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硅探测器中相对论粒子的集体激发和低能电离特征

Collective excitations and low-energy ionization signatures of relativistic particles in silicon detectors.

作者信息

Essig Rouven, Plestid Ryan, Singal Aman

机构信息

C. N. Yang Institute for Theoretical Physics, Stony Brook University, Stony Brook, NY 11794 USA.

Walter Burke Institute for Theoretical Physics, California Institute of Technology, Pasadena, CA 91125 USA.

出版信息

Commun Phys. 2024;7(1):416. doi: 10.1038/s42005-024-01904-2. Epub 2024 Dec 19.

DOI:10.1038/s42005-024-01904-2
PMID:39712928
原文链接:https://pmc.ncbi.nlm.nih.gov/articles/PMC11659158/
Abstract

Solid-state detectors with a low energy threshold have several applications, including searches of non-relativistic halo dark-matter particles with sub-GeV masses. When searching for relativistic, beyond-the-Standard-Model particles with enhanced cross sections for small energy transfers, a small detector with a low energy threshold may have better sensitivity than a larger detector with a higher energy threshold. In this paper, we calculate the low-energy ionization spectrum from high-velocity particles scattering in a dielectric material. We consider the full material response including the excitation of bulk plasmons. We generalize the energy-loss function to relativistic kinematics, and benchmark existing tools used for halo dark-matter scattering against electron energy-loss spectroscopy data. Compared to calculations commonly used in the literature, such as the Photo-Absorption-Ionization model or the free-electron model, including collective effects shifts the recoil ionization spectrum towards higher energies, typically peaking around 4-6 electron-hole pairs. We apply our results to the three benchmark examples: millicharged particles produced in a beam, neutrinos with a magnetic dipole moment produced in a reactor, and upscattered dark-matter particles. Our results show that the proper inclusion of collective effects typically enhances a detector's sensitivity to these particles, since detector backgrounds, such as dark counts, peak at lower energies.

摘要

具有低能量阈值的固态探测器有多种应用,包括搜寻质量低于吉电子伏特的非相对论性晕暗物质粒子。在搜寻具有增强的小能量转移截面的相对论性、超出标准模型的粒子时,一个具有低能量阈值的小型探测器可能比一个具有较高能量阈值的大型探测器具有更好的灵敏度。在本文中,我们计算了高速粒子在介电材料中散射产生的低能电离谱。我们考虑了包括体等离子体激元激发在内的完整材料响应。我们将能量损失函数推广到相对论运动学,并根据电子能量损失谱数据对用于晕暗物质散射的现有工具进行基准测试。与文献中常用的计算方法(如光吸收电离模型或自由电子模型)相比,包括集体效应会使反冲电离谱向更高能量移动,通常在4 - 6个电子 - 空穴对左右达到峰值。我们将我们的结果应用于三个基准示例:束流中产生的微带电粒子、反应堆中产生的具有磁偶极矩的中微子以及上散射暗物质粒子。我们的结果表明,适当地包含集体效应通常会提高探测器对这些粒子的灵敏度,因为探测器背景(如暗计数)在较低能量处达到峰值。

https://cdn.ncbi.nlm.nih.gov/pmc/blobs/cc78/11659158/d16b68543643/42005_2024_1904_Fig7_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/cc78/11659158/e0a72c20f093/42005_2024_1904_Fig1_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/cc78/11659158/87536dce6bc7/42005_2024_1904_Fig2_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/cc78/11659158/964aacdb37d1/42005_2024_1904_Fig3_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/cc78/11659158/132a8ad1f998/42005_2024_1904_Fig4_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/cc78/11659158/fdf9dad35333/42005_2024_1904_Fig5_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/cc78/11659158/8c1eda087a05/42005_2024_1904_Fig6_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/cc78/11659158/d16b68543643/42005_2024_1904_Fig7_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/cc78/11659158/e0a72c20f093/42005_2024_1904_Fig1_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/cc78/11659158/87536dce6bc7/42005_2024_1904_Fig2_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/cc78/11659158/964aacdb37d1/42005_2024_1904_Fig3_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/cc78/11659158/132a8ad1f998/42005_2024_1904_Fig4_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/cc78/11659158/fdf9dad35333/42005_2024_1904_Fig5_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/cc78/11659158/8c1eda087a05/42005_2024_1904_Fig6_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/cc78/11659158/d16b68543643/42005_2024_1904_Fig7_HTML.jpg

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本文引用的文献

1
Search by the SENSEI Experiment for Millicharged Particles Produced in the NuMI Beam.
Phys Rev Lett. 2024 Aug 16;133(7):071801. doi: 10.1103/PhysRevLett.133.071801.
2
Experimental Limits on Solar Reflected Dark Matter with a New Approach on Accelerated-Dark-Matter-Electron Analysis in Semiconductors.
Phys Rev Lett. 2024 Apr 26;132(17):171001. doi: 10.1103/PhysRevLett.132.171001.
3
First Constraints from DAMIC-M on Sub-GeV Dark-Matter Particles Interacting with Electrons.DAMIC-M 对与电子相互作用的亚GeV 暗物质粒子的首个限制。
Phys Rev Lett. 2023 Apr 28;130(17):171003. doi: 10.1103/PhysRevLett.130.171003.
4
Determining Dark-Matter-Electron Scattering Rates from the Dielectric Function.
Phys Rev Lett. 2021 Oct 8;127(15):151802. doi: 10.1103/PhysRevLett.127.151802.
5
Migdal Effect in Semiconductors.
Phys Rev Lett. 2021 Aug 20;127(8):081805. doi: 10.1103/PhysRevLett.127.081805.
6
Search for Light Dark Matter-Electron Scattering in the PandaX-II Experiment.在熊猫X-II实验中寻找轻暗物质与电子的散射。
Phys Rev Lett. 2021 May 28;126(21):211803. doi: 10.1103/PhysRevLett.126.211803.
7
SENSEI: Direct-Detection Results on sub-GeV Dark Matter from a New Skipper CCD.SENSEI:来自新型跳跃式电荷耦合器件的亚GeV暗物质直接探测结果。
Phys Rev Lett. 2020 Oct 23;125(17):171802. doi: 10.1103/PhysRevLett.125.171802.
8
First Germanium-Based Constraints on Sub-MeV Dark Matter with the EDELWEISS Experiment.利用EDELWEISS实验对亚兆电子伏特暗物质的首个锗基限制。
Phys Rev Lett. 2020 Oct 2;125(14):141301. doi: 10.1103/PhysRevLett.125.141301.
9
Improved Limits on Millicharged Particles Using the ArgoNeuT Experiment at Fermilab.利用费米实验室的阿贡中微子实验对微荷粒子的限制进行改进。
Phys Rev Lett. 2020 Apr 3;124(13):131801. doi: 10.1103/PhysRevLett.124.131801.
10
Light Dark Matter Search with Ionization Signals in XENON1T.利用 XENON1T 的电离信号进行暗物质搜索
Phys Rev Lett. 2019 Dec 20;123(25):251801. doi: 10.1103/PhysRevLett.123.251801.