Particle motion around generic black holes coupled to non-linear electrodynamics

Abstract We study spherically symmetric magnetically charged generic black hole solutions of general relativity coupled to non-linear electrodynamics (NED). For characteristic values of the generic spacetime parameters we give the position of horizons in dependence on the charge parameter, demonstra...

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Main Authors: Jaroslav Vrba, Ahmadjon Abdujabbarov, Arman Tursunov, Bobomurat Ahmedov, Zdeněk Stuchlík
Format: Article
Language:English
Published: SpringerOpen 2019-09-01
Series:European Physical Journal C: Particles and Fields
Online Access:http://link.springer.com/article/10.1140/epjc/s10052-019-7286-2
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author Jaroslav Vrba
Ahmadjon Abdujabbarov
Arman Tursunov
Bobomurat Ahmedov
Zdeněk Stuchlík
author_facet Jaroslav Vrba
Ahmadjon Abdujabbarov
Arman Tursunov
Bobomurat Ahmedov
Zdeněk Stuchlík
author_sort Jaroslav Vrba
collection DOAJ
description Abstract We study spherically symmetric magnetically charged generic black hole solutions of general relativity coupled to non-linear electrodynamics (NED). For characteristic values of the generic spacetime parameters we give the position of horizons in dependence on the charge parameter, demonstrating separation of the black hole and no-horizon solutions, and possibility of existence of solutions containing three horizons. We show that null, weak and strong energy conditions are violated when the outer horizon is approaching the center. We study effective potentials for photons and massive test particles and location of circular photon orbits (CPO) and innermost stable circular orbit (ISCO). We show that the unstable photon orbit can become stable, leading to the possibility of photon capture which affects on silhouette of the central object. The position of ISCO approaches the horizon with increasing charge parameter q and the energy at ISCO decreases with increasing charge parameter. We investigate this phenomenon and summarize for a variety of the generic spacetime parameters the upper estimate on the spin parameter of the Kerr black which can be mimicked by the generic charged black hole solutions.
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spelling doaj.art-e8db1ed654a642e99a581fe4a13d06172022-12-22T00:59:00ZengSpringerOpenEuropean Physical Journal C: Particles and Fields1434-60441434-60522019-09-0179911510.1140/epjc/s10052-019-7286-2Particle motion around generic black holes coupled to non-linear electrodynamicsJaroslav Vrba0Ahmadjon Abdujabbarov1Arman Tursunov2Bobomurat Ahmedov3Zdeněk Stuchlík4Institute of Physics and Research Centre of Theoretical Physics and Astrophysics, Faculty of Philosophy and Science, Silesian University in OpavaAmity University in TashkentInstitute of Physics and Research Centre of Theoretical Physics and Astrophysics, Faculty of Philosophy and Science, Silesian University in OpavaUlugh Beg Astronomical InstituteInstitute of Physics and Research Centre of Theoretical Physics and Astrophysics, Faculty of Philosophy and Science, Silesian University in OpavaAbstract We study spherically symmetric magnetically charged generic black hole solutions of general relativity coupled to non-linear electrodynamics (NED). For characteristic values of the generic spacetime parameters we give the position of horizons in dependence on the charge parameter, demonstrating separation of the black hole and no-horizon solutions, and possibility of existence of solutions containing three horizons. We show that null, weak and strong energy conditions are violated when the outer horizon is approaching the center. We study effective potentials for photons and massive test particles and location of circular photon orbits (CPO) and innermost stable circular orbit (ISCO). We show that the unstable photon orbit can become stable, leading to the possibility of photon capture which affects on silhouette of the central object. The position of ISCO approaches the horizon with increasing charge parameter q and the energy at ISCO decreases with increasing charge parameter. We investigate this phenomenon and summarize for a variety of the generic spacetime parameters the upper estimate on the spin parameter of the Kerr black which can be mimicked by the generic charged black hole solutions.http://link.springer.com/article/10.1140/epjc/s10052-019-7286-2
spellingShingle Jaroslav Vrba
Ahmadjon Abdujabbarov
Arman Tursunov
Bobomurat Ahmedov
Zdeněk Stuchlík
Particle motion around generic black holes coupled to non-linear electrodynamics
European Physical Journal C: Particles and Fields
title Particle motion around generic black holes coupled to non-linear electrodynamics
title_full Particle motion around generic black holes coupled to non-linear electrodynamics
title_fullStr Particle motion around generic black holes coupled to non-linear electrodynamics
title_full_unstemmed Particle motion around generic black holes coupled to non-linear electrodynamics
title_short Particle motion around generic black holes coupled to non-linear electrodynamics
title_sort particle motion around generic black holes coupled to non linear electrodynamics
url http://link.springer.com/article/10.1140/epjc/s10052-019-7286-2
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AT ahmadjonabdujabbarov particlemotionaroundgenericblackholescoupledtononlinearelectrodynamics
AT armantursunov particlemotionaroundgenericblackholescoupledtononlinearelectrodynamics
AT bobomuratahmedov particlemotionaroundgenericblackholescoupledtononlinearelectrodynamics
AT zdenekstuchlik particlemotionaroundgenericblackholescoupledtononlinearelectrodynamics