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dc.contributor.authorSilaev, Mikhail
dc.contributor.authorGaraud, Julien
dc.contributor.authorBabaev, Egor
dc.date.accessioned2017-02-27T10:48:53Z
dc.date.available2017-02-27T10:48:53Z
dc.date.issued2017
dc.identifier.citationSilaev, M., Garaud, J., & Babaev, E. (2017). Phase diagram of dirty two-band superconductors and observability of impurity-induced s + i s state. <i>Physical Review B</i>, <i>95</i>(2), 024517. <a href="https://doi.org/10.1103/PhysRevB.95.024517" target="_blank">https://doi.org/10.1103/PhysRevB.95.024517</a>
dc.identifier.otherCONVID_26549235
dc.identifier.otherTUTKAID_72990
dc.identifier.urihttps://jyx.jyu.fi/handle/123456789/53108
dc.description.abstractWe investigate the phase diagram of dirty two-band superconductors. This paper primarily focuses on the properties and observability of the time-reversal symmetry-breaking s + is superconducting states, which can be generated in two-band superconductors by interband impurity scattering. We show that such states can appear in two distinct ways. First, according to a previously discussed scenario, the s + is state can form as an intermediate phase at the impurity-driven crossover between s± and s++ states. We show that there is a second scenario where domains of the s + is state exists in the form of an isolated dome inside the s± domain, completely detached from the transition between s± and s++ states. We demonstrate that in both cases the s + is state generated by impurity scattering exists in an extremely small interval of impurity concentrations. Although this likely precludes direct experimental observation of the s + is state formation due to this mechanism, this physics leads to the appearance of a region inside both the s± and s++ domains with unusual properties due to softening of normal modes.
dc.language.isoeng
dc.publisherAmerican Physical Society
dc.relation.ispartofseriesPhysical Review B
dc.subject.otherphase diagrams
dc.titlePhase diagram of dirty two-band superconductors and observability of impurity-induced s + i s state
dc.typearticle
dc.identifier.urnURN:NBN:fi:jyu-201702141442
dc.contributor.laitosFysiikan laitosfi
dc.contributor.laitosDepartment of Physicsen
dc.contributor.oppiaineFysiikkafi
dc.contributor.oppiaineNanoscience Centerfi
dc.contributor.oppiainePhysicsen
dc.contributor.oppiaineNanoscience Centeren
dc.type.urihttp://purl.org/eprint/type/JournalArticle
dc.date.updated2017-02-14T13:15:15Z
dc.type.coarhttp://purl.org/coar/resource_type/c_2df8fbb1
dc.description.reviewstatuspeerReviewed
dc.format.pagerange024517
dc.relation.issn2469-9950
dc.relation.numberinseries2
dc.relation.volume95
dc.type.versionpublishedVersion
dc.rights.copyright© 2017 American Physical Society. Published in this repository with the kind permission of the publisher.
dc.rights.accesslevelopenAccessfi
dc.subject.ysosuprajohteet
jyx.subject.urihttp://www.yso.fi/onto/yso/p9946
dc.relation.doi10.1103/PhysRevB.95.024517
dc.type.okmA1


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