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- W3103017530 endingPage "023" @default.
- W3103017530 startingPage "023" @default.
- W3103017530 abstract "Motivated by the discovery of the first high-energy astrophysical neutrino source, the blazar TXS 0506+056, we revisit the IceCube flavor ratio analysis. Assuming large statistics from identified blazars, collected in the forthcoming years by the IceCube detector and its successor IceCube-Gen2, we demonstrate that the constraints on several new physics scenarios in which the baseline dependent terms in neutrino oscillation probabilities are not averaged, can be improved. As a representative case, we consider pseudo-Dirac neutrinos while neutrino decay is also discussed." @default.
- W3103017530 created "2020-11-23" @default.
- W3103017530 creator A5002054950 @default.
- W3103017530 creator A5066580887 @default.
- W3103017530 date "2019-02-13" @default.
- W3103017530 modified "2023-09-25" @default.
- W3103017530 title "IceCube flavor ratios with identified astrophysical sources: towards improving new physics testability" @default.
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- W3103017530 doi "https://doi.org/10.1088/1475-7516/2019/02/023" @default.
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