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spelling ftunivnantes:oai:HAL:hal-03210387v1 2023-05-15T17:53:32+02:00 KM3NeT: Status and Prospects for Neutrino Astronomy at Low and High Energies Huang, Feifei Institut Pluridisciplinaire Hubert Curien (IPHC) Université de Strasbourg (UNISTRA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS) Centre de Physique des Particules de Marseille (CPPM) Aix Marseille Université (AMU)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS) KM3NeT Prague, Czech Republic 2020-07-30 https://hal.science/hal-03210387 https://doi.org/10.22323/1.390.0138 en eng HAL CCSD info:eu-repo/semantics/altIdentifier/doi/10.22323/1.390.0138 hal-03210387 https://hal.science/hal-03210387 doi:10.22323/1.390.0138 INSPIRE: 1859667 PoS 40th International Conference on High Energy Physics https://hal.science/hal-03210387 40th International Conference on High Energy Physics, Jul 2020, Prague, Czech Republic. pp.138, ⟨10.22323/1.390.0138⟩ neutrino: energy: high neutrino: atmosphere energy: high KM3NeT GeV observatory oscillation supernova structure messenger galaxy [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph] [PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det] info:eu-repo/semantics/conferenceObject Conference papers 2020 ftunivnantes https://doi.org/10.22323/1.390.0138 2023-03-08T03:04:52Z International audience KM3NeT is a multi-purpose cubic-kilometer neutrino observatory currently being deployed at the bottom of the Mediterranean Sea. It consists of two detectors: ORCA and ARCA (for Oscillation and Astroparticle Research with Cosmics in the Abyss, respectively). ARCA will instrument 1 Gton of seawater, with the primary goal of detecting cosmic neutrinos with energies between several tens of GeV and PeV. Due to its position in the Northern Hemisphere, ARCA will provide an optimal view of the Southern sky including the Galactic Center. ORCA is a smaller (few Mtons) and denser array, optimized for the detection of atmospheric neutrinos in the 1 - 100 GeV range. It can also investigate low-energy neutrino astronomy, such as MeV-scale core-collapse supernova. This proceeding presents the current status of the KM3NeT infrastructure, its outlook on neutrino astronomy, and its multi-messenger program status. Conference Object Orca Université de Nantes: HAL-UNIV-NANTES Proceedings of 40th International Conference on High Energy physics — PoS(ICHEP2020) 138
institution Open Polar
collection Université de Nantes: HAL-UNIV-NANTES
op_collection_id ftunivnantes
language English
topic neutrino: energy: high
neutrino: atmosphere
energy: high
KM3NeT
GeV
observatory
oscillation
supernova
structure
messenger
galaxy
[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]
spellingShingle neutrino: energy: high
neutrino: atmosphere
energy: high
KM3NeT
GeV
observatory
oscillation
supernova
structure
messenger
galaxy
[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]
Huang, Feifei
KM3NeT: Status and Prospects for Neutrino Astronomy at Low and High Energies
topic_facet neutrino: energy: high
neutrino: atmosphere
energy: high
KM3NeT
GeV
observatory
oscillation
supernova
structure
messenger
galaxy
[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]
description International audience KM3NeT is a multi-purpose cubic-kilometer neutrino observatory currently being deployed at the bottom of the Mediterranean Sea. It consists of two detectors: ORCA and ARCA (for Oscillation and Astroparticle Research with Cosmics in the Abyss, respectively). ARCA will instrument 1 Gton of seawater, with the primary goal of detecting cosmic neutrinos with energies between several tens of GeV and PeV. Due to its position in the Northern Hemisphere, ARCA will provide an optimal view of the Southern sky including the Galactic Center. ORCA is a smaller (few Mtons) and denser array, optimized for the detection of atmospheric neutrinos in the 1 - 100 GeV range. It can also investigate low-energy neutrino astronomy, such as MeV-scale core-collapse supernova. This proceeding presents the current status of the KM3NeT infrastructure, its outlook on neutrino astronomy, and its multi-messenger program status.
author2 Institut Pluridisciplinaire Hubert Curien (IPHC)
Université de Strasbourg (UNISTRA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)
Centre de Physique des Particules de Marseille (CPPM)
Aix Marseille Université (AMU)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)
KM3NeT
format Conference Object
author Huang, Feifei
author_facet Huang, Feifei
author_sort Huang, Feifei
title KM3NeT: Status and Prospects for Neutrino Astronomy at Low and High Energies
title_short KM3NeT: Status and Prospects for Neutrino Astronomy at Low and High Energies
title_full KM3NeT: Status and Prospects for Neutrino Astronomy at Low and High Energies
title_fullStr KM3NeT: Status and Prospects for Neutrino Astronomy at Low and High Energies
title_full_unstemmed KM3NeT: Status and Prospects for Neutrino Astronomy at Low and High Energies
title_sort km3net: status and prospects for neutrino astronomy at low and high energies
publisher HAL CCSD
publishDate 2020
url https://hal.science/hal-03210387
https://doi.org/10.22323/1.390.0138
op_coverage Prague, Czech Republic
genre Orca
genre_facet Orca
op_source PoS
40th International Conference on High Energy Physics
https://hal.science/hal-03210387
40th International Conference on High Energy Physics, Jul 2020, Prague, Czech Republic. pp.138, ⟨10.22323/1.390.0138⟩
op_relation info:eu-repo/semantics/altIdentifier/doi/10.22323/1.390.0138
hal-03210387
https://hal.science/hal-03210387
doi:10.22323/1.390.0138
INSPIRE: 1859667
op_doi https://doi.org/10.22323/1.390.0138
container_title Proceedings of 40th International Conference on High Energy physics — PoS(ICHEP2020)
container_start_page 138
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