3D Global Relativistic Radiation Magnetohydrodynamics of Magnetically Arrested Disk Accretion Flows in Active Galactic Nuclei

We perform 3D radiation-relativistic magnetohydrodynamic (3D Rad-RMHD) simulations of accretion flows around spinning active galactic nuclei. Our study focuses on the magnetically arrested disk (MAD) state, adopting a single-temperature model that includes bremsstrahlung opacity as the sole radiatio...

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Bibliographic Details

Main Authors:	Ramiz Aktar, Kuo-Chuan Pan, Toru Okuda
Format:	Artigo
Language:	Inglês
Published:	IOP Publishing 2026-01-01
Series:	The Astrophysical Journal
Subjects:	Accretion Black hole physics Magnetohydrodynamics Radiative magnetohydrodynamics Relativistic jets Supermassive black holes
Online Access:	https://doi.org/10.3847/1538-4357/ae5184
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