K Akiyama, A Alberdi, W Alef, JC Algaba… - The Astrophysical …, 2022 - iopscience.iop.org
Astrophysical black holes are expected to be described by the Kerr metric. This is the only stationary, vacuum, axisymmetric metric, without electromagnetic charge, that satisfies …
Horizon-scale images of black holes (BHs) and their shadows have opened an unprecedented window onto tests of gravity and fundamental physics in the strong-field …
Astrophysical black holes are expected to be described by the Kerr metric. This is the only stationary, vacuum, axisymmetric metric, without electromagnetic charge, that satisfies …
RA Konoplya, AF Zinhailo - The European Physical Journal C, 2020 - Springer
Recently a D-dimensional regularization approach leading to the non-trivial (3+ 1)(3+ 1)- dimensional Einstein–Gauss–Bonnet (EGB) effective description of gravity was formulated …
The existence of black holes and spacetime singularities is a fundamental issue in science. Despite this, observations supporting their existence are scarce, and their interpretation is …
We consider a simple spherical model consisting of a Schwarzschild black hole of mass M and a dark matter of mass ΔM around it. The general formula for the radius of black-hole …
C Liu, T Zhu, Q Wu, K Jusufi, M Jamil, M Azreg-Aïnou… - Physical Review D, 2020 - APS
In this paper, we construct an effective rotating loop quantum black hole (LQBH) solution, starting from the spherical symmetric LQBH by applying the Newman-Janis algorithm …
SW Wei, YX Liu - The European Physical Journal Plus, 2021 - Springer
The recent discovery of the novel four-dimensional static and spherically symmetric Gauss– Bonnet black hole provides a promising bed to test Gauss–Bonnet gravity by using …