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【答案】应助回帖
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hf6391964: 金币+5, ★★★★★最佳答案, 非常感谢~~~~~ 2013-12-15 19:16:03
oven1986: 检索EPI+1, 感谢你的应助！ 2013-12-17 20:56:42
恭喜，EI收录了，SCI暂未收录
Accession number:
20134316877520
Title:
Plasma effect on the K α group emission of He-like molybdenum
Authors:
Hu, Feng1 ; Yang, Jiamin2
Author affiliation:
1School of Mathematic and Physical Science, Xuzhou Institute of Technology, Xuzhou 221400, China
2Research Center of Laser Fusion, China Academy of Engineering Physics, Mianyang 621900, China
Corresponding author:
Hu, F. (hufengscu@139.com)
Source title:
Radiation Effects and Defects in Solids
Abbreviated source title:
Radiat Eff Defects Solids
Volume:
168
Issue:
10
Issue date:
October 1, 2013
Publication year:
2013
Pages:
858-865
Language:
English
ISSN:
10420150
E-ISSN:
10294953
CODEN:
REDSEI
Document type:
Journal article (JA)
Publisher:
Taylor and Francis Inc., 325 Chestnut St, Suite 800, Philadelphia, PA 19106, United States
Abstract:
The intercombination line (1s2p(3P1)-1s2) and the resonance line (1s2p(1P1)-1s2) of He-like Mo, which are the two electronic dipole transitions in the Kα group emissions, are studied under dense plasma conditions by using the ion-sphere model combined with the multi-configuration Dirac-Fock model. The results show that the two electronic dipole transitions red shift nearly linearly with the increase in plasma electron density. Moreover, the red-shift energy becomes more sensitive to the plasma electron density, when the plasma electron temperature is lower. It is worth to note that the energy discrepancy between these two spectral lines is equal to the exchange energy of state 1s2p (3P1). This result may be useful to dense plasma diagnosis in connection with variation of the relative position and the spectral fine structure splitting in high-density plasmas. © 2013 Taylor & Francis. |
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