Dataset referencing 2025RA06
D.Rapagnani, O.Straniero, G.Imbriani, M.Aliotta, C.Ananna, F.Barile, L.Barbieri, D.Bemmerer, A.Best, A.Boeltzig, C.Broggini, C.G.Bruno, A.Caciolli, M.Campostrini, F.Casaburo, F.Cavanna, G.F.Ciani, P.Colombetti, A.Compagnucci, P.Corvisiero, L.Csedreki, T.Davinson, R.Depalo, A.Di Leva, Z.Elekes, F.Ferraro, A.Formicola, Zs.Fulop, G.Gervino, R.M.Gesue, Gy.Gyurky, A.Guglielmetti, C.Gustavino, M.Junker, M.Lugaro, P.Marigo, J.Marsh, E.Masha, R.Menegazzo, D.Mercogliano, V.Paticchio, D.Piatti, P.Prati, V.Rigato, D.Robb, R.S.Sidhu, J.Skowronski, T.Szucs, S.Zavatarelli, for the LUNA Collaboration
Revision of the CNO cycle: Rate of 17O destruction in stars
NUCLEAR REACTIONS 17O(p, γ), (p, α), E<1.4 MeV; analyzed available data; deduced S-factors, astrophysical reaction rates, oxygen isotopic ratio with R-matrix σ calculations based on available measurements of the relevant nuclear parameters (energies, widths, strengths of known resonances, interference patterns, etc.), coupled to a Monte Carlo procedure to evaluate the global reaction rate error.
doi: 10.1103/PhysRevC.111.025805