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Mixing of Degenerate Orbitals— First-Order Perturbations

1 Mixing of Degenerate Orbitals—First-Order Perturbations [Pg.845]

if we assume that S = 0, then lAE l = lAEI and closed-shell repulsion is undone. This may seem an unreasonable situation, but in fact many levels of theory make this approximation. As noted earlier in this chapter, most semi-empirical methods, such as AMI and MNDO, neglect overlap. As such, there is no closed-shell repulsion at these levels of theory, a serious deficiency in some situations. In contrast, for all its limitations, extended Hiickel theory (EHT) does not neglect overlap, and so closed-sheU repulsion survives. As discussed, classical Hiickel theory does neglect overlap. In fact, as previously noted, HMOT can be viewed as perturbation theory with S = 0, Haa = Hbb = a, and Hab = P. [Pg.845]




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Degenerate orbits

Degenerate perturbation

First-order mixing

First-order, degenerate mixing

Of degenerate

Orbital degenerate

Orbital first-order

Orbital order

Orbital perturbation

Orbital perturbed

Orbitally ordered

Orbitals degenerate

Orbitals perturbations

Ordered mixing

Ordering of orbitals

Perturbation degenerate orbitals

Perturbation first-order

Perturbation order

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