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Magnetic hour-glass dispersion and its relation to high-temperature superconductivity in iron-tuned Fe$_{1+y}$Te$_{0.7}$Se$_{0.3}$

机译:磁性沙漏分散及其与高温的关系   铁调的超导性Fe $ _ {1 + y} $ Te $ _ {0.7} $ se $ _ {0.3} $

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摘要

High-temperature superconductivity remains arguably the largest outstandingenigma of condensed matter physics. The discovery of iron-basedhigh-temperature superconductors has renewed the importance of understandingsuperconductivity in materials susceptible to magnetic order and fluctuations.Intriguingly they show magnetic fluctuations reminiscent of the superconducting(SC) cuprates, including a 'resonance' and an 'hour-glass' shaped dispersion,which provide an opportunity to new insight to the coupling between spinfluctuations and superconductivity. Here we report inelastic neutron scatteringdata on Fe$_{1+y}$Te$_{0.7}$Se$_{0.3}$ using excess iron concentration to tunebetween a SC ($y=0.02$) and a non-SC ($y=0.05$) ground states. We findincommensurate spectra in both samples but discover that in the one thatbecomes SC, a constriction towards a commensurate hourglass shape develop wellabove $T_c$. Conversely a spin-gap and concomitant spectral weight shift happenbelow $T_c$. Our results imply that the hourglass shaped dispersion is mostlikely a pre-requisite for superconductivity, whereas the spin-gap and shift ofspectral weight are consequences of superconductivity. We explain thisobservation by pointing out that an inwards dispersion towards the commensuratewave-vector is needed for the opening of a spin gap to lower the magneticexchange energy and hence provide the necessary condensation energy for the SCstate to emerge.
机译:高温超导可以说仍然是凝聚态物理最大的谜。铁基高温超导体的发现更新了理解易受磁序和波动影响的材料中超导性的重要性,有趣的是它们表现出的磁波动让人联想到超导(SC)铜酸盐,包括``共振''和``沙漏''。形状的分散体,这为新认识自旋涨落和超导之间的耦合提供了机会。在这里,我们报告了Fe $ _ {{1 + y} $ Te $ _ {0.7} $ Se $ _ {0.3} $上的非弹性中子散射数据,其中使用了过量的铁浓度在SC($ y = 0.02 $)和非SC之间进行调整。 ($ y = 0.05 $)基本状态。我们在两个样品中发现了不相称的光谱,但发现在成为SC的一个中,向相称的沙漏形状的收缩在$ T_c $之上发展。相反,自旋间隙和伴随的频谱权重偏移发生在$ T_c $以下。我们的结果表明,沙漏形分散体最有可能是超导性的先决条件,而自旋间隙和光谱重量的移动是超导性的结果。我们通过指出为使自旋间隙打开以降低磁交换能量并因此为SCstate出现提供必要的凝结能量,需要朝着相称的波矢量向内分散来解释这种观察。

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