Page 229 - Physical chemistry understanding our chemical world
P. 229

196    PHASE EQUILIBRIA

                      by 1.2 K if the pressure is increased fivefold. Calculate  V m for the wax as
                      it melts. Take  H (melt) = 8.064 kJ mol −1 .



                                              Justification Box 5.1

                         Consider two phases (call them 1 and 2) that reside together in thermodynamic equi-
                         librium. We can apply the Gibbs–Duhem equation (Equation 4.31) for each of the two
                         phases, 1 and 2.

                                      For phase 1 :  dG (1) = (V m(1) dp) − (S m(1) dT)   (5.2)

                                      For phase 2 :  dG (2) = (V m(2) dp) − (S m(2) dT)   (5.3)

                         where the subscripts ‘m’ imply molar quantities, i.e. per mole of substance in each phase.
                           Now, because equilibrium exists between the two phases 1 and 2, the dG term in
                         each equation must be the same. If they were different, then the change from phase 1 to
                         phase 2 (G (2) − G (1) ) would not be zero at all points; but at equilibrium, the value of
                          G will be zero, which occurs when G (2) = G (1) . In fact, along the line of the phase
                         boundary we say dG (1) = dG (2) .
                           In consequence, we may equate the two equations, saying:

                                   (V m(1) × dp) − (S m(1) × dT) = (V m(2) × dp) − (S m(2) × dT)

                         Factorizing will group together the two S and V terms to yield


                                            (S m(2) − S m(1) ) dT = (V m(2) − V m(1) ) dp

                         which, after a little rearranging, becomes

                                                     dp    S m(1→2)
                                                        =                                 (5.4)
                                                     dT    V m(1→2)

                                          O
                           Finally, since  G =  H  O  − T S  O  (Equation (4.21)), and since  G = 0at
                                                                                       O
                         equilibrium:
                                                     H  O
                                                       m
                                                         =  S m(1→2)
                                                     T
                         Inserting this relationship into Equation (5.4) yields the Clapeyron equation in its famil-
                         iar form.
                                                              O
                                                    dp     H m(1→2)
                                                       =
                                                    dT   T V m(1→2)
                         In fact, Equation (5.4) is also called the Clapeyron equation. This equation holds for
                         phase changes between any two phases and, at heart, quantitatively defines the phase
   224   225   226   227   228   229   230   231   232   233   234