The measurement of day and night neutrino energy spectra at Sudbury Neutrino Observatory (SNO) and constraints on neutrino mixing parameters were presented. A global solar neutrino analysis in terms of matter-enhanced oscillations of two active flavors strongly favored the large mixing angle solution. Results obtained were the first direct measurements of the day-night asymmetries in the νe flux and the total ν flux from the Sun was deduced
This thesis describes two seperate results in the study of solar neutrinos. The first is a measureme...
This thesis describes two seperate results in the study of solar neutrinos. The first is a measureme...
An updated analysis of all available neutrino oscillation evidence in reactor (Kamland, first 145 da...
The Sudbury Neutrino Observatory (SNO) has measured day and night solar neutrino energy spectra and ...
0031-9007 (Print) Journal ArticleThe Sudbury Neutrino Observatory (SNO) has measured day and night s...
The Sudbury Neutrino Observatory (SNO) is a heavy-water Cherenkov detector designed to study 8B neut...
An updated analysis of all available neutrino oscillation evidence in solar experiments (SK day and ...
This paper reviews the constraints imposed on the solar neutrino mixing parameters by data collected...
The physics implications of the just published salt phase data from the SNO experiment are examined....
Results are reported from the complete salt phase of the Sudbury Neutrino Observatory experiment in ...
Results are reported from the complete salt phase of the Sudbury Neutrino Observatory experiment in...
The Sudbury Neutrino Observatory is a 1000 T D2O Cerenkov detector that is sensitive to 8B solar neu...
The Sudbury Neutrino Observatory (SNO) is a 1000-tonne heavy water Cherenkov detector. Its usage of ...
This article provides the complete description of results from the Phase I data set of the Sudbury N...
We have performed analysis of the solar neutrino data including results from the SNO salt phase as w...
This thesis describes two seperate results in the study of solar neutrinos. The first is a measureme...
This thesis describes two seperate results in the study of solar neutrinos. The first is a measureme...
An updated analysis of all available neutrino oscillation evidence in reactor (Kamland, first 145 da...
The Sudbury Neutrino Observatory (SNO) has measured day and night solar neutrino energy spectra and ...
0031-9007 (Print) Journal ArticleThe Sudbury Neutrino Observatory (SNO) has measured day and night s...
The Sudbury Neutrino Observatory (SNO) is a heavy-water Cherenkov detector designed to study 8B neut...
An updated analysis of all available neutrino oscillation evidence in solar experiments (SK day and ...
This paper reviews the constraints imposed on the solar neutrino mixing parameters by data collected...
The physics implications of the just published salt phase data from the SNO experiment are examined....
Results are reported from the complete salt phase of the Sudbury Neutrino Observatory experiment in ...
Results are reported from the complete salt phase of the Sudbury Neutrino Observatory experiment in...
The Sudbury Neutrino Observatory is a 1000 T D2O Cerenkov detector that is sensitive to 8B solar neu...
The Sudbury Neutrino Observatory (SNO) is a 1000-tonne heavy water Cherenkov detector. Its usage of ...
This article provides the complete description of results from the Phase I data set of the Sudbury N...
We have performed analysis of the solar neutrino data including results from the SNO salt phase as w...
This thesis describes two seperate results in the study of solar neutrinos. The first is a measureme...
This thesis describes two seperate results in the study of solar neutrinos. The first is a measureme...
An updated analysis of all available neutrino oscillation evidence in reactor (Kamland, first 145 da...