Particle Acceleration in Magnetized Shear-Driven Turbulence

arXiv:2512.12720 · astro-ph.HE · Submitted 2025-12-14 · Read on arXiv

astro-ph.HE

Submitted: 2025-12-14

Updated: 2026-09-07

Comments: 25 pages, 18 figures. Accepted by ApJ

License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/

Terminology

• Anisotropy — 11× in this paper · explained in 3 episodes
• Alignment — 5× in this paper · explained in 1 episode
• AGN — 4× in this paper · explained in 1 episode
• Accretion Flows — 2× in this paper · explained in 1 episode
• Accuracy — 2× in this paper · explained in 1 episode
• Coherence Length — 2× in this paper · explained in 2 episodes
• Robustness — 2× in this paper · explained in 5 episodes
• Adam — 1× in this paper · explained in 2 episodes
• Aspen Center for Physics — 1× in this paper
• Cold front — 1× in this paper · explained in 2 episodes
• Kavli Institute for Theoretical Physics — 1× in this paper
• Momentum transfer — 1× in this paper · explained in 2 episodes
• Systematic Bias — 1× in this paper · explained in 3 episodes

Sources

• Studying the mirror acceleration via kinetic simulations of relativistic plasma turbulence
• Hybrid Simulations of Supersonic Shear Flows: I) Particle Acceleration
• Dissipation and particle acceleration in astrophysical jets with velocity and magnetic shear: Interaction of Kelvin-Helmholtz and Drift-Kink Instabilities

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