C. Howard

TL;DR: In this article, a statistical separation of charged-current events from other types based on event-isotropy criteria was made to extract the effective electron recoil energy spectrum, which is consistent with those expected for neutrino oscillations with the so-called large mixing angle parameters.

TL;DR: In this paper, a combined analysis of solar neutrino data from all phases of the Sudbury Neutrino Observatory was presented, which showed that particle identification information obtained from the proportional counters installed during the third phase improved background rejection in that phase of the experiment.

TL;DR: The Sudbury Neutrino Observatory (SNO) used an array of He3 proportional counters to measure the rate of neutral-current interactions in heavy water and precisely determined the total active (x) B8 solar neutrino flux as discussed by the authors.

TL;DR: In this paper, a joint analysis of Phase I and Phase II data from the Sudbury Neutrino Observatory is reported, where the total flux of active-flavor neutrinos from 8B decay in the Sun measured using the neutral current (NC) reaction, with no constraint on the 8B neutrino energy spectrum, is found to be FNC=5.5 MeV, the lowest analysis threshold yet achieved with water Cherenkov detector data.

TL;DR: Aharmim et al. as discussed by the authors reported the results of the complete salt phase of the Sudbury Neutrino Observatory experiment in which NaCl was dissolved in the D_2O target.