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2.6 Thermodynamic Potentials for a Single-Phase Systems with One Species   31


         U[7; P] = G = - RTln A,  where  A  is  the  isothermal-isobaric partition function;
         and  U[7;p] = -RTlnE,  where  E is  the  grand  canonical  ensemble  partition
         function. When a system involves several species, but  only  one can pass through
         a  membrane  to  a  reservoir,  U(T,pl] = -RTlnY,  where  Y  is  the  semigrand
         ensemble partition function. The last chapter of the book is on semigrand partition
         functions.
             Taking the differentials of the seven thermodynamic potentials defined above
         and substituting equation 2.6-1 yields the fundamental equations for these seven
         additional thermodynamic potentials:
                                   dH = TdS + VdP + pdn                  (2.6-7)

                                   dA = -SdT-  PdV+ pdn                  (2.6-8)
                                   dG = -SdT+  VdP + pdn                 (2.6-9)
                                dU[p]  = TdS - PdV-  ndp                (2.6-  1 0)

                              dU[P,p]  = TdS + VdP - ndp                (2.6-1 1)
                              dU[7;p]  = -SdT-  PdV-  ndp               (2.6-1 2)

                            dU[T,P,p]  = -SdT+  VdP-  ndp = 0           (2.6-  1 3)
         This last equation is the Gibbs-Duhem equation for the system, and it shows that
         only  two  of  the  three  intensive  properties  (7; P, and  p) are independent  for  a
         system containing one substance. Because of the Gibbs-Duhem equation, we can
         say  that  the  chemical  potential  of  a  pure  substance substance is  a  function  of
         temperature and  pressure.  The  number  F  of  independent  intensive  variables  is
         F  = 1 - 1 + 2 = 2,  and  so  D  = F + p  = 2 + 1 = 3.  Each  of  these  fundamental
         equations yields  D(D - 1)/2 = 3  Maxwell  equations,  and  there  are 24  Maxwell
         equations for the system.
             The integrated  forms of the eight fundamental equations for this system are
                                   U(S, vn) = TS - PV+ pn               (2.6-14)

                                  H(S, P, n) = TS + pn                  (2.6-15)
                                   A(7; vn) = -PV+  pn                  (2.6-16)

                                   G(7: P, n) = pn                      (2.6- 17)
                                U[p](S,  Kp) = TS ~  PV                 (2.6-18)
                             UCP, PI(S, p,   = TS                       (2.6-19)

                              WTpI(7; vp) = -PV                         (2.6-20)
                           u CT,P,PI(7; P,p) = 0                        (2.6-2 1)
         where the natural variables  are shown in parentheses.
             The basic question in all of thermodynamics is: A certain system is under such
         and such constraints, what is the equilibrium state that it can go to spontaneous-
         ly?  The  amazing  thing  is  that  this  question  can  be  answered  by  making
         macroscopic  measurements.  Thermodynamics does  not  deal  with  the  question
         as  to  how  long  it  will  take  to  reach  equilibrium.  We  now  have  seven  criteria
         for  equilibrium  in  a  one-phase  system  with  one  species  and  only  PV work.
         The  criteria  of  equilibrium  provided  by  these  thermodynamic  potentials  are
         (dU)s,",n d 0,  (dH)S,P,n  0,  (dA)T,",, d 0,  (dG)*,P,n d 0,  (d~CPl)s,v,fi d 0,
         (dWP, PI)S,P,@ d 0, and (d~CT,P1)T,v,fi d 0.
             The  reason  for  going  into  this  much  detail  on  all  of  the  thermodynamic
         potentials  that  can  be  defined  for  a  one-phase,  one-species  system  and  the
         corresponding criteria for spontaneous change is to illustrate the process by which
          these  thermodynamic potentials  are  defined  and  how  they  provide  criteria  for
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