Search for neutrino oscillations at the Palo Verde nuclear reactors

被引:242
|
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] Univ Alabama, Dept Phys & Astron, Tuscaloosa, AL 35487 USA
[2] Arizona State Univ, Dept Phys & Astron, Tempe, AZ 85287 USA
[3] CALTECH, Div Phys Math & Astron, Pasadena, CA 91125 USA
[4] Stanford Univ, Dept Phys, Stanford, CA 94305 USA
关键词
D O I
10.1103/PhysRevLett.84.3764
中图分类号
O4 [物理学];
学科分类号
0702 ;
摘要
We report on the initial results from a measurement of the antineutrino flux and spectrum at a distance of about 800 m from the three reactors of the Pale Verde Nuclear Generating Station using a segmented gadolinium-loaded scintillation detector. We find that the antineutrino flux agrees with that predicted in the absence of oscillations excluding at 90% C.L. <(nu)over bar>(e)-<(nu)over bar>(x) oscillations with Delta m(2) > 1.12 x 10(-3) eV(2) for maximal mixing and sin(2)2 theta > 0.21 for large Delta m(2). Our results support the conclusion that the atmospheric neutrino oscillations observed by Super-Kamiokande do not involve nu(e).
引用
收藏
页码:3764 / 3767
页数:4
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