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dc.contributor.authorVadimov, V. L.
dc.contributor.authorSilaev, Mikhail
dc.date.accessioned2018-09-24T10:03:24Z
dc.date.available2018-09-24T10:03:24Z
dc.date.issued2018
dc.identifier.citationVadimov, V. L., & Silaev, M. (2018). Polarization of the spontaneous magnetic field and magnetic fluctuations in s+is anisotropic multiband superconductors. <i>Physical Review B</i>, <i>98</i>(10), Article 104504. <a href="https://doi.org/10.1103/physrevb.98.104504" target="_blank">https://doi.org/10.1103/physrevb.98.104504</a>
dc.identifier.otherCONVID_28255653
dc.identifier.otherTUTKAID_78790
dc.identifier.urihttps://jyx.jyu.fi/handle/123456789/59629
dc.description.abstractWe show that multiband superconductors with broken time-reversal symmetry can produce spontaneous currents and magnetic fields in response to the local variations of pairing constants. Considering the iron pnictide superconductor Ba1−xKxFe2As2 as an example we demonstrate that both the point-group symmetric s+is state and the C4-symmetry-breaking s+id states produce, in general, the same magnitudes of spontaneous magnetic fields. In the s+is state these fields are polarized mainly on an ab crystal plane, whereas in the s+id state their ab-plane and c-axis components are of the same order. The same is true for the random magnetic fields which are produced by the order parameter fluctuations near the critical point of the time-reversal symmetry-breaking phase transition. Our findings can be used as a direct test of the s+is/s+id dichotomy and the additional discrete symmetry-breaking phase transitions with the help of muon spin-relaxation experiments.en
dc.format.mimetypeapplication/pdf
dc.languageeng
dc.language.isoeng
dc.publisherAmerican Physical Society
dc.relation.ispartofseriesPhysical Review B
dc.rightsCC BY 4.0
dc.subject.othermagneettikentätfi
dc.subject.othersuprajohteetfi
dc.subject.othermagnetic fieldsfi
dc.subject.othersuperconductorsfi
dc.titlePolarization of the spontaneous magnetic field and magnetic fluctuations in s+is anisotropic multiband superconductors
dc.typearticle
dc.identifier.urnURN:NBN:fi:jyu-201809124090
dc.contributor.laitosFysiikan laitosfi
dc.contributor.laitosDepartment of Physicsen
dc.contributor.oppiaineNanoscience Centerfi
dc.contributor.oppiaineNanoscience Centeren
dc.type.urihttp://purl.org/eprint/type/JournalArticle
dc.date.updated2018-09-12T12:15:21Z
dc.type.coarhttp://purl.org/coar/resource_type/c_2df8fbb1
dc.description.reviewstatuspeerReviewed
dc.relation.issn2469-9950
dc.relation.numberinseries10
dc.relation.volume98
dc.type.versionpublishedVersion
dc.rights.copyright© 2018 American Physical Society
dc.rights.accesslevelopenAccessfi
dc.relation.grantnumber297439
dc.subject.ysosuprajohteet
dc.subject.ysomagneettikentät
dc.format.contentfulltext
jyx.subject.urihttp://www.yso.fi/onto/yso/p9946
jyx.subject.urihttp://www.yso.fi/onto/yso/p19032
dc.rights.urlhttps://creativecommons.org/licenses/by/4.0/
dc.relation.doi10.1103/physrevb.98.104504
dc.relation.funderSuomen Akatemiafi
dc.relation.funderResearch Council of Finlanden
jyx.fundingprogramAkatemiatutkija, SAfi
jyx.fundingprogramAcademy Research Fellow, AoFen
jyx.fundinginformationThis work was supported by the Academy of Finland (Project No. 297439), the Russian Foundation for Basic Research (Grants No. 17-52-12044 and No. 18-02-00390), and the Foundation for the Advancement of Theoretical Physics “BASIS” Grant No. 109.
dc.type.okmA1


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