(eng)
The 18F(p,alpha)15O reaction is recognized to be one of the most important
reactions for nova gamma-ray astronomy as it governs the early E <= 511keV
gamma emission. However in the nova temperature regime, its rate remains
largely uncertain due to unknown low-energy resonance strengths. We report here
the measurement of the D(18F,p)19F(alpha)15N one-nucleon transfer reaction,
induced by a 14 MeV 18F radioactive beam impinging on a CD2 target; outgoing
protons and 15N (or alpha-particles) were detected in coincidence in two
silicon strip detectors. A DWBA analysis of the data resulted in new limits to
the contribution of low-energy resonances to the rate of the 18F(p,alpha)15O
reaction.
Comment: Rapid Communication to appear in Phys. Rev. C., 4 pages and 4 figures
de Sereville, N. ; Coc, A. ; Angulo, C. ; Assuncao, M. ; Beaumel, D. ; et. al. D(F-18, p alpha) N-15 reaction applied to nova gamma-ray emission. (2003) 4 p. pages