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Beta decay of nuclide (56)Fe,(56)Co,(56)Ni,(56)Mn,(56)Cr and(56)V due to strong electron screening in stellar interiors
引用本文:刘晶晶.Beta decay of nuclide (56)Fe,(56)Co,(56)Ni,(56)Mn,(56)Cr and(56)V due to strong electron screening in stellar interiors[J].中国物理 C,2010,34(11):1700-1703.
作者姓名:刘晶晶
作者单位:College of Science and Technology, Qiongzhou University, Sanya 572022, China
基金项目:Supported by Natural Science Foundation of Hainan Province (109004); Institution of Higher Education Scientific Research and Foundation of Hainan Provincial Education Department (Hjkj 2010–42); Institution of Higher Education Special Foundation of Sanya (YD09047)
摘    要:According to a new electron screening theory,we discuss the beta decay rates of nuclide 56Fe,56Co,56Ni,56Mn,56Cr and 56V with and without strong electron screening (SES).The results show that SES has only a slight effect on the beta decay rates for ρ/μe 108 g/cm3.However the beta decay rates would be influenced greatly for ρ/μe 108 g/cm3.Due to SES,the maximum values of the C-factor (in %) on beta decay rates of 56Fe,56Co,56Ni,56Mn,56Cr and 56V is of the order of 95.03%,35.02%,98.05%,80.33%,98.30% and 98.71% at T9 = 4.0 and 98.83%,98.89%,99.65%,10.32%,4.10% and 40.21% at T9 = 7.0,respectively.

关 键 词:电子屏蔽  核素  β衰变  恒星  衰变率  屏蔽理论    
收稿时间:2009-12-22
修稿时间:2010-7-20
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