Solar neutrino measurements in Super-Kamiokande-I

By 井上 邦雄. 2006

221 citations recorded by the source corpus.

View Paper: https://www.semanticscholar.org/paper/f4cd7ebc0c215132346288e7bf23a7ba0815e8b9

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Citations in the corpus

• Updated fit to three neutrino mixing: exploring the accelerator-reactor complementarity (2016, background): “• SK1 full energy and zenith spectrum [18], 44 data points.”
• Sterile neutrino oscillations after first MiniBooNE results (2007, background): “Reconciling the LSND signal with the other evidence for neutrino oscillations is a long-standing challenge for neutrino phenomenology, since it requires a mass-squared difference at the eV(2) scale, at odd with the values needed to explain atmospheric [4], longbaseline accelerator [5, 6], solar [7, ”
• Updated fit to three neutrino mixing: status of leptonic CP violation (2014, methodology): “• SK1 full energy and zenith spectrum [22], 44 data points.”
• Deep Underground Neutrino Experiment (DUNE), Far Detector Technical Design Report, Volume II: DUNE Physics (2020, methodology): “The complete data set used, as well as the parameters to which they are sensitive, are (1) from solar neutrino data [298, 413, 414, 415, 416, 417, 418, 419, 420, 421]: θ12, ∆m(2)21, and θ13; (2) from neutrino mode in long-baseline experiments K2K [422], MINOS [423, 424], T2K [425, 426], and NOνA [42”
• Neutrino oscillations (2013, unknown): “In this global analysis the following experimental information is included: the atmospheric neutrino data (Super-Kamiokande [93] phases 1–4), the long baseline accelerator experiments (K2K [42], disappearance and appearance data of MINOS [94], and T2K [90]), the reactor experiments (CHOOZ [95], Palo”
• Global fit to three neutrino mixing: critical look at present precision (2012, methodology): “For realtime experiments we include the 44 data points of the electron scattering (ES) SuperKamiokande phase I (SK1) energy-zenith spectrum [35] and the data from the three phases of SNO [36–38], including the results on the low energy threshold analysis of the combined SNO phases I–III [39].”
• Global analysis of three-flavour neutrino oscillations: synergies and tensions in the determination of θ23, δCP, and the mass ordering (2018, background): “• SK1 full energy and zenith spectrum [61], 44 data points.”
• Updated global analysis of neutrino oscillations in the presence of eV-scale sterile neutrinos (2018, unknown): “[76] Super-Kamkiokande Collaboration, J.”
• Three-flavour neutrino oscillation update (2008, methodology): “The new data from SNO and Borexino are combined with the global data on solar neutrinos [22]–[25], where we take into account the results of a recent re-analysis of the Gallex data yielding a combined Gallex and GNO rate of 67.”
• Updated global fit to three neutrino mixing: status of the hints of θ13 > 0 (2010, methodology): “For real-time experiments we include the 44 data points of the electron scattering (ES) Super-Kamiokande phase I (SK-I) energy-zenith spectrum [17] and the data from the three phases of SNO [18–20], including the results on the low energy threshold analysis of the combined SNO phase I and phase II [”
• Neutrino Oscillations and Non-standard Interactions (2017, background): “After its first three solar phases [46–48], Super-Kamiokande is already in its fourth phase, where a very low energy detection threshold of 3.5 MeV has been achieved [49].”