Up-down atmospheric neutrino flux asymmetry predictions for various neutrino oscillation scenarios

Details Up-down atmospheric neutrino flux asymmetry predictions for various neutrino oscillation scenarios Up-down atmospheric neutrino flux asymmetry predictions for various neutrino oscillation scenarios

1997-10-20

arxiv.org/abs/hep-ph/9710403v1

Phys.Lett.B421:245-249,1998

Physics

High Energy Physics

High Energy Physics - Phenomenology

6 pages, 6 figures, Latex

Scientific paper

10.1016/S0370-2693(98)00013-6

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 $\nu_{\mu} - \nu_{\tau}$ or $\nu_{\mu} - \nu_s$, (B) maximally mixed $\nu_{\mu} - \nu_e$, (C) threefold maximal mixing between $\nu_e, \nu_{\mu}$ and $\nu_{\tau}$, and (D) neutrino oscillations via Equivalence Principle or Lorentz invariance violation. We emphasise the role of different momentum cuts.

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