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| Paper IPM / P / 9565 |
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| Abstract: | |||||
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We examine the feasibility of deriving neutrino mixing parameters
δ and θ13 from the cosmic neutrino flavor composition under
the assumption that the flavor ratios of the cosmic neutrinos at the source were
Fνe+F―νe:Fνμ+F―νμ: Fντ+F―ντ=1:2:0. We then examine to what extent the
deviation of the initial flavor ratio from 1:2:0 can be tested by realistic
flavor ratio measurement at neutrino telescopes taking into account various
sources of uncertainty.
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