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Phys. Rev. D 62, 072002 (2000) [18 pages]

Results from the Palo Verde neutrino oscillation experiment

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F. Boehm3, J. Busenitz1, B. Cook3, G. Gratta4, H. Henrikson3, J. Kornis1, D. Lawrence2, K. B. Lee3, K. McKinny1, L. Miller4, V. Novikov3, A. Piepke1,3, B. Ritchie2, D. Tracy4, P. Vogel3, Y-F. Wang4, and J. Wolf1
1Department of Physics and Astronomy, University of Alabama, Tuscaloosa, Alabama 35487
2Department of Physics and Astronomy, Arizona State University, Tempe, Arizona 85287
3Division of Physics, Mathematics and Astronomy, Caltech, Pasadena, California 91125
4Physics Department, Stanford University, Stanford, California 94305

Received 16 March 2000; published 7 September 2000

The ν̅ e flux and spectrum have been measured at a distance of about 800 m from the reactors of the Palo Verde Nuclear Generating Station using a segmented Gd-loaded liquid scintillator detector. Correlated positron-neutron events from the reaction ν̅ epe+n were recorded for a period of 200 d including 55 d with one of the three reactors off for refueling. Backgrounds were accounted for by making use of the reactor-on and reactor-off cycles, and also with a novel technique based on the difference between signal and background under reversal of the e+ and n portions of the events. A detailed description of the detector calibration, background subtraction, and data analysis is presented here. Results from the experiment show no evidence for neutrino oscillations. ν̅ eν̅ x oscillations were excluded at 90% C.L. for Δm2>1.12×10-3 eV2 for full mixing and sin22θ>0.21 for large Δm2. These results support the conclusion that the observed atmospheric neutrino oscillations do not involve νe.

© 2000 The American Physical Society

URL:
http://link.aps.org/doi/10.1103/PhysRevD.62.072002
DOI:
10.1103/PhysRevD.62.072002
PACS:
13.15.+g, 14.60.Lm, 14.60.Pq