Supernova Detection at SNOLAB
Fuente:
arXiv
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| Autori principali: | , , |
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| Natura: | Preprint |
| Pubblicazione: |
2024
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| _version_ | 1866912378302496768 |
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| author | Caden, Erica Sekula, Stephen Yen, Stanley |
| author_facet | Caden, Erica Sekula, Stephen Yen, Stanley |
| contents | 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. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2412_12239 |
| institution | arXiv |
| publishDate | 2024 |
| record_format | arxiv |
| spellingShingle | Supernova Detection at SNOLAB Caden, Erica Sekula, Stephen Yen, Stanley High Energy Physics - Experiment High Energy Astrophysical Phenomena Nuclear Experiment 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. |
| title | Supernova Detection at SNOLAB |
| topic | High Energy Physics - Experiment High Energy Astrophysical Phenomena Nuclear Experiment |
| url | https://arxiv.org/abs/2412.12239 |