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20                                                          C. CHAVY ET AL.


                            1.1. HYDROGEN-LIKE ATOMS
                            In the case of hydrogen-like atoms the Schrödinger equation can be written as (in
                            atomic units) :





                            where T  represents the  kinetic  energy  operator,  Z the nuclear  charge, -Z/r the
                            Coulomb  electron-nuclear  attraction, e the  energy  and   the  orbital.

                            The solution   of  this  equation can be  factorised  into the  product  of  a  radial part
                            and an  angular  part  (spherical  harmonic  where  the  radial part   depends of
                            the quantum number l  but not of m (2).




                            Inserting this form of   into the  eq.(l)  gives the  equation to  be satisfied  by   the
                            so called  radial  equation :





                            It  can be  demonstrated (2)  that two linearly  independent solutions  of this  equation
                            can be  chosen  in  general (i.e. except  for  some  values of e) in  such  a  way  that one
                            of them  (the so  called  ’regular’  solution) is  continuous at the  origin  and  diverges at
                            infinity, and  the other one  (the so  called  ’irregular’  solution)  diverges at  the  origin
                            and tends to zero at infinity.

                            Neither of these two solutions is square summable in general.  However for some values
                            of e (the  ’eigen  values’) these two solutions  coincide and  can  be  accepted  physically
                            for atoms  since they  both are  continuous  at  the  origin  and they  both tend  to  zero at
                            infinity.
                            It should be emphasized that we are not interested here specifically by these particular
                            values of e.  On the contrary , what  is  useful  here i.e. for  the description of optimum
                            orbitals in  molecules is  to  study the  variation of  the  regular solution  when e varies
                            continuously.

                            To solve that problem,  we depart here from the  development used for  instance in  (2)
                            and we  write   in  the form  :

                                                                                                   (4)
                            Substituting  this  form of   into the  eq.(3)  leads to  :

                                                                                                   (5)

                            But  we are interested here only by the ’regular’ solution, and we can write  in  the
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