Enhancing the performance of NOMA-based VLC systems using a proposed adaptive superimposed constellation Algorithm with an exact SER analysis

IF 2.5 3区 物理与天体物理 Q2 OPTICS Optics Communications Pub Date : 2025-06-01 Epub Date: 2025-03-06 DOI:10.1016/j.optcom.2025.131701
Androw Sobhy , Shaimaa ElSayed , Hala Abd El-kader Mansour , Maher Abdelrasoul , Esraa M. Eid
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Abstract

Non-orthogonal multiple access (NOMA) is an impressive multi-access technology that enhances the spectral efficiency of visible light communication (VLC) systems. However, improved spectral efficiency might lead to performance reduction. To resolve this issue, this paper proposes an innovative approach termed the adaptive superimposed constellation algorithm (ASCA), which is intended for NOMA-based VLC systems. The proposed algorithm includes two fundamental methods: the optimal power allocation factor (OPAF) and adaptive M-QAM selection (AMS). The OPAF method determines the appropriate PA, ensuring non-overlapping decision regions for superimposed constellation symbols across different modulation orders supported by corresponding theoretical results. The AMS method dynamically selects the M-QAM modulation order for users, striking a balance between communication quality and data transmission rates. These methods collectively improve fairness among users, reduce the symbol error rate (SER), analyze limitations regarding the total number of users the system can serve, and evaluate the system's capacity to support multiple users effectively. This paper offers closed-form SER expressions for served users based on square QAM modulation and an imperfect successive interference cancellation (SIC) scenario. Theoretical analysis and simulations confirm the findings. The simulation results show that the proposed algorithm achieves better SER performance than other power domain (PD) NOMA schemes, making it a reliable and efficient solution for integrating NOMA into VLC systems.
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提出了一种具有精确SER分析的自适应叠加星座算法来提高基于noma的VLC系统的性能
非正交多址(NOMA)是一种令人印象深刻的多址技术,可以提高可见光通信(VLC)系统的频谱效率。然而,提高频谱效率可能会导致性能下降。为了解决这一问题,本文提出了一种创新的方法,称为自适应叠加星座算法(ASCA),用于基于noma的VLC系统。该算法包括最优功率分配因子(OPAF)和自适应M-QAM选择(AMS)两种基本方法。OPAF方法确定了适当的PA,保证了不同调制阶间重叠星座符号的决策区域不重叠,并得到相应理论结果的支持。AMS方法动态地为用户选择M-QAM调制顺序,在通信质量和数据传输速率之间取得平衡。这些方法共同提高了用户之间的公平性,降低了符号错误率(SER),分析了系统可以服务的用户总数的限制,并评估了系统有效支持多用户的能力。本文给出了基于方形QAM调制和不完全连续干扰消除(SIC)场景的服务用户的封闭SER表达式。理论分析和模拟证实了这一发现。仿真结果表明,该算法比其他功率域(PD) NOMA方案具有更好的SER性能,是将NOMA集成到VLC系统中可靠、高效的解决方案。
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来源期刊
Optics Communications
Optics Communications 物理-光学
CiteScore
5.10
自引率
8.30%
发文量
681
审稿时长
38 days
期刊介绍: Optics Communications invites original and timely contributions containing new results in various fields of optics and photonics. The journal considers theoretical and experimental research in areas ranging from the fundamental properties of light to technological applications. Topics covered include classical and quantum optics, optical physics and light-matter interactions, lasers, imaging, guided-wave optics and optical information processing. Manuscripts should offer clear evidence of novelty and significance. Papers concentrating on mathematical and computational issues, with limited connection to optics, are not suitable for publication in the Journal. Similarly, small technical advances, or papers concerned only with engineering applications or issues of materials science fall outside the journal scope.
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