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Article: STAR-IOS Aided NOMA Networks: Channel Model Approximation and Performance Analysis

TitleSTAR-IOS Aided NOMA Networks: Channel Model Approximation and Performance Analysis
Authors
KeywordsIntelligent omini-surface
non-orthogonal multiple access
physical layer channel model approximation
reconfigurable intelligent surfaces
Issue Date2022
Citation
IEEE Transactions on Wireless Communications, 2022, v. 21, n. 9, p. 6861-6876 How to Cite?
AbstractCompared with the conventional reconfigurable intelligent surfaces (RIS), simultaneous transmitting and reflecting intelligent omini-surfaces (STAR-IOSs) are able to achieve 360° coverage 'smart radio environments'. By splitting the energy or altering the active number of STAR-IOS elements, STAR-IOSs provide high flexibility of successive interference cancellation (SIC) orders for non-orthogonal multiple access (NOMA) systems. Based on the aforementioned advantages, this paper investigates a STAR-IOS-aided downlink NOMA network with randomly deployed users. We first propose three tractable channel models for different application scenarios, namely the central limit model, the curve fitting model, and the M-fold convolution model. More specifically, the central limit model fits the scenarios with large-size STAR-IOSs while the curve fitting model is extended to evaluate multi-cell networks. However, these two models cannot obtain accurate diversity orders. Hence, we figure out the M-fold convolution model to derive accurate diversity orders. We consider three protocols for STAR-IOSs, namely, the energy splitting (ES) protocol, the time switching (TS) protocol, and the mode switching (MS) protocol. Based on the ES protocol, we derive closed-form analytical expressions of outage probabilities for the paired NOMA users by the central limit model and the curve fitting model. Based on three STAR-IOS protocols, we derive the diversity gains of NOMA users by the M-fold convolution model. The analytical results reveal that the diversity gain of NOMA users is equal to the active number of STAR-IOS elements. Numerical results indicate that 1) in high signal-to-noise ratio regions, the central limit model performs as an upper bound of the simulation results, while a lower bound is obtained by the curve fitting model; 2) the TS protocol has the best performance but requesting more time blocks than other protocols; 3) the ES protocol outperforms the MS protocol as the ES protocol has higher diversity gains.
Persistent Identifierhttp://hdl.handle.net/10722/349697
ISSN
2023 Impact Factor: 8.9
2023 SCImago Journal Rankings: 5.371

 

DC FieldValueLanguage
dc.contributor.authorZhang, Chao-
dc.contributor.authorYi, Wenqiang-
dc.contributor.authorLiu, Yuanwei-
dc.contributor.authorDing, Zhiguo-
dc.contributor.authorSong, Lingyang-
dc.date.accessioned2024-10-17T07:00:12Z-
dc.date.available2024-10-17T07:00:12Z-
dc.date.issued2022-
dc.identifier.citationIEEE Transactions on Wireless Communications, 2022, v. 21, n. 9, p. 6861-6876-
dc.identifier.issn1536-1276-
dc.identifier.urihttp://hdl.handle.net/10722/349697-
dc.description.abstractCompared with the conventional reconfigurable intelligent surfaces (RIS), simultaneous transmitting and reflecting intelligent omini-surfaces (STAR-IOSs) are able to achieve 360° coverage 'smart radio environments'. By splitting the energy or altering the active number of STAR-IOS elements, STAR-IOSs provide high flexibility of successive interference cancellation (SIC) orders for non-orthogonal multiple access (NOMA) systems. Based on the aforementioned advantages, this paper investigates a STAR-IOS-aided downlink NOMA network with randomly deployed users. We first propose three tractable channel models for different application scenarios, namely the central limit model, the curve fitting model, and the M-fold convolution model. More specifically, the central limit model fits the scenarios with large-size STAR-IOSs while the curve fitting model is extended to evaluate multi-cell networks. However, these two models cannot obtain accurate diversity orders. Hence, we figure out the M-fold convolution model to derive accurate diversity orders. We consider three protocols for STAR-IOSs, namely, the energy splitting (ES) protocol, the time switching (TS) protocol, and the mode switching (MS) protocol. Based on the ES protocol, we derive closed-form analytical expressions of outage probabilities for the paired NOMA users by the central limit model and the curve fitting model. Based on three STAR-IOS protocols, we derive the diversity gains of NOMA users by the M-fold convolution model. The analytical results reveal that the diversity gain of NOMA users is equal to the active number of STAR-IOS elements. Numerical results indicate that 1) in high signal-to-noise ratio regions, the central limit model performs as an upper bound of the simulation results, while a lower bound is obtained by the curve fitting model; 2) the TS protocol has the best performance but requesting more time blocks than other protocols; 3) the ES protocol outperforms the MS protocol as the ES protocol has higher diversity gains.-
dc.languageeng-
dc.relation.ispartofIEEE Transactions on Wireless Communications-
dc.subjectIntelligent omini-surface-
dc.subjectnon-orthogonal multiple access-
dc.subjectphysical layer channel model approximation-
dc.subjectreconfigurable intelligent surfaces-
dc.titleSTAR-IOS Aided NOMA Networks: Channel Model Approximation and Performance Analysis-
dc.typeArticle-
dc.description.naturelink_to_subscribed_fulltext-
dc.identifier.doi10.1109/TWC.2022.3152703-
dc.identifier.scopuseid_2-s2.0-85125705136-
dc.identifier.volume21-
dc.identifier.issue9-
dc.identifier.spage6861-
dc.identifier.epage6876-
dc.identifier.eissn1558-2248-

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