Shock Vorticity Generation from Accelerated Ion Streaming in the Precursor of Ultrarelativistic Gamma-Ray Burst External Shocks
Sean M. Couch, Milos Milosavljevic, Ehud Nakar

TL;DR
This paper explores how accelerated ions in ultrarelativistic gamma-ray burst shocks generate vorticity and turbulence upstream, amplifying magnetic fields and affecting shock dynamics.
Contribution
It introduces a novel mechanism where ion-induced charge separation leads to upstream vorticity and turbulence, explaining magnetic field amplification in gamma-ray burst shocks.
Findings
Ion acceleration causes charge separation and upstream return currents.
Vorticity is generated at the shock transition due to density contrasts.
Turbulence amplifies magnetic fields consistent with observations.
Abstract
We investigate the interaction of nonthermal ions (protons and nuclei) accelerated in an ultrarelativistic blastwave with the pre-existing magnetic field of the medium into which the blastwave propagates. While particle acceleration processes such as diffusive shock acceleration can accelerate ions and electrons, the accelerated electrons suffer larger radiative losses. Under certain conditions, the ions can attain higher energies and reach farther ahead of the shock than the electrons, and so the nonthermal particles can be partially charge-separated. To compensate for the charge separation, the upstream plasma develops a return current, which, as it flows across the magnetic field, drives transverse acceleration of the upstream plasma and a growth of density contrast in the shock upstream. If the density contrast is strong by the time the fluid is shocked, vorticity is generated at…
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