Neutrino Flavor Ratio on Earth and at Astrophysical Sources
Abstract
We present the reconstruction of neutrino flavor ratios at astrophysical sources. For distinguishing the pion source and the muon-damped source to the 3σ level, the neutrino flux ratios, Rφ(μ)/(φ(e)+φ(τ)) and Sφ(e)/φ(τ), need to be measured in accuracies better than 10%.
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