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Transport and entanglement of orbital angular momentum photonic states in turbulent atmosphere

湍流大气中轨道角动量光子态的传输和纠缠

基本信息

批准号：
289382917
负责人：
Professor Dr. Andreas Buchleitner
金额：
--
依托单位：
National Metrology Institute of South Africa
依托单位国家：
德国
项目类别：
Research Grants
财政年份：
2015
资助国家：
德国
起止时间：
2014-12-31 至 2018-12-31
项目状态：
已结题

来源：
https://gepris.dfg.de/gepris/projekt/289382917?language=en
关键词：
Transport entanglement orbital angular momentum

项目摘要

Photons carrying orbital angular momentum can potentially revolutionise modern free space communication technologies, owing to the ability of such photons to encode highly-dimensional Hilbert spaces in their spatial wave fronts. However, the omnipresent atmospheric turbulence distorts the wave front and thus undermines the fidelity of the transmitted information. The first part of the present project therefore aims at developing a general and innovative transport theory for the propagation of photons in atmospheric turbulence. This theory will shed new light on several fundamental questions most pertinent to the field of free-space quantum communication. In particular, it will not only allow us to better understand and quantitatively describe the effect of atmospheric decoherence on photonic orbital angular momentum states, but also clarify the physical mechanism for the occurrence of large intensity fluctuations in the transmitted beam. In the second part of our project, we will aim at demonstrating the usefulness of orbital angular momentum states for free space quantum communication or quantum information technologies. For this purpose, we will develop efficient protocols for entanglement detection, identify robust entangled states that are most stable against the atmospheric decoherence, and propose experimentally realisable ways of further reducing the detrimental effects of propagation in atmosphere using methods of adaptive optics. The theoretical work in Freiburg will be performed in close cooperation with our experimental partner group in Pretoria.

携带轨道角动量的光子可能会彻底改变现代自由空间通信技术，因为这种光子能够在其空间波阵面中编码高维希尔伯特空间。然而，无处不在的大气湍流使波前发生畸变，从而破坏了传输信息的保真度。因此，本项目的第一部分旨在为光子在大气湍流中的传播发展一个通用的和创新的传输理论。这一理论将为自由空间量子通信领域的几个基本问题提供新的思路。特别是，它不仅可以让我们更好地理解和定量描述大气退相干对光子轨道角动量态的影响，而且还可以澄清透射光束中出现大强度起伏的物理机制。在我们项目的第二部分，我们将致力于证明轨道角动量态对自由空间量子通信或量子信息技术的有用性。为此，我们将开发有效的纠缠检测协议，识别对大气退相干最稳定的稳健纠缠态，并提出实验上可实现的方法，使用自适应光学方法进一步减少大气中传播的不利影响。在弗赖堡的理论工作将与我们在比勒陀利亚的实验伙伴小组密切合作进行。