TURIMOV, Bobur, Javlon RAYIMBAEV, Ahmadjon ABDUJABBAROV, Bobomurat AHMEDOV and Zdeněk STUCHLÍK. Test particle motion around a black hole in Einstein-Maxwell-scalar theory. Physical Review D. US - Spojené státy americké, 2020, vol. 102, No 6, p. "064052-1"-"064052-14", 14 pp. ISSN 1550-7998. Available from: https://dx.doi.org/10.1103/PhysRevD.102.064052.
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Basic information
Original name Test particle motion around a black hole in Einstein-Maxwell-scalar theory
Authors TURIMOV, Bobur (860 Uzbekistan, belonging to the institution), Javlon RAYIMBAEV, Ahmadjon ABDUJABBAROV (860 Uzbekistan), Bobomurat AHMEDOV (860 Uzbekistan) and Zdeněk STUCHLÍK (203 Czech Republic, belonging to the institution).
Edition Physical Review D, US - Spojené státy americké, 2020, 1550-7998.
Other information
Original language English
Type of outcome Article in a journal
Field of Study 10308 Astronomy
Country of publisher United States of America
Confidentiality degree is not subject to a state or trade secret
WWW URL
RIV identification code RIV/47813059:19630/20:A0000068
Organization unit Institute of physics in Opava
Doi http://dx.doi.org/10.1103/PhysRevD.102.064052
UT WoS 000570979500003
Keywords in English MAGNETIZED ORBITS; FIELD-THEORIES; SPACETIMES; GRAVITY; RESONANCE; CONSTANT; DYNAMICS; ENERGY; CHAOS; SPIN
Tags , FÚ2020, RIV21, SGS12-2019
Tags International impact, Reviewed
Changed by Changed by: Mgr. Pavlína Jalůvková, učo 25213. Changed: 19/4/2021 13:15.
Abstract
In this paper, we explore the test particle motion around black hole in Einstein-Maxwell-scalar (EMS) theory using three different black hole solutions within this theory. We have first analyzed the spacetime curvature structure of these solutions and shown the existence of two singularities and the first one is at the center r = 0. In black hole spacetime, there are two regions divided by the critical value of the cosmological parameter lambda(0). The photon sphere around black hole in EMS theory has also been studied and found that it does not depend on cosmological parameter lambda. We have analyzed the innermost stable circular orbits (ISCO) around black hole and shown that for all solutions ISCO radius for neutral particle decreases with the increase of black hole charge. We have also studied the charged particle motion around the black hole where charged particle motion is considered in the presence of gravitational field and the Coulomb potential. It is shown that ISCO radius for charged particles increases depending on the selected value of the coupling parameter which is in contradiction with observations of the inner edge of the accretion disks of the astrophysical black holes and can be used as powerful tool to rule out the EMS theory from consideration for the gravitational field theory. It also studied the fundamental frequencies governed by test particle orbiting around black hole in EMS theory. Finally, as test of black hole solution in EMS theory ISCO radii is compared with that in Kerr black hole and found that the spin parameter of Kerr can be mimic up to a/M similar or equal to 0.936.
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