Results from the Palo Verde neutrino oscillation experiment

F. Boehm, J. Busenitz, B. Cook, G. Gratta, H. Henrikson, J. Kornis, D. Lawrence, K. B. Lee, K. McKinny, L. Miller, V. Novikov, A. Piepke, B. Ritchie, D. Tracy, P. Vogel, Y-F. Wang, and J. Wolf
Phys. Rev. D 62, 072002 – Published 7 September 2000
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Abstract

The ν¯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 ν¯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. ν¯eν¯x oscillations were excluded at 90% C.L. for Δm2>1.12×103 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.

  • Received 16 March 2000

DOI:https://doi.org/10.1103/PhysRevD.62.072002

©2000 American Physical Society

Authors & Affiliations

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

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Vol. 62, Iss. 7 — 1 October 2000

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