Mildly relativistic magnetized shocks in electron–ion plasmas – II. Particle acceleration and heating

Author:

Ligorini Arianna1ORCID,Niemiec Jacek1ORCID,Kobzar Oleh2ORCID,Iwamoto Masanori3ORCID,Bohdan Artem4ORCID,Pohl Martin45ORCID,Matsumoto Yosuke6ORCID,Amano Takanobu7ORCID,Matsukiyo Shuichi3ORCID,Hoshino Masahiro7ORCID

Affiliation:

1. Institute of Nuclear Physics Polish Academy of Sciences, PL-31342 Krakow, Poland

2. Astronomical Observatory of the Jagiellonian University, PL-30244 Krakow, Poland

3. Faculty of Engineering Sciences, Kyushu University, Kasuga, Fukuoka 816-8580, Japan

4. DESY, D-15738 Zeuthen, Germany

5. Institute of Physics and Astronomy, University of Potsdam, D-14476 Potsdam, Germany

6. Department of Physics, Chiba University, 1-33 Yayoi, Inage-ku, Chiba 263-8522, Japan

7. Department of Earth and Planetary Science, University of Tokyo, 7-3-1 Hongo, Bunkyo-ku, Tokyo 113-0033, Japan

Abstract

ABSTRACT Particle acceleration and heating at mildly relativistic magnetized shocks in electron–ion plasma are investigated with unprecedentedly high-resolution 2D particle-in-cell simulations that include ion-scale shock rippling. Electrons are super-adiabatically heated at the shock, and most of the energy transfer from protons to electrons takes place at or downstream of the shock. We are the first to demonstrate that shock rippling is crucial for the energization of electrons at the shock. They remain well below equipartition with the protons. The downstream electron spectra are approximately thermal with a limited supra-thermal power-law component. Our results are discussed in the context of wakefield acceleration and the modelling of electromagnetic radiation from blazar cores.

Funder

Narodowe Centrum Nauki

Japan Society for the Promotion of Science

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

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