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Rings, ripples, and rotation: connecting black holes to black rings
2014
Journal of High Energy Physics
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
doi:10.1007/jhep07(2014)045
fatcat:oqbjzmd6cjen3bpy3czzqt6jxm