Astrophysical Rate for 12N(p,g)13O Direct Capture Reactions

Abstract

The proton capture on the unstable nuclei plays a very important role for the nucleonsynthesis. The 12N(p,g)13O reaction rates at the energies of astrophysical interests are estimated with the spectroscopic factor and asymptotic normalization coefficient methods. The present results show that the 12N(p,g)13O reaction may play an important role in x-ray bursts.

3 pages and 5 figures

References in corpus (2)

• Survey of ground state neutron Spectroscopic Factors from Li to Cr isotopes
• Reaction and proton-removal cross sections of ${}^6$Li, ${}^7$Be, ${}^{10}$B, ${}^{9,10,11}$C, $^{12$N, ${}^{13,15}$O and ${}^{17}$Ne on Si at 15 to 53 MeV/nucleon

Cited by in corpus (1)

• Determination of astrophysical 12N(p,g)13O reaction rate from the 2H(12N, 13O)n reaction and its astrophysical implications