论文标题

有效核心兴奋的状态轨道观点,可以计算X射线吸收过渡的确定性框架

Efficient core-excited state orbital perspective on calculating X-ray absorption transitions in determinant framework

论文作者

Roychoudhury, Subhayan, Prendergast, David

论文摘要

X射线吸收光谱(XAS)是对材料无人电子结构的明确探针,也是用于指纹各种电子特性和现象的宝贵工具。因此,能够模拟和分析此类光谱的计算方法非常需要补充实验结果并从中提取有价值的见解。特别是,最近提出的第一原理方法标题为“多体XAS(MBXA)”,该方法将最终(初始)状态近似为由Kohn-Sham(KS)轨道构建的Slater决定因素,该轨道在不存在相关核心孔的情况下优化了(存在),在评估过渡增长的情况下显示出了有希望的前景。在本文中,我们表明可以使用完全以核心兴奋的状态KS轨道表示的过渡操作员来重新验证MBXAS方法,并且这种重新构造具有实践实践和概念上的优势。除了规避相对于未占地地面轨道数量的先前收敛性问题外,上述表示形式通过完全不必要的不​​必要的计算来减少计算费用。重新经过的方法还提供了一种直接的途径,可以将多体近似与所谓的单粒子处理进行比较,并表明在观察到的XAS XAS强度的相对重要性是由核心激发引起的子空间占据的子空间。最后,使用核心兴奋的状态基础,我们将辅助轨道定义用于X射线吸收,并通过将它们与单粒子近似与激发态进行对比来说明它们在解释光谱强度时的效用。

X-ray absorption spectroscopy (XAS) is an explicit probe of the unoccupied electronic structure of materials and an invaluable tool for fingerprinting various electronic properties and phenomena. Computational methods capable of simulating and analysing such spectra are therefore in high demand for complementing the experimental results and for extracting valuable insights therefrom. In particular, a recently proposed first-principles approach titled Many-Body XAS (MBXAS), which approximates the final (initial) state as a Slater determinant constructed from Kohn-Sham (KS) orbitals optimized in absence (presence) of the relevant core-hole has shown promising prospects in evaluating the transition amplitudes. In this article, we show that the MBXAS approach can be rederived using a transition operator expressed entirely in the basis of core-excited state KS orbitals and that this reformulation offers substantial practical and conceptual advantages. In addition to circumventing previous issues of convergence with respect to the number of unoccupied ground-state orbitals, the aforementioned representation reduces the computational expense by rendering the calculation of such orbitals unnecessary altogether. The reformulated approach also provides a direct pathway for comparing the many-body approximation with the so-called single-particle treatment and indicates the relative importance in observed XAS intensity of the relaxation of the valence occupied subspace induced by the core excitation. Finally, using the core-excited state basis, we define auxiliary orbitals for x-ray absorption and demonstrate their utility in explaining the spectral intensity by contrasting them with single-particle approximations to the excited state.

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