RECENT RESULTS FROM AMANDA

Autor: W. Wu, E. Schneider, D. M. Lowder, G. C. Hill, D. Schneider, Y. D. He, K. Rawlins, P. Askebjer, P. B. Price, D. Bierenbaum, T. Scheider, T. O. B. Schmidt, James Madsen, M. Hellwig, E. Andres, H. G. Sander, Glenn Spiczak, H. Rubinstein, Kurt Woschnagg, P. Ekström, M. M. Boyce, R. Schwarz, F. M. Newcomer, C. Walck, R. Hardtke, R. Porrata, G. B. Yodh, C. Pérez de los Heros, Albrecht Karle, I. Liubarsky, A. Mihalyi, Staffan Carius, P. Lindahl, R. C. Bay, P. Niessen, S. Young, P. Romenesko, Ariel Goobar, Christian Spiering, N. Starinsky, B. Erlandsson, H. S. Matis, D. Steele, D. F. Cowen, D. Chirkin, S. Hundertmark, A. Biron, Stefan Richter, Marek Kowalski, M. Solarz, T. Mikolajski, S. Tilav, H. Heukenkamp, P. C. Mock, P. Miocinovic, C. H. Wiebusch, J. Ludvig, D. Ross, K. H. Becker, L. Gray, Xinhua Bai, J. Booth, L. Thollander, A. Silvestri, I. Taboada, R. G. Stokstad, R. Wischnewski, H. Leich, T. C. Miller, R. Morse, J. E. Jacobsen, B. Koci, T. Thon, Lars Bergström, Kael Hanson, J. Rodríguez Martino, Hakki Ögelman, Adam Bouchta, Steven W. Barwick, A. Richards, Francis Halzen, Paolo Desiati, Allan Hallgren, J. P Dewulf, Ole Streicher, T. Neunhöffer, M. Vander Donckt, Olga Botner, V. Kandhadai, Wolfgang Rhode, P. Loaiza, A. Goldschmidt, Y. Minaeva, G. Barouch, M. Gaug, Caroline Costa, Ch. Weinheimer, Matthias Leuthold, D. R. Nygren, P. Steffen, L. Köpke, Jan Conrad, T. Feser, H. Haase, Jodi Cooley, E. Dalberg, D. Bertrand, A. Chen, Joakim Edsjö, Q. Sun, C. Reed, J. Dailing, P. Doksus, Nicholas G. Usechak, J. Kim, T. De Young, P. O. Hulth, H. Wissing, Pawel Marciniewski
Rok vydání: 2001
Předmět:
Zdroj: International Journal of Modern Physics A. 16:1013-1015
ISSN: 1793-656X
0217-751X
Popis: We present results based on data taken in 1997 with the 302-PMT Antarctic Muon and Neutrino Detector Array-B10 ("AMANDA-B10") array. Atmospheric neutrinos created in the northern hemisphere are observed indirectly through their charged current interactions which produce relativistic, Cherenkov-light-emitting upgoing muons in the South Pole ice cap. The reconstructed angular distribution of these events is in good agreement with expectation and demonstrates the viability of this ice-based device as a neutrino telescope.
Databáze: OpenAIRE