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Contents
- Neutrino Astronomy
- Why Neutrinos
- Why not protons?
- Photon Attenuation on IR
- Origin of Cosmic Rays
- Alternative Models Bottom up
- Milagro (TeV) Diffuse Source
- Active Galactic Nuclei
- Generic GRB Explosion Models
- Lorentz Invariance Violation
- Galactic Microquasars
- What About Dark Matter?
- Wimp Capture
- Wimp Detection
- Cosmic Neutrino Factory
- Neutrinos from Cosmic Rays
- Muon Events Measure energy by counting the number of fired PMT.
- Determining Energy
- Flavor Ratios
- Supernova Monitor
- Large Scale Neutrino Detectors
- Radio Cherenkov Detectors
- Conclusions
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