Shaping the aggregates of discotic particles with directional pair interactions
B. Martínez-Haya, N. Morillo, A. Cuetos
TL;DR
This work investigates how directional pair interactions control discotic particle aggregation using the coarse-grained Oblate-Gay-Berne-Kihara (OGBK) model. By comparing three interaction schemes (K, E, F) through Monte Carlo and Brownian Dynamics simulations, it shows that topology ranges from globular clusters (K) to flat multilayer aggregates (E) to columnar bundles (F), with aggregation onset $T_c^*$ and percolation governed by density $\rho^*$ and temperature. The study provides cluster-size distributions, internal ordering insights, and kinetic analyses that reveal a non-monotonic temperature dependence of aggregation and density-driven percolation, illustrating how directionality can tailor suprastructural materials. These findings offer design principles for discotic materials with targeted electronic, optical, and sensing properties by tuning directional interactions.
Abstract
Aggregation processes in systems of planar macromolecules and colloids drive a broad range of phenomena in natural systems and soft materials. Depending on chemical architecture, intermolecular interactions in these systems may favor different relative pair orientations, such as stacking face-face or percolating edge-edge arrangements. In this work, we employ a versatile coarse-grained interaction model for disk-like particles to provide a general framework to rationalize the thermotropic formation of aggregates and predict the topology of the resulting suprastructures. Monte Carlo and Brownian Dynamics simulations show that, with an appropriate tuning of the interactions, discotics spontaneously nucleate into clusters with globular, planar or stacked geometries, leading to materials with specific internal order and associated physicochemical properties.
