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Wideband Gaussian Noise Model of Nonlinear Distortions From Semiconductor Optical Amplifiers

Optics 2026-03-16 v2 Signal Processing

Abstract

A wideband Gaussian Noise Model of the nonlinear noise power spectral density is developed for a single semiconductor optical amplifier as described by the Agrawal model. A simple, interpretable closed-form expression is obtained for the nonlinear noise-to-signal ratio of broadband wavelength-division multiplexed signals as a function of the Agrawal model parameters, the amplifier output power and the transmission bandwidth. The accuracy of the closed-form expression and its region of validity are assessed in numerical simulations. The error is smaller than 0.1 dB when the product of bandwidth and gain recovery time B×τcB\times\tau_c exceeds 100. A complete treatment of gain compression is shown to enhance nonlinear noise by a factor 1+Pout/Psat1+P_\text{out}/P_\text{sat} compared to the first-order perturbation theory result.

Keywords

Cite

@article{arxiv.2507.11517,
  title  = {Wideband Gaussian Noise Model of Nonlinear Distortions From Semiconductor Optical Amplifiers},
  author = {Hartmut Hafermann},
  journal= {arXiv preprint arXiv:2507.11517},
  year   = {2026}
}

Comments

Published in Journal of Lightwave Technology. DOI: 10.1109/JLT.2025.3643307