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If you have a question about this talk, please contact John Marshall. The continuously surprising and peculiar nature of neutrinos and the weak interaction have been a source of puzzlement since they were first discovered. In recent years, a remarkable paradigm has emerged that seeks to explain hidden symmetries, the scale of neutrino masses and the reason for the imbalance between matter and antimatter in the universe. A cornerstone of this includes the notion that the physical neutrinos we see are their own antiparticles. A pioneering new approach to searching for this rare process involves a novel use of the SNO detector in Canada as part of the SNO programme, which has a large UK involvement. In addition, the unique nature of the SNO instrument will allow for the study a remarkable variety of other physics as well. These include the ability to perform precision measurements of solar neutrinos at the transition between matter and vacuum-dominated oscillations to critically test fundamental neutrino couplings; making the first measurement of neutrinos from the CNO cycle to solve the “Solar Composition Problem”; the study of geo-neutrinos, reactor neutrinos and potential supernova neutrinos; and will even provide the most sensitive search for “invisible” modes of nucleon decay. This talk is part of the Cavendish HEP Seminars series. This talk is included in these lists:
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