pith:Y3GK7QPW
Finite Curvature Construction of Regular Black Holes and Quasinormal Mode Analysis
Prescribing finite curvature scalars produces regular black holes whose perturbation stability depends on the shape of the effective potential.
arxiv:2506.01035 v2 · 2025-06-01 · gr-qc · hep-th
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Claims
We show that the shape of the effective potential, particularly its width and the presence of potential valleys, plays a critical role in determining the QNMs. Models with a large peak-to-valley ratio in the potential barrier exhibit stable, exponentially decaying waveforms, while a small ratio may induce late-time instabilities.
The assumption that the chosen analytic profiles for the curvature functions (Gaussian, hyperbolic secant, rational) can be consistently integrated to produce metrics that are regular, asymptotically flat, and satisfy the dominant energy condition without introducing additional singularities or violations.
Regular black holes are built by prescribing finite Ricci or Weyl scalars with Gaussian, sech, and rational profiles to ensure regularity and energy conditions, with stability shown to depend on the peak-to-valley ratio of the perturbation potential.
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| First computed | 2026-05-21T01:04:14.293414Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
c6ccafc1f6ef156abc24bf1fa35ffbbd6effada96c4cb0e168718051f75b70a3
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Canonical record JSON
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