Mergers and typical black hole microstates

By I. Bena, Chih-Wei Wang, N. Warner. 2006

192 citations recorded by the source corpus.

We use mergers of microstates to obtain the first smooth horizonless microstate solutions corresponding to a BPS three-charge black hole with a classically large horizon area. These microstates have very long throats, that become infinite in the classical limit; nevertheless, their curvature is everywhere small. Having a classically-infinite throat makes these microstates very similar to the typical microstates of this black hole. A rough CFT analysis confirms this intuition, and indicates a possible class of dual CFT microstates. We also analyze the properties and the merging of microstates corresponding to zero-entropy BPS black holes and black rings. We find that these solutions have the same size as the horizon size of their classical counterparts, and we examine the changes of internal structure of these microstates during mergers.

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

View Paper: https://www.semanticscholar.org/paper/084a80a22aca16ffb6f8b7b9f6b796ff65a8f444

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The researchers whose trusted networks rank it highest, strongest advocate first. Every researcher gets a different order.

In Astronomy and Astrophysics

  1. Marika Taylor
  2. N. Warner
  3. I. Bena
  4. Kostas Skenderis
  5. J. Boer
  6. S. El-Showk
  7. I. Messamah
  8. Vijay Balasubramanian

In Nuclear and High Energy Physics

  1. Marika Taylor
  2. N. Warner
  3. I. Bena
  4. Kostas Skenderis
  5. J. Boer
  6. S. El-Showk
  7. Ashoke Sen
  8. I. Messamah

In Statistical and Nonlinear Physics

  1. N. Warner
  2. Marika Taylor
  3. I. Bena
  4. Kostas Skenderis
  5. Vijay Balasubramanian
  6. S. El-Showk
  7. I. Messamah
  8. J. Boer

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