High-energy neutrino astronomy with IceCube

The prospect of extending our knowledge of the astrophysical processes in the deepest recesses of the Universe by using neutrinos as astronomical messengers has been a dream of scientists since the 1960s. The vision is finally becoming a reality: the first-generation AMANDA neutrino telescope at the...

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Bibliographic Details
Main Author: Botner, O
Format: Article in Journal/Newspaper
Language:English
Published: CERN 2007
Subjects:
Particle Physics
South Pole
South pole
Online Access:https://dx.doi.org/10.5170/cern-2007-005.253
http://cds.cern.ch/record/1059056
id ftdatacite:10.5170/cern-2007-005.253
record_format openpolar
spelling ftdatacite:10.5170/cern-2007-005.253 2023-05-15T18:22:03+02:00 High-energy neutrino astronomy with IceCube Botner, O 2007 https://dx.doi.org/10.5170/cern-2007-005.253 http://cds.cern.ch/record/1059056 en eng CERN Particle Physics CreativeWork article 2007 ftdatacite https://doi.org/10.5170/cern-2007-005.253 2021-11-05T12:55:41Z The prospect of extending our knowledge of the astrophysical processes in the deepest recesses of the Universe by using neutrinos as astronomical messengers has been a dream of scientists since the 1960s. The vision is finally becoming a reality: the first-generation AMANDA neutrino telescope at the South Pole designed to search for high-energy neutrinos is being upgraded to a kilometre-scale array, IceCube, with a much improved sensitivity. A summary of the results from AMANDA, and the perspectives for IceCube are presented. Article in Journal/Newspaper South pole DataCite Metadata Store (German National Library of Science and Technology) South Pole
institution Open Polar
collection DataCite Metadata Store (German National Library of Science and Technology)
op_collection_id ftdatacite
language English
topic Particle Physics
spellingShingle Particle Physics
Botner, O
High-energy neutrino astronomy with IceCube
topic_facet Particle Physics
description The prospect of extending our knowledge of the astrophysical processes in the deepest recesses of the Universe by using neutrinos as astronomical messengers has been a dream of scientists since the 1960s. The vision is finally becoming a reality: the first-generation AMANDA neutrino telescope at the South Pole designed to search for high-energy neutrinos is being upgraded to a kilometre-scale array, IceCube, with a much improved sensitivity. A summary of the results from AMANDA, and the perspectives for IceCube are presented.
format Article in Journal/Newspaper
author Botner, O
author_facet Botner, O
author_sort Botner, O
title High-energy neutrino astronomy with IceCube
title_short High-energy neutrino astronomy with IceCube
title_full High-energy neutrino astronomy with IceCube
title_fullStr High-energy neutrino astronomy with IceCube
title_full_unstemmed High-energy neutrino astronomy with IceCube
title_sort high-energy neutrino astronomy with icecube
publisher CERN
publishDate 2007
url https://dx.doi.org/10.5170/cern-2007-005.253
http://cds.cern.ch/record/1059056
geographic South Pole
geographic_facet South Pole
genre South pole
genre_facet South pole
op_doi https://doi.org/10.5170/cern-2007-005.253
_version_ 1766201403932409856

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