Published April 30, 2024 | Version v1
Journal article

Ab initio investigation of phonon-mediated superconductivity in the ternary borides Mo5XB2 (X=P, Si, Ge): Comparison with W5SiB2

  • 1. Sakarya Üniversitesi, Fen Fakültesi, Fizik Bölümü, 54050 Sakarya, Turkey
  • 2. Department of Physics and Astronomy, University of Exeter, Stocker Road, Exeter EX4 4QL, United Kingdom

Description

In this work, we have investigated the elastic and mechanical properties, electronic band structure, lattice dynamics, and electron-phonon interaction in four ternary transition metal borides Mo5PB2, Mo5SiB2, W5SiB2, and Mo5GeB2 by executing systematic ab initio calculations based on density functional theory within the generalized gradient approximation. The calculated elastic constants and elastic moduli for Mo5SiB2 agree well with available experimental data. The calculated elastic constants and phonon dispersion relations show that all the considered borides are mechanically and dynamically stable. The electronic density of states near the Fermi level of these compounds is dominated by the transition metal d orbitals, which leads to low-frequency phonon modes arising from the vibrations of transition metal atoms being more strongly involved in the process of scattering of electrons rather than high-frequency phonon modes arising from the vibrations of lighter other two atoms. Our electron-phonon interaction calculations reveal that the electron-phonon coupling strength of Mo5PB2 is the strongest with a value of 0.959 among all the studied compounds, which in turn yields a superconducting transition temperature (Tc) value of 9.527 K, being higher than the Tc values of Mo5SiB2 (5.845 K), W5SiB2 (5.931 K), and Mo5GeB2 (6.193 K). All these Tc values harmonize with their respective experimental values of 9.2, 5.8, 5.8, and 5.8 K, indicating the reliability of our ab initio calculations.

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Identifiers

Publishing Information

Journal Title
Physical Review B
Journal Volume
109
Journal Issue
14
Journal Page Range
16 pgs.
ISSN
1550-235X

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Copyright
©2024 American Physical Society
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