Sensitivity for astrophysical neutrino searches with KM3NeT-ORCA
International audience The KM3NeT facility, the next generation of large neutrino detectors, is currently being deployedin the Mediterranean Sea. KM3NeT will consist of two ARCA ("Astroparticle Research withCosmics in the Abyss") building blocks, optimized for very high-energy astrophysica...
Published in: | Proceedings of 36th International Cosmic Ray Conference — PoS(ICRC2019) |
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ftunivaixmarseil:oai:HAL:hal-02507600v1 2024-05-19T07:46:44+00:00 Sensitivity for astrophysical neutrino searches with KM3NeT-ORCA de Wasseige, Gwenhael Kouchner, Antoine Colomer Molla, Marta Dornic, Damien Hallmann, Steffen AstroParticule et Cosmologie (APC (UMR_7164)) Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris Université Paris Sciences et Lettres (PSL)-Université Paris Sciences et Lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité) 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 Madison, United States 2019-07-24 https://hal.science/hal-02507600 https://hal.science/hal-02507600/document https://hal.science/hal-02507600/file/4-poster-NMO_ICRC_2019-GDW_infradev.pdf https://doi.org/10.22323/1.358.0934 en eng HAL CCSD info:eu-repo/semantics/altIdentifier/doi/10.22323/1.358.0934 hal-02507600 https://hal.science/hal-02507600 https://hal.science/hal-02507600/document https://hal.science/hal-02507600/file/4-poster-NMO_ICRC_2019-GDW_infradev.pdf doi:10.22323/1.358.0934 INSPIRE: 1785096 info:eu-repo/semantics/OpenAccess PoS 36th International Cosmic Ray Conference https://hal.science/hal-02507600 36th International Cosmic Ray Conference, Jul 2019, Madison, United States. pp.934, ⟨10.22323/1.358.0934⟩ neutrino: oscillation neutrino: atmosphere neutrino: detector detector: sensitivity KM3NeT gravitational radiation neutrino: energy: high VIRGO LIGO VHE gravitational radiation detector experimental equipment experimental methods experimental results statistical analysis data analysis method [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph] info:eu-repo/semantics/conferenceObject Conference papers 2019 ftunivaixmarseil https://doi.org/10.22323/1.358.0934 2024-04-25T00:55:40Z International audience The KM3NeT facility, the next generation of large neutrino detectors, is currently being deployedin the Mediterranean Sea. KM3NeT will consist of two ARCA ("Astroparticle Research withCosmics in the Abyss") building blocks, optimized for very high-energy astrophysical neutrinos,and of the ORCA one ("Oscillation Research with Cosmics in the Abyss"). While ORCA hasoriginally been designed to study neutrino oscillations using atmospheric neutrinos, this densearray may also be used for astrophysical neutrino searches. We present a first estimate of thesensitivity for GeV–100GeV neutrino searches in time/space coincidence with GW alerts sentby the LIGO and Virgo collaborations (LVC). We use the final configuration of ORCA, i.e.ORCA-115 detection units, to estimate the sensitivity of ORCA to gravitational wave events thatmay be detected by LVC during O3. Conference Object Orca Aix-Marseille Université: HAL Proceedings of 36th International Cosmic Ray Conference — PoS(ICRC2019) 934 |
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Aix-Marseille Université: HAL |
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ftunivaixmarseil |
language |
English |
topic |
neutrino: oscillation neutrino: atmosphere neutrino: detector detector: sensitivity KM3NeT gravitational radiation neutrino: energy: high VIRGO LIGO VHE gravitational radiation detector experimental equipment experimental methods experimental results statistical analysis data analysis method [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph] |
spellingShingle |
neutrino: oscillation neutrino: atmosphere neutrino: detector detector: sensitivity KM3NeT gravitational radiation neutrino: energy: high VIRGO LIGO VHE gravitational radiation detector experimental equipment experimental methods experimental results statistical analysis data analysis method [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph] de Wasseige, Gwenhael Kouchner, Antoine Colomer Molla, Marta Dornic, Damien Hallmann, Steffen Sensitivity for astrophysical neutrino searches with KM3NeT-ORCA |
topic_facet |
neutrino: oscillation neutrino: atmosphere neutrino: detector detector: sensitivity KM3NeT gravitational radiation neutrino: energy: high VIRGO LIGO VHE gravitational radiation detector experimental equipment experimental methods experimental results statistical analysis data analysis method [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph] |
description |
International audience The KM3NeT facility, the next generation of large neutrino detectors, is currently being deployedin the Mediterranean Sea. KM3NeT will consist of two ARCA ("Astroparticle Research withCosmics in the Abyss") building blocks, optimized for very high-energy astrophysical neutrinos,and of the ORCA one ("Oscillation Research with Cosmics in the Abyss"). While ORCA hasoriginally been designed to study neutrino oscillations using atmospheric neutrinos, this densearray may also be used for astrophysical neutrino searches. We present a first estimate of thesensitivity for GeV–100GeV neutrino searches in time/space coincidence with GW alerts sentby the LIGO and Virgo collaborations (LVC). We use the final configuration of ORCA, i.e.ORCA-115 detection units, to estimate the sensitivity of ORCA to gravitational wave events thatmay be detected by LVC during O3. |
author2 |
AstroParticule et Cosmologie (APC (UMR_7164)) Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris Université Paris Sciences et Lettres (PSL)-Université Paris Sciences et Lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité) 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 |
de Wasseige, Gwenhael Kouchner, Antoine Colomer Molla, Marta Dornic, Damien Hallmann, Steffen |
author_facet |
de Wasseige, Gwenhael Kouchner, Antoine Colomer Molla, Marta Dornic, Damien Hallmann, Steffen |
author_sort |
de Wasseige, Gwenhael |
title |
Sensitivity for astrophysical neutrino searches with KM3NeT-ORCA |
title_short |
Sensitivity for astrophysical neutrino searches with KM3NeT-ORCA |
title_full |
Sensitivity for astrophysical neutrino searches with KM3NeT-ORCA |
title_fullStr |
Sensitivity for astrophysical neutrino searches with KM3NeT-ORCA |
title_full_unstemmed |
Sensitivity for astrophysical neutrino searches with KM3NeT-ORCA |
title_sort |
sensitivity for astrophysical neutrino searches with km3net-orca |
publisher |
HAL CCSD |
publishDate |
2019 |
url |
https://hal.science/hal-02507600 https://hal.science/hal-02507600/document https://hal.science/hal-02507600/file/4-poster-NMO_ICRC_2019-GDW_infradev.pdf https://doi.org/10.22323/1.358.0934 |
op_coverage |
Madison, United States |
genre |
Orca |
genre_facet |
Orca |
op_source |
PoS 36th International Cosmic Ray Conference https://hal.science/hal-02507600 36th International Cosmic Ray Conference, Jul 2019, Madison, United States. pp.934, ⟨10.22323/1.358.0934⟩ |
op_relation |
info:eu-repo/semantics/altIdentifier/doi/10.22323/1.358.0934 hal-02507600 https://hal.science/hal-02507600 https://hal.science/hal-02507600/document https://hal.science/hal-02507600/file/4-poster-NMO_ICRC_2019-GDW_infradev.pdf doi:10.22323/1.358.0934 INSPIRE: 1785096 |
op_rights |
info:eu-repo/semantics/OpenAccess |
op_doi |
https://doi.org/10.22323/1.358.0934 |
container_title |
Proceedings of 36th International Cosmic Ray Conference — PoS(ICRC2019) |
container_start_page |
934 |
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1799486972254748672 |