Results from the AMANDA detector

Philip Olbrechts,A. C. Pohl,Elisa Bernardini,J. W. Nam,R. Hardtke,L. Gerhardt,Adam Bouchta,Kyle T. Mandli,L. Köpke,P. Ekström,R. Ganugapati,D. Steele,D. F. Cowen,H. Wissing,J. Braun,H. Albrecht,Francis Halzen,P. Desiati,Jan Conrad, Torsten Harenberg,K. Rawlins, P. Niessen,A. Gross,Anna Davour, L. Thollander,Heiko Geenen,C. De Clercq,M. Bartelt,A. Silvestri,C.P. Burgess, S. Boeser,J. Rodríguez Martino,C. Pérez de los Heros, R. Wischnewski,Olga Botner,David A. Schneider,D. J. Boersma,R. Porrata,Karl-Heinz Kampert,J. E. Jacobsen,P. Steffen, Ph. Herquet, D.R. Nygren,Kael Hanson,H. Leich,G.M. Spiczak,T. Feser,Othmane Bouhali,Dmitry Chirkin, C.P. McParland,J. L. Kelley,Hakki Ögelman, Wolfgang Rhode,S. Schlenstedt,K. Woschnagg,Wolfgang Wagner,T. Neunhöffer,H. G. Sander,M. Solarz, Klas Hultqvist,Y. Minaeva, I. Liubarsky,I. Taboada,R. Morse,R. C. Bay, T. Castermans,D. Hubert,Matthias Leuthold, B. Hughey,M. Hellwig,Albrecht Karle,A. Goldschmidt,Marek Kowalski, M. Stamatikos,Markus Ackermann,A. Hallgren, M. Walter,Thomas K. Gaisser,G. C. Hill,R.G. Stokstad,G. Yodh,D. Bertrand,P. O. Hulth,T. DeYoung,Xinhua Bai,C. Walck, T. Becka,P. Miocinovic,K. H. Becker, R. Nahnhauer,C. Spiering,K. Helbing, T. Messarius,G. T. Przybylski,Jens Madsen,B. Collin,S. Richter,J.K. Becker,R. Schwarz,M. Krasberg

Acta Physica Polonica B（2004）

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摘要

Author(s): Olbrechts, Philip; Barwick, S. W.; Gerhardt, L.; Kuehn, K.; Nam, J. W.; Silvestri, A.; Yodh, G.; AMANDA Collaboration, . | Abstract: The Antarctic Muon And Neutrino Detector Array (AMANDA) is a high-energy neutrino telescope based at the geographic South Pole. It is a lattice of photo-multiplier tubes buried deep in the polar ice, which is used as interaction and detection medium. The primary goal of this detector is the observation of astronomical sources of high-energy neutrinos. This paper shows the latest results of the search for a diffuse flux of extraterrestrial v(mu)s with energies between 10(11) eV and 10(18) eV, v(mu)s emitted from point sources and v(mu)s from dark matter annihilation in the Earth and the Sun.∗ Presented at the Cracow Epiphany Conference on Astroparticle Physics, Cracow, Poland, January 8–11, 2004.

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