Simulation of nanofluid thermal radiation in Marangoni convection flow of non-Newtonian fluid A revised model

被引:5
作者
Hayat, Tasawar [1 ]
Ullah, Ikram [1 ]
Waqas, Muhammad [2 ]
Alsaedi, Ahmed [3 ]
机构
[1] Quaid I Azam Univ, Dept Math, Islamabad, Pakistan
[2] Natl Univ Technol, NUTECH Sch Appl Sci & Humanities, Islamabad, Pakistan
[3] King Abdulaziz Univ, Dept Math, Jeddah, Saudi Arabia
关键词
Thermal radiation; Marangoni convection; Cross nanoliquid; Exponential space-dependent heat source; Zero mass flux condition; STAGNATION POINT FLOW; MIXED CONVECTION; VISCOUS DISSIPATION; HEAT-TRANSFER; NUMERICAL-SIMULATION; ENTROPY GENERATION; CARREAU-NANOFLUID; CHEMICAL-REACTION; STRETCHING SHEET; MHD FLOW;
D O I
10.1108/HFF-11-2018-0704
中图分类号
O414.1 [热力学];
学科分类号
摘要
Purpose The purpose of this study is to study the impacts of exponential space-dependent heat source (ESHS) and thermal radiation in Marangoni convective flow of Cross fluid. The passively controlled model is developed to exhibit the nanoparticles' concentration on the surface. Design/methodology/approach The resulting problem under consideration is tackled by using the shooting approach. Findings Temperature field augments with enhancement of the thermophoretic, exponential-based space heat source (ESHS) and radiation parameters, whereas it decays with the increase of the Marangoni ratio parameter. Originality/value To the best of the authors' knowledge, no such analysis has yet been reported.
引用
收藏
页码:2840 / 2853
页数:14
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