One can expect accessible lower bounds for the 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 the detection rate can naturally be due to spin-dependent interaction. Aimed at detecting dark matter with sensitivity higher than 10~(-5) event/kg/d, an experiment should have a nonzero-spin target. Perhaps, it is best to create a GENIUS-like detector with both ~(73)Ge (high spin) and ~(76)Ge nuclei.
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机译：由于对SUSY伙伴质量的限制，人们可以预期暗物质检测率的下界。为了探索这种相关性，需要一种新一代的大型探测器。检测率的绝对下限自然可以归因于自旋依赖性相互作用。为了检测灵敏度高于10〜（-5）事件/ kg / d的暗物质，实验应具有非零旋转目标。也许，最好创建一个同时具有〜（73）Ge（高自旋）和〜（76）Ge核的类GENIUS探测器。
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