BAKALA, Pavel, Alena BAKALOVA, Riccardo LA PLACA, Maurizio FALANGA and Luigi STELLA. Extreme amplification regimes of the Schwarzschild gravitational lens. ASTRONOMY & ASTROPHYSICS. LES ULIS CEDEX A: EDP SCIENCES S A, 2023, vol. 673, May 2023, p. "A164-1"-"A164-13", 13 pp. ISSN 0004-6361. Available from: https://dx.doi.org/10.1051/0004-6361/202245426.
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Basic information
Original name Extreme amplification regimes of the Schwarzschild gravitational lens
Authors BAKALA, Pavel (203 Czech Republic, belonging to the institution), Alena BAKALOVA, Riccardo LA PLACA, Maurizio FALANGA and Luigi STELLA.
Edition ASTRONOMY & ASTROPHYSICS, LES ULIS CEDEX A, EDP SCIENCES S A, 2023, 0004-6361.
Other information
Original language English
Type of outcome Article in a journal
Field of Study 10308 Astronomy
Country of publisher France
Confidentiality degree is not subject to a state or trade secret
WWW URL
RIV identification code RIV/47813059:19630/23:A0000322
Organization unit Institute of physics in Opava
Doi http://dx.doi.org/10.1051/0004-6361/202245426
UT WoS 001004184500016
Keywords in English gravitational lensing;strong;black hole physics;methods;analytical
Tags RIV24, UF
Tags International impact, Reviewed
Changed by Changed by: Mgr. Pavlína Jalůvková, učo 25213. Changed: 5/2/2024 08:35.
Abstract
We investigated a complete set of relativistic images of a small source located at an arbitrary distance from a Schwarzschild black hole gravitational lens. This paper offers a description of a simple and efficient fully relativistic method for calculating the bolometric intensity amplification. We focused our analysis primarily on sources located at small radii and close angular distance from the caustic line, both behind and in front of the compact lens. We term the corresponding large deflection regime 'extreme lensing'. We approximated the regime of fully-relativistic, extreme amplification of point sources by simple analytical formulae valid over a wide range of source distances. Using such approximations, we also derived formulae for the maximum amplification of extended sources close to or intercepted by the caustic line. Simple analytical approximations of the time delay between the brightest consecutive images in extreme amplification regimes are also presented.
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