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Analysis of Convective Instability in Dusty Ferromagnetic Fluids with Magnetic Field-Dependent Viscosity Under Fluid-Permeable Magnetic Boundaries Cover

Analysis of Convective Instability in Dusty Ferromagnetic Fluids with Magnetic Field-Dependent Viscosity Under Fluid-Permeable Magnetic Boundaries

Open Access
|Jun 2025

Abstract

The subject under consideration finds manifold applications across various disciplines, including biological, industrial, and environmental sectors. Therefore, this study aims to analytically investigate the onset of convective instability in a dusty ferromagnetic fluid layer, influenced by magnetic field-dependent viscosity and fluid-permeable magnetically active boundaries, when subjected to a uniform transverse magnetic field. The eigenvalue problem is formulated through the utilization of linear stability theory followed by normal mode analysis. To address this problem, a single-term Galerkin method is employed, followed by a numerical calculation of the critical magnetic Rayleigh number. It is investigated numerically and graphically that (Nc)Free ≤ (Nc)permeable ≤ (Nc)Rigid. It has been observed that as the dust particle parameter h1 increase, the critical Rayleigh number decreases, indicating the destabilizing nature of h1 On the other hand, the viscosity parameter δ and magnetic susceptibility χ and permeability parameter Das demonstrate a stabilizing effect on the system. Initially, measure of nonlinearity of magnetization M3 exhibits a destabilizing effect, but beyond a certain threshold, it switches to a stabilizing effect within the system.

DOI: https://doi.org/10.2478/ama-2025-0040 | Journal eISSN: 2300-5319 | Journal ISSN: 1898-4088
Language: English
Page range: 327 - 336
Submitted on: Dec 28, 2024
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Accepted on: May 3, 2025
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Published on: Jun 30, 2025
In partnership with: Paradigm Publishing Services
Publication frequency: 4 issues per year

© 2025 Awneesh KUMAR, Pankaj KUMAR, Abhishek THAKUR, Mandeep KAUR, published by Bialystok University of Technology
This work is licensed under the Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 License.