The F-18(p,alpha)O-15 reaction is recognized as one of the most important reaction for nova gamma-ray astronomy as it governs the early less than or equal to 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(F-18,palpha)N-15, at the CRC-RIB facility at Louvain La Neuve.
Study of the F-18(p,alpha)O-15 reaction for application to nova gamma-ray emission
CHERUBINI, SILVIO;
2003-01-01
Abstract
The F-18(p,alpha)O-15 reaction is recognized as one of the most important reaction for nova gamma-ray astronomy as it governs the early less than or equal to 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(F-18,palpha)N-15, at the CRC-RIB facility at Louvain La Neuve.File in questo prodotto:
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