Particles acceleration in quasi-perpendicular non-relativistic High Mach number shocks

Video Player is loading.
Loaded: 0%
Remaining Time 0:00
1x
  • Quality
    • 149 views

    • 0 favorites

    • uploaded July 7, 2021

    Discussion timeslot (ZOOM-Meeting): 16. July 2021 - 12:00
    ZOOM-Meeting URL: https://desy.zoom.us/j/92210078166
    ZOOM-Meeting ID: 92210078166
    ZOOM-Meeting Passcode: ICRC2021
    Corresponding Session: https://icrc2021-venue.desy.de/channel/12-Galactic-Particle-Acceleration-including-PIC-CRI-CRD-MM/127
    Live-Stream URL: https://icrc2021-venue.desy.de/livestream/Discussion-03/4

    Abstract:
    'Electron and ion acceleration at a non-relativistic collisionless shock is studied by employing large scale one-dimensional particle-in-cell (PIC) simulations in the de-Hoffmann and Teller (dHT) frame of reference. We demonstrate that diffusive shock acceleration of both electrons and ions occurs in quasi-perpendicular shocks configurations at large Alfven Mach numbers. We also identify the role of precursor waves on the electron energization in the upstream region. The emergence of a significant non-thermal ion component holds important implications for observations of hadronic emission from collisionless shocks occurring for example in supernova remnants, and colliding stellar winds.'

    Authors: Naveen Kumar
    Co-Authors: Brian Reville
    Indico-ID: 1377
    Proceeding URL: https://pos.sissa.it/395/485

    Tags:
    Presenter:

    Naveen Kumar


    More Media in "Cosmic Ray Indirect"