STUCHLÍK, Zdeněk and Jaroslav VRBA. Epicyclic Oscillations around Simpson-Visser Regular Black Holes and Wormholes. Universe. Switzerland, 2021, vol. 7, No 8, p. "279-1"-"279-15", 15 pp. ISSN 2218-1997. Available from: https://dx.doi.org/10.3390/universe7080279.
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Basic information
Original name Epicyclic Oscillations around Simpson-Visser Regular Black Holes and Wormholes
Authors STUCHLÍK, Zdeněk (203 Czech Republic, belonging to the institution) and Jaroslav VRBA (203 Czech Republic, belonging to the institution).
Edition Universe, Switzerland, 2021, 2218-1997.
Other information
Original language English
Type of outcome Article in a journal
Field of Study 10308 Astronomy
Country of publisher Switzerland
Confidentiality degree is not subject to a state or trade secret
WWW URL
RIV identification code RIV/47813059:19630/21:A0000115
Organization unit Institute of physics in Opava
Doi http://dx.doi.org/10.3390/universe7080279
UT WoS 000690006700001
Keywords in English wormhole; quasi-periodic oscillation; supermassive quasars
Tags 2022, , GA19-03950S, RIV22
Tags International impact, Reviewed
Links GA19-03950S, research and development project.
Changed by Changed by: Mgr. Pavlína Jalůvková, učo 25213. Changed: 15/3/2022 12:25.
Abstract
We study epicyclic oscillatory motion along circular geodesics of the Simpson-Visser metageometry describing in a unique way regular black-bounce black holes and reflection-symmetric wormholes by using a length parameter l. We give the frequencies of the orbital and epicyclic motion in a Keplerian disc with inner edge at the innermost circular geodesic located above the black hole outer horizon or on the our side of the wormhole. We use these frequencies in the epicyclic resonance version of the so-called geodesic models of high-frequency quasi-periodic oscillations (HF QPOs) observed in microquasars and around supermassive black holes in active galactic nuclei to test the ability of this meta-geometry to improve the fitting of HF QPOs observational data from the surrounding of supermassive black holes. We demonstrate that this is really possible for wormholes with sufficiently high length parameter l.
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