Reply to “Comment on ‘Greybody radiation and quasinormal modes of Kerr-like black hole in Bumblebee gravity model”’
Sara Kanzi, İzzet Sakallı
Abstract
In our recent study Ref. [1]: Eur. Phys. J. C 81, 501 (2021) , the main goal was to reveal the Lorentz symmetry breaking (LSB) effect in the rotating black holes via the greybody factor and quasinormal mode analyzes. Ding et al. [2] Kerr-like black hole solution of the bumblebee gravity model used in our paper [1] has unquestionably proven by Maluf and Muniz [3] that it is wrong. We now explain under which condition the greybody factor and quasinormal mode analyzes performed in [1] become valid. We re-make the calculations according to the condition in question and present the new results in this reply.
Topics & Concepts
PhysicsLorentz transformationSymmetry (geometry)Black hole (networking)BumblebeeMode (computer interface)Rotating black holeTheoretical physicsMathematical physicsClassical mechanicsAngular momentumGeometryMathematicsEcologyEngineeringOperating systemLink-state routing protocolRouting (electronic design automation)PollinatorComputer scienceBiologyElectronic engineeringPollinationPollenRouting protocolBlack Holes and Theoretical PhysicsNoncommutative and Quantum Gravity TheoriesCosmology and Gravitation Theories