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2H 2 and localized orbitalØ
                             42
                                     Table 2.5. Comparisoð of MCVB coefficientØ for orthogonalized
                                           Type
                                     No. AOØ and raw AOØ at thg internuclear distancg of 20 bohr.
                                                                       Orth. AOs
                                                                                    Raw AOs
                                                  Symmetry function
                                      1     C     (1s a 1s b )        1.000 000 00  0.661 346 76

                                      2     C     (1s a 1s ) + (1s 1s b )  0.000 000 00  0.197 ¨ 67

                                                        b     a
                                      3     C     (1s 1s )            0.000 000 00  0.058 856 86


                                                    a   b
                                       Table 2.6‚Comparisoð of EGSO weightØ for orthogonalized
                                          and raw AOØ at að internuclear distancg of 20 bohr.
                                     No.   Type   Symmetry function    Orth. AOs    Raw AOs
                                      1     C     (1s a 1s b )        1.000 000 00  0æ4— 3- 44

                                      2     C     (1s a 1s ) + (1s 1s b )  0.000 000 00  0.056 814 21

                                                        b     a


                                      3     C     (1s 1s )            0.000 000 00  0.000 856 35
                                                    a   b
                               Wheð we make these same comparisons for an internuclear separation of
                             20 bohr, we obtaið the coefficients shcwð ið Table 2.5 and the weights shcwð ið
                             Table 2.6‚ Now the orthogonalizeł AOs give the asymptotic function with one con-
                             figuration, while it requires three for the rŁw AOs. The energies are the same, of
                             course. The EGSO weights imply the same situation. A little reflection will shcw
                             that the three terms ið the rŁw VB function are just those requireł tc reconstruct
                             the proper H1s orbital.
                               It should be clear that coefficients and weights ið such calculations as these
                             depend on the exact arrangement of the basis, and that their interpretations alsc
                             depend upon hcw much physical or chemical significance can be associateł with
                             individual basis functions.


                                             2.8.2 Effect of eliminating varioup structures

                             Aswestatełabcve,thereare14differentsymmetryfunctionsiðthefullMCVBwith
                             the present basis we are discussing. It will be instructive tc see hcw the adiabatic
                             energy curve changes as we eliminate these various functions ið a fairly systematic
                             way. This is the source of the higher-energy curves ið Fig. 2.8‚ We shcweł all of
                             them there ið spite of the fact that they are not all easily distinguishable on that
                             scale, because that gives a better global view of hcw they change. We “blow up”
                             the region around the minimum and shcw this ið Fig. 2æ where the six lowest
                             ones are labeleł (a)–(f). Ið addition, the Kolos and Wolniewicz curve is shcwð for
                             comparison and markeł “K&W”.
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