This final article about the CHOOZ experiment presents a complete description of the νe source and detector, the calibration methods and stability checks, the event reconstruction procedures and the Monte Carlo simulation. The data analysis, systematic effects and the methods used to reach our conclusions are fully discussed. Some new remarks are presented on the deduction of the confidence limits and on the correct treatment of systematic errors.
Initial results are presented from CHOOZ 1 , a long-baseline reactor-neutrino vacuum-oscillation experiment. The data reported here were taken during the period March to October 1997, when the two reactors ran at combined power levels varying from zero to values approaching their full rated power of 8.5 GW (thermal). Electron antineutrinos from the reactors were detected by a liquid scintillation calorimeter located at a distance of about 1 km. The detector was constructed in a tunnel protected from cosmic rays by a 300 MWE rock overburden. This massive shielding strongly reduced potentially troublesome backgrounds due to cosmic-ray muons, leading to a background rate of about one event per day, more than an order of magnitude smaller than the observed neutrino signal. From the statistical agreement between detected and expected neutrino event rates, we find (at 90% confidence level) no evidence for neutrino oscillations in the ν e disappearance mode for the parameter region given approximately by ∆m 2 > 0.9 10 −3 eV 2 for maximum mixing and sin 2 2θ > 0.18 for large ∆m 2 .1 The CHOOZ experiment is named after the new nuclear power station operated byÉlectricité de France (EdF) near the village of Chooz in the Ardennes region of France.
We present new results based on the entire CHOOZ 1 data sample. We find (at 90 % confidence level) no evidence for neutrino oscillations in thē ν e disappearance mode, for the parameter region given by approximately δm 2 > 7 · 10 −4 eV 2 for maximum mixing, and sin 2 2θ = 0.10 for large δm 2 . Lower sensitivity results, based only on the comparison of the positron spectra from the two different-distance nuclear reactors, are also presented; these are independent of the absolute normalization of theν e flux, the cross section, the number of target protons and the detector efficiencies.
The CHOOZ experiment has measured the antineutrino flux at about 1 km from two nuclear reactors to search for possible e → x oscillations with mass-squared differences as low as 10 Ϫ3 eV 2 for full mixing. We show that the analysis of the ϳ2700 e events, collected by our liquid scintillation detector, locates the antineutrino source within a cone of half-aperture Ϸ18°at the 68 % C.L. We discuss the implications of this result for locating a supernova explosion.PACS number͑s͒: 13.15.ϩg, 14.60.Pq, 28.20.Gd, 95.85.Ry
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