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Searching for gravitational waves

机译:寻找引力波

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Gravitational waves, a new tool to facilitate our understanding the universe, have become a reality. Gravitational radiation, a prediction of Einstein's general theory of relativity, has not yet been directly verified. Recent technical developments have enabled the construction of detectors with sensitivities sufficient for directly measuring radiation from astrophysical sources. These detectors are to operate together as a network, taking data continuously, listening to waves from coalescing compact binary systems, stellar collapses, pulsars, and the background of the early universe. This review covers the present state of gravitational radiation detection, plans for future detectors, and the sources of gravitational waves that are likely to play an important role in the upcoming observations.
机译:引力波,一个促进我们理解宇宙的新工具已成为现实。 引力辐射,对爱因斯坦的一般相对论的预测尚未直接验证。 最近的技术开发使得探测器的构建能够敏感性,足以直接测量来自天体物理来源的辐射。 这些探测器将作为网络一起运行,连续进行数据,从聚结的紧凑二元系统,恒星坍塌,脉冲条和早期宇宙的背景中听到波浪。 本综述涵盖了目前的重力辐射检测状态,为未来探测器的计划以及可能在即将到来的观察中发挥重要作用的重力波来源。

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