A Mach-Zehnder interferometer based on orbital angular momentum for improved vortex coronagraph efficiency
P. Piron, C. Delacroix, E. Huby, D. Mawet, M. Karlsson ad, G. Ruane, S. Habraken, O. Absil, J. Surdej

TL;DR
This paper proposes a Mach-Zehnder interferometer utilizing orbital angular momentum to enhance vortex coronagraph efficiency, addressing birefringence issues with wave-plate compensation and providing a detailed mathematical model.
Contribution
It introduces a novel interferometer design with birefringent wave-plates to improve nulling performance in vortex coronagraphs, supported by a comprehensive Jones formalism analysis.
Findings
Performance improved with birefringent plate compensation
Mathematical model developed using Jones formalism
Potential for better star-planet contrast enhancement
Abstract
The Annular Groove Phase Mask (AGPM) is a vectorial vortex phase mask. It acts as a half-wave plate with a radial fast axis orientation operating in the mid infrared domain. When placed at the focus of a telescope element provides a continuous helical phase ramp for an on axis sources, which creates the orbital angular momentum. Thanks to that phase, the intensity of the central source is canceled by a down-stream pupil stop, while the off axis sources are not affected. However due to experimental conditions the nulling is hardly perfect. To improve the null, a Mach-Zehnder interferometer containing Dove prisms differently oriented can be proposed to sort out light based on its orbital angular momentum (OAM). Thanks to the differential rotation of the beam, a {\pi} phase shift is achieved for the on axis light affected by a non zero OAM. Therefore the contrast between the star and its…
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