KUČÁKOVÁ, Hana, Daniela PUGLIESE, Jan SCHEE and Zdeněk STUCHLÍK. Perfect fluid tori orbiting Kehagias-Sfetsos naked singularities. The European Physical Journal C. US - Spojené státy americké, 2015, vol. 75, No 9, p. "451-1"-"451-31", 31 pp. ISSN 1434-6044. Available from: https://dx.doi.org/10.1140/epjc/s10052-015-3663-7.
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Basic information
Original name Perfect fluid tori orbiting Kehagias-Sfetsos naked singularities
Authors KUČÁKOVÁ, Hana, Daniela PUGLIESE, Jan SCHEE and Zdeněk STUCHLÍK.
Edition The European Physical Journal C, US - Spojené státy americké, 2015, 1434-6044.
Other information
Original language English
Type of outcome Article in a journal
Field of Study 10308 Astronomy
Confidentiality degree is not subject to a state or trade secret
WWW www
Organization unit Faculty of Philosophy and Science in Opava
Doi http://dx.doi.org/10.1140/epjc/s10052-015-3663-7
UT WoS 000361822200004
Keywords in English naked singularity; accretion; perfect fluid tori
Tags UF
Tags International impact, Reviewed
Links GB14-37086G, research and development project.
Changed by Changed by: Mgr. Pavlína Jalůvková, učo 25213. Changed: 27/1/2021 10:29.
Abstract
We construct perfect fluid tori in the field of the Kehagias-Sfetsos (K-S) naked singularities. These are spherically symmetric vacuum solutions of the modified Horava quantum gravity, characterized by a dimensionless parameter omega M^2, combining the gravitational mass parameter M of the spacetime with the Horava parameter., reflecting the role of the quantum corrections. In dependence on the value of omega M^2, the K-S naked singularities demonstrate a variety of qualitatively different behavior of their circular geodesics that is fully reflected in the properties of the toroidal structures, demonstrating clear distinction to the properties of the torii in the Schwarzschild spacetimes. In all of the K-S naked singularity spacetimes the tori are located above an "antigravity" sphere where matter can stay in a stable equilibrium position, which is relevant for the stability of the orbiting fluid toroidal accretion structures. The signature of the K-S naked singularity is given by the
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