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The AMANDA neutrino telescope and the indirect search for dark matter: AMANDA Colaboration
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1998 (English)In: Physics reports, ISSN 0370-1573, E-ISSN 1873-6270, Vol. 307, no 1-4, 243-252 p.Article in journal (Refereed) Published
Abstract [en]

With an effective telescope area of order 104m2, a threshold of ~50GeV and a pointing accuracy of 2.5°, the AMANDA detector represents the first of a new generation of high energy neutrino telescopes, reaching a scale envisaged over 25 years ago. We describe its performance, focussing on the capability to detect halo dark matter particles via their annihilation into neutrinos.

Place, publisher, year, edition, pages
Elsevier, 1998. Vol. 307, no 1-4, 243-252 p.
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Physical Sciences
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URN: urn:nbn:se:lnu:diva-28467DOI: 10.1016/S0370-1573(98)00041-6OAI: oai:DiVA.org:lnu-28467DiVA: diva2:643951
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Source: Scopus

Available from: 2013-08-29 Created: 2013-08-26 Last updated: 2017-12-06Bibliographically approved

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Carius, Staffan

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