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引力波与引力波源

赵文 艾舜柯 朱宗宏 WANG Xiao-ge LEBIGOT Eric 都志辉 曹军威 钱进 殷聪 王建波 BLAIR David 张星 JU Li ZHAO Chun-nong WEN Lin-qing 刘小金 张杨 王运永 张帆 肇宇航 郭越凡 陈奕康

天文学进展2017,Vol.35Issue(3):316-344,29.
天文学进展2017,Vol.35Issue(3):316-344,29.DOI:10.3969/j.issn.1000-8349.2017.03.04

引力波与引力波源

Gravitation Wave and Gravitational-wave Sources

赵文 1艾舜柯 2朱宗宏 2WANG Xiao-ge 3LEBIGOT Eric 4都志辉 3曹军威 3钱进 3殷聪 5王建波 5BLAIR David 5张星 6JU Li 1ZHAO Chun-nong 6WEN Lin-qing 6刘小金 6张杨 1王运永 1张帆 2肇宇航 2郭越凡 2陈奕康2

作者信息

  • 1. 中国科学技术大学 天文学系,合肥 230026
  • 2. 北京师范大学 天文系,北京 100875
  • 3. 清华大学,北京 100084
  • 4. Michigan State University, East Lansing, MI 48821, USA
  • 5. 中国计量科学研究院,北京 100013
  • 6. University of Western Australia, WA 6009, Australia
  • 折叠

摘要

Abstract

The recent discovery of gravitational-wave burst GW150914 marks the coming of a new era of gravitational-wave astronomy, which provides a new window to study the physics in the strong gravitational fields, the extremely massive stars, extremely high energy processes and extremely early Universe. In this article, we introduce the basic characters of gravitational wave in Einstein's general relativity, their observational effects and main gener-ation mechanisms, including the rotation of neutron stars, the evolution of binary systems, the spontaneous generation in the inflation universe. Different sources produce the gravita-tional waves at quite different frequencies, which can be detected by different methods. In the lowest frequency range (f < 10-15 Hz), the detection is mainly dependent of the observation of B-mode polarization of cosmic microwave background radiation. In the middle frequency range (10-9 < f < 10-6 Hz), one detects gravitational waves by analyzing the timing resid-uals of millisecond second pulsars. In the high frequency range (10-4 < f < 104 Hz), it can be detected by space-based and ground-based laser interferometers. In particular, we focus on the main features, detection methods, detection status and the future prospects for sev-eral important sources, including the continuous sources (e.g. spinning neutron stars, stable binary systems), the burst sources (e.g. supernovae, the mergence of binary system), and the stochastic backgrounds generated by the astrophysical and cosmological process. In addition, we forecast the potential breakthrough processes in gravitational-wave astronomy in the near future, and the Chinese projects which might involve in these discoveries.

关键词

引力波/中子星/致密双星/超新星/暴胀

Key words

gravitational wave/neutron star/compact binary system/supernova/inflation

分类

天文与地球科学

引用本文复制引用

赵文,艾舜柯,朱宗宏,WANG Xiao-ge,LEBIGOT Eric,都志辉,曹军威,钱进,殷聪,王建波,BLAIR David,张星,JU Li,ZHAO Chun-nong,WEN Lin-qing,刘小金,张杨,王运永,张帆,肇宇航,郭越凡,陈奕康..引力波与引力波源[J].天文学进展,2017,35(3):316-344,29.

基金项目

国家自然科学基金(11633001,11603020,11653002,11322324,11173021,11275187,11675165,11653002,11421303) (11633001,11603020,11653002,11322324,11173021,11275187,11675165,11653002,11421303)

北京师范大学科学研究基金 ()

中央高校基础研究基金 ()

中国科学院战略先导项目(XDB09000000,XDB23010200) (XDB09000000,XDB23010200)

973项目(2012CB821804,2014CB845806) (2012CB821804,2014CB845806)

天文学进展

OA北大核心CSCDCSTPCD

1000-8349

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