PUGLIESE, Daniela and Zdeněk STUCHLÍK. Ringed accretion disks: equilibrium configurations. The Astrophysical Journal Supplement Series. GB - Spojené království Velké Británie a, 2015, vol. 221, No 2, p. 1-40. ISSN 0067-0049. Available from: https://dx.doi.org/10.1088/0067-0049/221/2/25.
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Basic information
Original name Ringed accretion disks: equilibrium configurations
Authors PUGLIESE, Daniela and Zdeněk STUCHLÍK.
Edition The Astrophysical Journal Supplement Series, GB - Spojené království Velké Británie a, 2015, 0067-0049.
Other information
Original language English
Type of outcome Article in a journal
Field of Study 10308 Astronomy
Confidentiality degree is not subject to a state or trade secret
WWW www
Organization unit Faculty of Philosophy and Science in Opava
Doi http://dx.doi.org/10.1088/0067-0049/221/2/25
UT WoS 000366620900003
Keywords in English accretion; black hole physics; hydrodynamics; accretion disks
Tags UF
Tags International impact, Reviewed
Links GB14-37086G, research and development project.
Changed by Changed by: Mgr. Pavlína Jalůvková, učo 25213. Changed: 27/1/2021 10:10.
Abstract
We investigate a model of a ringed accretion disk, made up by several rings rotating around a supermassive Kerr black hole attractor. Each toroid of the ringed disk is governed by the general relativity hydrodynamic Boyer condition of equilibrium configurations of rotating perfect fluids. Properties of the tori can then be determined by an appropriately defined effective potential reflecting the background Kerr geometry and the centrifugal effects. The ringed disks could be created in various regimes during the evolution of matter configurations around supermassive black holes. Therefore, both corotating and counterrotating rings have to be considered as being a constituent of the ringed disk. We provide constraints on the model parameters for the existence and stability of various ringed configurations and discuss occurrence of accretion onto the Kerr black hole and possible launching of jets from the ringed disk. We demonstrate that various ringed disks can be characterized by a maxi
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