× Updated! Potentials that share interactions are now listed as related models.
 
Citation: O.R. Deluigi, R.C. Pasianot, F.J. Valencia, A. Caro, D. Farkas, and E.M. Bringa (2021), "Simulations of primary damage in a High Entropy Alloy: Probing enhanced radiation resistance", Acta Materialia, 213, 116951. DOI: 10.1016/j.actamat.2021.116951.
Abstract: High Entropy Alloys (HEA) attract attention as possible radiation resistant materials, a feature observed in some experiments that has been attributed to several unique properties of HEA, in particular to the disorder-induced reduced thermal conductivity and to the peculiar defect properties originating from the chemical complexity. To explore the origin of such behavior we study the early stages (less than 0.1 ns), of radiation damage response of a HEA using molecular dynamics simulations of collision cascades induced by primary knock-on atoms (PKA) with 10, 20 and 40 keV, at room temperature, on an idealized model equiatomic quinary fcc FeNiCrCoCu alloy, the corresponding "Average Atom" (AA) material, and on pure Ni. We include accurate corrections to describe short-range atomic interactions during the cascade. In all cases the average number of defects in the HEA is lower than for pure Ni, which has been previously used to help claiming that HEA is radiation resistant. However, simulated defect evolution during primary damage, including the number of surviving Frenkel Pairs, and the defect cluster size distributions are nearly the same in all cases, within our statistical uncertainty. The number of surviving FP in the alloy is predicted fairly well by analytical models of defect production in pure materials. All of this indicates that the origin of radiation resistance in HEAs as observed in experiments may not be related to a reduction in primary damage due to chemical disorder, but is probably caused by longer-time defect evolution.

Notes: This is a modified version of 2018--Farkas-D-Caro-A--Fe-Ni-Cr-Co-Cu that adds the ZBL correction at shorter interatomic distances making it suitable for radiation studies.

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Notes: This file was provided by Diana Farkas (Virginia Tech) on May 16, 2021 and posted with her permission.
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Citation: D. Farkas, and A. Caro (2018), "Model interatomic potentials and lattice strain in a high-entropy alloy", Journal of Materials Research, 33(19), 3218-3225. DOI: 10.1557/jmr.2018.245.
Abstract: A set of embedded atom method model interatomic potentials is presented to represent a high-entropy alloy with five components. The set is developed to resemble but not model precisely face-centered cubic (fcc) near-equiatomic mixtures of Fe–Ni–Cr–Co–Cu. The individual components have atomic sizes deviating up to 3%. With the heats of mixing of all binary equiatomic random fcc mixtures being less than 0.7 kJ/mol and the corresponding value for the quinary being −0.0002 kJ/mol, the potentials predict the random equiatomic fcc quinary mixture to be stable with respect to phase separation or ordering and with respect to bcc and hcp random mixtures. The details of lattice distortion, strain, and stress states in this phase are reported. The standard deviation in the individual nearest neighbor bond lengths was found to be in the range of 2%. Most importantly, individual atoms in the alloy were found to be under atomic strains up to 0.5%, corresponding to individual atomic stresses up to several GPa.

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Notes: This file was provided by Diana Farkas (Virginia Tech) on 19 March 2019 and posted with her permission. Update 2019-05-20: Superseded by new version.
File(s): superseded


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Notes: This file was provided by Diana Farkas (Virginia Tech) on 20 May 2019. Professor Farkas notes "The update is to make the potentials go to zero smoothly for distances of 5.8 Å. The original version went up to 6 Å and the last 0.2 Å were not smooth. This does not affect any of the common calculations but may make a difference in some cases like Peierls stresses of dislocations."
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Date Created: October 5, 2010 | Last updated: June 09, 2022