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Scalar Perturbations of Charged Dilaton Black Holes

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arxiv hep-th/0312041 v3 pith:N4X7EWS6 submitted 2003-12-03 hep-th gr-qc

Sharmanthie Fernando , Keith Arnold This is my paper · ORCID
classification hep-thgr-qc
keywords blackdilatonholesmodesscalarchargeddimensionsnormal
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We have studied the scalar perturbation of static charged dilaton black holes in 3+1 dimensions. The black hole considered here is a solution to the low-energy string theory in 3+1 dimensions. The quasinormal modes for the scalar perturbations are calculated using the third order WKB method. The dilaton coupling constant has a considerable effect on the values of quasi normal modes. It is also observed that there is a linear relation between the quasi normal modes and the temperature for large black holes.

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  1. The shadow and quasinormal modes of the asymptotically flat hairy black holes with a dilaton potential

    gr-qc 2025-08 conditional novelty 5.0 of 10

    For exact asymptotically flat hairy charged black holes with a dilaton potential, the shadow radius, photon-orbit Lyapunov exponent, and scalar quasinormal frequencies are computed, showing strong coupling dependence ...

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