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dc.contributor.authorMackenzie, Andrew P
dc.contributor.authorScaffidi, Thomas
dc.contributor.authorHicks, Clifford W
dc.contributor.authorMaeno, Yoshiteru
dc.date.accessioned2017-07-20T09:30:10Z
dc.date.available2017-07-20T09:30:10Z
dc.date.issued2017-07-18
dc.identifier250512202
dc.identifierf2ed79ce-02b5-4def-b488-d662e7813375
dc.identifier85032361449
dc.identifier000407434200001
dc.identifier.citationMackenzie , A P , Scaffidi , T , Hicks , C W & Maeno , Y 2017 , ' Even odder after twenty-three years : the superconducting order parameter puzzle of Sr 2 RuO 4 ' , npj Quantum Materials , vol. 2 , 40 . https://doi.org/10.1038/s41535-017-0045-4en
dc.identifier.issn2397-4648
dc.identifier.otherArXiv: http://arxiv.org/abs/1706.01942v1
dc.identifier.urihttps://hdl.handle.net/10023/11256
dc.descriptionFunding: Max Planck Society.en
dc.description.abstractIn this short review, we aim to provide a topical update on the status of efforts to understand the superconductivity of Sr2RuO4. We concentrate on the quest to identify a superconducting order parameter symmetry that is compatible with all the major pieces of experimental knowledge of the material, and highlight some major discrepancies that have become even clearer in recent years. As the pun in the title suggests, we have tried to start the discussion from scratch, making no assumptions even about fundamental issues such as the parity of the superconducting state. We conclude that no consensus is currently achievable in Sr2RuO4, and that the reasons for this go to the heart of how well some of the key probes of unconventional superconductivity are really understood. This is therefore a puzzle that merits continued in-depth study.
dc.format.extent9
dc.format.extent1281116
dc.language.isoeng
dc.relation.ispartofnpj Quantum Materialsen
dc.subjectQC Physicsen
dc.subjectT Technologyen
dc.subject.lccQCen
dc.subject.lccTen
dc.titleEven odder after twenty-three years : the superconducting order parameter puzzle of Sr2RuO4en
dc.typeJournal itemen
dc.contributor.institutionUniversity of St Andrews. School of Physics and Astronomyen
dc.contributor.institutionUniversity of St Andrews. Condensed Matter Physicsen
dc.identifier.doi10.1038/s41535-017-0045-4
dc.description.statusPeer revieweden


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