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Light Elements and Cosmic Rays in the Early Galaxy
release_5gjifimd25d7zfxotobuvtj35u
by
R. Ramaty, B. Kozlovsky, R.E. Lingenfelter
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as a article
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(1996)
Abstract
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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