Phys. Rev. C 67, 052801(R) (2003) [4 pages]2H(18F,pα)15N reaction applied to nova γ-ray emission
The 18F(p,α)15O reaction is recognized to be one of the most important reactions for nova γ-ray astronomy, as it governs the early E<~511keV γ 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 2H(18F,p)19F(α)15N one-nucleon transfer reaction, induced by a 14-MeV 18F radioactive beam impinging on a CD2 target; outgoing protons and 15N (or α particles) were detected in coincidence in two silicon strip detectors. A distorted-wave Born approximation analysis of the data resulted in new limits to the contribution of low-energy resonances to the rate of the 18F(p,α)15O reaction. © 2003 The American Physical Society URL:
http://link.aps.org/doi/10.1103/PhysRevC.67.052801
DOI:
10.1103/PhysRevC.67.052801
PACS:
25.60.Je, 21.10.Jx, 26.30.+k, 27.20.+n
|
