Fermi acceleration in relativistic collisionless plasma shocks correlates with anisotropic energy gains
arXiv:2102.11975 · doi:10.1063/5.0061083
Abstract
Collisionless shocks generated by two colliding relativistic electron-positron plasma shells are studied using particle-in-cell (PIC) simulations. Shocks are mediated by the Weibel instability (WI), and the kinetic energy of the fastest accelerated particles is found to be anisotropically modified by WI-induced electric fields. Specifically, we show that all particles interacting with the shock bifurcate into two groups based on their final relativistic Lorentz factor : slow () and fast (), where is the bifurcation Lorentz factor that was found to be approximately twice the initial (upstream) Lorentz factor . We have found that the energies of the slow particles are equally affected by the longitudinal and transverse components of the shock electric field, whereas the fast particles are primarily accelerated by the transverse field component.
arXiv comment8 pages, 7 figures
References in corpus (36)
- The Physics of Gamma-Ray Bursts
- Generation of Magnetic Fields in the Relativistic Shock of Gamma-Ray-Burst Sources
- Particle acceleration by ultra-relativistic shocks: theory and simulations
- Particle acceleration in relativistic collisionless shocks: Fermi process at last?
- The Maximum Energy of Accelerated Particles in Relativistic Collisionless Shocks
- Interpenetrating plasma shells: near-equipartition magnetic field generation and non-thermal particle acceleration
- Particle acceleration at ultrarelativistic shocks: an eigenfunction method
- On the structure of relativistic collisionless shocks in electron-ion plasmas
- The microphysics of collisionless shock waves
- Energy spectra of cosmic rays accelerated at ultrarelativistic shock waves
- Relativistic Shocks: Particle Acceleration and Magnetization
- Long Term Evolution of Magnetic Turbulence in Relativistic Collisionless Shocks: Electron-Positron Plasmas
- Simulations of relativistic collisionless shocks: shock structure and particle acceleration
- Ion dynamics and acceleration in relativistic shocks
- Magnetic field evolution in relativistic unmagnetized collisionless shocks
- Particle acceleration and relativistic shocks
- On electromagnetic instabilities at ultra-relativistic shock waves
- Particle transport in tangled magnetic fields and Fermi acceleration at relativistic shocks
- Saturation mechanism of the Weibel instability in weakly magnetized plasmas
- Particle acceleration in relativistic outflows
- Fundamentals of collisionless shocks for astrophysical application, 2. Relativistic shocks
- Relativistic Collisionless Shocks in Unmagnetized Electron-Positron Plasmas
- Nonlinear Particle Acceleration in Relativistic Shocks
- Radiative Signatures of Relativistic Shocks
- Physics of Weibel-mediated relativistic collisionless shocks
- Perpendicular relativistic shocks in magnetized pair plasma
- 3D modeling of collisionless shocks
- Relativistic Fermi acceleration with shock compressed turbulence
- Steady-State Electrostatic Layers from Weibel Instability in Relativistic Collisionless Shocks
- Physics and phenomenology of weakly magnetized, relativistic astrophysical shock waves
- X-Dispersionless Maxwell solver for plasma-based particle acceleration
- Physics of relativistic collisionless shocks: The scattering center frame
- Physics of relativistic collisionless shocks: II Dynamics of the background plasma
- Electron and Ion Acceleration in Relativistic Shocks with Applications to GRB Afterglows
- Physics of relativistic collisionless shocks: III The suprathermal particles
- The impact of kinetic effects on the properties of relativistic electron-positron shocks