1Liège Univ. (Belgium) 2Univ. of California, Santa Barbara (United States) 3California Institute of Technology (United States) 4Jet Propulsion Lab., California Institute of Technology (United States)
PERSONAL Sign in with your SPIE account to access your personal subscriptions or to use specific features such as save to my library, sign up for alerts, save searches, etc.
Imaging Earth-like planets around sun-like stars has become one of the main science drivers for future space telescope missions. High-contrast imaging using a vortex coronagraph has proven to be a promising approach for achieving this goal. However, at the huge contrast levels required for future space-based telescopes the vectorial nature of the well-established vector vortex phase mask becomes a limiting factor, since it imprints phase ramps of opposite signs on the two circular polarizations. An alternative polarization-independent approach is using a scalar vortex phase mask, which affects both polarizations in the same way. The achromatic performance of scalar vortex phase masks for space-based applications has still to be improved, though. Metasurfaces provide a promising approach to implement a scalar vortex phase mask with relatively simple fabrication techniques. Their demonstrated ability to implement broadband phase and amplitude masks makes them a prime candidate for achieving achromatic performance in pursuit of the 10−10 contrast limit required by NASA’s Habitable Worlds Observatory. We present a metasurface-based design of a scalar vortex phase mask providing a helical phase ramp across a large bandwidth. We first use rigorous coupled-wave analysis to create a library of square metasurface building blocks (nanoblocks) and choose an optimal set of nanoblock sizes providing broadband 2π phase coverage at a given nanoblock height. We then arrange the nanoblocks in a design providing a helical phase ramp and propagate the phase and transmission provided by the mask through a wavefront propagation software to obtain contrast curves at several wavelengths. Finally we apply electric field conjugation to dig a half-sided dark hole from 3-10 λ/D reaching 3.7 × 10−9 contrast in 20% bandwidth.
Conference Presentation
(2023) Published by SPIE. Downloading of the abstract is permitted for personal use only.
Lorenzo König,Skyler Palatnick,Niyati Desai,Olivier Absil,Maxwell Millar-Blanchaer, andDimitri Mawet
"Metasurface-based scalar vortex phase mask in pursuit of 1e-10 contrast", Proc. SPIE 12680, Techniques and Instrumentation for Detection of Exoplanets XI, 126800Q (5 October 2023); https://doi.org/10.1117/12.2676174
ACCESS THE FULL ARTICLE
INSTITUTIONAL Select your institution to access the SPIE Digital Library.
PERSONAL Sign in with your SPIE account to access your personal subscriptions or to use specific features such as save to my library, sign up for alerts, save searches, etc.
The alert did not successfully save. Please try again later.
Lorenzo König, Skyler Palatnick, Niyati Desai, Olivier Absil, Maxwell Millar-Blanchaer, Dimitri Mawet, "Metasurface-based scalar vortex phase mask in pursuit of 1e-10 contrast," Proc. SPIE 12680, Techniques and Instrumentation for Detection of Exoplanets XI, 126800Q (5 October 2023); https://doi.org/10.1117/12.2676174