A model of solar radiation and Joule heating in magnetohydrodynamic (MHD) convective flow of thixotropic nanofluid

被引：155
作者：
Hayat, T. [1 ,2 ]
Waqas, M. [1 ,2 ]
Shehzad, S. A. [4 ]
Alsaedi, A. [3 ]
机构：
[1] Quaid I Azam Univ, Dept Math, Islamabad 45320, Pakistan
[2] Quaid I Azam Univ, Dept Math, Islamabad 44000, Pakistan
[3] King Abdulaziz Univ, Fac Sci, Dept Math, NAAM Res Grp, POB 80257, Jeddah 21589, Saudi Arabia
[4] Comsats Inst Informat Technol, Dept Math, Sahiwal 57000, Pakistan
来源：
JOURNAL OF MOLECULAR LIQUIDS | 2016年 / 215卷
关键词：
Hydromagnetics; Stagnation point flow; Thixotropic nanofluid; Joule heating; Viscous dissipation; Convective conditions; STAGNATION-POINT FLOW; 3-DIMENSIONAL FLOW; STRETCHING SHEET; JEFFREY FLUID; THERMOPHORESIS; SLIP; SIMULATION;
D O I：
10.1016/j.molliq.2016.01.005
中图分类号：
O64 [物理化学（理论化学）、化学物理学];
学科分类号：
070304 ; 081704 ;
摘要：
This paper reports the hydromagnetic stagnation point flow of thixotropic nanofluid towards an impermeable stretching surface. Effects of Brownian motion and thermophoresis are present. Heat and mass transfer analysis is performed in the presence of viscous dissipation, Joule heating and convective boundary conditions. Meaningful transformations are utilized to obtain nonlinear ordinary differential systems. Convergent solutions of the resulting differential systems are presented in series forms. Moreover the numerical values of skin friction coefficient, local Nusselt and Sherwood numbers are computed and analyzed. (C) 2016 Elsevier B.V. All rights reserved.
引用
收藏
页码：704 / 710
页数：7
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