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- W3052233182 abstract "We study the phenomena of mass inflation using the Ori model for a rotating BTZ black hole that is sufficiently far from extremality, and show that the right Cauchy horizon ($mathcal{CH}^+_R$) of the BTZ black hole becomes singular. Motivated by the recent analysis of Dias, Reall, Santos [J. High Energy Phys. 12 (2019) 097], we choose the retrograde quasinormal modes to govern the decay of perturbations exterior to the black hole. The resulting model captures the violation of the strong cosmic censorship conjecture near extremality. On the other hand, far from extremality, the $mathcal{CH}^+_R$ of a BTZ black hole develops a weak null singularity. Our analysis shows a slowly rotating BTZ black hole will respect strong cosmic censorship." @default.
- W3052233182 created "2020-08-24" @default.
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- W3052233182 date "2020-08-17" @default.
- W3052233182 modified "2023-10-03" @default.
- W3052233182 title "Mass inflation and strong cosmic censorship in a nonextreme BTZ black hole" @default.
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- W3052233182 doi "https://doi.org/10.1103/physrevd.102.044030" @default.
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