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- W1543302280 endingPage "1065" @default.
- W1543302280 startingPage "1049" @default.
- W1543302280 abstract "The pp interactions taking place in the cosmos around us are a source of the astrophysical neutrinos of all the three flavors. In these interactions, the electron and the muon neutrinos mainly come from the production and the decay of the pi^{pm} mesons, whereas the tau neutrinos mainly come from the production and the decay of the D^{pm}_{S} mesons. We estimate the three intrinsic neutrino flavor ratios for 1 GeV < E < 10^{12} GeV in the pp interactions and found them to be 1 : 2 : 3times 10^{-5}. We study the effects of neutrino oscillations on these intrinsic ratios. We point out that the three ratios become 1 : 1 : 1 if L(pc)/E(GeV)> 10^{-10} in the presence of neutrino oscillations, where L is the distance to the astrophysical neutrino source in units of parsecs." @default.
- W1543302280 created "2016-06-24" @default.
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- W1543302280 date "2006-04-30" @default.
- W1543302280 modified "2023-10-10" @default.
- W1543302280 title "INTRINSIC AND OSCILLATED ASTROPHYSICAL NEUTRINO FLAVOR RATIOS REVISITED" @default.
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- W1543302280 doi "https://doi.org/10.1142/s021773230602038x" @default.
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