We study neutral massless scalar field perturbations around an extreme dilaton black hole in 2 +1 dimensions: the wave equations of the massless scalar field is shown to be exactly solvable in terms of Whittaker functions. Thus, the quasinormal modes are computed exactly and shown to be purely imaginary: we show the existence of stable and unstable modes. Interestingly, the quasinormal modes do not depend on the black holes parameters and the fundamental mode is always unstable and depends only on the parameters of the test field. Also, we determine the quasinormal frequencies via the improved asymptotic iteration method which shows a good agreement with the analytical results.Comment: 19 pages, 1 figur
To obtain fermionic quasinormal modes, the Dirac equation for two types of black holes is investigat...
Here we show that the phenomenon of arbitrarily long-lived quasinormal modes (called quasiresonances...
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We found quasinormal modes, both in time and frequency domains, of the Ernst black holes, that is ne...
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We discuss whether the minimally coupled massless Klein-Gordon and Dirac fields have well defined qu...
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We show that in the limit where the number of spacetime dimensions D grows to infinity a very large ...
For a static and spherically symmetric black hole, a photon sphere is composed of circular null geod...
We study the quasinormal modes of fermionic perturbations for an asymptotically Lifshitz black hole ...
We study the propagation of scalar fields in the background of an asymptotically de Sitter black hol...
We show that in the limit where the number of spacetime dimensions D grows to infinity a very large ...
Quasinormal modes (QNMs) are the damped vibrations of black hole (BH) spacetimes, characterising m...
To obtain fermionic quasinormal modes, the Dirac equation for two types of black holes is investigat...
Here we show that the phenomenon of arbitrarily long-lived quasinormal modes (called quasiresonances...
It has been observed that many spacetimes which feature a near-extremal horizon exhibit the phenomen...
We found quasinormal modes, both in time and frequency domains, of the Ernst black holes, that is ne...
Abstract We study the stability under scalar perturbations, and we compute the quasinormal modes of ...
Quasinormal modes of massless test scalar field in the background of gravitational field for a non-e...
We discuss whether the minimally coupled massless Klein-Gordon and Dirac fields have well defined qu...
Quasinormal modes are eigenmodes of dissipative systems. Perturbations of classical gravitational ba...
In this work, we investigate the quasinormal modes for a massive scalar field with a nonminimal coup...
We show that in the limit where the number of spacetime dimensions D grows to infinity a very large ...
For a static and spherically symmetric black hole, a photon sphere is composed of circular null geod...
We study the quasinormal modes of fermionic perturbations for an asymptotically Lifshitz black hole ...
We study the propagation of scalar fields in the background of an asymptotically de Sitter black hol...
We show that in the limit where the number of spacetime dimensions D grows to infinity a very large ...
Quasinormal modes (QNMs) are the damped vibrations of black hole (BH) spacetimes, characterising m...
To obtain fermionic quasinormal modes, the Dirac equation for two types of black holes is investigat...
Here we show that the phenomenon of arbitrarily long-lived quasinormal modes (called quasiresonances...
It has been observed that many spacetimes which feature a near-extremal horizon exhibit the phenomen...