The Hartree-Fock Equations
Having chosen Slater determinants as trial functions and having worked
out the rules needed to evaluate the Average Value Theorem, the next step
in a variational method (Table 1.2) is to minimize the expectation value
of the Hamiltonian with respect to the variational parameters in the Slater
determinant, the set of LCAO-MO coefficients in the spin orbitals, and
thereby find the best single Slater determinant description of the molecular
system. Collectively, this process is called the Hartree-Fock method.
[5,13,14]
From case 1 of Slater's rules, one finds that the expectation value of
the total energy for a molecule in the state given by the determinant
is
 |
(33) |
In order to use Slater's rules, it is assumed that the set of spin orbitals
are orthonormal and that they satisfy
 |
(34) |
This constraint, g, together with the energy functional, f,
can be used to minimize f using the method of Lagrange's undetermined
multipliers. In order to employ this method one combines the constraint
and energy functionals by introducing a set of undetermined multipliers,
denoted by
,
with the foreknowledge that in the end they will represent orbital energies:
 |
(35) |
The next step in Lagrange's method of undetermined multipliers is to set
the first variation of L to zero:
 |
(36) |
Upon expansion, followed by simplification in which a and b
are replaced by the respective spin orbitals,
and ,
one eventually arrives at a sum of complex conjugates:
At this juncture it is convenient to introduce two operators, the Coulomb
and exchange operators,
and ,
which will help reduce the equations:
These two particular operators are chosen because they have the following
expectation values:
allowing the minimization condition to be rewritten as
Moreover, the quantity
is an arbitrary variation in
,
and therefore, if the right side of the above equation is to equal zero
for all possible cases, the quantity in brackets must also equal zero:
![\begin{displaymath}\left[ h(1) \chi_a (1) + \sum_{b}^{N} (\hat{J}_b(1) - \hat{K}_b(1))\chi_a(1) - \sum_{b}^{N} {E_a}_b \chi_b(1) \right] = 0 .\end{displaymath}](IMG107.GIF) |
(43) |
Moving the term involving
to the other side of the equal sign yields
![\begin{displaymath}\left[ h(1) + \sum_{b}^{N} (\hat{J}_b(1) - \hat{K}_b(1)) \right] \chi_a(1)= \sum_{b}^{N} {E_a}_b \chi_b(1).\end{displaymath}](IMG108.GIF) |
(44) |
The quantity in brackets on the left-hand side of the equal sign is known
as the Fock operator, denoted by .
Thus, the minimization condition is reduced to the convenient operator
equation
 |
(45) |
The minimization condition given above is not in the standard or canonical
form of a eigenvalue equation. In quantum mechanics, when an operator
acts upon a state function that is compatible with it, one fully expects
to get an eigenvalue equation. In the case of the Fock operator, one can
expect the Slater determinant and the Fock operator to be compatible given
the method of their construction; hence, an eigenvalue equation should
result. The minimization criteria takes a non-canonical form because any
single Slater determinant wave function
formed from a set of spin orbitals
retains a certain degree of flexibility in the spin orbitals: the spin
orbitals can be mixed among themselves without changing the expectation
value
.
Fortunately, it is possible to cast the above minimization criterion into
an eigenvalue equation by transforming the spin orbitals into a set of
canonical spin orbitals through a unitary transformation of the general
form
 |
(46) |
where U is a unitary matrix and
is its inverse. The unitary matrix U is chosen such that the matrix
of undetermined multipliers Ewith entries Eab
is diagonalized after the unitary transformation
 |
(47) |
The exact mathematical details behind the transformation are not important;
what is important is that upon completion of some mathematically allowable
unitary transformation of the form described, the minimization criterion
is finally cast into the standard form known as the canonical Hartree-Fock
equation:
 |
(48) |
|