A Xenon Solar Neutrino Detector
A. Sh. Georgadze, H. V. Klapdor-Kleingrothaus, H. Päs, Yu. G. Zdesenko
Abstract
The neutrino capture by 131Xe with a threshold at 352 keV as reaction to detect solar neutrinos is examined. The most important feature of this process is its high sensitivity to beryllium neutrinos, which contribute approximately 40% to the total capture rate (45 SNU) assuming the fluxes predicted by the Standard Solar Model.
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