Supernova Detection at SNOLAB
High Energy Physics - Experiment
2025-05-19 v2 High Energy Astrophysical Phenomena
Nuclear Experiment
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.
Cite
@article{arxiv.2412.12239,
title = {Supernova Detection at SNOLAB},
author = {Erica Caden and Stephen Sekula and Stanley Yen},
journal= {arXiv preprint arXiv:2412.12239},
year = {2025}
}
Comments
13 pages, 5 figures, for Astroparticle Physics special issue of Canadian Journal of Physics