Evolution of supernova remnants including particle acceleration

Details Evolution of supernova remnants including particle acceleration Evolution of supernova remnants including particle acceleration

Aug 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990a%26a...234..419d&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 234, no. 1-2, Aug. 1990, p. 419-434.

Astronomy and Astrophysics

Astrophysics

46

Cosmic Rays, Particle Acceleration, Shock Waves, Stellar Envelopes, Stellar Evolution, Supernova Remnants, Kinetic Energy, Mach Number

Scientific paper

Numerical models of SNR evolution including the nonlinear reaction of
cosmic ray acceleration in shock waves are studied. The calculations are
performed with a given time-independent and space-independent mean
diffusion coefficient. The resulting equation for particle energy
density, which involves only hydrodynamic quantities, is presented.

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