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ACKNOWLEDGEMENTS This work used the HPC resources provided by the Pleiades facility at NASA NAS and the Prometheus system at ACC Cyfronet AGH. The work of O.K. and J.N. is supported by Narodowe Centrum Nauki through research project DEC-2013/10/E/ST9/00662. Fig. 3: Phase-space in x-px (a,b) and x-py (c,d) for ambient electrons (a, c) and ions (b, d) at t=26.8/γmax. At x/Δ > 43,000 strong nonresonant turbulence nonlinearly backreacts on CRs and ambient plasma which results in a slowdown of the beam drift from vsh=0.4c to ~0.15c.

Spatial Evolution of Nonresonant Instabilities in the Precursors of Young Supernova Remnant Shocks