Instability and new phases of higher-dimensional rotating black holes

Details Instability and new phases of higher-dimensional rotating black holes Instability and new phases of higher-dimensional rotating black holes

2009-07-14

arxiv.org/abs/0907.2248v2

Phys.Rev.D80:111701,2009

Physics

High Energy Physics

High Energy Physics - Theory

5 pages, 5 figures. The instability of the black hole is argued to appear at the second zero mode. The first zero mode is not

Scientific paper

10.1103/PhysRevD.80.111701

It has been conjectured that higher-dimensional rotating black holes become unstable at a sufficiently large value of the rotation, and that new black holes with pinched horizons appear at the threshold of the instability. We search numerically, and find, the stationary axisymmetric perturbations of Myers-Perry black holes with a single spin that mark the onset of the instability and the appearance of the new black hole phases. We also find new ultraspinning Gregory-Laflamme instabilities of rotating black strings and branes.

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