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Instability of flux flow and production of vortex-antivortex pairs by current-driven Josephson vortices in layered superconductors

机译:层状超导体中电流驱动的约瑟夫森涡流的通量流动不稳定性和涡旋-反涡旋对的产生

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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:我们报告了由分层超导体中强直流电流驱动的约瑟夫森涡旋非线性动力学的数值模拟。求解了耦合的超导层堆叠中层间相差的动力学方程,以计算涡流的阻力系数eta(J)作为垂直直流电流密度J的函数。结果表明,运动涡流产生的Cherenkov辐射引起在高涡旋速度v时,显着的辐射阻力增加eta(upsilon),而驱动的约瑟夫森涡流的撞击不稳定性比终端速度upsilon(c)快。稳态通量流在nu> upsilon(c)处分解,这是因为涡旋开始产生级联的扩展涡旋-反涡旋对,这些涡旋对演变成平面大涡旋结构或分支的通量模式,这些通量模式沿层和跨层传播。由快速移动的涡流触发的这种涡流-反涡流对的产生在欠阻尼平面结的堆栈中最为明显,在平面结点中,它可能发生在J> J(s)处,远低于层间约瑟夫森临界电流密度。 upsilon(c)和J(s)均作为准粒子阻尼参数的函数进行计算,并且直流磁场平行于层施加。考虑了涡旋相互作用对约瑟夫森结环堆叠中移动的涡旋链和晶格的切伦科夫不稳定性的影响。结果表明,在有限长度的多层结构中,由电流密度J> J(s)驱动的涡流会激发自持的大振幅磁通量驻波,从而导致总磁矩的时间振动。我们评估了这种效应对样品辐射功率W的贡献,并表明W随着层数的增加而强烈增加。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平面流动的高dc电流密度下,来自分层铜酸盐的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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