First Neutrino Observations from the Sudbury Neutrino Observatory
arXiv:hep-ex/0011025 · doi:10.1016/S0920-5632(00)00918-X
Abstract
The first neutrino observations from the Sudbury Neutrino Observatory are presented from preliminary analyses. Based on energy, direction and location, the data in the region of interest appear to be dominated by 8B solar neutrinos, detected by the charged current reaction on deuterium and elastic scattering from electrons, with very little background. Measurements of radioactive backgrounds indicate that the measurement of all active neutrino types via the neutral current reaction on deuterium will be possible with small systematic uncertainties. Quantitative results for the fluxes observed with these reactions will be provided when further calibrations have been completed.
Latex, 7 pages, 10 figures, Invited paper at Neutrino 2000 Conference, Sudbury, Canada, June 16-21, 2000 to be published in the Proceedings
References in corpus (3)
Cited by in corpus (6)
- Neutrino Masses and Mixing: Evidence and Implications
- Giant star seismology
- Neutrinos from Stellar Collapse: Comparison of signatures in water and heavy water detectors
- Reviving the energy independent suppression of the solar neutrino flux
- High Energy Neutrino Signals of Four Neutrino Mixing
- Horizontal Muons and a Search for AGN Neutrinos in Soudan 2