Simulations of mode-selective photonic lanterns for efficient coupling of starlight into the single-mode regime
Momen Diab (1), Aashana Tripathi (1), John Davenport (1), Aline N., Dinkelaker (1), Kalaga Madhav (1), Martin M. Roth (1) ((1) innoFSPEC, Leibniz, Institute for Astrophysics Potsdam)

TL;DR
This paper demonstrates through simulations that mode-selective photonic lanterns can efficiently couple partially corrected starlight into fewer single-mode outputs, improving astronomical instrumentation.
Contribution
It introduces a mode-selective photonic lantern design and shows its effectiveness in reducing output channels for coupled starlight.
Findings
Two waveguides carry >95% of coupled light at D/r0 < 10
Mode-selective lanterns outperform non-selective ones in efficiency
Partial wavefront correction enhances coupling efficiency
Abstract
In ground-based astronomy, starlight distorted by the atmosphere couples poorly into single-mode waveguides but a correction by adaptive optics, even if only partial, can boost coupling into the few-mode regime allowing the use of photonic lanterns to convert into multiple single-mode beams. Corrected wavefronts result in focal patterns that couple mostly with the circularly symmetric waveguide modes. A mode-selective photonic lantern is hence proposed to convert the multimode light into a subset of the single-mode waveguides of the standard photonic lantern, thereby reducing the required number of outputs. We ran simulations to show that only two out of the six waveguides of a 1x6 photonic lantern carry >95% of the coupled light to the outputs at if the wavefront is partially corrected and the photonic lantern is made mode-selective.
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