dc.contributorUniversidade Estadual Paulista (Unesp)
dc.date.accessioned2014-05-20T14:05:40Z
dc.date.available2014-05-20T14:05:40Z
dc.date.created2014-05-20T14:05:40Z
dc.date.issued2004-05-01
dc.identifierPhysical Review D. College Pk: American Physical Soc, v. 69, n. 10, 3 p., 2004.
dc.identifier0556-2821
dc.identifierhttp://hdl.handle.net/11449/23055
dc.identifier10.1103/PhysRevD.69.107501
dc.identifierWOS:000222096200111
dc.identifierWOS000222096200111.pdf
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.
dc.languageeng
dc.publisherAmerican Physical Soc
dc.relationPhysical Review D
dc.rightsAcesso restrito
dc.sourceWeb of Science
dc.titlePhoton mass and gravitational deflection
dc.typeArtículos de revistas


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