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Search: (L773:0370 1573 OR L773:1873 6270) srt2:(1995-1999) > (1998) > The AMANDA neutrino...

The AMANDA neutrino telescope and the indirect search for dark matter

Bay, RC (author)
Uppsala universitet,Institutionen för kärn- och partikelfysik
He, Y (author)
Lowder, D (author)
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Miocinovic, P (author)
Price, PB (author)
Solarz, M (author)
Woschnagg, K (author)
Barwick, SW (author)
Booth, J (author)
Mock, PC (author)
Porrata, R (author)
Schneider, E (author)
Yodh, G (author)
Cowen, D (author)
Carlson, M (author)
Costa, CGS (author)
DeYoung, T (author)
Gray, L (author)
Halzen, F (author)
Hardtke, R (author)
Jacobsen, J (author)
Kankhadai, V (author)
Karle, A (author)
Liubarsky, I (author)
Mors, (author)
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 (creator_code:org_t)
ELSEVIER SCIENCE BV, 1998
1998
English.
In: PHYSICS REPORTS-REVIEW SECTION OF PHYSICS LETTERS. - : ELSEVIER SCIENCE BV. - 0370-1573. ; 307:1-4, s. 243-252
  • Journal article (other academic/artistic)
Abstract Subject headings
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  • With an effective telescope area of order 10(4) m(2), a threshold of similar to 50 GeV and a pointing accuracy of 2.5 degrees, the AMANDA detector represents the first of a new generation of high energy neutrino telescopes, reaching a scale envisaged over

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vet (subject category)
art (subject category)

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