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Supernova remnants and the effect of efficient cosmic ray acceleration

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Reville,  Brian
Division Prof. Dr. Werner Hofmann, MPI for Nuclear Physics, Max Planck Society;

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Citation

Reville, B. (2008). Supernova remnants and the effect of efficient cosmic ray acceleration. Talk presented at Canadian institute for Theoretical Astrophysics. Toronto, Canada. 2008-07-21.


Cite as: https://hdl.handle.net/11858/00-001M-0000-0011-78FA-F
Abstract
It is well known that electrons and probably cosmic rays are accelerated in supernova remnants. To maintain the observed steady galactic cosmic-ray spectrum, it is necessary that they be very efficient accelerators. The back reaction of the high-energy particles on the shock structure and environment are reviewed with a particular emphasis on the amplification of magnetic fields.