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Resonance reaction rate of 21Na(p, γ)22Mg
引用本文:刘宏林,刘门全,刘晶晶,罗志全. Resonance reaction rate of 21Na(p, γ)22Mg[J]. 中国物理, 2007, 16(11): 3300-3304
作者姓名:刘宏林  刘门全  刘晶晶  罗志全
作者单位:Institute of Theoretical Physics, China West Normal University,Nanchong 637002, China
基金项目:Project supported by the National Natural Science Foundation of China (GrantNo~10347008), the Scientific Research and Fund of Sichuan ProvincialEducation Department of China (Grant No~2006A079) and the Science and TechnologicalFoundation of China West
摘    要:By using the new Coulomb screening model and most recent experimental results, this paper calculates the resonance reaction rates of ^21Na(p,γ)^22Mg. The derived result shows that the effect of electron screening on resonant reaction is prominent in astrophysical interesting temperature range. In conjunction with the experimental results, the recommended rates of^21Na(p,γ)^22 Mg would increase at least 10%, which undoubtedly affect the nucleosynthesis of some heavier nuclei in a variety of astrophysical sites.[第一段]

关 键 词:电子筛选 谐振 反作用率 核合成
文章编号:1009-1963/2007/16(11)/3300-05
修稿时间:2007-01-17

Resonance reaction rate of 21Na(p, γ)22Mg
Liu Hong-Lin,Liu Men-Quan,Liu Jing-Jing and Luo Zhi-Quan. Resonance reaction rate of 21Na(p, γ)22Mg[J]. Chinese Physics, 2007, 16(11): 3300-3304
Authors:Liu Hong-Lin  Liu Men-Quan  Liu Jing-Jing  Luo Zhi-Quan
Affiliation:Institute of Theoretical Physics, China West Normal University, Nanchong 637002, China
Abstract:
Keywords:electron screening   nucleosynthesis   O-Ne nova   x-ray bursts   supernovae
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