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arXiv 2609.04311astro-ph.IMquant-ph

面向光学/红外干涉测量的量子技术发展

Development of quantum technologies for optical/infrared interferometry

  • University of Michigan(密歇根大学)

机构由 AI 辅助整理,请以论文原文为准。

John D. Monnier

AI总结:

本文围绕面向光学/红外干涉测量的量子技术,考察相关应用、关键模块演示,指出量子增强干涉测量的潜力,同时强调需克服量子接口的实际约束才能服务天文学。

AI中文摘要:

量子技术可通过新手段在相距遥远的望远镜间分布和保持电场振幅与相位关联,可能彻底变革光学干涉测量。在综述现有技术后,本文考察了拟议的量子传感与量子网络应用,并重点介绍了关键构建模块的近期实验室演示。量子增强型干涉测量可放宽基线超约1公里的场传输需求,实现亚毫角秒成像与微角秒级差分天体测量。不过,“转向量子”并非灵敏度的神奇捷径,因为许多极具吸引力的科学案例仍受光子与湍流限制。因此,本文强调必须克服量子接口的损耗、带宽、相干时间、同步及波长限制等实际约束,才能让这些能力在地面或空间部署时切实服务于天文学。

英文摘要:

Quantum technologies may revolutionize optical interferometry through new means to distribute and preserve electric-field amplitude and phase correlations between widely separated telescopes. After reviewing existing techniques, I survey proposed quantum-sensing and quantum-networking applications and highlight recent laboratory demonstrations of key building blocks. By easing field-transport demands for baselines beyond $\sim$1 km, quantum-enhanced interferometry could enable sub-milliarcsecond imaging and microarcsecond-class differential astrometry. That said, "going quantum" is not a magic shortcut to sensitivity because many of the most compelling science cases remain photon- and turbulence-limited. I therefore emphasize the practical constraints -- loss, bandwidth, coherence time, synchronization, and wavelength limits of quantum interfaces -- that must also be overcome to make these capabilities useful for astronomy, whether deployed on the ground or from space.

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