Perturbation theory, up to first order in the wave function and second order in the energy, is formulated for a many-electron system without requiring the perturbed one-electron states to be orthogonal. The most general self-consistent coupled equations, referred to as Method 1, form the counterpart of Langhoff, Karplus, and Hurst's (LKH) Method a for orthogonal orbitals. The uncoupling of the perturbations δψᵢ, δψⱼ to the zero order wave functions ψᵢ⁰ and ψⱼ⁰ produces equations referred to as Method 2. Further approximation in the Method-2 equations yields a set of equations called Method 3. Methods 2 and 3 are counterparts of LKH's Method b, but have computational advantages over Method b in that normalization and orthogonalization are accomplished in a particularly simple fashion. In comparing the uncoupled Method-3 equations with Dalgarno's equations, an additional difference is found involving the overlap integral between perturbed states, besides the difficulty pointed out by LKH. Application of the Method-2 and -3 equations is made to the spin-polarization problem of the Fe⁺³ ion, leading to a hyperfine constant in reasonable agreement with earlier unrestricted Hartree-Fock (UHF) calculations. A comparison between results obtained by Methods 2 and 3 and Dalgarno's equations permits a relative evaluation of these methods. We have also studied the effect of indirect spin polarization of the s electrons through the action of the p electrons which are in turn polarized by the unpaired d electrons. This contribution is found to be about 10% of the direct effect.
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Deff et al. (1968) studied this question.
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