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dc.contributor.author Ahmed, S. N.
dc.contributor.author Levine, Ilan
dc.date.accessioned 2021-04-14T17:47:51Z
dc.date.available 2021-04-14T17:47:51Z
dc.date.issued 2004
dc.identifier.uri https://hdl.handle.net/2022/26353
dc.description.abstract The Sudbury Neutrino Observatory (SNO) 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 the 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) x10^6 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 Delta m^{2} = 7.1^{+1.2}_{-0.6}x10^{-5} ev^2 and theta = 32.5^{+2.4}_{-2.3} degrees. Maximal mixing is rejected at the equivalent of 5.4 standard deviations en
dc.format.extent 6 pages
dc.language.iso en en
dc.publisher American Physical Society en
dc.subject.lcsh Particles (Nuclear physics)
dc.title Measurement of the Total Active 8B Solar Neutrino Flux at the Sudbury Neutrino Observatory with Enhanced Neutral Current Sensitivity en
dc.type Article en


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