蠕动管内气泡运动研究

IF 1.9 4区 物理与天体物理 Q2 PHYSICS, MULTIDISCIPLINARY
Pramana Pub Date : 2024-11-09 DOI:10.1007/s12043-024-02834-y
Abha Kumari, Rajat Tripathi, Amit Kumar
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引用次数: 0

摘要

本文讨论了一个轴对称长气泡(流体 1)在含有自润湿流体(流体 2)的垂直蠕动导管内的运动。导管内的流体和漂浮的气泡互不相溶、不可压缩且密度不同。蠕动通道有两个开口端。假设气泡可以在管内自由移动,不会受到管壁的限制或变形。我们讨论了两种流体之间的密度差、热梯度和溶质梯度引起的马兰戈尼对流以及施加的回流对气泡位置和形状的影响。气泡在蠕动管内的运动受热梯度和溶质梯度引起的马兰戈尼对流的影响,已在以下领域得到广泛应用:利用海泡对大气进行电气化、在微流体设备中进行高效混合、改善热交换器的冷却效果、设计疏水表面、喷涂照相技术、增强化学反应器中的传质、利用精确的流体控制推进各种工业和生物医学应用。利用二维圆柱极坐标系建立了该问题的数学模型。控制方程采用线性偏微分方程的形式,并已通过分析求解。通过绘制气泡位置图,讨论了微重力区域热固性马兰戈尼对流和外加回流的影响,以及在没有马兰戈尼对流或回流的情况下重力驱动对流对气泡运动的影响。初始半径和热溶解马兰戈尼对流决定了气泡在演变过程中的形态。当初始半径低于临界值时,气泡变宽变短;反之,当初始半径超过临界值时,气泡变长变细。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Study of the bubble motion inside a peristaltic tube

The motion of a long, axisymmetric bubble (fluid 1) inside a vertical peristaltic conduit containing a self-rewetting fluid (fluid 2) is discussed in this article. The fluid inside the tube and the floating bubble are immiscible, incompressible and have different densities. The peristaltic channel has two open ends. It is assumed that the bubble can move freely inside the tube without being restricted or deformed by the border wall. The effect of the density difference between the two fluids, Marangoni convection caused by the thermal and solutal gradient and an imposed back flow on the position and shape of the bubble have all been discussed. Motion of the bubble within a peristaltic tube, influenced by the Marangoni convection due to thermal and solutal gradients, has find various applications in the electrification of the atmosphere by sea bubbles, efficient mixing in microfluidic devices, improved cooling in heat exchangers, design of hydrophobic surfaces, spray coating thography techniques, enhanced mass transfer in chemical reactors, advancing various industrial and biomedical applications with precise fluid control. A mathematical model of the problem has been developed using a two-dimensional cylindrical polar coordinate system. The governing equations are in the form of linear partial differential equation and have been solved analytically. The effect of the thermo-solutal Marangoni convection in the microgravity region and the imposed back flow, impact of gravity-driven convection in the absence of the Marangoni convection or back flow, on the motion of bubble are discussed by plotting the position of the bubble. The initial radius and thermo-solutal Marangoni convection determine the bubble’s form as it evolves. When the initial radius falls below a critical value, the bubble becomes broader and shorter; conversely, when the original radius exceeds the crucial value, the bubble becomes longer and thinner.

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来源期刊
Pramana
Pramana 物理-物理:综合
CiteScore
3.60
自引率
7.10%
发文量
206
审稿时长
3 months
期刊介绍: Pramana - Journal of Physics is a monthly research journal in English published by the Indian Academy of Sciences in collaboration with Indian National Science Academy and Indian Physics Association. The journal publishes refereed papers covering current research in Physics, both original contributions - research papers, brief reports or rapid communications - and invited reviews. Pramana also publishes special issues devoted to advances in specific areas of Physics and proceedings of select high quality conferences.
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