HENSH, Sudipta, Jan SCHEE, Ahmadjon ABDUJABBAROV and Zdeněk STUCHLÍK. Strong gravitational lensing around Kehagias-Sfetsos compact objects surrounded by plasma. European Physical Journal Plus. DE - Spolková republika Německo, 2022, vol. 137, No 2, p. "242-1"-"242-9", 9 pp. ISSN 2190-5444. Available from: https://dx.doi.org/10.1140/epjp/s13360-022-02454-8.
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Basic information
Original name Strong gravitational lensing around Kehagias-Sfetsos compact objects surrounded by plasma
Authors HENSH, Sudipta (356 India, belonging to the institution), Jan SCHEE (203 Czech Republic, belonging to the institution), Ahmadjon ABDUJABBAROV and Zdeněk STUCHLÍK (203 Czech Republic, belonging to the institution).
Edition European Physical Journal Plus, DE - Spolková republika Německo, 2022, 2190-5444.
Other information
Original language English
Type of outcome Article in a journal
Field of Study 10308 Astronomy
Country of publisher Germany
Confidentiality degree is not subject to a state or trade secret
WWW URL
RIV identification code RIV/47813059:19630/22:A0000188
Organization unit Institute of physics in Opava
Doi http://dx.doi.org/10.1140/epjp/s13360-022-02454-8
UT WoS 000757841600002
Keywords in English Horava gravity;Kehagias-Sfetsos black holes;semi-analytical Bozza method
Tags , RIV23, SGS-12-2019
Tags International impact, Reviewed
Links GA19-03950S, research and development project.
Changed by Changed by: Mgr. Pavlína Jalůvková, učo 25213. Changed: 1/2/2023 11:46.
Abstract
We present the analysis how Horava gravity and plasma influence the strong lensing phenomena around Kehagias-Sfetsos (KS) black holes. Using the semi-analytical Bozza method of strong lensing limit, we determine the multiple images, namely their separation S, and magnification R. We apply our calculations to the case of supermassive black hole having mass M = 6.5x10(9)M(circle dot) and being at distance d(0) = 16.8Mpc from observer corresponding to those observed in M87. We show that the sensitivity of image magnification, image separation, and shadow angular size on KS parameter omega and plasma parameter k are of order from 1 to 10% for R and 16% for S.
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