The quantum parameter ζ modifies quasinormal frequency spectra of charged effective black holes with Λ, preserving non-monotonic behaviors while adding new features to overtone outbursts and complex-imaginary mode interactions.
Singh, Are loop quantum cosmos never singular?, Classical Quantum Gravity26, 125005 (2009)
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Quasinormal modes of charged covariant effective black holes with a cosmological constant
The quantum parameter ζ modifies quasinormal frequency spectra of charged effective black holes with Λ, preserving non-monotonic behaviors while adding new features to overtone outbursts and complex-imaginary mode interactions.