Neutrino Astrophysics in the cold: Amanda, Baikal and IceCube

Abstract

This talk review status and results from the two presently operating underwater/ice neutrino telescopes, NT-200 in Lake Baikal and Amanda-II at the South Pole. It also gives a description of the design and the expected performance of Icecube, the next-generation neutrino telescope at South Pole.

arXiv commentTalk given at the Nobel Symposium on Neutrino Physics, Haga Slott, Sweden, 2004, 14 pages, 10 figures

References in corpus (15)

• High Energy Neutrinos from Astrophysical Sources: An Upper Bound
• Sensitivity of the IceCube Detector to Astrophysical Sources of High Energy Muon Neutrinos
• High-energy Neutrino Astronomy: The Cosmic Ray Connection
• On the cosmic ray bound for models of extragalactic neutrino production
• Ultra-High Energy Neutrino Fluxes and Their Constraints
• High Energy Neutrinos from Quasars
• Search for extraterrestrial point sources of neutrinos with AMANDA-II
• Limits on diffuse fluxes of high energy extraterrestrial neutrinos with the AMANDA-B10 detector
• Signatures for a Cosmic Flux of Magnetic Monopoles
• Search for Supernova Neutrino-Bursts with the AMANDA Detector
• Search for Neutrino-Induced Cascades with AMANDA
• Registration of atmospheric neutrinos with the Baikal neutrino telescope
• Limits to the muon flux from WIMP annihilation in the center of the Earth with the AMANDA detector
• Extragalactic Sources of TeV Gamma Rays: A Summary
• High-Energy Neutrino Astronomy

Cited by in corpus (6)

• KM3NeT: Towards a km3 Mediterranean Neutrino Telescope
• ARIANNA: A New Concept for UHE Neutrino Detection
• Status of Radio and Acoustic Detection of Ultra-High Energy Cosmic Neutrinos and a Proposal on Reporting Results
• KM3NeT:a large underwater neutrino telescope in the Mediterranean Sea
• Flux of Primordial Monopoles
• Status and Perspectives of Astroparticle Physics in Europe