Determination of the Astrophysically Relevant 6Li(n, γ)7Li Cross Sections from the 7Li(6Li, 7Li)6Li Elastic-Transfer Reaction

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

doi:10.1088/1009-0630/14/5/03

Plasma Science and Technology > 2012 > 14(5): 364-366. > DOI: 10.1088/1009-0630/14/5/03

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

China Institute of Atomic Energy, Beijing 102413, China

Funds: supported by the National Basic Research Program of China (No 2007CB815003), National Natural Science Foundation of China (Nos.10675173, 10720101076, 10735100, 10975193).

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Received Date: May 16, 2011

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Abstract

Abstract

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.
- elastic-transfer reaction,
- spectroscopic factor,
- Big Bang nucleosynthesis

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