English

Particle acceleration at ultrarelativistic, perpendicular shock fronts

Plasma Physics 2022-12-21 v2 High Energy Astrophysical Phenomena Accelerator Physics

Abstract

Using an eigenfunction expansion to solve the transport equation, complemented by Monte-Carlo simulations, we show that ultrarelativistic shocks can be effective particle accelerators even when they fail to produce large amplitude turbulence in the downstream plasma. This finding contradicts the widely held belief that a uniform downstream magnetic field perpendicular to the shock normal inhibits acceleration by the first order Fermi process. In the ultrarelativistic limit, we find a stationary power-law particle spectrum of index s=4.17 for these shocks, close to that predicted for a strictly parallel shock.

Keywords

Cite

@article{arxiv.2212.02349,
  title  = {Particle acceleration at ultrarelativistic, perpendicular shock fronts},
  author = {John G. Kirk and Brian Reville and Zhi-Qiu Huang},
  journal= {arXiv preprint arXiv:2212.02349},
  year   = {2022}
}

Comments

9 pages, 6 figures, accepted for publication in Monthly Notices of the Royal Astronomical Society

R2 v1 2026-06-28T07:22:33.212Z