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Karataglidis, S.; Jennings, B.
Los Alamos National Lab., NM (United States). Funding organisation: US Department of Energy (United States)2000
Los Alamos National Lab., NM (United States). Funding organisation: US Department of Energy (United States)2000
AbstractAbstract
[en] The astrophysical S factor for the 7Be(p, γ)8B reaction at threshold is investigated using simple models to determine the model dependence in the extrapolation of the laboratory data to the region of astrophysical interest near 20 keV. We find that the energy dependence below 400 keV is largely well understood in terms of the Coulomb interaction and constrained by the data for the elastic scattering of low-energy neutrons from 7Li
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2000; 11 p; 9. International Conference on Nuclear Reaction Mechanisms; Varenna (Italy); 5-11 Jun 2000; W-7405-ENG-36; Also available from OSTI as DE00768967; PURL: https://www.osti.gov/servlets/purl/768967-vcNqVy/webviewable/
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