Ideas for a long-baseline neutrino detector

Details Ideas for a long-baseline neutrino detector Ideas for a long-baseline neutrino detector

Feb 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992lbno.workr..17b&link_type=abstract

Presented at the Workshop on Long-Baseline Neutrino Oscillations, Batavia, IL, 17-20 Nov. 1991

Physics

Cosmic Rays, Experiment Design, Neutrinos, Radiation Detectors, Radiation Measurement, Tests, Counters, Detection, Muons, Spectrometers

Scientific paper

The Atmospheric Neutrino Deficit defines a region in (Delta)m2-sin22(theta) space which ought to be conclusively tested in a long-baseline experiment. This talk sets out a region to cover (which may change as more data is analyzed) and translates that region into an L/E. I present exclusion curves for different experiments based on their distance and their precision; I conclude that an experiment which can detect oscillations down to 1 percent located at 1200 km will cleanly test the allowed region from Kamioka and IMB. I then describe the techniques which can perform such a measurement and outline both a detector capable of performing such an experiment and some of the systematic problems we might expect.

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