Macroscopic quantum mechanics in gravitational-wave observatories and beyond

IF 4.2 Q2 QUANTUM SCIENCE & TECHNOLOGY
R. Schnabel, M. Korobko
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引用次数: 5

Abstract

The existence of quantum correlations affects both microscopic and macroscopic systems. On macroscopic systems, they are difficult to observe and usually irrelevant for the system's evolution due to the frequent energy exchange with the environment. The world-wide network of gravitational-wave (GW) observatories exploits optical as well as mechanical systems that are highly macroscopic and largely decoupled from the environment. The quasi-monochromatic light fields in the kilometer-scale arm resonators have photon excitation numbers larger than 1019, and the mirrors that are quasi-free falling in propagation direction of the light fields have masses of around 40 kg. Recent observations on the GW observatories LIGO and Virgo clearly showed that the quantum uncertainty of one system affected the uncertainty of the other. Here, we review these observations and provide links to research goals targeted with mesoscopic optomechanical systems in other fields of fundamental physical research. These may have Gaussian quantum uncertainties as the ones in GW observatories or even non-Gaussian ones, such as Schrödinger cat states.
引力波天文台及其以外的宏观量子力学
量子关联的存在影响微观和宏观系统。在宏观系统上,由于与环境的频繁能量交换,它们很难观察到,通常与系统的进化无关。全球引力波观测站网络利用了高度宏观且与环境基本解耦的光学和机械系统。千米级臂谐振器中的准单色光场具有大于1019的光子激发数,并且在光场的传播方向上准自由落体的反射镜具有大约40的质量 最近对GW天文台LIGO和Virgo的观测清楚地表明,一个系统的量子不确定性会影响另一个系统。在这里,我们回顾了这些观察结果,并提供了与基础物理研究其他领域的介观光学机械系统目标研究的链接。这些可能具有高斯量子不确定性,就像GW天文台中的不确定性,甚至是非高斯不确定性,比如薛定谔猫态。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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来源期刊
CiteScore
9.90
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0.00%
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