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Study of the neutron induced reaction 17O(n,α)14C at astrophysical energies via the Trojan Horse Method

Authors :
G. Manicò
G. D’Agata
G. L. Guardo
N. de Séréville
C. Spitaleri
S. Romano
D. Lattuada
M. Lattuada
A. A. Oliva
Fairouz Hammache
Roberta Spartà
M. La Commara
M. L. Sergi
A. Tumino
Maria Letizia Pumo
S. Palmerini
M. Mazzocco
G. G. Rapisarda
I. Indelicato
S. Cherubini
S. Messina
S. Hayakawa
M. La Cognata
M. Gulino
P. Figuera
A. Cvetinović
Neven Soić
A. Di Pietro
R. G. Pizzone
L. Lamia
Institut de Physique Nucléaire d'Orsay (IPNO)
Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Sud - Paris 11 (UP11)
Laboratoire de Physique des 2 Infinis Irène Joliot-Curie (IJCLab)
Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Saclay-Centre National de la Recherche Scientifique (CNRS)
Université Paris-Sud - Paris 11 (UP11)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)
Source :
EPJ Web of Conferences, Vol 227, p 02007 (2020), EPJ Web Conf.
Publication Year :
2020
Publisher :
EDP Sciences, 2020.

Abstract

Neutron induced reactions are fundamental for the nucleosynthesis of elements in the universe. Indeed, to correctly study the reactions involved in the well-known s-process in stars, which produce about half of the elements beyond the iron peak, it is mandatory to know the neutron abundance available in those stars. The 17O(n, a)14C reaction is one of the so-called “neutron poisons” for the pro- cess and it could play an important role in the balance of the neutron abundance. The reaction is therefore investigated in the energy range of astrophysical inter- est between 0 and 350 keV in the center of mass by applying the Trojan Horse Method to the three body reaction 2H(17O, a14C)H.

Details

Language :
English
Volume :
227
Database :
OpenAIRE
Journal :
EPJ Web of Conferences
Accession number :
edsair.doi.dedup.....838abebd3e0a9028876967c24b0a3e32
Full Text :
https://doi.org/10.1051/epjconf/202022702007⟩