Holographic cosmology from “dimensional reduction” of N = 4 SYM vs. AdS5 × S 5
Autor(a) principal: | |
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Data de Publicação: | 2019 |
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Tipo de documento: | Artigo |
Idioma: | eng |
Título da fonte: | Repositório Institucional da UNESP |
Texto Completo: | http://dx.doi.org/10.1007/JHEP12(2019)025 http://hdl.handle.net/11449/199786 |
Resumo: | We propose a way to obtain holographic cosmology models for 3+1 dimensional cosmologies vs. 3 dimensional field theories from a “dimensional reduction” procedure, obtained by integrating over the time direction, of (modifed) standard holographic duals of 3+1 dimensional field theories. The example of a modified N = 4 SYM vs. AdS5 × S5 is presented, and in perturbation theory doesn’t match observations, though at strong coupling it might. But the proposed mechanism is more general, and it could in principle be applied to other top down holographic models. |
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Repositório Institucional da UNESP |
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Holographic cosmology from “dimensional reduction” of N = 4 SYM vs. AdS5 × S 5AdS-CFT CorrespondenceCosmology of Theories beyond the SMWe propose a way to obtain holographic cosmology models for 3+1 dimensional cosmologies vs. 3 dimensional field theories from a “dimensional reduction” procedure, obtained by integrating over the time direction, of (modifed) standard holographic duals of 3+1 dimensional field theories. The example of a modified N = 4 SYM vs. AdS5 × S5 is presented, and in perturbation theory doesn’t match observations, though at strong coupling it might. But the proposed mechanism is more general, and it could in principle be applied to other top down holographic models.Instituto de Física Teórica UNESP-Universidade Estadual Paulista, R. Dr. Bento T. Ferraz 271, Bl. IIInstituto de Física Teórica UNESP-Universidade Estadual Paulista, R. Dr. Bento T. Ferraz 271, Bl. IIUniversidade Estadual Paulista (Unesp)Bernardo, Heliudson [UNESP]Nastase, Horatiu [UNESP]2020-12-12T01:49:18Z2020-12-12T01:49:18Z2019-12-01info:eu-repo/semantics/publishedVersioninfo:eu-repo/semantics/articlehttp://dx.doi.org/10.1007/JHEP12(2019)025Journal of High Energy Physics, v. 2019, n. 12, 2019.1029-84791126-6708http://hdl.handle.net/11449/19978610.1007/JHEP12(2019)0252-s2.0-85076222402Scopusreponame:Repositório Institucional da UNESPinstname:Universidade Estadual Paulista (UNESP)instacron:UNESPengJournal of High Energy Physicsinfo:eu-repo/semantics/openAccess2021-10-23T09:49:02Zoai:repositorio.unesp.br:11449/199786Repositório InstitucionalPUBhttp://repositorio.unesp.br/oai/requestopendoar:29462024-08-05T22:15:01.558090Repositório Institucional da UNESP - Universidade Estadual Paulista (UNESP)false |
dc.title.none.fl_str_mv |
Holographic cosmology from “dimensional reduction” of N = 4 SYM vs. AdS5 × S 5 |
title |
Holographic cosmology from “dimensional reduction” of N = 4 SYM vs. AdS5 × S 5 |
spellingShingle |
Holographic cosmology from “dimensional reduction” of N = 4 SYM vs. AdS5 × S 5 Bernardo, Heliudson [UNESP] AdS-CFT Correspondence Cosmology of Theories beyond the SM |
title_short |
Holographic cosmology from “dimensional reduction” of N = 4 SYM vs. AdS5 × S 5 |
title_full |
Holographic cosmology from “dimensional reduction” of N = 4 SYM vs. AdS5 × S 5 |
title_fullStr |
Holographic cosmology from “dimensional reduction” of N = 4 SYM vs. AdS5 × S 5 |
title_full_unstemmed |
Holographic cosmology from “dimensional reduction” of N = 4 SYM vs. AdS5 × S 5 |
title_sort |
Holographic cosmology from “dimensional reduction” of N = 4 SYM vs. AdS5 × S 5 |
author |
Bernardo, Heliudson [UNESP] |
author_facet |
Bernardo, Heliudson [UNESP] Nastase, Horatiu [UNESP] |
author_role |
author |
author2 |
Nastase, Horatiu [UNESP] |
author2_role |
author |
dc.contributor.none.fl_str_mv |
Universidade Estadual Paulista (Unesp) |
dc.contributor.author.fl_str_mv |
Bernardo, Heliudson [UNESP] Nastase, Horatiu [UNESP] |
dc.subject.por.fl_str_mv |
AdS-CFT Correspondence Cosmology of Theories beyond the SM |
topic |
AdS-CFT Correspondence Cosmology of Theories beyond the SM |
description |
We propose a way to obtain holographic cosmology models for 3+1 dimensional cosmologies vs. 3 dimensional field theories from a “dimensional reduction” procedure, obtained by integrating over the time direction, of (modifed) standard holographic duals of 3+1 dimensional field theories. The example of a modified N = 4 SYM vs. AdS5 × S5 is presented, and in perturbation theory doesn’t match observations, though at strong coupling it might. But the proposed mechanism is more general, and it could in principle be applied to other top down holographic models. |
publishDate |
2019 |
dc.date.none.fl_str_mv |
2019-12-01 2020-12-12T01:49:18Z 2020-12-12T01:49:18Z |
dc.type.status.fl_str_mv |
info:eu-repo/semantics/publishedVersion |
dc.type.driver.fl_str_mv |
info:eu-repo/semantics/article |
format |
article |
status_str |
publishedVersion |
dc.identifier.uri.fl_str_mv |
http://dx.doi.org/10.1007/JHEP12(2019)025 Journal of High Energy Physics, v. 2019, n. 12, 2019. 1029-8479 1126-6708 http://hdl.handle.net/11449/199786 10.1007/JHEP12(2019)025 2-s2.0-85076222402 |
url |
http://dx.doi.org/10.1007/JHEP12(2019)025 http://hdl.handle.net/11449/199786 |
identifier_str_mv |
Journal of High Energy Physics, v. 2019, n. 12, 2019. 1029-8479 1126-6708 10.1007/JHEP12(2019)025 2-s2.0-85076222402 |
dc.language.iso.fl_str_mv |
eng |
language |
eng |
dc.relation.none.fl_str_mv |
Journal of High Energy Physics |
dc.rights.driver.fl_str_mv |
info:eu-repo/semantics/openAccess |
eu_rights_str_mv |
openAccess |
dc.source.none.fl_str_mv |
Scopus reponame:Repositório Institucional da UNESP instname:Universidade Estadual Paulista (UNESP) instacron:UNESP |
instname_str |
Universidade Estadual Paulista (UNESP) |
instacron_str |
UNESP |
institution |
UNESP |
reponame_str |
Repositório Institucional da UNESP |
collection |
Repositório Institucional da UNESP |
repository.name.fl_str_mv |
Repositório Institucional da UNESP - Universidade Estadual Paulista (UNESP) |
repository.mail.fl_str_mv |
|
_version_ |
1808129408990445568 |