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		<title>量子图灵机</title>
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		<updated>2023-02-15T02:35:39Z</updated>

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&lt;div&gt;{{#seo:&lt;br /&gt;
|keywords=量子计算机，量子算法，抽象机器&lt;br /&gt;
|description=是一种用来模拟量子计算机效果的抽象机器&lt;br /&gt;
}}&lt;br /&gt;
== 基础定义 ==&lt;br /&gt;
'''量子图灵机 quantum Turing machine (QTM)''' 又称为'''通用量子计算机'''，是一种用来模拟量子计算机效果的抽象机器。尽管说提供等效计算能力的量子电路是一种更常用的模型，但是量子图灵机是一个简单但能展现出量子计算的所有威力的模型。就像经典图灵机可以模拟人类所能进行的任何计算过程一样，量子图灵机可以描述任何量子算法。&amp;lt;ref name=&amp;quot;equivalence&amp;quot;&amp;gt;{{cite conference|author=[[Andrew Yao]]|title=Quantum circuit complexity|conference=34th Annual Symposium on Foundations of Computer Science|pages=352–361|year=1993}}&amp;lt;/ref&amp;gt;&amp;lt;ref name=&amp;quot;newequivalence&amp;quot;&amp;gt;{{cite arXiv|eprint=1808.01701|author1=Abel Molina|author2=John Watrous|title=Revisiting the simulation of quantum Turing machines by quantum circuits|date=2018|class=cs.CC}}&amp;lt;/ref&amp;gt;&lt;br /&gt;
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== 与经典计算的关系 ==&lt;br /&gt;
通过[[过渡矩阵]]，量子图灵机可以与经典图灵机和概率图灵机相关联。Lance Fortnow证明，量子图灵机的量子概率矩阵可以被拆解成是指定矩阵与经典或概率图灵机的矩阵的乘积。&amp;lt;ref name=&amp;quot;transition&amp;quot;&amp;gt;{{cite journal|author=Fortnow|first=Lance|year=2003|title=One Complexity Theorist's View of Quantum Computing|url=|journal=Theoretical Computer Science|volume=292|issue=3|pages=597–610|doi=10.1016/S0304-3975(01)00377-2|via=|arxiv=quant-ph/0003035}}&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
== 非正式草图定义 ==&lt;br /&gt;
&lt;br /&gt;
我们可以通过类比确定有限自动机 deterministic finite automaton到量子有限自动机 quantum finite automaton的转化来理解经典图灵机 Turing machine (TM)到量子图灵机的转化。 他们的差异在于，经典图灵机讨论的状态被推广到了Hilbert空间中。Hilbert空间是完备的内积空间，是有限维欧几里得空间的一个推广。它不局限于实数的情形和有限的维数，但又不失完备性。在量子图灵机中转换函数被一组映射Hilbert空间到自身的酉矩阵 unitary matrix取代。&amp;lt;ref name=&amp;quot;Deutsch1985&amp;quot; /&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
经典图灵机的诞生是因为图灵想用机器来模拟用纸笔进行数学运算的过程，这样的过程可以被看作下列两种简单的动作：&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
* 在纸带上写上或删除某个符号；&lt;br /&gt;
* 把笔尖从纸的一处移动到另一处；&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
现在我们假设有一条纸带无限长，并且被划分为一个接一个的小格子，每个格子上包含一个来自有限字母表的符号，字母表中有一个特殊的符号表示空白。假设我们有一个执笔机器又称为读写头（'''HEAD'''），它本身也可以具有一个状态。就像人今天可能因为某件事心情很好，也可能因为另一件事情很抑郁一样，它的状态会随着它的遭遇所改变。更重要的是执笔机器当前关注的纸上的某个位置的符号和当前的状态决定了下一步的动作。在遇到停止状态&amp;lt;math&amp;gt;F&amp;lt;/math&amp;gt;之前执笔机器可以&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
* 1. 写入（替换）或擦除当前符号；&lt;br /&gt;
* 2. 移动 '''HEAD'''， 'L'向左一步， 'R'向右一步或者'N'不移动；&lt;br /&gt;
* 3. 保持当前状态或者转到另一状态。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
总的来说，经典图灵机可以被一个七元有序组所描述，&amp;lt;math&amp;gt;M = \langle Q, \Gamma, b, \Sigma, \delta, q_0, F \rangle&amp;lt;/math&amp;gt;。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
* &amp;lt;math&amp;gt;Q&amp;lt;/math&amp;gt; 为被推广到了Hilbert空间的状态集；&lt;br /&gt;
* &amp;lt;math&amp;gt;\Gamma&amp;lt;/math&amp;gt; 是输入字母表；&lt;br /&gt;
* &amp;lt;math&amp;gt;b \in \Gamma&amp;lt;/math&amp;gt; 为''空白符''，也是唯一允许出现无限次的字符；&lt;br /&gt;
* 输入和输出符号 &amp;lt;math&amp;gt;\Sigma&amp;lt;/math&amp;gt;通常是一个离散集。和经典图灵机的输入输出符号一样，它们不需要是一个量子系统。&lt;br /&gt;
* &amp;lt;math&amp;gt;\delta : \Sigma \times Q  \otimes \Gamma \rightarrow \Sigma \times Q \otimes \Gamma \times \{L,R\}&amp;lt;/math&amp;gt;是被推广到了Hilbert空间的转移函数。我们也可以理解它们为一些在Hilbert空间中自同构的酉矩阵。&lt;br /&gt;
* &amp;lt;math&amp;gt;q_0 \in Q&amp;lt;/math&amp;gt;是起始状态，它可以是几种状态的混合也可以是一种状态；&lt;br /&gt;
* 停止状态&amp;lt;math&amp;gt;F&amp;lt;/math&amp;gt;是&amp;lt;math&amp;gt;Q&amp;lt;/math&amp;gt;的子集。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
以上只是一个量子图灵机的草图，而不是它的正式定义，因为它的一些重要细节仍然定义模糊：例如，我们以什么样的频率执行对于状态的观测；什么是一次观测量子有限自动机 measure-once和多次观测量子有限自动机 measure-many QFA之间的区别。这些观测问题会影响我们如何定义写入和输出纸带的方式。&lt;br /&gt;
&lt;br /&gt;
==历史==&lt;br /&gt;
物理学家 Paul Benioff 在1980 年和 1982 年发表的论文中，首次描述了图灵机的量子力学模型。&amp;lt;ref name=&amp;quot;:0&amp;quot;&amp;gt;{{cite journal |last1=Benioff | first1=Paul | title=The computer as a physical system: A microscopic quantum mechanical Hamiltonian model of computers as represented by Turing machines | journal=Journal of Statistical Physics |volume=22 | issue=5 | pages=563–591 | year=1980 | doi=10.1007/bf01011339|bibcode=1980JSP....22..563B }}&amp;lt;/ref&amp;gt;&amp;lt;ref name=&amp;quot;:1&amp;quot;&amp;gt;{{Cite journal | doi=10.1007/BF01342185 | last1=Benioff | first1=P. | title=Quantum mechanical hamiltonian models of turing machines | journal=Journal of Statistical Physics | volume=29 | issue=3 | pages=515–546 | year=1982|bibcode=1982JSP....29..515B }}&amp;lt;/ref&amp;gt;牛津大学物理学家 David Deutsch 在 1985 年撰写的一篇文章中进一步推广了量子计算机的概念，他提议量子门[[quantum gate]]应该以类似于传统数字计算二进制逻辑门的方式运行。&amp;lt;ref name=&amp;quot;Deutsch1985&amp;quot;&amp;gt;{{cite journal|last=Deutsch|first=David|date=July 1985|title=Quantum theory, the Church-Turing principle and the universal quantum computer|url=http://www.ceid.upatras.gr/tech_news/papers/quantum_theory.pdf|url-status=dead|journal=[[Proceedings of the Royal Society A]]|volume=400|issue=1818|pages=97–117|bibcode=1985RSPSA.400...97D|doi=10.1098/rspa.1985.0070|archiveurl=https://web.archive.org/web/20081123183419/http://www.ceid.upatras.gr/tech_news/papers/quantum_theory.pdf|archivedate=2008-11-23|citeseerx=10.1.1.41.2382}}&amp;lt;/ref&amp;gt;&lt;br /&gt;
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Iriyama、Ohya 和 Volovich 开发了线性量子图灵机 linear quantum Turing machine (LQTM) 模型。他们对具有混合状态并允许不可逆转换函数的量子图灵机进行了延伸。允许了在没有经典结果的情况下对量子的测量。&amp;lt;ref name=&amp;quot;:2&amp;quot;&amp;gt;{{cite journal|title=Classically-Controlled Quantum Computation|date=2007-04-04|pages=601–620|author1=Simon Perdrix|author2=Philippe Jorrand|volume=16|journal=Math. Struct. In Comp. Science|arxiv=quant-ph/0407008|doi=10.1017/S096012950600538X|issue=4}} also {{cite journal|title=Classically-Controlled Quantum Computation|author=Simon Perdrix and Philippe Jorrand|url=http://dcm-workshop.org.uk./2005/dcm-draft-proceedings.pdf|year=2006|pages=601–620|journal=Math. Struct. In Comp. Science|volume=16|doi=10.1017/S096012950600538X|issue=4|citeseerx=10.1.1.252.1823}}&amp;lt;/ref&amp;gt;&lt;br /&gt;
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Scott Aaronson 定义了具有后选择功能的量子图灵机，他证明了这种机器上的时间复杂度类 (PostBQP) 等于经典复杂度 PP。&amp;lt;ref name=&amp;quot;:3&amp;quot;&amp;gt;{{cite journal|last=Aaronson|first=Scott|year=2005|title=Quantum computing, postselection, and probabilistic polynomial-time|journal=[[Proceedings of the Royal Society A]]|volume=461|issue=2063|pages=3473–3482|doi=10.1098/rspa.2005.1546|bibcode = 2005RSPSA.461.3473A |arxiv=quant-ph/0412187}}  Preprint available at [https://arxiv.org/abs/quant-ph/0412187]&amp;lt;/ref&amp;gt;&lt;br /&gt;
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==参考文献==&lt;br /&gt;
&amp;lt;references/&amp;gt;&lt;br /&gt;
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==编者推荐==&lt;br /&gt;
===集智文章推荐===&lt;br /&gt;
*[https://swarma.org/?p=3652 神经网络与图灵机的复杂度博弈]&lt;br /&gt;
::1931年，天才数学家图灵提出了著名的图灵机模型，它奠定了人工智能的数学基础。1943年，麦克洛克 &amp;amp; 皮茨（McCulloch &amp;amp; Pitts）两人提出了著名的人工神经元模型，该模型一直沿用至今，它奠定了所有深度学习模型的基础。那么，这两个开山之作究竟是怎样一种相爱相杀的关系呢？天才数学家冯诺依曼指出，图灵机和神经元本质上虽然彼此等价，我们可以用图灵机模拟神经元，也可以用神经元模拟图灵机，但是它们却位于复杂度王国中的不同领地。神经网络代表了一大类擅长并行计算的复杂系统，它们自身的结构就构成了对自己最简洁的编码；而图灵机则代表了另一类以穿行方式计算的复杂系统，这些系统以通用图灵机作为复杂度的分水岭：一边，系统的行为可以被更短的代码描述；另一边，我们却无法绕过复杂度的沟壑。而先进的深度学习研究正在试图将这两类系统合成为一个：神经图灵机。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
===课程推荐===&lt;br /&gt;
*[https://campus.swarma.org/course/1155 图灵机]&lt;br /&gt;
::本课程将围绕图灵机，详细介绍图灵机的定义、图灵机的计算、图灵机框架的模拟、通用图灵机、以及图灵停机问题，说明算法的上界。&lt;br /&gt;
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&lt;br /&gt;
*[https://campus.swarma.org/course/3099 量子信息基础]&lt;br /&gt;
::量子力学作为现代物理学的两大核心理论之一，成功描述了微观物理体系的演化规律，奠定了现代信息科学特别是微电子学和光电子学的物理理论基础。量子概念的引入深刻地揭示了一系列与宏观体系截然不同的物理机制，在近年来逐渐发展出了包含量子通信、量子计算、量子模拟、量子测量等量子信息科学的全新研究领域和方向。&lt;br /&gt;
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本中文词条由[[tueryeye]]翻译，[[用户:薄荷|薄荷]]编辑，如有问题，欢迎在讨论页面留言。&lt;br /&gt;
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'''本词条内容源自wikipedia及公开资料，遵守 CC3.0协议。'''&lt;br /&gt;
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[[Category:图灵机]]&lt;br /&gt;
[[Category:量子复杂性理论]]&lt;/div&gt;</summary>
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		<title>玻尔兹曼分布</title>
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		<updated>2023-02-15T02:34:05Z</updated>

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&lt;div&gt;{{#seo:&lt;br /&gt;
|keywords=系统能态,粒子能级和速度,麦克斯韦-玻尔兹曼分布&lt;br /&gt;
|description=是一个概率分布或机率量测&lt;br /&gt;
}}&lt;br /&gt;
[[File:Exponential probability density.svg.png|upright=1.25|right|thumb|玻尔兹曼分布是指数分布。]]&lt;br /&gt;
[[File:Boltzmann distribution graph.svg.png|upright=1.25|right|thumb|玻尔兹曼因子 ''p&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;''&amp;amp;nbsp;/&amp;amp;nbsp;''p&amp;lt;sub&amp;gt;j&amp;lt;/sub&amp;gt;''（纵轴）作为温度 ''T''的函数，用于几个能量差 ''ε&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;''&amp;amp;nbsp;−&amp;amp;nbsp;''ε&amp;lt;sub&amp;gt;j&amp;lt;/sub&amp;gt;''。]]&lt;br /&gt;
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在统计力学和数学中，'''玻尔兹曼分布 Boltzmann distribution'''（也称为'''吉布斯分布 Gibbs distribution'''&amp;lt;ref name=&amp;quot;landau&amp;quot;&amp;gt;{{cite book | author=Landau, Lev Davidovich |author2=Lifshitz, Evgeny Mikhailovich |name-list-style=amp | title=Statistical Physics |volume=5 |series=Course of Theoretical Physics |edition=3 |origyear=1976 |year=1980 |place=Oxford |publisher=Pergamon Press|isbn=0-7506-3372-7}} Translated by J.B. Sykes and M.J. Kearsley. See section 28&amp;lt;/ref&amp;gt;)是一个概率分布或机率量测，它给出了一个系统处于某种量子态的概率，这个概率是该状态的能量和系统温度的函数。分布情况以下列形式表示:&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt;p_i \propto e^{-\frac{\varepsilon_i}{kT}}&amp;lt;/math&amp;gt; &lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
其中，{{mvar|p&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;}} 是系统处于状态{{mvar|i}}的概率, {{mvar|ε&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;}} 是该状态的能量，还有关于这个分布的一个常数 {{mvar|kT}} ，它是玻尔兹曼常数{{mvar|k}}和热力学温度 {{mvar|T}} 的乘积。符号 &amp;lt;math display=&amp;quot;inline&amp;quot;&amp;gt;\propto&amp;lt;/math&amp;gt;表示正比例(见附录中的比例常数)。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
这里的术语系统含义广泛，它可以从单个原子到宏观系统，如天然气储罐。正因为如此，波兹曼分布可以用来解决各种各样的问题。玻尔兹曼分布表明，能量较低的状态被占据的概率总是较高的。&lt;br /&gt;
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两种状态的概率之比被称为'''玻尔兹曼因子 Boltzmann factor'''，取决于两种状态的能量差:&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt;\frac{p_i}{p_j} = e^{\frac{\varepsilon_j - \varepsilon_i}{kT}}&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
波兹曼分布是根据[[路德维希·玻尔兹曼 Ludwig Edward Boltzmann]]1868年在研究统计力学中气体热平衡的时候首次提出的一个公式命名的。波尔兹曼的统计工作在他1877年的论文《论热力学第二基本定理与热平衡条件的概率计算之间的关系》中得到了体现。&amp;lt;ref&amp;gt;“On the Relationship between the Second Fundamental Theorem of the Mechanical Theory of Heat and Probability Calculations Regarding the Conditions for Thermal Equilibrium” Sitzungberichte der Kaiserlichen Akademie der Wissenschaften. Mathematisch-Naturwissen Classe. Abt. II, LXXVI 1877, pp 373-435 (Wien. Ber. 1877, 76:373-435). &amp;lt;/ref&amp;gt; 在玻尔兹曼分布被发明之后，[[约西亚·威拉德·吉布斯 Josiah Willard Gibbs]]充分地研究了它并在1902年提出了它的一般形式。&amp;lt;ref name=&amp;quot;gibbs&amp;quot;&amp;gt;{{cite book |last=Gibbs |first=Josiah Willard |title=Elementary Principles in Statistical Mechanics |year=1902 |publisher=Charles Scribner's Sons |location=New York}}&amp;lt;/ref&amp;gt;&lt;br /&gt;
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广义波兹曼分布是熵的统计力学定义（吉布斯熵公式  &amp;lt;math&amp;gt;S = -k_{\mathrm{B}}\sum_i p_i \log p_i&amp;lt;/math&amp;gt;）与熵的热力学定义（&amp;lt;math&amp;gt;d S = \frac{\delta Q_\text{rev}}{T}&amp;lt;/math&amp;gt;）等价的充要条件。&amp;lt;ref name=&amp;quot;:0&amp;quot;&amp;gt;{{cite journal |last1= Gao |first1= Xiang |last2= Gallicchio |first2= Emilio |first3= Adrian |last3= Roitberg  |date= 2019 |title= The generalized Boltzmann distribution is the only distribution in which the Gibbs-Shannon entropy equals the thermodynamic entropy |journal= The Journal of Chemical Physics|volume= 151|issue= 3|pages= 034113|doi= 10.1063/1.5111333|pmid= 31325924 |arxiv= 1903.02121 }}&amp;lt;/ref&amp;gt;&lt;br /&gt;
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值得一提的是，玻尔兹曼分布不应与[[麦克斯韦-玻尔兹曼分布]] Maxwell–Boltzmann distribution混淆。前者给出了系统处于某种状态的概率，作为该状态能量的函数；&amp;lt;ref name=&amp;quot;Atkins, P. W. 2010&amp;quot;&amp;gt;Atkins, P. W. (2010) Quanta, W. H. Freeman and Company, New York&amp;lt;/ref&amp;gt; 后者则是用于描述理想气体中的粒子速度。&lt;br /&gt;
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==分布==&lt;br /&gt;
&lt;br /&gt;
玻尔兹曼分布是一个[[概率分布]]，它给出了出于某种量子态处于某种能量和温度的时候的概率。&amp;lt;ref name=&amp;quot;McQuarrie, A. 2000&amp;quot;&amp;gt;McQuarrie, A. (2000) Statistical Mechanics, University Science Books, California&amp;lt;/ref&amp;gt;它被这样定义：&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt;&lt;br /&gt;
p_i=\frac{1}{Q}} {e^{- {\varepsilon}_i / k T}=\frac{e^{- {\varepsilon}_i / k T}}{\sum_{j=1}^{M}{e^{- {\varepsilon}_j / k T}}}&lt;br /&gt;
&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
其中 ''p&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;'' 是状态 i 的概率，''ε&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;'' 是状态 i 的能量，''k'' 是波兹曼常数，''T'' 是系统的温度，''M'' 是系统所能到达的所有量子态的数目。&amp;lt;ref name=&amp;quot;Atkins, P. W. 2010&amp;quot; /&amp;gt; &amp;lt;ref name=&amp;quot;McQuarrie, A. 2000&amp;quot; /&amp;gt;这里为了简洁美观，省略了''kT''周围的括弧。归一化的分母''Q''（被有些作者写为''Z''）是对于系统中所有量子态进行总和，此部分又被称为'''正则配分函数 canonical partition function'''。''&lt;br /&gt;
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所有量子态的概率之和为1.&lt;br /&gt;
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玻尔兹曼分布是使熵最大化的分布&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt;H(p_1,p_2,\cdots,p_M) = -\sum_{i=1}^{M} p_i\log_2 p_i&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
当&amp;lt;math&amp;gt;\sum {p_i {\varepsilon}_i} &amp;lt;/math&amp;gt;等于平均能量值时，玻尔兹曼分布是这种情况下能让熵最大化的分布。我们可以通过[[拉格朗日乘数法]]来证明。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
在知道量子态能量的情况下，这个配分函数可以被计算。对于原子来说，配分函数的值可以在NIST Atomic Spectra Database中找到。&amp;lt;ref name=&amp;quot;:1&amp;quot;&amp;gt;[http://physics.nist.gov/PhysRefData/ASD/levels_form.html NIST Atomic Spectra Database Levels Form] at nist.gov&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
玻尔兹曼分布指出，能量低的量子态总是有比能量高的量子态更高的概率被粒子占据。它同时也能让我们定量地比较两个量子态分布概率的关系。状态 i 和状态 j 的概率比为&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt;&lt;br /&gt;
{\frac{p_i}{p_j}}=e^{({\varepsilon}_j-{\varepsilon}_i) / k T}&lt;br /&gt;
&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
其中 p&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt; 是量子态 i 的概率， p&amp;lt;sub&amp;gt;j&amp;lt;/sub&amp;gt; 是量子态 j 的概率，ε&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt; 和 ε&amp;lt;sub&amp;gt;j&amp;lt;/sub&amp;gt; 分别是状态 i 和 j 的能量。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
玻尔兹曼分布通常被用来描述粒子的分布，比如原子或分子，在能量状态上的分布情况。如果我们有一个由许多粒子组成的系统，某个粒子处于量子态 i 的概率就等同于当我们从该系统中选择一个随机的粒子并观察它处于什么状态，发现它处于状态 i 的概率。这个概率等于量子态 i 的粒子数除以系统中粒子的总数，即那些占据量子态i的粒子的比例。&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt;&lt;br /&gt;
p_i={\frac{N_i}{N}}&lt;br /&gt;
&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
N&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt; 是位于量子态 i 的粒子数，N是系统中粒子的总数。我们可以用波兹曼分布来求出这个概率，它等于处于量子态i的粒子的比例。所以这个方程给出位于量子态 i 的粒子比例关于这个状态能量的函数&amp;lt;ref name=&amp;quot;Atkins, P. W. 2010&amp;quot; /&amp;gt;。&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt;&lt;br /&gt;
{\frac{N_i}{N}}={\frac{e^{- {\varepsilon}_i / k T}}{\sum_{j=1}^{M}{e^{- {\varepsilon}_j / k T}}}} &lt;br /&gt;
&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
这个等式对于光谱学来说很重要。在光谱中，我们期待能观察到一条原子或分子跃迁的谱线。&amp;lt;ref name=&amp;quot;Atkins, P. W. 2010&amp;quot; /&amp;gt;&amp;lt;ref name=&amp;quot;:2&amp;quot;&amp;gt;Atkins, P. W.; de Paula J. (2009) Physical Chemistry, 9th edition, Oxford University Press, Oxford, UK&amp;lt;/ref&amp;gt;在为了使这成为可能，必须有一些粒子处于第一个量子态，等待着发生跃迁。我们可以通过求第一态粒子的比例来满足这个条件。如果它可以忽略不计，那么在当前计算的温度下，则很难观察到这种跃迁。一般来说，处于第一状态的分子比例越大，意味着向第二状态跃迁的次数越多。&amp;lt;ref name=&amp;quot;:3&amp;quot;&amp;gt;Skoog, D. A.; Holler, F. J.; Crouch, S. R. (2006) Principles of Instrumental Analysis, Brooks/Cole, Boston, MA&amp;lt;/ref&amp;gt;这就产生了一条更强的谱线。然而，还有其他因素影响谱线的强度，例如它是否是被允许的跃迁还是被禁止的跃迁。&lt;br /&gt;
&lt;br /&gt;
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玻尔兹曼分布与机器学习中常用的[[归一化指数函数]]（Softmax 函数）有关。&lt;br /&gt;
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==统计力学==&lt;br /&gt;
&lt;br /&gt;
当独立的（或者几乎独立的）固定体系处于统计力学热平衡状态时，玻尔兹曼分布就会出现。最普遍的情况是概率分布的正则系综，但也有一些特殊的情况（从正则系综衍生）也显示了不同形式的玻尔兹曼分布:&lt;br /&gt;
&lt;br /&gt;
====正则系综（一般情况）====&lt;br /&gt;
&lt;br /&gt;
正则系综模型给出了在一个封闭固定体积，带有热浴的热平衡系统中的各种可能状态的概率。我们称正则系综为一个玻尔兹曼概率分布。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
====子系统状态的统计频率（在一个无交互的集合中）====&lt;br /&gt;
&lt;br /&gt;
当系统是一个较小子系统的许多非交互副本的集合时，有时我们需要在某个子系统集合中找到某个子系统的统计频率。当应用于这样一个集合时，这个子系统的正则系综具有可分离性: 只要不相互作用的子系统的组成是固定的，那么每个子系统的状态都是独立于其他子系统的，它们也拥有自己的正则系综。因此，子系统状态的期望统计频率分布形式是玻尔兹曼分布。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
====麦克斯韦-玻尔兹曼统计中的经典气体系统（非相互作用粒子系统）====&lt;br /&gt;
&lt;br /&gt;
在粒子系统中，许多粒子共享同一空间，并且相互之间有规律地改变位置; 它们所占据的单粒子状态空间是一个共享空间。[[麦克斯韦-玻尔兹曼统计]]给出了在一个给定的单粒子态，在一个处于平衡状态的非相互作用粒子的经典气体中所发现的粒子的预期数量。这个预期的数量分布具有玻尔兹曼分布形式。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
虽然这些案例有很多相似之处，但是当关键假设发生变化时，我们需要对它们以不同的方式进行归纳总结，因此区分它们是有帮助的:&lt;br /&gt;
&lt;br /&gt;
*当一个系统在能量交换和粒子交换方面都处于热力学平衡时，固定组成的要求就放宽了。这时我们就得到了一个[[巨正则系综]] grand canonical ensemble而不是正则系综。另一方面，如果成分和能量都是固定的，则可以使用[[微正则系综]] microcanonical ensemble。&lt;br /&gt;
&lt;br /&gt;
*如果集合中的子系统确实相互交互，则子系统状态的预期频率不再遵循玻尔兹曼分布，甚至可能没有解析解。&amp;lt;ref name=&amp;quot;:4&amp;quot;&amp;gt;A classic example of this is magnetic ordering. Systems of non-interacting spins show paramagnetic behaviour that can be understood with a single-particle canonical ensemble (resulting in the Brillouin function). Systems of ''interacting'' spins can show much more complex behaviour such as ferromagnetism or antiferromagnetism.&amp;lt;/ref&amp;gt;但是当整个系统是独立的并且处于热平衡状态，则正则系综仍然可以应用于作为一个整体考虑。&lt;br /&gt;
&lt;br /&gt;
*对于处于平衡状态的非相互作用粒子的量子气体，在给定的单粒子状态中发现的粒子数量并不遵循[[麦克斯韦-玻尔兹曼统计]]。并且正则系综中的量子气体没有简单的封闭表达式。在巨正则系综中，量子气体的统计分布状态由[[费米-狄拉克统计]] Fermi–Dirac statistics或[[玻色-爱因斯坦统计]] Bose–Einstein statistics来描述，具体则取决于该粒子是费米子 fermion还是玻色子 boson。&lt;br /&gt;
&lt;br /&gt;
&amp;lt;br&amp;gt;&lt;br /&gt;
&lt;br /&gt;
==数学==&lt;br /&gt;
&lt;br /&gt;
在更一般的数学环境中，玻尔兹曼分布也被称为'''吉布斯量度 Gibbs measure'''。在[[统计学]]和[[机器学习]]中，它被称为对数线性回归。在[[深度学习]]中，玻尔兹曼分布被用于随机神经网络的抽样分布，如玻尔兹曼机 [Boltzmann machine、受限玻尔兹曼机 Restricted Boltzmann machine、基于能量的模型 Energy-Based models和深度波茨曼机 Deep Boltzmann Machine。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==经济==&lt;br /&gt;
&lt;br /&gt;
在经济学中，玻尔兹曼分布被用来分配排放交易中的许可。&amp;lt;ref name=&amp;quot;Park, J.-W. 2012&amp;quot;&amp;gt;Park, J.-W., Kim, C. U. and Isard, W. (2012) Permit allocation in emissions trading using the Boltzmann distribution. Physica A 391: 4883–4890&amp;lt;/ref&amp;gt;&amp;lt;ref name=&amp;quot;:5&amp;quot;&amp;gt;[http://www.technologyreview.com/view/425051/the-thorny-problem-of-fair-allocation/ The Thorny Problem Of Fair Allocation]. ''Technology Review'' blog. August 17, 2011. Cites and summarizes Park, Kim and Isard (2012).&amp;lt;/ref&amp;gt;使用玻尔兹曼分布的新分配方法可以创造出在多个国家之间最可能的、自然的和无偏见的排放许可分配。这种新方法简单而通用，在经济和环保中有很大的应用潜力。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
玻尔兹曼分布与多项逻辑回归模型具有相同的形式。在Daniel McFadden登将它与随机效用最大化联系起来之后，成为了大家所熟知的一种离散选择模型。&lt;br /&gt;
&lt;br /&gt;
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==参考文献==&lt;br /&gt;
&lt;br /&gt;
&amp;lt;references /&amp;gt;&lt;br /&gt;
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==编者推荐==&lt;br /&gt;
[[File:全同粒子与统计.jpg|300px|thumb|right|课程：[https://campus.swarma.org/course/3095 全同粒子与统计]]]&lt;br /&gt;
===集智课程===&lt;br /&gt;
====[https://campus.swarma.org/course/3095 全同粒子与统计]====&lt;br /&gt;
在量子力学中，全同粒子具有不可区分性；粒子体系的哈密顿量具有交换不变性。两个粒子交换位置后，虽然哈密顿量具有不变性，但他们的波函数可以区分出两种情况，即对称波函数和反对称波函数，对应于玻色子和费米子。量子力学中的全同粒子不可分辨，两粒子互换后，与原状态没有区别，不表示新的微观态。微观态计数方法的不同，是经典统计和量子统计的重大区别。&lt;br /&gt;
&lt;br /&gt;
金潮渊老师讲解了光场量子化情形下，光子计数的波动范围遵循一定的统计规律。在可分辨粒子、全同费米子、全同玻色子情况下，微观粒子的三种统计分布，即麦克斯韦-玻尔兹曼统计、玻色-爱因斯坦统计、费米-狄拉克统计。在此基础上，引入狄拉克符号、表象变换、幺正算符等量子力学基本概念和HBT实验即第一个只能用量子理论解释的量子光学实验。&lt;br /&gt;
&lt;br /&gt;
&amp;lt;br&amp;gt;&lt;br /&gt;
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===集智文章===&lt;br /&gt;
*[https://swarma.org/?p=14945 进展：变分自回归神经网络求解统计力学问题]&lt;br /&gt;
*[https://swarma.org/?p=857 小装置，大未来：量子机器学习1.0时代]&lt;br /&gt;
*[https://swarma.org/?p=4444 量子纠缠：从量子物质态到深度学习]&lt;br /&gt;
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|keywords=系统能态,粒子能级和速度,麦克斯韦-玻尔兹曼分布&lt;br /&gt;
|description=是一个概率分布或机率量测&lt;br /&gt;
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[[File:Exponential probability density.svg.png|upright=1.25|right|thumb|玻尔兹曼分布是指数分布。]]&lt;br /&gt;
[[File:Boltzmann distribution graph.svg.png|upright=1.25|right|thumb|玻尔兹曼因子 ''p&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;''&amp;amp;nbsp;/&amp;amp;nbsp;''p&amp;lt;sub&amp;gt;j&amp;lt;/sub&amp;gt;''（纵轴）作为温度 ''T''的函数，用于几个能量差 ''ε&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;''&amp;amp;nbsp;−&amp;amp;nbsp;''ε&amp;lt;sub&amp;gt;j&amp;lt;/sub&amp;gt;''。]]&lt;br /&gt;
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在统计力学和数学中，'''玻尔兹曼分布 Boltzmann distribution'''（也称为'''吉布斯分布 Gibbs distribution'''&amp;lt;ref name=&amp;quot;landau&amp;quot;&amp;gt;{{cite book | author=Landau, Lev Davidovich |author2=Lifshitz, Evgeny Mikhailovich |name-list-style=amp | title=Statistical Physics |volume=5 |series=Course of Theoretical Physics |edition=3 |origyear=1976 |year=1980 |place=Oxford |publisher=Pergamon Press|isbn=0-7506-3372-7}} Translated by J.B. Sykes and M.J. Kearsley. See section 28&amp;lt;/ref&amp;gt;)是一个概率分布或机率量测，它给出了一个系统处于某种量子态的概率，这个概率是该状态的能量和系统温度的函数。分布情况以下列形式表示:&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt;p_i \propto e^{-\frac{\varepsilon_i}{kT}}&amp;lt;/math&amp;gt; &lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
其中，{{mvar|p&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;}} 是系统处于状态{{mvar|i}}的概率, {{mvar|ε&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;}} 是该状态的能量，还有关于这个分布的一个常数 {{mvar|kT}} ，它是玻尔兹曼常数{{mvar|k}}和热力学温度 {{mvar|T}} 的乘积。符号 &amp;lt;math display=&amp;quot;inline&amp;quot;&amp;gt;\propto&amp;lt;/math&amp;gt;表示正比例(见附录中的比例常数)。&lt;br /&gt;
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&lt;br /&gt;
这里的术语系统含义广泛，它可以从单个原子到宏观系统，如天然气储罐。正因为如此，波兹曼分布可以用来解决各种各样的问题。玻尔兹曼分布表明，能量较低的状态被占据的概率总是较高的。&lt;br /&gt;
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两种状态的概率之比被称为'''玻尔兹曼因子 Boltzmann factor'''，取决于两种状态的能量差:&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt;\frac{p_i}{p_j} = e^{\frac{\varepsilon_j - \varepsilon_i}{kT}}&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
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波兹曼分布是根据[[路德维希·玻尔兹曼 Ludwig Edward Boltzmann]]1868年在研究统计力学中气体热平衡的时候首次提出的一个公式命名的。波尔兹曼的统计工作在他1877年的论文《论热力学第二基本定理与热平衡条件的概率计算之间的关系》中得到了体现。&amp;lt;ref&amp;gt;“On the Relationship between the Second Fundamental Theorem of the Mechanical Theory of Heat and Probability Calculations Regarding the Conditions for Thermal Equilibrium” Sitzungberichte der Kaiserlichen Akademie der Wissenschaften. Mathematisch-Naturwissen Classe. Abt. II, LXXVI 1877, pp 373-435 (Wien. Ber. 1877, 76:373-435). &amp;lt;/ref&amp;gt; 在玻尔兹曼分布被发明之后，[[约西亚·威拉德·吉布斯 Josiah Willard Gibbs]]充分地研究了它并在1902年提出了它的一般形式。&amp;lt;ref name=&amp;quot;gibbs&amp;quot;&amp;gt;{{cite book |last=Gibbs |first=Josiah Willard |title=Elementary Principles in Statistical Mechanics |year=1902 |publisher=Charles Scribner's Sons |location=New York}}&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
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广义波兹曼分布是熵的统计力学定义（吉布斯熵公式  &amp;lt;math&amp;gt;S = -k_{\mathrm{B}}\sum_i p_i \log p_i&amp;lt;/math&amp;gt;）与熵的热力学定义（&amp;lt;math&amp;gt;d S = \frac{\delta Q_\text{rev}}{T}&amp;lt;/math&amp;gt;）等价的充要条件。&amp;lt;ref name=&amp;quot;:0&amp;quot;&amp;gt;{{cite journal |last1= Gao |first1= Xiang |last2= Gallicchio |first2= Emilio |first3= Adrian |last3= Roitberg  |date= 2019 |title= The generalized Boltzmann distribution is the only distribution in which the Gibbs-Shannon entropy equals the thermodynamic entropy |journal= The Journal of Chemical Physics|volume= 151|issue= 3|pages= 034113|doi= 10.1063/1.5111333|pmid= 31325924 |arxiv= 1903.02121 }}&amp;lt;/ref&amp;gt;&lt;br /&gt;
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值得一提的是，玻尔兹曼分布不应与[[麦克斯韦-玻尔兹曼分布]] Maxwell–Boltzmann distribution混淆。前者给出了系统处于某种状态的概率，作为该状态能量的函数；&amp;lt;ref name=&amp;quot;Atkins, P. W. 2010&amp;quot;&amp;gt;Atkins, P. W. (2010) Quanta, W. H. Freeman and Company, New York&amp;lt;/ref&amp;gt; 后者则是用于描述理想气体中的粒子速度。&lt;br /&gt;
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==分布==&lt;br /&gt;
&lt;br /&gt;
玻尔兹曼分布是一个[[概率分布]]，它给出了出于某种量子态处于某种能量和温度的时候的概率。&amp;lt;ref name=&amp;quot;McQuarrie, A. 2000&amp;quot;&amp;gt;McQuarrie, A. (2000) Statistical Mechanics, University Science Books, California&amp;lt;/ref&amp;gt;它被这样定义：&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt;&lt;br /&gt;
p_i=\frac{1}{Q}} {e^{- {\varepsilon}_i / k T}=\frac{e^{- {\varepsilon}_i / k T}}{\sum_{j=1}^{M}{e^{- {\varepsilon}_j / k T}}}&lt;br /&gt;
&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
其中 ''p&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;'' 是状态 i 的概率，''ε&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;'' 是状态 i 的能量，''k'' 是波兹曼常数，''T'' 是系统的温度，''M'' 是系统所能到达的所有量子态的数目。&amp;lt;ref name=&amp;quot;Atkins, P. W. 2010&amp;quot; /&amp;gt; &amp;lt;ref name=&amp;quot;McQuarrie, A. 2000&amp;quot; /&amp;gt;这里为了简洁美观，省略了''kT''周围的括弧。归一化的分母''Q''（被有些作者写为''Z''）是对于系统中所有量子态进行总和，此部分又被称为'''正则配分函数 canonical partition function'''。''&lt;br /&gt;
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所有量子态的概率之和为1.&lt;br /&gt;
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玻尔兹曼分布是使熵最大化的分布&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt;H(p_1,p_2,\cdots,p_M) = -\sum_{i=1}^{M} p_i\log_2 p_i&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
当&amp;lt;math&amp;gt;\sum {p_i {\varepsilon}_i} &amp;lt;/math&amp;gt;等于平均能量值时，玻尔兹曼分布是这种情况下能让熵最大化的分布。我们可以通过[[拉格朗日乘数法]]来证明。&lt;br /&gt;
&lt;br /&gt;
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在知道量子态能量的情况下，这个配分函数可以被计算。对于原子来说，配分函数的值可以在NIST Atomic Spectra Database中找到。&amp;lt;ref name=&amp;quot;:1&amp;quot;&amp;gt;[http://physics.nist.gov/PhysRefData/ASD/levels_form.html NIST Atomic Spectra Database Levels Form] at nist.gov&amp;lt;/ref&amp;gt;&lt;br /&gt;
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玻尔兹曼分布指出，能量低的量子态总是有比能量高的量子态更高的概率被粒子占据。它同时也能让我们定量地比较两个量子态分布概率的关系。状态 i 和状态 j 的概率比为&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt;&lt;br /&gt;
{\frac{p_i}{p_j}}=e^{({\varepsilon}_j-{\varepsilon}_i) / k T}&lt;br /&gt;
&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
其中 p&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt; 是量子态 i 的概率， p&amp;lt;sub&amp;gt;j&amp;lt;/sub&amp;gt; 是量子态 j 的概率，ε&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt; 和 ε&amp;lt;sub&amp;gt;j&amp;lt;/sub&amp;gt; 分别是状态 i 和 j 的能量。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
玻尔兹曼分布通常被用来描述粒子的分布，比如原子或分子，在能量状态上的分布情况。如果我们有一个由许多粒子组成的系统，某个粒子处于量子态 i 的概率就等同于当我们从该系统中选择一个随机的粒子并观察它处于什么状态，发现它处于状态 i 的概率。这个概率等于量子态 i 的粒子数除以系统中粒子的总数，即那些占据量子态i的粒子的比例。&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt;&lt;br /&gt;
p_i={\frac{N_i}{N}}&lt;br /&gt;
&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
N&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt; 是位于量子态 i 的粒子数，N是系统中粒子的总数。我们可以用波兹曼分布来求出这个概率，它等于处于量子态i的粒子的比例。所以这个方程给出位于量子态 i 的粒子比例关于这个状态能量的函数&amp;lt;ref name=&amp;quot;Atkins, P. W. 2010&amp;quot; /&amp;gt;。&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt;&lt;br /&gt;
{\frac{N_i}{N}}={\frac{e^{- {\varepsilon}_i / k T}}{\sum_{j=1}^{M}{e^{- {\varepsilon}_j / k T}}}} &lt;br /&gt;
&amp;lt;/math&amp;gt;&lt;br /&gt;
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&lt;br /&gt;
这个等式对于光谱学来说很重要。在光谱中，我们期待能观察到一条原子或分子跃迁的谱线。&amp;lt;ref name=&amp;quot;Atkins, P. W. 2010&amp;quot; /&amp;gt;&amp;lt;ref name=&amp;quot;:2&amp;quot;&amp;gt;Atkins, P. W.; de Paula J. (2009) Physical Chemistry, 9th edition, Oxford University Press, Oxford, UK&amp;lt;/ref&amp;gt;在为了使这成为可能，必须有一些粒子处于第一个量子态，等待着发生跃迁。我们可以通过求第一态粒子的比例来满足这个条件。如果它可以忽略不计，那么在当前计算的温度下，则很难观察到这种跃迁。一般来说，处于第一状态的分子比例越大，意味着向第二状态跃迁的次数越多。&amp;lt;ref name=&amp;quot;:3&amp;quot;&amp;gt;Skoog, D. A.; Holler, F. J.; Crouch, S. R. (2006) Principles of Instrumental Analysis, Brooks/Cole, Boston, MA&amp;lt;/ref&amp;gt;这就产生了一条更强的谱线。然而，还有其他因素影响谱线的强度，例如它是否是被允许的跃迁还是被禁止的跃迁。&lt;br /&gt;
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玻尔兹曼分布与机器学习中常用的[[归一化指数函数]]（Softmax 函数）有关。&lt;br /&gt;
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==统计力学==&lt;br /&gt;
&lt;br /&gt;
当独立的（或者几乎独立的）固定体系处于统计力学热平衡状态时，玻尔兹曼分布就会出现。最普遍的情况是概率分布的正则系综，但也有一些特殊的情况（从正则系综衍生）也显示了不同形式的玻尔兹曼分布:&lt;br /&gt;
&lt;br /&gt;
====正则系综（一般情况）====&lt;br /&gt;
&lt;br /&gt;
正则系综模型给出了在一个封闭固定体积，带有热浴的热平衡系统中的各种可能状态的概率。我们称正则系综为一个玻尔兹曼概率分布。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
====子系统状态的统计频率（在一个无交互的集合中）====&lt;br /&gt;
&lt;br /&gt;
当系统是一个较小子系统的许多非交互副本的集合时，有时我们需要在某个子系统集合中找到某个子系统的统计频率。当应用于这样一个集合时，这个子系统的正则系综具有可分离性: 只要不相互作用的子系统的组成是固定的，那么每个子系统的状态都是独立于其他子系统的，它们也拥有自己的正则系综。因此，子系统状态的期望统计频率分布形式是玻尔兹曼分布。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
====麦克斯韦-玻尔兹曼统计中的经典气体系统（非相互作用粒子系统）====&lt;br /&gt;
&lt;br /&gt;
在粒子系统中，许多粒子共享同一空间，并且相互之间有规律地改变位置; 它们所占据的单粒子状态空间是一个共享空间。[[麦克斯韦-玻尔兹曼统计]]给出了在一个给定的单粒子态，在一个处于平衡状态的非相互作用粒子的经典气体中所发现的粒子的预期数量。这个预期的数量分布具有玻尔兹曼分布形式。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
虽然这些案例有很多相似之处，但是当关键假设发生变化时，我们需要对它们以不同的方式进行归纳总结，因此区分它们是有帮助的:&lt;br /&gt;
&lt;br /&gt;
*当一个系统在能量交换和粒子交换方面都处于热力学平衡时，固定组成的要求就放宽了。这时我们就得到了一个[[巨正则系综]] grand canonical ensemble而不是正则系综。另一方面，如果成分和能量都是固定的，则可以使用[[微正则系综]] microcanonical ensemble。&lt;br /&gt;
&lt;br /&gt;
*如果集合中的子系统确实相互交互，则子系统状态的预期频率不再遵循玻尔兹曼分布，甚至可能没有解析解。&amp;lt;ref name=&amp;quot;:4&amp;quot;&amp;gt;A classic example of this is magnetic ordering. Systems of non-interacting spins show paramagnetic behaviour that can be understood with a single-particle canonical ensemble (resulting in the Brillouin function). Systems of ''interacting'' spins can show much more complex behaviour such as ferromagnetism or antiferromagnetism.&amp;lt;/ref&amp;gt;但是当整个系统是独立的并且处于热平衡状态，则正则系综仍然可以应用于作为一个整体考虑。&lt;br /&gt;
&lt;br /&gt;
*对于处于平衡状态的非相互作用粒子的量子气体，在给定的单粒子状态中发现的粒子数量并不遵循[[麦克斯韦-玻尔兹曼统计]]。并且正则系综中的量子气体没有简单的封闭表达式。在巨正则系综中，量子气体的统计分布状态由[[费米-狄拉克统计]] Fermi–Dirac statistics或[[玻色-爱因斯坦统计]] Bose–Einstein statistics来描述，具体则取决于该粒子是费米子 fermion还是玻色子 boson。&lt;br /&gt;
&lt;br /&gt;
&amp;lt;br&amp;gt;&lt;br /&gt;
&lt;br /&gt;
==数学==&lt;br /&gt;
&lt;br /&gt;
在更一般的数学环境中，玻尔兹曼分布也被称为'''吉布斯量度 Gibbs measure'''。在[[统计学]]和[[机器学习]]中，它被称为对数线性回归。在[[深度学习]]中，玻尔兹曼分布被用于随机神经网络的抽样分布，如玻尔兹曼机 [Boltzmann machine、受限玻尔兹曼机 Restricted Boltzmann machine、基于能量的模型 Energy-Based models和深度波茨曼机 Deep Boltzmann Machine。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==经济==&lt;br /&gt;
&lt;br /&gt;
在经济学中，玻尔兹曼分布被用来分配排放交易中的许可。&amp;lt;ref name=&amp;quot;Park, J.-W. 2012&amp;quot;&amp;gt;Park, J.-W., Kim, C. U. and Isard, W. (2012) Permit allocation in emissions trading using the Boltzmann distribution. Physica A 391: 4883–4890&amp;lt;/ref&amp;gt;&amp;lt;ref name=&amp;quot;:5&amp;quot;&amp;gt;[http://www.technologyreview.com/view/425051/the-thorny-problem-of-fair-allocation/ The Thorny Problem Of Fair Allocation]. ''Technology Review'' blog. August 17, 2011. Cites and summarizes Park, Kim and Isard (2012).&amp;lt;/ref&amp;gt;使用玻尔兹曼分布的新分配方法可以创造出在多个国家之间最可能的、自然的和无偏见的排放许可分配。这种新方法简单而通用，在经济和环保中有很大的应用潜力。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
玻尔兹曼分布与多项逻辑回归模型具有相同的形式。在Daniel McFadden登将它与随机效用最大化联系起来之后，成为了大家所熟知的一种离散选择模型。&lt;br /&gt;
&lt;br /&gt;
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==参考文献==&lt;br /&gt;
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&amp;lt;references /&amp;gt;&lt;br /&gt;
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==编者推荐==&lt;br /&gt;
[[File:全同粒子与统计.jpg|300px|thumb|right|课程：[https://campus.swarma.org/course/3095 全同粒子与统计]]]&lt;br /&gt;
===集智课程===&lt;br /&gt;
====[https://campus.swarma.org/course/3095 全同粒子与统计]====&lt;br /&gt;
在量子力学中，全同粒子具有不可区分性；粒子体系的哈密顿量具有交换不变性。两个粒子交换位置后，虽然哈密顿量具有不变性，但他们的波函数可以区分出两种情况，即对称波函数和反对称波函数，对应于玻色子和费米子。量子力学中的全同粒子不可分辨，两粒子互换后，与原状态没有区别，不表示新的微观态。微观态计数方法的不同，是经典统计和量子统计的重大区别。&lt;br /&gt;
&lt;br /&gt;
金潮渊老师讲解了光场量子化情形下，光子计数的波动范围遵循一定的统计规律。在可分辨粒子、全同费米子、全同玻色子情况下，微观粒子的三种统计分布，即麦克斯韦-玻尔兹曼统计、玻色-爱因斯坦统计、费米-狄拉克统计。在此基础上，引入狄拉克符号、表象变换、幺正算符等量子力学基本概念和HBT实验即第一个只能用量子理论解释的量子光学实验。&lt;br /&gt;
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===集智文章===&lt;br /&gt;
*[https://swarma.org/?p=14945 进展：变分自回归神经网络求解统计力学问题]&lt;br /&gt;
*[https://swarma.org/?p=857 小装置，大未来：量子机器学习1.0时代]&lt;br /&gt;
*[https://swarma.org/?p=4444 量子纠缠：从量子物质态到深度学习]&lt;br /&gt;
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本中文词条由[[用|tueryeye]]翻译和审校，[[用户:薄荷|薄荷]]编辑，如有问题，欢迎在讨论页面留言。&lt;br /&gt;
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'''本词条内容源自wikipedia及公开资料，遵守 CC3.0协议。'''&lt;br /&gt;
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[[Category:统计力学]]&lt;/div&gt;</summary>
		<author><name>Tueryeye</name></author>
	</entry>
	<entry>
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		<title>量子图灵机</title>
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		<updated>2022-03-31T04:33:28Z</updated>

		<summary type="html">&lt;p&gt;Tueryeye：阅读三遍&lt;/p&gt;
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&lt;div&gt;此词条由tueryeye翻译审校，未经专家审核，带来阅读不便，请见谅。{{Short description|Model of quantum computation}}&lt;br /&gt;
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{{Turing}}&lt;br /&gt;
&lt;br /&gt;
&amp;lt;!-- Basic definition --&amp;gt;&lt;br /&gt;
== 基础定义 ==&lt;br /&gt;
A '''quantum Turing machine''' ('''QTM''') or '''universal quantum computer''' is an [[abstract machine]] used to model the effects of a [[quantum computer]].  It provides a simple model that captures all of the power of quantum computation—that is, any [[quantum algorithm]] can be expressed formally as a particular quantum Turing machine. However, the computationally equivalent [[quantum circuit]] is a more common model.&amp;lt;ref name=&amp;quot;equivalence&amp;quot;&amp;gt;{{cite conference|author=[[Andrew Yao]]|title=Quantum circuit complexity|conference=34th Annual Symposium on Foundations of Computer Science|pages=352–361|year=1993}}&amp;lt;/ref&amp;gt;&amp;lt;ref name=&amp;quot;newequivalence&amp;quot;&amp;gt;{{cite arXiv|eprint=1808.01701|author1=Abel Molina|author2=John Watrous|author-link2=John Watrous (computer scientist)|title=Revisiting the simulation of quantum Turing machines by quantum circuits|date=2018|class=cs.CC}}&amp;lt;/ref&amp;gt;&lt;br /&gt;
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量子图灵机'''quantum Turing machine''' (QTM)又称为通用量子计算机是一种用来模拟量子计算机效果的抽象机器。尽管说提供等效计算能力的量子电路是一种更常用的模型，但是量子图灵机'''quantum Turing machine''' 是一个简单但能展现出量子计算的所有威力的模型。就像经典图灵机可以模拟人类所能进行的任何计算过程一样，量子图灵机可以描述任何量子算法。&amp;lt;ref name=&amp;quot;equivalence&amp;quot; /&amp;gt;&amp;lt;ref name=&amp;quot;newequivalence&amp;quot; /&amp;gt;&lt;br /&gt;
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&amp;lt;!-- Relation to classical computation --&amp;gt;&lt;br /&gt;
&lt;br /&gt;
== 与经典计算的关系 ==&lt;br /&gt;
Quantum Turing machines can be related to classical and probabilistic Turing machines in a framework based on [[Stochastic matrix|transition matrices]]. That is, a matrix can be specified whose product with the matrix representing a classical or probabilistic machine provides the quantum probability matrix representing the quantum machine. This was shown by [[Lance Fortnow]].&amp;lt;ref name=&amp;quot;transition&amp;quot;&amp;gt;{{cite journal|author=Fortnow|first=Lance|author-link=Lance Fortnow|year=2003|title=One Complexity Theorist's View of Quantum Computing|url=|journal=Theoretical Computer Science|volume=292|issue=3|pages=597–610|doi=10.1016/S0304-3975(01)00377-2|via=|arxiv=quant-ph/0003035}}&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
通过过渡矩阵[[Stochastic matrix|transition matrices]]，量子图灵机可以与经典图灵机和概率图灵机相关联。Lance Fortnow证明，量子图灵机的量子概率矩阵可以被拆解成是指定矩阵与经典或概率图灵机的矩阵的乘积。&amp;lt;ref name=&amp;quot;transition&amp;quot; /&amp;gt;&lt;br /&gt;
&lt;br /&gt;
== 非正式草图定义 ==&lt;br /&gt;
{{Unsolved|physics|Is a [[universal quantum computer]] sufficient to [[Algorithmic efficiency|efficiently]] [[Dynamical simulation|simulate]] an arbitrary physical system?}}&lt;br /&gt;
&lt;br /&gt;
A way of understanding the quantum Turing machine (QTM) is that it generalizes the classical [[Turing machine]] (TM) in the same way that the [[quantum finite automaton]] (QFA) generalizes the [[deterministic finite automaton]] (DFA).  In essence, the internal states of a classical TM are replaced by [[pure state|pure]] or [[mixed quantum state|mixed states]] in a Hilbert space; the transition function is replaced by a collection of [[unitary matrix|unitary matrices]] that map the Hilbert space to itself.&amp;lt;ref name=&amp;quot;Deutsch1985&amp;quot; /&amp;gt;&lt;br /&gt;
&lt;br /&gt;
我们可以通过类比确定有限自动机[[deterministic finite automaton]]到量子有限自动机[[quantum finite automaton]]的转化来理解经典图灵机到量子图灵机'''quantum Turing machine'''的转化。 他们的差异在于，经典图灵机讨论的状态被推广到了Hilbert空间中。Hilbert空间是'''完备的内积空间'''，是有限维欧几里得空间的一个推广。它不局限于实数的情形和有限的维数，但又不失完备性。在量子图灵机中转换函数被一组映射Hilbert空间到自身的酉矩阵[[unitary matrix|unitary matrices]]取代。&amp;lt;ref name=&amp;quot;Deutsch1985&amp;quot; /&amp;gt;&lt;br /&gt;
&lt;br /&gt;
经典图灵机的诞生是因为图灵想用机器来模拟用纸笔进行数学运算的过程，这样的过程可以被看作下列两种简单的动作：&lt;br /&gt;
&lt;br /&gt;
* 在纸带上写上或删除某个符号；&lt;br /&gt;
* 把笔尖从纸的一处移动到另一处；&lt;br /&gt;
&lt;br /&gt;
现在我们假设有一条纸带无限长，并且被划分为一个接一个的小格子，每个格子上包含一个来自有限字母表的符号，字母表中有一个特殊的符号表示空白。假设我们有一个执笔机器又称为读写头（'''HEAD），'''它本身也可以具有一个状态。就像人今天可能因为某件事心情很好，也可能因为另一件事情很抑郁一样，它的状态会随着它的遭遇所改变。更重要的是执笔机器当前关注的纸上的某个位置的符号和当前的状态决定了下一步的动作。在遇到停止状态&amp;lt;math&amp;gt;F&amp;lt;/math&amp;gt;之前执笔机器可以&lt;br /&gt;
&lt;br /&gt;
* 1. 写入（替换）或擦除当前符号；&lt;br /&gt;
* 2. 移动 '''HEAD'''， 'L'向左一步， 'R'向右一步或者'N'不移动；&lt;br /&gt;
* 3. 保持当前状态或者转到另一状态。&lt;br /&gt;
&lt;br /&gt;
That is, a classical Turing machine is described by  a 7-[[tuple]] &amp;lt;math&amp;gt;M = \langle Q, \Gamma, b, \Sigma, \delta, q_0, F \rangle&amp;lt;/math&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
总的来说，经典图灵机可以被一个七元有序组所描述，&amp;lt;math&amp;gt;M = \langle Q, \Gamma, b, \Sigma, \delta, q_0, F \rangle&amp;lt;/math&amp;gt;。&lt;br /&gt;
&lt;br /&gt;
* The set of states &amp;lt;math&amp;gt;Q&amp;lt;/math&amp;gt; is replaced by a [[Hilbert space]].&lt;br /&gt;
&lt;br /&gt;
* The tape alphabet symbols &amp;lt;math&amp;gt;\Gamma&amp;lt;/math&amp;gt; are likewise replaced by a Hilbert space (usually a different Hilbert space than the set of states).&lt;br /&gt;
&lt;br /&gt;
* The blank symbol &amp;lt;math&amp;gt;b \in \Gamma&amp;lt;/math&amp;gt; corresponds to the zero-vector.&lt;br /&gt;
&lt;br /&gt;
* The input and output symbols &amp;lt;math&amp;gt;\Sigma&amp;lt;/math&amp;gt; are usually taken as a discrete set, as in the classical system; thus, neither the input nor output to a quantum machine need be a quantum system itself.&lt;br /&gt;
&lt;br /&gt;
* The [[State transition system|transition function]] &amp;lt;math&amp;gt;\delta : \Sigma \times Q  \otimes \Gamma \rightarrow \Sigma \times Q \otimes \Gamma \times \{L,R\}&amp;lt;/math&amp;gt; is a generalization of a [[transition monoid]], and is understood to be a collection of [[unitary matrix|unitary matrices]] that are [[automorphism]]s of the Hilbert space &amp;lt;math&amp;gt;Q&amp;lt;/math&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
* The initial state &amp;lt;math&amp;gt;q_0 \in Q&amp;lt;/math&amp;gt; may be either a [[mixed quantum state|mixed state]] or a [[pure state]].&lt;br /&gt;
&lt;br /&gt;
* The set &amp;lt;math&amp;gt;F&amp;lt;/math&amp;gt; of ''final'' or ''accepting states'' is a subspace of the Hilbert space &amp;lt;math&amp;gt;Q&amp;lt;/math&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
* &amp;lt;math&amp;gt;Q&amp;lt;/math&amp;gt; 为被推广到了Hilbert空间的状态集；&lt;br /&gt;
* &amp;lt;math&amp;gt;\Gamma&amp;lt;/math&amp;gt; 是输入字母表；&lt;br /&gt;
* &amp;lt;math&amp;gt;b \in \Gamma&amp;lt;/math&amp;gt; 为''空白符''，也是唯一允许出现无限次的字符；&lt;br /&gt;
* 输入和输出符号 &amp;lt;math&amp;gt;\Sigma&amp;lt;/math&amp;gt;通常是一个离散集。和经典图灵机的输入输出符号一样，它们不需要是一个量子系统。&lt;br /&gt;
* &amp;lt;math&amp;gt;\delta : \Sigma \times Q  \otimes \Gamma \rightarrow \Sigma \times Q \otimes \Gamma \times \{L,R\}&amp;lt;/math&amp;gt;是被推广到了Hilbert空间的转移函数[[State transition system|transition function]]。我们也可以理解它们为一些在Hilbert空间中自同构的酉矩阵[[unitary matrix|unitary matrices]] 。&lt;br /&gt;
* &amp;lt;math&amp;gt;q_0 \in Q&amp;lt;/math&amp;gt;是起始状态，它可以是几种状态的混合也可以是一种状态；&lt;br /&gt;
* 停止状态&amp;lt;math&amp;gt;F&amp;lt;/math&amp;gt;是&amp;lt;math&amp;gt;Q&amp;lt;/math&amp;gt;的子集。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The above is merely a sketch of a quantum Turing machine, rather than its formal definition, as it leaves vague several important details: for example, how often a [[quantum measurement|measurement]] is performed; see for example, the difference between a measure-once and a measure-many QFA.  This question of measurement affects the way in which writes to the output tape are defined.&lt;br /&gt;
&lt;br /&gt;
以上只是一个量子图灵机的草图，而不是它的正式定义，因为它的一些重要细节仍然定义模糊：例如，我们以什么样的频率执行对于状态的观测；什么是一次观测量子有限自动机measure-once  [[quantum finite automaton]]和多次观测量子有限自动机 measure-many [[quantum finite automaton]] 之间的区别。这些观测问题会影响我们如何定义写入和输出纸带的方式。&lt;br /&gt;
&lt;br /&gt;
==历史==&lt;br /&gt;
&lt;br /&gt;
In 1980 and 1982, physicist [[Paul Benioff]] published papers&amp;lt;ref name=&amp;quot;:0&amp;quot;&amp;gt;{{cite journal |last1=Benioff | first1=Paul | title=The computer as a physical system: A microscopic quantum mechanical Hamiltonian model of computers as represented by Turing machines | journal=Journal of Statistical Physics |volume=22 | issue=5 | pages=563–591 | year=1980 | doi=10.1007/bf01011339|bibcode=1980JSP....22..563B }}&amp;lt;/ref&amp;gt;&amp;lt;ref name=&amp;quot;:1&amp;quot;&amp;gt;{{Cite journal | doi=10.1007/BF01342185 | last1=Benioff | first1=P. | title=Quantum mechanical hamiltonian models of turing machines | journal=Journal of Statistical Physics | volume=29 | issue=3 | pages=515–546 | year=1982|bibcode=1982JSP....29..515B }}&amp;lt;/ref&amp;gt; that first described a quantum mechanical model of [[Turing machines]]. A 1985 article written by Oxford University physicist [[David Deutsch]] further developed the idea of quantum computers by suggesting [[quantum gate]]s could function in a similar fashion to traditional digital computing [[Binary numeral system|binary]] [[logic gates]].&amp;lt;ref name=&amp;quot;Deutsch1985&amp;quot;&amp;gt;{{cite journal|last=Deutsch|first=David|author-link=David Deutsch|date=July 1985|title=Quantum theory, the Church-Turing principle and the universal quantum computer|url=http://www.ceid.upatras.gr/tech_news/papers/quantum_theory.pdf|url-status=dead|journal=[[Proceedings of the Royal Society A]]|volume=400|issue=1818|pages=97–117|bibcode=1985RSPSA.400...97D|doi=10.1098/rspa.1985.0070|archiveurl=https://web.archive.org/web/20081123183419/http://www.ceid.upatras.gr/tech_news/papers/quantum_theory.pdf|archivedate=2008-11-23|citeseerx=10.1.1.41.2382}}&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
物理学家 Paul Benioff 在1980 年和 1982 年发表的论文中，首次描述了图灵机的量子力学模型。&amp;lt;ref name=&amp;quot;:0&amp;quot; /&amp;gt;&amp;lt;ref name=&amp;quot;:1&amp;quot; /&amp;gt; 牛津大学物理学家 David Deutsch 在 1985 年撰写的一篇文章中进一步推广了量子计算机的概念，他提议量子门[[quantum gate]]应该以类似于传统数字计算二进制逻辑门的方式运行。&amp;lt;ref name=&amp;quot;Deutsch1985&amp;quot; /&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Iriyama, [[Masanori Ohya|Ohya]], and Volovich have developed a model of a ''linear quantum Turing machine'' (LQTM).  This is a generalization of a classical QTM that has mixed states and that allows irreversible transition functions.  These allow the representation of quantum measurements without classical outcomes.&amp;lt;ref name=&amp;quot;:2&amp;quot;&amp;gt;{{cite journal|title=Classically-Controlled Quantum Computation|date=2007-04-04|pages=601–620|author1=Simon Perdrix|author2=Philippe Jorrand|volume=16|journal=Math. Struct. In Comp. Science|arxiv=quant-ph/0407008|doi=10.1017/S096012950600538X|issue=4}} also {{cite journal|title=Classically-Controlled Quantum Computation|author=Simon Perdrix and Philippe Jorrand|url=http://dcm-workshop.org.uk./2005/dcm-draft-proceedings.pdf|year=2006|pages=601–620|journal=Math. Struct. In Comp. Science|volume=16|doi=10.1017/S096012950600538X|issue=4|citeseerx=10.1.1.252.1823}}&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
Iriyama、Ohya 和 Volovich 开发了线性量子图灵机 linear quantum Turing machine (LQTM) 模型。他们对具有混合状态并允许不可逆转换函数的量子图灵机进行了延伸。允许了在没有经典结果的情况下对量子的测量。&amp;lt;ref name=&amp;quot;:2&amp;quot; /&amp;gt;&lt;br /&gt;
&lt;br /&gt;
A ''quantum Turing machine with [[postselection]]'' was defined by [[Scott Aaronson]], who showed that the class of polynomial time on such a machine ([[PostBQP]]) is equal to the classical complexity class [[PP (complexity)|PP]].&amp;lt;ref name=&amp;quot;:3&amp;quot;&amp;gt;{{cite journal|last=Aaronson|first=Scott|year=2005|title=Quantum computing, postselection, and probabilistic polynomial-time|journal=[[Proceedings of the Royal Society A]]|volume=461|issue=2063|pages=3473–3482|doi=10.1098/rspa.2005.1546|bibcode = 2005RSPSA.461.3473A |arxiv=quant-ph/0412187}}  Preprint available at [https://arxiv.org/abs/quant-ph/0412187]&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
Scott Aaronson 定义了具有后选择功能的量子图灵机，他证明了这种机器上的时间复杂度类 (PostBQP) 等于经典复杂度 PP。&amp;lt;ref name=&amp;quot;:3&amp;quot; /&amp;gt;&lt;br /&gt;
&lt;br /&gt;
== 相关内容 ==&lt;br /&gt;
&lt;br /&gt;
Category:Turing machine&lt;br /&gt;
&lt;br /&gt;
类别: 图灵机&lt;br /&gt;
&lt;br /&gt;
*[[Quantum simulator#Solving physics problems|Quantum simulator § Solving physics problems]]&lt;br /&gt;
&lt;br /&gt;
范畴: 量子复杂性理论&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:Quantum Turing machine]]. Its edit history can be viewed at [[量子图灵机/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>Tueryeye</name></author>
	</entry>
	<entry>
		<id>https://wiki.swarma.org/index.php?title=%E9%87%8F%E5%AD%90%E5%9B%BE%E7%81%B5%E6%9C%BA&amp;diff=29904</id>
		<title>量子图灵机</title>
		<link rel="alternate" type="text/html" href="https://wiki.swarma.org/index.php?title=%E9%87%8F%E5%AD%90%E5%9B%BE%E7%81%B5%E6%9C%BA&amp;diff=29904"/>
		<updated>2022-03-31T04:29:41Z</updated>

		<summary type="html">&lt;p&gt;Tueryeye：阅读第二遍&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;此词条由tueryeye翻译审校，未经专家审核，带来阅读不便，请见谅。{{Short description|Model of quantum computation}}&lt;br /&gt;
&lt;br /&gt;
{{Turing}}&lt;br /&gt;
&lt;br /&gt;
&amp;lt;!-- Basic definition --&amp;gt;&lt;br /&gt;
== 基础定义 ==&lt;br /&gt;
A '''quantum Turing machine''' ('''QTM''') or '''universal quantum computer''' is an [[abstract machine]] used to model the effects of a [[quantum computer]].  It provides a simple model that captures all of the power of quantum computation—that is, any [[quantum algorithm]] can be expressed formally as a particular quantum Turing machine. However, the computationally equivalent [[quantum circuit]] is a more common model.&amp;lt;ref name=&amp;quot;equivalence&amp;quot;&amp;gt;{{cite conference|author=[[Andrew Yao]]|title=Quantum circuit complexity|conference=34th Annual Symposium on Foundations of Computer Science|pages=352–361|year=1993}}&amp;lt;/ref&amp;gt;&amp;lt;ref name=&amp;quot;newequivalence&amp;quot;&amp;gt;{{cite arXiv|eprint=1808.01701|author1=Abel Molina|author2=John Watrous|author-link2=John Watrous (computer scientist)|title=Revisiting the simulation of quantum Turing machines by quantum circuits|date=2018|class=cs.CC}}&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
量子图灵机'''quantum Turing machine''' (QTM)又称为通用量子计算机是一种用来模拟量子计算机效果的抽象机器。尽管说提供等效计算能力的量子电路是一种更常用的模型，但是量子图灵机'''quantum Turing machine''' 是一个简单但能展现出量子计算的所有威力的模型。就像经典图灵机可以模拟人类所能进行的任何计算过程一样，量子图灵机可以描述任何量子算法。&amp;lt;ref name=&amp;quot;equivalence&amp;quot; /&amp;gt;&amp;lt;ref name=&amp;quot;newequivalence&amp;quot; /&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&amp;lt;!-- Relation to classical computation --&amp;gt;&lt;br /&gt;
&lt;br /&gt;
== 与经典计算的关系 ==&lt;br /&gt;
Quantum Turing machines can be related to classical and probabilistic Turing machines in a framework based on [[Stochastic matrix|transition matrices]]. That is, a matrix can be specified whose product with the matrix representing a classical or probabilistic machine provides the quantum probability matrix representing the quantum machine. This was shown by [[Lance Fortnow]].&amp;lt;ref name=&amp;quot;transition&amp;quot;&amp;gt;{{cite journal|author=Fortnow|first=Lance|author-link=Lance Fortnow|year=2003|title=One Complexity Theorist's View of Quantum Computing|url=|journal=Theoretical Computer Science|volume=292|issue=3|pages=597–610|doi=10.1016/S0304-3975(01)00377-2|via=|arxiv=quant-ph/0003035}}&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
通过过渡矩阵[[Stochastic matrix|transition matrices]]，量子图灵机可以与经典图灵机和概率图灵机相关联。Lance Fortnow证明，量子图灵机的量子概率矩阵可以被拆解成是指定矩阵与经典或概率图灵机的矩阵的乘积。&amp;lt;ref name=&amp;quot;transition&amp;quot; /&amp;gt;&lt;br /&gt;
&lt;br /&gt;
== 非正式草图定义 ==&lt;br /&gt;
{{Unsolved|physics|Is a [[universal quantum computer]] sufficient to [[Algorithmic efficiency|efficiently]] [[Dynamical simulation|simulate]] an arbitrary physical system?}}&lt;br /&gt;
&lt;br /&gt;
A way of understanding the quantum Turing machine (QTM) is that it generalizes the classical [[Turing machine]] (TM) in the same way that the [[quantum finite automaton]] (QFA) generalizes the [[deterministic finite automaton]] (DFA).  In essence, the internal states of a classical TM are replaced by [[pure state|pure]] or [[mixed quantum state|mixed states]] in a Hilbert space; the transition function is replaced by a collection of [[unitary matrix|unitary matrices]] that map the Hilbert space to itself.&amp;lt;ref name=&amp;quot;Deutsch1985&amp;quot; /&amp;gt;&lt;br /&gt;
&lt;br /&gt;
我们可以通过类比确定有限自动机[[deterministic finite automaton]]到量子有限自动机[[quantum finite automaton]]的转化来理解经典图灵机到量子图灵机'''quantum Turing machine'''的转化。 他们的差异在于，经典图灵机讨论的状态被推广到了Hilbert空间中。Hilbert空间是'''完备的内积空间'''，是有限维欧几里得空间的一个推广。它不局限于实数的情形和有限的维数，但又不失完备性。在量子图灵机中转换函数被一组映射Hilbert空间到自身的酉矩阵[[unitary matrix|unitary matrices]]取代。&amp;lt;ref name=&amp;quot;Deutsch1985&amp;quot; /&amp;gt;&lt;br /&gt;
&lt;br /&gt;
经典图灵机的诞生是因为图灵想用机器来模拟用纸笔进行数学运算的过程，这样的过程可以被看作下列两种简单的动作：&lt;br /&gt;
&lt;br /&gt;
* 在纸带上写上或删除某个符号；&lt;br /&gt;
* 把笔尖从纸的一处移动到另一处；&lt;br /&gt;
&lt;br /&gt;
现在我们假设有一条纸带无限长，并且被划分为一个接一个的小格子，每个格子上包含一个来自有限字母表的符号，字母表中有一个特殊的符号表示空白。假设我们有一个执笔机器又称为读写头（'''HEAD），'''它本身也可以具有一个状态。就像人今天可能因为某件事心情很好，也可能因为另一件事情很抑郁一样，它的状态会随着它的遭遇所改变。更重要的是执笔机器当前关注的纸上的某个位置的符号和当前的状态决定了下一步的动作。在遇到停止状态&amp;lt;math&amp;gt;F&amp;lt;/math&amp;gt;之前执笔机器可以&lt;br /&gt;
&lt;br /&gt;
* 1. 写入（替换）或擦除当前符号；&lt;br /&gt;
* 2. 移动 '''HEAD'''， 'L'向左一步， 'R'向右一步或者'N'不移动；&lt;br /&gt;
* 3. 保持当前状态或者转到另一状态。&lt;br /&gt;
&lt;br /&gt;
That is, a classical Turing machine is described by  a 7-[[tuple]] &amp;lt;math&amp;gt;M = \langle Q, \Gamma, b, \Sigma, \delta, q_0, F \rangle&amp;lt;/math&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
总的来说，经典图灵机可以被一个七元有序组所描述，&amp;lt;math&amp;gt;M = \langle Q, \Gamma, b, \Sigma, \delta, q_0, F \rangle&amp;lt;/math&amp;gt;。&lt;br /&gt;
&lt;br /&gt;
* The set of states &amp;lt;math&amp;gt;Q&amp;lt;/math&amp;gt; is replaced by a [[Hilbert space]].&lt;br /&gt;
&lt;br /&gt;
* The tape alphabet symbols &amp;lt;math&amp;gt;\Gamma&amp;lt;/math&amp;gt; are likewise replaced by a Hilbert space (usually a different Hilbert space than the set of states).&lt;br /&gt;
&lt;br /&gt;
* The blank symbol &amp;lt;math&amp;gt;b \in \Gamma&amp;lt;/math&amp;gt; corresponds to the zero-vector.&lt;br /&gt;
&lt;br /&gt;
* The input and output symbols &amp;lt;math&amp;gt;\Sigma&amp;lt;/math&amp;gt; are usually taken as a discrete set, as in the classical system; thus, neither the input nor output to a quantum machine need be a quantum system itself.&lt;br /&gt;
&lt;br /&gt;
* The [[State transition system|transition function]] &amp;lt;math&amp;gt;\delta : \Sigma \times Q  \otimes \Gamma \rightarrow \Sigma \times Q \otimes \Gamma \times \{L,R\}&amp;lt;/math&amp;gt; is a generalization of a [[transition monoid]], and is understood to be a collection of [[unitary matrix|unitary matrices]] that are [[automorphism]]s of the Hilbert space &amp;lt;math&amp;gt;Q&amp;lt;/math&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
* The initial state &amp;lt;math&amp;gt;q_0 \in Q&amp;lt;/math&amp;gt; may be either a [[mixed quantum state|mixed state]] or a [[pure state]].&lt;br /&gt;
&lt;br /&gt;
* The set &amp;lt;math&amp;gt;F&amp;lt;/math&amp;gt; of ''final'' or ''accepting states'' is a subspace of the Hilbert space &amp;lt;math&amp;gt;Q&amp;lt;/math&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
* &amp;lt;math&amp;gt;Q&amp;lt;/math&amp;gt; 非空有穷状态集合被推广到了Hilbert空间；&lt;br /&gt;
* &amp;lt;math&amp;gt;\Gamma&amp;lt;/math&amp;gt; 是非空有穷输入字母表，其中不包含特殊的空白符也被推广到了Hilbert空间；&lt;br /&gt;
* &amp;lt;math&amp;gt;b \in \Gamma&amp;lt;/math&amp;gt; 为''空白符''，也是唯一允许出现无限次的字符；&lt;br /&gt;
* 输入和输出符号 &amp;lt;math&amp;gt;\Sigma&amp;lt;/math&amp;gt;通常是一个离散集。和经典图灵机的输入输出符号一样，它们不需要是一个量子系统。&lt;br /&gt;
* &amp;lt;math&amp;gt;\delta : \Sigma \times Q  \otimes \Gamma \rightarrow \Sigma \times Q \otimes \Gamma \times \{L,R\}&amp;lt;/math&amp;gt;是转移函数[[State transition system|transition function]]被推广到了Hilbert空间。我们也可以理解它们为一些在Hilbert空间中自同构的酉矩阵[[unitary matrix|unitary matrices]] 。&lt;br /&gt;
* &amp;lt;math&amp;gt;q_0 \in Q&amp;lt;/math&amp;gt;是起始状态，它可以是几种状态的混合也可以是一种状态；&lt;br /&gt;
* 停止状态&amp;lt;math&amp;gt;F&amp;lt;/math&amp;gt;是&amp;lt;math&amp;gt;Q&amp;lt;/math&amp;gt;的子集。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The above is merely a sketch of a quantum Turing machine, rather than its formal definition, as it leaves vague several important details: for example, how often a [[quantum measurement|measurement]] is performed; see for example, the difference between a measure-once and a measure-many QFA.  This question of measurement affects the way in which writes to the output tape are defined.&lt;br /&gt;
&lt;br /&gt;
以上只是一个量子图灵机的草图，而不是它的正式定义，因为它的一些重要细节仍然定义模糊：例如，我们以什么样的频率执行对于状态的观测；什么是一次观测量子有限自动机measure-once  [[quantum finite automaton]]和多次观测量子有限自动机 measure-many [[quantum finite automaton]] 之间的区别。这些观测问题会影响我们如何定义写入和输出纸带的方式。&lt;br /&gt;
&lt;br /&gt;
==历史==&lt;br /&gt;
&lt;br /&gt;
In 1980 and 1982, physicist [[Paul Benioff]] published papers&amp;lt;ref name=&amp;quot;:0&amp;quot;&amp;gt;{{cite journal |last1=Benioff | first1=Paul | title=The computer as a physical system: A microscopic quantum mechanical Hamiltonian model of computers as represented by Turing machines | journal=Journal of Statistical Physics |volume=22 | issue=5 | pages=563–591 | year=1980 | doi=10.1007/bf01011339|bibcode=1980JSP....22..563B }}&amp;lt;/ref&amp;gt;&amp;lt;ref name=&amp;quot;:1&amp;quot;&amp;gt;{{Cite journal | doi=10.1007/BF01342185 | last1=Benioff | first1=P. | title=Quantum mechanical hamiltonian models of turing machines | journal=Journal of Statistical Physics | volume=29 | issue=3 | pages=515–546 | year=1982|bibcode=1982JSP....29..515B }}&amp;lt;/ref&amp;gt; that first described a quantum mechanical model of [[Turing machines]]. A 1985 article written by Oxford University physicist [[David Deutsch]] further developed the idea of quantum computers by suggesting [[quantum gate]]s could function in a similar fashion to traditional digital computing [[Binary numeral system|binary]] [[logic gates]].&amp;lt;ref name=&amp;quot;Deutsch1985&amp;quot;&amp;gt;{{cite journal|last=Deutsch|first=David|author-link=David Deutsch|date=July 1985|title=Quantum theory, the Church-Turing principle and the universal quantum computer|url=http://www.ceid.upatras.gr/tech_news/papers/quantum_theory.pdf|url-status=dead|journal=[[Proceedings of the Royal Society A]]|volume=400|issue=1818|pages=97–117|bibcode=1985RSPSA.400...97D|doi=10.1098/rspa.1985.0070|archiveurl=https://web.archive.org/web/20081123183419/http://www.ceid.upatras.gr/tech_news/papers/quantum_theory.pdf|archivedate=2008-11-23|citeseerx=10.1.1.41.2382}}&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
物理学家 Paul Benioff 在1980 年和 1982 年发表的论文中，首次描述了图灵机的量子力学模型。&amp;lt;ref name=&amp;quot;:0&amp;quot; /&amp;gt;&amp;lt;ref name=&amp;quot;:1&amp;quot; /&amp;gt; 牛津大学物理学家 David Deutsch 在 1985 年撰写的一篇文章中进一步推广了量子计算机的概念，他提议量子门[[quantum gate]]应该以类似于传统数字计算二进制逻辑门的方式运行。&amp;lt;ref name=&amp;quot;Deutsch1985&amp;quot; /&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Iriyama, [[Masanori Ohya|Ohya]], and Volovich have developed a model of a ''linear quantum Turing machine'' (LQTM).  This is a generalization of a classical QTM that has mixed states and that allows irreversible transition functions.  These allow the representation of quantum measurements without classical outcomes.&amp;lt;ref name=&amp;quot;:2&amp;quot;&amp;gt;{{cite journal|title=Classically-Controlled Quantum Computation|date=2007-04-04|pages=601–620|author1=Simon Perdrix|author2=Philippe Jorrand|volume=16|journal=Math. Struct. In Comp. Science|arxiv=quant-ph/0407008|doi=10.1017/S096012950600538X|issue=4}} also {{cite journal|title=Classically-Controlled Quantum Computation|author=Simon Perdrix and Philippe Jorrand|url=http://dcm-workshop.org.uk./2005/dcm-draft-proceedings.pdf|year=2006|pages=601–620|journal=Math. Struct. In Comp. Science|volume=16|doi=10.1017/S096012950600538X|issue=4|citeseerx=10.1.1.252.1823}}&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
Iriyama、Ohya 和 Volovich 开发了线性量子图灵机 linear quantum Turing machine (LQTM) 模型。他们对具有混合状态并允许不可逆转换函数的量子图灵机进行了延伸。允许了在没有经典结果的情况下对量子的测量。&amp;lt;ref name=&amp;quot;:2&amp;quot; /&amp;gt;&lt;br /&gt;
&lt;br /&gt;
A ''quantum Turing machine with [[postselection]]'' was defined by [[Scott Aaronson]], who showed that the class of polynomial time on such a machine ([[PostBQP]]) is equal to the classical complexity class [[PP (complexity)|PP]].&amp;lt;ref name=&amp;quot;:3&amp;quot;&amp;gt;{{cite journal|last=Aaronson|first=Scott|year=2005|title=Quantum computing, postselection, and probabilistic polynomial-time|journal=[[Proceedings of the Royal Society A]]|volume=461|issue=2063|pages=3473–3482|doi=10.1098/rspa.2005.1546|bibcode = 2005RSPSA.461.3473A |arxiv=quant-ph/0412187}}  Preprint available at [https://arxiv.org/abs/quant-ph/0412187]&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
Scott Aaronson 定义了具有后选择功能的量子图灵机，他证明了这种机器上的时间复杂度类 (PostBQP) 等于经典复杂度 PP。&amp;lt;ref name=&amp;quot;:3&amp;quot; /&amp;gt;&lt;br /&gt;
&lt;br /&gt;
== 相关内容 ==&lt;br /&gt;
&lt;br /&gt;
Category:Turing machine&lt;br /&gt;
&lt;br /&gt;
类别: 图灵机&lt;br /&gt;
&lt;br /&gt;
*[[Quantum simulator#Solving physics problems|Quantum simulator § Solving physics problems]]&lt;br /&gt;
&lt;br /&gt;
范畴: 量子复杂性理论&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:Quantum Turing machine]]. Its edit history can be viewed at [[量子图灵机/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>Tueryeye</name></author>
	</entry>
	<entry>
		<id>https://wiki.swarma.org/index.php?title=%E9%87%8F%E5%AD%90%E5%9B%BE%E7%81%B5%E6%9C%BA&amp;diff=29903</id>
		<title>量子图灵机</title>
		<link rel="alternate" type="text/html" href="https://wiki.swarma.org/index.php?title=%E9%87%8F%E5%AD%90%E5%9B%BE%E7%81%B5%E6%9C%BA&amp;diff=29903"/>
		<updated>2022-03-31T04:26:06Z</updated>

		<summary type="html">&lt;p&gt;Tueryeye：删除一些唐突的原文&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;此词条由tueryeye翻译审校，未经专家审核，带来阅读不便，请见谅。{{Short description|Model of quantum computation}}&lt;br /&gt;
&lt;br /&gt;
{{Turing}}&lt;br /&gt;
&lt;br /&gt;
&amp;lt;!-- Basic definition --&amp;gt;&lt;br /&gt;
== 基础定义 ==&lt;br /&gt;
A '''quantum Turing machine''' ('''QTM''') or '''universal quantum computer''' is an [[abstract machine]] used to model the effects of a [[quantum computer]].  It provides a simple model that captures all of the power of quantum computation—that is, any [[quantum algorithm]] can be expressed formally as a particular quantum Turing machine. However, the computationally equivalent [[quantum circuit]] is a more common model.&amp;lt;ref name=&amp;quot;equivalence&amp;quot;&amp;gt;{{cite conference|author=[[Andrew Yao]]|title=Quantum circuit complexity|conference=34th Annual Symposium on Foundations of Computer Science|pages=352–361|year=1993}}&amp;lt;/ref&amp;gt;&amp;lt;ref name=&amp;quot;newequivalence&amp;quot;&amp;gt;{{cite arXiv|eprint=1808.01701|author1=Abel Molina|author2=John Watrous|author-link2=John Watrous (computer scientist)|title=Revisiting the simulation of quantum Turing machines by quantum circuits|date=2018|class=cs.CC}}&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
量子图灵机'''quantum Turing machine''' (QTM)又称为通用量子计算机是一种用来模拟量子计算机效果的抽象机器。尽管说提供等效计算能力的量子电路是一种更常用的模型，但是量子图灵机'''quantum Turing machine''' 是一个简单但能展现出量子计算的所有威力的模型。就像经典图灵机可以模拟人类所能进行的任何计算过程一样，量子图灵机可以描述任何量子算法。&amp;lt;ref name=&amp;quot;equivalence&amp;quot; /&amp;gt;&amp;lt;ref name=&amp;quot;newequivalence&amp;quot; /&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&amp;lt;!-- Relation to classical computation --&amp;gt;&lt;br /&gt;
&lt;br /&gt;
== 与经典计算的关系 ==&lt;br /&gt;
Quantum Turing machines can be related to classical and probabilistic Turing machines in a framework based on [[Stochastic matrix|transition matrices]]. That is, a matrix can be specified whose product with the matrix representing a classical or probabilistic machine provides the quantum probability matrix representing the quantum machine. This was shown by [[Lance Fortnow]].&amp;lt;ref name=&amp;quot;transition&amp;quot;&amp;gt;{{cite journal|author=Fortnow|first=Lance|author-link=Lance Fortnow|year=2003|title=One Complexity Theorist's View of Quantum Computing|url=|journal=Theoretical Computer Science|volume=292|issue=3|pages=597–610|doi=10.1016/S0304-3975(01)00377-2|via=|arxiv=quant-ph/0003035}}&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
通过过渡矩阵[[Stochastic matrix|transition matrices]]，量子图灵机可以与经典图灵机和概率图灵机相关联。Lance Fortnow证明，量子图灵机的量子概率矩阵可以被拆解成是指定矩阵与经典或概率图灵机的矩阵的乘积。&amp;lt;ref name=&amp;quot;transition&amp;quot; /&amp;gt;&lt;br /&gt;
&lt;br /&gt;
== 非正式草图定义 ==&lt;br /&gt;
{{Unsolved|physics|Is a [[universal quantum computer]] sufficient to [[Algorithmic efficiency|efficiently]] [[Dynamical simulation|simulate]] an arbitrary physical system?}}&lt;br /&gt;
&lt;br /&gt;
A way of understanding the quantum Turing machine (QTM) is that it generalizes the classical [[Turing machine]] (TM) in the same way that the [[quantum finite automaton]] (QFA) generalizes the [[deterministic finite automaton]] (DFA).  In essence, the internal states of a classical TM are replaced by [[pure state|pure]] or [[mixed quantum state|mixed states]] in a Hilbert space; the transition function is replaced by a collection of [[unitary matrix|unitary matrices]] that map the Hilbert space to itself.&amp;lt;ref name=&amp;quot;Deutsch1985&amp;quot; /&amp;gt;&lt;br /&gt;
&lt;br /&gt;
我们可以通过类比确定有限自动机[[deterministic finite automaton]]到量子有限自动机[[quantum finite automaton]]的转化来理解经典图灵机到量子图灵机'''quantum Turing machine'''的转化。 他们的差异在于，经典图灵机讨论的状态被推广到了Hilbert空间中。Hilbert空间是'''完备的内积空间'''，是有限维欧几里得空间的一个推广。它不局限于实数的情形和有限的维数，但又不失完备性。在量子图灵机中转换函数被一组映射Hilbert空间到自身的酉矩阵[[unitary matrix|unitary matrices]]取代。&amp;lt;ref name=&amp;quot;Deutsch1985&amp;quot; /&amp;gt;&lt;br /&gt;
&lt;br /&gt;
经典图灵机的诞生是因为图灵想用机器来模拟用纸笔进行数学运算的过程，这样的过程可以被看作下列两种简单的动作：&lt;br /&gt;
&lt;br /&gt;
* 在纸带上写上或删除某个符号；&lt;br /&gt;
* 把笔尖从纸的一处移动到另一处；&lt;br /&gt;
&lt;br /&gt;
现在我们假设有一条纸带无限长，并且被划分为一个接一个的小格子，每个格子上包含一个来自有限字母表的符号，字母表中有一个特殊的符号表示空白。假设我们有一个执笔机器又称为读写头（'''HEAD），'''它本身也可以具有一个状态。就像人今天可能因为某件事心情很好，也可能因为另一件事情很抑郁一样，它的状态会随着它的遭遇所改变。更重要的是执笔机器当前关注的纸上的某个位置的符号和当前的状态决定了下一步的动作。在遇到停止状态&amp;lt;math&amp;gt;F&amp;lt;/math&amp;gt;之前执笔机器可以&lt;br /&gt;
&lt;br /&gt;
* 1. 写入（替换）或擦除当前符号；&lt;br /&gt;
* 2. 移动 '''HEAD'''， 'L'向左一步， 'R'向右一步或者'N'不移动；&lt;br /&gt;
* 3. 保持当前状态或者转到另一状态。&lt;br /&gt;
&lt;br /&gt;
That is, a classical Turing machine is described by  a 7-[[tuple]] &amp;lt;math&amp;gt;M = \langle Q, \Gamma, b, \Sigma, \delta, q_0, F \rangle&amp;lt;/math&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
总的来说，经典图灵机可以被一个七元有序组所描述，&amp;lt;math&amp;gt;M = \langle Q, \Gamma, b, \Sigma, \delta, q_0, F \rangle&amp;lt;/math&amp;gt;。&lt;br /&gt;
&lt;br /&gt;
* The set of states &amp;lt;math&amp;gt;Q&amp;lt;/math&amp;gt; is replaced by a [[Hilbert space]].&lt;br /&gt;
&lt;br /&gt;
* The tape alphabet symbols &amp;lt;math&amp;gt;\Gamma&amp;lt;/math&amp;gt; are likewise replaced by a Hilbert space (usually a different Hilbert space than the set of states).&lt;br /&gt;
&lt;br /&gt;
* The blank symbol &amp;lt;math&amp;gt;b \in \Gamma&amp;lt;/math&amp;gt; corresponds to the zero-vector.&lt;br /&gt;
&lt;br /&gt;
* The input and output symbols &amp;lt;math&amp;gt;\Sigma&amp;lt;/math&amp;gt; are usually taken as a discrete set, as in the classical system; thus, neither the input nor output to a quantum machine need be a quantum system itself.&lt;br /&gt;
&lt;br /&gt;
* The [[State transition system|transition function]] &amp;lt;math&amp;gt;\delta : \Sigma \times Q  \otimes \Gamma \rightarrow \Sigma \times Q \otimes \Gamma \times \{L,R\}&amp;lt;/math&amp;gt; is a generalization of a [[transition monoid]], and is understood to be a collection of [[unitary matrix|unitary matrices]] that are [[automorphism]]s of the Hilbert space &amp;lt;math&amp;gt;Q&amp;lt;/math&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
* The initial state &amp;lt;math&amp;gt;q_0 \in Q&amp;lt;/math&amp;gt; may be either a [[mixed quantum state|mixed state]] or a [[pure state]].&lt;br /&gt;
&lt;br /&gt;
* The set &amp;lt;math&amp;gt;F&amp;lt;/math&amp;gt; of ''final'' or ''accepting states'' is a subspace of the Hilbert space &amp;lt;math&amp;gt;Q&amp;lt;/math&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
* &amp;lt;math&amp;gt;Q&amp;lt;/math&amp;gt; 非空有穷状态集合被推广到了Hilbert空间；&lt;br /&gt;
* &amp;lt;math&amp;gt;\Gamma&amp;lt;/math&amp;gt; 是非空有穷输入字母表，其中不包含特殊的空白符也被推广到了Hilbert空间；&lt;br /&gt;
* &amp;lt;math&amp;gt;b \in \Gamma&amp;lt;/math&amp;gt; 为''空白符''，也是唯一允许出现无限次的字符；&lt;br /&gt;
* 输入和输出符号 &amp;lt;math&amp;gt;\Sigma&amp;lt;/math&amp;gt;通常是一个离散集。和经典图灵机的输入输出符号一样，它们不需要是一个量子系统。&lt;br /&gt;
* &amp;lt;math&amp;gt;\delta : \Sigma \times Q  \otimes \Gamma \rightarrow \Sigma \times Q \otimes \Gamma \times \{L,R\}&amp;lt;/math&amp;gt;是转移函数[[State transition system|transition function]]被推广到了Hilbert空间。我们也可以理解它们为一些在Hilbert空间中自同构的酉矩阵[[unitary matrix|unitary matrices]] 。&lt;br /&gt;
* &amp;lt;math&amp;gt;q_0 \in Q&amp;lt;/math&amp;gt;是起始状态，它可以是几种状态的混合也可以是一种状态；&lt;br /&gt;
* 停止状态&amp;lt;math&amp;gt;F&amp;lt;/math&amp;gt;是&amp;lt;math&amp;gt;Q&amp;lt;/math&amp;gt;的子集。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The above is merely a sketch of a quantum Turing machine, rather than its formal definition, as it leaves vague several important details: for example, how often a [[quantum measurement|measurement]] is performed; see for example, the difference between a measure-once and a measure-many QFA.  This question of measurement affects the way in which writes to the output tape are defined.&lt;br /&gt;
&lt;br /&gt;
以上只是一个量子图灵机的草图，而不是它的正式定义，因为它的一些重要细节仍然定义模糊：例如，我们以什么样的频率执行对于状态的观测；什么是一次观测量子有限自动机和多次观测量子有限自动机 QFA 之间的区别。这些观测问题会影响我们如何定义写入和输出纸带的方式。&lt;br /&gt;
&lt;br /&gt;
==历史==&lt;br /&gt;
&lt;br /&gt;
In 1980 and 1982, physicist [[Paul Benioff]] published papers&amp;lt;ref name=&amp;quot;:0&amp;quot;&amp;gt;{{cite journal |last1=Benioff | first1=Paul | title=The computer as a physical system: A microscopic quantum mechanical Hamiltonian model of computers as represented by Turing machines | journal=Journal of Statistical Physics |volume=22 | issue=5 | pages=563–591 | year=1980 | doi=10.1007/bf01011339|bibcode=1980JSP....22..563B }}&amp;lt;/ref&amp;gt;&amp;lt;ref name=&amp;quot;:1&amp;quot;&amp;gt;{{Cite journal | doi=10.1007/BF01342185 | last1=Benioff | first1=P. | title=Quantum mechanical hamiltonian models of turing machines | journal=Journal of Statistical Physics | volume=29 | issue=3 | pages=515–546 | year=1982|bibcode=1982JSP....29..515B }}&amp;lt;/ref&amp;gt; that first described a quantum mechanical model of [[Turing machines]]. A 1985 article written by Oxford University physicist [[David Deutsch]] further developed the idea of quantum computers by suggesting [[quantum gate]]s could function in a similar fashion to traditional digital computing [[Binary numeral system|binary]] [[logic gates]].&amp;lt;ref name=&amp;quot;Deutsch1985&amp;quot;&amp;gt;{{cite journal|last=Deutsch|first=David|author-link=David Deutsch|date=July 1985|title=Quantum theory, the Church-Turing principle and the universal quantum computer|url=http://www.ceid.upatras.gr/tech_news/papers/quantum_theory.pdf|url-status=dead|journal=[[Proceedings of the Royal Society A]]|volume=400|issue=1818|pages=97–117|bibcode=1985RSPSA.400...97D|doi=10.1098/rspa.1985.0070|archiveurl=https://web.archive.org/web/20081123183419/http://www.ceid.upatras.gr/tech_news/papers/quantum_theory.pdf|archivedate=2008-11-23|citeseerx=10.1.1.41.2382}}&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
物理学家 Paul Benioff 在1980 年和 1982 年发表的论文中，首次描述了图灵机的量子力学模型。&amp;lt;ref name=&amp;quot;:0&amp;quot; /&amp;gt;&amp;lt;ref name=&amp;quot;:1&amp;quot; /&amp;gt; 牛津大学物理学家 David Deutsch 在 1985 年撰写的一篇文章中进一步发展了量子计算机的概念，他提议量子门[[quantum gate]]应该以类似于传统数字计算二进制逻辑门的方式运行。&amp;lt;ref name=&amp;quot;Deutsch1985&amp;quot; /&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Iriyama, [[Masanori Ohya|Ohya]], and Volovich have developed a model of a ''linear quantum Turing machine'' (LQTM).  This is a generalization of a classical QTM that has mixed states and that allows irreversible transition functions.  These allow the representation of quantum measurements without classical outcomes.&amp;lt;ref name=&amp;quot;:2&amp;quot;&amp;gt;{{cite journal|title=Classically-Controlled Quantum Computation|date=2007-04-04|pages=601–620|author1=Simon Perdrix|author2=Philippe Jorrand|volume=16|journal=Math. Struct. In Comp. Science|arxiv=quant-ph/0407008|doi=10.1017/S096012950600538X|issue=4}} also {{cite journal|title=Classically-Controlled Quantum Computation|author=Simon Perdrix and Philippe Jorrand|url=http://dcm-workshop.org.uk./2005/dcm-draft-proceedings.pdf|year=2006|pages=601–620|journal=Math. Struct. In Comp. Science|volume=16|doi=10.1017/S096012950600538X|issue=4|citeseerx=10.1.1.252.1823}}&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
Iriyama、Ohya 和 Volovich 开发了线性量子图灵机 (LQTM) 模型。他们对具有混合状态并允许不可逆转换函数的量子图灵机进行了延伸。允许了没有经典结果的情况对量子测量在。&amp;lt;ref name=&amp;quot;:2&amp;quot; /&amp;gt;&lt;br /&gt;
&lt;br /&gt;
A ''quantum Turing machine with [[postselection]]'' was defined by [[Scott Aaronson]], who showed that the class of polynomial time on such a machine ([[PostBQP]]) is equal to the classical complexity class [[PP (complexity)|PP]].&amp;lt;ref name=&amp;quot;:3&amp;quot;&amp;gt;{{cite journal|last=Aaronson|first=Scott|year=2005|title=Quantum computing, postselection, and probabilistic polynomial-time|journal=[[Proceedings of the Royal Society A]]|volume=461|issue=2063|pages=3473–3482|doi=10.1098/rspa.2005.1546|bibcode = 2005RSPSA.461.3473A |arxiv=quant-ph/0412187}}  Preprint available at [https://arxiv.org/abs/quant-ph/0412187]&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
Scott Aaronson 定义了具有后选择功能的量子图灵机，他证明了这种机器上的时间复杂度类 (PostBQP) 等于经典复杂度 PP。&amp;lt;ref name=&amp;quot;:3&amp;quot; /&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
== 相关内容 ==&lt;br /&gt;
&lt;br /&gt;
Category:Turing machine&lt;br /&gt;
&lt;br /&gt;
类别: 图灵机&lt;br /&gt;
&lt;br /&gt;
*[[Quantum simulator#Solving physics problems|Quantum simulator § Solving physics problems]]&lt;br /&gt;
&lt;br /&gt;
范畴: 量子复杂性理论&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:Quantum Turing machine]]. Its edit history can be viewed at [[量子图灵机/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>Tueryeye</name></author>
	</entry>
	<entry>
		<id>https://wiki.swarma.org/index.php?title=%E9%87%8F%E5%AD%90%E5%9B%BE%E7%81%B5%E6%9C%BA&amp;diff=29902</id>
		<title>量子图灵机</title>
		<link rel="alternate" type="text/html" href="https://wiki.swarma.org/index.php?title=%E9%87%8F%E5%AD%90%E5%9B%BE%E7%81%B5%E6%9C%BA&amp;diff=29902"/>
		<updated>2022-03-31T04:21:45Z</updated>

		<summary type="html">&lt;p&gt;Tueryeye：整理&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;此词条由tueryeye翻译审校，未经专家审核，带来阅读不便，请见谅。{{Short description|Model of quantum computation}}&lt;br /&gt;
&lt;br /&gt;
{{Turing}}&lt;br /&gt;
&lt;br /&gt;
&amp;lt;!-- Basic definition --&amp;gt;&lt;br /&gt;
== 基础定义 ==&lt;br /&gt;
A '''quantum Turing machine''' ('''QTM''') or '''universal quantum computer''' is an [[abstract machine]] used to model the effects of a [[quantum computer]].  It provides a simple model that captures all of the power of quantum computation—that is, any [[quantum algorithm]] can be expressed formally as a particular quantum Turing machine. However, the computationally equivalent [[quantum circuit]] is a more common model.&amp;lt;ref name=&amp;quot;equivalence&amp;quot;&amp;gt;{{cite conference|author=[[Andrew Yao]]|title=Quantum circuit complexity|conference=34th Annual Symposium on Foundations of Computer Science|pages=352–361|year=1993}}&amp;lt;/ref&amp;gt;&amp;lt;ref name=&amp;quot;newequivalence&amp;quot;&amp;gt;{{cite arXiv|eprint=1808.01701|author1=Abel Molina|author2=John Watrous|author-link2=John Watrous (computer scientist)|title=Revisiting the simulation of quantum Turing machines by quantum circuits|date=2018|class=cs.CC}}&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
量子图灵机计算机'''quantum Turing machine''' (QTM)又称为通用量子计算机是一种用来模拟量子计算机效果的抽象机器。虽然它是一个简单的模型，但它能展现出量子计算的所有威力。就像经典图灵机可以模拟人类所能进行的任何计算过程一样，量子图灵机可以描述任何量子算法。尽管说提供等效计算能力的量子电路是一种更常用的模型。&amp;lt;ref name=&amp;quot;equivalence&amp;quot; /&amp;gt;&amp;lt;ref name=&amp;quot;newequivalence&amp;quot; /&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&amp;lt;!-- Relation to classical computation --&amp;gt;&lt;br /&gt;
&lt;br /&gt;
== 与经典计算的关系 ==&lt;br /&gt;
Quantum Turing machines can be related to classical and probabilistic Turing machines in a framework based on [[Stochastic matrix|transition matrices]]. That is, a matrix can be specified whose product with the matrix representing a classical or probabilistic machine provides the quantum probability matrix representing the quantum machine. This was shown by [[Lance Fortnow]].&amp;lt;ref name=&amp;quot;transition&amp;quot;&amp;gt;{{cite journal|author=Fortnow|first=Lance|author-link=Lance Fortnow|year=2003|title=One Complexity Theorist's View of Quantum Computing|url=|journal=Theoretical Computer Science|volume=292|issue=3|pages=597–610|doi=10.1016/S0304-3975(01)00377-2|via=|arxiv=quant-ph/0003035}}&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
通过过渡矩阵，量子图灵机可以与经典图灵机和概率图灵机相关联。Lance Fortnow证明，量子图灵机的量子概率矩阵可以被拆解成是指定矩阵与经典或概率图灵机的矩阵的乘积。&amp;lt;ref name=&amp;quot;transition&amp;quot; /&amp;gt;&lt;br /&gt;
&lt;br /&gt;
== 非正式草图定义 ==&lt;br /&gt;
{{Unsolved|physics|Is a [[universal quantum computer]] sufficient to [[Algorithmic efficiency|efficiently]] [[Dynamical simulation|simulate]] an arbitrary physical system?}}&lt;br /&gt;
&lt;br /&gt;
A way of understanding the quantum Turing machine (QTM) is that it generalizes the classical [[Turing machine]] (TM) in the same way that the [[quantum finite automaton]] (QFA) generalizes the [[deterministic finite automaton]] (DFA).  In essence, the internal states of a classical TM are replaced by [[pure state|pure]] or [[mixed quantum state|mixed states]] in a Hilbert space; the transition function is replaced by a collection of [[unitary matrix|unitary matrices]] that map the Hilbert space to itself.&amp;lt;ref name=&amp;quot;Deutsch1985&amp;quot; /&amp;gt;&lt;br /&gt;
&lt;br /&gt;
我们可以通过类比确定有限自动机[[deterministic finite automaton]]到量子有限自动机[[quantum finite automaton]]的转化来理解经典图灵机到量子图灵机的转化。 他们的差异在于，经典图灵机讨论的状态被推广到了Hilbert空间中。Hilbert空间是'''完备的内积空间'''，是有限维欧几里得空间的一个推广。它不局限于实数的情形和有限的维数，但又不失完备性。在量子图灵机中转换函数被一组映射Hilbert空间到自身的酉矩阵[[unitary matrix|unitary matrices]]取代。&amp;lt;ref name=&amp;quot;Deutsch1985&amp;quot; /&amp;gt;&lt;br /&gt;
&lt;br /&gt;
经典图灵机的诞生是因为图灵想用机器来模拟用纸笔进行数学运算的过程，这样的过程可以被看作下列两种简单的动作：&lt;br /&gt;
&lt;br /&gt;
* 在纸带上写上或删除某个符号；&lt;br /&gt;
* 把笔尖从纸的一处移动到另一处；&lt;br /&gt;
&lt;br /&gt;
假设有一条纸带无限长，并且被划分为一个接一个的小格子，每个格子上包含一个来自有限字母表的符号，字母表中有一个特殊的符号表示空白。假设我们有一个执笔机器又称为读写头（'''HEAD），'''它本身也可以具有一个状态。就像人今天可能因为某件事心情很好，也可能因为另一件事情很抑郁一样，它的状态会随着它的遭遇所改变。更重要的是执笔机器当前关注的纸上的某个位置的符号和当前的状态决定了下一步的动作。在遇到停止状态&amp;lt;math&amp;gt;F&amp;lt;/math&amp;gt;之前执笔机器可以&lt;br /&gt;
&lt;br /&gt;
* 1. 写入（替换）或擦除当前符号；&lt;br /&gt;
* 2. 移动 '''HEAD'''， 'L'向左一步， 'R'向右一步或者'N'不移动；&lt;br /&gt;
* 3. 保持当前状态或者转到另一状态。&lt;br /&gt;
&lt;br /&gt;
That is, a classical Turing machine is described by  a 7-[[tuple]] &amp;lt;math&amp;gt;M = \langle Q, \Gamma, b, \Sigma, \delta, q_0, F \rangle&amp;lt;/math&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
经典图灵机可以被一个七元有序组所描述，&amp;lt;math&amp;gt;M = \langle Q, \Gamma, b, \Sigma, \delta, q_0, F \rangle&amp;lt;/math&amp;gt;。&lt;br /&gt;
&lt;br /&gt;
图灵机也可以拥有很多纸带，对于一个三纸带图灵机来说，它可以有一个纸带代表输入，一个纸带代表中间的运算过程，一个纸带代表输出。&lt;br /&gt;
&lt;br /&gt;
* The set of states &amp;lt;math&amp;gt;Q&amp;lt;/math&amp;gt; is replaced by a [[Hilbert space]].&lt;br /&gt;
&lt;br /&gt;
* The tape alphabet symbols &amp;lt;math&amp;gt;\Gamma&amp;lt;/math&amp;gt; are likewise replaced by a Hilbert space (usually a different Hilbert space than the set of states).&lt;br /&gt;
&lt;br /&gt;
* The blank symbol &amp;lt;math&amp;gt;b \in \Gamma&amp;lt;/math&amp;gt; corresponds to the zero-vector.&lt;br /&gt;
&lt;br /&gt;
* The input and output symbols &amp;lt;math&amp;gt;\Sigma&amp;lt;/math&amp;gt; are usually taken as a discrete set, as in the classical system; thus, neither the input nor output to a quantum machine need be a quantum system itself.&lt;br /&gt;
&lt;br /&gt;
* The [[State transition system|transition function]] &amp;lt;math&amp;gt;\delta : \Sigma \times Q  \otimes \Gamma \rightarrow \Sigma \times Q \otimes \Gamma \times \{L,R\}&amp;lt;/math&amp;gt; is a generalization of a [[transition monoid]], and is understood to be a collection of [[unitary matrix|unitary matrices]] that are [[automorphism]]s of the Hilbert space &amp;lt;math&amp;gt;Q&amp;lt;/math&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
* The initial state &amp;lt;math&amp;gt;q_0 \in Q&amp;lt;/math&amp;gt; may be either a [[mixed quantum state|mixed state]] or a [[pure state]].&lt;br /&gt;
&lt;br /&gt;
* The set &amp;lt;math&amp;gt;F&amp;lt;/math&amp;gt; of ''final'' or ''accepting states'' is a subspace of the Hilbert space &amp;lt;math&amp;gt;Q&amp;lt;/math&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
* &amp;lt;math&amp;gt;Q&amp;lt;/math&amp;gt; 非空有穷状态集合被推广到了Hilbert空间；&lt;br /&gt;
* &amp;lt;math&amp;gt;\Gamma&amp;lt;/math&amp;gt; 是非空有穷输入字母表，其中不包含特殊的空白符也被推广到了Hilbert空间；&lt;br /&gt;
* &amp;lt;math&amp;gt;b \in \Gamma&amp;lt;/math&amp;gt; 为''空白符''，也是唯一允许出现无限次的字符；&lt;br /&gt;
* 输入和输出符号 &amp;lt;math&amp;gt;\Sigma&amp;lt;/math&amp;gt;通常是一个离散集。和经典图灵机的输入输出符号一样，它们不需要是一个量子系统。&lt;br /&gt;
* &amp;lt;math&amp;gt;\delta : \Sigma \times Q  \otimes \Gamma \rightarrow \Sigma \times Q \otimes \Gamma \times \{L,R\}&amp;lt;/math&amp;gt;是转移函数[[State transition system|transition function]]被推广到了Hilbert空间。我们也可以理解它们为一些在Hilbert空间中自同构的酉矩阵[[unitary matrix|unitary matrices]] 。&lt;br /&gt;
* &amp;lt;math&amp;gt;q_0 \in Q&amp;lt;/math&amp;gt;是起始状态，它可以是几种状态的混合也可以是一种状态；&lt;br /&gt;
* 停止状态&amp;lt;math&amp;gt;F&amp;lt;/math&amp;gt;是&amp;lt;math&amp;gt;Q&amp;lt;/math&amp;gt;的子集。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The above is merely a sketch of a quantum Turing machine, rather than its formal definition, as it leaves vague several important details: for example, how often a [[quantum measurement|measurement]] is performed; see for example, the difference between a measure-once and a measure-many QFA.  This question of measurement affects the way in which writes to the output tape are defined.&lt;br /&gt;
&lt;br /&gt;
以上只是一个量子图灵机的草图，而不是它的正式定义，因为它的一些重要细节仍然定义模糊：例如，我们以什么样的频率执行对于状态的观测；什么是一次观测量子有限自动机和多次观测量子有限自动机 QFA 之间的区别。这些观测问题会影响我们如何定义写入和输出纸带的方式。&lt;br /&gt;
&lt;br /&gt;
==历史==&lt;br /&gt;
&lt;br /&gt;
In 1980 and 1982, physicist [[Paul Benioff]] published papers&amp;lt;ref name=&amp;quot;:0&amp;quot;&amp;gt;{{cite journal |last1=Benioff | first1=Paul | title=The computer as a physical system: A microscopic quantum mechanical Hamiltonian model of computers as represented by Turing machines | journal=Journal of Statistical Physics |volume=22 | issue=5 | pages=563–591 | year=1980 | doi=10.1007/bf01011339|bibcode=1980JSP....22..563B }}&amp;lt;/ref&amp;gt;&amp;lt;ref name=&amp;quot;:1&amp;quot;&amp;gt;{{Cite journal | doi=10.1007/BF01342185 | last1=Benioff | first1=P. | title=Quantum mechanical hamiltonian models of turing machines | journal=Journal of Statistical Physics | volume=29 | issue=3 | pages=515–546 | year=1982|bibcode=1982JSP....29..515B }}&amp;lt;/ref&amp;gt; that first described a quantum mechanical model of [[Turing machines]]. A 1985 article written by Oxford University physicist [[David Deutsch]] further developed the idea of quantum computers by suggesting [[quantum gate]]s could function in a similar fashion to traditional digital computing [[Binary numeral system|binary]] [[logic gates]].&amp;lt;ref name=&amp;quot;Deutsch1985&amp;quot;&amp;gt;{{cite journal|last=Deutsch|first=David|author-link=David Deutsch|date=July 1985|title=Quantum theory, the Church-Turing principle and the universal quantum computer|url=http://www.ceid.upatras.gr/tech_news/papers/quantum_theory.pdf|url-status=dead|journal=[[Proceedings of the Royal Society A]]|volume=400|issue=1818|pages=97–117|bibcode=1985RSPSA.400...97D|doi=10.1098/rspa.1985.0070|archiveurl=https://web.archive.org/web/20081123183419/http://www.ceid.upatras.gr/tech_news/papers/quantum_theory.pdf|archivedate=2008-11-23|citeseerx=10.1.1.41.2382}}&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
物理学家 Paul Benioff 在1980 年和 1982 年发表的论文中，首次描述了图灵机的量子力学模型。&amp;lt;ref name=&amp;quot;:0&amp;quot; /&amp;gt;&amp;lt;ref name=&amp;quot;:1&amp;quot; /&amp;gt; 牛津大学物理学家 David Deutsch 在 1985 年撰写的一篇文章中进一步发展了量子计算机的概念，他提议量子门[[quantum gate]]应该以类似于传统数字计算二进制逻辑门的方式运行。&amp;lt;ref name=&amp;quot;Deutsch1985&amp;quot; /&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Iriyama, [[Masanori Ohya|Ohya]], and Volovich have developed a model of a ''linear quantum Turing machine'' (LQTM).  This is a generalization of a classical QTM that has mixed states and that allows irreversible transition functions.  These allow the representation of quantum measurements without classical outcomes.&amp;lt;ref name=&amp;quot;:2&amp;quot;&amp;gt;{{cite journal|title=Classically-Controlled Quantum Computation|date=2007-04-04|pages=601–620|author1=Simon Perdrix|author2=Philippe Jorrand|volume=16|journal=Math. Struct. In Comp. Science|arxiv=quant-ph/0407008|doi=10.1017/S096012950600538X|issue=4}} also {{cite journal|title=Classically-Controlled Quantum Computation|author=Simon Perdrix and Philippe Jorrand|url=http://dcm-workshop.org.uk./2005/dcm-draft-proceedings.pdf|year=2006|pages=601–620|journal=Math. Struct. In Comp. Science|volume=16|doi=10.1017/S096012950600538X|issue=4|citeseerx=10.1.1.252.1823}}&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
Iriyama、Ohya 和 Volovich 开发了线性量子图灵机 (LQTM) 模型。他们对具有混合状态并允许不可逆转换函数的量子图灵机进行了延伸。允许了没有经典结果的情况对量子测量在。&amp;lt;ref name=&amp;quot;:2&amp;quot; /&amp;gt;&lt;br /&gt;
&lt;br /&gt;
A ''quantum Turing machine with [[postselection]]'' was defined by [[Scott Aaronson]], who showed that the class of polynomial time on such a machine ([[PostBQP]]) is equal to the classical complexity class [[PP (complexity)|PP]].&amp;lt;ref name=&amp;quot;:3&amp;quot;&amp;gt;{{cite journal|last=Aaronson|first=Scott|year=2005|title=Quantum computing, postselection, and probabilistic polynomial-time|journal=[[Proceedings of the Royal Society A]]|volume=461|issue=2063|pages=3473–3482|doi=10.1098/rspa.2005.1546|bibcode = 2005RSPSA.461.3473A |arxiv=quant-ph/0412187}}  Preprint available at [https://arxiv.org/abs/quant-ph/0412187]&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
Scott Aaronson 定义了具有后选择功能的量子图灵机，他证明了这种机器上的时间复杂度类 (PostBQP) 等于经典复杂度 PP。&amp;lt;ref name=&amp;quot;:3&amp;quot; /&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
== 相关内容 ==&lt;br /&gt;
&lt;br /&gt;
Category:Turing machine&lt;br /&gt;
&lt;br /&gt;
类别: 图灵机&lt;br /&gt;
&lt;br /&gt;
*[[Quantum simulator#Solving physics problems|Quantum simulator § Solving physics problems]]&lt;br /&gt;
&lt;br /&gt;
范畴: 量子复杂性理论&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:Quantum Turing machine]]. Its edit history can be viewed at [[量子图灵机/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>Tueryeye</name></author>
	</entry>
	<entry>
		<id>https://wiki.swarma.org/index.php?title=%E9%87%8F%E5%AD%90%E5%9B%BE%E7%81%B5%E6%9C%BA&amp;diff=29901</id>
		<title>量子图灵机</title>
		<link rel="alternate" type="text/html" href="https://wiki.swarma.org/index.php?title=%E9%87%8F%E5%AD%90%E5%9B%BE%E7%81%B5%E6%9C%BA&amp;diff=29901"/>
		<updated>2022-03-31T04:15:33Z</updated>

		<summary type="html">&lt;p&gt;Tueryeye：翻译完成&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;此词条暂由彩云小译翻译，翻译字数共319，未经人工整理和审校，带来阅读不便，请见谅。&lt;br /&gt;
&lt;br /&gt;
{{Short description|Model of quantum computation}}&lt;br /&gt;
&lt;br /&gt;
{{Turing}}&lt;br /&gt;
&lt;br /&gt;
&amp;lt;!-- Basic definition --&amp;gt;&lt;br /&gt;
== 基础定义 ==&lt;br /&gt;
A '''quantum Turing machine''' ('''QTM''') or '''universal quantum computer''' is an [[abstract machine]] used to model the effects of a [[quantum computer]].  It provides a simple model that captures all of the power of quantum computation—that is, any [[quantum algorithm]] can be expressed formally as a particular quantum Turing machine. However, the computationally equivalent [[quantum circuit]] is a more common model.&amp;lt;ref name=&amp;quot;equivalence&amp;quot;&amp;gt;{{cite conference|author=[[Andrew Yao]]|title=Quantum circuit complexity|conference=34th Annual Symposium on Foundations of Computer Science|pages=352–361|year=1993}}&amp;lt;/ref&amp;gt;&amp;lt;ref name=&amp;quot;newequivalence&amp;quot;&amp;gt;{{cite arXiv|eprint=1808.01701|author1=Abel Molina|author2=John Watrous|author-link2=John Watrous (computer scientist)|title=Revisiting the simulation of quantum Turing machines by quantum circuits|date=2018|class=cs.CC}}&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
量子图灵机计算机(QTM)又称为通用量子计算机是一种用来模拟量子计算机效果的抽象机器。虽然它是一个简单的模型，但它能展现出量子计算的所有威力。就像经典图灵机可以模拟人类所能进行的任何计算过程一样，量子图灵机可以描述任何量子算法。尽管说提供等效计算能力的量子电路是一种更常用的模型。&amp;lt;ref name=&amp;quot;equivalence&amp;quot; /&amp;gt;&amp;lt;ref name=&amp;quot;newequivalence&amp;quot; /&amp;gt;&lt;br /&gt;
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&lt;br /&gt;
&amp;lt;!-- Relation to classical computation --&amp;gt;&lt;br /&gt;
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== 与经典计算的关系 ==&lt;br /&gt;
Quantum Turing machines can be related to classical and probabilistic Turing machines in a framework based on [[Stochastic matrix|transition matrices]]. That is, a matrix can be specified whose product with the matrix representing a classical or probabilistic machine provides the quantum probability matrix representing the quantum machine. This was shown by [[Lance Fortnow]].&amp;lt;ref name=&amp;quot;transition&amp;quot;&amp;gt;{{cite journal|author=Fortnow|first=Lance|author-link=Lance Fortnow|year=2003|title=One Complexity Theorist's View of Quantum Computing|url=|journal=Theoretical Computer Science|volume=292|issue=3|pages=597–610|doi=10.1016/S0304-3975(01)00377-2|via=|arxiv=quant-ph/0003035}}&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
通过过渡矩阵，量子图灵机可以与经典图灵机和概率图灵机相关联。兰斯 · 福特诺（Lance Fortnow）证明，量子图灵机的量子概率矩阵可以被拆解成是指定矩阵与经典或概率图灵机的矩阵的乘积。&amp;lt;ref name=&amp;quot;transition&amp;quot; /&amp;gt;&lt;br /&gt;
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== 非正式草图定义 ==&lt;br /&gt;
{{Unsolved|physics|Is a [[universal quantum computer]] sufficient to [[Algorithmic efficiency|efficiently]] [[Dynamical simulation|simulate]] an arbitrary physical system?}}&lt;br /&gt;
&lt;br /&gt;
A way of understanding the quantum Turing machine (QTM) is that it generalizes the classical [[Turing machine]] (TM) in the same way that the [[quantum finite automaton]] (QFA) generalizes the [[deterministic finite automaton]] (DFA).  In essence, the internal states of a classical TM are replaced by [[pure state|pure]] or [[mixed quantum state|mixed states]] in a Hilbert space; the transition function is replaced by a collection of [[unitary matrix|unitary matrices]] that map the Hilbert space to itself.&amp;lt;ref name=&amp;quot;Deutsch1985&amp;quot; /&amp;gt;&lt;br /&gt;
&lt;br /&gt;
我们可以通过类比确定有限自动机（[[deterministic finite automaton]]）到量子有限自动机（[[quantum finite automaton]]）的转化来理解经典图灵机到量子图灵机的转化。 他们的差异在于，经典图灵机讨论的状态被推广到了希尔伯特空间（Hilbert space）中。希尔伯特空间是'''完备的内积空间'''，是有限维欧几里得空间的一个推广。它不局限于实数的情形和有限的维数，但又不失完备性。在量子图灵机中转换函数被一组映射希尔伯特空间到自身的酉矩阵取代。&amp;lt;ref name=&amp;quot;Deutsch1985&amp;quot; /&amp;gt;&lt;br /&gt;
&lt;br /&gt;
经典图灵机的诞生是因为图灵想用机器来模拟用纸笔进行数学运算的过程，这样的过程可以被看作下列两种简单的动作：&lt;br /&gt;
&lt;br /&gt;
* 在纸带上写上或删除某个符号；&lt;br /&gt;
* 把笔尖从纸的一处移动到另一处；&lt;br /&gt;
&lt;br /&gt;
假设有一条纸带无限长，并且被划分为一个接一个的小格子，每个格子上包含一个来自有限字母表的符号，字母表中有一个特殊的符号表示空白。假设我们有一个执笔机器又称为读写头（'''HEAD），'''它本身也可以具有一个状态。就像人今天可能因为某件事心情很好，也可能因为另一件事情很抑郁一样，它的状态会随着它的遭遇所改变。更重要的是执笔机器当前关注的纸上的某个位置的符号和当前的状态决定了下一步的动作。在遇到停止状态&amp;lt;math&amp;gt;F&amp;lt;/math&amp;gt;之前执笔机器可以&lt;br /&gt;
&lt;br /&gt;
* 1. 写入（替换）或擦除当前符号；&lt;br /&gt;
* 2. 移动 '''HEAD'''， 'L'向左一步， 'R'向右一步或者'N'不移动；&lt;br /&gt;
* 3. 保持当前状态或者转到另一状态。&lt;br /&gt;
&lt;br /&gt;
That is, a classical Turing machine is described by  a 7-[[tuple]] &amp;lt;math&amp;gt;M = \langle Q, \Gamma, b, \Sigma, \delta, q_0, F \rangle&amp;lt;/math&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
经典图灵机可以被一个七元有序组所描述，&amp;lt;math&amp;gt;M = \langle Q, \Gamma, b, \Sigma, \delta, q_0, F \rangle&amp;lt;/math&amp;gt;。&lt;br /&gt;
&lt;br /&gt;
图灵机也可以拥有很多纸带，对于一个三纸带图灵机来说，它可以有一个纸带代表输入，一个纸带代表中间的运算过程，一个纸带代表输出。&lt;br /&gt;
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* The set of states &amp;lt;math&amp;gt;Q&amp;lt;/math&amp;gt; is replaced by a [[Hilbert space]].&lt;br /&gt;
&lt;br /&gt;
* The tape alphabet symbols &amp;lt;math&amp;gt;\Gamma&amp;lt;/math&amp;gt; are likewise replaced by a Hilbert space (usually a different Hilbert space than the set of states).&lt;br /&gt;
&lt;br /&gt;
* The blank symbol &amp;lt;math&amp;gt;b \in \Gamma&amp;lt;/math&amp;gt; corresponds to the zero-vector.&lt;br /&gt;
&lt;br /&gt;
* The input and output symbols &amp;lt;math&amp;gt;\Sigma&amp;lt;/math&amp;gt; are usually taken as a discrete set, as in the classical system; thus, neither the input nor output to a quantum machine need be a quantum system itself.&lt;br /&gt;
&lt;br /&gt;
* The [[State transition system|transition function]] &amp;lt;math&amp;gt;\delta : \Sigma \times Q  \otimes \Gamma \rightarrow \Sigma \times Q \otimes \Gamma \times \{L,R\}&amp;lt;/math&amp;gt; is a generalization of a [[transition monoid]], and is understood to be a collection of [[unitary matrix|unitary matrices]] that are [[automorphism]]s of the Hilbert space &amp;lt;math&amp;gt;Q&amp;lt;/math&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
* The initial state &amp;lt;math&amp;gt;q_0 \in Q&amp;lt;/math&amp;gt; may be either a [[mixed quantum state|mixed state]] or a [[pure state]].&lt;br /&gt;
&lt;br /&gt;
* The set &amp;lt;math&amp;gt;F&amp;lt;/math&amp;gt; of ''final'' or ''accepting states'' is a subspace of the Hilbert space &amp;lt;math&amp;gt;Q&amp;lt;/math&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
* &amp;lt;math&amp;gt;Q&amp;lt;/math&amp;gt; 非空有穷状态集合被推广到了希尔伯特空间；&lt;br /&gt;
* &amp;lt;math&amp;gt;\Gamma&amp;lt;/math&amp;gt; 是非空有穷输入字母表，其中不包含特殊的空白符也被推广到了希尔伯特空间；&lt;br /&gt;
* &amp;lt;math&amp;gt;b \in \Gamma&amp;lt;/math&amp;gt; 为''空白符''，也是唯一允许出现无限次的字符；&lt;br /&gt;
* 输入和输出符号 &amp;lt;math&amp;gt;\Sigma&amp;lt;/math&amp;gt;通常是一个离散集。和经典图灵机的输入输出符号一样，它们不需要是一个量子系统。&lt;br /&gt;
* &amp;lt;math&amp;gt;\delta : \Sigma \times Q  \otimes \Gamma \rightarrow \Sigma \times Q \otimes \Gamma \times \{L,R\}&amp;lt;/math&amp;gt;是转移函数被推广到了希尔伯特空间。我们也可以理解它们为一些在希尔伯特空间中自同构的酉矩阵。&lt;br /&gt;
* &amp;lt;math&amp;gt;q_0 \in Q&amp;lt;/math&amp;gt;是起始状态，它可以是几种状态的混合也可以是一种状态；&lt;br /&gt;
* 停止状态&amp;lt;math&amp;gt;F&amp;lt;/math&amp;gt;是&amp;lt;math&amp;gt;Q&amp;lt;/math&amp;gt;的子集。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The above is merely a sketch of a quantum Turing machine, rather than its formal definition, as it leaves vague several important details: for example, how often a [[quantum measurement|measurement]] is performed; see for example, the difference between a measure-once and a measure-many QFA.  This question of measurement affects the way in which writes to the output tape are defined.&lt;br /&gt;
&lt;br /&gt;
以上只是一个量子图灵机的草图，而不是它的正式定义，因为它的一些重要细节仍然定义模糊：例如，我们以什么样的频率执行对于状态的观测；什么是一次观测量子有限自动机和多次观测量子有限自动机 QFA 之间的区别。这些观测问题会影响我们如何定义写入和输出纸带的方式。&lt;br /&gt;
&lt;br /&gt;
==历史==&lt;br /&gt;
&lt;br /&gt;
In 1980 and 1982, physicist [[Paul Benioff]] published papers&amp;lt;ref name=&amp;quot;:0&amp;quot;&amp;gt;{{cite journal |last1=Benioff | first1=Paul | title=The computer as a physical system: A microscopic quantum mechanical Hamiltonian model of computers as represented by Turing machines | journal=Journal of Statistical Physics |volume=22 | issue=5 | pages=563–591 | year=1980 | doi=10.1007/bf01011339|bibcode=1980JSP....22..563B }}&amp;lt;/ref&amp;gt;&amp;lt;ref name=&amp;quot;:1&amp;quot;&amp;gt;{{Cite journal | doi=10.1007/BF01342185 | last1=Benioff | first1=P. | title=Quantum mechanical hamiltonian models of turing machines | journal=Journal of Statistical Physics | volume=29 | issue=3 | pages=515–546 | year=1982|bibcode=1982JSP....29..515B }}&amp;lt;/ref&amp;gt; that first described a quantum mechanical model of [[Turing machines]]. A 1985 article written by Oxford University physicist [[David Deutsch]] further developed the idea of quantum computers by suggesting [[quantum gate]]s could function in a similar fashion to traditional digital computing [[Binary numeral system|binary]] [[logic gates]].&amp;lt;ref name=&amp;quot;Deutsch1985&amp;quot;&amp;gt;{{cite journal|last=Deutsch|first=David|author-link=David Deutsch|date=July 1985|title=Quantum theory, the Church-Turing principle and the universal quantum computer|url=http://www.ceid.upatras.gr/tech_news/papers/quantum_theory.pdf|url-status=dead|journal=[[Proceedings of the Royal Society A]]|volume=400|issue=1818|pages=97–117|bibcode=1985RSPSA.400...97D|doi=10.1098/rspa.1985.0070|archiveurl=https://web.archive.org/web/20081123183419/http://www.ceid.upatras.gr/tech_news/papers/quantum_theory.pdf|archivedate=2008-11-23|citeseerx=10.1.1.41.2382}}&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
物理学家 Paul Benioff 在1980 年和 1982 年发表的论文中，首次描述了图灵机的量子力学模型。&amp;lt;ref name=&amp;quot;:0&amp;quot; /&amp;gt;&amp;lt;ref name=&amp;quot;:1&amp;quot; /&amp;gt; 牛津大学物理学家 David Deutsch 在 1985 年撰写的一篇文章中进一步发展了量子计算机的概念，他提议量子门应该以类似于传统数字计算二进制逻辑门的方式运行。&amp;lt;ref name=&amp;quot;Deutsch1985&amp;quot; /&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Iriyama, [[Masanori Ohya|Ohya]], and Volovich have developed a model of a ''linear quantum Turing machine'' (LQTM).  This is a generalization of a classical QTM that has mixed states and that allows irreversible transition functions.  These allow the representation of quantum measurements without classical outcomes.&amp;lt;ref name=&amp;quot;:2&amp;quot;&amp;gt;{{cite journal|title=Classically-Controlled Quantum Computation|date=2007-04-04|pages=601–620|author1=Simon Perdrix|author2=Philippe Jorrand|volume=16|journal=Math. Struct. In Comp. Science|arxiv=quant-ph/0407008|doi=10.1017/S096012950600538X|issue=4}} also {{cite journal|title=Classically-Controlled Quantum Computation|author=Simon Perdrix and Philippe Jorrand|url=http://dcm-workshop.org.uk./2005/dcm-draft-proceedings.pdf|year=2006|pages=601–620|journal=Math. Struct. In Comp. Science|volume=16|doi=10.1017/S096012950600538X|issue=4|citeseerx=10.1.1.252.1823}}&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
Iriyama、Ohya 和 Volovich 开发了线性量子图灵机 (LQTM) 模型。他们对具有混合状态并允许不可逆转换函数的量子图灵机进行了延伸。允许了没有经典结果的情况对量子测量在。&amp;lt;ref name=&amp;quot;:2&amp;quot; /&amp;gt;&lt;br /&gt;
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&lt;br /&gt;
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&lt;br /&gt;
A ''quantum Turing machine with [[postselection]]'' was defined by [[Scott Aaronson]], who showed that the class of polynomial time on such a machine ([[PostBQP]]) is equal to the classical complexity class [[PP (complexity)|PP]].&amp;lt;ref name=&amp;quot;:3&amp;quot;&amp;gt;{{cite journal|last=Aaronson|first=Scott|year=2005|title=Quantum computing, postselection, and probabilistic polynomial-time|journal=[[Proceedings of the Royal Society A]]|volume=461|issue=2063|pages=3473–3482|doi=10.1098/rspa.2005.1546|bibcode = 2005RSPSA.461.3473A |arxiv=quant-ph/0412187}}  Preprint available at [https://arxiv.org/abs/quant-ph/0412187]&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
Scott Aaronson 定义了具有后选择功能的量子图灵机，他证明了这种机器上的时间复杂度类 (PostBQP) 等于经典复杂度 PP。&amp;lt;ref name=&amp;quot;:3&amp;quot; /&amp;gt;&lt;br /&gt;
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== 相关内容 ==&lt;br /&gt;
&lt;br /&gt;
Category:Turing machine&lt;br /&gt;
&lt;br /&gt;
类别: 图灵机&lt;br /&gt;
&lt;br /&gt;
*[[Quantum simulator#Solving physics problems|Quantum simulator § Solving physics problems]]&lt;br /&gt;
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Category:Quantum complexity theory&lt;br /&gt;
&lt;br /&gt;
范畴: 量子复杂性理论&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:Quantum Turing machine]]. Its edit history can be viewed at [[量子图灵机/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>Tueryeye</name></author>
	</entry>
	<entry>
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		<title>量子图灵机</title>
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		<updated>2022-03-31T03:31:46Z</updated>

		<summary type="html">&lt;p&gt;Tueryeye：&lt;/p&gt;
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&lt;div&gt;此词条暂由彩云小译翻译，翻译字数共319，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|Model of quantum computation}}&lt;br /&gt;
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{{Turing}}&lt;br /&gt;
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&amp;lt;!-- Basic definition --&amp;gt;&lt;br /&gt;
=== 基础定义 ===&lt;br /&gt;
A '''quantum Turing machine''' ('''QTM''') or '''universal quantum computer''' is an [[abstract machine]] used to model the effects of a [[quantum computer]].  It provides a simple model that captures all of the power of quantum computation—that is, any [[quantum algorithm]] can be expressed formally as a particular quantum Turing machine. However, the computationally equivalent [[quantum circuit]] is a more common model.&amp;lt;ref name=&amp;quot;equivalence&amp;quot;&amp;gt;{{cite conference|author=[[Andrew Yao]]|title=Quantum circuit complexity|conference=34th Annual Symposium on Foundations of Computer Science|pages=352–361|year=1993}}&amp;lt;/ref&amp;gt;&amp;lt;ref name=&amp;quot;newequivalence&amp;quot;&amp;gt;{{cite arXiv|eprint=1808.01701|author1=Abel Molina|author2=John Watrous|author-link2=John Watrous (computer scientist)|title=Revisiting the simulation of quantum Turing machines by quantum circuits|date=2018|class=cs.CC}}&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
量子图灵机计算机(QTM)又称为通用量子计算机是一种用来模拟量子计算机效果的抽象机器。虽然它是一个简单的模型，但它能展现出量子计算的所有威力，因为任何量子算法都可以被形式化地表示为一个特定的量子图灵机。尽管说提供等效计算能力的量子电路是一种更常用的模型。&amp;lt;ref name=&amp;quot;equivalence&amp;quot; /&amp;gt;&amp;lt;ref name=&amp;quot;newequivalence&amp;quot; /&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;!-- Relation to classical computation --&amp;gt;&lt;br /&gt;
&lt;br /&gt;
=== 与经典计算的关系 ===&lt;br /&gt;
Quantum Turing machines can be related to classical and probabilistic Turing machines in a framework based on [[Stochastic matrix|transition matrices]]. That is, a matrix can be specified whose product with the matrix representing a classical or probabilistic machine provides the quantum probability matrix representing the quantum machine. This was shown by [[Lance Fortnow]].&amp;lt;ref name=&amp;quot;transition&amp;quot;&amp;gt;{{cite journal|author=Fortnow|first=Lance|author-link=Lance Fortnow|year=2003|title=One Complexity Theorist's View of Quantum Computing|url=|journal=Theoretical Computer Science|volume=292|issue=3|pages=597–610|doi=10.1016/S0304-3975(01)00377-2|via=|arxiv=quant-ph/0003035}}&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
Quantum Turing machines can be related to classical and probabilistic Turing machines in a framework based on transition matrices. That is, a matrix can be specified whose product with the matrix representing a classical or probabilistic machine provides the quantum probability matrix representing the quantum machine. This was shown by Lance Fortnow.&lt;br /&gt;
&lt;br /&gt;
通过过渡矩阵，量子图灵机可以与经典图灵机和概率图灵机相关联。兰斯 · 福特诺（Lance Fortnow）证明，量子图灵机的量子概率矩阵可以被拆解成是指定矩阵与经典或概率图灵机的矩阵的乘积。&amp;lt;ref name=&amp;quot;transition&amp;quot; /&amp;gt;&lt;br /&gt;
&lt;br /&gt;
=== 通俗定义 ===&lt;br /&gt;
{{Unsolved|physics|Is a [[universal quantum computer]] sufficient to [[Algorithmic efficiency|efficiently]] [[Dynamical simulation|simulate]] an arbitrary physical system?}}&lt;br /&gt;
&lt;br /&gt;
A way of understanding the quantum Turing machine (QTM) is that it generalizes the classical [[Turing machine]] (TM) in the same way that the [[quantum finite automaton]] (QFA) generalizes the [[deterministic finite automaton]] (DFA).  In essence, the internal states of a classical TM are replaced by [[pure state|pure]] or [[mixed quantum state|mixed states]] in a Hilbert space; the transition function is replaced by a collection of [[unitary matrix|unitary matrices]] that map the Hilbert space to itself.&amp;lt;ref name=&amp;quot;Deutsch1985&amp;quot; /&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
我们可以通过类比确定有限自动机（[[deterministic finite automaton]]）到量子有限自动机（[[quantum finite automaton]]）的转化来理解经典图灵机到量子图灵机的转化。 他们的差异在于，经典图灵机讨论的状态被推广到了希尔伯特空间（Hilbert space）中。希尔伯特空间是'''完备的内积空间'''，是有限维欧几里得空间的一个推广。它不局限于实数的情形和有限的维数，但又不失完备性。转换函数被一组映射 Hilbert 空间到自身的酉矩阵取代。&amp;lt;ref name=&amp;quot;Deutsch1985&amp;quot; /&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
That is, a classical Turing machine is described by  a 7-[[tuple]] &amp;lt;math&amp;gt;M = \langle Q, \Gamma, b, \Sigma, \delta, q_0, F \rangle&amp;lt;/math&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
经典图灵机可以被一个七元有序组所描述，&amp;lt;math&amp;gt;M = \langle Q, \Gamma, b, \Sigma, \delta, q_0, F \rangle&amp;lt;/math&amp;gt;。&lt;br /&gt;
&lt;br /&gt;
Iriyama, Ohya, and Volovich have developed a model of a linear quantum Turing machine (LQTM).  This is a generalization of a classical QTM that has mixed states and that allows irreversible transition functions.  These allow the representation of quantum measurements without classical outcomes.&lt;br /&gt;
&lt;br /&gt;
Iriyama、 Ohya 和 Volovich 开发了一个线性量子图灵机模型(LQTM)。这是一个具有混合状态并允许不可逆转换函数的经典 QTM 的推广。这使得量子测量可以在没有经典结果的情况下进行表示。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
For a three-tape quantum Turing machine (one tape holding the input, a second tape holding intermediate calculation results, and a third tape holding output):&lt;br /&gt;
&lt;br /&gt;
A quantum Turing machine with postselection was defined by Scott Aaronson, who showed that the class of polynomial time on such a machine (PostBQP) is equal to the classical complexity class PP.&lt;br /&gt;
&lt;br /&gt;
一个具有后选择的量子图灵机由 Scott Aaronson 定义，他证明了这样一个机器上的多项式时间类(PostBQP)等于经典的复杂性类 PP。&lt;br /&gt;
&lt;br /&gt;
* The set of states &amp;lt;math&amp;gt;Q&amp;lt;/math&amp;gt; is replaced by a [[Hilbert space]].&lt;br /&gt;
&lt;br /&gt;
* The tape alphabet symbols &amp;lt;math&amp;gt;\Gamma&amp;lt;/math&amp;gt; are likewise replaced by a Hilbert space (usually a different Hilbert space than the set of states).&lt;br /&gt;
&lt;br /&gt;
* The blank symbol &amp;lt;math&amp;gt;b \in \Gamma&amp;lt;/math&amp;gt; corresponds to the zero-vector.&lt;br /&gt;
&lt;br /&gt;
* The input and output symbols &amp;lt;math&amp;gt;\Sigma&amp;lt;/math&amp;gt; are usually taken as a discrete set, as in the classical system; thus, neither the input nor output to a quantum machine need be a quantum system itself.&lt;br /&gt;
&lt;br /&gt;
* The [[State transition system|transition function]] &amp;lt;math&amp;gt;\delta : \Sigma \times Q  \otimes \Gamma \rightarrow \Sigma \times Q \otimes \Gamma \times \{L,R\}&amp;lt;/math&amp;gt; is a generalization of a [[transition monoid]], and is understood to be a collection of [[unitary matrix|unitary matrices]] that are [[automorphism]]s of the Hilbert space &amp;lt;math&amp;gt;Q&amp;lt;/math&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
* The initial state &amp;lt;math&amp;gt;q_0 \in Q&amp;lt;/math&amp;gt; may be either a [[mixed quantum state|mixed state]] or a [[pure state]].&lt;br /&gt;
&lt;br /&gt;
* The set &amp;lt;math&amp;gt;F&amp;lt;/math&amp;gt; of ''final'' or ''accepting states'' is a subspace of the Hilbert space &amp;lt;math&amp;gt;Q&amp;lt;/math&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The above is merely a sketch of a quantum Turing machine, rather than its formal definition, as it leaves vague several important details: for example, how often a [[quantum measurement|measurement]] is performed; see for example, the difference between a measure-once and a measure-many QFA.  This question of measurement affects the way in which writes to the output tape are defined.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==History==&lt;br /&gt;
&lt;br /&gt;
In 1980 and 1982, physicist [[Paul Benioff]] published papers&amp;lt;ref&amp;gt;{{cite journal |last1=Benioff | first1=Paul | title=The computer as a physical system: A microscopic quantum mechanical Hamiltonian model of computers as represented by Turing machines | journal=Journal of Statistical Physics |volume=22 | issue=5 | pages=563–591 | year=1980 | doi=10.1007/bf01011339|bibcode=1980JSP....22..563B }}&amp;lt;/ref&amp;gt;&amp;lt;ref&amp;gt;{{Cite journal | doi=10.1007/BF01342185 | last1=Benioff | first1=P. | title=Quantum mechanical hamiltonian models of turing machines | journal=Journal of Statistical Physics | volume=29 | issue=3 | pages=515–546 | year=1982|bibcode=1982JSP....29..515B }}&amp;lt;/ref&amp;gt; that first described a quantum mechanical model of [[Turing machines]]. A 1985 article written by Oxford University physicist [[David Deutsch]] further developed the idea of quantum computers by suggesting [[quantum gate]]s could function in a similar fashion to traditional digital computing [[Binary numeral system|binary]] [[logic gates]].&amp;lt;ref name=&amp;quot;Deutsch1985&amp;quot;&amp;gt;{{cite journal|last=Deutsch|first=David|author-link=David Deutsch|date=July 1985|title=Quantum theory, the Church-Turing principle and the universal quantum computer|url=http://www.ceid.upatras.gr/tech_news/papers/quantum_theory.pdf|url-status=dead|journal=[[Proceedings of the Royal Society A]]|volume=400|issue=1818|pages=97–117|bibcode=1985RSPSA.400...97D|doi=10.1098/rspa.1985.0070|archiveurl=https://web.archive.org/web/20081123183419/http://www.ceid.upatras.gr/tech_news/papers/quantum_theory.pdf|archivedate=2008-11-23|citeseerx=10.1.1.41.2382}}&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Iriyama, [[Masanori Ohya|Ohya]], and Volovich have developed a model of a ''linear quantum Turing machine'' (LQTM).  This is a generalization of a classical QTM that has mixed states and that allows irreversible transition functions.  These allow the representation of quantum measurements without classical outcomes.&amp;lt;ref&amp;gt;{{cite journal|title=Classically-Controlled Quantum Computation|date=2007-04-04|pages=601–620|author1=Simon Perdrix|author2=Philippe Jorrand|volume=16|journal=Math. Struct. In Comp. Science|arxiv=quant-ph/0407008|doi=10.1017/S096012950600538X|issue=4}} also {{cite journal|title=Classically-Controlled Quantum Computation|author=Simon Perdrix and Philippe Jorrand|url=http://dcm-workshop.org.uk./2005/dcm-draft-proceedings.pdf|year=2006|pages=601–620|journal=Math. Struct. In Comp. Science|volume=16|doi=10.1017/S096012950600538X|issue=4|citeseerx=10.1.1.252.1823}}&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
A ''quantum Turing machine with [[postselection]]'' was defined by [[Scott Aaronson]], who showed that the class of polynomial time on such a machine ([[PostBQP]]) is equal to the classical complexity class [[PP (complexity)|PP]].&amp;lt;ref&amp;gt;{{cite journal|last=Aaronson|first=Scott|year=2005|title=Quantum computing, postselection, and probabilistic polynomial-time|journal=[[Proceedings of the Royal Society A]]|volume=461|issue=2063|pages=3473–3482|doi=10.1098/rspa.2005.1546|bibcode = 2005RSPSA.461.3473A |arxiv=quant-ph/0412187}}  Preprint available at [https://arxiv.org/abs/quant-ph/0412187]&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
== See also ==&lt;br /&gt;
&lt;br /&gt;
Category:Turing machine&lt;br /&gt;
&lt;br /&gt;
类别: 图灵机&lt;br /&gt;
&lt;br /&gt;
*[[Quantum simulator#Solving physics problems|Quantum simulator § Solving physics problems]]&lt;br /&gt;
&lt;br /&gt;
Category:Quantum complexity theory&lt;br /&gt;
&lt;br /&gt;
范畴: 量子复杂性理论&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:Quantum Turing machine]]. Its edit history can be viewed at [[量子图灵机/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>Tueryeye</name></author>
	</entry>
	<entry>
		<id>https://wiki.swarma.org/index.php?title=%E9%87%8F%E5%AD%90%E5%9B%BE%E7%81%B5%E6%9C%BA&amp;diff=29741</id>
		<title>量子图灵机</title>
		<link rel="alternate" type="text/html" href="https://wiki.swarma.org/index.php?title=%E9%87%8F%E5%AD%90%E5%9B%BE%E7%81%B5%E6%9C%BA&amp;diff=29741"/>
		<updated>2022-03-27T16:55:03Z</updated>

		<summary type="html">&lt;p&gt;Tueryeye：&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;此词条暂由彩云小译翻译，翻译字数共319，未经人工整理和审校，带来阅读不便，请见谅。&lt;br /&gt;
&lt;br /&gt;
{{Short description|Model of quantum computation}}&lt;br /&gt;
&lt;br /&gt;
{{Turing}}&lt;br /&gt;
&lt;br /&gt;
&amp;lt;!-- Basic definition --&amp;gt;&lt;br /&gt;
=== 基础定义 ===&lt;br /&gt;
A '''quantum Turing machine''' ('''QTM''') or '''universal quantum computer''' is an [[abstract machine]] used to model the effects of a [[quantum computer]].  It provides a simple model that captures all of the power of quantum computation—that is, any [[quantum algorithm]] can be expressed formally as a particular quantum Turing machine. However, the computationally equivalent [[quantum circuit]] is a more common model.&amp;lt;ref name=&amp;quot;equivalence&amp;quot;&amp;gt;{{cite conference|author=[[Andrew Yao]]|title=Quantum circuit complexity|conference=34th Annual Symposium on Foundations of Computer Science|pages=352–361|year=1993}}&amp;lt;/ref&amp;gt;&amp;lt;ref name=&amp;quot;newequivalence&amp;quot;&amp;gt;{{cite arXiv|eprint=1808.01701|author1=Abel Molina|author2=John Watrous|author-link2=John Watrous (computer scientist)|title=Revisiting the simulation of quantum Turing machines by quantum circuits|date=2018|class=cs.CC}}&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
量子图灵机计算机(QTM)又称为通用量子计算机是一种用来模拟量子计算机效果的抽象机器。它提供了一个简单的模型，但又能展现出量子计算的所有威力。也就是说，任何量子算法都可以被形式化地表示为一个特定的量子图灵机。提供等效计算能力的量子电路是一种比较常用的模型。&amp;lt;ref name=&amp;quot;equivalence&amp;quot; /&amp;gt;&amp;lt;ref name=&amp;quot;newequivalence&amp;quot; /&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;!-- Relation to classical computation --&amp;gt;&lt;br /&gt;
&lt;br /&gt;
=== 与经典计算的关系 ===&lt;br /&gt;
Quantum Turing machines can be related to classical and probabilistic Turing machines in a framework based on [[Stochastic matrix|transition matrices]]. That is, a matrix can be specified whose product with the matrix representing a classical or probabilistic machine provides the quantum probability matrix representing the quantum machine. This was shown by [[Lance Fortnow]].&amp;lt;ref name=&amp;quot;transition&amp;quot;&amp;gt;{{cite journal|author=Fortnow|first=Lance|author-link=Lance Fortnow|year=2003|title=One Complexity Theorist's View of Quantum Computing|url=|journal=Theoretical Computer Science|volume=292|issue=3|pages=597–610|doi=10.1016/S0304-3975(01)00377-2|via=|arxiv=quant-ph/0003035}}&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
Quantum Turing machines can be related to classical and probabilistic Turing machines in a framework based on transition matrices. That is, a matrix can be specified whose product with the matrix representing a classical or probabilistic machine provides the quantum probability matrix representing the quantum machine. This was shown by Lance Fortnow.&lt;br /&gt;
&lt;br /&gt;
通过转移矩阵，量子图灵机可以与经典图灵机和概率图灵机相关联。兰斯 · 福特诺（Lance Fortnow）证明，指定一个矩阵，其与经典或概率图灵机的矩阵的乘积提供了量子机器的量子概率矩阵。&amp;lt;ref name=&amp;quot;transition&amp;quot; /&amp;gt;&lt;br /&gt;
&lt;br /&gt;
=== 通俗定义 ===&lt;br /&gt;
{{Unsolved|physics|Is a [[universal quantum computer]] sufficient to [[Algorithmic efficiency|efficiently]] [[Dynamical simulation|simulate]] an arbitrary physical system?}}&lt;br /&gt;
&lt;br /&gt;
A way of understanding the quantum Turing machine (QTM) is that it generalizes the classical [[Turing machine]] (TM) in the same way that the [[quantum finite automaton]] (QFA) generalizes the [[deterministic finite automaton]] (DFA).  In essence, the internal states of a classical TM are replaced by [[pure state|pure]] or [[mixed quantum state|mixed states]] in a Hilbert space; the transition function is replaced by a collection of [[unitary matrix|unitary matrices]] that map the Hilbert space to itself.&amp;lt;ref name=&amp;quot;Deutsch1985&amp;quot; /&amp;gt;&lt;br /&gt;
&lt;br /&gt;
A way of understanding the quantum Turing machine (QTM) is that it generalizes the classical Turing machine (TM) in the same way that the quantum finite automaton (QFA) generalizes the deterministic finite automaton (DFA).  In essence, the internal states of a classical TM are replaced by pure or mixed states in a Hilbert space; the transition function is replaced by a collection of unitary matrices that map the Hilbert space to itself. that first described a quantum mechanical model of Turing machines. A 1985 article written by Oxford University physicist David Deutsch further developed the idea of quantum computers by suggesting quantum gates could function in a similar fashion to traditional digital computing binary logic gates.&lt;br /&gt;
&lt;br /&gt;
理解量子图灵机的一个方法是它推广了经典的图灵机，就像量子有限自动机推广了确定有限状态自动机机一样。实质上，经典 TM 的内部状态被希尔伯特空间中的纯态或混合态所取代，转移函数被映射 Hilbert 空间到自身的一组酉矩阵所取代。首次描述了图灵机的量子力学模型。牛津大学物理学家大卫 · 多伊奇在1985年的一篇文章中进一步发展了量子计算机的概念，他提出量子门可以以类似于传统数字计算二进制逻辑门的方式运行。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
That is, a classical Turing machine is described by  a 7-[[tuple]] &amp;lt;math&amp;gt;M = \langle Q, \Gamma, b, \Sigma, \delta, q_0, F \rangle&amp;lt;/math&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
Iriyama, Ohya, and Volovich have developed a model of a linear quantum Turing machine (LQTM).  This is a generalization of a classical QTM that has mixed states and that allows irreversible transition functions.  These allow the representation of quantum measurements without classical outcomes.&lt;br /&gt;
&lt;br /&gt;
Iriyama、 Ohya 和 Volovich 开发了一个线性量子图灵机模型(LQTM)。这是一个具有混合状态并允许不可逆转换函数的经典 QTM 的推广。这使得量子测量可以在没有经典结果的情况下进行表示。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
For a three-tape quantum Turing machine (one tape holding the input, a second tape holding intermediate calculation results, and a third tape holding output):&lt;br /&gt;
&lt;br /&gt;
A quantum Turing machine with postselection was defined by Scott Aaronson, who showed that the class of polynomial time on such a machine (PostBQP) is equal to the classical complexity class PP.&lt;br /&gt;
&lt;br /&gt;
一个具有后选择的量子图灵机由 Scott Aaronson 定义，他证明了这样一个机器上的多项式时间类(PostBQP)等于经典的复杂性类 PP。&lt;br /&gt;
&lt;br /&gt;
* The set of states &amp;lt;math&amp;gt;Q&amp;lt;/math&amp;gt; is replaced by a [[Hilbert space]].&lt;br /&gt;
&lt;br /&gt;
* The tape alphabet symbols &amp;lt;math&amp;gt;\Gamma&amp;lt;/math&amp;gt; are likewise replaced by a Hilbert space (usually a different Hilbert space than the set of states).&lt;br /&gt;
&lt;br /&gt;
* The blank symbol &amp;lt;math&amp;gt;b \in \Gamma&amp;lt;/math&amp;gt; corresponds to the zero-vector.&lt;br /&gt;
&lt;br /&gt;
* The input and output symbols &amp;lt;math&amp;gt;\Sigma&amp;lt;/math&amp;gt; are usually taken as a discrete set, as in the classical system; thus, neither the input nor output to a quantum machine need be a quantum system itself.&lt;br /&gt;
&lt;br /&gt;
* The [[State transition system|transition function]] &amp;lt;math&amp;gt;\delta : \Sigma \times Q  \otimes \Gamma \rightarrow \Sigma \times Q \otimes \Gamma \times \{L,R\}&amp;lt;/math&amp;gt; is a generalization of a [[transition monoid]], and is understood to be a collection of [[unitary matrix|unitary matrices]] that are [[automorphism]]s of the Hilbert space &amp;lt;math&amp;gt;Q&amp;lt;/math&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
* The initial state &amp;lt;math&amp;gt;q_0 \in Q&amp;lt;/math&amp;gt; may be either a [[mixed quantum state|mixed state]] or a [[pure state]].&lt;br /&gt;
&lt;br /&gt;
* The set &amp;lt;math&amp;gt;F&amp;lt;/math&amp;gt; of ''final'' or ''accepting states'' is a subspace of the Hilbert space &amp;lt;math&amp;gt;Q&amp;lt;/math&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The above is merely a sketch of a quantum Turing machine, rather than its formal definition, as it leaves vague several important details: for example, how often a [[quantum measurement|measurement]] is performed; see for example, the difference between a measure-once and a measure-many QFA.  This question of measurement affects the way in which writes to the output tape are defined.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==History==&lt;br /&gt;
&lt;br /&gt;
In 1980 and 1982, physicist [[Paul Benioff]] published papers&amp;lt;ref&amp;gt;{{cite journal |last1=Benioff | first1=Paul | title=The computer as a physical system: A microscopic quantum mechanical Hamiltonian model of computers as represented by Turing machines | journal=Journal of Statistical Physics |volume=22 | issue=5 | pages=563–591 | year=1980 | doi=10.1007/bf01011339|bibcode=1980JSP....22..563B }}&amp;lt;/ref&amp;gt;&amp;lt;ref&amp;gt;{{Cite journal | doi=10.1007/BF01342185 | last1=Benioff | first1=P. | title=Quantum mechanical hamiltonian models of turing machines | journal=Journal of Statistical Physics | volume=29 | issue=3 | pages=515–546 | year=1982|bibcode=1982JSP....29..515B }}&amp;lt;/ref&amp;gt; that first described a quantum mechanical model of [[Turing machines]]. A 1985 article written by Oxford University physicist [[David Deutsch]] further developed the idea of quantum computers by suggesting [[quantum gate]]s could function in a similar fashion to traditional digital computing [[Binary numeral system|binary]] [[logic gates]].&amp;lt;ref name=&amp;quot;Deutsch1985&amp;quot;&amp;gt;{{cite journal|last=Deutsch|first=David|author-link=David Deutsch|date=July 1985|title=Quantum theory, the Church-Turing principle and the universal quantum computer|url=http://www.ceid.upatras.gr/tech_news/papers/quantum_theory.pdf|url-status=dead|journal=[[Proceedings of the Royal Society A]]|volume=400|issue=1818|pages=97–117|bibcode=1985RSPSA.400...97D|doi=10.1098/rspa.1985.0070|archiveurl=https://web.archive.org/web/20081123183419/http://www.ceid.upatras.gr/tech_news/papers/quantum_theory.pdf|archivedate=2008-11-23|citeseerx=10.1.1.41.2382}}&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Iriyama, [[Masanori Ohya|Ohya]], and Volovich have developed a model of a ''linear quantum Turing machine'' (LQTM).  This is a generalization of a classical QTM that has mixed states and that allows irreversible transition functions.  These allow the representation of quantum measurements without classical outcomes.&amp;lt;ref&amp;gt;{{cite journal|title=Classically-Controlled Quantum Computation|date=2007-04-04|pages=601–620|author1=Simon Perdrix|author2=Philippe Jorrand|volume=16|journal=Math. Struct. In Comp. Science|arxiv=quant-ph/0407008|doi=10.1017/S096012950600538X|issue=4}} also {{cite journal|title=Classically-Controlled Quantum Computation|author=Simon Perdrix and Philippe Jorrand|url=http://dcm-workshop.org.uk./2005/dcm-draft-proceedings.pdf|year=2006|pages=601–620|journal=Math. Struct. In Comp. Science|volume=16|doi=10.1017/S096012950600538X|issue=4|citeseerx=10.1.1.252.1823}}&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
A ''quantum Turing machine with [[postselection]]'' was defined by [[Scott Aaronson]], who showed that the class of polynomial time on such a machine ([[PostBQP]]) is equal to the classical complexity class [[PP (complexity)|PP]].&amp;lt;ref&amp;gt;{{cite journal|last=Aaronson|first=Scott|year=2005|title=Quantum computing, postselection, and probabilistic polynomial-time|journal=[[Proceedings of the Royal Society A]]|volume=461|issue=2063|pages=3473–3482|doi=10.1098/rspa.2005.1546|bibcode = 2005RSPSA.461.3473A |arxiv=quant-ph/0412187}}  Preprint available at [https://arxiv.org/abs/quant-ph/0412187]&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
== See also ==&lt;br /&gt;
&lt;br /&gt;
Category:Turing machine&lt;br /&gt;
&lt;br /&gt;
类别: 图灵机&lt;br /&gt;
&lt;br /&gt;
*[[Quantum simulator#Solving physics problems|Quantum simulator § Solving physics problems]]&lt;br /&gt;
&lt;br /&gt;
Category:Quantum complexity theory&lt;br /&gt;
&lt;br /&gt;
范畴: 量子复杂性理论&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:Quantum Turing machine]]. Its edit history can be viewed at [[量子图灵机/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>Tueryeye</name></author>
	</entry>
	<entry>
		<id>https://wiki.swarma.org/index.php?title=%E9%87%8F%E5%AD%90%E5%9B%BE%E7%81%B5%E6%9C%BA&amp;diff=29739</id>
		<title>量子图灵机</title>
		<link rel="alternate" type="text/html" href="https://wiki.swarma.org/index.php?title=%E9%87%8F%E5%AD%90%E5%9B%BE%E7%81%B5%E6%9C%BA&amp;diff=29739"/>
		<updated>2022-03-27T16:41:35Z</updated>

		<summary type="html">&lt;p&gt;Tueryeye：&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;此词条暂由彩云小译翻译，翻译字数共319，未经人工整理和审校，带来阅读不便，请见谅。&lt;br /&gt;
&lt;br /&gt;
{{Short description|Model of quantum computation}}&lt;br /&gt;
&lt;br /&gt;
{{Turing}}&lt;br /&gt;
&lt;br /&gt;
&amp;lt;!-- Basic definition --&amp;gt;&lt;br /&gt;
=== 基础定义 ===&lt;br /&gt;
A '''quantum Turing machine''' ('''QTM''') or '''universal quantum computer''' is an [[abstract machine]] used to model the effects of a [[quantum computer]].  It provides a simple model that captures all of the power of quantum computation—that is, any [[quantum algorithm]] can be expressed formally as a particular quantum Turing machine. However, the computationally equivalent [[quantum circuit]] is a more common model.&amp;lt;ref name=&amp;quot;equivalence&amp;quot;&amp;gt;{{cite conference|author=[[Andrew Yao]]|title=Quantum circuit complexity|conference=34th Annual Symposium on Foundations of Computer Science|pages=352–361|year=1993}}&amp;lt;/ref&amp;gt;&amp;lt;ref name=&amp;quot;newequivalence&amp;quot;&amp;gt;{{cite arXiv|eprint=1808.01701|author1=Abel Molina|author2=John Watrous|author-link2=John Watrous (computer scientist)|title=Revisiting the simulation of quantum Turing machines by quantum circuits|date=2018|class=cs.CC}}&amp;lt;/ref&amp;gt;{{rp|2}}&lt;br /&gt;
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量子图灵机计算机(QTM)又称为通用量子计算机是一种用来模拟量子计算机效果的抽象机器。它提供了一个简单的模型，但又能展现出量子计算的所有威力。也就是说，任何量子算法都可以被形式化地表示为一个特定的量子图灵机。提供等效计算能力的量子电路是一种比较常用的模型。&amp;lt;ref name=&amp;quot;equivalence&amp;quot; /&amp;gt;&amp;lt;ref name=&amp;quot;newequivalence&amp;quot; /&amp;gt;&lt;br /&gt;
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&amp;lt;!-- Relation to classical computation --&amp;gt;&lt;br /&gt;
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=== 与经典计算的关系 ===&lt;br /&gt;
Quantum Turing machines can be related to classical and probabilistic Turing machines in a framework based on [[Stochastic matrix|transition matrices]]. That is, a matrix can be specified whose product with the matrix representing a classical or probabilistic machine provides the quantum probability matrix representing the quantum machine. This was shown by [[Lance Fortnow]].&amp;lt;ref name=&amp;quot;transition&amp;quot;&amp;gt;{{cite journal|author=Fortnow|first=Lance|author-link=Lance Fortnow|year=2003|title=One Complexity Theorist's View of Quantum Computing|url=|journal=Theoretical Computer Science|volume=292|issue=3|pages=597–610|doi=10.1016/S0304-3975(01)00377-2|via=|arxiv=quant-ph/0003035}}&amp;lt;/ref&amp;gt;&lt;br /&gt;
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Quantum Turing machines can be related to classical and probabilistic Turing machines in a framework based on transition matrices. That is, a matrix can be specified whose product with the matrix representing a classical or probabilistic machine provides the quantum probability matrix representing the quantum machine. This was shown by Lance Fortnow.&lt;br /&gt;
&lt;br /&gt;
在基于转移矩阵的框架下，量子图灵机可以与经典图灵机和概率图灵机相关联。也就是说，可以指定一个矩阵，该矩阵与表示经典或概率机器的矩阵的乘积提供了表示量子机器的量子概率矩阵。这是由兰斯 · 福特诺展示的。&amp;lt;ref name=&amp;quot;transition&amp;quot; /&amp;gt;&lt;br /&gt;
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== Informal sketch ==&lt;br /&gt;
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{{Unsolved|physics|Is a [[universal quantum computer]] sufficient to [[Algorithmic efficiency|efficiently]] [[Dynamical simulation|simulate]] an arbitrary physical system?}}&lt;br /&gt;
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A way of understanding the quantum Turing machine (QTM) is that it generalizes the classical [[Turing machine]] (TM) in the same way that the [[quantum finite automaton]] (QFA) generalizes the [[deterministic finite automaton]] (DFA).  In essence, the internal states of a classical TM are replaced by [[pure state|pure]] or [[mixed quantum state|mixed states]] in a Hilbert space; the transition function is replaced by a collection of [[unitary matrix|unitary matrices]] that map the Hilbert space to itself.&amp;lt;ref name=&amp;quot;Deutsch1985&amp;quot; /&amp;gt;&lt;br /&gt;
&lt;br /&gt;
A way of understanding the quantum Turing machine (QTM) is that it generalizes the classical Turing machine (TM) in the same way that the quantum finite automaton (QFA) generalizes the deterministic finite automaton (DFA).  In essence, the internal states of a classical TM are replaced by pure or mixed states in a Hilbert space; the transition function is replaced by a collection of unitary matrices that map the Hilbert space to itself. that first described a quantum mechanical model of Turing machines. A 1985 article written by Oxford University physicist David Deutsch further developed the idea of quantum computers by suggesting quantum gates could function in a similar fashion to traditional digital computing binary logic gates.&lt;br /&gt;
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理解量子图灵机的一个方法是它推广了经典的图灵机，就像量子有限自动机推广了确定有限状态自动机机一样。实质上，经典 TM 的内部状态被希尔伯特空间中的纯态或混合态所取代，转移函数被映射 Hilbert 空间到自身的一组酉矩阵所取代。首次描述了图灵机的量子力学模型。牛津大学物理学家大卫 · 多伊奇在1985年的一篇文章中进一步发展了量子计算机的概念，他提出量子门可以以类似于传统数字计算二进制逻辑门的方式运行。&lt;br /&gt;
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That is, a classical Turing machine is described by  a 7-[[tuple]] &amp;lt;math&amp;gt;M = \langle Q, \Gamma, b, \Sigma, \delta, q_0, F \rangle&amp;lt;/math&amp;gt;.&lt;br /&gt;
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Iriyama, Ohya, and Volovich have developed a model of a linear quantum Turing machine (LQTM).  This is a generalization of a classical QTM that has mixed states and that allows irreversible transition functions.  These allow the representation of quantum measurements without classical outcomes.&lt;br /&gt;
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Iriyama、 Ohya 和 Volovich 开发了一个线性量子图灵机模型(LQTM)。这是一个具有混合状态并允许不可逆转换函数的经典 QTM 的推广。这使得量子测量可以在没有经典结果的情况下进行表示。&lt;br /&gt;
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For a three-tape quantum Turing machine (one tape holding the input, a second tape holding intermediate calculation results, and a third tape holding output):&lt;br /&gt;
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A quantum Turing machine with postselection was defined by Scott Aaronson, who showed that the class of polynomial time on such a machine (PostBQP) is equal to the classical complexity class PP.&lt;br /&gt;
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一个具有后选择的量子图灵机由 Scott Aaronson 定义，他证明了这样一个机器上的多项式时间类(PostBQP)等于经典的复杂性类 PP。&lt;br /&gt;
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* The set of states &amp;lt;math&amp;gt;Q&amp;lt;/math&amp;gt; is replaced by a [[Hilbert space]].&lt;br /&gt;
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* The tape alphabet symbols &amp;lt;math&amp;gt;\Gamma&amp;lt;/math&amp;gt; are likewise replaced by a Hilbert space (usually a different Hilbert space than the set of states).&lt;br /&gt;
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* The blank symbol &amp;lt;math&amp;gt;b \in \Gamma&amp;lt;/math&amp;gt; corresponds to the zero-vector.&lt;br /&gt;
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* The input and output symbols &amp;lt;math&amp;gt;\Sigma&amp;lt;/math&amp;gt; are usually taken as a discrete set, as in the classical system; thus, neither the input nor output to a quantum machine need be a quantum system itself.&lt;br /&gt;
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* The [[State transition system|transition function]] &amp;lt;math&amp;gt;\delta : \Sigma \times Q  \otimes \Gamma \rightarrow \Sigma \times Q \otimes \Gamma \times \{L,R\}&amp;lt;/math&amp;gt; is a generalization of a [[transition monoid]], and is understood to be a collection of [[unitary matrix|unitary matrices]] that are [[automorphism]]s of the Hilbert space &amp;lt;math&amp;gt;Q&amp;lt;/math&amp;gt;.&lt;br /&gt;
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* The initial state &amp;lt;math&amp;gt;q_0 \in Q&amp;lt;/math&amp;gt; may be either a [[mixed quantum state|mixed state]] or a [[pure state]].&lt;br /&gt;
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* The set &amp;lt;math&amp;gt;F&amp;lt;/math&amp;gt; of ''final'' or ''accepting states'' is a subspace of the Hilbert space &amp;lt;math&amp;gt;Q&amp;lt;/math&amp;gt;.&lt;br /&gt;
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The above is merely a sketch of a quantum Turing machine, rather than its formal definition, as it leaves vague several important details: for example, how often a [[quantum measurement|measurement]] is performed; see for example, the difference between a measure-once and a measure-many QFA.  This question of measurement affects the way in which writes to the output tape are defined.&lt;br /&gt;
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==History==&lt;br /&gt;
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In 1980 and 1982, physicist [[Paul Benioff]] published papers&amp;lt;ref&amp;gt;{{cite journal |last1=Benioff | first1=Paul | title=The computer as a physical system: A microscopic quantum mechanical Hamiltonian model of computers as represented by Turing machines | journal=Journal of Statistical Physics |volume=22 | issue=5 | pages=563–591 | year=1980 | doi=10.1007/bf01011339|bibcode=1980JSP....22..563B }}&amp;lt;/ref&amp;gt;&amp;lt;ref&amp;gt;{{Cite journal | doi=10.1007/BF01342185 | last1=Benioff | first1=P. | title=Quantum mechanical hamiltonian models of turing machines | journal=Journal of Statistical Physics | volume=29 | issue=3 | pages=515–546 | year=1982|bibcode=1982JSP....29..515B }}&amp;lt;/ref&amp;gt; that first described a quantum mechanical model of [[Turing machines]]. A 1985 article written by Oxford University physicist [[David Deutsch]] further developed the idea of quantum computers by suggesting [[quantum gate]]s could function in a similar fashion to traditional digital computing [[Binary numeral system|binary]] [[logic gates]].&amp;lt;ref name=&amp;quot;Deutsch1985&amp;quot;&amp;gt;{{cite journal|last=Deutsch|first=David|author-link=David Deutsch|date=July 1985|title=Quantum theory, the Church-Turing principle and the universal quantum computer|url=http://www.ceid.upatras.gr/tech_news/papers/quantum_theory.pdf|url-status=dead|journal=[[Proceedings of the Royal Society A]]|volume=400|issue=1818|pages=97–117|bibcode=1985RSPSA.400...97D|doi=10.1098/rspa.1985.0070|archiveurl=https://web.archive.org/web/20081123183419/http://www.ceid.upatras.gr/tech_news/papers/quantum_theory.pdf|archivedate=2008-11-23|citeseerx=10.1.1.41.2382}}&amp;lt;/ref&amp;gt;&lt;br /&gt;
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Iriyama, [[Masanori Ohya|Ohya]], and Volovich have developed a model of a ''linear quantum Turing machine'' (LQTM).  This is a generalization of a classical QTM that has mixed states and that allows irreversible transition functions.  These allow the representation of quantum measurements without classical outcomes.&amp;lt;ref&amp;gt;{{cite journal|title=Classically-Controlled Quantum Computation|date=2007-04-04|pages=601–620|author1=Simon Perdrix|author2=Philippe Jorrand|volume=16|journal=Math. Struct. In Comp. Science|arxiv=quant-ph/0407008|doi=10.1017/S096012950600538X|issue=4}} also {{cite journal|title=Classically-Controlled Quantum Computation|author=Simon Perdrix and Philippe Jorrand|url=http://dcm-workshop.org.uk./2005/dcm-draft-proceedings.pdf|year=2006|pages=601–620|journal=Math. Struct. In Comp. Science|volume=16|doi=10.1017/S096012950600538X|issue=4|citeseerx=10.1.1.252.1823}}&amp;lt;/ref&amp;gt;&lt;br /&gt;
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A ''quantum Turing machine with [[postselection]]'' was defined by [[Scott Aaronson]], who showed that the class of polynomial time on such a machine ([[PostBQP]]) is equal to the classical complexity class [[PP (complexity)|PP]].&amp;lt;ref&amp;gt;{{cite journal|last=Aaronson|first=Scott|year=2005|title=Quantum computing, postselection, and probabilistic polynomial-time|journal=[[Proceedings of the Royal Society A]]|volume=461|issue=2063|pages=3473–3482|doi=10.1098/rspa.2005.1546|bibcode = 2005RSPSA.461.3473A |arxiv=quant-ph/0412187}}  Preprint available at [https://arxiv.org/abs/quant-ph/0412187]&amp;lt;/ref&amp;gt;&lt;br /&gt;
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== See also ==&lt;br /&gt;
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Category:Turing machine&lt;br /&gt;
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类别: 图灵机&lt;br /&gt;
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*[[Quantum simulator#Solving physics problems|Quantum simulator § Solving physics problems]]&lt;br /&gt;
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Category:Quantum complexity theory&lt;br /&gt;
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范畴: 量子复杂性理论&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:Quantum Turing machine]]. Its edit history can be viewed at [[量子图灵机/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>Tueryeye</name></author>
	</entry>
	<entry>
		<id>https://wiki.swarma.org/index.php?title=%E9%87%8F%E5%AD%90%E5%9B%BE%E7%81%B5%E6%9C%BA&amp;diff=29738</id>
		<title>量子图灵机</title>
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		<updated>2022-03-27T16:32:14Z</updated>

		<summary type="html">&lt;p&gt;Tueryeye：&lt;/p&gt;
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&lt;div&gt;此词条暂由彩云小译翻译，翻译字数共319，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|Model of quantum computation}}&lt;br /&gt;
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{{Turing}}&lt;br /&gt;
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&amp;lt;!-- Basic definition --&amp;gt;&lt;br /&gt;
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A '''quantum Turing machine''' ('''QTM''') or '''universal quantum computer''' is an [[abstract machine]] used to model the effects of a [[quantum computer]].  It provides a simple model that captures all of the power of quantum computation—that is, any [[quantum algorithm]] can be expressed formally as a particular quantum Turing machine. However, the computationally equivalent [[quantum circuit]] is a more common model.&amp;lt;ref name=&amp;quot;equivalence&amp;quot;&amp;gt;{{cite conference|author=[[Andrew Yao]]|title=Quantum circuit complexity|conference=34th Annual Symposium on Foundations of Computer Science|pages=352–361|year=1993}}&amp;lt;/ref&amp;gt;&amp;lt;ref name=&amp;quot;newequivalence&amp;quot;&amp;gt;{{cite arXiv|eprint=1808.01701|author1=Abel Molina|author2=John Watrous|author-link2=John Watrous (computer scientist)|title=Revisiting the simulation of quantum Turing machines by quantum circuits|date=2018|class=cs.CC}}&amp;lt;/ref&amp;gt;{{rp|2}}&lt;br /&gt;
&lt;br /&gt;
A quantum Turing machine (QTM) or universal quantum computer is an abstract machine used to model the effects of a quantum computer.  It provides a simple model that captures all of the power of quantum computation—that is, any quantum algorithm can be expressed formally as a particular quantum Turing machine. However, the computationally equivalent quantum circuit is a more common model.&lt;br /&gt;
&lt;br /&gt;
量子图灵机计算机(QTM)又称为通用量子计算机是一种用来模拟量子计算机效果的抽象机器。它提供了一个简单的模型，可以捕捉到量子计算的所有威力---- 也就是说，任何量子算法都可以形式化地表示为一个特定的量子图灵机。然而，计算等效量子电路是一种比较常用的模型。&lt;br /&gt;
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&amp;lt;!-- Relation to classical computation --&amp;gt;&lt;br /&gt;
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&amp;lt;!-- Relation to classical computation --&amp;gt;&lt;br /&gt;
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&amp;lt; ! ! -- 与经典计算的关系 -- &amp;gt; &lt;br /&gt;
&lt;br /&gt;
Quantum Turing machines can be related to classical and probabilistic Turing machines in a framework based on [[Stochastic matrix|transition matrices]]. That is, a matrix can be specified whose product with the matrix representing a classical or probabilistic machine provides the quantum probability matrix representing the quantum machine. This was shown by [[Lance Fortnow]].&amp;lt;ref name=&amp;quot;transition&amp;quot;&amp;gt;{{cite journal|author=Fortnow|first=Lance|author-link=Lance Fortnow|year=2003|title=One Complexity Theorist's View of Quantum Computing|url=|journal=Theoretical Computer Science|volume=292|issue=3|pages=597–610|doi=10.1016/S0304-3975(01)00377-2|via=|arxiv=quant-ph/0003035}}&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
Quantum Turing machines can be related to classical and probabilistic Turing machines in a framework based on transition matrices. That is, a matrix can be specified whose product with the matrix representing a classical or probabilistic machine provides the quantum probability matrix representing the quantum machine. This was shown by Lance Fortnow.&lt;br /&gt;
&lt;br /&gt;
在基于转移矩阵的框架下，量子图灵机可以与经典图灵机和概率图灵机相关联。也就是说，可以指定一个矩阵，该矩阵与表示经典或概率机器的矩阵的乘积提供了表示量子机器的量子概率矩阵。这是由兰斯 · 福特诺展示的。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
== Informal sketch ==&lt;br /&gt;
&lt;br /&gt;
{{Unsolved|physics|Is a [[universal quantum computer]] sufficient to [[Algorithmic efficiency|efficiently]] [[Dynamical simulation|simulate]] an arbitrary physical system?}}&lt;br /&gt;
&lt;br /&gt;
A way of understanding the quantum Turing machine (QTM) is that it generalizes the classical [[Turing machine]] (TM) in the same way that the [[quantum finite automaton]] (QFA) generalizes the [[deterministic finite automaton]] (DFA).  In essence, the internal states of a classical TM are replaced by [[pure state|pure]] or [[mixed quantum state|mixed states]] in a Hilbert space; the transition function is replaced by a collection of [[unitary matrix|unitary matrices]] that map the Hilbert space to itself.&amp;lt;ref name=&amp;quot;Deutsch1985&amp;quot; /&amp;gt;&lt;br /&gt;
&lt;br /&gt;
A way of understanding the quantum Turing machine (QTM) is that it generalizes the classical Turing machine (TM) in the same way that the quantum finite automaton (QFA) generalizes the deterministic finite automaton (DFA).  In essence, the internal states of a classical TM are replaced by pure or mixed states in a Hilbert space; the transition function is replaced by a collection of unitary matrices that map the Hilbert space to itself. that first described a quantum mechanical model of Turing machines. A 1985 article written by Oxford University physicist David Deutsch further developed the idea of quantum computers by suggesting quantum gates could function in a similar fashion to traditional digital computing binary logic gates.&lt;br /&gt;
&lt;br /&gt;
理解量子图灵机的一个方法是它推广了经典的图灵机，就像量子有限自动机推广了确定有限状态自动机机一样。实质上，经典 TM 的内部状态被希尔伯特空间中的纯态或混合态所取代，转移函数被映射 Hilbert 空间到自身的一组酉矩阵所取代。首次描述了图灵机的量子力学模型。牛津大学物理学家大卫 · 多伊奇在1985年的一篇文章中进一步发展了量子计算机的概念，他提出量子门可以以类似于传统数字计算二进制逻辑门的方式运行。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
That is, a classical Turing machine is described by  a 7-[[tuple]] &amp;lt;math&amp;gt;M = \langle Q, \Gamma, b, \Sigma, \delta, q_0, F \rangle&amp;lt;/math&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
Iriyama, Ohya, and Volovich have developed a model of a linear quantum Turing machine (LQTM).  This is a generalization of a classical QTM that has mixed states and that allows irreversible transition functions.  These allow the representation of quantum measurements without classical outcomes.&lt;br /&gt;
&lt;br /&gt;
Iriyama、 Ohya 和 Volovich 开发了一个线性量子图灵机模型(LQTM)。这是一个具有混合状态并允许不可逆转换函数的经典 QTM 的推广。这使得量子测量可以在没有经典结果的情况下进行表示。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
For a three-tape quantum Turing machine (one tape holding the input, a second tape holding intermediate calculation results, and a third tape holding output):&lt;br /&gt;
&lt;br /&gt;
A quantum Turing machine with postselection was defined by Scott Aaronson, who showed that the class of polynomial time on such a machine (PostBQP) is equal to the classical complexity class PP.&lt;br /&gt;
&lt;br /&gt;
一个具有后选择的量子图灵机由 Scott Aaronson 定义，他证明了这样一个机器上的多项式时间类(PostBQP)等于经典的复杂性类 PP。&lt;br /&gt;
&lt;br /&gt;
* The set of states &amp;lt;math&amp;gt;Q&amp;lt;/math&amp;gt; is replaced by a [[Hilbert space]].&lt;br /&gt;
&lt;br /&gt;
* The tape alphabet symbols &amp;lt;math&amp;gt;\Gamma&amp;lt;/math&amp;gt; are likewise replaced by a Hilbert space (usually a different Hilbert space than the set of states).&lt;br /&gt;
&lt;br /&gt;
* The blank symbol &amp;lt;math&amp;gt;b \in \Gamma&amp;lt;/math&amp;gt; corresponds to the zero-vector.&lt;br /&gt;
&lt;br /&gt;
* The input and output symbols &amp;lt;math&amp;gt;\Sigma&amp;lt;/math&amp;gt; are usually taken as a discrete set, as in the classical system; thus, neither the input nor output to a quantum machine need be a quantum system itself.&lt;br /&gt;
&lt;br /&gt;
* The [[State transition system|transition function]] &amp;lt;math&amp;gt;\delta : \Sigma \times Q  \otimes \Gamma \rightarrow \Sigma \times Q \otimes \Gamma \times \{L,R\}&amp;lt;/math&amp;gt; is a generalization of a [[transition monoid]], and is understood to be a collection of [[unitary matrix|unitary matrices]] that are [[automorphism]]s of the Hilbert space &amp;lt;math&amp;gt;Q&amp;lt;/math&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
* The initial state &amp;lt;math&amp;gt;q_0 \in Q&amp;lt;/math&amp;gt; may be either a [[mixed quantum state|mixed state]] or a [[pure state]].&lt;br /&gt;
&lt;br /&gt;
* The set &amp;lt;math&amp;gt;F&amp;lt;/math&amp;gt; of ''final'' or ''accepting states'' is a subspace of the Hilbert space &amp;lt;math&amp;gt;Q&amp;lt;/math&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The above is merely a sketch of a quantum Turing machine, rather than its formal definition, as it leaves vague several important details: for example, how often a [[quantum measurement|measurement]] is performed; see for example, the difference between a measure-once and a measure-many QFA.  This question of measurement affects the way in which writes to the output tape are defined.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==History==&lt;br /&gt;
&lt;br /&gt;
In 1980 and 1982, physicist [[Paul Benioff]] published papers&amp;lt;ref&amp;gt;{{cite journal |last1=Benioff | first1=Paul | title=The computer as a physical system: A microscopic quantum mechanical Hamiltonian model of computers as represented by Turing machines | journal=Journal of Statistical Physics |volume=22 | issue=5 | pages=563–591 | year=1980 | doi=10.1007/bf01011339|bibcode=1980JSP....22..563B }}&amp;lt;/ref&amp;gt;&amp;lt;ref&amp;gt;{{Cite journal | doi=10.1007/BF01342185 | last1=Benioff | first1=P. | title=Quantum mechanical hamiltonian models of turing machines | journal=Journal of Statistical Physics | volume=29 | issue=3 | pages=515–546 | year=1982|bibcode=1982JSP....29..515B }}&amp;lt;/ref&amp;gt; that first described a quantum mechanical model of [[Turing machines]]. A 1985 article written by Oxford University physicist [[David Deutsch]] further developed the idea of quantum computers by suggesting [[quantum gate]]s could function in a similar fashion to traditional digital computing [[Binary numeral system|binary]] [[logic gates]].&amp;lt;ref name=&amp;quot;Deutsch1985&amp;quot;&amp;gt;{{cite journal|last=Deutsch|first=David|author-link=David Deutsch|date=July 1985|title=Quantum theory, the Church-Turing principle and the universal quantum computer|url=http://www.ceid.upatras.gr/tech_news/papers/quantum_theory.pdf|url-status=dead|journal=[[Proceedings of the Royal Society A]]|volume=400|issue=1818|pages=97–117|bibcode=1985RSPSA.400...97D|doi=10.1098/rspa.1985.0070|archiveurl=https://web.archive.org/web/20081123183419/http://www.ceid.upatras.gr/tech_news/papers/quantum_theory.pdf|archivedate=2008-11-23|citeseerx=10.1.1.41.2382}}&amp;lt;/ref&amp;gt;&lt;br /&gt;
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Iriyama, [[Masanori Ohya|Ohya]], and Volovich have developed a model of a ''linear quantum Turing machine'' (LQTM).  This is a generalization of a classical QTM that has mixed states and that allows irreversible transition functions.  These allow the representation of quantum measurements without classical outcomes.&amp;lt;ref&amp;gt;{{cite journal|title=Classically-Controlled Quantum Computation|date=2007-04-04|pages=601–620|author1=Simon Perdrix|author2=Philippe Jorrand|volume=16|journal=Math. Struct. In Comp. Science|arxiv=quant-ph/0407008|doi=10.1017/S096012950600538X|issue=4}} also {{cite journal|title=Classically-Controlled Quantum Computation|author=Simon Perdrix and Philippe Jorrand|url=http://dcm-workshop.org.uk./2005/dcm-draft-proceedings.pdf|year=2006|pages=601–620|journal=Math. Struct. In Comp. Science|volume=16|doi=10.1017/S096012950600538X|issue=4|citeseerx=10.1.1.252.1823}}&amp;lt;/ref&amp;gt;&lt;br /&gt;
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A ''quantum Turing machine with [[postselection]]'' was defined by [[Scott Aaronson]], who showed that the class of polynomial time on such a machine ([[PostBQP]]) is equal to the classical complexity class [[PP (complexity)|PP]].&amp;lt;ref&amp;gt;{{cite journal|last=Aaronson|first=Scott|year=2005|title=Quantum computing, postselection, and probabilistic polynomial-time|journal=[[Proceedings of the Royal Society A]]|volume=461|issue=2063|pages=3473–3482|doi=10.1098/rspa.2005.1546|bibcode = 2005RSPSA.461.3473A |arxiv=quant-ph/0412187}}  Preprint available at [https://arxiv.org/abs/quant-ph/0412187]&amp;lt;/ref&amp;gt;&lt;br /&gt;
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== See also ==&lt;br /&gt;
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Category:Turing machine&lt;br /&gt;
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类别: 图灵机&lt;br /&gt;
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*[[Quantum simulator#Solving physics problems|Quantum simulator § Solving physics problems]]&lt;br /&gt;
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Category:Quantum complexity theory&lt;br /&gt;
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范畴: 量子复杂性理论&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:Quantum Turing machine]]. Its edit history can be viewed at [[量子图灵机/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>Tueryeye</name></author>
	</entry>
	<entry>
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		<title>玻尔兹曼分布</title>
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		<updated>2021-10-21T02:02:50Z</updated>

		<summary type="html">&lt;p&gt;Tueryeye：修改段落空格&lt;/p&gt;
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&lt;div&gt;此词条暂由tueryeye翻译和审校，翻译字数共1452，带来阅读不便，请见谅。&lt;br /&gt;
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{{Use American English|date = March 2019}}&lt;br /&gt;
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{{Short description|Probability distribution of energy states of a system}}&lt;br /&gt;
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{{about|system energy states|particle energy levels and velocities|Maxwell–Boltzmann distribution}}&lt;br /&gt;
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[[File:Boltzmann distribution graph.svg|upright=1.75|right|thumb|Boltzmann factor ''p&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;''&amp;amp;nbsp;/&amp;amp;nbsp;''p&amp;lt;sub&amp;gt;j&amp;lt;/sub&amp;gt;'' (vertical axis) as a function of temperature ''T'' for several energy differences ''ε&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;''&amp;amp;nbsp;−&amp;amp;nbsp;''ε&amp;lt;sub&amp;gt;j&amp;lt;/sub&amp;gt;''.|链接=Special:FilePath/Boltzmann_distribution_graph.svg]]&lt;br /&gt;
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In [[statistical mechanics]] and [[mathematics]], a '''Boltzmann distribution''' (also called '''Gibbs distribution'''&amp;lt;ref name=&amp;quot;landau&amp;quot;&amp;gt;{{cite book | author=Landau, Lev Davidovich |author2=Lifshitz, Evgeny Mikhailovich |name-list-style=amp | title=Statistical Physics |volume=5 |series=Course of Theoretical Physics |edition=3 |origyear=1976 |year=1980 |place=Oxford |publisher=Pergamon Press|isbn=0-7506-3372-7|author-link=Lev Landau |author2-link=Evgeny Lifshitz }} Translated by J.B. Sykes and M.J. Kearsley. See section 28&amp;lt;/ref&amp;gt;) is a [[probability distribution]] or [[probability measure]] that gives the probability that a system will be in a certain [[microstate (statistical mechanics)|state]] as a function of that state's energy and the temperature of the system. The distribution is expressed in the form:&lt;br /&gt;
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在统计力学和数学中，波兹曼分布分布(也称为吉布斯分布&amp;lt;ref name=&amp;quot;landau&amp;quot; /&amp;gt;)是一个概率分布或机率量测，它给出了一个系统处于某种量子态的概率，这个概率是该状态的能量和系统温度的函数。分布情况以下列形式表示:&lt;br /&gt;
:&amp;lt;math&amp;gt;p_i \propto e^{-\frac{\varepsilon_i}{kT}}&amp;lt;/math&amp;gt; &lt;br /&gt;
&lt;br /&gt;
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where {{mvar|p&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;}} is the probability of the system being in state {{mvar|i}}, {{mvar|ε&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;}} is the energy of that state, and a constant {{mvar|kT}} of the distribution is the product of [[Boltzmann's constant]] {{mvar|k}} and [[thermodynamic temperature]] {{mvar|T}}. The symbol &amp;lt;math display=&amp;quot;inline&amp;quot;&amp;gt;\propto&amp;lt;/math&amp;gt; denotes [[proportionality (mathematics)|proportionality]] (see {{section link||The distribution}} for the proportionality constant).&lt;br /&gt;
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{{mvar|p&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;}} 是其中系统处于状态{{mvar|i}}的概率, {{mvar|ε&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;}} 是该状态的能量，还有关于这个分布的一个常数 {{mvar|kT}} ，它是玻尔兹曼常数{{mvar|k}}和热力学温度 {{mvar|T}} 的乘积。符号 &amp;lt;math display=&amp;quot;inline&amp;quot;&amp;gt;\propto&amp;lt;/math&amp;gt;表示正比例(见附录中的比例常数)。&lt;br /&gt;
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The term system here has a very wide meaning; it can range from a single atom to a macroscopic system such as a [[Natural gas storage|natural gas storage tank]]. Because of this the Boltzmann distribution can be used to solve a very wide variety of problems. The distribution shows that states with lower energy will always have a higher probability of being occupied .&lt;br /&gt;
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这里的术语系统含义广泛，它可以从单个原子到宏观系统，如天然气储罐。正因为如此，波兹曼分布可以用来解决各种各样的问题。玻尔兹曼分布表明，能量较低的状态被占据的概率总是较高的。&lt;br /&gt;
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The ''ratio'' of probabilities of two states is known as the '''Boltzmann factor''' and characteristically only depends on the states' energy difference:&lt;br /&gt;
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两种状态的概率之比被称为玻尔兹曼因子，取决于两种状态的能量差:&lt;br /&gt;
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&amp;lt;math&amp;gt;\frac{p_i}{p_j} = e^{\frac{\varepsilon_j - \varepsilon_i}{kT}}&amp;lt;/math&amp;gt;&lt;br /&gt;
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The Boltzmann distribution is named after [[Ludwig Boltzmann]] who first formulated it in 1868 during his studies of the [[statistical mechanics]] of gases in thermal equilibrium. Boltzmann's statistical work is borne out in his paper “On the Relationship between the Second Fundamental Theorem of the Mechanical Theory of Heat and Probability Calculations Regarding the Conditions for Thermal Equilibrium&amp;quot;&amp;lt;ref&amp;gt;http://crystal.med.upenn.edu/sharp-lab-pdfs/2015SharpMatschinsky_Boltz1877_Entropy17.pdf&amp;lt;/ref&amp;gt;. The distribution was later investigated extensively, in its modern generic form, by [[Josiah Willard Gibbs]] in 1902.&amp;lt;ref name=&amp;quot;gibbs&amp;quot;&amp;gt;{{cite book |last=Gibbs |first=Josiah Willard |authorlink=Josiah Willard Gibbs |title=Elementary Principles in Statistical Mechanics |year=1902 |publisher=[[Charles Scribner's Sons]] &lt;br /&gt;
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The distribution was later investigated extensively, in its modern generic form, by Josiah Willard Gibbs in 1902.&lt;br /&gt;
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这种分布后来在1902年由约西亚·威拉德·吉布斯进行了广泛的调查，以其现代通用形式。&lt;br /&gt;
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|location=New York|title-link=Elementary Principles in Statistical Mechanics }}&amp;lt;/ref&amp;gt;&lt;br /&gt;
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波兹曼分布是根据路德维希·玻尔兹曼1868年在研究统计力学中气体热平衡的时候首次提出的一个公式命名的。波尔兹曼的统计工作在他1877年的论文《论热力学第二基本定理与热平衡条件的概率计算之间的关系》中得到了体现。&amp;lt;ref&amp;gt;“On the Relationship between the Second Fundamental Theorem of the Mechanical Theory of Heat and Probability Calculations Regarding the Conditions for Thermal Equilibrium” Sitzungberichte der Kaiserlichen Akademie der Wissenschaften. Mathematisch-Naturwissen Classe. Abt. II, LXXVI 1877, pp 373-435 (Wien. Ber. 1877, 76:373-435). &amp;lt;/ref&amp;gt; 在玻尔兹曼分布被发明之后，约西亚·华纳德·吉布森充分地研究了它并在1902年提出了它的一般形式。&amp;lt;ref name=&amp;quot;gibbs&amp;quot; /&amp;gt;&lt;br /&gt;
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The generalized Boltzmann distribution is a sufficient and necessary condition for the equivalence between the statistical mechanics definition of [[entropy]] (The [[Entropy_(statistical_thermodynamics)#Gibbs_entropy_formula | Gibbs entropy formula]] &amp;lt;math&amp;gt;S = -k_{\mathrm{B}}\sum_i p_i \log p_i&amp;lt;/math&amp;gt;) and the thermodynamic definition of entropy (&amp;lt;math&amp;gt;d S = \frac{\delta Q_\text{rev}}{T}&amp;lt;/math&amp;gt;), and the [[fundamental thermodynamic relation]]).&amp;lt;ref name=&amp;quot;:0&amp;quot;&amp;gt;{{cite journal |last1= Gao |first1= Xiang |last2= Gallicchio |first2= Emilio |first3= Adrian |last3= Roitberg  |date= 2019 |title= The generalized Boltzmann distribution is the only distribution in which the Gibbs-Shannon entropy equals the thermodynamic entropy |journal= The Journal of Chemical Physics|volume= 151|issue= 3|pages= 034113|doi= 10.1063/1.5111333|pmid= 31325924 |arxiv= 1903.02121 |s2cid= 118981017 }}&amp;lt;/ref&amp;gt;&lt;br /&gt;
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广义波兹曼分布是熵的统计力学定义(吉布斯熵公式  &amp;lt;math&amp;gt;S = -k_{\mathrm{B}}\sum_i p_i \log p_i&amp;lt;/math&amp;gt;)与熵的热力学定义(&amp;lt;math&amp;gt;d S = \frac{\delta Q_\text{rev}}{T}&amp;lt;/math&amp;gt;)等价的充要条件。&amp;lt;ref name=&amp;quot;:0&amp;quot; /&amp;gt;&lt;br /&gt;
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The Boltzmann distribution should not be confused with the [[Maxwell–Boltzmann distribution]]. The former gives the probability that a system will be in a certain state as a function of that state's energy;&amp;lt;ref name=&amp;quot;Atkins, P. W. 2010&amp;quot;&amp;gt;Atkins, P. W. (2010) Quanta, W. H. Freeman and Company, New York&amp;lt;/ref&amp;gt; in contrast, the latter is used to describe particle speeds in idealized gases.&lt;br /&gt;
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值得一提的是，玻尔兹曼分布不应与麦克斯韦-玻尔兹曼分布混淆。前者给出了系统处于某种状态的概率，作为该状态能量的函数; 后者则是用于描述理想气体中的粒子速度。&lt;br /&gt;
==分布==&lt;br /&gt;
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The Boltzmann distribution is a [[probability distribution]] that gives the probability of a certain state as a function of that state's energy and  temperature of the [[system]] to which the distribution is applied.&amp;lt;ref name=&amp;quot;McQuarrie, A. 2000&amp;quot;&amp;gt;McQuarrie, A. (2000) Statistical Mechanics, University Science Books, California&amp;lt;/ref&amp;gt; It is given as&lt;br /&gt;
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波兹曼分布是一个概率分布，它给出了出于某种量子态处于某种能量和温度的时候的概率。它被这样定义：&lt;br /&gt;
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&amp;lt;math&amp;gt;&lt;br /&gt;
p_i=\frac{1}{Q}} {e^{- {\varepsilon}_i / k T}=\frac{e^{- {\varepsilon}_i / k T}}{\sum_{j=1}^{M}{e^{- {\varepsilon}_j / k T}}}&lt;br /&gt;
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&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
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where ''p&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;'' is the probability of state ''i'', ''ε&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;'' the energy of state ''i'', ''k'' the Boltzmann constant, ''T'' the temperature of the system and ''M'' is the number of all states accessible to the system of interest.&amp;lt;ref name=&amp;quot;McQuarrie, A. 2000&amp;quot; /&amp;gt;&amp;lt;ref name=&amp;quot;Atkins, P. W. 2010&amp;quot; /&amp;gt; Implied parentheses around the denominator ''kT'' are omitted for brevity. The normalization denominator ''Q'' (denoted by some authors by ''Z'') is the [[canonical partition function]]&lt;br /&gt;
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其中 ''p&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;'' 是状态 i 的概率，''ε&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;'' 是状态 i 的能量，''k'' 是波兹曼常数，''T'' 是系统的温度，''M'' 是系统所能到达的所有量子态的数目。&amp;lt;ref name=&amp;quot;Atkins, P. W. 2010&amp;quot; /&amp;gt; &amp;lt;ref name=&amp;quot;McQuarrie, A. 2000&amp;quot; /&amp;gt;这里为了简洁美观，省略了''kT''周围的括弧。归一化的分母''Q''（被有些作者写为''Z''）是对于系统中所有量子态进行总和，此部分又被称为[[Index.php?title=Canonical partition function|正则配分函数]]''。''&lt;br /&gt;
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It results from the constraint that the probabilities of all accessible states must add up to 1.&lt;br /&gt;
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所有量子态的概率之和为1.&lt;br /&gt;
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The Boltzmann distribution is the distribution that maximizes the [[entropy]]，&lt;br /&gt;
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&amp;lt;math&amp;gt;H(p_1,p_2,\cdots,p_M) = -\sum_{i=1}^{M} p_i\log_2 p_i&amp;lt;/math&amp;gt;&lt;br /&gt;
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subject to the constraint that &amp;lt;math&amp;gt;\sum {p_i {\varepsilon}_i} &amp;lt;/math&amp;gt; equals a particular mean energy value (which can be proven using [[Lagrange multipliers]]).&lt;br /&gt;
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当&amp;lt;math&amp;gt;\sum {p_i {\varepsilon}_i} &amp;lt;/math&amp;gt;等于平均能量值时，玻尔兹曼分布是这种情况下能让熵最大化的分布。我们可以通过拉格朗日乘数法来证明。&lt;br /&gt;
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The partition function can be calculated if we know the energies of the states accessible to the system of interest. For atoms the partition function values can be found in the NIST Atomic Spectra Database.&amp;lt;ref name=&amp;quot;:1&amp;quot;&amp;gt;[http://physics.nist.gov/PhysRefData/ASD/levels_form.html NIST Atomic Spectra Database Levels Form] at nist.gov&amp;lt;/ref&amp;gt;&lt;br /&gt;
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在知道量子态能量的情况下，这个配分函数可以被计算。对于原子来说，配分函数的值可以在NIST Atomic Spectra Database中找到。&amp;lt;ref name=&amp;quot;:1&amp;quot; /&amp;gt;&lt;br /&gt;
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The distribution shows that states with lower energy will always have a higher probability of being occupied than the states with higher energy. It can also give us the quantitative relationship between the probabilities of the two states being occupied. The ratio of probabilities for states i and j is given as&lt;br /&gt;
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玻尔兹曼分布指出，能量低的量子态总是有比能量高的量子态更高的概率被粒子占据。它同时也能让我们定量地比较两个量子态分布概率的关系。状态 i 和状态 j 的概率比为&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt;&lt;br /&gt;
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{\frac{p_i}{p_j}}=e^{({\varepsilon}_j-{\varepsilon}_i) / k T}&lt;br /&gt;
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&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
where p&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt; is the probability of state i,  p&amp;lt;sub&amp;gt;j&amp;lt;/sub&amp;gt; the probability of state j, and ε&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt; and ε&amp;lt;sub&amp;gt;j&amp;lt;/sub&amp;gt; are the energies of states i and j, respectively.&lt;br /&gt;
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其中 p&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt; 是量子态 i 的概率， p&amp;lt;sub&amp;gt;j&amp;lt;/sub&amp;gt; 是量子态 j 的概率，ε&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt; 和 ε&amp;lt;sub&amp;gt;j&amp;lt;/sub&amp;gt; 分别是状态 i 和 j 的能量。&lt;br /&gt;
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The Boltzmann distribution is often used to describe the distribution of particles, such as atoms or molecules, over energy states accessible to them. If we have a system consisting of many particles, the probability of a particle being in state i is practically the probability that, if we pick a random particle from that system and check what state it is in, we will find it is in state i. This probability is equal to the number of particles in state i divided by the total number of particles in the system, that is the fraction of particles that occupy state i.&lt;br /&gt;
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玻尔兹曼分布通常被用来描述粒子的分布，比如原子或分子，在能量状态上的分布情况。如果我们有一个由许多粒子组成的系统，某个粒子处于量子态 i 的概率就等同于当我们从该系统中选择一个随机的粒子并观察它处于什么状态，发现它处于状态 i 的概率。这个概率等于量子态 i 的粒子数除以系统中粒子的总数，即那些占据量子态i的粒子的比例。&lt;br /&gt;
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&amp;lt;math&amp;gt;&lt;br /&gt;
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p_i={\frac{N_i}{N}}&lt;br /&gt;
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&amp;lt;/math&amp;gt;&lt;br /&gt;
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where N&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt; is the number of particles in state i and N is the total number of particles in the system. We may use the Boltzmann distribution to find this probability that is, as we have seen, equal to the fraction of particles that are in state i. So the equation that gives the fraction of particles in state i as a function of the energy of that state is&lt;br /&gt;
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N&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt; 是位于量子态 i 的粒子数，N是系统中粒子的总数。我们可以用波兹曼分布来求出这个概率，它等于处于量子态i的粒子的比例。所以这个方程给出位于量子态 i 的粒子比例关于这个状态能量的函数&amp;lt;ref name=&amp;quot;Atkins, P. W. 2010&amp;quot; /&amp;gt;。&lt;br /&gt;
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&amp;lt;math&amp;gt;&lt;br /&gt;
{\frac{N_i}{N}}={\frac{e^{- {\varepsilon}_i / k T}}{\sum_{j=1}^{M}{e^{- {\varepsilon}_j / k T}}}} &lt;br /&gt;
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&amp;lt;/math&amp;gt;&lt;br /&gt;
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This equation is of great importance to [[spectroscopy]]. In spectroscopy we observe a [[spectral line]] of atoms or molecules that we are interested in going from one state to another.&amp;lt;ref name=&amp;quot;Atkins, P. W. 2010&amp;quot; /&amp;gt;&amp;lt;ref name=&amp;quot;:2&amp;quot;&amp;gt;Atkins, P. W.; de Paula J. (2009) Physical Chemistry, 9th edition, Oxford University Press, Oxford, UK&amp;lt;/ref&amp;gt; In order for this to be possible, there must be some particles in the first state to undergo the transition. We may find that this condition is fulfilled by finding the fraction of particles in the first state. If it is negligible, the transition is very likely not to be observed at the temperature for which the calculation was done. In general, a larger fraction of molecules in the first state means a higher number of transitions to the second state.&amp;lt;ref name=&amp;quot;:3&amp;quot;&amp;gt;Skoog, D. A.; Holler, F. J.; Crouch, S. R. (2006) Principles of Instrumental Analysis, Brooks/Cole, Boston, MA&amp;lt;/ref&amp;gt; This gives a stronger spectral line. However, there are other factors that influence the intensity of a spectral line, such as whether it is caused by an allowed or a [[forbidden transition]]&lt;br /&gt;
&lt;br /&gt;
这个等式对于光谱学来说很重要。在光谱中，我们期待能观察到一条原子或分子跃迁的谱线。&amp;lt;ref name=&amp;quot;Atkins, P. W. 2010&amp;quot; /&amp;gt;&amp;lt;ref name=&amp;quot;:2&amp;quot; /&amp;gt; 在为了使这成为可能，必须有一些粒子处于第一个量子态，等待着发生跃迁。我们可以通过求第一态粒子的比例来满足这个条件。如果它可以忽略不计，那么在当前计算的温度下，则很难观察到这种跃迁。一般来说，处于第一状态的分子比例越大，意味着向第二状态跃迁的次数越多。&amp;lt;ref name=&amp;quot;:3&amp;quot; /&amp;gt;这就产生了一条更强的谱线。然而，还有其他因素影响谱线的强度，例如它是否是被允许的跃迁还是被禁止的跃迁。&lt;br /&gt;
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The Boltzmann distribution is related to the [[softmax function]] commonly used in machine learning.&lt;br /&gt;
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玻尔兹曼分布与机器学习中常用的[[Index.php?title=Softmax function|归一化指数函数]]（Softmax 函数）有关。&lt;br /&gt;
=='''统计力学'''==&lt;br /&gt;
&lt;br /&gt;
{{main|Canonical ensemble|Maxwell–Boltzmann statistics}}The Boltzmann distribution appears in statistical mechanics when considering isolated (or nearly-isolated) systems of fixed composition that are in thermal equilibrium (equilibrium with respect to energy exchange). The most general case is the probability distribution for the canonical ensemble, but also some special cases (derivable from the canonical ensemble) also show the Boltzmann distribution in different aspects:&lt;br /&gt;
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当独立的(或者几乎独立的)固定体系处于统计力学热平衡状态时，玻尔兹曼分布就会出现。最普遍的情况是概率分布的正则系综，但也有一些特殊的情况(从正则系综衍生)也显示了不同形式的玻尔兹曼分布:&lt;br /&gt;
&lt;br /&gt;
;[[Canonical ensemble]] (general case)&lt;br /&gt;
;'''正则系综(一般情况)'''&lt;br /&gt;
;&lt;br /&gt;
;The [[canonical ensemble]] gives the [[probabilities]] of the various possible states of a closed system of fixed volume, in thermal equilibrium with a [[heat bath]]. The canonical ensemble is a probability distribution with the Boltzmann form.&lt;br /&gt;
&lt;br /&gt;
正则系综模型给出了在一个封闭固定体积，带有热浴的热平衡系统中的各种可能状态的概率。我们称正则系综为一个玻尔兹曼概率分布。&lt;br /&gt;
&lt;br /&gt;
;&lt;br /&gt;
;Statistical frequencies of subsystems' states (in a non-interacting collection)&lt;br /&gt;
'''子系统状态的统计频率(在一个无交互的集合中)'''&lt;br /&gt;
:When the system of interest is a collection of many non-interacting copies of a smaller subsystem, it is sometimes useful to find the [[statistical frequency]] of a given subsystem state, among the collection. The canonical ensemble has the property of separability when applied to such a collection: as long as the non-interacting subsystems have fixed composition, then each subsystem's state is independent of the others and is also characterized by a canonical ensemble. As a result, the [[expectation value|expected]] statistical frequency distribution of subsystem states has the Boltzmann form.&lt;br /&gt;
&lt;br /&gt;
当系统是一个较小子系统的许多非交互副本的集合时，有时我们需要在某个子系统集合中找到某个子系统的统计频率。当应用于这样一个集合时，这个子系统的正则系综具有可分离性: 只要不相互作用的子系统的组成是固定的，那么每个子系统的状态都是独立于其他子系统的，它们也拥有自己的正则系综。因此，子系统状态的期望统计频率分布形式是玻尔兹曼分布。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[Maxwell–Boltzmann statistics]] of classical gases (systems of non-interacting particles)&lt;br /&gt;
&lt;br /&gt;
'''Maxwell-Boltzmann 统计中的经典气体系统(非相互作用粒子系统)'''&lt;br /&gt;
&lt;br /&gt;
:In particle systems, many particles share the same space and regularly change places with each other; the single-particle state space they occupy is a shared space. [[Maxwell–Boltzmann statistics]] give the expected number of particles found in a given single-particle state, in a [[classical mechanics|classical]] gas of non-interacting particles at equilibrium. This expected number distribution has the Boltzmann form.&lt;br /&gt;
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在粒子系统中，许多粒子共享同一空间，并且相互之间有规律地改变位置; 它们所占据的单粒子状态空间是一个共享空间。[[Index.php?title=Maxwell–Boltzmann statistics|麦克斯韦-玻尔兹曼统计]]给出了在一个给定的单粒子态，在一个处于平衡状态的非相互作用粒子的经典气体中所发现的粒子的预期数量。这个预期的数量分布具有玻尔兹曼分布形式。&lt;br /&gt;
&lt;br /&gt;
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Although these cases have strong similarities, it is helpful to distinguish them as they generalize in different ways when the crucial assumptions are changed:&lt;br /&gt;
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虽然这些案例有很多相似之处，但是当关键假设发生变化时，我们需要对它们以不同的方式进行归纳总结，因此区分它们是有帮助的:&lt;br /&gt;
*When a system is in thermodynamic equilibrium with respect to both energy exchange ''and particle exchange'', the requirement of fixed composition is relaxed and a [[grand canonical ensemble]] is obtained rather than canonical ensemble. On the other hand, if both composition and energy are fixed, then a [[microcanonical ensemble]] applies instead.&lt;br /&gt;
*当一个系统在能量交换和粒子交换方面都处于热力学平衡时，固定组成的要求就放宽了。这时我们就得到了一个[[Index.php?title=Microcanonical ensemble|巨正则系综]]而不是正则系综。另一方面，如果成分和能量都是固定的，则可以使用[[微正则系综Index.php?title=Microcanonical ensemble|微正则系综]]。&lt;br /&gt;
&lt;br /&gt;
*If the subsystems within a collection ''do'' interact with each other, then the expected frequencies of subsystem states no longer follow a Boltzmann distribution, and even may not have an [[analytical solution]].&amp;lt;ref name=&amp;quot;:4&amp;quot;&amp;gt;A classic example of this is [[magnetic ordering]]. Systems of non-interacting [[spin (physics)|spins]] show [[paramagnetic]] behaviour that can be understood with a single-particle canonical ensemble (resulting in the [[Brillouin function]]). Systems of ''interacting'' spins can show much more complex behaviour such as [[ferromagnetism]] or [[antiferromagnetism]].&amp;lt;/ref&amp;gt; The canonical ensemble can however still be applied to the ''collective'' states of the entire system considered as a whole, provided the entire system is isolated and in thermal equilibrium.&lt;br /&gt;
*如果集合中的子系统确实相互交互，则子系统状态的预期频率不再遵循玻尔兹曼分布，甚至可能没有解析解。&amp;lt;ref name=&amp;quot;:4&amp;quot; /&amp;gt;但是当整个系统是独立的并且处于热平衡状态，则正则系综仍然可以应用于作为一个整体考虑。&lt;br /&gt;
&lt;br /&gt;
*With ''[[quantum mechanics|quantum]]'' gases of non-interacting particles in equilibrium, the number of particles found in a given single-particle state does not follow Maxwell–Boltzmann statistics, and there is no simple closed form expression for quantum gases in the canonical ensemble. In the grand canonical ensemble the state-filling statistics of quantum gases are described by [[Fermi–Dirac statistics]] or [[Bose–Einstein statistics]], depending on whether the particles are [[fermion]]s or [[boson]]s respectively.&lt;br /&gt;
*对于处于平衡状态的非相互作用粒子的量子气体，在给定的单粒子状态中发现的粒子数量并不遵循麦克斯韦-玻尔兹曼统计。并且正则系综中的量子气体没有简单的封闭表达式。在巨正则系综中，量子气体的统计分布状态由费米-狄拉克统计或玻色-爱因斯坦统计来描述，具体则取决于该粒子是费米子还是玻色子。&lt;br /&gt;
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==数学==&lt;br /&gt;
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In more general mathematical settings, the Boltzmann distribution is also known as the [[Gibbs measure]]. In statistics and machine learning, it is called a [[log-linear model]]. In [[deep learning]], the Boltzmann distribution is used in the sampling distribution of [[stochastic neural network]]s such as the [[Boltzmann machine]], [[Restricted Boltzmann machine]], [[Energy based model|Energy-Based models]] and [[Deep Boltzmann Machine|deep Boltzmann machine]]&lt;br /&gt;
&lt;br /&gt;
在更一般的数学环境中，玻尔兹曼分布也被称为吉布斯量度。在统计学和机器学习中，它被称为对数线性回归。在深度学习中，玻尔兹曼分布被用于随机神经网络的抽样分布，如玻尔兹曼机、受限玻尔兹曼机、基于能量的模型和深度波茨曼机。&lt;br /&gt;
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==经济==&lt;br /&gt;
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The Boltzmann distribution can be introduced to allocate permits in emissions trading.&amp;lt;ref name=&amp;quot;Park, J.-W. 2012&amp;quot;&amp;gt;Park, J.-W., Kim, C. U. and Isard, W. (2012) Permit allocation in emissions trading using the Boltzmann distribution. Physica A 391: 4883–4890&amp;lt;/ref&amp;gt;&amp;lt;ref name=&amp;quot;:5&amp;quot;&amp;gt;[http://www.technologyreview.com/view/425051/the-thorny-problem-of-fair-allocation/ The Thorny Problem Of Fair Allocation]. ''Technology Review'' blog. August 17, 2011. Cites and summarizes Park, Kim and Isard (2012).&amp;lt;/ref&amp;gt; The new allocation method using the Boltzmann distribution can describe the most probable, natural, and unbiased distribution of emissions permits among multiple countries. Simple and versatile, this new method holds potential for many economic and environmental applications.&lt;br /&gt;
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在经济学中，玻尔兹曼分布被用来分配排放交易中的许可。&amp;lt;ref name=&amp;quot;Park, J.-W. 2012&amp;quot; /&amp;gt;&amp;lt;ref name=&amp;quot;:5&amp;quot; /&amp;gt;  使用玻尔兹曼分布的新分配方法可以创造出在多个国家之间最可能的、自然的和无偏见的排放许可分配。这种新方法简单而通用，在经济和环保中有很大的应用潜力。&lt;br /&gt;
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The Boltzmann distribution has the same form as the [[Multinomial logistic regression|multinomial logit]] model. As a [[discrete choice]] model, this is very well known in economics since [[Daniel McFadden]] made the connection to random utility maximization.&lt;br /&gt;
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玻尔兹曼分布与多项逻辑回归模型具有相同的形式。在丹尼尔 · 麦克法登将它与随机效用最大化联系起来之后，成为了大家所熟知的一种离散选择模型。&lt;br /&gt;
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Category:Statistical mechanics&lt;br /&gt;
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类别: 统计力学&lt;br /&gt;
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本中文词条由[[用户:费米子|tueryeye]]编辑，欢迎在讨论页面留言。&lt;br /&gt;
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==See also==&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:Boltzmann distribution]]. Its edit history can be viewed at [[玻尔兹曼分布/edithistory]]&amp;lt;/small&amp;gt;&amp;lt;/noinclude&amp;gt;&lt;br /&gt;
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&lt;div&gt;此词条暂由tueryeye翻译和审校，翻译字数共1452，带来阅读不便，请见谅。&lt;br /&gt;
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{{Use American English|date = March 2019}}&lt;br /&gt;
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{{Short description|Probability distribution of energy states of a system}}&lt;br /&gt;
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{{about|system energy states|particle energy levels and velocities|Maxwell–Boltzmann distribution}}&lt;br /&gt;
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[[File:Boltzmann distribution graph.svg|upright=1.75|right|thumb|Boltzmann factor ''p&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;''&amp;amp;nbsp;/&amp;amp;nbsp;''p&amp;lt;sub&amp;gt;j&amp;lt;/sub&amp;gt;'' (vertical axis) as a function of temperature ''T'' for several energy differences ''ε&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;''&amp;amp;nbsp;−&amp;amp;nbsp;''ε&amp;lt;sub&amp;gt;j&amp;lt;/sub&amp;gt;''.|链接=Special:FilePath/Boltzmann_distribution_graph.svg]]&lt;br /&gt;
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In [[statistical mechanics]] and [[mathematics]], a '''Boltzmann distribution''' (also called '''Gibbs distribution'''&amp;lt;ref name=&amp;quot;landau&amp;quot;&amp;gt;{{cite book | author=Landau, Lev Davidovich |author2=Lifshitz, Evgeny Mikhailovich |name-list-style=amp | title=Statistical Physics |volume=5 |series=Course of Theoretical Physics |edition=3 |origyear=1976 |year=1980 |place=Oxford |publisher=Pergamon Press|isbn=0-7506-3372-7|author-link=Lev Landau |author2-link=Evgeny Lifshitz }} Translated by J.B. Sykes and M.J. Kearsley. See section 28&amp;lt;/ref&amp;gt;) is a [[probability distribution]] or [[probability measure]] that gives the probability that a system will be in a certain [[microstate (statistical mechanics)|state]] as a function of that state's energy and the temperature of the system. The distribution is expressed in the form:&lt;br /&gt;
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在统计力学和数学中，波兹曼分布分布(也称为吉布斯分布&amp;lt;ref name=&amp;quot;landau&amp;quot; /&amp;gt;)是一个概率分布或机率量测，它给出了一个系统处于某种量子态的概率，这个概率是该状态的能量和系统温度的函数。分布情况以下列形式表示:&lt;br /&gt;
:&amp;lt;math&amp;gt;p_i \propto e^{-\frac{\varepsilon_i}{kT}}&amp;lt;/math&amp;gt; &lt;br /&gt;
&lt;br /&gt;
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where {{mvar|p&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;}} is the probability of the system being in state {{mvar|i}}, {{mvar|ε&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;}} is the energy of that state, and a constant {{mvar|kT}} of the distribution is the product of [[Boltzmann's constant]] {{mvar|k}} and [[thermodynamic temperature]] {{mvar|T}}. The symbol &amp;lt;math display=&amp;quot;inline&amp;quot;&amp;gt;\propto&amp;lt;/math&amp;gt; denotes [[proportionality (mathematics)|proportionality]] (see {{section link||The distribution}} for the proportionality constant).&lt;br /&gt;
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{{mvar|p&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;}} 是其中系统处于状态{{mvar|i}}的概率, {{mvar|ε&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;}} 是该状态的能量，还有关于这个分布的一个常数 {{mvar|kT}} ，它是玻尔兹曼常数{{mvar|k}}和热力学温度 {{mvar|T}} 的乘积。符号 &amp;lt;math display=&amp;quot;inline&amp;quot;&amp;gt;\propto&amp;lt;/math&amp;gt;表示正比例(见附录中的比例常数)。&lt;br /&gt;
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The term system here has a very wide meaning; it can range from a single atom to a macroscopic system such as a [[Natural gas storage|natural gas storage tank]]. Because of this the Boltzmann distribution can be used to solve a very wide variety of problems. The distribution shows that states with lower energy will always have a higher probability of being occupied .&lt;br /&gt;
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这里的术语系统含义广泛， 它可以从单个原子到宏观系统，如天然气储罐。正因为如此，波兹曼分布可以用来解决各种各样的问题。玻尔兹曼分布表明，能量较低的状态被占据的概率总是较高的。&lt;br /&gt;
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The ''ratio'' of probabilities of two states is known as the '''Boltzmann factor''' and characteristically only depends on the states' energy difference:&lt;br /&gt;
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两种状态的概率之比被称为玻尔兹曼因子，取决于两种状态的能量差:&lt;br /&gt;
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&amp;lt;math&amp;gt;\frac{p_i}{p_j} = e^{\frac{\varepsilon_j - \varepsilon_i}{kT}}&amp;lt;/math&amp;gt;&lt;br /&gt;
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The Boltzmann distribution is named after [[Ludwig Boltzmann]] who first formulated it in 1868 during his studies of the [[statistical mechanics]] of gases in thermal equilibrium. Boltzmann's statistical work is borne out in his paper “On the Relationship between the Second Fundamental Theorem of the Mechanical Theory of Heat and Probability Calculations Regarding the Conditions for Thermal Equilibrium&amp;quot;&amp;lt;ref&amp;gt;http://crystal.med.upenn.edu/sharp-lab-pdfs/2015SharpMatschinsky_Boltz1877_Entropy17.pdf&amp;lt;/ref&amp;gt;. The distribution was later investigated extensively, in its modern generic form, by [[Josiah Willard Gibbs]] in 1902.&amp;lt;ref name=&amp;quot;gibbs&amp;quot;&amp;gt;{{cite book |last=Gibbs |first=Josiah Willard |authorlink=Josiah Willard Gibbs |title=Elementary Principles in Statistical Mechanics |year=1902 |publisher=[[Charles Scribner's Sons]] &lt;br /&gt;
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The distribution was later investigated extensively, in its modern generic form, by Josiah Willard Gibbs in 1902.&lt;br /&gt;
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这种分布后来在1902年由约西亚·威拉德·吉布斯进行了广泛的调查，以其现代通用形式。&lt;br /&gt;
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|location=New York|title-link=Elementary Principles in Statistical Mechanics }}&amp;lt;/ref&amp;gt;&lt;br /&gt;
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波兹曼分布是根据路德维希·玻尔兹曼1868年在研究统计力学中气体热平衡的时候首次提出的一个公式命名的。波尔兹曼的统计工作在他1877年的论文《论热力学第二基本定理与热平衡条件的概率计算之间的关系》中得到了体现。&amp;lt;ref&amp;gt;“On the Relationship between the Second Fundamental Theorem of the Mechanical Theory of Heat and Probability Calculations Regarding the Conditions for Thermal Equilibrium” Sitzungberichte der Kaiserlichen Akademie der Wissenschaften. Mathematisch-Naturwissen Classe. Abt. II, LXXVI 1877, pp 373-435 (Wien. Ber. 1877, 76:373-435). &amp;lt;/ref&amp;gt; 在玻尔兹曼分布被发明之后，约西亚·华纳德·吉布森充分地研究了它并在1902年提出了它的一般形式。&amp;lt;ref name=&amp;quot;gibbs&amp;quot; /&amp;gt;&lt;br /&gt;
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The generalized Boltzmann distribution is a sufficient and necessary condition for the equivalence between the statistical mechanics definition of [[entropy]] (The [[Entropy_(statistical_thermodynamics)#Gibbs_entropy_formula | Gibbs entropy formula]] &amp;lt;math&amp;gt;S = -k_{\mathrm{B}}\sum_i p_i \log p_i&amp;lt;/math&amp;gt;) and the thermodynamic definition of entropy (&amp;lt;math&amp;gt;d S = \frac{\delta Q_\text{rev}}{T}&amp;lt;/math&amp;gt;), and the [[fundamental thermodynamic relation]]).&amp;lt;ref name=&amp;quot;:0&amp;quot;&amp;gt;{{cite journal |last1= Gao |first1= Xiang |last2= Gallicchio |first2= Emilio |first3= Adrian |last3= Roitberg  |date= 2019 |title= The generalized Boltzmann distribution is the only distribution in which the Gibbs-Shannon entropy equals the thermodynamic entropy |journal= The Journal of Chemical Physics|volume= 151|issue= 3|pages= 034113|doi= 10.1063/1.5111333|pmid= 31325924 |arxiv= 1903.02121 |s2cid= 118981017 }}&amp;lt;/ref&amp;gt;&lt;br /&gt;
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广义波兹曼分布是熵的统计力学定义(吉布斯熵公式  &amp;lt;math&amp;gt;S = -k_{\mathrm{B}}\sum_i p_i \log p_i&amp;lt;/math&amp;gt;)与熵的热力学定义(&amp;lt;math&amp;gt;d S = \frac{\delta Q_\text{rev}}{T}&amp;lt;/math&amp;gt;)等价的充要条件。&amp;lt;ref name=&amp;quot;:0&amp;quot; /&amp;gt;&lt;br /&gt;
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The Boltzmann distribution should not be confused with the [[Maxwell–Boltzmann distribution]]. The former gives the probability that a system will be in a certain state as a function of that state's energy;&amp;lt;ref name=&amp;quot;Atkins, P. W. 2010&amp;quot;&amp;gt;Atkins, P. W. (2010) Quanta, W. H. Freeman and Company, New York&amp;lt;/ref&amp;gt; in contrast, the latter is used to describe particle speeds in idealized gases.&lt;br /&gt;
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值得一提的是，玻尔兹曼分布不应与麦克斯韦-玻尔兹曼分布混淆。前者给出了系统处于某种状态的概率，作为该状态能量的函数; 后者则是用于描述理想气体中的粒子速度。&lt;br /&gt;
==分布==&lt;br /&gt;
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The Boltzmann distribution is a [[probability distribution]] that gives the probability of a certain state as a function of that state's energy and  temperature of the [[system]] to which the distribution is applied.&amp;lt;ref name=&amp;quot;McQuarrie, A. 2000&amp;quot;&amp;gt;McQuarrie, A. (2000) Statistical Mechanics, University Science Books, California&amp;lt;/ref&amp;gt; It is given as&lt;br /&gt;
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波兹曼分布是一个概率分布，它给出了出于某种量子态处于某种能量和温度的时候的概率。它被这样定义：&lt;br /&gt;
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&amp;lt;math&amp;gt;&lt;br /&gt;
p_i=\frac{1}{Q}} {e^{- {\varepsilon}_i / k T}=\frac{e^{- {\varepsilon}_i / k T}}{\sum_{j=1}^{M}{e^{- {\varepsilon}_j / k T}}}&lt;br /&gt;
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&amp;lt;/math&amp;gt;&lt;br /&gt;
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where ''p&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;'' is the probability of state ''i'', ''ε&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;'' the energy of state ''i'', ''k'' the Boltzmann constant, ''T'' the temperature of the system and ''M'' is the number of all states accessible to the system of interest.&amp;lt;ref name=&amp;quot;McQuarrie, A. 2000&amp;quot; /&amp;gt;&amp;lt;ref name=&amp;quot;Atkins, P. W. 2010&amp;quot; /&amp;gt; Implied parentheses around the denominator ''kT'' are omitted for brevity. The normalization denominator ''Q'' (denoted by some authors by ''Z'') is the [[canonical partition function]]&lt;br /&gt;
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其中 ''p&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;'' 是状态 i 的概率，''ε&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;'' 是状态 i 的能量，''k'' 是波兹曼常数，''T'' 是系统的温度，''M'' 是系统所能到达的所有量子态的数目。&amp;lt;ref name=&amp;quot;Atkins, P. W. 2010&amp;quot; /&amp;gt; &amp;lt;ref name=&amp;quot;McQuarrie, A. 2000&amp;quot; /&amp;gt;这里为了简洁美观，省略了''kT''周围的括弧。归一化的分母''Q''（被有些作者写为''Z''）是对于系统中所有量子态进行总和，此部分又被称为[[Index.php?title=Canonical partition function|正则配分函数]]''。''&lt;br /&gt;
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It results from the constraint that the probabilities of all accessible states must add up to 1.&lt;br /&gt;
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所有量子态的概率之和为1.&lt;br /&gt;
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The Boltzmann distribution is the distribution that maximizes the [[entropy]]，&lt;br /&gt;
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&amp;lt;math&amp;gt;H(p_1,p_2,\cdots,p_M) = -\sum_{i=1}^{M} p_i\log_2 p_i&amp;lt;/math&amp;gt;&lt;br /&gt;
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subject to the constraint that &amp;lt;math&amp;gt;\sum {p_i {\varepsilon}_i} &amp;lt;/math&amp;gt; equals a particular mean energy value (which can be proven using [[Lagrange multipliers]]).&lt;br /&gt;
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当&amp;lt;math&amp;gt;\sum {p_i {\varepsilon}_i} &amp;lt;/math&amp;gt;等于平均能量值时，玻尔兹曼分布是这种情况下能让熵最大化的分布。我们可以通过拉格朗日乘数法来证明。&lt;br /&gt;
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The partition function can be calculated if we know the energies of the states accessible to the system of interest. For atoms the partition function values can be found in the NIST Atomic Spectra Database.&amp;lt;ref name=&amp;quot;:1&amp;quot;&amp;gt;[http://physics.nist.gov/PhysRefData/ASD/levels_form.html NIST Atomic Spectra Database Levels Form] at nist.gov&amp;lt;/ref&amp;gt;&lt;br /&gt;
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在知道量子态能量的情况下，这个配分函数可以被计算。对于原子来说，配分函数的值可以在NIST Atomic Spectra Database中找到。&amp;lt;ref name=&amp;quot;:1&amp;quot; /&amp;gt;&lt;br /&gt;
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The distribution shows that states with lower energy will always have a higher probability of being occupied than the states with higher energy. It can also give us the quantitative relationship between the probabilities of the two states being occupied. The ratio of probabilities for states i and j is given as&lt;br /&gt;
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玻尔兹曼分布指出，能量低的量子态总是有比能量高的量子态更高的概率被粒子占据。它同时也能让我们定量地比较两个量子态分布概率的关系。状态 i 和状态 j 的概率比为&lt;br /&gt;
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:&amp;lt;math&amp;gt;&lt;br /&gt;
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{\frac{p_i}{p_j}}=e^{({\varepsilon}_j-{\varepsilon}_i) / k T}&lt;br /&gt;
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&amp;lt;/math&amp;gt;&lt;br /&gt;
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where p&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt; is the probability of state i,  p&amp;lt;sub&amp;gt;j&amp;lt;/sub&amp;gt; the probability of state j, and ε&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt; and ε&amp;lt;sub&amp;gt;j&amp;lt;/sub&amp;gt; are the energies of states i and j, respectively.&lt;br /&gt;
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其中 p&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt; 是量子态 i 的概率， p&amp;lt;sub&amp;gt;j&amp;lt;/sub&amp;gt; 是量子态 j 的概率，ε&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt; 和 ε&amp;lt;sub&amp;gt;j&amp;lt;/sub&amp;gt; 分别是状态 i 和 j 的能量。&lt;br /&gt;
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The Boltzmann distribution is often used to describe the distribution of particles, such as atoms or molecules, over energy states accessible to them. If we have a system consisting of many particles, the probability of a particle being in state i is practically the probability that, if we pick a random particle from that system and check what state it is in, we will find it is in state i. This probability is equal to the number of particles in state i divided by the total number of particles in the system, that is the fraction of particles that occupy state i.&lt;br /&gt;
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玻尔兹曼分布通常被用来描述粒子的分布，比如原子或分子，在能量状态上的分布情况。如果我们有一个由许多粒子组成的系统，某个粒子处于量子态 i 的概率就等同于当我们从该系统中选择一个随机的粒子并观察它处于什么状态，发现它处于状态 i 的概率。这个概率等于量子态 i 的粒子数除以系统中粒子的总数，即那些占据量子态i的粒子的比例。&lt;br /&gt;
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&amp;lt;math&amp;gt;&lt;br /&gt;
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p_i={\frac{N_i}{N}}&lt;br /&gt;
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&amp;lt;/math&amp;gt;&lt;br /&gt;
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where N&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt; is the number of particles in state i and N is the total number of particles in the system. We may use the Boltzmann distribution to find this probability that is, as we have seen, equal to the fraction of particles that are in state i. So the equation that gives the fraction of particles in state i as a function of the energy of that state is&lt;br /&gt;
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N&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt; 是位于量子态 i 的粒子数，N是系统中粒子的总数。我们可以用波兹曼分布来求出这个概率，它等于处于量子态i的粒子的比例。所以这个方程给出位于量子态 i 的粒子比例关于这个状态能量的函数&amp;lt;ref name=&amp;quot;Atkins, P. W. 2010&amp;quot; /&amp;gt;。&lt;br /&gt;
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&amp;lt;math&amp;gt;&lt;br /&gt;
{\frac{N_i}{N}}={\frac{e^{- {\varepsilon}_i / k T}}{\sum_{j=1}^{M}{e^{- {\varepsilon}_j / k T}}}} &lt;br /&gt;
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&amp;lt;/math&amp;gt;&lt;br /&gt;
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This equation is of great importance to [[spectroscopy]]. In spectroscopy we observe a [[spectral line]] of atoms or molecules that we are interested in going from one state to another.&amp;lt;ref name=&amp;quot;Atkins, P. W. 2010&amp;quot; /&amp;gt;&amp;lt;ref name=&amp;quot;:2&amp;quot;&amp;gt;Atkins, P. W.; de Paula J. (2009) Physical Chemistry, 9th edition, Oxford University Press, Oxford, UK&amp;lt;/ref&amp;gt; In order for this to be possible, there must be some particles in the first state to undergo the transition. We may find that this condition is fulfilled by finding the fraction of particles in the first state. If it is negligible, the transition is very likely not to be observed at the temperature for which the calculation was done. In general, a larger fraction of molecules in the first state means a higher number of transitions to the second state.&amp;lt;ref name=&amp;quot;:3&amp;quot;&amp;gt;Skoog, D. A.; Holler, F. J.; Crouch, S. R. (2006) Principles of Instrumental Analysis, Brooks/Cole, Boston, MA&amp;lt;/ref&amp;gt; This gives a stronger spectral line. However, there are other factors that influence the intensity of a spectral line, such as whether it is caused by an allowed or a [[forbidden transition]]&lt;br /&gt;
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这个等式对于光谱学来说很重要。在光谱中，我们期待能观察到一条原子或分子跃迁的谱线。&amp;lt;ref name=&amp;quot;Atkins, P. W. 2010&amp;quot; /&amp;gt;&amp;lt;ref name=&amp;quot;:2&amp;quot; /&amp;gt; 在为了使这成为可能，必须有一些粒子处于第一个量子态，等待着发生跃迁。我们可以通过求第一态粒子的比例来满足这个条件。如果它可以忽略不计，那么在当前计算的温度下，则很难观察到这种跃迁。一般来说，处于第一状态的分子比例越大，意味着向第二状态跃迁的次数越多。&amp;lt;ref name=&amp;quot;:3&amp;quot; /&amp;gt;这就产生了一条更强的谱线。然而，还有其他因素影响谱线的强度，例如它是否是被允许的跃迁还是被禁止的跃迁。&lt;br /&gt;
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The Boltzmann distribution is related to the [[softmax function]] commonly used in machine learning.&lt;br /&gt;
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玻尔兹曼分布与机器学习中常用的[[Index.php?title=Softmax function|归一化指数函数]]（Softmax 函数）有关。&lt;br /&gt;
=='''统计力学'''==&lt;br /&gt;
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{{main|Canonical ensemble|Maxwell–Boltzmann statistics}}The Boltzmann distribution appears in statistical mechanics when considering isolated (or nearly-isolated) systems of fixed composition that are in thermal equilibrium (equilibrium with respect to energy exchange). The most general case is the probability distribution for the canonical ensemble, but also some special cases (derivable from the canonical ensemble) also show the Boltzmann distribution in different aspects:&lt;br /&gt;
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当独立的(或者几乎独立的)固定体系处于统计力学热平衡状态时，玻尔兹曼分布就会出现。最普遍的情况是概率分布的正则系综，但也有一些特殊的情况(从正则系综衍生)也显示了不同形式的玻尔兹曼分布:&lt;br /&gt;
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;[[Canonical ensemble]] (general case)&lt;br /&gt;
;'''正则系综(一般情况)'''&lt;br /&gt;
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;The [[canonical ensemble]] gives the [[probabilities]] of the various possible states of a closed system of fixed volume, in thermal equilibrium with a [[heat bath]]. The canonical ensemble is a probability distribution with the Boltzmann form.&lt;br /&gt;
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正则系综模型给出了在一个封闭固定体积，带有热浴的热平衡系统中的各种可能状态的概率。我们称正则系综为一个玻尔兹曼概率分布。&lt;br /&gt;
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;Statistical frequencies of subsystems' states (in a non-interacting collection)&lt;br /&gt;
'''子系统状态的统计频率(在一个无交互的集合中)'''&lt;br /&gt;
:When the system of interest is a collection of many non-interacting copies of a smaller subsystem, it is sometimes useful to find the [[statistical frequency]] of a given subsystem state, among the collection. The canonical ensemble has the property of separability when applied to such a collection: as long as the non-interacting subsystems have fixed composition, then each subsystem's state is independent of the others and is also characterized by a canonical ensemble. As a result, the [[expectation value|expected]] statistical frequency distribution of subsystem states has the Boltzmann form.&lt;br /&gt;
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当系统是一个较小子系统的许多非交互副本的集合时，有时我们需要在某个子系统集合中找到某个子系统的统计频率。当应用于这样一个集合时，这个子系统的正则系综具有可分离性: 只要不相互作用的子系统的组成是固定的，那么每个子系统的状态都是独立于其他子系统的，它们也拥有自己的正则系综。因此，子系统状态的期望统计频率分布形式是玻尔兹曼分布。&lt;br /&gt;
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[[Maxwell–Boltzmann statistics]] of classical gases (systems of non-interacting particles)&lt;br /&gt;
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'''Maxwell-Boltzmann 统计中的经典气体系统(非相互作用粒子系统)'''&lt;br /&gt;
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:In particle systems, many particles share the same space and regularly change places with each other; the single-particle state space they occupy is a shared space. [[Maxwell–Boltzmann statistics]] give the expected number of particles found in a given single-particle state, in a [[classical mechanics|classical]] gas of non-interacting particles at equilibrium. This expected number distribution has the Boltzmann form.&lt;br /&gt;
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在粒子系统中，许多粒子共享同一空间，并且相互之间有规律地改变位置; 它们所占据的单粒子状态空间是一个共享空间。[[Index.php?title=Maxwell–Boltzmann statistics|麦克斯韦-玻尔兹曼统计]]给出了在一个给定的单粒子态，在一个处于平衡状态的非相互作用粒子的经典气体中所发现的粒子的预期数量。这个预期的数量分布具有玻尔兹曼分布形式。&lt;br /&gt;
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Although these cases have strong similarities, it is helpful to distinguish them as they generalize in different ways when the crucial assumptions are changed:&lt;br /&gt;
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虽然这些案例有很多相似之处，但是当关键假设发生变化时，我们需要对它们以不同的方式进行归纳总结，因此区分它们是有帮助的:&lt;br /&gt;
*When a system is in thermodynamic equilibrium with respect to both energy exchange ''and particle exchange'', the requirement of fixed composition is relaxed and a [[grand canonical ensemble]] is obtained rather than canonical ensemble. On the other hand, if both composition and energy are fixed, then a [[microcanonical ensemble]] applies instead.&lt;br /&gt;
*当一个系统在能量交换和粒子交换方面都处于热力学平衡时，固定组成的要求就放宽了。这时我们就得到了一个[[Index.php?title=Microcanonical ensemble|巨正则系综]]而不是正则系综。另一方面，如果成分和能量都是固定的，则可以使用[[微正则系综Index.php?title=Microcanonical ensemble|微正则系综]]。&lt;br /&gt;
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*If the subsystems within a collection ''do'' interact with each other, then the expected frequencies of subsystem states no longer follow a Boltzmann distribution, and even may not have an [[analytical solution]].&amp;lt;ref name=&amp;quot;:4&amp;quot;&amp;gt;A classic example of this is [[magnetic ordering]]. Systems of non-interacting [[spin (physics)|spins]] show [[paramagnetic]] behaviour that can be understood with a single-particle canonical ensemble (resulting in the [[Brillouin function]]). Systems of ''interacting'' spins can show much more complex behaviour such as [[ferromagnetism]] or [[antiferromagnetism]].&amp;lt;/ref&amp;gt; The canonical ensemble can however still be applied to the ''collective'' states of the entire system considered as a whole, provided the entire system is isolated and in thermal equilibrium.&lt;br /&gt;
*如果集合中的子系统确实相互交互，则子系统状态的预期频率不再遵循玻尔兹曼分布，甚至可能没有解析解。&amp;lt;ref name=&amp;quot;:4&amp;quot; /&amp;gt;但是当整个系统是独立的并且处于热平衡状态，则正则系综仍然可以应用于作为一个整体考虑。&lt;br /&gt;
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*With ''[[quantum mechanics|quantum]]'' gases of non-interacting particles in equilibrium, the number of particles found in a given single-particle state does not follow Maxwell–Boltzmann statistics, and there is no simple closed form expression for quantum gases in the canonical ensemble. In the grand canonical ensemble the state-filling statistics of quantum gases are described by [[Fermi–Dirac statistics]] or [[Bose–Einstein statistics]], depending on whether the particles are [[fermion]]s or [[boson]]s respectively.&lt;br /&gt;
*对于处于平衡状态的非相互作用粒子的量子气体，在给定的单粒子状态中发现的粒子数量并不遵循麦克斯韦-玻尔兹曼统计。并且正则系综中的量子气体没有简单的封闭表达式。在巨正则系综中，量子气体的统计分布状态由费米-狄拉克统计或玻色-爱因斯坦统计来描述，具体则取决于该粒子是费米子还是玻色子。&lt;br /&gt;
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==数学==&lt;br /&gt;
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In more general mathematical settings, the Boltzmann distribution is also known as the [[Gibbs measure]]. In statistics and machine learning, it is called a [[log-linear model]]. In [[deep learning]], the Boltzmann distribution is used in the sampling distribution of [[stochastic neural network]]s such as the [[Boltzmann machine]], [[Restricted Boltzmann machine]], [[Energy based model|Energy-Based models]] and [[Deep Boltzmann Machine|deep Boltzmann machine]]&lt;br /&gt;
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在更一般的数学环境中，玻尔兹曼分布也被称为吉布斯量度。在统计学和机器学习中，它被称为对数线性回归。在深度学习中，玻尔兹曼分布被用于随机神经网络的抽样分布，如玻尔兹曼机、受限玻尔兹曼机、基于能量的模型和深度波茨曼机。&lt;br /&gt;
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==经济==&lt;br /&gt;
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The Boltzmann distribution can be introduced to allocate permits in emissions trading.&amp;lt;ref name=&amp;quot;Park, J.-W. 2012&amp;quot;&amp;gt;Park, J.-W., Kim, C. U. and Isard, W. (2012) Permit allocation in emissions trading using the Boltzmann distribution. Physica A 391: 4883–4890&amp;lt;/ref&amp;gt;&amp;lt;ref name=&amp;quot;:5&amp;quot;&amp;gt;[http://www.technologyreview.com/view/425051/the-thorny-problem-of-fair-allocation/ The Thorny Problem Of Fair Allocation]. ''Technology Review'' blog. August 17, 2011. Cites and summarizes Park, Kim and Isard (2012).&amp;lt;/ref&amp;gt; The new allocation method using the Boltzmann distribution can describe the most probable, natural, and unbiased distribution of emissions permits among multiple countries. Simple and versatile, this new method holds potential for many economic and environmental applications.&lt;br /&gt;
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在经济学中，玻尔兹曼分布被用来分配排放交易中的许可。&amp;lt;ref name=&amp;quot;Park, J.-W. 2012&amp;quot; /&amp;gt;&amp;lt;ref name=&amp;quot;:5&amp;quot; /&amp;gt;  使用玻尔兹曼分布的新分配方法可以创造出在多个国家之间最可能的、自然的和无偏见的排放许可分配。这种新方法简单而通用，在经济和环保中有很大的应用潜力。&lt;br /&gt;
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The Boltzmann distribution has the same form as the [[Multinomial logistic regression|multinomial logit]] model. As a [[discrete choice]] model, this is very well known in economics since [[Daniel McFadden]] made the connection to random utility maximization.&lt;br /&gt;
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玻尔兹曼分布与多项逻辑回归模型具有相同的形式。在丹尼尔 · 麦克法登将它与随机效用最大化联系起来之后，成为了大家所熟知的一种离散选择模型。&lt;br /&gt;
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Category:Statistical mechanics&lt;br /&gt;
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类别: 统计力学&lt;br /&gt;
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本中文词条由[[用户:费米子|tueryeye]]编辑，欢迎在讨论页面留言。&lt;br /&gt;
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==See also==&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:Boltzmann distribution]]. Its edit history can be viewed at [[玻尔兹曼分布/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;br /&gt;
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&amp;lt;references /&amp;gt;&lt;/div&gt;</summary>
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		<title>玻尔兹曼分布</title>
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&lt;div&gt;此词条暂由tueryeye翻译和审校，翻译字数共1452，带来阅读不便，请见谅。&lt;br /&gt;
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{{Use American English|date = March 2019}}&lt;br /&gt;
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{{Short description|Probability distribution of energy states of a system}}&lt;br /&gt;
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{{about|system energy states|particle energy levels and velocities|Maxwell–Boltzmann distribution}}&lt;br /&gt;
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[[File:Boltzmann distribution graph.svg|upright=1.75|right|thumb|Boltzmann factor ''p&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;''&amp;amp;nbsp;/&amp;amp;nbsp;''p&amp;lt;sub&amp;gt;j&amp;lt;/sub&amp;gt;'' (vertical axis) as a function of temperature ''T'' for several energy differences ''ε&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;''&amp;amp;nbsp;−&amp;amp;nbsp;''ε&amp;lt;sub&amp;gt;j&amp;lt;/sub&amp;gt;''.|链接=Special:FilePath/Boltzmann_distribution_graph.svg]]&lt;br /&gt;
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In [[statistical mechanics]] and [[mathematics]], a '''Boltzmann distribution''' (also called '''Gibbs distribution'''&amp;lt;ref name=&amp;quot;landau&amp;quot;&amp;gt;{{cite book | author=Landau, Lev Davidovich |author2=Lifshitz, Evgeny Mikhailovich |name-list-style=amp | title=Statistical Physics |volume=5 |series=Course of Theoretical Physics |edition=3 |origyear=1976 |year=1980 |place=Oxford |publisher=Pergamon Press|isbn=0-7506-3372-7|author-link=Lev Landau |author2-link=Evgeny Lifshitz }} Translated by J.B. Sykes and M.J. Kearsley. See section 28&amp;lt;/ref&amp;gt;) is a [[probability distribution]] or [[probability measure]] that gives the probability that a system will be in a certain [[microstate (statistical mechanics)|state]] as a function of that state's energy and the temperature of the system. The distribution is expressed in the form:&lt;br /&gt;
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在统计力学和数学中，波兹曼分布分布(也称为吉布斯分布&amp;lt;ref name=&amp;quot;landau&amp;quot; /&amp;gt;)是一个概率分布或机率量测，它给出了一个系统处于某种量子态的概率，这个概率是该状态的能量和系统温度的函数。分布情况以下列形式表示:&lt;br /&gt;
:&amp;lt;math&amp;gt;p_i \propto e^{-\frac{\varepsilon_i}{kT}}&amp;lt;/math&amp;gt; &lt;br /&gt;
&lt;br /&gt;
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where {{mvar|p&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;}} is the probability of the system being in state {{mvar|i}}, {{mvar|ε&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;}} is the energy of that state, and a constant {{mvar|kT}} of the distribution is the product of [[Boltzmann's constant]] {{mvar|k}} and [[thermodynamic temperature]] {{mvar|T}}. The symbol &amp;lt;math display=&amp;quot;inline&amp;quot;&amp;gt;\propto&amp;lt;/math&amp;gt; denotes [[proportionality (mathematics)|proportionality]] (see {{section link||The distribution}} for the proportionality constant).&lt;br /&gt;
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{{mvar|p&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;}} 是其中系统处于状态{{mvar|i}}的概率, {{mvar|ε&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;}} 是该状态的能量，还有关于这个分布的一个常数 {{mvar|kT}} ，它是玻尔兹曼常数{{mvar|k}}和热力学温度 {{mvar|T}} 的乘积。符号 &amp;lt;math display=&amp;quot;inline&amp;quot;&amp;gt;\propto&amp;lt;/math&amp;gt;表示正比例(见附录中的比例常数)。&lt;br /&gt;
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The term system here has a very wide meaning; it can range from a single atom to a macroscopic system such as a [[Natural gas storage|natural gas storage tank]]. Because of this the Boltzmann distribution can be used to solve a very wide variety of problems. The distribution shows that states with lower energy will always have a higher probability of being occupied .&lt;br /&gt;
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这里的术语系统含义广泛， 它可以从单个原子到宏观系统，如天然气储罐。正因为如此，波兹曼分布可以用来解决各种各样的问题。玻尔兹曼分布表明，能量较低的状态被占据的概率总是较高的。&lt;br /&gt;
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The ''ratio'' of probabilities of two states is known as the '''Boltzmann factor''' and characteristically only depends on the states' energy difference:&lt;br /&gt;
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两种状态的概率之比被称为玻尔兹曼因子，取决于两种状态的能量差:&lt;br /&gt;
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&amp;lt;math&amp;gt;\frac{p_i}{p_j} = e^{\frac{\varepsilon_j - \varepsilon_i}{kT}}&amp;lt;/math&amp;gt;&lt;br /&gt;
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The Boltzmann distribution is named after [[Ludwig Boltzmann]] who first formulated it in 1868 during his studies of the [[statistical mechanics]] of gases in thermal equilibrium. Boltzmann's statistical work is borne out in his paper “On the Relationship between the Second Fundamental Theorem of the Mechanical Theory of Heat and Probability Calculations Regarding the Conditions for Thermal Equilibrium&amp;quot;&amp;lt;ref&amp;gt;http://crystal.med.upenn.edu/sharp-lab-pdfs/2015SharpMatschinsky_Boltz1877_Entropy17.pdf&amp;lt;/ref&amp;gt;. The distribution was later investigated extensively, in its modern generic form, by [[Josiah Willard Gibbs]] in 1902.&amp;lt;ref name=&amp;quot;gibbs&amp;quot;&amp;gt;{{cite book |last=Gibbs |first=Josiah Willard |authorlink=Josiah Willard Gibbs |title=Elementary Principles in Statistical Mechanics |year=1902 |publisher=[[Charles Scribner's Sons]] &lt;br /&gt;
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The distribution was later investigated extensively, in its modern generic form, by Josiah Willard Gibbs in 1902.&lt;br /&gt;
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这种分布后来在1902年由约西亚·威拉德·吉布斯进行了广泛的调查，以其现代通用形式。&lt;br /&gt;
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|location=New York|title-link=Elementary Principles in Statistical Mechanics }}&amp;lt;/ref&amp;gt;&lt;br /&gt;
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波兹曼分布是根据路德维希·玻尔兹曼1868年在研究统计力学中气体热平衡的时候首次提出的一个公式命名的。波尔兹曼的统计工作在他1877年的论文《论热力学第二基本定理与热平衡条件的概率计算之间的关系》中得到了体现。&amp;lt;ref&amp;gt;“On the Relationship between the Second Fundamental Theorem of the Mechanical Theory of Heat and Probability Calculations Regarding the Conditions for Thermal Equilibrium” Sitzungberichte der Kaiserlichen Akademie der Wissenschaften. Mathematisch-Naturwissen Classe. Abt. II, LXXVI 1877, pp 373-435 (Wien. Ber. 1877, 76:373-435). &amp;lt;/ref&amp;gt; 在玻尔兹曼分布被发明之后，约西亚·华纳德·吉布森充分地研究了它并在1902年提出了它的一般形式。&amp;lt;ref name=&amp;quot;gibbs&amp;quot; /&amp;gt;&lt;br /&gt;
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The generalized Boltzmann distribution is a sufficient and necessary condition for the equivalence between the statistical mechanics definition of [[entropy]] (The [[Entropy_(statistical_thermodynamics)#Gibbs_entropy_formula | Gibbs entropy formula]] &amp;lt;math&amp;gt;S = -k_{\mathrm{B}}\sum_i p_i \log p_i&amp;lt;/math&amp;gt;) and the thermodynamic definition of entropy (&amp;lt;math&amp;gt;d S = \frac{\delta Q_\text{rev}}{T}&amp;lt;/math&amp;gt;, and the [[fundamental thermodynamic relation]]).&amp;lt;ref name=&amp;quot;:0&amp;quot;&amp;gt;{{cite journal |last1= Gao |first1= Xiang |last2= Gallicchio |first2= Emilio |first3= Adrian |last3= Roitberg  |date= 2019 |title= The generalized Boltzmann distribution is the only distribution in which the Gibbs-Shannon entropy equals the thermodynamic entropy |journal= The Journal of Chemical Physics|volume= 151|issue= 3|pages= 034113|doi= 10.1063/1.5111333|pmid= 31325924 |arxiv= 1903.02121 |s2cid= 118981017 }}&amp;lt;/ref&amp;gt;&lt;br /&gt;
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广义波兹曼分布是熵的统计力学定义(吉布斯熵公式  &amp;lt;math&amp;gt;S = -k_{\mathrm{B}}\sum_i p_i \log p_i&amp;lt;/math&amp;gt;)与熵的热力学定义(&amp;lt;math&amp;gt;d S = \frac{\delta Q_\text{rev}}{T}&amp;lt;/math&amp;gt;)等价的充要条件。&amp;lt;ref name=&amp;quot;:0&amp;quot; /&amp;gt;&lt;br /&gt;
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The Boltzmann distribution should not be confused with the [[Maxwell–Boltzmann distribution]]. The former gives the probability that a system will be in a certain state as a function of that state's energy;&amp;lt;ref name=&amp;quot;Atkins, P. W. 2010&amp;quot;&amp;gt;Atkins, P. W. (2010) Quanta, W. H. Freeman and Company, New York&amp;lt;/ref&amp;gt; in contrast, the latter is used to describe particle speeds in idealized gases.&lt;br /&gt;
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值得一提的是，玻尔兹曼分布不应与麦克斯韦-玻尔兹曼分布混淆。前者给出了系统处于某种状态的概率，作为该状态能量的函数; 后者则是用于描述理想气体中的粒子速度。&lt;br /&gt;
==分布==&lt;br /&gt;
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The Boltzmann distribution is a [[probability distribution]] that gives the probability of a certain state as a function of that state's energy and  temperature of the [[system]] to which the distribution is applied.&amp;lt;ref name=&amp;quot;McQuarrie, A. 2000&amp;quot;&amp;gt;McQuarrie, A. (2000) Statistical Mechanics, University Science Books, California&amp;lt;/ref&amp;gt; It is given as&lt;br /&gt;
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波兹曼分布是一个概率分布，它给出了出于某种量子态处于某种能量和温度的时候的概率。它被这样定义：&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt;&lt;br /&gt;
p_i=\frac{1}{Q}} {e^{- {\varepsilon}_i / k T}=\frac{e^{- {\varepsilon}_i / k T}}{\sum_{j=1}^{M}{e^{- {\varepsilon}_j / k T}}}&lt;br /&gt;
&lt;br /&gt;
&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
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where ''p&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;'' is the probability of state ''i'', ''ε&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;'' the energy of state ''i'', ''k'' the Boltzmann constant, ''T'' the temperature of the system and ''M'' is the number of all states accessible to the system of interest.&amp;lt;ref name=&amp;quot;McQuarrie, A. 2000&amp;quot; /&amp;gt;&amp;lt;ref name=&amp;quot;Atkins, P. W. 2010&amp;quot; /&amp;gt; Implied parentheses around the denominator ''kT'' are omitted for brevity. The normalization denominator ''Q'' (denoted by some authors by ''Z'') is the [[canonical partition function]]&lt;br /&gt;
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其中 ''p&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;'' 是状态 i 的概率，''ε&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;'' 是状态 i 的能量，''k'' 是波兹曼常数，''T'' 是系统的温度，''M'' 是系统所能到达的所有量子态的数目。&amp;lt;ref name=&amp;quot;Atkins, P. W. 2010&amp;quot; /&amp;gt; &amp;lt;ref name=&amp;quot;McQuarrie, A. 2000&amp;quot; /&amp;gt;这里为了简洁美观，省略了''kT''周围的括弧。归一化的分母''Q''（被有些作者写为''Z''）是对于系统中所有量子态进行总和，此部分又被称为[[Index.php?title=Canonical partition function|正则配分函数]]''。''&lt;br /&gt;
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It results from the constraint that the probabilities of all accessible states must add up to 1.&lt;br /&gt;
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所有量子态的概率之和为1.&lt;br /&gt;
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The Boltzmann distribution is the distribution that maximizes the [[entropy]]，&lt;br /&gt;
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&amp;lt;math&amp;gt;H(p_1,p_2,\cdots,p_M) = -\sum_{i=1}^{M} p_i\log_2 p_i&amp;lt;/math&amp;gt;&lt;br /&gt;
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subject to the constraint that &amp;lt;math&amp;gt;\sum {p_i {\varepsilon}_i} &amp;lt;/math&amp;gt; equals a particular mean energy value (which can be proven using [[Lagrange multipliers]]).&lt;br /&gt;
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当&amp;lt;math&amp;gt;\sum {p_i {\varepsilon}_i} &amp;lt;/math&amp;gt;等于平均能量值时，玻尔兹曼分布是这种情况下能让熵最大化的分布。我们可以通过拉格朗日乘数法来证明。&lt;br /&gt;
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The partition function can be calculated if we know the energies of the states accessible to the system of interest. For atoms the partition function values can be found in the NIST Atomic Spectra Database.&amp;lt;ref name=&amp;quot;:1&amp;quot;&amp;gt;[http://physics.nist.gov/PhysRefData/ASD/levels_form.html NIST Atomic Spectra Database Levels Form] at nist.gov&amp;lt;/ref&amp;gt;&lt;br /&gt;
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在知道量子态能量的情况下，这个配分函数可以被计算。对于原子来说，配分函数的值可以在NIST Atomic Spectra Database中找到。&amp;lt;ref name=&amp;quot;:1&amp;quot; /&amp;gt;&lt;br /&gt;
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The distribution shows that states with lower energy will always have a higher probability of being occupied than the states with higher energy. It can also give us the quantitative relationship between the probabilities of the two states being occupied. The ratio of probabilities for states i and j is given as&lt;br /&gt;
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玻尔兹曼分布指出，能量低的量子态总是有比能量高的量子态更高的概率被粒子占据。它同时也能让我们定量地比较两个量子态分布概率的关系。状态 i 和状态 j 的概率比为&lt;br /&gt;
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:&amp;lt;math&amp;gt;&lt;br /&gt;
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{\frac{p_i}{p_j}}=e^{({\varepsilon}_j-{\varepsilon}_i) / k T}&lt;br /&gt;
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&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
where p&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt; is the probability of state i,  p&amp;lt;sub&amp;gt;j&amp;lt;/sub&amp;gt; the probability of state j, and ε&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt; and ε&amp;lt;sub&amp;gt;j&amp;lt;/sub&amp;gt; are the energies of states i and j, respectively.&lt;br /&gt;
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其中 p&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt; 是量子态 i 的概率， p&amp;lt;sub&amp;gt;j&amp;lt;/sub&amp;gt; 是量子态 j 的概率，ε&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt; 和 ε&amp;lt;sub&amp;gt;j&amp;lt;/sub&amp;gt; 分别是状态 i 和 j 的能量。&lt;br /&gt;
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The Boltzmann distribution is often used to describe the distribution of particles, such as atoms or molecules, over energy states accessible to them. If we have a system consisting of many particles, the probability of a particle being in state i is practically the probability that, if we pick a random particle from that system and check what state it is in, we will find it is in state i. This probability is equal to the number of particles in state i divided by the total number of particles in the system, that is the fraction of particles that occupy state i.&lt;br /&gt;
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玻尔兹曼分布通常被用来描述粒子的分布，比如原子或分子，在能量状态上的分布情况。如果我们有一个由许多粒子组成的系统，某个粒子处于量子态 i 的概率就等同于当我们从该系统中选择一个随机的粒子并观察它处于什么状态，发现它处于状态 i 的概率。这个概率等于量子态 i 的粒子数除以系统中粒子的总数，即那些占据量子态i的粒子的比例。&lt;br /&gt;
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&amp;lt;math&amp;gt;&lt;br /&gt;
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p_i={\frac{N_i}{N}}&lt;br /&gt;
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&amp;lt;/math&amp;gt;&lt;br /&gt;
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where N&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt; is the number of particles in state i and N is the total number of particles in the system. We may use the Boltzmann distribution to find this probability that is, as we have seen, equal to the fraction of particles that are in state i. So the equation that gives the fraction of particles in state i as a function of the energy of that state is&lt;br /&gt;
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N&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt; 是位于量子态 i 的粒子数，N是系统中粒子的总数。我们可以用波兹曼分布来求出这个概率，它等于处于量子态i的粒子的比例。所以这个方程给出位于量子态 i 的粒子比例关于这个状态能量的函数&amp;lt;ref name=&amp;quot;Atkins, P. W. 2010&amp;quot; /&amp;gt;。&lt;br /&gt;
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&amp;lt;math&amp;gt;&lt;br /&gt;
{\frac{N_i}{N}}={\frac{e^{- {\varepsilon}_i / k T}}{\sum_{j=1}^{M}{e^{- {\varepsilon}_j / k T}}}} &lt;br /&gt;
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&amp;lt;/math&amp;gt;&lt;br /&gt;
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This equation is of great importance to [[spectroscopy]]. In spectroscopy we observe a [[spectral line]] of atoms or molecules that we are interested in going from one state to another.&amp;lt;ref name=&amp;quot;Atkins, P. W. 2010&amp;quot; /&amp;gt;&amp;lt;ref name=&amp;quot;:2&amp;quot;&amp;gt;Atkins, P. W.; de Paula J. (2009) Physical Chemistry, 9th edition, Oxford University Press, Oxford, UK&amp;lt;/ref&amp;gt; In order for this to be possible, there must be some particles in the first state to undergo the transition. We may find that this condition is fulfilled by finding the fraction of particles in the first state. If it is negligible, the transition is very likely not to be observed at the temperature for which the calculation was done. In general, a larger fraction of molecules in the first state means a higher number of transitions to the second state.&amp;lt;ref name=&amp;quot;:3&amp;quot;&amp;gt;Skoog, D. A.; Holler, F. J.; Crouch, S. R. (2006) Principles of Instrumental Analysis, Brooks/Cole, Boston, MA&amp;lt;/ref&amp;gt; This gives a stronger spectral line. However, there are other factors that influence the intensity of a spectral line, such as whether it is caused by an allowed or a [[forbidden transition]]&lt;br /&gt;
&lt;br /&gt;
这个等式对于光谱学来说很重要。在光谱中，我们期待能观察到一条原子或分子跃迁的谱线。&amp;lt;ref name=&amp;quot;Atkins, P. W. 2010&amp;quot; /&amp;gt;&amp;lt;ref name=&amp;quot;:2&amp;quot; /&amp;gt; 在为了使这成为可能，必须有一些粒子处于第一个量子态，等待着发生跃迁。我们可以通过求第一态粒子的比例来满足这个条件。如果它可以忽略不计，那么在当前计算的温度下，则很难观察到这种跃迁。一般来说，处于第一状态的分子比例越大，意味着向第二状态跃迁的次数越多。&amp;lt;ref name=&amp;quot;:3&amp;quot; /&amp;gt;这就产生了一条更强的谱线。然而，还有其他因素影响谱线的强度，例如它是否是被允许的跃迁还是被禁止的跃迁。&lt;br /&gt;
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The Boltzmann distribution is related to the [[softmax function]] commonly used in machine learning.&lt;br /&gt;
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玻尔兹曼分布与机器学习中常用的[[Index.php?title=Softmax function|归一化指数函数]]（Softmax 函数）有关。&lt;br /&gt;
=='''统计力学'''==&lt;br /&gt;
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{{main|Canonical ensemble|Maxwell–Boltzmann statistics}}The Boltzmann distribution appears in statistical mechanics when considering isolated (or nearly-isolated) systems of fixed composition that are in thermal equilibrium (equilibrium with respect to energy exchange). The most general case is the probability distribution for the canonical ensemble, but also some special cases (derivable from the canonical ensemble) also show the Boltzmann distribution in different aspects:&lt;br /&gt;
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当独立的(或者几乎独立的)固定体系处于统计力学热平衡状态时，玻尔兹曼分布就会出现。最普遍的情况是概率分布的正则系综，但也有一些特殊的情况(从正则系综衍生)也显示了不同形式的玻尔兹曼分布:&lt;br /&gt;
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;[[Canonical ensemble]] (general case)&lt;br /&gt;
;'''正则系综(一般情况)'''&lt;br /&gt;
;&lt;br /&gt;
;The [[canonical ensemble]] gives the [[probabilities]] of the various possible states of a closed system of fixed volume, in thermal equilibrium with a [[heat bath]]. The canonical ensemble is a probability distribution with the Boltzmann form.&lt;br /&gt;
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正则系综模型给出了在一个封闭固定体积，带有热浴的热平衡系统中的各种可能状态的概率。我们称正则系综为一个玻尔兹曼概率分布。&lt;br /&gt;
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;&lt;br /&gt;
;Statistical frequencies of subsystems' states (in a non-interacting collection)&lt;br /&gt;
'''子系统状态的统计频率(在一个无交互的集合中)'''&lt;br /&gt;
:When the system of interest is a collection of many non-interacting copies of a smaller subsystem, it is sometimes useful to find the [[statistical frequency]] of a given subsystem state, among the collection. The canonical ensemble has the property of separability when applied to such a collection: as long as the non-interacting subsystems have fixed composition, then each subsystem's state is independent of the others and is also characterized by a canonical ensemble. As a result, the [[expectation value|expected]] statistical frequency distribution of subsystem states has the Boltzmann form.&lt;br /&gt;
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当系统是一个较小子系统的许多非交互副本的集合时，有时我们需要在某个子系统集合中找到某个子系统的统计频率。当应用于这样一个集合时，这个子系统的正则系综具有可分离性: 只要不相互作用的子系统的组成是固定的，那么每个子系统的状态都是独立于其他子系统的，它们也拥有自己的正则系综。因此，子系统状态的期望统计频率分布形式是玻尔兹曼分布。&lt;br /&gt;
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[[Maxwell–Boltzmann statistics]] of classical gases (systems of non-interacting particles)&lt;br /&gt;
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'''Maxwell-Boltzmann 统计中的经典气体系统(非相互作用粒子系统)'''&lt;br /&gt;
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:In particle systems, many particles share the same space and regularly change places with each other; the single-particle state space they occupy is a shared space. [[Maxwell–Boltzmann statistics]] give the expected number of particles found in a given single-particle state, in a [[classical mechanics|classical]] gas of non-interacting particles at equilibrium. This expected number distribution has the Boltzmann form.&lt;br /&gt;
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在粒子系统中，许多粒子共享同一空间，并且相互之间有规律地改变位置; 它们所占据的单粒子状态空间是一个共享空间。[[Index.php?title=Maxwell–Boltzmann statistics|麦克斯韦-玻尔兹曼统计]]给出了在一个给定的单粒子态，在一个处于平衡状态的非相互作用粒子的经典气体中所发现的粒子的预期数量。这个预期的数量分布具有玻尔兹曼分布形式。&lt;br /&gt;
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Although these cases have strong similarities, it is helpful to distinguish them as they generalize in different ways when the crucial assumptions are changed:&lt;br /&gt;
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虽然这些案例有很多相似之处，但是当关键假设发生变化时，我们需要对它们以不同的方式进行归纳总结，因此区分它们是有帮助的:&lt;br /&gt;
*When a system is in thermodynamic equilibrium with respect to both energy exchange ''and particle exchange'', the requirement of fixed composition is relaxed and a [[grand canonical ensemble]] is obtained rather than canonical ensemble. On the other hand, if both composition and energy are fixed, then a [[microcanonical ensemble]] applies instead.&lt;br /&gt;
*当一个系统在能量交换和粒子交换方面都处于热力学平衡时，固定组成的要求就放宽了。这时我们就得到了一个[[Index.php?title=Microcanonical ensemble|巨正则系综]]而不是正则系综。另一方面，如果成分和能量都是固定的，则可以使用[[微正则系综Index.php?title=Microcanonical ensemble|微正则系综]]。&lt;br /&gt;
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*If the subsystems within a collection ''do'' interact with each other, then the expected frequencies of subsystem states no longer follow a Boltzmann distribution, and even may not have an [[analytical solution]].&amp;lt;ref name=&amp;quot;:4&amp;quot;&amp;gt;A classic example of this is [[magnetic ordering]]. Systems of non-interacting [[spin (physics)|spins]] show [[paramagnetic]] behaviour that can be understood with a single-particle canonical ensemble (resulting in the [[Brillouin function]]). Systems of ''interacting'' spins can show much more complex behaviour such as [[ferromagnetism]] or [[antiferromagnetism]].&amp;lt;/ref&amp;gt; The canonical ensemble can however still be applied to the ''collective'' states of the entire system considered as a whole, provided the entire system is isolated and in thermal equilibrium.&lt;br /&gt;
*如果集合中的子系统确实相互交互，则子系统状态的预期频率不再遵循玻尔兹曼分布，甚至可能没有解析解。&amp;lt;ref name=&amp;quot;:4&amp;quot; /&amp;gt;但是当整个系统是独立的并且处于热平衡状态，则正则系综仍然可以应用于作为一个整体考虑。&lt;br /&gt;
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*With ''[[quantum mechanics|quantum]]'' gases of non-interacting particles in equilibrium, the number of particles found in a given single-particle state does not follow Maxwell–Boltzmann statistics, and there is no simple closed form expression for quantum gases in the canonical ensemble. In the grand canonical ensemble the state-filling statistics of quantum gases are described by [[Fermi–Dirac statistics]] or [[Bose–Einstein statistics]], depending on whether the particles are [[fermion]]s or [[boson]]s respectively.&lt;br /&gt;
*对于处于平衡状态的非相互作用粒子的量子气体，在给定的单粒子状态中发现的粒子数量并不遵循麦克斯韦-玻尔兹曼统计。并且正则系综中的量子气体没有简单的封闭表达式。在巨正则系综中，量子气体的统计分布状态由费米-狄拉克统计或玻色-爱因斯坦统计来描述，具体则取决于该粒子是费米子还是玻色子。&lt;br /&gt;
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==数学==&lt;br /&gt;
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In more general mathematical settings, the Boltzmann distribution is also known as the [[Gibbs measure]]. In statistics and machine learning, it is called a [[log-linear model]]. In [[deep learning]], the Boltzmann distribution is used in the sampling distribution of [[stochastic neural network]]s such as the [[Boltzmann machine]], [[Restricted Boltzmann machine]], [[Energy based model|Energy-Based models]] and [[Deep Boltzmann Machine|deep Boltzmann machine]]&lt;br /&gt;
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在更一般的数学环境中，玻尔兹曼分布也被称为吉布斯量度。在统计学和机器学习中，它被称为对数线性回归。在深度学习中，玻尔兹曼分布被用于随机神经网络的抽样分布，如玻尔兹曼机、受限玻尔兹曼机、基于能量的模型和深度波茨曼机。&lt;br /&gt;
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==经济==&lt;br /&gt;
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The Boltzmann distribution can be introduced to allocate permits in emissions trading.&amp;lt;ref name=&amp;quot;Park, J.-W. 2012&amp;quot;&amp;gt;Park, J.-W., Kim, C. U. and Isard, W. (2012) Permit allocation in emissions trading using the Boltzmann distribution. Physica A 391: 4883–4890&amp;lt;/ref&amp;gt;&amp;lt;ref name=&amp;quot;:5&amp;quot;&amp;gt;[http://www.technologyreview.com/view/425051/the-thorny-problem-of-fair-allocation/ The Thorny Problem Of Fair Allocation]. ''Technology Review'' blog. August 17, 2011. Cites and summarizes Park, Kim and Isard (2012).&amp;lt;/ref&amp;gt; The new allocation method using the Boltzmann distribution can describe the most probable, natural, and unbiased distribution of emissions permits among multiple countries. Simple and versatile, this new method holds potential for many economic and environmental applications.&lt;br /&gt;
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在经济学中，玻尔兹曼分布被用来分配排放交易中的许可。&amp;lt;ref name=&amp;quot;Park, J.-W. 2012&amp;quot; /&amp;gt;&amp;lt;ref name=&amp;quot;:5&amp;quot; /&amp;gt;  使用玻尔兹曼分布的新分配方法可以创造出在多个国家之间最可能的、自然的和无偏见的排放许可分配。这种新方法简单而通用，在经济和环保中有很大的应用潜力。&lt;br /&gt;
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The Boltzmann distribution has the same form as the [[Multinomial logistic regression|multinomial logit]] model. As a [[discrete choice]] model, this is very well known in economics since [[Daniel McFadden]] made the connection to random utility maximization.&lt;br /&gt;
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玻尔兹曼分布与多项逻辑回归模型具有相同的形式。在丹尼尔 · 麦克法登将它与随机效用最大化联系起来之后，成为了大家所熟知的一种离散选择模型。&lt;br /&gt;
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Category:Statistical mechanics&lt;br /&gt;
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类别: 统计力学&lt;br /&gt;
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本中文词条由[[用户:费米子|tueryeye]]编辑，欢迎在讨论页面留言。&lt;br /&gt;
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==See also==&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:Boltzmann distribution]]. Its edit history can be viewed at [[玻尔兹曼分布/edithistory]]&amp;lt;/small&amp;gt;&amp;lt;/noinclude&amp;gt;&lt;br /&gt;
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&lt;div&gt;此词条暂由tueryeye翻译和审校，翻译字数共1452，带来阅读不便，请见谅。&lt;br /&gt;
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{{Use American English|date = March 2019}}&lt;br /&gt;
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{{Short description|Probability distribution of energy states of a system}}&lt;br /&gt;
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{{about|system energy states|particle energy levels and velocities|Maxwell–Boltzmann distribution}}&lt;br /&gt;
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[[File:Boltzmann distribution graph.svg|upright=1.75|right|thumb|Boltzmann factor ''p&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;''&amp;amp;nbsp;/&amp;amp;nbsp;''p&amp;lt;sub&amp;gt;j&amp;lt;/sub&amp;gt;'' (vertical axis) as a function of temperature ''T'' for several energy differences ''ε&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;''&amp;amp;nbsp;−&amp;amp;nbsp;''ε&amp;lt;sub&amp;gt;j&amp;lt;/sub&amp;gt;''.|链接=Special:FilePath/Boltzmann_distribution_graph.svg]]&lt;br /&gt;
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In [[statistical mechanics]] and [[mathematics]], a '''Boltzmann distribution''' (also called '''Gibbs distribution'''&amp;lt;ref name=&amp;quot;landau&amp;quot;&amp;gt;{{cite book | author=Landau, Lev Davidovich |author2=Lifshitz, Evgeny Mikhailovich |name-list-style=amp | title=Statistical Physics |volume=5 |series=Course of Theoretical Physics |edition=3 |origyear=1976 |year=1980 |place=Oxford |publisher=Pergamon Press|isbn=0-7506-3372-7|author-link=Lev Landau |author2-link=Evgeny Lifshitz }} Translated by J.B. Sykes and M.J. Kearsley. See section 28&amp;lt;/ref&amp;gt;) is a [[probability distribution]] or [[probability measure]] that gives the probability that a system will be in a certain [[microstate (statistical mechanics)|state]] as a function of that state's energy and the temperature of the system. The distribution is expressed in the form:&lt;br /&gt;
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在统计力学和数学中，波兹曼分布分布(也称为吉布斯分布&amp;lt;ref name=&amp;quot;landau&amp;quot; /&amp;gt;)是一个概率分布或机率量测，它给出了一个系统处于某种量子态的概率，这个概率是该状态的能量和系统温度的函数。分布情况以下列形式表示:&lt;br /&gt;
:&amp;lt;math&amp;gt;p_i \propto e^{-\frac{\varepsilon_i}{kT}}&amp;lt;/math&amp;gt; &lt;br /&gt;
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where {{mvar|p&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;}} is the probability of the system being in state {{mvar|i}}, {{mvar|ε&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;}} is the energy of that state, and a constant {{mvar|kT}} of the distribution is the product of [[Boltzmann's constant]] {{mvar|k}} and [[thermodynamic temperature]] {{mvar|T}}. The symbol &amp;lt;math display=&amp;quot;inline&amp;quot;&amp;gt;\propto&amp;lt;/math&amp;gt; denotes [[proportionality (mathematics)|proportionality]] (see {{section link||The distribution}} for the proportionality constant).&lt;br /&gt;
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{{mvar|p&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;}} 是其中系统处于状态{{mvar|i}}的概率, {{mvar|ε&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;}} 是该状态的能量，还有关于这个分布的一个常数 {{mvar|kT}} ，它是玻尔兹曼常数{{mvar|k}}和热力学温度 {{mvar|T}} 的乘积。符号 &amp;lt;math display=&amp;quot;inline&amp;quot;&amp;gt;\propto&amp;lt;/math&amp;gt;表示正比例(见附录中的比例常数)。&lt;br /&gt;
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The term system here has a very wide meaning; it can range from a single atom to a macroscopic system such as a [[Natural gas storage|natural gas storage tank]]. Because of this the Boltzmann distribution can be used to solve a very wide variety of problems. The distribution shows that states with lower energy will always have a higher probability of being occupied .&lt;br /&gt;
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这里的术语系统含义广泛; 它可以从单个原子到宏观系统，如天然气储罐。正因为如此，波兹曼分布可以用来解决各种各样的问题。玻尔兹曼分布表明，能量较低的状态被占据的概率总是较高的。&lt;br /&gt;
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The ''ratio'' of probabilities of two states is known as the '''Boltzmann factor''' and characteristically only depends on the states' energy difference:&lt;br /&gt;
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两种状态的概率之比被称为玻尔兹曼因子，取决于两种状态的能量差:&lt;br /&gt;
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&amp;lt;math&amp;gt;\frac{p_i}{p_j} = e^{\frac{\varepsilon_j - \varepsilon_i}{kT}}&amp;lt;/math&amp;gt;&lt;br /&gt;
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The Boltzmann distribution is named after [[Ludwig Boltzmann]] who first formulated it in 1868 during his studies of the [[statistical mechanics]] of gases in thermal equilibrium. Boltzmann's statistical work is borne out in his paper “On the Relationship between the Second Fundamental Theorem of the Mechanical Theory of Heat and Probability Calculations Regarding the Conditions for Thermal Equilibrium&amp;quot;&amp;lt;ref&amp;gt;http://crystal.med.upenn.edu/sharp-lab-pdfs/2015SharpMatschinsky_Boltz1877_Entropy17.pdf&amp;lt;/ref&amp;gt;. The distribution was later investigated extensively, in its modern generic form, by [[Josiah Willard Gibbs]] in 1902.&amp;lt;ref name=&amp;quot;gibbs&amp;quot;&amp;gt;{{cite book |last=Gibbs |first=Josiah Willard |authorlink=Josiah Willard Gibbs |title=Elementary Principles in Statistical Mechanics |year=1902 |publisher=[[Charles Scribner's Sons]] &lt;br /&gt;
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The distribution was later investigated extensively, in its modern generic form, by Josiah Willard Gibbs in 1902.&lt;br /&gt;
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这种分布后来在1902年由约西亚·威拉德·吉布斯进行了广泛的调查，以其现代通用形式。&lt;br /&gt;
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|location=New York|title-link=Elementary Principles in Statistical Mechanics }}&amp;lt;/ref&amp;gt;&lt;br /&gt;
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波兹曼分布是根据路德维希·玻尔兹曼1868年在研究统计力学中气体热平衡的时候首次提出的一个公式命名的。波尔兹曼的统计工作在他1877年的论文《论热力学第二基本定理与热平衡条件的概率计算之间的关系》中得到了体现。&amp;lt;ref&amp;gt;“On the Relationship between the Second Fundamental Theorem of the Mechanical Theory of Heat and Probability Calculations Regarding the Conditions for Thermal Equilibrium” Sitzungberichte der Kaiserlichen Akademie der Wissenschaften. Mathematisch-Naturwissen Classe. Abt. II, LXXVI 1877, pp 373-435 (Wien. Ber. 1877, 76:373-435). &amp;lt;/ref&amp;gt; 在玻尔兹曼分布被发明之后，约西亚·华纳德·吉布森充分地研究了它并在1902年提出了它的一般形式。&amp;lt;ref name=&amp;quot;gibbs&amp;quot; /&amp;gt;&lt;br /&gt;
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The generalized Boltzmann distribution is a sufficient and necessary condition for the equivalence between the statistical mechanics definition of [[entropy]] (The [[Entropy_(statistical_thermodynamics)#Gibbs_entropy_formula | Gibbs entropy formula]] &amp;lt;math&amp;gt;S = -k_{\mathrm{B}}\sum_i p_i \log p_i&amp;lt;/math&amp;gt;) and the thermodynamic definition of entropy (&amp;lt;math&amp;gt;d S = \frac{\delta Q_\text{rev}}{T}&amp;lt;/math&amp;gt;, and the [[fundamental thermodynamic relation]]).&amp;lt;ref name=&amp;quot;:0&amp;quot;&amp;gt;{{cite journal |last1= Gao |first1= Xiang |last2= Gallicchio |first2= Emilio |first3= Adrian |last3= Roitberg  |date= 2019 |title= The generalized Boltzmann distribution is the only distribution in which the Gibbs-Shannon entropy equals the thermodynamic entropy |journal= The Journal of Chemical Physics|volume= 151|issue= 3|pages= 034113|doi= 10.1063/1.5111333|pmid= 31325924 |arxiv= 1903.02121 |s2cid= 118981017 }}&amp;lt;/ref&amp;gt;&lt;br /&gt;
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广义波兹曼分布是熵的统计力学定义(吉布斯熵公式  &amp;lt;math&amp;gt;S = -k_{\mathrm{B}}\sum_i p_i \log p_i&amp;lt;/math&amp;gt;)与熵的热力学定义(&amp;lt;math&amp;gt;d S = \frac{\delta Q_\text{rev}}{T}&amp;lt;/math&amp;gt;)等价的充要条件。&amp;lt;ref name=&amp;quot;:0&amp;quot; /&amp;gt;&lt;br /&gt;
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The Boltzmann distribution should not be confused with the [[Maxwell–Boltzmann distribution]]. The former gives the probability that a system will be in a certain state as a function of that state's energy;&amp;lt;ref name=&amp;quot;Atkins, P. W. 2010&amp;quot;&amp;gt;Atkins, P. W. (2010) Quanta, W. H. Freeman and Company, New York&amp;lt;/ref&amp;gt; in contrast, the latter is used to describe particle speeds in idealized gases.&lt;br /&gt;
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值得一提的是，玻尔兹曼分布不应与麦克斯韦-玻尔兹曼分布混淆。前者给出了系统处于某种状态的概率，作为该状态能量的函数; 后者则是用于描述理想气体中的粒子速度。&lt;br /&gt;
==分布==&lt;br /&gt;
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The Boltzmann distribution is a [[probability distribution]] that gives the probability of a certain state as a function of that state's energy and  temperature of the [[system]] to which the distribution is applied.&amp;lt;ref name=&amp;quot;McQuarrie, A. 2000&amp;quot;&amp;gt;McQuarrie, A. (2000) Statistical Mechanics, University Science Books, California&amp;lt;/ref&amp;gt; It is given as&lt;br /&gt;
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波兹曼分布是一个概率分布，它给出了出于某种量子态处于某种能量和温度的时候的概率。它被这样定义：&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt;&lt;br /&gt;
p_i=\frac{1}{Q}} {e^{- {\varepsilon}_i / k T}=\frac{e^{- {\varepsilon}_i / k T}}{\sum_{j=1}^{M}{e^{- {\varepsilon}_j / k T}}}&lt;br /&gt;
&lt;br /&gt;
&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
where ''p&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;'' is the probability of state ''i'', ''ε&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;'' the energy of state ''i'', ''k'' the Boltzmann constant, ''T'' the temperature of the system and ''M'' is the number of all states accessible to the system of interest.&amp;lt;ref name=&amp;quot;McQuarrie, A. 2000&amp;quot; /&amp;gt;&amp;lt;ref name=&amp;quot;Atkins, P. W. 2010&amp;quot; /&amp;gt; Implied parentheses around the denominator ''kT'' are omitted for brevity. The normalization denominator ''Q'' (denoted by some authors by ''Z'') is the [[canonical partition function]]&lt;br /&gt;
&lt;br /&gt;
其中 ''p&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;'' 是状态 i 的概率，''ε&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;'' 是状态 i 的能量，''k'' 是波兹曼常数，''T'' 是系统的温度，''M'' 是系统所能到达的所有量子态的数目。&amp;lt;ref name=&amp;quot;Atkins, P. W. 2010&amp;quot; /&amp;gt; &amp;lt;ref name=&amp;quot;McQuarrie, A. 2000&amp;quot; /&amp;gt;这里为了简洁美观，省略了''kT''周围的括弧。归一化的分母''Q''（被有些作者写为''Z''）是对于系统中所有量子态进行总和，此部分又被称为[[Index.php?title=Canonical partition function|正则配分函数]]''。''&lt;br /&gt;
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It results from the constraint that the probabilities of all accessible states must add up to 1.&lt;br /&gt;
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所有量子态的概率之和为1.&lt;br /&gt;
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&lt;br /&gt;
The Boltzmann distribution is the distribution that maximizes the [[entropy]]，&lt;br /&gt;
&lt;br /&gt;
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&amp;lt;math&amp;gt;H(p_1,p_2,\cdots,p_M) = -\sum_{i=1}^{M} p_i\log_2 p_i&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
subject to the constraint that &amp;lt;math&amp;gt;\sum {p_i {\varepsilon}_i} &amp;lt;/math&amp;gt; equals a particular mean energy value (which can be proven using [[Lagrange multipliers]]).&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
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当&amp;lt;math&amp;gt;\sum {p_i {\varepsilon}_i} &amp;lt;/math&amp;gt;等于平均能量值时，玻尔兹曼分布是这种情况下能让熵最大化的分布。我们可以通过拉格朗日乘数法来证明。&lt;br /&gt;
&lt;br /&gt;
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The partition function can be calculated if we know the energies of the states accessible to the system of interest. For atoms the partition function values can be found in the NIST Atomic Spectra Database.&amp;lt;ref name=&amp;quot;:1&amp;quot;&amp;gt;[http://physics.nist.gov/PhysRefData/ASD/levels_form.html NIST Atomic Spectra Database Levels Form] at nist.gov&amp;lt;/ref&amp;gt;&lt;br /&gt;
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在知道量子态能量的情况下，这个配分函数可以被计算。对于原子来说，配分函数的值可以在NIST Atomic Spectra Database中找到。&amp;lt;ref name=&amp;quot;:1&amp;quot; /&amp;gt;&lt;br /&gt;
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The distribution shows that states with lower energy will always have a higher probability of being occupied than the states with higher energy. It can also give us the quantitative relationship between the probabilities of the two states being occupied. The ratio of probabilities for states i and j is given as&lt;br /&gt;
&lt;br /&gt;
玻尔兹曼分布指出，能量低的量子态总是有比能量高的量子态更高的概率被粒子占据。它同时也能让我们定量地比较两个量子态分布概率的关系。状态 i 和状态 j 的概率比为&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
{\frac{p_i}{p_j}}=e^{({\varepsilon}_j-{\varepsilon}_i) / k T}&lt;br /&gt;
&lt;br /&gt;
&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
where p&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt; is the probability of state i,  p&amp;lt;sub&amp;gt;j&amp;lt;/sub&amp;gt; the probability of state j, and ε&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt; and ε&amp;lt;sub&amp;gt;j&amp;lt;/sub&amp;gt; are the energies of states i and j, respectively.&lt;br /&gt;
&lt;br /&gt;
其中 p&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt; 是量子态 i 的概率， p&amp;lt;sub&amp;gt;j&amp;lt;/sub&amp;gt; 是量子态 j 的概率，ε&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt; 和 ε&amp;lt;sub&amp;gt;j&amp;lt;/sub&amp;gt; 分别是状态 i 和 j 的能量。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The Boltzmann distribution is often used to describe the distribution of particles, such as atoms or molecules, over energy states accessible to them. If we have a system consisting of many particles, the probability of a particle being in state i is practically the probability that, if we pick a random particle from that system and check what state it is in, we will find it is in state i. This probability is equal to the number of particles in state i divided by the total number of particles in the system, that is the fraction of particles that occupy state i.&lt;br /&gt;
&lt;br /&gt;
玻尔兹曼分布通常被用来描述粒子的分布，比如原子或分子，在能量状态上的分布情况。如果我们有一个由许多粒子组成的系统，某个粒子处于量子态 i 的概率就等同于当我们从该系统中选择一个随机的粒子并观察它处于什么状态，发现它处于状态 i 的概率。这个概率等于量子态 i 的粒子数除以系统中粒子的总数，即那些占据量子态i的粒子的比例。&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
p_i={\frac{N_i}{N}}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
where N&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt; is the number of particles in state i and N is the total number of particles in the system. We may use the Boltzmann distribution to find this probability that is, as we have seen, equal to the fraction of particles that are in state i. So the equation that gives the fraction of particles in state i as a function of the energy of that state is&lt;br /&gt;
&lt;br /&gt;
N&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt; 是位于量子态 i 的粒子数，N是系统中粒子的总数。我们可以用波兹曼分布来求出这个概率，它等于处于量子态i的粒子的比例。所以这个方程给出位于量子态 i 的粒子比例关于这个状态能量的函数&amp;lt;ref name=&amp;quot;Atkins, P. W. 2010&amp;quot; /&amp;gt;。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt;&lt;br /&gt;
{\frac{N_i}{N}}={\frac{e^{- {\varepsilon}_i / k T}}{\sum_{j=1}^{M}{e^{- {\varepsilon}_j / k T}}}} &lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
This equation is of great importance to [[spectroscopy]]. In spectroscopy we observe a [[spectral line]] of atoms or molecules that we are interested in going from one state to another.&amp;lt;ref name=&amp;quot;Atkins, P. W. 2010&amp;quot; /&amp;gt;&amp;lt;ref name=&amp;quot;:2&amp;quot;&amp;gt;Atkins, P. W.; de Paula J. (2009) Physical Chemistry, 9th edition, Oxford University Press, Oxford, UK&amp;lt;/ref&amp;gt; In order for this to be possible, there must be some particles in the first state to undergo the transition. We may find that this condition is fulfilled by finding the fraction of particles in the first state. If it is negligible, the transition is very likely not to be observed at the temperature for which the calculation was done. In general, a larger fraction of molecules in the first state means a higher number of transitions to the second state.&amp;lt;ref name=&amp;quot;:3&amp;quot;&amp;gt;Skoog, D. A.; Holler, F. J.; Crouch, S. R. (2006) Principles of Instrumental Analysis, Brooks/Cole, Boston, MA&amp;lt;/ref&amp;gt; This gives a stronger spectral line. However, there are other factors that influence the intensity of a spectral line, such as whether it is caused by an allowed or a [[forbidden transition]]&lt;br /&gt;
&lt;br /&gt;
这个等式对于光谱学来说很重要。在光谱中，我们期待能观察到一条原子或分子跃迁的谱线。&amp;lt;ref name=&amp;quot;Atkins, P. W. 2010&amp;quot; /&amp;gt;&amp;lt;ref name=&amp;quot;:2&amp;quot; /&amp;gt; 在为了使这成为可能，必须有一些粒子处于第一个量子态，等待着发生跃迁。我们可以通过求第一态粒子的比例来满足这个条件。如果它可以忽略不计，那么在当前计算的温度下，则很难观察到这种跃迁。一般来说，处于第一状态的分子比例越大，意味着向第二状态跃迁的次数越多。&amp;lt;ref name=&amp;quot;:3&amp;quot; /&amp;gt;这就产生了一条更强的谱线。然而，还有其他因素影响谱线的强度，例如它是否是被允许的跃迁还是被禁止的跃迁。&lt;br /&gt;
&lt;br /&gt;
The Boltzmann distribution is related to the [[softmax function]] commonly used in machine learning.&lt;br /&gt;
&lt;br /&gt;
玻尔兹曼分布与机器学习中常用的[[Index.php?title=Softmax function|归一化指数函数]]（Softmax 函数）有关。&lt;br /&gt;
=='''统计力学'''==&lt;br /&gt;
&lt;br /&gt;
{{main|Canonical ensemble|Maxwell–Boltzmann statistics}}The Boltzmann distribution appears in statistical mechanics when considering isolated (or nearly-isolated) systems of fixed composition that are in thermal equilibrium (equilibrium with respect to energy exchange). The most general case is the probability distribution for the canonical ensemble, but also some special cases (derivable from the canonical ensemble) also show the Boltzmann distribution in different aspects:&lt;br /&gt;
&lt;br /&gt;
当独立的(或者几乎独立的)固定体系处于统计力学热平衡状态时，玻尔兹曼分布就会出现。最普遍的情况是概率分布的正则系综，但也有一些特殊的情况(从正则系综衍生)也显示了不同形式的玻尔兹曼分布:&lt;br /&gt;
&lt;br /&gt;
;[[Canonical ensemble]] (general case)&lt;br /&gt;
;'''正则系综(一般情况)'''&lt;br /&gt;
;'''The [[canonical ensemble]] gives the [[probabilities]] of the various possible states of a closed system of fixed volume, in thermal equilibrium with a [[heat bath]]. The canonical ensemble is a probability distribution with the Boltzmann form.'''&lt;br /&gt;
&lt;br /&gt;
正则系综模型给出了在一个封闭固定体积，带有热浴的热平衡系统中的各种可能状态的概率。我们称正则系综为一个玻尔兹曼概率分布。&lt;br /&gt;
&lt;br /&gt;
;&lt;br /&gt;
;Statistical frequencies of subsystems' states (in a non-interacting collection)&lt;br /&gt;
'''子系统状态的统计频率(在一个无交互的集合中)'''&lt;br /&gt;
:When the system of interest is a collection of many non-interacting copies of a smaller subsystem, it is sometimes useful to find the [[statistical frequency]] of a given subsystem state, among the collection. The canonical ensemble has the property of separability when applied to such a collection: as long as the non-interacting subsystems have fixed composition, then each subsystem's state is independent of the others and is also characterized by a canonical ensemble. As a result, the [[expectation value|expected]] statistical frequency distribution of subsystem states has the Boltzmann form.&lt;br /&gt;
&lt;br /&gt;
当系统是一个较小子系统的许多非交互副本的集合时，有时我们需要在某个子系统集合中找到某个子系统的统计频率。当应用于这样一个集合时，这个子系统的正则系综具有可分离性: 只要不相互作用的子系统的组成是固定的，那么每个子系统的状态都是独立于其他子系统的，它们也拥有自己的正则系综。因此，子系统状态的期望统计频率分布形式是玻尔兹曼分布。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[Maxwell–Boltzmann statistics]] of classical gases (systems of non-interacting particles)&lt;br /&gt;
&lt;br /&gt;
'''Maxwell-Boltzmann 统计中的经典气体系统(非相互作用粒子系统)'''&lt;br /&gt;
&lt;br /&gt;
:In particle systems, many particles share the same space and regularly change places with each other; the single-particle state space they occupy is a shared space. [[Maxwell–Boltzmann statistics]] give the expected number of particles found in a given single-particle state, in a [[classical mechanics|classical]] gas of non-interacting particles at equilibrium. This expected number distribution has the Boltzmann form.&lt;br /&gt;
&lt;br /&gt;
在粒子系统中，许多粒子共享同一空间，并且相互之间有规律地改变位置; 它们所占据的单粒子状态空间是一个共享空间。[[Index.php?title=Maxwell–Boltzmann statistics|麦克斯韦-玻尔兹曼统计]]给出了在一个给定的单粒子态，在一个处于平衡状态的非相互作用粒子的经典气体中所发现的粒子的预期数量。这个预期的数量分布具有玻尔兹曼分布形式。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Although these cases have strong similarities, it is helpful to distinguish them as they generalize in different ways when the crucial assumptions are changed:&lt;br /&gt;
&lt;br /&gt;
虽然这些案例有很多相似之处，但是当关键假设发生变化时，我们需要对它们以不同的方式进行归纳总结，因此区分它们是有帮助的:&lt;br /&gt;
*When a system is in thermodynamic equilibrium with respect to both energy exchange ''and particle exchange'', the requirement of fixed composition is relaxed and a [[grand canonical ensemble]] is obtained rather than canonical ensemble. On the other hand, if both composition and energy are fixed, then a [[microcanonical ensemble]] applies instead.&lt;br /&gt;
*当一个系统在能量交换和粒子交换方面都处于热力学平衡时，固定组成的要求就放宽了。这时我们就得到了一个[[Index.php?title=Microcanonical ensemble|巨正则系综]]而不是正则系综。另一方面，如果成分和能量都是固定的，则可以使用[[微正则系综Index.php?title=Microcanonical ensemble|微正则系综]]。&lt;br /&gt;
&lt;br /&gt;
*If the subsystems within a collection ''do'' interact with each other, then the expected frequencies of subsystem states no longer follow a Boltzmann distribution, and even may not have an [[analytical solution]].&amp;lt;ref name=&amp;quot;:4&amp;quot;&amp;gt;A classic example of this is [[magnetic ordering]]. Systems of non-interacting [[spin (physics)|spins]] show [[paramagnetic]] behaviour that can be understood with a single-particle canonical ensemble (resulting in the [[Brillouin function]]). Systems of ''interacting'' spins can show much more complex behaviour such as [[ferromagnetism]] or [[antiferromagnetism]].&amp;lt;/ref&amp;gt; The canonical ensemble can however still be applied to the ''collective'' states of the entire system considered as a whole, provided the entire system is isolated and in thermal equilibrium.&lt;br /&gt;
*如果集合中的子系统确实相互交互，则子系统状态的预期频率不再遵循玻尔兹曼分布，甚至可能没有解析解。&amp;lt;ref name=&amp;quot;:4&amp;quot; /&amp;gt;但是当整个系统是独立的并且处于热平衡状态，则正则系综仍然可以应用于作为一个整体考虑。&lt;br /&gt;
&lt;br /&gt;
*With ''[[quantum mechanics|quantum]]'' gases of non-interacting particles in equilibrium, the number of particles found in a given single-particle state does not follow Maxwell–Boltzmann statistics, and there is no simple closed form expression for quantum gases in the canonical ensemble. In the grand canonical ensemble the state-filling statistics of quantum gases are described by [[Fermi–Dirac statistics]] or [[Bose–Einstein statistics]], depending on whether the particles are [[fermion]]s or [[boson]]s respectively.&lt;br /&gt;
*对于处于平衡状态的非相互作用粒子的量子气体，在给定的单粒子状态中发现的粒子数量并不遵循麦克斯韦-玻尔兹曼统计。并且正则系综中的量子气体没有简单的封闭表达式。在巨正则系综中，量子气体的统计分布状态由费米-狄拉克统计或玻色-爱因斯坦统计来描述，具体则取决于该粒子是费米子还是玻色子。&lt;br /&gt;
&lt;br /&gt;
==数学==&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
In more general mathematical settings, the Boltzmann distribution is also known as the [[Gibbs measure]]. In statistics and machine learning, it is called a [[log-linear model]]. In [[deep learning]], the Boltzmann distribution is used in the sampling distribution of [[stochastic neural network]]s such as the [[Boltzmann machine]], [[Restricted Boltzmann machine]], [[Energy based model|Energy-Based models]] and [[Deep Boltzmann Machine|deep Boltzmann machine]]&lt;br /&gt;
&lt;br /&gt;
在更一般的数学环境中，玻尔兹曼分布也被称为吉布斯量度。在统计学和机器学习中，它被称为对数线性回归。在深度学习中，玻尔兹曼分布被用于随机神经网络的抽样分布，如玻尔兹曼机、受限玻尔兹曼机、基于能量的模型和深度波茨曼机。&lt;br /&gt;
&lt;br /&gt;
==经济==&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The Boltzmann distribution can be introduced to allocate permits in emissions trading.&amp;lt;ref name=&amp;quot;Park, J.-W. 2012&amp;quot;&amp;gt;Park, J.-W., Kim, C. U. and Isard, W. (2012) Permit allocation in emissions trading using the Boltzmann distribution. Physica A 391: 4883–4890&amp;lt;/ref&amp;gt;&amp;lt;ref name=&amp;quot;:5&amp;quot;&amp;gt;[http://www.technologyreview.com/view/425051/the-thorny-problem-of-fair-allocation/ The Thorny Problem Of Fair Allocation]. ''Technology Review'' blog. August 17, 2011. Cites and summarizes Park, Kim and Isard (2012).&amp;lt;/ref&amp;gt; The new allocation method using the Boltzmann distribution can describe the most probable, natural, and unbiased distribution of emissions permits among multiple countries. Simple and versatile, this new method holds potential for many economic and environmental applications.&lt;br /&gt;
&lt;br /&gt;
在经济学中，玻尔兹曼分布被用来分配排放交易中的许可。&amp;lt;ref name=&amp;quot;Park, J.-W. 2012&amp;quot; /&amp;gt;&amp;lt;ref name=&amp;quot;:5&amp;quot; /&amp;gt;  使用玻尔兹曼分布的新分配方法可以创造出在多个国家之间最可能的、自然的和无偏见的排放许可分配。这种新方法简单而通用，在经济和环保中有很大的应用潜力。&lt;br /&gt;
&lt;br /&gt;
The Boltzmann distribution has the same form as the [[Multinomial logistic regression|multinomial logit]] model. As a [[discrete choice]] model, this is very well known in economics since [[Daniel McFadden]] made the connection to random utility maximization.&lt;br /&gt;
&lt;br /&gt;
玻尔兹曼分布与多项逻辑回归模型具有相同的形式。在丹尼尔 · 麦克法登将它与随机效用最大化联系起来之后，成为了大家所熟知的一种离散选择模型。&lt;br /&gt;
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Category:Statistical mechanics&lt;br /&gt;
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类别: 统计力学&lt;br /&gt;
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本中文词条由[[用户:费米子|tueryeye]]编辑，欢迎在讨论页面留言。&lt;br /&gt;
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==See also==&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:Boltzmann distribution]]. Its edit history can be viewed at [[玻尔兹曼分布/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;br /&gt;
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&amp;lt;references /&amp;gt;&lt;/div&gt;</summary>
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&lt;div&gt;此词条暂由tueryeye翻译和审校，翻译字数共1452，带来阅读不便，请见谅。&lt;br /&gt;
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{{Use American English|date = March 2019}}&lt;br /&gt;
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{{Short description|Probability distribution of energy states of a system}}&lt;br /&gt;
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{{about|system energy states|particle energy levels and velocities|Maxwell–Boltzmann distribution}}&lt;br /&gt;
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[[File:Boltzmann distribution graph.svg|upright=1.75|right|thumb|Boltzmann factor ''p&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;''&amp;amp;nbsp;/&amp;amp;nbsp;''p&amp;lt;sub&amp;gt;j&amp;lt;/sub&amp;gt;'' (vertical axis) as a function of temperature ''T'' for several energy differences ''ε&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;''&amp;amp;nbsp;−&amp;amp;nbsp;''ε&amp;lt;sub&amp;gt;j&amp;lt;/sub&amp;gt;''.|链接=Special:FilePath/Boltzmann_distribution_graph.svg]]&lt;br /&gt;
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In [[statistical mechanics]] and [[mathematics]], a '''Boltzmann distribution''' (also called '''Gibbs distribution'''&amp;lt;ref name=&amp;quot;landau&amp;quot;&amp;gt;{{cite book | author=Landau, Lev Davidovich |author2=Lifshitz, Evgeny Mikhailovich |name-list-style=amp | title=Statistical Physics |volume=5 |series=Course of Theoretical Physics |edition=3 |origyear=1976 |year=1980 |place=Oxford |publisher=Pergamon Press|isbn=0-7506-3372-7|author-link=Lev Landau |author2-link=Evgeny Lifshitz }} Translated by J.B. Sykes and M.J. Kearsley. See section 28&amp;lt;/ref&amp;gt;) is a [[probability distribution]] or [[probability measure]] that gives the probability that a system will be in a certain [[microstate (statistical mechanics)|state]] as a function of that state's energy and the temperature of the system. The distribution is expressed in the form:&lt;br /&gt;
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在统计力学和数学中，波兹曼分布分布(也称为吉布斯分布&amp;lt;ref name=&amp;quot;landau&amp;quot; /&amp;gt;)是一个概率分布或机率量测，它给出了一个系统处于某种量子态的概率，这个概率是该状态的能量和系统温度的函数。分布情况以下列形式表示:&lt;br /&gt;
:&amp;lt;math&amp;gt;p_i \propto e^{-\frac{\varepsilon_i}{kT}}&amp;lt;/math&amp;gt; &lt;br /&gt;
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where {{mvar|p&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;}} is the probability of the system being in state {{mvar|i}}, {{mvar|ε&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;}} is the energy of that state, and a constant {{mvar|kT}} of the distribution is the product of [[Boltzmann's constant]] {{mvar|k}} and [[thermodynamic temperature]] {{mvar|T}}. The symbol &amp;lt;math display=&amp;quot;inline&amp;quot;&amp;gt;\propto&amp;lt;/math&amp;gt; denotes [[proportionality (mathematics)|proportionality]] (see {{section link||The distribution}} for the proportionality constant).&lt;br /&gt;
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{{mvar|p&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;}} 是其中系统处于状态{{mvar|i}}的概率, {{mvar|ε&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;}} 是该状态的能量，还有关于这个分布的一个常数 {{mvar|kT}} ，它是玻尔兹曼常数{{mvar|k}}和热力学温度 {{mvar|T}} 的乘积。符号 &amp;lt;math display=&amp;quot;inline&amp;quot;&amp;gt;\propto&amp;lt;/math&amp;gt;表示正比例(见附录中的比例常数)。&lt;br /&gt;
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The term system here has a very wide meaning; it can range from a single atom to a macroscopic system such as a [[Natural gas storage|natural gas storage tank]]. Because of this the Boltzmann distribution can be used to solve a very wide variety of problems. The distribution shows that states with lower energy will always have a higher probability of being occupied .&lt;br /&gt;
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这里的术语系统含义广泛; 它可以从单个原子到宏观系统，如天然气储罐。正因为如此，波兹曼分布可以用来解决各种各样的问题。玻尔兹曼分布表明，能量较低的状态被占据的概率总是较高的。&lt;br /&gt;
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The ''ratio'' of probabilities of two states is known as the '''Boltzmann factor''' and characteristically only depends on the states' energy difference:&lt;br /&gt;
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两种状态的概率之比被称为玻尔兹曼因子，取决于两种状态的能量差:&lt;br /&gt;
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&amp;lt;math&amp;gt;\frac{p_i}{p_j} = e^{\frac{\varepsilon_j - \varepsilon_i}{kT}}&amp;lt;/math&amp;gt;&lt;br /&gt;
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The Boltzmann distribution is named after [[Ludwig Boltzmann]] who first formulated it in 1868 during his studies of the [[statistical mechanics]] of gases in thermal equilibrium. Boltzmann's statistical work is borne out in his paper “On the Relationship between the Second Fundamental Theorem of the Mechanical Theory of Heat and Probability Calculations Regarding the Conditions for Thermal Equilibrium&amp;quot;&amp;lt;ref&amp;gt;http://crystal.med.upenn.edu/sharp-lab-pdfs/2015SharpMatschinsky_Boltz1877_Entropy17.pdf&amp;lt;/ref&amp;gt;. The distribution was later investigated extensively, in its modern generic form, by [[Josiah Willard Gibbs]] in 1902.&amp;lt;ref name=&amp;quot;gibbs&amp;quot;&amp;gt;{{cite book |last=Gibbs |first=Josiah Willard |authorlink=Josiah Willard Gibbs |title=Elementary Principles in Statistical Mechanics |year=1902 |publisher=[[Charles Scribner's Sons]] &lt;br /&gt;
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The distribution was later investigated extensively, in its modern generic form, by Josiah Willard Gibbs in 1902.&lt;br /&gt;
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这种分布后来在1902年由约西亚·威拉德·吉布斯进行了广泛的调查，以其现代通用形式。&lt;br /&gt;
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|location=New York|title-link=Elementary Principles in Statistical Mechanics }}&amp;lt;/ref&amp;gt;&lt;br /&gt;
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波兹曼分布是根据路德维希·玻尔兹曼1868年在研究统计力学中气体热平衡的时候首次提出的一个公式命名的。波尔兹曼的统计工作在他1877年的论文《论热力学第二基本定理与热平衡条件的概率计算之间的关系》中得到了体现。&amp;lt;ref&amp;gt;“On the Relationship between the Second Fundamental Theorem of the Mechanical Theory of Heat and Probability Calculations Regarding the Conditions for Thermal Equilibrium” Sitzungberichte der Kaiserlichen Akademie der Wissenschaften. Mathematisch-Naturwissen Classe. Abt. II, LXXVI 1877, pp 373-435 (Wien. Ber. 1877, 76:373-435). &amp;lt;/ref&amp;gt; 在玻尔兹曼分布被发明之后，约西亚·华纳德·吉布森充分地研究了它并在1902年提出了它的一般形式。&amp;lt;ref name=&amp;quot;gibbs&amp;quot; /&amp;gt;&lt;br /&gt;
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The generalized Boltzmann distribution is a sufficient and necessary condition for the equivalence between the statistical mechanics definition of [[entropy]] (The [[Entropy_(statistical_thermodynamics)#Gibbs_entropy_formula | Gibbs entropy formula]] &amp;lt;math&amp;gt;S = -k_{\mathrm{B}}\sum_i p_i \log p_i&amp;lt;/math&amp;gt;) and the thermodynamic definition of entropy (&amp;lt;math&amp;gt;d S = \frac{\delta Q_\text{rev}}{T}&amp;lt;/math&amp;gt;, and the [[fundamental thermodynamic relation]]).&amp;lt;ref name=&amp;quot;:0&amp;quot;&amp;gt;{{cite journal |last1= Gao |first1= Xiang |last2= Gallicchio |first2= Emilio |first3= Adrian |last3= Roitberg  |date= 2019 |title= The generalized Boltzmann distribution is the only distribution in which the Gibbs-Shannon entropy equals the thermodynamic entropy |journal= The Journal of Chemical Physics|volume= 151|issue= 3|pages= 034113|doi= 10.1063/1.5111333|pmid= 31325924 |arxiv= 1903.02121 |s2cid= 118981017 }}&amp;lt;/ref&amp;gt;&lt;br /&gt;
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广义波兹曼分布是熵的统计力学定义(吉布斯熵公式  &amp;lt;math&amp;gt;S = -k_{\mathrm{B}}\sum_i p_i \log p_i&amp;lt;/math&amp;gt;)与熵的热力学定义(&amp;lt;math&amp;gt;d S = \frac{\delta Q_\text{rev}}{T}&amp;lt;/math&amp;gt;)等价的充要条件。&amp;lt;ref name=&amp;quot;:0&amp;quot; /&amp;gt;&lt;br /&gt;
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The Boltzmann distribution should not be confused with the [[Maxwell–Boltzmann distribution]]. The former gives the probability that a system will be in a certain state as a function of that state's energy;&amp;lt;ref name=&amp;quot;Atkins, P. W. 2010&amp;quot;&amp;gt;Atkins, P. W. (2010) Quanta, W. H. Freeman and Company, New York&amp;lt;/ref&amp;gt; in contrast, the latter is used to describe particle speeds in idealized gases.&lt;br /&gt;
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值得一提的是，玻尔兹曼分布不应与麦克斯韦-玻尔兹曼分布混淆。前者给出了系统处于某种状态的概率，作为该状态能量的函数; 后者则是用于描述理想气体中的粒子速度。&lt;br /&gt;
==分布==&lt;br /&gt;
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The Boltzmann distribution is a [[probability distribution]] that gives the probability of a certain state as a function of that state's energy and  temperature of the [[system]] to which the distribution is applied.&amp;lt;ref name=&amp;quot;McQuarrie, A. 2000&amp;quot;&amp;gt;McQuarrie, A. (2000) Statistical Mechanics, University Science Books, California&amp;lt;/ref&amp;gt; It is given as&lt;br /&gt;
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波兹曼分布是一个概率分布，它给出了出于某种量子态处于某种能量和温度的时候的概率。它被这样定义：&lt;br /&gt;
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p_i=\frac{1}{Q}} {e^{- {\varepsilon}_i / k T}=\frac{e^{- {\varepsilon}_i / k T}}{\sum_{j=1}^{M}{e^{- {\varepsilon}_j / k T}}}&lt;br /&gt;
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&amp;lt;/math&amp;gt;&lt;br /&gt;
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where ''p&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;'' is the probability of state ''i'', ''ε&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;'' the energy of state ''i'', ''k'' the Boltzmann constant, ''T'' the temperature of the system and ''M'' is the number of all states accessible to the system of interest.&amp;lt;ref name=&amp;quot;McQuarrie, A. 2000&amp;quot; /&amp;gt;&amp;lt;ref name=&amp;quot;Atkins, P. W. 2010&amp;quot; /&amp;gt; Implied parentheses around the denominator ''kT'' are omitted for brevity. The normalization denominator ''Q'' (denoted by some authors by ''Z'') is the [[canonical partition function]]&lt;br /&gt;
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其中 ''p&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;'' 是状态 i 的概率，''ε&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;'' 是状态 i 的能量，''k'' 是波兹曼常数，''T'' 是系统的温度，''M'' 是系统所能到达的所有量子态的数目。&amp;lt;ref name=&amp;quot;Atkins, P. W. 2010&amp;quot; /&amp;gt; &amp;lt;ref name=&amp;quot;McQuarrie, A. 2000&amp;quot; /&amp;gt;这里为了简洁美观，省略了''kT''周围的括弧。归一化的分母''Q''（被有些作者写为''Z''）是对于系统中所有量子态进行总和，此部分又被称为[[Index.php?title=Canonical partition function|正则配分函数]]''。''&lt;br /&gt;
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It results from the constraint that the probabilities of all accessible states must add up to 1.&lt;br /&gt;
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所有量子态的概率之和为1.&lt;br /&gt;
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The Boltzmann distribution is the distribution that maximizes the [[entropy]]，&lt;br /&gt;
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&amp;lt;math&amp;gt;H(p_1,p_2,\cdots,p_M) = -\sum_{i=1}^{M} p_i\log_2 p_i&amp;lt;/math&amp;gt;&lt;br /&gt;
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subject to the constraint that &amp;lt;math&amp;gt;\sum {p_i {\varepsilon}_i} &amp;lt;/math&amp;gt; equals a particular mean energy value (which can be proven using [[Lagrange multipliers]]).&lt;br /&gt;
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当&amp;lt;math&amp;gt;\sum {p_i {\varepsilon}_i} &amp;lt;/math&amp;gt;等于平均能量值时，玻尔兹曼分布是这种情况下能让熵最大化的分布。我们可以通过拉格朗日乘数法来证明。&lt;br /&gt;
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The partition function can be calculated if we know the energies of the states accessible to the system of interest. For atoms the partition function values can be found in the NIST Atomic Spectra Database.&amp;lt;ref name=&amp;quot;:1&amp;quot;&amp;gt;[http://physics.nist.gov/PhysRefData/ASD/levels_form.html NIST Atomic Spectra Database Levels Form] at nist.gov&amp;lt;/ref&amp;gt;&lt;br /&gt;
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在知道量子态能量的情况下，这个配分函数可以被计算。对于原子来说，配分函数的值可以在NIST Atomic Spectra Database中找到。&amp;lt;ref name=&amp;quot;:1&amp;quot; /&amp;gt;&lt;br /&gt;
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The distribution shows that states with lower energy will always have a higher probability of being occupied than the states with higher energy. It can also give us the quantitative relationship between the probabilities of the two states being occupied. The ratio of probabilities for states i and j is given as&lt;br /&gt;
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玻尔兹曼分布指出，能量低的量子态总是有比能量高的量子态更高的概率被粒子占据。它同时也能让我们定量地比较两个量子态分布概率的关系。状态 i 和状态 j 的概率比为&lt;br /&gt;
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:&amp;lt;math&amp;gt;&lt;br /&gt;
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{\frac{p_i}{p_j}}=e^{({\varepsilon}_j-{\varepsilon}_i) / k T}&lt;br /&gt;
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where p&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt; is the probability of state i,  p&amp;lt;sub&amp;gt;j&amp;lt;/sub&amp;gt; the probability of state j, and ε&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt; and ε&amp;lt;sub&amp;gt;j&amp;lt;/sub&amp;gt; are the energies of states i and j, respectively.&lt;br /&gt;
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其中 p&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt; 是量子态 i 的概率， p&amp;lt;sub&amp;gt;j&amp;lt;/sub&amp;gt; 是量子态 j 的概率，ε&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt; 和 ε&amp;lt;sub&amp;gt;j&amp;lt;/sub&amp;gt; 分别是状态 i 和 j 的能量。&lt;br /&gt;
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The Boltzmann distribution is often used to describe the distribution of particles, such as atoms or molecules, over energy states accessible to them. If we have a system consisting of many particles, the probability of a particle being in state i is practically the probability that, if we pick a random particle from that system and check what state it is in, we will find it is in state i. This probability is equal to the number of particles in state i divided by the total number of particles in the system, that is the fraction of particles that occupy state i.&lt;br /&gt;
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玻尔兹曼分布通常被用来描述粒子的分布，比如原子或分子，在能量状态上的分布情况。如果我们有一个由许多粒子组成的系统，某个粒子处于量子态 i 的概率就等同于当我们从该系统中选择一个随机的粒子并观察它处于什么状态，发现它处于状态 i 的概率。这个概率等于量子态 i 的粒子数除以系统中粒子的总数，即那些占据量子态i的粒子的比例。&lt;br /&gt;
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p_i={\frac{N_i}{N}}&lt;br /&gt;
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where N&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt; is the number of particles in state i and N is the total number of particles in the system. We may use the Boltzmann distribution to find this probability that is, as we have seen, equal to the fraction of particles that are in state i. So the equation that gives the fraction of particles in state i as a function of the energy of that state is&lt;br /&gt;
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N&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt; 是位于量子态 i 的粒子数，N是系统中粒子的总数。我们可以用波兹曼分布来求出这个概率，它等于处于量子态i的粒子的比例。所以这个方程给出位于量子态 i 的粒子比例关于这个状态能量的函数&amp;lt;ref name=&amp;quot;Atkins, P. W. 2010&amp;quot; /&amp;gt;。&lt;br /&gt;
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{\frac{N_i}{N}}={\frac{e^{- {\varepsilon}_i / k T}}{\sum_{j=1}^{M}{e^{- {\varepsilon}_j / k T}}}} &lt;br /&gt;
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This equation is of great importance to [[spectroscopy]]. In spectroscopy we observe a [[spectral line]] of atoms or molecules that we are interested in going from one state to another.&amp;lt;ref name=&amp;quot;Atkins, P. W. 2010&amp;quot; /&amp;gt;&amp;lt;ref name=&amp;quot;:2&amp;quot;&amp;gt;Atkins, P. W.; de Paula J. (2009) Physical Chemistry, 9th edition, Oxford University Press, Oxford, UK&amp;lt;/ref&amp;gt; In order for this to be possible, there must be some particles in the first state to undergo the transition. We may find that this condition is fulfilled by finding the fraction of particles in the first state. If it is negligible, the transition is very likely not to be observed at the temperature for which the calculation was done. In general, a larger fraction of molecules in the first state means a higher number of transitions to the second state.&amp;lt;ref name=&amp;quot;:3&amp;quot;&amp;gt;Skoog, D. A.; Holler, F. J.; Crouch, S. R. (2006) Principles of Instrumental Analysis, Brooks/Cole, Boston, MA&amp;lt;/ref&amp;gt; This gives a stronger spectral line. However, there are other factors that influence the intensity of a spectral line, such as whether it is caused by an allowed or a [[forbidden transition]]&lt;br /&gt;
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这个等式对于光谱学来说很重要。在光谱中，我们期待能观察到一条原子或分子跃迁的谱线。&amp;lt;ref name=&amp;quot;Atkins, P. W. 2010&amp;quot; /&amp;gt;&amp;lt;ref name=&amp;quot;:2&amp;quot; /&amp;gt; 在为了使这成为可能，必须有一些粒子处于第一个量子态，等待着发生跃迁。我们可以通过求第一态粒子的比例来满足这个条件。如果它可以忽略不计，那么在当前计算的温度下，则很难观察到这种跃迁。一般来说，处于第一状态的分子比例越大，意味着向第二状态跃迁的次数越多。&amp;lt;ref name=&amp;quot;:3&amp;quot; /&amp;gt;这就产生了一条更强的谱线。然而，还有其他因素影响谱线的强度，例如它是否是被允许的跃迁还是被禁止的跃迁。&lt;br /&gt;
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The Boltzmann distribution is related to the [[softmax function]] commonly used in machine learning.&lt;br /&gt;
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玻尔兹曼分布与机器学习中常用的[[Index.php?title=Softmax function|归一化指数函数]]（Softmax 函数）有关。&lt;br /&gt;
=='''统计力学'''==&lt;br /&gt;
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{{main|Canonical ensemble|Maxwell–Boltzmann statistics}}The Boltzmann distribution appears in statistical mechanics when considering isolated (or nearly-isolated) systems of fixed composition that are in thermal equilibrium (equilibrium with respect to energy exchange). The most general case is the probability distribution for the canonical ensemble, but also some special cases (derivable from the canonical ensemble) also show the Boltzmann distribution in different aspects:&lt;br /&gt;
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当独立的(或者几乎独立的)固定体系处于统计力学热平衡状态时，玻尔兹曼分布就会出现。最普遍的情况是概率分布的正则系综，但也有一些特殊的情况(从正则系综衍生)也显示了不同形式的玻尔兹曼分布:&lt;br /&gt;
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;[[Canonical ensemble]] (general case)&lt;br /&gt;
;'''正则系综(一般情况)'''&lt;br /&gt;
;'''The [[canonical ensemble]] gives the [[probabilities]] of the various possible states of a closed system of fixed volume, in thermal equilibrium with a [[heat bath]]. The canonical ensemble is a probability distribution with the Boltzmann form.'''&lt;br /&gt;
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正则系综模型给出了在一个封闭固定体积，带有热浴的热平衡系统中的各种可能状态的概率。我们称正则系综为一个玻尔兹曼概率分布。&lt;br /&gt;
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;Statistical frequencies of subsystems' states (in a non-interacting collection)&lt;br /&gt;
'''子系统状态的统计频率(在一个无交互的集合中)'''&lt;br /&gt;
:When the system of interest is a collection of many non-interacting copies of a smaller subsystem, it is sometimes useful to find the [[statistical frequency]] of a given subsystem state, among the collection. The canonical ensemble has the property of separability when applied to such a collection: as long as the non-interacting subsystems have fixed composition, then each subsystem's state is independent of the others and is also characterized by a canonical ensemble. As a result, the [[expectation value|expected]] statistical frequency distribution of subsystem states has the Boltzmann form.&lt;br /&gt;
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当系统是一个较小子系统的许多非交互副本的集合时，有时我们需要在某个子系统集合中找到某个子系统的统计频率。当应用于这样一个集合时，这个子系统的正则系综具有可分离性: 只要不相互作用的子系统的组成是固定的，那么每个子系统的状态都是独立于其他子系统的，它们也拥有自己的正则系综。因此，子系统状态的期望统计频率分布形式是玻尔兹曼分布。&lt;br /&gt;
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[[Maxwell–Boltzmann statistics]] of classical gases (systems of non-interacting particles)&lt;br /&gt;
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'''Maxwell-Boltzmann 统计中的经典气体系统(非相互作用粒子系统)'''&lt;br /&gt;
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:In particle systems, many particles share the same space and regularly change places with each other; the single-particle state space they occupy is a shared space. [[Maxwell–Boltzmann statistics]] give the expected number of particles found in a given single-particle state, in a [[classical mechanics|classical]] gas of non-interacting particles at equilibrium. This expected number distribution has the Boltzmann form.&lt;br /&gt;
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在粒子系统中，许多粒子共享同一空间，并且相互之间有规律地改变位置; 它们所占据的单粒子状态空间是一个共享空间。[[Index.php?title=Maxwell–Boltzmann statistics|麦克斯韦-玻尔兹曼统计]]给出了在一个给定的单粒子态，在一个处于平衡状态的非相互作用粒子的经典气体中所发现的粒子的预期数量。这个预期的数量分布具有玻尔兹曼分布形式。&lt;br /&gt;
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Although these cases have strong similarities, it is helpful to distinguish them as they generalize in different ways when the crucial assumptions are changed:&lt;br /&gt;
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虽然这些案例有很多相似之处，但是当关键假设发生变化时，我们需要对它们以不同的方式进行归纳总结，因此区分它们是有帮助的:&lt;br /&gt;
*When a system is in thermodynamic equilibrium with respect to both energy exchange ''and particle exchange'', the requirement of fixed composition is relaxed and a [[grand canonical ensemble]] is obtained rather than canonical ensemble. On the other hand, if both composition and energy are fixed, then a [[microcanonical ensemble]] applies instead.&lt;br /&gt;
*当一个系统在能量交换和粒子交换方面都处于热力学平衡时，固定组成的要求就放宽了。这时我们就得到了一个[[Index.php?title=Microcanonical ensemble|巨正则系综]]而不是正则系综。另一方面，如果成分和能量都是固定的，则可以使用[[微正则系综Index.php?title=Microcanonical ensemble|微正则系综]]。&lt;br /&gt;
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*If the subsystems within a collection ''do'' interact with each other, then the expected frequencies of subsystem states no longer follow a Boltzmann distribution, and even may not have an [[analytical solution]].&amp;lt;ref name=&amp;quot;:4&amp;quot;&amp;gt;A classic example of this is [[magnetic ordering]]. Systems of non-interacting [[spin (physics)|spins]] show [[paramagnetic]] behaviour that can be understood with a single-particle canonical ensemble (resulting in the [[Brillouin function]]). Systems of ''interacting'' spins can show much more complex behaviour such as [[ferromagnetism]] or [[antiferromagnetism]].&amp;lt;/ref&amp;gt; The canonical ensemble can however still be applied to the ''collective'' states of the entire system considered as a whole, provided the entire system is isolated and in thermal equilibrium.&lt;br /&gt;
*如果集合中的子系统确实相互交互，则子系统状态的预期频率不再遵循玻尔兹曼 分布，甚至可能没有解析解。&amp;lt;ref name=&amp;quot;:4&amp;quot; /&amp;gt;然而，如果整个系统是独立的并且处于热平衡状态，则正则系综仍然可以应用于作为一个整体考虑。&lt;br /&gt;
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*With ''[[quantum mechanics|quantum]]'' gases of non-interacting particles in equilibrium, the number of particles found in a given single-particle state does not follow Maxwell–Boltzmann statistics, and there is no simple closed form expression for quantum gases in the canonical ensemble. In the grand canonical ensemble the state-filling statistics of quantum gases are described by [[Fermi–Dirac statistics]] or [[Bose–Einstein statistics]], depending on whether the particles are [[fermion]]s or [[boson]]s respectively.&lt;br /&gt;
*对于处于平衡状态的非相互作用粒子的量子气体，在给定的单粒子状态中发现的粒子数量并不遵循麦克斯韦-玻尔兹曼统计。并且正则系综中的量子气体没有简单的封闭表达式。在巨正则系综中，量子气体的统计分布状态由费米-狄拉克统计或玻色-爱因斯坦统计来描述，具体则取决于该粒子是费米子还是玻色子。&lt;br /&gt;
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==数学==&lt;br /&gt;
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In more general mathematical settings, the Boltzmann distribution is also known as the [[Gibbs measure]]. In statistics and machine learning, it is called a [[log-linear model]]. In [[deep learning]], the Boltzmann distribution is used in the sampling distribution of [[stochastic neural network]]s such as the [[Boltzmann machine]], [[Restricted Boltzmann machine]], [[Energy based model|Energy-Based models]] and [[Deep Boltzmann Machine|deep Boltzmann machine]]&lt;br /&gt;
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在更一般的数学环境中，玻尔兹曼分布也被称为吉布斯量度。在统计学和机器学习中，它被称为对数线性回归。在深度学习中，玻尔兹曼分布被用于随机神经网络的抽样分布，如玻尔兹曼机、受限玻尔兹曼机、基于能量的模型和深度波茨曼机。&lt;br /&gt;
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==经济==&lt;br /&gt;
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The Boltzmann distribution can be introduced to allocate permits in emissions trading.&amp;lt;ref name=&amp;quot;Park, J.-W. 2012&amp;quot;&amp;gt;Park, J.-W., Kim, C. U. and Isard, W. (2012) Permit allocation in emissions trading using the Boltzmann distribution. Physica A 391: 4883–4890&amp;lt;/ref&amp;gt;&amp;lt;ref name=&amp;quot;:5&amp;quot;&amp;gt;[http://www.technologyreview.com/view/425051/the-thorny-problem-of-fair-allocation/ The Thorny Problem Of Fair Allocation]. ''Technology Review'' blog. August 17, 2011. Cites and summarizes Park, Kim and Isard (2012).&amp;lt;/ref&amp;gt; The new allocation method using the Boltzmann distribution can describe the most probable, natural, and unbiased distribution of emissions permits among multiple countries. Simple and versatile, this new method holds potential for many economic and environmental applications.&lt;br /&gt;
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在经济学中，玻尔兹曼分布被用来分配排放交易中的许可。&amp;lt;ref name=&amp;quot;Park, J.-W. 2012&amp;quot; /&amp;gt;&amp;lt;ref name=&amp;quot;:5&amp;quot; /&amp;gt;  使用玻尔兹曼分布的新分配方法可以创造出在多个国家之间最可能的、自然的和无偏见的排放许可分配。这种新方法简单而通用，在经济和环保中有很大的应用潜力。&lt;br /&gt;
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The Boltzmann distribution has the same form as the [[Multinomial logistic regression|multinomial logit]] model. As a [[discrete choice]] model, this is very well known in economics since [[Daniel McFadden]] made the connection to random utility maximization.&lt;br /&gt;
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玻尔兹曼分布与多项逻辑回归模型具有相同的形式。在丹尼尔 · 麦克法登将它与随机效用最大化联系起来之后，成为了大家所熟知的一种离散选择模型。&lt;br /&gt;
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Category:Statistical mechanics&lt;br /&gt;
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类别: 统计力学&lt;br /&gt;
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本中文词条由[[用户:费米子|tueryeye]]编辑，欢迎在讨论页面留言。&lt;br /&gt;
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==See also==&lt;br /&gt;
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Distribution&lt;br /&gt;
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分布&lt;br /&gt;
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&amp;lt;small&amp;gt;This page was moved from [[wikipedia:en:Boltzmann distribution]]. Its edit history can be viewed at [[玻尔兹曼分布/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;br /&gt;
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&lt;div&gt;此词条暂由tueryeye翻译和审校，翻译字数共1452，带来阅读不便，请见谅。&lt;br /&gt;
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{{Use American English|date = March 2019}}&lt;br /&gt;
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{{Short description|Probability distribution of energy states of a system}}&lt;br /&gt;
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{{about|system energy states|particle energy levels and velocities|Maxwell–Boltzmann distribution}}&lt;br /&gt;
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[[File:Boltzmann distribution graph.svg|upright=1.75|right|thumb|Boltzmann factor ''p&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;''&amp;amp;nbsp;/&amp;amp;nbsp;''p&amp;lt;sub&amp;gt;j&amp;lt;/sub&amp;gt;'' (vertical axis) as a function of temperature ''T'' for several energy differences ''ε&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;''&amp;amp;nbsp;−&amp;amp;nbsp;''ε&amp;lt;sub&amp;gt;j&amp;lt;/sub&amp;gt;''.|链接=Special:FilePath/Boltzmann_distribution_graph.svg]]&lt;br /&gt;
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In [[statistical mechanics]] and [[mathematics]], a '''Boltzmann distribution''' (also called '''Gibbs distribution'''&amp;lt;ref name=&amp;quot;landau&amp;quot;&amp;gt;{{cite book | author=Landau, Lev Davidovich |author2=Lifshitz, Evgeny Mikhailovich |name-list-style=amp | title=Statistical Physics |volume=5 |series=Course of Theoretical Physics |edition=3 |origyear=1976 |year=1980 |place=Oxford |publisher=Pergamon Press|isbn=0-7506-3372-7|author-link=Lev Landau |author2-link=Evgeny Lifshitz }} Translated by J.B. Sykes and M.J. Kearsley. See section 28&amp;lt;/ref&amp;gt;) is a [[probability distribution]] or [[probability measure]] that gives the probability that a system will be in a certain [[microstate (statistical mechanics)|state]] as a function of that state's energy and the temperature of the system. The distribution is expressed in the form:&lt;br /&gt;
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在统计力学和数学中，波兹曼分布分布(也称为吉布斯分布&amp;lt;ref name=&amp;quot;landau&amp;quot; /&amp;gt;)是一个概率分布或机率量测，它给出了一个系统处于某种量子态的概率，这个概率是该状态的能量和系统温度的函数。分布情况以下列形式表示:&lt;br /&gt;
:&amp;lt;math&amp;gt;p_i \propto e^{-\frac{\varepsilon_i}{kT}}&amp;lt;/math&amp;gt; &lt;br /&gt;
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where {{mvar|p&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;}} is the probability of the system being in state {{mvar|i}}, {{mvar|ε&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;}} is the energy of that state, and a constant {{mvar|kT}} of the distribution is the product of [[Boltzmann's constant]] {{mvar|k}} and [[thermodynamic temperature]] {{mvar|T}}. The symbol &amp;lt;math display=&amp;quot;inline&amp;quot;&amp;gt;\propto&amp;lt;/math&amp;gt; denotes [[proportionality (mathematics)|proportionality]] (see {{section link||The distribution}} for the proportionality constant).&lt;br /&gt;
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{{mvar|p&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;}} 是其中系统处于状态{{mvar|i}}的概率, {{mvar|ε&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;}} 是该状态的能量，还有关于这个分布的一个常数 {{mvar|kT}} ，它是玻尔兹曼常数{{mvar|k}}和热力学温度 {{mvar|T}} 的乘积。符号 &amp;lt;math display=&amp;quot;inline&amp;quot;&amp;gt;\propto&amp;lt;/math&amp;gt;表示正比例(见附录中的比例常数)。&lt;br /&gt;
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The term system here has a very wide meaning; it can range from a single atom to a macroscopic system such as a [[Natural gas storage|natural gas storage tank]]. Because of this the Boltzmann distribution can be used to solve a very wide variety of problems. The distribution shows that states with lower energy will always have a higher probability of being occupied .&lt;br /&gt;
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这里的术语系统含义广泛; 它可以从单个原子到宏观系统，如天然气储罐。正因为如此，波兹曼分布可以用来解决各种各样的问题。玻尔兹曼分布表明，能量较低的状态被占据的概率总是较高的。&lt;br /&gt;
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The ''ratio'' of probabilities of two states is known as the '''Boltzmann factor''' and characteristically only depends on the states' energy difference:&lt;br /&gt;
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两种状态的概率之比被称为玻尔兹曼因子，取决于两种状态的能量差:&lt;br /&gt;
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&amp;lt;math&amp;gt;\frac{p_i}{p_j} = e^{\frac{\varepsilon_j - \varepsilon_i}{kT}}&amp;lt;/math&amp;gt;&lt;br /&gt;
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The Boltzmann distribution is named after [[Ludwig Boltzmann]] who first formulated it in 1868 during his studies of the [[statistical mechanics]] of gases in thermal equilibrium. Boltzmann's statistical work is borne out in his paper “On the Relationship between the Second Fundamental Theorem of the Mechanical Theory of Heat and Probability Calculations Regarding the Conditions for Thermal Equilibrium&amp;quot;&amp;lt;ref&amp;gt;http://crystal.med.upenn.edu/sharp-lab-pdfs/2015SharpMatschinsky_Boltz1877_Entropy17.pdf&amp;lt;/ref&amp;gt;. The distribution was later investigated extensively, in its modern generic form, by [[Josiah Willard Gibbs]] in 1902.&amp;lt;ref name=&amp;quot;gibbs&amp;quot;&amp;gt;{{cite book |last=Gibbs |first=Josiah Willard |authorlink=Josiah Willard Gibbs |title=Elementary Principles in Statistical Mechanics |year=1902 |publisher=[[Charles Scribner's Sons]] &lt;br /&gt;
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The distribution was later investigated extensively, in its modern generic form, by Josiah Willard Gibbs in 1902.&lt;br /&gt;
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这种分布后来在1902年由约西亚·威拉德·吉布斯进行了广泛的调查，以其现代通用形式。&lt;br /&gt;
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|location=New York|title-link=Elementary Principles in Statistical Mechanics }}&amp;lt;/ref&amp;gt;&lt;br /&gt;
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波兹曼分布是根据路德维希·玻尔兹曼1868年在研究统计力学中气体热平衡的时候首次提出的一个公式命名的。波尔兹曼的统计工作在他1877年的论文《论热力学第二基本定理与热平衡条件的概率计算之间的关系》中得到了体现。&amp;lt;ref&amp;gt;“On the Relationship between the Second Fundamental Theorem of the Mechanical Theory of Heat and Probability Calculations Regarding the Conditions for Thermal Equilibrium” Sitzungberichte der Kaiserlichen Akademie der Wissenschaften. Mathematisch-Naturwissen Classe. Abt. II, LXXVI 1877, pp 373-435 (Wien. Ber. 1877, 76:373-435). &amp;lt;/ref&amp;gt; 在玻尔兹曼分布被发明之后，约西亚·华纳德·吉布森充分地研究了它并在1902年提出了它的一般形式。&amp;lt;ref name=&amp;quot;gibbs&amp;quot; /&amp;gt;&lt;br /&gt;
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The generalized Boltzmann distribution is a sufficient and necessary condition for the equivalence between the statistical mechanics definition of [[entropy]] (The [[Entropy_(statistical_thermodynamics)#Gibbs_entropy_formula | Gibbs entropy formula]] &amp;lt;math&amp;gt;S = -k_{\mathrm{B}}\sum_i p_i \log p_i&amp;lt;/math&amp;gt;) and the thermodynamic definition of entropy (&amp;lt;math&amp;gt;d S = \frac{\delta Q_\text{rev}}{T}&amp;lt;/math&amp;gt;, and the [[fundamental thermodynamic relation]]).&amp;lt;ref name=&amp;quot;:0&amp;quot;&amp;gt;{{cite journal |last1= Gao |first1= Xiang |last2= Gallicchio |first2= Emilio |first3= Adrian |last3= Roitberg  |date= 2019 |title= The generalized Boltzmann distribution is the only distribution in which the Gibbs-Shannon entropy equals the thermodynamic entropy |journal= The Journal of Chemical Physics|volume= 151|issue= 3|pages= 034113|doi= 10.1063/1.5111333|pmid= 31325924 |arxiv= 1903.02121 |s2cid= 118981017 }}&amp;lt;/ref&amp;gt;&lt;br /&gt;
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广义波兹曼分布是熵的统计力学定义(吉布斯熵公式  &amp;lt;math&amp;gt;S = -k_{\mathrm{B}}\sum_i p_i \log p_i&amp;lt;/math&amp;gt;))与熵的热力学定义(&amp;lt;math&amp;gt;d S = \frac{\delta Q_\text{rev}}{T}&amp;lt;/math&amp;gt;)等价的充要条件。&amp;lt;ref name=&amp;quot;:0&amp;quot; /&amp;gt;&lt;br /&gt;
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The Boltzmann distribution should not be confused with the [[Maxwell–Boltzmann distribution]]. The former gives the probability that a system will be in a certain state as a function of that state's energy;&amp;lt;ref name=&amp;quot;Atkins, P. W. 2010&amp;quot;&amp;gt;Atkins, P. W. (2010) Quanta, W. H. Freeman and Company, New York&amp;lt;/ref&amp;gt; in contrast, the latter is used to describe particle speeds in idealized gases.&lt;br /&gt;
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值得一提的是，玻尔兹曼分布不应与麦克斯韦-玻尔兹曼分布混淆。前者给出了系统处于某种状态的概率，作为该状态能量的函数; 后者则是用于描述理想气体中的粒子速度。&lt;br /&gt;
==分布==&lt;br /&gt;
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The Boltzmann distribution is a [[probability distribution]] that gives the probability of a certain state as a function of that state's energy and  temperature of the [[system]] to which the distribution is applied.&amp;lt;ref name=&amp;quot;McQuarrie, A. 2000&amp;quot;&amp;gt;McQuarrie, A. (2000) Statistical Mechanics, University Science Books, California&amp;lt;/ref&amp;gt; It is given as&lt;br /&gt;
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波兹曼分布是一个概率分布，它给出了出于某种量子态处于某种能量和温度的时候的概率。它被这样定义：&lt;br /&gt;
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&amp;lt;math&amp;gt;&lt;br /&gt;
p_i=\frac{1}{Q}} {e^{- {\varepsilon}_i / k T}=\frac{e^{- {\varepsilon}_i / k T}}{\sum_{j=1}^{M}{e^{- {\varepsilon}_j / k T}}}&lt;br /&gt;
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&amp;lt;/math&amp;gt;&lt;br /&gt;
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where ''p&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;'' is the probability of state ''i'', ''ε&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;'' the energy of state ''i'', ''k'' the Boltzmann constant, ''T'' the temperature of the system and ''M'' is the number of all states accessible to the system of interest.&amp;lt;ref name=&amp;quot;McQuarrie, A. 2000&amp;quot; /&amp;gt;&amp;lt;ref name=&amp;quot;Atkins, P. W. 2010&amp;quot; /&amp;gt; Implied parentheses around the denominator ''kT'' are omitted for brevity. The normalization denominator ''Q'' (denoted by some authors by ''Z'') is the [[canonical partition function]]&lt;br /&gt;
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其中 ''p&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;'' 是状态 i 的概率，''ε&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;'' 是状态 i 的能量，''k'' 是波兹曼常数，''T'' 是系统的温度，''M'' 是系统所能到达的所有量子态的数目。&amp;lt;ref name=&amp;quot;Atkins, P. W. 2010&amp;quot; /&amp;gt; &amp;lt;ref name=&amp;quot;McQuarrie, A. 2000&amp;quot; /&amp;gt;这里为了简洁美观，省略了''kT''周围的括弧。归一化的分母''Q''（被有些作者写为''Z''）是对于系统中所有量子态进行总和，此部分又被称为[[Index.php?title=Canonical partition function|正则配分函数]]''。''&lt;br /&gt;
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It results from the constraint that the probabilities of all accessible states must add up to 1.&lt;br /&gt;
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所有量子态的概率之和为1.&lt;br /&gt;
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The Boltzmann distribution is the distribution that maximizes the [[entropy]]，&lt;br /&gt;
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&amp;lt;math&amp;gt;H(p_1,p_2,\cdots,p_M) = -\sum_{i=1}^{M} p_i\log_2 p_i&amp;lt;/math&amp;gt;&lt;br /&gt;
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subject to the constraint that  ΣΡ&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;ε&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt; equals a particular mean energy value (which can be proven using [[Lagrange multipliers]]).&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
当 ΣΡ&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;ε&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;等于平均能量值时，玻尔兹曼分布是这种情况下能让熵最大化的分布。我们可以通过拉格朗日乘数法来证明。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The partition function can be calculated if we know the energies of the states accessible to the system of interest. For atoms the partition function values can be found in the NIST Atomic Spectra Database.&amp;lt;ref name=&amp;quot;:1&amp;quot;&amp;gt;[http://physics.nist.gov/PhysRefData/ASD/levels_form.html NIST Atomic Spectra Database Levels Form] at nist.gov&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
在知道量子态能量的情况下，这个配分函数可以被计算。对于原子来说，配分函数的值可以在NIST Atomic Spectra Database中找到。&amp;lt;ref name=&amp;quot;:1&amp;quot; /&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The distribution shows that states with lower energy will always have a higher probability of being occupied than the states with higher energy. It can also give us the quantitative relationship between the probabilities of the two states being occupied. The ratio of probabilities for states i and j is given as&lt;br /&gt;
&lt;br /&gt;
玻尔兹曼分布指出，能量低的量子态总是有比能量高的量子态更高的概率被粒子占据。它同时也能让我们定量地比较两个量子态分布概率的关系。状态 i 和状态 j 的概率比为&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
{\frac{p_i}{p_j}}=e^{({\varepsilon}_j-{\varepsilon}_i) / k T}&lt;br /&gt;
&lt;br /&gt;
&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
where p&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt; is the probability of state i,  p&amp;lt;sub&amp;gt;j&amp;lt;/sub&amp;gt; the probability of state j, and ε&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt; and ε&amp;lt;sub&amp;gt;j&amp;lt;/sub&amp;gt; are the energies of states i and j, respectively.&lt;br /&gt;
&lt;br /&gt;
其中 p&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt; 是量子态 i 的概率， p&amp;lt;sub&amp;gt;j&amp;lt;/sub&amp;gt; 是量子态 j 的概率，ε&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt; 和 ε&amp;lt;sub&amp;gt;j&amp;lt;/sub&amp;gt; 分别是状态 i 和 j 的能量。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The Boltzmann distribution is often used to describe the distribution of particles, such as atoms or molecules, over energy states accessible to them. If we have a system consisting of many particles, the probability of a particle being in state i is practically the probability that, if we pick a random particle from that system and check what state it is in, we will find it is in state i. This probability is equal to the number of particles in state i divided by the total number of particles in the system, that is the fraction of particles that occupy state i.&lt;br /&gt;
&lt;br /&gt;
玻尔兹曼分布通常被用来描述粒子的分布，比如原子或分子，在能量状态上的分布情况。如果我们有一个由许多粒子组成的系统，某个粒子处于量子态 i 的概率就等同于当我们从该系统中选择一个随机的粒子并观察它处于什么状态，发现它处于状态 i 的概率。这个概率等于量子态 i 的粒子数除以系统中粒子的总数，即那些占据量子态i的粒子的比例。&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
p_i={\frac{N_i}{N}}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
where N&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt; is the number of particles in state i and N is the total number of particles in the system. We may use the Boltzmann distribution to find this probability that is, as we have seen, equal to the fraction of particles that are in state i. So the equation that gives the fraction of particles in state i as a function of the energy of that state is&lt;br /&gt;
&lt;br /&gt;
N&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt; 是位于量子态 i 的粒子数，N是系统中粒子的总数。我们可以用波兹曼分布来求出这个概率，它等于处于量子态i的粒子的比例。所以这个方程给出位于量子态 i 的粒子比例关于这个状态能量的函数&amp;lt;ref name=&amp;quot;Atkins, P. W. 2010&amp;quot; /&amp;gt;。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt;&lt;br /&gt;
{\frac{N_i}{N}}={\frac{e^{- {\varepsilon}_i / k T}}{\sum_{j=1}^{M}{e^{- {\varepsilon}_j / k T}}}} &lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
This equation is of great importance to [[spectroscopy]]. In spectroscopy we observe a [[spectral line]] of atoms or molecules that we are interested in going from one state to another.&amp;lt;ref name=&amp;quot;Atkins, P. W. 2010&amp;quot; /&amp;gt;&amp;lt;ref name=&amp;quot;:2&amp;quot;&amp;gt;Atkins, P. W.; de Paula J. (2009) Physical Chemistry, 9th edition, Oxford University Press, Oxford, UK&amp;lt;/ref&amp;gt; In order for this to be possible, there must be some particles in the first state to undergo the transition. We may find that this condition is fulfilled by finding the fraction of particles in the first state. If it is negligible, the transition is very likely not to be observed at the temperature for which the calculation was done. In general, a larger fraction of molecules in the first state means a higher number of transitions to the second state.&amp;lt;ref name=&amp;quot;:3&amp;quot;&amp;gt;Skoog, D. A.; Holler, F. J.; Crouch, S. R. (2006) Principles of Instrumental Analysis, Brooks/Cole, Boston, MA&amp;lt;/ref&amp;gt; This gives a stronger spectral line. However, there are other factors that influence the intensity of a spectral line, such as whether it is caused by an allowed or a [[forbidden transition]]&lt;br /&gt;
&lt;br /&gt;
对于光谱学来说这很重要在。在光谱中，我们期待能观察到一条原子或分子跃迁的谱线。&amp;lt;ref name=&amp;quot;Atkins, P. W. 2010&amp;quot; /&amp;gt;&amp;lt;ref name=&amp;quot;:2&amp;quot; /&amp;gt; 在为了使这成为可能，必须有一些粒子处于第一个量子态，等待着发生跃迁。我们可以通过求第一态粒子的比例来满足这个条件。如果它可以忽略不计，那么在当前计算的温度下，则很难观察到这种跃迁。一般来说，处于第一状态的分子比例越大，意味着向第二状态跃迁的次数越多。&amp;lt;ref name=&amp;quot;:3&amp;quot; /&amp;gt;这就产生了一条更强的谱线。然而，还有其他因素影响谱线的强度，例如它是否是被允许的跃迁还是被禁止的跃迁。&lt;br /&gt;
&lt;br /&gt;
The Boltzmann distribution is related to the [[softmax function]] commonly used in machine learning.&lt;br /&gt;
&lt;br /&gt;
玻尔兹曼分布与机器学习中常用的[[Index.php?title=Softmax function|归一化指数函数]]（Softmax 函数）有关。&lt;br /&gt;
=='''统计力学'''==&lt;br /&gt;
&lt;br /&gt;
{{main|Canonical ensemble|Maxwell–Boltzmann statistics}}The Boltzmann distribution appears in statistical mechanics when considering isolated (or nearly-isolated) systems of fixed composition that are in thermal equilibrium (equilibrium with respect to energy exchange). The most general case is the probability distribution for the canonical ensemble, but also some special cases (derivable from the canonical ensemble) also show the Boltzmann distribution in different aspects:&lt;br /&gt;
&lt;br /&gt;
当独立的(或者几乎独立的)固定体系处于统计力学热平衡状态时，玻尔兹曼分布就会出现。最普遍的情况是概率分布的正则系综，但也有一些特殊的情况(从正则系综衍生)也显示了不同形式的玻尔兹曼分布:&lt;br /&gt;
&lt;br /&gt;
;[[Canonical ensemble]] (general case)&lt;br /&gt;
;'''正则系综(一般情况)'''&lt;br /&gt;
;'''The [[canonical ensemble]] gives the [[probabilities]] of the various possible states of a closed system of fixed volume, in thermal equilibrium with a [[heat bath]]. The canonical ensemble is a probability distribution with the Boltzmann form.'''&lt;br /&gt;
&lt;br /&gt;
正则系综模型给出了在一个封闭固定体积，带有热浴的热平衡系统中的各种可能状态的概率。我们称正则系综为一个玻尔兹曼概率分布。&lt;br /&gt;
&lt;br /&gt;
;&lt;br /&gt;
;Statistical frequencies of subsystems' states (in a non-interacting collection)&lt;br /&gt;
'''子系统状态的统计频率(在一个无交互的集合中)'''&lt;br /&gt;
:When the system of interest is a collection of many non-interacting copies of a smaller subsystem, it is sometimes useful to find the [[statistical frequency]] of a given subsystem state, among the collection. The canonical ensemble has the property of separability when applied to such a collection: as long as the non-interacting subsystems have fixed composition, then each subsystem's state is independent of the others and is also characterized by a canonical ensemble. As a result, the [[expectation value|expected]] statistical frequency distribution of subsystem states has the Boltzmann form.&lt;br /&gt;
&lt;br /&gt;
当系统是一个较小子系统的许多非交互副本的集合时，有时我们需要在某个子系统集合中找到某个子系统的统计频率。当应用于这样一个集合时，这个子系统的正则系综具有可分离性: 只要不相互作用的子系统的组成是固定的，那么每个子系统的状态都是独立于其他子系统的，它们也拥有自己的正则系综。因此，子系统状态的期望统计频率分布形式是玻尔兹曼分布。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[Maxwell–Boltzmann statistics]] of classical gases (systems of non-interacting particles)&lt;br /&gt;
&lt;br /&gt;
'''Maxwell-Boltzmann 统计中的经典气体系统(非相互作用粒子系统)'''&lt;br /&gt;
&lt;br /&gt;
:In particle systems, many particles share the same space and regularly change places with each other; the single-particle state space they occupy is a shared space. [[Maxwell–Boltzmann statistics]] give the expected number of particles found in a given single-particle state, in a [[classical mechanics|classical]] gas of non-interacting particles at equilibrium. This expected number distribution has the Boltzmann form.&lt;br /&gt;
&lt;br /&gt;
在粒子系统中，许多粒子共享同一空间，并且相互之间有规律地改变位置; 它们所占据的单粒子状态空间是一个共享空间。[[Index.php?title=Maxwell–Boltzmann statistics|麦克斯韦-玻尔兹曼统计]]给出了在一个给定的单粒子态，在一个处于平衡状态的非相互作用粒子的经典气体中所发现的粒子的预期数量。这个预期的数量分布具有玻尔兹曼分布形式。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Although these cases have strong similarities, it is helpful to distinguish them as they generalize in different ways when the crucial assumptions are changed:&lt;br /&gt;
&lt;br /&gt;
虽然这些案例有很多相似之处，但是当关键假设发生变化时，我们需要对它们以不同的方式进行归纳总结，因此区分它们是有帮助的:&lt;br /&gt;
*When a system is in thermodynamic equilibrium with respect to both energy exchange ''and particle exchange'', the requirement of fixed composition is relaxed and a [[grand canonical ensemble]] is obtained rather than canonical ensemble. On the other hand, if both composition and energy are fixed, then a [[microcanonical ensemble]] applies instead.&lt;br /&gt;
*当一个系统在能量交换和粒子交换方面都处于热力学平衡时，固定组成的要求就放宽了。这时我们就得到了一个[[Index.php?title=Microcanonical ensemble|巨正则系综]]而不是正则系综。另一方面，如果成分和能量都是固定的，则可以使用[[微正则系综Index.php?title=Microcanonical ensemble|微正则系综]]。&lt;br /&gt;
&lt;br /&gt;
*If the subsystems within a collection ''do'' interact with each other, then the expected frequencies of subsystem states no longer follow a Boltzmann distribution, and even may not have an [[analytical solution]].&amp;lt;ref name=&amp;quot;:4&amp;quot;&amp;gt;A classic example of this is [[magnetic ordering]]. Systems of non-interacting [[spin (physics)|spins]] show [[paramagnetic]] behaviour that can be understood with a single-particle canonical ensemble (resulting in the [[Brillouin function]]). Systems of ''interacting'' spins can show much more complex behaviour such as [[ferromagnetism]] or [[antiferromagnetism]].&amp;lt;/ref&amp;gt; The canonical ensemble can however still be applied to the ''collective'' states of the entire system considered as a whole, provided the entire system is isolated and in thermal equilibrium.&lt;br /&gt;
*如果集合中的子系统确实相互交互，则子系统状态的预期频率不再遵循玻尔兹曼 分布，甚至可能没有解析解。&amp;lt;ref name=&amp;quot;:4&amp;quot; /&amp;gt;然而，如果整个系统是独立的并且处于热平衡状态，则正则系综仍然可以应用于作为一个整体考虑。&lt;br /&gt;
&lt;br /&gt;
*With ''[[quantum mechanics|quantum]]'' gases of non-interacting particles in equilibrium, the number of particles found in a given single-particle state does not follow Maxwell–Boltzmann statistics, and there is no simple closed form expression for quantum gases in the canonical ensemble. In the grand canonical ensemble the state-filling statistics of quantum gases are described by [[Fermi–Dirac statistics]] or [[Bose–Einstein statistics]], depending on whether the particles are [[fermion]]s or [[boson]]s respectively.&lt;br /&gt;
*对于处于平衡状态的非相互作用粒子的量子气体，在给定的单粒子状态中发现的粒子数量并不遵循麦克斯韦-玻尔兹曼统计。并且正则系综中的量子气体没有简单的封闭表达式。在巨正则系综中，量子气体的统计分布状态由费米-狄拉克统计或玻色-爱因斯坦统计来描述，具体则取决于该粒子是费米子还是玻色子。&lt;br /&gt;
&lt;br /&gt;
==数学==&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
In more general mathematical settings, the Boltzmann distribution is also known as the [[Gibbs measure]]. In statistics and machine learning, it is called a [[log-linear model]]. In [[deep learning]], the Boltzmann distribution is used in the sampling distribution of [[stochastic neural network]]s such as the [[Boltzmann machine]], [[Restricted Boltzmann machine]], [[Energy based model|Energy-Based models]] and [[Deep Boltzmann Machine|deep Boltzmann machine]]&lt;br /&gt;
&lt;br /&gt;
在更一般的数学环境中，玻尔兹曼分布也被称为吉布斯量度。在统计学和机器学习中，它被称为对数线性回归。在深度学习中，玻尔兹曼分布被用于随机神经网络的抽样分布，如玻尔兹曼机、受限玻尔兹曼机、基于能量的模型和深度波茨曼机。&lt;br /&gt;
&lt;br /&gt;
==经济==&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The Boltzmann distribution can be introduced to allocate permits in emissions trading.&amp;lt;ref name=&amp;quot;Park, J.-W. 2012&amp;quot;&amp;gt;Park, J.-W., Kim, C. U. and Isard, W. (2012) Permit allocation in emissions trading using the Boltzmann distribution. Physica A 391: 4883–4890&amp;lt;/ref&amp;gt;&amp;lt;ref name=&amp;quot;:5&amp;quot;&amp;gt;[http://www.technologyreview.com/view/425051/the-thorny-problem-of-fair-allocation/ The Thorny Problem Of Fair Allocation]. ''Technology Review'' blog. August 17, 2011. Cites and summarizes Park, Kim and Isard (2012).&amp;lt;/ref&amp;gt; The new allocation method using the Boltzmann distribution can describe the most probable, natural, and unbiased distribution of emissions permits among multiple countries. Simple and versatile, this new method holds potential for many economic and environmental applications.&lt;br /&gt;
&lt;br /&gt;
在经济学中，玻尔兹曼分布被用来分配排放交易中的许可。&amp;lt;ref name=&amp;quot;Park, J.-W. 2012&amp;quot; /&amp;gt;&amp;lt;ref name=&amp;quot;:5&amp;quot; /&amp;gt;  使用玻尔兹曼分布的新分配方法可以创造出在多个国家之间最可能的、自然的和无偏见的排放许可分配。这种新方法简单而通用，在经济和环保中有很大的应用潜力。&lt;br /&gt;
&lt;br /&gt;
The Boltzmann distribution has the same form as the [[Multinomial logistic regression|multinomial logit]] model. As a [[discrete choice]] model, this is very well known in economics since [[Daniel McFadden]] made the connection to random utility maximization.&lt;br /&gt;
&lt;br /&gt;
玻尔兹曼分布与多项逻辑回归模型具有相同的形式。在丹尼尔 · 麦克法登将它与随机效用最大化联系起来之后，成为了大家所熟知的一种离散选择模型。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Category:Statistical mechanics&lt;br /&gt;
&lt;br /&gt;
类别: 统计力学&lt;br /&gt;
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本中文词条由[[用户:费米子|tueryeye]]编辑，欢迎在讨论页面留言。&lt;br /&gt;
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==See also==&lt;br /&gt;
&lt;br /&gt;
Distribution&lt;br /&gt;
&lt;br /&gt;
分布&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:Boltzmann distribution]]. Its edit history can be viewed at [[玻尔兹曼分布/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;br /&gt;
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&amp;lt;references /&amp;gt;&lt;/div&gt;</summary>
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&lt;div&gt;此词条暂由tueryeye翻译和审校，翻译字数共1452，带来阅读不便，请见谅。&lt;br /&gt;
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{{Use American English|date = March 2019}}&lt;br /&gt;
&lt;br /&gt;
{{Short description|Probability distribution of energy states of a system}}&lt;br /&gt;
&lt;br /&gt;
{{about|system energy states|particle energy levels and velocities|Maxwell–Boltzmann distribution}}&lt;br /&gt;
&lt;br /&gt;
[[File:Boltzmann distribution graph.svg|upright=1.75|right|thumb|Boltzmann factor ''p&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;''&amp;amp;nbsp;/&amp;amp;nbsp;''p&amp;lt;sub&amp;gt;j&amp;lt;/sub&amp;gt;'' (vertical axis) as a function of temperature ''T'' for several energy differences ''ε&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;''&amp;amp;nbsp;−&amp;amp;nbsp;''ε&amp;lt;sub&amp;gt;j&amp;lt;/sub&amp;gt;''.|链接=Special:FilePath/Boltzmann_distribution_graph.svg]]&lt;br /&gt;
&lt;br /&gt;
In [[statistical mechanics]] and [[mathematics]], a '''Boltzmann distribution''' (also called '''Gibbs distribution'''&amp;lt;ref name=&amp;quot;landau&amp;quot;&amp;gt;{{cite book | author=Landau, Lev Davidovich |author2=Lifshitz, Evgeny Mikhailovich |name-list-style=amp | title=Statistical Physics |volume=5 |series=Course of Theoretical Physics |edition=3 |origyear=1976 |year=1980 |place=Oxford |publisher=Pergamon Press|isbn=0-7506-3372-7|author-link=Lev Landau |author2-link=Evgeny Lifshitz }} Translated by J.B. Sykes and M.J. Kearsley. See section 28&amp;lt;/ref&amp;gt;) is a [[probability distribution]] or [[probability measure]] that gives the probability that a system will be in a certain [[microstate (statistical mechanics)|state]] as a function of that state's energy and the temperature of the system. The distribution is expressed in the form:&lt;br /&gt;
&lt;br /&gt;
在统计力学和数学中，波兹曼分布分布(也称为吉布斯分布&amp;lt;ref name=&amp;quot;landau&amp;quot; /&amp;gt;)是一个概率分布或机率量测，它给出了一个系统处于某种量子态的概率，这个概率是该状态的能量和系统温度的函数。分布情况以下列形式表示:&lt;br /&gt;
:&amp;lt;math&amp;gt;p_i \propto e^{-\frac{\varepsilon_i}{kT}}&amp;lt;/math&amp;gt; &lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
where {{mvar|p&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;}} is the probability of the system being in state {{mvar|i}}, {{mvar|ε&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;}} is the energy of that state, and a constant {{mvar|kT}} of the distribution is the product of [[Boltzmann's constant]] {{mvar|k}} and [[thermodynamic temperature]] {{mvar|T}}. The symbol &amp;lt;math display=&amp;quot;inline&amp;quot;&amp;gt;\propto&amp;lt;/math&amp;gt; denotes [[proportionality (mathematics)|proportionality]] (see {{section link||The distribution}} for the proportionality constant).&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
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{{mvar|p&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;}} 是其中系统处于状态{{mvar|i}}的概率, {{mvar|ε&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;}} 是该状态的能量，还有关于这个分布的一个常数 {{mvar|kT}} ，它是玻尔兹曼常数{{mvar|k}}和热力学温度 {{mvar|T}} 的乘积。符号 &amp;lt;math display=&amp;quot;inline&amp;quot;&amp;gt;\propto&amp;lt;/math&amp;gt;表示正比例(见附录中的比例常数)。&lt;br /&gt;
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The term system here has a very wide meaning; it can range from a single atom to a macroscopic system such as a [[Natural gas storage|natural gas storage tank]]. Because of this the Boltzmann distribution can be used to solve a very wide variety of problems. The distribution shows that states with lower energy will always have a higher probability of being occupied .&lt;br /&gt;
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这里的术语系统含义广泛; 它可以从单个原子到宏观系统，如天然气储罐。正因为如此，波兹曼分布可以用来解决各种各样的问题。玻尔兹曼分布表明，能量较低的状态被占据的概率总是较高的。&lt;br /&gt;
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The ''ratio'' of probabilities of two states is known as the '''Boltzmann factor''' and characteristically only depends on the states' energy difference:&lt;br /&gt;
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两种状态的概率之比被称为玻尔兹曼因子，取决于两种状态的能量差:&lt;br /&gt;
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&amp;lt;math&amp;gt;\frac{p_i}{p_j} = e^{\frac{\varepsilon_j - \varepsilon_i}{kT}}&amp;lt;/math&amp;gt;&lt;br /&gt;
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The Boltzmann distribution is named after [[Ludwig Boltzmann]] who first formulated it in 1868 during his studies of the [[statistical mechanics]] of gases in thermal equilibrium. Boltzmann's statistical work is borne out in his paper “On the Relationship between the Second Fundamental Theorem of the Mechanical Theory of Heat and Probability Calculations Regarding the Conditions for Thermal Equilibrium&amp;quot;&amp;lt;ref&amp;gt;http://crystal.med.upenn.edu/sharp-lab-pdfs/2015SharpMatschinsky_Boltz1877_Entropy17.pdf&amp;lt;/ref&amp;gt;. The distribution was later investigated extensively, in its modern generic form, by [[Josiah Willard Gibbs]] in 1902.&amp;lt;ref name=&amp;quot;gibbs&amp;quot;&amp;gt;{{cite book |last=Gibbs |first=Josiah Willard |authorlink=Josiah Willard Gibbs |title=Elementary Principles in Statistical Mechanics |year=1902 |publisher=[[Charles Scribner's Sons]] &lt;br /&gt;
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The distribution was later investigated extensively, in its modern generic form, by Josiah Willard Gibbs in 1902.&lt;br /&gt;
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这种分布后来在1902年由约西亚·威拉德·吉布斯进行了广泛的调查，以其现代通用形式。&lt;br /&gt;
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|location=New York|title-link=Elementary Principles in Statistical Mechanics }}&amp;lt;/ref&amp;gt;&lt;br /&gt;
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波兹曼分布是根据路德维希·玻尔兹曼1868年在研究统计力学中气体热平衡的时候首次提出的一个公式命名的。波尔兹曼的统计工作在他1877年的论文《论热力学第二基本定理与热平衡条件的概率计算之间的关系》中得到了体现。&amp;lt;ref&amp;gt;“On the Relationship between the Second Fundamental Theorem of the Mechanical Theory of Heat and Probability Calculations Regarding the Conditions for Thermal Equilibrium” Sitzungberichte der Kaiserlichen Akademie der Wissenschaften. Mathematisch-Naturwissen Classe. Abt. II, LXXVI 1877, pp 373-435 (Wien. Ber. 1877, 76:373-435). &amp;lt;/ref&amp;gt; 在玻尔兹曼分布被发明之后，约西亚·华纳德·吉布森充分地研究了它并在1902年提出了它的一般形式。&amp;lt;ref name=&amp;quot;gibbs&amp;quot; /&amp;gt;&lt;br /&gt;
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The generalized Boltzmann distribution is a sufficient and necessary condition for the equivalence between the statistical mechanics definition of [[entropy]] (The [[Entropy_(statistical_thermodynamics)#Gibbs_entropy_formula | Gibbs entropy formula]] &amp;lt;math&amp;gt;S = -k_{\mathrm{B}}\sum_i p_i \log p_i&amp;lt;/math&amp;gt;) and the thermodynamic definition of entropy (&amp;lt;math&amp;gt;d S = \frac{\delta Q_\text{rev}}{T}&amp;lt;/math&amp;gt;, and the [[fundamental thermodynamic relation]]).&amp;lt;ref name=&amp;quot;:0&amp;quot;&amp;gt;{{cite journal |last1= Gao |first1= Xiang |last2= Gallicchio |first2= Emilio |first3= Adrian |last3= Roitberg  |date= 2019 |title= The generalized Boltzmann distribution is the only distribution in which the Gibbs-Shannon entropy equals the thermodynamic entropy |journal= The Journal of Chemical Physics|volume= 151|issue= 3|pages= 034113|doi= 10.1063/1.5111333|pmid= 31325924 |arxiv= 1903.02121 |s2cid= 118981017 }}&amp;lt;/ref&amp;gt;&lt;br /&gt;
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广义波兹曼分布是熵的统计力学定义(吉布斯熵公式  &amp;lt;math&amp;gt;S = -k_{\mathrm{B}}\sum_i p_i \log p_i&amp;lt;/math&amp;gt;))与熵的热力学定义(&amp;lt;math&amp;gt;d S = \frac{\delta Q_\text{rev}}{T}&amp;lt;/math&amp;gt;)等价的充要条件。&amp;lt;ref name=&amp;quot;:0&amp;quot; /&amp;gt;&lt;br /&gt;
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The Boltzmann distribution should not be confused with the [[Maxwell–Boltzmann distribution]]. The former gives the probability that a system will be in a certain state as a function of that state's energy;&amp;lt;ref name=&amp;quot;Atkins, P. W. 2010&amp;quot;&amp;gt;Atkins, P. W. (2010) Quanta, W. H. Freeman and Company, New York&amp;lt;/ref&amp;gt; in contrast, the latter is used to describe particle speeds in idealized gases.&lt;br /&gt;
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值得一提的是，玻尔兹曼分布不应与麦克斯韦-玻尔兹曼分布混淆。前者给出了系统处于某种状态的概率，作为该状态能量的函数; 后者则是用于描述理想气体中的粒子速度。&lt;br /&gt;
==分布==&lt;br /&gt;
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The Boltzmann distribution is a [[probability distribution]] that gives the probability of a certain state as a function of that state's energy and  temperature of the [[system]] to which the distribution is applied.&amp;lt;ref name=&amp;quot;McQuarrie, A. 2000&amp;quot;&amp;gt;McQuarrie, A. (2000) Statistical Mechanics, University Science Books, California&amp;lt;/ref&amp;gt; It is given as&lt;br /&gt;
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波兹曼分布是一个概率分布，它给出了出于某种量子态处于某种能量和温度的时候的概率。它被这样定义：&lt;br /&gt;
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&amp;lt;math&amp;gt;&lt;br /&gt;
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:&amp;lt;math&amp;gt;&lt;br /&gt;
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p_i=\frac{1}{Q}} {e^{- {\varepsilon}_i / k T}=\frac{e^{- {\varepsilon}_i / k T}}{\sum_{j=1}^{M}{e^{- {\varepsilon}_j / k T}}}&lt;br /&gt;
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P _ i = frac {1}{ q }{ e ^ {-{ varepsilon } _ i/k t } = frac { e ^ {-{ varepsilon } _ i/k t }{ sum { j = 1} ^ { m }{ e ^ {-{ varepsilon } _ j/k t }}}}}&lt;br /&gt;
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p_i=\frac{1}{Q}} {e^{- {\varepsilon}_i / k T}=\frac{e^{- {\varepsilon}_i / k T}}{\sum_{j=1}^{M}{e^{- {\varepsilon}_j / k T}}}&lt;br /&gt;
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&amp;lt;/math&amp;gt;&lt;br /&gt;
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where ''p&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;'' is the probability of state ''i'', ''ε&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;'' the energy of state ''i'', ''k'' the Boltzmann constant, ''T'' the temperature of the system and ''M'' is the number of all states accessible to the system of interest.&amp;lt;ref name=&amp;quot;McQuarrie, A. 2000&amp;quot; /&amp;gt;&amp;lt;ref name=&amp;quot;Atkins, P. W. 2010&amp;quot; /&amp;gt; Implied parentheses around the denominator ''kT'' are omitted for brevity. The normalization denominator ''Q'' (denoted by some authors by ''Z'') is the [[canonical partition function]]&lt;br /&gt;
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其中 ''p&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;'' 是状态 i 的概率，''ε&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;'' 是状态 i 的能量，''k'' 是波兹曼常数，''T'' 是系统的温度，''M'' 是系统所能到达的所有量子态的数目。&amp;lt;ref name=&amp;quot;Atkins, P. W. 2010&amp;quot; /&amp;gt; &amp;lt;ref name=&amp;quot;McQuarrie, A. 2000&amp;quot; /&amp;gt;这里为了简洁美观，省略了''kT''周围的括弧。归一化的分母''Q''（被有些作者写为''Z''）是对于系统中所有量子态进行总和，此部分又被称为[[Index.php?title=Canonical partition function|正则配分函数]]''。''&lt;br /&gt;
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It results from the constraint that the probabilities of all accessible states must add up to 1.&lt;br /&gt;
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所有量子态的概率之和为1.&lt;br /&gt;
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The Boltzmann distribution is the distribution that maximizes the [[entropy]]，&lt;br /&gt;
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&amp;lt;math&amp;gt;H(p_1,p_2,\cdots,p_M) = -\sum_{i=1}^{M} p_i\log_2 p_i&amp;lt;/math&amp;gt;&lt;br /&gt;
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subject to the constraint that  ΣΡ&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;ε&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt; equals a particular mean energy value (which can be proven using [[Lagrange multipliers]]).&lt;br /&gt;
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当 ΣΡ&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;ε&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;等于平均能量值时，玻尔兹曼分布是这种情况下能让熵最大化的分布。我们可以通过拉格朗日乘数法来证明。&lt;br /&gt;
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The partition function can be calculated if we know the energies of the states accessible to the system of interest. For atoms the partition function values can be found in the NIST Atomic Spectra Database.&amp;lt;ref name=&amp;quot;:1&amp;quot;&amp;gt;[http://physics.nist.gov/PhysRefData/ASD/levels_form.html NIST Atomic Spectra Database Levels Form] at nist.gov&amp;lt;/ref&amp;gt;&lt;br /&gt;
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在知道量子态能量的情况下，这个配分函数可以被计算。对于原子来说，配分函数的值可以在NIST Atomic Spectra Database中找到。&amp;lt;ref name=&amp;quot;:1&amp;quot; /&amp;gt;&lt;br /&gt;
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The distribution shows that states with lower energy will always have a higher probability of being occupied than the states with higher energy. It can also give us the quantitative relationship between the probabilities of the two states being occupied. The ratio of probabilities for states i and j is given as&lt;br /&gt;
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玻尔兹曼分布指出，能量低的量子态总是有比能量高的量子态更高的概率被粒子占据。它同时也能让我们定量地比较两个量子态分布概率的关系。状态 i 和状态 j 的概率比为&lt;br /&gt;
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:&amp;lt;math&amp;gt;&lt;br /&gt;
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{\frac{p_i}{p_j}}=e^{({\varepsilon}_j-{\varepsilon}_i) / k T}&lt;br /&gt;
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&amp;lt;/math&amp;gt;&lt;br /&gt;
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where p&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt; is the probability of state i,  p&amp;lt;sub&amp;gt;j&amp;lt;/sub&amp;gt; the probability of state j, and ε&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt; and ε&amp;lt;sub&amp;gt;j&amp;lt;/sub&amp;gt; are the energies of states i and j, respectively.&lt;br /&gt;
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其中 p&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt; 是量子态 i 的概率， p&amp;lt;sub&amp;gt;j&amp;lt;/sub&amp;gt; 是量子态 j 的概率，ε&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt; 和 ε&amp;lt;sub&amp;gt;j&amp;lt;/sub&amp;gt; 分别是状态 i 和 j 的能量。&lt;br /&gt;
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The Boltzmann distribution is often used to describe the distribution of particles, such as atoms or molecules, over energy states accessible to them. If we have a system consisting of many particles, the probability of a particle being in state i is practically the probability that, if we pick a random particle from that system and check what state it is in, we will find it is in state i. This probability is equal to the number of particles in state i divided by the total number of particles in the system, that is the fraction of particles that occupy state i.&lt;br /&gt;
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玻尔兹曼分布通常被用来描述粒子的分布，比如原子或分子，在能量状态上的分布情况。如果我们有一个由许多粒子组成的系统，某个粒子处于量子态 i 的概率就等同于当我们从该系统中选择一个随机的粒子并观察它处于什么状态，发现它处于状态 i 的概率。这个概率等于量子态 i 的粒子数除以系统中粒子的总数，即那些占据量子态i的粒子的比例。&lt;br /&gt;
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where N&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt; is the number of particles in state i and N is the total number of particles in the system. We may use the Boltzmann distribution to find this probability that is, as we have seen, equal to the fraction of particles that are in state i. So the equation that gives the fraction of particles in state i as a function of the energy of that state is&lt;br /&gt;
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N&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt; 是位于量子态 i 的粒子数，N是系统中粒子的总数。我们可以用波兹曼分布来求出这个概率，它等于处于量子态i的粒子的比例。所以这个方程给出位于量子态 i 的粒子比例关于这个状态能量的函数&amp;lt;ref name=&amp;quot;Atkins, P. W. 2010&amp;quot; /&amp;gt;。&lt;br /&gt;
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&amp;lt;nowiki&amp;gt;[math]\displaystyle{ {\frac{N_i}{N}}={\frac{e^{- {\varepsilon}_i / k T}}{\sum_{j=1}^{M}{e^{- {\varepsilon}_j / k T}}}} }[/math]&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
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This equation is of great importance to [[spectroscopy]]. In spectroscopy we observe a [[spectral line]] of atoms or molecules that we are interested in going from one state to another.&amp;lt;ref name=&amp;quot;Atkins, P. W. 2010&amp;quot; /&amp;gt;&amp;lt;ref name=&amp;quot;:2&amp;quot;&amp;gt;Atkins, P. W.; de Paula J. (2009) Physical Chemistry, 9th edition, Oxford University Press, Oxford, UK&amp;lt;/ref&amp;gt; In order for this to be possible, there must be some particles in the first state to undergo the transition. We may find that this condition is fulfilled by finding the fraction of particles in the first state. If it is negligible, the transition is very likely not to be observed at the temperature for which the calculation was done. In general, a larger fraction of molecules in the first state means a higher number of transitions to the second state.&amp;lt;ref name=&amp;quot;:3&amp;quot;&amp;gt;Skoog, D. A.; Holler, F. J.; Crouch, S. R. (2006) Principles of Instrumental Analysis, Brooks/Cole, Boston, MA&amp;lt;/ref&amp;gt; This gives a stronger spectral line. However, there are other factors that influence the intensity of a spectral line, such as whether it is caused by an allowed or a [[forbidden transition]]&lt;br /&gt;
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对于光谱学来说这很重要在。在光谱中，我们期待能观察到一条原子或分子跃迁的谱线。&amp;lt;ref name=&amp;quot;Atkins, P. W. 2010&amp;quot; /&amp;gt;&amp;lt;ref name=&amp;quot;:2&amp;quot; /&amp;gt; 在为了使这成为可能，必须有一些粒子处于第一个量子态，等待着发生跃迁。我们可以通过求第一态粒子的比例来满足这个条件。如果它可以忽略不计，那么在当前计算的温度下，则很难观察到这种跃迁。一般来说，处于第一状态的分子比例越大，意味着向第二状态跃迁的次数越多。&amp;lt;ref name=&amp;quot;:3&amp;quot; /&amp;gt;这就产生了一条更强的谱线。然而，还有其他因素影响谱线的强度，例如它是否是被允许的跃迁还是被禁止的跃迁。&lt;br /&gt;
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The Boltzmann distribution is related to the [[softmax function]] commonly used in machine learning.&lt;br /&gt;
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玻尔兹曼分布与机器学习中常用的[[Index.php?title=Softmax function|归一化指数函数]]（Softmax 函数）有关。&lt;br /&gt;
=='''统计力学'''==&lt;br /&gt;
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{{main|Canonical ensemble|Maxwell–Boltzmann statistics}}The Boltzmann distribution appears in statistical mechanics when considering isolated (or nearly-isolated) systems of fixed composition that are in thermal equilibrium (equilibrium with respect to energy exchange). The most general case is the probability distribution for the canonical ensemble, but also some special cases (derivable from the canonical ensemble) also show the Boltzmann distribution in different aspects:&lt;br /&gt;
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当独立的(或者几乎独立的)固定体系处于统计力学热平衡状态时，玻尔兹曼分布就会出现。最普遍的情况是概率分布的正则系综，但也有一些特殊的情况(从正则系综衍生)也显示了不同形式的玻尔兹曼分布:&lt;br /&gt;
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;[[Canonical ensemble]] (general case)&lt;br /&gt;
;'''正则系综(一般情况)'''&lt;br /&gt;
;'''The [[canonical ensemble]] gives the [[probabilities]] of the various possible states of a closed system of fixed volume, in thermal equilibrium with a [[heat bath]]. The canonical ensemble is a probability distribution with the Boltzmann form.'''&lt;br /&gt;
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正则系综模型给出了在一个封闭固定体积，带有热浴的热平衡系统中的各种可能状态的概率。我们称正则系综为一个玻尔兹曼概率分布。&lt;br /&gt;
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;Statistical frequencies of subsystems' states (in a non-interacting collection)&lt;br /&gt;
'''子系统状态的统计频率(在一个无交互的集合中)'''&lt;br /&gt;
:When the system of interest is a collection of many non-interacting copies of a smaller subsystem, it is sometimes useful to find the [[statistical frequency]] of a given subsystem state, among the collection. The canonical ensemble has the property of separability when applied to such a collection: as long as the non-interacting subsystems have fixed composition, then each subsystem's state is independent of the others and is also characterized by a canonical ensemble. As a result, the [[expectation value|expected]] statistical frequency distribution of subsystem states has the Boltzmann form.&lt;br /&gt;
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当系统是一个较小子系统的许多非交互副本的集合时，有时我们需要在某个子系统集合中找到某个子系统的统计频率。当应用于这样一个集合时，这个子系统的正则系综具有可分离性: 只要不相互作用的子系统的组成是固定的，那么每个子系统的状态都是独立于其他子系统的，它们也拥有自己的正则系综。因此，子系统状态的期望统计频率分布形式是玻尔兹曼分布。&lt;br /&gt;
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[[Maxwell–Boltzmann statistics]] of classical gases (systems of non-interacting particles)&lt;br /&gt;
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'''Maxwell-Boltzmann 统计中的经典气体系统(非相互作用粒子系统)'''&lt;br /&gt;
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:In particle systems, many particles share the same space and regularly change places with each other; the single-particle state space they occupy is a shared space. [[Maxwell–Boltzmann statistics]] give the expected number of particles found in a given single-particle state, in a [[classical mechanics|classical]] gas of non-interacting particles at equilibrium. This expected number distribution has the Boltzmann form.&lt;br /&gt;
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在粒子系统中，许多粒子共享同一空间，并且相互之间有规律地改变位置; 它们所占据的单粒子状态空间是一个共享空间。[[Index.php?title=Maxwell–Boltzmann statistics|麦克斯韦-玻尔兹曼统计]]给出了在一个给定的单粒子态，在一个处于平衡状态的非相互作用粒子的经典气体中所发现的粒子的预期数量。这个预期的数量分布具有玻尔兹曼分布形式。&lt;br /&gt;
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Although these cases have strong similarities, it is helpful to distinguish them as they generalize in different ways when the crucial assumptions are changed:&lt;br /&gt;
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虽然这些案例有很多相似之处，但是当关键假设发生变化时，我们需要对它们以不同的方式进行归纳总结，因此区分它们是有帮助的:&lt;br /&gt;
*When a system is in thermodynamic equilibrium with respect to both energy exchange ''and particle exchange'', the requirement of fixed composition is relaxed and a [[grand canonical ensemble]] is obtained rather than canonical ensemble. On the other hand, if both composition and energy are fixed, then a [[microcanonical ensemble]] applies instead.&lt;br /&gt;
*当一个系统在能量交换和粒子交换方面都处于热力学平衡时，固定组成的要求就放宽了。这时我们就得到了一个[[Index.php?title=Microcanonical ensemble|巨正则系综]]而不是正则系综。另一方面，如果成分和能量都是固定的，则可以使用[[微正则系综Index.php?title=Microcanonical ensemble|微正则系综]]。&lt;br /&gt;
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*If the subsystems within a collection ''do'' interact with each other, then the expected frequencies of subsystem states no longer follow a Boltzmann distribution, and even may not have an [[analytical solution]].&amp;lt;ref name=&amp;quot;:4&amp;quot;&amp;gt;A classic example of this is [[magnetic ordering]]. Systems of non-interacting [[spin (physics)|spins]] show [[paramagnetic]] behaviour that can be understood with a single-particle canonical ensemble (resulting in the [[Brillouin function]]). Systems of ''interacting'' spins can show much more complex behaviour such as [[ferromagnetism]] or [[antiferromagnetism]].&amp;lt;/ref&amp;gt; The canonical ensemble can however still be applied to the ''collective'' states of the entire system considered as a whole, provided the entire system is isolated and in thermal equilibrium.&lt;br /&gt;
*如果集合中的子系统确实相互交互，则子系统状态的预期频率不再遵循玻尔兹曼 分布，甚至可能没有解析解。&amp;lt;ref name=&amp;quot;:4&amp;quot; /&amp;gt;然而，如果整个系统是独立的并且处于热平衡状态，则正则系综仍然可以应用于作为一个整体考虑。&lt;br /&gt;
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*With ''[[quantum mechanics|quantum]]'' gases of non-interacting particles in equilibrium, the number of particles found in a given single-particle state does not follow Maxwell–Boltzmann statistics, and there is no simple closed form expression for quantum gases in the canonical ensemble. In the grand canonical ensemble the state-filling statistics of quantum gases are described by [[Fermi–Dirac statistics]] or [[Bose–Einstein statistics]], depending on whether the particles are [[fermion]]s or [[boson]]s respectively.&lt;br /&gt;
*对于处于平衡状态的非相互作用粒子的量子气体，在给定的单粒子状态中发现的粒子数量并不遵循麦克斯韦-玻尔兹曼统计。并且正则系综中的量子气体没有简单的封闭表达式。在巨正则系综中，量子气体的统计分布状态由费米-狄拉克统计或玻色-爱因斯坦统计来描述，具体则取决于该粒子是费米子还是玻色子。&lt;br /&gt;
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==数学==&lt;br /&gt;
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In more general mathematical settings, the Boltzmann distribution is also known as the [[Gibbs measure]]. In statistics and machine learning, it is called a [[log-linear model]]. In [[deep learning]], the Boltzmann distribution is used in the sampling distribution of [[stochastic neural network]]s such as the [[Boltzmann machine]], [[Restricted Boltzmann machine]], [[Energy based model|Energy-Based models]] and [[Deep Boltzmann Machine|deep Boltzmann machine]]&lt;br /&gt;
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在更一般的数学环境中，玻尔兹曼分布也被称为吉布斯量度。在统计学和机器学习中，它被称为对数线性回归。在深度学习中，玻尔兹曼分布被用于随机神经网络的抽样分布，如玻尔兹曼机、受限玻尔兹曼机、基于能量的模型和深度波茨曼机。&lt;br /&gt;
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==经济==&lt;br /&gt;
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The Boltzmann distribution can be introduced to allocate permits in emissions trading.&amp;lt;ref name=&amp;quot;Park, J.-W. 2012&amp;quot;&amp;gt;Park, J.-W., Kim, C. U. and Isard, W. (2012) Permit allocation in emissions trading using the Boltzmann distribution. Physica A 391: 4883–4890&amp;lt;/ref&amp;gt;&amp;lt;ref name=&amp;quot;:5&amp;quot;&amp;gt;[http://www.technologyreview.com/view/425051/the-thorny-problem-of-fair-allocation/ The Thorny Problem Of Fair Allocation]. ''Technology Review'' blog. August 17, 2011. Cites and summarizes Park, Kim and Isard (2012).&amp;lt;/ref&amp;gt; The new allocation method using the Boltzmann distribution can describe the most probable, natural, and unbiased distribution of emissions permits among multiple countries. Simple and versatile, this new method holds potential for many economic and environmental applications.&lt;br /&gt;
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在经济学中，玻尔兹曼分布被用来分配排放交易中的许可。&amp;lt;ref name=&amp;quot;Park, J.-W. 2012&amp;quot; /&amp;gt;&amp;lt;ref name=&amp;quot;:5&amp;quot; /&amp;gt;  使用玻尔兹曼分布的新分配方法可以创造出在多个国家之间最可能的、自然的和无偏见的排放许可分配。这种新方法简单而通用，在经济和环保中有很大的应用潜力。&lt;br /&gt;
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The Boltzmann distribution has the same form as the [[Multinomial logistic regression|multinomial logit]] model. As a [[discrete choice]] model, this is very well known in economics since [[Daniel McFadden]] made the connection to random utility maximization.&lt;br /&gt;
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玻尔兹曼分布与多项逻辑回归模型具有相同的形式。在丹尼尔 · 麦克法登将它与随机效用最大化联系起来之后，成为了大家所熟知的一种离散选择模型。&lt;br /&gt;
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Category:Statistical mechanics&lt;br /&gt;
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类别: 统计力学&lt;br /&gt;
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本中文词条由[[用户:费米子|tueryeye]]编辑，欢迎在讨论页面留言。&lt;br /&gt;
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==See also==&lt;br /&gt;
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Distribution&lt;br /&gt;
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分布&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:Boltzmann distribution]]. Its edit history can be viewed at [[玻尔兹曼分布/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;br /&gt;
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&amp;lt;references /&amp;gt;&lt;/div&gt;</summary>
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&lt;div&gt;此词条暂由tueryeye翻译和审校，翻译字数共1452，带来阅读不便，请见谅。&lt;br /&gt;
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{{Use American English|date = March 2019}}&lt;br /&gt;
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{{Short description|Probability distribution of energy states of a system}}&lt;br /&gt;
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{{about|system energy states|particle energy levels and velocities|Maxwell–Boltzmann distribution}}&lt;br /&gt;
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[[File:Boltzmann distribution graph.svg|upright=1.75|right|thumb|Boltzmann factor ''p&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;''&amp;amp;nbsp;/&amp;amp;nbsp;''p&amp;lt;sub&amp;gt;j&amp;lt;/sub&amp;gt;'' (vertical axis) as a function of temperature ''T'' for several energy differences ''ε&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;''&amp;amp;nbsp;−&amp;amp;nbsp;''ε&amp;lt;sub&amp;gt;j&amp;lt;/sub&amp;gt;''.|链接=Special:FilePath/Boltzmann_distribution_graph.svg]]&lt;br /&gt;
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In [[statistical mechanics]] and [[mathematics]], a '''Boltzmann distribution''' (also called '''Gibbs distribution'''&amp;lt;ref name=&amp;quot;landau&amp;quot;&amp;gt;{{cite book | author=Landau, Lev Davidovich |author2=Lifshitz, Evgeny Mikhailovich |name-list-style=amp | title=Statistical Physics |volume=5 |series=Course of Theoretical Physics |edition=3 |origyear=1976 |year=1980 |place=Oxford |publisher=Pergamon Press|isbn=0-7506-3372-7|author-link=Lev Landau |author2-link=Evgeny Lifshitz }} Translated by J.B. Sykes and M.J. Kearsley. See section 28&amp;lt;/ref&amp;gt;) is a [[probability distribution]] or [[probability measure]] that gives the probability that a system will be in a certain [[microstate (statistical mechanics)|state]] as a function of that state's energy and the temperature of the system. The distribution is expressed in the form:&lt;br /&gt;
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在统计力学和数学中，波兹曼分布分布(也称为吉布斯分布&amp;lt;ref name=&amp;quot;landau&amp;quot; /&amp;gt;)是一个概率分布或机率量测，它给出了一个系统处于某种量子态的概率，这个概率是该状态的能量和系统温度的函数。分布情况以下列形式表示:&lt;br /&gt;
:&amp;lt;math&amp;gt;p_i \propto e^{-\frac{\varepsilon_i}{kT}}&amp;lt;/math&amp;gt; &lt;br /&gt;
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where {{mvar|p&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;}} is the probability of the system being in state {{mvar|i}}, {{mvar|ε&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;}} is the energy of that state, and a constant {{mvar|kT}} of the distribution is the product of [[Boltzmann's constant]] {{mvar|k}} and [[thermodynamic temperature]] {{mvar|T}}. The symbol &amp;lt;math display=&amp;quot;inline&amp;quot;&amp;gt;\propto&amp;lt;/math&amp;gt; denotes [[proportionality (mathematics)|proportionality]] (see {{section link||The distribution}} for the proportionality constant).&lt;br /&gt;
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{{mvar|p&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;}} 是其中系统处于状态{{mvar|i}}的概率, {{mvar|ε&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;}} 是该状态的能量，还有关于这个分布的一个常数 {{mvar|kT}} ，它是玻尔兹曼常数{{mvar|k}}和热力学温度 {{mvar|T}} 的乘积。符号 &amp;lt;math display=&amp;quot;inline&amp;quot;&amp;gt;\propto&amp;lt;/math&amp;gt;表示正比例(见附录中的比例常数)。&lt;br /&gt;
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The term system here has a very wide meaning; it can range from a single atom to a macroscopic system such as a [[Natural gas storage|natural gas storage tank]]. Because of this the Boltzmann distribution can be used to solve a very wide variety of problems. The distribution shows that states with lower energy will always have a higher probability of being occupied .&lt;br /&gt;
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这里的术语系统含义广泛; 它可以从单个原子到宏观系统，如天然气储罐。正因为如此，波兹曼分布可以用来解决各种各样的问题。玻尔兹曼分布表明，能量较低的状态被占据的概率总是较高的。&lt;br /&gt;
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The ''ratio'' of probabilities of two states is known as the '''Boltzmann factor''' and characteristically only depends on the states' energy difference:&lt;br /&gt;
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两种状态的概率之比被称为玻尔兹曼因子，取决于两种状态的能量差:&lt;br /&gt;
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&amp;lt;math&amp;gt;\frac{p_i}{p_j} = e^{\frac{\varepsilon_j - \varepsilon_i}{kT}}&amp;lt;/math&amp;gt;&lt;br /&gt;
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The Boltzmann distribution is named after [[Ludwig Boltzmann]] who first formulated it in 1868 during his studies of the [[statistical mechanics]] of gases in thermal equilibrium. Boltzmann's statistical work is borne out in his paper “On the Relationship between the Second Fundamental Theorem of the Mechanical Theory of Heat and Probability Calculations Regarding the Conditions for Thermal Equilibrium&amp;quot;&amp;lt;ref&amp;gt;http://crystal.med.upenn.edu/sharp-lab-pdfs/2015SharpMatschinsky_Boltz1877_Entropy17.pdf&amp;lt;/ref&amp;gt;&lt;br /&gt;
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波兹曼分布是根据路德维希·玻尔兹曼1868年在研究统计力学中气体热平衡的时候首次提出的一个公式命名的。波尔兹曼的统计工作在他1877年的论文《论热力学第二基本定理与热平衡条件的概率计算之间的关系》中得到了体现。&amp;lt;ref&amp;gt;“On the Relationship between the Second Fundamental Theorem of the Mechanical Theory of Heat and Probability Calculations Regarding the Conditions for Thermal Equilibrium” Sitzungberichte der Kaiserlichen Akademie der Wissenschaften. Mathematisch-Naturwissen Classe. Abt. II, LXXVI 1877, pp 373-435 (Wien. Ber. 1877, 76:373-435). &amp;lt;/ref&amp;gt;&lt;br /&gt;
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The distribution was later investigated extensively, in its modern generic form, by [[Josiah Willard Gibbs]] in 1902.&amp;lt;ref name=&amp;quot;gibbs&amp;quot;&amp;gt;{{cite book |last=Gibbs |first=Josiah Willard |authorlink=Josiah Willard Gibbs |title=Elementary Principles in Statistical Mechanics |year=1902 |publisher=[[Charles Scribner's Sons]] &lt;br /&gt;
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The distribution was later investigated extensively, in its modern generic form, by Josiah Willard Gibbs in 1902.&lt;br /&gt;
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这种分布后来在1902年由约西亚·威拉德·吉布斯进行了广泛的调查，以其现代通用形式。&lt;br /&gt;
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|location=New York|title-link=Elementary Principles in Statistical Mechanics }}&amp;lt;/ref&amp;gt;&lt;br /&gt;
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在玻尔兹曼分布被发明之后，约西亚·华纳德·吉布森充分地研究了它并在1902年提出了它的一般形式。&amp;lt;ref name=&amp;quot;gibbs&amp;quot; /&amp;gt;&lt;br /&gt;
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The generalized Boltzmann distribution is a sufficient and necessary condition for the equivalence between the statistical mechanics definition of [[entropy]] (The [[Entropy_(statistical_thermodynamics)#Gibbs_entropy_formula | Gibbs entropy formula]] &amp;lt;math&amp;gt;S = -k_{\mathrm{B}}\sum_i p_i \log p_i&amp;lt;/math&amp;gt;) and the thermodynamic definition of entropy (&amp;lt;math&amp;gt;d S = \frac{\delta Q_\text{rev}}{T}&amp;lt;/math&amp;gt;, and the [[fundamental thermodynamic relation]]).&amp;lt;ref name=&amp;quot;:0&amp;quot;&amp;gt;{{cite journal |last1= Gao |first1= Xiang |last2= Gallicchio |first2= Emilio |first3= Adrian |last3= Roitberg  |date= 2019 |title= The generalized Boltzmann distribution is the only distribution in which the Gibbs-Shannon entropy equals the thermodynamic entropy |journal= The Journal of Chemical Physics|volume= 151|issue= 3|pages= 034113|doi= 10.1063/1.5111333|pmid= 31325924 |arxiv= 1903.02121 |s2cid= 118981017 }}&amp;lt;/ref&amp;gt;&lt;br /&gt;
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广义波兹曼分布是熵的统计力学定义(吉布斯熵公式  &amp;lt;math&amp;gt;S = -k_{\mathrm{B}}\sum_i p_i \log p_i&amp;lt;/math&amp;gt;))与熵的热力学定义(&amp;lt;math&amp;gt;d S = \frac{\delta Q_\text{rev}}{T}&amp;lt;/math&amp;gt;)等价的充要条件。&amp;lt;ref name=&amp;quot;:0&amp;quot; /&amp;gt;&lt;br /&gt;
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The Boltzmann distribution should not be confused with the [[Maxwell–Boltzmann distribution]]. The former gives the probability that a system will be in a certain state as a function of that state's energy;&amp;lt;ref name=&amp;quot;Atkins, P. W. 2010&amp;quot;&amp;gt;Atkins, P. W. (2010) Quanta, W. H. Freeman and Company, New York&amp;lt;/ref&amp;gt; in contrast, the latter is used to describe particle speeds in idealized gases.&lt;br /&gt;
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值得一提的是，玻尔兹曼分布不应与麦克斯韦-玻尔兹曼分布混淆。前者给出了系统处于某种状态的概率，作为该状态能量的函数; 后者则是用于描述理想气体中的粒子速度。&lt;br /&gt;
==分布==&lt;br /&gt;
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The Boltzmann distribution is a [[probability distribution]] that gives the probability of a certain state as a function of that state's energy and  temperature of the [[system]] to which the distribution is applied.&amp;lt;ref name=&amp;quot;McQuarrie, A. 2000&amp;quot;&amp;gt;McQuarrie, A. (2000) Statistical Mechanics, University Science Books, California&amp;lt;/ref&amp;gt; It is given as&lt;br /&gt;
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波兹曼分布是一个概率分布，它给出了出于某种量子态处于某种能量和温度的时候的概率。它被这样定义：&lt;br /&gt;
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&amp;lt;math&amp;gt;&lt;br /&gt;
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《数学》&lt;br /&gt;
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:&amp;lt;math&amp;gt;&lt;br /&gt;
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p_i=\frac{1}{Q}} {e^{- {\varepsilon}_i / k T}=\frac{e^{- {\varepsilon}_i / k T}}{\sum_{j=1}^{M}{e^{- {\varepsilon}_j / k T}}}&lt;br /&gt;
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P _ i = frac {1}{ q }{ e ^ {-{ varepsilon } _ i/k t } = frac { e ^ {-{ varepsilon } _ i/k t }{ sum { j = 1} ^ { m }{ e ^ {-{ varepsilon } _ j/k t }}}}}&lt;br /&gt;
&lt;br /&gt;
p_i=\frac{1}{Q}} {e^{- {\varepsilon}_i / k T}=\frac{e^{- {\varepsilon}_i / k T}}{\sum_{j=1}^{M}{e^{- {\varepsilon}_j / k T}}}&lt;br /&gt;
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&amp;lt;/math&amp;gt;&lt;br /&gt;
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where ''p&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;'' is the probability of state ''i'', ''ε&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;'' the energy of state ''i'', ''k'' the Boltzmann constant, ''T'' the temperature of the system and ''M'' is the number of all states accessible to the system of interest.&amp;lt;ref name=&amp;quot;McQuarrie, A. 2000&amp;quot; /&amp;gt;&amp;lt;ref name=&amp;quot;Atkins, P. W. 2010&amp;quot; /&amp;gt; Implied parentheses around the denominator ''kT'' are omitted for brevity. The normalization denominator ''Q'' (denoted by some authors by ''Z'') is the [[canonical partition function]]&lt;br /&gt;
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其中 ''p&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;'' 是状态 i 的概率，''ε&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;'' 是状态 i 的能量，''k'' 是波兹曼常数，''T'' 是系统的温度，''M'' 是系统所能到达的所有量子态的数目。&amp;lt;ref name=&amp;quot;Atkins, P. W. 2010&amp;quot; /&amp;gt; &amp;lt;ref name=&amp;quot;McQuarrie, A. 2000&amp;quot; /&amp;gt;这里为了简洁美观，省略了''kT''周围的括弧。归一化的分母''Q''（被有些作者写为''Z''）是对于系统中所有量子态进行总和，此部分又被称为[[Index.php?title=Canonical partition function|正则配分函数]]''。''&lt;br /&gt;
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It results from the constraint that the probabilities of all accessible states must add up to 1.&lt;br /&gt;
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所有量子态的概率之和为1.&lt;br /&gt;
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The Boltzmann distribution is the distribution that maximizes the [[entropy]]，&lt;br /&gt;
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&amp;lt;math&amp;gt;H(p_1,p_2,\cdots,p_M) = -\sum_{i=1}^{M} p_i\log_2 p_i&amp;lt;/math&amp;gt;&lt;br /&gt;
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&amp;lt;nowiki&amp;gt;subject to the constraint that {\sum{p_i {\varepsilon}_i}} equals a particular mean energy value (which can be proven using &amp;lt;/nowiki&amp;gt;[[Lagrange multipliers]]).&lt;br /&gt;
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&amp;lt;nowiki&amp;gt;当 {\sum{p_i {\varepsilon}_i}} 等于平均能量值时，玻尔兹曼分布是这种情况下能让熵最大化的分布。我们可以通过拉格朗日乘数法来证明。&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
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The partition function can be calculated if we know the energies of the states accessible to the system of interest. For atoms the partition function values can be found in the NIST Atomic Spectra Database.&amp;lt;ref name=&amp;quot;:1&amp;quot;&amp;gt;[http://physics.nist.gov/PhysRefData/ASD/levels_form.html NIST Atomic Spectra Database Levels Form] at nist.gov&amp;lt;/ref&amp;gt;&lt;br /&gt;
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在知道量子态能量的情况下，这个配分函数可以被计算。对于原子来说，配分函数的值可以在NIST Atomic Spectra Database中找到。&amp;lt;ref name=&amp;quot;:1&amp;quot; /&amp;gt;&lt;br /&gt;
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The distribution shows that states with lower energy will always have a higher probability of being occupied than the states with higher energy. It can also give us the quantitative relationship between the probabilities of the two states being occupied. The ratio of probabilities for states i and j is given as&lt;br /&gt;
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玻尔兹曼分布指出，能量低的量子态总是有比能量高的量子态更高的概率被粒子占据。它同时也能让我们定量地比较两个量子态分布概率的关系。状态 i 和状态 j 的概率比为&lt;br /&gt;
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:&amp;lt;math&amp;gt;&lt;br /&gt;
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{\frac{p_i}{p_j}}=e^{({\varepsilon}_j-{\varepsilon}_i) / k T}&lt;br /&gt;
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&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
where p&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt; is the probability of state i,  p&amp;lt;sub&amp;gt;j&amp;lt;/sub&amp;gt; the probability of state j, and ε&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt; and ε&amp;lt;sub&amp;gt;j&amp;lt;/sub&amp;gt; are the energies of states i and j, respectively.&lt;br /&gt;
&lt;br /&gt;
其中 p&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt; 是量子态 i 的概率， p&amp;lt;sub&amp;gt;j&amp;lt;/sub&amp;gt; 是量子态 j 的概率，ε&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt; 和 ε&amp;lt;sub&amp;gt;j&amp;lt;/sub&amp;gt; 分别是状态 i 和 j 的能量。&lt;br /&gt;
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&lt;br /&gt;
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The Boltzmann distribution is often used to describe the distribution of particles, such as atoms or molecules, over energy states accessible to them. If we have a system consisting of many particles, the probability of a particle being in state i is practically the probability that, if we pick a random particle from that system and check what state it is in, we will find it is in state i. This probability is equal to the number of particles in state i divided by the total number of particles in the system, that is the fraction of particles that occupy state i.&lt;br /&gt;
&lt;br /&gt;
玻尔兹曼分布通常被用来描述粒子的分布，比如原子或分子，在能量状态上的分布情况。如果我们有一个由许多粒子组成的系统，某个粒子处于量子态 i 的概率就等同于当我们从该系统中选择一个随机的粒子并观察它处于什么状态，发现它处于状态 i 的概率。这个概率等于量子态 i 的粒子数除以系统中粒子的总数，即那些占据量子态i的粒子的比例。&lt;br /&gt;
&lt;br /&gt;
&amp;lt;nowiki&amp;gt;[math]\displaystyle{ {\frac{N_i}{N}}={\frac{e^{- {\varepsilon}_i / k T}}{\sum_{j=1}^{M}{e^{- {\varepsilon}_j / k T}}}} }[/math]&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
&lt;br /&gt;
where N&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt; is the number of particles in state i and N is the total number of particles in the system. We may use the Boltzmann distribution to find this probability that is, as we have seen, equal to the fraction of particles that are in state i. So the equation that gives the fraction of particles in state i as a function of the energy of that state is&lt;br /&gt;
&lt;br /&gt;
N&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt; 是位于量子态 i 的粒子数，N是系统中粒子的总数。我们可以用波兹曼分布来求出这个概率，它等于处于量子态i的粒子的比例。所以这个方程给出位于量子态 i 的粒子比例关于这个状态能量的函数&amp;lt;ref name=&amp;quot;Atkins, P. W. 2010&amp;quot; /&amp;gt;。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
This equation is of great importance to [[spectroscopy]]. In spectroscopy we observe a [[spectral line]] of atoms or molecules that we are interested in going from one state to another.&amp;lt;ref name=&amp;quot;Atkins, P. W. 2010&amp;quot; /&amp;gt;&amp;lt;ref name=&amp;quot;:2&amp;quot;&amp;gt;Atkins, P. W.; de Paula J. (2009) Physical Chemistry, 9th edition, Oxford University Press, Oxford, UK&amp;lt;/ref&amp;gt; In order for this to be possible, there must be some particles in the first state to undergo the transition. We may find that this condition is fulfilled by finding the fraction of particles in the first state. If it is negligible, the transition is very likely not to be observed at the temperature for which the calculation was done. In general, a larger fraction of molecules in the first state means a higher number of transitions to the second state.&amp;lt;ref name=&amp;quot;:3&amp;quot;&amp;gt;Skoog, D. A.; Holler, F. J.; Crouch, S. R. (2006) Principles of Instrumental Analysis, Brooks/Cole, Boston, MA&amp;lt;/ref&amp;gt; This gives a stronger spectral line. However, there are other factors that influence the intensity of a spectral line, such as whether it is caused by an allowed or a [[forbidden transition]]&lt;br /&gt;
&lt;br /&gt;
对于光谱学来说这很重要在。在光谱中，我们期待能观察到一条原子或分子跃迁的谱线。&amp;lt;ref name=&amp;quot;Atkins, P. W. 2010&amp;quot; /&amp;gt;&amp;lt;ref name=&amp;quot;:2&amp;quot; /&amp;gt; 在为了使这成为可能，必须有一些粒子处于第一个量子态，等待着发生跃迁。我们可以通过求第一态粒子的比例来满足这个条件。如果它可以忽略不计，那么在当前计算的温度下，则很难观察到这种跃迁。一般来说，处于第一状态的分子比例越大，意味着向第二状态跃迁的次数越多。&amp;lt;ref name=&amp;quot;:3&amp;quot; /&amp;gt;这就产生了一条更强的谱线。然而，还有其他因素影响谱线的强度，例如它是否是被允许的跃迁还是被禁止的跃迁。&lt;br /&gt;
&lt;br /&gt;
The Boltzmann distribution is related to the [[softmax function]] commonly used in machine learning.&lt;br /&gt;
&lt;br /&gt;
玻尔兹曼分布与机器学习中常用的[[Index.php?title=Softmax function|归一化指数函数]]（Softmax 函数）有关。&lt;br /&gt;
=='''统计力学''' ==&lt;br /&gt;
&lt;br /&gt;
{{main|Canonical ensemble|Maxwell–Boltzmann statistics}}The Boltzmann distribution appears in statistical mechanics when considering isolated (or nearly-isolated) systems of fixed composition that are in thermal equilibrium (equilibrium with respect to energy exchange). The most general case is the probability distribution for the canonical ensemble, but also some special cases (derivable from the canonical ensemble) also show the Boltzmann distribution in different aspects:&lt;br /&gt;
&lt;br /&gt;
当独立的(或者几乎独立的)固定体系处于统计力学热平衡状态时，玻尔兹曼分布就会出现。最普遍的情况是概率分布的正则系综，但也有一些特殊的情况(从正则系综衍生)也显示了不同形式的玻尔兹曼分布:&lt;br /&gt;
&lt;br /&gt;
; [[Canonical ensemble]] (general case)&lt;br /&gt;
; '''正则系综(一般情况)'''&lt;br /&gt;
; '''The [[canonical ensemble]] gives the [[probabilities]] of the various possible states of a closed system of fixed volume, in thermal equilibrium with a [[heat bath]]. The canonical ensemble is a probability distribution with the Boltzmann form.'''&lt;br /&gt;
&lt;br /&gt;
正则系综模型给出了在一个封闭固定体积，带有热浴的热平衡系统中的各种可能状态的概率。我们称正则系综为一个玻尔兹曼概率分布。&lt;br /&gt;
&lt;br /&gt;
; &lt;br /&gt;
; Statistical frequencies of subsystems' states (in a non-interacting collection)&lt;br /&gt;
'''子系统状态的统计频率(在一个无交互的集合中)'''&lt;br /&gt;
: When the system of interest is a collection of many non-interacting copies of a smaller subsystem, it is sometimes useful to find the [[statistical frequency]] of a given subsystem state, among the collection. The canonical ensemble has the property of separability when applied to such a collection: as long as the non-interacting subsystems have fixed composition, then each subsystem's state is independent of the others and is also characterized by a canonical ensemble. As a result, the [[expectation value|expected]] statistical frequency distribution of subsystem states has the Boltzmann form.&lt;br /&gt;
&lt;br /&gt;
当系统是一个较小子系统的许多非交互副本的集合时，有时我们需要在某个子系统集合中找到某个子系统的统计频率。当应用于这样一个集合时，这个子系统的正则系综具有可分离性: 只要不相互作用的子系统的组成是固定的，那么每个子系统的状态都是独立于其他子系统的，它们也拥有自己的正则系综。因此，子系统状态的期望统计频率分布形式是玻尔兹曼分布。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[Maxwell–Boltzmann statistics]] of classical gases (systems of non-interacting particles)&lt;br /&gt;
&lt;br /&gt;
'''Maxwell-Boltzmann 统计中的经典气体系统(非相互作用粒子系统)'''&lt;br /&gt;
&lt;br /&gt;
: In particle systems, many particles share the same space and regularly change places with each other; the single-particle state space they occupy is a shared space. [[Maxwell–Boltzmann statistics]] give the expected number of particles found in a given single-particle state, in a [[classical mechanics|classical]] gas of non-interacting particles at equilibrium. This expected number distribution has the Boltzmann form.&lt;br /&gt;
&lt;br /&gt;
在粒子系统中，许多粒子共享同一空间，并且相互之间有规律地改变位置; 它们所占据的单粒子状态空间是一个共享空间。[[Index.php?title=Maxwell–Boltzmann statistics|麦克斯韦-玻尔兹曼统计]]给出了在一个给定的单粒子态，在一个处于平衡状态的非相互作用粒子的经典气体中所发现的粒子的预期数量。这个预期的数量分布具有玻尔兹曼分布形式。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Although these cases have strong similarities, it is helpful to distinguish them as they generalize in different ways when the crucial assumptions are changed:&lt;br /&gt;
&lt;br /&gt;
虽然这些案例有很多相似之处，但是当关键假设发生变化时，我们需要对它们以不同的方式进行归纳总结，因此区分它们是有帮助的:&lt;br /&gt;
* When a system is in thermodynamic equilibrium with respect to both energy exchange ''and particle exchange'', the requirement of fixed composition is relaxed and a [[grand canonical ensemble]] is obtained rather than canonical ensemble. On the other hand, if both composition and energy are fixed, then a [[microcanonical ensemble]] applies instead.&lt;br /&gt;
* 当一个系统在能量交换和粒子交换方面都处于热力学平衡时，固定组成的要求就放宽了。这时我们就得到了一个[[Index.php?title=Microcanonical ensemble|巨正则系综]]而不是正则系综。另一方面，如果成分和能量都是固定的，则可以使用[[微正则系综Index.php?title=Microcanonical ensemble|微正则系综]]。&lt;br /&gt;
&lt;br /&gt;
* If the subsystems within a collection ''do'' interact with each other, then the expected frequencies of subsystem states no longer follow a Boltzmann distribution, and even may not have an [[analytical solution]].&amp;lt;ref name=&amp;quot;:4&amp;quot;&amp;gt;A classic example of this is [[magnetic ordering]]. Systems of non-interacting [[spin (physics)|spins]] show [[paramagnetic]] behaviour that can be understood with a single-particle canonical ensemble (resulting in the [[Brillouin function]]). Systems of ''interacting'' spins can show much more complex behaviour such as [[ferromagnetism]] or [[antiferromagnetism]].&amp;lt;/ref&amp;gt; The canonical ensemble can however still be applied to the ''collective'' states of the entire system considered as a whole, provided the entire system is isolated and in thermal equilibrium.&lt;br /&gt;
* 如果集合中的子系统确实相互交互，则子系统状态的预期频率不再遵循玻尔兹曼 分布，甚至可能没有解析解。&amp;lt;ref name=&amp;quot;:4&amp;quot; /&amp;gt;然而，如果整个系统是独立的并且处于热平衡状态，则正则系综仍然可以应用于作为一个整体考虑。&lt;br /&gt;
&lt;br /&gt;
* With ''[[quantum mechanics|quantum]]'' gases of non-interacting particles in equilibrium, the number of particles found in a given single-particle state does not follow Maxwell–Boltzmann statistics, and there is no simple closed form expression for quantum gases in the canonical ensemble. In the grand canonical ensemble the state-filling statistics of quantum gases are described by [[Fermi–Dirac statistics]] or [[Bose–Einstein statistics]], depending on whether the particles are [[fermion]]s or [[boson]]s respectively.&lt;br /&gt;
* 对于处于平衡状态的非相互作用粒子的量子气体，在给定的单粒子状态中发现的粒子数量并不遵循麦克斯韦-玻尔兹曼统计。并且正则系综中的量子气体没有简单的封闭表达式。在巨正则系综中，量子气体的统计分布状态由费米-狄拉克统计或玻色-爱因斯坦统计来描述，具体则取决于该粒子是费米子还是玻色子。&lt;br /&gt;
&lt;br /&gt;
== 数学 ==&lt;br /&gt;
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&lt;br /&gt;
In more general mathematical settings, the Boltzmann distribution is also known as the [[Gibbs measure]]. In statistics and machine learning, it is called a [[log-linear model]]. In [[deep learning]], the Boltzmann distribution is used in the sampling distribution of [[stochastic neural network]]s such as the [[Boltzmann machine]], [[Restricted Boltzmann machine]], [[Energy based model|Energy-Based models]] and [[Deep Boltzmann Machine|deep Boltzmann machine]]&lt;br /&gt;
&lt;br /&gt;
在更一般的数学环境中，玻尔兹曼分布也被称为吉布斯量度。在统计学和机器学习中，它被称为对数线性回归。在深度学习中，玻尔兹曼分布被用于随机神经网络的抽样分布，如玻尔兹曼机、受限玻尔兹曼机、基于能量的模型和深度波茨曼机。&lt;br /&gt;
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== 经济 ==&lt;br /&gt;
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The Boltzmann distribution can be introduced to allocate permits in emissions trading.&amp;lt;ref name=&amp;quot;Park, J.-W. 2012&amp;quot;&amp;gt;Park, J.-W., Kim, C. U. and Isard, W. (2012) Permit allocation in emissions trading using the Boltzmann distribution. Physica A 391: 4883–4890&amp;lt;/ref&amp;gt;&amp;lt;ref name=&amp;quot;:5&amp;quot;&amp;gt;[http://www.technologyreview.com/view/425051/the-thorny-problem-of-fair-allocation/ The Thorny Problem Of Fair Allocation]. ''Technology Review'' blog. August 17, 2011. Cites and summarizes Park, Kim and Isard (2012).&amp;lt;/ref&amp;gt; The new allocation method using the Boltzmann distribution can describe the most probable, natural, and unbiased distribution of emissions permits among multiple countries. Simple and versatile, this new method holds potential for many economic and environmental applications.&lt;br /&gt;
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在经济学中，玻尔兹曼分布被用来分配排放交易中的许可。&amp;lt;ref name=&amp;quot;Park, J.-W. 2012&amp;quot; /&amp;gt;&amp;lt;ref name=&amp;quot;:5&amp;quot; /&amp;gt;  使用玻尔兹曼分布的新分配方法可以创造出在多个国家之间最可能的、自然的和无偏见的排放许可分配。这种新方法简单而通用，在经济和环保中有很大的应用潜力。&lt;br /&gt;
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The Boltzmann distribution has the same form as the [[Multinomial logistic regression|multinomial logit]] model. As a [[discrete choice]] model, this is very well known in economics since [[Daniel McFadden]] made the connection to random utility maximization.&lt;br /&gt;
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玻尔兹曼分布与多项逻辑回归模型具有相同的形式。在丹尼尔 · 麦克法登将它与随机效用最大化联系起来之后，成为了大家所熟知的一种离散选择模型。&lt;br /&gt;
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Category:Statistical mechanics&lt;br /&gt;
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类别: 统计力学&lt;br /&gt;
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本中文词条由[[用户:费米子|tueryeye]]编辑，欢迎在讨论页面留言。&lt;br /&gt;
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==See also==&lt;br /&gt;
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Distribution&lt;br /&gt;
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分布&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:Boltzmann distribution]]. Its edit history can be viewed at [[玻尔兹曼分布/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>
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&lt;div&gt;此词条暂由tueryeye翻译和审校，翻译字数共1452，带来阅读不便，请见谅。&lt;br /&gt;
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{{Use American English|date = March 2019}}&lt;br /&gt;
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{{Short description|Probability distribution of energy states of a system}}&lt;br /&gt;
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{{about|system energy states|particle energy levels and velocities|Maxwell–Boltzmann distribution}}&lt;br /&gt;
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[[File:Boltzmann distribution graph.svg|upright=1.75|right|thumb|Boltzmann factor ''p&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;''&amp;amp;nbsp;/&amp;amp;nbsp;''p&amp;lt;sub&amp;gt;j&amp;lt;/sub&amp;gt;'' (vertical axis) as a function of temperature ''T'' for several energy differences ''ε&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;''&amp;amp;nbsp;−&amp;amp;nbsp;''ε&amp;lt;sub&amp;gt;j&amp;lt;/sub&amp;gt;''.|链接=Special:FilePath/Boltzmann_distribution_graph.svg]]&lt;br /&gt;
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In [[statistical mechanics]] and [[mathematics]], a '''Boltzmann distribution''' (also called '''Gibbs distribution'''&amp;lt;ref name=&amp;quot;landau&amp;quot;&amp;gt;{{cite book | author=Landau, Lev Davidovich |author2=Lifshitz, Evgeny Mikhailovich |name-list-style=amp | title=Statistical Physics |volume=5 |series=Course of Theoretical Physics |edition=3 |origyear=1976 |year=1980 |place=Oxford |publisher=Pergamon Press|isbn=0-7506-3372-7|author-link=Lev Landau |author2-link=Evgeny Lifshitz }} Translated by J.B. Sykes and M.J. Kearsley. See section 28&amp;lt;/ref&amp;gt;) is a [[probability distribution]] or [[probability measure]] that gives the probability that a system will be in a certain [[microstate (statistical mechanics)|state]] as a function of that state's energy and the temperature of the system. The distribution is expressed in the form:&lt;br /&gt;
&lt;br /&gt;
在统计力学和数学中，波兹曼分布分布(也称为吉布斯分布&amp;lt;ref name=&amp;quot;landau&amp;quot; /&amp;gt;)是一个概率分布或机率量测，它给出了一个系统处于某种量子态的概率，这个概率是该状态的能量和系统温度的函数。分布情况以下列形式表示:&lt;br /&gt;
:&amp;lt;math&amp;gt;p_i \propto e^{-\frac{\varepsilon_i}{kT}}&amp;lt;/math&amp;gt; &lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
where {{mvar|p&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;}} is the probability of the system being in state {{mvar|i}}, {{mvar|ε&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;}} is the energy of that state, and a constant {{mvar|kT}} of the distribution is the product of [[Boltzmann's constant]] {{mvar|k}} and [[thermodynamic temperature]] {{mvar|T}}. The symbol &amp;lt;math display=&amp;quot;inline&amp;quot;&amp;gt;\propto&amp;lt;/math&amp;gt; denotes [[proportionality (mathematics)|proportionality]] (see {{section link||The distribution}} for the proportionality constant).&lt;br /&gt;
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{{mvar|p&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;}} 是其中系统处于状态{{mvar|i}}的概率, {{mvar|ε&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;}} 是该状态的能量，还有关于这个分布的一个常数 {{mvar|kT}} ，它是玻尔兹曼常数{{mvar|k}}和热力学温度 {{mvar|T}} 的乘积。符号 &amp;lt;math display=&amp;quot;inline&amp;quot;&amp;gt;\propto&amp;lt;/math&amp;gt;表示正比例(见附录中的比例常数)。&lt;br /&gt;
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The term system here has a very wide meaning; it can range from a single atom to a macroscopic system such as a [[Natural gas storage|natural gas storage tank]]. Because of this the Boltzmann distribution can be used to solve a very wide variety of problems. The distribution shows that states with lower energy will always have a higher probability of being occupied .&lt;br /&gt;
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这里的术语系统含义广泛; 它可以从单个原子到宏观系统，如天然气储罐。正因为如此，波兹曼分布可以用来解决各种各样的问题。玻尔兹曼分布表明，能量较低的状态被占据的概率总是较高的。&lt;br /&gt;
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The ''ratio'' of probabilities of two states is known as the '''Boltzmann factor''' and characteristically only depends on the states' energy difference:&lt;br /&gt;
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两种状态的概率之比被称为玻尔兹曼因子，取决于两种状态的能量差:&lt;br /&gt;
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&amp;lt;math&amp;gt;\frac{p_i}{p_j} = e^{\frac{\varepsilon_j - \varepsilon_i}{kT}}&amp;lt;/math&amp;gt;&lt;br /&gt;
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The Boltzmann distribution is named after [[Ludwig Boltzmann]] who first formulated it in 1868 during his studies of the [[statistical mechanics]] of gases in thermal equilibrium. Boltzmann's statistical work is borne out in his paper “On the Relationship between the Second Fundamental Theorem of the Mechanical Theory of Heat and Probability Calculations Regarding the Conditions for Thermal Equilibrium&amp;quot;&amp;lt;ref&amp;gt;http://crystal.med.upenn.edu/sharp-lab-pdfs/2015SharpMatschinsky_Boltz1877_Entropy17.pdf&amp;lt;/ref&amp;gt;&lt;br /&gt;
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波兹曼分布是根据路德维希·玻尔兹曼1868年在研究统计力学中气体热平衡的时候首次提出的一个公式命名的。波尔兹曼的统计工作在他1877年的论文《论热力学第二基本定理与热平衡条件的概率计算之间的关系》中得到了体现。&amp;lt;ref&amp;gt;“On the Relationship between the Second Fundamental Theorem of the Mechanical Theory of Heat and Probability Calculations Regarding the Conditions for Thermal Equilibrium” Sitzungberichte der Kaiserlichen Akademie der Wissenschaften. Mathematisch-Naturwissen Classe. Abt. II, LXXVI 1877, pp 373-435 (Wien. Ber. 1877, 76:373-435). &amp;lt;/ref&amp;gt;&lt;br /&gt;
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The distribution was later investigated extensively, in its modern generic form, by [[Josiah Willard Gibbs]] in 1902.&amp;lt;ref name=&amp;quot;gibbs&amp;quot;&amp;gt;{{cite book |last=Gibbs |first=Josiah Willard |authorlink=Josiah Willard Gibbs |title=Elementary Principles in Statistical Mechanics |year=1902 |publisher=[[Charles Scribner's Sons]] &lt;br /&gt;
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The distribution was later investigated extensively, in its modern generic form, by Josiah Willard Gibbs in 1902.&lt;br /&gt;
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这种分布后来在1902年由约西亚·威拉德·吉布斯进行了广泛的调查，以其现代通用形式。&lt;br /&gt;
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|location=New York|title-link=Elementary Principles in Statistical Mechanics }}&amp;lt;/ref&amp;gt;&lt;br /&gt;
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在玻尔兹曼分布被发明之后，约西亚·华纳德·吉布森充分地研究了它并在1902年提出了它的一般形式。&amp;lt;ref name=&amp;quot;gibbs&amp;quot; /&amp;gt;&lt;br /&gt;
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The generalized Boltzmann distribution is a sufficient and necessary condition for the equivalence between the statistical mechanics definition of [[entropy]] (The [[Entropy_(statistical_thermodynamics)#Gibbs_entropy_formula | Gibbs entropy formula]] &amp;lt;math&amp;gt;S = -k_{\mathrm{B}}\sum_i p_i \log p_i&amp;lt;/math&amp;gt;) and the thermodynamic definition of entropy (&amp;lt;math&amp;gt;d S = \frac{\delta Q_\text{rev}}{T}&amp;lt;/math&amp;gt;, and the [[fundamental thermodynamic relation]]).&amp;lt;ref name=&amp;quot;:0&amp;quot;&amp;gt;{{cite journal |last1= Gao |first1= Xiang |last2= Gallicchio |first2= Emilio |first3= Adrian |last3= Roitberg  |date= 2019 |title= The generalized Boltzmann distribution is the only distribution in which the Gibbs-Shannon entropy equals the thermodynamic entropy |journal= The Journal of Chemical Physics|volume= 151|issue= 3|pages= 034113|doi= 10.1063/1.5111333|pmid= 31325924 |arxiv= 1903.02121 |s2cid= 118981017 }}&amp;lt;/ref&amp;gt;&lt;br /&gt;
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广义波兹曼分布是熵的统计力学定义(吉布斯熵公式  &amp;lt;math&amp;gt;S = -k_{\mathrm{B}}\sum_i p_i \log p_i&amp;lt;/math&amp;gt;))与熵的热力学定义(&amp;lt;math&amp;gt;d S = \frac{\delta Q_\text{rev}}{T}&amp;lt;/math&amp;gt;)等价的充要条件。&amp;lt;ref name=&amp;quot;:0&amp;quot; /&amp;gt;&lt;br /&gt;
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The Boltzmann distribution should not be confused with the [[Maxwell–Boltzmann distribution]]. The former gives the probability that a system will be in a certain state as a function of that state's energy;&amp;lt;ref name=&amp;quot;Atkins, P. W. 2010&amp;quot;&amp;gt;Atkins, P. W. (2010) Quanta, W. H. Freeman and Company, New York&amp;lt;/ref&amp;gt; in contrast, the latter is used to describe particle speeds in idealized gases.&lt;br /&gt;
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值得一提的是，玻尔兹曼分布不应与麦克斯韦-玻尔兹曼分布混淆。前者给出了系统处于某种状态的概率，作为该状态能量的函数; 后者则是用于描述理想气体中的粒子速度。&lt;br /&gt;
==分布==&lt;br /&gt;
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The Boltzmann distribution is a [[probability distribution]] that gives the probability of a certain state as a function of that state's energy and  temperature of the [[system]] to which the distribution is applied.&amp;lt;ref name=&amp;quot;McQuarrie, A. 2000&amp;quot;&amp;gt;McQuarrie, A. (2000) Statistical Mechanics, University Science Books, California&amp;lt;/ref&amp;gt; It is given as&lt;br /&gt;
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波兹曼分布是一个概率分布，它给出了出于某种量子态处于某种能量和温度的时候的概率。它被这样定义：&lt;br /&gt;
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&amp;lt;math&amp;gt;&lt;br /&gt;
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《数学》&lt;br /&gt;
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:&amp;lt;math&amp;gt;&lt;br /&gt;
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p_i=\frac{1}{Q}} {e^{- {\varepsilon}_i / k T}=\frac{e^{- {\varepsilon}_i / k T}}{\sum_{j=1}^{M}{e^{- {\varepsilon}_j / k T}}}&lt;br /&gt;
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P _ i = frac {1}{ q }{ e ^ {-{ varepsilon } _ i/k t } = frac { e ^ {-{ varepsilon } _ i/k t }{ sum { j = 1} ^ { m }{ e ^ {-{ varepsilon } _ j/k t }}}}}&lt;br /&gt;
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p_i=\frac{1}{Q}} {e^{- {\varepsilon}_i / k T}=\frac{e^{- {\varepsilon}_i / k T}}{\sum_{j=1}^{M}{e^{- {\varepsilon}_j / k T}}}&lt;br /&gt;
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&amp;lt;/math&amp;gt;&lt;br /&gt;
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where ''p&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;'' is the probability of state ''i'', ''ε&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;'' the energy of state ''i'', ''k'' the Boltzmann constant, ''T'' the temperature of the system and ''M'' is the number of all states accessible to the system of interest.&amp;lt;ref name=&amp;quot;McQuarrie, A. 2000&amp;quot; /&amp;gt;&amp;lt;ref name=&amp;quot;Atkins, P. W. 2010&amp;quot; /&amp;gt; Implied parentheses around the denominator ''kT'' are omitted for brevity. The normalization denominator ''Q'' (denoted by some authors by ''Z'') is the [[canonical partition function]]&lt;br /&gt;
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其中 ''p&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;'' 是状态 i 的概率，''ε&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;'' 是状态 i 的能量，''k'' 是波兹曼常数，''T'' 是系统的温度，''M'' 是系统所能到达的所有量子态的数目。&amp;lt;ref name=&amp;quot;Atkins, P. W. 2010&amp;quot; /&amp;gt; &amp;lt;ref name=&amp;quot;McQuarrie, A. 2000&amp;quot; /&amp;gt;这里为了简洁美观，省略了''kT''周围的括弧。归一化的分母''Q''（被有些作者写为''Z''）是对于系统中所有量子态进行总和，此部分又被称为[[Index.php?title=Canonical partition function|正则配分函数]]''。''&lt;br /&gt;
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It results from the constraint that the probabilities of all accessible states must add up to 1.&lt;br /&gt;
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所有量子态的概率之和为1.&lt;br /&gt;
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The Boltzmann distribution is the distribution that maximizes the [[entropy]]，&lt;br /&gt;
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&amp;lt;math&amp;gt;H(p_1,p_2,\cdots,p_M) = -\sum_{i=1}^{M} p_i\log_2 p_i&amp;lt;/math&amp;gt;&lt;br /&gt;
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&amp;lt;nowiki&amp;gt;subject to the constraint that {\sum{p_i {\varepsilon}_i}} equals a particular mean energy value (which can be proven using &amp;lt;/nowiki&amp;gt;[[Lagrange multipliers]]).&lt;br /&gt;
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&amp;lt;nowiki&amp;gt;当 {\sum{p_i {\varepsilon}_i}} 等于平均能量值时，玻尔兹曼分布是这种情况下能让熵最大化的分布。我们可以通过拉格朗日乘数法来证明。&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
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The partition function can be calculated if we know the energies of the states accessible to the system of interest. For atoms the partition function values can be found in the NIST Atomic Spectra Database.&amp;lt;ref name=&amp;quot;:1&amp;quot;&amp;gt;[http://physics.nist.gov/PhysRefData/ASD/levels_form.html NIST Atomic Spectra Database Levels Form] at nist.gov&amp;lt;/ref&amp;gt;&lt;br /&gt;
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在知道量子态能量的情况下，这个配分函数可以被计算。对于原子来说，配分函数的值可以在NIST Atomic Spectra Database中找到。&amp;lt;ref name=&amp;quot;:1&amp;quot; /&amp;gt;&lt;br /&gt;
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The distribution shows that states with lower energy will always have a higher probability of being occupied than the states with higher energy. It can also give us the quantitative relationship between the probabilities of the two states being occupied. The ratio of probabilities for states i and j is given as&lt;br /&gt;
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玻尔兹曼分布指出，能量低的量子态总是有比能量高的量子态更高的概率被粒子占据。它同时也能让我们定量地比较两个量子态分布概率的关系。状态 i 和状态 j 的概率比为&lt;br /&gt;
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:&amp;lt;math&amp;gt;&lt;br /&gt;
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{\frac{p_i}{p_j}}=e^{({\varepsilon}_j-{\varepsilon}_i) / k T}&lt;br /&gt;
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&amp;lt;/math&amp;gt;&lt;br /&gt;
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where p&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt; is the probability of state i,  p&amp;lt;sub&amp;gt;j&amp;lt;/sub&amp;gt; the probability of state j, and ε&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt; and ε&amp;lt;sub&amp;gt;j&amp;lt;/sub&amp;gt; are the energies of states i and j, respectively.&lt;br /&gt;
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其中 p&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt; 是量子态 i 的概率， p&amp;lt;sub&amp;gt;j&amp;lt;/sub&amp;gt; 是量子态 j 的概率，ε&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt; 和 ε&amp;lt;sub&amp;gt;j&amp;lt;/sub&amp;gt; 分别是状态 i 和 j 的能量。&lt;br /&gt;
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The Boltzmann distribution is often used to describe the distribution of particles, such as atoms or molecules, over energy states accessible to them. If we have a system consisting of many particles, the probability of a particle being in state i is practically the probability that, if we pick a random particle from that system and check what state it is in, we will find it is in state i. This probability is equal to the number of particles in state i divided by the total number of particles in the system, that is the fraction of particles that occupy state i.&lt;br /&gt;
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玻尔兹曼分布通常被用来描述粒子的分布，比如原子或分子，在能量状态上的分布情况。如果我们有一个由许多粒子组成的系统，某个粒子处于量子态 i 的概率就等同于当我们从该系统中选择一个随机的粒子并观察它处于什么状态，发现它处于状态 i 的概率。这个概率等于量子态 i 的粒子数除以系统中粒子的总数，即那些占据量子态i的粒子的比例。&lt;br /&gt;
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&amp;lt;nowiki&amp;gt;&amp;lt;math display=&amp;quot;inline&amp;quot;&amp;gt;&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
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&amp;lt;nowiki&amp;gt;p_i={\frac{N_i}{N}}&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
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P _ i = { frac { n _ i }{ n }&lt;br /&gt;
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&amp;lt;nowiki&amp;gt;{\sum{p_i {\varepsilon}_i}}&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
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where N&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt; is the number of particles in state i and N is the total number of particles in the system. We may use the Boltzmann distribution to find this probability that is, as we have seen, equal to the fraction of particles that are in state i. So the equation that gives the fraction of particles in state i as a function of the energy of that state is&lt;br /&gt;
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&amp;lt;nowiki&amp;gt;&amp;lt;/math&amp;gt;&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
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《数学公式丢失了》&lt;br /&gt;
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N&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt; 是位于量子态 i 的粒子数，N是系统中粒子的总数。我们可以用波兹曼分布来求出这个概率，它等于处于量子态i的粒子的比例。所以这个方程给出位于量子态 i 的粒子比例关于这个状态能量的函数&amp;lt;ref name=&amp;quot;Atkins, P. W. 2010&amp;quot; /&amp;gt;。&lt;br /&gt;
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This equation is of great importance to [[spectroscopy]]. In spectroscopy we observe a [[spectral line]] of atoms or molecules that we are interested in going from one state to another.&amp;lt;ref name=&amp;quot;Atkins, P. W. 2010&amp;quot; /&amp;gt;&amp;lt;ref name=&amp;quot;:2&amp;quot;&amp;gt;Atkins, P. W.; de Paula J. (2009) Physical Chemistry, 9th edition, Oxford University Press, Oxford, UK&amp;lt;/ref&amp;gt; In order for this to be possible, there must be some particles in the first state to undergo the transition. We may find that this condition is fulfilled by finding the fraction of particles in the first state. If it is negligible, the transition is very likely not to be observed at the temperature for which the calculation was done. In general, a larger fraction of molecules in the first state means a higher number of transitions to the second state.&amp;lt;ref name=&amp;quot;:3&amp;quot;&amp;gt;Skoog, D. A.; Holler, F. J.; Crouch, S. R. (2006) Principles of Instrumental Analysis, Brooks/Cole, Boston, MA&amp;lt;/ref&amp;gt; This gives a stronger spectral line. However, there are other factors that influence the intensity of a spectral line, such as whether it is caused by an allowed or a [[forbidden transition]]&lt;br /&gt;
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对于光谱学来说这很重要在。在光谱中，我们期待能观察到一条原子或分子跃迁的谱线。&amp;lt;ref name=&amp;quot;Atkins, P. W. 2010&amp;quot; /&amp;gt;&amp;lt;ref name=&amp;quot;:2&amp;quot; /&amp;gt; 在为了使这成为可能，必须有一些粒子处于第一个量子态，等待着发生跃迁。我们可以通过求第一态粒子的比例来满足这个条件。如果它可以忽略不计，那么在当前计算的温度下，则很难观察到这种跃迁。一般来说，处于第一状态的分子比例越大，意味着向第二状态跃迁的次数越多。&amp;lt;ref name=&amp;quot;:3&amp;quot; /&amp;gt;这就产生了一条更强的谱线。然而，还有其他因素影响谱线的强度，例如它是否是被允许的跃迁还是被禁止的跃迁。&lt;br /&gt;
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The Boltzmann distribution is related to the [[softmax function]] commonly used in machine learning.&lt;br /&gt;
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玻尔兹曼分布与机器学习中常用的[[Index.php?title=Softmax function|归一化指数函数]]（Softmax 函数）有关。&lt;br /&gt;
=='''统计力学''' ==&lt;br /&gt;
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{{main|Canonical ensemble|Maxwell–Boltzmann statistics}}The Boltzmann distribution appears in statistical mechanics when considering isolated (or nearly-isolated) systems of fixed composition that are in thermal equilibrium (equilibrium with respect to energy exchange). The most general case is the probability distribution for the canonical ensemble, but also some special cases (derivable from the canonical ensemble) also show the Boltzmann distribution in different aspects:&lt;br /&gt;
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当独立的(或者几乎独立的)固定体系处于统计力学热平衡状态时，玻尔兹曼分布就会出现。最普遍的情况是概率分布的正则系综，但也有一些特殊的情况(从正则系综衍生)也显示了不同形式的玻尔兹曼分布:&lt;br /&gt;
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; [[Canonical ensemble]] (general case)&lt;br /&gt;
; '''正则系综(一般情况)'''&lt;br /&gt;
; '''The [[canonical ensemble]] gives the [[probabilities]] of the various possible states of a closed system of fixed volume, in thermal equilibrium with a [[heat bath]]. The canonical ensemble is a probability distribution with the Boltzmann form.'''&lt;br /&gt;
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正则系综模型给出了在一个封闭固定体积，带有热浴的热平衡系统中的各种可能状态的概率。我们称正则系综为一个玻尔兹曼概率分布。&lt;br /&gt;
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; &lt;br /&gt;
; Statistical frequencies of subsystems' states (in a non-interacting collection)&lt;br /&gt;
'''子系统状态的统计频率(在一个无交互的集合中)'''&lt;br /&gt;
: When the system of interest is a collection of many non-interacting copies of a smaller subsystem, it is sometimes useful to find the [[statistical frequency]] of a given subsystem state, among the collection. The canonical ensemble has the property of separability when applied to such a collection: as long as the non-interacting subsystems have fixed composition, then each subsystem's state is independent of the others and is also characterized by a canonical ensemble. As a result, the [[expectation value|expected]] statistical frequency distribution of subsystem states has the Boltzmann form.&lt;br /&gt;
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当系统是一个较小子系统的许多非交互副本的集合时，有时我们需要在某个子系统集合中找到某个子系统的统计频率。当应用于这样一个集合时，这个子系统的正则系综具有可分离性: 只要不相互作用的子系统的组成是固定的，那么每个子系统的状态都是独立于其他子系统的，它们也拥有自己的正则系综。因此，子系统状态的期望统计频率分布形式是玻尔兹曼分布。&lt;br /&gt;
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[[Maxwell–Boltzmann statistics]] of classical gases (systems of non-interacting particles)&lt;br /&gt;
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'''Maxwell-Boltzmann 统计中的经典气体系统(非相互作用粒子系统)'''&lt;br /&gt;
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: In particle systems, many particles share the same space and regularly change places with each other; the single-particle state space they occupy is a shared space. [[Maxwell–Boltzmann statistics]] give the expected number of particles found in a given single-particle state, in a [[classical mechanics|classical]] gas of non-interacting particles at equilibrium. This expected number distribution has the Boltzmann form.&lt;br /&gt;
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在粒子系统中，许多粒子共享同一空间，并且相互之间有规律地改变位置; 它们所占据的单粒子状态空间是一个共享空间。[[Index.php?title=Maxwell–Boltzmann statistics|麦克斯韦-玻尔兹曼统计]]给出了在一个给定的单粒子态，在一个处于平衡状态的非相互作用粒子的经典气体中所发现的粒子的预期数量。这个预期的数量分布具有玻尔兹曼分布形式。&lt;br /&gt;
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Although these cases have strong similarities, it is helpful to distinguish them as they generalize in different ways when the crucial assumptions are changed:&lt;br /&gt;
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虽然这些案例有很多相似之处，但是当关键假设发生变化时，我们需要对它们以不同的方式进行归纳总结，因此区分它们是有帮助的:&lt;br /&gt;
* When a system is in thermodynamic equilibrium with respect to both energy exchange ''and particle exchange'', the requirement of fixed composition is relaxed and a [[grand canonical ensemble]] is obtained rather than canonical ensemble. On the other hand, if both composition and energy are fixed, then a [[microcanonical ensemble]] applies instead.&lt;br /&gt;
* 当一个系统在能量交换和粒子交换方面都处于热力学平衡时，固定组成的要求就放宽了。这时我们就得到了一个[[Index.php?title=Microcanonical ensemble|巨正则系综]]而不是正则系综。另一方面，如果成分和能量都是固定的，则可以使用[[微正则系综Index.php?title=Microcanonical ensemble|微正则系综]]。&lt;br /&gt;
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* If the subsystems within a collection ''do'' interact with each other, then the expected frequencies of subsystem states no longer follow a Boltzmann distribution, and even may not have an [[analytical solution]].&amp;lt;ref name=&amp;quot;:4&amp;quot;&amp;gt;A classic example of this is [[magnetic ordering]]. Systems of non-interacting [[spin (physics)|spins]] show [[paramagnetic]] behaviour that can be understood with a single-particle canonical ensemble (resulting in the [[Brillouin function]]). Systems of ''interacting'' spins can show much more complex behaviour such as [[ferromagnetism]] or [[antiferromagnetism]].&amp;lt;/ref&amp;gt; The canonical ensemble can however still be applied to the ''collective'' states of the entire system considered as a whole, provided the entire system is isolated and in thermal equilibrium.&lt;br /&gt;
* 如果集合中的子系统确实相互交互，则子系统状态的预期频率不再遵循玻尔兹曼 分布，甚至可能没有解析解。&amp;lt;ref name=&amp;quot;:4&amp;quot; /&amp;gt;然而，如果整个系统是独立的并且处于热平衡状态，则正则系综仍然可以应用于作为一个整体考虑。&lt;br /&gt;
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* With ''[[quantum mechanics|quantum]]'' gases of non-interacting particles in equilibrium, the number of particles found in a given single-particle state does not follow Maxwell–Boltzmann statistics, and there is no simple closed form expression for quantum gases in the canonical ensemble. In the grand canonical ensemble the state-filling statistics of quantum gases are described by [[Fermi–Dirac statistics]] or [[Bose–Einstein statistics]], depending on whether the particles are [[fermion]]s or [[boson]]s respectively.&lt;br /&gt;
* 对于处于平衡状态的非相互作用粒子的量子气体，在给定的单粒子状态中发现的粒子数量并不遵循麦克斯韦-玻尔兹曼统计。并且正则系综中的量子气体没有简单的封闭表达式。在巨正则系综中，量子气体的统计分布状态由费米-狄拉克统计或玻色-爱因斯坦统计来描述，具体则取决于该粒子是费米子还是玻色子。&lt;br /&gt;
&lt;br /&gt;
== 数学 ==&lt;br /&gt;
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In more general mathematical settings, the Boltzmann distribution is also known as the [[Gibbs measure]]. In statistics and machine learning, it is called a [[log-linear model]]. In [[deep learning]], the Boltzmann distribution is used in the sampling distribution of [[stochastic neural network]]s such as the [[Boltzmann machine]], [[Restricted Boltzmann machine]], [[Energy based model|Energy-Based models]] and [[Deep Boltzmann Machine|deep Boltzmann machine]]&lt;br /&gt;
&lt;br /&gt;
在更一般的数学环境中，玻尔兹曼分布也被称为吉布斯量度。在统计学和机器学习中，它被称为对数线性回归。在深度学习中，玻尔兹曼分布被用于随机神经网络的抽样分布，如玻尔兹曼机、受限玻尔兹曼机、基于能量的模型和深度波茨曼机。&lt;br /&gt;
&lt;br /&gt;
== 经济 ==&lt;br /&gt;
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The Boltzmann distribution can be introduced to allocate permits in emissions trading.&amp;lt;ref name=&amp;quot;Park, J.-W. 2012&amp;quot;&amp;gt;Park, J.-W., Kim, C. U. and Isard, W. (2012) Permit allocation in emissions trading using the Boltzmann distribution. Physica A 391: 4883–4890&amp;lt;/ref&amp;gt;&amp;lt;ref name=&amp;quot;:5&amp;quot;&amp;gt;[http://www.technologyreview.com/view/425051/the-thorny-problem-of-fair-allocation/ The Thorny Problem Of Fair Allocation]. ''Technology Review'' blog. August 17, 2011. Cites and summarizes Park, Kim and Isard (2012).&amp;lt;/ref&amp;gt; The new allocation method using the Boltzmann distribution can describe the most probable, natural, and unbiased distribution of emissions permits among multiple countries. Simple and versatile, this new method holds potential for many economic and environmental applications.&lt;br /&gt;
&lt;br /&gt;
在经济学中，玻尔兹曼分布被用来分配排放交易中的许可。&amp;lt;ref name=&amp;quot;Park, J.-W. 2012&amp;quot; /&amp;gt;&amp;lt;ref name=&amp;quot;:5&amp;quot; /&amp;gt;  使用玻尔兹曼分布的新分配方法可以创造出在多个国家之间最可能的、自然的和无偏见的排放许可分配。这种新方法简单而通用，在经济和环保中有很大的应用潜力。&lt;br /&gt;
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The Boltzmann distribution has the same form as the [[Multinomial logistic regression|multinomial logit]] model. As a [[discrete choice]] model, this is very well known in economics since [[Daniel McFadden]] made the connection to random utility maximization.&lt;br /&gt;
&lt;br /&gt;
玻尔兹曼分布与多项逻辑回归模型具有相同的形式。在丹尼尔 · 麦克法登将它与随机效用最大化联系起来之后，成为了大家所熟知的一种离散选择模型。&lt;br /&gt;
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Category:Statistical mechanics&lt;br /&gt;
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类别: 统计力学&lt;br /&gt;
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本中文词条由[[用户:费米子|tueryeye]]编辑，欢迎在讨论页面留言。&lt;br /&gt;
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==See also==&lt;br /&gt;
&lt;br /&gt;
Distribution&lt;br /&gt;
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分布&lt;br /&gt;
&lt;br /&gt;
&amp;lt;noinclude&amp;gt;&lt;br /&gt;
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&amp;lt;small&amp;gt;This page was moved from [[wikipedia:en:Boltzmann distribution]]. Its edit history can be viewed at [[玻尔兹曼分布/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>
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		<title>玻尔兹曼分布</title>
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		<updated>2021-10-20T05:23:02Z</updated>

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&lt;div&gt;此词条暂由tueryeye翻译和审校，翻译字数共1452，带来阅读不便，请见谅。&lt;br /&gt;
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{{Use American English|date = March 2019}}&lt;br /&gt;
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{{Short description|Probability distribution of energy states of a system}}&lt;br /&gt;
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{{about|system energy states|particle energy levels and velocities|Maxwell–Boltzmann distribution}}&lt;br /&gt;
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[[File:Boltzmann distribution graph.svg|upright=1.75|right|thumb|Boltzmann factor ''p&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;''&amp;amp;nbsp;/&amp;amp;nbsp;''p&amp;lt;sub&amp;gt;j&amp;lt;/sub&amp;gt;'' (vertical axis) as a function of temperature ''T'' for several energy differences ''ε&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;''&amp;amp;nbsp;−&amp;amp;nbsp;''ε&amp;lt;sub&amp;gt;j&amp;lt;/sub&amp;gt;''.|链接=Special:FilePath/Boltzmann_distribution_graph.svg]]&lt;br /&gt;
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In [[statistical mechanics]] and [[mathematics]], a '''Boltzmann distribution''' (also called '''Gibbs distribution'''&amp;lt;ref name=&amp;quot;landau&amp;quot;&amp;gt;{{cite book | author=Landau, Lev Davidovich |author2=Lifshitz, Evgeny Mikhailovich |name-list-style=amp | title=Statistical Physics |volume=5 |series=Course of Theoretical Physics |edition=3 |origyear=1976 |year=1980 |place=Oxford |publisher=Pergamon Press|isbn=0-7506-3372-7|author-link=Lev Landau |author2-link=Evgeny Lifshitz }} Translated by J.B. Sykes and M.J. Kearsley. See section 28&amp;lt;/ref&amp;gt;) is a [[probability distribution]] or [[probability measure]] that gives the probability that a system will be in a certain [[microstate (statistical mechanics)|state]] as a function of that state's energy and the temperature of the system. The distribution is expressed in the form:&lt;br /&gt;
&lt;br /&gt;
在统计力学和数学中，波兹曼分布分布(也称为吉布斯分布&amp;lt;ref name=&amp;quot;landau&amp;quot; /&amp;gt;)是一个概率分布或机率量测，它给出了一个系统处于某种量子态的概率，这个概率是该状态的能量和系统温度的函数。分布情况以下列形式表示:&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt;p_i \propto e^{-\frac{\varepsilon_i}{kT}}&amp;lt;/math&amp;gt; &lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt;p_i \propto e^{-\frac{\varepsilon_i}{kT}}&amp;lt;/math&amp;gt; &lt;br /&gt;
&lt;br /&gt;
[拉丁语]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
where {{mvar|p&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;}} is the probability of the system being in state {{mvar|i}}, {{mvar|ε&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;}} is the energy of that state, and a constant {{mvar|kT}} of the distribution is the product of [[Boltzmann's constant]] {{mvar|k}} and [[thermodynamic temperature]] {{mvar|T}}. The symbol &amp;lt;math display=&amp;quot;inline&amp;quot;&amp;gt;\propto&amp;lt;/math&amp;gt; denotes [[proportionality (mathematics)|proportionality]] (see {{section link||The distribution}} for the proportionality constant).&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{{mvar|p&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;}} 是其中系统处于状态{{mvar|i}}的概率, {{mvar|ε&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;}} 是该状态的能量，还有关于这个分布的一个常数 {{mvar|kT}} ，它是玻尔兹曼常数{{mvar|k}}和热力学温度 {{mvar|T}} 的乘积。符号 &amp;lt;math display=&amp;quot;inline&amp;quot;&amp;gt;\propto&amp;lt;/math&amp;gt;表示正比例(见附录中的比例常数)。&lt;br /&gt;
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The term system here has a very wide meaning; it can range from a single atom to a macroscopic system such as a [[Natural gas storage|natural gas storage tank]]. Because of this the Boltzmann distribution can be used to solve a very wide variety of problems. The distribution shows that states with lower energy will always have a higher probability of being occupied .&lt;br /&gt;
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这里的术语系统含义广泛; 它可以从单个原子到宏观系统，如天然气储罐。正因为如此，波兹曼分布可以用来解决各种各样的问题。玻尔兹曼分布表明，能量较低的状态被占据的概率总是较高的。&lt;br /&gt;
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The ''ratio'' of probabilities of two states is known as the '''Boltzmann factor''' and characteristically only depends on the states' energy difference:&lt;br /&gt;
&lt;br /&gt;
两种状态的概率之比被称为玻尔兹曼因子，取决于两种状态的能量差:&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt;\frac{p_i}{p_j} = e^{\frac{\varepsilon_j - \varepsilon_i}{kT}}&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[数学][数学]&lt;br /&gt;
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The Boltzmann distribution is named after [[Ludwig Boltzmann]] who first formulated it in 1868 during his studies of the [[statistical mechanics]] of gases in thermal equilibrium. Boltzmann's statistical work is borne out in his paper “On the Relationship between the Second Fundamental Theorem of the Mechanical Theory of Heat and Probability Calculations Regarding the Conditions for Thermal Equilibrium&amp;quot;&amp;lt;ref&amp;gt;http://crystal.med.upenn.edu/sharp-lab-pdfs/2015SharpMatschinsky_Boltz1877_Entropy17.pdf&amp;lt;/ref&amp;gt;&lt;br /&gt;
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波兹曼分布是根据路德维希·玻尔兹曼1868年在研究统计力学中气体热平衡的时候首次提出的一个公式命名的。波尔兹曼的统计工作在他1877年的论文《论热力学第二基本定理与热平衡条件的概率计算之间的关系》中得到了体现。&amp;lt;ref&amp;gt;“On the Relationship between the Second Fundamental Theorem of the Mechanical Theory of Heat and Probability Calculations Regarding the Conditions for Thermal Equilibrium” Sitzungberichte der Kaiserlichen Akademie der Wissenschaften. Mathematisch-Naturwissen Classe. Abt. II, LXXVI 1877, pp 373-435 (Wien. Ber. 1877, 76:373-435). &amp;lt;/ref&amp;gt;&lt;br /&gt;
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&lt;br /&gt;
&amp;lt;!--&lt;br /&gt;
&lt;br /&gt;
&amp;lt;!--&lt;br /&gt;
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&amp;lt;!--&lt;br /&gt;
&lt;br /&gt;
  It would be nice to have a citation here! The origin of the Boltzmann factor isn't entirely clear. According to some authors, Boltzmann's 1968 paper “On the Relationship between the Second Fundamental Theorem of the Mechanical Theory of Heat and Probability Calculations Regarding the Conditions for Thermal Equilibrium”&lt;br /&gt;
&lt;br /&gt;
  It would be nice to have a citation here! The origin of the Boltzmann factor isn't entirely clear. According to some authors, Boltzmann's 1968 paper “On the Relationship between the Second Fundamental Theorem of the Mechanical Theory of Heat and Probability Calculations Regarding the Conditions for Thermal Equilibrium”&lt;br /&gt;
&lt;br /&gt;
如果能在这里引用一下就好了！玻尔兹曼因子的起源并不完全清楚。根据一些作者的说法，Boltzmann 在1968年发表的论文《论热力学第二基本定理与热平衡条件的概率计算之间的关系》&lt;br /&gt;
&lt;br /&gt;
  &amp;quot;Studien über das Gleichgewicht der lebendigen Kraft zwischen bewegten materiellen Punkten&amp;quot; is the origin but I can't find this article at the moment,&lt;br /&gt;
&lt;br /&gt;
  &amp;quot;Studien über das Gleichgewicht der lebendigen Kraft zwischen bewegten materiellen Punkten&amp;quot; is the origin but I can't find this article at the moment,&lt;br /&gt;
&lt;br /&gt;
  &amp;quot;Studien über das Gleichgewicht der lebendigen Kraft zwischen bewegten materiellen Punkten&amp;quot; is the origin but I can't find this article at the moment,&lt;br /&gt;
&lt;br /&gt;
  so I cannot confirm.&lt;br /&gt;
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  so I cannot confirm.&lt;br /&gt;
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所以我不能确定。&lt;br /&gt;
&lt;br /&gt;
  For example, this book says so, but uses suspiciously modern terminology&lt;br /&gt;
&lt;br /&gt;
  For example, this book says so, but uses suspiciously modern terminology&lt;br /&gt;
&lt;br /&gt;
例如，这本书是这么说的，但是使用了可疑的现代术语&lt;br /&gt;
&lt;br /&gt;
    http://books.google.es/books?id=u13KiGlz2zcC&amp;amp;lpg=PA92&amp;amp;ots=8H1DRURdxn&amp;amp;pg=PA93#v=onepage&amp;amp;f=false&lt;br /&gt;
&lt;br /&gt;
    http://books.google.es/books?id=u13KiGlz2zcC&amp;amp;lpg=PA92&amp;amp;ots=8H1DRURdxn&amp;amp;pg=PA93#v=onepage&amp;amp;f=false&lt;br /&gt;
&lt;br /&gt;
Http://books.google.es/books?id=u13kiglz2zcc&amp;amp;lpg=pa92&amp;amp;ots=8h1drurdxn&amp;amp;pg=pa93#v=onepage&amp;amp;f=false&lt;br /&gt;
&lt;br /&gt;
  On the other hand, Uffink's &amp;quot;Compendium of the foundations of classical statistical physics&amp;quot; does not seem to indicate quite this equation but rather that Boltzmann's 1968 distribution was the simple Maxwell–Boltzmann distribution (for a classical nonrelativistic gas), modified for particles in a potential.&lt;br /&gt;
&lt;br /&gt;
  On the other hand, Uffink's &amp;quot;Compendium of the foundations of classical statistical physics&amp;quot; does not seem to indicate quite this equation but rather that Boltzmann's 1968 distribution was the simple Maxwell–Boltzmann distribution (for a classical nonrelativistic gas), modified for particles in a potential.&lt;br /&gt;
&lt;br /&gt;
另一方面，Uffink 的“经典统计物理学基础纲要”似乎并没有完全表明这个方程，而是说 Boltzmann 在1968年的分布是简单的 Maxwell-波兹曼分布(用于经典的非气体) ，修改为势中的粒子。&lt;br /&gt;
&lt;br /&gt;
--&amp;gt; &lt;br /&gt;
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--&amp;gt; &lt;br /&gt;
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--&amp;gt;&lt;br /&gt;
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The distribution was later investigated extensively, in its modern generic form, by [[Josiah Willard Gibbs]] in 1902.&amp;lt;ref name=&amp;quot;gibbs&amp;quot;&amp;gt;{{cite book |last=Gibbs |first=Josiah Willard |authorlink=Josiah Willard Gibbs |title=Elementary Principles in Statistical Mechanics |year=1902 |publisher=[[Charles Scribner's Sons]] &lt;br /&gt;
&lt;br /&gt;
The distribution was later investigated extensively, in its modern generic form, by Josiah Willard Gibbs in 1902.&lt;br /&gt;
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这种分布后来在1902年由约西亚·威拉德·吉布斯进行了广泛的调查，以其现代通用形式。&lt;br /&gt;
&lt;br /&gt;
|location=New York|title-link=Elementary Principles in Statistical Mechanics }}&amp;lt;/ref&amp;gt;{{rp|Ch.IV}}、&lt;br /&gt;
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在玻尔兹曼分布被发明之后，约西亚·华纳德·吉布森充分地研究了它并在1902年提出了它的一般形式。&amp;lt;ref name=&amp;quot;gibbs&amp;quot; /&amp;gt;&lt;br /&gt;
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The generalized Boltzmann distribution is a sufficient and necessary condition for the equivalence between the statistical mechanics definition of [[entropy]] (The [[Entropy_(statistical_thermodynamics)#Gibbs_entropy_formula | Gibbs entropy formula]] &amp;lt;math&amp;gt;S = -k_{\mathrm{B}}\sum_i p_i \log p_i&amp;lt;/math&amp;gt;) and the thermodynamic definition of entropy (&amp;lt;math&amp;gt;d S = \frac{\delta Q_\text{rev}}{T}&amp;lt;/math&amp;gt;, and the [[fundamental thermodynamic relation]]).&amp;lt;ref name=&amp;quot;:0&amp;quot;&amp;gt;{{cite journal |last1= Gao |first1= Xiang |last2= Gallicchio |first2= Emilio |first3= Adrian |last3= Roitberg  |date= 2019 |title= The generalized Boltzmann distribution is the only distribution in which the Gibbs-Shannon entropy equals the thermodynamic entropy |journal= The Journal of Chemical Physics|volume= 151|issue= 3|pages= 034113|doi= 10.1063/1.5111333|pmid= 31325924 |arxiv= 1903.02121 |s2cid= 118981017 }}&amp;lt;/ref&amp;gt;&lt;br /&gt;
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广义波兹曼分布是熵的统计力学定义(吉布斯熵公式  &amp;lt;math&amp;gt;S = -k_{\mathrm{B}}\sum_i p_i \log p_i&amp;lt;/math&amp;gt;))与熵的热力学定义(&amp;lt;math&amp;gt;d S = \frac{\delta Q_\text{rev}}{T}&amp;lt;/math&amp;gt;)等价的充要条件。&amp;lt;ref name=&amp;quot;:0&amp;quot; /&amp;gt;&lt;br /&gt;
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The Boltzmann distribution should not be confused with the [[Maxwell–Boltzmann distribution]]. The former gives the probability that a system will be in a certain state as a function of that state's energy;&amp;lt;ref name=&amp;quot;Atkins, P. W. 2010&amp;quot;&amp;gt;Atkins, P. W. (2010) Quanta, W. H. Freeman and Company, New York&amp;lt;/ref&amp;gt; in contrast, the latter is used to describe particle speeds in idealized gases.&lt;br /&gt;
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值得一提的是，玻尔兹曼分布不应与麦克斯韦-玻尔兹曼分布混淆。前者给出了系统处于某种状态的概率，作为该状态能量的函数; 后者则是用于描述理想气体中的粒子速度。&lt;br /&gt;
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==分布==&lt;br /&gt;
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The Boltzmann distribution is a [[probability distribution]] that gives the probability of a certain state as a function of that state's energy and  temperature of the [[system]] to which the distribution is applied.&amp;lt;ref name=&amp;quot;McQuarrie, A. 2000&amp;quot;&amp;gt;McQuarrie, A. (2000) Statistical Mechanics, University Science Books, California&amp;lt;/ref&amp;gt; It is given as&lt;br /&gt;
&lt;br /&gt;
波兹曼分布是一个概率分布，它给出了出于某种量子态处于某种能量和温度的时候的概率。它被这样定义：&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
《数学》&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
p_i=\frac{1}{Q}} {e^{- {\varepsilon}_i / k T}=\frac{e^{- {\varepsilon}_i / k T}}{\sum_{j=1}^{M}{e^{- {\varepsilon}_j / k T}}}&lt;br /&gt;
&lt;br /&gt;
P _ i = frac {1}{ q }{ e ^ {-{ varepsilon } _ i/k t } = frac { e ^ {-{ varepsilon } _ i/k t }{ sum { j = 1} ^ { m }{ e ^ {-{ varepsilon } _ j/k t }}}}}&lt;br /&gt;
&lt;br /&gt;
p_i=\frac{1}{Q}} {e^{- {\varepsilon}_i / k T}=\frac{e^{- {\varepsilon}_i / k T}}{\sum_{j=1}^{M}{e^{- {\varepsilon}_j / k T}}}&lt;br /&gt;
&lt;br /&gt;
&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
数学&lt;br /&gt;
&lt;br /&gt;
&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
where ''p&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;'' is the probability of state ''i'', ''ε&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;'' the energy of state ''i'', ''k'' the Boltzmann constant, ''T'' the temperature of the system and ''M'' is the number of all states accessible to the system of interest.&amp;lt;ref name=&amp;quot;McQuarrie, A. 2000&amp;quot; /&amp;gt;&amp;lt;ref name=&amp;quot;Atkins, P. W. 2010&amp;quot; /&amp;gt; Implied parentheses around the denominator ''kT'' are omitted for brevity. The normalization denominator ''Q'' (denoted by some authors by ''Z'') is the [[canonical partition function]]&lt;br /&gt;
&lt;br /&gt;
其中 ''p&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;'' 是状态 i 的概率，''ε&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;'' 是状态 i 的能量，''k'' 是波兹曼常数，''T'' 是系统的温度，''M'' 是系统所能到达的所有量子态的数目。&amp;lt;ref name=&amp;quot;Atkins, P. W. 2010&amp;quot; /&amp;gt; &amp;lt;ref name=&amp;quot;McQuarrie, A. 2000&amp;quot; /&amp;gt;这里为了简洁美观，省略了''kT''周围的括弧。归一化的分母''Q''（被有些作者写为''Z''）是对于系统中所有量子态进行总和，此部分又被称为[[Index.php?title=Canonical partition function|正则配分函数]]''。''&lt;br /&gt;
&lt;br /&gt;
It results from the constraint that the probabilities of all accessible states must add up to 1.&lt;br /&gt;
&lt;br /&gt;
所有量子态的概率之和为1.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The Boltzmann distribution is the distribution that maximizes the [[entropy]]，&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt;H(p_1,p_2,\cdots,p_M) = -\sum_{i=1}^{M} p_i\log_2 p_i&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&amp;lt;nowiki&amp;gt;subject to the constraint that {\sum{p_i {\varepsilon}_i}} equals a particular mean energy value (which can be proven using &amp;lt;/nowiki&amp;gt;[[Lagrange multipliers]]).&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&amp;lt;nowiki&amp;gt;当 {\sum{p_i {\varepsilon}_i}} 等于平均能量值时，玻尔兹曼分布是这种情况下能让熵最大化的分布。我们可以通过拉格朗日乘数法来证明。&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The partition function can be calculated if we know the energies of the states accessible to the system of interest. For atoms the partition function values can be found in the NIST Atomic Spectra Database.&amp;lt;ref name=&amp;quot;:1&amp;quot;&amp;gt;[http://physics.nist.gov/PhysRefData/ASD/levels_form.html NIST Atomic Spectra Database Levels Form] at nist.gov&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
在知道量子态能量的情况下，这个配分函数可以被计算。对于原子来说，配分函数的值可以在NIST Atomic Spectra Database中找到。&amp;lt;ref name=&amp;quot;:1&amp;quot; /&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The distribution shows that states with lower energy will always have a higher probability of being occupied than the states with higher energy. It can also give us the quantitative relationship between the probabilities of the two states being occupied. The ratio of probabilities for states i and j is given as&lt;br /&gt;
&lt;br /&gt;
玻尔兹曼分布指出，能量低的量子态总是有比能量高的量子态更高的概率被粒子占据。它同时也能让我们定量地比较两个量子态分布概率的关系。状态 i 和状态 j 的概率比为&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
{\frac{p_i}{p_j}}=e^{({\varepsilon}_j-{\varepsilon}_i) / k T}&lt;br /&gt;
&lt;br /&gt;
&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;nowiki&amp;gt;{\frac{p_i}{p_j}}=e^{({\varepsilon}_j-{\varepsilon}_i) / k T}&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;nowiki&amp;gt;{\frac{p_i}{p_j}}=e^{({\varepsilon}_j-{\varepsilon}_i) / k T}&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&amp;lt;nowiki&amp;gt;&amp;lt;/math&amp;gt;&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
&lt;br /&gt;
数学&lt;br /&gt;
&lt;br /&gt;
where p&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt; is the probability of state i,  p&amp;lt;sub&amp;gt;j&amp;lt;/sub&amp;gt; the probability of state j, and ε&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt; and ε&amp;lt;sub&amp;gt;j&amp;lt;/sub&amp;gt; are the energies of states i and j, respectively.&lt;br /&gt;
&lt;br /&gt;
其中 p&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt; 是量子态 i 的概率， p&amp;lt;sub&amp;gt;j&amp;lt;/sub&amp;gt; 是量子态 j 的概率，ε&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt; 和 ε&amp;lt;sub&amp;gt;j&amp;lt;/sub&amp;gt; 分别是状态 i 和 j 的能量。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The Boltzmann distribution is often used to describe the distribution of particles, such as atoms or molecules, over energy states accessible to them. If we have a system consisting of many particles, the probability of a particle being in state i is practically the probability that, if we pick a random particle from that system and check what state it is in, we will find it is in state i. This probability is equal to the number of particles in state i divided by the total number of particles in the system, that is the fraction of particles that occupy state i.&lt;br /&gt;
&lt;br /&gt;
玻尔兹曼分布通常被用来描述粒子的分布，比如原子或分子，在能量状态上的分布情况。如果我们有一个由许多粒子组成的系统，某个粒子处于量子态 i 的概率就等同于当我们从该系统中选择一个随机的粒子并观察它处于什么状态，发现它处于状态 i 的概率。这个概率等于量子态 i 的粒子数除以系统中粒子的总数，即那些占据量子态i的粒子的比例。&lt;br /&gt;
&lt;br /&gt;
&amp;lt;nowiki&amp;gt;&amp;lt;math display=&amp;quot;inline&amp;quot;&amp;gt;&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;nowiki&amp;gt;p_i={\frac{N_i}{N}}&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
&lt;br /&gt;
P _ i = { frac { n _ i }{ n }&lt;br /&gt;
&lt;br /&gt;
&amp;lt;nowiki&amp;gt;{\sum{p_i {\varepsilon}_i}}&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
where N&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt; is the number of particles in state i and N is the total number of particles in the system. We may use the Boltzmann distribution to find this probability that is, as we have seen, equal to the fraction of particles that are in state i. So the equation that gives the fraction of particles in state i as a function of the energy of that state is&lt;br /&gt;
&lt;br /&gt;
&amp;lt;nowiki&amp;gt;&amp;lt;/math&amp;gt;&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
&lt;br /&gt;
《数学公式丢失了》&lt;br /&gt;
&lt;br /&gt;
N&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt; 是位于量子态 i 的粒子数，N是系统中粒子的总数。我们可以用波兹曼分布来求出这个概率，它等于处于量子态i的粒子的比例。所以这个方程给出位于量子态 i 的粒子比例关于这个状态能量的函数&amp;lt;ref name=&amp;quot;Atkins, P. W. 2010&amp;quot; /&amp;gt;。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
This equation is of great importance to [[spectroscopy]]. In spectroscopy we observe a [[spectral line]] of atoms or molecules that we are interested in going from one state to another.&amp;lt;ref name=&amp;quot;Atkins, P. W. 2010&amp;quot; /&amp;gt;&amp;lt;ref name=&amp;quot;:2&amp;quot;&amp;gt;Atkins, P. W.; de Paula J. (2009) Physical Chemistry, 9th edition, Oxford University Press, Oxford, UK&amp;lt;/ref&amp;gt; In order for this to be possible, there must be some particles in the first state to undergo the transition. We may find that this condition is fulfilled by finding the fraction of particles in the first state. If it is negligible, the transition is very likely not to be observed at the temperature for which the calculation was done. In general, a larger fraction of molecules in the first state means a higher number of transitions to the second state.&amp;lt;ref name=&amp;quot;:3&amp;quot;&amp;gt;Skoog, D. A.; Holler, F. J.; Crouch, S. R. (2006) Principles of Instrumental Analysis, Brooks/Cole, Boston, MA&amp;lt;/ref&amp;gt; This gives a stronger spectral line. However, there are other factors that influence the intensity of a spectral line, such as whether it is caused by an allowed or a [[forbidden transition]]&lt;br /&gt;
&lt;br /&gt;
对于光谱学来说这很重要在。在光谱中，我们期待能观察到一条原子或分子跃迁的谱线。&amp;lt;ref name=&amp;quot;Atkins, P. W. 2010&amp;quot; /&amp;gt;&amp;lt;ref name=&amp;quot;:2&amp;quot; /&amp;gt; 在为了使这成为可能，必须有一些粒子处于第一个量子态，等待着发生跃迁。我们可以通过求第一态粒子的比例来满足这个条件。如果它可以忽略不计，那么在当前计算的温度下，则很难观察到这种跃迁。一般来说，处于第一状态的分子比例越大，意味着向第二状态跃迁的次数越多。&amp;lt;ref name=&amp;quot;:3&amp;quot; /&amp;gt;这就产生了一条更强的谱线。然而，还有其他因素影响谱线的强度，例如它是否是被允许的跃迁还是被禁止的跃迁。&lt;br /&gt;
&lt;br /&gt;
The Boltzmann distribution is related to the [[softmax function]] commonly used in machine learning.&lt;br /&gt;
&lt;br /&gt;
玻尔兹曼分布与机器学习中常用的[[Index.php?title=Softmax function|归一化指数函数]]（Softmax 函数）有关。&lt;br /&gt;
=='''统计力学''' ==&lt;br /&gt;
&lt;br /&gt;
{{main|Canonical ensemble|Maxwell–Boltzmann statistics}}The Boltzmann distribution appears in statistical mechanics when considering isolated (or nearly-isolated) systems of fixed composition that are in thermal equilibrium (equilibrium with respect to energy exchange). The most general case is the probability distribution for the canonical ensemble, but also some special cases (derivable from the canonical ensemble) also show the Boltzmann distribution in different aspects:&lt;br /&gt;
&lt;br /&gt;
当独立的(或者几乎独立的)固定体系处于统计力学热平衡状态时，玻尔兹曼分布就会出现。最普遍的情况是概率分布的正则系综，但也有一些特殊的情况(从正则系综衍生)也显示了不同形式的玻尔兹曼分布:&lt;br /&gt;
&lt;br /&gt;
; [[Canonical ensemble]] (general case)&lt;br /&gt;
; '''正则系综(一般情况)'''&lt;br /&gt;
; '''The [[canonical ensemble]] gives the [[probabilities]] of the various possible states of a closed system of fixed volume, in thermal equilibrium with a [[heat bath]]. The canonical ensemble is a probability distribution with the Boltzmann form.'''&lt;br /&gt;
&lt;br /&gt;
正则系综模型给出了在一个封闭固定体积，带有热浴的热平衡系统中的各种可能状态的概率。我们称正则系综为一个玻尔兹曼概率分布。&lt;br /&gt;
&lt;br /&gt;
; &lt;br /&gt;
; Statistical frequencies of subsystems' states (in a non-interacting collection)&lt;br /&gt;
'''子系统状态的统计频率(在一个无交互的集合中)'''&lt;br /&gt;
: When the system of interest is a collection of many non-interacting copies of a smaller subsystem, it is sometimes useful to find the [[statistical frequency]] of a given subsystem state, among the collection. The canonical ensemble has the property of separability when applied to such a collection: as long as the non-interacting subsystems have fixed composition, then each subsystem's state is independent of the others and is also characterized by a canonical ensemble. As a result, the [[expectation value|expected]] statistical frequency distribution of subsystem states has the Boltzmann form.&lt;br /&gt;
&lt;br /&gt;
当系统是一个较小子系统的许多非交互副本的集合时，有时我们需要在某个子系统集合中找到某个子系统的统计频率。当应用于这样一个集合时，这个子系统的正则系综具有可分离性: 只要不相互作用的子系统的组成是固定的，那么每个子系统的状态都是独立于其他子系统的，它们也拥有自己的正则系综。因此，子系统状态的期望统计频率分布形式是玻尔兹曼分布。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[Maxwell–Boltzmann statistics]] of classical gases (systems of non-interacting particles)&lt;br /&gt;
&lt;br /&gt;
'''Maxwell-Boltzmann 统计中的经典气体系统(非相互作用粒子系统)'''&lt;br /&gt;
&lt;br /&gt;
: In particle systems, many particles share the same space and regularly change places with each other; the single-particle state space they occupy is a shared space. [[Maxwell–Boltzmann statistics]] give the expected number of particles found in a given single-particle state, in a [[classical mechanics|classical]] gas of non-interacting particles at equilibrium. This expected number distribution has the Boltzmann form.&lt;br /&gt;
&lt;br /&gt;
在粒子系统中，许多粒子共享同一空间，并且相互之间有规律地改变位置; 它们所占据的单粒子状态空间是一个共享空间。[[Index.php?title=Maxwell–Boltzmann statistics|麦克斯韦-玻尔兹曼统计]]给出了在一个给定的单粒子态，在一个处于平衡状态的非相互作用粒子的经典气体中所发现的粒子的预期数量。这个预期的数量分布具有玻尔兹曼分布形式。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Although these cases have strong similarities, it is helpful to distinguish them as they generalize in different ways when the crucial assumptions are changed:&lt;br /&gt;
&lt;br /&gt;
虽然这些案例有很多相似之处，但是当关键假设发生变化时，我们需要对它们以不同的方式进行归纳总结，因此区分它们是有帮助的:&lt;br /&gt;
* When a system is in thermodynamic equilibrium with respect to both energy exchange ''and particle exchange'', the requirement of fixed composition is relaxed and a [[grand canonical ensemble]] is obtained rather than canonical ensemble. On the other hand, if both composition and energy are fixed, then a [[microcanonical ensemble]] applies instead.&lt;br /&gt;
* 当一个系统在能量交换和粒子交换方面都处于热力学平衡时，固定组成的要求就放宽了。这时我们就得到了一个[[Index.php?title=Microcanonical ensemble|巨正则系综]]而不是正则系综。另一方面，如果成分和能量都是固定的，则可以使用[[微正则系综Index.php?title=Microcanonical ensemble|微正则系综]]。&lt;br /&gt;
&lt;br /&gt;
* If the subsystems within a collection ''do'' interact with each other, then the expected frequencies of subsystem states no longer follow a Boltzmann distribution, and even may not have an [[analytical solution]].&amp;lt;ref name=&amp;quot;:4&amp;quot;&amp;gt;A classic example of this is [[magnetic ordering]]. Systems of non-interacting [[spin (physics)|spins]] show [[paramagnetic]] behaviour that can be understood with a single-particle canonical ensemble (resulting in the [[Brillouin function]]). Systems of ''interacting'' spins can show much more complex behaviour such as [[ferromagnetism]] or [[antiferromagnetism]].&amp;lt;/ref&amp;gt; The canonical ensemble can however still be applied to the ''collective'' states of the entire system considered as a whole, provided the entire system is isolated and in thermal equilibrium.&lt;br /&gt;
* 如果集合中的子系统确实相互交互，则子系统状态的预期频率不再遵循玻尔兹曼 分布，甚至可能没有解析解。&amp;lt;ref name=&amp;quot;:4&amp;quot; /&amp;gt;然而，如果整个系统是独立的并且处于热平衡状态，则正则系综仍然可以应用于作为一个整体考虑。&lt;br /&gt;
&lt;br /&gt;
* With ''[[quantum mechanics|quantum]]'' gases of non-interacting particles in equilibrium, the number of particles found in a given single-particle state does not follow Maxwell–Boltzmann statistics, and there is no simple closed form expression for quantum gases in the canonical ensemble. In the grand canonical ensemble the state-filling statistics of quantum gases are described by [[Fermi–Dirac statistics]] or [[Bose–Einstein statistics]], depending on whether the particles are [[fermion]]s or [[boson]]s respectively.&lt;br /&gt;
* 对于处于平衡状态的非相互作用粒子的量子气体，在给定的单粒子状态中发现的粒子数量并不遵循麦克斯韦-玻尔兹曼统计。并且正则系综中的量子气体没有简单的封闭表达式。在巨正则系综中，量子气体的统计分布状态由费米-狄拉克统计或玻色-爱因斯坦统计来描述，具体则取决于该粒子是费米子还是玻色子。&lt;br /&gt;
&lt;br /&gt;
== 数学 ==&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
In more general mathematical settings, the Boltzmann distribution is also known as the [[Gibbs measure]]. In statistics and machine learning, it is called a [[log-linear model]]. In [[deep learning]], the Boltzmann distribution is used in the sampling distribution of [[stochastic neural network]]s such as the [[Boltzmann machine]], [[Restricted Boltzmann machine]], [[Energy based model|Energy-Based models]] and [[Deep Boltzmann Machine|deep Boltzmann machine]]&lt;br /&gt;
&lt;br /&gt;
在更一般的数学环境中，玻尔兹曼分布也被称为吉布斯量度。在统计学和机器学习中，它被称为对数线性回归。在深度学习中，玻尔兹曼分布被用于随机神经网络的抽样分布，如玻尔兹曼机、受限玻尔兹曼机、基于能量的模型和深度波茨曼机。&lt;br /&gt;
&lt;br /&gt;
== 经济 ==&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The Boltzmann distribution can be introduced to allocate permits in emissions trading.&amp;lt;ref name=&amp;quot;Park, J.-W. 2012&amp;quot;&amp;gt;Park, J.-W., Kim, C. U. and Isard, W. (2012) Permit allocation in emissions trading using the Boltzmann distribution. Physica A 391: 4883–4890&amp;lt;/ref&amp;gt;&amp;lt;ref name=&amp;quot;:5&amp;quot;&amp;gt;[http://www.technologyreview.com/view/425051/the-thorny-problem-of-fair-allocation/ The Thorny Problem Of Fair Allocation]. ''Technology Review'' blog. August 17, 2011. Cites and summarizes Park, Kim and Isard (2012).&amp;lt;/ref&amp;gt; The new allocation method using the Boltzmann distribution can describe the most probable, natural, and unbiased distribution of emissions permits among multiple countries. Simple and versatile, this new method holds potential for many economic and environmental applications.&lt;br /&gt;
&lt;br /&gt;
在经济学中，玻尔兹曼分布被用来分配排放交易中的许可。&amp;lt;ref name=&amp;quot;Park, J.-W. 2012&amp;quot; /&amp;gt;&amp;lt;ref name=&amp;quot;:5&amp;quot; /&amp;gt;  使用玻尔兹曼分布的新分配方法可以创造出在多个国家之间最可能的、自然的和无偏见的排放许可分配。这种新方法简单而通用，在经济和环保中有很大的应用潜力。&lt;br /&gt;
&lt;br /&gt;
The Boltzmann distribution has the same form as the [[Multinomial logistic regression|multinomial logit]] model. As a [[discrete choice]] model, this is very well known in economics since [[Daniel McFadden]] made the connection to random utility maximization.&lt;br /&gt;
&lt;br /&gt;
玻尔兹曼分布与多项逻辑回归模型具有相同的形式。在丹尼尔 · 麦克法登将它与随机效用最大化联系起来之后，成为了大家所熟知的一种离散选择模型。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Category:Statistical mechanics&lt;br /&gt;
&lt;br /&gt;
类别: 统计力学&lt;br /&gt;
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本中文词条由[[用户:费米子|tueryeye]]编辑，欢迎在讨论页面留言。&lt;br /&gt;
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==See also==&lt;br /&gt;
&lt;br /&gt;
Distribution&lt;br /&gt;
&lt;br /&gt;
分布&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:Boltzmann distribution]]. Its edit history can be viewed at [[玻尔兹曼分布/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>
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{{Use American English|date = March 2019}}&lt;br /&gt;
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{{Short description|Probability distribution of energy states of a system}}&lt;br /&gt;
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{{about|system energy states|particle energy levels and velocities|Maxwell–Boltzmann distribution}}&lt;br /&gt;
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[[File:Boltzmann distribution graph.svg|upright=1.75|right|thumb|Boltzmann factor ''p&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;''&amp;amp;nbsp;/&amp;amp;nbsp;''p&amp;lt;sub&amp;gt;j&amp;lt;/sub&amp;gt;'' (vertical axis) as a function of temperature ''T'' for several energy differences ''ε&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;''&amp;amp;nbsp;−&amp;amp;nbsp;''ε&amp;lt;sub&amp;gt;j&amp;lt;/sub&amp;gt;''.|链接=Special:FilePath/Boltzmann_distribution_graph.svg]]&lt;br /&gt;
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In [[statistical mechanics]] and [[mathematics]], a '''Boltzmann distribution''' (also called '''Gibbs distribution'''&amp;lt;ref name=&amp;quot;landau&amp;quot;&amp;gt;{{cite book | author=Landau, Lev Davidovich |author2=Lifshitz, Evgeny Mikhailovich |name-list-style=amp | title=Statistical Physics |volume=5 |series=Course of Theoretical Physics |edition=3 |origyear=1976 |year=1980 |place=Oxford |publisher=Pergamon Press|isbn=0-7506-3372-7|author-link=Lev Landau |author2-link=Evgeny Lifshitz }} Translated by J.B. Sykes and M.J. Kearsley. See section 28&amp;lt;/ref&amp;gt;) is a [[probability distribution]] or [[probability measure]] that gives the probability that a system will be in a certain [[microstate (statistical mechanics)|state]] as a function of that state's energy and the temperature of the system. The distribution is expressed in the form:&lt;br /&gt;
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在统计力学和数学中，波兹曼分布分布(也称为吉布斯分布&amp;lt;ref name=&amp;quot;landau&amp;quot; /&amp;gt;)是一个概率分布或机率量测，它给出了一个系统处于某种量子态的概率，这个概率是该状态的能量和系统温度的函数。分布情况以下列形式表示:&lt;br /&gt;
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:&amp;lt;math&amp;gt;p_i \propto e^{-\frac{\varepsilon_i}{kT}}&amp;lt;/math&amp;gt; &lt;br /&gt;
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&amp;lt;math&amp;gt;p_i \propto e^{-\frac{\varepsilon_i}{kT}}&amp;lt;/math&amp;gt; &lt;br /&gt;
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[拉丁语]&lt;br /&gt;
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where {{mvar|p&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;}} is the probability of the system being in state {{mvar|i}}, {{mvar|ε&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;}} is the energy of that state, and a constant {{mvar|kT}} of the distribution is the product of [[Boltzmann's constant]] {{mvar|k}} and [[thermodynamic temperature]] {{mvar|T}}. The symbol &amp;lt;math display=&amp;quot;inline&amp;quot;&amp;gt;\propto&amp;lt;/math&amp;gt; denotes [[proportionality (mathematics)|proportionality]] (see {{section link||The distribution}} for the proportionality constant).&lt;br /&gt;
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{{mvar|p&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;}} 是其中系统处于状态{{mvar|i}}的概率, {{mvar|ε&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;}} 是该状态的能量，还有关于这个分布的一个常数 {{mvar|kT}} ，它是玻尔兹曼常数{{mvar|k}}和热力学温度 {{mvar|T}} 的乘积。符号 &amp;lt;math display=&amp;quot;inline&amp;quot;&amp;gt;\propto&amp;lt;/math&amp;gt;表示正比例(见附录中的比例常数)。&lt;br /&gt;
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The term system here has a very wide meaning; it can range from a single atom to a macroscopic system such as a [[Natural gas storage|natural gas storage tank]]. Because of this the Boltzmann distribution can be used to solve a very wide variety of problems. The distribution shows that states with lower energy will always have a higher probability of being occupied .&lt;br /&gt;
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这里的术语系统含义广泛; 它可以从单个原子到宏观系统，如天然气储罐。正因为如此，波兹曼分布可以用来解决各种各样的问题。玻尔兹曼分布表明，能量较低的状态被占据的概率总是较高的。&lt;br /&gt;
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The ''ratio'' of probabilities of two states is known as the '''Boltzmann factor''' and characteristically only depends on the states' energy difference:&lt;br /&gt;
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两种状态的概率之比被称为玻尔兹曼因子，取决于两种状态的能量差:&lt;br /&gt;
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:&amp;lt;math&amp;gt;\frac{p_i}{p_j} = e^{\frac{\varepsilon_j - \varepsilon_i}{kT}}&amp;lt;/math&amp;gt;&lt;br /&gt;
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[数学][数学]&lt;br /&gt;
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The Boltzmann distribution is named after [[Ludwig Boltzmann]] who first formulated it in 1868 during his studies of the [[statistical mechanics]] of gases in thermal equilibrium. Boltzmann's statistical work is borne out in his paper “On the Relationship between the Second Fundamental Theorem of the Mechanical Theory of Heat and Probability Calculations Regarding the Conditions for Thermal Equilibrium&amp;quot;&amp;lt;ref&amp;gt;http://crystal.med.upenn.edu/sharp-lab-pdfs/2015SharpMatschinsky_Boltz1877_Entropy17.pdf&amp;lt;/ref&amp;gt;&lt;br /&gt;
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波兹曼分布是根据路德维希·玻尔兹曼1868年在研究统计力学中气体热平衡的时候首次提出的一个公式命名的。波尔兹曼的统计工作在他1877年的论文《论热力学第二基本定理与热平衡条件的概率计算之间的关系》中得到了体现。&amp;lt;ref&amp;gt;“On the Relationship between the Second Fundamental Theorem of the Mechanical Theory of Heat and Probability Calculations Regarding the Conditions for Thermal Equilibrium” Sitzungberichte der Kaiserlichen Akademie der Wissenschaften. Mathematisch-Naturwissen Classe. Abt. II, LXXVI 1877, pp 373-435 (Wien. Ber. 1877, 76:373-435). &amp;lt;/ref&amp;gt;&lt;br /&gt;
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  It would be nice to have a citation here! The origin of the Boltzmann factor isn't entirely clear. According to some authors, Boltzmann's 1968 paper “On the Relationship between the Second Fundamental Theorem of the Mechanical Theory of Heat and Probability Calculations Regarding the Conditions for Thermal Equilibrium”&lt;br /&gt;
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  It would be nice to have a citation here! The origin of the Boltzmann factor isn't entirely clear. According to some authors, Boltzmann's 1968 paper “On the Relationship between the Second Fundamental Theorem of the Mechanical Theory of Heat and Probability Calculations Regarding the Conditions for Thermal Equilibrium”&lt;br /&gt;
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如果能在这里引用一下就好了！玻尔兹曼因子的起源并不完全清楚。根据一些作者的说法，Boltzmann 在1968年发表的论文《论热力学第二基本定理与热平衡条件的概率计算之间的关系》&lt;br /&gt;
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  &amp;quot;Studien über das Gleichgewicht der lebendigen Kraft zwischen bewegten materiellen Punkten&amp;quot; is the origin but I can't find this article at the moment,&lt;br /&gt;
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  &amp;quot;Studien über das Gleichgewicht der lebendigen Kraft zwischen bewegten materiellen Punkten&amp;quot; is the origin but I can't find this article at the moment,&lt;br /&gt;
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  &amp;quot;Studien über das Gleichgewicht der lebendigen Kraft zwischen bewegten materiellen Punkten&amp;quot; is the origin but I can't find this article at the moment,&lt;br /&gt;
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  so I cannot confirm.&lt;br /&gt;
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  so I cannot confirm.&lt;br /&gt;
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所以我不能确定。&lt;br /&gt;
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  For example, this book says so, but uses suspiciously modern terminology&lt;br /&gt;
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  For example, this book says so, but uses suspiciously modern terminology&lt;br /&gt;
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例如，这本书是这么说的，但是使用了可疑的现代术语&lt;br /&gt;
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    http://books.google.es/books?id=u13KiGlz2zcC&amp;amp;lpg=PA92&amp;amp;ots=8H1DRURdxn&amp;amp;pg=PA93#v=onepage&amp;amp;f=false&lt;br /&gt;
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    http://books.google.es/books?id=u13KiGlz2zcC&amp;amp;lpg=PA92&amp;amp;ots=8H1DRURdxn&amp;amp;pg=PA93#v=onepage&amp;amp;f=false&lt;br /&gt;
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Http://books.google.es/books?id=u13kiglz2zcc&amp;amp;lpg=pa92&amp;amp;ots=8h1drurdxn&amp;amp;pg=pa93#v=onepage&amp;amp;f=false&lt;br /&gt;
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  On the other hand, Uffink's &amp;quot;Compendium of the foundations of classical statistical physics&amp;quot; does not seem to indicate quite this equation but rather that Boltzmann's 1968 distribution was the simple Maxwell–Boltzmann distribution (for a classical nonrelativistic gas), modified for particles in a potential.&lt;br /&gt;
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  On the other hand, Uffink's &amp;quot;Compendium of the foundations of classical statistical physics&amp;quot; does not seem to indicate quite this equation but rather that Boltzmann's 1968 distribution was the simple Maxwell–Boltzmann distribution (for a classical nonrelativistic gas), modified for particles in a potential.&lt;br /&gt;
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另一方面，Uffink 的“经典统计物理学基础纲要”似乎并没有完全表明这个方程，而是说 Boltzmann 在1968年的分布是简单的 Maxwell-波兹曼分布(用于经典的非气体) ，修改为势中的粒子。&lt;br /&gt;
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--&amp;gt; &lt;br /&gt;
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--&amp;gt; &lt;br /&gt;
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--&amp;gt;&lt;br /&gt;
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The distribution was later investigated extensively, in its modern generic form, by [[Josiah Willard Gibbs]] in 1902.&amp;lt;ref name=&amp;quot;gibbs&amp;quot;&amp;gt;{{cite book |last=Gibbs |first=Josiah Willard |authorlink=Josiah Willard Gibbs |title=Elementary Principles in Statistical Mechanics |year=1902 |publisher=[[Charles Scribner's Sons]] &lt;br /&gt;
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The distribution was later investigated extensively, in its modern generic form, by Josiah Willard Gibbs in 1902.&lt;br /&gt;
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这种分布后来在1902年由约西亚·威拉德·吉布斯进行了广泛的调查，以其现代通用形式。&lt;br /&gt;
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|location=New York|title-link=Elementary Principles in Statistical Mechanics }}&amp;lt;/ref&amp;gt;{{rp|Ch.IV}}、&lt;br /&gt;
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在玻尔兹曼分布被发明之后，约西亚·华纳德·吉布森充分地研究了它并在1902年提出了它的一般形式。&amp;lt;ref name=&amp;quot;gibbs&amp;quot; /&amp;gt;&lt;br /&gt;
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The generalized Boltzmann distribution is a sufficient and necessary condition for the equivalence between the statistical mechanics definition of [[entropy]] (The [[Entropy_(statistical_thermodynamics)#Gibbs_entropy_formula | Gibbs entropy formula]] &amp;lt;math&amp;gt;S = -k_{\mathrm{B}}\sum_i p_i \log p_i&amp;lt;/math&amp;gt;) and the thermodynamic definition of entropy (&amp;lt;math&amp;gt;d S = \frac{\delta Q_\text{rev}}{T}&amp;lt;/math&amp;gt;, and the [[fundamental thermodynamic relation]]).&amp;lt;ref name=&amp;quot;:0&amp;quot;&amp;gt;{{cite journal |last1= Gao |first1= Xiang |last2= Gallicchio |first2= Emilio |first3= Adrian |last3= Roitberg  |date= 2019 |title= The generalized Boltzmann distribution is the only distribution in which the Gibbs-Shannon entropy equals the thermodynamic entropy |journal= The Journal of Chemical Physics|volume= 151|issue= 3|pages= 034113|doi= 10.1063/1.5111333|pmid= 31325924 |arxiv= 1903.02121 |s2cid= 118981017 }}&amp;lt;/ref&amp;gt;&lt;br /&gt;
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广义波兹曼分布是熵的统计力学定义(吉布斯熵公式  &amp;lt;math&amp;gt;S = -k_{\mathrm{B}}\sum_i p_i \log p_i&amp;lt;/math&amp;gt;))与熵的热力学定义(&amp;lt;math&amp;gt;d S = \frac{\delta Q_\text{rev}}{T}&amp;lt;/math&amp;gt;)等价的充要条件。&amp;lt;ref name=&amp;quot;:0&amp;quot; /&amp;gt;&lt;br /&gt;
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The Boltzmann distribution should not be confused with the [[Maxwell–Boltzmann distribution]]. The former gives the probability that a system will be in a certain state as a function of that state's energy;&amp;lt;ref name=&amp;quot;Atkins, P. W. 2010&amp;quot;&amp;gt;Atkins, P. W. (2010) Quanta, W. H. Freeman and Company, New York&amp;lt;/ref&amp;gt; in contrast, the latter is used to describe particle speeds in idealized gases.&lt;br /&gt;
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值得一提的是，玻尔兹曼分布不应与麦克斯韦-玻尔兹曼分布混淆。前者给出了系统处于某种状态的概率，作为该状态能量的函数; 后者则是用于描述理想气体中的粒子速度。&lt;br /&gt;
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==分布==&lt;br /&gt;
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The Boltzmann distribution is a [[probability distribution]] that gives the probability of a certain state as a function of that state's energy and  temperature of the [[system]] to which the distribution is applied.&amp;lt;ref name=&amp;quot;McQuarrie, A. 2000&amp;quot;&amp;gt;McQuarrie, A. (2000) Statistical Mechanics, University Science Books, California&amp;lt;/ref&amp;gt; It is given as&lt;br /&gt;
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波兹曼分布是一个概率分布，它给出了出于某种量子态处于某种能量和温度的时候的概率。它被这样定义：&lt;br /&gt;
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&amp;lt;math&amp;gt;&lt;br /&gt;
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《数学》&lt;br /&gt;
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:&amp;lt;math&amp;gt;&lt;br /&gt;
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p_i=\frac{1}{Q}} {e^{- {\varepsilon}_i / k T}=\frac{e^{- {\varepsilon}_i / k T}}{\sum_{j=1}^{M}{e^{- {\varepsilon}_j / k T}}}&lt;br /&gt;
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P _ i = frac {1}{ q }{ e ^ {-{ varepsilon } _ i/k t } = frac { e ^ {-{ varepsilon } _ i/k t }{ sum { j = 1} ^ { m }{ e ^ {-{ varepsilon } _ j/k t }}}}}&lt;br /&gt;
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p_i=\frac{1}{Q}} {e^{- {\varepsilon}_i / k T}=\frac{e^{- {\varepsilon}_i / k T}}{\sum_{j=1}^{M}{e^{- {\varepsilon}_j / k T}}}&lt;br /&gt;
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数学&lt;br /&gt;
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&amp;lt;/math&amp;gt;&lt;br /&gt;
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where ''p&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;'' is the probability of state ''i'', ''ε&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;'' the energy of state ''i'', ''k'' the Boltzmann constant, ''T'' the temperature of the system and ''M'' is the number of all states accessible to the system of interest.&amp;lt;ref name=&amp;quot;McQuarrie, A. 2000&amp;quot; /&amp;gt;&amp;lt;ref name=&amp;quot;Atkins, P. W. 2010&amp;quot; /&amp;gt; Implied parentheses around the denominator ''kT'' are omitted for brevity. The normalization denominator ''Q'' (denoted by some authors by ''Z'') is the [[canonical partition function]]&lt;br /&gt;
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其中 ''p&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;'' 是状态 i 的概率，''ε&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;'' 是状态 i 的能量，''k'' 是波兹曼常数，''T'' 是系统的温度，''M'' 是系统所能到达的所有量子态的数目。&amp;lt;ref name=&amp;quot;Atkins, P. W. 2010&amp;quot; /&amp;gt; &amp;lt;ref name=&amp;quot;McQuarrie, A. 2000&amp;quot; /&amp;gt;这里为了简洁美观，省略了''kT''周围的括弧。归一化的分母''Q''（被有些作者写为''Z''）是对于系统中所有量子态进行总和，此部分又被称为[[Index.php?title=Canonical partition function|正则配分函数]]''。''&lt;br /&gt;
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It results from the constraint that the probabilities of all accessible states must add up to 1.&lt;br /&gt;
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所有量子态的概率之和为1.&lt;br /&gt;
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The Boltzmann distribution is the distribution that maximizes the [[entropy]]，&lt;br /&gt;
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&amp;lt;math&amp;gt;H(p_1,p_2,\cdots,p_M) = -\sum_{i=1}^{M} p_i\log_2 p_i&amp;lt;/math&amp;gt;&lt;br /&gt;
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&amp;lt;nowiki&amp;gt;subject to the constraint that {\sum{p_i {\varepsilon}_i}} equals a particular mean energy value (which can be proven using &amp;lt;/nowiki&amp;gt;[[Lagrange multipliers]]).&lt;br /&gt;
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&amp;lt;nowiki&amp;gt;当 {\sum{p_i {\varepsilon}_i}} 等于平均能量值时，玻尔兹曼分布是这种情况下能让熵最大化的分布。我们可以通过拉格朗日乘数法来证明。&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
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The partition function can be calculated if we know the energies of the states accessible to the system of interest. For atoms the partition function values can be found in the NIST Atomic Spectra Database.&amp;lt;ref name=&amp;quot;:1&amp;quot;&amp;gt;[http://physics.nist.gov/PhysRefData/ASD/levels_form.html NIST Atomic Spectra Database Levels Form] at nist.gov&amp;lt;/ref&amp;gt;&lt;br /&gt;
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在知道量子态能量的情况下，这个配分函数可以被计算。对于原子来说，配分函数的值可以在NIST Atomic Spectra Database中找到。&amp;lt;ref name=&amp;quot;:1&amp;quot; /&amp;gt;&lt;br /&gt;
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The distribution shows that states with lower energy will always have a higher probability of being occupied than the states with higher energy. It can also give us the quantitative relationship between the probabilities of the two states being occupied. The ratio of probabilities for states i and j is given as&lt;br /&gt;
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玻尔兹曼分布指出，能量低的量子态总是有比能量高的量子态更高的概率被粒子占据。它同时也能让我们定量地比较两个量子态分布概率的关系。状态 i 和状态 j 的概率比为&lt;br /&gt;
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{\frac{p_i}{p_j}}=e^{({\varepsilon}_j-{\varepsilon}_i) / k T}&lt;br /&gt;
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&amp;lt;nowiki&amp;gt;{\frac{p_i}{p_j}}=e^{({\varepsilon}_j-{\varepsilon}_i) / k T}&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
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&amp;lt;nowiki&amp;gt;{\frac{p_i}{p_j}}=e^{({\varepsilon}_j-{\varepsilon}_i) / k T}&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
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where p&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt; is the probability of state i,  p&amp;lt;sub&amp;gt;j&amp;lt;/sub&amp;gt; the probability of state j, and ε&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt; and ε&amp;lt;sub&amp;gt;j&amp;lt;/sub&amp;gt; are the energies of states i and j, respectively.&lt;br /&gt;
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其中 p&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt; 是量子态 i 的概率， p&amp;lt;sub&amp;gt;j&amp;lt;/sub&amp;gt; 是量子态 j 的概率，ε&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt; 和 ε&amp;lt;sub&amp;gt;j&amp;lt;/sub&amp;gt; 分别是状态 i 和 j 的能量。&lt;br /&gt;
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The Boltzmann distribution is often used to describe the distribution of particles, such as atoms or molecules, over energy states accessible to them. If we have a system consisting of many particles, the probability of a particle being in state i is practically the probability that, if we pick a random particle from that system and check what state it is in, we will find it is in state i. This probability is equal to the number of particles in state i divided by the total number of particles in the system, that is the fraction of particles that occupy state i.&lt;br /&gt;
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玻尔兹曼分布通常被用来描述粒子的分布，比如原子或分子，在能量状态上的分布情况。如果我们有一个由许多粒子组成的系统，某个粒子处于量子态 i 的概率就等同于当我们从该系统中选择一个随机的粒子并观察它处于什么状态，发现它处于状态 i 的概率。这个概率等于量子态 i 的粒子数除以系统中粒子的总数，即那些占据量子态i的粒子的比例。&lt;br /&gt;
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&amp;lt;nowiki&amp;gt;&amp;lt;math display=&amp;quot;inline&amp;quot;&amp;gt;&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
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&amp;lt;nowiki&amp;gt;p_i={\frac{N_i}{N}}&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
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P _ i = { frac { n _ i }{ n }&lt;br /&gt;
&lt;br /&gt;
&amp;lt;nowiki&amp;gt;{\sum{p_i {\varepsilon}_i}}&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
where N&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt; is the number of particles in state i and N is the total number of particles in the system. We may use the Boltzmann distribution to find this probability that is, as we have seen, equal to the fraction of particles that are in state i. So the equation that gives the fraction of particles in state i as a function of the energy of that state is&lt;br /&gt;
&lt;br /&gt;
&amp;lt;nowiki&amp;gt;&amp;lt;/math&amp;gt;&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
&lt;br /&gt;
《数学公式丢失了》&lt;br /&gt;
&lt;br /&gt;
N&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt; 是位于量子态 i 的粒子数，N是系统中粒子的总数。我们可以用波兹曼分布来求出这个概率，它等于处于量子态i的粒子的比例。所以这个方程给出位于量子态 i 的粒子比例关于这个状态能量的函数&amp;lt;ref name=&amp;quot;Atkins, P. W. 2010&amp;quot; /&amp;gt;。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
This equation is of great importance to [[spectroscopy]]. In spectroscopy we observe a [[spectral line]] of atoms or molecules that we are interested in going from one state to another.&amp;lt;ref name=&amp;quot;Atkins, P. W. 2010&amp;quot; /&amp;gt;&amp;lt;ref name=&amp;quot;:2&amp;quot;&amp;gt;Atkins, P. W.; de Paula J. (2009) Physical Chemistry, 9th edition, Oxford University Press, Oxford, UK&amp;lt;/ref&amp;gt; In order for this to be possible, there must be some particles in the first state to undergo the transition. We may find that this condition is fulfilled by finding the fraction of particles in the first state. If it is negligible, the transition is very likely not to be observed at the temperature for which the calculation was done. In general, a larger fraction of molecules in the first state means a higher number of transitions to the second state.&amp;lt;ref name=&amp;quot;:3&amp;quot;&amp;gt;Skoog, D. A.; Holler, F. J.; Crouch, S. R. (2006) Principles of Instrumental Analysis, Brooks/Cole, Boston, MA&amp;lt;/ref&amp;gt; This gives a stronger spectral line. However, there are other factors that influence the intensity of a spectral line, such as whether it is caused by an allowed or a [[forbidden transition]]&lt;br /&gt;
&lt;br /&gt;
对于光谱学来说这很重要在。在光谱中，我们期待能观察到一条原子或分子跃迁的谱线。&amp;lt;ref name=&amp;quot;Atkins, P. W. 2010&amp;quot; /&amp;gt;&amp;lt;ref name=&amp;quot;:2&amp;quot; /&amp;gt; 在为了使这成为可能，必须有一些粒子处于第一个量子态，等待着发生跃迁。我们可以通过求第一态粒子的比例来满足这个条件。如果它可以忽略不计，那么在当前计算的温度下，则很难观察到这种跃迁。一般来说，处于第一状态的分子比例越大，意味着向第二状态跃迁的次数越多。&amp;lt;ref name=&amp;quot;:3&amp;quot; /&amp;gt;这就产生了一条更强的谱线。然而，还有其他因素影响谱线的强度，例如它是否是被允许的跃迁还是被禁止的跃迁。&lt;br /&gt;
&lt;br /&gt;
The Boltzmann distribution is related to the [[softmax function]] commonly used in machine learning.&lt;br /&gt;
&lt;br /&gt;
玻尔兹曼分布与机器学习中常用的[[Index.php?title=Softmax function|归一化指数函数]]（Softmax 函数）有关。&lt;br /&gt;
=='''统计力学''' ==&lt;br /&gt;
&lt;br /&gt;
{{main|Canonical ensemble|Maxwell–Boltzmann statistics}}The Boltzmann distribution appears in statistical mechanics when considering isolated (or nearly-isolated) systems of fixed composition that are in thermal equilibrium (equilibrium with respect to energy exchange). The most general case is the probability distribution for the canonical ensemble, but also some special cases (derivable from the canonical ensemble) also show the Boltzmann distribution in different aspects:&lt;br /&gt;
&lt;br /&gt;
当独立的(或者几乎独立的)固定体系处于统计力学热平衡状态时，玻尔兹曼分布就会出现。最普遍的情况是概率分布的正则系综，但也有一些特殊的情况(从正则系综衍生)也显示了不同形式的玻尔兹曼分布:&lt;br /&gt;
&lt;br /&gt;
; [[Canonical ensemble]] (general case)&lt;br /&gt;
; '''正则系综(一般情况)'''&lt;br /&gt;
; '''The [[canonical ensemble]] gives the [[probabilities]] of the various possible states of a closed system of fixed volume, in thermal equilibrium with a [[heat bath]]. The canonical ensemble is a probability distribution with the Boltzmann form.'''&lt;br /&gt;
&lt;br /&gt;
正则系综模型给出了在一个封闭固定体积，带有热浴的热平衡系统中的各种可能状态的概率。我们称正则系综为一个玻尔兹曼概率分布。&lt;br /&gt;
&lt;br /&gt;
; &lt;br /&gt;
; Statistical frequencies of subsystems' states (in a non-interacting collection)&lt;br /&gt;
'''子系统状态的统计频率(在一个无交互的集合中)'''&lt;br /&gt;
: When the system of interest is a collection of many non-interacting copies of a smaller subsystem, it is sometimes useful to find the [[statistical frequency]] of a given subsystem state, among the collection. The canonical ensemble has the property of separability when applied to such a collection: as long as the non-interacting subsystems have fixed composition, then each subsystem's state is independent of the others and is also characterized by a canonical ensemble. As a result, the [[expectation value|expected]] statistical frequency distribution of subsystem states has the Boltzmann form.&lt;br /&gt;
&lt;br /&gt;
当系统是一个较小子系统的许多非交互副本的集合时，有时我们需要在某个子系统集合中找到某个子系统的统计频率。当应用于这样一个集合时，这个子系统的正则系综具有可分离性: 只要不相互作用的子系统的组成是固定的，那么每个子系统的状态都是独立于其他子系统的，它们也拥有自己的正则系综。因此，子系统状态的期望统计频率分布形式是玻尔兹曼分布。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[Maxwell–Boltzmann statistics]] of classical gases (systems of non-interacting particles)&lt;br /&gt;
&lt;br /&gt;
'''Maxwell-Boltzmann 统计中的经典气体系统(非相互作用粒子系统)'''&lt;br /&gt;
&lt;br /&gt;
: In particle systems, many particles share the same space and regularly change places with each other; the single-particle state space they occupy is a shared space. [[Maxwell–Boltzmann statistics]] give the expected number of particles found in a given single-particle state, in a [[classical mechanics|classical]] gas of non-interacting particles at equilibrium. This expected number distribution has the Boltzmann form.&lt;br /&gt;
&lt;br /&gt;
在粒子系统中，许多粒子共享同一空间，并且相互之间有规律地改变位置; 它们所占据的单粒子状态空间是一个共享空间。[[Index.php?title=Maxwell–Boltzmann statistics|麦克斯韦-玻尔兹曼统计]]给出了在一个给定的单粒子态，在一个处于平衡状态的非相互作用粒子的经典气体中所发现的粒子的预期数量。这个预期的数量分布具有玻尔兹曼分布形式。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Although these cases have strong similarities, it is helpful to distinguish them as they generalize in different ways when the crucial assumptions are changed:&lt;br /&gt;
&lt;br /&gt;
虽然这些案例有很多相似之处，但是当关键假设发生变化时，我们需要对它们以不同的方式进行归纳总结，因此区分它们是有帮助的:&lt;br /&gt;
* When a system is in thermodynamic equilibrium with respect to both energy exchange ''and particle exchange'', the requirement of fixed composition is relaxed and a [[grand canonical ensemble]] is obtained rather than canonical ensemble. On the other hand, if both composition and energy are fixed, then a [[microcanonical ensemble]] applies instead.&lt;br /&gt;
* 当一个系统在能量交换和粒子交换方面都处于热力学平衡时，固定组成的要求就放宽了。这时我们就得到了一个[[Index.php?title=Microcanonical ensemble|巨正则系综]]而不是正则系综。另一方面，如果成分和能量都是固定的，则可以使用[[微正则系综Index.php?title=Microcanonical ensemble|微正则系综]]。&lt;br /&gt;
&lt;br /&gt;
* If the subsystems within a collection ''do'' interact with each other, then the expected frequencies of subsystem states no longer follow a Boltzmann distribution, and even may not have an [[analytical solution]].&amp;lt;ref name=&amp;quot;:4&amp;quot;&amp;gt;A classic example of this is [[magnetic ordering]]. Systems of non-interacting [[spin (physics)|spins]] show [[paramagnetic]] behaviour that can be understood with a single-particle canonical ensemble (resulting in the [[Brillouin function]]). Systems of ''interacting'' spins can show much more complex behaviour such as [[ferromagnetism]] or [[antiferromagnetism]].&amp;lt;/ref&amp;gt; The canonical ensemble can however still be applied to the ''collective'' states of the entire system considered as a whole, provided the entire system is isolated and in thermal equilibrium.&lt;br /&gt;
* 如果集合中的子系统确实相互交互，则子系统状态的预期频率不再遵循玻尔兹曼 分布，甚至可能没有解析解。&amp;lt;ref name=&amp;quot;:4&amp;quot; /&amp;gt;然而，如果整个系统是独立的并且处于热平衡状态，则正则系综仍然可以应用于作为一个整体考虑。&lt;br /&gt;
&lt;br /&gt;
* With ''[[quantum mechanics|quantum]]'' gases of non-interacting particles in equilibrium, the number of particles found in a given single-particle state does not follow Maxwell–Boltzmann statistics, and there is no simple closed form expression for quantum gases in the canonical ensemble. In the grand canonical ensemble the state-filling statistics of quantum gases are described by [[Fermi–Dirac statistics]] or [[Bose–Einstein statistics]], depending on whether the particles are [[fermion]]s or [[boson]]s respectively.&lt;br /&gt;
* 对于处于平衡状态的非相互作用粒子的量子气体，在给定的单粒子状态中发现的粒子数量并不遵循麦克斯韦-玻尔兹曼统计。并且正则系综中的量子气体没有简单的封闭表达式。在巨正则系综中，量子气体的统计分布状态由费米-狄拉克统计或玻色-爱因斯坦统计来描述，具体则取决于该粒子是费米子还是玻色子。&lt;br /&gt;
&lt;br /&gt;
== 数学 ==&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
In more general mathematical settings, the Boltzmann distribution is also known as the [[Gibbs measure]]. In statistics and machine learning, it is called a [[log-linear model]]. In [[deep learning]], the Boltzmann distribution is used in the sampling distribution of [[stochastic neural network]]s such as the [[Boltzmann machine]], [[Restricted Boltzmann machine]], [[Energy based model|Energy-Based models]] and [[Deep Boltzmann Machine|deep Boltzmann machine]]&lt;br /&gt;
&lt;br /&gt;
在更一般的数学环境中，玻尔兹曼分布也被称为吉布斯量度。在统计学和机器学习中，它被称为对数线性回归。在深度学习中，玻尔兹曼分布被用于随机神经网络的抽样分布，如玻尔兹曼机、受限玻尔兹曼机、基于能量的模型和深度波茨曼机。&lt;br /&gt;
&lt;br /&gt;
== 经济 ==&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The Boltzmann distribution can be introduced to allocate permits in emissions trading.&amp;lt;ref name=&amp;quot;Park, J.-W. 2012&amp;quot;&amp;gt;Park, J.-W., Kim, C. U. and Isard, W. (2012) Permit allocation in emissions trading using the Boltzmann distribution. Physica A 391: 4883–4890&amp;lt;/ref&amp;gt;&amp;lt;ref name=&amp;quot;:5&amp;quot;&amp;gt;[http://www.technologyreview.com/view/425051/the-thorny-problem-of-fair-allocation/ The Thorny Problem Of Fair Allocation]. ''Technology Review'' blog. August 17, 2011. Cites and summarizes Park, Kim and Isard (2012).&amp;lt;/ref&amp;gt; The new allocation method using the Boltzmann distribution can describe the most probable, natural, and unbiased distribution of emissions permits among multiple countries. Simple and versatile, this new method holds potential for many economic and environmental applications.&lt;br /&gt;
&lt;br /&gt;
在经济学中，玻尔兹曼分布被用来分配排放交易中的许可。&amp;lt;ref name=&amp;quot;Park, J.-W. 2012&amp;quot; /&amp;gt;&amp;lt;ref name=&amp;quot;:5&amp;quot; /&amp;gt;  使用玻尔兹曼分布的新分配方法可以创造出在多个国家之间最可能的、自然的和无偏见的排放许可分配。这种新方法简单而通用，在经济和环保中有很大的应用潜力。&lt;br /&gt;
&lt;br /&gt;
The Boltzmann distribution has the same form as the [[Multinomial logistic regression|multinomial logit]] model. As a [[discrete choice]] model, this is very well known in economics since [[Daniel McFadden]] made the connection to random utility maximization.&lt;br /&gt;
&lt;br /&gt;
玻尔兹曼分布与多项逻辑回归模型具有相同的形式。在丹尼尔 · 麦克法登将它与随机效用最大化联系起来之后，成为了大家所熟知的一种离散选择模型。&lt;br /&gt;
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Category:Statistical mechanics&lt;br /&gt;
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类别: 统计力学&lt;br /&gt;
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本中文词条由[[用户:费米子|tueryeye]]编辑，欢迎在讨论页面留言。&lt;br /&gt;
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==See also==&lt;br /&gt;
&lt;br /&gt;
Distribution&lt;br /&gt;
&lt;br /&gt;
分布&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:Boltzmann distribution]]. Its edit history can be viewed at [[玻尔兹曼分布/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>
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&lt;div&gt;li此词条暂由彩云小译翻译，翻译字数共1452，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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{{Use American English|date = March 2019}}&lt;br /&gt;
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{{Short description|Probability distribution of energy states of a system}}&lt;br /&gt;
&lt;br /&gt;
{{about|system energy states|particle energy levels and velocities|Maxwell–Boltzmann distribution}}&lt;br /&gt;
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[[File:Boltzmann distribution graph.svg|upright=1.75|right|thumb|Boltzmann factor ''p&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;''&amp;amp;nbsp;/&amp;amp;nbsp;''p&amp;lt;sub&amp;gt;j&amp;lt;/sub&amp;gt;'' (vertical axis) as a function of temperature ''T'' for several energy differences ''ε&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;''&amp;amp;nbsp;−&amp;amp;nbsp;''ε&amp;lt;sub&amp;gt;j&amp;lt;/sub&amp;gt;''.|链接=Special:FilePath/Boltzmann_distribution_graph.svg]]&lt;br /&gt;
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In [[statistical mechanics]] and [[mathematics]], a '''Boltzmann distribution''' (also called '''Gibbs distribution'''&amp;lt;ref name=&amp;quot;landau&amp;quot;&amp;gt;{{cite book | author=Landau, Lev Davidovich |author2=Lifshitz, Evgeny Mikhailovich |name-list-style=amp | title=Statistical Physics |volume=5 |series=Course of Theoretical Physics |edition=3 |origyear=1976 |year=1980 |place=Oxford |publisher=Pergamon Press|isbn=0-7506-3372-7|author-link=Lev Landau |author2-link=Evgeny Lifshitz }} Translated by J.B. Sykes and M.J. Kearsley. See section 28&amp;lt;/ref&amp;gt;) is a [[probability distribution]] or [[probability measure]] that gives the probability that a system will be in a certain [[microstate (statistical mechanics)|state]] as a function of that state's energy and the temperature of the system. The distribution is expressed in the form:&lt;br /&gt;
&lt;br /&gt;
在统计力学和数学中，波兹曼分布分布(也称为吉布斯分布&amp;lt;ref name=&amp;quot;landau&amp;quot; /&amp;gt;)是一个概率分布或机率量测，它给出了一个系统处于某种量子态的概率，这个概率是该状态的能量和系统温度的函数。分布情况以下列形式表示:&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt;p_i \propto e^{-\frac{\varepsilon_i}{kT}}&amp;lt;/math&amp;gt; &lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt;p_i \propto e^{-\frac{\varepsilon_i}{kT}}&amp;lt;/math&amp;gt; &lt;br /&gt;
&lt;br /&gt;
[拉丁语]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
where {{mvar|p&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;}} is the probability of the system being in state {{mvar|i}}, {{mvar|ε&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;}} is the energy of that state, and a constant {{mvar|kT}} of the distribution is the product of [[Boltzmann's constant]] {{mvar|k}} and [[thermodynamic temperature]] {{mvar|T}}. The symbol &amp;lt;math display=&amp;quot;inline&amp;quot;&amp;gt;\propto&amp;lt;/math&amp;gt; denotes [[proportionality (mathematics)|proportionality]] (see {{section link||The distribution}} for the proportionality constant).&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{{mvar|p&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;}} 是其中系统处于状态{{mvar|i}}的概率, {{mvar|ε&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;}} 是该状态的能量，还有关于这个分布的一个常数 {{mvar|kT}} ，它是玻耳兹曼常数{{mvar|k}}和热力学温度 {{mvar|T}} 的乘积。符号 &amp;lt;math display=&amp;quot;inline&amp;quot;&amp;gt;\propto&amp;lt;/math&amp;gt;表示相称性(见附录中的比例常数)。&lt;br /&gt;
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The term system here has a very wide meaning; it can range from a single atom to a macroscopic system such as a [[Natural gas storage|natural gas storage tank]]. Because of this the Boltzmann distribution can be used to solve a very wide variety of problems. The distribution shows that states with lower energy will always have a higher probability of being occupied .&lt;br /&gt;
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这里的术语系统含义广泛; 它可以从单个原子到宏观系统，如天然气储罐。正因为如此，波兹曼分布可以用来解决各种各样的问题。玻尔兹曼分布表明，能量较低的状态被占据的概率总是较高的。&lt;br /&gt;
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The ''ratio'' of probabilities of two states is known as the '''Boltzmann factor''' and characteristically only depends on the states' energy difference:&lt;br /&gt;
&lt;br /&gt;
两种状态的概率之比被称为玻尔兹曼因子，取决于两种状态的能量差:&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt;\frac{p_i}{p_j} = e^{\frac{\varepsilon_j - \varepsilon_i}{kT}}&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[数学][数学]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The Boltzmann distribution is named after [[Ludwig Boltzmann]] who first formulated it in 1868 during his studies of the [[statistical mechanics]] of gases in thermal equilibrium. Boltzmann's statistical work is borne out in his paper “On the Relationship between the Second Fundamental Theorem of the Mechanical Theory of Heat and Probability Calculations Regarding the Conditions for Thermal Equilibrium&amp;quot;&amp;lt;ref&amp;gt;http://crystal.med.upenn.edu/sharp-lab-pdfs/2015SharpMatschinsky_Boltz1877_Entropy17.pdf&amp;lt;/ref&amp;gt;&lt;br /&gt;
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波兹曼分布是根据路德维希·玻尔兹曼1868年在研究统计力学中气体热平衡的时候首次提出的一个公式命名的。波尔兹曼的统计工作在他1877年的论文《论热力学第二基本定理与热平衡条件的概率计算之间的关系》中得到了体现。&amp;lt;ref&amp;gt;“On the Relationship between the Second Fundamental Theorem of the Mechanical Theory of Heat and Probability Calculations Regarding the Conditions for Thermal Equilibrium” Sitzungberichte der Kaiserlichen Akademie der Wissenschaften. Mathematisch-Naturwissen Classe. Abt. II, LXXVI 1877, pp 373-435 (Wien. Ber. 1877, 76:373-435). &amp;lt;/ref&amp;gt;&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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  It would be nice to have a citation here! The origin of the Boltzmann factor isn't entirely clear. According to some authors, Boltzmann's 1968 paper “On the Relationship between the Second Fundamental Theorem of the Mechanical Theory of Heat and Probability Calculations Regarding the Conditions for Thermal Equilibrium”&lt;br /&gt;
&lt;br /&gt;
  It would be nice to have a citation here! The origin of the Boltzmann factor isn't entirely clear. According to some authors, Boltzmann's 1968 paper “On the Relationship between the Second Fundamental Theorem of the Mechanical Theory of Heat and Probability Calculations Regarding the Conditions for Thermal Equilibrium”&lt;br /&gt;
&lt;br /&gt;
如果能在这里引用一下就好了！玻尔兹曼因子的起源并不完全清楚。根据一些作者的说法，Boltzmann 在1968年发表的论文《论热力学第二基本定理与热平衡条件的概率计算之间的关系》&lt;br /&gt;
&lt;br /&gt;
  &amp;quot;Studien über das Gleichgewicht der lebendigen Kraft zwischen bewegten materiellen Punkten&amp;quot; is the origin but I can't find this article at the moment,&lt;br /&gt;
&lt;br /&gt;
  &amp;quot;Studien über das Gleichgewicht der lebendigen Kraft zwischen bewegten materiellen Punkten&amp;quot; is the origin but I can't find this article at the moment,&lt;br /&gt;
&lt;br /&gt;
  &amp;quot;Studien über das Gleichgewicht der lebendigen Kraft zwischen bewegten materiellen Punkten&amp;quot; is the origin but I can't find this article at the moment,&lt;br /&gt;
&lt;br /&gt;
  so I cannot confirm.&lt;br /&gt;
&lt;br /&gt;
  so I cannot confirm.&lt;br /&gt;
&lt;br /&gt;
所以我不能确定。&lt;br /&gt;
&lt;br /&gt;
  For example, this book says so, but uses suspiciously modern terminology&lt;br /&gt;
&lt;br /&gt;
  For example, this book says so, but uses suspiciously modern terminology&lt;br /&gt;
&lt;br /&gt;
例如，这本书是这么说的，但是使用了可疑的现代术语&lt;br /&gt;
&lt;br /&gt;
    http://books.google.es/books?id=u13KiGlz2zcC&amp;amp;lpg=PA92&amp;amp;ots=8H1DRURdxn&amp;amp;pg=PA93#v=onepage&amp;amp;f=false&lt;br /&gt;
&lt;br /&gt;
    http://books.google.es/books?id=u13KiGlz2zcC&amp;amp;lpg=PA92&amp;amp;ots=8H1DRURdxn&amp;amp;pg=PA93#v=onepage&amp;amp;f=false&lt;br /&gt;
&lt;br /&gt;
Http://books.google.es/books?id=u13kiglz2zcc&amp;amp;lpg=pa92&amp;amp;ots=8h1drurdxn&amp;amp;pg=pa93#v=onepage&amp;amp;f=false&lt;br /&gt;
&lt;br /&gt;
  On the other hand, Uffink's &amp;quot;Compendium of the foundations of classical statistical physics&amp;quot; does not seem to indicate quite this equation but rather that Boltzmann's 1968 distribution was the simple Maxwell–Boltzmann distribution (for a classical nonrelativistic gas), modified for particles in a potential.&lt;br /&gt;
&lt;br /&gt;
  On the other hand, Uffink's &amp;quot;Compendium of the foundations of classical statistical physics&amp;quot; does not seem to indicate quite this equation but rather that Boltzmann's 1968 distribution was the simple Maxwell–Boltzmann distribution (for a classical nonrelativistic gas), modified for particles in a potential.&lt;br /&gt;
&lt;br /&gt;
另一方面，Uffink 的“经典统计物理学基础纲要”似乎并没有完全表明这个方程，而是说 Boltzmann 在1968年的分布是简单的 Maxwell-波兹曼分布(用于经典的非气体) ，修改为势中的粒子。&lt;br /&gt;
&lt;br /&gt;
--&amp;gt; &lt;br /&gt;
&lt;br /&gt;
--&amp;gt; &lt;br /&gt;
&lt;br /&gt;
--&amp;gt;&lt;br /&gt;
&lt;br /&gt;
The distribution was later investigated extensively, in its modern generic form, by [[Josiah Willard Gibbs]] in 1902.&amp;lt;ref name=&amp;quot;gibbs&amp;quot;&amp;gt;{{cite book |last=Gibbs |first=Josiah Willard |authorlink=Josiah Willard Gibbs |title=Elementary Principles in Statistical Mechanics |year=1902 |publisher=[[Charles Scribner's Sons]] &lt;br /&gt;
&lt;br /&gt;
The distribution was later investigated extensively, in its modern generic form, by Josiah Willard Gibbs in 1902.&lt;br /&gt;
&lt;br /&gt;
这种分布后来在1902年由约西亚·威拉德·吉布斯进行了广泛的调查，以其现代通用形式。&lt;br /&gt;
&lt;br /&gt;
|location=New York|title-link=Elementary Principles in Statistical Mechanics }}&amp;lt;/ref&amp;gt;{{rp|Ch.IV}}、&lt;br /&gt;
&lt;br /&gt;
在玻尔兹曼分布被发明之后，约西亚·华纳德·吉布森充分地研究了它并在1902年提出了它的一般形式。&amp;lt;ref name=&amp;quot;gibbs&amp;quot; /&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The generalized Boltzmann distribution is a sufficient and necessary condition for the equivalence between the statistical mechanics definition of [[entropy]] (The [[Entropy_(statistical_thermodynamics)#Gibbs_entropy_formula | Gibbs entropy formula]] &amp;lt;math&amp;gt;S = -k_{\mathrm{B}}\sum_i p_i \log p_i&amp;lt;/math&amp;gt;) and the thermodynamic definition of entropy (&amp;lt;math&amp;gt;d S = \frac{\delta Q_\text{rev}}{T}&amp;lt;/math&amp;gt;, and the [[fundamental thermodynamic relation]]).&amp;lt;ref name=&amp;quot;:0&amp;quot;&amp;gt;{{cite journal |last1= Gao |first1= Xiang |last2= Gallicchio |first2= Emilio |first3= Adrian |last3= Roitberg  |date= 2019 |title= The generalized Boltzmann distribution is the only distribution in which the Gibbs-Shannon entropy equals the thermodynamic entropy |journal= The Journal of Chemical Physics|volume= 151|issue= 3|pages= 034113|doi= 10.1063/1.5111333|pmid= 31325924 |arxiv= 1903.02121 |s2cid= 118981017 }}&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
广义波兹曼分布是熵的统计力学定义(吉布斯熵公式  &amp;lt;math&amp;gt;S = -k_{\mathrm{B}}\sum_i p_i \log p_i&amp;lt;/math&amp;gt;))与熵的热力学定义(&amp;lt;math&amp;gt;d S = \frac{\delta Q_\text{rev}}{T}&amp;lt;/math&amp;gt;)等价的充要条件。&amp;lt;ref name=&amp;quot;:0&amp;quot; /&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The Boltzmann distribution should not be confused with the [[Maxwell–Boltzmann distribution]]. The former gives the probability that a system will be in a certain state as a function of that state's energy;&amp;lt;ref name=&amp;quot;Atkins, P. W. 2010&amp;quot;&amp;gt;Atkins, P. W. (2010) Quanta, W. H. Freeman and Company, New York&amp;lt;/ref&amp;gt; in contrast, the latter is used to describe particle speeds in idealized gases.&lt;br /&gt;
&lt;br /&gt;
值得一提的是，玻尔兹曼分布不应与麦克斯韦-玻尔兹曼分布混淆。前者给出了系统处于某种状态的概率，作为该状态能量的函数; 后者则是用于描述理想气体中的粒子速度。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==分布==&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The Boltzmann distribution is a [[probability distribution]] that gives the probability of a certain state as a function of that state's energy and  temperature of the [[system]] to which the distribution is applied.&amp;lt;ref name=&amp;quot;McQuarrie, A. 2000&amp;quot;&amp;gt;McQuarrie, A. (2000) Statistical Mechanics, University Science Books, California&amp;lt;/ref&amp;gt; It is given as&lt;br /&gt;
&lt;br /&gt;
波兹曼分布是一个概率分布，它给出了出于某种量子态处于某种能量和温度的时候的概率。它被这样定义：&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
《数学》&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
p_i=\frac{1}{Q}} {e^{- {\varepsilon}_i / k T}=\frac{e^{- {\varepsilon}_i / k T}}{\sum_{j=1}^{M}{e^{- {\varepsilon}_j / k T}}}&lt;br /&gt;
&lt;br /&gt;
P _ i = frac {1}{ q }{ e ^ {-{ varepsilon } _ i/k t } = frac { e ^ {-{ varepsilon } _ i/k t }{ sum { j = 1} ^ { m }{ e ^ {-{ varepsilon } _ j/k t }}}}}&lt;br /&gt;
&lt;br /&gt;
p_i=\frac{1}{Q}} {e^{- {\varepsilon}_i / k T}=\frac{e^{- {\varepsilon}_i / k T}}{\sum_{j=1}^{M}{e^{- {\varepsilon}_j / k T}}}&lt;br /&gt;
&lt;br /&gt;
&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
数学&lt;br /&gt;
&lt;br /&gt;
&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
where ''p&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;'' is the probability of state ''i'', ''ε&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;'' the energy of state ''i'', ''k'' the Boltzmann constant, ''T'' the temperature of the system and ''M'' is the number of all states accessible to the system of interest.&amp;lt;ref name=&amp;quot;McQuarrie, A. 2000&amp;quot; /&amp;gt;&amp;lt;ref name=&amp;quot;Atkins, P. W. 2010&amp;quot; /&amp;gt; Implied parentheses around the denominator ''kT'' are omitted for brevity. The normalization denominator ''Q'' (denoted by some authors by ''Z'') is the [[canonical partition function]]&lt;br /&gt;
&lt;br /&gt;
其中 ''p&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;'' 是状态 i 的概率，''ε&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;'' 是状态 i 的能量，''k'' 是波兹曼常数，''T'' 是系统的温度，''M'' 是系统所能到达的所有量子态的数目。&amp;lt;ref name=&amp;quot;Atkins, P. W. 2010&amp;quot; /&amp;gt; &amp;lt;ref name=&amp;quot;McQuarrie, A. 2000&amp;quot; /&amp;gt;这里为了简洁美观，省略了''kT''周围的括弧。归一化的分母''Q''（被有些作者写为''Z''）是对于系统中所有量子态进行总和，此部分又被称为[[Index.php?title=Canonical partition function|正则配分函数]]''。''&lt;br /&gt;
&lt;br /&gt;
It results from the constraint that the probabilities of all accessible states must add up to 1.&lt;br /&gt;
&lt;br /&gt;
所有量子态的概率之和为1.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The Boltzmann distribution is the distribution that maximizes the [[entropy]]，&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt;H(p_1,p_2,\cdots,p_M) = -\sum_{i=1}^{M} p_i\log_2 p_i&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&amp;lt;nowiki&amp;gt;subject to the constraint that {\sum{p_i {\varepsilon}_i}} equals a particular mean energy value (which can be proven using &amp;lt;/nowiki&amp;gt;[[Lagrange multipliers]]).&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&amp;lt;nowiki&amp;gt;当 {\sum{p_i {\varepsilon}_i}} 等于平均能量值时，玻尔兹曼分布是这种情况下能让熵最大化的分布。我们可以通过拉格朗日乘数法来证明。&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The partition function can be calculated if we know the energies of the states accessible to the system of interest. For atoms the partition function values can be found in the NIST Atomic Spectra Database.&amp;lt;ref name=&amp;quot;:1&amp;quot;&amp;gt;[http://physics.nist.gov/PhysRefData/ASD/levels_form.html NIST Atomic Spectra Database Levels Form] at nist.gov&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
在知道量子态能量的情况下，这个配分函数可以被计算。对于原子来说，配分函数的值可以在NIST Atomic Spectra Database中找到。&amp;lt;ref name=&amp;quot;:1&amp;quot; /&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The distribution shows that states with lower energy will always have a higher probability of being occupied than the states with higher energy. It can also give us the quantitative relationship between the probabilities of the two states being occupied. The ratio of probabilities for states i and j is given as&lt;br /&gt;
&lt;br /&gt;
玻尔兹曼分布指出，能量低的量子态总是有比能量高的量子态更高的概率被粒子占据。它同时也能让我们定量地比较两个量子态分布概率的关系。状态 i 和状态 j 的概率比为&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
{\frac{p_i}{p_j}}=e^{({\varepsilon}_j-{\varepsilon}_i) / k T}&lt;br /&gt;
&lt;br /&gt;
&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;nowiki&amp;gt;{\frac{p_i}{p_j}}=e^{({\varepsilon}_j-{\varepsilon}_i) / k T}&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;nowiki&amp;gt;{\frac{p_i}{p_j}}=e^{({\varepsilon}_j-{\varepsilon}_i) / k T}&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&amp;lt;nowiki&amp;gt;&amp;lt;/math&amp;gt;&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
&lt;br /&gt;
数学&lt;br /&gt;
&lt;br /&gt;
where p&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt; is the probability of state i,  p&amp;lt;sub&amp;gt;j&amp;lt;/sub&amp;gt; the probability of state j, and ε&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt; and ε&amp;lt;sub&amp;gt;j&amp;lt;/sub&amp;gt; are the energies of states i and j, respectively.&lt;br /&gt;
&lt;br /&gt;
其中 p&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt; 是量子态 i 的概率， p&amp;lt;sub&amp;gt;j&amp;lt;/sub&amp;gt; 是量子态 j 的概率，ε&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt; 和 ε&amp;lt;sub&amp;gt;j&amp;lt;/sub&amp;gt; 分别是状态 i 和 j 的能量。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The Boltzmann distribution is often used to describe the distribution of particles, such as atoms or molecules, over energy states accessible to them. If we have a system consisting of many particles, the probability of a particle being in state i is practically the probability that, if we pick a random particle from that system and check what state it is in, we will find it is in state i. This probability is equal to the number of particles in state i divided by the total number of particles in the system, that is the fraction of particles that occupy state i.&lt;br /&gt;
&lt;br /&gt;
玻尔兹曼分布通常被用来描述粒子的分布，比如原子或分子，在能量状态上的分布情况。如果我们有一个由许多粒子组成的系统，某个粒子处于量子态 i 的概率就等同于当我们从该系统中选择一个随机的粒子并观察它处于什么状态，发现它处于状态 i 的概率。这个概率等于量子态 i 的粒子数除以系统中粒子的总数，即那些占据量子态i的粒子的比例。&lt;br /&gt;
&lt;br /&gt;
&amp;lt;nowiki&amp;gt;&amp;lt;math display=&amp;quot;inline&amp;quot;&amp;gt;&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;nowiki&amp;gt;p_i={\frac{N_i}{N}}&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
&lt;br /&gt;
P _ i = { frac { n _ i }{ n }&lt;br /&gt;
&lt;br /&gt;
&amp;lt;nowiki&amp;gt;{\sum{p_i {\varepsilon}_i}}&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
where N&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt; is the number of particles in state i and N is the total number of particles in the system. We may use the Boltzmann distribution to find this probability that is, as we have seen, equal to the fraction of particles that are in state i. So the equation that gives the fraction of particles in state i as a function of the energy of that state is&lt;br /&gt;
&lt;br /&gt;
&amp;lt;nowiki&amp;gt;&amp;lt;/math&amp;gt;&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
&lt;br /&gt;
《数学公式丢失了》&lt;br /&gt;
&lt;br /&gt;
N&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt; 是位于量子态 i 的粒子数，N是系统中粒子的总数。我们可以用波兹曼分布来求出这个概率，它等于处于量子态i的粒子的比例。所以这个方程给出位于量子态 i 的粒子比例关于这个状态能量的函数&amp;lt;ref name=&amp;quot;Atkins, P. W. 2010&amp;quot; /&amp;gt;。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
This equation is of great importance to [[spectroscopy]]. In spectroscopy we observe a [[spectral line]] of atoms or molecules that we are interested in going from one state to another.&amp;lt;ref name=&amp;quot;Atkins, P. W. 2010&amp;quot; /&amp;gt;&amp;lt;ref name=&amp;quot;:2&amp;quot;&amp;gt;Atkins, P. W.; de Paula J. (2009) Physical Chemistry, 9th edition, Oxford University Press, Oxford, UK&amp;lt;/ref&amp;gt; In order for this to be possible, there must be some particles in the first state to undergo the transition. We may find that this condition is fulfilled by finding the fraction of particles in the first state. If it is negligible, the transition is very likely not to be observed at the temperature for which the calculation was done. In general, a larger fraction of molecules in the first state means a higher number of transitions to the second state.&amp;lt;ref name=&amp;quot;:3&amp;quot;&amp;gt;Skoog, D. A.; Holler, F. J.; Crouch, S. R. (2006) Principles of Instrumental Analysis, Brooks/Cole, Boston, MA&amp;lt;/ref&amp;gt; This gives a stronger spectral line. However, there are other factors that influence the intensity of a spectral line, such as whether it is caused by an allowed or a [[forbidden transition]]&lt;br /&gt;
&lt;br /&gt;
对于光谱学来说这很重要在。在光谱中，我们期待能观察到一条原子或分子跃迁的谱线。&amp;lt;ref name=&amp;quot;Atkins, P. W. 2010&amp;quot; /&amp;gt;&amp;lt;ref name=&amp;quot;:2&amp;quot; /&amp;gt; 在为了使这成为可能，必须有一些粒子处于第一个量子态，等待着发生跃迁。我们可以通过求第一态粒子的比例来满足这个条件。如果它可以忽略不计，那么在当前计算的温度下，则很难观察到这种跃迁。一般来说，处于第一状态的分子比例越大，意味着向第二状态跃迁的次数越多。&amp;lt;ref name=&amp;quot;:3&amp;quot; /&amp;gt;这就产生了一条更强的谱线。然而，还有其他因素影响谱线的强度，例如它是否是被允许的跃迁还是被禁止的跃迁。&lt;br /&gt;
&lt;br /&gt;
The Boltzmann distribution is related to the [[softmax function]] commonly used in machine learning.&lt;br /&gt;
&lt;br /&gt;
玻尔兹曼分布与机器学习中常用的[[Index.php?title=Softmax function|归一化指数函数]]（Softmax 函数）有关。&lt;br /&gt;
=='''统计力学''' ==&lt;br /&gt;
&lt;br /&gt;
{{main|Canonical ensemble|Maxwell–Boltzmann statistics}}The Boltzmann distribution appears in statistical mechanics when considering isolated (or nearly-isolated) systems of fixed composition that are in thermal equilibrium (equilibrium with respect to energy exchange). The most general case is the probability distribution for the canonical ensemble, but also some special cases (derivable from the canonical ensemble) also show the Boltzmann distribution in different aspects:&lt;br /&gt;
&lt;br /&gt;
当独立的(或者几乎独立的)固定体系处于统计力学热平衡状态时，玻尔兹曼分布就会出现。最普遍的情况是概率分布的正则系综，但也有一些特殊的情况(从正则系综衍生)也显示了不同形式的玻尔兹曼分布:&lt;br /&gt;
&lt;br /&gt;
; [[Canonical ensemble]] (general case)&lt;br /&gt;
; '''正则系综(一般情况)'''&lt;br /&gt;
; '''The [[canonical ensemble]] gives the [[probabilities]] of the various possible states of a closed system of fixed volume, in thermal equilibrium with a [[heat bath]]. The canonical ensemble is a probability distribution with the Boltzmann form.'''&lt;br /&gt;
&lt;br /&gt;
正则系综模型给出了在一个封闭固定体积，带有热浴的热平衡系统中的各种可能状态的概率。我们称正则系综为一个玻尔兹曼概率分布。&lt;br /&gt;
&lt;br /&gt;
; &lt;br /&gt;
; Statistical frequencies of subsystems' states (in a non-interacting collection)&lt;br /&gt;
'''子系统状态的统计频率(在一个无交互的集合中)'''&lt;br /&gt;
: When the system of interest is a collection of many non-interacting copies of a smaller subsystem, it is sometimes useful to find the [[statistical frequency]] of a given subsystem state, among the collection. The canonical ensemble has the property of separability when applied to such a collection: as long as the non-interacting subsystems have fixed composition, then each subsystem's state is independent of the others and is also characterized by a canonical ensemble. As a result, the [[expectation value|expected]] statistical frequency distribution of subsystem states has the Boltzmann form.&lt;br /&gt;
&lt;br /&gt;
当系统是一个较小子系统的许多非交互副本的集合时，有时我们需要在某个子系统集合中找到某个子系统的统计频率。当应用于这样一个集合时，这个子系统的正则系综具有可分离性: 只要不相互作用的子系统的组成是固定的，那么每个子系统的状态都是独立于其他子系统的，它们也拥有自己的正则系综。因此，子系统状态的期望统计频率分布形式是玻尔兹曼分布。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[Maxwell–Boltzmann statistics]] of classical gases (systems of non-interacting particles)&lt;br /&gt;
&lt;br /&gt;
'''Maxwell-Boltzmann 统计中的经典气体系统(非相互作用粒子系统)'''&lt;br /&gt;
&lt;br /&gt;
: In particle systems, many particles share the same space and regularly change places with each other; the single-particle state space they occupy is a shared space. [[Maxwell–Boltzmann statistics]] give the expected number of particles found in a given single-particle state, in a [[classical mechanics|classical]] gas of non-interacting particles at equilibrium. This expected number distribution has the Boltzmann form.&lt;br /&gt;
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在粒子系统中，许多粒子共享同一空间，并且相互之间有规律地改变位置; 它们所占据的单粒子状态空间是一个共享空间。[[Index.php?title=Maxwell–Boltzmann statistics|麦克斯韦-玻尔兹曼统计]]给出了在一个给定的单粒子态，在一个处于平衡状态的非相互作用粒子的经典气体中所发现的粒子的预期数量。这个预期的数量分布具有玻尔兹曼分布形式。&lt;br /&gt;
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Although these cases have strong similarities, it is helpful to distinguish them as they generalize in different ways when the crucial assumptions are changed:&lt;br /&gt;
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虽然这些案例有很多相似之处，但是当关键假设发生变化时，我们需要对它们以不同的方式进行归纳总结，因此区分它们是有帮助的:&lt;br /&gt;
* When a system is in thermodynamic equilibrium with respect to both energy exchange ''and particle exchange'', the requirement of fixed composition is relaxed and a [[grand canonical ensemble]] is obtained rather than canonical ensemble. On the other hand, if both composition and energy are fixed, then a [[microcanonical ensemble]] applies instead.&lt;br /&gt;
* 当一个系统在能量交换和粒子交换方面都处于热力学平衡时，固定组成的要求就放宽了。这时我们就得到了一个[[Index.php?title=Microcanonical ensemble|巨正则系综]]而不是正则系综。另一方面，如果成分和能量都是固定的，则可以使用[[微正则系综Index.php?title=Microcanonical ensemble|微正则系综]]。&lt;br /&gt;
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* If the subsystems within a collection ''do'' interact with each other, then the expected frequencies of subsystem states no longer follow a Boltzmann distribution, and even may not have an [[analytical solution]].&amp;lt;ref name=&amp;quot;:4&amp;quot;&amp;gt;A classic example of this is [[magnetic ordering]]. Systems of non-interacting [[spin (physics)|spins]] show [[paramagnetic]] behaviour that can be understood with a single-particle canonical ensemble (resulting in the [[Brillouin function]]). Systems of ''interacting'' spins can show much more complex behaviour such as [[ferromagnetism]] or [[antiferromagnetism]].&amp;lt;/ref&amp;gt; The canonical ensemble can however still be applied to the ''collective'' states of the entire system considered as a whole, provided the entire system is isolated and in thermal equilibrium.&lt;br /&gt;
* 如果集合中的子系统确实相互交互，则子系统状态的预期频率不再遵循玻尔兹曼 分布，甚至可能没有解析解。&amp;lt;ref name=&amp;quot;:4&amp;quot; /&amp;gt;然而，如果整个系统是独立的并且处于热平衡状态，则正则系综仍然可以应用于作为一个整体考虑。&lt;br /&gt;
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* With ''[[quantum mechanics|quantum]]'' gases of non-interacting particles in equilibrium, the number of particles found in a given single-particle state does not follow Maxwell–Boltzmann statistics, and there is no simple closed form expression for quantum gases in the canonical ensemble. In the grand canonical ensemble the state-filling statistics of quantum gases are described by [[Fermi–Dirac statistics]] or [[Bose–Einstein statistics]], depending on whether the particles are [[fermion]]s or [[boson]]s respectively.&lt;br /&gt;
* 对于处于平衡状态的非相互作用粒子的量子气体，在给定的单粒子状态中发现的粒子数量并不遵循麦克斯韦-玻尔兹曼统计。并且正则系综中的量子气体没有简单的封闭表达式。在巨正则系综中，量子气体的统计分布状态由费米-狄拉克统计或玻色-爱因斯坦统计来描述，具体则取决于该粒子是费米子还是玻色子。&lt;br /&gt;
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== 数学 ==&lt;br /&gt;
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In more general mathematical settings, the Boltzmann distribution is also known as the [[Gibbs measure]]. In statistics and machine learning, it is called a [[log-linear model]]. In [[deep learning]], the Boltzmann distribution is used in the sampling distribution of [[stochastic neural network]]s such as the [[Boltzmann machine]], [[Restricted Boltzmann machine]], [[Energy based model|Energy-Based models]] and [[Deep Boltzmann Machine|deep Boltzmann machine]]&lt;br /&gt;
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在更一般的数学环境中，玻尔兹曼分布也被称为吉布斯量度。在统计学和机器学习中，它被称为对数线性回归。在深度学习中，玻尔兹曼分布被用于随机神经网络的抽样分布，如玻尔兹曼机、受限玻尔兹曼机、基于能量的模型和深度波茨曼机。&lt;br /&gt;
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== 经济 ==&lt;br /&gt;
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The Boltzmann distribution can be introduced to allocate permits in emissions trading.&amp;lt;ref name=&amp;quot;Park, J.-W. 2012&amp;quot;&amp;gt;Park, J.-W., Kim, C. U. and Isard, W. (2012) Permit allocation in emissions trading using the Boltzmann distribution. Physica A 391: 4883–4890&amp;lt;/ref&amp;gt;&amp;lt;ref name=&amp;quot;:5&amp;quot;&amp;gt;[http://www.technologyreview.com/view/425051/the-thorny-problem-of-fair-allocation/ The Thorny Problem Of Fair Allocation]. ''Technology Review'' blog. August 17, 2011. Cites and summarizes Park, Kim and Isard (2012).&amp;lt;/ref&amp;gt; The new allocation method using the Boltzmann distribution can describe the most probable, natural, and unbiased distribution of emissions permits among multiple countries. Simple and versatile, this new method holds potential for many economic and environmental applications.&lt;br /&gt;
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在经济学中，玻尔兹曼分布被用来分配排放交易中的许可。&amp;lt;ref name=&amp;quot;Park, J.-W. 2012&amp;quot; /&amp;gt;&amp;lt;ref name=&amp;quot;:5&amp;quot; /&amp;gt;  使用玻尔兹曼分布的新分配方法可以创造出在多个国家之间最可能的、自然的和无偏见的排放许可分配。这种新方法简单而通用，在经济和环保中有很大的应用潜力。&lt;br /&gt;
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The Boltzmann distribution has the same form as the [[Multinomial logistic regression|multinomial logit]] model. As a [[discrete choice]] model, this is very well known in economics since [[Daniel McFadden]] made the connection to random utility maximization.&lt;br /&gt;
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玻尔兹曼分布与多项逻辑回归模型具有相同的形式。在丹尼尔 · 麦克法登将它与随机效用最大化联系起来之后，成为了大家所熟知的一种离散选择模型。&lt;br /&gt;
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Category:Statistical mechanics&lt;br /&gt;
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类别: 统计力学&lt;br /&gt;
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本中文词条由[[用户:费米子|tueryeye]]编辑，欢迎在讨论页面留言。&lt;br /&gt;
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==See also==&lt;br /&gt;
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Distribution&lt;br /&gt;
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分布&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:Boltzmann distribution]]. Its edit history can be viewed at [[玻尔兹曼分布/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>
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&lt;div&gt;li此词条暂由彩云小译翻译，翻译字数共1452，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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{{Use American English|date = March 2019}}&lt;br /&gt;
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{{Short description|Probability distribution of energy states of a system}}&lt;br /&gt;
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{{about|system energy states|particle energy levels and velocities|Maxwell–Boltzmann distribution}}&lt;br /&gt;
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[[File:Boltzmann distribution graph.svg|upright=1.75|right|thumb|Boltzmann factor ''p&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;''&amp;amp;nbsp;/&amp;amp;nbsp;''p&amp;lt;sub&amp;gt;j&amp;lt;/sub&amp;gt;'' (vertical axis) as a function of temperature ''T'' for several energy differences ''ε&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;''&amp;amp;nbsp;−&amp;amp;nbsp;''ε&amp;lt;sub&amp;gt;j&amp;lt;/sub&amp;gt;''.|链接=Special:FilePath/Boltzmann_distribution_graph.svg]]&lt;br /&gt;
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In [[statistical mechanics]] and [[mathematics]], a '''Boltzmann distribution''' (also called '''Gibbs distribution'''&amp;lt;ref name=&amp;quot;landau&amp;quot;&amp;gt;{{cite book | author=Landau, Lev Davidovich |author2=Lifshitz, Evgeny Mikhailovich |name-list-style=amp | title=Statistical Physics |volume=5 |series=Course of Theoretical Physics |edition=3 |origyear=1976 |year=1980 |place=Oxford |publisher=Pergamon Press|isbn=0-7506-3372-7|author-link=Lev Landau |author2-link=Evgeny Lifshitz }} Translated by J.B. Sykes and M.J. Kearsley. See section 28&amp;lt;/ref&amp;gt;) is a [[probability distribution]] or [[probability measure]] that gives the probability that a system will be in a certain [[microstate (statistical mechanics)|state]] as a function of that state's energy and the temperature of the system. The distribution is expressed in the form:&lt;br /&gt;
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在统计力学和数学中，波兹曼分布分布(也称为吉布斯分布&amp;lt;ref name=&amp;quot;landau&amp;quot; /&amp;gt;)是一个概率分布或机率量测，它给出了一个系统处于某种量子态的概率，这个概率是该状态的能量和系统温度的函数。分布情况以下列形式表示:&lt;br /&gt;
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:&amp;lt;math&amp;gt;p_i \propto e^{-\frac{\varepsilon_i}{kT}}&amp;lt;/math&amp;gt; &lt;br /&gt;
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&amp;lt;math&amp;gt;p_i \propto e^{-\frac{\varepsilon_i}{kT}}&amp;lt;/math&amp;gt; &lt;br /&gt;
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[拉丁语]&lt;br /&gt;
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where {{mvar|p&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;}} is the probability of the system being in state {{mvar|i}}, {{mvar|ε&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;}} is the energy of that state, and a constant {{mvar|kT}} of the distribution is the product of [[Boltzmann's constant]] {{mvar|k}} and [[thermodynamic temperature]] {{mvar|T}}. The symbol &amp;lt;math display=&amp;quot;inline&amp;quot;&amp;gt;\propto&amp;lt;/math&amp;gt; denotes [[proportionality (mathematics)|proportionality]] (see {{section link||The distribution}} for the proportionality constant).&lt;br /&gt;
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{{mvar|p&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;}} 是其中系统处于状态{{mvar|i}}的概率, {{mvar|ε&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;}} 是该状态的能量，还有关于这个分布的一个常数 {{mvar|kT}} ，它是玻耳兹曼常数{{mvar|k}}和热力学温度 {{mvar|T}} 的乘积。符号 &amp;lt;math display=&amp;quot;inline&amp;quot;&amp;gt;\propto&amp;lt;/math&amp;gt;表示相称性(见附录中的比例常数)。&lt;br /&gt;
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The term system here has a very wide meaning; it can range from a single atom to a macroscopic system such as a [[Natural gas storage|natural gas storage tank]]. Because of this the Boltzmann distribution can be used to solve a very wide variety of problems. The distribution shows that states with lower energy will always have a higher probability of being occupied .&lt;br /&gt;
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这里的术语系统含义广泛; 它可以从单个原子到宏观系统，如天然气储罐。正因为如此，波兹曼分布可以用来解决各种各样的问题。玻尔兹曼分布表明，能量较低的状态被占据的概率总是较高的。&lt;br /&gt;
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The ''ratio'' of probabilities of two states is known as the '''Boltzmann factor''' and characteristically only depends on the states' energy difference:&lt;br /&gt;
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两种状态的概率之比被称为玻尔兹曼因子，取决于两种状态的能量差:&lt;br /&gt;
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:&amp;lt;math&amp;gt;\frac{p_i}{p_j} = e^{\frac{\varepsilon_j - \varepsilon_i}{kT}}&amp;lt;/math&amp;gt;&lt;br /&gt;
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[数学][数学]&lt;br /&gt;
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The Boltzmann distribution is named after [[Ludwig Boltzmann]] who first formulated it in 1868 during his studies of the [[statistical mechanics]] of gases in thermal equilibrium. Boltzmann's statistical work is borne out in his paper “On the Relationship between the Second Fundamental Theorem of the Mechanical Theory of Heat and Probability Calculations Regarding the Conditions for Thermal Equilibrium&amp;quot;&amp;lt;ref&amp;gt;http://crystal.med.upenn.edu/sharp-lab-pdfs/2015SharpMatschinsky_Boltz1877_Entropy17.pdf&amp;lt;/ref&amp;gt;&lt;br /&gt;
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波兹曼分布是根据路德维希·玻尔兹曼1868年在研究统计力学中气体热平衡的时候首次提出的一个公式命名的。波尔兹曼的统计工作在他1877年的论文《论热力学第二基本定理与热平衡条件的概率计算之间的关系》中得到了体现。&amp;lt;ref&amp;gt;“On the Relationship between the Second Fundamental Theorem of the Mechanical Theory of Heat and Probability Calculations Regarding the Conditions for Thermal Equilibrium” Sitzungberichte der Kaiserlichen Akademie der Wissenschaften. Mathematisch-Naturwissen Classe. Abt. II, LXXVI 1877, pp 373-435 (Wien. Ber. 1877, 76:373-435). &amp;lt;/ref&amp;gt;&lt;br /&gt;
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  It would be nice to have a citation here! The origin of the Boltzmann factor isn't entirely clear. According to some authors, Boltzmann's 1968 paper “On the Relationship between the Second Fundamental Theorem of the Mechanical Theory of Heat and Probability Calculations Regarding the Conditions for Thermal Equilibrium”&lt;br /&gt;
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  It would be nice to have a citation here! The origin of the Boltzmann factor isn't entirely clear. According to some authors, Boltzmann's 1968 paper “On the Relationship between the Second Fundamental Theorem of the Mechanical Theory of Heat and Probability Calculations Regarding the Conditions for Thermal Equilibrium”&lt;br /&gt;
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如果能在这里引用一下就好了！玻尔兹曼因子的起源并不完全清楚。根据一些作者的说法，Boltzmann 在1968年发表的论文《论热力学第二基本定理与热平衡条件的概率计算之间的关系》&lt;br /&gt;
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  &amp;quot;Studien über das Gleichgewicht der lebendigen Kraft zwischen bewegten materiellen Punkten&amp;quot; is the origin but I can't find this article at the moment,&lt;br /&gt;
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  &amp;quot;Studien über das Gleichgewicht der lebendigen Kraft zwischen bewegten materiellen Punkten&amp;quot; is the origin but I can't find this article at the moment,&lt;br /&gt;
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  &amp;quot;Studien über das Gleichgewicht der lebendigen Kraft zwischen bewegten materiellen Punkten&amp;quot; is the origin but I can't find this article at the moment,&lt;br /&gt;
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  so I cannot confirm.&lt;br /&gt;
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  so I cannot confirm.&lt;br /&gt;
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所以我不能确定。&lt;br /&gt;
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  For example, this book says so, but uses suspiciously modern terminology&lt;br /&gt;
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  For example, this book says so, but uses suspiciously modern terminology&lt;br /&gt;
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例如，这本书是这么说的，但是使用了可疑的现代术语&lt;br /&gt;
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    http://books.google.es/books?id=u13KiGlz2zcC&amp;amp;lpg=PA92&amp;amp;ots=8H1DRURdxn&amp;amp;pg=PA93#v=onepage&amp;amp;f=false&lt;br /&gt;
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    http://books.google.es/books?id=u13KiGlz2zcC&amp;amp;lpg=PA92&amp;amp;ots=8H1DRURdxn&amp;amp;pg=PA93#v=onepage&amp;amp;f=false&lt;br /&gt;
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Http://books.google.es/books?id=u13kiglz2zcc&amp;amp;lpg=pa92&amp;amp;ots=8h1drurdxn&amp;amp;pg=pa93#v=onepage&amp;amp;f=false&lt;br /&gt;
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  On the other hand, Uffink's &amp;quot;Compendium of the foundations of classical statistical physics&amp;quot; does not seem to indicate quite this equation but rather that Boltzmann's 1968 distribution was the simple Maxwell–Boltzmann distribution (for a classical nonrelativistic gas), modified for particles in a potential.&lt;br /&gt;
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  On the other hand, Uffink's &amp;quot;Compendium of the foundations of classical statistical physics&amp;quot; does not seem to indicate quite this equation but rather that Boltzmann's 1968 distribution was the simple Maxwell–Boltzmann distribution (for a classical nonrelativistic gas), modified for particles in a potential.&lt;br /&gt;
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另一方面，Uffink 的“经典统计物理学基础纲要”似乎并没有完全表明这个方程，而是说 Boltzmann 在1968年的分布是简单的 Maxwell-波兹曼分布(用于经典的非气体) ，修改为势中的粒子。&lt;br /&gt;
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--&amp;gt; &lt;br /&gt;
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--&amp;gt; &lt;br /&gt;
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--&amp;gt;&lt;br /&gt;
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The distribution was later investigated extensively, in its modern generic form, by [[Josiah Willard Gibbs]] in 1902.&amp;lt;ref name=&amp;quot;gibbs&amp;quot;&amp;gt;{{cite book |last=Gibbs |first=Josiah Willard |authorlink=Josiah Willard Gibbs |title=Elementary Principles in Statistical Mechanics |year=1902 |publisher=[[Charles Scribner's Sons]] &lt;br /&gt;
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The distribution was later investigated extensively, in its modern generic form, by Josiah Willard Gibbs in 1902.&lt;br /&gt;
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这种分布后来在1902年由约西亚·威拉德·吉布斯进行了广泛的调查，以其现代通用形式。&lt;br /&gt;
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|location=New York|title-link=Elementary Principles in Statistical Mechanics }}&amp;lt;/ref&amp;gt;{{rp|Ch.IV}}、&lt;br /&gt;
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在玻尔兹曼分布被发明之后，约西亚·华纳德·吉布森充分地研究了它并在1902年提出了它的一般形式。&amp;lt;ref name=&amp;quot;gibbs&amp;quot; /&amp;gt;&lt;br /&gt;
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The generalized Boltzmann distribution is a sufficient and necessary condition for the equivalence between the statistical mechanics definition of [[entropy]] (The [[Entropy_(statistical_thermodynamics)#Gibbs_entropy_formula | Gibbs entropy formula]] &amp;lt;math&amp;gt;S = -k_{\mathrm{B}}\sum_i p_i \log p_i&amp;lt;/math&amp;gt;) and the thermodynamic definition of entropy (&amp;lt;math&amp;gt;d S = \frac{\delta Q_\text{rev}}{T}&amp;lt;/math&amp;gt;, and the [[fundamental thermodynamic relation]]).&amp;lt;ref name=&amp;quot;:0&amp;quot;&amp;gt;{{cite journal |last1= Gao |first1= Xiang |last2= Gallicchio |first2= Emilio |first3= Adrian |last3= Roitberg  |date= 2019 |title= The generalized Boltzmann distribution is the only distribution in which the Gibbs-Shannon entropy equals the thermodynamic entropy |journal= The Journal of Chemical Physics|volume= 151|issue= 3|pages= 034113|doi= 10.1063/1.5111333|pmid= 31325924 |arxiv= 1903.02121 |s2cid= 118981017 }}&amp;lt;/ref&amp;gt;&lt;br /&gt;
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广义波兹曼分布是熵的统计力学定义(吉布斯熵公式  &amp;lt;math&amp;gt;S = -k_{\mathrm{B}}\sum_i p_i \log p_i&amp;lt;/math&amp;gt;))与熵的热力学定义(&amp;lt;math&amp;gt;d S = \frac{\delta Q_\text{rev}}{T}&amp;lt;/math&amp;gt;)等价的充要条件。&amp;lt;ref name=&amp;quot;:0&amp;quot; /&amp;gt;&lt;br /&gt;
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The Boltzmann distribution should not be confused with the [[Maxwell–Boltzmann distribution]]. The former gives the probability that a system will be in a certain state as a function of that state's energy;&amp;lt;ref name=&amp;quot;Atkins, P. W. 2010&amp;quot;&amp;gt;Atkins, P. W. (2010) Quanta, W. H. Freeman and Company, New York&amp;lt;/ref&amp;gt; in contrast, the latter is used to describe particle speeds in idealized gases.&lt;br /&gt;
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值得一提的是，玻尔兹曼分布不应与麦克斯韦-玻尔兹曼分布混淆。前者给出了系统处于某种状态的概率，作为该状态能量的函数; 后者则是用于描述理想气体中的粒子速度。&lt;br /&gt;
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==分布==&lt;br /&gt;
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The Boltzmann distribution is a [[probability distribution]] that gives the probability of a certain state as a function of that state's energy and  temperature of the [[system]] to which the distribution is applied.&amp;lt;ref name=&amp;quot;McQuarrie, A. 2000&amp;quot;&amp;gt;McQuarrie, A. (2000) Statistical Mechanics, University Science Books, California&amp;lt;/ref&amp;gt; It is given as&lt;br /&gt;
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波兹曼分布是一个概率分布，它给出了出于某种量子态处于某种能量和温度的时候的概率。它被这样定义：&lt;br /&gt;
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&amp;lt;math&amp;gt;&lt;br /&gt;
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《数学》&lt;br /&gt;
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:&amp;lt;math&amp;gt;&lt;br /&gt;
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p_i=\frac{1}{Q}} {e^{- {\varepsilon}_i / k T}=\frac{e^{- {\varepsilon}_i / k T}}{\sum_{j=1}^{M}{e^{- {\varepsilon}_j / k T}}}&lt;br /&gt;
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P _ i = frac {1}{ q }{ e ^ {-{ varepsilon } _ i/k t } = frac { e ^ {-{ varepsilon } _ i/k t }{ sum { j = 1} ^ { m }{ e ^ {-{ varepsilon } _ j/k t }}}}}&lt;br /&gt;
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p_i=\frac{1}{Q}} {e^{- {\varepsilon}_i / k T}=\frac{e^{- {\varepsilon}_i / k T}}{\sum_{j=1}^{M}{e^{- {\varepsilon}_j / k T}}}&lt;br /&gt;
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&amp;lt;/math&amp;gt;&lt;br /&gt;
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数学&lt;br /&gt;
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&amp;lt;/math&amp;gt;&lt;br /&gt;
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where ''p&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;'' is the probability of state ''i'', ''ε&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;'' the energy of state ''i'', ''k'' the Boltzmann constant, ''T'' the temperature of the system and ''M'' is the number of all states accessible to the system of interest.&amp;lt;ref name=&amp;quot;McQuarrie, A. 2000&amp;quot; /&amp;gt;&amp;lt;ref name=&amp;quot;Atkins, P. W. 2010&amp;quot; /&amp;gt; Implied parentheses around the denominator ''kT'' are omitted for brevity. The normalization denominator ''Q'' (denoted by some authors by ''Z'') is the [[canonical partition function]]&lt;br /&gt;
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其中 ''p&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;'' 是状态 i 的概率，''ε&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;'' 是状态 i 的能量，''k'' 是波兹曼常数，''T'' 是系统的温度，''M'' 是系统所能到达的所有量子态的数目。&amp;lt;ref name=&amp;quot;Atkins, P. W. 2010&amp;quot; /&amp;gt; &amp;lt;ref name=&amp;quot;McQuarrie, A. 2000&amp;quot; /&amp;gt;这里为了简洁美观，省略了''kT''周围的括弧。归一化的分母''Q''（被有些作者写为''Z''）是对于系统中所有量子态进行总和，此部分又被称为[[Index.php?title=Canonical partition function|正则配分函数]]''。''&lt;br /&gt;
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It results from the constraint that the probabilities of all accessible states must add up to 1.&lt;br /&gt;
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所有量子态的概率之和为1.&lt;br /&gt;
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The Boltzmann distribution is the distribution that maximizes the [[entropy]]，&lt;br /&gt;
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&amp;lt;math&amp;gt;H(p_1,p_2,\cdots,p_M) = -\sum_{i=1}^{M} p_i\log_2 p_i&amp;lt;/math&amp;gt;&lt;br /&gt;
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&amp;lt;nowiki&amp;gt;subject to the constraint that {\sum{p_i {\varepsilon}_i}} equals a particular mean energy value (which can be proven using &amp;lt;/nowiki&amp;gt;[[Lagrange multipliers]]).&lt;br /&gt;
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&amp;lt;nowiki&amp;gt;当 {\sum{p_i {\varepsilon}_i}} 等于平均能量值时，玻尔兹曼分布是这种情况下能让熵最大化的分布。我们可以通过拉格朗日乘数法来证明。&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
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The partition function can be calculated if we know the energies of the states accessible to the system of interest. For atoms the partition function values can be found in the NIST Atomic Spectra Database.&amp;lt;ref name=&amp;quot;:1&amp;quot;&amp;gt;[http://physics.nist.gov/PhysRefData/ASD/levels_form.html NIST Atomic Spectra Database Levels Form] at nist.gov&amp;lt;/ref&amp;gt;&lt;br /&gt;
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在知道量子态能量的情况下，这个配分函数可以被计算。对于原子来说，配分函数的值可以在NIST Atomic Spectra Database中找到。&amp;lt;ref name=&amp;quot;:1&amp;quot; /&amp;gt;&lt;br /&gt;
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The distribution shows that states with lower energy will always have a higher probability of being occupied than the states with higher energy. It can also give us the quantitative relationship between the probabilities of the two states being occupied. The ratio of probabilities for states i and j is given as&lt;br /&gt;
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玻尔兹曼分布指出，能量低的量子态总是有比能量高的量子态更高的概率被粒子占据。它同时也能让我们定量地比较两个量子态分布概率的关系。状态 i 和状态 j 的概率比为&lt;br /&gt;
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:&amp;lt;math&amp;gt;&lt;br /&gt;
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{\frac{p_i}{p_j}}=e^{({\varepsilon}_j-{\varepsilon}_i) / k T}&lt;br /&gt;
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&amp;lt;nowiki&amp;gt;{\frac{p_i}{p_j}}=e^{({\varepsilon}_j-{\varepsilon}_i) / k T}&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
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&amp;lt;nowiki&amp;gt;{\frac{p_i}{p_j}}=e^{({\varepsilon}_j-{\varepsilon}_i) / k T}&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
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&amp;lt;nowiki&amp;gt;&amp;lt;/math&amp;gt;&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
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数学&lt;br /&gt;
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where p&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt; is the probability of state i,  p&amp;lt;sub&amp;gt;j&amp;lt;/sub&amp;gt; the probability of state j, and ε&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt; and ε&amp;lt;sub&amp;gt;j&amp;lt;/sub&amp;gt; are the energies of states i and j, respectively.&lt;br /&gt;
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其中 p&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt; 是量子态 i 的概率， p&amp;lt;sub&amp;gt;j&amp;lt;/sub&amp;gt; 是量子态 j 的概率，ε&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt; 和 ε&amp;lt;sub&amp;gt;j&amp;lt;/sub&amp;gt; 分别是状态 i 和 j 的能量。&lt;br /&gt;
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The Boltzmann distribution is often used to describe the distribution of particles, such as atoms or molecules, over energy states accessible to them. If we have a system consisting of many particles, the probability of a particle being in state i is practically the probability that, if we pick a random particle from that system and check what state it is in, we will find it is in state i. This probability is equal to the number of particles in state i divided by the total number of particles in the system, that is the fraction of particles that occupy state i.&lt;br /&gt;
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玻尔兹曼分布通常被用来描述粒子的分布，比如原子或分子，在能量状态上的分布情况。如果我们有一个由许多粒子组成的系统，某个粒子处于量子态 i 的概率就等同于当我们从该系统中选择一个随机的粒子并观察它处于什么状态，发现它处于状态 i 的概率。这个概率等于量子态 i 的粒子数除以系统中粒子的总数，即那些占据量子态i的粒子的比例。&lt;br /&gt;
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&amp;lt;nowiki&amp;gt;&amp;lt;math display=&amp;quot;inline&amp;quot;&amp;gt;&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
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&amp;lt;nowiki&amp;gt;p_i={\frac{N_i}{N}}&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
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P _ i = { frac { n _ i }{ n }&lt;br /&gt;
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&amp;lt;nowiki&amp;gt;{\sum{p_i {\varepsilon}_i}}&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
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where N&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt; is the number of particles in state i and N is the total number of particles in the system. We may use the Boltzmann distribution to find this probability that is, as we have seen, equal to the fraction of particles that are in state i. So the equation that gives the fraction of particles in state i as a function of the energy of that state is&lt;br /&gt;
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&amp;lt;nowiki&amp;gt;&amp;lt;/math&amp;gt;&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
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《数学公式丢失了》&lt;br /&gt;
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N&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt; 是位于量子态 i 的粒子数，N是系统中粒子的总数。我们可以用波兹曼分布来求出这个概率，它等于处于量子态i的粒子的比例。所以这个方程给出位于量子态 i 的粒子比例关于这个状态能量的函数&amp;lt;ref name=&amp;quot;Atkins, P. W. 2010&amp;quot; /&amp;gt;。&lt;br /&gt;
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This equation is of great importance to [[spectroscopy]]. In spectroscopy we observe a [[spectral line]] of atoms or molecules that we are interested in going from one state to another.&amp;lt;ref name=&amp;quot;Atkins, P. W. 2010&amp;quot; /&amp;gt;&amp;lt;ref name=&amp;quot;:2&amp;quot;&amp;gt;Atkins, P. W.; de Paula J. (2009) Physical Chemistry, 9th edition, Oxford University Press, Oxford, UK&amp;lt;/ref&amp;gt; In order for this to be possible, there must be some particles in the first state to undergo the transition. We may find that this condition is fulfilled by finding the fraction of particles in the first state. If it is negligible, the transition is very likely not to be observed at the temperature for which the calculation was done. In general, a larger fraction of molecules in the first state means a higher number of transitions to the second state.&amp;lt;ref name=&amp;quot;:3&amp;quot;&amp;gt;Skoog, D. A.; Holler, F. J.; Crouch, S. R. (2006) Principles of Instrumental Analysis, Brooks/Cole, Boston, MA&amp;lt;/ref&amp;gt; This gives a stronger spectral line. However, there are other factors that influence the intensity of a spectral line, such as whether it is caused by an allowed or a [[forbidden transition]]&lt;br /&gt;
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对于光谱学来说这很重要在。在光谱中，我们期待能观察到一条原子或分子跃迁的谱线。&amp;lt;ref name=&amp;quot;Atkins, P. W. 2010&amp;quot; /&amp;gt;&amp;lt;ref name=&amp;quot;:2&amp;quot; /&amp;gt; 在为了使这成为可能，必须有一些粒子处于第一个量子态，等待着发生跃迁。我们可以通过求第一态粒子的比例来满足这个条件。如果它可以忽略不计，那么在当前计算的温度下，则很难观察到这种跃迁。一般来说，处于第一状态的分子比例越大，意味着向第二状态跃迁的次数越多。&amp;lt;ref name=&amp;quot;:3&amp;quot; /&amp;gt;这就产生了一条更强的谱线。然而，还有其他因素影响谱线的强度，例如它是否是被允许的跃迁还是被禁止的跃迁。&lt;br /&gt;
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The Boltzmann distribution is related to the [[softmax function]] commonly used in machine learning.&lt;br /&gt;
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玻尔兹曼分布与机器学习中常用的[[Index.php?title=Softmax function|归一化指数函数]]（Softmax 函数）有关。&lt;br /&gt;
=='''统计力学''' ==&lt;br /&gt;
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{{main|Canonical ensemble|Maxwell–Boltzmann statistics}}The Boltzmann distribution appears in statistical mechanics when considering isolated (or nearly-isolated) systems of fixed composition that are in thermal equilibrium (equilibrium with respect to energy exchange). The most general case is the probability distribution for the canonical ensemble, but also some special cases (derivable from the canonical ensemble) also show the Boltzmann distribution in different aspects:&lt;br /&gt;
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当独立的(或者几乎独立的)固定体系处于统计力学热平衡状态时，玻尔兹曼分布就会出现。最普遍的情况是概率分布的正则系综，但也有一些特殊的情况(从正则系综衍生)也显示了不同形式的玻尔兹曼分布:&lt;br /&gt;
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; [[Canonical ensemble]] (general case)&lt;br /&gt;
; '''正则系综(一般情况)'''&lt;br /&gt;
; '''The [[canonical ensemble]] gives the [[probabilities]] of the various possible states of a closed system of fixed volume, in thermal equilibrium with a [[heat bath]]. The canonical ensemble is a probability distribution with the Boltzmann form.'''&lt;br /&gt;
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正则系综模型给出了在一个封闭固定体积，带有热浴的热平衡系统中的各种可能状态的概率。我们称正则系综为一个玻尔兹曼概率分布。&lt;br /&gt;
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; Statistical frequencies of subsystems' states (in a non-interacting collection)&lt;br /&gt;
'''子系统状态的统计频率(在一个无交互的集合中)'''&lt;br /&gt;
: When the system of interest is a collection of many non-interacting copies of a smaller subsystem, it is sometimes useful to find the [[statistical frequency]] of a given subsystem state, among the collection. The canonical ensemble has the property of separability when applied to such a collection: as long as the non-interacting subsystems have fixed composition, then each subsystem's state is independent of the others and is also characterized by a canonical ensemble. As a result, the [[expectation value|expected]] statistical frequency distribution of subsystem states has the Boltzmann form.&lt;br /&gt;
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当系统是一个较小子系统的许多非交互副本的集合时，有时我们需要在某个子系统集合中找到某个子系统的统计频率。当应用于这样一个集合时，这个子系统的正则系综具有可分离性: 只要不相互作用的子系统的组成是固定的，那么每个子系统的状态都是独立于其他子系统的，它们也拥有自己的正则系综。因此，子系统状态的期望统计频率分布形式是玻尔兹曼分布。&lt;br /&gt;
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[[Maxwell–Boltzmann statistics]] of classical gases (systems of non-interacting particles)&lt;br /&gt;
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'''Maxwell-Boltzmann 统计中的经典气体系统(非相互作用粒子系统)'''&lt;br /&gt;
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: In particle systems, many particles share the same space and regularly change places with each other; the single-particle state space they occupy is a shared space. [[Maxwell–Boltzmann statistics]] give the expected number of particles found in a given single-particle state, in a [[classical mechanics|classical]] gas of non-interacting particles at equilibrium. This expected number distribution has the Boltzmann form.&lt;br /&gt;
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在粒子系统中，许多粒子共享同一空间，并且相互之间有规律地改变位置; 它们所占据的单粒子状态空间是一个共享空间。[[Index.php?title=Maxwell–Boltzmann statistics|麦克斯韦-玻尔兹曼统计]]给出了在一个给定的单粒子态，在一个处于平衡状态的非相互作用粒子的经典气体中所发现的粒子的预期数量。这个预期的数量分布具有玻尔兹曼分布形式。&lt;br /&gt;
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Although these cases have strong similarities, it is helpful to distinguish them as they generalize in different ways when the crucial assumptions are changed:&lt;br /&gt;
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虽然这些案例有很多相似之处，但是当关键假设发生变化时，我们需要对它们以不同的方式进行归纳总结，因此区分它们是有帮助的:&lt;br /&gt;
* When a system is in thermodynamic equilibrium with respect to both energy exchange ''and particle exchange'', the requirement of fixed composition is relaxed and a [[grand canonical ensemble]] is obtained rather than canonical ensemble. On the other hand, if both composition and energy are fixed, then a [[microcanonical ensemble]] applies instead.&lt;br /&gt;
* 当一个系统在能量交换和粒子交换方面都处于热力学平衡时，固定组成的要求就放宽了。这时我们就得到了一个[[Index.php?title=Microcanonical ensemble|巨正则系综]]而不是正则系综。另一方面，如果成分和能量都是固定的，则可以使用[[微正则系综Index.php?title=Microcanonical ensemble|微正则系综]]。&lt;br /&gt;
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* If the subsystems within a collection ''do'' interact with each other, then the expected frequencies of subsystem states no longer follow a Boltzmann distribution, and even may not have an [[analytical solution]].&amp;lt;ref name=&amp;quot;:4&amp;quot;&amp;gt;A classic example of this is [[magnetic ordering]]. Systems of non-interacting [[spin (physics)|spins]] show [[paramagnetic]] behaviour that can be understood with a single-particle canonical ensemble (resulting in the [[Brillouin function]]). Systems of ''interacting'' spins can show much more complex behaviour such as [[ferromagnetism]] or [[antiferromagnetism]].&amp;lt;/ref&amp;gt; The canonical ensemble can however still be applied to the ''collective'' states of the entire system considered as a whole, provided the entire system is isolated and in thermal equilibrium.&lt;br /&gt;
* 如果集合中的子系统确实相互交互，则子系统状态的预期频率不再遵循玻尔兹曼 分布，甚至可能没有解析解。&amp;lt;ref name=&amp;quot;:4&amp;quot; /&amp;gt;然而，如果整个系统是独立的并且处于热平衡状态，则正则系综仍然可以应用于作为一个整体考虑。&lt;br /&gt;
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* With ''[[quantum mechanics|quantum]]'' gases of non-interacting particles in equilibrium, the number of particles found in a given single-particle state does not follow Maxwell–Boltzmann statistics, and there is no simple closed form expression for quantum gases in the canonical ensemble. In the grand canonical ensemble the state-filling statistics of quantum gases are described by [[Fermi–Dirac statistics]] or [[Bose–Einstein statistics]], depending on whether the particles are [[fermion]]s or [[boson]]s respectively.&lt;br /&gt;
* 对于处于平衡状态的非相互作用粒子的量子气体，在给定的单粒子状态中发现的粒子数量并不遵循麦克斯韦-玻尔兹曼统计。并且正则系综中的量子气体没有简单的封闭表达式。在巨正则系综中，量子气体的统计分布状态由费米-狄拉克统计或玻色-爱因斯坦统计来描述，具体则取决于该粒子是费米子还是玻色子。&lt;br /&gt;
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== 数学 ==&lt;br /&gt;
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In more general mathematical settings, the Boltzmann distribution is also known as the [[Gibbs measure]]. In statistics and machine learning, it is called a [[log-linear model]]. In [[deep learning]], the Boltzmann distribution is used in the sampling distribution of [[stochastic neural network]]s such as the [[Boltzmann machine]], [[Restricted Boltzmann machine]], [[Energy based model|Energy-Based models]] and [[Deep Boltzmann Machine|deep Boltzmann machine]]&lt;br /&gt;
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在更一般的数学环境中，玻尔兹曼分布也被称为吉布斯量度。在统计学和机器学习中，它被称为对数线性回归。在深度学习中，玻尔兹曼分布被用于随机神经网络的抽样分布，如玻尔兹曼机、受限玻尔兹曼机、基于能量的模型和深度波茨曼机。&lt;br /&gt;
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== 经济 ==&lt;br /&gt;
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The Boltzmann distribution can be introduced to allocate permits in emissions trading.&amp;lt;ref name=&amp;quot;Park, J.-W. 2012&amp;quot;&amp;gt;Park, J.-W., Kim, C. U. and Isard, W. (2012) Permit allocation in emissions trading using the Boltzmann distribution. Physica A 391: 4883–4890&amp;lt;/ref&amp;gt;&amp;lt;ref name=&amp;quot;:5&amp;quot;&amp;gt;[http://www.technologyreview.com/view/425051/the-thorny-problem-of-fair-allocation/ The Thorny Problem Of Fair Allocation]. ''Technology Review'' blog. August 17, 2011. Cites and summarizes Park, Kim and Isard (2012).&amp;lt;/ref&amp;gt; The new allocation method using the Boltzmann distribution can describe the most probable, natural, and unbiased distribution of emissions permits among multiple countries. Simple and versatile, this new method holds potential for many economic and environmental applications.&lt;br /&gt;
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在经济学中，玻尔兹曼分布被用来分配排放交易中的许可。&amp;lt;ref name=&amp;quot;Park, J.-W. 2012&amp;quot; /&amp;gt;&amp;lt;ref name=&amp;quot;:5&amp;quot; /&amp;gt;  使用玻尔兹曼分布的新分配方法可以创造出在多个国家之间最可能的、自然的和无偏见的排放许可分配。这种新方法简单而通用，在经济和环保中有很大的应用潜力。&lt;br /&gt;
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The Boltzmann distribution has the same form as the [[Multinomial logistic regression|multinomial logit]] model. As a [[discrete choice]] model, this is very well known in economics since [[Daniel McFadden]] made the connection to random utility maximization.&lt;br /&gt;
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玻尔兹曼分布与多项逻辑回归模型具有相同的形式。在丹尼尔 · 麦克法登将它与随机效用最大化联系起来之后，成为了大家所熟知的一种离散选择模型。&lt;br /&gt;
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Category:Statistical mechanics&lt;br /&gt;
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类别: 统计力学&lt;br /&gt;
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==See also==&lt;br /&gt;
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Distribution&lt;br /&gt;
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分布&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:Boltzmann distribution]]. Its edit history can be viewed at [[玻尔兹曼分布/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>Tueryeye</name></author>
	</entry>
	<entry>
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		<title>玻尔兹曼分布</title>
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		<updated>2021-10-19T07:19:38Z</updated>

		<summary type="html">&lt;p&gt;Tueryeye：翻译完成&lt;/p&gt;
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&lt;div&gt;li此词条暂由彩云小译翻译，翻译字数共1452，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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{{Use American English|date = March 2019}}&lt;br /&gt;
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{{Short description|Probability distribution of energy states of a system}}&lt;br /&gt;
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{{about|system energy states|particle energy levels and velocities|Maxwell–Boltzmann distribution}}&lt;br /&gt;
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[[File:Boltzmann distribution graph.svg|upright=1.75|right|thumb|Boltzmann factor ''p&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;''&amp;amp;nbsp;/&amp;amp;nbsp;''p&amp;lt;sub&amp;gt;j&amp;lt;/sub&amp;gt;'' (vertical axis) as a function of temperature ''T'' for several energy differences ''ε&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;''&amp;amp;nbsp;−&amp;amp;nbsp;''ε&amp;lt;sub&amp;gt;j&amp;lt;/sub&amp;gt;''.|链接=Special:FilePath/Boltzmann_distribution_graph.svg]]&lt;br /&gt;
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In [[statistical mechanics]] and [[mathematics]], a '''Boltzmann distribution''' (also called '''Gibbs distribution'''&amp;lt;ref name=&amp;quot;landau&amp;quot;&amp;gt;{{cite book | author=Landau, Lev Davidovich |author2=Lifshitz, Evgeny Mikhailovich |name-list-style=amp | title=Statistical Physics |volume=5 |series=Course of Theoretical Physics |edition=3 |origyear=1976 |year=1980 |place=Oxford |publisher=Pergamon Press|isbn=0-7506-3372-7|author-link=Lev Landau |author2-link=Evgeny Lifshitz }} Translated by J.B. Sykes and M.J. Kearsley. See section 28&amp;lt;/ref&amp;gt;) is a [[probability distribution]] or [[probability measure]] that gives the probability that a system will be in a certain [[microstate (statistical mechanics)|state]] as a function of that state's energy and the temperature of the system. The distribution is expressed in the form:&lt;br /&gt;
&lt;br /&gt;
In statistical mechanics and mathematics, a Boltzmann distribution (also called Gibbs distribution) is a probability distribution or probability measure that gives the probability that a system will be in a certain state as a function of that state's energy and the temperature of the system. The distribution is expressed in the form:&lt;br /&gt;
&lt;br /&gt;
在统计力学和数学中，波兹曼分布分布(也称为吉布斯分布&amp;lt;ref name=&amp;quot;landau&amp;quot; /&amp;gt;)是一个概率分布或机率量测，它给出了一个系统处于某种量子态的概率，这个概率是该状态的能量和系统温度的函数。分布情况以下列形式表示:&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
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:&amp;lt;math&amp;gt;p_i \propto e^{-\frac{\varepsilon_i}{kT}}&amp;lt;/math&amp;gt; &lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt;p_i \propto e^{-\frac{\varepsilon_i}{kT}}&amp;lt;/math&amp;gt; &lt;br /&gt;
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[拉丁语]&lt;br /&gt;
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where {{mvar|p&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;}} is the probability of the system being in state {{mvar|i}}, {{mvar|ε&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;}} is the energy of that state, and a constant {{mvar|kT}} of the distribution is the product of [[Boltzmann's constant]] {{mvar|k}} and [[thermodynamic temperature]] {{mvar|T}}. The symbol &amp;lt;math display=&amp;quot;inline&amp;quot;&amp;gt;\propto&amp;lt;/math&amp;gt; denotes [[proportionality (mathematics)|proportionality]] (see {{section link||The distribution}} for the proportionality constant).&lt;br /&gt;
&lt;br /&gt;
where  is the probability of the system being in state ,  is the energy of that state, and a constant  of the distribution is the product of Boltzmann's constant  and thermodynamic temperature . The symbol &amp;lt;math display=&amp;quot;inline&amp;quot;&amp;gt;\propto&amp;lt;/math&amp;gt; denotes proportionality (see  for the proportionality constant).&lt;br /&gt;
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{{mvar|p&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;}} 是其中系统处于状态{{mvar|i}}的概率, {{mvar|ε&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;}} 是该状态的能量，还有关于这个分布的一个常数 {{mvar|kT}} ，它是玻耳兹曼常数{{mvar|k}}和热力学温度 {{mvar|T}} 的乘积。符号 &amp;lt;math display=&amp;quot;inline&amp;quot;&amp;gt;\propto&amp;lt;/math&amp;gt;表示相称性(见附录中的比例常数)。&lt;br /&gt;
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The term system here has a very wide meaning; it can range from a single atom to a macroscopic system such as a [[Natural gas storage|natural gas storage tank]]. Because of this the Boltzmann distribution can be used to solve a very wide variety of problems. The distribution shows that states with lower energy will always have a higher probability of being occupied .&lt;br /&gt;
&lt;br /&gt;
The term system here has a very wide meaning; it can range from a single atom to a macroscopic system such as a natural gas storage tank. Because of this the Boltzmann distribution can be used to solve a very wide variety of problems. The distribution shows that states with lower energy will always have a higher probability of being occupied .&lt;br /&gt;
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这里的术语系统含义广泛; 它可以从单个原子到宏观系统，如天然气储罐。正因为如此，波兹曼分布可以用来解决各种各样的问题。玻尔兹曼分布表明，能量较低的状态被占据的概率总是较高的。&lt;br /&gt;
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The ''ratio'' of probabilities of two states is known as the '''Boltzmann factor''' and characteristically only depends on the states' energy difference:&lt;br /&gt;
&lt;br /&gt;
The ratio of probabilities of two states is known as the Boltzmann factor and characteristically only depends on the states' energy difference:&lt;br /&gt;
&lt;br /&gt;
两种状态的概率之比被称为玻尔兹曼因子，取决于两种状态的能量差:&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt;\frac{p_i}{p_j} = e^{\frac{\varepsilon_j - \varepsilon_i}{kT}}&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt;\frac{p_i}{p_j} = e^{\frac{\varepsilon_j - \varepsilon_i}{kT}}&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
[数学][数学]&lt;br /&gt;
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The Boltzmann distribution is named after [[Ludwig Boltzmann]] who first formulated it in 1868 during his studies of the [[statistical mechanics]] of gases in thermal equilibrium. Boltzmann's statistical work is borne out in his paper “On the Relationship between the Second Fundamental Theorem of the Mechanical Theory of Heat and Probability Calculations Regarding the Conditions for Thermal Equilibrium&amp;quot;&amp;lt;ref&amp;gt;http://crystal.med.upenn.edu/sharp-lab-pdfs/2015SharpMatschinsky_Boltz1877_Entropy17.pdf&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
The Boltzmann distribution is named after Ludwig Boltzmann who first formulated it in 1868 during his studies of the statistical mechanics of gases in thermal equilibrium. Boltzmann's statistical work is borne out in his paper “On the Relationship between the Second Fundamental Theorem of the Mechanical Theory of Heat and Probability Calculations Regarding the Conditions for Thermal Equilibrium&amp;quot;&lt;br /&gt;
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波兹曼分布是根据路德维希·玻尔兹曼1868年在研究统计力学中气体热平衡的时候首次提出的一个公式命名的。波尔兹曼的统计工作在他1877年的论文《论热力学第二基本定理与热平衡条件的概率计算之间的关系》中得到了体现。&amp;lt;ref&amp;gt;“On the Relationship between the Second Fundamental Theorem of the Mechanical Theory of Heat and Probability Calculations Regarding the Conditions for Thermal Equilibrium” Sitzungberichte der Kaiserlichen Akademie der Wissenschaften. Mathematisch-Naturwissen Classe. Abt. II, LXXVI 1877, pp 373-435 (Wien. Ber. 1877, 76:373-435). &amp;lt;/ref&amp;gt;&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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  It would be nice to have a citation here! The origin of the Boltzmann factor isn't entirely clear. According to some authors, Boltzmann's 1968 paper “On the Relationship between the Second Fundamental Theorem of the Mechanical Theory of Heat and Probability Calculations Regarding the Conditions for Thermal Equilibrium”&lt;br /&gt;
&lt;br /&gt;
  It would be nice to have a citation here! The origin of the Boltzmann factor isn't entirely clear. According to some authors, Boltzmann's 1968 paper “On the Relationship between the Second Fundamental Theorem of the Mechanical Theory of Heat and Probability Calculations Regarding the Conditions for Thermal Equilibrium”&lt;br /&gt;
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如果能在这里引用一下就好了！玻尔兹曼因子的起源并不完全清楚。根据一些作者的说法，Boltzmann 在1968年发表的论文《论热力学第二基本定理与热平衡条件的概率计算之间的关系》&lt;br /&gt;
&lt;br /&gt;
  &amp;quot;Studien über das Gleichgewicht der lebendigen Kraft zwischen bewegten materiellen Punkten&amp;quot; is the origin but I can't find this article at the moment,&lt;br /&gt;
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  &amp;quot;Studien über das Gleichgewicht der lebendigen Kraft zwischen bewegten materiellen Punkten&amp;quot; is the origin but I can't find this article at the moment,&lt;br /&gt;
&lt;br /&gt;
  &amp;quot;Studien über das Gleichgewicht der lebendigen Kraft zwischen bewegten materiellen Punkten&amp;quot; is the origin but I can't find this article at the moment,&lt;br /&gt;
&lt;br /&gt;
  so I cannot confirm.&lt;br /&gt;
&lt;br /&gt;
  so I cannot confirm.&lt;br /&gt;
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所以我不能确定。&lt;br /&gt;
&lt;br /&gt;
  For example, this book says so, but uses suspiciously modern terminology&lt;br /&gt;
&lt;br /&gt;
  For example, this book says so, but uses suspiciously modern terminology&lt;br /&gt;
&lt;br /&gt;
例如，这本书是这么说的，但是使用了可疑的现代术语&lt;br /&gt;
&lt;br /&gt;
    http://books.google.es/books?id=u13KiGlz2zcC&amp;amp;lpg=PA92&amp;amp;ots=8H1DRURdxn&amp;amp;pg=PA93#v=onepage&amp;amp;f=false&lt;br /&gt;
&lt;br /&gt;
    http://books.google.es/books?id=u13KiGlz2zcC&amp;amp;lpg=PA92&amp;amp;ots=8H1DRURdxn&amp;amp;pg=PA93#v=onepage&amp;amp;f=false&lt;br /&gt;
&lt;br /&gt;
Http://books.google.es/books?id=u13kiglz2zcc&amp;amp;lpg=pa92&amp;amp;ots=8h1drurdxn&amp;amp;pg=pa93#v=onepage&amp;amp;f=false&lt;br /&gt;
&lt;br /&gt;
  On the other hand, Uffink's &amp;quot;Compendium of the foundations of classical statistical physics&amp;quot; does not seem to indicate quite this equation but rather that Boltzmann's 1968 distribution was the simple Maxwell–Boltzmann distribution (for a classical nonrelativistic gas), modified for particles in a potential.&lt;br /&gt;
&lt;br /&gt;
  On the other hand, Uffink's &amp;quot;Compendium of the foundations of classical statistical physics&amp;quot; does not seem to indicate quite this equation but rather that Boltzmann's 1968 distribution was the simple Maxwell–Boltzmann distribution (for a classical nonrelativistic gas), modified for particles in a potential.&lt;br /&gt;
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另一方面，Uffink 的“经典统计物理学基础纲要”似乎并没有完全表明这个方程，而是说 Boltzmann 在1968年的分布是简单的 Maxwell-波兹曼分布(用于经典的非气体) ，修改为势中的粒子。&lt;br /&gt;
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--&amp;gt; &lt;br /&gt;
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--&amp;gt; &lt;br /&gt;
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--&amp;gt;&lt;br /&gt;
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The distribution was later investigated extensively, in its modern generic form, by [[Josiah Willard Gibbs]] in 1902.&amp;lt;ref name=&amp;quot;gibbs&amp;quot;&amp;gt;{{cite book |last=Gibbs |first=Josiah Willard |authorlink=Josiah Willard Gibbs |title=Elementary Principles in Statistical Mechanics |year=1902 |publisher=[[Charles Scribner's Sons]] &lt;br /&gt;
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The distribution was later investigated extensively, in its modern generic form, by Josiah Willard Gibbs in 1902.&lt;br /&gt;
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这种分布后来在1902年由约西亚·威拉德·吉布斯进行了广泛的调查，以其现代通用形式。&lt;br /&gt;
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|location=New York|title-link=Elementary Principles in Statistical Mechanics }}&amp;lt;/ref&amp;gt;{{rp|Ch.IV}}、&lt;br /&gt;
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在玻尔兹曼分布被发明之后，约西亚·华纳德·吉布森充分地研究了它并在1902年提出了它的一般形式。&amp;lt;ref name=&amp;quot;gibbs&amp;quot; /&amp;gt;&lt;br /&gt;
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The generalized Boltzmann distribution is a sufficient and necessary condition for the equivalence between the statistical mechanics definition of entropy (The  Gibbs entropy formula &amp;lt;math&amp;gt;S = -k_{\mathrm{B}}\sum_i p_i \log p_i&amp;lt;/math&amp;gt;) and the thermodynamic definition of entropy (&amp;lt;math&amp;gt;d S = \frac{\delta Q_\text{rev}}{T}&amp;lt;/math&amp;gt;, and the fundamental thermodynamic relation).&lt;br /&gt;
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The generalized Boltzmann distribution is a sufficient and necessary condition for the equivalence between the statistical mechanics definition of [[entropy]] (The [[Entropy_(statistical_thermodynamics)#Gibbs_entropy_formula | Gibbs entropy formula]] &amp;lt;math&amp;gt;S = -k_{\mathrm{B}}\sum_i p_i \log p_i&amp;lt;/math&amp;gt;) and the thermodynamic definition of entropy (&amp;lt;math&amp;gt;d S = \frac{\delta Q_\text{rev}}{T}&amp;lt;/math&amp;gt;, and the [[fundamental thermodynamic relation]]).&amp;lt;ref name=&amp;quot;:0&amp;quot;&amp;gt;{{cite journal |last1= Gao |first1= Xiang |last2= Gallicchio |first2= Emilio |first3= Adrian |last3= Roitberg  |date= 2019 |title= The generalized Boltzmann distribution is the only distribution in which the Gibbs-Shannon entropy equals the thermodynamic entropy |journal= The Journal of Chemical Physics|volume= 151|issue= 3|pages= 034113|doi= 10.1063/1.5111333|pmid= 31325924 |arxiv= 1903.02121 |s2cid= 118981017 }}&amp;lt;/ref&amp;gt;&lt;br /&gt;
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广义波兹曼分布是熵的统计力学定义(吉布斯熵公式  &amp;lt;math&amp;gt;S = -k_{\mathrm{B}}\sum_i p_i \log p_i&amp;lt;/math&amp;gt;))与熵的热力学定义(&amp;lt;math&amp;gt;d S = \frac{\delta Q_\text{rev}}{T}&amp;lt;/math&amp;gt;)等价的充要条件。&amp;lt;ref name=&amp;quot;:0&amp;quot; /&amp;gt;&lt;br /&gt;
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The Boltzmann distribution should not be confused with the Maxwell–Boltzmann distribution. The former gives the probability that a system will be in a certain state as a function of that state's energy; in contrast, the latter is used to describe particle speeds in idealized gases.&lt;br /&gt;
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值得一提的是，玻尔兹曼分布不应与麦克斯韦-玻尔兹曼分布混淆。前者给出了系统处于某种状态的概率，作为该状态能量的函数; 后者则是用于描述理想气体中的粒子速度。&lt;br /&gt;
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The Boltzmann distribution should not be confused with the [[Maxwell–Boltzmann distribution]]. The former gives the probability that a system will be in a certain state as a function of that state's energy;&amp;lt;ref name=&amp;quot;Atkins, P. W. 2010&amp;quot;&amp;gt;Atkins, P. W. (2010) Quanta, W. H. Freeman and Company, New York&amp;lt;/ref&amp;gt; in contrast, the latter is used to describe particle speeds in idealized gases.&lt;br /&gt;
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==The distribution==&lt;br /&gt;
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The Boltzmann distribution is a probability distribution that gives the probability of a certain state as a function of that state's energy and  temperature of the system to which the distribution is applied. It is given as&lt;br /&gt;
&lt;br /&gt;
波兹曼分布是一个概率分布，它给出了出于某种量子态处于某种能量和温度的时候的概率。它被这样定义：&lt;br /&gt;
&lt;br /&gt;
The Boltzmann distribution is a [[probability distribution]] that gives the probability of a certain state as a function of that state's energy and  temperature of the [[system]] to which the distribution is applied.&amp;lt;ref name=&amp;quot;McQuarrie, A. 2000&amp;quot;&amp;gt;McQuarrie, A. (2000) Statistical Mechanics, University Science Books, California&amp;lt;/ref&amp;gt; It is given as&lt;br /&gt;
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&amp;lt;math&amp;gt;&lt;br /&gt;
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《数学》&lt;br /&gt;
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:&amp;lt;math&amp;gt;&lt;br /&gt;
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p_i=\frac{1}{Q}} {e^{- {\varepsilon}_i / k T}=\frac{e^{- {\varepsilon}_i / k T}}{\sum_{j=1}^{M}{e^{- {\varepsilon}_j / k T}}}&lt;br /&gt;
&lt;br /&gt;
P _ i = frac {1}{ q }{ e ^ {-{ varepsilon } _ i/k t } = frac { e ^ {-{ varepsilon } _ i/k t }{ sum { j = 1} ^ { m }{ e ^ {-{ varepsilon } _ j/k t }}}}}&lt;br /&gt;
&lt;br /&gt;
p_i=\frac{1}{Q}} {e^{- {\varepsilon}_i / k T}=\frac{e^{- {\varepsilon}_i / k T}}{\sum_{j=1}^{M}{e^{- {\varepsilon}_j / k T}}}&lt;br /&gt;
&lt;br /&gt;
&amp;lt;/math&amp;gt;&lt;br /&gt;
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数学&lt;br /&gt;
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&amp;lt;/math&amp;gt;&lt;br /&gt;
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where p&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt; is the probability of state i, ε&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt; the energy of state i, k the Boltzmann constant, T the temperature of the system and M is the number of all states accessible to the system of interest.&lt;br /&gt;
&lt;br /&gt;
where ''p&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;'' is the probability of state ''i'', ''ε&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;'' the energy of state ''i'', ''k'' the Boltzmann constant, ''T'' the temperature of the system and ''M'' is the number of all states accessible to the system of interest.&amp;lt;ref name=&amp;quot;McQuarrie, A. 2000&amp;quot; /&amp;gt;&amp;lt;ref name=&amp;quot;Atkins, P. W. 2010&amp;quot; /&amp;gt; Implied parentheses around the denominator ''kT'' are omitted for brevity. The normalization denominator ''Q'' (denoted by some authors by ''Z'') is the [[canonical partition function]]&lt;br /&gt;
&lt;br /&gt;
其中 ''p&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;'' 是状态 i 的概率，''ε&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;'' 是状态 i 的能量，''k'' 是波兹曼常数，''T'' 是系统的温度，''M'' 是系统所能到达的所有量子态的数目。&amp;lt;ref name=&amp;quot;Atkins, P. W. 2010&amp;quot; /&amp;gt; &amp;lt;ref name=&amp;quot;McQuarrie, A. 2000&amp;quot; /&amp;gt;这里为了简洁美观，省略了''kT''周围的括弧。归一化的分母''Q''（被有些作者写为''Z''）是对于系统中所有量子态进行总和，此部分又被称为[[Index.php?title=Canonical partition function|正则配分函数]]''。''&lt;br /&gt;
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It results from the constraint that the probabilities of all accessible states must add up to 1.&lt;br /&gt;
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所有量子态的概率之和为1.&lt;br /&gt;
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The Boltzmann distribution is the distribution that maximizes the [[entropy]]，&lt;br /&gt;
&lt;br /&gt;
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&amp;lt;math&amp;gt;H(p_1,p_2,\cdots,p_M) = -\sum_{i=1}^{M} p_i\log_2 p_i&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&amp;lt;nowiki&amp;gt;subject to the constraint that {\sum{p_i {\varepsilon}_i}} equals a particular mean energy value (which can be proven using &amp;lt;/nowiki&amp;gt;[[Lagrange multipliers]]).&lt;br /&gt;
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&amp;lt;nowiki&amp;gt;当 {\sum{p_i {\varepsilon}_i}} 等于平均能量值时，玻尔兹曼分布是这种情况下能让熵最大化的分布。我们可以通过拉格朗日乘数法来证明。&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The partition function can be calculated if we know the energies of the states accessible to the system of interest. For atoms the partition function values can be found in the NIST Atomic Spectra Database.&amp;lt;ref name=&amp;quot;:1&amp;quot;&amp;gt;[http://physics.nist.gov/PhysRefData/ASD/levels_form.html NIST Atomic Spectra Database Levels Form] at nist.gov&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
在知道量子态能量的情况下，这个配分函数可以被计算。对于原子来说，配分函数的值可以在NIST Atomic Spectra Database中找到。&amp;lt;ref name=&amp;quot;:1&amp;quot; /&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The distribution shows that states with lower energy will always have a higher probability of being occupied than the states with higher energy. It can also give us the quantitative relationship between the probabilities of the two states being occupied. The ratio of probabilities for states ''i'' and ''j'' is given as&lt;br /&gt;
&lt;br /&gt;
:&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The distribution shows that states with lower energy will always have a higher probability of being occupied than the states with higher energy. It can also give us the quantitative relationship between the probabilities of the two states being occupied. The ratio of probabilities for states i and j is given as&lt;br /&gt;
&lt;br /&gt;
玻尔兹曼分布指出，能量低的量子态总是有比能量高的量子态更高的概率被粒子占据。它同时也能让我们定量地比较两个量子态分布概率的关系。状态 i 和状态 j 的概率比为&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
{\frac{p_i}{p_j}}=e^{({\varepsilon}_j-{\varepsilon}_i) / k T}&lt;br /&gt;
&lt;br /&gt;
&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;nowiki&amp;gt;{\frac{p_i}{p_j}}=e^{({\varepsilon}_j-{\varepsilon}_i) / k T}&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;nowiki&amp;gt;{\frac{p_i}{p_j}}=e^{({\varepsilon}_j-{\varepsilon}_i) / k T}&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&amp;lt;nowiki&amp;gt;&amp;lt;/math&amp;gt;&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
&lt;br /&gt;
数学&lt;br /&gt;
&lt;br /&gt;
where p&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt; is the probability of state i,  p&amp;lt;sub&amp;gt;j&amp;lt;/sub&amp;gt; the probability of state j, and ε&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt; and ε&amp;lt;sub&amp;gt;j&amp;lt;/sub&amp;gt; are the energies of states i and j, respectively.&lt;br /&gt;
&lt;br /&gt;
其中 p&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt; 是量子态 i 的概率， p&amp;lt;sub&amp;gt;j&amp;lt;/sub&amp;gt; 是量子态 j 的概率，ε&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt; 和 ε&amp;lt;sub&amp;gt;j&amp;lt;/sub&amp;gt; 分别是状态 i 和 j 的能量。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The Boltzmann distribution is often used to describe the distribution of particles, such as atoms or molecules, over energy states accessible to them. If we have a system consisting of many particles, the probability of a particle being in state i is practically the probability that, if we pick a random particle from that system and check what state it is in, we will find it is in state i. This probability is equal to the number of particles in state i divided by the total number of particles in the system, that is the fraction of particles that occupy state i.&lt;br /&gt;
&lt;br /&gt;
玻尔兹曼分布通常被用来描述粒子的分布，比如原子或分子，在能量状态上的分布情况。如果我们有一个由许多粒子组成的系统，某个粒子处于量子态 i 的概率就等同于当我们从该系统中选择一个随机的粒子并观察它处于什么状态，发现它处于状态 i 的概率。这个概率等于量子态 i 的粒子数除以系统中粒子的总数，即那些占据量子态i的粒子的比例。&lt;br /&gt;
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&amp;lt;nowiki&amp;gt;&amp;lt;math display=&amp;quot;inline&amp;quot;&amp;gt;&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
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&amp;lt;nowiki&amp;gt;p_i={\frac{N_i}{N}}&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
&lt;br /&gt;
P _ i = { frac { n _ i }{ n }&lt;br /&gt;
&lt;br /&gt;
&amp;lt;nowiki&amp;gt;{\sum{p_i {\varepsilon}_i}}&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
where N&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt; is the number of particles in state i and N is the total number of particles in the system. We may use the Boltzmann distribution to find this probability that is, as we have seen, equal to the fraction of particles that are in state i. So the equation that gives the fraction of particles in state i as a function of the energy of that state is&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
N&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt; 是位于量子态 i 的粒子数，N是系统中粒子的总数。我们可以用波兹曼分布来求出这个概率，它等于处于量子态i的粒子的比例。所以这个方程给出位于量子态 i 的粒子比例关于这个状态能量的函数&amp;lt;ref name=&amp;quot;Atkins, P. W. 2010&amp;quot; /&amp;gt;。&lt;br /&gt;
&lt;br /&gt;
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This equation is of great importance to [[spectroscopy]]. In spectroscopy we observe a [[spectral line]] of atoms or molecules that we are interested in going from one state to another.&amp;lt;ref name=&amp;quot;Atkins, P. W. 2010&amp;quot; /&amp;gt;&amp;lt;ref name=&amp;quot;:2&amp;quot;&amp;gt;Atkins, P. W.; de Paula J. (2009) Physical Chemistry, 9th edition, Oxford University Press, Oxford, UK&amp;lt;/ref&amp;gt; In order for this to be possible, there must be some particles in the first state to undergo the transition. We may find that this condition is fulfilled by finding the fraction of particles in the first state. If it is negligible, the transition is very likely not to be observed at the temperature for which the calculation was done. In general, a larger fraction of molecules in the first state means a higher number of transitions to the second state.&amp;lt;ref name=&amp;quot;:3&amp;quot;&amp;gt;Skoog, D. A.; Holler, F. J.; Crouch, S. R. (2006) Principles of Instrumental Analysis, Brooks/Cole, Boston, MA&amp;lt;/ref&amp;gt; This gives a stronger spectral line. However, there are other factors that influence the intensity of a spectral line, such as whether it is caused by an allowed or a [[forbidden transition]]&lt;br /&gt;
&lt;br /&gt;
对于光谱学来说这很重要在。在光谱中，我们期待能观察到一条原子或分子跃迁的谱线。&amp;lt;ref name=&amp;quot;Atkins, P. W. 2010&amp;quot; /&amp;gt;&amp;lt;ref name=&amp;quot;:2&amp;quot; /&amp;gt; 在为了使这成为可能，必须有一些粒子处于第一个量子态，等待着发生跃迁。我们可以通过求第一态粒子的比例来满足这个条件。如果它可以忽略不计，那么在当前计算的温度下，则很难观察到这种跃迁。一般来说，处于第一状态的分子比例越大，意味着向第二状态跃迁的次数越多。&amp;lt;ref name=&amp;quot;:3&amp;quot; /&amp;gt;这就产生了一条更强的谱线。然而，还有其他因素影响谱线的强度，例如它是否是被允许的跃迁还是被禁止的跃迁。&lt;br /&gt;
&lt;br /&gt;
The Boltzmann distribution is related to the [[softmax function]] commonly used in machine learning.&lt;br /&gt;
&lt;br /&gt;
The Boltzmann distribution is related to the softmax function commonly used in machine learning.&lt;br /&gt;
&lt;br /&gt;
玻尔兹曼分布与机器学习中常用的[[Index.php?title=Softmax function|归一化指数函数]]（Softmax 函数）有关。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
== In statistical mechanics '''统计力学''' ==&lt;br /&gt;
&lt;br /&gt;
{{main|Canonical ensemble|Maxwell–Boltzmann statistics}}&lt;br /&gt;
:&lt;br /&gt;
&lt;br /&gt;
The Boltzmann distribution appears in statistical mechanics when considering isolated (or nearly-isolated) systems of fixed composition that are in thermal equilibrium (equilibrium with respect to energy exchange). The most general case is the probability distribution for the canonical ensemble, but also some special cases (derivable from the canonical ensemble) also show the Boltzmann distribution in different aspects:&lt;br /&gt;
&lt;br /&gt;
当独立的(或者几乎独立的)固定体系处于统计力学热平衡状态时，玻尔兹曼分布就会出现。最普遍的情况是概率分布的正则系综，但也有一些特殊的情况(从正则系综衍生)也显示了不同形式的玻尔兹曼分布:&lt;br /&gt;
&lt;br /&gt;
; [[Canonical ensemble]] (general case)&lt;br /&gt;
; '''正则系综(一般情况)'''&lt;br /&gt;
; &lt;br /&gt;
; '''The [[canonical ensemble]] gives the [[probabilities]] of the various possible states of a closed system of fixed volume, in thermal equilibrium with a [[heat bath]]. The canonical ensemble is a probability distribution with the Boltzmann form.'''&lt;br /&gt;
&lt;br /&gt;
正则系综模型给出了在一个封闭固定体积，带有热浴的热平衡系统中的各种可能状态的概率。我们称正则系综为一个玻尔兹曼概率分布。&lt;br /&gt;
&lt;br /&gt;
; Statistical frequencies of subsystems' states (in a non-interacting collection)&lt;br /&gt;
'''子系统状态的统计频率(在一个无交互的集合中)'''&lt;br /&gt;
: When the system of interest is a collection of many non-interacting copies of a smaller subsystem, it is sometimes useful to find the [[statistical frequency]] of a given subsystem state, among the collection. The canonical ensemble has the property of separability when applied to such a collection: as long as the non-interacting subsystems have fixed composition, then each subsystem's state is independent of the others and is also characterized by a canonical ensemble. As a result, the [[expectation value|expected]] statistical frequency distribution of subsystem states has the Boltzmann form.&lt;br /&gt;
&lt;br /&gt;
当系统是一个较小子系统的许多非交互副本的集合时，有时我们需要在某个子系统集合中找到某个子系统的统计频率。当应用于这样一个集合时，这个子系统的正则系综具有可分离性: 只要不相互作用的子系统的组成是固定的，那么每个子系统的状态都是独立于其他子系统的，它们也拥有自己的正则系综。因此，子系统状态的期望统计频率分布形式是玻尔兹曼分布。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Maxwell–Boltzmann statistics of classical gases (systems of non-interacting particles)&lt;br /&gt;
&lt;br /&gt;
[[Maxwell–Boltzmann statistics]] of classical gases (systems of non-interacting particles)&lt;br /&gt;
&lt;br /&gt;
'''Maxwell-Boltzmann 统计中的经典气体系统(非相互作用粒子系统)'''&lt;br /&gt;
&lt;br /&gt;
: In particle systems, many particles share the same space and regularly change places with each other; the single-particle state space they occupy is a shared space. [[Maxwell–Boltzmann statistics]] give the expected number of particles found in a given single-particle state, in a [[classical mechanics|classical]] gas of non-interacting particles at equilibrium. This expected number distribution has the Boltzmann form.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
In particle systems, many particles share the same space and regularly change places with each other; the single-particle state space they occupy is a shared space. Maxwell–Boltzmann statistics give the expected number of particles found in a given single-particle state, in a classical gas of non-interacting particles at equilibrium. This expected number distribution has the Boltzmann form.&lt;br /&gt;
&lt;br /&gt;
在粒子系统中，许多粒子共享同一空间，并且相互之间有规律地改变位置; 它们所占据的单粒子状态空间是一个共享空间。[[Index.php?title=Maxwell–Boltzmann statistics|麦克斯韦-玻尔兹曼统计]]给出了在一个给定的单粒子态，在一个处于平衡状态的非相互作用粒子的经典气体中所发现的粒子的预期数量。这个预期的数量分布具有玻尔兹曼分布形式。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Although these cases have strong similarities, it is helpful to distinguish them as they generalize in different ways when the crucial assumptions are changed:&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Although these cases have strong similarities, it is helpful to distinguish them as they generalize in different ways when the crucial assumptions are changed:&lt;br /&gt;
&lt;br /&gt;
虽然这些案例有很多相似之处，但是当关键假设发生变化时，我们需要对它们以不同的方式进行归纳总结，因此区分它们是有帮助的:&lt;br /&gt;
* When a system is in thermodynamic equilibrium with respect to both energy exchange ''and particle exchange'', the requirement of fixed composition is relaxed and a [[grand canonical ensemble]] is obtained rather than canonical ensemble. On the other hand, if both composition and energy are fixed, then a [[microcanonical ensemble]] applies instead.&lt;br /&gt;
* 当一个系统在能量交换和粒子交换方面都处于热力学平衡时，固定组成的要求就放宽了。这时我们就得到了一个[[Index.php?title=Microcanonical ensemble|巨正则系综]]而不是正则系综。另一方面，如果成分和能量都是固定的，则可以使用[[微正则系综Index.php?title=Microcanonical ensemble|微正则系综]]。&lt;br /&gt;
&lt;br /&gt;
* If the subsystems within a collection ''do'' interact with each other, then the expected frequencies of subsystem states no longer follow a Boltzmann distribution, and even may not have an [[analytical solution]].&amp;lt;ref name=&amp;quot;:4&amp;quot;&amp;gt;A classic example of this is [[magnetic ordering]]. Systems of non-interacting [[spin (physics)|spins]] show [[paramagnetic]] behaviour that can be understood with a single-particle canonical ensemble (resulting in the [[Brillouin function]]). Systems of ''interacting'' spins can show much more complex behaviour such as [[ferromagnetism]] or [[antiferromagnetism]].&amp;lt;/ref&amp;gt; The canonical ensemble can however still be applied to the ''collective'' states of the entire system considered as a whole, provided the entire system is isolated and in thermal equilibrium.&lt;br /&gt;
* 如果集合中的子系统确实相互交互，则子系统状态的预期频率不再遵循玻尔兹曼 分布，甚至可能没有解析解。&amp;lt;ref name=&amp;quot;:4&amp;quot; /&amp;gt;然而，如果整个系统是独立的并且处于热平衡状态，则正则系综仍然可以应用于作为一个整体考虑。&lt;br /&gt;
&lt;br /&gt;
* With ''[[quantum mechanics|quantum]]'' gases of non-interacting particles in equilibrium, the number of particles found in a given single-particle state does not follow Maxwell–Boltzmann statistics, and there is no simple closed form expression for quantum gases in the canonical ensemble. In the grand canonical ensemble the state-filling statistics of quantum gases are described by [[Fermi–Dirac statistics]] or [[Bose–Einstein statistics]], depending on whether the particles are [[fermion]]s or [[boson]]s respectively.&lt;br /&gt;
* 对于处于平衡状态的非相互作用粒子的量子气体，在给定的单粒子状态中发现的粒子数量并不遵循麦克斯韦-玻尔兹曼统计。并且正则系综中的量子气体没有简单的封闭表达式。在巨正则系综中，量子气体的统计分布状态由费米-狄拉克统计或玻色-爱因斯坦统计来描述，具体则取决于该粒子是费米子还是玻色子。&lt;br /&gt;
&lt;br /&gt;
== In mathematics ==&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
In more general mathematical settings, the Boltzmann distribution is also known as the [[Gibbs measure]]. In statistics and machine learning, it is called a [[log-linear model]]. In [[deep learning]], the Boltzmann distribution is used in the sampling distribution of [[stochastic neural network]]s such as the [[Boltzmann machine]], [[Restricted Boltzmann machine]], [[Energy based model|Energy-Based models]] and [[Deep Boltzmann Machine|deep Boltzmann machine]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
In more general mathematical settings, the Boltzmann distribution is also known as the Gibbs measure. In statistics and machine learning, it is called a log-linear model. In deep learning, the Boltzmann distribution is used in the sampling distribution of stochastic neural networks such as the Boltzmann machine, Restricted Boltzmann machine, Energy-Based models and deep Boltzmann machine.&lt;br /&gt;
&lt;br /&gt;
在更一般的数学环境中，玻尔兹曼分布也被称为吉布斯量度。在统计学和机器学习中，它被称为对数线性回归。在深度学习中，玻尔兹曼分布被用于随机神经网络的抽样分布，如玻尔兹曼机、受限玻尔兹曼机、基于能量的模型和深度波茨曼机。&lt;br /&gt;
&lt;br /&gt;
== In economics ==&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The Boltzmann distribution can be introduced to allocate permits in emissions trading.&amp;lt;ref name=&amp;quot;Park, J.-W. 2012&amp;quot;&amp;gt;Park, J.-W., Kim, C. U. and Isard, W. (2012) Permit allocation in emissions trading using the Boltzmann distribution. Physica A 391: 4883–4890&amp;lt;/ref&amp;gt;&amp;lt;ref name=&amp;quot;:5&amp;quot;&amp;gt;[http://www.technologyreview.com/view/425051/the-thorny-problem-of-fair-allocation/ The Thorny Problem Of Fair Allocation]. ''Technology Review'' blog. August 17, 2011. Cites and summarizes Park, Kim and Isard (2012).&amp;lt;/ref&amp;gt; The new allocation method using the Boltzmann distribution can describe the most probable, natural, and unbiased distribution of emissions permits among multiple countries. Simple and versatile, this new method holds potential for many economic and environmental applications.&lt;br /&gt;
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在经济学中，玻尔兹曼分布被用来分配排放交易中的许可。&amp;lt;ref name=&amp;quot;Park, J.-W. 2012&amp;quot; /&amp;gt;&amp;lt;ref name=&amp;quot;:5&amp;quot; /&amp;gt;  使用玻尔兹曼分布的新分配方法可以创造出在多个国家之间最可能的、自然的和无偏见的排放许可分配。这种新方法简单而通用，在经济和环保中有很大的应用潜力。&lt;br /&gt;
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The Boltzmann distribution has the same form as the [[Multinomial logistic regression|multinomial logit]] model. As a [[discrete choice]] model, this is very well known in economics since [[Daniel McFadden]] made the connection to random utility maximization.&lt;br /&gt;
&lt;br /&gt;
玻尔兹曼分布与多项逻辑回归模型具有相同的形式。在丹尼尔 · 麦克法登将它与随机效用最大化联系起来之后，成为了大家所熟知的一种离散选择模型。&lt;br /&gt;
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Category:Statistical mechanics&lt;br /&gt;
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类别: 统计力学&lt;br /&gt;
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==See also==&lt;br /&gt;
&lt;br /&gt;
Distribution&lt;br /&gt;
&lt;br /&gt;
分布&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:Boltzmann distribution]]. Its edit history can be viewed at [[玻尔兹曼分布/edithistory]]&amp;lt;/small&amp;gt;&amp;lt;/noinclude&amp;gt;&lt;br /&gt;
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&lt;div&gt;li此词条暂由彩云小译翻译，翻译字数共1452，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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{{Use American English|date = March 2019}}&lt;br /&gt;
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{{Short description|Probability distribution of energy states of a system}}&lt;br /&gt;
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{{about|system energy states|particle energy levels and velocities|Maxwell–Boltzmann distribution}}&lt;br /&gt;
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[[File:Boltzmann distribution graph.svg|upright=1.75|right|thumb|Boltzmann factor ''p&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;''&amp;amp;nbsp;/&amp;amp;nbsp;''p&amp;lt;sub&amp;gt;j&amp;lt;/sub&amp;gt;'' (vertical axis) as a function of temperature ''T'' for several energy differences ''ε&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;''&amp;amp;nbsp;−&amp;amp;nbsp;''ε&amp;lt;sub&amp;gt;j&amp;lt;/sub&amp;gt;''.|链接=Special:FilePath/Boltzmann_distribution_graph.svg]]&lt;br /&gt;
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In [[statistical mechanics]] and [[mathematics]], a '''Boltzmann distribution''' (also called '''Gibbs distribution'''&amp;lt;ref name=&amp;quot;landau&amp;quot;&amp;gt;{{cite book | author=Landau, Lev Davidovich |author2=Lifshitz, Evgeny Mikhailovich |name-list-style=amp | title=Statistical Physics |volume=5 |series=Course of Theoretical Physics |edition=3 |origyear=1976 |year=1980 |place=Oxford |publisher=Pergamon Press|isbn=0-7506-3372-7|author-link=Lev Landau |author2-link=Evgeny Lifshitz }} Translated by J.B. Sykes and M.J. Kearsley. See section 28&amp;lt;/ref&amp;gt;) is a [[probability distribution]] or [[probability measure]] that gives the probability that a system will be in a certain [[microstate (statistical mechanics)|state]] as a function of that state's energy and the temperature of the system. The distribution is expressed in the form:&lt;br /&gt;
&lt;br /&gt;
In statistical mechanics and mathematics, a Boltzmann distribution (also called Gibbs distribution) is a probability distribution or probability measure that gives the probability that a system will be in a certain state as a function of that state's energy and the temperature of the system. The distribution is expressed in the form:&lt;br /&gt;
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在统计力学和数学中，波兹曼分布分布(也称为吉布斯分布&amp;lt;ref name=&amp;quot;landau&amp;quot; /&amp;gt;)是一个概率分布或机率量测，它给出了一个系统处于某种量子态的概率，这个概率是该状态的能量和系统温度的函数。分布情况以下列形式表示:&lt;br /&gt;
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:&amp;lt;math&amp;gt;p_i \propto e^{-\frac{\varepsilon_i}{kT}}&amp;lt;/math&amp;gt; &lt;br /&gt;
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&amp;lt;math&amp;gt;p_i \propto e^{-\frac{\varepsilon_i}{kT}}&amp;lt;/math&amp;gt; &lt;br /&gt;
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[拉丁语]&lt;br /&gt;
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where {{mvar|p&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;}} is the probability of the system being in state {{mvar|i}}, {{mvar|ε&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;}} is the energy of that state, and a constant {{mvar|kT}} of the distribution is the product of [[Boltzmann's constant]] {{mvar|k}} and [[thermodynamic temperature]] {{mvar|T}}. The symbol &amp;lt;math display=&amp;quot;inline&amp;quot;&amp;gt;\propto&amp;lt;/math&amp;gt; denotes [[proportionality (mathematics)|proportionality]] (see {{section link||The distribution}} for the proportionality constant).&lt;br /&gt;
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where  is the probability of the system being in state ,  is the energy of that state, and a constant  of the distribution is the product of Boltzmann's constant  and thermodynamic temperature . The symbol &amp;lt;math display=&amp;quot;inline&amp;quot;&amp;gt;\propto&amp;lt;/math&amp;gt; denotes proportionality (see  for the proportionality constant).&lt;br /&gt;
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{{mvar|p&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;}} 是其中系统处于状态{{mvar|i}}的概率, {{mvar|ε&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;}} 是该状态的能量，还有关于这个分布的一个常数 {{mvar|kT}} ，它是玻耳兹曼常数{{mvar|k}}和热力学温度 {{mvar|T}} 的乘积。符号 &amp;lt;math display=&amp;quot;inline&amp;quot;&amp;gt;\propto&amp;lt;/math&amp;gt;表示相称性(见附录中的比例常数)。&lt;br /&gt;
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The term system here has a very wide meaning; it can range from a single atom to a macroscopic system such as a [[Natural gas storage|natural gas storage tank]]. Because of this the Boltzmann distribution can be used to solve a very wide variety of problems. The distribution shows that states with lower energy will always have a higher probability of being occupied .&lt;br /&gt;
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The term system here has a very wide meaning; it can range from a single atom to a macroscopic system such as a natural gas storage tank. Because of this the Boltzmann distribution can be used to solve a very wide variety of problems. The distribution shows that states with lower energy will always have a higher probability of being occupied .&lt;br /&gt;
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这里的术语系统含义广泛; 它可以从单个原子到宏观系统，如天然气储罐。正因为如此，波兹曼分布可以用来解决各种各样的问题。玻尔兹曼分布表明，能量较低的状态被占据的概率总是较高的。&lt;br /&gt;
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The ''ratio'' of probabilities of two states is known as the '''Boltzmann factor''' and characteristically only depends on the states' energy difference:&lt;br /&gt;
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The ratio of probabilities of two states is known as the Boltzmann factor and characteristically only depends on the states' energy difference:&lt;br /&gt;
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两种状态的概率之比被称为玻尔兹曼因子，取决于两种状态的能量差:&lt;br /&gt;
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:&amp;lt;math&amp;gt;\frac{p_i}{p_j} = e^{\frac{\varepsilon_j - \varepsilon_i}{kT}}&amp;lt;/math&amp;gt;&lt;br /&gt;
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&amp;lt;math&amp;gt;\frac{p_i}{p_j} = e^{\frac{\varepsilon_j - \varepsilon_i}{kT}}&amp;lt;/math&amp;gt;&lt;br /&gt;
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[数学][数学]&lt;br /&gt;
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The Boltzmann distribution is named after [[Ludwig Boltzmann]] who first formulated it in 1868 during his studies of the [[statistical mechanics]] of gases in thermal equilibrium. Boltzmann's statistical work is borne out in his paper “On the Relationship between the Second Fundamental Theorem of the Mechanical Theory of Heat and Probability Calculations Regarding the Conditions for Thermal Equilibrium&amp;quot;&amp;lt;ref&amp;gt;http://crystal.med.upenn.edu/sharp-lab-pdfs/2015SharpMatschinsky_Boltz1877_Entropy17.pdf&amp;lt;/ref&amp;gt;&lt;br /&gt;
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The Boltzmann distribution is named after Ludwig Boltzmann who first formulated it in 1868 during his studies of the statistical mechanics of gases in thermal equilibrium. Boltzmann's statistical work is borne out in his paper “On the Relationship between the Second Fundamental Theorem of the Mechanical Theory of Heat and Probability Calculations Regarding the Conditions for Thermal Equilibrium&amp;quot;&lt;br /&gt;
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波兹曼分布是根据路德维希·玻尔兹曼1868年在研究统计力学中气体热平衡的时候首次提出的一个公式命名的。波尔兹曼的统计工作在他1877年的论文《论热力学第二基本定理与热平衡条件的概率计算之间的关系》中得到了体现。&amp;lt;ref&amp;gt;“On the Relationship between the Second Fundamental Theorem of the Mechanical Theory of Heat and Probability Calculations Regarding the Conditions for Thermal Equilibrium” Sitzungberichte der Kaiserlichen Akademie der Wissenschaften. Mathematisch-Naturwissen Classe. Abt. II, LXXVI 1877, pp 373-435 (Wien. Ber. 1877, 76:373-435). &amp;lt;/ref&amp;gt;&lt;br /&gt;
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  It would be nice to have a citation here! The origin of the Boltzmann factor isn't entirely clear. According to some authors, Boltzmann's 1968 paper “On the Relationship between the Second Fundamental Theorem of the Mechanical Theory of Heat and Probability Calculations Regarding the Conditions for Thermal Equilibrium”&lt;br /&gt;
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  It would be nice to have a citation here! The origin of the Boltzmann factor isn't entirely clear. According to some authors, Boltzmann's 1968 paper “On the Relationship between the Second Fundamental Theorem of the Mechanical Theory of Heat and Probability Calculations Regarding the Conditions for Thermal Equilibrium”&lt;br /&gt;
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如果能在这里引用一下就好了！玻尔兹曼因子的起源并不完全清楚。根据一些作者的说法，Boltzmann 在1968年发表的论文《论热力学第二基本定理与热平衡条件的概率计算之间的关系》&lt;br /&gt;
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  &amp;quot;Studien über das Gleichgewicht der lebendigen Kraft zwischen bewegten materiellen Punkten&amp;quot; is the origin but I can't find this article at the moment,&lt;br /&gt;
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  &amp;quot;Studien über das Gleichgewicht der lebendigen Kraft zwischen bewegten materiellen Punkten&amp;quot; is the origin but I can't find this article at the moment,&lt;br /&gt;
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  &amp;quot;Studien über das Gleichgewicht der lebendigen Kraft zwischen bewegten materiellen Punkten&amp;quot; is the origin but I can't find this article at the moment,&lt;br /&gt;
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  so I cannot confirm.&lt;br /&gt;
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  so I cannot confirm.&lt;br /&gt;
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所以我不能确定。&lt;br /&gt;
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  For example, this book says so, but uses suspiciously modern terminology&lt;br /&gt;
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  For example, this book says so, but uses suspiciously modern terminology&lt;br /&gt;
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例如，这本书是这么说的，但是使用了可疑的现代术语&lt;br /&gt;
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    http://books.google.es/books?id=u13KiGlz2zcC&amp;amp;lpg=PA92&amp;amp;ots=8H1DRURdxn&amp;amp;pg=PA93#v=onepage&amp;amp;f=false&lt;br /&gt;
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    http://books.google.es/books?id=u13KiGlz2zcC&amp;amp;lpg=PA92&amp;amp;ots=8H1DRURdxn&amp;amp;pg=PA93#v=onepage&amp;amp;f=false&lt;br /&gt;
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Http://books.google.es/books?id=u13kiglz2zcc&amp;amp;lpg=pa92&amp;amp;ots=8h1drurdxn&amp;amp;pg=pa93#v=onepage&amp;amp;f=false&lt;br /&gt;
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  On the other hand, Uffink's &amp;quot;Compendium of the foundations of classical statistical physics&amp;quot; does not seem to indicate quite this equation but rather that Boltzmann's 1968 distribution was the simple Maxwell–Boltzmann distribution (for a classical nonrelativistic gas), modified for particles in a potential.&lt;br /&gt;
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  On the other hand, Uffink's &amp;quot;Compendium of the foundations of classical statistical physics&amp;quot; does not seem to indicate quite this equation but rather that Boltzmann's 1968 distribution was the simple Maxwell–Boltzmann distribution (for a classical nonrelativistic gas), modified for particles in a potential.&lt;br /&gt;
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另一方面，Uffink 的“经典统计物理学基础纲要”似乎并没有完全表明这个方程，而是说 Boltzmann 在1968年的分布是简单的 Maxwell-波兹曼分布(用于经典的非气体) ，修改为势中的粒子。&lt;br /&gt;
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The distribution was later investigated extensively, in its modern generic form, by [[Josiah Willard Gibbs]] in 1902.&amp;lt;ref name=&amp;quot;gibbs&amp;quot;&amp;gt;{{cite book |last=Gibbs |first=Josiah Willard |authorlink=Josiah Willard Gibbs |title=Elementary Principles in Statistical Mechanics |year=1902 |publisher=[[Charles Scribner's Sons]] &lt;br /&gt;
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The distribution was later investigated extensively, in its modern generic form, by Josiah Willard Gibbs in 1902.&lt;br /&gt;
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这种分布后来在1902年由约西亚·威拉德·吉布斯进行了广泛的调查，以其现代通用形式。&lt;br /&gt;
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|location=New York|title-link=Elementary Principles in Statistical Mechanics }}&amp;lt;/ref&amp;gt;{{rp|Ch.IV}}、&lt;br /&gt;
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在玻尔兹曼分布被发明之后，约西亚·华纳德·吉布森充分地研究了它并在1902年提出了它的一般形式。&amp;lt;ref name=&amp;quot;gibbs&amp;quot; /&amp;gt;&lt;br /&gt;
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The generalized Boltzmann distribution is a sufficient and necessary condition for the equivalence between the statistical mechanics definition of entropy (The  Gibbs entropy formula &amp;lt;math&amp;gt;S = -k_{\mathrm{B}}\sum_i p_i \log p_i&amp;lt;/math&amp;gt;) and the thermodynamic definition of entropy (&amp;lt;math&amp;gt;d S = \frac{\delta Q_\text{rev}}{T}&amp;lt;/math&amp;gt;, and the fundamental thermodynamic relation).&lt;br /&gt;
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The generalized Boltzmann distribution is a sufficient and necessary condition for the equivalence between the statistical mechanics definition of [[entropy]] (The [[Entropy_(statistical_thermodynamics)#Gibbs_entropy_formula | Gibbs entropy formula]] &amp;lt;math&amp;gt;S = -k_{\mathrm{B}}\sum_i p_i \log p_i&amp;lt;/math&amp;gt;) and the thermodynamic definition of entropy (&amp;lt;math&amp;gt;d S = \frac{\delta Q_\text{rev}}{T}&amp;lt;/math&amp;gt;, and the [[fundamental thermodynamic relation]]).&amp;lt;ref name=&amp;quot;:0&amp;quot;&amp;gt;{{cite journal |last1= Gao |first1= Xiang |last2= Gallicchio |first2= Emilio |first3= Adrian |last3= Roitberg  |date= 2019 |title= The generalized Boltzmann distribution is the only distribution in which the Gibbs-Shannon entropy equals the thermodynamic entropy |journal= The Journal of Chemical Physics|volume= 151|issue= 3|pages= 034113|doi= 10.1063/1.5111333|pmid= 31325924 |arxiv= 1903.02121 |s2cid= 118981017 }}&amp;lt;/ref&amp;gt;&lt;br /&gt;
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广义波兹曼分布是熵的统计力学定义(吉布斯熵公式  &amp;lt;math&amp;gt;S = -k_{\mathrm{B}}\sum_i p_i \log p_i&amp;lt;/math&amp;gt;))与熵的热力学定义(&amp;lt;math&amp;gt;d S = \frac{\delta Q_\text{rev}}{T}&amp;lt;/math&amp;gt;)等价的充要条件。&amp;lt;ref name=&amp;quot;:0&amp;quot; /&amp;gt;&lt;br /&gt;
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The Boltzmann distribution should not be confused with the Maxwell–Boltzmann distribution. The former gives the probability that a system will be in a certain state as a function of that state's energy; in contrast, the latter is used to describe particle speeds in idealized gases.&lt;br /&gt;
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值得一提的是，玻尔兹曼分布不应与麦克斯韦-玻尔兹曼分布混淆。前者给出了系统处于某种状态的概率，作为该状态能量的函数; 后者则是用于描述理想气体中的粒子速度。&lt;br /&gt;
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The Boltzmann distribution should not be confused with the [[Maxwell–Boltzmann distribution]]. The former gives the probability that a system will be in a certain state as a function of that state's energy;&amp;lt;ref name=&amp;quot;Atkins, P. W. 2010&amp;quot;&amp;gt;Atkins, P. W. (2010) Quanta, W. H. Freeman and Company, New York&amp;lt;/ref&amp;gt; in contrast, the latter is used to describe particle speeds in idealized gases.&lt;br /&gt;
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==The distribution==&lt;br /&gt;
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The Boltzmann distribution is a probability distribution that gives the probability of a certain state as a function of that state's energy and  temperature of the system to which the distribution is applied. It is given as&lt;br /&gt;
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波兹曼分布是一个概率分布，它给出了出于某种量子态处于某种能量和温度的时候的概率。它被这样定义：&lt;br /&gt;
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The Boltzmann distribution is a [[probability distribution]] that gives the probability of a certain state as a function of that state's energy and  temperature of the [[system]] to which the distribution is applied.&amp;lt;ref name=&amp;quot;McQuarrie, A. 2000&amp;quot;&amp;gt;McQuarrie, A. (2000) Statistical Mechanics, University Science Books, California&amp;lt;/ref&amp;gt; It is given as&lt;br /&gt;
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p_i=\frac{1}{Q}} {e^{- {\varepsilon}_i / k T}=\frac{e^{- {\varepsilon}_i / k T}}{\sum_{j=1}^{M}{e^{- {\varepsilon}_j / k T}}}&lt;br /&gt;
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P _ i = frac {1}{ q }{ e ^ {-{ varepsilon } _ i/k t } = frac { e ^ {-{ varepsilon } _ i/k t }{ sum { j = 1} ^ { m }{ e ^ {-{ varepsilon } _ j/k t }}}}}&lt;br /&gt;
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p_i=\frac{1}{Q}} {e^{- {\varepsilon}_i / k T}=\frac{e^{- {\varepsilon}_i / k T}}{\sum_{j=1}^{M}{e^{- {\varepsilon}_j / k T}}}&lt;br /&gt;
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where p&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt; is the probability of state i, ε&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt; the energy of state i, k the Boltzmann constant, T the temperature of the system and M is the number of all states accessible to the system of interest.&lt;br /&gt;
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where ''p&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;'' is the probability of state ''i'', ''ε&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;'' the energy of state ''i'', ''k'' the Boltzmann constant, ''T'' the temperature of the system and ''M'' is the number of all states accessible to the system of interest.&amp;lt;ref name=&amp;quot;McQuarrie, A. 2000&amp;quot; /&amp;gt;&amp;lt;ref name=&amp;quot;Atkins, P. W. 2010&amp;quot; /&amp;gt; Implied parentheses around the denominator ''kT'' are omitted for brevity. The normalization denominator ''Q'' (denoted by some authors by ''Z'') is the [[canonical partition function]]&lt;br /&gt;
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其中 ''p&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;'' 是状态 i 的概率，''ε&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;'' 是状态 i 的能量，''k'' 是波兹曼常数，''T'' 是系统的温度，''M'' 是系统所能到达的所有量子态的数目。&amp;lt;ref name=&amp;quot;Atkins, P. W. 2010&amp;quot; /&amp;gt; &amp;lt;ref name=&amp;quot;McQuarrie, A. 2000&amp;quot; /&amp;gt;这里为了简洁美观，省略了''kT''周围的括弧。归一化的分母''Q''（被有些作者写为''Z''）是对于系统中所有量子态进行总和，此部分又被称为[[Index.php?title=Canonical partition function|正则配分函数]]''。''&lt;br /&gt;
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It results from the constraint that the probabilities of all accessible states must add up to 1.&lt;br /&gt;
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所有量子态的概率之和为1.&lt;br /&gt;
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The Boltzmann distribution is the distribution that maximizes the [[entropy]]，&lt;br /&gt;
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&amp;lt;math&amp;gt;H(p_1,p_2,\cdots,p_M) = -\sum_{i=1}^{M} p_i\log_2 p_i&amp;lt;/math&amp;gt;&lt;br /&gt;
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&amp;lt;nowiki&amp;gt;subject to the constraint that {\sum{p_i {\varepsilon}_i}} equals a particular mean energy value (which can be proven using &amp;lt;/nowiki&amp;gt;[[Lagrange multipliers]]).&lt;br /&gt;
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&amp;lt;nowiki&amp;gt;当 {\sum{p_i {\varepsilon}_i}} 等于平均能量值时，玻尔兹曼分布是这种情况下能让熵最大化的分布。我们可以通过拉格朗日乘数法来证明。&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
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The partition function can be calculated if we know the energies of the states accessible to the system of interest. For atoms the partition function values can be found in the NIST Atomic Spectra Database.&amp;lt;ref name=&amp;quot;:1&amp;quot;&amp;gt;[http://physics.nist.gov/PhysRefData/ASD/levels_form.html NIST Atomic Spectra Database Levels Form] at nist.gov&amp;lt;/ref&amp;gt;&lt;br /&gt;
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在知道量子态能量的情况下，这个配分函数可以被计算。对于原子来说，配分函数的值可以在NIST Atomic Spectra Database中找到。&amp;lt;ref name=&amp;quot;:1&amp;quot; /&amp;gt;&lt;br /&gt;
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The distribution shows that states with lower energy will always have a higher probability of being occupied than the states with higher energy. It can also give us the quantitative relationship between the probabilities of the two states being occupied. The ratio of probabilities for states i and j is given as&lt;br /&gt;
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玻尔兹曼分布表明，能量较低的状态被占据的概率总是高于能量较高的状态被占据的概率。玻尔兹曼分布还给出两个量子态被占据的概率之间的定量关系。状态 i 和状态 j 的概率比为&lt;br /&gt;
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Q={\sum_{i=1}^{M}{e^{- {\varepsilon}_i / k T}}}&lt;br /&gt;
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&amp;lt;nowiki&amp;gt;{\frac{p_i}{p_j}}=e^{({\varepsilon}_j-{\varepsilon}_i) / k T}&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
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&amp;lt;nowiki&amp;gt;{\frac{p_i}{p_j}}=e^{({\varepsilon}_j-{\varepsilon}_i) / k T}&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
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where p&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt; is the probability of state i,  p&amp;lt;sub&amp;gt;j&amp;lt;/sub&amp;gt; the probability of state j, and ε&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt; and ε&amp;lt;sub&amp;gt;j&amp;lt;/sub&amp;gt; are the energies of states i and j, respectively.&lt;br /&gt;
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其中 p&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt; 是量子态 i 的概率， p&amp;lt;sub&amp;gt;j&amp;lt;/sub&amp;gt; 是量子态 j 的概率，ε  i  和 ε  j  分别是状态 i 和 j 的能量。&lt;br /&gt;
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The Boltzmann distribution is often used to describe the distribution of particles, such as atoms or molecules, over energy states accessible to them. If we have a system consisting of many particles, the probability of a particle being in state i is practically the probability that, if we pick a random particle from that system and check what state it is in, we will find it is in state i. This probability is equal to the number of particles in state i divided by the total number of particles in the system, that is the fraction of particles that occupy state i.&lt;br /&gt;
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玻尔兹曼分布通常被用来描述粒子的分布，比如原子或分子，在能量状态上的分布情况。如果我们有一个由许多粒子组成的系统，某个粒子处于量子态 i 的概率就等同于当我们从该系统中选择一个随机的粒子并观察它处于什么状态，发现它处于状态 i 的概率。这个概率等于量子态 i 的粒子数除以系统中粒子的总数，即那些占据量子态i的粒子的比例。&lt;br /&gt;
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&amp;lt;nowiki&amp;gt;&amp;lt;math display=&amp;quot;inline&amp;quot;&amp;gt;&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
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&amp;lt;nowiki&amp;gt;p_i={\frac{N_i}{N}}&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
&lt;br /&gt;
P _ i = { frac { n _ i }{ n }&lt;br /&gt;
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&amp;lt;nowiki&amp;gt;{\sum{p_i {\varepsilon}_i}}&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
where N&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt; is the number of particles in state i and N is the total number of particles in the system. We may use the Boltzmann distribution to find this probability that is, as we have seen, equal to the fraction of particles that are in state i. So the equation that gives the fraction of particles in state i as a function of the energy of that state is   In order for this to be possible, there must be some particles in the first state to undergo the transition. We may find that this condition is fulfilled by finding the fraction of particles in the first state. If it is negligible, the transition is very likely not to be observed at the temperature for which the calculation was done. In general, a larger fraction of molecules in the first state means a higher number of transitions to the second state. This gives a stronger spectral line. However, there are other factors that influence the intensity of a spectral line, such as whether it is caused by an allowed or a forbidden transition.&lt;br /&gt;
&lt;br /&gt;
N&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt; 是位于量子态 i 的粒子数，N是系统中粒子的总数。我们可以用波兹曼分布来求出这个概率，它等于处于量子态i的粒子的比例。所以这个方程给出位于量子态 i 的粒子比例关于这个状态能量的函数。为了使这成为可能，必须有一些粒子处于第一个量子态，等待着发生跃迁。我们可以通过求第一态粒子的比例来满足这个条件。如果它可以忽略不计，那么在当前计算的温度下，则很难观察到这种跃迁。一般来说，处于第一状态的分子比例越大，意味着向第二状态跃迁的次数越多。这就产生了一条更强的谱线。然而，还有其他因素影响谱线的强度，例如它是否是被允许的跃迁还是被禁止的跃迁。&lt;br /&gt;
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The Boltzmann distribution is related to the softmax function commonly used in machine learning.&lt;br /&gt;
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玻尔兹曼分布与机器学习中常用的归一化指数函数（Softmax 函数）有关。&lt;br /&gt;
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The distribution shows that states with lower energy will always have a higher probability of being occupied than the states with higher energy. It can also give us the quantitative relationship between the probabilities of the two states being occupied. The ratio of probabilities for states ''i'' and ''j'' is given as&lt;br /&gt;
&lt;br /&gt;
玻尔兹曼分布指出，能量低的量子态总是有比能量高的量子态更高的概率被粒子占据。它同时也能让我们定量地比较两个量子态分布概率的关系。&lt;br /&gt;
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:&amp;lt;math&amp;gt;&lt;br /&gt;
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{\frac{p_i}{p_j}}=e^{({\varepsilon}_j-{\varepsilon}_i) / k T}&lt;br /&gt;
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&amp;lt;/math&amp;gt;&lt;br /&gt;
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The Boltzmann distribution appears in statistical mechanics when considering isolated (or nearly-isolated) systems of fixed composition that are in thermal equilibrium (equilibrium with respect to energy exchange). The most general case is the probability distribution for the canonical ensemble, but also some special cases (derivable from the canonical ensemble) also show the Boltzmann distribution in different aspects:&lt;br /&gt;
&lt;br /&gt;
当独立的(或者几乎独立的)固定体系处于统计力学热平衡状态时，玻尔兹曼分布就会出现。最普遍的情况是概率分布的正则系综，但也有一些特殊的情况(从正则系综衍生)也显示了不同形式的玻尔兹曼分布:&lt;br /&gt;
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&lt;br /&gt;
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 Canonical ensemble (general case)&lt;br /&gt;
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'''正则系综(一般情况)'''&lt;br /&gt;
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 The canonical ensemble gives the probabilities of the various possible states of a closed system of fixed volume, in thermal equilibrium with a heat bath. The canonical ensemble is a probability distribution with the Boltzmann form.&lt;br /&gt;
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正则系综模型给出了在一个封闭固定体积，带有热浴的热平衡系统中的各种可能状态的概率。我们称正则系综为一个玻尔兹曼概率分布。&lt;br /&gt;
&lt;br /&gt;
 Statistical frequencies of subsystems' states (in a non-interacting collection)&lt;br /&gt;
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'''子系统状态的统计频率(在一个无交互的集合中)'''&lt;br /&gt;
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 When the system of interest is a collection of many non-interacting copies of a smaller subsystem, it is sometimes useful to find the statistical frequency of a given subsystem state, among the collection. The canonical ensemble has the property of separability when applied to such a collection: as long as the non-interacting subsystems have fixed composition, then each subsystem's state is independent of the others and is also characterized by a canonical ensemble. As a result, the expected statistical frequency distribution of subsystem states has the Boltzmann form.&lt;br /&gt;
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当系统是一个较小子系统的许多非交互副本的集合时，有时我们需要在某个子系统集合中找到某个子系统的统计频率。当应用于这样一个集合时，这个子系统的正则系综具有可分离性: 只要不相互作用的子系统的组成是固定的，那么每个子系统的状态都是独立于其他子系统的，它们也拥有自己的正则系综。因此，子系统状态的期望统计频率分布形式是玻尔兹曼分布。&lt;br /&gt;
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Maxwell–Boltzmann statistics of classical gases (systems of non-interacting particles)&lt;br /&gt;
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'''Maxwell-Boltzmann 统计中的经典气体系统(非相互作用粒子系统)'''&lt;br /&gt;
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In particle systems, many particles share the same space and regularly change places with each other; the single-particle state space they occupy is a shared space. Maxwell–Boltzmann statistics give the expected number of particles found in a given single-particle state, in a classical gas of non-interacting particles at equilibrium. This expected number distribution has the Boltzmann form.&lt;br /&gt;
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在粒子系统中，许多粒子共享同一空间，并且相互之间有规律地改变位置; 它们所占据的单粒子状态空间是一个共享空间。麦克斯韦-玻尔兹曼统计给出了在一个给定的单粒子态，在一个处于平衡状态的非相互作用粒子的经典气体中所发现的粒子的预期数量。这个预期的数量分布具有玻尔兹曼分布形式。&lt;br /&gt;
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Although these cases have strong similarities, it is helpful to distinguish them as they generalize in different ways when the crucial assumptions are changed:&lt;br /&gt;
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虽然这些案例有很多相似之处，但是当关键假设发生变化时，我们需要对它们以不同的方式进行归纳总结，因此区分它们是有帮助的:&lt;br /&gt;
&lt;br /&gt;
* When a system is in thermodynamic equilibrium with respect to both energy exchange ''and particle exchange'', the requirement of fixed composition is relaxed and a grand canonical ensembleis obtained rather than canonical ensemble. On the other hand, if both composition and energy are fixed, then a microcanonical ensemble applies instead.&lt;br /&gt;
* If the subsystems within a collection ''do'' interact with each other, then the expected frequencies of subsystem states no longer follow a Boltzmann distribution, and even may not have an analytical solution. The canonical ensemble can however still be applied to the ''collective'' states of the entire system considered as a whole, provided the entire system is in thermal equilibrium.&lt;br /&gt;
* With ''quantum'' gases of non-interacting particles in equilibrium, the number of particles found in a given single-particle state does not follow Maxwell–Boltzmann statistics, and there is no simple closed form expression for quantum gases in the canonical ensemble. In the grand canonical ensemble the state-filling statistics of quantum gases are described by Fermi–Dirac statistics or Bose–Einstein statistics, depending on whether the particles are fermions or bosons, respectively.&lt;br /&gt;
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This equation is of great importance to [[spectroscopy]]. In spectroscopy we observe a [[spectral line]] of atoms or molecules that we are interested in going from one state to another.&amp;lt;ref name=&amp;quot;Atkins, P. W. 2010&amp;quot;/&amp;gt;&amp;lt;ref&amp;gt;Atkins, P. W.; de Paula J. (2009) Physical Chemistry, 9th edition, Oxford University Press, Oxford, UK&amp;lt;/ref&amp;gt; In order for this to be possible, there must be some particles in the first state to undergo the transition. We may find that this condition is fulfilled by finding the fraction of particles in the first state. If it is negligible, the transition is very likely not to be observed at the temperature for which the calculation was done. In general, a larger fraction of molecules in the first state means a higher number of transitions to the second state.&amp;lt;ref&amp;gt;Skoog, D. A.; Holler, F. J.; Crouch, S. R. (2006) Principles of Instrumental Analysis, Brooks/Cole, Boston, MA&amp;lt;/ref&amp;gt; This gives a stronger spectral line. However, there are other factors that influence the intensity of a spectral line, such as whether it is caused by an allowed or a [[forbidden transition]].&lt;br /&gt;
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The Boltzmann distribution is related to the [[softmax function]] commonly used in machine learning.&lt;br /&gt;
&lt;br /&gt;
In more general mathematical settings, the Boltzmann distribution is also known as the Gibbs measure. In statistics and machine learning, it is called a log-linear model. In deep learning, the Boltzmann distribution is used in the sampling distribution of stochastic neural networks such as the Boltzmann machine, Restricted Boltzmann machine, Energy-Based models and deep Boltzmann machine.&lt;br /&gt;
&lt;br /&gt;
在更一般的数学环境中，波兹曼分布也被称为吉布斯量度。在统计学和机器学习中，它被称为对数线性回归。在深度学习中，波兹曼分布被用于随机神经网络的抽样分布，如波茨曼机、受限玻尔兹曼机、基于能量的模型和深度波茨曼机。&lt;br /&gt;
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== In statistical mechanics ==&lt;br /&gt;
&lt;br /&gt;
{{main|Canonical ensemble|Maxwell–Boltzmann statistics}}&lt;br /&gt;
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&lt;br /&gt;
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The Boltzmann distribution can be introduced to allocate permits in emissions trading. The new allocation method using the Boltzmann distribution can describe the most probable, natural, and unbiased distribution of emissions permits among multiple countries. Simple and versatile, this new method holds potential for many economic and environmental applications.&lt;br /&gt;
&lt;br /&gt;
可以引入欧盟波兹曼分布来分配排放交易的许可。这种新的排放量分配方法使用波兹曼分布能够描述多个国家之间最可能、最自然和最无偏见的排放量分配。这种新方法简单而通用，具有许多经济和环境应用的潜力。&lt;br /&gt;
&lt;br /&gt;
The Boltzmann distribution appears in [[statistical mechanics]] when considering isolated (or nearly-isolated) systems of fixed composition that are in [[thermal equilibrium]] (equilibrium with respect to energy exchange). The most general case is the probability distribution for the canonical ensemble, but also some special cases (derivable from the canonical ensemble) also show the Boltzmann distribution in different aspects:&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The Boltzmann distribution has the same form as the multinomial logit model. As a discrete choice model, this is very well known in economics since Daniel McFadden made the connection to random utility maximization.&lt;br /&gt;
&lt;br /&gt;
波兹曼分布与多项式 logit 模型具有相同的形式。作为一个离散选择模型，这在经济学中非常著名，因为丹尼尔 · 麦克法登提出了随机效用最大化的联系。&lt;br /&gt;
&lt;br /&gt;
; [[Canonical ensemble]] (general case)&lt;br /&gt;
&lt;br /&gt;
: The [[canonical ensemble]] gives the [[probabilities]] of the various possible states of a closed system of fixed volume, in thermal equilibrium with a [[heat bath]]. The canonical ensemble is a probability distribution with the Boltzmann form.&lt;br /&gt;
&lt;br /&gt;
; Statistical frequencies of subsystems' states (in a non-interacting collection)&lt;br /&gt;
&lt;br /&gt;
: When the system of interest is a collection of many non-interacting copies of a smaller subsystem, it is sometimes useful to find the [[statistical frequency]] of a given subsystem state, among the collection. The canonical ensemble has the property of separability when applied to such a collection: as long as the non-interacting subsystems have fixed composition, then each subsystem's state is independent of the others and is also characterized by a canonical ensemble. As a result, the [[expectation value|expected]] statistical frequency distribution of subsystem states has the Boltzmann form.&lt;br /&gt;
&lt;br /&gt;
; [[Maxwell–Boltzmann statistics]] of classical gases (systems of non-interacting particles)&lt;br /&gt;
&lt;br /&gt;
: In particle systems, many particles share the same space and regularly change places with each other; the single-particle state space they occupy is a shared space. [[Maxwell–Boltzmann statistics]] give the expected number of particles found in a given single-particle state, in a [[classical mechanics|classical]] gas of non-interacting particles at equilibrium. This expected number distribution has the Boltzmann form.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Although these cases have strong similarities, it is helpful to distinguish them as they generalize in different ways when the crucial assumptions are changed:&lt;br /&gt;
&lt;br /&gt;
* When a system is in thermodynamic equilibrium with respect to both energy exchange ''and particle exchange'', the requirement of fixed composition is relaxed and a [[grand canonical ensemble]] is obtained rather than canonical ensemble. On the other hand, if both composition and energy are fixed, then a [[microcanonical ensemble]] applies instead.&lt;br /&gt;
&lt;br /&gt;
* If the subsystems within a collection ''do'' interact with each other, then the expected frequencies of subsystem states no longer follow a Boltzmann distribution, and even may not have an [[analytical solution]].&amp;lt;ref&amp;gt;A classic example of this is [[magnetic ordering]]. Systems of non-interacting [[spin (physics)|spins]] show [[paramagnetic]] behaviour that can be understood with a single-particle canonical ensemble (resulting in the [[Brillouin function]]). Systems of ''interacting'' spins can show much more complex behaviour such as [[ferromagnetism]] or [[antiferromagnetism]].&amp;lt;/ref&amp;gt; The canonical ensemble can however still be applied to the ''collective'' states of the entire system considered as a whole, provided the entire system is isolated and in thermal equilibrium.&lt;br /&gt;
&lt;br /&gt;
* With ''[[quantum mechanics|quantum]]'' gases of non-interacting particles in equilibrium, the number of particles found in a given single-particle state does not follow Maxwell–Boltzmann statistics, and there is no simple closed form expression for quantum gases in the canonical ensemble. In the grand canonical ensemble the state-filling statistics of quantum gases are described by [[Fermi–Dirac statistics]] or [[Bose–Einstein statistics]], depending on whether the particles are [[fermion]]s or [[boson]]s respectively.&lt;br /&gt;
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&lt;br /&gt;
|year=1868&lt;br /&gt;
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1868年&lt;br /&gt;
&lt;br /&gt;
== In mathematics ==&lt;br /&gt;
&lt;br /&gt;
|title=Studien über das Gleichgewicht der lebendigen Kraft zwischen bewegten materiellen Punkten&lt;br /&gt;
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|title=Studien über das Gleichgewicht der lebendigen Kraft zwischen bewegten materiellen Punkten&lt;br /&gt;
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|trans-title=Studies on the balance of living force between moving material points&lt;br /&gt;
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| 反题 = 移动物质点之间生命力平衡的研究&lt;br /&gt;
&lt;br /&gt;
{{main|Gibbs measure|Log-linear model|Boltzmann machine}}&lt;br /&gt;
&lt;br /&gt;
|journal=Wiener Berichte |volume=58 |pages=517–560&lt;br /&gt;
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| journal = Wiener Berichte | volume = 58 | pages = 517-560&lt;br /&gt;
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}}&lt;br /&gt;
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}}&lt;br /&gt;
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In more general mathematical settings, the Boltzmann distribution is also known as the [[Gibbs measure]]. In statistics and machine learning, it is called a [[log-linear model]]. In [[deep learning]], the Boltzmann distribution is used in the sampling distribution of [[stochastic neural network]]s such as the [[Boltzmann machine]], [[Restricted Boltzmann machine]], [[Energy based model|Energy-Based models]] and [[Deep Boltzmann Machine|deep Boltzmann machine]].&lt;br /&gt;
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|first=Josiah Willard |last=Gibbs |authorlink=Josiah Willard Gibbs&lt;br /&gt;
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2012年10月15日 | 约西亚·威拉德·吉布斯&lt;br /&gt;
&lt;br /&gt;
== In economics ==&lt;br /&gt;
&lt;br /&gt;
|year=1902&lt;br /&gt;
&lt;br /&gt;
1902年&lt;br /&gt;
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|title=Elementary Principles in Statistical Mechanics&lt;br /&gt;
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统计力学的基本原理&lt;br /&gt;
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The Boltzmann distribution can be introduced to allocate permits in emissions trading.&amp;lt;ref name=&amp;quot;Park, J.-W. 2012&amp;quot;&amp;gt;Park, J.-W., Kim, C. U. and Isard, W. (2012) Permit allocation in emissions trading using the Boltzmann distribution. Physica A 391: 4883–4890&amp;lt;/ref&amp;gt;&amp;lt;ref&amp;gt;[http://www.technologyreview.com/view/425051/the-thorny-problem-of-fair-allocation/ The Thorny Problem Of Fair Allocation]. ''Technology Review'' blog. August 17, 2011. Cites and summarizes Park, Kim and Isard (2012).&amp;lt;/ref&amp;gt; The new allocation method using the Boltzmann distribution can describe the most probable, natural, and unbiased distribution of emissions permits among multiple countries. Simple and versatile, this new method holds potential for many economic and environmental applications.&lt;br /&gt;
&lt;br /&gt;
|title-link=Elementary Principles in Statistical Mechanics }}&lt;br /&gt;
&lt;br /&gt;
| title-link = 基本原理统计力学}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The Boltzmann distribution has the same form as the [[Multinomial logistic regression|multinomial logit]] model. As a [[discrete choice]] model, this is very well known in economics since [[Daniel McFadden]] made the connection to random utility maximization.&lt;br /&gt;
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Category:Statistical mechanics&lt;br /&gt;
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类别: 统计力学&lt;br /&gt;
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==See also==&lt;br /&gt;
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Distribution&lt;br /&gt;
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分布&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:Boltzmann distribution]]. Its edit history can be viewed at [[玻尔兹曼分布/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>Tueryeye</name></author>
	</entry>
	<entry>
		<id>https://wiki.swarma.org/index.php?title=%E7%8E%BB%E5%B0%94%E5%85%B9%E6%9B%BC%E5%88%86%E5%B8%83&amp;diff=26966</id>
		<title>玻尔兹曼分布</title>
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		<updated>2021-10-19T04:07:09Z</updated>

		<summary type="html">&lt;p&gt;Tueryeye：第二section的翻译&lt;/p&gt;
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&lt;div&gt;此词条暂由彩云小译翻译，翻译字数共1452，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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{{Use American English|date = March 2019}}&lt;br /&gt;
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{{Short description|Probability distribution of energy states of a system}}&lt;br /&gt;
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{{about|system energy states|particle energy levels and velocities|Maxwell–Boltzmann distribution}}&lt;br /&gt;
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[[File:Boltzmann distribution graph.svg|upright=1.75|right|thumb|Boltzmann factor ''p&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;''&amp;amp;nbsp;/&amp;amp;nbsp;''p&amp;lt;sub&amp;gt;j&amp;lt;/sub&amp;gt;'' (vertical axis) as a function of temperature ''T'' for several energy differences ''ε&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;''&amp;amp;nbsp;−&amp;amp;nbsp;''ε&amp;lt;sub&amp;gt;j&amp;lt;/sub&amp;gt;''.|链接=Special:FilePath/Boltzmann_distribution_graph.svg]]&lt;br /&gt;
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In [[statistical mechanics]] and [[mathematics]], a '''Boltzmann distribution''' (also called '''Gibbs distribution'''&amp;lt;ref name=&amp;quot;landau&amp;quot;&amp;gt;{{cite book | author=Landau, Lev Davidovich |author2=Lifshitz, Evgeny Mikhailovich |name-list-style=amp | title=Statistical Physics |volume=5 |series=Course of Theoretical Physics |edition=3 |origyear=1976 |year=1980 |place=Oxford |publisher=Pergamon Press|isbn=0-7506-3372-7|author-link=Lev Landau |author2-link=Evgeny Lifshitz }} Translated by J.B. Sykes and M.J. Kearsley. See section 28&amp;lt;/ref&amp;gt;) is a [[probability distribution]] or [[probability measure]] that gives the probability that a system will be in a certain [[microstate (statistical mechanics)|state]] as a function of that state's energy and the temperature of the system. The distribution is expressed in the form:&lt;br /&gt;
&lt;br /&gt;
In statistical mechanics and mathematics, a Boltzmann distribution (also called Gibbs distribution) is a probability distribution or probability measure that gives the probability that a system will be in a certain state as a function of that state's energy and the temperature of the system. The distribution is expressed in the form:&lt;br /&gt;
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在统计力学和数学中，波兹曼分布分布(也称为吉布斯分布&amp;lt;ref name=&amp;quot;landau&amp;quot; /&amp;gt;)是一个概率分布或机率量测，它给出了一个系统处于某种量子态的概率，这个概率是该状态的能量和系统温度的函数。分布情况以下列形式表示:&lt;br /&gt;
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:&amp;lt;math&amp;gt;p_i \propto e^{-\frac{\varepsilon_i}{kT}}&amp;lt;/math&amp;gt; &lt;br /&gt;
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&amp;lt;math&amp;gt;p_i \propto e^{-\frac{\varepsilon_i}{kT}}&amp;lt;/math&amp;gt; &lt;br /&gt;
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[拉丁语]&lt;br /&gt;
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where {{mvar|p&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;}} is the probability of the system being in state {{mvar|i}}, {{mvar|ε&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;}} is the energy of that state, and a constant {{mvar|kT}} of the distribution is the product of [[Boltzmann's constant]] {{mvar|k}} and [[thermodynamic temperature]] {{mvar|T}}. The symbol &amp;lt;math display=&amp;quot;inline&amp;quot;&amp;gt;\propto&amp;lt;/math&amp;gt; denotes [[proportionality (mathematics)|proportionality]] (see {{section link||The distribution}} for the proportionality constant).&lt;br /&gt;
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where  is the probability of the system being in state ,  is the energy of that state, and a constant  of the distribution is the product of Boltzmann's constant  and thermodynamic temperature . The symbol &amp;lt;math display=&amp;quot;inline&amp;quot;&amp;gt;\propto&amp;lt;/math&amp;gt; denotes proportionality (see  for the proportionality constant).&lt;br /&gt;
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{{mvar|p&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;}} 是其中系统处于状态{{mvar|i}}的概率, {{mvar|ε&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;}} 是该状态的能量，还有关于这个分布的一个常数 {{mvar|kT}} ，它是玻耳兹曼常数{{mvar|k}}和热力学温度 {{mvar|T}} 的乘积。符号 &amp;lt;math display=&amp;quot;inline&amp;quot;&amp;gt;\propto&amp;lt;/math&amp;gt;表示相称性(见附录中的比例常数)。&lt;br /&gt;
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The term system here has a very wide meaning; it can range from a single atom to a macroscopic system such as a [[Natural gas storage|natural gas storage tank]]. Because of this the Boltzmann distribution can be used to solve a very wide variety of problems. The distribution shows that states with lower energy will always have a higher probability of being occupied .&lt;br /&gt;
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The term system here has a very wide meaning; it can range from a single atom to a macroscopic system such as a natural gas storage tank. Because of this the Boltzmann distribution can be used to solve a very wide variety of problems. The distribution shows that states with lower energy will always have a higher probability of being occupied .&lt;br /&gt;
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这里的术语系统含义广泛; 它可以从单个原子到宏观系统，如天然气储罐。正因为如此，波兹曼分布可以用来解决各种各样的问题。玻尔兹曼分布表明，能量较低的状态被占据的概率总是较高的。&lt;br /&gt;
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The ''ratio'' of probabilities of two states is known as the '''Boltzmann factor''' and characteristically only depends on the states' energy difference:&lt;br /&gt;
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The ratio of probabilities of two states is known as the Boltzmann factor and characteristically only depends on the states' energy difference:&lt;br /&gt;
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两种状态的概率之比被称为玻尔兹曼因子，取决于两种状态的能量差:&lt;br /&gt;
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:&amp;lt;math&amp;gt;\frac{p_i}{p_j} = e^{\frac{\varepsilon_j - \varepsilon_i}{kT}}&amp;lt;/math&amp;gt;&lt;br /&gt;
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&amp;lt;math&amp;gt;\frac{p_i}{p_j} = e^{\frac{\varepsilon_j - \varepsilon_i}{kT}}&amp;lt;/math&amp;gt;&lt;br /&gt;
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[数学][数学]&lt;br /&gt;
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The Boltzmann distribution is named after [[Ludwig Boltzmann]] who first formulated it in 1868 during his studies of the [[statistical mechanics]] of gases in thermal equilibrium. Boltzmann's statistical work is borne out in his paper “On the Relationship between the Second Fundamental Theorem of the Mechanical Theory of Heat and Probability Calculations Regarding the Conditions for Thermal Equilibrium&amp;quot;&amp;lt;ref&amp;gt;http://crystal.med.upenn.edu/sharp-lab-pdfs/2015SharpMatschinsky_Boltz1877_Entropy17.pdf&amp;lt;/ref&amp;gt;&lt;br /&gt;
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The Boltzmann distribution is named after Ludwig Boltzmann who first formulated it in 1868 during his studies of the statistical mechanics of gases in thermal equilibrium. Boltzmann's statistical work is borne out in his paper “On the Relationship between the Second Fundamental Theorem of the Mechanical Theory of Heat and Probability Calculations Regarding the Conditions for Thermal Equilibrium&amp;quot;&lt;br /&gt;
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波兹曼分布是根据路德维希·玻尔兹曼1868年在研究统计力学中气体热平衡的时候首次提出的一个公式命名的。波尔兹曼的统计工作在他1877年的论文《论热力学第二基本定理与热平衡条件的概率计算之间的关系》中得到了体现。&amp;lt;ref&amp;gt;“On the Relationship between the Second Fundamental Theorem of the Mechanical Theory of Heat and Probability Calculations Regarding the Conditions for Thermal Equilibrium” Sitzungberichte der Kaiserlichen Akademie der Wissenschaften. Mathematisch-Naturwissen Classe. Abt. II, LXXVI 1877, pp 373-435 (Wien. Ber. 1877, 76:373-435). &amp;lt;/ref&amp;gt;&lt;br /&gt;
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  It would be nice to have a citation here! The origin of the Boltzmann factor isn't entirely clear. According to some authors, Boltzmann's 1968 paper “On the Relationship between the Second Fundamental Theorem of the Mechanical Theory of Heat and Probability Calculations Regarding the Conditions for Thermal Equilibrium”&lt;br /&gt;
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  It would be nice to have a citation here! The origin of the Boltzmann factor isn't entirely clear. According to some authors, Boltzmann's 1968 paper “On the Relationship between the Second Fundamental Theorem of the Mechanical Theory of Heat and Probability Calculations Regarding the Conditions for Thermal Equilibrium”&lt;br /&gt;
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如果能在这里引用一下就好了！玻尔兹曼因子的起源并不完全清楚。根据一些作者的说法，Boltzmann 在1968年发表的论文《论热力学第二基本定理与热平衡条件的概率计算之间的关系》&lt;br /&gt;
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  &amp;quot;Studien über das Gleichgewicht der lebendigen Kraft zwischen bewegten materiellen Punkten&amp;quot; is the origin but I can't find this article at the moment,&lt;br /&gt;
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  &amp;quot;Studien über das Gleichgewicht der lebendigen Kraft zwischen bewegten materiellen Punkten&amp;quot; is the origin but I can't find this article at the moment,&lt;br /&gt;
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  &amp;quot;Studien über das Gleichgewicht der lebendigen Kraft zwischen bewegten materiellen Punkten&amp;quot; is the origin but I can't find this article at the moment,&lt;br /&gt;
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  so I cannot confirm.&lt;br /&gt;
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  so I cannot confirm.&lt;br /&gt;
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所以我不能确定。&lt;br /&gt;
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  For example, this book says so, but uses suspiciously modern terminology&lt;br /&gt;
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  For example, this book says so, but uses suspiciously modern terminology&lt;br /&gt;
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例如，这本书是这么说的，但是使用了可疑的现代术语&lt;br /&gt;
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    http://books.google.es/books?id=u13KiGlz2zcC&amp;amp;lpg=PA92&amp;amp;ots=8H1DRURdxn&amp;amp;pg=PA93#v=onepage&amp;amp;f=false&lt;br /&gt;
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    http://books.google.es/books?id=u13KiGlz2zcC&amp;amp;lpg=PA92&amp;amp;ots=8H1DRURdxn&amp;amp;pg=PA93#v=onepage&amp;amp;f=false&lt;br /&gt;
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Http://books.google.es/books?id=u13kiglz2zcc&amp;amp;lpg=pa92&amp;amp;ots=8h1drurdxn&amp;amp;pg=pa93#v=onepage&amp;amp;f=false&lt;br /&gt;
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  On the other hand, Uffink's &amp;quot;Compendium of the foundations of classical statistical physics&amp;quot; does not seem to indicate quite this equation but rather that Boltzmann's 1968 distribution was the simple Maxwell–Boltzmann distribution (for a classical nonrelativistic gas), modified for particles in a potential.&lt;br /&gt;
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  On the other hand, Uffink's &amp;quot;Compendium of the foundations of classical statistical physics&amp;quot; does not seem to indicate quite this equation but rather that Boltzmann's 1968 distribution was the simple Maxwell–Boltzmann distribution (for a classical nonrelativistic gas), modified for particles in a potential.&lt;br /&gt;
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另一方面，Uffink 的“经典统计物理学基础纲要”似乎并没有完全表明这个方程，而是说 Boltzmann 在1968年的分布是简单的 Maxwell-波兹曼分布(用于经典的非气体) ，修改为势中的粒子。&lt;br /&gt;
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The distribution was later investigated extensively, in its modern generic form, by [[Josiah Willard Gibbs]] in 1902.&amp;lt;ref name=&amp;quot;gibbs&amp;quot;&amp;gt;{{cite book |last=Gibbs |first=Josiah Willard |authorlink=Josiah Willard Gibbs |title=Elementary Principles in Statistical Mechanics |year=1902 |publisher=[[Charles Scribner's Sons]] &lt;br /&gt;
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The distribution was later investigated extensively, in its modern generic form, by Josiah Willard Gibbs in 1902.&lt;br /&gt;
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这种分布后来在1902年由约西亚·威拉德·吉布斯进行了广泛的调查，以其现代通用形式。&lt;br /&gt;
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|location=New York|title-link=Elementary Principles in Statistical Mechanics }}&amp;lt;/ref&amp;gt;{{rp|Ch.IV}}、&lt;br /&gt;
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在玻尔兹曼分布被发明之后，约西亚·华纳德·吉布森充分地研究了它并在1902年提出了它的一般形式。&amp;lt;ref name=&amp;quot;gibbs&amp;quot; /&amp;gt;&lt;br /&gt;
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The generalized Boltzmann distribution is a sufficient and necessary condition for the equivalence between the statistical mechanics definition of entropy (The  Gibbs entropy formula &amp;lt;math&amp;gt;S = -k_{\mathrm{B}}\sum_i p_i \log p_i&amp;lt;/math&amp;gt;) and the thermodynamic definition of entropy (&amp;lt;math&amp;gt;d S = \frac{\delta Q_\text{rev}}{T}&amp;lt;/math&amp;gt;, and the fundamental thermodynamic relation).&lt;br /&gt;
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The generalized Boltzmann distribution is a sufficient and necessary condition for the equivalence between the statistical mechanics definition of [[entropy]] (The [[Entropy_(statistical_thermodynamics)#Gibbs_entropy_formula | Gibbs entropy formula]] &amp;lt;math&amp;gt;S = -k_{\mathrm{B}}\sum_i p_i \log p_i&amp;lt;/math&amp;gt;) and the thermodynamic definition of entropy (&amp;lt;math&amp;gt;d S = \frac{\delta Q_\text{rev}}{T}&amp;lt;/math&amp;gt;, and the [[fundamental thermodynamic relation]]).&amp;lt;ref name=&amp;quot;:0&amp;quot;&amp;gt;{{cite journal |last1= Gao |first1= Xiang |last2= Gallicchio |first2= Emilio |first3= Adrian |last3= Roitberg  |date= 2019 |title= The generalized Boltzmann distribution is the only distribution in which the Gibbs-Shannon entropy equals the thermodynamic entropy |journal= The Journal of Chemical Physics|volume= 151|issue= 3|pages= 034113|doi= 10.1063/1.5111333|pmid= 31325924 |arxiv= 1903.02121 |s2cid= 118981017 }}&amp;lt;/ref&amp;gt;&lt;br /&gt;
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广义波兹曼分布是熵的统计力学定义(吉布斯熵公式  &amp;lt;math&amp;gt;S = -k_{\mathrm{B}}\sum_i p_i \log p_i&amp;lt;/math&amp;gt;))与熵的热力学定义(&amp;lt;math&amp;gt;d S = \frac{\delta Q_\text{rev}}{T}&amp;lt;/math&amp;gt;)等价的充要条件。&amp;lt;ref name=&amp;quot;:0&amp;quot; /&amp;gt;&lt;br /&gt;
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The Boltzmann distribution should not be confused with the Maxwell–Boltzmann distribution. The former gives the probability that a system will be in a certain state as a function of that state's energy; in contrast, the latter is used to describe particle speeds in idealized gases.&lt;br /&gt;
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值得一提的是，玻尔兹曼分布不应与麦克斯韦-玻尔兹曼分布混淆。前者给出了系统处于某种状态的概率，作为该状态能量的函数; 后者则是用于描述理想气体中的粒子速度。&lt;br /&gt;
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The Boltzmann distribution should not be confused with the [[Maxwell–Boltzmann distribution]]. The former gives the probability that a system will be in a certain state as a function of that state's energy;&amp;lt;ref name=&amp;quot;Atkins, P. W. 2010&amp;quot;&amp;gt;Atkins, P. W. (2010) Quanta, W. H. Freeman and Company, New York&amp;lt;/ref&amp;gt; in contrast, the latter is used to describe particle speeds in idealized gases.&lt;br /&gt;
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==The distribution==&lt;br /&gt;
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The Boltzmann distribution is a probability distribution that gives the probability of a certain state as a function of that state's energy and  temperature of the system to which the distribution is applied. It is given as&lt;br /&gt;
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波兹曼分布是一个概率分布，它给出了出于某种量子态处于某种能量和温度的时候的概率。它被这样定义：&lt;br /&gt;
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The Boltzmann distribution is a [[probability distribution]] that gives the probability of a certain state as a function of that state's energy and  temperature of the [[system]] to which the distribution is applied.&amp;lt;ref name=&amp;quot;McQuarrie, A. 2000&amp;quot;&amp;gt;McQuarrie, A. (2000) Statistical Mechanics, University Science Books, California&amp;lt;/ref&amp;gt; It is given as&lt;br /&gt;
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p_i=\frac{1}{Q}} {e^{- {\varepsilon}_i / k T}=\frac{e^{- {\varepsilon}_i / k T}}{\sum_{j=1}^{M}{e^{- {\varepsilon}_j / k T}}}&lt;br /&gt;
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P _ i = frac {1}{ q }{ e ^ {-{ varepsilon } _ i/k t } = frac { e ^ {-{ varepsilon } _ i/k t }{ sum { j = 1} ^ { m }{ e ^ {-{ varepsilon } _ j/k t }}}}}&lt;br /&gt;
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p_i=\frac{1}{Q}} {e^{- {\varepsilon}_i / k T}=\frac{e^{- {\varepsilon}_i / k T}}{\sum_{j=1}^{M}{e^{- {\varepsilon}_j / k T}}}&lt;br /&gt;
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where p&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt; is the probability of state i, ε&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt; the energy of state i, k the Boltzmann constant, T the temperature of the system and M is the number of all states accessible to the system of interest.&lt;br /&gt;
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where ''p&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;'' is the probability of state ''i'', ''ε&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;'' the energy of state ''i'', ''k'' the Boltzmann constant, ''T'' the temperature of the system and ''M'' is the number of all states accessible to the system of interest.&amp;lt;ref name=&amp;quot;McQuarrie, A. 2000&amp;quot; /&amp;gt;&amp;lt;ref name=&amp;quot;Atkins, P. W. 2010&amp;quot; /&amp;gt; Implied parentheses around the denominator ''kT'' are omitted for brevity. The normalization denominator ''Q'' (denoted by some authors by ''Z'') is the [[canonical partition function]]&lt;br /&gt;
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其中 ''p&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;'' 是状态 i 的概率，''ε&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;'' 是状态 i 的能量，''k'' 是波兹曼常数，''T'' 是系统的温度，''M'' 是系统所能到达的所有量子态的数目。&amp;lt;ref name=&amp;quot;Atkins, P. W. 2010&amp;quot; /&amp;gt; &amp;lt;ref name=&amp;quot;McQuarrie, A. 2000&amp;quot; /&amp;gt;这里为了简洁美观，省略了''kT''周围的括弧。归一化的分母''Q''（被有些作者写为''Z''）是对于系统中所有量子态进行总和，此部分又被称为[[Index.php?title=Canonical partition function|正则配分函数]]''。''&lt;br /&gt;
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The distribution shows that states with lower energy will always have a higher probability of being occupied than the states with higher energy. It can also give us the quantitative relationship between the probabilities of the two states being occupied. The ratio of probabilities for states i and j is given as&lt;br /&gt;
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玻尔兹曼分布表明，能量较低的状态被占据的概率总是高于能量较高的状态被占据的概率。玻尔兹曼分布还给出两个量子态被占据的概率之间的定量关系。状态 i 和状态 j 的概率比为&lt;br /&gt;
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Q={\sum_{i=1}^{M}{e^{- {\varepsilon}_i / k T}}}&lt;br /&gt;
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{\frac{p_i}{p_j}}=e^{({\varepsilon}_j-{\varepsilon}_i) / k T}&lt;br /&gt;
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&amp;lt;nowiki&amp;gt;{\frac{p_i}{p_j}}=e^{({\varepsilon}_j-{\varepsilon}_i) / k T}&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
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It results from the constraint that the probabilities of all accessible states must add up to 1.&lt;br /&gt;
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所有量子态的概率之和为1.&lt;br /&gt;
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where p&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt; is the probability of state i,  p&amp;lt;sub&amp;gt;j&amp;lt;/sub&amp;gt; the probability of state j, and ε&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt; and ε&amp;lt;sub&amp;gt;j&amp;lt;/sub&amp;gt; are the energies of states i and j, respectively.&lt;br /&gt;
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其中 p&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt; 是量子态 i 的概率， p&amp;lt;sub&amp;gt;j&amp;lt;/sub&amp;gt; 是量子态 j 的概率，ε  i  和 ε  j  分别是状态 i 和 j 的能量。&lt;br /&gt;
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The Boltzmann distribution is the distribution that maximizes the [[entropy]]&lt;br /&gt;
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假如说平均温度是固定的，玻尔兹曼分布是这种情况下能让熵最大化的分布。&lt;br /&gt;
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The Boltzmann distribution is often used to describe the distribution of particles, such as atoms or molecules, over energy states accessible to them. If we have a system consisting of many particles, the probability of a particle being in state i is practically the probability that, if we pick a random particle from that system and check what state it is in, we will find it is in state i. This probability is equal to the number of particles in state i divided by the total number of particles in the system, that is the fraction of particles that occupy state i.&lt;br /&gt;
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玻尔兹曼分布通常被用来描述粒子的分布，比如原子或分子，在能量状态上的分布情况。如果我们有一个由许多粒子组成的系统，某个粒子处于量子态 i 的概率就等同于当我们从该系统中选择一个随机的粒子并观察它处于什么状态，发现它处于状态 i 的概率。这个概率等于量子态 i 的粒子数除以系统中粒子的总数，即那些占据量子态i的粒子的比例。&lt;br /&gt;
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:&amp;lt;math&amp;gt;H(p_1,p_2,\cdots,p_M) = -\sum_{i=1}^{M} p_i\log_2 p_i&amp;lt;/math&amp;gt;&lt;br /&gt;
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subject to the constraint that &amp;lt;math display=&amp;quot;inline&amp;quot;&amp;gt;&lt;br /&gt;
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p_i={\frac{N_i}{N}}&lt;br /&gt;
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P _ i = { frac { n _ i }{ n }&lt;br /&gt;
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{\sum{p_i {\varepsilon}_i}}&lt;br /&gt;
&lt;br /&gt;
&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
数学&lt;br /&gt;
&lt;br /&gt;
&amp;lt;/math&amp;gt; equals a particular mean energy value (which can be proven using [[Lagrange multipliers]]).&lt;br /&gt;
&lt;br /&gt;
这也等于一个平均能量值。我们可以通过拉格朗日乘数法来证明。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
where N&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt; is the number of particles in state i and N is the total number of particles in the system. We may use the Boltzmann distribution to find this probability that is, as we have seen, equal to the fraction of particles that are in state i. So the equation that gives the fraction of particles in state i as a function of the energy of that state is   In order for this to be possible, there must be some particles in the first state to undergo the transition. We may find that this condition is fulfilled by finding the fraction of particles in the first state. If it is negligible, the transition is very likely not to be observed at the temperature for which the calculation was done. In general, a larger fraction of molecules in the first state means a higher number of transitions to the second state. This gives a stronger spectral line. However, there are other factors that influence the intensity of a spectral line, such as whether it is caused by an allowed or a forbidden transition.&lt;br /&gt;
&lt;br /&gt;
N&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt; 是位于量子态 i 的粒子数，N是系统中粒子的总数。我们可以用波兹曼分布来求出这个概率，它等于处于量子态i的粒子的比例。所以这个方程给出位于量子态 i 的粒子比例关于这个状态能量的函数。为了使这成为可能，必须有一些粒子处于第一个量子态，等待着发生跃迁。我们可以通过求第一态粒子的比例来满足这个条件。如果它可以忽略不计，那么在进行计算的温度下，极有可能不能观察到这种转变。一般来说，处于第一状态的分子比例越大，意味着向第二状态转变的次数越多。这就产生了一条更强的谱线。然而，还有其他因素影响谱线的强度，例如它是由允许的跃迁还是禁止的跃迁引起的。&lt;br /&gt;
&lt;br /&gt;
The partition function can be calculated if we know the energies of the states accessible to the system of interest. For atoms the partition function values can be found in the NIST Atomic Spectra Database.&amp;lt;ref&amp;gt;[http://physics.nist.gov/PhysRefData/ASD/levels_form.html NIST Atomic Spectra Database Levels Form] at nist.gov&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The Boltzmann distribution is related to the softmax function commonly used in machine learning.&lt;br /&gt;
&lt;br /&gt;
波兹曼分布学习与机器学习中常用的柔性最大激活函数学习有关。&lt;br /&gt;
&lt;br /&gt;
The distribution shows that states with lower energy will always have a higher probability of being occupied than the states with higher energy. It can also give us the quantitative relationship between the probabilities of the two states being occupied. The ratio of probabilities for states ''i'' and ''j'' is given as&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
{\frac{p_i}{p_j}}=e^{({\varepsilon}_j-{\varepsilon}_i) / k T}&lt;br /&gt;
&lt;br /&gt;
&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
The Boltzmann distribution appears in statistical mechanics when considering isolated (or nearly-isolated) systems of fixed composition that are in thermal equilibrium (equilibrium with respect to energy exchange). The most general case is the probability distribution for the canonical ensemble, but also some special cases (derivable from the canonical ensemble) also show the Boltzmann distribution in different aspects:&lt;br /&gt;
&lt;br /&gt;
当考虑孤立的(或者几乎孤立的)固定组成的体系处于平衡状态时，波兹曼分布出现在《统计力学热平衡。最普遍的情况是概率分布的正则系综，但也有一些特殊的情况(从正则系综衍生)也显示了波兹曼分布在不同的方面:&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
where ''p&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;'' is the probability of state ''i'',  ''p&amp;lt;sub&amp;gt;j&amp;lt;/sub&amp;gt;'' the probability of state ''j'', and ''ε&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;'' and ''ε&amp;lt;sub&amp;gt;j&amp;lt;/sub&amp;gt;'' are the energies of states ''i'' and ''j'', respectively.&lt;br /&gt;
&lt;br /&gt;
 Canonical ensemble (general case)&lt;br /&gt;
&lt;br /&gt;
正则系综(一般情况)&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
 The canonical ensemble gives the probabilities of the various possible states of a closed system of fixed volume, in thermal equilibrium with a heat bath. The canonical ensemble is a probability distribution with the Boltzmann form.&lt;br /&gt;
&lt;br /&gt;
正则系综模型给出了一个封闭的固定体积系统的各种可能状态的概率，这个封闭体积系统包括一个带有热浴的热平衡。正则系综是一个玻尔兹曼概率分布。&lt;br /&gt;
&lt;br /&gt;
The Boltzmann distribution is often used to describe the distribution of particles, such as atoms or molecules, over energy states accessible to them. If we have a system consisting of many particles, the probability of a particle being in state ''i'' is practically the probability that, if we pick a random particle from that system and check what state it is in, we will find it is in state ''i''. This probability is equal to the number of particles in state ''i'' divided by the total number of particles in the system, that is the fraction of particles that occupy state ''i''.&lt;br /&gt;
&lt;br /&gt;
 Statistical frequencies of subsystems' states (in a non-interacting collection)&lt;br /&gt;
&lt;br /&gt;
子系统状态的统计频率(在一个无交互的集合中)&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
 When the system of interest is a collection of many non-interacting copies of a smaller subsystem, it is sometimes useful to find the statistical frequency of a given subsystem state, among the collection. The canonical ensemble has the property of separability when applied to such a collection: as long as the non-interacting subsystems have fixed composition, then each subsystem's state is independent of the others and is also characterized by a canonical ensemble. As a result, the expected statistical frequency distribution of subsystem states has the Boltzmann form.&lt;br /&gt;
&lt;br /&gt;
当感兴趣的系统是一个较小子系统的许多非交互副本的集合时，在集合中查找给定子系统状态的统计频率有时是有用的。当应用于这样一个集合时，正则系综子系统具有可分离性: 只要不相互作用的子系统的组成是固定的，那么每个子系统的状态是独立于其他子系统的，也是一个拥有属性正则系综。因此，子系统状态的期望统计频率分布具有玻耳兹曼形式。&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 Maxwell–Boltzmann statistics of classical gases (systems of non-interacting particles)&lt;br /&gt;
&lt;br /&gt;
经典气体(非相互作用粒子系统)的 Maxwell-Boltzmann 统计&lt;br /&gt;
&lt;br /&gt;
p_i={\frac{N_i}{N}}&lt;br /&gt;
&lt;br /&gt;
 In particle systems, many particles share the same space and regularly change places with each other; the single-particle state space they occupy is a shared space. Maxwell–Boltzmann statistics give the expected number of particles found in a given single-particle state, in a classical gas of non-interacting particles at equilibrium. This expected number distribution has the Boltzmann form.&lt;br /&gt;
&lt;br /&gt;
在粒子系统中，许多粒子共享同一空间，并且相互之间有规律地改变位置; 它们所占据的单粒子状态空间是一个共享空间。麦克斯韦-玻尔兹曼统计给出了在一个给定的单粒子态，在一个处于平衡状态的非相互作用粒子的经典气体中所发现的粒子的预期数量。这个预期的数分布具有玻耳兹曼形式。&lt;br /&gt;
&lt;br /&gt;
&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Although these cases have strong similarities, it is helpful to distinguish them as they generalize in different ways when the crucial assumptions are changed:&lt;br /&gt;
&lt;br /&gt;
虽然这些案例有很多相似之处，但是当关键假设发生变化时，它们以不同的方式进行归纳，因此区分它们是有帮助的:&lt;br /&gt;
&lt;br /&gt;
where ''N&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;'' is the number of particles in state ''i'' and ''N'' is the total number of particles in the system. We may use the Boltzmann distribution to find this probability that is, as we have seen, equal to the fraction of particles that are in state i. So the equation that gives the fraction of particles in state ''i'' as a function of the energy of that state is  &amp;lt;ref name=&amp;quot;Atkins, P. W. 2010&amp;quot;/&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
{\frac{N_i}{N}}={\frac{e^{- {\varepsilon}_i / k T}}{\sum_{j=1}^{M}{e^{- {\varepsilon}_j / k T}}}}&lt;br /&gt;
&lt;br /&gt;
&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
This equation is of great importance to [[spectroscopy]]. In spectroscopy we observe a [[spectral line]] of atoms or molecules that we are interested in going from one state to another.&amp;lt;ref name=&amp;quot;Atkins, P. W. 2010&amp;quot;/&amp;gt;&amp;lt;ref&amp;gt;Atkins, P. W.; de Paula J. (2009) Physical Chemistry, 9th edition, Oxford University Press, Oxford, UK&amp;lt;/ref&amp;gt; In order for this to be possible, there must be some particles in the first state to undergo the transition. We may find that this condition is fulfilled by finding the fraction of particles in the first state. If it is negligible, the transition is very likely not to be observed at the temperature for which the calculation was done. In general, a larger fraction of molecules in the first state means a higher number of transitions to the second state.&amp;lt;ref&amp;gt;Skoog, D. A.; Holler, F. J.; Crouch, S. R. (2006) Principles of Instrumental Analysis, Brooks/Cole, Boston, MA&amp;lt;/ref&amp;gt; This gives a stronger spectral line. However, there are other factors that influence the intensity of a spectral line, such as whether it is caused by an allowed or a [[forbidden transition]].&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The Boltzmann distribution is related to the [[softmax function]] commonly used in machine learning.&lt;br /&gt;
&lt;br /&gt;
In more general mathematical settings, the Boltzmann distribution is also known as the Gibbs measure. In statistics and machine learning, it is called a log-linear model. In deep learning, the Boltzmann distribution is used in the sampling distribution of stochastic neural networks such as the Boltzmann machine, Restricted Boltzmann machine, Energy-Based models and deep Boltzmann machine.&lt;br /&gt;
&lt;br /&gt;
在更一般的数学环境中，波兹曼分布也被称为吉布斯量度。在统计学和机器学习中，它被称为对数线性回归。在深度学习中，波兹曼分布被用于随机神经网络的抽样分布，如波茨曼机、受限玻尔兹曼机、基于能量的模型和深度波茨曼机。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
== In statistical mechanics ==&lt;br /&gt;
&lt;br /&gt;
{{main|Canonical ensemble|Maxwell–Boltzmann statistics}}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The Boltzmann distribution can be introduced to allocate permits in emissions trading. The new allocation method using the Boltzmann distribution can describe the most probable, natural, and unbiased distribution of emissions permits among multiple countries. Simple and versatile, this new method holds potential for many economic and environmental applications.&lt;br /&gt;
&lt;br /&gt;
可以引入欧盟波兹曼分布来分配排放交易的许可。这种新的排放量分配方法使用波兹曼分布能够描述多个国家之间最可能、最自然和最无偏见的排放量分配。这种新方法简单而通用，具有许多经济和环境应用的潜力。&lt;br /&gt;
&lt;br /&gt;
The Boltzmann distribution appears in [[statistical mechanics]] when considering isolated (or nearly-isolated) systems of fixed composition that are in [[thermal equilibrium]] (equilibrium with respect to energy exchange). The most general case is the probability distribution for the canonical ensemble, but also some special cases (derivable from the canonical ensemble) also show the Boltzmann distribution in different aspects:&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The Boltzmann distribution has the same form as the multinomial logit model. As a discrete choice model, this is very well known in economics since Daniel McFadden made the connection to random utility maximization.&lt;br /&gt;
&lt;br /&gt;
波兹曼分布与多项式 logit 模型具有相同的形式。作为一个离散选择模型，这在经济学中非常著名，因为丹尼尔 · 麦克法登提出了随机效用最大化的联系。&lt;br /&gt;
&lt;br /&gt;
; [[Canonical ensemble]] (general case)&lt;br /&gt;
&lt;br /&gt;
: The [[canonical ensemble]] gives the [[probabilities]] of the various possible states of a closed system of fixed volume, in thermal equilibrium with a [[heat bath]]. The canonical ensemble is a probability distribution with the Boltzmann form.&lt;br /&gt;
&lt;br /&gt;
; Statistical frequencies of subsystems' states (in a non-interacting collection)&lt;br /&gt;
&lt;br /&gt;
: When the system of interest is a collection of many non-interacting copies of a smaller subsystem, it is sometimes useful to find the [[statistical frequency]] of a given subsystem state, among the collection. The canonical ensemble has the property of separability when applied to such a collection: as long as the non-interacting subsystems have fixed composition, then each subsystem's state is independent of the others and is also characterized by a canonical ensemble. As a result, the [[expectation value|expected]] statistical frequency distribution of subsystem states has the Boltzmann form.&lt;br /&gt;
&lt;br /&gt;
; [[Maxwell–Boltzmann statistics]] of classical gases (systems of non-interacting particles)&lt;br /&gt;
&lt;br /&gt;
: In particle systems, many particles share the same space and regularly change places with each other; the single-particle state space they occupy is a shared space. [[Maxwell–Boltzmann statistics]] give the expected number of particles found in a given single-particle state, in a [[classical mechanics|classical]] gas of non-interacting particles at equilibrium. This expected number distribution has the Boltzmann form.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Although these cases have strong similarities, it is helpful to distinguish them as they generalize in different ways when the crucial assumptions are changed:&lt;br /&gt;
&lt;br /&gt;
* When a system is in thermodynamic equilibrium with respect to both energy exchange ''and particle exchange'', the requirement of fixed composition is relaxed and a [[grand canonical ensemble]] is obtained rather than canonical ensemble. On the other hand, if both composition and energy are fixed, then a [[microcanonical ensemble]] applies instead.&lt;br /&gt;
&lt;br /&gt;
* If the subsystems within a collection ''do'' interact with each other, then the expected frequencies of subsystem states no longer follow a Boltzmann distribution, and even may not have an [[analytical solution]].&amp;lt;ref&amp;gt;A classic example of this is [[magnetic ordering]]. Systems of non-interacting [[spin (physics)|spins]] show [[paramagnetic]] behaviour that can be understood with a single-particle canonical ensemble (resulting in the [[Brillouin function]]). Systems of ''interacting'' spins can show much more complex behaviour such as [[ferromagnetism]] or [[antiferromagnetism]].&amp;lt;/ref&amp;gt; The canonical ensemble can however still be applied to the ''collective'' states of the entire system considered as a whole, provided the entire system is isolated and in thermal equilibrium.&lt;br /&gt;
&lt;br /&gt;
* With ''[[quantum mechanics|quantum]]'' gases of non-interacting particles in equilibrium, the number of particles found in a given single-particle state does not follow Maxwell–Boltzmann statistics, and there is no simple closed form expression for quantum gases in the canonical ensemble. In the grand canonical ensemble the state-filling statistics of quantum gases are described by [[Fermi–Dirac statistics]] or [[Bose–Einstein statistics]], depending on whether the particles are [[fermion]]s or [[boson]]s respectively.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
|year=1868&lt;br /&gt;
&lt;br /&gt;
1868年&lt;br /&gt;
&lt;br /&gt;
== In mathematics ==&lt;br /&gt;
&lt;br /&gt;
|title=Studien über das Gleichgewicht der lebendigen Kraft zwischen bewegten materiellen Punkten&lt;br /&gt;
&lt;br /&gt;
|title=Studien über das Gleichgewicht der lebendigen Kraft zwischen bewegten materiellen Punkten&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
|trans-title=Studies on the balance of living force between moving material points&lt;br /&gt;
&lt;br /&gt;
| 反题 = 移动物质点之间生命力平衡的研究&lt;br /&gt;
&lt;br /&gt;
{{main|Gibbs measure|Log-linear model|Boltzmann machine}}&lt;br /&gt;
&lt;br /&gt;
|journal=Wiener Berichte |volume=58 |pages=517–560&lt;br /&gt;
&lt;br /&gt;
| journal = Wiener Berichte | volume = 58 | pages = 517-560&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
}}&lt;br /&gt;
&lt;br /&gt;
}}&lt;br /&gt;
&lt;br /&gt;
In more general mathematical settings, the Boltzmann distribution is also known as the [[Gibbs measure]]. In statistics and machine learning, it is called a [[log-linear model]]. In [[deep learning]], the Boltzmann distribution is used in the sampling distribution of [[stochastic neural network]]s such as the [[Boltzmann machine]], [[Restricted Boltzmann machine]], [[Energy based model|Energy-Based models]] and [[Deep Boltzmann Machine|deep Boltzmann machine]].&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
|first=Josiah Willard |last=Gibbs |authorlink=Josiah Willard Gibbs&lt;br /&gt;
&lt;br /&gt;
2012年10月15日 | 约西亚·威拉德·吉布斯&lt;br /&gt;
&lt;br /&gt;
== In economics ==&lt;br /&gt;
&lt;br /&gt;
|year=1902&lt;br /&gt;
&lt;br /&gt;
1902年&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
|title=Elementary Principles in Statistical Mechanics&lt;br /&gt;
&lt;br /&gt;
统计力学的基本原理&lt;br /&gt;
&lt;br /&gt;
The Boltzmann distribution can be introduced to allocate permits in emissions trading.&amp;lt;ref name=&amp;quot;Park, J.-W. 2012&amp;quot;&amp;gt;Park, J.-W., Kim, C. U. and Isard, W. (2012) Permit allocation in emissions trading using the Boltzmann distribution. Physica A 391: 4883–4890&amp;lt;/ref&amp;gt;&amp;lt;ref&amp;gt;[http://www.technologyreview.com/view/425051/the-thorny-problem-of-fair-allocation/ The Thorny Problem Of Fair Allocation]. ''Technology Review'' blog. August 17, 2011. Cites and summarizes Park, Kim and Isard (2012).&amp;lt;/ref&amp;gt; The new allocation method using the Boltzmann distribution can describe the most probable, natural, and unbiased distribution of emissions permits among multiple countries. Simple and versatile, this new method holds potential for many economic and environmental applications.&lt;br /&gt;
&lt;br /&gt;
|title-link=Elementary Principles in Statistical Mechanics }}&lt;br /&gt;
&lt;br /&gt;
| title-link = 基本原理统计力学}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The Boltzmann distribution has the same form as the [[Multinomial logistic regression|multinomial logit]] model. As a [[discrete choice]] model, this is very well known in economics since [[Daniel McFadden]] made the connection to random utility maximization.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Category:Statistical mechanics&lt;br /&gt;
&lt;br /&gt;
类别: 统计力学&lt;br /&gt;
&lt;br /&gt;
==See also==&lt;br /&gt;
&lt;br /&gt;
Distribution&lt;br /&gt;
&lt;br /&gt;
分布&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:Boltzmann distribution]]. Its edit history can be viewed at [[玻尔兹曼分布/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>Tueryeye</name></author>
	</entry>
	<entry>
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		<title>玻尔兹曼分布</title>
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		<updated>2021-10-13T14:22:19Z</updated>

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&lt;div&gt;此词条暂由彩云小译翻译，翻译字数共1452，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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{{Use American English|date = March 2019}}&lt;br /&gt;
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{{Short description|Probability distribution of energy states of a system}}&lt;br /&gt;
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{{about|system energy states|particle energy levels and velocities|Maxwell–Boltzmann distribution}}&lt;br /&gt;
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[[File:Boltzmann distribution graph.svg|upright=1.75|right|thumb|Boltzmann factor ''p&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;''&amp;amp;nbsp;/&amp;amp;nbsp;''p&amp;lt;sub&amp;gt;j&amp;lt;/sub&amp;gt;'' (vertical axis) as a function of temperature ''T'' for several energy differences ''ε&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;''&amp;amp;nbsp;−&amp;amp;nbsp;''ε&amp;lt;sub&amp;gt;j&amp;lt;/sub&amp;gt;''.|链接=Special:FilePath/Boltzmann_distribution_graph.svg]]&lt;br /&gt;
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In [[statistical mechanics]] and [[mathematics]], a '''Boltzmann distribution''' (also called '''Gibbs distribution'''&amp;lt;ref name=&amp;quot;landau&amp;quot;&amp;gt;{{cite book | author=Landau, Lev Davidovich |author2=Lifshitz, Evgeny Mikhailovich |name-list-style=amp | title=Statistical Physics |volume=5 |series=Course of Theoretical Physics |edition=3 |origyear=1976 |year=1980 |place=Oxford |publisher=Pergamon Press|isbn=0-7506-3372-7|author-link=Lev Landau |author2-link=Evgeny Lifshitz }} Translated by J.B. Sykes and M.J. Kearsley. See section 28&amp;lt;/ref&amp;gt;) is a [[probability distribution]] or [[probability measure]] that gives the probability that a system will be in a certain [[microstate (statistical mechanics)|state]] as a function of that state's energy and the temperature of the system. The distribution is expressed in the form:&lt;br /&gt;
&lt;br /&gt;
In statistical mechanics and mathematics, a Boltzmann distribution (also called Gibbs distribution) is a probability distribution or probability measure that gives the probability that a system will be in a certain state as a function of that state's energy and the temperature of the system. The distribution is expressed in the form:&lt;br /&gt;
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在统计力学和数学中，波兹曼分布分布(也称为吉布斯分布&amp;lt;ref name=&amp;quot;landau&amp;quot; /&amp;gt;)是一个概率分布或机率量测，它给出了一个系统处于某种状态的概率，这个概率是该状态的能量和系统温度的函数。分布情况以下列形式表示:&lt;br /&gt;
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:&amp;lt;math&amp;gt;p_i \propto e^{-\frac{\varepsilon_i}{kT}}&amp;lt;/math&amp;gt; &lt;br /&gt;
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&amp;lt;math&amp;gt;p_i \propto e^{-\frac{\varepsilon_i}{kT}}&amp;lt;/math&amp;gt; &lt;br /&gt;
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[拉丁语]&lt;br /&gt;
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where {{mvar|p&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;}} is the probability of the system being in state {{mvar|i}}, {{mvar|ε&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;}} is the energy of that state, and a constant {{mvar|kT}} of the distribution is the product of [[Boltzmann's constant]] {{mvar|k}} and [[thermodynamic temperature]] {{mvar|T}}. The symbol &amp;lt;math display=&amp;quot;inline&amp;quot;&amp;gt;\propto&amp;lt;/math&amp;gt; denotes [[proportionality (mathematics)|proportionality]] (see {{section link||The distribution}} for the proportionality constant).&lt;br /&gt;
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where  is the probability of the system being in state ,  is the energy of that state, and a constant  of the distribution is the product of Boltzmann's constant  and thermodynamic temperature . The symbol &amp;lt;math display=&amp;quot;inline&amp;quot;&amp;gt;\propto&amp;lt;/math&amp;gt; denotes proportionality (see  for the proportionality constant).&lt;br /&gt;
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{{mvar|p&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;}} 是其中系统处于状态{{mvar|i}}的概率, {{mvar|ε&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;}} 是该状态的能量，还有关于这个分布的一个常数 {{mvar|kT}} ，它是玻耳兹曼常数{{mvar|k}}和热力学温度 {{mvar|T}} 的乘积。符号 &amp;lt;math display=&amp;quot;inline&amp;quot;&amp;gt;\propto&amp;lt;/math&amp;gt;表示相称性(见附录中的比例常数)。&lt;br /&gt;
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The term system here has a very wide meaning; it can range from a single atom to a macroscopic system such as a [[Natural gas storage|natural gas storage tank]]. Because of this the Boltzmann distribution can be used to solve a very wide variety of problems. The distribution shows that states with lower energy will always have a higher probability of being occupied .&lt;br /&gt;
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The term system here has a very wide meaning; it can range from a single atom to a macroscopic system such as a natural gas storage tank. Because of this the Boltzmann distribution can be used to solve a very wide variety of problems. The distribution shows that states with lower energy will always have a higher probability of being occupied .&lt;br /&gt;
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这里的术语系统含义广泛; 它可以从单个原子到宏观系统，如天然气储罐。正因为如此，波兹曼分布可以用来解决各种各样的问题。玻尔兹曼分布表明，能量较低的状态被占据的概率总是较高的。&lt;br /&gt;
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The ''ratio'' of probabilities of two states is known as the '''Boltzmann factor''' and characteristically only depends on the states' energy difference:&lt;br /&gt;
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The ratio of probabilities of two states is known as the Boltzmann factor and characteristically only depends on the states' energy difference:&lt;br /&gt;
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两种状态的概率之比被称为玻尔兹曼因子，取决于两种状态的能量差:&lt;br /&gt;
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:&amp;lt;math&amp;gt;\frac{p_i}{p_j} = e^{\frac{\varepsilon_j - \varepsilon_i}{kT}}&amp;lt;/math&amp;gt;&lt;br /&gt;
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&amp;lt;math&amp;gt;\frac{p_i}{p_j} = e^{\frac{\varepsilon_j - \varepsilon_i}{kT}}&amp;lt;/math&amp;gt;&lt;br /&gt;
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[数学][数学]&lt;br /&gt;
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The Boltzmann distribution is named after [[Ludwig Boltzmann]] who first formulated it in 1868 during his studies of the [[statistical mechanics]] of gases in thermal equilibrium. Boltzmann's statistical work is borne out in his paper “On the Relationship between the Second Fundamental Theorem of the Mechanical Theory of Heat and Probability Calculations Regarding the Conditions for Thermal Equilibrium&amp;quot;&amp;lt;ref&amp;gt;http://crystal.med.upenn.edu/sharp-lab-pdfs/2015SharpMatschinsky_Boltz1877_Entropy17.pdf&amp;lt;/ref&amp;gt;&lt;br /&gt;
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The Boltzmann distribution is named after Ludwig Boltzmann who first formulated it in 1868 during his studies of the statistical mechanics of gases in thermal equilibrium. Boltzmann's statistical work is borne out in his paper “On the Relationship between the Second Fundamental Theorem of the Mechanical Theory of Heat and Probability Calculations Regarding the Conditions for Thermal Equilibrium&amp;quot;&lt;br /&gt;
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波兹曼分布是根据路德维希·玻尔兹曼1868年在研究统计力学中气体热平衡的时候首次提出的一个公式命名的。波尔兹曼的统计工作在他的论文《论热力学第二基本定理与热平衡条件的概率计算之间的关系》中得到了体现。&lt;br /&gt;
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  It would be nice to have a citation here! The origin of the Boltzmann factor isn't entirely clear. According to some authors, Boltzmann's 1968 paper “On the Relationship between the Second Fundamental Theorem of the Mechanical Theory of Heat and Probability Calculations Regarding the Conditions for Thermal Equilibrium”&lt;br /&gt;
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  It would be nice to have a citation here! The origin of the Boltzmann factor isn't entirely clear. According to some authors, Boltzmann's 1968 paper “On the Relationship between the Second Fundamental Theorem of the Mechanical Theory of Heat and Probability Calculations Regarding the Conditions for Thermal Equilibrium”&lt;br /&gt;
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如果能在这里引用一下就好了！玻尔兹曼因子的起源并不完全清楚。根据一些作者的说法，Boltzmann 在1968年发表的论文《论热力学第二基本定理与热平衡条件的概率计算之间的关系》&lt;br /&gt;
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  &amp;quot;Studien über das Gleichgewicht der lebendigen Kraft zwischen bewegten materiellen Punkten&amp;quot; is the origin but I can't find this article at the moment,&lt;br /&gt;
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  &amp;quot;Studien über das Gleichgewicht der lebendigen Kraft zwischen bewegten materiellen Punkten&amp;quot; is the origin but I can't find this article at the moment,&lt;br /&gt;
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  &amp;quot;Studien über das Gleichgewicht der lebendigen Kraft zwischen bewegten materiellen Punkten&amp;quot; is the origin but I can't find this article at the moment,&lt;br /&gt;
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  so I cannot confirm.&lt;br /&gt;
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  so I cannot confirm.&lt;br /&gt;
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所以我不能确定。&lt;br /&gt;
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  For example, this book says so, but uses suspiciously modern terminology&lt;br /&gt;
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  For example, this book says so, but uses suspiciously modern terminology&lt;br /&gt;
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例如，这本书是这么说的，但是使用了可疑的现代术语&lt;br /&gt;
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    http://books.google.es/books?id=u13KiGlz2zcC&amp;amp;lpg=PA92&amp;amp;ots=8H1DRURdxn&amp;amp;pg=PA93#v=onepage&amp;amp;f=false&lt;br /&gt;
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    http://books.google.es/books?id=u13KiGlz2zcC&amp;amp;lpg=PA92&amp;amp;ots=8H1DRURdxn&amp;amp;pg=PA93#v=onepage&amp;amp;f=false&lt;br /&gt;
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Http://books.google.es/books?id=u13kiglz2zcc&amp;amp;lpg=pa92&amp;amp;ots=8h1drurdxn&amp;amp;pg=pa93#v=onepage&amp;amp;f=false&lt;br /&gt;
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  On the other hand, Uffink's &amp;quot;Compendium of the foundations of classical statistical physics&amp;quot; does not seem to indicate quite this equation but rather that Boltzmann's 1968 distribution was the simple Maxwell–Boltzmann distribution (for a classical nonrelativistic gas), modified for particles in a potential.&lt;br /&gt;
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  On the other hand, Uffink's &amp;quot;Compendium of the foundations of classical statistical physics&amp;quot; does not seem to indicate quite this equation but rather that Boltzmann's 1968 distribution was the simple Maxwell–Boltzmann distribution (for a classical nonrelativistic gas), modified for particles in a potential.&lt;br /&gt;
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另一方面，Uffink 的“经典统计物理学基础纲要”似乎并没有完全表明这个方程，而是说 Boltzmann 在1968年的分布是简单的 Maxwell-波兹曼分布(用于经典的非气体) ，修改为势中的粒子。&lt;br /&gt;
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--&amp;gt; &lt;br /&gt;
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--&amp;gt; &lt;br /&gt;
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--&amp;gt;&lt;br /&gt;
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The distribution was later investigated extensively, in its modern generic form, by [[Josiah Willard Gibbs]] in 1902.&amp;lt;ref name=&amp;quot;gibbs&amp;quot;&amp;gt;{{cite book |last=Gibbs |first=Josiah Willard |authorlink=Josiah Willard Gibbs |title=Elementary Principles in Statistical Mechanics |year=1902 |publisher=[[Charles Scribner's Sons]] &lt;br /&gt;
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The distribution was later investigated extensively, in its modern generic form, by Josiah Willard Gibbs in 1902.&lt;br /&gt;
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这种分布后来在1902年由约西亚·威拉德·吉布斯进行了广泛的调查，以其现代通用形式。&lt;br /&gt;
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|location=New York|title-link=Elementary Principles in Statistical Mechanics }}&amp;lt;/ref&amp;gt;{{rp|Ch.IV}}、&lt;br /&gt;
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在玻尔兹曼分布被发明之后，约西亚·华纳德·吉布森充分地研究了它并在1902年提出了它的一般形式。&amp;lt;ref name=&amp;quot;gibbs&amp;quot; /&amp;gt;&lt;br /&gt;
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The generalized Boltzmann distribution is a sufficient and necessary condition for the equivalence between the statistical mechanics definition of entropy (The  Gibbs entropy formula &amp;lt;math&amp;gt;S = -k_{\mathrm{B}}\sum_i p_i \log p_i&amp;lt;/math&amp;gt;) and the thermodynamic definition of entropy (&amp;lt;math&amp;gt;d S = \frac{\delta Q_\text{rev}}{T}&amp;lt;/math&amp;gt;, and the fundamental thermodynamic relation).&lt;br /&gt;
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The generalized Boltzmann distribution is a sufficient and necessary condition for the equivalence between the statistical mechanics definition of [[entropy]] (The [[Entropy_(statistical_thermodynamics)#Gibbs_entropy_formula | Gibbs entropy formula]] &amp;lt;math&amp;gt;S = -k_{\mathrm{B}}\sum_i p_i \log p_i&amp;lt;/math&amp;gt;) and the thermodynamic definition of entropy (&amp;lt;math&amp;gt;d S = \frac{\delta Q_\text{rev}}{T}&amp;lt;/math&amp;gt;, and the [[fundamental thermodynamic relation]]).&amp;lt;ref name=&amp;quot;:0&amp;quot;&amp;gt;{{cite journal |last1= Gao |first1= Xiang |last2= Gallicchio |first2= Emilio |first3= Adrian |last3= Roitberg  |date= 2019 |title= The generalized Boltzmann distribution is the only distribution in which the Gibbs-Shannon entropy equals the thermodynamic entropy |journal= The Journal of Chemical Physics|volume= 151|issue= 3|pages= 034113|doi= 10.1063/1.5111333|pmid= 31325924 |arxiv= 1903.02121 |s2cid= 118981017 }}&amp;lt;/ref&amp;gt;&lt;br /&gt;
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广义波兹曼分布是熵的统计力学定义(吉布斯熵公式  &amp;lt;math&amp;gt;S = -k_{\mathrm{B}}\sum_i p_i \log p_i&amp;lt;/math&amp;gt;))与熵的热力学定义(&amp;lt;math&amp;gt;d S = \frac{\delta Q_\text{rev}}{T}&amp;lt;/math&amp;gt;)等价的充要条件。&amp;lt;ref name=&amp;quot;:0&amp;quot; /&amp;gt;&lt;br /&gt;
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The Boltzmann distribution should not be confused with the Maxwell–Boltzmann distribution. The former gives the probability that a system will be in a certain state as a function of that state's energy; in contrast, the latter is used to describe particle speeds in idealized gases.&lt;br /&gt;
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值得一提的是，玻尔兹曼分布不应与麦克斯韦-玻尔兹曼分布混淆。前者给出了系统处于某种状态的概率，作为该状态能量的函数; 后者则是用于描述理想气体中的粒子速度。&lt;br /&gt;
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The Boltzmann distribution should not be confused with the [[Maxwell–Boltzmann distribution]]. The former gives the probability that a system will be in a certain state as a function of that state's energy;&amp;lt;ref name=&amp;quot;Atkins, P. W. 2010&amp;quot;&amp;gt;Atkins, P. W. (2010) Quanta, W. H. Freeman and Company, New York&amp;lt;/ref&amp;gt; in contrast, the latter is used to describe particle speeds in idealized gases.&lt;br /&gt;
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==The distribution==&lt;br /&gt;
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The Boltzmann distribution is a probability distribution that gives the probability of a certain state as a function of that state's energy and  temperature of the system to which the distribution is applied. It is given as&lt;br /&gt;
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波兹曼分布是一个概率分布，它给出了出于某种能量态处于某种能量和温度的时候的概率。它被给出为&lt;br /&gt;
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The Boltzmann distribution is a [[probability distribution]] that gives the probability of a certain state as a function of that state's energy and  temperature of the [[system]] to which the distribution is applied.&amp;lt;ref name=&amp;quot;McQuarrie, A. 2000&amp;quot;&amp;gt;McQuarrie, A. (2000) Statistical Mechanics, University Science Books, California&amp;lt;/ref&amp;gt; It is given as&lt;br /&gt;
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p_i=\frac{1}{Q}} {e^{- {\varepsilon}_i / k T}=\frac{e^{- {\varepsilon}_i / k T}}{\sum_{j=1}^{M}{e^{- {\varepsilon}_j / k T}}}&lt;br /&gt;
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P _ i = frac {1}{ q }{ e ^ {-{ varepsilon } _ i/k t } = frac { e ^ {-{ varepsilon } _ i/k t }{ sum { j = 1} ^ { m }{ e ^ {-{ varepsilon } _ j/k t }}}}}&lt;br /&gt;
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p_i=\frac{1}{Q}} {e^{- {\varepsilon}_i / k T}=\frac{e^{- {\varepsilon}_i / k T}}{\sum_{j=1}^{M}{e^{- {\varepsilon}_j / k T}}}&lt;br /&gt;
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where p&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt; is the probability of state i, ε&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt; the energy of state i, k the Boltzmann constant, T the temperature of the system and M is the number of all states accessible to the system of interest.&lt;br /&gt;
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其中 p &amp;lt; sub &amp;gt; i  是状态 i 的概率，ε &amp;lt; sub &amp;gt; i  是状态 i 的能量，k 是波兹曼常数，t 是系统的温度，m 是感兴趣的系统所能到达的所有状态的数目。&lt;br /&gt;
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where ''p&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;'' is the probability of state ''i'', ''ε&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;'' the energy of state ''i'', ''k'' the Boltzmann constant, ''T'' the temperature of the system and ''M'' is the number of all states accessible to the system of interest.&amp;lt;ref name=&amp;quot;McQuarrie, A. 2000&amp;quot;/&amp;gt;&amp;lt;ref name=&amp;quot;Atkins, P. W. 2010&amp;quot;/&amp;gt; Implied parentheses around the denominator ''kT'' are omitted for brevity. The normalization denominator ''Q'' (denoted by some authors by ''Z'') is the [[canonical partition function]]&lt;br /&gt;
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The distribution shows that states with lower energy will always have a higher probability of being occupied than the states with higher energy. It can also give us the quantitative relationship between the probabilities of the two states being occupied. The ratio of probabilities for states i and j is given as&lt;br /&gt;
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分布表明，能量较低的状态被占据的概率总是高于能量较高的状态。它还可以给出两个状态被占领概率之间的定量关系。给出了状态 i 和状态 j 的概率比为&lt;br /&gt;
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Q={\sum_{i=1}^{M}{e^{- {\varepsilon}_i / k T}}}&lt;br /&gt;
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{\frac{p_i}{p_j}}=e^{({\varepsilon}_j-{\varepsilon}_i) / k T}&lt;br /&gt;
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{ frac { p _ i }{ p _ j } = e ^ {({ varepsilon } _ j-{ varepsilon } _ i)/k t }&lt;br /&gt;
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It results from the constraint that the probabilities of all accessible states must add up to 1.&lt;br /&gt;
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where p&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt; is the probability of state i,  p&amp;lt;sub&amp;gt;j&amp;lt;/sub&amp;gt; the probability of state j, and ε&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt; and ε&amp;lt;sub&amp;gt;j&amp;lt;/sub&amp;gt; are the energies of states i and j, respectively.&lt;br /&gt;
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其中 p &amp;lt; sub &amp;gt; i  是状态 i 的概率，p &amp;lt; sub &amp;gt; j  状态 j 的概率，ε  i  和 ε  j  分别是状态 i 和 j 的能量。&lt;br /&gt;
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The Boltzmann distribution is the distribution that maximizes the [[entropy]]&lt;br /&gt;
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The Boltzmann distribution is often used to describe the distribution of particles, such as atoms or molecules, over energy states accessible to them. If we have a system consisting of many particles, the probability of a particle being in state i is practically the probability that, if we pick a random particle from that system and check what state it is in, we will find it is in state i. This probability is equal to the number of particles in state i divided by the total number of particles in the system, that is the fraction of particles that occupy state i.&lt;br /&gt;
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波兹曼分布通常被用来描述粒子，比如原子或分子，在能量状态上的分布情况。如果我们有一个由许多粒子组成的系统，粒子处于状态 i 的概率实际上等于，如果我们从该系统中选择一个随机粒子并检查它处于什么状态，我们会发现它处于状态 i 的概率。这个概率等于状态 i 的粒子数除以系统中粒子的总数，即占据状态 i 的粒子的比例。&lt;br /&gt;
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:&amp;lt;math&amp;gt;H(p_1,p_2,\cdots,p_M) = -\sum_{i=1}^{M} p_i\log_2 p_i&amp;lt;/math&amp;gt;&lt;br /&gt;
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subject to the constraint that &amp;lt;math display=&amp;quot;inline&amp;quot;&amp;gt;&lt;br /&gt;
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p_i={\frac{N_i}{N}}&lt;br /&gt;
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P _ i = { frac { n _ i }{ n }&lt;br /&gt;
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{\sum{p_i {\varepsilon}_i}}&lt;br /&gt;
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&amp;lt;/math&amp;gt; equals a particular mean energy value (which can be proven using [[Lagrange multipliers]]).&lt;br /&gt;
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where N&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt; is the number of particles in state i and N is the total number of particles in the system. We may use the Boltzmann distribution to find this probability that is, as we have seen, equal to the fraction of particles that are in state i. So the equation that gives the fraction of particles in state i as a function of the energy of that state is   In order for this to be possible, there must be some particles in the first state to undergo the transition. We may find that this condition is fulfilled by finding the fraction of particles in the first state. If it is negligible, the transition is very likely not to be observed at the temperature for which the calculation was done. In general, a larger fraction of molecules in the first state means a higher number of transitions to the second state. This gives a stronger spectral line. However, there are other factors that influence the intensity of a spectral line, such as whether it is caused by an allowed or a forbidden transition.&lt;br /&gt;
&lt;br /&gt;
其中 n &amp;lt; sub &amp;gt; i  是状态 i 的粒子数，n 是系统中粒子的总数。我们可以用波兹曼分布来求出这个概率，就像我们看到的那样，等于处于 i 状态的粒子的比例。所以给出状态 i 的粒子比例，作为状态能量的函数的方程是，为了使这成为可能，必须有一些粒子处于第一个状态，才能发生跃迁。我们可以通过求第一态粒子的比例来满足这个条件。如果它可以忽略不计，那么在进行计算的温度下，极有可能不能观察到这种转变。一般来说，处于第一状态的分子比例越大，意味着向第二状态转变的次数越多。这就产生了一条更强的谱线。然而，还有其他因素影响谱线的强度，例如它是由允许的跃迁还是禁止的跃迁引起的。&lt;br /&gt;
&lt;br /&gt;
The partition function can be calculated if we know the energies of the states accessible to the system of interest. For atoms the partition function values can be found in the NIST Atomic Spectra Database.&amp;lt;ref&amp;gt;[http://physics.nist.gov/PhysRefData/ASD/levels_form.html NIST Atomic Spectra Database Levels Form] at nist.gov&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The Boltzmann distribution is related to the softmax function commonly used in machine learning.&lt;br /&gt;
&lt;br /&gt;
波兹曼分布学习与机器学习中常用的柔性最大激活函数学习有关。&lt;br /&gt;
&lt;br /&gt;
The distribution shows that states with lower energy will always have a higher probability of being occupied than the states with higher energy. It can also give us the quantitative relationship between the probabilities of the two states being occupied. The ratio of probabilities for states ''i'' and ''j'' is given as&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
{\frac{p_i}{p_j}}=e^{({\varepsilon}_j-{\varepsilon}_i) / k T}&lt;br /&gt;
&lt;br /&gt;
&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
The Boltzmann distribution appears in statistical mechanics when considering isolated (or nearly-isolated) systems of fixed composition that are in thermal equilibrium (equilibrium with respect to energy exchange). The most general case is the probability distribution for the canonical ensemble, but also some special cases (derivable from the canonical ensemble) also show the Boltzmann distribution in different aspects:&lt;br /&gt;
&lt;br /&gt;
当考虑孤立的(或者几乎孤立的)固定组成的体系处于平衡状态时，波兹曼分布出现在《统计力学热平衡。最普遍的情况是概率分布的正则系综，但也有一些特殊的情况(从正则系综衍生)也显示了波兹曼分布在不同的方面:&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
where ''p&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;'' is the probability of state ''i'',  ''p&amp;lt;sub&amp;gt;j&amp;lt;/sub&amp;gt;'' the probability of state ''j'', and ''ε&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;'' and ''ε&amp;lt;sub&amp;gt;j&amp;lt;/sub&amp;gt;'' are the energies of states ''i'' and ''j'', respectively.&lt;br /&gt;
&lt;br /&gt;
 Canonical ensemble (general case)&lt;br /&gt;
&lt;br /&gt;
正则系综(一般情况)&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
 The canonical ensemble gives the probabilities of the various possible states of a closed system of fixed volume, in thermal equilibrium with a heat bath. The canonical ensemble is a probability distribution with the Boltzmann form.&lt;br /&gt;
&lt;br /&gt;
正则系综模型给出了一个封闭的固定体积系统的各种可能状态的概率，这个封闭体积系统包括一个带有热浴的热平衡。正则系综是一个玻尔兹曼概率分布。&lt;br /&gt;
&lt;br /&gt;
The Boltzmann distribution is often used to describe the distribution of particles, such as atoms or molecules, over energy states accessible to them. If we have a system consisting of many particles, the probability of a particle being in state ''i'' is practically the probability that, if we pick a random particle from that system and check what state it is in, we will find it is in state ''i''. This probability is equal to the number of particles in state ''i'' divided by the total number of particles in the system, that is the fraction of particles that occupy state ''i''.&lt;br /&gt;
&lt;br /&gt;
 Statistical frequencies of subsystems' states (in a non-interacting collection)&lt;br /&gt;
&lt;br /&gt;
子系统状态的统计频率(在一个无交互的集合中)&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
 When the system of interest is a collection of many non-interacting copies of a smaller subsystem, it is sometimes useful to find the statistical frequency of a given subsystem state, among the collection. The canonical ensemble has the property of separability when applied to such a collection: as long as the non-interacting subsystems have fixed composition, then each subsystem's state is independent of the others and is also characterized by a canonical ensemble. As a result, the expected statistical frequency distribution of subsystem states has the Boltzmann form.&lt;br /&gt;
&lt;br /&gt;
当感兴趣的系统是一个较小子系统的许多非交互副本的集合时，在集合中查找给定子系统状态的统计频率有时是有用的。当应用于这样一个集合时，正则系综子系统具有可分离性: 只要不相互作用的子系统的组成是固定的，那么每个子系统的状态是独立于其他子系统的，也是一个拥有属性正则系综。因此，子系统状态的期望统计频率分布具有玻耳兹曼形式。&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 Maxwell–Boltzmann statistics of classical gases (systems of non-interacting particles)&lt;br /&gt;
&lt;br /&gt;
经典气体(非相互作用粒子系统)的 Maxwell-Boltzmann 统计&lt;br /&gt;
&lt;br /&gt;
p_i={\frac{N_i}{N}}&lt;br /&gt;
&lt;br /&gt;
 In particle systems, many particles share the same space and regularly change places with each other; the single-particle state space they occupy is a shared space. Maxwell–Boltzmann statistics give the expected number of particles found in a given single-particle state, in a classical gas of non-interacting particles at equilibrium. This expected number distribution has the Boltzmann form.&lt;br /&gt;
&lt;br /&gt;
在粒子系统中，许多粒子共享同一空间，并且相互之间有规律地改变位置; 它们所占据的单粒子状态空间是一个共享空间。麦克斯韦-玻尔兹曼统计给出了在一个给定的单粒子态，在一个处于平衡状态的非相互作用粒子的经典气体中所发现的粒子的预期数量。这个预期的数分布具有玻耳兹曼形式。&lt;br /&gt;
&lt;br /&gt;
&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Although these cases have strong similarities, it is helpful to distinguish them as they generalize in different ways when the crucial assumptions are changed:&lt;br /&gt;
&lt;br /&gt;
虽然这些案例有很多相似之处，但是当关键假设发生变化时，它们以不同的方式进行归纳，因此区分它们是有帮助的:&lt;br /&gt;
&lt;br /&gt;
where ''N&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;'' is the number of particles in state ''i'' and ''N'' is the total number of particles in the system. We may use the Boltzmann distribution to find this probability that is, as we have seen, equal to the fraction of particles that are in state i. So the equation that gives the fraction of particles in state ''i'' as a function of the energy of that state is  &amp;lt;ref name=&amp;quot;Atkins, P. W. 2010&amp;quot;/&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
{\frac{N_i}{N}}={\frac{e^{- {\varepsilon}_i / k T}}{\sum_{j=1}^{M}{e^{- {\varepsilon}_j / k T}}}}&lt;br /&gt;
&lt;br /&gt;
&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
This equation is of great importance to [[spectroscopy]]. In spectroscopy we observe a [[spectral line]] of atoms or molecules that we are interested in going from one state to another.&amp;lt;ref name=&amp;quot;Atkins, P. W. 2010&amp;quot;/&amp;gt;&amp;lt;ref&amp;gt;Atkins, P. W.; de Paula J. (2009) Physical Chemistry, 9th edition, Oxford University Press, Oxford, UK&amp;lt;/ref&amp;gt; In order for this to be possible, there must be some particles in the first state to undergo the transition. We may find that this condition is fulfilled by finding the fraction of particles in the first state. If it is negligible, the transition is very likely not to be observed at the temperature for which the calculation was done. In general, a larger fraction of molecules in the first state means a higher number of transitions to the second state.&amp;lt;ref&amp;gt;Skoog, D. A.; Holler, F. J.; Crouch, S. R. (2006) Principles of Instrumental Analysis, Brooks/Cole, Boston, MA&amp;lt;/ref&amp;gt; This gives a stronger spectral line. However, there are other factors that influence the intensity of a spectral line, such as whether it is caused by an allowed or a [[forbidden transition]].&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The Boltzmann distribution is related to the [[softmax function]] commonly used in machine learning.&lt;br /&gt;
&lt;br /&gt;
In more general mathematical settings, the Boltzmann distribution is also known as the Gibbs measure. In statistics and machine learning, it is called a log-linear model. In deep learning, the Boltzmann distribution is used in the sampling distribution of stochastic neural networks such as the Boltzmann machine, Restricted Boltzmann machine, Energy-Based models and deep Boltzmann machine.&lt;br /&gt;
&lt;br /&gt;
在更一般的数学环境中，波兹曼分布也被称为吉布斯量度。在统计学和机器学习中，它被称为对数线性回归。在深度学习中，波兹曼分布被用于随机神经网络的抽样分布，如波茨曼机、受限玻尔兹曼机、基于能量的模型和深度波茨曼机。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
== In statistical mechanics ==&lt;br /&gt;
&lt;br /&gt;
{{main|Canonical ensemble|Maxwell–Boltzmann statistics}}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The Boltzmann distribution can be introduced to allocate permits in emissions trading. The new allocation method using the Boltzmann distribution can describe the most probable, natural, and unbiased distribution of emissions permits among multiple countries. Simple and versatile, this new method holds potential for many economic and environmental applications.&lt;br /&gt;
&lt;br /&gt;
可以引入欧盟波兹曼分布来分配排放交易的许可。这种新的排放量分配方法使用波兹曼分布能够描述多个国家之间最可能、最自然和最无偏见的排放量分配。这种新方法简单而通用，具有许多经济和环境应用的潜力。&lt;br /&gt;
&lt;br /&gt;
The Boltzmann distribution appears in [[statistical mechanics]] when considering isolated (or nearly-isolated) systems of fixed composition that are in [[thermal equilibrium]] (equilibrium with respect to energy exchange). The most general case is the probability distribution for the canonical ensemble, but also some special cases (derivable from the canonical ensemble) also show the Boltzmann distribution in different aspects:&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The Boltzmann distribution has the same form as the multinomial logit model. As a discrete choice model, this is very well known in economics since Daniel McFadden made the connection to random utility maximization.&lt;br /&gt;
&lt;br /&gt;
波兹曼分布与多项式 logit 模型具有相同的形式。作为一个离散选择模型，这在经济学中非常著名，因为丹尼尔 · 麦克法登提出了随机效用最大化的联系。&lt;br /&gt;
&lt;br /&gt;
; [[Canonical ensemble]] (general case)&lt;br /&gt;
&lt;br /&gt;
: The [[canonical ensemble]] gives the [[probabilities]] of the various possible states of a closed system of fixed volume, in thermal equilibrium with a [[heat bath]]. The canonical ensemble is a probability distribution with the Boltzmann form.&lt;br /&gt;
&lt;br /&gt;
; Statistical frequencies of subsystems' states (in a non-interacting collection)&lt;br /&gt;
&lt;br /&gt;
: When the system of interest is a collection of many non-interacting copies of a smaller subsystem, it is sometimes useful to find the [[statistical frequency]] of a given subsystem state, among the collection. The canonical ensemble has the property of separability when applied to such a collection: as long as the non-interacting subsystems have fixed composition, then each subsystem's state is independent of the others and is also characterized by a canonical ensemble. As a result, the [[expectation value|expected]] statistical frequency distribution of subsystem states has the Boltzmann form.&lt;br /&gt;
&lt;br /&gt;
; [[Maxwell–Boltzmann statistics]] of classical gases (systems of non-interacting particles)&lt;br /&gt;
&lt;br /&gt;
: In particle systems, many particles share the same space and regularly change places with each other; the single-particle state space they occupy is a shared space. [[Maxwell–Boltzmann statistics]] give the expected number of particles found in a given single-particle state, in a [[classical mechanics|classical]] gas of non-interacting particles at equilibrium. This expected number distribution has the Boltzmann form.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Although these cases have strong similarities, it is helpful to distinguish them as they generalize in different ways when the crucial assumptions are changed:&lt;br /&gt;
&lt;br /&gt;
* When a system is in thermodynamic equilibrium with respect to both energy exchange ''and particle exchange'', the requirement of fixed composition is relaxed and a [[grand canonical ensemble]] is obtained rather than canonical ensemble. On the other hand, if both composition and energy are fixed, then a [[microcanonical ensemble]] applies instead.&lt;br /&gt;
&lt;br /&gt;
* If the subsystems within a collection ''do'' interact with each other, then the expected frequencies of subsystem states no longer follow a Boltzmann distribution, and even may not have an [[analytical solution]].&amp;lt;ref&amp;gt;A classic example of this is [[magnetic ordering]]. Systems of non-interacting [[spin (physics)|spins]] show [[paramagnetic]] behaviour that can be understood with a single-particle canonical ensemble (resulting in the [[Brillouin function]]). Systems of ''interacting'' spins can show much more complex behaviour such as [[ferromagnetism]] or [[antiferromagnetism]].&amp;lt;/ref&amp;gt; The canonical ensemble can however still be applied to the ''collective'' states of the entire system considered as a whole, provided the entire system is isolated and in thermal equilibrium.&lt;br /&gt;
&lt;br /&gt;
* With ''[[quantum mechanics|quantum]]'' gases of non-interacting particles in equilibrium, the number of particles found in a given single-particle state does not follow Maxwell–Boltzmann statistics, and there is no simple closed form expression for quantum gases in the canonical ensemble. In the grand canonical ensemble the state-filling statistics of quantum gases are described by [[Fermi–Dirac statistics]] or [[Bose–Einstein statistics]], depending on whether the particles are [[fermion]]s or [[boson]]s respectively.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
|year=1868&lt;br /&gt;
&lt;br /&gt;
1868年&lt;br /&gt;
&lt;br /&gt;
== In mathematics ==&lt;br /&gt;
&lt;br /&gt;
|title=Studien über das Gleichgewicht der lebendigen Kraft zwischen bewegten materiellen Punkten&lt;br /&gt;
&lt;br /&gt;
|title=Studien über das Gleichgewicht der lebendigen Kraft zwischen bewegten materiellen Punkten&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
|trans-title=Studies on the balance of living force between moving material points&lt;br /&gt;
&lt;br /&gt;
| 反题 = 移动物质点之间生命力平衡的研究&lt;br /&gt;
&lt;br /&gt;
{{main|Gibbs measure|Log-linear model|Boltzmann machine}}&lt;br /&gt;
&lt;br /&gt;
|journal=Wiener Berichte |volume=58 |pages=517–560&lt;br /&gt;
&lt;br /&gt;
| journal = Wiener Berichte | volume = 58 | pages = 517-560&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
}}&lt;br /&gt;
&lt;br /&gt;
}}&lt;br /&gt;
&lt;br /&gt;
In more general mathematical settings, the Boltzmann distribution is also known as the [[Gibbs measure]]. In statistics and machine learning, it is called a [[log-linear model]]. In [[deep learning]], the Boltzmann distribution is used in the sampling distribution of [[stochastic neural network]]s such as the [[Boltzmann machine]], [[Restricted Boltzmann machine]], [[Energy based model|Energy-Based models]] and [[Deep Boltzmann Machine|deep Boltzmann machine]].&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
|first=Josiah Willard |last=Gibbs |authorlink=Josiah Willard Gibbs&lt;br /&gt;
&lt;br /&gt;
2012年10月15日 | 约西亚·威拉德·吉布斯&lt;br /&gt;
&lt;br /&gt;
== In economics ==&lt;br /&gt;
&lt;br /&gt;
|year=1902&lt;br /&gt;
&lt;br /&gt;
1902年&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
|title=Elementary Principles in Statistical Mechanics&lt;br /&gt;
&lt;br /&gt;
统计力学的基本原理&lt;br /&gt;
&lt;br /&gt;
The Boltzmann distribution can be introduced to allocate permits in emissions trading.&amp;lt;ref name=&amp;quot;Park, J.-W. 2012&amp;quot;&amp;gt;Park, J.-W., Kim, C. U. and Isard, W. (2012) Permit allocation in emissions trading using the Boltzmann distribution. Physica A 391: 4883–4890&amp;lt;/ref&amp;gt;&amp;lt;ref&amp;gt;[http://www.technologyreview.com/view/425051/the-thorny-problem-of-fair-allocation/ The Thorny Problem Of Fair Allocation]. ''Technology Review'' blog. August 17, 2011. Cites and summarizes Park, Kim and Isard (2012).&amp;lt;/ref&amp;gt; The new allocation method using the Boltzmann distribution can describe the most probable, natural, and unbiased distribution of emissions permits among multiple countries. Simple and versatile, this new method holds potential for many economic and environmental applications.&lt;br /&gt;
&lt;br /&gt;
|title-link=Elementary Principles in Statistical Mechanics }}&lt;br /&gt;
&lt;br /&gt;
| title-link = 基本原理统计力学}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The Boltzmann distribution has the same form as the [[Multinomial logistic regression|multinomial logit]] model. As a [[discrete choice]] model, this is very well known in economics since [[Daniel McFadden]] made the connection to random utility maximization.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Category:Statistical mechanics&lt;br /&gt;
&lt;br /&gt;
类别: 统计力学&lt;br /&gt;
&lt;br /&gt;
==See also==&lt;br /&gt;
&lt;br /&gt;
Distribution&lt;br /&gt;
&lt;br /&gt;
分布&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:Boltzmann distribution]]. Its edit history can be viewed at [[玻尔兹曼分布/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>Tueryeye</name></author>
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		<title>玻尔兹曼分布</title>
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&lt;div&gt;此词条暂由彩云小译翻译，翻译字数共1452，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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{{Use American English|date = March 2019}}&lt;br /&gt;
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{{Short description|Probability distribution of energy states of a system}}&lt;br /&gt;
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{{about|system energy states|particle energy levels and velocities|Maxwell–Boltzmann distribution}}&lt;br /&gt;
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[[File:Boltzmann distribution graph.svg|upright=1.75|right|thumb|Boltzmann factor ''p&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;''&amp;amp;nbsp;/&amp;amp;nbsp;''p&amp;lt;sub&amp;gt;j&amp;lt;/sub&amp;gt;'' (vertical axis) as a function of temperature ''T'' for several energy differences ''ε&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;''&amp;amp;nbsp;−&amp;amp;nbsp;''ε&amp;lt;sub&amp;gt;j&amp;lt;/sub&amp;gt;''.|链接=Special:FilePath/Boltzmann_distribution_graph.svg]]&lt;br /&gt;
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In [[statistical mechanics]] and [[mathematics]], a '''Boltzmann distribution''' (also called '''Gibbs distribution'''&amp;lt;ref name=&amp;quot;landau&amp;quot;&amp;gt;{{cite book | author=Landau, Lev Davidovich |author2=Lifshitz, Evgeny Mikhailovich |name-list-style=amp | title=Statistical Physics |volume=5 |series=Course of Theoretical Physics |edition=3 |origyear=1976 |year=1980 |place=Oxford |publisher=Pergamon Press|isbn=0-7506-3372-7|author-link=Lev Landau |author2-link=Evgeny Lifshitz }} Translated by J.B. Sykes and M.J. Kearsley. See section 28&amp;lt;/ref&amp;gt;) is a [[probability distribution]] or [[probability measure]] that gives the probability that a system will be in a certain [[microstate (statistical mechanics)|state]] as a function of that state's energy and the temperature of the system. The distribution is expressed in the form:&lt;br /&gt;
&lt;br /&gt;
In statistical mechanics and mathematics, a Boltzmann distribution (also called Gibbs distribution) is a probability distribution or probability measure that gives the probability that a system will be in a certain state as a function of that state's energy and the temperature of the system. The distribution is expressed in the form:&lt;br /&gt;
&lt;br /&gt;
在统计力学和数学中，波兹曼分布分布(也称为吉布斯分布&amp;lt;ref name=&amp;quot;landau&amp;quot; /&amp;gt;)是一个概率分布或机率量测，它给出了一个系统处于某种状态的概率，这个概率是该状态的能量和系统温度的函数。分布情况以下列形式表示:&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt;p_i \propto e^{-\frac{\varepsilon_i}{kT}}&amp;lt;/math&amp;gt; &lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt;p_i \propto e^{-\frac{\varepsilon_i}{kT}}&amp;lt;/math&amp;gt; &lt;br /&gt;
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[拉丁语]&lt;br /&gt;
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where {{mvar|p&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;}} is the probability of the system being in state {{mvar|i}}, {{mvar|ε&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;}} is the energy of that state, and a constant {{mvar|kT}} of the distribution is the product of [[Boltzmann's constant]] {{mvar|k}} and [[thermodynamic temperature]] {{mvar|T}}. The symbol &amp;lt;math display=&amp;quot;inline&amp;quot;&amp;gt;\propto&amp;lt;/math&amp;gt; denotes [[proportionality (mathematics)|proportionality]] (see {{section link||The distribution}} for the proportionality constant).&lt;br /&gt;
&lt;br /&gt;
where  is the probability of the system being in state ,  is the energy of that state, and a constant  of the distribution is the product of Boltzmann's constant  and thermodynamic temperature . The symbol &amp;lt;math display=&amp;quot;inline&amp;quot;&amp;gt;\propto&amp;lt;/math&amp;gt; denotes proportionality (see  for the proportionality constant).&lt;br /&gt;
&lt;br /&gt;
{{mvar|p&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;}}是其中系统处于状态{{mvar|i}}的概率, {{mvar|ε&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;}} 是该状态的能量，还有关于这个分布的一个常数{{mvar|kT}} ，它是玻耳兹曼常数{{mvar|k}}和热力学温度 {{mvar|T}}的乘积。符号 &amp;lt; math display = &amp;quot; inline&amp;quot; &amp;gt; propto &amp;lt;nowiki&amp;gt;&amp;lt;/math &amp;gt;&amp;lt;/nowiki&amp;gt; 表示相称性(见附录中的比例常数)。&lt;br /&gt;
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The term system here has a very wide meaning; it can range from a single atom to a macroscopic system such as a [[Natural gas storage|natural gas storage tank]]. Because of this the Boltzmann distribution can be used to solve a very wide variety of problems. The distribution shows that states with lower energy will always have a higher probability of being occupied .&lt;br /&gt;
&lt;br /&gt;
The term system here has a very wide meaning; it can range from a single atom to a macroscopic system such as a natural gas storage tank. Because of this the Boltzmann distribution can be used to solve a very wide variety of problems. The distribution shows that states with lower energy will always have a higher probability of being occupied .&lt;br /&gt;
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这里的术语系统含义广泛; 它可以从单个原子到宏观系统，如天然气储罐。正因为如此，波兹曼分布可以用来解决各种各样的问题。玻尔兹曼分布表明，能量较低的状态被占据的概率总是较高的。&lt;br /&gt;
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The ''ratio'' of probabilities of two states is known as the '''Boltzmann factor''' and characteristically only depends on the states' energy difference:&lt;br /&gt;
&lt;br /&gt;
The ratio of probabilities of two states is known as the Boltzmann factor and characteristically only depends on the states' energy difference:&lt;br /&gt;
&lt;br /&gt;
两种状态的概率之比被称为玻尔兹曼因子，取决于两种状态的能量差:&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
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:&amp;lt;math&amp;gt;\frac{p_i}{p_j} = e^{\frac{\varepsilon_j - \varepsilon_i}{kT}}&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt;\frac{p_i}{p_j} = e^{\frac{\varepsilon_j - \varepsilon_i}{kT}}&amp;lt;/math&amp;gt;&lt;br /&gt;
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[数学][数学]&lt;br /&gt;
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The Boltzmann distribution is named after [[Ludwig Boltzmann]] who first formulated it in 1868 during his studies of the [[statistical mechanics]] of gases in thermal equilibrium. Boltzmann's statistical work is borne out in his paper “On the Relationship between the Second Fundamental Theorem of the Mechanical Theory of Heat and Probability Calculations Regarding the Conditions for Thermal Equilibrium&amp;quot;&amp;lt;ref&amp;gt;http://crystal.med.upenn.edu/sharp-lab-pdfs/2015SharpMatschinsky_Boltz1877_Entropy17.pdf&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
The Boltzmann distribution is named after Ludwig Boltzmann who first formulated it in 1868 during his studies of the statistical mechanics of gases in thermal equilibrium. Boltzmann's statistical work is borne out in his paper “On the Relationship between the Second Fundamental Theorem of the Mechanical Theory of Heat and Probability Calculations Regarding the Conditions for Thermal Equilibrium&amp;quot;&lt;br /&gt;
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波兹曼分布是根据路德维希·玻尔兹曼1868年在研究统计力学中气体热平衡的时候首次提出的一个公式命名的。波尔兹曼的统计工作在他的论文《论热力学第二基本定理与热平衡条件的概率计算之间的关系》中得到了体现。&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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  It would be nice to have a citation here! The origin of the Boltzmann factor isn't entirely clear. According to some authors, Boltzmann's 1968 paper “On the Relationship between the Second Fundamental Theorem of the Mechanical Theory of Heat and Probability Calculations Regarding the Conditions for Thermal Equilibrium”&lt;br /&gt;
&lt;br /&gt;
  It would be nice to have a citation here! The origin of the Boltzmann factor isn't entirely clear. According to some authors, Boltzmann's 1968 paper “On the Relationship between the Second Fundamental Theorem of the Mechanical Theory of Heat and Probability Calculations Regarding the Conditions for Thermal Equilibrium”&lt;br /&gt;
&lt;br /&gt;
如果能在这里引用一下就好了！玻尔兹曼因子的起源并不完全清楚。根据一些作者的说法，Boltzmann 在1968年发表的论文《论热力学第二基本定理与热平衡条件的概率计算之间的关系》&lt;br /&gt;
&lt;br /&gt;
  &amp;quot;Studien über das Gleichgewicht der lebendigen Kraft zwischen bewegten materiellen Punkten&amp;quot; is the origin but I can't find this article at the moment,&lt;br /&gt;
&lt;br /&gt;
  &amp;quot;Studien über das Gleichgewicht der lebendigen Kraft zwischen bewegten materiellen Punkten&amp;quot; is the origin but I can't find this article at the moment,&lt;br /&gt;
&lt;br /&gt;
  &amp;quot;Studien über das Gleichgewicht der lebendigen Kraft zwischen bewegten materiellen Punkten&amp;quot; is the origin but I can't find this article at the moment,&lt;br /&gt;
&lt;br /&gt;
  so I cannot confirm.&lt;br /&gt;
&lt;br /&gt;
  so I cannot confirm.&lt;br /&gt;
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所以我不能确定。&lt;br /&gt;
&lt;br /&gt;
  For example, this book says so, but uses suspiciously modern terminology&lt;br /&gt;
&lt;br /&gt;
  For example, this book says so, but uses suspiciously modern terminology&lt;br /&gt;
&lt;br /&gt;
例如，这本书是这么说的，但是使用了可疑的现代术语&lt;br /&gt;
&lt;br /&gt;
    http://books.google.es/books?id=u13KiGlz2zcC&amp;amp;lpg=PA92&amp;amp;ots=8H1DRURdxn&amp;amp;pg=PA93#v=onepage&amp;amp;f=false&lt;br /&gt;
&lt;br /&gt;
    http://books.google.es/books?id=u13KiGlz2zcC&amp;amp;lpg=PA92&amp;amp;ots=8H1DRURdxn&amp;amp;pg=PA93#v=onepage&amp;amp;f=false&lt;br /&gt;
&lt;br /&gt;
Http://books.google.es/books?id=u13kiglz2zcc&amp;amp;lpg=pa92&amp;amp;ots=8h1drurdxn&amp;amp;pg=pa93#v=onepage&amp;amp;f=false&lt;br /&gt;
&lt;br /&gt;
  On the other hand, Uffink's &amp;quot;Compendium of the foundations of classical statistical physics&amp;quot; does not seem to indicate quite this equation but rather that Boltzmann's 1968 distribution was the simple Maxwell–Boltzmann distribution (for a classical nonrelativistic gas), modified for particles in a potential.&lt;br /&gt;
&lt;br /&gt;
  On the other hand, Uffink's &amp;quot;Compendium of the foundations of classical statistical physics&amp;quot; does not seem to indicate quite this equation but rather that Boltzmann's 1968 distribution was the simple Maxwell–Boltzmann distribution (for a classical nonrelativistic gas), modified for particles in a potential.&lt;br /&gt;
&lt;br /&gt;
另一方面，Uffink 的“经典统计物理学基础纲要”似乎并没有完全表明这个方程，而是说 Boltzmann 在1968年的分布是简单的 Maxwell-波兹曼分布(用于经典的非气体) ，修改为势中的粒子。&lt;br /&gt;
&lt;br /&gt;
--&amp;gt; &lt;br /&gt;
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--&amp;gt; &lt;br /&gt;
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--&amp;gt;&lt;br /&gt;
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The distribution was later investigated extensively, in its modern generic form, by [[Josiah Willard Gibbs]] in 1902.&amp;lt;ref name=&amp;quot;gibbs&amp;quot;&amp;gt;{{cite book |last=Gibbs |first=Josiah Willard |authorlink=Josiah Willard Gibbs |title=Elementary Principles in Statistical Mechanics |year=1902 |publisher=[[Charles Scribner's Sons]] &lt;br /&gt;
&lt;br /&gt;
The distribution was later investigated extensively, in its modern generic form, by Josiah Willard Gibbs in 1902.&lt;br /&gt;
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这种分布后来在1902年由约西亚·威拉德·吉布斯进行了广泛的调查，以其现代通用形式。&lt;br /&gt;
&lt;br /&gt;
|location=New York|title-link=Elementary Principles in Statistical Mechanics }}&amp;lt;/ref&amp;gt;{{rp|Ch.IV}}、&lt;br /&gt;
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在玻尔兹曼分布被发明之后，约西亚·华纳德·吉布森充分地研究了它并在1902年提出了它的一般形式。&amp;lt;ref name=&amp;quot;gibbs&amp;quot; /&amp;gt;&lt;br /&gt;
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The generalized Boltzmann distribution is a sufficient and necessary condition for the equivalence between the statistical mechanics definition of entropy (The  Gibbs entropy formula &amp;lt;math&amp;gt;S = -k_{\mathrm{B}}\sum_i p_i \log p_i&amp;lt;/math&amp;gt;) and the thermodynamic definition of entropy (&amp;lt;math&amp;gt;d S = \frac{\delta Q_\text{rev}}{T}&amp;lt;/math&amp;gt;, and the fundamental thermodynamic relation).&lt;br /&gt;
&lt;br /&gt;
The generalized Boltzmann distribution is a sufficient and necessary condition for the equivalence between the statistical mechanics definition of [[entropy]] (The [[Entropy_(statistical_thermodynamics)#Gibbs_entropy_formula | Gibbs entropy formula]] &amp;lt;math&amp;gt;S = -k_{\mathrm{B}}\sum_i p_i \log p_i&amp;lt;/math&amp;gt;) and the thermodynamic definition of entropy (&amp;lt;math&amp;gt;d S = \frac{\delta Q_\text{rev}}{T}&amp;lt;/math&amp;gt;, and the [[fundamental thermodynamic relation]]).&amp;lt;ref name=&amp;quot;:0&amp;quot;&amp;gt;{{cite journal |last1= Gao |first1= Xiang |last2= Gallicchio |first2= Emilio |first3= Adrian |last3= Roitberg  |date= 2019 |title= The generalized Boltzmann distribution is the only distribution in which the Gibbs-Shannon entropy equals the thermodynamic entropy |journal= The Journal of Chemical Physics|volume= 151|issue= 3|pages= 034113|doi= 10.1063/1.5111333|pmid= 31325924 |arxiv= 1903.02121 |s2cid= 118981017 }}&amp;lt;/ref&amp;gt;&lt;br /&gt;
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广义波兹曼分布是熵的统计力学定义(吉布斯熵公式 &amp;lt; math &amp;gt; s =-k { mathrm { b } sum i log pi i &amp;lt;nowiki&amp;gt;&amp;lt;/math &amp;gt;&amp;lt;/nowiki&amp;gt;)与熵的热力学定义(&amp;lt; math &amp;gt; ds = frac { delta q { rev }{ t } &amp;lt;nowiki&amp;gt;&amp;lt;/math &amp;gt;&amp;lt;/nowiki&amp;gt;)等价的充要条件。&amp;lt;ref name=&amp;quot;:0&amp;quot; /&amp;gt;&lt;br /&gt;
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The Boltzmann distribution should not be confused with the Maxwell–Boltzmann distribution. The former gives the probability that a system will be in a certain state as a function of that state's energy; in contrast, the latter is used to describe particle speeds in idealized gases.&lt;br /&gt;
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值得一提的是，玻尔兹曼分布不应与麦克斯韦-玻尔兹曼分布混淆。前者给出了系统处于某种状态的概率，作为该状态能量的函数; 后者则是用于描述理想气体中的粒子速度。&lt;br /&gt;
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The Boltzmann distribution should not be confused with the [[Maxwell–Boltzmann distribution]]. The former gives the probability that a system will be in a certain state as a function of that state's energy;&amp;lt;ref name=&amp;quot;Atkins, P. W. 2010&amp;quot;&amp;gt;Atkins, P. W. (2010) Quanta, W. H. Freeman and Company, New York&amp;lt;/ref&amp;gt; in contrast, the latter is used to describe particle speeds in idealized gases.&lt;br /&gt;
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==The distribution==&lt;br /&gt;
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The Boltzmann distribution is a probability distribution that gives the probability of a certain state as a function of that state's energy and  temperature of the system to which the distribution is applied. It is given as&lt;br /&gt;
&lt;br /&gt;
波兹曼分布是一个概率分布，它给出了出于某种能量态处于某种能量和温度的时候的概率。它被给出为&lt;br /&gt;
&lt;br /&gt;
The Boltzmann distribution is a [[probability distribution]] that gives the probability of a certain state as a function of that state's energy and  temperature of the [[system]] to which the distribution is applied.&amp;lt;ref name=&amp;quot;McQuarrie, A. 2000&amp;quot;&amp;gt;McQuarrie, A. (2000) Statistical Mechanics, University Science Books, California&amp;lt;/ref&amp;gt; It is given as&lt;br /&gt;
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&amp;lt;math&amp;gt;&lt;br /&gt;
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《数学》&lt;br /&gt;
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:&amp;lt;math&amp;gt;&lt;br /&gt;
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p_i=\frac{1}{Q}} {e^{- {\varepsilon}_i / k T}=\frac{e^{- {\varepsilon}_i / k T}}{\sum_{j=1}^{M}{e^{- {\varepsilon}_j / k T}}}&lt;br /&gt;
&lt;br /&gt;
P _ i = frac {1}{ q }{ e ^ {-{ varepsilon } _ i/k t } = frac { e ^ {-{ varepsilon } _ i/k t }{ sum { j = 1} ^ { m }{ e ^ {-{ varepsilon } _ j/k t }}}}}&lt;br /&gt;
&lt;br /&gt;
p_i=\frac{1}{Q}} {e^{- {\varepsilon}_i / k T}=\frac{e^{- {\varepsilon}_i / k T}}{\sum_{j=1}^{M}{e^{- {\varepsilon}_j / k T}}}&lt;br /&gt;
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&amp;lt;/math&amp;gt;&lt;br /&gt;
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数学&lt;br /&gt;
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&amp;lt;/math&amp;gt;&lt;br /&gt;
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where p&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt; is the probability of state i, ε&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt; the energy of state i, k the Boltzmann constant, T the temperature of the system and M is the number of all states accessible to the system of interest.&lt;br /&gt;
&lt;br /&gt;
其中 p &amp;lt; sub &amp;gt; i  是状态 i 的概率，ε &amp;lt; sub &amp;gt; i  是状态 i 的能量，k 是波兹曼常数，t 是系统的温度，m 是感兴趣的系统所能到达的所有状态的数目。&lt;br /&gt;
&lt;br /&gt;
where ''p&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;'' is the probability of state ''i'', ''ε&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;'' the energy of state ''i'', ''k'' the Boltzmann constant, ''T'' the temperature of the system and ''M'' is the number of all states accessible to the system of interest.&amp;lt;ref name=&amp;quot;McQuarrie, A. 2000&amp;quot;/&amp;gt;&amp;lt;ref name=&amp;quot;Atkins, P. W. 2010&amp;quot;/&amp;gt; Implied parentheses around the denominator ''kT'' are omitted for brevity. The normalization denominator ''Q'' (denoted by some authors by ''Z'') is the [[canonical partition function]]&lt;br /&gt;
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The distribution shows that states with lower energy will always have a higher probability of being occupied than the states with higher energy. It can also give us the quantitative relationship between the probabilities of the two states being occupied. The ratio of probabilities for states i and j is given as&lt;br /&gt;
&lt;br /&gt;
分布表明，能量较低的状态被占据的概率总是高于能量较高的状态。它还可以给出两个状态被占领概率之间的定量关系。给出了状态 i 和状态 j 的概率比为&lt;br /&gt;
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:&amp;lt;math&amp;gt;&lt;br /&gt;
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Q={\sum_{i=1}^{M}{e^{- {\varepsilon}_i / k T}}}&lt;br /&gt;
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&amp;lt;math&amp;gt;&lt;br /&gt;
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《数学》&lt;br /&gt;
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&amp;lt;/math&amp;gt;&lt;br /&gt;
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{\frac{p_i}{p_j}}=e^{({\varepsilon}_j-{\varepsilon}_i) / k T}&lt;br /&gt;
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{ frac { p _ i }{ p _ j } = e ^ {({ varepsilon } _ j-{ varepsilon } _ i)/k t }&lt;br /&gt;
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&amp;lt;/math&amp;gt;&lt;br /&gt;
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数学&lt;br /&gt;
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It results from the constraint that the probabilities of all accessible states must add up to 1.&lt;br /&gt;
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where p&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt; is the probability of state i,  p&amp;lt;sub&amp;gt;j&amp;lt;/sub&amp;gt; the probability of state j, and ε&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt; and ε&amp;lt;sub&amp;gt;j&amp;lt;/sub&amp;gt; are the energies of states i and j, respectively.&lt;br /&gt;
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其中 p &amp;lt; sub &amp;gt; i  是状态 i 的概率，p &amp;lt; sub &amp;gt; j  状态 j 的概率，ε  i  和 ε  j  分别是状态 i 和 j 的能量。&lt;br /&gt;
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The Boltzmann distribution is the distribution that maximizes the [[entropy]]&lt;br /&gt;
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The Boltzmann distribution is often used to describe the distribution of particles, such as atoms or molecules, over energy states accessible to them. If we have a system consisting of many particles, the probability of a particle being in state i is practically the probability that, if we pick a random particle from that system and check what state it is in, we will find it is in state i. This probability is equal to the number of particles in state i divided by the total number of particles in the system, that is the fraction of particles that occupy state i.&lt;br /&gt;
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波兹曼分布通常被用来描述粒子，比如原子或分子，在能量状态上的分布情况。如果我们有一个由许多粒子组成的系统，粒子处于状态 i 的概率实际上等于，如果我们从该系统中选择一个随机粒子并检查它处于什么状态，我们会发现它处于状态 i 的概率。这个概率等于状态 i 的粒子数除以系统中粒子的总数，即占据状态 i 的粒子的比例。&lt;br /&gt;
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:&amp;lt;math&amp;gt;H(p_1,p_2,\cdots,p_M) = -\sum_{i=1}^{M} p_i\log_2 p_i&amp;lt;/math&amp;gt;&lt;br /&gt;
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《数学》&lt;br /&gt;
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subject to the constraint that &amp;lt;math display=&amp;quot;inline&amp;quot;&amp;gt;&lt;br /&gt;
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p_i={\frac{N_i}{N}}&lt;br /&gt;
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P _ i = { frac { n _ i }{ n }&lt;br /&gt;
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{\sum{p_i {\varepsilon}_i}}&lt;br /&gt;
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数学&lt;br /&gt;
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&amp;lt;/math&amp;gt; equals a particular mean energy value (which can be proven using [[Lagrange multipliers]]).&lt;br /&gt;
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where N&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt; is the number of particles in state i and N is the total number of particles in the system. We may use the Boltzmann distribution to find this probability that is, as we have seen, equal to the fraction of particles that are in state i. So the equation that gives the fraction of particles in state i as a function of the energy of that state is   In order for this to be possible, there must be some particles in the first state to undergo the transition. We may find that this condition is fulfilled by finding the fraction of particles in the first state. If it is negligible, the transition is very likely not to be observed at the temperature for which the calculation was done. In general, a larger fraction of molecules in the first state means a higher number of transitions to the second state. This gives a stronger spectral line. However, there are other factors that influence the intensity of a spectral line, such as whether it is caused by an allowed or a forbidden transition.&lt;br /&gt;
&lt;br /&gt;
其中 n &amp;lt; sub &amp;gt; i  是状态 i 的粒子数，n 是系统中粒子的总数。我们可以用波兹曼分布来求出这个概率，就像我们看到的那样，等于处于 i 状态的粒子的比例。所以给出状态 i 的粒子比例，作为状态能量的函数的方程是，为了使这成为可能，必须有一些粒子处于第一个状态，才能发生跃迁。我们可以通过求第一态粒子的比例来满足这个条件。如果它可以忽略不计，那么在进行计算的温度下，极有可能不能观察到这种转变。一般来说，处于第一状态的分子比例越大，意味着向第二状态转变的次数越多。这就产生了一条更强的谱线。然而，还有其他因素影响谱线的强度，例如它是由允许的跃迁还是禁止的跃迁引起的。&lt;br /&gt;
&lt;br /&gt;
The partition function can be calculated if we know the energies of the states accessible to the system of interest. For atoms the partition function values can be found in the NIST Atomic Spectra Database.&amp;lt;ref&amp;gt;[http://physics.nist.gov/PhysRefData/ASD/levels_form.html NIST Atomic Spectra Database Levels Form] at nist.gov&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The Boltzmann distribution is related to the softmax function commonly used in machine learning.&lt;br /&gt;
&lt;br /&gt;
波兹曼分布学习与机器学习中常用的柔性最大激活函数学习有关。&lt;br /&gt;
&lt;br /&gt;
The distribution shows that states with lower energy will always have a higher probability of being occupied than the states with higher energy. It can also give us the quantitative relationship between the probabilities of the two states being occupied. The ratio of probabilities for states ''i'' and ''j'' is given as&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
{\frac{p_i}{p_j}}=e^{({\varepsilon}_j-{\varepsilon}_i) / k T}&lt;br /&gt;
&lt;br /&gt;
&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
The Boltzmann distribution appears in statistical mechanics when considering isolated (or nearly-isolated) systems of fixed composition that are in thermal equilibrium (equilibrium with respect to energy exchange). The most general case is the probability distribution for the canonical ensemble, but also some special cases (derivable from the canonical ensemble) also show the Boltzmann distribution in different aspects:&lt;br /&gt;
&lt;br /&gt;
当考虑孤立的(或者几乎孤立的)固定组成的体系处于平衡状态时，波兹曼分布出现在《统计力学热平衡。最普遍的情况是概率分布的正则系综，但也有一些特殊的情况(从正则系综衍生)也显示了波兹曼分布在不同的方面:&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
where ''p&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;'' is the probability of state ''i'',  ''p&amp;lt;sub&amp;gt;j&amp;lt;/sub&amp;gt;'' the probability of state ''j'', and ''ε&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;'' and ''ε&amp;lt;sub&amp;gt;j&amp;lt;/sub&amp;gt;'' are the energies of states ''i'' and ''j'', respectively.&lt;br /&gt;
&lt;br /&gt;
 Canonical ensemble (general case)&lt;br /&gt;
&lt;br /&gt;
正则系综(一般情况)&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
 The canonical ensemble gives the probabilities of the various possible states of a closed system of fixed volume, in thermal equilibrium with a heat bath. The canonical ensemble is a probability distribution with the Boltzmann form.&lt;br /&gt;
&lt;br /&gt;
正则系综模型给出了一个封闭的固定体积系统的各种可能状态的概率，这个封闭体积系统包括一个带有热浴的热平衡。正则系综是一个玻尔兹曼概率分布。&lt;br /&gt;
&lt;br /&gt;
The Boltzmann distribution is often used to describe the distribution of particles, such as atoms or molecules, over energy states accessible to them. If we have a system consisting of many particles, the probability of a particle being in state ''i'' is practically the probability that, if we pick a random particle from that system and check what state it is in, we will find it is in state ''i''. This probability is equal to the number of particles in state ''i'' divided by the total number of particles in the system, that is the fraction of particles that occupy state ''i''.&lt;br /&gt;
&lt;br /&gt;
 Statistical frequencies of subsystems' states (in a non-interacting collection)&lt;br /&gt;
&lt;br /&gt;
子系统状态的统计频率(在一个无交互的集合中)&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
 When the system of interest is a collection of many non-interacting copies of a smaller subsystem, it is sometimes useful to find the statistical frequency of a given subsystem state, among the collection. The canonical ensemble has the property of separability when applied to such a collection: as long as the non-interacting subsystems have fixed composition, then each subsystem's state is independent of the others and is also characterized by a canonical ensemble. As a result, the expected statistical frequency distribution of subsystem states has the Boltzmann form.&lt;br /&gt;
&lt;br /&gt;
当感兴趣的系统是一个较小子系统的许多非交互副本的集合时，在集合中查找给定子系统状态的统计频率有时是有用的。当应用于这样一个集合时，正则系综子系统具有可分离性: 只要不相互作用的子系统的组成是固定的，那么每个子系统的状态是独立于其他子系统的，也是一个拥有属性正则系综。因此，子系统状态的期望统计频率分布具有玻耳兹曼形式。&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 Maxwell–Boltzmann statistics of classical gases (systems of non-interacting particles)&lt;br /&gt;
&lt;br /&gt;
经典气体(非相互作用粒子系统)的 Maxwell-Boltzmann 统计&lt;br /&gt;
&lt;br /&gt;
p_i={\frac{N_i}{N}}&lt;br /&gt;
&lt;br /&gt;
 In particle systems, many particles share the same space and regularly change places with each other; the single-particle state space they occupy is a shared space. Maxwell–Boltzmann statistics give the expected number of particles found in a given single-particle state, in a classical gas of non-interacting particles at equilibrium. This expected number distribution has the Boltzmann form.&lt;br /&gt;
&lt;br /&gt;
在粒子系统中，许多粒子共享同一空间，并且相互之间有规律地改变位置; 它们所占据的单粒子状态空间是一个共享空间。麦克斯韦-玻尔兹曼统计给出了在一个给定的单粒子态，在一个处于平衡状态的非相互作用粒子的经典气体中所发现的粒子的预期数量。这个预期的数分布具有玻耳兹曼形式。&lt;br /&gt;
&lt;br /&gt;
&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Although these cases have strong similarities, it is helpful to distinguish them as they generalize in different ways when the crucial assumptions are changed:&lt;br /&gt;
&lt;br /&gt;
虽然这些案例有很多相似之处，但是当关键假设发生变化时，它们以不同的方式进行归纳，因此区分它们是有帮助的:&lt;br /&gt;
&lt;br /&gt;
where ''N&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;'' is the number of particles in state ''i'' and ''N'' is the total number of particles in the system. We may use the Boltzmann distribution to find this probability that is, as we have seen, equal to the fraction of particles that are in state i. So the equation that gives the fraction of particles in state ''i'' as a function of the energy of that state is  &amp;lt;ref name=&amp;quot;Atkins, P. W. 2010&amp;quot;/&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
{\frac{N_i}{N}}={\frac{e^{- {\varepsilon}_i / k T}}{\sum_{j=1}^{M}{e^{- {\varepsilon}_j / k T}}}}&lt;br /&gt;
&lt;br /&gt;
&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
This equation is of great importance to [[spectroscopy]]. In spectroscopy we observe a [[spectral line]] of atoms or molecules that we are interested in going from one state to another.&amp;lt;ref name=&amp;quot;Atkins, P. W. 2010&amp;quot;/&amp;gt;&amp;lt;ref&amp;gt;Atkins, P. W.; de Paula J. (2009) Physical Chemistry, 9th edition, Oxford University Press, Oxford, UK&amp;lt;/ref&amp;gt; In order for this to be possible, there must be some particles in the first state to undergo the transition. We may find that this condition is fulfilled by finding the fraction of particles in the first state. If it is negligible, the transition is very likely not to be observed at the temperature for which the calculation was done. In general, a larger fraction of molecules in the first state means a higher number of transitions to the second state.&amp;lt;ref&amp;gt;Skoog, D. A.; Holler, F. J.; Crouch, S. R. (2006) Principles of Instrumental Analysis, Brooks/Cole, Boston, MA&amp;lt;/ref&amp;gt; This gives a stronger spectral line. However, there are other factors that influence the intensity of a spectral line, such as whether it is caused by an allowed or a [[forbidden transition]].&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The Boltzmann distribution is related to the [[softmax function]] commonly used in machine learning.&lt;br /&gt;
&lt;br /&gt;
In more general mathematical settings, the Boltzmann distribution is also known as the Gibbs measure. In statistics and machine learning, it is called a log-linear model. In deep learning, the Boltzmann distribution is used in the sampling distribution of stochastic neural networks such as the Boltzmann machine, Restricted Boltzmann machine, Energy-Based models and deep Boltzmann machine.&lt;br /&gt;
&lt;br /&gt;
在更一般的数学环境中，波兹曼分布也被称为吉布斯量度。在统计学和机器学习中，它被称为对数线性回归。在深度学习中，波兹曼分布被用于随机神经网络的抽样分布，如波茨曼机、受限玻尔兹曼机、基于能量的模型和深度波茨曼机。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
== In statistical mechanics ==&lt;br /&gt;
&lt;br /&gt;
{{main|Canonical ensemble|Maxwell–Boltzmann statistics}}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The Boltzmann distribution can be introduced to allocate permits in emissions trading. The new allocation method using the Boltzmann distribution can describe the most probable, natural, and unbiased distribution of emissions permits among multiple countries. Simple and versatile, this new method holds potential for many economic and environmental applications.&lt;br /&gt;
&lt;br /&gt;
可以引入欧盟波兹曼分布来分配排放交易的许可。这种新的排放量分配方法使用波兹曼分布能够描述多个国家之间最可能、最自然和最无偏见的排放量分配。这种新方法简单而通用，具有许多经济和环境应用的潜力。&lt;br /&gt;
&lt;br /&gt;
The Boltzmann distribution appears in [[statistical mechanics]] when considering isolated (or nearly-isolated) systems of fixed composition that are in [[thermal equilibrium]] (equilibrium with respect to energy exchange). The most general case is the probability distribution for the canonical ensemble, but also some special cases (derivable from the canonical ensemble) also show the Boltzmann distribution in different aspects:&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The Boltzmann distribution has the same form as the multinomial logit model. As a discrete choice model, this is very well known in economics since Daniel McFadden made the connection to random utility maximization.&lt;br /&gt;
&lt;br /&gt;
波兹曼分布与多项式 logit 模型具有相同的形式。作为一个离散选择模型，这在经济学中非常著名，因为丹尼尔 · 麦克法登提出了随机效用最大化的联系。&lt;br /&gt;
&lt;br /&gt;
; [[Canonical ensemble]] (general case)&lt;br /&gt;
&lt;br /&gt;
: The [[canonical ensemble]] gives the [[probabilities]] of the various possible states of a closed system of fixed volume, in thermal equilibrium with a [[heat bath]]. The canonical ensemble is a probability distribution with the Boltzmann form.&lt;br /&gt;
&lt;br /&gt;
; Statistical frequencies of subsystems' states (in a non-interacting collection)&lt;br /&gt;
&lt;br /&gt;
: When the system of interest is a collection of many non-interacting copies of a smaller subsystem, it is sometimes useful to find the [[statistical frequency]] of a given subsystem state, among the collection. The canonical ensemble has the property of separability when applied to such a collection: as long as the non-interacting subsystems have fixed composition, then each subsystem's state is independent of the others and is also characterized by a canonical ensemble. As a result, the [[expectation value|expected]] statistical frequency distribution of subsystem states has the Boltzmann form.&lt;br /&gt;
&lt;br /&gt;
; [[Maxwell–Boltzmann statistics]] of classical gases (systems of non-interacting particles)&lt;br /&gt;
&lt;br /&gt;
: In particle systems, many particles share the same space and regularly change places with each other; the single-particle state space they occupy is a shared space. [[Maxwell–Boltzmann statistics]] give the expected number of particles found in a given single-particle state, in a [[classical mechanics|classical]] gas of non-interacting particles at equilibrium. This expected number distribution has the Boltzmann form.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Although these cases have strong similarities, it is helpful to distinguish them as they generalize in different ways when the crucial assumptions are changed:&lt;br /&gt;
&lt;br /&gt;
* When a system is in thermodynamic equilibrium with respect to both energy exchange ''and particle exchange'', the requirement of fixed composition is relaxed and a [[grand canonical ensemble]] is obtained rather than canonical ensemble. On the other hand, if both composition and energy are fixed, then a [[microcanonical ensemble]] applies instead.&lt;br /&gt;
&lt;br /&gt;
* If the subsystems within a collection ''do'' interact with each other, then the expected frequencies of subsystem states no longer follow a Boltzmann distribution, and even may not have an [[analytical solution]].&amp;lt;ref&amp;gt;A classic example of this is [[magnetic ordering]]. Systems of non-interacting [[spin (physics)|spins]] show [[paramagnetic]] behaviour that can be understood with a single-particle canonical ensemble (resulting in the [[Brillouin function]]). Systems of ''interacting'' spins can show much more complex behaviour such as [[ferromagnetism]] or [[antiferromagnetism]].&amp;lt;/ref&amp;gt; The canonical ensemble can however still be applied to the ''collective'' states of the entire system considered as a whole, provided the entire system is isolated and in thermal equilibrium.&lt;br /&gt;
&lt;br /&gt;
* With ''[[quantum mechanics|quantum]]'' gases of non-interacting particles in equilibrium, the number of particles found in a given single-particle state does not follow Maxwell–Boltzmann statistics, and there is no simple closed form expression for quantum gases in the canonical ensemble. In the grand canonical ensemble the state-filling statistics of quantum gases are described by [[Fermi–Dirac statistics]] or [[Bose–Einstein statistics]], depending on whether the particles are [[fermion]]s or [[boson]]s respectively.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
|year=1868&lt;br /&gt;
&lt;br /&gt;
1868年&lt;br /&gt;
&lt;br /&gt;
== In mathematics ==&lt;br /&gt;
&lt;br /&gt;
|title=Studien über das Gleichgewicht der lebendigen Kraft zwischen bewegten materiellen Punkten&lt;br /&gt;
&lt;br /&gt;
|title=Studien über das Gleichgewicht der lebendigen Kraft zwischen bewegten materiellen Punkten&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
|trans-title=Studies on the balance of living force between moving material points&lt;br /&gt;
&lt;br /&gt;
| 反题 = 移动物质点之间生命力平衡的研究&lt;br /&gt;
&lt;br /&gt;
{{main|Gibbs measure|Log-linear model|Boltzmann machine}}&lt;br /&gt;
&lt;br /&gt;
|journal=Wiener Berichte |volume=58 |pages=517–560&lt;br /&gt;
&lt;br /&gt;
| journal = Wiener Berichte | volume = 58 | pages = 517-560&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
}}&lt;br /&gt;
&lt;br /&gt;
}}&lt;br /&gt;
&lt;br /&gt;
In more general mathematical settings, the Boltzmann distribution is also known as the [[Gibbs measure]]. In statistics and machine learning, it is called a [[log-linear model]]. In [[deep learning]], the Boltzmann distribution is used in the sampling distribution of [[stochastic neural network]]s such as the [[Boltzmann machine]], [[Restricted Boltzmann machine]], [[Energy based model|Energy-Based models]] and [[Deep Boltzmann Machine|deep Boltzmann machine]].&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
|first=Josiah Willard |last=Gibbs |authorlink=Josiah Willard Gibbs&lt;br /&gt;
&lt;br /&gt;
2012年10月15日 | 约西亚·威拉德·吉布斯&lt;br /&gt;
&lt;br /&gt;
== In economics ==&lt;br /&gt;
&lt;br /&gt;
|year=1902&lt;br /&gt;
&lt;br /&gt;
1902年&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
|title=Elementary Principles in Statistical Mechanics&lt;br /&gt;
&lt;br /&gt;
统计力学的基本原理&lt;br /&gt;
&lt;br /&gt;
The Boltzmann distribution can be introduced to allocate permits in emissions trading.&amp;lt;ref name=&amp;quot;Park, J.-W. 2012&amp;quot;&amp;gt;Park, J.-W., Kim, C. U. and Isard, W. (2012) Permit allocation in emissions trading using the Boltzmann distribution. Physica A 391: 4883–4890&amp;lt;/ref&amp;gt;&amp;lt;ref&amp;gt;[http://www.technologyreview.com/view/425051/the-thorny-problem-of-fair-allocation/ The Thorny Problem Of Fair Allocation]. ''Technology Review'' blog. August 17, 2011. Cites and summarizes Park, Kim and Isard (2012).&amp;lt;/ref&amp;gt; The new allocation method using the Boltzmann distribution can describe the most probable, natural, and unbiased distribution of emissions permits among multiple countries. Simple and versatile, this new method holds potential for many economic and environmental applications.&lt;br /&gt;
&lt;br /&gt;
|title-link=Elementary Principles in Statistical Mechanics }}&lt;br /&gt;
&lt;br /&gt;
| title-link = 基本原理统计力学}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The Boltzmann distribution has the same form as the [[Multinomial logistic regression|multinomial logit]] model. As a [[discrete choice]] model, this is very well known in economics since [[Daniel McFadden]] made the connection to random utility maximization.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Category:Statistical mechanics&lt;br /&gt;
&lt;br /&gt;
类别: 统计力学&lt;br /&gt;
&lt;br /&gt;
==See also==&lt;br /&gt;
&lt;br /&gt;
Distribution&lt;br /&gt;
&lt;br /&gt;
分布&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:Boltzmann distribution]]. Its edit history can be viewed at [[玻尔兹曼分布/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>Tueryeye</name></author>
	</entry>
	<entry>
		<id>https://wiki.swarma.org/index.php?title=%E7%8E%BB%E5%B0%94%E5%85%B9%E6%9B%BC%E5%88%86%E5%B8%83&amp;diff=26934</id>
		<title>玻尔兹曼分布</title>
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		<updated>2021-10-05T15:17:26Z</updated>

		<summary type="html">&lt;p&gt;Tueryeye：修正编辑翻译的内容&lt;/p&gt;
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&lt;div&gt;此词条暂由彩云小译翻译，翻译字数共1452，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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{{Use American English|date = March 2019}}&lt;br /&gt;
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{{Short description|Probability distribution of energy states of a system}}&lt;br /&gt;
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{{about|system energy states|particle energy levels and velocities|Maxwell–Boltzmann distribution}}&lt;br /&gt;
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[[File:Boltzmann distribution graph.svg|upright=1.75|right|thumb|Boltzmann factor ''p&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;''&amp;amp;nbsp;/&amp;amp;nbsp;''p&amp;lt;sub&amp;gt;j&amp;lt;/sub&amp;gt;'' (vertical axis) as a function of temperature ''T'' for several energy differences ''ε&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;''&amp;amp;nbsp;−&amp;amp;nbsp;''ε&amp;lt;sub&amp;gt;j&amp;lt;/sub&amp;gt;''.|链接=Special:FilePath/Boltzmann_distribution_graph.svg]]&lt;br /&gt;
&lt;br /&gt;
Boltzmann factor p&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;&amp;amp;nbsp;/&amp;amp;nbsp;p&amp;lt;sub&amp;gt;j&amp;lt;/sub&amp;gt; (vertical axis) as a function of temperature T for several energy differences ε&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;&amp;amp;nbsp;−&amp;amp;nbsp;ε&amp;lt;sub&amp;gt;j&amp;lt;/sub&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
玻尔兹曼因子 p&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;&amp;amp;nbsp;/&amp;amp;nbsp;p&amp;lt;sub&amp;gt;j&amp;lt;/sub&amp;gt; (垂直轴) 作为温度 T 对于几个能量差异ε&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;&amp;amp;nbsp;−&amp;amp;nbsp;ε&amp;lt;sub&amp;gt;j&amp;lt;/sub&amp;gt;的函数 。&lt;br /&gt;
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In [[statistical mechanics]] and [[mathematics]], a '''Boltzmann distribution''' (also called '''Gibbs distribution'''&amp;lt;ref name=&amp;quot;landau&amp;quot;&amp;gt;{{cite book | author=Landau, Lev Davidovich |author2=Lifshitz, Evgeny Mikhailovich |name-list-style=amp | title=Statistical Physics |volume=5 |series=Course of Theoretical Physics |edition=3 |origyear=1976 |year=1980 |place=Oxford |publisher=Pergamon Press|isbn=0-7506-3372-7|author-link=Lev Landau |author2-link=Evgeny Lifshitz }} Translated by J.B. Sykes and M.J. Kearsley. See section 28&amp;lt;/ref&amp;gt;) is a [[probability distribution]] or [[probability measure]] that gives the probability that a system will be in a certain [[microstate (statistical mechanics)|state]] as a function of that state's energy and the temperature of the system. The distribution is expressed in the form:&lt;br /&gt;
&lt;br /&gt;
In statistical mechanics and mathematics, a Boltzmann distribution (also called Gibbs distribution) is a probability distribution or probability measure that gives the probability that a system will be in a certain state as a function of that state's energy and the temperature of the system. The distribution is expressed in the form:&lt;br /&gt;
&lt;br /&gt;
在统计力学和数学中，波兹曼分布分布(也称为吉布斯分布&amp;lt;ref name=&amp;quot;landau&amp;quot; /&amp;gt;)是一个概率分布或机率量测，它给出了一个系统处于某种状态的概率，这个概率是该状态的能量和系统温度的函数。分布情况以下列形式表示:&lt;br /&gt;
&lt;br /&gt;
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:&amp;lt;math&amp;gt;p_i \propto e^{-\frac{\varepsilon_i}{kT}}&amp;lt;/math&amp;gt; &lt;br /&gt;
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&amp;lt;math&amp;gt;p_i \propto e^{-\frac{\varepsilon_i}{kT}}&amp;lt;/math&amp;gt; &lt;br /&gt;
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[拉丁语]&lt;br /&gt;
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where {{mvar|p&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;}} is the probability of the system being in state {{mvar|i}}, {{mvar|ε&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;}} is the energy of that state, and a constant {{mvar|kT}} of the distribution is the product of [[Boltzmann's constant]] {{mvar|k}} and [[thermodynamic temperature]] {{mvar|T}}. The symbol &amp;lt;math display=&amp;quot;inline&amp;quot;&amp;gt;\propto&amp;lt;/math&amp;gt; denotes [[proportionality (mathematics)|proportionality]] (see {{section link||The distribution}} for the proportionality constant).&lt;br /&gt;
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where  is the probability of the system being in state ,  is the energy of that state, and a constant  of the distribution is the product of Boltzmann's constant  and thermodynamic temperature . The symbol &amp;lt;math display=&amp;quot;inline&amp;quot;&amp;gt;\propto&amp;lt;/math&amp;gt; denotes proportionality (see  for the proportionality constant).&lt;br /&gt;
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{{mvar|p&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;}}是其中系统处于状态{{mvar|i}}的概率, {{mvar|ε&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;}} 是该状态的能量，还有关于这个分布的一个常数{{mvar|kT}} ，它是玻耳兹曼常数{{mvar|k}}和热力学温度 {{mvar|T}}的乘积。符号 &amp;lt; math display = &amp;quot; inline&amp;quot; &amp;gt; propto &amp;lt;nowiki&amp;gt;&amp;lt;/math &amp;gt;&amp;lt;/nowiki&amp;gt; 表示相称性(见附录中的比例常数)。&lt;br /&gt;
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The term system here has a very wide meaning; it can range from a single atom to a macroscopic system such as a [[Natural gas storage|natural gas storage tank]]. Because of this the Boltzmann distribution can be used to solve a very wide variety of problems. The distribution shows that states with lower energy will always have a higher probability of being occupied .&lt;br /&gt;
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The term system here has a very wide meaning; it can range from a single atom to a macroscopic system such as a natural gas storage tank. Because of this the Boltzmann distribution can be used to solve a very wide variety of problems. The distribution shows that states with lower energy will always have a higher probability of being occupied .&lt;br /&gt;
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这里的术语系统有非常广泛的含义; 它可以从单个原子到宏观系统，如天然气储罐。正因为如此，波兹曼分布可以用来解决各种各样的问题。分布表明，能量较低的状态被占据的概率总是较高的。&lt;br /&gt;
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The ''ratio'' of probabilities of two states is known as the '''Boltzmann factor''' and characteristically only depends on the states' energy difference:&lt;br /&gt;
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The ratio of probabilities of two states is known as the Boltzmann factor and characteristically only depends on the states' energy difference:&lt;br /&gt;
&lt;br /&gt;
两种状态的概率之比被称为玻尔兹曼因子，其特点仅取决于两种状态的能量差:&lt;br /&gt;
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:&amp;lt;math&amp;gt;\frac{p_i}{p_j} = e^{\frac{\varepsilon_j - \varepsilon_i}{kT}}&amp;lt;/math&amp;gt;&lt;br /&gt;
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&amp;lt;math&amp;gt;\frac{p_i}{p_j} = e^{\frac{\varepsilon_j - \varepsilon_i}{kT}}&amp;lt;/math&amp;gt;&lt;br /&gt;
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[数学][数学]&lt;br /&gt;
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The Boltzmann distribution is named after [[Ludwig Boltzmann]] who first formulated it in 1868 during his studies of the [[statistical mechanics]] of gases in thermal equilibrium. Boltzmann's statistical work is borne out in his paper “On the Relationship between the Second Fundamental Theorem of the Mechanical Theory of Heat and Probability Calculations Regarding the Conditions for Thermal Equilibrium&amp;quot;&amp;lt;ref&amp;gt;http://crystal.med.upenn.edu/sharp-lab-pdfs/2015SharpMatschinsky_Boltz1877_Entropy17.pdf&amp;lt;/ref&amp;gt;&lt;br /&gt;
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The Boltzmann distribution is named after Ludwig Boltzmann who first formulated it in 1868 during his studies of the statistical mechanics of gases in thermal equilibrium. Boltzmann's statistical work is borne out in his paper “On the Relationship between the Second Fundamental Theorem of the Mechanical Theory of Heat and Probability Calculations Regarding the Conditions for Thermal Equilibrium&amp;quot;&lt;br /&gt;
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波兹曼分布是根据1868年他在研究统计力学气体在热平衡的时候首次提出的一个公式命名的。波尔兹曼的统计工作在他的论文《论热力学第二基本定理与热平衡条件的概率计算之间的关系》中得到了证实&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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  It would be nice to have a citation here! The origin of the Boltzmann factor isn't entirely clear. According to some authors, Boltzmann's 1968 paper “On the Relationship between the Second Fundamental Theorem of the Mechanical Theory of Heat and Probability Calculations Regarding the Conditions for Thermal Equilibrium”&lt;br /&gt;
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  It would be nice to have a citation here! The origin of the Boltzmann factor isn't entirely clear. According to some authors, Boltzmann's 1968 paper “On the Relationship between the Second Fundamental Theorem of the Mechanical Theory of Heat and Probability Calculations Regarding the Conditions for Thermal Equilibrium”&lt;br /&gt;
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如果能在这里引用一下就好了！玻尔兹曼因子的起源并不完全清楚。根据一些作者的说法，Boltzmann 在1968年发表的论文《论热力学第二基本定理与热平衡条件的概率计算之间的关系》&lt;br /&gt;
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  &amp;quot;Studien über das Gleichgewicht der lebendigen Kraft zwischen bewegten materiellen Punkten&amp;quot; is the origin but I can't find this article at the moment,&lt;br /&gt;
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  &amp;quot;Studien über das Gleichgewicht der lebendigen Kraft zwischen bewegten materiellen Punkten&amp;quot; is the origin but I can't find this article at the moment,&lt;br /&gt;
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  &amp;quot;Studien über das Gleichgewicht der lebendigen Kraft zwischen bewegten materiellen Punkten&amp;quot; is the origin but I can't find this article at the moment,&lt;br /&gt;
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  so I cannot confirm.&lt;br /&gt;
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  so I cannot confirm.&lt;br /&gt;
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所以我不能确定。&lt;br /&gt;
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  For example, this book says so, but uses suspiciously modern terminology&lt;br /&gt;
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  For example, this book says so, but uses suspiciously modern terminology&lt;br /&gt;
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例如，这本书是这么说的，但是使用了可疑的现代术语&lt;br /&gt;
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    http://books.google.es/books?id=u13KiGlz2zcC&amp;amp;lpg=PA92&amp;amp;ots=8H1DRURdxn&amp;amp;pg=PA93#v=onepage&amp;amp;f=false&lt;br /&gt;
&lt;br /&gt;
    http://books.google.es/books?id=u13KiGlz2zcC&amp;amp;lpg=PA92&amp;amp;ots=8H1DRURdxn&amp;amp;pg=PA93#v=onepage&amp;amp;f=false&lt;br /&gt;
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Http://books.google.es/books?id=u13kiglz2zcc&amp;amp;lpg=pa92&amp;amp;ots=8h1drurdxn&amp;amp;pg=pa93#v=onepage&amp;amp;f=false&lt;br /&gt;
&lt;br /&gt;
  On the other hand, Uffink's &amp;quot;Compendium of the foundations of classical statistical physics&amp;quot; does not seem to indicate quite this equation but rather that Boltzmann's 1968 distribution was the simple Maxwell–Boltzmann distribution (for a classical nonrelativistic gas), modified for particles in a potential.&lt;br /&gt;
&lt;br /&gt;
  On the other hand, Uffink's &amp;quot;Compendium of the foundations of classical statistical physics&amp;quot; does not seem to indicate quite this equation but rather that Boltzmann's 1968 distribution was the simple Maxwell–Boltzmann distribution (for a classical nonrelativistic gas), modified for particles in a potential.&lt;br /&gt;
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另一方面，Uffink 的“经典统计物理学基础纲要”似乎并没有完全表明这个方程，而是说 Boltzmann 在1968年的分布是简单的 Maxwell-波兹曼分布(用于经典的非气体) ，修改为势中的粒子。&lt;br /&gt;
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--&amp;gt; &lt;br /&gt;
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--&amp;gt; &lt;br /&gt;
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--&amp;gt;&lt;br /&gt;
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The distribution was later investigated extensively, in its modern generic form, by [[Josiah Willard Gibbs]] in 1902.&amp;lt;ref name=&amp;quot;gibbs&amp;quot;&amp;gt;{{cite book |last=Gibbs |first=Josiah Willard |authorlink=Josiah Willard Gibbs |title=Elementary Principles in Statistical Mechanics |year=1902 |publisher=[[Charles Scribner's Sons]] &lt;br /&gt;
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The distribution was later investigated extensively, in its modern generic form, by Josiah Willard Gibbs in 1902.&lt;br /&gt;
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这种分布后来在1902年由约西亚·威拉德·吉布斯进行了广泛的调查，以其现代通用形式。&lt;br /&gt;
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|location=New York|title-link=Elementary Principles in Statistical Mechanics }}&amp;lt;/ref&amp;gt;{{rp|Ch.IV}}&lt;br /&gt;
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The generalized Boltzmann distribution is a sufficient and necessary condition for the equivalence between the statistical mechanics definition of entropy (The  Gibbs entropy formula &amp;lt;math&amp;gt;S = -k_{\mathrm{B}}\sum_i p_i \log p_i&amp;lt;/math&amp;gt;) and the thermodynamic definition of entropy (&amp;lt;math&amp;gt;d S = \frac{\delta Q_\text{rev}}{T}&amp;lt;/math&amp;gt;, and the fundamental thermodynamic relation).&lt;br /&gt;
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广义波兹曼分布是熵的统计力学定义(吉布斯熵公式 &amp;lt; math &amp;gt; s =-k { mathrm { b } sum i log pi i &amp;lt;/math &amp;gt;)与熵的热力学定义(&amp;lt; math &amp;gt; ds = frac { delta q { rev }{ t } &amp;lt;/math &amp;gt;)等价的充要条件。&lt;br /&gt;
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The generalized Boltzmann distribution is a sufficient and necessary condition for the equivalence between the statistical mechanics definition of [[entropy]] (The [[Entropy_(statistical_thermodynamics)#Gibbs_entropy_formula | Gibbs entropy formula]] &amp;lt;math&amp;gt;S = -k_{\mathrm{B}}\sum_i p_i \log p_i&amp;lt;/math&amp;gt;) and the thermodynamic definition of entropy (&amp;lt;math&amp;gt;d S = \frac{\delta Q_\text{rev}}{T}&amp;lt;/math&amp;gt;, and the [[fundamental thermodynamic relation]]).&amp;lt;ref&amp;gt;{{cite journal |last1= Gao |first1= Xiang |last2= Gallicchio |first2= Emilio |first3= Adrian |last3= Roitberg  |date= 2019 |title= The generalized Boltzmann distribution is the only distribution in which the Gibbs-Shannon entropy equals the thermodynamic entropy |journal= The Journal of Chemical Physics|volume= 151|issue= 3|pages= 034113|doi= 10.1063/1.5111333|pmid= 31325924 |arxiv= 1903.02121 |s2cid= 118981017 }}&amp;lt;/ref&amp;gt;&lt;br /&gt;
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The Boltzmann distribution should not be confused with the Maxwell–Boltzmann distribution. The former gives the probability that a system will be in a certain state as a function of that state's energy; in contrast, the latter is used to describe particle speeds in idealized gases.&lt;br /&gt;
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波兹曼分布不应与麦克斯韦-波兹曼分布混淆。前者给出了系统处于某种状态的概率，作为该状态能量的函数; 相反，后者用于描述理想气体中的粒子速度。&lt;br /&gt;
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The Boltzmann distribution should not be confused with the [[Maxwell–Boltzmann distribution]]. The former gives the probability that a system will be in a certain state as a function of that state's energy;&amp;lt;ref name=&amp;quot;Atkins, P. W. 2010&amp;quot;&amp;gt;Atkins, P. W. (2010) Quanta, W. H. Freeman and Company, New York&amp;lt;/ref&amp;gt; in contrast, the latter is used to describe particle speeds in idealized gases.&lt;br /&gt;
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==The distribution==&lt;br /&gt;
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The Boltzmann distribution is a probability distribution that gives the probability of a certain state as a function of that state's energy and  temperature of the system to which the distribution is applied. It is given as&lt;br /&gt;
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波兹曼分布是一个概率分布，它给出了某种状态的概率，作为该状态的能量和温度的函数，该分布适用于系统。它被给出为&lt;br /&gt;
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The Boltzmann distribution is a [[probability distribution]] that gives the probability of a certain state as a function of that state's energy and  temperature of the [[system]] to which the distribution is applied.&amp;lt;ref name=&amp;quot;McQuarrie, A. 2000&amp;quot;&amp;gt;McQuarrie, A. (2000) Statistical Mechanics, University Science Books, California&amp;lt;/ref&amp;gt; It is given as&lt;br /&gt;
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:&amp;lt;math&amp;gt;&lt;br /&gt;
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p_i=\frac{1}{Q}} {e^{- {\varepsilon}_i / k T}=\frac{e^{- {\varepsilon}_i / k T}}{\sum_{j=1}^{M}{e^{- {\varepsilon}_j / k T}}}&lt;br /&gt;
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P _ i = frac {1}{ q }{ e ^ {-{ varepsilon } _ i/k t } = frac { e ^ {-{ varepsilon } _ i/k t }{ sum { j = 1} ^ { m }{ e ^ {-{ varepsilon } _ j/k t }}}}}&lt;br /&gt;
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p_i=\frac{1}{Q}} {e^{- {\varepsilon}_i / k T}=\frac{e^{- {\varepsilon}_i / k T}}{\sum_{j=1}^{M}{e^{- {\varepsilon}_j / k T}}}&lt;br /&gt;
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&amp;lt;/math&amp;gt;&lt;br /&gt;
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&amp;lt;/math&amp;gt;&lt;br /&gt;
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where p&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt; is the probability of state i, ε&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt; the energy of state i, k the Boltzmann constant, T the temperature of the system and M is the number of all states accessible to the system of interest.&lt;br /&gt;
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其中 p &amp;lt; sub &amp;gt; i  是状态 i 的概率，ε &amp;lt; sub &amp;gt; i  是状态 i 的能量，k 是波兹曼常数，t 是系统的温度，m 是感兴趣的系统所能到达的所有状态的数目。&lt;br /&gt;
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where ''p&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;'' is the probability of state ''i'', ''ε&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;'' the energy of state ''i'', ''k'' the Boltzmann constant, ''T'' the temperature of the system and ''M'' is the number of all states accessible to the system of interest.&amp;lt;ref name=&amp;quot;McQuarrie, A. 2000&amp;quot;/&amp;gt;&amp;lt;ref name=&amp;quot;Atkins, P. W. 2010&amp;quot;/&amp;gt; Implied parentheses around the denominator ''kT'' are omitted for brevity. The normalization denominator ''Q'' (denoted by some authors by ''Z'') is the [[canonical partition function]]&lt;br /&gt;
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The distribution shows that states with lower energy will always have a higher probability of being occupied than the states with higher energy. It can also give us the quantitative relationship between the probabilities of the two states being occupied. The ratio of probabilities for states i and j is given as&lt;br /&gt;
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分布表明，能量较低的状态被占据的概率总是高于能量较高的状态。它还可以给出两个状态被占领概率之间的定量关系。给出了状态 i 和状态 j 的概率比为&lt;br /&gt;
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:&amp;lt;math&amp;gt;&lt;br /&gt;
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Q={\sum_{i=1}^{M}{e^{- {\varepsilon}_i / k T}}}&lt;br /&gt;
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{\frac{p_i}{p_j}}=e^{({\varepsilon}_j-{\varepsilon}_i) / k T}&lt;br /&gt;
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{ frac { p _ i }{ p _ j } = e ^ {({ varepsilon } _ j-{ varepsilon } _ i)/k t }&lt;br /&gt;
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It results from the constraint that the probabilities of all accessible states must add up to 1.&lt;br /&gt;
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where p&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt; is the probability of state i,  p&amp;lt;sub&amp;gt;j&amp;lt;/sub&amp;gt; the probability of state j, and ε&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt; and ε&amp;lt;sub&amp;gt;j&amp;lt;/sub&amp;gt; are the energies of states i and j, respectively.&lt;br /&gt;
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其中 p &amp;lt; sub &amp;gt; i  是状态 i 的概率，p &amp;lt; sub &amp;gt; j  状态 j 的概率，ε  i  和 ε  j  分别是状态 i 和 j 的能量。&lt;br /&gt;
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The Boltzmann distribution is the distribution that maximizes the [[entropy]]&lt;br /&gt;
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The Boltzmann distribution is often used to describe the distribution of particles, such as atoms or molecules, over energy states accessible to them. If we have a system consisting of many particles, the probability of a particle being in state i is practically the probability that, if we pick a random particle from that system and check what state it is in, we will find it is in state i. This probability is equal to the number of particles in state i divided by the total number of particles in the system, that is the fraction of particles that occupy state i.&lt;br /&gt;
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波兹曼分布通常被用来描述粒子，比如原子或分子，在能量状态上的分布情况。如果我们有一个由许多粒子组成的系统，粒子处于状态 i 的概率实际上等于，如果我们从该系统中选择一个随机粒子并检查它处于什么状态，我们会发现它处于状态 i 的概率。这个概率等于状态 i 的粒子数除以系统中粒子的总数，即占据状态 i 的粒子的比例。&lt;br /&gt;
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:&amp;lt;math&amp;gt;H(p_1,p_2,\cdots,p_M) = -\sum_{i=1}^{M} p_i\log_2 p_i&amp;lt;/math&amp;gt;&lt;br /&gt;
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subject to the constraint that &amp;lt;math display=&amp;quot;inline&amp;quot;&amp;gt;&lt;br /&gt;
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p_i={\frac{N_i}{N}}&lt;br /&gt;
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P _ i = { frac { n _ i }{ n }&lt;br /&gt;
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{\sum{p_i {\varepsilon}_i}}&lt;br /&gt;
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&amp;lt;/math&amp;gt; equals a particular mean energy value (which can be proven using [[Lagrange multipliers]]).&lt;br /&gt;
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&lt;br /&gt;
where N&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt; is the number of particles in state i and N is the total number of particles in the system. We may use the Boltzmann distribution to find this probability that is, as we have seen, equal to the fraction of particles that are in state i. So the equation that gives the fraction of particles in state i as a function of the energy of that state is   In order for this to be possible, there must be some particles in the first state to undergo the transition. We may find that this condition is fulfilled by finding the fraction of particles in the first state. If it is negligible, the transition is very likely not to be observed at the temperature for which the calculation was done. In general, a larger fraction of molecules in the first state means a higher number of transitions to the second state. This gives a stronger spectral line. However, there are other factors that influence the intensity of a spectral line, such as whether it is caused by an allowed or a forbidden transition.&lt;br /&gt;
&lt;br /&gt;
其中 n &amp;lt; sub &amp;gt; i  是状态 i 的粒子数，n 是系统中粒子的总数。我们可以用波兹曼分布来求出这个概率，就像我们看到的那样，等于处于 i 状态的粒子的比例。所以给出状态 i 的粒子比例，作为状态能量的函数的方程是，为了使这成为可能，必须有一些粒子处于第一个状态，才能发生跃迁。我们可以通过求第一态粒子的比例来满足这个条件。如果它可以忽略不计，那么在进行计算的温度下，极有可能不能观察到这种转变。一般来说，处于第一状态的分子比例越大，意味着向第二状态转变的次数越多。这就产生了一条更强的谱线。然而，还有其他因素影响谱线的强度，例如它是由允许的跃迁还是禁止的跃迁引起的。&lt;br /&gt;
&lt;br /&gt;
The partition function can be calculated if we know the energies of the states accessible to the system of interest. For atoms the partition function values can be found in the NIST Atomic Spectra Database.&amp;lt;ref&amp;gt;[http://physics.nist.gov/PhysRefData/ASD/levels_form.html NIST Atomic Spectra Database Levels Form] at nist.gov&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The Boltzmann distribution is related to the softmax function commonly used in machine learning.&lt;br /&gt;
&lt;br /&gt;
波兹曼分布学习与机器学习中常用的柔性最大激活函数学习有关。&lt;br /&gt;
&lt;br /&gt;
The distribution shows that states with lower energy will always have a higher probability of being occupied than the states with higher energy. It can also give us the quantitative relationship between the probabilities of the two states being occupied. The ratio of probabilities for states ''i'' and ''j'' is given as&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
{\frac{p_i}{p_j}}=e^{({\varepsilon}_j-{\varepsilon}_i) / k T}&lt;br /&gt;
&lt;br /&gt;
&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
The Boltzmann distribution appears in statistical mechanics when considering isolated (or nearly-isolated) systems of fixed composition that are in thermal equilibrium (equilibrium with respect to energy exchange). The most general case is the probability distribution for the canonical ensemble, but also some special cases (derivable from the canonical ensemble) also show the Boltzmann distribution in different aspects:&lt;br /&gt;
&lt;br /&gt;
当考虑孤立的(或者几乎孤立的)固定组成的体系处于平衡状态时，波兹曼分布出现在《统计力学热平衡。最普遍的情况是概率分布的正则系综，但也有一些特殊的情况(从正则系综衍生)也显示了波兹曼分布在不同的方面:&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
where ''p&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;'' is the probability of state ''i'',  ''p&amp;lt;sub&amp;gt;j&amp;lt;/sub&amp;gt;'' the probability of state ''j'', and ''ε&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;'' and ''ε&amp;lt;sub&amp;gt;j&amp;lt;/sub&amp;gt;'' are the energies of states ''i'' and ''j'', respectively.&lt;br /&gt;
&lt;br /&gt;
 Canonical ensemble (general case)&lt;br /&gt;
&lt;br /&gt;
正则系综(一般情况)&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
 The canonical ensemble gives the probabilities of the various possible states of a closed system of fixed volume, in thermal equilibrium with a heat bath. The canonical ensemble is a probability distribution with the Boltzmann form.&lt;br /&gt;
&lt;br /&gt;
正则系综模型给出了一个封闭的固定体积系统的各种可能状态的概率，这个封闭体积系统包括一个带有热浴的热平衡。正则系综是一个玻尔兹曼概率分布。&lt;br /&gt;
&lt;br /&gt;
The Boltzmann distribution is often used to describe the distribution of particles, such as atoms or molecules, over energy states accessible to them. If we have a system consisting of many particles, the probability of a particle being in state ''i'' is practically the probability that, if we pick a random particle from that system and check what state it is in, we will find it is in state ''i''. This probability is equal to the number of particles in state ''i'' divided by the total number of particles in the system, that is the fraction of particles that occupy state ''i''.&lt;br /&gt;
&lt;br /&gt;
 Statistical frequencies of subsystems' states (in a non-interacting collection)&lt;br /&gt;
&lt;br /&gt;
子系统状态的统计频率(在一个无交互的集合中)&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
 When the system of interest is a collection of many non-interacting copies of a smaller subsystem, it is sometimes useful to find the statistical frequency of a given subsystem state, among the collection. The canonical ensemble has the property of separability when applied to such a collection: as long as the non-interacting subsystems have fixed composition, then each subsystem's state is independent of the others and is also characterized by a canonical ensemble. As a result, the expected statistical frequency distribution of subsystem states has the Boltzmann form.&lt;br /&gt;
&lt;br /&gt;
当感兴趣的系统是一个较小子系统的许多非交互副本的集合时，在集合中查找给定子系统状态的统计频率有时是有用的。当应用于这样一个集合时，正则系综子系统具有可分离性: 只要不相互作用的子系统的组成是固定的，那么每个子系统的状态是独立于其他子系统的，也是一个拥有属性正则系综。因此，子系统状态的期望统计频率分布具有玻耳兹曼形式。&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
 Maxwell–Boltzmann statistics of classical gases (systems of non-interacting particles)&lt;br /&gt;
&lt;br /&gt;
经典气体(非相互作用粒子系统)的 Maxwell-Boltzmann 统计&lt;br /&gt;
&lt;br /&gt;
p_i={\frac{N_i}{N}}&lt;br /&gt;
&lt;br /&gt;
 In particle systems, many particles share the same space and regularly change places with each other; the single-particle state space they occupy is a shared space. Maxwell–Boltzmann statistics give the expected number of particles found in a given single-particle state, in a classical gas of non-interacting particles at equilibrium. This expected number distribution has the Boltzmann form.&lt;br /&gt;
&lt;br /&gt;
在粒子系统中，许多粒子共享同一空间，并且相互之间有规律地改变位置; 它们所占据的单粒子状态空间是一个共享空间。麦克斯韦-玻尔兹曼统计给出了在一个给定的单粒子态，在一个处于平衡状态的非相互作用粒子的经典气体中所发现的粒子的预期数量。这个预期的数分布具有玻耳兹曼形式。&lt;br /&gt;
&lt;br /&gt;
&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Although these cases have strong similarities, it is helpful to distinguish them as they generalize in different ways when the crucial assumptions are changed:&lt;br /&gt;
&lt;br /&gt;
虽然这些案例有很多相似之处，但是当关键假设发生变化时，它们以不同的方式进行归纳，因此区分它们是有帮助的:&lt;br /&gt;
&lt;br /&gt;
where ''N&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;'' is the number of particles in state ''i'' and ''N'' is the total number of particles in the system. We may use the Boltzmann distribution to find this probability that is, as we have seen, equal to the fraction of particles that are in state i. So the equation that gives the fraction of particles in state ''i'' as a function of the energy of that state is  &amp;lt;ref name=&amp;quot;Atkins, P. W. 2010&amp;quot;/&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
{\frac{N_i}{N}}={\frac{e^{- {\varepsilon}_i / k T}}{\sum_{j=1}^{M}{e^{- {\varepsilon}_j / k T}}}}&lt;br /&gt;
&lt;br /&gt;
&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
This equation is of great importance to [[spectroscopy]]. In spectroscopy we observe a [[spectral line]] of atoms or molecules that we are interested in going from one state to another.&amp;lt;ref name=&amp;quot;Atkins, P. W. 2010&amp;quot;/&amp;gt;&amp;lt;ref&amp;gt;Atkins, P. W.; de Paula J. (2009) Physical Chemistry, 9th edition, Oxford University Press, Oxford, UK&amp;lt;/ref&amp;gt; In order for this to be possible, there must be some particles in the first state to undergo the transition. We may find that this condition is fulfilled by finding the fraction of particles in the first state. If it is negligible, the transition is very likely not to be observed at the temperature for which the calculation was done. In general, a larger fraction of molecules in the first state means a higher number of transitions to the second state.&amp;lt;ref&amp;gt;Skoog, D. A.; Holler, F. J.; Crouch, S. R. (2006) Principles of Instrumental Analysis, Brooks/Cole, Boston, MA&amp;lt;/ref&amp;gt; This gives a stronger spectral line. However, there are other factors that influence the intensity of a spectral line, such as whether it is caused by an allowed or a [[forbidden transition]].&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The Boltzmann distribution is related to the [[softmax function]] commonly used in machine learning.&lt;br /&gt;
&lt;br /&gt;
In more general mathematical settings, the Boltzmann distribution is also known as the Gibbs measure. In statistics and machine learning, it is called a log-linear model. In deep learning, the Boltzmann distribution is used in the sampling distribution of stochastic neural networks such as the Boltzmann machine, Restricted Boltzmann machine, Energy-Based models and deep Boltzmann machine.&lt;br /&gt;
&lt;br /&gt;
在更一般的数学环境中，波兹曼分布也被称为吉布斯量度。在统计学和机器学习中，它被称为对数线性回归。在深度学习中，波兹曼分布被用于随机神经网络的抽样分布，如波茨曼机、受限玻尔兹曼机、基于能量的模型和深度波茨曼机。&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
== In statistical mechanics ==&lt;br /&gt;
&lt;br /&gt;
{{main|Canonical ensemble|Maxwell–Boltzmann statistics}}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The Boltzmann distribution can be introduced to allocate permits in emissions trading. The new allocation method using the Boltzmann distribution can describe the most probable, natural, and unbiased distribution of emissions permits among multiple countries. Simple and versatile, this new method holds potential for many economic and environmental applications.&lt;br /&gt;
&lt;br /&gt;
可以引入欧盟波兹曼分布来分配排放交易的许可。这种新的排放量分配方法使用波兹曼分布能够描述多个国家之间最可能、最自然和最无偏见的排放量分配。这种新方法简单而通用，具有许多经济和环境应用的潜力。&lt;br /&gt;
&lt;br /&gt;
The Boltzmann distribution appears in [[statistical mechanics]] when considering isolated (or nearly-isolated) systems of fixed composition that are in [[thermal equilibrium]] (equilibrium with respect to energy exchange). The most general case is the probability distribution for the canonical ensemble, but also some special cases (derivable from the canonical ensemble) also show the Boltzmann distribution in different aspects:&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The Boltzmann distribution has the same form as the multinomial logit model. As a discrete choice model, this is very well known in economics since Daniel McFadden made the connection to random utility maximization.&lt;br /&gt;
&lt;br /&gt;
波兹曼分布与多项式 logit 模型具有相同的形式。作为一个离散选择模型，这在经济学中非常著名，因为丹尼尔 · 麦克法登提出了随机效用最大化的联系。&lt;br /&gt;
&lt;br /&gt;
; [[Canonical ensemble]] (general case)&lt;br /&gt;
&lt;br /&gt;
: The [[canonical ensemble]] gives the [[probabilities]] of the various possible states of a closed system of fixed volume, in thermal equilibrium with a [[heat bath]]. The canonical ensemble is a probability distribution with the Boltzmann form.&lt;br /&gt;
&lt;br /&gt;
; Statistical frequencies of subsystems' states (in a non-interacting collection)&lt;br /&gt;
&lt;br /&gt;
: When the system of interest is a collection of many non-interacting copies of a smaller subsystem, it is sometimes useful to find the [[statistical frequency]] of a given subsystem state, among the collection. The canonical ensemble has the property of separability when applied to such a collection: as long as the non-interacting subsystems have fixed composition, then each subsystem's state is independent of the others and is also characterized by a canonical ensemble. As a result, the [[expectation value|expected]] statistical frequency distribution of subsystem states has the Boltzmann form.&lt;br /&gt;
&lt;br /&gt;
; [[Maxwell–Boltzmann statistics]] of classical gases (systems of non-interacting particles)&lt;br /&gt;
&lt;br /&gt;
: In particle systems, many particles share the same space and regularly change places with each other; the single-particle state space they occupy is a shared space. [[Maxwell–Boltzmann statistics]] give the expected number of particles found in a given single-particle state, in a [[classical mechanics|classical]] gas of non-interacting particles at equilibrium. This expected number distribution has the Boltzmann form.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Although these cases have strong similarities, it is helpful to distinguish them as they generalize in different ways when the crucial assumptions are changed:&lt;br /&gt;
&lt;br /&gt;
* When a system is in thermodynamic equilibrium with respect to both energy exchange ''and particle exchange'', the requirement of fixed composition is relaxed and a [[grand canonical ensemble]] is obtained rather than canonical ensemble. On the other hand, if both composition and energy are fixed, then a [[microcanonical ensemble]] applies instead.&lt;br /&gt;
&lt;br /&gt;
* If the subsystems within a collection ''do'' interact with each other, then the expected frequencies of subsystem states no longer follow a Boltzmann distribution, and even may not have an [[analytical solution]].&amp;lt;ref&amp;gt;A classic example of this is [[magnetic ordering]]. Systems of non-interacting [[spin (physics)|spins]] show [[paramagnetic]] behaviour that can be understood with a single-particle canonical ensemble (resulting in the [[Brillouin function]]). Systems of ''interacting'' spins can show much more complex behaviour such as [[ferromagnetism]] or [[antiferromagnetism]].&amp;lt;/ref&amp;gt; The canonical ensemble can however still be applied to the ''collective'' states of the entire system considered as a whole, provided the entire system is isolated and in thermal equilibrium.&lt;br /&gt;
&lt;br /&gt;
* With ''[[quantum mechanics|quantum]]'' gases of non-interacting particles in equilibrium, the number of particles found in a given single-particle state does not follow Maxwell–Boltzmann statistics, and there is no simple closed form expression for quantum gases in the canonical ensemble. In the grand canonical ensemble the state-filling statistics of quantum gases are described by [[Fermi–Dirac statistics]] or [[Bose–Einstein statistics]], depending on whether the particles are [[fermion]]s or [[boson]]s respectively.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
|year=1868&lt;br /&gt;
&lt;br /&gt;
1868年&lt;br /&gt;
&lt;br /&gt;
== In mathematics ==&lt;br /&gt;
&lt;br /&gt;
|title=Studien über das Gleichgewicht der lebendigen Kraft zwischen bewegten materiellen Punkten&lt;br /&gt;
&lt;br /&gt;
|title=Studien über das Gleichgewicht der lebendigen Kraft zwischen bewegten materiellen Punkten&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
|trans-title=Studies on the balance of living force between moving material points&lt;br /&gt;
&lt;br /&gt;
| 反题 = 移动物质点之间生命力平衡的研究&lt;br /&gt;
&lt;br /&gt;
{{main|Gibbs measure|Log-linear model|Boltzmann machine}}&lt;br /&gt;
&lt;br /&gt;
|journal=Wiener Berichte |volume=58 |pages=517–560&lt;br /&gt;
&lt;br /&gt;
| journal = Wiener Berichte | volume = 58 | pages = 517-560&lt;br /&gt;
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}}&lt;br /&gt;
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}}&lt;br /&gt;
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In more general mathematical settings, the Boltzmann distribution is also known as the [[Gibbs measure]]. In statistics and machine learning, it is called a [[log-linear model]]. In [[deep learning]], the Boltzmann distribution is used in the sampling distribution of [[stochastic neural network]]s such as the [[Boltzmann machine]], [[Restricted Boltzmann machine]], [[Energy based model|Energy-Based models]] and [[Deep Boltzmann Machine|deep Boltzmann machine]].&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
|first=Josiah Willard |last=Gibbs |authorlink=Josiah Willard Gibbs&lt;br /&gt;
&lt;br /&gt;
2012年10月15日 | 约西亚·威拉德·吉布斯&lt;br /&gt;
&lt;br /&gt;
== In economics ==&lt;br /&gt;
&lt;br /&gt;
|year=1902&lt;br /&gt;
&lt;br /&gt;
1902年&lt;br /&gt;
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&lt;br /&gt;
&lt;br /&gt;
|title=Elementary Principles in Statistical Mechanics&lt;br /&gt;
&lt;br /&gt;
统计力学的基本原理&lt;br /&gt;
&lt;br /&gt;
The Boltzmann distribution can be introduced to allocate permits in emissions trading.&amp;lt;ref name=&amp;quot;Park, J.-W. 2012&amp;quot;&amp;gt;Park, J.-W., Kim, C. U. and Isard, W. (2012) Permit allocation in emissions trading using the Boltzmann distribution. Physica A 391: 4883–4890&amp;lt;/ref&amp;gt;&amp;lt;ref&amp;gt;[http://www.technologyreview.com/view/425051/the-thorny-problem-of-fair-allocation/ The Thorny Problem Of Fair Allocation]. ''Technology Review'' blog. August 17, 2011. Cites and summarizes Park, Kim and Isard (2012).&amp;lt;/ref&amp;gt; The new allocation method using the Boltzmann distribution can describe the most probable, natural, and unbiased distribution of emissions permits among multiple countries. Simple and versatile, this new method holds potential for many economic and environmental applications.&lt;br /&gt;
&lt;br /&gt;
|title-link=Elementary Principles in Statistical Mechanics }}&lt;br /&gt;
&lt;br /&gt;
| title-link = 基本原理统计力学}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The Boltzmann distribution has the same form as the [[Multinomial logistic regression|multinomial logit]] model. As a [[discrete choice]] model, this is very well known in economics since [[Daniel McFadden]] made the connection to random utility maximization.&lt;br /&gt;
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Category:Statistical mechanics&lt;br /&gt;
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类别: 统计力学&lt;br /&gt;
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==See also==&lt;br /&gt;
&lt;br /&gt;
Distribution&lt;br /&gt;
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分布&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:Boltzmann distribution]]. Its edit history can be viewed at [[玻尔兹曼分布/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>Tueryeye</name></author>
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