Strong gravitational lensing around Kehagias-Sfetsos compact objects surrounded by plasma

Fuente: arXiv
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Hauptverfasser: Hensh, Sudipta, Schee, Jan, Abdujabbarov, Ahmadjon, Stuchlík, Zdeněk
Format: Preprint
Veröffentlicht: 2021
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author Hensh, Sudipta
Schee, Jan
Abdujabbarov, Ahmadjon
Stuchlík, Zdeněk
author_facet Hensh, Sudipta
Schee, Jan
Abdujabbarov, Ahmadjon
Stuchlík, Zdeněk
contents We present the analysis how Hořava 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 $M=6.5\times 10^{9}\textrm{M}_\odot$ and being at distance $d_0=16.8\textrm{Mpc}$ 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 $ω$ and plasma parameter $k$ are of order from $1\%$ to $10\%$ for $R$ and $~\,16\%$ for $S$.
format Preprint
id arxiv_https___arxiv_org_abs_2110_13600
institution arXiv
publishDate 2021
record_format arxiv
spellingShingle Strong gravitational lensing around Kehagias-Sfetsos compact objects surrounded by plasma
Hensh, Sudipta
Schee, Jan
Abdujabbarov, Ahmadjon
Stuchlík, Zdeněk
General Relativity and Quantum Cosmology
We present the analysis how Hořava 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 $M=6.5\times 10^{9}\textrm{M}_\odot$ and being at distance $d_0=16.8\textrm{Mpc}$ 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 $ω$ and plasma parameter $k$ are of order from $1\%$ to $10\%$ for $R$ and $~\,16\%$ for $S$.
title Strong gravitational lensing around Kehagias-Sfetsos compact objects surrounded by plasma
topic General Relativity and Quantum Cosmology
url https://arxiv.org/abs/2110.13600