Entropy generation in dissipative flow of Williamson fluid between two rotating disks

被引:151
作者
Qayyum, Sumaira [1 ]
Khan, M. Ijaz [1 ]
Hayat, T. [1 ,2 ]
Alsaedi, A. [2 ]
Tamoor, M. [3 ]
机构
[1] Quaid I Azam Univ, Dept Math, Islamabad 44000, Pakistan
[2] King Abdulaziz Univ, Fac Sci, Dept Math, NAAM Res Grp, Jeddah 21589, Saudi Arabia
[3] Univ Chinese Acad Sci, Inst Proc Engn, Beijing 100190, Peoples R China
关键词
Double rotating disks; Entropy generation; Williamson fluid; Viscous dissipation; Thermal radiation; Heat generation/absorption; CHRISTOV HEAT-FLUX; STAGNATION POINT FLOW; THERMAL-RADIATION; CARBON NANOTUBES; VISCOUS DISSIPATION; ACTIVATION-ENERGY; MHD FLOW; NANOFLUIDS; WATER; SWCNTS;
D O I
10.1016/j.ijheatmasstransfer.2018.08.034
中图分类号
O414.1 [热力学];
学科分类号
摘要
This communication addresses flow characteristics of Williamson fluid between two rotating disks. Electrically conducting fluid is considered. Total entropy generation rate is calculated through implementation of second law of thermodynamics. The lower and upper disks have different stretching rates and angular velocities for rotation. Characteristics of heat transport are expressed through dissipation, heat generation/absorption and thermal radiation. Von Karman transformations are utilized to convert the dimensional flow expressions into dimensionless form. Convergent series solutions are constructed. Influence of different pertinent variables on velocity, temperature, entropy number, skin friction coefficients and Nusselt numbers are studied. It is observed that the axial and tangential velocities increase for higher Weissenberg number while radial velocity decays. Further entropy number remarkably increases for magnetic, radiation and Brinkman number. Bejan number is less for higher magnetic parameter, stretching parameter, Brinkman number and Weissenberg number. (C) 2018 Elsevier Ltd. All rights reserved.
引用
收藏
页码:933 / 942
页数:10
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