https://doi.org/10.1140/epjp/s13360-022-02410-6
Regular Article
Aspects of infinite shear rate viscosity and heat transport of magnetized Carreau nanofluid
1
Department of Mathematics & Statistics, Hazara University, Mansehra, Pakistan
2
GRC Department, Faculty of Applied Studies, King Abdulaziz University, Jeddah, Saudi Arabia
3
Statistics Department, Faculty of Science, King Abdulaziz University, Jeddah, Saudi Arabia
4
Department of Mathematics, Zagazig Faculty of Engineering, Zagazig University, Zagazig, Egypt
5
Faculty of Engineering and Technology, Future University, Cairo, Egypt
6
Department of Basic Science, Faculty of Engineering at Benha, Benha University, 13512, Benha, Egypt
f eng_rahmaelsadat@yahoo.com, Mohamed.Reda@fue.edu.eg
Received:
14
June
2021
Accepted:
22
January
2022
Published online:
20
February
2022
Viscosity of fluid keeps its leading role in the polymer process, biological fluids, mayonnaise, colloidal suspensions, melt solutions and lubrication models. The Carreau nanofluid viscosity model can explain features of non-Newtonian fluids in the shear-thinning/thickening regions. This article describes the Lorentz force effects with the use of the infinite shear rate of the Carreau viscosity model and thermal radiation along with the influence of non-uniform heat source/sink transportation phenomenon of heat over the surface. The transformations of dimensionless variables are implemented to convert the partial differential equations into nonlinear coupled ordinary differential equations (ODEs). The solution of these ODEs is performed using the Runge–Kutta Fehlberg method along with the shooting scheme. The effects of the We, Pr, M, Nr, β*, β, B*and A*parameters denote the Weissenberg number, Prandtl number, radiation parameter, temperature ratio parameter, viscosity ratio parameter, stretching parameter, coefficients of space and temperature-dependent heat source/sink. For the correctness and exactness of the scheme, a comparison study is also provided based on the present results and the published results.
© The Author(s), under exclusive licence to Società Italiana di Fisica and Springer-Verlag GmbH Germany, part of Springer Nature 2022