Conveners
(PPD) M1-8 Neutrino Telescopes | Télescopes à neutrinos (PPD)
- Caleb Miller
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Patrick Krause (SFU)09/06/2025, 10:15Particle Physics / Physique des particules (PPD)Invited Speaker / Conférencier(ère) invité(e)
The Pacific Ocean Neutrino Experiment (P-ONE) is a planned multi-cubic-kilometer neutrino telescope in the Northeast Pacific Ocean off Vancouver Island, British Columbia. Its primary goal is to detect high-energy neutrinos, offering key insights into cosmic ray origins and acceleration mechanisms. Building on two successful pathfinder missions, the collaboration, in partnership with Ocean...
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Daniel Durnford (University of Alberta)09/06/2025, 10:45Particle Physics / Physique des particules (PPD)Invited Speaker / Conférencier(ère) invité(e)
The IceCube neutrino observatory is a Cherenkov light detector in the Antarctic ice sheet, at the South Pole. Composed of a cubic kilometer of detector volume instrumented with over 5000 photo-multiplier tubes, it is the largest neutrino detector in the world, observing neutrinos incident from all directions. Having collected data for 13 years in its current configuration, the IceCube...
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Akanksha Katil (University of Alberta)09/06/2025, 11:15Particle Physics / Physique des particules (PPD)Oral not-in-competition (Graduate Student) / Orale non-compétitive (Étudiant(e) du 2e ou 3e cycle)
The IceCube Neutrino Observatory detects Cherenkov light from neutrino interactions in the Antarctic ice. Despite more than a decade of operation, distinguishing electromagnetic and hadronic showers remains a persistent challenge. Accurately identifying electromagnetic showers provides a charged-current electron-neutrino-rich sample, which plays a pivotal role in Neutrino Mass Ordering...
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Nathan Molberg09/06/2025, 11:30Particle Physics / Physique des particules (PPD)Oral not-in-competition (Graduate Student) / Orale non-compétitive (Étudiant(e) du 2e ou 3e cycle)
The P-ONE neutrino observatory is a proposed water Cherenkov detector for the study of astrophysical neutrinos in the TeV-PeV energy range. Upon completion the detector will contain tens of thousands of photo-multiplier tubes in a cubic-kilometer array located on the seafloor at Cascadia basin, just off the shore of Vancouver Island. To accurately reconstruct the type, energy, and direction of...
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Dr Asish Moharana (Carleton University)09/06/2025, 11:45Particle Physics / Physique des particules (PPD)Oral (Non-Student) / Orale (non-étudiant(e))
ARGO is a future dark matter direct-detection experiment based on a liquid argon (LAr) target that is proposed to be built at SNOLAB in the next decade. ARGO will produce leading sensitivity to heavy dark matter searches above 50 GeV/c2. It will also have excellent sensitivity to detect core-collapse supernova neutrinos and produce high-precision measurements of solar neutrinos at and above...
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