Inner-shell excitation energy levels, and radiative and Auger transitions of B-like nitrogen

Inner-shell excitation energy levels, and radiative and Auger transitions of B-like nitrogen
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B 类氮的内壳层激发能级以及辐射和俄歇跃迁

DOI:
10.1139/cjp-2016-0298
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发表时间:
2016-07
影响因子:
1.2
通讯作者:
Zhang Chunmei
Zhang Chunmei
中科院分区:
物理与天体物理4区
文献类型:
--
作者:
Chen Chao;Gou Bingcong;Zhang Chunmei

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用鞍点变分和鞍点复转方法计算了类B氮的1s2s22p2,1s2s22p3p,1s2s2p3,1s2p4和1s2p33p2,4L(L=S,P,D)的内壳层激发能级、辐射跃迁和俄歇跃迁。用一阶微扰理论计算相对论和质量极化修正。这些共振的自电离能级、辐射跃迁速率和波长、俄歇速率和俄歇电子能量与文献中的理论和实验数据符合得很好,将为未来的天体物理和等离子体物理提供有价值的背景数据。
Inner-shell excitation energy levels, and radiative and Auger transitions of the 1s2s22p2, 1s2s22p3p, 1s2s2p3, 1s2p4, and 1s2p33p 2,4L (L = S, P, D) resonances for B-like nitrogen are calculated using the saddle-point variation and saddle-point complex-rotation methods. The first-order perturbation theory is used to calculate relativistic and mass polarization corrections. Present autoionization energy levels, radiative transition rates and wavelengths, Auger rates, and Auger electron energies for these resonances agree well with theoretical and experimental data available in the literature, and will provide valuable background data for astrophysics and plasma physics in future.
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