Structure and energy of point defects in TiC: An ab initio study

Weiwei Sun, Hossein Ehteshami, and Pavel A. Korzhavyi
Phys. Rev. B 91, 134111 – Published 24 April 2015
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Abstract

We employ first-principles calculations to study the atomic and electronic structure of various point defects such as vacancies, interstitials, and antisites in the stoichiometric as well as slightly off-stoichiometric Ti1cCc (including both C-poor and C-rich compositions, 0.49c0.51). The atomic structure analysis has revealed that both interstitial and antisite defects can exist in split conformations involving dumbbells. To characterize the electronic structure changes caused by a defect, we introduce differential density of states (dDOS) defined as a local perturbation of the density of states (DOS) on the defect site and its surrounding relative to the perfect TiC. This definition allows us to identify the DOS peaks characteristic of the studied defects in several conformations. So far, characteristic defect states have been discussed only in connection with carbon vacancies. Here, in particular, we have identified dDOS peaks of carbon interstitials and dumbbells, which can be used for experimental detection of such defects in TiC. The formation energies of point defects in TiC are derived in the framework of a grand-canonical formalism. Among the considered defects, carbon vacancies and interstitials are shown to have, respectively, the lowest and the second-lowest formation energies. Their formation energetics are consistent with the thermodynamic data on the phase stability of nonstoichiometric TiC. A cluster type of point defect is found to be next in energy, a titanium [100] dumbbell terminated by two carbon vacancies.

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  • Received 12 December 2014
  • Revised 2 April 2015

DOI:https://doi.org/10.1103/PhysRevB.91.134111

©2015 American Physical Society

Authors & Affiliations

Weiwei Sun1,2,*, Hossein Ehteshami1, and Pavel A. Korzhavyi1,3

  • 1Department of Material Science and Engineering, KTH-Royal Institute of Technology, SE-100 44 Stockholm, Sweden
  • 2Department of Physics and Astronomy, Uppsala University, Box 516, SE-751 20 Uppsala, Sweden
  • 3Institute of Metal Physics, Ural Division of the Russian Academy of Sciences, 620219 Ekaterinburg, Russia

  • *Corresponding author: provels8467@gmail.com

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Issue

Vol. 91, Iss. 13 — 1 April 2015

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