Power dissipation and entropy production rate of high-dimensional optical matter systems.

IF 2.2 3区 物理与天体物理 Q2 PHYSICS, FLUIDS & PLASMAS
Shiqi Chen, Emmanuel Valenton, Grant M Rotskoff, Andrew L Ferguson, Stuart A Rice, Norbert F Scherer
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引用次数: 0

Abstract

Entropy production is an essential aspect of creating and maintaining nonequilibrium systems. Despite their ubiquity, calculation of entropy production rates is challenging for high-dimensional systems, so it has only been reported for simple (i.e., l-particle) systems. Moreover, there is a dearth of nontrivial experimental systems where precise measurements of entropy production rate and characterization of the nonequilibrium steady state (NESS) are simultaneously possible. We report an approach to calculate the entropy production rate of overdamped, nonconservative, N-body systems and demonstrate this on a six-particle triangle optical matter (OM) system as a nontrivial example. OM systems consist of (nano-)particles organized into ordered arrays that are bound by electrodynamic interactions associated with the scattering and interference of light, and the associated induced-polarizations in and among the particles in coherent optical beams. The flux of laser light in OM systems in a solution environment necessitates that they dissipate energy, produce entropy, and relax to a NESS. The NESS may have several ordered particle configurations (i.e., isomers) that can interchange by barrier crossing processes. Understanding the power dissipation and entropy production rate of a NESS in an OM system along different (collective) modes of motion can advance understanding of the relative stability of the NESSs as well as inform design and control of OM structures. Therefore, we compute the components of the entropy production rate and power dissipation along the collective coordinates of the 6 Ag nanoparticle triangle OM system from OM NESS trajectory data and verify the Seifert relation [U. Seifert, Rep. Prog. Phys. 75, 126001 (2012)10.1088/0034-4885/75/12/126001] for these complex systems with a nuanced interpretation.

高维光学物质系统的功率耗散和熵产生率。
熵产生是创建和维持非平衡系统的一个重要方面。尽管熵的产生无处不在,但对于高维系统来说,熵产生率的计算具有挑战性,因此只有关于简单(即 l 粒子)系统的报告。此外,同时可以精确测量熵产生率和非平衡稳态(NESS)特征的非简单实验系统非常缺乏。我们报告了一种计算过阻尼、非守恒、N 体系统熵产生率的方法,并以一个六粒子三角形光学物质(OM)系统作为非微观示例进行了演示。光学物质系统由有序排列的(纳米)粒子组成,这些粒子受到与光的散射和干涉有关的电动相互作用以及相干光束中粒子内部和粒子之间的相关诱导极化的约束。在溶液环境中,OM 系统中的激光通量要求它们耗散能量、产生熵并弛豫到 NESS。NESS 中可能有几种有序的粒子构型(即异构体),这些粒子构型可以通过越障过程进行互换。了解 OM 系统中 NESS 沿不同(集体)运动模式的功率耗散和熵产生率,有助于加深对 NESS 相对稳定性的理解,并为 OM 结构的设计和控制提供参考。因此,我们根据 OM NESS 轨迹数据计算了 6 个银纳米粒子三角形 OM 系统沿集体坐标的熵产生率和功率耗散分量,并验证了 Seifert 关系 [U. Seifert, Rep. Progress.Seifert, Rep.75, 126001 (2012)10.1088/0034-4885/75/12/126001]对这些复杂系统的细微解释。
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
Physical Review E
Physical Review E PHYSICS, FLUIDS & PLASMASPHYSICS, MATHEMAT-PHYSICS, MATHEMATICAL
CiteScore
4.50
自引率
16.70%
发文量
2110
期刊介绍: Physical Review E (PRE), broad and interdisciplinary in scope, focuses on collective phenomena of many-body systems, with statistical physics and nonlinear dynamics as the central themes of the journal. Physical Review E publishes recent developments in biological and soft matter physics including granular materials, colloids, complex fluids, liquid crystals, and polymers. The journal covers fluid dynamics and plasma physics and includes sections on computational and interdisciplinary physics, for example, complex networks.
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