Wavelengths of 2l→3l′ transitions in L-shell ions of iron and nickel:: A combined configuration interaction and many-body perturbation theory approach

被引:78
作者
Gu, MF [1 ]
机构
[1] Stanford Univ, Dept Phys, Stanford, CA 94305 USA
[2] Stanford Univ, Kavli Inst Particle Astrophys & Cosmol, Stanford, CA 94305 USA
关键词
atomic data; atomic processes;
D O I
10.1086/425915
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Using a combined configuration interaction and many-body perturbation theory approach, we calculate the level energies of 1s(2)2l(q) and 1s(2)2l(q-1)3l' (1less than or equal toqless than or equal to8) complexes in iron and nickel ions. Comparison of 1s(2)2l(q) energies with experimental results shows that the calculation is accurate to within similar to0.15 eV for these levels. The accuracy of 1s(2)2l(q-1)3l' energies can be slightly worse, at similar to0.5 eV. The theoretical wavelengths of 2-->3 transitions of iron ions are compared with the published experimental measurements, and discrepancies are found to be mostly within +/-10 mAngstrom. Similar accuracy is expected for wavelengths of nickel ions. Such accuracy is a significant improvement over that obtainable with standard configuration interaction methods. A complete table of 2l-->3l' transition wavelengths of all L-shell ions of iron and nickel is presented.
引用
收藏
页码:105 / 110
页数:6
相关论文
共 3 条
  • [1] Many-body perturbation theory wavelengths of high-n X-ray transitions of Fe and Ni L-shell ions
    Gu, M. F.
    ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES, 2007, 169 (01) : 154 - 158
  • [2] SYSTEMATIC CALCULATIONS OF ENERGY LEVELS AND TRANSITION RATES OF BE-LIKE IONS WITH Z=10-30 USING A COMBINED CONFIGURATION INTERACTION AND MANY-BODY PERTURBATION THEORY APPROACH
    Wang, K.
    Guo, X. L.
    Liu, H. T.
    Li, D. F.
    Long, F. Y.
    Han, X. Y.
    Duan, B.
    Li, J. G.
    Huang, M.
    Wang, Y. S.
    Hutton, R.
    Zou, Y. M.
    Zeng, J. L.
    Chen, C. Y.
    Yan, J.
    ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES, 2015, 218 (02)
  • [3] Laboratory measurements of iron L-shell emission:: 3→2 transitions of Fe XXI-XXIV between 10.5 and 12.5 Å
    Gu, MF
    Kahn, SM
    Savin, DW
    Behar, E
    Beiersdorfer, P
    Brown, GV
    Liedahl, DA
    Reed, KJ
    ASTROPHYSICAL JOURNAL, 2001, 563 (01) : 462 - 471