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.

Astronomical Society of the Pacific
Conference Series

© Copyright 1988 - 2024 - Astronomical Society of the Pacific
No part of the material protected by this copyright may be reproduced or used in any form other than for personal use without written permission from the ASP.

Page generated in 0.036 seconds