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Title: RECENT SNO RESULTS.

Conference ·
OSTI ID:809654

Solar Neutrinos from the decay of {sup 8}B have been detected at the Sudbury Neutrino Observatory (SNO) by charged current (CC) and neutral current (NC) interactions on deuterium and elastic scattering (ES) of electrons. The SNO data indicate that with the assumption of undistorted {sup 8}B shape, the flux for v{sub e} is {phi}{sub e} = 1.76{sub -0.05}{sup +0.05}(stat.){sub -0.09}{sup +0.09}(syst.) x 10{sup 6} cm{sup -2} s{sup -1} for a kinetic energy threshold of 5 MeV. The non-v{sub e} flux is {phi}{sub {mu}{tau}} = 3.41{sub -0.45}{sup +0.45}(stat.){sub -0.45}{sup +0.48}(syst.) x 10{sup 6} cm{sup -2}s{sup -1}. This provides strong evidence for solar v{sub e} flavor transformation. The day and night solar neutrino energy spectra and rates have also been measured. For CC events, the v{sub e} asymmetry is 14.0% {+-} 6.3%{sub -1.4}{sup +1.5}%. By additionally constraining the total (NC) flux of active neutrinos to have no asymmetry, the v{sub e} asymmetry becomes 7.0% {+-} 4.9%{sub -1.2}{sup +1.3}%. A global solar neutrino analysis strongly favors the Large Mixing Angle (LMA) solution in a two-flavor neutrino oscillation model.

Research Organization:
Brookhaven National Lab. (BNL), Upton, NY (United States)
Sponsoring Organization:
USDOE Office of Energy Research (ER) (US)
DOE Contract Number:
AC02-98CH10886
OSTI ID:
809654
Report Number(s):
BNL-71097-2003-CP; R&D Project: CO001; KB0401022; TRN: US0302598
Resource Relation:
Conference: PROCEEDINGS OF THE CORAL GABLES CONFERENCE, FORT LAUDERDALE, FL (US), 12/10/2002--12/15/2002; Other Information: PBD: 10 Dec 2002
Country of Publication:
United States
Language:
English