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The Feynman model                          109

            7.4 The Feynman model
            This is the one I like best, because it combines mathematical simplicity with
            an eloquent physical picture. It is essentially a generalization of the model we
            used before to understand the covalent bond—another use of the coupled mode
            approach.
               Remember, the energy levels of two interacting atoms are split; one is
            slightly above, the other slightly below the original (uncoupled) energy. What
            happens when n atoms are brought close together? It is not unreasonable to ex-
            pect that there will be an n-fold split in energy. So if the n atoms are far away
            from each other, each one has its original energy levels denoted by E 1 and E 2
            in Fig. 7.9(a), but when there is interaction they split into n separate energy
            levels. Now looking at this cluster of energy levels displayed in Fig. 7.9(b), we
            are perfectly entitled to refer to allowed energy bands and to forbidden gaps
            between them.
               To make the relationship a little more quantitative, let us consider the one-
            dimensional array of atoms shown in Fig. 7.10. We shall now put a single
            electron on atom j into an energy level E 1 and define by this the state ( j). Just
            as we discussed before in connection with the hydrogen molecular ion, there is
            a finite probability that the electron will jump from atom j to atom j + 1, that is
            from state ( j) into state ( j + 1). There is of course no reason why the electron
            should jump only in one direction; it has a chance of jumping the other way
            too. So the transition from state ( j) into state ( j–1) must have equal probability.
            It is quite obvious that a direct jump to an atom farther away is also possible
            but much less likely; we shall therefore disregard that possibility.




              ) a (                      ) b (
                                                      n
                                                      n –1
                                                      n/2+2
             E                                        n/2+1        Allowed
              2                                       n/2
                                                      n/2–1
                                                      1
                                                      0
                                                                   Forbidden
                                                      n
                                                      n –1
                                                      n/2+2
                                                      n/2+1                  Fig. 7.9
             E                                        n/2          Allowed
              1
                                                      n/2–1                  There is an n-fold split in energy
                                                                             when n atoms are brought close to
                                                      2                      each other, resulting in a band of
                                                      1                      allowed energies, when n is large.

                      j–2         j–1      j       j+1         j+2
                                                                             Fig. 7.10
                                               a
                                                                             A one-dimensional array of atoms.
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