Practical post-Kohn-Sham methods for time-reversal symmetry breaking references

08 February 2023, Version 1
This content is a preprint and has not undergone peer review at the time of posting.

Abstract

Reduced scaling algorithms based on auxiliary subspace methods for correlation energies from the random phase approximation(RPA) as well as correlation self-energies from the GW method are derived for time-reversal symmetry breaking Kohn-Sham (KS) references. This allows for an efficient evaluation of RPA energies and GW quasiparticle energies for molecular systems with KS references that break time-reversal symmetry. The latter occur for example in magnetic fields. Furthermore, KS references for relativistic open-shell molecules also break time-reversal symmetry due to the single determinant ansatz used. Errors of the newly developed reduced-scaling algorithms are shown to be negligible compared to reference implementations, while the overall computational scaling is reduced by two orders of magnitude. Ionization energies obtained from the GW approximation are shown to be robust even for the electronically complicated group of trivalent lanthanoid ions. Starting from GW quasiparticle energies, it is subsequently shown that light-matter interactions of these systems can be calculated using the Bethe-Salpeter equation (BSE). Using the combined GW -BSE method, the absorption and emission spectra of a molecular europium(III) complex can be obtained including spin-orbit coupling.

Keywords

random phase approximation
time reversal symmetry
GW
excited states
lantahnoids
magnetic field
Bethe-Salpeter equation

Supplementary materials

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Supporting Information
Description
Reference and auxiliary subspace based RPA correlation energies and G0W0 correlation self-energies for 36 small organic molecules at 1000 tesla, detailed RPA and PBE0 energies of [Mn(taa)] from 0 to 150 tesla, evGW quasiparticle energies for trivalent lanthanoid ions, and the optimized structures of [Mn(taa)] (S = 1 and S = 2 states) and [Eu(PDCA)3 ]3+ in xyz format can be found .
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