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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.relation.ispartofPhysical Review D
dc.sourceWeb of Science
dc.titlePhoton mass and gravitational deflectionen
dc.typeArtigo
dcterms.licensehttp://publish.aps.org/authors/transfer-of-copyright-agreement
dcterms.rightsHolderAmerican Physical Soc
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
unesp.campusUniversidade Estadual Paulista (UNESP), Instituto de Física Teórica (IFT), São Paulopt
dc.identifier.fileWOS000222096200111.pdf
unesp.author.lattes7513476405206824[1]
unesp.author.orcid0000-0002-8113-8890[1]
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