Rings, Ripples, and Rotation: Connecting Black Holes to Black Rings
arXiv:1402.6345 · doi:10.1007/JHEP07(2014)045
Abstract
Singly-spinning Myers-Perry black holes in d>5 spacetime dimensions are unstable for sufficiently large angular momentum. We numerically construct (in d=6 and d=7) two new stationary branches of lumpy (rippled) black hole solutions which bifurcate from the onset of this ultraspinning instability. We give evidence that one of these branches connects through a topology-changing merger to black ring solutions which we also construct numerically. The other branch approaches a solution with large curvature invariants. We are also able to compare the d=7 ring solutions with results from finite-size corrections to the blackfold approach, finding excellent agreement.
14 pages. 8 figures. v2: Appendix with discussion of numerical details and references added. Matches published version
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- Rayleigh-Plateau and Gregory-Laflamme instabilities of black strings
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