Phenomenological Introduction to Direct Dark Matter Detection

Details Phenomenological Introduction to Direct Dark Matter Detection Phenomenological Introduction to Direct Dark Matter Detection

1996-05-13

arxiv.org/abs/hep-ph/9605290v1

Physics

High Energy Physics

High Energy Physics - Phenomenology

9 pages. uses epsf, rotate. 4 embedded postscript figures. Invited talk at the XXXI Rencontres de Moriond, "Dark Matter in Cos

Scientific paper

The dark matter of our galactic halo may be constituted by elementary particles that interact weakly with ordinary matter (WIMPs). In spite of the very low counting rates expected for these dark matter particles to scatter off nuclei in a laboratory detector, such direct WIMP searches are possible and are experimentally carried out at present. An introduction to the theoretical ingredients entering the counting rates predictions, together with a short discussion of the major theoretical uncertainties, is here presented.

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