Updated 14N(p,gamma)15O data from LUNA

Marta, M.; Bemmerer, D.; Caciolli, A.; Bonetti, R.; Broggini, C.; Confortola, F.; Corvisiero, P.; Costantini, H.; Elekes, Z.; Formicola, A.; Fulop, Zs.; Gervino, G.; Guglielmetti, A.; Gustavino, C.; Gyurky, Gy.; Imbriani, G.; Junker, M.; Lemut, A.; Limata, B.; Mazzocchi, C.; Menegazzo, R.; Prati, P.; Roca, V.; Rolfs, C.; Alvarez, C. R.; Somorjai, E.; Straniero, O.; Strieder, F.; Terrasi, F.; Trautvetter, H. P.

Publications Repository - Helmholtz-Zentrum Dresden-Rossendorf

Total number to be selected: 1 Record

1 Publication

Updated 14N(p,gamma)15O data from LUNA

Marta, M.; Bemmerer, D.; Caciolli, A.; Bonetti, R.; Broggini, C.; Confortola, F.; Corvisiero, P.; Costantini, H.; Elekes, Z.; Formicola, A.; Fulop, Z.; Gervino, G.; Guglielmetti, A.; Gustavino, C.; Gyurky, G.; Imbriani, G.; Junker, M.; Lemut, A.; Limata, B.; Mazzocchi, C.; Menegazzo, R.; Prati, P.; Roca, V.; Rolfs, C.; Alvarez, C. R.; Somorjai, E.; Straniero, O.; Strieder, F.; Terrasi, F.; Trautvetter, H. P.

Abstract

The 14N(p,gamma)15O reaction controls the rate of the hydrogen burning CNO cycle. By detecting solar CNO neutrinos (e.g. in Borexino, SNO+) one can in principle measure directly the carbon and nitrogen abundance at the center of the Sun. However this requires more precise nuclear data. Updated experimental results on capture to various excited states (as well as to the ground state) in 15O are shown, together with improved branching ratios obtained for the E_p = 278 keV resonance.

Keywords: Nuclear astrophysics; LUNA; CNO cycle; Clover detector; TiN solid target

Lecture (Conference)
Frühjahrstagung des DPG - Fachverbands Hadronen und Kerne, 15.-19.03.2010, Bonn, Deutschland

Permalink: https://www.hzdr.de/publications/Publ-13977

Years: 2023 2022 2021 2020 2019 2018 2017 2016 2015