Grand canonical ensemble: Difference between revisions
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| 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 == | ||
| The  corresponding thermodynamic potential, the '''grand potential''', <math>\Omega</math>, | |||
| for the aforementioned grand canonical partition function is: | |||
| The  corresponding thermodynamic  | |||
| : <math> \Omega = \left. A - \mu N \right. </math>,  | |||
| where ''A'' is the [[Helmholtz energy function]]. | |||
| Using the relation  | |||
| :<math>\left.U\right.=TS -pV + \mu N</math> | |||
| one arrives at  | |||
| : <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