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First experimental limit on the [sup 19]Ne([ital p],[gamma])[sup 20]Na resonance strength, of astrophysical interest

Journal Article · · Physical Review Letters; (United States)
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  1. Department of Physics and Astronomy; University of Edinburgh; The King's Buildings; Edinburgh EH9 3JZ (United Kingdom) Instituut voor Kern-en Stralingsfysika; Katholieke Universiteit Leuven; Leuven; B-3001 (Belgium) Institut d'Astronomie; d'Astrophysique et de Geophysique; Universite Libre de Bruxelles; B-1050 Bruxelles (Belgium) Institut de Physique Nucleaire; Universite Catholique de Louvain; Louvain-la-Neuve; B-1348 (Belgium) Institute of Nuclear Techniques; Technical University of Budapest; H-1521 Budapest (Hungary) Department of Physics; University of Notre Dame; Notre Dame; Indiana 46556 (United States)
The [sup 19]Ne([ital p],[gamma])[sup 20]Na reaction may influence considerably the reaction flow between the CNO and NeNa mass regions in high temperature hydrogen burning conditions. The 447 keV resonance has been studied by exploiting radioactive [sup 19]Ne beams with novel detection techniques to measure [beta][sup +]-delayed [alpha] radioactivity of [sup 20]Na nuclei produced in reactions with polyethylene targets. A 90% C.L. upper limit of 18 meV for the resonance strength has been determined and implications for the spin assignment of the 2.646 MeV state in [sup 20]Na and the stellar reaction are discussed.
OSTI ID:
7062265
Journal Information:
Physical Review Letters; (United States), Journal Name: Physical Review Letters; (United States) Vol. 73:23; ISSN 0031-9007; ISSN PRLTAO
Country of Publication:
United States
Language:
English