High-Energy Neutrino Astronomy: from AMANDA to Icecube
| dc.creator | Halzen, F. | |
| dc.date | 2003-10-31 | |
| dc.date.accessioned | 2026-07-07T02:10:59Z | |
| dc.date.available | 2026-07-07T02:10:59Z | |
| dc.description | 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 10^{20} and 10^{13} 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. | |
| dc.description | Talk presented at the IAU XXV General Assembly, Sydney, Australia, July 2003. 8 pages, Latex2e with graphicx.sty, 4 postscript figures | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0311004 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0311004 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/6926 | |
| dc.subject | Astrophysics | |
| dc.title | High-Energy Neutrino Astronomy: from AMANDA to Icecube | |
| dc.type | text |