Free_entropy Knowpia

A thermodynamic free entropy is an entropic thermodynamic potential analogous to the free energy. Also known as a Massieu, Planck, or Massieu–Planck potentials (or functions), or (rarely) free information. In statistical mechanics, free entropies frequently appear as the logarithm of a partition function. The Onsager reciprocal relations in particular, are developed in terms of entropic potentials. In mathematics, free entropy means something quite different: it is a generalization of entropy defined in the subject of free probability.

A free entropy is generated by a Legendre transformation of the entropy. The different potentials correspond to different constraints to which the system may be subjected.

Examples edit

The most common examples are:

Name	Function	Alt. function	Natural variables
Entropy	$S={\frac {1}{T}}U+{\frac {P}{T}}V-\sum _{i=1}^{s}{\frac {\mu _{i}}{T}}N_{i}\,$		$~~~~~U,V,\{N_{i}\}\,$
Massieu potential \ Helmholtz free entropy	$\Phi =S-{\frac {1}{T}}U$	$=-{\frac {A}{T}}$	$~~~~~{\frac {1}{T}},V,\{N_{i}\}\,$
Planck potential \ Gibbs free entropy	$\Xi =\Phi -{\frac {P}{T}}V$	$=-{\frac {G}{T}}$	$~~~~~{\frac {1}{T}},{\frac {P}{T}},\{N_{i}\}\,$

where

S

is entropy

\Phi

is the Massieu potential^[1]^[2]

\Xi

is the Planck potential^[1]

U

is internal energy

T

is temperature

P

is pressure

V

is volume

A

is Helmholtz free energy

G

is Gibbs free energy

N_{i}

is number of particles (or number of moles) composing the i-th chemical component

\mu _{i}

is the chemical potential of the i-th chemical component

s

is the total number of components

i

is the

i

^th components.

Note that the use of the terms "Massieu" and "Planck" for explicit Massieu-Planck potentials are somewhat obscure and ambiguous. In particular "Planck potential" has alternative meanings. The most standard notation for an entropic potential is $\psi$ , used by both Planck and Schrödinger. (Note that Gibbs used $\psi$ to denote the free energy.) Free entropies where invented by French engineer François Massieu in 1869, and actually predate Gibbs's free energy (1875).

Dependence of the potentials on the natural variables edit

Entropy edit

S=S(U,V,\{N_{i}\})

By the definition of a total differential,

dS={\frac {\partial S}{\partial U}}dU+{\frac {\partial S}{\partial V}}dV+\sum _{i=1}^{s}{\frac {\partial S}{\partial N_{i}}}dN_{i}.

From the equations of state,

dS={\frac {1}{T}}dU+{\frac {P}{T}}dV+\sum _{i=1}^{s}\left(-{\frac {\mu _{i}}{T}}\right)dN_{i}.

The differentials in the above equation are all of extensive variables, so they may be integrated to yield

S={\frac {U}{T}}+{\frac {PV}{T}}+\sum _{i=1}^{s}\left(-{\frac {\mu _{i}N}{T}}\right).

Massieu potential / Helmholtz free entropy edit

\Phi =S-{\frac {U}{T}}

\Phi ={\frac {U}{T}}+{\frac {PV}{T}}+\sum _{i=1}^{s}\left(-{\frac {\mu _{i}N}{T}}\right)-{\frac {U}{T}}

\Phi ={\frac {PV}{T}}+\sum _{i=1}^{s}\left(-{\frac {\mu _{i}N}{T}}\right)

Starting over at the definition of $\Phi$ and taking the total differential, we have via a Legendre transform (and the chain rule)

d\Phi =dS-{\frac {1}{T}}dU-Ud{\frac {1}{T}},

d\Phi ={\frac {1}{T}}dU+{\frac {P}{T}}dV+\sum _{i=1}^{s}\left(-{\frac {\mu _{i}}{T}}\right)dN_{i}-{\frac {1}{T}}dU-Ud{\frac {1}{T}},

d\Phi =-Ud{\frac {1}{T}}+{\frac {P}{T}}dV+\sum _{i=1}^{s}\left(-{\frac {\mu _{i}}{T}}\right)dN_{i}.

The above differentials are not all of extensive variables, so the equation may not be directly integrated. From $d\Phi$ we see that

\Phi =\Phi ({\frac {1}{T}},V,\{N_{i}\}).

If reciprocal variables are not desired,^[3]^: 222

d\Phi =dS-{\frac {TdU-UdT}{T^{2}}},

d\Phi =dS-{\frac {1}{T}}dU+{\frac {U}{T^{2}}}dT,

d\Phi ={\frac {1}{T}}dU+{\frac {P}{T}}dV+\sum _{i=1}^{s}\left(-{\frac {\mu _{i}}{T}}\right)dN_{i}-{\frac {1}{T}}dU+{\frac {U}{T^{2}}}dT,

d\Phi ={\frac {U}{T^{2}}}dT+{\frac {P}{T}}dV+\sum _{i=1}^{s}\left(-{\frac {\mu _{i}}{T}}\right)dN_{i},

\Phi =\Phi (T,V,\{N_{i}\}).

Planck potential / Gibbs free entropy edit

\Xi =\Phi -{\frac {PV}{T}}

\Xi ={\frac {PV}{T}}+\sum _{i=1}^{s}\left(-{\frac {\mu _{i}N}{T}}\right)-{\frac {PV}{T}}

\Xi =\sum _{i=1}^{s}\left(-{\frac {\mu _{i}N}{T}}\right)

Starting over at the definition of $\Xi$ and taking the total differential, we have via a Legendre transform (and the chain rule)

d\Xi =d\Phi -{\frac {P}{T}}dV-Vd{\frac {P}{T}}

d\Xi =-Ud{\frac {2}{T}}+{\frac {P}{T}}dV+\sum _{i=1}^{s}\left(-{\frac {\mu _{i}}{T}}\right)dN_{i}-{\frac {P}{T}}dV-Vd{\frac {P}{T}}

d\Xi =-Ud{\frac {1}{T}}-Vd{\frac {P}{T}}+\sum _{i=1}^{s}\left(-{\frac {\mu _{i}}{T}}\right)dN_{i}.

The above differentials are not all of extensive variables, so the equation may not be directly integrated. From $d\Xi$ we see that

\Xi =\Xi \left({\frac {1}{T}},{\frac {P}{T}},\{N_{i}\}\right).

If reciprocal variables are not desired,^[3]^: 222

d\Xi =d\Phi -{\frac {T(PdV+VdP)-PVdT}{T^{2}}},

d\Xi =d\Phi -{\frac {P}{T}}dV-{\frac {V}{T}}dP+{\frac {PV}{T^{2}}}dT,

d\Xi ={\frac {U}{T^{2}}}dT+{\frac {P}{T}}dV+\sum _{i=1}^{s}\left(-{\frac {\mu _{i}}{T}}\right)dN_{i}-{\frac {P}{T}}dV-{\frac {V}{T}}dP+{\frac {PV}{T^{2}}}dT,

d\Xi ={\frac {U+PV}{T^{2}}}dT-{\frac {V}{T}}dP+\sum _{i=1}^{s}\left(-{\frac {\mu _{i}}{T}}\right)dN_{i},

\Xi =\Xi (T,P,\{N_{i}\}).

References edit

^ ^a ^b Antoni Planes; Eduard Vives (2000-10-24). "Entropic variables and Massieu-Planck functions". Entropic Formulation of Statistical Mechanics. Universitat de Barcelona. Archived from the original on 2008-10-11. Retrieved 2007-09-18.
^ T. Wada; A.M. Scarfone (December 2004). "Connections between Tsallis' formalisms employing the standard linear average energy and ones employing the normalized q-average energy". Physics Letters A. 335 (5–6): 351–362. arXiv:cond-mat/0410527. Bibcode:2005PhLA..335..351W. doi:10.1016/j.physleta.2004.12.054. S2CID 17101164.
^ ^a ^b The Collected Papers of Peter J. W. Debye. New York, New York: Interscience Publishers, Inc. 1954.