Predictions for the cosmogenic neutrino flux in light of new data from the Pierre Auger Observatory
Predictions for the cosmogenic neutrino flux in light of new data from the Pierre Auger Observatory
The Pierre Auger Observatory (PAO) has measured the spectrum and composition of the ultrahigh energy cosmic rays with unprecedented precision. We use these measurements to constrain their spectrum and composition as injected from their sources and, in turn, use these results to estimate the spectrum of cosmogenic neutrinos generated in …