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SNO (e.g. A. McDonald for the SNO Collaboration, talk presented at “Neutrino ’98, XVIII International Conference on Neutrino Physics and Astrophysics,” to appear in the proceedings), a heavy water detector, is expected to have a measurable neutral current event rate if the solar neutrino problem is solved by conversion of (Formula presented) to (Formula presented) or (Formula presented) Both Super-Kamiokande and SNO will look for deviations from the expected recoil electron spectrum, as well as anomalous seasonal or diurnal time variations
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SNO (e.g. A. McDonald for the SNO Collaboration, talk presented at “Neutrino ’98, XVIII International Conference on Neutrino Physics and Astrophysics,” to appear in the proceedings), a heavy water detector, is expected to have a measurable neutral current event rate if the solar neutrino problem is solved by conversion of (Formula presented) to (Formula presented) or (Formula presented) Both Super-Kamiokande and SNO will look for deviations from the expected recoil electron spectrum, as well as anomalous seasonal or diurnal time variations
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the status of the Super-Kamiokande data on these signals is reported in Super-Kamiokande Collaboration, Y Fukuda, Phys. Rev. Lett. 82, 2430 (1999)
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