Simulations of black hole accretion torus in various magnetic field configurations

@inproceedings{45604,
   author = {Kološ, Martin and Janiuk, Agnieszka},
   address = {Opava},
   booktitle = {Proceedings of RAGtime 22: Workshops on black holes and neutron stars},
   editor = {Stuchlik Z.,Torok G.,Karas V.},
   keywords = {GRMHD simulation; accretion; black hole; magnetic field},
   howpublished = {tištěná verze "print"},
   language = {eng},
   location = {Opava},
   isbn = {978-80-7510-432-8},
   pages = {153-164},
   publisher = {Slezská univerzita v Opavě, Fyzikální ústav v Opavě},
   title = {Simulations of black hole accretion torus in various magnetic field configurations},
   url = {http://proceedings.physics.cz/images/proc21/kol2.pdf},
   year = {2020}
}

TY  - JOUR
ID  - 45604
AU  - Kološ, Martin - Janiuk, Agnieszka
PY  - 2020
TI  - Simulations of black hole accretion torus in various magnetic field configurations
PB  - Slezská univerzita v Opavě, Fyzikální ústav v Opavě
CY  - Opava
SN  - 9788075104328
KW  - GRMHD simulation
KW  - accretion
KW  - black hole
KW  - magnetic field
UR  - http://proceedings.physics.cz/images/proc21/kol2.pdf
N2  - 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.
ER  - 

KOLOŠ, Martin a Agnieszka JANIUK. Simulations of black hole accretion torus in various magnetic field configurations. In Stuchlik Z.,Torok G.,Karas V. \textit{Proceedings of RAGtime 22: Workshops on black holes and neutron stars}. Opava: Slezská univerzita v Opavě, Fyzikální ústav v Opavě, 2020, s.~153-164. ISBN~978-80-7510-432-8.