Tau neutrinos in IceCube, KM3NeT and the Pierre Auger Observatory

Daan van Eijk

SciPost Phys. Proc. 1, 030 (2019) · published 20 February 2019

Proceedings event

The 15th International Workshop on Tau Lepton Physics

Abstract

In 2018, the IceCube collaboration reported evidence for the identification of a blazar as an astrophysical neutrino source. That evidence is briefly summarised here before focusing on the prospects of tau neutrino physics in IceCube, both at high energies (astrophysical neutrinos) and at lower energies (atmospheric neutrino oscillations). In addition, future neutrino detectors such as KM3NeT and the IceCube Upgrade and their tau neutrino physics potential are discussed. Finally, the detection mechanism for high-energy (tau) neutrinos in the Pierre Auger Observatory and the resulting flux upper limits are presented.


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