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dc.contributor.authorSimensen, Haakon Thømt
dc.contributor.authorJohnsen, Lina G.
dc.contributor.authorLinder, Jacob
dc.contributor.authorBrataas, Arne
dc.date.accessioned2022-03-02T09:47:21Z
dc.date.available2022-03-02T09:47:21Z
dc.date.created2021-01-22T17:13:44Z
dc.date.issued2021
dc.identifier.citationPhysical review B (PRB). 2021, 103 (2), .en_US
dc.identifier.issn2469-9950
dc.identifier.urihttps://hdl.handle.net/11250/2982361
dc.description.abstractDynamical magnets can pump spin currents into superconductors. To understand such a phenomenon, we develop a method utilizing the generalized Usadel equation to describe time-dependent situations in superconductors in contact with dynamical ferromagnets. Our proof-of-concept theory is valid when there is sufficient dephasing at finite temperatures, and when the ferromagnetic insulators are weakly polarized. We derive the effective equation of motion for the Keldysh Green's function focusing on a thin film superconductor sandwiched between two noncollinear ferromagnetic insulators, one of which is dynamical. In turn, we compute the spin currents in the system as a function of the temperature and the magnetizations' relative orientations. When the induced Zeeman splitting is weak, we find that the spin accumulation in the superconducting state is smaller than in the normal states due to the lack of quasiparticle states inside the gap. This feature gives a lower backflow spin current from the superconductor as compared to a normal metal. Furthermore, in superconductors, we find that the ratio between the backflow spin current in the parallel and antiparallel magnetization configuration depends strongly on temperature, in contrast to the constant ratio in normal metals.en_US
dc.language.isoengen_US
dc.publisherAmerican Physical Societyen_US
dc.titleSpin pumping between noncollinear ferromagnetic insulators through thin superconductorsen_US
dc.typePeer revieweden_US
dc.typeJournal articleen_US
dc.description.versionpublishedVersionen_US
dc.rights.holder© 2021 American Physical Societyen_US
dc.source.pagenumber12en_US
dc.source.volume103en_US
dc.source.journalPhysical review B (PRB)en_US
dc.source.issue2en_US
dc.identifier.doi10.1103/PhysRevB.103.024524
dc.identifier.cristin1877458
dc.relation.projectNorges forskningsråd: 262633en_US
cristin.ispublishedtrue
cristin.fulltextpostprint
cristin.qualitycode2


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