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Quasinormal mode expansion and the exact solution of the Cauchy problem for wave equations

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abstract

Solutions for a class of wave equations with effective potentials are obtained by a method of a Laplace-transform. Quasinormal modes appear naturally in the solutions only in a spatially truncated form; their coefficients are uniquely determined by the initial data and are constant only in some region of spacetime -- in contrast to normal modes. This solves the problem of divergence of the usual expansion into spatially unbounded quasinormal modes and a contradiction with the causal propagation of signals. It also partially answers the question about the region of validity of the expansion. Results of numerical simulations are presented. They fully support the theoretical predictions.

fields

gr-qc 1

years

2025 1

verdicts

UNVERDICTED 1

representative citing papers

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

gr-qc · 2025-10-20 · unverdicted · novelty 5.0

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 waveform decomposition.

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  • Green function of the P\"{o}schl-Teller potential gr-qc · 2025-10-20 · unverdicted · none · ref 20 · internal anchor

    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 waveform decomposition.