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Quantum chaos and unitary black hole evaporation

Journal Article · · Journal of High Energy Physics (Online)
 [1];  [2]
  1. Brown University, Providence, RI (United States); Brown Univ., Providence, RI (United States)
  2. University of Iceland, Reykjavik (Iceland); Stockholm University (Sweden); KTH Royal Institute of Technology, Stockholm (Sweden)
The formation and evaporation of small AdS black holes in a theory with a holographic dual is governed by the usual rules of quantum mechanics. The eigenstate thermalization hypothesis explains the validity of semiclassical gravity for local bulk observables and can be used to quantify the magnitude of quantum corrections to the semi-classical approximation. The holographic dual produces a basis of black hole states with finite energy width, and observables that are smooth functions on the classical phase space will self-average over a large number of energy eigenstates, exponential in the Bekenstein-Hawking entropyS, leading to results that are consistent with semiclassical gravity up to small corrections of order e–S/2. As expected, the semiclassical description breaks down for transition amplitudes that reflect the unitary evolution of the holographic theory.
Research Organization:
Brown Univ., Providence, RI (United States); Brown University, Providence, RI (United States)
Sponsoring Organization:
Icelandic Research Fund; USDOE Office of Science (SC); USDOE Office of Science (SC), High Energy Physics (HEP); University of Iceland Research Fund
Grant/Contract Number:
SC0010010
OSTI ID:
1976481
Alternate ID(s):
OSTI ID: 2340786
Journal Information:
Journal of High Energy Physics (Online), Journal Name: Journal of High Energy Physics (Online) Journal Issue: 5 Vol. 2022; ISSN 1029-8479
Publisher:
Springer NatureCopyright Statement
Country of Publication:
United States
Language:
English

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