STUCHLÍK, Zdeněk. Influence of the relict cosmological constant on accretion discs. Modern Physics Letters A. US - Spojené státy americké, 2005, vol. 20, No 8, p. 561-575, 14 pp. ISSN 0217-7323. Available from: https://dx.doi.org/10.1142/S0217732305016865.
Other formats:   BibTeX LaTeX RIS
Basic information
Original name Influence of the relict cosmological constant on accretion discs
Authors STUCHLÍK, Zdeněk.
Edition Modern Physics Letters A, US - Spojené státy americké, 2005, 0217-7323.
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/10.1142/S0217732305016865
UT WoS 000228162800001
Keywords in English Accretion, accretion discs, black-hole physics, relativity, cosmological constant, jets, radii
Tags UF
Tags International impact, Reviewed
Links MSM4781305903, plan (intention).
Changed by Changed by: Mgr. Pavlína Jalůvková, učo 25213. Changed: 18/12/2020 10:18.
Abstract
Surprisingly, the relict cosmological constant has a crucial influence on properties of accretion discs orbiting black holes in quasars and active galactic nuclei. We show it by considering basic properties of both the geometrically thin and thick accretion discs in the Kerr - de Sitter black-hole (naked-singularity) spacetimes. Both thin and thick discs must have an outer edge allowing out ow of matter into the outer space, located nearby the so called static radius, where the gravitational attractionof a black hole is balanced by the cosmological repulsion. Jets produced by thick discs can be significantly collimated after crossing the static radius. Extension of discs in quasars is comparable with extension of the associated galaxies, indicating apossibility that the relict cosmological constant puts an upper limit on extension of galaxies.
PrintDisplayed: 7/5/2024 03:02