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PhysRevLett.112.156404.pdf541.91 kBAdobe PDF見る/開く
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dc.contributor.authorShimozawa, M.en
dc.contributor.authorGoh, S. K.en
dc.contributor.authorEndo, R.en
dc.contributor.authorKobayashi, R.en
dc.contributor.authorWatashige, T.en
dc.contributor.authorMizukami, Y.en
dc.contributor.authorIkeda, H.en
dc.contributor.authorShishido, H.en
dc.contributor.authorYanase, Y.en
dc.contributor.authorTerashima, T.en
dc.contributor.authorShibauchi, T.en
dc.contributor.authorMatsuda, Y.en
dc.contributor.alternative下澤, 雅明ja
dc.date.accessioned2014-06-06T05:59:39Z-
dc.date.available2014-06-06T05:59:39Z-
dc.date.issued2014-04-18-
dc.identifier.issn0031-9007-
dc.identifier.urihttp://hdl.handle.net/2433/187796-
dc.description.abstractBy using a molecular beam epitaxy technique, we fabricate a new type of superconducting superlattices with controlled atomic layer thicknesses of alternating blocks between the heavy-fermion superconductor CeCoIn[5], which exhibits a strong Pauli pair-breaking effect, and nonmagnetic metal YbCoIn[5]. The introduction of the thickness modulation of YbCoIn5 block layers breaks the inversion symmetry centered at the superconducting block of CeCoIn[5]. This configuration leads to dramatic changes in the temperature and angular dependence of the upper critical field, which can be understood by considering the effect of the Rashba spin-orbit interaction arising from the inversion symmetry breaking and the associated weakening of the Pauli pair-breaking effect. Since the degree of thickness modulation is a design feature of this type of superlattices, the Rashba interaction and the nature of pair breaking are largely tunable in these modulated superlattices with strong spin-orbit couplingen
dc.format.mimetypeapplication/pdf-
dc.language.isoeng-
dc.publisherAmerican Physical Societyen
dc.rights© 2014 American Physical Societyen
dc.titleControllable Rashba Spin-Orbit Interaction in Artificially Engineered Superlattices Involving the Heavy-Fermion Superconductor CeCoIn[5]en
dc.typejournal article-
dc.type.niitypeJournal Article-
dc.identifier.ncidAA00773679-
dc.identifier.jtitlePhysical Review Lettersen
dc.identifier.volume112-
dc.identifier.issue15-
dc.relation.doi10.1103/PhysRevLett.112.156404-
dc.textversionpublisher-
dc.identifier.artnum156404-
dc.identifier.pmid24785062-
dcterms.accessRightsopen access-
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