Gedanken experiments at high-order approximation: Kerr black hole cannot be overspun
arXiv:2108.03454 · doi:10.1007/JHEP09(2021)095
Abstract
Sorce and Wald proposed a new version of gedanken experiments to examine the weak cosmic censorship conjecture (WCCC) in Kerr-Newmann black holes. However, their discussion only includes the second-order approximation of perturbation and there exists an optimal condition such that the validity of the WCCC is determined by the higher-order approximations. Therefore, in this paper, we extended their discussions into the high-order approximations to study the WCCC in a nearly extremal Kerr black hole. After assuming that the spacetime satisfies the stability condition and the perturbation matter fields satisfy the null energy condition, based on the Noether charge method by Iyer and Wald, we completely calculate the first four order perturbation inequalities and discuss the corresponding gedanken experiment to overspin the Kerr black hole. As a result, we find that the nearly extremal Kerr black holes cannot be destroyed under the fourth-order approximation of perturbation. Then, by using the mathematical induction, we strictly prove the th order perturbation inequality when the first order perturbation inequalities are saturated. Using these results, we discuss the first order approximation of the gedanken experiments and find that the WCCC in Kerr black hole is valid under the higher-order approximation of perturbation. Our investigation implies that the WCCC might be strictly satisfied in Kerr black holes under the perturbation level.
21 pages, 2 figures
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- Gedanken Experiments to Destroy a Black Hole II: Kerr-Newman Black Holes Cannot be Over-Charged or Over-Spun
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Cited by in corpus (4)
- Destroying the event horizon of a nonsingular rotating quantum-corrected black hole
- First law of black hole thermodynamics and the weak cosmic censorship conjecture for Kerr-Newman Taub-NUT black holes
- The First Law and Weak Cosmic Censorship for de Sitter Black Holes
- Overcharging a nonsingular black hole in general relativity: the nonlinear electrodynamic field effects