Imprint of SNO neutral current data on the solar neutrino problem

被引:119
作者
Barger, V
Marfatia, D
Whisnant, K
Wood, BP
机构
[1] Univ Wisconsin, Dept Phys, Madison, WI 53706 USA
[2] Boston Univ, Dept Phys, Boston, MA 02215 USA
[3] Iowa State Univ Sci & Technol, Dept Phys & Astron, Ames, IA 50011 USA
关键词
D O I
10.1016/S0370-2693(02)01955-X
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We perform a global analysis in the framework of two active neutrino oscillations of all solar neutrino data, including the recent SNO day and night spectra (comprised of the charged current (CC), elastic scattering (ES) and neutral current (NC) events), the Super-Kamiokande (SK) day and night spectra (from 1496 days) and the updated SAGE results. We find that the Large Mixing Angle (LMA) solution is selected at the 99% C.L.; the best-fit parameters are Deltam(2) = 5.6 x 10(-5) eV(2) and theta = 32degrees. No solutions with theta greater than or equal to pi/4 are allowed at the 5sigma C.L. Oscillations to a pure sterile state are excluded at 5.3sigma, but a sizeable sterile neutrino component could still be present in the solar flux. (C) 2002 Elsevier Science B.V. All rights reserved.
引用
收藏
页码:179 / 186
页数:8
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