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In this paper we consider quasi-normal modes of test scalar andelectromagnetic fields in the background of a non-Schwarzschild black hole inthe Einstein-Weyl gravity. We find the dependence of the modes on the newparameter $p$, which is related to the coupling constant $\alpha$, fordifferent values of the angular parameter $l$ and show that when $l$ isincreasing, the frequencies tend to linear dependence on $p$. We have alsoexamined the case of a massive scalar field for which we have shown that thearbitrarily long lived modes (called quasi-resonances) exist in the spectrum.

Quasinormal modes of the four-dimensional black hole in Einstein-Weyl gravity