Solid-solid collapse transition in a two dimensional model molecular system

TL;DR

This study uses Monte Carlo simulations to explore the microscopic mechanisms of solid-solid collapse transitions in a 2D molecular model, revealing unique nucleation pathways and cluster geometries driven by competing interactions.

Contribution

It introduces a detailed simulation analysis of the collapse transition in a 2D molecular system with isotropic and anisotropic interactions, highlighting novel nucleation behaviors.

Findings

Linear strip-like nucleating clusters observed

Growth involves branched and ring-like strips

Nucleation influenced by competing interactions and intermediate phases

Abstract

Solid-solid collapse transition in open framework structures is ubiquitous in nature. The real difficulty in understanding detailed microscopic aspects of such transitions in molecular systems arises from the interplay between different energy and length scales involved in molecular systems, often mediated through a solvent. In this work we employ Monte Carlo (MC) simulations to study the collapse transition in a model molecular system interacting via both isotropic as well as anisotropic interactions having different length and energy scales. The model we use is known as Mercedes-Benz (MB) which for a specific set of parameters sustains three solid phases: honeycomb, oblique and triangular. In order to study the temperature induced collapse transition, we start with a metastable honeycomb solid and induce transition by heating. High density oblique solid so formed has two characteristic length scales corresponding to isotropic and anisotropic parts of interaction potential. Contrary to the common believe and classical nucleation theory, interestingly, we find linear strip-like nucleating clusters having significantly different order and average coordination number than the bulk stable phase. In the early stage of growth, the cluster grows as linear strip followed by branched and ring-like strips. The geometry of growing cluster is a consequence of the delicate balance between two types of interactions which enables the dominance of stabilizing energy over the destabilizing surface energy. The nuclei of stable oblique phase are wetted by intermediate order particles which minimizes the surface free energy. We observe different pathways for pressure and temperature induced transitions.