Effect of Uniform and Non-uniform wall heating on Three-Dimensional Magneto-Hydrodynamics Natural Convection and Entropy Generation: A computational study using New Higher Order Super Compact Scheme

TL;DR

This computational study investigates how uniform and non-uniform wall heating influence 3D magnetohydrodynamic natural convection and entropy generation in a molten lithium-filled cavity, using a novel higher-order scheme to analyze thermal and flow behaviors.

Contribution

It introduces a new Higher-Order Super Compact scheme for analyzing complex 3D MHD convection with varied wall heating conditions, demonstrating its effectiveness and novelty.

Findings

Increased Rayleigh number enhances heat transfer.

Higher Hartman number reduces fluid velocity and heat transfer.

Uniform heating results in maximum entropy generation.

Abstract

Current research work deals with the effect of uniform and non-uniform wall heating on magnetohydrodynamic (MHD) natural convection within a three-dimensional (3D) cavity filled with molten lithium. A new Higher-Order Super Compact (HOSC) finite difference scheme is used to analyze the thermal behavior under both heating scenarios. After the quantitative and qualitative validations, the computed results are analyzed for a range of Hartman number ($Ha = 25, 50, 100, 150$) and Rayleigh number ($Ra = 10^3, 10^4, 10^5$) with fixed $Pr=0.065$ (molten lithium). Three distinct heating scenarios, i.e., uniform heating ($T_h = 1$), $y$-dependent non-uniform heating ($T_h = sin(\pi y$)), and a combination of $y$ and $z$-dependent non-uniform heating ($T_h = sin(\pi y)sin(\pi z)$) are investigated on the left wall ($x=0$) of the cubic cavity. It is found that variations in the $Ha$ and $Ra$, along with distinct thermal boundary conditions, exert significant effects on both the temperature distribution and flow field inside the 3D cubical cavity. Specifically, an increase in $Ra$ corresponds to enhanced heat transfer, highlighting the dominance of convection. Conversely, an increase in $Ha$ leads to a reduction in heat transfer due to the deceleration of fluid velocity. The scenario in which walls are uniformly heated exhibits the most significant total entropy generation. It is observed that with an increase in the $Ra$, the Bejan number ($Be$) decreases, which ultimately leads to an increase in total entropy generation. The implementation of the new HOSC scheme in this analysis showcases its effectiveness in capturing the complexities of 3D MHD-driven natural convection and entropy generation. This study offers significant information that might help improve the optimization and design of relevant engineering systems. Thus, our work stands out as genuinely novel and pioneering in its approach.