dc.contributorUniversidade Estadual Paulista (UNESP)
dc.creatorMaluf, J. W.
dc.creatorDa Rocha-Neto, J. F.
dc.creatorToribio, T. M L
dc.creatorCastello-Branco, K. H.
dc.date2014-05-27T11:20:32Z
dc.date2016-10-25T18:18:07Z
dc.date2014-05-27T11:20:32Z
dc.date2016-10-25T18:18:07Z
dc.date2002-12-01
dc.date.accessioned2017-04-06T01:03:45Z
dc.date.available2017-04-06T01:03:45Z
dc.identifierPhysical Review D, v. 65, n. 12, 2002.
dc.identifier0556-2821
dc.identifierhttp://hdl.handle.net/11449/67048
dc.identifierhttp://acervodigital.unesp.br/handle/11449/67048
dc.identifier10.1103/PhysRevD.65.124001
dc.identifier2-s2.0-0037098343.pdf
dc.identifier2-s2.0-0037098343
dc.identifierhttp://dx.doi.org/10.1103/PhysRevD.65.124001
dc.identifier.urihttp://repositorioslatinoamericanos.uchile.cl/handle/2250/888540
dc.descriptionThe Hamiltonian formulation of the teleparallel equivalent of general relativity is considered. Definitions of energy, momentum and angular momentum of the gravitational field arise from the integral form of the constraint equations of the theory. In particular, the gravitational energy-momentum is given by the integral of scalar densities over a three-dimensional spacelike hypersurface. The definition for the gravitational energy is investigated in the context of the Kerr black hole. In the evaluation of the energy contained within the external event horizon of the Kerr black hole, we obtain a value strikingly close to the irreducible mass of the latter. The gravitational angular momentum is evaluated for the gravitational field of a thin, slowly rotating mass shell. © 2002 The American Physical Society.
dc.languageeng
dc.relationPhysical Review D
dc.rightsinfo:eu-repo/semantics/closedAccess
dc.subjectdensity
dc.subjectenergy
dc.subjectgeometry
dc.subjectgravity
dc.subjectmass
dc.subjectmathematical model
dc.subjectquantum theory
dc.subjectrotation
dc.titleEnergy and angular momentum of the gravitational field in the teleparallel geometry
dc.typeOtro


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