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Weak cosmic censorship conjecture in the pure Lovelock gravity
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abstract
It is well known that a rotating black hole in four dimension could be overspun by linear order test particle accretion which however always gets overturned when non-linear perturbations are included. It turns out that in the Einstein gravity, repulsion due to rotation dominates over attraction due to mass in dimensions, $D>5$, and consequently black hole cannot be overspun even for linear order accretion. For the pure Lovelock rotating black hole, this dimensional threshold is $D>4N+1$ where $N$ is degree of single $N$th order term in the Lovelock polynomial in the action. Thus the pure Lovelock rotating black holes always obey the weak cosmic censorship conjecture (WCCC) in all dimensions greater than $4N+1$. Since overall gravity being repulsive beyond this dimensional threshold, how is rotating black hole then formed there?
Forward citations
Cited by 2 Pith papers
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Weak Cosmic Censorship Conjecture in Gedanken Experiments at All Orders
At every perturbation order, black hole gedanken experiments preserve cosmic censorship whenever the thermodynamic quantity W is positive.
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Extending the Comisso-Asenjo Energy Extraction Mechanism to Pure Lovelock Gravity
For rotating pure Lovelock black holes in 6–9 dimensions, magnetic reconnection extracts more rotational energy as dimension grows, with the 9-dimensional case most efficient and sometimes outpacing the Blandford-Znaj...
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