PETRÁSEK, Martin, Jiří KOVÁŘ and Zdeněk STUCHLÍK. Stationary observers in Kerr-de Sitter spacetimes. International Journal of Modern Physics D. SG - Singapurská republika, 2023, vol. 32, No 12, p. "2350084-1"-"2350084-18", 18 pp. ISSN 0218-2718. Available from: https://dx.doi.org/10.1142/S0218271823500840.
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Basic information
Original name Stationary observers in Kerr-de Sitter spacetimes
Authors PETRÁSEK, Martin (203 Czech Republic, belonging to the institution), Jiří KOVÁŘ (203 Czech Republic, belonging to the institution) and Zdeněk STUCHLÍK (203 Czech Republic, belonging to the institution).
Edition International Journal of Modern Physics D, SG - Singapurská republika, 2023, 0218-2718.
Other information
Original language English
Type of outcome Article in a journal
Field of Study 10308 Astronomy
Country of publisher Singapore
Confidentiality degree is not subject to a state or trade secret
WWW URL
RIV identification code RIV/47813059:19630/23:A0000279
Organization unit Institute of physics in Opava
Doi http://dx.doi.org/10.1142/S0218271823500840
UT WoS 001077432500001
Keywords in English Stationary observerKerr-de Sitter spacetime;orbital velocity;inertial force;black hole;naked singularity
Tags RIV24, UF
Tags International impact, Reviewed
Changed by Changed by: Mgr. Pavlína Jalůvková, učo 25213. Changed: 12/2/2024 09:58.
Abstract
In this paper, we present a study of basic classes of stationary observers orbiting in stationary and axially symmetric Kerr-de Sitter spacetimes. Along with proper definitions of these classes, we focus on their possible matching on particular circular orbits. Especially, we determine a number of such orbits in a given spacetime characterized by its rotational and cosmological parameters that leads to a comprehensive classification of the Kerr-de Sitter spacetimes. Studied profiles of orbital velocities of the observers and of forces keeping them on their orbits directly reflect complex structure of the Kerr-de Sitter spacetimes that is caused by a unique interplay of attraction and rotation of a central object and an ambient cosmic repulsion.
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