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Grant: Subatomic Physics Envelope - Project

Simon Fraser University

$558,000.00

Harnessing the high-energy universe with IceCube and P-ONE

FY 2024-25

Summary
Neutrinos are one of nature's most abundant and enigmatic fundamental particles, and their study provides unique opportunities to probe new phenomena in the Universe. Extreme astrophysical objects are nature's particle accelerators, with the ability to produce a high flux of neutrinos either directly at the source or via related cosmic rays that subsequently impinge the Earth's atmosphere. Large-scale neutrino telescopes employ a relatively simple detector principle, deploying an array of light sensors with volumes of cubic-kilometres within natural deep optically-transparent media that acts as the target material for the rare neutrino interactions. These instruments have demonstrated the ability to leverage the broad energy range and distances traversed by these astrophysical and atmospheric neutrinos to study the underlying properties of the particle and probe the production and acceleration mechanisms of the sources. To fully harness the scientific potential of these discovery-driven instruments, in addition to continued operation of current detectors, development of a new generation of neutrino telescopes is underway. This proposal addresses the Canadian particle-astrophysics community's activities in neutrino telescopes, specifically associated with the IceCube Neutrino Observatory (IceCube) and the Pacific Ocean Neutrino Experiment (P-ONE). IceCube, situated at the geographic South Pole, instruments cubic-kilometer of the deep Antarctic ice sheet and has been in full operation since 2010. Among its most notable achievements, IceCube has discovered the existence of the high-energy astrophysical neutrino flux, has started to observe indications of potential sources of that flux, and has advanced precision measurements of neutrino oscillations. The IceCube detector will complete construction of the Upgrade array in 2026, providing enhanced reach across the core scientific program. In the same period, P-ONE, a new telescope array to be deployed off the coast of Vancouver Island in the Cascading Basin, will complete construction of the first phase "Demonstrator" detector. The proposed activities leverage the unique expertise of the team in data analysis, calibrations, and detector hardware development, positioning Canadian researchers to maintain their leadership in this rapidly emerging field.
Program
Subatomic Physics Envelope - Project
Location
British Columbia, Canada
Recipient Type
Academia
Type
Grant
Source
NSERC's Awards Data

As published

Application id
SAPPJ-2024-00023
Name nom
Grant, Darren
Department département
Physics - Physics
Organization id
5
Institution établissement
Simon Fraser University
Province en
British Columbia
Province fr
Colombie-Britannique
Country en
CANADA
Country fr
CANADA
Fiscal year exercice financier
2024
Competition year année de concours
2024
Award amount
558000
Program id
SAPPJ
Program name en
Subatomic Physics Envelope - Project
Program name fr
Enveloppe de physique subatomique - De projet
Group en
DISCOVERY RESEARCH
Group fr
RECHERCHE AXÉE SUR 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
Field of research list names en
Not available
Field of research list names fr
Non disponible
Socioeconomic objective list names en
Not available
Socioeconomic objective list names fr
Non disponible
Application title
Harnessing the high-energy universe with IceCube and P-ONE
Keywords
neutrino physics; high energy physics; astroparticle physics; multi-messenger; neutrino oscillations; beyond the standard model; photodetection technologies; weak interactions
Application summary
Neutrinos are one of nature's most abundant and enigmatic fundamental particles, and their study provides unique opportunities to probe new phenomena in the Universe. Extreme astrophysical objects are nature's particle accelerators, with the ability to produce a high flux of neutrinos either directly at the source or via related cosmic rays that subsequently impinge the Earth's atmosphere. Large-scale neutrino telescopes employ a relatively simple detector principle, deploying an array of light sensors with volumes of cubic-kilometres within natural deep optically-transparent media that acts as the target material for the rare neutrino interactions. These instruments have demonstrated the ability to leverage the broad energy range and distances traversed by these astrophysical and atmospheric neutrinos to study the underlying properties of the particle and probe the production and acceleration mechanisms of the sources. To fully harness the scientific potential of these discovery-driven instruments, in addition to continued operation of current detectors, development of a new generation of neutrino telescopes is underway. This proposal addresses the Canadian particle-astrophysics community's activities in neutrino telescopes, specifically associated with the IceCube Neutrino Observatory (IceCube) and the Pacific Ocean Neutrino Experiment (P-ONE). IceCube, situated at the geographic South Pole, instruments cubic-kilometer of the deep Antarctic ice sheet and has been in full operation since 2010. Among its most notable achievements, IceCube has discovered the existence of the high-energy astrophysical neutrino flux, has started to observe indications of potential sources of that flux, and has advanced precision measurements of neutrino oscillations. The IceCube detector will complete construction of the Upgrade array in 2026, providing enhanced reach across the core scientific program. In the same period, P-ONE, a new telescope array to be deployed off the coast of Vancouver Island in the Cascading Basin, will complete construction of the first phase "Demonstrator" detector. The proposed activities leverage the unique expertise of the team in data analysis, calibrations, and detector hardware development, positioning Canadian researchers to maintain their leadership in this rapidly emerging field.
Simon Fraser University - $558,000 Grant (2024-25) | Canada Spends