On the Viscous Ringed Disk Evolution in the Kerr Black Hole Spacetime

Supermassive black holes <b>(SMBHs)</b> are observed in active galactic nuclei interacting with their environments, where chaotical, discontinuous accretion episodes may leave matter remnants orbiting the central attractor in the form of sequences of orbiting toroidal structures, with st...

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Bibliographic Details
Main Authors: Daniela Pugliese, Zdenek Stuchlík, Vladimir Karas
Format: Article
Language:English
Published: MDPI AG 2024-11-01
Series:Universe
Subjects:
Online Access:https://www.mdpi.com/2218-1997/10/12/435
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