2H(6He,7Li)n, 12C(7Li, 6He)13N reactions and 12C(p,γ)13N astrophysical S(E) factors

Details 2H(6He,7Li)n, 12C(7Li, 6He)13N reactions and 12C(p,γ)13N astrophysical S(E) factors 2H(6He,7Li)n, 12C(7Li, 6He)13N reactions and 12C(p,γ)13N astrophysical S(E) factors

Mar 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010nupha.834..661l&link_type=abstract

Nuclear Physics A, Volume 834, Issue 1-4, p. 661-663c.

Physics

Nuclear Physics

1

Scientific paper

Angular distributions of 2H(6He,7Li)n and 12C(7Li,6He)13N reactions were measured at the HI-13 tandem accelerator, Beijing. Asymptotic normalization coefficient (ANC) of 13N → 12C + p was derived to be 1.64±0.11 fm-1 through distorted wave Born approximation (DWBA) analysis, which was then used to deduce the astrophysical S(E) factors for direct capture in 12C(p,γ)13N at energies of astrophysical relevance.

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