Numerical simulation of combined effects of a vertical magnetic field and thermal radiation on natural convection of non-Newtonian fluids confined between circular and square concentric cylinders

被引:6
|
作者
Chtaibi, Khalid [1 ,2 ]
Dahani, Youssef [1 ]
Amahmid, Abdelkhalek [1 ]
Hasnaoui, Mohammed [1 ]
Ben Hamed, Haikel [2 ]
机构
[1] Cadi Ayyad Univ, Dept Phys, Unit Affiliated CNRST URL CNRTST 16, Lab Fluid Mech & Energet LMFE,Fac Sci Semlalia, BP 2390, Marrakech, Morocco
[2] Picardie Jules Verne Univ, Inst Technol Univ, Lab Innovates Technol LTI, Amiens, France
关键词
Non-Newtonian fluid; Thermal radiation; Magnetic field; Horizontal circular cylinder; Power-law behavior; LATTICE-BOLTZMANN METHOD; HEAT-TRANSFER; BOUNDARY-CONDITIONS; FLOW PATTERNS; NANOFLUID; ENCLOSURE; ANNULUS; MODELS;
D O I
10.1016/j.jtice.2024.105538
中图分类号
TQ [化学工业];
学科分类号
0817 ;
摘要
Background: This study addresses magnetohydrodynamic (MHD) natural convection involving non-Newtonian fluids. Focusing on the annular region between concentric circular and square cylinders, the research examines the impact of a vertical magnetic field and thermal radiation. Methods: The Multiple Relaxation Time Lattice Boltzmann Method (MRT-LBM) is employed to simulate momentum and energy interactions in non-Newtonian fluid. Control parameters like Rayleigh number, Hartmann number, Radiation parameter, aspect ratio, square cylinder subdivision, and power-law index are systematically varied, while maintaining a constant Prandtl number. Significant findings: Using shear-thinning fluid (n n < 1) significantly improves cooling, particularly in conjunction with radiation effect. Correlations for the mean Nusselt number are established, offering insights. Results emphasize the substantial influence of parameters like Ra, Rd, and AR. High values of the latter promote the flow intensity and heat evacuation. For n < 1, increasing Ra from 103 3 to 5 x 104 4 results in a substantial increase in the heat transfer rate reaching 65 %. For shear-thickening fluid, the heat transfer rate is reduced by 25.31 % at Ra = 5 x 10(4) when Ha is increased from 0 to 50 in the absence of radiation. In addition, radiation enhances the heat transfer rate by 71.41 % by incrementing Rd from 0 to 0.8 for Ha = 0. The most pronounced effect of the radiation parameter is observed in the cases of Newtonian and shear-thickening fluids. Conversely, Ha and n act by reduction effects on the outputs of the problem. The attenuating effect of the magnetic field is more pronounced in the case of shear-thinning fluids. The plot of mean Nusselt number vs. AR shows an hysteresis phenomenon due to the existence of multiple steady solutions in a range of this parameter. In the latter range of AR, heat transfer induced by multicellular flow is higher than that induced by bicellular one. Heat transfer is somewhat enhanced by the RC configuration, compared to SC one.
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页数:20
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