A xenon solar neutrino detector.

Details A xenon solar neutrino detector. A xenon solar neutrino detector.

Jan 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999nuphs..70..354g&link_type=abstract

Nuclear Physics B - Proceedings Supplements, vol. 70, issue 1-3, pp. 354-357

Physics

Nuclear Physics

Solar Neutrinos: Detectors

Scientific paper

The neutrino capture reaction by 131Xe with the threshold of 352 keV is suggested for solar neutrinos detection. The most important feature of this process is its high sensitivity to beryllium neutrinos, that contribute approximately 40% to the total capture rate predicted in the standard solar model (45 SNU). The expected counting rate of the xenon detector from the main solar neutrino sources predicted by the standard solar model is ≡1500 events/yr.

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