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Cryogenic Wide-Area Light Detectors for Neutrino and Dark Matter Searches

机译:用于中微子和暗物质搜索的低温广域光探测器

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摘要

Large-mass arrays of bolometers proved to be good detectors for neutrino-less double beta decay (0vDBD) and dark matter searches. CUORE and LUCIFER are bolometric 0vDBD experiments that will start to take data in 2015 at Laboratori Nazionali del Gran Sasso in Italy. The sensitivity of CUORE could be increased by removing the background due to α particles, by detecting the small amount of Cerenkov light (~100 eV) emitted by the βs' signal and not by as. LUCIFER could be extended to detect also dark matter, provided that the background from β/γ particles (~100 eV of scintillation light) is discriminated from nuclear recoils of about 10 keV energy (no light). We have recently started to develop light detectors for CUORE, LUCIFER and similar bolometric experiments. The aim is to obtain detectors with an active area of 5 × 5 cm~2 (the face of bolometric crystals), operating at 10 mK, and with an energy resolution at the baseline below 20 eV RMS. We have chosen to develop phonon-mediated detectors with KID sensors. We are currently testing the first prototypes.
机译:大型辐射热计阵列被证明是无中微子双β衰变(0vDBD)和暗物质搜索的良好探测器。 CUORE和LUCIFER是辐射热测量0vDBD实验,将于2015年在意大利的Laboratori Nazionali del Gran Sasso开始获取数据。 CUORE的灵敏度可以通过去除由α粒子引起的背景,检测由βs信号而不是as发出的少量切伦科夫光(〜100 eV)来提高。 LUCIFER可以扩展到还可以检测暗物质,只要能将β/γ粒子(约100 eV的闪烁光)的背景与约10keV能量的核后座力(无光)区分开即可。我们最近开始开发用于CUORE,LUCIFER和类似辐射热测定实验的光检测器。目的是获得有效面积为5×5 cm〜2(辐射热分析晶体的表面),工作于10 mK,能量分辨率为20 eV RMS以下的探测器。我们选择开发具有KID传感器的声子介导的探测器。我们目前正在测试第一批原型。

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