Grand canonical ensemble: Difference between revisions
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The '''grand-canonical ensemble''' is particularly well suited to simulation studies of adsorption. | The '''grand-canonical ensemble''' is for "open" systems, where the number of particles, <math>N</math>, can change. It can be viewed as an ensemble of [[canonical ensemble]]s; there being a canonical ensemble for each value of <math>N</math>, and the (weighted) sum over <math>N</math> of these canonical ensembles constitutes the grand canonical ensemble. The weighting factor is <math> \exp \left[ \beta \mu \right]</math> and is known as the [[fugacity]]. | ||
The grand-canonical ensemble is particularly well suited to simulation studies of adsorption. | |||
== Ensemble variables == | == Ensemble variables == | ||
* [[chemical potential]], <math> \left. \mu \right. </math> | |||
* volume, <math> \left. V \right. </math> | |||
* [[temperature]], <math> \left. T \right. </math> | |||
== Grand canonical partition function == | |||
The grand canonical partition function for a one-component system in a three-dimensional space is given by: | |||
:<math> \Xi_{\mu VT} = \sum_{N=0}^{\infty} \exp \left[ \beta \mu N \right] Q_{NVT} </math> | |||
where <math>Q_{NVT}</math> represents the [[Canonical ensemble#Partition Function | canonical ensemble partition function]]. | |||
For example, for a ''classical'' system one has | |||
:<math> \Xi_{\mu VT} = \sum_{N=0}^{\infty} \exp \left[ \beta \mu N \right] \frac{ V^N}{N! \Lambda^{3N} } \int d (R^*)^{3N} \exp \left[ - \beta U \left( V, (R^*)^{3N} \right) \right] </math> | |||
where: | where: | ||
*<math> | * <math>N</math> is the number of particles | ||
* <math> \left. \Lambda \right. </math> is the [[de Broglie thermal wavelength]] (which depends on the temperature) | * <math> \left. \Lambda \right. </math> is the [[de Broglie thermal wavelength]] (which depends on the temperature) | ||
* <math> \beta </math> is the [[inverse temperature]] | |||
* <math> \beta | * <math>U</math> is the potential energy, which depends on the coordinates of the particles (and on the [[models | interaction model]]) | ||
* <math> | |||
* <math> \left( R^*\right)^{3N} </math> represent the <math>3N</math> position coordinates of the particles (reduced with the system size): i.e. <math> \int d (R^*)^{3N} = 1 </math> | * <math> \left( R^*\right)^{3N} </math> represent the <math>3N</math> position coordinates of the particles (reduced with the system size): i.e. <math> \int d (R^*)^{3N} = 1 </math> | ||
== Helmholtz energy and partition function == | == Helmholtz energy and partition function == | ||
The corresponding thermodynamic potential, the '''grand potential''', <math>\Omega</math>, | The corresponding thermodynamic potential, the '''grand potential''', <math>\Omega</math>, | ||
for the | for the aforementioned grand canonical partition function is: | ||
: <math> \Omega = \left. A - \mu N \right. </math>, | : <math> \Omega = \left. A - \mu N \right. </math>, | ||
where ''A'' is the [[Helmholtz energy function]]. | where ''A'' is the [[Helmholtz energy function]]. | ||
Using the relation | Using the relation | ||
:<math>\left.U\right.=TS - | :<math>\left.U\right.=TS -pV + \mu N</math> | ||
one arrives at | one arrives at | ||
: <math> \left. \Omega \right.= - | : <math> \left. \Omega \right.= -pV</math> | ||
i.e.: | i.e.: | ||
:<math> \left. p V = k_B T \ | :<math> \left. p V = k_B T \ln \Xi_{\mu V T } \right. </math> | ||
==See also== | |||
*[[Grand canonical Monte Carlo]] | |||
*[[Mass-stat]] | |||
==References== | |||
<references/> | |||
;Related reading | |||
*[http://dx.doi.org/10.1103/PhysRev.57.1160 Richard C. Tolman "On the Establishment of Grand Canonical Distributions", Physical Review '''57''' pp. 1160-1168 (1940)] | |||
[[Category:Statistical mechanics]] | [[Category:Statistical mechanics]] |
Latest revision as of 16:09, 1 April 2014
The grand-canonical ensemble is for "open" systems, where the number of particles, , can change. It can be viewed as an ensemble of canonical ensembles; there being a canonical ensemble for each value of , and the (weighted) sum over of these canonical ensembles constitutes the grand canonical ensemble. The weighting factor is and is known as the fugacity. The grand-canonical ensemble is particularly well suited to simulation studies of adsorption.
Ensemble variables[edit]
- chemical potential,
- volume,
- temperature,
Grand canonical partition function[edit]
The grand canonical partition function for a one-component system in a three-dimensional space is given by:
where represents the canonical ensemble partition function. For example, for a classical system one has
where:
- is the number of particles
- is the de Broglie thermal wavelength (which depends on the temperature)
- is the inverse temperature
- is the potential energy, which depends on the coordinates of the particles (and on the interaction model)
- represent the position coordinates of the particles (reduced with the system size): i.e.
Helmholtz energy and partition function[edit]
The corresponding thermodynamic potential, the grand potential, , for the aforementioned grand canonical partition function is:
- ,
where A is the Helmholtz energy function. Using the relation
one arrives at
i.e.:
See also[edit]
References[edit]
- Related reading