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Constraints on low-mass WIMPs from the EDELWEISS-III dark matter search

机译:EDELWEISS-III暗物质搜索对低质量WIMP的约束

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We present the results of a search for elastic scattering from galactic dark matter in the form of Weakly Interacting Massive Particles (WIMPs) in the 4-30 GeV/c(2) mass range. We make use of a 582 kg-day fiducial exposure from an array of 800 g Germanium bolometers equipped with a set of interleaved electrodes with full surface coverage. We searched specifically for similar to 2.5-20 keV nuclear recoils inside the detector fiducial volume. As an illustration the number of observed events in the search for 5 (resp. 20) GeV/c(2) WIMPs are 9 (resp. 4), compared to an expected background of 6.1 (resp. 1.4). A 90% CL limit of 4.3 x 10(-4)0 cm(2) (resp. 9.4 x 10(-44) cm(2)) is set on the spin-independent WIMP-nucleon scattering cross-section for 5 (resp. 20) GeV/c(2) WIMPs. This result represents a 41-fold improvement with respect to the previous EDELWEISS-II low-mass WIMP search for 7 GeV/c(2) WIMPs. The derived constraint is in tension with hints of WIMP signals from some recent experiments, thus confirming results obtained with different detection techniques.
机译:我们目前的结果是从4-30 GeV / c(2)质量范围内的弱相互作用质量粒子(WIMP)形式从银河暗物质寻找弹性散射。我们利用800 g锗测辐射热计阵列中的582 kg-day基准暴露量,该测辐射仪配有一组交错的电极,具有完整的表面覆盖范围。我们专门搜索了探测器基准体积内类似于2.5-20 keV的核反冲。作为说明,与预期背景6.1(第1.4)相比,搜索5(第20)GeV / c(2)WIMP时观察到的事件数为9(第4)。 90%的CL极限为4.3 x 10(-4)0 cm(2)(分别为9.4 x 10(-44)cm(2)),设置为5(分别为20)GeV / c(2)WIMP。与以前的EDELWEISS-II低质量WIMP搜索7 GeV / c(2)WIMP相比,该结果代表41倍的改进。导出的约束与最近的一些实验提示的WIMP信号紧密相关,从而证实了使用不同检测技术获得的结果。

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