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Grant: Subatomic Physics Envelope - Project

Queen's University

$160,000.00

SuperCDMS SNOLAB continued construction

EF 2017-18

Résumé
The existence of dark matter is largely undisputed, yet even 80 years after its first discovery all evidence is based on gravitational effects on large scales only. After more than two decades of dedicated effort, the sensitivity of searches for Weakly Interacting Massive Particles (WIMPs) proposed to explain the dark matter observations has reached a level that overlaps largely with the prediction of models developed with the most basic assumptions. The lack of a signal in direct searches for WIMP interactions as well as the lack of evidence for new particles at the LHC forces us to consider models other than the simplest SuperSymmetric extensions of the standard model of particle physics. The Super Cryogenic Dark Matter Search experiment (SuperCDMS) embraces this demand by improving the design of the cryogenic semiconductor detectors to extending the sensitivity to particles with masses down to below half a GeV/c2, considerably below the traditional search range for Supersymmetric WIMPs. Using different target materials (germanium and silicon) also opens the door to testing no-standard interaction mechanisms between dark matter particle and atomic nuclei. SuperCDMS SNOLAB will be constructed with capital funding from DOE and NSF in the US and CFI in Canada over the coming years. This proposal requests operating funds for the Canadian SuperCDMS groups over the critical period during which SuperCDMS SNOLAB will be constructed. Canadian group members have key responsibility for data acquisition, trigger, experiment infrastructure, and detector testing for the new SNOLAB experiment. The requested funds will support postdoctoral fellows and graduate students at Queen's, UBC, the University of Toronto and at Laurentian University/SNOLAB, travel costs for group members to the different SuperCDMS test facilities for DAQ work and detector testing and to Sudbury during the construction phase, as well as collaboration meetings, visits to collaborating institutions and conference travel.
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
SAPPJ-2017-00030
Name nom
Rau, Wolfgang
Department département
Physics, Engineering Physics & Astronomy - Physics, Engineering Physics & Astron
Organization id
29
Institution établissement
Queen's University
Province en
Ontario
Province fr
Ontario
Country en
CANADA
Country fr
CANADA
Fiscal year exercice financier
2017
Competition year année de concours
2017
Award amount
160000
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
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
SuperCDMS SNOLAB continued construction
Keyword
NSERC
Application summary
The existence of dark matter is largely undisputed, yet even 80 years after its first discovery all evidence is based on gravitational effects on large scales only. After more than two decades of dedicated effort, the sensitivity of searches for Weakly Interacting Massive Particles (WIMPs) proposed to explain the dark matter observations has reached a level that overlaps largely with the prediction of models developed with the most basic assumptions. The lack of a signal in direct searches for WIMP interactions as well as the lack of evidence for new particles at the LHC forces us to consider models other than the simplest SuperSymmetric extensions of the standard model of particle physics. The Super Cryogenic Dark Matter Search experiment (SuperCDMS) embraces this demand by improving the design of the cryogenic semiconductor detectors to extending the sensitivity to particles with masses down to below half a GeV/c2, considerably below the traditional search range for Supersymmetric WIMPs. Using different target materials (germanium and silicon) also opens the door to testing no-standard interaction mechanisms between dark matter particle and atomic nuclei. SuperCDMS SNOLAB will be constructed with capital funding from DOE and NSF in the US and CFI in Canada over the coming years. This proposal requests operating funds for the Canadian SuperCDMS groups over the critical period during which SuperCDMS SNOLAB will be constructed. Canadian group members have key responsibility for data acquisition, trigger, experiment infrastructure, and detector testing for the new SNOLAB experiment. The requested funds will support postdoctoral fellows and graduate students at Queen's, UBC, the University of Toronto and at Laurentian University/SNOLAB, travel costs for group members to the different SuperCDMS test facilities for DAQ work and detector testing and to Sudbury during the construction phase, as well as collaboration meetings, visits to collaborating institutions and conference travel.