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Essentials of Computational Chemistry

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256 8 DENSITY FUNCTIONAL THEORY<br />

Note that the ‘difficult’ terms T and Vee have been lumped together in a term Exc,<br />

typically referred to as the exchange-correlation energy. This is something <strong>of</strong> a misnomer,<br />

ins<strong>of</strong>ar as it is less than comprehensive – the term includes not only the effects <strong>of</strong> quantum<br />

mechanical exchange and correlation, but also the correction for the classical self-interaction<br />

energy (discussed in Section 8.1.2) and for the difference in kinetic energy between the<br />

fictitious non-interacting system and the real one.<br />

If we undertake in the usual fashion to find the orbitals χ that minimize E in Eq. (8.15),<br />

we find that they satisfy the pseudoeigenvalue equations<br />

where the Kohn–Sham (KS) one-electron operator is defined as<br />

and<br />

h KS<br />

i =−1<br />

2 ∇2 i −<br />

nuclei <br />

k<br />

h KS<br />

i χi = εiχi (8.17)<br />

Zk<br />

|ri − rk| +<br />

<br />

Vxc = δExc<br />

δρ<br />

ρ(r ′ )<br />

|ri − r ′ | dr′ + Vxc<br />

(8.18)<br />

(8.19)<br />

Vxc is a so-called functional derivative. A functional derivative is analogous in spirit to more<br />

typical derivatives, and Vxc is perhaps best described as the one-electron operator for which<br />

the expectation value <strong>of</strong> the KS Slater determinant is Exc.<br />

Note that because the E <strong>of</strong> Eq. (8.14) that we are minimizing is exact, the orbitals χ must<br />

provide the exact density (i.e., the minimum must correspond to reality). Further note that<br />

it is these orbitals that form the Slater-determinantal eigenfunction for the separable noninteracting<br />

Hamiltonian defined as the sum <strong>of</strong> the Kohn–Sham operators in Eq. (8.18), i.e.,<br />

N<br />

i=1<br />

h KS<br />

i |χ1χ2 ···χN〉 =<br />

N<br />

εi|χ1χ2 ···χN〉 (8.20)<br />

so there is internal consistency in the Kohn–Sham approach <strong>of</strong> positing a non-interacting<br />

system with a density identical to that for the real system. It is therefore justified to use<br />

the first term on the r.h.s. <strong>of</strong> Eq. (8.15) to compute the kinetic energy <strong>of</strong> the non-interacting<br />

electrons, which turns out to be a large fraction <strong>of</strong> the kinetic energy <strong>of</strong> the actual system.<br />

As for determination <strong>of</strong> the KS orbitals, we may take a productive approach along the<br />

lines <strong>of</strong> that developed within the context <strong>of</strong> MO theory in Chapter 4. Namely, we express<br />

them within a basis set <strong>of</strong> functions {φ}, and we determine the individual orbital coefficients<br />

by solution <strong>of</strong> a secular equation entirely analogous to that employed for HF theory, except<br />

that the elements Fµν are replaced by elements Kµν defined by<br />

Kµν =<br />

<br />

φµ|− 1<br />

2 ∇2 −<br />

nuclei <br />

k<br />

i=1<br />

Zk<br />

|r − rk| +<br />

<br />

ρ(r ′ )<br />

|r − r ′ | dr′ <br />

+ Vxc|φν<br />

(8.21)

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