Particle Acceleration Time due to Turbulent-Induced Magnetic Reconnection

arXiv:2410.13071 · astro-ph.HE, hep-ph · Submitted 2026-08-17 · Read on arXiv

Elisabete M. de Gouveia Dal Pino, Tania E. Medina-Torrejon

astro-ph.HE, hep-ph

Submitted: 2026-08-17

Updated: 2026-08-19

Comments: Accepted for publication in the ApJ

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

Terminology

• AGN — 1× in this paper · explained in 1 episode
• Accretion Flows — 1× in this paper · explained in 1 episode
• Consistency — 1× in this paper · explained in 3 episodes
• Kavli Institute for Theoretical Physics — 1× in this paper
• Magnetohydrodynamics (MHD) — 1× in this paper · explained in 3 episodes
• Robustness — 1× in this paper · explained in 5 episodes

Sources

• Diffusion of large-scale magnetic fields by reconnection in MHD turbulence
• Do plasmoids induce fast magnetic reconnection in well-resolved current sheets in 2D MHD simulations?
• Search for Magnetic Monopoles in Magnetic Reconnection Regions

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