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Title:
Density jump as a function of magnetic field strength for parallel collisionless shocks in pair plasmas
Authors:
Bret, Antoine; Narayan, Ramesh
Affiliation:
AA(ETSI Industriales, Universidad de Castilla-La Mancha, 13071 Ciudad Real, Spain), AB(Harvard-Smithsonian Center for Astrophysics, Harvard University, 60 Garden St., Cambridge, MA 02138, USA)
Publication:
Journal of Plasma Physics, Volume 84, Issue 6, article id. 905840604, 17 pp.
Publication Date:
12/2018
Origin:
CUP
Keywords:
astrophysical plasmas, plasma nonlinear phenomena, space plasma physics
Abstract Copyright:
(c) 2018: © Cambridge University Press 2018
DOI:
10.1017/S0022377818001125
Bibliographic Code:
2018JPlPh..84f9004B

Abstract

Collisionless shocks follow the Rankine-Hugoniot jump conditions to a good approximation. However, for a shock propagating parallel to a magnetic field, magnetohydrodynamics states that the shock properties are independent of the field strength, whereas recent particle-in-cell simulations reveal a significant departure from magnetohydrodynamics behaviour for such shocks in the collisionless regime. This departure is found to be caused by a field-driven anisotropy in the downstream pressure, but the functional dependence of this anisotropy on the field strength is yet to be determined. Here, we present a non-relativistic model of the plasma evolution through the shock front, allowing for a derivation of the downstream anisotropy in terms of the field strength. Our scenario assumes double adiabatic evolution of a pair plasma through the shock front. As a result, the perpendicular temperature is conserved. If the resulting downstream is firehose stable, then the plasma remains in this state. If unstable, it migrates towards the firehose stability threshold. In both cases, the conservation equations, together with the relevant hypothesis made on the temperature, allows a full determination of the downstream anisotropy in terms of the field strength.
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