SCHEE, Jan and Zdeněk STUCHLÍK. Counter-rotating Keplerian discs around Kerr superspinars. Classical and Quantum Gravity. GB - Spojené království Velké Británie a, 2012, vol. 29, No 2, 22 pp. ISSN 0264-9381. Available from: https://dx.doi.org/10.1088/0264-9381/29/2/025008.
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Basic information
Original name Counter-rotating Keplerian discs around Kerr superspinars
Authors SCHEE, Jan and Zdeněk STUCHLÍK.
Edition Classical and Quantum Gravity, GB - Spojené království Velké Británie a, 2012, 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/10.1088/0264-9381/29/2/025008
UT WoS 000298676600008
Keywords in English Black-hole spin; Naked-singularity; Gravitational collapse
Tags UF
Tags International impact, Reviewed
Links GA202/09/0772, research and development project. LC06014, research and development project. MSM4781305903, plan (intention).
Changed by Changed by: Mgr. Pavlína Jalůvková, učo 25213. Changed: 14/1/2021 10:41.
Abstract
The appearance of corotating Keplerian discs orbiting Kerr superspinars has been shown to be strongly dependent on the value of the superspinar spin in both their shape and frequency shift profile, demonstrating clear distinctions from the corotating discs around black holes. However, it has to be modified in the innermost parts of the disc by the self-illumination effect caused by the photons trapped in the strong gravitational field near the superspinars with spin a < 9. Here we demonstrate that self-illumination is irrelevant for counter-rotating Keplerian discs orbiting in the field of all Kerr superspinars since such discs are located at the regions where none of the radiated photons can be trapped. Therefore, the results obtained by considering the escaping photons only are quite relevant for the appearance of the counter-rotating Keplerian discs orbiting Kerr superspinars. The appearance and spectral continuum of such discs differ from those of counter-rotating discs in the fiel
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