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Published December 7, 2015 | Published
Journal Article Open

Temperature-dependent elastic properties of Ti_(1−x)Al_xN alloys

Abstract

Ti_(1−x)Al_xN is a technologically important alloy that undergoes a process of high temperature age-hardening that is strongly influenced by its elastic properties. We have performed first principles calculations of the elastic constants and anisotropy using the symmetry imposed force constant temperature dependent effective potential method, which include lattice vibrations and therefore the effects of temperature, including thermal expansion and intrinsic anharmonicity. These are compared with in situ high temperature x-ray diffraction measurements of the lattice parameter. We show that anharmonic effects are crucial to the recovery of finite temperature elasticity. The effects of thermal expansion and intrinsic anharmonicity on the elastic constants are of the same order, and cannot be considered separately. Furthermore, the effect of thermal expansion on elastic constants is such that the volume change induced by zero point motion has a significant effect. For TiAlN, the elastic constants soften non-uniformly with temperature: C_(11) decreases substantially when the temperature increases for all compositions, resulting in an increased anisotropy. These findings suggest that an increased Al content and annealing at higher temperatures will result in a harder alloy.

Additional Information

© 2015 AIP Publishing LLC. (Received 26 September 2015; accepted 19 November 2015; published online 8 December 2015) Support from the Swedish Research Council (VR programs 621-2011-4426, 621-2012-4401, and 637-2013-7296), Swedish Foundation for Strategic Research (SSF programs RMA08-0069 (MultiFilms) and SRL10-0026), and VINNOVA (M-Era.net project 2013-02355(MC2)) is acknowledged. N.S. acknowledges support from the Erasmus Mundus Joint European Doctoral Program DocMASE. I.A.A. acknowledges the support from the Grant of Ministry of Education and Science of the Russian Federation (Grant No. 14.Y26.31.0005) and Tomsk State University Academic D. I. Mendeleev Fund Program. All calculations were performed using the supercomputer resources of the Swedish National Infrastructure for Computing (SNIC), PDC and NSC centers. The use of Petra III was supported by a Rontgen-Angstrom Cluster frame grant (VR 2011-6505).

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