Magnetized Black Holes: Ionized Keplerian Disks and
Acceleration of Ultra-High Energy Particles

D 2019

Magnetized Black Holes: Ionized Keplerian Disks and Acceleration of Ultra-High Energy Particles

STUCHLÍK, Zdeněk; Martin KOLOŠ and Arman TURSUNOV

Basic information

Original name

Magnetized Black Holes: Ionized Keplerian Disks and Acceleration of Ultra-High Energy Particles

Authors

STUCHLÍK, Zdeněk (203 Czech Republic, guarantor, belonging to the institution); Martin KOLOŠ (203 Czech Republic, belonging to the institution) and Arman TURSUNOV (860 Uzbekistan, belonging to the institution)

Edition

Basel, Switzerland, Proceedings 2019, 17(1), 13. RPRA 2019 - Recent Progress in Relativistic Astrophysics Fudan University, Shanghai, China, 6–8 May 2019, p. "13-1"-"13-24", 24 pp. 2019

Publisher

Proceedings (MDPI)

Other information

Language

English

Type of outcome

Proceedings paper

Field of Study

10308 Astronomy

Country of publisher

Switzerland

Confidentiality degree

is not subject to a state or trade secret

Publication form

electronic version available online

References:

URL

RIV identification code

RIV/47813059:19240/19:A0000568

Organization unit

Faculty of Philosophy and Science in Opava

ISSN

DOI

https://doi.org/10.3390/proceedings2019017013

Keywords in English

black hole; magnetic field; magnetosphere; charged particle dynamic

Abstract

In the original language

Properties of charged particle motion in the field of magnetized black holes (BHs) imply four possible regimes of behavior of ionized Keplerian disks: survival in regular epicyclic motion, transformation into chaotic toroidal state, destruction due to fall into the BHs, destruction due to escape along magnetic field lines (escape to infinity for disks orbiting Kerr BHs). The regime of the epicyclic motion influenced by very weak magnetic fields can be related to the observed high-frequency quasiperiodic oscillations. In the case of very strong magnetic fields particles escaping to infinity could form UHECR due to extremely efficient magnetic Penrose process – protons with energy E > 10^(21) eV can be accelerated by supermassive black holes with M ~ 10^(10) M_Sun immersed in magnetic field with B~ 10^4 Gs.

Cite

STUCHLÍK, Zdeněk; Martin KOLOŠ and Arman TURSUNOV. Magnetized Black Holes: Ionized Keplerian Disks and Acceleration of Ultra-High Energy Particles. Online. In Cosimo Bambi, Sourabh Nampalliwar. Proceedings 2019, 17(1), 13. RPRA 2019 - Recent Progress in Relativistic Astrophysics Fudan University, Shanghai, China, 6–8 May 2019. Basel, Switzerland: Proceedings (MDPI), 2019, p. "13-1"-"13-24", 24 pp. ISSN 2504-3900. Available from: https://doi.org/10.3390/proceedings2019017013.

@inproceedings{37912,
   author = {Stuchlík, Zdeněk and Kološ, Martin and Tursunov, Arman},
   address = {Basel, Switzerland},
   booktitle = {Proceedings 2019, 17(1), 13. RPRA 2019 - Recent Progress in Relativistic Astrophysics Fudan University, Shanghai, China, 6–8 May 2019},
   doi = {https://doi.org/10.3390/proceedings2019017013},
   editor = {Cosimo Bambi, Sourabh Nampalliwar},
   keywords = {black hole; magnetic field; magnetosphere; charged particle dynamic},
   howpublished = {elektronická verze "online"},
   language = {eng},
   location = {Basel, Switzerland},
   pages = {"13-1"-"13-24"},
   publisher = {Proceedings (MDPI)},
   title = {Magnetized Black Holes: Ionized Keplerian Disks and Acceleration of Ultra-High Energy Particles},
   url = {https://www.mdpi.com/2504-3900/17/1/13},
   year = {2019}
}

TY  - CONF
ID  - 37912
AU  - Stuchlík, Zdeněk - Kološ, Martin - Tursunov, Arman
PY  - 2019
TI  - Magnetized Black Holes: Ionized Keplerian Disks and Acceleration of Ultra-High Energy Particles
PB  - Proceedings (MDPI)
CY  - Basel, Switzerland
KW  - black hole
KW  - magnetic field
KW  - magnetosphere
KW  - charged particle dynamic
UR  - https://www.mdpi.com/2504-3900/17/1/13
L2  - https://www.mdpi.com/2504-3900/17/1/13
N2  - Properties of charged particle motion in the field of magnetized black holes (BHs) imply four possible regimes of behavior of ionized Keplerian disks: survival in regular epicyclic motion, transformation into chaotic toroidal state, destruction due to fall into the BHs, destruction due to escape along magnetic field lines (escape to infinity for disks orbiting Kerr BHs). The regime of the epicyclic motion influenced by very weak magnetic fields can be related to the observed high-frequency quasiperiodic oscillations. In the case of very strong magnetic fields particles escaping to infinity could form UHECR due to extremely efficient magnetic Penrose process – protons with energy E > 10^(21) eV can be accelerated by supermassive black holes with M ~ 10^(10) M_Sun immersed in magnetic field with B~ 10^4 Gs.
ER  -

STUCHLÍK, Zdeněk; Martin KOLOŠ and Arman TURSUNOV. Magnetized Black Holes: Ionized Keplerian Disks and Acceleration of Ultra-High Energy Particles. Online. In Cosimo Bambi, Sourabh Nampalliwar. \textit{Proceedings 2019, 17(1), 13. RPRA 2019 - Recent Progress in Relativistic Astrophysics Fudan University, Shanghai, China, 6–8 May 2019}. Basel, Switzerland: Proceedings (MDPI), 2019, p.~''13-1''-''13-24'', 24 pp. ISSN~2504-3900. Available from: https://doi.org/10.3390/proceedings2019017013.

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