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Quasinormal modes of five-dimensional black holes in non-commutative geometry

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Abstract

We compute the spectrum of quasinormal frequencies of five-dimensional black holes obtained in noncommutative geometry. In particular, we study scalar perturbations of a massive scalar field adopting the sixth order WKB approximation. We investigate in detail the impact of the mass of the scalar field, the angular degree and the overtone number on the spectrum. All modes are found to be stable.

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Acknowledgements

The author G. P. thanks the Fundação para a Ciência e Tecnologia (FCT), Portugal, for the financial support to the Center for Astrophysics and Gravitation-CENTRA, Instituto Superior Técnico, Universidade de Lisboa, through the Grant No. UID/FIS/00099/2013. The author Á. R. acknowledges DI-VRIEA for financial support through Proyecto Postdoctorado 2019 VRIEA-PUCV.

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  1. Departamento de Física, Instituto Superior Técnico-IST, Centro de Astrofísica e Gravitação, Universidade de Lisboa-UL, Av. Rovisco Pais, 1049-001, Lisboa, Portugal

    Grigoris Panotopoulos

  2. Instituto de Física, Pontificia Universidad Católica de Valparaíso, Avenida Brasil 2950, Casilla 4059, Valparaíso, Chile

    Ángel Rincón

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  1. Grigoris Panotopoulos
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Panotopoulos, G., Rincón, Á. Quasinormal modes of five-dimensional black holes in non-commutative geometry. Eur. Phys. J. Plus 135, 33 (2020). https://doi.org/10.1140/epjp/s13360-019-00016-z

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