Determination of Astrophysical 13N(p,γ)14O S-factors from the Asymptotic Normalization Coefficient of 14C → 13C + n

Details Determination of Astrophysical 13N(p,γ)14O S-factors from the Asymptotic Normalization Coefficient of 14C → 13C + n Determination of Astrophysical 13N(p,γ)14O S-factors from the Asymptotic Normalization Coefficient of 14C → 13C + n

Jan 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007chphl..24...65g&link_type=abstract

Chinese Physics Letters, Volume 24, Issue 1, pp. 65-68 (2007).

Physics

2

Scientific paper

The angular distribution of the 13C(d,p)14C reaction is reanalysed using the Johnson Soper approach. The squared asymptotic normalization coefficient (ANC) of virtual decay 14C → 13C + n is then derived to be 21.4±5.0 fm-1. The squared ANC and spectroscopic factor (SF) of 14O → 13N + p are extracted to be 30.4±7.1 fm-1 and 1.94±0.45, respectively. The astrophysical S-factors and reaction rates of 13N(p,γ)14O are determined from the ANC of 14O → 13N + p using the R-matrix approach.

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