We determine the characteristic timescales associated with the linearized relaxation dynamics of the composed Reissner–Nordström-black-hole-charged-massive-scalar-field system. To that end, the quasinormal resonant frequencies {ωn(μ,q,M,Q)}n=0n=∞ which characterize the dynamics of a charged scalar field of mass μ and charge coupling constant q in the charged Reissner–Nordström black-hole spacetime of mass M and electric charge Q are determined analytically in the eikonal regime 1≪Mμ<qQ. Interestingly, we find that, for a given value of the dimensionless black-hole electric charge Q/M, the imaginary part of the resonant oscillation frequency is a monotonically decreasing function of the dimensionless ratio μ/q. In particular, it is shown tha...
Recent numerical studies of the coupled Einstein–Klein–Gordon system in a cavity have provided compe...
We evaluate quasinormal modes of a massive scalar field of the Ernst spacetime, an exact solution of...
It is proved that dynamically formed Reissner-Nordström-de Sitter (RNdS) black holes, which have rec...
AbstractWe determine the characteristic timescales associated with the linearized relaxation dynamic...
The quasinormal resonance spectrum {ωn(μ,q,M,Q)}n=0n=∞ of charged massive scalar fields in the charg...
The linearized dynamics of charged massive scalar fields in the near-extremal charged Reissner–Nords...
AbstractThe quasinormal resonance spectrum {ωn(μ,q,M,Q)}n=0n=∞ of charged massive scalar fields in t...
Abstract The quasi-bound states of charged massive scalar fields in the near-extremal charged Reissn...
The quasinormal resonance frequency of the higher-dimensional Reissner–Nordström (RN) black hole due...
AbstractWe compute characteristic (quasinormal) frequencies corresponding to decay of a massive char...
Here we show that the phenomenon of arbitrarily long-lived quasinormal modes (called quasiresonances...
Abstract Numerous numerical investigations of the quasinormal resonant spectra of Kerr-Newman black ...
AbstractRotating black holes can support quasi-stationary (unstable) bound-state resonances of massi...
Rotating black holes can support quasi-stationary (unstable) bound-state resonances of massive scala...
We investigate the quasibound states of charged massive scalar fields in the Kerr–Newman black hole ...
Recent numerical studies of the coupled Einstein–Klein–Gordon system in a cavity have provided compe...
We evaluate quasinormal modes of a massive scalar field of the Ernst spacetime, an exact solution of...
It is proved that dynamically formed Reissner-Nordström-de Sitter (RNdS) black holes, which have rec...
AbstractWe determine the characteristic timescales associated with the linearized relaxation dynamic...
The quasinormal resonance spectrum {ωn(μ,q,M,Q)}n=0n=∞ of charged massive scalar fields in the charg...
The linearized dynamics of charged massive scalar fields in the near-extremal charged Reissner–Nords...
AbstractThe quasinormal resonance spectrum {ωn(μ,q,M,Q)}n=0n=∞ of charged massive scalar fields in t...
Abstract The quasi-bound states of charged massive scalar fields in the near-extremal charged Reissn...
The quasinormal resonance frequency of the higher-dimensional Reissner–Nordström (RN) black hole due...
AbstractWe compute characteristic (quasinormal) frequencies corresponding to decay of a massive char...
Here we show that the phenomenon of arbitrarily long-lived quasinormal modes (called quasiresonances...
Abstract Numerous numerical investigations of the quasinormal resonant spectra of Kerr-Newman black ...
AbstractRotating black holes can support quasi-stationary (unstable) bound-state resonances of massi...
Rotating black holes can support quasi-stationary (unstable) bound-state resonances of massive scala...
We investigate the quasibound states of charged massive scalar fields in the Kerr–Newman black hole ...
Recent numerical studies of the coupled Einstein–Klein–Gordon system in a cavity have provided compe...
We evaluate quasinormal modes of a massive scalar field of the Ernst spacetime, an exact solution of...
It is proved that dynamically formed Reissner-Nordström-de Sitter (RNdS) black holes, which have rec...