dc.contributorUniversidade Estadual Paulista (UNESP)
dc.creatorAccioly, Antonio Jose
dc.creatorHelayel-Neto, Jose
dc.creatorScatena, Eslley
dc.date2013-09-30T18:56:19Z
dc.date2014-05-20T14:10:47Z
dc.date2016-10-25T17:22:19Z
dc.date2013-09-30T18:56:19Z
dc.date2014-05-20T14:10:47Z
dc.date2016-10-25T17:22:19Z
dc.date2010-08-16
dc.date.accessioned2017-04-05T21:57:01Z
dc.date.available2017-04-05T21:57:01Z
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.identifierhttp://acervodigital.unesp.br/handle/11449/24367
dc.identifier10.1016/j.physleta.2010.07.050
dc.identifierWOS:000281367900002
dc.identifierhttp://dx.doi.org/10.1016/j.physleta.2010.07.050
dc.identifier.urihttp://repositorioslatinoamericanos.uchile.cl/handle/2250/869341
dc.descriptionA 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.descriptionConselho Nacional de Desenvolvimento Científico e Tecnológico (CNPq)
dc.descriptionCoordenação de Aperfeiçoamento de Pessoal de Nível Superior (CAPES)
dc.languageeng
dc.publisherElsevier B.V.
dc.relationPhysics Letters A
dc.rightsinfo:eu-repo/semantics/closedAccess
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.typeOtro


Este ítem pertenece a la siguiente institución