  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.
