Angular melting scenarios in binary dusty-plasma Coulomb balls: Magic versus normal clusters

Abstract

Molecular-dynamic simulations were performed in order to investigate the melting processes of isotropically confined binary systems. We considered two species of particles, which differ by their amount of electric charge. A Lindemann type of criterion was used to determine the angular melting temperature. We demonstrate that the magic-to-normal cluster transition can evolve in two distinct ways, that is, through a structural phase transition of the first order or via a smooth transition where an increase of the shells' width leads to a continuous decreasing mechanical stability of the system. Moreover, for large systems, we demonstrate that the internal cluster exerts a minor effect on the mechanical stability of the external shell. Furthermore, we show that highly symmetric configurations, such as those found for multiple ring structures, have large mechanical stability, i.e., high angular melting temperature.

Resolving structural transitions in spherical dust clusters

“…[31][32][33] and on "magic" configurations (closed shells). Furthermore, the melting process of small Coulomb clusters is known to consist of multiple transition [34][35][36][37]. This makes a theoretical analysis of melting complicated because different quantities that agree among each other for macroscopic systems may yield very different predictions in finite systems.…”