id ftunivaixmarseil:oai:HAL:hal-02966274v1
record_format openpolar
spelling ftunivaixmarseil:oai:HAL:hal-02966274v1 2024-05-12T08:09:30+00:00 Search for Sterile Neutrinos with KM3NeT/ORCA Domi, Alba Coelho, Joao 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) Laboratoire de l'Accélérateur Linéaire (LAL) Université Paris-Sud - Paris 11 (UP11)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS) KM3NeT ANTARES Madison, United States 2019-07-24 https://hal.science/hal-02966274 https://doi.org/10.22323/1.358.0870 en eng HAL CCSD info:eu-repo/semantics/altIdentifier/doi/10.22323/1.358.0870 hal-02966274 https://hal.science/hal-02966274 doi:10.22323/1.358.0870 INSPIRE: 1819144 PoS 36th International Cosmic Ray Conference https://hal.science/hal-02966274 36th International Cosmic Ray Conference, Jul 2019, Madison, United States. pp.870, ⟨10.22323/1.358.0870⟩ neutrino: detector neutrino: sterile neutrino: oscillation neutrino: atmosphere neutrino: sterile: search for neutrino: energy: low ANTARES KM3NeT exotic sensitivity [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 2019 ftunivaixmarseil https://doi.org/10.22323/1.358.0870 2024-04-18T00:33:33Z International audience Neutrino Telescopes such as ANTARES and KM3NeT are promising candidates to probe exotic oscillation phenomena such as sterile neutrinos. ANTARES (Astronomy with a Neutrino Telescope and Abyss Environmental RESearch) is the largest deep-sea neutrino telescope in operation, covering an area of 0.01 km3 and taking data since 2007. KM3NeT in totality is much more extended than ANTARES and it is under construction in the Mediterranean Sea. When completed, it will consist of two separate detectors: ARCA (Astroparticle Research with Cosmics in the Abyss), optimised for high-energy neutrino astronomy, and ORCA (Oscillation Research with Cosmics in the Abyss) for neutrino oscillation studies with atmospheric neutrinos. ORCA will have an effective mass of 8 Mtons and a low neutrino energy detection threshold of 1 GeV. For this reason it is a promising candidate to study neutrinos properties. Here we present the upper limits from ANTARES and sensitivities of ORCA to sterile neutrinos in the (3+1) model. Conference Object Orca Aix-Marseille Université: HAL Proceedings of 36th International Cosmic Ray Conference — PoS(ICRC2019) 870
institution Open Polar
collection Aix-Marseille Université: HAL
op_collection_id ftunivaixmarseil
language English
topic neutrino: detector
neutrino: sterile
neutrino: oscillation
neutrino: atmosphere
neutrino: sterile: search for
neutrino: energy: low
ANTARES
KM3NeT
exotic
sensitivity
[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]
spellingShingle neutrino: detector
neutrino: sterile
neutrino: oscillation
neutrino: atmosphere
neutrino: sterile: search for
neutrino: energy: low
ANTARES
KM3NeT
exotic
sensitivity
[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]
Domi, Alba
Coelho, Joao
Search for Sterile Neutrinos with KM3NeT/ORCA
topic_facet neutrino: detector
neutrino: sterile
neutrino: oscillation
neutrino: atmosphere
neutrino: sterile: search for
neutrino: energy: low
ANTARES
KM3NeT
exotic
sensitivity
[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 Neutrino Telescopes such as ANTARES and KM3NeT are promising candidates to probe exotic oscillation phenomena such as sterile neutrinos. ANTARES (Astronomy with a Neutrino Telescope and Abyss Environmental RESearch) is the largest deep-sea neutrino telescope in operation, covering an area of 0.01 km3 and taking data since 2007. KM3NeT in totality is much more extended than ANTARES and it is under construction in the Mediterranean Sea. When completed, it will consist of two separate detectors: ARCA (Astroparticle Research with Cosmics in the Abyss), optimised for high-energy neutrino astronomy, and ORCA (Oscillation Research with Cosmics in the Abyss) for neutrino oscillation studies with atmospheric neutrinos. ORCA will have an effective mass of 8 Mtons and a low neutrino energy detection threshold of 1 GeV. For this reason it is a promising candidate to study neutrinos properties. Here we present the upper limits from ANTARES and sensitivities of ORCA to sterile neutrinos in the (3+1) model.
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)
Laboratoire de l'Accélérateur Linéaire (LAL)
Université Paris-Sud - Paris 11 (UP11)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)
KM3NeT
ANTARES
format Conference Object
author Domi, Alba
Coelho, Joao
author_facet Domi, Alba
Coelho, Joao
author_sort Domi, Alba
title Search for Sterile Neutrinos with KM3NeT/ORCA
title_short Search for Sterile Neutrinos with KM3NeT/ORCA
title_full Search for Sterile Neutrinos with KM3NeT/ORCA
title_fullStr Search for Sterile Neutrinos with KM3NeT/ORCA
title_full_unstemmed Search for Sterile Neutrinos with KM3NeT/ORCA
title_sort search for sterile neutrinos with km3net/orca
publisher HAL CCSD
publishDate 2019
url https://hal.science/hal-02966274
https://doi.org/10.22323/1.358.0870
op_coverage Madison, United States
genre Orca
genre_facet Orca
op_source PoS
36th International Cosmic Ray Conference
https://hal.science/hal-02966274
36th International Cosmic Ray Conference, Jul 2019, Madison, United States. pp.870, ⟨10.22323/1.358.0870⟩
op_relation info:eu-repo/semantics/altIdentifier/doi/10.22323/1.358.0870
hal-02966274
https://hal.science/hal-02966274
doi:10.22323/1.358.0870
INSPIRE: 1819144
op_doi https://doi.org/10.22323/1.358.0870
container_title Proceedings of 36th International Cosmic Ray Conference — PoS(ICRC2019)
container_start_page 870
_version_ 1798852766415716352