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Supernova model discrimination
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Classroom Contents
Status of the Hyper-K Experiment - Michael Smy (UCI)
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- 1 Intro
- 2 What is HyperK
- 3 Collaboration picture
- 4 Groundbreaking ceremony
- 5 Schedule
- 6 PMD Production
- 7 First 300 PMTs
- 8 MultiPMT Modules
- 9 Photo Sensor Configuration
- 10 Trusted B Monitor
- 11 ND 280
- 12 HyperK Physics Signals
- 13 Neutrinos
- 14 Octant
- 15 Atmospheric neutrino
- 16 HyperK
- 17 Supernova neutrinos
- 18 Supernova model discrimination
- 19 Matrix plot of likelihood ratios
- 20 Diffuse flux
- 21 Solar neutrino observations
- 22 Solar neutrino interactions
- 23 Hep neutrino
- 24 US contributions
- 25 How does it work
- 26 Cosmogenic radioactivity
- 27 Superplay
- 28 Conclusion
- 29 What makes the biggest effect
- 30 Uncertainty
- 31 Interaction rate
- 32 Beam delivery
- 33 Excavation schedule
- 34 Pileup of supernova neutrino events
