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Scalar and axial quasinormal modes of massive static phantom wormholes

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arxiv 1806.03282 v1 pith:3US6AUL7 submitted 2018-06-08 gr-qc

Jose Luis Blázquez-Salcedo , Xiao Yan Chew , Jutta Kunz This is my paper · ORCID
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keywords modesquasinormalscalaraxialblackmassivephantomspectrum
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abstract

We study the quasinormal modes for scalar, axial and radial perturbations of massive static spherically symmetric wormholes supported by a phantom scalar field, calculating the modes directly and employing the WKB approximation. The spectrum of the quasinormal modes is compared with the spectrum of Schwarzschild black holes. For fixed multipole number $l$ and large mass $M$ the wormhole modes approach their black hole counterparts as $1/M$.

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  1. Transition from Regular Black Holes to Wormholes in Covariant Effective Quantum Gravity: Scattering, Quasinormal Modes, and Hawking Radiation

    gr-qc 2025-02 conditional novelty 6.0 of 10

    For a quantum-corrected spacetime, the fundamental quasinormal mode differs little from Schwarzschild, higher overtones deviate significantly, and wormhole states have extremely long-lived modes.

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