Litcius/Paper detail

The acceleration of charged particles and formation of power-law energy spectra in nonrelativistic magnetic reconnection

Xiaocan Li, Fan Guo, Yi-Hsin Liu

2021Physics of Plasmas42 citationsDOIOpen Access PDF

Abstract

Magnetic reconnection is a primary driver of particle acceleration processes in space and astrophysical plasmas. Understanding how particles are accelerated and the resulting particle energy spectra are among the central topics in reconnection studies. We review recent advances in addressing this problem in nonrelativistic reconnection that is relevant to space and solar plasmas and beyond. We focus on particle acceleration mechanisms, particle transport due to 3D reconnection physics, and their roles in forming power-law particle energy spectra. We conclude by pointing out the challenges in studying particle acceleration and transport in a large-scale reconnection layer and the relevant issues to be addressed in the future.

Topics & Concepts

PhysicsMagnetic reconnectionParticle accelerationAccelerationCharged particlePlasmaParticle (ecology)Astrophysical plasmaComputational physicsSpace (punctuation)Spectral lineSolar energetic particlesRelativistic particleEnergy transportEnergy (signal processing)Current sheetQuantum electrodynamicsMagnetic fieldClassical mechanicsCharged particle beamFocus (optics)Atomic physicsSolar flarePlasma accelerationField (mathematics)Electric fieldParticle beamIonosphere and magnetosphere dynamicsSolar and Space Plasma DynamicsLightning and Electromagnetic Phenomena
The acceleration of charged particles and formation of power-law energy spectra in nonrelativistic magnetic reconnection | Litcius