KM3NeT: Status and Prospects for Neutrino Astronomy at Low and High Energies
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 instrumen...
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ftccsdartic: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) Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université de Strasbourg (UNISTRA)-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.archives-ouvertes.fr/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.archives-ouvertes.fr/hal-03210387 doi:10.22323/1.390.0138 INSPIRE: 1859667 PoS 40th International Conference on High Energy Physics https://hal.archives-ouvertes.fr/hal-03210387 40th International Conference on High Energy Physics, Jul 2020, Prague, Czech Republic. pp.138, ⟨10.22323/1.390.0138⟩ galaxy messenger structure supernova oscillation observatory KM3NeT GeV energy: high neutrino: atmosphere neutrino: energy: high [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 ftccsdartic https://doi.org/10.22323/1.390.0138 2021-10-23T23:46:13Z 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 Archive ouverte HAL (Hyper Article en Ligne, CCSD - Centre pour la Communication Scientifique Directe) Proceedings of 40th International Conference on High Energy physics — PoS(ICHEP2020) 138 |
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Archive ouverte HAL (Hyper Article en Ligne, CCSD - Centre pour la Communication Scientifique Directe) |
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galaxy messenger structure supernova oscillation observatory KM3NeT GeV energy: high neutrino: atmosphere neutrino: energy: high [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph] [PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det] |
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galaxy messenger structure supernova oscillation observatory KM3NeT GeV energy: high neutrino: atmosphere neutrino: energy: high [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 |
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galaxy messenger structure supernova oscillation observatory KM3NeT GeV energy: high neutrino: atmosphere neutrino: energy: high [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. |
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Institut Pluridisciplinaire Hubert Curien (IPHC) Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université de Strasbourg (UNISTRA)-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.archives-ouvertes.fr/hal-03210387 https://doi.org/10.22323/1.390.0138 |
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Prague, Czech Republic |
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Orca |
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Orca |
op_source |
PoS 40th International Conference on High Energy Physics https://hal.archives-ouvertes.fr/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.archives-ouvertes.fr/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) |
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138 |
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1766161231563980800 |