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Phys. Rev. D 69, 011104(R) (2004) [5 pages]

Precise measurement of the solar neutrino day-night and seasonal variation in Super-Kamiokande-I

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M. B. Smy et al. (Super-Kamiokande Collaboration)
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Received 4 September 2003; revised 18 November 2003; published 30 January 2004

The time variation of the elastic scattering rate of solar neutrinos with electrons in Super-Kamiokande-I was fit to the variations expected from active two-neutrino oscillations. The best fit in the large mixing angle solution has a mixing angle of tan2θ=0.55 and a mass squared difference of Δm2=6.3×10-5eV2 between the two neutrino mass eigenstates. The fitted day-night asymmetry of -1.8±1.6(stat)-1.2+1.3(syst)% has improved statistical precision over previous measurements and agrees well with the expected asymmetry of -2.1%.

© 2004 The American Physical Society

URL:
http://link.aps.org/doi/10.1103/PhysRevD.69.011104
DOI:
10.1103/PhysRevD.69.011104
PACS:
14.60.Pq, 26.65.+t, 95.85.Ry, 96.40.Tv