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We consider scalar and spinorial perturbations on a background described by a$z=3$ three-dimensional Lifshitz black hole. We obtained the correspondingquasinormal modes which perfectly agree with the analytical result for thequasinormal frequency in the scalar case. The numerical results for thespinorial perturbations reinforce our conclusion on the stability of the modelunder these perturbations. We also calculate the area spectrum, which prove tobe equally spaced, as an application of our results.

Quasinormal modes and thermodynamical aspects of the 3D Lifshitz black hole