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Scalar and spinor QNMs of a black hole with a global monopole in f (R) gravity

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Abstract

The quasinormal modes for scalar and spinor fields in the background spacetime corresponding to a black hole with a global monopole in f(R) gravity are calculated using the WKB approximation. In the obtained results we emphasize the role played by the parameter \(\psi _{0}\), associated with the f (R) gravity. We discuss the appropriate limit \(\psi _{0} \rightarrow 0\), in which case the results concerning to the Schwarzschild black hole are obtained, as it should be expected.

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Acknowledgments

J.P.M.G. was supported by CAPES Fellowship. H.S.V. and V.B.B. would like to thank Conselho Nacional de Desenvolvimento Científico e Tecnológico (CNPq) for partial financial support. The authors would like to thank an anonymous referee for their valuable comments.

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  1. Departamento de Físics, Universidade Federal da Paraíba, Caixa Postal 5008, João Pessoa, PB, 58051-970, Brazil

    J. P. Morais Graça, H. S. Vieira & V. B. Bezerra

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  1. J. P. Morais Graça
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  2. H. S. Vieira
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  3. V. B. Bezerra
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Correspondence to J. P. Morais Graça.

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Graça, J.P.M., Vieira, H.S. & Bezerra, V.B. Scalar and spinor QNMs of a black hole with a global monopole in f (R) gravity. Gen Relativ Gravit 48, 38 (2016). https://doi.org/10.1007/s10714-016-2024-7

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