A statistical model for galactic cosmic rays.

Details A statistical model for galactic cosmic rays. A statistical model for galactic cosmic rays.

Jun 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997hepnp..21..486x&link_type=abstract

High Energ. Phys. Nucl. Phys., Vol. 21, No. 6, p. 486 - 493

Statistics

2

Galaxy: Cosmic Rays, Statistics: Cosmic Rays

Scientific paper

Suppose that all of cosmic ray particles of energy below 3×1018eV are mainly originated and accelerated in an individual explosion of the galactic supernovae (SNs). By using an isotropic diffusion propagation model, non-steady state density of the iron nucleus is investigated. Considering the effect of extra-galactic cosmic rays and the variety of the galactic cosmic ray nuclei, the statistical model of galactic cosmic rays with a reasonable distribution of the SNs in space and time can account for the spectrum of cosmic rays in the energy range of 1012 - 1020eV quite well.

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