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Ab-Initio Method for X-Ray Absorption Spectra Simulation of Hydride Molecular Ions

机译:氢化物分子离子X射线吸收光谱法模拟AB-Initio方法

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Soft X-ray absorption spectra of molecular ions are important data for the modeling and understanding of laboratory and astrophysical plasma. In this work, we present an ab-initio method, based on the Configuration Interaction (CI) approach, for the calculations of energy positions and oscillator strengths of X-ray absorption spectra. Furthermore, we investigate the effects of the choice of the nature and number of spin-orbitals used in the CI expansion on the spectra. The method is applied on three hydride molecular ions, namely CH~+, OH~+ and SiH~+. However, the approach proposed here is general and may thus be applied to any kind of molecular ions.
机译:分子离子的软X射线吸收光谱是对实验室和天体物理等离子体的建模和理解的重要数据。在这项工作中,我们提出了一种基于配置交互(CI)方法的AB-Initio方法,用于计算X射线吸收光谱的能量位置和振荡器强度。此外,我们研究了CI扩展在光谱上使用的旋转轨道性质和旋转轨道数量的影响。该方法施加在三个氢化物分子离子上,即CH〜+,OH〜+和SIH〜+。然而,这里所提出的方法是一般的,因此可以应用于任何种类的分子离子。

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