Ebrahim Momoniat
Current Organizations / Institutes
The organizations/institutes from the scholar's latest article
Previous Organizations / Institutes
The organizations / institutes from the scholar's other articles in the past ten years
Ebrahim Momoniat has a total of 114 co-authors. Here are the top co-authors by number of shared publications:
- Charis Harley
Department of Electrical and Electronic Engineering Science, Faculty of Engineering and the Built Environment, University of Johannesburg, Johannesburg 2006, South Africa
24 shared publications - Prabhugouda Mallanagouda Patil
Department of Mathematics, KLE Technological University, Hubballi, India
18 shared publications - Fazal Mahmood Mahomed
DSI-NRF Centre of Excellence in Mathematical and Statistical Sciences, School of Computer Science and Applied Mathematics, University of the Witwatersrand, Johannesburg, South Africa
15 shared publications - Satyajit Roy
Indian Inst Technol, Dept Math, Madras 600036, Tamil Nadu, India
12 shared publications T. Hayat
School of Computational and Applied Mathematics, University of the Witwatersrand, Johannesburg, Private Bag 3, Wits 2050, South Africa
12 shared publications- Mohammad Mehdi Rashidi
Institute of Fundamental and Frontier Sciences, University of Electronic Science and Technology of China, Chengdu 611730, China
11 shared publications
Latest Publications
- Open Access
- 4 June 2026
- Published by Elsevier in Case Studies in Thermal Engineering
- Vol. 83
Thermo-bioconvective transport in sutterby ternary hybrid nanofluids with nonlinear pollutant effects
- 4 June 2026
- Published by Elsevier in Case Studies in Thermal Engineering
- Vol. 83
Open AccessThermo-bioconvective transport in sutterby ternary hybrid nanofluids with nonlinear pollutant effects
- 18 November 2025
- Published by Springer Nature in International Journal of Theoretical Physics
- Vol. 64 (12) , 328
Solving Lane-Emden-Type Eigenvalue Problems with Physics-Informed Neural Networks
- 18 November 2025
- Published by Springer Nature in International Journal of Theoretical Physics
- Vol. 64 (12) , 328
Solving Lane-Emden-Type Eigenvalue Problems with Physics-Informed Neural Networks
- Open Access
- 11 September 2025
- Published by Elsevier in Partial Differential Equations in Applied Mathematics
- Vol. 16
Pseudo-planar deformations of a linearized elastic solid
- 11 September 2025
- Published by Elsevier in Partial Differential Equations in Applied Mathematics
- Vol. 16
Open AccessPseudo-planar deformations of a linearized elastic solid
- Open Access
Solving Lane-Emden-Type Eigenvalue Problems with Physics-Informed Neural Networks
The Lane-Emden equation, a nonlinear second-order ordinary differential equation, plays a fundamental role in theoretical physics and astrophysics, particularly in modeling the structure of stellar interiors. Also referred to as the polytropic differential equation, it describes the behavior of self-gravitating polytropic spheres. In this study, we present a novel approach to the solution of the eigenvalue problem which arises when considering the Lane-Emden equation for n = 0, 1, 2, 3, 4 using Physics-Informed Neural Networks (PINNs). The novelty of this work is that, we not only solve the Lane-Emden equation via PINNS but we also determine the eigenvalue, r, which is the stellar radius. Hyperparameter tuning was conducted using Bayesian optimization in the Optuna framework to identify optimal values for the number of hidden layers, number of neurons, activation function, optimizer, and learning rate for each value of n. The results show that, for n = 0, 1, PINNs achieve near-exact agreement with theoretical eigenvalues (errors < 0.000806%). While for more nonlinear cases, n = 2, 3 and n=4, PINNs yield errors below 0.0009% and 0.05% respectively, validating their robustness.
Open AccessSolving Lane-Emden-Type Eigenvalue Problems with Physics-Informed Neural Networks
The Lane-Emden equation, a nonlinear second-order ordinary differential equation, plays a fundamental role in theoretical physics and astrophysics, particularly in modeling the structure of stellar interiors. Also referred to as the polytropic differential equation, it describes the behavior of self-gravitating polytropic spheres. In this study, we present a novel approach to the solution of the eigenvalue problem which arises when considering the Lane-Emden equation for n = 0, 1, 2, 3, 4 using Physics-Informed Neural Networks (PINNs). The novelty of this work is that, we not only solve the Lane-Emden equation via PINNS but we also determine the eigenvalue, r, which is the stellar radius. Hyperparameter tuning was conducted using Bayesian optimization in the Optuna framework to identify optimal values for the number of hidden layers, number of neurons, activation function, optimizer, and learning rate for each value of n. The results show that, for n = 0, 1, PINNs achieve near-exact agreement with theoretical eigenvalues (errors < 0.000806%). While for more nonlinear cases, n = 2, 3 and n=4, PINNs yield errors below 0.0009% and 0.05% respectively, validating their robustness.
- Open Access
- 29 November 2024
- Published by Elsevier in Partial Differential Equations in Applied Mathematics
- Vol. 12
Comparison of hyperbolic and parabolic equations modelling buoyancy driven flow in a square cavity
- 29 November 2024
- Published by Elsevier in Partial Differential Equations in Applied Mathematics
- Vol. 12
Open AccessComparison of hyperbolic and parabolic equations modelling buoyancy driven flow in a square cavity
- Open Access
- 23 September 2024
- Published by Emerald Publishing in International Journal of Numerical Methods for Heat & Fluid Flow
- Vol. 34 (12) , 4181-4205
Casson-Williamson ternary hybrid nanofluid flow over a yawed cylinder with the impacts of multiple slips
Many industries use non-Newtonian ternary hybrid nanofluids (THNF) because of how well they control rheological and heat transport. This being the case, this paper aims to numerically study the Casson-Williamson THNF flow over a yawed cylinder, considering the effects of several slips and an inclined magnetic field. The THNF comprises Al2O3-TiO2-SiO2 nanoparticles because they improve heat transmission due to large thermal conductivity. Applying suitable nonsimilarity variables transforms the coupled highly dimensional nonlinear partial differential equations (PDEs) into a system of nondimensional PDEs. To accomplish the goal of achieving the solution, an implicit finite difference approach is used in conjunction with Quasilinearization. With the assistance of a script written in MATLAB, the numerical results and the graphical representation of those solutions were ascertained. As the Casson parameter increases, there is an improvement in the velocity profiles in both chord and span orientations, while the gradients reduce for the same variations of . The velocities of Casson THNF are greater than those of Casson-Williamson THNF. Approximately, a 202% and a 32% ascension are remarked in the magnitudes of and for Casson-Williamson THNF than the Casson THNF only. When velocity slip attribute jumps to 1 from 0.5, magnitude of both and fell down and it is reflected to be 396% at , and . An augmentation in thermal jump results in advanced fluid temperature and lower . In particular, about 159% of down drift is detected when taking 1. There is no existing research on the effects of Casson-Williamson THNF flow over a yawed cylinder with multiple slips and an angled magnetic field, according to the literature.- 23 September 2024
- Published by Emerald Publishing in International Journal of Numerical Methods for Heat & Fluid Flow
- Vol. 34 (12) , 4181-4205
Open AccessCasson-Williamson ternary hybrid nanofluid flow over a yawed cylinder with the impacts of multiple slips
Many industries use non-Newtonian ternary hybrid nanofluids (THNF) because of how well they control rheological and heat transport. This being the case, this paper aims to numerically study the Casson-Williamson THNF flow over a yawed cylinder, considering the effects of several slips and an inclined magnetic field. The THNF comprises Al2O3-TiO2-SiO2 nanoparticles because they improve heat transmission due to large thermal conductivity. Applying suitable nonsimilarity variables transforms the coupled highly dimensional nonlinear partial differential equations (PDEs) into a system of nondimensional PDEs. To accomplish the goal of achieving the solution, an implicit finite difference approach is used in conjunction with Quasilinearization. With the assistance of a script written in MATLAB, the numerical results and the graphical representation of those solutions were ascertained. As the Casson parameter increases, there is an improvement in the velocity profiles in both chord and span orientations, while the gradients reduce for the same variations of . The velocities of Casson THNF are greater than those of Casson-Williamson THNF. Approximately, a 202% and a 32% ascension are remarked in the magnitudes of and for Casson-Williamson THNF than the Casson THNF only. When velocity slip attribute jumps to 1 from 0.5, magnitude of both and fell down and it is reflected to be 396% at , and . An augmentation in thermal jump results in advanced fluid temperature and lower . In particular, about 159% of down drift is detected when taking 1. There is no existing research on the effects of Casson-Williamson THNF flow over a yawed cylinder with multiple slips and an angled magnetic field, according to the literature. - Open Access
- 23 June 2024
- Published by Wiley
Magneto - bioconvective flow of a Casson -- Williamson nanoliquid containing oxytactic microorganisms
This paper investigates the collective impacts of magnetic field, Brownian diffusion, thermophoresis, and buoyancy force on the Casson – Williamson nanoliquid over a rough slender cylinder. The novelty of this paper is to inspect the effect of inclined magnetic field (in particular, at an angle of 45 0 to the liquid flow) over an oxytactic bioconvective nanoliquid flow. To simulate the problem, a set of nonlinearly coupled partial differential equations is employed, and nonsimilar transformations are used to reduce them into nondimensional form. For mathematical simplification, an implicit finite difference scheme and Quasilinearization technique are used. The outcomes for the influences of several significant parameters on the mass and heat transmission properties are illustrated through graphs. Temperature and velocity profiles are pronounced to be more for augmenting values of thermophoresis and Brownian motion parameters. The heat transmission and coefficient of skin friction are enhanced with the surface roughness parameter, while skin friction increases and the heat transmission decreases with the magnetic parameter. The mass transmission rate of oxygen liquid, and microbial density number enhance with the higher bioconvection Lewis number and Peclet number. In a comparison with earlier published works, the results are discovered to be highly concordant.
- 23 June 2024
- Published by Wiley
Open AccessMagneto - bioconvective flow of a Casson -- Williamson nanoliquid containing oxytactic microorganisms
This paper investigates the collective impacts of magnetic field, Brownian diffusion, thermophoresis, and buoyancy force on the Casson – Williamson nanoliquid over a rough slender cylinder. The novelty of this paper is to inspect the effect of inclined magnetic field (in particular, at an angle of 45 0 to the liquid flow) over an oxytactic bioconvective nanoliquid flow. To simulate the problem, a set of nonlinearly coupled partial differential equations is employed, and nonsimilar transformations are used to reduce them into nondimensional form. For mathematical simplification, an implicit finite difference scheme and Quasilinearization technique are used. The outcomes for the influences of several significant parameters on the mass and heat transmission properties are illustrated through graphs. Temperature and velocity profiles are pronounced to be more for augmenting values of thermophoresis and Brownian motion parameters. The heat transmission and coefficient of skin friction are enhanced with the surface roughness parameter, while skin friction increases and the heat transmission decreases with the magnetic parameter. The mass transmission rate of oxygen liquid, and microbial density number enhance with the higher bioconvection Lewis number and Peclet number. In a comparison with earlier published works, the results are discovered to be highly concordant.
- 5 November 2023
- Published by Elsevier in Chinese Journal of Physics
- Vol. 89, 565-581
Unsteady magneto bioconvective Sutterby nanofluid flow: Influence of g-Jitter effect
- 5 November 2023
- Published by Elsevier in Chinese Journal of Physics
- Vol. 89, 565-581
Unsteady magneto bioconvective Sutterby nanofluid flow: Influence of g-Jitter effect
- Open Access
- 1 October 2023
- Published by Elsevier in Case Studies in Thermal Engineering
- Vol. 51
Thermal analysis of bioconvective nanofluid flow over a sphere in presence of multiple diffusions and a periodic magnetic field
- 1 October 2023
- Published by Elsevier in Case Studies in Thermal Engineering
- Vol. 51
Open AccessThermal analysis of bioconvective nanofluid flow over a sphere in presence of multiple diffusions and a periodic magnetic field
- Open Access
- 29 September 2023
- Published by Elsevier in Alexandria Engineering Journal
- Vol. 81, 636-655
Bioconvective periodic MHD Eyring-Powell fluid flow around a rotating cone: Influence of multiple diffusions and oxytactic microorganisms
- 29 September 2023
- Published by Elsevier in Alexandria Engineering Journal
- Vol. 81, 636-655
Open AccessBioconvective periodic MHD Eyring-Powell fluid flow around a rotating cone: Influence of multiple diffusions and oxytactic microorganisms