STUCHLÍK, Zdeněk, Daniel CHARBULÁK and Jan SCHEE. Light escape cones in local reference frames of Kerr-de Sitter black hole spacetimes and related black hole shadows. European Physical Journal C. 2018, vol. 78, No 3, p. "180-1"-"180-32", 32 pp. ISSN 1434-6044. Available from: https://dx.doi.org/10.1140/epjc/s10052-018-5578-6.
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Basic information
Original name Light escape cones in local reference frames of Kerr-de Sitter black hole spacetimes and related black hole shadows
Authors STUCHLÍK, Zdeněk (203 Czech Republic, guarantor, belonging to the institution), Daniel CHARBULÁK (203 Czech Republic, belonging to the institution) and Jan SCHEE (203 Czech Republic, belonging to the institution).
Edition European Physical Journal C, 2018, 1434-6044.
Other information
Original language English
Type of outcome Article in a journal
Field of Study 10308 Astronomy
Country of publisher United States of America
Confidentiality degree is not subject to a state or trade secret
WWW URL
RIV identification code RIV/47813059:19240/18:A0000269
Organization unit Faculty of Philosophy and Science in Opava
Doi http://dx.doi.org/10.1140/epjc/s10052-018-5578-6
UT WoS 000426838900004
Keywords in English Kerr-de Sitter black holes; light escape cones; black hole shadows
Tags International impact, Reviewed
Links GB14-37086G, research and development project.
Changed by Changed by: RNDr. Jan Hladík, Ph.D., učo 25379. Changed: 4/4/2019 10:49.
Abstract
We construct the light escape cones of isotropic spot sources of radiation residing in special classes of reference frames in the Kerr-de Sitter (KdS) black hole space-times, namely in the fundamental class of 'non-geodesic' locally non-rotating reference frames (LNRFs), and two classes of 'geodesic' frames, the radial geodesic frames (RGFs), both falling and escaping, and the frames related to the circular geodesic orbits (CGFs). We compare the cones constructed in a given position for the LNRFs, RGFs, and CGFs. We have shown that the photons locally counter-rotating relative to LNRFs with positive impact parameter and negative covariant energy are confined to the ergosphere region. Finally, we demonstrate that the light escaping cones govern the shadows of black holes located in front of a radiating screen, as seen by the observers in the considered frames. For shadows related to distant static observers the LNRFs are relevant.
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