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2014

IceCube events and decaying dark matter: hints and constraints

Esmaili, Arman, Kang, Sin Kyu, Serpico, Pasquale Dario

Understand

In the light of the new IceCube data on the (yet unidentified) astrophysical neutrino flux in the PeV and sub-PeV range, we present an update on the status of decaying dark matter interpretation of the events.

In particular, we develop further the angular distribution analysis and discuss the perspectives for diagnostics.
By performing various statistical tests (maximum likelihood, Kolmogorov-Smirnov and Anderson-Darling tests) we conclude that currently the data show a mild preference (below the two sigma level) for the angular distribution expected from dark matter decay vs.
the isotropic distribution foreseen for a conventional astrophysical flux of extragalactic origin.