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首页> 外文期刊>Physical review, D >Direct detection of sub-GeV dark matter using a superfluid ~4He target
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Direct detection of sub-GeV dark matter using a superfluid ~4He target

机译:使用Superfluid〜4HE靶直接检测亚gev暗物质

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摘要

A promising technology concept for sub-GeV dark matter detection is described, in which lowtemperature microcalorimeters serve as the sensors and superfluid ~4He serves as the target material. We name this concept "HeRALD," helium roton apparatus for light dark matter. A superfluid helium target has several advantageous properties, including a light nuclear mass for better kinematic matching with light dark matter particles, copious production of scintillation light, extreme intrinsic radiopurity, high impedance to external vibration noise, and a unique "quantum evaporation" signal channel enabling the detection of phononlike modes via liberation of ~4He atoms into a vacuum. In this concept, both scintillation photons and triplet excimers are detected using calorimeters, including calorimeters immersed in the superfluid. Kinetic excitations of the superfluid medium (rotons and phonons) are detected using quantum evaporation and subsequent atomic adsorption onto a calorimeter suspended in vacuum above the target helium. The energy of adsorption amplifies the phonon/roton signal before calorimetric sensing, producing a gain mechanism that can reduce the technology's recoil energy threshold below the calorimeter energy threshold.We describe signal production and signal sensing probabilities, and estimate the resulting electron recoil discrimination. We simulate radioactive backgrounds from gamma rays and construct an overall background spectrum expectation also including neutrons and solar neutrinos. Finally, we calculate projected sensitivities to dark matter-nucleon elastic scattering, demonstrating that even very small (sub-kg) target masses can probe wide regions of as-yet untested dark matter parameter space.
机译:描述了用于子GEV暗物质检测的有希望的技术概念,其中低温微观率为传感器和超流〜4He用作目标材料。我们命名这个概念“先驱”,氦圈装置,用于光暗物质。超流氦靶具有若干有利的性质,包括轻质核质量,用于更好地与光暗物质颗粒的运动匹配,闪烁的闪烁,极端内在的辐射度,对外振动噪声的高阻抗,以及独特的“量子蒸发”信号通道通过将〜4HE原子释放到真空中,能够通过释放敏感模式检测。在该概念中,使用量热计检测闪烁的光子和三联屈光剂,包括浸入超流体中的量热计。使用量子蒸发和随后的原子吸附在靶氦上方真空悬浮在悬浮在靶氦的真空中的热量计上来检测超流血液介质(旋转和声子)的动力激发。吸附能量在量热感测之前放大了声子/旋转信号,产生了可以降低热量计能量阈值以下技术的反冲能量阈值的增益机制。我们描述了信号产生和信号感测概率,并估计所得到的电子反冲辨别率。我们模拟从伽马射线的放射性背景,并构建整体背景频谱期望,也包括中子和太阳中微子。最后,我们计算投影的敏感性至暗物质核心弹性散射,表明即使非常小(Sub-kg)目标质量可以探测到尚未测试的暗物质参数空间的宽区域。

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