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

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

2002-01-08

arxiv.org/abs/hep-ph/0201046v1

Phys.Atom.Nucl. 66 (2003) 490-493; Yad.Fiz. 66 (2003) 518-520

Physics

High Energy Physics

High Energy Physics - Phenomenology

latex, 5 pages, 3 figures. Talk given at the III International Conference on Non-accelerator New Physics (NANP'01), Dubna, 19-

Scientific paper

10.1134/1.1563711

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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