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

Greybody Radiation and Quasinormal Modes of Kerr-like Black Hole in Bumblebee Gravity Model