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Statistical Mechanics - Physics at Oregon State University

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2.6. PROPERTIES OF THE HELMHOLTZ FREE ENERGY. 33<br />

function of U and U is an increasing function of T! The ability to switch back<br />

and forth between different sets of independent variables implies constant signs<br />

for certain deriv<strong>at</strong>ives, and for response functions. For example, a solid always<br />

expands as a function of temper<strong>at</strong>ure. In thermodynamics we rel<strong>at</strong>ed these<br />

properties in a rigorous way to criteria for stability.<br />

2.6 Properties of the Helmholtz free energy.<br />

For a system <strong>at</strong> constant temper<strong>at</strong>ure and volume, the Helmholtz free energy is<br />

the st<strong>at</strong>e function determining all physical properties of the system. For example,<br />

consider a system in thermal contact with a large reservoir <strong>at</strong> temper<strong>at</strong>ure<br />

T. The volume of the system is V. Energy can flow back and forth between<br />

the system and the reservoir; the energy of the system is ɛ and the energy of<br />

the combin<strong>at</strong>ion reservoir plus system is U0. In order to find the value of ɛ<br />

which corresponds to the equilibrium value for the system, i.e. which is equal<br />

to U(T,V), we have to maximize the entropy of the combin<strong>at</strong>ion system plus<br />

reservoir. Since<br />

Stot(ɛ) = SR(U0 − ɛ) + SS(ɛ) ≈ SR(U0) − 1<br />

T (ɛ − T SS(ɛ)) (2.39)<br />

this means we have to minimize ɛ − T SS(ɛ). In other words, if we specify the<br />

temper<strong>at</strong>ure and volume of a system, we can give the energy ɛ an arbitrary<br />

value, but th<strong>at</strong> value will in general not correspond to a system in equilibrium.<br />

The equilibrium value of ɛ is found by minimizing the Helmholtz free energy<br />

ɛ − T S(ɛ). This equilibrium value is called U. Very often, not<strong>at</strong>ion is sloppy<br />

and one tells you to minimize U − T S(U). The Helmholtz energies in st<strong>at</strong>istical<br />

mechanics and in thermodynamics therefore have identical properties, and again<br />

the st<strong>at</strong>istical mechanical and thermodynamical descriptions are the same.<br />

The pressure as a function of temper<strong>at</strong>ure and volume is rel<strong>at</strong>ed to the<br />

internal energy U and the entropy S by<br />

p(T, V ) = −<br />

∂U<br />

∂V<br />

<br />

T<br />

+ T<br />

<br />

∂S<br />

∂V T<br />

(2.40)<br />

Both terms can be important, although in general in a solid the first term is<br />

larger and in a gas the second. Beware, however, of the errors introduced by<br />

approxim<strong>at</strong>ing the pressure by only one of the terms in this expression.<br />

How are they rel<strong>at</strong>ed?<br />

In thermodynamics we have seen th<strong>at</strong> a system as a function of T and V (and<br />

N) is described by the Helmholtz energy F (T, V, N). In st<strong>at</strong>istical mechanics we<br />

needed the partition function Z(T, V, N). These two functions must therefore<br />

be rel<strong>at</strong>ed. It is possible to elimin<strong>at</strong>e S from the definition of the Helmholtz free<br />

energy F, since S = − <br />

∂F<br />

∂T . This gives<br />

V,N

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