Published July 25, 2005 | Version v1
Journal article

The 18F(p,α)15O reaction rate for application to nova γ-ray emission

  • 1. CSNSM, CNRS/IN2P3/UPS, Ba t. 104, 91405 Orsay Campus (France)
  • 2. CEA, DAPNIA/SPhN, F-91191 Gif-sur-Yvette Cedex (France)
  • 3. CSNSM, CNRS/IN2P3/UPS, Bat. 104, 91405 Orsay Campus (France)

Description

The 18F(p,α)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. We report here on our lastest results concerning the study of the D(18F,pα)15N reaction, as well as on the determination of the 18F(p,α)15O reaction rate using the R-matrix theory. Remaining uncertainties are discussed

Additional details

Identifiers

DOI
10.1016/j.nuclphysa.2005.05.197;
arXiv
arXiv:nucl-ex/0408001v1;
PII
S0375-9474(05)00829-8;

Publishing Information

Journal Title
Nuclear Physics. A
Journal Volume
758
Journal Page Range
p. 745-748
ISSN
0375-9474
CODEN
NUPABL

Conference

Title
8. international symposium on nuclei in the cosmos
Dates
19-23 Jul 2004
Place
Vancouver, BC (Canada)

Optional Information

Copyright
Copyright (c) 2005 Elsevier Science B.V., Amsterdam, The Netherlands, All rights reserved.