Observation of high energy atmospheric neutrinos with AMANDA

Karle, A.; Andres, E.; Askebjer, P.; Bai, X.; Barouch, G.; Barwick, S. W.; Bay, R. C.; Becker, K.-H.; Bergström, L.; Bertrand, D.; Bierenbaum, D.; Biron, A.; Booth, J.; Botner, O.; Bouchta, A.; Boyce, M. M.; Carius, S.; Chen, A.; Chirkin, D.; Conrad, J.; Cooley, J.; Costa, C. G. S.; Cowen, D. F.; Dailing, J.; Dalberg, E.; DeYoung, T.; Desiati, P.; Dewulf, J.-P.; Doksus, P.; Edsjö, J.; Ekström, P.; Erlandsson, B.; Feser, T.; Gaug, M.; Goldschmidt, A.; Goobar, A.; Gray, L.; Haase, H.; Hallgren, A.; Halzen, F.; Hanson, K.; Hardtke, R.; He, Y. D.; Hellwig, M.; Heukenkamp, H.; Hill, G. C.; Hulth, P. O.; Hundertmark, S.; Jacobsen, J.; Kandhadai, V.; Kim, J.; Koci, B.; Köpke, L.; Kowalski, M.; Leich, H.; Leuthold, M.; Lindahl, P.; Liubarsky, I.; Loaiza, P.; Lowder, D. M.; Ludvig, J.; Madsen, J.; Marciniewski, P.; Matis, H. S.; Mihalyi, A.; Mikolajski, T.; Miller, T. C.; Minaeva, Y.; Miocinovic, P.; Mock, P. C.; Morse, R.; Neunhöffer, T.; Newcomer, F. M.; Niessen, P.; Nygren, D. R.; Ogelman, H.; de los Heros, C. Pérez; Porrata, R.; Price, P. B.; Rawlins, K.; Reed, C.; Rhode, W.; Richards, A.; Richter, S.; Martino, J. Rodriguez; Romenesko, P.; Ross, D.; Rubinstein, H.; Sander, H.-G.; Scheider, T.; Schmidt, T.; Schneider, D.; Schneider, E.; Schwarz, R.; Silvestri, A.; Solarz, M.; Spiczak, G.; Spiering, C.; Starinsky, N.; Steele, D.; Steffen, P.; Stokstad, R. G.; Streicher, O.; Sun, Q.; Taboada, I.; Thollander, L.; Thon, T.; Tilav, S.; Usechak, N.; Donckt, M. Vander; Walck, C.; Weinheimer, C.; Wiebusch, C. H.; Wischnewski, R.; Woschnagg, K.; Wu, W.; Yodh, G.; Young, S.

doi:10.1063/1.1345374

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Research Article| December 12 2000

Observation of high energy atmospheric neutrinos with AMANDA

A. Karle;

A. Karle

11Department of Physics, University of Wisconsin, Madison, Wisconsin

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11Department of Physics, University of Wisconsin, Madison, Wisconsin

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13Fysikum, Stockholm University, Stockholm, Sweden

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X. Bai;

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1Bartol Research Institute, University of Delaware, Newark, Delaware

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G. Barouch;

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11Department of Physics, University of Wisconsin, Madison, Wisconsin

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8Department of Physics and Astronomy, University of California, Irvine, California

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R. C. Bay;

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7Department of Physics, University of California, Berkeley, California

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K.-H. Becker;

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13Fysikum, Stockholm University, Stockholm, Sweden

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3Brussels Free University, Brussels, Belgium

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8Department of Physics and Astronomy, University of California, Irvine, California

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AIP Conf. Proc. 549, 823–827 (2000)

https://doi.org/10.1063/1.1345374

In 1997 the Antarctic Muon and Neutrino Detector Array (AMANDA) started operating with 10 strings. In an analysis of data taken during the first year of operation 188 atmospheric neutrino candidates were found. Their zenith angle distribution agrees with expectations based on Monte Carlo simulations. A preliminary upper limit is given on a diffuse flux of high energy neutrinos of astrophysical origin.

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