Study of the ^18F(p, alpha)^15O reaction for application to nova   gamma-ray emission
  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. 
N. de Sereville, A. Coc, C. Angulo, M. Assuncao, D. Beaumel, B.   Bouzid, S. Cherubini, M. Couder, P. Demaret, F. de Oliveir...