Mildly relativistic magnetized shocks in electron-ion plasmas -- II. Particle acceleration and heating
arXiv:2101.09256 · doi:10.1093/mnras/stab220
Abstract
Particle acceleration and heating at mildly relativistic magnetized shocks in electron-ion plasma are investigated with unprecedentedly high-resolution two-dimensional particle-in-cell simulations that include ion-scale shock rippling. Electrons are super-adiabatically heated at the shock, and most of the energy transfer from protons to electrons takes place at or downstream of the shock. We are the first to demonstrate that shock rippling is crucial for the energization of electrons at the shock. They remain well below equipartition with the protons. The downstream electron spectra are approximately thermal with a limited supra-thermal power-law component. Our results are discussed in the context of wakefield acceleration and the modelling of electromagnetic radiation from blazar cores.
11 pages, 11 figures; This is a pre-copyedited, author-produced PDF of an article accepted for publication in MNRAS following peer review
References in corpus (17)
- The power of blazar jets
- A very-high-energy component deep in the Gamma-ray Burst afterglow
- Observation of inverse Compton emission from a long -ray burst
- Gamma-Ray Studies of Blazars: Synchro-Compton Analysis of Flat Spectrum Radio Quasars
- Production of Magnetic Turbulence by Cosmic Rays Drifting Upstream of Supernova Remnant Shocks
- The synchrotron maser emission from relativistic shocks in Fast Radio Bursts: 1D PIC simulations of cold pair plasmas
- Heating and Non-thermal Particle Acceleration in Relativistic, Transverse Magnetosonic Shock Waves in Proton-Electron-Positron Plasmas
- Wakefield Acceleration by Radiation Pressure in Relativistic Shock Waves
- Cosmic-Ray Acceleration at Ultrarelativistic Shock Waves: Effects of Downstream Short-Wave Turbulence
- Electron-ion coupling upstream of relativistic collisionless shocks
- Discovery of the low-energy cutoff in a powerful giant radio galaxy
- PIC Simulation Methods for Cosmic Radiation and Plasma Instabilities
- The synchrotron maser emission from relativistic magnetized shocks: Dependence on the pre-shock temperature
- Particle diffusion and localized acceleration in inhomogeneous AGN jets - Part I: Steady-state spectra
- Corrugation of relativistic magnetized shock waves
- Discovery of Very High Energy Gamma Rays from 1ES 1440+122
- Mildly relativistic magnetized shocks in electron-ion plasmas I. Electromagnetic shock structure
Cited by in corpus (12)
- Non-thermal particle acceleration at highly oblique non-relativistic shocks
- Multi-collision internal shock lepto-hadronic models for energetic GRBs
- Linearly-polarized Coherent Emission from Relativistic Magnetized Ion-electron Shocks
- Modeling kilonova afterglows: Effects of the thermal electron population and interaction with GRB outflows
- Saturation of the asymmetric current filamentation instability under conditions relevant to relativistic shock precursors
- Particle Acceleration by Pickup Process Upstream of Relativistic Shocks
- Non-thermal emission from mildly relativistic dynamical ejecta of neutron star mergers: spectrum and sky image
- X-ray Spectral Analysis of the Jet Termination Shock in Pictor A on Sub-Arcsecond Scales with Chandra
- Late-time non-thermal emission from mildly relativistic tidal ejecta of compact objects merger
- Reverse shock forming condition for magnetized relativistic outflows: reconciling theories and simulations
- Particle acceleration by counter-propagating circularly polarized Alfvén waves
- Synchrotron break frequencies of mildly-to-highly relativistic outflows observed off-axis