.PNG){kind=link}
.PNG){kind=link}
.PNG){kind=link}
.PNG){kind=link}
.PNG){kind=link}
.PNG){kind=link}
.PNG){kind=link}
.PNG){kind=link}
.PNG){kind=link}
.PNG){kind=link}
.PNG){kind=link}
.PNG){kind=link}
.PNG){kind=link}
.PNG){kind=link}
.PNG){kind=link}
.PNG){kind=link}
.PNG){kind=link}
.PNG){kind=link}
.PNG){kind=link}
.PNG){kind=link}
.PNG){kind=link}
.PNG){kind=link}
.PNG){kind=link}
.PNG){kind=link}
.PNG){kind=link}
.PNG){kind=link}
.PNG){kind=link}
.PNG){kind=link}
.PNG){kind=link}
.PNG){kind=link}
.PNG){kind=link}
.PNG){kind=link}
.PNG){kind=link}
.PNG){kind=link}
.PNG){kind=link}
.PNG){kind=link}
.PNG){kind=link}
.PNG){kind=link}
.PNG){kind=link}
.PNG){kind=link}
.PNG){kind=link}
.PNG){kind=link}
.PNG){kind=link}
.PNG){kind=link}
.PNG){kind=link}
.PNG){kind=link}
.PNG){kind=link}
.PNG){kind=link}
.PNG){kind=link}
.PNG){kind=link}
.PNG){kind=link}
.PNG){kind=link}
.PNG){kind=link}
.PNG){kind=link}
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
Last added presentations
- Space Radiation
- Magnetic field uses sound waves to ignite sun's ring of fire
- Solar Thermal Energy
- Sensory and Motor Mechanisms
- Direct heat utilization of geothermal energy
- The Effects of Radiation on Living Things
- Radioactivity and Nuclear Reactions
© 2010-2024 powerpoint presentations