Recent results of the Sudbury Neutrino Observatory

被引：0

作者：

Wilson, JR ^{[1
]}

机构：

[1] Univ Oxford, Dept Phys, Oxford OX1 3RH, England

来源：

NUCLEAR PHYSICS A | 2003年 / 719卷

关键词：

D O I：

10.1016/S0375-9474(03)00986-2

中图分类号：

O57 [原子核物理学、高能物理学];

学科分类号：

070202 ;

摘要：

The Sudbury Neutrino Observatory (SNO) employs one kilotonne of ultra-pure D2O to measure the flux of B-8 neutrinos from the Sun through charged current (CC), neutral current (NC) and elastic scattering (ES) reactions. Based on data from "Phase I" of the experiment the non-v, component of the solar neutrino flux is found to be different from zero at the 5.3sigma level, providing strong evidence for solar v, flavour transformation into active species. Global analyses of SNO data along with other solar neutrino experimental data, favour the large mixing angle (LMA) MSW solution at the 99% confidence level compared to other oscillation solutions. Future measurements of the SNO experiment are also discussed.

引用

页码：161C / 168C

页数：8

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