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August 18, 2010 11:36      9in x 6in     b985-ch06     Elementary Physical Chemistry





                                                Phase and Chemical Equilibria              51



                              Comment: The way the chemical potential behaves is similar to the
                              behavior of the free energy. Thus, we have ∆µ ≤ 0, where the equal
                              sign pertains to equilibrium and the unequal sign to non-equilibrium
                              situations. If a system can exist in two different states, the most
                              favored state is the one with the lowest µ. When liquid and vapor
                                                                                         ∗
                              are at equilibrium (coexist), say at the normal boiling point, T ,
                                                                                        b
                              the chemical potentials of the two phases must be equal. Above the
                              normal boiling temperature, the vapor phase is the more stable state,
                              and the chemical potential of the vapor will be lower than that of the
                              pure liquid. Below the normal boiling temperature, the liquid phase
                              is the stable phase, and the chemical potential of the liquid will be
                              the lowest. Similar considerations apply to the chemical potentials
                              responsible for the lowering of the freezing point (see Fig. 6.4).



                               Let us denote the normal boiling point and normal freezing point of the
                                                            ∗
                                                     ∗
                            pure liquid respectively as T and T and the boiling and freezing points
                                                     b
                                                            f
                            of the actual solutions as T b and T f .We can write
                                                             ∗
                                                 ∆T b = T b − T = m bK b              (6.14a)
                                                             b
                                                         ∗
                                                  ∆T f = T − T f = m f K f            (6.14b)
                                                         f
                            where m b is the molality of solute and K b and K f are respectively the
                            boiling point elevation constant and freezing point depression constant.
                            (These constants can readily be related to thermodynamic functions, but
                            will not be developed in this course.)
                                                                                         3
                            Example 6.3. Calculate the boiling point of a solution of 250 cm of
                            H 2 O(l) containing 7.5 g of a solute. The normal boiling point of H 2 O(l)
                            is 373.25 K. The boiling-point elevation constant, K b is 0.51K kg mol −1 .
                            The molecular weight of the solute is M = 342 g mol −1 .

                            Solution
                                        3
                            7.5 g in 250 cm of water is equivalent to 30.0g of solute in 1 L of water. The
                            mole fraction of 30.0 g of solute in 1 L of H 2 O(l) is m =30.0 g/342g mol −1  =
                            8.77 × 10 −2  mol and thus the molarity of the solute is 8.77 × 10 −2  mol/L.
                            Assuming that 1 L of water at the normal boiling point weighs essentially
                            1 kg, we can equate the molarity m to the molality, m b ,and write m b =
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