General Relativistic Radiation Magnetohydrodynamics Simulations of Precessing Tilted Super-Eddington Disks

We perform a three-dimensional general relativistic radiation magnetohydrodynamics simulation of a tilted super-Eddington accretion disk around a spinning black hole (BH). The disk, which tilts and twists as it approaches the BH, precesses while maintaining its shape. The gas is mainly ejected aroun...

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Bibliographic Details

Published in:	The Astrophysical Journal
Main Authors:	Yuta Asahina, Ken Ohsuga
Format:	Article
Language:	English
Published:	IOP Publishing 2024-01-01
Subjects:	Black holes Accretion Radiative magnetohydrodynamics General relativity
Online Access:	https://doi.org/10.3847/1538-4357/ad6cd9