# Cooperative Rate-Splitting for MISO Broadcast Channel with User   Relaying, and Performance Benefits over Cooperative NOMA

**Authors:** Jian Zhang, Bruno Clerckx, Jianhua Ge, and Yijie Mao

arXiv: 1906.07761 · 2020-01-08

## TL;DR

This paper introduces a Cooperative Rate-Splitting strategy for MISO broadcast channels with user relaying, showing it outperforms non-cooperative and NOMA strategies in various propagation conditions.

## Contribution

It proposes a novel CRS scheme with optimized precoding and resource allocation, enhancing rate regions over existing cooperative and non-cooperative methods.

## Key findings

- CRS achieves higher sum rates than non-cooperative schemes.
- CRS outperforms cooperative NOMA in diverse channel conditions.
- Optimized precoding improves overall system performance.

## Abstract

Due to its promising performance in a wide range of practical scenarios, Rate-Splitting (RS) has recently received significant attention in academia for the downlink of communication systems. In this letter, we propose and analyse a Cooperative Rate-Splitting (CRS) strategy based on the three-node relay channel where the transmitter is equipped with multiple antennas. By splitting user messages and linearly precoding common and private streams at the transmitter, and opportunistically asking the relaying user to forward its decoded common message, CRS can efficiently cope with a wide range of propagation conditions (disparity of user channel strengths and directions) and compensate for the performance degradation due to deep fading. The precoder design and the resource allocation are optimized by solving the Weighted Sum Rate (WSR) maximization problem. Numerical results demonstrate that our proposed CRS scheme can achieve an explicit rate region improvement compared to its non-cooperative counterpart and other cooperative strategies (such as cooperative NOMA).

## Full text

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## Figures

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## References

25 references — full list in the complete paper: https://tomesphere.com/paper/1906.07761/full.md

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Source: https://tomesphere.com/paper/1906.07761