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

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 ± 5.0fm-1. The squared ANC and spectroscopic factor (SF) of 14O → 13N + p are extracted to be 30.4 ± 7.1fm-1 and 1.94 ± 0.45, respectively. The astrophysical S-factors and reaction rates of 13N(pγ)14O are determined from the ANC of 14O → 13N + p using the R-matrix approach.