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电子亲和能含时密度泛函理论:形式体系及其对芯激发态的应用

Electron-Affinity Time-Dependent Density Functional Theory: Formalism and Applications to Core-Excited States.

作者信息

Carter-Fenk Kevin, Cunha Leonardo A, Arias-Martinez Juan E, Head-Gordon Martin

机构信息

Kenneth S. Pitzer Center for Theoretical Chemistry, Department of Chemistry, University of California, Berkeley, California94720, United States.

Chemical Sciences Division, Lawrence Berkeley National Laboratory, Berkeley, California94720, United States.

出版信息

J Phys Chem Lett. 2022 Oct 20;13(41):9664-9672. doi: 10.1021/acs.jpclett.2c02564. Epub 2022 Oct 10.

Abstract

The lack of particle-hole attraction and orbital relaxation within time-dependent density functional theory (TDDFT) lead to extreme errors in the prediction of K-edge X-ray absorption spectra (XAS). We derive a linear-response formalism that uses optimized orbitals of the - 1-electron system as the reference, building orbital relaxation and a proper hole into the initial density. Our approach is an exact generalization of the static-exchange approximation that ameliorates the particle-hole interaction error associated with the adiabatic approximation and reduces errors in TDDFT XAS by orders of magnitude. With a statistical performance of just 0.5 eV root-mean-square error and the same computational scaling as TDDFT under the core-valence separation approximation, we anticipate that this approach will be of great utility in XAS calculations of large systems.

摘要

含时密度泛函理论(TDDFT)中粒子-空穴吸引和轨道弛豫的缺失,导致在预测K边X射线吸收光谱(XAS)时出现极大误差。我们推导了一种线性响应形式,它使用N - 1电子体系的优化轨道作为参考,在初始密度中构建轨道弛豫和一个适当的空穴。我们的方法是静态交换近似的精确推广,它改善了与绝热近似相关的粒子-空穴相互作用误差,并将TDDFT XAS中的误差降低了几个数量级。在芯价分离近似下,该方法的统计性能仅为0.5 eV的均方根误差,且具有与TDDFT相同的计算标度,我们预计这种方法在大体系的XAS计算中将具有很大的实用性。

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