Turbulence and Particle Acceleration in Shearing Flows
arXiv:2101.06014 · doi:10.3847/2041-8213/abd567
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 () 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
References in corpus (14)
- Kinematics of the jet in M87 on scales of 100 -- 1000 Schwarzschild radii
- A numerical simulation of the evolution and fate of a FRI jet. The case of 3C 31
- Formation of dynamical structures in relativistic jets: the FRI case
- Three-Dimensional Relativistic MHD Simulations of the Kelvin-Helmholtz Instability: Magnetic Field Amplification by a Turbulent Dynamo
- A microscopic analysis of shear acceleration
- Resolving acceleration to very high energies along the Jet of Centaurus A
- Particle Acceleration in Mildly Relativistic Shearing Flows: the Interplay of Systematic and Stochastic Effects, and the Origin of the Extended High-energy Emission in AGN Jets
- Resonant Kelvin-Helmholtz modes in sheared relativistic flows
- Particle Acceleration in Shearing Flows: Efficiencies and Limits
- Triggering mixing and deceleration in FRI jets: a solution
- Constraining the shear acceleration model for the X-ray emission of large-scale extragalactic jets
- Derivation of the physical parameters of the jet in S5 0836+710 from stability analysis
- Shear Acceleration in Expanding Flows
- On radiative acceleration in spine-sheath structured blazar jets