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Please use this identifier to cite or link to this item: http://acervodigital.unesp.br/handle/11449/23055
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dc.contributor.authorAccioly, A.-
dc.contributor.authorPaszko, R.-
dc.date.accessioned2014-05-20T14:05:40Z-
dc.date.available2014-05-20T14:05:40Z-
dc.date.issued2004-05-01-
dc.identifierhttp://dx.doi.org/10.1103/PhysRevD.69.107501-
dc.identifier.citationPhysical Review D. College Pk: American Physical Soc, v. 69, n. 10, 3 p., 2004.-
dc.identifier.issn0556-2821-
dc.identifier.urihttp://hdl.handle.net/11449/23055-
dc.description.abstractThe deflection of a massive photon by an external gravitational field is energy-dependent. Interesting enough, any massive quantum particle, no matter what its spin is, undergoes dispersive deflection in external gravitational fields. Exploiting the dispersive deflection of the quantized massive electromagnetic radiation by the gravitational field of the Sun, we find an upper bound for the photon mass.en
dc.format.extent3-
dc.language.isoeng-
dc.publisherAmerican Physical Soc-
dc.sourceWeb of Science-
dc.titlePhoton mass and gravitational deflectionen
dc.typeoutro-
dc.contributor.institutionUniversidade Estadual Paulista (UNESP)-
dc.description.affiliationUniv Estadual Paulista, Inst Fis Teor, BR-01405000 São Paulo, Brazil-
dc.description.affiliationUnespUniv Estadual Paulista, Inst Fis Teor, BR-01405000 São Paulo, Brazil-
dc.identifier.doi10.1103/PhysRevD.69.107501-
dc.identifier.wosWOS:000222096200111-
dc.rights.accessRightsAcesso restrito-
dc.identifier.fileWOS000222096200111.pdf-
dc.relation.ispartofPhysical Review D-
Appears in Collections:Artigos, TCCs, Teses e Dissertações da Unesp

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