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Particle acceleration and wave excitation in quasi-parallel high-Mach-number collisionless shocks: Particle-in-cell simulation

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arxiv 1407.1971 v2 pith:DBP27USL submitted 2014-07-08 astro-ph.HE physics.plasm-phphysics.space-ph

classification astro-ph.HEphysics.plasm-phphysics.space-ph
keywords shockprocessprotonsacceleratedaccelerationupstreamwaveselectrons
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We herein investigate shock formation and particle acceleration processes for both protons and electrons in a quasi-parallel high-Mach-number collisionless shock through a long-term, large-scale particle-in-cell simulation. We show that both protons and electrons are accelerated in the shock and that these accelerated particles generate large-amplitude Alfv\'{e}nic waves in the upstream region of the shock. After the upstream waves have grown sufficiently, the local structure of the collisionless shock becomes substantially similar to that of a quasi-perpendicular shock due to the large transverse magnetic field of the waves. A fraction of protons are accelerated in the shock with a power-law-like energy distribution. The rate of proton injection to the acceleration process is approximately constant, and in the injection process, the phase-trapping mechanism for the protons by the upstream waves can play an important role. The dominant acceleration process is a Fermi-like process through repeated shock crossings of the protons. This process is a `fast' process in the sense that the time required for most of the accelerated protons to complete one cycle of the acceleration process is much shorter than the diffusion time. A fraction of the electrons is also accelerated by the same mechanism, and have a power-law-like energy distribution. However, the injection does not enter a steady state during the simulation, which may be related to the intermittent activity of the upstream waves. Upstream of the shock, a fraction of the electrons is pre-accelerated before reaching the shock, which may contribute to steady electron injection at a later time.

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  1. Speed-dependent Threshold for Electron Injection into Diffusive Shock Acceleration

    astro-ph.HE 2025-06 conditional novelty 6.0 of 10

    Electrons enter diffusive shock acceleration once their speed exceeds the shock speed, producing nonthermal tails that start at low momenta.

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