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Antineutrino Spectroscopy with Large Water Čerenkov Detectors

2003/09/26 by J. F. Beacom, John F. Beacom, M. R. Vagins +1 · 2 voices · 10 citations
Physics and Astronomy · #Neutrino Physics Research #Dark Matter and Cosmic Phenomena #Astrophysics and Cosmic Phenomena

paper · pdf · doi:10.1103/physrevlett.93.171101

Abstract

We propose modifying large water \ifmmode \checkC\else \vC\fierenkov detectors by the addition of 0.2% gadolinium trichloride, which is highly soluble, newly inexpensive, and transparent in solution. Since Gd has an enormous cross section for radiative neutron capture, with \ensuremath∑E_\ensuremathγ=8 MeV, this would make neutrons visible for the first time in such detectors, allowing antineutrino tagging by the coincidence detection reaction \ensuremathνe+p\ensuremath→e++n (similarly for \ensuremathν_\ensuremathμ). Taking Super-Kamiokande as a working example, dramatic consequences for reactor neutrino measurements, first observation of the diffuse supernova neutrino background, galactic supernova detection, and other topics are discussed.

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