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Essentials of Computational Chemistry

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5.3 CNDO FORMALISM 137<br />

Thus, the only integrals that are non-zero have µ and ν as identical orbitals on the<br />

same atom, and λ and σ also as identical orbitals on the same atom, but the second<br />

atom might be different than the first (the decision to set to zero any integrals involving<br />

overlap <strong>of</strong> different basis functions gives rise to the model name).<br />

4. For the surviving two-electron integrals,<br />

(µµ|λλ) = γAB<br />

(5.6)<br />

where A and B are the atoms on which basis functions µ and λ reside, respectively. The<br />

term γ can either be computed explicitly from s-type STOs (note that since γ depends<br />

only on the atoms A and B, (sAsA|sBsB) = (p A p A |sBsB) = (p A p A |p B p B ), etc.) or it can<br />

be treated as a parameter. One popular parametric form involves using the so-called<br />

Pariser–Parr approximation for the one-center term (Pariser and Parr 1953).<br />

γAA = IPA − EAA<br />

(5.7)<br />

where IP and EA are the atomic ionization potential and electron affinity, respectively.<br />

For the two-center term, the Mataga–Nishimoto formalism adopts<br />

γAB =<br />

γAA + γBB<br />

2 + rAB(γAA + γBB)<br />

(5.8)<br />

where rAB is the interatomic distance (Mataga and Nishimoto 1957). Note the intuitive<br />

limits on γ in Eq. (5.8). At large distance, it goes to 1/rAB, as expected for widely<br />

separated charge clouds, while at short distances, it approaches the average <strong>of</strong> the two<br />

one-center parameters.<br />

5. One-electron integrals for diagonal matrix elements are defined by<br />

<br />

<br />

<br />

µ <br />

−1<br />

2 ∇2 − <br />

<br />

<br />

Zk <br />

<br />

µ<br />

<br />

=−IPµ − <br />

(Zk − δZAZk )γAk<br />

k<br />

rk<br />

k<br />

(5.9)<br />

where µ is centered on atom A. Equation (5.9) looks a bit opaque at first glance, but<br />

it is actually quite straightforward. Remember that the full Fock matrix element Fµµ is<br />

the sum <strong>of</strong> the one-electron integral Eq. (5.9) and a series <strong>of</strong> two-electron integrals. If<br />

the number <strong>of</strong> valence electrons on each atom is exactly equal to the valence nuclear<br />

charge (i.e., every atom has a partial atomic charge <strong>of</strong> zero) then the repulsive twoelectron<br />

terms will exactly cancel the attractive nuclear terms appearing at the end <strong>of</strong><br />

Eq. (5.9) and we will recapture the expected result, namely that the energy associated<br />

with the diagonal matrix element is the ionization potential <strong>of</strong> the orbital. The Kronecker<br />

delta affecting the nuclear charge for atom A itself simply avoids correcting for a nonexistent<br />

two-electron repulsion <strong>of</strong> an electron in basis function µ with itself. (Removing<br />

the attraction to nuclei other than A from the r.h.s. <strong>of</strong> Eq. (5.9) defines a commonly<br />

tabulated semiempirical parameter that is typically denoted Uµ.)

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