Electron Energy Spectra, Fluxes, and Day-Night Asymmetries of ${}^8$B Solar Neutrinos from the 391-Day Salt Phase SNO Data Set

Abstract

Results are reported from the complete salt phase of the Sudbury Neutrino Observatory experiment in which NaCl was dissolved in the D${}_2$O target. The addition of salt enhanced the signal from neutron capture, as compared to the pure D${}_2$O detector. By making a statistical separation of charged-current events from other types based on event-isotropy criteria, the effective electron recoil energy spectrum has been extracted. In units of $10^6$ cm${}^{-2}$ s${}^{-1}$, the total flux of active-flavor neutrinos from ${}^8$B decay in the Sun is found to be $4.94_{-0.21}^{+0.21}{(stat)}_{-0.34}^{+0.38}(syst)$ and the integral flux of electron neutrinos for an undistorted ${}^8$B spectrum is $1.68_{-0.06}^{+0.06}{(stat)}_{-0.09}^{+0.08}(syst)$; the signal from (${\nu }_x$,e) elastic scattering is equivalent to an electron-neutrino flux of $2.35_{-0.22}^{+0.22}{(stat)}_{-0.15}^{+0.15}(syst)$. These results are consistent with those expected for neutrino oscillations with the so-called Large Mixing Angle parameters, and also with an undistorted spectrum. A search for matter-enhancement effects in the Earth through a possible day-night asymmetry in the charged-current integral rate is consistent with no asymmetry. Including results from other experiments, the best-fit values for two-neutrino mixing parameters are $\Delta m^2=(8.0_{-0.4}^{+0.6})\times 10^{-5}$ eV${}^2$ and $\theta =33.9_{-2.2}^{+2.4}$ degrees.

45 pages, 36 figures in 49 eps files

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