Relativistic Nonthermal Particle Acceleration in Two-Dimensional Collisionless Magnetic Reconnection
Dmitri A. Uzdensky (Univ. Colorado Boulder)

TL;DR
This paper presents an analytical model explaining how relativistic magnetic reconnection accelerates particles to nonthermal energies, linking the particle spectrum's features to plasma magnetization, system size, and plasmoid dynamics.
Contribution
The paper introduces a simple self-similar analytical model that explains the dependencies of particle energy spectra on plasma parameters in relativistic reconnection.
Findings
Power-law index depends on the balance between electric acceleration and magnetization.
High-energy cutoff is governed by particle trapping in large plasmoids.
Model aligns with numerical observations of particle spectra in reconnection.
Abstract
Magnetic reconnection, especially in the relativistic regime, provides an efficient mechanism for accelerating relativistic particles and thus offers an attractive physical explanation for nonthermal high-energy emission from various astrophysical sources. I present a simple analytical model that elucidates key physical processes responsible for reconnection-driven relativistic nonthermal particle acceleration (NTPA) in the large-system, plasmoid-dominated regime in two dimensions. The model aims to explain the numerically-observed dependencies of the power-law index and high-energy cutoff of the resulting nonthermal particle energy spectrum on the ambient plasma magnetization , and (for ) on the system size . In this self-similar model, energetic particles are continuously accelerated by the out-of-plane reconnection electric field…
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