Kavli Affiliate: Shunsaku Horiuchi | Summary:The cosmic neutrino background (C$ν$B) can be boosted to high energies due to scatterings with energetic cosmic rays (CRs) across cosmological scales. Previous calculations focused on neutral current incoherent and coherent elastic scatterings of cosmic-ray protons off relic neutrinos. However, charged current interactions and deep inelastic scatterings are also expected […]
Continue.. The Cosmic Neutrino Background is within Reach of Future Neutrino Telescopes