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A 1 m3 Gas Time Projection Chamber with Optical Readout for Directional Dark Matter Searches: the CYGNO Experiment

机译:1 m 3 气体时间投影室,带有光学读数,用于定向暗物质搜索:CYGNO实验

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The aim of the CYGNO project is the construction and operation of a 1 m3 gas TPC for directional dark matter searches and coherent neutrino scattering measurements, as a prototype toward the 100-1000 m3 (0.15-1.5 tons) CYGNUS network of underground experiments. In such a TPC, electrons produced by dark-matter- or neutrino-induced nuclear recoils will drift toward and will be multiplied by a three-layer GEM structure, and the light produced in the avalanche processes will be readout by a sCMOS camera, providing a 2D image of the event with a resolution of a few hundred micrometers. Photomultipliers will also provide a simultaneous fast readout of the time profile of the light production, giving information about the third coordinate and hence allowing a 3D reconstruction of the event, from which the direction of the nuclear recoil and consequently the direction of the incoming particle can be inferred. Such a detailed reconstruction of the event topology will also allow a pure and efficient signal to background discrimination. These two features are the key to reach and overcome the solar neutrino background that will ultimately limit non-directional dark matter searches.
机译:Cygno项目的目的是1米的建设和运营 3 气体TPC用于定向暗物质搜索和相干的中微子散射测量,作为100-1000米的原型 3 (0.15-1.5吨)Cygnus网络地下实验。在这种TPC中,由暗物质或中微子诱导的核反冲产生的电子将朝向并将乘以三层宝石结构,并且在雪崩过程中产生的光将被SCMOS相机读出,提供该事件的2D图像,分辨率为几百微米。光电倍增器还将提供光产生的时间轮廓的同时快速读出,提供关于第三坐标的信息,从而允许事件的3D重建,核反冲的方向和所以从而可以从中的进入粒子的方向推断。这种事件拓扑的这种详细的重建也将允许纯粹和有效的信号到背景歧视。这两个特征是达到和克服太阳中微子背景的关键,最终会限制非定向暗物质搜索。

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