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dc.contributor.authorQureshi, HAen_US
dc.contributor.authorOh, Sen_US
dc.contributor.authorKhan, Nen_US
dc.contributor.authorKim, YHen_US
dc.contributor.authorNallanathan, Aen_US
dc.date.accessioned2024-07-11T13:55:35Z
dc.date.issued2024-01-01en_US
dc.identifier.issn2162-2337en_US
dc.identifier.urihttps://qmro.qmul.ac.uk/xmlui/handle/123456789/98025
dc.description.abstractThis letter investigates the effect of an extremely large (XL) simultaneously transmitting and reflecting intelligent reconfigurable surface (STAR-RIS) on the sum rate of the uplink nonorthogonal multiple access (NOMA). For the XL-STAR-RIS supporting NOMA in energy-splitting mode, we develop a sum rate maximization algorithm under the minimum rate constraints that accommodates XL-STAR-RIS in a computationally efficient way. We also analyze upper and lower bounds on the sum rate to identify governing factors of the channel models. The results show that the sum rate gain with respect to the number of STAR-RIS elements is reduced when the channels between the STAR-RIS and users become near-field, which entails the use of the correct channel model to estimate the exact value of an XL-STAR-RIS.en_US
dc.relation.ispartofIEEE Wireless Communications Lettersen_US
dc.rights© 2024 IEEE. Personal use of this material is permitted. Permission from IEEE must be obtained for all other uses, in any current or future media, including reprinting/republishing this material for advertising or promotional purposes, creating new collective works, for resale or redistribution to servers or lists, or reuse of any copyrighted component of this work in other works.
dc.titleSum Rate of Extremely Large STAR-RIS Aided Uplink NOMAen_US
dc.typeArticle
dc.identifier.doi10.1109/LWC.2024.3401690en_US
pubs.notesNot knownen_US
pubs.publication-statusPublisheden_US
rioxxterms.funderDefault funderen_US
rioxxterms.identifier.projectDefault projecten_US
rioxxterms.funder.projectb215eee3-195d-4c4f-a85d-169a4331c138en_US


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