Grant: Subatomic Physics Envelope - Project
Queen's University
$150,000.00
Sudbury Neutrino Observatory project B On-site
EF 2008-09
Résumé
This proposal (SNO Project Grant B) is a request for three years of support for the Canadian part of the on-site research costs for the Sudbury Neutrino Observatory experiment (SNO), a large international project to study fundamental particles called neutrinos. International project participants also pay their portion of on-site research costs. Neutrinos are able to penetrate out from the thermonuclear furnaces powering the Sun and are detected in the SNO detector, situated 2 km underground near Sudbury, Ontario. Observation of these neutrinos gives specific information about the energy generation processes in the Sun, basic properties of neutrinos themselves and information about the influence of neutrinos on the evolution of the Universe. The experimental program for the present phase of SNO with neutron detectors in the heavy water will continue to provide unique information on solar neutrinos, while also studying neutrinos produced in the Earth's atmosphere, in supernovae and in other astrophysical sources. Properties of solar neutrinos will be studied through more accurate measurements of flavour change, including day-night flux comparisons to search for regeneration in the Earth and measurements of possible periodic variations in neutrino fluxes. These studies can define the allowed range of masses and coupling parameters for electron neutrinos much more strongly than at present. A protocol has been developed for providing early information to the astronomical community in the event of a supernova in our Galaxy.
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
233596-2006
Name nom
McDonald, Arthur
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
2006
Award amount
150000
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
9999
Area of application group en
Not available
Area of application group fr
Non disponible
Area of application en
Not available
Area of application fr
Non disponible
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
3
Nb partie
3
Application title
Sudbury Neutrino Observatory project B On-site
Keyword
NA
Application summary
This proposal (SNO Project Grant B) is a request for three years of support for the Canadian part of the on-site research costs for the Sudbury Neutrino Observatory experiment (SNO), a large international project to study fundamental particles called neutrinos. International project participants also pay their portion of on-site research costs. Neutrinos are able to penetrate out from the thermonuclear furnaces powering the Sun and are detected in the SNO detector, situated 2 km underground near Sudbury, Ontario. Observation of these neutrinos gives specific information about the energy generation processes in the Sun, basic properties of neutrinos themselves and information about the influence of neutrinos on the evolution of the Universe. The experimental program for the present phase of SNO with neutron detectors in the heavy water will continue to provide unique information on solar neutrinos, while also studying neutrinos produced in the Earth's atmosphere, in supernovae and in other astrophysical sources. Properties of solar neutrinos will be studied through more accurate measurements of flavour change, including day-night flux comparisons to search for regeneration in the Earth and measurements of possible periodic variations in neutrino fluxes. These studies can define the allowed range of masses and coupling parameters for electron neutrinos much more strongly than at present. A protocol has been developed for providing early information to the astronomical community in the event of a supernova in our Galaxy.