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My PhD thesis - Condensed Matter Theory - Imperial College London

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CHAPTER 2.<br />

MECHANICS<br />

THE SIMPLIFICATION OF MANY-ELECTRON QUANTUM<br />

The Coulomb operator ĵ represents the interaction of each electron with the average<br />

charge density; the unrestricted sum means that its own contribution to this charge<br />

density is included. This would give rise to an unphysical self-interaction, were it<br />

not for the fact that a corresponding term exists in ˆk, and the two cancel.<br />

An important point about the non-local exchange operator ˆk may be highlighted<br />

by making explicit the dependence of φ i on spin:<br />

φ i (x) = φ i (r, σ) = ζ i (r)δ σσi . (2.21)<br />

Substituting this expression into equation (2.20) gives<br />

ˆkφ i (x) = ∑ j<br />

φ j (x)δ σi σ j<br />

∫ ζ<br />

∗<br />

j (r ′ )ζ i (r ′ )<br />

|r − r ′ |<br />

dr ′ (2.22)<br />

showing that the exchange interaction only affects electrons with like spins. In<br />

Hartree-Fock theory, electrons of like spin are kept apart, and this lowers the energy<br />

expectation value. The exchange energy is the difference between the Hartree and<br />

Hartree-Fock values.<br />

Unfortunately, the theory does nothing to keep electrons of opposite spin apart.<br />

Such electrons interact only via the average charge density appearing in the Coulomb<br />

operator; there is no pairwise interaction to make it unfavourable for electrons of<br />

opposite spin to come together. This means that the ground-state energy calculated<br />

in Hartree-Fock theory is always higher than the true ground-state energy. The<br />

correlation energy is defined as the difference between the exact energy of the system<br />

and that calculated in Hartree-Fock theory.<br />

2.4 Density-functional theory<br />

The theorem underlying density-functional theory, due to Hohenberg and Kohn [35],<br />

states that the ground state of an N-electron system is completely determined by<br />

the one-electron density<br />

N∑<br />

∫<br />

n(r) = |Ψ(x 1 , . . . , x N )| 2 δ(r − r i ) dx 1 · · · dx N . (2.23)<br />

i=1<br />

25

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