Version 2 2025-05-09, 16:00Version 2 2025-05-09, 16:00
Version 1 2025-01-31, 17:00Version 1 2025-01-31, 17:00
preprint
posted on 2025-05-09, 16:00authored byCade Peters, Isaac Nape, Andrew Forbes
Light's spatial degree of freedom is emerging as a potential resource for a myriad of applications, in both classical and quantum domains, including secure communication, sensing and imaging. However, it has been repeatedly shown that a complex medium (atmosphere, optical fibre, turbid media, etc.) can perturb the spatial amplitude, phase and polarization of the structured light fields leading to a degradation in their performance. A promising solution to this is the use of invariant modes to whom the medium appears transparent. While the creation and robustness of these modes has been experimentally demonstrated, they are difficult to implement in many important applications due to large channel matrices, a susceptibility to numerical artefacts, non-physical solutions and unreliable performance. In this work, we outline a procedure for determining these invariant modes using a modal basis, which results in a set of eigenmodes that are free of these issues, are consistently realisable and require a much smaller channel matrix to compute. Using atmospheric turbulence and LG modes as the underlying basis as an illustrative example, we find robust modes for a variety of turbulence strengths with a basis of only 231 modes, one order of magnitude smaller than previous approaches. These modes consistently show a fidelity of above 80% after propagating through the complex channel, a significant improvement over sending the individual LG modes themselves and reveal an invariant modal spectrum through the channel. Our approach will work for any complex medium and modal basis, paving the way for the effective implementation of the eigenmode approach in real-world situations.
History
Disclaimer
This arXiv metadata record was not reviewed or approved by, nor does it necessarily express or reflect the policies or opinions of, arXiv.