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Ringed Accretion Disks: Evolution of Double Toroidal Configurations

The result's identifiers

  • Result code in IS VaVaI

    <a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F47813059%3A19240%2F17%3AA0000024" target="_blank" >RIV/47813059:19240/17:A0000024 - isvavai.cz</a>

  • Result on the web

    <a href="http://iopscience.iop.org/article/10.3847/1538-4365/aa68e6/meta" target="_blank" >http://iopscience.iop.org/article/10.3847/1538-4365/aa68e6/meta</a>

  • DOI - Digital Object Identifier

    <a href="http://dx.doi.org/10.3847/1538-4365/aa68e6" target="_blank" >10.3847/1538-4365/aa68e6</a>

Alternative languages

  • Result language

    angličtina

  • Original language name

    Ringed Accretion Disks: Evolution of Double Toroidal Configurations

  • Original language description

    We investigate ringed accretion disks composed of two tori (rings) orbiting on the equatorial plane of a central supermassive Kerr black hole. We discuss the emergence of the instability phases of each ring of the macro-configuration (ringed disk) according to the Paczynski violation of mechanical equilibrium. In the full general relativistic treatment, we consider the effects of the geometry of the Kerr spacetimes relevant to the characterization of the evolution of these configurations. The discussion of ring stability in different spacetimes enables us to identify particular classes of central Kerr attractors depending on their dimensionless spin. As a result of this analysis, we set constraints on the evolutionary schemes of the ringed disks relative to the torus morphology and on their rotation relative to the central black hole and to each other. The dynamics of the unstable phases of this system is significant for the high-energy phenomena related to accretion onto supermassive black holes in active galactic nuclei and the extremely energetic phenomena in quasars, which could be observed in their X-ray emission.

  • Czech name

  • Czech description

Classification

  • Type

    J<sub>imp</sub> - Article in a specialist periodical, which is included in the Web of Science database

  • CEP classification

  • OECD FORD branch

    10308 - Astronomy (including astrophysics,space science)

Result continuities

  • Project

    Result was created during the realization of more than one project. More information in the Projects tab.

  • Continuities

    P - Projekt vyzkumu a vyvoje financovany z verejnych zdroju (s odkazem do CEP)<br>I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace

Others

  • Publication year

    2017

  • Confidentiality

    S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

Data specific for result type

  • Name of the periodical

    Astrophysical Journal Supplement Series

  • ISSN

    0067-0049

  • e-ISSN

    1538-4365

  • Volume of the periodical

    229

  • Issue of the periodical within the volume

    2

  • Country of publishing house

    GB - UNITED KINGDOM

  • Number of pages

    28

  • Pages from-to

    '40-1'-'40-28'

  • UT code for WoS article

    000399583600003

  • EID of the result in the Scopus database

    2-s2.0-85018942105