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Strong gravitational lensing by Kiselev black hole

Younas, A; Jamil, M; Bahamonde, S; Hussain, S; (2015) Strong gravitational lensing by Kiselev black hole. Physical Review D , 92 (8) , Article 084042. 10.1103/PhysRevD.92.084042. Green open access

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Abstract

We investigate the gravitational lensing scenario due to Schwarzschild-like black hole surrounded by quintessence (Kiselev black hole). We work for the special case of Kiselev black hole where we take the state parameter w q = − 2 3 . For the detailed derivation and analysis of the bending angle involved in the deflection of light, we discuss three special cases of Kiselev black hole: nonextreme, extreme, and naked singularity. We also calculate the approximate bending angle and compare it with the exact bending angle. We found the relation of bending angles in the decreasing order as: naked singularity, extreme Kiselev black hole, nonextreme Kiselev black hole, and Schwarzschild black hole. In the weak field approximation, we compute the position and total magnification of relativistic images as well.

Type: Article
Title: Strong gravitational lensing by Kiselev black hole
Open access status: An open access version is available from UCL Discovery
DOI: 10.1103/PhysRevD.92.084042
Publisher version: http://doi.org/10.1103/PhysRevD.92.084042
Language: English
Additional information: © 2015 American Physical Society
Keywords: Science & Technology, Physical Sciences, Astronomy & Astrophysics, Physics, Particles & Fields, Physics, COSMOLOGICAL CONSTANT, DARK ENERGY, LIGHT, FIELD, QUINTESSENCE, SUPERNOVAE, GRAVITY, LENSES, LIMIT
UCL classification: UCL
UCL > Provost and Vice Provost Offices > UCL BEAMS
UCL > Provost and Vice Provost Offices > UCL BEAMS > Faculty of Maths and Physical Sciences
URI: https://discovery.ucl.ac.uk/id/eprint/1520919
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