Turbulence and Particle Acceleration in Shearing Flows

Abstract

We explore constraints imposed by shear-driven instabilities on the acceleration of energetic particles in relativistic shearing flows. We show that shearing layers in large-scale AGN jets are likely to encompass a sizeable fraction ($\ge 0.1$) of the jet radius, requiring seed injection of GeV electrons for efficient acceleration. While the diffusion process may depend on pre-developed turbulence if injection occurs at higher energies, electron acceleration to PeV and proton acceleration to EeV energies appears possible within the constraints imposed by jet stability.

6 pages, 2 figures; ApJL to appear

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Cited by in corpus (7)

• Dynamics of relativistic radio jets in asymmetric environments
• Particle acceleration in shearing flows: the self-generation of turbulent spine-sheath structures in relativistic MHD jet simulations
• Active Galactic Nuclei as potential Sources of Ultra-High Energy Cosmic Rays
• Blazars at Very High Energies: Emission Modelling
• Particle acceleration in shearing flows: the case for large-scale jets
• High energy emission component, population, and contribution to the extragalactic gamma-ray background of gamma-ray emitting radio galaxies
• Particle Acceleration in Relativistic Shearing Flows: Energy Spectrum