Fractal time numerical modelling of radiative heat and mass transfer in Carreau–Yasuda mixed convective flow

This paper demonstrates a computational process in simulating the unsteady radiative mixed convective flow of a Carreau-Yasuda nanofluid by a porous material, when subjected to a magnetic field. Fractal time derivatives are used to model an approach that captures the memory-dependent behaviour of complex transport phenomena. A novel three-stage explicit time integration scheme is developed, delivering third-order temporal accuracy tailored to fractal-time partial differential equations. For spatial discretization, a compact sixth-order scheme is used to improve numerical precision in the interior domain. The proposed framework incorporates thermal and solutal buoyancy effects, nonlinear rheology, Brownian motion, thermophoresis, and contributions from a heat source. It also accounts for the influence of oscillatory boundary conditions and Darcy-Forchheimer drag within porous structures. Rigorous stability and convergence analyses confirm the robustness of the scheme. Quantitative comparisons reveal that at a time step of Δt=0.12250, the proposed scheme achieves an L2 error of 6.72×10−5 and consumes approximately 97.62 s, while the second-order scheme reaches an error of 1.06×10−4 with a runtime of 173.82 s under the same compact discretization, highlighting both its efficiency and stability. Numerical experiments demonstrate that the method outperforms existing first- and second-order schemes in both accuracy and computational efficiency. Furthermore, a velocity reduction of over 30% observed when increasing the power-law index from 0.6 to 1.2, highlighting enhanced shear-thinning behaviour. The proposed methodology not only ensures numerical stability under fine discretization but also demonstrates robustness in capturing complex flow behaviour in porous, radiatively influenced environments. This fractal-based computational framework offers a valuable tool for simulating non-Newtonian nanofluid systems in emerging thermal technologies. Fractal time derivatives effectively capture memory-dependent, scale-invariant transport phenomena, offering computational advantages and localised accuracy over traditional fractional operators.

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Publication Details

Journal
Physics Open
Published
2025-12-20
DOI
https://doi.org/10.1016/j.physo.2025.100359
Primary Topic
Nanofluid Flow and Heat Transfer
Type
article
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article

Fractal time numerical modelling of radiative heat and mass transfer in Carreau–Yasuda mixed convective flow

Muhammad Shoaib Arif, Kamaleldin Abodayeh, Yasir Nawaz
Physics Open
Nanofluid Flow and Heat Transfer
article

Fractal time numerical modelling of radiative heat and mass transfer in Carreau–Yasuda mixed convective flow

Muhammad Shoaib Arif, Kamaleldin Abodayeh, Yasir Nawaz
article en

Abstract

This paper demonstrates a computational process in simulating the unsteady radiative mixed convective flow of a Carreau-Yasuda nanofluid by a porous material, when subjected to a magnetic field. Fractal time derivatives are used to model an approach that captures the memory-dependent behaviour of complex transport phenomena. A novel three-stage explicit time integration scheme is developed, delivering third-order temporal accuracy tailored to fractal-time partial differential equations. For spatial discretization, a compact sixth-order scheme is used to improve numerical precision in the interior domain. The proposed framework incorporates thermal and solutal buoyancy effects, nonlinear rheology, Brownian motion, thermophoresis, and contributions from a heat source. It also accounts for the influence of oscillatory boundary conditions and Darcy-Forchheimer drag within porous structures. Rigorous stability and convergence analyses confirm the robustness of the scheme. Quantitative comparisons reveal that at a time step of Δt=0.12250, the proposed scheme achieves an L2 error of 6.72×10−5 and consumes approximately 97.62 s, while the second-order scheme reaches an error of 1.06×10−4 with a runtime of 173.82 s under the same compact discretization, highlighting both its efficiency and stability. Numerical experiments demonstrate that the method outperforms existing first- and second-order schemes in both accuracy and computational efficiency. Furthermore, a velocity reduction of over 30% observed when increasing the power-law index from 0.6 to 1.2, highlighting enhanced shear-thinning behaviour. The proposed methodology not only ensures numerical stability under fine discretization but also demonstrates robustness in capturing complex flow behaviour in porous, radiatively influenced environments. This fractal-based computational framework offers a valuable tool for simulating non-Newtonian nanofluid systems in emerging thermal technologies. Fractal time derivatives effectively capture memory-dependent, scale-invariant transport phenomena, offering computational advantages and localised accuracy over traditional fractional operators.

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Fractal time numerical modelling of radiative heat and mass transfer in Carreau–Yasuda mixed convective flow — Muhammad Shoaib Arif, Kamaleldin Abodayeh, et al. · Physics Open (2025) | TGRS Research Map | TGRS