Stationary scalar clouds around a BTZ black hole
arXiv:1707.08133 · doi:10.1016/j.physletb.2017.08.017
Abstract
We establish the existence of stationary clouds of massive test scalar fields around BTZ black holes. These clouds are zero-modes of the superradiant instability and are possible when Robin boundary conditions (RBCs) are considered at the AdS boundary. These boundary conditions are the most general ones that ensure the AdS space is an isolated system, and include, as a particular case, the commonly considered Dirichlet or Neumann-type boundary conditions (DBCs or NBCs). We obtain an explicit, closed form, resonance condition, relating the RBCs that allow the existence of normalizable (and regular on and outside the horizon) clouds to the system's parameters. Such RBCs never include pure DBCs or NBCs. We illustrate the spatial distribution of these clouds, their energy and angular momentum density for some cases. Our results show that BTZ black holes with scalar hair can be constructed, as the non-linear realization of these clouds.
7 pages, 2 figures
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- The extreme orbital period in scalar hairy kerr black holes
- Anisotropic Generalized Polytropic Spheres: Regular 3D Black Holes
- Ground state for a massive scalar field in BTZ spacetime with Robin boundary conditions
- Black holes, stationary clouds and magnetic fields
- Quasinormal modes of charged BTZ black holes
- Analog model for the BTZ black hole
- Boundary conditions for isolated asymptotically anti-de Sitter spacetimes