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Exact Solutions of Regge-Wheeler Equation and Quasi-Normal Modes of Compact Objects

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arxiv gr-qc/0509123 v5 pith:XWXN7POC submitted 2005-09-30 gr-qc

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keywords equationcompactmathematicalmodesobjectsquasi-normalregge-wheeleranalytical
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The well-known Regge-Wheeler equation describes the axial perturbations of Schwarzschild metric in the linear approximation. From a mathematical point of view it presents a particular case of the confluent Heun equation and can be solved exactly, due to recent mathematical developments. We present the basic properties of its general solution. A novel analytical approach and numerical techniques for study the boundary problems which correspond to quasi-normal modes of black holes and other simple models of compact objects are developed.

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Cited by 3 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Quasinormal Modes of Extremal Reissner-Nordstrom Black Holes via Seiberg-Witten Quantization

    hep-th 2026-03 unverdicted novelty 7.0 of 10

    Quasinormal-mode frequencies of extremal Reissner-Nordström black holes for charged and massive scalar fields are computed through Seiberg-Witten/Nekrasov-Shatashvili quantization.

  2. Green function of the P\"{o}schl-Teller potential

    gr-qc 2025-10 unverdicted novelty 5.0 of 10

    Exact time-domain Green function computed for the Pöschl-Teller approximation to black-hole perturbation potentials, revealing additional early-time exponentially growing modes and a light-cone plus historical wavefor...

  3. Deriving effective descriptions and signal predictions for dynamical gravitational systems

    gr-qc 2026-06 unverdicted novelty 4.0 of 10

    Presents cavity-based effective descriptions for scalar radiation from black holes and modified models, linking them to wave profiles and accumulated phase shifts for detecting small deviations from classical behavior.

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