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Please use this identifier to cite or link to this item: http://acervodigital.unesp.br/handle/11449/23878
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dc.contributor.authorPereira, J. G.-
dc.contributor.authorVargas, T.-
dc.contributor.authorZhang, C. M.-
dc.date.accessioned2014-05-20T14:08:05Z-
dc.date.accessioned2016-10-25T17:13:42Z-
dc.date.available2014-05-20T14:08:05Z-
dc.date.available2016-10-25T17:13:42Z-
dc.date.issued2001-03-07-
dc.identifierhttp://dx.doi.org/10.1088/0264-9381/18/5/306-
dc.identifier.citationClassical and Quantum Gravity. Bristol: Iop Publishing Ltd, v. 18, n. 5, p. 833-841, 2001.-
dc.identifier.issn0264-9381-
dc.identifier.urihttp://hdl.handle.net/11449/23878-
dc.identifier.urihttp://acervodigital.unesp.br/handle/11449/23878-
dc.description.abstractIn the context of the teleparallel equivalent of general relativity, we obtain the tetrad and the torsion fields of the stationary axisymmetric Kerr spacetime. It is shown that, in the slow rotation and weak-field approximations, the axial-vector torsion plays the role of the gravitomagnetic component of the gravitational field, and is thus responsible for the Lense-Thirring effect.en
dc.format.extent833-841-
dc.language.isoeng-
dc.publisherIop Publishing Ltd-
dc.sourceWeb of Science-
dc.titleAxial-vector torsion and the teleparallel Kerr spacetimeen
dc.typeoutro-
dc.contributor.institutionUniversidade Estadual Paulista (UNESP)-
dc.description.affiliationUniv Estadual Paulista, Inst Fis Teor, BR-01405900 São Paulo, Brazil-
dc.description.affiliationUnespUniv Estadual Paulista, Inst Fis Teor, BR-01405900 São Paulo, Brazil-
dc.identifier.doi10.1088/0264-9381/18/5/306-
dc.identifier.wosWOS:000167882000007-
dc.rights.accessRightsAcesso restrito-
dc.relation.ispartofClassical and Quantum Gravity-
Appears in Collections:Artigos, TCCs, Teses e Dissertações da Unesp

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