# Dissipative Soliton Mediated Radiations in Active Silicon-Based Waveguides

## TL;DR

This paper investigates how dissipative solitons in silicon-based active waveguides can radiate dispersive waves due to third-order dispersion, with theoretical predictions and numerical simulations revealing multiple radiation frequencies influenced by various parameters.

## Contribution

It introduces a silicon-based active waveguide design supporting stable dissipative solitons and derives a phase-matching condition to predict multiple radiation frequencies.

## Key findings

- Stable dissipative solitons can radiate dispersive waves in presence of third-order dispersion.
- The phase-matching relation accurately predicts the radiation frequencies.
- Free carriers from two-photon absorption influence the radiation dynamics.

## Abstract

The Ginzburg-Landau (GL) equation is in general not integrable by the inverse scattering method and support solitary-wave solution, called dissipative soliton (DS). We numerically demonstrate that, a DS can radiate dispersive waves (DWs) in presence of third-order dispersion (TOD). We propose a silicon-based active waveguide that excites stable DSs. Energy can be transferred from these stable DS to linear DWs when a resonance condition is achieved. The dynamics of the DS is governed by the complex GL equation which we solve numerically for different operational parameters. Numerical solution of the perturbed GL equation exhibits multiple radiations, when the stable DS is allowed to propagate through a large distance. We theoretically derive a special phase-matching relation that can predict the frequencies of these multiple radiations, which are found numerically. In our theoretical and numerical calculations we include the role of free carriers which appear inside semiconductor waveguides as a consequence of two-photon absorption (TPA). We demonstrate that apart from TOD, TPA and gain dispersion are two additional parameters that can control the radiation emitted by DS. The DS-mediated radiation is different in nature and demands an intuitive understanding. In this work we try to provide some insights of this fascinating radiation phenomenon by elaborate analytical and numerical calculations.