Conditions for the onset of the current filamentation instability in the laboratory
arXiv:1709.09747 · doi:10.1017/S0022377818000314
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 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.
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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