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

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arxiv nucl-ex/0209017 v1 pith:5IYAJWV4 submitted 2002-09-24 nucl-ex astro-ph

N. de Sereville , A. Coc , C. Angulo , M. Assuncao , D. Beaumel , B. Bouzid , S. Cherubini , M. Couder
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P. Demaret F. de Oliveira Santos P. Figuera S. Fortier M. Gaelens F. Hammache J. Kiener D. Labar A. Lefebvre P. Leleux M. Loiselet A. Ninane S. Ouichaoui G. Ryckewaert N. Smirnova V. Tatischeff J.-P. Thibaud
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classification nucl-exastro-ph
keywords reactionalphanovaemissiongamma-rayrateapplicationastronomy
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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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