Abstract
It is demonstrated that the challenging core hole-particle (CHP) orbital relaxation for core
electron spectra can be readily achieved by the mixed-reference spin-flip (MRSF)-TDDFT.
With the additional scalar relativistic effects on K-edge excitation energies of 24 second- and
17 third-row molecules, the particular ∆CHP-MRSF(R) exhibited near perfect predictions
with RMSE ∼ 0.5 eV, featuring a median value of 0.3 and and an interquartile range of 0.4.
Overall, the CHP effect is 2 ∼ 4 times stronger than relativistic ones, contributing more than 20 eV in the cases of sulfur and chlorine third-row atoms. Such high precision allows to explain the splitting and spectral shapes of O, N and C atom K-edges in the ground state of thymine with atom as well as orbital specific accuracy. The same protocol with a double hole particle relaxation also produced remarkably accurate K-edge spectra of core to valence hole excitation energies from the first (nO8π∗) and second (ππ∗) excited states of thymine, confirming the assignment of 1s → n excitation for the experimentally observed 526.4 eV peak. Regarding both accuracy and practicality, therefore, MRSF-TDDFT provides a promising protocol for core electron spectra both of ground and excited electronic states alike.
Supplementary materials
Title
Supporting Information: Mixed-Reference Spin-Flip Time-Dependent Density Functional Theory for Accurate X-ray Absorption Spectroscopy
Description
XAS C- O- and N- K-edge excitation energies from the ground state and the lowest two excited singlet states.
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