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首个配备硅光电倍增管的双相氙时间投影室及其特性研究 。（原文表述似乎不完整，此译文根据已有内容尽量完善了语义）

The first dual-phase xenon TPC equipped with silicon photomultipliers and characterisation with .

作者信息

Baudis L, Biondi Y, Galloway M, Girard F, Hochrein S, Reichard S, Sanchez-Lucas P, Thieme K, Wulf J

机构信息

Department of Physics, University of Zurich, Winterthurerstrasse 190, 8057 Zurich, Switzerland.

出版信息

Eur Phys J C Part Fields. 2020;80(5):477. doi: 10.1140/epjc/s10052-020-8031-6. Epub 2020 May 26.

DOI:10.1140/epjc/s10052-020-8031-6
PMID:32508522
原文链接:https://pmc.ncbi.nlm.nih.gov/articles/PMC7250964/
Abstract

For the first time, a small dual-phase (liquid/gas) xenon time projection chamber was equipped with a top array of silicon photomultipliers for light and charge readout. Here we describe the instrument in detail, as well as the data processing and the event position reconstruction algorithms. We obtain a spatial resolution of in the horizontal plane. To characterise the detector performance, we show calibration data with internal and sources, and we detail the production of the latter as well as its introduction into the system. We finally compare the observed light and charge yields down to electronic recoil energies of to predictions based on NEST v2.0.

摘要

首次将一个小型双相（液体/气体）氙时间投影室配备了用于光和电荷读出的顶部硅光电倍增管阵列。在此，我们详细描述该仪器，以及数据处理和事件位置重建算法。我们在水平面上获得了 的空间分辨率。为了表征探测器性能，我们展示了使用内部 和 源的校准数据，并详细说明了后者的产生及其引入系统的过程。我们最终将观测到的低至 电子反冲能量的光产额和电荷产额与基于NEST v2.0的预测进行了比较。

https://cdn.ncbi.nlm.nih.gov/pmc/blobs/e44b/7250964/f70aea1f47da/10052_2020_8031_Fig13_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/e44b/7250964/7ed95d7700a5/10052_2020_8031_Fig1_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/e44b/7250964/7be8dc9e1e16/10052_2020_8031_Fig2_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/e44b/7250964/6742a46bf7e1/10052_2020_8031_Fig3_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/e44b/7250964/6e0c3c43de7b/10052_2020_8031_Fig4_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/e44b/7250964/2ad5671d7d7e/10052_2020_8031_Fig5_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/e44b/7250964/36b4811ca2e7/10052_2020_8031_Fig6_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/e44b/7250964/2893753ee952/10052_2020_8031_Fig7_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/e44b/7250964/46aec0e4f203/10052_2020_8031_Fig8_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/e44b/7250964/4026280071d5/10052_2020_8031_Fig9_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/e44b/7250964/5ac4fdaea200/10052_2020_8031_Fig10_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/e44b/7250964/fe57e61e5d01/10052_2020_8031_Fig11_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/e44b/7250964/8cc2b8c2dbf4/10052_2020_8031_Fig12_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/e44b/7250964/f70aea1f47da/10052_2020_8031_Fig13_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/e44b/7250964/7ed95d7700a5/10052_2020_8031_Fig1_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/e44b/7250964/7be8dc9e1e16/10052_2020_8031_Fig2_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/e44b/7250964/6742a46bf7e1/10052_2020_8031_Fig3_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/e44b/7250964/6e0c3c43de7b/10052_2020_8031_Fig4_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/e44b/7250964/2ad5671d7d7e/10052_2020_8031_Fig5_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/e44b/7250964/36b4811ca2e7/10052_2020_8031_Fig6_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/e44b/7250964/2893753ee952/10052_2020_8031_Fig7_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/e44b/7250964/46aec0e4f203/10052_2020_8031_Fig8_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/e44b/7250964/4026280071d5/10052_2020_8031_Fig9_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/e44b/7250964/5ac4fdaea200/10052_2020_8031_Fig10_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/e44b/7250964/fe57e61e5d01/10052_2020_8031_Fig11_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/e44b/7250964/8cc2b8c2dbf4/10052_2020_8031_Fig12_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/e44b/7250964/f70aea1f47da/10052_2020_8031_Fig13_HTML.jpg

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本文引用的文献

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Dark Matter Results from 54-Ton-Day Exposure of PandaX-II Experiment.熊猫X-II实验54吨·天曝光量的暗物质研究结果。
Phys Rev Lett. 2017 Nov 3;119(18):181302. doi: 10.1103/PhysRevLett.119.181302. Epub 2017 Oct 30.
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Spatially uniform calibration of a liquid xenon detector at low energies using (83m)Kr.
Rev Sci Instrum. 2010 Jul;81(7):073303. doi: 10.1063/1.3436636.