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Neutron Spectroscopic Factors of ^7Li and Astrophysical ^6Li(n,γ)^7Li Reaction Rates
引用本文:苏俊,李志宏,郭冰,白希祥,李志常,刘建成,王友宝,连钢,曾晟,王宝祥,颜胜权,李云居,李二涛,樊启文,柳卫平.Neutron Spectroscopic Factors of ^7Li and Astrophysical ^6Li(n,γ)^7Li Reaction Rates[J].中国物理快报,2010(5):54-57.
作者姓名:苏俊  李志宏  郭冰  白希祥  李志常  刘建成  王友宝  连钢  曾晟  王宝祥  颜胜权  李云居  李二涛  樊启文  柳卫平
作者单位:China Institute of Atomic Energy, PO Box 275(10), Beijing 102413
基金项目:Supported by the National Basic Research Program of China under Grant No 2007CB815003, the National Natural Science Foundation of China under Grant Nos 10675173, 10720101076, 10735100 and 10975193.
摘    要:Angular distributions of the ^7Li(^6Li, ^6Li)^7Li elastic scattering and the ^7Li(^6Li, ^7Lig.s.)^6Li, ^7Li(^6Li, ^7Li0.48)^6Li transfer reactions at Ec.m. = 23.7 MeV are measured with the Q3D magnetic spectrograph. The optical potential of ^6Li + ^7Li is obtained by fitting the elastic scattering differential cross sections. Based on the distorted wave Born approximation (DWBA) analysis, spectroscopic factors of ^7Li =^6Li n are determined to be 0.73 ± 0.05 and 0.90 ± 0.09 for the ground and first exited states in ^7Li, respectively. Using the spectroscopic factors, the cross sections of the ^6 Li(n, γ0,1)^7 Li direct neutron capture reactions and the astrophysical ^6Li(n, γ)^7 Li reaction rates are derived.

关 键 词:天体物理学  反应率  光谱  弹性散射微分截面  中子  扭曲波玻恩近似  Q3D磁谱仪  转移反应
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