The transport and acceleration of test particles in hydrodynamical simulations

Details The transport and acceleration of test particles in hydrodynamical simulations The transport and acceleration of test particles in hydrodynamical simulations

Aug 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001icrc....6.2046d&link_type=abstract

Proceedings of the 27th International Cosmic Ray Conference. 07-15 August, 2001. Hamburg, Germany. Under the auspices of the Int

Physics

Scientific paper

The interaction of supernovae with their surroundings has been studied with hydrodynamical codes which capture the shock waves produced when the ejecta interact with the medium close to the progenitor star. Observationally it is known that core-collapse supernovae, of which SN1987A and SN1993J are two well-studied examples, emit nonthermal radiation which is associated with electron acceleration at these shock waves. We present a model for the transport and acceleration of test particles in hydrodynamical simulations of young radio supernovae.

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