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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Auteur principal:	Alex Buchel
Format:	article
Langue:	EN
Publié:	Elsevier 2021
Sujets:	Nuclear and particle physics. Atomic energy. Radioactivity QC770-798
Accès en ligne:	https://doaj.org/article/6b3ed4306c7d48e188b82a20337c844f
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id	oai: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
_version_	1718373036703350784

Compactified holographic conformal order

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