Astrophysical Rates for the 6He(p, γ)7Li Reaction

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

doi:10.1088/0256-307X/28/5/052102

Abstract

Angular distribution of the ⁶He(d,n)⁷Li reaction at E_c.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.

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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]. Chin. Phys. Lett., 2011, 28(5): 052102. DOI: 10.1088/0256-307X/28/5/052102

Astrophysical Rates for the ⁶He(p, γ)⁷Li Reaction

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Astrophysical Rates for the 6He(p, γ)7Li Reaction

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Astrophysical Rates for the ⁶He(p, γ)⁷Li Reaction