Large-Scale MIMO Transmitters for CR-NOMA in Fixed Physical Space: The Effect of Realistic System Impairments Using Stochastic Geometry

IF 5.3 Q1 ENGINEERING, ELECTRICAL & ELECTRONIC IEEE Open Journal of Vehicular Technology Pub Date : 2024-07-09 DOI:10.1109/OJVT.2024.3425061
Emmanuel Ampoma Affum;Samuel Tweneboah-Koduah;Owusu Agyeman Antwi;Benjamin Asubam Weyori;Willie Ofosu
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Abstract

Hardware impairments (HWI) are imperfections in hardware components that diminish wireless communication performance. Unlike Geometric-based Stochastic Models (GBSMs), existing works on the impact of HWI on cooperative-relay (CR) Non-Orthogonal Multiple Access (NOMA) systems employ the Correlated-based Stochastic Model (CBSM), which does not capture realistic propagation mechanisms. Moreover, studies on CR-NOMA with large antenna transmitters (LATs) using CBSM and GBSM have attracted little attention in academia. We consider this as a computational issue. Although considerable work has been done, there is still a significant knowledge gap about how HWI and imperfect successive interference cancellation affect far-users in CR-NOMA with the LAT system. In this study, the LAT is considered a cylindrical array, and parameters such as delay spread, angle of arrival, and departure are incorporated to achieve a CR-NOMA-GBSM system with amplify-and-forward (AF) or decode-and-forward (DF) relaying schemes. To reduce computing demands, we offer a novel concept of using the physical dimensions of the array to derive the location vector of the antenna element. Using Monte Carlo simulation, near and far users' BER performances deteriorate for AF and DF at 15 dB and 5 dB or below, respectively. As far-users can receive comparable performances as near-users for both AF and DF in terms of achievable rates, this demonstrates the potential rewards of CR-NOMA with LAT.
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固定物理空间中用于 CR-NOMA 的大规模 MIMO 发射机:使用随机几何的真实系统损伤的影响
硬件损伤(HWI)是硬件组件中的缺陷,会降低无线通信性能。与基于几何的随机模型(GBSM)不同,现有关于硬件损伤对合作中继(CR)非正交多址(NOMA)系统影响的研究采用的是基于相关的随机模型(CBSM),该模型无法捕捉现实的传播机制。此外,学术界对使用 CBSM 和 GBSM 的带有大型天线发射器 (LAT) 的 CR-NOMA 的研究也很少关注。我们认为这是一个计算问题。虽然已经做了大量工作,但对于 HWI 和不完美的连续干扰消除如何影响带有 LAT 系统的 CR-NOMA 中的远端用户,仍然存在很大的知识差距。在本研究中,LAT 被视为一个圆柱形阵列,并纳入了延迟扩散、到达角和离去角等参数,以实现具有放大-前向(AF)或解码-前向(DF)中继方案的 CR-NOMA-GBSM 系统。为了减少计算需求,我们提出了一个新概念,即利用阵列的物理尺寸来推导天线元件的位置矢量。通过蒙特卡洛仿真,AF 和 DF 的近端和远端用户误码率性能分别在 15 dB 和 5 dB 或更低时恶化。在可实现速率方面,AF 和 DF 的远端用户可获得与近端用户相当的性能,这证明了带有 LAT 的 CR-NOMA 的潜在回报。
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来源期刊
CiteScore
9.60
自引率
0.00%
发文量
25
审稿时长
10 weeks
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