English

Simple Calibration of Block Copolymer Melt Models

Soft Condensed Matter 2024-08-16 v1

Abstract

According to the universality hypothesis, the phase behavior of different block copolymer melt models having fixed composition depends solely on two parameters: the invariant chain length Nˉ\bar{N} and the effective interaction parameter χN\chi N. If models behave universally, they can be compared to each other and can predict experiment quantitatively. Here, we present a simple way to achieve this universality for coarse-grained models. Our method relies on the properties of the monomer interaction potential energy zz distribution. In particular, models having near-symmetric zz-distributions exhibit universal phase behavior using the standard linear definition of the Flory-Huggins parameter χα\chi\propto\alpha, where α=ϵAB(ϵAA+ϵBB)/2\alpha = \epsilon_{AB}-(\epsilon_{AA}+\epsilon_{BB})/2, and ϵxy\epsilon_{xy} is the interaction energy between monomers of type xx and yy. Previously, universality had been achieved using a nonlinear χ(α)\chi(\alpha) function which is difficult to obtain and interpret physically. The main parameter controlling the symmetry of the zz-distribution is the monomer density ρ\rho. Above certain ρ\rho, models have symmetric zz-distributions, and their order-disorder transition points follow the universal curve predicted by Fredrickson-Helfand theory in the experimentally relevant Nˉ>102\bar{N} > 10^2 range. On the other hand, low-ρ\rho models exhibit skewed zz-distributions, and the simple χα\chi\propto\alpha formula is no longer universally applicable to them. Our results can be used for correct block copolymer model building leading to a simple and direct comparison of simulations to experiments, which will facilitate the screening of new block copolymer morphologies and support materials design.

Keywords

Cite

@article{arxiv.2402.18760,
  title  = {Simple Calibration of Block Copolymer Melt Models},
  author = {Artem Petrov and Hejin Huang and Alfredo Alexander-Katz},
  journal= {arXiv preprint arXiv:2402.18760},
  year   = {2024}
}
R2 v1 2026-06-28T15:03:56.831Z