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首页> 外文期刊>Physical review. B, Condensed Matter And Materals Physics >Evolution of multigap superconductivity in the atomically thin limit: Strain-enhanced three-gap superconductivity in monolayer MgB_2
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Evolution of multigap superconductivity in the atomically thin limit: Strain-enhanced three-gap superconductivity in monolayer MgB_2

机译:原子薄极限内多能隙超导的演化:单层MgB_2中应变增强的三能隙超导

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摘要

Starting from first principles, we show the formation and evolution of superconducting gaps in MgB_2 at its ultrathin limit. Atomically thin MgB_2 is distinctly different from bulk MgB_2 in that surface states become comparable in electronic density to the bulklike σ and π bands. Combining the ab initio electron-phonon coupling with the anisotropic Eliashberg equations, we show that monolayer MgB_2 develops three distinct superconducting gaps, on completely separate parts of the Fermi surface due to the emergent surface contribution. These gaps hybridize nontrivially with every extra monolayer added to the film owing to the opening of additional coupling channels. Furthermore, we reveal that the three-gap superconductivity in monolayer MgB_2 is robust over the entire temperature range that stretches up to a considerably high critical temperature of 20 K. The latter can be boosted to >50 K under biaxial tensile strain of ~4%, which is an enhancement that is stronger than in any other graphene-related superconductor known to date.
机译:从第一个原理开始,我们显示了MgB_2超薄间隙中超导间隙的形成和演化。原子上薄的MgB_2与块状MgB_2的明显不同之处在于,表面态的电子密度与块状σ和π带相当。结合从头算电子声子耦合与各向异性Eliashberg方程,我们表明,由于出现了表面贡献,单层MgB_2在费米表面的完全分离的部分上形成了三个不同的超导间隙。由于打开了额外的耦合通道,这些间隙与添加到薄膜上的每一个额外的单层非平凡地杂交。此外,我们揭示了单层MgB_2中的三能隙超导性在整个温度范围内均很稳定,该温度范围一直延伸到相当高的临界温度20K。在〜4%的双轴拉伸应变下,后者可以提高到> 50 K ,这是一种增强效果,比迄今为止已知的任何其他石墨烯相关超导体都要强。

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  • 来源
    《Physical review. B, Condensed Matter And Materals Physics》 |2017年第9期|094510.1-094510.7|共7页
  • 作者单位

    Department of Physics, University of Antwerp, Groenenborgerlaan 171, B-2020 Antwerp, Belgium;

    Department of Physics and Astronomy, Uppsala University, Box 516, SE-751 20 Uppsala, Sweden;

    Department of Physics, University of Antwerp, Groenenborgerlaan 171, B-2020 Antwerp, Belgium;

    Department of Physics and Astronomy, Uppsala University, Box 516, SE-751 20 Uppsala, Sweden;

    Department of Physics, University of Antwerp, Groenenborgerlaan 171, B-2020 Antwerp, Belgium;

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