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精确双组分 TDDFT 与简单的双电子图像变化校正:四分量质量在双组分成本下的 L 和 M 边缘附近的 X 射线吸收光谱。

Exact Two-Component TDDFT with Simple Two-Electron Picture-Change Corrections: X-ray Absorption Spectra Near L- and M-Edges of Four-Component Quality at Two-Component Cost.

机构信息

Hylleraas Centre for Quantum Molecular Sciences, Department of Chemistry, UiT The Arctic University of Norway, N-9037Tromsø, Norway.

Center for Free Electron Laser Science, Max Planck Institute for the Structure and Dynamics of Matter, Luruper Chaussee 149, 22761Hamburg, Germany.

出版信息

J Phys Chem A. 2023 Feb 9;127(5):1360-1376. doi: 10.1021/acs.jpca.2c08307. Epub 2023 Feb 1.

DOI:10.1021/acs.jpca.2c08307
PMID:36722848
原文链接:https://pmc.ncbi.nlm.nih.gov/articles/PMC9923756/
Abstract

X-ray absorption spectroscopy (XAS) has gained popularity in recent years as it probes matter with high spatial and elemental sensitivities. However, the theoretical modeling of XAS is a challenging task since XAS spectra feature a fine structure due to scalar (SC) and spin-orbit (SO) relativistic effects, in particular near L and M absorption edges. While full four-component (4c) calculations of XAS are nowadays feasible, there is still interest in developing approximate relativistic methods that enable XAS calculations at the two-component (2c) level while maintaining the accuracy of the parent 4c approach. In this article we present theoretical and numerical insights into two simple yet accurate 2c approaches based on an (extended) atomic mean-field exact two-component Hamiltonian framework, (e)amfX2C, for the calculation of XAS using linear eigenvalue and damped response time-dependent density functional theory (TDDFT). In contrast to the commonly used one-electron X2C (1eX2C) Hamiltonian, both amfX2C and eamfX2C account for the SC and SO two-electron and exchange-correlation picture-change (PC) effects that arise from the X2C transformation. As we demonstrate on L- and M-edge XAS spectra of transition metal and actinide compounds, the absence of PC corrections in the 1eX2C approximation results in a substantial overestimation of SO splittings, whereas (e)amfX2C Hamiltonians reproduce all essential spectral features such as shape, position, and SO splitting of the 4c references in excellent agreement, while offering significant computational savings. Therefore, the (e)amfX2C PC correction models presented here constitute reliable relativistic 2c quantum-chemical approaches for modeling XAS.

摘要

X 射线吸收光谱学(XAS)近年来越来越受欢迎,因为它具有高空间和元素灵敏度,可以探测物质。然而,XAS 的理论建模是一项具有挑战性的任务,因为 XAS 光谱由于标量(SC)和自旋轨道(SO)相对论效应而具有精细结构,特别是在 L 和 M 吸收边缘附近。虽然现在可以进行全四分量(4c)的 XAS 计算,但仍然有兴趣开发近似相对论方法,以便在保持 4c 方法准确性的同时,在两分量(2c)水平上进行 XAS 计算。在本文中,我们提出了基于(扩展)原子平均场精确两分量哈密顿量框架(e)amfX2C 的两种简单而精确的 2c 方法的理论和数值见解,用于使用线性本征值和阻尼响应时间相关密度泛函理论(TDDFT)计算 XAS。与常用的单电子 X2C(1eX2C)哈密顿量不同,amfX2C 和 eamfX2C 都考虑了 SC 和 SO 双电子和交换相关图变化(PC)效应,这些效应来自于 X2C 变换。正如我们在过渡金属和锕系化合物的 L 和 M 边缘 XAS 光谱上所证明的那样,在 1eX2C 近似中没有 PC 校正会导致 SO 分裂的大幅高估,而(e)amfX2C 哈密顿量则以极好的一致性再现了所有重要的光谱特征,例如形状、位置和 4c 参考的 SO 分裂,同时提供了显著的计算节省。因此,这里提出的(e)amfX2C PC 校正模型构成了用于模拟 XAS 的可靠相对论 2c 量子化学方法。

https://cdn.ncbi.nlm.nih.gov/pmc/blobs/752f/9923756/7b41b7929c87/jp2c08307_0006.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/752f/9923756/a02700a520e9/jp2c08307_0001.jpg
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https://cdn.ncbi.nlm.nih.gov/pmc/blobs/752f/9923756/1fbe4b2c3ca3/jp2c08307_0003.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/752f/9923756/f5595393316a/jp2c08307_0004.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/752f/9923756/e5eedca78bec/jp2c08307_0005.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/752f/9923756/7b41b7929c87/jp2c08307_0006.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/752f/9923756/a02700a520e9/jp2c08307_0001.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/752f/9923756/a6782461e1cd/jp2c08307_0002.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/752f/9923756/1fbe4b2c3ca3/jp2c08307_0003.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/752f/9923756/f5595393316a/jp2c08307_0004.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/752f/9923756/e5eedca78bec/jp2c08307_0005.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/752f/9923756/7b41b7929c87/jp2c08307_0006.jpg

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