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Hanbury Brown and Twiss interferometry with twisted light

机译:Hanbury Brown和Twiss干涉光

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摘要

The rich physics exhibited by random optical wave fields permitted Hanbury Brown and Twiss to unveil fundamental aspects of light. Furthermore, it has been recognized that optical vortices are ubiquitous in random light and that the phase distribution around these optical singularities imprints a spectrum of orbital angular momentum onto a light field. We demonstrate that random fluctuations of intensity give rise to the formation of correlations in the orbital angular momentum components and angular positions of pseudothermal light. The presence of these correlations is manifested through distinct interference structures in the orbital angular momentum–mode distribution of random light. These novel forms of interference correspond to the azimuthal analog of the Hanbury Brown and Twiss effect. This family of effects can be of fundamental importance in applications where entanglement is not required and where correlations in angular position and orbital angular momentum suffice. We also suggest that the azimuthal Hanbury Brown and Twiss effect can be useful in the exploration of novel phenomena in other branches of physics and astrophysics.
机译:随机光波场表现出的丰富物理特性使Hanbury Brown和Twiss揭示了光的基本方面。此外,已经认识到光学涡旋在随机光中无处不在,并且这些光学奇点周围的相位分布将轨道角动量谱印在光场上。我们证明强度的随机波动会引起轨道角动量分量和伪热光的角位置之间的相关性的形成。这些相关性的存在通过随机光在轨道角动量-模式分布中的明显干涉结构得以体现。这些新颖的干扰形式对应于汉伯里·布朗和特维斯效应的方位角类似物。在不需要纠缠且角位置和轨道角动量的相关性足够的应用中,这一系列效应可能具有根本的重要性。我们还建议,方位角的汉伯里·布朗(Hanbury Brown)和特维斯(Twiss)效应可用于探索物理学和天体物理学其他分支中的新现象。

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