Neutrino Telescopes: a Review

Neutrino astronomy is an interesting way to probe deep Universe. Indeed, despite their great success, photon observations in astrophysics suffer from limitations due to photon interaction at high energy, while cosmic ray observations are impaired by GZK effect at high energies and by proton deflecti...

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Main Author: Ernenwein, J.-P.
Other Authors: 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), ANTARES
Format: Conference Object
Language:English
Published: HAL CCSD 2011
Subjects:
Online Access:https://hal.in2p3.fr/in2p3-00684677
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spelling ftunivaixmarseil:oai:HAL:in2p3-00684677v1 2024-05-12T08:11:14+00:00 Neutrino Telescopes: a Review Ernenwein, J.-P. 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) ANTARES Come, Italy 2011-10-03 https://hal.in2p3.fr/in2p3-00684677 en eng HAL CCSD in2p3-00684677 https://hal.in2p3.fr/in2p3-00684677 13th ICATPP Conference on Astroparticle, Particle, Space Physics and Detectors for Physics Applications https://hal.in2p3.fr/in2p3-00684677 13th ICATPP Conference on Astroparticle, Particle, Space Physics and Detectors for Physics Applications, Oct 2011, Come, Italy [SDU.ASTR.CO]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO] [PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO] [SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE] [PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE] [SDU.ASTR.IM]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM] [PHYS.ASTR.IM]Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM] info:eu-repo/semantics/conferenceObject Conference papers 2011 ftunivaixmarseil 2024-04-18T00:24:13Z Neutrino astronomy is an interesting way to probe deep Universe. Indeed, despite their great success, photon observations in astrophysics suffer from limitations due to photon interaction at high energy, while cosmic ray observations are impaired by GZK effect at high energies and by proton deflection in magnetic fields at low energies. A neutrino telescope is based on Cherenkov light detection: the neutrino interaction inside large volumes of matter surrounding the detector produces charged particles leading to Cherenkov photon emission in ice or water. A neutrino telescope is an assembly of photomultipliers observing the darkness of deep‐sea or ice, and waiting for light produced by muons or showers induced by cosmic neutrinos. Several neutrino telescopes are in operation in the World: ICECUBE in the ice of the South Pole, BAIKAL in the Baikal lake, ANTARES in the Mediterranean sea. A project of a Mediterranean cubic‐kilometre‐scale neutrino telescope is under study: KM3NeT. With an instrumented volume of about 5 km3, it will have an unsurpassed sensitivity and angular resolution ‐down to 0.1 degrees at 100 TeV. We will present the characteristics of these experiments, as well as the results of their observations and expected performances. Conference Object South pole Aix-Marseille Université: HAL South Pole
institution Open Polar
collection Aix-Marseille Université: HAL
op_collection_id ftunivaixmarseil
language English
topic [SDU.ASTR.CO]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]
[PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]
[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]
[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]
[SDU.ASTR.IM]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]
[PHYS.ASTR.IM]Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]
spellingShingle [SDU.ASTR.CO]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]
[PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]
[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]
[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]
[SDU.ASTR.IM]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]
[PHYS.ASTR.IM]Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]
Ernenwein, J.-P.
Neutrino Telescopes: a Review
topic_facet [SDU.ASTR.CO]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]
[PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]
[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]
[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]
[SDU.ASTR.IM]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]
[PHYS.ASTR.IM]Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]
description Neutrino astronomy is an interesting way to probe deep Universe. Indeed, despite their great success, photon observations in astrophysics suffer from limitations due to photon interaction at high energy, while cosmic ray observations are impaired by GZK effect at high energies and by proton deflection in magnetic fields at low energies. A neutrino telescope is based on Cherenkov light detection: the neutrino interaction inside large volumes of matter surrounding the detector produces charged particles leading to Cherenkov photon emission in ice or water. A neutrino telescope is an assembly of photomultipliers observing the darkness of deep‐sea or ice, and waiting for light produced by muons or showers induced by cosmic neutrinos. Several neutrino telescopes are in operation in the World: ICECUBE in the ice of the South Pole, BAIKAL in the Baikal lake, ANTARES in the Mediterranean sea. A project of a Mediterranean cubic‐kilometre‐scale neutrino telescope is under study: KM3NeT. With an instrumented volume of about 5 km3, it will have an unsurpassed sensitivity and angular resolution ‐down to 0.1 degrees at 100 TeV. We will present the characteristics of these experiments, as well as the results of their observations and expected performances.
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)
ANTARES
format Conference Object
author Ernenwein, J.-P.
author_facet Ernenwein, J.-P.
author_sort Ernenwein, J.-P.
title Neutrino Telescopes: a Review
title_short Neutrino Telescopes: a Review
title_full Neutrino Telescopes: a Review
title_fullStr Neutrino Telescopes: a Review
title_full_unstemmed Neutrino Telescopes: a Review
title_sort neutrino telescopes: a review
publisher HAL CCSD
publishDate 2011
url https://hal.in2p3.fr/in2p3-00684677
op_coverage Come, Italy
geographic South Pole
geographic_facet South Pole
genre South pole
genre_facet South pole
op_source 13th ICATPP Conference on Astroparticle, Particle, Space Physics and Detectors for Physics Applications
https://hal.in2p3.fr/in2p3-00684677
13th ICATPP Conference on Astroparticle, Particle, Space Physics and Detectors for Physics Applications, Oct 2011, Come, Italy
op_relation in2p3-00684677
https://hal.in2p3.fr/in2p3-00684677
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