Hostname: page-component-586b7cd67f-dsjbd Total loading time: 0 Render date: 2024-11-26T03:24:00.873Z Has data issue: false hasContentIssue false
  • English
  • Français

Neutrino Telescopes in Antarctica

Published online by Cambridge University Press:  05 March 2013

Jenni Adams
Jenni Adams*
Affiliation:
Department of Physics and Astronomy, University of Canterbury, Private Bag 4800, Christchurch, New Zealand; [email protected]
Rights & Permissions [Opens in a new window]

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.

It is hoped that in the near future neutrino astronomy will reach throughout and beyond our galaxy and make measurements relevant to cosmology, astrophysics, cosmic-ray and particle physics. The construction of a high-energy neutrino telescope requires a huge volume of very transparent, deeply buried material such as ocean water or ice, which acts as the medium for detecting the particles. I will describe two experiments using Antarctic ice as this medium: the AMANDA experiment employing photomultiplier tubes and RICE utilising radio receivers.

Keywords

cosmic rays
Type
Research Article
Information
Publications of the Astronomical Society of Australia , Volume 17 , Issue 1 , 2000 , pp. 13 - 17
Copyright
Copyright © Astronomical Society of Australia 2000

References

Askebjer, P., et al. 1995, Science, 267, 1147 CrossRefGoogle Scholar
Bay, R. 1999, in ICRC XXVI: Proc. 26th Int. Cosmic Rays Conf., ed. D. Kieda et al., Vol. 2, 225 Section HE 4·2·06Google Scholar
Frichter, G. M. 1999, in ICRC XXVI: Proc. 26th Int. Cosmic Rays Conf., ed. D. Kieda et al., Vol. 2, 467 Section HE 6·3·12Google Scholar
Frichter, G. M., Ralston, J. P., & McKay, D. W. 1996, Phys. Rev. D, 53, 1684 CrossRefGoogle Scholar
Gaisser, T. K., Halzen, F., & Stanev, T. 1995, Phys. Rep., 258, 173 CrossRefGoogle Scholar
Halzen, F. 1999, in ICRC XXVI: Proc. 26th Int. Cosmic Rays Conf., ed. D. Kieda et al., Vol. 2, 428 Section HE 6·3·01Google Scholar
Hill, G. C. 1999, in ICRC XXVI: Proc. 26th Int. Cosmic Rays Conf., ed. D. Kieda et al., Vol. 2, 432 Section HE 6·3·02Google Scholar
Karle, A. 1999, in ICRC XXVI: Proc. 26th Int. Cosmic Rays Conf., ed. D. Kieda et al., Vol. 2, 221 Section HE 4·2·05Google Scholar
Kim, J. H. 1999, in ICRC XXVI: Proc. 26th Int. Cosmic Rays Conf., ed. D. Kieda et al., Vol. 2, 196 Section HE 4·1·14Google Scholar
Mannheim, K. 1993, A&A, 269, 67 Google Scholar
Mannheim, K. 1995, Astropart. Phys., 3, 295 CrossRefGoogle Scholar
Miller, T. C. 1999, in ICRC XXVI: Proc. 26th Int. Cosmic Rays Conf., ed. D. Kieda et al., Vol. 2, 465 Section HE 6·3·11Google Scholar
Price, P. B. 1996, Astropart. Phys., 5, 43 CrossRefGoogle Scholar
Protheroe, R. J. 1997, in Accretion Phenomena and Related Outflows, ed. D. T. Wickramisinghe et al., ASP Conf. Series, Vol. 121 (San Francisco: ASP), p. 585 (astro-ph/960““)Google Scholar
Protheroe, R. J. 1998, astro-ph/9809144Google Scholar
Seckel, D., & Frichter, G. 1999, in ICRC XXVI: Proc. 26th Int. Cosmic Rays Conf., ed. D. Kieda et al., Vol. 2, 471 Section HE 6·3·13Google Scholar
Stecker, F. W., & Salamon, M. H. 1996, Space Sci. Rev., 75, 341 (astro-ph/9501064)Google Scholar
Stecker, F. W., Done, C., Salamon, M. H., & Sommers, P. 1991, Phys. Rev. Lett., 66, 2697 CrossRefGoogle Scholar
Stecker, F. W., Done, C., Salamon, M. H., & Sommers, P. 1992, Phys. Rev. Lett., 69, 2738(E)CrossRefGoogle Scholar
Szabo, A. P., & Protheroe, R. J. 1992, Phys. Rev. Lett., 69, 2285 Google Scholar
Szabo, A. P., & Protheroe, R. J. 1994, Astropart. Phys., 2, 375 CrossRefGoogle Scholar
Waxman, E., & Bahcall, J. 1997, Phys. Rev. Lett., 78, 2292 CrossRefGoogle Scholar
Woschnagg, K. 1999, in ICRC XXVI: Proc. 26th Int. Cosmic Rays Conf., ed. D. Kieda et al., Vol. 2, 200 Section HE 4·1·15Google Scholar
Zas, E., Halzen, F., & Stanev, T. 1992, Phys. Rev. D, 45, 362 CrossRefGoogle Scholar