首页> 外文期刊>Journal of chemical theory and computation: JCTC >Ab Initio Wave Function-Based Determination of Element Specific Shifts for the Efficient Calculation of X-ray Absorption Spectra of Main Group Elements and First Row Transition Metals
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Ab Initio Wave Function-Based Determination of Element Specific Shifts for the Efficient Calculation of X-ray Absorption Spectra of Main Group Elements and First Row Transition Metals

机译:基于AB的初始波函数的元素特定变化的测定,用于高效计算主要组元素和第一行过渡金属的X射线吸收光谱

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In this study, a detailed calibration of the performance of modern ab initio wave function methods in the domain of X-ray absorption spectroscopy (XAS) is presented. It has been known for some time that for a given level of approximation, for example, using time-dependent density functional theory (TD-DFT) in conjunction with a given basis set, there are systematic deviations of the calculated transition energies from their experimental values that depend on the functional, the basis set, and the chosen treatment of scalar relativistic effects. This necessitates a linear correlation for a given element/functional/basis set combination to be established before chemical applications can be performed. This is a laborious undertaking since it involves sourcing trustworthy experimental data, lengthy geometry optimizations, and detailed comparisons between theory and experiment. In this work, reference values for the element-specific shifts of all the first-row transition metal atoms and the main group elements C, N, O, F, Si, P, S, and Cl have been computed by using a protocol that is based on the complete active space configuration interaction in conjunction with second-order N-electron valence state perturbation theory (CASCI/NEVPT2). It is shown that by extrapolating the results to the basis set limit of the method and taking into account scalar relativistic effects via the second-order Douglas-Kroll-Hess (DKH2) corrections, the predicted element shifts are on average less than 0.75 eV across all the absorption edges and a very good agreement between theory and experiment in all the studied XAS cases is observed. The transferability of these errors to molecular systems is thoroughly investigated. The constructed CASCI/NEVPT2 database of element shifts is used to evaluate the performance and to automatically calibrate prior to comparison with the experiment two commonly used methods in X-ray spectroscopy, namely, DFT/Restricted open shell configuration interaction singles (DFT/ROCIS) and TD-DFT methods.
机译:在本研究中,提出了在X射线吸收光谱(XAS)结构域中的现代AB初始波函数方法的性能的详细校准。已经知道,对于给定水平的近似,例如,使用时间相关的密度泛函理论(TD-DFT)与给定的基础集合,计算出的过渡能量与其实验有系统偏差依赖于函数,基础集和所选的标量相同效应的值。这需要在可以在进行化学应用之前建立给定元素/功能/基础集合的线性相关性。这是一个费力的事业,因为它涉及采购值得信赖的实验数据,冗长的几何优化,以及理论与实验之间的详细比较。在这项工作中,通过使用协议来计算所有第一行过渡金属原子和主组元素C,N,O,F,SI,P,S和CL的元素特定班次的参考值基于结合二阶N电子价扰动理论(Casci / Nevpt2)的完整活动空间配置交互。结果表明,通过将结果推断到该方法的基础设定极限,并考虑到通过二阶Douglas-Kroll-Hess(DKH2)校正来考虑标量相对论效应,预测元件偏移平均小于0.75 eV观察到所有研究和实验之间的所有吸收边缘和非常良好的一致性。彻底研究了这些误差对分子系统的可转移性。元素换档的构建Casci / Nevpt2数据库用于评估性能并在与实验中的实验中的两个常用方法进行比较之前自动校准,即DFT /限制开放壳配置交互单打(DFT / Rocis)和TD-DFT方法。

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