The AMANDA Neutrino Telescope and the Indirect Search for Dark Matter

Details The AMANDA Neutrino Telescope and the Indirect Search for Dark Matter The AMANDA Neutrino Telescope and the Indirect Search for Dark Matter

1998-04-16

arxiv.org/abs/hep-ex/9804007v1

Phys.Rept.307:243-252,1998

Physics

High Energy Physics

High Energy Physics - Experiment

Latex2.09, 16 pages, uses epsf.sty to place 15 postscript figures. Talk presented at the 3rd International Symposium on Source

Scientific paper

10.1016/S0370-1573(98)00041-6

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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