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- W3100782425 abstract "We perform a fit to the full data set corresponding to 33.3 kt-yr of data of the Super-Kamiokande experiment as well as to all other experiments in order to compare the two most likely solutions to the atmospheric neutrino anomaly in terms of oscillations in the $nu_mu to nu_tau$ and $nu_mu to nu_s$ channels. Using state-of-the-art atmospheric neutrino fluxes we have determined the allowed regions of oscillation parameters for both channels. We find that the $Delta m^2$ values for the active-sterile oscillations (both for positive and negative $Delta m^2$) are higher than for the $nu_mu to nu_tau$ case, and that the increased Super-Kamiokande sample slightly favours $nu_mu to nu_tau$ oscillations over oscillations into a sterile species $nu_s$, $nu_mu to nu_s$, and disfavours $nu_mu to nu_e$. We also give the zenith angle distributions predicted for the best fit points in each of the possible oscillation channels. Finally we compare our determinations of the atmospheric neutrino oscillation parameters with the expected sensitivities of future long-baseline experiments K2K, MINOS, ICARUS, OPERA and NOE." @default.
- W3100782425 created "2020-11-23" @default.
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- W3100782425 date "1999-03-01" @default.
- W3100782425 modified "2023-10-01" @default.
- W3100782425 title "Active-active and active-sterile neutrino oscillation solutions to the atmospheric neutrino anomaly" @default.
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- W3100782425 doi "https://doi.org/10.1016/s0550-3213(98)00834-7" @default.
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