Proton capture on 14C and its astrophysical implications

Details Proton capture on 14C and its astrophysical implications Proton capture on 14C and its astrophysical implications

Oct 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990nupha.517..329g&link_type=abstract

Nuclear Physics A, Volume 517, Issue 2, p. 329-339.

Physics

Nuclear Physics

11

Nuclear Reaction

Scientific paper

The reaction 14C(p, γ)15N has been measured in the proton energy range of Ep = 250-740 keV. Five resonances have been observed and their strengths were determined. Additionally, 5 nonresonant γ-rays were found to the states at Ex = 0.0, 5.27, 5.30, 6.32 and 9.05 MeV. The energy dependence of their cross sections can be described by the direct capture process and the low-energy tails of the broad resonances at ER= 1319 and 1509 keV.

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