Helmholtz energy function: Difference between revisions

From SklogWiki
Jump to navigation Jump to search
No edit summary
No edit summary
Line 25: Line 25:


:<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):

A=U−TS

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

dA=dU−TdS−SdT

From the second law of thermodynamics one obtains

dA=TdS−pdV−TdS−SdT

thus one arrives at

dA=−pdV−SdT.

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

dA=(∂A∂T)VdT+(∂A∂V)TdV

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

A=−kBTlnQNVT

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

See also