SCHEE, Jan and Zdeněk STUCHLÍK. Gravitational lensing and ghost images in the regular Bardeen no-horizon spacetimes. Journal of Cosmology and Astroparticle Physics. GB - Spojené království Velké Británie a, 2015, No 6, p. "048-1"-"048-46", 46 pp. ISSN 1475-7516. Available from: https://dx.doi.org/10.1088/1475-7516/2015/06/048.
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Basic information
Original name Gravitational lensing and ghost images in the regular Bardeen no-horizon spacetimes
Authors SCHEE, Jan and Zdeněk STUCHLÍK.
Edition Journal of Cosmology and Astroparticle Physics, GB - Spojené království Velké Británie a, 2015, 1475-7516.
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/10.1088/1475-7516/2015/06/048
UT WoS 000359215400049
Keywords in English modified gravity; gravitational lensing; no-horizon spacetimes
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 11:15.
Abstract
We study deflection of light rays and gravitational lensing in the regular Bardeen no-horizon spacetimes. Flatness of these spacetimes in the central region implies existence of interesting optical effects related to photons crossing the gravitational field of the no-horizon spacetimes with low impact parameters. These effects occur due to existence of a critical impact parameter giving maximal deflection of light rays in the Bardeen no-horizon spacetimes. We give the critical impact parameter in dependence on the specific charge of the spacetimes, and discuss "ghost" direct and indirect images of Keplerian discs, generated by photons with low impact parameters. The ghost direct images can occur only for large inclination angles of distant observers, while ghost indirect images can occur also for small inclination angles. We determine the range of the frequency shift of photons generating the ghost images and determine distribution of the frequency shift across these images. We compare
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