Physics
Scientific paper
Aug 1988
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988stin...8911675b&link_type=abstract
Unknown
Physics
Abundance, Erosion, Light Elements, Photons, Photonuclear Reactions, Active Galactic Nuclei, Big Bang Cosmology, Chemical Evolution, Cosmic Rays, High Energy Interactions, Spallation
Scientific paper
The abundances of the rare light elements H-2, He-3, Li-7, and B-11 are shown to be potentially affected by photoerosion. That process, involving the interaction of high energy photons from galactic centers with atomic nuclei, will increase the abundances of H-2, He-3, and B-11 while lowering slightly those of Li-7 and He-4. In some regions of galaxies the effects may be large enough to impact their chemical evolution. In particular this process may have enhanced the H-2 and He-3 abundances near the center of our galaxy over and above those from the big bang, as well as the galactic B-11 abundance over that from cosmic-ray spallation.
Boyd Richard N.
Ferland Gary J.
Schramm David N.
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