Radiative Efficiency Enhancement by Electromagnetic Energy Dissipation in Strongly Magnetized Supercritical Accretion Flows around Kerr Black Holes

arXiv:2609.03250 · astro-ph.HE · Submitted 2026-09-03 · Read on arXiv

astro-ph.HE

Submitted: 2026-09-03

Updated: 2026-09-03

Terminology

• Accretion Flows — 12× in this paper · explained in 1 episode
• Degeneracy — 2× in this paper · explained in 3 episodes
• AGN — 1× in this paper · explained in 1 episode
• Angular Momentum Transport — 1× in this paper · explained in 3 episodes
• Consistency — 1× in this paper · explained in 3 episodes
• Magnetohydrodynamics (MHD) — 1× in this paper · explained in 3 episodes
• Robustness — 1× in this paper · explained in 5 episodes

Sources

• Black Hole Binaries
• Acceleration of wind in optically thin and thick black hole accretion disks simulated in general relativity
• A Novel Jet Model: Magnetically Collimated, Radiation-Pressure Driven Jet

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