J 2021

On exact analytical solution of Einstein-Maxwell-scalar field equations

TURIMOV, Bobur, Bobomurat AHMEDOV and Zdeněk STUCHLÍK

Basic information

Original name

On exact analytical solution of Einstein-Maxwell-scalar field equations

Authors

TURIMOV, Bobur (860 Uzbekistan, belonging to the institution), Bobomurat AHMEDOV (860 Uzbekistan) and Zdeněk STUCHLÍK (203 Czech Republic, belonging to the institution)

Edition

Physics of the Dark Universe, Netherlands, 2021, 2212-6864

Other information

Language

English

Type of outcome

Článek v odborném periodiku

Field of Study

10308 Astronomy

Country of publisher

Netherlands

Confidentiality degree

není předmětem státního či obchodního tajemství

References:

URL

RIV identification code

RIV/47813059:19630/21:A0000141

Organization unit

Institute of physics in Opava

DOI

http://dx.doi.org/10.1016/j.dark.2021.100868

UT WoS

000704383100031

Keywords in English

Einstein-Maxwell-scalar equations;Exact solutions;Curvature invariants;Naked singularity;Geodesic motion

Tags

2022, , RIV22, SGS-12-2019

Tags

International impact, Reviewed
Změněno: 28/3/2022 11:33, Mgr. Pavlína Jalůvková

Abstract

V originále

The exact analytical solution of Einstein-Maxwell-scalar (EMS) field equations has been explored which covers several well-known solutions such as the Reissner-Nordstrom, Schwarzschild-MOG (Modified Gravity), Janis-Newman-Winicour, and Schwarzschild solutions. It has been assumed that the interactions between the tensor, vector, and scalar fields are negligible. The newly obtained solution is characterized by three free parameters as the total mass M, electric (magnetic) charge Q(e) (Q(m)), and scalar charge C (or n parameter) of the gravitational compact object. It is also shown that dual solution for the vector potential A(phi) = Q(m) cos theta is satisfied by the EMS field equations and the electric charge can be safely replaced by magnetic charge Q(m). Finally, we have studied curvature invariants and test particle motion around the gravitational source described the obtained new spacetime metric. We have also provided analysis of degeneracy values of spin parameter of the rotating Kerr black hole and charge parameter of compact object described by the new spacetime metric through comparison of radii of ISCO, photonsphere and energy efficiency. It is shown that new black hole solution in Einstein-Maxwell-scalar field theory can mimic spin parameter of the Kerr black hole up to a(*) less than or similar to 0.6 while the astrophysical black hole' observations that it reaches up to a(*) less than or similar to 0.99. Consequently, one may conclude that the obtained new black hole solution can be considered as realistic candidate for the astrophysical black holes with a(*) less than or similar to 0.6.
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