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arXiv · astro-ph/0204145

Expected Performance of a Neutrino Telescope for Seeing AGN/GC Behind a Mountain

George W. S. Hou·M. A. Huang
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Abstract

We study the expected performance of building a neutrino telescope, which targets at energy greater than $10^{14}$ eV utilizing a mountain to interact with neutrinos. The telescope's efficiency in converting neutrinos into leptons is first examined. Then using a potential site on the Big Island of Hawaii, we estimate the acceptance of the proposed detector. The neutrino flux limit at event rate 0.3/year/half decade of energy is estimated to be comparable to that of AMANDA neutrino flux limit at above $10^{16}$ eV.

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George W. S. Hou, M. A. Huang. 2002-04-09. Expected Performance of a Neutrino Telescope for Seeing AGN/GC Behind a Mountain. https://doi.org/10.1142/9789812776860_0006

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