Lane formation in gravitationally driven colloid mixtures consisting of up to three different particle sizes

dc.contributor.authorHofmann, Kay
dc.contributor.authorIsele, Marc
dc.contributor.authorErbe, Artur
dc.contributor.authorLeiderer, Paul
dc.contributor.authorNielaba, Peter
dc.date.accessioned2024-06-05T07:44:21Z
dc.date.available2024-06-05T07:44:21Z
dc.date.issued2024
dc.description.abstractBrownian dynamics simulations are utilized to study segregation phenomena far from thermodynamic equilibrium. In the present study, we expand upon the analysis of binary colloid mixtures and introduce a third particle species to further our understanding of colloidal systems. Gravitationally driven, spherical colloids immersed in an implicit solvent are confined in two-dimensional linear microchannels. The interaction between the colloids is modeled by the Weeks-Chandler-Andersen potential, and the confinement of the colloids is realized by hard walls based on the solution of the Smoluchowski equation in half space. In binary and ternary colloidal systems, a difference in the driving force is achieved by differing colloid sizes but fixed mass density. We observe for both the binary and ternary systems that a driving force difference induces a nonequilibrium phase transition to lanes. For ternary systems, we study the tendency of lane formation to depend on the diameter of the medium-sized colloids. Here we find a sweet spot for lane formation in ternary systems. Furthermore, we study the interaction of two differently sized colloids at the channel walls. Recently we observed that driven large colloids push smaller colloids to the walls. This results in small particle lanes at the walls at early simulation times. In this work we additionally find that thin lanes are unstable and dissolve over very long time frames. Furthermore, we observe a connection between lane formation and the nonuniform distribution of particles along the channel length. This nonuniform distribution occurs either alongside lane formation or in shared lanes (i.e., lanes consisting of two colloid types).
dc.description.versionpublisheddeu
dc.identifier.doi10.1103/physreve.109.064601
dc.identifier.urihttps://kops.uni-konstanz.de/handle/123456789/70068
dc.language.isoeng
dc.subject.ddc530
dc.titleLane formation in gravitationally driven colloid mixtures consisting of up to three different particle sizeseng
dc.typeJOURNAL_ARTICLE
dspace.entity.typePublication
kops.citation.bibtex
@article{Hofmann2024forma-70068,
  year={2024},
  doi={10.1103/physreve.109.064601},
  title={Lane formation in gravitationally driven colloid mixtures consisting of up to three different particle sizes},
  number={6},
  volume={109},
  issn={2470-0045},
  journal={Physical Review E},
  author={Hofmann, Kay and Isele, Marc and Erbe, Artur and Leiderer, Paul and Nielaba, Peter},
  note={Article Number: 064601}
}
kops.citation.iso690HOFMANN, Kay, Marc ISELE, Artur ERBE, Paul LEIDERER, Peter NIELABA, 2024. Lane formation in gravitationally driven colloid mixtures consisting of up to three different particle sizes. In: Physical Review E. American Physical Society (APS). 2024, 109(6), 064601. ISSN 2470-0045. eISSN 2470-0053. Verfügbar unter: doi: 10.1103/physreve.109.064601deu
kops.citation.iso690HOFMANN, Kay, Marc ISELE, Artur ERBE, Paul LEIDERER, Peter NIELABA, 2024. Lane formation in gravitationally driven colloid mixtures consisting of up to three different particle sizes. In: Physical Review E. American Physical Society (APS). 2024, 109(6), 064601. ISSN 2470-0045. eISSN 2470-0053. Available under: doi: 10.1103/physreve.109.064601eng
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kops.sourcefield.plainPhysical Review E. American Physical Society (APS). 2024, 109(6), 064601. ISSN 2470-0045. eISSN 2470-0053. Available under: doi: 10.1103/physreve.109.064601eng
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