Solution for a local straight cosmic string in the braneworld gravity
Autor(a) principal: | |
---|---|
Data de Publicação: | 2015 |
Outros Autores: | , |
Tipo de documento: | Artigo |
Idioma: | eng |
Título da fonte: | Repositório Institucional da UNESP |
Texto Completo: | http://dx.doi.org/10.1140/epjc/s10052-015-3669-1 http://hdl.handle.net/11449/172097 |
Resumo: | In this work we deal with the spacetime shaped by a straight cosmic string, emerging from local gauge theories, in the braneworld gravity context. We search for physical consequences of string features due to the modified gravitational scenario encoded in the projected gravitational equations. It is shown that cosmic strings in braneworld gravity may present significant differences when compared to the general relativity predictions, since its linear density is modified and the deficit angle produced by the cosmic string is attenuated. Furthermore, the existence of cosmic strings in that scenario requires a strong restriction to the braneworld tension: $$\lambda \ge 3 \times 10^{-17}$$λ≥3×<sup>10-17</sup>, in Planck units. |
id |
UNSP_edebde60e5568434ca09638c6d19fa38 |
---|---|
oai_identifier_str |
oai:repositorio.unesp.br:11449/172097 |
network_acronym_str |
UNSP |
network_name_str |
Repositório Institucional da UNESP |
repository_id_str |
2946 |
spelling |
Solution for a local straight cosmic string in the braneworld gravityIn this work we deal with the spacetime shaped by a straight cosmic string, emerging from local gauge theories, in the braneworld gravity context. We search for physical consequences of string features due to the modified gravitational scenario encoded in the projected gravitational equations. It is shown that cosmic strings in braneworld gravity may present significant differences when compared to the general relativity predictions, since its linear density is modified and the deficit angle produced by the cosmic string is attenuated. Furthermore, the existence of cosmic strings in that scenario requires a strong restriction to the braneworld tension: $$\lambda \ge 3 \times 10^{-17}$$λ≥3×<sup>10-17</sup>, in Planck units.Coordenação de Aperfeiçoamento de Pessoal de Nível Superior (CAPES)Conselho Nacional de Desenvolvimento Científico e Tecnológico (CNPq)Instituto de Física Teórica, UNESP, Universidade Estadual Paulista, Rua Dr. Bento Teobaldo Ferraz 271, Bloco II, Barra-Funda, Caixa Postal 70532-2Departamento de Física e Química, UNESP, Universidade Estadual Paulista, Av. Dr. Ariberto Pereira da Cunha, 333Instituto de Física Teórica, UNESP, Universidade Estadual Paulista, Rua Dr. Bento Teobaldo Ferraz 271, Bloco II, Barra-Funda, Caixa Postal 70532-2Departamento de Física e Química, UNESP, Universidade Estadual Paulista, Av. Dr. Ariberto Pereira da Cunha, 333CNPq: 308623/2012-6CNPq: 482043/2011-3Universidade Estadual Paulista (Unesp)Abdalla, M. C.B. [UNESP]Carlesso, P. F. [UNESP]Hoff da Silva, J. M. [UNESP]2018-12-11T16:58:39Z2018-12-11T16:58:39Z2015-09-29info:eu-repo/semantics/publishedVersioninfo:eu-repo/semantics/articleapplication/pdfhttp://dx.doi.org/10.1140/epjc/s10052-015-3669-1European Physical Journal C, v. 75, n. 9, 2015.1434-60521434-6044http://hdl.handle.net/11449/17209710.1140/epjc/s10052-015-3669-12-s2.0-849423088632-s2.0-84942308863.pdfScopusreponame:Repositório Institucional da UNESPinstname:Universidade Estadual Paulista (UNESP)instacron:UNESPengEuropean Physical Journal C2,0222,022info:eu-repo/semantics/openAccess2023-10-31T06:10:11Zoai:repositorio.unesp.br:11449/172097Repositório InstitucionalPUBhttp://repositorio.unesp.br/oai/requestopendoar:29462024-08-05T16:31:56.634439Repositório Institucional da UNESP - Universidade Estadual Paulista (UNESP)false |
dc.title.none.fl_str_mv |
Solution for a local straight cosmic string in the braneworld gravity |
title |
Solution for a local straight cosmic string in the braneworld gravity |
spellingShingle |
Solution for a local straight cosmic string in the braneworld gravity Abdalla, M. C.B. [UNESP] |
title_short |
Solution for a local straight cosmic string in the braneworld gravity |
title_full |
Solution for a local straight cosmic string in the braneworld gravity |
title_fullStr |
Solution for a local straight cosmic string in the braneworld gravity |
title_full_unstemmed |
Solution for a local straight cosmic string in the braneworld gravity |
title_sort |
Solution for a local straight cosmic string in the braneworld gravity |
author |
Abdalla, M. C.B. [UNESP] |
author_facet |
Abdalla, M. C.B. [UNESP] Carlesso, P. F. [UNESP] Hoff da Silva, J. M. [UNESP] |
author_role |
author |
author2 |
Carlesso, P. F. [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 |
Abdalla, M. C.B. [UNESP] Carlesso, P. F. [UNESP] Hoff da Silva, J. M. [UNESP] |
description |
In this work we deal with the spacetime shaped by a straight cosmic string, emerging from local gauge theories, in the braneworld gravity context. We search for physical consequences of string features due to the modified gravitational scenario encoded in the projected gravitational equations. It is shown that cosmic strings in braneworld gravity may present significant differences when compared to the general relativity predictions, since its linear density is modified and the deficit angle produced by the cosmic string is attenuated. Furthermore, the existence of cosmic strings in that scenario requires a strong restriction to the braneworld tension: $$\lambda \ge 3 \times 10^{-17}$$λ≥3×<sup>10-17</sup>, in Planck units. |
publishDate |
2015 |
dc.date.none.fl_str_mv |
2015-09-29 2018-12-11T16:58:39Z 2018-12-11T16:58:39Z |
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/10.1140/epjc/s10052-015-3669-1 European Physical Journal C, v. 75, n. 9, 2015. 1434-6052 1434-6044 http://hdl.handle.net/11449/172097 10.1140/epjc/s10052-015-3669-1 2-s2.0-84942308863 2-s2.0-84942308863.pdf |
url |
http://dx.doi.org/10.1140/epjc/s10052-015-3669-1 http://hdl.handle.net/11449/172097 |
identifier_str_mv |
European Physical Journal C, v. 75, n. 9, 2015. 1434-6052 1434-6044 10.1140/epjc/s10052-015-3669-1 2-s2.0-84942308863 2-s2.0-84942308863.pdf |
dc.language.iso.fl_str_mv |
eng |
language |
eng |
dc.relation.none.fl_str_mv |
European Physical Journal C 2,022 2,022 |
dc.rights.driver.fl_str_mv |
info:eu-repo/semantics/openAccess |
eu_rights_str_mv |
openAccess |
dc.format.none.fl_str_mv |
application/pdf |
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_ |
1808128667498315776 |