… For 10 2 eV neutrinos, the cross section is about 2.4 times previous estimates. We also …
sections for neutrino interactions with atomic electrons. Some consequences for interaction rates …

… energies associated with ultrahigh-energy (UHE) cosmic rays (1). Relic neutrinos that are …
her understanding of ultrahigh-energy neutrino interactions. The author thanks B. Zhou, F. …

… , and the resulting neutrino-nucleon interaction lengths. We also give a brief account of
neutrino-electron cross sections and interaction lengths. Ultrahigh-energy neutrino rates for a …

… high-energy neutrino observation. Furthermore, for ultrahigh-energy neutrino observation, we
… both Earth-emergent tau leptons and regenerated tau neutrinos. Finally, for LHC’s Forward …

… It has been suggested that ultrahigh energy neutrinos can … by neutrinos which are the only
known primaries able to travel long distances unimpeded. We have calculated the neutrino-…

… We present a calculation of the production of neutrinos during propagation of ultrahigh
energy cosmic rays, as may be produced in astrophysical sources. Photoproduction interactions …

… able to measure neutrino-… neutrino interactions below the surface is inversely proportional
to snN . This contrasts with the rate of horizontal air showers (HAS) due to neutrino interactions …

… and photons from decaying Z-bosons produced by UHE neutrinos interacting with the relic
neutrino background 45. The big drawback of this scenario is the need for enormous primary …

… The neutrino intensity arising from cosmic ray interactions with interstellar hydrogen. The …
actually escape from the source will produce neutrinos from the interaction of these protons …

… At energies in excess of 1021 eV, ultrahigh energy cosmic rays can be produced by the
interaction of ultrahigh energy neutrinos with the very cold (2 K) neutrinos which are relics of the …