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 10:46, 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.