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dc.contributor.authorJohnsen, Lina G.
dc.contributor.authorLinder, Jacob
dc.date.accessioned2022-03-04T09:36:28Z
dc.date.available2022-03-04T09:36:28Z
dc.date.created2021-10-29T16:12:34Z
dc.date.issued2021
dc.identifier.citationPhysical review B (PRB). 2021, 104 (14), .en_US
dc.identifier.issn2469-9950
dc.identifier.urihttps://hdl.handle.net/11250/2983040
dc.description.abstractThe spin transport inside an odd-frequency spin-triplet superconductor differs from that of a conventional superconductor due to its distinct symmetry properties. We study spin transport inside an emergent odd-frequency superconductor by replacing the spin-singlet gap matrix in the Usadel equation with a matrix representing spin-triplet pairing that is odd under inversion of energy. We show that the peculiar nature of the density of states allows for an even larger spin injection than in the normal state. Moreover, when the odd-frequency pairing inherits its temperature dependence from a conventional superconductor through the proximity effect, the density of states can transition from gapless to gapped as the temperature decreases. At the transition point, the spin accumulation inside the odd-frequency superconductor is peaked and larger than in the normal state. While the spin-flip scattering time is known to decrease below the superconducting transition temperature in conventional superconductors, we find that the same is true for the spin-orbit scattering time in odd-frequency superconductors. This renormalization is particularly large for energies close to the gap edge, if such a gap is present.en_US
dc.language.isoengen_US
dc.publisherAmerican Physical Societyen_US
dc.titleSpin injection and spin relaxation in odd-frequency superconductorsen_US
dc.typePeer revieweden_US
dc.typeJournal articleen_US
dc.description.versionpublishedVersionen_US
dc.rights.holder©2021 American Physical Societyen_US
dc.source.pagenumber10en_US
dc.source.volume104en_US
dc.source.journalPhysical review B (PRB)en_US
dc.source.issue14en_US
dc.identifier.doi10.1103/PhysRevB.104.144513
dc.identifier.cristin1949753
dc.relation.projectNorges forskningsråd: QuSpinen_US
dc.relation.projectNorges forskningsråd: 262633en_US
cristin.ispublishedtrue
cristin.fulltextpostprint
cristin.qualitycode2


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