Particle Acceleration by Pickup Process Upstream of Relativistic Shocks
Masanori Iwamoto, Takanobu Amano, Yosuke Matsumoto, Shuichi Matsukiyo,, Masahiro Hoshino

TL;DR
This paper investigates particle acceleration mechanisms at relativistic shocks using particle-in-cell simulations, revealing how wakefields and filamentation induce particle pickup and acceleration, with implications for astrophysical phenomena like gamma-ray bursts.
Contribution
It introduces a novel pickup process driven by wakefields and filamentation in relativistic shocks, estimating maximum particle energies and highlighting their astrophysical significance.
Findings
Particles are decoupled from upstream flow by wakefields.
Particles are re-accelerated by motional electric fields.
Maximum Lorentz factors scale with shock parameters, indicating efficient acceleration.
Abstract
Particle acceleration at magnetized purely perpendicular relativistic shocks in electron-ion plasmas are studied by means of two-dimensional particle-in-cell simulations. Magnetized shocks with the upstream bulk Lorentz factor are known to emit intense electromagnetic waves from the shock front, which induce electrostatic plasma waves (wakefield) and transverse filamentary structures in the upstream region via the stimulated/induced Raman scattering and the filamentation instability, respectively. The wakefield and filaments inject a fraction of incoming particles into a particle acceleration process, in which particles are once decoupled from the upstream bulk flow by the wakefield, and are piked up again by the flow. The picked-up particles are accelerated by the motional electric field. The maximum attainable Lorentz factor is estimated as $\gamma_{max,e} \sim…
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Taxonomy
TopicsAstrophysics and Cosmic Phenomena · Gamma-ray bursts and supernovae · Laser-Plasma Interactions and Diagnostics
