4.5 Self-consistency and exchange: Hartree–Fock theory 57therefore calculate the expectation value of the energy for an arbitrary Slater determ-
inant using the Born–Oppenheimer Hamiltonian and then minimise the result with
respect to the spin-orbitals in the determinant.
We write the Hamiltonian as follows:
H=∑
ih(i)+1
2
∑
i,j;i=jg(i,j) withg(i,j)=1
|ri−rj|
andh(i)=−1
2
∇i^2 −∑
nZn
|ri−Rn|.
(4.34)
h(i)depends onrionly andg(i,j)onriandrj. Writing the Slater determinantψas
a sum of products of spin-orbitals and using the orthonormality of the latter, it can
easily be verified that this determinant is normalised, and for the matrix element of
the one-electron part of the Hamiltonian, we find (see Problem 4.3)
〈
AS
∣∣
∣∣
∣
∑
ih(i)∣∣
∣∣
∣
AS
〉
=N·
(N− 1 )!
N!
∑
k〈ψk|h|ψk〉=
∑
k〈ψk|h|ψk〉=∑
k∫
dxψk∗(x)h(r)ψk(x). (4.35)By
∫
dxwe denote an integral over the spatial coordinates and a sum over the
spin-degrees of freedom as usual.
The matrix element of the two-electron termg(i,j)for a Slater determinant not
only gives a nonzero contribution when the spin-orbitals in the left and right hand
sides of the inner product occur in the same order, but also forkandlinterchanged
on one side (the derivation is treated in Problem 4.3):
〈
AS
∣∣
∣∣
∣∣
∑
i,jg(i,j)∣∣
∣∣
∣∣AS
〉
=
∑
k,l〈ψkψl|g|ψkψl〉−∑
k,l〈ψkψl|g|ψlψk〉. (4.36)In this equation, the following notation is used:
〈ψkψl|g|ψmψn〉=∫
dx 1 dx 2 ψk∗(x 1 )ψl∗(x 2 )1
|r 1 −r 2 |ψm(x 1 )ψn(x 2 ). (4.37)In summary, we obtain for the expectation value of the energy:
E=∑
k〈ψk|h|ψk〉+1
2
∑
kl[〈ψkψl|g|ψkψl〉−〈ψkψl|g|ψlψk〉]. (4.38)