Ion-electron instabilities in the precursor of weakly magnetized, transrelativistic shocks
arXiv:2407.17137 · doi:10.3847/1538-4357/ad5346
Abstract
Collisionless shocks are known to induce turbulence via upstream ion reflection within the precursor region. This study elucidates the properties of electrostatic and electromagnetic instabilities, exploring their role over the transrelativistic range. Notably, the growth of oblique Buneman waves and previously overlooked, secondary small-scale ion-electron instabilities is observed to be particularly promoted in the relativistic regime. Furthermore, the growth of large-scale electromagnetic modes encounters severe limitations in any cold, baryon-loaded precursor. It is argued that electron pre-heating in electrostatic modes may alleviate these constraints, facilitating the subsequent growth of large-scale filamentation modes in the precursor of transrelativistic shocks.
arXiv comment15 pages
References in corpus (23)
- Multi-messenger Observations of a Binary Neutron Star Merger
- The Physics of Gamma-Ray Bursts
- A kilonova as the electromagnetic counterpart to a gravitational-wave source
- Generation of Magnetic Fields in the Relativistic Shock of Gamma-Ray-Burst Sources
- Illuminating Gravitational Waves: A Concordant Picture of Photons from a Neutron Star Merger
- Particle Acceleration in Relativistic Magnetized Collisionless Electron-Ion Shocks
- Interpenetrating plasma shells: near-equipartition magnetic field generation and non-thermal particle acceleration
- Cosmic ray acceleration and escape from supernova remnants
- A cocoon shock breakout as the origin of the -ray emission in GW170817
- Ultra-high-energy cosmic ray acceleration by relativistic blast waves
- Magnetic field evolution in relativistic unmagnetized collisionless shocks
- Non-Fermi Power law Acceleration in Astrophysical Plasma Shocks
- Collisionless shock formation, spontaneous electromagnetic fluctuations and streaming instabilities
- Electron Shock Surfing Acceleration in Multidimensions: Two-dimensional Particle-In-Cell Simulation of Collisionless Perpendicular Shock
- Are GRB shocks mediated by the Weibel instability?
- Cosmic Ray Acceleration at Relativistic Shock Waves with a "Realistic" Magnetic Field Structure
- Particle transport and heating in the microturbulent precursor of relativistic shocks
- Dispersion and thermal effects on electromagnetic instabilities in the precursor of relativistic shocks
- Oblique Ion Two-Stream Instability in the Foot Region of a Collisionless Shock
- Improved Numerical Cherenkov Instability Suppression in the Generalized PSTD PIC Algorithm
- Two-stream-like instability in dilute hot relativistic beams and astrophysical relativistic shocks
- Long wavelength unstable modes in the far upstream of relativistic collisionless shocks
- Origin of intense electron heating in relativistic blast waves