Sudbury Neutrino Observatory

The Sudbury Neutrino Observatory (SNO) detector, located at Sudbury, Ontario, Canada, consists of 1000 tons of heavy water (D20) mounted 2 km below the surface in the Sudbury Nickel Mine. In addition to neutrino-electron scattering, this detector can also utilize nuclear reactions involving deuterium ... 

Ahlen, S. P, Avignone, F. T., Brodzinski, R. L., Drukier, A. K., Gelmini, G. Spergel, D. N. 1987. Limits On Cold Dark Matter Candidates From An Ultralow Background Germanium Spectrometer, Phys. Lett. B195, 603 Ahmad, Q. R., et al. [SNO Collaboration] 2002. Direct evidence for neutrino flavor transformation from neutral-current interactions in the Sudbury Neutrino Observatory, Phys. Rev. Lett.89, 011301 Ahrens, J., et al. [AMANDA Collaboration] 2002. Limits to the muon flux from WIMP annihilation in the center of the earth with the AMANDA detector, Phys. Rev. D66, 032006... 

Ahmad, Q. R. et al. (The Sudbury Neutrino Observatory Collaboration) Direct Evidence for Neutrino Flavor Transformation from Neutral-Current Interactions in the Sudbury Neutrino Observatory. Physical Review Letters 2002,59,011301-1. 

H.H. Chen, The Sudbury Neutrino Observatory, Nuclear Instruments and Methods in Physics Research A264, p. 50. (1988). 

Aharmin et al. 2005, Sudbury Neutrino Observatory, Canada). This result clearly shows that is non zero. The KamLAND (Japan) experiment, which studies reactor electron... 

During the 10-year period in which the data in Tables V and VI were acquired, the electronic solar neutrino experiment in the Sudbury Neutrino Observatory (SNO) in Canada was completed and began data taking. The heart of SNO is a transparent acryclic sphere holding 1000 tons of heavy (deuterated) water with which to observe the reaction initiated by Ve from the in the sun. 

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