Light Elements and Cosmic Rays in the Early Galaxy release_rev_3b12d619-1713-4b8c-8a36-f8f06b4f2970

by R. Ramaty, B. Kozlovsky, R.E. Lingenfelter

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We derive constraints on the cosmic rays responsible for the Be and part of the B observed in stars formed in the early Galaxy: the cosmic rays cannot be accelerated from the ISM; their energy spectrum must be relatively hard (the bulk of the nuclear reactions should occur at >30 MeV/nucl); and only 10^49 erg/SNII in high metallicity, accelerated particle kinetic energy could suffice to produce the Be and B. The reverse SNII shock could accelerate the particles.
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Type  article
Stage   submitted
Date   1996-10-30
Version   v1
Language   en ?
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Revision: 3b12d619-1713-4b8c-8a36-f8f06b4f2970