General Slater determinant spin-orbital form
(Why a "Slater Determinant" instead of a "dirac Determinant"?)
Energy = sum of single body terms, direct coulomb,
and exchange
Solution by minimization using variational theorem
and Lagrange multipliers for orthonormality constraints
Nonlinear "Schroedinger-like" Equations, with difficult
non-local exchange terms
Two-electron example (following Koonin, also similar to Thijssen)
Restricted Hartree Fock approximations: Open Shell vs. Closed Shell
"Spin Restricted": Occupy states just as in a non-interacting theory
Require equal spin up and spin down orbitals
Correct solution for cases which are "closed shell"
"Orbital Restricted": Allow unequal determinants and orbitals
for up and down spins
Require potential for each state (n,l,ml,ms)
to depend only on (n,l,ms); i.e.,
independent of ml
Essential for some cases - like H atom!
Approximate solution for "Open Shell systems"
"Unrestricted": no assumptions on symmetry of potential
Numerical methods for solution of equations for an atom
Of of the few cases where the H-F equations can be solved
directly by integrating differential equations
Continuation of discussion of solution of eigenvalue problems
related to Homework 2
Hartree-Fock solution for atom requires solution of
coupled Schroedinger-like and Poisson Eqs.
Explicit formulas take advantage of expansions for Coulomb terms
Equations for full Unrestricted case prepared by Tim Wilkens based
upon formulas from Slater and other sources
Ouline for computer program for solution. More later
Last Modified Feb. 7
Email question/comments/corrections to
rmartin@uiuc.edu
.