| Article ID | Journal | Published Year | Pages | File Type |
|---|---|---|---|---|
| 9857315 | Nuclear Physics B - Proceedings Supplements | 2005 | 6 Pages |
Abstract
The Sudbury Neutrino Observatory (SNO) detects 8B solar neutrinos via charged-current (CC) and neutral-current (NC) neutrino-deuteron reactions, as well as the elastic scattering of neutrinos on electrons. The SNO experiment was designed to run in three phases. In each phase, the method for detecting the free neutron produced by NC reactions is different. This contribution describes and compares the different phases of the SNO experiment and reviews the published results from the first two phases.
Related Topics
Physical Sciences and Engineering
Physics and Astronomy
Nuclear and High Energy Physics
Authors
M.C. Chen, the SNO Collaboration the SNO Collaboration,