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2.10        PRINCIPLES OF OPERATION

                             and
                                                            RT       RT
                                                         n =   ln i -   ln i                     (2.24)
                                                            α  nF  o  α  nF
                             which is the Tafel equation introduced earlier in a generalized form as Eq. (2.7). It can now be
                             seen that the kinetic treatment here is self-consistent with both the Nernst equation [see Eq. (2.19)]
                             (for equilibrium conditions) and the Tafel relationship [see Eq. (2.7)](for unidirectional processes).
                             To present the kinetic treatment in its most useful form, a transformation into a net current flow
                             form is appropriate. Using
                                                              i =  i -  f  i                     (2.25)
                                                                    b
                             substitute Eqs. (2.10), (2.13), and (2.18),
                                                                                  o
                                                                 o
                                                          - α  nFE     (1 - )α  nFE   
                                              i =  nFAk C exp   C    - C exp   C            (2.26)
                                                    
                                                      O
                                                                      R
                                                                               T
                                                           RT            RT    
                                                                                    
                             When this equation is applied in practice, it is very important to remember that C  and C  are
                                                                                                 R
                                                                                           O
                             concentrations  at  the  surface  of  the  electrode,  or  are  the  effective  concentrations. These  are  not
                             necessarily the same as the bulk concentrations. Concentrations at the interface are often (almost
                             always) modified by differences in electric potential between the surface and the bulk solution. The
                             effects of potential differences that are manifest at the electrode-electrolyte interface are given in
                             the following section.
                 2.4  ELECTRICAL DOUBLE-LAYER CAPACITY AND
                 IONIC ADSORPTION
                             When an electrode (metal surface) is immersed in an electrolyte, the electronic charge on the metal
                             attracts ions of opposite charge and orients the solvent dipoles. There exist a layer of charge in the metal
                             and a layer of charge in the electrolyte. This charge separation establishes what is commonly known
                                                    5
                             as the “electrical double layer.”  Experimentally, the electrical double-layer effect is manifest in the
                             phenomenon named “electrocapillarity.” The phenomenon has been studied for many years, and there
                             exist ther modynamic relationships that relate interfacial surface tension between electrode and elec-
                             trolyte solution to the structure of the double layer. Typically the metal used for these mea surements is
                             mercury since it is the only conveniently available metal that is liquid at room temperature (although
                             some work has been carried out with gallium, Wood’s met al, and lead at elevated temperature).
                                Determinations of the interfacial surface tension between mercury and electrolyte solution can
                             be made with a relatively simple apparatus. All that is needed are (1) a mercury-solution interface
                             that is polarizable, (2) a nonpolarizable interface as reference potential, (3) an external source of
                             variable potential, and (4) an arrangement to measure the surface tension of the mercury-electrolyte
                             interface. An experimental system that will fulfill these requirements is shown in Fig. 2.7. The inter-
                             facial surface tension is measured by applying pressure to the mercury-electrolyte interface by rais-
                             ing the mercury “head.” At the interface, the forces are balanced, as shown in Fig. 2.8. If the angle of
                             contact at the capillary wall is zero (typically the case for clean surfaces and clean electrolyte), then
                             it is a relatively simple arithmetic exercise to show that the interfacial surface tension is given by

                                                                  ρ
                                                              γ =  hgr                           (2.27)
                                                                  2
                             where γ = interfacial surface tension, ρ = density of mercury, g = force of gravity, r = radius of capil-
                             lary, and h = height of mercury column in capillary.
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