Are GRMHD Mean-Field Dynamo Models of Thick Accretion Disks SANE?

The remarkable results by the Event Horizon Telescope collaboration concerning the emission from M87* and, more recently, its polarization properties, require an increasingly accurate modeling of the plasma flows around the accreting black hole. Radiatively inefficient sources such as M87* and Sgr A...

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Bibliographic Details
Published in:	Universe
Main Authors:	Niccolò Tomei, Luca Del Zanna, Matteo Bugli, Niccolò Bucciantini
Format:	Article
Language:	English
Published:	MDPI AG 2021-07-01
Subjects:	accretion disks relativistic processes magnetohydrodynamics (MHD) dynamo
Online Access:	https://www.mdpi.com/2218-1997/7/8/259

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