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超导涡旋簇在 S/F 混合体中的观察。

Observation of superconducting vortex clusters in S/F hybrids.

机构信息

"E.R. Caianiello" Physics Department, University of Salerno, Fisciano (SA), 84084, Italy.

Physics Department, Temple University, Philadelphia, PA 19122, United States.

出版信息

Sci Rep. 2016 Dec 9;6:38557. doi: 10.1038/srep38557.

Abstract

While Abrikosov vortices repel each other and form a uniform vortex lattice in bulk type-II superconductors, strong confinement potential profoundly affects their spatial distribution eventually leading to vortex cluster formation. The confinement could be induced by the geometric boundaries in mesoscopic-size superconductors or by the spatial modulation of the magnetic field in superconductor/ferromagnet (S/F) hybrids. Here we study the vortex confinement in S/F thin film heterostructures and we observe that vortex clusters appear near magnetization inhomogeneities in the ferromagnet, called bifurcations. We use magnetic force microscopy to image magnetic bifurcations and superconducting vortices, while high resolution scanning tunneling microscopy is used to obtain detailed information of the local electronic density of states outside and inside the vortex cluster. We find an intervortex spacing at the bifurcation shorter than the one predicted for the same superconductor in a uniform magnetic field equal to the thermodynamical upper critical field H. This result is due to a local enhanced stray field and a competition between vortex-vortex repulsion and Lorentz force. Our findings suggest that special magnetic topologies could result in S/F hybrids that support superconductivity even when locally the vortex density exceeds the thermodynamic critical threshold value beyond which the superconductivity is destroyed.

摘要

虽然在体相 II 型超导体中,Abrikosov 涡旋相互排斥并形成均匀的涡旋晶格,但强约束势深刻地影响了它们的空间分布,最终导致涡旋簇的形成。这种约束可以由介观尺寸超导体的几何边界或超导体/铁磁体(S/F)混合体中磁场的空间调制引起。在这里,我们研究了 S/F 薄膜异质结构中的涡旋约束,我们观察到在铁磁体中的磁各向异性附近出现涡旋簇,称为分叉。我们使用磁力显微镜来成像磁分叉和超导涡旋,同时使用高分辨率扫描隧道显微镜来获得涡旋簇内外局部电子态密度的详细信息。我们发现分叉处的涡旋间距比在相同的超导体中处于均匀磁场时预测的要短,等于热力学上的上临界场 H。这一结果是由于局部增强的杂散场以及涡旋-涡旋排斥和洛伦兹力之间的竞争。我们的发现表明,特殊的磁场拓扑结构可能导致 S/F 混合体即使在局部涡旋密度超过超导性被破坏的热力学临界阈值时也能支持超导性。

https://cdn.ncbi.nlm.nih.gov/pmc/blobs/7172/5146919/6945d5d42d12/srep38557-f1.jpg

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