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Detection of astrophysical tau neutrino candidates in IceCube
Journal article   Open access   Peer reviewed

Detection of astrophysical tau neutrino candidates in IceCube

IceCube Collaboration, R Abbasi, M Ackermann, J Adams, J A Aguilar, M Ahlers, M Ahrens, C Alispach, A A Alves, N M Amin, …
The European physical journal. C, Particles and fields, v 82(11), 1031
01 Nov 2022
url
https://doi.org/10.1140/epjc/s10052-022-10795-yView
Published, Version of Record (VoR)CC BY V4.0 Open

Abstract

Atomic Molecular Nuclear Nuclear & Particles Physics Particle and Plasma Physics Quantum Physics
High-energy tau neutrinos are rarely produced in atmospheric cosmic-ray showers or at cosmic particle accelerators, but are expected to emerge during neutrino propagation over cosmic distances due to flavor mixing. When high energy tau neutrinos interact inside the IceCube detector, two spatially separated energy depositions may be resolved, the first from the charged current interaction and the second from the tau lepton decay. We report a novel analysis of 7.5 years of IceCube data that identifies two candidate tau neutrinos among the 60 “High-Energy Starting Events” (HESE) collected during that period. The HESE sample offers high purity, all-sky sensitivity, and distinct observational signatures for each neutrino flavor, enabling a new measurement of the flavor composition. The measured astrophysical neutrino flavor composition is consistent with expectations, and an astrophysical tau neutrino flux is indicated at 2.8σ significance.

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Domestic collaboration
International collaboration
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Physics, Particles & Fields
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