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Grant: Subatomic Physics Envelope - Project

Queen's University

$829,000.00

SNO+

FY 2008-09

Summary
A new experiment is being developed at the Sudbury Neutrino Observatory (SNO), Canada's world-leading neutrino physics facility. The experiment is called SNO+ and it consists of filling the SNO detector with a liquid scintillator now that the heavy water that was in SNO has been removed. By turning SNO into SNO+, a multipurpose experiment with diverse scientific goals would be created. SNO+ will be able to address fundamental questions in particle physics, in geophysics, and in astrophysics. SNO+ will start where SNO leaves off and it will expand our understanding of the neutrino and its impact on the physical universe. A liquid scintillator emits 100 times more light when a neutrino interacts in it compared to a neutrino interaction in water. This means that SNO+ will be able to detect neutrinos with lower energies. 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, antineutrinos from natural radioactivity in the Earth will be detected by SNO+. SNO+ will thus be able to assay the total amount of uranium and thorium radioactivity in the deep Earth. The fraction of Earth's heat that originates from radioactivity is a fundamental question that could be answered. An extremely rare nuclear decay will be studied in SNO+ by dissolving neodymium in the liquid scintillator. Observation of this process, known as neutrinoless double beta decay, would shed light on the fundamental nature of the neutrino with potential impact on our understanding of matter and antimatter in the Universe. SNO+ has been conducting R&D, funded by NSERC since April 2005. In 2007 SNO+ has been completing full technical designs for the engineered components of the new detector. At this point in the development of the project, SNO+ is ready for implementation. We are ready to move forward with capital construction and this proposal requests funding for a portion of the capital costs of the SNO+ experiment, with the remainder to be requested from a CFI infrastructure grant. This proposal also includes amounts to support SNO+ research activities at Queen's, Alberta and Laurentian.
Program
Subatomic Physics Envelope - Project
Location
Ontario, Canada
Recipient Type
Academia
Type
Grant
Source
NSERC's Awards Data

As published

Application id
219858-2008
Name nom
Chen, Mark
Department département
Physics
Organization id
29
Institution établissement
Queen's University
Province en
Ontario
Province fr
Ontario
Country en
CANADA
Country fr
CANADA
Fiscal year exercice financier
2008
Competition year année de concours
2008
Award amount
829000
Program id
SAPPJ
Program nane 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+
Keyword
NA
Application summary
A new experiment is being developed at the Sudbury Neutrino Observatory (SNO), Canada's world-leading neutrino physics facility. The experiment is called SNO+ and it consists of filling the SNO detector with a liquid scintillator now that the heavy water that was in SNO has been removed. By turning SNO into SNO+, a multipurpose experiment with diverse scientific goals would be created. SNO+ will be able to address fundamental questions in particle physics, in geophysics, and in astrophysics. SNO+ will start where SNO leaves off and it will expand our understanding of the neutrino and its impact on the physical universe. A liquid scintillator emits 100 times more light when a neutrino interacts in it compared to a neutrino interaction in water. This means that SNO+ will be able to detect neutrinos with lower energies. 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, antineutrinos from natural radioactivity in the Earth will be detected by SNO+. SNO+ will thus be able to assay the total amount of uranium and thorium radioactivity in the deep Earth. The fraction of Earth's heat that originates from radioactivity is a fundamental question that could be answered. An extremely rare nuclear decay will be studied in SNO+ by dissolving neodymium in the liquid scintillator. Observation of this process, known as neutrinoless double beta decay, would shed light on the fundamental nature of the neutrino with potential impact on our understanding of matter and antimatter in the Universe. SNO+ has been conducting R&D, funded by NSERC since April 2005. In 2007 SNO+ has been completing full technical designs for the engineered components of the new detector. At this point in the development of the project, SNO+ is ready for implementation. We are ready to move forward with capital construction and this proposal requests funding for a portion of the capital costs of the SNO+ experiment, with the remainder to be requested from a CFI infrastructure grant. This proposal also includes amounts to support SNO+ research activities at Queen's, Alberta and Laurentian.