Gravitational perturbations of the Hayward spacetime and testing the correspondence between quasinormal modes and grey-body factors
Zainab Malik

TL;DR
This study investigates gravitational perturbations of the Hayward black hole, confirming the correspondence between quasinormal modes and grey-body factors and analyzing quantum correction effects on these phenomena.
Contribution
It provides the first detailed comparison of grey-body factors and quasinormal modes for the Hayward black hole, including quantum correction effects.
Findings
Grey-body factors decrease with quantum corrections.
The quasinormal mode and grey-body factor correspondence is highly accurate.
Quantum corrections suppress absorption cross-sections.
Abstract
The paper studies axial gravitational perturbations of the Hayward black hole, a regular geometry that also arises as an effective solution in asymptotically safe gravity. By computing grey-body factors with the 6th-order WKB method and comparing them to predictions based on the quasinormal modes, the correspondence between transmission coefficients and quasinormal spectra is verified. Quantum corrections, parametrized by , are shown to suppress both the grey-body factors and the absorption cross-section, while the correspondence remains accurate at the percent level for low multipoles and essentially exact for higher ones.
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