Systematic analysis of astrophysical S-factors and thermonuclear reaction rates

Journal Article · Mon May 12 00:00:00 EDT 2008 · AIP Conference Proceedings

DOI:https://doi.org/10.1063/1.2939331· OSTI ID:21143381

Katsuma, M ^[1]

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1. Institut d'Astronomie et d'Astrophysique, Universite Libre de Bruxelles, Campus de la Plaine, 1050 Brussels (Belgium)

The astrophysical S-factors of the {sup 13}C({alpha},n){sup 16}O, {sup 17}O({alpha},n){sup 20}Ne, {sup 21}Ne({alpha},n){sup 24}Mg and {sup 25}Mg({alpha},n){sup 28}Si reactions are analyzed with DWBA. The gross structures of the experimental data are reproduced by the DWBA calculations. The resulting reaction rates are compared with those in the CF88 and NACRE compilations.

• OSTI ID: 21143381
• Journal Information: AIP Conference Proceedings, Vol. 1012, Issue 1; Conference: FINUSTAR: 2. conference on Frontiers In NUclear STructure, Astrophysics and Reactions, Crete (Greece), 10-14 Sep 2007; Other Information: DOI: 10.1063/1.2939331; (c) 2008 American Institute of Physics; Country of input: International Atomic Energy Agency (IAEA); ISSN 0094-243X
• Country of Publication: United States
• Language: English

Related Subjects

73 NUCLEAR PHYSICS AND RADIATION PHYSICS
ALPHA REACTIONS
ASTROPHYSICS
BINDING ENERGY
CARBON 13 TARGET
COMPARATIVE EVALUATIONS
DWBA
MAGNESIUM 24
MAGNESIUM 25 TARGET
NEON 20
NEON 21 TARGET
NEUTRONS
NUCLEAR REACTION KINETICS
OXYGEN 16
OXYGEN 17 TARGET
SILICON 28
THERMONUCLEAR REACTIONS