Abstract
We discuss the various scales determining the temporal behaviour of correlation functions in the presence of eternal black holes. We point out the origins of the failure of the semiclassical gravity approximation to respect a unitarity-based bound suggested by Maldacena. We find that the presence of a subleading (in the large N approximation involved) master field does restore the compliance with one bound but additional configurations are needed to explain the more detailed expected time dependence of the Poincare recurrences and their magnitude.
| Original language | English |
|---|---|
| Journal | Proceedings of Science |
| Volume | 11 |
| State | Published - 2003 |
| Event | 27th Johns Hopkins Workshop on Current Problems in Particle Theory: Symmetries and Mysteries of M Theory, JHW 2003 - Goteborg, Sweden Duration: 24 Aug 2003 → 26 Aug 2003 |
Bibliographical note
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