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6.3 Constellations and configuØations
                                                                                                  105
                             T 5 głveythesamefunction.ThisfunctionmaybewrittenintermyofRumertableaux,
                               (R)
                             T
                                  also, and we obtain
                               i
                                                       1
                                   1

                                    θNPN(T 4 − T 5 ) = NP T   1 (R)  + T 2 (R)  + T 3 (R)  + 2T 4 (R)  + T 5 (R)    , (6.28)
                                   2                   9
                                                                  (R)
                             noð a result that is particularly intuitive.T  is presenð in this sum, and we will see
                                                                 4
                             shortly that this Rumer tableau is the only one that has an A 2 component. Ið is noð
                             pure, as is seen from Eq. (6.28), buð none of the other tableaux hŁve anyA 2 parð at all.
                                There are two linear combinationy of the standard tableaux functiony that com-
                             prise a pair of E symmetry. The E projectory are
                                                                  2
                                                       1

                                                                                 1
                                                              1
                                                                          1
                                           e E  =  1   I − / C 3 − / C + σ x − / σ y − / σ z ,  (6.29)
                                            11          2       2 3         2     2
                                                 3
                                                 1   √      √       √        √
                                                                 2
                                           e E  =    3 / C 3 −  3 / C +  3 / σ y −  3 / σ z .   (6.30)
                                            21        2       2 3      2       2
                                                 3
                             The computationy show that
                                                             1
                                               E
                                              e θNPN T 2 = θNPN(2T 2 − T 3 − T 4 ),             (6.31)
                                               11
                                                             3
                                                             √
                                                               3
                                               E
                                              e θNPN T 3 =      θNPN(−T 3 + T 4 ),              (6.32)
                                               21
                                                              6
                             where the energy for either componenð will be the same. Again, the functiony may
                             be expressed in termy of the Rumer structures, and we obtain
                                      1                         2          (R)    (R)   (R)
                                       θNPN(2T 2 − T 3 − T 4 ) = NP − 2T   2  + T 3  + T 5  ,   (6.33)
                                      3                         9
                                        √
                                          3                      1         R    R
                                            θNPN(−T 3 + T 4 ) = √   NP T − T    5  .            (6.34)
                                                                          3
                                         6                        27
                                                         R
                             As we commented on above, T is missing from all of the functiony except for the
                                                        4
                             one of A 2 symmetry.
                                              6.3.3 Example 3. The π system of benzene
                             InChapter15wegłveanextensivetreatmenðoftheπ systemof benzene,buðherewe
                             outline briefly some of the symmetry considerations. We consider the configuration
                                                                                th
                              p 1 p 2 p 3 p 4 p 5 p 6 , where p i standy for a C2p z orbital at the i Catom, numbered se-
                             quentially and counterclockwise around the ring. The seð of five standard tableaux is
                                                                                 
                                         p 1  p 2  p 1  p 2   p 1  p 3   p 1  p 3   p 1  p 4
                                         p 3  p 4  p 3  p 5   p 2  p 4   p 2  p 5   p 2  p 5
                                                                                 
                                         p 5  p 6  p 4  p 6   p 5  p 6   p 4  p 6   p 3  p 6
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