Motion of particles and gravitational lensing around the (2+1)-dimensional BTZ black hole in Gauss–Bonnet gravity

Abstract We study the motion of test particles and photons in the vicinity of the (2+1)-dimensional Gauss–Bonnet (GB) BTZ black hole. We find that the presence of the coupling constant serves as an attractive gravitational charge, shifting the innermost stable circular orbits outward with respect to...

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Main Authors: Bakhtiyor Narzilloev, Sanjar Shaymatov, Ibrar Hussain, Ahmadjon Abdujabbarov, Bobomurat Ahmedov, Cosimo Bambi
Format: Article
Language:English
Published: SpringerOpen 2021-09-01
Series:European Physical Journal C: Particles and Fields
Online Access:https://doi.org/10.1140/epjc/s10052-021-09617-4
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spelling doaj-2d64dab564a84d368e56db5dd5a784b72021-09-26T11:16:31ZengSpringerOpenEuropean Physical Journal C: Particles and Fields1434-60441434-60522021-09-0181911010.1140/epjc/s10052-021-09617-4Motion of particles and gravitational lensing around the (2+1)-dimensional BTZ black hole in Gauss–Bonnet gravityBakhtiyor Narzilloev0Sanjar Shaymatov1Ibrar Hussain2Ahmadjon Abdujabbarov3Bobomurat Ahmedov4Cosimo Bambi5Department of Physics, Center for Field Theory and Particle Physics, Fudan UniversityAkfa UniversitySchool of Electrical Engineering and Computer Science, National University of Sciences and TechnologyUlugh Beg Astronomical InstituteUlugh Beg Astronomical InstituteDepartment of Physics, Center for Field Theory and Particle Physics, Fudan UniversityAbstract We study the motion of test particles and photons in the vicinity of the (2+1)-dimensional Gauss–Bonnet (GB) BTZ black hole. We find that the presence of the coupling constant serves as an attractive gravitational charge, shifting the innermost stable circular orbits outward with respect to the one for this theory in four dimensions. Further, we consider the gravitational lensing, to test the GB gravity in (2+1) dimensions and show that the presence of the GB parameter causes the bending angle to first increase with the increase in the inverse of the closest approach distance, $$u_0$$ u 0 , reaching a peak value for a specific $$u_0^*$$ u 0 ∗ , and then decreasing to zero. We also show that the increase in the value of the GB parameter decreases the bending angle, and the increase in the absolute value of the negative cosmological constant produces an opposite effect on this angle.https://doi.org/10.1140/epjc/s10052-021-09617-4
collection DOAJ
language English
format Article
sources DOAJ
author Bakhtiyor Narzilloev
Sanjar Shaymatov
Ibrar Hussain
Ahmadjon Abdujabbarov
Bobomurat Ahmedov
Cosimo Bambi
spellingShingle Bakhtiyor Narzilloev
Sanjar Shaymatov
Ibrar Hussain
Ahmadjon Abdujabbarov
Bobomurat Ahmedov
Cosimo Bambi
Motion of particles and gravitational lensing around the (2+1)-dimensional BTZ black hole in Gauss–Bonnet gravity
European Physical Journal C: Particles and Fields
author_facet Bakhtiyor Narzilloev
Sanjar Shaymatov
Ibrar Hussain
Ahmadjon Abdujabbarov
Bobomurat Ahmedov
Cosimo Bambi
author_sort Bakhtiyor Narzilloev
title Motion of particles and gravitational lensing around the (2+1)-dimensional BTZ black hole in Gauss–Bonnet gravity
title_short Motion of particles and gravitational lensing around the (2+1)-dimensional BTZ black hole in Gauss–Bonnet gravity
title_full Motion of particles and gravitational lensing around the (2+1)-dimensional BTZ black hole in Gauss–Bonnet gravity
title_fullStr Motion of particles and gravitational lensing around the (2+1)-dimensional BTZ black hole in Gauss–Bonnet gravity
title_full_unstemmed Motion of particles and gravitational lensing around the (2+1)-dimensional BTZ black hole in Gauss–Bonnet gravity
title_sort motion of particles and gravitational lensing around the (2+1)-dimensional btz black hole in gauss–bonnet gravity
publisher SpringerOpen
series European Physical Journal C: Particles and Fields
issn 1434-6044
1434-6052
publishDate 2021-09-01
description Abstract We study the motion of test particles and photons in the vicinity of the (2+1)-dimensional Gauss–Bonnet (GB) BTZ black hole. We find that the presence of the coupling constant serves as an attractive gravitational charge, shifting the innermost stable circular orbits outward with respect to the one for this theory in four dimensions. Further, we consider the gravitational lensing, to test the GB gravity in (2+1) dimensions and show that the presence of the GB parameter causes the bending angle to first increase with the increase in the inverse of the closest approach distance, $$u_0$$ u 0 , reaching a peak value for a specific $$u_0^*$$ u 0 ∗ , and then decreasing to zero. We also show that the increase in the value of the GB parameter decreases the bending angle, and the increase in the absolute value of the negative cosmological constant produces an opposite effect on this angle.
url https://doi.org/10.1140/epjc/s10052-021-09617-4
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