Published April 24, 2009 | Version v1
Journal article

Discovery of a New Broad Resonance in 19Ne: Implications for the Destruction of the Cosmic γ-Ray Emitter 18F

  • 1. Grand Accelerateur National d'Ions Lourds (GANIL), CEA/DSM-CNRS/IN2P3, B.P. 55027, F-14076 Caen Cedex 5 (France)
  • 2. Laboratoire de Physique Corpusculaire ENSICAEN, CNRS-IN2P3 UMR 6534 et Universite de Caen, F-14050 Caen (France)
  • 3. School of Physics and Astronomy, University of Edinburgh, Edinburgh EH9 3JZ (United Kingdom)
  • 4. Centre de Recherche du Cyclotron, Universite catholique de Louvain, B-1348 Louvain-la-Neuve (Belgium)
  • 5. CSNSM UMR 8609, CNRS-IN2P3/Universite Paris-Sud, Batiment 104, 91405 Orsay Campus (France)
  • 6. Horia Hulubei National Institute of Physics and Nuclear Engineering, P.O. Box MG6, Bucharest-Margurele (Romania)

Description

Six proton-emitting states in 19Ne were studied through the inelastic scattering reaction H(19Ne,p)19Ne*(p)18F. Their energies and widths were derived from the protons detected at zero degree, while proton-proton angular correlations between the detector at zero degree and a segmented annular detector were used to determine their spin value. In addition to the known states, a new broad J=(1/2) resonance has been evidenced at Ex≅7.9 MeV, ≅1.45 MeV above the proton emission threshold. By introducing this resonance, the 18F(p,α)15O destruction rate in novae is significantly enhanced. This reduces the chance to observe the cosmic γ-ray emission of 18F from novae in space telescopes.

Additional details

Publishing Information

Journal Title
Physical Review Letters
Journal Volume
102
Journal Issue
16
Journal Page Range
p. 162503-162503.4
ISSN
0031-9007
CODEN
PRLTAO

Optional Information

Notes
(c) 2009 The American Physical Society