End Point of the Ultraspinning Instability and Violation of Cosmic Censorship - INSPIRE

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End Point of the Ultraspinning Instability and Violation of Cosmic Censorship

Feb 6, 2017

6 pages

Published in:

Phys.Rev.Lett. 118 (2017) 15, 151103

Published: Apr 11, 2017

e-Print:

1702.01755 [hep-th]

DOI:

10.1103/PhysRevLett.118.151103

View in:

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Abstract: (APS)

We determine the end point of the axisymmetric ultraspinning instability of asymptotically flat Myers-Perry black holes in D=6 spacetime dimensions. In the nonlinear regime, this instability gives rise to a sequence of concentric rings connected by segments of black membrane on the rotation plane. The latter become thinner over time, resulting in the formation of a naked singularity in finite asymptotic time and hence a violation of the weak cosmic censorship conjecture in asymptotically flat higher-dimensional spaces.

Note:

Matches the published version. 4 pages plus references and supplemental material, 8 figures

cosmic censorship: violation
space-time: dimension: 6
black hole: Myers-Perry
symmetry: axial
stability
higher-dimensional
singularity
nonlinear
membrane
rotation

References(42)

Figures(17)

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