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

Author:

Rayimbaev Javlon1234ORCID,Juraeva Nozima56,Khudoyberdiyeva Malika45,Abdujabbarov Ahmadjon57ORCID,Abdullaev Mardon8

Affiliation:

1. School of Mathematics and Natural Sciences, New Uzbekistan University, Mustaqillik Ave. 54, Tashkent 100007, Uzbekistan

2. School of Engineering, Central Asian University, Tashkent 111221, Uzbekistan

3. Institute of Fundamental and Applied Research, TIIAME National Research University, Kori Niyoziy 39, Tashkent 100000, Uzbekistan

4. Faculty of Physics, National University of Uzbekistan, Tashkent 100174, Uzbekistan

5. Ulugh Beg Astronomical Institute, Astronomy Str. 33, Tashkent 100052, Uzbekistan

6. Institute of Nuclear Physics, Ulugbek 1, Tashkent 100214, Uzbekistan

7. Faculty of Computer Engineering, Tashkent University of Applied Sciences, Gavhar Str. 1, Tashkent 100149, Uzbekistan

8. Power Engineering Faculty, Tashkent State Technical University, Tashkent 100095, Uzbekistan

Abstract

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.

Funder

Ministry of Higher Education, Science, and Innovation of the Republic of Uzbekistan

Publisher

MDPI AG

Subject

Astronomy and Astrophysics

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