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American Institute of Physics, AIP Conference Proceedings, 2014

DOI: 10.1063/1.4874065

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

Journal article published in 2014 by S. Cherubini, M. Gulino, C. Spitaleri ORCID, 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 and other authors.
This paper was not found in any repository, but could be made available legally by the author.
This paper was not found in any repository, but could be made available legally by the author.

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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.