A Combined OMNIS and Neutrino Factor at WIPP

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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

Author: David Cline