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dc.contributorUniversity of Marylanden_US
dc.contributor.authorJoost, William J.
dc.contributor.authorAnkem, Sreeramamurthy
dc.contributor.authorKuklja, Maija M.
dc.contributor.otherwilliam.joost@gmail.comen_US
dc.date.accessioned2015-09-03T14:51:36Z
dc.date.available2015-09-03T14:51:36Z
dc.identifier.citationInteraction Between Oxygen Interstitials and Deformation Twins in alpha-Titanium, Acta Materialia v. 105 (2016), pp. 44 - 51 http://dx.doi.org/10.1016/j.actamat.2015.12.019en_US
dc.identifier.urihttp://hdl.handle.net/11256/272
dc.description.abstractThese data files provide input/output VASP and LAMMPS data along with spreadsheets containing data used to produce graphs in our above-reference article. The article abstract is: Twinning is an important deformation mechanism in many hexagonal close packed metals, including alpha-titanium (Ti) alloys. However, the mechanisms for twin nucleation, growth, and interaction with other defects are not completely understood. In this study we interrogate the behavior of oxygen (O) interstitials near a (10-12) twin boundary using a combination of density functional theory (DFT) and modified embedded atom method (MEAM) calculations. The presence of the twin boundary significantly affects both interstitial formation energy as well as the activation barriers for diffusion between sites. We demonstrate that a tetrahedral interstitial is stable in the twin boundary, despite being unstable in bulk Ti, while the formation energies of the octahedral, hexahedral, and crowdion interstitials are all modified by a nearby twin. Further, the activation barriers for diffusion in the region near the twin are uniformly lower than in the bulk. An atom diffusing across the twin boundary moves through several paths with peak activation barriers more than 0.3 eV lower than for comparable diffusion far from the twin, suggesting that the (10-12) twin is a fast diffusion pathway and movement of oxygen interstitials across the twin during twin growth is possible.en_US
dc.description.sponsorshipWe appreciate access to and use of resources of the National Energy Research Scientific Computing Center (NERSC), which is supported by the Office of Science of the U.S. Department of Energy under Contract No. DE-AC02-05CH11231. We acknowledge the University of Maryland supercomputing resources (http://www.it.umd.edu/hpcc) made available in conducting the research reported in this research. Portions of this work were supported by the National Science Foundation under Grant No. DMR-0906994.en_US
dc.relation.haspartW.J. Joost, S. Ankem, and M.M. Kuklja, Mod. Sim. Mat. Sci. and Eng., vol. 23, no. 1, p. 015006, 2015en_US
dc.rightsAttribution 3.0 United States*
dc.rights.urihttp://creativecommons.org/licenses/by/3.0/us/*
dc.subjectTitanium, Oxygen, Diffusion, Twinen_US
dc.titleInteraction Between Oxygen Interstitials and Deformation Twins in alpha-Titaniumen_US
dc.typeDataseten_US


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Attribution 3.0 United States
Except where otherwise noted, this item's license is described as Attribution 3.0 United States