Supernova Detection at SNOLAB

Abstract

Neutrinos carry most of the energy released by a core-collapse supernova. SNOLAB has two neutrino-capable detectors, SNO+ and HALO, that have complementary neutrino flavour sensitivities. SNOLAB is also host to existing facilities, or plans to host future projects, that can enhance sensitivity to these neutrinos. These detectors, together with others worldwide both in existence and planned, will provide insights to a variety of different models using neutrinos from the next galactic supernova.

13 pages, 5 figures, for Astroparticle Physics special issue of Canadian Journal of Physics

References in corpus (31)

• Explosion Mechanisms of Core-Collapse Supernovae
• Observation of Coherent Elastic Neutrino-Nucleus Scattering
• Collective Neutrino Oscillations
• Monte Carlo Study of Supernova Neutrino Spectra Formation
• The Sudbury Neutrino Observatory
• Neutrino Signal of Electron-Capture Supernovae from Core Collapse to Cooling
• SNEWS: The SuperNova Early Warning System
• NEXO: Neutrinoless double beta decay search beyond $10^{28}$ year half-life sensitivity
• High-resolution supernova neutrino spectra represented by a simple fit
• On the rate of core collapse supernovae in the Milky Way
• A dynamical collective calculation of supernova neutrino signals
• The SNO+ Experiment
• The role of $\nu$-induced reactions on lead and iron in neutrino detectors
• Mu- and Tau-Neutrino Spectra Formation in Supernovae
• SNEWS 2.0: A Next-Generation SuperNova Early Warning System for Multi-messenger Astronomy
• Neutrino Emission from Supernovae
• What Can Be Learned with a Lead-Based Supernova-Neutrino Detector?
• KamLAND Sensitivity to Neutrinos from Pre-Supernova Stars
• Neutrino beams as a probe of the nuclear isospin and spin-isospin excitations
• Neutrino mean free path in neutron stars
• (Down-to-)Earth matter effect in supernova neutrinos
• The neutrino signal at HALO: learning about the primary supernova neutrino fluxes and neutrino properties
• Charged-current reactions in the supernova neutrino-sphere
• Sensitivity of the PICO-500 Bubble Chamber to Supernova Neutrinos Through Coherent Nuclear Elastic Scattering
• Efficient estimation method for time evolution of proto-neutron star mass and radius from supernova neutrino signal
• Detectability of Collective Neutrino Oscillation Signatures in the Supernova Explosion of a 8.8 $M_{\odot }$ star
• Combined Pre-Supernova Alert System with Kamland and Super-Kamiokande
• Measurement of ${}^{nat}$Pb(${\nu }_e$,X$n$) production with a stopped-pion neutrino source
• Neutrino Echos following Black Hole Formation in Core-Collapse Supernovae
• Event-by-Event Direction Reconstruction of Solar Neutrinos in a High Light-Yield Liquid Scintillator
• The calibration system for the photomultiplier array of the SNO+ experiment