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• W3105382275 abstract "We discuss the spectrum of the different components in the astrophysical neutrino flux reaching the Earth, and the possible contribution of each component to the high-energy IceCube data. We show that the diffuse flux from cosmic ray (CR) interactions with gas in our galaxy implies just two events among the 54-event sample. We argue that the neutrino flux from CR interactions in the intergalactic (intracluster) space depends critically on the transport parameter δ describing the energy dependence in the diffusion coefficient of galactic CRs. Our analysis motivates a neutrino spectrum with a drop at PeV energies that fits the data well, including the non-observation of the Glashow resonance at 6.3 PeV. We also show that a CR flux described by an unbroken power law may produce a neutrino flux with interesting spectral features (bumps and breaks) related to changes in the CR composition." @default.
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• W3105382275 date "2018-01-05" @default.
• W3105382275 modified "2023-10-15" @default.
• W3105382275 title "Origin of the High-energy Neutrino Flux at IceCube" @default.
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• W3105382275 doi "https://doi.org/10.3847/1538-4357/aa9d94" @default.
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