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arXiv 2201.05640physics.opticsphysics.ins-detquant-ph

因镜面粗糙导致的精密计量中的散射损耗

Scattering Loss in Precision Metrology due to Mirror Roughness

Yehonathan Drori, Johannes Eichholz, Tega Edo, Hiro Yamamoto, Yutaro Enomoto, Gautam Venugopalan, Koji Arai, Rana X Adhikari

AI总结:

研究通过直接测量谐振腔和镜面损耗,结合数值模拟,揭示了光学腔体中散射损耗的统一估算方法,以减少量子增强精密计量中的退相干。

摘要:

光学损耗会降低激光干涉仪的灵敏度。它们减少信号光子的数量,并引入与漫射光相关的技术噪声。在量子增强计量中,它们破坏相关光子之间的纠缠。这种退相干是实现高量子噪声减少水平的主要障碍之一。在本工作中,我们比较了Caltech 40m引力波探测器原型干涉仪中谐振腔和镜面损耗的直接测量结果,与通过使用镜面表面轮廓图进行半解析内腔波前模拟得到的数值估计。我们展示了一种统一的方法来估算光学腔体(如LIGO引力探测器)中的总损耗,这将引导向工程化具有最小退相干的系统,以实现量子增强的精密计量。

英文摘要:

Optical losses degrade the sensitivity of laser interferometric instruments. They reduce the number of signal photons and introduce technical noise associated with diffuse light. In quantum-enhanced metrology, they break the entanglement between correlated photons. Such decoherence is one of the primary obstacles in achieving high levels of quantum noise reduction in precision metrology. In this work, we compare direct measurements of cavity and mirror losses in the Caltech 40m gravitational-wave detector prototype interferometer with numerical estimates obtained from semi-analytic intra-cavity wavefront simulations using mirror surface profile maps. We show a unified approach to estimating the total loss in optical cavities (such as the LIGO gravitational detectors) that will lead towards the engineering of systems with minimum decoherence for quantum-enhanced precision metrology.

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