IceCube (2013+) detects astrophysical neutrinos at TeV-PeV energies via Cherenkov light from secondary muons (tracks) and electromagnetic/hadronic cascades in 1 km³ of Antarctic ice. Diffuse astrophysical flux (isotropic component above…
IceCube (2013+) detects astrophysical neutrinos at TeV-PeV energies via Cherenkov light from secondary muons (tracks) and electromagnetic/hadronic cascades in 1 km³ of Antarctic ice. Diffuse astrophysical flux (isotropic component above…