Electronic and bonding analysis of hardness in pyrite-type transition-metal pernitrides

Z. T. Y. Liu, D. Gall, and S. V. Khare
Phys. Rev. B 90, 134102 – Published 8 October 2014
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Abstract

Most commonly known hard transition-metal nitrides crystallize in rocksalt structure (B1). The discovery of ultraincompressible pyrite-type PtN2 10 years ago has raised a question about the cause of its exceptional mechanical properties. We answer this question by a systematic computational analysis of the pyrite-type PtN2 and other transition-metal pernitrides (MN2) with density functional theory. Apart from PtN2, the three hardest phases are found among them in the 3d transition-metal period. They are MnN2, CoN2, and NiN2, with computed Vickers hardness (HV) values of 19.9 GPa, 16.5 GPa, and 15.7 GPa, respectively. Harder than all of these is PtN2, with a HV of 23.5 GPa. We found the following trends and correlations that explain the origin of hardness in these pernitrides. (a) Charge transfer from M to N controls the length of the N-N bond, resulting in a correlation with bulk modulus, dominantly by providing Coulomb repulsion between the pairing N atoms. (b) Elastic constant C44, an indicator of mechanical stability and hardness is correlated with total density of states at E, an indicator of metallicity. (c) Often cited monotonic variation of HV and Pugh's ratio with valence electron concentration found in rocksalt-type early transition-metal nitrides is not evident in this structure. (d) The change in MM bond strength under a shearing strain indicated by crystal orbital Hamilton population is predictive of hardness. This is a direct connection between a specific bond and shear related mechanical properties. This panoptic view involving ionicity, metallicity, and covalency is essential to obtain a clear microscopic understanding of hardness.

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  • Received 23 June 2014
  • Revised 25 August 2014

DOI:https://doi.org/10.1103/PhysRevB.90.134102

©2014 American Physical Society

Authors & Affiliations

Z. T. Y. Liu1, D. Gall2, and S. V. Khare1,*

  • 1Department of Physics and Astronomy, The University of Toledo, 2801 West Bancroft Street, Toledo, Ohio 43606, USA
  • 2Department of Materials Science and Engineering, Rensselaer Polytechnic Institute, 110 8th Street, Troy, New York 12180, USA

  • *sanjay.khare@utoledo.edu

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Issue

Vol. 90, Iss. 13 — 1 October 2014

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