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Linear response results for phonons and electron-phonon coupling in hexagonal close packed Sc-spin fluctuations, and implications for superconductivity

机译:六方密堆积Sc自旋涨落中声子和电子-声子耦合的线性响应结果及其对超导性的影响

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We present a FP-LMTO (full-potential linear muffin-tin orbital) study of the variation in the electronic structure, phonon frequencies and electron-phonon coupling in hexagonal close packed (hcp) Sc under pressure. The electron-phonon coupling constant lambda is found to increase steadily with pressure in the hcp phase, until the pressure reaches a value where the hcp phase becomes unstable. Linear response calculations for the normal pressure c/a ratio predict a phase change somewhere between calculated pressures of 22 and 30 GPa. The calculated frequencies for the equilibrium hcp lattice parameters are in good agreement with the inelastic neutron scattering results. There is a small upward shift in the Gamma-point E-2g mode frequency under pressure, in qualitative agreement with the Raman spectroscopy study of Olijnyk et al (2006 J. Phys.: Condens. Matter 18 10971). From the measured value of the electronic specific heat constant and the calculated values of the Fermi level density of states and electron-phonon coupling constant, we conclude that the electron-paramagnon coupling constant in hcp Sc should be comparable to the electron-phonon coupling constant. This indicates that the spin fluctuation effects are strong enough to suppress superconductivity completely in hcp Sc. We argue that spin fluctuations should be reduced by a factor of two or more in the high pressure Sc-II phase. On the basis of estimates of the electron-paramagnon coupling constants and the calculated or estimated electron-phonon coupling constants, we argue that the hcp phase may become superconducting with a very low transition temperature immediately prior to the transition to the Sc-II phase and that the Sc-II phase should indeed be superconducting. The electronic, electron-phonon and spin fluctuation properties of hcp Sc under pressure are compared with those of the high pressure hcp phase of Fe, which was reported to be superconducting a few years back.
机译:我们提出了在压力下六方密堆积(hcp)Sc中电子结构,声子频率和电子-声子耦合变化的FP-LMTO(全势线性松饼-锡轨道)研究。发现电子-声子耦合常数λ随着hcp相中的压力稳定增加,直到压力达到hcp相变得不稳定的值。法向压力c / a比率的线性响应计算可预测在22至30 GPa的压力之间的某个相位变化。平衡hcp晶格参数的计算频率与非弹性中子散射结果非常吻合。与Olijnyk等人(2006 J. Phys .: Condens。Matter 18 10971)的拉曼光谱研究定性地一致,在压力下,伽马点E-2g模频率有一个小的向上偏移。从电子比热常数的测量值和状态的费米能级密度和电子-声子耦合常数的计算值,我们得出结论:hcp Sc中的电子-顺磁子耦合常数应与电子-声子耦合常数相当。这表明自旋起伏效应足够强大,可以完全抑制hcp Sc中的超导。我们认为,在高压Sc-II相中,自旋波动应减少两倍或更多。根据对电子-顺​​磁子耦合常数的估计以及计算或估计的电子-声子耦合常数,我们认为hcp相可能会在过渡到Sc-II相之前立即以非常低的转变温度超导。 Sc-II相确实应该是超导的。将hcp Sc在压力下的电子,电子声子和自旋涨落特性与Fe的高压hcp相进行了比较,据报道,Fe在几年前是超导的。

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