Combining general relativity, massive QED and Very Long Baseline Interferometry to gravitationally constrain the photon mass

dc.contributorCentro Brasileiro de Pesquisas Físicas (CBPF)
dc.contributorUniversidade Estadual Paulista (Unesp)
dc.date.accessioned2013-09-30T18:56:19Z
dc.date.accessioned2014-05-20T14:10:47Z
dc.date.accessioned2022-10-05T15:06:46Z
dc.date.available2013-09-30T18:56:19Z
dc.date.available2014-05-20T14:10:47Z
dc.date.available2022-10-05T15:06:46Z
dc.date.created2013-09-30T18:56:19Z
dc.date.created2014-05-20T14:10:47Z
dc.date.issued2010-08-16
dc.identifierPhysics Letters A. Amsterdam: Elsevier B.V., v. 374, n. 37, p. 3806-3809, 2010.
dc.identifier0375-9601
dc.identifierhttp://hdl.handle.net/11449/24367
dc.identifier10.1016/j.physleta.2010.07.050
dc.identifierWOS:000281367900002
dc.identifier.urihttp://repositorioslatinoamericanos.uchile.cl/handle/2250/3897557
dc.description.abstractA constraint between the photon mass and the parameters gamma (the deflection parameter determined by experimentalists) and nu (the photon frequency) is found by judiciously combining General Relativity and Massive QED. By adopting this scenario and by considering as inputs the most recent measurements of the solar gravitational deflection of radio waves obtained by means of the Very Long Baseline Interferometry, gravitational upper bounds on the photon mass are estimated. (C) 2010 Elsevier B.V. All rights reserved.
dc.languageeng
dc.publisherElsevier B.V.
dc.relationPhysics Letters A
dc.relation1.863
dc.relation0,595
dc.rightsAcesso aberto
dc.sourceWeb of Science
dc.subjectGravitational deflection
dc.subjectMassive QED
dc.subjectPhoton mass
dc.subjectVery Long Baseline Interferometry
dc.titleCombining general relativity, massive QED and Very Long Baseline Interferometry to gravitationally constrain the photon mass
dc.typeTrabalho apresentado em evento


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