星团(航天器)
胶体
化学物理
航程(航空)
胶粒
粒子(生态学)
球状星团
絮凝作用
相(物质)
物理
材料科学
统计物理学
纳米技术
化学
地质学
星星
物理化学
天体物理学
复合材料
海洋学
有机化学
量子力学
程序设计语言
计算机科学
作者
Antonio Díaz Pozuelo,Diego González-Salgado,E. Lomba
摘要
A simple three-dimensional model of a fluid whose constituent particles interact via a short range attractive and long range repulsive potential is used to model the aggregation into large spherical-like clusters made up of hundreds of particles. The model can be thought of as a straightforward rendition of colloid flocculation into large spherical aggregates. We illustrate how temperature and particle density influence the cluster size distribution and affect inter- and intra-cluster dynamics. The system is shown to exhibit two well separated length and time scales, which can be tuned by the balance between repulsive and attractive forces. Interestingly, cluster aggregates at moderate/low temperatures approach a cluster glassy phase, whereas cluster particles retain a local liquid-like structure. These states present a strong suppression of density fluctuations for a significant range of relatively large wavelengths, meeting the criterion of effective disordered hyperuniform materials as far as the intercluster structure is concerned.
科研通智能强力驱动
Strongly Powered by AbleSci AI