Pressure-Induced Stabilization and Insulator-Superconductor Transition of BH

被引:84
作者
Hu, Chao-Hao [1 ,2 ]
Oganov, Artem R. [2 ,3 ]
Zhu, Qiang [2 ]
Qian, Guang-Rui [2 ]
Frapper, Gilles [4 ]
Lyakhov, Andriy O. [2 ]
Zhou, Huai-Ying [1 ]
机构
[1] Guilin Univ Elect Technol, Sch Mat Sci & Engn, Guilin 541004, Peoples R China
[2] SUNY Stony Brook, Dept Phys & Astron, Dept Geosci, Stony Brook, NY 11794 USA
[3] Moscow MV Lomonosov State Univ, Dept Geol, Moscow 119992, Russia
[4] Univ Poitiers, CNRS, IC2MP UMR 7285, F-86022 Poitiers, France
基金
中国国家自然科学基金;
关键词
CRYSTAL-STRUCTURE PREDICTION; TEMPERATURE;
D O I
10.1103/PhysRevLett.110.165504
中图分类号
O4 [物理学];
学科分类号
0702 ;
摘要
Diborane (B2H6), a high energy density material, was believed to be stable in a wide P, T interval. A systematic investigation of the B-H system using the ab initio variable-composition evolutionary simulations shows that boron monohydride (BH) is thermodynamically stable and can coexist with solid B, H-2, and B2H6 in a wide pressure range above 50 GPa. B2H6 becomes unstable and decomposes into the Ibam phase of BH and H-2 (C2/c) at 153 GPa. The semiconducting layered Ibam structure of BH at 168 GPa transforms into a metallic phase with space group P6/mmm and a 3D topology with strong B-B and B-H covalent bonds. The Ibam-P6/mmm transformation pathway suggests the possibility of obtaining the metastable Pbcm phase on cold decompression of the P6/mmm phase. The electron-phonon coupling calculations indicate that P6/mmm-BH is a phonon-mediated superconductor with a critical temperature of superconductivity (T-c) of 14.1-21.4 K at 175 GPa. DOI: 10.1103/PhysRevLett.110.165504
引用
收藏
页数:5
相关论文
共 30 条
  • [1] Crystalline diborane at high pressures
    Abe, Kazutaka
    Ashcroft, N. W.
    [J]. PHYSICAL REVIEW B, 2011, 84 (10)
  • [2] TRANSITION-TEMPERATURE OF STRONG-COUPLED SUPERCONDUCTORS REANALYZED
    ALLEN, PB
    DYNES, RC
    [J]. PHYSICAL REVIEW B, 1975, 12 (03): : 905 - 922
  • [3] Hydrogen dominant metallic alloys: High temperature superconductors?
    Ashcroft, NW
    [J]. PHYSICAL REVIEW LETTERS, 2004, 92 (18) : 187002 - 1
  • [4] PROJECTOR AUGMENTED-WAVE METHOD
    BLOCHL, PE
    [J]. PHYSICAL REVIEW B, 1994, 50 (24): : 17953 - 17979
  • [5] Pressure-induced metallization of silane
    Chen, Xiao-Jia
    Struzhkin, Viktor V.
    Song, Yang
    Goncharov, Alexander F.
    Ahart, Muhtar
    Liu, Zhenxian
    Mao, Ho-kwang
    Hemley, Russell J.
    [J]. PROCEEDINGS OF THE NATIONAL ACADEMY OF SCIENCES OF THE UNITED STATES OF AMERICA, 2008, 105 (01) : 20 - 23
  • [6] Superconductivity in hydrogen dominant materials: Silane
    Eremets, M. I.
    Trojan, I. A.
    Medvedev, S. A.
    Tse, J. S.
    Yao, Y.
    [J]. SCIENCE, 2008, 319 (5869) : 1506 - 1509
  • [7] Structures and potential superconductivity in SiH4 at high pressure:: En route to "metallic hydrogen" -: art. no. 017006
    Feng, J
    Grochala, W
    Jaron, T
    Hoffmann, R
    Bergara, A
    Ashcroft, NW
    [J]. PHYSICAL REVIEW LETTERS, 2006, 96 (01)
  • [8] QUANTUM ESPRESSO: a modular and open-source software project for quantum simulations of materials
    Giannozzi, Paolo
    Baroni, Stefano
    Bonini, Nicola
    Calandra, Matteo
    Car, Roberto
    Cavazzoni, Carlo
    Ceresoli, Davide
    Chiarotti, Guido L.
    Cococcioni, Matteo
    Dabo, Ismaila
    Dal Corso, Andrea
    de Gironcoli, Stefano
    Fabris, Stefano
    Fratesi, Guido
    Gebauer, Ralph
    Gerstmann, Uwe
    Gougoussis, Christos
    Kokalj, Anton
    Lazzeri, Michele
    Martin-Samos, Layla
    Marzari, Nicola
    Mauri, Francesco
    Mazzarello, Riccardo
    Paolini, Stefano
    Pasquarello, Alfredo
    Paulatto, Lorenzo
    Sbraccia, Carlo
    Scandolo, Sandro
    Sclauzero, Gabriele
    Seitsonen, Ari P.
    Smogunov, Alexander
    Umari, Paolo
    Wentzcovitch, Renata M.
    [J]. JOURNAL OF PHYSICS-CONDENSED MATTER, 2009, 21 (39)
  • [9] The revealing role of pressure in the condensed matter sciences
    Hemley, RJ
    Ashcroft, NW
    [J]. PHYSICS TODAY, 1998, 51 (08) : 26 - 32
  • [10] Kortus J, 2001, PHYS REV LETT, V86, P4656, DOI 10.1103/PhysRevLett.86.4656