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SU Jun(苏 俊), LI Zhihong(李志宏), GUO Bing(郭冰), BAI Xixiang(白希祥), LI Zhichang(李志常), LIU Jiancheng(刘建成), WANG Youbao(王友宝), LIAN Gang(连钢), ZENG Sheng(曾 晟), WANG Baoxiang(王宝祥), YAN Shengquan(颜胜权), LI Yunju(李云居), et al. Determination of the Astrophysically Relevant 6Li(n, γ)7Li Cross Sections from the 7Li(6Li, 7Li)6Li Elastic-Transfer Reaction[J]. Plasma Science and Technology, 2012, 14(5): 364-366. DOI: 10.1088/1009-0630/14/5/03
Citation: SU Jun(苏 俊), LI Zhihong(李志宏), GUO Bing(郭冰), BAI Xixiang(白希祥), LI Zhichang(李志常), LIU Jiancheng(刘建成), WANG Youbao(王友宝), LIAN Gang(连钢), ZENG Sheng(曾 晟), WANG Baoxiang(王宝祥), YAN Shengquan(颜胜权), LI Yunju(李云居), et al. Determination of the Astrophysically Relevant 6Li(n, γ)7Li Cross Sections from the 7Li(6Li, 7Li)6Li Elastic-Transfer Reaction[J]. Plasma Science and Technology, 2012, 14(5): 364-366. DOI: 10.1088/1009-0630/14/5/03
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Determination of the Astrophysically Relevant 6Li(n, γ)7Li Cross Sections from the 7Li(6Li, 7Li)6Li Elastic-Transfer Reaction

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  • Angular distributions for the 7Li(6Li, 7Li)6Li elastic-transfer reaction have been measured with the Q3D magnetic spectrograph at the HI-13 tandem accelerator of Beijing, China. The neutron spectroscopic factors of 7Li are derived by comparing the calculated differential cross sections, which is obtained through the distorted-wave Born approximation (DWBA) calculation, to the experimental data. And these spectroscopic factors are then used to deduce the direct capture cross sections in 6Li(n, γ)7Li at energies of astrophysical relevance.
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