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PHOTON MASS and VERY LONG BASELINE INTERFEROMETRY

dc.contributorCentro Brasileiro de Pesquisas Físicas (CBPF)
dc.contributorUniversidade Estadual Paulista (Unesp)
dc.date.accessioned2013-09-30T18:56:21Z
dc.date.accessioned2014-05-20T14:10:48Z
dc.date.available2013-09-30T18:56:21Z
dc.date.available2014-05-20T14:10:48Z
dc.date.created2013-09-30T18:56:21Z
dc.date.created2014-05-20T14:10:48Z
dc.date.issued2010-12-01
dc.identifierInternational Journal of Modern Physics D. Singapore: World Scientific Publ Co Pte Ltd, v. 19, n. 14, p. 2393-2403, 2010.
dc.identifier0218-2718
dc.identifierhttp://hdl.handle.net/11449/24374
dc.identifier10.1142/S021827181001844X
dc.identifierWOS:000286112000025
dc.description.abstractA relation between the photon mass, its frequency, nu, and the deflection parameter, gamma, determined by experimentalists (that characterizes the contribution of space curvature to gravitational deflection) is found. This amazing result allows us to conclude that the knowledge of the parameters nu and gamma is all we need to set up gravitational bounds on the photon mass. By considering as inputs the most recent measurements of the solar gravitational deflection of radio waves obtained via the Very Long Baseline Interferometry, upper bounds on the photon mass are estimated.
dc.languageeng
dc.publisherWorld Scientific Publ Co Pte Ltd
dc.relationInternational Journal of Modern Physics D
dc.relation2.171
dc.relation1,079
dc.rightsAcesso restrito
dc.sourceWeb of Science
dc.subjectGravitational deflection
dc.subjectmassive QED
dc.subjectphoton mass
dc.subjectvery long baseline interferometry
dc.titlePHOTON MASS and VERY LONG BASELINE INTERFEROMETRY
dc.typeArtículos de revistas


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