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Quasinormal modes and shadow of noncommutative black hole

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arxiv 2103.10659 v3 pith:IAZE5XQK submitted 2021-03-19 hep-th gr-qc

J. A. V. Campos , M. A. Anacleto , F. A. Brito , E. Passos This is my paper · ORCID
classification hep-thgr-qc
keywords noncommutativequasinormalshadowblackholemodesnoncommutativityparameter
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In this paper we investigate quasinormal modes (QNM) for a scalar field around a noncommutative Schwarzschild black hole. We verify the effect of noncommutativity on quasinormal frequencies by applying two procedures widely used in the literature. The first is the Wentzel-Kramers-Brillouin (WKB) approximation up to sixth order. In the second case we use the continuous fraction method developed by Leaver. Besides, we also show that due to noncommutativity, the shadow radius is reduced when we increase the noncommutative parameter. In addition, we find that the shadow radius is nonzero even at the zero mass limit for finite noncommutative parameter.

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  1. Scalar quasinormal modes, Lyapunov exponents and radii of null geodesics of rotating regular black holes

    gr-qc 2025-04 conditional novelty 4.0 of 10

    The paper computes scalar quasinormal modes of rotating Bardeen and Hayward black holes and finds they follow the eikonal null-geodesic relations, with Bardeen deviations up to about 19% from Kerr.

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