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Please use this identifier to cite or link to this item: http://acervodigital.unesp.br/handle/11449/34473
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dc.contributor.authorGuzzo, M. M.-
dc.contributor.authorBellandi, J.-
dc.contributor.authorAquino, V. M.-
dc.date.accessioned2014-05-20T15:23:46Z-
dc.date.accessioned2016-10-25T17:57:45Z-
dc.date.available2014-05-20T15:23:46Z-
dc.date.available2016-10-25T17:57:45Z-
dc.date.issued1994-02-01-
dc.identifierhttp://dx.doi.org/10.1103/PhysRevD.49.1404-
dc.identifier.citationPhysical Review D. College Pk: Amer Physical Soc, v. 49, n. 3, p. 1404-1408, 1994.-
dc.identifier.issn1550-7998-
dc.identifier.urihttp://hdl.handle.net/11449/34473-
dc.identifier.urihttp://acervodigital.unesp.br/handle/11449/34473-
dc.description.abstractEmploying the Feynman procedure of ordered exponential operators and the stationary phase method to evaluate the multiple integrals involved, we calculate the level-crossing probability and analyze the role of a resonance in the evolution of a two-level neutrino system. We compare this procedure with more conventional ones, such as Landau's method and the ansatz of Kuo and Pantaleone and Petcov. We verify that our results reproduce the correct extreme nonadiabatic limit and give the standard solutions in the adiabatic regime for any arbitrary matter density distributions. We discuss in particular the case of solar neutrino propagation using the standard solar model predictions for the matter distribution in the Sun.en
dc.format.extent1404-1408-
dc.language.isoeng-
dc.publisherAmer Physical Soc-
dc.sourceWeb of Science-
dc.titleNONADIABATIC NEUTRINO OSCILLATIONS REEXAMINEDen
dc.typeoutro-
dc.contributor.institutionUniversidade Estadual Paulista (UNESP)-
dc.contributor.institutionUniversidade Estadual de Londrina (UEL)-
dc.description.affiliationUNIV ESTADUAL PAULISTA, INST FIS TEOR, BR-14501405 SAO PAULO, SP, BRAZIL-
dc.description.affiliationUNIV ESTADUAL LONDRINA, DEPT FIS, BR-86000970 LONDRINA, PARANA, BRAZIL-
dc.description.affiliationUnespUNIV ESTADUAL PAULISTA, INST FIS TEOR, BR-14501405 SAO PAULO, SP, BRAZIL-
dc.identifier.doi10.1103/PhysRevD.49.1404-
dc.identifier.wosWOS:A1994MV51900030-
dc.rights.accessRightsAcesso restrito-
dc.identifier.fileWOSA1994MV51900030.pdf-
dc.relation.ispartofPhysical Review D-
Appears in Collections:Artigos, TCCs, Teses e Dissertações da Unesp

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