Greybody factor and quasinormal modes of Regular Black Holes

Ángel Rincón (Instituto de Física, Pontificia Universidad Católica de Valparaíso, Avenida Brasil 2950, Casilla, Valparaíso, 4059, Chile) ; Victor Santos (Fundação Cearense de Apoio ao Desenvolvimento Científico e Tecnológico (FUNCAP), Av. Oliveira Paiva, 941, Cidade dos Funcionários, Fortaleza, CE, 60822-130, Brazil)

In this work, we investigate the quasinormal frequencies of a class of regular black hole solutions which generalize Bardeen and Hayward spacetimes. In particular, we analyze scalar, vector and gravitational perturbations of the black hole with the semianalytic WKB method. We analyze in detail the behaviour of the spectrum depending on the parameter p/q of the black hole, the quantum number of angular momentum and the s number. In addition, we compare our results with the classical solution valid for $$p = q = 1$$ p = q = 1 .

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      "value": "In this work, we investigate the quasinormal frequencies of a class of regular black hole solutions which generalize Bardeen and Hayward spacetimes. In particular, we analyze scalar, vector and gravitational perturbations of the black hole with the semianalytic WKB method. We analyze in detail the behaviour of the spectrum depending on the parameter p/q of the black hole, the quantum number of angular momentum and the s number. In addition, we compare our results with the classical solution valid for  $$p = q = 1$$  <math> <mrow> <mi>p</mi> <mo>=</mo> <mi>q</mi> <mo>=</mo> <mn>1</mn> </mrow> </math>  ."
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Published on:
02 October 2020
Publisher:
Springer
Published in:
European Physical Journal C , Volume 80 (2020)
Issue 10
Pages 1-7
DOI:
https://doi.org/10.1140/epjc/s10052-020-08445-2
Copyrights:
The Author(s)
Licence:
CC-BY-4.0

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