Speaker
Mr
Marco Chianese
(Università di Napoli Federico II & INFN, Sezione di Napoli)
Description
The recent study on the the 6-year up-going muon neutrinos by the IceCube Collaboration and the multi-messenger analyses support the hypothesis of a two-component scenario explaining the diffuse TeV-PeV neutrino flux. In particular, a low-energy excess in the IceCube data is shown in the energy range 10-100 TeV. A statistical analysis on the neutrino energy spectrum and on the angular distribution of neutrino arrival directions is performed in order to shed light on the origin of such excess. We characterize a two-component neutrino flux where decaying/annihilating Dark Matter particles provide a contribution to the IceCube observations.
Author
Mr
Marco Chianese
(Università di Napoli Federico II & INFN, Sezione di Napoli)