Can Cosmic Rays Dominate Supernova Remnant Shocks

Details Can Cosmic Rays Dominate Supernova Remnant Shocks Can Cosmic Rays Dominate Supernova Remnant Shocks

Aug 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995mnras.275.1211k&link_type=abstract

Monthly Notices of the Royal Astronomical Society, Vol. 275, NO. 4/AUG15, P.1211, 1995

Astronomy and Astrophysics

Astronomy

1

Acceleration Of Particles - Diffusion - Shock Waves - Cosmic Rays - Supernova Remnants

Scientific paper

In this article we discuss the possibility of a cosmic-ray-dominated supernova remnant shock from the point of view of the diffusive confinement of cosmic rays near the shock. We examine the conditions under which this may be possible. Several examples are presented to illustrate the conditions. As expected, a cosmic-ray-dominated supernova remnant shock forms more `easily' if the supernova progenitor has created a large wind bubble.

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