SHAHZADI, Misbah, Martin KOLOŠ, Zdeněk STUCHLÍK and Yousaf HABIB. Testing alternative theories of gravity by fitting the hot-spot data of Sgr A*. European Physical Journal C. New York (USA): SPRINGER, 2022, vol. 82, No 5, p. "407-1"-"407-22", 22 pp. ISSN 1434-6044. Available from: https://dx.doi.org/10.1140/epjc/s10052-022-10347-4.
Other formats:   BibTeX LaTeX RIS
Basic information
Original name Testing alternative theories of gravity by fitting the hot-spot data of Sgr A*
Authors SHAHZADI, Misbah, Martin KOLOŠ (203 Czech Republic, belonging to the institution), Zdeněk STUCHLÍK (203 Czech Republic, belonging to the institution) and Yousaf HABIB.
Edition European Physical Journal C, New York (USA), SPRINGER, 2022, 1434-6044.
Other information
Original language English
Type of outcome Article in a journal
Field of Study 10308 Astronomy
Country of publisher United States of America
Confidentiality degree is not subject to a state or trade secret
WWW URL
RIV identification code RIV/47813059:19630/22:A0000186
Organization unit Institute of physics in Opava
Doi http://dx.doi.org/10.1140/epjc/s10052-022-10347-4
UT WoS 000791400300002
Keywords in English Sagittarius A* ;Sgr A*;Kerr black hole;nonlinear electrodynamics;general relativity;dark matter
Tags , RIV23
Tags International impact, Reviewed
Links GA19-03950S, research and development project.
Changed by Changed by: Mgr. Pavlína Jalůvková, učo 25213. Changed: 31/1/2023 12:07.
Abstract
We are fitting dynamics of electrically neutral hot-spot orbiting around Sagittarius A* (Sgr A*) source in Galactic center, represented by various modifications of the standard Kerr black hole (BH), to the three flares observed by the GRAVITY instrument on May 27, July 22, July 28, 2018. We consider stationary, axisymmetric, and asymptotically flat spacetimes describing charged BHs in general relativity (GR) combined with nonlinear electrodynamics, or reflecting the influence of dark matter (DM), or in so called parameterized dirty Kerr spacetimes, and test them using the hot-spot data. We show that the orbital frequencies as well as positions of the hot-spots orbiting the considered BHs fit the observed positions and periods of the flare orbits, and give relevant constraints on the parameters of the considered BH spacetimes and the gravity or other theories behind such modified spacetimes.
PrintDisplayed: 17/5/2024 19:30