Effects of statistical post-acceleration on nuclear abundances of cosmic rays

Statistics

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Abundance, Cosmic Rays, Fermi-Dirac Statistics, Nuclear Particles, Particle Acceleration, Energy Distribution, Galactic Radiation, Particle Energy

Scientific paper

Effects of statistical 'post-acceleration' on primary cosmic radiation with the standard power-law differential energy distribution are considered. It is shown that one cannot be certain that post-acceleration effects are absent from or insignificant in measurements of cosmic-ray abundance ratios. The degree to which post-acceleration affects various cosmic-ray components is investigated. It is concluded that post-acceleration effects are likely to occur during the passage of supernova-accelerated cosmic-ray particles through the envelope and that these effects will modify the energy spectra and abundance ratios of the various components distinctly and appreciably.

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