AMANDA Observations Constrain the Ultrahigh Energy Neutrino Flux
AMANDA Observations Constrain the Ultrahigh Energy Neutrino Flux
A number of experimental techniques are currently being deployed in an effort to make the first detection of ultrahigh energy cosmic neutrinos. To accomplish this goal, techniques using radio and acoustic detectors are being developed, which are optimally designed for studying neutrinos with energies in the PeV-EeV range and above. …