Gaussian basis sets violate nuclear cusp conditions.
      
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This may lead to large errors in wave function at nuclei,
particularly for spin density calculations.
      
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 This problem
can be alleviated by using an averaging operator that compute wave function
density based on constraints that wave function must satisfy near Coulomb
singularity.
      
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 The derivation of operators is
based on hyper virial theorem
      
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 and presented in
Ref. 
      1104
      
         
            
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. Application to molecular spin densities for
spin-polarized
      
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 and DFT
      
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 wave functions show
considerable improvement over traditional delta function operator.
One of the simplest forms of such operators is based on the Gaussian weight
function 
that samples the vicinity of a nucleus of charge  located at . The parameter 
has to be small enough to neglect two-electron contributions of the order
 but large enough for meaningful averaging. The range of values
between 0.15–0.3 a.u. has been shown to be adequate, with final answer being
relatively insensitive to the exact choice of .
      
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The value of  is chosen by
RC_R0 keyword in the units of 0.001 a.u. The averaging operators are
implemented for single determinant Hartree-Fock and DFT, and correlated SSG
wave functions. Spin and charge densities are printed for all nuclei in a
molecule, including ghost atoms.
RC_R0
RC_R0
      
Determines the parameter in the Gaussian weight function used to smooth the
density at the nuclei.
TYPE:
      
INTEGER
DEFAULT:
      
0
OPTIONS:
      
0
Corresponds the traditional delta function spin and charge densities
corresponding to  a.u.
RECOMMENDATION:
      
We recommend value of 250 for a typical spit valence basis. For basis sets
with increased flexibility in the nuclear vicinity the smaller values of 
also yield adequate spin density.