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Vertical ionization energies from inverse generalized Kohn-Sham calculations at fixed electron density

Published 15 Oct 2026 in physics.chem-ph | (2610.22024v1)

Abstract: The exact Kohn--Sham (KS) system must have its highest occupied orbital energy equal to the negative of the lowest vertical ionization energy (VIE). No comparable theorem connects the deeper occupied levels εk\varepsilon_k to the higher VIEs IkI_k. Chong, Gritsenko and Baerends (CGB) established empirically that Ik+εk∝εHOMO−εkI_k + \varepsilon_k\propto\sqrt{\varepsilon_{\mathrm{HOMO}}-\varepsilon_k}. We ask whether a similar relation holds for the exact generalized Kohn-Sham (GKS) system, which incorporates a fraction αα of Hartree-Fock exchange. We invert near-exact CCSD/aug-cc-pVQZ ground-state densities of LiH, LiF, H2_2O, HF, CO, N2_2 and F2_2 at α=0,0.25,0.5,0.75,1.0α= 0, 0.25, 0.5, 0.75, 1.0 and obtain the exact GKS systems at each admixture. As the density is held fixed and only the operator is varied, the resulting occupied spectra separate the effect of exact-exchange admixture on orbital energies from its effect on the density, two contributions inseparable in a self-consistent hybrid calculation. The CGB relation holds broadly across the family, with a proportionality coefficient linear in αα, c(α)=c(0)−sαc(α)=c(0)-sα, where c(0)=1.185±0.017c(0)=1.185\pm0.017 eV<sup>1/2<sup>{1/2} and s=1.987±0.041s=1.987\pm0.041 eV<sup>1/2<sup>{1/2}, with R<sup>2≥0.9996R<sup>{2}\ge0.9996 for H2_2O, CO, HF and N2_2. Using the response-potential matrix elements tabulated by Gritsenko, Braïda and Baerends, we decompose the CGB coefficient into response and spectroscopic parts, and find ss to agree with the homogeneous-electron-gas step-height coefficient Kg=1.9932K_g = 1.9932 eV<sup>1/2<sup>{1/2}, which we conjecture is its origin. The coefficient vanishes at α<sup>∗=0.597±0.008α<sup>{*}=0.597\pm0.008. At α<sup>∗α<sup>{*} the HOMO-referenced GKS occupied levels satisfy εk≈−Ik\varepsilon_k\approx-I_k across the whole occupied range. The zero crossing is fixed by the core orbitals; in the outer valence the CGB coefficient is already indistinguishable from zero at α=0α=0.

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