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On long time unitarity restoring processes in the presence of eternal black holes
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...
Autores principales: | , |
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Lenguaje: | eng |
Publicado: |
2004
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Materias: | |
Acceso en línea: | https://dx.doi.org/10.1002/prop.200410157 http://cds.cern.ch/record/727085 |
_version_ | 1780903783922925568 |
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author | Barbón, José L F Rabinovici, Eliezer |
author_facet | Barbón, José L F Rabinovici, Eliezer |
author_sort | Barbón, José L F |
collection | CERN |
description | 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. |
id | cern-727085 |
institution | Organización Europea para la Investigación Nuclear |
language | eng |
publishDate | 2004 |
record_format | invenio |
spelling | cern-7270852019-09-30T06:29:59Zdoi:10.1002/prop.200410157http://cds.cern.ch/record/727085engBarbón, José L FRabinovici, EliezerOn long time unitarity restoring processes in the presence of eternal black holesParticle Physics - TheoryGeneral Relativity and CosmologyWe 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.hep-th/0403268CERN-PH-TH-2004-059oai:cds.cern.ch:7270852004-03-26 |
spellingShingle | Particle Physics - Theory General Relativity and Cosmology Barbón, José L F Rabinovici, Eliezer On long time unitarity restoring processes in the presence of eternal black holes |
title | On long time unitarity restoring processes in the presence of eternal black holes |
title_full | On long time unitarity restoring processes in the presence of eternal black holes |
title_fullStr | On long time unitarity restoring processes in the presence of eternal black holes |
title_full_unstemmed | On long time unitarity restoring processes in the presence of eternal black holes |
title_short | On long time unitarity restoring processes in the presence of eternal black holes |
title_sort | on long time unitarity restoring processes in the presence of eternal black holes |
topic | Particle Physics - Theory General Relativity and Cosmology |
url | https://dx.doi.org/10.1002/prop.200410157 http://cds.cern.ch/record/727085 |
work_keys_str_mv | AT barbonjoself onlongtimeunitarityrestoringprocessesinthepresenceofeternalblackholes AT rabinovicieliezer onlongtimeunitarityrestoringprocessesinthepresenceofeternalblackholes |