Collisionless Magnetorotational Turbulence in Pair Plasmas: Steady-state Dynamics, Particle Acceleration, and Radiative Cooling
High Energy Astrophysical Phenomena
2024-06-17 v2 Plasma Physics
Abstract
We present 3D fully kinetic shearing-box simulations of pair-plasma magnetorotational turbulence with unprecedented macro-to-microscopic scale separation. While retrieving the expected fluid behavior of the plasma at large scales, we observe a steepening of turbulent spectra at kinetic scales and substantial angular-momentum transport linked with kinetic processes. For the first time, we provide a definitive demonstration of nonthermal particle acceleration in kinetic magnetorotational turbulence agnostically of initial conditions, by means of a novel strategy exploiting synchrotron cooling.
Keywords
Cite
@article{arxiv.2401.01399,
title = {Collisionless Magnetorotational Turbulence in Pair Plasmas: Steady-state Dynamics, Particle Acceleration, and Radiative Cooling},
author = {Fabio Bacchini and Vladimir Zhdankin and Evgeny A. Gorbunov and Gregory R. Werner and Lev Arzamasskiy and Mitchell C. Begelman and Dmitri A. Uzdensky},
journal= {arXiv preprint arXiv:2401.01399},
year = {2024}
}
Comments
Accepted in PRL