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Goldstone-like phonon modes in a (111)-strained perovskite

dc.contributor.authorMarthinsen, Astrid
dc.contributor.authorGriffin, Sinead M
dc.contributor.authorMoreau, Magnus
dc.contributor.authorGrande, Tor
dc.contributor.authorTybell, Per Thomas Martin
dc.contributor.authorSelbach, Sverre Magnus
dc.date.accessioned2019-03-01T09:24:42Z
dc.date.available2019-03-01T09:24:42Z
dc.date.created2018-08-27T22:04:56Z
dc.date.issued2018
dc.identifier.issn2475-9953
dc.identifier.urihttp://hdl.handle.net/11250/2588201
dc.description.abstractGoldstone modes are massless particles resulting from spontaneous symmetry breaking. Although such modes are found in elementary particle physics as well as in condensed-matter systems like superfluid helium, superconductors, and magnons, structural Goldstone modes are rare. Epitaxial strain in thin films can induce structures and properties not accessible in bulk and has been intensively studied for (001)-oriented perovskite oxides. Here we predict Goldstone-like phonon modes in (111)-strainednb_NO
dc.language.isoengnb_NO
dc.publisherAmerican Physical Societynb_NO
dc.titleGoldstone-like phonon modes in a (111)-strained perovskitenb_NO
dc.typeJournal articlenb_NO
dc.typePeer reviewednb_NO
dc.description.versionpublishedVersionnb_NO
dc.source.volume2nb_NO
dc.source.journalPHYSICAL REVIEW MATERIALSnb_NO
dc.source.issue1nb_NO
dc.identifier.doi10.1103/PhysRevMaterials.2.014404
dc.identifier.cristin1604790
dc.relation.projectNorges forskningsråd: 231430nb_NO
dc.relation.projectNorges forskningsråd: 231290nb_NO
dc.relation.projectNotur/NorStore: NN9301Knb_NO
dc.relation.projectNotur/NorStore: NN9264Knb_NO
dc.description.localcode© 2018 American Physical Societynb_NO
cristin.unitcode194,66,35,0
cristin.unitcode194,63,35,0
cristin.unitnameInstitutt for materialteknologi
cristin.unitnameInstitutt for elektroniske systemer
cristin.ispublishedtrue
cristin.fulltextpostprint
cristin.qualitycode1


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