Atomic structure and transition parameters of the V XVIII carbon-like ion

IF 0.4 4区 物理与天体物理 Q4 ASTRONOMY & ASTROPHYSICS
L. Abu El Maati, M. Ahmad, I. S. Mahmoud, S. Tawfik, N. Alwadii, N. Ben Nessib, M. Dimitrijević
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引用次数: 0

Abstract

. The atomic and transition parameters of carbon-like ions are sig-nificant for many important astrophysical researches, such as the modeling of stellar atmospheres, the determination of stellar abundance, the analysis of spectral lines for laboratory plasmas or astronomical objects. In this contri-bution, we calculated the energy levels and lifetimes of the carbon-like vanadium ion (V XVIII) using the atomic structure codes AUTOSTRUCTURE and GRASP2018. Weighted oscillator strengths and transition probabilities are also calculated for the allowed transitions between the energy levels considered. The calculations were carried out for the first 17 configurations: 2s 2 2p 2 , 2p 4 , 2s 2 2p3p, 2s2p 2 3s, 2s2p 2 3d, 2p 3 3p, 2s 2 2p4p, 2s 2 3d 2 , 2s2p 3 , 2s 2 2p3s, 2s 2 2p3d, 2s2p 2 3p, 2p 3 3s, 2p 3 3d, 2s 2 2p4s, 2s 2 2p4d and 2s2p3d 2 .
XVIII类碳离子的原子结构和跃迁参数
. 类碳离子的原子和跃迁参数对于许多重要的天体物理研究都具有重要意义,例如恒星大气的建模、恒星丰度的测定、实验室等离子体或天体的光谱线分析。在这篇文章中,我们使用原子结构代码AUTOSTRUCTURE和GRASP2018计算了类碳钒离子(V XVIII)的能级和寿命。加权振荡强度和跃迁概率也计算了所考虑的能级之间的允许跃迁。对前17种构型进行了计算:2s 22p 2、2p4、2s 2p3p、2s 22p 23s、2s 22p 23d、2p 33p、2s 22p4p、2s 23d、2s 22p 3、2s 2p3s、2s2p3d、2s 22p 23p、2p 33s、2p 33d、2s 22p4s、2s 2p4d和2s2p3d 2。
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来源期刊
CiteScore
1.10
自引率
20.00%
发文量
4
审稿时长
>12 weeks
期刊介绍: Contributions of the Astronomical Observatory Skalnate Pleso" (CAOSP) is published by the Astronomical Institute of the Slovak Academy of Sciences (SAS). The journal publishes new results of astronomical and astrophysical research, preferentially covering the fields of Interplanetary Matter, Stellar Astrophysics and Solar Physics. We publish regular papers, expert comments and review contributions.
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