Sensitivity of multi-PMT optical modules in Antarctic ice to supernova neutrinos of MeV energy
Abstract New optical sensors with a segmented photosensitive area are being developed for the next generation of neutrino telescopes at the South Pole. In addition to increasing sensitivity to high-energy astrophysical neutrinos, we show that this will also lead to a significant improvement in sensi...
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ftdoajarticles:oai:doaj.org/article:56fe0c7148d84098ba79b0db7ec784ee 2023-05-15T13:46:37+02:00 Sensitivity of multi-PMT optical modules in Antarctic ice to supernova neutrinos of MeV energy C. J. Lozano Mariscal L. Classen M. A. Unland Elorrieta A. Kappes 2021-12-01T00:00:00Z https://doi.org/10.1140/epjc/s10052-021-09809-y https://doaj.org/article/56fe0c7148d84098ba79b0db7ec784ee EN eng SpringerOpen https://doi.org/10.1140/epjc/s10052-021-09809-y https://doaj.org/toc/1434-6044 https://doaj.org/toc/1434-6052 doi:10.1140/epjc/s10052-021-09809-y 1434-6044 1434-6052 https://doaj.org/article/56fe0c7148d84098ba79b0db7ec784ee European Physical Journal C: Particles and Fields, Vol 81, Iss 12, Pp 1-11 (2021) Astrophysics QB460-466 Nuclear and particle physics. Atomic energy. Radioactivity QC770-798 article 2021 ftdoajarticles https://doi.org/10.1140/epjc/s10052-021-09809-y 2022-12-31T05:05:25Z Abstract New optical sensors with a segmented photosensitive area are being developed for the next generation of neutrino telescopes at the South Pole. In addition to increasing sensitivity to high-energy astrophysical neutrinos, we show that this will also lead to a significant improvement in sensitivity to MeV neutrinos, such as those produced in core-collapse supernovae (CCSN). These low-energy neutrinos can provide a detailed picture of the events after stellar core collapse, testing our understanding of these violent explosions. We present studies on the event-based detection of MeV neutrinos with a segmented sensor and, for the first time, the potential of a corresponding detector in the deep ice at the South Pole for the detection of extra-galactic CCSN. We find that exploiting temporal coincidences between signals in different photocathode segments, a $$27\ \mathrm {M}_{\odot }$$ 27 M ⊙ progenitor mass CCSN can be detected up to a distance of 341 kpc with a false detection rate of $${0.01}\,\hbox {year}^{-1}$$ 0.01 year - 1 with a detector consisting of 10,000 sensors. Increasing the number of sensors to 20,000 and reducing the optical background by a factor of 70 expands the range such that a CCSN detection rate of 0.1 per year is achieved, while keeping the false detection rate at $${0.01}\,{\hbox {year}^{-1}}$$ 0.01 year - 1 . Article in Journal/Newspaper Antarc* Antarctic South pole South pole Directory of Open Access Journals: DOAJ Articles Antarctic South Pole The European Physical Journal C 81 12 |
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Open Polar |
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Directory of Open Access Journals: DOAJ Articles |
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ftdoajarticles |
language |
English |
topic |
Astrophysics QB460-466 Nuclear and particle physics. Atomic energy. Radioactivity QC770-798 |
spellingShingle |
Astrophysics QB460-466 Nuclear and particle physics. Atomic energy. Radioactivity QC770-798 C. J. Lozano Mariscal L. Classen M. A. Unland Elorrieta A. Kappes Sensitivity of multi-PMT optical modules in Antarctic ice to supernova neutrinos of MeV energy |
topic_facet |
Astrophysics QB460-466 Nuclear and particle physics. Atomic energy. Radioactivity QC770-798 |
description |
Abstract New optical sensors with a segmented photosensitive area are being developed for the next generation of neutrino telescopes at the South Pole. In addition to increasing sensitivity to high-energy astrophysical neutrinos, we show that this will also lead to a significant improvement in sensitivity to MeV neutrinos, such as those produced in core-collapse supernovae (CCSN). These low-energy neutrinos can provide a detailed picture of the events after stellar core collapse, testing our understanding of these violent explosions. We present studies on the event-based detection of MeV neutrinos with a segmented sensor and, for the first time, the potential of a corresponding detector in the deep ice at the South Pole for the detection of extra-galactic CCSN. We find that exploiting temporal coincidences between signals in different photocathode segments, a $$27\ \mathrm {M}_{\odot }$$ 27 M ⊙ progenitor mass CCSN can be detected up to a distance of 341 kpc with a false detection rate of $${0.01}\,\hbox {year}^{-1}$$ 0.01 year - 1 with a detector consisting of 10,000 sensors. Increasing the number of sensors to 20,000 and reducing the optical background by a factor of 70 expands the range such that a CCSN detection rate of 0.1 per year is achieved, while keeping the false detection rate at $${0.01}\,{\hbox {year}^{-1}}$$ 0.01 year - 1 . |
format |
Article in Journal/Newspaper |
author |
C. J. Lozano Mariscal L. Classen M. A. Unland Elorrieta A. Kappes |
author_facet |
C. J. Lozano Mariscal L. Classen M. A. Unland Elorrieta A. Kappes |
author_sort |
C. J. Lozano Mariscal |
title |
Sensitivity of multi-PMT optical modules in Antarctic ice to supernova neutrinos of MeV energy |
title_short |
Sensitivity of multi-PMT optical modules in Antarctic ice to supernova neutrinos of MeV energy |
title_full |
Sensitivity of multi-PMT optical modules in Antarctic ice to supernova neutrinos of MeV energy |
title_fullStr |
Sensitivity of multi-PMT optical modules in Antarctic ice to supernova neutrinos of MeV energy |
title_full_unstemmed |
Sensitivity of multi-PMT optical modules in Antarctic ice to supernova neutrinos of MeV energy |
title_sort |
sensitivity of multi-pmt optical modules in antarctic ice to supernova neutrinos of mev energy |
publisher |
SpringerOpen |
publishDate |
2021 |
url |
https://doi.org/10.1140/epjc/s10052-021-09809-y https://doaj.org/article/56fe0c7148d84098ba79b0db7ec784ee |
geographic |
Antarctic South Pole |
geographic_facet |
Antarctic South Pole |
genre |
Antarc* Antarctic South pole South pole |
genre_facet |
Antarc* Antarctic South pole South pole |
op_source |
European Physical Journal C: Particles and Fields, Vol 81, Iss 12, Pp 1-11 (2021) |
op_relation |
https://doi.org/10.1140/epjc/s10052-021-09809-y https://doaj.org/toc/1434-6044 https://doaj.org/toc/1434-6052 doi:10.1140/epjc/s10052-021-09809-y 1434-6044 1434-6052 https://doaj.org/article/56fe0c7148d84098ba79b0db7ec784ee |
op_doi |
https://doi.org/10.1140/epjc/s10052-021-09809-y |
container_title |
The European Physical Journal C |
container_volume |
81 |
container_issue |
12 |
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1766244695578509312 |