KOVÁŘ, Jiří, Petr SLANÝ and Zdeněk STUCHLÍK. Pseudo-Newtonian and general relativistic barotropic tori in Schwarzschild-de Sitter spacetimes. Classical and Quantum Gravity. GB - Spojené království Velké Británie a, 2009, vol. 26, No 21, 35 pp. ISSN 0264-9381. Available from: https://dx.doi.org/10.1088/0264-9381/26/21/215013.
Other formats:   BibTeX LaTeX RIS
Basic information
Original name Pseudo-Newtonian and general relativistic barotropic tori in Schwarzschild-de Sitter spacetimes
Authors KOVÁŘ, Jiří, Petr SLANÝ and Zdeněk STUCHLÍK.
Edition Classical and Quantum Gravity, GB - Spojené království Velké Británie a, 2009, 0264-9381.
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
Organization unit Faculty of Philosophy and Science in Opava
Doi http://dx.doi.org/10.1088/0264-9381/26/21/215013
UT WoS 000270903900014
Keywords in English Cosmological constant, accretion tori, pseudonewtonian approach
Tags UF
Tags International impact, Reviewed
Links MSM4781305903, plan (intention).
Changed by Changed by: Mgr. Pavlína Jalůvková, učo 25213. Changed: 21/12/2020 14:57.
Abstract
Pseudo-Newtonian gravitational potential introduced in spherically symmetric black-hole spacetimes with a repulsive cosmological constant is tested for equilibrium toroidal configurations of barotropic perfect fluid orbiting the black holes. Shapes and potential depths are determined for the marginally stable barotropic tori with uniform distribution of specific angular momentum, using both the pseudo-Newtonian and fully relativistic approach. For the adiabatic (isoentropic) perfect fluid, temperature profiles, mass-density and pressure profiles and total masses of pseudo-Newtonian and relativistic tori are compared providing important information on the relevance of the test-disc approximation in both the approaches.
PrintDisplayed: 2/5/2024 19:08