Slide 1 Peter Mészáros Pennsylvania State University Astrophysical Sources of TeV to GZK neutrinos Slide 2 Energy (eV ) Radio CMB Visible GeV -rays 1 TeV Flux 400…
Peter Mészáros Pennsylvania State University Astrophysical Sources of TeV to GZK neutrinos Energy (eV) Radio CMB Visible GeV g-rays 1 TeV Flux 400 microwave photons per…
Results from the Antarctic Muon and Neutrino Detector Array (AMANDA) **Talk prepared largely by: Doug Cowen Pennsylvania State University, [email protected] For the most…