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Theory of Orbital Optimisation in SCF and MCSCF Calculations





                          C. CHAVY, J.  RIDARD and  B.LEVY
                          Groupe de  Chimie  Quantique,  Laboratoire  de  Physico-Chimie des Rayonnements,
                          (UA CNRS  75), bât.  337,  Université  Paris Sud,  91405,  Orsay  Cedex,  France



                          The aim of the present article is to present a qualitative description of the ’optimised’
                          orbitals of molecular systems i.e. of the  orbitals  resulting from  SCF calculations  or
                          from  MCSCF calculations  involving a  valence CI :  we  do  not  present  here a  new
                          formal  development (although  some  formalism is  necessary),  nor a  new  computa-
                          tional  method, nor  an  actual calculation  of  an  observable  quantity ...  but  merely
                          the description  of the  orbitals.
                          In  fact,  it turns out  that the  orbitals  resulting  from SCF  or valence  MCSCF  calcu-
                          lations in  molecules can be  described in  extremely simple terms by comparing  them
                          with the RHF  orbitals of the  separated  atoms.

                          In  the  case of a  valence  MCSCF  calculation  the  difference  between the  optimised
                          orbitals and these atomic RHF orbitals simply represents the way in which the atoms
                          are distorted by the  molecular environment.  Thus,  this  difference is  closely related
                          to the idea of ’atoms in molecules’ (l). However, here, the atoms are represented only
                          at  the RHF  level,  and the  difference  concerns only  the  orbitals,  not the intra-  atomic
                          correlation.
                          The starting  step of  the  present  work is a  specific  analysis  of  the solution of  the
                          Schrödinger equation for atoms (section 1).  The successive steps for the application of
                          this  analysis to molecules are presented in the section 2  (description of the optimised
                          orbitals  near of the  nuclei), 3  (description of the orbitals  outside the  molecule), and
                          4 (numerical test in  the case of   ).  The study of other molecules will be presented
                          elsewhere.

                          1. The atomic case

                          We briefly  recall  here a  few basic  features of  the radial  equation for hydrogen-like
                          atoms.  Then we  discuss  the energy  dependence of the  regular solution of the  radial
                          equation  near the origin in the case of hydrogen-like as  well as polyelectronic atoms.
                          This dependence will turn out to be the most  significant aspect  of the radial  equation
                          for  the description  of the  optimum orbitals in  molecules.
                                                              19
                          Y. Ellinger and M. Defranceschi (eds.), Strategies and Applications in Quantum Chemistry, 19–37.
                          © 1996 Kluwer Academic Publishers. Printed in the Netherlands.
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