dc.contributorUniversidade Estadual Paulista (Unesp)
dc.date.accessioned2014-05-20T14:07:21Z
dc.date.available2014-05-20T14:07:21Z
dc.date.created2014-05-20T14:07:21Z
dc.date.issued2000-08-01
dc.identifierGeneral Relativity and Gravitation. New York: Kluwer Academic/plenum Publ, v. 32, n. 8, p. 1633-1637, 2000.
dc.identifier0001-7701
dc.identifierhttp://hdl.handle.net/11449/23631
dc.identifier10.1023/A:1001902706237
dc.identifierWOS:000088967400012
dc.identifier1599966126072450
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.
dc.languageeng
dc.publisherKluwer Academic/plenum Publ
dc.relationGeneral Relativity and Gravitation
dc.relation1.721
dc.relation0,598
dc.rightsAcesso aberto
dc.sourceWeb of Science
dc.subjectneutrino oscillation
dc.subjectinterference phase
dc.subjectweak field
dc.titleSome remarks on the neutrino oscillation phase in a gravitational field
dc.typeOtros


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