Cosmic censorship violation in black hole collisions in higher dimensions

Dec 12, 2018
10 pages
Published in:
  • JHEP 04 (2019) 121
  • Published: Apr 18, 2019
e-Print:

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Abstract: (arXiv)
We argue that cosmic censorship is violated in the collision of two black holes in high spacetime dimension D when the initial total angular momentum is sufficiently large. The two black holes merge and form an unstable bar-like horizon, which grows a neck in its middle that pinches down with diverging curvature. When D is large, the emission of gravitational radiation is strongly suppressed and cannot spin down the system to a stable rotating black hole before the neck grows. The phenomenon is demonstrated using simple numerical simulations of the effective theory in the 1/D expansion. We propose that, even though cosmic censorship is violated, the loss of predictability is small independently of D.
Note:
  • 9 pages, 2 figures. v2: matches published version
  • Black Holes
  • Spacetime Singularities
  • Classical Theories of Gravity
  • cosmic censorship: violation
  • black hole: rotation
  • gravitational radiation: emission
  • space-time: dimension
  • stability: rotation
  • numerical calculations
  • higher-dimensional