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The Palo Verde reactor neutrino experiment a test for long baseline neutrino oscillations

Identifieur interne : 000592 ( Main/Exploration ); précédent : 000591; suivant : 000593

The Palo Verde reactor neutrino experiment a test for long baseline neutrino oscillations

Auteurs : F. Boehm [États-Unis] ; J. Busenitz [États-Unis] ; J. Cornis [États-Unis] ; M. Dugger [États-Unis] ; G. Gratta [États-Unis] ; J. Hanson [États-Unis] ; H. Henrikson [États-Unis] ; D. Lawrence [États-Unis] ; D. Michael [États-Unis] ; L. Miller [États-Unis] ; V. M. Novikov [États-Unis] ; A. Piepke [États-Unis] ; S. Pittalwala [États-Unis] ; B. Ritchie [États-Unis] ; D. Tracy [États-Unis] ; A. Vital [États-Unis] ; J. P. Vogel [États-Unis] ; Y. F. Wang [États-Unis] ; R. Wilferd [États-Unis] ; J. Wolf [États-Unis] ; S. Young [États-Unis]

Source :

RBID : ISTEX:6CAA21124C3D1719B097335E190C450D89BCEE0E

Abstract

Our collaboration has installed a long baseline neutrino oscillation experiment at the Palo Verde Nuclear Generating Station in Arizona. 12 tons of Gd loaded liquid scintillator, in a segmented detector, are used to search for νe ↔ νx oscillations at 740 m distance to three reactors. The anti-neutrino capture on the proton serves as detection reaction. The experiment is expected to reach a sensitivity of Δm2 > 1.3 · 10−3 eV2 and sin22Θ > 0.1. Our range of sensitivity is tuned to test the νμ ↔ νe solution of the atmospheric neutrino anomaly.

Url:
DOI: 10.1016/S0920-5632(98)00413-7


Affiliations:


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Le document en format XML

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<div type="abstract" xml:lang="en">Our collaboration has installed a long baseline neutrino oscillation experiment at the Palo Verde Nuclear Generating Station in Arizona. 12 tons of Gd loaded liquid scintillator, in a segmented detector, are used to search for νe ↔ νx oscillations at 740 m distance to three reactors. The anti-neutrino capture on the proton serves as detection reaction. The experiment is expected to reach a sensitivity of Δm2 > 1.3 · 10−3 eV2 and sin22Θ > 0.1. Our range of sensitivity is tuned to test the νμ ↔ νe solution of the atmospheric neutrino anomaly.</div>
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