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System-size Convergence of Nonthermal Particle Acceleration in Relativistic Plasma Turbulence

TitleSystem-size Convergence of Nonthermal Particle Acceleration in Relativistic Plasma Turbulence
Publication TypeJournal Article
Year of Publication2018
AuthorsZhdankin, V, Uzdensky, DA, Werner, GR, Begelman, MC
JournalThe Astrophysical Journal
Volume867
Issue1
Date Published2018-10
Keywordsmagnetohydrodynamics, particle acceleration, plasmas, turbulence
Abstract

We apply collisionless particle-in-cell simulations of relativistic pair plasmas to explore whether driven turbulence is a viable high-energy astrophysical particle accelerator. We characterize nonthermal particle distributions for varying system sizes up to L/2πρe0 = 163, where L/2π is the driving scale and ρe0 is the initial characteristic Larmor radius. We show that turbulent particle acceleration produces power-law energy distributions that, when compared at a fixed number of large-scale dynamical times, slowly steepen with increasing system size. We demonstrate, however, that convergence is obtained by comparing the distributions at different times that increase with system size (approximately logarithmically). We suggest that the system-size dependence arises from the time required for particles to reach the highest accessible energies via Fermi acceleration. The converged power-law index of the energy distribution, α ≈ 3.0 for magnetization σ = 3/8, makes turbulence a possible explanation for nonthermal spectra observed in systems such as the Crab Nebula.

URLhttp://iopscience.iop.org/article/10.3847/2041-8213/aae88c/meta
DOI10.3847/2041-8213/aae88c

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