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Characterization of the Three-Flavor Composition of Cosmic Neutrinos with IceCube

2025/10/28 by Abbasi, R., Ackermann, M., Adams, J. +429 · 2 citations
#FOS: Physical sciences #High Energy Astrophysical Phenomena (astro-ph.HE) #High Energy Physics - Experiment (hep-ex) #High Energy Physics - Phenomenology (hep-ph)

paper · doi:10.48550/arxiv.2510.24957

Abstract

Neutrinos oscillate over cosmic distances. Using 11.4 years of IceCube data, the flavor composition of the all-sky neutrino flux from 5 TeV--10 PeV is studied. We report the first measurement down to the O(TeV) scale using events classified into three flavor-dependent morphologies. The best fit flavor ratio is fe:fμ:fτ = 0.30:0.37:0.33, consistent with the standard three-flavor neutrino oscillation model. Each fraction is constrained to be >0 at > 90% confidence level, assuming a broken power law for cosmic neutrinos. We infer the flavor composition of cosmic neutrinos at their sources, and find production via neutron decay lies outside the 99% confidence interval.

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