Introduction of templates for low-frequency gravitational waves

YANG Shucheng; HAN Wenbiao

doi:10.13471/j.cnki.acta.snus.2020.11.06.2020B118

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Introduction of templates for low-frequency gravitational waves

Invited review | 更新时间：2023-11-01

- Introduction of templates for low-frequency gravitational waves
- Acta Scientiarum Naturalium Universitatis Sunyatseni Vol. 60, Issue 1, Pages: 99-111(2021)
- 作者机构：
  
  1.中国科学院上海天文台，上海 200030
  2.中国科学院大学天文与空间科学学院，北京 100049
- 作者简介：
- 基金信息：
- DOI：10.13471/j.cnki.acta.snus.2020.11.06.2020B118
  CLC： O412
- Published：25 January 2021，
  
  Published Online：15 January 2021，
  
  Received：06 November 2020，
  
  Accepted：17 November 2020
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杨舒程,韩文标.低频引力波波形模板介绍[J].中山大学学报(自然科学版),2021,60(01):99-111.

YANG Shucheng,HAN Wenbiao.Introduction of templates for low-frequency gravitational waves[J].Acta Scientiarum Naturalium Universitatis Sunyatseni,2021,60(01):99-111.
杨舒程,韩文标.低频引力波波形模板介绍[J].中山大学学报(自然科学版),2021,60(01):99-111. DOI： 10.13471/j.cnki.acta.snus.2020.11.06.2020B118.

YANG Shucheng,HAN Wenbiao.Introduction of templates for low-frequency gravitational waves[J].Acta Scientiarum Naturalium Universitatis Sunyatseni,2021,60(01):99-111. DOI： 10.13471/j.cnki.acta.snus.2020.11.06.2020B118.

摘要

引力波的探测和参数估计依赖于匹配滤波技术。而匹配滤波需要大量理论计算的引力波波形，称为波形模板。空间引力波探测器主要探测低频引力波，这些信号的持续时间长，从几天到几年不等，对理论波形的精度要求高；同时一些低频波源的构型复杂，往往带有大偏心率和轨道进动，使得波形参数空间很大，需要的模板数量巨大。因此对于空间引力波探测，多数波形模板在计算精度和效率上的要求要比地面引力波探测更高。本文回顾了低频引力波的一些主要波源（超大质量双黑洞、极端质量比旋近、河内致密双星）的波形模板研究，总结了这些模板的特点，展望了低频引力波天文学研究的未来。

Abstract

Matched filtering is critical in the detection and parameter estimation of gravitational waves （GWs）. The application of matched filtering requires waveform templates， which are lots of GW waveforms from theoretical calculations. Space-borne GW detectors aim at low-frequency GWs. These signals have long timescales， ranging from several days to several years， and require theoretical waveforms with high accuracy. Moreover， some low-frequency GW sources have complicated configurations， such as large eccentricities and precession， which leads to a large parameter space of waveforms， and numerous templates are required. Therefore， comparing with ground-based GW detection， space-borne GW detection requires more efficiency and quality for most waveform templates. In this paper， we first review some waveform templates of primary low-frequency GW sources （supermassive binary black holes， extreme-mass-ratio inspirals， and compact binary stars in the Galaxy）. Then we summarize the characteristics of these templates and look into the future of the research for low-frequency GW astronomy.

关键词

低频引力波匹配滤波数据处理

Keywords

low-frequency gravitational wavesmatched filteringdata processing

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