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, N. De Séréville, F. Hammache

Publikation: Beitrag in Buch/Bericht/KonferenzbandKonferenzbeitragBegutachtung

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.

OriginalspracheEnglisch
TitelOrigin of Matter and Evolution of Galaxies 2013 - Proceedings of the 12th International Symposium on Origin of Matter and Evolution of Galaxies, OMEG 2013
Herausgeber (Verlag)American Institute of Physics Inc.
Seiten184-189
Seitenumfang6
ISBN (Print)9780735412286
DOIs
PublikationsstatusVeröffentlicht - 2014
Veranstaltung12th International Symposium on Origin of Matter and Evolution of Galaxies, OMEG 2013 - Tsukuba, Japan
Dauer: 18 Nov. 201321 Nov. 2013

Publikationsreihe

NameAIP Conference Proceedings
Band1594
ISSN (Print)0094-243X
ISSN (elektronisch)1551-7616

Konferenz

Konferenz12th International Symposium on Origin of Matter and Evolution of Galaxies, OMEG 2013
Land/GebietJapan
OrtTsukuba
Zeitraum18/11/1321/11/13

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