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American Physical Society, Physical Review D, Particles and fields, 1(61), 1999

DOI: 10.1103/physrevd.61.012001

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Determination of neutrino incoming direction in the CHOOZ experiment and its application to Supernova explosion location by scintillator detectors

This paper is available in a repository.
This paper is available in a repository.

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Data provided by SHERPA/RoMEO

Abstract

The CHOOZ experiment has measured the antineutrino flux at about 1 km from two nuclear reactors to search for possible ν̅ e→ν̅ x oscillations with mass-squared differences as low as 10-3 eV2 for full mixing. We show that the analysis of the ∼2700 ν̅ e events, collected by our liquid scintillation detector, locates the antineutrino source within a cone of half-aperture ≈18° at the 68% C.L. We discuss the implications of this result for locating a supernova explosion.