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On possible lower bounds for the direct detection rate of SUSY Dark Matter

V. A. Bednyakov
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Abstract

One can expect accessible lower bounds for dark matter detection rate due to restrictions on masses of the SUSY-partners. To explore this correlation one needs a new-generation large-mass detector. The absolute lower bound for detection rate can naturally be due to spin-dependent interaction. Aimed at detecting dark matter with sensitivity higher than $10^{-5}$ event/day/kg an experiment should have a non-zero-spin target. Perhaps, the best is to create a GENIUS-like detector with both Ge-73 (high spin) and Ge-76 nuclei.

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V. A. Bednyakov. 2002-01-08. On possible lower bounds for the direct detection rate of SUSY Dark Matter. https://doi.org/10.1134/1.1563711

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