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dc.contributor.authorCowan, KJ
dc.contributor.authorBerry, SJ
dc.contributor.authorHibbins, AP
dc.contributor.authorPowell, AW
dc.date.accessioned2024-11-01T13:14:04Z
dc.date.issued2024-10-28
dc.date.updated2024-11-01T11:41:58Z
dc.description.abstractDark modes are defined by their lack of radiative coupling to the far field. However, the modes can be made to couple to far field radiation by symmetry breaking. For a resonant dimer, obliquely incident waves can create a phase difference in the currents between the elements, resulting in symmetry breaking. This work reduces symmetry breaking effects by minimizing the size of a dimer of dipolar elements with respect to its resonant wavelength. We obtain a mode that can experimentally be excited from the near field but has negligible excitation in the far field for obliquely incident waves. Such a mode could have use in wireless security applications.en_GB
dc.description.sponsorshipEngineering and Physical Sciences Research Council (EPSRC)en_GB
dc.description.sponsorshipQinetiQen_GB
dc.identifier.citationVol. 125, No. 18, article 181101en_GB
dc.identifier.doihttps://doi.org/10.1063/5.0227519
dc.identifier.grantnumberEP/X524906/1en_GB
dc.identifier.grantnumber220181en_GB
dc.identifier.urihttp://hdl.handle.net/10871/137877
dc.identifierORCID: 0000-0001-5406-0162 (Hibbins, Alastair P)
dc.identifierScopusID: 6603571907 (Hibbins, Alastair P)
dc.identifierORCID: 0000-0001-6357-5408 (Powell, Alexander W)
dc.language.isoenen_GB
dc.publisherAIP Publishingen_GB
dc.rights© 2024 Author(s). All article content, except where otherwise noted, is licensed under a Creative Commons Attribution (CC BY) license (https:// creativecommons.org/licenses/by/4.0/).en_GB
dc.subjectResonanceen_GB
dc.subjectResonator deviceen_GB
dc.subjectElectromagnetic scatteringen_GB
dc.subjectMicrowave radiationen_GB
dc.subjectMicrowave frequenciesen_GB
dc.subjectNear field communicationen_GB
dc.subjectRADARen_GB
dc.titleKeeping dark modes dark: Reducing the effects of symmetry breaking at oblique incidenceen_GB
dc.typeArticleen_GB
dc.date.available2024-11-01T13:14:04Z
dc.identifier.issn0003-6951
dc.descriptionThis is the final version. Available from AIP Publishing via the DOI in this record. en_GB
dc.descriptionDATA AVAILABILITY: The data that support the findings of this study are available from the corresponding author upon reasonable request.en_GB
dc.identifier.eissn1077-3118
dc.identifier.journalApplied Physics Lettersen_GB
dc.relation.ispartofApplied Physics Letters, 125(18)
dc.rights.urihttp://creativecommons.org/licenses/by/4.0/en_GB
dcterms.dateAccepted2024-10-15
rioxxterms.versionVoRen_GB
rioxxterms.licenseref.startdate2024-10-28
rioxxterms.typeJournal Article/Reviewen_GB
refterms.dateFCD2024-11-01T13:10:03Z
refterms.versionFCDVoR
refterms.dateFOA2025-03-07T01:03:12Z
refterms.panelBen_GB
refterms.dateFirstOnline2024-10-28
exeter.rights-retention-statementNo


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© 2024 Author(s). All article content, except where otherwise noted, is licensed under a Creative Commons Attribution (CC BY) license (https:// creativecommons.org/licenses/by/4.0/).
Except where otherwise noted, this item's licence is described as © 2024 Author(s). All article content, except where otherwise noted, is licensed under a Creative Commons Attribution (CC BY) license (https:// creativecommons.org/licenses/by/4.0/).