Study of the ^18F(p, alpha)^15O reaction for application to nova gamma-ray emission

Details Study of the ^18F(p, alpha)^15O reaction for application to nova gamma-ray emission Study of the ^18F(p, alpha)^15O reaction for application to nova gamma-ray emission

2002-09-24

arxiv.org/abs/nucl-ex/0209017v1

Nucl.Phys. A718 (2003) 259-262

Physics

Nuclear Physics

Nuclear Experiment

Contribution to The Seventh International Symposium on Nuclei in the Cosmos

Scientific paper

The ^18F(p, alpha)^15O reaction is recognized as one of the most important reaction for nova gamma-ray astronomy as it governs the early =< 511 keV emission. However, its rate remains largely uncertain at nova temperatures due to unknown low-energy resonance strengths. In order to better constrain this reaction rate, we have studied the one-nucleon transfer reaction, D(^18F,p alpha)^15N, at the CRC-RIB facility at Louvain La Neuve.

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