Constraining the S factor of 15N(p,g)16O at Astrophysical Energies
Constraining the S factor of 15N(p,g)16O at Astrophysical Energies
Leblanc, P. J.; Imbriani, G.; Goerres, J.; Junker, M.; Azuma, R.; Beard, M.; Bemmerer, D.; Best, A.; Broggini, C.; Caciolli, A.; Corvisiero, P.; Costantini, H.; Couder, M.; Deboer, R.; Elekes, Z.; Falahat, S.; Formicola, A.; Fulop, Z.; Gervino, G.; Guglielmetti, A.; Gustavino, C.; Gyurky, G.; Kaeppeler, F.; Kontos, A.; Kuntz, R.; Leiste, H.; Lemut, A.; Li, Q.; Limata, B.; Marta, M.; Mazzocchi, C.; Menegazzo, R.; O'Brien, S.; Palumbo, A.; Prati, P.; Roca, V.; Rolfs, C.; Rossi Alvarez, C.; Somorjai, E.; Stech, E.; Straniero, O.; Strieder, F.; Tan, W.; Terrasi, F.; Trautvetter, H. P.; Uberseder, E.; Wiescher, M.
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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Physical Review C 82(2010), 055804
DOI: 10.1103/PhysRevC.82.055804
Cited 40 times in Scopus -
Contribution to WWW
ArXiV preprint server: http://arxiv.org/abs/1011.2518
Permalink: https://www.hzdr.de/publications/Publ-14900
