Sensitivity to θ13 and δ in the Decaying Astrophysical Neutrino Scenario
Abstract
We have previously shown that the decay of high-energy neutrinos from distant astrophysical sources would be revealed by flavor ratios that deviate strongly from the φ_e:φ_μ:φ_τ = 1:1:1 expected from oscillations alone. Here we show that the deviations are significantly larger when the mixing angle θ13 and the CP phase δ are allowed to be nonzero. If neutrinos decay, this could allow measurement of θ13 and δ in IceCube and other near-term neutrino telescopes.
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