Reply to "Comment on 'Greybody radiation and quasinormal modes of Kerr-like black hole in Bumblebee gravity model' "
arXiv:2202.11708 · doi:10.1140/epjc/s10052-022-10044-2
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.
References in corpus (4)
- Finite-distance gravitational deflection of massive particles by the Kerr-like black hole in the bumblebee gravity model
- Greybody Radiation and Quasinormal Modes of Kerr-like Black Hole in Bumblebee Gravity Model
- Slowly rotating Einstein-bumblebee black hole solution and its greybody factor in a Lorentz violation model
- Superradiant instability of the Kerr-like black hole in Einstein-bumblebee gravity
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- Topical Review: Greybody Factors and Quasinormal Modes for Black Holes in Various Theories -- Fingerprints of Invisibles
- Some Observable Physical Properties of the Higher Dimensional dS/AdS Black Holes in Einstein-Bumblebee Gravity Theory
- Probing the Lorentz Invariance Violation via Gravitational Lensing and Analytical Eigenmodes of Perturbed Slowly Rotating Bumblebee Black Holes
- Geodesics structure and deflection angle of electrically charged black holes in gravity with a background Kalb-Ramond field
- Quasinormal modes of the bumblebee black holes with a global monopole
- Quasinormal modes of the spherical bumblebee black holes with a global monopole
- Lorentz Symmetry Violation in Charged Black Hole Thermodynamics and Gravitational Lensing: Effects of the Kalb-Ramond Field
- Exact modifications on a vacuum spacetime due to a gradient bumblebee field at its vacuum expectation value
- Fermionic and Bosonic Greybody Factors as well as Quasinormal Modes for Charged Taub NUT Black Holes
- Superradiant (In)stability, Greybody Radiation, and Quasinormal Modes of Rotating Black Holes in non-linear Maxwell f (R) Gravity
- Super-entropy bumblebee AdS black holes
- Gravitational time advancement effect in Bumblebee gravity for Earth bound systems
- Kerr-Sen-like Lorentz violating black holes and Superradiance phenomena
- Optical and Thermodynamic Signatures of Lorentz Symmetry Breaking in Bumblebee AdS Black Holes