Compactified holographic conformal order

We study holographic conformal order compactified on S3. The corresponding boundary CFT4 has a thermal phase with a nonzero expectation value of a certain operator. The gravitational dual to the ordered phase is represented by a black hole in asymptotically AdS5 that violates the no-hair theorem. Wh...

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Autor principal: Alex Buchel
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Lenguaje:EN
Publicado: Elsevier 2021
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Acceso en línea:https://doaj.org/article/6b3ed4306c7d48e188b82a20337c844f
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spelling oai:doaj.org-article:6b3ed4306c7d48e188b82a20337c844f2021-12-04T04:32:59ZCompactified holographic conformal order0550-321310.1016/j.nuclphysb.2021.115605https://doaj.org/article/6b3ed4306c7d48e188b82a20337c844f2021-12-01T00:00:00Zhttp://www.sciencedirect.com/science/article/pii/S0550321321003023https://doaj.org/toc/0550-3213We study holographic conformal order compactified on S3. The corresponding boundary CFT4 has a thermal phase with a nonzero expectation value of a certain operator. The gravitational dual to the ordered phase is represented by a black hole in asymptotically AdS5 that violates the no-hair theorem. While the compactification does not destroy the ordered phase, it does not cure its perturbative instability: we identify the scalar channel QNM of the hairy black hole with Im[w]>0. On the contrary, we argue that the disordered thermal phase of the boundary CFT is perturbatively stable in holographic models of Einstein gravity and scalars.Alex BuchelElsevierarticleNuclear and particle physics. Atomic energy. RadioactivityQC770-798ENNuclear Physics B, Vol 973, Iss , Pp 115605- (2021)
institution DOAJ
collection DOAJ
language EN
topic Nuclear and particle physics. Atomic energy. Radioactivity
QC770-798
spellingShingle Nuclear and particle physics. Atomic energy. Radioactivity
QC770-798
Alex Buchel
Compactified holographic conformal order
description We study holographic conformal order compactified on S3. The corresponding boundary CFT4 has a thermal phase with a nonzero expectation value of a certain operator. The gravitational dual to the ordered phase is represented by a black hole in asymptotically AdS5 that violates the no-hair theorem. While the compactification does not destroy the ordered phase, it does not cure its perturbative instability: we identify the scalar channel QNM of the hairy black hole with Im[w]>0. On the contrary, we argue that the disordered thermal phase of the boundary CFT is perturbatively stable in holographic models of Einstein gravity and scalars.
format article
author Alex Buchel
author_facet Alex Buchel
author_sort Alex Buchel
title Compactified holographic conformal order
title_short Compactified holographic conformal order
title_full Compactified holographic conformal order
title_fullStr Compactified holographic conformal order
title_full_unstemmed Compactified holographic conformal order
title_sort compactified holographic conformal order
publisher Elsevier
publishDate 2021
url https://doaj.org/article/6b3ed4306c7d48e188b82a20337c844f
work_keys_str_mv AT alexbuchel compactifiedholographicconformalorder
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