Indirect Searches for Kaluza-Klein Dark Matter

Details Indirect Searches for Kaluza-Klein Dark Matter Indirect Searches for Kaluza-Klein Dark Matter

2004-09-23

arxiv.org/abs/hep-ph/0409272v1

Physics

High Energy Physics

High Energy Physics - Phenomenology

6 pages, 3 figures, for the proceedings of IDM 2004, Edinburgh

Scientific paper

In this talk, we discuss the potential for the indirect detection of Kaluza-Klein dark matter using neutrino telescopes and cosmic positron experiments. We find that future kilometer-scale neutrino telescopes, such as IceCube, as well as future experiments capable of measuring the cosmic positron spectrum, such as PAMELA and AMS-02, will be quite sensitive to this scenario. Current data from the HEAT experiment can also be explained by the presence of Kaluza-Klein dark matter in the Galactic halo.

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