Next-generation neutrino experiments will push the limits in our understanding of
astroparticle physics in the neutrino sector to energies orders of magnitude higher than the …

Neutrinos are key to probing the deep structure of matter and the high-energy Universe. Yet,
until recently, their interactions had only been measured at laboratory energies up to about …

The flux of high-energy neutrinos passing through the Earth is attenuated due to their
interactions with matter. The interaction rate is determined by the neutrino interaction cross …

The IceCube neutrino discovery was punctuated by three showers with E ν≈ 1–2 PeV.
Interest is intense in possible fluxes at higher energies, though a deficit of E ν≈ 6 PeV …

In the past decade IceCube's observations have revealed a flux of astrophysical neutrinos
extending to 10 7 GeV. The forthcoming generation of neutrino observatories promises to …

Next generation kilometer-scale neutrino telescopes, such as ICECUBE, can test standard
model predictions for neutrino-nucleon cross sections at energies well beyond the reach of …

IceCube has observed 80 astrophysical neutrino candidates in the energy range 0.02≲ E
ν/PeV≲ 2. Deep inelastic scattering of these neutrinos with nucleons on Antarctic ice sheet …

Astrophysical and atmospheric neutrinos are important probes of the powerful accelerators
that produce cosmic rays with EeV energies. Understanding these accelerators is a key goal …

The astrophysical neutrinos discovered by IceCube have the highest detected neutrino
energies---from TeV to PeV---and likely travel the longest distances---up to a few Gpc, the …

High-energy tau neutrinos are rarely produced in atmospheric cosmic-ray showers or at
cosmic particle accelerators, but are expected to emerge during neutrino propagation over …