  In the framework of the Lorentz symmetry breaking (LSB), we investigate the
quasinormal modes (QNMs) and the greybody factors (GFs) of the Kerr-like black
hole spacetime obtained from the bumblebee gravity model. In particular, we
analyze the scalar and fermionic perturbations of the black hole within the
framework of both semi-analytic WKB method and the time domain approach. The
impacts of the LSB on the bosonic/fermionic QNMs and GFs of the Kerr-like black
hole are investigated in detail. The obtained results are graphically depicted
and discussed.
