Condensed Matter Physics, 2017, vol. 20, No. 1, 13802
DOI:10.5488/CMP.20.13802           arXiv:1703.10401

Title: Shape characteristics of the aggregates formed by amphiphilic stars in water: dissipative particle dynamics study
Author(s):
  O.Y. Kalyuzhnyi (Institute for Condensed Matter Physics of the National Academy of Sciences of Ukraine, 1 Svientsitskii St., 79011 Lviv, Ukraine; Doctoral College for the Statistical Physics of Complex Systems, Leipzig-Lorraine-Lviv-Coventry 4, D-04009 Leipzig, Germany) ,
  J.M. Ilnytskyi (Institute for Condensed Matter Physics of the National Academy of Sciences of Ukraine, 1 Svientsitskii St., 79011 Lviv, Ukraine; Doctoral College for the Statistical Physics of Complex Systems, Leipzig-Lorraine-Lviv-Coventry 4, D-04009 Leipzig, Germany) ,
  C. von Ferber (Applied Mathematics Research Centre, Coventry University, Coventry, CV1 5FB, United Kingdom; Heinrich-Heine Universität Düsseldorf, D-40225 Düsseldorf, Germany; Doctoral College for the Statistical Physics of Complex Systems, Leipzig-Lorraine-Lviv-Coventry 4, D-04009 Leipzig, Germany)

We study the effect of the molecular architecture of amphiphilic star polymers on the shape of aggregates they form in water. Both solute and solvent are considered at a coarse-grained level by means of dissipative particle dynamics simulations. Four different molecular architectures are considered: the miktoarm star, two different diblock stars and a group of linear diblock copolymers, all of the same composition and molecular weight. Aggregation is started from a closely packed bunch of Na molecules immersed into water. In most cases, a single aggregate is observed as a result of equilibration, and its shape characteristics are studied depending on the aggregation number Na. Four types of aggregate shape are observed: spherical, rod-like and disc-like micelle and a spherical vesicle. We estimate "phase boundaries" between these shapes depending on the molecular architecture. Sharp transitions between aspherical micelle and a vesicle are found in most cases. The pretransition region shows large amplitude oscillations of the shape characteristics with the oscillation frequency strongly dependent on the molecular architecture.

Key words: star-like polymer, amphiphiles, micelle, vesicle, dissipative particle dynamics
PACS: 82.70.Uv, 78.67.Ve, 61.20.Ja


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