The Laser Interferometer Space Antenna mission

W. Folkner, S. Horowitz
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Abstract

The Laser Interferometer Space Antenna (LISA) mission is designed to detect and study low-frequency gravitational radiation. The types of exciting astrophysical sources potentially visible to LISA include extragalactic massive black hole binaries at cosmological distances, binary systems composed of a compact star and a massive black hole, Galactic neutron star-black hole binaries, and background radiation from the Big Bang. LISA will also observe Galactic binary systems which are known to exist.
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激光干涉仪空间天线任务
激光干涉仪空间天线(LISA)任务旨在探测和研究低频重力辐射。LISA可能看到的令人兴奋的天体物理源类型包括宇宙距离外的星系外大质量黑洞双星,由致密恒星和大质量黑洞组成的双星系统,银河系中子星-黑洞双星,以及大爆炸的背景辐射。LISA还将观测已知存在的银河系双星系统。
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