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高温超导铜氧化物中超导和磁关联的高磁场 μSR 研究。

High-field μSR studies of superconducting and magnetic correlations in cuprates above T(c).

机构信息

Department of Physics, Simon Fraser University, Burnaby, BC, V5A 1S6, Canada.

出版信息

J Phys Condens Matter. 2010 May 26;22(20):203202. doi: 10.1088/0953-8984/22/20/203202. Epub 2010 Apr 26.

Abstract

The advent of high transverse field muon spin rotation (TF-μSR) has led to recent μSR investigations of the magnetic field response of cuprates above the superconducting transition temperature T(c). Here the results of such experiments on hole-doped cuprates are reviewed. Although these investigations are currently ongoing, it is clear that the effects of high field on the internal magnetic field distribution of these materials is dependent upon competition between superconductivity and magnetism. In La(2 - x)Sr(x)CuO(4) the response to the external field above T(c) is dominated by heterogeneous spin magnetism. However, the magnetism that dominates the observed inhomogeneous line broadening below x ∼ 0.19 is overwhelmed by the emergence of a completely different kind of magnetism in the heavily overdoped regime. The origin of the magnetism above x ∼ 0.19 is probably related to intrinsic disorder, but the systematic evolution of the magnetism with doping changes in the doping range beyond the superconducting 'dome'. In contrast, the width of the internal field distribution of underdoped Y Ba(2)Cu(3)O(y) above T(c) is observed to track T(c) and the density of superconducting carriers. This observation suggests that the magnetic response above T(c) is not dominated by electronic moments, but rather inhomogeneous fluctuating superconductivity. The spatially inhomogeneous response of Y Ba(2)Cu(3)O(y) to the applied field may be a means of minimizing energy, rather than being caused by intrinsic disorder.

摘要

高横向磁场 μ 自旋旋转(TF-μSR)的出现导致了最近对高于超导转变温度 T(c)的铜酸盐的磁场响应的 μSR 研究。这里回顾了对空穴掺杂铜酸盐的此类实验的结果。尽管这些研究目前仍在进行中,但很明显,高场对这些材料内部磁场分布的影响取决于超导性和磁性之间的竞争。在 La(2 - x)Sr(x)CuO(4)中,高于 T(c)的对外场的响应主要由非均匀自旋磁性决定。然而,在 x ∼ 0.19 以下主导观察到的不均匀线宽的磁性被在过掺杂区域中出现的完全不同种类的磁性所压倒。在 x ∼ 0.19 以上的磁性的起源可能与内在无序有关,但在超导“穹顶”之外的掺杂范围内,磁性随掺杂的系统演化发生了变化。相比之下,在高于 T(c)的掺杂 Y Ba(2)Cu(3)O(y)中,内部磁场分布的宽度被观察到与 T(c)和超导载流子的密度相吻合。这一观察结果表明,高于 T(c)的磁响应不是由电子磁矩主导,而是由不均匀的超导波动主导。Y Ba(2)Cu(3)O(y)对外部磁场的空间非均匀响应可能是最小化能量的一种手段,而不是由内在无序引起的。

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