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Are Reconnection X-points Important for Nonthermal Particle Acceleration in Relativistic Magnetic Reconnection?

ORAL · Invited

Abstract

There is strong evidence suggesting that reconnection is an efficient process for producing energetic particles various plasma systems. Reconnection x-points (regions with electric field larger than the magnetic field for a vanishing guide field) have been suggested to be important for particle injection that boosts particle energy to the lower energy bound of the power-law energy distribution in relativistic magnetic reconnection. We carry out particle-in-cell kinetic simulations and analyses to elucidate the roles of x-points among different injection mechanisms during nonthermal particle acceleration in relativistic magnetic reconnection. We show that for a vanishing guide field, the x-points can only host particles for a short time, leading to a limited energy gain insufficient for particle injection. Meanwhile, most energy gain for particle injection and nonthermal particle acceleration are through regions outside of the x-points. Interestingly, we also find that some energy gain already occurs before particles interact with the x-points. By evolving a test-particle component in the PIC simulation that does not "see" the x-point electric field, we show that particles can still be efficiently accelerated. Meanwhile, the mechanisms associated with electric field perpendicular to the magnetic field outside the x-points dominates the injection process. We conclude that X-points are not important for particle injection or nonthermal particle acceleration during relativistic magnetic reconnection.

Presenters

  • Fan Guo

    Los Alamos National Laboratory

Authors

  • Fan Guo

    Los Alamos National Laboratory

  • Xiaocan Li

    Dartmouth College

  • Omar J French

    University of Colorado, Boulder

  • Qile Zhang

    Los Alamos National Laboratory

  • William S Daughton

    Los Alamos Natl Lab

  • Yi-Hsin Liu

    Dartmouth College

  • William H Matthaeus

    University of Delaware

  • Patrick Kilian

    Space Science Institute

  • Grant Johnson

    Princeton Plasma Physics Laboratory

  • Hui Li

    LANL