Friedmann-Lemaitre-Robertson-Walker braneworlds
Autor(a) principal: | |
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Data de Publicação: | 2017 |
Outros Autores: | , |
Tipo de documento: | Artigo |
Idioma: | eng |
Título da fonte: | Repositório Institucional da UNESP |
Texto Completo: | http://dx.doi.org/10.1016/j.physletb.2017.06.072 http://hdl.handle.net/11449/163465 |
Resumo: | We study the cosmological evolution with nonsingular branes generated by a bulk scalar field coupled to gravity. The specific setup investigated leads to branes with a time-dependent warp factor. We calculate the effective Hubble parameter and the effective scale factor for the FLRW branes obtained solutions. The spatially dependent branes solutions also were found. (c) 2017 The Authors. Published by Elsevier B.V. |
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Repositório Institucional da UNESP |
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2946 |
spelling |
Friedmann-Lemaitre-Robertson-Walker braneworldsWe study the cosmological evolution with nonsingular branes generated by a bulk scalar field coupled to gravity. The specific setup investigated leads to branes with a time-dependent warp factor. We calculate the effective Hubble parameter and the effective scale factor for the FLRW branes obtained solutions. The spatially dependent branes solutions also were found. (c) 2017 The Authors. Published by Elsevier B.V.Conselho Nacional de Desenvolvimento Científico e Tecnológico (CNPq)Coordenação de Aperfeiçoamento de Pessoal de Nível Superior (CAPES)Univ Estadual Paulista, Dept Fis & Quim, Av Dr Ariberto Pereira da Cunha 333, Guaratingueta, SP, BrazilUniv Estadual Paulista, Dept Fis & Quim, Av Dr Ariberto Pereira da Cunha 333, Guaratingueta, SP, BrazilCNPq: 301073/2016-3CNPq: 304629/2015-4CNPq: 445385/2014-6Elsevier B.V.Universidade Estadual Paulista (Unesp)Silva, P. Michel L. T. da [UNESP]Souza Dutra, A. de [UNESP]Hoff da Silva, J. M. [UNESP]2018-11-26T17:42:08Z2018-11-26T17:42:08Z2017-11-10info:eu-repo/semantics/publishedVersioninfo:eu-repo/semantics/article482-488application/pdfhttp://dx.doi.org/10.1016/j.physletb.2017.06.072Physics Letters B. Amsterdam: Elsevier Science Bv, v. 774, p. 482-488, 2017.0370-2693http://hdl.handle.net/11449/16346510.1016/j.physletb.2017.06.072WOS:000414973200065WOS000414973200065.pdfWeb of Sciencereponame:Repositório Institucional da UNESPinstname:Universidade Estadual Paulista (UNESP)instacron:UNESPengPhysics Letters B2,336info:eu-repo/semantics/openAccess2024-07-01T20:52:27Zoai:repositorio.unesp.br:11449/163465Repositório InstitucionalPUBhttp://repositorio.unesp.br/oai/requestopendoar:29462024-08-05T20:00:44.093642Repositório Institucional da UNESP - Universidade Estadual Paulista (UNESP)false |
dc.title.none.fl_str_mv |
Friedmann-Lemaitre-Robertson-Walker braneworlds |
title |
Friedmann-Lemaitre-Robertson-Walker braneworlds |
spellingShingle |
Friedmann-Lemaitre-Robertson-Walker braneworlds Silva, P. Michel L. T. da [UNESP] |
title_short |
Friedmann-Lemaitre-Robertson-Walker braneworlds |
title_full |
Friedmann-Lemaitre-Robertson-Walker braneworlds |
title_fullStr |
Friedmann-Lemaitre-Robertson-Walker braneworlds |
title_full_unstemmed |
Friedmann-Lemaitre-Robertson-Walker braneworlds |
title_sort |
Friedmann-Lemaitre-Robertson-Walker braneworlds |
author |
Silva, P. Michel L. T. da [UNESP] |
author_facet |
Silva, P. Michel L. T. da [UNESP] Souza Dutra, A. de [UNESP] Hoff da Silva, J. M. [UNESP] |
author_role |
author |
author2 |
Souza Dutra, A. de [UNESP] Hoff da Silva, J. M. [UNESP] |
author2_role |
author author |
dc.contributor.none.fl_str_mv |
Universidade Estadual Paulista (Unesp) |
dc.contributor.author.fl_str_mv |
Silva, P. Michel L. T. da [UNESP] Souza Dutra, A. de [UNESP] Hoff da Silva, J. M. [UNESP] |
description |
We study the cosmological evolution with nonsingular branes generated by a bulk scalar field coupled to gravity. The specific setup investigated leads to branes with a time-dependent warp factor. We calculate the effective Hubble parameter and the effective scale factor for the FLRW branes obtained solutions. The spatially dependent branes solutions also were found. (c) 2017 The Authors. Published by Elsevier B.V. |
publishDate |
2017 |
dc.date.none.fl_str_mv |
2017-11-10 2018-11-26T17:42:08Z 2018-11-26T17:42:08Z |
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.2017.06.072 Physics Letters B. Amsterdam: Elsevier Science Bv, v. 774, p. 482-488, 2017. 0370-2693 http://hdl.handle.net/11449/163465 10.1016/j.physletb.2017.06.072 WOS:000414973200065 WOS000414973200065.pdf |
url |
http://dx.doi.org/10.1016/j.physletb.2017.06.072 http://hdl.handle.net/11449/163465 |
identifier_str_mv |
Physics Letters B. Amsterdam: Elsevier Science Bv, v. 774, p. 482-488, 2017. 0370-2693 10.1016/j.physletb.2017.06.072 WOS:000414973200065 WOS000414973200065.pdf |
dc.language.iso.fl_str_mv |
eng |
language |
eng |
dc.relation.none.fl_str_mv |
Physics Letters B 2,336 |
dc.rights.driver.fl_str_mv |
info:eu-repo/semantics/openAccess |
eu_rights_str_mv |
openAccess |
dc.format.none.fl_str_mv |
482-488 application/pdf |
dc.publisher.none.fl_str_mv |
Elsevier B.V. |
publisher.none.fl_str_mv |
Elsevier B.V. |
dc.source.none.fl_str_mv |
Web of Science 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_ |
1808129149580083200 |