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磁场对液体界面处各向异性磁性颗粒取向的影响。

Influence of magnetic field on the orientation of anisotropic magnetic particles at liquid interfaces.

作者信息

Newton Bethany J, Brakke Kenneth A, Buzza D Martin A

机构信息

Theory of Condensed Matter Group, Department of Physics and Mathematics, University of Hull, Hull, HU6 7RX, UK.

出版信息

Phys Chem Chem Phys. 2014 Dec 21;16(47):26051-8. doi: 10.1039/c4cp04270k. Epub 2014 Oct 31.

Abstract

We study theoretically the influence of an external magnetic field on the orientation of an ellipsoidal magnetic particle adsorbed at a liquid interface. Using the finite element program Surface Evolver, we calculate the equilibrium meniscus shape around the ellipsoidal particle and its equilibrium tilt angle with respect to the undeformed interface θt when a magnetic field B is applied perpendicular to the interface. We find that as we increase field strength, θt increases and at a critical magnetic field Bc1 and tilt angle θc1, the particle undergoes a discontinuous transition to the 'perpendicular' orientation (θt = 90°). Our results agree qualitatively with the simplified theory of Bresme and Faraudo [F. Bresme and J. Faraudo, J. Phys.: Condens. Matter, 2007, 19, 375110] which assumes that the liquid interface is flat, while they agree quantitatively with recent lattice-Boltzmann simulations of Davies et al. [G. Davies et al., Soft Matter, 2014, 10, 6742] which account for the deformation of the liquid meniscus. We also show for the first time that upon reducing the external magnetic field, at a critical magnetic field Bc2 < Bc1, the particle undergoes a second discontinuous transition from the perpendicular orientation to a finite tilt angle θc2 < θc1. In other words, for micron-sized particles where the thermal energy kBT is negligible compared to the interfacial energy, the tilt angle vs. magnetic field curve exhibits hysteresis behaviour. Due to the higher degree of accuracy of the Surface Evolver method, we are able to analyse the behaviour of the particles near these orientational transitions accurately and study how the critical quantities Bc1, Bc2, θc1 and θc2 vary with particle aspect ratio and contact angle.

摘要

我们从理论上研究了外部磁场对吸附在液体界面的椭球形磁性颗粒取向的影响。使用有限元程序Surface Evolver,当垂直于界面施加磁场B时,我们计算了椭球形颗粒周围的平衡弯月面形状及其相对于未变形界面的平衡倾斜角θt。我们发现,随着磁场强度的增加,θt增大,并且在临界磁场Bc1和倾斜角θc1时,颗粒经历不连续转变到“垂直”取向(θt = 90°)。我们的结果在定性上与Bresme和Faraudo的简化理论[F. Bresme和J. Faraudo,《物理学报:凝聚态物质》,2007年,19卷,375110]一致,该理论假设液体界面是平的,而在定量上与Davies等人最近的格子玻尔兹曼模拟[G. Davies等人,《软物质》,2014年,10卷,6742]一致,后者考虑了液体弯月面的变形。我们还首次表明,在降低外部磁场时,在临界磁场Bc2 < Bc1时,颗粒经历从垂直取向到有限倾斜角θc2 < θc1的第二次不连续转变。换句话说,对于微米级颗粒,其中热能kBT与界面能相比可忽略不计,倾斜角与磁场曲线表现出滞后行为。由于Surface Evolver方法具有更高的精度,我们能够准确分析颗粒在这些取向转变附近的行为,并研究临界量Bc1、Bc2、θc1和θc2如何随颗粒纵横比和接触角变化。

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