Inspiraling Compact Binaries
Inspiraling Compact Binaries
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鼓舞人心的紧凑型双星
DOI：
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发表时间：
1997
期刊：
影响因子：
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通讯作者：
L. Blanchet
中科院分区：
文献类型：
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作者：
L. Blanchet
在这篇文章中，我们回顾了几个天体物理性质的吸气紧凑双星，使这些系统的独特性，非常重要的潜在的引力辐射源，以观察未来的探测器LIGO和处女座。强调高度相对论性的吸入紧凑型双星，我们讨论了它们的建模由两个非旋转点质量的系统，发射引力波在一个高的后牛顿近似超过占主导地位的四极辐射。
In this contribution we review several astrophysical properties of inspiraling compact binaries which make these systems unique, and very important as potential sources of gravitational radiation to be observed by the future detectors LIGO and VIRGO. Emphasizing the highly relativistic nature of inspiraling compact binaries, we discuss their modelisation by a system of two non-spinning point masses, emitting gravitational waves at a high post-Newtonian approximation beyond the dominant quadrupolar radiation.