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dc.contributor.authorPereira, J. G.-
dc.contributor.authorZhang, C. M.-
dc.date.accessioned2014-05-20T14:07:21Z-
dc.date.accessioned2016-10-25T17:12:40Z-
dc.date.available2014-05-20T14:07:21Z-
dc.date.available2016-10-25T17:12:40Z-
dc.date.issued2000-08-01-
dc.identifierhttp://dx.doi.org/10.1023/A:1001902706237-
dc.identifier.citationGeneral Relativity and Gravitation. New York: Kluwer Academic/plenum Publ, v. 32, n. 8, p. 1633-1637, 2000.-
dc.identifier.issn0001-7701-
dc.identifier.urihttp://hdl.handle.net/11449/23631-
dc.identifier.urihttp://acervodigital.unesp.br/handle/11449/23631-
dc.description.abstractThe weak gravitational field expansion method to account for the gravitationally induced neutrino oscillation effect is critically examined, then it is shown that the splitting of the neutrino phase into a kinematic and a gravitational phase is not always possible because the relativistic factor modifies the particle interference phase splitting condition in a gravitational field.en
dc.format.extent1633-1637-
dc.language.isoeng-
dc.publisherKluwer Academic/plenum Publ-
dc.sourceWeb of Science-
dc.subjectneutrino oscillationpt
dc.subjectinterference phasept
dc.subjectweak fieldpt
dc.titleSome remarks on the neutrino oscillation phase in a gravitational fielden
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.doi10.1023/A:1001902706237-
dc.identifier.wosWOS:000088967400012-
dc.rights.accessRightsAcesso restrito-
dc.relation.ispartofGeneral Relativity and Gravitation-
Appears in Collections:Artigos, TCCs, Teses e Dissertações da Unesp

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