Status of SNO and future solar neutrino experiments

被引：0
|
作者：
Farine, J [1 ]
机构：
[1] Carleton Univ, Ctr Res Particle Phys, Ottawa, ON K1S 5B6, Canada
来源：
HIGH ENERGY PHYSICS 99, PROCEEDINGS | 2000年
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D O I：
暂无
中图分类号：
O412 [相对论、场论]; O572.2 [粒子物理学];
学科分类号：
摘要：
The Sudbury Neutrino Observatory is a 1 kTD(2)O Cerenkov detector designed to determine whether the currently observed solar neutrino deficit is a result of neutrino oscillations. The performance of the detector in the early stage of operations is presented, and the three planned configurations (pure D2O, addition of MgCl2 or neutron detectors) are discussed. Finally, the status of future solar experiments is briefly reviewed.
引用
收藏
页码：894 / 896
页数：3
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