Event-by-Event Direction Reconstruction of Solar Neutrinos in a High Light-Yield Liquid Scintillator
arXiv:2309.06341 · doi:10.1103/PhysRevD.109.072002
Abstract
The direction of individual B solar neutrinos has been reconstructed using the SNO+ liquid scintillator detector. Prompt, directional Cherenkov light was separated from the slower, isotropic scintillation light using time information, and a maximum likelihood method was used to reconstruct the direction of individual scattered electrons. A clear directional signal was observed, correlated with the solar angle. The observation was aided by a period of low primary fluor concentration that resulted in a slower scintillator decay time. This is the first time that event-by-event direction reconstruction in high light-yield liquid scintillator has been demonstrated in a large-scale detector.
arXiv comment6 pages, 6 figures. Accepted manuscript by PRD
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- Study of neutron production for 360 GeV cosmic muons
- New Spallation Background Rejection Techniques to Greatly Improve the Solar Neutrino Sensitivity of JUNO
- Canadian Contributions to the Search for Neutrinoless Double Beta Decay
- Supernova Detection at SNOLAB