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26                                                          C.CHAVY ET AL.
                            for Si)  the  deviation   is still smaller than 10%  of the  value of the orbital at  the last
                            extremum.

                            These  results  illustrate  the fact that the orbital is  weakly dependent of the  energy
                             e at the peak for r=0 (Cusp theorem) but also down in the valley and even on the
                             next hill if any (Valley theorem).




















































                            In  the case of the p  and  d  orbitals  (fig.  4-6) the deviations  are  larger than the
                            deviations obtained  with s  orbitals. This  is simply because the  magnitudes of the
                            p and d  orbitals are  larger  than  those of the  s  orbitals for r  ca.  1.0 B  due to the
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