IceCube: A Multipurpose Neutrino Telescope

Katherine Rawlins, for the IceCube Collaboration: A. Achte, J. Ahrens,J. N. Bahcall,X. Bai,R. C. Bay, T. Becka, K.-H. Becker, J. Bergmans, D. Berley,E. Bernardini,D. Bertrand, D. Z. Besson,E. Blaufuss, D. J. Boersma,S. Böser, C. Bohm,O. Botner, A. Bouchta,O. Bouhali, T. Burgess,W. Carithers, T. Castermans, J. Cavin, W. Chinowsky, D. Chirkin, B. Collin, J. Conrad, J. Cooley,D. F. Cowen, A. Davour,C. De Clercq, T. DeYoung, P. Desiati, R. Ehrlich, R. W. Ellsworth,P. A. Evenson, A. R. Fazely, T. Feser, T. K. Gaisser,J. Gallagher, R. Ganugapati, H. Geenen,A. Goldschmidt, J. A. Goodman, R. M. Gunasingha,A. Hallgren,F. Halzen, K. Hanson, R. Hardtke, T. Hauschildt,D. Hays,K. Helbing, M. Hellwig, P. Herquet, G. C. Hill, D. Hubert, B. Hughey, P. O. Hulth, K. Hultqvist, S. Hundertmark,J. Jacobsen, G. S. Japaridze,A. Jones, A. Karle, H. Kawai, M. Kestel, N. Kitamura, R. Koch, L. Köpke, M. Kowalski, J. I. Lamoureux, N. Langer, H. Leich, I. Liubarsky, J. Madsen, K. Mandli, H. S. Matis, C. P. McParland, T. Messarius, P. Mészáros, Y. Minaeva, R. H. Minor, P. Miočinović, H. Miyamoto, R. Morse, R. Nahnhauer, T. Neunhöffer, P. Niessen, D. R. Nygren, H. Ögelman,Ph. Olbrechts, S. Patton, R. Paulos,C. Pérez de los Heros, A. C. Pohl, J. Pretz, P. B. Price, G. T. Przybylski, K. Rawlins, S. Razzaque, E. Resconi, W. Rhode, M. Ribordy,S. Richter, H.-G. Sander, K. Schinarakis, S. Schlenstedt, D. Schneider, R. Schwarz, D. Seckel,A. J. Smith, M. Solarz, G. M. Spiczak, C. Spiering, M. Stamatikos, T. Stanev, D. Steele, P. Steffen, T. Stezelberger, R. G. Stokstad, K.-H. Sulanke, G. W. Sullivan, T. J. Sumner, I. Taboada, S. Tilav,N. van Eijndhoven, W. Wagner, C. Walck,Y.-R. Wang, C. H. Wiebusch, C. Wiedemann, R. Wischnewski, H. Wissing, K. Woschnagg, S. Yoshida

Journal of the Physical Society of Japan(2008)

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摘要
IceCube is a new high-energy neutrino telescope which will be coming online in the near future. IceCube will be capable of measuring fluxes of all three flavors of neutrino, and its peak neutrino energy sensitivity will be in the TeV–PeV range. Here, after a brief description of the detector, we describe its anticipated performance with a selection of physics topics: supernovae, extraterrestrial diffuse and point sources of neutrinos, gamma-ray bursts, neutrinos from WIMP annihilation, and cosmic ray composition.
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neutrino
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