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Grant: Subatomic Physics Envelope - Project

Queen's University

$335,000.00

DEAP-3600 Installation, Commissioning and Analysis

EF 2012-13

Résumé
It is well-established that most of the matter in our universe is dark; more than three quarters of all matter currently evades direct observation. The origin and nature of this dark matter is currently one of the most important questions in particle astrophysics, evidenced by the active global research effort aimed at dark matter detection. A favored hypothesis is that the dark matter consists of WIMPs, weakly interacting massive particles, which could be detected by observing their elastic scattering from nuclei. This proposal will enable the completion and first analysis of the DEAP-3600 experiment at SNOLAB for a very sensitive dark matter search. Unique to DEAP-3600 is the novel technique of discriminating background events using the time evolution of the scintillation pulse, which leads to a simple detector design that can be scaled to a very large target mass. Operation at the deep underground SNOLAB facility allows extremely low backgrounds which would otherwise mask dark matter signals. DEAP-3600 will increase sensitivity to dark matter particles by a factor of one hundred, allowing tests of theoretical models that predict dark matter detection is possible. The project has been under development for several years, and is currently being installed in the SNOLAB cube hall. The central detector consists of a large (85 cm radius) acrylic vessel which contains the 3600 kg cryogenic liquid argon and is viewed by 255 photomultiplier tubes to detect argon scintillation light pulses from nuclear recoils. The experiment will be housed in an 8 meter diameter water shielding tank and supported by a deck structure, both of which have been completed at SNOLAB. Installation of the detector subsystems (acrylic vessel, argon purification equipment, readout electronics and trigger, and associated infrastructure) is expected to continue until May 2013, after which the detector will be filled and prepared for data collection. This proposal will lead to further training of highly qualified personnel in Canada. In addition to attracting students and international highly qualified researchers, it is anticipated that the post-doctoral fellows, RAs, and students supported by this request will have the opportunity to take part in this leading-edge science.
Programme
Subatomic Physics Envelope - Project
Bénéficiaire
Emplacement
Ontario, Canada
Type de bénéficiaire
Academia
Type
Grant
Source
NSERC's Awards Data

Tel que publié

Application id
341311-2012
Name nom
Boulay, 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
2012
Competition year année de concours
2012
Award amount
335000
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
1202
Area of application group en
Advancement of knowledge
Area of application group fr
Avancement des connaissances
Area of application en
Physical sciences
Area of application fr
Sciences physiques
Research subject code
3106
Research subject group en
Physics
Research subject group fr
Physique
Research subject en
Weak interactions
Research subject fr
Interactions faibles
Partie
1
Nb partie
1
Application title
DEAP-3600 Installation, Commissioning and Analysis
Keyword
NSERC
Application summary
It is well-established that most of the matter in our universe is dark; more than three quarters of all matter currently evades direct observation. The origin and nature of this dark matter is currently one of the most important questions in particle astrophysics, evidenced by the active global research effort aimed at dark matter detection. A favored hypothesis is that the dark matter consists of WIMPs, weakly interacting massive particles, which could be detected by observing their elastic scattering from nuclei. This proposal will enable the completion and first analysis of the DEAP-3600 experiment at SNOLAB for a very sensitive dark matter search. Unique to DEAP-3600 is the novel technique of discriminating background events using the time evolution of the scintillation pulse, which leads to a simple detector design that can be scaled to a very large target mass. Operation at the deep underground SNOLAB facility allows extremely low backgrounds which would otherwise mask dark matter signals. DEAP-3600 will increase sensitivity to dark matter particles by a factor of one hundred, allowing tests of theoretical models that predict dark matter detection is possible. The project has been under development for several years, and is currently being installed in the SNOLAB cube hall. The central detector consists of a large (85 cm radius) acrylic vessel which contains the 3600 kg cryogenic liquid argon and is viewed by 255 photomultiplier tubes to detect argon scintillation light pulses from nuclear recoils. The experiment will be housed in an 8 meter diameter water shielding tank and supported by a deck structure, both of which have been completed at SNOLAB. Installation of the detector subsystems (acrylic vessel, argon purification equipment, readout electronics and trigger, and associated infrastructure) is expected to continue until May 2013, after which the detector will be filled and prepared for data collection. This proposal will lead to further training of highly qualified personnel in Canada. In addition to attracting students and international highly qualified researchers, it is anticipated that the post-doctoral fellows, RAs, and students supported by this request will have the opportunity to take part in this leading-edge science.