Observation of the growth of a magnetic vortex in the transition layer of a mildly relativistic oblique plasma shock
G. C. Murphy, M. E. Dieckmann, L. O'C. Drury

TL;DR
This study uses 2D particle simulations to observe the formation and growth of a magnetic vortex in a plasma shock, revealing potential mechanisms for magnetic field generation in gamma-ray burst jets.
Contribution
It demonstrates the development of a magnetic vortex structure in a relativistic plasma shock, linking simulation results to astrophysical phenomena.
Findings
Magnetic vortex structure forms at the shock front.
Electrons and magnetic fields reach energy equipartition with ions.
The structure resembles a force-free spheromak, relevant to GRB jets.
Abstract
A 2D particle simulation models the collision of two electron-ion plasma clouds along a quasi-parallel magnetic field. The collision speed is 0.9c and the density ratio 10. A current sheet forms at the front of the dense cloud, in which the electrons and the magnetic field reach energy equipartition with the ions. A structure composed of a solenoidal and a toroidal magnetic field grows in this sheet. It resembles that in the cross-section of the torus of a force-free spheromak, which may provide the coherent magnetic fields in gamma-ray burst (GRB) jets needed for their prompt emissions.
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