activity
20152025
most citedCurrent Status and Future Prospects of the SNO+ Experiment

277 citations · 562 across the 8 of their papers we have counts for

collaborators

8 papers

hep-ex2025★ 4 cited

Measurement of reactor antineutrino oscillation at SNO+

SNO+ Collaboration, :, M. Abreu +298

The SNO+ collaboration reports its second spectral analysis of reactor antineutrino oscillation using 286 tonne-years of new data. The measured energies of reactor antineutrino can…

physics.ins-det2022

Slow-Fluor Scintillator for Low Energy Solar Neutrinos and Neutrinoless Double Beta Decay

Jack Dunger, Edward J. Leming, Steven D. Biller

The potential for using slow-fluor liquid scintillators to study low energy solar neutrinos and neutrinoless double beta decay (0nbb) is explored through a series of simulations. T…

physics.ins-det2021★ 129 cited

The SNO+ Experiment

SNO+ Collaboration, :, V. Albanese +251

The SNO+ experiment is located 2 km underground at SNOLAB in Sudbury, Canada. A low background search for neutrinoless double beta () decay will be conducted using 780 tonnes…

physics.ins-det2020★ 41 cited

Development, characterisation, and deployment of the SNO+ liquid scintillator

SNO+ Collaboration, :, M. R. Anderson +223

A liquid scintillator consisting of linear alkylbenzene as the solvent and 2,5-diphenyloxazole as the fluor was developed for the SNO+ experiment. This mixture was chosen as it is…

physics.ins-det2019★ 14 cited

Multi-site Event Discrimination in Large Liquid Scintillation Detectors

Jack Dunger, Steven D. Biller

Simulation studies have been carried out to explore the ability to discriminate between single-site and multi-site energy depositions in large scale liquid scintillation detectors.…

hep-ex2019★ 46 cited

Measurement of the B Solar Neutrino Flux in SNO+ with Very Low Backgrounds

The SNO+ Collaboration, :, M. Anderson +120

A measurement of the B solar neutrino flux has been made using a 69.2 kt-day dataset acquired with the SNO+ detector during its water commissioning phase. At energies above 6 M…