Parametric analysis of magnetic field-dependent viscosity and advection–diffusion between rotating discs

The constitutive expressions of unsteady Newtonian fluid are employed in the mathematical formulation to model the flow between the circular space of porous and contracting discs. The flow behavior is investigated for magnetic field-dependent (MFD) viscosity and heat/mass transfers under the influen...

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Main Authors: Rehan Ali Shah, Aamir Khan, Amjad Ali
Format: Article
Language:English
Published: SAGE Publishing 2020-01-01
Series:Advanced Composites Letters
Online Access:https://doi.org/10.1177/2633366X19896373
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spelling doaj-cb89381a3973485199f8630fe9fb194c2020-11-25T04:10:02ZengSAGE PublishingAdvanced Composites Letters0963-69352020-01-012910.1177/2633366X19896373Parametric analysis of magnetic field-dependent viscosity and advection–diffusion between rotating discsRehan Ali ShahAamir KhanAmjad AliThe constitutive expressions of unsteady Newtonian fluid are employed in the mathematical formulation to model the flow between the circular space of porous and contracting discs. The flow behavior is investigated for magnetic field-dependent (MFD) viscosity and heat/mass transfers under the influence of a variable magnetic field. The equation for conservation of mass, modified Navier–Stokes, Maxwell, advection diffusion and transport equations are coupled as a system of ordinary differential equations. The expressions for torques and magnetohydrodynamic pressure gradient equation are derived. The MFD viscosity ϑ , magnetic Reynolds number ℵ e m , squeezing Reynolds number ℵ b , rotational Reynolds number ℵ a , magnetic field components ℵ c , ℵ d , pressure F pres and the torques ϱ ′ 0 , ϱ 1 which the fluid exerts on discs are discussed through numerical results and graphical aids. It is concluded that magnetic Reynolds number causes an increase in magnetic field distributions and decrease in tangential velocity of flow field, also the fluid temperature is decreasing with increase in magnetic Reynolds number. The azimuthal and axial components of magnetic field have opposite behavior with increase in MFD viscosity.https://doi.org/10.1177/2633366X19896373
collection DOAJ
language English
format Article
sources DOAJ
author Rehan Ali Shah
Aamir Khan
Amjad Ali
spellingShingle Rehan Ali Shah
Aamir Khan
Amjad Ali
Parametric analysis of magnetic field-dependent viscosity and advection–diffusion between rotating discs
Advanced Composites Letters
author_facet Rehan Ali Shah
Aamir Khan
Amjad Ali
author_sort Rehan Ali Shah
title Parametric analysis of magnetic field-dependent viscosity and advection–diffusion between rotating discs
title_short Parametric analysis of magnetic field-dependent viscosity and advection–diffusion between rotating discs
title_full Parametric analysis of magnetic field-dependent viscosity and advection–diffusion between rotating discs
title_fullStr Parametric analysis of magnetic field-dependent viscosity and advection–diffusion between rotating discs
title_full_unstemmed Parametric analysis of magnetic field-dependent viscosity and advection–diffusion between rotating discs
title_sort parametric analysis of magnetic field-dependent viscosity and advection–diffusion between rotating discs
publisher SAGE Publishing
series Advanced Composites Letters
issn 0963-6935
publishDate 2020-01-01
description The constitutive expressions of unsteady Newtonian fluid are employed in the mathematical formulation to model the flow between the circular space of porous and contracting discs. The flow behavior is investigated for magnetic field-dependent (MFD) viscosity and heat/mass transfers under the influence of a variable magnetic field. The equation for conservation of mass, modified Navier–Stokes, Maxwell, advection diffusion and transport equations are coupled as a system of ordinary differential equations. The expressions for torques and magnetohydrodynamic pressure gradient equation are derived. The MFD viscosity ϑ , magnetic Reynolds number ℵ e m , squeezing Reynolds number ℵ b , rotational Reynolds number ℵ a , magnetic field components ℵ c , ℵ d , pressure F pres and the torques ϱ ′ 0 , ϱ 1 which the fluid exerts on discs are discussed through numerical results and graphical aids. It is concluded that magnetic Reynolds number causes an increase in magnetic field distributions and decrease in tangential velocity of flow field, also the fluid temperature is decreasing with increase in magnetic Reynolds number. The azimuthal and axial components of magnetic field have opposite behavior with increase in MFD viscosity.
url https://doi.org/10.1177/2633366X19896373
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