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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Veröffentlicht in:	The Astrophysical journal 2024-09, Vol.973 (1), p.45
Hauptverfasser:	Asahina, Yuta, Ohsuga, Ken
Format:	Artikel
Sprache:	eng
Schlagworte:	Accretion Accretion disks Black holes General relativity Luminosity Magnetohydrodynamic simulation Magnetohydrodynamics Precession Radiation Radiative magnetohydrodynamics Relativistic effects Rotating disks Solar oscillations Time X ray sources
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