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Quasiperiodic Oscillations and Dynamics of Test Particles around Regular-Kiselev Black Holes

Javlon RayimbaevFaculty of Physics, National University of Uzbekistan, Tashkent 100174, UzbekistanNozima JuraevaInstitute of Nuclear Physics, Ulugbek 1, Tashkent 100214, UzbekistanMalika KhudoyberdiyevaFaculty of Physics, National University of Uzbekistan, Tashkent 100174, UzbekistanAhmadjon AbdujabbarovFaculty of Computer Engineering, Tashkent University of Applied Sciences, Gavhar Str. 1, Tashkent 100149, UzbekistanMardon AbdullaevPower Engineering Faculty, Tashkent State Technical University, Tashkent 100095, Uzbekistan
Galaxiesjournal2023en
ABI

Аннотация

Testing gravity theories combining (massive and massless) scalar & electrodynamic fields become the most important issue in relativistic astrophysics using data from, black hole observations. In the present work, we first show a spherically symmetric black hole solution in general relativity coupling to generic-type nonlinear electrodynamics (NED) together with the quintessential field. We also obtain possible values for the parameters of the quintessential field and NED charge in the black hole environment for different values of degree of nonlinearity. Also, event horizon properties and scalar invariants of the black hole spacetime are studied. We investigate the equatorial motion of test particles around the regular-Kiselev black holes and study the combined effects of quintessential field and the NED charge of the black hole on particle angular momentum together with its energy at their circular orbits as well as their innermost circular stable orbits (ISCOs) and compared the obtained results with Reissner-Nordström black hole (RN BH) case. Moreover, we study particle oscillations along the orbits above than ISCO and applications to quasiperiodic oscillations (QPOs) where we obtain constrain values for the quintessential parameter and black hole mass charge parameters using observational QPO data from microquasars.

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