MHD stagnation point flow of viscoelastic nanofluid with non-linear radiation effects

被引:286
作者
Farooq, M. [1 ]
Khan, M. Ijaz [2 ]
Waqas, M. [2 ]
Hayat, T. [2 ,3 ]
Alsaedi, A. [3 ]
Khan, M. Imran [4 ]
机构
[1] Riphah Int Univ, Dept Math, Islamabad 44000, Pakistan
[2] Quaid I Azam Univ, Dept Math, Islamabad 44000, Pakistan
[3] King Abdulaziz Univ, Dept Math, Nonlinear Anal & Appl Math NAAM Res Grp, Fac Sci, POB 80203, Jeddah 21589, Saudi Arabia
[4] Heriot Watt Univ, Edinburgh Campus, Edinburgh EH14 4AS, Midlothian, Scotland
关键词
Non-linear radiative effect; Viscoelastic fluid; Convective boundary condition; VARIABLE THERMAL-CONDUCTIVITY; CHRISTOV HEAT-FLUX; JEFFREY FLUID; STRETCHING SHEET; MAGNETOHYDRODYNAMIC FLOW; SURFACE; SLIP; STRATIFICATION; THERMOPHORESIS; VELOCITY;
D O I
10.1016/j.molliq.2016.06.077
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 article addresses the MHD stagnation point flow of a viscoelastic nanofluid towards a stretching surface with nonlinear radiative effects. The nanofluid model consists of Brownian motion and thermophoresis. Heat transfer is studied by employing convective condition at the stretching surface. A newly constructed condition for heat transfer is imposed. The relevant problems are modeled by considering nonlinear thermal radiation. Similarity transformation is utilized to reduce the nonlinear partial differential equations into coupled nonlinear ordinary differential equations. The convergent solutions for velocity, temperature and concentration equations are developed. Graphical results are drawn for the velocity, temperature, concentration, skin friction coefficient and Nusselt number. It is noticed that skin friction increases for a larger magnetic parameter. (C) 2016 Elsevier B.V. All rights reserved.
引用
收藏
页码:1097 / 1103
页数:7
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