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dc.contributor.authorAdo, I. A.
dc.contributor.authorQaiumzadeh, Alireza
dc.contributor.authorBrataas, Arne
dc.contributor.authorTitov, M.
dc.date.accessioned2020-04-20T07:26:14Z
dc.date.available2020-04-20T07:26:14Z
dc.date.created2020-04-16T10:39:33Z
dc.date.issued2020
dc.identifier.citationPhysical review B (PRB). 2020, 101 161403-?.en_US
dc.identifier.issn2469-9950
dc.identifier.urihttps://hdl.handle.net/11250/2651602
dc.description.abstractWe consider a contribution w ch to the micromagnetic energy density that is linear with respect to the first spatial derivatives of the local magnetization direction. For a generalized two-dimensional Rashba ferromagnet, we present a microscopic analysis of this contribution and, in particular, demonstrate that it cannot be expressed through Lifshitz invariants beyond the linear order in the spin-orbit coupling (SOC) strength. Terms in wch beyond Lifshitz invariants emerge as a result of spin rotation symmetry breaking caused by SOC. The effects of these terms on the phase diagram of magnetic states and spin-wave dispersion are discussed. Finally, we present a classification of terms in w ch, allowed by symmetry, for each crystallographic point group.en_US
dc.language.isoengen_US
dc.publisherAmerican Physical Societyen_US
dc.titleChiral ferromagnetism beyond Lifshitz invariantsen_US
dc.typePeer revieweden_US
dc.typeJournal articleen_US
dc.description.versionpublishedVersionen_US
dc.source.pagenumber161403-?en_US
dc.source.volume101en_US
dc.source.journalPhysical review B (PRB)en_US
dc.identifier.doi10.1103/PhysRevB.101.161403
dc.identifier.cristin1806557
dc.relation.projectEC/H2020/669442en_US
dc.relation.projectNorges forskningsråd: 262633en_US
dc.description.localcode© 2020 American Physical Societyen_US
cristin.ispublishedtrue
cristin.fulltextoriginal
cristin.qualitycode2


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