Plasma physics of trapping of cosmic rays around supernova

Details Plasma physics of trapping of cosmic rays around supernova Plasma physics of trapping of cosmic rays around supernova

Jun 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979icrc...12..128k&link_type=abstract

16th International Cosmic Ray Conference, Vol. 12. Published by the Institute for Cosmic Ray Research, University of Tokyo, 3-2-

Physics

Plasma Physics

Cosmic Rays, Plasma Physics, Supernovae, Anisotropy, Magnetohydrodynamic Waves, Stellar Magnetic Fields

Scientific paper

Two problems associated with the question of whether a large number of cosmic rays produced in the early stages of expansion of a supernova bubble would be trapped in it are discussed. They are the determination of the manner in which the cosmic ray anisotropy and the Alfven wave energy density, driven unstable by this anisotropy evolve towards equilibrium balance and how the singularity associated with standard quasilinear theory for resonant interaction, which occurs for pitch angles near 90 degrees, are treated by inclusion of other nonlinear effects.

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