The mechanism of efficient electron acceleration at parallel non-relativistic shocks
arXiv:2202.05288 · doi:10.3847/1538-4357/ac6ce7
Abstract
Thermal electrons cannot directly participate in the process of diffusive acceleration at electron-ion shocks because their Larmor radii are smaller than the shock transition width: this is the well-known electron injection problem of diffusive shock acceleration. Instead, an efficient pre-acceleration process must exist that scatters electrons off of electromagnetic fluctuations on scales much shorter than the ion gyro radius. The recently found intermediate-scale instability provides a natural way to produce such fluctuations in parallel shocks. The instability drives comoving (with the upstream plasma) ion-cyclotron waves at the shock front and only operates when the drift speed is smaller than half of the electron Alfven speed. Here, we perform particle-in-cell simulations with the SHARP code to study the impact of this instability on electron acceleration at parallel non-relativistic, electron-ion shocks. To this end, we compare a shock simulation in which the intermediate-scale instability is expected to grow to simulations where it is suppressed. In particular, the simulation with an Alfvenic Mach number large enough to quench the intermediate instability shows a great reduction (by two orders of magnitude) of the electron acceleration efficiency. Moreover, the simulation with a reduced ion-to-electron mass ratio (where the intermediate instability is also suppressed) not only artificially precludes electron acceleration but also results in erroneous electron and ion heating in the downstream and shock transition regions. This finding opens up a promising route for a plasma physical understanding of diffusive shock acceleration of electrons, which necessarily requires realistic mass ratios in simulations of collisionless electron-ion shocks.
12 pages, 8 figures, 1 table, Accepted to ApJ
References in corpus (16)
- Diffuse Radio Emission from Galaxy Clusters
- Detecting shock waves in cosmological smoothed particle hydrodynamics simulations
- Simultaneous Acceleration of Protons and Electrons at Nonrelativistic Quasiparallel Collisionless Shocks
- Shock Waves in Eulerian Cosmological Simulations: Main Properties and Acceleration of Cosmic Rays
- First detection of VHE gamma-rays from SN 1006 by H.E.S.S
- Simulating cosmic rays in clusters of galaxies - II. A unified scheme for radio halos and relics with predictions of the gamma-ray emission
- Spatial Structure and Collisionless Electron Heating in Balmer-dominated Shocks
- Variation of cosmic ray injection across supernova shocks
- On the electron-ion temperature ratio established by collisionless shocks
- Theory of Stochastic Shock Drift Acceleration for Electrons in the Shock Transition Region
- Equilibration processes in the Warm-Hot Intergalactic Medium
- A critical Mach number for electron injection in collisionless shocks
- The Acceleration of Electrons at Collisionless Shocks Moving Through a Turbulent Magnetic Field
- 3D MHD simulation of polarized emission in SN 1006
- Non-thermal particle acceleration at highly oblique non-relativistic shocks
- Simulating TeV gamma-ray morphologies of shell-type supernova remnants