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Astrophysical production rates for Li, Be, and B isotopes from energetic /sup 1/H and /sup 4/He reactions with HeCNO nuclei

Journal Article · · Astrophys. J.; (United States)
DOI:https://doi.org/10.1086/163740· OSTI ID:5961954
Calculations for Li, Be, and B nucleosynthesis in reactions of energetic /sup 1/H and /sup 4/He nuclei with /sup 4/He, /sup 12,13/C, /sup 14/N, and /sup 16/O nuclei have been performed. The calculations employed a recent compilation of cross section systematics for these reactions. Spcific models examined include galactic cosmic-ray interactions with the interstllar medium, synthesis in flares, and formation in shock waves. The GCR+ISM calculations are able to account for the absolute abundances of /sup 6/Li, /sup 9/Be, /sup 10/B, and /sup 11/B satisfactorily, but require a low-energy component of spectral form E/sup -//sup ..gamma../ to account for the /sup 11/B//sup 10/B isotopic ratio, where ..gamma.. = 5--7. In these calculations /sup 7/Li is underproduced by an order of magnitude. The required /sup 7/Li is most probably provided by the big bang, and assumption that is consistent with an open universe. Synthesis solely in a flare mechanism cannot reproduce the observed relative abundances. The shock wave mechanism can account for the relative abundances, but only in a very narrow window near E/A = 10 MeV.
Research Organization:
Department of Astronomy, Indiana University
OSTI ID:
5961954
Journal Information:
Astrophys. J.; (United States), Journal Name: Astrophys. J.; (United States) Vol. 299:2; ISSN ASJOA
Country of Publication:
United States
Language:
English