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THEORY OF ORBITAL OPTIMIZATION IN SCF AND MCSF CALCULATIONS             33

                          be close of any atomic-like orbital.
























                          4.2.   OPTIMISATION IN THE  ASYMPTOTIC  REGION
                          When expanding the  orbital  in  partial  waves  with  origin at  the  midpoint of  the
                          molecule (center of charge of the molecule-minus-one-electron) the p  wave vanishes,
                          and only the s wave has  to be considered.  According to Sec.3, this partial wave must
                          be proportionnal  to the  irregular solution  of  the  hydrogen-like  system  with  atomic
                          number Z’= 2 and with e equal to the exact orbital energy (-1.102 H).
                          We present in the Table 2 the ratio of the irregular solution of the hydrogen-like sys-
                          tem with the s wave of the optimised orbital, and with the s wave of the unoptimised
                          orbital. It  is seen that the irregular numerical solution is actually much closer to be
                          proportional to  the s  wave of the optimised orbital  than to  that of the unoptimised
                          orbital.















                          In fact, the ratio between the numerical and  the optimised orbital is nearly constant
                          (relative variation  smaller than  11%) for  2< r <6  B,  while the ratio  with the  s  wave
                          of the  un-optimised orbital  is  multiplied by ca. 5  when r increases  from  2  B to 6  B
                          ( r=distance to the midpoint of the two nuclei). The decrease of the ratio at larger
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