Composition-dependent acceleration of UHE Cosmic Rays in AGN electric fields

arXiv:2609.28668 · astro-ph.HE · Submitted 2026-09-23 · Read on arXiv

astro-ph.HE

Submitted: 2026-09-23

Updated: 2026-09-23

Terminology

• AGN — 33× in this paper · explained in 1 episode
• Abundance — 11× in this paper · explained in 1 episode
• Trace — 6× in this paper · explained in 2 episodes
• Benchmark — 5× in this paper · explained in 2 episodes
• Degeneracy — 5× in this paper · explained in 3 episodes
• AGN Environments — 3× in this paper · explained in 1 episode
• Accretion Flows — 2× in this paper · explained in 1 episode
• Bayesian Inference — 2× in this paper · explained in 5 episodes
• Active Galactic Nuclei (AGN) — 1× in this paper · explained in 1 episode
• Anisotropy — 1× in this paper · explained in 3 episodes
• Consistency — 1× in this paper · explained in 3 episodes
• Core — 1× in this paper · explained in 2 episodes
• Generative AI — 1× in this paper · explained in 2 episodes
• Monte Carlo framework — 1× in this paper · explained in 2 episodes

Sources

• Modeling individual nearby radio galaxies as ultra-high-energy cosmic-ray accelerators
• EPOS LHC : test of collective hadronization with LHC data
• Particle Acceleration in Collisionless Magnetically Arrested Disks

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