English

Particle Acceleration by MHD Turbulence

Astrophysics 2016-08-30 v2

Abstract

Recent advances in understanding of magnetohydrodynamic (MHD) turbulence call for revisions in the picture of particle acceleration. We make use of the recently established scaling of slow and fast MHD modes in strong and weak MHD turbulence to provide a systematic study of particle acceleration in magnetic pressure (low-β\beta) and gaseous pressure (high-β\beta) dominated plasmas. We consider the acceleration by large scale compressions in both slow and fast particle diffusion limits. We compare the results with the acceleration rate that arises from resonance scattering and Transit-Time Damping (TTD). We establish that fast modes accelerate particles more efficiently than slow modes. We find that particle acceleration by pitch-angle scattering and TTD dominates acceleration by slow or fast modes when the spatial diffusion rate is small. When the rate of spatial diffusion of particles is high, we establish an enhancement of the efficiency of particle acceleration by slow and fast modes in weak turbulence. We show that highly supersonic turbulence is an efficient agent for particle acceleration. We find that even incompressible turbulence can accelerate particles on the scales comparable with the particle mean free path.

Keywords

Cite

@article{arxiv.astro-ph/0509385,
  title  = {Particle Acceleration by MHD Turbulence},
  author = {Jungyeon Cho and A. Lazarian},
  journal= {arXiv preprint arXiv:astro-ph/0509385},
  year   = {2016}
}

Comments

17 pages, 4 figures, accepted by ApJ; Some sections re-arranged

R2 v1 2026-07-22T08:57:20.232Z