The Sudbury Neutrino Observatory (SNO) used an array of 3He proportional counters to measure the rate of neutral-current interactions in heavy water and precisely determined the total active (nu_x) 8B solar neutrino flux. This technique is independent of previous methods employed by SNO. The total flux is found to be 5.54_-0.31;+0.33(stat)-0.34+0.36(syst)x10(6) cm(-2) s(-1), in agreement with previous measurements and standard solar models. A global analysis of solar and reactor neutrino results yields Deltam2=7.59_-0.21;+0.19x10(-5) eV2 and theta=34.4_-1.2;+1.3 degrees. The uncertainty on the mixing angle has been reduced from SNO's previous results
The Sudbury Neutrino Observatory (SNO) used an array of He3 proportional counters to measure the rat...
This work presents experimental measurements obtained by analyzing the first 254 live days of data f...
The Sudbury Neutrino Observatory has precisely determined the total active (nu(x)) B-8 solar neutrin...
The Sudbury Neutrino Observatory (SNO) used an array of He3 proportional counters to measure the rat...
The Sudbury Neutrino Observatory (SNO) used an array of He3 proportional counters to measure the rat...
The Sudbury Neutrino Observatory has precisely determined the total active (nu(x)) 8B solar neutrino...
This paper details the solar neutrino analysis of the 385.17-day phase-III data set acquired by the ...
The measurements performed for determining the total active 8B solar neutrino flux at the Sudbury Ne...
This paper details the solar neutrino analysis of the 385.17-day Phase-III data set acquired by the ...
This paper details the solar neutrino analysis of the 385.17-day phase-III data set acquired by the ...
The Sudbury Neutrino Observatory (SNO) used an array of He3 proportional counters to measure the rat...
The Sudbury Neutrino Observatory (SNO) used an array of 3He proportional counters to measure the rat...
The Sudbury Neutrino Observatory (SNO) was a heavy water Cerenkov detector that had the unique abili...
The Sudbury Neutrino Observatory (SNO) used an array of {sup 3}He proportional counters to measure t...
The Sudbury Neutrino Observatory (SNO) is a 1000-tonne heavy water Cherenkov detector. Its usage of ...
The Sudbury Neutrino Observatory (SNO) used an array of He3 proportional counters to measure the rat...
This work presents experimental measurements obtained by analyzing the first 254 live days of data f...
The Sudbury Neutrino Observatory has precisely determined the total active (nu(x)) B-8 solar neutrin...
The Sudbury Neutrino Observatory (SNO) used an array of He3 proportional counters to measure the rat...
The Sudbury Neutrino Observatory (SNO) used an array of He3 proportional counters to measure the rat...
The Sudbury Neutrino Observatory has precisely determined the total active (nu(x)) 8B solar neutrino...
This paper details the solar neutrino analysis of the 385.17-day phase-III data set acquired by the ...
The measurements performed for determining the total active 8B solar neutrino flux at the Sudbury Ne...
This paper details the solar neutrino analysis of the 385.17-day Phase-III data set acquired by the ...
This paper details the solar neutrino analysis of the 385.17-day phase-III data set acquired by the ...
The Sudbury Neutrino Observatory (SNO) used an array of He3 proportional counters to measure the rat...
The Sudbury Neutrino Observatory (SNO) used an array of 3He proportional counters to measure the rat...
The Sudbury Neutrino Observatory (SNO) was a heavy water Cerenkov detector that had the unique abili...
The Sudbury Neutrino Observatory (SNO) used an array of {sup 3}He proportional counters to measure t...
The Sudbury Neutrino Observatory (SNO) is a 1000-tonne heavy water Cherenkov detector. Its usage of ...
The Sudbury Neutrino Observatory (SNO) used an array of He3 proportional counters to measure the rat...
This work presents experimental measurements obtained by analyzing the first 254 live days of data f...
The Sudbury Neutrino Observatory has precisely determined the total active (nu(x)) B-8 solar neutrin...