Abstract
We present a formalism to study three-flavor effects in flavor conversions of dense neutrino ensembles. The main idea is to use the smallness of Δm2⊙Δm2atm and θ13. The formalism has immediate applications to neutrinos from supernovae or the early Universe. We outline some consequences for supernova neutrino phenomenology, e.g hierarchy determination at extremely small θ13.
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