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276                                            M. TADJEDDINE AND J. P. FLAMENT

                             Owing to  the  very  large  discrepancies in the  data on   we have made new  com-
                             putations  with  other  basis sets   but  with the  same  process;  they  converge
                             at less than 4%  from the previous ones, giving confidence in our results and in our
                             procedure.

                             3.4. APPLICATION TO Be AND Ne
                             The two preceding applications showed that our hydrogenic model fits well with the
                             helium atom and the dihydrogen molecule for the determination of the polarization
                             functions except that their exponent  is different from  which is the exponent of
                             the genuine basis set     It is obvious that the hydrogenic model will fit less and
                             less as the atom will be described by more and more electrons.
                             Nevertheless our method of  and  calculations has been successfully extended to
                             Be and Ne atoms (21). Let us resume the principal results :

                                1. For less than 1% error for  it is sufficient to ”polarize” only the valence
                                  electrons in Be; the polarization of the 1s orbital leads to an  value within
                                  0.1% of HFL value. Contrary to Be, the polarization of the inner shell is now
                                  absolutly negligible for Ne.

                                2. The transfer of exponent to the   set leads to good values of  : for Be :
                                            instead of the HF limit             and for Ne : 68 instead of
                                   70  (42).
                                3. Contrary to the previous applications     we observe an increase of the
                                  values of  with the     polarization function because  contains p func-
                                  tions improving the first  order wavefunction which,  despite its  size, was  not  at
                                  the HF  limit.

                                4. At last, it is possible to still improve the results on  by using two different
                                  values of the exponent :

                                         by optimization of   for the STO of
                                         by optimization of   for the STO of
                             This last result is important for the generalization of our procedure to more compli-
                             cated systems.

                             4.Conclusion

                             The computation  of  polarizabilities requires consideration of  two complementary
                             problems: the computational method and  the basis set used.
                             We have  first  been  concerned  with the  computational point  of  view.  Through  the
                             calculation of the dynamic polarizability of CO,  we have developed a method  based
                             on the conventional SCF–CI method, using the variational– perturbation techniques :
                             the first–order wavefunction includes two parts (i) the traditional one, developed over
                             the excited states and (ii) additional terms obtained by multiplying the zeroth–order
                             function by  a  polynomial of  first–order in  the  electronic coordinates.  This dipolar
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