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arXiv · nucl-ex/9707006

A Xenon Solar Neutrino Detector

A. Sh. Georgadze·H. V. Klapdor-Kleingrothaus·H. Päs·Yu. G. Zdesenko
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Abstract

The neutrino capture by $^{131}$Xe 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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A. Sh. Georgadze, H. V. Klapdor-Kleingrothaus, H. Päs, Yu. G. Zdesenko. 1997-07-25. A Xenon Solar Neutrino Detector. https://doi.org/10.1016/s0927-6505(97)00017-0

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