Characterization of fluid flow and heat transfer of a periodic magnetohydrodynamics nano non‐Newtonian liquid with Arrhenius activation energy and nonlinear radiation

Abstract

The focus of this study is to better understand the boundary layer phenomena of nonlinear radiative nano non-Newtonian (Casson) fluid flow caused by a stretched periphery with a periodic magnetic field and Arrhenius activation energy. The time-based controlling equations are translated into a suitable dimensionless form using the explicit finite difference (EFD) approach.However, to make the solution convergent, detailed stability and convergence criteria have been devised. In addition, the oscillatory form of velocity, isothermal, and streamline profiles, as well as the conventional shape of other flow fields are displayed. Using tabular analysis, a correlation between non-Newtonian and Newtonian fluids has even been demonstrated. When the radiative heat flux is evaluated in a linear pattern rather than a nonlinear one, the Lorentz force has been demonstrated to diminish the flow profiles convincingly. Also, another finding is that when the magnetic factor is considered in the sinusoidal form it is controlling the heat transfer factors of nanofluid substantially. As a chemical reaction requires a high-temperature mechanism to proceed, the

Numerical simulation of mass and heat transport phenomena of hydromagnetic flow of Casson fluid with sinusoidal boundary conditions

“…All of the discussion that has been presented in the Section 6.1 are in a good agreement with the several published works. 3,4,7,9,16…”

“…The introduction of a magnetic phenomenon dramatically changes the mass transportation and heat transfer capabilities of common electrically conducting flows, according to a number of anticipated experiments 1,2 . At recent time, Reza‐E‐Rabbi et al 3 studied out the influence of periodic MHD on a nanofluid flow. It has been illustrated that periodic magnetic factor influenced the heat transfer characteristics of nanofluid significantly under the impact of nonlinear radiation.…”

Homotopic solution of the chemically reactive magnetohydrodynamic flow of a hybrid nanofluid over a rotating disk with Brownian motion and thermophoresis effects

“…Oyelakin et al [28] explored the time-dependent Casson fluid flow past a stretching sheet with activation energy and have proved that activation energy factor has upsurge the concentration characteristics of fluid. Reza-E-Rabbi et al [29] characterized the thermal flow transportation of MHD nanofluid with activation energy and nonlinear thermal radiation and found that the velocity has declined while thermal profile has expanded with augmenting values of solid volume fraction. Yasir et al [30] inspected the radiative nanoliquid flow over a cylinder subject to activation energy.…”

“…Reza‐E‐Rabbi et al. [29] characterized the thermal flow transportation of MHD nanofluid with activation energy and nonlinear thermal radiation and found that the velocity has declined while thermal profile has expanded with augmenting values of solid volume fraction. Yasir et al.…”

Numerical Simulation of Mass and Heat Transport Phenomena of Hydromagnetic Flow of Casson Fluid with Sinusoidal Boundary Conditions

“…They also used the keller box method. Reza-E-Rabbi et al 34 studied out the investigation of heat transfer and fluid flow of a periodic MHD nano non-Newtonian fluid with Arrhenius activation energy and nonlinear radiation. They applied the explicit finite difference (EFD) approach for further analysis.…”