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dc.contributor.authorAmini, Majeed
dc.contributor.authorLaird, Brian Bostian
dc.date.accessioned2014-12-16T21:13:44Z
dc.date.available2014-12-16T21:13:44Z
dc.date.issued2008-10-30
dc.identifier.citationAmini, Majeed; Laird, Brian Bostian. (2008). "Crystal-melt interfacial free energy of binary hard spheres from capillary fluctuations." Physical Review B, 78(14):144112. http://dx.doi.org/10.1103/PhysRevB.78.144112
dc.identifier.issn1098-0122
dc.identifier.urihttp://hdl.handle.net/1808/16131
dc.descriptionThis is the publisher's version, also available electronically from http://journals.aps.org/prb/abstract/10.1103/PhysRevB.78.144112.
dc.description.abstractUsing molecular-dynamics simulation coupled with an analysis of equilibrium capillary fluctuations in interfacial position, we compute the magnitude and anisotropy of the interfacial free energy γ for a binary hard-sphere system with a diameter ratio α=0.9. This system, in which the fluid mixture coexists with a randomly substituted face-centered-cubic solid solution, is a useful reference model for alloys. Our results show that γ increases with increasing mole fraction of the smaller sized particle when temperature is held constant. However, after rescaling the results to fixed pressure and varying temperature, we find that γ decreases with increased alloying by the smaller particle (corresponding to lower temperatures). Thus, γ is seen to decrease with increasing concentration of the lower melting point solute, consistent with earlier simulations on Ni/Cu and Lennard-Jones mixtures. The anisotropy in γ is such that the inequality γ100>γ110>γ111 holds for all concentrations studied. Using the classification scheme of Haxhimali et al., [Nat. Mater. 5, 660 (2006)] we find that the anisotropy in γ is consistent with a predicted ⟨100⟩ primary dendrite growth direction.
dc.publisherAmerican Physical Society
dc.titleCrystal-melt interfacial free energy of binary hard spheres from capillary fluctuations
dc.typeArticle
kusw.kuauthorAmini, Majeed
kusw.kuauthorLaird, Brian Bostian
kusw.kudepartmentPhysics and Astronomy
kusw.kudepartmentChemistry
dc.identifier.doi10.1103/PhysRevB.78.144112
kusw.oaversionScholarly/refereed, publisher version
kusw.oapolicyThis item does not meet KU Open Access policy criteria.
dc.rights.accessrightsopenAccess


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