The role of N defects in paramagnetic CrN at finite temperatures from first-principles
Elham Mozafari, Bj\"orn Alling, Peter Steneteg, and Igor A. Abrikosov

TL;DR
This study uses first-principles simulations to analyze nitrogen defects in paramagnetic CrN at high temperatures, revealing defect energetics, electronic structure impacts, and temperature effects on the band gap.
Contribution
It provides the first detailed first-principles analysis of nitrogen vacancies and interstitials in CrN at elevated temperatures, considering magnetic disorder and lattice vibrations.
Findings
Vacancy formation energy is 2.28 eV with minimal temperature effect.
Nitrogen interstitial formation energy is about 3.77 eV, increasing slightly at high temperature.
At 900 K, CrN shows a non-zero density of states at the Fermi level, indicating possible metallic behavior.
Abstract
Simulations of defects in paramagnetic materials at high temperature constitute a formidable challenge to solid state theory due to the interaction of magnetic disorder, vibrations, and structural relaxations. CrN is a material where these effects are particularly large due to a strong magneto-lattice coupling and a tendency for deviations from the nominal 1:1 stoichiometry. In this work we present a first-principles study of nitrogen vacancies and nitrogen interstitals in CrN at elevated temperature. We report on formation energetics, the geometry of interstital nitrogen dimers, and impact on the electronic structure caused by the defects. We find a vacancy formation energy of 2.28 eV with a small effect of temperature, a formation energy for N interstitial in the form of a oriented split-bond of 3.77 eV with an increase to 3.97 at 1000 K. Vacancies are found to add…
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