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| 引力波理论和实验的新进展 | |
| 引用本文： | 黄玉梅,王运永,汤克云,康飞,张承民,徐军,郭有光.引力波理论和实验的新进展[J].天文学进展,2007,25(1):58-73. |
| 作者姓名： | 黄玉梅 王运永 汤克云 康飞 张承民 徐军 郭有光 |
| 作者单位： | 1. 北京师范大学,天文系,北京,100875 2. 中国科学院,国家天文台,北京,100012 3. 中国机械科学研究院,北京,100044 4. 中国科学院,上海光学精密机械研究所,上海,201800 5. 中国计量科学研究院,北京,200013 |
| 摘 要： | 引力波的存在是爱因斯坦在广义相对论理论中提出的一个重要预言．由于目前技术水平的限制,无法在实验室产生足以被探测到的引力波,因此宇宙中大量的大质量剧烈活动的天体成为科学家研究引力波的首选,从而诞生了引力波天文学．引力波探测将开启研究宇宙的新窗口,是继电磁辐射、宇宙线和中微子探测后探索宇宙奥秘的又一重要手段,对天文学研究有着极为重要的意义.新一代应用了高灵敏度的迈克耳逊干涉仪装置的长基线引力波探测仪正在建造中．该综述从引力波理论出发,阐述了目前研究较多的可探测引力波源,给出了目前观测上的最新进展,并展望了今后的发展前景． |
| 关 键 词： | 天体物理学 引力波 综述 广义相对论 中子双星 引力波探测仪 |
| 文章编号： | 1000-8349（2007）01-0058-16 |
| 收稿时间： | 09 14 2005 12:00AM |
| 修稿时间： | 2005-09-142006-06-22 |
The new Development of Gravitational Waves Theory and Detection |
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| HUANG Yu-mei,WANG Yun-yong,TANG Ke-yun,KANG Fei,ZHANG Cheng-min,XU Jun,GUO You-guang.The new Development of Gravitational Waves Theory and Detection[J].Progress In Astronomy,2007,25(1):58-73. | |
| Authors: | HUANG Yu-mei WANG Yun-yong TANG Ke-yun KANG Fei ZHANG Cheng-min XU Jun GUO You-guang |
| Institution: | 1. Department of Astronomy, Bejing Normal University, Beijing 100875, China; 2. National Astronomical Observatories, Chinese Academy of Sciences, Bejing 100012, China; 3. China Academy of Machinery Science and Technology, Beijing 100044, China; 4. Shanghai Institute of Optics and Fine Machines, Chinese Academy of Sciences, Shanghai 201800, China; 5. National Institute of Metrology, Beijing 100013, China |
| Abstract: | Gravitational Waves(GW)are perturbations of space-time, which propagate at the speed of light. This is one of the predictions from the general relativistic theory proposed by Einstein in 1916. So far, their existence has been proven indirectly by Taylor and Hulse's observation on the decay of the orbital period in the binary pulsar PSR 1913 16. Now the field of gravitational waves astronomy is inaugurated. The theory of gravitational radiation already makes an important contribution to the understanding of a lot of astronomical systems, such as binary neutron stars, cataclysmic variables, young neutron stars, low-mass X-ray binaries, and even the anisotropy of the microwave background radiation. Direct detection of GW is one of the most exciting subjects in physics and in modern astronomy. Up to now it is impossible to generate gravitational waves strong enough in laboratory that they can be detected with the aid of present technology in the world. The celestial sources of gravitational wave become the first choice of scientists for studying gravitational waves because of their huge mass and high speed. Gravitational waves are quite different from electro-magnetic waves, which give rise to the expectation that the detection of gravitational waves will reveal a new and different view of the universe. We can say the observations of gravitational waves will significantly complement the observations of electromagnetic waves, cosmic rays and neutrinos. A new generation of long baseline gravitational wave detectors is currently under construction. They incorporate high sensitive Michelson interferometers and high power stabilized laser sources, suspended optical components and high performance seismic filters. They have arm lengths of up to 4 km and operate in an ultra high vacuum environment. In this paper, we describe the theory of gravitational waves first. Then discuss the origin of gravitational waves. Various efforts for detecting gravitational waves are reviewed briefly. Furthermore, this review discusses the promise of this field, outlining why gravitational waves are worth pursuing. |
| Keywords: | astrophysics gravitational wave review general relativistic theory sources of gravitational waves |
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