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Updated: Jun 1, 2025

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下一代地面引力波观测站的低振动冷测试设施
D P Kapasi1, T G McRae1, J Eichholz1
1OzGrav-ANU, ARC Centre for Gravitational Astrophysics, College of Science, The Australian National University, Canberra ACT2601, Australia.
The Review of scientific instruments
|January 21, 2025
概括
我们开发了一个冷测试设施,以测量10^-16m/√Hz的支架位移噪声. 这一进步对于测试下一代引力波探测器中的热噪声模型至关重要.
科学领域:
- 实验物理学的实验物理.
- 引力波检测引力波探测器
- 低温工程 低温工程是什么?
背景情况:
- 未来的引力波探测器需要精确测量热噪声.
- 悬浮样本是这些探测器的关键组件.
- 现有的设施缺乏在低温温度下测试热噪声模型的灵敏度.
研究的目的:
- 设计和调试一个冷低振动测试设施.
- 在冷温度下测量支柱的位移噪声.
- 为了测试引力波探测器悬浮的热噪声模型.
主要方法:
- 一个~36L的辐射屏蔽光学腔冷却到123K.
- 一个用于振动隔离的多阶段.
- 干涉计测量50 Hz至10 kHz之间的位移噪声.
主要成果:
- 在1kHz时达到10^-16m/√Hz的位移噪声灵敏度.
- 在123K的温度下,在几个月内保持±1mK的温度稳定性.
- 证明了测量温度依赖的宽带位移噪声的能力.
结论:
- 低温装置可以在123K的水晶中进行宽带热噪声测量.
- 这项研究将为未来的探测器,如LIGO Voyager和爱因斯坦望远镜的悬浮设计提供信息.
- 该设施还适合测试冷镜面涂层.
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