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Possible light-induced superconductivity in K3C60 at high temperature

机译:高温下K3C60中可能的光诱导超导性

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摘要

The non-equilibrium control of emergent phenomena in solids is an important research frontier, encompassing effects such as the optical enhancement of superconductivity(1). Nonlinear excitation(2,3) of certain phonons in bilayer copper oxides was recently shown to induce superconducting-like optical properties at temperatures far greater than the superconducting transition temperature, T-c (refs 4-6). This effect was accompanied by the disruption of competing charge-density-wave correlations(7,8), which explained some but not all of the experimental results. Here we report a similar phenomenon in a very different compound, K3C60. By exciting metallic K3C60 with mid-infrared optical pulses, we induce a large increase in carrier mobility, accompanied by the opening of a gap in the optical conductivity. These same signatures are observed at equilibrium when cooling metallic K3C60 below T-c (20 kelvin). Although optical techniques alone cannot unequivocally identify non-equilibrium high-temperature superconductivity, we propose this as a possible explanation of our results.
机译:固体中涌现现象的非平衡控制是一个重要的研究前沿,其中包括超导性的光学增强等效应(1)。最近发现双层氧化铜中某些声子的非线性激发(2,3)在远高于超导转变温度T-c的温度下会诱发类超导光学性质(参考文献4-6)。这种效应伴随着竞争性电荷密度波相关性的破坏(7,8),这解释了部分但并非全部实验结果。在这里,我们报道了在非常不同的化合物K3C60中的类似现象。通过用中红外光脉冲激发金属K3C60,我们诱导了载流子迁移率的大幅提高,并伴随着光导率间隙的打开。当将金属K3C60冷却到T-c(20开尔文)以下时,在平衡时观察到这些相同的特征。尽管仅凭光学技术无法明确地识别非平衡高温超导性,但我们建议将其作为对结果的可能解释。

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  • 来源
    《Nature》 |2016年第7591期|461-464|共4页
  • 作者单位

    Max Planck Inst Struct & Dynam Matter, Luruper Chaussee 149, D-22761 Hamburg, Germany;

    Max Planck Inst Struct & Dynam Matter, Luruper Chaussee 149, D-22761 Hamburg, Germany|Hamburg Ctr Ultrafast Imaging, Luruper Chaussee 149, D-22761 Hamburg, Germany;

    Max Planck Inst Struct & Dynam Matter, Luruper Chaussee 149, D-22761 Hamburg, Germany|Hamburg Ctr Ultrafast Imaging, Luruper Chaussee 149, D-22761 Hamburg, Germany;

    Max Planck Inst Struct & Dynam Matter, Luruper Chaussee 149, D-22761 Hamburg, Germany;

    INSTM UdR Trieste ST, Area Sci Pk, I-34012 Trieste, Italy|Elettra Sincrotrone Trieste SCpA, Area Sci Pk, I-34012 Trieste, Italy;

    Univ Roma La Sapienza, CNR IOM, Piazzale A Moro 2, I-00185 Rome, Italy|Univ Roma La Sapienza, Dipartimento Fis, Piazzale A Moro 2, I-00185 Rome, Italy;

    INSTM UdR Trieste ST, Area Sci Pk, I-34012 Trieste, Italy|Elettra Sincrotrone Trieste SCpA, Area Sci Pk, I-34012 Trieste, Italy;

    Univ Parma, Dipartimento Fis & Sci Terra, Parco Area Sci 7-A, I-43124 Parma, Italy;

    Univ Parma, Dipartimento Fis & Sci Terra, Parco Area Sci 7-A, I-43124 Parma, Italy;

    Max Planck Inst Struct & Dynam Matter, Luruper Chaussee 149, D-22761 Hamburg, Germany|Univ Bath, Dept Phys, Bath BA2 7AY, Avon, England|Univ Oxford, Dept Phys, Parks Rd, Oxford OX1 3PU, England;

    Univ Oxford, Dept Phys, Parks Rd, Oxford OX1 3PU, England|Natl Univ Singapore, Ctr Quantum Technol, 3 Sci Dr 2, Singapore 117543, Singapore;

    Max Planck Inst Struct & Dynam Matter, Luruper Chaussee 149, D-22761 Hamburg, Germany|Hamburg Ctr Ultrafast Imaging, Luruper Chaussee 149, D-22761 Hamburg, Germany|Univ Oxford, Dept Phys, Parks Rd, Oxford OX1 3PU, England;

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  • 入库时间 2022-08-18 02:52:04

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