The Sudbury Neutrino Observatory has precisely determined the total active (nu(x)) 8B solar neutrino flux without assumptions about the energy dependence of the nu(e) survival probability. The measurements were made with dissolved NaCl in heavy water to enhance the sensitivity and signature for neutral-current interactions. The flux is found to be 5.21 +/- 0.27(stat)+/-0.38(syst) x 10(6) cm(-2) s(-1), in agreement with previous measurements and standard solar models. A global analysis of these and other solar and reactor neutrino results yields Deltam(2)=7.1(+1.2)(-0.6) x 10(-5) eV(2) and theta=32.5(+2.4)(-2.3) degrees. Maximal mixing is rejected at the equivalent of 5.4 standard deviations
The Sudbury Neutrino Observatory (SNO) was a heavy water Cerenkov detector that had the unique abili...
The Sudbury Neutrino Observatory uses 1000 tonnes of heavy water in an ultra-clean Cherenkov detecto...
The Sudbury Neutrino Observatory, through its measurements of the solar 8B neutrino flux via the cha...
The Sudbury Neutrino Observatory has precisely determined the total active (nu(x)) 8B solar neutrino...
The measurements performed for determining the total active 8B solar neutrino flux at the Sudbury Ne...
The Sudbury Neutrino Observatory (SNO) used an array of 3He 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 (SNO) used an array of He3 proportional counters to measure the rat...
The Sudbury Neutrino Observatory has precisely determined the total active (nu(x)) B-8 solar neutrin...
This paper details the solar neutrino analysis of the 385.17-day phase-III data set acquired by the ...
This work presents experimental measurements obtained by analyzing the first 254 live days of data f...
The Sudbury Neutrino Observatory (SNO) is a 1000-tonne heavy water Cherenkov detector. Its usage of ...
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 ...
The Sudbury Neutrino Observatory (SNO) was a heavy water Cerenkov detector that had the unique abili...
The Sudbury Neutrino Observatory uses 1000 tonnes of heavy water in an ultra-clean Cherenkov detecto...
The Sudbury Neutrino Observatory, through its measurements of the solar 8B neutrino flux via the cha...
The Sudbury Neutrino Observatory has precisely determined the total active (nu(x)) 8B solar neutrino...
The measurements performed for determining the total active 8B solar neutrino flux at the Sudbury Ne...
The Sudbury Neutrino Observatory (SNO) used an array of 3He 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 (SNO) used an array of He3 proportional counters to measure the rat...
The Sudbury Neutrino Observatory has precisely determined the total active (nu(x)) B-8 solar neutrin...
This paper details the solar neutrino analysis of the 385.17-day phase-III data set acquired by the ...
This work presents experimental measurements obtained by analyzing the first 254 live days of data f...
The Sudbury Neutrino Observatory (SNO) is a 1000-tonne heavy water Cherenkov detector. Its usage of ...
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 ...
The Sudbury Neutrino Observatory (SNO) was a heavy water Cerenkov detector that had the unique abili...
The Sudbury Neutrino Observatory uses 1000 tonnes of heavy water in an ultra-clean Cherenkov detecto...
The Sudbury Neutrino Observatory, through its measurements of the solar 8B neutrino flux via the cha...