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High-pressure vibrational properties of dense rubidium

机译:致密id的高压振动特性

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摘要

At ambient conditions, alkali metals adopt the body centered cubic structure, while if compressed up to tens of GPa and above, they exhibit complex low-symmetry modifications, due to the density-driven transition of the valence electrons from the s state to states of higher angular momentum. These high-pressure, low-symmetry phases, whose unit cells may include up to tens of atoms, allow rich Raman activity, which was previously observed only in lighter alkalis Na and Li. Here we report an extensive study of the optical phonons of highly dense Rb up to 100 GPa in diamond anvil cells, conducted by challenging experimental Raman spectroscopy measurements and ab initio computer simulations. The relative (relative to the normal condition value) density behavior of Raman frequencies of Rb is compared to that of Na and Li, once the frequencies of the two light alkali elements have been rescaled by (M_(Na)/M_(Rb))~(1/2) and (M_(Li)/M_(Rb))~(1/2), respectively, where M_(Na), M_(Li), and N_(Rb) are the atomic masses of the here considered alkali elements. Importantly, while the rescaled density behaviors of Na and Li agree with each other, Rb significantly differs, which highlights the different nature of the valence electron transition being of the s-d and of the s-p type in heavy and light alkali metals, respectively, a result that calls for further similar investigations of K and Cs.
机译:在环境条件下,碱金属采用体心立方结构,而如果压缩​​到数十GPa或更高,由于价电子从s态到C态的密度驱动跃迁,它们表现出复杂的低对称性修饰。更高的角动量。这些高压,低对称相的晶胞最多可包含数十个原子,它们具有很强的拉曼活性,以前仅在较轻的碱金属Na和Li中才能观察到。在这里,我们报告了具有挑战性的拉曼光谱实验测量和从头算计算机模拟,对金刚石砧座细胞中高达100 GPa的高密度Rb的光学声子进行了广泛的研究。一旦两个轻碱元素的频率被重新标定了(M_(Na)/ M_(Rb)),就将Rb的拉曼频率的相对(相对于正常条件值)密度行为与Na和Li的相对密度行为进行比较。 〜(1/2)和(M_(Li)/ M_(Rb))〜(1/2),其中M_(Na),M_(Li)和N_(Rb)是此处的原子质量被认为是碱性元素。重要的是,尽管Na和Li的重标密度行为彼此吻合,但Rb明显不同,这突显了重碱金属和轻碱金属中sd和sp型的价电子跃迁分别具有不同的性质,结果这就要求对K和C进行进一步的类似研究。

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  • 来源
    《Physical review. B, Condensed Matter And Materals Physics》 |2018年第10期|104107.1-104107.7|共7页
  • 作者单位

    National Institute of Optics, INO-CNR, and LENS, via N. Carrara 1, I-50019 Sesto Fiorentino, Italy;

    Institute of Applied Physics, IFAC-CNR, via Madonna del Piano 10, I-50019 Sesto Fiorentino, Italy;

    TCM Group, Cavendish Laboratory, University of Cambridge, J. J. Thomson Avenue, Cambridge CB3 0HE, United Kingdom;

    Centre for Science at Extreme Conditions and School of Physics and Astronomy, University of Edinburgh, Edinburgh EH9 3JZ, United Kingdom;

    Institute of Applied Physics, IFAC-CNR, via Madonna del Piano 10, I-50019 Sesto Fiorentino, Italy;

    National Institute of Optics, INO-CNR, and LENS, via N. Carrara 1, I-50019 Sesto Fiorentino, Italy;

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