Up-down atmospheric neutrino flux asymmetry predictions for various neutrino oscillation scenarios
Abstract
We compute up-down asymmetries for atmospheric neutrino induced electron and muon events in the SuperKamiokande detector for the following neutrino oscillation models: (A) maximally mixed μ - τ or μ - s, (B) maximally mixed μ - e, (C) threefold maximal mixing between e, μ and τ, and (D) neutrino oscillations via Equivalence Principle or Lorentz invariance violation. We emphasise the role of different momentum cuts.
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