Detailed Information on Publication Record
2007
Properties of pseudo-Newtonian gravitational potential in Schwarzschild-de Sitter spacetimes
KOVÁŘ, Jiří and Zdeněk STUCHLÍKBasic information
Original name
Properties of pseudo-Newtonian gravitational potential in Schwarzschild-de Sitter spacetimes
Authors
Edition
Opava, Proceedings of RAGtime 8/9: Workshops on black holes and neutron stars, p. 417-431, 14 pp. 2007
Publisher
Slezská univerzita v Opavě, Filozoficko-přírodovědecká fakulta, Ústav fyziky
Other information
Language
English
Type of outcome
Stať ve sborníku
Field of Study
10308 Astronomy
Confidentiality degree
není předmětem státního či obchodního tajemství
Organization unit
Faculty of Philosophy and Science in Opava
ISBN
978-80-7248-419-5
Keywords in English
Schwarzschild-de Sitter geometry, pseudo-Newtonian gravitational potential, cosmological constant, black hole
Tags
International impact
Links
GA202/06/0041, research and development project. MSM4781305903, plan (intention).
Změněno: 18/12/2020 11:28, Mgr. Pavlína Jalůvková
Abstract
V originále
We introduce the gravitational potential for the pseudo-Newtonian description of the gravitational field around static and spherically symmetric black holes in the universe with the repulsive cosmological constant, described in terms of the general relativistic approach by the Schwarzschild{de Sitter geometry. In order to demonstrate the accuracy of the pseudo-Newtonian approach and its possible applications, we construct the effective potential for a test particle motion and compare its behaviour withits general relativistic counterpart. Our results indicate that the pseudo-Newtonian potential could be useful in applications of developed Newtonian theories of accretion disks in astrophysically interesting situations in large galactic structures for spacetimes with the cosmological parameter y = Lambda*M^2/3 <= 10^-6.