Measurement of the rate of νe+d → p+p+e− interactions produced by 8B solar neutrinos at the Sudbury Neutrino Observatory

By J. Farine. 2002

567 citations recorded by the source corpus.

Subfields: Nuclear and High Energy Physics

View Paper: https://www.semanticscholar.org/paper/df48ce0d3effdba58b91d03e3c942194f1124196

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In Nuclear and High Energy Physics

1. Stefano Gariazzo
2. C. Ternes
3. O. Mena
4. Z. Xing
5. P. F. de Salas
6. M. Tórtola
7. M. Beuthe
8. J. Marteau

Citations in the corpus

• New results on νμ → ντ appearance with the OPERA experiment in the CNGS beam (2013, background): “A few years later, after being investigated for decades by real-time and geochemical experiments [7–12], the so-called solar neutrino problem could also be interpreted (after the SNO results [13])”
• Neutrino Mass Ordering from Oscillations and Beyond: 2018 Status and Future Prospects (2018, background): “…. ] New discoveries about the deepest neutrino secrets are expected to change our current understanding of the history, structure and future fate of the Universe” (see Fukuda et al., 1998; Ahmad et al., 2001, 2002; Eguchi et al., 2003; Abe et al., 2011a; An et al., 2012) for essential publications.”
• Flavor structures of charged fermions and massive neutrinos (2019, background): “In fact, the Super-Kamiokande [66, 380] and SNO [65, 67, 381] experiments have measured the flux of solar 8B neutrinos to a much better degree of accuracy.”
• Oscillations of neutrinos and mesons in quantum field theory (2001, background): “In the 90’s, the persistent deficit in solar neutrinos [10, 11] observed at Homestake was confirmed by several other experiments [12, 13, 14, 15] and, very recently, the Sudbury Neutrino Observatory announced the detection of a nonelectronic component in the solar neutrino flux [16].”
• Charged Lepton Flavour Violation: An Experimental and Theoretical Introduction (2017, background): “The discovery of neutrino oscillations [25, 26, 27] has however demonstrated that the lepton family numbers are not conserved even though, as we shall see later, this has no practical effect in inducing transitions among charged leptons in the framework of the Standard Model.”