Hydrodynamic approach to cosmic ray acceleration

Details Hydrodynamic approach to cosmic ray acceleration Hydrodynamic approach to cosmic ray acceleration

Dec 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001jkas...34..289k&link_type=abstract

Journal of the Korean Astronomical Society, vol. 34, no. 4, pp. 289-291

Astronomy and Astrophysics

Astronomy

Scientific paper

To study the structure and dynamics of a cosmic-ray-plasma system, hydrodynamic approach is a fairly good approximation. In this approach, there are three basic energy transfer mechanisms: work done by the plasma flow against pressure gradients, cosmic ray streaming instability and stochastic acceleration. The interplay between these mechanisms gives a range of structures. We present some results of different version of the hydrodynamic approach, e.g., flow structure, injection, instability, acceleration with and without shocks.

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