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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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作者 苏俊 李志宏 +12 位作者 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 《Plasma Science and Technology》 SCIE EI CAS CSCD 2012年第5期364-366,共3页
Angular distributions for the 7^Li(6^Li, 7^Li)6^Li elastic-transfer reaction have been measured with the Q3D magnetic spectrograph at the HI-13 tandem accelerator of Beijing, China. The neutron spectroscopic factors... Angular distributions for the 7^Li(6^Li, 7^Li)6^Li 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 7^Li are derived by comparing the calculated differential cross sections, which are 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 6^Li(n, γ)TLi at energies of astrophysical relevance. 展开更多
关键词 elastic-transfer reaction spectroscopic factor Big Bang nucleosynthesis
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