• Citation: P. Olsson, J. Wallenius, C. Domain, K. Nordlund, and L. Malerba (2005), "Two-band modeling of α-prime phase formation in Fe-Cr", Physical Review B, 72(21), 214119. DOI: 10.1103/physrevb.72.214119.
    Abstract: We have developed a two-band model of Fe-Cr, fitted to properties of the ferromagnetic alloy. Fitting many-body functionals to the calculated mixing enthalpy of the alloy and the mixed interstitial binding energy in iron, our potential reproduces changes in sign of the formation energy as a function of Cr concentration. When applied in kinetic Monte Carlo simulations, the potential correctly predicts decomposition of initially random Fe-Cr alloys into the α-prime phase as function of Cr concentration.
    Citation: P. Olsson, J. Wallenius, C. Domain, K. Nordlund, and L. Malerba (2006), "Erratum: Two-band modeling of α-prime phase formation in Fe-Cr [Phys. Rev. B 72, 214119 (2005)]", Physical Review B, 74(22), 229906. DOI: 10.1103/physrevb.74.229906.

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  • Citation: J. Wallenius, P. Olsson, and C. Lagerstedt (2005), "Relation between thermal expansion and interstitial formation energy in pure Fe and Cr", Nuclear Instruments and Methods in Physics Research Section B: Beam Interactions with Materials and Atoms, 228(1-4), 122-125. DOI: 10.1016/j.nimb.2004.10.032.
    Abstract: By fitting a potential of modified Finnis–Sinclair type to the thermal expansion of ferromagnetic Fe and paramagnetic Cr, stability of the <110> self-interstitial atom is obtained. The resulting potentials are relatively hard, yielding high SIA formation energies. Less hard potentials give lower interstitial formation energy, but predict too small thermal expansion. We also show that the formation energy of the <111> SIA depends on distances in-between the 2nd and 3rd neighbour. By raising the value of the pair potential in this region, the energy difference with respect to the <110> configuration calculated with VASP in the PAW approximation can be reproduced.

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Date Created: October 5, 2010 | Last updated: March 05, 2025