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Quasinormal Modes of Near-Extremal Black Holes and Black Strings in Massive Gravity Background

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arxiv 1911.11448 v4 pith:EIBKQWTG submitted 2019-11-26 gr-qc hep-th

Taum Wuthicharn , Supakchai Ponglertsakul , Piyabut Burikham This is my paper · ORCID
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keywords blackholesnear-extremalanalyticbackgroundformulamethodmodes
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Two numerical methods are used to calculate quasinormal modes (QNMs) of near-extremal black holes/strings in the generalized spherically/cylindrically symmetric background, the Asymptotic Iteration Method (AIM) and the Spectral Method. The numerical results confirm the accuracy of the approximate analytic formula using the P\"{o}schl-Teller potential. Our analytic formula is used to investigate the Strong Cosmic Censorship conjecture of extremal and near-extremal black holes in Ref. \cite{Burikham:2020dfi}.

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  1. Constructing regular black holes from multi-polytropic equations of state

    gr-qc 2025-02 reject novelty 5.0 of 10

    Two regular black hole metrics are derived from anisotropic multi-polytropic TOV equations; one reduces to the known Hayward geometry and the other is new, with repulsive-gravity regions outside the horizon for partic...

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