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Strong cosmic censorship in the BTZ black hole
Abstract
A bstract: Recently it has been shown that quantum fields can be regular on the inner, Cauchy horizon of a rotating BTZ black hole, which appears to indicate a failure of strong cosmic censorship. We argue that, instead, what these results imply is that the inner horizon remains non-singular when leading-order backreaction of the quantum fields is computed, but, after next-order backreaction is accounted for, it will become singular. Then, strong cosmic censorship will be enforced in the BTZ black hole. We support our claims using a four-dimensional holographic dual of the system, which connects the instability of the inner horizon of the BTZ black hole to that of Kerr-type black holes.
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Rotating quantum BTZ has a singular inner horizon.
“Consequently, as argued in [300], and verified in [301] using the techniques of [299], rotating quantum BTZ has a singular inner horizon.”
From Three-Dimensional Quantum Black Holes: A Primer (2024) · cites this paper as [300]
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Cited by
Sorted by citations
Three-Dimensional Quantum Black Holes: A Primer
Panella, E., Pedraza, J. F., & Svesko, A. (2024) · Universe · doi:10.3390/universe10090358 · Cited by 24
Unveiling horizons in quantum critical collapse
Tomašević, M., & Wu, C.-H. (2026) · Journal of High Energy Physics · doi:10.1007/jhep04(2026)151 · Cited by 5
Self-citation
Metadata
- Authors
- Emparan, R., & Tomašević, M.
- ORCID
- Emparan, Roberto
- Venue
- Journal of High Energy Physics
- Published
- 2020-06-04
- Volume
- 2020
- Issue
- 6
- ISSN
- 1029-8479
- Cited by
- 32
- References
- 0
- Language
- en
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