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Essentials of Computational Chemistry

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134 5 SEMIEMPIRICAL IMPLEMENTATIONS OF MO THEORY<br />

5.2 Extended Hückel Theory<br />

Prior to considering semiempirical methods designed on the basis <strong>of</strong> HF theory, it is instructive<br />

to revisit one-electron effective Hamiltonian methods like the Hückel model described<br />

in Section 4.4. Such models tend to involve the most drastic approximations, but as a result<br />

their rationale is tied closely to experimental concepts and they tend to be intuitive. One<br />

such model that continues to see extensive use today is the so-called extended Hückel<br />

theory (EHT). Recall that the key step in finding the MOs for an effective Hamiltonian is<br />

the formation <strong>of</strong> the secular determinant for the secular equation<br />

<br />

<br />

H11 <br />

− ES11 H12 − ES12 ... H1N − ES1N <br />

<br />

H21 <br />

− ES21 H22 − ES22 ... H2N − ES2N <br />

<br />

<br />

<br />

. = 0 (5.1)<br />

.<br />

. .. . <br />

<br />

HN1 − ESN1 HN2 − ESN2 ... HNN − ESNN<br />

The dimension <strong>of</strong> the secular determinant for a given molecule depends on the choice<br />

<strong>of</strong> basis set. EHT adopts two critical conventions. First, all core electrons are ignored. It<br />

is assumed that core electrons are sufficiently invariant to differing chemical environments<br />

that changes in their orbitals as a function <strong>of</strong> environment are <strong>of</strong> no chemical consequence,<br />

energetic or otherwise. All modern semiempirical methodologies make this approximation. In<br />

EHT calculations, if an atom has occupied d orbitals, typically the highest occupied level <strong>of</strong><br />

d orbitals is considered to contribute to the set <strong>of</strong> valence orbitals.<br />

Each remaining valence orbital is represented by a so-called Slater-type orbital (STO). The<br />

mathematical form <strong>of</strong> a normalized STO used in EHT (in atom-centered polar coordinates) is<br />

ϕ(r,θ,φ; ζ,n,l,m) = (2ζ)n+1/2<br />

[(2n)!] 1/2 rn−1e −ζr Y m<br />

l<br />

(θ, φ) (5.2)<br />

where ζ is an exponent that can be chosen according to a simple set <strong>of</strong> rules developed by<br />

Slater that depend, inter alia, on the atomic number (Slater 1930), n is the principal quantum<br />

number for the valence orbital, and the spherical harmonic functions Y m<br />

l (θ,φ), depending<br />

on the angular momentum quantum numbers l and m, are those familiar from solution <strong>of</strong><br />

the Schrödinger equation for the hydrogen atom and can be found in any standard quantum<br />

mechanics text. Thus, the size <strong>of</strong> the secular determinant in Eq. (5.2) is dictated by the total<br />

number <strong>of</strong> valence orbitals in the molecule. For instance, the basis set for the MnO4 − anion<br />

would include a total <strong>of</strong> 25 STO basis functions: one 2s and three 2p functions for each<br />

oxygen (for a subtotal <strong>of</strong> 16) and one 4s, three 4p, and five 3d functions for manganese.<br />

STOs have a number <strong>of</strong> features that make them attractive. The orbital has the correct<br />

exponential decay with increasing r, the angular component is hydrogenic, and the 1s orbital<br />

has, as it should, a cusp at the nucleus (i.e., it is not smooth). More importantly, from a<br />

practical point <strong>of</strong> view, overlap integrals between two STOs as a function <strong>of</strong> interatomic<br />

distance are readily computed (Mulliken Rieke and Orl<strong>of</strong>f 1949; Bishop 1966). Thus, in<br />

contrast to simple Hückel theory, overlap matrix elements in EHT are not assumed to be<br />

equal to the Kronecker delta, but are directly computed in every instance.

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