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Dragged surfaces. On the accretion tori in the ergoregion

The result's identifiers

  • Result code in IS VaVaI

    <a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F47813059%3A19630%2F21%3AA0000149" target="_blank" >RIV/47813059:19630/21:A0000149 - isvavai.cz</a>

  • Result on the web

    <a href="https://academic.oup.com/pasj/article-abstract/73/6/1497/6413829?redirectedFrom=fulltext" target="_blank" >https://academic.oup.com/pasj/article-abstract/73/6/1497/6413829?redirectedFrom=fulltext</a>

  • DOI - Digital Object Identifier

    <a href="http://dx.doi.org/10.1093/pasj/psab093" target="_blank" >10.1093/pasj/psab093</a>

Alternative languages

  • Result language

    angličtina

  • Original language name

    Dragged surfaces. On the accretion tori in the ergoregion

  • Original language description

    We discuss the conditions for the existence of extended matter configurations orbiting in the ergoregion or close to the outer ergosurface of the Kerr black hole ("dragged" configurations). The co-rotating tori under consideration are perfect fluid configurations with barotropic equations of state, orbiting on the equatorial plane of the central Kerr black hole. The possibility of magnetized tori with a toroidal magnetic field is also discussed. Indications on the attractors where dragged tori can be observed are provided with the analysis of the fluid characteristics and geometrical features, relevant for the torus stability and their observations. QPO emissions from the inner edges of the dragged tori are also discussed. We argue that the smaller dragged tori could be subjected to a characteristic instability: the effect of the frame-dragging. This possibility is thoroughly explored. This can finally lead to the destruction of the torus (disk exfoliation) which can combine with accretion and processes present in the region very close to the black hole horizon. Tori are characterized according to the central attractor dimensionless spin. These structures can be observed in orbiting black holes with dimensionless spin a &gt; 0.9897 M.

  • 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

  • Continuities

    I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace

Others

  • Publication year

    2021

  • Confidentiality

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

Data specific for result type

  • Name of the periodical

    Publications Of The Astronomical Society Of Japan

  • ISSN

    0004-6264

  • e-ISSN

    2053-051X

  • Volume of the periodical

    73

  • Issue of the periodical within the volume

    6

  • Country of publishing house

    GB - UNITED KINGDOM

  • Number of pages

    43

  • Pages from-to

    1497-1539

  • UT code for WoS article

    000733238200006

  • EID of the result in the Scopus database

    2-s2.0-85122462049