Non-empirical phase equilibria in the Cr–Mo system: A combination of first-principles calculations, cluster expansion and Monte Carlo simulations

Abstract

In this work, the low temperature part of the Cr–Mo phase diagram is calculated by a combination of first-principles calculations, cluster expansion, and Monte Carlo simulations without the use of empirical parameters. In brief, the miscibility gap in the bcc phase is computed through lattice Monte Carlo simulations with the energetics of the Cr–Mo system represented by cluster expansion Hamiltonians, wherein the Hamiltonians are firstly constructed using first-principles calculations of formation energies for supercells of various bulk compositions. It is demonstrated that the onset (critical) temperature of the miscibility gap is preliminarily computed to be Tc = 1720 K, and is significantly decreased to 1150 K once excess vibrational contribution to the free energy is considered. The resulting solid-state miscibility gap of the Cr–Mo binary system, largely improved by the contributions of atomic relaxation and positive excess volume of mixing in the Cr–Mo bcc alloys, also favors the approaches that extrapolate the Gibbs energy of the bcc phase retrieved at high temperatures, as in the CALPHAD method.