Solution of the cosmological constant problem within holographic cosmology
Autor(a) principal: | |
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Data de Publicação: | 2020 |
Tipo de documento: | Artigo |
Idioma: | eng |
Título da fonte: | Repositório Institucional da UNESP |
Texto Completo: | http://dx.doi.org/10.1016/j.physletb.2019.135168 http://hdl.handle.net/11449/199862 |
Resumo: | Within the holographic cosmology paradigm, specifically the model of McFadden and Skenderis, but more generally than that, the cosmological constant is found to naturally flow from a large value, to a small value, which can even be as low as the needed ∼10−120 times the original, along with the dual RG flow. Within this context then, the cosmological constant problem is mapped to a simple quantum field theory property, even though the exact mechanism for it in gravity is still obscure. I consider several examples of gravity duals to explain the mechanism. |
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Repositório Institucional da UNESP |
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Solution of the cosmological constant problem within holographic cosmologyWithin the holographic cosmology paradigm, specifically the model of McFadden and Skenderis, but more generally than that, the cosmological constant is found to naturally flow from a large value, to a small value, which can even be as low as the needed ∼10−120 times the original, along with the dual RG flow. Within this context then, the cosmological constant problem is mapped to a simple quantum field theory property, even though the exact mechanism for it in gravity is still obscure. I consider several examples of gravity duals to explain the mechanism.Fundação de Amparo à Pesquisa do Estado de São Paulo (FAPESP)Conselho Nacional de Desenvolvimento Científico e Tecnológico (CNPq)Instituto de Física Teórica UNESP-Universidade Estadual Paulista, Rua Dr. Bento T. Ferraz 271, Bl. IIInstituto de Física Teórica UNESP-Universidade Estadual Paulista, Rua Dr. Bento T. Ferraz 271, Bl. IIFAPESP: 2014/18634-9FAPESP: 2016/01343-7CNPq: 304006/2016-5Universidade Estadual Paulista (Unesp)Nastase, Horatiu [UNESP]2020-12-12T01:51:20Z2020-12-12T01:51:20Z2020-02-10info:eu-repo/semantics/publishedVersioninfo:eu-repo/semantics/articlehttp://dx.doi.org/10.1016/j.physletb.2019.135168Physics Letters, Section B: Nuclear, Elementary Particle and High-Energy Physics, v. 801.0370-2693http://hdl.handle.net/11449/19986210.1016/j.physletb.2019.1351682-s2.0-85077063730Scopusreponame:Repositório Institucional da UNESPinstname:Universidade Estadual Paulista (UNESP)instacron:UNESPengPhysics Letters, Section B: Nuclear, Elementary Particle and High-Energy Physicsinfo:eu-repo/semantics/openAccess2021-10-23T10:11:12Zoai:repositorio.unesp.br:11449/199862Repositório InstitucionalPUBhttp://repositorio.unesp.br/oai/requestopendoar:29462024-08-05T22:52:57.385212Repositório Institucional da UNESP - Universidade Estadual Paulista (UNESP)false |
dc.title.none.fl_str_mv |
Solution of the cosmological constant problem within holographic cosmology |
title |
Solution of the cosmological constant problem within holographic cosmology |
spellingShingle |
Solution of the cosmological constant problem within holographic cosmology Nastase, Horatiu [UNESP] |
title_short |
Solution of the cosmological constant problem within holographic cosmology |
title_full |
Solution of the cosmological constant problem within holographic cosmology |
title_fullStr |
Solution of the cosmological constant problem within holographic cosmology |
title_full_unstemmed |
Solution of the cosmological constant problem within holographic cosmology |
title_sort |
Solution of the cosmological constant problem within holographic cosmology |
author |
Nastase, Horatiu [UNESP] |
author_facet |
Nastase, Horatiu [UNESP] |
author_role |
author |
dc.contributor.none.fl_str_mv |
Universidade Estadual Paulista (Unesp) |
dc.contributor.author.fl_str_mv |
Nastase, Horatiu [UNESP] |
description |
Within the holographic cosmology paradigm, specifically the model of McFadden and Skenderis, but more generally than that, the cosmological constant is found to naturally flow from a large value, to a small value, which can even be as low as the needed ∼10−120 times the original, along with the dual RG flow. Within this context then, the cosmological constant problem is mapped to a simple quantum field theory property, even though the exact mechanism for it in gravity is still obscure. I consider several examples of gravity duals to explain the mechanism. |
publishDate |
2020 |
dc.date.none.fl_str_mv |
2020-12-12T01:51:20Z 2020-12-12T01:51:20Z 2020-02-10 |
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/10.1016/j.physletb.2019.135168 Physics Letters, Section B: Nuclear, Elementary Particle and High-Energy Physics, v. 801. 0370-2693 http://hdl.handle.net/11449/199862 10.1016/j.physletb.2019.135168 2-s2.0-85077063730 |
url |
http://dx.doi.org/10.1016/j.physletb.2019.135168 http://hdl.handle.net/11449/199862 |
identifier_str_mv |
Physics Letters, Section B: Nuclear, Elementary Particle and High-Energy Physics, v. 801. 0370-2693 10.1016/j.physletb.2019.135168 2-s2.0-85077063730 |
dc.language.iso.fl_str_mv |
eng |
language |
eng |
dc.relation.none.fl_str_mv |
Physics Letters, Section B: Nuclear, Elementary Particle and 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_ |
1808129470144446464 |