On overspinning of black holes in higher dimensions
arXiv:2004.09242 · doi:10.1016/j.dark.2020.100758
Abstract
It turns out that repulsive effect due to rotation of a rotating black hole dominates over attraction due to mass for large in dimensions . This gives rise to a remarkable result that black hole in these higher dimensions in contrast to lower dimensional ones cannot be overspun even under linear test particle accretion. Further if a black hole in dimension has one of its rotation parameters zero, it has only one horizon and hence it can never be overspun. Thus rotating black holes in six and higher dimensions, and those with one rotation parameter switched off, would always obey the weak cosmic censorship conjecture (WCCC).
7 pages, 2 figures; references added, minor changes made
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Cited by in corpus (13)
- Motion of Particles and Gravitational Lensing Around (2+1)-dimensional BTZ black holes in Gauss-Bonnet Gravity
- Extending the weak cosmic censorship conjecture to the charged Buchdahl star by employing the gedanken experiments
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- Cosmic censorship, massless fermionic test fields, and absorption probabilities
- Weak Cosmic Censorship Conjecture in Myers-Perry Black Hole with Separability
- The Hookean Law of Black Holes and Fragmentation: Insights from Maximum Force Conjecture and Ruppeiner Geometry
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- Self energy in Kerr-Sen space-time incorporated to overspinning and overcharging problems