The AMANDA neutrino telescope and the indirect search for dark matter: AMANDA Colaboration

R. C. Bay, Y. He, D. Lowder, P. Miocinovic, P. B. Price, M. Solarz, K. Woschnagg, S. W. Barwick, J. Booth, P. C. Mock, R. Porrata, E. Schneider, G. Yodh, D. Cowen, M. Carlson, C. G.S. Costa, T. Deyoung, L. Gray, F. Halzen, R. HardtkeJ. Jacobsen, V. Kankhadai, A. Karle, I. Liubarsky, R. Morse, S. Tilav, T. C. Miller, E. C. Andrés, P. Askebjer, L. Bergström, A. Bouchta, E. Dalberg, P. Ekström, A. Goobar, P. O. Hulth, C. Walck, A. Hallgren, C. P.De Los Heros, P. Marciniewski, H. Rubinstein, S. Carius, P. Lindahl, A. Biron, S. Hundertmark, M. Leuthold, P. Niessen, C. Spiering, O. Streicher, T. Thon, C. H. Wiebusch, R. Wischnewski, D. Nygren, A. Jones, S. Hart, D. Potter, G. Hill, R. Schwarz

Research output: Contribution to journalArticle

Abstract

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.

Original languageEnglish (US)
Pages (from-to)243-252
Number of pages10
JournalPhysics Report
Volume307
Issue number1-4
DOIs
StatePublished - Dec 1 1998

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dark matter
neutrinos
telescopes
halos
thresholds
detectors
energy

All Science Journal Classification (ASJC) codes

  • Physics and Astronomy(all)

Cite this

Bay, R. C., He, Y., Lowder, D., Miocinovic, P., Price, P. B., Solarz, M., ... Schwarz, R. (1998). The AMANDA neutrino telescope and the indirect search for dark matter: AMANDA Colaboration. Physics Report, 307(1-4), 243-252. https://doi.org/10.1016/S0370-1573(98)00041-6
Bay, R. C. ; He, Y. ; Lowder, D. ; Miocinovic, P. ; Price, P. B. ; Solarz, M. ; Woschnagg, K. ; Barwick, S. W. ; Booth, J. ; Mock, P. C. ; Porrata, R. ; Schneider, E. ; Yodh, G. ; Cowen, D. ; Carlson, M. ; Costa, C. G.S. ; Deyoung, T. ; Gray, L. ; Halzen, F. ; Hardtke, R. ; Jacobsen, J. ; Kankhadai, V. ; Karle, A. ; Liubarsky, I. ; Morse, R. ; Tilav, S. ; Miller, T. C. ; Andrés, E. C. ; Askebjer, P. ; Bergström, L. ; Bouchta, A. ; Dalberg, E. ; Ekström, P. ; Goobar, A. ; Hulth, P. O. ; Walck, C. ; Hallgren, A. ; Heros, C. P.De Los ; Marciniewski, P. ; Rubinstein, H. ; Carius, S. ; Lindahl, P. ; Biron, A. ; Hundertmark, S. ; Leuthold, M. ; Niessen, P. ; Spiering, C. ; Streicher, O. ; Thon, T. ; Wiebusch, C. H. ; Wischnewski, R. ; Nygren, D. ; Jones, A. ; Hart, S. ; Potter, D. ; Hill, G. ; Schwarz, R. / The AMANDA neutrino telescope and the indirect search for dark matter : AMANDA Colaboration. In: Physics Report. 1998 ; Vol. 307, No. 1-4. pp. 243-252.
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Bay, RC, He, Y, Lowder, D, Miocinovic, P, Price, PB, Solarz, M, Woschnagg, K, Barwick, SW, Booth, J, Mock, PC, Porrata, R, Schneider, E, Yodh, G, Cowen, D, Carlson, M, Costa, CGS, Deyoung, T, Gray, L, Halzen, F, Hardtke, R, Jacobsen, J, Kankhadai, V, Karle, A, Liubarsky, I, Morse, R, Tilav, S, Miller, TC, Andrés, EC, Askebjer, P, Bergström, L, Bouchta, A, Dalberg, E, Ekström, P, Goobar, A, Hulth, PO, Walck, C, Hallgren, A, Heros, CPDL, Marciniewski, P, Rubinstein, H, Carius, S, Lindahl, P, Biron, A, Hundertmark, S, Leuthold, M, Niessen, P, Spiering, C, Streicher, O, Thon, T, Wiebusch, CH, Wischnewski, R, Nygren, D, Jones, A, Hart, S, Potter, D, Hill, G & Schwarz, R 1998, 'The AMANDA neutrino telescope and the indirect search for dark matter: AMANDA Colaboration', Physics Report, vol. 307, no. 1-4, pp. 243-252. https://doi.org/10.1016/S0370-1573(98)00041-6

The AMANDA neutrino telescope and the indirect search for dark matter : AMANDA Colaboration. / Bay, R. C.; He, Y.; Lowder, D.; Miocinovic, P.; Price, P. B.; Solarz, M.; Woschnagg, K.; Barwick, S. W.; Booth, J.; Mock, P. C.; Porrata, R.; Schneider, E.; Yodh, G.; Cowen, D.; Carlson, M.; Costa, C. G.S.; Deyoung, T.; Gray, L.; Halzen, F.; Hardtke, R.; Jacobsen, J.; Kankhadai, V.; Karle, A.; Liubarsky, I.; Morse, R.; Tilav, S.; Miller, T. C.; Andrés, E. C.; Askebjer, P.; Bergström, L.; Bouchta, A.; Dalberg, E.; Ekström, P.; Goobar, A.; Hulth, P. O.; Walck, C.; Hallgren, A.; Heros, C. P.De Los; Marciniewski, P.; Rubinstein, H.; Carius, S.; Lindahl, P.; Biron, A.; Hundertmark, S.; Leuthold, M.; Niessen, P.; Spiering, C.; Streicher, O.; Thon, T.; Wiebusch, C. H.; Wischnewski, R.; Nygren, D.; Jones, A.; Hart, S.; Potter, D.; Hill, G.; Schwarz, R.

In: Physics Report, Vol. 307, No. 1-4, 01.12.1998, p. 243-252.

Research output: Contribution to journalArticle

TY - JOUR

T1 - The AMANDA neutrino telescope and the indirect search for dark matter

T2 - AMANDA Colaboration

AU - Bay, R. C.

AU - He, Y.

AU - Lowder, D.

AU - Miocinovic, P.

AU - Price, P. B.

AU - Solarz, M.

AU - Woschnagg, K.

AU - Barwick, S. W.

AU - Booth, J.

AU - Mock, P. C.

AU - Porrata, R.

AU - Schneider, E.

AU - Yodh, G.

AU - Cowen, D.

AU - Carlson, M.

AU - Costa, C. G.S.

AU - Deyoung, T.

AU - Gray, L.

AU - Halzen, F.

AU - Hardtke, R.

AU - Jacobsen, J.

AU - Kankhadai, V.

AU - Karle, A.

AU - Liubarsky, I.

AU - Morse, R.

AU - Tilav, S.

AU - Miller, T. C.

AU - Andrés, E. C.

AU - Askebjer, P.

AU - Bergström, L.

AU - Bouchta, A.

AU - Dalberg, E.

AU - Ekström, P.

AU - Goobar, A.

AU - Hulth, P. O.

AU - Walck, C.

AU - Hallgren, A.

AU - Heros, C. P.De Los

AU - Marciniewski, P.

AU - Rubinstein, H.

AU - Carius, S.

AU - Lindahl, P.

AU - Biron, A.

AU - Hundertmark, S.

AU - Leuthold, M.

AU - Niessen, P.

AU - Spiering, C.

AU - Streicher, O.

AU - Thon, T.

AU - Wiebusch, C. H.

AU - Wischnewski, R.

AU - Nygren, D.

AU - Jones, A.

AU - Hart, S.

AU - Potter, D.

AU - Hill, G.

AU - Schwarz, R.

PY - 1998/12/1

Y1 - 1998/12/1

N2 - 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.

AB - 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.

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UR - http://www.scopus.com/inward/citedby.url?scp=0039500250&partnerID=8YFLogxK

U2 - 10.1016/S0370-1573(98)00041-6

DO - 10.1016/S0370-1573(98)00041-6

M3 - Article

AN - SCOPUS:0039500250

VL - 307

SP - 243

EP - 252

JO - Physics Reports

JF - Physics Reports

SN - 0370-1573

IS - 1-4

ER -