O-17(p,alpha)N-14 reaction measurement at astrophysical energies

0486389 - ÚJF 2018 RIV US eng C - Konferenční příspěvek (zahraniční konf.)
Sergi, M. L. - Spitaleri, C. - Pizzone, R. G. - Burjan, Václav - Cherubini, S. - Coc, A. - Gulino, M. - Hammache, F. - Hons, Zdeněk - Irgaziev, B. - Kiss, G. G. - Kroha, Václav - La Cognata, M. - Lamia, L. - Mukhamedzhanov, A. M. - Puglia, S. M. R. - Rapisarda, G. G. - Romano, S. - de Sereville, N. - Somorjai, E. - Tumino, A.
O-17(p,alpha)N-14 reaction measurement at astrophysical energies.
AIP Conference Proceedings. Vol. 1595. Melville: American Institute of Physics, 2014, s. 208-210. ISBN 978-0-7354-1229-3. ISSN 0094-243X.
[7th European Summer School on Experimental Nuclear Astrophysics. Catania (IT), 15.09.2013-27.09.2013]
Institucionální podpora: RVO:61389005
Klíčová slova: nuclear astrophysics * direct reactions * nucleosynthesis in novae
Obor OECD: Astronomy (including astrophysics,space science)

The O-17(p,alpha)N-14 reaction is of paramount importance for the nucleosynthesis in a number of stellar sites, including red giants (RG), asymptotic giant branch (AGB) stars, massive stars and classical novae. We report on the indirect study of the O-17(p,alpha)N-14 reaction via the Trojan Horse Method by applying the approach recently developed for extracting the resonance strength of narrow resonance in the ultra-low energy region.
Trvalý link: http://hdl.handle.net/11104/0281215