Relativistic Orbital-Optimized Density Functional Theory forAccurate Core-Level Spectroscopy

被引:37
作者
Cunha, Leonardo A. [1 ,2 ]
Hait, Diptarka [1 ,2 ]
Kang, Richard [1 ,2 ]
Mao, Yuezhi [3 ]
Head-Gordon, Martin [1 ,2 ]
机构
[1] Univ Calif Berkeley, Kenneth S Pitzer Ctr Theoret Chem, Dept Chem, Berkeley, CA 94720 USA
[2] Lawrence Berkeley Natl Lab, Chem Sci Div, Berkeley, CA 94720 USA
[3] Stanford Univ, Dept Chem, Stanford, CA 94305 USA
关键词
X-RAY-ABSORPTION; 2P PHOTOELECTRON SHIFTS; COUPLED-CLUSTER METHODS; SULFUR K-EDGE; EXCITED-STATES; PHOTOABSORPTION SPECTRA; INNER-SHELL; ELECTRONIC-STRUCTURE; CHEMICAL-SHIFTS; HARTREE-FOCK;
D O I
10.1021/acs.jpclett.2c00578
中图分类号
O64 [物理化学(理论化学)、化学物理学];
学科分类号
070304 ; 081704 ;
摘要
Core-level spectra of 1s electrons of elements heavier than Ne showsignificant relativistic effects. We combine advances in orbital-optimized densityfunctional theory (OO-DFT) with the spin-free exact two-component (X2C) modelfor scalar relativistic effects to study K-edge spectra of third period elements. OO-DFT/X2C is found to be quite accurate at predicting energies, yielding a similar to 0.5 eV root-mean-square error versus experiment with the modern SCAN (and related) functionals. Thismarks a significant improvement over the >50 eV deviations that are typical for thepopular time-dependent DFT (TDDFT) approach. Consequently, experimental spectraare quite well reproduced by OO-DFT/X2C, sans empirical shifts for alignment. OO-DFT/X2C combines high accuracy with ground state DFT cost and is thus a promisingroute for computing core-level spectra of third period elements. We also explored K and Ledges of 3d transition metals to identify limitations of the OO-DFT/X2C approach inmodeling the spectra of heavier atoms.
引用
收藏
页码:3438 / 3449
页数:12
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