Statistics
Scientific paper
Aug 1979
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979nciml..25..435s&link_type=abstract
Nuovo Cimento, Lettere, Serie 2, vol. 25, Aug. 4, 1979, p. 435-442.
Statistics
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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