The study of 18F+p reaction at astrophysical energies

Details The study of 18F+p reaction at astrophysical energies The study of 18F+p reaction at astrophysical energies

May 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009aipc.1120..294c&link_type=abstract

PERSPECTIVE IN NUCLEAR PHYSICS: Proceedings of the 6th Japan-Italy Symposium on Heavy-Ion Physics. AIP Conference Proceedings,

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Nucleosynthesis In Novae, Supernovae, And Other Explosive Environments, Radiation Detectors, Beams In Particle Accelerators, Gas-Filled Counters: Ionization Chambers, Proportional, And Avalanche Counters

Scientific paper

The abundance of 18F 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 18F(p,α)15O stands as one of the main 18F 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.

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