Astrophysical Rates for the 6He(p, γ)7Li Reaction
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.
- Publication:
-
Chinese Physics Letters
- Pub Date:
- May 2011
- DOI:
- 10.1088/0256-307X/28/5/052102
- Bibcode:
- 2011ChPhL..28e2102L