Results from the Palo Verde neutrino oscillation experiment

被引:157
作者
Boehm, F [1 ]
Busenitz, J
Cook, B
Gratta, G
Henrikson, H
Kornis, J
Lawrence, D
Lee, KB
McKinny, K
Miller, L
Novikov, V
Piepke, A
Ritchie, B
Tracy, D
Vogel, P
Wang, YF
Wolf, J
机构
[1] CALTECH, Div Phys Math & Astron, Pasadena, CA 91125 USA
[2] Arizona State Univ, Dept Phys & Astron, Tempe, AZ 85287 USA
[3] Univ Alabama, Dept Phys & Astron, Tuscaloosa, AL 35487 USA
[4] Stanford Univ, Dept Phys, Stanford, CA 94305 USA
关键词
D O I
10.1103/PhysRevD.62.072002
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The <(nu)over bar>(e) flux and spectrum have been measured at a distance of about 800 m from the reactors of the Pale Verde Nuclear Generating Station using a segmented Gd-loaded Liquid scintillator detector. Correlated positron-neutron events from the reaction <(nu)over bar>(e)p --> e(+) 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 ef 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. <(nu)over bar>(e) --><(nu)over bar>(x) oscillations were excluded at 90% C.L. for Delta m(2)>1.12x10(-3) eV(2) for full mixing and sin(2)2 theta>0.21 for large Delta m(2). These results support the conclusion that the observed atmospheric neutrino oscillations do not involve nu(e).
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页码:1 / 18
页数:18
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