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dc.date.accessioned2019-03-05T14:23:32Z
dc.date.available2019-03-05T14:23:32Z
dc.date.created2018-08-07T11:49:26Z
dc.date.issued2018
dc.identifier.citationGolovchanskiy, Igor A. Pan, A. V. Johansen, Tom Henning George, Jonathan Rudnev, Igor A. Rosenfeld, Anatoly Fedoseev, Sergey A. . Origin of magnetic flux-jumps in Nb films subject to mechanical vibrations and corresponding magnetic perturbations. Physical Review B. 2018, 97(1)
dc.identifier.urihttp://hdl.handle.net/10852/67060
dc.description.abstractIn this paper the origin of flux-jumps in Nb thin films is established during magnetization measurements using a vibrating sample magnetometer (VSM). Magnetization measurements of the flux avalanche activity show its strong dependence on frequency and amplitude of VSM vibration. In particular, under certain conditions the vibrations induce a transition from a stable superconducting critical state to an undercritical state, accompanied by the 20-fold drop in the magnetic moment. These features allow the elucidation of the origin of the flux-jumps. In contrast to the commonly assumed thermomagnetic instabilities to be responsible for the flux-jumps in Nb films, our results provide solid support for an alternative explanation being due to criticality-built instability well represented by a sandpile. Considering properties of the flux-flow during a flux avalanche regime allows us to estimate nonuniformity of a magnetic field in a VSM sample space developed as a result of vibrations.en_US
dc.languageEN
dc.titleOrigin of magnetic flux-jumps in Nb films subject to mechanical vibrations and corresponding magnetic perturbationsen_US
dc.typeJournal articleen_US
dc.creator.authorGolovchanskiy, Igor A.
dc.creator.authorPan, A. V.
dc.creator.authorJohansen, Tom Henning
dc.creator.authorGeorge, Jonathan
dc.creator.authorRudnev, Igor A.
dc.creator.authorRosenfeld, Anatoly
dc.creator.authorFedoseev, Sergey A.
cristin.unitcode185,15,4,10
cristin.unitnameKondenserte fasers fysikk
cristin.ispublishedtrue
cristin.fulltextoriginal
cristin.qualitycode2
dc.identifier.cristin1600159
dc.identifier.bibliographiccitationinfo:ofi/fmt:kev:mtx:ctx&ctx_ver=Z39.88-2004&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.jtitle=Physical Review B&rft.volume=97&rft.spage=&rft.date=2018
dc.identifier.jtitlePhysical Review B
dc.identifier.volume97
dc.identifier.issue1
dc.identifier.doihttp://dx.doi.org/10.1103/PhysRevB.97.014524
dc.identifier.urnURN:NBN:no-70244
dc.type.documentTidsskriftartikkelen_US
dc.type.peerreviewedPeer reviewed
dc.source.issn2469-9950
dc.identifier.fulltextFulltext https://www.duo.uio.no/bitstream/handle/10852/67060/1/PhysRevB.97.014524.pdf
dc.type.versionPublishedVersion


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