TL;DRAbstract
The 6He secondary beams with the energy of 26, 32 and 38 MeV were produced via the 2H (7Li, 6He)3He reaction on the secondary beam facility at the HI-13 tandem accelerator, Beijing. The intensity of the collimated 6He beam with a purity of 99% is about 900 s^(-1). The angular distribution of 2H (6He, 7Li)n reaction can be measured using this secondary 6He beam in inverse kinematics, and the astrophysical S-factor and rate of the 6He(p, γ)7Li reaction can be derived.
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The 6He secondary beams with the energy of 26, 32 and 38 MeV were produced via the 2H (7Li, 6He)3He reaction on the secondary beam facility at the HI-13 tandem accelerator, Beijing. The intensity of the collimated 6He beam with a purity of 99% is about 900 s^(-1). The angular distribution of 2H (6He, 7Li)n reaction can be measured using this secondary 6He beam in inverse kinematics, and the astrophysical S-factor and rate of the 6He(p, γ)7Li reaction can be derived.
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