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Please use this identifier to cite or link to this item: http://acervodigital.unesp.br/handle/11449/36780
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dc.contributor.authorAccioly, A.-
dc.contributor.authorMukai, H.-
dc.date.accessioned2014-05-20T15:26:38Z-
dc.date.accessioned2016-10-25T18:01:18Z-
dc.date.available2014-05-20T15:26:38Z-
dc.date.available2016-10-25T18:01:18Z-
dc.date.issued1997-04-01-
dc.identifierhttp://en.sif.it/journals/ncb/econtents/1997/112/04/article/0-
dc.identifier.citationNuovo Cimento Della Societa Italiana Di Fisica B-general Physics Relativity Astronomy and Mathematical Physics and Methods. Bologna: Editrice Compositori Bologna, v. 112, n. 4, p. 639-643, 1997.-
dc.identifier.issn0369-3554-
dc.identifier.urihttp://hdl.handle.net/11449/36780-
dc.identifier.urihttp://acervodigital.unesp.br/handle/11449/36780-
dc.description.abstractThe recipe used to compute the symmetric energy-momentum tensor in the framework of ordinary field theory bears little resemblance to that used in the context of general relativity, if any. We show that if one stal ts fi om the field equations instead of the Lagrangian density, one obtains a unified algorithm for computing the symmetric energy-momentum tensor in the sense that it can be used for both usual field theory and general relativity.en
dc.format.extent639-643-
dc.language.isoeng-
dc.publisherEditrice Compositori Bologna-
dc.sourceWeb of Science-
dc.titleOn the dissimilarity between the algorithms for computing the symmetric energy-momentum tensor in ordinary field theory and general relativityen
dc.typeoutro-
dc.contributor.institutionUniversidade Estadual de Maringá (UEM)-
dc.contributor.institutionUniversidade Estadual Paulista (UNESP)-
dc.description.affiliationFDN UNIV ESTADUAL MARINGA,DEPT FIS,BR-87020900 MARINGA,PARANA,BRAZIL-
dc.identifier.wosWOS:A1997XC67200012-
dc.rights.accessRightsAcesso aberto-
dc.identifier.fileWOSA1997XC67200012.pdf-
dc.relation.ispartofNuovo Cimento Della Societa Italiana Di Fisica B-general Physics Relativity Astronomy and Mathematical Physics and Methods-
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