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首次展示用于无中微子双β衰变搜索的基于热电子发射光谱(TES)的低温锂钼探测器。

First demonstration of a TES based cryogenic Li MoO detector for neutrinoless double beta decay search.

作者信息

Bratrud G, Chang C L, Chen R, Cudmore E, Figueroa-Feliciano E, Hong Z, Kennard K T, Lewis S, Lisovenko M, Mateo L O, Novati V, Novosad V, Oliveri E, Ren R, Scarpaci J A, Schmidt B, Wang G, Winslow L, Yefremenko V G, Zhang J, Baxter D, Hollister M, James C, Lukens P, Temples D J

机构信息

Northwestern University, 633 Clark St, Evanston, IL 60208 USA.

Argonne National Laboratory, 9700 S Cass Ave, Lemont, IL 60439 USA.

出版信息

Eur Phys J C Part Fields. 2025;85(2):118. doi: 10.1140/epjc/s10052-025-13844-4. Epub 2025 Jan 31.

DOI:10.1140/epjc/s10052-025-13844-4
PMID:39896824
原文链接:https://pmc.ncbi.nlm.nih.gov/articles/PMC11785649/
Abstract

Cryogenic calorimetric experiments to search for neutrinoless double-beta decay ( ) are highly competitive, scalable and versatile in isotope. The largest planned detector array, CUPID, is comprised of about 1500 individual Li MoO detector modules with a further scale up envisioned for a follow up experiment (CUPID-1T). In this article, we present a novel detector concept targeting this second stage with a low impedance TES based readout for the Li MoO absorber that is easily mass-produced and lends itself to a multiplexed readout. We present the detector design and results from a first prototype detector operated at the NEXUS shallow underground facility at Fermilab. The detector is a 2-cm-side cube with 21 g mass that is strongly thermally coupled to its readout chip to allow rise-times of 0.5 ms. This design is more than one order of magnitude faster than present NTD based detectors and is hence expected to effectively mitigate backgrounds generated through the pile-up of two independent two neutrino decay events coinciding close in time. Together with a baseline resolution of 1.95 keV (FWHM) these performance parameters extrapolate to a background index from pile-up as low as  counts/keV/kg/yr in CUPID size crystals. The detector was calibrated up to the MeV region showing sufficient dynamic range for searches. In combination with a SuperCDMS HVeV detector this setup also allowed us to perform a precision measurement of the scintillation time constants of Li MoO , which showed a primary component with a fast O(20  s) time scale.

摘要

用于寻找无中微子双β衰变( )的低温量热实验在同位素方面具有高度竞争力、可扩展性和通用性。计划中的最大探测器阵列CUPID由约1500个独立的Li MoO 探测器模块组成,并设想在后续实验(CUPID - 1T)中进一步扩大规模。在本文中,我们提出了一种针对第二阶段的新型探测器概念,该概念采用基于低阻抗TES的读出方式用于Li MoO 吸收体,这种吸收体易于大规模生产且适合复用读出。我们展示了探测器设计以及在费米实验室NEXUS浅层地下设施运行的首个原型探测器的结果。该探测器是一个边长为2厘米的立方体,质量为21克,与读出芯片紧密热耦合,上升时间为0.5毫秒。这种设计比目前基于NTD的探测器快一个多数量级,因此有望有效减轻由于两个独立的双中微子衰变事件在时间上紧密重合而产生的堆积背景。连同1.95 keV(半高宽)的基线分辨率,这些性能参数外推至CUPID尺寸晶体中由堆积产生的背景指数低至 计数/keV/kg/yr。该探测器已校准至兆电子伏特区域,显示出足够用于 搜索的动态范围。结合一个SuperCDMS HVeV探测器,此装置还使我们能够对Li MoO 的闪烁时间常数进行精确测量,结果显示主要成分具有快速的O(20 s)时间尺度。

https://cdn.ncbi.nlm.nih.gov/pmc/blobs/f4ce/11785649/9e1cb1af7dc9/10052_2025_13844_Fig13_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/f4ce/11785649/b99628fce343/10052_2025_13844_Fig1_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/f4ce/11785649/fe4f4ffafbd2/10052_2025_13844_Fig2_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/f4ce/11785649/d14b6145acab/10052_2025_13844_Fig3_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/f4ce/11785649/d331c321579b/10052_2025_13844_Fig4_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/f4ce/11785649/db547f274b4c/10052_2025_13844_Fig5_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/f4ce/11785649/e449df86156b/10052_2025_13844_Fig6_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/f4ce/11785649/25222a6102d7/10052_2025_13844_Fig7_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/f4ce/11785649/63b03c0f4f65/10052_2025_13844_Fig8_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/f4ce/11785649/68cbea75feb6/10052_2025_13844_Fig9_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/f4ce/11785649/4390fa298b06/10052_2025_13844_Fig10_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/f4ce/11785649/410b08db063e/10052_2025_13844_Fig11_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/f4ce/11785649/cdf5d347950d/10052_2025_13844_Fig12_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/f4ce/11785649/9e1cb1af7dc9/10052_2025_13844_Fig13_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/f4ce/11785649/b99628fce343/10052_2025_13844_Fig1_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/f4ce/11785649/fe4f4ffafbd2/10052_2025_13844_Fig2_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/f4ce/11785649/d14b6145acab/10052_2025_13844_Fig3_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/f4ce/11785649/d331c321579b/10052_2025_13844_Fig4_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/f4ce/11785649/db547f274b4c/10052_2025_13844_Fig5_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/f4ce/11785649/e449df86156b/10052_2025_13844_Fig6_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/f4ce/11785649/25222a6102d7/10052_2025_13844_Fig7_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/f4ce/11785649/63b03c0f4f65/10052_2025_13844_Fig8_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/f4ce/11785649/68cbea75feb6/10052_2025_13844_Fig9_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/f4ce/11785649/4390fa298b06/10052_2025_13844_Fig10_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/f4ce/11785649/410b08db063e/10052_2025_13844_Fig11_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/f4ce/11785649/cdf5d347950d/10052_2025_13844_Fig12_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/f4ce/11785649/9e1cb1af7dc9/10052_2025_13844_Fig13_HTML.jpg

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