Information flow in black hole evaporation

By H. Chen, Zachary Kenneth Fisher, Juan P. Hernandez, R. Myers, Shan-Ming Ruan. Journal of High Energy Physics, 2019

138 citations recorded by the source corpus.

Recently, new holographic models of black hole evaporation have given fresh insights into the information paradox [1–3]. In these models, the black hole evaporates into an auxiliary bath space after a quantum quench, wherein the holographic theory and the bath are joined. One particularly exciting development is the appearance of ‘ER=EPR’-like wormholes in the (doubly) holographic model of [3]. At late times, the entanglement wedge of the bath includes the interior of the black hole. In this paper, we employ both numerical and analytic methods to study how information about the black hole interior is encoded in the Hawking radiation. In particular, we systematically excise intervals from the bath from the system and study the corresponding Page transition. Repeating this process ad infinitum, we end up with a fractal structure on which the black hole interior is encoded, implementing the überholography protocol of [4].

Subfields: Astronomy and Astrophysics, Nuclear and High Energy Physics, Statistical and Nonlinear Physics

View Paper: https://www.semanticscholar.org/paper/790dd9d966ba3296fd70b1f3c406de8e8aef3998

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In Astronomy and Astrophysics

  1. D. Stanford
  2. J. Maldacena
  3. R. Myers
  4. S. Shenker
  5. S. Raju
  6. D. Harlow
  7. Thomas Hartman
  8. L. Susskind

In Nuclear and High Energy Physics

  1. D. Stanford
  2. R. Myers
  3. S. Raju
  4. J. Maldacena
  5. S. Shenker
  6. Thomas Hartman
  7. D. Harlow
  8. Zhenbin Yang

In Statistical and Nonlinear Physics

  1. D. Stanford
  2. S. Raju
  3. R. Myers
  4. J. Maldacena
  5. S. Shenker
  6. Thomas Hartman
  7. H. Chen
  8. Zhenbin Yang

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