Enhancing four-wave mixing efficiency in optical fibers: the role of core radius fluctuations and mitigation strategies

We introduce a versatile, easy-to-implement Gaussian process model that provides a flexible framework for modeling core-radius fluctuations of an optical fiber. The flexibility of the model allows for easy modification of the fiber profile to fit known characteristics, such as forcing the profile through carefully measured radii at specific points. The model is then used to show the drastic impact that fluctuations have on the efficiency of wide-spanning four-wave mixing systems. Furthermore, by optimizing the fiber design of a simple step-index fiber, we show that the efficiency of the four-wave mixing can be drastically improved even in the presence of large core-radius fluctuations.

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Publication Details

Journal
Optics Express
Published
2025-05-05
DOI
https://doi.org/10.1364/oe.558307
Citations
1
Primary Topic
Optical Network Technologies
Type
article
Field-Weighted Citation Impact
0.73

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Enhancing four-wave mixing efficiency in optical fibers: the role of core radius fluctuations and mitigation strategies

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Enhancing four-wave mixing efficiency in optical fibers: the role of core radius fluctuations and mitigation strategies

Lars Søgaard Rishøj, Jacob G. Koefoed, Michael Galili, Karsten Rottwitt, Thjalfe Ulvenberg
article en
1 citations

Abstract

We introduce a versatile, easy-to-implement Gaussian process model that provides a flexible framework for modeling core-radius fluctuations of an optical fiber. The flexibility of the model allows for easy modification of the fiber profile to fit known characteristics, such as forcing the profile through carefully measured radii at specific points. The model is then used to show the drastic impact that fluctuations have on the efficiency of wide-spanning four-wave mixing systems. Furthermore, by optimizing the fiber design of a simple step-index fiber, we show that the efficiency of the four-wave mixing can be drastically improved even in the presence of large core-radius fluctuations.

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