Extracting the Asymptotic Normalization Coefficients in Neutron Transfer Reactions to Determine the Astrophysical Reaction Rates for {sup 22}Mg(p,{gamma}){sup 23}Al and {sup 17}F(p,{gamma}){sup 18}Ne
Journal Article
·
· AIP Conference Proceedings
- Cyclotron Institute, Texas A and M University, College Station, TX 77843 (United States)
- National Institute for Nuclear Physics and Engineering, P.O. Box MG-6, Bucharest (Romania)
It was expected that {gamma} rays from {sup 18}F and {sup 22}Na would be observed in massive One novae, but neither has been to date. The {sup 17}F(p,{gamma}){sup 18}Ne and {sup 22}Mg(p,{gamma}){sup 23}Al reactions may play important roles in the production and destruction of {sup 18}F and {sup 22}Na. We have determined the asymptotic normalization coefficients for {sup 18}Ne and {sup 23}Al through measurements of peripheral neutron transfer reactions in the mirror nuclear systems. We use the ANCs to calculate the astrophysical S-factors and reaction rates for these two reactions.
- OSTI ID:
- 21052881
- Journal Information:
- AIP Conference Proceedings, Vol. 972, Issue 1; Conference: Carpathian summer school of physics 2007 on exotic nuclei and nuclear/particle astrophysics (II), Sinaia (Romania), 21-31 Aug 2007; Other Information: DOI: 10.1063/1.2870381; (c) 2008 American Institute of Physics; Country of input: International Atomic Energy Agency (IAEA); ISSN 0094-243X
- Country of Publication:
- United States
- Language:
- English
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