Preliminary analysis of space gravitational wave detection telescope system technology

FAN Wengtong; ZHAO Hongchao; FAN Lei; YAN Yong

doi:10.13471/j.cnki.acta.snus.2020.11.02.2020B111

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Preliminary analysis of space gravitational wave detection telescope system technology

Invited review | 更新时间：2023-11-01

- Preliminary analysis of space gravitational wave detection telescope system technology
- Acta Scientiarum Naturalium Universitatis Sunyatseni Vol. 60, Issue 1, Pages: 178-185(2021)
- 作者机构：
  
  天琴计划”教育部重点实验室，中山大学天琴中心 & 物理与天文学院，天琴前沿科学中心，国家航天局引力波研究中心，广东珠海 519082
- 作者简介：
- 基金信息：
- DOI：10.13471/j.cnki.acta.snus.2020.11.02.2020B111
  CLC： TH743
- Published：25 January 2021，
  
  Published Online：13 January 2021，
  
  Received：02 November 2020，
  
  Accepted：09 December 2020
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范纹彤,赵宏超,范磊等.空间引力波探测望远镜系统技术初步分析[J].中山大学学报(自然科学版),2021,60(01):178-185.

FAN Wengtong,ZHAO Hongchao,FAN Lei,et al.Preliminary analysis of space gravitational wave detection telescope system technology[J].Acta Scientiarum Naturalium Universitatis Sunyatseni,2021,60(01):178-185.
范纹彤,赵宏超,范磊等.空间引力波探测望远镜系统技术初步分析[J].中山大学学报(自然科学版),2021,60(01):178-185. DOI： 10.13471/j.cnki.acta.snus.2020.11.02.2020B111.

FAN Wengtong,ZHAO Hongchao,FAN Lei,et al.Preliminary analysis of space gravitational wave detection telescope system technology[J].Acta Scientiarum Naturalium Universitatis Sunyatseni,2021,60(01):178-185. DOI： 10.13471/j.cnki.acta.snus.2020.11.02.2020B111.

摘要

为探测到0.1 mHz~1 Hz频段的引力波，天琴、LISA、太极等空间引力波探测器编队（或星座）需在几十万到几百万公里量级的臂长上，实现pm级精度的测量。因此直接作为星间干涉测量光路一部分的望远镜面临巨大的技术挑战。空间引力波探测望远镜有超高精度和超高稳定性的特点。本文以LISA引力波探测器望远镜为研究对象，根据星间激光干涉测量核心指标10 pm/ Hz

1/2

@0.1 mHz~1 Hz的要求和引力波探测的实际需求，分析了望远镜的光学设计方案。在设计基础上，就材料选择、光学加工、装调及杂散光抑制等方面进行了分析和探讨，为后续望远镜的研制提供了参考依据。

Abstract

In order to realize the detection of gravitational waves in the frequency range of 0.1 mHz~1 Hz， the formations（or constellations） of space gravitational wave detectors such as Tianqin， LISA， and Taiji needs to achieve picometer-level measurement accuracy on the order of hundreds of thousands or even millions of kilometers. Therefore， telescopes directly used as part of the inter-satellite interferometry optical path are facing huge technical challenges. Space gravitational wave detection telescope has the characteristics of ultra-high precision and ultra-high stability. This article takes the LISA gravitational wave detector telescope as the research object， and analyzes the optical design scheme of the telescope according to the requirements of 10 pm/Hz

1/2

core index of inter-satellite laser interferometry and the actual demand of gravitational wave detection. And based on the design， analysis and discussion on material selection， optical processing， adjustment and stray light suppression are carried out， which provides a reference for the subsequent development of the telescope.

关键词

望远镜引力波LISA杂散光

Keywords

telescopegravitational waveLISAstray light

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