Energy levels, radiative rates and electron impact excitation rates for transitions in He-like Ti XXI, V XXII, Cr XXIII and Mn XXIV

被引:9
作者
Aggarwal, Kanti M. [1 ]
Keenan, Francis P. [1 ]
机构
[1] Queens Univ Belfast, Sch Math & Phys, Astrophys Res Ctr, Belfast BT7 1NN, Antrim, North Ireland
基金
英国工程与自然科学研究理事会;
关键词
HELIUM-LIKE IONS; DIAGNOSTIC APPLICATION; ASTROPHYSICAL PLASMAS; EMISSION-LINES; WAVELENGTHS; LIFETIMES; SPECTRA; FUSION; IRON;
D O I
10.1088/0031-8949/85/06/065301
中图分类号
O4 [物理学];
学科分类号
0702 ;
摘要
We report calculations of energy levels, radiative rates and electron impact excitation cross sections and rates for transitions in He-like Ti XXI, V XXII, Cr XXIII and Mn XXIV. grasp (general-purpose relativistic atomic structure package) is adopted for calculating energy levels and radiative rates. For determining the collision strengths and subsequently the excitation rates, the Dirac atomic R-matrix code (DARC) is used. Oscillator strengths, radiative rates and line strengths are reported for all E1, E2, M1 and M2 transitions among the lowest 49 levels of each ion. Additionally, theoretical lifetimes are listed for all the 49 levels of the above four ions. Collision strengths are averaged over a Maxwellian velocity distribution and the effective collision strengths obtained listed over a wide temperature range up to 10(7.5) K. Comparisons are made with similar data obtained using the flexible atomic code (FAC) to highlight the importance of resonances, included in calculations with DARC, in the determination of effective collision strengths. Discrepancies between the collision strengths from DARC and FAC, in particular for forbidden transitions, are also discussed. Finally, discrepancies between the present results for effective collision strengths with the DARC code and earlier semi-relativistic R-matrix data are noted over a wide range of electron temperatures for many transitions in all ions.
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页数:20
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