Time evolutions of scalar field perturbations in D-dimensional Reissner–Nordström Anti-de Sitter black holes

@article{Li2016TimeEO,
  title={Time evolutions of scalar field perturbations in D-dimensional Reissner–Nordstr{\"o}m Anti-de Sitter black holes},
  author={Ran Li and Hongbao Zhang and Junkun Zhao},
  journal={Physics Letters B},
  year={2016},
  volume={758},
  pages={359-364}
}

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References

SHOWING 1-10 OF 84 REFERENCES

Superradiant Instability of Five-Dimensional Rotating Charged AdS Black Holes

We study the instability of small AdS black holes with two independent rotation parameters in minimal five-dimensional gauged supergravity to massless scalar perturbations. We analytically solve the

Nonlinear Evolution and Final Fate of Charged Anti-de Sitter Black Hole Superradiant Instability.

We describe the full nonlinear development of the superradiant instability for a charged massless scalar field coupled to general relativity and electromagnetism, in the vicinity of a

Superradiant instabilities of rotating black holes in the time domain

Bosonic fields on rotating black hole spacetimes are subject to amplification by superradiance, which induces exponentially-growing instabilities (the “black hole bomb”) in two scenarios: if the

Maxwell perturbations on Kerr–anti–de Sitter black holes: Quasinormal modes, superradiant instabilities, and vector clouds

Scalar and gravitational perturbations on Kerr-anti-de Sitter (Kerr-AdS) black holes have been addressed in the literature and have been shown to exhibit a rich phenomenology. In this paper we

Explosion and Final State of an Unstable Reissner-Nordström Black Hole.

It is shown that (i) the process stops before all the charge is extracted from the BH, and (ii) the system settles down into a hairy BH: a charged horizon in equilibrium with a scalar field condensate, whose phase is oscillating at the final) critical frequency.

Time evolution of superradiant instabilities for charged black holes in a cavity

Departamento de Fisica da Universidade de Aveiro and I3N, Campus de Santiago,3810-183 Aveiro, Portugal(Received 8 January 2014; published 6 March 2014)Frequency domain studies have recently

Quasinormal modes of a massless charged scalar field on a small Reissner-Nordström-anti-de Sitter black hole

We investigate quasinormal modes of a massless charged scalar field on a small Reissner-Nordstroem-anti-de Sitter (RN-AdS) black hole both with analytical and numerical approaches. In the analytical

Analytical study of greybody factor and quasinormal modes for the scalar field in rotating linear dilaton black hole

The rotating linear dilaton black hole is an asymptotically non-flat solution to Einstein–Maxwell-Dilaton–Axion gravity theory due to the existence of non-trivial matter fields. We have analytically

Marginal scalar and Proca clouds around Reissner-Nordström black holes

Massive scalar test fields around Kerr black holes can form quasi-bound states with complex frequencies. Some of these states decay in time, but some others -- in the superradiant regime -- grow,
...