Gravitational Energy-Momentum Density in Teleparallel Gravity

dc.contributorUniversidade Estadual Paulista (Unesp)
dc.date.accessioned2014-05-27T11:19:54Z
dc.date.available2014-05-27T11:19:54Z
dc.date.created2014-05-27T11:19:54Z
dc.date.issued2000-05-15
dc.identifierPhysical Review Letters, v. 84, n. 20, p. 4533-4536, 2000.
dc.identifier0031-9007
dc.identifierhttp://hdl.handle.net/11449/66159
dc.identifier10.1103/PhysRevLett.84.4533
dc.identifierWOS:000086997100005
dc.identifier2-s2.0-0001285465
dc.identifier2-s2.0-0001285465.pdf
dc.identifier1599966126072450
dc.description.abstractIn the context of a gauge theory for the translation group, a conserved energy-momentum gauge current for the gravitational field is obtained. It is a true spacetime and gauge tensor, and transforms covariantly under global Lorentz transformations. By rewriting the gauge gravitational field equation in a purely spacetime form, it becomes the teleparallel equivalent of Einstein's equation, and the gauge current reduces to the Møller's canonical energy-momentum density of the gravitational field.
dc.languageeng
dc.relationPhysical Review Letters
dc.relation8.839
dc.relation3,622
dc.rightsAcesso aberto
dc.sourceScopus
dc.titleGravitational Energy-Momentum Density in Teleparallel Gravity
dc.typeArtículos de revistas


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