Astronomy and Astrophysics – Astronomy
Scientific paper
Sep 2004
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004mnras.353..550b&link_type=abstract
Monthly Notices of the Royal Astronomical Society, Volume 353, Issue 2, pp. 550-558.
Astronomy and Astrophysics
Astronomy
281
Acceleration Of Particles, Magnetic Fields, Plasmas, Shock Waves, Turbulence, Cosmic Rays
Scientific paper
The diffusive shock acceleration of cosmic rays by supernova remnants depends upon the generation of magnetic fluctuations by cosmic rays upstream of the shock. Strongly driven, non-resonant, nearly purely growing modes grow more rapidly than the resonant Alfvén waves usually considered. Non-linear simulation shows that the magnetic field can be amplified from its seed value by orders of magnitude. The consequences for the maximum attainable cosmic ray energy in supernova remnants are explored.
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