  In this work we present an updated study of the flavor composition suggested
by astrophysical neutrinos observed by IceCube. The main novelties compared to
previous studies are the following: 1) we use the most recent measurements,
namely 8 years of throughgoing muons and 7.5 years of High Energy Starting
Events (HESE); 2) we consider a broken power law spectrum, in order to be
consistent with the observations between 30 TeV and few PeV; 3) we use the
throughgoing muon flux to predict the number of astrophysical HESE tracks. We
show that accounting for the three previous elements, the result favors
surprisingly the hypothesis of neutrinos produced by neutron decay, disfavoring
the standard picture of neutrinos from pion decay at 2.0$\sigma$ and the damped
muons regime at $2.6 \sigma$, once the atmospheric background is considered.
Although the conventional scenario is not yet completely ruled out in the
statistically and alternative interpretations are also plausible, such as an
energy spectrum characterized by a non trivial shape, this intriguing result
may suggest new directions for both theoretical interpretation and experimental
search strategies.
