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• W2045474745 abstract "or more than 30 years, experiments have detected neutrinos produced in the thermonuclear fusion reactions which power the Sun. These reactions fuse protons into helium and release neu­ trinos with an energy of up to 15 MeY. Data from these solar neutrino experiments were found to be incompatible with the predictions of solar models. More precisely, the flux of neutrinos detected on Earth was less than expected, and the relative intensi­ ties of the sources of neutrinos in the sun was incompatible with those predicted by solar models. By the mid-1990's the data were beginning to suggest that one could not even in principle adjust solar models sufficiently to account for the effects. Novel proper­ ties of neutrinos seemed to be called for. With the recent measurements of the Sudbury Neutrino Observatory (SNO), it has finally become possible to test the solar model predictions and the particle properties of neutrinos independently. Solar models that simulate the interior of the Sun and explain stellar evolution have been developed using experimental and theoretical inputs from nuclear physics, astrophysics, and particle physics. These models are based on the assumption of light ele­ ment fusion in the Sun. As more and more astrophysical data have become available, solar models were tested through a variety of observables and found to be successful in many respects. A variety of hypotheses that require new particle physics have been postulated to explain the discrepancy between the solar model expectations and the apparent deficit of solar neutrinos detected on Earth. In the Standard Model, neutrinos belong to the family ofleptons. Neutrinos were believed to be massless particles with three distinct flavors (electron, muon, and tau) depending on the weak interaction process that created them. One flavor could not transform into another. All three types of neutrinos SNO" @default.
• W2045474745 created "2016-06-24" @default.
• W2045474745 creator A5045015534 @default.
• W2045474745 date "2001-09-01" @default.
• W2045474745 modified "2023-09-25" @default.
• W2045474745 title "Resolving the solar neutrino problem: Evidence for massive neutrinos in the Sudbury Neutrino Observatory" @default.
• W2045474745 doi "https://doi.org/10.1051/epn:2001506" @default.
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