Hostname: page-component-7bb8b95d7b-qxsvm Total loading time: 0 Render date: 2024-09-11T10:10:17.010Z Has data issue: false hasContentIssue false
  • English
  • Français

High-energy Neutrino Astronomy: From AMANDA to IceCube

Published online by Cambridge University Press:  30 March 2016

Francis Halzen
Francis Halzen*
Affiliation:
Department of Physics, University of Wisconsin, Madison, WI 53706

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

Kilometer-scale neutrino detectors such as IceCube are discovery instruments covering nuclear and particle physics, cosmology and astronomy. Examples of their multidisciplinary missions include the search for the particle nature of dark matter and for additional small dimensions of space. In the end, their conceptual design is very much anchored to the observational fact that Nature accelerates protons and photons to energies in excess of 1020 and 1013 eV, respectively. The cosmic ray connection sets the scale of cosmic neutrino fluxes. In this context, we discuss the first results of the completed AMANDA detector and the reach of its extension, IceCube.

Type
I. Joint Discussions
Information
Highlights of Astronomy , Volume 13 , 2005 , pp. 13 - 17
Copyright
Copyright © Astronomical Society of Pacific 2005

References

Ahrens, J. et al. (AMANDA Collaboration) 2003, Phys. Rev. Lett. 90, 251101, astroph/0303218Google Scholar
Alvarez-Muniz, J. & Halzen, F. 2002, Ap. J. 576, L33;CrossRefGoogle Scholar
Crocker, R. M. 2002, PhD thesis (University of Melbourne)Google Scholar
Andres, E. et al. (AMANDA Collaboration) 2001, Nature 410, 441; 2000, Astroparticle Physics 13, 1 Google Scholar
Bahcall, J. N. & Waxman, E. 2001, Phys. Rev. D 64, 023002 CrossRefGoogle Scholar
Gaisser, T. K. 2002, in Proceedings of the 31st International Conference on High Energy Physics, Amsterdam, The Netherlands, July 2002 Google Scholar
Gaisser, T. K. 1997, astro-ph/9707283>, talk presented at the OECD Megascience Forum, Taormina, Italy, 1997 ,+talk+presented+at+the+OECD+Megascience+Forum,+Taormina,+Italy,+1997>Google Scholar
Gaisser, T. K., Halzen, F. & Stanev, T. 1995, Phys. Rept. 258, 173 [Erratum 271, 355 (1995)], hep-ph/9410384CrossRefGoogle Scholar
Halzen, F. 2003, these proceedingsCrossRefGoogle Scholar
Hauschildt, T. & Steele, D. 2003, in Proc. of the 28th International Cosmic Ray Conference, Tsukuba, Japan, August 2003 Google Scholar
Karle, A. et al. (IceCube Collaboration) 2002, in Proc. of the XXth International Conference on Neutrino Physics and Astrophysics, Munich, Germany, May 2002, astro-ph/020955Google Scholar
Wissing, H. 2003, PhD thesis (Humbold University, Berlin); Particle Astrophysics (in press) and http://icecube.wisc.edu/science/sci-tech-docs/ Google Scholar