Relativistic Core-Valence-Separated Molecular Mean-Field Exact-Two-Component Equation-of-Motion Coupled Cluster Theory: Applications to L-edge X-ray Absorption Spectroscopy
Samragni Banerjee, Run R. Li, Brandon C. Cooper, Tianyuan Zhang, Edward F. Valeev, Xiaosong Li, A. Eugene DePrince
TL;DR
This work develops a fully relativistic core-valence-separated equation-of-motion CCSD method within the molecular mean-field X2C framework (CVS-DCB-X2C-EOM-CCSD) to predict L-edge X-ray absorption spectra. By solving the Dirac–Coulomb–Breit problem and projecting onto a two-component space, the approach incorporates scalar and spin–orbit relativistic effects and restricts excitations to core-like configurations, enabling accurate predictions of peak energies, splittings, and intensities across first-row transition-metal complexes. Against experimental data and relativistic TDDFT benchmarks, the method shows improved accuracy in energy shifts and spectral shapes, with basis-set recontraction proving robust. Limitations remain in high-density regions where higher-order (triples and beyond) correlation and more complete basis sets are needed, guiding future extensions toward even more reliable core-excitation spectroscopy.
Abstract
L-edge X-ray absorption spectra for first-row transition metal complexes are obtained from relativistic equation-of-motion singles and doubles coupled-cluster (EOM-CCSD) calculations that make use of the core-valence separation (CVS) scheme, with scalar and spin--orbit relativistic effects modeled within the molecular mean-field exact two-component (X2C) framework. By incorporating relativistic effects variationally at the Dirac--Coulomb--Breit (DCB) reference level, this method delivers accurate predictions of L-edge features, including energy shifts, intensity ratios, and fine-structure splittings, across a range of molecular systems. Benchmarking against perturbative spin--orbit treatments and relativistic TDDFT highlights the superior performance and robustness of the CVS-DCB-X2C-EOM-CCSD approach, including the reliability of basis set recontraction schemes. While limitations remain in describing high-density spectral regions, our results establish CVS-DCB-X2C-EOM-CCSD as a powerful and broadly applicable tool for relativistic core-excitation spectroscopy.
