Table of Contents
Title Slide
A Combined OMNIS and Neutrino Factor at WIPP
Neutrino Mass Physics
Real Time SW II Detection
Neutrino Spectrum from a SN II
Neutrino events from 1987a agrees with current SN model
Limits on Oscillation Based on SN 1987a
Detection of mu/tau From SuperNova Neutrinos in Real Time
Original Concept for SNBO from 1992
Events from a Galactic SN II
Expected events in Pb/Fe with and w/o Mixing
One Scheme (Li-loaded optical fiber) to Consider for OMNIS
Only One US Site Possible for a Neutrino Factory Detector
FNAL Feasibility Study for a muon Storage Ring
A Neutrino Factory is more of a Global Product than any Other
Non-planar bow-tie ring beams to two distant detectors
Think World-Wide Effort
UCLA Bow-Tie Storage Ring Design
Neutrino Factory 2000 (Monterey) Meeting
The Global Nature of this Project
ICANOE
ICANOE Proposal - First Beam in May, 2005
Gran Sasso Halls Point to CERN within few Degrees
One Possibility: A Combined Neutrino Factory Detector
Any Neutrino Factory will Require 10-50 KT Detector
Proposed Neutrino Factory Detector at WIPP
Progress Towards an OMNIS/SNBO Detector at WIPP
Progress Towards an OMNIS/SNBO Detector at WIPP (cont.)
Conclusions
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