2026-04-17T03:49:18Zhttps://recercat.cat/oai/request

oai:recercat.cat:2445/1788962025-12-05T16:40:45Zcom_2072_1057col_2072_478823col_2072_478917

00925njm 22002777a 4500 dc Emparan García de Salazar, Roberto A. author Tomasevic, Marija author 2021-07-06T17:12:05Z 2021-07-06T17:12:05Z 2020-06-04 2021-07-06T17:12:05Z 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. Espai i temps Forats negres (Astronomia) Gravitació Space and time Black holes (Astronomy) Gravitation Strong cosmic censorship in the BTZ black hole