Indirect Dark Matter search with large neutrino telescopes

Dark matter is one of the main goals of neutrino astronomy. At present, there are two big neutrino telescopes based on the Cherenkov technique in ice and water: IceCube at the South Pole and ANTARES in the northern hemisphere. Both telescopes are performing an indirect search for Dark Matter by look...

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Bibliographic Details
Main Author: Fermani, Paolo
Format: Text
Language:unknown
Published: arXiv 2013
Subjects:
High Energy Astrophysical Phenomena astro-ph.HE
FOS Physical sciences
South Pole
South pole
Online Access:https://dx.doi.org/10.48550/arxiv.1307.2402
https://arxiv.org/abs/1307.2402
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spelling ftdatacite:10.48550/arxiv.1307.2402 2023-05-15T18:22:23+02:00 Indirect Dark Matter search with large neutrino telescopes Fermani, Paolo 2013 https://dx.doi.org/10.48550/arxiv.1307.2402 https://arxiv.org/abs/1307.2402 unknown arXiv arXiv.org perpetual, non-exclusive license http://arxiv.org/licenses/nonexclusive-distrib/1.0/ High Energy Astrophysical Phenomena astro-ph.HE FOS Physical sciences article-journal Article ScholarlyArticle Text 2013 ftdatacite https://doi.org/10.48550/arxiv.1307.2402 2022-04-01T13:11:57Z Dark matter is one of the main goals of neutrino astronomy. At present, there are two big neutrino telescopes based on the Cherenkov technique in ice and water: IceCube at the South Pole and ANTARES in the northern hemisphere. Both telescopes are performing an indirect search for Dark Matter by looking for a statistical excess of neutrinos coming from astrophysical massive objects. This excess could be an evidence of the possible annihilation of dark matter particles in the centre of these objects. In one of the most popular scenarios the Dark Matter is composed of WIMP particles. The analysis and results of the ANTARES neutrino telescope for the indirect detection of Dark Matter fluxes from the Sun are here presented, as well as the latest IceCube published sensitivity results, for different Dark Matter models. : 13 pages, 6 figures, published proceeding of the conference DARK 2012, Frascati (Italy) Text 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 unknown
topic High Energy Astrophysical Phenomena astro-ph.HE
FOS Physical sciences
spellingShingle High Energy Astrophysical Phenomena astro-ph.HE
FOS Physical sciences
Fermani, Paolo
Indirect Dark Matter search with large neutrino telescopes
topic_facet High Energy Astrophysical Phenomena astro-ph.HE
FOS Physical sciences
description Dark matter is one of the main goals of neutrino astronomy. At present, there are two big neutrino telescopes based on the Cherenkov technique in ice and water: IceCube at the South Pole and ANTARES in the northern hemisphere. Both telescopes are performing an indirect search for Dark Matter by looking for a statistical excess of neutrinos coming from astrophysical massive objects. This excess could be an evidence of the possible annihilation of dark matter particles in the centre of these objects. In one of the most popular scenarios the Dark Matter is composed of WIMP particles. The analysis and results of the ANTARES neutrino telescope for the indirect detection of Dark Matter fluxes from the Sun are here presented, as well as the latest IceCube published sensitivity results, for different Dark Matter models. : 13 pages, 6 figures, published proceeding of the conference DARK 2012, Frascati (Italy)
format Text
author Fermani, Paolo
author_facet Fermani, Paolo
author_sort Fermani, Paolo
title Indirect Dark Matter search with large neutrino telescopes
title_short Indirect Dark Matter search with large neutrino telescopes
title_full Indirect Dark Matter search with large neutrino telescopes
title_fullStr Indirect Dark Matter search with large neutrino telescopes
title_full_unstemmed Indirect Dark Matter search with large neutrino telescopes
title_sort indirect dark matter search with large neutrino telescopes
publisher arXiv
publishDate 2013
url https://dx.doi.org/10.48550/arxiv.1307.2402
https://arxiv.org/abs/1307.2402
geographic South Pole
geographic_facet South Pole
genre South pole
genre_facet South pole
op_rights arXiv.org perpetual, non-exclusive license
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
op_doi https://doi.org/10.48550/arxiv.1307.2402
_version_ 1766201788791259136

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