Recent Results from the AMANDA Experiment

• Main Authors: Niessen, P, Ahrens, J, Bai, X, Barwick, S W, Becka, T, Becker, J K, Becker, K H, Bernardini, E, Bertrand, D, Binon, Freddy G, Biron, A, Boersma, D J, Boser, S, Botner, O, Bouchta, A, Bouhali, O, Burgess, T, Carius, S, Castermans, T, Chen, A, Chirkin, D, Collin, B, Conrad, J, Cooley, J, Cowen, D F, Davour, A, De Clercq, C, De Young, T R, Desiati, P, Dewulf, J P, Doksus, P, Ekstrom, P, Feser, T, Gaisser, T K, Ganugapati, R, Geenen, H, Gerhardt, L, Goldmann, K S, Goldschmidt, A, Gross, A, Hallgren, A, Halzen, F, Hanson, K, Hardtke, R, Hauschildt, T, Helbing, K, Hellwig, M, Herquet, P, Hill, G C, Hubert, D, Hughey, B, Hulth, P O, Hultqvist, K, Hundertmark, S, Jacobsen, J, Karle, A, Kestel, M, Köpke, L, Kowalski, M, Kühn, K, Lamoureux, J I, Leich, H, Leuthold, M J, Lindahl, P, Liubarsky, I, Madsen, J, Mandli, K, Marciniewski, P, Matis, H S, McParland, C P, Messarius, T, Minaeva, Y, Miocinovic, P, Morse, R, Nahnhauer, R, Nam, J, Neunhoffer, T, Nygren, D R, Ögelman, H B, Olbrechts, P, Pérez de los Heros, C, Pohl, A C, Price, P B, Przybylski, G T, Rawlins, K, Resconi, E, Rhode, W, Ribordy, M, Richter, S, Rodríguez-Martino, J, Ross, D, Sander, H G, Schirinakis, K, Schlenstedt, S, Schmidt, T, Schneider, D, Schwarz, R, Silvestri, A, Solarz, M, Spiczak, G M, Spiering, C, Stamatikos, M, Steele, D, Steffen, P, Stokstad, R G, Sulanke, K H, Taboada, I, Thollander, L, Tilav, S, Wagner, W, Walck, C, Wang, Y R, Wiebusch, C, Wiedemann, C, Wischnewski, R, Wissing, H, Woschnagg, K, Yodh, G B
• Language: English
• Published: 2003
• Subjects: Astrophysics and Astronomy; Antarctic; Antarc*
• Online Access: http://cds.cern.ch/record/620709

AMANDA (Antarctic Muon And Neutrino Detector Array) is a neutrino telescope built under the southern polar icecap and its scope is to explore the possibility to detect high energy cosmic neutrinos. This should generate insight into the powerful celestial objects where acceleration mechanisms can bring up to $10^{20}$ eV. We describe the achievements and results from the AMANDA-B10 prototype and the preliminary results from the current AMANDA-II detector which show dramatic increase in sensitivity.