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超自旋不稳定性的终点与宇宙监督假设的违背

End Point of the Ultraspinning Instability and Violation of Cosmic Censorship.

作者信息

Figueras Pau, Kunesch Markus, Lehner Luis, Tunyasuvunakool Saran

机构信息

School of Mathematical Sciences, Queen Mary University of London, Mile End Road, London E1 4NS, United Kingdom.

Department of Applied Mathematics and Theoretical Physics (DAMTP), Centre for Mathematical Sciences, University of Cambridge, Wilberforce Road, Cambridge CB3 0WA, United Kingdom.

出版信息

Phys Rev Lett. 2017 Apr 14;118(15):151103. doi: 10.1103/PhysRevLett.118.151103. Epub 2017 Apr 11.

Abstract

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.

摘要

我们确定了六维时空维度中渐近平直的迈尔斯 - 佩里黑洞轴对称超旋转不稳定性的终点。在非线性 regime 中,这种不稳定性在旋转平面上产生了一系列由黑色膜段连接的同心环。随着时间的推移,后者会变得更薄,导致在有限的渐近时间内形成裸奇点,从而在渐近平直的高维空间中违反了弱宇宙审查猜想。

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