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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的限制

摘要

We present the results of a search for elastic scattering from galactic dark matterudin the form of Weakly Interacting Massive Particles (WIMPs) in the 4 − 30 GeV/c2 massudrange. We make use of a 582 kg-day fiducial exposure from an array of 800 g Germaniumudbolometers equipped with a set of interleaved electrodes with full surface coverage. Weudsearched specifically for ∼ 2.5 − 20 keV nuclear recoils inside the detector fiducial volume.udAs an illustration the number of observed events in the search for 5 (resp. 20) GeV/c2udWIMPs are 9 (resp. 4), compared to an expected background of 6.1 (resp. 1.4). A 90% CLudlimit of 4.3 × 10−40 cm2ud(resp. 9.4 × 10−44 cm2ud) is set on the spin-independent WIMPnucleonudscattering cross-section for 5 (resp. 20) GeV/c2 WIMPs. This result represents aud41-fold improvement with respect to the previous EDELWEISS-II low-mass WIMP search forud7 GeV/c2 WIMPs. The derived constraint is in tension with hints of WIMP signals from someudrecent experiments, thus confirming results obtained with different detection techniques.
机译:我们提出了从银河暗物质 udin中以4-30 GeV / c2质量 udrange的弱相互作用质量粒子(WIMP)的形式进行弹性散射的搜索结果。我们利用800 g锗/辐射计的阵列进行582 kg-day的基准暴露,该阵列配备了一组具有完整表面覆盖范围的交错电极。我们专门针对探测器基准体积内的〜2.5-20 keV核反冲进行了研究。 ud作为说明,在搜索5个(分别为20个)GeV / c2 udWIMP时观察到的事件数量为9个(分别为4个),相比之下,预期背景为6.1(第1.4版)。 90%CL udlimit为4.3×10-40 cm2 ud(分别为9.4×10-44 cm2 ud),在自旋无关的WIMPnucleon udscattering截面上设置了5个(分别为20)GeV / c2 WIMP。与以前的EDELWEISS-II低质量WIMP搜索 ud7 GeV / c2 WIMP相比,该结果表示提高了ud41倍。导出的约束与来自一些最近的实验的WIMP信号的提示处于紧张状态,从而确认了使用不同检测技术获得的结果。

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