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Convective heat transfer during the flow of Williamson nanofluid with thermal radiation and magnetic effects

机译:威廉森纳米流体流动过程中具有热辐射和磁效应的对流传热

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摘要

.Recently, several studies have been presented to show that nanofluids are amongst the best tools for the enhancement of heat transfer characteristics. It has been experimentally verified that nanofluids are a new type of enhanced working fluids, engineered with enhanced thermo-physical properties. Therefore, we present a novel study to develop and understand a mathematical model for a non-Newtonian Williamson fluid flow in the presence of nanoparticles. This study aims at describing the thermal characteristics of nanoparticles via Rosseland approximation to illustrate the non-linear radiation effects. Convective heat transfer model alongside Brownian motion are studied for the electrically conducting nanofluids flow. A set of partial differential equations for Williamson nanofluid flow has been derived by basic conservation laws, i.e., momentum, energy and concentration conservations. These equations are initially converted to ordinary differential equations by employing non-dimensional quantities. The numerical simulation of these equations is performed using the Runge-Kutta-Fehlberg scheme. The corresponding important physical parameters have been produced as function of the unsteadiness parameter, Weissenberg number, magnetic parameter, radiation parameter, Brownian motion parameter, thermophoresis parameter, Prandtl number, Biot number, velocity slip parameter and Lewis number. The examination is done to investigate the impact of the above-said parameters on momentum, thermal and concentration boundary layers. It is concluded from our computations that the nanofluids velocity and temperature accelerate when the Brownian motion parameter rises. Results proved that temperature gradient enhances with increase of solid particle concentration, while it decreases with increasing magnetic field. Finally, a comparison of the obtained numerical solution against previous literature is presented which shows satisfactory agreement.
机译:如图所示,已经提出了几项研究表明纳米流体是增强传热特性的最佳工具之一。它已经通过实验验证,纳米流体是一种新型的增强工作流体,设计具有增强的热物理性质。因此,我们提出了一种新的研究,可以在存在纳米颗粒存在下为非牛顿的威廉姆森流体流动进行开发和理解数学模型。该研究旨在通过rosseland近似来描述纳米颗粒的热特性,以说明非线性辐射效应。研究了棕色运动的对流传热模型,用于导电纳米流体流动。威廉姆森纳米流体流动的一组局部微分方程是由基本保护法,即势头,能源和集中保守的衍生。通过采用非尺寸量,最初将这些等式转换为普通微分方程。使用Runge-Kutta-Fehlberg方案进行这些等式的数值模拟。相应的重要物理参数已作为不稳定参数,Weissenberg编号,磁场,辐射参数,布朗运动参数,热量参数,Prandtl号,Biot Numbers,速度滑动参数和Lewis编号的功能。进行检查以研究上述参数对动量,热和浓度边界层的影响。从我们的计算结束,即纳米流体速度和温度在布朗运动参数上升时加速。结果证明,温度梯度随着固体颗粒浓度的增加而增强,同时随着磁场的增加而降低。最后,提出了对先前文献的所得数值解决方案的比较,其显示令人满意的协议。

著录项

  • 来源
    《European Physical Journal Plus》 |2019年第2期|共12页
  • 作者

    Hashim; Khan Masood; Hamid Aamir;

  • 作者单位

    Quaid I Azam Univ Dept Math Islamabad 44000 Pakistan;

    Quaid I Azam Univ Dept Math Islamabad 44000 Pakistan;

    Quaid I Azam Univ Dept Math Islamabad 44000 Pakistan;

  • 收录信息
  • 原文格式 PDF
  • 正文语种 eng
  • 中图分类 物理学;
  • 关键词

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