Cosmic ray acceleration by multiple spherical shocks

Details Cosmic ray acceleration by multiple spherical shocks Cosmic ray acceleration by multiple spherical shocks

May 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000aph....13..161k&link_type=abstract

Astroparticle Physics, Volume 13, Issue 2-3, p. 161-172.

Physics

17

Scientific paper

Diffusive shock acceleration of energetic particles in a system of numerous stellar wind termination shocks and stellar-wind/supernova blast wave shocks is considered. We derive equations for the particle distribution function on momentum that describes collective particle acceleration. The form of the steady-state spectrum of accelerated particles depends on the global pattern of the interstellar gas flow. These results are discussed within a context of cosmic ray acceleration in star associations and in connection with a problem of cosmic ray reacceleration in the galactic disk.

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