A relativistic partially electromagnetic planar plasma shock
arXiv:astro-ph/0702055 · doi:10.1086/525516
Abstract
We model relativistically colliding plasma by PIC simulations in one and two spatial dimensions, taking an ion-to-electron mass ratio of 400. Energy dissipation by a wave precursor of mixed polarity and different densities of the colliding plasma slabs results in a relativistic forward shock forming on millisecond timescales. The forward shock accelerates electrons to ultrarelativistic energies and reflects upstream ions, which drag the electrons along to preserve the plasma quasi-neutrality. No reverse shock forms. The shock may be representative for internal gamma ray burst shocks.
References in corpus (25)
- Gamma-Ray Bursts and the Fireball Model
- Generation of Magnetic Fields in the Relativistic Shock of Gamma-Ray-Burst Sources
- The shock break-out of GRB 060218/SN 2006aj
- GRS 1915+105 and the Disc-Jet Coupling in Accreting Black Hole Systems
- Interpenetrating plasma shells: near-equipartition magnetic field generation and non-thermal particle acceleration
- On the structure of relativistic collisionless shocks in electron-ion plasmas
- Magnetic Field Generation in Collisionless Shocks; Pattern Growth and Transport
- The Cooling Behavior of Thermal Pulses in Gamma-Ray Bursts
- Characterization of the initial filamentation of a relativistic electron beam passing through a plasma
- Long Term Evolution of Magnetic Turbulence in Relativistic Collisionless Shocks: Electron-Positron Plasmas
- Nonthermal Electrons at High Mach Number Shocks: Electron Shock Surfing Acceleration
- The electromagnetic model of Gamma Ray Bursts
- Non-Fermi Power law Acceleration in Astrophysical Plasma Shocks
- Ion leakage from quasiparallel collisionless shocks: implications for injection and shock dissipation
- Very High Mach Number Electrostatic Shocks in Collisionless Plasmas
- Electron Injection at High Mach Number Quasi-Perpendicular Shocks : Surfing and Drift Acceleration
- The Influence of an Ambient Magnetic Field on Relativistic Collisionless Plasma Shocks
- Gamma-ray bursts and collisionless shocks
- Acceleration Mechanics in Relativistic Shocks by the Weibel Instability
- A General Relativistic Magnetohydrodynamics Simulation of Jet Formation
- Simulations of Gamma-Ray Bursts from External Shocks: Time Variability and Spectral Correlations
- A Plasma Instability Theory of Gamma-Ray Burst Emission
- GRB Fireball Physics: Prompt and Early Emission
- Phase speed of electrostatic waves: The critical parameter for efficient electron surfing acceleration
- Time lag between prompt optical emission and gamma-rays in GRBs
Cited by in corpus (20)
- The Astrophysics of Ultrahigh Energy Cosmic Rays
- Weibel, Two-Stream, Filamentation, Oblique, Bell, Buneman... which one grows faster ?
- On electromagnetic instabilities at ultra-relativistic shock waves
- Weibel instability and associated strong fields in a fully 3D simulation of a relativistic shock
- On Fermi acceleration and MHD-instabilities at ultra-relativistic magnetized shock waves
- PIC methods in astrophysics: Simulations of relativistic jets and kinetic physics in astrophysical systems
- How large can the electron to proton mass ratio be in Particle-In-Cell simulations of unstable systems?
- Evolution of Global Relativistic Jets: Collimations and Expansion with kKHI and the Weibel Instability
- Magnetic Field Generation in Core-Sheath Jets via the Kinetic Kelvin-Helmholtz Instability
- Nonlinear Plasma Wave in Magnetized Plasmas
- PIC simulation of a strong double layer in a nonrelativistic plasma flow: Electron acceleration to ultrarelativistic speeds
- Magnetic field amplification and electron acceleration to near-energy equipartition with ions by a mildly relativistic quasi-parallel plasma protoshock
- Radiation from relativistic shocks with turbulent magnetic fields
- 3D PIC Simulations for Relativistic Jets with a Toroidal Magnetic Field
- Simulation of Relativistic Jets and Associated Self-consistent Radiation
- Multidimensional simulations of magnetic field amplification and electron acceleration to near-energy equipartition with ions by a mildly relativistic quasi-parallel plasma collision
- Observation of the growth of a magnetic vortex in the transition layer of a mildly relativistic oblique plasma shock
- The influence of the mass-ratio on the acceleration of particles by filamentation instabilities
- A New Time-Dependent Finite Difference Method for Relativistic Shock Acceleration
- Structure of a strong supernova shock wave and rapid electron acceleration confined in its transition region