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. Hardtke; J. 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

doi:10.1016/S0370-1573(98)00041-6

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

Physics and Astronomy (Twin Cities)

Research output: Contribution to journal › Article › peer-review

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 language	English (US)
Pages (from-to)	243-252
Number of pages	10
Journal	Physics Report
Volume	307
Issue number	1-4
DOIs	https://doi.org/10.1016/S0370-1573(98)00041-6
State	Published - Dec 1 1998

Bibliographical note

Funding Information:
The AMANDA collaboration is indebted to the Polar Ice Coring Office and to Bruce Koci for the successful drilling operations, and to the National Science Foundation (USA), the Swedish National Research Council, the K.A. Wallenberg Foundation and the Swedish Polar Research Secretariat. F.H. was supported in part by the U.S. Department of Energy under Grant No. DE-FG02-95ER40896 and in part by the University of Wisconsin Research Committee with funds granted by the Wisconsin Alumni Research Foundation.

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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., ... 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, 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

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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.",

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author = "Bay, {R. C.} and Y. He and D. Lowder and P. Miocinovic and Price, {P. B.} and M. Solarz and K. Woschnagg and Barwick, {S. W.} and J. Booth and Mock, {P. C.} and R. Porrata and E. Schneider and G. Yodh and D. Cowen and M. Carlson and Costa, {C. G S} and T. Deyoung and L. Gray and F. Halzen and R. Hardtke and J. Jacobsen and V. Kankhadai and A. Karle and I. Liubarsky and R. Morse and S. Tilav and Miller, {T. C.} and Andr{\'e}s, {E. C.} and P. Askebjer and L. Bergstr{\"o}m and A. Bouchta and E. Dalberg and P. Ekstr{\"o}m and A. Goobar and Hulth, {P. O.} and C. Walck and A. Hallgren and Heros, {C. P De Los} and P. Marciniewski and H. Rubinstein and S. Carius and P. Lindahl and A. Biron and S. Hundertmark and M. Leuthold and P. Niessen and C. Spiering and O. Streicher and T. Thon and Wiebusch, {C. H.} and R. Wischnewski and D. Nygren and A. Jones and S. Hart and D. Potter and G. Hill and R. Schwarz",

note = "Funding Information: The AMANDA collaboration is indebted to the Polar Ice Coring Office and to Bruce Koci for the successful drilling operations, and to the National Science Foundation (USA), the Swedish National Research Council, the K.A. Wallenberg Foundation and the Swedish Polar Research Secretariat. F.H. was supported in part by the U.S. Department of Energy under Grant No. DE-FG02-95ER40896 and in part by the University of Wisconsin Research Committee with funds granted by the Wisconsin Alumni Research Foundation.",

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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.

N1 - Funding Information: The AMANDA collaboration is indebted to the Polar Ice Coring Office and to Bruce Koci for the successful drilling operations, and to the National Science Foundation (USA), the Swedish National Research Council, the K.A. Wallenberg Foundation and the Swedish Polar Research Secretariat. F.H. was supported in part by the U.S. Department of Energy under Grant No. DE-FG02-95ER40896 and in part by the University of Wisconsin Research Committee with funds granted by the Wisconsin Alumni Research Foundation.

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.

KW - 95.35+d ■ ■ ■

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

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

SN - 0370-1573

VL - 307

SP - 243

EP - 252

JO - Physics Report

JF - Physics Report

IS - 1-4

ER -

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

Abstract

Bibliographical note

Keywords

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