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...
Guardado en:
Autor principal: | |
---|---|
Formato: | article |
Lenguaje: | EN |
Publicado: |
Elsevier
2021
|
Materias: | |
Acceso en línea: | https://doaj.org/article/6b3ed4306c7d48e188b82a20337c844f |
Etiquetas: |
Agregar Etiqueta
Sin Etiquetas, Sea el primero en etiquetar este registro!
|
id |
oai:doaj.org-article:6b3ed4306c7d48e188b82a20337c844f |
---|---|
record_format |
dspace |
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 |