6533b863fe1ef96bd12c7876

RESEARCH PRODUCT

Atmospheric neutrinos and nu mass hierarchy

Jose BernabeuSergio Palomares-ruizSergio Palomares-ruizSergio Palomares-ruiz

subject

PhysicsNuclear and High Energy PhysicsParticle physicsHigh Energy Physics::PhenomenologyFOS: Physical sciencesObservableAtomic and Molecular Physics and OpticsHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)Mass spectrumHigh Energy Physics::ExperimentAtmospheric neutrinoNeutrinoNeutrino oscillationMass hierarchy

description

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.

10.1016/j.nuclphysbps.2004.11.089http://hdl.handle.net/10550/53367