Origin and evolution of the light elements Li, Be, and B

Details Origin and evolution of the light elements Li, Be, and B Origin and evolution of the light elements Li, Be, and B

Feb 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998aipc..425..571c&link_type=abstract

Tours symposium on nuclear physics III. AIP Conference Proceedings, Volume 425, pp. 571-580 (1998).

Physics

Nuclear Physics

Cosmic Rays, Hydrostatic Stellar Nucleosynthesis

Scientific paper

The increase in observational data in recent years concerning the light elements Li, Be, and B has led us to reexamine the standard picture of their production through galactic cosmic-ray spallation. The recent observations in the Orion star forming region of strong gamma-ray emission lines of C and O indicate that the weak shocks and turbulence found in star forming regions lead to the acceleration of these elements. Interactions between fast C and O and the ambient H and He may in fact be the primary production mechanism of B and Be and not cosmic-ray reactions as has been previously thought.

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