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.
Title resolution pending
4 Pith papers cite this work. Polarity classification is still indexing.
4
Pith papers citing it
fields
gr-qc 4verdicts
UNVERDICTED 4representative citing papers
Greybody lower bounds and absorption cross sections for massless fields of spins 0, 1, and 1/2 are computed in the Euler-Heisenberg black hole with perfect fluid dark matter, revealing monotonic increases with frequency and parameter-dependent deformations of the spectra.
Tsallis statistics applied to Reissner-Nordström black holes yields a generalized entropy leading to Van der Waals-like phase transitions whose critical behavior is reflected in photon-sphere observables.
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
-
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.
-
Perturbations and greybody bounds of Euler-Heisenberg black holes surrounded by perfect fluid dark matter
Greybody lower bounds and absorption cross sections for massless fields of spins 0, 1, and 1/2 are computed in the Euler-Heisenberg black hole with perfect fluid dark matter, revealing monotonic increases with frequency and parameter-dependent deformations of the spectra.
-
Black Hole Thermodynamics via Tsallis Statistical Mechanics and Phase Transitions Probed by Optical Characteristics
Tsallis statistics applied to Reissner-Nordström black holes yields a generalized entropy leading to Van der Waals-like phase transitions whose critical behavior is reflected in photon-sphere observables.
-
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.