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SNO+

Steve Biller

Professor of Particle Physics

Sub department

  • Particle Physics

Research groups

  • SNO+
Steven.Biller@physics.ox.ac.uk
Telephone: 01865 (2)73386
Denys Wilkinson Building, room 568a
Personal Website
  • About
  • Publications

A New Technique to Load 130Te in Liquid Scintillator for Neutrinoless Double Beta Decay Experiments

Journal of Physics Conference Series IOP Publishing 888:1 (2017) 012084

Authors:

Steven Biller, Szymon Manecki, SNO collaboration
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Current status and future prospects of the SNO+ experiment

Advances in High Energy Physics Hindawi Publishing Corporation 2016 (2016) 6194250-6194250

Authors:

Steven D Biller, Luca A Cavalli, Jack T Dunger, Nicholas A Jelley, Christopher Jones, Peter G Jones, Jeffrey Lidgard, Krishana Majumdar, Armin Reichold, Laura Segui, Jeffrey C-L Tseng

Abstract:

SNO+ is a large liquid scintillator-based experiment located 2km underground at SNOLAB, Sudbury, Canada. It reuses the Sudbury Neutrino Observatory detector, consisting of a 12m diameter acrylic vessel which will be filled with about 780 tonnes of ultra-pure liquid scintillator. Designed as a multipurpose neutrino experiment, the primary goal of SNO+ is a search for the neutrinoless double-beta decay (0$\nu\beta\beta$) of 130Te. In Phase I, the detector will be loaded with 0.3% natural tellurium, corresponding to nearly 800 kg of 130Te, with an expected effective Majorana neutrino mass sensitivity in the region of 55-133 meV, just above the inverted mass hierarchy. Recently, the possibility of deploying up to ten times more natural tellurium has been investigated, which would enable SNO+ to achieve sensitivity deep into the parameter space for the inverted neutrino mass hierarchy in the future. Additionally, SNO+ aims to measure reactor antineutrino oscillations, low-energy solar neutrinos, and geoneutrinos, to be sensitive to supernova neutrinos, and to search for exotic physics. A first phase with the detector filled with water will begin soon, with the scintillator phase expected to start after a few months of water data taking. The 0$\nu\beta\beta$ Phase I is foreseen for 2017.
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Purification of telluric acid for SNO+ neutrinoless double-beta decay search

Nuclear Instruments and Methods in Physics Research Section A Accelerators Spectrometers Detectors and Associated Equipment Elsevier 795 (2015) 132-139

Authors:

S Hans, R Rosero, L Hu, O Chkvorets, WT Chan, S Guan, W Beriguete, A Wright, R Ford, MC Chen, S Biller, M Yeh
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Another look at confidence intervals: Proposal for a more relevant and transparent approach

Nuclear Instruments and Methods in Physics Research Section A Accelerators Spectrometers Detectors and Associated Equipment Elsevier 774 (2015) 103-119

Authors:

Steven D Biller, Scott M Oser
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SNO+ with Tellurium

Physics Procedia Elsevier 61 (2015) 205-210
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