Constraining the S factor of 15N(p,g)16O at Astrophysical Energies

Details Constraining the S factor of 15N(p,g)16O at Astrophysical Energies Constraining the S factor of 15N(p,g)16O at Astrophysical Energies

2010-11-10

arxiv.org/abs/1011.2518v1

Phys.Rev.C82:055804,2010; Erratum-ibid.C84:019902,2011

Physics

Nuclear Physics

Nuclear Experiment

15 pages, 9 figures

Scientific paper

10.1103/PhysRevC.82.055804 10.11

The 15N(p,g)16O reaction represents a break out reaction linking the first and second cycle of the CNO cycles redistributing the carbon and nitrogen abundances into the oxygen range. The reaction is dominated by two broad resonances at Ep = 338 keV and 1028 keV and a Direct Capture contribution to the ground state of 16O. Interference effects between these contributions in both the low energy region (Ep < 338 keV) and in between the two resonances (338

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