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arXiv · hep-ex/9804007

The AMANDA Neutrino Telescope and the Indirect Search for Dark Matter

F. Halzen
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Abstract

With an effective telescope area of order 10^4 m^2, a threshold of ~50 GeV and a pointing accuracy of 2.5 degrees, the AMANDA detector represents the first of a new generation of high energy neutrino telescopes, reaching a scale envisaged over 25 years ago. We describe its performance, focussing on the capability to detect halo dark matter particles via their annihilation into neutrinos.

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F. Halzen. 1998-04-16. The AMANDA Neutrino Telescope and the Indirect Search for Dark Matter. https://doi.org/10.1016/s0370-1573(98)00041-6

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