修正原子轨道理论框架下Ne原子离子的光离

I. Sakho
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引用次数: 1

摘要

我们报道了Ne中性原子系列的精确共振能量和宽度,分别为1s \({}^{2}\) p \({}^{6}\) n p \({}^{1}\) p \({}^{1}\)和1s \({}^{2}\) 2s2p \({}^{6}\) n p \({}^{1}\) p \({}_{1}\)。计算是在修正原子轨道理论(MAOT)框架下进行的。与舒尔茨等人的高同步辐射测量结果非常吻合。[物理][j]和Muller等人。天体物理学。[j].农业科学,2016,32(1)。所制表的高精度共振能可作为解释天体天体中Ne中性原子谱线的基准数据。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Photoionization of Ne Atom Ions in the Framework of the Modified Atomic Orbital Theory
We report accurate resonance energies and width of the 1s2s\({}^{2}\)p\({}^{6}\) n p \({}^{1}\)P\({}^{1}\) and 1s\({}^{2}\)2s2p\({}^{6}\) n p \({}^{1}\)P\({}_{1}\) series of Ne neutral atom. Calculations are performed in the framework of the Modified atomic orbital theory (MAOT). Excellent agreements is obtained with high synchrotron radiation measurements of Schulz et al . [ Phys. Rev. A 54 , 3095 (1996)] and of Muller et al . [ Astrophys. J. 836 , 166 (2017)]. The high lying accurate resonance energies tabulated may be benchmarked data for interpreting spectra lines of Ne neutral atom from astrophysical objects.
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