Radiative MHD sutterby nanofluid flow past a moving sheet: Scaling group analysis
The present theoretical work endeavors to solve the Sutterby nanofluid flow and heat transfer problem over a permeable moving sheet, together with the presence of thermal radiation and magnetohydrodynamics (MHD). The fluid flow and heat transfer features near the stagnation region are considered. A...
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my.utm.934102021-11-30T08:28:55Z http://eprints.utm.my/id/eprint/93410/ Radiative MHD sutterby nanofluid flow past a moving sheet: Scaling group analysis Fayyadh, Mohammed M. Naganthran, Kohilavani Md. Basir, Md. Faisal Hashim, Ishak Roslan, Rozaini QA Mathematics The present theoretical work endeavors to solve the Sutterby nanofluid flow and heat transfer problem over a permeable moving sheet, together with the presence of thermal radiation and magnetohydrodynamics (MHD). The fluid flow and heat transfer features near the stagnation region are considered. A new form of similarity transformations is introduced through scaling group analysis to simplify the governing boundary layer equations, which then eases the computational process in the MATLAB bvp4c function. The variation in the values of the governing parameters yields two different numerical solutions. One of the solutions is stable and physically reliable, while the other solution is unstable and is associated with flow separation. An increased effect of the thermal radiation improves the rate of convective heat transfer past the permeable shrinking sheet. MDPI AG 2020 Article PeerReviewed application/pdf en http://eprints.utm.my/id/eprint/93410/1/MohammadFaisal2020_RadiativeMHDSutterbyNanofluidFlow.pdf Fayyadh, Mohammed M. and Naganthran, Kohilavani and Md. Basir, Md. Faisal and Hashim, Ishak and Roslan, Rozaini (2020) Radiative MHD sutterby nanofluid flow past a moving sheet: Scaling group analysis. Mathematics, 8 (9). ISSN 2227-7390 http://dx.doi.org/10.3390/MATH8091430 |
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QA Mathematics Fayyadh, Mohammed M. Naganthran, Kohilavani Md. Basir, Md. Faisal Hashim, Ishak Roslan, Rozaini Radiative MHD sutterby nanofluid flow past a moving sheet: Scaling group analysis |
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The present theoretical work endeavors to solve the Sutterby nanofluid flow and heat transfer problem over a permeable moving sheet, together with the presence of thermal radiation and magnetohydrodynamics (MHD). The fluid flow and heat transfer features near the stagnation region are considered. A new form of similarity transformations is introduced through scaling group analysis to simplify the governing boundary layer equations, which then eases the computational process in the MATLAB bvp4c function. The variation in the values of the governing parameters yields two different numerical solutions. One of the solutions is stable and physically reliable, while the other solution is unstable and is associated with flow separation. An increased effect of the thermal radiation improves the rate of convective heat transfer past the permeable shrinking sheet. |
format |
Article |
author |
Fayyadh, Mohammed M. Naganthran, Kohilavani Md. Basir, Md. Faisal Hashim, Ishak Roslan, Rozaini |
author_facet |
Fayyadh, Mohammed M. Naganthran, Kohilavani Md. Basir, Md. Faisal Hashim, Ishak Roslan, Rozaini |
author_sort |
Fayyadh, Mohammed M. |
title |
Radiative MHD sutterby nanofluid flow past a moving sheet: Scaling group analysis |
title_short |
Radiative MHD sutterby nanofluid flow past a moving sheet: Scaling group analysis |
title_full |
Radiative MHD sutterby nanofluid flow past a moving sheet: Scaling group analysis |
title_fullStr |
Radiative MHD sutterby nanofluid flow past a moving sheet: Scaling group analysis |
title_full_unstemmed |
Radiative MHD sutterby nanofluid flow past a moving sheet: Scaling group analysis |
title_sort |
radiative mhd sutterby nanofluid flow past a moving sheet: scaling group analysis |
publisher |
MDPI AG |
publishDate |
2020 |
url |
http://eprints.utm.my/id/eprint/93410/1/MohammadFaisal2020_RadiativeMHDSutterbyNanofluidFlow.pdf http://eprints.utm.my/id/eprint/93410/ http://dx.doi.org/10.3390/MATH8091430 |
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1718926064032415744 |
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13.18916 |