论文标题
从头开始计算XUV地面和激发态的第一行过渡金属氧化物
Ab Initio Calculations of XUV Ground and Excited States for First-Row Transition Metal Oxides
论文作者
论文摘要
由于对载体职业的敏感性以及局部化学或结构动力学的敏感性,瞬态X射线光谱已无处不在研究太阳能材料的光激发动力学。但是,核心孔扰动和由此产生的多体动力学的解释使固态光激发动力学的解释变得复杂。在这里,开发了一种从头算,伯特 - 盐的方程式(BSE)方法,可以结合光激发固态材料的状态效应。地面,光激发和热膨胀状态的极端紫外线(XUV)吸收光谱 - $ tiO_2,α-CR_2O_3,β-MNO_2,α-fe_2o_3,co_3o_4,co_3o_4,nio,cuo,cuo和zno $ - 是为了证明该方法的准确性,该方法是准确的。该理论用于将所研究的每种过渡金属氧化物分解为X射线过渡汉密尔顿X射线转变的单独成分。分解提供了有关XUV光谱特征的起源以及光启示后光谱将如何变化的物理直觉。该方法很容易被推广到其他K,L,M和N边缘,以提供分析瞬态X射线吸收或反射数据的一般方法。
Transient X-ray spectroscopies have become ubiquitous in studying photoexcited dynamics in solar energy materials due to their sensitivity to carrier occupations and local chemical or structural dynamics. The interpretation of solid-state photoexcited dynamics, however, is complicated by the core-hole perturbation and the resulting many-body dynamics. Here, an ab initio, Bethe-Salpeter equation (BSE) approach is developed that can incorporate photoexcited state effects for solid-state materials. The extreme ultraviolet (XUV) absorption spectra for the ground, photoexcited, and thermally expanded states of first row transition metal oxides - $TiO_2, α-Cr_2O_3, β-MnO_2, α-Fe_2O_3, Co_3O_4, NiO, CuO, and ZnO$ - are calculated to demonstrate the accuracy of this approach. The theory is used to decompose the core-valence excitons into the separate components of the X-ray transition Hamiltonian for each of the transition metal oxides investigated. The decomposition provides a physical intuition about the origins of XUV spectral features as well as how the spectra will change following photoexcitation. The method is easily generalized to other K, L, M, and N edges to provide a general approach for analyzing transient X-ray absorption or reflection data.