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		<id>http://www.sklogwiki.org/SklogWiki/index.php?title=Grand_canonical_ensemble&amp;diff=11704</id>
		<title>Grand canonical ensemble</title>
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		<updated>2011-08-30T10:08:43Z</updated>

		<summary type="html">&lt;p&gt;82.53.107.46: /* Grand canonical partition function */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;The &#039;&#039;&#039;grand-canonical ensemble&#039;&#039;&#039; is particularly well suited to simulation studies of adsorption. &lt;br /&gt;
== Ensemble variables ==&lt;br /&gt;
* [[Chemical potential]], &amp;lt;math&amp;gt; \left. \mu \right.  &amp;lt;/math&amp;gt;&lt;br /&gt;
* Volume, &amp;lt;math&amp;gt; \left. V  \right. &amp;lt;/math&amp;gt;&lt;br /&gt;
* [[Temperature]], &amp;lt;math&amp;gt; \left. T \right. &amp;lt;/math&amp;gt;&lt;br /&gt;
== Grand canonical partition function ==&lt;br /&gt;
The classical grand canonical partition function for a one-component system in a three-dimensional space is given by: &lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt; Q_{\mu VT} = \sum_{N=0}^{\infty} \frac{ \exp \left[ \beta \mu N \right]}{N! \Lambda^{3N} } \int  d (R^*)^{3N} \exp \left[ - \beta U \left( V, (R^*)^{3N} \right) \right] &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
where:&lt;br /&gt;
&lt;br /&gt;
* &#039;&#039;N&#039;&#039; is the number of particles&lt;br /&gt;
* &amp;lt;math&amp;gt; \left. \Lambda \right. &amp;lt;/math&amp;gt; is the [[de Broglie thermal wavelength]] (which depends on the temperature)&lt;br /&gt;
* &amp;lt;math&amp;gt; \beta = \frac{1}{k_B T} &amp;lt;/math&amp;gt;, with &amp;lt;math&amp;gt; k_B &amp;lt;/math&amp;gt; being the [[Boltzmann constant]]&lt;br /&gt;
* &#039;&#039;U&#039;&#039; is the potential energy, which depends on the coordinates of the particles (and on the [[models | interaction model]])&lt;br /&gt;
* &amp;lt;math&amp;gt; \left( R^*\right)^{3N} &amp;lt;/math&amp;gt; represent the &amp;lt;math&amp;gt;3N&amp;lt;/math&amp;gt; position coordinates of the particles (reduced with the system size): i.e. &amp;lt;math&amp;gt; \int d (R^*)^{3N} = 1 &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
== Helmholtz energy and partition function ==&lt;br /&gt;
The  corresponding thermodynamic potential, the &#039;&#039;&#039;grand potential&#039;&#039;&#039;, &amp;lt;math&amp;gt;\Omega&amp;lt;/math&amp;gt;,&lt;br /&gt;
for the aforementioned grand canonical partition function is:&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt; \Omega = \left. A - \mu N \right. &amp;lt;/math&amp;gt;, &lt;br /&gt;
where &#039;&#039;A&#039;&#039; is the [[Helmholtz energy function]].&lt;br /&gt;
Using the relation &lt;br /&gt;
:&amp;lt;math&amp;gt;\left.U\right.=TS -PV + \mu N&amp;lt;/math&amp;gt;&lt;br /&gt;
one arrives at &lt;br /&gt;
: &amp;lt;math&amp;gt; \left. \Omega \right.= -PV&amp;lt;/math&amp;gt;&lt;br /&gt;
i.e.:&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt; \left. p V = k_B T \log Q_{\mu V T } \right. &amp;lt;/math&amp;gt;&lt;br /&gt;
==See also==&lt;br /&gt;
*[[Monte Carlo in the grand-canonical ensemble]]&lt;br /&gt;
==References==&lt;br /&gt;
#[http://dx.doi.org/10.1103/PhysRev.57.1160 Richard C. Tolman &amp;quot;On the Establishment of Grand Canonical Distributions&amp;quot;, Physical Review &#039;&#039;&#039;57&#039;&#039;&#039; pp. 1160-1168 (1940)]&lt;br /&gt;
[[Category:Statistical mechanics]]&lt;/div&gt;</summary>
		<author><name>82.53.107.46</name></author>
	</entry>
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