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We discuss the phenomenon of energization of relativistic charged particles in three-dimensional incompressible MHD turbulence and the diffusive properties of the motion of the same particles. We show that the random electric field induced by turbulent plasma motion leads test particles moving in a simulated box to be accelerated in a stochastic way, a second-order Fermi process. A small fraction of these particles happen to be trapped in large- scale structures, most likely formed due to the interaction of islands in the tu ...
Published by: \apj Published on: mar
YEAR: 2022   DOI: 10.3847/1538-4357/ac5332
Published by: \prd Published on: 11/2020
YEAR: 2020   DOI: 10.1103/PhysRevD.102.103016
Published by: \apj Published on: 03/2017
YEAR: 2017   DOI: 10.3847/1538-4357/aa603a
Parker Data Used; astroparticle physics; cosmic rays; diffusion; magnetic fields; scattering; turbulence; Physics - Space Physics; Astrophysics - High Energy Astrophysical Phenomena; Astrophysics - Solar and Stellar Astrophysics