The instability spectra of near-extremal Reissner-Nordström-de Sitter black holes
arXiv:1808.04077 · doi:10.1016/j.physletb.2018.09.039
Abstract
The linearized dynamics of charged massive scalar fields in the near-extremal charged Reissner-Nordström-de Sitter (RNdS) black-hole spacetime is studied analytically. Interestingly, it is proved that the non-asymptotically flat charged black-hole-field system is characterized by {\it unstable} (exponentially growing in time) complex resonant modes. Using a WKB analysis in the eikonal large-mass regime , we provide a remarkably compact analytical formula for the quasinormal resonant spectrum which characterizes the unstable modes of the composed RNdS-black-hole-charged-massive-scalar-field system [here are respectively the mass, electric charge, and cosmological constant of the black-hole spacetime, and are the proper mass and charge coupling constant of the linearized field].
7 pages. This is an improved version of the one published in PLB
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Cited by in corpus (11)
- Superradiant instability of charged scalar fields in higher-dimensional Reissner-Nordström-de Sitter black holes
- Circular Motion of Charged Particles near Charged Black Hole
- Black Hole Superradiance in the Presence of Lorentz Symmetry Violation
- Near-extremal black holes in Weyl gravity: Quasinormal modes and geodesic instability
- Quantum (dis)charge of black hole interiors
- The renormalized charged scalar current in the Reissner-Nordström-de Sitter spacetime
- The fastest relaxation rate of higher-dimensional Reissner--Nordström black hole
- Relaxation rate of RNdS black hole
- Scalar tachyonic instabilities in gravitational backgrounds: Existence and growth rate
- Reissner-Nordström black holes in de Sitter space-time: bounds with quasinormal frequencies
- Superradiance and instabilities in black holes surrounded by anisotropic fluids