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New Signatures and Sources for the Detection of WIMP Dark Matter in the Solar System

Lawrence M. Krauss
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Abstract

I first outline new results on the angular modulation of WIMP dark matter scattering on targets in terrestrial laboratories, based on our uncertainties of the WIMP halo distribution, I then outline an exciting new result which indicates that for the high end of allowed SUSY WIMP scattering cross sections there exists a new distribution of WIMP dark matter in our solar system which could produce a dramatically different signal from halo WIMP dark matter in terrestrial detectors.

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Lawrence M. Krauss. 1998-07-14. New Signatures and Sources for the Detection of WIMP Dark Matter in the Solar System. https://doi.org/10.1016/s0370-1573(98)00066-0

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