Author:
Hu Xin-Yun,Israr Aslam M.,Saleem Rabia,Zeng Xiao-Xiong
Abstract
Abstract
In the context of holography, the Einstein ring of an AdS black hole (BH) in massive
gravity (MG) is depicted. An oscillating Gaussian source on one side of the AdS boundary
propagates in bulk, and we impose a response function to explain it. Using a wave optics imaging
system, we obtain the optical appearance of the Einstein ring. Our research reveals that the ring
can change into a luminosity-deformed ring or light spots depending on the variation of parameters
and observational positions. When observers are positioned at the north pole, the holographic
profiles always appear as a ring with concentric stripe surroundings, and a bright ring appears at
the location of the photon sphere of the BH. To investigate the distinct features of the MG AdS BH
from previous studies, we discussed the relation between the temperature T and the event horizon
ue
, which shows the decaying behavior with the increasing values of the event horizon
ue
, when the graviton parameter m is fixed. These in turn influence the behavior of the
response function and the Einstein ring. For example, the amplitude of the lensed response
function |〈O〉| increases with the increasing values of the graviton parameter m,
for the fixed value of the horizon ue
. On the other hand, the amplitude of the lensed
response function |〈O〉| decreases with the increasing values of the horizon
ue
, for the fixed value of graviton parameter m. These differences are also reflected in
the Einstein ring, where the intensities and the locations of the Einstein ring significantly vary
according to the numerical values of the involved parameters. These findings are also observed in
the brightness profiles and the best fit comparison between the results obtained by wave optics
and geometric optics for different values of graviton parameter m. In this perspective, our
study contributes to a better understanding of the analytical studies of holographic theory, which
can be used to evaluate different types of BHs for a fixed wave source and optical system.
Subject
Astronomy and Astrophysics
Cited by
4 articles.
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