Relativistic configuration interaction calculations of energy levels, isotope shifts, hyperfine structures, and transition rates in the 2s22p2–2s2p3 transition array for the carbon-like sequence
Relativistic configuration interaction calculations of energy levels, isotope shifts, hyperfine structures, and transition rates in the 2s22p2–2s2p3 transition array for the carbon-like sequence
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DOI：
10.1088/0953-4075/43/7/074023
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发表时间：
2010-04
期刊：
影响因子：
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通讯作者：
P. Jönsson;J. Bieroń
中科院分区：
文献类型：
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作者：
P. Jönsson;J. Bieroń
报告了 N II、O III、F IV、Ne V 和 Ti XVII 中 2s22p2–2s2p3 跃迁阵列的能级、精细结构分离、特定质量位移参数、同位素位移、超精细相互作用常数、Landé gJ 因子和跃迁概率。使用多配置狄拉克-哈特里-福克方法确定波函数，并考虑化合价、核-化合价和核-核相关效应。将跃迁能量和速率与实验数据以及其他计算值进行比较。
Energy levels, fine-structure separations, specific mass shift parameters, isotope shifts, hyperfine interaction constants, Landé gJ-factors and transition probabilities are reported for the 2s22p2–2s2p3 transition array in N II, O III, F IV, Ne V and Ti XVII. Wavefunctions were determined using the multiconfiguration Dirac–Hartree–Fock method with account for valence, core-valence and core–core correlation effects. The transition energies and rates are compared with experimental data and with values from other calculations.