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Towards Teraton EeV Neutrino Telescopes

Published online by Cambridge University Press:  26 May 2016

Peter W. Gorham
Peter W. Gorham*
Affiliation:
Dept. Of Physics & Astronomy, University of Hawaii at Manoa, 2505 Correa Rd., Honolulu, HI, 96822, USA

Abstract

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The highest energy cosmic rays provide compelling evidence for EeV neutrino sources, if we can achieve the Teraton target volumes needed. At 10 TeV energies and above neutrino astronomy is in fact the only astronomy with a clear view of the whole universe. Radio detection of neutrino cascade interactions in ice and other solid dielectric media, via the Askaryan effect, provide a realistic path toward this goal.

Type
Part 10 Non-Photon Astrophysics and the Future
Information
Symposium - International Astronomical Union , Volume 214: High Energy Processes and Phenomena in Astrophysics , 2003 , pp. 372 - 375
Copyright
Copyright © Astronomical Society of the Pacific 2003 

References

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