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We present results of time evolution of oblique MHD plane shocks including diffusive cosmic ray acceleration with backreaction on the plasma flows.
The ponderomotive force due to cosmic ray generated alfven waves
A. Achterberg · 1981
Earlier work this paper cites.
An introduction to the theory of diffusive shock acceleration of energetic particles in tenuous plasmas
L. Drury · 1983
Earlier work this paper cites.
Particle acceleration at astrophysical shocks - a theory of cosmic-ray origin
R. D. Blandford and D. Eichler · 1987
Earlier work this paper cites.
Alfven wave transport effects in the time evolution of parallel cosmic-ray-modified shocks
T. W. Jones · 1993
Earlier work this paper cites.
Time-dependent simulation of oblique mhd cosmic-ray shocks using the two-fluid model
A. Frank T. W. Jones and D. Ryu · 1995
Cited alongside, same era.
Kinetic theory of cosmic rays and gamma rays in supernova remnants. i. uniform interstellar medium
E. Berezhko and H. Völk · 1997
Cited alongside, same era.
Nonlinear shock acceleration and photon emission in supernova remnants
Ellison D. Berezhko E. and M. Baring · 2000
Cited alongside, same era.
Time Evolution of Cosmic-Ray Modified MHD Shocks
T. W. Jones · 2005
Cited alongside, same era.
An Efficient Numerical Scheme for Simulating Particle Acceleration in Evolving Cosmic-Ray Modified Shocks
T. W. Jones and H. Kang · 2005
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Self-similar evolution of cr modified quais-parallel plane shocks
H. Kang and T. W. Jones · 2007
Closest in time.
Morlino G. Blasi P. and M. Vietri · 2007
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