S Abdul Gaffar
Computation of hydromagnetic tangent hyperbolic non-Newtonian flow from a rotating non- isothermal cone to a non-darcy porous medium with thermal radiative flux
Abdul Gaffar, S; Anwar Bég, O; Kuharat, S; Bég, T A
Authors
Prof Osman Beg O.A.Beg@salford.ac.uk
Professor
Ms Sireetorn Kuharat S.Kuharat2@salford.ac.uk
Lecturer
T A Bég
Contributors
Prof Osman Beg O.A.Beg@salford.ac.uk
Project Leader
Abstract
A theoretical and numerical study is conducted on nonlinear, steady-state thermal convection boundary layer flow of a magnetized incompressible Tangent Hyperbolic non-Newtonian fluid from a rotating cone to a non-Darcy porous medium. Power-law variation in temperature on the cone surface is considered and thermal radiation heat transfer is also present. The Brinkman-Darcy-Forchheimer model is deployed for the porous medium. The study is motivated by rotational (spin) coating with new emerging magnetic rheological polymers, a process which often utilizes filtration media and high temperatures. The transformed non-dimensional conservation equations are solved numerically subject to physically appropriate boundary conditions using a second-order accurate implicit finite-difference Keller Box technique. The numerical code is validated with previous studies. Extensive visualization of axial, tangential velocity components and temperature distributions with variation in key parameters including Rosseland radiative number, Darcy number, Forchheimer number (non-Darcy inertial parameter), magnetic interaction parameter, tangent-hyperbolic non-Newtonian power-law index and Weissenberg (non-Newtonian) number is included. Additionally, axial and tangential (circumferential) skin friction and Nusselt number values are tabulated for variation in key control parameters. With increasing Weissenberg number, axial velocity is depleted near the cone surface, tangential velocity is suppressed throughout the boundary layer regime and temperature is strongly enhanced. Axial flow is strongly decelerated further from the cone surface with increasing tangent-hyperbolic power-law index and there is also a significant depletion in tangential (swirl) velocity. Temperature is however boosted throughout the boundary layer transverse to the cone surface with
Citation
Abdul Gaffar, S., Anwar Bég, O., Kuharat, S., & Bég, T. A. (2024). Computation of hydromagnetic tangent hyperbolic non-Newtonian flow from a rotating non- isothermal cone to a non-darcy porous medium with thermal radiative flux. #Journal not on list, 19, https://doi.org/10.1016/j.physo.2024.100216
Journal Article Type | Article |
---|---|
Acceptance Date | Apr 3, 2024 |
Online Publication Date | Apr 12, 2024 |
Publication Date | May 1, 2024 |
Deposit Date | Apr 3, 2024 |
Publicly Available Date | Apr 12, 2024 |
Journal | Physics Open |
Electronic ISSN | 2666-0326 |
Peer Reviewed | Peer Reviewed |
Volume | 19 |
DOI | https://doi.org/10.1016/j.physo.2024.100216 |
Publisher URL | https://www.sciencedirect.com/journal/physics-open/about/aims-and-scope |
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Publisher Licence URL
http://creativecommons.org/licenses/by-nc-nd/4.0/
Accepted Version
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Publisher Licence URL
http://creativecommons.org/licenses/by/4.0/
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