ASPCS
 
Back to Volume
Paper: Astrophysical S-factor of the 15N(p, α),sup>12C Reaction at sub-Coulomb Energies via the Trojan-Horse Method
Volume: 378, Why Galaxies Care About AGB Stars: Their Importance as Actors and Probes
Page: 125
Authors: La Cognata, M.; Romano, S.; Spitaleri, C.; Cherubini, S.; Crucilla, V.; Gulino, M.; Lamia, L.; Mudo, F.; Pizzone, R.G.; Sergi, M.L.; Tudisco, S.; Tumino, A.; Tribble, R.; Trache, L.; Fu, C.; Goldberg, V.; Mukhamedzhanov, A.; Tabacaru, G.
Abstract: The bare-nucleus astrophysical S-factor for the 15N(p, α)12C reaction is extracted down to zero energy by means of the Trojan-Horse Method. A fair agreement is found down to 70 keV, while the low-energy behavior of the S-factor provides a smaller rate than reported in the literature.
Back to Volume