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A direct measurement of the {sup 19}Ne(p,{gamma}){sup 20}Na reaction

Journal Article · · AIP Conference Proceedings
DOI:https://doi.org/10.1063/1.47407· OSTI ID:172066
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  1. Department of Physics and Astronomy, University of Edinburgh, The King`s Buildings, Edinburgh EH9 3JZ (United Kingdom)
  2. Instituut vor Kern- en Stralingsfysika, Katholieke Universiteit Leuven, Leuven, B-3001 (Belgium)
  3. Institut d`Astronomie, d`Astrophysique et de Geophysique, Universite Libre de Bruxelles, B-1050 Bruxelles (Belgium)
  4. Institut de Physique Nucleaire, Universite Catholique de Louvain, Louvain-la-Neuve, B-1348 (Belgium)
  5. Institute of Nuclear Techniques, Technical University of Budapest, H-1521 Budapest (Hungary)
+ Show Author Affiliations
The {sup 19}Ne(p,{gamma}){sup 20}Na reaction may be of considerable influence for the reaction flow between the CNO and NeNa mass region in high temperature hydrogen burning conditions. The proposed low energy resonance at 0.447 MeV has been measured in inverse kinematics with the Louvain-la-Neuve {sup 19}Ne beam, using novel activation techniques. An upper limit to the resonance strength has been determined and the implications for the spin assignment of the 2.646 MeV state in {sup 20}Na as well as for the stellar reaction rate are discussed. {copyright} {ital 1995} {ital American} {ital Institute} {ital of} {ital Physics}.
Sponsoring Organization:
USDOE
OSTI ID:
172066
Report Number(s):
CONF-9407131--
Journal Information:
AIP Conference Proceedings, Journal Name: AIP Conference Proceedings Journal Issue: 1 Vol. 327; ISSN 0094-243X; ISSN APCPCS
Country of Publication:
United States
Language:
English

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Related Subjects

66 PHYSICS
CAPTURE
ENERGY LEVELS
HYDROGEN BURNING
KEV RANGE 100-1000
NEON 19
PROTON REACTIONS
RESONANCE
SODIUM 20