SCHEE, Jan and Zdeněk STUCHLÍK. Circular geodesic of Bardeen and Ayon-Beato-Garcia regular black-hole and no-horizon spacetimes. International Journal of Modern Physics D. SG - Singapurská republika, 2015, vol. 24, No 2, p. "1550020-1"-"1550020-31", 31 pp. ISSN 0218-2718. Available from: https://dx.doi.org/10.1142/S0218271815500200.
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Basic information
Original name Circular geodesic of Bardeen and Ayon-Beato-Garcia regular black-hole and no-horizon spacetimes
Authors SCHEE, Jan and Zdeněk STUCHLÍK.
Edition International Journal of Modern Physics D, SG - Singapurská republika, 2015, 0218-2718.
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/10.1142/S0218271815500200
UT WoS 000349637600012
Keywords in English regular spacetimes; circular geodesics; profiled lines
Tags UF
Tags International impact, Reviewed
Links GB14-37086G, research and development project.
Changed by Changed by: Mgr. Pavlína Jalůvková, učo 25213. Changed: 27/1/2021 11:46.
Abstract
In this paper, we study circular geodesic motion of test particles and photons in the Bardeen and Ayon-Beato-Garcia (ABG) geometry describing spherically symmetric regular black-hole or no-horizon spacetimes. While the Bardeen geometry is not exact solution of Einstein's equations, the ABG spacetime is related to self-gravitating charged sources governed by Einstein's gravity and nonlinear electrodynamics. They both are characterized by the mass parameter m and the charge parameter g. We demonstrate that in similarity to the Reissner-Nordstrom (RN) naked singularity spacetimes an anti-gravity static sphere should exist in all the no-horizon Bardeen and ABG solutions that can be surrounded by a Keplerian accretion disc. However, contrary to the RN nakedsingularity spacetimes, the ABG no-horizon spacetimes with parameter g/m > 2 can contain also an additional inner Keplerian disc hidden under the static anti-gravity sphere. Properties of the geodesic structure are reflected by simple ob
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