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Essentials of Computational Chemistry

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8.4 EXCHANGE-CORRELATION FUNCTIONALS 259<br />

in ρ has already been noted). In practice, the only functionals conforming to this definition<br />

that have seen much application are those that derive from analysis <strong>of</strong> the uniform electron<br />

gas (where the density has the same value at every position), and as a result LDA is <strong>of</strong>ten<br />

used more narrowly to imply that it is these exchange and correlation functionals that are<br />

being employed.<br />

The distinction is probably best indicated by example. Following from Eq. (8.7) and<br />

the discussion in Section 8.1.2, the exchange energy for the uniform electron gas can be<br />

computed exactly, and is given by Eq. (8.23) with the constant α equal to 2<br />

. However, the<br />

3<br />

Slater approach takes a value for α <strong>of</strong> 1, and the Xα model most typically uses 3<br />

4 .All<strong>of</strong><br />

these models have the same ‘local’ dependence on the density, but only the first is typically<br />

referred to as LDA, while the other two are referred to by name as Slater (S) and Xα .<br />

The LDA, Slater, and Xα methods can all be extended to the spin-polarized regime using<br />

εx[ρ(r), ζ ] = ε 0 x [ρ(r)] + ε 1 x [ρ(r)] − ε0 x [ρ(r)] (1 + ζ) 4/3 + (1 − ζ) 4/3 − 2<br />

2(21/3 <br />

− 1)<br />

(8.26)<br />

where the superscript-zero exchange energy density is given by Eq. (8.23) with the appropriate<br />

value <strong>of</strong> α (referring here to the empirical constant, not the electron spin), and the<br />

superscript-one energy is the analogous expression derived from consideration <strong>of</strong> a uniform<br />

electron gas composed only <strong>of</strong> electrons <strong>of</strong> like spin. Noting that ζ = 0 everywhere for an<br />

unpolarized system, it is immediately apparent that the second term in Eq. (8.26) is zero<br />

for that special case. Systems including spin polarization (e.g., open-shell systems) must use<br />

the spin-polarized formalism, and its greater generality is sometimes distinguished by the<br />

sobriquet ‘local spin density approximation’ (LSDA).<br />

As for the correlation energy density, even for the ‘simple’ uniform electron gas no<br />

analytical derivation <strong>of</strong> this functional has proven possible (although some analytical details<br />

about the zero- and infinite-density limits can be established). However, using quantum<br />

Monte Carlo techniques, Ceperley and Alder (1980) computed the total energy for uniform<br />

electron gases <strong>of</strong> several different densities to very high numerical accuracy. By subtracting<br />

the analytical exchange energy for each case, they were able to determine the correlation<br />

energy in these systems. Vosko, Wilk, and Nusair (1980) later designed local functionals<br />

<strong>of</strong> the density fitting to these results (and the analytical low and high density limits). In<br />

particular, they proposed one spin-polarized functional completely analogous to Eq. (8.26)<br />

in terms <strong>of</strong> its dependence on ζ , but with the unpolarized and fully polarized energy densities<br />

expressed (now in terms <strong>of</strong> rS instead <strong>of</strong> ρ, see Eq. (8.24)) as<br />

ε i c (rS) = A<br />

<br />

ln<br />

2<br />

rS<br />

rS + b √ rS + c +<br />

bx0<br />

−<br />

x2 0 + bx0<br />

<br />

ln<br />

+ c<br />

2b<br />

√ 4c − b 2 tan−1<br />

( √ rS − x0) 2<br />

rS + b √ <br />

+<br />

rS + c<br />

2(b + 2x0)<br />

√ <br />

4c − b2 2 √ rS + b<br />

√ 4c − b 2 tan−1<br />

√ <br />

4c − b2 2 √ rS + b<br />

(8.27)

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