CHARBULÁK, Daniel and Zdeněk STUCHLÍK. Spherical photon orbits in the field of Kerr naked singularities. European Physical Journal C. 2018, vol. 78, No 11, p. "879-1"-"879-25", 25 pp. ISSN 1434-6044. Available from: https://dx.doi.org/10.1140/epjc/s10052-018-6336-5.
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Basic information
Original name Spherical photon orbits in the field of Kerr naked singularities
Authors CHARBULÁK, Daniel (203 Czech Republic, belonging to the institution) and Zdeněk STUCHLÍK (203 Czech Republic, guarantor, 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:A0000245
Organization Filozoficko-přírodovědecká fakulta – Slezská univerzita v Opavě – Repository
Doi http://dx.doi.org/10.1140/epjc/s10052-018-6336-5
UT WoS 000448860000004
Keywords in English Kerr naked singularity; photon orbits; stable circular geodesics
Tags CTP, GJ16-03564Y, ÚF
Tags International impact, Reviewed
Links GJ16-03564Y, research and development project.
Changed by Changed by: Jan Hladík, učo 1305. Changed: 5/4/2019 02:03.
Abstract
For the Kerr naked singularity (KNS) spacetimes, we study properties of spherical photon orbits (SPOs) confined to constant Boyer-Lindquist radius r. Some new features of the SPOs are found, having no counterparts in the Kerr black hole (KBH) spacetimes, especially stable orbits that could be pure prograde/retrograde, or with turning point in the azimuthal direction. At r > 1 (r < 1) the covariant photon energy E > 0 (E < 0), at r = 1 there is E = 0. All unstable orbits must have E > 0. It is shown that the polar SPOs can exist only in the spacetimes with dimensionless spin a < 1.7996. Existence of closed SPOs with vanishing total change of the azimuth is demonstrated. Classification of the KNS and KBH spacetimes in dependence on their dimensionless spin a is proposed, considering the properties of the SPOs. For selected types of the KNS spacetimes, typical SPOs are constructed, including the closed paths. It is shown that the stable SPOs intersect the equatorial plane in a region of stable circular orbits of test particles, depending on the spin a. Relevance of this intersection for the Keplerian accretion discs is outlined and observational effects are estimated.
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