Abstract
We investigate ways of accurately simulating the propagation of energetic charged particles over small times where the standard Monte Carlo approximation to diffusive transport breaks down. We find that a small-angle scattering procedure with appropriately chosen step-lengths and scattering angles gives accurate results, and we apply this to the simulation of propagation upstream in relativistic shock acceleration.
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Protheroe, R., Meli, A. & Donea, AC. Small-Angle Scattering and Diffusion: Application to Relativistic Shock Acceleration. Space Science Reviews 107, 369–372 (2003). https://doi.org/10.1023/A:1025541704838
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DOI: https://doi.org/10.1023/A:1025541704838