Atmospheric neutrinos at Super-Kamiokande and parametric resonance in neutrino oscillations

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dc.creatorAkhmedov, E. Kh.
dc.creatorDighe, A.
dc.creatorLipari, P.
dc.creatorSmirnov, A. Yu.
dc.date1998-08-09
dc.date1998-10-07
dc.date.accessioned2026-07-07T10:52:52Z
dc.date.available2026-07-07T10:52:52Z
dc.descriptionWe consider the oscillations of atmospheric neutrinos in the earth in the three-neutrino scheme with a $Δm^2$ hierarchy and a small admixture of the electron neutrino in the heavy mass eigenstate characterized by the mixing angle $θ_{13}$. We show that for $Δm^2 \simeq (0.5 - 3) \times 10^{-3}$ eV$^2$ indicated by the Super-Kamiokande data and $\sin^2 2θ_{13} \aprle 0.2$, the oscillations of multi-GeV neutrinos in the subdominant $ν_μ \leftrightarrow ν_e$ mode are enhanced by the MSW and parametric resonances. The parametric resonance, which occurs when the neutrinos cross the core of the earth, dominates for $Δm^2 \simeq (1 - 2)\times 10^{-3}$ eV$^2$, $\sin^2 2θ_{13} \aprle 0.06$. The resonance matter effects lead to an observable excess of the e-like events with a specific zenith angle dependence even for small $θ_{13}$. The up-down asymmetry of the multi-GeV e-like events can reach 15% for $|\cos Θ_e| > 0.2$ and up to 30% for $|\cos Θ_e| > 0.6$, where $Θ_e$ is the zenith angle of the electron. The resonance matter effects are relevant for the interpretation of the Super-Kamiokande data.
dc.descriptionLaTex, 48 pages, 16 figures. Substantial changes; new figure added
dc.identifierhttps://arxiv.org/abs/hep-ph/9808270
dc.identifierhttp://arxiv.org/abs/hep-ph/9808270
dc.identifierNucl.Phys.B542:3-30,1999
dc.identifierdoi:10.1016/S0550-3213(98)00825-6
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/185300
dc.subjectHigh Energy Physics - Phenomenology
dc.subjectHigh Energy Physics - Experiment
dc.titleAtmospheric neutrinos at Super-Kamiokande and parametric resonance in neutrino oscillations
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