Spectrum of cosmic rays accelerated by a supernova blast wave

Details Spectrum of cosmic rays accelerated by a supernova blast wave Spectrum of cosmic rays accelerated by a supernova blast wave

Jun 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990azh....67..572a&link_type=abstract

Astronomicheskii Zhurnal (ISSN 0004-6299), vol. 67, May-June 1990, p. 572-581. In Russian.

Astronomy and Astrophysics

Astronomy

2

Galactic Cosmic Rays, Particle Acceleration, Shock Wave Propagation, Supernova Remnants, Mach Number, Shock Fronts, Transport Properties

Scientific paper

A numerical solution of the transport equation is obtained for cosmic-ray acceleration by a supernova blast wave. The important role of the cosmic-ray escape phenomenon (i.e., the intensive escape of cosmic rays from the vicinity of the shock front as some limiting energy is reached) is confirmed, and the significant contribution of the free expansion stage to the resulting cosmic-ray spectrum is demonstrated.

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