Helmholtz energy function: Difference between revisions

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:<math>\left.A\right.=-k_B T \ln Q_{NVT}</math>
:<math>\left.A\right.=-k_B T \ln Q_{NVT}</math>
where <math>k_B</math> is the [[Boltzmann constant]], ''T'' is the [[temperature]], and <math>Q_{NVT}</math> is the [[Canonical ensemble | canonical ensemble partition function]].
==See also==
==See also==
*[[Canonical ensemble]]
*[[Canonical ensemble]]

Revision as of 11:46, 25 June 2007

Hermann Ludwig Ferdinand von Helmholtz Definition of A (for arbeit):

where U is the internal energy, T is the temperature and S is the entropy. (TS) is a conjugate pair. The differential of this function is

From the second law of thermodynamics one obtains

thus one arrives at

.

For A(T,V) one has the following total differential

The following equation provides a link between classical thermodynamics and statistical mechanics:

where is the Boltzmann constant, T is the temperature, and is the canonical ensemble partition function.

See also