Journal
EUROPEAN PHYSICAL JOURNAL C
Volume 78, Issue 12, Pages -Publisher
SPRINGER
DOI: 10.1140/epjc/s10052-018-6467-8
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Funding
- Research Center for Theoretical Physics and Astrophysics, Faculty of Philosophy and Science of Sileasian University at Opava
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In this paper we consider quasi-normal modes of test scalar and electromagnetic fields in the background of a non-Schwarzschild black hole in the Einstein-Weyl gravity. We find the dependence of the modes on the new parameter p, which is related to the coupling constant a, for different values of the angular parameter l and show that when l is increasing, the frequencies tend to linear dependence on p. We have also examined the case of a massive scalar field for which we have shown that the arbitrarily long lived modes (called quasi-resonances) exist in the spectrum.
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