Status of the SNO experiment

The Sudbury Neutrino Observatory (SNO) is a 1-kt heavy water Cherenkov detector sensitive to the flavor content of the ⁸B neutrinos originating in the Sun. The analysis of the second phase, in which salt (NaCl) was added to the heavy water in order to increase the cross section for neutrons and therefore enhance the sensitivity to solar neutrinos, is completed. Results from 391 d of data (June 2001 until September 2003) are summarized and constraints on the neutrino mixing parameters are given. The third phase of operation has started in which ³He proportional counters have been deployed inside the D₂O. These neutral-current detectors will perform a systematically independent measurement of the Solar-neutrino flux on a event-by-event basis. SNO finishes data taking at the end of 2006 and the heavy water will be removed. A new experiment using liquid scintillator to measure the pep solar neutrinos and geoneutrinos is proposed and will be described briefly. for the SNO Collaboration The text was submitted by the author in English.