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Proceeding Paper

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

Institute of Physics and Research Centre for Theoretical Physics and Astrophysics, Silesian University in Opava, Bezručovo nám.13, CZ-74601 Opava, Czech Republic
*
Author to whom correspondence should be addressed.
Presented at the meeting Recent Progress in Relativistic Astrophysics, Shanghai, China, 6–8 May 2019.
Proceedings 2019, 17(1), 13; https://doi.org/10.3390/proceedings2019017013
Published: 24 October 2019
(This article belongs to the Proceedings of Recent Progress in Relativistic Astrophysics)

Abstract

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 immersed in magnetic field with B 10 4 Gs.
Keywords: black hole; magnetic field; magnetosphere; charged particle dynamic black hole; magnetic field; magnetosphere; charged particle dynamic

Share and Cite

MDPI and ACS Style

Stuchlík, Z.; Kološ, M.; Tursunov, A. Magnetized Black Holes: Ionized Keplerian Disks and Acceleration of Ultra-High Energy Particles. Proceedings 2019, 17, 13. https://doi.org/10.3390/proceedings2019017013

AMA Style

Stuchlík Z, Kološ M, Tursunov A. Magnetized Black Holes: Ionized Keplerian Disks and Acceleration of Ultra-High Energy Particles. Proceedings. 2019; 17(1):13. https://doi.org/10.3390/proceedings2019017013

Chicago/Turabian Style

Stuchlík, Zdeněk, Martin Kološ, and Arman Tursunov. 2019. "Magnetized Black Holes: Ionized Keplerian Disks and Acceleration of Ultra-High Energy Particles" Proceedings 17, no. 1: 13. https://doi.org/10.3390/proceedings2019017013

APA Style

Stuchlík, Z., Kološ, M., & Tursunov, A. (2019). Magnetized Black Holes: Ionized Keplerian Disks and Acceleration of Ultra-High Energy Particles. Proceedings, 17(1), 13. https://doi.org/10.3390/proceedings2019017013

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