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	<title>Mean-field approximation and the Curie-Weiss model - 版本历史</title>
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		<title>思无涯咿呀咿呀：创建页面，内容为“ ==Naïve Mean-Field Approximation== For a general coupling distribution, the macroscopic observables associated with the Boltzmann distribution are usually hard to…”</title>
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		<summary type="html">&lt;p&gt;创建页面，内容为“ ==Naïve Mean-Field Approximation== For a general coupling distribution, the macroscopic observables associated with the Boltzmann distribution are usually hard to…”&lt;/p&gt;
&lt;p&gt;&lt;b&gt;新页面&lt;/b&gt;&lt;/p&gt;&lt;div&gt;&lt;br /&gt;
==Naïve Mean-Field Approximation==&lt;br /&gt;
For a general coupling distribution, the macroscopic observables associated with the Boltzmann distribution are usually hard to solve, thus we usually need approximations. The simplest mean-field approximation is called ''Naïve Mean-Field'' or ''Variational Mean-Field''. It also has a strong relation to the variational inference approaches, which will be shown later.&lt;br /&gt;
&lt;br /&gt;
First of all we see that once a configuration &amp;lt;math&amp;gt;\textstyle\underline\sigma^t&amp;lt;/math&amp;gt; is given, a spin ''i'' experiences a ''local field'' as&lt;br /&gt;
:&amp;lt;math&amp;gt; h_i=\sum_jJ_{ij}\sigma^t_j.&amp;lt;/math&amp;gt;&lt;br /&gt;
As in the Glauber dynamics, the expectation of value that spin ''i'' in the &amp;quot;next time&amp;quot; when we flip spin ''i'' is given by &lt;br /&gt;
:&amp;lt;math&amp;gt; m_i^{t+1}=\tanh(\beta\sum_iJ_{ij}\sigma_j^t).&amp;lt;/math&amp;gt;&lt;br /&gt;
Then a simple approximation says that let us forget the time indices, and replace the spin values by its mean, this results to the ''Naïve Mean-Field'' approximation:&lt;br /&gt;
:&amp;lt;math&amp;gt; m_i=\tanh(\beta\sum_iJ_{ij}m_j).&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
==Curie-Weiss model and the phase transition==&lt;br /&gt;
The Curie-Weiss model is the most simple model for ferromagnets, where &amp;lt;math&amp;gt;\textstyle J_{ij}=J/n&amp;lt;/math&amp;gt;, a constant, and system is fully connected.&lt;br /&gt;
&lt;br /&gt;
Without the external field (which is considered in the whole lecture) In the model there is a symmetry that for any configuration, flipping each spin to its opposite value does not alter the energy of the configuration, i.e.&lt;br /&gt;
:&amp;lt;math&amp;gt;E(\underline\sigma)=E(-\underline\sigma).&amp;lt;/math&amp;gt;&lt;br /&gt;
It means that the magnetization of each spin should be always zero, as marginal distribution for spin ''i'' has to satisfy &amp;lt;math&amp;gt;\textstyle p_i(\sigma_i)=-p_i(\sigma_i).&amp;lt;/math&amp;gt;&lt;br /&gt;
This is indeed the case at high temperature where &amp;lt;math&amp;gt;\textstyle \beta&amp;lt;/math&amp;gt; is small. This is called the ''Paramagnetic'' state. However at a low temperature we can not see this state, because of&lt;br /&gt;
the spontaneous symmetry breaking, at which point the paramagnetic state becomes unstable. We can show the phenomenon using the Naïve Mean-Field Approximation.&lt;br /&gt;
&lt;br /&gt;
Here the couplings are identical, the mean-field equation for the magnetization simply becomes&lt;br /&gt;
:&amp;lt;math&amp;gt;m=\tanh(\beta Jm).&amp;lt;/math&amp;gt; &lt;br /&gt;
The fixed-points of above equation can be shown in the following figure where &amp;lt;math&amp;gt;\beta J=0.2, 0.5, 1, 2, 20.&amp;lt;/math&amp;gt; &lt;br /&gt;
&lt;br /&gt;
[[File:CurrieWeiss.png|400px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[category:旧词条迁移]]&lt;/div&gt;</summary>
		<author><name>思无涯咿呀咿呀</name></author>
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