Lectures on high-energy neutrino astronomy - INSPIRE

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Lectures on high-energy neutrino astronomy

F. Halzen
(
- Wisconsin U., Madison
)

Jan 3, 2006

34 pages

Part of Proceedings, Cinvestav Advanced Summer School 2005 : Cinvestav, Mexico , 11-22 Jul 2005, 130-163

Published in:

AIP Conf.Proc. 809 (2006) 1, 130-163

Contribution to:

Cinvestav Advanced Summer School 2005, 130-163

Published: Jan 3, 2006

DOI:

10.1063/1.2160978

View in:

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Abstract: (AIP)

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 produces protons and photons with 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 science reach of its extension, IceCube. Similar experiments are under construction in the Mediterranean. Neutrino astronomy is also expanding in new directions with efforts to detect air showers, acoustic and radio signals initiated by super‐EeV neutrinos. The outline of these lectures is as follows: • Introduction • Cosmic Neutrinos Associated with the Highest Energy Cosmic Rays • Why Kilometer‐Scale Detectors? • Blueprints of Cosmic Accelerators: Gamma Ray Bursts and Active Galaxies • High Energy Neutrino Telescopes: Methodologies of Neutrino Detection • High Energy Neutrino Telescopes: Status

96.50.-e
95.55.Vj
neutrino detection
cosmic ray apparatus
astronomical telescopes
cosmic ray neutrinos
lectures
neutrino: astrophysics
dark matter
space-time: higher-dimensional

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