Study of {sup 17}O(p,{alpha}){sup 14}N reaction via the Trojan Horse Method for application to {sup 17}O nucleosynthesis
Journal Article
·
· AIP Conference Proceedings
- Laboratori Nazionali del Sud, Catania (Italy)
- CSNSM, CNRS/IN2P3/UPS, Batiment 104, 91405 Orsay Campus (France)
- Nuclear Physics Institute of ASCR, Rez near Prague (Czech Republic)
- IPN, IN2P3-CNRS et Universite de Paris-Sud, 91406 Orsay Cedex (France)
- Institute of Nuclear Research of Hungarian Academy of Sciences (ATOMKI), Debrecen (Hungary)
Because of the still present uncertainties on its rate, the {sup 17}O(p,{alpha}){sup 14}N is one of the most important reaction to be studied in order to get more information about the fate of {sup 17}O in different astrophysical scenarios. The preliminary study of the three-body reaction {sup 2}H({sup 17}O,{alpha}{sup 14}N)n is presented here as a first stage of the indirect study of this important {sup 17}O(p,{alpha}){sup 14}N reaction through the Trojan Horse Method (THM)
- OSTI ID:
- 21143500
- Journal Information:
- AIP Conference Proceedings, Vol. 1016, Issue 1; Conference: 10. international symposium on origin of matter and evolution of galaxies: From the dawn of Universe to the formation of solar system, Sapporo (Japan), 4-7 Dec 2007; Other Information: DOI: 10.1063/1.2943616; (c) 2008 American Institute of Physics; Country of input: International Atomic Energy Agency (IAEA); ISSN 0094-243X
- Country of Publication:
- United States
- Language:
- English
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