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dc.contributor.authorChronister, Aaron
dc.contributor.authorPustogow, Andrej
dc.contributor.authorKikugawa, Naoki
dc.contributor.authorSokolov, Dmitry A.
dc.contributor.authorJerzembeck, Fabian
dc.contributor.authorHicks, Clifford W.
dc.contributor.authorMackenzie, A.P.
dc.contributor.authorBauer, Eric D.
dc.contributor.authorBrown, Stuart E.
dc.date.accessioned2021-12-22T00:41:10Z
dc.date.available2021-12-22T00:41:10Z
dc.date.issued2021-06-22
dc.identifier.citationChronister , A , Pustogow , A , Kikugawa , N , Sokolov , D A , Jerzembeck , F , Hicks , C W , Mackenzie , A P , Bauer , E D & Brown , S E 2021 , ' Evidence for even parity unconventional superconductivity in Sr 2 RuO 4 ' , Proceedings of the National Academy of Sciences of the United States of America , vol. 118 , no. 25 , e2025313118 . https://doi.org/10.1073/pnas.2025313118en
dc.identifier.issn0027-8424
dc.identifier.otherPURE: 274777273
dc.identifier.otherPURE UUID: f941e0a0-48fe-43fb-8002-cf61777f01b2
dc.identifier.otherRIS: urn:E4EC40D2A91ED31BD5BB784DF67D6F7B
dc.identifier.otherScopus: 85107940535
dc.identifier.otherWOS: 000675808200008
dc.identifier.urihttp://hdl.handle.net/10023/24559
dc.descriptionFunding: A.C. is grateful for support from the Julian Schwinger Foundation for Physics Research. A.P. acknowledges support by the Alexander von Humboldt Foundation through the Feodor Lynen Fellowship. Work at Los Alamos was funded by Laboratory Directed Research and Development (LDRD) program, and A.P. acknowledges partial support through the LDRD. N.K. acknowledges the support by the Grants-in-Aid for Scientific Research (KAKENHI, Grant JP18K04715 and JP21H01033) from Japan Society for the Promotion of Science (JSPS). The work at Dresden was funded by the Deutsche Forschungsgemeinschaft - TRR 288 - 422213477 (projects A10 and B01). The work at University of California, Los Angeles, was supported by NSF Grants 1709304 and 2004553.en
dc.description.abstractUnambiguous identification of the superconducting order parameter symmetry in Sr2RuO4 has remained elusive for more than a quarter century. While a chiral p-wave ground state analogue to superfluid 3He-A was ruled out only very recently, other proposed triplet-pairing scenarios are still viable. Establishing the condensate magnetic susceptibility reveals a sharp distinction between even-parity (singlet) and odd-parity (triplet) pairing since the superconducting condensate is magnetically polarizable only in the latter case. Here field-dependent 17O Knight shift measurements, being sensitive to the spin polarization, are compared to previously reported specific heat measurements for the purpose of distinguishing the condensate contribution from that due to quasiparticles. We conclude that the shift results can be accounted for entirely by the expected field-induced quasiparticle response. An upper bound for the condensate magnetic response of < 10% of the normal state susceptibility is sufficient to exclude all purely odd-parity candidates. 
dc.format.extent5
dc.language.isoeng
dc.relation.ispartofProceedings of the National Academy of Sciences of the United States of Americaen
dc.rightsCopyright © 2021 the Author(s). This work has been made available online in accordance with publisher policies or with permission. Permission for further reuse of this content should be sought from the publisher or the rights holder. This is the author created accepted manuscript following peer review and may differ slightly from the final published version. The final published version of this work is available at https://doi.org/10.1073/pnas.2025313118.en
dc.subjectUnconventional superconductivityen
dc.subjectTriplet pairingen
dc.subjectSr2RuO4en
dc.subjectNuclear magnetic resonanceen
dc.subjectKnight shiften
dc.subjectOrder parameteren
dc.subjectQC Physicsen
dc.subjectTK Electrical engineering. Electronics Nuclear engineeringen
dc.subjectDASen
dc.subject.lccQCen
dc.subject.lccTKen
dc.titleEvidence for even parity unconventional superconductivity in Sr2RuO4en
dc.typeJournal articleen
dc.description.versionPostprinten
dc.contributor.institutionUniversity of St Andrews.School of Physics and Astronomyen
dc.contributor.institutionUniversity of St Andrews.Condensed Matter Physicsen
dc.identifier.doihttps://doi.org/10.1073/pnas.2025313118
dc.description.statusPeer revieweden
dc.date.embargoedUntil2021-12-22


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