besicovitch 维度。 &lt;br /&gt;
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The Hausdorff dimension, more specifically, is a further dimensional number associated with a given set, where the distances between all members of that set are defined. Such a set is termed a [[metric space]]. The dimension is drawn from the [[Extended real number line|extended real numbers]], &amp;lt;math&amp;gt;\overline{\mathbb{R}}&amp;lt;/math&amp;gt;, as opposed to the more intuitive notion of dimension, which is not associated to general metric spaces, and only takes values in the non-negative integers.&lt;br /&gt;
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The Hausdorff dimension, more specifically, is a further dimensional number associated with a given set, where the distances between all members of that set are defined. Such a set is termed a metric space. The dimension is drawn from the extended real numbers, &amp;lt;math&amp;gt;\overline{\mathbb{R}}&amp;lt;/math&amp;gt;, as opposed to the more intuitive notion of dimension, which is not associated to general metric spaces, and only takes values in the non-negative integers.&lt;br /&gt;
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更具体地说，豪斯多夫维数是一个与给定集合相关联的更进一步的维数，其中定义了该集合所有成员之间的距离。这样的集合称为度量空间。维数是从扩展的实数，&amp;lt;math&amp;gt;\overline{\mathbb{R}}&amp;lt;/math&amp;gt;，而不是更直观的维数概念(它不与一般的度量空间相关联，只取非负整数的值)。&lt;br /&gt;
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In mathematical terms, the Hausdorff dimension generalizes the notion of the dimension of a real [[vector space]]. That is, the Hausdorff dimension of an ''n''-dimensional [[inner product space]] equals ''n''. This underlies the earlier statement that the Hausdorff dimension of a point is zero, of a line is one, etc., and that [[fractal|irregular sets]] can have noninteger Hausdorff dimensions. For instance, the [[Koch snowflake]] shown at right is constructed from an equilateral triangle; in each iteration, its component line segments are divided into 3 segments of unit length, the newly created middle segment is used as the base of a new [[equilateral]] triangle that points outward, and this base segment is then deleted to leave a final object from the iteration of unit length of 4.&amp;lt;ref&amp;gt;Larry Riddle, 2014, &amp;quot;Classic Iterated Function Systems: Koch Snowflake&amp;quot;, Agnes Scott College e-Academy (online), see [http://ecademy.agnesscott.edu/~lriddle/ifs/ksnow/ksnow.htm], accessed 5 March 2015.&amp;lt;/ref&amp;gt; That is, after the first iteration, each original line segment has been replaced with N=4, where each self-similar copy is 1/S = 1/3 as long as the original.&amp;lt;ref name=CampbellAnnenberg15/&amp;gt; Stated another way, we have taken an object with Euclidean dimension, D, and reduced its linear scale by 1/3 in each direction, so that its length increases to N=S&amp;lt;sup&amp;gt;D&amp;lt;/sup&amp;gt;.&amp;lt;ref name=ClaytonSCTPLS96&amp;gt;Keith Clayton, 1996, &amp;quot;Fractals and the Fractal Dimension,&amp;quot; ''Basic Concepts in Nonlinear Dynamics and Chaos'' (workshop), Society for Chaos Theory in Psychology and the Life Sciences annual meeting, June 28, 1996, Berkeley, California, see [http://www.vanderbilt.edu/AnS/psychology/cogsci/chaos/workshop/Workshop.html], accessed 5 March 2015.&amp;lt;/ref&amp;gt; This equation is easily solved for D, yielding the ratio of logarithms (or [[natural logarithm]]s) appearing in the figures, and giving—in the Koch and other fractal cases—non-integer dimensions for these objects.&lt;br /&gt;
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In mathematical terms, the Hausdorff dimension generalizes the notion of the dimension of a real vector space. That is, the Hausdorff dimension of an n-dimensional inner product space equals n. This underlies the earlier statement that the Hausdorff dimension of a point is zero, of a line is one, etc., and that irregular sets can have noninteger Hausdorff dimensions. For instance, the Koch snowflake shown at right is constructed from an equilateral triangle; in each iteration, its component line segments are divided into 3 segments of unit length, the newly created middle segment is used as the base of a new equilateral triangle that points outward, and this base segment is then deleted to leave a final object from the iteration of unit length of 4. That is, after the first iteration, each original line segment has been replaced with N=4, where each self-similar copy is 1/S = 1/3 as long as the original. This equation is easily solved for D, yielding the ratio of logarithms (or natural logarithms) appearing in the figures, and giving—in the Koch and other fractal cases—non-integer dimensions for these objects.&lt;br /&gt;
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用数学术语来说，豪斯多夫维数概括了实向量空间维数的概念。也就是说，n 维内积空间的豪斯多夫维数等于 n。 这就是早期假设的基础，一个点的豪斯多夫维数是零，一条线是一等等，不规则集可以有非整数的豪斯多夫维数。例如，右边所示的 Koch 雪花是由一个正三角形构成的; 在每次迭代中，它的组成线段被分成单位长度的3段，新创建的中间线段被用作一个指向外部的新正三角形的基础，然后人们删除这个基础线段用来保留单位长度4的迭代中的最终对象。也就是说，在第一次迭代之后，每个原始线段都被替换为 N=4，其中每个自相似拷贝的长度是原始线段的1/S = 1/3 。这个方程很容易求解为 D，产生出现在图形中的对数(或自然对数)的比率，并给出——在 Koch 和其他分形情况下——这些对象的非整数维数。&lt;br /&gt;
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The Hausdorff dimension is a successor to the simpler, but usually equivalent, box-counting or [[Minkowski–Bouligand dimension]].&lt;br /&gt;
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The Hausdorff dimension is a successor to the simpler, but usually equivalent, box-counting or Minkowski–Bouligand dimension.&lt;br /&gt;
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豪斯多夫维数是更简单但通常等价的'''&amp;lt;font color = '#ff8000'&amp;gt;计盒维数box-counting&amp;lt;/font&amp;gt;'''或'''&amp;lt;font color = '#ff8000'&amp;gt;闵可夫斯基维数Minkowski-Bouligand&amp;lt;/font&amp;gt;'''的继承者。&lt;br /&gt;
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==Intuition概念==&lt;br /&gt;
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The intuitive concept of dimension of a geometric object ''X'' is the number of independent parameters one needs to pick out a unique point inside. However, any point specified by two parameters can be instead specified by one, because the [[cardinality]] of the [[real plane]] is equal to the cardinality of the [[real line]] (this can be seen by an [[Cantor's diagonal argument|argument]] involving interweaving the digits of two numbers to yield a single number encoding the same information). The example of a [[space-filling curve]] shows that one can even map the real line to the real plane [[Surjective function|surjectively]] (taking one real number into a pair of real numbers in a way so that all pairs of numbers are covered) and ''continuously'', so that a one-dimensional object completely fills up a higher-dimensional object.&lt;br /&gt;
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The intuitive concept of dimension of a geometric object X is the number of independent parameters one needs to pick out a unique point inside. However, any point specified by two parameters can be instead specified by one, because the cardinality of the real plane is equal to the cardinality of the real line (this can be seen by an argument involving interweaving the digits of two numbers to yield a single number encoding the same information). The example of a space-filling curve shows that one can even map the real line to the real plane surjectively (taking one real number into a pair of real numbers in a way so that all pairs of numbers are covered) and continuously, so that a one-dimensional object completely fills up a higher-dimensional object.&lt;br /&gt;
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几何物体X的直观尺寸概念就是一个物体需要多少个独立参数才能找到一个独特的点。但是，任何由两个参数指定的点都可以由一个参数指定，因为实际平面的基数等于实际行的基数(这可以通过一个参数看到，该参数涉及交织两个数字的数字以产生一个编码相同信息的单个数字)。'''&amp;lt;font color = '#ff8000'&amp;gt;皮亚诺曲线&amp;lt;/font&amp;gt;'''的例子表明，一个人甚至可以完美和连续地映射实际线到真正的平面(把一个实数转换成一对实数，这样所有的数对都被覆盖)，由此一维物体完全填充了一个高维物体。&lt;br /&gt;
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Every space filling curve hits some points multiple times, and does not have a continuous inverse. It is impossible to map two dimensions onto one in a way that is continuous and continuously invertible. The topological dimension, also called [[Lebesgue covering dimension]], explains why. This dimension is ''n'' if, in every covering of ''X'' by small open balls, there is at least one point where ''n''&amp;amp;nbsp;+&amp;amp;nbsp;1 balls overlap. For example, when one covers a line with short open intervals, some points must be covered twice, giving dimension&amp;amp;nbsp;''n''&amp;amp;nbsp;=&amp;amp;nbsp;1.&lt;br /&gt;
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Every space filling curve hits some points multiple times, and does not have a continuous inverse. It is impossible to map two dimensions onto one in a way that is continuous and continuously invertible. The topological dimension, also called Lebesgue covering dimension, explains why. This dimension is n if, in every covering of X by small open balls, there is at least one point where n&amp;amp;nbsp;+&amp;amp;nbsp;1 balls overlap. For example, when one covers a line with short open intervals, some points must be covered twice, giving dimension&amp;amp;nbsp;n&amp;amp;nbsp;=&amp;amp;nbsp;1.&lt;br /&gt;
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每条空间填充曲线都会多次撞击某些点，且不存在连续的倒数。将两个维度以连续和连续可逆的方式映射到一个维度是不可能的。'''&amp;lt;font color = '#ff8000'&amp;gt;拓扑维度 topological dimension&amp;lt;/font&amp;gt;'''，也被称为拓朴维数，解释了为什么。这个维度是 n，如果在 x 的每个小开球覆盖中，至少有一个点 n + 1个球重叠。例如，当一个点覆盖一条具有短开区间的直线时，某些点必须被覆盖两次，给出维数''n''&amp;amp;nbsp;=&amp;amp;nbsp;1。&lt;br /&gt;
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But topological dimension is a very crude measure of the local size of a space (size near a point). A curve that is almost space-filling can still have topological dimension one, even if it fills up most of the area of a region. A [[fractal]] has an integer topological dimension, but in terms of the amount of space it takes up, it behaves like a higher-dimensional space.&lt;br /&gt;
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But topological dimension is a very crude measure of the local size of a space (size near a point). A curve that is almost space-filling can still have topological dimension one, even if it fills up most of the area of a region. A fractal has an integer topological dimension, but in terms of the amount of space it takes up, it behaves like a higher-dimensional space.&lt;br /&gt;
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但是，拓扑维度是对空间局部尺寸(点附近的尺寸)的一个非常粗略的度量。一条几乎是空间填充的曲线仍然可以有一维拓扑，即使它填充了一个区域的大部分面积。分形具有整数的拓扑维数，但就其所占空间的数量而言，它看起来像一个更高维的空间。&lt;br /&gt;
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The Hausdorff dimension measures the local size of a space taking into account the distance between points, the [[metric space|metric]]. Consider the number ''N''(''r'') of [[ball (mathematics)|balls]] of radius at most ''r'' required to cover ''X'' completely. When ''r'' is very small, ''N''(''r'') grows polynomially with 1/''r''. For a sufficiently well-behaved  ''X'', the Hausdorff dimension is the unique number ''d'' such that N(''r'') grows as 1/''r&amp;lt;sup&amp;gt;d&amp;lt;/sup&amp;gt;'' as ''r'' approaches zero. More precisely, this defines the [[Minkowski–Bouligand dimension|box-counting dimension]], which equals the Hausdorff dimension when the value ''d'' is a critical boundary between growth rates that are insufficient to cover the space, and growth rates that are overabundant.&lt;br /&gt;
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The Hausdorff dimension measures the local size of a space taking into account the distance between points, the metric. Consider the number N(r) of balls of radius at most r required to cover X completely. When r is very small, N(r) grows polynomially with 1/r. For a sufficiently well-behaved  X, the Hausdorff dimension is the unique number d such that N(r) grows as 1/r&amp;lt;sup&amp;gt;d&amp;lt;/sup&amp;gt; as r approaches zero. More precisely, this defines the box-counting dimension, which equals the Hausdorff dimension when the value d is a critical boundary between growth rates that are insufficient to cover the space, and growth rates that are overabundant.&lt;br /&gt;
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豪斯多夫维数测量一个空间的局部大小时，会考虑到点之间距离的度量。考虑半径最大为 r 的球数 ''N'' (r) ，需要完全覆盖 ''X''。当 r 很小时，n (r)以1/''r'' 增长多项式。对于一个表现足够好的 ''X''，豪斯多夫维数是唯一的数 d，这样当 r 趋近于零时， N(r)增长为1/r&amp;lt;sup&amp;gt;d&amp;lt;/sup&amp;gt; 。更确切地说，这定义了盒子计数维度，当值 d 是不足以覆盖空间的增长率和过度充裕的增长率之间的关键边界时，它等于豪斯多夫维数。&lt;br /&gt;
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For shapes that are smooth, or shapes with a small number of corners, the shapes of traditional geometry and science, the Hausdorff dimension is an integer agreeing with the topological dimension. But [[Benoit Mandelbrot]] observed that [[fractal]]s, sets with noninteger Hausdorff dimensions, are found everywhere in nature. He observed that the proper idealization of most rough shapes you see around you is not in terms of smooth idealized shapes, but in terms of fractal idealized shapes:&lt;br /&gt;
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For shapes that are smooth, or shapes with a small number of corners, the shapes of traditional geometry and science, the Hausdorff dimension is an integer agreeing with the topological dimension. But Benoit Mandelbrot observed that fractals, sets with noninteger Hausdorff dimensions, are found everywhere in nature. He observed that the proper idealization of most rough shapes you see around you is not in terms of smooth idealized shapes, but in terms of fractal idealized shapes:&lt;br /&gt;
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对于光滑的形状，或者有少量棱角的形状，传统几何和科学的形状，豪斯多夫维数是一个整数，与拓扑维度一致。但是伯努·曼德布洛特观察到分形---- 具有非整数豪斯多夫维数的集合---- 在自然界中随处可见。他观察到，我们周围大多数粗糙形状的理想化不是光滑的理想化形状，而是分形理想化形状:&lt;br /&gt;
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&amp;lt;blockquote&amp;gt;Clouds are not spheres, mountains are not cones, coastlines are not circles, and bark is not smooth, nor does lightning travel in a straight line.&amp;lt;ref name=&amp;quot;mandelbrot&amp;quot;&amp;gt;{{cite book   | last = Mandelbrot   | first = Benoît   | authorlink = Benoit Mandelbrot   | title = The Fractal Geometry of Nature   | publisher = W. H. Freeman   | series = Lecture notes in mathematics 1358   | year = 1982   | doi =    | isbn = 0-7167-1186-9   | url-access = registration   | url = https://archive.org/details/fractalgeometryo00beno   }}&amp;lt;/ref&amp;gt;&amp;lt;/blockquote&amp;gt;&lt;br /&gt;
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&amp;lt;blockquote&amp;gt;Clouds are not spheres, mountains are not cones, coastlines are not circles, and bark is not smooth, nor does lightning travel in a straight line.&amp;lt;/blockquote&amp;gt;&lt;br /&gt;
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&amp;lt;blockquote&amp;gt;云不是球体，山不是锥体，海岸线不是圆圈，树皮不平滑，闪电也不是直线运动。 &amp;lt;/blockquote&amp;gt;&lt;br /&gt;
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For fractals that occur in nature, the Hausdorff and [[Minkowski–Bouligand dimension|box-counting dimension]] coincide. The [[packing dimension]] is yet another similar notion which gives the same value for many shapes, but there are well documented exceptions where all these dimensions differ.&lt;br /&gt;
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For fractals that occur in nature, the Hausdorff and box-counting dimension coincide. The packing dimension is yet another similar notion which gives the same value for many shapes, but there are well documented exceptions where all these dimensions differ.&lt;br /&gt;
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对于自然界中出现的分形，豪斯多夫维数和盒计数维数是一致的。封装尺寸是另一个类似的概念，它给出了许多形状相同的值，但是在所有这些尺寸不同的情况，都做了很好的说明。&lt;br /&gt;
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==Formal definitions形式化定义==&lt;br /&gt;
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===Hausdorff content豪斯多夫集===&lt;br /&gt;
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Let ''X'' be a [[metric space]]. If ''S'' ⊂ ''X'' and ''d'' ∈ [0, ∞), the ''d''-dimensional '''unlimited Hausdorff content''' of ''S'' is defined by&lt;br /&gt;
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Let X be a metric space. If S ⊂ X and d ∈ [0, ∞), the d-dimensional unlimited Hausdorff content of S is defined by&lt;br /&gt;
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设 ''X''是度量空间。若''S'' ⊂ ''X'' 和 ''d'' ∈ [0, ∞) ，则 ''S'' 的''d''维无限 豪斯多夫集定义为&lt;br /&gt;
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:&amp;lt;math&amp;gt;C_H^d(S):=\inf\Bigl\{\sum_i r_i^d:\text{ there is a cover of } S\text{ by balls with radii }r_i&amp;gt;0\Bigr\}.&amp;lt;/math&amp;gt;&lt;br /&gt;
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&amp;lt;math&amp;gt;C_H^d(S):=\inf\Bigl\{\sum_i r_i^d:\text{ there is a cover of } S\text{ by balls with radii }r_i&amp;gt;0\Bigr\}.&amp;lt;/math&amp;gt;&lt;br /&gt;
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&amp;lt;math&amp;gt;C_H^d(S):=\inf\Bigl\{\sum_i r_i^d:\text{ there is a cover of } S\text{ by balls with radii }r_i&amp;gt;0\Bigr\}.&amp;lt;/math&amp;gt;&lt;br /&gt;
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In other words, &amp;lt;math&amp;gt;C_H^d(S)&amp;lt;/math&amp;gt; is the [[infimum]] of the set of numbers &amp;lt;math&amp;gt;\delta \geq 0&amp;lt;/math&amp;gt; such that there is some (indexed) collection of [[ball (mathematics)|ball]]s &amp;lt;math&amp;gt;\{B(x_i,r_i):i\in I\}&amp;lt;/math&amp;gt; covering ''S'' with ''r&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;''&amp;amp;nbsp;&amp;gt;&amp;amp;nbsp;0 for each ''i''&amp;amp;nbsp;∈&amp;amp;nbsp;''I'' that satisfies &amp;lt;math&amp;gt;\sum_{i\in I} r_i^d&amp;lt;\delta &amp;lt;/math&amp;gt;. (Here, we use the standard convention that [[infimum|inf&amp;amp;nbsp;Ø&amp;amp;nbsp;=&amp;amp;nbsp;∞]].)&lt;br /&gt;
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In other words, &amp;lt;math&amp;gt;C_H^d(S)&amp;lt;/math&amp;gt; is the infimum of the set of numbers &amp;lt;math&amp;gt;\delta \geq 0&amp;lt;/math&amp;gt; such that there is some (indexed) collection of balls &amp;lt;math&amp;gt;\{B(x_i,r_i):i\in I\}&amp;lt;/math&amp;gt; covering S with r&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;&amp;amp;nbsp;&amp;gt;&amp;amp;nbsp;0 for each i&amp;amp;nbsp;∈&amp;amp;nbsp;I that satisfies &amp;lt;math&amp;gt;\sum_{i\in I} r_i^d&amp;lt;\delta &amp;lt;/math&amp;gt;. (Here, we use the standard convention that inf&amp;amp;nbsp;Ø&amp;amp;nbsp;=&amp;amp;nbsp;∞.)&lt;br /&gt;
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换句话说，&amp;lt;math&amp;gt;C_H^d(S)&amp;lt;/math&amp;gt; 是数字集合&amp;lt;math&amp;gt;\delta \geq 0&amp;lt;/math&amp;gt;的下确界，使得在 ''i''&amp;amp;nbsp;∈&amp;amp;nbsp中存在一些球集合 &amp;lt;math&amp;gt;\{B(x_i,r_i):i\in I\}&amp;lt;/math&amp;gt;  i 包含 s，对于每个 ''r&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;''&amp;amp;nbsp;&amp;gt;&amp;amp;nbsp;0 满足 i 中的和&amp;lt;math&amp;gt;\sum_{i\in I} r_i^d&amp;lt;\delta &amp;lt;/math&amp;gt; (在这里，我们使用inf&amp;amp;nbsp;Ø&amp;amp;nbsp;=&amp;amp;nbsp;∞ )的标准约定。&lt;br /&gt;
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===Hausdorff measurement豪斯多夫分形测量===&lt;br /&gt;
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The Hausdorff outer measure is different from the unbounded Hausdorf content in that rather than considering all possible coverings of ''S'', we see what happens when the sizes of the balls go to zero. This is  for &amp;lt;math&amp;gt;d \geq 0 &amp;lt;/math&amp;gt;, we define the ''d''-dimensional Hausdorff outer measure of ''S'' as&lt;br /&gt;
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The Hausdorff outer measure is different from the unbounded Hausdorf content in that rather than considering all possible coverings of S, we see what happens when the sizes of the balls go to zero. This is  for &amp;lt;math&amp;gt;d \geq 0 &amp;lt;/math&amp;gt;, we define the d-dimensional Hausdorff outer measure of S as&lt;br /&gt;
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豪斯多夫外测度不同于无界的豪斯多夫，因为我们不考虑 s 的所有可能，我们看到当球的大小为零时会发生什么。这是为了数学  &amp;lt;math&amp;gt;d \geq 0 &amp;lt;/math&amp;gt;，我们定义了  ''S''的 ''d''维豪斯多夫Hausdorff 外测度为&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt; \mathcal{H}^d(S):=\lim_{r \to 0} \inf\Bigl\{\sum_i r_i^d:\text{ there is a cover of } S\text{ by balls with radii } 0 &amp;lt; r_i &amp;lt; r\Bigr\}.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \mathcal{H}^d(S):=\lim_{r \to 0} \inf\Bigl\{\sum_i r_i^d:\text{ there is a cover of } S\text{ by balls with radii } 0 &amp;lt; r_i &amp;lt; r\Bigr\}.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \mathcal{H}^d(S):=\lim_{r \to 0} \inf\Bigl\{\sum_i r_i^d:\text{有一个面} S\text{ 球 } 0 &amp;lt; r_i &amp;lt; r\Bigr\}.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
===Hausdorff dimension豪斯多夫维数===&lt;br /&gt;
&lt;br /&gt;
The '''Hausdorff dimension''' of ''X'' is defined by&lt;br /&gt;
&lt;br /&gt;
The Hausdorff dimension of X is defined by&lt;br /&gt;
&lt;br /&gt;
X 的豪斯多夫维数定义为&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt;\dim_{\operatorname{H}}(X):=\inf\{d\ge 0: \mathcal{H}^d(X)=0\}.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt;\dim_{\operatorname{H}}(X):=\inf\{d\ge 0: \mathcal{H}^d(X)=0\}.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Equivalently, dim&amp;lt;sub&amp;gt;H&amp;lt;/sub&amp;gt;(''X'') may be defined as the [[infimum]] of the set of ''d'' ∈ [0, ∞) such that the ''d''-dimensional [[Hausdorff measure]] of ''X'' is zero. This is the same as the supremum of the set of ''d''&amp;amp;nbsp;∈&amp;amp;nbsp;[0,&amp;amp;nbsp;∞) such that the ''d''-dimensional Hausdorff measure of ''X'' is infinite (except that when this latter set of numbers ''d'' is empty the Hausdorff dimension is zero).&lt;br /&gt;
&lt;br /&gt;
Equivalently, dim&amp;lt;sub&amp;gt;H&amp;lt;/sub&amp;gt;(X) may be defined as the infimum of the set of d ∈ [0, ∞) such that the d-dimensional Hausdorff measure of X is zero. This is the same as the supremum of the set of d&amp;amp;nbsp;∈&amp;amp;nbsp;[0,&amp;amp;nbsp;∞) such that the d-dimensional Hausdorff measure of X is infinite (except that when this latter set of numbers d is empty the Hausdorff dimension is zero).&lt;br /&gt;
&lt;br /&gt;
等价地，dim &amp;lt;sub&amp;gt;H&amp;lt;/sub&amp;gt;(''X'')可定义为 ''d'' ∈ [0, ∞) 集的下确界，使得''X'' 的''d''-维 [[豪斯多夫测度]] 为零。这与 ''d''&amp;amp;nbsp;∈&amp;amp;nbsp;[0,&amp;amp;nbsp;∞)的集合的上确界相同，因此''X''的 d 维豪斯多夫测度是无限的(除非后一个集合 ''d'' 是空的，豪斯多夫维数为零)。&lt;br /&gt;
&lt;br /&gt;
==Examples实例==&lt;br /&gt;
&lt;br /&gt;
[[Image:Sierpinski deep.svg|thumb|250px|Dimension of a further [[fractal]] example. The [[Sierpinski triangle]], an object with Hausdorff dimension of log(3)/log(2)≈1.58.&amp;lt;ref name=ClaytonSCTPLS96/&amp;gt;]]&lt;br /&gt;
&lt;br /&gt;
Dimension of a further [[fractal example. The Sierpinski triangle, an object with Hausdorff dimension of log(3)/log(2)≈1.58.]]&lt;br /&gt;
&lt;br /&gt;
[[Image:谢尔宾斯基三角形 deep.svg|thumb|250px|进一步的[[分形维数]]的例子，进一步的分形维数的例子是谢尔宾斯基三角形，它是一个豪斯多夫维数为log(3)/log(2)≈1.58.&amp;lt;ref name=ClaytonSCTPLS96/&amp;gt;的物体]]&lt;br /&gt;
&lt;br /&gt;
* [[Countable set]]s have Hausdorff dimension 0.&amp;lt;ref name=&amp;quot;schleicher&amp;quot;&amp;gt;{{cite journal |last1=Schleicher |first1=Dierk |title=Hausdorff Dimension, Its Properties, and Its Surprises |journal=The American Mathematical Monthly |date=June 2007 |volume=114 |issue=6 |pages=509–528 |doi=10.1080/00029890.2007.11920440 |language=en |issn=0002-9890|arxiv=math/0505099 }}&amp;lt;/ref&amp;gt;&lt;br /&gt;
*[[可数集]]拥有豪斯多夫维数0.&amp;lt;ref name=&amp;quot;schleicher&amp;quot;&amp;gt;{{cite journal |last1=Schleicher |first1=Dierk |title=豪斯多夫维数, Its Properties, and Its Surprises |journal=The American Mathematical Monthly美国数学期刊 |date=June 2007 |volume=114 |issue=6 |pages=509–528 |doi=10.1080/00029890.2007.11920440 |language=en |issn=0002-9890|arxiv=math/0505099 }}&amp;lt;/ref&amp;gt;&lt;br /&gt;
* The [[Euclidean space]] ℝ&amp;lt;sup&amp;gt;''n''&amp;lt;/sup&amp;gt; has Hausdorff dimension ''n'', and the circle '''S'''&amp;lt;sup&amp;gt;1&amp;lt;/sup&amp;gt; has Hausdorff dimension 1.&amp;lt;ref name=&amp;quot;schleicher&amp;quot; /&amp;gt;&lt;br /&gt;
*[[教育空间]] ℝ&amp;lt;sup&amp;gt;''n''&amp;lt;/sup&amp;gt; 有豪斯多夫维数 ''n''，循环'''S'''&amp;lt;sup&amp;gt;1&amp;lt;/sup&amp;gt; 拥有豪斯多夫维数1.&amp;lt;ref name=&amp;quot;schleicher&amp;quot; /&amp;gt;&lt;br /&gt;
* [[Fractal]]s often are spaces whose Hausdorff dimension strictly exceeds the [[topological dimension]].&amp;lt;ref name=&amp;quot;mandelbrot&amp;quot; /&amp;gt; For example, the [[Cantor set]], a zero-dimensional topological space, is a union of two copies of itself, each copy shrunk by a factor 1/3; hence, it can be shown that its Hausdorff dimension is ln(2)/ln(3)&amp;amp;nbsp;≈&amp;amp;nbsp;0.63.&amp;lt;ref&amp;gt;{{cite book | last=Falconer | first = Kenneth |title=Fractal Geometry: Mathematical Foundations and Applications | publisher=[[John Wiley and Sons]] | edition=2nd | year=2003}}&amp;lt;/ref&amp;gt; The [[Sierpinski triangle]] is a union of three copies of itself, each copy shrunk by a factor of&amp;amp;nbsp;1/2; this yields a Hausdorff dimension of ln(3)/ln(2)&amp;amp;nbsp;≈&amp;amp;nbsp;1.58.&amp;lt;ref name=CampbellAnnenberg15/&amp;gt; These Hausdorff dimensions are related to the &amp;quot;critical exponent&amp;quot; of the [[Master theorem (analysis of algorithms)|Master theorem]] for solving [[Recurrence relation|recurrence relations]] in the [[analysis of algorithms]].&lt;br /&gt;
*[[分形]]一般是那些豪斯多夫维数直接超过其拓扑维数的空间。例如[[康托尔集]]是一个o维拓扑空间，由两个自己复制而成，每一个复制品都是原来的三分之一，因此它的豪斯多夫维数是 ln(2)/ln(3)&amp;amp;nbsp;≈&amp;amp;nbsp;0.63。&amp;lt;ref&amp;gt;{{cite book | last=Falconer | first = Kenneth |title=Fractal Geometry: Mathematical Foundations and Applications | publisher=[[John Wiley and Sons]] | edition=2nd | year=2003}}&amp;lt;/ref&amp;gt;一个[[谢尔宾斯基三角]]是他自身三个复制的组合。每一个是原来的&amp;amp;nbsp;1/2，它的豪斯多夫维数ln(3)/ln(2)&amp;amp;nbsp;≈&amp;amp;nbsp;1.58。&amp;lt;ref name=CampbellAnnenberg15/&amp;gt;在递归算法中解决递归关系时，这些豪斯多夫维数与[[算法分析主定理]]的临界指标相联系。&lt;br /&gt;
* [[Space-filling curve]]s like the [[Peano curve]] have the same Hausdorff dimension as the space they fill.&lt;br /&gt;
*[[空间填充曲线]]拥有和他们填充空间同样的豪斯多夫维数，如[[皮亚诺曲线]]。&lt;br /&gt;
* The trajectory of [[Brownian motion]] in dimension 2 and above is conjectured to be Hausdorff dimension 2.&amp;lt;ref&amp;gt;{{cite book | last=Morters | first=Peres | title= Brownian Motion | publisher=[[Cambridge University Press]] | year=2010 }}&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
[[image:Great Britain Hausdorff.svg|thumb|250px|Estimating the Hausdorff dimension of the [[How Long Is the Coast of Britain? Statistical Self-Similarity and Fractional Dimension|coast of Great Britain]]]]&lt;br /&gt;
&lt;br /&gt;
coast of Great Britain]]&lt;br /&gt;
&lt;br /&gt;
[[大不列颠海岸&lt;br /&gt;
&lt;br /&gt;
* 刘易斯·弗赖伊·理查森[[Lewis Fry Richardson]] has performed detailed experiments to measure the approximate Hausdorff dimension for various coastlines. His results have varied from 1.02 for the coastline of [[South Africa]] to 1.25 for the west coast of [[Great Britain]].&amp;lt;ref name=&amp;quot;mandelbrot&amp;quot; /&amp;gt;&lt;br /&gt;
*刘易斯·弗赖伊·理查森（Lewis Fry Richardson）已经通过豪斯多夫维数去测量了很多海岸线。它的结果涵盖从1.02的南非海岸线到1.25的大英帝国西海岸模型。]]&lt;br /&gt;
&lt;br /&gt;
==Properties of Hausdorff dimension豪斯多夫维数特性==&lt;br /&gt;
&lt;br /&gt;
{{refimprove section|date=March 2015}}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
=== Hausdorff dimension and inductive dimension 豪斯多夫维数和归纳维数===&lt;br /&gt;
&lt;br /&gt;
Let ''X'' be an arbitrary [[Separable space|separable]] metric space. There is a [[topology|topological]] notion of [[inductive dimension]] for ''X'' which is defined recursively. It is always an integer (or +∞) and is denoted dim&amp;lt;sub&amp;gt;ind&amp;lt;/sub&amp;gt;(''X'').&lt;br /&gt;
&lt;br /&gt;
Let X be an arbitrary separable metric space. There is a topological notion of inductive dimension for X which is defined recursively. It is always an integer (or +∞) and is denoted dim&amp;lt;sub&amp;gt;ind&amp;lt;/sub&amp;gt;(X).&lt;br /&gt;
&lt;br /&gt;
设''X'' 是[[任意可分度量空间]]。对于''X'' 有一个递归定义的归纳维数拓扑概念。它总是一个整数(或 + ∞) ，并且表示dim&amp;lt;sub&amp;gt;ind&amp;lt;/sub&amp;gt;(''X'')。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
'''Theorem'''. Suppose ''X'' is non-empty. Then &lt;br /&gt;
&lt;br /&gt;
Theorem. Suppose X is non-empty. Then &lt;br /&gt;
&lt;br /&gt;
'''定理'''：假设''X'' 是非空的。那么&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt; \dim_{\mathrm{Haus}}(X) \geq \dim_{\operatorname{ind}}(X). &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \dim_{\mathrm{Haus}}(X) \geq \dim_{\operatorname{ind}}(X). &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Moreover,&lt;br /&gt;
&lt;br /&gt;
Moreover,&lt;br /&gt;
&lt;br /&gt;
此外,&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \inf_Y \dim_{\operatorname{Haus}}(Y) =\dim_{\operatorname{ind}}(X), &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \inf_Y \dim_{\operatorname{Haus}}(Y) =\dim_{\operatorname{ind}}(X), &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
where ''Y'' ranges over metric spaces [[homeomorphic]] to ''X''. In other words, ''X'' and ''Y'' have the same underlying set of points and the metric ''d''&amp;lt;sub&amp;gt;''Y''&amp;lt;/sub&amp;gt; of ''Y'' is topologically equivalent to ''d''&amp;lt;sub&amp;gt;''X''&amp;lt;/sub&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
where Y ranges over metric spaces homeomorphic to X. In other words, X and Y have the same underlying set of points and the metric d&amp;lt;sub&amp;gt;Y&amp;lt;/sub&amp;gt; of Y is topologically equivalent to d&amp;lt;sub&amp;gt;X&amp;lt;/sub&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
其中''Y''是度量空间同胚到 ''X''的范围。换句话说， ''X''和 ''Y''具有相同的基本点集，''Y''的度规''d''&amp;lt;sub&amp;gt;''Y''&amp;lt;/sub&amp;gt; 的子拓扑等价于''d''&amp;lt;sub&amp;gt;''X''&amp;lt;/sub&amp;gt;。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
These results were originally established by [[Edward Szpilrajn]] (1907–1976), e.g., see Hurewicz and Wallman, Chapter VII.{{full citation needed|date=March 2015}}&lt;br /&gt;
&lt;br /&gt;
These results were originally established by Edward Szpilrajn (1907–1976), e.g., see Hurewicz and Wallman, Chapter VII.&lt;br /&gt;
&lt;br /&gt;
这些结果最初是由 [[Edward Szpilrajn]] (1907–1976)建立的,  参见 Hurewicz and Wallman, Chapter VII.{{full citation needed|date=March 2015}}第七章。&lt;br /&gt;
&lt;br /&gt;
=== Hausdorff dimension and Minkowski dimension 豪斯多夫维数和闵可夫斯基维度===&lt;br /&gt;
&lt;br /&gt;
The [[Minkowski dimension]] is similar to, and at least as large as, the Hausdorff dimension, and they are equal in many situations. However, the set of [[rational number|rational]] points in [0, 1] has Hausdorff dimension zero and Minkowski dimension one. There are also compact sets for which the Minkowski dimension is strictly larger than the Hausdorff dimension.&lt;br /&gt;
&lt;br /&gt;
The Minkowski dimension is similar to, and at least as large as, the Hausdorff dimension, and they are equal in many situations. However, the set of rational points in [0, 1] has Hausdorff dimension zero and Minkowski dimension one. There are also compact sets for which the Minkowski dimension is strictly larger than the Hausdorff dimension.&lt;br /&gt;
&lt;br /&gt;
[[闵可夫斯基维数]]与豪斯多夫维数相似，至少和它一样大，而且在许多情况下是相等的。然而，[0,1]中有理点集的豪斯多夫维数为0，闵可夫斯基维数为1。还有一些紧集的闵可夫斯基维数绝对大于豪斯多夫维数。&lt;br /&gt;
&lt;br /&gt;
=== Hausdorff dimensions and Frostman measures 豪斯多夫维度和弗洛斯曼测度===&lt;br /&gt;
&lt;br /&gt;
If there is a [[measure (mathematics)|measure]] μ defined on [[Borel measure|Borel]] subsets of a metric space ''X'' such that ''μ''(''X'') &amp;gt; 0 and ''μ''(''B''(''x'', ''r'')) ≤ ''r&amp;lt;sup&amp;gt;s&amp;lt;/sup&amp;gt;'' holds for some constant ''s'' &amp;gt; 0 and for every ball ''B''(''x'', ''r'') in ''X'', then dim&amp;lt;sub&amp;gt;Haus&amp;lt;/sub&amp;gt;(''X'') ≥ ''s''. A partial converse is provided by [[Frostman's lemma]].{{citation needed|date=March 2015}}&amp;lt;ref&amp;gt;This Wikipedia article also discusses further useful characterizations of the Hausdorff dimension.{{clarify|date=March 2015}}&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
If there is a measure μ defined on Borel subsets of a metric space X such that μ(X) &amp;gt; 0 and μ(B(x, r)) ≤ r&amp;lt;sup&amp;gt;s&amp;lt;/sup&amp;gt; holds for some constant s &amp;gt; 0 and for every ball B(x, r) in X, then dim&amp;lt;sub&amp;gt;Haus&amp;lt;/sub&amp;gt;(X) ≥ s. A partial converse is provided by Frostman's lemma.&lt;br /&gt;
&lt;br /&gt;
如果在度量空间 ''X'' 的 Borel 子集上定义一个测度 μ，使得''μ''(''X'') &amp;gt; 0 和''μ''(''B''(''x'', ''r'')) ≤ ''r&amp;lt;sup&amp;gt;s&amp;lt;/sup&amp;gt;''，对于某个常数 ''s'' &amp;gt; 0  和 ''X'' 中的每个球 ''B''(''x'', ''r'') 成立，则 dim&amp;lt;sub&amp;gt;Haus&amp;lt;/sub&amp;gt;(''X'') ≥ ''s'' 。 部分逆向转换由弗洛斯曼引理定义。&lt;br /&gt;
&lt;br /&gt;
=== Behaviour under unions and products ===&lt;br /&gt;
&lt;br /&gt;
If &amp;lt;math&amp;gt;X=\bigcup_{i\in I}X_i&amp;lt;/math&amp;gt; is a finite or countable union, then&lt;br /&gt;
&lt;br /&gt;
If &amp;lt;math&amp;gt;X=\bigcup_{i\in I}X_i&amp;lt;/math&amp;gt; is a finite or countable union, then&lt;br /&gt;
&lt;br /&gt;
如果 &amp;lt;math&amp;gt;X=\bigcup_{i\in I}X_i&amp;lt;/math&amp;gt; 是一个有限或可数的联合，则&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \dim_{\operatorname{Haus}}(X) =\sup_{i\in I} \dim_{\operatorname{Haus}}(X_i).&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \dim_{\operatorname{Haus}}(X) =\sup_{i\in I} \dim_{\operatorname{Haus}}(X_i).&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
This can be verified directly from the definition.&lt;br /&gt;
&lt;br /&gt;
This can be verified directly from the definition.&lt;br /&gt;
&lt;br /&gt;
这可以直接从定义得到验证。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
If ''X'' and ''Y'' are non-empty metric spaces, then the Hausdorff dimension of their product satisfies&amp;lt;ref&amp;gt;{{cite journal |author=Marstrand, J. M. |title=The dimension of Cartesian product sets |journal=Proc. Cambridge Philos. Soc. |volume=50 |issue=3 |pages=198–202 |year=1954 |doi=10.1017/S0305004100029236 |bibcode = 1954PCPS...50..198M }}&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
If X and Y are non-empty metric spaces, then the Hausdorff dimension of their product satisfies&lt;br /&gt;
&lt;br /&gt;
如果 ''X'' 和''Y''是非空度量空间，那么它们乘积的豪斯多夫维数满足&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt; \dim_{\operatorname{Haus}}(X\times Y)\ge \dim_{\operatorname{Haus}}(X)+ \dim_{\operatorname{Haus}}(Y).&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \dim_{\operatorname{Haus}}(X\times Y)\ge \dim_{\operatorname{Haus}}(X)+ \dim_{\operatorname{Haus}}(Y).&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
This inequality can be strict. It is possible to find two sets of dimension 0 whose product has dimension 1.&amp;lt;ref&amp;gt;{{cite book  | last = Falconer  | first = Kenneth J.  | title = Fractal geometry. Mathematical foundations and applications  | publisher = John Wiley &amp;amp; Sons, Inc., Hoboken, New Jersey  | year = 2003  | doi =   | isbn = }}&amp;lt;/ref&amp;gt; In the opposite direction, it is known that when ''X'' and ''Y'' are Borel subsets of '''R'''&amp;lt;sup&amp;gt;''n''&amp;lt;/sup&amp;gt;, the Hausdorff dimension of ''X'' × ''Y'' is bounded from above by the Hausdorff dimension of ''X'' plus the [[packing dimension|upper packing dimension]] of ''Y''. These facts are discussed in Mattila (1995).&lt;br /&gt;
&lt;br /&gt;
This inequality can be strict. It is possible to find two sets of dimension 0 whose product has dimension 1. In the opposite direction, it is known that when X and Y are Borel subsets of R&amp;lt;sup&amp;gt;n&amp;lt;/sup&amp;gt;, the Hausdorff dimension of X × Y is bounded from above by the Hausdorff dimension of X plus the upper packing dimension of Y. These facts are discussed in Mattila (1995).&lt;br /&gt;
&lt;br /&gt;
这种不平等可以是绝对的。有可能找到两个维数为0的集合，其乘积的维数为1。相反，我们知道当''X''和''Y''是 '''R'''&amp;lt;sup&amp;gt;''n''&amp;lt;/sup&amp;gt;的 Borel 子集时， ''X'' × ''Y''的豪斯多夫维数从上面以 ''X''的豪斯多夫维数加上 ''Y''的填充维数为界。Mattila (1995)曾就这些情况进行了讨论。&lt;br /&gt;
&lt;br /&gt;
==Self-similar sets自相似集合==&lt;br /&gt;
&lt;br /&gt;
{{refimprove section|date=March 2015}}&lt;br /&gt;
&lt;br /&gt;
Many sets defined by a self-similarity condition have dimensions which can be determined explicitly. Roughly, a set ''E'' is self-similar if it is the fixed point of a set-valued transformation ψ, that is ψ(''E'') = ''E'', although the exact definition is given below.&lt;br /&gt;
&lt;br /&gt;
Many sets defined by a self-similarity condition have dimensions which can be determined explicitly. Roughly, a set E is self-similar if it is the fixed point of a set-valued transformation ψ, that is ψ(E) = E, although the exact definition is given below.&lt;br /&gt;
&lt;br /&gt;
许多由自相似条件定义的集合具有可以显式确定的维数。粗略地说，集合''E'' 是自相似的，如果它是集值ψ变换的不动点，即ψ(''E'') = ''E''，尽管下面给出了确切的定义。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&amp;lt;blockquote&amp;gt;'''Theorem'''. Suppose&lt;br /&gt;
&lt;br /&gt;
&amp;lt;blockquote&amp;gt;Theorem. Suppose&lt;br /&gt;
&lt;br /&gt;
&amp;lt;blockquote&amp;gt;'''定理'''：假设&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt; \psi_i: \mathbf{R}^n \rightarrow \mathbf{R}^n, \quad i=1, \ldots , m &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \psi_i: \mathbf{R}^n \rightarrow \mathbf{R}^n, \quad i=1, \ldots , m &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
are [[Contraction mapping|contractive]] mappings on '''R'''&amp;lt;sup&amp;gt;''n''&amp;lt;/sup&amp;gt; with contraction constant ''r&amp;lt;sub&amp;gt;j&amp;lt;/sub&amp;gt;'' &amp;lt; 1. Then there is a unique ''non-empty'' compact set ''A'' such that&lt;br /&gt;
&lt;br /&gt;
are contractive mappings on R&amp;lt;sup&amp;gt;n&amp;lt;/sup&amp;gt; with contraction constant r&amp;lt;sub&amp;gt;j&amp;lt;/sub&amp;gt; &amp;lt; 1. Then there is a unique non-empty compact set A such that&lt;br /&gt;
&lt;br /&gt;
是'''R'''&amp;lt;sup&amp;gt;''n''&amp;lt;/sup&amp;gt;上的压缩常数''r&amp;lt;sub&amp;gt;j&amp;lt;/sub&amp;gt;'&amp;lt; 1的压缩映射。然后有一个唯一的非空紧集A &lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt; A = \bigcup_{i=1}^m \psi_i (A). &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; A = \bigcup_{i=1}^m \psi_i (A). &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&amp;lt;/blockquote&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;/blockquote&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The theorem follows from [[Stefan Banach]]'s [[Contractive mapping theorem|contractive mapping fixed point theorem]] applied to the complete metric space of non-empty compact subsets of '''R'''&amp;lt;sup&amp;gt;''n''&amp;lt;/sup&amp;gt; with the [[Hausdorff distance]].&amp;lt;ref&amp;gt;{{cite book |author=Falconer, K. J. |title=The Geometry of Fractal Sets |publisher=Cambridge University Press |location=Cambridge, UK |year=1985 |isbn=0-521-25694-1 |chapter=Theorem 8.3}}&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
The theorem follows from Stefan Banach's contractive mapping fixed point theorem applied to the complete metric space of non-empty compact subsets of R&amp;lt;sup&amp;gt;n&amp;lt;/sup&amp;gt; with the Hausdorff distance.&lt;br /&gt;
&lt;br /&gt;
这个定理来源于 Stefan Banach 的压缩映射不动点定理，该定理应用于 '''R'''&amp;lt;sup&amp;gt;''n''&amp;lt;/sup&amp;gt; 的非空紧子集的完备空间豪斯多夫距离。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
===The open set condition开集条件===&lt;br /&gt;
&lt;br /&gt;
To determine the dimension of the self-similar set ''A'' (in certain cases), we need a technical condition called the ''open set condition'' (OSC) on the sequence of contractions ψ&amp;lt;sub&amp;gt;''i''&amp;lt;/sub&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
To determine the dimension of the self-similar set A (in certain cases), we need a technical condition called the open set condition (OSC) on the sequence of contractions ψ&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
为了确定自相似集''A'' 的维数(在某些情况下) ，我们需要一个称为''开集条件''(OSC)的技术条件ψ&amp;lt;sub&amp;gt;''i''&amp;lt;/sub&amp;gt;。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
There is a relatively compact open set ''V'' such that&lt;br /&gt;
&lt;br /&gt;
There is a relatively compact open set V such that&lt;br /&gt;
&lt;br /&gt;
有一个相对紧的开集''V''&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt; \bigcup_{i=1}^m\psi_i (V) \subseteq V, &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \bigcup_{i=1}^m\psi_i (V) \subseteq V, &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
where the sets in union on the left are pairwise [[disjoint sets|disjoint]].&lt;br /&gt;
&lt;br /&gt;
where the sets in union on the left are pairwise disjoint.&lt;br /&gt;
&lt;br /&gt;
左边的集合是成对不相交的。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The open set condition is a separation condition that ensures the images ψ&amp;lt;sub&amp;gt;''i''&amp;lt;/sub&amp;gt;(''V'') do not overlap &amp;quot;too much&amp;quot;.&lt;br /&gt;
&lt;br /&gt;
The open set condition is a separation condition that ensures the images ψ&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;(V) do not overlap &amp;quot;too much&amp;quot;.&lt;br /&gt;
&lt;br /&gt;
开集条件是保证图像子ψ&amp;lt;sub&amp;gt;''i''&amp;lt;/sub&amp;gt;(''V'') 不重叠“太多”的分离条件。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
'''Theorem'''. Suppose the open set condition holds and each ψ&amp;lt;sub&amp;gt;''i''&amp;lt;/sub&amp;gt; is a similitude, that is a composition of an [[isometry]] and a [[dilation (metric space)|dilation]] around some point. Then the unique fixed point of ψ is a set whose Hausdorff dimension is ''s'' where ''s'' is the unique solution of&amp;lt;ref&amp;gt;{{cite journal | last=Hutchinson | first=John E. | title=Fractals and self similarity | journal=Indiana Univ. Math. J. | volume=30 | year=1981 | pages=713–747 | doi=10.1512/iumj.1981.30.30055 | issue=5 | doi-access=free }}&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
Theorem. Suppose the open set condition holds and each ψ&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt; is a similitude, that is a composition of an isometry and a dilation around some point. Then the unique fixed point of ψ is a set whose Hausdorff dimension is s where s is the unique solution of&lt;br /&gt;
&lt;br /&gt;
'''定理'''假设开集条件成立，并且每个ψ&amp;lt;sub&amp;gt;''i''&amp;lt;/sub&amp;gt; 是一个相似量，这是一个等距和围绕某一点的膨胀的合成。那么唯一的不动点是一个集合，它的豪斯多夫维数是 ''s'' ，其中  ''s'' 是 ''s'' &amp;lt;ref&amp;gt;{{cite journal | last=Hutchinson | first=John E. | title=Fractals and self similarity | journal=Indiana Univ. Math. J. | volume=30 | year=1981 | pages=713–747 | doi=10.1512/iumj.1981.30.30055 | issue=5 | doi-access=free }}&amp;lt;/ref&amp;gt;的唯一解&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt; \sum_{i=1}^m r_i^s = 1. &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \sum_{i=1}^m r_i^s = 1. &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The contraction coefficient of a similitude is the magnitude of the dilation.&lt;br /&gt;
&lt;br /&gt;
The contraction coefficient of a similitude is the magnitude of the dilation.&lt;br /&gt;
&lt;br /&gt;
相似物的收缩系数就是膨胀的大小。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
We can use this theorem to compute the Hausdorff dimension of the Sierpinski triangle (or sometimes called Sierpinski gasket). Consider three [[non-collinear points]] ''a''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;, ''a''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;, ''a''&amp;lt;sub&amp;gt;3&amp;lt;/sub&amp;gt; in the plane '''R'''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; and let ψ&amp;lt;sub&amp;gt;''i''&amp;lt;/sub&amp;gt; be the dilation of ratio 1/2 around ''a&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;''. The unique non-empty fixed point of the corresponding mapping ψ is a Sierpinski gasket and the dimension ''s'' is the unique solution of&lt;br /&gt;
&lt;br /&gt;
We can use this theorem to compute the Hausdorff dimension of the Sierpinski triangle (or sometimes called Sierpinski gasket). Consider three non-collinear points a&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;, a&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;, a&amp;lt;sub&amp;gt;3&amp;lt;/sub&amp;gt; in the plane R&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; and let ψ&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt; be the dilation of ratio 1/2 around a&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;. The unique non-empty fixed point of the corresponding mapping ψ is a Sierpinski gasket and the dimension s is the unique solution of&lt;br /&gt;
&lt;br /&gt;
我们可以使用这个定理来计算谢尔宾斯基三角形的豪斯多夫维数(或者有时候叫做谢尔宾斯基垫圈)。考虑R&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; 平面上的三个非共线点，''a''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;，''a''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;，''a''&amp;lt;sub&amp;gt;3&amp;lt;/sub&amp;gt;，让ψ&amp;lt;sub&amp;gt;''i''&amp;lt;/sub&amp;gt;是围绕着''a&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;''膨胀比率的1/2。对应映射的唯一非空不动点是一个谢尔宾斯基垫圈，其维数''s''是对应映射的唯一解&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt; \left(\frac{1}{2}\right)^s+\left(\frac{1}{2}\right)^s+\left(\frac{1}{2}\right)^s = 3 \left(\frac{1}{2}\right)^s =1. &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \left(\frac{1}{2}\right)^s+\left(\frac{1}{2}\right)^s+\left(\frac{1}{2}\right)^s = 3 \left(\frac{1}{2}\right)^s =1. &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Taking [[natural logarithm]]s of both sides of the above equation, we can solve for ''s'', that is: ''s'' = ln(3)/ln(2).  The Sierpinski gasket is self-similar and satisfies the OSC. In general a set ''E'' which is a fixed point of a mapping&lt;br /&gt;
&lt;br /&gt;
Taking natural logarithms of both sides of the above equation, we can solve for s, that is: s = ln(3)/ln(2).  The Sierpinski gasket is self-similar and satisfies the OSC. In general a set E which is a fixed point of a mapping&lt;br /&gt;
&lt;br /&gt;
取上述方程两边的自然对数，我们可以求出 ''s''，即: ''s'' = ln(3)/ln(2)。该密封垫具有自相似性，满足 OSC 要求。一般来说，集合 ''E''是一个映射的不动点&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt; A \mapsto \psi(A) = \bigcup_{i=1}^m \psi_i(A) &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt; A \mapsto \psi(A) = \bigcup_{i=1}^m \psi_i(A) &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
is self-similar if and only if the intersections&lt;br /&gt;
&lt;br /&gt;
is self-similar if and only if the intersections&lt;br /&gt;
&lt;br /&gt;
是自相似的，当且仅当&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt; H^s\left(\psi_i(E) \cap \psi_j(E)\right) =0, &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; H^s\left(\psi_i(E) \cap \psi_j(E)\right) =0, &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
where ''s'' is the Hausdorff dimension of ''E'' and ''H&amp;lt;sup&amp;gt;s&amp;lt;/sup&amp;gt;'' denotes [[Hausdorff measure]]. This is clear in the case of the Sierpinski gasket (the intersections are just points), but is also true more generally:&lt;br /&gt;
&lt;br /&gt;
where s is the Hausdorff dimension of E and H&amp;lt;sup&amp;gt;s&amp;lt;/sup&amp;gt; denotes Hausdorff measure. This is clear in the case of the Sierpinski gasket (the intersections are just points), but is also true more generally:&lt;br /&gt;
&lt;br /&gt;
其中 ''s''是''E''的豪斯多夫维数， ''E'' and ''H&amp;lt;sup&amp;gt;s&amp;lt;/sup&amp;gt;'' 表示 豪斯多夫测度。对于谢尔宾斯基垫圈(交叉点就是点)来说，这一点很明显，但更普遍的情况是:&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
'''Theorem'''. Under the same conditions as the previous theorem, the unique fixed point of ψ is self-similar.&lt;br /&gt;
&lt;br /&gt;
Theorem. Under the same conditions as the previous theorem, the unique fixed point of ψ is self-similar.&lt;br /&gt;
&lt;br /&gt;
'''定理'''：在与前一定理相同的条件下，其唯一不动点是自相似的。&lt;br /&gt;
&lt;br /&gt;
==See also参阅==&lt;br /&gt;
&lt;br /&gt;
* [[List of fractals by Hausdorff dimension豪斯多夫分形维数列表]] Examples of deterministic fractals, random and natural fractals.确定性分形与随机和自然分形的示例。&lt;br /&gt;
&lt;br /&gt;
* [[Assouad dimension  Assouad维数]], another variation of fractal dimension that, like Hausdorff dimension, is defined using coverings by balls其他被球覆盖方式定义的分形维数，例如豪斯多夫维数。&lt;br /&gt;
&lt;br /&gt;
* [[Intrinsic dimension固有维数]]&lt;br /&gt;
&lt;br /&gt;
* [[Packing dimension填充维数]]&lt;br /&gt;
&lt;br /&gt;
* [[Fractal dimension分形维数]]&lt;br /&gt;
&lt;br /&gt;
==References参考文献==&lt;br /&gt;
&lt;br /&gt;
{{reflist}}&lt;br /&gt;
&lt;br /&gt;
==Further reading拓展阅读==&lt;br /&gt;
&lt;br /&gt;
* {{cite book |last1=Dodson |first1=M. Maurice |title=Fractal Geometry and Applications: A Jubilee of Benoît Mandelbrot |volume=72 |issue=1 |pages=305–347 |last2=Kristensen |first2=Simon |chapter=Hausdorff Dimension and Diophantine Approximation |date=June 12, 2003 |arxiv=math/0305399 |bibcode = 2003math......5399D |doi=10.1090/pspum/072.1/2112110|series=Proceedings of Symposia in Pure Mathematics |isbn=9780821836378 }}&lt;br /&gt;
&lt;br /&gt;
* {{cite book |last1=Hurewicz |first1=Witold |authorlink1=Witold Hurewicz |last2=Wallman |first2=Henry |authorlink2=Henry Wallman |title=Dimension Theory |url=https://archive.org/details/in.ernet.dli.2015.84609 |publisher=Princeton University Press |year=1948 }}&lt;br /&gt;
&lt;br /&gt;
* {{cite journal |author作者=E. Szpilrajn |authorlink=Edward Marczewski |title=La dimension et la mesure |journal=Fundamenta Mathematicae |volume=28 |pages=81–9 |year=1937 }}&lt;br /&gt;
&lt;br /&gt;
* {{cite journal&lt;br /&gt;
&lt;br /&gt;
 | last1=Marstrand&lt;br /&gt;
&lt;br /&gt;
 | last1=Marstrand&lt;br /&gt;
&lt;br /&gt;
 | last1=马斯特兰德&lt;br /&gt;
&lt;br /&gt;
 | first1=J. M. | title=The dimension of cartesian product sets | year=1954 | journal=Proc. Cambridge Philos. Soc.&lt;br /&gt;
&lt;br /&gt;
 | first1=J. M. | title=The dimension of cartesian product sets | year=1954 | journal=Proc. Cambridge Philos. Soc.&lt;br /&gt;
&lt;br /&gt;
 | first1= J. M. | title=笛卡儿积集的维数 | 1954年 |  journal=Proc. Cambridge Philos. Soc.&lt;br /&gt;
&lt;br /&gt;
 | volume=50&lt;br /&gt;
&lt;br /&gt;
 | volume=50&lt;br /&gt;
&lt;br /&gt;
 | 第50卷&lt;br /&gt;
&lt;br /&gt;
 | issue=3&lt;br /&gt;
&lt;br /&gt;
 | issue=3&lt;br /&gt;
&lt;br /&gt;
 | 第三期&lt;br /&gt;
&lt;br /&gt;
 | pages=198–202&lt;br /&gt;
&lt;br /&gt;
 | pages=198–202&lt;br /&gt;
&lt;br /&gt;
 | 第198-202页&lt;br /&gt;
&lt;br /&gt;
 | doi=10.1017/S0305004100029236|bibcode = 1954PCPS...50..198M }}&lt;br /&gt;
&lt;br /&gt;
 | doi=10.1017/S0305004100029236|bibcode = 1954PCPS...50..198M }}&lt;br /&gt;
&lt;br /&gt;
10.1017 / S0305004100029236 | bibcode 1954PCPS... 50. . 198 m }&lt;br /&gt;
&lt;br /&gt;
* {{Cite book&lt;br /&gt;
&lt;br /&gt;
 | last1=Mattila&lt;br /&gt;
&lt;br /&gt;
 | last1=Mattila&lt;br /&gt;
&lt;br /&gt;
 | last1=Mattila&lt;br /&gt;
&lt;br /&gt;
 | first1=Pertti | author1-link=Pertti Mattila| title=Geometry of sets and measures in Euclidean spaces | publisher=[[Cambridge University Press]]&lt;br /&gt;
&lt;br /&gt;
 | first1=Pertti | author1-link=Pertti Mattila| title=Geometry of sets and measures in Euclidean spaces | publisher=Cambridge University Press&lt;br /&gt;
&lt;br /&gt;
| first1 Pertti | author1-link Pertti Mattila | title 欧几里德空间中集合和度量的几何 | 出版商剑桥大学出版社&lt;br /&gt;
&lt;br /&gt;
 | isbn=978-0-521-65595-8 | year=1995}}&lt;br /&gt;
&lt;br /&gt;
 | isbn=978-0-521-65595-8 | year=1995}}&lt;br /&gt;
&lt;br /&gt;
| isbn 978-0-521-65595-8 | year 1995}&lt;br /&gt;
&lt;br /&gt;
* {{cite journal |author=A. S. Besicovitch |authorlink=A. S. Besicovitch |title=On Linear Sets of Points of Fractional Dimensions |journal=[[Mathematische Annalen]] |volume=101 |year=1929 | doi=10.1007/BF01454831| issue=1 |pages= 161–193}}&lt;br /&gt;
&lt;br /&gt;
* {{cite journal |author1=A. S. Besicovitch |authorlink1=A. S. Besicovitch |author2=H. D. Ursell |authorlink2=H. D. Ursell |title=Sets of Fractional Dimensions |journal=Journal of the London Mathematical Society |volume=12 |year=1937 | issue=1 | doi=10.1112/jlms/s1-12.45.18  | pages=18–25 }}&amp;lt;br/&amp;gt;Several selections from this volume are reprinted in {{cite book |author=Edgar, Gerald A. |title=Classics on fractals |publisher=Addison-Wesley |location=Boston |year=1993 |isbn=0-201-58701-7}} See chapters 9,10,11&lt;br /&gt;
&lt;br /&gt;
* {{cite journal |author=F. Hausdorff |authorlink=F. Hausdorff |title=Dimension und äußeres Maß |journal=Mathematische Annalen |volume=79 |issue=1–2 |pages=157–179 |date=March 1919 |doi=10.1007/BF01457179|hdl=10338.dmlcz/100363 |url=http://dml.cz/bitstream/handle/10338.dmlcz/100363/CzechMathJ_09-1959-3_5.pdf }}&lt;br /&gt;
&lt;br /&gt;
* {{cite journal | last=Hutchinson | first=John E. | title=Fractals and self similarity | journal=Indiana Univ. Math. J. | volume=30 | year=1981 | pages=713–747 | doi=10.1512/iumj.1981.30.30055 | issue=5 | doi-access=free }}&lt;br /&gt;
&lt;br /&gt;
*{{cite book | last=Falconer | first = Kenneth |title=Fractal Geometry: Mathematical Foundations and Applications | publisher=[[John Wiley and Sons]] | edition=2nd | year=2003}}&lt;br /&gt;
&lt;br /&gt;
==External links外部链接==&lt;br /&gt;
&lt;br /&gt;
* [https://www.encyclopediaofmath.org/index.php/Hausdorff_dimension Hausdorff dimension] 在 [https://www.encyclopediaofmath.org/ Encyclopedia of Mathematics]&lt;br /&gt;
&lt;br /&gt;
* [https://www.encyclopediaofmath.org/index.php/Hausdorff_measure Hausdorff measure] 在 [https://www.encyclopediaofmath.org/ Encyclopedia of Mathematics]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{{DEFAULTSORT:Hausdorff Dimension豪斯多夫维数}}&lt;br /&gt;
&lt;br /&gt;
[[Category分类:Fractals分形]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[Category分类:Metric geometry度量几何]]&lt;br /&gt;
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&lt;br /&gt;
&lt;br /&gt;
[[Category分类:Dimension theory维度理论]]&lt;br /&gt;
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&lt;br /&gt;
&amp;lt;noinclude&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;small&amp;gt;This page was moved from [[wikipedia:en:Hausdorff dimension]]. Its edit history can be viewed at [[分形维数/edithistory]]&amp;lt;/small&amp;gt;&amp;lt;/noinclude&amp;gt;&lt;br /&gt;
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[[Category:待整理页面]]&lt;/div&gt;</summary>
		<author><name>Ruili</name></author>
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		<title>分形维数</title>
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		<updated>2020-10-27T16:05:37Z</updated>

		<summary type="html">&lt;p&gt;Ruili：&lt;/p&gt;
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&lt;div&gt;此词条暂由彩云小译翻译，未经人工整理和审校，带来阅读不便，请见谅。&lt;br /&gt;
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Example of non-integer dimensions. The first four [[iteration]]s of the [[Koch snowflake|Koch curve]], where after each iteration, all original line segments are replaced with four, each a self-similar copy that is 1/3 the length of the original. One formalism of the Hausdorff dimension uses this scale factor (3) and the number of self-similar objects (4) to calculate the dimension, D, after the first iteration to be D = (log N)/(log S) = (log 4)/(log 3) ≈ 1.26.&amp;lt;ref name=CampbellAnnenberg15&amp;gt;MacGregor Campbell, 2013, &amp;quot;5.6 Scaling and the Hausdorff Dimension,&amp;quot; at ''Annenberg Learner:MATHematics illuminated'', see [http://www.learner.org/courses/mathilluminated/units/5/textbook/06.php], accessed 5 March 2015.&amp;lt;/ref&amp;gt; That is, while the Hausdorff dimension of a single [[point (geometry)|point]] is zero, of a [[line segment]] is 1, of a [[square]] is 2, and of a [[cube]] is 3, for [[fractal]]s such as this, the object can have a non-integer dimension.&lt;br /&gt;
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Example of non-integer dimensions. The first four iterations of the Koch curve, where after each iteration, all original line segments are replaced with four, each a self-similar copy that is 1/3 the length of the original. One formalism of the Hausdorff dimension uses this scale factor (3) and the number of self-similar objects (4) to calculate the dimension, D, after the first iteration to be D = (log N)/(log S) = (log 4)/(log 3) ≈ 1.26. That is, while the Hausdorff dimension of a single point is zero, of a line segment is 1, of a square is 2, and of a cube is 3, for fractals such as this, the object can have a non-integer dimension.&lt;br /&gt;
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非整数维度示例：前四个[[Koch 曲线]]的迭代，在每次迭代后，所有原始线段都被替换为四个，每个自相似的复制是原始线段长度的1 / 3。豪斯多夫维数的一个建模是使用这个比例因子(3)和自相似物体的数量(4)来计算维度，设在第一次迭代后为 D = (log N)/(log S) = (log 4)/(log 3) ≈ 1.26.&amp;lt;ref name=CampbellAnnenberg15&amp;gt;。MacGregor Campbell, 2013, &amp;quot;5.6 Scaling and the Hausdorff Dimension,&amp;quot; 在 ''Annenberg Learner:MATHematics illuminated'', 参见 [http://www.learner.org/courses/mathilluminated/units/5/textbook/06.php], accessed 5 March 2015.&amp;lt;/ref&amp;gt; 也就是说，当一个点的豪斯多夫维数为零，线段为1，正方形为2，立方体为3时，对于像这样的分形，物体可以有一个非整数维度。&lt;br /&gt;
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In [[mathematics]], '''Hausdorff dimension''' is a measure of ''roughness'', or more specifically, [[fractal dimension]], that was first introduced in 1918 by [[mathematician]] [[Felix Hausdorff]].&amp;lt;ref&amp;gt;{{Cite journal |arxiv = 1101.1444|doi = 10.1214/11-STS370|title = Estimators of Fractal Dimension: Assessing the Roughness of Time Series and Spatial Data|journal = Statistical Science|volume = 27|issue = 2|pages = 247–277|year = 2012|last1 = Gneiting|first1 = Tilmann|last2 = Ševčíková|first2 = Hana|last3 = Percival|first3 = Donald B.}}&amp;lt;/ref&amp;gt; For instance, the Hausdorff dimension of a single [[point (geometry)|point]] is zero, of a [[line segment]] is 1, of a [[square]] is 2, and of a [[cube]] is 3. That is, for sets of points that define a smooth shape or a shape that has a small number of corners—the shapes of traditional geometry and science—the Hausdorff dimension is an [[integer]] agreeing with the usual sense of dimension, also known as the [[Inductive dimension|topological dimension]]. However, formulas have also been developed that allow calculation of the dimension of other less simple objects, where, solely on the basis of their properties of [[scaling (geometry)|scaling]] and [[self-similarity]], one is led to the conclusion that particular objects—including [[fractal]]s—have non-integer Hausdorff dimensions. Because of the significant technical advances made by [[Abram Samoilovitch Besicovitch]] allowing computation of dimensions for highly irregular or &amp;quot;rough&amp;quot; sets, this dimension is also commonly referred to as the ''Hausdorff–Besicovitch dimension.''&lt;br /&gt;
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In mathematics, Hausdorff dimension is a measure of roughness, or more specifically, fractal dimension, that was first introduced in 1918 by mathematician Felix Hausdorff. For instance, the Hausdorff dimension of a single point is zero, of a line segment is 1, of a square is 2, and of a cube is 3. That is, for sets of points that define a smooth shape or a shape that has a small number of corners—the shapes of traditional geometry and science—the Hausdorff dimension is an integer agreeing with the usual sense of dimension, also known as the topological dimension. However, formulas have also been developed that allow calculation of the dimension of other less simple objects, where, solely on the basis of their properties of scaling and self-similarity, one is led to the conclusion that particular objects—including fractals—have non-integer Hausdorff dimensions. Because of the significant technical advances made by Abram Samoilovitch Besicovitch allowing computation of dimensions for highly irregular or &amp;quot;rough&amp;quot; sets, this dimension is also commonly referred to as the Hausdorff–Besicovitch dimension.&lt;br /&gt;
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在[[数学]]中，'''&amp;lt;font color = '#ff8000'&amp;gt;豪斯多夫维数Hausdorff dimension&amp;lt;/font&amp;gt;'''是一种粗糙度的度量单位，或者更确切地说，分形维数，是由数学家 Felix Hausdorff 在1918年首次提出的。例如，单点的豪斯多夫维数为零，线段为1，正方形为2，立方体为3。也就是说，对于定义了一个光滑形状或一个有少数几个角的形状---- 传统几何学和科学的形状---- 的点集来说，豪斯多夫维数是一个整数，符合通常的维度意义，也称为拓扑维度。然而，还有一些公式允许计算其他不太简单的对象的维数，其中仅仅根据它们的标度和自相似特性，就可以得出结论: 特定的对象ー包括分形ー具有非整数的 Hausdorff 维数。由于阿布拉姆·萨莫伊洛维奇·贝西科维奇的重大技术进步，允许计算高度不规则或“粗糙”集的维度，这个维度通常也被称为 Hausdorff-Besicovitch 维度。 &lt;br /&gt;
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The Hausdorff dimension, more specifically, is a further dimensional number associated with a given set, where the distances between all members of that set are defined. Such a set is termed a [[metric space]]. The dimension is drawn from the [[Extended real number line|extended real numbers]], &amp;lt;math&amp;gt;\overline{\mathbb{R}}&amp;lt;/math&amp;gt;, as opposed to the more intuitive notion of dimension, which is not associated to general metric spaces, and only takes values in the non-negative integers.&lt;br /&gt;
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The Hausdorff dimension, more specifically, is a further dimensional number associated with a given set, where the distances between all members of that set are defined. Such a set is termed a metric space. The dimension is drawn from the extended real numbers, &amp;lt;math&amp;gt;\overline{\mathbb{R}}&amp;lt;/math&amp;gt;, as opposed to the more intuitive notion of dimension, which is not associated to general metric spaces, and only takes values in the non-negative integers.&lt;br /&gt;
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更具体地说，豪斯多夫维数是一个与给定集合相关联的更进一步的维数，其中定义了该集合所有成员之间的距离。这样的集合称为度量空间。维数是从扩展的实数，&amp;lt;math&amp;gt;\overline{\mathbb{R}}&amp;lt;/math&amp;gt;，而不是更直观的维数概念(它不与一般的度量空间相关联，只取非负整数的值)。&lt;br /&gt;
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In mathematical terms, the Hausdorff dimension generalizes the notion of the dimension of a real [[vector space]]. That is, the Hausdorff dimension of an ''n''-dimensional [[inner product space]] equals ''n''. This underlies the earlier statement that the Hausdorff dimension of a point is zero, of a line is one, etc., and that [[fractal|irregular sets]] can have noninteger Hausdorff dimensions. For instance, the [[Koch snowflake]] shown at right is constructed from an equilateral triangle; in each iteration, its component line segments are divided into 3 segments of unit length, the newly created middle segment is used as the base of a new [[equilateral]] triangle that points outward, and this base segment is then deleted to leave a final object from the iteration of unit length of 4.&amp;lt;ref&amp;gt;Larry Riddle, 2014, &amp;quot;Classic Iterated Function Systems: Koch Snowflake&amp;quot;, Agnes Scott College e-Academy (online), see [http://ecademy.agnesscott.edu/~lriddle/ifs/ksnow/ksnow.htm], accessed 5 March 2015.&amp;lt;/ref&amp;gt; That is, after the first iteration, each original line segment has been replaced with N=4, where each self-similar copy is 1/S = 1/3 as long as the original.&amp;lt;ref name=CampbellAnnenberg15/&amp;gt; Stated another way, we have taken an object with Euclidean dimension, D, and reduced its linear scale by 1/3 in each direction, so that its length increases to N=S&amp;lt;sup&amp;gt;D&amp;lt;/sup&amp;gt;.&amp;lt;ref name=ClaytonSCTPLS96&amp;gt;Keith Clayton, 1996, &amp;quot;Fractals and the Fractal Dimension,&amp;quot; ''Basic Concepts in Nonlinear Dynamics and Chaos'' (workshop), Society for Chaos Theory in Psychology and the Life Sciences annual meeting, June 28, 1996, Berkeley, California, see [http://www.vanderbilt.edu/AnS/psychology/cogsci/chaos/workshop/Workshop.html], accessed 5 March 2015.&amp;lt;/ref&amp;gt; This equation is easily solved for D, yielding the ratio of logarithms (or [[natural logarithm]]s) appearing in the figures, and giving—in the Koch and other fractal cases—non-integer dimensions for these objects.&lt;br /&gt;
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In mathematical terms, the Hausdorff dimension generalizes the notion of the dimension of a real vector space. That is, the Hausdorff dimension of an n-dimensional inner product space equals n. This underlies the earlier statement that the Hausdorff dimension of a point is zero, of a line is one, etc., and that irregular sets can have noninteger Hausdorff dimensions. For instance, the Koch snowflake shown at right is constructed from an equilateral triangle; in each iteration, its component line segments are divided into 3 segments of unit length, the newly created middle segment is used as the base of a new equilateral triangle that points outward, and this base segment is then deleted to leave a final object from the iteration of unit length of 4. That is, after the first iteration, each original line segment has been replaced with N=4, where each self-similar copy is 1/S = 1/3 as long as the original. This equation is easily solved for D, yielding the ratio of logarithms (or natural logarithms) appearing in the figures, and giving—in the Koch and other fractal cases—non-integer dimensions for these objects.&lt;br /&gt;
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用数学术语来说，豪斯多夫维数概括了实向量空间维数的概念。也就是说，n 维内积空间的豪斯多夫维数等于 n。 这就是早期假设的基础，一个点的豪斯多夫维数是零，一条线是一等等，不规则集可以有非整数的豪斯多夫维数。例如，右边所示的 Koch 雪花是由一个正三角形构成的; 在每次迭代中，它的组成线段被分成单位长度的3段，新创建的中间线段被用作一个指向外部的新正三角形的基础，然后人们删除这个基础线段用来保留单位长度4的迭代中的最终对象。也就是说，在第一次迭代之后，每个原始线段都被替换为 N=4，其中每个自相似拷贝的长度是原始线段的1/S = 1/3 。这个方程很容易求解为 D，产生出现在图形中的对数(或自然对数)的比率，并给出——在 Koch 和其他分形情况下——这些对象的非整数维数。&lt;br /&gt;
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The Hausdorff dimension is a successor to the simpler, but usually equivalent, box-counting or [[Minkowski–Bouligand dimension]].&lt;br /&gt;
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The Hausdorff dimension is a successor to the simpler, but usually equivalent, box-counting or Minkowski–Bouligand dimension.&lt;br /&gt;
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豪斯多夫维数是更简单但通常等价的'''&amp;lt;font color = '#ff8000'&amp;gt;计盒维数box-counting&amp;lt;/font&amp;gt;'''或'''&amp;lt;font color = '#ff8000'&amp;gt;闵可夫斯基维数Minkowski-Bouligand&amp;lt;/font&amp;gt;'''的继承者。&lt;br /&gt;
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==Intuition概念==&lt;br /&gt;
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The intuitive concept of dimension of a geometric object ''X'' is the number of independent parameters one needs to pick out a unique point inside. However, any point specified by two parameters can be instead specified by one, because the [[cardinality]] of the [[real plane]] is equal to the cardinality of the [[real line]] (this can be seen by an [[Cantor's diagonal argument|argument]] involving interweaving the digits of two numbers to yield a single number encoding the same information). The example of a [[space-filling curve]] shows that one can even map the real line to the real plane [[Surjective function|surjectively]] (taking one real number into a pair of real numbers in a way so that all pairs of numbers are covered) and ''continuously'', so that a one-dimensional object completely fills up a higher-dimensional object.&lt;br /&gt;
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The intuitive concept of dimension of a geometric object X is the number of independent parameters one needs to pick out a unique point inside. However, any point specified by two parameters can be instead specified by one, because the cardinality of the real plane is equal to the cardinality of the real line (this can be seen by an argument involving interweaving the digits of two numbers to yield a single number encoding the same information). The example of a space-filling curve shows that one can even map the real line to the real plane surjectively (taking one real number into a pair of real numbers in a way so that all pairs of numbers are covered) and continuously, so that a one-dimensional object completely fills up a higher-dimensional object.&lt;br /&gt;
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几何物体X的直观尺寸概念就是一个物体需要多少个独立参数才能找到一个独特的点。但是，任何由两个参数指定的点都可以由一个参数指定，因为实际平面的基数等于实际行的基数(这可以通过一个参数看到，该参数涉及交织两个数字的数字以产生一个编码相同信息的单个数字)。'''&amp;lt;font color = '#ff8000'&amp;gt;皮亚诺曲线&amp;lt;/font&amp;gt;'''的例子表明，一个人甚至可以完美和连续地映射实际线到真正的平面(把一个实数转换成一对实数，这样所有的数对都被覆盖)，由此一维物体完全填充了一个高维物体。&lt;br /&gt;
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Every space filling curve hits some points multiple times, and does not have a continuous inverse. It is impossible to map two dimensions onto one in a way that is continuous and continuously invertible. The topological dimension, also called [[Lebesgue covering dimension]], explains why. This dimension is ''n'' if, in every covering of ''X'' by small open balls, there is at least one point where ''n''&amp;amp;nbsp;+&amp;amp;nbsp;1 balls overlap. For example, when one covers a line with short open intervals, some points must be covered twice, giving dimension&amp;amp;nbsp;''n''&amp;amp;nbsp;=&amp;amp;nbsp;1.&lt;br /&gt;
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Every space filling curve hits some points multiple times, and does not have a continuous inverse. It is impossible to map two dimensions onto one in a way that is continuous and continuously invertible. The topological dimension, also called Lebesgue covering dimension, explains why. This dimension is n if, in every covering of X by small open balls, there is at least one point where n&amp;amp;nbsp;+&amp;amp;nbsp;1 balls overlap. For example, when one covers a line with short open intervals, some points must be covered twice, giving dimension&amp;amp;nbsp;n&amp;amp;nbsp;=&amp;amp;nbsp;1.&lt;br /&gt;
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每条空间填充曲线都会多次撞击某些点，且不存在连续的倒数。将两个维度以连续和连续可逆的方式映射到一个维度是不可能的。'''&amp;lt;font color = '#ff8000'&amp;gt;拓扑维度 topological dimension&amp;lt;/font&amp;gt;'''，也被称为拓朴维数，解释了为什么。这个维度是 n，如果在 x 的每个小开球覆盖中，至少有一个点 n + 1个球重叠。例如，当一个点覆盖一条具有短开区间的直线时，某些点必须被覆盖两次，给出维数''n''&amp;amp;nbsp;=&amp;amp;nbsp;1。&lt;br /&gt;
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But topological dimension is a very crude measure of the local size of a space (size near a point). A curve that is almost space-filling can still have topological dimension one, even if it fills up most of the area of a region. A [[fractal]] has an integer topological dimension, but in terms of the amount of space it takes up, it behaves like a higher-dimensional space.&lt;br /&gt;
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But topological dimension is a very crude measure of the local size of a space (size near a point). A curve that is almost space-filling can still have topological dimension one, even if it fills up most of the area of a region. A fractal has an integer topological dimension, but in terms of the amount of space it takes up, it behaves like a higher-dimensional space.&lt;br /&gt;
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但是，拓扑维度是对空间局部尺寸(点附近的尺寸)的一个非常粗略的度量。一条几乎是空间填充的曲线仍然可以有一维拓扑，即使它填充了一个区域的大部分面积。分形具有整数的拓扑维数，但就其所占空间的数量而言，它看起来像一个更高维的空间。&lt;br /&gt;
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The Hausdorff dimension measures the local size of a space taking into account the distance between points, the [[metric space|metric]]. Consider the number ''N''(''r'') of [[ball (mathematics)|balls]] of radius at most ''r'' required to cover ''X'' completely. When ''r'' is very small, ''N''(''r'') grows polynomially with 1/''r''. For a sufficiently well-behaved  ''X'', the Hausdorff dimension is the unique number ''d'' such that N(''r'') grows as 1/''r&amp;lt;sup&amp;gt;d&amp;lt;/sup&amp;gt;'' as ''r'' approaches zero. More precisely, this defines the [[Minkowski–Bouligand dimension|box-counting dimension]], which equals the Hausdorff dimension when the value ''d'' is a critical boundary between growth rates that are insufficient to cover the space, and growth rates that are overabundant.&lt;br /&gt;
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The Hausdorff dimension measures the local size of a space taking into account the distance between points, the metric. Consider the number N(r) of balls of radius at most r required to cover X completely. When r is very small, N(r) grows polynomially with 1/r. For a sufficiently well-behaved  X, the Hausdorff dimension is the unique number d such that N(r) grows as 1/r&amp;lt;sup&amp;gt;d&amp;lt;/sup&amp;gt; as r approaches zero. More precisely, this defines the box-counting dimension, which equals the Hausdorff dimension when the value d is a critical boundary between growth rates that are insufficient to cover the space, and growth rates that are overabundant.&lt;br /&gt;
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豪斯多夫维数测量一个空间的局部大小时，会考虑到点之间距离的度量。考虑半径最大为 r 的球数 ''N'' (r) ，需要完全覆盖 ''X''。当 r 很小时，n (r)以1/''r'' 增长多项式。对于一个表现足够好的 ''X''，豪斯多夫维数是唯一的数 d，这样当 r 趋近于零时， N(r)增长为1/r&amp;lt;sup&amp;gt;d&amp;lt;/sup&amp;gt; 。更确切地说，这定义了盒子计数维度，当值 d 是不足以覆盖空间的增长率和过度充裕的增长率之间的关键边界时，它等于豪斯多夫维数。&lt;br /&gt;
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For shapes that are smooth, or shapes with a small number of corners, the shapes of traditional geometry and science, the Hausdorff dimension is an integer agreeing with the topological dimension. But [[Benoit Mandelbrot]] observed that [[fractal]]s, sets with noninteger Hausdorff dimensions, are found everywhere in nature. He observed that the proper idealization of most rough shapes you see around you is not in terms of smooth idealized shapes, but in terms of fractal idealized shapes:&lt;br /&gt;
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For shapes that are smooth, or shapes with a small number of corners, the shapes of traditional geometry and science, the Hausdorff dimension is an integer agreeing with the topological dimension. But Benoit Mandelbrot observed that fractals, sets with noninteger Hausdorff dimensions, are found everywhere in nature. He observed that the proper idealization of most rough shapes you see around you is not in terms of smooth idealized shapes, but in terms of fractal idealized shapes:&lt;br /&gt;
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对于光滑的形状，或者有少量棱角的形状，传统几何和科学的形状，豪斯多夫维数是一个整数，与拓扑维度一致。但是伯努·曼德布洛特观察到分形---- 具有非整数豪斯多夫维数的集合---- 在自然界中随处可见。他观察到，我们周围大多数粗糙形状的理想化不是光滑的理想化形状，而是分形理想化形状:&lt;br /&gt;
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&amp;lt;blockquote&amp;gt;Clouds are not spheres, mountains are not cones, coastlines are not circles, and bark is not smooth, nor does lightning travel in a straight line.&amp;lt;ref name=&amp;quot;mandelbrot&amp;quot;&amp;gt;{{cite book   | last = Mandelbrot   | first = Benoît   | authorlink = Benoit Mandelbrot   | title = The Fractal Geometry of Nature   | publisher = W. H. Freeman   | series = Lecture notes in mathematics 1358   | year = 1982   | doi =    | isbn = 0-7167-1186-9   | url-access = registration   | url = https://archive.org/details/fractalgeometryo00beno   }}&amp;lt;/ref&amp;gt;&amp;lt;/blockquote&amp;gt;&lt;br /&gt;
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&amp;lt;blockquote&amp;gt;Clouds are not spheres, mountains are not cones, coastlines are not circles, and bark is not smooth, nor does lightning travel in a straight line.&amp;lt;/blockquote&amp;gt;&lt;br /&gt;
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&amp;lt;blockquote&amp;gt;云不是球体，山不是锥体，海岸线不是圆圈，树皮不平滑，闪电也不是直线运动。 &amp;lt;/blockquote&amp;gt;&lt;br /&gt;
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For fractals that occur in nature, the Hausdorff and [[Minkowski–Bouligand dimension|box-counting dimension]] coincide. The [[packing dimension]] is yet another similar notion which gives the same value for many shapes, but there are well documented exceptions where all these dimensions differ.&lt;br /&gt;
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For fractals that occur in nature, the Hausdorff and box-counting dimension coincide. The packing dimension is yet another similar notion which gives the same value for many shapes, but there are well documented exceptions where all these dimensions differ.&lt;br /&gt;
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对于自然界中出现的分形，豪斯多夫维数和盒计数维数是一致的。封装尺寸是另一个类似的概念，它给出了许多形状相同的值，但是在所有这些尺寸不同的情况，都做了很好的说明。&lt;br /&gt;
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==Formal definitions形式化定义==&lt;br /&gt;
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===Hausdorff content豪斯多夫集===&lt;br /&gt;
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Let ''X'' be a [[metric space]]. If ''S'' ⊂ ''X'' and ''d'' ∈ [0, ∞), the ''d''-dimensional '''unlimited Hausdorff content''' of ''S'' is defined by&lt;br /&gt;
&lt;br /&gt;
Let X be a metric space. If S ⊂ X and d ∈ [0, ∞), the d-dimensional unlimited Hausdorff content of S is defined by&lt;br /&gt;
&lt;br /&gt;
设 ''X''是度量空间。若''S'' ⊂ ''X'' 和 ''d'' ∈ [0, ∞) ，则 ''S'' 的''d''维无限 豪斯多夫集定义为&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt;C_H^d(S):=\inf\Bigl\{\sum_i r_i^d:\text{ there is a cover of } S\text{ by balls with radii }r_i&amp;gt;0\Bigr\}.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt;C_H^d(S):=\inf\Bigl\{\sum_i r_i^d:\text{ there is a cover of } S\text{ by balls with radii }r_i&amp;gt;0\Bigr\}.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt;C_H^d(S):=\inf\Bigl\{\sum_i r_i^d:\text{ there is a cover of } S\text{ by balls with radii }r_i&amp;gt;0\Bigr\}.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
In other words, &amp;lt;math&amp;gt;C_H^d(S)&amp;lt;/math&amp;gt; is the [[infimum]] of the set of numbers &amp;lt;math&amp;gt;\delta \geq 0&amp;lt;/math&amp;gt; such that there is some (indexed) collection of [[ball (mathematics)|ball]]s &amp;lt;math&amp;gt;\{B(x_i,r_i):i\in I\}&amp;lt;/math&amp;gt; covering ''S'' with ''r&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;''&amp;amp;nbsp;&amp;gt;&amp;amp;nbsp;0 for each ''i''&amp;amp;nbsp;∈&amp;amp;nbsp;''I'' that satisfies &amp;lt;math&amp;gt;\sum_{i\in I} r_i^d&amp;lt;\delta &amp;lt;/math&amp;gt;. (Here, we use the standard convention that [[infimum|inf&amp;amp;nbsp;Ø&amp;amp;nbsp;=&amp;amp;nbsp;∞]].)&lt;br /&gt;
&lt;br /&gt;
In other words, &amp;lt;math&amp;gt;C_H^d(S)&amp;lt;/math&amp;gt; is the infimum of the set of numbers &amp;lt;math&amp;gt;\delta \geq 0&amp;lt;/math&amp;gt; such that there is some (indexed) collection of balls &amp;lt;math&amp;gt;\{B(x_i,r_i):i\in I\}&amp;lt;/math&amp;gt; covering S with r&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;&amp;amp;nbsp;&amp;gt;&amp;amp;nbsp;0 for each i&amp;amp;nbsp;∈&amp;amp;nbsp;I that satisfies &amp;lt;math&amp;gt;\sum_{i\in I} r_i^d&amp;lt;\delta &amp;lt;/math&amp;gt;. (Here, we use the standard convention that inf&amp;amp;nbsp;Ø&amp;amp;nbsp;=&amp;amp;nbsp;∞.)&lt;br /&gt;
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换句话说，&amp;lt;math&amp;gt;C_H^d(S)&amp;lt;/math&amp;gt; 是数字集合&amp;lt;math&amp;gt;\delta \geq 0&amp;lt;/math&amp;gt;的下确界，使得在 ''i''&amp;amp;nbsp;∈&amp;amp;nbsp中存在一些球集合 &amp;lt;math&amp;gt;\{B(x_i,r_i):i\in I\}&amp;lt;/math&amp;gt;  i 包含 s，对于每个 ''r&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;''&amp;amp;nbsp;&amp;gt;&amp;amp;nbsp;0 满足 i 中的和&amp;lt;math&amp;gt;\sum_{i\in I} r_i^d&amp;lt;\delta &amp;lt;/math&amp;gt; (在这里，我们使用inf&amp;amp;nbsp;Ø&amp;amp;nbsp;=&amp;amp;nbsp;∞ )的标准约定。&lt;br /&gt;
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===Hausdorff measurement豪斯多夫分形测量===&lt;br /&gt;
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The Hausdorff outer measure is different from the unbounded Hausdorf content in that rather than considering all possible coverings of ''S'', we see what happens when the sizes of the balls go to zero. This is  for &amp;lt;math&amp;gt;d \geq 0 &amp;lt;/math&amp;gt;, we define the ''d''-dimensional Hausdorff outer measure of ''S'' as&lt;br /&gt;
&lt;br /&gt;
The Hausdorff outer measure is different from the unbounded Hausdorf content in that rather than considering all possible coverings of S, we see what happens when the sizes of the balls go to zero. This is  for &amp;lt;math&amp;gt;d \geq 0 &amp;lt;/math&amp;gt;, we define the d-dimensional Hausdorff outer measure of S as&lt;br /&gt;
&lt;br /&gt;
豪斯多夫外测度不同于无界的豪斯多夫，因为我们不考虑 s 的所有可能，我们看到当球的大小为零时会发生什么。这是为了数学  &amp;lt;math&amp;gt;d \geq 0 &amp;lt;/math&amp;gt;，我们定义了  ''S''的 ''d''维豪斯多夫Hausdorff 外测度为&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt; \mathcal{H}^d(S):=\lim_{r \to 0} \inf\Bigl\{\sum_i r_i^d:\text{ there is a cover of } S\text{ by balls with radii } 0 &amp;lt; r_i &amp;lt; r\Bigr\}.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \mathcal{H}^d(S):=\lim_{r \to 0} \inf\Bigl\{\sum_i r_i^d:\text{ there is a cover of } S\text{ by balls with radii } 0 &amp;lt; r_i &amp;lt; r\Bigr\}.&amp;lt;/math&amp;gt;&lt;br /&gt;
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&amp;lt;math&amp;gt; \mathcal{H}^d(S):=\lim_{r \to 0} \inf\Bigl\{\sum_i r_i^d:\text{有一个面} S\text{ 球 } 0 &amp;lt; r_i &amp;lt; r\Bigr\}.&amp;lt;/math&amp;gt;&lt;br /&gt;
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===Hausdorff dimension豪斯多夫维数===&lt;br /&gt;
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The '''Hausdorff dimension''' of ''X'' is defined by&lt;br /&gt;
&lt;br /&gt;
The Hausdorff dimension of X is defined by&lt;br /&gt;
&lt;br /&gt;
X 的豪斯多夫维数定义为&lt;br /&gt;
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:&amp;lt;math&amp;gt;\dim_{\operatorname{H}}(X):=\inf\{d\ge 0: \mathcal{H}^d(X)=0\}.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt;\dim_{\operatorname{H}}(X):=\inf\{d\ge 0: \mathcal{H}^d(X)=0\}.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
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Equivalently, dim&amp;lt;sub&amp;gt;H&amp;lt;/sub&amp;gt;(''X'') may be defined as the [[infimum]] of the set of ''d'' ∈ [0, ∞) such that the ''d''-dimensional [[Hausdorff measure]] of ''X'' is zero. This is the same as the supremum of the set of ''d''&amp;amp;nbsp;∈&amp;amp;nbsp;[0,&amp;amp;nbsp;∞) such that the ''d''-dimensional Hausdorff measure of ''X'' is infinite (except that when this latter set of numbers ''d'' is empty the Hausdorff dimension is zero).&lt;br /&gt;
&lt;br /&gt;
Equivalently, dim&amp;lt;sub&amp;gt;H&amp;lt;/sub&amp;gt;(X) may be defined as the infimum of the set of d ∈ [0, ∞) such that the d-dimensional Hausdorff measure of X is zero. This is the same as the supremum of the set of d&amp;amp;nbsp;∈&amp;amp;nbsp;[0,&amp;amp;nbsp;∞) such that the d-dimensional Hausdorff measure of X is infinite (except that when this latter set of numbers d is empty the Hausdorff dimension is zero).&lt;br /&gt;
&lt;br /&gt;
等价地，dim &amp;lt;sub&amp;gt;H&amp;lt;/sub&amp;gt;(''X'')可定义为 ''d'' ∈ [0, ∞) 集的下确界，使得''X'' 的''d''-维 [[豪斯多夫测度]] 为零。这与 ''d''&amp;amp;nbsp;∈&amp;amp;nbsp;[0,&amp;amp;nbsp;∞)的集合的上确界相同，因此''X''的 d 维豪斯多夫测度是无限的(除非后一个集合 ''d'' 是空的，豪斯多夫维数为零)。&lt;br /&gt;
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==Examples实例==&lt;br /&gt;
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[[Image:Sierpinski deep.svg|thumb|250px|Dimension of a further [[fractal]] example. The [[Sierpinski triangle]], an object with Hausdorff dimension of log(3)/log(2)≈1.58.&amp;lt;ref name=ClaytonSCTPLS96/&amp;gt;]]&lt;br /&gt;
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Dimension of a further [[fractal example. The Sierpinski triangle, an object with Hausdorff dimension of log(3)/log(2)≈1.58.]]&lt;br /&gt;
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[[Image:谢尔宾斯基三角形 deep.svg|thumb|250px|进一步的[[分形维数]]的例子，进一步的分形维数的例子是谢尔宾斯基三角形，它是一个豪斯多夫维数为log(3)/log(2)≈1.58.&amp;lt;ref name=ClaytonSCTPLS96/&amp;gt;的物体]]&lt;br /&gt;
&lt;br /&gt;
* [[Countable set]]s have Hausdorff dimension 0.&amp;lt;ref name=&amp;quot;schleicher&amp;quot;&amp;gt;{{cite journal |last1=Schleicher |first1=Dierk |title=Hausdorff Dimension, Its Properties, and Its Surprises |journal=The American Mathematical Monthly |date=June 2007 |volume=114 |issue=6 |pages=509–528 |doi=10.1080/00029890.2007.11920440 |language=en |issn=0002-9890|arxiv=math/0505099 }}&amp;lt;/ref&amp;gt;&lt;br /&gt;
*[[可数集]]拥有豪斯多夫维数0.&amp;lt;ref name=&amp;quot;schleicher&amp;quot;&amp;gt;{{cite journal |last1=Schleicher |first1=Dierk |title=豪斯多夫维数, Its Properties, and Its Surprises |journal=The American Mathematical Monthly美国数学期刊 |date=June 2007 |volume=114 |issue=6 |pages=509–528 |doi=10.1080/00029890.2007.11920440 |language=en |issn=0002-9890|arxiv=math/0505099 }}&amp;lt;/ref&amp;gt;&lt;br /&gt;
* The [[Euclidean space]] ℝ&amp;lt;sup&amp;gt;''n''&amp;lt;/sup&amp;gt; has Hausdorff dimension ''n'', and the circle '''S'''&amp;lt;sup&amp;gt;1&amp;lt;/sup&amp;gt; has Hausdorff dimension 1.&amp;lt;ref name=&amp;quot;schleicher&amp;quot; /&amp;gt;&lt;br /&gt;
*[[教育空间]] ℝ&amp;lt;sup&amp;gt;''n''&amp;lt;/sup&amp;gt; 有豪斯多夫维数 ''n''，循环'''S'''&amp;lt;sup&amp;gt;1&amp;lt;/sup&amp;gt; 拥有豪斯多夫维数1.&amp;lt;ref name=&amp;quot;schleicher&amp;quot; /&amp;gt;&lt;br /&gt;
* [[Fractal]]s often are spaces whose Hausdorff dimension strictly exceeds the [[topological dimension]].&amp;lt;ref name=&amp;quot;mandelbrot&amp;quot; /&amp;gt; For example, the [[Cantor set]], a zero-dimensional topological space, is a union of two copies of itself, each copy shrunk by a factor 1/3; hence, it can be shown that its Hausdorff dimension is ln(2)/ln(3)&amp;amp;nbsp;≈&amp;amp;nbsp;0.63.&amp;lt;ref&amp;gt;{{cite book | last=Falconer | first = Kenneth |title=Fractal Geometry: Mathematical Foundations and Applications | publisher=[[John Wiley and Sons]] | edition=2nd | year=2003}}&amp;lt;/ref&amp;gt; The [[Sierpinski triangle]] is a union of three copies of itself, each copy shrunk by a factor of&amp;amp;nbsp;1/2; this yields a Hausdorff dimension of ln(3)/ln(2)&amp;amp;nbsp;≈&amp;amp;nbsp;1.58.&amp;lt;ref name=CampbellAnnenberg15/&amp;gt; These Hausdorff dimensions are related to the &amp;quot;critical exponent&amp;quot; of the [[Master theorem (analysis of algorithms)|Master theorem]] for solving [[Recurrence relation|recurrence relations]] in the [[analysis of algorithms]].&lt;br /&gt;
*[[分形]]一般是那些豪斯多夫维数直接超过其拓扑维数的空间。例如[[康托尔集]]是一个o维拓扑空间，由两个自己复制而成，每一个复制品都是原来的三分之一，因此它的豪斯多夫维数是 ln(2)/ln(3)&amp;amp;nbsp;≈&amp;amp;nbsp;0.63。&amp;lt;ref&amp;gt;{{cite book | last=Falconer | first = Kenneth |title=Fractal Geometry: Mathematical Foundations and Applications | publisher=[[John Wiley and Sons]] | edition=2nd | year=2003}}&amp;lt;/ref&amp;gt;一个[[谢尔宾斯基三角]]是他自身三个复制的组合。每一个是原来的&amp;amp;nbsp;1/2，它的豪斯多夫维数ln(3)/ln(2)&amp;amp;nbsp;≈&amp;amp;nbsp;1.58。&amp;lt;ref name=CampbellAnnenberg15/&amp;gt;在递归算法中解决递归关系时，这些豪斯多夫维数与[[算法分析主定理]]的临界指标相联系。&lt;br /&gt;
* [[Space-filling curve]]s like the [[Peano curve]] have the same Hausdorff dimension as the space they fill.&lt;br /&gt;
*[[空间填充曲线]]拥有和他们填充空间同样的豪斯多夫维数，如[[皮亚诺曲线]]。&lt;br /&gt;
* The trajectory of [[Brownian motion]] in dimension 2 and above is conjectured to be Hausdorff dimension 2.&amp;lt;ref&amp;gt;{{cite book | last=Morters | first=Peres | title= Brownian Motion | publisher=[[Cambridge University Press]] | year=2010 }}&amp;lt;/ref&amp;gt;&lt;br /&gt;
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[[image:Great Britain Hausdorff.svg|thumb|250px|Estimating the Hausdorff dimension of the [[How Long Is the Coast of Britain? Statistical Self-Similarity and Fractional Dimension|coast of Great Britain]]]]&lt;br /&gt;
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coast of Great Britain]]&lt;br /&gt;
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[[大不列颠海岸&lt;br /&gt;
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* 刘易斯·弗赖伊·理查森[[Lewis Fry Richardson]] has performed detailed experiments to measure the approximate Hausdorff dimension for various coastlines. His results have varied from 1.02 for the coastline of [[South Africa]] to 1.25 for the west coast of [[Great Britain]].&amp;lt;ref name=&amp;quot;mandelbrot&amp;quot; /&amp;gt;&lt;br /&gt;
*刘易斯·弗赖伊·理查森（Lewis Fry Richardson）已经通过豪斯多夫维数去测量了很多海岸线。它的结果涵盖从1.02的南非海岸线到1.25的大英帝国西海岸模型。]]&lt;br /&gt;
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==Properties of Hausdorff dimension豪斯多夫维数特性==&lt;br /&gt;
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{{refimprove section|date=March 2015}}&lt;br /&gt;
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=== Hausdorff dimension and inductive dimension 豪斯多夫维数和归纳维数===&lt;br /&gt;
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Let ''X'' be an arbitrary [[Separable space|separable]] metric space. There is a [[topology|topological]] notion of [[inductive dimension]] for ''X'' which is defined recursively. It is always an integer (or +∞) and is denoted dim&amp;lt;sub&amp;gt;ind&amp;lt;/sub&amp;gt;(''X'').&lt;br /&gt;
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Let X be an arbitrary separable metric space. There is a topological notion of inductive dimension for X which is defined recursively. It is always an integer (or +∞) and is denoted dim&amp;lt;sub&amp;gt;ind&amp;lt;/sub&amp;gt;(X).&lt;br /&gt;
&lt;br /&gt;
设''X'' 是[[任意可分度量空间]]。对于''X'' 有一个递归定义的归纳维数拓扑概念。它总是一个整数(或 + ∞) ，并且表示dim&amp;lt;sub&amp;gt;ind&amp;lt;/sub&amp;gt;(''X'')。&lt;br /&gt;
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'''Theorem'''. Suppose ''X'' is non-empty. Then &lt;br /&gt;
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Theorem. Suppose X is non-empty. Then &lt;br /&gt;
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'''定理'''：假设''X'' 是非空的。那么&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt; \dim_{\mathrm{Haus}}(X) \geq \dim_{\operatorname{ind}}(X). &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \dim_{\mathrm{Haus}}(X) \geq \dim_{\operatorname{ind}}(X). &amp;lt;/math&amp;gt;&lt;br /&gt;
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&lt;br /&gt;
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Moreover,&lt;br /&gt;
&lt;br /&gt;
Moreover,&lt;br /&gt;
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此外,&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \inf_Y \dim_{\operatorname{Haus}}(Y) =\dim_{\operatorname{ind}}(X), &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \inf_Y \dim_{\operatorname{Haus}}(Y) =\dim_{\operatorname{ind}}(X), &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
where ''Y'' ranges over metric spaces [[homeomorphic]] to ''X''. In other words, ''X'' and ''Y'' have the same underlying set of points and the metric ''d''&amp;lt;sub&amp;gt;''Y''&amp;lt;/sub&amp;gt; of ''Y'' is topologically equivalent to ''d''&amp;lt;sub&amp;gt;''X''&amp;lt;/sub&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
where Y ranges over metric spaces homeomorphic to X. In other words, X and Y have the same underlying set of points and the metric d&amp;lt;sub&amp;gt;Y&amp;lt;/sub&amp;gt; of Y is topologically equivalent to d&amp;lt;sub&amp;gt;X&amp;lt;/sub&amp;gt;.&lt;br /&gt;
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其中''Y''是度量空间同胚到 ''X''的范围。换句话说， ''X''和 ''Y''具有相同的基本点集，''Y''的度规''d''&amp;lt;sub&amp;gt;''Y''&amp;lt;/sub&amp;gt; 的子拓扑等价于''d''&amp;lt;sub&amp;gt;''X''&amp;lt;/sub&amp;gt;。&lt;br /&gt;
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These results were originally established by [[Edward Szpilrajn]] (1907–1976), e.g., see Hurewicz and Wallman, Chapter VII.{{full citation needed|date=March 2015}}&lt;br /&gt;
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These results were originally established by Edward Szpilrajn (1907–1976), e.g., see Hurewicz and Wallman, Chapter VII.&lt;br /&gt;
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这些结果最初是由 [[Edward Szpilrajn]] (1907–1976)建立的,  参见 Hurewicz and Wallman, Chapter VII.{{full citation needed|date=March 2015}}第七章。&lt;br /&gt;
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=== Hausdorff dimension and Minkowski dimension 豪斯多夫维数和闵可夫斯基维度===&lt;br /&gt;
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The [[Minkowski dimension]] is similar to, and at least as large as, the Hausdorff dimension, and they are equal in many situations. However, the set of [[rational number|rational]] points in [0, 1] has Hausdorff dimension zero and Minkowski dimension one. There are also compact sets for which the Minkowski dimension is strictly larger than the Hausdorff dimension.&lt;br /&gt;
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The Minkowski dimension is similar to, and at least as large as, the Hausdorff dimension, and they are equal in many situations. However, the set of rational points in [0, 1] has Hausdorff dimension zero and Minkowski dimension one. There are also compact sets for which the Minkowski dimension is strictly larger than the Hausdorff dimension.&lt;br /&gt;
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[[闵可夫斯基维数]]与豪斯多夫维数相似，至少和它一样大，而且在许多情况下是相等的。然而，[0,1]中有理点集的豪斯多夫维数为0，闵可夫斯基维数为1。还有一些紧集的闵可夫斯基维数绝对大于豪斯多夫维数。&lt;br /&gt;
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=== Hausdorff dimensions and Frostman measures 豪斯多夫维度和弗洛斯曼测度===&lt;br /&gt;
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If there is a [[measure (mathematics)|measure]] μ defined on [[Borel measure|Borel]] subsets of a metric space ''X'' such that ''μ''(''X'') &amp;gt; 0 and ''μ''(''B''(''x'', ''r'')) ≤ ''r&amp;lt;sup&amp;gt;s&amp;lt;/sup&amp;gt;'' holds for some constant ''s'' &amp;gt; 0 and for every ball ''B''(''x'', ''r'') in ''X'', then dim&amp;lt;sub&amp;gt;Haus&amp;lt;/sub&amp;gt;(''X'') ≥ ''s''. A partial converse is provided by [[Frostman's lemma]].{{citation needed|date=March 2015}}&amp;lt;ref&amp;gt;This Wikipedia article also discusses further useful characterizations of the Hausdorff dimension.{{clarify|date=March 2015}}&amp;lt;/ref&amp;gt;&lt;br /&gt;
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If there is a measure μ defined on Borel subsets of a metric space X such that μ(X) &amp;gt; 0 and μ(B(x, r)) ≤ r&amp;lt;sup&amp;gt;s&amp;lt;/sup&amp;gt; holds for some constant s &amp;gt; 0 and for every ball B(x, r) in X, then dim&amp;lt;sub&amp;gt;Haus&amp;lt;/sub&amp;gt;(X) ≥ s. A partial converse is provided by Frostman's lemma.&lt;br /&gt;
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如果在度量空间 ''X'' 的 Borel 子集上定义一个测度 μ，使得''μ''(''X'') &amp;gt; 0 和''μ''(''B''(''x'', ''r'')) ≤ ''r&amp;lt;sup&amp;gt;s&amp;lt;/sup&amp;gt;''，对于某个常数 ''s'' &amp;gt; 0  和 ''X'' 中的每个球 ''B''(''x'', ''r'') 成立，则 dim&amp;lt;sub&amp;gt;Haus&amp;lt;/sub&amp;gt;(''X'') ≥ ''s'' 。 部分逆向转换由弗洛斯曼引理定义。&lt;br /&gt;
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=== Behaviour under unions and products ===&lt;br /&gt;
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If &amp;lt;math&amp;gt;X=\bigcup_{i\in I}X_i&amp;lt;/math&amp;gt; is a finite or countable union, then&lt;br /&gt;
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If &amp;lt;math&amp;gt;X=\bigcup_{i\in I}X_i&amp;lt;/math&amp;gt; is a finite or countable union, then&lt;br /&gt;
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如果 &amp;lt;math&amp;gt;X=\bigcup_{i\in I}X_i&amp;lt;/math&amp;gt; 是一个有限或可数的联合，则&lt;br /&gt;
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&amp;lt;math&amp;gt; \dim_{\operatorname{Haus}}(X) =\sup_{i\in I} \dim_{\operatorname{Haus}}(X_i).&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \dim_{\operatorname{Haus}}(X) =\sup_{i\in I} \dim_{\operatorname{Haus}}(X_i).&amp;lt;/math&amp;gt;&lt;br /&gt;
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This can be verified directly from the definition.&lt;br /&gt;
&lt;br /&gt;
This can be verified directly from the definition.&lt;br /&gt;
&lt;br /&gt;
这可以直接从定义得到验证。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
If ''X'' and ''Y'' are non-empty metric spaces, then the Hausdorff dimension of their product satisfies&amp;lt;ref&amp;gt;{{cite journal |author=Marstrand, J. M. |title=The dimension of Cartesian product sets |journal=Proc. Cambridge Philos. Soc. |volume=50 |issue=3 |pages=198–202 |year=1954 |doi=10.1017/S0305004100029236 |bibcode = 1954PCPS...50..198M }}&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
If X and Y are non-empty metric spaces, then the Hausdorff dimension of their product satisfies&lt;br /&gt;
&lt;br /&gt;
如果 ''X'' 和''Y''是非空度量空间，那么它们乘积的豪斯多夫维数满足&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt; \dim_{\operatorname{Haus}}(X\times Y)\ge \dim_{\operatorname{Haus}}(X)+ \dim_{\operatorname{Haus}}(Y).&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \dim_{\operatorname{Haus}}(X\times Y)\ge \dim_{\operatorname{Haus}}(X)+ \dim_{\operatorname{Haus}}(Y).&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
This inequality can be strict. It is possible to find two sets of dimension 0 whose product has dimension 1.&amp;lt;ref&amp;gt;{{cite book  | last = Falconer  | first = Kenneth J.  | title = Fractal geometry. Mathematical foundations and applications  | publisher = John Wiley &amp;amp; Sons, Inc., Hoboken, New Jersey  | year = 2003  | doi =   | isbn = }}&amp;lt;/ref&amp;gt; In the opposite direction, it is known that when ''X'' and ''Y'' are Borel subsets of '''R'''&amp;lt;sup&amp;gt;''n''&amp;lt;/sup&amp;gt;, the Hausdorff dimension of ''X'' × ''Y'' is bounded from above by the Hausdorff dimension of ''X'' plus the [[packing dimension|upper packing dimension]] of ''Y''. These facts are discussed in Mattila (1995).&lt;br /&gt;
&lt;br /&gt;
This inequality can be strict. It is possible to find two sets of dimension 0 whose product has dimension 1. In the opposite direction, it is known that when X and Y are Borel subsets of R&amp;lt;sup&amp;gt;n&amp;lt;/sup&amp;gt;, the Hausdorff dimension of X × Y is bounded from above by the Hausdorff dimension of X plus the upper packing dimension of Y. These facts are discussed in Mattila (1995).&lt;br /&gt;
&lt;br /&gt;
这种不平等可以是绝对的。有可能找到两个维数为0的集合，其乘积的维数为1。相反，我们知道当''X''和''Y''是 '''R'''&amp;lt;sup&amp;gt;''n''&amp;lt;/sup&amp;gt;的 Borel 子集时， ''X'' × ''Y''的豪斯多夫维数从上面以 ''X''的豪斯多夫维数加上 ''Y''的填充维数为界。Mattila (1995)曾就这些情况进行了讨论。&lt;br /&gt;
&lt;br /&gt;
==Self-similar sets自相似集合==&lt;br /&gt;
&lt;br /&gt;
{{refimprove section|date=March 2015}}&lt;br /&gt;
&lt;br /&gt;
Many sets defined by a self-similarity condition have dimensions which can be determined explicitly. Roughly, a set ''E'' is self-similar if it is the fixed point of a set-valued transformation ψ, that is ψ(''E'') = ''E'', although the exact definition is given below.&lt;br /&gt;
&lt;br /&gt;
Many sets defined by a self-similarity condition have dimensions which can be determined explicitly. Roughly, a set E is self-similar if it is the fixed point of a set-valued transformation ψ, that is ψ(E) = E, although the exact definition is given below.&lt;br /&gt;
&lt;br /&gt;
许多由自相似条件定义的集合具有可以显式确定的维数。粗略地说，集合''E'' 是自相似的，如果它是集值ψ变换的不动点，即ψ(''E'') = ''E''，尽管下面给出了确切的定义。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&amp;lt;blockquote&amp;gt;'''Theorem'''. Suppose&lt;br /&gt;
&lt;br /&gt;
&amp;lt;blockquote&amp;gt;Theorem. Suppose&lt;br /&gt;
&lt;br /&gt;
&amp;lt;blockquote&amp;gt;'''定理'''：假设&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt; \psi_i: \mathbf{R}^n \rightarrow \mathbf{R}^n, \quad i=1, \ldots , m &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \psi_i: \mathbf{R}^n \rightarrow \mathbf{R}^n, \quad i=1, \ldots , m &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
are [[Contraction mapping|contractive]] mappings on '''R'''&amp;lt;sup&amp;gt;''n''&amp;lt;/sup&amp;gt; with contraction constant ''r&amp;lt;sub&amp;gt;j&amp;lt;/sub&amp;gt;'' &amp;lt; 1. Then there is a unique ''non-empty'' compact set ''A'' such that&lt;br /&gt;
&lt;br /&gt;
are contractive mappings on R&amp;lt;sup&amp;gt;n&amp;lt;/sup&amp;gt; with contraction constant r&amp;lt;sub&amp;gt;j&amp;lt;/sub&amp;gt; &amp;lt; 1. Then there is a unique non-empty compact set A such that&lt;br /&gt;
&lt;br /&gt;
是'''R'''&amp;lt;sup&amp;gt;''n''&amp;lt;/sup&amp;gt;上的压缩常数''r&amp;lt;sub&amp;gt;j&amp;lt;/sub&amp;gt;'&amp;lt; 1的压缩映射。然后有一个唯一的非空紧集A &lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt; A = \bigcup_{i=1}^m \psi_i (A). &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; A = \bigcup_{i=1}^m \psi_i (A). &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&amp;lt;/blockquote&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;/blockquote&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The theorem follows from [[Stefan Banach]]'s [[Contractive mapping theorem|contractive mapping fixed point theorem]] applied to the complete metric space of non-empty compact subsets of '''R'''&amp;lt;sup&amp;gt;''n''&amp;lt;/sup&amp;gt; with the [[Hausdorff distance]].&amp;lt;ref&amp;gt;{{cite book |author=Falconer, K. J. |title=The Geometry of Fractal Sets |publisher=Cambridge University Press |location=Cambridge, UK |year=1985 |isbn=0-521-25694-1 |chapter=Theorem 8.3}}&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
The theorem follows from Stefan Banach's contractive mapping fixed point theorem applied to the complete metric space of non-empty compact subsets of R&amp;lt;sup&amp;gt;n&amp;lt;/sup&amp;gt; with the Hausdorff distance.&lt;br /&gt;
&lt;br /&gt;
这个定理来源于 Stefan Banach 的压缩映射不动点定理，该定理应用于 '''R'''&amp;lt;sup&amp;gt;''n''&amp;lt;/sup&amp;gt; 的非空紧子集的完备空间豪斯多夫距离。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
===The open set condition开集条件===&lt;br /&gt;
&lt;br /&gt;
To determine the dimension of the self-similar set ''A'' (in certain cases), we need a technical condition called the ''open set condition'' (OSC) on the sequence of contractions ψ&amp;lt;sub&amp;gt;''i''&amp;lt;/sub&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
To determine the dimension of the self-similar set A (in certain cases), we need a technical condition called the open set condition (OSC) on the sequence of contractions ψ&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
为了确定自相似集''A'' 的维数(在某些情况下) ，我们需要一个称为''开集条件''(OSC)的技术条件ψ&amp;lt;sub&amp;gt;''i''&amp;lt;/sub&amp;gt;。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
There is a relatively compact open set ''V'' such that&lt;br /&gt;
&lt;br /&gt;
There is a relatively compact open set V such that&lt;br /&gt;
&lt;br /&gt;
有一个相对紧的开集''V''&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt; \bigcup_{i=1}^m\psi_i (V) \subseteq V, &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \bigcup_{i=1}^m\psi_i (V) \subseteq V, &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
where the sets in union on the left are pairwise [[disjoint sets|disjoint]].&lt;br /&gt;
&lt;br /&gt;
where the sets in union on the left are pairwise disjoint.&lt;br /&gt;
&lt;br /&gt;
左边的集合是成对不相交的。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The open set condition is a separation condition that ensures the images ψ&amp;lt;sub&amp;gt;''i''&amp;lt;/sub&amp;gt;(''V'') do not overlap &amp;quot;too much&amp;quot;.&lt;br /&gt;
&lt;br /&gt;
The open set condition is a separation condition that ensures the images ψ&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;(V) do not overlap &amp;quot;too much&amp;quot;.&lt;br /&gt;
&lt;br /&gt;
开集条件是保证图像子ψ&amp;lt;sub&amp;gt;''i''&amp;lt;/sub&amp;gt;(''V'') 不重叠“太多”的分离条件。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
'''Theorem'''. Suppose the open set condition holds and each ψ&amp;lt;sub&amp;gt;''i''&amp;lt;/sub&amp;gt; is a similitude, that is a composition of an [[isometry]] and a [[dilation (metric space)|dilation]] around some point. Then the unique fixed point of ψ is a set whose Hausdorff dimension is ''s'' where ''s'' is the unique solution of&amp;lt;ref&amp;gt;{{cite journal | last=Hutchinson | first=John E. | title=Fractals and self similarity | journal=Indiana Univ. Math. J. | volume=30 | year=1981 | pages=713–747 | doi=10.1512/iumj.1981.30.30055 | issue=5 | doi-access=free }}&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
Theorem. Suppose the open set condition holds and each ψ&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt; is a similitude, that is a composition of an isometry and a dilation around some point. Then the unique fixed point of ψ is a set whose Hausdorff dimension is s where s is the unique solution of&lt;br /&gt;
&lt;br /&gt;
'''定理'''假设开集条件成立，并且每个ψ&amp;lt;sub&amp;gt;''i''&amp;lt;/sub&amp;gt; 是一个相似量，这是一个等距和围绕某一点的膨胀的合成。那么唯一的不动点是一个集合，它的豪斯多夫维数是 ''s'' ，其中  ''s'' 是 ''s'' &amp;lt;ref&amp;gt;{{cite journal | last=Hutchinson | first=John E. | title=Fractals and self similarity | journal=Indiana Univ. Math. J. | volume=30 | year=1981 | pages=713–747 | doi=10.1512/iumj.1981.30.30055 | issue=5 | doi-access=free }}&amp;lt;/ref&amp;gt;的唯一解&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt; \sum_{i=1}^m r_i^s = 1. &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \sum_{i=1}^m r_i^s = 1. &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The contraction coefficient of a similitude is the magnitude of the dilation.&lt;br /&gt;
&lt;br /&gt;
The contraction coefficient of a similitude is the magnitude of the dilation.&lt;br /&gt;
&lt;br /&gt;
相似物的收缩系数就是膨胀的大小。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
We can use this theorem to compute the Hausdorff dimension of the Sierpinski triangle (or sometimes called Sierpinski gasket). Consider three [[non-collinear points]] ''a''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;, ''a''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;, ''a''&amp;lt;sub&amp;gt;3&amp;lt;/sub&amp;gt; in the plane '''R'''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; and let ψ&amp;lt;sub&amp;gt;''i''&amp;lt;/sub&amp;gt; be the dilation of ratio 1/2 around ''a&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;''. The unique non-empty fixed point of the corresponding mapping ψ is a Sierpinski gasket and the dimension ''s'' is the unique solution of&lt;br /&gt;
&lt;br /&gt;
We can use this theorem to compute the Hausdorff dimension of the Sierpinski triangle (or sometimes called Sierpinski gasket). Consider three non-collinear points a&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;, a&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;, a&amp;lt;sub&amp;gt;3&amp;lt;/sub&amp;gt; in the plane R&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; and let ψ&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt; be the dilation of ratio 1/2 around a&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;. The unique non-empty fixed point of the corresponding mapping ψ is a Sierpinski gasket and the dimension s is the unique solution of&lt;br /&gt;
&lt;br /&gt;
我们可以使用这个定理来计算谢尔宾斯基三角形的豪斯多夫维数(或者有时候叫做谢尔宾斯基垫圈)。考虑R&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; 平面上的三个非共线点，''a''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;，''a''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;，''a''&amp;lt;sub&amp;gt;3&amp;lt;/sub&amp;gt;，让ψ&amp;lt;sub&amp;gt;''i''&amp;lt;/sub&amp;gt;是围绕着''a&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;''膨胀比率的1/2。对应映射的唯一非空不动点是一个谢尔宾斯基垫圈，其维数''s''是对应映射的唯一解&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt; \left(\frac{1}{2}\right)^s+\left(\frac{1}{2}\right)^s+\left(\frac{1}{2}\right)^s = 3 \left(\frac{1}{2}\right)^s =1. &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \left(\frac{1}{2}\right)^s+\left(\frac{1}{2}\right)^s+\left(\frac{1}{2}\right)^s = 3 \left(\frac{1}{2}\right)^s =1. &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Taking [[natural logarithm]]s of both sides of the above equation, we can solve for ''s'', that is: ''s'' = ln(3)/ln(2).  The Sierpinski gasket is self-similar and satisfies the OSC. In general a set ''E'' which is a fixed point of a mapping&lt;br /&gt;
&lt;br /&gt;
Taking natural logarithms of both sides of the above equation, we can solve for s, that is: s = ln(3)/ln(2).  The Sierpinski gasket is self-similar and satisfies the OSC. In general a set E which is a fixed point of a mapping&lt;br /&gt;
&lt;br /&gt;
取上述方程两边的自然对数，我们可以求出 ''s''，即: ''s'' = ln(3)/ln(2)。该密封垫具有自相似性，满足 OSC 要求。一般来说，集合 ''E''是一个映射的不动点&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt; A \mapsto \psi(A) = \bigcup_{i=1}^m \psi_i(A) &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt; A \mapsto \psi(A) = \bigcup_{i=1}^m \psi_i(A) &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
is self-similar if and only if the intersections&lt;br /&gt;
&lt;br /&gt;
is self-similar if and only if the intersections&lt;br /&gt;
&lt;br /&gt;
是自相似的，当且仅当&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt; H^s\left(\psi_i(E) \cap \psi_j(E)\right) =0, &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; H^s\left(\psi_i(E) \cap \psi_j(E)\right) =0, &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
where ''s'' is the Hausdorff dimension of ''E'' and ''H&amp;lt;sup&amp;gt;s&amp;lt;/sup&amp;gt;'' denotes [[Hausdorff measure]]. This is clear in the case of the Sierpinski gasket (the intersections are just points), but is also true more generally:&lt;br /&gt;
&lt;br /&gt;
where s is the Hausdorff dimension of E and H&amp;lt;sup&amp;gt;s&amp;lt;/sup&amp;gt; denotes Hausdorff measure. This is clear in the case of the Sierpinski gasket (the intersections are just points), but is also true more generally:&lt;br /&gt;
&lt;br /&gt;
其中 ''s''是''E''的豪斯多夫维数， ''E'' and ''H&amp;lt;sup&amp;gt;s&amp;lt;/sup&amp;gt;'' 表示 豪斯多夫测度。对于谢尔宾斯基垫圈(交叉点就是点)来说，这一点很明显，但更普遍的情况是:&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
'''Theorem'''. Under the same conditions as the previous theorem, the unique fixed point of ψ is self-similar.&lt;br /&gt;
&lt;br /&gt;
Theorem. Under the same conditions as the previous theorem, the unique fixed point of ψ is self-similar.&lt;br /&gt;
&lt;br /&gt;
'''定理'''：在与前一定理相同的条件下，其唯一不动点是自相似的。&lt;br /&gt;
&lt;br /&gt;
==See also参阅==&lt;br /&gt;
&lt;br /&gt;
* [[List of fractals by Hausdorff dimension豪斯多夫分形维数列表]] Examples of deterministic fractals, random and natural fractals.确定性分形与随机和自然分形的示例。&lt;br /&gt;
&lt;br /&gt;
* [[Assouad dimension  Assouad维数]], another variation of fractal dimension that, like Hausdorff dimension, is defined using coverings by balls其他被球覆盖方式定义的分形维数，例如豪斯多夫维数。&lt;br /&gt;
&lt;br /&gt;
* [[Intrinsic dimension固有维数]]&lt;br /&gt;
&lt;br /&gt;
* [[Packing dimension填充维数]]&lt;br /&gt;
&lt;br /&gt;
* [[Fractal dimension分形维数]]&lt;br /&gt;
&lt;br /&gt;
==References参考文献==&lt;br /&gt;
&lt;br /&gt;
{{reflist}}&lt;br /&gt;
&lt;br /&gt;
==Further reading拓展阅读==&lt;br /&gt;
&lt;br /&gt;
* {{cite book |last1=Dodson |first1=M. Maurice |title=Fractal Geometry and Applications: A Jubilee of Benoît Mandelbrot |volume=72 |issue=1 |pages=305–347 |last2=Kristensen |first2=Simon |chapter=Hausdorff Dimension and Diophantine Approximation |date=June 12, 2003 |arxiv=math/0305399 |bibcode = 2003math......5399D |doi=10.1090/pspum/072.1/2112110|series=Proceedings of Symposia in Pure Mathematics |isbn=9780821836378 }}&lt;br /&gt;
&lt;br /&gt;
* {{cite book |last1=Hurewicz |first1=Witold |authorlink1=Witold Hurewicz |last2=Wallman |first2=Henry |authorlink2=Henry Wallman |title=Dimension Theory |url=https://archive.org/details/in.ernet.dli.2015.84609 |publisher=Princeton University Press |year=1948 }}&lt;br /&gt;
&lt;br /&gt;
* {{cite journal |author作者=E. Szpilrajn |authorlink=Edward Marczewski |title=La dimension et la mesure |journal=Fundamenta Mathematicae |volume=28 |pages=81–9 |year=1937 }}&lt;br /&gt;
&lt;br /&gt;
* {{cite journal&lt;br /&gt;
&lt;br /&gt;
 | last1=Marstrand&lt;br /&gt;
&lt;br /&gt;
 | last1=Marstrand&lt;br /&gt;
&lt;br /&gt;
 | last1=马斯特兰德&lt;br /&gt;
&lt;br /&gt;
 | first1=J. M. | title=The dimension of cartesian product sets | year=1954 | journal=Proc. Cambridge Philos. Soc.&lt;br /&gt;
&lt;br /&gt;
 | first1=J. M. | title=The dimension of cartesian product sets | year=1954 | journal=Proc. Cambridge Philos. Soc.&lt;br /&gt;
&lt;br /&gt;
 | first1= J. M. | title=笛卡儿积集的维数 | 1954年 |  journal=Proc. Cambridge Philos. Soc.&lt;br /&gt;
&lt;br /&gt;
 | volume=50&lt;br /&gt;
&lt;br /&gt;
 | volume=50&lt;br /&gt;
&lt;br /&gt;
 | 第50卷&lt;br /&gt;
&lt;br /&gt;
 | issue=3&lt;br /&gt;
&lt;br /&gt;
 | issue=3&lt;br /&gt;
&lt;br /&gt;
 | 第三期&lt;br /&gt;
&lt;br /&gt;
 | pages=198–202&lt;br /&gt;
&lt;br /&gt;
 | pages=198–202&lt;br /&gt;
&lt;br /&gt;
 | 第198-202页&lt;br /&gt;
&lt;br /&gt;
 | doi=10.1017/S0305004100029236|bibcode = 1954PCPS...50..198M }}&lt;br /&gt;
&lt;br /&gt;
 | doi=10.1017/S0305004100029236|bibcode = 1954PCPS...50..198M }}&lt;br /&gt;
&lt;br /&gt;
10.1017 / S0305004100029236 | bibcode 1954PCPS... 50. . 198 m }&lt;br /&gt;
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* {{Cite book&lt;br /&gt;
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 | last1=Mattila&lt;br /&gt;
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 | last1=Mattila&lt;br /&gt;
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 | first1=Pertti | author1-link=Pertti Mattila| title=Geometry of sets and measures in Euclidean spaces | publisher=[[Cambridge University Press]]&lt;br /&gt;
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 | first1=Pertti | author1-link=Pertti Mattila| title=Geometry of sets and measures in Euclidean spaces | publisher=Cambridge University Press&lt;br /&gt;
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| first1 Pertti | author1-link Pertti Mattila | title 欧几里德空间中集合和度量的几何 | 出版商剑桥大学出版社&lt;br /&gt;
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 | isbn=978-0-521-65595-8 | year=1995}}&lt;br /&gt;
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 | isbn=978-0-521-65595-8 | year=1995}}&lt;br /&gt;
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| isbn 978-0-521-65595-8 | year 1995}&lt;br /&gt;
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* {{cite journal |author=A. S. Besicovitch |authorlink=A. S. Besicovitch |title=On Linear Sets of Points of Fractional Dimensions |journal=[[Mathematische Annalen]] |volume=101 |year=1929 | doi=10.1007/BF01454831| issue=1 |pages= 161–193}}&lt;br /&gt;
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* {{cite journal |author1=A. S. Besicovitch |authorlink1=A. S. Besicovitch |author2=H. D. Ursell |authorlink2=H. D. Ursell |title=Sets of Fractional Dimensions |journal=Journal of the London Mathematical Society |volume=12 |year=1937 | issue=1 | doi=10.1112/jlms/s1-12.45.18  | pages=18–25 }}&amp;lt;br/&amp;gt;Several selections from this volume are reprinted in {{cite book |author=Edgar, Gerald A. |title=Classics on fractals |publisher=Addison-Wesley |location=Boston |year=1993 |isbn=0-201-58701-7}} See chapters 9,10,11&lt;br /&gt;
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* {{cite journal |author=F. Hausdorff |authorlink=F. Hausdorff |title=Dimension und äußeres Maß |journal=Mathematische Annalen |volume=79 |issue=1–2 |pages=157–179 |date=March 1919 |doi=10.1007/BF01457179|hdl=10338.dmlcz/100363 |url=http://dml.cz/bitstream/handle/10338.dmlcz/100363/CzechMathJ_09-1959-3_5.pdf }}&lt;br /&gt;
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* {{cite journal | last=Hutchinson | first=John E. | title=Fractals and self similarity | journal=Indiana Univ. Math. J. | volume=30 | year=1981 | pages=713–747 | doi=10.1512/iumj.1981.30.30055 | issue=5 | doi-access=free }}&lt;br /&gt;
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*{{cite book | last=Falconer | first = Kenneth |title=Fractal Geometry: Mathematical Foundations and Applications | publisher=[[John Wiley and Sons]] | edition=2nd | year=2003}}&lt;br /&gt;
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==External links外部链接==&lt;br /&gt;
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* [https://www.encyclopediaofmath.org/index.php/Hausdorff_dimension Hausdorff dimension] 在 [https://www.encyclopediaofmath.org/ Encyclopedia of Mathematics]&lt;br /&gt;
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* [https://www.encyclopediaofmath.org/index.php/Hausdorff_measure Hausdorff measure] 在 [https://www.encyclopediaofmath.org/ Encyclopedia of Mathematics]&lt;br /&gt;
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{{DEFAULTSORT:Hausdorff Dimension豪斯多夫维数}}&lt;br /&gt;
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[[Category分类:Metric geometry度量几何]]&lt;br /&gt;
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[[Category分类:Dimension theory维度理论]]&lt;br /&gt;
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&amp;lt;small&amp;gt;This page was moved from [[wikipedia:en:Hausdorff dimension]]. Its edit history can be viewed at [[分形维数/edithistory]]&amp;lt;/small&amp;gt;&amp;lt;/noinclude&amp;gt;&lt;br /&gt;
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[[Category:待整理页面]]&lt;/div&gt;</summary>
		<author><name>Ruili</name></author>
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		<title>分形维数</title>
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		<updated>2020-10-27T15:35:48Z</updated>

		<summary type="html">&lt;p&gt;Ruili：&lt;/p&gt;
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&lt;div&gt;此词条暂由彩云小译翻译，未经人工整理和审校，带来阅读不便，请见谅。&lt;br /&gt;
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Example of non-integer dimensions. The first four [[iteration]]s of the [[Koch snowflake|Koch curve]], where after each iteration, all original line segments are replaced with four, each a self-similar copy that is 1/3 the length of the original. One formalism of the Hausdorff dimension uses this scale factor (3) and the number of self-similar objects (4) to calculate the dimension, D, after the first iteration to be D = (log N)/(log S) = (log 4)/(log 3) ≈ 1.26.&amp;lt;ref name=CampbellAnnenberg15&amp;gt;MacGregor Campbell, 2013, &amp;quot;5.6 Scaling and the Hausdorff Dimension,&amp;quot; at ''Annenberg Learner:MATHematics illuminated'', see [http://www.learner.org/courses/mathilluminated/units/5/textbook/06.php], accessed 5 March 2015.&amp;lt;/ref&amp;gt; That is, while the Hausdorff dimension of a single [[point (geometry)|point]] is zero, of a [[line segment]] is 1, of a [[square]] is 2, and of a [[cube]] is 3, for [[fractal]]s such as this, the object can have a non-integer dimension.&lt;br /&gt;
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Example of non-integer dimensions. The first four [[iterations of the Koch curve, where after each iteration, all original line segments are replaced with four, each a self-similar copy that is 1/3 the length of the original. One formalism of the Hausdorff dimension uses this scale factor (3) and the number of self-similar objects (4) to calculate the dimension, D, after the first iteration to be D = (log N)/(log S) = (log 4)/(log 3) ≈ 1.26. That is, while the Hausdorff dimension of a single point is zero, of a line segment is 1, of a square is 2, and of a cube is 3, for fractals such as this, the object can have a non-integer dimension.&lt;br /&gt;
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非整数维度示例：前四个[[Koch 曲线]]的迭代，在每次迭代后，所有原始线段都被替换为四个，每个自相似的复制是原始线段长度的1 / 3。豪斯多夫维数的一个建模是使用这个比例因子(3)和自相似物体的数量(4)来计算维度，设在第一次迭代后为 D = (log N)/(log S) = (log 4)/(log 3) ≈ 1.26.&amp;lt;ref name=CampbellAnnenberg15&amp;gt;。MacGregor Campbell, 2013, &amp;quot;5.6 Scaling and the Hausdorff Dimension,&amp;quot; 在 ''Annenberg Learner:MATHematics illuminated'', 参见 [http://www.learner.org/courses/mathilluminated/units/5/textbook/06.php], accessed 5 March 2015.&amp;lt;/ref&amp;gt; 也就是说，当一个点的豪斯多夫维数为零，线段为1，正方形为2，立方体为3时，对于像这样的分形，物体可以有一个非整数维度。&lt;br /&gt;
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In [[mathematics]], '''Hausdorff dimension''' is a measure of ''roughness'', or more specifically, [[fractal dimension]], that was first introduced in 1918 by [[mathematician]] [[Felix Hausdorff]].&amp;lt;ref&amp;gt;{{Cite journal |arxiv = 1101.1444|doi = 10.1214/11-STS370|title = Estimators of Fractal Dimension: Assessing the Roughness of Time Series and Spatial Data|journal = Statistical Science|volume = 27|issue = 2|pages = 247–277|year = 2012|last1 = Gneiting|first1 = Tilmann|last2 = Ševčíková|first2 = Hana|last3 = Percival|first3 = Donald B.}}&amp;lt;/ref&amp;gt; For instance, the Hausdorff dimension of a single [[point (geometry)|point]] is zero, of a [[line segment]] is 1, of a [[square]] is 2, and of a [[cube]] is 3. That is, for sets of points that define a smooth shape or a shape that has a small number of corners—the shapes of traditional geometry and science—the Hausdorff dimension is an [[integer]] agreeing with the usual sense of dimension, also known as the [[Inductive dimension|topological dimension]]. However, formulas have also been developed that allow calculation of the dimension of other less simple objects, where, solely on the basis of their properties of [[scaling (geometry)|scaling]] and [[self-similarity]], one is led to the conclusion that particular objects—including [[fractal]]s—have non-integer Hausdorff dimensions. Because of the significant technical advances made by [[Abram Samoilovitch Besicovitch]] allowing computation of dimensions for highly irregular or &amp;quot;rough&amp;quot; sets, this dimension is also commonly referred to as the ''Hausdorff–Besicovitch dimension.''&lt;br /&gt;
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In mathematics, Hausdorff dimension is a measure of roughness, or more specifically, fractal dimension, that was first introduced in 1918 by mathematician Felix Hausdorff. For instance, the Hausdorff dimension of a single point is zero, of a line segment is 1, of a square is 2, and of a cube is 3. That is, for sets of points that define a smooth shape or a shape that has a small number of corners—the shapes of traditional geometry and science—the Hausdorff dimension is an integer agreeing with the usual sense of dimension, also known as the topological dimension. However, formulas have also been developed that allow calculation of the dimension of other less simple objects, where, solely on the basis of their properties of scaling and self-similarity, one is led to the conclusion that particular objects—including fractals—have non-integer Hausdorff dimensions. Because of the significant technical advances made by Abram Samoilovitch Besicovitch allowing computation of dimensions for highly irregular or &amp;quot;rough&amp;quot; sets, this dimension is also commonly referred to as the Hausdorff–Besicovitch dimension.&lt;br /&gt;
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在[[数学]]中，'''&amp;lt;font color = '#ff8000'&amp;gt;豪斯多夫维数Hausdorff dimension&amp;lt;/font&amp;gt;'''是一种粗糙度的度量单位，或者更确切地说，分形维数，是由数学家 Felix Hausdorff 在1918年首次提出的。例如，单点的豪斯多夫维数为零，线段为1，正方形为2，立方体为3。也就是说，对于定义了一个光滑形状或一个有少数几个角的形状---- 传统几何学和科学的形状---- 的点集来说，豪斯多夫维数是一个整数，符合通常的维度意义，也称为拓扑维度。然而，还有一些公式允许计算其他不太简单的对象的维数，其中仅仅根据它们的标度和自相似特性，就可以得出结论: 特定的对象ー包括分形ー具有非整数的 Hausdorff 维数。由于阿布拉姆·萨莫伊洛维奇·贝西科维奇的重大技术进步，允许计算高度不规则或“粗糙”集的维度，这个维度通常也被称为 Hausdorff-Besicovitch 维度。 &lt;br /&gt;
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The Hausdorff dimension, more specifically, is a further dimensional number associated with a given set, where the distances between all members of that set are defined. Such a set is termed a [[metric space]]. The dimension is drawn from the [[Extended real number line|extended real numbers]], &amp;lt;math&amp;gt;\overline{\mathbb{R}}&amp;lt;/math&amp;gt;, as opposed to the more intuitive notion of dimension, which is not associated to general metric spaces, and only takes values in the non-negative integers.&lt;br /&gt;
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The Hausdorff dimension, more specifically, is a further dimensional number associated with a given set, where the distances between all members of that set are defined. Such a set is termed a metric space. The dimension is drawn from the extended real numbers, &amp;lt;math&amp;gt;\overline{\mathbb{R}}&amp;lt;/math&amp;gt;, as opposed to the more intuitive notion of dimension, which is not associated to general metric spaces, and only takes values in the non-negative integers.&lt;br /&gt;
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更具体地说，豪斯多夫维数是一个与给定集合相关联的更进一步的维数，其中定义了该集合所有成员之间的距离。这样的集合称为度量空间。维数是从扩展的实数，&amp;lt;math&amp;gt;\overline{\mathbb{R}}&amp;lt;/math&amp;gt;，而不是更直观的维数概念(它不与一般的度量空间相关联，只取非负整数的值)。&lt;br /&gt;
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In mathematical terms, the Hausdorff dimension generalizes the notion of the dimension of a real [[vector space]]. That is, the Hausdorff dimension of an ''n''-dimensional [[inner product space]] equals ''n''. This underlies the earlier statement that the Hausdorff dimension of a point is zero, of a line is one, etc., and that [[fractal|irregular sets]] can have noninteger Hausdorff dimensions. For instance, the [[Koch snowflake]] shown at right is constructed from an equilateral triangle; in each iteration, its component line segments are divided into 3 segments of unit length, the newly created middle segment is used as the base of a new [[equilateral]] triangle that points outward, and this base segment is then deleted to leave a final object from the iteration of unit length of 4.&amp;lt;ref&amp;gt;Larry Riddle, 2014, &amp;quot;Classic Iterated Function Systems: Koch Snowflake&amp;quot;, Agnes Scott College e-Academy (online), see [http://ecademy.agnesscott.edu/~lriddle/ifs/ksnow/ksnow.htm], accessed 5 March 2015.&amp;lt;/ref&amp;gt; That is, after the first iteration, each original line segment has been replaced with N=4, where each self-similar copy is 1/S = 1/3 as long as the original.&amp;lt;ref name=CampbellAnnenberg15/&amp;gt; Stated another way, we have taken an object with Euclidean dimension, D, and reduced its linear scale by 1/3 in each direction, so that its length increases to N=S&amp;lt;sup&amp;gt;D&amp;lt;/sup&amp;gt;.&amp;lt;ref name=ClaytonSCTPLS96&amp;gt;Keith Clayton, 1996, &amp;quot;Fractals and the Fractal Dimension,&amp;quot; ''Basic Concepts in Nonlinear Dynamics and Chaos'' (workshop), Society for Chaos Theory in Psychology and the Life Sciences annual meeting, June 28, 1996, Berkeley, California, see [http://www.vanderbilt.edu/AnS/psychology/cogsci/chaos/workshop/Workshop.html], accessed 5 March 2015.&amp;lt;/ref&amp;gt; This equation is easily solved for D, yielding the ratio of logarithms (or [[natural logarithm]]s) appearing in the figures, and giving—in the Koch and other fractal cases—non-integer dimensions for these objects.&lt;br /&gt;
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In mathematical terms, the Hausdorff dimension generalizes the notion of the dimension of a real vector space. That is, the Hausdorff dimension of an n-dimensional inner product space equals n. This underlies the earlier statement that the Hausdorff dimension of a point is zero, of a line is one, etc., and that irregular sets can have noninteger Hausdorff dimensions. For instance, the Koch snowflake shown at right is constructed from an equilateral triangle; in each iteration, its component line segments are divided into 3 segments of unit length, the newly created middle segment is used as the base of a new equilateral triangle that points outward, and this base segment is then deleted to leave a final object from the iteration of unit length of 4. That is, after the first iteration, each original line segment has been replaced with N=4, where each self-similar copy is 1/S = 1/3 as long as the original. This equation is easily solved for D, yielding the ratio of logarithms (or natural logarithms) appearing in the figures, and giving—in the Koch and other fractal cases—non-integer dimensions for these objects.&lt;br /&gt;
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用数学术语来说，豪斯多夫维数概括了实向量空间维数的概念。也就是说，n 维内积空间的豪斯多夫维数等于 n。 这就是早期假设的基础，一个点的豪斯多夫维数是零，一条线是一等等，不规则集可以有非整数的豪斯多夫维数。例如，右边所示的 Koch 雪花是由一个正三角形构成的; 在每次迭代中，它的组成线段被分成单位长度的3段，新创建的中间线段被用作一个指向外部的新正三角形的基础，然后人们删除这个基础线段用来保留单位长度4的迭代中的最终对象。也就是说，在第一次迭代之后，每个原始线段都被替换为 N=4，其中每个自相似拷贝的长度是原始线段的1/S = 1/3 。这个方程很容易求解为 D，产生出现在图形中的对数(或自然对数)的比率，并给出——在 Koch 和其他分形情况下——这些对象的非整数维数。&lt;br /&gt;
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The Hausdorff dimension is a successor to the simpler, but usually equivalent, box-counting or [[Minkowski–Bouligand dimension]].&lt;br /&gt;
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The Hausdorff dimension is a successor to the simpler, but usually equivalent, box-counting or Minkowski–Bouligand dimension.&lt;br /&gt;
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豪斯多夫维数是更简单但通常等价的'''&amp;lt;font color = '#ff8000'&amp;gt;计盒维数box-counting&amp;lt;/font&amp;gt;'''或'''&amp;lt;font color = '#ff8000'&amp;gt;闵可夫斯基维数Minkowski-Bouligand&amp;lt;/font&amp;gt;'''的继承者。&lt;br /&gt;
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==Intuition概念==&lt;br /&gt;
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The intuitive concept of dimension of a geometric object ''X'' is the number of independent parameters one needs to pick out a unique point inside. However, any point specified by two parameters can be instead specified by one, because the [[cardinality]] of the [[real plane]] is equal to the cardinality of the [[real line]] (this can be seen by an [[Cantor's diagonal argument|argument]] involving interweaving the digits of two numbers to yield a single number encoding the same information). The example of a [[space-filling curve]] shows that one can even map the real line to the real plane [[Surjective function|surjectively]] (taking one real number into a pair of real numbers in a way so that all pairs of numbers are covered) and ''continuously'', so that a one-dimensional object completely fills up a higher-dimensional object.&lt;br /&gt;
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The intuitive concept of dimension of a geometric object X is the number of independent parameters one needs to pick out a unique point inside. However, any point specified by two parameters can be instead specified by one, because the cardinality of the real plane is equal to the cardinality of the real line (this can be seen by an argument involving interweaving the digits of two numbers to yield a single number encoding the same information). The example of a space-filling curve shows that one can even map the real line to the real plane surjectively (taking one real number into a pair of real numbers in a way so that all pairs of numbers are covered) and continuously, so that a one-dimensional object completely fills up a higher-dimensional object.&lt;br /&gt;
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几何物体X的直观尺寸概念就是一个物体需要多少个独立参数才能找到一个独特的点。但是，任何由两个参数指定的点都可以由一个参数指定，因为实际平面的基数等于实际行的基数(这可以通过一个参数看到，该参数涉及交织两个数字的数字以产生一个编码相同信息的单个数字)。'''&amp;lt;font color = '#ff8000'&amp;gt;皮亚诺曲线&amp;lt;/font&amp;gt;'''的例子表明，一个人甚至可以完美和连续地映射实际线到真正的平面(把一个实数转换成一对实数，这样所有的数对都被覆盖)，由此一维物体完全填充了一个高维物体。&lt;br /&gt;
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Every space filling curve hits some points multiple times, and does not have a continuous inverse. It is impossible to map two dimensions onto one in a way that is continuous and continuously invertible. The topological dimension, also called [[Lebesgue covering dimension]], explains why. This dimension is ''n'' if, in every covering of ''X'' by small open balls, there is at least one point where ''n''&amp;amp;nbsp;+&amp;amp;nbsp;1 balls overlap. For example, when one covers a line with short open intervals, some points must be covered twice, giving dimension&amp;amp;nbsp;''n''&amp;amp;nbsp;=&amp;amp;nbsp;1.&lt;br /&gt;
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Every space filling curve hits some points multiple times, and does not have a continuous inverse. It is impossible to map two dimensions onto one in a way that is continuous and continuously invertible. The topological dimension, also called Lebesgue covering dimension, explains why. This dimension is n if, in every covering of X by small open balls, there is at least one point where n&amp;amp;nbsp;+&amp;amp;nbsp;1 balls overlap. For example, when one covers a line with short open intervals, some points must be covered twice, giving dimension&amp;amp;nbsp;n&amp;amp;nbsp;=&amp;amp;nbsp;1.&lt;br /&gt;
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每条空间填充曲线都会多次撞击某些点，且不存在连续的倒数。将两个维度以连续和连续可逆的方式映射到一个维度是不可能的。'''&amp;lt;font color = '#ff8000'&amp;gt;拓扑维度 topological dimension&amp;lt;/font&amp;gt;'''，也被称为拓朴维数，解释了为什么。这个维度是 n，如果在 x 的每个小开球覆盖中，至少有一个点 n + 1个球重叠。例如，当一个点覆盖一条具有短开区间的直线时，某些点必须被覆盖两次，给出维数''n''&amp;amp;nbsp;=&amp;amp;nbsp;1。&lt;br /&gt;
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But topological dimension is a very crude measure of the local size of a space (size near a point). A curve that is almost space-filling can still have topological dimension one, even if it fills up most of the area of a region. A [[fractal]] has an integer topological dimension, but in terms of the amount of space it takes up, it behaves like a higher-dimensional space.&lt;br /&gt;
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But topological dimension is a very crude measure of the local size of a space (size near a point). A curve that is almost space-filling can still have topological dimension one, even if it fills up most of the area of a region. A fractal has an integer topological dimension, but in terms of the amount of space it takes up, it behaves like a higher-dimensional space.&lt;br /&gt;
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但是，拓扑维度是对空间局部尺寸(点附近的尺寸)的一个非常粗略的度量。一条几乎是空间填充的曲线仍然可以有一维拓扑，即使它填充了一个区域的大部分面积。分形具有整数的拓扑维数，但就其所占空间的数量而言，它看起来像一个更高维的空间。&lt;br /&gt;
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The Hausdorff dimension measures the local size of a space taking into account the distance between points, the [[metric space|metric]]. Consider the number ''N''(''r'') of [[ball (mathematics)|balls]] of radius at most ''r'' required to cover ''X'' completely. When ''r'' is very small, ''N''(''r'') grows polynomially with 1/''r''. For a sufficiently well-behaved  ''X'', the Hausdorff dimension is the unique number ''d'' such that N(''r'') grows as 1/''r&amp;lt;sup&amp;gt;d&amp;lt;/sup&amp;gt;'' as ''r'' approaches zero. More precisely, this defines the [[Minkowski–Bouligand dimension|box-counting dimension]], which equals the Hausdorff dimension when the value ''d'' is a critical boundary between growth rates that are insufficient to cover the space, and growth rates that are overabundant.&lt;br /&gt;
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The Hausdorff dimension measures the local size of a space taking into account the distance between points, the metric. Consider the number N(r) of balls of radius at most r required to cover X completely. When r is very small, N(r) grows polynomially with 1/r. For a sufficiently well-behaved  X, the Hausdorff dimension is the unique number d such that N(r) grows as 1/r&amp;lt;sup&amp;gt;d&amp;lt;/sup&amp;gt; as r approaches zero. More precisely, this defines the box-counting dimension, which equals the Hausdorff dimension when the value d is a critical boundary between growth rates that are insufficient to cover the space, and growth rates that are overabundant.&lt;br /&gt;
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豪斯多夫维数测量一个空间的局部大小时，会考虑到点之间距离的度量。考虑半径最大为 r 的球数 ''N'' (r) ，需要完全覆盖 ''X''。当 r 很小时，n (r)以1/''r'' 增长多项式。对于一个表现足够好的 ''X''，豪斯多夫维数是唯一的数 d，这样当 r 趋近于零时， N(r)增长为1/r&amp;lt;sup&amp;gt;d&amp;lt;/sup&amp;gt; 。更确切地说，这定义了盒子计数维度，当值 d 是不足以覆盖空间的增长率和过度充裕的增长率之间的关键边界时，它等于豪斯多夫维数。&lt;br /&gt;
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For shapes that are smooth, or shapes with a small number of corners, the shapes of traditional geometry and science, the Hausdorff dimension is an integer agreeing with the topological dimension. But [[Benoit Mandelbrot]] observed that [[fractal]]s, sets with noninteger Hausdorff dimensions, are found everywhere in nature. He observed that the proper idealization of most rough shapes you see around you is not in terms of smooth idealized shapes, but in terms of fractal idealized shapes:&lt;br /&gt;
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For shapes that are smooth, or shapes with a small number of corners, the shapes of traditional geometry and science, the Hausdorff dimension is an integer agreeing with the topological dimension. But Benoit Mandelbrot observed that fractals, sets with noninteger Hausdorff dimensions, are found everywhere in nature. He observed that the proper idealization of most rough shapes you see around you is not in terms of smooth idealized shapes, but in terms of fractal idealized shapes:&lt;br /&gt;
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对于光滑的形状，或者有少量棱角的形状，传统几何和科学的形状，豪斯多夫维数是一个整数，与拓扑维度一致。但是伯努·曼德布洛特观察到分形---- 具有非整数豪斯多夫维数的集合---- 在自然界中随处可见。他观察到，我们周围大多数粗糙形状的理想化不是光滑的理想化形状，而是分形理想化形状:&lt;br /&gt;
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&amp;lt;blockquote&amp;gt;Clouds are not spheres, mountains are not cones, coastlines are not circles, and bark is not smooth, nor does lightning travel in a straight line.&amp;lt;ref name=&amp;quot;mandelbrot&amp;quot;&amp;gt;{{cite book   | last = Mandelbrot   | first = Benoît   | authorlink = Benoit Mandelbrot   | title = The Fractal Geometry of Nature   | publisher = W. H. Freeman   | series = Lecture notes in mathematics 1358   | year = 1982   | doi =    | isbn = 0-7167-1186-9   | url-access = registration   | url = https://archive.org/details/fractalgeometryo00beno   }}&amp;lt;/ref&amp;gt;&amp;lt;/blockquote&amp;gt;&lt;br /&gt;
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&amp;lt;blockquote&amp;gt;Clouds are not spheres, mountains are not cones, coastlines are not circles, and bark is not smooth, nor does lightning travel in a straight line.&amp;lt;/blockquote&amp;gt;&lt;br /&gt;
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&amp;lt;blockquote&amp;gt;云不是球体，山不是锥体，海岸线不是圆圈，树皮不平滑，闪电也不是直线运动。 &amp;lt;/blockquote&amp;gt;&lt;br /&gt;
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For fractals that occur in nature, the Hausdorff and [[Minkowski–Bouligand dimension|box-counting dimension]] coincide. The [[packing dimension]] is yet another similar notion which gives the same value for many shapes, but there are well documented exceptions where all these dimensions differ.&lt;br /&gt;
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For fractals that occur in nature, the Hausdorff and box-counting dimension coincide. The packing dimension is yet another similar notion which gives the same value for many shapes, but there are well documented exceptions where all these dimensions differ.&lt;br /&gt;
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对于自然界中出现的分形，豪斯多夫维数和盒计数维数是一致的。封装尺寸是另一个类似的概念，它给出了许多形状相同的值，但是在所有这些尺寸不同的情况，都做了很好的说明。&lt;br /&gt;
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==Formal definitions形式化定义==&lt;br /&gt;
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{{unreferenced section|date=March 2015}}&lt;br /&gt;
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===Hausdorff content豪斯多夫集===&lt;br /&gt;
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Let ''X'' be a [[metric space]]. If ''S'' ⊂ ''X'' and ''d'' ∈ [0, ∞), the ''d''-dimensional '''unlimited Hausdorff content''' of ''S'' is defined by&lt;br /&gt;
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Let X be a metric space. If S ⊂ X and d ∈ [0, ∞), the d-dimensional unlimited Hausdorff content of S is defined by&lt;br /&gt;
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设 ''X''是度量空间。若''S'' ⊂ ''X'' 和 ''d'' ∈ [0, ∞) ，则 ''S'' 的''d''维无限 豪斯多夫集定义为&lt;br /&gt;
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:&amp;lt;math&amp;gt;C_H^d(S):=\inf\Bigl\{\sum_i r_i^d:\text{ there is a cover of } S\text{ by balls with radii }r_i&amp;gt;0\Bigr\}.&amp;lt;/math&amp;gt;&lt;br /&gt;
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&amp;lt;math&amp;gt;C_H^d(S):=\inf\Bigl\{\sum_i r_i^d:\text{ there is a cover of } S\text{ by balls with radii }r_i&amp;gt;0\Bigr\}.&amp;lt;/math&amp;gt;&lt;br /&gt;
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&amp;lt;math&amp;gt;C_H^d(S):=\inf\Bigl\{\sum_i r_i^d:\text{ there is a cover of } S\text{ by balls with radii }r_i&amp;gt;0\Bigr\}.&amp;lt;/math&amp;gt;&lt;br /&gt;
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In other words, &amp;lt;math&amp;gt;C_H^d(S)&amp;lt;/math&amp;gt; is the [[infimum]] of the set of numbers &amp;lt;math&amp;gt;\delta \geq 0&amp;lt;/math&amp;gt; such that there is some (indexed) collection of [[ball (mathematics)|ball]]s &amp;lt;math&amp;gt;\{B(x_i,r_i):i\in I\}&amp;lt;/math&amp;gt; covering ''S'' with ''r&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;''&amp;amp;nbsp;&amp;gt;&amp;amp;nbsp;0 for each ''i''&amp;amp;nbsp;∈&amp;amp;nbsp;''I'' that satisfies &amp;lt;math&amp;gt;\sum_{i\in I} r_i^d&amp;lt;\delta &amp;lt;/math&amp;gt;. (Here, we use the standard convention that [[infimum|inf&amp;amp;nbsp;Ø&amp;amp;nbsp;=&amp;amp;nbsp;∞]].)&lt;br /&gt;
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In other words, &amp;lt;math&amp;gt;C_H^d(S)&amp;lt;/math&amp;gt; is the infimum of the set of numbers &amp;lt;math&amp;gt;\delta \geq 0&amp;lt;/math&amp;gt; such that there is some (indexed) collection of balls &amp;lt;math&amp;gt;\{B(x_i,r_i):i\in I\}&amp;lt;/math&amp;gt; covering S with r&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;&amp;amp;nbsp;&amp;gt;&amp;amp;nbsp;0 for each i&amp;amp;nbsp;∈&amp;amp;nbsp;I that satisfies &amp;lt;math&amp;gt;\sum_{i\in I} r_i^d&amp;lt;\delta &amp;lt;/math&amp;gt;. (Here, we use the standard convention that inf&amp;amp;nbsp;Ø&amp;amp;nbsp;=&amp;amp;nbsp;∞.)&lt;br /&gt;
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换句话说，&amp;lt;math&amp;gt;C_H^d(S)&amp;lt;/math&amp;gt; 是数字集合&amp;lt;math&amp;gt;\delta \geq 0&amp;lt;/math&amp;gt;的下确界，使得在 ''i''&amp;amp;nbsp;∈&amp;amp;nbsp中存在一些球集合 &amp;lt;math&amp;gt;\{B(x_i,r_i):i\in I\}&amp;lt;/math&amp;gt;  i 包含 s，对于每个 ''r&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;''&amp;amp;nbsp;&amp;gt;&amp;amp;nbsp;0 满足 i 中的和&amp;lt;math&amp;gt;\sum_{i\in I} r_i^d&amp;lt;\delta &amp;lt;/math&amp;gt; (在这里，我们使用inf&amp;amp;nbsp;Ø&amp;amp;nbsp;=&amp;amp;nbsp;∞ )的标准约定。&lt;br /&gt;
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===Hausdorff measurement豪斯多夫分形测量===&lt;br /&gt;
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The Hausdorff outer measure is different from the unbounded Hausdorf content in that rather than considering all possible coverings of ''S'', we see what happens when the sizes of the balls go to zero. This is  for &amp;lt;math&amp;gt;d \geq 0 &amp;lt;/math&amp;gt;, we define the ''d''-dimensional Hausdorff outer measure of ''S'' as&lt;br /&gt;
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The Hausdorff outer measure is different from the unbounded Hausdorf content in that rather than considering all possible coverings of S, we see what happens when the sizes of the balls go to zero. This is  for &amp;lt;math&amp;gt;d \geq 0 &amp;lt;/math&amp;gt;, we define the d-dimensional Hausdorff outer measure of S as&lt;br /&gt;
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豪斯多夫外测度不同于无界的豪斯多夫，因为我们不考虑 s 的所有可能，我们看到当球的大小为零时会发生什么。这是为了数学  &amp;lt;math&amp;gt;d \geq 0 &amp;lt;/math&amp;gt;，我们定义了  ''S''的 ''d''维豪斯多夫Hausdorff 外测度为&lt;br /&gt;
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:&amp;lt;math&amp;gt; \mathcal{H}^d(S):=\lim_{r \to 0} \inf\Bigl\{\sum_i r_i^d:\text{ there is a cover of } S\text{ by balls with radii } 0 &amp;lt; r_i &amp;lt; r\Bigr\}.&amp;lt;/math&amp;gt;&lt;br /&gt;
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&amp;lt;math&amp;gt; \mathcal{H}^d(S):=\lim_{r \to 0} \inf\Bigl\{\sum_i r_i^d:\text{ there is a cover of } S\text{ by balls with radii } 0 &amp;lt; r_i &amp;lt; r\Bigr\}.&amp;lt;/math&amp;gt;&lt;br /&gt;
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&amp;lt;math&amp;gt; \mathcal{H}^d(S):=\lim_{r \to 0} \inf\Bigl\{\sum_i r_i^d:\text{有一个面} S\text{ 球 } 0 &amp;lt; r_i &amp;lt; r\Bigr\}.&amp;lt;/math&amp;gt;&lt;br /&gt;
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===Hausdorff dimension豪斯多夫维数===&lt;br /&gt;
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The '''Hausdorff dimension''' of ''X'' is defined by&lt;br /&gt;
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The Hausdorff dimension of X is defined by&lt;br /&gt;
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X 的豪斯多夫维数定义为&lt;br /&gt;
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:&amp;lt;math&amp;gt;\dim_{\operatorname{H}}(X):=\inf\{d\ge 0: \mathcal{H}^d(X)=0\}.&amp;lt;/math&amp;gt;&lt;br /&gt;
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&amp;lt;math&amp;gt;\dim_{\operatorname{H}}(X):=\inf\{d\ge 0: \mathcal{H}^d(X)=0\}.&amp;lt;/math&amp;gt;&lt;br /&gt;
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Equivalently, dim&amp;lt;sub&amp;gt;H&amp;lt;/sub&amp;gt;(''X'') may be defined as the [[infimum]] of the set of ''d'' ∈ [0, ∞) such that the ''d''-dimensional [[Hausdorff measure]] of ''X'' is zero. This is the same as the supremum of the set of ''d''&amp;amp;nbsp;∈&amp;amp;nbsp;[0,&amp;amp;nbsp;∞) such that the ''d''-dimensional Hausdorff measure of ''X'' is infinite (except that when this latter set of numbers ''d'' is empty the Hausdorff dimension is zero).&lt;br /&gt;
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Equivalently, dim&amp;lt;sub&amp;gt;H&amp;lt;/sub&amp;gt;(X) may be defined as the infimum of the set of d ∈ [0, ∞) such that the d-dimensional Hausdorff measure of X is zero. This is the same as the supremum of the set of d&amp;amp;nbsp;∈&amp;amp;nbsp;[0,&amp;amp;nbsp;∞) such that the d-dimensional Hausdorff measure of X is infinite (except that when this latter set of numbers d is empty the Hausdorff dimension is zero).&lt;br /&gt;
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等价地，dim &amp;lt;sub&amp;gt;H&amp;lt;/sub&amp;gt;(''X'')可定义为 ''d'' ∈ [0, ∞) 集的下确界，使得''X'' 的''d''-维 [[豪斯多夫测度]] 为零。这与 ''d''&amp;amp;nbsp;∈&amp;amp;nbsp;[0,&amp;amp;nbsp;∞)的集合的上确界相同，因此''X''的 d 维豪斯多夫测度是无限的(除非后一个集合 ''d'' 是空的，豪斯多夫维数为零)。&lt;br /&gt;
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==Examples实例==&lt;br /&gt;
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[[Image:Sierpinski deep.svg|thumb|250px|Dimension of a further [[fractal]] example. The [[Sierpinski triangle]], an object with Hausdorff dimension of log(3)/log(2)≈1.58.&amp;lt;ref name=ClaytonSCTPLS96/&amp;gt;]]&lt;br /&gt;
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Dimension of a further [[fractal example. The Sierpinski triangle, an object with Hausdorff dimension of log(3)/log(2)≈1.58.]]&lt;br /&gt;
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[[Image:谢尔宾斯基三角形 deep.svg|thumb|250px|进一步的[[分形维数]]的例子，进一步的分形维数的例子是谢尔宾斯基三角形，它是一个豪斯多夫维数为log(3)/log(2)≈1.58.&amp;lt;ref name=ClaytonSCTPLS96/&amp;gt;的物体]]&lt;br /&gt;
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* [[Countable set]]s have Hausdorff dimension 0.&amp;lt;ref name=&amp;quot;schleicher&amp;quot;&amp;gt;{{cite journal |last1=Schleicher |first1=Dierk |title=Hausdorff Dimension, Its Properties, and Its Surprises |journal=The American Mathematical Monthly |date=June 2007 |volume=114 |issue=6 |pages=509–528 |doi=10.1080/00029890.2007.11920440 |language=en |issn=0002-9890|arxiv=math/0505099 }}&amp;lt;/ref&amp;gt;&lt;br /&gt;
*[[可数集]]拥有豪斯多夫维数0.&amp;lt;ref name=&amp;quot;schleicher&amp;quot;&amp;gt;{{cite journal |last1=Schleicher |first1=Dierk |title=豪斯多夫维数, Its Properties, and Its Surprises |journal=The American Mathematical Monthly美国数学期刊 |date=June 2007 |volume=114 |issue=6 |pages=509–528 |doi=10.1080/00029890.2007.11920440 |language=en |issn=0002-9890|arxiv=math/0505099 }}&amp;lt;/ref&amp;gt;&lt;br /&gt;
* The [[Euclidean space]] ℝ&amp;lt;sup&amp;gt;''n''&amp;lt;/sup&amp;gt; has Hausdorff dimension ''n'', and the circle '''S'''&amp;lt;sup&amp;gt;1&amp;lt;/sup&amp;gt; has Hausdorff dimension 1.&amp;lt;ref name=&amp;quot;schleicher&amp;quot; /&amp;gt;&lt;br /&gt;
*[[教育空间]] ℝ&amp;lt;sup&amp;gt;''n''&amp;lt;/sup&amp;gt; 有豪斯多夫维数 ''n''，循环'''S'''&amp;lt;sup&amp;gt;1&amp;lt;/sup&amp;gt; 拥有豪斯多夫维数1.&amp;lt;ref name=&amp;quot;schleicher&amp;quot; /&amp;gt;&lt;br /&gt;
* [[Fractal]]s often are spaces whose Hausdorff dimension strictly exceeds the [[topological dimension]].&amp;lt;ref name=&amp;quot;mandelbrot&amp;quot; /&amp;gt; For example, the [[Cantor set]], a zero-dimensional topological space, is a union of two copies of itself, each copy shrunk by a factor 1/3; hence, it can be shown that its Hausdorff dimension is ln(2)/ln(3)&amp;amp;nbsp;≈&amp;amp;nbsp;0.63.&amp;lt;ref&amp;gt;{{cite book | last=Falconer | first = Kenneth |title=Fractal Geometry: Mathematical Foundations and Applications | publisher=[[John Wiley and Sons]] | edition=2nd | year=2003}}&amp;lt;/ref&amp;gt; The [[Sierpinski triangle]] is a union of three copies of itself, each copy shrunk by a factor of&amp;amp;nbsp;1/2; this yields a Hausdorff dimension of ln(3)/ln(2)&amp;amp;nbsp;≈&amp;amp;nbsp;1.58.&amp;lt;ref name=CampbellAnnenberg15/&amp;gt; These Hausdorff dimensions are related to the &amp;quot;critical exponent&amp;quot; of the [[Master theorem (analysis of algorithms)|Master theorem]] for solving [[Recurrence relation|recurrence relations]] in the [[analysis of algorithms]].&lt;br /&gt;
*[[分形]]一般是那些豪斯多夫维数直接超过其拓扑维数的空间。例如[[康托尔集]]是一个o维拓扑空间，由两个自己复制而成，每一个复制品都是原来的三分之一，因此它的豪斯多夫维数是 ln(2)/ln(3)&amp;amp;nbsp;≈&amp;amp;nbsp;0.63。&amp;lt;ref&amp;gt;{{cite book | last=Falconer | first = Kenneth |title=Fractal Geometry: Mathematical Foundations and Applications | publisher=[[John Wiley and Sons]] | edition=2nd | year=2003}}&amp;lt;/ref&amp;gt;一个[[谢尔宾斯基三角]]是他自身三个复制的组合。每一个是原来的&amp;amp;nbsp;1/2，它的豪斯多夫维数ln(3)/ln(2)&amp;amp;nbsp;≈&amp;amp;nbsp;1.58。&amp;lt;ref name=CampbellAnnenberg15/&amp;gt;在递归算法中解决递归关系时，这些豪斯多夫维数与[[算法分析主定理]]的临界指标相联系。&lt;br /&gt;
* [[Space-filling curve]]s like the [[Peano curve]] have the same Hausdorff dimension as the space they fill.&lt;br /&gt;
*[[空间填充曲线]]拥有和他们填充空间同样的豪斯多夫维数，如[[皮亚诺曲线]]。&lt;br /&gt;
* The trajectory of [[Brownian motion]] in dimension 2 and above is conjectured to be Hausdorff dimension 2.&amp;lt;ref&amp;gt;{{cite book | last=Morters | first=Peres | title= Brownian Motion | publisher=[[Cambridge University Press]] | year=2010 }}&amp;lt;/ref&amp;gt;&lt;br /&gt;
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[[image:Great Britain Hausdorff.svg|thumb|250px|Estimating the Hausdorff dimension of the [[How Long Is the Coast of Britain? Statistical Self-Similarity and Fractional Dimension|coast of Great Britain]]]]&lt;br /&gt;
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coast of Great Britain]]&lt;br /&gt;
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[[大不列颠海岸&lt;br /&gt;
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* 刘易斯·弗赖伊·理查森[[Lewis Fry Richardson]] has performed detailed experiments to measure the approximate Hausdorff dimension for various coastlines. His results have varied from 1.02 for the coastline of [[South Africa]] to 1.25 for the west coast of [[Great Britain]].&amp;lt;ref name=&amp;quot;mandelbrot&amp;quot; /&amp;gt;&lt;br /&gt;
*刘易斯·弗赖伊·理查森（Lewis Fry Richardson）已经通过豪斯多夫维数去测量了很多海岸线。它的结果涵盖从1.02的南非海岸线到1.25的大英帝国西海岸模型。]]&lt;br /&gt;
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==Properties of Hausdorff dimension豪斯多夫维数特性==&lt;br /&gt;
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{{refimprove section|date=March 2015}}&lt;br /&gt;
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=== Hausdorff dimension and inductive dimension 豪斯多夫维数和归纳维数===&lt;br /&gt;
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Let ''X'' be an arbitrary [[Separable space|separable]] metric space. There is a [[topology|topological]] notion of [[inductive dimension]] for ''X'' which is defined recursively. It is always an integer (or +∞) and is denoted dim&amp;lt;sub&amp;gt;ind&amp;lt;/sub&amp;gt;(''X'').&lt;br /&gt;
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Let X be an arbitrary separable metric space. There is a topological notion of inductive dimension for X which is defined recursively. It is always an integer (or +∞) and is denoted dim&amp;lt;sub&amp;gt;ind&amp;lt;/sub&amp;gt;(X).&lt;br /&gt;
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设''X'' 是[[任意可分度量空间]]。对于''X'' 有一个递归定义的归纳维数拓扑概念。它总是一个整数(或 + ∞) ，并且表示dim&amp;lt;sub&amp;gt;ind&amp;lt;/sub&amp;gt;(''X'')。&lt;br /&gt;
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'''Theorem'''. Suppose ''X'' is non-empty. Then &lt;br /&gt;
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Theorem. Suppose X is non-empty. Then &lt;br /&gt;
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'''定理'''：假设''X'' 是非空的。那么&lt;br /&gt;
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:&amp;lt;math&amp;gt; \dim_{\mathrm{Haus}}(X) \geq \dim_{\operatorname{ind}}(X). &amp;lt;/math&amp;gt;&lt;br /&gt;
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&amp;lt;math&amp;gt; \dim_{\mathrm{Haus}}(X) \geq \dim_{\operatorname{ind}}(X). &amp;lt;/math&amp;gt;&lt;br /&gt;
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Moreover,&lt;br /&gt;
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Moreover,&lt;br /&gt;
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此外,&lt;br /&gt;
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&amp;lt;math&amp;gt; \inf_Y \dim_{\operatorname{Haus}}(Y) =\dim_{\operatorname{ind}}(X), &amp;lt;/math&amp;gt;&lt;br /&gt;
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&amp;lt;math&amp;gt; \inf_Y \dim_{\operatorname{Haus}}(Y) =\dim_{\operatorname{ind}}(X), &amp;lt;/math&amp;gt;&lt;br /&gt;
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where ''Y'' ranges over metric spaces [[homeomorphic]] to ''X''. In other words, ''X'' and ''Y'' have the same underlying set of points and the metric ''d''&amp;lt;sub&amp;gt;''Y''&amp;lt;/sub&amp;gt; of ''Y'' is topologically equivalent to ''d''&amp;lt;sub&amp;gt;''X''&amp;lt;/sub&amp;gt;.&lt;br /&gt;
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where Y ranges over metric spaces homeomorphic to X. In other words, X and Y have the same underlying set of points and the metric d&amp;lt;sub&amp;gt;Y&amp;lt;/sub&amp;gt; of Y is topologically equivalent to d&amp;lt;sub&amp;gt;X&amp;lt;/sub&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
其中''Y''是度量空间同胚到 ''X''的范围。换句话说， ''X''和 ''Y''具有相同的基本点集，''Y''的度规''d''&amp;lt;sub&amp;gt;''Y''&amp;lt;/sub&amp;gt; 的子拓扑等价于''d''&amp;lt;sub&amp;gt;''X''&amp;lt;/sub&amp;gt;。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
These results were originally established by [[Edward Szpilrajn]] (1907–1976), e.g., see Hurewicz and Wallman, Chapter VII.{{full citation needed|date=March 2015}}&lt;br /&gt;
&lt;br /&gt;
These results were originally established by Edward Szpilrajn (1907–1976), e.g., see Hurewicz and Wallman, Chapter VII.&lt;br /&gt;
&lt;br /&gt;
这些结果最初是由 [[Edward Szpilrajn]] (1907–1976)建立的,  参见 Hurewicz and Wallman, Chapter VII.{{full citation needed|date=March 2015}}第七章。&lt;br /&gt;
&lt;br /&gt;
=== Hausdorff dimension and Minkowski dimension 豪斯多夫维数和闵可夫斯基维度===&lt;br /&gt;
&lt;br /&gt;
The [[Minkowski dimension]] is similar to, and at least as large as, the Hausdorff dimension, and they are equal in many situations. However, the set of [[rational number|rational]] points in [0, 1] has Hausdorff dimension zero and Minkowski dimension one. There are also compact sets for which the Minkowski dimension is strictly larger than the Hausdorff dimension.&lt;br /&gt;
&lt;br /&gt;
The Minkowski dimension is similar to, and at least as large as, the Hausdorff dimension, and they are equal in many situations. However, the set of rational points in [0, 1] has Hausdorff dimension zero and Minkowski dimension one. There are also compact sets for which the Minkowski dimension is strictly larger than the Hausdorff dimension.&lt;br /&gt;
&lt;br /&gt;
[[闵可夫斯基维数]]与豪斯多夫维数相似，至少和它一样大，而且在许多情况下是相等的。然而，[0,1]中有理点集的豪斯多夫维数为0，闵可夫斯基维数为1。还有一些紧集的闵可夫斯基维数绝对大于豪斯多夫维数。&lt;br /&gt;
&lt;br /&gt;
=== Hausdorff dimensions and Frostman measures 豪斯多夫维度和弗洛斯曼测度===&lt;br /&gt;
&lt;br /&gt;
If there is a [[measure (mathematics)|measure]] μ defined on [[Borel measure|Borel]] subsets of a metric space ''X'' such that ''μ''(''X'') &amp;gt; 0 and ''μ''(''B''(''x'', ''r'')) ≤ ''r&amp;lt;sup&amp;gt;s&amp;lt;/sup&amp;gt;'' holds for some constant ''s'' &amp;gt; 0 and for every ball ''B''(''x'', ''r'') in ''X'', then dim&amp;lt;sub&amp;gt;Haus&amp;lt;/sub&amp;gt;(''X'') ≥ ''s''. A partial converse is provided by [[Frostman's lemma]].{{citation needed|date=March 2015}}&amp;lt;ref&amp;gt;This Wikipedia article also discusses further useful characterizations of the Hausdorff dimension.{{clarify|date=March 2015}}&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
If there is a measure μ defined on Borel subsets of a metric space X such that μ(X) &amp;gt; 0 and μ(B(x, r)) ≤ r&amp;lt;sup&amp;gt;s&amp;lt;/sup&amp;gt; holds for some constant s &amp;gt; 0 and for every ball B(x, r) in X, then dim&amp;lt;sub&amp;gt;Haus&amp;lt;/sub&amp;gt;(X) ≥ s. A partial converse is provided by Frostman's lemma.&lt;br /&gt;
&lt;br /&gt;
如果在度量空间 ''X'' 的 Borel 子集上定义一个测度 μ，使得''μ''(''X'') &amp;gt; 0 和''μ''(''B''(''x'', ''r'')) ≤ ''r&amp;lt;sup&amp;gt;s&amp;lt;/sup&amp;gt;''，对于某个常数 ''s'' &amp;gt; 0  和 ''X'' 中的每个球 ''B''(''x'', ''r'') 成立，则 dim&amp;lt;sub&amp;gt;Haus&amp;lt;/sub&amp;gt;(''X'') ≥ ''s'' 。 部分逆向转换由弗洛斯曼引理定义。&lt;br /&gt;
&lt;br /&gt;
=== Behaviour under unions and products ===&lt;br /&gt;
&lt;br /&gt;
If &amp;lt;math&amp;gt;X=\bigcup_{i\in I}X_i&amp;lt;/math&amp;gt; is a finite or countable union, then&lt;br /&gt;
&lt;br /&gt;
If &amp;lt;math&amp;gt;X=\bigcup_{i\in I}X_i&amp;lt;/math&amp;gt; is a finite or countable union, then&lt;br /&gt;
&lt;br /&gt;
如果 &amp;lt;math&amp;gt;X=\bigcup_{i\in I}X_i&amp;lt;/math&amp;gt; 是一个有限或可数的联合，则&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \dim_{\operatorname{Haus}}(X) =\sup_{i\in I} \dim_{\operatorname{Haus}}(X_i).&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \dim_{\operatorname{Haus}}(X) =\sup_{i\in I} \dim_{\operatorname{Haus}}(X_i).&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
This can be verified directly from the definition.&lt;br /&gt;
&lt;br /&gt;
This can be verified directly from the definition.&lt;br /&gt;
&lt;br /&gt;
这可以直接从定义得到验证。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
If ''X'' and ''Y'' are non-empty metric spaces, then the Hausdorff dimension of their product satisfies&amp;lt;ref&amp;gt;{{cite journal |author=Marstrand, J. M. |title=The dimension of Cartesian product sets |journal=Proc. Cambridge Philos. Soc. |volume=50 |issue=3 |pages=198–202 |year=1954 |doi=10.1017/S0305004100029236 |bibcode = 1954PCPS...50..198M }}&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
If X and Y are non-empty metric spaces, then the Hausdorff dimension of their product satisfies&lt;br /&gt;
&lt;br /&gt;
如果 ''X'' 和''Y''是非空度量空间，那么它们乘积的豪斯多夫维数满足&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt; \dim_{\operatorname{Haus}}(X\times Y)\ge \dim_{\operatorname{Haus}}(X)+ \dim_{\operatorname{Haus}}(Y).&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \dim_{\operatorname{Haus}}(X\times Y)\ge \dim_{\operatorname{Haus}}(X)+ \dim_{\operatorname{Haus}}(Y).&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
This inequality can be strict. It is possible to find two sets of dimension 0 whose product has dimension 1.&amp;lt;ref&amp;gt;{{cite book  | last = Falconer  | first = Kenneth J.  | title = Fractal geometry. Mathematical foundations and applications  | publisher = John Wiley &amp;amp; Sons, Inc., Hoboken, New Jersey  | year = 2003  | doi =   | isbn = }}&amp;lt;/ref&amp;gt; In the opposite direction, it is known that when ''X'' and ''Y'' are Borel subsets of '''R'''&amp;lt;sup&amp;gt;''n''&amp;lt;/sup&amp;gt;, the Hausdorff dimension of ''X'' × ''Y'' is bounded from above by the Hausdorff dimension of ''X'' plus the [[packing dimension|upper packing dimension]] of ''Y''. These facts are discussed in Mattila (1995).&lt;br /&gt;
&lt;br /&gt;
This inequality can be strict. It is possible to find two sets of dimension 0 whose product has dimension 1. In the opposite direction, it is known that when X and Y are Borel subsets of R&amp;lt;sup&amp;gt;n&amp;lt;/sup&amp;gt;, the Hausdorff dimension of X × Y is bounded from above by the Hausdorff dimension of X plus the upper packing dimension of Y. These facts are discussed in Mattila (1995).&lt;br /&gt;
&lt;br /&gt;
这种不平等可以是绝对的。有可能找到两个维数为0的集合，其乘积的维数为1。相反，我们知道当''X''和''Y''是 '''R'''&amp;lt;sup&amp;gt;''n''&amp;lt;/sup&amp;gt;的 Borel 子集时， ''X'' × ''Y''的豪斯多夫维数从上面以 ''X''的豪斯多夫维数加上 ''Y''的填充维数为界。Mattila (1995)曾就这些情况进行了讨论。&lt;br /&gt;
&lt;br /&gt;
==Self-similar sets自相似集合==&lt;br /&gt;
&lt;br /&gt;
{{refimprove section|date=March 2015}}&lt;br /&gt;
&lt;br /&gt;
Many sets defined by a self-similarity condition have dimensions which can be determined explicitly. Roughly, a set ''E'' is self-similar if it is the fixed point of a set-valued transformation ψ, that is ψ(''E'') = ''E'', although the exact definition is given below.&lt;br /&gt;
&lt;br /&gt;
Many sets defined by a self-similarity condition have dimensions which can be determined explicitly. Roughly, a set E is self-similar if it is the fixed point of a set-valued transformation ψ, that is ψ(E) = E, although the exact definition is given below.&lt;br /&gt;
&lt;br /&gt;
许多由自相似条件定义的集合具有可以显式确定的维数。粗略地说，集合''E'' 是自相似的，如果它是集值ψ变换的不动点，即ψ(''E'') = ''E''，尽管下面给出了确切的定义。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&amp;lt;blockquote&amp;gt;'''Theorem'''. Suppose&lt;br /&gt;
&lt;br /&gt;
&amp;lt;blockquote&amp;gt;Theorem. Suppose&lt;br /&gt;
&lt;br /&gt;
&amp;lt;blockquote&amp;gt;'''定理'''：假设&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt; \psi_i: \mathbf{R}^n \rightarrow \mathbf{R}^n, \quad i=1, \ldots , m &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \psi_i: \mathbf{R}^n \rightarrow \mathbf{R}^n, \quad i=1, \ldots , m &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
are [[Contraction mapping|contractive]] mappings on '''R'''&amp;lt;sup&amp;gt;''n''&amp;lt;/sup&amp;gt; with contraction constant ''r&amp;lt;sub&amp;gt;j&amp;lt;/sub&amp;gt;'' &amp;lt; 1. Then there is a unique ''non-empty'' compact set ''A'' such that&lt;br /&gt;
&lt;br /&gt;
are contractive mappings on R&amp;lt;sup&amp;gt;n&amp;lt;/sup&amp;gt; with contraction constant r&amp;lt;sub&amp;gt;j&amp;lt;/sub&amp;gt; &amp;lt; 1. Then there is a unique non-empty compact set A such that&lt;br /&gt;
&lt;br /&gt;
是'''R'''&amp;lt;sup&amp;gt;''n''&amp;lt;/sup&amp;gt;上的压缩常数''r&amp;lt;sub&amp;gt;j&amp;lt;/sub&amp;gt;'&amp;lt; 1的压缩映射。然后有一个唯一的非空紧集A &lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt; A = \bigcup_{i=1}^m \psi_i (A). &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; A = \bigcup_{i=1}^m \psi_i (A). &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&amp;lt;/blockquote&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;/blockquote&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The theorem follows from [[Stefan Banach]]'s [[Contractive mapping theorem|contractive mapping fixed point theorem]] applied to the complete metric space of non-empty compact subsets of '''R'''&amp;lt;sup&amp;gt;''n''&amp;lt;/sup&amp;gt; with the [[Hausdorff distance]].&amp;lt;ref&amp;gt;{{cite book |author=Falconer, K. J. |title=The Geometry of Fractal Sets |publisher=Cambridge University Press |location=Cambridge, UK |year=1985 |isbn=0-521-25694-1 |chapter=Theorem 8.3}}&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
The theorem follows from Stefan Banach's contractive mapping fixed point theorem applied to the complete metric space of non-empty compact subsets of R&amp;lt;sup&amp;gt;n&amp;lt;/sup&amp;gt; with the Hausdorff distance.&lt;br /&gt;
&lt;br /&gt;
这个定理来源于 Stefan Banach 的压缩映射不动点定理，该定理应用于 '''R'''&amp;lt;sup&amp;gt;''n''&amp;lt;/sup&amp;gt; 的非空紧子集的完备空间豪斯多夫距离。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
===The open set condition开集条件===&lt;br /&gt;
&lt;br /&gt;
To determine the dimension of the self-similar set ''A'' (in certain cases), we need a technical condition called the ''open set condition'' (OSC) on the sequence of contractions ψ&amp;lt;sub&amp;gt;''i''&amp;lt;/sub&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
To determine the dimension of the self-similar set A (in certain cases), we need a technical condition called the open set condition (OSC) on the sequence of contractions ψ&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
为了确定自相似集''A'' 的维数(在某些情况下) ，我们需要一个称为''开集条件''(OSC)的技术条件ψ&amp;lt;sub&amp;gt;''i''&amp;lt;/sub&amp;gt;。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
There is a relatively compact open set ''V'' such that&lt;br /&gt;
&lt;br /&gt;
There is a relatively compact open set V such that&lt;br /&gt;
&lt;br /&gt;
有一个相对紧的开集''V''&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt; \bigcup_{i=1}^m\psi_i (V) \subseteq V, &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \bigcup_{i=1}^m\psi_i (V) \subseteq V, &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
where the sets in union on the left are pairwise [[disjoint sets|disjoint]].&lt;br /&gt;
&lt;br /&gt;
where the sets in union on the left are pairwise disjoint.&lt;br /&gt;
&lt;br /&gt;
左边的集合是成对不相交的。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The open set condition is a separation condition that ensures the images ψ&amp;lt;sub&amp;gt;''i''&amp;lt;/sub&amp;gt;(''V'') do not overlap &amp;quot;too much&amp;quot;.&lt;br /&gt;
&lt;br /&gt;
The open set condition is a separation condition that ensures the images ψ&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;(V) do not overlap &amp;quot;too much&amp;quot;.&lt;br /&gt;
&lt;br /&gt;
开集条件是保证图像子ψ&amp;lt;sub&amp;gt;''i''&amp;lt;/sub&amp;gt;(''V'') 不重叠“太多”的分离条件。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
'''Theorem'''. Suppose the open set condition holds and each ψ&amp;lt;sub&amp;gt;''i''&amp;lt;/sub&amp;gt; is a similitude, that is a composition of an [[isometry]] and a [[dilation (metric space)|dilation]] around some point. Then the unique fixed point of ψ is a set whose Hausdorff dimension is ''s'' where ''s'' is the unique solution of&amp;lt;ref&amp;gt;{{cite journal | last=Hutchinson | first=John E. | title=Fractals and self similarity | journal=Indiana Univ. Math. J. | volume=30 | year=1981 | pages=713–747 | doi=10.1512/iumj.1981.30.30055 | issue=5 | doi-access=free }}&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
Theorem. Suppose the open set condition holds and each ψ&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt; is a similitude, that is a composition of an isometry and a dilation around some point. Then the unique fixed point of ψ is a set whose Hausdorff dimension is s where s is the unique solution of&lt;br /&gt;
&lt;br /&gt;
'''定理'''假设开集条件成立，并且每个ψ&amp;lt;sub&amp;gt;''i''&amp;lt;/sub&amp;gt; 是一个相似量，这是一个等距和围绕某一点的膨胀的合成。那么唯一的不动点是一个集合，它的豪斯多夫维数是 ''s'' ，其中  ''s'' 是 ''s'' &amp;lt;ref&amp;gt;{{cite journal | last=Hutchinson | first=John E. | title=Fractals and self similarity | journal=Indiana Univ. Math. J. | volume=30 | year=1981 | pages=713–747 | doi=10.1512/iumj.1981.30.30055 | issue=5 | doi-access=free }}&amp;lt;/ref&amp;gt;的唯一解&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt; \sum_{i=1}^m r_i^s = 1. &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \sum_{i=1}^m r_i^s = 1. &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The contraction coefficient of a similitude is the magnitude of the dilation.&lt;br /&gt;
&lt;br /&gt;
The contraction coefficient of a similitude is the magnitude of the dilation.&lt;br /&gt;
&lt;br /&gt;
相似物的收缩系数就是膨胀的大小。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
We can use this theorem to compute the Hausdorff dimension of the Sierpinski triangle (or sometimes called Sierpinski gasket). Consider three [[non-collinear points]] ''a''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;, ''a''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;, ''a''&amp;lt;sub&amp;gt;3&amp;lt;/sub&amp;gt; in the plane '''R'''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; and let ψ&amp;lt;sub&amp;gt;''i''&amp;lt;/sub&amp;gt; be the dilation of ratio 1/2 around ''a&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;''. The unique non-empty fixed point of the corresponding mapping ψ is a Sierpinski gasket and the dimension ''s'' is the unique solution of&lt;br /&gt;
&lt;br /&gt;
We can use this theorem to compute the Hausdorff dimension of the Sierpinski triangle (or sometimes called Sierpinski gasket). Consider three non-collinear points a&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;, a&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;, a&amp;lt;sub&amp;gt;3&amp;lt;/sub&amp;gt; in the plane R&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; and let ψ&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt; be the dilation of ratio 1/2 around a&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;. The unique non-empty fixed point of the corresponding mapping ψ is a Sierpinski gasket and the dimension s is the unique solution of&lt;br /&gt;
&lt;br /&gt;
我们可以使用这个定理来计算谢尔宾斯基三角形的豪斯多夫维数(或者有时候叫做谢尔宾斯基垫圈)。考虑R&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; 平面上的三个非共线点，''a''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;，''a''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;，''a''&amp;lt;sub&amp;gt;3&amp;lt;/sub&amp;gt;，让ψ&amp;lt;sub&amp;gt;''i''&amp;lt;/sub&amp;gt;是围绕着''a&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;''膨胀比率的1/2。对应映射的唯一非空不动点是一个谢尔宾斯基垫圈，其维数''s''是对应映射的唯一解&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt; \left(\frac{1}{2}\right)^s+\left(\frac{1}{2}\right)^s+\left(\frac{1}{2}\right)^s = 3 \left(\frac{1}{2}\right)^s =1. &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \left(\frac{1}{2}\right)^s+\left(\frac{1}{2}\right)^s+\left(\frac{1}{2}\right)^s = 3 \left(\frac{1}{2}\right)^s =1. &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Taking [[natural logarithm]]s of both sides of the above equation, we can solve for ''s'', that is: ''s'' = ln(3)/ln(2).  The Sierpinski gasket is self-similar and satisfies the OSC. In general a set ''E'' which is a fixed point of a mapping&lt;br /&gt;
&lt;br /&gt;
Taking natural logarithms of both sides of the above equation, we can solve for s, that is: s = ln(3)/ln(2).  The Sierpinski gasket is self-similar and satisfies the OSC. In general a set E which is a fixed point of a mapping&lt;br /&gt;
&lt;br /&gt;
取上述方程两边的自然对数，我们可以求出 ''s''，即: ''s'' = ln(3)/ln(2)。该密封垫具有自相似性，满足 OSC 要求。一般来说，集合 ''E''是一个映射的不动点&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt; A \mapsto \psi(A) = \bigcup_{i=1}^m \psi_i(A) &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt; A \mapsto \psi(A) = \bigcup_{i=1}^m \psi_i(A) &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
is self-similar if and only if the intersections&lt;br /&gt;
&lt;br /&gt;
is self-similar if and only if the intersections&lt;br /&gt;
&lt;br /&gt;
是自相似的，当且仅当&lt;br /&gt;
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:&amp;lt;math&amp;gt; H^s\left(\psi_i(E) \cap \psi_j(E)\right) =0, &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; H^s\left(\psi_i(E) \cap \psi_j(E)\right) =0, &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
where ''s'' is the Hausdorff dimension of ''E'' and ''H&amp;lt;sup&amp;gt;s&amp;lt;/sup&amp;gt;'' denotes [[Hausdorff measure]]. This is clear in the case of the Sierpinski gasket (the intersections are just points), but is also true more generally:&lt;br /&gt;
&lt;br /&gt;
where s is the Hausdorff dimension of E and H&amp;lt;sup&amp;gt;s&amp;lt;/sup&amp;gt; denotes Hausdorff measure. This is clear in the case of the Sierpinski gasket (the intersections are just points), but is also true more generally:&lt;br /&gt;
&lt;br /&gt;
其中 ''s''是''E''的豪斯多夫维数， ''E'' and ''H&amp;lt;sup&amp;gt;s&amp;lt;/sup&amp;gt;'' 表示 豪斯多夫测度。对于谢尔宾斯基垫圈(交叉点就是点)来说，这一点很明显，但更普遍的情况是:&lt;br /&gt;
&lt;br /&gt;
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&lt;br /&gt;
'''Theorem'''. Under the same conditions as the previous theorem, the unique fixed point of ψ is self-similar.&lt;br /&gt;
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Theorem. Under the same conditions as the previous theorem, the unique fixed point of ψ is self-similar.&lt;br /&gt;
&lt;br /&gt;
'''定理'''：在与前一定理相同的条件下，其唯一不动点是自相似的。&lt;br /&gt;
&lt;br /&gt;
==See also参阅==&lt;br /&gt;
&lt;br /&gt;
* [[List of fractals by Hausdorff dimension豪斯多夫分形维数列表]] Examples of deterministic fractals, random and natural fractals.确定性分形与随机和自然分形的示例。&lt;br /&gt;
&lt;br /&gt;
* [[Assouad dimension  Assouad维数]], another variation of fractal dimension that, like Hausdorff dimension, is defined using coverings by balls其他被球覆盖方式定义的分形维数，例如豪斯多夫维数。&lt;br /&gt;
&lt;br /&gt;
* [[Intrinsic dimension固有维数]]&lt;br /&gt;
&lt;br /&gt;
* [[Packing dimension填充维数]]&lt;br /&gt;
&lt;br /&gt;
* [[Fractal dimension分形维数]]&lt;br /&gt;
&lt;br /&gt;
==References参考文献==&lt;br /&gt;
&lt;br /&gt;
{{reflist}}&lt;br /&gt;
&lt;br /&gt;
==Further reading拓展阅读==&lt;br /&gt;
&lt;br /&gt;
* {{cite book |last1=Dodson |first1=M. Maurice |title=Fractal Geometry and Applications: A Jubilee of Benoît Mandelbrot |volume=72 |issue=1 |pages=305–347 |last2=Kristensen |first2=Simon |chapter=Hausdorff Dimension and Diophantine Approximation |date=June 12, 2003 |arxiv=math/0305399 |bibcode = 2003math......5399D |doi=10.1090/pspum/072.1/2112110|series=Proceedings of Symposia in Pure Mathematics |isbn=9780821836378 }}&lt;br /&gt;
&lt;br /&gt;
* {{cite book |last1=Hurewicz |first1=Witold |authorlink1=Witold Hurewicz |last2=Wallman |first2=Henry |authorlink2=Henry Wallman |title=Dimension Theory |url=https://archive.org/details/in.ernet.dli.2015.84609 |publisher=Princeton University Press |year=1948 }}&lt;br /&gt;
&lt;br /&gt;
* {{cite journal |author作者=E. Szpilrajn |authorlink=Edward Marczewski |title=La dimension et la mesure |journal=Fundamenta Mathematicae |volume=28 |pages=81–9 |year=1937 }}&lt;br /&gt;
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* {{cite journal&lt;br /&gt;
&lt;br /&gt;
 | last1=Marstrand&lt;br /&gt;
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 | last1=Marstrand&lt;br /&gt;
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 | last1=马斯特兰德&lt;br /&gt;
&lt;br /&gt;
 | first1=J. M. | title=The dimension of cartesian product sets | year=1954 | journal=Proc. Cambridge Philos. Soc.&lt;br /&gt;
&lt;br /&gt;
 | first1=J. M. | title=The dimension of cartesian product sets | year=1954 | journal=Proc. Cambridge Philos. Soc.&lt;br /&gt;
&lt;br /&gt;
 | first1= J. M. | title=笛卡儿积集的维数 | 1954年 |  journal=Proc. Cambridge Philos. Soc.&lt;br /&gt;
&lt;br /&gt;
 | volume=50&lt;br /&gt;
&lt;br /&gt;
 | volume=50&lt;br /&gt;
&lt;br /&gt;
 | 第50卷&lt;br /&gt;
&lt;br /&gt;
 | issue=3&lt;br /&gt;
&lt;br /&gt;
 | issue=3&lt;br /&gt;
&lt;br /&gt;
 | 第三期&lt;br /&gt;
&lt;br /&gt;
 | pages=198–202&lt;br /&gt;
&lt;br /&gt;
 | pages=198–202&lt;br /&gt;
&lt;br /&gt;
 | 第198-202页&lt;br /&gt;
&lt;br /&gt;
 | doi=10.1017/S0305004100029236|bibcode = 1954PCPS...50..198M }}&lt;br /&gt;
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 | doi=10.1017/S0305004100029236|bibcode = 1954PCPS...50..198M }}&lt;br /&gt;
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10.1017 / S0305004100029236 | bibcode 1954PCPS... 50. . 198 m }&lt;br /&gt;
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* {{Cite book&lt;br /&gt;
&lt;br /&gt;
 | last1=Mattila&lt;br /&gt;
&lt;br /&gt;
 | last1=Mattila&lt;br /&gt;
&lt;br /&gt;
 | last1=Mattila&lt;br /&gt;
&lt;br /&gt;
 | first1=Pertti | author1-link=Pertti Mattila| title=Geometry of sets and measures in Euclidean spaces | publisher=[[Cambridge University Press]]&lt;br /&gt;
&lt;br /&gt;
 | first1=Pertti | author1-link=Pertti Mattila| title=Geometry of sets and measures in Euclidean spaces | publisher=Cambridge University Press&lt;br /&gt;
&lt;br /&gt;
| first1 Pertti | author1-link Pertti Mattila | title 欧几里德空间中集合和度量的几何 | 出版商剑桥大学出版社&lt;br /&gt;
&lt;br /&gt;
 | isbn=978-0-521-65595-8 | year=1995}}&lt;br /&gt;
&lt;br /&gt;
 | isbn=978-0-521-65595-8 | year=1995}}&lt;br /&gt;
&lt;br /&gt;
| isbn 978-0-521-65595-8 | year 1995}&lt;br /&gt;
&lt;br /&gt;
* {{cite journal |author=A. S. Besicovitch |authorlink=A. S. Besicovitch |title=On Linear Sets of Points of Fractional Dimensions |journal=[[Mathematische Annalen]] |volume=101 |year=1929 | doi=10.1007/BF01454831| issue=1 |pages= 161–193}}&lt;br /&gt;
&lt;br /&gt;
* {{cite journal |author1=A. S. Besicovitch |authorlink1=A. S. Besicovitch |author2=H. D. Ursell |authorlink2=H. D. Ursell |title=Sets of Fractional Dimensions |journal=Journal of the London Mathematical Society |volume=12 |year=1937 | issue=1 | doi=10.1112/jlms/s1-12.45.18  | pages=18–25 }}&amp;lt;br/&amp;gt;Several selections from this volume are reprinted in {{cite book |author=Edgar, Gerald A. |title=Classics on fractals |publisher=Addison-Wesley |location=Boston |year=1993 |isbn=0-201-58701-7}} See chapters 9,10,11&lt;br /&gt;
&lt;br /&gt;
* {{cite journal |author=F. Hausdorff |authorlink=F. Hausdorff |title=Dimension und äußeres Maß |journal=Mathematische Annalen |volume=79 |issue=1–2 |pages=157–179 |date=March 1919 |doi=10.1007/BF01457179|hdl=10338.dmlcz/100363 |url=http://dml.cz/bitstream/handle/10338.dmlcz/100363/CzechMathJ_09-1959-3_5.pdf }}&lt;br /&gt;
&lt;br /&gt;
* {{cite journal | last=Hutchinson | first=John E. | title=Fractals and self similarity | journal=Indiana Univ. Math. J. | volume=30 | year=1981 | pages=713–747 | doi=10.1512/iumj.1981.30.30055 | issue=5 | doi-access=free }}&lt;br /&gt;
&lt;br /&gt;
*{{cite book | last=Falconer | first = Kenneth |title=Fractal Geometry: Mathematical Foundations and Applications | publisher=[[John Wiley and Sons]] | edition=2nd | year=2003}}&lt;br /&gt;
&lt;br /&gt;
==External links外部链接==&lt;br /&gt;
&lt;br /&gt;
* [https://www.encyclopediaofmath.org/index.php/Hausdorff_dimension Hausdorff dimension] 在 [https://www.encyclopediaofmath.org/ Encyclopedia of Mathematics]&lt;br /&gt;
&lt;br /&gt;
* [https://www.encyclopediaofmath.org/index.php/Hausdorff_measure Hausdorff measure] 在 [https://www.encyclopediaofmath.org/ Encyclopedia of Mathematics]&lt;br /&gt;
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{{DEFAULTSORT:Hausdorff Dimension豪斯多夫维数}}&lt;br /&gt;
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[[Category分类:Fractals分形]]&lt;br /&gt;
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[[Category分类:Metric geometry度量几何]]&lt;br /&gt;
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[[Category分类:Dimension theory维度理论]]&lt;br /&gt;
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&amp;lt;noinclude&amp;gt;&lt;br /&gt;
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&amp;lt;small&amp;gt;This page was moved from [[wikipedia:en:Hausdorff dimension]]. Its edit history can be viewed at [[分形维数/edithistory]]&amp;lt;/small&amp;gt;&amp;lt;/noinclude&amp;gt;&lt;br /&gt;
&lt;br /&gt;
[[Category:待整理页面]]&lt;/div&gt;</summary>
		<author><name>Ruili</name></author>
	</entry>
	<entry>
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		<title>分形维数</title>
		<link rel="alternate" type="text/html" href="https://wiki.swarma.org/index.php?title=%E5%88%86%E5%BD%A2%E7%BB%B4%E6%95%B0&amp;diff=17267"/>
		<updated>2020-10-27T15:33:55Z</updated>

		<summary type="html">&lt;p&gt;Ruili：&lt;/p&gt;
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&lt;div&gt;此词条暂由彩云小译翻译，未经人工整理和审校，带来阅读不便，请见谅。&lt;br /&gt;
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{{short description|Invariant}}&lt;br /&gt;
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[[File:KochFlake.svg|thumb|280px|Example of non-integer dimensions. The first four [[iteration]]s of the [[Koch snowflake|Koch curve]], where after each iteration, all original line segments are replaced with four, each a self-similar copy that is 1/3 the length of the original. One formalism of the Hausdorff dimension uses this scale factor (3) and the number of self-similar objects (4) to calculate the dimension, D, after the first iteration to be D = (log N)/(log S) = (log 4)/(log 3) ≈ 1.26.&amp;lt;ref name=CampbellAnnenberg15&amp;gt;MacGregor Campbell, 2013, &amp;quot;5.6 Scaling and the Hausdorff Dimension,&amp;quot; at ''Annenberg Learner:MATHematics illuminated'', see [http://www.learner.org/courses/mathilluminated/units/5/textbook/06.php], accessed 5 March 2015.&amp;lt;/ref&amp;gt; That is, while the Hausdorff dimension of a single [[point (geometry)|point]] is zero, of a [[line segment]] is 1, of a [[square]] is 2, and of a [[cube]] is 3, for [[fractal]]s such as this, the object can have a non-integer dimension.]]&lt;br /&gt;
&lt;br /&gt;
Example of non-integer dimensions. The first four [[iterations of the Koch curve, where after each iteration, all original line segments are replaced with four, each a self-similar copy that is 1/3 the length of the original. One formalism of the Hausdorff dimension uses this scale factor (3) and the number of self-similar objects (4) to calculate the dimension, D, after the first iteration to be D = (log N)/(log S) = (log 4)/(log 3) ≈ 1.26. That is, while the Hausdorff dimension of a single point is zero, of a line segment is 1, of a square is 2, and of a cube is 3, for fractals such as this, the object can have a non-integer dimension.]]&lt;br /&gt;
&lt;br /&gt;
File:KochFlake.svg|thumb|280px|非整数维度示例：前四个[[Koch 曲线]]的迭代，在每次迭代后，所有原始线段都被替换为四个，每个自相似的复制是原始线段长度的1 / 3。豪斯多夫维数的一个建模是使用这个比例因子(3)和自相似物体的数量(4)来计算维度，设在第一次迭代后为 D = (log N)/(log S) = (log 4)/(log 3) ≈ 1.26.&amp;lt;ref name=CampbellAnnenberg15&amp;gt;。MacGregor Campbell, 2013, &amp;quot;5.6 Scaling and the Hausdorff Dimension,&amp;quot; 在 ''Annenberg Learner:MATHematics illuminated'', 参见 [http://www.learner.org/courses/mathilluminated/units/5/textbook/06.php], accessed 5 March 2015.&amp;lt;/ref&amp;gt; 也就是说，当一个点的豪斯多夫维数为零，线段为1，正方形为2，立方体为3时，对于像这样的分形，物体可以有一个非整数维度。]]&lt;br /&gt;
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In [[mathematics]], '''Hausdorff dimension''' is a measure of ''roughness'', or more specifically, [[fractal dimension]], that was first introduced in 1918 by [[mathematician]] [[Felix Hausdorff]].&amp;lt;ref&amp;gt;{{Cite journal |arxiv = 1101.1444|doi = 10.1214/11-STS370|title = Estimators of Fractal Dimension: Assessing the Roughness of Time Series and Spatial Data|journal = Statistical Science|volume = 27|issue = 2|pages = 247–277|year = 2012|last1 = Gneiting|first1 = Tilmann|last2 = Ševčíková|first2 = Hana|last3 = Percival|first3 = Donald B.}}&amp;lt;/ref&amp;gt; For instance, the Hausdorff dimension of a single [[point (geometry)|point]] is zero, of a [[line segment]] is 1, of a [[square]] is 2, and of a [[cube]] is 3. That is, for sets of points that define a smooth shape or a shape that has a small number of corners—the shapes of traditional geometry and science—the Hausdorff dimension is an [[integer]] agreeing with the usual sense of dimension, also known as the [[Inductive dimension|topological dimension]]. However, formulas have also been developed that allow calculation of the dimension of other less simple objects, where, solely on the basis of their properties of [[scaling (geometry)|scaling]] and [[self-similarity]], one is led to the conclusion that particular objects—including [[fractal]]s—have non-integer Hausdorff dimensions. Because of the significant technical advances made by [[Abram Samoilovitch Besicovitch]] allowing computation of dimensions for highly irregular or &amp;quot;rough&amp;quot; sets, this dimension is also commonly referred to as the ''Hausdorff–Besicovitch dimension.''&lt;br /&gt;
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In mathematics, Hausdorff dimension is a measure of roughness, or more specifically, fractal dimension, that was first introduced in 1918 by mathematician Felix Hausdorff. For instance, the Hausdorff dimension of a single point is zero, of a line segment is 1, of a square is 2, and of a cube is 3. That is, for sets of points that define a smooth shape or a shape that has a small number of corners—the shapes of traditional geometry and science—the Hausdorff dimension is an integer agreeing with the usual sense of dimension, also known as the topological dimension. However, formulas have also been developed that allow calculation of the dimension of other less simple objects, where, solely on the basis of their properties of scaling and self-similarity, one is led to the conclusion that particular objects—including fractals—have non-integer Hausdorff dimensions. Because of the significant technical advances made by Abram Samoilovitch Besicovitch allowing computation of dimensions for highly irregular or &amp;quot;rough&amp;quot; sets, this dimension is also commonly referred to as the Hausdorff–Besicovitch dimension.&lt;br /&gt;
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在[[数学]]中，'''&amp;lt;font color = '#ff8000'&amp;gt;豪斯多夫维数Hausdorff dimension&amp;lt;/font&amp;gt;'''是一种粗糙度的度量单位，或者更确切地说，分形维数，是由数学家 Felix Hausdorff 在1918年首次提出的。例如，单点的豪斯多夫维数为零，线段为1，正方形为2，立方体为3。也就是说，对于定义了一个光滑形状或一个有少数几个角的形状---- 传统几何学和科学的形状---- 的点集来说，豪斯多夫维数是一个整数，符合通常的维度意义，也称为拓扑维度。然而，还有一些公式允许计算其他不太简单的对象的维数，其中仅仅根据它们的标度和自相似特性，就可以得出结论: 特定的对象ー包括分形ー具有非整数的 Hausdorff 维数。由于阿布拉姆·萨莫伊洛维奇·贝西科维奇的重大技术进步，允许计算高度不规则或“粗糙”集的维度，这个维度通常也被称为 Hausdorff-Besicovitch 维度。 &lt;br /&gt;
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The Hausdorff dimension, more specifically, is a further dimensional number associated with a given set, where the distances between all members of that set are defined. Such a set is termed a [[metric space]]. The dimension is drawn from the [[Extended real number line|extended real numbers]], &amp;lt;math&amp;gt;\overline{\mathbb{R}}&amp;lt;/math&amp;gt;, as opposed to the more intuitive notion of dimension, which is not associated to general metric spaces, and only takes values in the non-negative integers.&lt;br /&gt;
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The Hausdorff dimension, more specifically, is a further dimensional number associated with a given set, where the distances between all members of that set are defined. Such a set is termed a metric space. The dimension is drawn from the extended real numbers, &amp;lt;math&amp;gt;\overline{\mathbb{R}}&amp;lt;/math&amp;gt;, as opposed to the more intuitive notion of dimension, which is not associated to general metric spaces, and only takes values in the non-negative integers.&lt;br /&gt;
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更具体地说，豪斯多夫维数是一个与给定集合相关联的更进一步的维数，其中定义了该集合所有成员之间的距离。这样的集合称为度量空间。维数是从扩展的实数，&amp;lt;math&amp;gt;\overline{\mathbb{R}}&amp;lt;/math&amp;gt;，而不是更直观的维数概念(它不与一般的度量空间相关联，只取非负整数的值)。&lt;br /&gt;
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In mathematical terms, the Hausdorff dimension generalizes the notion of the dimension of a real [[vector space]]. That is, the Hausdorff dimension of an ''n''-dimensional [[inner product space]] equals ''n''. This underlies the earlier statement that the Hausdorff dimension of a point is zero, of a line is one, etc., and that [[fractal|irregular sets]] can have noninteger Hausdorff dimensions. For instance, the [[Koch snowflake]] shown at right is constructed from an equilateral triangle; in each iteration, its component line segments are divided into 3 segments of unit length, the newly created middle segment is used as the base of a new [[equilateral]] triangle that points outward, and this base segment is then deleted to leave a final object from the iteration of unit length of 4.&amp;lt;ref&amp;gt;Larry Riddle, 2014, &amp;quot;Classic Iterated Function Systems: Koch Snowflake&amp;quot;, Agnes Scott College e-Academy (online), see [http://ecademy.agnesscott.edu/~lriddle/ifs/ksnow/ksnow.htm], accessed 5 March 2015.&amp;lt;/ref&amp;gt; That is, after the first iteration, each original line segment has been replaced with N=4, where each self-similar copy is 1/S = 1/3 as long as the original.&amp;lt;ref name=CampbellAnnenberg15/&amp;gt; Stated another way, we have taken an object with Euclidean dimension, D, and reduced its linear scale by 1/3 in each direction, so that its length increases to N=S&amp;lt;sup&amp;gt;D&amp;lt;/sup&amp;gt;.&amp;lt;ref name=ClaytonSCTPLS96&amp;gt;Keith Clayton, 1996, &amp;quot;Fractals and the Fractal Dimension,&amp;quot; ''Basic Concepts in Nonlinear Dynamics and Chaos'' (workshop), Society for Chaos Theory in Psychology and the Life Sciences annual meeting, June 28, 1996, Berkeley, California, see [http://www.vanderbilt.edu/AnS/psychology/cogsci/chaos/workshop/Workshop.html], accessed 5 March 2015.&amp;lt;/ref&amp;gt; This equation is easily solved for D, yielding the ratio of logarithms (or [[natural logarithm]]s) appearing in the figures, and giving—in the Koch and other fractal cases—non-integer dimensions for these objects.&lt;br /&gt;
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In mathematical terms, the Hausdorff dimension generalizes the notion of the dimension of a real vector space. That is, the Hausdorff dimension of an n-dimensional inner product space equals n. This underlies the earlier statement that the Hausdorff dimension of a point is zero, of a line is one, etc., and that irregular sets can have noninteger Hausdorff dimensions. For instance, the Koch snowflake shown at right is constructed from an equilateral triangle; in each iteration, its component line segments are divided into 3 segments of unit length, the newly created middle segment is used as the base of a new equilateral triangle that points outward, and this base segment is then deleted to leave a final object from the iteration of unit length of 4. That is, after the first iteration, each original line segment has been replaced with N=4, where each self-similar copy is 1/S = 1/3 as long as the original. This equation is easily solved for D, yielding the ratio of logarithms (or natural logarithms) appearing in the figures, and giving—in the Koch and other fractal cases—non-integer dimensions for these objects.&lt;br /&gt;
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用数学术语来说，豪斯多夫维数概括了实向量空间维数的概念。也就是说，n 维内积空间的豪斯多夫维数等于 n。 这就是早期假设的基础，一个点的豪斯多夫维数是零，一条线是一等等，不规则集可以有非整数的豪斯多夫维数。例如，右边所示的 Koch 雪花是由一个正三角形构成的; 在每次迭代中，它的组成线段被分成单位长度的3段，新创建的中间线段被用作一个指向外部的新正三角形的基础，然后人们删除这个基础线段用来保留单位长度4的迭代中的最终对象。也就是说，在第一次迭代之后，每个原始线段都被替换为 N=4，其中每个自相似拷贝的长度是原始线段的1/S = 1/3 。这个方程很容易求解为 D，产生出现在图形中的对数(或自然对数)的比率，并给出——在 Koch 和其他分形情况下——这些对象的非整数维数。&lt;br /&gt;
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The Hausdorff dimension is a successor to the simpler, but usually equivalent, box-counting or [[Minkowski–Bouligand dimension]].&lt;br /&gt;
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The Hausdorff dimension is a successor to the simpler, but usually equivalent, box-counting or Minkowski–Bouligand dimension.&lt;br /&gt;
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豪斯多夫维数是更简单但通常等价的'''&amp;lt;font color = '#ff8000'&amp;gt;计盒维数box-counting&amp;lt;/font&amp;gt;'''或'''&amp;lt;font color = '#ff8000'&amp;gt;闵可夫斯基维数Minkowski-Bouligand&amp;lt;/font&amp;gt;'''的继承者。&lt;br /&gt;
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==Intuition概念==&lt;br /&gt;
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The intuitive concept of dimension of a geometric object ''X'' is the number of independent parameters one needs to pick out a unique point inside. However, any point specified by two parameters can be instead specified by one, because the [[cardinality]] of the [[real plane]] is equal to the cardinality of the [[real line]] (this can be seen by an [[Cantor's diagonal argument|argument]] involving interweaving the digits of two numbers to yield a single number encoding the same information). The example of a [[space-filling curve]] shows that one can even map the real line to the real plane [[Surjective function|surjectively]] (taking one real number into a pair of real numbers in a way so that all pairs of numbers are covered) and ''continuously'', so that a one-dimensional object completely fills up a higher-dimensional object.&lt;br /&gt;
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The intuitive concept of dimension of a geometric object X is the number of independent parameters one needs to pick out a unique point inside. However, any point specified by two parameters can be instead specified by one, because the cardinality of the real plane is equal to the cardinality of the real line (this can be seen by an argument involving interweaving the digits of two numbers to yield a single number encoding the same information). The example of a space-filling curve shows that one can even map the real line to the real plane surjectively (taking one real number into a pair of real numbers in a way so that all pairs of numbers are covered) and continuously, so that a one-dimensional object completely fills up a higher-dimensional object.&lt;br /&gt;
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几何物体X的直观尺寸概念就是一个物体需要多少个独立参数才能找到一个独特的点。但是，任何由两个参数指定的点都可以由一个参数指定，因为实际平面的基数等于实际行的基数(这可以通过一个参数看到，该参数涉及交织两个数字的数字以产生一个编码相同信息的单个数字)。'''&amp;lt;font color = '#ff8000'&amp;gt;皮亚诺曲线&amp;lt;/font&amp;gt;'''的例子表明，一个人甚至可以完美和连续地映射实际线到真正的平面(把一个实数转换成一对实数，这样所有的数对都被覆盖)，由此一维物体完全填充了一个高维物体。&lt;br /&gt;
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Every space filling curve hits some points multiple times, and does not have a continuous inverse. It is impossible to map two dimensions onto one in a way that is continuous and continuously invertible. The topological dimension, also called [[Lebesgue covering dimension]], explains why. This dimension is ''n'' if, in every covering of ''X'' by small open balls, there is at least one point where ''n''&amp;amp;nbsp;+&amp;amp;nbsp;1 balls overlap. For example, when one covers a line with short open intervals, some points must be covered twice, giving dimension&amp;amp;nbsp;''n''&amp;amp;nbsp;=&amp;amp;nbsp;1.&lt;br /&gt;
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Every space filling curve hits some points multiple times, and does not have a continuous inverse. It is impossible to map two dimensions onto one in a way that is continuous and continuously invertible. The topological dimension, also called Lebesgue covering dimension, explains why. This dimension is n if, in every covering of X by small open balls, there is at least one point where n&amp;amp;nbsp;+&amp;amp;nbsp;1 balls overlap. For example, when one covers a line with short open intervals, some points must be covered twice, giving dimension&amp;amp;nbsp;n&amp;amp;nbsp;=&amp;amp;nbsp;1.&lt;br /&gt;
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每条空间填充曲线都会多次撞击某些点，且不存在连续的倒数。将两个维度以连续和连续可逆的方式映射到一个维度是不可能的。'''&amp;lt;font color = '#ff8000'&amp;gt;拓扑维度 topological dimension&amp;lt;/font&amp;gt;'''，也被称为拓朴维数，解释了为什么。这个维度是 n，如果在 x 的每个小开球覆盖中，至少有一个点 n + 1个球重叠。例如，当一个点覆盖一条具有短开区间的直线时，某些点必须被覆盖两次，给出维数''n''&amp;amp;nbsp;=&amp;amp;nbsp;1。&lt;br /&gt;
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But topological dimension is a very crude measure of the local size of a space (size near a point). A curve that is almost space-filling can still have topological dimension one, even if it fills up most of the area of a region. A [[fractal]] has an integer topological dimension, but in terms of the amount of space it takes up, it behaves like a higher-dimensional space.&lt;br /&gt;
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But topological dimension is a very crude measure of the local size of a space (size near a point). A curve that is almost space-filling can still have topological dimension one, even if it fills up most of the area of a region. A fractal has an integer topological dimension, but in terms of the amount of space it takes up, it behaves like a higher-dimensional space.&lt;br /&gt;
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但是，拓扑维度是对空间局部尺寸(点附近的尺寸)的一个非常粗略的度量。一条几乎是空间填充的曲线仍然可以有一维拓扑，即使它填充了一个区域的大部分面积。分形具有整数的拓扑维数，但就其所占空间的数量而言，它看起来像一个更高维的空间。&lt;br /&gt;
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The Hausdorff dimension measures the local size of a space taking into account the distance between points, the [[metric space|metric]]. Consider the number ''N''(''r'') of [[ball (mathematics)|balls]] of radius at most ''r'' required to cover ''X'' completely. When ''r'' is very small, ''N''(''r'') grows polynomially with 1/''r''. For a sufficiently well-behaved  ''X'', the Hausdorff dimension is the unique number ''d'' such that N(''r'') grows as 1/''r&amp;lt;sup&amp;gt;d&amp;lt;/sup&amp;gt;'' as ''r'' approaches zero. More precisely, this defines the [[Minkowski–Bouligand dimension|box-counting dimension]], which equals the Hausdorff dimension when the value ''d'' is a critical boundary between growth rates that are insufficient to cover the space, and growth rates that are overabundant.&lt;br /&gt;
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The Hausdorff dimension measures the local size of a space taking into account the distance between points, the metric. Consider the number N(r) of balls of radius at most r required to cover X completely. When r is very small, N(r) grows polynomially with 1/r. For a sufficiently well-behaved  X, the Hausdorff dimension is the unique number d such that N(r) grows as 1/r&amp;lt;sup&amp;gt;d&amp;lt;/sup&amp;gt; as r approaches zero. More precisely, this defines the box-counting dimension, which equals the Hausdorff dimension when the value d is a critical boundary between growth rates that are insufficient to cover the space, and growth rates that are overabundant.&lt;br /&gt;
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豪斯多夫维数测量一个空间的局部大小时，会考虑到点之间距离的度量。考虑半径最大为 r 的球数 ''N'' (r) ，需要完全覆盖 ''X''。当 r 很小时，n (r)以1/''r'' 增长多项式。对于一个表现足够好的 ''X''，豪斯多夫维数是唯一的数 d，这样当 r 趋近于零时， N(r)增长为1/r&amp;lt;sup&amp;gt;d&amp;lt;/sup&amp;gt; 。更确切地说，这定义了盒子计数维度，当值 d 是不足以覆盖空间的增长率和过度充裕的增长率之间的关键边界时，它等于豪斯多夫维数。&lt;br /&gt;
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For shapes that are smooth, or shapes with a small number of corners, the shapes of traditional geometry and science, the Hausdorff dimension is an integer agreeing with the topological dimension. But [[Benoit Mandelbrot]] observed that [[fractal]]s, sets with noninteger Hausdorff dimensions, are found everywhere in nature. He observed that the proper idealization of most rough shapes you see around you is not in terms of smooth idealized shapes, but in terms of fractal idealized shapes:&lt;br /&gt;
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For shapes that are smooth, or shapes with a small number of corners, the shapes of traditional geometry and science, the Hausdorff dimension is an integer agreeing with the topological dimension. But Benoit Mandelbrot observed that fractals, sets with noninteger Hausdorff dimensions, are found everywhere in nature. He observed that the proper idealization of most rough shapes you see around you is not in terms of smooth idealized shapes, but in terms of fractal idealized shapes:&lt;br /&gt;
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对于光滑的形状，或者有少量棱角的形状，传统几何和科学的形状，豪斯多夫维数是一个整数，与拓扑维度一致。但是伯努·曼德布洛特观察到分形---- 具有非整数豪斯多夫维数的集合---- 在自然界中随处可见。他观察到，我们周围大多数粗糙形状的理想化不是光滑的理想化形状，而是分形理想化形状:&lt;br /&gt;
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&amp;lt;blockquote&amp;gt;Clouds are not spheres, mountains are not cones, coastlines are not circles, and bark is not smooth, nor does lightning travel in a straight line.&amp;lt;ref name=&amp;quot;mandelbrot&amp;quot;&amp;gt;{{cite book   | last = Mandelbrot   | first = Benoît   | authorlink = Benoit Mandelbrot   | title = The Fractal Geometry of Nature   | publisher = W. H. Freeman   | series = Lecture notes in mathematics 1358   | year = 1982   | doi =    | isbn = 0-7167-1186-9   | url-access = registration   | url = https://archive.org/details/fractalgeometryo00beno   }}&amp;lt;/ref&amp;gt;&amp;lt;/blockquote&amp;gt;&lt;br /&gt;
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&amp;lt;blockquote&amp;gt;Clouds are not spheres, mountains are not cones, coastlines are not circles, and bark is not smooth, nor does lightning travel in a straight line.&amp;lt;/blockquote&amp;gt;&lt;br /&gt;
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&amp;lt;blockquote&amp;gt;云不是球体，山不是锥体，海岸线不是圆圈，树皮不平滑，闪电也不是直线运动。 &amp;lt;/blockquote&amp;gt;&lt;br /&gt;
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For fractals that occur in nature, the Hausdorff and [[Minkowski–Bouligand dimension|box-counting dimension]] coincide. The [[packing dimension]] is yet another similar notion which gives the same value for many shapes, but there are well documented exceptions where all these dimensions differ.&lt;br /&gt;
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For fractals that occur in nature, the Hausdorff and box-counting dimension coincide. The packing dimension is yet another similar notion which gives the same value for many shapes, but there are well documented exceptions where all these dimensions differ.&lt;br /&gt;
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对于自然界中出现的分形，豪斯多夫维数和盒计数维数是一致的。封装尺寸是另一个类似的概念，它给出了许多形状相同的值，但是在所有这些尺寸不同的情况，都做了很好的说明。&lt;br /&gt;
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==Formal definitions形式化定义==&lt;br /&gt;
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{{unreferenced section|date=March 2015}}&lt;br /&gt;
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===Hausdorff content豪斯多夫集===&lt;br /&gt;
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Let ''X'' be a [[metric space]]. If ''S'' ⊂ ''X'' and ''d'' ∈ [0, ∞), the ''d''-dimensional '''unlimited Hausdorff content''' of ''S'' is defined by&lt;br /&gt;
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Let X be a metric space. If S ⊂ X and d ∈ [0, ∞), the d-dimensional unlimited Hausdorff content of S is defined by&lt;br /&gt;
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设 ''X''是度量空间。若''S'' ⊂ ''X'' 和 ''d'' ∈ [0, ∞) ，则 ''S'' 的''d''维无限 豪斯多夫集定义为&lt;br /&gt;
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:&amp;lt;math&amp;gt;C_H^d(S):=\inf\Bigl\{\sum_i r_i^d:\text{ there is a cover of } S\text{ by balls with radii }r_i&amp;gt;0\Bigr\}.&amp;lt;/math&amp;gt;&lt;br /&gt;
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&amp;lt;math&amp;gt;C_H^d(S):=\inf\Bigl\{\sum_i r_i^d:\text{ there is a cover of } S\text{ by balls with radii }r_i&amp;gt;0\Bigr\}.&amp;lt;/math&amp;gt;&lt;br /&gt;
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&amp;lt;math&amp;gt;C_H^d(S):=\inf\Bigl\{\sum_i r_i^d:\text{ there is a cover of } S\text{ by balls with radii }r_i&amp;gt;0\Bigr\}.&amp;lt;/math&amp;gt;&lt;br /&gt;
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In other words, &amp;lt;math&amp;gt;C_H^d(S)&amp;lt;/math&amp;gt; is the [[infimum]] of the set of numbers &amp;lt;math&amp;gt;\delta \geq 0&amp;lt;/math&amp;gt; such that there is some (indexed) collection of [[ball (mathematics)|ball]]s &amp;lt;math&amp;gt;\{B(x_i,r_i):i\in I\}&amp;lt;/math&amp;gt; covering ''S'' with ''r&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;''&amp;amp;nbsp;&amp;gt;&amp;amp;nbsp;0 for each ''i''&amp;amp;nbsp;∈&amp;amp;nbsp;''I'' that satisfies &amp;lt;math&amp;gt;\sum_{i\in I} r_i^d&amp;lt;\delta &amp;lt;/math&amp;gt;. (Here, we use the standard convention that [[infimum|inf&amp;amp;nbsp;Ø&amp;amp;nbsp;=&amp;amp;nbsp;∞]].)&lt;br /&gt;
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In other words, &amp;lt;math&amp;gt;C_H^d(S)&amp;lt;/math&amp;gt; is the infimum of the set of numbers &amp;lt;math&amp;gt;\delta \geq 0&amp;lt;/math&amp;gt; such that there is some (indexed) collection of balls &amp;lt;math&amp;gt;\{B(x_i,r_i):i\in I\}&amp;lt;/math&amp;gt; covering S with r&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;&amp;amp;nbsp;&amp;gt;&amp;amp;nbsp;0 for each i&amp;amp;nbsp;∈&amp;amp;nbsp;I that satisfies &amp;lt;math&amp;gt;\sum_{i\in I} r_i^d&amp;lt;\delta &amp;lt;/math&amp;gt;. (Here, we use the standard convention that inf&amp;amp;nbsp;Ø&amp;amp;nbsp;=&amp;amp;nbsp;∞.)&lt;br /&gt;
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换句话说，&amp;lt;math&amp;gt;C_H^d(S)&amp;lt;/math&amp;gt; 是数字集合&amp;lt;math&amp;gt;\delta \geq 0&amp;lt;/math&amp;gt;的下确界，使得在 ''i''&amp;amp;nbsp;∈&amp;amp;nbsp中存在一些球集合 &amp;lt;math&amp;gt;\{B(x_i,r_i):i\in I\}&amp;lt;/math&amp;gt;  i 包含 s，对于每个 ''r&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;''&amp;amp;nbsp;&amp;gt;&amp;amp;nbsp;0 满足 i 中的和&amp;lt;math&amp;gt;\sum_{i\in I} r_i^d&amp;lt;\delta &amp;lt;/math&amp;gt; (在这里，我们使用inf&amp;amp;nbsp;Ø&amp;amp;nbsp;=&amp;amp;nbsp;∞ )的标准约定。&lt;br /&gt;
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===Hausdorff measurement豪斯多夫分形测量===&lt;br /&gt;
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The Hausdorff outer measure is different from the unbounded Hausdorf content in that rather than considering all possible coverings of ''S'', we see what happens when the sizes of the balls go to zero. This is  for &amp;lt;math&amp;gt;d \geq 0 &amp;lt;/math&amp;gt;, we define the ''d''-dimensional Hausdorff outer measure of ''S'' as&lt;br /&gt;
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The Hausdorff outer measure is different from the unbounded Hausdorf content in that rather than considering all possible coverings of S, we see what happens when the sizes of the balls go to zero. This is  for &amp;lt;math&amp;gt;d \geq 0 &amp;lt;/math&amp;gt;, we define the d-dimensional Hausdorff outer measure of S as&lt;br /&gt;
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豪斯多夫外测度不同于无界的豪斯多夫，因为我们不考虑 s 的所有可能，我们看到当球的大小为零时会发生什么。这是为了数学  &amp;lt;math&amp;gt;d \geq 0 &amp;lt;/math&amp;gt;，我们定义了  ''S''的 ''d''维豪斯多夫Hausdorff 外测度为&lt;br /&gt;
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:&amp;lt;math&amp;gt; \mathcal{H}^d(S):=\lim_{r \to 0} \inf\Bigl\{\sum_i r_i^d:\text{ there is a cover of } S\text{ by balls with radii } 0 &amp;lt; r_i &amp;lt; r\Bigr\}.&amp;lt;/math&amp;gt;&lt;br /&gt;
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&amp;lt;math&amp;gt; \mathcal{H}^d(S):=\lim_{r \to 0} \inf\Bigl\{\sum_i r_i^d:\text{ there is a cover of } S\text{ by balls with radii } 0 &amp;lt; r_i &amp;lt; r\Bigr\}.&amp;lt;/math&amp;gt;&lt;br /&gt;
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&amp;lt;math&amp;gt; \mathcal{H}^d(S):=\lim_{r \to 0} \inf\Bigl\{\sum_i r_i^d:\text{有一个面} S\text{ 球 } 0 &amp;lt; r_i &amp;lt; r\Bigr\}.&amp;lt;/math&amp;gt;&lt;br /&gt;
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===Hausdorff dimension豪斯多夫维数===&lt;br /&gt;
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The '''Hausdorff dimension''' of ''X'' is defined by&lt;br /&gt;
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The Hausdorff dimension of X is defined by&lt;br /&gt;
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X 的豪斯多夫维数定义为&lt;br /&gt;
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:&amp;lt;math&amp;gt;\dim_{\operatorname{H}}(X):=\inf\{d\ge 0: \mathcal{H}^d(X)=0\}.&amp;lt;/math&amp;gt;&lt;br /&gt;
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&amp;lt;math&amp;gt;\dim_{\operatorname{H}}(X):=\inf\{d\ge 0: \mathcal{H}^d(X)=0\}.&amp;lt;/math&amp;gt;&lt;br /&gt;
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Equivalently, dim&amp;lt;sub&amp;gt;H&amp;lt;/sub&amp;gt;(''X'') may be defined as the [[infimum]] of the set of ''d'' ∈ [0, ∞) such that the ''d''-dimensional [[Hausdorff measure]] of ''X'' is zero. This is the same as the supremum of the set of ''d''&amp;amp;nbsp;∈&amp;amp;nbsp;[0,&amp;amp;nbsp;∞) such that the ''d''-dimensional Hausdorff measure of ''X'' is infinite (except that when this latter set of numbers ''d'' is empty the Hausdorff dimension is zero).&lt;br /&gt;
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Equivalently, dim&amp;lt;sub&amp;gt;H&amp;lt;/sub&amp;gt;(X) may be defined as the infimum of the set of d ∈ [0, ∞) such that the d-dimensional Hausdorff measure of X is zero. This is the same as the supremum of the set of d&amp;amp;nbsp;∈&amp;amp;nbsp;[0,&amp;amp;nbsp;∞) such that the d-dimensional Hausdorff measure of X is infinite (except that when this latter set of numbers d is empty the Hausdorff dimension is zero).&lt;br /&gt;
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等价地，dim &amp;lt;sub&amp;gt;H&amp;lt;/sub&amp;gt;(''X'')可定义为 ''d'' ∈ [0, ∞) 集的下确界，使得''X'' 的''d''-维 [[豪斯多夫测度]] 为零。这与 ''d''&amp;amp;nbsp;∈&amp;amp;nbsp;[0,&amp;amp;nbsp;∞)的集合的上确界相同，因此''X''的 d 维豪斯多夫测度是无限的(除非后一个集合 ''d'' 是空的，豪斯多夫维数为零)。&lt;br /&gt;
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==Examples实例==&lt;br /&gt;
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[[Image:Sierpinski deep.svg|thumb|250px|Dimension of a further [[fractal]] example. The [[Sierpinski triangle]], an object with Hausdorff dimension of log(3)/log(2)≈1.58.&amp;lt;ref name=ClaytonSCTPLS96/&amp;gt;]]&lt;br /&gt;
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Dimension of a further [[fractal example. The Sierpinski triangle, an object with Hausdorff dimension of log(3)/log(2)≈1.58.]]&lt;br /&gt;
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[[Image:谢尔宾斯基三角形 deep.svg|thumb|250px|进一步的[[分形维数]]的例子，进一步的分形维数的例子是谢尔宾斯基三角形，它是一个豪斯多夫维数为log(3)/log(2)≈1.58.&amp;lt;ref name=ClaytonSCTPLS96/&amp;gt;的物体]]&lt;br /&gt;
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* [[Countable set]]s have Hausdorff dimension 0.&amp;lt;ref name=&amp;quot;schleicher&amp;quot;&amp;gt;{{cite journal |last1=Schleicher |first1=Dierk |title=Hausdorff Dimension, Its Properties, and Its Surprises |journal=The American Mathematical Monthly |date=June 2007 |volume=114 |issue=6 |pages=509–528 |doi=10.1080/00029890.2007.11920440 |language=en |issn=0002-9890|arxiv=math/0505099 }}&amp;lt;/ref&amp;gt;&lt;br /&gt;
*[[可数集]]拥有豪斯多夫维数0.&amp;lt;ref name=&amp;quot;schleicher&amp;quot;&amp;gt;{{cite journal |last1=Schleicher |first1=Dierk |title=豪斯多夫维数, Its Properties, and Its Surprises |journal=The American Mathematical Monthly美国数学期刊 |date=June 2007 |volume=114 |issue=6 |pages=509–528 |doi=10.1080/00029890.2007.11920440 |language=en |issn=0002-9890|arxiv=math/0505099 }}&amp;lt;/ref&amp;gt;&lt;br /&gt;
* The [[Euclidean space]] ℝ&amp;lt;sup&amp;gt;''n''&amp;lt;/sup&amp;gt; has Hausdorff dimension ''n'', and the circle '''S'''&amp;lt;sup&amp;gt;1&amp;lt;/sup&amp;gt; has Hausdorff dimension 1.&amp;lt;ref name=&amp;quot;schleicher&amp;quot; /&amp;gt;&lt;br /&gt;
*[[教育空间]] ℝ&amp;lt;sup&amp;gt;''n''&amp;lt;/sup&amp;gt; 有豪斯多夫维数 ''n''，循环'''S'''&amp;lt;sup&amp;gt;1&amp;lt;/sup&amp;gt; 拥有豪斯多夫维数1.&amp;lt;ref name=&amp;quot;schleicher&amp;quot; /&amp;gt;&lt;br /&gt;
* [[Fractal]]s often are spaces whose Hausdorff dimension strictly exceeds the [[topological dimension]].&amp;lt;ref name=&amp;quot;mandelbrot&amp;quot; /&amp;gt; For example, the [[Cantor set]], a zero-dimensional topological space, is a union of two copies of itself, each copy shrunk by a factor 1/3; hence, it can be shown that its Hausdorff dimension is ln(2)/ln(3)&amp;amp;nbsp;≈&amp;amp;nbsp;0.63.&amp;lt;ref&amp;gt;{{cite book | last=Falconer | first = Kenneth |title=Fractal Geometry: Mathematical Foundations and Applications | publisher=[[John Wiley and Sons]] | edition=2nd | year=2003}}&amp;lt;/ref&amp;gt; The [[Sierpinski triangle]] is a union of three copies of itself, each copy shrunk by a factor of&amp;amp;nbsp;1/2; this yields a Hausdorff dimension of ln(3)/ln(2)&amp;amp;nbsp;≈&amp;amp;nbsp;1.58.&amp;lt;ref name=CampbellAnnenberg15/&amp;gt; These Hausdorff dimensions are related to the &amp;quot;critical exponent&amp;quot; of the [[Master theorem (analysis of algorithms)|Master theorem]] for solving [[Recurrence relation|recurrence relations]] in the [[analysis of algorithms]].&lt;br /&gt;
*[[分形]]一般是那些豪斯多夫维数直接超过其拓扑维数的空间。例如[[康托尔集]]是一个o维拓扑空间，由两个自己复制而成，每一个复制品都是原来的三分之一，因此它的豪斯多夫维数是 ln(2)/ln(3)&amp;amp;nbsp;≈&amp;amp;nbsp;0.63。&amp;lt;ref&amp;gt;{{cite book | last=Falconer | first = Kenneth |title=Fractal Geometry: Mathematical Foundations and Applications | publisher=[[John Wiley and Sons]] | edition=2nd | year=2003}}&amp;lt;/ref&amp;gt;一个[[谢尔宾斯基三角]]是他自身三个复制的组合。每一个是原来的&amp;amp;nbsp;1/2，它的豪斯多夫维数ln(3)/ln(2)&amp;amp;nbsp;≈&amp;amp;nbsp;1.58。&amp;lt;ref name=CampbellAnnenberg15/&amp;gt;在递归算法中解决递归关系时，这些豪斯多夫维数与[[算法分析主定理]]的临界指标相联系。&lt;br /&gt;
* [[Space-filling curve]]s like the [[Peano curve]] have the same Hausdorff dimension as the space they fill.&lt;br /&gt;
*[[空间填充曲线]]拥有和他们填充空间同样的豪斯多夫维数，如[[皮亚诺曲线]]。&lt;br /&gt;
* The trajectory of [[Brownian motion]] in dimension 2 and above is conjectured to be Hausdorff dimension 2.&amp;lt;ref&amp;gt;{{cite book | last=Morters | first=Peres | title= Brownian Motion | publisher=[[Cambridge University Press]] | year=2010 }}&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
[[image:Great Britain Hausdorff.svg|thumb|250px|Estimating the Hausdorff dimension of the [[How Long Is the Coast of Britain? Statistical Self-Similarity and Fractional Dimension|coast of Great Britain]]]]&lt;br /&gt;
&lt;br /&gt;
coast of Great Britain]]&lt;br /&gt;
&lt;br /&gt;
[[大不列颠海岸&lt;br /&gt;
&lt;br /&gt;
* 刘易斯·弗赖伊·理查森[[Lewis Fry Richardson]] has performed detailed experiments to measure the approximate Hausdorff dimension for various coastlines. His results have varied from 1.02 for the coastline of [[South Africa]] to 1.25 for the west coast of [[Great Britain]].&amp;lt;ref name=&amp;quot;mandelbrot&amp;quot; /&amp;gt;&lt;br /&gt;
*刘易斯·弗赖伊·理查森（Lewis Fry Richardson）已经通过豪斯多夫维数去测量了很多海岸线。它的结果涵盖从1.02的南非海岸线到1.25的大英帝国西海岸模型。]]&lt;br /&gt;
&lt;br /&gt;
==Properties of Hausdorff dimension豪斯多夫维数特性==&lt;br /&gt;
&lt;br /&gt;
{{refimprove section|date=March 2015}}&lt;br /&gt;
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&lt;br /&gt;
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=== Hausdorff dimension and inductive dimension 豪斯多夫维数和归纳维数===&lt;br /&gt;
&lt;br /&gt;
Let ''X'' be an arbitrary [[Separable space|separable]] metric space. There is a [[topology|topological]] notion of [[inductive dimension]] for ''X'' which is defined recursively. It is always an integer (or +∞) and is denoted dim&amp;lt;sub&amp;gt;ind&amp;lt;/sub&amp;gt;(''X'').&lt;br /&gt;
&lt;br /&gt;
Let X be an arbitrary separable metric space. There is a topological notion of inductive dimension for X which is defined recursively. It is always an integer (or +∞) and is denoted dim&amp;lt;sub&amp;gt;ind&amp;lt;/sub&amp;gt;(X).&lt;br /&gt;
&lt;br /&gt;
设''X'' 是[[任意可分度量空间]]。对于''X'' 有一个递归定义的归纳维数拓扑概念。它总是一个整数(或 + ∞) ，并且表示dim&amp;lt;sub&amp;gt;ind&amp;lt;/sub&amp;gt;(''X'')。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
'''Theorem'''. Suppose ''X'' is non-empty. Then &lt;br /&gt;
&lt;br /&gt;
Theorem. Suppose X is non-empty. Then &lt;br /&gt;
&lt;br /&gt;
'''定理'''：假设''X'' 是非空的。那么&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt; \dim_{\mathrm{Haus}}(X) \geq \dim_{\operatorname{ind}}(X). &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \dim_{\mathrm{Haus}}(X) \geq \dim_{\operatorname{ind}}(X). &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Moreover,&lt;br /&gt;
&lt;br /&gt;
Moreover,&lt;br /&gt;
&lt;br /&gt;
此外,&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \inf_Y \dim_{\operatorname{Haus}}(Y) =\dim_{\operatorname{ind}}(X), &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \inf_Y \dim_{\operatorname{Haus}}(Y) =\dim_{\operatorname{ind}}(X), &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
where ''Y'' ranges over metric spaces [[homeomorphic]] to ''X''. In other words, ''X'' and ''Y'' have the same underlying set of points and the metric ''d''&amp;lt;sub&amp;gt;''Y''&amp;lt;/sub&amp;gt; of ''Y'' is topologically equivalent to ''d''&amp;lt;sub&amp;gt;''X''&amp;lt;/sub&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
where Y ranges over metric spaces homeomorphic to X. In other words, X and Y have the same underlying set of points and the metric d&amp;lt;sub&amp;gt;Y&amp;lt;/sub&amp;gt; of Y is topologically equivalent to d&amp;lt;sub&amp;gt;X&amp;lt;/sub&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
其中''Y''是度量空间同胚到 ''X''的范围。换句话说， ''X''和 ''Y''具有相同的基本点集，''Y''的度规''d''&amp;lt;sub&amp;gt;''Y''&amp;lt;/sub&amp;gt; 的子拓扑等价于''d''&amp;lt;sub&amp;gt;''X''&amp;lt;/sub&amp;gt;。&lt;br /&gt;
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&lt;br /&gt;
&lt;br /&gt;
These results were originally established by [[Edward Szpilrajn]] (1907–1976), e.g., see Hurewicz and Wallman, Chapter VII.{{full citation needed|date=March 2015}}&lt;br /&gt;
&lt;br /&gt;
These results were originally established by Edward Szpilrajn (1907–1976), e.g., see Hurewicz and Wallman, Chapter VII.&lt;br /&gt;
&lt;br /&gt;
这些结果最初是由 [[Edward Szpilrajn]] (1907–1976)建立的,  参见 Hurewicz and Wallman, Chapter VII.{{full citation needed|date=March 2015}}第七章。&lt;br /&gt;
&lt;br /&gt;
=== Hausdorff dimension and Minkowski dimension 豪斯多夫维数和闵可夫斯基维度===&lt;br /&gt;
&lt;br /&gt;
The [[Minkowski dimension]] is similar to, and at least as large as, the Hausdorff dimension, and they are equal in many situations. However, the set of [[rational number|rational]] points in [0, 1] has Hausdorff dimension zero and Minkowski dimension one. There are also compact sets for which the Minkowski dimension is strictly larger than the Hausdorff dimension.&lt;br /&gt;
&lt;br /&gt;
The Minkowski dimension is similar to, and at least as large as, the Hausdorff dimension, and they are equal in many situations. However, the set of rational points in [0, 1] has Hausdorff dimension zero and Minkowski dimension one. There are also compact sets for which the Minkowski dimension is strictly larger than the Hausdorff dimension.&lt;br /&gt;
&lt;br /&gt;
[[闵可夫斯基维数]]与豪斯多夫维数相似，至少和它一样大，而且在许多情况下是相等的。然而，[0,1]中有理点集的豪斯多夫维数为0，闵可夫斯基维数为1。还有一些紧集的闵可夫斯基维数绝对大于豪斯多夫维数。&lt;br /&gt;
&lt;br /&gt;
=== Hausdorff dimensions and Frostman measures 豪斯多夫维度和弗洛斯曼测度===&lt;br /&gt;
&lt;br /&gt;
If there is a [[measure (mathematics)|measure]] μ defined on [[Borel measure|Borel]] subsets of a metric space ''X'' such that ''μ''(''X'') &amp;gt; 0 and ''μ''(''B''(''x'', ''r'')) ≤ ''r&amp;lt;sup&amp;gt;s&amp;lt;/sup&amp;gt;'' holds for some constant ''s'' &amp;gt; 0 and for every ball ''B''(''x'', ''r'') in ''X'', then dim&amp;lt;sub&amp;gt;Haus&amp;lt;/sub&amp;gt;(''X'') ≥ ''s''. A partial converse is provided by [[Frostman's lemma]].{{citation needed|date=March 2015}}&amp;lt;ref&amp;gt;This Wikipedia article also discusses further useful characterizations of the Hausdorff dimension.{{clarify|date=March 2015}}&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
If there is a measure μ defined on Borel subsets of a metric space X such that μ(X) &amp;gt; 0 and μ(B(x, r)) ≤ r&amp;lt;sup&amp;gt;s&amp;lt;/sup&amp;gt; holds for some constant s &amp;gt; 0 and for every ball B(x, r) in X, then dim&amp;lt;sub&amp;gt;Haus&amp;lt;/sub&amp;gt;(X) ≥ s. A partial converse is provided by Frostman's lemma.&lt;br /&gt;
&lt;br /&gt;
如果在度量空间 ''X'' 的 Borel 子集上定义一个测度 μ，使得''μ''(''X'') &amp;gt; 0 和''μ''(''B''(''x'', ''r'')) ≤ ''r&amp;lt;sup&amp;gt;s&amp;lt;/sup&amp;gt;''，对于某个常数 ''s'' &amp;gt; 0  和 ''X'' 中的每个球 ''B''(''x'', ''r'') 成立，则 dim&amp;lt;sub&amp;gt;Haus&amp;lt;/sub&amp;gt;(''X'') ≥ ''s'' 。 部分逆向转换由弗洛斯曼引理定义。&lt;br /&gt;
&lt;br /&gt;
=== Behaviour under unions and products ===&lt;br /&gt;
&lt;br /&gt;
If &amp;lt;math&amp;gt;X=\bigcup_{i\in I}X_i&amp;lt;/math&amp;gt; is a finite or countable union, then&lt;br /&gt;
&lt;br /&gt;
If &amp;lt;math&amp;gt;X=\bigcup_{i\in I}X_i&amp;lt;/math&amp;gt; is a finite or countable union, then&lt;br /&gt;
&lt;br /&gt;
如果 &amp;lt;math&amp;gt;X=\bigcup_{i\in I}X_i&amp;lt;/math&amp;gt; 是一个有限或可数的联合，则&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \dim_{\operatorname{Haus}}(X) =\sup_{i\in I} \dim_{\operatorname{Haus}}(X_i).&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \dim_{\operatorname{Haus}}(X) =\sup_{i\in I} \dim_{\operatorname{Haus}}(X_i).&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
This can be verified directly from the definition.&lt;br /&gt;
&lt;br /&gt;
This can be verified directly from the definition.&lt;br /&gt;
&lt;br /&gt;
这可以直接从定义得到验证。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
If ''X'' and ''Y'' are non-empty metric spaces, then the Hausdorff dimension of their product satisfies&amp;lt;ref&amp;gt;{{cite journal |author=Marstrand, J. M. |title=The dimension of Cartesian product sets |journal=Proc. Cambridge Philos. Soc. |volume=50 |issue=3 |pages=198–202 |year=1954 |doi=10.1017/S0305004100029236 |bibcode = 1954PCPS...50..198M }}&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
If X and Y are non-empty metric spaces, then the Hausdorff dimension of their product satisfies&lt;br /&gt;
&lt;br /&gt;
如果 ''X'' 和''Y''是非空度量空间，那么它们乘积的豪斯多夫维数满足&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt; \dim_{\operatorname{Haus}}(X\times Y)\ge \dim_{\operatorname{Haus}}(X)+ \dim_{\operatorname{Haus}}(Y).&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \dim_{\operatorname{Haus}}(X\times Y)\ge \dim_{\operatorname{Haus}}(X)+ \dim_{\operatorname{Haus}}(Y).&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
This inequality can be strict. It is possible to find two sets of dimension 0 whose product has dimension 1.&amp;lt;ref&amp;gt;{{cite book  | last = Falconer  | first = Kenneth J.  | title = Fractal geometry. Mathematical foundations and applications  | publisher = John Wiley &amp;amp; Sons, Inc., Hoboken, New Jersey  | year = 2003  | doi =   | isbn = }}&amp;lt;/ref&amp;gt; In the opposite direction, it is known that when ''X'' and ''Y'' are Borel subsets of '''R'''&amp;lt;sup&amp;gt;''n''&amp;lt;/sup&amp;gt;, the Hausdorff dimension of ''X'' × ''Y'' is bounded from above by the Hausdorff dimension of ''X'' plus the [[packing dimension|upper packing dimension]] of ''Y''. These facts are discussed in Mattila (1995).&lt;br /&gt;
&lt;br /&gt;
This inequality can be strict. It is possible to find two sets of dimension 0 whose product has dimension 1. In the opposite direction, it is known that when X and Y are Borel subsets of R&amp;lt;sup&amp;gt;n&amp;lt;/sup&amp;gt;, the Hausdorff dimension of X × Y is bounded from above by the Hausdorff dimension of X plus the upper packing dimension of Y. These facts are discussed in Mattila (1995).&lt;br /&gt;
&lt;br /&gt;
这种不平等可以是绝对的。有可能找到两个维数为0的集合，其乘积的维数为1。相反，我们知道当''X''和''Y''是 '''R'''&amp;lt;sup&amp;gt;''n''&amp;lt;/sup&amp;gt;的 Borel 子集时， ''X'' × ''Y''的豪斯多夫维数从上面以 ''X''的豪斯多夫维数加上 ''Y''的填充维数为界。Mattila (1995)曾就这些情况进行了讨论。&lt;br /&gt;
&lt;br /&gt;
==Self-similar sets自相似集合==&lt;br /&gt;
&lt;br /&gt;
{{refimprove section|date=March 2015}}&lt;br /&gt;
&lt;br /&gt;
Many sets defined by a self-similarity condition have dimensions which can be determined explicitly. Roughly, a set ''E'' is self-similar if it is the fixed point of a set-valued transformation ψ, that is ψ(''E'') = ''E'', although the exact definition is given below.&lt;br /&gt;
&lt;br /&gt;
Many sets defined by a self-similarity condition have dimensions which can be determined explicitly. Roughly, a set E is self-similar if it is the fixed point of a set-valued transformation ψ, that is ψ(E) = E, although the exact definition is given below.&lt;br /&gt;
&lt;br /&gt;
许多由自相似条件定义的集合具有可以显式确定的维数。粗略地说，集合''E'' 是自相似的，如果它是集值ψ变换的不动点，即ψ(''E'') = ''E''，尽管下面给出了确切的定义。&lt;br /&gt;
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&lt;br /&gt;
&lt;br /&gt;
&amp;lt;blockquote&amp;gt;'''Theorem'''. Suppose&lt;br /&gt;
&lt;br /&gt;
&amp;lt;blockquote&amp;gt;Theorem. Suppose&lt;br /&gt;
&lt;br /&gt;
&amp;lt;blockquote&amp;gt;'''定理'''：假设&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt; \psi_i: \mathbf{R}^n \rightarrow \mathbf{R}^n, \quad i=1, \ldots , m &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \psi_i: \mathbf{R}^n \rightarrow \mathbf{R}^n, \quad i=1, \ldots , m &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
are [[Contraction mapping|contractive]] mappings on '''R'''&amp;lt;sup&amp;gt;''n''&amp;lt;/sup&amp;gt; with contraction constant ''r&amp;lt;sub&amp;gt;j&amp;lt;/sub&amp;gt;'' &amp;lt; 1. Then there is a unique ''non-empty'' compact set ''A'' such that&lt;br /&gt;
&lt;br /&gt;
are contractive mappings on R&amp;lt;sup&amp;gt;n&amp;lt;/sup&amp;gt; with contraction constant r&amp;lt;sub&amp;gt;j&amp;lt;/sub&amp;gt; &amp;lt; 1. Then there is a unique non-empty compact set A such that&lt;br /&gt;
&lt;br /&gt;
是'''R'''&amp;lt;sup&amp;gt;''n''&amp;lt;/sup&amp;gt;上的压缩常数''r&amp;lt;sub&amp;gt;j&amp;lt;/sub&amp;gt;'&amp;lt; 1的压缩映射。然后有一个唯一的非空紧集A &lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt; A = \bigcup_{i=1}^m \psi_i (A). &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; A = \bigcup_{i=1}^m \psi_i (A). &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&amp;lt;/blockquote&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;/blockquote&amp;gt;&lt;br /&gt;
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&lt;br /&gt;
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&lt;br /&gt;
The theorem follows from [[Stefan Banach]]'s [[Contractive mapping theorem|contractive mapping fixed point theorem]] applied to the complete metric space of non-empty compact subsets of '''R'''&amp;lt;sup&amp;gt;''n''&amp;lt;/sup&amp;gt; with the [[Hausdorff distance]].&amp;lt;ref&amp;gt;{{cite book |author=Falconer, K. J. |title=The Geometry of Fractal Sets |publisher=Cambridge University Press |location=Cambridge, UK |year=1985 |isbn=0-521-25694-1 |chapter=Theorem 8.3}}&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
The theorem follows from Stefan Banach's contractive mapping fixed point theorem applied to the complete metric space of non-empty compact subsets of R&amp;lt;sup&amp;gt;n&amp;lt;/sup&amp;gt; with the Hausdorff distance.&lt;br /&gt;
&lt;br /&gt;
这个定理来源于 Stefan Banach 的压缩映射不动点定理，该定理应用于 '''R'''&amp;lt;sup&amp;gt;''n''&amp;lt;/sup&amp;gt; 的非空紧子集的完备空间豪斯多夫距离。&lt;br /&gt;
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&lt;br /&gt;
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===The open set condition开集条件===&lt;br /&gt;
&lt;br /&gt;
To determine the dimension of the self-similar set ''A'' (in certain cases), we need a technical condition called the ''open set condition'' (OSC) on the sequence of contractions ψ&amp;lt;sub&amp;gt;''i''&amp;lt;/sub&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
To determine the dimension of the self-similar set A (in certain cases), we need a technical condition called the open set condition (OSC) on the sequence of contractions ψ&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
为了确定自相似集''A'' 的维数(在某些情况下) ，我们需要一个称为''开集条件''(OSC)的技术条件ψ&amp;lt;sub&amp;gt;''i''&amp;lt;/sub&amp;gt;。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
There is a relatively compact open set ''V'' such that&lt;br /&gt;
&lt;br /&gt;
There is a relatively compact open set V such that&lt;br /&gt;
&lt;br /&gt;
有一个相对紧的开集''V''&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt; \bigcup_{i=1}^m\psi_i (V) \subseteq V, &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \bigcup_{i=1}^m\psi_i (V) \subseteq V, &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
where the sets in union on the left are pairwise [[disjoint sets|disjoint]].&lt;br /&gt;
&lt;br /&gt;
where the sets in union on the left are pairwise disjoint.&lt;br /&gt;
&lt;br /&gt;
左边的集合是成对不相交的。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The open set condition is a separation condition that ensures the images ψ&amp;lt;sub&amp;gt;''i''&amp;lt;/sub&amp;gt;(''V'') do not overlap &amp;quot;too much&amp;quot;.&lt;br /&gt;
&lt;br /&gt;
The open set condition is a separation condition that ensures the images ψ&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;(V) do not overlap &amp;quot;too much&amp;quot;.&lt;br /&gt;
&lt;br /&gt;
开集条件是保证图像子ψ&amp;lt;sub&amp;gt;''i''&amp;lt;/sub&amp;gt;(''V'') 不重叠“太多”的分离条件。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
'''Theorem'''. Suppose the open set condition holds and each ψ&amp;lt;sub&amp;gt;''i''&amp;lt;/sub&amp;gt; is a similitude, that is a composition of an [[isometry]] and a [[dilation (metric space)|dilation]] around some point. Then the unique fixed point of ψ is a set whose Hausdorff dimension is ''s'' where ''s'' is the unique solution of&amp;lt;ref&amp;gt;{{cite journal | last=Hutchinson | first=John E. | title=Fractals and self similarity | journal=Indiana Univ. Math. J. | volume=30 | year=1981 | pages=713–747 | doi=10.1512/iumj.1981.30.30055 | issue=5 | doi-access=free }}&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
Theorem. Suppose the open set condition holds and each ψ&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt; is a similitude, that is a composition of an isometry and a dilation around some point. Then the unique fixed point of ψ is a set whose Hausdorff dimension is s where s is the unique solution of&lt;br /&gt;
&lt;br /&gt;
'''定理'''假设开集条件成立，并且每个ψ&amp;lt;sub&amp;gt;''i''&amp;lt;/sub&amp;gt; 是一个相似量，这是一个等距和围绕某一点的膨胀的合成。那么唯一的不动点是一个集合，它的豪斯多夫维数是 ''s'' ，其中  ''s'' 是 ''s'' &amp;lt;ref&amp;gt;{{cite journal | last=Hutchinson | first=John E. | title=Fractals and self similarity | journal=Indiana Univ. Math. J. | volume=30 | year=1981 | pages=713–747 | doi=10.1512/iumj.1981.30.30055 | issue=5 | doi-access=free }}&amp;lt;/ref&amp;gt;的唯一解&lt;br /&gt;
&lt;br /&gt;
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:&amp;lt;math&amp;gt; \sum_{i=1}^m r_i^s = 1. &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \sum_{i=1}^m r_i^s = 1. &amp;lt;/math&amp;gt;&lt;br /&gt;
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The contraction coefficient of a similitude is the magnitude of the dilation.&lt;br /&gt;
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The contraction coefficient of a similitude is the magnitude of the dilation.&lt;br /&gt;
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相似物的收缩系数就是膨胀的大小。&lt;br /&gt;
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We can use this theorem to compute the Hausdorff dimension of the Sierpinski triangle (or sometimes called Sierpinski gasket). Consider three [[non-collinear points]] ''a''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;, ''a''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;, ''a''&amp;lt;sub&amp;gt;3&amp;lt;/sub&amp;gt; in the plane '''R'''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; and let ψ&amp;lt;sub&amp;gt;''i''&amp;lt;/sub&amp;gt; be the dilation of ratio 1/2 around ''a&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;''. The unique non-empty fixed point of the corresponding mapping ψ is a Sierpinski gasket and the dimension ''s'' is the unique solution of&lt;br /&gt;
&lt;br /&gt;
We can use this theorem to compute the Hausdorff dimension of the Sierpinski triangle (or sometimes called Sierpinski gasket). Consider three non-collinear points a&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;, a&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;, a&amp;lt;sub&amp;gt;3&amp;lt;/sub&amp;gt; in the plane R&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; and let ψ&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt; be the dilation of ratio 1/2 around a&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;. The unique non-empty fixed point of the corresponding mapping ψ is a Sierpinski gasket and the dimension s is the unique solution of&lt;br /&gt;
&lt;br /&gt;
我们可以使用这个定理来计算谢尔宾斯基三角形的豪斯多夫维数(或者有时候叫做谢尔宾斯基垫圈)。考虑R&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; 平面上的三个非共线点，''a''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;，''a''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;，''a''&amp;lt;sub&amp;gt;3&amp;lt;/sub&amp;gt;，让ψ&amp;lt;sub&amp;gt;''i''&amp;lt;/sub&amp;gt;是围绕着''a&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;''膨胀比率的1/2。对应映射的唯一非空不动点是一个谢尔宾斯基垫圈，其维数''s''是对应映射的唯一解&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt; \left(\frac{1}{2}\right)^s+\left(\frac{1}{2}\right)^s+\left(\frac{1}{2}\right)^s = 3 \left(\frac{1}{2}\right)^s =1. &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \left(\frac{1}{2}\right)^s+\left(\frac{1}{2}\right)^s+\left(\frac{1}{2}\right)^s = 3 \left(\frac{1}{2}\right)^s =1. &amp;lt;/math&amp;gt;&lt;br /&gt;
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Taking [[natural logarithm]]s of both sides of the above equation, we can solve for ''s'', that is: ''s'' = ln(3)/ln(2).  The Sierpinski gasket is self-similar and satisfies the OSC. In general a set ''E'' which is a fixed point of a mapping&lt;br /&gt;
&lt;br /&gt;
Taking natural logarithms of both sides of the above equation, we can solve for s, that is: s = ln(3)/ln(2).  The Sierpinski gasket is self-similar and satisfies the OSC. In general a set E which is a fixed point of a mapping&lt;br /&gt;
&lt;br /&gt;
取上述方程两边的自然对数，我们可以求出 ''s''，即: ''s'' = ln(3)/ln(2)。该密封垫具有自相似性，满足 OSC 要求。一般来说，集合 ''E''是一个映射的不动点&lt;br /&gt;
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: &amp;lt;math&amp;gt; A \mapsto \psi(A) = \bigcup_{i=1}^m \psi_i(A) &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt; A \mapsto \psi(A) = \bigcup_{i=1}^m \psi_i(A) &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
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is self-similar if and only if the intersections&lt;br /&gt;
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is self-similar if and only if the intersections&lt;br /&gt;
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是自相似的，当且仅当&lt;br /&gt;
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:&amp;lt;math&amp;gt; H^s\left(\psi_i(E) \cap \psi_j(E)\right) =0, &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; H^s\left(\psi_i(E) \cap \psi_j(E)\right) =0, &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
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where ''s'' is the Hausdorff dimension of ''E'' and ''H&amp;lt;sup&amp;gt;s&amp;lt;/sup&amp;gt;'' denotes [[Hausdorff measure]]. This is clear in the case of the Sierpinski gasket (the intersections are just points), but is also true more generally:&lt;br /&gt;
&lt;br /&gt;
where s is the Hausdorff dimension of E and H&amp;lt;sup&amp;gt;s&amp;lt;/sup&amp;gt; denotes Hausdorff measure. This is clear in the case of the Sierpinski gasket (the intersections are just points), but is also true more generally:&lt;br /&gt;
&lt;br /&gt;
其中 ''s''是''E''的豪斯多夫维数， ''E'' and ''H&amp;lt;sup&amp;gt;s&amp;lt;/sup&amp;gt;'' 表示 豪斯多夫测度。对于谢尔宾斯基垫圈(交叉点就是点)来说，这一点很明显，但更普遍的情况是:&lt;br /&gt;
&lt;br /&gt;
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'''Theorem'''. Under the same conditions as the previous theorem, the unique fixed point of ψ is self-similar.&lt;br /&gt;
&lt;br /&gt;
Theorem. Under the same conditions as the previous theorem, the unique fixed point of ψ is self-similar.&lt;br /&gt;
&lt;br /&gt;
'''定理'''：在与前一定理相同的条件下，其唯一不动点是自相似的。&lt;br /&gt;
&lt;br /&gt;
==See also参阅==&lt;br /&gt;
&lt;br /&gt;
* [[List of fractals by Hausdorff dimension豪斯多夫分形维数列表]] Examples of deterministic fractals, random and natural fractals.确定性分形与随机和自然分形的示例。&lt;br /&gt;
&lt;br /&gt;
* [[Assouad dimension  Assouad维数]], another variation of fractal dimension that, like Hausdorff dimension, is defined using coverings by balls其他被球覆盖方式定义的分形维数，例如豪斯多夫维数。&lt;br /&gt;
&lt;br /&gt;
* [[Intrinsic dimension固有维数]]&lt;br /&gt;
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* [[Packing dimension填充维数]]&lt;br /&gt;
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* [[Fractal dimension分形维数]]&lt;br /&gt;
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==References参考文献==&lt;br /&gt;
&lt;br /&gt;
{{reflist}}&lt;br /&gt;
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==Further reading拓展阅读==&lt;br /&gt;
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* {{cite book |last1=Dodson |first1=M. Maurice |title=Fractal Geometry and Applications: A Jubilee of Benoît Mandelbrot |volume=72 |issue=1 |pages=305–347 |last2=Kristensen |first2=Simon |chapter=Hausdorff Dimension and Diophantine Approximation |date=June 12, 2003 |arxiv=math/0305399 |bibcode = 2003math......5399D |doi=10.1090/pspum/072.1/2112110|series=Proceedings of Symposia in Pure Mathematics |isbn=9780821836378 }}&lt;br /&gt;
&lt;br /&gt;
* {{cite book |last1=Hurewicz |first1=Witold |authorlink1=Witold Hurewicz |last2=Wallman |first2=Henry |authorlink2=Henry Wallman |title=Dimension Theory |url=https://archive.org/details/in.ernet.dli.2015.84609 |publisher=Princeton University Press |year=1948 }}&lt;br /&gt;
&lt;br /&gt;
* {{cite journal |author作者=E. Szpilrajn |authorlink=Edward Marczewski |title=La dimension et la mesure |journal=Fundamenta Mathematicae |volume=28 |pages=81–9 |year=1937 }}&lt;br /&gt;
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* {{cite journal&lt;br /&gt;
&lt;br /&gt;
 | last1=Marstrand&lt;br /&gt;
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 | last1=Marstrand&lt;br /&gt;
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 | last1=马斯特兰德&lt;br /&gt;
&lt;br /&gt;
 | first1=J. M. | title=The dimension of cartesian product sets | year=1954 | journal=Proc. Cambridge Philos. Soc.&lt;br /&gt;
&lt;br /&gt;
 | first1=J. M. | title=The dimension of cartesian product sets | year=1954 | journal=Proc. Cambridge Philos. Soc.&lt;br /&gt;
&lt;br /&gt;
 | first1= J. M. | title=笛卡儿积集的维数 | 1954年 |  journal=Proc. Cambridge Philos. Soc.&lt;br /&gt;
&lt;br /&gt;
 | volume=50&lt;br /&gt;
&lt;br /&gt;
 | volume=50&lt;br /&gt;
&lt;br /&gt;
 | 第50卷&lt;br /&gt;
&lt;br /&gt;
 | issue=3&lt;br /&gt;
&lt;br /&gt;
 | issue=3&lt;br /&gt;
&lt;br /&gt;
 | 第三期&lt;br /&gt;
&lt;br /&gt;
 | pages=198–202&lt;br /&gt;
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 | pages=198–202&lt;br /&gt;
&lt;br /&gt;
 | 第198-202页&lt;br /&gt;
&lt;br /&gt;
 | doi=10.1017/S0305004100029236|bibcode = 1954PCPS...50..198M }}&lt;br /&gt;
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 | doi=10.1017/S0305004100029236|bibcode = 1954PCPS...50..198M }}&lt;br /&gt;
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10.1017 / S0305004100029236 | bibcode 1954PCPS... 50. . 198 m }&lt;br /&gt;
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* {{Cite book&lt;br /&gt;
&lt;br /&gt;
 | last1=Mattila&lt;br /&gt;
&lt;br /&gt;
 | last1=Mattila&lt;br /&gt;
&lt;br /&gt;
 | last1=Mattila&lt;br /&gt;
&lt;br /&gt;
 | first1=Pertti | author1-link=Pertti Mattila| title=Geometry of sets and measures in Euclidean spaces | publisher=[[Cambridge University Press]]&lt;br /&gt;
&lt;br /&gt;
 | first1=Pertti | author1-link=Pertti Mattila| title=Geometry of sets and measures in Euclidean spaces | publisher=Cambridge University Press&lt;br /&gt;
&lt;br /&gt;
| first1 Pertti | author1-link Pertti Mattila | title 欧几里德空间中集合和度量的几何 | 出版商剑桥大学出版社&lt;br /&gt;
&lt;br /&gt;
 | isbn=978-0-521-65595-8 | year=1995}}&lt;br /&gt;
&lt;br /&gt;
 | isbn=978-0-521-65595-8 | year=1995}}&lt;br /&gt;
&lt;br /&gt;
| isbn 978-0-521-65595-8 | year 1995}&lt;br /&gt;
&lt;br /&gt;
* {{cite journal |author=A. S. Besicovitch |authorlink=A. S. Besicovitch |title=On Linear Sets of Points of Fractional Dimensions |journal=[[Mathematische Annalen]] |volume=101 |year=1929 | doi=10.1007/BF01454831| issue=1 |pages= 161–193}}&lt;br /&gt;
&lt;br /&gt;
* {{cite journal |author1=A. S. Besicovitch |authorlink1=A. S. Besicovitch |author2=H. D. Ursell |authorlink2=H. D. Ursell |title=Sets of Fractional Dimensions |journal=Journal of the London Mathematical Society |volume=12 |year=1937 | issue=1 | doi=10.1112/jlms/s1-12.45.18  | pages=18–25 }}&amp;lt;br/&amp;gt;Several selections from this volume are reprinted in {{cite book |author=Edgar, Gerald A. |title=Classics on fractals |publisher=Addison-Wesley |location=Boston |year=1993 |isbn=0-201-58701-7}} See chapters 9,10,11&lt;br /&gt;
&lt;br /&gt;
* {{cite journal |author=F. Hausdorff |authorlink=F. Hausdorff |title=Dimension und äußeres Maß |journal=Mathematische Annalen |volume=79 |issue=1–2 |pages=157–179 |date=March 1919 |doi=10.1007/BF01457179|hdl=10338.dmlcz/100363 |url=http://dml.cz/bitstream/handle/10338.dmlcz/100363/CzechMathJ_09-1959-3_5.pdf }}&lt;br /&gt;
&lt;br /&gt;
* {{cite journal | last=Hutchinson | first=John E. | title=Fractals and self similarity | journal=Indiana Univ. Math. J. | volume=30 | year=1981 | pages=713–747 | doi=10.1512/iumj.1981.30.30055 | issue=5 | doi-access=free }}&lt;br /&gt;
&lt;br /&gt;
*{{cite book | last=Falconer | first = Kenneth |title=Fractal Geometry: Mathematical Foundations and Applications | publisher=[[John Wiley and Sons]] | edition=2nd | year=2003}}&lt;br /&gt;
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==External links外部链接==&lt;br /&gt;
&lt;br /&gt;
* [https://www.encyclopediaofmath.org/index.php/Hausdorff_dimension Hausdorff dimension] 在 [https://www.encyclopediaofmath.org/ Encyclopedia of Mathematics]&lt;br /&gt;
&lt;br /&gt;
* [https://www.encyclopediaofmath.org/index.php/Hausdorff_measure Hausdorff measure] 在 [https://www.encyclopediaofmath.org/ Encyclopedia of Mathematics]&lt;br /&gt;
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{{DEFAULTSORT:Hausdorff Dimension豪斯多夫维数}}&lt;br /&gt;
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[[Category分类:Fractals分形]]&lt;br /&gt;
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[[Category分类:Metric geometry度量几何]]&lt;br /&gt;
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[[Category分类:Dimension theory维度理论]]&lt;br /&gt;
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&amp;lt;noinclude&amp;gt;&lt;br /&gt;
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&amp;lt;small&amp;gt;This page was moved from [[wikipedia:en:Hausdorff dimension]]. Its edit history can be viewed at [[分形维数/edithistory]]&amp;lt;/small&amp;gt;&amp;lt;/noinclude&amp;gt;&lt;br /&gt;
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[[Category:待整理页面]]&lt;/div&gt;</summary>
		<author><name>Ruili</name></author>
	</entry>
	<entry>
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		<title>分形维数</title>
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		<updated>2020-10-27T13:48:23Z</updated>

		<summary type="html">&lt;p&gt;Ruili：&lt;/p&gt;
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&lt;div&gt;此词条暂由彩云小译翻译，未经人工整理和审校，带来阅读不便，请见谅。&lt;br /&gt;
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{{short description|Invariant}}&lt;br /&gt;
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[[File:KochFlake.svg|thumb|280px|Example of non-integer dimensions. The first four [[iteration]]s of the [[Koch snowflake|Koch curve]], where after each iteration, all original line segments are replaced with four, each a self-similar copy that is 1/3 the length of the original. One formalism of the Hausdorff dimension uses this scale factor (3) and the number of self-similar objects (4) to calculate the dimension, D, after the first iteration to be D = (log N)/(log S) = (log 4)/(log 3) ≈ 1.26.&amp;lt;ref name=CampbellAnnenberg15&amp;gt;MacGregor Campbell, 2013, &amp;quot;5.6 Scaling and the Hausdorff Dimension,&amp;quot; at ''Annenberg Learner:MATHematics illuminated'', see [http://www.learner.org/courses/mathilluminated/units/5/textbook/06.php], accessed 5 March 2015.&amp;lt;/ref&amp;gt; That is, while the Hausdorff dimension of a single [[point (geometry)|point]] is zero, of a [[line segment]] is 1, of a [[square]] is 2, and of a [[cube]] is 3, for [[fractal]]s such as this, the object can have a non-integer dimension.]]&lt;br /&gt;
&lt;br /&gt;
Example of non-integer dimensions. The first four [[iterations of the Koch curve, where after each iteration, all original line segments are replaced with four, each a self-similar copy that is 1/3 the length of the original. One formalism of the Hausdorff dimension uses this scale factor (3) and the number of self-similar objects (4) to calculate the dimension, D, after the first iteration to be D = (log N)/(log S) = (log 4)/(log 3) ≈ 1.26. That is, while the Hausdorff dimension of a single point is zero, of a line segment is 1, of a square is 2, and of a cube is 3, for fractals such as this, the object can have a non-integer dimension.]]&lt;br /&gt;
&lt;br /&gt;
[[File:KochFlake.svg|thumb|280px|非整数维度示例：前四个[[Koch 曲线]]的迭代，在每次迭代后，所有原始线段都被替换为四个，每个自相似的复制是原始线段长度的1 / 3。豪斯多夫维数的一个建模是使用这个比例因子(3)和自相似物体的数量(4)来计算维度，设在第一次迭代后为 D = (log N)/(log S) = (log 4)/(log 3) ≈ 1.26.&amp;lt;ref name=CampbellAnnenberg15&amp;gt;。MacGregor Campbell, 2013, &amp;quot;5.6 Scaling and the Hausdorff Dimension,&amp;quot; 在 ''Annenberg Learner:MATHematics illuminated'', 参见 [http://www.learner.org/courses/mathilluminated/units/5/textbook/06.php], accessed 5 March 2015.&amp;lt;/ref&amp;gt; 也就是说，当一个点的豪斯多夫维数为零，线段为1，正方形为2，立方体为3时，对于像这样的分形，物体可以有一个非整数维度。]]&lt;br /&gt;
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In [[mathematics]], '''Hausdorff dimension''' is a measure of ''roughness'', or more specifically, [[fractal dimension]], that was first introduced in 1918 by [[mathematician]] [[Felix Hausdorff]].&amp;lt;ref&amp;gt;{{Cite journal |arxiv = 1101.1444|doi = 10.1214/11-STS370|title = Estimators of Fractal Dimension: Assessing the Roughness of Time Series and Spatial Data|journal = Statistical Science|volume = 27|issue = 2|pages = 247–277|year = 2012|last1 = Gneiting|first1 = Tilmann|last2 = Ševčíková|first2 = Hana|last3 = Percival|first3 = Donald B.}}&amp;lt;/ref&amp;gt; For instance, the Hausdorff dimension of a single [[point (geometry)|point]] is zero, of a [[line segment]] is 1, of a [[square]] is 2, and of a [[cube]] is 3. That is, for sets of points that define a smooth shape or a shape that has a small number of corners—the shapes of traditional geometry and science—the Hausdorff dimension is an [[integer]] agreeing with the usual sense of dimension, also known as the [[Inductive dimension|topological dimension]]. However, formulas have also been developed that allow calculation of the dimension of other less simple objects, where, solely on the basis of their properties of [[scaling (geometry)|scaling]] and [[self-similarity]], one is led to the conclusion that particular objects—including [[fractal]]s—have non-integer Hausdorff dimensions. Because of the significant technical advances made by [[Abram Samoilovitch Besicovitch]] allowing computation of dimensions for highly irregular or &amp;quot;rough&amp;quot; sets, this dimension is also commonly referred to as the ''Hausdorff–Besicovitch dimension.''&lt;br /&gt;
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In mathematics, Hausdorff dimension is a measure of roughness, or more specifically, fractal dimension, that was first introduced in 1918 by mathematician Felix Hausdorff. For instance, the Hausdorff dimension of a single point is zero, of a line segment is 1, of a square is 2, and of a cube is 3. That is, for sets of points that define a smooth shape or a shape that has a small number of corners—the shapes of traditional geometry and science—the Hausdorff dimension is an integer agreeing with the usual sense of dimension, also known as the topological dimension. However, formulas have also been developed that allow calculation of the dimension of other less simple objects, where, solely on the basis of their properties of scaling and self-similarity, one is led to the conclusion that particular objects—including fractals—have non-integer Hausdorff dimensions. Because of the significant technical advances made by Abram Samoilovitch Besicovitch allowing computation of dimensions for highly irregular or &amp;quot;rough&amp;quot; sets, this dimension is also commonly referred to as the Hausdorff–Besicovitch dimension.&lt;br /&gt;
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在[[数学]]中，'''&amp;lt;font color = '#ff8000'&amp;gt;豪斯多夫维数Hausdorff dimension&amp;lt;/font&amp;gt;'''是一种粗糙度的度量单位，或者更确切地说，分形维数，是由数学家 Felix Hausdorff 在1918年首次提出的。例如，单点的豪斯多夫维数为零，线段为1，正方形为2，立方体为3。也就是说，对于定义了一个光滑形状或一个有少数几个角的形状---- 传统几何学和科学的形状---- 的点集来说，豪斯多夫维数是一个整数，符合通常的维度意义，也称为拓扑维度。然而，还有一些公式允许计算其他不太简单的对象的维数，其中仅仅根据它们的标度和自相似特性，就可以得出结论: 特定的对象ー包括分形ー具有非整数的 Hausdorff 维数。由于阿布拉姆·萨莫伊洛维奇·贝西科维奇的重大技术进步，允许计算高度不规则或“粗糙”集的维度，这个维度通常也被称为 Hausdorff-Besicovitch 维度。 &lt;br /&gt;
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The Hausdorff dimension, more specifically, is a further dimensional number associated with a given set, where the distances between all members of that set are defined. Such a set is termed a [[metric space]]. The dimension is drawn from the [[Extended real number line|extended real numbers]], &amp;lt;math&amp;gt;\overline{\mathbb{R}}&amp;lt;/math&amp;gt;, as opposed to the more intuitive notion of dimension, which is not associated to general metric spaces, and only takes values in the non-negative integers.&lt;br /&gt;
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The Hausdorff dimension, more specifically, is a further dimensional number associated with a given set, where the distances between all members of that set are defined. Such a set is termed a metric space. The dimension is drawn from the extended real numbers, &amp;lt;math&amp;gt;\overline{\mathbb{R}}&amp;lt;/math&amp;gt;, as opposed to the more intuitive notion of dimension, which is not associated to general metric spaces, and only takes values in the non-negative integers.&lt;br /&gt;
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更具体地说，豪斯多夫维数是一个与给定集合相关联的更进一步的维数，其中定义了该集合所有成员之间的距离。这样的集合称为度量空间。维数是从扩展的实数，&amp;lt;math&amp;gt;\overline{\mathbb{R}}&amp;lt;/math&amp;gt;，而不是更直观的维数概念(它不与一般的度量空间相关联，只取非负整数的值)。&lt;br /&gt;
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In mathematical terms, the Hausdorff dimension generalizes the notion of the dimension of a real [[vector space]]. That is, the Hausdorff dimension of an ''n''-dimensional [[inner product space]] equals ''n''. This underlies the earlier statement that the Hausdorff dimension of a point is zero, of a line is one, etc., and that [[fractal|irregular sets]] can have noninteger Hausdorff dimensions. For instance, the [[Koch snowflake]] shown at right is constructed from an equilateral triangle; in each iteration, its component line segments are divided into 3 segments of unit length, the newly created middle segment is used as the base of a new [[equilateral]] triangle that points outward, and this base segment is then deleted to leave a final object from the iteration of unit length of 4.&amp;lt;ref&amp;gt;Larry Riddle, 2014, &amp;quot;Classic Iterated Function Systems: Koch Snowflake&amp;quot;, Agnes Scott College e-Academy (online), see [http://ecademy.agnesscott.edu/~lriddle/ifs/ksnow/ksnow.htm], accessed 5 March 2015.&amp;lt;/ref&amp;gt; That is, after the first iteration, each original line segment has been replaced with N=4, where each self-similar copy is 1/S = 1/3 as long as the original.&amp;lt;ref name=CampbellAnnenberg15/&amp;gt; Stated another way, we have taken an object with Euclidean dimension, D, and reduced its linear scale by 1/3 in each direction, so that its length increases to N=S&amp;lt;sup&amp;gt;D&amp;lt;/sup&amp;gt;.&amp;lt;ref name=ClaytonSCTPLS96&amp;gt;Keith Clayton, 1996, &amp;quot;Fractals and the Fractal Dimension,&amp;quot; ''Basic Concepts in Nonlinear Dynamics and Chaos'' (workshop), Society for Chaos Theory in Psychology and the Life Sciences annual meeting, June 28, 1996, Berkeley, California, see [http://www.vanderbilt.edu/AnS/psychology/cogsci/chaos/workshop/Workshop.html], accessed 5 March 2015.&amp;lt;/ref&amp;gt; This equation is easily solved for D, yielding the ratio of logarithms (or [[natural logarithm]]s) appearing in the figures, and giving—in the Koch and other fractal cases—non-integer dimensions for these objects.&lt;br /&gt;
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In mathematical terms, the Hausdorff dimension generalizes the notion of the dimension of a real vector space. That is, the Hausdorff dimension of an n-dimensional inner product space equals n. This underlies the earlier statement that the Hausdorff dimension of a point is zero, of a line is one, etc., and that irregular sets can have noninteger Hausdorff dimensions. For instance, the Koch snowflake shown at right is constructed from an equilateral triangle; in each iteration, its component line segments are divided into 3 segments of unit length, the newly created middle segment is used as the base of a new equilateral triangle that points outward, and this base segment is then deleted to leave a final object from the iteration of unit length of 4. That is, after the first iteration, each original line segment has been replaced with N=4, where each self-similar copy is 1/S = 1/3 as long as the original. This equation is easily solved for D, yielding the ratio of logarithms (or natural logarithms) appearing in the figures, and giving—in the Koch and other fractal cases—non-integer dimensions for these objects.&lt;br /&gt;
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用数学术语来说，豪斯多夫维数概括了实向量空间维数的概念。也就是说，n 维内积空间的豪斯多夫维数等于 n。 这就是早期假设的基础，一个点的豪斯多夫维数是零，一条线是一等等，不规则集可以有非整数的豪斯多夫维数。例如，右边所示的 Koch 雪花是由一个正三角形构成的; 在每次迭代中，它的组成线段被分成单位长度的3段，新创建的中间线段被用作一个指向外部的新正三角形的基础，然后人们删除这个基础线段用来保留单位长度4的迭代中的最终对象。也就是说，在第一次迭代之后，每个原始线段都被替换为 N=4，其中每个自相似拷贝的长度是原始线段的1/S = 1/3 。这个方程很容易求解为 D，产生出现在图形中的对数(或自然对数)的比率，并给出——在 Koch 和其他分形情况下——这些对象的非整数维数。&lt;br /&gt;
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The Hausdorff dimension is a successor to the simpler, but usually equivalent, box-counting or [[Minkowski–Bouligand dimension]].&lt;br /&gt;
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The Hausdorff dimension is a successor to the simpler, but usually equivalent, box-counting or Minkowski–Bouligand dimension.&lt;br /&gt;
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豪斯多夫维数是更简单但通常等价的'''&amp;lt;font color = '#ff8000'&amp;gt;计盒维数box-counting&amp;lt;/font&amp;gt;'''或'''&amp;lt;font color = '#ff8000'&amp;gt;闵可夫斯基维数Minkowski-Bouligand&amp;lt;/font&amp;gt;'''的继承者。&lt;br /&gt;
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==Intuition概念==&lt;br /&gt;
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The intuitive concept of dimension of a geometric object ''X'' is the number of independent parameters one needs to pick out a unique point inside. However, any point specified by two parameters can be instead specified by one, because the [[cardinality]] of the [[real plane]] is equal to the cardinality of the [[real line]] (this can be seen by an [[Cantor's diagonal argument|argument]] involving interweaving the digits of two numbers to yield a single number encoding the same information). The example of a [[space-filling curve]] shows that one can even map the real line to the real plane [[Surjective function|surjectively]] (taking one real number into a pair of real numbers in a way so that all pairs of numbers are covered) and ''continuously'', so that a one-dimensional object completely fills up a higher-dimensional object.&lt;br /&gt;
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The intuitive concept of dimension of a geometric object X is the number of independent parameters one needs to pick out a unique point inside. However, any point specified by two parameters can be instead specified by one, because the cardinality of the real plane is equal to the cardinality of the real line (this can be seen by an argument involving interweaving the digits of two numbers to yield a single number encoding the same information). The example of a space-filling curve shows that one can even map the real line to the real plane surjectively (taking one real number into a pair of real numbers in a way so that all pairs of numbers are covered) and continuously, so that a one-dimensional object completely fills up a higher-dimensional object.&lt;br /&gt;
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几何物体X的直观尺寸概念就是一个物体需要多少个独立参数才能找到一个独特的点。但是，任何由两个参数指定的点都可以由一个参数指定，因为实际平面的基数等于实际行的基数(这可以通过一个参数看到，该参数涉及交织两个数字的数字以产生一个编码相同信息的单个数字)。'''&amp;lt;font color = '#ff8000'&amp;gt;皮亚诺曲线&amp;lt;/font&amp;gt;'''的例子表明，一个人甚至可以完美和连续地映射实际线到真正的平面(把一个实数转换成一对实数，这样所有的数对都被覆盖)，由此一维物体完全填充了一个高维物体。&lt;br /&gt;
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Every space filling curve hits some points multiple times, and does not have a continuous inverse. It is impossible to map two dimensions onto one in a way that is continuous and continuously invertible. The topological dimension, also called [[Lebesgue covering dimension]], explains why. This dimension is ''n'' if, in every covering of ''X'' by small open balls, there is at least one point where ''n''&amp;amp;nbsp;+&amp;amp;nbsp;1 balls overlap. For example, when one covers a line with short open intervals, some points must be covered twice, giving dimension&amp;amp;nbsp;''n''&amp;amp;nbsp;=&amp;amp;nbsp;1.&lt;br /&gt;
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Every space filling curve hits some points multiple times, and does not have a continuous inverse. It is impossible to map two dimensions onto one in a way that is continuous and continuously invertible. The topological dimension, also called Lebesgue covering dimension, explains why. This dimension is n if, in every covering of X by small open balls, there is at least one point where n&amp;amp;nbsp;+&amp;amp;nbsp;1 balls overlap. For example, when one covers a line with short open intervals, some points must be covered twice, giving dimension&amp;amp;nbsp;n&amp;amp;nbsp;=&amp;amp;nbsp;1.&lt;br /&gt;
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每条空间填充曲线都会多次撞击某些点，且不存在连续的倒数。将两个维度以连续和连续可逆的方式映射到一个维度是不可能的。'''&amp;lt;font color = '#ff8000'&amp;gt;拓扑维度 topological dimension&amp;lt;/font&amp;gt;'''，也被称为拓朴维数，解释了为什么。这个维度是 n，如果在 x 的每个小开球覆盖中，至少有一个点 n + 1个球重叠。例如，当一个点覆盖一条具有短开区间的直线时，某些点必须被覆盖两次，给出维数''n''&amp;amp;nbsp;=&amp;amp;nbsp;1。&lt;br /&gt;
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But topological dimension is a very crude measure of the local size of a space (size near a point). A curve that is almost space-filling can still have topological dimension one, even if it fills up most of the area of a region. A [[fractal]] has an integer topological dimension, but in terms of the amount of space it takes up, it behaves like a higher-dimensional space.&lt;br /&gt;
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But topological dimension is a very crude measure of the local size of a space (size near a point). A curve that is almost space-filling can still have topological dimension one, even if it fills up most of the area of a region. A fractal has an integer topological dimension, but in terms of the amount of space it takes up, it behaves like a higher-dimensional space.&lt;br /&gt;
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但是，拓扑维度是对空间局部尺寸(点附近的尺寸)的一个非常粗略的度量。一条几乎是空间填充的曲线仍然可以有一维拓扑，即使它填充了一个区域的大部分面积。分形具有整数的拓扑维数，但就其所占空间的数量而言，它看起来像一个更高维的空间。&lt;br /&gt;
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The Hausdorff dimension measures the local size of a space taking into account the distance between points, the [[metric space|metric]]. Consider the number ''N''(''r'') of [[ball (mathematics)|balls]] of radius at most ''r'' required to cover ''X'' completely. When ''r'' is very small, ''N''(''r'') grows polynomially with 1/''r''. For a sufficiently well-behaved  ''X'', the Hausdorff dimension is the unique number ''d'' such that N(''r'') grows as 1/''r&amp;lt;sup&amp;gt;d&amp;lt;/sup&amp;gt;'' as ''r'' approaches zero. More precisely, this defines the [[Minkowski–Bouligand dimension|box-counting dimension]], which equals the Hausdorff dimension when the value ''d'' is a critical boundary between growth rates that are insufficient to cover the space, and growth rates that are overabundant.&lt;br /&gt;
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The Hausdorff dimension measures the local size of a space taking into account the distance between points, the metric. Consider the number N(r) of balls of radius at most r required to cover X completely. When r is very small, N(r) grows polynomially with 1/r. For a sufficiently well-behaved  X, the Hausdorff dimension is the unique number d such that N(r) grows as 1/r&amp;lt;sup&amp;gt;d&amp;lt;/sup&amp;gt; as r approaches zero. More precisely, this defines the box-counting dimension, which equals the Hausdorff dimension when the value d is a critical boundary between growth rates that are insufficient to cover the space, and growth rates that are overabundant.&lt;br /&gt;
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豪斯多夫维数测量一个空间的局部大小时，会考虑到点之间距离的度量。考虑半径最大为 r 的球数 ''N'' (r) ，需要完全覆盖 ''X''。当 r 很小时，n (r)以1/''r'' 增长多项式。对于一个表现足够好的 ''X''，豪斯多夫维数是唯一的数 d，这样当 r 趋近于零时， N(r)增长为1/r&amp;lt;sup&amp;gt;d&amp;lt;/sup&amp;gt; 。更确切地说，这定义了盒子计数维度，当值 d 是不足以覆盖空间的增长率和过度充裕的增长率之间的关键边界时，它等于豪斯多夫维数。&lt;br /&gt;
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For shapes that are smooth, or shapes with a small number of corners, the shapes of traditional geometry and science, the Hausdorff dimension is an integer agreeing with the topological dimension. But [[Benoit Mandelbrot]] observed that [[fractal]]s, sets with noninteger Hausdorff dimensions, are found everywhere in nature. He observed that the proper idealization of most rough shapes you see around you is not in terms of smooth idealized shapes, but in terms of fractal idealized shapes:&lt;br /&gt;
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For shapes that are smooth, or shapes with a small number of corners, the shapes of traditional geometry and science, the Hausdorff dimension is an integer agreeing with the topological dimension. But Benoit Mandelbrot observed that fractals, sets with noninteger Hausdorff dimensions, are found everywhere in nature. He observed that the proper idealization of most rough shapes you see around you is not in terms of smooth idealized shapes, but in terms of fractal idealized shapes:&lt;br /&gt;
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对于光滑的形状，或者有少量棱角的形状，传统几何和科学的形状，豪斯多夫维数是一个整数，与拓扑维度一致。但是伯努·曼德布洛特观察到分形---- 具有非整数豪斯多夫维数的集合---- 在自然界中随处可见。他观察到，我们周围大多数粗糙形状的理想化不是光滑的理想化形状，而是分形理想化形状:&lt;br /&gt;
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&amp;lt;blockquote&amp;gt;Clouds are not spheres, mountains are not cones, coastlines are not circles, and bark is not smooth, nor does lightning travel in a straight line.&amp;lt;ref name=&amp;quot;mandelbrot&amp;quot;&amp;gt;{{cite book   | last = Mandelbrot   | first = Benoît   | authorlink = Benoit Mandelbrot   | title = The Fractal Geometry of Nature   | publisher = W. H. Freeman   | series = Lecture notes in mathematics 1358   | year = 1982   | doi =    | isbn = 0-7167-1186-9   | url-access = registration   | url = https://archive.org/details/fractalgeometryo00beno   }}&amp;lt;/ref&amp;gt;&amp;lt;/blockquote&amp;gt;&lt;br /&gt;
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&amp;lt;blockquote&amp;gt;Clouds are not spheres, mountains are not cones, coastlines are not circles, and bark is not smooth, nor does lightning travel in a straight line.&amp;lt;/blockquote&amp;gt;&lt;br /&gt;
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&amp;lt;blockquote&amp;gt;云不是球体，山不是锥体，海岸线不是圆圈，树皮不平滑，闪电也不是直线运动。 &amp;lt;/blockquote&amp;gt;&lt;br /&gt;
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For fractals that occur in nature, the Hausdorff and [[Minkowski–Bouligand dimension|box-counting dimension]] coincide. The [[packing dimension]] is yet another similar notion which gives the same value for many shapes, but there are well documented exceptions where all these dimensions differ.&lt;br /&gt;
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For fractals that occur in nature, the Hausdorff and box-counting dimension coincide. The packing dimension is yet another similar notion which gives the same value for many shapes, but there are well documented exceptions where all these dimensions differ.&lt;br /&gt;
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对于自然界中出现的分形，豪斯多夫维数和盒计数维数是一致的。封装尺寸是另一个类似的概念，它给出了许多形状相同的值，但是在所有这些尺寸不同的情况，都做了很好的说明。&lt;br /&gt;
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==Formal definitions形式化定义==&lt;br /&gt;
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===Hausdorff content豪斯多夫集===&lt;br /&gt;
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Let ''X'' be a [[metric space]]. If ''S'' ⊂ ''X'' and ''d'' ∈ [0, ∞), the ''d''-dimensional '''unlimited Hausdorff content''' of ''S'' is defined by&lt;br /&gt;
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Let X be a metric space. If S ⊂ X and d ∈ [0, ∞), the d-dimensional unlimited Hausdorff content of S is defined by&lt;br /&gt;
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设 ''X''是度量空间。若''S'' ⊂ ''X'' 和 ''d'' ∈ [0, ∞) ，则 ''S'' 的''d''维无限 豪斯多夫集定义为&lt;br /&gt;
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:&amp;lt;math&amp;gt;C_H^d(S):=\inf\Bigl\{\sum_i r_i^d:\text{ there is a cover of } S\text{ by balls with radii }r_i&amp;gt;0\Bigr\}.&amp;lt;/math&amp;gt;&lt;br /&gt;
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&amp;lt;math&amp;gt;C_H^d(S):=\inf\Bigl\{\sum_i r_i^d:\text{ there is a cover of } S\text{ by balls with radii }r_i&amp;gt;0\Bigr\}.&amp;lt;/math&amp;gt;&lt;br /&gt;
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&amp;lt;math&amp;gt;C_H^d(S):=\inf\Bigl\{\sum_i r_i^d:\text{ there is a cover of } S\text{ by balls with radii }r_i&amp;gt;0\Bigr\}.&amp;lt;/math&amp;gt;&lt;br /&gt;
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In other words, &amp;lt;math&amp;gt;C_H^d(S)&amp;lt;/math&amp;gt; is the [[infimum]] of the set of numbers &amp;lt;math&amp;gt;\delta \geq 0&amp;lt;/math&amp;gt; such that there is some (indexed) collection of [[ball (mathematics)|ball]]s &amp;lt;math&amp;gt;\{B(x_i,r_i):i\in I\}&amp;lt;/math&amp;gt; covering ''S'' with ''r&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;''&amp;amp;nbsp;&amp;gt;&amp;amp;nbsp;0 for each ''i''&amp;amp;nbsp;∈&amp;amp;nbsp;''I'' that satisfies &amp;lt;math&amp;gt;\sum_{i\in I} r_i^d&amp;lt;\delta &amp;lt;/math&amp;gt;. (Here, we use the standard convention that [[infimum|inf&amp;amp;nbsp;Ø&amp;amp;nbsp;=&amp;amp;nbsp;∞]].)&lt;br /&gt;
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In other words, &amp;lt;math&amp;gt;C_H^d(S)&amp;lt;/math&amp;gt; is the infimum of the set of numbers &amp;lt;math&amp;gt;\delta \geq 0&amp;lt;/math&amp;gt; such that there is some (indexed) collection of balls &amp;lt;math&amp;gt;\{B(x_i,r_i):i\in I\}&amp;lt;/math&amp;gt; covering S with r&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;&amp;amp;nbsp;&amp;gt;&amp;amp;nbsp;0 for each i&amp;amp;nbsp;∈&amp;amp;nbsp;I that satisfies &amp;lt;math&amp;gt;\sum_{i\in I} r_i^d&amp;lt;\delta &amp;lt;/math&amp;gt;. (Here, we use the standard convention that inf&amp;amp;nbsp;Ø&amp;amp;nbsp;=&amp;amp;nbsp;∞.)&lt;br /&gt;
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换句话说，&amp;lt;math&amp;gt;C_H^d(S)&amp;lt;/math&amp;gt; 是数字集合&amp;lt;math&amp;gt;\delta \geq 0&amp;lt;/math&amp;gt;的下确界，使得在 ''i''&amp;amp;nbsp;∈&amp;amp;nbsp中存在一些球集合 &amp;lt;math&amp;gt;\{B(x_i,r_i):i\in I\}&amp;lt;/math&amp;gt;  i 包含 s，对于每个 ''r&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;''&amp;amp;nbsp;&amp;gt;&amp;amp;nbsp;0 满足 i 中的和&amp;lt;math&amp;gt;\sum_{i\in I} r_i^d&amp;lt;\delta &amp;lt;/math&amp;gt; (在这里，我们使用inf&amp;amp;nbsp;Ø&amp;amp;nbsp;=&amp;amp;nbsp;∞ )的标准约定。&lt;br /&gt;
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===Hausdorff measurement豪斯多夫分形测量===&lt;br /&gt;
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The Hausdorff outer measure is different from the unbounded Hausdorf content in that rather than considering all possible coverings of ''S'', we see what happens when the sizes of the balls go to zero. This is  for &amp;lt;math&amp;gt;d \geq 0 &amp;lt;/math&amp;gt;, we define the ''d''-dimensional Hausdorff outer measure of ''S'' as&lt;br /&gt;
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The Hausdorff outer measure is different from the unbounded Hausdorf content in that rather than considering all possible coverings of S, we see what happens when the sizes of the balls go to zero. This is  for &amp;lt;math&amp;gt;d \geq 0 &amp;lt;/math&amp;gt;, we define the d-dimensional Hausdorff outer measure of S as&lt;br /&gt;
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豪斯多夫外测度不同于无界的豪斯多夫，因为我们不考虑 s 的所有可能，我们看到当球的大小为零时会发生什么。这是为了数学  &amp;lt;math&amp;gt;d \geq 0 &amp;lt;/math&amp;gt;，我们定义了  ''S''的 ''d''维豪斯多夫Hausdorff 外测度为&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt; \mathcal{H}^d(S):=\lim_{r \to 0} \inf\Bigl\{\sum_i r_i^d:\text{ there is a cover of } S\text{ by balls with radii } 0 &amp;lt; r_i &amp;lt; r\Bigr\}.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \mathcal{H}^d(S):=\lim_{r \to 0} \inf\Bigl\{\sum_i r_i^d:\text{ there is a cover of } S\text{ by balls with radii } 0 &amp;lt; r_i &amp;lt; r\Bigr\}.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \mathcal{H}^d(S):=\lim_{r \to 0} \inf\Bigl\{\sum_i r_i^d:\text{有一个面} S\text{ 球 } 0 &amp;lt; r_i &amp;lt; r\Bigr\}.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
===Hausdorff dimension豪斯多夫维数===&lt;br /&gt;
&lt;br /&gt;
The '''Hausdorff dimension''' of ''X'' is defined by&lt;br /&gt;
&lt;br /&gt;
The Hausdorff dimension of X is defined by&lt;br /&gt;
&lt;br /&gt;
X 的豪斯多夫维数定义为&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt;\dim_{\operatorname{H}}(X):=\inf\{d\ge 0: \mathcal{H}^d(X)=0\}.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt;\dim_{\operatorname{H}}(X):=\inf\{d\ge 0: \mathcal{H}^d(X)=0\}.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Equivalently, dim&amp;lt;sub&amp;gt;H&amp;lt;/sub&amp;gt;(''X'') may be defined as the [[infimum]] of the set of ''d'' ∈ [0, ∞) such that the ''d''-dimensional [[Hausdorff measure]] of ''X'' is zero. This is the same as the supremum of the set of ''d''&amp;amp;nbsp;∈&amp;amp;nbsp;[0,&amp;amp;nbsp;∞) such that the ''d''-dimensional Hausdorff measure of ''X'' is infinite (except that when this latter set of numbers ''d'' is empty the Hausdorff dimension is zero).&lt;br /&gt;
&lt;br /&gt;
Equivalently, dim&amp;lt;sub&amp;gt;H&amp;lt;/sub&amp;gt;(X) may be defined as the infimum of the set of d ∈ [0, ∞) such that the d-dimensional Hausdorff measure of X is zero. This is the same as the supremum of the set of d&amp;amp;nbsp;∈&amp;amp;nbsp;[0,&amp;amp;nbsp;∞) such that the d-dimensional Hausdorff measure of X is infinite (except that when this latter set of numbers d is empty the Hausdorff dimension is zero).&lt;br /&gt;
&lt;br /&gt;
等价地，dim &amp;lt;sub&amp;gt;H&amp;lt;/sub&amp;gt;(''X'')可定义为 ''d'' ∈ [0, ∞) 集的下确界，使得''X'' 的''d''-维 [[豪斯多夫测度]] 为零。这与 ''d''&amp;amp;nbsp;∈&amp;amp;nbsp;[0,&amp;amp;nbsp;∞)的集合的上确界相同，因此''X''的 d 维豪斯多夫测度是无限的(除非后一个集合 ''d'' 是空的，豪斯多夫维数为零)。&lt;br /&gt;
&lt;br /&gt;
==Examples实例==&lt;br /&gt;
&lt;br /&gt;
[[Image:Sierpinski deep.svg|thumb|250px|Dimension of a further [[fractal]] example. The [[Sierpinski triangle]], an object with Hausdorff dimension of log(3)/log(2)≈1.58.&amp;lt;ref name=ClaytonSCTPLS96/&amp;gt;]]&lt;br /&gt;
&lt;br /&gt;
Dimension of a further [[fractal example. The Sierpinski triangle, an object with Hausdorff dimension of log(3)/log(2)≈1.58.]]&lt;br /&gt;
&lt;br /&gt;
[[Image:谢尔宾斯基三角形 deep.svg|thumb|250px|进一步的[[分形维数]]的例子，进一步的分形维数的例子是谢尔宾斯基三角形，它是一个豪斯多夫维数为log(3)/log(2)≈1.58.&amp;lt;ref name=ClaytonSCTPLS96/&amp;gt;的物体]]&lt;br /&gt;
&lt;br /&gt;
* [[Countable set]]s have Hausdorff dimension 0.&amp;lt;ref name=&amp;quot;schleicher&amp;quot;&amp;gt;{{cite journal |last1=Schleicher |first1=Dierk |title=Hausdorff Dimension, Its Properties, and Its Surprises |journal=The American Mathematical Monthly |date=June 2007 |volume=114 |issue=6 |pages=509–528 |doi=10.1080/00029890.2007.11920440 |language=en |issn=0002-9890|arxiv=math/0505099 }}&amp;lt;/ref&amp;gt;&lt;br /&gt;
*[[可数集]]拥有豪斯多夫维数0.&amp;lt;ref name=&amp;quot;schleicher&amp;quot;&amp;gt;{{cite journal |last1=Schleicher |first1=Dierk |title=豪斯多夫维数, Its Properties, and Its Surprises |journal=The American Mathematical Monthly美国数学期刊 |date=June 2007 |volume=114 |issue=6 |pages=509–528 |doi=10.1080/00029890.2007.11920440 |language=en |issn=0002-9890|arxiv=math/0505099 }}&amp;lt;/ref&amp;gt;&lt;br /&gt;
* The [[Euclidean space]] ℝ&amp;lt;sup&amp;gt;''n''&amp;lt;/sup&amp;gt; has Hausdorff dimension ''n'', and the circle '''S'''&amp;lt;sup&amp;gt;1&amp;lt;/sup&amp;gt; has Hausdorff dimension 1.&amp;lt;ref name=&amp;quot;schleicher&amp;quot; /&amp;gt;&lt;br /&gt;
*[[教育空间]] ℝ&amp;lt;sup&amp;gt;''n''&amp;lt;/sup&amp;gt; 有豪斯多夫维数 ''n''，循环'''S'''&amp;lt;sup&amp;gt;1&amp;lt;/sup&amp;gt; 拥有豪斯多夫维数1.&amp;lt;ref name=&amp;quot;schleicher&amp;quot; /&amp;gt;&lt;br /&gt;
* [[Fractal]]s often are spaces whose Hausdorff dimension strictly exceeds the [[topological dimension]].&amp;lt;ref name=&amp;quot;mandelbrot&amp;quot; /&amp;gt; For example, the [[Cantor set]], a zero-dimensional topological space, is a union of two copies of itself, each copy shrunk by a factor 1/3; hence, it can be shown that its Hausdorff dimension is ln(2)/ln(3)&amp;amp;nbsp;≈&amp;amp;nbsp;0.63.&amp;lt;ref&amp;gt;{{cite book | last=Falconer | first = Kenneth |title=Fractal Geometry: Mathematical Foundations and Applications | publisher=[[John Wiley and Sons]] | edition=2nd | year=2003}}&amp;lt;/ref&amp;gt; The [[Sierpinski triangle]] is a union of three copies of itself, each copy shrunk by a factor of&amp;amp;nbsp;1/2; this yields a Hausdorff dimension of ln(3)/ln(2)&amp;amp;nbsp;≈&amp;amp;nbsp;1.58.&amp;lt;ref name=CampbellAnnenberg15/&amp;gt; These Hausdorff dimensions are related to the &amp;quot;critical exponent&amp;quot; of the [[Master theorem (analysis of algorithms)|Master theorem]] for solving [[Recurrence relation|recurrence relations]] in the [[analysis of algorithms]].&lt;br /&gt;
*[[分形]]一般是那些豪斯多夫维数直接超过其拓扑维数的空间。例如[[康托尔集]]是一个o维拓扑空间，由两个自己复制而成，每一个复制品都是原来的三分之一，因此它的豪斯多夫维数是 ln(2)/ln(3)&amp;amp;nbsp;≈&amp;amp;nbsp;0.63。&amp;lt;ref&amp;gt;{{cite book | last=Falconer | first = Kenneth |title=Fractal Geometry: Mathematical Foundations and Applications | publisher=[[John Wiley and Sons]] | edition=2nd | year=2003}}&amp;lt;/ref&amp;gt;一个[[谢尔宾斯基三角]]是他自身三个复制的组合。每一个是原来的&amp;amp;nbsp;1/2，它的豪斯多夫维数ln(3)/ln(2)&amp;amp;nbsp;≈&amp;amp;nbsp;1.58。&amp;lt;ref name=CampbellAnnenberg15/&amp;gt;在递归算法中解决递归关系时，这些豪斯多夫维数与[[算法分析主定理]]的临界指标相联系。&lt;br /&gt;
* [[Space-filling curve]]s like the [[Peano curve]] have the same Hausdorff dimension as the space they fill.&lt;br /&gt;
*[[空间填充曲线]]拥有和他们填充空间同样的豪斯多夫维数，如[[皮亚诺曲线]]。&lt;br /&gt;
* The trajectory of [[Brownian motion]] in dimension 2 and above is conjectured to be Hausdorff dimension 2.&amp;lt;ref&amp;gt;{{cite book | last=Morters | first=Peres | title= Brownian Motion | publisher=[[Cambridge University Press]] | year=2010 }}&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
[[image:Great Britain Hausdorff.svg|thumb|250px|Estimating the Hausdorff dimension of the [[How Long Is the Coast of Britain? Statistical Self-Similarity and Fractional Dimension|coast of Great Britain]]]]&lt;br /&gt;
&lt;br /&gt;
coast of Great Britain]]&lt;br /&gt;
&lt;br /&gt;
[[大不列颠海岸&lt;br /&gt;
&lt;br /&gt;
* 刘易斯·弗赖伊·理查森[[Lewis Fry Richardson]] has performed detailed experiments to measure the approximate Hausdorff dimension for various coastlines. His results have varied from 1.02 for the coastline of [[South Africa]] to 1.25 for the west coast of [[Great Britain]].&amp;lt;ref name=&amp;quot;mandelbrot&amp;quot; /&amp;gt;&lt;br /&gt;
*刘易斯·弗赖伊·理查森（Lewis Fry Richardson）已经通过豪斯多夫维数去测量了很多海岸线。它的结果涵盖从1.02的南非海岸线到1.25的大英帝国西海岸模型。]]&lt;br /&gt;
&lt;br /&gt;
==Properties of Hausdorff dimension豪斯多夫维数特性==&lt;br /&gt;
&lt;br /&gt;
{{refimprove section|date=March 2015}}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
=== Hausdorff dimension and inductive dimension 豪斯多夫维数和归纳维数===&lt;br /&gt;
&lt;br /&gt;
Let ''X'' be an arbitrary [[Separable space|separable]] metric space. There is a [[topology|topological]] notion of [[inductive dimension]] for ''X'' which is defined recursively. It is always an integer (or +∞) and is denoted dim&amp;lt;sub&amp;gt;ind&amp;lt;/sub&amp;gt;(''X'').&lt;br /&gt;
&lt;br /&gt;
Let X be an arbitrary separable metric space. There is a topological notion of inductive dimension for X which is defined recursively. It is always an integer (or +∞) and is denoted dim&amp;lt;sub&amp;gt;ind&amp;lt;/sub&amp;gt;(X).&lt;br /&gt;
&lt;br /&gt;
设''X'' 是[[任意可分度量空间]]。对于''X'' 有一个递归定义的归纳维数拓扑概念。它总是一个整数(或 + ∞) ，并且表示dim&amp;lt;sub&amp;gt;ind&amp;lt;/sub&amp;gt;(''X'')。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
'''Theorem'''. Suppose ''X'' is non-empty. Then &lt;br /&gt;
&lt;br /&gt;
Theorem. Suppose X is non-empty. Then &lt;br /&gt;
&lt;br /&gt;
'''定理'''：假设''X'' 是非空的。那么&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt; \dim_{\mathrm{Haus}}(X) \geq \dim_{\operatorname{ind}}(X). &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \dim_{\mathrm{Haus}}(X) \geq \dim_{\operatorname{ind}}(X). &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Moreover,&lt;br /&gt;
&lt;br /&gt;
Moreover,&lt;br /&gt;
&lt;br /&gt;
此外,&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \inf_Y \dim_{\operatorname{Haus}}(Y) =\dim_{\operatorname{ind}}(X), &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \inf_Y \dim_{\operatorname{Haus}}(Y) =\dim_{\operatorname{ind}}(X), &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
where ''Y'' ranges over metric spaces [[homeomorphic]] to ''X''. In other words, ''X'' and ''Y'' have the same underlying set of points and the metric ''d''&amp;lt;sub&amp;gt;''Y''&amp;lt;/sub&amp;gt; of ''Y'' is topologically equivalent to ''d''&amp;lt;sub&amp;gt;''X''&amp;lt;/sub&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
where Y ranges over metric spaces homeomorphic to X. In other words, X and Y have the same underlying set of points and the metric d&amp;lt;sub&amp;gt;Y&amp;lt;/sub&amp;gt; of Y is topologically equivalent to d&amp;lt;sub&amp;gt;X&amp;lt;/sub&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
其中''Y''是度量空间同胚到 ''X''的范围。换句话说， ''X''和 ''Y''具有相同的基本点集，''Y''的度规''d''&amp;lt;sub&amp;gt;''Y''&amp;lt;/sub&amp;gt; 的子拓扑等价于''d''&amp;lt;sub&amp;gt;''X''&amp;lt;/sub&amp;gt;。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
These results were originally established by [[Edward Szpilrajn]] (1907–1976), e.g., see Hurewicz and Wallman, Chapter VII.{{full citation needed|date=March 2015}}&lt;br /&gt;
&lt;br /&gt;
These results were originally established by Edward Szpilrajn (1907–1976), e.g., see Hurewicz and Wallman, Chapter VII.&lt;br /&gt;
&lt;br /&gt;
这些结果最初是由 [[Edward Szpilrajn]] (1907–1976)建立的,  参见 Hurewicz and Wallman, Chapter VII.{{full citation needed|date=March 2015}}第七章。&lt;br /&gt;
&lt;br /&gt;
=== Hausdorff dimension and Minkowski dimension 豪斯多夫维数和闵可夫斯基维度===&lt;br /&gt;
&lt;br /&gt;
The [[Minkowski dimension]] is similar to, and at least as large as, the Hausdorff dimension, and they are equal in many situations. However, the set of [[rational number|rational]] points in [0, 1] has Hausdorff dimension zero and Minkowski dimension one. There are also compact sets for which the Minkowski dimension is strictly larger than the Hausdorff dimension.&lt;br /&gt;
&lt;br /&gt;
The Minkowski dimension is similar to, and at least as large as, the Hausdorff dimension, and they are equal in many situations. However, the set of rational points in [0, 1] has Hausdorff dimension zero and Minkowski dimension one. There are also compact sets for which the Minkowski dimension is strictly larger than the Hausdorff dimension.&lt;br /&gt;
&lt;br /&gt;
[[闵可夫斯基维数]]与豪斯多夫维数相似，至少和它一样大，而且在许多情况下是相等的。然而，[0,1]中有理点集的豪斯多夫维数为0，闵可夫斯基维数为1。还有一些紧集的闵可夫斯基维数绝对大于豪斯多夫维数。&lt;br /&gt;
&lt;br /&gt;
=== Hausdorff dimensions and Frostman measures 豪斯多夫维度和弗洛斯曼测度===&lt;br /&gt;
&lt;br /&gt;
If there is a [[measure (mathematics)|measure]] μ defined on [[Borel measure|Borel]] subsets of a metric space ''X'' such that ''μ''(''X'') &amp;gt; 0 and ''μ''(''B''(''x'', ''r'')) ≤ ''r&amp;lt;sup&amp;gt;s&amp;lt;/sup&amp;gt;'' holds for some constant ''s'' &amp;gt; 0 and for every ball ''B''(''x'', ''r'') in ''X'', then dim&amp;lt;sub&amp;gt;Haus&amp;lt;/sub&amp;gt;(''X'') ≥ ''s''. A partial converse is provided by [[Frostman's lemma]].{{citation needed|date=March 2015}}&amp;lt;ref&amp;gt;This Wikipedia article also discusses further useful characterizations of the Hausdorff dimension.{{clarify|date=March 2015}}&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
If there is a measure μ defined on Borel subsets of a metric space X such that μ(X) &amp;gt; 0 and μ(B(x, r)) ≤ r&amp;lt;sup&amp;gt;s&amp;lt;/sup&amp;gt; holds for some constant s &amp;gt; 0 and for every ball B(x, r) in X, then dim&amp;lt;sub&amp;gt;Haus&amp;lt;/sub&amp;gt;(X) ≥ s. A partial converse is provided by Frostman's lemma.&lt;br /&gt;
&lt;br /&gt;
如果在度量空间 ''X'' 的 Borel 子集上定义一个测度 μ，使得''μ''(''X'') &amp;gt; 0 和''μ''(''B''(''x'', ''r'')) ≤ ''r&amp;lt;sup&amp;gt;s&amp;lt;/sup&amp;gt;''，对于某个常数 ''s'' &amp;gt; 0  和 ''X'' 中的每个球 ''B''(''x'', ''r'') 成立，则 dim&amp;lt;sub&amp;gt;Haus&amp;lt;/sub&amp;gt;(''X'') ≥ ''s'' 。 部分逆向转换由弗洛斯曼引理定义。&lt;br /&gt;
&lt;br /&gt;
=== Behaviour under unions and products ===&lt;br /&gt;
&lt;br /&gt;
If &amp;lt;math&amp;gt;X=\bigcup_{i\in I}X_i&amp;lt;/math&amp;gt; is a finite or countable union, then&lt;br /&gt;
&lt;br /&gt;
If &amp;lt;math&amp;gt;X=\bigcup_{i\in I}X_i&amp;lt;/math&amp;gt; is a finite or countable union, then&lt;br /&gt;
&lt;br /&gt;
如果 &amp;lt;math&amp;gt;X=\bigcup_{i\in I}X_i&amp;lt;/math&amp;gt; 是一个有限或可数的联合，则&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \dim_{\operatorname{Haus}}(X) =\sup_{i\in I} \dim_{\operatorname{Haus}}(X_i).&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \dim_{\operatorname{Haus}}(X) =\sup_{i\in I} \dim_{\operatorname{Haus}}(X_i).&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
This can be verified directly from the definition.&lt;br /&gt;
&lt;br /&gt;
This can be verified directly from the definition.&lt;br /&gt;
&lt;br /&gt;
这可以直接从定义得到验证。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
If ''X'' and ''Y'' are non-empty metric spaces, then the Hausdorff dimension of their product satisfies&amp;lt;ref&amp;gt;{{cite journal |author=Marstrand, J. M. |title=The dimension of Cartesian product sets |journal=Proc. Cambridge Philos. Soc. |volume=50 |issue=3 |pages=198–202 |year=1954 |doi=10.1017/S0305004100029236 |bibcode = 1954PCPS...50..198M }}&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
If X and Y are non-empty metric spaces, then the Hausdorff dimension of their product satisfies&lt;br /&gt;
&lt;br /&gt;
如果 ''X'' 和''Y''是非空度量空间，那么它们乘积的豪斯多夫维数满足&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt; \dim_{\operatorname{Haus}}(X\times Y)\ge \dim_{\operatorname{Haus}}(X)+ \dim_{\operatorname{Haus}}(Y).&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \dim_{\operatorname{Haus}}(X\times Y)\ge \dim_{\operatorname{Haus}}(X)+ \dim_{\operatorname{Haus}}(Y).&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
This inequality can be strict. It is possible to find two sets of dimension 0 whose product has dimension 1.&amp;lt;ref&amp;gt;{{cite book  | last = Falconer  | first = Kenneth J.  | title = Fractal geometry. Mathematical foundations and applications  | publisher = John Wiley &amp;amp; Sons, Inc., Hoboken, New Jersey  | year = 2003  | doi =   | isbn = }}&amp;lt;/ref&amp;gt; In the opposite direction, it is known that when ''X'' and ''Y'' are Borel subsets of '''R'''&amp;lt;sup&amp;gt;''n''&amp;lt;/sup&amp;gt;, the Hausdorff dimension of ''X'' × ''Y'' is bounded from above by the Hausdorff dimension of ''X'' plus the [[packing dimension|upper packing dimension]] of ''Y''. These facts are discussed in Mattila (1995).&lt;br /&gt;
&lt;br /&gt;
This inequality can be strict. It is possible to find two sets of dimension 0 whose product has dimension 1. In the opposite direction, it is known that when X and Y are Borel subsets of R&amp;lt;sup&amp;gt;n&amp;lt;/sup&amp;gt;, the Hausdorff dimension of X × Y is bounded from above by the Hausdorff dimension of X plus the upper packing dimension of Y. These facts are discussed in Mattila (1995).&lt;br /&gt;
&lt;br /&gt;
这种不平等可以是绝对的。有可能找到两个维数为0的集合，其乘积的维数为1。相反，我们知道当''X''和''Y''是 '''R'''&amp;lt;sup&amp;gt;''n''&amp;lt;/sup&amp;gt;的 Borel 子集时， ''X'' × ''Y''的豪斯多夫维数从上面以 ''X''的豪斯多夫维数加上 ''Y''的填充维数为界。Mattila (1995)曾就这些情况进行了讨论。&lt;br /&gt;
&lt;br /&gt;
==Self-similar sets自相似集合==&lt;br /&gt;
&lt;br /&gt;
{{refimprove section|date=March 2015}}&lt;br /&gt;
&lt;br /&gt;
Many sets defined by a self-similarity condition have dimensions which can be determined explicitly. Roughly, a set ''E'' is self-similar if it is the fixed point of a set-valued transformation ψ, that is ψ(''E'') = ''E'', although the exact definition is given below.&lt;br /&gt;
&lt;br /&gt;
Many sets defined by a self-similarity condition have dimensions which can be determined explicitly. Roughly, a set E is self-similar if it is the fixed point of a set-valued transformation ψ, that is ψ(E) = E, although the exact definition is given below.&lt;br /&gt;
&lt;br /&gt;
许多由自相似条件定义的集合具有可以显式确定的维数。粗略地说，集合''E'' 是自相似的，如果它是集值ψ变换的不动点，即ψ(''E'') = ''E''，尽管下面给出了确切的定义。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&amp;lt;blockquote&amp;gt;'''Theorem'''. Suppose&lt;br /&gt;
&lt;br /&gt;
&amp;lt;blockquote&amp;gt;Theorem. Suppose&lt;br /&gt;
&lt;br /&gt;
&amp;lt;blockquote&amp;gt;'''定理'''：假设&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt; \psi_i: \mathbf{R}^n \rightarrow \mathbf{R}^n, \quad i=1, \ldots , m &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \psi_i: \mathbf{R}^n \rightarrow \mathbf{R}^n, \quad i=1, \ldots , m &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
are [[Contraction mapping|contractive]] mappings on '''R'''&amp;lt;sup&amp;gt;''n''&amp;lt;/sup&amp;gt; with contraction constant ''r&amp;lt;sub&amp;gt;j&amp;lt;/sub&amp;gt;'' &amp;lt; 1. Then there is a unique ''non-empty'' compact set ''A'' such that&lt;br /&gt;
&lt;br /&gt;
are contractive mappings on R&amp;lt;sup&amp;gt;n&amp;lt;/sup&amp;gt; with contraction constant r&amp;lt;sub&amp;gt;j&amp;lt;/sub&amp;gt; &amp;lt; 1. Then there is a unique non-empty compact set A such that&lt;br /&gt;
&lt;br /&gt;
是'''R'''&amp;lt;sup&amp;gt;''n''&amp;lt;/sup&amp;gt;上的压缩常数''r&amp;lt;sub&amp;gt;j&amp;lt;/sub&amp;gt;'&amp;lt; 1的压缩映射。然后有一个唯一的非空紧集A &lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt; A = \bigcup_{i=1}^m \psi_i (A). &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; A = \bigcup_{i=1}^m \psi_i (A). &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&amp;lt;/blockquote&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;/blockquote&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The theorem follows from [[Stefan Banach]]'s [[Contractive mapping theorem|contractive mapping fixed point theorem]] applied to the complete metric space of non-empty compact subsets of '''R'''&amp;lt;sup&amp;gt;''n''&amp;lt;/sup&amp;gt; with the [[Hausdorff distance]].&amp;lt;ref&amp;gt;{{cite book |author=Falconer, K. J. |title=The Geometry of Fractal Sets |publisher=Cambridge University Press |location=Cambridge, UK |year=1985 |isbn=0-521-25694-1 |chapter=Theorem 8.3}}&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
The theorem follows from Stefan Banach's contractive mapping fixed point theorem applied to the complete metric space of non-empty compact subsets of R&amp;lt;sup&amp;gt;n&amp;lt;/sup&amp;gt; with the Hausdorff distance.&lt;br /&gt;
&lt;br /&gt;
这个定理来源于 Stefan Banach 的压缩映射不动点定理，该定理应用于 '''R'''&amp;lt;sup&amp;gt;''n''&amp;lt;/sup&amp;gt; 的非空紧子集的完备空间豪斯多夫距离。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
===The open set condition开集条件===&lt;br /&gt;
&lt;br /&gt;
To determine the dimension of the self-similar set ''A'' (in certain cases), we need a technical condition called the ''open set condition'' (OSC) on the sequence of contractions ψ&amp;lt;sub&amp;gt;''i''&amp;lt;/sub&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
To determine the dimension of the self-similar set A (in certain cases), we need a technical condition called the open set condition (OSC) on the sequence of contractions ψ&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
为了确定自相似集''A'' 的维数(在某些情况下) ，我们需要一个称为''开集条件''(OSC)的技术条件ψ&amp;lt;sub&amp;gt;''i''&amp;lt;/sub&amp;gt;。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
There is a relatively compact open set ''V'' such that&lt;br /&gt;
&lt;br /&gt;
There is a relatively compact open set V such that&lt;br /&gt;
&lt;br /&gt;
有一个相对紧的开集''V''&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt; \bigcup_{i=1}^m\psi_i (V) \subseteq V, &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \bigcup_{i=1}^m\psi_i (V) \subseteq V, &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
where the sets in union on the left are pairwise [[disjoint sets|disjoint]].&lt;br /&gt;
&lt;br /&gt;
where the sets in union on the left are pairwise disjoint.&lt;br /&gt;
&lt;br /&gt;
左边的集合是成对不相交的。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The open set condition is a separation condition that ensures the images ψ&amp;lt;sub&amp;gt;''i''&amp;lt;/sub&amp;gt;(''V'') do not overlap &amp;quot;too much&amp;quot;.&lt;br /&gt;
&lt;br /&gt;
The open set condition is a separation condition that ensures the images ψ&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;(V) do not overlap &amp;quot;too much&amp;quot;.&lt;br /&gt;
&lt;br /&gt;
开集条件是保证图像子ψ&amp;lt;sub&amp;gt;''i''&amp;lt;/sub&amp;gt;(''V'') 不重叠“太多”的分离条件。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
'''Theorem'''. Suppose the open set condition holds and each ψ&amp;lt;sub&amp;gt;''i''&amp;lt;/sub&amp;gt; is a similitude, that is a composition of an [[isometry]] and a [[dilation (metric space)|dilation]] around some point. Then the unique fixed point of ψ is a set whose Hausdorff dimension is ''s'' where ''s'' is the unique solution of&amp;lt;ref&amp;gt;{{cite journal | last=Hutchinson | first=John E. | title=Fractals and self similarity | journal=Indiana Univ. Math. J. | volume=30 | year=1981 | pages=713–747 | doi=10.1512/iumj.1981.30.30055 | issue=5 | doi-access=free }}&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
Theorem. Suppose the open set condition holds and each ψ&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt; is a similitude, that is a composition of an isometry and a dilation around some point. Then the unique fixed point of ψ is a set whose Hausdorff dimension is s where s is the unique solution of&lt;br /&gt;
&lt;br /&gt;
'''定理'''假设开集条件成立，并且每个ψ&amp;lt;sub&amp;gt;''i''&amp;lt;/sub&amp;gt; 是一个相似量，这是一个等距和围绕某一点的膨胀的合成。那么唯一的不动点是一个集合，它的豪斯多夫维数是 ''s'' ，其中  ''s'' 是 ''s'' &amp;lt;ref&amp;gt;{{cite journal | last=Hutchinson | first=John E. | title=Fractals and self similarity | journal=Indiana Univ. Math. J. | volume=30 | year=1981 | pages=713–747 | doi=10.1512/iumj.1981.30.30055 | issue=5 | doi-access=free }}&amp;lt;/ref&amp;gt;的唯一解&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt; \sum_{i=1}^m r_i^s = 1. &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \sum_{i=1}^m r_i^s = 1. &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The contraction coefficient of a similitude is the magnitude of the dilation.&lt;br /&gt;
&lt;br /&gt;
The contraction coefficient of a similitude is the magnitude of the dilation.&lt;br /&gt;
&lt;br /&gt;
相似物的收缩系数就是膨胀的大小。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
We can use this theorem to compute the Hausdorff dimension of the Sierpinski triangle (or sometimes called Sierpinski gasket). Consider three [[non-collinear points]] ''a''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;, ''a''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;, ''a''&amp;lt;sub&amp;gt;3&amp;lt;/sub&amp;gt; in the plane '''R'''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; and let ψ&amp;lt;sub&amp;gt;''i''&amp;lt;/sub&amp;gt; be the dilation of ratio 1/2 around ''a&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;''. The unique non-empty fixed point of the corresponding mapping ψ is a Sierpinski gasket and the dimension ''s'' is the unique solution of&lt;br /&gt;
&lt;br /&gt;
We can use this theorem to compute the Hausdorff dimension of the Sierpinski triangle (or sometimes called Sierpinski gasket). Consider three non-collinear points a&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;, a&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;, a&amp;lt;sub&amp;gt;3&amp;lt;/sub&amp;gt; in the plane R&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; and let ψ&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt; be the dilation of ratio 1/2 around a&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;. The unique non-empty fixed point of the corresponding mapping ψ is a Sierpinski gasket and the dimension s is the unique solution of&lt;br /&gt;
&lt;br /&gt;
我们可以使用这个定理来计算谢尔宾斯基三角形的豪斯多夫维数(或者有时候叫做谢尔宾斯基垫圈)。考虑R&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; 平面上的三个非共线点，''a''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;，''a''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;，''a''&amp;lt;sub&amp;gt;3&amp;lt;/sub&amp;gt;，让ψ&amp;lt;sub&amp;gt;''i''&amp;lt;/sub&amp;gt;是围绕着''a&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;''膨胀比率的1/2。对应映射的唯一非空不动点是一个谢尔宾斯基垫圈，其维数''s''是对应映射的唯一解&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt; \left(\frac{1}{2}\right)^s+\left(\frac{1}{2}\right)^s+\left(\frac{1}{2}\right)^s = 3 \left(\frac{1}{2}\right)^s =1. &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \left(\frac{1}{2}\right)^s+\left(\frac{1}{2}\right)^s+\left(\frac{1}{2}\right)^s = 3 \left(\frac{1}{2}\right)^s =1. &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Taking [[natural logarithm]]s of both sides of the above equation, we can solve for ''s'', that is: ''s'' = ln(3)/ln(2).  The Sierpinski gasket is self-similar and satisfies the OSC. In general a set ''E'' which is a fixed point of a mapping&lt;br /&gt;
&lt;br /&gt;
Taking natural logarithms of both sides of the above equation, we can solve for s, that is: s = ln(3)/ln(2).  The Sierpinski gasket is self-similar and satisfies the OSC. In general a set E which is a fixed point of a mapping&lt;br /&gt;
&lt;br /&gt;
取上述方程两边的自然对数，我们可以求出 ''s''，即: ''s'' = ln(3)/ln(2)。该密封垫具有自相似性，满足 OSC 要求。一般来说，集合 ''E''是一个映射的不动点&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt; A \mapsto \psi(A) = \bigcup_{i=1}^m \psi_i(A) &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt; A \mapsto \psi(A) = \bigcup_{i=1}^m \psi_i(A) &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
is self-similar if and only if the intersections&lt;br /&gt;
&lt;br /&gt;
is self-similar if and only if the intersections&lt;br /&gt;
&lt;br /&gt;
是自相似的，当且仅当&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt; H^s\left(\psi_i(E) \cap \psi_j(E)\right) =0, &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; H^s\left(\psi_i(E) \cap \psi_j(E)\right) =0, &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
where ''s'' is the Hausdorff dimension of ''E'' and ''H&amp;lt;sup&amp;gt;s&amp;lt;/sup&amp;gt;'' denotes [[Hausdorff measure]]. This is clear in the case of the Sierpinski gasket (the intersections are just points), but is also true more generally:&lt;br /&gt;
&lt;br /&gt;
where s is the Hausdorff dimension of E and H&amp;lt;sup&amp;gt;s&amp;lt;/sup&amp;gt; denotes Hausdorff measure. This is clear in the case of the Sierpinski gasket (the intersections are just points), but is also true more generally:&lt;br /&gt;
&lt;br /&gt;
其中 ''s''是''E''的豪斯多夫维数， ''E'' and ''H&amp;lt;sup&amp;gt;s&amp;lt;/sup&amp;gt;'' 表示 豪斯多夫测度。对于谢尔宾斯基垫圈(交叉点就是点)来说，这一点很明显，但更普遍的情况是:&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
'''Theorem'''. Under the same conditions as the previous theorem, the unique fixed point of ψ is self-similar.&lt;br /&gt;
&lt;br /&gt;
Theorem. Under the same conditions as the previous theorem, the unique fixed point of ψ is self-similar.&lt;br /&gt;
&lt;br /&gt;
'''定理'''：在与前一定理相同的条件下，其唯一不动点是自相似的。&lt;br /&gt;
&lt;br /&gt;
==See also参阅==&lt;br /&gt;
&lt;br /&gt;
* [[List of fractals by Hausdorff dimension豪斯多夫分形维数列表]] Examples of deterministic fractals, random and natural fractals.确定性分形与随机和自然分形的示例。&lt;br /&gt;
&lt;br /&gt;
* [[Assouad dimension  Assouad维数]], another variation of fractal dimension that, like Hausdorff dimension, is defined using coverings by balls其他被球覆盖方式定义的分形维数，例如豪斯多夫维数。&lt;br /&gt;
&lt;br /&gt;
* [[Intrinsic dimension固有维数]]&lt;br /&gt;
&lt;br /&gt;
* [[Packing dimension填充维数]]&lt;br /&gt;
&lt;br /&gt;
* [[Fractal dimension分形维数]]&lt;br /&gt;
&lt;br /&gt;
==References参考文献==&lt;br /&gt;
&lt;br /&gt;
{{reflist}}&lt;br /&gt;
&lt;br /&gt;
==Further reading拓展阅读==&lt;br /&gt;
&lt;br /&gt;
* {{cite book |last1=Dodson |first1=M. Maurice |title=Fractal Geometry and Applications: A Jubilee of Benoît Mandelbrot |volume=72 |issue=1 |pages=305–347 |last2=Kristensen |first2=Simon |chapter=Hausdorff Dimension and Diophantine Approximation |date=June 12, 2003 |arxiv=math/0305399 |bibcode = 2003math......5399D |doi=10.1090/pspum/072.1/2112110|series=Proceedings of Symposia in Pure Mathematics |isbn=9780821836378 }}&lt;br /&gt;
&lt;br /&gt;
* {{cite book |last1=Hurewicz |first1=Witold |authorlink1=Witold Hurewicz |last2=Wallman |first2=Henry |authorlink2=Henry Wallman |title=Dimension Theory |url=https://archive.org/details/in.ernet.dli.2015.84609 |publisher=Princeton University Press |year=1948 }}&lt;br /&gt;
&lt;br /&gt;
* {{cite journal |author作者=E. Szpilrajn |authorlink=Edward Marczewski |title=La dimension et la mesure |journal=Fundamenta Mathematicae |volume=28 |pages=81–9 |year=1937 }}&lt;br /&gt;
&lt;br /&gt;
* {{cite journal&lt;br /&gt;
&lt;br /&gt;
 | last1=Marstrand&lt;br /&gt;
&lt;br /&gt;
 | last1=Marstrand&lt;br /&gt;
&lt;br /&gt;
 | last1=马斯特兰德&lt;br /&gt;
&lt;br /&gt;
 | first1=J. M. | title=The dimension of cartesian product sets | year=1954 | journal=Proc. Cambridge Philos. Soc.&lt;br /&gt;
&lt;br /&gt;
 | first1=J. M. | title=The dimension of cartesian product sets | year=1954 | journal=Proc. Cambridge Philos. Soc.&lt;br /&gt;
&lt;br /&gt;
 | first1= J. M. | title=笛卡儿积集的维数 | 1954年 |  journal=Proc. Cambridge Philos. Soc.&lt;br /&gt;
&lt;br /&gt;
 | volume=50&lt;br /&gt;
&lt;br /&gt;
 | volume=50&lt;br /&gt;
&lt;br /&gt;
 | 第50卷&lt;br /&gt;
&lt;br /&gt;
 | issue=3&lt;br /&gt;
&lt;br /&gt;
 | issue=3&lt;br /&gt;
&lt;br /&gt;
 | 第三期&lt;br /&gt;
&lt;br /&gt;
 | pages=198–202&lt;br /&gt;
&lt;br /&gt;
 | pages=198–202&lt;br /&gt;
&lt;br /&gt;
 | 第198-202页&lt;br /&gt;
&lt;br /&gt;
 | doi=10.1017/S0305004100029236|bibcode = 1954PCPS...50..198M }}&lt;br /&gt;
&lt;br /&gt;
 | doi=10.1017/S0305004100029236|bibcode = 1954PCPS...50..198M }}&lt;br /&gt;
&lt;br /&gt;
10.1017 / S0305004100029236 | bibcode 1954PCPS... 50. . 198 m }&lt;br /&gt;
&lt;br /&gt;
* {{Cite book&lt;br /&gt;
&lt;br /&gt;
 | last1=Mattila&lt;br /&gt;
&lt;br /&gt;
 | last1=Mattila&lt;br /&gt;
&lt;br /&gt;
 | last1=Mattila&lt;br /&gt;
&lt;br /&gt;
 | first1=Pertti | author1-link=Pertti Mattila| title=Geometry of sets and measures in Euclidean spaces | publisher=[[Cambridge University Press]]&lt;br /&gt;
&lt;br /&gt;
 | first1=Pertti | author1-link=Pertti Mattila| title=Geometry of sets and measures in Euclidean spaces | publisher=Cambridge University Press&lt;br /&gt;
&lt;br /&gt;
| first1 Pertti | author1-link Pertti Mattila | title 欧几里德空间中集合和度量的几何 | 出版商剑桥大学出版社&lt;br /&gt;
&lt;br /&gt;
 | isbn=978-0-521-65595-8 | year=1995}}&lt;br /&gt;
&lt;br /&gt;
 | isbn=978-0-521-65595-8 | year=1995}}&lt;br /&gt;
&lt;br /&gt;
| isbn 978-0-521-65595-8 | year 1995}&lt;br /&gt;
&lt;br /&gt;
* {{cite journal |author=A. S. Besicovitch |authorlink=A. S. Besicovitch |title=On Linear Sets of Points of Fractional Dimensions |journal=[[Mathematische Annalen]] |volume=101 |year=1929 | doi=10.1007/BF01454831| issue=1 |pages= 161–193}}&lt;br /&gt;
&lt;br /&gt;
* {{cite journal |author1=A. S. Besicovitch |authorlink1=A. S. Besicovitch |author2=H. D. Ursell |authorlink2=H. D. Ursell |title=Sets of Fractional Dimensions |journal=Journal of the London Mathematical Society |volume=12 |year=1937 | issue=1 | doi=10.1112/jlms/s1-12.45.18  | pages=18–25 }}&amp;lt;br/&amp;gt;Several selections from this volume are reprinted in {{cite book |author=Edgar, Gerald A. |title=Classics on fractals |publisher=Addison-Wesley |location=Boston |year=1993 |isbn=0-201-58701-7}} See chapters 9,10,11&lt;br /&gt;
&lt;br /&gt;
* {{cite journal |author=F. Hausdorff |authorlink=F. Hausdorff |title=Dimension und äußeres Maß |journal=Mathematische Annalen |volume=79 |issue=1–2 |pages=157–179 |date=March 1919 |doi=10.1007/BF01457179|hdl=10338.dmlcz/100363 |url=http://dml.cz/bitstream/handle/10338.dmlcz/100363/CzechMathJ_09-1959-3_5.pdf }}&lt;br /&gt;
&lt;br /&gt;
* {{cite journal | last=Hutchinson | first=John E. | title=Fractals and self similarity | journal=Indiana Univ. Math. J. | volume=30 | year=1981 | pages=713–747 | doi=10.1512/iumj.1981.30.30055 | issue=5 | doi-access=free }}&lt;br /&gt;
&lt;br /&gt;
*{{cite book | last=Falconer | first = Kenneth |title=Fractal Geometry: Mathematical Foundations and Applications | publisher=[[John Wiley and Sons]] | edition=2nd | year=2003}}&lt;br /&gt;
&lt;br /&gt;
==External links外部链接==&lt;br /&gt;
&lt;br /&gt;
* [https://www.encyclopediaofmath.org/index.php/Hausdorff_dimension Hausdorff dimension] 在 [https://www.encyclopediaofmath.org/ Encyclopedia of Mathematics]&lt;br /&gt;
&lt;br /&gt;
* [https://www.encyclopediaofmath.org/index.php/Hausdorff_measure Hausdorff measure] 在 [https://www.encyclopediaofmath.org/ Encyclopedia of Mathematics]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{{DEFAULTSORT:Hausdorff Dimension豪斯多夫维数}}&lt;br /&gt;
&lt;br /&gt;
[[Category分类:Fractals分形]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[Category分类:Metric geometry度量几何]]&lt;br /&gt;
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&lt;br /&gt;
&lt;br /&gt;
[[Category分类:Dimension theory维度理论]]&lt;br /&gt;
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&lt;br /&gt;
&amp;lt;noinclude&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;small&amp;gt;This page was moved from [[wikipedia:en:Hausdorff dimension]]. Its edit history can be viewed at [[分形维数/edithistory]]&amp;lt;/small&amp;gt;&amp;lt;/noinclude&amp;gt;&lt;br /&gt;
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[[Category:待整理页面]]&lt;/div&gt;</summary>
		<author><name>Ruili</name></author>
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		<title>分形维数</title>
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		<updated>2020-10-27T13:45:29Z</updated>

		<summary type="html">&lt;p&gt;Ruili：&lt;/p&gt;
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&lt;div&gt;此词条暂由彩云小译翻译，未经人工整理和审校，带来阅读不便，请见谅。&lt;br /&gt;
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[[File:KochFlake.svg|thumb|280px|Example of non-integer dimensions. The first four [[iteration]]s of the [[Koch snowflake|Koch curve]], where after each iteration, all original line segments are replaced with four, each a self-similar copy that is 1/3 the length of the original. One formalism of the Hausdorff dimension uses this scale factor (3) and the number of self-similar objects (4) to calculate the dimension, D, after the first iteration to be D = (log N)/(log S) = (log 4)/(log 3) ≈ 1.26.&amp;lt;ref name=CampbellAnnenberg15&amp;gt;MacGregor Campbell, 2013, &amp;quot;5.6 Scaling and the Hausdorff Dimension,&amp;quot; at ''Annenberg Learner:MATHematics illuminated'', see [http://www.learner.org/courses/mathilluminated/units/5/textbook/06.php], accessed 5 March 2015.&amp;lt;/ref&amp;gt; That is, while the Hausdorff dimension of a single [[point (geometry)|point]] is zero, of a [[line segment]] is 1, of a [[square]] is 2, and of a [[cube]] is 3, for [[fractal]]s such as this, the object can have a non-integer dimension.]]&lt;br /&gt;
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Example of non-integer dimensions. The first four [[iterations of the Koch curve, where after each iteration, all original line segments are replaced with four, each a self-similar copy that is 1/3 the length of the original. One formalism of the Hausdorff dimension uses this scale factor (3) and the number of self-similar objects (4) to calculate the dimension, D, after the first iteration to be D = (log N)/(log S) = (log 4)/(log 3) ≈ 1.26. That is, while the Hausdorff dimension of a single point is zero, of a line segment is 1, of a square is 2, and of a cube is 3, for fractals such as this, the object can have a non-integer dimension.]]&lt;br /&gt;
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[[File:KochFlake.svg|thumb|280px|非整数维度示例：前四个[[Koch 曲线]]的迭代，在每次迭代后，所有原始线段都被替换为四个，每个自相似的复制是原始线段长度的1 / 3。豪斯多夫维数的一个建模是使用这个比例因子(3)和自相似物体的数量(4)来计算维度，设在第一次迭代后为 D = (log N)/(log S) = (log 4)/(log 3) ≈ 1.26.&amp;lt;ref name=CampbellAnnenberg15&amp;gt;。MacGregor Campbell, 2013, &amp;quot;5.6 Scaling and the Hausdorff Dimension,&amp;quot; 在 ''Annenberg Learner:MATHematics illuminated'', 参见 [http://www.learner.org/courses/mathilluminated/units/5/textbook/06.php], accessed 5 March 2015.&amp;lt;/ref&amp;gt; 也就是说，当一个点的豪斯多夫维数为零，线段为1，正方形为2，立方体为3时，对于像这样的分形，物体可以有一个非整数维度。]]&lt;br /&gt;
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In [[mathematics]], '''Hausdorff dimension''' is a measure of ''roughness'', or more specifically, [[fractal dimension]], that was first introduced in 1918 by [[mathematician]] [[Felix Hausdorff]].&amp;lt;ref&amp;gt;{{Cite journal |arxiv = 1101.1444|doi = 10.1214/11-STS370|title = Estimators of Fractal Dimension: Assessing the Roughness of Time Series and Spatial Data|journal = Statistical Science|volume = 27|issue = 2|pages = 247–277|year = 2012|last1 = Gneiting|first1 = Tilmann|last2 = Ševčíková|first2 = Hana|last3 = Percival|first3 = Donald B.}}&amp;lt;/ref&amp;gt; For instance, the Hausdorff dimension of a single [[point (geometry)|point]] is zero, of a [[line segment]] is 1, of a [[square]] is 2, and of a [[cube]] is 3. That is, for sets of points that define a smooth shape or a shape that has a small number of corners—the shapes of traditional geometry and science—the Hausdorff dimension is an [[integer]] agreeing with the usual sense of dimension, also known as the [[Inductive dimension|topological dimension]]. However, formulas have also been developed that allow calculation of the dimension of other less simple objects, where, solely on the basis of their properties of [[scaling (geometry)|scaling]] and [[self-similarity]], one is led to the conclusion that particular objects—including [[fractal]]s—have non-integer Hausdorff dimensions. Because of the significant technical advances made by [[Abram Samoilovitch Besicovitch]] allowing computation of dimensions for highly irregular or &amp;quot;rough&amp;quot; sets, this dimension is also commonly referred to as the ''Hausdorff–Besicovitch dimension.''&lt;br /&gt;
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In mathematics, Hausdorff dimension is a measure of roughness, or more specifically, fractal dimension, that was first introduced in 1918 by mathematician Felix Hausdorff. For instance, the Hausdorff dimension of a single point is zero, of a line segment is 1, of a square is 2, and of a cube is 3. That is, for sets of points that define a smooth shape or a shape that has a small number of corners—the shapes of traditional geometry and science—the Hausdorff dimension is an integer agreeing with the usual sense of dimension, also known as the topological dimension. However, formulas have also been developed that allow calculation of the dimension of other less simple objects, where, solely on the basis of their properties of scaling and self-similarity, one is led to the conclusion that particular objects—including fractals—have non-integer Hausdorff dimensions. Because of the significant technical advances made by Abram Samoilovitch Besicovitch allowing computation of dimensions for highly irregular or &amp;quot;rough&amp;quot; sets, this dimension is also commonly referred to as the Hausdorff–Besicovitch dimension.&lt;br /&gt;
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在[[数学]]中，'''&amp;lt;font color = '#ff8000'&amp;gt;豪斯多夫维数Hausdorff dimension&amp;lt;/font&amp;gt;'''是一种粗糙度的度量单位，或者更确切地说，分形维数，是由数学家 Felix Hausdorff 在1918年首次提出的。例如，单点的豪斯多夫维数为零，线段为1，正方形为2，立方体为3。也就是说，对于定义了一个光滑形状或一个有少数几个角的形状---- 传统几何学和科学的形状---- 的点集来说，豪斯多夫维数是一个整数，符合通常的维度意义，也称为拓扑维度。然而，还有一些公式允许计算其他不太简单的对象的维数，其中仅仅根据它们的标度和自相似特性，就可以得出结论: 特定的对象ー包括分形ー具有非整数的 Hausdorff 维数。由于阿布拉姆·萨莫伊洛维奇·贝西科维奇的重大技术进步，允许计算高度不规则或“粗糙”集的维度，这个维度通常也被称为 Hausdorff-Besicovitch 维度。 &lt;br /&gt;
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The Hausdorff dimension, more specifically, is a further dimensional number associated with a given set, where the distances between all members of that set are defined. Such a set is termed a [[metric space]]. The dimension is drawn from the [[Extended real number line|extended real numbers]], &amp;lt;math&amp;gt;\overline{\mathbb{R}}&amp;lt;/math&amp;gt;, as opposed to the more intuitive notion of dimension, which is not associated to general metric spaces, and only takes values in the non-negative integers.&lt;br /&gt;
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The Hausdorff dimension, more specifically, is a further dimensional number associated with a given set, where the distances between all members of that set are defined. Such a set is termed a metric space. The dimension is drawn from the extended real numbers, &amp;lt;math&amp;gt;\overline{\mathbb{R}}&amp;lt;/math&amp;gt;, as opposed to the more intuitive notion of dimension, which is not associated to general metric spaces, and only takes values in the non-negative integers.&lt;br /&gt;
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更具体地说，豪斯多夫维数是一个与给定集合相关联的更进一步的维数，其中定义了该集合所有成员之间的距离。这样的集合称为度量空间。维数是从扩展的实数，&amp;lt;math&amp;gt;\overline{\mathbb{R}}&amp;lt;/math&amp;gt;，而不是更直观的维数概念(它不与一般的度量空间相关联，只接受非负整数的值)。&lt;br /&gt;
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In mathematical terms, the Hausdorff dimension generalizes the notion of the dimension of a real [[vector space]]. That is, the Hausdorff dimension of an ''n''-dimensional [[inner product space]] equals ''n''. This underlies the earlier statement that the Hausdorff dimension of a point is zero, of a line is one, etc., and that [[fractal|irregular sets]] can have noninteger Hausdorff dimensions. For instance, the [[Koch snowflake]] shown at right is constructed from an equilateral triangle; in each iteration, its component line segments are divided into 3 segments of unit length, the newly created middle segment is used as the base of a new [[equilateral]] triangle that points outward, and this base segment is then deleted to leave a final object from the iteration of unit length of 4.&amp;lt;ref&amp;gt;Larry Riddle, 2014, &amp;quot;Classic Iterated Function Systems: Koch Snowflake&amp;quot;, Agnes Scott College e-Academy (online), see [http://ecademy.agnesscott.edu/~lriddle/ifs/ksnow/ksnow.htm], accessed 5 March 2015.&amp;lt;/ref&amp;gt; That is, after the first iteration, each original line segment has been replaced with N=4, where each self-similar copy is 1/S = 1/3 as long as the original.&amp;lt;ref name=CampbellAnnenberg15/&amp;gt; Stated another way, we have taken an object with Euclidean dimension, D, and reduced its linear scale by 1/3 in each direction, so that its length increases to N=S&amp;lt;sup&amp;gt;D&amp;lt;/sup&amp;gt;.&amp;lt;ref name=ClaytonSCTPLS96&amp;gt;Keith Clayton, 1996, &amp;quot;Fractals and the Fractal Dimension,&amp;quot; ''Basic Concepts in Nonlinear Dynamics and Chaos'' (workshop), Society for Chaos Theory in Psychology and the Life Sciences annual meeting, June 28, 1996, Berkeley, California, see [http://www.vanderbilt.edu/AnS/psychology/cogsci/chaos/workshop/Workshop.html], accessed 5 March 2015.&amp;lt;/ref&amp;gt; This equation is easily solved for D, yielding the ratio of logarithms (or [[natural logarithm]]s) appearing in the figures, and giving—in the Koch and other fractal cases—non-integer dimensions for these objects.&lt;br /&gt;
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In mathematical terms, the Hausdorff dimension generalizes the notion of the dimension of a real vector space. That is, the Hausdorff dimension of an n-dimensional inner product space equals n. This underlies the earlier statement that the Hausdorff dimension of a point is zero, of a line is one, etc., and that irregular sets can have noninteger Hausdorff dimensions. For instance, the Koch snowflake shown at right is constructed from an equilateral triangle; in each iteration, its component line segments are divided into 3 segments of unit length, the newly created middle segment is used as the base of a new equilateral triangle that points outward, and this base segment is then deleted to leave a final object from the iteration of unit length of 4. That is, after the first iteration, each original line segment has been replaced with N=4, where each self-similar copy is 1/S = 1/3 as long as the original. This equation is easily solved for D, yielding the ratio of logarithms (or natural logarithms) appearing in the figures, and giving—in the Koch and other fractal cases—non-integer dimensions for these objects.&lt;br /&gt;
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用数学术语来说，豪斯多夫维数概括了实向量空间维数的概念。也就是说，n 维内积空间的豪斯多夫维数等于 n。 这就是早期假设的基础，一个点的豪斯多夫维数是零，一条线是一等等，不规则集可以有非整数的豪斯多夫维数。例如，右边所示的 Koch 雪花是由一个正三角形构成的; 在每次迭代中，它的组成线段被分成单位长度的3段，新创建的中间线段被用作一个指向外部的新正三角形的基础，然后人们删除这个基础线段用来保留单位长度4的迭代中的最终对象。也就是说，在第一次迭代之后，每个原始线段都被替换为 N=4，其中每个自相似拷贝的长度是原始线段的1/S = 1/3 。这个方程很容易求解为 D，产生出现在图形中的对数(或自然对数)的比率，并给出——在 Koch 和其他分形情况下——这些对象的非整数维数。&lt;br /&gt;
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The Hausdorff dimension is a successor to the simpler, but usually equivalent, box-counting or [[Minkowski–Bouligand dimension]].&lt;br /&gt;
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The Hausdorff dimension is a successor to the simpler, but usually equivalent, box-counting or Minkowski–Bouligand dimension.&lt;br /&gt;
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豪斯多夫维数是更简单但通常等价的'''&amp;lt;font color = '#ff8000'&amp;gt;计盒维数box-counting&amp;lt;/font&amp;gt;'''或'''&amp;lt;font color = '#ff8000'&amp;gt;闵可夫斯基维数Minkowski-Bouligand&amp;lt;/font&amp;gt;'''的继承者。&lt;br /&gt;
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==Intuition概念==&lt;br /&gt;
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The intuitive concept of dimension of a geometric object ''X'' is the number of independent parameters one needs to pick out a unique point inside. However, any point specified by two parameters can be instead specified by one, because the [[cardinality]] of the [[real plane]] is equal to the cardinality of the [[real line]] (this can be seen by an [[Cantor's diagonal argument|argument]] involving interweaving the digits of two numbers to yield a single number encoding the same information). The example of a [[space-filling curve]] shows that one can even map the real line to the real plane [[Surjective function|surjectively]] (taking one real number into a pair of real numbers in a way so that all pairs of numbers are covered) and ''continuously'', so that a one-dimensional object completely fills up a higher-dimensional object.&lt;br /&gt;
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The intuitive concept of dimension of a geometric object X is the number of independent parameters one needs to pick out a unique point inside. However, any point specified by two parameters can be instead specified by one, because the cardinality of the real plane is equal to the cardinality of the real line (this can be seen by an argument involving interweaving the digits of two numbers to yield a single number encoding the same information). The example of a space-filling curve shows that one can even map the real line to the real plane surjectively (taking one real number into a pair of real numbers in a way so that all pairs of numbers are covered) and continuously, so that a one-dimensional object completely fills up a higher-dimensional object.&lt;br /&gt;
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几何物体X的直观尺寸概念就是一个物体需要多少个独立参数才能找到一个独特的点。但是，任何由两个参数指定的点都可以由一个参数指定，因为实际平面的基数等于实际行的基数(这可以通过一个参数看到，该参数涉及交织两个数字的数字以产生一个编码相同信息的单个数字)。'''&amp;lt;font color = '#ff8000'&amp;gt;皮亚诺曲线&amp;lt;/font&amp;gt;'''的例子表明，一个人甚至可以完美和连续地映射实际线到真正的平面(把一个实数转换成一对实数，这样所有的数对都被覆盖)，由此一维物体完全填充了一个高维物体。&lt;br /&gt;
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Every space filling curve hits some points multiple times, and does not have a continuous inverse. It is impossible to map two dimensions onto one in a way that is continuous and continuously invertible. The topological dimension, also called [[Lebesgue covering dimension]], explains why. This dimension is ''n'' if, in every covering of ''X'' by small open balls, there is at least one point where ''n''&amp;amp;nbsp;+&amp;amp;nbsp;1 balls overlap. For example, when one covers a line with short open intervals, some points must be covered twice, giving dimension&amp;amp;nbsp;''n''&amp;amp;nbsp;=&amp;amp;nbsp;1.&lt;br /&gt;
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Every space filling curve hits some points multiple times, and does not have a continuous inverse. It is impossible to map two dimensions onto one in a way that is continuous and continuously invertible. The topological dimension, also called Lebesgue covering dimension, explains why. This dimension is n if, in every covering of X by small open balls, there is at least one point where n&amp;amp;nbsp;+&amp;amp;nbsp;1 balls overlap. For example, when one covers a line with short open intervals, some points must be covered twice, giving dimension&amp;amp;nbsp;n&amp;amp;nbsp;=&amp;amp;nbsp;1.&lt;br /&gt;
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每条空间填充曲线都会多次撞击某些点，且不存在连续的倒数。将两个维度以连续和连续可逆的方式映射到一个维度是不可能的。'''&amp;lt;font color = '#ff8000'&amp;gt;拓扑维度 topological dimension&amp;lt;/font&amp;gt;'''，也被称为拓朴维数，解释了为什么。这个维度是 n，如果在 x 的每个小开球覆盖中，至少有一个点 n + 1个球重叠。例如，当一个点覆盖一条具有短开区间的直线时，某些点必须被覆盖两次，给出维数''n''&amp;amp;nbsp;=&amp;amp;nbsp;1。&lt;br /&gt;
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But topological dimension is a very crude measure of the local size of a space (size near a point). A curve that is almost space-filling can still have topological dimension one, even if it fills up most of the area of a region. A [[fractal]] has an integer topological dimension, but in terms of the amount of space it takes up, it behaves like a higher-dimensional space.&lt;br /&gt;
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But topological dimension is a very crude measure of the local size of a space (size near a point). A curve that is almost space-filling can still have topological dimension one, even if it fills up most of the area of a region. A fractal has an integer topological dimension, but in terms of the amount of space it takes up, it behaves like a higher-dimensional space.&lt;br /&gt;
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但是，拓扑维度是对空间局部尺寸(点附近的尺寸)的一个非常粗略的度量。一条几乎是空间填充的曲线仍然可以有一维拓扑，即使它填充了一个区域的大部分面积。分形具有整数的拓扑维数，但就其所占空间的数量而言，它看起来像一个更高维的空间。&lt;br /&gt;
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The Hausdorff dimension measures the local size of a space taking into account the distance between points, the [[metric space|metric]]. Consider the number ''N''(''r'') of [[ball (mathematics)|balls]] of radius at most ''r'' required to cover ''X'' completely. When ''r'' is very small, ''N''(''r'') grows polynomially with 1/''r''. For a sufficiently well-behaved  ''X'', the Hausdorff dimension is the unique number ''d'' such that N(''r'') grows as 1/''r&amp;lt;sup&amp;gt;d&amp;lt;/sup&amp;gt;'' as ''r'' approaches zero. More precisely, this defines the [[Minkowski–Bouligand dimension|box-counting dimension]], which equals the Hausdorff dimension when the value ''d'' is a critical boundary between growth rates that are insufficient to cover the space, and growth rates that are overabundant.&lt;br /&gt;
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The Hausdorff dimension measures the local size of a space taking into account the distance between points, the metric. Consider the number N(r) of balls of radius at most r required to cover X completely. When r is very small, N(r) grows polynomially with 1/r. For a sufficiently well-behaved  X, the Hausdorff dimension is the unique number d such that N(r) grows as 1/r&amp;lt;sup&amp;gt;d&amp;lt;/sup&amp;gt; as r approaches zero. More precisely, this defines the box-counting dimension, which equals the Hausdorff dimension when the value d is a critical boundary between growth rates that are insufficient to cover the space, and growth rates that are overabundant.&lt;br /&gt;
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豪斯多夫维数测量一个空间的局部大小时，会考虑到点之间距离的度量。考虑半径最大为 r 的球数 ''N'' (r) ，需要完全覆盖 ''X''。当 r 很小时，n (r)以1/''r'' 增长多项式。对于一个表现足够好的 ''X''，豪斯多夫维数是唯一的数 d，这样当 r 趋近于零时， N(r)增长为1/r&amp;lt;sup&amp;gt;d&amp;lt;/sup&amp;gt; 。更确切地说，这定义了盒子计数维度，当值 d 是不足以覆盖空间的增长率和过度充裕的增长率之间的关键边界时，它等于豪斯多夫维数。&lt;br /&gt;
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For shapes that are smooth, or shapes with a small number of corners, the shapes of traditional geometry and science, the Hausdorff dimension is an integer agreeing with the topological dimension. But [[Benoit Mandelbrot]] observed that [[fractal]]s, sets with noninteger Hausdorff dimensions, are found everywhere in nature. He observed that the proper idealization of most rough shapes you see around you is not in terms of smooth idealized shapes, but in terms of fractal idealized shapes:&lt;br /&gt;
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For shapes that are smooth, or shapes with a small number of corners, the shapes of traditional geometry and science, the Hausdorff dimension is an integer agreeing with the topological dimension. But Benoit Mandelbrot observed that fractals, sets with noninteger Hausdorff dimensions, are found everywhere in nature. He observed that the proper idealization of most rough shapes you see around you is not in terms of smooth idealized shapes, but in terms of fractal idealized shapes:&lt;br /&gt;
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对于光滑的形状，或者有少量棱角的形状，传统几何和科学的形状，豪斯多夫维数是一个整数，与拓扑维度一致。但是伯努·曼德布洛特观察到分形---- 具有非整数豪斯多夫维数的集合---- 在自然界中随处可见。他观察到，我们周围大多数粗糙形状的理想化不是光滑的理想化形状，而是分形理想化形状:&lt;br /&gt;
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&amp;lt;blockquote&amp;gt;Clouds are not spheres, mountains are not cones, coastlines are not circles, and bark is not smooth, nor does lightning travel in a straight line.&amp;lt;ref name=&amp;quot;mandelbrot&amp;quot;&amp;gt;{{cite book   | last = Mandelbrot   | first = Benoît   | authorlink = Benoit Mandelbrot   | title = The Fractal Geometry of Nature   | publisher = W. H. Freeman   | series = Lecture notes in mathematics 1358   | year = 1982   | doi =    | isbn = 0-7167-1186-9   | url-access = registration   | url = https://archive.org/details/fractalgeometryo00beno   }}&amp;lt;/ref&amp;gt;&amp;lt;/blockquote&amp;gt;&lt;br /&gt;
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&amp;lt;blockquote&amp;gt;Clouds are not spheres, mountains are not cones, coastlines are not circles, and bark is not smooth, nor does lightning travel in a straight line.&amp;lt;/blockquote&amp;gt;&lt;br /&gt;
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&amp;lt;blockquote&amp;gt;云不是球体，山不是锥体，海岸线不是圆圈，树皮不平滑，闪电也不是直线运动。 &amp;lt;/blockquote&amp;gt;&lt;br /&gt;
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For fractals that occur in nature, the Hausdorff and [[Minkowski–Bouligand dimension|box-counting dimension]] coincide. The [[packing dimension]] is yet another similar notion which gives the same value for many shapes, but there are well documented exceptions where all these dimensions differ.&lt;br /&gt;
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For fractals that occur in nature, the Hausdorff and box-counting dimension coincide. The packing dimension is yet another similar notion which gives the same value for many shapes, but there are well documented exceptions where all these dimensions differ.&lt;br /&gt;
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对于自然界中出现的分形，豪斯多夫维数和盒计数维数是一致的。封装尺寸是另一个类似的概念，它给出了许多形状相同的值，但是在所有这些尺寸不同的情况，都做了很好的说明。&lt;br /&gt;
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==Formal definitions形式化定义==&lt;br /&gt;
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===Hausdorff content豪斯多夫集===&lt;br /&gt;
&lt;br /&gt;
Let ''X'' be a [[metric space]]. If ''S'' ⊂ ''X'' and ''d'' ∈ [0, ∞), the ''d''-dimensional '''unlimited Hausdorff content''' of ''S'' is defined by&lt;br /&gt;
&lt;br /&gt;
Let X be a metric space. If S ⊂ X and d ∈ [0, ∞), the d-dimensional unlimited Hausdorff content of S is defined by&lt;br /&gt;
&lt;br /&gt;
设 ''X''是度量空间。若''S'' ⊂ ''X'' 和 ''d'' ∈ [0, ∞) ，则 ''S'' 的''d''维无限 豪斯多夫集定义为&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt;C_H^d(S):=\inf\Bigl\{\sum_i r_i^d:\text{ there is a cover of } S\text{ by balls with radii }r_i&amp;gt;0\Bigr\}.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt;C_H^d(S):=\inf\Bigl\{\sum_i r_i^d:\text{ there is a cover of } S\text{ by balls with radii }r_i&amp;gt;0\Bigr\}.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt;C_H^d(S):=\inf\Bigl\{\sum_i r_i^d:\text{ there is a cover of } S\text{ by balls with radii }r_i&amp;gt;0\Bigr\}.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
In other words, &amp;lt;math&amp;gt;C_H^d(S)&amp;lt;/math&amp;gt; is the [[infimum]] of the set of numbers &amp;lt;math&amp;gt;\delta \geq 0&amp;lt;/math&amp;gt; such that there is some (indexed) collection of [[ball (mathematics)|ball]]s &amp;lt;math&amp;gt;\{B(x_i,r_i):i\in I\}&amp;lt;/math&amp;gt; covering ''S'' with ''r&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;''&amp;amp;nbsp;&amp;gt;&amp;amp;nbsp;0 for each ''i''&amp;amp;nbsp;∈&amp;amp;nbsp;''I'' that satisfies &amp;lt;math&amp;gt;\sum_{i\in I} r_i^d&amp;lt;\delta &amp;lt;/math&amp;gt;. (Here, we use the standard convention that [[infimum|inf&amp;amp;nbsp;Ø&amp;amp;nbsp;=&amp;amp;nbsp;∞]].)&lt;br /&gt;
&lt;br /&gt;
In other words, &amp;lt;math&amp;gt;C_H^d(S)&amp;lt;/math&amp;gt; is the infimum of the set of numbers &amp;lt;math&amp;gt;\delta \geq 0&amp;lt;/math&amp;gt; such that there is some (indexed) collection of balls &amp;lt;math&amp;gt;\{B(x_i,r_i):i\in I\}&amp;lt;/math&amp;gt; covering S with r&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;&amp;amp;nbsp;&amp;gt;&amp;amp;nbsp;0 for each i&amp;amp;nbsp;∈&amp;amp;nbsp;I that satisfies &amp;lt;math&amp;gt;\sum_{i\in I} r_i^d&amp;lt;\delta &amp;lt;/math&amp;gt;. (Here, we use the standard convention that inf&amp;amp;nbsp;Ø&amp;amp;nbsp;=&amp;amp;nbsp;∞.)&lt;br /&gt;
&lt;br /&gt;
换句话说，&amp;lt;math&amp;gt;C_H^d(S)&amp;lt;/math&amp;gt; 是数字集合&amp;lt;math&amp;gt;\delta \geq 0&amp;lt;/math&amp;gt;的下确界，使得在 ''i''&amp;amp;nbsp;∈&amp;amp;nbsp中存在一些球集合 &amp;lt;math&amp;gt;\{B(x_i,r_i):i\in I\}&amp;lt;/math&amp;gt;  i 包含 s，对于每个 ''r&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;''&amp;amp;nbsp;&amp;gt;&amp;amp;nbsp;0 满足 i 中的和&amp;lt;math&amp;gt;\sum_{i\in I} r_i^d&amp;lt;\delta &amp;lt;/math&amp;gt; (在这里，我们使用inf&amp;amp;nbsp;Ø&amp;amp;nbsp;=&amp;amp;nbsp;∞ )的标准约定。&lt;br /&gt;
&lt;br /&gt;
===Hausdorff measurement豪斯多夫分形测量===&lt;br /&gt;
&lt;br /&gt;
The Hausdorff outer measure is different from the unbounded Hausdorf content in that rather than considering all possible coverings of ''S'', we see what happens when the sizes of the balls go to zero. This is  for &amp;lt;math&amp;gt;d \geq 0 &amp;lt;/math&amp;gt;, we define the ''d''-dimensional Hausdorff outer measure of ''S'' as&lt;br /&gt;
&lt;br /&gt;
The Hausdorff outer measure is different from the unbounded Hausdorf content in that rather than considering all possible coverings of S, we see what happens when the sizes of the balls go to zero. This is  for &amp;lt;math&amp;gt;d \geq 0 &amp;lt;/math&amp;gt;, we define the d-dimensional Hausdorff outer measure of S as&lt;br /&gt;
&lt;br /&gt;
豪斯多夫外测度不同于无界的豪斯多夫，因为我们不考虑 s 的所有可能，我们看到当球的大小为零时会发生什么。这是为了数学  &amp;lt;math&amp;gt;d \geq 0 &amp;lt;/math&amp;gt;，我们定义了  ''S''的 ''d''维豪斯多夫Hausdorff 外测度为&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt; \mathcal{H}^d(S):=\lim_{r \to 0} \inf\Bigl\{\sum_i r_i^d:\text{ there is a cover of } S\text{ by balls with radii } 0 &amp;lt; r_i &amp;lt; r\Bigr\}.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \mathcal{H}^d(S):=\lim_{r \to 0} \inf\Bigl\{\sum_i r_i^d:\text{ there is a cover of } S\text{ by balls with radii } 0 &amp;lt; r_i &amp;lt; r\Bigr\}.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \mathcal{H}^d(S):=\lim_{r \to 0} \inf\Bigl\{\sum_i r_i^d:\text{有一个面} S\text{ 球 } 0 &amp;lt; r_i &amp;lt; r\Bigr\}.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
===Hausdorff dimension豪斯多夫维数===&lt;br /&gt;
&lt;br /&gt;
The '''Hausdorff dimension''' of ''X'' is defined by&lt;br /&gt;
&lt;br /&gt;
The Hausdorff dimension of X is defined by&lt;br /&gt;
&lt;br /&gt;
X 的豪斯多夫维数定义为&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt;\dim_{\operatorname{H}}(X):=\inf\{d\ge 0: \mathcal{H}^d(X)=0\}.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt;\dim_{\operatorname{H}}(X):=\inf\{d\ge 0: \mathcal{H}^d(X)=0\}.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Equivalently, dim&amp;lt;sub&amp;gt;H&amp;lt;/sub&amp;gt;(''X'') may be defined as the [[infimum]] of the set of ''d'' ∈ [0, ∞) such that the ''d''-dimensional [[Hausdorff measure]] of ''X'' is zero. This is the same as the supremum of the set of ''d''&amp;amp;nbsp;∈&amp;amp;nbsp;[0,&amp;amp;nbsp;∞) such that the ''d''-dimensional Hausdorff measure of ''X'' is infinite (except that when this latter set of numbers ''d'' is empty the Hausdorff dimension is zero).&lt;br /&gt;
&lt;br /&gt;
Equivalently, dim&amp;lt;sub&amp;gt;H&amp;lt;/sub&amp;gt;(X) may be defined as the infimum of the set of d ∈ [0, ∞) such that the d-dimensional Hausdorff measure of X is zero. This is the same as the supremum of the set of d&amp;amp;nbsp;∈&amp;amp;nbsp;[0,&amp;amp;nbsp;∞) such that the d-dimensional Hausdorff measure of X is infinite (except that when this latter set of numbers d is empty the Hausdorff dimension is zero).&lt;br /&gt;
&lt;br /&gt;
等价地，dim &amp;lt;sub&amp;gt;H&amp;lt;/sub&amp;gt;(''X'')可定义为 ''d'' ∈ [0, ∞) 集的下确界，使得''X'' 的''d''-维 [[豪斯多夫测度]] 为零。这与 ''d''&amp;amp;nbsp;∈&amp;amp;nbsp;[0,&amp;amp;nbsp;∞)的集合的上确界相同，因此''X''的 d 维豪斯多夫测度是无限的(除非后一个集合 ''d'' 是空的，豪斯多夫维数为零)。&lt;br /&gt;
&lt;br /&gt;
==Examples实例==&lt;br /&gt;
&lt;br /&gt;
[[Image:Sierpinski deep.svg|thumb|250px|Dimension of a further [[fractal]] example. The [[Sierpinski triangle]], an object with Hausdorff dimension of log(3)/log(2)≈1.58.&amp;lt;ref name=ClaytonSCTPLS96/&amp;gt;]]&lt;br /&gt;
&lt;br /&gt;
Dimension of a further [[fractal example. The Sierpinski triangle, an object with Hausdorff dimension of log(3)/log(2)≈1.58.]]&lt;br /&gt;
&lt;br /&gt;
[[Image:谢尔宾斯基三角形 deep.svg|thumb|250px|进一步的[[分形维数]]的例子，进一步的分形维数的例子是谢尔宾斯基三角形，它是一个豪斯多夫维数为log(3)/log(2)≈1.58.&amp;lt;ref name=ClaytonSCTPLS96/&amp;gt;的物体]]&lt;br /&gt;
&lt;br /&gt;
* [[Countable set]]s have Hausdorff dimension 0.&amp;lt;ref name=&amp;quot;schleicher&amp;quot;&amp;gt;{{cite journal |last1=Schleicher |first1=Dierk |title=Hausdorff Dimension, Its Properties, and Its Surprises |journal=The American Mathematical Monthly |date=June 2007 |volume=114 |issue=6 |pages=509–528 |doi=10.1080/00029890.2007.11920440 |language=en |issn=0002-9890|arxiv=math/0505099 }}&amp;lt;/ref&amp;gt;&lt;br /&gt;
*[[可数集]]拥有豪斯多夫维数0.&amp;lt;ref name=&amp;quot;schleicher&amp;quot;&amp;gt;{{cite journal |last1=Schleicher |first1=Dierk |title=豪斯多夫维数, Its Properties, and Its Surprises |journal=The American Mathematical Monthly美国数学期刊 |date=June 2007 |volume=114 |issue=6 |pages=509–528 |doi=10.1080/00029890.2007.11920440 |language=en |issn=0002-9890|arxiv=math/0505099 }}&amp;lt;/ref&amp;gt;&lt;br /&gt;
* The [[Euclidean space]] ℝ&amp;lt;sup&amp;gt;''n''&amp;lt;/sup&amp;gt; has Hausdorff dimension ''n'', and the circle '''S'''&amp;lt;sup&amp;gt;1&amp;lt;/sup&amp;gt; has Hausdorff dimension 1.&amp;lt;ref name=&amp;quot;schleicher&amp;quot; /&amp;gt;&lt;br /&gt;
*[[教育空间]] ℝ&amp;lt;sup&amp;gt;''n''&amp;lt;/sup&amp;gt; 有豪斯多夫维数 ''n''，循环'''S'''&amp;lt;sup&amp;gt;1&amp;lt;/sup&amp;gt; 拥有豪斯多夫维数1.&amp;lt;ref name=&amp;quot;schleicher&amp;quot; /&amp;gt;&lt;br /&gt;
* [[Fractal]]s often are spaces whose Hausdorff dimension strictly exceeds the [[topological dimension]].&amp;lt;ref name=&amp;quot;mandelbrot&amp;quot; /&amp;gt; For example, the [[Cantor set]], a zero-dimensional topological space, is a union of two copies of itself, each copy shrunk by a factor 1/3; hence, it can be shown that its Hausdorff dimension is ln(2)/ln(3)&amp;amp;nbsp;≈&amp;amp;nbsp;0.63.&amp;lt;ref&amp;gt;{{cite book | last=Falconer | first = Kenneth |title=Fractal Geometry: Mathematical Foundations and Applications | publisher=[[John Wiley and Sons]] | edition=2nd | year=2003}}&amp;lt;/ref&amp;gt; The [[Sierpinski triangle]] is a union of three copies of itself, each copy shrunk by a factor of&amp;amp;nbsp;1/2; this yields a Hausdorff dimension of ln(3)/ln(2)&amp;amp;nbsp;≈&amp;amp;nbsp;1.58.&amp;lt;ref name=CampbellAnnenberg15/&amp;gt; These Hausdorff dimensions are related to the &amp;quot;critical exponent&amp;quot; of the [[Master theorem (analysis of algorithms)|Master theorem]] for solving [[Recurrence relation|recurrence relations]] in the [[analysis of algorithms]].&lt;br /&gt;
*[[分形]]一般是那些豪斯多夫维数直接超过其拓扑维数的空间。例如[[康托尔集]]是一个o维拓扑空间，由两个自己复制而成，每一个复制品都是原来的三分之一，因此它的豪斯多夫维数是 ln(2)/ln(3)&amp;amp;nbsp;≈&amp;amp;nbsp;0.63。&amp;lt;ref&amp;gt;{{cite book | last=Falconer | first = Kenneth |title=Fractal Geometry: Mathematical Foundations and Applications | publisher=[[John Wiley and Sons]] | edition=2nd | year=2003}}&amp;lt;/ref&amp;gt;一个[[谢尔宾斯基三角]]是他自身三个复制的组合。每一个是原来的&amp;amp;nbsp;1/2，它的豪斯多夫维数ln(3)/ln(2)&amp;amp;nbsp;≈&amp;amp;nbsp;1.58。&amp;lt;ref name=CampbellAnnenberg15/&amp;gt;在递归算法中解决递归关系时，这些豪斯多夫维数与[[算法分析主定理]]的临界指标相联系。&lt;br /&gt;
* [[Space-filling curve]]s like the [[Peano curve]] have the same Hausdorff dimension as the space they fill.&lt;br /&gt;
*[[空间填充曲线]]拥有和他们填充空间同样的豪斯多夫维数，如[[皮亚诺曲线]]。&lt;br /&gt;
* The trajectory of [[Brownian motion]] in dimension 2 and above is conjectured to be Hausdorff dimension 2.&amp;lt;ref&amp;gt;{{cite book | last=Morters | first=Peres | title= Brownian Motion | publisher=[[Cambridge University Press]] | year=2010 }}&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
[[image:Great Britain Hausdorff.svg|thumb|250px|Estimating the Hausdorff dimension of the [[How Long Is the Coast of Britain? Statistical Self-Similarity and Fractional Dimension|coast of Great Britain]]]]&lt;br /&gt;
&lt;br /&gt;
coast of Great Britain]]&lt;br /&gt;
&lt;br /&gt;
[[大不列颠海岸&lt;br /&gt;
&lt;br /&gt;
* 刘易斯·弗赖伊·理查森[[Lewis Fry Richardson]] has performed detailed experiments to measure the approximate Hausdorff dimension for various coastlines. His results have varied from 1.02 for the coastline of [[South Africa]] to 1.25 for the west coast of [[Great Britain]].&amp;lt;ref name=&amp;quot;mandelbrot&amp;quot; /&amp;gt;&lt;br /&gt;
*刘易斯·弗赖伊·理查森（Lewis Fry Richardson）已经通过豪斯多夫维数去测量了很多海岸线。它的结果涵盖从1.02的南非海岸线到1.25的大英帝国西海岸模型。]]&lt;br /&gt;
&lt;br /&gt;
==Properties of Hausdorff dimension豪斯多夫维数特性==&lt;br /&gt;
&lt;br /&gt;
{{refimprove section|date=March 2015}}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
=== Hausdorff dimension and inductive dimension 豪斯多夫维数和归纳维数===&lt;br /&gt;
&lt;br /&gt;
Let ''X'' be an arbitrary [[Separable space|separable]] metric space. There is a [[topology|topological]] notion of [[inductive dimension]] for ''X'' which is defined recursively. It is always an integer (or +∞) and is denoted dim&amp;lt;sub&amp;gt;ind&amp;lt;/sub&amp;gt;(''X'').&lt;br /&gt;
&lt;br /&gt;
Let X be an arbitrary separable metric space. There is a topological notion of inductive dimension for X which is defined recursively. It is always an integer (or +∞) and is denoted dim&amp;lt;sub&amp;gt;ind&amp;lt;/sub&amp;gt;(X).&lt;br /&gt;
&lt;br /&gt;
设''X'' 是[[任意可分度量空间]]。对于''X'' 有一个递归定义的归纳维数拓扑概念。它总是一个整数(或 + ∞) ，并且表示dim&amp;lt;sub&amp;gt;ind&amp;lt;/sub&amp;gt;(''X'')。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
'''Theorem'''. Suppose ''X'' is non-empty. Then &lt;br /&gt;
&lt;br /&gt;
Theorem. Suppose X is non-empty. Then &lt;br /&gt;
&lt;br /&gt;
'''定理'''：假设''X'' 是非空的。那么&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt; \dim_{\mathrm{Haus}}(X) \geq \dim_{\operatorname{ind}}(X). &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \dim_{\mathrm{Haus}}(X) \geq \dim_{\operatorname{ind}}(X). &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Moreover,&lt;br /&gt;
&lt;br /&gt;
Moreover,&lt;br /&gt;
&lt;br /&gt;
此外,&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \inf_Y \dim_{\operatorname{Haus}}(Y) =\dim_{\operatorname{ind}}(X), &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \inf_Y \dim_{\operatorname{Haus}}(Y) =\dim_{\operatorname{ind}}(X), &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
where ''Y'' ranges over metric spaces [[homeomorphic]] to ''X''. In other words, ''X'' and ''Y'' have the same underlying set of points and the metric ''d''&amp;lt;sub&amp;gt;''Y''&amp;lt;/sub&amp;gt; of ''Y'' is topologically equivalent to ''d''&amp;lt;sub&amp;gt;''X''&amp;lt;/sub&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
where Y ranges over metric spaces homeomorphic to X. In other words, X and Y have the same underlying set of points and the metric d&amp;lt;sub&amp;gt;Y&amp;lt;/sub&amp;gt; of Y is topologically equivalent to d&amp;lt;sub&amp;gt;X&amp;lt;/sub&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
其中''Y''是度量空间同胚到 ''X''的范围。换句话说， ''X''和 ''Y''具有相同的基本点集，''Y''的度规''d''&amp;lt;sub&amp;gt;''Y''&amp;lt;/sub&amp;gt; 的子拓扑等价于''d''&amp;lt;sub&amp;gt;''X''&amp;lt;/sub&amp;gt;。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
These results were originally established by [[Edward Szpilrajn]] (1907–1976), e.g., see Hurewicz and Wallman, Chapter VII.{{full citation needed|date=March 2015}}&lt;br /&gt;
&lt;br /&gt;
These results were originally established by Edward Szpilrajn (1907–1976), e.g., see Hurewicz and Wallman, Chapter VII.&lt;br /&gt;
&lt;br /&gt;
这些结果最初是由 [[Edward Szpilrajn]] (1907–1976)建立的,  参见 Hurewicz and Wallman, Chapter VII.{{full citation needed|date=March 2015}}第七章。&lt;br /&gt;
&lt;br /&gt;
=== Hausdorff dimension and Minkowski dimension 豪斯多夫维数和闵可夫斯基维度===&lt;br /&gt;
&lt;br /&gt;
The [[Minkowski dimension]] is similar to, and at least as large as, the Hausdorff dimension, and they are equal in many situations. However, the set of [[rational number|rational]] points in [0, 1] has Hausdorff dimension zero and Minkowski dimension one. There are also compact sets for which the Minkowski dimension is strictly larger than the Hausdorff dimension.&lt;br /&gt;
&lt;br /&gt;
The Minkowski dimension is similar to, and at least as large as, the Hausdorff dimension, and they are equal in many situations. However, the set of rational points in [0, 1] has Hausdorff dimension zero and Minkowski dimension one. There are also compact sets for which the Minkowski dimension is strictly larger than the Hausdorff dimension.&lt;br /&gt;
&lt;br /&gt;
[[闵可夫斯基维数]]与豪斯多夫维数相似，至少和它一样大，而且在许多情况下是相等的。然而，[0,1]中有理点集的豪斯多夫维数为0，闵可夫斯基维数为1。还有一些紧集的闵可夫斯基维数绝对大于豪斯多夫维数。&lt;br /&gt;
&lt;br /&gt;
=== Hausdorff dimensions and Frostman measures 豪斯多夫维度和弗洛斯曼测度===&lt;br /&gt;
&lt;br /&gt;
If there is a [[measure (mathematics)|measure]] μ defined on [[Borel measure|Borel]] subsets of a metric space ''X'' such that ''μ''(''X'') &amp;gt; 0 and ''μ''(''B''(''x'', ''r'')) ≤ ''r&amp;lt;sup&amp;gt;s&amp;lt;/sup&amp;gt;'' holds for some constant ''s'' &amp;gt; 0 and for every ball ''B''(''x'', ''r'') in ''X'', then dim&amp;lt;sub&amp;gt;Haus&amp;lt;/sub&amp;gt;(''X'') ≥ ''s''. A partial converse is provided by [[Frostman's lemma]].{{citation needed|date=March 2015}}&amp;lt;ref&amp;gt;This Wikipedia article also discusses further useful characterizations of the Hausdorff dimension.{{clarify|date=March 2015}}&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
If there is a measure μ defined on Borel subsets of a metric space X such that μ(X) &amp;gt; 0 and μ(B(x, r)) ≤ r&amp;lt;sup&amp;gt;s&amp;lt;/sup&amp;gt; holds for some constant s &amp;gt; 0 and for every ball B(x, r) in X, then dim&amp;lt;sub&amp;gt;Haus&amp;lt;/sub&amp;gt;(X) ≥ s. A partial converse is provided by Frostman's lemma.&lt;br /&gt;
&lt;br /&gt;
如果在度量空间 ''X'' 的 Borel 子集上定义一个测度 μ，使得''μ''(''X'') &amp;gt; 0 和''μ''(''B''(''x'', ''r'')) ≤ ''r&amp;lt;sup&amp;gt;s&amp;lt;/sup&amp;gt;''，对于某个常数 ''s'' &amp;gt; 0  和 ''X'' 中的每个球 ''B''(''x'', ''r'') 成立，则 dim&amp;lt;sub&amp;gt;Haus&amp;lt;/sub&amp;gt;(''X'') ≥ ''s'' 。 部分逆向转换由弗洛斯曼引理定义。&lt;br /&gt;
&lt;br /&gt;
=== Behaviour under unions and products ===&lt;br /&gt;
&lt;br /&gt;
If &amp;lt;math&amp;gt;X=\bigcup_{i\in I}X_i&amp;lt;/math&amp;gt; is a finite or countable union, then&lt;br /&gt;
&lt;br /&gt;
If &amp;lt;math&amp;gt;X=\bigcup_{i\in I}X_i&amp;lt;/math&amp;gt; is a finite or countable union, then&lt;br /&gt;
&lt;br /&gt;
如果 &amp;lt;math&amp;gt;X=\bigcup_{i\in I}X_i&amp;lt;/math&amp;gt; 是一个有限或可数的联合，则&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \dim_{\operatorname{Haus}}(X) =\sup_{i\in I} \dim_{\operatorname{Haus}}(X_i).&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \dim_{\operatorname{Haus}}(X) =\sup_{i\in I} \dim_{\operatorname{Haus}}(X_i).&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
This can be verified directly from the definition.&lt;br /&gt;
&lt;br /&gt;
This can be verified directly from the definition.&lt;br /&gt;
&lt;br /&gt;
这可以直接从定义得到验证。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
If ''X'' and ''Y'' are non-empty metric spaces, then the Hausdorff dimension of their product satisfies&amp;lt;ref&amp;gt;{{cite journal |author=Marstrand, J. M. |title=The dimension of Cartesian product sets |journal=Proc. Cambridge Philos. Soc. |volume=50 |issue=3 |pages=198–202 |year=1954 |doi=10.1017/S0305004100029236 |bibcode = 1954PCPS...50..198M }}&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
If X and Y are non-empty metric spaces, then the Hausdorff dimension of their product satisfies&lt;br /&gt;
&lt;br /&gt;
如果 ''X'' 和''Y''是非空度量空间，那么它们乘积的豪斯多夫维数满足&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt; \dim_{\operatorname{Haus}}(X\times Y)\ge \dim_{\operatorname{Haus}}(X)+ \dim_{\operatorname{Haus}}(Y).&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \dim_{\operatorname{Haus}}(X\times Y)\ge \dim_{\operatorname{Haus}}(X)+ \dim_{\operatorname{Haus}}(Y).&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
This inequality can be strict. It is possible to find two sets of dimension 0 whose product has dimension 1.&amp;lt;ref&amp;gt;{{cite book  | last = Falconer  | first = Kenneth J.  | title = Fractal geometry. Mathematical foundations and applications  | publisher = John Wiley &amp;amp; Sons, Inc., Hoboken, New Jersey  | year = 2003  | doi =   | isbn = }}&amp;lt;/ref&amp;gt; In the opposite direction, it is known that when ''X'' and ''Y'' are Borel subsets of '''R'''&amp;lt;sup&amp;gt;''n''&amp;lt;/sup&amp;gt;, the Hausdorff dimension of ''X'' × ''Y'' is bounded from above by the Hausdorff dimension of ''X'' plus the [[packing dimension|upper packing dimension]] of ''Y''. These facts are discussed in Mattila (1995).&lt;br /&gt;
&lt;br /&gt;
This inequality can be strict. It is possible to find two sets of dimension 0 whose product has dimension 1. In the opposite direction, it is known that when X and Y are Borel subsets of R&amp;lt;sup&amp;gt;n&amp;lt;/sup&amp;gt;, the Hausdorff dimension of X × Y is bounded from above by the Hausdorff dimension of X plus the upper packing dimension of Y. These facts are discussed in Mattila (1995).&lt;br /&gt;
&lt;br /&gt;
这种不平等可以是绝对的。有可能找到两个维数为0的集合，其乘积的维数为1。相反，我们知道当''X''和''Y''是 '''R'''&amp;lt;sup&amp;gt;''n''&amp;lt;/sup&amp;gt;的 Borel 子集时， ''X'' × ''Y''的豪斯多夫维数从上面以 ''X''的豪斯多夫维数加上 ''Y''的填充维数为界。Mattila (1995)曾就这些情况进行了讨论。&lt;br /&gt;
&lt;br /&gt;
==Self-similar sets自相似集合==&lt;br /&gt;
&lt;br /&gt;
{{refimprove section|date=March 2015}}&lt;br /&gt;
&lt;br /&gt;
Many sets defined by a self-similarity condition have dimensions which can be determined explicitly. Roughly, a set ''E'' is self-similar if it is the fixed point of a set-valued transformation ψ, that is ψ(''E'') = ''E'', although the exact definition is given below.&lt;br /&gt;
&lt;br /&gt;
Many sets defined by a self-similarity condition have dimensions which can be determined explicitly. Roughly, a set E is self-similar if it is the fixed point of a set-valued transformation ψ, that is ψ(E) = E, although the exact definition is given below.&lt;br /&gt;
&lt;br /&gt;
许多由自相似条件定义的集合具有可以显式确定的维数。粗略地说，集合''E'' 是自相似的，如果它是集值ψ变换的不动点，即ψ(''E'') = ''E''，尽管下面给出了确切的定义。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&amp;lt;blockquote&amp;gt;'''Theorem'''. Suppose&lt;br /&gt;
&lt;br /&gt;
&amp;lt;blockquote&amp;gt;Theorem. Suppose&lt;br /&gt;
&lt;br /&gt;
&amp;lt;blockquote&amp;gt;'''定理'''：假设&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt; \psi_i: \mathbf{R}^n \rightarrow \mathbf{R}^n, \quad i=1, \ldots , m &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \psi_i: \mathbf{R}^n \rightarrow \mathbf{R}^n, \quad i=1, \ldots , m &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
are [[Contraction mapping|contractive]] mappings on '''R'''&amp;lt;sup&amp;gt;''n''&amp;lt;/sup&amp;gt; with contraction constant ''r&amp;lt;sub&amp;gt;j&amp;lt;/sub&amp;gt;'' &amp;lt; 1. Then there is a unique ''non-empty'' compact set ''A'' such that&lt;br /&gt;
&lt;br /&gt;
are contractive mappings on R&amp;lt;sup&amp;gt;n&amp;lt;/sup&amp;gt; with contraction constant r&amp;lt;sub&amp;gt;j&amp;lt;/sub&amp;gt; &amp;lt; 1. Then there is a unique non-empty compact set A such that&lt;br /&gt;
&lt;br /&gt;
是'''R'''&amp;lt;sup&amp;gt;''n''&amp;lt;/sup&amp;gt;上的压缩常数''r&amp;lt;sub&amp;gt;j&amp;lt;/sub&amp;gt;'&amp;lt; 1的压缩映射。然后有一个唯一的非空紧集A &lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt; A = \bigcup_{i=1}^m \psi_i (A). &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; A = \bigcup_{i=1}^m \psi_i (A). &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&amp;lt;/blockquote&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;/blockquote&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The theorem follows from [[Stefan Banach]]'s [[Contractive mapping theorem|contractive mapping fixed point theorem]] applied to the complete metric space of non-empty compact subsets of '''R'''&amp;lt;sup&amp;gt;''n''&amp;lt;/sup&amp;gt; with the [[Hausdorff distance]].&amp;lt;ref&amp;gt;{{cite book |author=Falconer, K. J. |title=The Geometry of Fractal Sets |publisher=Cambridge University Press |location=Cambridge, UK |year=1985 |isbn=0-521-25694-1 |chapter=Theorem 8.3}}&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
The theorem follows from Stefan Banach's contractive mapping fixed point theorem applied to the complete metric space of non-empty compact subsets of R&amp;lt;sup&amp;gt;n&amp;lt;/sup&amp;gt; with the Hausdorff distance.&lt;br /&gt;
&lt;br /&gt;
这个定理来源于 Stefan Banach 的压缩映射不动点定理，该定理应用于 '''R'''&amp;lt;sup&amp;gt;''n''&amp;lt;/sup&amp;gt; 的非空紧子集的完备空间豪斯多夫距离。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
===The open set condition开集条件===&lt;br /&gt;
&lt;br /&gt;
To determine the dimension of the self-similar set ''A'' (in certain cases), we need a technical condition called the ''open set condition'' (OSC) on the sequence of contractions ψ&amp;lt;sub&amp;gt;''i''&amp;lt;/sub&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
To determine the dimension of the self-similar set A (in certain cases), we need a technical condition called the open set condition (OSC) on the sequence of contractions ψ&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
为了确定自相似集''A'' 的维数(在某些情况下) ，我们需要一个称为''开集条件''(OSC)的技术条件ψ&amp;lt;sub&amp;gt;''i''&amp;lt;/sub&amp;gt;。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
There is a relatively compact open set ''V'' such that&lt;br /&gt;
&lt;br /&gt;
There is a relatively compact open set V such that&lt;br /&gt;
&lt;br /&gt;
有一个相对紧的开集''V''&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt; \bigcup_{i=1}^m\psi_i (V) \subseteq V, &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \bigcup_{i=1}^m\psi_i (V) \subseteq V, &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
where the sets in union on the left are pairwise [[disjoint sets|disjoint]].&lt;br /&gt;
&lt;br /&gt;
where the sets in union on the left are pairwise disjoint.&lt;br /&gt;
&lt;br /&gt;
左边的集合是成对不相交的。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The open set condition is a separation condition that ensures the images ψ&amp;lt;sub&amp;gt;''i''&amp;lt;/sub&amp;gt;(''V'') do not overlap &amp;quot;too much&amp;quot;.&lt;br /&gt;
&lt;br /&gt;
The open set condition is a separation condition that ensures the images ψ&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;(V) do not overlap &amp;quot;too much&amp;quot;.&lt;br /&gt;
&lt;br /&gt;
开集条件是保证图像子ψ&amp;lt;sub&amp;gt;''i''&amp;lt;/sub&amp;gt;(''V'') 不重叠“太多”的分离条件。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
'''Theorem'''. Suppose the open set condition holds and each ψ&amp;lt;sub&amp;gt;''i''&amp;lt;/sub&amp;gt; is a similitude, that is a composition of an [[isometry]] and a [[dilation (metric space)|dilation]] around some point. Then the unique fixed point of ψ is a set whose Hausdorff dimension is ''s'' where ''s'' is the unique solution of&amp;lt;ref&amp;gt;{{cite journal | last=Hutchinson | first=John E. | title=Fractals and self similarity | journal=Indiana Univ. Math. J. | volume=30 | year=1981 | pages=713–747 | doi=10.1512/iumj.1981.30.30055 | issue=5 | doi-access=free }}&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
Theorem. Suppose the open set condition holds and each ψ&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt; is a similitude, that is a composition of an isometry and a dilation around some point. Then the unique fixed point of ψ is a set whose Hausdorff dimension is s where s is the unique solution of&lt;br /&gt;
&lt;br /&gt;
'''定理'''假设开集条件成立，并且每个ψ&amp;lt;sub&amp;gt;''i''&amp;lt;/sub&amp;gt; 是一个相似量，这是一个等距和围绕某一点的膨胀的合成。那么唯一的不动点是一个集合，它的豪斯多夫维数是 ''s'' ，其中  ''s'' 是 ''s'' &amp;lt;ref&amp;gt;{{cite journal | last=Hutchinson | first=John E. | title=Fractals and self similarity | journal=Indiana Univ. Math. J. | volume=30 | year=1981 | pages=713–747 | doi=10.1512/iumj.1981.30.30055 | issue=5 | doi-access=free }}&amp;lt;/ref&amp;gt;的唯一解&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt; \sum_{i=1}^m r_i^s = 1. &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \sum_{i=1}^m r_i^s = 1. &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The contraction coefficient of a similitude is the magnitude of the dilation.&lt;br /&gt;
&lt;br /&gt;
The contraction coefficient of a similitude is the magnitude of the dilation.&lt;br /&gt;
&lt;br /&gt;
相似物的收缩系数就是膨胀的大小。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
We can use this theorem to compute the Hausdorff dimension of the Sierpinski triangle (or sometimes called Sierpinski gasket). Consider three [[non-collinear points]] ''a''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;, ''a''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;, ''a''&amp;lt;sub&amp;gt;3&amp;lt;/sub&amp;gt; in the plane '''R'''&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; and let ψ&amp;lt;sub&amp;gt;''i''&amp;lt;/sub&amp;gt; be the dilation of ratio 1/2 around ''a&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;''. The unique non-empty fixed point of the corresponding mapping ψ is a Sierpinski gasket and the dimension ''s'' is the unique solution of&lt;br /&gt;
&lt;br /&gt;
We can use this theorem to compute the Hausdorff dimension of the Sierpinski triangle (or sometimes called Sierpinski gasket). Consider three non-collinear points a&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;, a&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;, a&amp;lt;sub&amp;gt;3&amp;lt;/sub&amp;gt; in the plane R&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; and let ψ&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt; be the dilation of ratio 1/2 around a&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;. The unique non-empty fixed point of the corresponding mapping ψ is a Sierpinski gasket and the dimension s is the unique solution of&lt;br /&gt;
&lt;br /&gt;
我们可以使用这个定理来计算谢尔宾斯基三角形的豪斯多夫维数(或者有时候叫做谢尔宾斯基垫圈)。考虑R&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; 平面上的三个非共线点，''a''&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;，''a''&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;，''a''&amp;lt;sub&amp;gt;3&amp;lt;/sub&amp;gt;，让ψ&amp;lt;sub&amp;gt;''i''&amp;lt;/sub&amp;gt;是围绕着''a&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;''膨胀比率的1/2。对应映射的唯一非空不动点是一个谢尔宾斯基垫圈，其维数''s''是对应映射的唯一解&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt; \left(\frac{1}{2}\right)^s+\left(\frac{1}{2}\right)^s+\left(\frac{1}{2}\right)^s = 3 \left(\frac{1}{2}\right)^s =1. &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \left(\frac{1}{2}\right)^s+\left(\frac{1}{2}\right)^s+\left(\frac{1}{2}\right)^s = 3 \left(\frac{1}{2}\right)^s =1. &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Taking [[natural logarithm]]s of both sides of the above equation, we can solve for ''s'', that is: ''s'' = ln(3)/ln(2).  The Sierpinski gasket is self-similar and satisfies the OSC. In general a set ''E'' which is a fixed point of a mapping&lt;br /&gt;
&lt;br /&gt;
Taking natural logarithms of both sides of the above equation, we can solve for s, that is: s = ln(3)/ln(2).  The Sierpinski gasket is self-similar and satisfies the OSC. In general a set E which is a fixed point of a mapping&lt;br /&gt;
&lt;br /&gt;
取上述方程两边的自然对数，我们可以求出 ''s''，即: ''s'' = ln(3)/ln(2)。该密封垫具有自相似性，满足 OSC 要求。一般来说，集合 ''E''是一个映射的不动点&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt; A \mapsto \psi(A) = \bigcup_{i=1}^m \psi_i(A) &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt; A \mapsto \psi(A) = \bigcup_{i=1}^m \psi_i(A) &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
is self-similar if and only if the intersections&lt;br /&gt;
&lt;br /&gt;
is self-similar if and only if the intersections&lt;br /&gt;
&lt;br /&gt;
是自相似的，当且仅当&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt; H^s\left(\psi_i(E) \cap \psi_j(E)\right) =0, &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; H^s\left(\psi_i(E) \cap \psi_j(E)\right) =0, &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
where ''s'' is the Hausdorff dimension of ''E'' and ''H&amp;lt;sup&amp;gt;s&amp;lt;/sup&amp;gt;'' denotes [[Hausdorff measure]]. This is clear in the case of the Sierpinski gasket (the intersections are just points), but is also true more generally:&lt;br /&gt;
&lt;br /&gt;
where s is the Hausdorff dimension of E and H&amp;lt;sup&amp;gt;s&amp;lt;/sup&amp;gt; denotes Hausdorff measure. This is clear in the case of the Sierpinski gasket (the intersections are just points), but is also true more generally:&lt;br /&gt;
&lt;br /&gt;
其中 ''s''是''E''的豪斯多夫维数， ''E'' and ''H&amp;lt;sup&amp;gt;s&amp;lt;/sup&amp;gt;'' 表示 豪斯多夫测度。对于谢尔宾斯基垫圈(交叉点就是点)来说，这一点很明显，但更普遍的情况是:&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
'''Theorem'''. Under the same conditions as the previous theorem, the unique fixed point of ψ is self-similar.&lt;br /&gt;
&lt;br /&gt;
Theorem. Under the same conditions as the previous theorem, the unique fixed point of ψ is self-similar.&lt;br /&gt;
&lt;br /&gt;
'''定理'''：在与前一定理相同的条件下，其唯一不动点是自相似的。&lt;br /&gt;
&lt;br /&gt;
==See also参阅==&lt;br /&gt;
&lt;br /&gt;
* [[List of fractals by Hausdorff dimension豪斯多夫分形维数列表]] Examples of deterministic fractals, random and natural fractals.确定性分形与随机和自然分形的示例。&lt;br /&gt;
&lt;br /&gt;
* [[Assouad dimension  Assouad维数]], another variation of fractal dimension that, like Hausdorff dimension, is defined using coverings by balls其他被球覆盖方式定义的分形维数，例如豪斯多夫维数。&lt;br /&gt;
&lt;br /&gt;
* [[Intrinsic dimension固有维数]]&lt;br /&gt;
&lt;br /&gt;
* [[Packing dimension填充维数]]&lt;br /&gt;
&lt;br /&gt;
* [[Fractal dimension分形维数]]&lt;br /&gt;
&lt;br /&gt;
==References参考文献==&lt;br /&gt;
&lt;br /&gt;
{{reflist}}&lt;br /&gt;
&lt;br /&gt;
==Further reading拓展阅读==&lt;br /&gt;
&lt;br /&gt;
* {{cite book |last1=Dodson |first1=M. Maurice |title=Fractal Geometry and Applications: A Jubilee of Benoît Mandelbrot |volume=72 |issue=1 |pages=305–347 |last2=Kristensen |first2=Simon |chapter=Hausdorff Dimension and Diophantine Approximation |date=June 12, 2003 |arxiv=math/0305399 |bibcode = 2003math......5399D |doi=10.1090/pspum/072.1/2112110|series=Proceedings of Symposia in Pure Mathematics |isbn=9780821836378 }}&lt;br /&gt;
&lt;br /&gt;
* {{cite book |last1=Hurewicz |first1=Witold |authorlink1=Witold Hurewicz |last2=Wallman |first2=Henry |authorlink2=Henry Wallman |title=Dimension Theory |url=https://archive.org/details/in.ernet.dli.2015.84609 |publisher=Princeton University Press |year=1948 }}&lt;br /&gt;
&lt;br /&gt;
* {{cite journal |author作者=E. Szpilrajn |authorlink=Edward Marczewski |title=La dimension et la mesure |journal=Fundamenta Mathematicae |volume=28 |pages=81–9 |year=1937 }}&lt;br /&gt;
&lt;br /&gt;
* {{cite journal&lt;br /&gt;
&lt;br /&gt;
 | last1=Marstrand&lt;br /&gt;
&lt;br /&gt;
 | last1=Marstrand&lt;br /&gt;
&lt;br /&gt;
 | last1=马斯特兰德&lt;br /&gt;
&lt;br /&gt;
 | first1=J. M. | title=The dimension of cartesian product sets | year=1954 | journal=Proc. Cambridge Philos. Soc.&lt;br /&gt;
&lt;br /&gt;
 | first1=J. M. | title=The dimension of cartesian product sets | year=1954 | journal=Proc. Cambridge Philos. Soc.&lt;br /&gt;
&lt;br /&gt;
 | first1= J. M. | title=笛卡儿积集的维数 | 1954年 |  journal=Proc. Cambridge Philos. Soc.&lt;br /&gt;
&lt;br /&gt;
 | volume=50&lt;br /&gt;
&lt;br /&gt;
 | volume=50&lt;br /&gt;
&lt;br /&gt;
 | 第50卷&lt;br /&gt;
&lt;br /&gt;
 | issue=3&lt;br /&gt;
&lt;br /&gt;
 | issue=3&lt;br /&gt;
&lt;br /&gt;
 | 第三期&lt;br /&gt;
&lt;br /&gt;
 | pages=198–202&lt;br /&gt;
&lt;br /&gt;
 | pages=198–202&lt;br /&gt;
&lt;br /&gt;
 | 第198-202页&lt;br /&gt;
&lt;br /&gt;
 | doi=10.1017/S0305004100029236|bibcode = 1954PCPS...50..198M }}&lt;br /&gt;
&lt;br /&gt;
 | doi=10.1017/S0305004100029236|bibcode = 1954PCPS...50..198M }}&lt;br /&gt;
&lt;br /&gt;
10.1017 / S0305004100029236 | bibcode 1954PCPS... 50. . 198 m }&lt;br /&gt;
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* {{Cite book&lt;br /&gt;
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 | last1=Mattila&lt;br /&gt;
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 | last1=Mattila&lt;br /&gt;
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 | last1=Mattila&lt;br /&gt;
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 | first1=Pertti | author1-link=Pertti Mattila| title=Geometry of sets and measures in Euclidean spaces | publisher=[[Cambridge University Press]]&lt;br /&gt;
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 | first1=Pertti | author1-link=Pertti Mattila| title=Geometry of sets and measures in Euclidean spaces | publisher=Cambridge University Press&lt;br /&gt;
&lt;br /&gt;
| first1 Pertti | author1-link Pertti Mattila | title 欧几里德空间中集合和度量的几何 | 出版商剑桥大学出版社&lt;br /&gt;
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 | isbn=978-0-521-65595-8 | year=1995}}&lt;br /&gt;
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 | isbn=978-0-521-65595-8 | year=1995}}&lt;br /&gt;
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| isbn 978-0-521-65595-8 | year 1995}&lt;br /&gt;
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* {{cite journal |author=A. S. Besicovitch |authorlink=A. S. Besicovitch |title=On Linear Sets of Points of Fractional Dimensions |journal=[[Mathematische Annalen]] |volume=101 |year=1929 | doi=10.1007/BF01454831| issue=1 |pages= 161–193}}&lt;br /&gt;
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* {{cite journal |author1=A. S. Besicovitch |authorlink1=A. S. Besicovitch |author2=H. D. Ursell |authorlink2=H. D. Ursell |title=Sets of Fractional Dimensions |journal=Journal of the London Mathematical Society |volume=12 |year=1937 | issue=1 | doi=10.1112/jlms/s1-12.45.18  | pages=18–25 }}&amp;lt;br/&amp;gt;Several selections from this volume are reprinted in {{cite book |author=Edgar, Gerald A. |title=Classics on fractals |publisher=Addison-Wesley |location=Boston |year=1993 |isbn=0-201-58701-7}} See chapters 9,10,11&lt;br /&gt;
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* {{cite journal |author=F. Hausdorff |authorlink=F. Hausdorff |title=Dimension und äußeres Maß |journal=Mathematische Annalen |volume=79 |issue=1–2 |pages=157–179 |date=March 1919 |doi=10.1007/BF01457179|hdl=10338.dmlcz/100363 |url=http://dml.cz/bitstream/handle/10338.dmlcz/100363/CzechMathJ_09-1959-3_5.pdf }}&lt;br /&gt;
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* {{cite journal | last=Hutchinson | first=John E. | title=Fractals and self similarity | journal=Indiana Univ. Math. J. | volume=30 | year=1981 | pages=713–747 | doi=10.1512/iumj.1981.30.30055 | issue=5 | doi-access=free }}&lt;br /&gt;
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*{{cite book | last=Falconer | first = Kenneth |title=Fractal Geometry: Mathematical Foundations and Applications | publisher=[[John Wiley and Sons]] | edition=2nd | year=2003}}&lt;br /&gt;
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==External links外部链接==&lt;br /&gt;
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* [https://www.encyclopediaofmath.org/index.php/Hausdorff_dimension Hausdorff dimension] 在 [https://www.encyclopediaofmath.org/ Encyclopedia of Mathematics]&lt;br /&gt;
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* [https://www.encyclopediaofmath.org/index.php/Hausdorff_measure Hausdorff measure] 在 [https://www.encyclopediaofmath.org/ Encyclopedia of Mathematics]&lt;br /&gt;
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{{DEFAULTSORT:Hausdorff Dimension豪斯多夫维数}}&lt;br /&gt;
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[[Category分类:Fractals分形]]&lt;br /&gt;
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[[Category分类:Metric geometry度量几何]]&lt;br /&gt;
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[[Category分类:Dimension theory维度理论]]&lt;br /&gt;
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&amp;lt;small&amp;gt;This page was moved from [[wikipedia:en:Hausdorff dimension]]. Its edit history can be viewed at [[分形维数/edithistory]]&amp;lt;/small&amp;gt;&amp;lt;/noinclude&amp;gt;&lt;br /&gt;
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[[Category:待整理页面]]&lt;/div&gt;</summary>
		<author><name>Ruili</name></author>
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