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

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de Sereville, N. Angulo, C. [UCL] Cherubini, S. [UCL] Couder, M. Gaelens, M. [UCL] Demaret, Paul [UCL] Ninane, Alain [UCL] Ryckewaert, Guido [UCL]

(eng) 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. Comment: Contribution to The Seventh International Symposium on Nuclei in the Cosmos

Document type Article de périodique (Journal article) – Article de recherche
Access type Accès libre
Publication date 2002
Journal information "arXiv"
Affiliation UCL - SC/PHYS - Département de physique
Keywords Nuclear Experiment ; Astrophysics
Links
Bibliographic reference de Sereville, N. ; Angulo, C. ; Cherubini, S. ; Couder, M. ; Gaelens, M. ; et. al. Study of the F-18(p, alpha) O-15 reaction for application to nova gamma-ray emission. In: arXiv,
Permanent URL http://hdl.handle.net/2078/30829