Abstract
In this work, we have presented a detailed analysis of the event horizon of regular black holes (BHs) in modified gravity known as MOG, the so-called regular MOG BH. The motion of neutral particles around the BH has also been explored. The test particle motion study shows that the positive (negative) values of the MOG parameter mimic the spin of a rotating Kerr BH, providing the same values for the innermost stable pro-grade (retrograde) orbits of the particles in the range of the spin parameter a/M∈(−0.4125,0.6946). The efficiency of energy release from the accretion disk by the Novikov–Thorne model has been calculated, and the efficiency was shown to be linearly proportional to the increase of the MOG parameter α. Moreover, we have developed a new methodology to test gravity theories in strong-field regimes using precision data from twin-peaked quasiperiodic oscillations (QPOs) of objects calculating possible values of upper and lower frequencies. However, it is obtained that the positive MOG parameter can not mimic the spin of Kerr BHs in terms of the same QPO frequencies. We have provided possible ranges for upper and lower frequencies of twin-peak QPOs with the ratio of the upper and lower frequencies of 3:2 around regular MOG BHs in the different models. Moreover, as an example, we provide detailed numerical analysis of the QPO of GRS 1915+105 with the frequencies νU=168±5Hz and νL=113±3Hz. It is shown that the central BH of the QPO object can be a regular MOG BH when the value of the parameter is α=0.2844−0.1317+0.0074 and shines in the orbits located at the distance r/M=7.6322−0.0826+0.0768 from the central BH. It is also shown that the orbits where QPOs shine are located near the innermost stable circular orbit (ISCO) of the test particle. The correlation between the radii of ISCO and the QPO orbits is found, and it can be used as a new theoretical way to determine ISCO radius through observational data from the QPOs around various compact objects.
Highlights
The vicinity of the astrophysical BHS being a compact gravitating object may serve as a laboratory for testing the gravity theories in the strong-field regime
We provide the figure in order to see how the MOG parameter can mimic the spin parameter of rotating Kerr black holes (BHs) providing the same values to the innermost stable circular orbit (ISCO) radius
We have studied the properties of the spacetime and event horizon of regular BH in MOG gravity
Summary
The vicinity of the astrophysical BHS being a compact gravitating object may serve as a laboratory for testing the gravity theories in the strong-field regime. Electric and magnetic regular BH solutions obtained by coupling general relativity to nonlinear electrodynamics obeying the singularity problem and physical properties of the BHs such as thermodynamics, thermal stability and possible phase transition, QNMs and photon motions are studied in, e.g., refs. The role of the MOG field on plasma magnetospheric radiation from rotating magnetized relativistic stars and magnetized particles motion around gravitating compact objects have been discussed in refs. The Latin indices run from 1 to, 3 and the Greek ones from 0 to 3
Sign-in/Register to view highlights & summary Talk to us
Join us for a 30 min session where you can share your feedback and ask us any queries you have
Schedule a callDisclaimer: All third-party content on this website/platform is and will remain the property of their respective owners and is provided on "as is" basis without any warranties, express or implied. Use of third-party content does not indicate any affiliation, sponsorship with or endorsement by them. Any references to third-party content is to identify the corresponding services and shall be considered fair use under The CopyrightLaw.
