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We engage in the computation of quasinormal modes associated with scalar andDirac fields around spherically symmetric black holes with a global monopole inbumblebee gravity. The frequency of oscillation and the damping rate exhibitsignificant decreasing as the global monopole parameter is increased. Anintriguing observation arises in the extreme limit, where the quasinormal modesmanifest a form of universal behavior: the actual oscillation frequency remainsunaltered despite variations in the Lorentz symmetry breaking (LSB) parameter.Our calculations are conducted through two distinct methods, both of whichyield results that align remarkably well. Furthermore, we derive an analyticalformula for quasinormal modes within the eikonal approximation.

Quasinormal modes of the bumblebee black holes with a global monopole