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Multi-configuration dirac-hartree-fock calculations of the transition rates of 2s(2)2p(2)-2s2p(3) and 2s2p(3)-2s(2)2pnl (n >= 3) e1 transitions of n+

文献类型:期刊论文

作者Shen, Xiaozhi1,2; Liu, Juan3,4; Zhou, Fuyang5
刊名Monthly notices of the royal astronomical society
出版日期2016-10-21
卷号462期号:2页码:1203-1214
关键词Atomic data Line: identification Methods: data analysis
ISSN号0035-8711
DOI10.1093/mnras/stw1648
通讯作者Shen, xiaozhi(shenxz@buaa.edu.cn)
英文摘要Wavefunctions were determined using the multi-configuration dirac-hartree-fock method. the core-core, core-valence, valence correlation, breit interaction and quantum electrodynamics effects, as well as some higher-order correlation effects, were considered to obtain accurate wavelengths (lambda), oscillator strengths (gf) and transition rates (a) of 2s(2)2p(2) - 2s2p(3), 2s2p(3) - 2s(2)2pnl (n >= 3) and 2s2p(3) - 2s2p(2)3s e1 transitions. the branching ratio of 2s2p(3) s-5(2)o (namely a(lambda 2143.45)/a(lambda 2139.68)) based on the latest calculation of 2.462 +/- 0.119 is recommended for the determination of a nebula's electron temperature and electron density. the largest calculated gf value of 2s2p(3) -2s(2)2p4p is lambda 630.65, differing from that of lambda 1060.2 (i.e. 2s2p(3) p-3(2)o - 2s(2)2p4p s-3(1)) that was observed with the largest intensities in the orion nebula spectrum. in addition, the energy levels and the splittings of 2s2p(3), the extremely difficult calculations of the rates of two-electron one-photon transitions as well as those of the very small intercombination a of 2s2p(3) s-5(2)o were studied in detail. because of the weak spin-orbit interaction, accurately calculating the levels p-3(1,2,0)o (or d-3(3,2,1)o) and their transition matrix elements is very sensitive to relativistic and electron correlation effects. a special case for this is when the transition operators synchronously applied to wavefunctions with regard to 2s2p(3) p-3(o) and 2s(2)2pnl (n = 4) become extremely sensitive to some higher-order correlation effects.
WOS关键词OSCILLATOR-STRENGTHS ; RADIATIVE LIFETIME ; AURORAL SPECTRUM ; METASTABLE STATE ; ORION NEBULA ; NII LINES ; PROBABILITIES ; NITROGEN ; PACKAGE
WOS研究方向Astronomy & Astrophysics
WOS类目Astronomy & Astrophysics
语种英语
WOS记录号WOS:000384674100005
出版者OXFORD UNIV PRESS
URI标识http://www.irgrid.ac.cn/handle/1471x/2375070
专题中国科学院大学
通讯作者Shen, Xiaozhi
作者单位1.Beihang Univ, Sch Phys & Nucl Energy Engn, Beijing 100191, Peoples R China
2.Handan Coll, Sch Mech & Elect Engn, Handan 056005, Peoples R China
3.Handan Coll, Sch Math & Phys, Handan 056005, Peoples R China
4.Renmin Univ China, Sch Informat, Beijing 100872, Peoples R China
5.Univ Chinese Acad Sci, Coll Mat Sci & Optoelect Technol, Beijing 100049, Peoples R China
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GB/T 7714
Shen, Xiaozhi,Liu, Juan,Zhou, Fuyang. Multi-configuration dirac-hartree-fock calculations of the transition rates of 2s(2)2p(2)-2s2p(3) and 2s2p(3)-2s(2)2pnl (n >= 3) e1 transitions of n+[J]. Monthly notices of the royal astronomical society,2016,462(2):1203-1214.
APA Shen, Xiaozhi,Liu, Juan,&Zhou, Fuyang.(2016).Multi-configuration dirac-hartree-fock calculations of the transition rates of 2s(2)2p(2)-2s2p(3) and 2s2p(3)-2s(2)2pnl (n >= 3) e1 transitions of n+.Monthly notices of the royal astronomical society,462(2),1203-1214.
MLA Shen, Xiaozhi,et al."Multi-configuration dirac-hartree-fock calculations of the transition rates of 2s(2)2p(2)-2s2p(3) and 2s2p(3)-2s(2)2pnl (n >= 3) e1 transitions of n+".Monthly notices of the royal astronomical society 462.2(2016):1203-1214.

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