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Please use this identifier to cite or link to this item: http://acervodigital.unesp.br/handle/11449/23836
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dc.contributor.authorCasana, R.-
dc.contributor.authorde Melo, C. A. M.-
dc.contributor.authorPimentel, B. M.-
dc.date.accessioned2014-05-20T14:07:57Z-
dc.date.accessioned2016-10-25T17:13:33Z-
dc.date.available2014-05-20T14:07:57Z-
dc.date.available2016-10-25T17:13:33Z-
dc.date.issued2006-10-01-
dc.identifierhttp://dx.doi.org/10.1007/s10509-006-9048-5-
dc.identifier.citationAstrophysics and Space Science. Dordrecht: Springer, v. 305, n. 2, p. 125-132, 2006.-
dc.identifier.issn0004-640X-
dc.identifier.urihttp://hdl.handle.net/11449/23836-
dc.identifier.urihttp://acervodigital.unesp.br/handle/11449/23836-
dc.description.abstractThe Dirac field is studied in a Lyra space-time background by means of the classical Schwinger Variational Principle. We obtain the equations of motion, establish the conservation laws, and get a scale relation relating the energy-momentum and spin tensors. Such scale relation is an intrinsic property for matter fields in Lyra background.en
dc.format.extent125-132-
dc.language.isoeng-
dc.publisherSpringer-
dc.sourceWeb of Science-
dc.subjectLyra geometrypt
dc.subjectSchwinger Variational Principlept
dc.subjectclassical fields on non-euclidean manifoldspt
dc.titleSpinorial field and Lyra geometryen
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.doi10.1007/s10509-006-9048-5-
dc.identifier.wosWOS:000242145300002-
dc.rights.accessRightsAcesso restrito-
dc.relation.ispartofAstrophysics and Space Science-
Appears in Collections:Artigos, TCCs, Teses e Dissertações da Unesp

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