面向空间引力波探测的弱光探测器性能检测与分析

李玉琼; 王璐钰; 王晨昱

doi:10.3788/OPE.20192708.1710

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面向空间引力波探测的弱光探测器性能检测与分析

现代应用光学 | 更新时间：2020-08-13

- 面向空间引力波探测的弱光探测器性能检测与分析
- Preliminary test of performance detection and analysis of weak-light detector for space gravitational wave detection
- 光学精密工程 2019年27卷第8期页码：1710-1718
- 作者机构：
  
  1.中国科学院力学研究所国家微重力实验室，北京 100190
  2.中国科学院光电研究院浮空器系统研究发展中心，北京 100094
  3.中国科学院大学光电学院，北京 100049
  4.中国科学院大学工程科学学院，北京 100049
- 作者简介：
  
  [ "李玉琼(1982-)，男，湖南娄底人，博士，副研究员、中国科学院青年创新促进委员会会员，2005年于陕西科技大学获得学士学位，2010年于北京理工大学获得博士学位，主要从事面向空间引力波探测的激光干涉测量研究。E-mail：liyuqiong@imech.ac.cn" ]
- 基金信息：
  
  中国科学院战略性先导科技专项(B类)(XDB23030200);国家自然科学基金资助项目(61575209);中国科学院青年创新促进会项目(2018024)
- DOI：10.3788/OPE.20192708.1710
  中图分类号： TN15;P142.84
- 收稿日期：2018-12-24，
  
  录用日期：2019-1-25，
  
  纸质出版日期：2019-08-15
- 稿件说明：
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李玉琼, 王璐钰, 王晨昱. 面向空间引力波探测的弱光探测器性能检测与分析[J]. 光学精密工程, 2019,27(8):1710-1718.

Yu-qiong LI, Lu-yu WANG, Chen-yu WANG. Preliminary test of performance detection and analysis of weak-light detector for space gravitational wave detection[J]. Optics and precision engineering, 2019, 27(8): 1710-1718.
李玉琼, 王璐钰, 王晨昱. 面向空间引力波探测的弱光探测器性能检测与分析[J]. 光学精密工程, 2019,27(8):1710-1718. DOI： 10.3788/OPE.20192708.1710.

Yu-qiong LI, Lu-yu WANG, Chen-yu WANG. Preliminary test of performance detection and analysis of weak-light detector for space gravitational wave detection[J]. Optics and precision engineering, 2019, 27(8): 1710-1718. DOI： 10.3788/OPE.20192708.1710.

摘要

为了研制出满足未来空间引力波探测需求的弱光探测器，初步进行了弱光探测器性能检测，分析了探测器的响应度、响应带宽、本底噪声等性能指标，以筛选出能满足未来空间引力波探测要求的探测器研制途径和解决方案。首先，根据空间引力波探测太极计划的激光器功率、轨道、星间距等设计方案，推算出太极计划所需探测器的性能指标；然后，与中国电子科技集团公司第四十四研究所、西南技术物理研究所和中国科学院上海技术物理研究所等单位合作研制了3款弱光探测器；最后，利用本课题组研制的低噪外差激光干涉系统对其响应度、响应带宽及本底噪声等指标进行检测，并分析了影响探测器性能指标的因素。实验结果表明：其中两款探测器的响应度优于1.8×10

V/W，响应带宽大于10 MHz；3款探测器的本底噪声均低于10 pm/

http://html.publish.founderss.cn/rc-pub/api/common/picture?pictureId=1719247&type=

http://html.publish.founderss.cn/rc-pub/api/common/picture?pictureId=1719247&type=small

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@10 mHz (0.1 mHz~1 Hz)，信噪比高于20 dB。这3款探测器在响应度、响应带宽和信噪比等方面具有满足未来太极计划实验星要求的潜力。

Abstract

To develop a weak-light detector that meets the needs of space gravitational wave detection in the future

the performance detection of weak-light detectors was initially carried out

and the performance parameters

such as responsiveness

response bandwidth and background noise

of the detectors were analyzed

for finding out the method and solution of weak-light detector development that can meet the requirements of future space gravitational wave detection. Firstly

according to the design scheme of the space gravitational wave detection

e.g. Taiji

including laser power

orbit design and star spacing

the parameters of the detector required by Taiji were calculated. Next

three kinds of weak-light detectors were developed by the China Electronics Technology Group Corporation No.44 Research Institute

Southwest Institute of Technical Physics

Shanghai Institute of Technical Physics of the Chinese Academy of Sciences with joint efforts of our research group. Finally

the responsivity

response bandwidth

and background noise of the detectors were tested by the low-noise heterodyne laser interferometry system developed by our research group

and the factors affecting the performance of the detectors were analyzed. The experimental results show that the responsiveness of two detectors is better than 1.8×10

V/W and that the response bandwidth is greater than 10 MHz. The ground noise of the three detectors is lower than 10 pm/

http://html.publish.founderss.cn/rc-pub/api/common/picture?pictureId=1719247&type=

http://html.publish.founderss.cn/rc-pub/api/common/picture?pictureId=1719247&type=small

http://html.publish.founderss.cn/rc-pub/api/common/picture?pictureId=1719247&type=middle

@10 mHz (0.1 mHz-1 Hz)

and the signal-to-noise ratio is higher than 20 dB. According to the aforementioned experimental results

the three detectors have the potential to meet the requirements of the Taiji Pathfinder in terms of responsiveness

response bandwidth

and signal-to-noise ratio.

关键词

Keywords

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