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Please use this identifier to cite or link to this item: http://acervodigital.unesp.br/handle/11449/74987
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dc.contributor.authorBemfica, F. S.-
dc.contributor.authorDias, M.-
dc.contributor.authorGomes, M.-
dc.contributor.authorHoff da Silva, J. M.-
dc.date.accessioned2014-05-27T11:28:46Z-
dc.date.accessioned2016-10-25T18:46:30Z-
dc.date.available2014-05-27T11:28:46Z-
dc.date.available2016-10-25T18:46:30Z-
dc.date.issued2013-04-01-
dc.identifierhttp://dx.doi.org/10.1140/epjc/s10052-013-2376-z-
dc.identifier.citationEuropean Physical Journal C, v. 73, n. 4, p. 1-11, 2013.-
dc.identifier.issn1434-6044-
dc.identifier.issn1434-6052-
dc.identifier.urihttp://hdl.handle.net/11449/74987-
dc.identifier.urihttp://acervodigital.unesp.br/handle/11449/74987-
dc.description.abstractIn this work we study a Hořava-like 5-dimensional model in the context of braneworld theory. The equations of motion of such model are obtained and, within the realm of warped geometry, we show that the model is consistent if and only if λ takes its relativistic value 1. Furthermore, we show that the elimination of problematic terms involving the warp factor second order derivatives are eliminated by imposing detailed balance condition in the bulk. Afterwards, Israel's junction conditions are computed, allowing the attainment of an effective Lagrangian in the visible brane. In particular, we show that the resultant effective Lagrangian in the brane corresponds to a (3 + 1)-dimensional Hořava-like model with an emergent positive cosmological constant but without detailed balance condition. Now, restoration of detailed balance condition, at this time imposed over the brane, plays an interesting role by fitting accordingly the sign of the arbitrary constant β, insuring a positive brane tension and a real energy for the graviton within its dispersion relation. Also, the brane consistency equations are obtained and, as a result, the model admits positive brane tensions in the compactification scheme if, and only if, β is negative and the detailed balance condition is imposed. © 2013 Springer-Verlag Berlin Heidelberg and Società Italiana di Fisica.en
dc.format.extent1-11-
dc.language.isoeng-
dc.sourceScopus-
dc.titleBraneworlds scenarios in a gravity model with higher order spatial three-curvature termsen
dc.typeoutro-
dc.contributor.institutionUniversidade Federal do Rio Grande do Norte (UFRN)-
dc.contributor.institutionUniversidade de São Paulo (USP)-
dc.contributor.institutionUniversidade Federal de São Paulo (UNIFESP)-
dc.contributor.institutionUniversidade Estadual Paulista (UNESP)-
dc.description.affiliationEscola de Ciências e Tecnologia Universidade Federal do Rio Grande do Norte, Caixa Postal 1524, 59072-970 Natal, Rio Grande do Norte-
dc.description.affiliationInstituto de Física Universidade de São Paulo, Caixa Postal 66318, 05315-970 São Paulo, SP-
dc.description.affiliationDepartamento de Ciências Exatas e da Terra Universidade Federal de São Paulo, Diadema, SP-
dc.description.affiliationUNESP-Campus Guaratinguetá-DFQ, Av. Dr. Ariberto Pereira da Cunha, 333, 12516-410 Guaratinguetá, SP-
dc.description.affiliationUnespUNESP-Campus Guaratinguetá-DFQ, Av. Dr. Ariberto Pereira da Cunha, 333, 12516-410 Guaratinguetá, SP-
dc.identifier.doi10.1140/epjc/s10052-013-2376-z-
dc.identifier.wosWOS:000318292200013-
dc.rights.accessRightsAcesso restrito-
dc.relation.ispartofEuropean Physical Journal C-
dc.identifier.scopus2-s2.0-84875525902-
Appears in Collections:Artigos, TCCs, Teses e Dissertações da Unesp

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