Five-dimensional f(R) braneworld models
Autor(a) principal: | |
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Data de Publicação: | 2011 |
Outros Autores: | |
Tipo de documento: | Artigo |
Idioma: | eng |
Título da fonte: | Repositório Institucional da UNESP |
Texto Completo: | http://dx.doi.org/10.1103/PhysRevD.84.066011 http://hdl.handle.net/11449/226556 |
Resumo: | After incorporating f(R) gravity into the general braneworld sum rules scope, it is shown that some particular class of warped five-dimensional nonlinear braneworld models, which may be interesting for the hierarchy problem solution, still require a negative tension brane. For other classes of warp factors (suitable and not suitable for approaching the hierarchy problem) any negative brane tension in the compactification scheme is not necessary. In this vein, it is argued that, in the bulk f(R) gravity context, some types of warp factors may be useful for approaching the hierarchy problem and for evading the necessity of a negative brane tension in the compactification scheme. © 2011 American Physical Society. |
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Five-dimensional f(R) braneworld modelsAfter incorporating f(R) gravity into the general braneworld sum rules scope, it is shown that some particular class of warped five-dimensional nonlinear braneworld models, which may be interesting for the hierarchy problem solution, still require a negative tension brane. For other classes of warp factors (suitable and not suitable for approaching the hierarchy problem) any negative brane tension in the compactification scheme is not necessary. In this vein, it is argued that, in the bulk f(R) gravity context, some types of warp factors may be useful for approaching the hierarchy problem and for evading the necessity of a negative brane tension in the compactification scheme. © 2011 American Physical Society.UNESP Campus de Guaratinguetá DFQ, Avenida Dr. Ariberto Pereira da Cunha, 333, CEP 12516-410, Guaratinguetá-São PauloDepartamento de Ciências Exatas e da Terra Universidade Federal de São Paulo, Diadema-São PauloUNESP Campus de Guaratinguetá DFQ, Avenida Dr. Ariberto Pereira da Cunha, 333, CEP 12516-410, Guaratinguetá-São PauloUniversidade Estadual Paulista (UNESP)Universidade Federal de São Paulo (UNIFESP)Hoff Da Silva, J. M. [UNESP]Dias, M.2022-04-29T01:14:04Z2022-04-29T01:14:04Z2011-09-30info:eu-repo/semantics/publishedVersioninfo:eu-repo/semantics/articlehttp://dx.doi.org/10.1103/PhysRevD.84.066011Physical Review D - Particles, Fields, Gravitation and Cosmology, v. 84, n. 6, 2011.1550-79981550-2368http://hdl.handle.net/11449/22655610.1103/PhysRevD.84.0660112-s2.0-80053913054Scopusreponame:Repositório Institucional da UNESPinstname:Universidade Estadual Paulista (UNESP)instacron:UNESPengPhysical Review D - Particles, Fields, Gravitation and Cosmologyinfo:eu-repo/semantics/openAccess2024-07-01T20:52:37Zoai:repositorio.unesp.br:11449/226556Repositório InstitucionalPUBhttp://repositorio.unesp.br/oai/requestopendoar:29462024-08-05T21:39:01.227156Repositório Institucional da UNESP - Universidade Estadual Paulista (UNESP)false |
dc.title.none.fl_str_mv |
Five-dimensional f(R) braneworld models |
title |
Five-dimensional f(R) braneworld models |
spellingShingle |
Five-dimensional f(R) braneworld models Hoff Da Silva, J. M. [UNESP] |
title_short |
Five-dimensional f(R) braneworld models |
title_full |
Five-dimensional f(R) braneworld models |
title_fullStr |
Five-dimensional f(R) braneworld models |
title_full_unstemmed |
Five-dimensional f(R) braneworld models |
title_sort |
Five-dimensional f(R) braneworld models |
author |
Hoff Da Silva, J. M. [UNESP] |
author_facet |
Hoff Da Silva, J. M. [UNESP] Dias, M. |
author_role |
author |
author2 |
Dias, M. |
author2_role |
author |
dc.contributor.none.fl_str_mv |
Universidade Estadual Paulista (UNESP) Universidade Federal de São Paulo (UNIFESP) |
dc.contributor.author.fl_str_mv |
Hoff Da Silva, J. M. [UNESP] Dias, M. |
description |
After incorporating f(R) gravity into the general braneworld sum rules scope, it is shown that some particular class of warped five-dimensional nonlinear braneworld models, which may be interesting for the hierarchy problem solution, still require a negative tension brane. For other classes of warp factors (suitable and not suitable for approaching the hierarchy problem) any negative brane tension in the compactification scheme is not necessary. In this vein, it is argued that, in the bulk f(R) gravity context, some types of warp factors may be useful for approaching the hierarchy problem and for evading the necessity of a negative brane tension in the compactification scheme. © 2011 American Physical Society. |
publishDate |
2011 |
dc.date.none.fl_str_mv |
2011-09-30 2022-04-29T01:14:04Z 2022-04-29T01:14:04Z |
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/10.1103/PhysRevD.84.066011 Physical Review D - Particles, Fields, Gravitation and Cosmology, v. 84, n. 6, 2011. 1550-7998 1550-2368 http://hdl.handle.net/11449/226556 10.1103/PhysRevD.84.066011 2-s2.0-80053913054 |
url |
http://dx.doi.org/10.1103/PhysRevD.84.066011 http://hdl.handle.net/11449/226556 |
identifier_str_mv |
Physical Review D - Particles, Fields, Gravitation and Cosmology, v. 84, n. 6, 2011. 1550-7998 1550-2368 10.1103/PhysRevD.84.066011 2-s2.0-80053913054 |
dc.language.iso.fl_str_mv |
eng |
language |
eng |
dc.relation.none.fl_str_mv |
Physical Review D - Particles, Fields, Gravitation and Cosmology |
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_ |
1808129343905333248 |