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Grant: Subatomic Physics Envelope - Project

Queen's University

$421,000.00

SNO+ Final Construction, Commissioning and First Data

FY 2013-14

Summary
SNO+ is the follow-up experiment to the Sudbury Neutrino Observatory (SNO). With a liquid scintillator in place of the heavy water that was in the SNO detector, a new experiment with extended sensitivity at lower energies is being built. SNO+ will be able to address fundamental questions in particle physics, in geosciences, and in astrophysics. SNO+ will start where SNO left off and it will expand our understanding of the neutrino and its impact on the physical universe. A liquid scintillator emits over 50 times more light when a neutrino interacts in it compared to in water. Consequently SNO+ will be able to detect neutrinos with lower energies than SNO. Lower energy neutrinos from the Sun will be studied to shed light on the properties of neutrinos and the energy generation processes in stars. Separately, ""geo neutrinos"" from natural radioactivity in the Earth will be detected by SNO+. The quantity of geo neutrinos detected can be related to the total amount of radioactivity in the deep Earth and its role in Earth's thermal processes and history. Finally, an extremely rare nuclear decay will also be studied in SNO+ by dissolving neodymium or other isotope in the liquid scintillator. Observation of this process, known as neutrinoless double beta decay, would tell physicists about the matter-antimatter properties of the neutrino, and its connection to cosmological questions about matter and antimatter in the Universe. SNO+ detector construction is nearing completion. In 2013, the detector will be filled/operated with water to study optics and backgrounds, and to complete electronics/DAQ commissioning. The underground installation of the scintillator purification plant will take place concurrently. Later in 2013, the plant and the SNO+ detector will be ready to receive scintillator. During the 2013-2015 period of this NSERC proposal, there will be a strong Canadian analysis effort that will extract physics from first SNO+ data. This proposal requests funds to support: HQP training, travel, materials and supplies related to final construction, commissioning, data taking and first physics.
Program
Subatomic Physics Envelope - Project
Location
Ontario, Canada
Recipient Type
Academia
Type
Grant
Source
NSERC's Awards Data

As published

Application id
219858-2013
Name nom
Chen, Mark
Department département
Physics, Engineering Physics & Astronomy
Organization id
29
Institution établissement
Queen's University
Province en
Ontario
Province fr
Ontario
Country en
CANADA
Country fr
CANADA
Fiscal year exercice financier
2013
Competition year année de concours
2013
Award amount
421000
Program id
SAPPJ
Program name en
Subatomic Physics Envelope - Project
Program name fr
Enveloppe de physique subatomique - De projet
Group en
Discovery grants programs
Group fr
Programmes de subventions à la découverte
Committee code
19
Committee name en
Subatomic Physics
Committee name fr
Physique subatomique
Area of application code
1200
Area of application group en
Advancement of knowledge
Area of application group fr
Avancement des connaissances
Area of application en
Advancement of knowledge
Area of application fr
Avancement des connaissances
Research subject code
3104
Research subject group en
Physics
Research subject group fr
Physique
Research subject en
Particle physics
Research subject fr
Physique des particules
Partie
1
Nb partie
2
Application title
SNO+ Final Construction, Commissioning and First Data
Keyword
NSERC
Application summary
SNO+ is the follow-up experiment to the Sudbury Neutrino Observatory (SNO). With a liquid scintillator in place of the heavy water that was in the SNO detector, a new experiment with extended sensitivity at lower energies is being built. SNO+ will be able to address fundamental questions in particle physics, in geosciences, and in astrophysics. SNO+ will start where SNO left off and it will expand our understanding of the neutrino and its impact on the physical universe. A liquid scintillator emits over 50 times more light when a neutrino interacts in it compared to in water. Consequently SNO+ will be able to detect neutrinos with lower energies than SNO. Lower energy neutrinos from the Sun will be studied to shed light on the properties of neutrinos and the energy generation processes in stars. Separately, ""geo neutrinos"" from natural radioactivity in the Earth will be detected by SNO+. The quantity of geo neutrinos detected can be related to the total amount of radioactivity in the deep Earth and its role in Earth's thermal processes and history. Finally, an extremely rare nuclear decay will also be studied in SNO+ by dissolving neodymium or other isotope in the liquid scintillator. Observation of this process, known as neutrinoless double beta decay, would tell physicists about the matter-antimatter properties of the neutrino, and its connection to cosmological questions about matter and antimatter in the Universe. SNO+ detector construction is nearing completion. In 2013, the detector will be filled/operated with water to study optics and backgrounds, and to complete electronics/DAQ commissioning. The underground installation of the scintillator purification plant will take place concurrently. Later in 2013, the plant and the SNO+ detector will be ready to receive scintillator. During the 2013-2015 period of this NSERC proposal, there will be a strong Canadian analysis effort that will extract physics from first SNO+ data. This proposal requests funds to support: HQP training, travel, materials and supplies related to final construction, commissioning, data taking and first physics.