Canonical ensemble: Difference between revisions

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* <math> \left( R^*\right)^{3N} </math> represent the 3N 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 3N position coordinates of the particles (reduced with the system size): i.e. <math> \int d (R^*)^{3N} = 1 </math>


== [[Free energy]] ==
== [[Free energy|Helmholtz energy function]] ==

Revision as of 20:49, 19 February 2007

Canonical Ensemble:

Variables:

  • Number of Particles,
  • Volume,
  • Temperature,

Partition Function

Classical Partition Function (one-component system) in a three-dimensional space:

where:

  • , with being the Boltzmann constant,
  • is the potential energy, which depends on the coordinates of the particles (and on the interaction model)
  • represent the 3N position coordinates of the particles (reduced with the system size): i.e.

Helmholtz energy function