在化学反应的作用下,极性纳米流体在伸长的可渗透表面上的惯性阻力与不均匀的发热/吸热效应相结合,对水磁流产生影响

Subhajit Panda, Pradyumna Kumar Pattnaik, Rupa Baithalu, Satya Ranjan Mishra
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引用次数: 0

摘要

由于各种工程应用,布朗流和热泳在研究极性纳米流体的流动特性方面发挥着举足轻重的作用。在用于热疗的生物医学纳米医学领域,为了增强热和传输特性;在冷却电子设备、热交换器和汽车发动机中,为了提高热交换过程的效率,布朗和热泳的使用非常重要。因此,本研究揭示了达西-福克海默惯性阻力以及与空间和温度相关的热量产生/吸收对极性纳米流体在拉伸表面上流动的重要性。表面被认为是可渗透的,在热辐射、布朗运动和热泳的作用下,水磁流动会对流动现象产生重大影响。通过实施适当的相似性规则,将根据上述物理特性设计的拟议流动模型标准化为非线性普通方程组。此外,通过使用传统的 Rung-Kutta 四阶技术对系统进行求解,可以得出各种物理量的特征。此外,还通过图形对几个因素进行了简要分析,并通过表格对速率系数进行了模拟。研究的重要结果是,热浮力和溶质浮力的加入会增强速度分布,而惯性阻力的增加则会产生相反的影响。此外,与空间和温度相关的热源会增强温度分布,但路易斯数会显著降低流体浓度。
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Inertial drag combined with non‐uniform heat generation/absorption effects on the hydromagnetic flow of polar nanofluid over an elongating permeable surface due to the impose of chemical reaction
The pivotal role of Brownian and thermophoresis in investigating the flow characteristic of polar nanofluid is important nowadays due to various engineering applications. The enhanced thermal and transport properties in the field of biomedical nanomedicine for hyperthermia treatments, and for enhancing the efficiency of heat exchange processes in cooling electronic devices, heat exchangers, and automotive engines the use of Brownian and thermophoresis is important. Therefore, the present study reveals the importance of Darcy–Forchheimer inertial drag combined with the space‐ and temperature‐dependent heat generation/absorption on the flow of polar nanofluid over an elongating surface. The surface is considered to be permeable for which the hydromagnetic flow in the presence of thermal radiation specifically, Brownian and thermophoresis affects the flow phenomena significantly. The proposed flow model designed with the aforementioned physical properties is standardized into the set of nonlinear ordinary equations by the implementation of suitable similarity rules. Further, the characteristics of various physical quantities are deployed by solving the system by using traditional Rung–Kutta fourth‐order technique. Further, the analysis of several factors is deployed briefly via graphically, and simulation of rate coefficients is presented through tables. The important outcomes of the study are deployed as the inclusion of thermal and solutal buoyancy enhances the velocity distribution, whereas reverse impact is observed for the increasing inertial drag. Also, space‐ and temperature‐dependent heat source augments the temperature profile but Lewis number decelerates the fluid concentration significantly.
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