Gravitational effects on structure development in quenched complex fluids

被引:7
|
作者
Badalassi, VE [1 ]
Ceniceros, HD
Banerjee, S
机构
[1] Univ Calif Santa Barbara, Dept Chem Engn, Santa Barbara, CA 93106 USA
[2] Univ Calif Santa Barbara, Dept Math, Santa Barbara, CA 93106 USA
来源
关键词
Cahn-Hilliard equation; Navier-Stokes equations; Model H; phase separation under gravity;
D O I
10.1196/annals.1324.031
中图分类号
Q6 [生物物理学];
学科分类号
071011 ;
摘要
When binary liquid mixtures are cooled rapidly from a homogeneous phase into a two-phase system, domains of the two equilibrium phases form and grow (coarsen) with time. In the absence of an external forcing due to gravity or an imposed shear flow, a dynamic scaling regime emerges in which the domain morphology is statistically self-similar at different times with a length-scale that grows with time. In the presence of gravity, however, multiple length scales develop, with the system coarsening more rapidly in the direction of the force. The late-time behavior of such a system is characterized in this study by the calculation of anisotropic growth laws. Gravitation effects significantly affect scaling laws, even with small density mismatch, and the growth mechanism has some similarities to the sedimentation process. However, very few numerical studies have been made of such effects; this is one of the first.
引用
收藏
页码:371 / 382
页数:12
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