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Equatorial and Polar Quasinormal Modes and Quasiperiodic Oscillations of Quantum Deformed Kerr Black Hole

Kimet JusufiPhysics Department, State University of Tetovo, Ilinden Street nn, 1200 Tetovo, North MacedoniaMustapha Azreg‐AïnouEngineering Faculty, Bağlıca Campus, Başkent University, Ankara 06790, TurkeyMubasher JamilInstitute for Theoretical Physics and Cosmology, Zhejiang University of Technology, Hangzhou 310023, ChinaQiang WuInstitute for Theoretical Physics and Cosmology, Zhejiang University of Technology, Hangzhou 310023, China

2022en

ABI

Annotatsiya

In this paper, we focus on the relation between quasinormal modes (QNMs) and a rotating black hole shadow. As a specific example, we consider the quantum deformed Kerr black hole obtained via Newman–Janis–Azreg-Aïnou algorithm. In particular, using the geometric-optics correspondence between the parameters of a QNMs and the conserved quantities along geodesics, we show that, in the eikonal limit, the real part of QNMs is related to the Keplerian frequency for equatorial orbits. To this end, we explore the typical shadow radius for the viewing angles, θ0=π/2, and obtained an interesting relation in the case of viewing angle θ0=0 (or equivalently θ0=π). Furthermore we have computed the corresponding equatorial and polar modes and the thermodynamical stability of the quantum deformed Kerr black hole. We also investigate other astrophysical applications such as the quasiperiodic oscillations and the motion of S2 star to constrain the quantum deforming parameter.

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Identifikatorlar

DOI: 10.3390/universe8040210

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