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Procesy fuzji jądrowych, które zasilają Słońce energią, zachodzą w tak wysokich temperaturach, że jądra atomów są w stanie łączyć się ze sobą. W procesach tych powstaje olbrzymia liczba cząstek elementarnych zwanych neutrinami.
The Sudbury Neutrino Observatory (SNO) experiment was constructed by an international scientific collaboration primarily to provide a clear determination of whether solar neutrinos change their flavor in transit from the core of the sun to the earth. The detector used 1000 tonnes of heavy water (>99.92% D2O) in an ultra‐clean location 2 km underground in INCO's Creighton mine near Sudbury, Canada...
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