Determination of the 12C( p, γ)13N reaction rates from the 12C(7Li,6He)13N reaction

Details Determination of the 12C( p, γ)13N reaction rates from the 12C(7Li,6He)13N reaction Determination of the 12C( p, γ)13N reaction rates from the 12C(7Li,6He)13N reaction

Apr 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010scchg..53..658l&link_type=abstract

Science China Physics, Mechanics and Astronomy, Volume 53, Issue 4, pp.658-663

Astronomy and Astrophysics

Astronomy

Scientific paper

The angular distribution of the 12C(7Li,6He)13N reaction at E(7Li) = 44.0 MeV was measured at the HI-13 tandem accelerator of Beijing, China. The asymptotic normalization coefficient (ANC) of 13N → 12C + p was derived to be (1.64 ± 0.11) fm-1/2 through the distorted wave Born approximation (DWBA) analysis. The ANC was then used to deduce the astrophysical S( E) factors and reaction rates for the 12C( p, γ)13N direct capture reaction at energies of astrophysical relevance.

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