STUCHLÍK, Zdeněk and Gabriel TÖRÖK. Epicyclic frequencies of Keplerian motion in Kerr spacetimes. In Proceedings of RAGtime 6/7: Workshops on black holes and neutron stars. Opava: Slezská univerzita v Opavě, Filozoficko-přírodovědecká fakulta, Ústav fyziky, 2005, p. 315-336, 21 pp. ISBN 80-7248-334-X.
Other formats:   BibTeX LaTeX RIS
Basic information
Original name Epicyclic frequencies of Keplerian motion in Kerr spacetimes
Authors STUCHLÍK, Zdeněk and Gabriel TÖRÖK.
Edition Opava, Proceedings of RAGtime 6/7: Workshops on black holes and neutron stars, p. 315-336, 21 pp. 2005.
Publisher Slezská univerzita v Opavě, Filozoficko-přírodovědecká fakulta, Ústav fyziky
Other information
Original language English
Type of outcome Proceedings paper
Field of Study 10308 Astronomy
Country of publisher Czech Republic
Confidentiality degree is not subject to a state or trade secret
Organization unit Faculty of Philosophy and Science in Opava
ISBN 80-7248-334-X
Keywords in English black hole, naked singularities, theory, observations, X-ray variability
Tags , MSM4781305903, RAGtime, sbornik
Tags International impact
Links MSM4781305903, plan (intention).
Changed by Changed by: Mgr. Pavlína Jalůvková, učo 25213. Changed: 3/12/2020 10:02.
Abstract
Relativistic Keplerian orbital frequency and the related epicyclic frequencies play an important role in the physics of accretion discs orbiting Kerr black holes. We examine in detail their properties in Kerr spacetimes and discuss some possible observational implications resulting from their behaviour in the black hole case. Characteristics of the fundamental orbital frequencies of Keplerian motion are also analysed with the intention to find the phenomena which could observationally distinguisha hypothetical naked singularity from black holes. We explore the significant differences in behaviour of the epicyclic frequencies. These suggest that oscillations of discs orbiting Kerr black holes and naked singularities could be very different, and the information, given through X-ray variability of the source, could distinguish between the naked singularities and the black holes in general.
PrintDisplayed: 28/4/2024 12:50