Skip to main navigation Skip to search Skip to main content

IceCube - The next generation neutrino telescope at the South Pole

  • J. Ahrens*
  • , J. N. Bahcall
  • , X. Bai
  • , T. Becka
  • , K. H. Becker
  • , D. Z. Besson
  • , D. Berley
  • , E. Bernardinis
  • , D. Bertrand
  • , F. Binon
  • , A. Biron
  • , S. Böser
  • , C. Bohm
  • , O. Botner
  • , O. Bouhali
  • , Th Burgess
  • , T. Castermans
  • , D. Chirkin
  • , J. Conrad
  • , J. Cooley
  • D. F. Cowen, A. Davour, C. de Clercq, T. DeYoung, P. Desiati, J. P. Dewulf, B. Dingus, R. Ellsworth, P. A. Evenson, A. R. Fazely, T. Feser, T. K. Gaisser, J. Gallagher, R. Ganugapati, A. Goldschmidt, J. Goodman, A. Hallgren, F. Halzen, K. Hanson, R. Hardtke, T. Hauschildt, M. Hellwig, P. Herquet, G. C. Hill, P. O. Hulth, K. Hultqvist, S. Hundertmark, J. Jacobsen, G. S. Japaridze, A. Karle, L. Köpke, M. Kowalski, J. I. Lamoureux, H. Leich, M. Leuthold, P. Lindahl, I. Liubarsky, J. Madsen, P. Marciniewski, H. S. Matis, C. P. McParland, Y. Minaeva, P. Miočinović, R. Morse, R. Nahnhauer, T. Neunhöffer, P. Niessen, D. R. Nygren, H. Ogelman, Ph Olbrechts, C. Pérez de los Heros, A. C. Pohl, P. B. Price, G. T. Przybylski, K. Rawlins, E. Resconi, W. Rhode, M. Ribordy, S. Richter, H. G. Sander, T. Schmidt, D. Schneider, D. Seckel, M. Solarz, L. Sparke, G. M. Spiczak, C. Spiering, T. Stanev, D. Steele, P. Steffen, R. G. Stokstad, P. Sudhoff, K. H. Sulanke, G. W. Sullivan, T. Sumners, I. Taboada, L. Thollander, S. Tilav, C. Walck, C. Weinheimer, C. H. Wiebusch, Ch Wiedemann, R. Wischnewski, H. Wissing, K. Woschnagg, Sh Yoshida
*Corresponding author for this work
  • Johannes Gutenberg University Mainz
  • Institute for Advanced Studies
  • University of Delaware
  • University of Wuppertal
  • University of Kansas
  • University of Maryland, College Park
  • German Electron Synchrotron
  • Université libre de Bruxelles
  • Uppsala University
  • Stockholm University
  • Universite de Mons
  • University of California at Berkeley
  • University of Wisconsin-Madison
  • Pennsylvania State University
  • Vrije Universiteit Brussel
  • University of California at Santa Cruz
  • Southern University and A&M College
  • Lawrence Berkeley National Laboratory
  • Clark Atlanta University
  • Imperial College London
  • University of Wisconsin-River Falls
  • Universidad Simón Bolívar
  • CERN
  • Chiba University

Research output: Contribution to journalArticlepeer-review

Abstract

IceCube is a large neutrino telescope of the next generation to be constructed in the Antarctic Ice Sheet near the South Pole. We present the conceptual design and the sensitivity of the IceCube detector to predicted fluxes of neutrinos, both atmospheric and extra-terrestrial. A complete simulation of the detector design has been used to study the detector's capability to search for neutrinos from sources such as active galaxies, and gamma-ray bursts.

Original languageEnglish
Pages (from-to)388-395
Number of pages8
JournalNuclear Physics B - Proceedings Supplements
Volume118
DOIs
Publication statusPublished - Apr 2003
Externally publishedYes

Fingerprint

Dive into the research topics of 'IceCube - The next generation neutrino telescope at the South Pole'. Together they form a unique fingerprint.

Cite this