论文标题

扩展纤维非线性干扰能力建模以说明一般双极化4D调制格式

Extending fibre nonlinear interference power modelling to account for general dual-polarisation 4D modulation formats

论文作者

Liga, Gabriele, Barreiro, Astrid, Rabbani, Hami, Alvarado, Alex

论文摘要

在光学通信中,四维(4D)调制格式将信息编码在光场极化的两个任意正交状态的正交成分上。这些格式最近由于其潜在的功率效率,非线性耐受性以及最终未开发的塑造增益而重新引起了人们的关注。与纤维光通道一样,塑形增益与给定调制格式的非线性耐受性密切相关,预测非线性的效果是有效优化传输星座的关键。光学通信文献中可用的许多分析模型允许在一阶扰动框架内,即在相干纤维光线传输系统中累积的非线性干扰(NLI)平均功率的计算。但是,所有当前模型仅在传播的极化 - 多形的二维(PM-2D)调制格式的假设下运行。 PM-2D格式代表了可能的双极化4D格式的有限子集,即,仅在每个极化通道上传输的数据是相互独立且分布相同的数据。本文档提出了将现有NLI模型扩展到任意双极化4D调制格式的逐步数学推导。特别是,所采用的方法遵循流行的增强高斯噪声模型之一,尽管在传输4D调制格式的几何形状和统计上删除了大多数假设。最终表达式表明,尽管在PM-2D情况下,NLI功率仅取决于每个极化成分的不同统计高阶矩,但对于一般的4D星座,还需要考虑其他几个交叉极化相关性。

In optical communications, four-dimensional (4D) modulation formats encode information onto the quadrature components of two arbitrary orthogonal states of polarisation of the optical field. These formats have recently regained attention due their potential power efficiency, nonlinearity tolerance, and ultimately to their still unexplored shaping gains. As in the fibre-optic channel the shaping gain is closely related to the nonlinearity tolerance of a given modulation format, predicting the effect of nonlinearity is key to effectively optimise the transmitted constellation. Many analytical models available in the optical communication literature allow, within a first-order perturbation framework, the computation of the average power of the nonlinear interference (NLI) accumulated in coherent fibre-optic transmission systems. However, all current models only operate under the assumption of a transmitted polarisation-multiplexed, two-dimensional (PM-2D) modulation format. PM-2D formats represent a limited subset of the possible dual-polarisation 4D formats, namely, only those where data transmitted on each polarisation channel are mutually independent and identically distributed. This document presents a step-by-step mathematical derivation of the extension of existing NLI models to the class of arbitrary dual-polarisation 4D modulation formats. In particular, the methodology adopted follows the one of the popular enhanced Gaussian noise model, albeit dropping most assumptions on the geometry and statistic of the transmitted 4D modulation format. The resulting expressions show that, whilst in the PM-2D case the NLI power depends only on different statistical high-order moments of each polarisation component, for a general 4D constellation also several others cross-polarisation correlations need to be taken into account.

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