The Casimir-like effect induced by active nematics.

IF 2.3 4区 物理与天体物理 Q3 PHYSICS, CONDENSED MATTER Journal of Physics: Condensed Matter Pub Date : 2024-08-12 DOI:10.1088/1361-648X/ad69f1
Fahimeh Karimi Pour Haddadan
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Abstract

We consider an active nematic phase and use hydrodynamical equations of it to model the activity as an internal field. The interaction of this field with the nematic director in a confined geometry is included in the Hamiltonian of the system. Based on this model Hamiltonian and the standard field theoretical approach, the Casimir-like force induced between the boundaries of such a confined film is discussed. The force depends on the geometrical shape and the dynamical character of the constituents of our active phase, as well as the anchoring conditions. For homeotropically aligned rod-like particles which in principle tend to align along a planar flow field, extensile activity enhances the attraction present in a thin nematic film. As the film thickness increases the force reduces. Beyond a critical thickness, a planar flow field instantaneous to a bend distortion sets in. Near but below the threshold of this activity-induced instability, the force crosses zero and repulsively diverges right at the critical threshold of this so-called flow instability. For contractile rods, in the same geometry as above, the structure is stable and the Casimir-like force diminishes by an exponential factor as a function of the film thickness. On the other side for a planar director alignment, rod-like contractile particles can induce opposite shear flows at the boundaries creating a splay distortion for the director between the plates. In this configuration, we obtain the same universal pretransitional behavior for the force as above. Vice versa, for extensile rod-like particles in this geometry, the director fluctuations become massive and the Casimir-like force diminishes again by an exponential factor as the film thickness increases. The effect of the active field on thermal fluctuations of the director and the fluctuation-induced Casimir force per area is derived through a "semi"-dynamical approach as well. However, the results of the calculation due to a mathematical sum over the fluctuating modes do not lead to an approved closed form.

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主动线粒体诱发的卡西米尔效应
我们考虑了活性向列相,并使用其流体力学方程将活性模拟为内部场。这个场与封闭几何中的向列导的相互作用被包含在系统的哈密顿中。根据这个哈密顿模型和标准场论方法,讨论了在这种封闭薄膜的边界之间诱发的卡西米尔力。卡西米尔力取决于活性相的几何形状、组成成分的动力学特性以及锚定条件。对于顺向排列的杆状颗粒(原则上倾向于沿着平面流场排列),拉伸活动增强了向列薄膜中存在的吸引力。随着薄膜厚度的增加,吸引力会减小。超过临界厚度后,平面流场会瞬间发生弯曲变形。在接近但低于这种活动诱发的不稳定性临界点时,力会趋于零,并在这种所谓的流动不稳定性临界点处发生排斥性发散。对于收缩棒,在上述相同的几何形状下,结构是稳定的,卡西米尔样力随着薄膜厚度的增加以指数系数减小。另一方面,在平面导向对齐的情况下,棒状收缩粒子会在边界处引起相反的剪切流,导致板间的导向产生倾斜变形。在这种结构中,我们可以得到与上述相同的力的普遍预过渡行为。反之亦然,对于这种几何形状中的伸展杆状粒子,导线波动变得巨大,卡西米尔力随着薄膜厚度的增加以指数系数再次减小。我们还通过 "半 "动力学方法推导出了有源场对导线热波动的影响以及由波动引起的单位面积卡西米尔力。然而,通过对波动模式进行数学求和得出的计算结果并没有得到认可的封闭形式。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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来源期刊
Journal of Physics: Condensed Matter
Journal of Physics: Condensed Matter 物理-物理:凝聚态物理
CiteScore
5.30
自引率
7.40%
发文量
1288
审稿时长
2.1 months
期刊介绍: Journal of Physics: Condensed Matter covers the whole of condensed matter physics including soft condensed matter and nanostructures. Papers may report experimental, theoretical and simulation studies. Note that papers must contain fundamental condensed matter science: papers reporting methods of materials preparation or properties of materials without novel condensed matter content will not be accepted.
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