Astronomy and Astrophysics – Astrophysics
Scientific paper
Jun 1990
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990apj...356..501j&link_type=abstract
Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 356, June 20, 1990, p. 501-506.
Astronomy and Astrophysics
Astrophysics
15
Accretion Disks, Black Holes (Astronomy), Lithium Isotopes, Nuclear Astrophysics, Nuclear Fusion, Stellar Physics, Abundance, Deuterium, Milky Way Galaxy, Stellar Mass Accretion
Scientific paper
An investigation has been made of spallation nuclear processes in an ion pressure-supported accretion torus around a black hole. It has been found that, within the torus, Be-9, B-10, and B-11 are produced in cosmic abundance ratios relative to Li-7, while D and He-3 production is relatively small, and Li-6 production is high by a factor of 3. However, Li-6 nuclei produced in the torus are preferentially destroyed in cooler regions, hence outflow from the torus may effectively serve to enrich the universe with Li-7. It is shown that the ion torus that may exist around a black hole at the Galactic center, or the hypothetical black holes which constitute the Galactic dark matter, could have been the site of Li-7 production. In case of the dark matter black holes, for plausible accretion disk viscosities, this mechanism requires massive black holes of M greater than 500 solar masses.
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