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               Chapter 4                 where we defined the functions M and N as
               Material Equilibrium
                                                               M   10z>0x2 ,   N   10z>0y2 x                (4.41)
                                                                          y
                                         From Eq. (1.36), the order of partial differentiation does not matter:

                                                                     0  0z     0   0z
                                                                       a  b      a   b                      (4.42)
                                                                    0y 0x      0x 0y
                                         Hence Eqs. (4.40) to (4.42) give
                                                           0M        0N
                                                          a   b   a     b     if  dz   M dx   N dy         (4.43)*
                                                            0y  x    0x  y
                                         Equation (4.43) is the Euler reciprocity relation. Since M appears in front of dx in the
                                         expression for dz, M is (
z/
x) and since we want to equate the mixed second partial
                                                                   y
                                         derivatives, we take (
M/
y) .
                                                                 x
                                         The Maxwell Relations
                                         The Gibbs equation (4.33) for dU is

                                             dU   T dS   P dV   M dx   N dy  where M   T, N    P, x   S, y   V

                                         The Euler relation (
M/
y)   (
N/
x) gives
                                                                          y
                                                                x
                                                            10T>0V2   301 P2>0S4   10P>0S2   V
                                                                                 V
                                                                   S
                                         Application of the Euler relation to the other three Gibbs equations gives three more
                                         thermodynamic relations. We find (Prob. 4.5)
                                                           0T         0P          0T       0V
                                                          a   b    a     b ,   a    b   a    b              (4.44)
                                                           0V  S      0S  V      0P  S     0S  P
                                                           0S        0P           0S         0V
                                                          a   b   a    b ,      a   b    a     b            (4.45)
                                                           0V  T     0T  V       0P  T       0T  P
                                         These are the Maxwell relations (after James Clerk Maxwell, one of the greatest of
                                         nineteenth-century physicists). The first two Maxwell relations are little used. The last
                                         two are extremely valuable, since they relate the isothermal pressure and volume vari-
                                         ations of entropy to measurable properties.
                                             The equations in (4.45) are examples of the powerful and remarkable relationships
                                         that thermodynamics gives us. Suppose we want to know the effect of an isothermal
                                         pressure change on the entropy of a system. We cannot check out an entropy meter
                                         from the stockroom to monitor  S as P changes. However, the relation (
S/
P)
                                                                                                              T
                                          (
V/
T) in (4.45) tells us that all we have to do is measure the rate of change of the
                                                  P
                                         system’s volume with temperature at constant P, and this simple measurement enables
                                         us to calculate the rate of change of the system’s entropy with respect to pressure at
                                         constant T.

                                         Dependence of State Functions on T, P, and V
                                         We now find the dependence of U, H, S, and G on the variables of the system. The most
                                         common independent variables are T and P. We shall relate the temperature and pres-
                                         sure variations of H, S, and G to the directly measurable properties C , a, and k. For U,
                                                                                                  P
                                         the quantity (
U/
V) occurs more often than (
U/
P) , so we shall find the tempera-
                                                                                       T
                                                           T
                                         ture and volume variations of U.
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