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The 17O(p,α)14N reaction measurement via the Trojan horse method and its application to 17O nucleosynthesis

M. L. Sergi C. Spitaleri R. G. Pizzone S. V. Burjan S. Cherubini A. Coc 1 M. Gulino F. Hammache 2 Z. Hons B. Irgaziev G. G. Kiss V. Kroha M. La Cognata L. Lamia A. Mukhamedzhanov S. M. R. Puglia G. G. Rapisarda S. Romano N. de Séréville 2 E. Somorjai A. Tumino
1 CSNSM AS
CSNSM - Centre de Sciences Nucléaires et de Sciences de la Matière
2 IPNO - Institut de Physique Nucléaire d'Orsay
Abstract : The 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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Conference papers
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http://hal.in2p3.fr/in2p3-01068312
Contributor : Christine Hadrossek <>
Submitted on : Thursday, September 25, 2014 - 2:07:15 PM
Last modification on : Wednesday, September 16, 2020 - 5:43:31 PM

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M. L. Sergi, C. Spitaleri, R. G. Pizzone, S. V. Burjan, S. Cherubini, et al.. The 17O(p,α)14N reaction measurement via the Trojan horse method and its application to 17O nucleosynthesis. Origin of matter and evolution of galaxies 2013 : Proceedings of the 12th International Symposium on Origin of Matter and Evolution of Galaxies (OMEG12), 2013, Tsukuba, Japan. pp.201-205, ⟨10.1063/1.4874068⟩. ⟨in2p3-01068312⟩

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