GRMHD Evolution of Interacting Double Accretion Tori Orbiting a
Central Black Hole

J 2022

GRMHD Evolution of Interacting Double Accretion Tori Orbiting a Central Black Hole

BARDIEV, Dilshodbek; Martin KOLOŠ; Daniela PUGLIESE and Zdeněk STUCHLÍK

Basic information

Original name

GRMHD Evolution of Interacting Double Accretion Tori Orbiting a Central Black Hole

Authors

BARDIEV, Dilshodbek (860 Uzbekistan, belonging to the institution); Martin KOLOŠ (203 Czech Republic, belonging to the institution); Daniela PUGLIESE (380 Italy, belonging to the institution) and Zdeněk STUCHLÍK (203 Czech Republic, belonging to the institution)

Edition

Astrophysical Journal, GB - Spojené království Velké Británie a, 2022, 0004-637X

Other information

Language

English

Type of outcome

Article in a journal

Field of Study

10308 Astronomy

Country of publisher

United Kingdom of Great Britain and Northern Ireland

Confidentiality degree

is not subject to a state or trade secret

References:

URL

Impact factor

Impact factor: 4.900

RIV identification code

RIV/47813059:19630/22:A0000202

Organization unit

Institute of physics in Opava

DOI

https://doi.org/10.3847/1538-4357/aca0a3

UT WoS

000901548100001

EID Scopus

2-s2.0-85145370977

Keywords in English

misaligned accreation;tidal disruptions;disks;field

Abstract

In the original language

The matter orbiting black holes (BHs) in microquasars or active galactic nuclei forms toroidal accretion disk structures, and multiple torus structures have been recently described as ringed accretion disks (RADs) in a full general relativistic approach. Here we realize full general relativistic magnetohydrodynamic (GRMHD) numerical simulations related to double toroidal structure immersed in the equatorial plane of the gravitomagnetic field of a central Schwarzschild BH in an asymptotically uniform magnetic field. We study the merging dynamics of an initial RAD structure constructed by two corotating or counterrotating tori, where accretion of matter from the outer torus is assumed onto the inner torus, using the 2.5D GRMHD simulation schemes with the HARM numerical code. We study the dynamics of the system assuming various initial conditions, and we have demonstrated that the initial matter density is the relevant factor governing the system evolution.

Cite

BARDIEV, Dilshodbek; Martin KOLOŠ; Daniela PUGLIESE and Zdeněk STUCHLÍK. GRMHD Evolution of Interacting Double Accretion Tori Orbiting a Central Black Hole. Astrophysical Journal. GB - Spojené království Velké Británie a, 2022, vol. 941, No 2, p. "173-1"-"173-14", 14 pp. ISSN 0004-637X. Available from: https://doi.org/10.3847/1538-4357/aca0a3.

@article{65723,
   author = {Bardiev, Dilshodbek and Kološ, Martin and Pugliese, Daniela and Stuchlík, Zdeněk},
   article_location = {GB - Spojené království Velké Británie a},
   article_number = {2},
   doi = {https://doi.org/10.3847/1538-4357/aca0a3},
   keywords = {misaligned accreation;tidal disruptions;disks;field},
   language = {eng},
   issn = {0004-637X},
   journal = {Astrophysical Journal},
   title = {GRMHD Evolution of Interacting Double Accretion Tori Orbiting a Central Black Hole},
   url = {https://iopscience.iop.org/article/10.3847/1538-4357/aca0a3},
   volume = {941},
   year = {2022}
}

TY  - JOUR
ID  - 65723
AU  - Bardiev, Dilshodbek - Kološ, Martin - Pugliese, Daniela - Stuchlík, Zdeněk
PY  - 2022
TI  - GRMHD Evolution of Interacting Double Accretion Tori Orbiting a Central Black Hole
JF  - Astrophysical Journal
VL  - 941
IS  - 2
SP  - "173-1"-"173-14"
EP  - "173-1"-"173-14"
SN  - 0004637X
KW  - misaligned accreation;tidal disruptions;disks;field
UR  - https://iopscience.iop.org/article/10.3847/1538-4357/aca0a3
N2  - The matter orbiting black holes (BHs) in microquasars or active galactic nuclei forms toroidal accretion disk structures, and multiple torus structures have been recently described as ringed accretion disks (RADs) in a full general relativistic approach. Here we realize full general relativistic magnetohydrodynamic (GRMHD) numerical simulations related to double toroidal structure immersed in the equatorial plane of the gravitomagnetic field of a central Schwarzschild BH in an asymptotically uniform magnetic field. We study the merging dynamics of an initial RAD structure constructed by two corotating or counterrotating tori, where accretion of matter from the outer torus is assumed onto the inner torus, using the 2.5D GRMHD simulation schemes with the HARM numerical code. We study the dynamics of the system assuming various initial conditions, and we have demonstrated that the initial matter density is the relevant factor governing the system evolution.
ER  -

BARDIEV, Dilshodbek; Martin KOLOŠ; Daniela PUGLIESE and Zdeněk STUCHLÍK. GRMHD Evolution of Interacting Double Accretion Tori Orbiting a Central Black Hole. \textit{Astrophysical Journal}. GB - Spojené království Velké Británie a, 2022, vol.~941, No~2, p.~''173-1''-''173-14'', 14 pp. ISSN~0004-637X. Available from: https://doi.org/10.3847/1538-4357/aca0a3.

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