KM3NeT-ORCA: Oscillation Research with Cosmics in the Abyss
27th International Conference on Neutrino Physics and Astrophysics (Neutrino 2016) International audience KM3NeT, currently under construction in the abysses of the Mediterranean Sea, is a distributed research infrastructure that will host a km3-scale neutrino telescope (ARCA) for high-energy neutri...
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Online Access: | https://hal.in2p3.fr/in2p3-01427749 https://doi.org/10.1088/1742-6596/888/1/012024 |
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ftunivnantes:oai:HAL:in2p3-01427749v1 2023-05-15T17:53:29+02:00 KM3NeT-ORCA: Oscillation Research with Cosmics in the Abyss Coyle, Paschal 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 Londre, United Kingdom 2016-07-04 https://hal.in2p3.fr/in2p3-01427749 https://doi.org/10.1088/1742-6596/888/1/012024 en eng HAL CCSD info:eu-repo/semantics/altIdentifier/arxiv/1701.01382 info:eu-repo/semantics/altIdentifier/doi/10.1088/1742-6596/888/1/012024 in2p3-01427749 https://hal.in2p3.fr/in2p3-01427749 ARXIV: 1701.01382 doi:10.1088/1742-6596/888/1/012024 INSPIRE: 1507874 Journal of Physics Conference Series XXVII International Conference on Neutrino Physics and Astrophysics (Neutrino 2016) https://hal.in2p3.fr/in2p3-01427749 XXVII International Conference on Neutrino Physics and Astrophysics (Neutrino 2016), Jul 2016, Londre, United Kingdom. pp.012024, ⟨10.1088/1742-6596/888/1/012024⟩ [PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det] [PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE] [PHYS]Physics [physics] [PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph] [PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex] info:eu-repo/semantics/conferenceObject Conference papers 2016 ftunivnantes https://doi.org/10.1088/1742-6596/888/1/012024 2023-03-08T06:56:54Z 27th International Conference on Neutrino Physics and Astrophysics (Neutrino 2016) International audience KM3NeT, currently under construction in the abysses of the Mediterranean Sea, is a distributed research infrastructure that will host a km3-scale neutrino telescope (ARCA) for high-energy neutrino astronomy, and a megaton scale detector (ORCA) for neutrino oscillation studies of atmospheric neutrinos. ORCA is optimised for a measurement of the mass hierarchy, providing a sensitivity of 3{\sigma} after 3-4 years. It will also measure the atmospheric mixing parameters $\Delta m_{32}^2$ and $\theta_{23}$ with a precision comparable to the NOvA and T2K experiments using both the muon neutrino disappearance and tau neutrino appearance channels. It will provide a measurement of the tau neutrino appearance rate with better than 10% precision, a crucial ingredient for tests of unitarity. It will probe the octant of the mixing angle $\theta_{23}$ via matter resonance effects on neutrinos and antineutrinos crossing the core and mantle, which are largely independent on the CP phase. The observation of neutrino oscillations over a wide range of baselines and energies will provide broad sensitivity to new physics such as non-standard neutrino interactions (NSI) and sterile neutrinos. Conference Object Orca Université de Nantes: HAL-UNIV-NANTES Journal of Physics: Conference Series 888 012024 |
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Université de Nantes: HAL-UNIV-NANTES |
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ftunivnantes |
language |
English |
topic |
[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det] [PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE] [PHYS]Physics [physics] [PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph] [PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex] |
spellingShingle |
[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det] [PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE] [PHYS]Physics [physics] [PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph] [PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex] Coyle, Paschal KM3NeT-ORCA: Oscillation Research with Cosmics in the Abyss |
topic_facet |
[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det] [PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE] [PHYS]Physics [physics] [PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph] [PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex] |
description |
27th International Conference on Neutrino Physics and Astrophysics (Neutrino 2016) International audience KM3NeT, currently under construction in the abysses of the Mediterranean Sea, is a distributed research infrastructure that will host a km3-scale neutrino telescope (ARCA) for high-energy neutrino astronomy, and a megaton scale detector (ORCA) for neutrino oscillation studies of atmospheric neutrinos. ORCA is optimised for a measurement of the mass hierarchy, providing a sensitivity of 3{\sigma} after 3-4 years. It will also measure the atmospheric mixing parameters $\Delta m_{32}^2$ and $\theta_{23}$ with a precision comparable to the NOvA and T2K experiments using both the muon neutrino disappearance and tau neutrino appearance channels. It will provide a measurement of the tau neutrino appearance rate with better than 10% precision, a crucial ingredient for tests of unitarity. It will probe the octant of the mixing angle $\theta_{23}$ via matter resonance effects on neutrinos and antineutrinos crossing the core and mantle, which are largely independent on the CP phase. The observation of neutrino oscillations over a wide range of baselines and energies will provide broad sensitivity to new physics such as non-standard neutrino interactions (NSI) and sterile neutrinos. |
author2 |
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 |
Coyle, Paschal |
author_facet |
Coyle, Paschal |
author_sort |
Coyle, Paschal |
title |
KM3NeT-ORCA: Oscillation Research with Cosmics in the Abyss |
title_short |
KM3NeT-ORCA: Oscillation Research with Cosmics in the Abyss |
title_full |
KM3NeT-ORCA: Oscillation Research with Cosmics in the Abyss |
title_fullStr |
KM3NeT-ORCA: Oscillation Research with Cosmics in the Abyss |
title_full_unstemmed |
KM3NeT-ORCA: Oscillation Research with Cosmics in the Abyss |
title_sort |
km3net-orca: oscillation research with cosmics in the abyss |
publisher |
HAL CCSD |
publishDate |
2016 |
url |
https://hal.in2p3.fr/in2p3-01427749 https://doi.org/10.1088/1742-6596/888/1/012024 |
op_coverage |
Londre, United Kingdom |
genre |
Orca |
genre_facet |
Orca |
op_source |
Journal of Physics Conference Series XXVII International Conference on Neutrino Physics and Astrophysics (Neutrino 2016) https://hal.in2p3.fr/in2p3-01427749 XXVII International Conference on Neutrino Physics and Astrophysics (Neutrino 2016), Jul 2016, Londre, United Kingdom. pp.012024, ⟨10.1088/1742-6596/888/1/012024⟩ |
op_relation |
info:eu-repo/semantics/altIdentifier/arxiv/1701.01382 info:eu-repo/semantics/altIdentifier/doi/10.1088/1742-6596/888/1/012024 in2p3-01427749 https://hal.in2p3.fr/in2p3-01427749 ARXIV: 1701.01382 doi:10.1088/1742-6596/888/1/012024 INSPIRE: 1507874 |
op_doi |
https://doi.org/10.1088/1742-6596/888/1/012024 |
container_title |
Journal of Physics: Conference Series |
container_volume |
888 |
container_start_page |
012024 |
_version_ |
1766161185289273344 |