90 GHz CMB TES 波束仪的设计与特性分析

IF 2.7 3区 物理与天体物理 Q2 ASTRONOMY & ASTROPHYSICS Experimental Astronomy Pub Date : 2024-03-02 DOI:10.1007/s10686-024-09927-x
Yu Xu, Zhengwei Li, Yongping Li, Yifei Zhang, Xufang Li, Xuefeng Lu, Guofu Liao, Qingchen Li, Fangjun Lu, Laiyu Zhang, Yudong Gu, Zhouhui Liu, Shibo Shu, Zhi Chang, Guofeng Wang, Yongjie Zhang, He Gao, Aimei Zhang, Daikang Yan, Congzhan Liu
{"title":"90 GHz CMB TES 波束仪的设计与特性分析","authors":"Yu Xu,&nbsp;Zhengwei Li,&nbsp;Yongping Li,&nbsp;Yifei Zhang,&nbsp;Xufang Li,&nbsp;Xuefeng Lu,&nbsp;Guofu Liao,&nbsp;Qingchen Li,&nbsp;Fangjun Lu,&nbsp;Laiyu Zhang,&nbsp;Yudong Gu,&nbsp;Zhouhui Liu,&nbsp;Shibo Shu,&nbsp;Zhi Chang,&nbsp;Guofeng Wang,&nbsp;Yongjie Zhang,&nbsp;He Gao,&nbsp;Aimei Zhang,&nbsp;Daikang Yan,&nbsp;Congzhan Liu","doi":"10.1007/s10686-024-09927-x","DOIUrl":null,"url":null,"abstract":"<div><p>The transition-edge sensor (TES) as a type of low-temperature superconducting detector offers superior sensitivity due to its low thermal noise. In this work, we present a prototype TES bolometer designed for cosmic microwave background (CMB) polarization measurements. This TES is made of aluminum doped with a low concentration of manganese (2000 ppm by atomic percentage), and is deposited on the SiNx membrane which connects to the silicon substrate via narrow legs. In order to calculate its electrothermal parameters we have performed dark characterizations, which include measuring voltage-current (IV) curve at different bath temperatures, square-wave time response at various bias voltages, and noise level. This TES bolometer shows a noise equivalent power (NEP) of about <span>\\(5\\times 10^{-17}\\)</span> W/<span>\\(\\sqrt{\\textrm{Hz}}\\)</span>, which meets the requirement of CMB observation. However, its saturation power is smaller and time constant is larger than what are expected. We have analyzed the reasons and will make corresponding improvements in our future work.</p></div>","PeriodicalId":551,"journal":{"name":"Experimental Astronomy","volume":"57 2","pages":""},"PeriodicalIF":2.7000,"publicationDate":"2024-03-02","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":"{\"title\":\"Design and characterization of a 90 GHz CMB TES bolometer\",\"authors\":\"Yu Xu,&nbsp;Zhengwei Li,&nbsp;Yongping Li,&nbsp;Yifei Zhang,&nbsp;Xufang Li,&nbsp;Xuefeng Lu,&nbsp;Guofu Liao,&nbsp;Qingchen Li,&nbsp;Fangjun Lu,&nbsp;Laiyu Zhang,&nbsp;Yudong Gu,&nbsp;Zhouhui Liu,&nbsp;Shibo Shu,&nbsp;Zhi Chang,&nbsp;Guofeng Wang,&nbsp;Yongjie Zhang,&nbsp;He Gao,&nbsp;Aimei Zhang,&nbsp;Daikang Yan,&nbsp;Congzhan Liu\",\"doi\":\"10.1007/s10686-024-09927-x\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"<div><p>The transition-edge sensor (TES) as a type of low-temperature superconducting detector offers superior sensitivity due to its low thermal noise. In this work, we present a prototype TES bolometer designed for cosmic microwave background (CMB) polarization measurements. This TES is made of aluminum doped with a low concentration of manganese (2000 ppm by atomic percentage), and is deposited on the SiNx membrane which connects to the silicon substrate via narrow legs. In order to calculate its electrothermal parameters we have performed dark characterizations, which include measuring voltage-current (IV) curve at different bath temperatures, square-wave time response at various bias voltages, and noise level. This TES bolometer shows a noise equivalent power (NEP) of about <span>\\\\(5\\\\times 10^{-17}\\\\)</span> W/<span>\\\\(\\\\sqrt{\\\\textrm{Hz}}\\\\)</span>, which meets the requirement of CMB observation. However, its saturation power is smaller and time constant is larger than what are expected. We have analyzed the reasons and will make corresponding improvements in our future work.</p></div>\",\"PeriodicalId\":551,\"journal\":{\"name\":\"Experimental Astronomy\",\"volume\":\"57 2\",\"pages\":\"\"},\"PeriodicalIF\":2.7000,\"publicationDate\":\"2024-03-02\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"\",\"citationCount\":\"0\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"Experimental Astronomy\",\"FirstCategoryId\":\"101\",\"ListUrlMain\":\"https://link.springer.com/article/10.1007/s10686-024-09927-x\",\"RegionNum\":3,\"RegionCategory\":\"物理与天体物理\",\"ArticlePicture\":[],\"TitleCN\":null,\"AbstractTextCN\":null,\"PMCID\":null,\"EPubDate\":\"\",\"PubModel\":\"\",\"JCR\":\"Q2\",\"JCRName\":\"ASTRONOMY & ASTROPHYSICS\",\"Score\":null,\"Total\":0}","platform":"Semanticscholar","paperid":null,"PeriodicalName":"Experimental Astronomy","FirstCategoryId":"101","ListUrlMain":"https://link.springer.com/article/10.1007/s10686-024-09927-x","RegionNum":3,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q2","JCRName":"ASTRONOMY & ASTROPHYSICS","Score":null,"Total":0}
引用次数: 0

摘要

过渡边沿传感器(TES)是一种低温超导探测器,因其热噪声低而具有极高的灵敏度。在这项工作中,我们展示了一个为宇宙微波背景(CMB)偏振测量而设计的过渡边传感器原型。这种 TES 由掺有低浓度锰(按原子百分比为 2000 ppm)的铝制成,沉积在 SiNx 膜上,通过狭窄的支脚与硅基底相连。为了计算其电热参数,我们对其进行了暗特性分析,包括测量不同槽温下的电压-电流(IV)曲线、不同偏置电压下的方波时间响应以及噪声水平。该TES波长计的噪声等效功率(NEP)约为(5㎎/次 10^{-17})W/\(\sqrt\textrm{Hz}}\),满足CMB观测的要求。但是,它的饱和功率比预期的小,时间常数比预期的大。我们分析了原因,并将在今后的工作中做相应的改进。
本文章由计算机程序翻译,如有差异,请以英文原文为准。

摘要图片

查看原文
分享 分享
微信好友 朋友圈 QQ好友 复制链接
本刊更多论文
Design and characterization of a 90 GHz CMB TES bolometer

The transition-edge sensor (TES) as a type of low-temperature superconducting detector offers superior sensitivity due to its low thermal noise. In this work, we present a prototype TES bolometer designed for cosmic microwave background (CMB) polarization measurements. This TES is made of aluminum doped with a low concentration of manganese (2000 ppm by atomic percentage), and is deposited on the SiNx membrane which connects to the silicon substrate via narrow legs. In order to calculate its electrothermal parameters we have performed dark characterizations, which include measuring voltage-current (IV) curve at different bath temperatures, square-wave time response at various bias voltages, and noise level. This TES bolometer shows a noise equivalent power (NEP) of about \(5\times 10^{-17}\) W/\(\sqrt{\textrm{Hz}}\), which meets the requirement of CMB observation. However, its saturation power is smaller and time constant is larger than what are expected. We have analyzed the reasons and will make corresponding improvements in our future work.

求助全文
通过发布文献求助,成功后即可免费获取论文全文。 去求助
来源期刊
Experimental Astronomy
Experimental Astronomy 地学天文-天文与天体物理
CiteScore
5.30
自引率
3.30%
发文量
57
审稿时长
6-12 weeks
期刊介绍: Many new instruments for observing astronomical objects at a variety of wavelengths have been and are continually being developed. Furthermore, a vast amount of effort is being put into the development of new techniques for data analysis in order to cope with great streams of data collected by these instruments. Experimental Astronomy acts as a medium for the publication of papers of contemporary scientific interest on astrophysical instrumentation and methods necessary for the conduct of astronomy at all wavelength fields. Experimental Astronomy publishes full-length articles, research letters and reviews on developments in detection techniques, instruments, and data analysis and image processing techniques. Occasional special issues are published, giving an in-depth presentation of the instrumentation and/or analysis connected with specific projects, such as satellite experiments or ground-based telescopes, or of specialized techniques.
期刊最新文献
CNNCat: categorizing high-energy photons in a Compton/Pair telescope with convolutional neural networks Reflectivity test method of x-ray optics at the 100-m x-ray test facility Ground calibration and network of the first CATCH pathfinder Simulations and machine learning models for cosmic-ray short-term variations and test-mass charging on board LISA The ground calibration of the HERMES-Pathfinder payload flight models
×
引用
GB/T 7714-2015
复制
MLA
复制
APA
复制
导出至
BibTeX EndNote RefMan NoteFirst NoteExpress
×
×
提示
您的信息不完整,为了账户安全,请先补充。
现在去补充
×
提示
您因"违规操作"
具体请查看互助需知
我知道了
×
提示
现在去查看 取消
×
提示
确定
0
微信
客服QQ
Book学术公众号 扫码关注我们
反馈
×
意见反馈
请填写您的意见或建议
请填写您的手机或邮箱
已复制链接
已复制链接
快去分享给好友吧!
我知道了
×
扫码分享
扫码分享
Book学术官方微信
Book学术文献互助
Book学术文献互助群
群 号:481959085
Book学术
文献互助 智能选刊 最新文献 互助须知 联系我们:info@booksci.cn
Book学术提供免费学术资源搜索服务,方便国内外学者检索中英文文献。致力于提供最便捷和优质的服务体验。
Copyright © 2023 Book学术 All rights reserved.
ghs 京公网安备 11010802042870号 京ICP备2023020795号-1