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14 October 2024
 
  » arxiv » 2206.00198

 Article overview



Inside Flat Event Horizons
Brett McInnes ;
Date 1 Jun 2022
AbstractGrinberg and Maldacena have recently used certain thermal one-point functions, evaluated outside an AdS black hole, to determine the proper time of fall from the event horizon to the singularity (in the uncharged case) or to the Cauchy horizon (in the charged, unperturbed case). This raises the hope that one can use data outside the black hole to investigate the claim that black holes "have no interiors", by proving that the time of fall is exceptionally short, perhaps effectively zero. We examine this question for the particularly interesting case of a black hole (with a flat, toroidal event horizon) emitted by a larger black hole, after the manner postulated by the Weak Gravity Conjecture. We find that the proper time of fall to the Cauchy horizon is indeed always very short for these black holes, so they are prime candidates for an investigation of this kind.
Source arXiv, 2206.00198
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