The 13N(p, γ)14O reaction at stellar energies

Details The 13N(p, γ)14O reaction at stellar energies The 13N(p, γ)14O reaction at stellar energies

Mar 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985nupha.435..657l&link_type=abstract

Nuclear Physics A, Volume 435, Issue 2, p. 657-668.

Physics

Nuclear Physics

22

Scientific paper

We present a microscopically-founded potential model for the 13N(p, γ)14O reaction at energies of astrophysical interest. The model is shown to reproduce the 13C(p, γ)14Ocross section very well. The 13N(p, γ)14O reaction is dominated by the first excited J = 1- resonance in 14O. For this resonance we find a proton width of Γc.m. = 40.1 keV and a photon width of Γγ = 1.50 eV.

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