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Quantum states of the spacetime, and formation of black holes in AdS

We argue that a non-perturbative description of quantum gravity should involve two (non-interacting) copies of a dual field theory on the boundary, and describe the states of the spacetimes accordingly. So, for instance, a complete description of the asymptotically Anti-de-Sitter spacetimes is given...

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Autor principal: Botta Cantcheff, Marcelo
Lenguaje:eng
Publicado: 2012
Materias:
Acceso en línea:https://dx.doi.org/10.1142/S0218271812420096
http://cds.cern.ch/record/1449029
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author Botta Cantcheff, Marcelo
author_facet Botta Cantcheff, Marcelo
author_sort Botta Cantcheff, Marcelo
collection CERN
description We argue that a non-perturbative description of quantum gravity should involve two (non-interacting) copies of a dual field theory on the boundary, and describe the states of the spacetimes accordingly. So, for instance, a complete description of the asymptotically Anti-de-Sitter spacetimes is given by two copies of the conformal field theory associated to the global AdS spacetime. We also argue that, in this context, gravitational collapse and formation of a black hole may be described by unitary evolution of the dual non-perturbative degrees of freedom.
id cern-1449029
institution Organización Europea para la Investigación Nuclear
language eng
publishDate 2012
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spelling cern-14490292023-03-14T19:30:12Zdoi:10.1142/S0218271812420096http://cds.cern.ch/record/1449029engBotta Cantcheff, MarceloQuantum states of the spacetime, and formation of black holes in AdSParticle Physics - TheoryWe argue that a non-perturbative description of quantum gravity should involve two (non-interacting) copies of a dual field theory on the boundary, and describe the states of the spacetimes accordingly. So, for instance, a complete description of the asymptotically Anti-de-Sitter spacetimes is given by two copies of the conformal field theory associated to the global AdS spacetime. We also argue that, in this context, gravitational collapse and formation of a black hole may be described by unitary evolution of the dual non-perturbative degrees of freedom.We argue that a non-perturbative description of quantum gravity should involve two (non-interacting) copies of a dual field theory on the boundary, and describe the states of the spacetimes accordingly. So, for instance, a complete description of the asymptotically Anti-de-Sitter spacetimes is given by two copies of the conformal field theory associated to the global AdS spacetime. We also argue that, in this context, gravitational collapse and formation of a black hole may be described by unitary evolution of the dual non-perturbative degrees of freedom.arXiv:1205.3113oai:cds.cern.ch:14490292012-05-15
spellingShingle Particle Physics - Theory
Botta Cantcheff, Marcelo
Quantum states of the spacetime, and formation of black holes in AdS
title Quantum states of the spacetime, and formation of black holes in AdS
title_full Quantum states of the spacetime, and formation of black holes in AdS
title_fullStr Quantum states of the spacetime, and formation of black holes in AdS
title_full_unstemmed Quantum states of the spacetime, and formation of black holes in AdS
title_short Quantum states of the spacetime, and formation of black holes in AdS
title_sort quantum states of the spacetime, and formation of black holes in ads
topic Particle Physics - Theory
url https://dx.doi.org/10.1142/S0218271812420096
http://cds.cern.ch/record/1449029
work_keys_str_mv AT bottacantcheffmarcelo quantumstatesofthespacetimeandformationofblackholesinads