A Combined Astrophysical and Dark Matter Interpretation of the IceCube HESE and Throughgoing Muon Events
Yicong Sui, P. S. Bhupal Dev

TL;DR
This paper analyzes six years of IceCube neutrino data using a two-component model involving astrophysical sources and dark matter, finding a mild preference for the combined explanation over purely astrophysical models.
Contribution
It introduces a combined astrophysical and dark matter model for IceCube neutrino data and evaluates its compatibility with gamma-ray constraints, showing it is mildly favored over pure astrophysical models.
Findings
Combined model mildly preferred over pure astrophysical explanation.
Two source flavor compositions are considered, with muon-damped slightly favored.
Model is compatible with gamma-ray constraints, unlike single-component fits.
Abstract
We perform a combined likelihood analysis for the IceCube 6-year high-energy starting events (HESE) and 8-year throughgoing muon events above 10 TeV using a two-component neutrino flux model. The two-component flux can be motivated either from purely astrophysical sources or due to a beyond Standard Model contribution, such as decaying heavy dark matter. We find that the astrophysical plus dark matter interpretation is mildly preferred by the current data over the purely astrophysical explanation. As for the astrophysical neutrinos, we consider two different source flavor compositions corresponding to the standard pion decay and muon-damped pion decay sources. We find that the latter is slightly preferred over the former as the high-energy component, while the low-energy component does not show any such preference. We also take into account the multi-messenger gamma-ray constraints and…
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