Pith. sign in

REVIEW 2 cited by

Stability and Quasinormal Modes of Black Holes in Conformal Weyl Gravity

Not yet reviewed by Pith; the record is open.

Re-run · record.json Download PDF Read on arXiv ↗

This paper has not been read by Pith yet. Machine review is queued; the pith claim, tier, and objections will appear here once it completes.

SPECIMEN: schema-true, not a live event

T0 review · schema-true

One-sentence machine reading of the paper's core claim.

pith:XXXXXXXX · record.json · timestamp

arxiv 1807.01792 v3 pith:WE65CQ7M submitted 2018-07-04 hep-th gr-qc

Mehrab Momennia , Seyed Hossein Hendi , Fatemeh Soltani Bidgoli This is my paper · ORCID
classification hep-thgr-qc
keywords blackmodesquasinormalholesconformalsolutionsthermalweyl
verification ladder T0 review T1 audit T2 compute T3 formal
0 comments
read the original abstract

In this paper, we first investigate the thermal stability of black holes in conformal Weyl gravity with a comparison with the Schwarzschild black holes. Then, we consider a minimally coupled massive scalar perturbation and calculate the quasinormal modes in asymptotically dS spacetime by employing the sixth order WKB approximation and asymptotic iteration method. The deviations from those of the Schwarzschild-dS solutions are obtained and the possibility of the presence of quasi-resonance modes for Weyl black hole solutions is investigated. Finally, we consider a massless scalar perturbation in the background of asymptotically AdS solutions and calculate the quasinormal modes by using the pseudospectral method. The effects of the free parameter of the theory on the quasinormal modes are studied and deviations from those of the Schwarzschild-AdS black holes are investigated. The imaginary part of quasinormal frequencies in AdS spacetime is the time scale of a thermal state (in the conformal field theory) to approach thermal equilibrium.

Discussion (0). Continue with ORCID to comment.

Forward citations

Cited by 2 Pith papers

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

  1. Hawking Emission from Black Holes Evaporating toward Wormholes and the Accuracy of the WKB Approximation

    gr-qc 2026-06 unverdicted novelty 5.5 of 10

    Numerical greybody factors for photons and massless Dirac fields in Simpson-Visser and Casadio-Fabbri-Mazzacurati geometries reveal that WKB overestimates luminosities by orders of magnitude near wormhole endpoints, i...

  2. Black hole shadow parameters and quasi-normal modes for Weyl-incorporated gravity

    gr-qc 2026-07 conditional novelty 4.0 of 10

    In WIG with a constant-density halo, shadow radii and test-field scalar QNMs are computed for mass-dependent λ values fitted to keep a horizon, showing mild GR deviations and long-lived damped modes.

Pith tools