Conditions for the onset of the current filamentation instability in the laboratory

Abstract

Current Filamentation Instability (CFI) is capable of generating strong magnetic fields relevant to explain radiation processes in astrophysical objects and lead to the onset of particle acceleration in collisionless shocks. Probing such extreme scenarios in the laboratory is still an open challenge. In this work, we investigate the possibility of using neutral $e^{-}$ $e^{+}$ beams to explore the CFI with realistic parameters, by performing 2D particle-in-cell simulations. We show that CFI can occur unless the rate at which the beam expands due to finite beam emittance is larger than the CFI growth rate and as long as the role of competing electrostatic two-stream instability (TSI) is negligible. We also show that the longitudinal energy spread, typical of plasma based accelerated electron-positron fireball beams, plays a minor role in the growth of CFI in these scenarios.

References in corpus (28)

• The Physics of Gamma-Ray Bursts
• Origin of Galactic and Extragalactic Magnetic Fields
• Generation of Magnetic Fields in the Relativistic Shock of Gamma-Ray-Burst Sources
• Interpenetrating plasma shells: near-equipartition magnetic field generation and non-thermal particle acceleration
• Magnetic Field Generation in Collisionless Shocks; Pattern Growth and Transport
• One-to-one direct modeling of experiments and astrophysical scenarios: pushing the envelope on kinetic plasma simulations
• Long-time evolution of magnetic fields in relativistic GRB shocks
• Absorption of High Energy Gamma Rays by Interactions With Starlight Photons in Extragalactic Space at High Redshifts and the High Energy Gamma-Ray Background
• Weibel, Two-Stream, Filamentation, Oblique, Bell, Buneman... which one grows faster ?
• Weibel-instability-mediated collisionless shocks in laboratory with ultraintense lasers
• Exploiting multi-scale parallelism for large scale numerical modelling of laser wakefield accelerators
• Plasma Physics of Extreme Astrophysical Environments
• Weibel instability and associated strong fields in a fully 3D simulation of a relativistic shock
• Relativistic Pair Beams from TeV Blazars: A Source of Reprocessed GeV Emission rather than IGM Heating
• Growth and phase velocity of self-modulated beam-driven plasma waves
• The Cosmological Impact of Luminous TeV Blazars II: Rewriting the Thermal History of the Intergalactic Medium
• Ultra High Energy Cosmic Ray Acceleration in Engine-driven Relativistic Supernovae
• Plasma effects on fast pair beams II. Reactive versus kinetic instability of parallel electrostatic wave
• The Effect of Nonlinear Landau Damping on Ultrarelativistic Beam Plasma Instabilities
• Magnetic Fields in Gamma-Ray Bursts: A Short Review
• The Linear Instability of Dilute Ultrarelativistic $e^{\pm }$ Pair Beams
• Importance of resolving the spectral support of beam-plasma instabilities in simulations
• Conditions for the onset of the current filamentation instability in the laboratory
• Implications of Plasma Beam Instabilities for the Statistics of the Fermi Hard Gamma-ray Blazars and the Origin of the Extragalactic Gamma-Ray Background
• Constraints on the Local Sources of Ultra High-Energy Cosmic Rays
• Simulation study of the filamentation of counter-streaming beams of the electrons and positrons in plasmas
• Interaction of Ultra Relativistic e- e+ Fireball Beam with Plasma
• Relativity at Action or Gamma-Ray Bursts

Cited by in corpus (8)

• Conditions for the onset of the current filamentation instability in the laboratory
• Anisotropic heating and magnetic field generation due to Raman scattering in laser-plasma interactions
• Magnetic field amplification by a plasma cavitation instability in relativistic shock precursors
• Generating ultra-dense pair beams using 400 GeV/c protons
• Positron acceleration in plasma waves driven by non-neutral fireball beams
• Slowdown of interpenetration of two counterpropagating plasma slab due to collective effects
• General features of experiments on the dynamics of laser-driven electron-positron beams
• Generation of quasi continuous-wave electron beams in an L-band normal conducting pulsed RF injector for laboratory astrophysics experiments