标题:K-shell energy levels and radiative rates for transitions in Si XI
作者:Wei, H. G.; Shi, J. R.; Zhao, G.; Liang, Z. T.
作者机构:[Wei, H. G.; Liang, Z. T.] Shandong Univ, Sch Phys, Jinan 250100, Shandong, Peoples R China.; [Wei, H. G.; Shi, J. R.; Zhao, G.] Chinese Acad Sci, N 更多
通讯作者:Wei, H G
通讯作者地址:[Wei, HG]Shandong Univ, Sch Phys, Jinan 250100, Shandong, Peoples R China.
来源:ASTRONOMY & ASTROPHYSICS
出版年:2010
卷:522
期:8
DOI:10.1051/0004-6361/201014923
关键词:atomic data; atomic processes
摘要:Context. Atomic data for K-shell transitions are essential for modeling the K absorption lines, which have been observed in the spectra of active galaxies by high-resolution X-ray observatories, e. g. XMM, Chandra, and Suzaku. These accurate atomic data are also needed for line identifications and spectroscopic diagnostic of plasmas in laboratory generated by laser or beam-foil method.; Aims. We calculate atomic data using the atomic code flexible atomic code (FAC) taking relativistic effects and configuration interactions into account.; Methods. We calculate the K-shell transitions among the configurations of 1s(2)2s(2), 1s(2)2s2p, 1s(2)2p(2), 1s(2)2sn'l', 1s(2)2pn'l', 1s2s(2)2p, 1s2s2p(2), 1s2p(3), 1s2s2pn'l', and 1s2p(2)n'l', n' <= 4, l' <= n' for beryllium-like Si xi. We present the K-shell energy levels, wavelengths, radiative rates, and oscillator strengths for Si xi. To assess the accuracy of current data, we compare our results with both former experiments and other theoretical works.; Results. The present K-shell level energies and wavelengths are accurate to within 2 eV and 10 m angstrom, respectively. The radiative rates have an accuracy of around 20% for the majority of our transitions.
收录类别:EI;SCOPUS;SCIE
WOS核心被引频次:7
Scopus被引频次:6
资源类型:期刊论文
原文链接:https://www.scopus.com/inward/record.uri?eid=2-s2.0-78149439877&doi=10.1051%2f0004-6361%2f201014923&partnerID=40&md5=8632689533457fc11840736dd9f7c5f1
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