Photoerosion and the abundances of the light elements

Physics

Scientific paper

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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.

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