KOLOŠ, Martin, Misbah SHAHZADI and Zdeněk STUCHLÍK. Quasi-periodic oscillations around Kerr-MOG black holes. European Physical Journal C. 2020, vol. 80, No 2, p. "133-1"-"133-12", 12 pp. ISSN 1434-6044. Available from: https://dx.doi.org/10.1140/epjc/s10052-020-7692-5.
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Basic information
Original name Quasi-periodic oscillations around Kerr-MOG black holes
Authors KOLOŠ, Martin (203 Czech Republic, belonging to the institution), Misbah SHAHZADI and Zdeněk STUCHLÍK (203 Czech Republic, belonging to the institution).
Edition European Physical Journal C, 2020, 1434-6044.
Other information
Original language English
Type of outcome Article in a journal
Field of Study 10303 Particles and field physics
Country of publisher United States of America
Confidentiality degree is not subject to a state or trade secret
WWW URL
RIV identification code RIV/47813059:19630/20:A0000035
Organization unit Institute of physics in Opava
Doi http://dx.doi.org/10.1140/epjc/s10052-020-7692-5
UT WoS 000517130800001
Keywords in English X-RAY BINARIES; MASS; QPOS; MODEL; FIELD; RADIATION; MOTION; SPIN
Tags , FÚ2020, GA19-03950S, GB14-37086G, RIV21
Tags International impact, Reviewed
Links GA19-03950S, research and development project. GB14-37086G, research and development project.
Changed by Changed by: Mgr. Pavlína Jalůvková, učo 25213. Changed: 23/3/2021 22:03.
Abstract
The study of the quasi-periodic oscillations (QPOs) of X-ray flux observed in the stellar-mass black hole (BH) binaries can provide a powerful tool for testing the phenomena occurring in strong gravity regime. We thus present and apply to three known microquasars the model of epicyclic oscillations of Keplerian discs orbiting rotating BHs governed by the modified theory of gravity (MOG). We show that the standard geodesic models of QPOs can explain the observationally fixed data from the three microquasars, GRO 1655-40, XTE 1550-564, and GRS 1915+105. We perform a successful fitting of the high frequency (HF) QPOs observed in these microquasars, under assumption of MOG BHs, for epicyclic resonance and its variants, relativistic precession and its variants, tidal disruption, as well as warped disc models and discuss the corresponding constraints of parameters of the model, which are the mass and spin and parameter alpha of the BH.
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