A Metasurface-Based Scalar Vortex Phase Mask Design

L. König, O. Absil, Niyati Desai, Dimitri Mawet, Skyler Palatnick, M. Millar-Blanchaer
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引用次数: 1

Abstract

The technique best suited for direct imaging of exoplanets is high contrast direct imaging using a coronagraph. In particular, the vortex coronagraph has proven to be one of the most promising approaches for imaging Earth-like planets with future space-based optical/infrared telescopes. However, differential polarization aberrations become difficult to control at the high contrasts required for this goal, requiring careful wavefront control in both polarizations independently. While the well-established vector vortex coronagraph is polarization-sensitive, a polarization-independent (scalar) vortex coronagraph circumvents this issue since it imprints the same phase ramp regardless of polarization [1]. Metasurfaces provide a promising approach for implementing a scalar vortex with relatively simple microfabrication techniques. The freedom introduced by different design topologies makes them a prime candidate for achieving achromatic performance.
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基于超表面的标量涡旋相位掩模设计
最适合系外行星直接成像的技术是使用日冕仪进行高对比度直接成像。特别是,涡旋日冕仪已被证明是未来天基光学/红外望远镜成像类地行星最有前途的方法之一。然而,微分偏振像差在高对比度下很难控制,需要在两个偏振中独立地仔细控制波前。虽然成熟的矢量涡旋日冕仪对极化敏感,但与极化无关的(标量)涡旋日冕仪避开了这一问题,因为无论极化如何,它都会留下相同的相位斜坡[1]。通过相对简单的微加工技术,元表面为实现标量涡旋提供了一种很有前途的方法。由不同的设计拓扑引入的自由度使它们成为实现消色差性能的主要候选。
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