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• W2098656848 abstract "IceCube has measured a diffuse astrophysical flux of TeV–PeV neutrinos. The most plausible sources are unique high energy cosmic ray accelerators like hypernova remnants (HNRs) and remnants from gamma ray bursts in star-burst galaxies, which can produce primary cosmic rays with the required energies and abundance. In this case, however, ordinary supernova remnants (SNRs), which are far more abundant than HNRs, produce a comparable or larger neutrino flux in the ranges up to 100–150 TeV energies, implying a spectral break in the IceCube signal around these energies. The SNRs contribution in the diffuse flux up to these hundred TeV energies provides a natural baseline and then constrains the expected PeV flux." @default.
• W2098656848 created "2016-06-24" @default.
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• W2098656848 date "2015-05-01" @default.
• W2098656848 modified "2023-10-18" @default.
• W2098656848 title "Diffuse neutrinos from extragalactic supernova remnants: Dominating the 100 TeV IceCube flux" @default.
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• W2098656848 doi "https://doi.org/10.1016/j.physletb.2015.04.032" @default.
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