Melting and heat generating influences on radiative flow of two-phase magneto-Williamson nanofluid via stretchable surface with slippage velocity and activation energy
Melting heat and solutal transference in a magnetohydrodynamic flowing of Williamson nanofluid have been described, with the mathematical model guided by Arrhenius activation energy, chemically reactive species, and convective boundary restrictions. By implementing suitable similarity conversions, t...
Saved in:
Main Authors: | , , , , , , , |
---|---|
Format: | Article |
Published: |
Taylor and Francis
2024
|
Online Access: | http://psasir.upm.edu.my/id/eprint/112054/ https://www.tandfonline.com/doi/full/10.1080/10407782.2024.2322703 |
Tags: |
Add Tag
No Tags, Be the first to tag this record!
|
id |
my.upm.eprints.112054 |
---|---|
record_format |
eprints |
spelling |
my.upm.eprints.1120542024-10-28T03:42:04Z http://psasir.upm.edu.my/id/eprint/112054/ Melting and heat generating influences on radiative flow of two-phase magneto-Williamson nanofluid via stretchable surface with slippage velocity and activation energy Ullah, Imran Jamshed, Wasim Katbar, Nek Muhammad Eid, Mohamed R. Duraihem, Faisal Z. Mohamed Isa, Siti Suzilliana Putri Ibrahim, Rabha W. AlDerea, Afrah M. Melting heat and solutal transference in a magnetohydrodynamic flowing of Williamson nanofluid have been described, with the mathematical model guided by Arrhenius activation energy, chemically reactive species, and convective boundary restrictions. By implementing suitable similarity conversions, the regulating equations of partial differential equations (PDEs) (formed by continuity, impetus, energy, and concentricity components) are condensed to an arrangement of ordinary differential equations (ODEs). These commonalities are in nonlinear form, which includes the fluid’s velocity, heat, and concentration changes. Finally, the standard Keller box approach is used to solve this ODEs system computationally (KBM). Under the influence of regulating parameters, the computational results are tallied and displayed in suitable diagrams. The friction force factor, local Nusselt, and Sherwood values are tabulated. Furthermore, the velocity, energy, and concentration contours are plotted versus fluid thickness. The attributes of Williamson nanofluid flowing, melting heat transfer, and mass transference are debated in depth toward the end of this study. Among the most important outcomes that have been reached is that the rate of heat and solutal transport heightened between 52.5 and 55.2% by detraction of the magnetic field, Weissenberg number, and Brownian motion. We also found that there is an inverse relationship between the mass transmission and heat generating factor. © 2024 Taylor & Francis Group, LLC. Taylor and Francis 2024 Article PeerReviewed Ullah, Imran and Jamshed, Wasim and Katbar, Nek Muhammad and Eid, Mohamed R. and Duraihem, Faisal Z. and Mohamed Isa, Siti Suzilliana Putri and Ibrahim, Rabha W. and AlDerea, Afrah M. (2024) Melting and heat generating influences on radiative flow of two-phase magneto-Williamson nanofluid via stretchable surface with slippage velocity and activation energy. Numerical Heat Transfer, Part A: Applications. pp. 1-23. ISSN 1040-7782; ESSN: 1521-0634 https://www.tandfonline.com/doi/full/10.1080/10407782.2024.2322703 10.1080/10407782.2024.2322703 |
institution |
Universiti Putra Malaysia |
building |
UPM Library |
collection |
Institutional Repository |
continent |
Asia |
country |
Malaysia |
content_provider |
Universiti Putra Malaysia |
content_source |
UPM Institutional Repository |
url_provider |
http://psasir.upm.edu.my/ |
description |
Melting heat and solutal transference in a magnetohydrodynamic flowing of Williamson nanofluid have been described, with the mathematical model guided by Arrhenius activation energy, chemically reactive species, and convective boundary restrictions. By implementing suitable similarity conversions, the regulating equations of partial differential equations (PDEs) (formed by continuity, impetus, energy, and concentricity components) are condensed to an arrangement of ordinary differential equations (ODEs). These commonalities are in nonlinear form, which includes the fluid’s velocity, heat, and concentration changes. Finally, the standard Keller box approach is used to solve this ODEs system computationally (KBM). Under the influence of regulating parameters, the computational results are tallied and displayed in suitable diagrams. The friction force factor, local Nusselt, and Sherwood values are tabulated. Furthermore, the velocity, energy, and concentration contours are plotted versus fluid thickness. The attributes of Williamson nanofluid flowing, melting heat transfer, and mass transference are debated in depth toward the end of this study. Among the most important outcomes that have been reached is that the rate of heat and solutal transport heightened between 52.5 and 55.2% by detraction of the magnetic field, Weissenberg number, and Brownian motion. We also found that there is an inverse relationship between the mass transmission and heat generating factor. © 2024 Taylor & Francis Group, LLC. |
format |
Article |
author |
Ullah, Imran Jamshed, Wasim Katbar, Nek Muhammad Eid, Mohamed R. Duraihem, Faisal Z. Mohamed Isa, Siti Suzilliana Putri Ibrahim, Rabha W. AlDerea, Afrah M. |
spellingShingle |
Ullah, Imran Jamshed, Wasim Katbar, Nek Muhammad Eid, Mohamed R. Duraihem, Faisal Z. Mohamed Isa, Siti Suzilliana Putri Ibrahim, Rabha W. AlDerea, Afrah M. Melting and heat generating influences on radiative flow of two-phase magneto-Williamson nanofluid via stretchable surface with slippage velocity and activation energy |
author_facet |
Ullah, Imran Jamshed, Wasim Katbar, Nek Muhammad Eid, Mohamed R. Duraihem, Faisal Z. Mohamed Isa, Siti Suzilliana Putri Ibrahim, Rabha W. AlDerea, Afrah M. |
author_sort |
Ullah, Imran |
title |
Melting and heat generating influences on radiative flow of two-phase magneto-Williamson nanofluid via stretchable surface with slippage velocity and activation energy |
title_short |
Melting and heat generating influences on radiative flow of two-phase magneto-Williamson nanofluid via stretchable surface with slippage velocity and activation energy |
title_full |
Melting and heat generating influences on radiative flow of two-phase magneto-Williamson nanofluid via stretchable surface with slippage velocity and activation energy |
title_fullStr |
Melting and heat generating influences on radiative flow of two-phase magneto-Williamson nanofluid via stretchable surface with slippage velocity and activation energy |
title_full_unstemmed |
Melting and heat generating influences on radiative flow of two-phase magneto-Williamson nanofluid via stretchable surface with slippage velocity and activation energy |
title_sort |
melting and heat generating influences on radiative flow of two-phase magneto-williamson nanofluid via stretchable surface with slippage velocity and activation energy |
publisher |
Taylor and Francis |
publishDate |
2024 |
url |
http://psasir.upm.edu.my/id/eprint/112054/ https://www.tandfonline.com/doi/full/10.1080/10407782.2024.2322703 |
_version_ |
1814936522620665856 |
score |
13.211869 |