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Probing charged excited state of dark matter

机译:探测带电兴奋的暗物质状态

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If the neutral component of weak-scale dark matter is accompanied by a charged excitation separated by a mass gap of less than ~20 MeV, WIMPs can form stable bound states with nuclei.We show that the recent progress in experiments searching for neutrinoless double-beta decay sets the first direct constraint on the exoergic reaction of WIMP-nucleus bound state formation. We calculate the rate for such process in representative models and show that the double-beta decay experiments provide unique sensitivity to a large fraction of parameter space of the WIMP doublet model, complementary to constraints imposed by cosmology and direct collider searches.
机译:如果弱尺寸暗质物质的中性分量伴有带电激发分离的质量差距小于〜20meV,则WIMPS可以用核形成稳定的结合状态。我们展示了寻找中微子的实验中的最近进展β衰减将WIMP-核结合状态形成的exoergic反应设定了第一个直接约束。我们计算代表模型中这种过程的速率,并表明双β衰变实验为WIMP DOPBLET模型的大部分参数空间提供了独特的敏感性,与宇宙学和直接撞机搜索所施加的约束互补。

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