The study of {sup 18}F+p reaction at astrophysical energies
Journal Article
·
· AIP Conference Proceedings
- Universita di Catania and INFN-LNS, Catania (Italy)
- Center for Nuclear Study, University of Tokyo (Japan)
- Department of Physics, Tohoku University, Sendai (Japan)
- Department of Physics, Yamagata University, Yamagata (Japan)
- Department of Physics, Tsukuba University, Tsukuba (Japan)
- Department of Physics, Kyushu University, Fukuoka (Japan)
- Centre de Spectrometrie Nucleaire et de Spectrometrie de Masse, IN2P3, F-91405 Orsay (France)
- Institut de Physique Nucleaire, IN2P3, F-91405 Orsay (France)
The abundance of {sup 18}F in Nova explosionsis an important issue in understanding this astrophysical phenomenon. For this reason it is necessary to study processes that produce or destroy this isotope in novae. Among these latter processes, the {sup 18}F(p,{alpha}){sup 15}O stands as one of the main {sup 18}F destruction channels. We report here on the status of a new experiment recently performed using the CRIB apparatus of the Center for Nuclear Study of the Tokyo University based at the RIKEN Wako branch.
- OSTI ID:
- 21304793
- Journal Information:
- AIP Conference Proceedings, Vol. 1120, Issue 1; Conference: 6. Japan-Italy symposium on heavy-ion physics, Tokai (Japan), 11-15 Nov 2008; Other Information: DOI: 10.1063/1.3141665; (c) 2009 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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