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首页> 外文期刊>Physical review >Instability of flux flow and production of vortex-antivortex pairs by current-driven Josephson vortices in layered superconductors
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Instability of flux flow and production of vortex-antivortex pairs by current-driven Josephson vortices in layered superconductors

机译:在分层超导体中的电流驱动的Josephson涡流透气流量和涡旋抗触发对的稳定性

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摘要

We report numerical simulations of the nonlinear dynamics of Josephson vortices driven by strong dc currents in layered superconductors. Dynamic equations for interlayer phase differences in a stack of coupled superconducting layers were solved to calculate a drag coefficient eta(J) of the vortex as a function of the perpendicular dc current density J. It is shown that Cherenkov radiation produced by a moving vortex causes significant radiation drag increasing eta(upsilon) at high vortex velocities v and striking instabilities of driven Josephson vortices moving faster than a terminal velocity upsilon(c). The steady-state flux flow breaks down at nu upsilon(c) as the vortex starts producing a cascade of expanding vortex-antivortex pairs evolving into either planar macrovortex structures or branching flux patterns propagating both along and across the layers. This vortex-antivortex pair production triggered by a rapidly moving vortex is most pronounced in a stack of underdamped planar junctions where it can occur at J J(s) well below the interlayer Josephson critical current density. Both upsilon(c) and J(s) were calculated as functions of the quasiparticle damping parameter, and the dc magnetic field was applied parallel to the layers. The effects of vortex interaction on the Cherenkov instability of moving vortex chains and lattices in annular stacks of Josephson junctions were considered. It is shown that a vortex driven by a current density J J(s) in a multilayer of finite length excites self-sustained large-amplitude standing waves of magnetic flux, resulting in temporal oscillations of the total magnetic moment. We evaluated a contribution of this effect to the power W radiated by the sample and showed that W increases strongly as the number of layers increases. These mechanisms can result in nonlinearity of the c-axis electromagnetic response and contribute to THz radiation from the layered cuprates at high dc current densities flowing perpendicular to the ab planes.
机译:我们报告了由层超导体强直流电流驱动的Josephson涡流的非线性动力学的数值模拟。解决了耦合超导层堆叠中层间相差的动态方程,以计算涡流的拖动系数ETA(j)作为垂直Dc电流密度J的函数。显示通过移动涡流产生的Cherenkov辐射在高涡流速度V的高涡流速度V和驱动的Josephson Voltices的引人势上的显着辐射阻力增加η(Upsilon)比终端速度Upsilon(C)更快地移动。稳态磁通流量在Nu> Upsilon(C)中突破,因为涡旋开始产生扩展的vortex-antivortex对的级联,从而进化到平面宏观波动结构或沿着层次传播的支链磁通图案。通过快速移动的涡旋触发的这种涡旋 - 反象的对生产最为明显,在一堆被拒绝的平面连接堆中,它可以在J> J(s)良好下方在中间josephson临界电流密度下方发生。将upsilon(c)和j(s)作为Quasiparticle阻尼参数的功能计算,并且DC磁场平行于层施加。考虑了涡旋相互作用对Josephson结的环形堆的移动涡旋链和格子的Cherenkov不稳定性的影响。结果表明,由电流密度J> J> J> J> J> J> J> J> J> J> J> J> J> J> J> J> J> J> J> J> J> J> J> j> j> j> j> j> j> j> j> j> j> j> j>磁通自持续的大幅度驻距波的自持续的磁通量。总磁矩的时间振荡导致。我们评估了这种效果对样品辐射的功率W的贡献,并且显示随着层数增加而强烈增加。这些机制可以导致C轴电磁响应的非线性,并有助于在垂直于AB平面的高DC电流密度下从层状铜替代的THz辐射。

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  • 来源
    《Physical review》 |2019年第21期|214512.1-214512.15|共15页
  • 作者单位

    Old Dominion Univ Dept Phys Norfolk VA 23529 USA;

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