The authors introduce physical field-vanishing boundary conditions for RN-AdS black holes, translate them to master-function conditions, and compute quasinormal frequencies that show new spectral features.
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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.
citing papers explorer
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Quasinormal modes of Reissner-Nordstr\"om-AdS black holes under physical field-vanishing boundary conditions
The authors introduce physical field-vanishing boundary conditions for RN-AdS black holes, translate them to master-function conditions, and compute quasinormal frequencies that show new spectral features.
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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.