Simulations of black hole accretion torus in various magnetic field configurations

Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F47813059%3A19630%2F20%3AA0000048" target="_blank" >RIV/47813059:19630/20:A0000048 - isvavai.cz</a>
Result on the web
<a href="http://proceedings.physics.cz/images/proc21/kol2.pdf" target="_blank" >http://proceedings.physics.cz/images/proc21/kol2.pdf</a>
DOI - Digital Object Identifier
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Result language
angličtina
Original language name
Simulations of black hole accretion torus in various magnetic field configurations
Original language description
Using general relativistic magnetohydrodynamics simulations we study evolutionof accretion torus around black hole endowed with five different initial magneticfield configurations: contour, loop, parabolic, monopole, uniform. Due to accretion of material onto black hole, parabolic magnetic field will develop in accretion torusfunnel around vertical axis, while turbulent and chaotic magnetic field insideaccretion torus will redistribute angular momentum inside torus and create corona around it.
Czech name
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Czech description
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Project
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Continuities
I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace

Publication year
2020
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

Article name in the collection
Proceedings of RAGtime 22: Workshops on black holes and neutron stars
ISBN
9788075104328
ISSN
2336-5676
e-ISSN
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Number of pages
12
Pages from-to
153-164
Publisher name
Slezská univerzita v Opavě, Fyzikální ústav v Opavě
Place of publication
Opava
Event location
Opava
Event date
Oct 19, 2020
Type of event by nationality
WRD - Celosvětová akce
UT code for WoS article
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