Determination of solar neutrino oscillation parameters using 1496 days of Super-Kamiokande-I data
By The Super-Kamiokande Collaboration. 2002
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Abstract A number of different fits to solar neutrino mixing and mass square difference were performed using 1496 days of Super-Kamiokande-I's solar neutrino data. These data select two allowed areas at large neutrino mixing when combined with either the solar 8B flux prediction of the standard solar model or the SNO interaction rate measurements. A global fit combining SK data with the solar neutrino interaction rates measured by Homestake, SNO, Gallex/GNO and SAGE prefers a single allowed area, the Large Mixing Angle solution, at the 98.9% confidence level. The mass square difference Δm2 between the two mass eigenstates ranges from about 3 to 19×10−5 eV2, while the mixing angle θ is in the range of tan2θ≈0.25–0.65.
Subfields: Atmospheric Science, Nuclear and High Energy Physics
View Paper: https://www.semanticscholar.org/paper/362b890a2473555727cc4e39afcd375c67b4d9d1
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In Atmospheric Science
In Nuclear and High Energy Physics
Citations in the corpus
- Sterile neutrino oscillations after first MiniBooNE results (2007, background): “In the framework of so-called (3+2) five-neutrino mass schemes we find severe tension between appearance and disappearance experiments at the level of more than 3σ, and hence no satistfactory fit to the global data is possible in (3+2) schemes.”
- 10,000 Standard Solar Models: A Monte Carlo Simulation (2005, methodology): “Section 8.1 describes the histogram of results for the 8B neutrinos which have been measured directly in the Kamiokande (Fukuda et al. 1996), Super-Kamiokande (Fukuda et al. 2001, 2002) and SNO experiments (Ahmed et al. 2004; Aharmin et al. 2005).”