Cosmic-ray upscattering of the diffuse supernova neutrino background produces a flux about 20 orders below the galactic diffuse emission and about 18 orders below current limits, making the channel undetectable.
Connection of the virtual γ∗ p cross section of ep deep inelastic scattering to real γp scattering, and the implications for νN and ep total cross sections
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Cosmic-Ray Boosted Diffuse Supernova Neutrinos
Cosmic-ray upscattering of the diffuse supernova neutrino background produces a flux about 20 orders below the galactic diffuse emission and about 18 orders below current limits, making the channel undetectable.