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

de Sereville, N.;Angulo, C.;Cherubini, S.;Couder, M.;Ryckewaert, Guido;et.al.
(2002) arXiv —

Files

Preprint.pdf
  • Open Access
  • Adobe PDF
  • 65.6 KB
Download

Details

Authors
  • de Sereville, N.
    Author
  • Angulo, C.UCLouvain
    Author
  • Cherubini, S.UCLouvain
    Author
  • Couder, M.
    Author
  • Gaelens, M.UCLouvain
    Author
  • Demaret, PaulUCLouvain
    Author
  • Ninane, AlainUCLouvain
    Author
  • Ryckewaert, GuidoUCLouvain
    Author
  • et. al.
Show more
Abstract
(en) 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
Affiliations

Citations

  • APA
  • Chicago
  • FWB

de Sereville, N., Angulo, C., Cherubini, S., Couder, M., Gaelens, M., Demaret, P., Leleux, P., Loiselet, M., Ninane, A., Ryckewaert, G., & et al. (2002). Study of the F-18(p, alpha) O-15 reaction for application to nova gamma-ray emission. arXiv. https://hdl.handle.net/2078.5/257135