Shock formation in magnetised electron–positron plasmas: mechanism and timing

The shock formation process in electron–positron pair plasmas is investigated in the presence of an ambient perpendicular magnetic field. In initially unmagnetised plasmas, which are dominated by the Weibel or filamentation instability, the shock formation time is a multiple of the saturation time o...

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Main Authors: A Stockem Novo, A Bret, U Sinha
Format: Article
Language:English
Published: IOP Publishing 2016-01-01
Series:New Journal of Physics
Subjects:
Online Access:https://doi.org/10.1088/1367-2630/18/10/105002
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author A Stockem Novo
A Bret
U Sinha
author_facet A Stockem Novo
A Bret
U Sinha
author_sort A Stockem Novo
collection DOAJ
description The shock formation process in electron–positron pair plasmas is investigated in the presence of an ambient perpendicular magnetic field. In initially unmagnetised plasmas, which are dominated by the Weibel or filamentation instability, the shock formation time is a multiple of the saturation time of the linear instability. While in weakly magnetised plasmas the mechanism is still the same, higher magnetisations induce synchrotron maser modes such that the shock formation is dominated by magnetic reflection. As a consequence the formation times are reduced. The focus is on the detailed picture of the particle kinetics, in which the transition between Weibel and magneto-hydrodynamic shocks can be clearly identified.
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spelling doaj.art-6d6ac91c2551418c8fa167baf4d405e42023-08-08T14:23:57ZengIOP PublishingNew Journal of Physics1367-26302016-01-01181010500210.1088/1367-2630/18/10/105002Shock formation in magnetised electron–positron plasmas: mechanism and timingA Stockem Novo0A Bret1U Sinha2Institut für Theoretische Physik, Lehrstuhl IV: Weltraum- & Astrophysik, Ruhr-Universität , Bochum, GermanyETSI Industriales, Universidad de Castilla-La Mancha , E-13071 Ciudad Real, Spain; Instituto de Investigaciones Energéticas y Aplicaciones Industriales, Campus Universitario de Ciudad Real , E-13071 Ciudad Real, SpainGoLP/Instituto de Plasmas e Fusão Nuclear, Instituto Superior Técnico, Universidade de Lisboa , Lisboa, PortugalThe shock formation process in electron–positron pair plasmas is investigated in the presence of an ambient perpendicular magnetic field. In initially unmagnetised plasmas, which are dominated by the Weibel or filamentation instability, the shock formation time is a multiple of the saturation time of the linear instability. While in weakly magnetised plasmas the mechanism is still the same, higher magnetisations induce synchrotron maser modes such that the shock formation is dominated by magnetic reflection. As a consequence the formation times are reduced. The focus is on the detailed picture of the particle kinetics, in which the transition between Weibel and magneto-hydrodynamic shocks can be clearly identified.https://doi.org/10.1088/1367-2630/18/10/105002instabilitiesrelativistic processesshock waves
spellingShingle A Stockem Novo
A Bret
U Sinha
Shock formation in magnetised electron–positron plasmas: mechanism and timing
New Journal of Physics
instabilities
relativistic processes
shock waves
title Shock formation in magnetised electron–positron plasmas: mechanism and timing
title_full Shock formation in magnetised electron–positron plasmas: mechanism and timing
title_fullStr Shock formation in magnetised electron–positron plasmas: mechanism and timing
title_full_unstemmed Shock formation in magnetised electron–positron plasmas: mechanism and timing
title_short Shock formation in magnetised electron–positron plasmas: mechanism and timing
title_sort shock formation in magnetised electron positron plasmas mechanism and timing
topic instabilities
relativistic processes
shock waves
url https://doi.org/10.1088/1367-2630/18/10/105002
work_keys_str_mv AT astockemnovo shockformationinmagnetisedelectronpositronplasmasmechanismandtiming
AT abret shockformationinmagnetisedelectronpositronplasmasmechanismandtiming
AT usinha shockformationinmagnetisedelectronpositronplasmasmechanismandtiming