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JOURNALS // Teoreticheskaya i Matematicheskaya Fizika // Archive

TMF, 2025 Volume 223, Number 3, Pages 429–448 (Mi tmf10896)

This article is cited in 2 papers

Hall current and MHD impacts on a 3D Maxwell nanofluid flow across a porous stretching surface

G. Muralia, J. Venkata Madhub, G. Deepac, P. Sureshc, Sk. Nuslina

a Department of Mathematics, Geethanjali College of Engineering and Technology, Cheeryal, India
b Department of Mathematics, Sreenidhi Institute of Science and Technology, India
c Department of Mathematics, Chaitanya Bharathi Institute of Technology, Gandipet, India

Abstract: The purpose of this study is to investigate the influence that heat radiation has on the flow of a three-dimensional, viscous, electrically conducting, incompressible, upper-convicted Maxwell nanofluid over a bidirectional stretching surface. Additionally, aspects such as magnetic fields, porous media, thermophoresis, and Brownian motion are taken into consideration. Nonlinear radiative heat transmission is included in the energy equation in the Rosseland approximation version of the equation. For the purpose of resolving the ordinary differential equations that are formed from the reduction of the main governing nonlinear partial differential equations by similarity transformations, the “bvp4c” solver by MATLAB is used. The skin-friction, heat transfer rates, and mass transfer coefficients are analyzed numerically, and visual representations are used to demonstrate the impacts of a large number of important components on the velocity, temperature, and concentration profiles. The numerical findings of the study have been evaluated, and it has been determined that they are substantially in accord with the results available in the literature.

Keywords: nanofluid, Maxwell fluid, three-dimensional flow, thermal radiation, magnetic field, Hall current, porous medium, bidirectional stretching surface.

MSC: 76,35,65

Received: 25.01.2025
Revised: 25.01.2025

DOI: 10.4213/tmf10896


 English version:
Theoretical and Mathematical Physics, 2025, 223:3, 899–914

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© Steklov Math. Inst. of RAS, 2025