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arxiv: hep-ph/0309300 · v1 · submitted 2003-09-26 · ✦ hep-ph · astro-ph· hep-ex· nucl-ex· nucl-th

GADZOOKS! Antineutrino Spectroscopy with Large Water Cerenkov Detectors

classification ✦ hep-ph astro-phhep-exnucl-exnucl-th
keywords detectorsantineutrinodetectionfirstlargeneutrinosupernovawater
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We propose modifying large water \v{C}erenkov 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 $\sum E_\gamma = 8$ MeV, this would make neutrons visible for the first time in such detectors, allowing antineutrino tagging by the coincidence detection reaction $\bar{\nu}_e + p \to e^+ + n$ (similarly for $\bar{\nu}_\mu$). 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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