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Title: Astroparticle Physics with Neutrinos

Abstract

The status and results of high energy neutrino telescopes that are operating (AMANDA, NT200) or under construction (IceCube, Antares, Nestor) are reviewed. Future projects, including novel ideas to extend the sensitivity to higher energies, are discussed.

Authors:
 [1]
  1. University of Mainz, Institut fuer Physik, Staudinger Weg 7, D55099 (Germany)
Publication Date:
OSTI Identifier:
20798057
Resource Type:
Journal Article
Resource Relation:
Journal Name: AIP Conference Proceedings; Journal Volume: 815; Journal Issue: 1; Conference: 25. international conference on physics in collision, Prague (Czech Republic), 5-9 Jul 2005; Other Information: DOI: 10.1063/1.2173579; (c) 2006 American Institute of Physics; Country of input: International Atomic Energy Agency (IAEA)
Country of Publication:
United States
Language:
English
Subject:
72 PHYSICS OF ELEMENTARY PARTICLES AND FIELDS; ASTROPHYSICS; NEUTRINO DETECTION; NEUTRINOS; SENSITIVITY; TELESCOPE COUNTERS

Citation Formats

Koepke, Lutz. Astroparticle Physics with Neutrinos. United States: N. p., 2006. Web. doi:10.1063/1.2173579.
Koepke, Lutz. Astroparticle Physics with Neutrinos. United States. doi:10.1063/1.2173579.
Koepke, Lutz. Wed . "Astroparticle Physics with Neutrinos". United States. doi:10.1063/1.2173579.
@article{osti_20798057,
title = {Astroparticle Physics with Neutrinos},
author = {Koepke, Lutz},
abstractNote = {The status and results of high energy neutrino telescopes that are operating (AMANDA, NT200) or under construction (IceCube, Antares, Nestor) are reviewed. Future projects, including novel ideas to extend the sensitivity to higher energies, are discussed.},
doi = {10.1063/1.2173579},
journal = {AIP Conference Proceedings},
number = 1,
volume = 815,
place = {United States},
year = {Wed Feb 08 00:00:00 EST 2006},
month = {Wed Feb 08 00:00:00 EST 2006}
}
  • I briefly discuss the role of neutrinos as probes in astroparticle physics and review the status of neutrino oscillation parameters as of June 2006, including recent fluxes, and latest SNO, K2K and MINOS results. I comment on the origin of neutrino masses in seesaw-type and low-scale models and mention some of their experimental signals.
  • No abstract prepared.
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