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Monte Carlo simulation of inelastic neutrino scattering in DUMAND. [2 TeV]

Technical Report ·
DOI:https://doi.org/10.2172/5884484· OSTI ID:5884484
Detailed Monte Carlo calculations simulating the detection in the DUMAND 1-km/sup 3/ optical detector of inelastic neutrino scattering by nucleons at 2 TeV and above show that the measurement of the y distribution is subject to systematic errors due to experimental errors and intrinsic fluctuations which produce errors in the energy determinations of hadronic cascade and muon; uncertainty in the exact amount of antineutrino fraction in the cosmic-ray neutrino flux. The nature of these errors is explored, and methods for removing them from the data developed. The remaining uncertainties are those in the evaluation of the errors in energy determination, and in the antineutrino contamination. It appears that these errors, not statistical ones, will eventually govern the accuracy of the y distributions obtained. Nonetheless, the effect of the boson propagator on the y distribution is so marked that no plausible scenario can be found in which the residual errors cast doubt on whether or not the propagator effect is present.
Research Organization:
Fermi National Accelerator Lab., Batavia, IL (USA)
DOE Contract Number:
EY-76-C-02-3000
OSTI ID:
5884484
Report Number(s):
FERMILAB-CONF-78/95-EXP
Country of Publication:
United States
Language:
English