Non-linear diffusion of cosmic rays

Details Non-linear diffusion of cosmic rays Non-linear diffusion of cosmic rays

Aug 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008adspr..42..486p&link_type=abstract

Advances in Space Research, Volume 42, Issue 3, p. 486-490.

Physics

7

Scientific paper

The propagation of cosmic rays in the interstellar medium after their release from the sources supernova remnants can be attended by the development of streaming instability. The instability creates MHD turbulence that changes the conditions of particle transport and leads to a non-linear diffusion of cosmic rays. We present a self-similar solution of the equation of non-linear diffusion for particles ejected from a SNR and discuss how obtained results may change the physical picture of cosmic ray propagation in the Galaxy.

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