LI Er-Tao1, LI Zhi-Hong1**, SU Jun1, GUO Bing1, LI Yun-Ju1, YAN Sheng-Quan1, BAI Xi-Xiang1, WANG You-Bao1, WANG Bao-Xiang1, LIAN Gang1, ZENG Sheng1, FANG Xiao1, ZHAO Wei-Juan2, LIU Wei-Ping1
1China Institute of Atomic Energy, Beijing 102413 2Institute of Physical Engineering, Zhengzhou University, Zhengzhou 450052
Astrophysical Rates for the 6He(p, γ)7Li Reaction
LI Er-Tao1, LI Zhi-Hong1**, SU Jun1, GUO Bing1, LI Yun-Ju1, YAN Sheng-Quan1, BAI Xi-Xiang1, WANG You-Bao1, WANG Bao-Xiang1, LIAN Gang1, ZENG Sheng1, FANG Xiao1, ZHAO Wei-Juan2, LIU Wei-Ping1
1China Institute of Atomic Energy, Beijing 102413 2Institute of Physical Engineering, Zhengzhou University, Zhengzhou 450052
摘要Angular distribution of the 6He(d,n)7Li reaction at Ec.m.=9.1 MeV is measured in inverse kinematics for the first time. The proton spectroscopic factors for the ground and first excited states of 7Li are derived by using the distorted wave Born approximation analysis. The astrophysical rates of 6He(p,γ)7Li reaction are then deduced and fitted with an expression of REACLIB.
Abstract：Angular distribution of the 6He(d,n)7Li reaction at Ec.m.=9.1 MeV is measured in inverse kinematics for the first time. The proton spectroscopic factors for the ground and first excited states of 7Li are derived by using the distorted wave Born approximation analysis. The astrophysical rates of 6He(p,γ)7Li reaction are then deduced and fitted with an expression of REACLIB.
LI Er-Tao;LI Zhi-Hong**;SU Jun;GUO Bing;LI Yun-Ju;YAN Sheng-Quan;BAI Xi-Xiang;WANG You-Bao;WANG Bao-Xiang;LIAN Gang;ZENG Sheng;FANG Xiao;ZHAO Wei-Juan;LIU Wei-Ping
. Astrophysical Rates for the 6He(p, γ)7Li Reaction[J]. 中国物理快报, 2011, 28(5): 52102-052102.
LI Er-Tao, LI Zhi-Hong**, SU Jun, GUO Bing, LI Yun-Ju, YAN Sheng-Quan, BAI Xi-Xiang, WANG You-Bao, WANG Bao-Xiang, LIAN Gang, ZENG Sheng, FANG Xiao, ZHAO Wei-Juan, LIU Wei-Ping
. Astrophysical Rates for the 6He(p, γ)7Li Reaction. Chin. Phys. Lett., 2011, 28(5): 52102-052102.
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2011, Vol. 28 
