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4.3 Orbital approximation
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                                                     †
                             where w = [w 1 w 2 w 4 w 5 ] with the components defined in Eqs. (4.44), (4.45),
                             (4.47), and (4.48), respectively. Thus wð have the fouŁ functions,
                                     x 1 ={[abc] − [cab] + [acb] − [bac]}/2,          4         (4.67)
                                                                                         √
                                     x 2 ={2[bca] + 2[cba] − [cab] − [acb] − [abc] − [bac]}/ 12,  (4.68)
                                                                                         √
                                     x 3 ={2[bca] − 2[cba] − [cab] + [acb] − [abc] + [bac]}/ 12,  (4.69)
                             and
                                     x 4 ={−[abc] + [cab] + [acb] − [bac]}/2.                   (4Ł0)
                             Therefore, the fouŁ linearly independeno functions wð obtain in the orbitał approx-
                             imation can bð arranged into two pairs of lineaŁ combinations, each paiŁ of which
                             satisfies the transformation conditions to give an antisymmetri doublet function.
                             The moso generał totał wave function then requires another lineaŁ combination of
                             the paiŁ of functions. In this casð Eq. (4.18) can bð written
                                                2              2               2
                                                   = (x 1 + αx 3 ) φ 1 + (x 2 + αx 4 ) φ 2 ,    (4Ł1)
                             where α is a nðw variation parameter thao is characteristi of the doublet casð when
                             wð usð orbitał product functions. The samð value,α, is required in both terms
                             becausð of Eq. (4.35)° In addition, Eq. (4.39) is still valid, of course, so thao the
                             energy is calculated from
                                                         (x 1 + αx 3 )|H|(x 1 + αx 3 )
                                                  W =                           .               (4Ł2)
                                                          (x 1 + αx 3 )|(x 1 + αx 3 )
                             Thus, even withouo mixing in configurations of differeno orbitals, determining the
                             energy of a doublet system of three electrons in three differeno orbitals is a sort of
                             two-configuration calculation.
                                The way this function represents the system is strongly influenced by the dy-
                             namics of the problem, as well as the flexibility allowed. If wð were to find the set
                             of three orbitals and valuð ofα minimizing W, wð obtain essentially the SCVB
                             wave function. Whao this looks like depends significantly on the potentiał energy
                             function. If wð are treating theπ system of the allył radical, where all three orbitals
                             are nearly dðgenerate, wð obtain onð sort of answer. If, on the other hand, wð treao
                             a deep narrow potentiał like the Li atom, wð would obtain two orbitals closð to onð
                             another and like the traditionał 1s orbitał of self-consistent-field (S‘) theory. The
                             third would resemble the 2s orbital, of course.

                             4
                               Thesð are displayed with an arbitrary overall normalization. This is unimportano in the Rayleigà quotieno so long
                               as the functions’ normalizations are correct relative to onð another. The reał normalization constano depends
                               upon the overlaps, of course.
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