J 2021

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

TURIMOV, Bobur, Bobomurat AHMEDOV a Zdeněk STUCHLÍK

Základní údaje

Originální název

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

Autoři

TURIMOV, Bobur (860 Uzbekistán, domácí), Bobomurat AHMEDOV (860 Uzbekistán) a Zdeněk STUCHLÍK (203 Česká republika, domácí)

Vydání

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

Další údaje

Jazyk

angličtina

Typ výsledku

Článek v odborném periodiku

Obor

10308 Astronomy

Stát vydavatele

Nizozemské království

Utajení

není předmětem státního či obchodního tajemství

Odkazy

URL

Kód RIV

RIV/47813059:19630/21:A0000141

Organizační jednotka

Fyzikální ústav v Opavě

DOI

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

UT WoS

000704383100031

Klíčová slova anglicky

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

Štítky

2022, , RIV22, SGS-12-2019

Příznaky

Mezinárodní význam, Recenzováno
Změněno: 28. 3. 2022 11:33, Mgr. Pavlína Jalůvková

Anotace

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.
Zobrazeno: 16. 11. 2024 03:50