Randomized trial demonstrates improved exchange energy calculations in atoms and solids, suggesting enhanced accuracy in electronic structure modeling.
The electronic exchange energy as a functional of the density may be approximated as Eₓ[n]=Aₓ∫d³rn4/3F(s), where s=|∇n|2kFn, kF=(3π²n)1/3, and F(s)=(1+1.296s²+14s⁴+0.2s⁶)1/15. The basis for this approximation is the gradient expansion of the exchange hole, with real-space cutoffs chosen to guarantee that the hole is negative everywhere and represents a deficit of one electron. Unlike the previously publsihed version of it, this functional is simple enough to be applied routinely in self-consistent calculations for atoms, molecules, and solids. Calculated exchange energies for atoms fall within 1% of Hartree-Fock values. Significant improvements over other simple functionals are also found in the exchange contributions to the valence-shell removal energy of an atom and to the surface energy of jellium within the infinite barrier model.
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Perdew et al. (1986) studied this question.
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