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首页> 外文期刊>Bulletin of the American Physical Society >APS -APS March Meeting 2017 - Event - Quantum enhanced interferometry using imperfect repeaters.
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APS -APS March Meeting 2017 - Event - Quantum enhanced interferometry using imperfect repeaters.

机译:APS -APS 2017年3月会议-事件-使用不完善的中继器的量子增强型干涉仪。

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The baseline size of telescopic arrays used in stellar interferometry - maximum distance between two telescopes in the array - determines the angular resolution of the array. Larger baselines lead to finer resolution of the intensity distribution of the distant extended source. Since interferometry relies on bringing the photons, collected at the distant telescopes, together for eventual interference – their loss in the connecting optical channels limits how far the baselines may be practically extended. One can use shared entangled states between the nodes of a quantum network to mitigate the effects of photon loss that leads to a loss in the sensitivity of the telescopic array. We show how using distributed entangled quantum states between two telescopes - the size of the baselines can be increased. This leads to improved angular resolution of the telescope array in the weak source regime – where the light from distant sources may be considered at the single-photon level. In our work we consider quantum networks with access to imperfectly entangled quantum states and determine their utility towards optical interferometry of signals from distant sources.
机译:恒星干涉测量中使用的望远镜阵列的基线大小-阵列中两个望远镜之间的最大距离-决定了阵列的角分辨率。较大的基线会导致较远的扩展源的强度分布更精细的分辨率。由于干涉测量法依赖于将在遥远的望远镜上收集的光子聚集在一起以最终产生干扰,因此光子在连接光学通道中的损耗限制了基线可以实际扩展的范围。可以在量子网络的节点之间使用共享的纠缠态来减轻光子损失的影响,从而导致望远镜阵列的灵敏度降低。我们展示了如何在两个望远镜之间使用分布式纠缠量子态-可以增加基线的大小。在弱光源状态下,这可以提高望远镜阵列的角分辨率-在这种情况下,可以将来自遥远光源的光视为单光子级。在我们的工作中,我们考虑可以访问不完全纠缠的量子态的量子网络,并确定其对来自遥远源的信号进行光学干涉测量的效用。

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