arXiv · hep-ph/0006090
Masses and Mixings from Neutrino Beams pointing to Neutrino Telescopes
Abstract
We discuss the potential to determine leading oscillation parameters, the value and the sign of Δm^2_{31}, as well as the magnitude of \sin^2 2θ_{13} using a conventional wide band neutrino beam pointing to water or ice Cherenkov neutrino detectors known as ``Neutrino Telescopes''. We find that precision measurements of Δm^2_{31} and θ_{23} are possible and that, even though it is not possible to discriminate between charges in the detector, there is a remarkably good sensitivity to the mixing angle θ_{13} and the sign of Δm^2_{31}.
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K. Dick, M. Freund, P. Huber, M. Lindner. 2000-06-09. Masses and Mixings from Neutrino Beams pointing to Neutrino Telescopes. https://doi.org/10.1016/s0550-3213(00)00512-5
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