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arXiv · hep-ph/9408391

Signals of Neutralino Dark Matter from Earth and Sun

A. Bottino·N. Fornengo·G. Mignola·L. Moscoso
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Abstract

We evaluate the fluxes of up--going muons detectable in a neutrino telescope and due to the annihilation of relic neutralinos in the Earth and in the Sun, taking realistically into account the fact that neutralinos might provide only a fraction of the local (solar neighbourhood) dark matter (DM). We determine the relation between the exposure $A t$ of the neutrino telescope ($A$ being the telescope area, $t$ the live time) and the explorable range of the neutralino mass and composition, when the signal--to--background ratio is optimized by an appropriate angular selection.

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A. Bottino, N. Fornengo, G. Mignola, L. Moscoso. 1994-08-30. Signals of Neutralino Dark Matter from Earth and Sun. https://doi.org/10.1016/0927-6505(94)00028-2

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