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Ideas for a long-baseline neutrino detector [electronic resource].

Published
Washington, D.C. : United States. Dept. of Energy, 1992.
Oak Ridge, Tenn. : Distributed by the Office of Scientific and Technical Information, U.S. Dept. of Energy.
Physical Description
12 pages : digital, PDF file
Additional Creators
Fermi National Accelerator Laboratory, United States. Department of Energy, and United States. Department of Energy. Office of Scientific and Technical Information
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Summary
The Atmospheric Neutrino Deficit defines a region in Δm²-sin²2θ 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% 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.
Report Numbers
E 1.99:fnal/c--92/63
E 1.99: conf-9111141--5
conf-9111141--5
fnal/c--92/63
Subject(s)
Other Subject(s)
Note
Published through SciTech Connect.
02/01/1992.
"fnal/c--92/63"
" conf-9111141--5"
"DE92010650"
Workshop on long-baseline neutrino oscillations,Batavia, IL (United States),17-20 Nov 1991.
Bernstein, R.
Funding Information
AC02-76CH03000
View MARC record | catkey: 14400369