Helmholtz Free Energy

    Define the Helmholtz free energy as
 
 
F = U - t s
(6.1)

If the system is in contact with a reservoir, F will be a minimum when the two systems are in equilibrium. To see this, consider an infintesimal transfer of energy from the system to the reservoir at constant temperature. Then
 


dF = dU - t ds


But, by definition, formula, so we see that dU = t ds. Thus, dF = 0, which is the condition of an extremum. To show this is a minimum, recall that since the total energy of the combined system is U = UR + US, the entropy of the combined system is
 


formula


Now recall that the system is in its most probable configuration at equilibrium. This means that the entropy of the combined system is maximized. This can only be true of FS is a minimum at equilibrium.
    Consider an infinitesimal change in F
 


dF = dU - t ds - s dt


From the thermodynamic identity found earlier, we see that dU - t ds = -p dV, so this becomes
 


dF = -p dV - sdt


but in general,
 


formula


so we get the identifications
 
 

formula
and
formula
(6.2)

 

Maxwell Relations

    Now consider the second derivatives formula andformula. We know that they must be equal to each other. Substituting the equalities in (6.2), we get the relation
 
 
formula
(6.3)

This is the first of what are known as Maxwell relations. We will derive more later in the course.
    Since we have stated that the partition function is extremely important and is used to derive many of the macroscopic properties of the system, we would like to recast the Helmholtz free energy as a function of Z. Start with the definition of F
 


F = U - t s


From (6.2) we saw that formula so this becomes a differential equation,
 


formula


Dividing through by t, we see that this is equivalent to
 
 

formula
(6.4)

Recall that U is the average energy of the system, <eS>, and that after defining the partition function we showed that
 


formula


Substituting this for U, we get
 


formula


or
 


F = -t ln Z + t A(V)


We can evaluate the volume dependent function by noting that as t ® 0, the entropy must reduce to ln g0, where g0 are the states at the lowest energy e0. In this limit the energy of all the states reduces to e0 and formula. Thus, formula. So the entropy becomes
 


formula


But this can be ln g0 only if A(V) = 0. Thus
 
 

F = -t ln Z
(6.5)

We can rearrage (6.5) to get Z as a function of F. This yields
 


Z = e-F/t


Substituting this into the definition of the probability of the system being in any quantum state associated with energy es, we get
 
 

formula
(6.6)