Quasinormal modes and greybody factors are calculated via 6th-order WKB for the QOS black hole with quintessence and string clouds, with parameter effects analyzed and rigorous bounds given for scalar greybody factors.
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The work calculates scalar quasinormal mode spectra for a rotating quantum-corrected black hole and constructs a methodological pipeline to infer the quantum correction parameter from gravitational-wave ringdown data using informative priors.
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Quasinormal Modes, Greybody Factors and Rigorous Bounds for Quantum Oppenheimer-Snyder Black Hole with Quintessential Dark Energy and a String Clouds
Quasinormal modes and greybody factors are calculated via 6th-order WKB for the QOS black hole with quintessence and string clouds, with parameter effects analyzed and rigorous bounds given for scalar greybody factors.
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The quasinormal modes of the rotating quantum corrected black holes
The work calculates scalar quasinormal mode spectra for a rotating quantum-corrected black hole and constructs a methodological pipeline to infer the quantum correction parameter from gravitational-wave ringdown data using informative priors.