You are in the accessibility menu

Please use this identifier to cite or link to this item: http://acervodigital.unesp.br/handle/11449/67318
Full metadata record
DC FieldValueLanguage
dc.contributor.authorNunokawa, H.-
dc.contributor.authorPeres, O. L G-
dc.contributor.authorZukanovich Funchal, R.-
dc.date.accessioned2014-05-27T11:20:40Z-
dc.date.accessioned2016-10-25T18:18:42Z-
dc.date.available2014-05-27T11:20:40Z-
dc.date.available2016-10-25T18:18:42Z-
dc.date.issued2003-06-12-
dc.identifierhttp://dx.doi.org/10.1016/S0370-2693(03)00603-8-
dc.identifier.citationPhysics Letters, Section B: Nuclear, Elementary Particle and High-Energy Physics, v. 562, n. 3-4, p. 279-290, 2003.-
dc.identifier.issn0370-2693-
dc.identifier.urihttp://hdl.handle.net/11449/67318-
dc.identifier.urihttp://acervodigital.unesp.br/handle/11449/67318-
dc.description.abstractWe show in this Letter that the observation of the angular distribution of upward-going muons and cascade events induced by atmospheric neutrinos at the TeV energy scale which can be performed by a kilometer-scale neutrino telescope, such as the IceCube detector, can be used to probe a large neutrino mass splitting, |Δm 2| ∼ (0.5-2.0) eV 2, implied by the LSND experiment and discriminate among four neutrino mass schemes. This is due to the fact that such a large mass scale can promote non-negligible v μ → v e, v τ/v μ → v e, v τ conversions at these energies by the MSW effect as well as vacuum oscillation, unlike what is expected if all the neutrino mass splittings are small. © 2003 Elsevier Science B.V. All rights reserved.en
dc.format.extent279-290-
dc.language.isoeng-
dc.sourceScopus-
dc.subjectatmosphere-
dc.subjectatomic particle-
dc.subjectenergy-
dc.subjectmass-
dc.subjectoscillation-
dc.subjectphysics-
dc.subjectvacuum-
dc.titleProbing the LSND mass scale and four neutrino scenarios with a neutrino telescopeen
dc.typeoutro-
dc.contributor.institutionUniversidade Estadual Paulista (UNESP)-
dc.contributor.institutionUniversity of California-
dc.contributor.institutionUniversidade Estadual de Campinas (UNICAMP)-
dc.contributor.institutionUniversidade de São Paulo (USP)-
dc.description.affiliationInstituto de Fisica Teorica Universidade Estadual Paulista, Rua Pamplona 145, 01405-900 São Paulo-
dc.description.affiliationKavli Inst. for Theoretical Physics University of California, Santa Barbara, CA 93106-
dc.description.affiliationInstituto de Fisica Gleb Wataghin Universidade Estadual de Campinas UNICAMP, 13083-970 Campinas-
dc.description.affiliationInstituto de Física Universidade de São Paulo, C.P. 66.318, 05315-970 São Paulo-
dc.description.affiliationUnespInstituto de Fisica Teorica Universidade Estadual Paulista, Rua Pamplona 145, 01405-900 São Paulo-
dc.identifier.doi10.1016/S0370-2693(03)00603-8-
dc.identifier.wosWOS:000183287600019-
dc.rights.accessRightsAcesso restrito-
dc.relation.ispartofPhysics Letters, Section B: Nuclear, Elementary Particle and High-Energy Physics-
dc.identifier.scopus2-s2.0-0037737557-
Appears in Collections:Artigos, TCCs, Teses e Dissertações da Unesp

There are no files associated with this item.
 

Items in DSpace are protected by copyright, with all rights reserved, unless otherwise indicated.