论文标题
部分可观测时空混沌系统的无模型预测
Imaging stars with quantum error correction
论文作者
论文摘要
高分辨率,大基线光学干涉仪的发展将彻底改变天文成像。但是,经典技术受到物理局限性的阻碍,包括损失,噪声以及收到的光通常是量子的事实。我们展示了如何使用量子通信技术克服这些问题。我们提出了一个通用框架,用于使用量子误差校正代码,以保护在遥远的望远镜站点收到的图像星光。在我们的方案中,光的量子状态通过刺激的拉曼绝热通道连贯地捕获到非辐射原子状态中,然后将其刻在量子误差校正法中。该代码在提取图像参数所需的潜在嘈杂操作中保护信号。我们表明,即使是少量的量子误差校正代码也可以为噪声提供明显的保护。对于大型代码,我们发现可以保留信息的噪声阈值。我们的方案代表了近期量子设备的应用,该设备可以将成像分辨率增加超出经典技术的可行性。
The development of high-resolution, large-baseline optical interferometers would revolutionize astronomical imaging. However, classical techniques are hindered by physical limitations including loss, noise, and the fact that the received light is generally quantum in nature. We show how to overcome these issues using quantum communication techniques. We present a general framework for using quantum error correction codes for protecting and imaging starlight received at distant telescope sites. In our scheme, the quantum state of light is coherently captured into a non-radiative atomic state via Stimulated Raman Adiabatic Passage, which is then imprinted into a quantum error correction code. The code protects the signal during subsequent potentially noisy operations necessary to extract the image parameters. We show that even a small quantum error correction code can offer significant protection against noise. For large codes, we find noise thresholds below which the information can be preserved. Our scheme represents an application for near-term quantum devices that can increase imaging resolution beyond what is feasible using classical techniques.