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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...

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Detalles Bibliográficos
Autores principales: Barbón, José L F, Rabinovici, Eliezer
Lenguaje:eng
Publicado: 2004
Materias:
Acceso en línea:https://dx.doi.org/10.1002/prop.200410157
http://cds.cern.ch/record/727085
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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
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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
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