EPJ Web of Conferences (Jan 2020)

Studying particle acceleration from driven magnetic reconnection at the termination shock of a relativistic striped wind using particle-in-cell simulations

  • Lu Yingchao,
  • Guo Fan,
  • Kilian Patrick,
  • Li Hui,
  • Huang Chengkun,
  • Liang Edison

DOI
https://doi.org/10.1051/epjconf/202023507003
Journal volume & issue
Vol. 235
p. 07003

Abstract

Read online

A rotating pulsar creates a surrounding pulsar wind nebula (PWN) by steadily releasing an energetic wind into the interior of the expanding shockwave of supernova remnant or interstellar medium. At the termination shock of a PWN, the Poynting-flux- dominated relativistic striped wind is compressed. Magnetic reconnection is driven by the compression and converts magnetic energy into particle kinetic energy and accelerating particles to high energies. We carrying out particle-in-cell (PIC) simulations to study the shock structure as well as the energy conversion and particle acceleration mechanism. By analyzing particle trajectories, we find that many particles are accelerated by Fermi-type mechanism. The maximum energy for electrons and positrons can reach hundreds of TeV.