Systematic analysis of astrophysical S-factors and thermonuclear reaction rates

Details Systematic analysis of astrophysical S-factors and thermonuclear reaction rates Systematic analysis of astrophysical S-factors and thermonuclear reaction rates

May 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008aipc.1012..365k&link_type=abstract

FRONTIERS IN NUCLEAR STRUCTURE, ASTROPHYSICS, AND REACTIONS: FINUSTAR 2. AIP Conference Proceedings, Volume 1012, pp. 365-367 (

Astronomy and Astrophysics

Astrophysics

Fusion Reactors, Nuclear Data Compilation, Binding Energies And Masses

Scientific paper

The astrophysical S-factors of the 13C(α,n)16O, 17O(α,n)20Ne, 21Ne(α,n)24Mg and 25Mg(α,n)28Si 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.

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