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arXiv 1303.4282physics.atom-ph
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镁离子的K壳层光吸收

K-Shell Photoabsorption of Magnesium Ions

M. F. Hasoglu, Sh. A. Abdel-Naby, E. Gatuzz, J. Garcia, T. R. Kallman, C. Mendoza, T. W. Gorczyca

摘要:

用$R$矩阵方法计算了所有镁离子的X射线光吸收截面。与其他可用的数据Mg II-Mg X的比较表明,在所得的共振形状良好的定性协议。然而,对于较低的电离阶段,特别是对于单电离的Mg II,由于忽略了重要的轨道弛豫效应,先前的$R$矩阵结果(Witthoeft et al.2009; Witthoeft et al.2011)高估了K边缘位置,因此这些截面的光子能量整体向下移动是有道理的。我们发现Mg I和Mg II的截面由于M-壳层($n=3$)占据而进一步复杂化。因此,使用基于多通道量子亏损理论和光学势的方法来处理$1s\rightarrow np$共振的旁观者俄歇衰变变得有问题,使得有必要实施中性Mg的俄歇衰变的替代近似处理。新的截面被用来拟合低质量X射线双星GS 1826-238的XMM-牛顿谱中的Mg K边缘,其中大部分星际Mg被发现是以电离形式存在的。

英文摘要:

X-ray photoabsorption cross sections have been computed for all magnesium ions using the $R$-matrix method. A comparison with the other available data for Mg II-Mg X shows good qualitative agreement in the resultant resonance shapes. However, for the lower ionization stages, and for singly-ionized Mg II in particular, the previous $R$-matrix results (Witthoeft et al.2009; Witthoeft et al. 2011) overestimate the K-edge position due to the neglect of important orbital relaxation effects, and a global shift downward in photon energy of those cross sections is therefore warranted. We have found that the cross sections for Mg I and Mg II are further complicated by the M-shell ($n=3$) occupancy. As a result, the treatment of spectator Auger decay of $1s\rightarrow np$ resonances using a method based on multichannel quantum defect theory and an optical potential becomes problematic, making it necessary to implement an alternative, approximate treatment of Auger decay for neutral Mg. The new cross sections are used to fit the Mg K edge in XMM-Newton spectra of the low-mass X-ray binary GS 1826-238, where most of the interstellar Mg is found to be in ionized form.

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