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Mergers and Typical Black Hole Microstates

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; never the less, their curvature is ev...

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Detalles Bibliográficos
Autores principales: Bena, I, Wang, C W, Warner, Nicholas P
Lenguaje:eng
Publicado: 2006
Materias:
Acceso en línea:https://dx.doi.org/10.1088/1126-6708/2006/11/042
http://cds.cern.ch/record/980945
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author Bena, I
Wang, C W
Warner, Nicholas P
author_facet Bena, I
Wang, C W
Warner, Nicholas P
author_sort Bena, I
collection CERN
description 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; never the less, 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.
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institution Organización Europea para la Investigación Nuclear
language eng
publishDate 2006
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spelling cern-9809452019-09-30T06:29:59Zdoi:10.1088/1126-6708/2006/11/042http://cds.cern.ch/record/980945engBena, IWang, C WWarner, Nicholas PMergers and Typical Black Hole MicrostatesParticle Physics - TheoryWe 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; never the less, 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.hep-th/0608217CERN-PH-TH-2006-151NSF-KITP-06-26oai:cds.cern.ch:9809452006-08-30
spellingShingle Particle Physics - Theory
Bena, I
Wang, C W
Warner, Nicholas P
Mergers and Typical Black Hole Microstates
title Mergers and Typical Black Hole Microstates
title_full Mergers and Typical Black Hole Microstates
title_fullStr Mergers and Typical Black Hole Microstates
title_full_unstemmed Mergers and Typical Black Hole Microstates
title_short Mergers and Typical Black Hole Microstates
title_sort mergers and typical black hole microstates
topic Particle Physics - Theory
url https://dx.doi.org/10.1088/1126-6708/2006/11/042
http://cds.cern.ch/record/980945
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