SLANÝ, Petr and Zdeněk STUCHLÍK. Perfect fluid tori in the Kerr-de Sitter naked singularity backgrounds. 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. 167-187, 20 pp. ISBN 80-7248-334-X.
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Basic information
Original name Perfect fluid tori in the Kerr-de Sitter naked singularity backgrounds
Authors SLANÝ, Petr and Zdeněk STUCHLÍK.
Edition Opava, Proceedings of RAGtime 6/7: Workshops on black holes and neutron stars, p. 167-187, 20 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
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 perfect fluid, Kerr-de Sitter geometry, naked singularity, cosmological constant, accretion, excretion
Tags RAGtime, sbornik, UF
Tags International impact
Links MSM4781305903, plan (intention).
Changed by Changed by: Mgr. Pavlína Jalůvková, učo 25213. Changed: 18/12/2020 10:07.
Abstract
Perfect fluid tori with uniform distribution of the specific angular momentum, $ell(r,theta)=mathrm{const}$, orbiting the Kerr--de~Sitter naked singularities are discussed. Closed equipotential surfaces corresponding to stationary thick discs are allowed only in the spacetimes admitting stable circular geodesics. The last closed surface crosses itself in the cusp(s) enabling outflows of matter from the torus due to the violation of hydrostatic equilibrium. The inner cusp enables the accretion onto the ring singularity. Influence of the repulsive cosmological constant, $Lambda >0$, resides in the existence of the outer cusp enabling the emph{excretion} (outflow of matter from the torus into the outer space) and gives rise to completely new type ofa disc called the emph{excretion disc}. The plus-family accretion and excretion discs can be both the corotating or counterrotating discs, the minus-family ones are always the counterrotating discs, as related to locally non-rotating fra
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