Cargando…

Status of the ANTARES Project

The ANTARES collaboration is constructing a neutrino telescope in the Mediterranean Sea at a depth of 2400 metres, about 40 kilometres off the French coast near Toulon. The detector will consist of 12 vertical strings anchored at the sea bottom, each supporting 25 triplets of optical modules equippe...

Descripción completa

Detalles Bibliográficos
Autor principal: Katz, U F
Lenguaje:eng
Publicado: 2003
Materias:
Acceso en línea:https://dx.doi.org/10.1140/epjcd/s2004-03-1755-x
http://cds.cern.ch/record/678806
_version_ 1780901022779047936
author Katz, U F
author_facet Katz, U F
author_sort Katz, U F
collection CERN
description The ANTARES collaboration is constructing a neutrino telescope in the Mediterranean Sea at a depth of 2400 metres, about 40 kilometres off the French coast near Toulon. The detector will consist of 12 vertical strings anchored at the sea bottom, each supporting 25 triplets of optical modules equipped with photomultipliers, yielding sensitivity to neutrinos with energies above some 10 GeV. The effective detector area is roughly 0.1 square kilometres for neutrino energies exceeding 10 TeV. The measurement of the Cherenkov light emitted by muons produced in muon-neutrino charged-current interactions in water and under-sea rock will permit the reconstruction of the neutrino direction with an accuracy of better than 0.3 degrees at high energies. ANTARES will complement the field of view of neutrino telescopes at the South Pole in the low-background searches for point-sources of high-energy cosmic neutrinos and will also be sensitive to neutrinos produced by WIMP annihilation in the Sun or the Galactic centre.
id cern-678806
institution Organización Europea para la Investigación Nuclear
language eng
publishDate 2003
record_format invenio
spelling cern-6788062019-09-30T06:29:59Zdoi:10.1140/epjcd/s2004-03-1755-xhttp://cds.cern.ch/record/678806engKatz, U FStatus of the ANTARES ProjectAstrophysics and AstronomyThe ANTARES collaboration is constructing a neutrino telescope in the Mediterranean Sea at a depth of 2400 metres, about 40 kilometres off the French coast near Toulon. The detector will consist of 12 vertical strings anchored at the sea bottom, each supporting 25 triplets of optical modules equipped with photomultipliers, yielding sensitivity to neutrinos with energies above some 10 GeV. The effective detector area is roughly 0.1 square kilometres for neutrino energies exceeding 10 TeV. The measurement of the Cherenkov light emitted by muons produced in muon-neutrino charged-current interactions in water and under-sea rock will permit the reconstruction of the neutrino direction with an accuracy of better than 0.3 degrees at high energies. ANTARES will complement the field of view of neutrino telescopes at the South Pole in the low-background searches for point-sources of high-energy cosmic neutrinos and will also be sensitive to neutrinos produced by WIMP annihilation in the Sun or the Galactic centre.astro-ph/0310736FAU-PI-1-2003-01oai:cds.cern.ch:6788062003-10-26
spellingShingle Astrophysics and Astronomy
Katz, U F
Status of the ANTARES Project
title Status of the ANTARES Project
title_full Status of the ANTARES Project
title_fullStr Status of the ANTARES Project
title_full_unstemmed Status of the ANTARES Project
title_short Status of the ANTARES Project
title_sort status of the antares project
topic Astrophysics and Astronomy
url https://dx.doi.org/10.1140/epjcd/s2004-03-1755-x
http://cds.cern.ch/record/678806
work_keys_str_mv AT katzuf statusoftheantaresproject