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Atmospheric neutrinos and nu mass hierarchy

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Atmospheric neutrinos and nu mass hierarchy

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dc.contributor.author Palomares Ruiz, Sergio
dc.contributor.author Bernabeu Alberola, José
dc.date.accessioned 2016-05-04T08:22:03Z
dc.date.available 2016-05-04T08:22:03Z
dc.date.issued 2005
dc.identifier.citation Palomares Ruiz, Sergio; Bernabeu Alberola, José (2005) Atmospheric neutrinos and nu mass hierarchy Nuclear Physics B-Proceedings Supplements 138 398 401
dc.identifier.uri http://hdl.handle.net/10550/53367
dc.description.abstract We discuss the possibility for matter effects in the three-neutrino oscillations of the atmospheric nu_e (bar{nu}_e) and nu_mu (bar{nu}_mu), driven by one neutrino mass squared difference, |Delta m2_{31}| >> Delta m2_{21}, to be observable under appropriate conditions. We derive predictions for the Nadir angle (theta_n) dependence of the ratio N_mu/N_e of the rates of the mu-like and e-like multi-GeV events which is particularly sensitive to the Earth matter effects in the atmospheric neutrino oscillations, and thus to the values of sin2{theta_{13}} and sin2{theta_{23}}, and also to the type of neutrino mass spectrum.
dc.language.iso eng
dc.relation.ispartof Nuclear Physics B-Proceedings Supplements, 2005, vol. 138, p. 398-401
dc.title Atmospheric neutrinos and nu mass hierarchy
dc.type journal article es_ES
dc.date.updated 2016-05-04T08:22:03Z
dc.identifier.doi 10.1016/j.nuclphysbps.2004.11.089
dc.identifier.idgrec 069008
dc.rights.accessRights open access es_ES

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