The 17O(p,α)14N reaction measurement via the Trojan horse method and its application to 17O nucleosynthesis
Author(s) -
M. L. Sergi,
C. Spitaleri,
R. G. Pizzone,
S. V. Burjan,
S. Cherubini,
A. Coc,
M. Gulino,
F. Hammache,
Z. Hons,
B. F. Irgaziev,
G. Kiss,
V. Kroha,
M. La Cognata,
L. Lamia,
A. M. Mukhamedzhanov,
Chengbo Li,
G. G. Rapisarda,
S. Romano,
N. de Séréville,
E. Somorjai,
А. Туміно
Publication year - 2014
Publication title -
aip conference proceedings
Language(s) - English
Resource type - Conference proceedings
eISSN - 1551-7616
pISSN - 0094-243X
DOI - 10.1063/1.4874068
Subject(s) - nucleosynthesis , physics , stellar nucleosynthesis , trojan horse , reaction rate , astrophysics , nuclear reaction , nuclear physics , computer science , chemistry , operating system , biochemistry , catalysis
International audienceThe role of oxygen in astrophysics is related to different problems as novae nucleosynthesis and gamma-ray astronomy. In particular, owing to the still present uncertainties on its rate, the 17O(p,α)14N is one of the most important reaction to be studied in order to get more information about the fate of oxygen in different astrophysical scenarios
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