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First results of Trojan horse method using radioactive ion beams: 18F(p,α) at astrophysical energies

S. Cherubini M. Gulino C. Spitaleri M. La Cognata L. Lamia S. Puglia G. Rapisarda S. Romano S. Kubono H. Yamaguchi D. Binh S. Hayakawa Y. Kurihara Y. Wakabayashi S. Bishop A. Coc 1 N. de Séréville 2 F. Hammache 2
1 CSNSM AN
CSNSM - Centre de Spectrométrie Nucléaire et de Spectrométrie de Masse, CSNSM - Centre de Sciences Nucléaires et de Sciences de la Matière
Abstract : The abundance of 18F in Nova explosions is considered to be an important piece of information for the understanding of this astrophysical phenomenon. It is then necessary to study the nuclear processess that both produce and destroy this isotope in Novae. Among these latter reactions, the 18F(p,α)15O is one of the most important 18F destruction channels. Here we report on an experiment performed using the CRIB apparatus of the Center for Nuclear Study of the University of Tokyo. This was the first experiment that used the Trojan Horse method applied to a Radioactive Ion Beam induced reaction.
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http://hal.in2p3.fr/in2p3-01068314
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Submitted on : Thursday, September 25, 2014 - 2:13:46 PM
Last modification on : Wednesday, September 16, 2020 - 5:43:21 PM

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S. Cherubini, M. Gulino, C. Spitaleri, M. La Cognata, L. Lamia, et al.. First results of Trojan horse method using radioactive ion beams: 18F(p,α) at astrophysical energies. Origin of matter and evolution of galaxies 2013 : Proceedings of the 12th International Symposium on Origin of Matter and Evolution of Galaxies (OMEG12), Nov 2013, Tsukuba, Japan. pp.184-189, ⟨10.1063/1.4874065⟩. ⟨in2p3-01068314⟩

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