Black resonators and geons in AdS
arXiv:1810.11089 · doi:10.1088/1361-6382/ab1d76
Abstract
We construct dynamical black hole solutions with a helical symmetry in AdS, called black resonators, as well as their horizonless limits, called geons. We introduce a cohomogeneity-1 metric describing a class of black resonators and geons whose isometry group is . This allows us to study them in a wide range of parameters. We obtain the phase diagram for the black resonators, geons, and Myers-Perry-AdS, where the black resonators emerge from the onset of a superradiant instability of the Myers-Perry-AdS with equal angular momenta and are connected to the geons in the small horizon limit. The angular velocities of the black resonators always satisfy in units of the AdS radius. A black resonator is shown to have higher entropy than a Myers-Perry-AdS black hole with the same asymptotic charges. This implies that the Myers-Perry-AdS can dynamically evolve into the black resonator under the exact -symmetry although its endpoint will be further unstable to -violating perturbations.
27 pages, 9 figures
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Cited by in corpus (13)
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- Resonant Hamiltonian systems and weakly nonlinear dynamics in AdS spacetimes
- Energy extraction from AdS black holes via superradiance
- Multioscillating black holes
- Superradiant instability of black resonators and geons
- Gregory-Laflamme encounters Superradiance
- Gregory-Laflamme and Superradiance encounter Black Resonator Strings
- Photonic black resonators and photon stars in AdS
- Stability of small charged anti-de Sitter black holes in the Robin boundary
- Phase diagram of the charged black hole bomb system
- Superradiance and black resonator strings encounter helical black strings
- static, charged black holes, strings and rings with resonant, scalar -hair