Simulation of a hybrid optical/radio/acoustic extension to icecube for eev neutrino detection
Dec, 20054 pages
Part of Proceedings, 1st International Workshop on Acoustic and Radio EeV Neutrino Detection Activities (ARENA 2005) : Zeuthen, Germany, May 17-19, 2005, 259-264
Published in:
- Int.J.Mod.Phys.A 21S1 (2006) 259-264
Contribution to:
- , 259-264,
- ARENA 2005
- , 21-24
- ICRC 2005
e-Print:
- astro-ph/0512604 [astro-ph]
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Abstract: (arXiv)
Astrophysical neutrinos at EeV energies promise to be an interesting source for astrophysics and particle physics. Detecting the predicted cosmogenic (``GZK'') neutrinos at 10 - 10 eV would test models of cosmic ray production at these energies and probe particle physics at 100 TeV center-of-mass energy. While IceCube could detect 1 GZK event per year, it is necessary to detect 10 or more events per year in order to study temporal, angular, and spectral distributions. The IceCube observatory may be able to achieve such event rates with an extension including optical, radio, and acoustic receivers. We present results from simulating such a hybrid detector.Note:
- 4 pages, 2 figures; to appear in the Proceedings of the 29th ICRC, Pune, India
References(13)
Figures(2)