首页> 外文会议>Conference on Gravitational-Wave Detection, Aug 23-25, 2002, Waikoloa, Hawaii, USA >Second generation instruments for the Laser Interferometer Gravitational Wave Observatory (LIGO)
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Second generation instruments for the Laser Interferometer Gravitational Wave Observatory (LIGO)

机译:激光干涉仪重力波天文台(LIGO)的第二代仪器

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摘要

The interferometers being planned for second generation LIGO promise an order of magnitude increase in broadband strain sensitivity-with the corresponding cubic increase in detection volume-and an extension of the observation band to lower frequencies. In addition, one of the interferometers may be designed for narrowband performance, giving further improved sensitivity over roughly an octave band above a few hundred Hertz. This article discusses the physics and technology of these new interferometer designs, and presents their projected sensitivity spectra.
机译:计划用于第二代LIGO的干涉仪可保证宽带应变灵敏度增加一个数量级-相应增加检测体积的三次方-并将观察带扩展到较低的频率。另外,其中一种干涉仪可设计用于窄带性能,从而在几百赫兹以上的大约八度音带上进一步提高灵敏度。本文讨论了这些新型干涉仪设计的物理和技术,并介绍了其预计的灵敏度谱。

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