Computational Physics - Department of Physics

(Axel Boer) #1

15.4 Derivation of the Hartree-Fock equations 505


15.4.2 Varying the single-particle wave functions


If we generalize the Euler-Lagrange equations to more variables and introduceN^2 Lagrange
multipliers which we denote byεμ ν, we can write the variational equation for the functional
of Eq. (15.23) as


δE−

N

μ= 1

N

ν= 1

εμ νδ


ψμ∗ψν= 0. (15.23)

For the orthogonal wave functionsψμthis reduces to


δE−

N

μ= 1

εμδ


ψμ∗ψμ= 0. (15.24)

Variation with respect to the single-particle wave functionsψμyields then

N

μ= 1


δ ψμ∗hˆiψμdxi+^1
2

N

μ= 1

N

ν= 1

[∫

δ ψ∗μψν∗^1
ri j
ψμψνd(xixj)−


δ ψμ∗ψν∗^1
ri j
ψνψμdridrj

]

+

N

μ= 1


ψμ∗hˆiδ ψμdri+

1

2

N

μ= 1

N

ν= 1

[∫

ψ∗μψν∗

1

ri j
δ ψμψνdridrj−


ψμ∗ψν∗

1

ri j
ψνδ ψμdridrj

]


N

μ= 1



δ ψ∗μψμdxi−

N

μ= 1



ψμ∗δ ψμdri= 0.

(15.25)

Although the variationsδ ψandδ ψ∗are not independent, they may in fact be treated as
such, so that the terms dependent on eitherδ ψandδ ψ∗individually may be set equal to
zero. To see this, simply replace the arbitrary variationδ ψbyiδ ψ, so thatδ ψ∗is replaced by
−iδ ψ∗, and combine the two equations. We thus arrive at the Hartree-Fock equations
[


1

2

∇^2 i−

Z

ri

+

N

ν= 1


ψν∗(rj)

1

ri j
ψν(rj)drj

]

ψμ(xi)


[N


ν= 1


ψν∗(rj)

1

ri j
ψμ(rj)drj

]

ψν(ri) =εμψμ(ri).

(15.26)

Notice that the integration


drjimplies an integration over the spatial coordinatesrjand
a summation over the spin-coordinate of electronj.
The two first terms are the one-body kinetic energy and the electron-nucleus potential.
The third ordirectterm is the averaged electronic repulsion of the other electrons. This
term includes the ’self-interaction’ of electrons wheni=j. The self-interaction is cancelled in
the fourth term, or theexchangeterm. The exchange term results from our inclusion of the
Pauli principle and the assumed determinantal form of the wave-function. The effect of the
exchange is for electrons of like-spin to avoid each other. Atheoretically convenient form of
the Hartree-Fock equation is to regard the direct and exchange operator defined through the
following operators


Vμd(ri) =


ψμ∗(rj)^1
ri j
ψμ(rj)drj (15.27)

and


Vμex(ri)g(ri) =

(∫

ψ∗μ(rj)

1

ri jg(rj)drj

)

ψμ(ri), (15.28)
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