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 > 0.9897 M.
Czech name
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Czech description
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Classification
Type
J<sub>imp</sub> - Article in a specialist periodical, which is included in the Web of Science database
CEP classification
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OECD FORD branch
10308 - Astronomy (including astrophysics,space science)
Result continuities
Project
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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