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

Authors :
M. La Cognata
Z. Hons
Gabor Kiss
A. M. Mukhamedzhanov
S. V. Burjan
Marisa Gulino
Aurora Tumino
E. Somorjai
C. Spitaleri
G. G. Rapisarda
S. Romano
Silvio Cherubini
S. M. R. Puglia
F. Hammache
M. L. Sergi
B. F. Irgaziev
Livio Lamia
R. G. Pizzone
A. Coc
N. de Séréville
V. Kroha
Source :
AIP Conference Proceedings.
Publication Year :
2014
Publisher :
AIP Publishing LLC, 2014.

Abstract

The 17O(p,α)14N 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 17O(p,α)14N 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.

Details

ISSN :
0094243X
Database :
OpenAIRE
Journal :
AIP Conference Proceedings
Accession number :
edsair.doi...........65436876193c6141e8cb44100c35963d
Full Text :
https://doi.org/10.1063/1.4875312