Photonic black resonators and photon stars in AdS
arXiv:1910.03234 · doi:10.1088/1361-6382/ab7418
Abstract
Rapidly rotating Myers-Perry-AdS (MPAdS) black holes are shown to be unstable against rotational superradiance of a Maxwell field. From the onset of the instability, time-periodic neutral black hole solutions equipped with a nontrivial electromagnetic wave are obtained, which we call {\it photonic black resonators}. In the horizonless limit, they reduce to geon solutions which may be called {\it photon stars}. Specifically, we introduce a cohomogeneity-1 ansatz for the metric and Maxwell field and construct such solutions with an isometry group. We compute thermodynamic quantities and obtain phase diagrams. It turns out that a photonic black resonator has a higher entropy than a MPAdS black hole, while it also has a smaller entropy than a black resonator without the Maxwell field. This suggests what is expected for nonlinear dynamics following the Maxwell superradiant instability with the isometry.
23 pages, 10 figures
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- Superradiant instability of black resonators and geons
- Gregory-Laflamme encounters Superradiance
- Stability of small charged anti-de Sitter black holes in the Robin boundary
- Superradiance and black resonator strings encounter helical black strings