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Please use this identifier to cite or link to this item: http://acervodigital.unesp.br/handle/11449/117199
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dc.contributor.authorCuzinatto, R. R.-
dc.contributor.authorPompeia, P. J.-
dc.contributor.authorMontigny, M. de-
dc.contributor.authorKhanna, F. C.-
dc.contributor.authorHoff da Silva, J. M.-
dc.date.accessioned2015-03-18T15:55:30Z-
dc.date.accessioned2016-10-25T20:34:43Z-
dc.date.available2015-03-18T15:55:30Z-
dc.date.available2016-10-25T20:34:43Z-
dc.date.issued2014-08-12-
dc.identifierhttp://dx.doi.org/10.1140/epjc/s10052-014-3017-x-
dc.identifier.citationEuropean Physical Journal C. New York: Springer, v. 74, n. 8, 10 p., 2014.-
dc.identifier.issn1434-6044-
dc.identifier.urihttp://hdl.handle.net/11449/117199-
dc.identifier.urihttp://acervodigital.unesp.br/handle/11449/117199-
dc.description.abstractWe discuss a way to obtain information about higher dimensions from observations by studying a brane-based spherically symmetric solution. The three classic tests of General Relativity are analyzed in detail: the perihelion shift of the planet Mercury, the deflection of light by the Sun, and the gravitational redshift of atomic spectral lines. The braneworld version of these tests exhibits an additional parameter b related to the fifth-coordinate. This constant b can be constrained by comparison with observational data for massive and massless particles.en
dc.description.sponsorshipNatural Sciences and Engineering Research Council (NSERC) of Canada-
dc.description.sponsorshipFundação de Amparo à Pesquisa do Estado de Minas Gerais (FAPEMIG)-
dc.description.sponsorshipConselho Nacional de Desenvolvimento Científico e Tecnológico (CNPq)-
dc.format.extent10-
dc.language.isoeng-
dc.publisherSpringer-
dc.sourceWeb of Science-
dc.titleClassic tests of General Relativity described by brane-based spherically symmetric solutionsen
dc.typeoutro-
dc.contributor.institutionUniv Fed Alfenas-
dc.contributor.institutionInst Fomento & Coordenacao Ind-
dc.contributor.institutionInst Tecnol Aeronaut-
dc.contributor.institutionUniv Alberta-
dc.contributor.institutionTRIUMF-
dc.contributor.institutionUniv Victoria-
dc.contributor.institutionUniversidade Estadual Paulista (UNESP)-
dc.description.affiliationUniv Fed Alfenas, Inst Ciencia & Tecnol, BR-37715400 Pocos De Caldas, MG, Brazil-
dc.description.affiliationInst Fomento & Coordenacao Ind, Dept Ciencia & Tecnol Aeroesp, BR-12228901 Sao Jose Dos Campos, SP, Brazil-
dc.description.affiliationInst Tecnol Aeronaut, Dept Ciencia & Tecnol Aeroesp, BR-12228900 Sao Jose Dos Campos, SP, Brazil-
dc.description.affiliationUniv Alberta, Inst Theoret Phys, Edmonton, AB T6G 2J1, Canada-
dc.description.affiliationUniv Alberta, Edmonton, AB T6C 4G9, Canada-
dc.description.affiliationTRIUMF, Vancouver, BC V6T 2A3, Canada-
dc.description.affiliationUniv Victoria, Dept Phys & Astron, STN CSC, Victoria, BC V8W 2Y2, Canada-
dc.description.affiliationUniv Estadual Paulista, Dept Quim & Fis, BR-12516410 Guaratingueta, SP, Brazil-
dc.description.affiliationUnespUniv Estadual Paulista, Dept Quim & Fis, BR-12516410 Guaratingueta, SP, Brazil-
dc.identifier.doi10.1140/epjc/s10052-014-3017-x-
dc.identifier.wosWOS:000340547000001-
dc.rights.accessRightsAcesso aberto-
dc.identifier.fileWOS000340547000001.pdf-
dc.relation.ispartofEuropean Physical Journal C-
Appears in Collections:Artigos, TCCs, Teses e Dissertações da Unesp

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