SCHEE, Jan and Zdeněk STUCHLÍK. Optical effects related to Keplerian discs orbiting Kehagias-Sfetsos naked singularities. Classical and Quantum Gravity. GB - Spojené království Velké Británie a, 2014, vol. 31, No 19, p. "195013 - 1"-"195013 - 50", 50 pp. ISSN 0264-9381. Available from: https://dx.doi.org/10.1088/0264-9381/31/19/195013.
Other formats:   BibTeX LaTeX RIS
Basic information
Original name Optical effects related to Keplerian discs orbiting Kehagias-Sfetsos naked singularities
Authors SCHEE, Jan and Zdeněk STUCHLÍK.
Edition Classical and Quantum Gravity, GB - Spojené království Velké Británie a, 2014, 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
WWW www
Organization unit Faculty of Philosophy and Science in Opava
Doi http://dx.doi.org/10.1088/0264-9381/31/19/195013
UT WoS 000343411400013
Keywords in English Hořava gravity; optical phenomena; Keplerian disc
Tags UF
Tags International impact, Reviewed
Links GB14-37086G, research and development project.
Changed by Changed by: Mgr. Pavlína Jalůvková, učo 25213. Changed: 26/1/2021 15:24.
Abstract
We demonstrate possible optical signatures of the Kehagias-Sfetsos (KS) naked singularity spacetimes representing a spherically symmetric vacuum solution of the modified Horava gravity. In such spacetimes, accretion structures significantly different from those present in standard black hole spacetimes occur due to the 'antigravity' effect, which causes an internal static sphere surrounded by Keplerian discs. We focus our attention on the optical effects related to the Keplerian accretion discs, constructing the optical appearance of the Keplerian discs, the spectral continuum due to their thermal radiation, and the spectral profiled lines generated in the innermost parts of such discs. The KS naked singularity signature is strongly encoded in the characteristics of predicted optical effects, especially in cases where the spectral continuum and spectral lines are profiled by the strong gravity of the spacetimes due to the vanishing region of the angular velocity gradient influencing th
PrintDisplayed: 2/5/2024 07:32